From - Fri Feb 7 20:11:39 2003 X-UIDL: 3df25b3100000727 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h17J9cZj023306 for ; Fri, 7 Feb 2003 20:09:38 +0100 (MET) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h17J9bu05731 for ; Fri, 7 Feb 2003 20:09:37 +0100 (MET) Received: from curlew.cs.man.ac.uk(130.88.13.7) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAhLaqml; Fri, 7 Feb 03 20:09:36 +0100 Received: from star1.jb.man.ac.uk ([130.88.24.176]) by curlew.cs.man.ac.uk with esmtp (Exim 4.12) id 18hDsW-000CkR-00 for ucd@ivoa.net; Fri, 07 Feb 2003 19:09:36 +0000 Received: from [130.88.24.148] (helo=adikia) by star1.jb.man.ac.uk with esmtp (Exim 3.03 #2) id 18hDsn-0002L9-00 for ucd@ivoa.net; Fri, 07 Feb 2003 19:09:53 +0000 Date: Fri, 7 Feb 2003 19:09:26 +0000 (GMT) From: Anita Richards X-X-Sender: amsr@adikia To: ucd@ivoa.net Subject: initiate discussion Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanner: exiscan for exim4 (http://duncanthrax.net/exiscan/) *18hDsW-000CkR-00*l9hWH3vILnw* X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: The main reference point for this is of course CDS http://cdsweb.u-strasbg.fr/doc/UCD.htx but you can find some AstroGrid documents on UCDs http://wiki.astrogrid.org/bin/view/Astrogrid/OntologyDocs One obvious starting point is what we have learnt from the AVO First Light Demo. My first thought is that it is very useful when you can answer a query by a partial UCD, e.g. plotting anything with a REDSHIFT whether it is REDSHIFT_PHOT or REDSHIFT_HC etc; or PHOT_*_V where * can be JHN or COUS or MAG or .... (e.g. in Aladin, for filters or for the SED tool..) However you also need to be able to track how much uncertainty you are introducing (as well as using the more exact UCD if you want of course) - e.g. any old PHOT_MAG_V might do as part of a radio-to-x-ray SED but not for fine inter-optical comparisons. So any restructuring of UCDs should take this into account. cheers Anita - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - Dr. Anita M. S. Richards, AVO Astronomer MERLIN/VLBI National Facility, University of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire SK11 9DL, U.K. tel +44 (0)1477 572683 (direct); 571321 (switchboard); 571618 (fax). From - Thu Feb 20 23:03:59 2003 X-UIDL: 3df25b3100000969 X-Mozilla-Status: 0001 X-Mozilla-Status2: 10000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h1KM4N3v009154 for ; Thu, 20 Feb 2003 23:04:23 +0100 (MET) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h1KM4Ml10593 for ; Thu, 20 Feb 2003 23:04:22 +0100 (MET) Received: from newb6.u-strasbg.fr(130.79.128.16) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAO7aaSu; Thu, 20 Feb 03 23:04:21 +0100 Received: from astro.u-strasbg.fr (localhost [127.0.0.1]) by newb6.u-strasbg.fr (8.9.3/8.9.3) with ESMTP id XAA10523 for ; Thu, 20 Feb 2003 23:00:29 +0100 (MET) Sender: derriere@newb6.u-strasbg.fr Message-ID: <3E554FFD.6BD3BD89@astro.u-strasbg.fr> Date: Thu, 20 Feb 2003 23:00:29 +0100 From: Sebastien Derriere Organization: Observatoire de Strasbourg X-Mailer: Mozilla 4.7 [en] (X11; I; SunOS 5.6 sun4u) X-Accept-Language: en MIME-Version: 1.0 To: ucd@ivoa.net Subject: UCDs status and perspectives Content-Type: multipart/mixed; boundary="------------4770D292B544D00A3A991C4E" X-MailScanner: Found to be clean X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: This is a multi-part message in MIME format. --------------4770D292B544D00A3A991C4E Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit Hello, I have tried to summarize in a short document the current status of UCDs, and the various suggestions that have been made concerning their possible extension, evolution, refactoring, ... I don't draw any conclusion at the end of this short paper. I just tried to collect the various informations available here and there, and put them together. The goal is to stimulate discussions! Best regards, Sebastien. -- _______ / ~ /, Sebastien Derriere mailto:derriere@astro.u-strasbg.fr / ~~~~ // Observatoire de Strasbourg Phone +33 (0) 390 242 444 /______// 11, rue de l'universite Telefax +33 (0) 390 242 417 (______(/ F-67000 Strasbourg France --------------4770D292B544D00A3A991C4E Content-Type: application/pdf; name="UCD-status0203.pdf" Content-Transfer-Encoding: base64 Content-Disposition: inline; filename="UCD-status0203.pdf" JVBERi0xLjMKMyAwIG9iaiA8PAovTGVuZ3RoIDE1MDIgICAgICAKL0ZpbHRlciAvRmxhdGVE ZWNvZGUKPj4Kc3RyZWFtCnjarVdLc9s2EL7rV/BIzZQwQQAkmJOSuGmbiadpLJ+SHCASMpnw ofBhx/713QVAWZnqYaW5gAS4WOy3j2/BV8vZxRsaexEniUy85dqjnBMKK3EqiUykt8w/+jfz gIWR/9o+LvFB/Rd2dj2oOfWHsccp83HS5PbTZh5Esa87+ESnSTaUd3N86eefl2/hbOFRSlIh 8Gw4WvDUCxJKKLNHXxPQBfKXuutK3Wk7C9zmZGdzHBNJUy8023INdnQdDLAJRr2AQfUDrrYw kDGA0c7R5H51i6trnKPu2e/LGQVdoUfhiJBIwT0RJyRNIy+rZ99mHz+HXj4LvbezkLBUevfw HhKapl49Y1ICDubm1ex69s9WWTBpC3bUvTJR2PUEjSThlHmCJyRh3LpC6z2wo4hEUjjYBQIa 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3e5baf6500000104 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Return-Path: Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h27G0F5O007277 for ; Fri, 7 Mar 2003 17:00:15 +0100 (MET) Received: from eso.org (nb008487.ads.eso.org [134.171.27.211]) by serapis.hq.eso.org (8.11.6+Sun/8.11.6) with ESMTP id h27G2Td06105 for ; Fri, 7 Mar 2003 17:02:29 +0100 (MET) Message-ID: <3E68C20F.7020700@eso.org> Date: Fri, 07 Mar 2003 17:00:15 +0100 From: Marco Leoni Reply-To: Marco.Leoni@eso.org Organization: Astrophysical Virtual Observatory @ESO User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.0.1) Gecko/20020823 Netscape/7.0 (CK-ESO) X-Accept-Language: en-us, en MIME-Version: 1.0 To: ucd@ivoa.net Subject: [Fwd: RE: UCDs - repost] Content-Type: multipart/alternative; boundary="------------080406030705070601010506" X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: --------------080406030705070601010506 Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit -------- Original Message -------- Subject: RE: UCDs - repost Date: Fri, 7 Mar 2003 09:25:19 -0500 From: "Wil O'Mullane" To: registry@ivoa.net I note in your paper you mention not being able to express functions in an Ontology. Many years ago I worked with Ontoloigua and KIF(Knowledge Interchange Format) this indeed allows one to express functions on numbers . http://logic.stanford.edu/kif/kif.html Of course KIF is lisp (Lots of Incomprehensilble Silly Brackets indeed) based and not very pretty . Still I see KSL have now extended Ontalingua in to the web world and suggest provideing it as a Server... it may bear looking at. Perhaps this has already been explored .. wil > > Hello all, > > Maybe some of you have not subscribed to the > ucd@ivoa.net list, but might have interest in > reading the paper I posted there: > > http://www.ivoa.net/forum/ucd/0001.htm > > Sorry for those who received this info twice. > > Sebastien. > -- > _______ > / ~ /, Sebastien Derriere mailto:derriere@astro.u-strasbg.fr > / ~~~~ // Observatoire de Strasbourg Phone +33 (0) 390 242 444 > /______// 11, rue de l'universite Telefax +33 (0) 390 242 417 > (______(/ F-67000 Strasbourg France ----- End forwarded message ----- --------------080406030705070601010506 Content-Type: text/html; charset=us-ascii Content-Transfer-Encoding: 7bit

-------- Original Message --------
Subject: RE: UCDs - repost
Date: Fri, 7 Mar 2003 09:25:19 -0500
From: "Wil O'Mullane" <womullan@skysrv.pha.jhu.edu>
To: registry@ivoa.net 


I note in your paper you mention not being able to express functions in an Ontology.
Many years ago I worked with Ontoloigua and KIF(Knowledge Interchange Format)
this indeed allows one to express functions on numbers .
http://logic.stanford.edu/kif/kif.html

Of course KIF is lisp (Lots of Incomprehensilble Silly Brackets indeed) based and not very pretty .

Still I see KSL have now extended Ontalingua in to the web world and suggest provideing it as a Server... it may bear looking at.

Perhaps this has already been explored ..

wil
> 
>   Hello all,
> 
>   Maybe some of you have not subscribed to the 
> ucd@ivoa.net list, but might have interest in
> reading the paper I posted there:
> 
> http://www.ivoa.net/forum/ucd/0001.htm
> 
>   Sorry for those who received this info twice.
> 
> Sebastien.
> -- 
>     _______
>    /  ~   /, Sebastien Derriere   mailto:derriere@astro.u-strasbg.fr
>   / ~~~~ //  Observatoire de Strasbourg    Phone +33 (0) 390 242 444
>  /______//   11, rue de l'universite     Telefax +33 (0) 390 242 417
> (______(/    F-67000 Strasbourg  France


----- End forwarded message -----
--------------080406030705070601010506-- From - Mon Mar 17 18:40:33 2003 X-UIDL: 3e5baf6500000196 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h2HG5vTd015643 for ; Mon, 17 Mar 2003 17:05:58 +0100 (MET) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h2HG5vK09923 for ; Mon, 17 Mar 2003 17:05:57 +0100 (MET) Received: from gannet.scg.man.ac.uk(130.88.94.110) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAMOaqyt; Mon, 17 Mar 03 17:05:56 +0100 Received: from star1.jb.man.ac.uk ([130.88.24.176]) by gannet.scg.man.ac.uk with esmtp (Exim 2.05 #6) id 18ux6K-000Jtu-00; Mon, 17 Mar 2003 16:04:36 +0000 Received: from [130.88.24.80] (helo=aten) by star1.jb.man.ac.uk with esmtp (Exim 3.03 #2) id 18ux6f-0007Ln-00; Mon, 17 Mar 2003 16:04:57 +0000 Date: Mon, 17 Mar 2003 16:03:55 +0000 (GMT) From: Anita Richards X-X-Sender: amsr@aten To: ucd@ivoa.net, derriere@newb6.u-strasbg.fr Subject: UCD Status and Perscpectives Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Sebastien's 'UCD: Status and Perspectives' gives a very clear summary of the recent discussions, responding on the basis of the considerable experience of CDS. Thanks very much - I actually enjoyed reading it, especially the ontology section. It suggests to me some issues which it would help if we made decisions on, or at least reached a working agreement for the immediate future. Maybe Sebastien (or anyone) could suggest what is most urgently needed for discussion at the IVOA registry meeting Wednesday 19 Mar - is anyone planning a presentation? This is what occurs to me: 1) Registries needs UCDs. 'Status and Perspectives' discusses relevant issues in '3. UCDs and data models'. We need general UCDs which describe an entire data set ("Header metadata"), e.g. for which wavelength regime (Radio, IR, Optical etc) - where such currently UCDs exist, they are often parts or parents, rather than ones which are instantiated. See e.g. [[http://www.stsci.edu/~hanisch/NVO/ResourceServiceMetadataV6.doc][Bob Hanisch ResourceServiceMetadataV6.doc]] or [[http://www.stsci.edu/~hanisch/NVO/ResourceServiceMetadataV6.pdf][ResourceServiceMetadataV6.pdf]] and [[http://wiki.astrogrid.org/bin/view/Astrogrid/RegistrySchema][AstroGrid draft registry schema]] We also need a means to associate header data with column labels, e.g. if all data in one catalogue is at 1.4 GHz and another at 1.6 GHz this currently has two separate column UCDs, PHOT_FLUX_RADIO_1.4G and PHOT_FLUX_RADIO_1.6G - dozens of UCDs in all. Using the atom idea across the header and the columns, this could be achieved using one column UCD PHOT_FLUX, and header UCDs for the wavelength regime (radio) and the nominal frequency. This does require that we evaluate the data corresponding to UCDs, see below. 2) Evaluating data identified by UCDs Many people think of UCDs as primarily for selection of catalogues for a human to then view the contents. This is their primary funtion as far as the Registry is concerned, but for actually executing queries we need to compare values within cagtalogues and possibly associate the results with a new UCD (e.g. compare flux densities to derive a colour). Until recently, UCDs were only evaluated routinely (e.g. via Vizier) in one of the most difficult cases - coordinate conversion. Otherwise, the user said 'give me a list of catalogues containing information about x' and the service converted x into UCDs and returned a list of catalogues containing columns corresponding to x. This is now extended to photometry but only for special formats (see above or the AVO demo). We now need UCDs which can enable selection via evaluating UCDs, e.g. if I want flux density measurements between 1.4 and 1.6 GHz I should be able to access data at 1.5 GHz too, via the registry search seeing there is a catalogue containing radio flux densities, and the query execution finding OBS_FREQUENCY 1.5 GHz - in the header, or as a column heading for a collection of measurements at a range of frequencies, as well as a column PHOT_FLUX. This may be a problem where one UCD describes several columns e.g. TIME_DATE for the start and stop of observations, but we want to evaluate both e.g. for error bars on a proper motion measurement. Or do we just need an algorithm which says 'if there are two TIME_DATEs and they are different, take the difference'? 3. Who reads UCDs? The document asks 'how do I find the proper UCD to decribe my data set'. At present, this is done automatically if you are someone contributing a 'simple' table e.g. out of a paper; the average astronomer is not _forced_ to be exposed to UCDs, and a user doing a search certainly isn't (although they might want to use them directly). Data providers of major archives may need to investigate them to check they are allocated correctly or suggest new ones, as do VO workers. Thus they should be reasonably human-readable and available for anyone, but not restricted to the lowest common denominator of astronomical understanding. We could increase the present number ten or even 100 fold (still <10^5) - I am not saying we should, but we need to be afraid of it. For example, if I am using the SED tool in Aladin, I really do not want to know that an optical data set has UCDs for photometric zero point and colour corrections (although an optical astronomer might and I had to learn...) but fortunately the Aladin prototype SED tool knows how to use these to plot magnitudes in Jy. Conversely an optical astronomer does not want to know parameters associated with radio visibility data but if s/he wants to extract an off-centre image at a certain resolution from the MERLIN archive, they need the extraction tool to know about baseline lengths, visibility integration times etc. to chose a data set with an appropriate field of view and resolution. Thus, completeness of UCDs for their purpose is more important than economy, and in fact the savings in going to an atomic structure would probably mean we could add UCDs for specific errors, and remove the degeneracy of things currently under 'TIME_DATE' or 'NUMBER' etc., without making UCDs unmanagable. As the document says, the creation of new UCDs should certainly be restricted to defined bodies (e.g. via a central monitoring panel) to avoid duplication and maintain consistency at a functional level. This probably means UCDs will proliferate slowly, acquire some clumsy ones, and then be pruned or refactored over a cycle of months or years. Best wishes Anita - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - Dr. Anita M. S. Richards, AVO Astronomer MERLIN/VLBI National Facility, University of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire SK11 9DL, U.K. tel +44 (0)1477 572683 (direct); 571321 (switchboard); 571618 (fax). From - Tue Mar 18 14:13:06 2003 X-UIDL: 3e5baf65000001d2 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h2IDCCBp024644 for ; Tue, 18 Mar 2003 14:12:12 +0100 (MET) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h2IDCCm23350 for ; Tue, 18 Mar 2003 14:12:12 +0100 (MET) Received: from mailsend.le.ac.uk(143.210.16.129) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAmgaGMT; Tue, 18 Mar 03 14:12:11 +0100 Received: from print.star.le.ac.uk ([143.210.36.58] helo=mail.star.le.ac.uk) by homer.le.ac.uk with smtp (Exim 4.14) id 18vGp3-0007YC-7m for ucd@ivoa.net; Tue, 18 Mar 2003 13:08:05 +0000 Received: (qmail 15825 invoked from network); 18 Mar 2003 13:08:39 -0000 Received: from sparky.star.le.ac.uk (143.210.36.10) by mail.star.le.ac.uk with SMTP; 18 Mar 2003 13:08:39 -0000 Date: Tue, 18 Mar 2003 13:08:39 +0000 (GMT) From: "Patricio F. Ortiz" To: Anita Richards cc: ucd@ivoa.net, , Clive Page Subject: Re: UCD Status and Perscpectives In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Spam-Score: -4.4 (----) X-Scanner: exiscan for exim4 *18vGp3-0007YC-7m*E1enz/Tv.fc* X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Hi Anita, as a reflexion on your thought I wrote the following lines, which I think may be relevant. I must add that I agree with your points nearly 100% :-) Cheers, Patricio UCDs for the photometric and time domain. At nearly 5 years since the beginning of the work on UCDs a number of things have evolved which make it worth re-thinking how these two observation-related quantities can be represented for the new usages broght by the advent of the IVO and the possible usages by both human users or machine users (eg registries). Both of these variables can be seen as continuous, and one single observation will cover a certain range in wavelength (frequency) and a certain range in time. Historically, the wavelength domain has been split in "bands" by the use of photometric systems and observing bands in the different domains. UCDs tried to adjust to this scheme as it is useful to find comparable quantities in a simple datamining model. What was done was very similar to have POS_EQ_RA_MAIN_1H, POS_EQ_RA_MAIN_2H... The position in the sky, of course, was never constrained by instrumental settings and systems. Today though, we have seen the broad possibilities of searching in archived data and this scheme attached to UCDs can hardly cope with some of the newly imposed requirements. The problem is not to add more UCDs to the system, as that was seen as a clear possibility since the beginning, but to have a system able to respond in a simple way to queries like "I want observations in this wavelength regime". UCDs can (and should) still be attached to columns for proper characterization of each data column, but a solution can be found in a similar way to characterizing the sky coverage (where one can split the sky in arbitrary tiles and put 1 when observations exist in a given catalogue). What I propose is a system which represents the whole electromagnetic spectrum in a linear way. If one takes the space of log(wavelength) going from 0.003 nm to 3km we have nearly 15 decades of coverage, which could be split in 1000 parts to give enough spectral resolution. Each photometric filter and bandpass will be represented by a series of bits which should be set to 1. A catalogue which contains Jonhson's V magnitue and B-V colour index plus some radio data and X-ray data would have a fingerprint where the bits on will be the ones corresponding to the B and V filters, the radio bandpass(es) and the X-ray band(s). This information will be part of the catalogue's metainformation and should be stored in data-centers and possibly registries to which users will have access. A user may then submit a query to a registry where s/he can decide which ranges in the EMS to search for. The registry machine will create a "search fingerprint" to compare with the catalogues it knows about and/or it could pass this fingerprint to another grid service which will do its own search. The user should then receive a list of catalogue handles which satisfy his/her requirements. A number of scenarios of search logics can be envisioned, from full intersection to partial intersection of fingerprints. That is a point we should develop based on use cases. I've experimented with a solution where I split the interval (in log) in 15000 bins (1000 per decade) and it gives a reasonably good resolution in all wavelength regimes. More testing is needed and suggestions are welcome. The time domain It presents itself as a similar problem to wavelength. One could define a starting point, and fix a time resolution, then each timed observation could be defined by a series of bits set to 1 wherever this observation falls. If one were to take 1 day as the time resolution, 100yrs require 36525 bits If one were to take 1 hour as the time resolution, 100yrs require 876600 bits The numbers look large, but one can represent the time coverage of a catalogue by just a few bits set to 1. Each catalogue time-fingerprint can be reconstructed on the fly. Again, a user may form his/her own time-fingerprint to perform searches, like "I'm interested in recovering data for region X observed in this period of time or periods separated by one year afterwards", eg, one wants to measure proper motions. In summary, by linearizing and binning these two quantities one can build search engines which give users high flexibility to perform searches and solve so the problem of multiplying UCDs to high levels. Patricio F. Ortiz On Mon, 17 Mar 2003, Anita Richards wrote: > > > Sebastien's 'UCD: Status and Perspectives' gives a very clear summary of > the recent discussions, responding on the basis of the considerable ..... --- Dr. Patricio F. Ortiz pfo@star.le.ac.uk AstroGrid project Department of Physics and Astronomy University of Leicester Tel: +44 (0)116 252 2015 LE1 7RH, UK From - Wed Mar 19 15:09:21 2003 X-UIDL: 3e5baf6500000253 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h2JDhkqj029116 for ; Wed, 19 Mar 2003 14:43:46 +0100 (MET) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h2JDhj518646 for ; Wed, 19 Mar 2003 14:43:46 +0100 (MET) Received: from head-cfa.cfa.harvard.edu(131.142.41.8) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAuiaOAK; Wed, 19 Mar 03 14:43:44 +0100 Received: from urania.cfa.harvard.edu (urania [131.142.52.147]) by head-cfa.cfa.harvard.edu (8.12.8/8.12.8) with ESMTP id h2JDaEHG028625 for ; Wed, 19 Mar 2003 08:36:14 -0500 (EST) Received: (from jcm@localhost) by urania.cfa.harvard.edu (8.11.1/8.11.1) id h2JDaDs05535 for ucd@ivoa.net; Wed, 19 Mar 2003 08:36:13 -0500 (EST) Date: Wed, 19 Mar 2003 08:36:13 -0500 (EST) Message-Id: <200303191336.h2JDaDs05535@urania.cfa.harvard.edu> From: jcm@head-cfa.cfa.harvard.edu To: ucd@ivoa.net Subject: UCD Status and Perspectives X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Dear Patricio, I think your suggestion ("UCDs for the photometric and time domain") works well for search engines and catalog queries, but it does not work to describe the data precisely enough to do on-the-fly interconversions ("match this table with fluxes at 4100A to this other table with fluxes at 4200A assuming a spectral index of 0.7") at the level of accuracy wanted for data analysis, never mind the problem of "convert this kind of B filter to this slightly different kind of B filter". Maybe that's OK, but in that case some other language analogous to UCDs will be needed for robust data description and we should be clear that UCDs will only apply to the query process (indeed their current and original intention). Anita's comments are well taken, but perhaps she can clarify: you are suggesting replacing PHOT_FLUX_RADIO_1.4G with PHOT_FLUX and a header UCD of OBS_FREQUENCY 1.4 GHz, right? But what if you have three flux columns in the catalog, ( a bit like the problem you alluded to of TIME_DATE for start and stop), say PHOT_FLUX_RADIO_1.4G and PHOT_FLUX_RADIO_5.0G and PHOT_FLUX_RADIO_22.0G? Then we need three OBS_FREQUENCY header UCDs and a way to map them to the respective columns - which is essentially the 'parameterized UCD' I have suggested elsewhere. - Jonathan McDowell From - Wed Mar 19 15:22:27 2003 X-UIDL: 3e5baf6500000256 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h2JEMEqj007340 for ; Wed, 19 Mar 2003 15:22:14 +0100 (MET) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h2JEMDF20523 for ; Wed, 19 Mar 2003 15:22:13 +0100 (MET) Received: from homer.le.ac.uk(143.210.16.129) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAApRaqfO; Wed, 19 Mar 03 15:22:13 +0100 Received: from print.star.le.ac.uk ([143.210.36.58] helo=mail.star.le.ac.uk) by homer.le.ac.uk with smtp (Exim 4.14) id 18veOK-0005nK-8U for ucd@ivoa.net; Wed, 19 Mar 2003 14:18:04 +0000 Received: (qmail 22813 invoked from network); 19 Mar 2003 14:18:43 -0000 Received: from sparky.star.le.ac.uk (143.210.36.10) by mail.star.le.ac.uk with SMTP; 19 Mar 2003 14:18:43 -0000 Date: Wed, 19 Mar 2003 14:18:43 +0000 (GMT) From: "Patricio F. Ortiz" To: jcm@head-cfa.cfa.harvard.edu cc: ucd@ivoa.net Subject: Re: UCD Status and Perspectives In-Reply-To: <200303191336.h2JDaDs05535@urania.cfa.harvard.edu> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Spam-Score: -4.9 (----) X-Scanner: exiscan for exim4 *18veOK-0005nK-8U*8qbpheX5Fnc* X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Dear Jonathan, On Wed, 19 Mar 2003 jcm@head-cfa.cfa.harvard.edu wrote: > Dear Patricio, > > I think your suggestion ("UCDs for the photometric and time domain") > works well for search engines and catalog queries, but it does not work > to describe the data precisely enough to do on-the-fly interconversions > ("match this table with fluxes at 4100A to this other table with fluxes > at 4200A assuming a spectral index of 0.7") at the level of accuracy > wanted for data analysis, never mind the problem of "convert this kind > of B filter to this slightly different kind of B filter". Maybe that's > OK, but in that case some other language analogous to UCDs will be > needed for robust data description and we should be clear that UCDs will > only apply to the query process (indeed their current and original > intention). I couldn't agree more with you on this point. Discovering the existence of information is one issue, which could be solved with the scheme I proposed, and with UCDs but converting or transforming quantities is a completely different ball game. As we discussed in the meeting at CfA, full characterization of the filters and bandpasses should be achieved before attempting the conversion and a lot of "knowledge" or expertise will be required for us to get to this point. Can you expand on your first example please? "match this table with fluxes at 4100A to this other table with fluxes at 4200A assuming a spectral index of 0.7" What do you have in mind? Do you want to match by position first and then find the sources which have similar fluxes based on 4100 and 4200 band? I find your example quite interesting, that's why I'd like to know more what you have in mind. > > Anita's comments are well taken, but perhaps she can clarify: > you are suggesting replacing PHOT_FLUX_RADIO_1.4G with PHOT_FLUX > and a header UCD of OBS_FREQUENCY 1.4 GHz, right? But what if you > have three flux columns in the catalog, ( a bit like the problem > you alluded to of TIME_DATE for start and stop), say PHOT_FLUX_RADIO_1.4G > and PHOT_FLUX_RADIO_5.0G and PHOT_FLUX_RADIO_22.0G? Then we need three > OBS_FREQUENCY header UCDs and a way to map them to the respective columns > - which is essentially the 'parameterized UCD' I have suggested elsewhere. > > - Jonathan McDowell Although the last question is for Anita, let me jump in the case as well. If I understand well enough, when you produce a catalogue which contain observations in one frequency (band) one might think in calling the column PHOT_FLUX and qualify the whole catalogue. Well, that was exactly the situation we found in the published data. Tables made full sense when attached to their paper, and even the table name could tell us what band someone was observing. There were hundreds of tables where the column name was "Mag"; taking the table out of context (like in a table depository) one had no idea what this Mag meant, that's why UCDs were introduced, to solve this kind of degeneracy. I feel that if we do so with UCDs we'll go backwards in a sense. Jonathan, can you point me to a document with your proposed 'parameterized UCD'? I just searched with google and got nowhere :-( Cheers, Patricio --- Dr. Patricio F. Ortiz pfo@star.le.ac.uk AstroGrid project Department of Physics and Astronomy University of Leicester Tel: +44 (0)116 252 2015 LE1 7RH, UK From - Thu Mar 20 17:00:44 2003 X-UIDL: 3e5baf650000027b X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h2KG0aHA013115; Thu, 20 Mar 2003 17:00:36 +0100 (MET) Received: from eso.org (pc003499.hq.eso.org [134.171.40.117]) by serapis.hq.eso.org (8.11.6+Sun/8.11.6) with ESMTP id h2KG37F04594; Thu, 20 Mar 2003 17:03:07 +0100 (MET) Message-ID: <3E79E53F.3050209@eso.org> Date: Thu, 20 Mar 2003 16:58:55 +0100 From: Markus Dolensky Organization: European Southern Observatory User-Agent: Mozilla/5.0 (X11; U; Linux i686; en-US; rv:1.0.2) Gecko/20030208 Netscape/7.02 X-Accept-Language: en, de-AT MIME-Version: 1.0 To: DIDELON Pierre CC: ucd@ivoa.net Subject: Re: UCDs status and perspectives References: <200303201516.h2KFG7P07723@rosetta.saclay.cea.fr> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Hi Pierre, I couldn't agree more on the notion of your second point: > 2) Adding UCD. > > As Patricio said, "the problem is not to add more UCDs", everbody > would agree on that, but it is certainly _how_ to perform > the metadata bank update, when _really_ needed. > A very strict and tedious approvment by an "expert group", > as proposed in sebastien's doc, is certainly not appropriate > for a lot of cases, where quick even instantaneous > response is needed. > Once more, migrating to parametrized atomic Descr (PAD?), > will perhaps facilitate their dynamic handling. It would be great if we could agree on some rules for using UCDs rather than looking at them individually. This might not be fully in line with the original idea when UCDs were invented as some sort of table column identifiers. The scope, however, is much broader now - it's about meta data in a more general sense. We need them in the registry, as query specifiers, as a way for interpreting VOTable docs, as tags in data models, ... Markus +--- | Markus Dolensky Mailto:Markus.Dolensky@eso.org | AVO Technical Lead Web: www.euro-vo.org | Voice: ++49 89 32006/261 Fax: ++49 89 32006/480 +--- From - Thu Mar 20 16:25:43 2003 X-UIDL: 3e5baf650000027a X-Mozilla-Status: 0013 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h2KFNeHA028549 for ; Thu, 20 Mar 2003 16:23:40 +0100 (MET) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h2KFNdh06854 for ; Thu, 20 Mar 2003 16:23:39 +0100 (MET) Received: from sainfoin.saclay.cea.fr(132.166.192.126) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAARra4xn; Thu, 20 Mar 03 16:23:39 +0100 Received: from rosetta.saclay.cea.fr (rosetta.saclay.cea.fr [132.166.13.210]) by sainfoin.saclay.cea.fr (8.12.8/CEAnet-Internet.1.0) with ESMTP id h2KFG9P4025168 for ; Thu, 20 Mar 2003 16:16:09 +0100 (MET) Received: (from dide@localhost) by rosetta.saclay.cea.fr (8.10.2+Sun/8.10.2) id h2KFG7P07723; Thu, 20 Mar 2003 16:16:07 +0100 (MET) Date: Thu, 20 Mar 2003 16:16:07 +0100 (MET) From: DIDELON Pierre Message-Id: <200303201516.h2KFG7P07723@rosetta.saclay.cea.fr> To: ucd@ivoa.net Subject: RE:UCDs status and perspectives X-Sun-Charset: US-ASCII X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Hello UCD Fan's and Pro's, the ongoing discussion seems very promising to me, and the experts certainly have a goog understanding of that's going on. Nevertheless I would like to make comments on three recurrent subjects. My point of view is perhaps obvious and trivial, but as UCD, and more generaly ontology, try to make implicit assumption became explicit, I felt free to post the following. The points are related to the UCD handling, the way of adding UCD, and UCD usage at different levels. 1) UCD Handling I was very happy to read the following in Sebastien's doc. "The hierchical tree is not fundamental - it's merely a way of classification". What is actually very important for me is the knowledge base represented by the UCDs, which certainly describe very well, even if not exhaustively the columns of astronomical catalogs. The ways, different people want to look at this metadata pond/container will certainly be differents. But actually the UCD structure and even the name structure itself does not promote or facilitate others point of view on this fabulous metadata bank. But as stressed also in sebastien's doc, "it is clear that the definition of right roots does not exist, and is influenced by the user's own needs". It means that a static absolute and final UCD structuration is not realistic, and so "different structures corresponding to different views" of UCD must coexist. It is one more argument in addition to a parametrized and atomic definition of Descriptors. 2) Adding UCD. As Patricio said, "the problem is not to add more UCDs", everbody would agree on that, but it is certainly _how_ to perform the metadata bank update, when _really_ needed. A very strict and tedious approvment by an "expert group", as proposed in sebastien's doc, is certainly not appropriate for a lot of cases, where quick even instantaneous response is needed. Once more, migrating to parametrized atomic Descr (PAD?), will perhaps facilitate their dynamic handling. To clarify my point of view, perhaps a little bit too broad and common, let's take an example. Try to imagine a Web service which can create data on the flight and must be able to assign UCDs to these _dynamic_ data. A very simple example would be a data bank of SED or photometric data covering a very wide spectral range, and which can delivered a flux, mag, color or anyelse sensible combined data at whatever wavelength required by the user. This service don't want to register one predifine UCD for any data conmbination but needs only to parametrize the UCD and perhaps, in the most complex case re-organize the basic predifined atoms. Then the atoms definitions and the combination rules allowed must be approved by an "expert group", but the parameter s and the combinations used can be freely adapted by each data provider, portal or anyelse service or tool. 3) UCD usage at different level As already mention by sebastien and anita, any UCD used as column description in one dataset can be used as header or global metadata in another dataset, and some times an association between these two uses must be performed. To my feeling the answer already exist in the VOTable structure. UCDs exist in two class, FIELD and PARAM. And it is obvious that they are specialization of a more general class which could be called vardescr (variables descriptors). In the particular case of PARAM instances, the values are attached to the description, while for the FIELD the data link is more loosely. Adressing this more general class would certainly facilitate the association between global/header metadata and column description. The main problem is that UCD are historically concerned with column descriptors and so cover very well this field of interest but it is not obvious how exhaustive are the existing UCD to cover the needs of global metadata used in headers (Fits) or definitions (VOTable). I hope that these comments are not out of scope, and that the expression of my feelings are not unpleasant to anybody. Sincerely yours, Pierre Didelon From - Thu Mar 20 18:20:00 2003 X-UIDL: 3e5baf650000027d X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h2KGXDHA027343 for ; Thu, 20 Mar 2003 17:33:13 +0100 (MET) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h2KGXDg15076 for ; Thu, 20 Mar 2003 17:33:13 +0100 (MET) Received: from sainfoin.saclay.cea.fr(132.166.192.126) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcCAAH9aWBD; Thu, 20 Mar 03 17:33:12 +0100 Received: from rosetta.saclay.cea.fr (rosetta.saclay.cea.fr [132.166.13.210]) by sainfoin.saclay.cea.fr (8.12.8/CEAnet-Internet.1.0) with ESMTP id h2KGPeP4002509; Thu, 20 Mar 2003 17:25:41 +0100 (MET) Received: (from dide@localhost) by rosetta.saclay.cea.fr (8.10.2+Sun/8.10.2) id h2KGPcu07938; Thu, 20 Mar 2003 17:25:38 +0100 (MET) Date: Thu, 20 Mar 2003 17:25:38 +0100 (MET) From: DIDELON Pierre Message-Id: <200303201625.h2KGPcu07938@rosetta.saclay.cea.fr> To: Markus.Dolensky@eso.org Subject: Re: UCDs status and perspectives Cc: ucd@ivoa.net X-Sun-Charset: US-ASCII X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: > From Markus.Dolensky@eso.org Thu Mar 20 17:01:00 2003 > To: DIDELON Pierre > CC: ucd@ivoa.net > Subject: Re: UCDs status and perspectives > > Hi Pierre, > > I couldn't agree more on the notion of your second point: > > > 2) Adding UCD. > > > > As Patricio said, "the problem is not to add more UCDs", everbody > > would agree on that, but it is certainly _how_ to perform > > the metadata bank update, when _really_ needed. > > A very strict and tedious approvment by an "expert group", > > as proposed in sebastien's doc, is certainly not appropriate > > for a lot of cases, where quick even instantaneous > > response is needed. > > Once more, migrating to parametrized atomic Descr (PAD?), > > will perhaps facilitate their dynamic handling. > > It would be great if we could agree on some rules for using UCDs rather > than looking at them individually. I totally agree. What I had in mind is not a traduction one by one of all the existing UCD, but the definition of atoms and parameters which allow to handle the existing UCD in a more flexible way. So, PAD can point to UCD, but the reverse would perhaps not always be true. But it is not clear to me, if the two systems coexists in the future, which will be the needs of update synchronism and joined maintenance! >...This might not be fully in line with > the original idea when UCDs were invented as some sort of table column > identifiers. The scope, however, is much broader now That's why PAD is perhaps more appropriate than UCD, because we no longer deal only with column descriptors but with _global_ metadata. >...- it's about meta > data in a more general sense. We need them in the registry, as query > specifiers, as a way for interpreting VOTable docs, as tags in data > models, ... > > Markus > Sorry for being unclear with rough english, cordially, Pierre From - Tue Mar 25 23:35:44 2003 X-UIDL: 3e5baf65000002f9 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h2PMYjwt013519; Tue, 25 Mar 2003 23:34:45 +0100 (MET) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h2PMYiE26012; Tue, 25 Mar 2003 23:34:44 +0100 (MET) Received: from rings.gsfc.nasa.gov(128.183.190.139) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAtMaaZY; Tue, 25 Mar 03 23:34:43 +0100 Received: from rings.gsfc.nasa.gov (rings.gsfc.nasa.gov [128.183.190.139]) by rings.gsfc.nasa.gov (8.9.3/8.9.3) with SMTP id RAA09366; Tue, 25 Mar 2003 17:30:55 -0500 (EST) Message-Id: <200303252230.RAA09366@rings.gsfc.nasa.gov> Date: Tue, 25 Mar 2003 17:30:55 -0500 (EST) From: Kirk Borne Reply-To: Kirk Borne Subject: Re: UCDs status and perspectives To: ucd@ivoa.net, registry@ivoa.net MIME-Version: 1.0 Content-Type: TEXT/plain; charset=us-ascii Content-MD5: tyTDm/xR3n8qPDsjDt1qCw== X-Mailer: dtmail 1.3.0 @(#)CDE Version 1.3.5 SunOS 5.7 sun4u sparc X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Ray: I believe that your suggestions carry a lot of merit. I had a nagging feeling when reading Jonathan's comments that our metadata efforts could easily diverge (as you suggest) if we are not careful. The data model is key to this -- consequently, the ability of XML Schema to carry the knowledge about both the data model and the metadata relationships, using standardized techniques, makes a lot of sense -- especially with regard to reconciling the two metadata approaches that you mention. I think that disaster can be averted, and Jonathan's and your suggestions can illuminate the way. The PHOT_FLUX(PHOT_BAND_ID) is an excellent example of the problem and a good solution. - Kirk > Date: Tue, 25 Mar 2003 15:15:13 -0600 (CST) > From: Ray Plante > To: ucd@ivoa.net > Subject: Re: UCDs status and perspectives > > We have been bouncing around in our community two models for tagging > metadata that we will eventually need to reconcile. One is essentially > XML-based and the other is based on the current UCD set. The former makes > the most sense for descriptions stored in a registry, while the latter is > useful for tagging a set of data (e.g. in a table column). Both are > important and necessary. Both reflect a common data model. However, it > would inconvenient if not disasterous if there were not a direct > correlation between to two representations. > > I feel the answer can be found in existing XML technologies. I would > claim that the atomic descriptors being discussed (PAD, PCD, etc.) are > really just a short hop from an XML model. The main thing that PCD has > in common with XML tags is that both are essentially pointers into a > data model. The main difference between them is that with a UCD/PCD, we > need that pointer to be representable as a simple string (e.g. that can be > put in the ucd attribute in a VOTable). > > XML has such a pointer; it's called an XPath. If we define the data > model as an XML Schema, then our UCD/PCDs fall right out. There are other > advantages: > * XML Schema provides a machine readable form for a data dictionary. > * The extensibility of XML schemas provides the extensibility for > UCDs automatically. > * When necessary, metadata in direct XML form (as envisioned in a > registry) into UCD-tagged VOTable data. > * The modeling that Jonathan proposed is largely still applicable. > * The approach is consistant with the data modeling activities that > have been done to date. > > As an example, consider the example Jonathan cited: > > > For instance the two UCDs PHOT_FLUX_RADIO_1.4G > > and PHOT_FLUX_RADIO_1.6G would map to a single PCD > > PHOT_FLUX(PHOT_BAND_ID) with PHOT_BAND_ID taking the values 1.4 GHz and > > 1.6 GHz. > > Suppose a data model defined more or less in the following way: > > > > > > Secondly, however, how much can be done 'seamlessly' based on the > existing, working CDS UCD system? It is important to keep that going, not > just because astronoemrs depend on it and want to see it do these things > they hear about in reports from VO meetings, but because we need to test > developments on the community as much as possible, and we will find > subjects much more easily if we can give people prototypes which look as > familiar as possible (as with the AVO demo). Also many new functions e.g. > the SED tool and VOPlot are being developed based on the existing UCDs. I completely agree. It will take some time to shake out a refactored model that covers everything already in the current UCDs. Therefore, we will need a mechanism for continuing to support UCDs as they are now. It's important to note that the current UCDs represent the most practical use-case as they were drawn directly from real catalogs. As we build up more complicated models, e.g. photometry measurements, even images, we will need to make sure that the relevent UCD concepts are covered. In fact, that could be made a formal of the definition process. cheers, Ray From - Wed Mar 26 17:25:45 2003 X-UIDL: 3e5baf6500000315 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h2QGNJx1002075 for ; Wed, 26 Mar 2003 17:23:34 +0100 (MET) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h2QGJpr10085 for ; Wed, 26 Mar 2003 17:19:51 +0100 (MET) Received: from smtp1.linkline.com(66.59.240.1) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAAaaGRt; Wed, 26 Mar 03 17:19:50 +0100 Received: from roxy (dsl-pb-1504.linkline.com [64.30.223.60]) by smtp1.linkline.com (Postfix) with SMTP id 6F6259F63C for ; Wed, 26 Mar 2003 08:15:46 -0800 (PST) Message-ID: <003a01c2f3b3$727a2be0$6601a8c0@roxy> From: "Roy Williams" To: Subject: Fw: UCDs and XML Date: Wed, 26 Mar 2003 08:19:13 -0800 MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1106 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: My thinking on UCD is going around the idea of "recognition". In writing code for VO applications, I am looking for specific UCDs. Reading the result of a cone search means finding the POS_EQ_RA_MAIN. Reading the result of a SIAP means looking for the UCD called VOX:Image_AccessReference. Therefore it should be allowed to have multiple UCDs describing the same attribute, so that different applications can recognize and use it. One person sees a galaxy, another sees a database record, another sees clip-art -- but it's all the same entity underneath. This recognition idea allows us to use UCD to subclass objects. If I have a table from a cone search, then it must have UCDs corresponding to RA, Dec, ID. Let us subclass this, for example, to a service that returns black-hole candidates. In this case, we would expect further UCDs to be present: BH_mass and BH_Spin. There is a lot that can be done with UCD, and the real question is how to allow this semantic flexibility to blossom, but without having everyone make their own UCD and losing all interoperability! Roy --- Caltech Center for Advanced Computing Research roy@cacr.caltech.edu 626 395 3670 From - Tue Mar 25 04:55:44 2003 X-UIDL: 3e5baf65000002cc X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h2P3orhM002011 for ; Tue, 25 Mar 2003 04:50:53 +0100 (MET) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h2P3oq202132 for ; Tue, 25 Mar 2003 04:50:52 +0100 (MET) Received: from head-cfa.cfa.harvard.edu(131.142.41.8) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAdHaWje; Tue, 25 Mar 03 04:50:50 +0100 Received: from urania.cfa.harvard.edu (urania [131.142.52.147]) by head-cfa.cfa.harvard.edu (8.12.8/8.12.8) with ESMTP id h2P3hKaU027490 for ; Mon, 24 Mar 2003 22:43:20 -0500 (EST) Received: (from jcm@localhost) by urania.cfa.harvard.edu (8.11.1/8.11.1) id h2P3hJN18502 for ucd@ivoa.net; Mon, 24 Mar 2003 22:43:19 -0500 (EST) Date: Mon, 24 Mar 2003 22:43:19 -0500 (EST) Message-Id: <200303250343.h2P3hJN18502@urania.cfa.harvard.edu> From: jcm@head-cfa.cfa.harvard.edu To: ucd@ivoa.net Subject: Re: UCDs status and perspectives X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Dear UCD list, Following the discussion of last week, I append below some notes on a controlled vocabulary related to UCDs that I sent to Sebastien some time ago. It represents a more radical change than most people are probably ready to go for, but I think it may be relevant to the current discussion. - Jonathan McDowell -------------------------------------------------------------------- I've been thinking a lot this week about UCDs and their possible role in VO data models. My conclusion is that while the present design of UCDs is very useful for the catalog cross matching problem, we need a somewhat more flexible data dictionary to handle the data analysis problem. I think we need both kinds of dictionary, with of course a mapping between the two for the applications that need the appropriate ones. Specifically, I propose to parallel the UCDs with PCDs (Parameterized Content Descriptors). These differ from UCDs in that they can include functional parameters. For instance the two UCDs PHOT_FLUX_RADIO_1.4G and PHOT_FLUX_RADIO_1.6G would map to a single PCD PHOT_FLUX(PHOT_BAND_ID) with PHOT_BAND_ID taking the values 1.4 GHz and 1.6 GHz. This reflects the fact that PHOT_FLUX_RADIO_1.4G and PHOT_FLUX_RADIO_1.6G do not really describe fundamentally different physical quantities. The PCD also differ from UCD in that they are organized to form the bottom level attributes of a structured data model for astronomy, so the top level domains are different from the UCDs. So far my proposed main PCD fields are (1) about the universe PHYS Physical data which is true generally and not a property of a specific astronomical location or object. POP Properties of a population of astronomical objects SAMPLE Properties of a sample of sources. OBJ The things we study are astronomical objects in space (with more or less defined boundaries). MED To understand the physics of these objects we describe the physical medium constituting them, including matter (solid, liquid, gas, plasma), radiation, and electromagnetic, gravitational and other fields. LOS A direction on the sky we observe corresponds to a line of sight along which objects may lie. (2) about our observations of the universe SRC When we have a dataset, we can identify a subset of that dataset as a source, which we can identify with an object. PCDs are SRC when they are to do with the direct measurements of an object with a telescope, and OBJ when they are to do with the intrinsic properties of the object (in its rest frame, without LOS effects etc). BKG A special sort of source we call the background OBS We have to describe things to do with the observing instrument, configuration and conditions. (a major subset is OBS_COV_ which ) SURVEY_ A group of observations SRC_PHOT We measure the absolute intensity of radiation from the sky SRC_SPEC Like PHOT, but dealing with many photon energies at once? EVENT A detected photon or background event _POS Information about positions (also OBJ_POS etc) _TIME Information about times (also in OBS_COV_TIME...?) (3) about our analysis of the observations DATA We also need to describe things about the datasets themselves. REFER Bibliographic info Below I give my first attempt at mapping the UCDs to a data model oriented set of PCDs. There are quite a few UCDs that I still have to understand by looking at their actual use in catalogs, so this is only a sketch and some are left blank. At the end I give the beginnings of extra UCD/PCD names needed for X-ray astronomy datasets. Appendix 1: A possible list of PCDs to be the data model equivalent of UCDs. Given in UCD alphabetical order. PHYS_AT_ AT Atomic Data PHYS_AT_COLL AT_COLL Atomic Collisional Quantities PHYS_AT_COLL_RATE AT_COLL_EXCIT-RATE Collisional Excitation Rate # Is this an atom prop or a line prop? PHYS_AT_COLL_STRENGTH AT_COLL_STRENGTH Collisional strength PHYS_AT_CONFIG . AT_CONFIG Electronic Configuration PHYS_AT_CONST? AT_CONSTANT Atomic Constant PHYS_AT_DAMPING_ AT_DAMPING Atomic Damping Quantities PHYS_AT_DAMPING_VDW AT_DAMPING_VDWAALS Van der Waals damping ? AT_DATA Various Atomic data PHYS_AT_DEGEN? AT_DEGENERACY Atomic Degeneracy Parameter PHYS_AT_DIPOLE_? AT_DIPOLE Atomic Dipole ? AT_DIPOLE_MISC Atomic Dipole PHYS_AT_DIPOLE_MOMENT AT_DIPOLE_MOMENT Atomic Dipole Moment PHYS_AT_EIGENVECTOR AT_EIGENVECTOR Atomic Eigenvector PHYS_AT_ELECCOEFF AT_ELEC-COEFF Atomic Electric Coefficient PHYS_AT_ELEMENT AT_ELEMENT Atomic Element Name or number, eventually with ionization stage # See also PHYS_AT_Z PHYS_PLASMA_EMISSIVITY_AT AT_EMISSIVITY Atomic Emissivity #What does this mean? It's a function of physical conditions. #It's a property of the plasma expressed on a per-atom basis. #So it's not PHYS_AT_EMISSIVITY but #eg PHYS_PLASMA_EMISSIVITY_AT(Z,T,n) PHYS_AT_ENERGY_ AT_ENERGY Atomic Energy or Potential #Heterogeneous class? PHYS_AT_TRANS_NAME AT_ENERGY_BAND Atomic (molecular) Energy Band PHYS_AT_TRANS_ENERGY_DISCREPANCY AT_ENERGY_DIFF Energy difference between experimental and calculated quantities PHYS_AT_TRANS_ENERGY AT_ENERGY_EXCIT Excitation Energy PHYS_AT_STATE_ENERGY_IONIZATION AT_ENERGY_IONIZ Ionization Energy or Potential PHYS_AT_STATE_ENERGY(LEVEL) AT_ENERGY_LEVEL Energy Level PHYS_AT_ENERGY_FORM AT_ENERGY_FORMATION Formation energy (or heat for molecules) PHYS_AT_ENERG_POT AT_ENERGY_POTENTIAL Atomic Energy or Potential PHYS_AT_STATE_ENERGY_ROT AT_ENERGY_ROTATION Rotation Energy PHYS_AT_STATE_ENERGY_TOT AT_ENERGY_TOTAL Total atomic energy PHYS_AT_TRANS_FREQ AT_FREQUENCY Transition Frequency PHYS_AT_TRANS_FREQ_REST AT_FREQUENCY_NU Transition Frequency at rest PHYS_AT_TRANS_FREQ_ROT AT_FREQUENCY_ROTAT Rotation Frequency PHYS_AT_FS_ AT_FS Fine Structure Quantities PHYS_AT_FS_COLLSTR AT_FS_COLL-STR Fine Structure Collision Strength PHYS_AT_FS_CONST? AT_FS_CONSTANT Fine Structure Constant PHYS_AT_TRANS_FS_WIDTH AT_FS_CONTRIB Fine Structure Contribution to Line Profile PHYS_AT_TRANS_FS_SPLIT AT_FS_SPLIT Fine Structure Splitting PHYS_AT_TRANS_GA AT_GA Atomic ga value PHYS_AT_LINE_INTENSITY AT_INTENSITY Line Intensity PHYS_AT_ION_ AT_ION Ions PHYS_AT_ION_ID AT_ION_ID Ion Identification PHYS_AT_ION_STAGE AT_ION_STAGE Ionization Stage PHYS_AT_LANDEFACT AT_LANDE-FACT Lande Factor (gf) PHYS_AT_LEVEL AT_LEVEL Level Identification PHYS_AT_STATE_LIFE AT_LIFETIME Radiative Lifetime PHYS_AT_LINE_ AT_LINE Atomic or Molecular Lines # What is the difference between LINE and TRANS? PHYS_AT_LINE_EMISSIVITY AT_LINE_EMISSIVITY Line Emissivity PHYS_AT_LINE_FLOURYIELD AT_LINE_FLUOR-YIELD Line Fluorescence Yield PHYS_AT_LINE_ID AT_LINE_ID Line Identification PHYS_AT_LINE_STRENGTH AT_LINE_STRENGTH Line Strength PHYS_AT_LINE_MAIN-TERM? AT_MAIN-TERM Main Term PHYS_AT_MOL_ AT_MOL Quantities Related to Molecules PHYS_AT_MOL_DIELFN AT_MOL_DIEL-FN Molecular Dielectric Function PHYS_AT_MOL_EDISSOC AT_MOL_DISS-ENRGY Molecular Dissociation Energy PHYS_AT_MOL_ID AT_MOL_ID Molecule Identification PHYS_AT_TRANS_MOL_LEVEL AT_MOL_LEVEL Molecule Transition Level PHYS_AT_MULTIPLET_ AT_MULTIPLET Quantities Related to Multiplets PHYS_AT_MULTIPLET_ID AT_MULTIPLET_ID Multiplet Identification PHYS_AT_MULTIPLET_N AT_MULTIPLET_N Multiplet Number element PHYS_AT_Z AT_NUMBER Atomic Number PHYS_AT_OSC_ AT_OSC Oscillator Related Quantities PHYS_AT_OSC? AT_OSC_STRENGTH Oscillator Strength PHYS_AT_PARITY AT_PARITY Atomic Parity PHYS_AT_Q_ AT_Q-N Atomic Structure, Quantum Numbers PHYS_AT_Q_L AT_Q-N_ANG-MOM Angular Momentum Quantum Number PHYS_AT_Q_K AT_Q-N_K K quantum number PHYS_AT_Q_UNK AT_Q-N_MISC Atomic Structure Quantum Number PHYS_AT_Q_ORB AT_Q-N_ORBITAL Orbital Quantum Number PHYS_AT_Q_PRIN AT_Q-N_PRINCIPAL Principal Quantum Number PHYS_AT_Q_PRIN1 AT_Q-N_PRINCIPAL_FIRST First Principal Quantum Number PHYS_AT_Q_PRIN2 AT_Q-N_PRINCIPAL_SECOND Second Principal Quantum Number PHYS_AT_Q_ROT AT_Q-N_ROTATIONAL Rotational Quantum Number PHYS_AT_Q_TOR AT_Q-N_TORSIONAL Torsional Quantum Number PHYS_AT_Q_VIB AT_Q-N_VIBRATIONAL Vibrational Quantum Number PHYS_AT_REACTION AT_REACTION Atomic Reaction PHYS_AT_SHELL AT_SHELL-NUMBER Shell Quantum Numbers PHYS_AT_SPECIES_LIST AT_SPECIES Atomic Species Participating in a Reaction PHYS_AT_TRANS_STARK_ AT_STARK Stark Effect PHYS_AT_TRANS_STARK_BROAD AT_STARK_BROAD Broadening due to Stark Effect PHYS_AT_TRANS_STARK_INT AT_STARK_INTENSITY Intensity due to Stark Effect PHYS_AT_TRANS_SWEIGHT AT_STAT-WEIGHT Statistical Weight PHYS_AT_TRANS_WIDTH? AT_STRENGTH-PARAM Strength Parameter or Expect Width PHYS_AT_TRANS AT_TRANS Quantities Related to Transitions PHYS_AT_TRANS_BRANCH AT_TRANS_BRNCH-RATIO Transition Branching Ratio PHYS_AT_TRANS_ENERGY AT_TRANS_ENERGY Transition Energy (or wave number) PHYS_AT_TRANS_ID AT_TRANS_ID Transition Identification PHYS_AT_TRANS_LEVELS AT_TRANS_LEVELS Transition Level PHYS_AT_TRANS_PROB AT_TRANS_PROB Transition Probability PHYS_AT_TRANS_STRENGTH AT_TRANS_STRENGTH Transition Strength PHYS_AT_TRANS_TYPE AT_TRANS_TYPE Transition Type PHYS_AT_TRANS_RECOMB AT_TRANS_RECOMBIN Recombination coefficients in atomic transitions PHYS_AT_TRANS_LAMBDA AT_WAVELENGTH Laboratory or Theoretical Line Wavelength PHYS_AT_WEIGHT AT_WEIGHT Atomic Weight OBJ_CLASS+ CLASS Various Classification Descriptors OBJ_CLASS_CODE CLASS_CODE Classification Code OBJ_CLASS_COLOR CLASS_COLOR Color Classification OBJ_CLASS_STAR_MK_TYPE OBJ_CLASS_CLG_DIST CLASS_DISTANCE Abell Distance Class OBJ_CLASS CLASS_MISC Various Classification Descriptors OBJ_CLASS CLASS_OBJECT Object Type Classification OBJ_CLASS_CLG_RIC CLASS_RICHNESS Abell Richness Class OBJ_CLASS_UNK_GAL CLASS_STAR/GALAXY Star galaxy discriminator or classification. OBJ_CLASS_UNK_BM CLASS_STRUCT Structure Classification (e.g. cluster Bautz-Morgan classification) _CODE CODE Codes or Flags _ERROR_CODE CODE_ERROR Flag denoting uncertainty about a given quantity _FLAG_LIMIT CODE_LIMIT Lower or Upper limit Flag _FLAG_MEMB CODE_MEMB Membership Code _CODE CODE_MISC Miscellaneous Codes or Flags OBJ_CLASS_MULT CODE_MULT Codes related to Multiplicity (particularly stars) OBJ_CLASS_MULT CODE_MULT_FLAG A code or flag indicating a multiplicity of binarity OBJ_CLASS_MULT_N CODE_MULT_FREQUENCY Multiplicity Frequency Code OBJ_CLASS_MULT_N CODE_MULT_INDEX Multiplicity Index Code _QUAL CODE_QUALITY Quality Code OBJ_CLASS_VAR CODE_VARIAB Variability Code or Flag DATA_ DATA Quantities Related to the Data _SCALE_EXP DATA_FACTOR-EXP Scale Factor Exponent (Base 10) DATA_LINK DATA_LINK Link to additional data (in VizieR or any other database) _MAX DATA_MAXIMUM Maximum data value found in a database column _SCALE DATA_SCALE-FACTOR Factor to Convert a Data Column to a normal value _DATATYPE DATA_TYPE Data Type DYN_ DYN Dynamic Data Quantities (mixed column content) DYN_QUANTITY DYN_QUANTITY Used when a Column means more than one thing. DYN_VALUE DYN_VALUE Identification of a Dynamic Value _ERROR ERROR Error or Uncertainty in Measurements POS(,EQ)_RA_ERROR ERROR # I/176 POS(,EQ)_DEC_ERROR ERROR # I/176 PHOT_FLUX(5 GHz)_ERROR ERROR # VIII/14 SRC_REG EXTENSION Quantities used to describe the extension in the sky of objects SRC_REG_AREA EXTENSION_AREA Angular Area Covered by an Object SRC_REG_DIA_DEC EXTENSION_DEC Angular Extension in Declination SRC_REG_DIA EXTENSION_DIAM Angular Diameter or Size of the Major Axis SRC_REG_DIA_FWHM EXTENSION_FWHM Angular Full Width at Half Maximum (FWHM) SRC_REG_DIA_FWHM EXTENSION_FWHM_CIRC Angular Full Width at Half Maximum (FWHM) SRC_REG_DIA_MAJ_AXIS_FWHM EXTENSION_FWHM_MAJ Angular FWHM along the Major Axis SRC_REG_DIA_MIN_AXIS_FWHM EXTENSION_FWHM_MIN Angular FWHM along the Minor Axis SRC_REG_DIA_MIN_AXIS_FWHI EXTENSION_HALFINT Angular Size at Half Intensity along the Minor Axis SRC_REG_DIA_MIN_AXIS EXTENSION_MIN Angular Diameter of an object along the Minor Axis SRC_REG_DIA_BEAMS EXTENSION_NORM Angular diameter normalized to beam size SRC_REG_DIA_RA EXTENSION_RA Angular extension in right ascension SRC_REG_RADIUS EXTENSION_RAD Angular radius of an object or Semi-major axis SRC_REG_RADIUS_SCALELENGTH EXTENSION_SC-LENGTH Angular Scale Length (bulge or disk) SRC_REG_RADIUS_MIN_AXIS EXTENSION_SMIN Angular size of Semi-Minor Axis _FIT FIT Fits of Models to Observational Data _FIT_ERR FIT_ERROR Fit Error _FIT_GOODNESS FIT_GOODNESS Fit Goodness _FIT_ID FIT_ID Identification of the fit or solution POP_LF FIT_LF Luminosity function POP_LF_FIT_PARAMS FIT_LF Fit of Luminosity Function POP_LF_FIT FIT_LF_GENERAL Fit of Luminosity Function POP_LF_FIT_MAG? FIT_LF_MAG Magnitudes related to the LF POP_LF_FIT_MAG_MAX FIT_LF_MAG_MAX Magnitude interval upper limit POP_LF_FIT_MAG_MIN FIT_LF_MAG_MIN Magnitude interval lower limit _FIT_RATIO FIT_MEAS/THEOR Ratio of Measurement to Theoretical Value _FIT_PAR FIT_PARAM Fit Parameter _FIT_PAR_ID FIT_PARAM_ID Fit Parameter Identification _FIT_MISC FIT_PARAM_MISC Miscellaneous fit parameters POS(,EQ)_RA_STAT_SIGMA FIT_PARAM_MISC # In I/176 S0RA, FIT_PARAM_MISC is the sigma-0 (?) for the RA _FIT_COVAR FIT_PARAM_COVAR Covariance of the fitting parameter _FIT_RESID FIT_RESIDUAL Fit Residual _FIT_CHI2 FIT_CHI2 Chi-square Fit Measurement _FIT_SIGMA FIT_STDEV Fit's Standard Deviation _FIT_TYPE FIT_TYPE Fit or Solution Type POS(,EQ)_FIT_TYPE FIT_TYPE I/176 _ZERO FIT_ZP Fit Zero Point (mostly in linear fits) PHOT_COL_INDEX_DIFF FIT_ZP # In III/218 DIFF, FIT_ZP is the scatter in mag of the spectroscopic index POS(,EQ)_DEC_STAT_SIGMA FIT_ZP # In I/176 S0DE, FIT_ZP is the sigma-0 (?) in arcseconds? for the Dec - ID Fields Used as Identifiers OBJ_ID_ALT ID_ALTERNATIVE Alternative identification OBJ_ID_FIELD ID_AREA Area Identification (usually in a photographic plate) SRC_ID_XID ID_ASSOCIATED Identification of Associated Object (counterpart) SRC_ID_AUTHOR ID_AUTHOR Author Name SRC_ID_CAND ID_CANDIDATE Candidate Identification SRC_ID_CAT ID_CATALOG Catalog Identification SRC_ID_FCHART ID_CHART Finding Chart Identification SRC_ID_COMP ID_COMPARISON Name of a Comparison Object SRC_ID_CONSTEL ID_CONSTEL Constellation Name SRC_ID_XID ID_CROSSID Cross Identification (counterpart) OBS_DB_ID ID_DATABASE Database Identification OBS_DS_ID ID_DATASET Data-Set Identification OBS_EXP_ID ID_EXPOSURE Exposure Identification INST_FIBER ID_FIBER Fiber Optics Identification (for M.O.S.) OBS_FIELD ID_FIELD Field Identification SRC_NOTES_FIG ID_FIGURE Figure Identification Number SRC_NOTES_FILE ID_FILE File Identification SRC_NOTES_FRAME ID_FRAME Frame Identification ? ID_GROUP Group Identification OBS_AUTHOR_CODE ID_HUMAN Identification of Discoverer or Observer SRC_DISCOVERER_CODE ID_HUMAN SRC_ID_INTERNAL ID_IDENTIFIER Identification of a source or object, incomplete or for internal use. OBS_IMAGE_ID ID_IMAGE Image Identification SRC_ID (or OBJ_ID?) ID_MAIN Main Identifier of a Celestial Object SRC_ID:1 ID_MAIN:1 First component of an identification field. SRC_ID:2 ID_MAIN:2 Second component of an identification field. SRC_ID:3 ID_MAIN:3 Third component of an identification field. ? ID_MAP Map Identification SRC_CAT_ID ID_NUMBER Numeric Identification (usually sequential) ? ID_PARAM Identification or name of a parameter, or the name of a column in a table SRC_PARENT ID_PARENT Parent Identification (galaxy, cluster, nebulae) OBS_PLATE ID_PLATE Plate Identification OBS_REGION_ID ID_REGION Region Identification (not necessarily sky region) OBS_SET_ID ID_SET Set or Subset Identification, also bin or sample number OBS_SITE_ID ID_SITE Site/Location/Observatory/City/Country identifier INST_APER_ID ID_SLIT Slit Identification (usually in the context of M.O.S.) # Hmm MOS have many apertures, 1 disperser? SRC_ID_SURVEY ID_SURVEY Survey Identification SRC_ID_TABLE ID_TABLE Table Identification SRC_ID_TARGET? ID_TARGET Target Identifier OBJ_CLASS_VAR? ID_VARIAB Variable Object Identification DATA_PROC_SYS_VER ID_VERSION Identification of the software version. ? ID_VOLUME Volume Identification ? ID_ZONE Durchmusterung zone identification/sign INST_ INST Instrumental Quantities - INST_ANG Angular Properties of the Instruments/Telescopes SRC_OFFAX INST_ANG_OFFAXIS Off-axis angle respect to main direction of observation # Presumably the instrument coords of a source, not a prop of the instru OBS_SITE_ORBIT_PHASEANG INST_ANG_PHASE Satellite phase angle INST_RESP_SPATIAL_RES INST_ANG_RESOL Angular resolution of instrument OBS_SITE_ORBIT_ANGVEL INST_ANG_VEL Satellite angular velocity INST_DET_NOISE_TANT INST_ANTENNA-TEMP Antenna temperature INST_GEOM_DIA INST_APERT Instrument/telescope aperture INST_GEOM_AREA INST_AREA Collecting area or detector area PHOT_BKG_INST INST_BACKGROUND Background contribution INST_COV_BAND INST_BAND Instrumental Band quantities INST_CAL_BAND_DRIFT INST_BAND_DRIFT Band's drift rate INST_COV_BAND_TRANS? INST_BAND_PASS Bandpass INST_COV_BAND_WIDTH INST_BANDWIDTH Spectral window used for the observation INST_INT_BASELINE INST_BASELINE Baseline (interferometry) INST_RESP_SPATIAL INST_BEAM Beam properties ? INST_BEAM_MISC Miscellaneous beam properties INST_RESP_SPATIAL_RES INST_BEAM_SIZE Beam width or size INST_DET_NOISE_TBEAM INST_BEAM_TEMP Beam temperature INST_PHOT_CAL INST_CALIB Instrument calibration quantities INST_PHOT_CAL_ERR INST_CALIB_ERROR Instrument calibration error ? INST_CALIB_MISC Miscellaneous instrument calibration quantities ? INST_CALIB_PARAM Calibration parameter ? INST_CORR-FACTOR Correction (no only correction factor) INST_DET INST_DET Detector parameters INST_PHOT_FLUX_LIMIT INST_DET_LIMIT Detector limit UNK INST_DET_MISC Miscellaneous quantities related to the detector (plate or CCD) INST_GEOM_SIZE INST_DET_SIZE Detector size # number of pixels, vs DET_SIZE with mm size INST_DISP_SCALE INST_DISPERSION Dispersion scale in a spectrograph INST_QE INST_EFFICIENCY Instrument efficiency PHOT_ERR_INST INST_ERROR Errors associated to the instrument INST_FILTER INST_FILTER Filter characteristics INST_FILTER INST_FILTER_CODE Filter characteristics type/code INST_COV_BAND_FWHM INST_FILTER_FWHM FWHM of the used filter (also bandpass) INST_COV_BAND_TRANS INST_FILTER_TRANSM Transmission characteristics of the filter (response) INST_NAME INST_ID Instrument/Detector Identification INST_LINE_WIDTH INST_LINE-WIDTH Instrumental Line-Width INST_DET_NOISE INST_NOISE Detector/Instrument noise level rms INST_PARAM? INST_PARAM Various Instrumental Parameters INST_GEOM_PIX_SIZE INST_PIXSIZE Pixel Size # distinguish pix size in mm and arcsec INST_DET_PLATE INST_PLATE Quantities related to Photographic Plates INST_DET_SIZE INST_PLATE_DIMENSION Size or plate dimension # Is the fact that it's a plate relevant? could be any detector SRC_OFFSET_PIX INST_PLATE_DIST Distance measurement on a plate # ? distance between two sources in pixels? INST_DET_PLATE_EMULSION INST_PLATE_EMULSION Plate Emulsion Type # Now we care about it being a plate, only plates have emulsion SRC_REG_DIA_PIX INST_PLATE_EXTENSION Extension of an object in a plate (in plate units) INST_DET_POS INST_POS Position on a detector or M.O.S template INST_PHOT_PRECISION INST_PRECISION Instrumental Precision # Presumably photometric? INST_RESP_SPATIAL INST_PSF Detector's Point Spread Function (PSF) INST_DET_QE INST_QE Detector's Quantum Efficiency SRC_DET_SN INST_S/N Instrumental signal to noise ratio (S/N) # What does this mean? The S/N for a particular source? INST_RESP_TIME_RES INST_SAMP-TIME Instrumental Sampling Time INST_GEOM_SCALE INST_SCALE Instrumental Scale (ccd or plate) # In arcsec/mm? otherwise pixel size INST_RESP_SPATIAL_RES INST_SEEING Seeing or fwhm of PSF INST_PHOT_FLUX_LIMIT INST_SENSITIVITY Detector's Sensitivity (Flux limit) INST_SETUP INST_SETUP Instrument configuration or set-up - INST_SKY Instrumental Sky Properties PHOT_COUNTS_SKY? INST_SKY_LEVEL Local Sky Level PHOT_TEMP_SKY INST_SKY_TEMP Sky Temperature PHOT_TEMP_SIGMA_SKY INST_SKY_SIGMA Sigma of sky value distribution - INST_SPECT Spectroscopic instruments' quantities INST_COV_BAND_LAMBDA_RANGE INST_SPECT_BAND Spectroscopic observation band INST_DISP_TYPE_CODE INST_SPECT_CODE Spectroscopic instrument specification (prism, grism, grating) INST_DISP_ORDER INST_SPECT_ORDER Spectral Order INST_DISP_SLIT_DX INST_SPECT_SLIT-LENGTH Slit Length INST_DISP_SLIT_DY INST_SPECT_SLIT-WIDTH Slit Width - INST_TEMP Instrument Temperature (radio regime) INST_DET_NOISE_TBEAM INST_TEMP_BEAM Beam Temperature or Brightness # TEMP_BEAM is a way of describing the instrument noise INST_DET_TSYS INST_TEMP_SYST System Temperature INST_DET_TRIGGER? INST_TRIGGER Detector's triggering Threshold INST_TYPE INST_TYPE Instrument Type INST_COV_BAND_VEL? INST_VELOC Velocity Quantities at the Instrumental Level INST_COV_BAND_VEL0 INST_VELOC_CENTRAL Instrumental Central Velocity INST_COV_BAND_VEL_RES INST_VELOC_SPACING Instrumental Velocity Channel Spacing INST_COV_BAND_VEL_RANGE INST_VELOC_WINDOW Detector's Velocity Range OBS_COV_BAND_LAMBDA INST_WAVELENGTH Observation's Wavelength properties # We should distinguish between the wavelength coverage designed into an instrument # and the wavelength coverage of a specific observation, I think the latter is meant here. OBS_COV_BAND_LAMBDA_RANGE INST_WAVELENGTH_COVERAGE Instrument's Wavelength Range OBS_COV_BAND_LAMBDA_EFF INST_WAVELENGTH_EFFECTIVE Observation's Effective Wavelength OBS_COV_BAND_LAMBDA INST_WAVELENGTH_VALUE Wavelength related to an instrument, filter, etc. MUTUAL_OCCULT(*OBJ) - MUTUAL_OCCULT(L) LUNAR-OCCULT Lunar Occultaion related quantities # Occultations of anything could have the same parameters. So let's specify that # it's lunar by an argument L, and generalize eg # MUTUAL_OCCULT(PLUTO)_ANG MUTUAL_OCCULT(L)_ANG LUNAR-OCCULT_ANGLE Lunar Occultation Contact Angle MUTUAL_OCCULT(L)_FRAC LUNAR-OCCULT_FRACTION Percentage of the moon illuminated during the time of occultation MUTUAL_OCCULT(L)_LIMBSLOPE LUNAR-OCCULT_LIMB-SLOPE Lunar Occultation Limb Slope _MODEL MODEL Quantities generated by Models SPEC_CONT_FLUX MODEL_CONTINUUM Continuum level _CORR MODEL_CORRECTION Correction or adjustment OBJ_VEL_DRIFT MODEL_DRIFT-VELOC Terminal drift velocity OBJ_GEOM_TRIAX MODEL_DYN-TRIAX Dynamical triaxiality ? MODEL_ENERGY Energy modeled quantities SPEC_SED_MODEL MODEL_ENERGY_DIST Energy distribution PHYS_BULK_EOS MODEL_EOS Equation of state PHYS_BULK_EOS_ID MODEL_EOS_ID Name of used equation of state LOS_ISM_EXT MODEL_EXTINCTION Interstellar extinction quantities LOS_ISM_EXT_COEFF MODEL_EXTINCTION_COEFF Insterstellar extinction coefficient # Extinction coeffs and other theory are always 'model'. _MODEL_FEATURE MODEL_FEATURE Model Feature PHOT_FLUX_MODEL MODEL_FLUX Modeled Flux _MODEL_ID MODEL_ID Model Identification SPEC_LINE_FLUX_MODEL MODEL_LINE-FLUX Model Spectral Line Flux PHOT_MAG_MODEL MODEL_MAG Model-generated Magnitude _MODEL_DIFF MODEL_MAG_CORR Magnitude Correction or Difference _MODEL MODEL_MAG_VALUE Magnitude (in any band) generated by a model (or templates) ? MODEL_MOMENT-FLUX-RATIO Moment Flux Ratio _MODEL_PARAM MODEL_PARAM Model Parameter POP_SPEC_SYNTH MODEL_POP-SYNTHESIS Population Synthesis Quantity _MODEL_RESIDUAL MODEL_RESIDUAL Model Residual _MODEL_RESULT MODEL_RESULT Model Solution Value _MODEL_TYPE MODEL_TYPE Model Type PHYS_AT_TRANS_ZEEMAN MODEL_ZEEMAN Zeeman Effect Quantities PHYS_AT_TRANS_ZEEMAN_CO MODEL_ZEEMAN_COEFF Zeeman Effect Coefficient OBJ_CLASS_MORPH? MORPH Morphology of celestial objects OBJ_CLASS_GAL_ARMS MORPH_ARMS Spiral Arms Structure (galaxies) OBJ_CLASS_GAL_ARMS_RATIO MORPH_ARMS_RATIO Ratio of Spiral Arm (galaxies) OBJ_CLASS_GAL_ARMS_WOUND MORPH_ARMS_WOUND Wound Parameter of a spiral arm galaxy OBJ_CLASS_GAL_ASYM MORPH_ASYMMETRY Asymmetry Induced by Rotation OBJ_CLASS_GAL_BAR MORPH_BAR Presence or detection of a bar in a galaxy OBJ_CLASS_MORPH_CODE MORPH_CODE Code refering to a morphological property OBJ_CLASS_MORPH_PARAM MORPH_PARAM Morphological (geometrical) parameter OBJ_CLASS_MORPH_TYPE MORPH_TYPE Morphological Type _NOTE NOTE A Note related to a certain quantity or value _N NUMBER Number Of ``things'' (stars, observations, etc.) OBJ(*OBJ) - Specific object OBJ(E)_NUT NUTATION Earth's Nutation Related Quantities OBJ(E)_NUT_ANGLE NUTATION_PARAM Nutation Parameter # I'm guessing this is the angle _OBS ? OBS Observational Quantities SRC_REG_DIA OBS_ANG-SIZE Observational angular size OBS_INST_BAND OBS_BAND Band or Filter used for the observation PHOT_CAL OBS_CALIB Calibrations related to observations PHOT_CAL_ZERO OBS_CALIB_CONST Calibration's Constant PHOT_CAL_SCALE OBS_CALIB_FACTOR Calibration conversion factor # This is heterogeneous...I'm guessing flux cal is meant here, but # need ones for wave cal too etc OBS_ID OBS_CODE Observation code for observing run OBS_SITE_CONDS OBS_CONDITIONS Observation condition PHOT_LIMIT OBS_DETECT-LIMIT Detection Limit # This is a property of a region of an observation - you may have an upper limit # at a point or a single detection limit for a whole field, it's the same thing # (so note there is an association between limit and region) # It may have suffix of bandpass SRC_DET_SIG OBS_DETECT-SIGNIF Detection Significance # This is a property of a detected source _DIFF OBS_DIFF Observations' offset, difference, or deviation # Append to UCD of whatever is offset OBS_POS_UNC_DRIFT OBS_DRIFT Positional drift during the observation OBS_COV_BAND_FREQ OBS_FREQUENCY Frequency of the observation OBS_ID OBS_ID Observation identification # Comment: OBS_ mixes observation conditions and observed quantities. SPEC_LINE_WIDTH_G OBS_LW Observed gaussian line-width OBS_METHOD OBS_METHOD Observational Method/Technique UNK OBS_OTHER Other Measurements # Comment: useless? OBS_PARAM ? OBS_PARAM Additional Observational Parameters OBS_PLATE ? OBS_PLATE Quantities related to measurements on plates SRC_REG_DIA? OBS_PLATE_APERT Plate (Circular) Aperture SRC_REG_DIA OBS_PLATE_EXTENSION Linear diameter of an object measured on a Plate # Comment: what does this really mean? Is this really different to a normal measured diameter? _MODEL_RATIO OBS_PRED/OBS Fraction of predicted to observed quantities # Comment: is this really different to FIT MEAS/THEORY? Need to attach to whatever UCD is being measured. OBS_RUN OBS_RUN Observation run SRC_REG_DIA OBS_SIZE Observed size # Comment: I doubt that OBS_SIZE and EXTENSION_DIAM are really different. SRC_REG_DIA_DEC OBS_SIZE_DEC Observed size in declination OBS_DISP OBS_SLIT Spectroscopic slit properties # Applies to any dispersive system, not always a slit spectrograph? SRC_DISP_Y OBS_SLIT_OFFSET Slit offset respect to the nucleus of galaxy # Comment: this is really "position of source in slit coordinates". OBS_DISP_THETA OBS_SLIT_ORIENT Slit orientation # Comment: is this "PA of slit on sky" or "orientation of slit wrt source major axis"? # I suspect the former. OBS_SPECTRUM? OBS_SPECTRUM Spectral observations OBS_TYPE ? OBS_TYPE Type of observation OBS_SITE OBSTY Data on Observatories OBS_SITE_POS_ALT OBSTY_ALTITUDE Observatory Altitude OBS_SITE_CODE OBSTY_CODE Observatory Code OBS_SITE_NAME OBSTY_ID Observatory Identification/Name ORBIT ORBIT Orbital elements (planets, double stars, galaxies) ORBIT_ELT_NODE ORBIT_ASC-NODE Longitude of ascending node ORBIT_COMET? ORBIT_COMETS Cometary orbit parameter ORBIT_CONV_ANG? ORBIT_CONV-ANGLE Convergence angle ORBIT_PERI ORBIT_DISTANCE Distance, perihelion, or separation between components ORBIT_DIST ORBIT_DISTANCE Distance, perihelion, or separation between components # Here instantaneous distance ORBIT_ELT_E ORBIT_ECCENTRICITY Orbital eccentricity ORBIT_ELONG ORBIT_ELONGATION Elongation of radiant ORBIT_FREQ ORBIT_FREQUENCY Orbital frequency (orbital angular velocity) ORBIT_ELT_M ORBIT_MEAN-ANOMALY Mean anomaly - ORBIT_P-ASTRON Quantities related to the Periastron ORBIT_ELT_AOP ORBIT_P-ASTRON_ARG Periastron argument or longitude ORBIT_ELT_TPERI ORBIT_P-ASTRON_DATE Date of occurance of periastron ORBIT_PERIDOT ORBIT_P-ASTRON_RATE Rate of periastron advance ORBIT_ELT_AOP ORBIT_P-HELION Perihelion argument or longitude - ORBIT_PARAM Orbital parameter ORBIT_PERIOD ORBIT_PERIOD Orbital period ORBIT_PDOT ORBIT_PERIOD_DERIVATIVE Time derivative of orbital period ORBIT_PHASEANG ORBIT_PHASE-ANGLE Orbital phase angle ORBIT_RV ORBIT_RV Orbital radial velocity properties ORBIT_RV_AMP ORBIT_RV_S-AMPLITUDE Semi amplitude of radial velocity curve ORBIT_DIA_PROJ ORBIT_SEPARATION Orbital Separation (angular distance) ORBIT_DIA ORBIT_SIZE Orbital size ORBIT_RADIUS ORBIT_SIZE_RADIUS Orbital radius (binary stars) ORBIT_ELT_A ORBIT_SIZE_SMAJ Semi-major axis of the orbit PHOT_ PHOT Photometry, extending to several wavelength regimes (X to Radio) PHOT_MAG_13C_ PHOT_13C 13 color system (Stellar Applications) GCPD#66 PHOT_COL(13C,33-52) PHOT_13C_33-52 Color index 33-52 (13C) PHOT_COL(13C,35-52) PHOT_13C_35-52 Color index 35-52 (13C) PHOT_COL(13C,37-52) PHOT_13C_37-52 Color index 37-52 (13C) PHOT_COL(13C,40-52) PHOT_13C_40-52 Color index 40-52 (13C) PHOT_COL(13C,45-52) PHOT_13C_45-52 Color index 45-52 (13C) PHOT_MAG(13C,52) PHOT_13C_52 Magnitude 52 (13C) PHOT_COL(13C,52-110) PHOT_13C_52-110 Color index 52-110 (13C) PHOT_COL(13C,52-58) PHOT_13C_52-58 Color index 52-58 (13C) PHOT_COL(13C,52-63) PHOT_13C_52-63 Color index 52-63 (13C) PHOT_COL(13C,52-72) PHOT_13C_52-72 Color index 52-72 (13C) PHOT_COL(13C,52-80) PHOT_13C_52-80 Color index 52-80 (13C) PHOT_COL(13C,52-86) PHOT_13C_52-86 Color index 52-86 (13C) PHOT_COL(13C,52-99) PHOT_13C_52-99 Color index 52-99 (13C) _ABS PHOT_ABS-MAG Absolute magnitude _ABS PHOT_ABS-MAG_BAND Absolute magnitude in a band, regardles of band PHOT_MAG_BOL_ABS PHOT_ABS-MAG_BOL Bolometric absolute magnitude OBS_ATM_ PHOT_ATM Earth Atmosphere Parameters Linked to Photometry OBS_ATM_AIRMASS PHOT_ATM_AIRMASS Air mass OBS_ATM_EXT PHOT_ATM_EXT Atmospheric extinction coefficient PHOT_BOL_ PHOT_BOL Bolometric Quantities PHOT_COL_BOL() PHOT_BOL_CORR Bolometric correction PHOT_FLUX_BOL PHOT_BOL_FLUX Bolometric Flux PHOT_LUM_BOL PHOT_BOL_LUMINOSITY Bolometric luminosity PHOT_MAG_BOL PHOT_BOL_MAG Bolometric magnitude SRC_IMAGE_SLOPE PHOT_BRIGHTNESS-SLOPE Spatial brightness distribution slope # This is part of a spatial flux model for a source # PHOT_COL PHOT_CI Color index in unspecified system PHOT_COL(,102-C220) PHOT_CI_102-C220 Color index 102-C220 PHOT_COL(UNK,B-R) PHOT_CI_B-R Color index B-r PHOT_COL(HALPHA,LINE-CONT) PHOT_CI_ALPHA Color index based on H-alpha line PHOT_COL(HBETA,LINE-CONT) PHOT_CI_BETA Color index beta or h-beta (not Stroemgren index) PHOT_COL(BALMER,LINE-CONT) PHOT_CI_BALMER Color index using the Balmer lines Hgamma or higher PHOT_COL(UNK,B-I) PHOT_CI_B-I Color index B-I from heterogeneous photometric systems PHOT_COL(UNK,B-K) PHOT_CI_B-K Color index B-K from heterogeneous photometric systems PHOT_COL(UNK,B-V) PHOT_CI_B-V Color index B-V in a non-conventional system PHOT_COL(,CN-TiO) PHOT_CI_CN-TIO Color index CN-TiO PHOT_COL_CODE PHOT_CI_CODE Codes associated with color index PHOT_COL_FRACT PHOT_CI_FRACT Fractional color index PHOT_COL(g,b-v) PHOT_CI_GB-GV Color index gb-gv PHOT_COL(g,u-b) PHOT_CI_GU-GB Color index gu-gb PHOT_COL(IRAS,) PHOT_CI_IR Various far IR color indices (e.g. with IRAS bands) PHOT_COL(,IR-OPT) PHOT_CI_IR-OPT Color index Infrared minus optical PHOT_COL(,M-51) PHOT_CI_M-51 Color index M-51 PHOT_COL(,R-HALPHA) PHOT_CI_R-HALPHA Color index R minus Halpha PHOT_COL(,R-I) PHOT_CI_R-I Color index R-I PHOT_COL(,U-B) PHOT_CI_U-B Color index u-B U-B PHOT_COL(,U-R) PHOT_CI_U-R Color index u-r PHOT_COL(UNK,UNK) PHOT_CI_UNDEF Color index in unspecified system PHOT_COL(,UV-OPT) PHOT_CI_UV-OPT Color index uv minus Optical (UV-OPT) PHOT_COL(,V-I) PHOT_CI_V-I Color index V-I (no standard system specified) PHOT_COL(,V-R) PHOT_CI_V-R Color index V-R (no standard system specified) ? PHOT_CLASS Classification of photometry PHOT_COL_ PHOT_COLOR Quantities related to color indices PHOT_COL_EXCESS PHOT_COLOR_EXCESS Color excess (not just E(B-V)) PHOT_RATE PHOT_COUNT-RATE Count rates in several wavelength regimes PHOT_RATE(UV) PHOT_COUNT-RATE_UV Count rate in ultraviolet PHOT_RATE(XR) PHOT_COUNT-RATE_X Count rate in x-ray PHOT_COUNTS PHOT_COUNTS Count measured in the detector PHOT_COUNTS(IUE/SWP) PHOT_COUNTS_IUE Count from IUE PHOT_COUNTS(IUE/LWP) PHOT_COUNTS_IUE Count from IUE PHOT_COUNTS PHOT_COUNTS_MISC Count measurement in the detector PHOT_COUNTS(RADIO) PHOT_COUNTS_RADIO Counts in radio regime PHOT_COUNTS(GAMMA) PHOT_COUNTS_GAMMA Count in gamma-ray regime PHOT_RATE(GAMMA) PHOT_COUNT-RATE_GAMMA Count rate of gamma photons PHOT_COUNT_RATIO PHOT_COUNTS_RATIO Ratio of photon counts, or relative counts. PHOT_COUNTS(XR) PHOT_COUNTS_X Counts in X-ray PHOT_MAG(COUS) PHOT_COUS Cousins photometric system GCPD#54 PHOT_MAG(COUS,I) PHOT_COUS_I Cousins magnitude Ic PHOT_MAG(COUS,R) PHOT_COUS_R Cousins magnitude R COUS PHOT_COL(COUS,R-I) PHOT_COUS_R-I Cousins R-I color index COUS PHOT_COL(COUS,V-I) PHOT_COUS_V-I (Kron-)Cousins V-I color index COUS PHOT_COL(COUS,V-R) PHOT_COUS_V-R (Kron-)Cousins V-R color index PHOT_MAG(DDO,) PHOT_DDO DDO Photometric System GCPD#12 PHOT_COL(DDO,35-38) PHOT_DDO_35-38 Color index 35-38 DDO PHOT_COL(DDO,38-41) PHOT_DDO_38-41 Color index 38-41 DDO PHOT_COL(DDO,41-42) PHOT_DDO_41-42 Color index 41-42 DDO PHOT_COL(DDO,42-45) PHOT_DDO_42-45 Color index 42-45 DDO PHOT_COL(DDO,42-48) PHOT_DDO_42-48 Color index 42-48 DDO PHOT_COL(DDO,45-48) PHOT_DDO_45-48 Color index 45-48 DDO PHOT_COL(DDO,48-51) PHOT_DDO_48-51 Color index 48-51 DDO PHOT_MAG(DDO,48) PHOT_DDO_M48 Magnitude m48 DDO - PHOT_DIFF Differences or differential quantities PHOT_COL()_DIFF PHOT_DIFF_CI Difference in color index PHOT_MAG()_DIFF PHOT_DIFF_MAG Difference in or differential magnitude PHOT_SB()_DIFF PHOT_DIFF_SB Difference in surface brightness SRC_DIST_MAG PHOT_DIST-MOD Distance Modulus # Distance modulus is not a brightness, it's a distance expressed in mag PHOT_EXT PHOT_EXTINCTION Extinction total to differential PHOT_EXT_GAL PHOT_EXTINCTION_GAL Galactic extinction PHOT_EXT_INT PHOT_EXTINCTION_INT Internal extinction PHOT_EXT_ISM PHOT_EXTINCTION_ISM Interstellar Absorption PHOT_EXT_R PHOT_EXTINCTION_R Insterstellar extinction (ratio total to differential) PHOT_EXT_TOT PHOT_EXTINCTION_TOTAL Total Extinction PHOT_FLUENCE PHOT_FLUENCE Fluence PHOT_FLUX PHOT_FLUX Flux PHOT_FLUXD PHOT_FLUX_DENSITY Flux density PHOT_FLUX(GAMMA) PHOT_FLUX_GAMMA Flux in gamma rays PHOT_FLUX(HALPHA) PHOT_FLUX_HALPHA H-Alpha Flux PHOT_FLUX(HBETA) PHOT_FLUX_HBETA H Beta line flux PHOT_FLUX(IRAS) PHOT_FLUX_IR IR flux (IRAS or others) PHOT_FLUX(6 mu) PHOT_FLUX_IR_6 Flux density around 6 microns (e.g. ISO at 6.7 microns) close to M filter PHOT_FLUX(9 mu) PHOT_FLUX_IR_9 Flux density around 9 microns (range 8-10) PHOT_FLUX(IRAS12) PHOT_FLUX_IR_12 Flux density (IRAS) at 12 microns, or around 12 microns (ISO at 14.3) PHOT_FLUX(IRAS25) PHOT_FLUX_IR_25 Flux density (IRAS) at 25 microns PHOT_FLUX(3.5 mu) PHOT_FLUX_IR_3.5 Flux density at 3.5 microns PHOT_FLUX(15 mu) PHOT_FLUX_IR_15 Flux density around 15 microns (e.g. 14.3um ISO) PHOT_FLUX(IRAS60) PHOT_FLUX_IR_60 Flux density (IRAS) at 60 microns PHOT_FLUX(IRAS100) PHOT_FLUX_IR_100 Flux density (IRAS) at 100 microns PHOT_FLUX(170 mu) PHOT_FLUX_IR_170 Far infra-red Flux density around 170um (1750GHz) PHOT_FLUX(300 mu) PHOT_FLUX_IR_300 Far infra-red Flux density around 300um (3000GHz) PHOT_FLUX(FIR) PHOT_FLUX_IR_FAR Far Infrared flux PHOT_FLUX(H) PHOT_FLUX_IR_H Flux Density in Johnson's H Band PHOT_FLUX(L) PHOT_FLUX_IR_L Flux Density in Johnson's L Band PHOT_FLUX(UNK) PHOT_FLUX_IR_MISC Miscellaneous IR fluxes PHOT_FLUX_RATIO PHOT_FLUX_NORM Normalized Flux, always dimensionless PHOT_FLUX(OPTICAL) PHOT_FLUX_OPTICAL Flux in the Optical (unspecified system and/or units) PHOT_FLUX(RADIO) PHOT_FLUX_RADIO Flux density at radio frequencies PHOT_FLUX(22 MHz) PHOT_FLUX_RADIO_22M Radio flux density around 22MHz (13.6m) PHOT_FLUX(31 MHz) PHOT_FLUX_RADIO_31M Radio flux density around 31MHz (9.7m) PHOT_FLUX(43 MHz) PHOT_FLUX_RADIO_43M Radio flux density around 43MHz (7.0m) PHOT_FLUX(61 MHz) PHOT_FLUX_RADIO_61M Radio flux density around 61MHz (4.9m) PHOT_FLUX(87 MHz) PHOT_FLUX_RADIO_87M Radio flux density around 87MHz (3.5m) PHOT_FLUX(110 MHz) PHOT_FLUX_RADIO_110M Radio flux density around 110MHz (2.7m) PHOT_FLUX(150 MHz) PHOT_FLUX_RADIO_150M Radio flux density around 150MHz (2.0m) PHOT_FLUX(175 MHz) PHOT_FLUX_RADIO_175M Radio flux density around 175MHz (1.7m) PHOT_FLUX(250 MHz) PHOT_FLUX_RADIO_250M Radio flux density around 250MHz (1.2m) PHOT_FLUX(325 MHz) PHOT_FLUX_RADIO_325M Radio flux density around 325MHz (92cm) PHOT_FLUX(365 MHz) PHOT_FLUX_RADIO_365M Radio flux density around 365MHz (82cm) PHOT_FLUX(400 MHz) PHOT_FLUX_RADIO_400M Radio flux density around 400MHz (75cm) PHOT_FLUX(500 MHz) PHOT_FLUX_RADIO_500M Radio flux density around 500MHz (60cm) PHOT_FLUX(600 MHz) PHOT_FLUX_RADIO_600M Radio flux density around 600MHz (50cm) PHOT_FLUX(700 MHz) PHOT_FLUX_RADIO_700M Radio flux density around 700MHz (43cm) PHOT_FLUX(850 MHz) PHOT_FLUX_RADIO_850M Radio flux density around 850MHz (35cm) PHOT_FLUX(1 GHz) PHOT_FLUX_RADIO_1G Radio flux density around 1GHz (30cm) PHOT_FLUX(1.4 GHz) PHOT_FLUX_RADIO_1.4G Radio flux density around 1.4GHz (21cm) PHOT_FLUX(1.6 GHz) PHOT_FLUX_RADIO_1.6G Radio flux density around (OH maser) PHOT_FLUX(2.0 GHz) PHOT_FLUX_RADIO_2G Radio flux density around 2GHz (15cm) PHOT_FLUX(2.7 GHz) PHOT_FLUX_RADIO_2.7G Radio flux density around 2.7GHz (11cm) PHOT_FLUX(3.9 GHz) PHOT_FLUX_RADIO_3.9G Radio flux density around 3.9GHz (7.7cm) PHOT_FLUX(5.0 GHz) PHOT_FLUX_RADIO_5G Radio flux density around 5GHz (6cm) PHOT_FLUX(7.5 GHz) PHOT_FLUX_RADIO_7.5G Radio flux density around 7.5GHz (4cm) PHOT_FLUX(8.4 GHz) PHOT_FLUX_RADIO_8.4G Radio flux density around 8.4GHz (3.6cm) PHOT_FLUX(10.7 GHz) PHOT_FLUX_RADIO_10.7G Radio flux density around 10.7GHz (2.8cm) PHOT_FLUX(15.0 GHz) PHOT_FLUX_RADIO_15G Radio flux density around 15GHz (2cm) PHOT_FLUX(22.0 GHz) PHOT_FLUX_RADIO_22G Radio flux density around (H2O maser) PHOT_FLUX(36.0 GHz) PHOT_FLUX_RADIO_36G Radio flux density around 36GHz (8.3mm) PHOT_FLUX(43.0 GHz) PHOT_FLUX_RADIO_43G Radio flux density around 43GHz (7.0mm) PHOT_FLUX(63.0 GHz) PHOT_FLUX_RADIO_63G Radio flux density around 63GHz (4.8mm) PHOT_FLUX(90.0 GHz) PHOT_FLUX_RADIO_90G Radio flux density around 90GHz (3.3mm) PHOT_FLUX(125.0 GHz) PHOT_FLUX_RADIO_125G Radio flux density around 125GHz (2.4mm) PHOT_FLUX(180.0 GHz) PHOT_FLUX_RADIO_180G Radio flux density around 180GHz (1.7mm) PHOT_FLUX(250.0 GHz) PHOT_FLUX_RADIO_250G Radio flux density around 250GHz (1.2mm) PHOT_FLUX(350.0 GHz) PHOT_FLUX_RADIO_350G Radio flux density around 350GHz (860um) PHOT_FLUX(500.0 GHz) PHOT_FLUX_RADIO_500G Radio flux density around 500GHz (600um) PHOT_FLUX(700.0 GHz) PHOT_FLUX_RADIO_700G Radio flux density around 700GHz (430um) PHOT_FLUX(RADIO) PHOT_FLUX_RADIO_MISC Miscellaneous Radio flux density PHOT_FLUX(SiO-Maser) PHOT_FLUX_RADIO_SIO-MASER SiO maser peak radio flux PHOT_FLUX_RATIO PHOT_FLUX_RATIO Flux ratio PHOT_FLUX_RATIO PHOT_FLUX_REL Relative (normalized) flux PHOT_FLUX(UV) PHOT_FLUX_UV Ultraviolet flux (uv far-uv euv) PHOT_FLUX(X) PHOT_FLUX_X X-ray flux PHOT_MAG(GEN,) PHOT_GEN Geneva's photometric system GCPD#13 PHOT_COL(GEN,B-V) PHOT_GEN_B-V Geneva color index B-V (GEN) PHOT_COL(GEN,B1-B) PHOT_GEN_B1-B Geneva color index B1-B (GEN) PHOT_COL(GEN,B2-B) PHOT_GEN_B2-B Geneva color index B2-B (GEN) PHOT_COL(GEN,G-B) PHOT_GEN_G-B Geneva color index G-B (GEN) PHOT_COL(GEN,) PHOT_GEN_MISC various geneva photometric color indices (and linear combinations) PHOT_COL(GEN,U-B) PHOT_GEN_U-B Geneva color index U-B (GEN) PHOT_MAG(GEN,V) PHOT_GEN_V Geneva magnitude filter V (GEN) PHOT_COL(GEN,V-B) PHOT_GEN_V-B Geneva color index V-B (GEN) PHOT_COL(GEN,V1-B) PHOT_GEN_V1-B Geneva color index V1-B (GEN) PHOT_MAG(GUNN,) PHOT_GUNN Gunn Photometric System GCPD#38 PHOT_MAG(GUNN,G) PHOT_GUNN_G Magnitude g (GUNN) PHOT_COL(GUNN,G-I) PHOT_GUNN_G-I Color index g-i (GUNN) PHOT_COL(GUNN,G-R) PHOT_GUNN_G-R Color index g-r (GUNN) PHOT_MAG(GUNN,I) PHOT_GUNN_I Magnitude i (GUNN), also used in DENIS (0.82{mu}m) PHOT_COL(GUNN,I-Z) PHOT_GUNN_I-Z Color index I-z (GUNN) PHOT_MAG(GUNN,R) PHOT_GUNN_R Magnitude R (GUNN) PHOT_COL(GUNN,R-I) PHOT_GUNN_R-I Color index R-I (GUNN) PHOT_MAG(GUNN,V) PHOT_GUNN_V Magnitude v (GUNN) PHOT_COL(GUNN,V-R) PHOT_GUNN_V-R Color index V-R (GUNN) PHOT_MAG(GUNN,Z) PHOT_GUNN_Z Magnitude z (GUNN) PHOT_MAG(HEI,) PHOT_HEI Heidelberg s Photometric System (HEI) PHOT_COL(HEI,U-B) PHOT_HEI_U-B Heidelberg photometry U-B (HEI) PHOT_MAG(HIP,) PHOT_HIPPAR Hipparcos' photometry system PHOT_MAG(HST,) PHOT_HST HST Photometric System (by filter name) (HST) PHOT_MAG(HST,F1042M) PHOT_HST_F1042M Magnitude F1042M (HST) PHOT_MAG(HST,F140W) PHOT_HST_F140W Magnitude M104W (HST) PHOT_COL(HST,IR-IR) PHOT_HST_CI_IR HST Color Index from IR filters, e.g. F140W-F210W PHOT_COL(HST,U-B) PHOT_HST_CI_U-B HST Color Index close to U-B, e.g. F336W-F430W PHOT_MAG(HST,F170W) PHOT_HST_F170W Magnitude F170W (HST) PHOT_MAG(HST,F175W) PHOT_HST_F175W Magnitude F175W (HST) PHOT_MAG(HST,F220W) PHOT_HST_F220W Magnitude F220W (HST) PHOT_MAG(HST,F255W) PHOT_HST_F255W Magnitude F255W (HST) PHOT_MAG(HST,F275W) PHOT_HST_F275W Magnitude F275W (HST) PHOT_MAG(HST,F300W) PHOT_HST_F300W Ultraviolet Magnitude F300W (HST) PHOT_COL(HST,U-V) PHOT_HST_CI_U-V HST Color Index close to U-V, e.g. F336W-F555W PHOT_MAG(HST,F342W) PHOT_HST_F342W Ultraviolet Magnitude in filters F330W or F342W (HST) PHOT_MAG(HST,F430W) PHOT_HST_F430W Ultraviolet magnitude F430W or F439W (HST) PHOT_COL(HST,B-V) PHOT_HST_CI_B-V HST Color Index close to B-V, e.g. F430W-F555W PHOT_MAG(HST,F450W) PHOT_HST_F450W Ultraviolet Magnitude F450W (HST) PHOT_MAG(HST,F480LP) PHOT_HST_F480LP Magnitude F480LP (HST) PHOT_MAG(HST,F547M) PHOT_HST_F547M Magnitude F547M (HST) PHOT_MAG(HST,F555W) PHOT_HST_F555W Magnitude F555W (HST) PHOT_COL(HST,B-R) PHOT_HST_CI_B-R HST Color Index close to B-R, e.g. F430W-F675W PHOT_COL(HST,V-R) PHOT_HST_CI_V-R HST Color Index close to V-R, e.g. F555W-F675W PHOT_COL(HST,R-I) PHOT_HST_CI_R-I HST Color Index close to R-I, e.g. F675W-F814W PHOT_MAG(HST,F569W) PHOT_HST_F569W Magnitude F569W (HST) PHOT_MAG(HST,F606W) PHOT_HST_F606W Magnitude F606W (HST) PHOT_COL(HST,V-I) PHOT_HST_CI_V-I HST Color Index close to V-I, e.g. F555W-F814W PHOT_MAG(HST,F622W) PHOT_HST_F622W Magnitude F622W (HST) PHOT_MAG(HST,F675W) PHOT_HST_F675W Magnitude F675W (HST) PHOT_MAG(HST,F702W) PHOT_HST_F702W Magnitude F702W (HST) PHOT_MAG(HST,F725LP) PHOT_HST_F725LP Magnitude F725LP (HST) PHOT_MAG(HST,F785LP) PHOT_HST_F785LP Magnitude F785LP (HST) PHOT_MAG(HST,F791W) PHOT_HST_F791W Magnitude F791W (HST) PHOT_MAG(HST,F814W) PHOT_HST_F814W Magnitude F814W (HST) PHOT_MAG(HST,F850LP) PHOT_HST_F850LP Magnitude F850LP (HST) PHOT_MAG(HST,V) PHOT_HST_V Magnitude V (visual) HST (unspecified filter name) PHOT_COL() PHOT_INDX Photometric index (usually in narrow bands) PHOT_COL(,HI) PHOT_INDX_HI Neutral hydrogen HI photometry index PHOT_MAG()_INT PHOT_INT-MAG Integrated or isophotal magnitudes PHOT_MAG(,B)_INT PHOT_INT-MAG_B Integrated total or isophotal blue magnitude PHOT_MAG(,I)_INT PHOT_INT-MAG_I Integrated, total or isophotal, I magnitude PHOT_MAG(UNK,)_INT PHOT_INT-MAG_MISC Miscellaneous Integrated or isophotal magnitudes PHOT_MAG(,R)_INT PHOT_INT-MAG_R Integrated, total or isophotal, R magnitude PHOT_MAG(,I)_INT PHOT_INT-MAG_U Integrated, total or isophotal, V magnitude PHOT_MAG(,V)_INT PHOT_INT-MAG_V Integrated, total or isophotal, V magnitude PHOT_INTENSITY_ PHOT_INTENSITY Intensity PHOT_INTENSITY_ADU PHOT_INTENSITY_ADU Intensity expressed in ADU (analog to digital units) PHOT_INTENSITY_ADU PHOT_INTENSITY_ESTIMATED Estimated intensity # What in astronomy is *not* estimated? PHOT_INTENSITY_ADU? PHOT_INTENSITY_MISC Miscellaneous Intensity PHOT_INTENSITY_RATIO PHOT_INTENSITY_NORMALIZED Normalized intensity SRC_IMAGE_RADIAL_PROFILE_INTENSITY PHOT_INTENSITY_PROFILE Intensity profile PHOT_INTENSITY_RATIO PHOT_INTENSITY_RATIO Intensity ratio PHOT_MAG(,IR) PHOT_IR Infrared magnitudes (not well inserted in photometric systems) PHOT_COL(IRAS,IRAS12-IRAS25) PHOT_IR_12-25 Infrared color index 12-25 (IRAS) PHOT_COL(CO 2.29mu,LINE-CONT) PHOT_IR_2.29 CO band index magnitude at 2.29 micron PHOT_COL(IRAS Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h2RAi1Md026534 for ; Thu, 27 Mar 2003 11:44:01 +0100 (MET) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h2RAi1A21118 for ; Thu, 27 Mar 2003 11:44:01 +0100 (MET) Received: from sainfoin.saclay.cea.fr(132.166.192.126) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAASmaOpP; Thu, 27 Mar 03 11:44:00 +0100 Received: from rosetta.saclay.cea.fr (rosetta.saclay.cea.fr [132.166.13.210]) by sainfoin.saclay.cea.fr (8.12.8/CEAnet-Internet.1.0) with ESMTP id h2RAaUP4007258; Thu, 27 Mar 2003 11:36:30 +0100 (MET) Received: (from dide@localhost) by rosetta.saclay.cea.fr (8.11.6+Sun/8.10.2) id h2RAaUd29807; Thu, 27 Mar 2003 11:36:30 +0100 (MET) Date: Thu, 27 Mar 2003 11:36:30 +0100 (MET) From: DIDELON Pierre Message-Id: <200303271036.h2RAaUd29807@rosetta.saclay.cea.fr> To: amsr@jb.man.ac.uk, rplante@ncsa.uiuc.edu Subject: Re: UCDs status and perspectives Cc: ucd@ivoa.net Content-Type: X-sun-attachment X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: ---------- X-Sun-Data-Type: text X-Sun-Data-Description: text X-Sun-Data-Name: text X-Sun-Charset: us-ascii X-Sun-Content-Lines: 25 Hi Anita, Ray et al, I globally and fully agree with all your points and comments, the most important one is to use the only available quite exhaustive metadata (UCD) as a crucial use case to elaborate a more flexible and sophisticated schema. I am impressed by Ray's willingness to define a metadata model to refactored the domain, and I am waiting it with great eagerness. I was thinking about such a process and the most difficult part for me is the mechanism to keep a link to UCD and continuing to support them. I tried to formalize the possible inter-relations in the attached UML diag, (triangle at the beginning of a line is inheritance, others lines are relations; assoc,agreg....). Several question araise already in my mind even at this very simple level : - Does Descriptor and Group... need to inheritate from Atom and Descriptor, or is the association use/is_part_of sufficient? In other words, do we need several level of composition? Group of group of Descriptors?... - is the relation UCD/PAD formally needed? - Which is the link between the actual UCD_Tree and all the possible and usefull descriptors associations? cheers, pierre ---------- X-Sun-Data-Type: gif-file X-Sun-Data-Description: gif-file X-Sun-Data-Name: AtomUCD-UML.gif X-Sun-Encoding-Info: uuencode X-Sun-Content-Lines: 162 begin 600 AtomUCD-UML.gif M1TE&.#=A\@)S O< /\ /___^CX !4 , . \ #_ "^ #8 ) M J /]Z "0 +X -D ( " ( .," "!, +X6 -J* 1H 2 ! $ M ) "L $" )!,% 9 %L %Z Q &@ -D" %Q, 8 #V GX !6( M I #F "7D 'X /8# ;_ $"^ #9 UL !< $ \ $D $@\%. M 8 \"% & ?(!$ +0 ! !% +< / " , 3X0 =@ 90, <@ & M=P! <@ ":0 Z= ( C> :0

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8475 l cp gs col0 s gr % Polyline n 4800 6525 m 7725 6525 l 7725 7725 l gs col0 s gr % Polyline n 5400 8100 m 6975 8100 l gs col0 s gr % Polyline n 9750 8175 m 11325 8175 l 11325 8700 l 9750 8700 l cp gs col0 s gr % Polyline n 8250 8025 m 9750 8400 l gs col0 s gr % Polyline n 2625 4650 m 1650 4650 l 1650 825 l 4125 825 l gs col0 s gr % Polyline n 1350 8100 m 600 8100 l 600 4950 l 2625 4950 l gs col0 s gr % Polyline gs clippath 3488 5660 m 3600 5300 l 3713 5660 l 3713 5205 l 3488 5205 l cp clip n 3600 5250 m 3600 6525 l 2475 6525 l 2475 7800 l gs col0 s gr gr % arrowhead n 3488 5660 m 3600 5300 l 3713 5660 l 3600 5660 l 3488 5660 l cp gs col7 1.00 shd ef gr col0 s /Times-Roman ff 270.00 scf sf 4350 975 m gs 1 -1 sc (Atom) col0 sh gr $F2psEnd rs showpage From - Mon Mar 31 02:40:49 2003 X-UIDL: 3e5baf6500000372 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h2V0abQk023240 for ; Mon, 31 Mar 2003 02:36:38 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h2V0abR26259 for ; Mon, 31 Mar 2003 02:36:37 +0200 (MEST) Received: from head-cfa.cfa.harvard.edu(131.142.41.8) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAlQaqsZ; Mon, 31 Mar 03 02:36:36 +0200 Received: from urania.cfa.harvard.edu (urania [131.142.52.147]) by head-cfa.cfa.harvard.edu (8.12.8/8.12.8) with ESMTP id h2V0T589007342 for ; Sun, 30 Mar 2003 19:29:05 -0500 (EST) Received: (from jcm@localhost) by urania.cfa.harvard.edu (8.11.1/8.11.1) id h2V0T5M29580 for ucd@ivoa.net; Sun, 30 Mar 2003 19:29:05 -0500 (EST) Date: Sun, 30 Mar 2003 19:29:05 -0500 (EST) Message-Id: <200303310029.h2V0T5M29580@urania.cfa.harvard.edu> From: jcm@head-cfa.cfa.harvard.edu To: ucd@ivoa.net Subject: Re: UCD Status and Perspectives X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Patricio, I realize I never followed up your message of Mar 19. For the record, what I had in mind with my spectral index example, I had in mind finding the sources in a subsample and calculating what their 4100A fluxes are, for instance to get a sample for an observing proposal of the 10 brighest northern objects of a particular class, brightest by 4100A flux. And I want to do it even including objects whose 4100A flux is not actually known, but can be guessed from other published fluxes assuming an SED. In general, the existing UCDs are great for getting general information but not for knowing exactly what you have, that was the broader point. A side point from this example is that I think the VO will need to allow users to specify certain assumptions to provide a context for queries (I'm looking for quasars, and here's what you can assume about quasars - e.g. a typical SED - so that you can handle my query even in cases where the information is incomplete... a bit like a Bayesian prior in spirit, I guess). Regards, Jonathan From - Tue Apr 1 14:35:19 2003 X-UIDL: 3e5baf65000003a7 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h31CYll7008286 for ; Tue, 1 Apr 2003 14:34:47 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h31CYlg09912 for ; Tue, 1 Apr 2003 14:34:47 +0200 (MEST) Received: from maroon.csi.cam.ac.uk(131.111.8.2) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAA4Ka4wt; Tue, 1 Apr 03 14:34:46 +0200 Received: from cass41.ast.cam.ac.uk ([131.111.69.186]) by maroon.csi.cam.ac.uk with esmtp (Exim 4.12) id 190KyU-0000s4-00 for ucd@ivoa.net; Tue, 01 Apr 2003 13:34:46 +0100 Received: from cappc33.ast.cam.ac.uk (cappc33 [131.111.69.212]) by cass41.ast.cam.ac.uk (8.12.8+Sun/8.12.8) with ESMTP id h31CYj8Z014588 for ; Tue, 1 Apr 2003 13:34:45 +0100 (BST) Date: Tue, 1 Apr 2003 13:12:55 +0100 (BST) From: Nicholas A Walton To: ucd@ivoa.net Subject: Cambridge, UK, May 12-16, 2003, InterOperability meetings Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII Status: Dear All, ** registration now open at ** http://www.ivoa.net/twiki/bin/view/IVOA/InterOpMay2003 please check http://www.ivoa.net/twiki/bin/view/IVOA/InterOpMay2003 and related links for emerging details as to the upcoming InterOp meetings in Cambridge. I provide details and links to hotels on the above page. I would advise that you consider booking your accommodation as soon as possible. Yours, Nic Walton ======================================================================== Dr N. A. Walton (AstroGrid Project Scientist) Tel: +44 1223 337503 Institute of Astronomy FAX: +44 1223 337523 University of Cambridge WWW: http://www.astrogrid.org Madingley Road WWW: http://www.ast.cam.ac.uk/~naw Cambridge, CB3 0HA email: naw@ast.cam.ac.uk ======================================================================== From - Fri Apr 4 19:41:58 2003 X-UIDL: 3e5baf6500000475 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h34HcnGa006390 for ; Fri, 4 Apr 2003 19:38:49 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h34HcnF22965 for ; Fri, 4 Apr 2003 19:38:49 +0200 (MEST) Received: from mailhost.cacr.caltech.edu(131.215.145.180) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAA1say2S; Fri, 4 Apr 03 19:38:48 +0200 Received: from lugh.cacr.caltech.edu (lugh.cacr.caltech.edu [131.215.145.183]) by mailhost.cacr.caltech.edu (8.9.3/8.9.1) with ESMTP id JAA04636; Fri, 4 Apr 2003 09:35:21 -0800 (PST) Received: from roxy (lugh.cacr.caltech.edu [131.215.145.183]) by lugh.cacr.caltech.edu (8.8.8+Sun/8.8.5) with SMTP id JAA24861; Fri, 4 Apr 2003 09:35:21 -0800 (PST) Message-ID: <01b101c2fad0$9168a0d0$d2add783@roxy> From: "Roy Williams" To: Cc: "Francoise Genova" , "Roy Williams" Subject: Pre-meeting UCD question Date: Fri, 4 Apr 2003 09:35:21 -0800 MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1106 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Dear UCD'ers In a few weeks Francoise Genova and I will be organizing a working group in Cambridge, UK to discuss the future of the UCD concept as a "common vocabulary" for the VO effort. The working group will meet May 12-14. (1) If you would like to make a short presentation to the working group in Cambridge, please send a note to Francoise and myself with a title. (2) Perhaps we can start a discussion by asking for requirements in trhe following question: ***** WHAT ARE UCD USED FOR -- now and future ***** Please try to write your opinions on this question and send to this group. Some references below. Please DO NOT suggest implementation, syntax, or other solutions -- let us try for requirements. It seems to me that once we know what we are trying to do, our time in Cambridge can be used more productively to find solutions. I hope you agree that this requirements list would be a good start. Thank You Roy Williams Ref 1: Archives of this mailing list http://www.ivoa.net/forum/ucd/ Ref 2: UCD Status and Perspectives, S. Derriere http://www.ivoa.net/internal/IVOA/IvoaUCD/UCD-status0203.pdf --- Caltech Center for Advanced Computing Research roy@cacr.caltech.edu 626 395 3670 From - Mon Apr 7 06:28:33 2003 X-UIDL: 3e5baf6500000492 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h374NhAu009381 for ; Mon, 7 Apr 2003 06:23:44 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h374NgS05022 for ; Mon, 7 Apr 2003 06:23:42 +0200 (MEST) Received: from dns.ph.unimelb.edu.au(128.250.50.25) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAABxaOZj; Mon, 7 Apr 03 06:23:41 +0200 Received: (qmail 8341 invoked from network); 7 Apr 2003 04:17:44 -0000 Received: from isis.ph.unimelb.edu.au (128.250.51.69) by indy.ph.unimelb.edu.au with SMTP; 7 Apr 2003 04:17:44 -0000 Received: (from dbarnes@localhost) by isis.ph.unimelb.edu.au (8.11.6+Sun/8.9.1) id h374MWv29499; Mon, 7 Apr 2003 14:22:32 +1000 (EST) From: David Barnes Message-Id: <200304070422.h374MWv29499@isis.ph.unimelb.edu.au> Subject: re: Pre-meeting UCD question To: ucd@ivoa.net Date: Mon, 7 Apr 2003 14:22:32 +1000 (EST) Cc: dbarnes@isis.ph.unimelb.edu.au (David Barnes) Reply-To: barnesd@unimelb.edu.au X-Mailer: ELM [version 2.5 PL3] MIME-Version: 1.0 Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Hi all, Roy asked: > (2) Perhaps we can start a discussion by asking for requirements in trhe > following question: > ***** WHAT ARE UCD USED FOR -- now and future ***** First up, I'm new, so please forgive (and correct) any misconceptions on my part :-) Anyway, here is my 2 cents worth. I'm not sure if I'll be able to make the meeting, but we're hoping to have someone from Aus-VO there... > Ref 2: UCD Status and Perspectives, S. Derriere > http://www.ivoa.net/internal/IVOA/IvoaUCD/UCD-status0203.pdf On the top of page 3 of this document, I am told that UCDs are not: - accurate definitions, - expressing physical dimensionality, or - tied to units. Why not? I would imagine that UCDs would be most useful if they were *all* of the above. Accurate definitions: if they are not accurate, what good are they? Why would I want to search a bunch of UCDs to find one that *might* measure what I'm looking for, rather than one that *does*? I imagine an accurate definition would be needed for this. Expressing physical dimensionality: why shouldn't they? This is a simple concept, and one that certainly could assist with at least figuring out if two apparently different UCDs can actually be compared. It's certainly not in and of its own a powerful concept, but it's perfectly possible that I might want to look for any columns which measure a length of time... On the other hand, physical dimensionality can often be derived from the units, so this is not a critical inclusion. Tied to units: again, I'm not clear on why they shouldn't be in the UCD. If we don't store units in the UCD, they have to be stored somewhere else, and then the column values are useless without *both* the UCD and this other bit of information. Overall I am in favour of having all information which describes a single measurement stored in the one place. The UCD seems like a good candidate to be that place. More generally, I felt that one way to categorize UCDs would be as: - instrumental UCDs - measurement UCDs - derived UCDs in the sense that any particular column is generally going to be either, respectively: - a setting you made on your telescope or in your theoretical software (eg. a table of frequencies corresponding to each channel of a spectrometer, or the number of particles in your simulation, ...) - a measurement you actually made (eg. the flux density at each channel of your spectrometer, the energy of each of your simulation particles) - a derived quantity, such as the line-integrated flux of your spectrum, or the total energy of your particles Then measurement UCDs would include "links" to the minimal set of instrumental UCDs needed to repeat the measurement, and derived UCDs would include "links" to the minimal set of measurement UCDs (and implicitly instrumental UCDs) to repeat the obtaining of the derived value. I think a scheme like this would enable some pretty advanced searching, such as finding catalogues (or more generally sources of data) who measured the same thing as you but in a different way. Just one idea really. Maybe I have sidetracked on to the data model, please let me know if I have. Apologies if all the above has been said and discussed in the past. Interested to hear what others think of the above. David. From - Thu Apr 10 07:33:39 2003 X-UIDL: 3e5baf6500000527 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h3A5UThl019621 for ; Thu, 10 Apr 2003 07:30:30 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h3A5UTn28563 for ; Thu, 10 Apr 2003 07:30:29 +0200 (MEST) Received: from dns.ph.unimelb.edu.au(128.250.50.25) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAxXaqY3; Thu, 10 Apr 03 07:30:27 +0200 Received: (qmail 24188 invoked from network); 10 Apr 2003 05:24:25 -0000 Received: from isis.ph.unimelb.edu.au (128.250.51.69) by indy.ph.unimelb.edu.au with SMTP; 10 Apr 2003 05:24:25 -0000 Received: (from dbarnes@localhost) by isis.ph.unimelb.edu.au (8.11.6+Sun/8.9.1) id h3A5TLF15651; Thu, 10 Apr 2003 15:29:21 +1000 (EST) From: David Barnes Message-Id: <200304100529.h3A5TLF15651@isis.ph.unimelb.edu.au> Subject: Re: Pre-meeting UCD question To: rplante@ncsa.uiuc.edu Date: Thu, 10 Apr 2003 15:29:21 +1000 (EST) Cc: ucd@ivoa.net In-Reply-To: from "Ray Plante" at Apr 10, 2003 12:15:45 AM Reply-To: barnesd@unimelb.edu.au X-Mailer: ELM [version 2.5 PL3] MIME-Version: 1.0 Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Hi, > > Accurate definitions: if they are not accurate, what good > > are they? > > The practice of UCD use to date has been mainly about relating quantities > from different catalogs which may use different column names but otherwise > refer to the same or related concepts. In other words, UCDs are a common > vocabulary that can be used to bridge different local schemas. I think, > in general, the more accurate the definitions, the more meaningful the > comparisons one can make. However, there is often a point where accuracy > begins to work against you. Rarely are two columns from different tables > exactly the same thing which can be compared directly. If your > definitions are two precise, you might not be able to recognize two things > as similar. > > I like to say that when interoperating between diverse resources, you need > to squint your eyes a bit and blur the details. How much you have to blur > is measure of how meaningful or accurate your interoperation is. > > What would be nice would be a UCD framework that allows the user to > choose (to some extent) the level of accuracy at "run-time" (rather than > having it frozen in an instance of a catalog). This might involve parsing > the UCD in some way. For example, if two frequencies are both in the > radio, that might be close enough. (Is there a requirement in here > somewhere?) I certainly agree with the general idea that for nearly any comparison you need to apply some sort of "blur" to the details. But to me this suggests that the UCDs *should* be as accurate as possible, and then they can be interpreted at the desired level of accuracy. They can be used to describe the data, *and* to interoperate. I suppose most catalogues would then have their own UCDs, but hopefully well-enough described UCDs so that comparisons can indeed be made. - David. From - Thu Apr 10 07:18:38 2003 X-UIDL: 3e5baf6500000526 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h3A5Glhl014211 for ; Thu, 10 Apr 2003 07:16:47 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h3A5Gk828231 for ; Thu, 10 Apr 2003 07:16:46 +0200 (MEST) Received: from poplar.ncsa.uiuc.edu(141.142.65.122) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAadaWi3; Thu, 10 Apr 03 07:16:45 +0200 Received: from localhost (rplante@localhost) by poplar.ncsa.uiuc.edu (8.11.6/8.11.6) with ESMTP id h3A5Fjq27924 for ; Thu, 10 Apr 2003 00:15:45 -0500 Date: Thu, 10 Apr 2003 00:15:45 -0500 (CDT) From: Ray Plante Reply-To: Ray Plante To: ucd@ivoa.net Subject: re: Pre-meeting UCD question In-Reply-To: <200304070422.h374MWv29499@isis.ph.unimelb.edu.au> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Hi David, On Mon, 7 Apr 2003, David Barnes wrote: > Maybe I have sidetracked on to the data model, please let > me know if I have. Well, I think this simply illustrates that there is (or should be) a close relationship between data models and UCDs. > Accurate definitions: if they are not accurate, what good > are they? The practice of UCD use to date has been mainly about relating quantities from different catalogs which may use different column names but otherwise refer to the same or related concepts. In other words, UCDs are a common vocabulary that can be used to bridge different local schemas. I think, in general, the more accurate the definitions, the more meaningful the comparisons one can make. However, there is often a point where accuracy begins to work against you. Rarely are two columns from different tables exactly the same thing which can be compared directly. If your definitions are two precise, you might not be able to recognize two things as similar. I like to say that when interoperating between diverse resources, you need to squint your eyes a bit and blur the details. How much you have to blur is measure of how meaningful or accurate your interoperation is. What would be nice would be a UCD framework that allows the user to choose (to some extent) the level of accuracy at "run-time" (rather than having it frozen in an instance of a catalog). This might involve parsing the UCD in some way. For example, if two frequencies are both in the radio, that might be close enough. (Is there a requirement in here somewhere?) cheers, Ray From - Thu Apr 10 06:58:39 2003 X-UIDL: 3e5baf6500000525 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h3A4rWhl005607 for ; Thu, 10 Apr 2003 06:53:33 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h3A4rWx27791 for ; Thu, 10 Apr 2003 06:53:32 +0200 (MEST) Received: from poplar.ncsa.uiuc.edu(141.142.65.122) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAMQaOr2; Thu, 10 Apr 03 06:53:31 +0200 Received: from localhost (rplante@localhost) by poplar.ncsa.uiuc.edu (8.11.6/8.11.6) with ESMTP id h3A4qUO27899 for ; Wed, 9 Apr 2003 23:52:30 -0500 Date: Wed, 9 Apr 2003 23:52:30 -0500 (CDT) From: Ray Plante Reply-To: Ray Plante To: ucd@ivoa.net Subject: Re: Pre-meeting UCD question In-Reply-To: <01b101c2fad0$9168a0d0$d2add783@roxy> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: On Fri, 4 Apr 2003, Roy Williams wrote: > (2) Perhaps we can start a discussion by asking for requirements in trhe > following question: > ***** WHAT ARE UCD USED FOR -- now and future ***** What UCDs are used for now: I feel this is well summarized in Sabastien's document (http://www.ivoa.net/internal/IVOA/IvoaUCD/UCD-status0203.pdf), section 1.4.2. The uses, I believe, all leverage off the tagging of catalog columns with UCD names, relating the column to a common concept. (Is that correct?) Requirements for the Future: Disclosure: *-ed items represent my own peculiar take on UCDs o A UCD must be able to serve as a reference to a common concept applicable across heterogenous datasets and applications. o It must be possible to use a UCD as a concept reference in a variety of contexts. In particular, it must be possible to: - tag data representing instances or values of a common concept and stored in a generic container; e.g. a VOTable column. - tag data stored in an XML document using some local schema - refer to common concepts to be used in a query, either as part of a query constraint or results request. [A single string of limited length is generally the most flexible in meeting this requirement.] o There should be an accessible document or resource that provides the definitive UCD definitions (i.e. the mapping of UCD names to the concepts they refer to). * There should be a clear, straight-forward relationship between UCDs, metadata, and data models; that is, there should be an obvious relationship between a UCD, a metadatum, and a data model component that refer to the same basic concept. Extension and Standardization: * It should be possible for a community to recommend a preferred set or sets of UCDs that can be applied across diverse resources. * It should be possible for a limited community to define new UCDs that are not covered by a currently accepted set, but understood only within a limited context. It should be possible to use them transparently alongside the currently accepted set. * There should exist a process by which new UCDs can be folded into the broadly accepted set. Compatability: * Any new UCD framework should allow the continued use of the current CDS/ESO UCDs. While they may be individually depricated as new UCDs are defined, backward-compatibility should be preserved. From - Mon Apr 28 20:54:48 2003 X-UIDL: 3e5baf6500000717 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h3SIqv0V003172; Mon, 28 Apr 2003 20:52:57 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h3SIqv423289; Mon, 28 Apr 2003 20:52:57 +0200 (MEST) Received: from ns1.u-strasbg.fr(130.79.200.1) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAA5uaaFT; Mon, 28 Apr 03 20:52:56 +0200 Received: from vizir.u-strasbg.fr (vizir.u-strasbg.fr [130.79.128.13]) by ns1.u-strasbg.fr (8.12.6p2/jtpda-5.4) with ESMTP id h3SIpeNF078442 ; Mon, 28 Apr 2003 20:51:40 +0200 (CEST) Received: (from francois@localhost) by vizir.u-strasbg.fr (8.11.6+Sun/8.9.1) id h3SIp9n14227; Mon, 28 Apr 2003 20:51:09 +0200 (MET DST) Date: Mon, 28 Apr 2003 20:51:09 +0200 (MET DST) From: Francois Ochsenbein Message-Id: <200304281851.h3SIp9n14227@vizir.u-strasbg.fr> To: votable@ivoa.net Subject: Column Groups in VOTable Cc: ucd@ivoa.net X-Antivirus: scanned by sophos at u-strasbg.fr X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Dear All, The forthcoming meeting in Cambridge could be a good opportunity to discuss how "column groups" can be introduced in VOTable. Such a functionality was already expressed (maybe not explicitely); I feel that this it has also implication on UCDs, and I'm therefore posting this message to both VOTable and UCD groups. I apologize to those who will receive this message twice. -- Francois ================================================================================ Francois Ochsenbein ------ Observatoire Astronomique de Strasbourg 11, rue de l'Universite F-67000 STRASBOURG Phone: +33-(0)390 24 24 29 Email: francois@astro.u-strasbg.fr (France) Fax: +33-(0)390 24 24 17 ================================================================================ ================================================================================ The "column groups" proposition tries to answer questions frequently themail: Undefined variable asked about column associations, typically: --> error (or standard deviation) associated to a column, e.g. a flux consists of two numbers: the measured value + the mean error --> qualities or weights associated to values --> source or origin (e.g. telescope, or bibliographical reference) of a value --> individual components e.g. x,y position of a CCD --> etc... This "column grouping" has obviously the same role as defining structures made of columns; defining structures made of structures can also be viewed as grouping groups of columns. I see essentially two ways of defining such "column groups" in VOTable: a) generalize the method currently used to describe the coordinate systems. This kind of "by reference" method defines a structure, and any can declare (via the "ref" attribute) to be a member of that structure. As an illustration of a group of columns containing a flux value and its error, the XML code could look like: 1. within the element, define a structure as e.g.: 2. within the definition, columns belonging to this structure refer to it: b) introduce a new element e.g. in the
description which would contain the fields. The same example of a flux + its associated error would be coded as: Value of the flux at 8.4GHz Error on flux value There could be a third way which would introduce new tags within each table element like e.g. and to give but it would be against the current philosophy of VOTable which defines all metadata first, and is followed by the data alone, in order to keep the efficiency and the FITS compatibility; this third method would also require frequent modifications of the schema (XMLSchema) -- generally disturbing for working applications. The defined in b) above seems to me to be a good framework for this definition. I see several advantages: => the basic tabular scheme remains -- VOTable can still be viewed as a relational database, and keeps a full compatibility with existing FITS binary tables; => groups of groups (i.e. recursive tags) enables a definition of arbitrary complex structures; => the UCDs become more accurate when defined in a group: -- adding tags within a nicely introduces a way of parametrizing a UCD -- FIELDs defined in a group can acquire the UCD of the group e.g. the error part of the flux group of fields just need the "ERROR" UCD. Using the "ref" attribute in also permits one column to be a member of several groups: for example, an error common to two fluxes measured at different frequencies can be defined as: Value of the flux at 8.4GHz Error on flux values, both at 8.4 and 7.5GHz Value of the flux at 7.5GHz ================================================================================ From - Tue Apr 29 11:24:49 2003 X-UIDL: 3e5baf6500000744 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h3T9MdWg009346 for ; Tue, 29 Apr 2003 11:22:39 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h3T9McM21402 for ; Tue, 29 Apr 2003 11:22:38 +0200 (MEST) Received: from ns1.u-strasbg.fr(130.79.200.1) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAy7aOYP; Tue, 29 Apr 03 11:22:37 +0200 Received: from vizir.u-strasbg.fr (vizir.u-strasbg.fr [130.79.128.13]) by ns1.u-strasbg.fr (8.12.6p2/jtpda-5.4) with ESMTP id h3T9LMNF070683 for ; Tue, 29 Apr 2003 11:21:22 +0200 (CEST) Received: from vizier (localhost [127.0.0.1]) by vizir.u-strasbg.fr (8.11.6+Sun/8.9.1) with ESMTP id h3T9KoV10291 for ; Tue, 29 Apr 2003 11:20:50 +0200 (MET DST) Message-Id: <200304290920.h3T9KoV10291@vizir.u-strasbg.fr> To: ucd@ivoa.net Subject: Column Grouping in VOTable and UCD implications Date: Tue, 29 Apr 2003 11:20:50 +0200 From: Francois Ochsenbein X-Antivirus: scanned by sophos at u-strasbg.fr X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Dear All, The forthcoming meeting in Cambridge could be a good opportunity to discuss how "column groups" can be introduced in VOTable. Such a functionality was already expressed (maybe not explicitely); I feel that this it has also implication on UCDs, and I'm therefore posting this message to both VOTable and UCD groups. I apologize to those who will receive this message twice. -- Francois ================================================================================ Francois Ochsenbein ------ Observatoire Astronomique de Strasbourg 11, rue de l'Universite F-67000 STRASBOURG Phone: +33-(0)390 24 24 29 Email: francois@astro.u-strasbg.fr (France) Fax: +33-(0)390 24 24 17 ================================================================================ ================================================================================ The "column groups" proposition tries to answer questions frequently themail: Undefined variable asked about column associations, typically: --> error (or standard deviation) associated to a column, e.g. a flux consists of two numbers: the measured value + the mean error --> qualities or weights associated to values --> source or origin (e.g. telescope, or bibliographical reference) of a value --> individual components e.g. x,y position of a CCD --> etc... This "column grouping" has obviously the same role as defining structures made of columns; defining structures made of structures can also be viewed as grouping groups of columns. I see essentially two ways of defining such "column groups" in VOTable: a) generalize the method currently used to describe the coordinate systems. This kind of "by reference" method defines a structure, and any can declare (via the "ref" attribute) to be a member of that structure. As an illustration of a group of columns containing a flux value and its error, the XML code could look like: 1. within the element, define a structure as e.g.: 2. within the
11.351.12
definition, columns belonging to this structure refer to it: b) introduce a new element e.g. in the
description which would contain the fields. The same example of a flux + its associated error would be coded as: Value of the flux at 8.4GHz Error on flux value There could be a third way which would introduce new tags within each table element like e.g. and to give but it would be against the current philosophy of VOTable which defines all metadata first, and is followed by the data alone, in order to keep the efficiency and the FITS compatibility; this third method would also require frequent modifications of the schema (XMLSchema) -- generally disturbing for working applications. The defined in b) above seems to me to be a good framework for this definition. I see several advantages: => the basic tabular scheme remains -- VOTable can still be viewed as a relational database, and keeps a full compatibility with existing FITS binary tables; => groups of groups (i.e. recursive tags) enables a definition of arbitrary complex structures; => the UCDs become more accurate when defined in a group: -- adding tags within a nicely introduces a way of parametrizing a UCD -- FIELDs defined in a group can acquire the UCD of the group e.g. the error part of the flux group of fields just need the "ERROR" UCD. Using the "ref" attribute in also permits one column to be a member of several groups: for example, an error common to two fluxes measured at different frequencies can be defined as: Value of the flux at 8.4GHz Error on flux values, both at 8.4 and 7.5GHz Value of the flux at 7.5GHz ================================================================================ From - Fri May 2 16:44:51 2003 X-UIDL: 3e5baf650000081d X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h42EhY5a026041 for ; Fri, 2 May 2003 16:43:35 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h42EhYb27930 for ; Fri, 2 May 2003 16:43:34 +0200 (MEST) Received: from gannet.scg.man.ac.uk(130.88.94.110) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAWsaaJ2; Fri, 2 May 03 16:43:33 +0200 Received: from star1.jb.man.ac.uk ([130.88.24.176]) by gannet.scg.man.ac.uk with esmtp (Exim 2.05 #6) id 19Bbl7-000BMS-00 for ucd@ivoa.net; Fri, 2 May 2003 15:43:33 +0100 Received: from [130.88.24.148] (helo=adikia) by star1.jb.man.ac.uk with esmtp (Exim 3.03 #2) id 19BblY-0001Mh-00 for ucd@ivoa.net; Fri, 02 May 2003 15:44:00 +0100 Date: Fri, 2 May 2003 15:43:21 +0100 (BST) From: Anita Richards X-X-Sender: amsr@adikia To: ucd@ivoa.net Subject: Re: Pre-meeting UCD question Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Ray Plante's 'Requirements for the Future' is a very neat summary, and I am especially glad he has put on record the need for * Accessible documentation and * Backward compatibility - and I think it is a good basis for the Cambridge discussion There are a couple of things which have come up previously: The use of UCDs other than for column content descriptors - e.g. for the ResourceMetadata which summarises the content of a dataset for the Registry. Should these be taken from exactly the same set of UCDs? Or should these embody their context (e.g. by reserving superclass UCDs, such as the first element if we use Guy Rixon's atoms...)? How to qualify UCDs? At the moment we have some 'degenerate' UCDs, e.g. SPEC_WAVELENGTH in the IDHA model for both the high and low bandpass limits. This means you have to evaluate both, if you just want data above a certain frequency (say). Then we have some overspecified, e.g. all the PHOT ones for U B V R I, RADIO_1.6, _1.4 etc. In some cases this might be solved just by adding MAX/MIN or equivalent (LONG and SHORT for the bandpass as MAX/MIN is ambiguous unless you know if it is freq. or wavelength). However with XML we can be more intelligent, as has been pointed out, and give them properties or attributes or values. How do we cope with the cases where the required information (ie another UCD?) is elsewhere in the same data set, e.g. another column or in the header? e.g. for associating cumulative errors with a data point, or for realising that an entire catalogue is at 1.4 GHz or in the Cousins photometry convention? That is, we need not only to be able to select on the basis of UCDs, but to be able to interpret their properties at the Registry level. In some cases we might need to evaluate the data they describe at the Registry (as in the present bandpass example I gave), but perhaps that can be avoided, or should be, if possible, so that you only have to dive into the dataset itself when you are answering the query in detail? This can be summed up as saying that we want UCDs to describe data but we should avoid as much as possible using UCDs as data. Thoughts on some of David's comments: Units and accuracy When we are using UCDs (assuming this includes the ResourceMetadata) in the Registry, we do not need high accuracy as long as we err on the side of inclusion (so a catalogue spanning 10 - 3001 GHz would be both radio and IR). If we want catalogues with photometry, we do not need to know what units the flux is measured in. However if we want a certain level of accuracy we do need units (at least if we are to avoid quality factors etc. which will be very arbitrary) - but here, the Registry could standardise everything to one sort of unit for each quantity as the conversion does not need to be accurate (e.g. noise < 0.0001 Jy derived from a certain limiting magnitude) as long as it is rounded down/up as appropriate. This is analogous to Ray's squinting. I think it is crucial that do not tie UCDs to certain units or whatever, as we then make it difficult to interconvert. Any conversion errors should be carried in proper UCDs for errors - thus, if you ask for x-ray photometry in counts, you will get a result which will probably ahve greater accuracy than if you ask for it in Jy - but the latter is vital if you want to compare it with data at other wavelengths. Cheers a - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - Dr. Anita M. S. Richards, AVO Astronomer MERLIN/VLBI National Facility, University of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire SK11 9DL, U.K. tel +44 (0)1477 572683 (direct); 571321 (switchboard); 571618 (fax). From - Mon May 12 07:10:03 2003 X-UIDL: 3e5baf6500000946 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h4C57VAC005525 for ; Mon, 12 May 2003 07:07:31 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h4C57VA09290 for ; Mon, 12 May 2003 07:07:31 +0200 (MEST) Received: from phobos.caltech.edu(131.215.102.1) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAiGaijs; Mon, 12 May 03 07:07:30 +0200 Received: from avyakta.caltech.edu (avyakta [131.215.102.12]) by phobos.caltech.edu (8.12.2/8.12.5) with ESMTP id h4C4xwZE005217 for ; Sun, 11 May 2003 21:59:58 -0700 (PDT) Received: from localhost (localhost.localdomain [127.0.0.1]) by avyakta.caltech.edu (8.12.8/8.11.2) with ESMTP id h4C509gC001046 for ; Sun, 11 May 2003 22:00:09 -0700 Date: Sun, 11 May 2003 22:00:09 -0700 (PDT) From: Ashish Mahabal X-X-Sender: aam@avyakta.caltech.edu To: ucd@ivoa.net Subject: Some comments on UCDs Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Hi, Since I will not be personally present when many of you meet in Europe (now), I decided to send in my two cents to the group. Over the last few months, talking to several VO people from US and Europe, it is clear that everyone agrees that something like the UCDs is great. Not everyone agrees on (1) the number of UCDs, (2) the hierarchical nature they are currently arranged in, (3) mechanisms of adding UCDs, ... Suggestions range from leave UCDs as they are to completely replace them with alternate mechanisms (some of which have at least partially been thought of). Having worked with UCDs for making Topic Maps based on UCDs in catalogs (examples at http://www.astro.caltech.edu/~aam/science/topicmaps/ucd.html - a specialised application based on these will be ready soon), I have come to like the ease with which one can use UCDs to build structure around them (though they certainly have their limitations, as is seen by some "gaps" in some of the topic maps). I have not been required to deal with the entire set of UCDs (e.g. Atomic Data, Orbit etc. related UCDs) as I have not dealt with all kinds of catalogs. But the hierarchical structure seems very useable. Having error terms on various individual UCDs will be good and some work could go in there. Of the 1400 or so UCDs, the 100 most accessed catalogs at Vizier use only about 250 UCDs in all. Allowing people to make their own UCDs (just like standards should not be a plural, not everyone should create their own Universals) will bring us back to square one even if what the personal UCDs mean is well documented. My R magnitude UCD is GunnR and some one elses is GR (both having used the Thuan-Gunn system). Okay so far. But then I also use GR to mean Gamma Ratio (whatever that is), and all hell breaks loose. A lot of time may have to be spent in writing more intelligent software to deal with these issues which could in the first place have been avoided. So should there be "UCD police" who decide what new UCDs should get added? Perhaps not. But everybody concerned can try to come up with a list of what is currently missiing, and what will probably be needed in the next 10 years (and later on there will be surprises of course), and simply add the resulting list. And keep a mechanism for adding more. Should the list be changed from a hierarchy to something else? That should not really matter much. (Broadly speaking - software should be able to handle that). Should the UCDs serve as an ontology for astronomy? I beileve that in a sense it is. However, I also believe that anything that is related to astronomy (e.g. astronomers, instruments, observatories etc.) should also be part of that ontology and could be represented by UCDs in the hierarchy (adding a few hundred more terms). These can then be used in many other tables (derived data products). So a growing branch could stay open there. More later. Cheers and wishing you all a good time, -ashish PS: Does some one plan to email session summaries to the group? Ashish Mahabal, Caltech Astronomy, Pasadena, CA 91125 http://www.astro.caltech.edu/~aam aam@astro.caltech.edu Lawyer: How far apart were the vehicles at the time of the collision? From - Fri May 16 13:15:11 2003 X-UIDL: 3e5baf65000009db X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h4GBFmmR018971 for ; Fri, 16 May 2003 13:15:48 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h4GBFmc24844 for ; Fri, 16 May 2003 13:15:48 +0200 (MEST) Received: from ny2.fastmail.fm(66.111.4.3) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAA0wayHW; Fri, 16 May 03 13:15:47 +0200 Received: from smtp.us2.messagingengine.com (server2.internal [10.202.2.133]) by server2.messagingengine.com (Postfix) with ESMTP id 034E14DAEE for ; Fri, 16 May 2003 07:14:45 -0400 (EDT) Received: from 127.0.0.1 ([127.0.0.1] helo=smtp.us2.messagingengine.com) by messagingengine.com with SMTP; Fri, 16 May 2003 07:14:45 -0400 Received: by smtp.us2.messagingengine.com (Postfix, from userid 99) id F2F465C479; Fri, 16 May 2003 07:14:44 -0400 (EDT) Content-Disposition: inline Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset="ISO-8859-1" MIME-Version: 1.0 X-Mailer: MIME::Lite 1.2 (F2.71; T1.001; A1.51; B2.12; Q2.03) From: "Tony Linde" To: ucd@ivoa.net Date: Fri, 16 May 2003 12:14:44 +0100 X-Epoch: 1053083685 X-Sasl-enc: g/ybv8vno84R6lEizHDxyw Subject: MyUCDs Message-Id: <20030516111444.F2F465C479@smtp.us2.messagingengine.com> X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: I've posted a document on the IVOA wiki which summarises my understanding of the UCD discussion in the plenary session yesterday. Perhaps some people could peruse that and provide feedback on this mailing list about any errors or differences of opinion on the implications that I see. I hope it helps others with any of their own misunderstandings. http://www.ivoa.net/twiki/bin/view/IVOA/TonyOnUCDs Cheers, Tony. __ Tony Linde Phone: +44 (0)116 223 1292 AstroGrid Project Manager Fax: +44 (0)116 252 3311 Dept of Physics & Astronomy Mobile: +44 (0)7753 603356 University of Leicester Email: ael@star.le.ac.uk Leicester, UK LE1 7RH Web: http://www.astrogrid.org From - Fri May 16 14:50:11 2003 X-UIDL: 3e5baf65000009dc X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h4GCkBUE021731 for ; Fri, 16 May 2003 14:46:11 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h4GCkBp02411 for ; Fri, 16 May 2003 14:46:11 +0200 (MEST) Received: from apollo.le.ac.uk(143.210.16.125) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAHpaiTe; Fri, 16 May 03 14:46:10 +0200 Received: from [143.210.36.58] (helo=mail.star.le.ac.uk) by apollo.le.ac.uk with smtp (Exim 4.14) id 19GeXW-0001cU-UY for ucd@ivoa.net; Fri, 16 May 2003 13:42:22 +0100 Received: (qmail 99 invoked from network); 16 May 2003 12:42:43 -0000 Received: from sparky.star.le.ac.uk (143.210.36.10) by mail.star.le.ac.uk with SMTP; 16 May 2003 12:42:43 -0000 Date: Fri, 16 May 2003 13:42:43 +0100 (BST) From: "Patricio F. Ortiz" To: Tony Linde cc: ucd@ivoa.net Subject: Re: MyUCDs In-Reply-To: <20030516111444.F2F465C479@smtp.us2.messagingengine.com> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Spam-Score: (--------------------------) -26.4 X-Scanner: exiscan for exim4 *19GeXW-0001cU-UY*hJH7t.WeYa2* Status: On Fri, 16 May 2003, Tony Linde wrote: > I've posted a document on the IVOA wiki which summarises my understanding > of the UCD discussion in the plenary session yesterday. Perhaps some > people could peruse that and provide feedback on this mailing list about > any errors or differences of opinion on the implications that I see. I > hope it helps others with any of their own misunderstandings. > > http://www.ivoa.net/twiki/bin/view/IVOA/TonyOnUCDs Here go my comments to Tony's document: > My understanding of UCDs > > The way this came up was my question in the plenary UCD session about > how we can identify columns within a table uniquely. Basically, the > answer was that UCDs will not solve this problem and are not intended > to do so. This page will summarise what I now understand as the purpose > of UCDs and some of the implications of this. > > UCDs as Data Types > > Comment was made that UCDs can be considered as data types, so a column > in a table has a data type of, POS_EQ_RA, say. I assume that the > reasons for having UCDs as data types are to allow: > > * operations on columns: comparison, addition, subtraction, > multiplication, etc plus specific astronomical operations > * conversion between data types: eg converting between equitorial and > galactic coordinates As their name say, UCDs are meant to describe the content of a column uniquely. Within any given table, column names do not repeat (unless in exceptional cases where the authors want to repeat a column for easy reading. The problem arose when column names became degenerate when analyzing different tables/catalogues. The most common scenario for astronomy was a column called "Mag" , meant to represent the brightness of a celestial object in some photometric system. The problem was/is that "Mag" was "overloaded" and just comparing two columns labeled "Mag" was a cry for trouble. UCDs were introduced to break the degeneracy. column (catalog=c1 name=Mag unit=mag UCD=PHOT_JHN_V) has nothing to do with column (catalog=c2 name=Mag unit=mag UCD=PHOT_STR_B) > Do we thus need (or already have) some hierarchical structure of the > UCDs based on allowable operations? In normal data types, we have > numerical types, subdivided by integral and floating point, subdivided > by storage size etc; one can add all numerical types but (generally) > cannot add a number and a string (without pre-defining what such an > addition will do). Although one can add numerical types and not add strings or strings and numbers, not all numbers should be allowed to be added. One should not allow adding a velocity measured in km/s to a right ascention in equatorial coordinates (an angle). Whatever mechanism is used to perform table combination should be provided with this kind of knowledge. > Aligned to that: should we define the operations that can be performed > on the individual data types (UCDs), the rules for those operations > given specific types, and the type resulting from such operations. Yes and no, thinking of all combination is unrealistic, plus, it's only in adding/subtracting where you have problems. No-one could impede you to take ratios of columns or multiply columns. As Peter Quinn pointed out in the plenary, some decisions should always be the responsibility of the astronomer. > UCDs as Keywords > > In this context, the UCDs is part of the metadata for a table. It > indicates the type of data held in a table, so having POS_EQ_RA > identified with a table says that this table includes positional data > in equitorial coordinates. That said, maybe the UCD for the table > should include POS_EQ instead (since it is unlikely that it'll have RA > without DEC). Unlikely but not impossible. I've seen tables in which that's the case. UCD's were meant to be attached to columns, talking about a table's UCD is IMHO a confusion. A Table can have a set of UCDs attached to it (like a list), which may be shorter than the number of columns in the table if some columns happen to be representative of the same physical quantity therefore they DO have the same UCD. > So the idea of being able to query which resources have POS_EQ* makes sense. Sure it does. Not all catalogues contain RA-Dec. > UCDs as Pointers into Data Model > > This was a very interesting comment, that UCDs can be seen as a pointer > into the data model (DM). How this might be implemented and how > feasible it is is still open. I guess there are two potential problem > areas: > > * a UCD refers to multiple DM points (classes, objects or whatever > they are called) this is likely but does indicate areas in which the > UCDs are not the lowest level of metadata > > * one DM point is referred to by several UCDs > if this occurs, it would indicate that the DM requires further analysis Yes and no. Yes if we are talking about the so called "core-UCDs", which are the UCDs which can be attached to a column. No if we develop the concept of an "alias-UCD", which represents a list of UCDs design for discovery purposes. I'd say that a DM should have one "core-UCD" and 0 or more "alias-UCDs" > I suspect that, as the DM expands and covers more areas of astronomy, > we will need a more efficient version of UCDs that accurately maps to > the DM; the current '_' separated textual names will have limited > extensibility (even with the additional modifiers agreed at this > meeting). Most likely. > Unique Column Identification > > Given that we cannot use UCDs as unique column identifiers, how do we do this? > It seems that the only possible unique identifier for a column in a > table is the resourceID of the table (from the Registry) plus the > columnName (for explanation of resourceID, see the discussion on this > in the Registry mailing list: > http://www.ivoa.net/forum/registry/0091.htm and related messages). Absolutely, Within a table, the column name IS a unique column identifier. The pair catalogueName.columnName is in 99.9% of the cases unique, and for the future, one can impose that columnName be unique within a table (most DBMS won't be so happy if you assign 2 columns with the same name). If we ever converge to assign unique IDs to catalogues, then cataloqueUniqueID.columnName is unique Adding a UCD to this structure would be redundant eg, cataloqueUniqueID.columnName.columnUCD > So, to summarise the discussion from the plenary session, a query can > be sent to a table with either UCDs or column names or a mixture of > both. If a UCD is included in a query, the data source can resolve this > if there is only one column with that UCD or there are multiple columns > but one has the modifier MAIN attached to only one of the column UCDs. > Otherwise the query will fail. Let me include here another element before the submission of a query to the resource handling catalogues: The registry. Any registry will contain metadata about the services listed, ie, the catalogues. The registry would know (among other things), - catalogueName (possibly catalogueUniqueID) - catalogueTitle - catalogueKeywords - catalogueAuthor - number of columns - number of records - column names, UCDs, units - name ID,MAIN --- - RA POS_EQ_RA,MAIN h:m:s - Dec POS_EQ_DEC,MAIN d:m:s .... - Vmag PHOT_JHN_V mag - Bmag PHOT_JHN_B mag - z REDSHIFT --- IMHO, a query can be accurately formulated for any given resource after consulting the registry. It should be decided at the registry level what we want to extract from any given catalogue, therefore, the query received by the resource handling that catalogue has to make no decision, and what's best, the query should not even be submitted if we know ahead of time that it will fail. > Conclusion > > I hope people will provide feedback on the mailing list to these > comments. I reiterate that they are only my understanding of what was > said and my belief of the implications. Another use of UCDs would be to discover resources (catalogues) which contain certain QUANTITIES. Scenario 1 If I formulate a query in the line "select catalogueName where UCDs include REDSHIT POS_EQ_RA,MAIN POS_EQ_DEC,MAIN PHOT_JHN_V from registryXX" I should get back a listing of catalogues which contain that information (plus probably the column names, units and UCDs which make the catalogue satisfy our request). Titles and keywords are short handles and do not always tell about all is listed in a catalogue. The astronomer should know what to do with this information, perhaps s/he will pick up a few of these catalogues and submit a query to them. Scenario 2 "select ucd;ID,MAIN ucd;POS_EQ_RA,MAIN ucd;POS_EQ_RA,MAIN ucd;PHOT_JHN_V ucd;REDSHIFT from [catalogueName where UCDs include REDSHIFT PHOT_JHN_V POS_EQ_RA,MAIN POS_EQ_DEC,MAIN from registryXX] where ucd;REDSHIFT > 2.5" The user doesn't know ahead of times if any ocatalogue exists to satisfy the query, but if it exist, s/he would like to print the equivalent of Name, RA, Dec, Vmag, and z This query should first find out a list of catalogues which contain all those UCDs and the name of their respective columns. Once this is known, individual queries should be sent to each of the catalogues requesting the columns which identify with the UCDs the user requested and which satisfy redshift > 2.5. Note that I've used a very loose notation above on purpose Cheers, Patricio --- Patricio F. Ortiz pfo@star.le.ac.uk AstroGrid project Department of Physics and Astronomy University of Leicester Tel: +44 (0)116 252 2015 LE1 7RH, UK From - Mon May 19 16:50:18 2003 X-UIDL: 3e5baf6500000a17 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h4JEmiG1025776; Mon, 19 May 2003 16:48:44 +0200 (MEST) Received: from eso.org (nb008487.ads.eso.org [134.171.27.211]) by serapis.hq.eso.org (8.11.6+Sun/8.11.6) with ESMTP id h4JEnGL03823; Mon, 19 May 2003 16:49:16 +0200 (MEST) Message-ID: <3EC8EECB.1000604@eso.org> Date: Mon, 19 May 2003 16:48:43 +0200 From: "Marco C. Leoni" Reply-To: mleoni@eso.org Organization: Astrophysical Virtual Observatory @ESO User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.0.1) Gecko/20020823 Netscape/7.0 (CK-ESO) X-Accept-Language: en, en-us MIME-Version: 1.0 To: "Patricio F. Ortiz" CC: ucd@ivoa.net Subject: Re: MyUCDs References: Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Hi Patricio, one question about the point below: > Let me include here another element before the submission of a > query to the resource handling catalogues: The registry. > > Any registry will contain metadata about the services listed, ie, > the catalogues. > The registry would know (among other things), > - catalogueName (possibly catalogueUniqueID) > - catalogueTitle > - catalogueKeywords > - catalogueAuthor > - number of columns > - number of records > - column names, UCDs, units > - name ID,MAIN --- > - RA POS_EQ_RA,MAIN h:m:s > - Dec POS_EQ_DEC,MAIN d:m:s > .... > - Vmag PHOT_JHN_V mag > - Bmag PHOT_JHN_B mag > - z REDSHIFT --- > are you sure the Registry will include all these information? Perhaps "column names" and "units" will be resolved by the service provider, and not by the registry itself. Cheers, Marco From - Mon May 19 17:25:18 2003 X-UIDL: 3e5baf6500000a1b X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h4JFKpG1008793 for ; Mon, 19 May 2003 17:20:51 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h4JFKop27714 for ; Mon, 19 May 2003 17:20:50 +0200 (MEST) Received: from mailsend.le.ac.uk(143.210.16.126) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAW4a4h2; Mon, 19 May 03 17:20:49 +0200 Received: from [143.210.36.58] (helo=mail.star.le.ac.uk) by artemis.le.ac.uk with smtp (Exim 4.14) id 19HmNm-0006bO-Se for ucd@ivoa.net; Mon, 19 May 2003 16:16:58 +0100 Received: (qmail 10416 invoked from network); 19 May 2003 15:17:13 -0000 Received: from sparky.star.le.ac.uk (143.210.36.10) by mail.star.le.ac.uk with SMTP; 19 May 2003 15:17:13 -0000 Date: Mon, 19 May 2003 16:17:13 +0100 (BST) From: "Patricio F. Ortiz" To: "Marco C. Leoni" cc: ucd@ivoa.net Subject: Re: MyUCDs In-Reply-To: <3EC8EECB.1000604@eso.org> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Spam-Score: (-------------------------) -25.3 X-Scanner: exiscan for exim4 *19HmNm-0006bO-Se*Qhm57OFrR/s* X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: On Mon, 19 May 2003, Marco C. Leoni wrote: > Hi Patricio, > one question about the point below: > > > Let me include here another element before the submission of a > > query to the resource handling catalogues: The registry. > > > > Any registry will contain metadata about the services listed, ie, > > the catalogues. > > The registry would know (among other things), > > - catalogueName (possibly catalogueUniqueID) > > - catalogueTitle > > - catalogueKeywords > > - catalogueAuthor > > - number of columns > > - number of records > > - column names, UCDs, units > > - name ID,MAIN --- > > - RA POS_EQ_RA,MAIN h:m:s > > - Dec POS_EQ_DEC,MAIN d:m:s > > .... > > - Vmag PHOT_JHN_V mag > > - Bmag PHOT_JHN_B mag > > - z REDSHIFT --- > > > > are you sure the Registry will include all these information? > Perhaps "column names" and "units" will be resolved by the service > provider, and not by the registry itself. > > Cheers, > Marco Hi Marco, well, I would have thought so. It's done already by vizier meta-information tables (which could be considered a local registry) and surely by other services. It's a good point though, how much is a registry supposed to know? In the scheme that Keith Noddle presented in Cambridge, I would expect at least the local register (read service provider's) should know about about this. Whether the higher level registers decide to collect this information is to be seen, but if you ask *me*, I would say yes, they should keep this information. We are not talking about a huge data volume here; the advantages are large though, as you don't have to go everywhere with your query. I just had to deal with getting a mortgage and run from bank to bank filling up applications not knowing if I satisfied all the conditions they asked; then a consultant phoned us and we dealt with him, he found out who would lend us the money and it worked fine. The analogy seems quite appropriate for our situation in VO. An astronomer wants to formulate a general query, he or she has no idea where this could be done, so s/he asks a service to lauch the query urbe et orbi... Surely the data will come back to the astronomer, but if we apply a filtering system which can select the services which may give a positive answer (and weed off the ones with a negative), then the number of transactions diminishes and the response time is shorter. An intermediate solution would be to send the query to broker-services urbe et orbi, and let those services do the filtering and send the query to places which may give a positive answer. IMHO not using this meta-information would be a real waste. Cheers, Patricio --- Patricio F. Ortiz pfo@star.le.ac.uk AstroGrid project Department of Physics and Astronomy University of Leicester Tel: +44 (0)116 252 2015 LE1 7RH, UK From - Mon May 19 18:10:19 2003 X-UIDL: 3e5baf6500000a1e X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h4JGAGG1027567; Mon, 19 May 2003 18:10:16 +0200 (MEST) Received: from eso.org (nb008487.ads.eso.org [134.171.27.211]) by serapis.hq.eso.org (8.11.6+Sun/8.11.6) with ESMTP id h4JGAnL06056; Mon, 19 May 2003 18:10:49 +0200 (MEST) Message-ID: <3EC901E8.40307@eso.org> Date: Mon, 19 May 2003 18:10:16 +0200 From: "Marco C. Leoni" Reply-To: mleoni@eso.org Organization: Astrophysical Virtual Observatory @ESO User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.0.1) Gecko/20020823 Netscape/7.0 (CK-ESO) X-Accept-Language: en, en-us MIME-Version: 1.0 To: "Patricio F. Ortiz" CC: ucd@ivoa.net Subject: Re: MyUCDs & Registry References: Content-Type: multipart/alternative; boundary="------------080100070000060309030501" X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: --------------080100070000060309030501 Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit Patricio F. Ortiz wrote: >On Mon, 19 May 2003, Marco C. Leoni wrote: > > >>Hi Patricio, >> one question about the point below: >> >> >> >>> Let me include here another element before the submission of a >>> query to the resource handling catalogues: The registry. >>> >>> Any registry will contain metadata about the services listed, ie, >>> the catalogues. >>> The registry would know (among other things), >>> - catalogueName (possibly catalogueUniqueID) >>> - catalogueTitle >>> - catalogueKeywords >>> - catalogueAuthor >>> - number of columns >>> - number of records >>> - column names, UCDs, units >>> - name ID,MAIN --- >>> - RA POS_EQ_RA,MAIN h:m:s >>> - Dec POS_EQ_DEC,MAIN d:m:s >>> .... >>> - Vmag PHOT_JHN_V mag >>> - Bmag PHOT_JHN_B mag >>> - z REDSHIFT --- >>> >>> >>> >>are you sure the Registry will include all these information? >>Perhaps "column names" and "units" will be resolved by the service >>provider, and not by the registry itself. >> >>Cheers, >> Marco >> >> > >Hi Marco, > >well, I would have thought so. It's done already by vizier meta-information >tables (which could be considered a local registry) and surely by other >services. It's a good point though, how much is a registry supposed to >know? In the scheme that Keith Noddle presented in Cambridge, I would >expect at least the local register (read service provider's) should know >about about this. Whether the higher level registers decide to collect this >information is to be seen, but if you ask *me*, I would say yes, they >should keep this information. We are not talking about a huge data volume >here; the advantages are large though, as you don't have to go everywhere >with your query. > >I just had to deal with getting a mortgage and run from bank to bank >filling up applications not knowing if I satisfied all the conditions they >asked; then a consultant phoned us and we dealt with him, he found out >who would lend us the money and it worked fine. The analogy seems quite >appropriate for our situation in VO. An astronomer wants to formulate a >general query, he or she has no idea where this could be done, so s/he >asks a service to lauch the query urbe et orbi... Surely the data will >come back to the astronomer, but if we apply a filtering system which >can select the services which may give a positive answer (and weed off >the ones with a negative), then the number of transactions diminishes >and the response time is shorter. > >An intermediate solution would be to send the query to broker-services urbe >et orbi, and let those services do the filtering and send the query to >places which may give a positive answer. > >IMHO not using this meta-information would be a real waste. > >Cheers, > >Patricio > >--- >Patricio F. Ortiz pfo@star.le.ac.uk >AstroGrid project >Department of Physics and Astronomy >University of Leicester Tel: +44 (0)116 252 2015 >LE1 7RH, UK > Patricio, I agree that a filtering system would be nice, and in fact a registry is supposed to do that (in my opinion): if necessary it will send an "urbi et orbi" query and give back to the astronomer only the relevant results, where this means compare them with the original requirements (e.g. exclude all the "no info about it" answers). The same before sending the query, if the registry has enough information about services (this is not the case if we think of registries containing only references to other registries, but this will simply add one more level to the structure). What I meant before is that probably we need only UCDs in the registry without any unique column names: when the query reaches the service then it will be translated and UCDs mapped to comlumn names. - On the other side, if the user already knows the unique column name then using it will remove any control about UCDs. - Last possibility, giving both unique column name and UCD will create a well-defined detailed query, with specific result even in the "urbi et orbi" case. Cheers, Marco --------------080100070000060309030501 Content-Type: text/html; charset=us-ascii Content-Transfer-Encoding: 7bit

Patricio F. Ortiz wrote:
On Mon, 19 May 2003, Marco C. Leoni wrote:
  
Hi Patricio,
    one question about the point below:

    
	Let me include here another element before the submission of a
	query to the resource handling catalogues: The registry.

	Any registry will contain metadata about the services listed, ie,
	the catalogues.
	The registry would know (among other things),
		- catalogueName (possibly catalogueUniqueID)
		- catalogueTitle
		- catalogueKeywords
		- catalogueAuthor
		- number of columns
		- number of records
		- column names, UCDs, units
			- name	ID,MAIN	---
			- RA	POS_EQ_RA,MAIN	h:m:s
			- Dec	POS_EQ_DEC,MAIN d:m:s
			....
			- Vmag	PHOT_JHN_V	mag
			- Bmag	PHOT_JHN_B	mag
			- z	REDSHIFT	---

      
are you sure the Registry will include all these information?
Perhaps "column names" and "units" will be resolved by the service
provider, and not by the registry itself.

Cheers,
    Marco
    

Hi Marco,

well, I would have thought so. It's done already by vizier meta-information
tables (which could be considered a local registry) and surely by other
services. It's a good point though, how much is a registry supposed to
know? In the scheme that Keith Noddle presented in Cambridge, I would
expect at least the local register (read service provider's) should know
about about this. Whether the higher level registers decide to collect this
information is to be seen, but if you ask *me*, I would say yes, they
should keep this information. We are not talking about a huge data volume
here; the advantages are large though, as you don't have to go everywhere
with your query.

I just had to deal with getting a mortgage and run from bank to bank
filling up applications not knowing if I satisfied all the conditions they
asked; then a consultant phoned us and we dealt with him, he found out
who would lend us the money and it worked fine. The analogy seems quite
appropriate for our situation in VO. An astronomer wants to formulate a
general query, he or she has no idea where this could be done, so s/he
asks a service to lauch the query urbe et orbi... Surely the data will
come back to the astronomer, but if we apply a filtering system which
can select the services which may give a positive answer (and weed off
the ones with a negative), then the number of transactions diminishes
and the response time is shorter.

An intermediate solution would be to send the query to broker-services urbe
et orbi, and let those services do the filtering and send the query to
places which may give a positive answer.

IMHO not using this meta-information would be a real waste.

Cheers,

Patricio

---
Patricio F. Ortiz			pfo@star.le.ac.uk
AstroGrid project
Department of Physics and Astronomy
University of Leicester			Tel: +44 (0)116 252 2015
LE1 7RH, UK

Patricio,

    I agree that a filtering system would be nice, and in fact a registry is supposed to do that (in my opinion): if necessary it will send an "urbi et orbi" query and give back to the astronomer only the relevant results, where this means compare them with the original requirements (e.g. exclude all the "no info about it" answers). The same before sending the query, if the registry has enough information about services (this is not the case if we think of registries containing only references to other registries, but this will simply add one more level to the structure).

What I meant before is that probably we need only UCDs in the registry without any unique column names: when the query reaches the service then it will be translated and UCDs mapped to comlumn names.
- On the other side, if the user already knows the unique column name then using it will remove any control about UCDs.
- Last possibility, giving both unique column name and UCD will create a well-defined detailed query, with specific result even in the "urbi et orbi" case.


Cheers,
    Marco
--------------080100070000060309030501-- From - Mon May 19 18:45:18 2003 X-UIDL: 3e5baf6500000a21 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h4JGjAG1009232 for ; Mon, 19 May 2003 18:45:10 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h4JGj9q02594 for ; Mon, 19 May 2003 18:45:09 +0200 (MEST) Received: from queue4-win.server.ntlworld.com(62.253.162.224) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAveaidf; Mon, 19 May 03 18:45:08 +0200 Received: from brolga ([213.105.123.90]) by mta02-svc.ntlworld.com (InterMail vM.4.01.03.37 201-229-121-137-20020806) with ESMTP id <20030519151436.CZN9882.mta02-svc.ntlworld.com@brolga> for ; Mon, 19 May 2003 16:14:36 +0100 Reply-To: From: "Tony Linde" To: Subject: RE: MyUCDs Date: Mon, 19 May 2003 16:14:37 +0100 Organization: University of Leicester Message-ID: <003401c31e19$5c9d3c50$1001a8c0@brolga> MIME-Version: 1.0 Content-Type: text/plain; charset="US-ASCII" Content-Transfer-Encoding: 7bit X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook, Build 10.0.4510 In-Reply-To: <3EC8EECB.1000604@eso.org> X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 Importance: Normal X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: The Registry should answer the question 'what are the column names for resource X?', however that question might be phrased. Whether the registry retains that data for the resource or retrieves it from the resource itself when it is asked the question is entirely up to the registry builder. Cheers, Tony. > -----Original Message----- > From: Marco C. Leoni [mailto:mleoni@eso.org] > Sent: 19 May 2003 15:49 > To: Patricio F. Ortiz > Cc: ucd@ivoa.net > Subject: Re: MyUCDs > > > Hi Patricio, > one question about the point below: > > > Let me include here another element before the submission of a > > query to the resource handling catalogues: The registry. > > > > Any registry will contain metadata about the services > listed, ie, > > the catalogues. > > The registry would know (among other things), > > - catalogueName (possibly catalogueUniqueID) > > - catalogueTitle > > - catalogueKeywords > > - catalogueAuthor > > - number of columns > > - number of records > > - column names, UCDs, units > > - name ID,MAIN --- > > - RA POS_EQ_RA,MAIN h:m:s > > - Dec POS_EQ_DEC,MAIN d:m:s > > .... > > - Vmag PHOT_JHN_V mag > > - Bmag PHOT_JHN_B mag > > - z REDSHIFT --- > > > > are you sure the Registry will include all these information? > Perhaps "column names" and "units" will be resolved by the service > provider, and not by the registry itself. > > Cheers, > Marco > From - Mon May 19 19:30:18 2003 X-UIDL: 3e5baf6500000a26 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h4JHSvG1022323 for ; Mon, 19 May 2003 19:28:57 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h4JHSuY04361 for ; Mon, 19 May 2003 19:28:56 +0200 (MEST) Received: from mailsend.le.ac.uk(143.210.16.126) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAyDaGGi; Mon, 19 May 03 19:28:55 +0200 Received: from [143.210.36.58] (helo=mail.star.le.ac.uk) by artemis.le.ac.uk with smtp (Exim 4.14) id 19HoNn-0003Sb-Ld for ucd@ivoa.net; Mon, 19 May 2003 18:25:07 +0100 Received: (qmail 17349 invoked from network); 19 May 2003 17:25:28 -0000 Received: from sparky.star.le.ac.uk (143.210.36.10) by mail.star.le.ac.uk with SMTP; 19 May 2003 17:25:28 -0000 Date: Mon, 19 May 2003 18:25:28 +0100 (BST) From: "Patricio F. Ortiz" To: "Marco C. Leoni" cc: ucd@ivoa.net Subject: Re: MyUCDs & Registry In-Reply-To: <3EC901E8.40307@eso.org> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Spam-Score: (-------------------------) -25.3 X-Scanner: exiscan for exim4 *19HoNn-0003Sb-Ld*yTdAMBMeRx2* X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: On Mon, 19 May 2003, Marco C. Leoni wrote: > >Hi Marco, > > > >well, I would have thought so. It's done already by vizier meta-information > >tables (which could be considered a local registry) and surely by other > >services. It's a good point though, how much is a registry supposed to > >know? In the scheme that Keith Noddle presented in Cambridge, I would > >expect at least the local register (read service provider's) should know > >about about this. Whether the higher level registers decide to collect this > >information is to be seen, but if you ask *me*, I would say yes, they > >should keep this information. We are not talking about a huge data volume > >here; the advantages are large though, as you don't have to go everywhere > >with your query. > > > >I just had to deal with getting a mortgage and run from bank to bank > >filling up applications not knowing if I satisfied all the conditions they > >asked; then a consultant phoned us and we dealt with him, he found out > >who would lend us the money and it worked fine. The analogy seems quite > >appropriate for our situation in VO. An astronomer wants to formulate a > >general query, he or she has no idea where this could be done, so s/he > >asks a service to lauch the query urbe et orbi... Surely the data will > >come back to the astronomer, but if we apply a filtering system which > >can select the services which may give a positive answer (and weed off > >the ones with a negative), then the number of transactions diminishes > >and the response time is shorter. > > > >An intermediate solution would be to send the query to broker-services urbe > >et orbi, and let those services do the filtering and send the query to > >places which may give a positive answer. > > > >IMHO not using this meta-information would be a real waste. > > > >Cheers, > > > >Patricio > > > >--- > >Patricio F. Ortiz pfo@star.le.ac.uk > >AstroGrid project > >Department of Physics and Astronomy > >University of Leicester Tel: +44 (0)116 252 2015 > >LE1 7RH, UK > > > > Patricio, > > I agree that a filtering system would be nice, and in fact a > registry is supposed to do that (in my opinion): if necessary it will > send an "urbi et orbi" query and give back to the astronomer only the > relevant results, where this means compare them with the original > requirements (e.g. exclude all the "no info about it" answers). The same > before sending the query, if the registry has enough information about > services (this is not the case if we think of registries containing only > references to other registries, but this will simply add one more level > to the structure). > > What I meant before is that probably we need only UCDs in the registry > without any unique column names: when the query reaches the service then > it will be translated and UCDs mapped to comlumn names. I see your point now. However, remember that what's unique within a table is a column name, not UCDs, therefore, a UCD-driven request may expand to more columns than UCDs (just think of catalogues generated from sextractor) and generate columns which are absolutely meaningless for a user. > - On the other side, if the user already knows the unique column name > then using it will remove any control about UCDs. Unique name within a table, because names are not unique across tables and bear different meaning, the very reason UCDs were introduced. > - Last possibility, giving both unique column name and UCD will create a > well-defined detailed query, with specific result even in the "urbi et > orbi" case. True, but then we may start getting partial answers If I look for (colname=redshift, ucd=REDSHIFT) I would get those catalogues where redshift is called redshift but would live out cases like (colname=z, ucd=REDSHIFT). I think we should put together a list of questions and see what we need to solve them. I can see several families of questions, from the very specialized to the very broad, from the one where the user knows what resource to consult to the ones where the user wants to discover resources. Searching the metadata at any level can prove quite productive! I don't know about dropping the units from a registry (at any level). One problem in datamining is to make sure that one compares apples with apples, so if for instance, I want to compare the extension of galaxies it is important to know whether the units are in arcmin, degrees, arcsec or whatever. Say that I lauch a query where I request all data about galaxies around a particular location and I want to list ID, RA, DEC, diameter, maybe as a user I would like to force consulting catalogues which quote diameters in arcmin only. How do we do that? Alternatively, I could make it part of the query that I want the diameters expressed in arcmin regardless of how they are measured... Food for thought, I'll put some queries together and hopefully we can construct a bunch of cases to explore the needs. Cheers, Patricio --- Patricio F. Ortiz pfo@star.le.ac.uk AstroGrid project Department of Physics and Astronomy University of Leicester Tel: +44 (0)116 252 2015 LE1 7RH, UK From - Tue May 20 01:25:18 2003 X-UIDL: 3e5baf6500000a33 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h4JNNgSi007093 for ; Tue, 20 May 2003 01:23:42 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h4JNNeu19039 for ; Tue, 20 May 2003 01:23:41 +0200 (MEST) Received: from mail.cacr.caltech.edu(131.215.145.9) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAb_aqkL; Tue, 20 May 03 01:23:36 +0200 Received: from SARA (sara.cacr.caltech.edu [131.215.145.107]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.3) with ESMTP id h4JNIVdL020573 (version=TLSv1/SSLv3 cipher=RC4-MD5 bits=128 verify=NO) for ; Mon, 19 May 2003 16:18:31 -0700 Message-ID: <000901c31e5d$ef233680$6b91d783@cacr.caltech.edu> From: "Roy Williams" To: References: <200305181119.h4IBJOKF011031@urania.cfa.harvard.edu> Subject: Cambridge presentations Date: Mon, 19 May 2003 16:25:23 -0700 MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2720.3000 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2600.0000 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Dear UCD list The presentation of the UCD working group from Cambridge is at http://www.ivoa.net/internal/IVOA/IvoaUCD/Cambridge-ucd.ppt http://www.ivoa.net/internal/IVOA/IvoaUCD/Cambridge-ucd.pdf There is a new UCD Steering Committee (below) who will be implementing some of the recommendations in the above, with the objective of making a draft document available that the next IVOA meeting in October. Roy -------------------------- UCD Steering Committee: Sebastien Derriere, CDS, F Norman Gray, Starlink UK Jonathan McDowell, CfA, US Francois Ochsenbein, CDS, F Pedro Osuna, ESA, E Andrea Preite-Martinez, CDS, F Guy Rixon, Cambridge, UK Roy Williams, Caltech, US -------- Caltech Center for Advanced Computing Research roy@cacr.caltech.edu 626 395 3670 From - Tue May 20 01:30:18 2003 X-UIDL: 3e5baf6500000a34 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h4JNR0Si008089 for ; Tue, 20 May 2003 01:27:00 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h4JNR0V19182 for ; Tue, 20 May 2003 01:27:00 +0200 (MEST) Received: from ns1.u-strasbg.fr(130.79.200.1) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAZyaODL; Tue, 20 May 03 01:26:59 +0200 Received: from vizir.u-strasbg.fr (vizir.u-strasbg.fr [130.79.128.13]) by ns1.u-strasbg.fr (8.12.6p2/jtpda-5.4) with ESMTP id h4JNPhHT093359 for ; Tue, 20 May 2003 01:25:43 +0200 (CEST) Received: from vizier (localhost [127.0.0.1]) by vizir.u-strasbg.fr (8.11.6+Sun/8.9.1) with ESMTP id h4JNP0707168 for ; Tue, 20 May 2003 01:25:00 +0200 (MET DST) Message-Id: <200305192325.h4JNP0707168@vizir.u-strasbg.fr> To: ucd@ivoa.net Subject: Re: patricio UCD/Tony In-reply-to: Your message of Fri, 16 May 2003 16:00:33 +0200 (MEST) . Date: Tue, 20 May 2003 01:25:00 +0200 From: Francois Ochsenbein X-Antivirus: scanned by sophos at u-strasbg.fr X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Following Tony's post on "My understanding of UCDs", I would like to thank first Tony for his action -- it helps to clarify the discussions -- and I support Patricio's details. I would like to add a few more details: 1. UCDs as Data Types: yes, UCDs help to define what is a "legal" operation, but they do not replace the units. 2. UCDs as Keywords: Querying from UCDs to retrieve which resources do match a set of UCDs is one of the possible applications of the UCDs. For example, there is a version of VizieR which retrieves the catalogues containing a set of UCD at http://vizier.u-strasbg.fr/viz-bin/VizieR?-ucd Note that this URL does more than retrieving resources: it can retrieve directly the results by specifying e.g. PHOT_STR* in one of the UCD input specification, and a position on the sky, the search find those objects close to the position and which have a Stroemgren photometry. The UCDs allow more than just retrieving catalogues having this parameter: it allow to specify CONSTRAINTS on that UCD (Patricio's Scenario 2) something like Select ID, POS_EQ_RA_MAIN, POS_EQ_DEC_MAIN, REDSHIFT_HC From [all catalogues] Where REDSHIFT_HC > 3 PROVIDING that a rule is defined to specify what to do in case of multiple columns matching a UCD. The default rule could be something like for, say, the REDSHIFT_HC parameter: -> if a REDSHIFT_HC has a qualifier MAIN , use this one; -> otherwise, use the first non-null value of the possible REDSHIFT_HCs. The real advantage in using UCDs for actual queries is to be able to use GENERIC queries without having first to ask for the details of the catalogues (at the registry level or from the resource server). And when thousands of catalogues are involved, it makes a difference ! Notice also that the rule of the "first non-null" value is not that easy to write as an SQL statement... 3. UCDs as Pointers into Data Model I'm not sure to understand the problem -- why could not a DM point refer to a set of UCDs ? --Francois ================================================================================ Francois Ochsenbein ------ Observatoire Astronomique de Strasbourg 11, rue de l'Universite F-67000 STRASBOURG Phone: +33-(0)390 24 24 29 Email: francois@astro.u-strasbg.fr (France) Fax: +33-(0)390 24 24 32 ================================================================================ From - Tue May 20 09:40:19 2003 X-UIDL: 3e5baf6500000a48 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h4K7dfSi001858; Tue, 20 May 2003 09:39:41 +0200 (MEST) Received: from eso.org (nb008487.ads.eso.org [134.171.27.211]) by serapis.hq.eso.org (8.11.6+Sun/8.11.6) with ESMTP id h4K7eFL16938; Tue, 20 May 2003 09:40:15 +0200 (MEST) Message-ID: <3EC9DBBD.60703@eso.org> Date: Tue, 20 May 2003 09:39:41 +0200 From: "Marco C. Leoni" Reply-To: mleoni@eso.org Organization: Astrophysical Virtual Observatory @ESO User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.0.1) Gecko/20020823 Netscape/7.0 (CK-ESO) X-Accept-Language: en, en-us MIME-Version: 1.0 To: Roy Williams CC: ucd@ivoa.net Subject: Re: Cambridge presentations References: <200305181119.h4IBJOKF011031@urania.cfa.harvard.edu> <000901c31e5d$ef233680$6b91d783@cacr.caltech.edu> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Hi Roy, just one thing: could please add myself to the list? Thanks a lot! Cheers, Marco Roy Williams wrote: >Dear UCD list > >The presentation of the UCD working group from Cambridge is at >http://www.ivoa.net/internal/IVOA/IvoaUCD/Cambridge-ucd.ppt >http://www.ivoa.net/internal/IVOA/IvoaUCD/Cambridge-ucd.pdf > >There is a new UCD Steering Committee (below) who will be implementing some >of the recommendations in the above, with the objective of making a draft >document available that the next IVOA meeting in October. > >Roy >-------------------------- >UCD Steering Committee: >Sebastien Derriere, CDS, F >Norman Gray, Starlink UK >Jonathan McDowell, CfA, US >Francois Ochsenbein, CDS, F >Pedro Osuna, ESA, E >Andrea Preite-Martinez, CDS, F >Guy Rixon, Cambridge, UK >Roy Williams, Caltech, US > >-------- >Caltech Center for Advanced Computing Research >roy@cacr.caltech.edu >626 395 3670 > From - Tue May 20 11:05:18 2003 X-UIDL: 3e5baf6500000a4d X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h4K92VSi003205 for ; Tue, 20 May 2003 11:02:31 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h4K92Vt07434 for ; Tue, 20 May 2003 11:02:31 +0200 (MEST) Received: from mailsend.le.ac.uk(143.210.16.126) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAi4aiHo; Tue, 20 May 03 11:02:30 +0200 Received: from [143.210.36.58] (helo=mail.star.le.ac.uk) by artemis.le.ac.uk with smtp (Exim 4.14) id 19I2xI-0004SU-QS for ucd@ivoa.net; Tue, 20 May 2003 09:58:44 +0100 Received: (qmail 25314 invoked from network); 20 May 2003 08:59:06 -0000 Received: from brolga.star.le.ac.uk (HELO brolga) (143.210.36.204) by mail.star.le.ac.uk with SMTP; 20 May 2003 08:59:06 -0000 Reply-To: From: "Tony Linde" To: Subject: RE: patricio UCD/Tony Date: Tue, 20 May 2003 09:58:44 +0100 Organization: University of Leicester Message-ID: <007a01c31eae$04cf8ec0$1001a8c0@brolga> MIME-Version: 1.0 Content-Type: text/plain; charset="US-ASCII" X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook, Build 10.0.4510 In-Reply-To: <200305192325.h4JNP0707168@vizir.u-strasbg.fr> X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 Importance: Normal X-Spam-Score: (------) -6.5 X-Scanner: exiscan for exim4 *19I2xI-0004SU-QS*Pev1B1W/Wt2* X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id h4K92dSi003255 Status: > 1. UCDs as Data Types: > yes, UCDs help to define what is a "legal" operation, but they do not > replace the units. Agreed, but units are not sufficient to define legal operations. Just because two columns have units of 'time' does not mean they can necessarily be combined in any meaningful way. But two columns from different tables with POS_EQ_RA,MAIN can be compared with a meaningful result, even if each has different units. This is why I think that if UCDs are content descriptors, it makes sense to define rules about: which units are valid for a specific type of data; how one converts from one unit to another; which operations are valid on that data and on combinations of data with different UCDs and which UCDs result from those operations (eg POS* can be multiplied by FREQ* to get DENSITY - ridiculous but I'll let the astros come up with real examples). > Note that this URL does more than retrieving resources: it can > retrieve directly the results by specifying e.g. PHOT_STR* in one But this is not a *standard* Registry function. > PROVIDING that a rule is defined to specify what to do in case of > multiple columns matching a UCD. The default rule could be Therein lies the rub! > use GENERIC queries without having first to ask for the details of > the catalogues (at the registry level or from the resource server). But the Registry can determine which of the catalogues being searched have duplicate UCDs which are not easily resolvable and can then ask the user to pick the appropriate columns - even in a set of '000s of catalogues, this is likely to only be a small number (I hope!). > Notice also that the rule of the "first non-null" value is not > that easy to write as an SQL statement... It doesn't need to be easy. The dataset will receive a VOQL query and will translate UCDs in that to column names in a SQL query - it is in this translation that resolution of the correct column name will happen, not in the sql query. > 3. UCDs as Pointers into Data Model > I'm not sure to understand the problem -- why could not a DM point > refer to a set of UCDs ? One could have UCDs of CURRENCY, FLOAT and INTEGER all pointing to a DM entity of 'number'; this is not a problem but does indicate that perhaps the data model needs to be resolved to a lower level if UCDs exist for which there are no unique entities. Cheers, Tony. > -----Original Message----- > From: Francois Ochsenbein [mailto:francois@vizir.u-strasbg.fr] > Sent: 20 May 2003 00:25 > To: ucd@ivoa.net > Subject: Re: patricio UCD/Tony > > ... From - Mon May 19 19:20:18 2003 X-UIDL: 3e5baf6500000a24 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h4JHHhG1019109; Mon, 19 May 2003 19:17:43 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h4JHHhb03865; Mon, 19 May 2003 19:17:43 +0200 (MEST) Received: from mailhost.cacr.caltech.edu(131.215.145.180) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcCAA_GaGIh; Mon, 19 May 03 19:17:42 +0200 Received: from SARA (sara.cacr.caltech.edu [131.215.145.107]) by mailhost.cacr.caltech.edu (8.9.3/8.9.1) with SMTP id KAA27406; Mon, 19 May 2003 10:14:12 -0700 (PDT) Message-ID: <007701c31e2a$57c5b3e0$6b91d783@cacr.caltech.edu> From: "Roy Williams" To: , "Patricio F. Ortiz" Cc: , References: <3EC901E8.40307@eso.org> Subject: Re: MyUCDs & Registry Date: Mon, 19 May 2003 10:16:10 -0700 MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2720.3000 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2600.0000 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Patrick and Marco > are you sure the Registry will include all these information? > Perhaps "column names" and "units" will be resolved by > the service provider, and not by the registry itself. My understanding is that every registry entry is based on the Resource and Service Metadata (RSM) document (*). Everything in the registry has the basic stuff like title and publisher and description, also spectral and sky coverage. Then there are extension pieces, and so far we only have a good idea of extending to services. The metadata for these includes the URL, the mime type of what comes back, and other stuff that defines standard VO services (eg SIA, Cone etc). Whta is missing from the RSM is an extension that deal specifically with tables. It would include much of the VOTable header information I assume, including the UCDs. I think that now would be a good time to sketch an XML schema for catalog metadata. We already have curation and coverage from the Resource base, but then how is the extension document different from a VOTable header? Roy (*) http://www.ivoa.net/internal/IVOA/IvoaResReg/ResourceServiceMetadataV7.doc -------- Caltech Center for Advanced Computing Research roy@cacr.caltech.edu 626 395 3670 > Any registry will contain metadata about the services listed, ie, > the catalogues. > The registry would know (among other things), > - catalogueName (possibly catalogueUniqueID) > - catalogueTitle > - catalogueKeywords > - catalogueAuthor > - number of columns > - number of records > - column names, UCDs, units > - name ID,MAIN --- > - RA POS_EQ_RA,MAIN h:m:s > - Dec POS_EQ_DEC,MAIN d:m:s > .... > - Vmag PHOT_JHN_V mag > - Bmag PHOT_JHN_B mag > - z REDSHIFT --- > are you sure the Registry will include all these information? Perhaps "column names" and "units" will be resolved by the service provider, and not by the registry itself. Cheers, Marco From - Mon May 19 19:25:17 2003 X-UIDL: 3e5baf6500000a25 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h4JHPVG1021397; Mon, 19 May 2003 19:25:31 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h4JHPUL04206; Mon, 19 May 2003 19:25:30 +0200 (MEST) Received: from poplar.ncsa.uiuc.edu(141.142.65.122) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAA2faGni; Mon, 19 May 03 19:25:29 +0200 Received: from localhost (rplante@localhost) by poplar.ncsa.uiuc.edu (8.11.6/8.11.6) with ESMTP id h4JHOSO25675; Mon, 19 May 2003 12:24:28 -0500 Date: Mon, 19 May 2003 12:24:28 -0500 (CDT) From: Ray Plante Reply-To: Ray Plante To: ucd@ivoa.net cc: registry@ivoa.net Subject: Re: MyUCDs & Registry In-Reply-To: <3EC901E8.40307@eso.org> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Hi Guys, The current registry model allows for catalogs to be registered individually and that the descriptions stored in the registry could contain all the information that Patricio listed. The main question is how fine-grained you want the registry to be and, thus, whether catalogs are within your limit. I think we heard at the interop meeting last week sufficient interest in registering catalogs. So then the next step would be to model the catalog description, using the generic Resource metadata as a starting point. We would ask ourselves what additional information do we want in the description. Column UCDs and names would be an example of that type of information. I'll note that in our prototype schema for describing SIA services, we included a description of the columns returned by an image query. This was done using the VOTable FIELD elements; thus, it included both the local names and the UCDs (along with the IDs, type, and anything else you can stick in a FIELD element and its children). This could be done for a catalog description as well (regardless of whether it is actually available in VOTable format). hope this helps, Ray On Mon, 19 May 2003, Marco C. Leoni wrote: > > > Patricio F. Ortiz wrote: > > >On Mon, 19 May 2003, Marco C. Leoni wrote: > > > > > >>Hi Patricio, > >> one question about the point below: > >> > >> > >> > >>> Let me include here another element before the submission of a > >>> query to the resource handling catalogues: The registry. > >>> > >>> Any registry will contain metadata about the services listed, ie, > >>> the catalogues. > >>> The registry would know (among other things), > >>> - catalogueName (possibly catalogueUniqueID) > >>> - catalogueTitle > >>> - catalogueKeywords > >>> - catalogueAuthor > >>> - number of columns > >>> - number of records > >>> - column names, UCDs, units > >>> - name ID,MAIN --- > >>> - RA POS_EQ_RA,MAIN h:m:s > >>> - Dec POS_EQ_DEC,MAIN d:m:s > >>> .... > >>> - Vmag PHOT_JHN_V mag > >>> - Bmag PHOT_JHN_B mag > >>> - z REDSHIFT --- > >>> > >>> > >>> > >>are you sure the Registry will include all these information? > >>Perhaps "column names" and "units" will be resolved by the service > >>provider, and not by the registry itself. > >> > >>Cheers, > >> Marco > >> > >> > > > >Hi Marco, > > > >well, I would have thought so. It's done already by vizier meta-information > >tables (which could be considered a local registry) and surely by other > >services. It's a good point though, how much is a registry supposed to > >know? In the scheme that Keith Noddle presented in Cambridge, I would > >expect at least the local register (read service provider's) should know > >about about this. Whether the higher level registers decide to collect this > >information is to be seen, but if you ask *me*, I would say yes, they > >should keep this information. We are not talking about a huge data volume > >here; the advantages are large though, as you don't have to go everywhere > >with your query. > > > >I just had to deal with getting a mortgage and run from bank to bank > >filling up applications not knowing if I satisfied all the conditions they > >asked; then a consultant phoned us and we dealt with him, he found out > >who would lend us the money and it worked fine. The analogy seems quite > >appropriate for our situation in VO. An astronomer wants to formulate a > >general query, he or she has no idea where this could be done, so s/he > >asks a service to lauch the query urbe et orbi... Surely the data will > >come back to the astronomer, but if we apply a filtering system which > >can select the services which may give a positive answer (and weed off > >the ones with a negative), then the number of transactions diminishes > >and the response time is shorter. > > > >An intermediate solution would be to send the query to broker-services urbe > >et orbi, and let those services do the filtering and send the query to > >places which may give a positive answer. > > > >IMHO not using this meta-information would be a real waste. > > > >Cheers, > > > >Patricio > > > >--- > >Patricio F. Ortiz pfo@star.le.ac.uk > >AstroGrid project > >Department of Physics and Astronomy > >University of Leicester Tel: +44 (0)116 252 2015 > >LE1 7RH, UK > > > > Patricio, > > I agree that a filtering system would be nice, and in fact a > registry is supposed to do that (in my opinion): if necessary it will > send an "urbi et orbi" query and give back to the astronomer only the > relevant results, where this means compare them with the original > requirements (e.g. exclude all the "no info about it" answers). The same > before sending the query, if the registry has enough information about > services (this is not the case if we think of registries containing only > references to other registries, but this will simply add one more level > to the structure). > > What I meant before is that probably we need only UCDs in the registry > without any unique column names: when the query reaches the service then > it will be translated and UCDs mapped to comlumn names. > - On the other side, if the user already knows the unique column name > then using it will remove any control about UCDs. > - Last possibility, giving both unique column name and UCD will create a > well-defined detailed query, with specific result even in the "urbi et > orbi" case. > > > Cheers, > Marco > From - Mon May 19 19:45:18 2003 X-UIDL: 3e5baf6500000a27 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h4JHiiG1026963; Mon, 19 May 2003 19:44:44 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h4JHihU04903; Mon, 19 May 2003 19:44:43 +0200 (MEST) Received: from donner.stsci.edu(130.167.251.65) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAA7DaqKj; Mon, 19 May 03 19:44:42 +0200 Received: from JAZZY (jazzy.stsci.edu [130.167.250.43]) by donner.stsci.edu (Mirapoint Messaging Server MOS 3.3.3-GR) with ESMTP id AEH10707; Mon, 19 May 2003 13:43:23 -0400 (EDT) From: "Gretchen Greene" To: "'Ray Plante'" , Cc: Subject: RE: MyUCDs & Registry Date: Mon, 19 May 2003 13:43:23 -0400 Message-ID: <000a01c31e2e$25517490$2bfaa782@stsci.edu> MIME-Version: 1.0 Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 7bit X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook, Build 10.0.2627 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 Importance: Normal In-Reply-To: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: If the registry is going to supply 'Subject' , i.e. keywords for targeting specific astronomical topics, then I think it would equally serve to provide the UCDs and their associated tags (units, type, etc.) for refining queries. Not to sound harsh, my only question is why do we have to consider generating more schema files to do this? UCD's are fundamental descriptors in my mind and could be included in the base terms as optional elements. I guess the discretion comes from service providers with column descriptions not mapped into UCD's? -Gretchen -----Original Message----- From: Ray Plante [mailto:rplante@poplar.ncsa.uiuc.edu] Sent: Monday, May 19, 2003 1:24 PM To: ucd@ivoa.net Cc: registry@ivoa.net Subject: Re: MyUCDs & Registry Hi Guys, The current registry model allows for catalogs to be registered individually and that the descriptions stored in the registry could contain all the information that Patricio listed. The main question is how fine-grained you want the registry to be and, thus, whether catalogs are within your limit. I think we heard at the interop meeting last week sufficient interest in registering catalogs. So then the next step would be to model the catalog description, using the generic Resource metadata as a starting point. We would ask ourselves what additional information do we want in the description. Column UCDs and names would be an example of that type of information. I'll note that in our prototype schema for describing SIA services, we included a description of the columns returned by an image query. This was done using the VOTable FIELD elements; thus, it included both the local names and the UCDs (along with the IDs, type, and anything else you can stick in a FIELD element and its children). This could be done for a catalog description as well (regardless of whether it is actually available in VOTable format). hope this helps, Ray On Mon, 19 May 2003, Marco C. Leoni wrote: > > > Patricio F. Ortiz wrote: > > >On Mon, 19 May 2003, Marco C. Leoni wrote: > > > > > >>Hi Patricio, > >> one question about the point below: > >> > >> > >> > >>> Let me include here another element before the submission of a > >>> query to the resource handling catalogues: The registry. > >>> > >>> Any registry will contain metadata about the services listed, ie, > >>> the catalogues. > >>> The registry would know (among other things), > >>> - catalogueName (possibly catalogueUniqueID) > >>> - catalogueTitle > >>> - catalogueKeywords > >>> - catalogueAuthor > >>> - number of columns > >>> - number of records > >>> - column names, UCDs, units > >>> - name ID,MAIN --- > >>> - RA POS_EQ_RA,MAIN h:m:s > >>> - Dec POS_EQ_DEC,MAIN d:m:s > >>> .... > >>> - Vmag PHOT_JHN_V mag > >>> - Bmag PHOT_JHN_B mag > >>> - z REDSHIFT --- > >>> > >>> > >>> > >>are you sure the Registry will include all these information? > >>Perhaps "column names" and "units" will be resolved by the service > >>provider, and not by the registry itself. > >> > >>Cheers, > >> Marco > >> > >> > > > >Hi Marco, > > > >well, I would have thought so. It's done already by vizier meta-information > >tables (which could be considered a local registry) and surely by other > >services. It's a good point though, how much is a registry supposed to > >know? In the scheme that Keith Noddle presented in Cambridge, I would > >expect at least the local register (read service provider's) should know > >about about this. Whether the higher level registers decide to collect this > >information is to be seen, but if you ask *me*, I would say yes, they > >should keep this information. We are not talking about a huge data volume > >here; the advantages are large though, as you don't have to go everywhere > >with your query. > > > >I just had to deal with getting a mortgage and run from bank to bank > >filling up applications not knowing if I satisfied all the conditions they > >asked; then a consultant phoned us and we dealt with him, he found out > >who would lend us the money and it worked fine. The analogy seems quite > >appropriate for our situation in VO. An astronomer wants to formulate a > >general query, he or she has no idea where this could be done, so s/he > >asks a service to lauch the query urbe et orbi... Surely the data will > >come back to the astronomer, but if we apply a filtering system which > >can select the services which may give a positive answer (and weed off > >the ones with a negative), then the number of transactions diminishes > >and the response time is shorter. > > > >An intermediate solution would be to send the query to broker-services urbe > >et orbi, and let those services do the filtering and send the query to > >places which may give a positive answer. > > > >IMHO not using this meta-information would be a real waste. > > > >Cheers, > > > >Patricio > > > >--- > >Patricio F. Ortiz pfo@star.le.ac.uk > >AstroGrid project > >Department of Physics and Astronomy > >University of Leicester Tel: +44 (0)116 252 2015 > >LE1 7RH, UK > > > > Patricio, > > I agree that a filtering system would be nice, and in fact a > registry is supposed to do that (in my opinion): if necessary it will > send an "urbi et orbi" query and give back to the astronomer only the > relevant results, where this means compare them with the original > requirements (e.g. exclude all the "no info about it" answers). The same > before sending the query, if the registry has enough information about > services (this is not the case if we think of registries containing only > references to other registries, but this will simply add one more level > to the structure). > > What I meant before is that probably we need only UCDs in the registry > without any unique column names: when the query reaches the service then > it will be translated and UCDs mapped to comlumn names. > - On the other side, if the user already knows the unique column name > then using it will remove any control about UCDs. > - Last possibility, giving both unique column name and UCD will create a > well-defined detailed query, with specific result even in the "urbi et > orbi" case. > > > Cheers, > Marco > From - Mon May 19 20:45:18 2003 X-UIDL: 3e5baf6500000a29 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h4JIi1G1019875; Mon, 19 May 2003 20:44:01 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h4JIi1P07186; Mon, 19 May 2003 20:44:01 +0200 (MEST) Received: from poplar.ncsa.uiuc.edu(141.142.65.122) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAzjaico; Mon, 19 May 03 20:44:00 +0200 Received: from localhost (rplante@localhost) by poplar.ncsa.uiuc.edu (8.11.6/8.11.6) with ESMTP id h4JIgwK25771; Mon, 19 May 2003 13:42:58 -0500 Date: Mon, 19 May 2003 13:42:58 -0500 (CDT) From: Ray Plante Reply-To: Ray Plante To: Gretchen Greene cc: ucd@ivoa.net, Subject: RE: MyUCDs & Registry In-Reply-To: <000a01c31e2e$25517490$2bfaa782@stsci.edu> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Hi Gretchen, On Mon, 19 May 2003, Gretchen Greene wrote: > If the registry is going to supply 'Subject' , i.e. keywords for > targeting specific astronomical topics, then I think it would equally > serve to provide the UCDs and their associated tags (units, type, etc.) > for refining queries. > > Not to sound harsh, my only question is why do we have to consider > generating more schema files to do this? UCD's are fundamental > descriptors in my mind and could be included in the base terms as > optional elements. I guess the discretion comes from service providers > with column descriptions not mapped into UCD's? There is precedence for integrating it into the generic resource metadata: the current VOResource contains Coverage. However, it was pointed out last week that it is unclear, for example, what Coverage means when it applies to an organization. It was suggested (and I plan to look at this) that Coverage only be associated with descriptions of Data Collections and Services. I mention this because it illustrates a basic modeling issue. When UCDs are associated with a description of an SIA service, it can be made clear what the role the UCDs play in the service (i.e. these are the UCDs associated with the columns returned from an image query). Similarly, the connection is clear when made part of a Catalog description. However, if they are associated with a generic resource, their role is ambiguous. That is, what does it mean to search for Organizations based on UCDs? > my only question is why do we have to consider > generating more schema files to do this? Your question suggests that dealing with multiple schema files has additional overhead costs associated with it (as opposed to just have one schema). Do you see this as a problem? We put the metadata that is not purely generic Resource metadata into a separate schema because it makes for a friendlier extension mechanism. If we add new metadata that, say, specifically describes Catalogs into the VOResource schema, it affects all users of this schema regardless of whether they care about Catalogs. (They may have to change their software to cope with the new version.) However, if we put the metadata into its own schema that extends VOResource, it only affects those that want to describe Catalogs. cheers, Ray From - Mon May 19 21:25:18 2003 X-UIDL: 3e5baf6500000a2a X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h4JJLiG1007011; Mon, 19 May 2003 21:21:44 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h4JJLht09772; Mon, 19 May 2003 21:21:43 +0200 (MEST) Received: from donner.stsci.edu(130.167.251.65) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAA0Iayft; Mon, 19 May 03 21:21:42 +0200 Received: from JAZZY (jazzy.stsci.edu [130.167.250.43]) by donner.stsci.edu (Mirapoint Messaging Server MOS 3.3.3-GR) with ESMTP id AEH14116; Mon, 19 May 2003 15:21:40 -0400 (EDT) From: "Gretchen Greene" To: "'Ray Plante'" Cc: , Subject: RE: MyUCDs & Registry Date: Mon, 19 May 2003 15:21:40 -0400 Message-ID: <000c01c31e3b$dff0a660$2bfaa782@stsci.edu> MIME-Version: 1.0 Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 7bit X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook, Build 10.0.2627 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1106 Importance: Normal In-Reply-To: X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Thanks for the insights Ray, I realize I missed out on some discussions that occurred at the IVOA. Still, in building this first registry with the existing schemas, I am finding that there are subtleties to the implementation and my concern is in chasing down multiple schema versions and metadata definitions prohibits efficient prototyping. For example, the existing repositories (OAI, previous Cone registry, etc.) all have varying elements and content. Now which schema files to I pursue to bring about uniformity? This is only the very beginning. The other point is that there are not huge numbers of entries/resources yet in these registries (remember I'm used to the GSC2 billions) and so it seems a little odd to create a highly designed configuration before ever implementing one even though the design ideas are good ones. So...I cheer on the designing but encourage people to start working with the standard schemas/files and see how they interface before going too far. -Gretchen -----Original Message----- From: Ray Plante [mailto:rplante@poplar.ncsa.uiuc.edu] Sent: Monday, May 19, 2003 2:43 PM To: Gretchen Greene Cc: ucd@ivoa.net; registry@ivoa.net Subject: RE: MyUCDs & Registry Hi Gretchen, On Mon, 19 May 2003, Gretchen Greene wrote: > If the registry is going to supply 'Subject' , i.e. keywords for > targeting specific astronomical topics, then I think it would equally > serve to provide the UCDs and their associated tags (units, type, etc.) > for refining queries. > > Not to sound harsh, my only question is why do we have to consider > generating more schema files to do this? UCD's are fundamental > descriptors in my mind and could be included in the base terms as > optional elements. I guess the discretion comes from service providers > with column descriptions not mapped into UCD's? There is precedence for integrating it into the generic resource metadata: the current VOResource contains Coverage. However, it was pointed out last week that it is unclear, for example, what Coverage means when it applies to an organization. It was suggested (and I plan to look at this) that Coverage only be associated with descriptions of Data Collections and Services. I mention this because it illustrates a basic modeling issue. When UCDs are associated with a description of an SIA service, it can be made clear what the role the UCDs play in the service (i.e. these are the UCDs associated with the columns returned from an image query). Similarly, the connection is clear when made part of a Catalog description. However, if they are associated with a generic resource, their role is ambiguous. That is, what does it mean to search for Organizations based on UCDs? > my only question is why do we have to consider > generating more schema files to do this? Your question suggests that dealing with multiple schema files has additional overhead costs associated with it (as opposed to just have one schema). Do you see this as a problem? We put the metadata that is not purely generic Resource metadata into a separate schema because it makes for a friendlier extension mechanism. If we add new metadata that, say, specifically describes Catalogs into the VOResource schema, it affects all users of this schema regardless of whether they care about Catalogs. (They may have to change their software to cope with the new version.) However, if we put the metadata into its own schema that extends VOResource, it only affects those that want to describe Catalogs. cheers, Ray From - Mon May 19 21:45:17 2003 X-UIDL: 3e5baf6500000a2b X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h4JJi5G1017575; Mon, 19 May 2003 21:44:05 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h4JJi5Q10868; Mon, 19 May 2003 21:44:05 +0200 (MEST) Received: from cfa.harvard.edu(131.142.10.1) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAjeaaov; Mon, 19 May 03 21:44:04 +0200 Received: from xena.cfa.harvard.edu (xena [131.142.24.153]) by cfa.harvard.edu (8.9.2/8.9.2/cfunix Mast-Sol 0.5) with ESMTP id PAA20943; Mon, 19 May 2003 15:40:45 -0400 (EDT) Received: from cfa.harvard.edu (localhost [127.0.0.1]) by xena.cfa.harvard.edu (8.9.2/8.9.2/cfunix S 0.5) with ESMTP id PAA15728; Mon, 19 May 2003 15:40:44 -0400 (EDT) Sender: mink@cfa.harvard.edu Message-ID: <3EC9333C.CFC31104@cfa.harvard.edu> Date: Mon, 19 May 2003 15:40:44 -0400 From: Doug Mink X-Mailer: Mozilla 4.8 [en] (X11; U; SunOS 5.8 sun4u) X-Accept-Language: en MIME-Version: 1.0 CC: ucd@ivoa.net, registry@ivoa.net Subject: Re: MyUCDs & Registry References: <000c01c31e3b$dff0a660$2bfaa782@stsci.edu> Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Gretchen Greene wrote: > The other point is that there are not huge numbers of entries/resources > yet in these registries (remember I'm used to the GSC2 billions) and so > it seems a little odd to create a highly designed configuration before > ever implementing one even though the design ideas are good ones. At the Center for Astrophysics, we tried gathering descriptions of as many types of archived data as we could find hanging around here and tried to get knowledgeable people to describe them in a uniform way which we developed in parallel to the larger VO effort. We thought that working from the archives up could be complementary to the grand design work that many others were doing. We do not have a VO standard interface to the information we collected, but I think that the data could be translated into the protocols which are being discussed. We would be interested in what other people who have data they want to publish to the VO think about the parameters we have been able to collect. Check it out at http://tdc-www.harvard.edu/vo -Doug Mink From - Tue Apr 29 11:14:49 2003 X-UIDL: 3e5baf6500000743 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h3T9ELWg005633; Tue, 29 Apr 2003 11:14:21 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h3T9ELO20990; Tue, 29 Apr 2003 11:14:21 +0200 (MEST) Received: from newb6.u-strasbg.fr(130.79.128.16) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAMAaO_O; Tue, 29 Apr 03 11:14:20 +0200 Received: from astro.u-strasbg.fr (localhost [127.0.0.1]) by newb6.u-strasbg.fr (8.9.3/8.9.3) with ESMTP id LAA13552; Tue, 29 Apr 2003 11:12:28 +0200 (MET DST) Sender: derriere@newb6.u-strasbg.fr Message-ID: <3EAE41FB.E9DDB87E@astro.u-strasbg.fr> Date: Tue, 29 Apr 2003 11:12:27 +0200 From: Sebastien Derriere Organization: Observatoire de Strasbourg X-Mailer: Mozilla 4.7 [en] (X11; I; SunOS 5.6 sun4u) X-Accept-Language: en MIME-Version: 1.0 To: semantics@ivoa.net, ucd@ivoa.net Subject: ESSW03 paper accepted Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit X-MailScanner: Found to be clean by sophos at astro.u-strasbg.fr X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: Hello, The paper on UCDs that was submitted to the ESSW03 Workshop (E-Services and the Semantic Web) has been accepted! This Workshop is part of the 12th WWW conference held in Budapest this year (workshop on May 20). I have placed a copy of the paper on the Wiki Website: http://www.ivoa.net/twiki/bin/view/IVOA/IvoaUCD Sebastien. -- _______ / ~ /, Sebastien Derriere mailto:derriere@astro.u-strasbg.fr / ~~~~ // Observatoire de Strasbourg Phone +33 (0) 390 242 444 /______// 11, rue de l'universite Telefax +33 (0) 390 242 417 (______(/ F-67000 Strasbourg France From - Tue May 27 13:11:32 2003 X-UIDL: 3e5baf6500000bf5 X-Mozilla-Status: 0001 X-Mozilla-Status2: 10000000 Return-Path: Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h4R9uUKL019426; Tue, 27 May 2003 11:56:30 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h4R9uU300171; Tue, 27 May 2003 11:56:30 +0200 (MEST) Received: from ns1.u-strasbg.fr(130.79.200.1) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAuYaqva; Tue, 27 May 03 11:56:28 +0200 Received: from simbad.u-strasbg.fr (simbad.u-strasbg.fr [130.79.128.4]) by ns1.u-strasbg.fr (8.12.6p2/jtpda-5.4) with ESMTP id h4R9tDHT023439 ; Tue, 27 May 2003 11:55:13 +0200 (CEST) Received: from astro.u-strasbg.fr (zeltron.u-strasbg.fr [130.79.129.150]) by simbad.u-strasbg.fr (8.11.6+Sun/8.11.6) with ESMTP id h4R9xqR29741; Tue, 27 May 2003 11:59:57 +0200 (MEST) Message-ID: <3ED33720.8424CD86@astro.u-strasbg.fr> Date: Tue, 27 May 2003 12:00:00 +0200 From: Andre Schaaff Reply-To: schaaff@newb6.u-strasbg.fr Organization: CDS X-Mailer: Mozilla 4.79 [en] (Windows NT 5.0; U) X-Accept-Language: en MIME-Version: 1.0 To: "ws@ivoa.net" , grid@ivoa.net, ucd@ivoa.net Subject: New Web Service at CDS Content-Type: multipart/mixed; boundary="------------5B8B6C3FDB5EB8A463F8403D" X-Antivirus: scanned by sophos at u-strasbg.fr X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Status: This is a multi-part message in MIME format. --------------5B8B6C3FDB5EB8A463F8403D Content-Type: text/plain; charset=iso-8859-1 Content-Transfer-Encoding: quoted-printable X-MIME-Autoconverted: from 8bit to quoted-printable by ns1.u-strasbg.fr id h4R9tDHT023439 Hello, A UCD resolver is now available as a Web Service at CDS. See http://cdsweb.u-strasbg.fr/cdsws.gml for more details and an example of use. Regards, Andr=E9 --------------5B8B6C3FDB5EB8A463F8403D Content-Type: text/x-vcard; charset=us-ascii; name="schaaff.vcf" Content-Description: Card for Andre Schaaff Content-Disposition: attachment; filename="schaaff.vcf" Content-Transfer-Encoding: quoted-printable X-MIME-Autoconverted: from 8bit to quoted-printable by ns1.u-strasbg.fr id h4R9tDHT023439 begin:vcard=20 n:Schaaff;Andr=E9 x-mozilla-html:FALSE url:http://cdsweb.u-strasbg.fr org:Observatoire Astronomique;CDS adr:;;11, rue de l'Universit=E9;Strasbourg;;67000;France version:2.1 fn:Andr=E9 Schaaff end:vcard --------------5B8B6C3FDB5EB8A463F8403D-- From - Tue Jun 17 22:00:53 2003 X-UIDL: 3e5baf65000010eb X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h5HK1M1p009431 for ; Tue, 17 Jun 2003 22:01:22 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h5HK1LDS009428 for ucd-outgoing; Tue, 17 Jun 2003 22:01:21 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h5HK131p009328; Tue, 17 Jun 2003 22:01:03 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h5HK13222544; Tue, 17 Jun 2003 22:01:03 +0200 (MEST) Received: from mail.cacr.caltech.edu(131.215.145.9) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAkxaWbS; Tue, 17 Jun 03 22:01:02 +0200 Received: from SARA (sara.cacr.caltech.edu [131.215.145.107]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.6/8.12.6/Debian-7) with ESMTP id h5HK0YJ9012834 (version=TLSv1/SSLv3 cipher=RC4-MD5 bits=128 verify=NO); Tue, 17 Jun 2003 13:00:34 -0700 Message-ID: <02f601c3350b$83283ab0$6b91d783@cacr.caltech.edu> From: "Roy Williams" To: , Subject: UCD for SIAP Date: Tue, 17 Jun 2003 13:03:25 -0700 MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2720.3000 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2600.0000 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Roy Williams" Status: One of my actions as part of the UCD steering committee is to work with the "VOX" new UCDs that were created for the SIAP protocol. Below, I have listed all of the VOX UCDs that could find in the SIAP definition, with a little bit of the description. I have tried to find an equivalent in the standard UCD set, and in many cases was successful. For example is there a reason for VOX:Image_AccessReference as a new UCD, why can't we simply use DATA_LINK from the existing set? This is why it says "**existing: DATA_LINK" for that entry. Of course, there will a revision when we steel on the "base+modifier" scheme for UCD that we decided in Cambridge. Please can some of you look at the suggested equivalents fron the exisiting set, and the suggested new UCDs in the listing below? We gain interoperability from reusing and following the existing tree -- but do we lose anything? Thenk You Roy -------- Caltech Center for Advanced Computing Research roy@cacr.caltech.edu 626 395 3670 VOX:Image_Title ** existing: ID_IMAGE containing a short (usually one line) description of the image. VOX:Image_MJDateObs ** existing: TIME_DATE with datatype="double", representing the mean modified Julian date of the observation. VOX:Image_Naxes ** new: POS_TRANSF_WCS_NAXES specifying the number of image axes. VOX:Image_Naxis ** new: POS_TRANSF_WCS_NAXIS NOTE: Can a UCD refer to an array like this? with the array value giving the length in pixels of each image axis. VOX:Image_Scale ** new: POS_TRANSF_WCS_CDELT NOTE: Can a UCD refer to an array like this? with the array value giving the scale in degrees per pixel of each image axis. VOX:Image_Format ** new: DATA_TYPE_MIME specifying the MIME-type of the object associated with the image acref, e.g., image/fits", "text/html", and so forth. VOX:STC_CoordRefFrame ** existing: ID_FRAME representing the coordinate system reference frame, selected from "ICRS", "FK5", "FK4", "ECL", "GAL", and "SGAL". VOX:STC_CoordEquinox ** existing: TIME_EQUINOX representing the Equinox (not required for ICRS) of the coordinate system used for the image world coordinate system (WCS). VOX:WCS_CoordProjection ** new: POS_TRANSF_WCS_CTYPE with the array value being the three-character code ("TAN", "ARC", "SIN", etc.) VOX:WCS_CoordRefPixel ** new: POS_TRANSF_WCS_CRPIX with the array value specifying the image pixel coordinates of the WCS reference pixel. This is identical to "CRPIX" in FITS WCS. VOX:WCS_CoordRefValue ** new: POS_TRANSF_WCS_CRVAL with the array value specifying the world coordinates of the WCS reference pixel. This is identical to "CRVAL" in FITS WCS. VOX:WCS_CDMatrix ** new: POS_TRANSF_WCS_CD with the array (matrix) value specifying the WCS CD matrix. VOX:BandPass_ID ** existing: INST_FILTER_CODE identifying the bandpass by name (e.g., "V", "SDSS_U", "K", "K-Band", etc.). VOX:BandPass_Unit ** existing: UNITS -- but should be GROUPED with Bandpass identifying the units used to represent spectral values, selected from "meters", "hertz", and "keV". VOX:BandPass_RefValue ** new: INST_FILTER_REF specifying the characteristic (reference) frequency, wavelength, or energy for the bandpass model. VOX:BandPass_HiLimit ** new: INST_FILTER_MAX specifying the upper limit of the bandpass. VOX:BandPass_LoLimit ** new: INST_FILTER_MIN specifying the lower limit of the bandpass. VOX:Image_PixFlags ** existing: CODE_MISC specifying the type of processing done by the image service to produce an output image pixel. The string value should be formed from some combination of the following character codes: C, F, X, Z, V VOX:Image_AccessReference ** existing: DATA_LINK specifying the URL to be used to access or retrieve the image. VOX:Image_AccessRefTTL ** existing: TIME_DELAY specifying the minimum time to live in seconds of the access reference. VOX:Image_FileSize ** new: DATA_SIZE representing the actual or estimated size of the encoded image in bytes (not pixels!). From - Wed Jun 18 06:20:54 2003 X-UIDL: 3e5baf65000010f4 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h5I4J0SN029598 for ; Wed, 18 Jun 2003 06:19:00 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h5I4J000029597 for ucd-outgoing; Wed, 18 Jun 2003 06:19:00 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h5I4IuSN029584; Wed, 18 Jun 2003 06:18:56 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h5I4Iuh11893; Wed, 18 Jun 2003 06:18:56 +0200 (MEST) Received: from dns.noao.edu(140.252.1.54) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAWDaGox; Wed, 18 Jun 03 06:18:54 +0200 X-SpamCatcher-Score: 1 [X] Received: from [209.155.156.44] (account tody HELO lepus.tuc.noao.edu) by noao.edu (CommuniGate Pro SMTP 4.1b8) with ESMTP id 7753686; Tue, 17 Jun 2003 21:17:37 -0700 Date: Tue, 17 Jun 2003 22:17:36 -0600 (MDT) From: Doug Tody X-X-Sender: dtody@localhost.localdomain To: Roy Williams cc: ucd@ivoa.net, Subject: Re: UCD for SIAP In-Reply-To: <02f601c3350b$83283ab0$6b91d783@cacr.caltech.edu> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Doug Tody Status: Roy - Certainly we can replace the VOX: namespace UCDs with global UCDs, so long as we are willing to make up new UCDs where needed. This might be a good short-term solution. The key problem I see with trying to use existing UCDs is that historically UCDs have been used primarily as fuzzy tags to link similar fields in catalogs. In data access metadata such as is introduced in SIA we are using UCDs to identify the fields of a formal data model. Here the tag is not fuzzy at all, linking similar fields of unrelated catalogs, rather it is a link to a field of a formally defined data model. Precision is important for these data models - we are precisely defining attributes of the data model. We should formally define data models such as spectralBandpass or WCS and define, as part of the data model, the UCD tag used to identify an attribute of the data model. When we represent a data model as a set of related columns in a table, or as an entity struct in XML (as in IDHA or HDX), we will use the UCDs to formally type the data model attributes so that programs can use them unambiguously, so that we can use XML Schemas for automated validation, and so forth. This one-to-one mapping of UCDs to formal data models is a concept that does not currently exist in UCDs. If we try to take a more classical UCD-like approach and use UCDs to associate "similar" fields of different data models, then we no longer have a precisely defined data model. This association of "similar" fields of different data models should occur in the data model definitions, where data models may define attributes in terms of more fundamental data models or quantities. Some more specific comments based on your proposed UCDs. I haven't tried to be complete, these are only examples. > example is there a reason for VOX:Image_AccessReference as a new UCD, why > can't we simply use DATA_LINK from the existing set? This would work if we have only one DATA_LINK in an interface such as SIA, and we define that within this particular interface, DATA_LINK means the formally defined SIA Image_AccessReference. If for some reason we have two DATA_LINK attributes then we are in trouble, as the type is then overloaded and the meaning is ambiguous. The problem with what you suggest is that we are inherently overloading the type. It might work for a while, but will cause a problem in the future if we apply the same logic to a similar attribute. Since the attribute is precisely defined we gain nothing by using a fuzzy tag. > VOX:Image_Naxes > ** new: POS_TRANSF_WCS_NAXES > specifying the number of image axes. > > VOX:Image_Naxis > ** new: POS_TRANSF_WCS_NAXIS > NOTE: Can a UCD refer to an array like this? > with the array value giving the length in pixels of each image axis. This sort of mapping of the WCS data model onto "standard" UCDs (if newly defined) is certainly possible, so long as we define these tags as part of the WCS data model. However, the geometry of an image (NAXES, NAXIS) is not really part of the WCS - these are image attributes (in FITS they existed long before WCS). A WCS is associated with an image. CDELT, FRAME, etc., are part of the WCS. Do we need an image geometry data model? A general image attributes data model? NAXES, NAXIS are clearly (or shall we say, clearly should be) precisely defined terms of some formal image data model. > VOX:BandPass_ID > ** existing: INST_FILTER_CODE > identifying the bandpass by name (e.g., "V", "SDSS_U", "K", "K-Band", etc.). BandPass is a more general concept that "instrument" or "filter". Filters and instruments are examples of specific entities that have a bandpass. "bandpass" should be a formal data model with "bandpass"-specific attributes (UCDs). > VOX:BandPass_Unit > ** existing: UNITS -- but should be GROUPED with Bandpass > identifying the units used to represent spectral values, selected from > "meters", "hertz", and "keV". What do you do once there are two data models both of which need to define their units? GROUPED above, whatever that is, may address this, but it is better to have an explicit, unambiguous attribute. The units have to be precisely defined. The data model could define a default if this parameter is absent. > VOX:Image_PixFlags > ** existing: CODE_MISC > specifying the type of processing done by the image service to produce an > output image pixel. The string value should be formed from some > > combination of the following character codes: C, F, X, Z, V What do you do as soon as there are two fields with UCD=CODE_MISC in the metadata? In the current SIA, the implication is that Image_PixFlags is an attribute of some sort of "image" data model used in SIA, hence it has a precise definition. Similar comments apply to other UCDs where we confuse UCD associations with data model terms. I think it would help a lot if we just took one of these simple data models, e.g., spectralBandpass, and formally defined it, with UCDs assigned to identify attributes. Then we could use the same approach to define all the other SIA image attributes, grouped by data model. Later perhaps we can show how to define data models in terms of other data models or ultimately Quantities, to fully define complex data objects via a hierarchy of formal definitions. - Doug From - Fri Jun 20 17:35:58 2003 X-UIDL: 3e5baf6500001142 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h5KFZkN0029040 for ; Fri, 20 Jun 2003 17:35:46 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h5KFZkG1029039 for ucd-outgoing; Fri, 20 Jun 2003 17:35:46 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h5KFZdN0029002; Fri, 20 Jun 2003 17:35:39 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h5KFZc409244; Fri, 20 Jun 2003 17:35:38 +0200 (MEST) Received: from newb6.u-strasbg.fr(130.79.128.16) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAyQaWcs; Fri, 20 Jun 03 17:35:37 +0200 Received: from astro.u-strasbg.fr (localhost [127.0.0.1]) by newb6.u-strasbg.fr (8.9.3/8.9.3) with ESMTP id RAA16645; Fri, 20 Jun 2003 17:34:56 +0200 (MET DST) Message-ID: <3EF329A0.6B013D17@astro.u-strasbg.fr> Date: Fri, 20 Jun 2003 17:34:56 +0200 From: Sebastien Derriere Organization: Observatoire de Strasbourg X-Mailer: Mozilla 4.7 [en] (X11; I; SunOS 5.6 sun4u) X-Accept-Language: en MIME-Version: 1.0 To: Doug Tody CC: ucd@ivoa.net, dm@ivoa.net Subject: Re: UCD for SIAP References: Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit X-MailScanner: Found to be clean by sophos at astro.u-strasbg.fr X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Sebastien Derriere Status: Doug Tody wrote: > > The key problem I see with trying to use existing UCDs is that historically > UCDs have been used primarily as fuzzy tags to link similar fields in > catalogs. In data access metadata such as is introduced in SIA we are > using UCDs to identify the fields of a formal data model. Here the tag > is not fuzzy at all, linking similar fields of unrelated catalogs, rather > it is a link to a field of a formally defined data model. Precision is > important for these data models - we are precisely defining attributes > of the data model. > > We should formally define data models such as spectralBandpass or WCS > and define, as part of the data model, the UCD tag used to identify an > attribute of the data model. When we represent a data model as a set of > related columns in a table, or as an entity struct in XML (as in IDHA or > HDX), we will use the UCDs to formally type the data model attributes so > that programs can use them unambiguously, so that we can use XML Schemas > for automated validation, and so forth. Hello, The primary goal of UCDs is to ensure interoperability between heterogeneous datasets. That's why they have been defined to some "reasonable" level of precision (what you call fuzziness). Internal attributes of a formally defined data model can be defined at any level of precision, and have their own names. But you can have *in addition* a UCD attached to every attribute (see the case of the IDHA model). Those UCD can ensure interoperability between different data models, and between data models and datasets. The names of the attributes can not a priori ensure this task, because nothing prevents from having the same concept named differently in different models. Sebastien. -- _______ / ~ /, Sebastien Derriere mailto:derriere@astro.u-strasbg.fr / ~~~~ // Observatoire de Strasbourg Phone +33 (0) 390 242 444 /______// 11, rue de l'universite Telefax +33 (0) 390 242 417 (______(/ F-67000 Strasbourg France From - Fri Jun 20 20:55:58 2003 X-UIDL: 3e5baf650000114a X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h5KIteN0011971 for ; Fri, 20 Jun 2003 20:55:40 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h5KIteZR011970 for ucd-outgoing; Fri, 20 Jun 2003 20:55:40 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h5KItbN0011952; Fri, 20 Jun 2003 20:55:37 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h5KItaP19935; Fri, 20 Jun 2003 20:55:36 +0200 (MEST) Received: from nrao.edu(192.33.115.2) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAA_6aO7M; Fri, 20 Jun 03 20:55:35 +0200 Received: from polaris.cv.nrao.edu (polaris.cv.nrao.edu [192.33.115.101]) by cv3.cv.nrao.edu (8.11.6/8.11.6) with ESMTP id h5KItVP26707; Fri, 20 Jun 2003 14:55:31 -0400 Received: from oak (oak.aoc.nrao.edu [146.88.1.137]) by polaris.cv.nrao.edu (8.11.6/8.11.6) with ESMTP id h5KItUV29412; Fri, 20 Jun 2003 14:55:30 -0400 Date: Fri, 20 Jun 2003 12:55:29 -0600 (MDT) From: Doug Tody X-X-Sender: dtody@oak To: Sebastien Derriere cc: ucd@ivoa.net, , Subject: Re: UCD for SIAP In-Reply-To: <3EF329A0.6B013D17@astro.u-strasbg.fr> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-MailScanner: Found to be clean X-MailScanner-SpamCheck: not spam, SpamAssassin (score=-2.2, required 7, EMAIL_ATTRIBUTION, IN_REP_TO, SPAM_PHRASE_00_01, USER_AGENT_PINE) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Doug Tody Status: Sebastien - Good - we agree I think. This is exactly the point I was trying to make about data models and UCDs. The attributes of formal data models need to be defined precisely and unambiguously. The attributes of different data models need to be uniquely identified by some means, e.g., a globally unique name or reference (e.g., a form of UCD), a namespace (e.g., our temporary VOX namespace), or some hierarchical structure as in IDHA. The attributes of different data models, although they need to be distinguished from one another, may well share the same fundamental type, and a UCD could be used to express this. Using different approaches to naming data model attributes and types (UCDs), as I think you are suggesting below, is one way to solve the problem. This provides both the precision required to identify DM attributes, and the means to associate elements of different data models for interoperability. The only problem I see with this is that we would like flexibility in how we represent data models and metadata. Mapping DM attributes into the columns of a flat table, as in SIA or in a FITS header, is convenient and can simplify representations, up to a point. If datasets get complex enough then eventually one needs more structure and an approach such as IDHA or HDX may be called for. In many cases the simpler representation is adequate. It would be good if the underlying mechanisms, such as UCDs and how we define data models, were flexible enough to permit a variety of such representations. If we map the attributes of a DM into table columns and we do NOT use the UCD to identify the DM attribute, then we need another tag of some sort for this purpose. This would be no problem in XML, but we would have the nuisance of carrying along an additional tag separate from the UCD. In VOTable this would give us NAME, ID, UCD, plus a new tag for the formal DM attribute assocation (conceivably ID could be used for this purpose but it already has other uses). In a representation such as FITS, (e.g., if we try to represent VO data in FITS), then it is harder. In this case one might want to use the comment field of a FITS keyword to contain something like a UCD: keyword = value / UCD. I am not saying we necessarily want to do this, but it is an example of representation flexibility and it would be good if our scheme could extend to this level. If we DO use the UCD to carry this additional meaning, then the global UCD namespace could include both formal DM attribute names, and the more fundamental types used to associate different data elements as at present. UCDs would then provide a global naming index, with a single name (the UCD) being sufficient to carry all this meaning. Given the UCDs and an understanding of the associated DM (stored separately) we would then be able to recognize that different metadata elements (table columns in this case) are associated, define and use an XML schema to verify the integrity of the DM subset in these columns, use semantic relationships for inference, and so forth. In this case what we would do is use the UCD tag in a representation to convey the data model attribute name, uniquely identifying both the data model and the attribute of the data model. The formal definition of the DM would then define each attribute of the DM, ** giving for each attribute the UCD type of the attribute **. If this UCD type is elemental then we would have the desired interoperability, and the means to associate and compare similar data elements. UCDs would thus provide the metadata "glue" to link related concepts such as fundamental quantities and data models, making possible a uniform representation for both. To summarize, UCDs or something like them can play a key role to structure and link fundamental metadata and data models. The issue has already come up in interfaces like SIA and IDHA. Can we come up with something which is sufficiently powerful and general to provide both types of representations? - Doug On Fri, 20 Jun 2003, Sebastien Derriere wrote: > Doug Tody wrote: > > > > The key problem I see with trying to use existing UCDs is that historically > > UCDs have been used primarily as fuzzy tags to link similar fields in > > catalogs. In data access metadata such as is introduced in SIA we are > > using UCDs to identify the fields of a formal data model. Here the tag > > is not fuzzy at all, linking similar fields of unrelated catalogs, rather > > it is a link to a field of a formally defined data model. Precision is > > important for these data models - we are precisely defining attributes > > of the data model. > > > > We should formally define data models such as spectralBandpass or WCS > > and define, as part of the data model, the UCD tag used to identify an > > attribute of the data model. When we represent a data model as a set of > > related columns in a table, or as an entity struct in XML (as in IDHA or > > HDX), we will use the UCDs to formally type the data model attributes so > > that programs can use them unambiguously, so that we can use XML Schemas > > for automated validation, and so forth. > > Hello, > > The primary goal of UCDs is to ensure interoperability between > heterogeneous datasets. That's why they have been defined to some > "reasonable" level of precision (what you call fuzziness). > Internal attributes of a formally defined data model can be defined > at any level of precision, and have their own names. But you can > have *in addition* a UCD attached to every attribute (see the case > of the IDHA model). Those UCD can ensure interoperability between > different data models, and between data models and datasets. > The names of the attributes can not a priori ensure this task, > because nothing prevents from having the same concept named > differently in different models. > > Sebastien. From - Sat Jun 21 02:15:59 2003 X-UIDL: 3e5baf650000114e X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h5L0DNgt016944 for ; Sat, 21 Jun 2003 02:13:23 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h5L0DNQ6016943 for ucd-outgoing; Sat, 21 Jun 2003 02:13:23 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h5L0DIgt016922; Sat, 21 Jun 2003 02:13:18 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h5L0DIo01929; Sat, 21 Jun 2003 02:13:18 +0200 (MEST) Received: from email.noao.edu(140.252.1.54) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAANaaXd; Sat, 21 Jun 03 02:13:17 +0200 X-SpamCatcher-Score: 1 [X] Received: from [209.155.156.44] (account tody HELO lepus.tuc.noao.edu) by noao.edu (CommuniGate Pro SMTP 4.1b8) with ESMTP id 7787223; Fri, 20 Jun 2003 17:13:14 -0700 Date: Fri, 20 Jun 2003 18:13:10 -0600 (MDT) From: Doug Tody X-X-Sender: dtody@localhost.localdomain To: Roy Williams cc: ucd@ivoa.net, , IVOA Data Access Layer Subject: Re: UCD for SIAP In-Reply-To: <02f601c3350b$83283ab0$6b91d783@cacr.caltech.edu> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Doug Tody Status: Roy - I don't think we are actually very far apart on this. The main thing I am trying to do is determine how to deal with data models in DAL headers such as for SIA. An SIA contains two types of information all collected together in a flat votable: - Attributes which are part of the SIA interface (e.g., AccessReference). - Attributes which are part of formal data models which are mapped into the columns of the table, e.g., BandPass, WCS. The current SIA defines these as part of the interface but in principle what you see represents formally defined data models which are defined external to SIA. The SIA interface attributes could use standard UCDs (e.g., DATA_LINK) since the SIA interface is a controlled namespace and we can precisely defined what UCDs mean when present in an SIA votable. The data model attributes are something different. In general we might want to use any set of data models to define the attributes of a dataset described by a DAL service. A data model like BandPass or WCS should stand on its own, and be reusable in various contexts, e.g., any DAL service, or any VOTable (or VO-in-FITS) representation of a dataset. If we map the attributes of a data model into the columns of a VOtable (or the keywords of a FITS header) then the attributes need to be uniquely named so that they don't get confused with one another, so that we can verify data model integrity (no missing required attributes), and so forth. Some mechanism is needed to uniquely and unambiguously identify the attributes of a data model in such a context. It doesn't have to be the UCD, but this seems to be a natural extension of the UCD concept and usage. Your suggested UCDs for BandPass are close to what is needed, since they are basically direct one-to-one mappings of the data model attributes. We just need to go one step further and define a formal relationship between such UCDs and data model attributes. I went back and looked at your slides from the IVOA workshop again to see what I could learn. The summary slide goes like this: UCD is inherently fuzzy UCD is a description, not a unique name ... UCD will be eventually replaced by "pointers into data model" It seems to me this is exactly what we have been talking about. Conventional UCDs are fuzzy tags used to associate similar data elements. If we use a UCD to tag an attribute of a data model this UCD is a **pointer into a data model**. If we then go and look up the definition of this data model, it may state that the pointed-to DM attribute in turn has a UCD defining its "type", allowing it to be associated with other similar data elements in the more conventional UCD way. It is not clear if UCDs really need to be replaced by a new scheme providing pointers into data models - they come pretty close to this already. This is what SIA is trying to do; some such scheme is needed to represent data models in DAL protocols like SIA, even for these early versions. Well that's it for me for a while as I am about to leave on travel. I do think we are close to resolving this, and maybe even taking a step forward towards integrating data models and metadata via UCDs. We would like to do something more standard for these new "data model" UCDs in the upcoming DAL interfaces. - Doug On Tue, 17 Jun 2003, Roy Williams wrote: > One of my actions as part of the UCD steering committee is to work with the > "VOX" new UCDs that were created for the SIAP protocol. > > Below, I have listed all of the VOX UCDs that could find in the SIAP > definition, with a little bit of the description. I have tried to find an > equivalent in the standard UCD set, and in many cases was successful. For > example is there a reason for VOX:Image_AccessReference as a new UCD, why > can't we simply use DATA_LINK from the existing set? This is why it says > "**existing: DATA_LINK" for that entry. > > Of course, there will a revision when we steel on the "base+modifier" scheme > for UCD that we decided in Cambridge. > > Please can some of you look at the suggested equivalents fron the exisiting > set, and the suggested new UCDs in the listing below? We gain > interoperability from reusing and following the existing tree -- but do we > lose anything? > > Thenk You > Roy > > -------- > Caltech Center for Advanced Computing Research > roy@cacr.caltech.edu > 626 395 3670 > > VOX:Image_Title > ** existing: ID_IMAGE > containing a short (usually one line) description of the image. > > VOX:Image_MJDateObs > ** existing: TIME_DATE > with datatype="double", representing the mean modified Julian date of the > observation. > > VOX:Image_Naxes > ** new: POS_TRANSF_WCS_NAXES > specifying the number of image axes. > > VOX:Image_Naxis > ** new: POS_TRANSF_WCS_NAXIS > NOTE: Can a UCD refer to an array like this? > with the array value giving the length in pixels of each image axis. > > VOX:Image_Scale > ** new: POS_TRANSF_WCS_CDELT > NOTE: Can a UCD refer to an array like this? > with the array value giving the scale in degrees per pixel of each image > axis. > > VOX:Image_Format > ** new: DATA_TYPE_MIME > specifying the MIME-type of the object associated with the image acref, > e.g., image/fits", "text/html", and so forth. > > VOX:STC_CoordRefFrame > ** existing: ID_FRAME > representing the coordinate system reference frame, selected from "ICRS", > "FK5", "FK4", "ECL", "GAL", and "SGAL". > > VOX:STC_CoordEquinox > ** existing: TIME_EQUINOX > representing the Equinox (not required for ICRS) of the coordinate system > used for the image world coordinate system (WCS). > > VOX:WCS_CoordProjection > ** new: POS_TRANSF_WCS_CTYPE > with the array value being the three-character code ("TAN", "ARC", "SIN", > etc.) > > VOX:WCS_CoordRefPixel > ** new: POS_TRANSF_WCS_CRPIX > with the array value specifying the image pixel coordinates of the WCS > > reference pixel. This is identical to "CRPIX" in FITS WCS. > > VOX:WCS_CoordRefValue > ** new: POS_TRANSF_WCS_CRVAL > with the array value specifying the world coordinates of the WCS reference > pixel. This is identical to "CRVAL" in FITS WCS. > > VOX:WCS_CDMatrix > ** new: POS_TRANSF_WCS_CD > with the array (matrix) value specifying the WCS CD matrix. > > VOX:BandPass_ID > ** existing: INST_FILTER_CODE > identifying the bandpass by name (e.g., "V", "SDSS_U", "K", "K-Band", etc.). > > VOX:BandPass_Unit > ** existing: UNITS -- but should be GROUPED with Bandpass > identifying the units used to represent spectral values, selected from > "meters", "hertz", and "keV". > > VOX:BandPass_RefValue > ** new: INST_FILTER_REF > specifying the characteristic (reference) frequency, wavelength, or energy > for the bandpass model. > > VOX:BandPass_HiLimit > ** new: INST_FILTER_MAX > specifying the upper limit of the bandpass. > > VOX:BandPass_LoLimit > ** new: INST_FILTER_MIN > specifying the lower limit of the bandpass. > > VOX:Image_PixFlags > ** existing: CODE_MISC > specifying the type of processing done by the image service to produce an > output image pixel. The string value should be formed from some > > combination of the following character codes: C, F, X, Z, V > > VOX:Image_AccessReference > ** existing: DATA_LINK > specifying the URL to be used to access or retrieve the image. > > VOX:Image_AccessRefTTL > ** existing: TIME_DELAY > specifying the minimum time to live in seconds of the access reference. > > VOX:Image_FileSize > ** new: DATA_SIZE > representing the actual or estimated size of the encoded image in bytes (not > pixels!). > > From - Tue Jul 1 19:58:21 2003 X-UIDL: 3e5baf650000140e X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h61HssG0001166 for ; Tue, 1 Jul 2003 19:54:54 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h61HssYc001165 for ucd-outgoing; Tue, 1 Jul 2003 19:54:54 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h61HspG0001157 for ; Tue, 1 Jul 2003 19:54:51 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h61Hspu26959 for ; Tue, 1 Jul 2003 19:54:51 +0200 (MEST) Received: from sol.star.bris.ac.uk(137.222.58.39) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAACraWP0; Tue, 1 Jul 03 19:54:50 +0200 Received: from andromeda.star.bris.ac.uk ([137.222.58.155] ident=mail) by sol.star.bris.ac.uk with esmtp (Exim 3.35 #1) id 19XPL8-0007Cs-00 for ucd@ivoa.net; Tue, 01 Jul 2003 18:54:50 +0100 Received: from mbt (helo=localhost) by andromeda.star.bris.ac.uk with local-esmtp (Exim 3.16 #1) id 19XPL8-0000d7-00 for ucd@ivoa.net; Tue, 01 Jul 2003 18:54:50 +0100 Date: Tue, 1 Jul 2003 18:54:50 +0100 (BST) From: Mark Taylor X-X-Sender: mbt@andromeda.star.bris.ac.uk To: ucd@ivoa.net Subject: Re: New Web Service at CDS Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Mark Taylor Status: > A UCD resolver is now available as a Web Service at CDS. > See http://cdsweb.u-strasbg.fr/cdsws.gml for more details and an example > of use. Another web service which would be useful is provision of a list of all the currently-defined UCDs (with descriptions). TOPCAT, a table-editing tool I am developing, has cause to ask the user to select a UCD with which to label a column from a list of all known UCDs. I currently construct this list by screen-scraping the page at http://vizier.u-strasbg.fr/viz-bin/UCDs, which is downloaded and stored at build time. It could be good however to be able to retrieve and parse such a list at run time, so that recently-defined UCDs are available even when an old version of the tool is being used. I'm not a SOAP expert so I'm not sure what would be the best way to supply the result of such a query, but I guess it could be a simple XML document, perhaps reflecting the hierarchical nature of the list, something like: ... ... you get the idea. Even something as simple as a flat tab-separated list would be OK though, as long as the endpoint and format could be relied upon. Mark -- Mark Taylor Starlink Programmer Physics, Bristol University, UK m.b.taylor@bris.ac.uk 0117 928 8776 http://www.star.bris.ac.uk/~mbt/ From owner-ucd@eso.org Thu Jul 17 17:05:09 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h6HF4iCK029489 for ; Thu, 17 Jul 2003 17:04:44 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h6HF4iNj029488 for ucd-outgoing; Thu, 17 Jul 2003 17:04:44 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h6HF4ZCK029449 for ; Thu, 17 Jul 2003 17:04:36 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h6HF4ZO07890 for ; Thu, 17 Jul 2003 17:04:35 +0200 (MEST) Received: from ns1.u-strasbg.fr(130.79.200.1) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAApeaaAp; Thu, 17 Jul 03 17:04:34 +0200 Received: from simbad.u-strasbg.fr (simbad.u-strasbg.fr [130.79.128.4]) by ns1.u-strasbg.fr (8.12.9/jtpda-5.4) with ESMTP id h6HF4Vr7020843 ; Thu, 17 Jul 2003 17:04:31 +0200 (CEST) Received: from astro.u-strasbg.fr (titeuf.u-strasbg.fr [130.79.129.106]) by simbad.u-strasbg.fr (8.11.6+Sun/8.11.6) with ESMTP id h6HF9kr06084; Thu, 17 Jul 2003 17:09:46 +0200 (MEST) Message-ID: <3F16BAFC.52C3B543@astro.u-strasbg.fr> Date: Thu, 17 Jul 2003 17:04:28 +0200 From: Andre Schaaff Organization: CDS X-Mailer: Mozilla 4.79 [en] (Windows NT 5.0; U) X-Accept-Language: en,fr,fr-FR MIME-Version: 1.0 To: Mark Taylor CC: ucd@ivoa.net Subject: Re: New Web Service at CDS References: Content-Type: multipart/mixed; boundary="------------E46BBC4E363F638BD36AF9EF" X-Antivirus: scanned by sophos at u-strasbg.fr X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Andre Schaaff X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 This is a multi-part message in MIME format. --------------E46BBC4E363F638BD36AF9EF Content-Type: text/plain; charset=iso-8859-1 Content-Transfer-Encoding: quoted-printable X-MIME-Autoconverted: from 8bit to quoted-printable by ns1.u-strasbg.fr id h6HF4Vr7020843 Hello, I have implemented a Web Service which is near what you suggest. If you want to use a Web Service without special soap client, you can use= the useful following online tool : How to do it : replace just the default URL with the below URL and push t= he Retrieve button The URL to access to the Web Service : http://cdsws.u-strasbg.fr/axis/UCDList.jws?wsdl The online tool : http://www.soapclient.com/soaptest.html Regards, Andr=E9 P.S. : the online tool may not work with too old browsers Mark Taylor wrote: > > A UCD resolver is now available as a Web Service at CDS. > > See http://cdsweb.u-strasbg.fr/cdsws.gml for more details and an exam= ple > > of use. > > Another web service which would be useful is provision of a list of all > the currently-defined UCDs (with descriptions). > > TOPCAT, > a table-editing tool I am developing, has cause to ask the user to > select a UCD with which to label a column from a list of all known UCDs. > I currently construct this list by screen-scraping the page at > http://vizier.u-str= asbg.fr/viz-bin/UCDs, > which is downloaded and stored at build time. > It could be good however to be able to retrieve and parse such a list > at run time, so that recently-defined UCDs are available even when > an old version of the tool is being used. > > I'm not a SOAP expert so I'm not sure what would be the best way to > supply the result of such a query, but I guess it could be a simple > XML document, perhaps reflecting the hierarchical nature of the list, > something like: > > > > > > ... > > > > ... > > you get the idea. Even something as simple as a flat tab-separated lis= t > would be OK though, as long as the endpoint and format could be > relied upon. > > Mark > > -- > Mark Taylor Starlink Programmer Physics, Bristol University, UK > m.b.taylor@bris.ac.uk 0117 928 8776 http://www.star.bris.ac.uk/~mbt/ --------------E46BBC4E363F638BD36AF9EF Content-Type: text/x-vcard; charset=us-ascii; name="schaaff.vcf" Content-Description: Card for Andre Schaaff Content-Disposition: attachment; filename="schaaff.vcf" Content-Transfer-Encoding: quoted-printable X-MIME-Autoconverted: from 8bit to quoted-printable by ns1.u-strasbg.fr id h6HF4Vr7020843 begin:vcard=20 n:Schaaff;Andr=E9 x-mozilla-html:FALSE url:http://cdsweb.u-strasbg.fr org:Observatoire Astronomique;CDS adr:;;11, rue de l'Universit=E9;Strasbourg;;67000;France version:2.1 fn:Andr=E9 Schaaff end:vcard --------------E46BBC4E363F638BD36AF9EF-- From owner-ucd@eso.org Fri Oct 3 03:06:34 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9315krR008384 for ; Fri, 3 Oct 2003 03:05:46 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9315kbj008382 for ucd-outgoing; Fri, 3 Oct 2003 03:05:46 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from eso-wall-ext.hq.eso.org (firewall-user@eso-wall-int.hq.eso.org [134.171.68.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9315CrR008263 for ; Fri, 3 Oct 2003 03:05:12 +0200 (MEST) Received: (from uucp@localhost) by eso-wall-ext.hq.eso.org (8.10.2+Sun/8.10.2) id h9315CO24239 for ; Fri, 3 Oct 2003 03:05:12 +0200 (MEST) Received: from mail.cacr.caltech.edu(131.215.145.9) by eso-wall-ext.hq.eso.org via csmap (V6.0) id srcAAAE5aOvV; Fri, 3 Oct 03 03:05:11 +0200 Received: from SARA (sara.cacr.caltech.edu [131.215.145.107]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id h93159RJ026042 (version=TLSv1/SSLv3 cipher=RC4-MD5 bits=128 verify=NO) for ; Thu, 2 Oct 2003 18:05:09 -0700 Message-ID: <053601c3894b$08d03080$6b91d783@cacr.caltech.edu> From: "Roy Williams" To: Subject: UCD document 1.9.4 for IVOA Interop Date: Thu, 2 Oct 2003 18:09:45 -0700 MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2720.3000 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2727.1300 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Roy Williams" X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Welcome back to the UCD Forum at the IVOA. This message is to present the latest draft (1.9.4) of a paper that the UCD Steering Committee has been working on over the last few weeks (especially Derriere, Mann, McDowell, Ochsenbein, Osuna, and myself), and to request that you read it in preparation for the UCD session of the IVOA Interop meeting two weeks from today. This is the time to make your opinions known. Please try to generate edits to the document in the form of replacement paragraphs, addtional paragraphs or sentences. This will make your view much more likely to be incorporated than if you send comments or opinions. After your revisions, we would like the paper to be labelled version 2.0, placed into the IVOA standards process as a definition of the new UCD structure (known as UCD2). This new structure has much in common with what was discussed at the last Interop at Cambridge, but it has significant change, to bring the UCD in line with semantic web language. The idea from Cambridge (base+specifiers) has been replaced by (property+concepts). The document is here: http://www.ivoa.net/internal/IVOA/IvoaUCD/UCD-1.9.4.pdf The UCD Twiki is at: http://www.ivoa.net/twiki/bin/view/IVOA/IvoaUCD Thank You Roy Williams Chair, UCD Steering Committee -------- Caltech Center for Advanced Computing Research roy@cacr.caltech.edu 626 395 3670 From owner-ucd@eso.org Thu Oct 9 10:56:23 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h998tTpF026211 for ; Thu, 9 Oct 2003 10:55:29 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h998tSxZ026209 for ucd-outgoing; Thu, 9 Oct 2003 10:55:28 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h998skpF025995 for ; Thu, 9 Oct 2003 10:54:47 +0200 (MEST) Received: from kintyre.roe.ac.uk (kintyre.roe.ac.uk [195.194.120.72]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h998skCL010758 for ; Thu, 9 Oct 2003 10:54:46 +0200 (CEST) Received: from kintyre.roe.ac.uk (localhost [127.0.0.1]) by kintyre.roe.ac.uk (Postfix) with ESMTP id 430F646049 for ; Thu, 9 Oct 2003 09:54:46 +0100 (BST) Received: from somehost by kintyre.roe.ac.uk (postfixilter 1.3) with SMTP id 26438; Thu, 09 Oct 2003 09:54:46 +0100 (BST) Received: from kintyre.roe.ac.uk (localhost [127.0.0.1]) by localhost (Postfix) with ESMTP id B931D45F88 for ; Thu, 9 Oct 2003 09:54:45 +0100 (BST) Received: from relnx02.roe.ac.uk (relnx02.roe.ac.uk [195.194.120.138]) by kintyre.roe.ac.uk (Postfix) with ESMTP id 3563A4607C for ; Thu, 9 Oct 2003 09:54:45 +0100 (BST) Date: Thu, 9 Oct 2003 09:54:45 +0100 (BST) From: Bob Mann To: ucd@ivoa.net Subject: Re: UCD document 1.9.4 for IVOA Interop In-Reply-To: <053601c3894b$08d03080$6b91d783@cacr.caltech.edu> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Spam-Status: No, hits=0.0 required=1000.0 tests=none version=2.53 X-Spam-Level: X-Spam-Checker-Version: SpamAssassin 2.53 (1.174.2.15-2003-03-30-exp) X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Bob Mann X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi folks, I have only a few comments on v1.9.4 - I think it's a great improvement on the previous version, so Roy and Sebastien are to be congratulated. In particular, Section 3.1 is very clear and lays out the path to UCD3 very well. My first comment picks up something from the discussion leading up to this draft. It was said that we should emphasise that UCD2s are about discovering relevant data, not using them, as that requires more expressive power. If people still believe that, can a sentence to that effect be added in the introductory stuff?...it's in Section 4.1, of course, but I think that the restriction is important enough that it should come earlier, too. My next comment is just to check something. It seems that "data" has been dropped from the list of basic elements, and "metadata" has arrived. Am I right to assume that "metadata" is now the branch under which I will find the UCDs for recording provenance information? - e.g. versions of data reduction software used, names of astrometric catalogues, etc. If so, that's fine - it's just that that has to go somewhere. My final comment is my only real concern about this draft, which is whether the examples of Section 3.4 are too ambitious - especially the ones for the error on a right ascension of a galaxy. That seems to be introducing semantics by stealth, and without enough support - i.e. there seems to me to be too much structure in the relationships between those three quantities for UCD2. Maybe I missed it, but is there any semantic distinction to be made between the second and third terms in stat.error, pos.eq.ra, src.galaxy ? The third term relates to the second which relates to the third, so if I swap the order of the second and third the meaning is lost. On the other hand, I'm not sure that the example for photometric colour is good enough, since I don't see how to specify a generic flux ratio between two random passbands - I don't think it's good enough to enumerate the standard optical colours, since, when we federate multiwavelength datasets, I may well be interested in the ratio of a hard X-ray band flux and a K band magnitude, say. cheers Bob From owner-ucd@eso.org Thu Oct 16 04:16:23 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9G2BF0u020849 for ; Thu, 16 Oct 2003 04:11:15 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9G2BFEi020848 for ucd-outgoing; Thu, 16 Oct 2003 04:11:15 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9G2Ag0u020715 for ; Thu, 16 Oct 2003 04:10:42 +0200 (MEST) Received: from mail.cacr.caltech.edu (mail.cacr.caltech.edu [131.215.145.9]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9G2Aes3027742 for ; Thu, 16 Oct 2003 04:10:41 +0200 (CEST) Received: from Ropy (lugh.cacr.caltech.edu [131.215.145.183]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id h9G2AYM9024345 (version=TLSv1/SSLv3 cipher=RC4-MD5 bits=128 verify=NO) for ; Wed, 15 Oct 2003 19:10:38 -0700 Message-ID: <02b701c3938a$b2c2b2e0$e5c54f82@Ropy> From: "Roy Williams" To: Subject: Version 1.9.9 of UCD definition Date: Wed, 15 Oct 2003 19:07:57 -0700 MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Roy Williams" X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 There is a new version of the UCD specification document on the IVOA Twiki, labelled 1.9.9 in expectation of its promotion to version 2.0 at the IVOA interop meeting today in Strasbourg. The draft is available as pdf and MS word (links below). Please try to read this before the meeting today. Thank You Roy Williams http://www.ivoa.net/internal/IVOA/IvoaUCD/UCD-1.9.9.pdf http://www.ivoa.net/internal/IVOA/IvoaUCD/UCD-1.9.9.doc -------- Caltech Center for Advanced Computing Research roy@cacr.caltech.edu 626 395 3670 From owner-ucd@eso.org Mon Oct 20 19:34:00 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9KHTdMY028777 for ; Mon, 20 Oct 2003 19:29:39 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9KHTdAr028776 for ucd-outgoing; Mon, 20 Oct 2003 19:29:39 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9KHRiMa028113; Mon, 20 Oct 2003 19:28:30 +0200 (MEST) Received: from milkyway.gsfc.nasa.gov (lheapop.gsfc.nasa.gov [128.183.16.62]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9KE6VB1023398; Mon, 20 Oct 2003 16:06:33 +0200 (CEST) Received: from nasa.gov (lheapop [128.183.16.62]) by milkyway.gsfc.nasa.gov (8.12.9/8.12.9) with ESMTP id h9KE6PTd023177; Mon, 20 Oct 2003 10:06:26 -0400 Message-ID: <3F93EC05.8050108@nasa.gov> Date: Mon, 20 Oct 2003 10:07:01 -0400 From: Tom McGlynn User-Agent: Mozilla/5.0 (Windows; U; Win 9x 4.90; en-US; rv:1.4) Gecko/20030624 Netscape/7.1 (ax) X-Accept-Language: en-us, en MIME-Version: 1.0 To: martin hill CC: ucd@ivoa.net, dm@ivoa.net Subject: Re: UCDS vs DM - Peacekeeping References: <1066406745.3f90135915f9f@netmail.pipex.net> In-Reply-To: <1066406745.3f90135915f9f@netmail.pipex.net> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Tom McGlynn X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Martin, So far I've been a non-combatant in this war, but as you may know I had some reservations about the UCD2 framework presented at the interoperability meeting. Over the past two days I have been writing a revised proposal. This proposal includes a whole new discussion of the interaction between UCDs and table grouping constructs that I feel may play a major role in mediating among UCDs, data models and the DAL. I'll be publishing this within a day or two, but one key concept is the UCDTree which shows the UCDs of a table in a structured way. It is my hope that methods of abstract data models can be translated into actions on data by straightforward analysis of UCDTree. I expect to be send out the proposal today or tomorrow after I have a chance to check that what I've written during the flight back makes sense when I read it in a non-sleep-deprived state. Regards, Tom martin hill wrote: >I've been trying to sort out in my own head the differences between UCD2s and >data models. Particularly as one doesn't seem to work entirely without the >other. So donning my UN peacekeepers hat (which in the British case is a >tatty gardeners hat in a rather trendy camouflage, not a kevlar helmet): > >It strikes me that data models are about structure, and UCDs about describing >elements in that structure. > >Now it is probably possible that the way data models are defined could include >naming elements to define what they mean. I suggest that these should be (or >include as attributes) UCDs, at the very least so that we can compare data >items that have been formally modelled with those that haven't. > >For example, we can say (simplistically) that a coordinate is an RA, DEC, >error, and refers to some co-ordinate frame, and might look like this in XML: > > > > > 42 > 23 > > > 42 > 23 > > > > > 72.3 > 1 > > > etc > > >Now this is a horribly simple example (sorry about the mixed-up case >conventions) - how do people feel about it? It means that we should avoid >trying to describe structure/context in UCDs (which has the potential of >making them horribly long and complicated) and gives us an immediately useful >way of giving wider meaning to our data structures. > >It kind of implies that we then have a method for appending our UCDs up a data >model tree if we need to get more context for them. Thus we don't have to >have src.galaxy;phot.mag.ObscureOptical;error *as a defined UCD*. Instead >such strings are constructed out of individual UCDs as required by the program >that is investigating the data. > >It also means that UCDs don't have to be specific (which the UCD group are >avoiding cos it's a horrible task, small wonder) and yet I as a developer can >assemble specifics for doing cross comparisons. > >I've only had a pint and it still seems a good idea. It was a big pint though. > > > > From owner-ucd@eso.org Mon Oct 20 20:00:24 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9KHthMY005299 for ; Mon, 20 Oct 2003 19:55:43 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9KHtgdv005295 for ucd-outgoing; Mon, 20 Oct 2003 19:55:42 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9KHt8MY005129; Mon, 20 Oct 2003 19:55:08 +0200 (MEST) Received: from milkyway.gsfc.nasa.gov (lheapop.gsfc.nasa.gov [128.183.16.62]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9KHt6B1029112; Mon, 20 Oct 2003 19:55:07 +0200 (CEST) Received: from nasa.gov (lheapop [128.183.16.62]) by milkyway.gsfc.nasa.gov (8.12.9/8.12.9) with ESMTP id h9KHt2Td009395; Mon, 20 Oct 2003 13:55:02 -0400 Message-ID: <3F94219A.4050901@nasa.gov> Date: Mon, 20 Oct 2003 13:55:38 -0400 From: Tom McGlynn User-Agent: Mozilla/5.0 (Windows; U; Win 9x 4.90; en-US; rv:1.4) Gecko/20030624 Netscape/7.1 (ax) X-Accept-Language: en-us, en MIME-Version: 1.0 To: Tom McGlynn CC: martin hill , ucd@ivoa.net, dm@ivoa.net Subject: Re: UCDS vs DM - Peacekeeping References: <1066406745.3f90135915f9f@netmail.pipex.net> <3F93EC05.8050108@nasa.gov> In-Reply-To: <3F93EC05.8050108@nasa.gov> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Tom McGlynn X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 One thing I should have made clearer in the earlier message is that the revision I'm sending does not reflect any consensus on the correct approach. Rather it's a very detailed alternative to the approach presented by Roy at Strasbourg. It builds upon the same basic elements that Roy and Sebastien suggested but puts them together in -- for me at least -- a more coherent fashion. This approach does naturally lend itself to the concerns Martin raised, but it's certainly not a done deal. Tom Tom McGlynn wrote: > Over the > past two days I have been writing a revised proposal. > From owner-dm@eso.org Fri Oct 17 18:07:19 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9HG6Kwb007278 for ; Fri, 17 Oct 2003 18:06:20 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9HG6KAl007277 for dm-outgoing; Fri, 17 Oct 2003 18:06:20 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dm@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9HG5kwb007162; Fri, 17 Oct 2003 18:05:46 +0200 (MEST) Received: from nmail1.systems.pipex.net (nmail1.systems.pipex.net [62.241.160.130]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9HG5jB1027821; Fri, 17 Oct 2003 18:05:45 +0200 (CEST) Received: from nmail1.systems.pipex.net (localhost [127.0.0.1]) by nmail1.systems.pipex.net (8.12.10/8.12.10) with ESMTP id h9HG5jm7004682; Fri, 17 Oct 2003 17:05:45 +0100 Received: (from nobody@localhost) by nmail1.systems.pipex.net (8.12.10/8.12.10/Submit) id h9HG5jvO004681; Fri, 17 Oct 2003 17:05:45 +0100 Received: from 80.15.168.44 ( [80.15.168.44]) as user abm36@dial.pipex.com by netmail.pipex.net with HTTP; Fri, 17 Oct 2003 17:05:45 +0100 Message-ID: <1066406745.3f90135915f9f@netmail.pipex.net> Date: Fri, 17 Oct 2003 17:05:45 +0100 From: martin hill To: ucd@ivoa.net, dm@ivoa.net Subject: UCDS vs DM - Peacekeeping MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1 Content-Transfer-Encoding: 8bit User-Agent: PIPEX NetMail (IMP3.1) X-Originating-IP: 80.15.168.44 X-PIPEX-Username: abm36%dial.pipex.com X-Usage: PIPEX NetMail is subject to the standard PIPEX terms and conditions of use X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-dm@eso.org Precedence: bulk Reply-To: martin hill X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 I've been trying to sort out in my own head the differences between UCD2s and data models. Particularly as one doesn't seem to work entirely without the other. So donning my UN peacekeepers hat (which in the British case is a tatty gardeners hat in a rather trendy camouflage, not a kevlar helmet): It strikes me that data models are about structure, and UCDs about describing elements in that structure. Now it is probably possible that the way data models are defined could include naming elements to define what they mean. I suggest that these should be (or include as attributes) UCDs, at the very least so that we can compare data items that have been formally modelled with those that haven't. For example, we can say (simplistically) that a coordinate is an RA, DEC, error, and refers to some co-ordinate frame, and might look like this in XML: 42 23 42 23 72.3 1 etc Now this is a horribly simple example (sorry about the mixed-up case conventions) - how do people feel about it? It means that we should avoid trying to describe structure/context in UCDs (which has the potential of making them horribly long and complicated) and gives us an immediately useful way of giving wider meaning to our data structures. It kind of implies that we then have a method for appending our UCDs up a data model tree if we need to get more context for them. Thus we don't have to have src.galaxy;phot.mag.ObscureOptical;error *as a defined UCD*. Instead such strings are constructed out of individual UCDs as required by the program that is investigating the data. It also means that UCDs don't have to be specific (which the UCD group are avoiding cos it's a horrible task, small wonder) and yet I as a developer can assemble specifics for doing cross comparisons. I've only had a pint and it still seems a good idea. It was a big pint though. -- Martin Hill 07901 55 24 66 www.mchill.net From owner-dm@eso.org Tue Oct 21 11:00:10 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9L8pPPG013870 for ; Tue, 21 Oct 2003 10:51:25 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9L8pPYM013869 for dm-outgoing; Tue, 21 Oct 2003 10:51:25 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dm@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9L8odPG013522; Tue, 21 Oct 2003 10:50:39 +0200 (MEST) Received: from esacom51.vilspa.esa.int (esacom51-ext.vilspa.esa.int [192.171.2.19]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9L8ocB1014354; Tue, 21 Oct 2003 10:50:38 +0200 (CEST) Received: from iso.vilspa.esa.es (isous5.vilspa.esa.es [193.147.153.100]) by esacom51.vilspa.esa.int (8.12.9/8.12.9/ESA-External-v3.2) with ESMTP id h9L8oVaI003964; Tue, 21 Oct 2003 10:50:36 +0200 (MET DST) Received: from isou53 (isou53 [193.147.153.35]) by iso.vilspa.esa.es (8.12.10/8.12.10) with SMTP id h9L8oOBU000969; Tue, 21 Oct 2003 10:50:25 +0200 (MEST) Date: Tue, 21 Oct 2003 10:50:24 +0200 From: posuna@iso.vilspa.esa.es To: Tom McGlynn Cc: mchill@dial.pipex.com, ucd@ivoa.net, dm@ivoa.net Subject: UCDS and DM and "Catalogue" tables Message-Id: <20031021105024.0698fc07.posuna@iso.vilspa.esa.es> In-Reply-To: <3F94219A.4050901@nasa.gov> References: <1066406745.3f90135915f9f@netmail.pipex.net> <3F93EC05.8050108@nasa.gov> <3F94219A.4050901@nasa.gov> X-Mailer: Sylpheed version 0.9.2 (GTK+ 1.2.9; sparc-sun-solaris2.8) Mime-Version: 1.0 Content-Type: text/plain; charset=US-ASCII Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-dm@eso.org Precedence: bulk Reply-To: posuna@iso.vilspa.esa.es X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear all, the fact that I have been one of the authors of the UCD2 draft document (as a member of the UCD steering committee) made it very bizarre that I "voted" for the UCD1 option, together with other very few people. I think that if we use a Data Model to access metadata, then it is enough with the UCD1 that was created at the beginning. For me, there is no need to have more specificity, neither is there a need for matching functions and other more complex syntactical operations to be performed with the UCDs. For me, all that should be done through the Data Model and/or proper VOQL language. However, I do appreciate that many providers do have their data in the form of catalogues (what I normally call 2D tables, or X-Y tables, as catalogue, for me, can be several different things). I understand that people having data in X-Y tables do NOT want to hear about data models: they only want to be able to perform operations with the columns of their tables. It is in that context (X-Y table handling) where I believe the need of an overall complex UCD structure appears, as any comparison operation (or more complex ones as addition, substraction, ...) they want to do it by comparing (or adding/substracting/...) directly the columns. As the UCD2 is just adding more capabilities to the UCD1 without chopping off any of the existing ones, and as we ("Data Model" oriented ones) can always use the UCDs in the limited way we want them (i.e., just to describe the metadata we give back so that they are "Universally" understandable) I see no reason to stop the UCD2 to include more syntactical and operational capabilities: people "Data-Model oriented" will make use of very limited UCD capabilities (as they don't need them) and people "X-Y Table" oriented will make use of as many UCD "functionalities" as possible. In summary, I'm OK with new funtionalities of the UCDs but I guess I'll do a very limited use of them in the case that I use the Data Model to access my data, and hence my vote for the UCD1 "paradigm". Maybe the UCD document should reflect two main "Areas of Interest", something like: - Simple UCD handling: Data Model access - Complex UCD handling: Syntactical operations on X-Y (catalogue) table columns I wait for your comments... Cheers, Pedro. On Mon, 20 Oct 2003 13:55:38 -0400 Tom McGlynn wrote: > > One thing I should have made clearer in the earlier message is that > the revision I'm sending > does not reflect any consensus on the correct approach. Rather it's a > > very detailed alternative to the > approach presented by Roy at Strasbourg. It builds upon the same > basic elements that Roy and Sebastien suggested but puts them > together in -- for me at least -- > a more coherent fashion. This approach does naturally lend itself > to the concerns Martin raised, but > it's certainly not a done deal. > > Tom > > Tom McGlynn wrote: > > > Over the > > past two days I have been writing a revised proposal. > > > -- Pedro Osuna Alcalaya SOFTWARE Development Group XMM-Newton Science Archive e-mail: Pedro.Osuna@esa.int Tel + 34 91 8131314 European Space Agency VILLAFRANCA Satellites Tracking Station P.O. Box 50727 E-28080 Villafranca del Castillo MADRID - SPAIN From owner-ucd@eso.org Tue Oct 21 11:20:44 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9L9FxPG021264 for ; Tue, 21 Oct 2003 11:15:59 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9L9FxbH021263 for ucd-outgoing; Tue, 21 Oct 2003 11:15:59 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9L9FMPG021109 for ; Tue, 21 Oct 2003 11:15:22 +0200 (MEST) Received: from artemis.le.ac.uk (ntp2c.le.ac.uk [143.210.16.126]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9L9FLs3026322 for ; Tue, 21 Oct 2003 11:15:21 +0200 (CEST) Received: from [143.210.36.58] (helo=mail.star.le.ac.uk) by artemis.le.ac.uk with smtp (Exim 4.24) id 1ABsbo-00044f-JZ for ucd@ivoa.net; Tue, 21 Oct 2003 10:15:20 +0100 Received: (qmail 7397 invoked from network); 21 Oct 2003 09:15:35 -0000 Received: from peneca.star.le.ac.uk (143.210.36.224) by mail.star.le.ac.uk with SMTP; 21 Oct 2003 09:15:35 -0000 Date: Tue, 21 Oct 2003 10:15:35 +0100 (BST) From: Clive Page To: ucd@ivoa.net, Subject: Re: UCDS and DM and "Catalogue" tables In-Reply-To: <20031021105024.0698fc07.posuna@iso.vilspa.esa.es> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Clive Page X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 On Tue, 21 Oct 2003 posuna@iso.vilspa.esa.es wrote: > I understand that people having data in X-Y tables do NOT want to hear > about data models: they only want to be able to perform operations with > the columns of their tables. I'm not sure that's entirely true. I think the problem is that three partially overlapping groups of people have been trying over several years to make sense of astronomical data, so they canclassify or organise it to make data access simpler and more uniform. (1) Those devising UCDs, which started out exclusively for tables in VizieR. I think it is now generally agreed that some hierarchical scheme should replace the original flat namespace (though designed with components which split naturally into layers). (2) Those devising Data Models. The problem for those outside this effort is that there have been so many data models, different in structure and detail, but all apparently equally valid. I didn't manage to attend the DM sesssion in Strasbourg, but am pleased to hear of serious convergence. (3) Those devising query languages and data access routines, who need some DM or UCD scheme to do the job properly, except for the serious problem that a UCD does not lead to a unique column in some (many?) tables. I thought that Tom's ideas at Strasbourg sounded good, and look forward to seeing his proposal in print. If it's true that there is now a single agreed Data Model, does that not suggest that UCDs should be assigned on the same hierarchical basis? -- Clive Page Dept of Physics & Astronomy, University of Leicester, Tel +44 116 252 3551 Leicester, LE1 7RH, U.K. Fax +44 116 252 3311 From owner-ucd@eso.org Tue Oct 21 13:13:22 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9LB94PG025206 for ; Tue, 21 Oct 2003 13:09:04 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9LB94ZH025204 for ucd-outgoing; Tue, 21 Oct 2003 13:09:04 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9LB7vPG024866; Tue, 21 Oct 2003 13:07:57 +0200 (MEST) Received: from curlew.cs.man.ac.uk (curlew.cs.man.ac.uk [130.88.13.7]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9LB7uB1017318; Tue, 21 Oct 2003 13:07:56 +0200 (CEST) Received: from star1.jb.man.ac.uk ([130.88.24.176]) by curlew.cs.man.ac.uk with esmtp (Exim 4.20) id 1ABuMm-0004CH-A8; Tue, 21 Oct 2003 12:07:56 +0100 Received: from [130.88.24.80] (helo=aten) by star1.jb.man.ac.uk with esmtp (Exim 3.03 #2) id 1ABuMj-0001yn-00; Tue, 21 Oct 2003 12:07:53 +0100 Date: Tue, 21 Oct 2003 12:08:57 +0100 (BST) From: Anita Richards X-X-Sender: amsr@aten To: ucd@ivoa.net, registry@ivoa.net Subject: Re: Version 1.9.9 of UCD definition Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanner: exiscan for exim4 (http://duncanthrax.net/exiscan/) *1ABuMm-0004CH-A8*dRZHQ.Wg9ns* X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Anita Richards X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 At the interoperability workshop following ADASS, there was some mention of contradictions between the spectral divisions in the UCD2 document and the groupings in RM v0.82. There was also debate about whether and where an mm or sub-mm band should be introduced in RMv0.82. I think that consistency between UCD2 and the RM (whatever is the stable outcome for defining the Registry) would be very useful but in fact the discrepancies are minor. Personally, I hope that we do not spend much time discussing the exact divisions as we cannot avoid splitting the coverage of some present instruments, let alone future ones. However it might be sensible to be guided by the current/immediate future major observatories. Perhaps the responses to the SSA / spectral data model questionnaire might help. These are my suggestions: The boundaries of the spectral UCD2s are consistent with fitting into the RM categories with minor changes: Some of the UCD2 frequency ranges at the high freq end of IR have become transposed (I think - it is indeed hard to think in 3 sets of units!) I apologise for having created confusion over the new mm band in RMv0.82. The proposed range of ALMA is 30 - 900 GHz according to the web page. In fact, I understand that initially the lower limit is more like 86 GHz. Therefore I suggest that consistency can be achieved by having instead: SUBMM 100 micron - 3 mm (100 - 3000 GHz) The RMv0.82 x-ray regime goes from 0.12 - 120 keV; the UCD2 regime goes from 0.12 - 12 keV Accoding to their web pages, CHANDRA covers 0.1 - 10 keV (I have also been told 0.12 - 12...) and XMM covers 0.15 - 15 keV; ROSAT was within this. The CRO covered > 30 keV and SWIFT, 15 - 150 keV Thus, to keep the 'decades', this seems more suitable: XRAY 0.12 - 12 keV (as per UCD2) GAMMARAY > 12 keV but maybe a high energy astronomer can advise.... OVERLAPPING DATA Suppose that I have a catalogue with data taken around 1 micron. I hope I am right in thinking that the Registry entry can contaiin both Optical and IR as values of the relevant spectral coverage keyword, and this is used OK in searches etc. How will the UCDs be used? As I understand it, in order to use Vizier or the Aladin SED tool to search for e.g. radio observations between 1.3 and 1.7 GHz (radio L-band), the software would look for UCDs em.radio.750-1500MHz and em.radio.1.5-3GHz. However there may be catalogues giving radio observations or flux densities between 1.4 and 1.7 GHz. This might or might not give the exact observing frequency, but for many purposes the general flux density or image would be useful. As I understand it, this would simply have the UCD em.radio and would not be found. This is _not_ a plea to divide the ranges differently, but a reflection of the fact that we are no longer restricted to observing in well-defined filters. Broad-band receivers and optical fibres in the radio, ALMA, space observatories etc. mean that we observe at all frequencies seamlessly, and sensitivity to higher redshifts means that lines no longer fall even in a single regime. Maybe there is a solution already. If not, the only satisfactory things I can see are to do one of the following: * allow bracketting UCDs e.g. em.radio.0.75-3GHz * allow two (or more) UCDs to a column, where these are adjacent (up to a sensible max) * not use the fine divisions in UCDs, but treat frequency like position and treat every query as a 1D cone search, ie a linear segment search. cheers a - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - Dr. Anita M. S. Richards, AVO Astronomer MERLIN/VLBI National Facility, University of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire SK11 9DL, U.K. tel +44 (0)1477 572683 (direct); 571321 (switchboard); 571618 (fax). From - Tue Oct 21 13:19:10 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9LAfnPG017608 for ; Tue, 21 Oct 2003 12:41:49 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9LAfnkN017607 for dm-outgoing; Tue, 21 Oct 2003 12:41:49 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dm@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9LAefPG017365; Tue, 21 Oct 2003 12:40:41 +0200 (MEST) Received: from newb6.u-strasbg.fr (newb6.u-strasbg.fr [130.79.128.16]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9LAefB1016732; Tue, 21 Oct 2003 12:40:41 +0200 (CEST) Received: from astro.u-strasbg.fr (localhost [127.0.0.1]) by newb6.u-strasbg.fr (8.9.3/8.9.3) with ESMTP id MAA26307; Tue, 21 Oct 2003 12:40:21 +0200 (MET DST) Message-ID: <3F950D15.AEDBC59C@astro.u-strasbg.fr> Date: Tue, 21 Oct 2003 12:40:21 +0200 From: Sebastien Derriere Organization: Observatoire de Strasbourg X-Mailer: Mozilla 4.7 [en] (X11; I; SunOS 5.6 sun4u) X-Accept-Language: en MIME-Version: 1.0 To: martin hill CC: ucd@ivoa.net, dm@ivoa.net Subject: Re: UCDS vs DM - Peacekeeping References: <1066406745.3f90135915f9f@netmail.pipex.net> Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit X-MailScanner: Found to be clean by sophos at astro.u-strasbg.fr X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-dm@eso.org Precedence: bulk Reply-To: Sebastien Derriere Status: X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 X-UIDL: 3f68a56400000021 martin hill wrote: > > It strikes me that data models are about structure, and UCDs about describing > elements in that structure. > > Now it is probably possible that the way data models are defined could include > naming elements to define what they mean. I suggest that these should be (or > include as attributes) UCDs, at the very least so that we can compare data > items that have been formally modelled with those that haven't. This kind of work has been done in the case of the IDHA model: trying to find a relevant UCD for the different model elements. But I don't think that we should impose every element of every data model to be associated to a UCD. In fact, the link between UCD and DM can exist in both directions: - there can be a 'ucd' attribute for elements of data model, to indicate the corresponding UCD - the 'utype' attribute in VOTable allows to give a link to some data model element In the first approach, people building the data model make the effort to associate UCD to their view. The second approach can be used when there are no ucd attribute in the DM, to link the description of a dataset to a DM. Of course, both are not exclusive: there can be a ucd attribute in the DM, AND a utype for a or that would point, hopefully, to the same element of the DM ! Sebastien. -- _______ / ~ /, Sebastien Derriere mailto:derriere@astro.u-strasbg.fr / ~~~~ // Observatoire de Strasbourg Phone +33 (0) 390 242 444 /______// 11, rue de l'universite Telefax +33 (0) 390 242 417 (______(/ F-67000 Strasbourg France From owner-dm@eso.org Tue Oct 21 14:01:25 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9LBuLPG009573 for ; Tue, 21 Oct 2003 13:56:21 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9LBuLH9009571 for dm-outgoing; Tue, 21 Oct 2003 13:56:21 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dm@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9LBtSPG009258 for ; Tue, 21 Oct 2003 13:55:28 +0200 (MEST) Received: from artemis.le.ac.uk (artemis.le.ac.uk [143.210.16.126]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9LBj7B1018124 for ; Tue, 21 Oct 2003 13:45:08 +0200 (CEST) Received: from [143.210.36.58] (helo=mail.star.le.ac.uk) by artemis.le.ac.uk with smtp (Exim 4.24) id 1ABuwl-0005Jp-0Z for dm@ivoa.net; Tue, 21 Oct 2003 12:45:07 +0100 Received: (qmail 4423 invoked from network); 21 Oct 2003 11:45:19 -0000 Received: from sparky.star.le.ac.uk (143.210.36.10) by mail.star.le.ac.uk with SMTP; 21 Oct 2003 11:45:19 -0000 Date: Tue, 21 Oct 2003 12:45:18 +0100 (BST) From: "Patricio F. Ortiz" To: Anita Richards cc: dm@ivoa.net, Subject: Re: UCDS and DM In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-dm@eso.org Precedence: bulk Reply-To: "Patricio F. Ortiz" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 On Tue, 21 Oct 2003, Anita Richards wrote: > Please can I clarify a possible application, which may initially be done > in an ad-hoc way until data models are fully harnessed: > > Supposing we are harvesting a catalogue which consists of radio flux > densities measured at 22 GHz. This is stated in the Abstract or ReadMe or > maybe even the title, but there is no table in the data saying 'observing > frequency'. As I understand it, we could add a virtual column > em.radio.12-25GHz, in which all the entries are the same. Can this be > done as a default, so that the data are recognised at their proper > frequency? Anita, the way UCD1 would handle this is that the UCD associated to the flux will reflect the region of the radio spectrum, eg, PHOT_FLUX_RADIO_11-25GHz, therefore, your catalogue will be discovered by the presence of that UCD without having to add a virtual column describing the observed frequency range. This case was very common, and not only in radio. There are hundreds of columns with "magnitude" as explanation, and you find the waveband in either the readme or the table title. UCDs are supposed to reflect the quantity as well as possible, that's why even with UCD1 one can launch discovery queries of this type and discover catalogues which have no indication of that part of their content in other pieces of meta-data information. Cheers, Patricio --- Patricio F. Ortiz pfo@star.le.ac.uk AstroGrid project Department of Physics and Astronomy University of Leicester Tel: +44 (0)116 252 2015 LE1 7RH, UK From owner-ucd@eso.org Tue Oct 21 13:31:40 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9LBS5PG001053 for ; Tue, 21 Oct 2003 13:28:05 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9LBS5Hh001050 for ucd-outgoing; Tue, 21 Oct 2003 13:28:05 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9LBRSPG000814 for ; Tue, 21 Oct 2003 13:27:28 +0200 (MEST) Received: from artemis.le.ac.uk (artemis.le.ac.uk [143.210.16.126]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9LBRSs3029094 for ; Tue, 21 Oct 2003 13:27:28 +0200 (CEST) Received: from [143.210.36.58] (helo=mail.star.le.ac.uk) by artemis.le.ac.uk with smtp (Exim 4.24) id 1ABufe-0004Bm-UG for ucd@ivoa.net; Tue, 21 Oct 2003 12:27:26 +0100 Received: (qmail 3067 invoked from network); 21 Oct 2003 11:27:48 -0000 Received: from peneca.star.le.ac.uk (143.210.36.224) by mail.star.le.ac.uk with SMTP; 21 Oct 2003 11:27:48 -0000 Date: Tue, 21 Oct 2003 12:27:48 +0100 (BST) From: Clive Page To: ucd@ivoa.net cc: registry@ivoa.net Subject: Re: Version 1.9.9 of UCD definition In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Clive Page X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 On Tue, 21 Oct 2003, Anita Richards wrote: > Thus, to keep the 'decades', this seems more suitable: > XRAY 0.12 - 12 keV (as per UCD2) > GAMMARAY > 12 keV > but maybe a high energy astronomer can advise.... I think that boundary between the two is reasonable: some past instruments called 'X-ray' have some coverage up to maybe 15 keV, but most modern telescopes depend on grazing-incidence reflection, which practically stops working above about 10 or 12 keV. > OVERLAPPING DATA > How will the UCDs be used? As I understand it, in order to use Vizier or > the Aladin SED tool to search for e.g. radio observations between 1.3 and > 1.7 GHz (radio L-band), the software would look for UCDs > em.radio.750-1500MHz and em.radio.1.5-3GHz. I think the way it has to work is this: the UCD defined for some dataset should be as specific as possible, so if the data fall practically within a single band (say within 750-1500 MHz) then you declare the UCD as "em.radio.750-1500MHz". If not then you have to fall back on a less specific UCD of "em.radio". A user wanting radio measurments at some frequency should be prepared to search for both _the_ most specific UCD and the less specific UCD, i.e. "em.radio". This may bring up some false positives, but so will any scheme that we can devise. The alternative, as you say, is to apply a two or more UCDs to a dataset. That might be better in principle, but difficult in practice. > * not use the fine divisions in UCDs, but treat frequency like position > and treat every query as a 1D cone search, ie a linear segment search. Well that's similar to a proposal I made some time ago (maybe in a Data Models context). Datasets should specify the range of frequencies they cover (which requires two numbers for the min frequency and max frequency, which doesn't imply that coverage between the limits is continuous, gaps should be ignored); then users also specify the range of interest. It's then a trivial exercise for a computer to compare the two intervals and work out which resources overlap the range of interest. All this without us having to dream up any artificial divisions between wavebands. But that doesn't fit in with UCDs as devised up to now, and I don't see any easy way to make it fit. -- Clive Page Dept of Physics & Astronomy, University of Leicester, Tel +44 116 252 3551 Leicester, LE1 7RH, U.K. Fax +44 116 252 3311 From owner-registry@eso.org Tue Oct 21 14:57:12 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9LCqjck027023 for ; Tue, 21 Oct 2003 14:52:45 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9LCqj60027020 for registry-outgoing; Tue, 21 Oct 2003 14:52:45 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-registry@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9LCq7ck026792 for ; Tue, 21 Oct 2003 14:52:07 +0200 (MEST) Received: from artemis.le.ac.uk (mailsend.le.ac.uk [143.210.16.126]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9LCq6B1019645 for ; Tue, 21 Oct 2003 14:52:06 +0200 (CEST) Received: from [143.210.36.58] (helo=mail.star.le.ac.uk) by artemis.le.ac.uk with smtp (Exim 4.24) id 1ABvzZ-0000yK-R4 for registry@ivoa.net; Tue, 21 Oct 2003 13:52:05 +0100 Received: (qmail 8325 invoked from network); 21 Oct 2003 12:52:27 -0000 Received: from sparky.star.le.ac.uk (143.210.36.10) by mail.star.le.ac.uk with SMTP; 21 Oct 2003 12:52:27 -0000 Date: Tue, 21 Oct 2003 13:52:27 +0100 (BST) From: "Patricio F. Ortiz" To: Clive Page cc: ucd@ivoa.net, Subject: Re: Version 1.9.9 of UCD definition In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-registry@eso.org Precedence: bulk Reply-To: "Patricio F. Ortiz" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi, I'm glad we are going into this discussion, not because it's an easy subject, but because it is a relevant one. The EMS is perhaps the most important 'tree' which we want to describe properly. I see several different regimes: a) broad band observations (eg, Johnson's V, radio bands, X-ray bands) b) narrow bands c) line spectroscopy (H-alpha, 21cm, CO, OIII, etc) d) continuum spectroscopy (eg, from blue to red) e) flux ratios The question of how to describe these quantities is strongly linked to what we want to use with the descriptors. It is different what we assign to the column (the UCD) and the type of search we intend to perform. If our goal is to find all radio fluxes, then we could cut the UCD in phot.flux.radio at the level of search, so even if we have infinite granularity (eg, phot.flux.radio.22Ghz), this column will be recognized. If on the other hand we are interested in finding observations in 22GHz, having an assigned UCD phot.flux.radio assures us to find the 22GHz data (eventually), but the S/N will be quite low, having to browse through hundreds of catalogues to find 1 is not desirable, and it's not what we had in mind when UCDs were introduced. Specifity also means that one can discover quantities which are comparable, that one will not mix a line measurement with a continuum one (despite being very close in frequency). What I think is important to decide now is if up to what extent the UCDs can do the job, without complicating them too much or oversimplifying them to the point of becoming useless for discovery purposes. One thing I wouldn't like to see is to see UCDs become as ambiguous as column descriptions. It is quite possible that we should resource to another element of meta-information for the description of a quantity and for its discovery. I thought that 'utype' could be used to link observational windows with their description (data model?). eg, UCD="phot.mag.opt" utype="strongrem.B" or UCD="phot.flux.radio" utype="JBO.22Ghz" or UCD="phot.flux.radio" utype="VLA.6cm" For accurate matching, one would have to use both pieces of information to avoid mixing apples with oranges. The method that Anita and Clive mention (a fine piano-keyboard mask) is something I've considered as well. It is broader than the UCD, but requires accurate knowledge of each band observation window (I'm not saying it's not doable). Users could then specify which part of the spectrum they are interested in and they will find the tables which contain data in those parts of the EMS. This works quite well for broad bands, but it is not so great if one is interested in narrow bands. Imagine one searches data around HBeta. Most catalogues with "blue broad band" observations will have 1's in that area of the spectrum, therefore, the noise will be huge! The same is valid for lines in other areas of the spectruma. (that's why I didn't pursue this model farther). Same is valid for colour indices: looking for V-K in terms of its initial and final wavelength will bring a large number of undesired catalogues/columns. One solution I've proposed is to stick to a very fine granularity at the UCD level which will allow us to compare alike quantities, but to create "virtual containers" in as many orthogonal directions as needed to solve the EM problem, as boundaries will continue shifting and being taste dependent. Imagine for a second that we keep the fine granularity, having UCDs like phot.jhn.B, phot.jhn.V, phot.jhn.R, phot.jhn.I, phot.str.B, .... phot.sloan.b (if exists) The original UCD structure allowed users to retrieve any catalogue with Johnson's photometry (just search for /phot.jhn/ and voila), but there was no room to look for "catalogues with blue broad-band observations" A "virtual container" for this example could be phot.opt.blue.bb. No column will ever be assigned this VC-UCD, but a search engine will understand it as "hmm, phot.opt.blue.bb is not a UCD, I need to look for catalogues which contain any of the UCDs listed in its index". To follow the example, phot.opt.blue.bb := ("phot.jhn.B", "phot.str.B", "phot.sloan.b"); And if later, GAIA introduces its own blue filter, phot.gaia.B will be created as a UCD, and "phot.gaia.B" will become part of this list: phot.opt.blue.bb := ("phot.jhn.B", "phot.str.B", "phot.sloan.b", "phot.gaia.b"); Finally, alhough a column should have one and only one UCD, nothing should prevent that a UCD could belong to several virtual containers. UCDs would describe what quantities are, VCs are used to describe contexts or related concepts accepted by the community at any time, and quite possibly user-definable in the future. Food for thought... after all, > 50% of the current and future quantities are related to the EMS! Cheers, Patricio --- Patricio F. Ortiz pfo@star.le.ac.uk AstroGrid project Department of Physics and Astronomy University of Leicester Tel: +44 (0)116 252 2015 LE1 7RH, UK From owner-ucd@eso.org Tue Oct 21 16:27:22 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9LENXco028990 for ; Tue, 21 Oct 2003 16:24:37 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9LEKkKZ028045 for ucd-outgoing; Tue, 21 Oct 2003 16:20:46 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9LDqBe2018354; Tue, 21 Oct 2003 16:19:42 +0200 (MEST) Received: from esacom51.vilspa.esa.int (esacom51-ext.vilspa.esa.int [192.171.2.19]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9LCZps3000839; Tue, 21 Oct 2003 14:35:52 +0200 (CEST) Received: from iso.vilspa.esa.es (isous5.vilspa.esa.es [193.147.153.100]) by esacom51.vilspa.esa.int (8.12.9/8.12.9/ESA-External-v3.2) with ESMTP id h9LCZpih008834; Tue, 21 Oct 2003 14:35:51 +0200 (MET DST) Received: from isou53 (isou53 [193.147.153.35]) by iso.vilspa.esa.es (8.12.10/8.12.10) with SMTP id h9LCZjBU010850; Tue, 21 Oct 2003 14:35:45 +0200 (MEST) Date: Tue, 21 Oct 2003 14:35:45 +0200 From: posuna@iso.vilspa.esa.es To: Anita Richards Cc: dm@ivoa.net, ucd@ivoa.net Subject: Re: UCDS and DM Message-Id: <20031021143545.375a8cf4.posuna@iso.vilspa.esa.es> In-Reply-To: References: <1066406745.3f90135915f9f@netmail.pipex.net> <3F950D15.AEDBC59C@astro.u-strasbg.fr> X-Mailer: Sylpheed version 0.9.2 (GTK+ 1.2.9; sparc-sun-solaris2.8) Mime-Version: 1.0 Content-Type: multipart/mixed; boundary="Multipart_Tue__21_Oct_2003_14:35:45_+0200_002ece08" X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: posuna@iso.vilspa.esa.es X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 This is a multi-part message in MIME format. --Multipart_Tue__21_Oct_2003_14:35:45_+0200_002ece08 Content-Type: text/plain; charset=US-ASCII Content-Transfer-Encoding: 7bit Hi, > I was slightly puzzled by comments at the interoperability workshop > about data collections which do not have catalogues/tables. Surely > even a collection of FITS spectra or images or etc. must be accessed > via a descriptive list? Although I suppose a data collection could > consist of a single image (or etc.). In either case, though, is this > is another example of where it would be useful to take UCDs from what > might be a single description ("images taken at 0.05 arcsec resolution > ...") of the whole data collection - and use them to form or augment a > table to allow access to the data? We do have quite complex data models for our data; you can see part of the ISO model in the attached figures called iso_cdm_obss.gif and iso_pdm_obss.gif which are part of our (database jargon) CDM (Conceptual Data Model) and PDM (Physical Data Model) documents (where you can see loads of very project-specific things). The access to our data is not done through a descriptive list, but through database queries. However, in the case that someone wants a catalogue/table from our data, we can provide one. This is what we do with CDS: we provide them with the table they store in Vizier and that can be used as the rest of catalogues there for data mining (I'm not sure whether this is the word...I mean data discovery, etc.). You can find this table at: ftp://cdsarc.u-strasbg.fr/cats/B/iso/isolog.dat.gz However, that is only a very specific view of our data which can, otherwise, be accessed through other means, e.g., by SIAP or future SSAP, etc., or in the case of a proper general Data Model, through a proper VOQl to the Data Model (how we translate the future "Standard VO data Model" to ours is another story...(unfortunately, only up to us I'm afraid...)). Cheers, Pedro. -- Pedro Osuna Alcalaya SOFTWARE Development Group XMM-Newton Science Archive e-mail: Pedro.Osuna@esa.int Tel + 34 91 8131314 European Space Agency VILLAFRANCA Satellites Tracking Station P.O. 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from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9LEgeck005417 for ; Tue, 21 Oct 2003 16:42:40 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9LEgeVo005416 for ucd-outgoing; Tue, 21 Oct 2003 16:42:40 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9LEerck004885; Tue, 21 Oct 2003 16:40:53 +0200 (MEST) Received: from mail.cacr.caltech.edu (mail.cacr.caltech.edu [131.215.145.9]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9LEeqs3003969; Tue, 21 Oct 2003 16:40:52 +0200 (CEST) Received: from Ropy (dsl-pb-1504.linkline.com [64.30.223.60]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id h9LEeoM9001164 (version=TLSv1/SSLv3 cipher=RC4-MD5 bits=128 verify=NO); Tue, 21 Oct 2003 07:40:51 -0700 Message-ID: <049b01c397e1$57b39ad0$6501a8c0@Ropy> From: "Roy Williams" To: , References: Subject: UCD use cases Date: Tue, 21 Oct 2003 07:40:58 -0700 MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Roy Williams" X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Please find below some possible use cases for UCD. -- How do the different proposed UCD/DM schemes help with these cases? -- What does the query look like in each case, and how would that query be coded? -- Can you supply additional use cases? Please try to stay within the realm of the possible here! -- If you refer to a Data Model, please try to be concrete about who/how/example. Please do not simply invoke "the Future IVOA Data Model". Thank you Roy -------------------------- (1) Cone search. How to decide which columns are the RA,Dec that was used in the search. What frame (B1950, J2000, ...) do these come from? If there are columns with ID, what sort of ID is it, and how do I resolve it? (2) SIAP search. Find the column that contains the URLs where the images are. Find out if there are other columns that have RA,Dec of the image center. (3) We have for example a crossmatch service that is clever enough to know about error ellipses. How does it get from a table the most sophisticated error info that is there: (a) position (b) circular error (c) ellipse error. (4) We want to compare photometry in two tables covering the same star cluster. How do I decide if they share measurements in the same filter? One has R band, the other has Halpha. What happens if fluxes are expressed differently -- eg number / energy / magnitude / luminosity density. (5) I want distances to stellar objects measured in meters, so I can make a 3D display for the children. How do I recognize a redshift (z) value, how do I recognize a radial velocity, how do I recognize an actual distance measure? (6) I am looking for supernovae that have both optical and Xray measurements. Can I (should I) use UCD to help my search? (7) How do I find 21cm observations (that may be redshifted), which also have polarization information? From owner-ucd@eso.org Tue Oct 21 19:03:20 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9LGwbd5020666 for ; Tue, 21 Oct 2003 18:58:37 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9LGwbMb020661 for ucd-outgoing; Tue, 21 Oct 2003 18:58:37 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9LGuhd9019930 for ; Tue, 21 Oct 2003 18:57:50 +0200 (MEST) Received: from artemis.le.ac.uk (mailsend.le.ac.uk [143.210.16.126]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9LFkHB1024359 for ; Tue, 21 Oct 2003 17:46:17 +0200 (CEST) Received: from [143.210.36.58] (helo=mail.star.le.ac.uk) by artemis.le.ac.uk with smtp (Exim 4.24) id 1AByi8-0003mH-II for ucd@ivoa.net; Tue, 21 Oct 2003 16:46:16 +0100 Received: (qmail 9886 invoked from network); 21 Oct 2003 15:46:37 -0000 Received: from sparky.star.le.ac.uk (143.210.36.10) by mail.star.le.ac.uk with SMTP; 21 Oct 2003 15:46:37 -0000 Date: Tue, 21 Oct 2003 16:46:37 +0100 (BST) From: "Patricio F. Ortiz" To: Roy Williams cc: dm@ivoa.net, Subject: Re: UCD use cases In-Reply-To: <049b01c397e1$57b39ad0$6501a8c0@Ropy> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Patricio F. Ortiz" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi Roy, here are my 2 cents. On Tue, 21 Oct 2003, Roy Williams wrote: > Please find below some possible use cases for UCD. > > -- How do the different proposed UCD/DM schemes help with these cases? > > -- What does the query look like in each case, and how would that query be > coded? > > -- Can you supply additional use cases? Please try to stay within the realm > of the possible here! > > -- If you refer to a Data Model, please try to be concrete about > who/how/example. Please do not simply invoke "the Future IVOA Data Model". > > Thank you > Roy > -------------------------- > > (1) Cone search. How to decide which columns are the RA,Dec that was used in > the search. What frame (B1950, J2000, ...) do these come from? If there are > columns with ID, what sort of ID is it, and how do I resolve it? pick RA and dec from UCDs: pos.eq.ra;main, pos.eq.dec;main If the source is a VOTable, one can use the COOSYS element to figure out the equinox/epoch. If the source is plain metadata, we're missing the equinox element by using the plain UCD. Within a DM, the equinox should be there and can be used to solve the ambiguity. Now, if they are different, the question is whether they should be precessed. I assume that you mean src.object_id... Hmmm, invoke simbad or ned or any name-solver with the appropriate output equinox. However, I would advocate at this point in time to strongly avoid the existence of catalogues where only the ID is provided. It would be an effort to solve those names for all these catalogues, but once done, we don't have to worry about it anymore. > (2) SIAP search. Find the column that contains the URLs where the images > are. Find out if there are other columns that have RA,Dec of the image > center. I can see your point of differentiating RA/dec for sources as opposed to observations in a log. RA/dec are coordinates regardless of what one measure, so UCD1 didn't do anything about it. In the image catalogues, pos.eq.[ra|dec];main represent the image pointing. > (3) We have for example a crossmatch service that is clever enough to know > about error ellipses. How does it get from a table the most sophisticated > error info that is there: (a) position (b) circular error (c) ellipse error. Thought about this one before :-) Most complete case: elliptic error: - semi-major axis error.pos.smaj - semi-minor axis error.pos.smin - ellipse orientation (PA) error.pos-ang Alternatively, one could have ellipticity (error.ellipt) xor axis-ratio (error.pos.ax-ratio) and major axis, in which case one has to compute the semi-minor axis Circular, simpler, we only need err.pos.smaj (or err.pos.rad) Roy, please extend this case not just to errors, but to extended objects, as we could be talking about overlap between galaxies or molecular clouds or other extended structures/objects. > (4) We want to compare photometry in two tables covering the same star > cluster. How do I decide if they share measurements in the same filter? One > has R band, the other has Halpha. What happens if fluxes are expressed > differently -- eg number / energy / > magnitude / luminosity density. In a first approximation, I'd say stick to compare apples with apples and oranges with oranges. UCDs should tell you which band is observed (oops, that's UCD1s), therefore it should be clear whether the two tables contain the same type of observations. One interesting scenario here is to have a real Xmatch machine which identifies the stars of one table with the ones with the other. I may want to produce a diagram type R vs Halpha. If more than two tables are involved, and one chooses one filter, we are talking about forming light curves. > (5) I want distances to stellar objects measured in meters, so I can make a > 3D display for the children. How do I recognize a redshift (z) value, how do > I recognize a radial velocity, how do I recognize an actual distance > measure? Redshift, by its UCD: redshift.hc radial velocity: veloc.hc (beware of radial velocities of expanding stars) distance: phys.distance.true, drop anything measured in kpc or Mpc :-) beware of things measured in km or au Or, go to any catalogue measuring parallax and convert to distance. convert your distances to meters (tool to be built) > (6) I am looking for supernovae that have both optical and Xray > measurements. Can I (should I) use UCD to help my search? Optical and Xray UCDs appear not only in catalogues related to supernovae. Look for catalogues with supernova in their title and then use the X-RAy UCDs (SN are still discovered in optical, so they'll surely have optical fluxes). Look at a few catalogues with SNe for quantities which are proper of these objects (var.??) > (7) How do I find 21cm observations (that may be redshifted), which also > have polarization information? UCDs will help you with polarization. Try /pol./, 21cm for sure frequency-wise: phot.flux.radio.1.4G (that's why we didn't use '.' to separate the UCDs :-) but no assurance if the redshift is too high. Scan the table title for /21/ && /cm/ if the radio UCD. I'd expect the results to be nearly the same. Note: I just used http://barbara.star.le.ac.uk/datoz/mykats.html to perform the last search... I found a few cats with POL_ and RADIO_FLUX in 1.4Ghz Sorry, no time to write the queries in a WLQL (wish list query language) :-) Cheers, Patricio --- Patricio F. Ortiz pfo@star.le.ac.uk AstroGrid project Department of Physics and Astronomy University of Leicester Tel: +44 (0)116 252 2015 LE1 7RH, UK From owner-ucd@eso.org Tue Oct 21 19:04:55 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9LGxsd5021151 for ; Tue, 21 Oct 2003 18:59:54 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9LGxrdX021144 for ucd-outgoing; Tue, 21 Oct 2003 18:59:53 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9LGuhdB019930; Tue, 21 Oct 2003 18:58:36 +0200 (MEST) Received: from plum.csi.cam.ac.uk (plum.csi.cam.ac.uk [131.111.8.3]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9LFThB1023907; Tue, 21 Oct 2003 17:29:43 +0200 (CEST) Received: from cass41.ast.cam.ac.uk ([131.111.69.186]) by plum.csi.cam.ac.uk with esmtp (Exim 4.20) id 1AByRf-0004d0-Aa; Tue, 21 Oct 2003 16:29:15 +0100 Received: from cass123.ast.cam.ac.uk (cass123 [IPv6:2001:630:200:4240:203:baff:fe17:f117]) by cass41.ast.cam.ac.uk (8.12.10+Sun/8.12.10) with ESMTP id h9LFTEtu020087; Tue, 21 Oct 2003 16:29:15 +0100 (BST) Received: from cass123.ast.cam.ac.uk (localhost [127.0.0.1]) by cass123.ast.cam.ac.uk (8.12.10+Sun/8.12.10) with ESMTP id h9LFTEbe020303; Tue, 21 Oct 2003 16:29:14 +0100 (BST) Received: from localhost (gtr@localhost) by cass123.ast.cam.ac.uk (8.12.10+Sun/8.12.8/Submit) with ESMTP id h9LFTEMO020300; Tue, 21 Oct 2003 16:29:14 +0100 (BST) X-Authentication-Warning: cass123.ast.cam.ac.uk: gtr owned process doing -bs Date: Tue, 21 Oct 2003 16:29:14 +0100 (BST) From: Guy Rixon To: Roy Williams cc: dm@ivoa.net, ucd@ivoa.net Subject: Re: UCD use cases In-Reply-To: <049b01c397e1$57b39ad0$6501a8c0@Ropy> Message-ID: References: <049b01c397e1$57b39ad0$6501a8c0@Ropy> MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Cam-ScannerInfo: http://www.cam.ac.uk/cs/email/scanner/ X-Cam-AntiVirus: No virus found X-Cam-SpamDetails: Not scanned X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Guy Rixon X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 An additional case: I have a heap of data expressing modelled and observed values for a handful of quantities; celestial coords and proper motions would do as an example. I want to read out all the modelled versions of one of these quantities and compare them to assess the spread of the models. Then I want to do the same with the observations. What do I look for? On Tue, 21 Oct 2003, Roy Williams wrote: > Please find below some possible use cases for UCD. > > -- How do the different proposed UCD/DM schemes help with these cases? > > -- What does the query look like in each case, and how would that query be > coded? > > -- Can you supply additional use cases? Please try to stay within the realm > of the possible here! > > -- If you refer to a Data Model, please try to be concrete about > who/how/example. Please do not simply invoke "the Future IVOA Data Model". > > Thank you > Roy > -------------------------- > > (1) Cone search. How to decide which columns are the RA,Dec that was used in > the search. What frame (B1950, J2000, ...) do these come from? If there are > columns with ID, what sort of ID is it, and how do I resolve it? > > (2) SIAP search. Find the column that contains the URLs where the images > are. Find out if there are other columns that have RA,Dec of the image > center. > > (3) We have for example a crossmatch service that is clever enough to know > about error ellipses. How does it get from a table the most sophisticated > error info that is there: (a) position (b) circular error (c) ellipse error. > > (4) We want to compare photometry in two tables covering the same star > cluster. How do I decide if they share measurements in the same filter? One > has R band, the other has Halpha. What happens if fluxes are expressed > differently -- eg number / energy / > magnitude / luminosity density. > > (5) I want distances to stellar objects measured in meters, so I can make a > 3D display for the children. How do I recognize a redshift (z) value, how do > I recognize a radial velocity, how do I recognize an actual distance > measure? > > (6) I am looking for supernovae that have both optical and Xray > measurements. Can I (should I) use UCD to help my search? > > (7) How do I find 21cm observations (that may be redshifted), which also > have polarization information? > Guy Rixon gtr@ast.cam.ac.uk Institute of Astronomy Tel: +44-1223-337542 Madingley Road, Cambridge, UK, CB3 0HA Fax: +44-1223-337523 From owner-dm@eso.org Tue Oct 21 19:32:42 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9LHSPd5029323 for ; Tue, 21 Oct 2003 19:28:25 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9LHSPwG029321 for dm-outgoing; Tue, 21 Oct 2003 19:28:25 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dm@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9LHRHd5029023; Tue, 21 Oct 2003 19:27:17 +0200 (MEST) Received: from curlew.cs.man.ac.uk (curlew.cs.man.ac.uk [130.88.13.7]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9LHRHB1026687; Tue, 21 Oct 2003 19:27:17 +0200 (CEST) Received: from star1.jb.man.ac.uk ([130.88.24.176]) by curlew.cs.man.ac.uk with esmtp (Exim 4.20) id 1AC0Hs-000NJ2-Mf; Tue, 21 Oct 2003 18:27:16 +0100 Received: from [130.88.24.80] (helo=aten) by star1.jb.man.ac.uk with esmtp (Exim 3.03 #2) id 1AC0Hs-0005S5-00; Tue, 21 Oct 2003 18:27:16 +0100 Date: Tue, 21 Oct 2003 18:28:24 +0100 (BST) From: Anita Richards X-X-Sender: amsr@aten To: Roy Williams , posuna@iso.vilspa.esa.es cc: dm@ivoa.net, ucd@ivoa.net Subject: Re: UCD use cases In-Reply-To: <049b01c397e1$57b39ad0$6501a8c0@Ropy> Message-ID: References: <049b01c397e1$57b39ad0$6501a8c0@Ropy> MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanner: exiscan for exim4 (http://duncanthrax.net/exiscan/) *1AC0Hs-000NJ2-Mf*aCCTY48m5BY* X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-dm@eso.org Precedence: bulk Reply-To: Anita Richards X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi Roy, Great to see something practical happening. One comment - we do need to see the use of UCDs alongside the use of the Registry and data models (e.g. Pedro Osuna's very helpful reply which has indeed lifted my confusion about non-table data - or that bit of it anyway). Hence, when people provide implimentation of use cases, it would be nice to see: Where/if UCDs are used in the Registry to select data-sets (and if only UCDs, not other entries e.g. spectral coverage, keywords, serve a particular purpose); How UCDs are used (ideally in the context of a data model) to enable the processing steps in the execution of a query. Use case - if you are sick of Brown Dwarfs read no further: http://wiki.astrogrid.org/bin/view/Astrogrid/BrownDwarfRegistryRequirements The RegistryQuery steps use some things which could be UCDs like Proper Motion but they might also be key words. Specific colours are also used, but it might be sufficient to know that a catalogue contains optical and colour data. The DataSetQuery/Evaluation steps use these UCDs above and others. The new UCD structure enabling the use of partial matches would be a great help as the workflow contains choices where you use a quantity (e.g. colour) if already defined but if not you derive it ("you" being a data processing software agent). More examples could be drawn from the AstroGrid Ten... cheers a - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - Dr. Anita M. S. Richards, AVO Astronomer MERLIN/VLBI National Facility, University of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire SK11 9DL, U.K. tel +44 (0)1477 572683 (direct); 571321 (switchboard); 571618 (fax). From owner-dal@eso.org Tue Oct 21 21:33:59 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9LJU4d5016385 for ; Tue, 21 Oct 2003 21:30:04 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9LJU483016384 for dal-outgoing; Tue, 21 Oct 2003 21:30:04 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dal@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9LJSUd5015689; Tue, 21 Oct 2003 21:28:31 +0200 (MEST) Received: from milkyway.gsfc.nasa.gov (lheapop.gsfc.nasa.gov [128.183.16.62]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9LJSSs3010478; Tue, 21 Oct 2003 21:28:29 +0200 (CEST) Received: from lheapop.gsfc.nasa.gov (silk3.gsfc.nasa.gov [128.183.18.68]) by milkyway.gsfc.nasa.gov (8.12.9/8.12.9) with ESMTP id h9LJSRTd020928; Tue, 21 Oct 2003 15:28:27 -0400 Message-ID: <3F9588DF.3030805@lheapop.gsfc.nasa.gov> Date: Tue, 21 Oct 2003 15:28:31 -0400 From: Thomas McGlynn Organization: NASA Goddard Space Flight Center User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.5) Gecko/20030925 X-Accept-Language: en-us, en MIME-Version: 1.0 To: ucd@ivoa.net, dm@ivoa.net, dal@ivoa.net Subject: A suggested revision for UCDs Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-dal@eso.org Precedence: bulk Reply-To: Thomas McGlynn X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 A few minutes ago I uploaded a version of my suggested revised proposal for UCDs to the Twiki. This is just a Word version since I don't have a PDF generator handy. The URL is http://www.ivoa.net/internal/IVOA/IvoaUCD/UCD-1.9.9b.doc This builds upon Roy and Sebastien's division of UCDs into concepts and propeties but puts them together rather differently. In addition and largely independently, it includes a discussion of the use of UCDs in the context of groups of columns and tables as a whole. With the approach suggested, I hope that the ambiguities that have heretofore precluded considering using UCDs to mediate between data models and data can be removed and we may no longer require a utype parameter. Some discussion of the document is included (in red) within the text. This mostly describes the relationship of this version to the 1.9.9 version. Sections 3 and 6 of the document are copied from the previous version. (though section 6 was section 8 in that document) from the previous version. The abstract is altered to reflect the discussion of grouping constructs. Section 2 -- describing the status of the document -- has been changed to discuss the implications of the adoption of this recommendation upon existing software systems and protocols. I think that some such statement should be part of draft recommendations. Not sure if that's part of the recommendation process but it probably should be. Section 4 is the discussion of UCDs and UCD syntax. At the end of section 4 there is a long parenthetical discussion of some of the ways this proposal differs from 1.9.9 since people seemed to be concerned about that last Thursday. If they've gotten this far they probably don't need this anymore but it may be of interest. This section tries to be rather rigorous -- addressing a fair number of nits that had not been talked about in the earlier proposal even though it makes the proposal somewhat longer (e.g., the discussion of array valued cells, a much more detailed discussion of comparability of columns, how to ensure the uniqueness of UCDs, ...) The actual definition of all of the valid words for UCDs is deferred as it was in the earlier version, but a substantial number of examples are given. [In fact, most of the words should transfer between the two versions fairly transparently. The differences lie mostly in how they are put together.] Section 5 is the dicussion of UCDs and grouping structures. I'm quite excited by this since I think it real potential for helping to unify discussions of data, data models and data access. The discussion in this chapter is less rigorous -- even if the basic idea is adopted I'm sure it will need substantially more work but I think it has real possibilities for linking data models and data. This chapter is why I've sent this message to the DAL and DM groups as well as to the UCD group. Apologies to all of you who get this twice or thrice! I trust there will be comments... Tom From owner-ucd@eso.org Tue Oct 21 21:56:40 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9LJqOd5024031 for ; Tue, 21 Oct 2003 21:52:24 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9LJqO0i024030 for ucd-outgoing; Tue, 21 Oct 2003 21:52:24 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9LJpHd5023794; Tue, 21 Oct 2003 21:51:17 +0200 (MEST) Received: from milkyway.gsfc.nasa.gov (lheapop.gsfc.nasa.gov [128.183.16.62]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9LJpEs3010970; Tue, 21 Oct 2003 21:51:15 +0200 (CEST) Received: from lheapop.gsfc.nasa.gov (silk3.gsfc.nasa.gov [128.183.18.68]) by milkyway.gsfc.nasa.gov (8.12.9/8.12.9) with ESMTP id h9LJpETd022259; Tue, 21 Oct 2003 15:51:14 -0400 Message-ID: <3F958E35.1090703@lheapop.gsfc.nasa.gov> Date: Tue, 21 Oct 2003 15:51:17 -0400 From: Thomas McGlynn Organization: NASA Goddard Space Flight Center User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.5) Gecko/20030925 X-Accept-Language: en-us, en MIME-Version: 1.0 To: dal@ivoa.net, ucd@ivoa.net Subject: Re: UCD use cases References: <049b01c397e1$57b39ad0$6501a8c0@Ropy> In-Reply-To: <049b01c397e1$57b39ad0$6501a8c0@Ropy> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Thomas McGlynn X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Here are some thoughts about how the new UCD scheme I've proposed might help in Roy's scenarios. I'd sent this to Roy directly earlier without realizing that it had been sent to the UCD and DM groups.... Tom > > (1) Cone search. How to decide which columns are the RA,Dec that was used in > the search. What frame (B1950, J2000, ...) do these come from? If there are > columns with ID, what sort of ID is it, and how do I resolve it? > UCDtrees look something like: src;instance meta.id[.type];value pos;instance ra/dec, l/b columns pos.coosys;value Optional, either table coosys element of the table or a table wide parameter Look for highest pos;instance and meta.id;value to get the correct id and pos columns. If we want to handle B1950 coordinates then we need to include a table parameter or parameters including the coordinate system. Of course the cone search protocol requires that the output be in J2000, but it would be easy to support genericity if we want. I suggested that the coosys element in tables could have a UCD, but less controversial would be a table parameter giving the information. That's not quite as elegant. However I don't like duplicating metadata information. Maybe the best solution is to include a parameter but make it point to the coosys using the XML ID. Not sure what you mean by resolve the id, but assuming that this isn't addressed by specific subtypes of id, replace meta.id;value with meta.id;instance meta.id;value meta.id.resolver;value meta.resolver;value would presumably be a parameter but in principal if there was a different resolver for each row in the table it could be a column. > (2) SIAP search. Find the column that contains the URLs where the images > are. Find out if there are other columns that have RA,Dec of the image > center. Basic UCDTree is: obs;instance meta.id;value # The required id field meta.link;value # The link field pos;instance # The required position These are mandated columns in the SIAP protocol and the protocol should also specify that there is only one pos, meta.id and meta.link element at the top level. Note, by the by, that if we want to allow the SIAP protocol to return galactic positions, it's easy to do. [This isn't necessarily a good idea for SIAP, but the it shows the expressivity of the UCDTrees.] Could there be an image center that is distinct from this image? This would require there to be an associated observation to the main observation. [If I really want to go overboard I might have made the table UCD obs;filter.cutout;instance but I don't think that that is going to be useful to most people, though it does show a nice use of my suggested filter hierarchy.] This could be suggested by adding the following to the tree obs;instance meta.id;value pos;instance The issue which is harder to address is understanding the relationship between this secondary observation and the primary observation. This is a semantic issue not a structural one, so a UCD must be involved. E.g., we need to define concepts for background, center, offset, ... If we have done that (and I would suggest they belong in my meas tree since they have to do with idea of a measurement) then the previous addendum becomes [and I've put in a background image for good measure] obs.instance meta.id;value obs;meas.center pos;instance obs.instance meta.id;value obs;meas.background pos;instance How do I find this... I look for associated observations and search for one which has the desired measurement attribute. I believe an XQuery expression can do this pretty easily. > > (3) We have for example a crossmatch service that is clever enough to know > about error ellipses. How does it get from a table the most sophisticated > error info that is there: (a) position (b) circular error (c) ellipse error. This is pretty easy... Looking just at a given position, we might have: pos;instance pos.eq.ra;value pos.eq.dec;value pos.eq.ra;meas.error Errors in the coordinates pos.eq.ra;meas.error pos;meas.2d.error This is a circular 2-d error pos;meas.2d.error.elliptical;instance pos;meas.2d.error.elliptical.x pos;meas.2d.error.elliptical.y pos;meas.2d.error.elliptical.posang which gives all three of these. While there may be a better name for the last two errors, I don't think it matters much. Whatever error there is is directly associated with the position and it's easy to find out what errors are availalbe. The question of which error the user should use, is not appropriate for the UCD scheme. That's up to the user. The UCDs indicate which errors are available. I'm not sure if we want to elaborate the measurement tree to this level, maybe it could be done more simply in some other way. However I don't think this is an unreasonable approach. > > (4) We want to compare photometry in two tables covering the same star > cluster. How do I decide if they share measurements in the same filter? One > has R band, the other has Halpha. What happens if fluxes are expressed > differently -- eg number / energy / > magnitude / luminosity density. Well I don't think unit conversions are an issue that UCDs should address. So I'll pass on that. [That's what units keywords are for after all.] The columns should describe the bands in which they were taken. If we want to assure that we actually have the same filter, then we need UCDs that are specific down to the filter level. The old UCD tree (and I assume you've kept it in the current one) puts all of that info in the initial word. I'd tend to use the em modifier here to define the band. E.g., phot.mag;em.optical.filter.v.johnson;value phot.flux;em.optical.filter.v.johnson;value and phot.counts;em.optical.filter.v.johnson;value for magnitude, flux and counts (in a photon counting instrument) If the question is whether the filters overlap, then I don't think this is a question the UCDs answer directly. It's expert knowledge about the concepts (Just like the exact relationship between RA and Dec isn't specified in the UCD. That's expert knowledge too.) > (5) I want distances to stellar objects measured in meters, so I can make a > 3D display for the children. How do I recognize a redshift (z) value, how do > I recognize a radial velocity, how do I recognize an actual distance > measure? Units are not a UCD issue. The other questions simply need distinct UCDs. As I understand the schema they would just be different elements of the phys tree but that's a bit of a guess. Redshift is a different concept from distance as is a radial velocity. They can be converted into each other in certain circumstances, but it is not the role of UCDs to understand the transformation rules -- just as it is not the role of UCDs to understand how to convert from RA,Dec to L,B. I think it may be reasonable to have all of the base concepts: phys.distance A distance of some kind phys.distance.z A redshift in a cosmological context phys.distance.vrad A radial velocity in a cosmological context phys.z A redshift in non-cosmological context phys.vrad A radial or to only have the single distance concept and leave it to the user to recognize that they are in a cosmological context so that radial velocities can be converted to distances. That's probably safer from the context of trying to ensure that there is only one UCD for a given concept so I'd tend to go that way. Users put z in a table rather than distance for a reason. UCDs describe what a column is, they need not and should not describe what you can do with a column. I gather that is the role of ontologies. > > (6) I am looking for supernovae that have both optical and Xray > measurements. Can I (should I) use UCD to help my search? You can certainly try. This depends a bit upon the specific UCD tree. If table UCDs are often of the form src.[type];instance you can search the registry for tables of the form src.supernova;instance Similarly ou can use search columns the phot and look for optical and X-ray qualifiers. If you get tables that meet all the criteria you've got a great place to start. I.e., look for UCDTree that matches the template src.supernovae;instance //phot*;em.xray*;value //phot*;em.optical*;value [Where this is some Xqueryish kind of match to the UCDTree hierarchy] and you've got a great chance that this has the information you wnat. Even if there is no match, you can consider tables that are partial hits and look to see if you can join information appropriately using multiple tables. A real win here would be a VO service to enable comparison of class information among tables. Right now source classes are a real mess and we need a Simbad- or NED-like service to address it. That will probably be needed if you want to interrogate the vast majority of UCDTrees that with have src;instance and some classification parameter inside. > > (7) How do I find 21cm observations (that may be redshifted), which also > have polarization information? > > Look for all tables that have columns that match flux.phot*;em.pol*;value to get polarization information Limit to tables that have a flux value in the 21cm region -- don't know if that has it's own special UCD -- or which has flux in the region from 10-100 cm and a redshift or radial velocity. This assumes there is some service that gives me the em qualifiers I need to look for given a specific energy/wavelength/frequency range. It wouldn't be too hard by hand either. This is a straightforward analysis of the column UCDs that doesn't need to worry about the structure UCDs at all. From owner-dal@eso.org Wed Oct 22 19:21:20 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9MHGMKp003608 for ; Wed, 22 Oct 2003 19:16:22 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9MHGMIh003607 for dal-outgoing; Wed, 22 Oct 2003 19:16:22 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dal@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9MHFmKp003459; Wed, 22 Oct 2003 19:15:48 +0200 (MEST) Received: from donner.stsci.edu (donner.stsci.edu [130.167.251.65]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9MHFis3004937; Wed, 22 Oct 2003 19:15:45 +0200 (CEST) Received: from aria (aria.stsci.edu [130.167.236.125]) by donner.stsci.edu (Mirapoint Messaging Server MOS 3.3.6-GR) with ESMTP id AGU13171; Wed, 22 Oct 2003 13:15:37 -0400 (EDT) Message-ID: <021901c398c0$1ec33c00$7deca782@stsci.edu> From: "Robert Hanisch" To: , Subject: Fw: A suggested revision for UCDs Date: Wed, 22 Oct 2003 13:15:37 -0400 Organization: Space Telescope Science Institute MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Junkmail-Whitelist: YES (by domain whitelist at donner.stsci.edu) X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-dal@eso.org Precedence: bulk Reply-To: "Robert Hanisch" X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Here is a discussion that Tom and I had off-list, but I think are number of points of more general interest are raised. Warning -- it is quite long! Bob - - - - - Hi Bob, Thanks for the review and comments. I'm particularly interested in the areas that were unclear. It seemed to me that I needed to actually put the ideas out where I could get some detailed reactions. A fair number of typo issues were addressed in the version I uploaded to the Twiki and announced to the UCD, DM and DAL groups. Haven't heard of any reaction. I've responded to your comments below (there a lot of detail but I thought it user to think these things through). Tom Robert Hanisch wrote: > Hi Tom. I read through your revised UCD document this evening. Phew. > There is much in it I like, much I don't, and much I don't follow. Perhaps > the two latter categories mix together. > > I guess my biggest problem is that the roles of concept, attribute, and > modifier are partly defined by syntax (where they appear in the string) and > partly by having to know what names (em, pos, flux) have been allocated to > which category. This seems very arbitrary (and very confusing) to me. > Although I have never written a parser in my life, it looks to me like a > parser for this would be a zillion if statements. Maybe this is fewer if > statements than for other approaches, but it still looks very complex. > I agree that this is a major issue, although my biggest concern with it is a little different. I'm giving a long answer to help me organize my thoughts. The writer of a table presumably has access to the documentation for UCDs so it shouldn't be a big problem dealing with the three types -- especially once there are examples. The problem is more in using UCDs when reading tables. In practice I'm not sure this would be a big deal for 'real' tools. E.g., something like VOPlot is going to need to know about the value and meas.error attributes internally so that it can plot values and error bars for a given quantity. I.e., it's just going to look for pairs of columns within the same group of the form: SomeString;value and SomeString;meas.error A spectral processing tool is going to look for pairs like phot.flux*;value and phys.wavelength;value. Specific tools internalize this kind of knowledge -- or even better read it in as a data model. These tools don't really know about how UCDs are organized. The organization is intended to make it easy for them to search for the appropriate strings, but they just take advantage of that. Generic tools for manipulating UCDs and for validating them are where the problem really begin to show up. Currently there are only 6 trees that are not basic concepts (em, frame and intent for modifiers and filter, stat and meas for attributes). I think the single word attributes are important enough that they will not cause a problem. So a complete algorithm to determine what word belongs in what vocabulary is currently pretty easy... Psuedocode is just: firstAtom = substring(ucd, index(ucd,".")) switch (firstAtom) { 'em', 'frame','intent': return thisIsAModifier 'stat','filter','meas': return thisIsAnAttribute 'value','local','instance','multiplet', 'vector': return thisIsAnAttribute } return thisIsAConcept Alternatively we're talking about validating UCDs against an IVOA schema to define the valid words and the match against this could give the type. There are other simple ways to deal with this: Begin all modifiers with m. and attributes with a. Or I've suggested in the draft that all modifiers could be in the frame tree -- the idea is that the role of modifiers is to limit the context to which the concept applies. I don't think the attribute trees join as easily but if it's important enough we could pick a name for all of the attribute trees. The biggest problem is non-standard namespaces. How do we handle a new UCD tree? In some sense the issue is moot. Non-standard words shouldn't be used outside of some developers local context. They can be responsible for handling them. However I suspect that non-standard words will escape into the wild. The validate against the schema approach still works, but it's impossible for writers for tables to know how to use these UCDs. There are some other ideas that might help address this issue: Your suggestion of another separator character is nice. I thought about it but decided that it was too radial a change. Maybe separate atributes and modifiers within themselves by commas but separate them by '-'s. e.g., a complex UCd might be: flux.phot-em.optical,intent.calculated-meas.error,stat.max I'd still like to keep the vocabularies separate, but now it's trivial to parse the UCD. For the moment I tried to minimize the change from the original proposal. Note that this is all much harder in the original proposal. There is no way to tell what anything after the first word is. In that proposal the first word is a property, but all subsequent words can be either properties or concepts. Nor there any lexical definition of what a property is (i.e., any word can be a property). > The document has a lot of signs of a rush job -- is it Uniform or Unified? > (Unified, I think.) I always thought it was Uniform so that wasn't a typo but an error or my part... Sigh... Is flux a 0-level concept? Or is it phot.flux? That I think is fixed in the published version (it's always phot.flux) On p. > 3 you say that units are not part of UCDs, but on p.16 you create a UCD, > phys.degrees;value I wasn't quite sure what the UCD should be there. Maybe phys.angle.separation;value? , that is all about units. On p.12, I really like the > typo(?) in 'pudding' (pubbing). Alas that is also fixed. [That kind of error must reflect some curious things about the mind. I clearly picked the mirror image letter even though the typing motion for it is nothing like 'd'] > > I'm not sure how others have reacted -- have not gone to the UCD list yet to > see. But I was particularly confused by the following things. > > o p.4, you say that > > phot.flux;em.optical;intent.calculated;value > > is equivalent to > > phot.flux;intent.calculated;em.flux;value > > But there must be a mistake here. Shouldn't 'flux' in the second line be > 'optical'? And isn't the first form illegal if alphabetical order is > required? The typos in the UCD were fixed and I hope that would help clarify what I was trying to say. The two UCDs should have been phot.flux;em.optical;intent.calculated;value and phot.flux;intent.calculated;em.optical;value The statement I was trying to make was that there is no natural reason to prefer one of these to the other, so we had to choose an arbitrary rule to try to ensure uniqueness of UCDs. Thus indeed the second is illegal. > > I find the goal of brevity at conflict with the goal of clarity. What does > 'em' mean to a human reader? Why 'src' and not 'source'? Why 'value' and > not 'scalar' (parallel structure to 'vector')? Why default on 'value' in a > otherwise well-defined ontology? I can't really argue with most of these. The tension between various goals it why I tried to list them all together. I would be happy to change to longer words. The default for value was just meant to be a convenience for writers of tables. If it confuses things I'm happy to drop it. I like value rather than scalar because a value can be a vector quantity. E.g., if we have a cell that contains an array of fluxes it's UCD might be phot.spectrum;value That's because the concept of spectrum is inherently non-scalar. A field that had a UCD of phot.spectrum;vector would imply that each cell contained an array of spectra (i.e, that the cell was presumably a 2-d array). However this is no big deal. > > I think if a clear distinction is to be made between attributes and > modifiers, it must be encoded explicitly (i.e., not just based on a list of > magic words). I do not like the semicolons as delimiters; this is not what > they mean in English grammar. (The semicolon in the last sentence was used > properly. The second clause is not necessarily a direct modifier of the > first, but rather is related in some intimate way.) This is fine by me -- I gave an example above using different separators. I think the grammar is just as simple. > > I don't understand how to use the concept 'concept' in a practical sense. > Well I tried to give two examples: If you have a VOTable in an editor how do you find the fields that don't have a defined concept? If a user simply omits the UCD field it's kind of painful to find them. However one can just do a string search for "concept" if the user has entered ucd='concept;value' to explicitly mark that the underlying UCD is unknown. The real reason is given in the last example in section 5. When correlating two tables that describe different kinds of quantities, e.g., sources and observations, I need to be able to describe what the ouput table is. There are two objects in every row so it's a multiplet (in my scheme), but what kind of multiplet? I can't call it a source, and I can't call it an observation, so I need to go up to a more generic word, i.e., concept. Basically it just provides the root for entire concept hierarchy. If we really wanted to be regular, we could start all of the base concepts as using this word... > Your definition of 'pos' does not include solar or planetary coordinate > systems, though later you give an example that does. I don't know what the current hierarchy under pos is... What I'd guess is that it would contain something like: pos.body.lat and pos.body.lon and then the frame modifier would be used to specify which body. [Or maybe I left an inconsistency in from the previous version] > > 'intent' is defined as the 'human context' of the concept. Huh? How are > 'calculated', 'predicted', and 'simulated' anymore human concepts than > 'observed' or 'measured'? Observed and measured would be fine additions here except that they are likely to be considered the default. I.e., a time.exposure;value is assumed to be the measured time, so I don't need to put that in. [Note that meas is short for measurement]. The explanation probably needs to be better, but I think we need some kind of modifier that distinguishes between 'real' values and predicted, scheduled, calculated, ... values. This doesn't come up so much in VizieR tables, but many of the tables that I deal with are riddled with situations where I may have an allocated exposure time, a predicted exposure time and an actual exposure time. So something is assumed to be actual/measured/observed unless an intent is specified. > > In 4.4 you insist that full words should be used ('electron' instead of > 'el'), but at the same time assert that 'phys', 'temp', 'em', etc., are all > ok. I don't have a horse in this race... I tried to match the usage of the previous paper, but I'd be happy to go either way. > > Example 2 (p.14) does not convey to me anything semantically different if I > disregard your comments. How am I supposed to understand something about > guide stars and plate centers from the structure of the UCDs alone? I take > issue with your assertion that "both software and humans should have no > trouble distinguishing the very different semantics of the two tables." > Well... I'd hope that by looking at the table UCD, you would immediately note that one table returned source information and the other returned observation information. That's no small matter. The structure immediately shows which concept is subordinate to the other. The actual semantics of the relationship were not described. You could do that if you want that level of detail. I'm not sure what the right UCDs are. E.g., in the source table might have included (hope the indentation survives the mail): obs.instance meta.id;value pos;meas.center pos.eq.ra;value pos.eq.dec;value I guess if we really want to include the concept of a guide star in the UCD hierarchy, they probably belong in the base concept or maybe in frame somehow, but I think this is too detailed. If we went ahead with it... The guide star might be src;frame.usage.guiding;instance meta.id;value pos.instance Note that in the first case it's the position that got the extra information, because the observation is just a standard observation (as far as we know). In the second case we're suggesting that this is a special kind of source. But I don't think I want to put that in the relatively simple examples. What I was trying to show was how the need for main columns has disappeared and that we could get source or observation information from either table with equivalent ease. > I don't like 'arith' as a concept. 'math' would be ok. If we need it at > all. Well I did try to discourage it... I have no problem with math. > > I don't like 'soft' as a concept. Is it so bad to just say 'software'? All > this stuff will be encoded in XML, which is notoriously verbose. If we > chose unclear abbreviations we will obscure whatever semantic meaning is to > be found. Fine with me... > > OK, a lot of these criticisms are not really directed to you, but to the > predecessor document. I understood your presentation in Strasbourg (I > thought) but do not follow the document sufficiently well that I would ever > be comfortable promoting it forward. I did not like Roy and Sebatien's > premise that concept and property could morph, one into the other, depending > on context. I do like your attempt to structure things more rigidly. It > seems to me not rigid enough. And when I ran into phys.degrees I felt like > the whole thing was falling down around me. The concept is an angular > distance, which of course can be expressed in degrees, radians, arcsec, etc. Agreed... {see above) > > It might be worth our time to look at the AIPS++ measures definitions. If I > were to construct a quick hierarchy, what we are trying to do here is > distinguish various sorts of measurements, metadata about those > measurements, and metadata about the people/organizations associated with > those measurements. So our fundamental concept is a measurement, of which > there are various sorts: > > measurement > photometric > spectroscopic (which is just photometric per wavelength in an ordered sort > of way) > astrometric ('pos') > temporal > instrumental > > Ancillary information about measurements comes in the form of metadata: > > metadata > identifiers > people > organizations > > And we may have some special classes: > > software > source (to collect measurements of an object in space-time) > > Measurements are taken in bandpasses, and in certain coordinate frames, and > from either the real universe or from computer simulations. A bandpass is a > 'frame' restricting coverage in the em-spectrum. A coordinate frame > describes a restriction on the spatial coverage. The idea of 'intent' has > nothing to do with anything; it is simply a mode of collecting measurements. > > Allright, enough of my rantings for this evening. I applaud your attempt to > add rationality to Roy and Sebastien's work, but feel we still have some way > to go. > Thanks... I don't disagree with what you are saying and I hope that we can a least reopen the discussion. Tom From owner-dm@eso.org Wed Oct 22 19:49:21 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9MHj2Kp010723 for ; Wed, 22 Oct 2003 19:45:02 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9MHj2VQ010721 for dm-outgoing; Wed, 22 Oct 2003 19:45:02 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dm@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9MHhqKp010439; Wed, 22 Oct 2003 19:43:52 +0200 (MEST) Received: from othello.physics.gla.ac.uk (othello.physics.gla.ac.uk [130.209.204.200]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9MHhpB1024875; Wed, 22 Oct 2003 19:43:51 +0200 (CEST) Received: from ptolemy.astro.gla.ac.uk ([130.209.45.140]) by othello.physics.gla.ac.uk with esmtp (Exim 4.14) id 1ACN1Q-0008PO-QR; Wed, 22 Oct 2003 18:43:48 +0100 Received: from norman (helo=localhost) by ptolemy.astro.gla.ac.uk with local-esmtp (Exim 3.35 #1) id 1ACN1Q-0003Ho-00; Wed, 22 Oct 2003 18:43:48 +0100 Date: Wed, 22 Oct 2003 18:43:48 +0100 (BST) From: Norman Gray To: Thomas McGlynn cc: ucd@ivoa.net, , Subject: Re: A suggested revision for UCDs In-Reply-To: <3F9588DF.3030805@lheapop.gsfc.nasa.gov> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Spam-Score: -2.0 (--) X-Scanner: exiscan for exim4 (http://duncanthrax.net/exiscan/) *1ACN1Q-0008PO-QR*bN0SIfGukkA* X-Othello-SMTP: True X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-dm@eso.org Precedence: bulk Reply-To: Norman Gray X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Greetings, all, and Tom in particular. On Tue, 21 Oct 2003, Thomas McGlynn wrote: > > A few minutes ago I uploaded a version of my suggested revised > proposal for UCDs to the Twiki. This is just a Word version since > I don't have a PDF generator handy. The URL is > http://www.ivoa.net/internal/IVOA/IvoaUCD/UCD-1.9.9b.doc I've appended a (longish) set of comments below. I've just noticed that Bob has forwarded a long set of comments to the list. I haven't read those yet. By the way, I notice that this announcement/discussion has been posted to no fewer than _three_ lists, namely ucd, dm and dal. It would be at the very least neater if it were on only one -- ucd@ivoa.net is the obvious one. What do folk think -- are there folk on the other two lists who have an interest in this and aren't on the ucd@ivoa.net list? I'm sure I'm not the only one to find Tom's proposal very thought-provoking. The suggestions bring up several new use-cases; and the idea of the `local' atom in particular is valuable, and a gap in the 1.9.9 proposals (though I'd put it in a different place). I think there are very likely several places in the 1.9.9 proposals which are underspecified, and some where I personally would probably explain things slightly differently from Roy and Sebastien, but these are editorial matters. I have a few difficulties with some aspects of Tom's proposal, however, which I'll discuss here, and add a few more general remarks at the end. I'm speaking for myself of course, rather than the group of authors, and thus it's probable that my opinion and interpretation of some 1.9.9 points is at variance with others in the group, or goes beyond what the document aims to say (which would be a useful datapoint). Most urgent, I think, is Tom's discussion, in his section 4.5, of the distinction between his proposals and the 1.9.9 ones. These are crucial, since these criticisms are what would ultimately justify replacing the 1.9.9 proposals with Tom's more complicated ones. In the 1.9.9 proposals, the function of a word is always the same: some things such as `src' are concepts (and only concepts), and every other word names a property. The distinction is that concepts can't have a value, but can have properties; and a property always has a value. Now, the property;concept _pair_ also names a concept, which can therefore have properties in turn (this has the same potential as Tom's proposals for generating long UCDs in principle, but probably very unlikely in practice). There will doubtless be some rather formal language which makes this cast-iron, but it's actually fairly intuitive once you get the property/concept dichotomy and read `;' as `of a' or something like that. Section 3.1 in the 1.9.9 proposals -- the crucial section of the document, for which everything else is to some extent just scaffolding, and without which the rest of the document makes rather less sense -- is what attempts to describe this. Perhaps that explanation needs work. At any rate, I do not believe that one has to sign up to the (basically ontology-inspired) language in that section in order to use the UCDs thus justified. Indeed, it might be useful for that section to be split into two, one to communicate the underlying idea to folk who simply want to _use_ UCDs, and another to reexpress it more formally for the ontology enthusiasts. In his section 4.5, Tom also remarks that ``Indeed I'm not sure that any string of words can be determined to be illegal in the old scheme''. I'd probably agree in outline: there are significantly fewer rules necessary in the 1.9.9 proposals than in Tom's proposals. The only place a base concept can go is in the right-most position, and thus you can't have a concept sitting on its own, since the left-most position is the name of the property, the value of which is the number/column/whatever which has been annotated by this UCD (the syntactic mechanism for making that annotation is outside of scope for the UCD proposals, I'd think). Also, there are some property-concept pairs that make no sense, such as stat.err;src. But that's about it -- you don't need any more rules than that. Tom constructs an `arith.diff;arith.sum;phot.flux;...' UCD. That does look unwieldy (but note there's no need for parentheses in the 1.9.9 proposals), but I get the impression that the `arith' UCD tree was to some extent a kite being flown, and I for one would be surprised if it made it much beyond this version, partly because it would seem to encourage such odd-looking UCDs. Also, there's no tying of one table to another in the 1.9.9 proposals -- I'd think that was out of scope for UCD (and quite properly so: I'll mention this below). The 1.9.9 proposals allow no ambiguity in the way that UCDs are written: properties queue up in front of the single base concept, and ordering matters, so that stat.max;stat.err;phot.flux is different from stat.err;stat.max;phot.flux. More specific points in Tom's proposal, in document order rather than any other (section references are to Tom's document): Section 4.1: Bringing the number of terms up to three -- concept, attribute and modifier -- reminds me of the qualifier/modifier idea that was in previous versions of the draft, which I still think is an unstable distinction, and which Roy and Sebastien thankfully managed to get rid of by simplifying the syntax down to just concept plus properties (but see below). Also, there's no syntactic distinction between modifiers and attributes, so in order to apply the extra ordering rules for those, or even to break the UCD into its three parts, you have to know which words are of which type. That is, you can't do it at parse time. Section 4.1.2 (not an important point, I don't think): I'm puzzled at the requirement that words in the non-standard namespace must be distinct from all words in the IVOA namespace. The point of having a namespace is to make this possible, or (since such duplication would surely be condemned as bad practice) at least not an error. The rule also means that if a new word were added to the IVOA namespace which happened to match a word in a private namespace, the namespaced UCDs would thereby suddenly become invalid, with no change in the spec. Section 4.2.2: The `intent' modifier has no corresponding notion in the 1.9.9 proposals, but it's not clear to me where in those proposals this would fit in, and I think this is a _problem_ for the 1.9.9 proposals. I can see how it would fit in to what I take the underlying 1.9.9 model to be, but not into the serialisation of that model that the 1.9.9 syntax represents. I can see three approaches to this problem within the general framework of the 1.9.9 proposals. (i) Rule it out of scope: it's not UCD's problem to talk about what values are intended to be, since they're only for data discovery, and are not required to be capable of driving analysis, so that if this `intent' distinction matters to you, you're going to have to understand the utype somehow. (ii) Add modifiers like this to the 1.9.9 model and syntax: that's potentially quite a lot of work, since it would require thinking very clearly about just what the distinction is between modifiers and properties, _and_ working out a usable syntax for adding them in -- they _have_ to be distinguishable at parse time. (iii) Think about it more and discover a way they can be viewed as properties in a principled way. The point isn't just about this `intent' modifier: if we can convince ourselves that there are things like `intent' (and that they're in scope) which are in principle qualitatively distinct from properties (and I would at least dispute that `em' and `frame' count here), then that has to be dealt with. Perhaps this example will help us find the stable distinction between `qualifiers' and `modifiers' that escaped us in earlier versions. Section 4.2.3: The `value', `vector', `instance' and `multiplet' attributes seem overly complicated. The `value' attribute is not required in the 1.9.9 proposals because all properties have a value, namely the value they're being used to annotate. The other three seem artefacts of the `complex UCDs' which Tom is introducing in these proposals. These complex UCDs seem problematic to me because they seem tightly bound to VOTable. That destroys the orthogonality of the UCD and VOTable specs (the W3C has had _terrible_ trouble with non-orthogonal specs, tying itself in knots trying to resolve their dependencies on each other), and makes it harder to use UCDs in other contexts, such as queries. I feel that UCDs should be seen as annotating a `thing', whether that `thing' be a value, a column, a group, or a query `phrase', and it should be the responsibility of whatever defines the syntax of that annotation (that is, VOTable or SIA) to define precisely what the thing is that the annotation applies to. Thus, VOTable might say that when a UCD appears in a then it indicates a set of relationships between the corresponding entries of the table; when it appears in a it means something different; and so on. Dealing with the typing and complexity issues of this in a general way within the UCD spec would surely make it impossibly unwieldy and limit its scope. This is also a general worry for all of Tom's Section 5; I really think this should be out of scope for UCD, to the extent that Tom's ``The grouping does not describe the semantics of the relationship. That is the role of UCDs'' would be much better as ``The grouping describes (some of?) the semantics of the relationship. That is not the role of UCDs''. This is a can of worms. Section 4.2.3 (local): I agree this is a gap in the 1.9.9 proposals. Another way of dealing with it would be to say that a UCD `local.X' meant exactly the same as the `X', but was not comparable with it. More general points: Tom's document seems to discuss his proposals in object terms. However the property-concept parts of the UCD proposal are _not_ an object model, and if you cram them into an object model, they won't fit, and the result will inevitably look like a mess, and look backwards. The model is simpler than this, however: things which are purely concepts (such as `src') don't have values. Concepts do have properties though, and these properties have numeric values, namely the numeric values we're trying to annotate with this UCD. As regards ordering, yes, as Tom said, it doesn't fundamentally matter, and it's just a matter of syntax, rather than of the model. However having the property first seems natural, since it's this which posesses the numerical value which is being annotated, and so it's this which I would have thought it best would be shown up-front. Now, there is a _vague_ object model implicit in the construction of the UCD words like `pos.eq.ra', but this is only because, along with the replacement of underscores with dots, came the explicit freedom to crop each word at a dot from the right, and use the result as a UCD word also. This prompts a natural perception of the words as hierarchical, or object-oriented if you must. The actual words are basically little changed from the original UCDs, though there's a review of these under way. These words weren't the main point of the UCD2 proposals. At present these words are those mined from the column names actually occurring in the databases in the CDS collection; they are thus unprincipled. Whether this is a good or a bad thing is an open question. I'm sure it is this which causes some people (I'm thinking of Gerard Lemson and Pat Dowler) to gasp and, in their poster, pick out pos_eq_ra for special deprecation as incoherent. If you believe that principled generation of UCD words would be a Good Thing (and that would probably be my prejudice), then I suspect that paths in (say) Gerard and Pat's model would be a good way to do it (do Gerard and Pat claim that every UCD word is thus expressible?). If you believe, on the other hand, that the mined nature of the words is of primary importance (and I can see the force of that, too), then they might need little more than a review or tidy-up, to make sure that the `croppability' is reasonable in fact, and that the implications, or suggestions, of the words chosen do in fact fit in with a properties-based model (or whatever we end up with). Phew! I think that's probably quite enough for just now -- I should let someone else get a word in. All the best, Norman -- --------------------------------------------------------------------------- Norman Gray http://www.astro.gla.ac.uk/users/norman/ Physics and Astronomy, University of Glasgow, UK norman@astro.gla.ac.uk From owner-ucd@eso.org Wed Oct 22 20:38:35 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9MIYOKp029374 for ; Wed, 22 Oct 2003 20:34:24 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9MIYNrQ029373 for ucd-outgoing; Wed, 22 Oct 2003 20:34:23 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9MIXkKp029151; Wed, 22 Oct 2003 20:33:46 +0200 (MEST) Received: from mail630.gsfc.nasa.gov (mail630.gsfc.nasa.gov [128.183.190.39]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9MIXes3006523; Wed, 22 Oct 2003 20:33:40 +0200 (CEST) Received: from gsfc.nasa.gov (ram.gsfc.nasa.gov [128.183.114.136]) by mail630.gsfc.nasa.gov (8.12.8/8.12.5) with ESMTP id h9MIXaAM007111; Wed, 22 Oct 2003 14:33:36 -0400 Message-ID: <3F96CE02.8020804@gsfc.nasa.gov> Date: Wed, 22 Oct 2003 14:35:46 -0400 From: Ed Shaya User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.4) Gecko/20030529 X-Accept-Language: en-us, en MIME-Version: 1.0 To: Ed Shaya , dm@ivoa.net, dal@ivoa.net, ucd@ivoa.net Subject: UCD changes on top of McGlynn's changes Content-Type: multipart/mixed; boundary="------------010506050500090703000306" X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Ed Shaya X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 This is a multi-part message in MIME format. --------------010506050500090703000306 Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit I have made numerous tracked changes in the 1-9.9b of McGlynn and created a 1-9.9c. So if one has a recent version of Word one can accept or reject these changes as seen fit. I think someone will need to post this to the UCD and dal lists cause I am not on them. Here are some "highlights" -------------------------------------------------------------------------- The term property was used in a confusing manner. Everything was at some point in the specification referred to as a property including the basic concept as well as the attribute and modifier. So, I changed attribute property to attribute and modifier property to modifier. I think this is pretty good but it is missing something. The modifiers are in effect extending the hierarchicial tree of basic concepts into the virtual tree of full concepts. This is not mentioned and probably should be. But, if it is true then sometimes the order of the modifiers should make a difference. I don't have an example but I am worried that there will be concepts that require A;B;C and other concepts that are A;C;B but they are not the same. I don't see how to ensure that that never happens. ------------------------------------------------------------ Word and atom were a bit confused. Atoms looked like words to me and Words were clearly composed of several words (not good). There was no atom in the Backus-Naur notation. But there were examples of atoms of the physics type (yikes). So I made the following simplification. atom -> word word -> term word-component -> word ----------------------------------- I changed a few occurrence of "column" to "contents" so that it did not seem that this was for tables only. And so the Contents in "UCD" would be meaningful. -------------------------------------- Why is there a meas.error and a stat.erro, and one is a concept and one is an attribute? Perhaps this was suppose to be a stat:max? 1 x1:experimental.quantity;x2:new.modifier;stat.error ---------------------------------------------------- Why not have a different symbol to separate the attributes from the base and modifiers? pos.eq;phys.electron#value;vector pos.eq;phys.electron#stat.error;vector This is clearer. It says, if you are looking for instances of the concept of a positional measure of electrons, here it is. By the way it is in vector format and there is an error associate with it, you may need to transform this format. Queries will be keying on the concept and so it should be cleanly separated. If the query finds additional attribute information it may grab them for completeness even if they were not specificied in the query. --------------------------- Why not allow a namespaced term to reuse existing term? That is what namespace is for! 1 phot.flux;x1:meas.error Namespace reuses existing term-------------------------- In the Group of pos.eq.ra and pos.eq.dec the UCD of the group should be pos.eq, not pos.instance. The "eq" is there because one should be as specifying as possible. The instance should not be there since this is a table level term and is redundant here. ------------------------------------------------------------ I don't buy the idea that the main pos is always in the least indented or grouped column. This is a extremely fragile and restrictive way to go. There are many ways that the targets are in a more groups than the plate positions or the guide stars. What if the target stars have position groups and so one wants a second grouping of ra, dec l,b or what if the grouping of stars is by cluster or by spectral type or by accuracy of measurements etc? That is not to say that I like the idea of a main UCD. Rather, the best way is to ensure that the structural container of the data has a way of refering the properties to the objects that has these properties. A quanitty needs to have a isPropertyOf attribute that refers to the object. So, a positional property column should have isPropertyOf="column(starName)". The default could be isPropertyOf=column(1). --------------------------------------------------------- Finally. I find it curious that this system makes no descrimination between properties of objects (color, brightness, distance, size) and objects (electrons, atoms, planets, stars, galaxies). Every time one uses a UCD-property there must be implicitly a UCD-object that has been left off. A brightness is always of a star or a planet or a human. A query system must then be able to infer this from other metadata in the dataset. Therefore one needs to ensure that every data set has somewhere atleast one UCD-object. This will be hard to do if they are not somehow separated out I just wanted to point that out. It may or may not be a fatal flaw. 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AAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAA AAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAA AAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAA AAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAAA= --------------010506050500090703000306-- From owner-ucd@eso.org Wed Oct 22 21:25:42 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9MJLoKp022914 for ; Wed, 22 Oct 2003 21:21:50 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9MJLoew022913 for ucd-outgoing; Wed, 22 Oct 2003 21:21:50 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9MJKHKp021778; Wed, 22 Oct 2003 21:20:17 +0200 (MEST) Received: from nrcvicex1.hia.nrc.ca (nrcvicex1a.hia.nrc.ca [204.174.103.8]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9MJKFB1026989; Wed, 22 Oct 2003 21:20:16 +0200 (CEST) Received: from frodo (cadc-nat.vic.hia.nrc.ca [204.174.103.36]) by nrcvicex1.hia.nrc.ca with SMTP (Microsoft Exchange Internet Mail Service Version 5.5.2653.13) id VHHWQ495; Wed, 22 Oct 2003 12:20:12 -0700 Content-Type: text/plain; charset="iso-8859-1" From: Patrick Dowler Organization: National Research Council Canada To: Norman Gray Subject: Re: A suggested revision for UCDs Date: Wed, 22 Oct 2003 12:19:29 -0700 User-Agent: KMail/1.4.3 Cc: ucd@ivoa.net, dm@ivoa.net, dal@ivoa.net References: In-Reply-To: MIME-Version: 1.0 Message-Id: <200310221219.29068.patrick.dowler@nrc-cnrc.gc.ca> X-Scanned-By: MIMEDefang 2.35 X-MIME-Autoconverted: from 8bit to quoted-printable by apollo.hq.eso.org id h9MJKFB1026989 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id h9MJKoKp022446 Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Patrick Dowler X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 On Wednesday 22 October 2003 10:43, Norman Gray wrote: > I'm sure it is this which causes some people (I'm thinking of Gerard > Lemson and Pat Dowler) to gasp and, in their poster, pick out pos_eq_ra > for special deprecation as incoherent. If you believe that principled > generation of UCD words would be a Good Thing (and that would probably > be my prejudice), then I suspect that paths in (say) Gerard and Pat's > model would be a good way to do it (do Gerard and Pat claim that every > UCD word is thus expressible?). That particular example was chosen to show that the different parts of the POS_EQ_RA_MAIN (UCD1) are quite different types of things with different realtionships to the thing being described. In the data model, POS is the "position" phenomenon, EQ is a particular ReferenceSystem, RA is one component of a point (the type used to represent a position in that ReferenceSystem). I still don't know that MAIN would belong in a data model. It isn't "incoherent" so much as it includes some very different kinds of things. In the concept;property style of UCD2, I don't think it is inconsistent with the data model we presented. The difference between UCD and DM is that in a model one explicitly states the relationship between the concept and the property, So, for example, in our DM we are expliclty saying that the relationship between a position and the ReferenceSystem is a different relationship that between the position and the RA (a component of the data type/structure). UCD2 leaves the relationship implicit by having only one relationship: "propertyOf". Whether that's good or bad thing is an open issue. -- Patrick Dowler Tel/Tél: (250) 363-6914 | fax/télécopieur: (250) 363-0045 Canadian Astronomy Data Centre | Centre canadien de donnees astronomiques National Research Council Canada | Conseil national de recherches Canada Government of Canada | Gouvernement du Canada 5071 West Saanich Road | 5071, chemin West Saanich Victoria, BC | Victoria (C.-B.) From owner-ucd@eso.org Wed Oct 22 22:20:11 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9MKFPKp013795 for ; Wed, 22 Oct 2003 22:15:25 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9MKFPdf013794 for ucd-outgoing; Wed, 22 Oct 2003 22:15:25 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9MKEqKp013683 for ; Wed, 22 Oct 2003 22:14:52 +0200 (MEST) Received: from milkyway.gsfc.nasa.gov (lheapop.gsfc.nasa.gov [128.183.16.62]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9MKEnB1028089 for ; Wed, 22 Oct 2003 22:14:50 +0200 (CEST) Received: from lheapop.gsfc.nasa.gov (silk3.gsfc.nasa.gov [128.183.18.68]) by milkyway.gsfc.nasa.gov (8.12.9/8.12.9) with ESMTP id h9MKEYTd029399; Wed, 22 Oct 2003 16:14:35 -0400 Message-ID: <3F96E52F.8060402@lheapop.gsfc.nasa.gov> Date: Wed, 22 Oct 2003 16:14:39 -0400 From: Thomas McGlynn Organization: NASA Goddard Space Flight Center User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.5) Gecko/20030925 X-Accept-Language: en-us, en MIME-Version: 1.0 To: Norman Gray CC: ucd@ivoa.net Subject: Re: A suggested revision for UCDs References: In-Reply-To: Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Thomas McGlynn X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi Norman, Thanks for your comments. I've got some responses for some, I'm glad you found some good in this! In keeping with your suggestion I've only sent this to the UCD group. I sent the original proposal to the other groups since I thought the use of complex UCDs is relevant, but I'm sure we can live without three copies and hopefully they have subscribed so they can hear this interesting(!?) debate. Tom Norman Gray wrote: ... > > Most urgent, I think, is Tom's discussion, in his section 4.5, ... That was really meant to be at the end of section 4, rather than part of 4.5... >... of the > distinction between his proposals and the 1.9.9 ones. These are crucial, > since these criticisms are what would ultimately justify replacing the > 1.9.9 proposals with Tom's more complicated ones. > > In the 1.9.9 proposals, the function of a word is always the same: > some things such as `src' are concepts (and only concepts), and > every other word names a property. The distinction is that > concepts can't have a value, but can have properties; and a property > always has a value. Now, the property;concept _pair_ also names a > concept, which can therefore have properties in turn (this has the > same potential as Tom's proposals for generating long UCDs in > principle, but probably very unlikely in practice). There will > doubtless be some rather formal language which makes this cast-iron, > but it's actually fairly intuitive once you get the property/concept > dichotomy and read `;' as `of a' or something like that. Well there are two distinct issues here. First lexically how can I tell what is a property and what is a concept? In 1.9.9 there is no way to tell. The only lexical statement it makes is that the first word is a property. What about the second word, or the third? The 1.9.9 proposal allows properties that modify other properties. The second issue is the semantic confusion. The second word can be (according to section 4.2 in 1.9.9) a concept referred to another property referred to information related to the primary word. In section 3.4 in defining the error in RA of a galaxy we have the phrase We identify the central property as "error", and the concept as right ascension", with a subsidiary word about "galaxy". So in fact version 1.9.9 has all three of concept property and modifier but just tries to hide the fact and doesn't give you any way of telling which is which... Suppose I give one a UCD of word1;word2;word3 Does word3 modify word1 or do both of them modify word1? No way to tell. stat.error;phot.flux;em.optical (word3 modifies word2) or phot.flux;em.optical;src.galaxy (word3 modifies word1) There is an explicit statement that some things (pos.eq.ra) are sometimes concepts and sometimes secondary words and the rules make it trivial to build UCDs that are simply incomplete semantically. stat.error is a perfectly valid UCD but it has no rooted semantic content. You may say "Well what about meta.id, isn't that the same?" Not really because I can suggest (and indeed I do suggest) that UCDs need to be interpreted in the context of what the table is about. So for a source table meta.id refers to the id for a source, for an observation table meta.id refers to the id for a source. But what does stat.error refer to.... The error in the source? That doesn't make sense. > > Section 3.1 in the 1.9.9 proposals -- the crucial section of the document, > for which everything else is to some extent just scaffolding, and without > which the rest of the document makes rather less sense -- is what attempts > to describe this. Perhaps that explanation needs work. At any rate, I do > not believe that one has to sign up to the (basically ontology-inspired) > language in that section in order to use the UCDs thus justified. > Indeed, it might be useful for that section to be split into two, one to > communicate the underlying idea to folk who simply want to _use_ UCDs, > and another to reexpress it more formally for the ontology enthusiasts. > > In his section 4.5, Tom also remarks that ``Indeed I'm not sure that any > string of words can be determined to be illegal in the old scheme''. > I'd probably agree in outline: there are significantly fewer rules > necessary in the 1.9.9 proposals than in Tom's proposals. The only place > a base concept can go is in the right-most position, and thus you can't > have a concept sitting on its own, since the left-most position is the > name of the property, the value of which is the number/column/whatever > which has been annotated by this UCD (the syntactic mechanism for making > that annotation is outside of scope for the UCD proposals, I'd think). > Also, there are some property-concept pairs that make no sense, such > as stat.err;src. But that's about it -- you don't need any more rules > than that. > > Tom constructs an `arith.diff;arith.sum;phot.flux;...' UCD. That does > look unwieldy (but note there's no need for parentheses in the 1.9.9 > proposals), but I get the impression that the `arith' UCD tree was to > some extent a kite being flown, and I for one would be surprised if it > made it much beyond this version, partly because it would seem to encourage > such odd-looking UCDs. Also, there's no tying of one table to another > in the 1.9.9 proposals -- I'd think that was out of scope for UCD (and > quite properly so: I'll mention this below). > Sorry that's a typo... Should have said tying of one column to another. > The 1.9.9 proposals allow no ambiguity in the way that UCDs are > written: properties queue up in front of the single base concept, and > ordering matters, so that stat.max;stat.err;phot.flux is different > from stat.err;stat.max;phot.flux. What I call attributes and the properties you specify here are indeed largely unambiguous in both cases. However what I call modifiers and what 1.9.9 calls either subsidiary words or 'information related to the primary word' are less clear. E.g., suppose I'm detecting circularly polarized light in the radio. That natural UCD for this would be: phot.flux;em.radio;em.polarized;circular or is it phot.flux;em.polarized;circular;em.radio or do we have to multiply the size of the vocabulary to add polarized and polarized.circular (and the other variants) to every wavelength spec we have? That seems silly... So we need to fix that. There's a similar problem with arith (another nail for the coffin perhaps) is it arith.sum;property1;property2 or arith.sum;property2;property2 And this general idea that properties can refer to other properties in an uncontrolled way... Here's a UCD describing the flux of galaxies... phot.flux;em.optical;src.galaxy or is it phot.flux;src.galaxy;em.optical ? E.g., suppose I have a column that is the maximum flux from any of three wavebands. Can I write stat.max;flux.phot;em.optical;flux.phot;em.xray;phot.flux;em.radio I hope not, but the document seems to encourage it. This would be illegal in the revision since it includes three base concepts. > > > > > More specific points in Tom's proposal, in document order rather than > any other (section references are to Tom's document): > > Section 4.1: Bringing the number of terms up to three -- concept, > attribute and modifier -- reminds me of the qualifier/modifier idea > that was in previous versions of the draft, which I still think is an > unstable distinction, and which Roy and Sebastien thankfully managed > to get rid of by simplifying the syntax down to just concept plus > properties (but see below). ... but they haven't, they have just not told you about the difference. The words stat.max, em.optical, and phot.flux have distinct grammar rules in how they are used in 1.9.9 but you have no way to tell that. I.e., phot.flux can appear as he initial word or any subsidiary word but can never appear before stat.max or any other word of the class I would call attribute. em.optical can appear after words of the same class as phot.flux and possibly after words of the same class as itself. stat.max can appear anywhere in a UCD but it really should appear either before either a word of the class of phot.flux or a word of its own class. There are three kinds of words and we should just recognize that in the grammar. Also, there's no syntactic distinction > between modifiers and attributes, so in order to apply the extra > ordering rules for those, or even to break the UCD into its three > parts, you have to know which words are of which type. That is, you > can't do it at parse time. Sure you can. At least if the number of modifiers remains small. Note that table writers should have access to appropriate documentation when writing their tables (or writing the software that writes tables) so even if it gets more complex the writers have no problems and the readers don't care. See my response to Bob on this issue. I've suggested that all modifiers be put in the frame tree, though largely to address this issue. > > Section 4.1.2 (not an important point, I don't think): I'm puzzled at > the requirement that words in the non-standard namespace must be > distinct from all words in the IVOA namespace. The point of having a > namespace is to make this possible, or (since such duplication would > surely be condemned as bad practice) at least not an error. The rule > also means that if a new word were added to the IVOA namespace which > happened to match a word in a private namespace, the namespaced UCDs > would thereby suddenly become invalid, with no change in the spec. > This idea is copied from the previous proposal. I think the idea is that we don't want proliferation of new uncontrolled UCDs. I put this in a separate section, but I believe the content is the same as the previous proposal. I leave it to others to decide which is right. > Section 4.2.2: The `intent' modifier has no corresponding notion in > the 1.9.9 proposals, but it's not clear to me where in those proposals > this would fit in, and I think this is a _problem_ for the 1.9.9 > proposals. I can see how it would fit in to what I take the > underlying 1.9.9 model to be, but not into the serialisation of that > model that the 1.9.9 syntax represents. I can see three approaches to > this problem within the general framework of the 1.9.9 proposals. (i) > Rule it out of scope: it's not UCD's problem to talk about what values > are intended to be, since they're only for data discovery, and are not > required to be capable of driving analysis, so that if this `intent' > distinction matters to you, you're going to have to understand the utype > somehow. That's not acceptable for observation tables. We frequently have multiple columns in a table which differ only in intent (proposed and actual exposure times), predicated and actual times of events, predicated and actual fluxes and we need to know which to use for various purposes. Spectral fitting will be sadly served if we can't put distinguish the calculated and actual spectra. What happens when we want to compare simulated and real data? (ii) Add modifiers like this to the 1.9.9 model and syntax: > that's potentially quite a lot of work, since it would require > thinking very clearly about just what the distinction is between > modifiers and properties, _and_ working out a usable syntax for adding > them in -- they _have_ to be distinguishable at parse time. I'm happy to trade intent for frame.human and put all the modifiers in frame. (iii) > Think about it more and discover a way they can be viewed as > properties in a principled way. The point isn't just about this > `intent' modifier: if we can convince ourselves that there are things > like `intent' (and that they're in scope) which are in principle > qualitatively distinct from properties (and I would at least dispute > that `em' and `frame' count here), then that has to be dealt with. > Perhaps this example will help us find the stable distinction between > `qualifiers' and `modifiers' that escaped us in earlier versions. Personally I take a modifier as something that limits the context of a concept. > > Section 4.2.3: The `value', `vector', `instance' and `multiplet' > attributes seem overly complicated. The `value' attribute is not > required in the 1.9.9 proposals because all properties have a value, > namely the value they're being used to annotate. The word value is the price I pay for making sure attributes, concepts are distinct. Personally I think it's worth it. The other three seem > artefacts of the `complex UCDs' which Tom is introducing in these > proposals. Vector is not... It's simply to warn the user that the column has is a vector. While VOTables have a array attribute that does this, I don't want to tie this proposal to VOTables... More on that below. .These complex UCDs seem problematic to me because they > seem tightly bound to VOTable. That destroys the orthogonality of the > UCD and VOTable specs (the W3C has had _terrible_ trouble with > non-orthogonal specs, tying itself in knots trying to resolve their > dependencies on each other), and makes it harder to use UCDs in other > contexts, such as queries. I feel that UCDs should be seen as > annotating a `thing', whether that `thing' be a value, a column, a > group, or a query `phrase', and it should be the responsibility of > whatever defines the syntax of that annotation (that is, VOTable or > SIA) to define precisely what the thing is that the annotation applies > to. Thus, VOTable might say that when a UCD appears in a then > it indicates a set of relationships between the corresponding entries > of the table; when it appears in a it means something > different; and so on. Dealing with the typing and complexity issues > of this in a general way within the UCD spec would surely make it > impossibly unwieldy and limit its scope. This is also a general worry > for all of Tom's Section 5; I really think this should be out of scope > for UCD, to the extent that Tom's ``The grouping does not describe the > semantics of the relationship. That is the role of UCDs'' would be > much better as ``The grouping describes (some of?) the semantics of > the relationship. That is not the role of UCDs''. This is a can of > worms. I think this is completely wrong. The grouping proposal has no special relationship to VOTables other than that they happen to support it. [Or they may soon!] Any other structure that supports groupings of tables would do just as well. This is a fairly natural attribute of object relational as well as hierarchical databases. It just that VOTables have finally decided to enable the natural abilities that XML's hierarchical structure supports. > > Section 4.2.3 (local): I agree this is a gap in the 1.9.9 proposals. > Another way of dealing with it would be to say that a UCD > `local.X' meant exactly the same as the `X', but was not > comparable with it. > That's essentially what my proposal mod the order difference. > > > > > More general points: > > Tom's document seems to discuss his proposals in object terms. > However the property-concept parts of the UCD proposal are _not_ an > object model, and if you cram them into an object model, they won't > fit, and the result will inevitably look like a mess, and look > backwards. The model is simpler than this, however: things which are > purely concepts (such as `src') don't have values. Concepts do have > properties though, and these properties have numeric values, namely > the numeric values we're trying to annotate with this UCD. Sounds like objects and attributes to me... What's the difference here? But the old proposal doesn't agree anyway! Is phot.flux a concept? Seems like it to me. But it's a property in 1.9.9. Sometimes... In the UCD phot.flux. But it's sort of a concept in stat.err;phot.flux Or is it a property there? I'm not sure and there is no way to tell! By specifying a value attribute I've cleared away this confusion. > > As regards ordering, yes, as Tom said, it doesn't fundamentally > matter, and it's just a matter of syntax, rather than of the model. > However having the property first seems natural, since it's this > which posesses the numerical value which is being annotated, and > so it's this which I would have thought it best would be shown > up-front. This is not critical, but since I believe the model is analogous to the object/attribute relationship using the same order that has conventionally been used there is helpful. > > Now, there is a _vague_ object model implicit in the construction of > the UCD words like `pos.eq.ra', but this is only because, along with > the replacement of underscores with dots, came the explicit freedom to > crop each word at a dot from the right, and use the result as a UCD > word also. This prompts a natural perception of the words as > hierarchical, or object-oriented if you must. Well I don't have to but I sure would like to! .. The actual words are > basically little changed from the original UCDs, though there's a > review of these under way. These words weren't the main point of the > UCD2 proposals. > > At present these words are those mined from the column names actually > occurring in the databases in the CDS collection; they are thus > unprincipled. Whether this is a good or a bad thing is an open question. > I'm sure it is this which causes some people (I'm thinking of Gerard > Lemson and Pat Dowler) to gasp and, in their poster, pick out pos_eq_ra > for special deprecation as incoherent. If you believe that principled > generation of UCD words would be a Good Thing (and that would probably > be my prejudice), then I suspect that paths in (say) Gerard and Pat's > model would be a good way to do it (do Gerard and Pat claim that every > UCD word is thus expressible?). If you believe, on the other hand, that > the mined nature of the words is of primary importance (and I can see > the force of that, too), then they might need little more than a review > or tidy-up, to make sure that the `croppability' is reasonable in fact, > and that the implications, or suggestions, of the words chosen do in > fact fit in with a properties-based model (or whatever we end up with). > > As in 1.9.9 I didn't build a complete list but I agree that most words will transfer between the two proposals. From owner-dal@eso.org Wed Oct 22 22:37:47 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9MKXMKp020753 for ; Wed, 22 Oct 2003 22:33:22 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9MKXMYP020749 for dal-outgoing; Wed, 22 Oct 2003 22:33:22 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dal@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9MKWGKp020460; Wed, 22 Oct 2003 22:32:16 +0200 (MEST) Received: from mail.cacr.caltech.edu (mail.cacr.caltech.edu [131.215.145.9]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9MKWEs3010300; Wed, 22 Oct 2003 22:32:15 +0200 (CEST) Received: from SARA (sara.cacr.caltech.edu [131.215.145.107]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id h9MKWDM9025960 (version=TLSv1/SSLv3 cipher=RC4-MD5 bits=128 verify=NO); Wed, 22 Oct 2003 13:32:13 -0700 Message-ID: <01c501c398db$9ef8ef80$6b91d783@cacr.caltech.edu> From: "Roy Williams" To: , , References: <3F96CE02.8020804@gsfc.nasa.gov> Subject: Re: UCD changes on top of McGlynn's changes Date: Wed, 22 Oct 2003 13:32:32 -0700 MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2720.3000 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2727.1300 X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-dal@eso.org Precedence: bulk Reply-To: "Roy Williams" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 All: >From now on, please do not cross-post UCD material to dm and dal. Please send UCD-related posting to ucd@ivoa.net only. Those of you on the other lists, please join the ucd list to continue reading UCD material. Thank You Roy -------- Caltech Center for Advanced Computing Research roy@cacr.caltech.edu 626 395 3670 From owner-ucd@eso.org Wed Oct 22 22:45:32 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9MKfXKp026528 for ; Wed, 22 Oct 2003 22:41:33 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9MKfWkj026527 for ucd-outgoing; Wed, 22 Oct 2003 22:41:32 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9MKevKp026403 for ; Wed, 22 Oct 2003 22:40:57 +0200 (MEST) Received: from milkyway.gsfc.nasa.gov (lheapop.gsfc.nasa.gov [128.183.16.62]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9MKeus3010484 for ; Wed, 22 Oct 2003 22:40:56 +0200 (CEST) Received: from lheapop.gsfc.nasa.gov (silk3.gsfc.nasa.gov [128.183.18.68]) by milkyway.gsfc.nasa.gov (8.12.9/8.12.9) with ESMTP id h9MKesTd031726; Wed, 22 Oct 2003 16:40:54 -0400 Message-ID: <3F96EB5B.8000001@lheapop.gsfc.nasa.gov> Date: Wed, 22 Oct 2003 16:40:59 -0400 From: Thomas McGlynn Organization: NASA Goddard Space Flight Center User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.5) Gecko/20030925 X-Accept-Language: en-us, en MIME-Version: 1.0 To: Ed Shaya , ucd@ivoa.net Subject: Re: UCD changes on top of McGlynn's changes References: <3F96CE02.8020804@gsfc.nasa.gov> In-Reply-To: <3F96CE02.8020804@gsfc.nasa.gov> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Thomas McGlynn X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi Ed, Most of this ounds reasonable to me... Some short (just to show I can do it) comments. Tom Ed Shaya wrote: ... > I think this is pretty good but it is missing something. The modifiers > are in effect extending the hierarchicial tree of basic concepts into > the virtual tree of full concepts. This is not mentioned and probably > should be. But, if it is true then sometimes the order of the modifiers > should make a difference. I don't have an example but I am worried > that there will be concepts that require A;B;C and other concepts that > are A;C;B but they are not the same. I don't see how to ensure that > that never happens. I just haven't seen where it happens... So I'm crossing my fingers! > -------------------------------------- > Why is there a meas.error and a stat.erro, and one is a concept and one > is an attribute? > Perhaps this was suppose to be a stat:max? > > 1 x1:experimental.quantity;x2:new.modifier;stat.error > Probably just missed it when I introduced the meas tree. > > Why not have a different symbol to separate the attributes from the base > and modifiers? > pos.eq;phys.electron#value;vector > pos.eq;phys.electron#stat.error;vector Bob and you both suggested that. Sounds good to me. I'd probably have written the first as just pos.eq;phys.electron#vector > --------------------------- > > Why not allow a namespaced term to reuse existing term? That is what > namespace is for! Talk to Ray and Sebastien. I think they feel that it's best for UCDs to be highly controlled so that namespaces are only used for experimental terms before they are introduced to the standard namespace. Both approaches seem reasonable to me. > ------------------------------------------------------------ > I don't buy the idea that the main pos is always in the least indented > or grouped column. This is a extremely fragile and restrictive way to > go. There are many ways that the targets are in a more groups than the > plate positions or the guide stars. I don't want to suggest that one cannot build tables that would break the proposal. But I was unable to find a circumstance where I couldn't use structure to make the main elements clear. I.e., I'm not trying to cater to every reasonable structure for tables, but trying to see if the proposal allows sufficient flexibility for tables to express mainness assuming they are written by friends. I tried to allude to that with the sense that we'll need templates for how to use structures. What if the target stars have > position groups > and so one wants a second grouping of > > > > ra, dec > > > l,b > > > or what if the grouping of stars is by cluster or by spectral type or > by accuracy of measurements etc? In these examples it would be the responsibility of the table writer to think about how the table could be written to express what readers need to know. If we're allowed the full flexibility of the VOTable grouping structures, then we might have the same fields referenced more than once: near the root so that they are seen to be main, and within some more nested structures. This would use the reference capability. However I'd be interested if we have any actual instances of tables where this is needed or whether it's something that's possible but not very likely. > That is not to say that I like the idea of a main UCD. > Rather, the best way is to ensure that the structural container of the > data has a way of refering the properties to the objects that has these > properties. A quanitty needs to have a isPropertyOf attribute that > refers to the object. So, a positional property column should have > isPropertyOf="column(starName)". The default could be > isPropertyOf=column(1). With references to virtual columns I suspect this is equivalent to what I suggest, but it might be cleaner. > --------------------------------------------------------- > Finally. I find it curious that this system makes no descrimination > between > properties of objects (color, brightness, distance, size) and objects > (electrons, > atoms, planets, stars, galaxies). Every time one uses a UCD-property there > must be implicitly a UCD-object that has been left off. A brightness is > always of a star or a planet or a human. A query system must then be > able to > infer this from other metadata in the dataset. Therefore one needs to > ensure that every data set has somewhere atleast one UCD-object. This > will be hard to do if they are > not somehow separated out I just wanted to point that out. > It may or may not be a fatal flaw. > I guess this is what I'm typically indicting as the table UCD. E.g., the table UCD is the source, but the column UCDs are the properties of the sources. From owner-ucd@eso.org Thu Oct 23 03:07:36 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9N12gv7003732 for ; Thu, 23 Oct 2003 03:02:42 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9N12gp5003731 for ucd-outgoing; Thu, 23 Oct 2003 03:02:42 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9N128v7003645 for ; Thu, 23 Oct 2003 03:02:08 +0200 (MEST) Received: from mail.cacr.caltech.edu (mail.cacr.caltech.edu [131.215.145.9]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9N127B1003819 for ; Thu, 23 Oct 2003 03:02:07 +0200 (CEST) Received: from Ropy (dsl-pb-1504.linkline.com [64.30.223.60]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id h9N125M9030041 (version=TLSv1/SSLv3 cipher=RC4-MD5 bits=128 verify=NO) for ; Wed, 22 Oct 2003 18:02:05 -0700 Message-ID: <05e001c39901$4a189d50$6501a8c0@Ropy> From: "Roy Williams" To: Subject: is UCD out of control? Date: Wed, 22 Oct 2003 18:02:10 -0700 MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Roy Williams" X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 I must say that I find Tom's version of the UCD paper has a number of definite improvements, such as the importance of Groups, with the child inheriting UCD from its parent. However, I find the suggested syntax confusing and muddying. It seems to be going back to the old model of "base + other stuff" that we discussed in Cambridge. What I do not understand is how a machine would parse the other stuff, these modifiers and attribute properties and so on. I do not understand which is a modifier and which is an attribute. The reason we went with the new scheme was that we couldn't imagine writing code to disentangle the Cambridge scheme. In the 1.9.9 document, the first word of the UCD corresponds to the thing that has the units. In "stat.variance; phys.length", we know that the unit is L*L (its a variance). The second word was the concept to which this relates. Everything in UCD2 should be of the form "The of the ". Forget the attempts to justify three words. Leave that for UCD3. Every UCD has at most two words. Keep It Simple! In the 1.9.9 document, we tried to keep as close as we can to the metadata mines -- the 3000 tables of Vizier from which all this comes. We thought that had more validity than somebody (anybody) sitting down and inventing structure. Look at the problems we get when we move away from mining real metadata: Tom thinks that "error" belongs in a tree called "measurement", and the earlier version put it in a tree called "statistics". There is no right or wrong here, just opinion. I pointed this out in the earlier document concerning the "equinox" concept, but that has been deleted. We must make every attempt to follow what 3000 published paper have done -- not push our own opinions. In Tom's paper, there seem to be lots of new attributes (value, vector, multiplet, local, human, soft) that further stretch the scope UCD. If there are multiple values in a table cell, then the VOTable will indicate this in other ways. Perhaps Tom can put in a few more attibutes so we can find out if the data quantitiy is a float or an integer? UCD is about *semantic type*, not all this other stuff. What *real* tables use the "human" section? Are humans base, attribute, or modifier? I think we can all agree that UCD as currently formulated cannot express the complexity inherent in its task. What is really needed is a well-thought RDF vocabulary of predicates and objects, and that is the idea of UCD3. The intention of UCD2 is to provide a stopgap that will be backward compatible when UCD3 arrives. We use only one predicate for now "propertyOf". But Tom has chosen to remove all the discussion of why and what we are doing, where we are going, and driven instead down a road that tries to put a lot of complexity into this string representation. The result is something terribly complicated and not very understandable. Of course the proof is in the pudding. As usual in the VO, we are making a language that is very expressive, then hope to eventually write the code that understands it. So let's think it through now. How do I construct code that "understands" something like "phot.flux; em.optical; intent.calculated; value". I want to know what kind of data structure can be created from this, I want to know how to compare UCDs, I want to know how to convert a UCD into a human-readable description of what it represents. I know how to do these things with the 2-word property/concept style, but not with this grab-bag of attributes and modifiers. In conclusion is my IF ... ELSE clause: IF { we cannot find a killer app for UCD2, if we cannot write code to understand them, we should stick with UCD1, that has been improved and groomed in the last months. Then next year we can make UCD3. } ELSE { I like simplicity. I want to turn every table cell into " of the " so that every UCD2 would have at most two words. } -------- Caltech Center for Advanced Computing Research roy@cacr.caltech.edu 626 395 3670 From owner-ucd@eso.org Thu Oct 23 10:42:02 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9N8eov7001372 for ; Thu, 23 Oct 2003 10:40:50 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9N8eojB001367 for ucd-outgoing; Thu, 23 Oct 2003 10:40:50 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9N8eGv7001112 for ; Thu, 23 Oct 2003 10:40:16 +0200 (MEST) Received: from apollo.le.ac.uk (mailsend.le.ac.uk [143.210.16.125]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9N8eGB1011162 for ; Thu, 23 Oct 2003 10:40:16 +0200 (CEST) Received: from [143.210.36.58] (helo=mail.star.le.ac.uk) by apollo.le.ac.uk with smtp (Exim 4.24) id 1ACb0x-0007RB-I1 for ucd@ivoa.net; Thu, 23 Oct 2003 09:40:15 +0100 Received: (qmail 2570 invoked from network); 23 Oct 2003 08:40:37 -0000 Received: from peneca.star.le.ac.uk (143.210.36.224) by mail.star.le.ac.uk with SMTP; 23 Oct 2003 08:40:37 -0000 Date: Thu, 23 Oct 2003 09:40:37 +0100 (BST) From: Clive Page To: ucd@ivoa.net Subject: Re: A suggested revision for UCDs In-Reply-To: <3F9588DF.3030805@lheapop.gsfc.nasa.gov> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Clive Page X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 On Tue, 21 Oct 2003, Thomas McGlynn wrote: > A few minutes ago I uploaded a version of my suggested revised > proposal for UCDs to the Twiki. This is just a Word version since > I don't have a PDF generator handy. An off-topic note to Tom (and others with the same problem in producing PDFs): Many of us on Unix/Linux systems find Word documents inconvenient; I thought OpenOffice.org might cope with your file, but it produces illegible results without a lot of playing with fonts, and even then was very poor. Not long ago, however, I came across an on-line service for converting Word documents to PDF (or HTML) which seems quite useful: http://www.gobcl.com/ You upload your document and they email you the PDF a couple of minutes later. I haven't received any obvious spam as a result, and don't know what their privacy policy is, but for documents to be published, this doesn't seem important. I don't know why they provide this service free of charge, but I've found it useful. Actually I got an error message when I submitted Tom's recent UCD document, but the PDF came back anyway, and seems ok, still in glorious technicolor. -- Clive Page Dept of Physics & Astronomy, University of Leicester, Tel +44 116 252 3551 Leicester, LE1 7RH, U.K. Fax +44 116 252 3311 From owner-ucd@eso.org Thu Oct 23 14:00:26 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9NBxXv7002755 for ; Thu, 23 Oct 2003 13:59:33 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9NBxX6l002754 for ucd-outgoing; Thu, 23 Oct 2003 13:59:33 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9NBwwv7002607 for ; Thu, 23 Oct 2003 13:58:58 +0200 (MEST) Received: from head-cfa.cfa.harvard.edu (head-cfa.cfa.harvard.edu [131.142.41.8]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9NBwvB1015750 for ; Thu, 23 Oct 2003 13:58:58 +0200 (CEST) Received: from urania.cfa.harvard.edu (urania [131.142.52.147]) by head-cfa.cfa.harvard.edu (8.12.10/8.12.8) with ESMTP id h9NBwveR027594 for ; Thu, 23 Oct 2003 07:58:57 -0400 (EDT) From: Jonathan McDowell Received: (from jcm@localhost) by urania.cfa.harvard.edu (8.12.8p1/8.12.8) id h9NBwv9a025610 for ucd@ivoa.net; Thu, 23 Oct 2003 07:58:57 -0400 (EDT) Date: Thu, 23 Oct 2003 07:58:57 -0400 (EDT) Message-Id: <200310231158.h9NBwv9a025610@urania.cfa.harvard.edu> To: ucd@ivoa.net Subject: Re: A suggested revision for UCDs X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Jonathan McDowell X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 > Many of us on Unix/Linux systems find Word documents inconvenient I strongly second Clive's remarks; thanks for putting the 1.9.9b PDF version up, there's now a chance I'll read it before this morning's NVO telecon. We're trying for interoperability here, and Word isn't that. Jonathan From owner-ucd@eso.org Thu Oct 23 15:00:28 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9NCxPv7021307 for ; Thu, 23 Oct 2003 14:59:25 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9NCxPwE021303 for ucd-outgoing; Thu, 23 Oct 2003 14:59:25 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9NCwJv7020967 for ; Thu, 23 Oct 2003 14:58:19 +0200 (MEST) Received: from milkyway.gsfc.nasa.gov (lheapop.gsfc.nasa.gov [128.183.16.62]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9NCwGs3026707 for ; Thu, 23 Oct 2003 14:58:18 +0200 (CEST) Received: from lheapop.gsfc.nasa.gov (silk3.gsfc.nasa.gov [128.183.18.68]) by milkyway.gsfc.nasa.gov (8.12.9/8.12.9) with ESMTP id h9NCwETd031388; Thu, 23 Oct 2003 08:58:14 -0400 Message-ID: <3F97D06C.8000105@lheapop.gsfc.nasa.gov> Date: Thu, 23 Oct 2003 08:58:20 -0400 From: Thomas McGlynn Organization: NASA Goddard Space Flight Center User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.5) Gecko/20030925 X-Accept-Language: en-us, en MIME-Version: 1.0 To: Jonathan McDowell CC: ucd@ivoa.net Subject: Re: A suggested revision for UCDs References: <200310231158.h9NBwv9a025610@urania.cfa.harvard.edu> In-Reply-To: <200310231158.h9NBwv9a025610@urania.cfa.harvard.edu> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Thomas McGlynn X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Jonathan McDowell wrote: >>Many of us on Unix/Linux systems find Word documents inconvenient > > > I strongly second Clive's remarks; thanks for putting the 1.9.9b > PDF version up, there's now a chance I'll read it before this morning's > NVO telecon. We're trying for interoperability here, and Word isn't that. > Jonathan > > It looks like Marco Leoni posted a PDF version shortly after I uploaded the original... The URL is http://www.ivoa.net/internal/IVOA/IvoaUCD/UCD-1.9.9b.pdf So it's there! Cheers, Tom From owner-ucd@eso.org Thu Oct 23 15:56:23 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9NDtBv7009710 for ; Thu, 23 Oct 2003 15:55:11 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9NDtBrL009704 for ucd-outgoing; Thu, 23 Oct 2003 15:55:11 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9NDsKv7009453 for ; Thu, 23 Oct 2003 15:54:20 +0200 (MEST) Received: from head-cfa.cfa.harvard.edu (head-cfa.cfa.harvard.edu [131.142.41.8]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9NDsJB1018645 for ; Thu, 23 Oct 2003 15:54:19 +0200 (CEST) Received: from urania.cfa.harvard.edu (urania [131.142.52.147]) by head-cfa.cfa.harvard.edu (8.12.10/8.12.8) with ESMTP id h9NDsIeR006435 for ; Thu, 23 Oct 2003 09:54:18 -0400 (EDT) From: Jonathan McDowell Received: (from jcm@localhost) by urania.cfa.harvard.edu (8.12.8p1/8.12.8) id h9NDsIii025671 for ucd@ivoa.net; Thu, 23 Oct 2003 09:54:18 -0400 (EDT) Date: Thu, 23 Oct 2003 09:54:18 -0400 (EDT) Message-Id: <200310231354.h9NDsIii025671@urania.cfa.harvard.edu> To: ucd@ivoa.net Subject: Re: A suggested revision for UCDs X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Jonathan McDowell X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Tom, Now that I've read the document and absorbed at least some of the emails, I must say that I like your proposal a lot. Although there are certainly details to be cleaned up, and I agree with most of Norman's and some of Bob's comments, it feels to me a more solid basis for a UCD2. My biggest beef (which goes directly against Norman's prejudice that UCDs are not an object model!) is that I don't like the distinction between "value" and "instance", especially given that array-valued "values" like "spectrum.value" are mentioned by you. I think your instance is just the value of a higher level term, and I would like to replace "pos.instance" with "pos.value", and then immediately drop the optional ".value" and just say "pos". Why is that a bad idea? Thanks for doing this work! Jonathan From owner-ucd@eso.org Thu Oct 23 16:01:12 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9NDtevN009902 for ; Thu, 23 Oct 2003 15:59:55 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9NDRBkI001246 for ucd-outgoing; Thu, 23 Oct 2003 15:27:11 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9NDQNv7001008 for ; Thu, 23 Oct 2003 15:26:24 +0200 (MEST) Received: from head-cfa.cfa.harvard.edu (head-cfa.cfa.harvard.edu [131.142.41.8]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9NDQNs3027469 for ; Thu, 23 Oct 2003 15:26:23 +0200 (CEST) Received: from xebec.cfa.harvard.edu (xebec [131.142.52.100]) by head-cfa.cfa.harvard.edu (8.12.10/8.12.8) with ESMTP id h9NDQLeR003882; Thu, 23 Oct 2003 09:26:22 -0400 (EDT) From: Arnold Rots Received: (from arots@localhost) by xebec.cfa.harvard.edu (8.12.8p1/8.12.8) id h9NDQLPR001855; Thu, 23 Oct 2003 09:26:21 -0400 (EDT) Message-Id: <200310231326.h9NDQLPR001855@xebec.cfa.harvard.edu> Subject: Re: A suggested revision for UCDs In-Reply-To: To: Clive Page Date: Thu, 23 Oct 2003 09:26:21 -0400 (EDT) CC: ucd@ivoa.net X-Mailer: ELM [version 2.4ME+ PL99 (25)] MIME-Version: 1.0 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Arnold Rots X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 It's a simple choice: those who shelled out the money for a Word license can either try to force the rest of the community to do the same by sending around Word documents, or spend themselves a little more by buying an Acrobat license and thus allow everybody to spend his/her money as (s)he sees fit. Personally, I think Word should always be bundled with Acrobat, at least in our community. - Arnold Clive Page wrote: > On Tue, 21 Oct 2003, Thomas McGlynn wrote: > > > A few minutes ago I uploaded a version of my suggested revised > > proposal for UCDs to the Twiki. This is just a Word version since > > I don't have a PDF generator handy. > > An off-topic note to Tom (and others with the same problem in producing > PDFs): > > Many of us on Unix/Linux systems find Word documents inconvenient; I > ... > > -- > Clive Page > Dept of Physics & Astronomy, > University of Leicester, Tel +44 116 252 3551 > Leicester, LE1 7RH, U.K. Fax +44 116 252 3311 > -------------------------------------------------------------------------- Arnold H. Rots Chandra X-ray Science Center Smithsonian Astrophysical Observatory tel: +1 617 496 7701 60 Garden Street, MS 67 fax: +1 617 495 7356 Cambridge, MA 02138 arots@head-cfa.harvard.edu USA http://hea-www.harvard.edu/~arots/ -------------------------------------------------------------------------- From owner-ucd@eso.org Thu Oct 23 16:49:30 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9NElmTV029934 for ; Thu, 23 Oct 2003 16:48:29 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9NEU4nj022646 for ucd-outgoing; Thu, 23 Oct 2003 16:30:04 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9NET8v7022303 for ; Thu, 23 Oct 2003 16:29:08 +0200 (MEST) Received: from artemis.le.ac.uk (ntp2c.le.ac.uk [143.210.16.126]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9NET7s3029256 for ; Thu, 23 Oct 2003 16:29:07 +0200 (CEST) Received: from [143.210.36.58] (helo=mail.star.le.ac.uk) by artemis.le.ac.uk with smtp (Exim 4.24) id 1ACgSZ-0001BU-57 for ucd@ivoa.net; Thu, 23 Oct 2003 15:29:07 +0100 Received: (qmail 5383 invoked from network); 23 Oct 2003 14:29:13 -0000 Received: from gnowee.star.le.ac.uk (HELO gnowee) (143.210.36.97) by mail.star.le.ac.uk with SMTP; 23 Oct 2003 14:29:13 -0000 From: "Tony Linde" To: Subject: Another pdf generator Date: Thu, 23 Oct 2003 15:29:05 +0100 Organization: University of Leicester Message-ID: <007801c39972$031c1780$6124d28f@gnowee> MIME-Version: 1.0 Content-Type: text/plain; charset="US-ASCII" Content-Transfer-Encoding: 7bit X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook, Build 10.0.4510 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 In-Reply-To: <200310231326.h9NDQLPR001855@xebec.cfa.harvard.edu> Importance: Normal X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Tony Linde" X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 A PDF generator that I use a lot is at http://www.pdf995.com/ - it is a printer driver that, afaik, is windows only but works well. Cheers, Tony. > -----Original Message----- > From: owner-ucd@eso.org [mailto:owner-ucd@eso.org] On Behalf > Of Arnold Rots > Sent: 23 October 2003 14:26 > To: Clive Page > Cc: ucd@ivoa.net > Subject: Re: A suggested revision for UCDs > > > It's a simple choice: those who shelled out the money for a > Word license can either try to force the rest of the > community to do the same by sending around Word documents, or > spend themselves a little more by buying an Acrobat license > and thus allow everybody to spend his/her money as (s)he sees > fit. Personally, I think Word should always be bundled with > Acrobat, at least in our community. > > - Arnold > > Clive Page wrote: > > On Tue, 21 Oct 2003, Thomas McGlynn wrote: > > > > > A few minutes ago I uploaded a version of my suggested revised > > > proposal for UCDs to the Twiki. This is just a Word > version since I > > > don't have a PDF generator handy. > > > > An off-topic note to Tom (and others with the same problem in > > producing > > PDFs): > > > > Many of us on Unix/Linux systems find Word documents > inconvenient; I > > ... > > > > -- > > Clive Page > > Dept of Physics & Astronomy, > > University of Leicester, Tel +44 116 252 3551 > > Leicester, LE1 7RH, U.K. Fax +44 116 252 3311 > > > -------------------------------------------------------------- > ------------ > Arnold H. Rots Chandra X-ray > Science Center > Smithsonian Astrophysical Observatory tel: +1 > 617 496 7701 > 60 Garden Street, MS 67 fax: +1 > 617 495 7356 > Cambridge, MA 02138 > arots@head-cfa.harvard.edu > USA > http://hea-www.harvard.edu/~arots/ > > -------------------------------------------------------------- > ------------ > From owner-ucd@eso.org Thu Oct 23 16:51:33 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9NEogTR001024 for ; Thu, 23 Oct 2003 16:50:42 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9NEogAO001023 for ucd-outgoing; Thu, 23 Oct 2003 16:50:42 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9NElxTb000031 for ; Thu, 23 Oct 2003 16:50:04 +0200 (MEST) Received: from nmail1.systems.pipex.net (nmail1.systems.pipex.net [62.241.160.130]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9NEBVB1019083 for ; Thu, 23 Oct 2003 16:11:31 +0200 (CEST) Received: from nmail1.systems.pipex.net (localhost [127.0.0.1]) by nmail1.systems.pipex.net (8.12.10/8.12.10) with ESMTP id h9NEBRm7007159; Thu, 23 Oct 2003 15:11:27 +0100 Received: (from nobody@localhost) by nmail1.systems.pipex.net (8.12.10/8.12.10/Submit) id h9NEBQsw007158; Thu, 23 Oct 2003 15:11:26 +0100 Received: from 81.86.240.222 ( [81.86.240.222]) as user abm36@dial.pipex.com by netmail.pipex.net with HTTP; Thu, 23 Oct 2003 15:11:26 +0100 Message-ID: <1066918286.3f97e18ebc274@netmail.pipex.net> Date: Thu, 23 Oct 2003 15:11:26 +0100 From: martin hill To: Arnold Rots Cc: Clive Page , ucd@ivoa.net Subject: Off topic document formats... References: <200310231326.h9NDQLPR001855@xebec.cfa.harvard.edu> In-Reply-To: <200310231326.h9NDQLPR001855@xebec.cfa.harvard.edu> MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1 Content-Transfer-Encoding: 8bit User-Agent: PIPEX NetMail (IMP3.1) X-Originating-IP: 81.86.240.222 X-PIPEX-Username: abm36%dial.pipex.com X-Usage: PIPEX NetMail is subject to the standard PIPEX terms and conditions of use X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: martin hill X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Er, so everyone is forced to send around Acrobat documents? And buy Acrobat licences instead of Word ones? Isn't there a Word converter for Open Office? Even much more better still, how about posting as hmtl (if there are no diagrams)? Everyone can read it and almost everything has a converter to it. Or, since it's an AVO standard, I'm sure we could find some way of using VOTable... Cheers, Martin from the "Standards are evil" dept Quoting Arnold Rots : > It's a simple choice: those who shelled out the money for a Word > license can either try to force the rest of the community to do the > same by sending around Word documents, or spend themselves a little > more by buying an Acrobat license and thus allow everybody to spend > his/her money as (s)he sees fit. > Personally, I think Word should always be bundled with Acrobat, at > least in our community. > > - Arnold > > Clive Page wrote: > > On Tue, 21 Oct 2003, Thomas McGlynn wrote: > > > > > A few minutes ago I uploaded a version of my suggested revised > > > proposal for UCDs to the Twiki. This is just a Word version since > > > I don't have a PDF generator handy. > > > > An off-topic note to Tom (and others with the same problem in producing > > PDFs): > > > > Many of us on Unix/Linux systems find Word documents inconvenient; I > > ... > > > > -- > > Clive Page > > Dept of Physics & Astronomy, > > University of Leicester, Tel +44 116 252 3551 > > Leicester, LE1 7RH, U.K. Fax +44 116 252 3311 > > > -------------------------------------------------------------------------- > Arnold H. Rots Chandra X-ray Science Center > Smithsonian Astrophysical Observatory tel: +1 617 496 7701 > 60 Garden Street, MS 67 fax: +1 617 495 7356 > Cambridge, MA 02138 arots@head-cfa.harvard.edu > USA http://hea-www.harvard.edu/~arots/ > -------------------------------------------------------------------------- > > -- Martin Hill 07901 55 24 66 www.mchill.net From owner-ucd@eso.org Thu Oct 23 16:54:03 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9NEqvTR002291 for ; Thu, 23 Oct 2003 16:52:57 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9NEqvcQ002289 for ucd-outgoing; Thu, 23 Oct 2003 16:52:57 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9NElxTf000031 for ; Thu, 23 Oct 2003 16:52:22 +0200 (MEST) Received: from milkyway.gsfc.nasa.gov (lheapop.gsfc.nasa.gov [128.183.16.62]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9NDXUB1018158 for ; Thu, 23 Oct 2003 15:33:31 +0200 (CEST) Received: from lheapop.gsfc.nasa.gov (silk3.gsfc.nasa.gov [128.183.18.68]) by milkyway.gsfc.nasa.gov (8.12.9/8.12.9) with ESMTP id h9NDWwTd001938; Thu, 23 Oct 2003 09:32:58 -0400 Message-ID: <3F97D88F.9030501@lheapop.gsfc.nasa.gov> Date: Thu, 23 Oct 2003 09:33:03 -0400 From: Thomas McGlynn Organization: NASA Goddard Space Flight Center User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.5) Gecko/20030925 X-Accept-Language: en-us, en MIME-Version: 1.0 To: Roy Williams , ucd@ivoa.net Subject: Re: is UCD out of control? References: <05e001c39901$4a189d50$6501a8c0@Ropy> In-Reply-To: <05e001c39901$4a189d50$6501a8c0@Ropy> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Thomas McGlynn X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi Roy, I guess I find the current discussion stimulating and not a sign of a problem. One concern on my part.... My guess is that we only get to make one change to UCDs where the revision is incompatible with the previous set. I don't think the community will want to change their software twice while we're getting our act together. Even Microsoft can't get away with that! Absent your killer app, I'm not sure that a revision to UCDs is on the critical path for the VO so we should take the time to do it right and live with the current standard as long as needed. Personally, I think that UCDTrees or something like them (along with XQuery style queries on them) can be a link between abstract data models and concrete data representations. Tools that search for data matching a given data model could be that killer app. We'll see if this pans out when looked at in detail. Talk to you later. Tom From owner-ucd@eso.org Thu Oct 23 17:05:38 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9NF4cTR006371 for ; Thu, 23 Oct 2003 17:04:38 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9NF4cA9006367 for ucd-outgoing; Thu, 23 Oct 2003 17:04:38 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9NF3fTR006019 for ; Thu, 23 Oct 2003 17:03:42 +0200 (MEST) Received: from head-cfa.cfa.harvard.edu (head-cfa.cfa.harvard.edu [131.142.41.8]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9NF3es3000281 for ; Thu, 23 Oct 2003 17:03:41 +0200 (CEST) Received: from urania.cfa.harvard.edu (urania [131.142.52.147]) by head-cfa.cfa.harvard.edu (8.12.10/8.12.8) with ESMTP id h9NF3eeR012938 for ; Thu, 23 Oct 2003 11:03:40 -0400 (EDT) From: Jonathan McDowell Received: (from jcm@localhost) by urania.cfa.harvard.edu (8.12.8p1/8.12.8) id h9NF3e82025726 for ucd@ivoa.net; Thu, 23 Oct 2003 11:03:40 -0400 (EDT) Date: Thu, 23 Oct 2003 11:03:40 -0400 (EDT) Message-Id: <200310231503.h9NF3e82025726@urania.cfa.harvard.edu> To: ucd@ivoa.net Subject: Re: Off topic document formats... X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Jonathan McDowell X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 > so everyone is forced to send around Acrobat documents? And buy Acrobat licences instead of Word ones? Well, ps2pdf and /usr/bin/acroread are free... I'm happy if you make it postscript or ascii, but PDF seems a reasonable compromise that's ok for people in both the Windows and Unix worlds. OpenOffice is still - at least for me - a continual struggle with not-quite-adequate compatibility, slow printing, yucky interface, and of course fails whenever MS updates Word. And I worry about .doc documents on the twiki being reliably readable in the future. > how about posting as hmtl (sic) Fine by me, although it's inconvenient to print a long document all at once. > I'm sure we could find some way of using VOTable Y'know, I was tempted to make this suggestion before, but manfully resisted... :-) Indeed the IVOA standard for documents, so I understand, is html. Perhaps this should be discussed more widely (in the standards WG, or whatever it's called?) In the meantime, perhaps I'll just post latex DVI files.... Jonathan From owner-ucd@eso.org Thu Oct 23 17:57:02 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9NFtpTR023433 for ; Thu, 23 Oct 2003 17:55:51 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9NFtpsx023432 for ucd-outgoing; Thu, 23 Oct 2003 17:55:51 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9NFqKTd022155 for ; Thu, 23 Oct 2003 17:55:03 +0200 (MEST) Received: from mail.cacr.caltech.edu (mail.cacr.caltech.edu [131.215.145.9]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9NEwns3000131 for ; Thu, 23 Oct 2003 16:58:50 +0200 (CEST) Received: from Ropy (dsl-pb-1504.linkline.com [64.30.223.60]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id h9NEwhM9005515 (version=TLSv1/SSLv3 cipher=RC4-MD5 bits=128 verify=NO); Thu, 23 Oct 2003 07:58:44 -0700 Message-ID: <074601c39976$2cb69620$6501a8c0@Ropy> From: "Roy Williams" To: "martin hill" , "Arnold Rots" Cc: "Clive Page" , References: <200310231326.h9NDQLPR001855@xebec.cfa.harvard.edu> <1066918286.3f97e18ebc274@netmail.pipex.net> Subject: Re: Off topic document formats... Date: Thu, 23 Oct 2003 07:58:51 -0700 MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Roy Williams" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 > Even much more better still, how about posting as hmtl (if there are no > diagrams)? Everyone can read it and almost everything has a converter to it. I think this is best, when it converges, I will have the UCD document converted to the clean HTML -- I mean the stuff that can be edited by a human! Roy From owner-ucd@eso.org Thu Oct 23 17:57:55 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9NFufTR023733 for ; Thu, 23 Oct 2003 17:56:41 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9NFuefv023728 for ucd-outgoing; Thu, 23 Oct 2003 17:56:40 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9NFqKTf022155 for ; Thu, 23 Oct 2003 17:55:50 +0200 (MEST) Received: from revere.aoc.nrao.edu (revere.aoc.nrao.edu [146.88.1.15]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9NF05s3000196 for ; Thu, 23 Oct 2003 17:00:06 +0200 (CEST) Received: from zia.aoc.nrao.edu (zia [146.88.1.4]) by revere.aoc.nrao.edu (8.11.6/8.11.6) with ESMTP id h9NErgE15600; Thu, 23 Oct 2003 08:53:43 -0600 Received: from oak (oak [146.88.1.137]) by zia.aoc.nrao.edu (8.12.9/8.12.5) with ESMTP id h9NErd72006571; Thu, 23 Oct 2003 08:53:39 -0600 (MDT) Date: Thu, 23 Oct 2003 08:53:38 -0600 (MDT) From: Doug Tody X-X-Sender: dtody@oak To: Clive Page cc: ucd@ivoa.net Subject: Re: A suggested revision for UCDs In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-MailScanner: Found to be clean X-MailScanner-SpamCheck: not spam, SpamAssassin (score=-2.5, required 7, EMAIL_ATTRIBUTION, IN_REP_TO, SPAM_PHRASE_01_02, USER_AGENT_PINE) X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Doug Tody X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Ok, we are off topic but... A simple solution is to run vmware (or something similar) on Linux, with Windows in the vm, using samba to share the unix file system. This provides the best of both worlds. Doug On Thu, 23 Oct 2003, Clive Page wrote: > On Tue, 21 Oct 2003, Thomas McGlynn wrote: > > > A few minutes ago I uploaded a version of my suggested revised > > proposal for UCDs to the Twiki. This is just a Word version since > > I don't have a PDF generator handy. > > An off-topic note to Tom (and others with the same problem in producing > PDFs): > > Many of us on Unix/Linux systems find Word documents inconvenient; I > thought OpenOffice.org might cope with your file, but it produces > illegible results without a lot of playing with fonts, and even then was > very poor. > From owner-ucd@eso.org Thu Oct 23 18:11:32 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9NGAQTR028091 for ; Thu, 23 Oct 2003 18:10:26 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9NGAQBe028090 for ucd-outgoing; Thu, 23 Oct 2003 18:10:26 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9NG4mTf026218 for ; Thu, 23 Oct 2003 18:09:45 +0200 (MEST) Received: from head-cfa.cfa.harvard.edu (head-cfa.cfa.harvard.edu [131.142.41.8]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9NEHls3028972 for ; Thu, 23 Oct 2003 16:17:47 +0200 (CEST) Received: from xebec.cfa.harvard.edu (xebec [131.142.52.100]) by head-cfa.cfa.harvard.edu (8.12.10/8.12.8) with ESMTP id h9NEHieR008797; Thu, 23 Oct 2003 10:17:44 -0400 (EDT) From: Arnold Rots Received: (from arots@localhost) by xebec.cfa.harvard.edu (8.12.8p1/8.12.8) id h9NEHhaS001976; Thu, 23 Oct 2003 10:17:43 -0400 (EDT) Message-Id: <200310231417.h9NEHhaS001976@xebec.cfa.harvard.edu> Subject: Re: Off topic document formats... In-Reply-To: <1066918286.3f97e18ebc274@netmail.pipex.net> To: martin hill Date: Thu, 23 Oct 2003 10:17:43 -0400 (EDT) CC: Arnold Rots , Clive Page , ucd@ivoa.net X-Mailer: ELM [version 2.4ME+ PL99 (25)] MIME-Version: 1.0 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Arnold Rots X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 martin hill wrote: > Er, so everyone is forced to send around Acrobat documents? And buy Acrobat > licences instead of Word ones? Only those who pay for Word licenses in the first place. Acrobat reader is free. > > Isn't there a Word converter for Open Office? Doesn't always work well - see Clive's roiginal post. > > Even much more better still, how about posting as hmtl (if there are no > diagrams)? Everyone can read it and almost everything has a converter to it. Fine with me, though PDF is quite a reasonable standard for documents. > Or, since it's an AVO standard, I'm sure we could find some way of using VOTable... > > Cheers, > > Martin > from the "Standards are evil" dept > > > > Quoting Arnold Rots : > > > It's a simple choice: those who shelled out the money for a Word > > license can either try to force the rest of the community to do the > > same by sending around Word documents, or spend themselves a little > > more by buying an Acrobat license and thus allow everybody to spend > > his/her money as (s)he sees fit. > > Personally, I think Word should always be bundled with Acrobat, at > > least in our community. > > > > - Arnold > > > > Clive Page wrote: > > > On Tue, 21 Oct 2003, Thomas McGlynn wrote: > > > > > > > A few minutes ago I uploaded a version of my suggested revised > > > > proposal for UCDs to the Twiki. This is just a Word version since > > > > I don't have a PDF generator handy. > > > > > > An off-topic note to Tom (and others with the same problem in producing > > > PDFs): > > > > > > Many of us on Unix/Linux systems find Word documents inconvenient; I > > > ... > > > > > > -- > > > Clive Page > > > Dept of Physics & Astronomy, > > > University of Leicester, Tel +44 116 252 3551 > > > Leicester, LE1 7RH, U.K. Fax +44 116 252 3311 > > > > > -------------------------------------------------------------------------- > > Arnold H. Rots Chandra X-ray Science Center > > Smithsonian Astrophysical Observatory tel: +1 617 496 7701 > > 60 Garden Street, MS 67 fax: +1 617 495 7356 > > Cambridge, MA 02138 arots@head-cfa.harvard.edu > > USA http://hea-www.harvard.edu/~arots/ > > -------------------------------------------------------------------------- > > > > > > > -- > Martin Hill > 07901 55 24 66 > www.mchill.net > -------------------------------------------------------------------------- Arnold H. Rots Chandra X-ray Science Center Smithsonian Astrophysical Observatory tel: +1 617 496 7701 60 Garden Street, MS 67 fax: +1 617 495 7356 Cambridge, MA 02138 arots@head-cfa.harvard.edu USA http://hea-www.harvard.edu/~arots/ -------------------------------------------------------------------------- From owner-ucd@eso.org Thu Oct 23 19:28:13 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9NHRHTR020012 for ; Thu, 23 Oct 2003 19:27:17 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9NHRHnC020004 for ucd-outgoing; Thu, 23 Oct 2003 19:27:17 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9NHQeTR019874 for ; Thu, 23 Oct 2003 19:26:40 +0200 (MEST) Received: from sainfoin.saclay.cea.fr (sainfoin.saclay.cea.fr [132.166.192.126]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9NHQeB1024421 for ; Thu, 23 Oct 2003 19:26:40 +0200 (CEST) Received: from rosetta.saclay.cea.fr (rosetta.saclay.cea.fr [132.166.13.210]) by sainfoin.saclay.cea.fr (8.12.10/8.12.9/CEAnet-Internet.2.0) with ESMTP id h9NHQdfj023664; Thu, 23 Oct 2003 19:26:39 +0200 (MEST) Received: (from dide@localhost) by rosetta.saclay.cea.fr (8.11.6+Sun/8.10.2) id h9NHQgH11982; Thu, 23 Oct 2003 19:26:42 +0200 (MEST) Date: Thu, 23 Oct 2003 19:26:42 +0200 (MEST) From: DIDELON Pierre Message-Id: <200310231726.h9NHQgH11982@rosetta.saclay.cea.fr> To: tam@lheapop.gsfc.nasa.gov Subject: Re: A suggested revision for UCDs Cc: ucd@ivoa.net X-Sun-Charset: US-ASCII X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: DIDELON Pierre X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi Tom, Big and impressive work. I have read and try to absorb the document and most of the following mails. I try to digest all. It is not so obvious for a frenchy like me and I hope that my comments below are appropriate. I apologize for any misunderstanding or confusion, by jumping in the discussion, but a really want to make a few points. If a clearly understand the concern of Pedro Osuna, the actual discussion illustrate what he stressed in strasbourg and his further mail. UCD1 and a data model for context evaluation is sufficient, because DM is not available some structure is needed to be introduced and so UCD2 came. But unless we put DM in UCD (eventually using VOTable structure) it will be incomplete. Even UCDTree (which I really like) needed additional structure/template or external reference as stressed in the document 1.9.9b: p16 last paragraph, p18 last paragraph. I like several aspect of this proposal, and I agree of some of the comments of Norman, Ed and Jonathan, but as it is very tedious for me to write in english, I will not do an extensive comment list of what is hapenning in the discussion but go directly to the pb I had. Instead of specific words or context meaning to distinguish between 3 kind of thing; concept, modifier property and attribute property I would be more comfortable with a syntax distinction and a specific separator (i.e. #). The complexity of the three trees with specific words seems very strange and is confusing me. My main concern is related to Attributes. - I did not understand the meaning of local. You can always correlated a property with an identical or similar property, it depend of the purpose of your correlation, and without presuposition you cannot exclude apriori some intressting thing that can be extract from data. Taking your example: you can extract data where temperature jitter of the data acquisition system is above a certain threshold and try to correlate these with phot,flux;error or any kind of measurement error available. Perhaps not used very often, but not forbidden I hope? - It seems to me that there are some dangerous redundancy in the basic word of the attribute tree. For example value, vector, instance, multiplet are common data properties distinguish by their use or the context in which they appear. IMO there is no differences between vector and multiplet and each time you use multiplet you could replace it by vector. No? Like jonathan, if you put vectors in value, I did not see the need for instance. The relation of measurements, errors and all this kind of things with the precedding is even more complicated. A value (I mean a real scalar) can be a unique measurement value, a statistical property of a measurement serie (like mean, mode, error, std.dev., skewness...), a parameter and perhaps other meaning I am not able to think of now. Trying to be brief, (but unfortunatly uncomplete) I feel that the pb came from the fact that diff data property are mixed together (I believe that the same pb occurs in DM group). Mainly data structure, data meaning (could be extended to purpose) and data representation (without speaking of format and location). Data structure would include ; value (scalar), vector (avoiding multiplet) tree, and extended easly with matrix or composite structure. For me instance is A structure, but wich one? A free formatted structure, a VOTable tree formatted? It is not clear. data meaning is related to measurement, error and all staistical properties. data representation mixed both things; a measurement serie can be represented by a vector (even in a VOTable cell), or by one or several statistical prop. (mean, mean+std.dev.) structured in very diff way (mean and error in separate cols, mean+mode+median in one col ...) I feel that refurbishing is needed here to clarify UCD usage more than UCD existance. I agree with earlier comments that stressed that the big advantage of UCD1 is the fact that they are not due to apriori/re-invented structure but are the illustration of the existing data. - I did not see the filter needs. It seems to me that it try to catch a part of the data history, but it seems so restrive that it will be very soon unappropriate I bet. - concept seems only due to the uncompltness of the words available in the concept tree root. In your example (p18) a word correlation (which would certainly be needed for VO) would better match the needs. I stop here because it's late and I would become confused, if not yet done. Thanks for the food for thought, sincerely, Pierre ------------------------------------------------------------------------------- DIDELON e-mail : pdidelon_at_cea.fr CEA SACLAY - Service d'Astrophysique W3 : http://www-dapnia.cea.fr/Sap/ 91191 Gif-Sur-Yvette Cedex Phone : 33 (0)1 69 08 58 89 ------------------------------------------------------------------------------- From owner-ucd@eso.org Thu Oct 23 22:00:57 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9NK01TR021387 for ; Thu, 23 Oct 2003 22:00:01 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9NK0111021385 for ucd-outgoing; Thu, 23 Oct 2003 22:00:01 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9NJxRTR021247 for ; Thu, 23 Oct 2003 21:59:27 +0200 (MEST) Received: from mail630.gsfc.nasa.gov (mail630.gsfc.nasa.gov [128.183.190.39]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9NJxPB1027660 for ; Thu, 23 Oct 2003 21:59:26 +0200 (CEST) Received: from gsfc.nasa.gov (ram.gsfc.nasa.gov [128.183.114.136]) by mail630.gsfc.nasa.gov (8.12.8/8.12.5) with ESMTP id h9NJxNAM015479 for ; Thu, 23 Oct 2003 15:59:24 -0400 Message-ID: <3F9833BD.40604@gsfc.nasa.gov> Date: Thu, 23 Oct 2003 16:02:05 -0400 From: Ed Shaya User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.4) Gecko/20030529 X-Accept-Language: en-us, en MIME-Version: 1.0 To: ucd@ivoa.net Subject: Use case: distance Content-Type: text/html; charset=us-ascii Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Ed Shaya X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000
Roy again asked for some use cases for UCD's so here is my favorite.
I need accurate distances to nearby galaxies.  So, I am very picky as to the kind of distance estimate.  E.G., a distance derived from a redshift will not do for nearby galaxies. So I can't just query on phys:distance, there must be a simple way to distinguish the distance quantity by method used to obtain the distance.  And to look through every paper on distances of galaxies, one by one, would take months.

Most desireable methods:
Period-Luminosity Relation of Cepheid variables
ditto for RR-Lyrae variables
CCD-based  IR-Tully-Fisher Relation (rotation velocity  vs.  IR  Magnitude)
Tip of the Red Giant Branch (brightest TRGB stars)    
Supergiant Stars atomic hydrogen Equivalent widths vs stellar mag
spectroscopic eclipsing binaries (none published yet)
Maser orbits
Type Ia Supernovae Peak Brightness
Surface Brightness Fluctuations

Less desired (>20% error):
Redshift using Hubble relation or some other flow model
Brightest Stars
B-band Tully-Fisher Relation
IR-Tully-Fisher with single aperture IR magnitudes
Dn-Sigma (alias: Faber-Jackson Relation) (central size vs velocity displersion)
Expanding Photosphere (Baade-Wasselink Method)
    *Supernova
    *Planetary Nebula
Largest HII regions

Perhaps the simplest thing is to have error bars for all data and then one could
simply ask for small error bar data.  But distance papers are notorious for underestimating errors.  So one needs to use knowledge from cross-studies on what the real errors on these various distance estimators are.

Another similar example would be the temperature of a star or ISM cloud.
There are various techniques for obtaining that property, but each one measures a substantially different statistic of T or T at various depth.

So, is this a job for UCDs?  Data Model?  Shouldn't standard astronomical methods of obtaining a property be part of our controlled vocabulary?  If not in UCDs then in some other dictionary/ontology? Or is it beyond our wildest dreams? (Well not mine, but ours.)

Ed

From owner-ucd@eso.org Wed Oct 29 19:44:29 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id h9TIdUMW012620 for ; Wed, 29 Oct 2003 19:39:30 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id h9TIdUvZ012600 for ucd-outgoing; Wed, 29 Oct 2003 19:39:30 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id h9TIcYMW012289 for ; Wed, 29 Oct 2003 19:38:34 +0100 (MET) Received: from milkyway.gsfc.nasa.gov (lheapop.gsfc.nasa.gov [128.183.16.62]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id h9TIcQB1011926 for ; Wed, 29 Oct 2003 19:38:29 +0100 (CET) Received: from lheapop.gsfc.nasa.gov (silk3.gsfc.nasa.gov [128.183.18.68]) by milkyway.gsfc.nasa.gov (8.12.9/8.12.9) with ESMTP id h9TIcKTd009035 for ; Wed, 29 Oct 2003 13:38:20 -0500 Message-ID: <3FA00924.3040502@lheapop.gsfc.nasa.gov> Date: Wed, 29 Oct 2003 13:38:28 -0500 From: Thomas McGlynn Organization: NASA Goddard Space Flight Center User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.5) Gecko/20030925 X-Accept-Language: en-us, en MIME-Version: 1.0 To: ucd@ivoa.net Subject: Further thoughts on UCDs Content-Type: text/plain; charset=windows-1252; format=flowed X-Scanned-By: MIMEDefang 2.35 X-MIME-Autoconverted: from 8bit to quoted-printable by milkyway.gsfc.nasa.gov id h9TIcKTd009035 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id h9TIdPMW012586 Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Thomas McGlynn X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 One of my problems in understanding how or whether we should change the UCD strings is the indefiniteness of the current UCD2 proposals which do not specify the full list of UCDs. I've just spent a few minutes looking at the PHOT hierarchy. Probably Sebastien and Roy have done this with far greater care, but I've gone through the old UCD tree and tried to see what UCDs are suggested by what's in the PHOT hierarchy, where I have explicitly left out any band information from the UCDs assuming that to be supplied by qualifiers in the em hierarchy. There are only about 25 distinct phot words here versus just under 500 in the original UCD1 tree. Most of this savings is at the cost of having an extensive em tree describing the bands, but I think that's helpful since we want to be able to combine fluxes from different bands. I think it makes the photometry tree much more accessible. One thought expressed here is that we should not distinguish between flux, magnitudes and counts in the UCDs, but rather do that with the units. I'm not sure if this is a good idea but it seems to me that they are more 'similar' to each other than each is to say a fluence or a color. There is a question as to whether we specify colors by providing special keywords for each color, or by using a pair of em qualifiers. In the latter case, then the order of the em qualifiers may be significant. If we go this route (and I think it makes more sense) then my proposal for well-formed UCDs would have to be modified to say something like: 'where the order of qualifiers is not significant, they should be given in alphabetical order'. phot phot.flux … distinctions between counts, magnitudes, fluxes, etc should be carried in the … units not the UCD. phot.flux.surfaceBrightness phot.fluence phot.flux.absolute phot.color (This is really a ratio, but we use color as the traditional name). phot.color.diff (A difference in colors, i.e., a kind of second derivative) phot.color.excess em.bolometric (Bolometric measurements are after all just specifying a very broad band) phot.atmosphere phot.atmosphere.airmass phot.atmosphere.extinction phot.class phot.extinction.galactic phot.extinction.internal phot.extinction.ism phot.extinction.total phot.flux.isophotal phot.flux.central phot.correction.k phot.flux.limit phot.flux.offset phot.profile math/arith.ratio (for the phot_sd/b-bright, phot_tot-Bright/b-bright UCDs) phot.system (is this different from phot.class?) phot.parameter (some parameter of the photometric system phot.zeropoint phot.spectrum (vector valued fields) phot.timeseries (vector valued fields) phot.image (vector valued fields) This was just a quick exercise and doubtless there are better specific choices, but the phot hierarchy is one area where I imagine that our software may be very UCD aware. If we really can simplify it to this extent, then I think this alone is a major impetus for going to UCD2. Tom From owner-ucd@eso.org Wed Nov 5 13:59:16 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id hA5CwlfE001240 for ; Wed, 5 Nov 2003 13:58:47 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id hA5Cwk59001238 for ucd-outgoing; Wed, 5 Nov 2003 13:58:46 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id hA5CwffE001193 for ; Wed, 5 Nov 2003 13:58:43 +0100 (MET) Received: from smtp.pspl.co.in ([202.54.11.65]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id hA5Cwcs3012308 for ; Wed, 5 Nov 2003 13:58:40 +0100 (CET) Received: (from root@localhost) by smtp.pspl.co.in (8.12.9/8.12.9) id hA5Cwl3A009884 for ; Wed, 5 Nov 2003 18:28:47 +0530 Received: from ps0075 (PS0075.intranet.pspl.co.in [192.168.7.111]) (authenticated bits=0) by persistent.co.in (8.12.9/8.12.9) with ESMTP id hA5Cwkob009869 for ; Wed, 5 Nov 2003 18:28:47 +0530 Message-ID: <02c401c3a39c$86360a20$6f07a8c0@persistent.co.in> From: "Sonali A. Kale" To: Subject: UCD matching function Date: Wed, 5 Nov 2003 18:28:35 +0530 Organization: Persistent Systems Private Limited MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 5.50.4807.1700 x-mimeole: Produced By Microsoft MimeOLE V5.50.4910.0300 X-Spam-Status: No, hits=0.0 required=7.0 tests=none version=2.54 X-Spam-Level: X-Spam-Checker-Version: SpamAssassin 2.54 (1.174.2.17-2003-05-11-exp) X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Sonali A. Kale" X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hello, Could someone throw light on the UCD matching function ? Will there be separate parsers written for the matching ? In VOPlot as of now, we use UCDs to look for similar columns from another VOTable. This is a simple string match, but I guess the matching function for the new UCD system will be more complex. Will the matching be provided as a web service ? How much data will a software have to carry with it for the actual matching (if the matching is done by the software tool) ? I am especially worried about this since VOPlot is an applet and an applet with a heavy footprint will not be usable. I would really appreciate any help on this. - Thanks, Sonali ------------------------------------ Sonali A. Kale Persistent Systems Private Limited http://www.persistent.co.in Ph: +91 (20) 567 8900 (ext. 328) ------------------------------------ From owner-ucd@eso.org Wed Nov 5 15:50:27 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id hA5EnVfE009991 for ; Wed, 5 Nov 2003 15:49:31 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id hA5EnUM3009978 for ucd-outgoing; Wed, 5 Nov 2003 15:49:30 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id hA5EmKfI009530 for ; Wed, 5 Nov 2003 15:48:56 +0100 (MET) Received: from mail.cacr.caltech.edu (mail.cacr.caltech.edu [131.215.145.9]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id hA5EF2B1018175 for ; Wed, 5 Nov 2003 15:15:03 +0100 (CET) Received: from Ropy (dsl-pb-1504.linkline.com [64.30.223.60]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id hA5EF1M9010021 (version=TLSv1/SSLv3 cipher=RC4-MD5 bits=128 verify=NO); Wed, 5 Nov 2003 06:15:01 -0800 Message-ID: <072e01c3a3a7$361c34f0$6401a8c0@Ropy> From: "Roy Williams" To: "Sonali A. Kale" , References: <02c401c3a39c$86360a20$6f07a8c0@persistent.co.in> Subject: Re: UCD matching function Date: Wed, 5 Nov 2003 06:15:05 -0800 MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Roy Williams" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Sonali Thank you for your burst of cold reality in this increasingly abstract discussion. In debating the structure of UCD2, I have been continually thinking of you and others who build actual software that "understands" UCD. Unfortunately, I cannot answer your questions. I could simply say there will be a web service for doing the matching, but then you will say who and where and when. I do not know. Can I call here fo volunteers to make the UCD2 services? How soon? I am beginning to think that adopting UCD2 will require a lot of hard work by a lot of people -- data providers as well as consumers -- and I am not seeing the concrete and immediate benefits. Perhaps we should start working towards a very sophisticated RDF-based model ("UCD3") for alpha release in a year or two. But stay with a cleaned-up UCD1 for the near to medium term. Comments anyone? Roy -------- Caltech Center for Advanced Computing Research roy@cacr.caltech.edu 626 395 3670 ----- Original Message ----- From: "Sonali A. Kale" To: Sent: Wednesday, November 05, 2003 4:58 AM Subject: UCD matching function > Hello, > > Could someone throw light on the UCD matching > function ? Will there be separate parsers written for > the matching ? In VOPlot as of now, we use UCDs > to look for similar columns from another VOTable. > This is a simple string match, but I guess the matching > function for the new UCD system will be more complex. > > Will the matching be provided as a web service ? How > much data will a software have to carry with it for the > actual matching (if the matching is done by the software tool) ? > I am especially worried about this since VOPlot is an applet > and an applet with a heavy footprint will not be usable. > > I would really appreciate any help on this. > > - Thanks, > Sonali > ------------------------------------ > Sonali A. Kale > Persistent Systems Private Limited > http://www.persistent.co.in > Ph: +91 (20) 567 8900 (ext. 328) > ------------------------------------ > > From owner-ucd@eso.org Wed Nov 5 16:30:27 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id hA5FTGfI022214 for ; Wed, 5 Nov 2003 16:29:49 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id hA5F0iHu013511 for ucd-outgoing; Wed, 5 Nov 2003 16:00:44 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id hA5ExwfE013322 for ; Wed, 5 Nov 2003 15:59:58 +0100 (MET) Received: from apollo.le.ac.uk (apollo.le.ac.uk [143.210.16.125]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id hA5Exvs3015696 for ; Wed, 5 Nov 2003 15:59:57 +0100 (CET) Received: from [143.210.36.58] (helo=mail.star.le.ac.uk) by apollo.le.ac.uk with smtp (Exim 4.24) id 1AHP8W-0000fO-K6 for ucd@ivoa.net; Wed, 05 Nov 2003 14:59:56 +0000 Received: (qmail 3235 invoked from network); 5 Nov 2003 15:00:00 -0000 Received: from sparky.star.le.ac.uk (143.210.36.10) by mail.star.le.ac.uk with SMTP; 5 Nov 2003 15:00:00 -0000 Date: Wed, 5 Nov 2003 15:00:00 +0000 (GMT) From: "Patricio F. Ortiz" To: Roy Williams cc: "Sonali A. Kale" , Subject: Re: UCD matching function In-Reply-To: <072e01c3a3a7$361c34f0$6401a8c0@Ropy> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Patricio F. Ortiz" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 On Wed, 5 Nov 2003, Roy Williams wrote: > > Perhaps we should start working towards a very sophisticated RDF-based > model ("UCD3") for alpha release in a year or two. But stay with a > cleaned-up UCD1 for the near to medium term. > > Comments anyone? Roy, I'm all for that! Let's make some necessary modifications to UCD1 and start using them. I went through examining the ERROR 'box', assuming that each ERROR could be transformed to "error.QUANTITY_UCD". It works most of the time, but there are some cases where it simply doesn't work. Bottom line is that in Vizier's metadata there are around 9000 ERROR columns, which translate into about 570 new error descriptors. Assuming what we want to do is to "change the labels" from UCD1 to UCD_N, then we will preserve the degree of comparability. If we start shuffling columns from one box to another, and merging boxes, then the work will be much more!! Cheers, Patricio --- Patricio F. Ortiz pfo@star.le.ac.uk AstroGrid project Department of Physics and Astronomy University of Leicester Tel: +44 (0)116 252 2015 LE1 7RH, UK From owner-ucd@eso.org Wed Nov 5 19:40:13 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id hA5IdxfE024219 for ; Wed, 5 Nov 2003 19:39:59 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id hA5Idx0F024215 for ucd-outgoing; Wed, 5 Nov 2003 19:39:59 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with SMTP id hA5IdtfE024183 for ; Wed, 5 Nov 2003 19:39:56 +0100 (MET) Received: from po1.wam.umd.edu (po1.wam.umd.edu [128.8.10.163]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with SMTP id hA5Idss3021404 for ; Wed, 5 Nov 2003 19:39:55 +0100 (CET) Received: from gsfc.nasa.gov (atlas.astro.umd.edu [129.2.14.14]) by po1.wam.umd.edu (8.11.6-20030924/8.11.6) with ESMTP id hA5IdlP26378; Wed, 5 Nov 2003 13:39:47 -0500 (EST) Message-ID: <3FA943DC.20007@gsfc.nasa.gov> Date: Wed, 05 Nov 2003 13:39:24 -0500 From: Ed Shaya User-Agent: Mozilla/5.0 (X11; U; Linux i686; en-US; rv:1.5b) Gecko/20030827 X-Accept-Language: en-us, en MIME-Version: 1.0 To: Roy Williams , ucd@ivoa.net Subject: Re: UCD matching function References: <02c401c3a39c$86360a20$6f07a8c0@persistent.co.in> <072e01c3a3a7$361c34f0$6401a8c0@Ropy> In-Reply-To: <072e01c3a3a7$361c34f0$6401a8c0@Ropy> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Ed Shaya X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Roy, This makes sense to me. So wherever you need a UCD you can put an rdf:id or rdf:resource that identifies a proper descriptive term by URL. At that URL is the OWL class within the class hierarchy and with its definition. There one can define the dimensional analysis of the item and how it differs from similar terms. However, one does not escape the painful reality that each concept needs a name and so one still needs to come up with agreement on these names. The only advantage for this aspect is that one can reflect hierarchies in the directory structure and the URL with the "/" symbol, as in http://ivoa.net/OWL/physics/StokesParameters/S0.owl Ed Roy Williams wrote: >Sonali > >Thank you for your burst of cold reality in this increasingly abstract >discussion. In debating the structure of UCD2, I have been continually >thinking of you and others who build actual software that >"understands" UCD. > >Unfortunately, I cannot answer your questions. I could simply say >there will be a web service for doing the matching, but then you will >say who and where and when. I do not know. Can I call here fo >volunteers to make the UCD2 services? How soon? > >I am beginning to think that adopting UCD2 will require a lot of hard >work by a lot of people -- data providers as well as consumers -- and >I am not seeing the concrete and immediate benefits. > >Perhaps we should start working towards a very sophisticated RDF-based >model ("UCD3") for alpha release in a year or two. But stay with a >cleaned-up UCD1 for the near to medium term. > >Comments anyone? >Roy > >-------- >Caltech Center for Advanced Computing Research >roy@cacr.caltech.edu >626 395 3670 > >----- Original Message ----- >From: "Sonali A. Kale" >To: >Sent: Wednesday, November 05, 2003 4:58 AM >Subject: UCD matching function > > > > >>Hello, >> >>Could someone throw light on the UCD matching >>function ? Will there be separate parsers written for >>the matching ? In VOPlot as of now, we use UCDs >>to look for similar columns from another VOTable. >>This is a simple string match, but I guess the matching >>function for the new UCD system will be more complex. >> >>Will the matching be provided as a web service ? How >>much data will a software have to carry with it for the >>actual matching (if the matching is done by the software tool) ? >>I am especially worried about this since VOPlot is an applet >>and an applet with a heavy footprint will not be usable. >> >>I would really appreciate any help on this. >> >>- Thanks, >>Sonali >>------------------------------------ >>Sonali A. Kale >>Persistent Systems Private Limited >>http://www.persistent.co.in >>Ph: +91 (20) 567 8900 (ext. 328) >>------------------------------------ >> >> >> >> > > > From owner-interop@eso.org Thu Dec 4 20:09:12 2003 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id hB4J4alK023581 for ; Thu, 4 Dec 2003 20:04:37 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id hB4J4aVI023564 for interop-outgoing; Thu, 4 Dec 2003 20:04:36 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-interop@eso.org using -f Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id hB4J2E1u022783; Thu, 4 Dec 2003 20:02:14 +0100 (MET) Received: from eso.org (nb008487.ads.eso.org [134.171.27.211]) by serapis.hq.eso.org (8.11.7+Sun/8.11.7) with ESMTP id hB4J2Et07715; Thu, 4 Dec 2003 20:02:14 +0100 (MET) Message-ID: <3FCF84B6.9070507@eso.org> Date: Thu, 04 Dec 2003 20:02:14 +0100 From: "Marco C. Leoni" Organization: Astrophysical Virtual Observatory @ESO User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.4) Gecko/20030624 Netscape/7.1 (ax) X-Accept-Language: en, en-us MIME-Version: 1.0 To: mleoni@eso.org Subject: Server down X-Priority: 1 (highest) Content-Type: multipart/alternative; boundary="------------000202050900060205000601" Sender: owner-interop@eso.org Precedence: bulk Reply-To: "Marco C. Leoni" X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Mozilla-Status: c001 X-Mozilla-Status2: 00000000 This is a multi-part message in MIME format. --------------000202050900060205000601 Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit Due to maintenance of the electrical systems this week-end in Garching, we have been requested to switch off all computer systems during this period. For this reason all the services (mailing lists, web sites, twikis) will be unavailable on Saturday Dec. 6 . Sorry for the short notice. Best regards, Marco -- Marco C. Leoni Astrophysical Virtual Observatory - http://www.euro-vo.org tel 0049 89 3200 6560 fax 0049 89 3200 6480 mleoni@eso.org --------------000202050900060205000601 Content-Type: text/html; charset=us-ascii Content-Transfer-Encoding: 7bit Due to maintenance of the electrical systems this week-end in Garching, we have been requested to switch off all computer systems during this period.
For this reason all the services (mailing lists, web sites, twikis) will be unavailable on Saturday Dec. 6 .

Sorry for the short notice.


Best regards,
    Marco




--
Marco C. Leoni

Astrophysical Virtual Observatory - http://www.euro-vo.org
11.351.12
tel 0049 89 3200 6560
fax 0049 89 3200 6480
mleoni@eso.org --------------000202050900060205000601-- From owner-dal@eso.org Wed Mar 24 19:46:00 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2OIjQvR008187 for ; Wed, 24 Mar 2004 19:45:26 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2OIjQkm008186 for dal-outgoing; Wed, 24 Mar 2004 19:45:26 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dal@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2OIjNvR008174; Wed, 24 Mar 2004 19:45:23 +0100 (MET) Received: from mail.cacr.caltech.edu (mail.cacr.caltech.edu [131.215.145.9]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i2OIjK3R007309; Wed, 24 Mar 2004 19:45:21 +0100 (CET) Received: from SARA (roy-nat.cacr.caltech.edu [131.215.144.149]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id i2OIjIk4002303 (version=TLSv1/SSLv3 cipher=RC4-MD5 bits=128 verify=NO); Wed, 24 Mar 2004 10:45:19 -0800 Message-ID: <02f401c411d0$3215b650$0c0ba8c0@cacr.caltech.edu> From: "Roy Williams" To: , Subject: New UCD1+ for SIA protocol Date: Wed, 24 Mar 2004 10:45:35 -0800 MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-dal@eso.org Precedence: bulk Reply-To: "Roy Williams" X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear UCD and DAL folks Three of us (Sebastian Derriere, Andrea Preite-Martinez, myself) have been working on an update for the SIA protocol that uses the standard UCD set, now called UCD1+, rather than the ad hoc namespace VOX that SIA 1.0 has been using. In the following, all UCD from the original SIA specification are listed below. The old SIA UCD is written first, then the suggested new UCD1+ is written in the line beginning "-->" The UCD1+ is not fully documented yet, but you can find a dictionary from UCD1 to UCD1+ at http://vizier.u-strasbg.fr/UCD/lists/ucd1-ucd1p.txt and http://vizier.u-strasbg.fr/UCD/lists/ucd1p-composed.txt The SIA protocol is defined at http://us-vo.org/pubs/files/ACF8DE.pdf The new SIA will be version 1.1, and we are hoping to draft and approve this at the IVOA meeting at the end of May. Thank you for your comments and suggestions on these new assignments Andrea, Roy, Sebastian -------------------------------------------------------- VOX:Image_Title --> meta.title containing a short (usually one line) description of the image. This should concisely describe the image to a user, typically identifying the image source (e.g., survey name), object name or field coordinates, bandpass/filter, and so forth. INST_ID --> meta.id;instr identifying the instrument or instruments used to make the observation, VOX:Image_MJDateObs --> time.epoch representing the mean modified Julian date of the observation. POS_EQ_RA_MAIN --> pos.eq.ra representing the ICRS right-ascension of the center of the image. POS_EQ_DEC_MAIN --> pos.eq.dec representing the ICRS declination of the center of the image. VOX:Image_Naxes --> pos.wcs.naxes specifying the number of image axes. VOX:Image_Naxis --> pos.wcs.naxis with the array value giving the length in pixels of each image axis. VOX:Image_Scale --> instr.scale with the array value giving the scale in degrees per pixel of each image axis. VOX:Image_Format --> meta.code.mime specifying the MIME-type of the object associated with the image acref, VOX:STC_CoordRefFrame --> pos.frame representing the coordinate system reference frame, selected from "ICRS", "FK5", "FK4", "ECL", "GAL", and "SGAL". VOX:STC_CoordEquinox --> time.equinox representing the Equinox (not required for ICRS) of the coordinate system VOX:WCS_CoordProjection --> pos.wcs.ctype the array value being the three-character code ("TAN", "ARC", "SIN", and so forth) specifying the celestial projection VOX:WCS_CoordRefPixel --> pos.wcs.crpix with the array value specifying the image pixel coordinates of the WCS reference pixel. This is identical to "CRPIX" in FITS WCS. VOX:WCS_CoordRefValue --> pos.wcs.crval with the array value specifying the world coordinates of the WCS reference pixel. This is identical to "CRVAL" in FITS WCS. VOX:WCS_CDMatrix --> pos.wcs.cdmatrix with the array (matrix) value specifying the WCS CD matrix. This is identical to the "CD" term in FITS WCS, and defines the scale and rotation (among other things) of the image. VOX:BandPass_ID --> instr.bandpass identifying the bandpass by name (e.g., "V", "SDSS_U", "K", "K-Band", etc.). VOX:BandPass_Unit --> meta.unit identifying the units used to represent spectral values, selected from "meters", "hertz", and "keV". VOX:BandPass_RefValue --> em.wl OR em.freq OR em.energy specifying the characteristic (reference) frequency, wavelength, or energy for the bandpass model. VOX:BandPass_HiLimit --> em.wl;stat.max OR em.freq;stat.max OR em.energy;stat.max specifying the upper limit of the bandpass. VOX:BandPass_LoLimit --> em.wl;stat.min OR em.freq;stat.min OR em.energy;stat.min specifying the lower limit of the bandpass. VOX:Image_PixFlags --> meta.code specifying the type of processing done by the image service to produce an output image pixel. VOX:Image_AccessReference --> meta.ref.url specifying the URL to be used to access or retrieve the image. VOX:Image_AccessRefTTL --> time.interval;stat.min specifying the minimum time to live in seconds of the access reference. VOX:Image_FileSize --> phys.size;meta.file representing the actual or estimated size of the encoded image in bytes (not pixels!). From owner-dal@eso.org Wed Mar 24 19:57:18 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2OIv2vR010355 for ; Wed, 24 Mar 2004 19:57:02 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2OIv2rA010345 for dal-outgoing; Wed, 24 Mar 2004 19:57:02 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dal@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2OIuwvR010324; Wed, 24 Mar 2004 19:56:58 +0100 (MET) Received: from skysrv.pha.jhu.edu (skysrv.pha.jhu.edu [128.220.233.32]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i2OIuumW021979; Wed, 24 Mar 2004 19:56:56 +0100 (CET) Received: (from womullan@localhost) by skysrv.pha.jhu.edu (8.11.6/8.11.6) id i2OIutT29883; Wed, 24 Mar 2004 13:56:55 -0500 Date: Wed, 24 Mar 2004 13:56:55 -0500 From: "Wil O'Mullane" To: Roy Williams Cc: dal@ivoa.net, ucd@ivoa.net Subject: Re: New UCD1+ for SIA protocol Message-ID: <20040324135655.D29227@skysrv.pha.jhu.edu> References: <02f401c411d0$3215b650$0c0ba8c0@cacr.caltech.edu> Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii Content-Disposition: inline User-Agent: Mutt/1.2.5.1i In-Reply-To: <02f401c411d0$3215b650$0c0ba8c0@cacr.caltech.edu>; from roy@cacr.caltech.edu on Wed, Mar 24, 2004 at 10:45:35AM -0800 X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-dal@eso.org Precedence: bulk Reply-To: "Wil O'Mullane" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 At the risk of being told this laready and having forgotten ... why do the standard ones like POS_EQ_RA_MAIN change ? I thought this was a move to reomve the VOX: not rename all ucds ... Although I like the dots more than the _.. wil this will break lots of apps which rely on thoose ucds .. On Wed, Mar 24, 2004 at 10:45:35AM -0800, Roy Williams wrote: > Dear UCD and DAL folks > > Three of us (Sebastian Derriere, Andrea Preite-Martinez, myself) have been > working on an update for the SIA protocol that uses the standard UCD set, > now called UCD1+, rather than the ad hoc namespace VOX that SIA 1.0 has been > using. > > In the following, all UCD from the original SIA specification are listed > below. The old SIA UCD is written first, then the suggested new UCD1+ is > written in the line beginning "-->" > > The UCD1+ is not fully documented yet, but you can find a dictionary from > UCD1 to UCD1+ at > http://vizier.u-strasbg.fr/UCD/lists/ucd1-ucd1p.txt > and > http://vizier.u-strasbg.fr/UCD/lists/ucd1p-composed.txt > > The SIA protocol is defined at > http://us-vo.org/pubs/files/ACF8DE.pdf > > The new SIA will be version 1.1, and we are hoping to draft and approve this > at the IVOA meeting at the end of May. > > Thank you for your comments and suggestions on these new assignments > Andrea, Roy, Sebastian > > -------------------------------------------------------- > > VOX:Image_Title > --> meta.title > containing a short (usually one line) description of the image. This should > concisely describe the image to a user, typically identifying the image > source (e.g., survey name), object name or field coordinates, > bandpass/filter, and so forth. > > INST_ID > --> meta.id;instr > identifying the instrument or instruments used to make the observation, > > VOX:Image_MJDateObs > --> time.epoch > representing the mean modified Julian date of the observation. > > POS_EQ_RA_MAIN > --> pos.eq.ra > representing the ICRS right-ascension of the center of the image. > > POS_EQ_DEC_MAIN > --> pos.eq.dec > representing the ICRS declination of the center of the image. > > VOX:Image_Naxes > --> pos.wcs.naxes > specifying the number of image axes. > > VOX:Image_Naxis > --> pos.wcs.naxis > with the array value giving the length in pixels of each image axis. > > VOX:Image_Scale > --> instr.scale > with the array value giving the scale in degrees per pixel of each image > axis. > > VOX:Image_Format > --> meta.code.mime > specifying the MIME-type of the object associated with the image acref, > > VOX:STC_CoordRefFrame > --> pos.frame > representing the coordinate system reference frame, selected from "ICRS", > "FK5", "FK4", "ECL", "GAL", and "SGAL". > > VOX:STC_CoordEquinox > --> time.equinox > representing the Equinox (not required for ICRS) of the coordinate system > > VOX:WCS_CoordProjection > --> pos.wcs.ctype > the array value being the three-character code ("TAN", "ARC", "SIN", and so > forth) specifying the celestial projection > > VOX:WCS_CoordRefPixel > --> pos.wcs.crpix > with the array value specifying the image pixel coordinates of the WCS > reference pixel. This is identical to "CRPIX" in FITS WCS. > > VOX:WCS_CoordRefValue > --> pos.wcs.crval > with the array value specifying the world coordinates of the WCS reference > pixel. This is identical to "CRVAL" in FITS WCS. > > VOX:WCS_CDMatrix > --> pos.wcs.cdmatrix > with the array (matrix) value specifying the WCS CD matrix. This is > identical to the "CD" term in FITS WCS, and defines the scale and rotation > (among other things) of the image. > > VOX:BandPass_ID > --> instr.bandpass > identifying the bandpass by name (e.g., "V", "SDSS_U", "K", "K-Band", etc.). > > VOX:BandPass_Unit > --> meta.unit > identifying the units used to represent spectral values, selected from > "meters", "hertz", and "keV". > > VOX:BandPass_RefValue > --> em.wl OR em.freq OR em.energy > specifying the characteristic (reference) frequency, wavelength, or energy > for the bandpass model. > > VOX:BandPass_HiLimit > --> em.wl;stat.max OR em.freq;stat.max OR em.energy;stat.max > specifying the upper limit of the bandpass. > > VOX:BandPass_LoLimit > --> em.wl;stat.min OR em.freq;stat.min OR em.energy;stat.min > specifying the lower limit of the bandpass. > > VOX:Image_PixFlags > --> meta.code > specifying the type of processing done by the image service to produce an > output image pixel. > > VOX:Image_AccessReference > --> meta.ref.url > specifying the URL to be used to access or retrieve the image. > > VOX:Image_AccessRefTTL > --> time.interval;stat.min > specifying the minimum time to live in seconds of the access reference. > > VOX:Image_FileSize > --> phys.size;meta.file > representing the actual or estimated size of the encoded image in bytes (not > pixels!). From owner-ucd@eso.org Wed Mar 24 20:46:37 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2OJkMvR001398 for ; Wed, 24 Mar 2004 20:46:22 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2OJkMPB001396 for ucd-outgoing; Wed, 24 Mar 2004 20:46:22 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2OJkJvR001370; Wed, 24 Mar 2004 20:46:19 +0100 (MET) Received: from head.cfa.harvard.edu (head.cfa.harvard.edu [131.142.41.8]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i2OJkGmW023737; Wed, 24 Mar 2004 20:46:17 +0100 (CET) Received: from xebec.cfa.harvard.edu (xebec [131.142.52.100]) by head.cfa.harvard.edu (d/w) with ESMTP id i2OJkEsw005782; Wed, 24 Mar 2004 14:46:14 -0500 (EST) From: Arnold Rots Received: (from arots@localhost) by xebec.cfa.harvard.edu (8.12.8p1/8.12.8) id i2OJkEu1003422; Wed, 24 Mar 2004 14:46:14 -0500 (EST) Message-Id: <200403241946.i2OJkEu1003422@xebec.cfa.harvard.edu> Subject: Re: New UCD1+ for SIA protocol In-Reply-To: <02f401c411d0$3215b650$0c0ba8c0@cacr.caltech.edu> To: Roy Williams Date: Wed, 24 Mar 2004 14:46:14 -0500 (EST) CC: dal@ivoa.net, ucd@ivoa.net X-Mailer: ELM [version 2.4ME+ PL99 (25)] MIME-Version: 1.0 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Arnold Rots X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 SIAP 1.1: I had asked that SCORE (used to be GRADE) be included in the list of optional input and output parameters and there seemed to be agreement that it is a useful thing. Output SCORE is a floating point value that ranks returned images according to their relevance for the query as perceived by the server. This is meant to aid the client (especially the non-specialist client) in choosing from a list of images in case more than one image satisfies the query criteria. The scale is always relative and only meaningful in the context of the result in which it is provided. It may measure things like exposure time, image quality, proximity to the specified position, resolution, etc. Input SCORE is a string and may assume two values: SCORE=TOP If multiple images satisfy the query criteria, only the one with the highest value of SCORE (in output) is returned. SCORE=ALL (default) All images satisfying the query criteria are returned. This issue is important for archives of pointed observations where dozens of images may be available satisfying a single query. Expert users may want to see the metadata on all of them and choose, but less sophisticated users and more general services (the issue came up in some of our prototypes/demos as a real problem!) are more likely get annoyed and say: just get me what you think is the best one. And that's what this is about. There is no UCD that fits this, it's a context-dependent thing and, besides, it has a different datatype on input and output. But I'd appreciate its being added. - Arnold Roy Williams wrote: > Dear UCD and DAL folks > > Three of us (Sebastian Derriere, Andrea Preite-Martinez, myself) have been > working on an update for the SIA protocol that uses the standard UCD set, > now called UCD1+, rather than the ad hoc namespace VOX that SIA 1.0 has been > using. > > In the following, all UCD from the original SIA specification are listed > below. The old SIA UCD is written first, then the suggested new UCD1+ is > written in the line beginning "-->" > > The UCD1+ is not fully documented yet, but you can find a dictionary from > UCD1 to UCD1+ at > http://vizier.u-strasbg.fr/UCD/lists/ucd1-ucd1p.txt > and > http://vizier.u-strasbg.fr/UCD/lists/ucd1p-composed.txt > > The SIA protocol is defined at > http://us-vo.org/pubs/files/ACF8DE.pdf > > The new SIA will be version 1.1, and we are hoping to draft and approve this > at the IVOA meeting at the end of May. > > Thank you for your comments and suggestions on these new assignments > Andrea, Roy, Sebastian > > -------------------------------------------------------- > > VOX:Image_Title > --> meta.title > containing a short (usually one line) description of the image. This should > concisely describe the image to a user, typically identifying the image > source (e.g., survey name), object name or field coordinates, > bandpass/filter, and so forth. > > INST_ID > --> meta.id;instr > identifying the instrument or instruments used to make the observation, > > VOX:Image_MJDateObs > --> time.epoch > representing the mean modified Julian date of the observation. > > POS_EQ_RA_MAIN > --> pos.eq.ra > representing the ICRS right-ascension of the center of the image. > > POS_EQ_DEC_MAIN > --> pos.eq.dec > representing the ICRS declination of the center of the image. > > VOX:Image_Naxes > --> pos.wcs.naxes > specifying the number of image axes. > > VOX:Image_Naxis > --> pos.wcs.naxis > with the array value giving the length in pixels of each image axis. > > VOX:Image_Scale > --> instr.scale > with the array value giving the scale in degrees per pixel of each image > axis. > > VOX:Image_Format > --> meta.code.mime > specifying the MIME-type of the object associated with the image acref, > > VOX:STC_CoordRefFrame > --> pos.frame > representing the coordinate system reference frame, selected from "ICRS", > "FK5", "FK4", "ECL", "GAL", and "SGAL". > > VOX:STC_CoordEquinox > --> time.equinox > representing the Equinox (not required for ICRS) of the coordinate system > > VOX:WCS_CoordProjection > --> pos.wcs.ctype > the array value being the three-character code ("TAN", "ARC", "SIN", and so > forth) specifying the celestial projection > > VOX:WCS_CoordRefPixel > --> pos.wcs.crpix > with the array value specifying the image pixel coordinates of the WCS > reference pixel. This is identical to "CRPIX" in FITS WCS. > > VOX:WCS_CoordRefValue > --> pos.wcs.crval > with the array value specifying the world coordinates of the WCS reference > pixel. This is identical to "CRVAL" in FITS WCS. > > VOX:WCS_CDMatrix > --> pos.wcs.cdmatrix > with the array (matrix) value specifying the WCS CD matrix. This is > identical to the "CD" term in FITS WCS, and defines the scale and rotation > (among other things) of the image. > > VOX:BandPass_ID > --> instr.bandpass > identifying the bandpass by name (e.g., "V", "SDSS_U", "K", "K-Band", etc.). > > VOX:BandPass_Unit > --> meta.unit > identifying the units used to represent spectral values, selected from > "meters", "hertz", and "keV". > > VOX:BandPass_RefValue > --> em.wl OR em.freq OR em.energy > specifying the characteristic (reference) frequency, wavelength, or energy > for the bandpass model. > > VOX:BandPass_HiLimit > --> em.wl;stat.max OR em.freq;stat.max OR em.energy;stat.max > specifying the upper limit of the bandpass. > > VOX:BandPass_LoLimit > --> em.wl;stat.min OR em.freq;stat.min OR em.energy;stat.min > specifying the lower limit of the bandpass. > > VOX:Image_PixFlags > --> meta.code > specifying the type of processing done by the image service to produce an > output image pixel. > > VOX:Image_AccessReference > --> meta.ref.url > specifying the URL to be used to access or retrieve the image. > > VOX:Image_AccessRefTTL > --> time.interval;stat.min > specifying the minimum time to live in seconds of the access reference. > > VOX:Image_FileSize > --> phys.size;meta.file > representing the actual or estimated size of the encoded image in bytes (not > pixels!). > -------------------------------------------------------------------------- Arnold H. Rots Chandra X-ray Science Center Smithsonian Astrophysical Observatory tel: +1 617 496 7701 60 Garden Street, MS 67 fax: +1 617 495 7356 Cambridge, MA 02138 arots@head.cfa.harvard.edu USA http://hea-www.harvard.edu/~arots/ -------------------------------------------------------------------------- From owner-ucd@eso.org Wed Mar 24 21:56:37 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2OKuMvR018830 for ; Wed, 24 Mar 2004 21:56:22 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2OKuMXu018829 for ucd-outgoing; Wed, 24 Mar 2004 21:56:22 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2OKuCvR018764; Wed, 24 Mar 2004 21:56:12 +0100 (MET) Received: from [134.171.76.11] (vpn-11.hq.eso.org [134.171.76.11]) by serapis.hq.eso.org (8.11.7+Sun/8.11.7) with ESMTP id i2OKuCs28590; Wed, 24 Mar 2004 21:56:12 +0100 (MET) In-Reply-To: <02f401c411d0$3215b650$0c0ba8c0@cacr.caltech.edu> References: <02f401c411d0$3215b650$0c0ba8c0@cacr.caltech.edu> Mime-Version: 1.0 (Apple Message framework v613) Content-Type: text/plain; charset=US-ASCII; format=flowed Message-Id: Content-Transfer-Encoding: 7bit Cc: , From: Alberto Micol Subject: Re: New UCD1+ for SIA protocol Date: Wed, 24 Mar 2004 21:56:11 +0100 To: "Roy Williams" X-Mailer: Apple Mail (2.613) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Alberto Micol X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 After a first glance: I like it! Well, this is not really helping anybody out there, is it? Only two points (in the temporary absence of an established data model): > VOX:Image_Scale > --> instr.scale > with the array value giving the scale in degrees per pixel of each > image > axis. > Wouldn't it be better to have it as --> pos.wcs.scale ? This parameter has to do with the way the data are sampled, and any software could resample it (eg drizzle) onto a different grid than the original instrumental pixel scale (and think of the case where data from different instruments are mosaic'd together). In the end the instrument (instr.) has nothing to do with the pixel scale. And, anyway the pixel scale can be computed from the pos.wcs.cdmatrix... why do we need it? Probably for queries ... Unless you meant the actual resolution (Rayleigh, seeing, etc) Yet again in this case instr. is not the place to store it. Actually, where is the resolution in this scheme? Probably it was not in the SIAP, but I should read the SIAP specs again. > VOX:Image_AccessReference > --> meta.ref.url > specifying the URL to be used to access or retrieve the image. This is complex ... there could be various URLs associated to the same image, e.g., to access the full product or only a preview; but I need to read the SIAP doc again before insisting on this. Alberto From owner-ucd@eso.org Wed Mar 24 22:32:17 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2OLW2vR000344 for ; Wed, 24 Mar 2004 22:32:02 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2OLW2H4000343 for ucd-outgoing; Wed, 24 Mar 2004 22:32:02 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2OLVxvR000310; Wed, 24 Mar 2004 22:31:59 +0100 (MET) Received: from mxsf23.cluster1.charter.net (mxsf23.cluster1.charter.net [209.225.28.223]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i2OLVv3R014200; Wed, 24 Mar 2004 22:31:58 +0100 (CET) Received: from mlaptop.localdomain (68-117-223-254.cpe.ga.charter.com [68.117.223.254]) by mxsf23.cluster1.charter.net (8.12.10/8.12.8) with ESMTP id i2OLMXAv011672; Wed, 24 Mar 2004 16:22:34 -0500 (EST) (envelope-from brian.thomas@gsfc.nasa.gov) From: Brian Thomas To: Alberto Micol Subject: Re: New UCD1+ for SIA protocol Date: Wed, 24 Mar 2004 16:21:17 -0500 User-Agent: KMail/1.6 References: <02f401c411d0$3215b650$0c0ba8c0@cacr.caltech.edu> In-Reply-To: Cc: , MIME-Version: 1.0 Content-Disposition: inline Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit Message-Id: <200403241621.17502.brian.thomas@gsfc.nasa.gov> X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Brian Thomas X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 On Wednesday 24 March 2004 03:56 pm, Alberto Micol wrote: > After a first glance: I like it! Well, this is not really helping > anybody out there, is it? Well, I will try to push for this in the NOAO data model that our group is working on. =b.t. From owner-ucd@eso.org Wed Mar 24 22:53:06 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2OLqjvR009632 for ; Wed, 24 Mar 2004 22:52:45 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2OLqjBv009631 for ucd-outgoing; Wed, 24 Mar 2004 22:52:45 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2OLqgvR009620; Wed, 24 Mar 2004 22:52:42 +0100 (MET) Received: from revere.aoc.nrao.edu (revere.aoc.nrao.edu [146.88.1.15]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i2OLqd3R016089; Wed, 24 Mar 2004 22:52:40 +0100 (CET) Received: from zia.aoc.nrao.edu (zia [146.88.1.4]) by revere.aoc.nrao.edu (8.11.6/8.11.6) with ESMTP id i2OLqZs29058; Wed, 24 Mar 2004 14:52:35 -0700 Received: from oak.aoc.nrao.edu (oak.aoc.nrao.edu [146.88.3.232]) by zia.aoc.nrao.edu (8.12.9/8.12.5) with ESMTP id i2OLqXUr021770; Wed, 24 Mar 2004 14:52:34 -0700 (MST) Date: Wed, 24 Mar 2004 14:52:33 -0700 (MST) From: Doug Tody X-X-Sender: dtody@oak To: Alberto Micol cc: Roy Williams , , Subject: Re: New UCD1+ for SIA protocol In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-MailScanner-Information: Please contact postmaster@aoc.nrao.edu for more information X-MailScanner: Found to be clean X-MailScanner-SpamCheck: not spam, SpamAssassin (score=-6.7, required 7, BAYES_01 -5.40, EMAIL_ATTRIBUTION -0.50, IN_REP_TO -0.37, QUOTED_EMAIL_TEXT -0.38, REPLY_WITH_QUOTES 0.00, USER_AGENT_PINE 0.00) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Doug Tody X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi Alberto - On Wed, 24 Mar 2004, Alberto Micol wrote: > Only two points (in the temporary absence of an established data model): > > > VOX:Image_Scale > > --> instr.scale > > with the array value giving the scale in degrees per pixel of each > > image > > axis. > > > > Wouldn't it be better to have it as --> pos.wcs.scale ? > This parameter has to do with the way the data are sampled, > and any software could resample it (eg drizzle) onto a different grid > than the original instrumental pixel scale (and think of the case where > data from different instruments are mosaic'd together). > In the end the instrument (instr.) has nothing to do with the pixel > scale. > > And, anyway the pixel scale can be computed from the pos.wcs.cdmatrix... > why do we need it? Probably for queries ... All we are doing here is normalizing the UCDs for SIA - for V1.1 we would prefer to minimize serious changes to the interface. Anyway, although the image scale can be computed from the CD matrix, 1) scale is a major image attribute which we prefer to have readily available to the client without having to process the WCS, 2) while the image scale is a required parameter, the WCS is merely "strongly recommended" and data providers are not required to provide it. If the WCS is missing, it can be approximated from the required image parameters, i.e., CRPIX the image center, CRVAL is POS in IRCS coordinates, the image is assumed to be nonrotated, and the CD matrix is thus defined by the naxis and scale values. > Actually, where is the resolution in this scheme? > Probably it was not in the SIAP, but I should read the SIAP specs again. SIA does not currently have the full sampling/bandpass data characterization which we have discussed elsewhere. At some point we would like to add this. V1.1 is conceivable if it comes along fast enough. > > VOX:Image_AccessReference > > --> meta.ref.url > > specifying the URL to be used to access or retrieve the image. > > This is complex ... there could be various URLs associated to > the same image, e.g., to access the full product or only a preview; > but I need to read the SIAP doc again before insisting on this. These each get a different row of the query response VOTable, hence each has a different acref URL. We have another proposal (again from Roy) to define an optional logical name which can be used to tag each row in the query result. Rows which refer to the "same image" but differ only in image format, bandpass, or whatever, would have the same logical name to indicate that they are associated. - Doug From owner-ucd@eso.org Wed Mar 24 23:19:55 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2OMJevR013831 for ; Wed, 24 Mar 2004 23:19:40 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2OMJeTk013830 for ucd-outgoing; Wed, 24 Mar 2004 23:19:40 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2OMJYvR013799; Wed, 24 Mar 2004 23:19:34 +0100 (MET) Received: from [134.171.76.11] (vpn-11.hq.eso.org [134.171.76.11]) by serapis.hq.eso.org (8.11.7+Sun/8.11.7) with ESMTP id i2OMJYs01316; Wed, 24 Mar 2004 23:19:34 +0100 (MET) In-Reply-To: <200403241621.17502.brian.thomas@gsfc.nasa.gov> References: <02f401c411d0$3215b650$0c0ba8c0@cacr.caltech.edu> <200403241621.17502.brian.thomas@gsfc.nasa.gov> Mime-Version: 1.0 (Apple Message framework v613) Content-Type: text/plain; charset=US-ASCII; format=flowed Message-Id: <5441B66E-7DE1-11D8-A564-000A95D007D2@eso.org> Content-Transfer-Encoding: 7bit Cc: "" From: Alberto Micol Subject: Re: New UCD1+ for SIA protocol Date: Wed, 24 Mar 2004 23:19:34 +0100 To: "" X-Mailer: Apple Mail (2.613) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Alberto Micol X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Dear Doug, Yes, I completely agree with all you said, and understand the normalisation of UCDs; my only objection was on the UCD name not to be linked to the instrument (instr.scale) but to the pos.wcs. That is, I'm proposing: instr.scale to be replaced by pos.wcs.scale for all the reasons I already reported. Sorry not to have been too clear the first time. Alberto PS: I understand from Brian that also my comment ("not helping anybody out there") was misunderstood: I was in no way criticising the normalisation, which in fact I like. It looks like this is not my day, better I close here and go to bed ... From owner-dal@eso.org Thu Mar 25 15:48:11 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PEiYiR010325 for ; Thu, 25 Mar 2004 15:44:34 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2PEiYO8010323 for dal-outgoing; Thu, 25 Mar 2004 15:44:34 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dal@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PEiEiR010242; Thu, 25 Mar 2004 15:44:14 +0100 (MET) Received: from donner.stsci.edu (donner.stsci.edu [130.167.251.65]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i2PEi93R013337; Thu, 25 Mar 2004 15:44:10 +0100 (CET) Received: from aria (aria.stsci.edu [130.167.236.125]) by donner.stsci.edu (Mirapoint Messaging Server MOS 3.3.6-GR) with ESMTP id AJW64036; Thu, 25 Mar 2004 09:44:06 -0500 (EST) Message-ID: <00cc01c41277$9ffe2e20$7deca782@stsci.edu> From: "Robert Hanisch" To: "Doug Tody" , "Alberto Micol" Cc: "Roy Williams" , , References: Subject: Re: New UCD1+ for SIA protocol Date: Thu, 25 Mar 2004 09:44:06 -0500 Organization: Space Telescope Science Institute MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Junkmail-Whitelist: YES (by domain whitelist at donner.stsci.edu) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-dal@eso.org Precedence: bulk Reply-To: "Robert Hanisch" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 I just want to add my support for Alberto's objection to instr.scale -- I think this could be very confusing. The scale here is not an attribute of the instrument, but of the image. Glancing quickly through the UCD-UCD1+ mapping, however, I do not see a UCD that fits very well. Is meta.bullshit going to stay? Bob ----- Original Message ----- From: "Doug Tody" To: "Alberto Micol" Cc: "Roy Williams" ; ; Sent: Wednesday, March 24, 2004 4:52 PM Subject: Re: New UCD1+ for SIA protocol > Hi Alberto - > > On Wed, 24 Mar 2004, Alberto Micol wrote: > > Only two points (in the temporary absence of an established data model): > > > > > VOX:Image_Scale > > > --> instr.scale > > > with the array value giving the scale in degrees per pixel of each > > > image > > > axis. > > > > > > > Wouldn't it be better to have it as --> pos.wcs.scale ? > > This parameter has to do with the way the data are sampled, > > and any software could resample it (eg drizzle) onto a different grid > > than the original instrumental pixel scale (and think of the case where > > data from different instruments are mosaic'd together). > > In the end the instrument (instr.) has nothing to do with the pixel > > scale. > > > > And, anyway the pixel scale can be computed from the pos.wcs.cdmatrix... > > why do we need it? Probably for queries ... > > All we are doing here is normalizing the UCDs for SIA - for V1.1 we would > prefer to minimize serious changes to the interface. Anyway, although > the image scale can be computed from the CD matrix, 1) scale is a major > image attribute which we prefer to have readily available to the client > without having to process the WCS, 2) while the image scale is a required > parameter, the WCS is merely "strongly recommended" and data providers are > not required to provide it. If the WCS is missing, it can be approximated > from the required image parameters, i.e., CRPIX the image center, CRVAL > is POS in IRCS coordinates, the image is assumed to be nonrotated, and > the CD matrix is thus defined by the naxis and scale values. > > > Actually, where is the resolution in this scheme? > Probably it was > not in the SIAP, but I should read the SIAP specs again. > > SIA does not currently have the full sampling/bandpass data characterization > which we have discussed elsewhere. At some point we would like to add this. > V1.1 is conceivable if it comes along fast enough. > > > > VOX:Image_AccessReference > > > --> meta.ref.url > > > specifying the URL to be used to access or retrieve the image. > > > > This is complex ... there could be various URLs associated to > > the same image, e.g., to access the full product or only a preview; > > but I need to read the SIAP doc again before insisting on this. > > These each get a different row of the query response VOTable, hence each > has a different acref URL. We have another proposal (again from Roy) > to define an optional logical name which can be used to tag each row in > the query result. Rows which refer to the "same image" but differ only > in image format, bandpass, or whatever, would have the same logical name > to indicate that they are associated. > > - Doug > > From owner-dal@eso.org Thu Mar 25 16:14:15 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PFDqiR018136 for ; Thu, 25 Mar 2004 16:13:52 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2PFDqSS018130 for dal-outgoing; Thu, 25 Mar 2004 16:13:52 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dal@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PFBnir017475; Thu, 25 Mar 2004 16:13:38 +0100 (MET) Received: from virgo.sdc.org (virgo.sdc.org [209.155.42.1]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i2PF4MmW028059; Thu, 25 Mar 2004 16:04:23 +0100 (CET) Received: from lepus.tuc.noao.edu (dtody [209.155.156.44]) by virgo.sdc.org (8.12.8/8.12.8) with ESMTP id i2PF4BHI014386; Thu, 25 Mar 2004 08:04:13 -0700 Date: Thu, 25 Mar 2004 08:04:09 -0700 (MST) From: Doug Tody X-X-Sender: dtody@lepus.tuc.noao.edu To: Robert Hanisch cc: Alberto Micol , Roy Williams , , Subject: Re: New UCD1+ for SIA protocol In-Reply-To: <00cc01c41277$9ffe2e20$7deca782@stsci.edu> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-RAVMilter-Version: 8.4.3(snapshot 20030212) (virgo) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-dal@eso.org Precedence: bulk Reply-To: Doug Tody X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 On Thu, 25 Mar 2004, Robert Hanisch wrote: > I just want to add my support for Alberto's objection to instr.scale -- I > think this could be very confusing. The scale here is not an attribute of > the instrument, but of the image. Glancing quickly through the UCD-UCD1+ > mapping, however, I do not see a UCD that fits very well. I also agree, this is the image scale not an instrument attribute. A larger point here is that in the process of normalizing the UCDS in SIA V1.1, we also plan to introduce UTYPE. The recommendation for folks writing software interfaces to interpret SIA tables will be to use UTYPE to identify the formally defined elements of the interface. This is very straightforward whereas UCD is not; we can evolve UCD independently and our interfaces will not break. Hence it is up to the UCD folks to assign the best UCDs for these fields, and if we have to adjust or generalize them later we will be able do so. In general I think UCD should be used for hard things like inference, semantic associations, smart queries, etc. UTYPE is much simpler and is what we need to identify interface elements in a straightforward manner. - Doug From owner-ucd@eso.org Thu Mar 25 16:15:00 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PFEWiR018348 for ; Thu, 25 Mar 2004 16:14:32 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2PFEWA6018344 for ucd-outgoing; Thu, 25 Mar 2004 16:14:32 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PFEHiR018271; Thu, 25 Mar 2004 16:14:17 +0100 (MET) Received: from gannet.scg.man.ac.uk (gannet.scg.man.ac.uk [130.88.94.110]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i2PFEFmW028462; Thu, 25 Mar 2004 16:14:15 +0100 (CET) Received: from star1.jb.man.ac.uk ([130.88.24.176]) by gannet.scg.man.ac.uk with esmtp (Exim 4.20) id 1B6WYg-000COW-7Y; Thu, 25 Mar 2004 15:14:14 +0000 Received: from [130.88.24.148] (helo=adikia) by star1.jb.man.ac.uk with esmtp (Exim 3.03 #2) id 1B6WYg-0000MS-00; Thu, 25 Mar 2004 15:14:14 +0000 Date: Thu, 25 Mar 2004 15:14:13 +0000 (GMT) From: Anita Richards X-X-Sender: amsr@adikia To: Robert Hanisch cc: Doug Tody , Alberto Micol , Roy Williams , dal@ivoa.net, ucd@ivoa.net Subject: Re: New UCD1+ for SIA protocol In-Reply-To: <00cc01c41277$9ffe2e20$7deca782@stsci.edu> Message-ID: References: <00cc01c41277$9ffe2e20$7deca782@stsci.edu> MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanner: exiscan for exim4 (http://duncanthrax.net/exiscan/) *1B6WYg-000COW-7Y*CN.rzMY6nNo* X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Anita Richards X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Bob Hanisch wrote > I just want to add my support for Alberto's objection to instr.scale -- I > think this could be very confusing. The scale here is not an attribute of > the instrument, but of the image. Glancing quickly through the UCD-UCD1+ > mapping, however, I do not see a UCD that fits very well. Alberto (I think) wrote > > Actually, where is the resolution in this scheme? > Probably it was > not in the SIAP, but I should read the SIAP specs again. To underline these points, I think thaat there may be a tendency to think of images as products of instruments using pixel detectors, where the pixel scale of the instrument determines the resolution of the image and the sampling interval of the image. But of course that ain't necessarily so. As has been pointed out, data processing can change the image pixel size of even CCD images let alone other forms of data. The resolution is determined by the PSF, but even that means different things in different regimes. Both pixel size and resolution are variable e.g. by weighting radio data. Hence for describing images you need an image pixel size. Resolution is tricker since even in a single image that can be brightness dependent. In the Registry we would use a range but in describing images I think that the choices are 1) Just use image pixel size and assume that everyone uses something close to the convention of 3 pixels across a resolution element most of the time (but as resolution is unspecified the user will have to think about it and hence will not be misled). This is probably best for images but maybe not for catalogue data. 2) Use a 'characteristic resolution'. However, that is problematic for images as this may not be specified in the FITS header (e.g. in radio images the restoring beam size is usually in there but can be buried deep in the history). However it is often what is given in catalogues. cheers a - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - - Dr. Anita M. S. Richards, AVO Astronomer MERLIN/VLBI National Facility, University of Manchester, Jodrell Bank Observatory, Macclesfield, Cheshire SK11 9DL, U.K. tel +44 (0)1477 572683 (direct); 571321 (switchboard); 571618 (fax). From owner-dal@eso.org Thu Mar 25 16:39:00 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PFcciR025027 for ; Thu, 25 Mar 2004 16:38:38 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2PFcbT7025021 for dal-outgoing; Thu, 25 Mar 2004 16:38:37 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dal@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PFThjT022260; Thu, 25 Mar 2004 16:38:25 +0100 (MET) Received: from mail.cacr.caltech.edu (mail.cacr.caltech.edu [131.215.145.9]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i2PFHC3R014810; Thu, 25 Mar 2004 16:17:12 +0100 (CET) Received: from Ropy (dsl-64-30-223-60.lcinet.net [64.30.223.60]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id i2PFH8k4026888 (version=TLSv1/SSLv3 cipher=RC4-MD5 bits=128 verify=NO); Thu, 25 Mar 2004 07:17:09 -0800 Message-ID: <020801c4127c$3bf4a530$7201a8c0@Ropy> From: "Roy Williams" To: "Robert Hanisch" , "Doug Tody" , "Alberto Micol" Cc: , References: <00cc01c41277$9ffe2e20$7deca782@stsci.edu> Subject: Re: New UCD1+ for SIA protocol Date: Thu, 25 Mar 2004 07:17:04 -0800 MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-dal@eso.org Precedence: bulk Reply-To: "Roy Williams" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 > Is meta.bullshit going to stay? Definitely. From owner-ucd@eso.org Thu Mar 25 16:45:45 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PFjSiR026825 for ; Thu, 25 Mar 2004 16:45:28 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2PFjSE0026824 for ucd-outgoing; Thu, 25 Mar 2004 16:45:28 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PFjFiR026767; Thu, 25 Mar 2004 16:45:15 +0100 (MET) Received: from E1000.artov.rm.cnr.it (saturn.rm.iasf.cnr.it [150.146.136.11]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i2PFj53R016057; Thu, 25 Mar 2004 16:45:08 +0100 (CET) Received: from saturn.rm.iasf.cnr.it(150.146.136.11) by E1000.artov.rm.cnr.it via csmap id 96e8c404_7e73_11d8_89dd_0002b3da0f69_31452; Thu, 25 Mar 2004 16:46:36 +0100 (CET) Received: from apm.rm.iasf.cnr.it (apm.rm.iasf.cnr.it [150.146.136.115]) by saturn.rm.iasf.cnr.it (8.11.3/8.11.3) with ESMTP id i2PFl0P11634; Thu, 25 Mar 2004 16:47:00 +0100 Date: Thu, 25 Mar 2004 16:45:07 +0100 (ora solare Europa occidentale) From: Andrea Preite Martinez To: Robert Hanisch cc: Doug Tody , Alberto Micol , Roy Williams , dal@ivoa.net, ucd@ivoa.net Subject: Re: New UCD1+ for SIA protocol In-Reply-To: <00cc01c41277$9ffe2e20$7deca782@stsci.edu> Message-ID: References: <00cc01c41277$9ffe2e20$7deca782@stsci.edu> X-X-Sender: andrea@saturn.rm.iasf.cnr.it MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Andrea Preite Martinez X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 A comment on 1) VOX:Image_Scale --> instr.scale and 2) UCD1+:meta.bullshit (Bob's message) 1. In the list of ucd1+ that I derived, the atoms "image" and "scale" are present in instr.scale and obs.image . To me the concept of scale in this context is more important than the concept of image, then I supported "instr.scale". A much better alternative could be the definition of the new ucd1+: obs.image.scale 2. While examining all the tables and columns in Vizier I came across 2 or 3 columns whose names and descriptions were so cryptical that even going to the original papers I could not understand the nature of what the author(s) had in mind to describe. My limitation, of course. I then marked those cases with this (probably a bit offensive) tag. The file ~/ucd1-ucd1p.txt was then automatically generated from a much bigger/detailed file, and the tag slipped through. If and when we will move to ucd1+, I'll remove it. Andrea ============================================================================== Andrea Preite Martinez andrea@rm.iasf.cnr.it Istituto di Astrofisica Spaziale Tel.:+39.06.4993.4641 Area di Ricerca di Tor Vergata Fax.:+39.06.2066.0188 Via del Fosso del Cavaliere 100 Cell:+39.339.3817355 00133 Roma ============================================================================== From owner-dal@eso.org Thu Mar 25 16:52:54 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PFqaiR028698 for ; Thu, 25 Mar 2004 16:52:36 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2PFqa1R028695 for dal-outgoing; Thu, 25 Mar 2004 16:52:36 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dal@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PFqTiR028660; Thu, 25 Mar 2004 16:52:29 +0100 (MET) Received: from donner.stsci.edu (donner.stsci.edu [130.167.251.65]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i2PFqQmW000179; Thu, 25 Mar 2004 16:52:27 +0100 (CET) Received: from aria (aria.stsci.edu [130.167.236.125]) by donner.stsci.edu (Mirapoint Messaging Server MOS 3.3.6-GR) with ESMTP id AJW68556; Thu, 25 Mar 2004 10:52:09 -0500 (EST) Message-ID: <018101c41281$219f5db0$7deca782@stsci.edu> From: "Robert Hanisch" To: "Andrea Preite Martinez" Cc: "Doug Tody" , "Alberto Micol" , "Roy Williams" , , References: <00cc01c41277$9ffe2e20$7deca782@stsci.edu> Subject: Re: New UCD1+ for SIA protocol Date: Thu, 25 Mar 2004 10:52:09 -0500 Organization: Space Telescope Science Institute MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Junkmail-Whitelist: YES (by domain whitelist at donner.stsci.edu) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-dal@eso.org Precedence: bulk Reply-To: "Robert Hanisch" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 ----- Original Message ----- From: "Andrea Preite Martinez" To: "Robert Hanisch" Cc: "Doug Tody" ; "Alberto Micol" ; "Roy Williams" ; ; Sent: Thursday, March 25, 2004 10:45 AM Subject: Re: New UCD1+ for SIA protocol > A comment on > > 1) VOX:Image_Scale --> instr.scale > and > > 2) UCD1+:meta.bullshit (Bob's message) > > 1. In the list of ucd1+ that I derived, the atoms "image" and "scale" are > present in instr.scale and obs.image . To me the concept of scale in this > context is more important than the concept of image, then I supported > "instr.scale". > A much better alternative could be the definition of the new ucd1+: > obs.image.scale Yes, much better! > 2. While examining all the tables and columns in Vizier I came across 2 or > 3 columns whose names and descriptions were so cryptical that even going to > the original papers I could not understand the nature of what the author(s) > had in mind to describe. My limitation, of course. I then marked those > cases with this (probably a bit offensive) tag. > The file ~/ucd1-ucd1p.txt was then automatically generated from a much > bigger/detailed file, and the tag slipped through. If and when we will move > to ucd1+, I'll remove it. How about meta.unknown? Not that I am so easy to offend, mind you, but... Bob > > Andrea > ============================================================================ == > Andrea Preite Martinez andrea@rm.iasf.cnr.it > Istituto di Astrofisica Spaziale Tel.:+39.06.4993.4641 > Area di Ricerca di Tor Vergata Fax.:+39.06.2066.0188 > Via del Fosso del Cavaliere 100 Cell:+39.339.3817355 > 00133 Roma > ============================================================================ == > > > From owner-ucd@eso.org Thu Mar 25 17:00:06 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PFxiiR000327 for ; Thu, 25 Mar 2004 16:59:44 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2PFxiqP000322 for ucd-outgoing; Thu, 25 Mar 2004 16:59:44 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PFxQiR000240; Thu, 25 Mar 2004 16:59:26 +0100 (MET) Received: from revere.aoc.nrao.edu (revere.aoc.nrao.edu [146.88.1.15]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i2PFxOmW000599; Thu, 25 Mar 2004 16:59:24 +0100 (CET) Received: from zia.aoc.nrao.edu (zia [146.88.1.4]) by revere.aoc.nrao.edu (8.11.6/8.11.6) with ESMTP id i2PFxHs26098; Thu, 25 Mar 2004 08:59:18 -0700 Received: from oak.aoc.nrao.edu (oak.aoc.nrao.edu [146.88.3.232]) by zia.aoc.nrao.edu (8.12.9/8.12.5) with ESMTP id i2PFxGUr011535; Thu, 25 Mar 2004 08:59:16 -0700 (MST) Date: Thu, 25 Mar 2004 08:59:16 -0700 (MST) From: Doug Tody X-X-Sender: dtody@oak To: dal@ivoa.net, Subject: Re: New UCD1+ for SIA protocol In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-MailScanner-Information: Please contact postmaster@aoc.nrao.edu for more information X-MailScanner: Found to be clean X-MailScanner-SpamCheck: not spam, SpamAssassin (score=-6.7, required 7, BAYES_01 -5.40, EMAIL_ATTRIBUTION -0.50, IN_REP_TO -0.37, QUOTED_EMAIL_TEXT -0.38, REPLY_WITH_QUOTES 0.00, USER_AGENT_PINE 0.00) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Doug Tody X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Taking this one step further: if we start inventing UCDs which are nothing more than the names of data model attributes, this may indicate that something is wrong. Perhaps what we should be doing is using UTYPE to define the data model attribute or interface element (if there is one), and UCD to say something about the quantity given as the value. For example, if the UTYPE is something like image.scale, then the UCD might define the type of physical quantity including units. Currently we try to fix the quantity/units, but there are cases where this needs to vary even though we are talking about a single data model attribute. - Doug On Thu, 25 Mar 2004, Doug Tody wrote: > On Thu, 25 Mar 2004, Robert Hanisch wrote: > > I just want to add my support for Alberto's objection to instr.scale -- I > > think this could be very confusing. The scale here is not an attribute of > > the instrument, but of the image. Glancing quickly through the UCD-UCD1+ > > mapping, however, I do not see a UCD that fits very well. > > I also agree, this is the image scale not an instrument attribute. > > A larger point here is that in the process of normalizing the UCDS in > SIA V1.1, we also plan to introduce UTYPE. The recommendation for folks > writing software interfaces to interpret SIA tables will be to use UTYPE > to identify the formally defined elements of the interface. This is very > straightforward whereas UCD is not; we can evolve UCD independently and > our interfaces will not break. Hence it is up to the UCD folks to assign > the best UCDs for these fields, and if we have to adjust or generalize them > later we will be able do so. > > In general I think UCD should be used for hard things like inference, > semantic associations, smart queries, etc. UTYPE is much simpler and is > what we need to identify interface elements in a straightforward manner. > > - Doug > > From owner-ucd@eso.org Thu Mar 25 17:00:45 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PG0OiR000674 for ; Thu, 25 Mar 2004 17:00:24 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2PG0O47000670 for ucd-outgoing; Thu, 25 Mar 2004 17:00:24 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PG0BiR000588; Thu, 25 Mar 2004 17:00:11 +0100 (MET) Received: from gannet.scg.man.ac.uk (gannet.scg.man.ac.uk [130.88.94.110]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i2PG09mW000639; Thu, 25 Mar 2004 17:00:09 +0100 (CET) Received: from star1.jb.man.ac.uk ([130.88.24.176]) by gannet.scg.man.ac.uk with esmtp (Exim 4.20) id 1B6XH6-000Iw3-E0; Thu, 25 Mar 2004 16:00:08 +0000 Received: from [130.88.24.148] (helo=adikia) by star1.jb.man.ac.uk with esmtp (Exim 3.03 #2) id 1B6XH6-0000zT-00; Thu, 25 Mar 2004 16:00:08 +0000 Date: Thu, 25 Mar 2004 16:00:08 +0000 (GMT) From: Anita Richards X-X-Sender: amsr@adikia To: Andrea Preite Martinez cc: Robert Hanisch , Doug Tody , Alberto Micol , Roy Williams , dal@ivoa.net, ucd@ivoa.net Subject: Re: New UCD1+ for SIA protocol In-Reply-To: Message-ID: References: <00cc01c41277$9ffe2e20$7deca782@stsci.edu> MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanner: exiscan for exim4 (http://duncanthrax.net/exiscan/) *1B6XH6-000Iw3-E0*edTjeeCqleA* X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Anita Richards X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 > > 1) VOX:Image_Scale --> instr.scale > > A much better alternative could be the definition of the new ucd1+: > obs.image.scale That still suggest to me that the scale is inherant to the observations - but it is better > 2) UCD1+:meta.bullshit (Bob's message) > bigger/detailed file, and the tag slipped through. If and when we will move > to ucd1+, I'll remove it. Or jsut wait until your critics stop talking bullshit? You and Roy and Sebastien have done a pretty good job if people can only find 1.5 ucd1+'s to complain about! a From owner-dal@eso.org Thu Mar 25 17:02:32 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PG2EiR001477 for ; Thu, 25 Mar 2004 17:02:15 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2PG2E3A001475 for dal-outgoing; Thu, 25 Mar 2004 17:02:14 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dal@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PG1ciR001211; Thu, 25 Mar 2004 17:01:38 +0100 (MET) Received: from head.cfa.harvard.edu (head.cfa.harvard.edu [131.142.41.8]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i2PG1amW000685; Thu, 25 Mar 2004 17:01:37 +0100 (CET) Received: from urania.cfa.harvard.edu (urania [131.142.52.147]) by head.cfa.harvard.edu (d/w) with ESMTP id i2PG1Xph012044; Thu, 25 Mar 2004 11:01:33 -0500 (EST) From: Jonathan McDowell Received: (from jcm@localhost) by urania.cfa.harvard.edu (8.12.8p1/8.12.8) id i2PG1VKf007368; Thu, 25 Mar 2004 11:01:31 -0500 (EST) Date: Thu, 25 Mar 2004 11:01:31 -0500 (EST) Message-Id: <200403251601.i2PG1VKf007368@urania.cfa.harvard.edu> To: ucd@ivoa.net, roy@cacr.caltech.edu, andrea@rm.iasf.cnr.it, alberto.micol@eso.org, hanisch@stsci.edu, dal@ivoa.net, dtody@aoc.nrao.edu Subject: Re: New UCD1+ for SIA protocol X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-dal@eso.org Precedence: bulk Reply-To: Jonathan McDowell X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Apologies if this is already covered, I missed some emails.. My biggest problem is "pos.wcs" which generalizes poorly. Seems to me that naxis and naxes are properties of the pixels, and indeed of the image and not of pos itself. What if you have an x,y,time cube? I would argue it would be obs.image.naxes obs.image.naxis or perhaps obs.image.wcs.naxes obs.image.wcs.naxis (or array.naxes or whatever the top level thing, but not pos) but not pos.naxes = 2 time.naxes = 1 pos.naxis = 512 512 time.naxis = 30 Similarly, the other wcs.* should probably be image.wcs.* not pos.wcs.* ? I agree with others comments about instr.scale; Should be image.wcs.scale I am generally confused about what is in "wcs" and what is not: "pos.frame" not part of wcs, but "pos.wcs.naxes" is? > > meta.bullshit > meta.unknown? I think the first is a more accurate description; how about meta.badly_defined or meta.obscure :-) - Jonathan From owner-ucd@eso.org Thu Mar 25 17:05:54 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PG5NiR002573 for ; Thu, 25 Mar 2004 17:05:23 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2PG5NGr002571 for ucd-outgoing; Thu, 25 Mar 2004 17:05:23 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PG51iR002426; Thu, 25 Mar 2004 17:05:01 +0100 (MET) Received: from eso.org (st14.hq.eso.org [134.171.10.25]) by serapis.hq.eso.org (8.11.7+Sun/8.11.7) with ESMTP id i2PG51s23577; Thu, 25 Mar 2004 17:05:01 +0100 (MET) Message-ID: <4063032C.2090803@eso.org> Date: Thu, 25 Mar 2004 17:05:00 +0100 From: Alberto Micol User-Agent: Mozilla/5.0 (X11; U; SunOS sun4u; en-US; rv:1.0.1) Gecko/20020920 Netscape/7.0 X-Accept-Language: en-us, en MIME-Version: 1.0 To: Andrea Preite Martinez CC: dal@ivoa.net, ucd@ivoa.net Subject: Re: New UCD1+ for SIA protocol References: <00cc01c41277$9ffe2e20$7deca782@stsci.edu> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Alberto Micol X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 >1. In the list of ucd1+ that I derived, the atoms "image" and "scale" are >present in instr.scale and obs.image . To me the concept of scale in this >context is more important than the concept of image, then I supported >"instr.scale". >A much better alternative could be the definition of the new ucd1+: >obs.image.scale > Sorry Andrea, But if we go for obs.image.scale then one would also think that the following should exist: obs.spectrum.scale And furthermore, personally if I see a scale at that level then I also expect: obs.image.wcs.ctype obs.image.wcs.crpix obs.image.wcs.crval obs.image.wcs.cdmatrix etc. and similarly for obs.spectrum ... Hence, I like much better the pos than the obs.image because it is more generic. So in the end I like much better: pos.wcs.ctype pos.wcs.crval pos.wcs.scale !!! etc etc because we can reuse it in many different contexts (spectra, images etc). Let's keep together all the "how is the dataset sampled?" elements under the same UCD (pos) and not let them spread under different ones. Alberto PS: Yes Anita they did a good job indeed! From owner-ucd@eso.org Thu Mar 25 17:14:45 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PGELiR005106 for ; Thu, 25 Mar 2004 17:14:21 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2PGEL63005105 for ucd-outgoing; Thu, 25 Mar 2004 17:14:21 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PGE4iR005008 for ; Thu, 25 Mar 2004 17:14:04 +0100 (MET) Received: from sainfoin.extra.cea.fr (sainfoin.extra.cea.fr [132.166.172.103]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i2PGE23R017445 for ; Thu, 25 Mar 2004 17:14:02 +0100 (CET) Received: from araneus.saclay.cea.fr (araneus.saclay.cea.fr [132.166.192.110]) by sainfoin.extra.cea.fr (8.12.10/8.12.9/CEAnet-Internet.2.0) with ESMTP id i2PGE1op029716 for ; Thu, 25 Mar 2004 17:14:01 +0100 (MET) Received: from nenuphar.saclay.cea.fr (unverified) by araneus.saclay.cea.fr (Content Technologies SMTPRS 4.3.12) with ESMTP id ; Thu, 25 Mar 2004 17:14:15 +0100 Received: from discovery.saclay.cea.fr (discovery.saclay.cea.fr [132.166.26.121]) by nenuphar.saclay.cea.fr (8.12.10/8.12.9/CEAnet-Internet.2.0) with ESMTP id i2PGE0Zq028058; Thu, 25 Mar 2004 17:14:00 +0100 (MET) Received: from cea.fr by discovery.saclay.cea.fr (8.8.8+Sun/SMI-SVR4) id RAA23995; Thu, 25 Mar 2004 17:13:52 +0100 (MET) Message-ID: <40630548.2030906@cea.fr> Date: Thu, 25 Mar 2004 17:14:00 +0100 From: Pierre Didelon Organization: CEA User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.4) Gecko/20030624 Netscape/7.1 (ax) X-Accept-Language: en-us, en MIME-Version: 1.0 To: Andrea Preite Martinez CC: Robert Hanisch , ucd@ivoa.net Subject: Re: New UCD1+ for SIA protocol References: <00cc01c41277$9ffe2e20$7deca782@stsci.edu> <018101c41281$219f5db0$7deca782@stsci.edu> In-Reply-To: <018101c41281$219f5db0$7deca782@stsci.edu> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Pierre Didelon X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Robert Hanisch wrote: > ----- Original Message ----- > From: "Andrea Preite Martinez" > To: "Robert Hanisch" > Cc: "Doug Tody" ; "Alberto Micol" > ; "Roy Williams" ; > ; > Sent: Thursday, March 25, 2004 10:45 AM > Subject: Re: New UCD1+ for SIA protocol > > > >>A comment on >> >>1) VOX:Image_Scale --> instr.scale >>and >> >>2) UCD1+:meta.bullshit (Bob's message) >> >>1. In the list of ucd1+ that I derived, the atoms "image" and "scale" are >>present in instr.scale and obs.image . To me the concept of scale in this >>context is more important than the concept of image, then I supported >>"instr.scale". >>A much better alternative could be the definition of the new ucd1+: >>obs.image.scale > > > Yes, much better! > Does images always be related tightly to observation? what about an image loosely related to observation, obtained, as already stressed, by drizzle or anyother image processing task, or even "images" obtained by simulation and so no much link with obs.? But this is may be a too DM oriented view. -- Pierre -------------------------------------------------------------------------- DIDELON :@: pdidelon_at_cea.fr Phone : 33 (0)1 69 08 58 89 CEA SACLAY - Service d'Astrophysique 91191 Gif-Sur-Yvette Cedex -------------------------------------------------------------------------- From owner-dal@eso.org Thu Mar 25 18:49:22 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PHmuiR025107 for ; Thu, 25 Mar 2004 18:48:56 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2PHmt8J025106 for dal-outgoing; Thu, 25 Mar 2004 18:48:55 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dal@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PHmfiR025029; Thu, 25 Mar 2004 18:48:41 +0100 (MET) Received: from revere.aoc.nrao.edu (revere.aoc.nrao.edu [146.88.1.15]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i2PHmc3R021259; Thu, 25 Mar 2004 18:48:39 +0100 (CET) Received: from zia.aoc.nrao.edu (zia [146.88.1.4]) by revere.aoc.nrao.edu (8.11.6/8.11.6) with ESMTP id i2PHjMs02939; Thu, 25 Mar 2004 10:45:22 -0700 Received: from oak.aoc.nrao.edu (oak.aoc.nrao.edu [146.88.3.232]) by zia.aoc.nrao.edu (8.12.9/8.12.5) with ESMTP id i2PHjKUr001828; Thu, 25 Mar 2004 10:45:20 -0700 (MST) Date: Thu, 25 Mar 2004 10:45:20 -0700 (MST) From: Doug Tody X-X-Sender: dtody@oak To: Anita Richards cc: dal@ivoa.net, Subject: Re: New UCD1+ for SIA protocol In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-MailScanner-Information: Please contact postmaster@aoc.nrao.edu for more information X-MailScanner: Found to be clean X-MailScanner-SpamCheck: not spam, SpamAssassin (score=-6.7, required 7, BAYES_01 -5.40, EMAIL_ATTRIBUTION -0.50, IN_REP_TO -0.37, QUOTED_EMAIL_TEXT -0.38, REPLY_WITH_QUOTES 0.00, USER_AGENT_PINE 0.00) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-dal@eso.org Precedence: bulk Reply-To: Doug Tody X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 On Thu, 25 Mar 2004, Anita Richards wrote: > > 1) VOX:Image_Scale --> instr.scale > > > > A much better alternative could be the definition of the new ucd1+: > > obs.image.scale > > That still suggest to me that the scale is inherant to the observations - > but it is better This is a general issue with what we are calling the "observation" data model. This may be just a naming issue but I worry that we may try to describe actual observations. What we really need to do for VO is characterize the physical attributes of a dataset. A dataset may be a calibrated observation, or it may be the result of an arbitrary amount of processing of multiple observations, or it may be synthetic data. It does not matter how the dataset was generated if we describe only the physical attributes of the actual final dataset we are dealing with. Scale and resolution are good examples of such physical attributes. For VO data analysis where we may need to deal uniformly with data from many origins, physical dataset characterization is what is needed. At this level we should not have any information about the actual observations, instrument characteristics, etc., (if any) used to produce the dataset. Such information may be present in each individual dataset, and can be useful to fully understand individual datasets, but is not very useful for automated processing of data from many origins. A simple example is exposure time. While a typical attribute of an individual original observation, it tells us almost nothing about an arbitrary dataset. To understand what this means we would have to understand the full instrumental model and configuration, and all the post-processing done to get to the final dataset we are actually looking at. The related physical dataset attributes are the sampling and coverage in time of the final (possibly aggregate) dataset, and some physical measure of the limiting flux of a signal detected by the dataset. From owner-ucd@eso.org Thu Mar 25 19:22:21 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PIM5iR000863 for ; Thu, 25 Mar 2004 19:22:06 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2PIM56T000862 for ucd-outgoing; Thu, 25 Mar 2004 19:22:05 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2PIM2iR000841 for ; Thu, 25 Mar 2004 19:22:02 +0100 (MET) Received: from apollo.le.ac.uk (ntp2b.le.ac.uk [143.210.16.125]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i2PIM03R022517 for ; Thu, 25 Mar 2004 19:22:00 +0100 (CET) Received: from [143.210.36.58] (helo=mail.star.le.ac.uk) by apollo.le.ac.uk with smtp (Exim 4.30) id 1B6ZUN-0002QL-Lb for ucd@ivoa.net; Thu, 25 Mar 2004 18:21:59 +0000 Received: (qmail 22101 invoked from network); 25 Mar 2004 18:22:20 -0000 Received: from sparky.star.le.ac.uk (143.210.36.10) by mail.star.le.ac.uk with SMTP; 25 Mar 2004 18:22:20 -0000 Date: Thu, 25 Mar 2004 18:22:20 +0000 (GMT) From: "Patricio F. Ortiz" To: Doug Tody cc: Anita Richards , , Subject: Re: New UCD1+ for SIA protocol In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Patricio F. Ortiz" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Doug, I fully agree with you, I think you hit the nail, it is the dataset that the user gets what needs proper description, regardless of what's been done to reach this result. A dataset has an angular scale ("/pix) or a linear scale (km/pix, eg, solar or planetary images), the dataset's origin may be real observations or simulations, simple observations (classical CCD image), mosaics, images based on radio data, multiwavelength composites, whatever. Scales can be degraded or modified from the initial products (eg, DSS) As you said, something similar happens when describing the time coverage. Quantities which make sense to individual observations don't necessariry apply to final products (datasets), for instance, exposure_time != end_of_exposure - start_of_exposure in a dataset which does not represent an individual observation. Color composite images are another example of a final product where the individual observations' parameters may vary considerably, talking about instrument.scale or obs.scale does not seem appropriate anymore. At the time of the construction of UCD0 it did make sense to group these items (read drop these items) in the "instrumental" category. That doesn't apply any longer. Cheers, Patricio On Thu, 25 Mar 2004, Doug Tody wrote: > On Thu, 25 Mar 2004, Anita Richards wrote: > > > > 1) VOX:Image_Scale --> instr.scale > > > > > > A much better alternative could be the definition of the new ucd1+: > > > obs.image.scale > > > > That still suggest to me that the scale is inherant to the observations - > > but it is better > > This is a general issue with what we are calling the "observation" > data model. This may be just a naming issue but I worry that we may try > to describe actual observations. > > What we really need to do for VO is characterize the physical attributes > of a dataset. A dataset may be a calibrated observation, or it may be > the result of an arbitrary amount of processing of multiple observations, > or it may be synthetic data. It does not matter how the dataset was > generated if we describe only the physical attributes of the actual final > dataset we are dealing with. Scale and resolution are good examples of > such physical attributes. > > For VO data analysis where we may need to deal uniformly with data from > many origins, physical dataset characterization is what is needed. At this > level we should not have any information about the actual observations, > instrument characteristics, etc., (if any) used to produce the dataset. > Such information may be present in each individual dataset, and can be > useful to fully understand individual datasets, but is not very useful > for automated processing of data from many origins. > > A simple example is exposure time. While a typical attribute of an > individual original observation, it tells us almost nothing about an > arbitrary dataset. To understand what this means we would have to > understand the full instrumental model and configuration, and all the > post-processing done to get to the final dataset we are actually looking at. > The related physical dataset attributes are the sampling and coverage in > time of the final (possibly aggregate) dataset, and some physical measure > of the limiting flux of a signal detected by the dataset. --- Patricio F. Ortiz pfo@star.le.ac.uk AstroGrid project Department of Physics and Astronomy University of Leicester Tel: +44 (0)116 252 2015 LE1 7RH, UK From owner-dal@eso.org Fri Mar 26 18:52:21 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2QHpkEJ000625 for ; Fri, 26 Mar 2004 18:51:46 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2QHpkt7000624 for dal-outgoing; Fri, 26 Mar 2004 18:51:46 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dal@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2QHpfEJ000600; Fri, 26 Mar 2004 18:51:41 +0100 (MET) Received: from newb6.u-strasbg.fr (newb6.u-strasbg.fr [130.79.128.16]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i2QHpd3R003877; Fri, 26 Mar 2004 18:51:39 +0100 (CET) Received: from astro.u-strasbg.fr (localhost [127.0.0.1]) by newb6.u-strasbg.fr (8.9.3/8.9.3) with ESMTP id SAA05257; Fri, 26 Mar 2004 18:50:50 +0100 (MET) Message-ID: <40646D7A.9EE207DD@astro.u-strasbg.fr> Date: Fri, 26 Mar 2004 18:50:50 +0100 From: Sebastien Derriere Organization: Observatoire de Strasbourg X-Mailer: Mozilla 4.7 [en] (X11; I; SunOS 5.6 sun4u) X-Accept-Language: en MIME-Version: 1.0 To: Arnold Rots CC: dal@ivoa.net, ucd@ivoa.net Subject: Re: New UCD1+ for SIA protocol References: <200403241946.i2OJkEu1003422@xebec.cfa.harvard.edu> Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit X-MailScanner-Astro: Message analyse non infecte par sophos sur astro.u-strasbg.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-dal@eso.org Precedence: bulk Reply-To: Sebastien Derriere X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Arnold Rots wrote: > > SIAP 1.1: > > I had asked that SCORE (used to be GRADE) be included in the list of > optional input and output parameters and there seemed to be agreement > that it is a useful thing. Hello Arnold, If this SCORE is added to the parameters, there is one UCD that could be used: meta.code.qual is a quality/precision/reliability index or flag. Sebastien. -- _______ / ~ /, Sebastien Derriere mailto:derriere@astro.u-strasbg.fr / ~~~~ // Observatoire de Strasbourg Phone +33 (0) 390 242 444 /______// 11, rue de l'universite Telefax +33 (0) 390 242 417 (______(/ F-67000 Strasbourg France From owner-dal@eso.org Fri Mar 26 21:35:45 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2QKZQEJ012285 for ; Fri, 26 Mar 2004 21:35:26 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i2QKZQwd012284 for dal-outgoing; Fri, 26 Mar 2004 21:35:26 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dal@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i2QKZIEJ012253; Fri, 26 Mar 2004 21:35:18 +0100 (MET) Received: from head.cfa.harvard.edu (head.cfa.harvard.edu [131.142.41.8]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i2QKZG3R009198; Fri, 26 Mar 2004 21:35:16 +0100 (CET) Received: from xebec.cfa.harvard.edu (xebec [131.142.52.100]) by head.cfa.harvard.edu (d/w) with ESMTP id i2QKZCph022151; Fri, 26 Mar 2004 15:35:12 -0500 (EST) From: Arnold Rots Received: (from arots@localhost) by xebec.cfa.harvard.edu (8.12.8p1/8.12.8) id i2QKZCM4000824; Fri, 26 Mar 2004 15:35:12 -0500 (EST) Message-Id: <200403262035.i2QKZCM4000824@xebec.cfa.harvard.edu> Subject: Re: New UCD1+ for SIA protocol In-Reply-To: <40646D7A.9EE207DD@astro.u-strasbg.fr> To: Sebastien Derriere Date: Fri, 26 Mar 2004 15:35:11 -0500 (EST) CC: Arnold Rots , dal@ivoa.net, ucd@ivoa.net X-Mailer: ELM [version 2.4ME+ PL99 (25)] MIME-Version: 1.0 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-dal@eso.org Precedence: bulk Reply-To: Arnold Rots X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Sebastien, Yes, I had noticed that one but thought that maybe it should be preserved for a more formal and precise quality or, more specifically, the quality of the data. For instance, when you have two exposures, one of 1000 s and one of 100000 s, the score of the latter may be higher, even though the quality of the data in the former may be better. What it amounts to is that score and quality are notr quite the same concept. Data quality is a component but not the only thing that goes into a score. - Arnold Sebastien Derriere wrote: > Arnold Rots wrote: > > > > SIAP 1.1: > > > > I had asked that SCORE (used to be GRADE) be included in the list of > > optional input and output parameters and there seemed to be agreement > > that it is a useful thing. > > Hello Arnold, > > If this SCORE is added to the parameters, there is one UCD that > could be used: meta.code.qual is a quality/precision/reliability > index or flag. > > Sebastien. > > -- > _______ > / ~ /, Sebastien Derriere mailto:derriere@astro.u-strasbg.fr > / ~~~~ // Observatoire de Strasbourg Phone +33 (0) 390 242 444 > /______// 11, rue de l'universite Telefax +33 (0) 390 242 417 > (______(/ F-67000 Strasbourg France > -------------------------------------------------------------------------- Arnold H. Rots Chandra X-ray Science Center Smithsonian Astrophysical Observatory tel: +1 617 496 7701 60 Garden Street, MS 67 fax: +1 617 495 7356 Cambridge, MA 02138 arots@head.cfa.harvard.edu USA http://hea-www.harvard.edu/~arots/ -------------------------------------------------------------------------- From owner-ucd@eso.org Thu Apr 1 17:21:23 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i31FKxTa016782 for ; Thu, 1 Apr 2004 17:20:59 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i31FKxK6016777 for ucd-outgoing; Thu, 1 Apr 2004 17:20:59 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i31FKuTa016763; Thu, 1 Apr 2004 17:20:56 +0200 (MEST) Received: from head.cfa.harvard.edu (head.cfa.harvard.edu [131.142.41.8]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i31FKs3R013633; Thu, 1 Apr 2004 17:20:55 +0200 (CEST) Received: from xebec.cfa.harvard.edu (xebec [131.142.52.100]) by head.cfa.harvard.edu (d/w) with ESMTP id i31FKr3P020622; Thu, 1 Apr 2004 10:20:53 -0500 (EST) From: Arnold Rots Received: (from arots@localhost) by xebec.cfa.harvard.edu (8.12.8p1/8.12.8) id i31FKqLc016068; Thu, 1 Apr 2004 10:20:52 -0500 (EST) Message-Id: <200404011520.i31FKqLc016068@xebec.cfa.harvard.edu> Subject: Re: New UCD1+ for SIA protocol In-Reply-To: <200403241946.i2OJkEu1003422@xebec.cfa.harvard.edu> To: dal@ivoa.net, ucd@ivoa.net Date: Thu, 1 Apr 2004 10:20:52 -0500 (EST) X-Mailer: ELM [version 2.4ME+ PL99 (25)] MIME-Version: 1.0 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-milter (http://amavis.org/) X-Virus-Scanned: by amavisd-milter (http://amavis.org/) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Arnold Rots X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 I was asked to write something about the SCORE parameter for SIAP: SCORE This parameter is intended to aid the user in selecting an image in cases where a SIAP query would return multiple images. This is especially intended for non-expert users and for users who have no need, for their present purposes, to check through the metadata provided in other parameters. The criteria for determining the SCORE are entirely up to the service provider, since different considerations come into play for different archives. Some hints are provided below. We implicitly trust the providers to choose the best algorithm for the majority of the users, based on the fact that they know their data properties better than anybody else. Output SCORE is a floating point value that ranks returned images according to their relevance for the query as perceived by the server. This is meant to aid the client (especially the non-specialist client) in choosing from a list of images in case more than one image satisfies the query criteria. The scale is always relative and only meaningful in the context of the result in which it is provided. The highest number represents the "best" image available that satisfies the query. There is no specified range. It may measure things like exposure time, image quality, proximity to the specified position, resolution, etc. Input SCORE is a string and may assume two values: SCORE=TOP If multiple images satisfy the query criteria, only the one with the highest value of SCORE (in output) is returned. SCORE=ALL (default) All images satisfying the query criteria are returned. This issue is important for archives of pointed observations where dozens of images may be available satisfying a single query. Expert users may want to see the metadata on all of them and choose, but less sophisticated users and more general services (the issue came up in some of our prototypes/demos as a real problem!) are more likely get annoyed and say: just get me what you think is the best one. And that's what this is about. Note that SCORE is not necessarily a measure of data quality: a 1000 s exposure of high-quality data may still score lower than a 100000 s exposure of somewhat poorer quality. Nor does it say anything about how well each image satisfies the query: all returned images are expected to match the query's criteria. The question really is: among all these matches, how well do we think the user will like them, or how well will they fit the user's purposes? I would like to emphasize two things: 1. The scoring scale should be relative and only have meaning within a particular response list. I.e., you cannot necessarily compare the scores that come from two different queries and deduce any meaningful conclusion. The scoring may not even be linear. 2. The user is free to like or to dislike, to trust or to distrust the scores that are returned. If the user does not like the scores, (s)he should look at the actual metadata returned with each image in the response. Designing a scoring algorithm takes some thought and will be very mission/observatory specific. To illustrate this let me list the considerations that went into the Chandra archive's algorithm: - Exposure time; clearly, longer exposures produce higher-quality images - Instrument: ACIS-I/S, HRC-I/S; this is based on the different sensitivities and spectral responses - Co-allignment with requested position; Chandra's PSF quickly gets worse off-axis - Image resolution; we have two canned images at different resolutions and with different FOV. One might consider adding other factors, such as seeing/aspect quality. It is likely that we will continue to fine-tune the algorithm. I don't think it is particularly useful to publish the algorithm or its description. Frankly, I suspect that those who rely on SCORE don't really care and that those who care wnat to inspect the metadata to make their own decision. There is no UCD that fits SCORE, it's a context-dependent thing and, besides, it has a different datatype on input and output. - Arnold -------------------------------------------------------------------------- Arnold H. Rots Chandra X-ray Science Center Smithsonian Astrophysical Observatory tel: +1 617 496 7701 60 Garden Street, MS 67 fax: +1 617 495 7356 Cambridge, MA 02138 arots@head.cfa.harvard.edu USA http://hea-www.harvard.edu/~arots/ -------------------------------------------------------------------------- From owner-ucd@eso.org Mon Apr 26 16:50:58 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i3QEoaOH022198 for ; Mon, 26 Apr 2004 16:50:37 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i3QEoaZe022197 for ucd-outgoing; Mon, 26 Apr 2004 16:50:36 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i3QEoYOH022188 for ; Mon, 26 Apr 2004 16:50:34 +0200 (MEST) Received: from newb6.u-strasbg.fr (newb6.u-strasbg.fr [130.79.128.16]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i3QEoWXe005233 for ; Mon, 26 Apr 2004 16:50:32 +0200 (CEST) Received: from astro.u-strasbg.fr (localhost [127.0.0.1]) by newb6.u-strasbg.fr (8.9.3/8.9.3) with ESMTP id QAA15191; Mon, 26 Apr 2004 16:49:31 +0200 (MET DST) Message-ID: <408D217A.58F8CB30@astro.u-strasbg.fr> Date: Mon, 26 Apr 2004 16:49:30 +0200 From: Sebastien Derriere Organization: Observatoire de Strasbourg X-Mailer: Mozilla 4.7 [en] (X11; I; SunOS 5.6 sun4u) X-Accept-Language: en MIME-Version: 1.0 To: ucd@ivoa.net Subject: towards UCD1+ Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit X-MailScanner-Astro: Message analyse non infecte par sophos sur astro.u-strasbg.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Sebastien Derriere X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hello, I have placed on the IVOA wiki a PDF version of the latest document on UCD: http://www.ivoa.net/internal/IVOA/IvoaUCD/WD-UCD-20040426.pdf This document describes the motivations and procedure to evolve the first generation of UCD into a new scheme called UCD1+. The new scheme has been quite successfully tested on VizieR. It also includes inputs from other fields, like the latest SIAP discussions. As the UCD1+ vocabulary is likely to evolve faster than the reference document itself, the reference lists are available online, together with old versions and history of changes: http://vizier.u-strasbg.fr/UCD/lists/ The document currently has a Working Draft status, but the idea is to promote it to an IVOA Proposed Recommendation. This can be done once agreement is reached within the discussion group, if I understand well the IVOA document lifecycle. So... time for discussion now ! Sebastien. -- _______ / ~ /, Sebastien Derriere mailto:derriere@astro.u-strasbg.fr / ~~~~ // Observatoire de Strasbourg Phone +33 (0) 390 242 444 /______// 11, rue de l'universite Telefax +33 (0) 390 242 417 (______(/ F-67000 Strasbourg France From owner-ucd@eso.org Wed Apr 28 10:48:57 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i3S8mTqP021545 for ; Wed, 28 Apr 2004 10:48:29 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i3S8mTg0021543 for ucd-outgoing; Wed, 28 Apr 2004 10:48:29 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i3S8mOqP021523 for ; Wed, 28 Apr 2004 10:48:24 +0200 (MEST) Received: from katrine.roe.ac.uk (katrine.roe.ac.uk [195.194.120.81]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i3S8mMTY016392 for ; Wed, 28 Apr 2004 10:48:22 +0200 (CEST) Received: from katrine.roe.ac.uk (localhost [127.0.0.1]) by katrine.roe.ac.uk (Postfix) with ESMTP id E045544021; Wed, 28 Apr 2004 09:48:21 +0100 (BST) Received: from somehost by katrine.roe.ac.uk (postfixilter 1.4) with SMTP id 31497; Wed, 28 Apr 2004 09:48:20 +0100 (BST) Received: from katrine (localhost [127.0.0.1]) by localhost (Postfix) with ESMTP id 879C344019; Wed, 28 Apr 2004 09:48:20 +0100 (BST) Received: from localhost ([127.0.0.1]) by katrine.roe.ac.uk (MailMonitor for SMTP v1.2.2 ) ; Wed, 28 Apr 2004 09:48:20 +0100 (BST) Received: from dial.pipex.com (snizort.roe.ac.uk [195.194.120.31]) by katrine.roe.ac.uk (Postfix) with ESMTP id 4DDBE44019; Wed, 28 Apr 2004 09:48:19 +0100 (BST) Message-ID: <408F6FD3.6020009@dial.pipex.com> Date: Wed, 28 Apr 2004 09:48:19 +0100 From: Martin Hill User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.0; en-US; rv:1.5) Gecko/20031013 Thunderbird/0.3 X-Accept-Language: en-us, en MIME-Version: 1.0 To: Sebastien Derriere Cc: ucd@ivoa.net Subject: Re: towards UCD1+ References: <408D217A.58F8CB30@astro.u-strasbg.fr> In-Reply-To: <408D217A.58F8CB30@astro.u-strasbg.fr> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit X-Spam-Checker-Version: SpamAssassin 2.62 (2004-01-11) on katrine.roe.ac.uk X-Spam-Status: No, hits=0.0 required=1000.0 tests=none autolearn=no version=2.62 X-Spam-Level: X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Martin Hill X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi again I agree entirely that UCDs should be used to describe what a value represents rather than how it relates to other things. I think that combining UCDs with data models will give us everything we need. English/typos: Could we use 'phrase' instead of 'words' since really 'phys.temp' consists of two words 'phys' and 'temp' assembled together? Sec 3.3 two cases of "applies a magnitude" I think should read "applies to a magnitude"? Most of these are requests for explanation rather than a request for change: An astronomical question: given UCDs are not supposed to describe units, why do we still have UCDS like 'phot.mag'? Should this be 'phys.brightness', where the units are magnitudes or janskies or ergs or whatever? How are words assembled - eg, why pos.eq.ra instead of pos.ra? How will they be extended? We need more detail on how the UCDs are built up. Using the example of instrument temperature maximum: why is the 'stat.max' added at the end, instead of say, 'phys.temp;stat.max;instr'. Indeed if 'stat.max' is secondary, shouldn't the error be 'phys.temp;stat.error' and we add a 'stat.value' word? Or should we say that order does not matter? If order *is* important this could all get rather fraught. What is the conceptual difference between a word and a phrase? ie, why phys.temp;stat.max;instr instead of 'instr.temp.max', the latter being built from UCD words 'instr' 'temp' and 'max'? Requests for change: Personally I would rather see full names used instead of abbreviations (eg 'physical' instead of 'phys', 'position' instead of 'pos') for anything other than really common terms (ra, dec, max, min). Abbreviations make an insignificant difference to software performance, and can cause confusion especially when non-astronomers are involved in development. Cheers, Martin Sebastien Derriere wrote: > Hello, > > I have placed on the IVOA wiki a PDF version of the latest document > on UCD: http://www.ivoa.net/internal/IVOA/IvoaUCD/WD-UCD-20040426.pdf > This document describes the motivations and procedure to evolve > the first generation of UCD into a new scheme called UCD1+. > The new scheme has been quite successfully tested on VizieR. It also > includes inputs from other fields, like the latest SIAP discussions. > As the UCD1+ vocabulary is likely to evolve faster than the reference > document itself, the reference lists are available online, together with > old > versions and history of changes: > http://vizier.u-strasbg.fr/UCD/lists/ > > The document currently has a Working Draft status, but the idea is > to promote it to an IVOA Proposed Recommendation. This can be done > once agreement is reached within the discussion group, if I understand > well the IVOA document lifecycle. > So... time for discussion now ! > > Sebastien. -- Martin Hill Software Engineer AstroGrid @ ROE Tel: +44 7901 55 24 66 www.astrogrid.org From owner-ucd@eso.org Tue May 4 13:41:43 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i44BexU5001608 for ; Tue, 4 May 2004 13:40:59 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i44BexFc001607 for ucd-outgoing; Tue, 4 May 2004 13:40:59 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i44BeuU5001596 for ; Tue, 4 May 2004 13:40:56 +0200 (MEST) Received: from apollo.le.ac.uk (apollo.le.ac.uk [143.210.16.125]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i44BetXe020503 for ; Tue, 4 May 2004 13:40:55 +0200 (CEST) Received: from [143.210.36.58] (helo=mail.star.le.ac.uk) by apollo.le.ac.uk with smtp (Exim 4.30) id 1BKyIA-0004ja-7r for ucd@ivoa.net; Tue, 04 May 2004 12:40:54 +0100 Received: (qmail 21456 invoked from network); 4 May 2004 11:41:15 -0000 Received: from sparky.star.le.ac.uk (143.210.36.10) by mail.star.le.ac.uk with SMTP; 4 May 2004 11:41:15 -0000 Date: Tue, 4 May 2004 12:41:15 +0100 (BST) From: "Patricio F. Ortiz" To: Sebastien Derriere cc: ucd@ivoa.net Subject: Re: towards UCD1+ In-Reply-To: <408D217A.58F8CB30@astro.u-strasbg.fr> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Patricio F. Ortiz" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi Sebastien, here are some of my comments on UCD1+. Section 2: Syntax if UCDs are case insensitive for all practical purposes, why not limiting the valid characters to uppercase or lowercase alphabet? Allowing both may suggest that B-V is different from b-v (as in the original UCDs), and given that it is easier to type in lowercase than uppercase, I'd suggest that we define UCDs in lowercase only. Section 3.3: combining simple words. After the example, refering to meta.code it says applies a magnitude should say applies to a magnitude In the same section: Examples of UCD1+... in the case of a "maximum temperature of an instrument" my initial reading was "maximum reachable temperature of an instrument" rather than "maximum temperatured reached by an instrument during observation". Surely you meant the second. For the first, do we have now something to denote a feasible range? I can think of few cases where this could be needed though. Page 10, right after equation 2: I think it should read "And define \mu ..." About distances and matching functions: I would like to point to the usefulness of using regular expressions as a way to "discover" related UCDs. Accurate matching is paramount, distances are quite useful, but what if I want to find the quantities involving em.opt.b Those could be phot.mag, colors, errors, etc. As em.opt.b is not a primary word, measuring distances using this element as the starting point may or may not lead anywhere in the matchhing functions described. I've had the chance to play with these features in the original UCDs and sometimes one does not need to start with the main word (or perhaps as Martin pointed out, we should name it differently, "concept" perhaps?) Fortunately, this is an implementation issue and does not require any changes in the structure to UCD1+ to offer a regExp search engine. Section 7.3: hidden in one of the paragraphs is a phrase which I think deserves to be highlighted: << The capacity to lauch broad scope queries (to a number of services) looking for resources containing certain UCDs, freeing ourselves of having to know the specific column names which at the end the service DBMS should use to dig the data. >> The goal is not small, as it implies - accepting UCDs and column names within a query language, - a mechanism to recognize that a "name" represents a UCD - a mechanism to locate those resources which contain the UCDs present in the query and a conversion to column names - a mechanism to launch individual queries to each selected resource - a collection and delivery mechanism. Comment on pos.eq.ra and pos.eq.dec A serious problem I found last year while working in a data federation tool was the fact that ra and dec are meaningless without knowing to which equinox they refer to. In a number of catalogues (I was using Vizier's metadata) the position refered as POS_EQ_RA_MAIN in one catalogue was for J2000, while in others it was for B1950 or other equinoxes. VOTable provides the coosys element, but even with this feature it's not always possible to find the correct match other than resourcing to the using the column name (which is the case of vizier is OK because of its homogeneity, but is not assured in the case of other minor data providers). Besides, some catalogues list positions in more than one equinox and VOTable crashes there. I feel that a sensible way to address this issue is to attach to pos.eq.ra the equinox element, eg, eqnx.J2000 or eqnx.B1975. It is not the best solution, as new elements of meta-data seem to be needed, also to define Groups of elements. I'm thinking in the cases when one works with the meta-data at the registry level rather than the VOTable level, besides, the VOTAble groups and coosys must come from some kind of registry elements (I can guess where these are in Vizier :-) I also feel that the problem is serious enough for us to adress it as soon as possible, as exchange services are being built and they will face these issues as soon as they leave their sand-box and interact with the real world. Finally, congratulations for the document and the way to address the issues, it seems to be a big step in the right direction. Cheers, Patricio On Mon, 26 Apr 2004, Sebastien Derriere wrote: > > Hello, > > I have placed on the IVOA wiki a PDF version of the latest document > on UCD: http://www.ivoa.net/internal/IVOA/IvoaUCD/WD-UCD-20040426.pdf > This document describes the motivations and procedure to evolve > the first generation of UCD into a new scheme called UCD1+. > The new scheme has been quite successfully tested on VizieR. It also > includes inputs from other fields, like the latest SIAP discussions. > As the UCD1+ vocabulary is likely to evolve faster than the reference > document itself, the reference lists are available online, together with > old > versions and history of changes: > http://vizier.u-strasbg.fr/UCD/lists/ > > The document currently has a Working Draft status, but the idea is > to promote it to an IVOA Proposed Recommendation. This can be done > once agreement is reached within the discussion group, if I understand > well the IVOA document lifecycle. > So... time for discussion now ! > > Sebastien. > -- > _______ > / ~ /, Sebastien Derriere mailto:derriere@astro.u-strasbg.fr > / ~~~~ // Observatoire de Strasbourg Phone +33 (0) 390 242 444 > /______// 11, rue de l'universite Telefax +33 (0) 390 242 417 > (______(/ F-67000 Strasbourg France > --- Patricio F. Ortiz pfo@star.le.ac.uk AstroGrid project Department of Physics and Astronomy University of Leicester Tel: +44 (0)116 252 2015 LE1 7RH, UK From owner-ucd@eso.org Wed May 5 13:45:07 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i45BilaN014224 for ; Wed, 5 May 2004 13:44:47 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i45BilTq014223 for ucd-outgoing; Wed, 5 May 2004 13:44:47 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i45BikaN014218 for ; Wed, 5 May 2004 13:44:47 +0200 (MEST) Received: from eso.org (st14.hq.eso.org [134.171.10.25]) by serapis.hq.eso.org (8.11.7+Sun/8.11.7) with ESMTP id i45Bikp28560 for ; Wed, 5 May 2004 13:44:46 +0200 (MEST) Message-ID: <4098D3AE.5050209@eso.org> Date: Wed, 05 May 2004 13:44:46 +0200 From: Alberto Micol User-Agent: Mozilla/5.0 (X11; U; SunOS sun4u; en-US; rv:1.0.1) Gecko/20020920 Netscape/7.0 X-Accept-Language: en-us, en MIME-Version: 1.0 To: ucd@ivoa.net Subject: UCDs as substrings of other UCDs? Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Alberto Micol X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 After having written my original message (see below) I found the solution to my problem (also explained below). I explicit the solution here first asking the following question: Would it be possible to change ::= | to ::= | ? To understand what I'm talking about, I think it's better to read the original message, unless you are good -damn good- at those games where given an answer you have to guess the question. Alberto PS: If you like to play, the subject probably helps ... --- original message, which explains the problem and the way I got to the above-mentioned solution--- Dear UCD builders, It would be very convenient NOT to allow a word to be a substring of other words. Example: Suppose the following two UCDs existed (I'm inventing here): 1. em.IR.H 2. em.IR.Hgamma (Luckily the second one is just only my invention, but it is just to illustrate the point) In this case 1. would be a substring of 2. Why it woud be bad? Because it would unnecessarily complicate a sql query to a table listing UCDs. A query like select * from whatever where UCD like "%em.IR.H%" would return not only the UCD I'm really interested in (em.IR.H) but also the em.IT.Hgamma. The way out, given the fact that UCDs are composed of multiple words semicolon separated, would be to use an "OR" but that is not so efficient: select * from whatever (could be a complicated join) where UCD like "%em.IR.H" or UCD like "%em.IR.H;%" OR, as said, are not efficiently handled. To simplify the usage of UCD in RDBMSes it would be nice to see such rule (not allowing substrings) explicited in the UCD document. I checked the UCD1+ list and I could not find any such case (probably by design?), a part from those obvious cases like em.IR being a substring of em.IR.H where the hierarchy is implied. Even these cases could be avoided if the high level UCD would be formulated differently, eg, em.IR.main (or em.IR.def, def for definition or default) instead of em.IR. But this is less disturbing then the example cited above. Actually, another way out would be to always terminate a word with the semicolon! even if at the end of UCD. E.g., "em.IR;" would do the job quite nicely. This could be avoided quite nicely by change the Backus-Naur definition to always end with a semicolon! Thanks, Alberto From owner-ucd@eso.org Wed May 5 14:43:57 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i45ChiaN022263 for ; Wed, 5 May 2004 14:43:44 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i45ChiTl022262 for ucd-outgoing; Wed, 5 May 2004 14:43:44 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i45ChhaN022256 for ; Wed, 5 May 2004 14:43:43 +0200 (MEST) Received: from eso.org (st14.hq.eso.org [134.171.10.25]) by serapis.hq.eso.org (8.11.7+Sun/8.11.7) with ESMTP id i45Chhp00770 for ; Wed, 5 May 2004 14:43:43 +0200 (MEST) Message-ID: <4098E17F.2000000@eso.org> Date: Wed, 05 May 2004 14:43:43 +0200 From: Alberto Micol User-Agent: Mozilla/5.0 (X11; U; SunOS sun4u; en-US; rv:1.0.1) Gecko/20020920 Netscape/7.0 X-Accept-Language: en-us, en MIME-Version: 1.0 To: ucd@ivoa.net Subject: Re: UCDs as substrings of other UCDs? References: <4098D3AE.5050209@eso.org> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Alberto Micol X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 > Would it be possible to change > ::= | > to > ::= > | > ? I forgot to mention that, obviously, also the Backus-Naur form for UCD should be changed accordingly, that is, by removing the which was moved to the level of a : ::= | Alberto PS: Basically, I find better to always have explicit separators, and not to rely on the implicit "end of string" one. From owner-ucd@eso.org Fri May 7 16:55:02 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i47EsJQX001159 for ; Fri, 7 May 2004 16:54:19 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i47EsI7e001154 for ucd-outgoing; Fri, 7 May 2004 16:54:18 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i47EsBQX001138 for ; Fri, 7 May 2004 16:54:11 +0200 (MEST) Received: from katrine.roe.ac.uk (katrine.roe.ac.uk [195.194.120.81]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i47EsAXe011046 for ; Fri, 7 May 2004 16:54:10 +0200 (CEST) Received: from katrine.roe.ac.uk (localhost [127.0.0.1]) by katrine.roe.ac.uk (Postfix) with ESMTP id 1936944029 for ; Fri, 7 May 2004 15:54:10 +0100 (BST) Received: from somehost by katrine.roe.ac.uk (postfixilter 1.4) with SMTP id 31807; Fri, 07 May 2004 15:54:08 +0100 (BST) Received: from katrine (localhost [127.0.0.1]) by localhost (Postfix) with ESMTP id CF51444028 for ; Fri, 7 May 2004 15:54:08 +0100 (BST) Received: from localhost ([127.0.0.1]) by katrine.roe.ac.uk (MailMonitor for SMTP v1.2.2 ) ; Fri, 7 May 2004 15:54:08 +0100 (BST) Received: from lismore.roe.ac.uk (lismore.roe.ac.uk [195.194.120.117]) by katrine.roe.ac.uk (Postfix) with ESMTP id A41A144028 for ; Fri, 7 May 2004 15:54:08 +0100 (BST) Date: Fri, 7 May 2004 15:54:08 +0100 (BST) From: Bob Mann To: ucd@ivoa.net Subject: Re: towards UCD1+ In-Reply-To: <408D217A.58F8CB30@astro.u-strasbg.fr> Message-ID: References: <408D217A.58F8CB30@astro.u-strasbg.fr> MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Spam-Checker-Version: SpamAssassin 2.62 (2004-01-11) on katrine.roe.ac.uk X-Spam-Status: No, hits=0.0 required=1000.0 tests=none autolearn=no version=2.62 X-Spam-Level: X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Bob Mann X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi folks, I've read with interest the new document from Sebastien and Andrea, and the comments from Martin, Alberto and Patricio. I think that the new document is a clear statement of good principles, and is a significant improvement on the previous documents that have been circulated. I have only a few specific comments, but one general comment on skimming through the current list of UCDs > http://vizier.u-strasbg.fr/UCD/lists/ is that it still shows too strongly its origin in Vizier: a system that defines a specific term for a (b-y) Stromgren colour, but doesn't, so far as I can tell, provide a simple mechanism for denoting something as being an X-ray/optical flux ratio seems a little biased in its perspective to me. If UCD1+ is supposed to be modest in ambition, then my vote would be to have phot.fluxratio (or some such) and delete all the specific phot.color UCDs. One strength of the new document is the discussion of the matching functions. I'd not been convinced of their practical utility before, but I am now, after reading the example given. It would be interesting for that table of mu values to include those from the other proposed matching function, just to indicate how similar they are. I agree with Martin's suggestion that it would be preferable to use complete words, rather than abbreviations. Patricio's comment about equinoxes is an interesting one. The same goes for units, of course, since they are also additional metadata without which the data cannot be used in a meaningful way. But modifying UCD1+ to include grouping of UCDs, as he suggests, would seem to be a significant change, albeit one that is attractive from many points of view. I won't be attending the interoperability meeting in Boston, but I trust that the UCD discussion goes well there - it should, given that Sebastien and Andrea have given it a firm foundation with this document. cheers Bob From owner-ucd@eso.org Tue May 11 17:02:27 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i4BF2A5t018912 for ; Tue, 11 May 2004 17:02:10 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i4BF2Api018911 for ucd-outgoing; Tue, 11 May 2004 17:02:10 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i4BF255t018896 for ; Tue, 11 May 2004 17:02:05 +0200 (MEST) Received: from mail.cacr.caltech.edu (mail.cacr.caltech.edu [131.215.145.9]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i4BF23TY003184 for ; Tue, 11 May 2004 17:02:04 +0200 (CEST) Received: from Ropy (dsl-64-30-223-60.lcinet.net [64.30.223.60]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id i4BF21k4019598 (version=TLSv1/SSLv3 cipher=RC4-MD5 bits=128 verify=NO) for ; Tue, 11 May 2004 08:02:02 -0700 Message-ID: <032701c43768$e9ee1fc0$6701a8c0@Ropy> From: "Roy Williams" To: References: <408D217A.58F8CB30@astro.u-strasbg.fr> <408F6FD3.6020009@dial.pipex.com> Subject: Re: towards UCD1+ Date: Tue, 11 May 2004 08:01:59 -0700 MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1409 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1409 X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Roy Williams" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 I would also like to thank Sebastien and Andrea for this excellent paper. I look forward to discussing in Boston the comments from Martin Hill, Patricio Ortiz, and Bob Mann. However, I think there needs to be an additional document showing the current state of the UCD1+ tree. A printable, versioned IVOA draft document. This will force the rigour of versioning, and allow the IVOA process to control the list of words. When Sebastian and Andrea want to make changes, they should not just change it arbitrarily, but rather build a new version of the UCD Tree document and run it past the IVOA, or the UCD Steering committee, or this mailing list. Is that too rigid and formal? Comments? Roy -------- California Institute of Technology roy@caltech.edu 626 395 3670 From owner-ucd@eso.org Tue May 11 17:25:57 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i4BFPe5t023125 for ; Tue, 11 May 2004 17:25:40 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i4BFPeel023124 for ucd-outgoing; Tue, 11 May 2004 17:25:40 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i4BFPX5t023098 for ; Tue, 11 May 2004 17:25:33 +0200 (MEST) Received: from esacom51.vilspa.esa.int (esacom51-ext.vilspa.esa.int [192.171.2.19]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i4BFPVTY004490 for ; Tue, 11 May 2004 17:25:32 +0200 (CEST) Received: from iso.vilspa.esa.es (isous5.vilspa.esa.es [193.147.153.100]) by esacom51.vilspa.esa.int (8.12.10/8.12.10/ESA-External-v3.2) with ESMTP id i4BFPSVH010387; Tue, 11 May 2004 17:25:28 +0200 (MET DST) Received: from isol03.vilspa.esa.int (isol03.vilspa.esa.int [193.147.153.17]) by iso.vilspa.esa.es (8.12.10/8.12.10) with ESMTP id i4BFPNaT004275; Tue, 11 May 2004 17:25:23 +0200 (MEST) Subject: Re: towards UCD1+ From: Pedro Osuna To: Roy Williams Cc: Pedro.Osuna@esa.int, ucd@ivoa.net In-Reply-To: <032701c43768$e9ee1fc0$6701a8c0@Ropy> References: <408D217A.58F8CB30@astro.u-strasbg.fr> <408F6FD3.6020009@dial.pipex.com> <032701c43768$e9ee1fc0$6701a8c0@Ropy> Content-Type: text/plain Message-Id: <1084289123.12201.7381.camel@isol03.vilspa.esa.int> Mime-Version: 1.0 X-Mailer: Ximian Evolution 1.4.5 (1.4.5-1) Date: Tue, 11 May 2004 17:25:23 +0200 Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Pedro Osuna X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi Roy, we proposed to have a proper board for the control of the UCDs, and a centralized place where all UCD related issues (concerning the inclusion of new UCDs, procedures for request of inclusion of new UCDs, etc) should be handled. I would think it is time to implement this solution (chapter 9 of the latest UCD document). What I do not know is whether this should be agreed at a IVOA exec or what... What do you think? P. On Tue, 2004-05-11 at 17:01, Roy Williams wrote: > I would also like to thank Sebastien and Andrea for this excellent paper. > > I look forward to discussing in Boston the comments from Martin Hill, Patricio > Ortiz, and Bob Mann. > > However, I think there needs to be an additional document showing the current > state of the UCD1+ tree. A printable, versioned IVOA draft document. This will > force the rigour of versioning, and allow the IVOA process to control the list > of words. When Sebastian and Andrea want to make changes, they should not just > change it arbitrarily, but rather build a new version of the UCD Tree document > and run it past the IVOA, or the UCD Steering committee, or this mailing list. > > Is that too rigid and formal? Comments? > > Roy > > -------- > California Institute of Technology > roy@caltech.edu > 626 395 3670 -- Pedro Osuna Alcalaya Software Engineer VILSPA Archive Development Team e-mail: Pedro.Osuna@esa.int Tel + 34 91 8131314 European Space Agency VILLAFRANCA Satellites Tracking Station P.O. Box 50727 E-28080 Villafranca del Castillo MADRID - SPAIN From owner-ucd@eso.org Tue May 11 17:37:05 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i4BFaj5t024737 for ; Tue, 11 May 2004 17:36:45 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i4BFajpj024736 for ucd-outgoing; Tue, 11 May 2004 17:36:45 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i4BFae5t024728 for ; Tue, 11 May 2004 17:36:41 +0200 (MEST) Received: from mail.cacr.caltech.edu (mail.cacr.caltech.edu [131.215.145.9]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i4BFacXe013605 for ; Tue, 11 May 2004 17:36:39 +0200 (CEST) Received: from Ropy (dsl-64-30-223-60.lcinet.net [64.30.223.60]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id i4BFaTk4020874 (version=TLSv1/SSLv3 cipher=RC4-MD5 bits=128 verify=NO); Tue, 11 May 2004 08:36:30 -0700 Message-ID: <037a01c4376d$ba961f20$6701a8c0@Ropy> From: "Roy Williams" To: "Pedro Osuna" Cc: References: <408D217A.58F8CB30@astro.u-strasbg.fr> <408F6FD3.6020009@dial.pipex.com> <032701c43768$e9ee1fc0$6701a8c0@Ropy> <1084289123.12201.7381.camel@isol03.vilspa.esa.int> Subject: Re: towards UCD1+ Date: Tue, 11 May 2004 08:36:28 -0700 MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1409 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1409 X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Roy Williams" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Yes I know. My idea is to have the UCD Steering Committee work with CDS on (a) The next version of the list of words -- working through the IVOA drafting process. (b) The application of UCD in the Simple Data Services (cone, SIAP, SSAP) Are you coming to Boston? Roy -------- California Institute of Technology roy@caltech.edu 626 395 3670 ----- Original Message ----- From: "Pedro Osuna" To: "Roy Williams" Cc: ; Sent: Tuesday, May 11, 2004 8:25 AM Subject: Re: towards UCD1+ > Hi Roy, > > we proposed to have a proper board for the control of the UCDs, and a > centralized place where all UCD related issues (concerning the inclusion > of new UCDs, procedures for request of inclusion of new UCDs, etc) > should be handled. I would think it is time to implement this solution > (chapter 9 of the latest UCD document). What I do not know is whether > this should be agreed at a IVOA exec or what... What do you think? > > P. > > On Tue, 2004-05-11 at 17:01, Roy Williams wrote: > > I would also like to thank Sebastien and Andrea for this excellent paper. > > > > I look forward to discussing in Boston the comments from Martin Hill, Patricio > > Ortiz, and Bob Mann. > > > > However, I think there needs to be an additional document showing the current > > state of the UCD1+ tree. A printable, versioned IVOA draft document. This will > > force the rigour of versioning, and allow the IVOA process to control the list > > of words. When Sebastian and Andrea want to make changes, they should not just > > change it arbitrarily, but rather build a new version of the UCD Tree document > > and run it past the IVOA, or the UCD Steering committee, or this mailing list. > > > > Is that too rigid and formal? Comments? > > > > Roy > > > > -------- > > California Institute of Technology > > roy@caltech.edu > > 626 395 3670 > -- > Pedro Osuna Alcalaya > > > Software Engineer > VILSPA Archive Development Team > e-mail: Pedro.Osuna@esa.int > Tel + 34 91 8131314 > > European Space Agency > VILLAFRANCA Satellites Tracking Station > P.O. Box 50727 > E-28080 Villafranca del Castillo > MADRID - SPAIN > > > From owner-ucd@eso.org Tue May 11 17:41:07 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i4BFem5t025687 for ; Tue, 11 May 2004 17:40:48 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i4BFemLa025686 for ucd-outgoing; Tue, 11 May 2004 17:40:48 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i4BFeg5t025675 for ; Tue, 11 May 2004 17:40:42 +0200 (MEST) Received: from esacom51.vilspa.esa.int (esacom51-ext.vilspa.esa.int [192.171.2.19]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i4BFeeXe013764 for ; Tue, 11 May 2004 17:40:41 +0200 (CEST) Received: from iso.vilspa.esa.es (isous5.vilspa.esa.es [193.147.153.100]) by esacom51.vilspa.esa.int (8.12.10/8.12.10/ESA-External-v3.2) with ESMTP id i4BFecVH010903; Tue, 11 May 2004 17:40:38 +0200 (MET DST) Received: from isol03.vilspa.esa.int (isol03.vilspa.esa.int [193.147.153.17]) by iso.vilspa.esa.es (8.12.10/8.12.10) with ESMTP id i4BFeXaT005161; Tue, 11 May 2004 17:40:33 +0200 (MEST) Subject: Re: towards UCD1+ From: Pedro Osuna To: Roy Williams Cc: Pedro.Osuna@esa.int, ucd@ivoa.net In-Reply-To: <037a01c4376d$ba961f20$6701a8c0@Ropy> References: <408D217A.58F8CB30@astro.u-strasbg.fr> <408F6FD3.6020009@dial.pipex.com> <032701c43768$e9ee1fc0$6701a8c0@Ropy> <1084289123.12201.7381.camel@isol03.vilspa.esa.int> <037a01c4376d$ba961f20$6701a8c0@Ropy> Content-Type: text/plain Message-Id: <1084290033.12201.7392.camel@isol03.vilspa.esa.int> Mime-Version: 1.0 X-Mailer: Ximian Evolution 1.4.5 (1.4.5-1) Date: Tue, 11 May 2004 17:40:33 +0200 Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Pedro Osuna X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Yes, I will arrive there on saturday the 22nd with Jesus Salgado for whatever might be needed (including beers on sunday, if applicable). P. On Tue, 2004-05-11 at 17:36, Roy Williams wrote: > Yes I know. > > My idea is to have the UCD Steering Committee work with CDS on > > (a) The next version of the list of words -- working through the IVOA drafting > process. > > (b) The application of UCD in the Simple Data Services (cone, SIAP, SSAP) > > Are you coming to Boston? > Roy > > > -------- > California Institute of Technology > roy@caltech.edu > 626 395 3670 > ----- Original Message ----- > From: "Pedro Osuna" > To: "Roy Williams" > Cc: ; > Sent: Tuesday, May 11, 2004 8:25 AM > Subject: Re: towards UCD1+ > > > > Hi Roy, > > > > we proposed to have a proper board for the control of the UCDs, and a > > centralized place where all UCD related issues (concerning the inclusion > > of new UCDs, procedures for request of inclusion of new UCDs, etc) > > should be handled. I would think it is time to implement this solution > > (chapter 9 of the latest UCD document). What I do not know is whether > > this should be agreed at a IVOA exec or what... What do you think? > > > > P. > > > > On Tue, 2004-05-11 at 17:01, Roy Williams wrote: > > > I would also like to thank Sebastien and Andrea for this excellent paper. > > > > > > I look forward to discussing in Boston the comments from Martin Hill, > Patricio > > > Ortiz, and Bob Mann. > > > > > > However, I think there needs to be an additional document showing the > current > > > state of the UCD1+ tree. A printable, versioned IVOA draft document. This > will > > > force the rigour of versioning, and allow the IVOA process to control the > list > > > of words. When Sebastian and Andrea want to make changes, they should not > just > > > change it arbitrarily, but rather build a new version of the UCD Tree > document > > > and run it past the IVOA, or the UCD Steering committee, or this mailing > list. > > > > > > Is that too rigid and formal? Comments? > > > > > > Roy > > > > > > -------- > > > California Institute of Technology > > > roy@caltech.edu > > > 626 395 3670 > > -- > > Pedro Osuna Alcalaya > > > > > > Software Engineer > > VILSPA Archive Development Team > > e-mail: Pedro.Osuna@esa.int > > Tel + 34 91 8131314 > > > > European Space Agency > > VILLAFRANCA Satellites Tracking Station > > P.O. Box 50727 > > E-28080 Villafranca del Castillo > > MADRID - SPAIN > > > > > > -- Pedro Osuna Alcalaya Software Engineer VILSPA Archive Development Team e-mail: Pedro.Osuna@esa.int Tel + 34 91 8131314 European Space Agency VILLAFRANCA Satellites Tracking Station P.O. Box 50727 E-28080 Villafranca del Castillo MADRID - SPAIN From owner-ucd@eso.org Mon May 17 20:36:38 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i4HIaLgw019596 for ; Mon, 17 May 2004 20:36:21 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i4HIaL7u019595 for ucd-outgoing; Mon, 17 May 2004 20:36:21 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i4HIaHgw019586; Mon, 17 May 2004 20:36:17 +0200 (MEST) Received: from mail.cacr.caltech.edu (mail.cacr.caltech.edu [131.215.145.9]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i4HIaFTY004761; Mon, 17 May 2004 20:36:16 +0200 (CEST) Received: from SARA (roy-nat.cacr.caltech.edu [131.215.144.149]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id i4HIaEk4012957 (version=TLSv1/SSLv3 cipher=RC4-MD5 bits=128 verify=NO); Mon, 17 May 2004 11:36:14 -0700 Message-ID: <0a8e01c43c3d$fc8765e0$0c0ba8c0@cacr.caltech.edu> From: "Roy Williams" To: Cc: Subject: UCD agenda and UCD/DAL agenda Date: Mon, 17 May 2004 11:37:19 -0700 MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1158 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1165 X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Roy Williams" X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Please find below a suggested draft agenda for the UCD session at the Interop meeting. Note that the second half is joint with the DAL group. If you would like to contribute to the session, or change the agenda below, please drop me a line. Roy ---------------------------------------------- UCD working group Agenda for Interop meeting 1. Sebastien Derriere, UCD Services at CDS 2. Andrea Preite-Martinez, Realization of UCD1+ 3. Roy Williams, UCDs for the Image Access Protocol 4. Doug Tody, UCDs for the Spectral Access Protocol -------- California Institute of Technology roy@caltech.edu 626 395 3670 From owner-ucd@eso.org Fri May 21 19:38:54 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i4LHcbU4000219 for ; Fri, 21 May 2004 19:38:38 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i4LHcbHp000218 for ucd-outgoing; Fri, 21 May 2004 19:38:37 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i4LHcYU4000210 for ; Fri, 21 May 2004 19:38:34 +0200 (MEST) Received: from newb6.u-strasbg.fr (newb6.u-strasbg.fr [130.79.128.16]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i4LHcWTY007854 for ; Fri, 21 May 2004 19:38:32 +0200 (CEST) Received: from astro.u-strasbg.fr (localhost [127.0.0.1]) by newb6.u-strasbg.fr (8.9.3/8.9.3) with ESMTP id TAA16657; Fri, 21 May 2004 19:37:10 +0200 (MET DST) Message-ID: <40AE3E46.57E45165@astro.u-strasbg.fr> Date: Fri, 21 May 2004 19:37:10 +0200 From: Sebastien Derriere Organization: Observatoire de Strasbourg X-Mailer: Mozilla 4.7 [en] (X11; I; SunOS 5.6 sun4u) X-Accept-Language: en MIME-Version: 1.0 To: ucd@ivoa.net Subject: UCD material Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit X-MailScanner-Astro: Message analyse non infecte par sophos sur astro.u-strasbg.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Sebastien Derriere X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hello, I have placed on the IVOA Wiki some new documents: http://www.ivoa.net/twiki/bin/view/IVOA/IvoaUCD A revised version of the EM Spectrum division for UCD v0.3 (following the registry main domains): http://www.ivoa.net/internal/IVOA/IvoaUCD/NoteEMSpectrum-20040520.pdf A slightly revised list of words for UCD1+, with explanations on the choice of the top-level 'atoms' (branches): v0.1 http://www.ivoa.net/internal/IVOA/IvoaUCD/WD-UCDlist-20040520.pdf There is also an on-line form to leave feedback for deletion/ modification/addition of new words: http://cdsweb.u-strasbg.fr/UCD/cgi-bin/comment/ucdComments This can be a technical support for the board in charge of UCD1+, as it sends notifications by email when feedback is left. See you in Boston, Sebastien. -- _______ / ~ /, Sebastien Derriere mailto:derriere@astro.u-strasbg.fr / ~~~~ // Observatoire de Strasbourg Phone +33 (0) 390 242 444 /______// 11, rue de l'universite Telefax +33 (0) 390 242 417 (______(/ F-67000 Strasbourg France From owner-ucd@eso.org Fri Jul 2 15:26:47 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i62DPaLw029640 for ; Fri, 2 Jul 2004 15:26:02 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i62DB9G2027857 for ucd-outgoing; Fri, 2 Jul 2004 15:11:09 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i62DAqLg027822 for ; Fri, 2 Jul 2004 15:10:53 +0200 (MEST) Received: from katrine.roe.ac.uk (katrine.roe.ac.uk [195.194.120.81]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i62DAmEQ000766 for ; Fri, 2 Jul 2004 15:10:49 +0200 (CEST) Received: from katrine.roe.ac.uk (localhost [127.0.0.1]) by katrine.roe.ac.uk (Postfix) with ESMTP id 9AA2B4401B; Fri, 2 Jul 2004 14:10:48 +0100 (BST) Received: from somehost by katrine.roe.ac.uk (postfixilter 1.4) with SMTP id 15985; Fri, 02 Jul 2004 14:10:47 +0100 (BST) Received: from katrine (localhost [127.0.0.1]) by localhost (Postfix) with ESMTP id 554BC4400E; Fri, 2 Jul 2004 14:10:47 +0100 (BST) Received: from localhost ([127.0.0.1]) by katrine.roe.ac.uk (MailMonitor for SMTP v1.2.2 ) ; Fri, 2 Jul 2004 14:10:47 +0100 (BST) Received: from roe.ac.uk (unknown [195.194.122.26]) by katrine.roe.ac.uk (Postfix) with ESMTP id 1A3954400E; Fri, 2 Jul 2004 14:10:47 +0100 (BST) Message-ID: <40E55ED6.3070908@roe.ac.uk> Date: Fri, 02 Jul 2004 14:10:46 +0100 From: "Martin Hill @ ROE" Organization: ROE User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.0; en-US; rv:1.5) Gecko/20031013 Thunderbird/0.3 X-Accept-Language: en-us, en MIME-Version: 1.0 To: ucd@ivoa.net Subject: UCD1 to UCD1+ - one to one mapping? Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit X-Spam-Checker-Version: SpamAssassin 2.62 (2004-01-11) on katrine.roe.ac.uk X-Spam-Status: No, hits=0.0 required=1000.0 tests=none autolearn=no version=2.62 X-Spam-Level: X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Martin Hill @ ROE" X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Is there really a one-one conversion between UCDs and UCD1+s? *Both ways*? That rather sounds as if UCD1+s don't offer anything new! -- Martin Hill, Software Engineer AstroGrid (ROE) +44 7901 55 24 66 http://harris.roe.ac.uk/~mch/ From owner-ucd@eso.org Fri Jul 2 16:31:19 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i62EUbLg009968 for ; Fri, 2 Jul 2004 16:30:37 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i62EUacV009960 for ucd-outgoing; Fri, 2 Jul 2004 16:30:36 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i62EU6Lk009844 for ; Fri, 2 Jul 2004 16:30:28 +0200 (MEST) Received: from ns1.u-strasbg.fr (ns1.u-strasbg.fr [130.79.200.1]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i62Dm9EQ002666 for ; Fri, 2 Jul 2004 15:48:09 +0200 (CEST) Received: from astro.u-strasbg.fr (cluster.u-strasbg.fr [130.79.128.8]) by ns1.u-strasbg.fr (8.12.9p2/jtpda-5.4) with ESMTP id i62Dm8vY067990 ; Fri, 2 Jul 2004 15:48:08 +0200 (CEST) Received: (from genova@localhost) by astro.u-strasbg.fr (8.11.7p1+Sun/8.10.2) id i62Dm7G16122; Fri, 2 Jul 2004 15:48:07 +0200 (MEST) Date: Fri, 2 Jul 2004 15:48:07 +0200 (MEST) Message-Id: <200407021348.i62Dm7G16122@astro.u-strasbg.fr> From: genova@cluster.u-strasbg.fr (Francoise Genova) To: mch@roe.ac.uk, ucd@ivoa.net Cc: genova@newb6.u-strasbg.fr Subject: Re: UCD1 to UCD1+ - one to one mapping? X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-1.5.3 (ns1.u-strasbg.fr [130.79.200.1]); Fri, 02 Jul 2004 15:48:09 +0200 (CEST) X-Antivirus: scanned by sophos at u-strasbg.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: genova@cluster.u-strasbg.fr (Francoise Genova) X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 There is no one-one conversion between UCD and UCD1+. Sorry to say it only now but it takes lot of times to try to follow the discussion... Sebastien is travelling today and I leave a more detail answer to him Francoise From owner-ucd@eso.org Mon Aug 23 17:03:44 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i7NF3c2r025564 for ; Mon, 23 Aug 2004 17:03:38 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id i7NF3ct5025562 for ucd-outgoing; Mon, 23 Aug 2004 17:03:38 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i7NF3c2r025556 for ; Mon, 23 Aug 2004 17:03:38 +0200 (MEST) Received: from newb6.u-strasbg.fr (newb6.u-strasbg.fr [130.79.128.16]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i7NF3a7p029955 for ; Mon, 23 Aug 2004 17:03:37 +0200 (CEST) Received: from astro.u-strasbg.fr (localhost [127.0.0.1]) by newb6.u-strasbg.fr (8.9.3/8.9.3) with ESMTP id RAA14040; Mon, 23 Aug 2004 17:03:11 +0200 (MET DST) Message-ID: <412A072F.363E694B@astro.u-strasbg.fr> Date: Mon, 23 Aug 2004 17:03:11 +0200 From: Sebastien Derriere Organization: Observatoire de Strasbourg X-Mailer: Mozilla 4.7 [en] (X11; I; SunOS 5.6 sun4u) X-Accept-Language: en MIME-Version: 1.0 To: ucd@ivoa.net CC: Dubernet Marie-Lise Subject: PR UCD1+ version 1.05 Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit X-MailScanner-Astro: Message analyse non infecte par sophos sur astro.u-strasbg.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.6.1.107272, Antispam-Core: 4.6.1.104326, Antispam-Data: 2004.8.22.111004 Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Sebastien Derriere X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hello, A new version of the UCD1+ document (v 1.05) is available: http://vizir.u-strasbg.fr/UCD/PR-UCD-20040823.pdf (should be soon on the IVOA web site too). The document is submitted as a Proposed Recommendation, as we seem close to general agreement on this topic. The changes are listed in section 10 of the document. These are mainly further explanations on the guidelines for words combination, but also on the role of the UCD board. The corresponding list of words has been significantly upgraded, and a new document issued: http://www.ivoa.net/internal/IVOA/IvoaUCD/WD-UCDlist-20040823.pdf See appendix B for all changes. The most noticeable are: - the update of the phys.at and phys.mol sections (and the creation of phys.atmol) for better description of atomic and molecular data; - the simplification of the phot.color section to reflect a new syntax for photometric colors; - the creation of a em.line section to describe the commonly used lines (allowing to write now: phot.flux;em.line.Halpha or spect.index;em.line.Hbeta) Also, old UCD material (related to UCD1) has been moved to a new URL: http://vizir.u-strasbg.fr/UCD/old/ while the URL http://vizir.u-strasbg.fr/UCD/ now points to the current definitions of UCD1+. A form is also available to send feedback on UCD1+: http://vizier.u-strasbg.fr/UCD/cgi-bin/comment/ucdComments For each submission, an email is send to a list of email addresses. If you would like to be on this list of board members, just let me know. Sebastien. -- _______ / ~ /, Sebastien Derriere mailto:derriere@astro.u-strasbg.fr / ~~~~ // Observatoire de Strasbourg Phone +33 (0) 390 242 444 /______// 11, rue de l'universite Telefax +33 (0) 390 242 417 (______(/ F-67000 Strasbourg France From owner-ucd@eso.org Mon Aug 23 18:18:34 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i7NGIT2r006672 for ; Mon, 23 Aug 2004 18:18:29 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id i7NGITtB006671 for ucd-outgoing; Mon, 23 Aug 2004 18:18:29 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i7NGIS2r006667 for ; Mon, 23 Aug 2004 18:18:28 +0200 (MEST) Received: from newb6.u-strasbg.fr (newb6.u-strasbg.fr [130.79.128.16]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i7NGIOi6020829 for ; Mon, 23 Aug 2004 18:18:25 +0200 (CEST) Received: from astro.u-strasbg.fr (localhost [127.0.0.1]) by newb6.u-strasbg.fr (8.9.3/8.9.3) with ESMTP id SAA15157; Mon, 23 Aug 2004 18:17:47 +0200 (MET DST) Message-ID: <412A18AB.35AECB88@astro.u-strasbg.fr> Date: Mon, 23 Aug 2004 18:17:47 +0200 From: Sebastien Derriere Organization: Observatoire de Strasbourg X-Mailer: Mozilla 4.7 [en] (X11; I; SunOS 5.6 sun4u) X-Accept-Language: en MIME-Version: 1.0 To: ucd@ivoa.net CC: Dubernet Marie-Lise Subject: Re: PR UCD1+ version 1.05 References: <412A072F.363E694B@astro.u-strasbg.fr> Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit X-MailScanner-Astro: Message analyse non infecte par sophos sur astro.u-strasbg.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.6.1.107272, Antispam-Core: 4.6.1.104326, Antispam-Data: 2004.8.22.111004 Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Sebastien Derriere X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 > Hello, > > A new version of the UCD1+ document (v 1.05) is available: The document has been moved to the IVOA web site: http://www.ivoa.net/Documents/latest/UCD.html Use this URL to access the latest PDF version (or HTML if you prefer) instead of the previous one. Sebastien. From owner-ucd@eso.org Tue Nov 23 16:26:05 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iANFPrZI006498 for ; Tue, 23 Nov 2004 16:25:53 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id iANFPrAF006497 for ucd-outgoing; Tue, 23 Nov 2004 16:25:53 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iANFPkZI006478; Tue, 23 Nov 2004 16:25:46 +0100 (MET) Received: from newb6.u-strasbg.fr (newb6.u-strasbg.fr [130.79.128.16]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iANFPi2i004492; Tue, 23 Nov 2004 16:25:44 +0100 (CET) Received: from astro.u-strasbg.fr (localhost [127.0.0.1]) by newb6.u-strasbg.fr (8.9.3/8.9.3) with ESMTP id QAA16926; Tue, 23 Nov 2004 16:23:25 +0100 (MET) Message-ID: <41A355EC.C9CE978B@astro.u-strasbg.fr> Date: Tue, 23 Nov 2004 16:23:24 +0100 From: Sebastien Derriere Organization: Observatoire de Strasbourg X-Mailer: Mozilla 4.7 [en] (X11; I; SunOS 5.6 sun4u) X-Accept-Language: en MIME-Version: 1.0 To: interop@ivoa.net CC: ucd@ivoa.net Subject: RFC for UCD is ending References: <417F94B0.3491FD4D@astro.u-strasbg.fr> Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit X-MailScanner-Astro: Message analyse non infecte par sophos sur astro.u-strasbg.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.0.111621, Antispam-Engine: 2.0.1.0, Antispam-Data: 2004.11.22.52 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Sebastien Derriere X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hello, The RFC period for the UCD document is ending, and there have been no comments yet !! If you have remarks or want changes, it is time to make them public. Sebastien. Sebastien Derriere wrote: > > Dear all, > > The UCD reference document has been uploaded to the PR area of the > IVOA document repository: > > http://www.ivoa.net/Documents/latest/UCD.html > > I would like to open the 4-weeks RFC period for this document as > of today (Oct 27), with a close date on Nov 24, before promotion to > the Recommendation status. > > A dedicated page has been created for posting comments: > http://www.ivoa.net/twiki/bin/view/IVOA/UnifiedContentDescriptorRFC > and discussions will be conducted on the UCD mailing list > (ucd@ivoa.net). > > Sebastien. -- _______ / ~ /, Sebastien Derriere mailto:derriere@astro.u-strasbg.fr / ~~~~ // Observatoire de Strasbourg Phone +33 (0) 390 242 444 /______// 11, rue de l'universite Telefax +33 (0) 390 242 417 (______(/ F-67000 Strasbourg France From owner-interop@eso.org Tue Nov 23 18:33:33 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iANHWuZI022417 for ; Tue, 23 Nov 2004 18:32:56 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id iANHWuNi022415 for interop-outgoing; Tue, 23 Nov 2004 18:32:56 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-interop@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iANHWoZI022402; Tue, 23 Nov 2004 18:32:50 +0100 (MET) Received: from donner.stsci.edu (donner.stsci.edu [130.167.251.65]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iANHWl2i010163; Tue, 23 Nov 2004 18:32:48 +0100 (CET) Received: from aria (aria.stsci.edu [130.167.236.125]) by donner.stsci.edu (MOS 3.5.5-GR) with ESMTP id BAQ08209; Tue, 23 Nov 2004 12:32:34 -0500 (EST) Message-ID: <009701c4d182$81aeb280$7deca782@stsci.edu> From: "Robert Hanisch" To: "Sebastien Derriere" , Cc: References: <417F94B0.3491FD4D@astro.u-strasbg.fr> <41A355EC.C9CE978B@astro.u-strasbg.fr> Subject: Re: RFC for UCD is ending Date: Tue, 23 Nov 2004 12:33:12 -0500 MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2800.1437 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1441 X-Junkmail-Status: score=0/50, host=donner.stsci.edu X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.0.111621, Antispam-Engine: 2.0.1.0, Antispam-Data: 2004.11.22.52 X-Virus-Scanned: by amavisd-new Sender: owner-interop@eso.org Precedence: bulk Reply-To: "Robert Hanisch" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Sorry for being so late to this discussion, but the advantage is that this is a fresh look at the UCD1+ proposal. Well, that is my rationale, anyway! Minor issues: there are a number of grammatical errors and inconsistent usages (e.g., sometimes UCD is singular and sometimes plural; it would be clearer, I think, to write "UCDs" when the plural is intended). Has anyone expert in Backus-Naur Form checked Section 2.2? There is one mistake, I think, in that is defined with a capital A but the subsequent components refer to . UCDs are case-insensitive, but is BNF? On p.7, the paragraph beginning "The order in which words are arranged..." seems like circular reasoning to me. It says the order matters only if the order matters. I think the standard should be clear on this -- does the order matter or not? The text elsewhere suggests yes. I find Section 3.4 confusing...does anyone else? phot.color is a difference of two magnitudes, but does NOT have the associated word arith.diff. A temperature ratio is not a temperature, so phys.temperature;arith.ratio seems backwards to me. I can't use arith.ratio for M/L, so instead I see that this is defined as phys.mass.light. The UCD phys.mass;phys.luminosity;arith.ratio would seem to make more sense. If phot.color;em.opt.B;em.opt.V means B-V and phot.color;em.opt.V;em.opt.B means V-B, then order is clearly important. The concern this all raises for me is that the construction rules for new UCDs are not very clear, and that the existing UCD1+s have a certain (large) amount of arbitrariness. I think the list of UCD1+ words at http://cdsweb.u-strasbg.fr/UCD/ucd1p-words.txt HAS to be included in this document, or else we do not have a complete specification. I understand that the vocabulary is to be extensible. An acceptable alternative would be to put forward the full list of UCD1+s in a second document, but I think it is important that this document is under IVOA auspices and that revisions ultimately go through the same review process. This is somewhat at odds with Section 9, I realize. I suspect Section 9 is written the way it is to assure flexibility and timeliness in adding new UCDs. Hopefully our process is flexible and timely enough now, but if not, one could certainly entertain "provisional" UCDs, which are deemed reasonable by the UCD Steering Committee but remain subject to broader review. It is great that our colleagues at CDS have set up the interface for requesting new UCDs and is keeping the UCD lists up to date, but I think it is really best if these services/lists migrate to the IVOA site. In the UCD word list, why does "Q" indicate both primary and secondary usage? I think Section 6 should be moved to an Appendix -- it is usage advice, not something central to the UCD1+ definition. Cheers, Bob ----- Original Message ----- From: "Sebastien Derriere" To: Cc: Sent: Tuesday, November 23, 2004 10:23 AM Subject: RFC for UCD is ending > > Hello, > > The RFC period for the UCD document is ending, and there have > been no comments yet !! > If you have remarks or want changes, it is time to make them > public. > > Sebastien. > > Sebastien Derriere wrote: > > > > Dear all, > > > > The UCD reference document has been uploaded to the PR area of the > > IVOA document repository: > > > > http://www.ivoa.net/Documents/latest/UCD.html > > > > I would like to open the 4-weeks RFC period for this document as > > of today (Oct 27), with a close date on Nov 24, before promotion to > > the Recommendation status. > > > > A dedicated page has been created for posting comments: > > http://www.ivoa.net/twiki/bin/view/IVOA/UnifiedContentDescriptorRFC > > and discussions will be conducted on the UCD mailing list > > (ucd@ivoa.net). > > > > Sebastien. > > -- > _______ > / ~ /, Sebastien Derriere mailto:derriere@astro.u-strasbg.fr > / ~~~~ // Observatoire de Strasbourg Phone +33 (0) 390 242 444 > /______// 11, rue de l'universite Telefax +33 (0) 390 242 417 > (______(/ F-67000 Strasbourg France > From owner-ucd@eso.org Wed Nov 24 11:59:31 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iAOAx8R8017635 for ; Wed, 24 Nov 2004 11:59:08 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id iAOAx8qn017634 for ucd-outgoing; Wed, 24 Nov 2004 11:59:08 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iAOAwuR8017612; Wed, 24 Nov 2004 11:58:56 +0100 (MET) Received: from eso.org (st14.hq.eso.org [134.171.10.25]) by serapis.hq.eso.org (8.11.7+Sun/8.11.7) with ESMTP id iAOAwuD14363; Wed, 24 Nov 2004 11:58:56 +0100 (MET) Message-ID: <41A4696F.2070601@eso.org> Date: Wed, 24 Nov 2004 11:58:55 +0100 From: Alberto Micol Organization: ST-ECF User-Agent: Mozilla/5.0 (X11; U; SunOS sun4u; en-US; rv:1.4) Gecko/20040414 X-Accept-Language: en-us, en MIME-Version: 1.0 To: Robert Hanisch CC: Sebastien Derriere , interop@ivoa.net, ucd@ivoa.net Subject: Re: RFC for UCD is ending References: <417F94B0.3491FD4D@astro.u-strasbg.fr> <41A355EC.C9CE978B@astro.u-strasbg.fr> <009701c4d182$81aeb280$7deca782@stsci.edu> In-Reply-To: <009701c4d182$81aeb280$7deca782@stsci.edu> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Alberto Micol X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Dear Sebastein, Two things: (a) Backus Naur form and (b) versioning/conformity. a) Backus Naur I'd like to re-instantiate what I already proposed in Boston (sorry Sebastien to come back with this one): All UCDs should terminate with a semicolon. I'd like to see this implemented for one main reason: simplicity which can be explicit with the following two arguments: 1) a UCD should never be a substring of another UCD (how else to formulate this concept in a Backus Naur form?) 2) having a terminator helps when parsing or when building an SQL queries looking for a given UCD; without a terminator a more complex SQL is necessary or otherwise parsing of the result set is required. b) versioning/conformity Robert Hansich wrote: >I think the list of UCD1+ words at >http://cdsweb.u-strasbg.fr/UCD/ucd1p-words.txt HAS to be included in this >document, or else we do not have a complete specification. > I totally agree. Of course the UCD vocabulary must have its own versioning. In other words, the UCD vocabulary should specify its own version AND should specify which specs it conforms to (UCD1, UCD1+, UCD3, etc). I think the machanism for versioning and conformity SHALL be described in the document. Alberto From owner-interop@eso.org Wed Nov 24 12:03:10 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iAOB1DR8017935 for ; Wed, 24 Nov 2004 12:01:13 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id iAOB1DX8017934 for interop-outgoing; Wed, 24 Nov 2004 12:01:13 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-interop@eso.org using -f Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iAOB0wR8017889; Wed, 24 Nov 2004 12:00:58 +0100 (MET) Received: from eso.org (st14.hq.eso.org [134.171.10.25]) by serapis.hq.eso.org (8.11.7+Sun/8.11.7) with ESMTP id iAOB0vD14419; Wed, 24 Nov 2004 12:00:57 +0100 (MET) Message-ID: <41A469E9.9060906@eso.org> Date: Wed, 24 Nov 2004 12:00:57 +0100 From: Alberto Micol Organization: ST-ECF User-Agent: Mozilla/5.0 (X11; U; SunOS sun4u; en-US; rv:1.4) Gecko/20040414 X-Accept-Language: en-us, en MIME-Version: 1.0 To: Sebastien Derriere , interop@ivoa.net CC: Robert Hanisch , ucd@ivoa.net Subject: Confusing? References: <417F94B0.3491FD4D@astro.u-strasbg.fr> <41A355EC.C9CE978B@astro.u-strasbg.fr> <009701c4d182$81aeb280$7deca782@stsci.edu> In-Reply-To: <009701c4d182$81aeb280$7deca782@stsci.edu> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit X-Virus-Scanned: by amavisd-new Sender: owner-interop@eso.org Precedence: bulk Reply-To: Alberto Micol X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Robert Hanisch wrote: >On p.7, the paragraph beginning "The order in which words are arranged..." >seems like circular reasoning to me. It says the order matters only if the >order matters. I think the standard should be clear on this -- does the >order matter or not? The text elsewhere suggests yes. > >I find Section 3.4 confusing...does anyone else? phot.color is a difference >of two magnitudes, but does NOT have the associated word arith.diff. A >temperature ratio is not a temperature, so phys.temperature;arith.ratio >seems backwards to me. I can't use arith.ratio for M/L, so instead I see >that this is defined as phys.mass.light. The UCD >phys.mass;phys.luminosity;arith.ratio would seem to make more sense. If >phot.color;em.opt.B;em.opt.V means B-V and phot.color;em.opt.V;em.opt.B >means V-B, then order is clearly important. The concern this all raises for >me is that the construction rules for new UCDs are not very clear, and that >the existing UCD1+s have a certain (large) amount of arbitrariness. > > I found myself exactly in the same position as Bob. It IS confusing. Nevertheless... The fundamental requirement of the UCDs is (quote): the primary word carries most of the meaning as to "what the quantity is". Hence, Bob's suggestion for *phys.mass;phys.luminosity;arith.ratio* would make the UCDinterpreter think that the described quantity is a mass. It is not. The fact is that, despite being a ratio, it is a quantity that carries some physical meaning (for a galaxy it could give indications on the type of stars and the amount of dark matter), hence the existence of a ucd. The same is true for example for other quantities, for which nobody objects the availability of a proper UCD. One for all: velocity, it is a ratio between a distance and a time ... (After all, the dimensional analysis of a quantity will always reveal a ratio between mass length and time, some times even for adimensional quantities) Other more complex examples of the same problem are those UCDs which simply describe a different mathematical expression of the same thing, eg phot.mag and phot.flux. phot.mag it is the 2.5 log10 of a flux ratio One could say that the correct ucd is: *phot.flux;em.opt.V;arith.mag* expliciting the algorithm applied to the flux using a special arith.mag The question is: Why to complicate things? In fact, not to complicate things, * phot.color;em.opt.V;em.opt.B* complies to that fundamental requirement (it is a color) and expresses an implicit arith.diff. So, it is confusing, but it is difficult to keep it simple. What is the way out? Can the UCDs be built in a more more mathematical way, so to avoid confusion or would that complicate too much the problem? For the time being I'm afraid we have to live with such fuzzy definition. Let's hopw that UCD3 will address all this. Alberto From owner-ucd@eso.org Wed Nov 24 17:02:09 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iAOFxJR8002292 for ; Wed, 24 Nov 2004 16:59:19 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id iAOFxJMw002290 for ucd-outgoing; Wed, 24 Nov 2004 16:59:19 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iAOFxFR8002282 for ; Wed, 24 Nov 2004 16:59:15 +0100 (MET) Received: from mail.cacr.caltech.edu (mail.cacr.caltech.edu [131.215.145.9]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iAOFxDRQ018414 for ; Wed, 24 Nov 2004 16:59:14 +0100 (CET) Received: from Ropy (mercury.cacr.caltech.edu [131.215.145.175]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id iAOFx94J005264 (version=TLSv1/SSLv3 cipher=RC4-MD5 bits=128 verify=NO) for ; Wed, 24 Nov 2004 07:59:12 -0800 Message-ID: <007001c4d23e$8ae58740$6801a8c0@Ropy> From: "Roy Williams" To: References: <417F94B0.3491FD4D@astro.u-strasbg.fr> <41A355EC.C9CE978B@astro.u-strasbg.fr> <009701c4d182$81aeb280$7deca782@stsci.edu> <41A469E9.9060906@eso.org> Subject: Re: Confusing? Date: Wed, 24 Nov 2004 07:57:59 -0800 MIME-Version: 1.0 Content-Type: text/plain; format=flowed; charset="iso-8859-1"; reply-type=response Content-Transfer-Encoding: 7bit X-Priority: 3 X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook Express 6.00.2900.2180 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2180 X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.0.111621, Antispam-Engine: 2.0.1.0, Antispam-Data: 2004.11.23.51 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Roy Williams" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 >>On p.7, the paragraph beginning "The order in which words are arranged..." >>seems like circular reasoning to me. It says the order matters only if the >>order matters. I think the standard should be clear on this -- does the >>order matter or not? The text elsewhere suggests yes. My understanding is that the first word matters because it is the primary type. Each subsequent word modifies what goes before. Think of a ucd "A; B; C; D" as "((((A) B) C) D)". For example: stat.mean; phys.temperature; arith.diff; stat.max The maximum of the difference of two mean temperatures stat.mean; phys.temperature; stat.max; arith.diff The difference of the two maximum temperatures >>I find Section 3.4 confusing...does anyone else? phot.color is a difference >>of two magnitudes, but does NOT have the associated word arith.diff. In this case there is a special semantic concept for the difference of magnitudes, which is called color. It would be equally correct to say "arith.diff; phot.magnitude", but it is more efficient to use one word than two. >> A temperature ratio is not a temperature, so phys.temperature;arith.ratio seems >> backwards to me. I agree. This should be "arith.ratio: phys.temperature" >> If phot.color;em.opt.B;em.opt.V means B-V and phot.color;em.opt.V;em.opt.B >>means V-B, then order is clearly important. The concern this all raises for >>me is that the construction rules for new UCDs are not very clear, and that >>the existing UCD1+s have a certain (large) amount of arbitrariness. Yes that is true. But not because of the UCD construction, rather because of the word "color". Perhaps I can ask those mor knowledgeable than myself how exactly color is defined? If I say "BV color" or "VB color", do they have opposite sign? Or do I rather subtract the highest wavelength magnitude from the lowest wavelength? Roy From owner-ucd@eso.org Wed Nov 24 18:52:17 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iAOHq6R8020809 for ; Wed, 24 Nov 2004 18:52:06 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id iAOHq5D5020808 for ucd-outgoing; Wed, 24 Nov 2004 18:52:05 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iAOHptR8020787; Wed, 24 Nov 2004 18:51:56 +0100 (MET) Received: from eso.org (st14.hq.eso.org [134.171.10.25]) by serapis.hq.eso.org (8.11.7+Sun/8.11.7) with ESMTP id iAOHptD29556; Wed, 24 Nov 2004 18:51:55 +0100 (MET) Message-ID: <41A4CA3A.1050001@eso.org> Date: Wed, 24 Nov 2004 18:51:54 +0100 From: Alberto Micol Organization: ST-ECF User-Agent: Mozilla/5.0 (X11; U; SunOS sun4u; en-US; rv:1.4) Gecko/20040414 X-Accept-Language: en-us, en MIME-Version: 1.0 To: Roy Williams CC: ucd@ivoa.net Subject: Re: Confusing? References: <417F94B0.3491FD4D@astro.u-strasbg.fr> <41A355EC.C9CE978B@astro.u-strasbg.fr> <009701c4d182$81aeb280$7deca782@stsci.edu> <41A469E9.9060906@eso.org> <007001c4d23e$8ae58740$6801a8c0@Ropy> In-Reply-To: <007001c4d23e$8ae58740$6801a8c0@Ropy> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Alberto Micol X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Roy Williams wrote: >>> On p.7, the paragraph beginning "The order in which words are >>> arranged..." >>> seems like circular reasoning to me. It says the order matters only >>> if the >>> order matters. I think the standard should be clear on this -- does >>> the >>> order matter or not? The text elsewhere suggests yes. >> > > My understanding is that the first word matters because it is the > primary type. Each subsequent word modifies what goes before. Think of > a ucd "A; B; C; D" as "((((A) B) C) D)". For example: > > stat.mean; phys.temperature; arith.diff; stat.max > The maximum of the difference of two mean temperatures stat.mean is not allowed as primary word... You probably mean phys.temperature;stat.mean;arith.diff;stat.max > I agree. This should be "arith.ratio: phys.temperature" Nope, again arith.ratio is not allowed as primary word. Double confusing, isn't it? We need a coffee, or rather, at this time for us in Europe, a beer... Alberto From owner-ucd@eso.org Wed Nov 24 19:00:55 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iAOI0iR8021856 for ; Wed, 24 Nov 2004 19:00:44 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id iAOI0i5V021855 for ucd-outgoing; Wed, 24 Nov 2004 19:00:44 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iAOI0dR8021847 for ; Wed, 24 Nov 2004 19:00:39 +0100 (MET) Received: from saturn.rm.iasf.cnr.it (saturn.rm.iasf.cnr.it [150.146.136.11]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iAOI0bRQ024216 for ; Wed, 24 Nov 2004 19:00:38 +0100 (CET) Received: from (150.146.136.11) by e1000.artov.rm.cnr.it via smtp id 134c_c86ffec2_3e42_11d9_9836_0002b3da0f69; Wed, 24 Nov 2004 19:00:53 +0100 (CET) Received: from saturn.rm.iasf.cnr.it (saturn.rm.iasf.cnr.it [150.146.136.11]) by saturn.rm.iasf.cnr.it (8.11.3/8.11.3) with ESMTP id iAOIFq146168; Wed, 24 Nov 2004 19:15:52 +0100 Date: Wed, 24 Nov 2004 19:15:52 +0100 (NFT) From: Andrea Preite Martinez To: Roy Williams cc: Subject: Re: Confusing? In-Reply-To: <007001c4d23e$8ae58740$6801a8c0@Ropy> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.0.111621, Antispam-Engine: 2.0.1.0, Antispam-Data: 2004.11.23.51 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Andrea Preite Martinez X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Dear Roy, On Wed, 24 Nov 2004, Roy Williams wrote: > >>I find Section 3.4 confusing...does anyone else? phot.color is a difference > >>of two magnitudes, but does NOT have the associated word arith.diff. > > In this case there is a special semantic concept for the difference of magnit$ > is called color. It would be equally correct to say "arith.diff; phot.magnitu$ > is more efficient to use one word than two. Yes, this is exactly the reason for using phot.color > >> A temperature ratio is not a temperature, so phys.temperature;arith.ratio $ > >> backwards to me. > > I agree. This should be "arith.ratio: phys.temperature" arith.ratio also means "normalized", and a normalized temperature to me is closer to the concept of "temperature" than to an anodin "ratio". By the way, also "temperature in units of .... " is expressed by the two words "arith.ratio" and "phys.temperature". In this respect I dare say that absolute, non-relative values do not exist in our context (please, don't open a debate on this particular case!!) >> >> If phot.color;em.opt.B;em.opt.V means B-V and phot.color;em.opt.V;em.opt.B > >>means V-B, then order is clearly important. The concern this all raises for > >>me is that the construction rules for new UCDs are not very clear, and that > >>the existing UCD1+s have a certain (large) amount of arbitrariness. > > Yes that is true. But not because of the UCD construction, rather because of > "color". Perhaps I can ask those mor knowledgeable than myself how exactly color is > defined? If I say "BV color" or "VB color", do they have opposite sign? Or do$ > subtract the highest wavelength magnitude from the lowest wavelength? > B-V color means (Bmag - Vmag), so B-V = -(V-B) so there is no arbitrariness in the order of em-bands when colors are concerned. Any way, we are testing an "ucd1+ builder" that will help in building correct ucds from a list of words. Example: >From a description like: "Optical V magnitude" you can get from an assignation tool the words: em.opt, em.opt.V, phot.mag . The buider will propose: phot.mag;em.opt.V >From a description like: "Optical to infrared color" the builder will propose: phot.color;em.opt;em.IR To Bob: The reason for "Q" quantities is twofold: 1. Q is between P and S in the alphabet, as in ucd1+s 2. Q stands for "quantity", while P/S-words are usually not quantities Andrea ============================================================================== Andrea Preite Martinez andrea@rm.iasf.cnr.it Istituto di Astrofisica Spaziale Tel.:+39.06.4993.4641 Area di Ricerca di Tor Vergata Fax.:+39.06.2066.0188 Via del Fosso del Cavaliere 100 Cell: 339.3817355 00133 Roma CDS: +33.3.90242448 ============================================================================== From owner-ucd@eso.org Thu Nov 25 17:52:22 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iAPGpwUS012172 for ; Thu, 25 Nov 2004 17:51:58 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id iAPGpwVN012171 for ucd-outgoing; Thu, 25 Nov 2004 17:51:58 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iAPGpmUS012118 for ; Thu, 25 Nov 2004 17:51:48 +0100 (MET) Received: from athena.le.ac.uk (athena.le.ac.uk [143.210.16.127]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id iAPGpk2i001208 for ; Thu, 25 Nov 2004 17:51:47 +0100 (CET) Received: from [143.210.36.58] (helo=mail.star.le.ac.uk) by athena.le.ac.uk with smtp (Exim 4.43) id 1CXMqL-0005ve-Ak for ucd@ivoa.net; Thu, 25 Nov 2004 16:51:42 +0000 Received: (qmail 28866 invoked from network); 25 Nov 2004 16:51:28 -0000 Received: from morpheus.star.le.ac.uk (143.210.36.121) by mail.star.le.ac.uk with SMTP; 25 Nov 2004 16:51:28 -0000 Date: Thu, 25 Nov 2004 16:51:26 +0000 (GMT) From: "Patricio F. Ortiz" To: derriere@newb6.u-strasbg.fr cc: ucd@ivoa.net Subject: Comments on UCD draft Message-ID: MIME-Version: 1.0 Content-Type: MULTIPART/MIXED; BOUNDARY="-762349276-478456792-1101401486=:10798" X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.0.111621, Antispam-Engine: 2.0.1.0, Antispam-Data: 2004.11.24.47 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Patricio F. Ortiz" X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 This message is in MIME format. The first part should be readable text, while the remaining parts are likely unreadable without MIME-aware tools. Send mail to mime@docserver.cac.washington.edu for more info. ---762349276-478456792-1101401486=:10798 Content-Type: TEXT/PLAIN; charset=US-ASCII Dear Sebastien, here are my comments to the UCD document. I must say that I fully agree with Bob Hanish's comments. Alberto's and Andrea's points are also quite valid. The evolution of UCDs seems to me is going in the right direction, so my comments are more in the line of nitpicking in hope of improving the system (just as in the old days when we started with the UCDs and used them to do some quality control :-) I will concentrate my comments on the study of the two documents you provided: "ucd1-ucd1p.txt", "ucd1p-composed.txt", which are the closest to real data we have. I've always had in mind using UCDs to tell us what quantities of different origins could be compared when taken out of context in a relatively safe fashion. The original work on UCDs payed special attention to group quantities with equivalent units (not always a success or a trivial thing to do though). First, the obvious: phys.extension;stat.error seems to be mistaken, not sure about meta.code;stat.error on the same line, we're missing most of the error columns with their corresponding ucds. stat.stdev seems at first to be at the same level as stat.max, stat.min, stat.mean. The latter are always used as a qualifyer (a word after a semicolon), yet stat.stdev is used the other way, having said that, stat.stdev and stat.error are not too different though. stat.min, stat.max: are used in many observables, which is fine, but also in other quantities in which the meaning of minimum and maximum is not given by the sampled elements but by observational limits, eg, maximum and minimum of an observational window (bandpass) or limiting magnitude/flux src.fwhm and extensions Sooner or later we'll need to recognize quantities which relate to source extensions (or instrument coverage) in order to compute overlaps (eg, if a galaxy is located within the FOV of a plate). We require to know the geometry (or infer it) [rectangular, elliptic, polygonal). The quantities introduced in UCD1 for this purpose are lost in UCD1+. I believe this to be an oversimplification which we may regret later on. velocities src.veloc.compon UCD is a real mixture between any possible velocity component: cartesian, expressed in km/s (or equivalent) and polar (radial and tangential) Perhaps we shold think of adding some qualifiers for coordinates system, eg: coord.cart.X coord.cart.Y coord.cart.Z coord.polar.rad coord.polar.tang etc! The following could apply: VELOC_GAL_U -> src.veloc.compon ==> src.veloc.gc;coord.cart.X VELOC_TANG_GAL -> src.veloc.compon ==> src.veloc.gc;coord.polar.tang VELOC_RELAT -> src.veloc.component looks more like src.veloc;arith.diff (but in some cases it is :-) Gradients: I'd argue that gradients are physical properties rather than arithmetical, then phys.grad rather than arith.grad. Surface brightness. I'd argue that we should have phot.sb rather than phot.mag.sb UCDs and units: I think we're mixing things here: pos.eq.dec.arcsec pos.eq.ra.minutes pos.eq.ra.seconds If they represent dec and ra in different units, it's not up to the UCDs to resolve them. At best it looks confusing Wavelengths: em.wl em.wl.central em.wl.effective seems to me that "central" and "effective" are qualifiers, as the nature of the main quantity does not change. I think it would look better as em.wl;qual.central em.wl;qual.effective a similar situation happens with the effective temperature Photometry although I agree that having broad categories help locating a number of quantities, the lack of granularity means that we're no longer able to search for specific things. Say that I really want to locate magnitudes measured with PHOT_HST_F622W. In UCD1, only these quantities would be recovered. in UCD1+, I would have to ask for phot.mag;em.opt.R, and get 20 other quantities (involving an undetermined number of tables). Fishing for data in registries will be so fuzzy that will in practice render the system ineffective. In a google era, users would expect a low overhead rate; we are diverting from that trend. Despite going against the stream, I propose that we keep the granularity in photometric systems, define the proper qualifiers, and even allow individual frequencies/wavelenghts (as I've heard Pedro proposing). What we can do is to produce a way of linking a group of UCDs to a single one in order to simplify broad searches. So, if I look for phot.mag;em.opt.R, it should actually match to phot.mag;band.jhn.r phot.mag;band.gunn.r phot.mag;band.hst.f622w etc. OK, I'll stop here. Attached you'll find a summary of the matches from UCD1 <--> UCD1+ which I found quite useful and have used to present this analysis. I'm fully aware of how difficult it is to work with the raw data, and UCDs are an excellent way to use the registries to their full extent, hence my pickiness on some issues. The next thing we should be thinking is how to estimulate people to accept queries using only UCDs rather than column names, that propmts my concern about loosing granularity. Cheers, Patricio --- Patricio F. Ortiz pfo@star.le.ac.uk Department of Physics & Astronomy Phone: +44 (0)116 252 2015 University of Leicester Leicester, LE1 7RH, UK ---762349276-478456792-1101401486=:10798 Content-Type: APPLICATION/x-gzip; name="ucd1-1+summary.gz" Content-Transfer-Encoding: BASE64 Content-ID: Content-Description: Content-Disposition: attachment; filename="ucd1-1+summary.gz" H4sICCMMpkEAA3VjZDEtMStzdW1tYXJ5AKSdSXPbxraA186vyObVXbwCwkGU 5KTqVYEgSELCQGOgJL8Fi6IgiRUOCknFcX79PT2PICB7YRPd/fV0uvv06QFQ 6Y+6vzr/92sJv//7S/fz1a/f1qfXXzu/bpen1Wt1/MUrIBj+X/hpFNHHkRfP wmTCXOEsjQLqCJIgmzxQxzgLvpRB4nN3Th/CNKFPUZiwqHHK0o/LqAhnUcCy TnOfPn1xEvG0mGVh4oczj8XLCy+7pc9F5iU4Oz/ycvKQjnBWI6/w8O8DTiu4 L4IkpyXijsX4bhojn3EIhRwvYm/CXDMv82IQx9zLkFeY5AX7XXhEKvh56CUj 4Qi8mDt8LwqH3DUKRPxgPA79kIkMe+W3D4s8nMQe9ymCeMYd8yBKfe6688Ad JJNiirxiqHHEH6S2oe77AuRX0KrHaTabLrwsxsJKh+xHlBY5ZpFXBMyRh1/F cxQW9LnAeaTZMES9Jg6KXLhnQRamI+HO5uKZJTebpgX7XXT7Pn/2hrlDG4K4 i5g/D0nvwc9+KB7TKM0kV5kUTkarILxy2Skco1EqnsPxmDtUyWGvcVTeK45F 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(8.12.10+Sun/8.12.10) with ESMTP id j3197jPI021132 for ; Fri, 1 Apr 2005 11:07:45 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3197jNo021131 for ucd-outgoing; Fri, 1 Apr 2005 11:07:45 +0200 (MEST) Message-Id: <200504010907.j3197jNo021131@mercury.hq.eso.org> X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Date: Thu, 31 Mar 2005 16:43:11 +0200 From: Andrea Preite Martinez To: ucd@ivoa.net Subject: Kyoto Interop MIME-Version: 1.0 Content-Disposition: inline Content-Transfer-Encoding: 7bit User-Agent: Internet Messaging Program (IMP) H3 (4.0.1) Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Andrea Preite Martinez X-Virus-Scanned: by amavisd-new X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear members of the UCDs working group, In its last January meeting the IVOA-Exec board has appointed me as the new chair-person of this working group. The former chair-person (Roy) moved to chair the new VO-Event wg. Thank you Roy for your work, and your very effective way of moderating the bursts of discussion! - KYOTO Kyoto Interop meeting is approaching. In the preliminary schedule one UCD session is foreseen, Friday morning (20May2005). For the moment I only have the contributions from S.Derriere and myself. I invite you to propose to contribute to the session. - UCD1+ WORDS A new list of UCD1+ words will be made available soon (within next week) - TOOLS New UCD tools are available. They will be presented at the session in Kyoto, but will be made available for testing next week. See you soon Ciao Andrea ============================================================================== Andrea Preite Martinez andrea@rm.iasf.cnr.it Istituto di Astrofisica Spaziale Tel.:+39.06.4993.4641 Area di Ricerca di Tor Vergata Fax.:+39.06.2066.0188 Via del Fosso del Cavaliere 100 Cell:+39.339.3817355 00133 Roma ============================================================================== From owner-ucd@eso.org Fri Apr 22 19:50:54 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3MHobnm000647 for ; Fri, 22 Apr 2005 19:50:37 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3MHob5J000646 for ucd-outgoing; Fri, 22 Apr 2005 19:50:37 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3MHoUnm000633; Fri, 22 Apr 2005 19:50:31 +0200 (MEST) Received: from mail.cacr.caltech.edu (mail.cacr.caltech.edu [131.215.145.9]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3MHoS73011161; Fri, 22 Apr 2005 19:50:29 +0200 (CEST) Received: from [192.168.10.71] (windows-nat.cacr.caltech.edu [131.215.144.144]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id j3MHoMQm026023; Fri, 22 Apr 2005 10:50:25 -0700 Message-ID: <4269395A.9010802@cacr.caltech.edu> Date: Fri, 22 Apr 2005 10:50:18 -0700 From: Roy Williams User-Agent: Mozilla Thunderbird 1.0.2 (Macintosh/20050317) X-Accept-Language: en-us, en MIME-Version: 1.0 To: Andrea Preite Martinez , Sebastien Derriere CC: ucd@ivoa.net, voevent@ivoa.net Subject: New UCDs for VOEvent please Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.22.9 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Roy Williams X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear Andrea and Sebastien This note is to ask the UCD working group for help in building a new section of the UCD vocabulary in support of the VOEvent working group. The first meeting of the VOEvent WG was last week in Pasadena, with the objective of describing "immediate astronomical events" in a semantically-meaningful way. One of the parts of that schema is parameters that say what was observed, and another part is a "hypothesis" of what astrophysics may be behind the event. As an example, what was observed could be a "mag 17 source in galaxy X that was not there last week", and the hypothesis could be "supernova". We would like the "hypothesis" section to be based on a standard vocabulary, so that people can select and query based on these words. In other words, we would like a UCD section covering astronomical event types. Could you help us with doing this? Perhaps a meeting at the Kyoto IVOA would be appropriate? I cannot be there, but Arnold Rots and Alasdair Allen could speak for VOEvent. In the meeting last week, we came up with the words below as a start. It is in two parts -- the astrophysical objects, and the actual events that relate to the objects. Roy Williams California Institute of Technology 626 395 3670 ** Object types AGN, Binaries, Black Holes, Globular Clusters, Pulsars, Quasars, Neutron Stars, Supernova Remnants, Soft Gamma-ray Repeaters, Planets (minor), Comets, Meteors, ** Events (includes discovery of the above and...) Solar flares Cataclysmic Variables report Gamma-Ray Bursts, Supernovae, Microlensing Events, Novae, Outbursts Of Unusual Variable Stars, Cepheid period change change from what? Inspirals Xray burst LIGO burst neutrino planetary transit pulsar glitch References -- IVOA VOEvent Working Group http://www.ivoa.net/twiki/bin/view/IVOA/IvoaVOEvent Presentations are available at http://www.ivoa.net/twiki/bin/view/IVOA/VOEventSchedule -- IVOA Unified Content Descriptors http://www.ivoa.net/Documents/latest/UCD.html http://cdsweb.u-strasbg.fr/UCD/ucd1p-words.txt -- Two example VOEvents are here: http://www.ivoa.net/internal/IVOA/VoeventWorkshop/voevent_example.xml http://www.ivoa.net/internal/IVOA/VoeventWorkshop/voevent_example_smallest.xml (if this XML renders badly in your browser, choose "View/Source") From owner-voevent@eso.org Fri Apr 22 20:17:40 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3MIHOnm004516 for ; Fri, 22 Apr 2005 20:17:24 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3MIHOWN004515 for voevent-outgoing; Fri, 22 Apr 2005 20:17:24 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-voevent@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3MIH3nm004434; Fri, 22 Apr 2005 20:17:03 +0200 (MEST) Received: from darkstar.astro.washington.edu (darkstar.astro.washington.edu [128.95.99.45]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3MIH073012476; Fri, 22 Apr 2005 20:17:01 +0200 (CEST) Received: from darkstar.astro.washington.edu (becker@localhost [127.0.0.1]) by darkstar.astro.washington.edu (8.13.4/8.13.4/Debian-1) with ESMTP id j3MIGr8o024938 (version=TLSv1/SSLv3 cipher=DHE-RSA-AES256-SHA bits=256 verify=NOT); Fri, 22 Apr 2005 11:16:54 -0700 Received: (from becker@localhost) by darkstar.astro.washington.edu (8.13.4/8.13.4/Submit) id j3MIGr4Y024933; Fri, 22 Apr 2005 11:16:53 -0700 Date: Fri, 22 Apr 2005 11:16:53 -0700 From: Andrew Becker Message-Id: <200504221816.j3MIGr4Y024933@darkstar.astro.washington.edu> To: roy@cacr.caltech.edu CC: andrea@rm.iasf.cnr.it, derriere@newb6.u-strasbg.fr, ucd@ivoa.net, voevent@ivoa.net In-reply-to: <4269395A.9010802@cacr.caltech.edu> (message from Roy Williams on Fri, 22 Apr 2005 10:50:18 -0700) Subject: Re: New UCDs for VOEvent please References: <4269395A.9010802@cacr.caltech.edu> X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.22.10 X-Virus-Scanned: by amavisd-new Sender: owner-voevent@eso.org Precedence: bulk Reply-To: Andrew Becker X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi all - A quick read-through suggests a couple omissions in the "object types" - there are no basic "star" categories! E.g flare star, periodic variable star, AGB star, main sequence star, etc... /\ From owner-ucd@eso.org Fri Apr 22 21:27:05 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3MJQsnm014566 for ; Fri, 22 Apr 2005 21:26:54 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3MJQscQ014565 for ucd-outgoing; Fri, 22 Apr 2005 21:26:54 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3MJQinm014535; Fri, 22 Apr 2005 21:26:44 +0200 (MEST) Received: from apollo.le.ac.uk (apollo.le.ac.uk [143.210.16.125]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3MJQhXW015930; Fri, 22 Apr 2005 21:26:43 +0200 (CEST) Received: from [143.210.36.63] (helo=mail.star.le.ac.uk) by apollo.le.ac.uk with esmtp (Exim 4.44) id 1DP3nR-0005d7-Iw; Fri, 22 Apr 2005 20:26:37 +0100 Received: from barbara.star.le.ac.uk (barbara.star.le.ac.uk [143.210.36.88]) by mail.star.le.ac.uk (Postfix) with ESMTP id 5EF0D271A0A; Fri, 22 Apr 2005 20:26:37 +0100 (BST) Date: Fri, 22 Apr 2005 20:26:17 +0100 (BST) From: "Patricio F. Ortiz" To: Mark Taylor Cc: Tony Linde , IVOA VOTable , Subject: Re: datetime In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-UoL-Id: 7870beed100dc81907af5dc41b31e634@1DP3nR-0005d7-Iw@apollo.le.ac.uk X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.22.11 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Patricio F. Ortiz" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Glad to see this subject poping up, Francois Ochsenbein and I had a small exchange of ideas a few weeks back. Mark's explanation is quite good, but I would like to add a couple of things: a "datetime" (however it is represented) corresponds to an instant in time. Julian Date and Modified Julian Date (which do assume the usage of UTC) seem to be one of the most appropriate way of representing such instant in time. Using the ISO standard (string representation) is quite common, but any application wanting to compare instants in time needs to convert it to a floatinng number (double). Instants in time may mean a number of different things, which at this point we don't have any way to handle (more later). One of the problems I'm working on at the moment deal with comparing "simultaneity" or overlapping of time intervals. In this case, the application requires two instants in time: begining of event and end of event. One of the sample VOTables I'm using has five (yes 5) times listed, and as it is an observing log, they represent 1- begining of observation 2- end of observation 3- begining of event (a solar flare) 4- end of event 5- mid point of observation. UCDs don't have the structure to let us differentiate one "instant" from another, units don't help either, utype? Perhaps, but few people are using it yet, column explanation? We're lucky if there is one attached! At the end, the application I wrote let the user specify the columns for start_event & end_event... And those 5 examples are not the only ones, we could have - light curve peak time - time of discovery - time of minimum/maximun in a periodic light curve - time of transit - time of measurement etc. etc. etc. Seems to me that we need to: first agree in valid/meaningful ways of representing time, and spread the voice urbe et orbi, as we'll soon start wanting to know which events were observed with given instruments, in particular if the logs are available in the VO. second, start thinking how to identify the different things that an instant of time may mean, and to start, encourage people generating data to add meaningful explanations to the columns, so if the user is forced to make a decision by hand, at least it is an informed one. The sample VOTables I'm using right now don't have such explanations attached automagically yet I'm sure that information is available somewhere. Cheers, Patricio On Fri, 22 Apr 2005, Mark Taylor wrote: > On Fri, 22 Apr 2005, Tony Linde wrote: > > > Can I ask why datetime is not a datatype in VOTable? > > > > Cheers, > > Tony. > > Because there is no corresponding FITS BINTABLE TFORMn value; see: > > http://www.ivoa.net/Documents/REC/VOTable/VOTable-20040811.html#ToC11 > http://archive.stsci.edu/fits/fits_standard/node68.html#3124 > > VOTable takes its idea of what datatype a FIELD (or PARAM) can store > from the FITS binary table specification and not from XML Schema > (or anywhere else) and thus it's pretty low-level - there isn't even a > String type as such, you can only represent one as an array of characters. > The only type in VOTable but not FITS is unicodeChar, which is > presumably allowed because there is a clear 1:1 mapping between > UCS-2 Unicode characters and short integers. > > The datatype attribute is there to tell VOTable parsers how to > turn the content of a TD element or some bytes in a BINARY (and > possibly FITS) stream into a numeric/character value. Any semantic > interpretations put on those numbers/characters is up to the > application, perhaps by looking at other attributes such as > ucd/utype/units. The most obvious place to note that the > content of a particular column is intended to be understood as > a datetime-type value would probably be the units attribute, but > I don't think there is any standard way of doing this. > > It would certainly be useful for generic VOTable-consuming applications > if there was a standard way of telling that a string should be > interpreted to mean a date (or sky coordinate, ...) in a particular way, > but at the moment the VOTable standard does not operate at this level. > > Mark > > -- > Mark Taylor Starlink Programmer Physics, Bristol University, UK > m.b.taylor@bris.ac.uk +44-117-928-8776 http://www.star.bris.ac.uk/~mbt/ > > --- Patricio F. Ortiz pfo@star.le.ac.uk Department of Physics & Astronomy Phone: +44 (0)116 252 2015 University of Leicester Leicester, LE1 7RH, UK From owner-votable@eso.org Fri Apr 22 22:01:42 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3MK1Onm017149 for ; Fri, 22 Apr 2005 22:01:24 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3MK1OUD017142 for votable-outgoing; Fri, 22 Apr 2005 22:01:24 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-votable@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3MK1Cnm017111; Fri, 22 Apr 2005 22:01:12 +0200 (MEST) Received: from noao.edu (noao.edu [140.252.1.54]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3MK19XW016636; Fri, 22 Apr 2005 22:01:10 +0200 (CEST) X-Spam-Checker-Version: SpamAssassin 3.0.2 (2004-11-16) on noao.edu X-Spam-Level: X-Spam-Status: No, score=-5.8 required=4.5 tests=ALL_TRUSTED,AWL,BAYES_00 autolearn=ham version=3.0.2 X-TFF-CGPSA-Version: 1.4f1 X-TFF-CGPSA-Filter: Scanned Received: from [140.252.4.27] (account seaman HELO [140.252.4.27]) by noao.edu (CommuniGate Pro SMTP 4.2.10) with ESMTP-TLS id 17797453; Fri, 22 Apr 2005 13:00:56 -0700 In-Reply-To: References: Mime-Version: 1.0 (Apple Message framework v619.2) Content-Type: text/plain; charset=US-ASCII; format=flowed Message-Id: <37f3be7d4fa97c140bc4f8526774b646@noao.edu> Content-Transfer-Encoding: 7bit Cc: IVOA VOTable , Mark Taylor , Tony Linde , From: Rob Seaman Subject: Re: datetime Date: Fri, 22 Apr 2005 13:01:01 -0700 To: "Patricio F. Ortiz" X-Mailer: Apple Mail (2.619.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.22.11 X-Virus-Scanned: by amavisd-new Sender: owner-votable@eso.org Precedence: bulk Reply-To: Rob Seaman X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Patricio Ortiz says: > a "datetime" (however it is represented) corresponds to an instant in > time. Well, simultaneity is not just an issue for GR. A datetime, whatever time scale is used, only makes sense with respect to the location of the observation (or a derived location such as the barycenter). Some representation with a complexity similar to STC is required to unambiguously capture that instant in full. > Julian Date and Modified Julian Date (which do assume the usage of UTC) > seem to be one of the most appropriate way of representing such instant > in time. Using the ISO standard (string representation) is quite > common, > but any application wanting to compare instants in time needs to > convert > it to a floatinng number (double). If the precision required is larger than a second (a typical case for ground based observations), an integer (long) may be preferable. A simple epsilon test may be sufficient to test for equality. A more general case may be constructing a histogram representing the passage of a wavefront (or non-EM event) - in that case we may want to consider more obscure questions like whether the histogram intervals are half-open on the top or the bottom. Deciding the simultaneity of two events that are extended in time rather than instantaneous is a more interesting question than simply whether two intervals overlap. (Even ignoring the differing physics of signal generation and propagation that may apply to two different wavelength regimes.) Rob Seaman NOAO From owner-ucd@eso.org Fri Apr 22 23:03:46 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3ML3Ynm023353 for ; Fri, 22 Apr 2005 23:03:34 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3ML3Xjr023352 for ucd-outgoing; Fri, 22 Apr 2005 23:03:33 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3ML3Qnm023340; Fri, 22 Apr 2005 23:03:26 +0200 (MEST) Received: from apollo.le.ac.uk (mailsend.le.ac.uk [143.210.16.125]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3ML3O73018617; Fri, 22 Apr 2005 23:03:24 +0200 (CEST) Received: from [143.210.36.63] (helo=mail.star.le.ac.uk) by apollo.le.ac.uk with esmtp (Exim 4.44) id 1DP5J1-0007KR-A4; Fri, 22 Apr 2005 22:03:19 +0100 Received: from barbara.star.le.ac.uk (barbara.star.le.ac.uk [143.210.36.88]) by mail.star.le.ac.uk (Postfix) with ESMTP id F3315271A05; Fri, 22 Apr 2005 22:03:18 +0100 (BST) Date: Fri, 22 Apr 2005 22:03:00 +0100 (BST) From: "Patricio F. Ortiz" To: Rob Seaman Cc: IVOA VOTable , Subject: Re: datetime In-Reply-To: <37f3be7d4fa97c140bc4f8526774b646@noao.edu> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-UoL-Id: 8a94d7f9afb4872b315f86d61558906e@1DP5J1-0007KR-A4@apollo.le.ac.uk X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.22.11 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Patricio F. Ortiz" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi Bob, now we're getting into the insteresting stuff :-) On Fri, 22 Apr 2005, Rob Seaman wrote: > Patricio Ortiz says: > > > a "datetime" (however it is represented) corresponds to an instant in > > time. > > Well, simultaneity is not just an issue for GR. A datetime, whatever > time scale is used, only makes sense with respect to the location of > the observation (or a derived location such as the barycenter). Some > representation with a complexity similar to STC is required to > unambiguously capture that instant in full. Yes, I've seen several flavours of time scales. The picture I painted was the most simplistic of all! > > Julian Date and Modified Julian Date (which do assume the usage of UTC) > > seem to be one of the most appropriate way of representing such instant > > in time. Using the ISO standard (string representation) is quite > > common, > > but any application wanting to compare instants in time needs to > > convert > > it to a floatinng number (double). > > If the precision required is larger than a second (a typical case for > ground based observations), an integer (long) may be preferable. A > simple epsilon test may be sufficient to test for equality. In any case it is an 8-byte representation. People determining periods usfing fourier transform methods can obtain results with several significant digits of a second. For practical applications, I doubt that equality will be of much interest, but I may be totally wrong in this one. > A more > general case may be constructing a histogram representing the passage > of a wavefront (or non-EM event) - in that case we may want to consider > more obscure questions like whether the histogram intervals are > half-open on the top or the bottom. Deciding the simultaneity of two > events that are extended in time rather than instantaneous is a more > interesting question than simply whether two intervals overlap. (Even > ignoring the differing physics of signal generation and propagation > that may apply to two different wavelength regimes.) Indeed that's one of the most interesting aspects, eg, observed solar events (flares or whatever) with atmospheric phenomena (aurorae or other), or GRBs with their subsequent X-ray/optical/IR/radio afterglow. Even orbit determination of solar system objects may fall into that category, one is not interested in simultaneous events in space-time, but events which are somehow related. Few things are instantaneous anyways, observations (other than perhaps, in photon counting mode) extend over a period of time (fractions of a second to hours or days). Perhaps "instants" can only be defined at a post-processing stage (eg, Peak time of a SN light curve), but even in those cases, the presence of an error bar in the determination of such instants convert them into intervals for comparison purposes. Cheers, Patricio --- Patricio F. Ortiz pfo@star.le.ac.uk Department of Physics & Astronomy Phone: +44 (0)116 252 2015 University of Leicester Leicester, LE1 7RH, UK From owner-votable@eso.org Sat Apr 23 01:44:06 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3MNhlWi004199 for ; Sat, 23 Apr 2005 01:43:48 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3MNhlV7004198 for votable-outgoing; Sat, 23 Apr 2005 01:43:47 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-votable@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3MNhdWi004183; Sat, 23 Apr 2005 01:43:40 +0200 (MEST) Received: from head.cfa.harvard.edu (head.cfa.harvard.edu [131.142.41.8]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3MNhZ73021466; Sat, 23 Apr 2005 01:43:36 +0200 (CEST) Received: from xebec.cfa.harvard.edu (xebec [131.142.52.100]) by head.cfa.harvard.edu (d/w) with ESMTP id j3MNhKpU015992; Fri, 22 Apr 2005 19:43:20 -0400 (EDT) From: Arnold Rots Received: (from arots@localhost) by xebec.cfa.harvard.edu (8.12.8p1/8.12.8) id j3MNhJRf018702; Fri, 22 Apr 2005 19:43:19 -0400 (EDT) Message-Id: <200504222343.j3MNhJRf018702@xebec.cfa.harvard.edu> Subject: Re: datetime In-Reply-To: To: "Patricio F. Ortiz" Date: Fri, 22 Apr 2005 19:43:18 -0400 (EDT) CC: Mark Taylor , Tony Linde , IVOA VOTable , ucd@ivoa.net X-Mailer: ELM [version 2.4ME+ PL99 (25)] MIME-Version: 1.0 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.22.14 X-Virus-Scanned: by amavisd-new Sender: owner-votable@eso.org Precedence: bulk Reply-To: Arnold Rots X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Several people have already addressed most of the important points. Accurate time needs a specification of time scale and reference position. STC contains an astronTimeType that may be helpful. However, let me say emphatically that JD and MJD (and ISO-8601, for that matter), only define something akin to a format and imply nothing about the associated timescale. A JD or MJD without a timescale is meaningless; UTC cannot be assumed. - Arnold Patricio F. Ortiz wrote: > > Julian Date and Modified Julian Date (which do assume the usage of UTC) > seem to be one of the most appropriate way of representing such instant > in time. Using the ISO standard (string representation) is quite common, > but any application wanting to compare instants in time needs to convert > it to a floatinng number (double). > -------------------------------------------------------------------------- Arnold H. Rots Chandra X-ray Science Center Smithsonian Astrophysical Observatory tel: +1 617 496 7701 60 Garden Street, MS 67 fax: +1 617 495 7356 Cambridge, MA 02138 arots@head.cfa.harvard.edu USA http://hea-www.harvard.edu/~arots/ -------------------------------------------------------------------------- From owner-ucd@eso.org Sat Apr 23 02:03:31 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3N03KWi005166 for ; Sat, 23 Apr 2005 02:03:20 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3N03KJC005165 for ucd-outgoing; Sat, 23 Apr 2005 02:03:20 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3N03CWi005150; Sat, 23 Apr 2005 02:03:12 +0200 (MEST) Received: from galaxy.systems.pipex.net (galaxy.systems.pipex.net [62.241.162.31]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3N03A73021705; Sat, 23 Apr 2005 02:03:11 +0200 (CEST) Received: from dial.pipex.com (81-86-244-16.dsl.pipex.com [81.86.244.16]) by galaxy.systems.pipex.net (Postfix) with ESMTP id 57A94E0001DA; Sat, 23 Apr 2005 01:03:01 +0100 (BST) Message-ID: <4269904A.80704@dial.pipex.com> Date: Sat, 23 Apr 2005 01:01:14 +0100 From: Martin Hill User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.0; en-US; rv:1.6b) Gecko/20031205 Thunderbird/0.4 X-Accept-Language: en-us, en MIME-Version: 1.0 Cc: IVOA VOTable , ucd@ivoa.net Subject: Re: datetime References: <200504222343.j3MNhJRf018702@xebec.cfa.harvard.edu> In-Reply-To: <200504222343.j3MNhJRf018702@xebec.cfa.harvard.edu> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.22.16 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Martin Hill X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 It seems to me that for *most* practical purposes the ISO-8601 form with an assumed UTC is sufficient. As an ignorant layman I thought UTC did indeed have a reference point and a timescale... It may not be ideal, but it seems the ideal needs a bit more thrashing out. If it's not sufficient, can anyone explain (in ignorant laymans terms please!) why not? Or obviously just point us at something that does so. What we really want for now is a way of including datetimes in our standard message forms; it doesn't really matter if they're perfectly described yet as the people using them understand the context they're given in. Cheers Martin Arnold Rots wrote: > Several people have already addressed most of the important points. > Accurate time needs a specification of time scale and reference > position. STC contains an astronTimeType that may be helpful. > > However, let me say emphatically that JD and MJD (and ISO-8601, for > that matter), only define something akin to a format and imply nothing > about the associated timescale. A JD or MJD without a timescale is > meaningless; UTC cannot be assumed. > > - Arnold > > Patricio F. Ortiz wrote: > >>Julian Date and Modified Julian Date (which do assume the usage of UTC) >>seem to be one of the most appropriate way of representing such instant >>in time. Using the ISO standard (string representation) is quite common, >>but any application wanting to compare instants in time needs to convert >>it to a floatinng number (double). >> > > -------------------------------------------------------------------------- > Arnold H. Rots Chandra X-ray Science Center > Smithsonian Astrophysical Observatory tel: +1 617 496 7701 > 60 Garden Street, MS 67 fax: +1 617 495 7356 > Cambridge, MA 02138 arots@head.cfa.harvard.edu > USA http://hea-www.harvard.edu/~arots/ > -------------------------------------------------------------------------- > -- Martin Hill www.mchill.net 07901 55 24 66 0131 668 8100 (ROE) From owner-ucd@eso.org Sat Apr 23 02:58:27 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3N0wEWi007860 for ; Sat, 23 Apr 2005 02:58:14 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3N0wEei007859 for ucd-outgoing; Sat, 23 Apr 2005 02:58:14 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3N0w6Wi007850; Sat, 23 Apr 2005 02:58:06 +0200 (MEST) Received: from fed1rmmtao09.cox.net (fed1rmmtao09.cox.net [68.230.241.30]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3N0w373022413; Sat, 23 Apr 2005 02:58:04 +0200 (CEST) Received: from [10.0.1.64] (really [68.231.133.145]) by fed1rmmtao09.cox.net (InterMail vM.6.01.04.00 201-2131-118-20041027) with ESMTP id <20050423005753.NLLK7275.fed1rmmtao09.cox.net@[10.0.1.64]>; Fri, 22 Apr 2005 20:57:53 -0400 In-Reply-To: <4269904A.80704@dial.pipex.com> References: <200504222343.j3MNhJRf018702@xebec.cfa.harvard.edu> <4269904A.80704@dial.pipex.com> Mime-Version: 1.0 (Apple Message framework v619.2) Content-Type: text/plain; charset=US-ASCII; format=flowed Message-Id: <487e3908aee1907c801ecfa1ecb78c60@noao.edu> Content-Transfer-Encoding: 7bit Cc: ucd@ivoa.net, Rob Seaman , IVOA VOTable From: Rob Seaman Subject: Re: datetime Date: Fri, 22 Apr 2005 17:58:01 -0700 To: Martin Hill X-Mailer: Apple Mail (2.619.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.22.16 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Rob Seaman X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 On Apr 22, 2005, at 5:01 PM, Martin Hill wrote: > It seems to me that for *most* practical purposes the ISO-8601 form > with an assumed UTC is sufficient. As an ignorant layman I thought > UTC did indeed have a reference point and a timescale... It may not be > ideal, but it seems the ideal needs a bit more thrashing out. I agree with the skepticism shown by the quotes around "most". For *many* utility purposes, UTC has indeed been the default, with GMT before that. If there has ever been a default reference location, that has likely been topocentric, i.e., the location at which an observation was made. Thus, even in this rather ad hoc default case, some indication of a reference location would be required. For many purposes it might be sufficient to refer to an observatory DB such as maintained by the IRAF NOAO package. > If it's not sufficient, can anyone explain (in ignorant laymans terms > please!) why not? Or obviously just point us at something that does > so. UTC has been under attack for several years. The threat of discontinuing leap seconds - while continuing to refer to civil time as "UTC" - would make our prior usage of UTC as an approximation to GMT completely invalid. See Steve Allen's excellent UTC resource page at: http://www.ucolick.org/~sla/leapsecs Note that the future of UTC is largely out of our direct control. We may be able to convince the precision timing community to rename civil time something other than UTC, but the question of whether leap seconds will continue to be issued is under the control (it appears) of the International Telecommunications Union. In any event, it would be prudent for VO and astronomy in general to plan for the worst. > Solar events are based on times rather than spatial positions, and so > the queries and the result sets need to include these times. These > are generally UTC timestamps and the solar community know how to deal > with them in their context For some utility purposes even a bastardized UTC would be acceptable as a timestamp. UTC will remain monotonic, for instance. (There is good reason to believe there could never be a negative leap second.) One imagines, however, that solar astronomers will care more than most about the relationship of time to the angle of the Earth relative to the Sun. It is this angular information that would be jettisoned with leap seconds. Mean Solar Time would no longer bear any simple relationship to the clock on the wall. > As a first-step I would suggest UTC of the standard string form, with > a datatype of 'datetime' (and units as 'UTC' perhaps?); there are > already plenty of libraries to handle this format for > simple/primitive/low level operations such as sorting and matching. > This at least gives us a way of including dates in a VO-standard way > while we thrash out the deeper problems. This is similar to FITS DATE-OBS usage and may be acceptable for a range of utility purposes. The general solution (typically required for precise, scientifically useful, purposes) requires something similar in complexity to STC. Rob Seaman NOAO From owner-ucd@eso.org Sat Apr 23 04:15:37 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3N2FOWi012959 for ; Sat, 23 Apr 2005 04:15:24 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3N2FOpp012958 for ucd-outgoing; Sat, 23 Apr 2005 04:15:24 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3N2FKWi012954; Sat, 23 Apr 2005 04:15:20 +0200 (MEST) Received: from mail.cacr.caltech.edu (mail.cacr.caltech.edu [131.215.145.9]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3N2FHXW024091; Sat, 23 Apr 2005 04:15:18 +0200 (CEST) Received: from [192.168.1.101] (64-30-223-60.dsl.linkline.com [64.30.223.60]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id j3N2EkQm012097; Fri, 22 Apr 2005 19:15:15 -0700 Message-ID: <4269AF91.2090702@cacr.caltech.edu> Date: Fri, 22 Apr 2005 19:14:41 -0700 From: Roy Williams User-Agent: Mozilla Thunderbird 1.0.2 (Macintosh/20050317) X-Accept-Language: en-us, en MIME-Version: 1.0 To: ucd@ivoa.net, IVOA VOTable Subject: Re: datetime References: <200504222343.j3MNhJRf018702@xebec.cfa.harvard.edu> <4269904A.80704@dial.pipex.com> <487e3908aee1907c801ecfa1ecb78c60@noao.edu> In-Reply-To: <487e3908aee1907c801ecfa1ecb78c60@noao.edu> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.22.18 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Roy Williams X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 There are two things being discussed here: Scientific Time and what we can call Human Time or Office Time. The former has careful astronomical coordinates around it, and we are using STC. For the latter I would suggest ISO 8601, which is what the registry harvesting is using. From owner-ucd@eso.org Sat Apr 23 05:37:39 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3N3bQWi016260 for ; Sat, 23 Apr 2005 05:37:26 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3N3bPAE016259 for ucd-outgoing; Sat, 23 Apr 2005 05:37:25 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3N3bFWi016249; Sat, 23 Apr 2005 05:37:16 +0200 (MEST) Received: from fed1rmmtao07.cox.net (fed1rmmtao07.cox.net [68.230.241.32]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3N3bD73024769; Sat, 23 Apr 2005 05:37:14 +0200 (CEST) Received: from [10.0.1.67] (really [68.231.133.145]) by fed1rmmtao07.cox.net (InterMail vM.6.01.04.00 201-2131-118-20041027) with ESMTP id <20050423033652.RFCC1367.fed1rmmtao07.cox.net@[10.0.1.67]>; Fri, 22 Apr 2005 23:36:52 -0400 In-Reply-To: <4269AF91.2090702@cacr.caltech.edu> References: <200504222343.j3MNhJRf018702@xebec.cfa.harvard.edu> <4269904A.80704@dial.pipex.com> <487e3908aee1907c801ecfa1ecb78c60@noao.edu> <4269AF91.2090702@cacr.caltech.edu> Mime-Version: 1.0 (Apple Message framework v619.2) Content-Type: text/plain; charset=US-ASCII; format=flowed Message-Id: <7cb83e110c016f28d565d09d3cbde09a@noao.edu> Content-Transfer-Encoding: 7bit Cc: ucd@ivoa.net, Rob Seaman , IVOA VOTable From: Rob Seaman Subject: Re: datetime Date: Fri, 22 Apr 2005 20:36:59 -0700 To: Roy Williams X-Mailer: Apple Mail (2.619.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.22.19 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Rob Seaman X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 On Apr 22, 2005, at 7:14 PM, Roy Williams wrote: > There are two things being discussed here: Scientific Time and what we > can call Human Time or Office Time. The name "Civil Time" is proving to be pretty standard in the UTC "deliberations". > The former has careful astronomical coordinates around it, and we are > using STC. > For the latter I would suggest ISO 8601, which is what the registry > harvesting is using. I don't have ISO 8601 in front of me, but from the various discussions surrounding the Y2K remediation wars I suspect that its connection to UTC is only tenuous at best. There is the business of appending "Z" to indicate Zulu time, but Zulu is really a specification of GMT in "zone" (so called standard time) parlance. And, of course, an implicit assumption is that such a timestamp is valid at all locations. I suspect we could find examples for why this might not be the case in civil usage as well as scientific usage. That said, current astronomical usage, e.g., FITS, does rely on ISO 8601 (a subset, at least) to express UTC (loosely, at least) for utility purposes (both civil and scientific) with topocentric observatory locations (or locationless specifications of time). Even for purely utilitarian purposes, the astronomical community faces the prospect of having to distinguish between situations in which the Earth orientation nature of time is important versus situations in which the Civil (clock on the wall) nature of time is more important. We may not be able to rely on a single time scale continuing to express both. Rob Seaman NOAO From owner-ucd@eso.org Mon Apr 25 10:16:48 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3P8GWqT026298 for ; Mon, 25 Apr 2005 10:16:32 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3P8GWYL026297 for ucd-outgoing; Mon, 25 Apr 2005 10:16:32 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3P8GPqT026289; Mon, 25 Apr 2005 10:16:25 +0200 (MEST) Received: from alpha.uni-sw.gwdg.de (alpha.uni-sw.gwdg.de [134.76.205.222]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3P8GNXW027172; Mon, 25 Apr 2005 10:16:24 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1DPylO-0008U0-FP; Mon, 25 Apr 2005 10:16:18 +0200 In-Reply-To: <200504221816.j3MIGr4Y024933@darkstar.astro.washington.edu> References: <4269395A.9010802@cacr.caltech.edu> <200504221816.j3MIGr4Y024933@darkstar.astro.washington.edu> Mime-Version: 1.0 (Apple Message framework v622) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <46c44a5a3d9584a474a8ba7a0287abf4@Astro.physik.Uni-Goettingen.DE> Content-Transfer-Encoding: 7bit Cc: voevent@ivoa.net, roy@cacr.caltech.edu, ucd@ivoa.net, derriere@newb6.u-strasbg.fr, andrea@rm.iasf.cnr.it From: "Frederic V. \"Rick\" Hessman" Subject: Re: New UCDs for VOEvent please Date: Mon, 25 Apr 2005 10:18:24 +0200 To: Andrew Becker X-Mailer: Apple Mail (2.622) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.24.23 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Frederic V. \"Rick\" Hessman" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Before everyone stars to put too much work into a list, I suggest looking at the one I've started at our VOEvent Twiki site: http://monet.uni-sw.gwdg.de/twiki/bin/view/VOEvent/ UnifiedContentDescriptors It's based on the ApJ keywords (a likely place to start, it would seem to me). Everyone is heartily invited to register at http://monet.uni-sw.gwdg.de/twiki/bin/view/TWiki/TWikiRegistration and edit on the list communally. This also gives you write-access to the VOEvent and RTML schema pages. Rick P.S. The schema at http://monet.uni-sw.gwdg.de/twiki/bin/view/VOEvent/ SchemaTableOfContents isn't quite there yet, but very soon now..... On 22 Apr 2005, at 8:16 pm, Andrew Becker wrote: > Hi all - A quick read-through suggests a couple omissions in the > "object types" - there are no basic "star" categories! E.g flare > star, periodic variable star, AGB star, main sequence star, etc... > > /\ > > ------------------------------------------------------------------------ ------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Universitaets-Sternwarte Tel. +49-551-39-5052 Geismarlandstr. 11 Fax +49-551-39-5043 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman ------------------------------------------------------------------------ ------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.uni-goettingen.de ------------------------------------------------------------------------ ------------------------- From owner-voevent@eso.org Tue Apr 26 12:27:00 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3QAQeKn013602 for ; Tue, 26 Apr 2005 12:26:40 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3QAQeeR013601 for voevent-outgoing; Tue, 26 Apr 2005 12:26:40 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-voevent@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3QAQZKn013578; Tue, 26 Apr 2005 12:26:35 +0200 (MEST) Received: from alpha.uni-sw.gwdg.de (alpha.uni-sw.gwdg.de [134.76.205.222]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3QAQX73002396; Tue, 26 Apr 2005 12:26:34 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1DQNGr-000P9l-Nd; Tue, 26 Apr 2005 12:26:25 +0200 In-Reply-To: <4269395A.9010802@cacr.caltech.edu> References: <4269395A.9010802@cacr.caltech.edu> Mime-Version: 1.0 (Apple Message framework v622) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: Content-Transfer-Encoding: 7bit Cc: Sebastien Derriere , Allan Alasdair , Andrea Preite Martinez , ucd@ivoa.net, IVOA List VOEvent From: "Frederic V. \"Rick\" Hessman" Subject: Re: New UCDs for VOEvent please Date: Tue, 26 Apr 2005 12:28:32 +0200 To: Roy Williams X-Mailer: Apple Mail (2.622) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.26.0 X-Virus-Scanned: by amavisd-new Sender: owner-voevent@eso.org Precedence: bulk Reply-To: "Frederic V. \"Rick\" Hessman" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Gentlemen (and Ladies?), I've added more VOEvent examples, several suggestions for IVOA/UCD to the proposed object/event/process UCD list at http://monet.uni-sw.gwdg.de/twiki/bin/view/VOEvent/ UnifiedContentDescriptors (which I've tentatively called "VOThings" for the lack of any better name - "VOObjects" sounds a bit too software-ish and something like "VOZoology" sounds too trite) and have achieved a fairly complete equivalence to the ApJ/A&A/MN keyword list, including things like most types of variable stars. If something like this list has already been created, I'd appreciate hearing about it before I put much more work into our own. May I suggest that the issue of an additional UCD be placed prominently in the Kyoto discussion, since it tangents the work of many different groups (e.g. VOTable, VOEvent, Virtual Repository, Data Modelling). I'd love to go to Kyoto, but it's a long way away...... Rick ------------------------------------------------------------------------ ------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Universitaets-Sternwarte Tel. +49-551-39-5052 Geismarlandstr. 11 Fax +49-551-39-5043 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman ------------------------------------------------------------------------ ------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.uni-goettingen.de ------------------------------------------------------------------------ ------------------------- From owner-ucd@eso.org Tue Apr 26 16:20:47 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3QEKSKn028299 for ; Tue, 26 Apr 2005 16:20:29 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3QEKSnZ028298 for ucd-outgoing; Tue, 26 Apr 2005 16:20:28 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3QEKKKn028273; Tue, 26 Apr 2005 16:20:20 +0200 (MEST) Received: from fed1rmmtao08.cox.net (fed1rmmtao08.cox.net [68.230.241.31]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3QEKHXW017818; Tue, 26 Apr 2005 16:20:18 +0200 (CEST) Received: from [10.0.1.95] (really [68.231.133.145]) by fed1rmmtao08.cox.net (InterMail vM.6.01.04.00 201-2131-118-20041027) with ESMTP id <20050426141950.HDMJ16890.fed1rmmtao08.cox.net@[10.0.1.95]>; Tue, 26 Apr 2005 10:19:50 -0400 In-Reply-To: References: <4269395A.9010802@cacr.caltech.edu> Mime-Version: 1.0 (Apple Message framework v619.2) Content-Type: multipart/alternative; boundary=Apple-Mail-3-926535793 Message-Id: <816d402df50341a5d44aee3e499f23e8@noao.edu> Cc: Sebastien Derriere , Allan Alasdair , Andrea Preite Martinez , Rob Seaman , ucd@ivoa.net, Roy Williams , IVOA List VOEvent From: Rob Seaman Subject: Re: New UCDs for VOEvent please Date: Tue, 26 Apr 2005 07:20:05 -0700 To: "Frederic V. \"Rick\" Hessman" X-Mailer: Apple Mail (2.619.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.26.0 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Rob Seaman X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 --Apple-Mail-3-926535793 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed On Apr 26, 2005, at 3:28 AM, Rick Hessman wrote: > I've added more VOEvent examples, several suggestions for IVOA/UCD to > the proposed > object/event/process UCD list at > > http://monet.uni-sw.gwdg.de/twiki/bin/view/VOEvent/ > UnifiedContentDescriptors Good start at a list. A search facility would add immensely to its usefulness as the list grows. This would also function as a validator for an astronomer's guess as to the proper syntax for a familiar class of objects. > If something like this list has already been created, I'd appreciate > hearing about > it before I put much more work into our own. This would be a good opportunity for VO to reach out to the larger community. It really isn't for us to mandate nomenclature. An interactive dictionary/beastiary of astronomical objects and processes could be useful all by itself, and will be of obvious utility for various VO projects. A common understanding of each "hypothesis" will indeed be key to VOEvent, for instance. I'm not sure, however, that the ApJ keywords are the best model for constructing this content descriptor list. Keywords are a way to partition the level of interest a member of the community may have in reading a paper. A UCD is a way of partitioning the underlying physics. For instance, given that the interest in working on this is arising out of VOEvent, it isn't surprising that there is a focus on processes more than objects, and that the selection of objects would be weighted toward time variability in various ways. There are dozens of fine shadings between variable stars. On the other hand, while one can distinguish between elliptical, irregular and spiral galaxies, there isn't any mechanism (yet) for specifying the precise type of each. I'm leery of encouraging these descriptors to become longer than they are, but it seems inappropriate to specify generally descriptive classes, like: stars.variable.irregular stars.variable.long_period stars.variable.semi-regular at the same level as members of prototypical classes, like: stars.variable.Cepheid stars.variable.RR_Lyr stars.variable.RS_CVn (And where is stars.variable.W_UMa? Just pointing out that the list will never be complete.) Perhaps it should be stars.variable.class.Cepheid? Or better yet, adjust in the other direction, maybe stars.variable.period.irregular? Or ideally, a general mechanism might be provided for parametrically classifying periodicity. The challenge here is not only that the list will never be complete, it is that we should be encouraging researchers to actively augment and improve the list. A workable classification scheme is often the first step in organizing a research program. But the result of a research program is often to overturn the original classification scheme. We don't want to provide a mechanism that is only useful for describing objects far removed from the cutting edge. Rob Seaman NOAO --Apple-Mail-3-926535793 Content-Transfer-Encoding: 7bit Content-Type: text/enriched; charset=US-ASCII Lucida SansOn Apr 26, 2005, at 3:28 AM, Rick Hessman wrote: I've added more VOEvent examples, several suggestions for IVOA/UCD to the proposed object/event/process UCD list at http://monet.uni-sw.gwdg.de/twiki/bin/view/VOEvent/UnifiedContentDescriptors Good start at a list. A search facility would add immensely to its usefulness as the list grows. This would also function as a validator for an astronomer's guess as to the proper syntax for a familiar class of objects. If something like this list has already been created, I'd appreciate hearing about it before I put much more work into our own. This would be a good opportunity for VO to reach out to the larger community. It really isn't for us to mandate nomenclature. An interactive dictionary/beastiary of astronomical objects and processes could be useful all by itself, and will be of obvious utility for various VO projects. A common understanding of each "hypothesis" will indeed be key to VOEvent, for instance. I'm not sure, however, that the ApJ keywords are the best model for constructing this content descriptor list. Keywords are a way to partition the level of interest a member of the community may have in reading a paper. A UCD is a way of partitioning the underlying physics. For instance, given that the interest in working on this is arising out of VOEvent, it isn't surprising that there is a focus on processes more than objects, and that the selection of objects would be weighted toward time variability in various ways. There are dozens of fine shadings between variable stars. On the other hand, while one can distinguish between elliptical, irregular and spiral galaxies, there isn't any mechanism (yet) for specifying the precise type of each. I'm leery of encouraging these descriptors to become longer than they are, but it seems inappropriate to specify generally descriptive classes, like: stars.variable.irregular stars.variable.long_period stars.variable.semi-regular at the same level as members of prototypical classes, like: stars.variable.Cepheid stars.variable.RR_Lyr stars.variable.RS_CVn (And where is stars.variable.W_UMa? Just pointing out that the list will never be complete.) Perhaps it should be stars.variable.class.Cepheid? Or better yet, adjust in the other direction, maybe stars.variable.period.irregular? Or ideally, a general mechanism might be provided for parametrically classifying periodicity. The challenge here is not only that the list will never be complete, it is that we should be encouraging researchers to actively augment and improve the list. A workable classification scheme is often the first step in organizing a research program. But the result of a research program is often to overturn the original classification scheme. We don't want to provide a mechanism that is only useful for describing objects far removed from the cutting edge. Rob Seaman NOAO --Apple-Mail-3-926535793-- From owner-voevent@eso.org Tue Apr 26 16:43:51 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3QEhZKn003916 for ; Tue, 26 Apr 2005 16:43:35 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3QEhZRH003915 for voevent-outgoing; Tue, 26 Apr 2005 16:43:35 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-voevent@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3QEhTKn003899; Tue, 26 Apr 2005 16:43:29 +0200 (MEST) Received: from alpha.uni-sw.gwdg.de (alpha.uni-sw.gwdg.de [134.76.205.222]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3QEhRXW018761; Tue, 26 Apr 2005 16:43:27 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1DQRHV-000S0n-6s; Tue, 26 Apr 2005 16:43:21 +0200 In-Reply-To: <816d402df50341a5d44aee3e499f23e8@noao.edu> References: <4269395A.9010802@cacr.caltech.edu> <816d402df50341a5d44aee3e499f23e8@noao.edu> Mime-Version: 1.0 (Apple Message framework v622) Content-Type: multipart/alternative; boundary=Apple-Mail-1-928057872 Message-Id: <83f2d949bed1694f983c1b81f65c67e2@Astro.physik.Uni-Goettingen.DE> Cc: Sebastien Derriere , Allan Alasdair , Andrea Preite Martinez , ucd@ivoa.net, Roy Williams , IVOA List VOEvent From: "Frederic V. \"Rick\" Hessman" Subject: Re: New UCDs for VOEvent please Date: Tue, 26 Apr 2005 16:45:27 +0200 To: Rob Seaman X-Mailer: Apple Mail (2.622) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.26.0 X-Virus-Scanned: by amavisd-new Sender: owner-voevent@eso.org Precedence: bulk Reply-To: "Frederic V. \"Rick\" Hessman" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 --Apple-Mail-1-928057872 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed On 26 Apr 2005, at 4:20 pm, Rob Seaman wrote: > On Apr 26, 2005, at 3:28 AM, Rick Hessman wrote: > >> I've added more VOEvent examples, several suggestions for IVOA/UCD to >> the proposed >> object/event/process UCD list at >> >> http://monet.uni-sw.gwdg.de/twiki/bin/view/VOEvent/ >> UnifiedContentDescriptors > > Good start at a list. A search facility would add immensely to its > usefulness as the list grows. This would also function as a validator > for an astronomer's guess as to the proper syntax for a familiar class > of objects. > >> If something like this list has already been created, I'd appreciate >> hearing about >> it before I put much more work into our own. > > This would be a good opportunity for VO to reach out to the larger > community. It really isn't for us to mandate nomenclature. An > interactive dictionary/beastiary of astronomical objects and processes > could be useful all by itself, and will be of obvious utility for > various VO projects. A common understanding of each "hypothesis" will > indeed be key to VOEvent, for instance. On the other hand, one can't have TOO many people laying on their hands, since there is a need for some level of editorial control. We'd be happy to provide our Twiki more-or-less as it is, since it's already interactive and available to anyone interested. > I'm not sure, however, that the ApJ keywords are the best model for > constructing this content descriptor list. Keywords are a way to > partition the level of interest a member of the community may have in > reading a paper. A UCD is a way of partitioning the underlying > physics. For instance, given that the interest in working on this is > arising out of VOEvent, it isn't surprising that there is a focus on > processes more than objects, and that the selection of objects would > be weighted toward time variability in various ways. There are dozens > of fine shadings between variable stars. On the other hand, while one > can distinguish between elliptical, irregular and spiral galaxies, > there isn't any mechanism (yet) for specifying the precise type of > each. Actually, the ApJ/A&A/MN keywords should really be a GREAT place to start, since they are supposed to capture what is eventually done with the content. It's clear that they don't provide a uniform and uniformly deep level of description, but at least they provide a good and evenly distributed place to start. > I'm leery of encouraging these descriptors to become longer than they > are, but it seems inappropriate to specify generally descriptive > classes, like: > > stars.variable.irregular > stars.variable.long_period > stars.variable.semi-regular > > at the same level as members of prototypical classes, like: > > stars.variable.Cepheid > stars.variable.RR_Lyr > stars.variable.RS_CVn > > (And where is stars.variable.W_UMa? Just pointing out that the list > will never be complete.) > Perhaps it should be stars.variable.class.Cepheid? Or better yet, > adjust in the other direction, maybe stars.variable.period.irregular? > Or ideally, a general mechanism might be provided for parametrically > classifying periodicity. No no no no : these are individual stars but names commonly used to typify a certain variable star behavior (just as we say "Cepheids" and really mean "delta Cepheids" = "stars like delta Cep"). There really are "W UMa" stars. Of course, the UCD can't be defined for individual objects other than a very few like the Sun, Moon, and major planets. Thus, "stars.variable.W_UMa" means the same as "stars.variable.class.W_UMa"; I suppose we could add on the "*.class*" just as a reminder, but at the cost of an additional hierarchical level of detail. > The challenge here is not only that the list will never be complete, > it is that we should be encouraging researchers to actively augment > and improve the list. A workable classification scheme is often the > first step in organizing a research program. But the result of a > research program is often to overturn the original classification > scheme. We don't want to provide a mechanism that is only useful for > describing objects far removed from the cutting edge. Fortunately, astronomers - even very good ones - are often rather traditional in their use of nomenclature, so we'll need such metadata whether someone thinks it's quaint or not. As a stellar astrophysicist interested in variability and accretion, I've included things I'd like to have and will leave it to others to include their own metatdata. Rick ------------------------------------------------------------------------ ------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Universitaets-Sternwarte Tel. +49-551-39-5052 Geismarlandstr. 11 Fax +49-551-39-5043 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman ------------------------------------------------------------------------ ------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.uni-goettingen.de ------------------------------------------------------------------------ ------------------------- --Apple-Mail-1-928057872 Content-Transfer-Encoding: 7bit Content-Type: text/enriched; charset=US-ASCII On 26 Apr 2005, at 4:20 pm, Rob Seaman wrote: Lucida SansOn Apr 26, 2005, at 3:28 AM, Rick Hessman wrote: I've added more VOEvent examples, several suggestions for IVOA/UCD to the proposed object/event/process UCD list at http://monet.uni-sw.gwdg.de/twiki/bin/view/VOEvent/UnifiedContentDescriptors Good start at a list. A search facility would add immensely to its usefulness as the list grows. This would also function as a validator for an astronomer's guess as to the proper syntax for a familiar class of objects. If something like this list has already been created, I'd appreciate hearing about it before I put much more work into our own. This would be a good opportunity for VO to reach out to the larger community. It really isn't for us to mandate nomenclature. An interactive dictionary/beastiary of astronomical objects and processes could be useful all by itself, and will be of obvious utility for various VO projects. A common understanding of each "hypothesis" will indeed be key to VOEvent, for instance. On the other hand, one can't have TOO many people laying on their hands, since there is a need for some level of editorial control. We'd be happy to provide our Twiki more-or-less as it is, since it's already interactive and available to anyone interested. Lucida SansI'm not sure, however, that the ApJ keywords are the best model for constructing this content descriptor list. Keywords are a way to partition the level of interest a member of the community may have in reading a paper. A UCD is a way of partitioning the underlying physics. For instance, given that the interest in working on this is arising out of VOEvent, it isn't surprising that there is a focus on processes more than objects, and that the selection of objects would be weighted toward time variability in various ways. There are dozens of fine shadings between variable stars. On the other hand, while one can distinguish between elliptical, irregular and spiral galaxies, there isn't any mechanism (yet) for specifying the precise type of each. Actually, the ApJ/A&A/MN keywords should really be a GREAT place to start, since they are supposed to capture what is eventually done with the content. It's clear that they don't provide a uniform and uniformly deep level of description, but at least they provide a good and evenly distributed place to start. Lucida SansI'm leery of encouraging these descriptors to become longer than they are, but it seems inappropriate to specify generally descriptive classes, like: stars.variable.irregular stars.variable.long_period stars.variable.semi-regular at the same level as members of prototypical classes, like: stars.variable.Cepheid stars.variable.RR_Lyr stars.variable.RS_CVn (And where is stars.variable.W_UMa? Just pointing out that the list will never be complete.) Perhaps it should be stars.variable.class.Cepheid? Or better yet, adjust in the other direction, maybe stars.variable.period.irregular? Or ideally, a general mechanism might be provided for parametrically classifying periodicity. No no no no : these are individual stars but names commonly used to typify a certain variable star behavior (just as we say "Cepheids" and really mean "delta Cepheids" = "stars like delta Cep"). There really are "W UMa" stars. Of course, the UCD can't be defined for individual objects other than a very few like the Sun, Moon, and major planets. Thus, "stars.variable.W_UMa" means the same as "stars.variable.class.W_UMa"; I suppose we could add on the "*.class*" just as a reminder, but at the cost of an additional hierarchical level of detail. Lucida SansThe challenge here is not only that the list will never be complete, it is that we should be encouraging researchers to actively augment and improve the list. A workable classification scheme is often the first step in organizing a research program. But the result of a research program is often to overturn the original classification scheme. We don't want to provide a mechanism that is only useful for describing objects far removed from the cutting edge. Fortunately, astronomers - even very good ones - are often rather traditional in their use of nomenclature, so we'll need such metadata whether someone thinks it's quaint or not. As a stellar astrophysicist interested in variability and accretion, I've included things I'd like to have and will leave it to others to include their own metatdata. Rick Lucida Sans ------------------------------------------------------------------------------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Universitaets-Sternwarte Tel. +49-551-39-5052 Geismarlandstr. 11 Fax +49-551-39-5043 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman ------------------------------------------------------------------------------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.uni-goettingen.de ------------------------------------------------------------------------------------------------- --Apple-Mail-1-928057872-- From owner-ucd@eso.org Tue Apr 26 16:56:02 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3QEtkKn006613 for ; Tue, 26 Apr 2005 16:55:46 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3QEtkqN006611 for ucd-outgoing; Tue, 26 Apr 2005 16:55:46 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3QEtaKn006582; Tue, 26 Apr 2005 16:55:36 +0200 (MEST) Received: from alpha.uni-sw.gwdg.de (alpha.uni-sw.gwdg.de [134.76.205.222]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3QEtZXW019268; Tue, 26 Apr 2005 16:55:35 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1DQRTE-000SEo-TI; Tue, 26 Apr 2005 16:55:28 +0200 In-Reply-To: <816d402df50341a5d44aee3e499f23e8@noao.edu> References: <4269395A.9010802@cacr.caltech.edu> <816d402df50341a5d44aee3e499f23e8@noao.edu> Mime-Version: 1.0 (Apple Message framework v622) Content-Type: multipart/alternative; boundary=Apple-Mail-2-928785644 Message-Id: Cc: Sebastien Derriere , Allan Alasdair , Andrea Preite Martinez , ucd@ivoa.net, Roy Williams , IVOA List VOEvent From: "Frederic V. \"Rick\" Hessman" Subject: Re: New UCDs for VOEvent please Date: Tue, 26 Apr 2005 16:57:35 +0200 To: Rob Seaman X-Mailer: Apple Mail (2.622) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.26.2 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Frederic V. \"Rick\" Hessman" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 --Apple-Mail-2-928785644 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Another thought.... On 26 Apr 2005, at 4:20 pm, Rob Seaman wrote: > The challenge here is not only that the list will never be complete, > it is that we should be encouraging researchers to actively augment > and improve the list. A workable classification scheme is often the > first step in organizing a research program. But the result of a > research program is often to overturn the original classification > scheme. We don't want to provide a mechanism that is only useful for > describing objects far removed from the cutting edge. The "cutting edge" will always be such that one won't have a useful classification scheme other than unusual combinations of the more general bits and pieces. That's why the UCD has to be hierarchical (to emphasize/extract general properties even when given specifics) and easily combined. Let's see..... cosmology.dark_energy <== cosmology.background;em.microwave cosmology.background.polarization;em.microwave stars.supernova.Type_Ia;process.eruption.hydrodynamic; process.eruption.thermonuclear galaxies.velocity_curve cosmology.abund .... (Aha - already discovered a few important UCD's to add....!) Rick ------------------------------------------------------------------------ ------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Universitaets-Sternwarte Tel. +49-551-39-5052 Geismarlandstr. 11 Fax +49-551-39-5043 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman ------------------------------------------------------------------------ ------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.uni-goettingen.de ------------------------------------------------------------------------ ------------------------- --Apple-Mail-2-928785644 Content-Transfer-Encoding: 7bit Content-Type: text/enriched; charset=US-ASCII Another thought.... On 26 Apr 2005, at 4:20 pm, Rob Seaman wrote: Lucida SansThe challenge here is not only that the list will never be complete, it is that we should be encouraging researchers to actively augment and improve the list. A workable classification scheme is often the first step in organizing a research program. But the result of a research program is often to overturn the original classification scheme. We don't want to provide a mechanism that is only useful for describing objects far removed from the cutting edge. The "cutting edge" will always be such that one won't have a useful classification scheme other than unusual combinations of the more general bits and pieces. That's why the UCD has to be hierarchical (to emphasize/extract general properties even when given specifics) and easily combined. Let's see..... cosmology.dark_energy <<== cosmology.background;em.microwave cosmology.background.polarization;em.microwave stars.supernova.Type_Ia;process.eruption.hydrodynamic;process.eruption.thermonuclear galaxies.velocity_curve cosmology.abund .... (Aha - already discovered a few important UCD's to add....!) Rick ------------------------------------------------------------------------------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Universitaets-Sternwarte Tel. +49-551-39-5052 Geismarlandstr. 11 Fax +49-551-39-5043 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman ------------------------------------------------------------------------------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.uni-goettingen.de ------------------------------------------------------------------------------------------------- --Apple-Mail-2-928785644-- From owner-ucd@eso.org Tue Apr 26 20:21:06 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3QIKoKn013101 for ; Tue, 26 Apr 2005 20:20:51 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3QIKomq013098 for ucd-outgoing; Tue, 26 Apr 2005 20:20:50 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3QIKiKn012983; Tue, 26 Apr 2005 20:20:46 +0200 (MEST) Received: from noao.edu (noao.edu [140.252.1.54]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3QIKeXW026614; Tue, 26 Apr 2005 20:20:41 +0200 (CEST) X-Spam-Checker-Version: SpamAssassin 3.0.2 (2004-11-16) on noao.edu X-Spam-Level: X-Spam-Status: No, score=-5.8 required=4.5 tests=ALL_TRUSTED,AWL,BAYES_00 autolearn=ham version=3.0.2 X-TFF-CGPSA-Version: 1.4f1 X-TFF-CGPSA-Filter: Scanned Received: from [140.252.10.225] (account seaman HELO [140.252.10.225]) by noao.edu (CommuniGate Pro SMTP 4.3c5) with ESMTPSA id 17885855; Tue, 26 Apr 2005 11:02:47 -0700 In-Reply-To: References: <4269395A.9010802@cacr.caltech.edu> <816d402df50341a5d44aee3e499f23e8@noao.edu> Mime-Version: 1.0 (Apple Message framework v619.2) Content-Type: multipart/alternative; boundary=Apple-Mail-7-939911923 Message-Id: Cc: IVOA List VOEvent , Rob Seaman , ucd@ivoa.net From: Rob Seaman Subject: Re: New UCDs for VOEvent please Date: Tue, 26 Apr 2005 11:03:01 -0700 To: "Frederic V. \"Rick\" Hessman" X-Mailer: Apple Mail (2.619.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.26.5 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Rob Seaman X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 --Apple-Mail-7-939911923 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed I said: >> The challenge here is not only that the list will never be complete, >> it is that we should be encouraging researchers to actively augment >> and improve the list. A workable classification scheme is often the >> first step in organizing a research program. But the result of a >> research program is often to overturn the original classification >> scheme. We don't want to provide a mechanism that is only useful for >> describing objects far removed from the cutting edge. Rick Hessman says: > The "cutting edge" will always be such that one won't have a useful > classification scheme other than unusual combinations of the more > general bits and pieces. That's why the UCD has to be hierarchical > (to emphasize/extract general properties even when given specifics) > and easily combined. Let's see..... > > cosmology.dark_energy <== cosmology.background;em.microwave > cosmology.background.polarization;em.microwave > stars.supernova.Type_Ia;process.eruption.hydrodynamic; > process.eruption.thermonuclear > galaxies.velocity_curve > cosmology.abund > .... > > (Aha - already discovered a few important UCD's to add....!) I'm becoming more skeptical that IVOA standard UCDs are appropriate for representing the often slippery nature of astronomical "processes" and "objects". (As I pointed out at in a similar context at the VOEvent workshop - one might choose to regard an object simply as a long lived process. A main sequence star is a ~10 Gy thermonuclear reaction.) But a UCD is targeted differently (from UCD-1.9.9b): "The Unified Content Descriptor (UCD) is a formal vocabulary for astronomical metadata that is controlled by the International Virtual Observatory Alliance (IVOA)." The question is whether the characterization of astronomical objects/processes represents "metadata". The whole point of the precision of a UCD specification (e.g., phot.flux;em.optical;meas.error;stat.max) is to provide a solid foundation for building a sound scientific argument - but such an argument typically results in drawing new insights and building new logical connections - often using new vocabulary. On the other hand, even the most well established nomenclature regarding astronomical objects and processes is subject to revision and extension as better data and more profound theory collide. Namespaces provide a possible way to address this. For instance, IVOA is developing a very basic namespace and various astronomical constituencies then support richer, and perhaps shorter latency, vocabularies of their own. However, we have this bit of constraining boilerplate to muddy the waters: "4.1.2 Namespaces. The use of namespaces, indicated by the presence of a colon in the word is possible, but should be avoided as far as possible. The namespace is defined by the string before the colon and the word follows. The words in the non-standard namespace must be distinct from all words currently in the IVOA namespace. While developers may need local namespace, they should be used only temporarily, for words that are not yet included into the UCD validated by the IVOA. New words should be added using the procedures discussed in section XX." What is the justification for trying to require that words in a non-standard namespace be distinct? For instance, we couldn't possibly require that two different non-standard namespaces not overlap. Why regard the IVOA namespace as *necessarily* preeminent? "Standard" does not equate with "compulsory". Either the standard makes sense or you won't be able to force folks to use it anyway. In any event, one would think that alternate interpretations of the same vocabulary would be one of the strongest justifications for alternate namespaces. This isn't an opportunity to lose control of alternate vocabulary - it's the way to enforce control of alternate usages. I also find the word "temporarily" to be curiously undefined for a science in which observations and inferences from decades and even centuries gone by may be revisited. To the list of UCD commandments: 1. UCDs should be short. 2. They should suggest the concept being labeled. 3. Only a single UCD should be appropriate for a given concept. 4. UCDs should be complete, describing all concepts of interest. 5. The vocabulary used within UCDs should be as small as possible. 6. Related concepts should have related UCDs. 7. Quantities with the same UCD should be comparable. I might suggest adding: 8. For IVOA to control its vocabulary, it must provide the opportunity for others to control their own. Ralph Waldo Emerson may shed some light: "The poets made all the words, and therefore language is the archives of history, and, if we must say it, a sort of tomb of the muses For, though the origin of most of our words is forgotten, each word was at a stroke of genius, and obtained currency, because for the moment it symbolizes the world to the first speaker and to the hearer. The etymologist finds the deadest word to have been once a brilliant picture. Language is fossil poetry." However much effort is expended to constrain and mandate standard usage, the users will seek ways to subvert the dominant paradigm. This isn't just the nature of users, it is the nature of science as poetry. Careful support for alternate usage is the key to controlling anarchy. Rob Seaman NOAO --Apple-Mail-7-939911923 Content-Transfer-Encoding: 7bit Content-Type: text/enriched; charset=US-ASCII Lucida SansI said: The challenge here is not only that the list will never be complete, it is that we should be encouraging researchers to actively augment and improve the list. A workable classification scheme is often the first step in organizing a research program. But the result of a research program is often to overturn the original classification scheme. We don't want to provide a mechanism that is only useful for describing objects far removed from the cutting edge. Rick Hessman says: The "cutting edge" will always be such that one won't have a useful classification scheme other than unusual combinations of the more general bits and pieces. That's why the UCD has to be hierarchical (to emphasize/extract general properties even when given specifics) and easily combined. Let's see..... cosmology.dark_energy <<== cosmology.background;em.microwave cosmology.background.polarization;em.microwave stars.supernova.Type_Ia;process.eruption.hydrodynamic;process.eruption.thermonuclear galaxies.velocity_curve cosmology.abund .... (Aha - already discovered a few important UCD's to add....!) I'm becoming more skeptical that IVOA standard UCDs are appropriate for representing the often slippery nature of astronomical "processes" and "objects". (As I pointed out at in a similar context at the VOEvent workshop - one might choose to regard an object simply as a long lived process. A main sequence star is a ~10 Gy thermonuclear reaction.) But a UCD is targeted differently (from UCD-1.9.9b): "The Unified Content Descriptor (UCD) is a formal vocabulary for astronomical metadata that is controlled by the International Virtual Observatory Alliance (IVOA)." The question is whether the characterization of astronomical objects/processes represents "metadata". The whole point of the precision of a UCD specification (e.g., phot.flux;em.optical;meas.error;stat.max) is to provide a solid foundation for building a sound scientific argument - but such an argument typically results in drawing new insights and building new logical connections - often using new vocabulary. On the other hand, even the most well established nomenclature regarding astronomical objects and processes is subject to revision and extension as better data and more profound theory collide. Namespaces provide a possible way to address this. For instance, IVOA is developing a very basic namespace and various astronomical constituencies then support richer, and perhaps shorter latency, vocabularies of their own. However, we have this bit of constraining boilerplate to muddy the waters: "4.1.2 Namespaces. The use of namespaces, indicated by the presence of a colon in the word is possible, but should be avoided as far as possible. The namespace is defined by the string before the colon and the word follows. The words in the non-standard namespace must be distinct from all words currently in the IVOA namespace. While developers may need local namespace, they should be used only temporarily, for words that are not yet included into the UCD validated by the IVOA. New words should be added using the procedures discussed in section XX." What is the justification for trying to require that words in a non-standard namespace be distinct? For instance, we couldn't possibly require that two different non-standard namespaces not overlap. Why regard the IVOA namespace as *necessarily* preeminent? "Standard" does not equate with "compulsory". Either the standard makes sense or you won't be able to force folks to use it anyway. In any event, one would think that alternate interpretations of the same vocabulary would be one of the strongest justifications for alternate namespaces. This isn't an opportunity to lose control of alternate vocabulary - it's the way to enforce control of alternate usages. I also find the word "temporarily" to be curiously undefined for a science in which observations and inferences from decades and even centuries gone by may be revisited. To the list of UCD commandments: 1. UCDs should be short. 2. They should suggest the concept being labeled. 3. Only a single UCD should be appropriate for a given concept. 4. UCDs should be complete, describing all concepts of interest. 5. The vocabulary used within UCDs should be as small as possible. 6. Related concepts should have related UCDs. 7. Quantities with the same UCD should be comparable. I might suggest adding: 8. For IVOA to control its vocabulary, it must provide the opportunity for others to control their own. Ralph Waldo Emerson may shed some light: "The poets made all the words, and therefore language is the archives of history, and, if we must say it, a sort of tomb of the muses For, though the origin of most of our words is forgotten, each word was at a stroke of genius, and obtained currency, because for the moment it symbolizes the world to the first speaker and to the hearer. The etymologist finds the deadest word to have been once a brilliant picture. Language is fossil poetry." However much effort is expended to constrain and mandate standard usage, the users will seek ways to subvert the dominant paradigm. This isn't just the nature of users, it is the nature of science as poetry. Careful support for alternate usage is the key to controlling anarchy. Rob Seaman NOAO --Apple-Mail-7-939911923-- From owner-ucd@eso.org Wed Apr 27 12:13:54 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RADcl1000684 for ; Wed, 27 Apr 2005 12:13:39 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3RADcnB000683 for ucd-outgoing; Wed, 27 Apr 2005 12:13:38 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RADSl1000654; Wed, 27 Apr 2005 12:13:28 +0200 (MEST) Received: from alpha.uni-sw.gwdg.de (alpha.uni-sw.gwdg.de [134.76.205.222]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RADQ73010091; Wed, 27 Apr 2005 12:13:26 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1DQjXl-000cgw-8z; Wed, 27 Apr 2005 12:13:21 +0200 In-Reply-To: References: <4269395A.9010802@cacr.caltech.edu> <816d402df50341a5d44aee3e499f23e8@noao.edu> Mime-Version: 1.0 (Apple Message framework v622) Content-Type: multipart/alternative; boundary=Apple-Mail-1-998258357 Message-Id: <0b948e6b641050d8843597c4d28fc850@Astro.physik.Uni-Goettingen.DE> Cc: IVOA List VOEvent , ucd@ivoa.net From: "Frederic V. \"Rick\" Hessman" Subject: Re: New UCDs for VOEvent please Date: Wed, 27 Apr 2005 12:15:28 +0200 To: Rob Seaman X-Mailer: Apple Mail (2.622) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.27.1 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Frederic V. \"Rick\" Hessman" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 --Apple-Mail-1-998258357 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed > I'm becoming more skeptical that IVOA standard UCDs are appropriate > for representing the often slippery nature of astronomical "processes" > and "objects". The question is whether the characterization of > astronomical objects/processes represents "metadata". The whole point > of the precision of a UCD specification (e.g., > phot.flux;em.optical;meas.error;stat.max) is to provide a solid > foundation for building a sound scientific argument - but such an > argument typically results in drawing new insights and building new > logical connections - often using new vocabulary. On the other hand, > even the most well established nomenclature regarding astronomical > objects and processes is subject to revision and extension as better > data and more profound theory collide. Ah, but the point of UCDs is not to let computers write papers but to be able to let computers organize and re-organize information using terms which we can easily formulate/manipulate. At a pretty trivial level, it can be something as simple as saying what the point of an observation is/was (the reason why a target classification is needed in RTML) or to describe what is roughly happening so that a computer can respond to it (the reason it's needed in VOEvent), but a broader use within the VO is obvious. While we're all spoiled by the services provided by Simbad, resolving astronomical names and querying catalogues won't permit us to combine information to the fullest unless we can express what it is we have and what we want in a fashion which goes far beyond the present IVOA/UCD (crafted really only for VOTable). Thus, RTML and VOEvent would certainly get by using their own little classification lists, but the adoption of a more generally used UCD for astronomical objects and processes is bound to become necessary. The earlier we start discussing it, the faster we will be able to profit from it. Fortunately, a supernova will always remain a supernova and a spiral galaxy won't loose it's spirals within our lifetime, so the evolution of UCD's will be in the direction of the addition of new terms - as they become needed - and the passive abandonment of old UCD's which no longer serve any but a purely historical purpose - well, we should let historians of science keep their access to old terms (they may actually want to know what a W UMa star was/is ;-) > 3. Only a single UCD should be appropriate for a given concept. > 4. UCDs should be complete, describing all concepts of interest. Rots of ruck! A UCD which attempts (!) to describe what it is we do will never be complete and unambiguous. The point is not that it can be perfect but that it exists at all. > However much effort is expended to constrain and mandate standard > usage, the users will seek ways to subvert the dominant paradigm. > This isn't just the nature of users, it is the nature of science as > poetry. Careful support for alternate usage is the key to controlling > anarchy. Frankly, I imagine that most users won't even see it. We're doing this to help stupid computers become more useful and not to constrain the science of our colleagues. Rick ------------------------------------------------------------------------ ------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Universitaets-Sternwarte Tel. +49-551-39-5052 Geismarlandstr. 11 Fax +49-551-39-5043 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman ------------------------------------------------------------------------ ------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.uni-goettingen.de ------------------------------------------------------------------------ ------------------------- --Apple-Mail-1-998258357 Content-Transfer-Encoding: 7bit Content-Type: text/enriched; charset=US-ASCII Lucida SansI'm becoming more skeptical that IVOA standard UCDs are appropriate for representing the often slippery nature of astronomical "processes" and "objects". The question is whether the characterization of astronomical objects/processes represents "metadata". The whole point of the precision of a UCD specification (e.g., phot.flux;em.optical;meas.error;stat.max) is to provide a solid foundation for building a sound scientific argument - but such an argument typically results in drawing new insights and building new logical connections - often using new vocabulary. On the other hand, even the most well established nomenclature regarding astronomical objects and processes is subject to revision and extension as better data and more profound theory collide. Ah, but the point of UCDs is not to let computers write papers but to be able to let computers organize and re-organize information using terms which we can easily formulate/manipulate. At a pretty trivial level, it can be something as simple as saying what the point of an observation is/was (the reason why a target classification is needed in RTML) or to describe what is roughly happening so that a computer can respond to it (the reason it's needed in VOEvent), but a broader use within the VO is obvious. While we're all spoiled by the services provided by Simbad, resolving astronomical names and querying catalogues won't permit us to combine information to the fullest unless we can express what it is we have and what we want in a fashion which goes far beyond the present IVOA/UCD (crafted really only for VOTable). Thus, RTML and VOEvent would certainly get by using their own little classification lists, but the adoption of a more generally used UCD for astronomical objects and processes is bound to become necessary. The earlier we start discussing it, the faster we will be able to profit from it. Fortunately, a supernova will always remain a supernova and a spiral galaxy won't loose it's spirals within our lifetime, so the evolution of UCD's will be in the direction of the addition of new terms - as they become needed - and the passive abandonment of old UCD's which no longer serve any but a purely historical purpose - well, we should let historians of science keep their access to old terms (they may actually want to know what a W UMa star was/is ;-) Lucida Sans 3. Only a single UCD should be appropriate for a given concept. 4. UCDs should be complete, describing all concepts of interest.Lucida Sans Rots of ruck! A UCD which attempts (!) to describe what it is we do will never be complete and unambiguous. The point is not that it can be perfect but that it exists at all. Lucida SansHowever much effort is expended to constrain and mandate standard usage, the users will seek ways to subvert the dominant paradigm. This isn't just the nature of users, it is the nature of science as poetry. Careful support for alternate usage is the key to controlling anarchy. Lucida Sans Frankly, I imagine that most users won't even see it. We're doing this to help stupid computers become more useful and not to constrain the science of our colleagues. Rick ------------------------------------------------------------------------------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Universitaets-Sternwarte Tel. +49-551-39-5052 Geismarlandstr. 11 Fax +49-551-39-5043 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman ------------------------------------------------------------------------------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.uni-goettingen.de ------------------------------------------------------------------------------------------------- --Apple-Mail-1-998258357-- From owner-voevent@eso.org Wed Apr 27 12:44:32 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RAiGl1006663 for ; Wed, 27 Apr 2005 12:44:16 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3RAiGid006662 for voevent-outgoing; Wed, 27 Apr 2005 12:44:16 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-voevent@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RAiBl1006646; Wed, 27 Apr 2005 12:44:12 +0200 (MEST) Received: from apollo.le.ac.uk (mailsend.le.ac.uk [143.210.16.125]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RAi873010777; Wed, 27 Apr 2005 12:44:08 +0200 (CEST) Received: from [143.210.36.63] (helo=mail.star.le.ac.uk) by apollo.le.ac.uk with esmtp (Exim 4.44) id 1DQk1S-0007GJ-So; Wed, 27 Apr 2005 11:44:02 +0100 Received: from barbara.star.le.ac.uk (barbara.star.le.ac.uk [143.210.36.88]) by mail.star.le.ac.uk (Postfix) with ESMTP id B2717271A04; Wed, 27 Apr 2005 11:44:02 +0100 (BST) Date: Wed, 27 Apr 2005 11:43:04 +0100 (BST) From: "Patricio F. Ortiz" To: "Frederic V. \"Rick\" Hessman" Cc: Rob Seaman , IVOA List VOEvent , Subject: Re: New UCDs for VOEvent please In-Reply-To: <0b948e6b641050d8843597c4d28fc850@Astro.physik.Uni-Goettingen.DE> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-UoL-Id: d2459c807f892f2d747440999d060aba@1DQk1S-0007GJ-So@apollo.le.ac.uk X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.27.1 X-Virus-Scanned: by amavisd-new Sender: owner-voevent@eso.org Precedence: bulk Reply-To: "Patricio F. Ortiz" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi, I didn't want to jump into this discussion, but what the heck :-) OK, I'm concerned about the usage of this new proposal. UCDs were born to identify quantities listed in tables (essentially a way to let automated software recognize the nature of the columns in such table). We left out any attempt to include object types, after all, a magnitude is something which applies to a planet, star, galaxy, QSO, whatever, and so with many things like spectral features. It is obvious that in the context of the VO, we would like to have some way to attach a label to the kind of object we are talking about. And the proposed schemes sound doable, not easy, not 100% reliable, but workable. My questions to anyone interested are: "how do you envision using these new UODs (Unified Object-type Descriptor)?" By that, I mean, in which part of the metadata would you like to insert theses descriptors? Catalogues like USNO, 2mass, etc, contain a mixture of objects, and even homogeneous catalogues (like galaxies catalogues) will contain several flavours of galaxies, hence my concern. An object type may not be unique... How do we handle those cases? (after all, these are flags/labels to make our life easier. If the core of a galaxy is an AGN, what does the descriptor look like? UCDs of physical quantities are much easier to handle in that sense! (as noted below regarding the unicity of a UCD). How deep do we want to describe an object? Say that the same AGN has exhibited variations in HBeta flux (ok, kick for the incorrectness :-) :-) Do we want to describe such variability? For some people/applications it will be important, for others not. Although Frederic says that a SN will always be a SN, sure, but what about before? If Eta Car went SN next month, how would we label it? Furthermore, objects may not change in human-lifetime scales, but our perception can... I recall in the mid 80's that the core of the Tarantula Nebula (R136??) was thought to be a super-massive star, only to be discovered later, using instrument with higher angular resolution that it was a compact star cluster... I'm nearly sure there are other examples floating around. For the historians, as Frederic says, should we think of attaching a time stamp to any UOD/object pair? After all, if tomorrow we have to change it, should we erase the previous knowledge? Just my 2 pences :-) Patricio On Wed, 27 Apr 2005, Frederic V. "Rick" Hessman wrote: > > I'm becoming more skeptical that IVOA standard UCDs are appropriate > > for representing the often slippery nature of astronomical "processes" > > and "objects". The question is whether the characterization of > > astronomical objects/processes represents "metadata". The whole point > > of the precision of a UCD specification (e.g., > > phot.flux;em.optical;meas.error;stat.max) is to provide a solid > > foundation for building a sound scientific argument - but such an > > argument typically results in drawing new insights and building new > > logical connections - often using new vocabulary. On the other hand, > > even the most well established nomenclature regarding astronomical > > objects and processes is subject to revision and extension as better > > data and more profound theory collide. > > Ah, but the point of UCDs is not to let computers write papers but to > be able to let computers organize and re-organize information using > terms which we can easily formulate/manipulate. At a pretty trivial > level, it can be something as simple as saying what the point of an > observation is/was (the reason why a target classification is needed in > RTML) or to describe what is roughly happening so that a computer can > respond to it (the reason it's needed in VOEvent), but a broader use > within the VO is obvious. While we're all spoiled by the services > provided by Simbad, resolving astronomical names and querying > catalogues won't permit us to combine information to the fullest unless > we can express what it is we have and what we want in a fashion which > goes far beyond the present IVOA/UCD (crafted really only for VOTable). > > Thus, RTML and VOEvent would certainly get by using their own little > classification lists, but the adoption of a more generally used UCD for > astronomical objects and processes is bound to become necessary. The > earlier we start discussing it, the faster we will be able to profit > from it. > > Fortunately, a supernova will always remain a supernova and a spiral > galaxy won't loose it's spirals within our lifetime, so the evolution > of UCD's will be in the direction of the addition of new terms - as > they become needed - and the passive abandonment of old UCD's which no > longer serve any but a purely historical purpose - well, we should let > historians of science keep their access to old terms (they may actually > want to know what a W UMa star was/is ;-) > > > 3. Only a single UCD should be appropriate for a given concept. > > 4. UCDs should be complete, describing all concepts of interest. > > Rots of ruck! A UCD which attempts (!) to describe what it is we do > will never be complete and unambiguous. The point is not that it can > be perfect but that it exists at all. > > > However much effort is expended to constrain and mandate standard > > usage, the users will seek ways to subvert the dominant paradigm. > > This isn't just the nature of users, it is the nature of science as > > poetry. Careful support for alternate usage is the key to controlling > > anarchy. > > Frankly, I imagine that most users won't even see it. We're doing > this to help stupid computers become more useful and not to constrain > the science of our colleagues. > > Rick --- Patricio F. Ortiz pfo@star.le.ac.uk Department of Physics & Astronomy Phone: +44 (0)116 252 2015 University of Leicester Leicester, LE1 7RH, UK From owner-ucd@eso.org Wed Apr 27 12:50:26 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RAoFl1007364 for ; Wed, 27 Apr 2005 12:50:15 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3RAoFCK007363 for ucd-outgoing; Wed, 27 Apr 2005 12:50:15 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RAo6l1007339; Wed, 27 Apr 2005 12:50:07 +0200 (MEST) Received: from hermesnew.ex.ac.uk (dot.ex.ac.uk [144.173.6.11]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RAo573010920; Wed, 27 Apr 2005 12:50:05 +0200 (CEST) Received: from klunk.astro.ex.ac.uk ([144.173.229.19]) by hermesnew.ex.ac.uk with esmtp (Exim 4.50/mail) id 1DQk7E-0001Q5-0Q; Wed, 27 Apr 2005 11:50:00 +0100 In-Reply-To: <0b948e6b641050d8843597c4d28fc850@Astro.physik.Uni-Goettingen.DE> References: <4269395A.9010802@cacr.caltech.edu> <816d402df50341a5d44aee3e499f23e8@noao.edu> <0b948e6b641050d8843597c4d28fc850@Astro.physik.Uni-Goettingen.DE> Mime-Version: 1.0 (Apple Message framework v618) Content-Type: text/plain; charset=US-ASCII; format=flowed Message-Id: <2087F54E-B70A-11D9-BE5F-000D93C0E1F0@astro.ex.ac.uk> Content-Transfer-Encoding: 7bit Cc: ucd@ivoa.net From: Alasdair Allan Subject: Re: New UCDs for VOEvent please Date: Wed, 27 Apr 2005 11:50:10 +0100 To: IVOA List VOEvent X-Mailer: Apple Mail (2.618) X-Exeter-Interface: mail X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.27.2 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Alasdair Allan X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Rick Hessman wrote: > Rob Seaman wrote; >> However much effort is expended to constrain and mandate standard >> usage, the users will seek ways to subvert the dominant paradigm. >> This isn't just the nature of users, it is the nature of science as >> poetry. Careful support for alternate usage is the key to >> controlling anarchy. > > Frankly, I imagine that most users won't even see it. We're doing > this to help stupid computers become more useful and not to constrain > the science of our colleagues. Exactly, this isn't for user consumption, this is so that bits of software can route messages correctly. VOEvent messages are never meant to be consumed, or even seen, by a human user. Al. From owner-ucd@eso.org Wed Apr 27 13:33:20 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RBWvl1015194 for ; Wed, 27 Apr 2005 13:32:58 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3RBWvZm015193 for ucd-outgoing; Wed, 27 Apr 2005 13:32:57 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RBWrl1015187; Wed, 27 Apr 2005 13:32:53 +0200 (MEST) Received: from alpha.uni-sw.gwdg.de (alpha.uni-sw.gwdg.de [134.76.205.222]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RBWq73012029; Wed, 27 Apr 2005 13:32:52 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1DQkmc-000dgR-Sp; Wed, 27 Apr 2005 13:32:46 +0200 In-Reply-To: References: Mime-Version: 1.0 (Apple Message framework v622) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <32fd4a5efbfd9d3afbbae300411c0379@Astro.physik.Uni-Goettingen.DE> Content-Transfer-Encoding: 7bit Cc: IVOA List VOEvent , Rob Seaman , From: "Frederic V. \"Rick\" Hessman" Subject: Re: New UCDs for VOEvent please Date: Wed, 27 Apr 2005 13:34:54 +0200 To: "Patricio F. Ortiz" X-Mailer: Apple Mail (2.622) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.27.3 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Frederic V. \"Rick\" Hessman" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 > "how do you envision using these new UODs (Unified Object-type > Descriptor)?" By that, I mean, in which part of the metadata would you > like to insert theses descriptors? To explain where I'm coming from, let's look at VOEvent and RTML: - the VOEvent now has a element, where (name) can be something like "supernova" or "gamma-ray burst". - RTML has a TargetType used by a (name) element. Sound pretty similar? Yes, VOEvent could adopt RTML's element or vice versa, but what do the Virtual Repository people do? Is it really the job of VOEvent to suggest how all the VO colleagues are supposed to classify objects when they get around to needing such, especially when others start needed descriptions of objects and processes which will never produce an event? I admit I'm a newcomer with no (as yet) official function, but I can't imagine the VO getting much farther without being able to teach the software how to describe what is is we're actually studying beyond saying that the number in a table is supposed to mean (admittedly an important first step). > An object type may not be unique... How do we handle those cases? > (after > all, these are flags/labels to make our life easier. If the core of a > galaxy is an AGN, what does the descriptor look like? > UCDs of physical quantities are much easier to handle in that sense! > (as > noted below regarding the unicity of a UCD). Why the need for a final description? From a VOEvent perspective, something should gradually shift from one description to another, e.g. process.burst;em.gamma -> process.burst;em.vis -> galaxies;stars.supernova or - something which is bound to happen eventually (since it already has) - galaxies.Seyfert;galaxies.nucleus;em.X-ray -> stars.variable.cataclysmic.polar This capability for being able to descibe what people/computers think is happening has quite practical consequences when it comes to things like follow-up observations: some won't be interested in Seyferts, others in polars, and the Chandra ToO may insist that it be one or the other. > How deep do we want to describe an object? Say that the same AGN has > exhibited variations in HBeta flux (ok, kick for the incorrectness :-) > :-) > Do we want to describe such variability? For some people/applications > it > will be important, for others not. Deep enough to be useful, shallow enough to be manageable. Rick ------------------------------------------------------------------------ ------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Universitaets-Sternwarte Tel. +49-551-39-5052 Geismarlandstr. 11 Fax +49-551-39-5043 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman ------------------------------------------------------------------------ ------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.uni-goettingen.de ------------------------------------------------------------------------ ------------------------- From owner-ucd@eso.org Wed Apr 27 18:11:44 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RGBRl1013272 for ; Wed, 27 Apr 2005 18:11:28 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3RGBRlr013270 for ucd-outgoing; Wed, 27 Apr 2005 18:11:27 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RGBBl1013207; Wed, 27 Apr 2005 18:11:12 +0200 (MEST) Received: from noao.edu (noao.edu [140.252.1.54]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RGB7XW000607; Wed, 27 Apr 2005 18:11:07 +0200 (CEST) X-Spam-Checker-Version: SpamAssassin 3.0.2 (2004-11-16) on noao.edu X-Spam-Level: X-Spam-Status: No, score=-5.8 required=4.5 tests=ALL_TRUSTED,AWL,BAYES_00 autolearn=ham version=3.0.2 X-TFF-CGPSA-Version: 1.4f1 X-TFF-CGPSA-Filter: Scanned Received: from [140.252.4.27] (account seaman HELO [140.252.4.27]) by noao.edu (CommuniGate Pro SMTP 4.3c5) with ESMTPSA id 17902390; Wed, 27 Apr 2005 09:10:55 -0700 In-Reply-To: <32fd4a5efbfd9d3afbbae300411c0379@Astro.physik.Uni-Goettingen.DE> References: <32fd4a5efbfd9d3afbbae300411c0379@Astro.physik.Uni-Goettingen.DE> Mime-Version: 1.0 (Apple Message framework v619.2) Content-Type: text/plain; charset=US-ASCII; format=flowed Message-Id: <72138974eda1f17ad78589973743b4ee@noao.edu> Content-Transfer-Encoding: 7bit From: Rob Seaman Subject: Re: New UCDs for VOEvent please Date: Wed, 27 Apr 2005 09:10:42 -0700 To: " " , IVOA List VOEvent X-Mailer: Apple Mail (2.619.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.27.8 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Rob Seaman X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 This is a timely discussion for the VOEvent folks, but likely perplexing for the UCD folks. The gist of my previous comments was not that VOEvent didn't need to wrestle with characterizing coherent descriptions for the "hypothesis" section of an event. The hypothesis is the key to fielding a richly useful VOEvent facility. Rather, I question whether a UCD, per se, is the correct way to represent this kind of information - clearly itself not a brand new topic for the UCD list :-) It might be that we need to borrow the syntax from UCD's and roll our own - or it might be that we just need to pick another namespace(s). Both the VO and the larger astronomical community would benefit from wrestling with the issues Rick has raised. In the mean time, Patricio asks a lot of good questions. Rob Seaman NOAO From owner-voevent@eso.org Wed Apr 27 18:16:49 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RGGZl1014984 for ; Wed, 27 Apr 2005 18:16:35 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3RGGZ16014982 for voevent-outgoing; Wed, 27 Apr 2005 18:16:35 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-voevent@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RGGUl1014927; Wed, 27 Apr 2005 18:16:31 +0200 (MEST) Received: from mail.cacr.caltech.edu (mail.cacr.caltech.edu [131.215.145.9]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RGGR73022870; Wed, 27 Apr 2005 18:16:28 +0200 (CEST) Received: from [131.215.146.187] ([131.215.146.187]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id j3RGGIQm014665; Wed, 27 Apr 2005 09:16:18 -0700 Message-ID: <426FBAC9.2050600@cacr.caltech.edu> Date: Wed, 27 Apr 2005 09:16:09 -0700 From: Matthew Graham User-Agent: Mozilla Thunderbird 1.0.2 (Macintosh/20050317) X-Accept-Language: en-us, en MIME-Version: 1.0 To: "Frederic V. \"Rick\" Hessman" CC: "Patricio F. Ortiz" , IVOA List VOEvent , Rob Seaman , ucd@ivoa.net Subject: Re: New UCDs for VOEvent please References: <32fd4a5efbfd9d3afbbae300411c0379@Astro.physik.Uni-Goettingen.DE> In-Reply-To: <32fd4a5efbfd9d3afbbae300411c0379@Astro.physik.Uni-Goettingen.DE> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.27.7 X-Virus-Scanned: by amavisd-new Sender: owner-voevent@eso.org Precedence: bulk Reply-To: Matthew Graham X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi, One alternative, though I do not know how practically viable it would be at present, is to use the astronomy ontology that Ed Shaya at University of Maryland is developing and presented a poster about at last year's ADASS. Cheers, Matthew From owner-ucd@eso.org Wed Apr 27 18:28:15 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RGRxl1018056 for ; Wed, 27 Apr 2005 18:27:59 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3RGRxoA018055 for ucd-outgoing; Wed, 27 Apr 2005 18:27:59 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RGRrl1018037 for ; Wed, 27 Apr 2005 18:27:53 +0200 (MEST) Received: from smtp1.sic.rm.cnr.it (mailrelay.artov.rm.cnr.it [150.146.129.253]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RGRp73023763 for ; Wed, 27 Apr 2005 18:27:52 +0200 (CEST) Received: (qmail 3532 invoked by uid 508); 27 Apr 2005 16:27:45 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.84. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.039285 secs); 27 Apr 2005 16:27:45 -0000 Received: from unknown (HELO localhost) ([10.1.1.2]) (envelope-sender ) by smtp1.sic.rm.cnr.it (qmail-ldap-1.03) with SMTP for ; 27 Apr 2005 16:27:45 -0000 Received: from apm.rm.iasf.cnr.it (apm.rm.iasf.cnr.it [150.146.136.115]) by webmail.sic.rm.cnr.it (Horde) with HTTP for ; Wed, 27 Apr 2005 18:27:45 +0200 Message-ID: <20050427182745.g87w5yhcs76swcok@webmail.sic.rm.cnr.it> Date: Wed, 27 Apr 2005 18:27:45 +0200 From: Andrea Preite Martinez To: ucd@ivoa.net Subject: UCDs and VOEvents MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1 Content-Disposition: inline Content-Transfer-Encoding: 7bit User-Agent: Internet Messaging Program (IMP) H3 (4.0.1) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.27.7 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Andrea Preite Martinez X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear Roy, dear members of the VOE group, > Dear Andrea and Sebastien > This note is to ask the UCD working group for help in building a new section of the UCD > vocabulary in support of the VOEvent working group. > ... thank you for your very interesting and challenging proposal! We think the UCDwg can be the right place to discuss all semantic aspects of the VO, not only those related to "bona fide" UCDs. Of course, we should clearly keep on the right track, as already defined in the last years, for what concerns the UCDs, their definition, their semantics, their syntax, their usage. For the main document on UCDs we have to go on from the stage of Proposed Recommendation to the formal stage of IVOA Recommendation. We also have to upgrade the (new!) list of ucd-words from the level of Draft to that of PR, through a formal RFC. We can do this in Kyoto. Your proposal of opening a discussion in the UCDwg > with the objective of > describing "immediate astronomical events" in a semantically-meaningful way > ... > covering astronomical event types is, as we said, both interesting and challenging. Interesting, because - it is a problem that has been tackled many times giving rise to a number of "subjective" solutions (each one valid/sound in its own context): it is time to discuss it starting from the work already done, but trying to do it in a "semantically-meaningful way" - it has to do with a semantic problem that is hard to locate in/assign to other IVOA WGs; - the UCDwg has the right competences to do the job. Challenging, because - definitely hard to do - not to be mixed up with UCDs, that are ment to serve other purposes. The "mail storm" produced by your proposal is a clear indication of interest, but it also tells us that the discussion has to be kept within clear and firm boundaries, having in mind the distinction between UCDs and their role on one hand, and the "event vocabulary" on the other. In conclusion, the answer to your questions: > Could you help us with doing this? > Perhaps a meeting at the Kyoto IVOA would be appropriate? is yes, we can help, yes, the final part of the UCD session in Kyoto will be devoted to the "event vocabulary". All VOEvent people are of course invited to this session. A tentative agenda could be: - A short presentation of the problem (somebody from the VOEwg has to volunteer for that! Please, let me (=>Andrea) know.) - Plenary discussion, actions. In order not to diverge too much before the start of the discussion in Kyoto, here you can find a few remarks/comments on http://monet.uni-sw.gwdg.de/twiki/bin/view/VOEvent/UnifiedContentDescriptors > Unfortunately, the IVOA/UCD list is incomplete: there's no complete > wavelength/frequency coverage in "em.*", for instance (e.g. no em.microwave). The UCD coverage of the electromagnetic spectrum *is* complete. The top-level wavelength/frequency division simply follows the one adopted for the Registry description for more compatibility, that is 7 large bands: radio, mm, IR, optical, UV, X-ray, gamma-ray. See "Spectral Coverage" in http://www.ivoa.net/Documents/REC/ResMetadata/RM-20040426.html Therefore, there is no top level like EUV, sub-mm or microwave, but I guess microwave is covered by the following UCD : em.radio.1500-3000MHz, em.radio.3-6GHz, em.radio.6-12GHz, ... It is important to first notice that the description of the electromagnetic division in the em.* words of the UCD is a special case: it can be seen as an enumeration of possible values for the observation passband. Take for example the description of an IRAS 12 micron flux in VOTable. We can write it: But we could have written: The introduction of all the em.* terms in the UCD vocabulary was done to allow the first description, instead of the 2nd that is less standard, because different people would use different values for the "bandpass" description (12um, IRAS 12 micron, 8.5-15micron, ...) The em.* words can be seen as named instances of the generic "instr.bandpass" UCD. These words were introduced into the vocabulary for two reasons: - they are absolutely needed: most astronomical information comes from photons, and we need to expres in which part of the spectrum a flux or magnitude was measured. - the problem is relatively simple, as it roughly only implies defining intervals on a one-dimensional axis. The astronomical object types haven't been so far introduced in the UCD vocabulary for several reasons: - the main use of UCDs is to describe table columns. The existing "src.class" and "meta.code.class" UCDs were sufficient for this purpose, allowing to describe that a catalogue's column contains an astronomical source classification. This classification (often a numeric code for UCD meta.code.class) is what the author of the catalogue writes, and is not standardized. - Even for the description of a single measurement, we should avoid putting all the metadata into a UCD. We'd hate to see that value 5.23mag is described by ucd="phot.mag;em.opt.V;object.star.supernova.individual.SN1987A;time.epoch.1990" Instead, we'd rather say (in VOTable-like syntax): - The precise definition of object types is very complex. There are examples in the journal keywords, but also in SIMBAD: http://simbad.u-strasbg.fr/guide/chF.htx or the IAU thesaurus http://msowww.anu.edu.au/library/thesaurus/english/ ... The object type definition is difficult, because we often have to deal with hierarchical structure/classification, and an object can belong to different classes: a galaxy can be at the same time: - galaxy - galaxy in cluster - IR source - radio source - X-ray source - emission-line galaxy - galaxy with active nucleus (AGN) - ... The classification can depend on the background of the astronomer (e.g. radio or optical astronomer), and in some cases the boundaries between different classes are fuzzy... (Also !) for these reasons, the definition of standard words for object types was deliberately left out of the UCD vocabulary. But it might be useful to create a new "object" branch, to enumerate a list of possible standardized object types. A careful explanation of each term should be provided, so there is no ambiguity: e.g. does Planetary_Nebula mean the central star, the nebula or both? This list of terms would correspond to an enumeration of possible values corresponding to ucd="src.class". In the same spirit, the "events" are poorly described with the current ucd words. There are a few ones, like pos.lunar.occult, phys.mass.loss or src.var.pulse, but they can certainly be better described by domain specialists. Andrea Sebastien From owner-voevent@eso.org Wed Apr 27 18:53:53 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RGrZl1023712 for ; Wed, 27 Apr 2005 18:53:35 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3RGrZEa023711 for voevent-outgoing; Wed, 27 Apr 2005 18:53:35 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-voevent@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RGrVl1023701; Wed, 27 Apr 2005 18:53:31 +0200 (MEST) Received: from mail.cacr.caltech.edu (mail.cacr.caltech.edu [131.215.145.9]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RGrS73025765; Wed, 27 Apr 2005 18:53:29 +0200 (CEST) Received: from [131.215.146.179] ([131.215.146.179]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id j3RGrQQm015648; Wed, 27 Apr 2005 09:53:26 -0700 Message-ID: <426FC384.5080509@cacr.caltech.edu> Date: Wed, 27 Apr 2005 09:53:24 -0700 From: Roy Williams User-Agent: Mozilla Thunderbird 1.0.2 (Macintosh/20050317) X-Accept-Language: en-us, en MIME-Version: 1.0 To: IVOA List VOEvent , ucd@ivoa.net Subject: Re: New UCDs for VOEvent please References: <32fd4a5efbfd9d3afbbae300411c0379@Astro.physik.Uni-Goettingen.DE> <426FBAC9.2050600@cacr.caltech.edu> In-Reply-To: <426FBAC9.2050600@cacr.caltech.edu> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.27.8 X-Virus-Scanned: by amavisd-new Sender: owner-voevent@eso.org Precedence: bulk Reply-To: Roy Williams X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Part of the trouble with ontology/vocabulary discussions is that they can fly away so easily into abstraction. I would like to try and ground the discussion with some examples that I have heard over the last few days. How can we make the UCD set so that the following are possible? (1) Selection of events A client may wish to get, for example: "All events that involve cepheid sources" "All supernova events brighter than 18 magnitude" In order to service these subscriptions, the client would use specific UCDs in place of the natural language words "cepheid" and "supernova". We assume that a machine-learning system in the data pipeline has made probabilistic assessments that the event is "cepheid" or "supernova". We could also do this without the formal UCD structure by doing keyword search in the natural language "description" section of the event -- which of course assumes that some human had written the textual description. (2) When a followup changes the hypothesis Suppose there is an interesting event that is classified somehow (eg supernova). There might be many followup observations that cite the original event ID, and some of these might show a different classification. How can we decide if the classification status of an event has significantly changed, or become more definite, due to followup? From owner-ucd@eso.org Wed Apr 27 19:04:38 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RH4Ol1026121 for ; Wed, 27 Apr 2005 19:04:24 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3RH4Oga026120 for ucd-outgoing; Wed, 27 Apr 2005 19:04:24 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RH4Cl1026077; Wed, 27 Apr 2005 19:04:12 +0200 (MEST) Received: from noao.edu (noao.edu [140.252.1.54]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3RH47XW005032; Wed, 27 Apr 2005 19:04:08 +0200 (CEST) X-Spam-Checker-Version: SpamAssassin 3.0.2 (2004-11-16) on noao.edu X-Spam-Level: X-Spam-Status: No, score=-5.8 required=4.5 tests=ALL_TRUSTED,AWL,BAYES_00 autolearn=ham version=3.0.2 X-TFF-CGPSA-Version: 1.4f1 X-TFF-CGPSA-Filter: Scanned Received: from [140.252.4.27] (account seaman HELO [140.252.4.27]) by noao.edu (CommuniGate Pro SMTP 4.3c5) with ESMTPSA id 17903475; Wed, 27 Apr 2005 10:03:54 -0700 In-Reply-To: <426FBAC9.2050600@cacr.caltech.edu> References: <32fd4a5efbfd9d3afbbae300411c0379@Astro.physik.Uni-Goettingen.DE> <426FBAC9.2050600@cacr.caltech.edu> Mime-Version: 1.0 (Apple Message framework v619.2) Content-Type: text/plain; charset=US-ASCII; format=flowed Message-Id: Content-Transfer-Encoding: 7bit Cc: ucd@ivoa.net From: Rob Seaman Subject: Re: New UCDs for VOEvent please Date: Wed, 27 Apr 2005 10:03:42 -0700 To: IVOA List VOEvent X-Mailer: Apple Mail (2.619.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.27.8 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Rob Seaman X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 On Apr 27, 2005, at 9:16 AM, Matthew Graham wrote: > One alternative, though I do not know how practically viable it would > be at present, is to use the astronomy ontology that Ed Shaya at > University of Maryland is developing and presented a poster about at > last year's ADASS. I didn't want to muddy the waters by bringing up the "O" word. Google "Shaya astronomy ontology" for lots of hits on this. My visceral reaction to discussions over the last couple of years as well as the last couple of days is similar. A noble effort - so large and grand that pragmatic functioning systems can't possibly rely on the results in any strong sense. I also have a deep skepticism that practicing astronomers will embrace the results. Noble nonetheless and worthy of the best efforts that the VO can spare. On the other hand, VOEvent will amount to nothing if it is not rigorously pragmatic. I don't think that "pragmatic" and "ontology" are incompatible - and VOEvent provides a great test case for demonstrating this. We need to describe only certain astronomical processes/objects - the ones with a time varying nature. Our list should be biased by an artful sense of where the productive science lies - start with shadings of GRBs, SNs, solar system objects - and some variations on grab bag categories of "other" or "none of the above" or even "all of the above". Establish a process for adding to the list. And don't get too torqued up about "technical correctness". Rob Seaman NOAO From owner-ucd@eso.org Fri Apr 29 20:52:38 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3TIqGBl007950 for ; Fri, 29 Apr 2005 20:52:16 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3TIqG0V007949 for ucd-outgoing; Fri, 29 Apr 2005 20:52:16 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3TIq7Bl007935; Fri, 29 Apr 2005 20:52:08 +0200 (MEST) Received: from earth.astro.umd.edu (earth.astro.umd.edu [129.2.14.2]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3TIq573004740; Fri, 29 Apr 2005 20:52:06 +0200 (CEST) Received: from [129.2.15.131] (lap31.astro.umd.edu [129.2.15.131]) by earth.astro.umd.edu (Postfix) with ESMTP id 88A9A109AF; Fri, 29 Apr 2005 14:51:59 -0400 (EDT) Message-ID: <4272824B.7010900@gsfc.nasa.gov> Date: Fri, 29 Apr 2005 14:51:55 -0400 From: Ed Shaya User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.7.6) Gecko/20050319 X-Accept-Language: en-us, en MIME-Version: 1.0 To: Rob Seaman Cc: IVOA List VOEvent , ucd@ivoa.net Subject: Re: New UCDs for VOEvent please References: <32fd4a5efbfd9d3afbbae300411c0379@Astro.physik.Uni-Goettingen.DE> <426FBAC9.2050600@cacr.caltech.edu> In-Reply-To: Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.4.29.22 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Ed Shaya X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Rob Seaman wrote: > On Apr 27, 2005, at 9:16 AM, Matthew Graham wrote: > >> One alternative, though I do not know how practically viable it would >> be at present, is to use the astronomy ontology that Ed Shaya at >> University of Maryland is developing and presented a poster about at >> last year's ADASS. > > > I didn't want to muddy the waters by bringing up the "O" word. Google > "Shaya astronomy ontology" for lots of hits on this. My! I took this advice and googled on "ontology shaya" and found the following information: *C. Paths to Enlightenment: Buddhist Art in India and Java* *The Life and Teachings of the Buddha (ca. 563-483):* Prince Siddhartha, surname Gautama, son of Queen Maya and King Suddhodana, born in the small kingdom of Kapilavastu near the Nepalese border. Known as Shakyamuni ("Sage of the Shaya Clan"). Nirvana, Parinirvana at Kusignagara. Formation of the Sangha or Order of Monks What this says is that an alias name for Buddha/Siddhartha is "Sage of the Shaya Clan". It logically follows that Ontology is part of the eightfold path to enlightenment or possibly the ninth fold. > My visceral reaction to discussions over the last couple of years as > well as the last couple of days is similar. A noble effort - so large > and grand that pragmatic functioning systems can't possibly rely on > the results in any strong sense. I also have a deep skepticism that > practicing astronomers will embrace the results. Noble nonetheless > and worthy of the best efforts that the VO can spare. > > On the other hand, VOEvent will amount to nothing if it is not > rigorously pragmatic. I don't think that "pragmatic" and "ontology" > are incompatible - and VOEvent provides a great test case for > demonstrating this. We need to describe only certain astronomical > processes/objects - the ones with a time varying nature. Our list > should be biased by an artful sense of where the productive science > lies - start with shadings of GRBs, SNs, solar system objects - and > some variations on grab bag categories of "other" or "none of the > above" or even "all of the above". Establish a process for adding to > the list. And don't get too torqued up about "technical correctness". With th end of the NVO NSF grant within 18 months, it certainly makes sense to find the quickest and simplest set of terms to fashion into a message for VOEvent alerting. Afterall, we just want to say an event happened at such a time and it appears to be one of these things. And it appears that it is almost finished except for a few details and agreement to standards. But we can also be keeping another eye on the longer time scale where we want to be able to put data in machine understandable terms so that applications can do the most possible on our behalf. This requires something a bit more sophisticated than just a simple class hierarchy of terms. An ontology would be more complete but probably not even an order of magnitude (factor 10) more than the UCD is now. In fact, given the requests and requirements to augment UCDs, with time, the UCD will probably grow to the size of an ontology anyway. So, it is probably wise to start doing some thinking in terms of the formal OWL standard now. What we do with the ontology can vary greatly. 1. Use it as a string identifier, exactly as UCDs are. The advantage is that one can read the Ontology at that point to get more context for the meaning of the term. 2. Use it as one more model builder for developing schemas. This is like UML but more in tune with knowledge/information structures. I think this is what Mathew had in mind. 3. Use it to test completeness and consistency of terms. This would not be on the fly, but rather as one adds new terms one can see whether it is clashing with other terms and Venn diagrams let you see something about completeness. This then makes it more acceptable for groups to be adding terms into their namespace without going to the VO heads or the IAU. 4. One can use it as the defining structure of all information being exchanged. Sounds daring but in fact several other related science fields are preparing to do just that, including space physics. 5. One can use it to reason out pathways to converting, pipelining, and analysing data. It should be possible to automatically find the transformation and queries needed to satisfy an arbitrary stated goal or request. Our group at UMD has an NASA/AISRP grant to figure out the basics of how this might be done using OWL. Ed > Rob Seaman > NOAO > > From owner-ucd@eso.org Mon May 2 07:16:21 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j425FvoQ023119 for ; Mon, 2 May 2005 07:15:57 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j425FvXr023118 for ucd-outgoing; Mon, 2 May 2005 07:15:57 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j425FroQ023114 for ; Mon, 2 May 2005 07:15:53 +0200 (MEST) Received: from smtp1.sic.rm.cnr.it (mailrelay.artov.rm.cnr.it [150.146.129.253]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j425Fp73017632 for ; Mon, 2 May 2005 07:15:52 +0200 (CEST) Received: (qmail 23540 invoked by uid 508); 2 May 2005 05:15:46 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.84. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.030478 secs); 02 May 2005 05:15:46 -0000 Received: from unknown (HELO localhost) ([10.1.1.2]) (envelope-sender ) by smtp1.sic.rm.cnr.it (qmail-ldap-1.03) with SMTP for ; 2 May 2005 05:15:45 -0000 Received: from host31-74.pool80181.interbusiness.it (host31-74.pool80181.interbusiness.it [80.181.74.31]) by webmail.sic.rm.cnr.it (Horde) with HTTP for ; Mon, 2 May 2005 07:15:45 +0200 Message-ID: <20050502071545.o2qry3nmgtcgok8s@webmail.sic.rm.cnr.it> Date: Mon, 2 May 2005 07:15:45 +0200 From: Andrea Preite Martinez To: ucd@ivoa.net Subject: New list of words MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1 Content-Disposition: inline Content-Transfer-Encoding: 7bit User-Agent: Internet Messaging Program (IMP) H3 (4.0.1) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.1.42 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Andrea Preite Martinez X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear member of the UCD_wg, since last Friday (20050429) an updated list of UCD words is available at: http://vizier.u-strasbg.fr/UCD/ucd1p-words.txt at the UCD page: http://vizier.u-strasbg.fr/UCD/ The new list of words has been edited according to the very valuable comments coming from the community and also thanks to the (almost!) every day use of them made by Sebastien and myself. The most important differences with the previous version (20040823) concern - distances and sizes (linear/angular) - the introduction of a rectangular/cartesian reference frame - the phot.color section, much simplified - spelling, abbreviations, syntax ... At the UCD page you can also find un updated version of the UCD_tree browser(s) and a new tool, the ucd_builder: http://vizier.u-strasbg.fr/UCD/cgi-bin/descr2ucd that uses a description in "natural" language to find the relevant ucd_words, and then tries to build a valid ucd out of them. In these two weeks before Kyoto please explore the list, use the tools and send back comments. A more "formal" comment page is available to suggest changes in the list of words at: http://vizier.u-strasbg.fr/UCD/cgi-bin/comment/ucdComments Have fun. Andrea ============================================================================== Andrea Preite Martinez andrea@rm.iasf.cnr.it Istituto di Astrofisica Spaziale Tel.:+39.06.4993.4641 Area di Ricerca di Tor Vergata Fax.:+39.06.2066.0188 Via del Fosso del Cavaliere 100 Cell:+39.339.3817355 00133 Roma ============================================================================== From owner-ucd@eso.org Mon May 2 12:26:14 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j42AQ0GH003910 for ; Mon, 2 May 2005 12:26:00 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j42AQ0be003909 for ucd-outgoing; Mon, 2 May 2005 12:26:00 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j42APoGH003836; Mon, 2 May 2005 12:25:50 +0200 (MEST) Received: from [134.171.10.12] (ma008861.hq.eso.org [134.171.10.12]) by serapis.hq.eso.org (8.11.7+Sun/8.11.7) with ESMTP id j42APoD25689; Mon, 2 May 2005 12:25:50 +0200 (MEST) In-Reply-To: <20050502071545.o2qry3nmgtcgok8s@webmail.sic.rm.cnr.it> References: <20050502071545.o2qry3nmgtcgok8s@webmail.sic.rm.cnr.it> Mime-Version: 1.0 (Apple Message framework v622) Content-Type: text/plain; charset=US-ASCII; format=flowed Message-Id: Content-Transfer-Encoding: 7bit Cc: ucd@ivoa.net From: Alberto Micol Subject: Re: New list of words Date: Mon, 2 May 2005 12:25:47 +0200 To: Andrea Preite Martinez X-Mailer: Apple Mail (2.622) X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Alberto Micol X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Dear Andrea, Thanks a lot for the new list! A couple of comments/suggestions: Versioning: the ucd1p-words.txt file does not contain any version one could refer to. On this topic, the UCD page (http://vizier.u-strasbg.fr/UCD/) provides a link to "ucd1p-words.txt" and a link to "ucd1p-words-20050429.txt" and it is not clear whether one is a link to the other (I would prefer to always see the version in the file name). Also, beware that the document pointed to in the UCD page ("Explanations on the vocabulary are available in IVOA WD-UCDlist-20050429.pdf") is not found on the ivoa web site. Then, looking at the list with biased eyes given that these days I'm working on the Characterisation DM, I have a remark on some asymmetry within the list. For example let's take the Resolution concept for which I can find: Q|instr.angRes |Angular resolution Q|instr.spect.resolution |Spectral (or velocity) resolution Q|time.resolution |Time resolution The problems I see with this are: 1.- the resolution (think of an image from the ground) is not only a instrumental effect (unless one thinks of the atmosphere as part of the instrument) 2.- In the charcterisation DM, resolution on the various axes is treated symmetrically Hence, my preference would go for something along these lines: Q|pos.resolution |Angular resolution Q|spect.resolution |Spectral (or velocity) resolution Q|time.resolution |Time resolution What do you think? Ciao, Alberto PS: Just another little question on: S|instr.pixel |Pixel what is that for? In which case is it used? Thanks. On May 2, 2005, at 07:15, Andrea Preite Martinez wrote: > Dear member of the UCD_wg, > > since last Friday (20050429) an updated list of UCD words is available > at: > > http://vizier.u-strasbg.fr/UCD/ucd1p-words.txt > > at the UCD page: > > http://vizier.u-strasbg.fr/UCD/ > ... From owner-ucd@eso.org Mon May 2 14:39:00 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j42CcjGH024012 for ; Mon, 2 May 2005 14:38:45 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j42CcjNr024011 for ucd-outgoing; Mon, 2 May 2005 14:38:45 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j42CceGH023990 for ; Mon, 2 May 2005 14:38:41 +0200 (MEST) Received: from smtp1.sic.rm.cnr.it (mailrelay.artov.rm.cnr.it [150.146.129.253]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j42Bur73029092 for ; Mon, 2 May 2005 13:56:54 +0200 (CEST) Received: (qmail 27003 invoked by uid 508); 2 May 2005 11:56:47 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.84. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.030166 secs); 02 May 2005 11:56:47 -0000 Received: from unknown (HELO localhost) ([10.1.1.2]) (envelope-sender ) by smtp1.sic.rm.cnr.it (qmail-ldap-1.03) with SMTP for ; 2 May 2005 11:56:47 -0000 Received: from eddington.rm.iasf.cnr.it (eddington.rm.iasf.cnr.it [150.146.136.118]) by webmail.sic.rm.cnr.it (Horde) with HTTP for ; Mon, 2 May 2005 13:56:47 +0200 Message-ID: <20050502135647.sugef32llp0gkk4g@webmail.sic.rm.cnr.it> Date: Mon, 2 May 2005 13:56:47 +0200 From: Andrea Preite Martinez To: Alberto Micol Cc: ucd@ivoa.net Subject: Re: New list of words References: <20050502071545.o2qry3nmgtcgok8s@webmail.sic.rm.cnr.it> In-Reply-To: MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1; format="flowed" Content-Disposition: inline Content-Transfer-Encoding: 7bit User-Agent: Internet Messaging Program (IMP) H3 (4.0.1) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.2.8 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Andrea Preite Martinez X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Dear Alberto > > beware that the document pointed to in the UCD page > ("Explanations on the vocabulary are available in IVOA > WD-UCDlist-20050429.pdf") is not found on the ivoa web site. sorry, still editing a section... > I have a remark on some asymmetry within the list. For example > let's take the Resolution ... > ... my preference would go for something along these lines: > > Q|pos.resolution |Angular resolution > Q|spect.resolution |Spectral (or velocity) > resolution > Q|time.resolution |Time resolution > > What do you think? I like your proposal. I'm sure you'll have other before Kyoto! > PS: Just another little question on: > S|instr.pixel |Pixel > what is that for? In which case is it used? Try "pixel size" on the builder. Andrea From owner-ucd@eso.org Mon May 2 14:56:58 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j42CugGH028270 for ; Mon, 2 May 2005 14:56:42 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j42CugQA028269 for ucd-outgoing; Mon, 2 May 2005 14:56:42 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j42CuXGH028203; Mon, 2 May 2005 14:56:34 +0200 (MEST) Received: from alpha.uni-sw.gwdg.de (alpha.uni-sw.gwdg.de [134.76.205.222]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j42CuW73000966; Mon, 2 May 2005 14:56:32 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1DSaTK-001dex-P6; Mon, 02 May 2005 14:56:26 +0200 In-Reply-To: <4272824B.7010900@gsfc.nasa.gov> References: <32fd4a5efbfd9d3afbbae300411c0379@Astro.physik.Uni-Goettingen.DE> <426FBAC9.2050600@cacr.caltech.edu> <4272824B.7010900@gsfc.nasa.gov> Mime-Version: 1.0 (Apple Message framework v622) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <71e0852515f7c6122fe60632c6efb16d@Astro.physik.Uni-Goettingen.DE> Content-Transfer-Encoding: 7bit Cc: IVOA List VOEvent , Rob Seaman , ucd@ivoa.net From: "Frederic V. \"Rick\" Hessman" Subject: Re: New UCDs for VOEvent please Date: Mon, 2 May 2005 14:58:37 +0200 To: Ed Shaya X-Mailer: Apple Mail (2.622) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.2.9 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Frederic V. \"Rick\" Hessman" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 On 29 Apr 2005, at 8:51 pm, Ed Shaya wrote: > But we can also be keeping another eye on the longer time scale where > we want to be able to put data in machine understandable terms so that > applications can do the most possible on our behalf. This requires > something a bit more sophisticated than just a simple class hierarchy > of terms. An ontology would be more complete but probably not even an > order of magnitude (factor 10) more than the UCD is now. In fact, > given the requests and requirements to augment UCDs, with time, the > UCD will probably grow to the size of an ontology anyway. So, it is > probably wise to start doing some thinking in terms of the formal OWL > standard now. What we do with the ontology can vary greatly. > 1. Use it as a string identifier, exactly as UCDs are. The advantage > is that one can read the Ontology at that point to get more context > for the meaning of the term. > 2. Use it as one more model builder for developing schemas. This is > like UML but more in tune with knowledge/information structures. I > think this is what Mathew had in mind. > 3. Use it to test completeness and consistency of terms. This would > not be on the fly, but rather as one adds new terms one can see > whether it is clashing with other terms and Venn diagrams let you see > something about completeness. This then makes it more acceptable for > groups to be adding terms into their namespace without going to the VO > heads or the IAU. > 4. One can use it as the defining structure of all information being > exchanged. Sounds daring but in fact several other related science > fields are preparing to do just that, including space physics. > 5. One can use it to reason out pathways to converting, pipelining, > and analysing data. It should be possible to automatically find the > transformation and queries needed to satisfy an arbitrary stated goal > or request. Our group at UMD has an NASA/AISRP grant to figure out > the basics of how this might be done using OWL. Ummm.... maybe my googling didn't go quite as far or I'm missing something: the "ontology" I found was a "low-level" (no - that sounds too negative - let's say "very fundamental") means of describing scientific quantities - nothing particularly "astronomical" about it. If this is as far as anyone has gotten, then I vote for a mid-term temporary solution - what I've called "VOThings" - which someone else can turn into a full astronomical ontology in the future. Thus, - Small, multiple, overlapping, incompatible lists within different schemata will be an unnecessary pain, so we need a minimal common-ground list. - A formal development of a real astronomical ontology will take many years and we can't wait that long. - We should resist the temptation to make VOThings "complete" since it won't ever be such and we'd waste time in trying. Maybe having such a terrible name will be a good thing - let's get it over quickly knowing that some day somebody else will get it right. Rick ------------------------------------------------------------------------ ------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Universitaets-Sternwarte Tel. +49-551-39-5052 Geismarlandstr. 11 Fax +49-551-39-5043 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman ------------------------------------------------------------------------ ------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.uni-goettingen.de ------------------------------------------------------------------------ ------------------------- From owner-ucd@eso.org Tue May 3 10:55:47 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j438t6YH024745 for ; Tue, 3 May 2005 10:55:06 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j438t6Q4024743 for ucd-outgoing; Tue, 3 May 2005 10:55:06 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j438ssYH024705; Tue, 3 May 2005 10:54:54 +0200 (MEST) Received: from [134.171.10.12] (ma008861.hq.eso.org [134.171.10.12]) by serapis.hq.eso.org (8.11.7+Sun/8.11.7) with ESMTP id j438ssD27829; Tue, 3 May 2005 10:54:54 +0200 (MEST) In-Reply-To: <20050502135647.sugef32llp0gkk4g@webmail.sic.rm.cnr.it> References: <20050502071545.o2qry3nmgtcgok8s@webmail.sic.rm.cnr.it> <20050502135647.sugef32llp0gkk4g@webmail.sic.rm.cnr.it> Mime-Version: 1.0 (Apple Message framework v622) Content-Type: text/plain; charset=US-ASCII; format=flowed Message-Id: Content-Transfer-Encoding: 7bit Cc: ucd@ivoa.net From: Alberto Micol Subject: Re: New list of words Date: Tue, 3 May 2005 10:54:53 +0200 To: Andrea Preite Martinez X-Mailer: Apple Mail (2.622) X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Alberto Micol X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Dear Andrea, > I'm sure you'll have other before Kyoto! I'm taking it seriously :-) Here some other comments, in no particular order: 1. pos.frame exists, can we also add the spect.frame and time.frame? 2. instr.spec: probably not needed because otherwise we would also need instr.imager, and similarly for other kinds of instruments. Also, instr.spect.dispersion could simply be instr.dispersion instr.spect.order " " " instr.order (in fact there is no need to say instr.imager.scale, instr.scale is enough). 3. Transmission (an old friend of mine): some time ago Sebastien and I exchanged some emails and, if I remember correctly, we agreed that there should be a phys.transmission which could be attached to any of: instr.det, instr.filter, instr to distinguish between the transmission/sensitivity of the various components (detector, filter, optical elements) and the overall transmission (filter * detector * optical elements) including even the atmosphere if necessary. 4. instr.sensitivity; Its description reads: Instrument sensitivity, detection threshold I would say that sensitivity and detection threshold, while linked, are two different concepts, and would be better to split that one into 2 different UCDs 5. Descriptions: sometimes the description of a ucd is ambiguous, e.g.: a. instr.tel.focus (Q): Telescope focus b. instr.bandpass (Q): Bandpass of instrument c. instr.pixel (S): Pixel a. Is instr.tel.focus the "name" of the telescope focus (eg nasmith), or the focal length of the telescope? b. instr.bandpass How many services will make use of this ucd to describe a table column that contains the numeric transmission at a given wavelength of a given filter? Some other service will use this ucd to describe the name of the bandpass (or the filter name). Which one of the two is legitimate, both? (see (3) above). c. Another, though different, example is the instr.pixel I can think of a catalog associated with an image, where X and Y indicate at which detector coordinates the source was found (pos;instr.pixel). But it can be used to indicate the pixel scale of the detector (phys.angSize;instr.pixel) The fact is that instr.pixel is a Secondary word, hence its meaning could be broader. For that reason probably both above mentioned cases are legitimate: instr.pixel is only an attribute (an adjective in a grammar-speak). I think it is very important to be clear, especially on those words that could be Primary, because otherwise people might misuse UCDs and that would make the entire concept collapse. 6. Abbreviations: Why temperature is some times abbreviated and some other times not? (e.g., instr.skyTemp, phot.antennaTemp, phys.temperature) Wouldn't be better to be consistent? 7. wcs information pos.wcs.ctype: How would the software recognise ctype1 from ctype2 ? Would it be possible to say: pos.wcs.ctype;arith.first and pos.wcs.ctype;arith.second? Or maybe (see cdmatrix below): arith.1 and arith.2 The same for pos.wcs.crpix, crval and naxis pos.wcs.cdmatrix: how to distinguish the various matrix elements? what about accompaining the cdmatrix with a arith.1_1, arith.1_2, etc.? That arith.1, etc. could be useful to rank things. 8. question regarding files meta.file exists; how can I describe the size (eg in bytes) of a file? and its CRC? Probably enough for this morning... ;-) And, beware, I might come back with more DM issues. :-) Ciao, Alberto From owner-ucd@eso.org Tue May 3 16:19:01 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j43EIaYH005964 for ; Tue, 3 May 2005 16:18:36 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j43EIaAQ005963 for ucd-outgoing; Tue, 3 May 2005 16:18:36 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j43EIVYH005950 for ; Tue, 3 May 2005 16:18:31 +0200 (MEST) Received: from othello.physics.gla.ac.uk (othello.physics.gla.ac.uk [130.209.204.200]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j43EITXW010620 for ; Tue, 3 May 2005 16:18:29 +0200 (CEST) Received: from gw-trusted.physics.gla.ac.uk ([130.209.204.195] helo=[192.168.78.115]) by othello.physics.gla.ac.uk:587 with asmtp (TLS-1.0:RSA_ARCFOUR_SHA:16) (Exim 4.34) id 1DSyEA-000206-P3 for ucd@ivoa.net; Tue, 03 May 2005 15:18:24 +0100 Mime-Version: 1.0 (Apple Message framework v622) Content-Transfer-Encoding: 7bit Message-Id: <1eff2d5b2ed291becf05825cb37fd8e6@astro.gla.ac.uk> Content-Type: text/plain; charset=US-ASCII; format=flowed To: ucd@ivoa.net From: Norman Gray Subject: UCD name documentation Date: Tue, 3 May 2005 15:18:22 +0100 X-Mailer: Apple Mail (2.622) X-PHYSCI-Spam-Score: 0.0 (/) X-PHYSCI-Spam-Report: 0.0/5.0 X-Othello-SMTP: True X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.3.12 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Norman Gray X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Greetings, I've just been involved in a discussion in another forum about UCDs, and their general desirability as metadata keywords (in fact it was in the context of the keywords to be extracted by a putative FITS plugin for MacOS X 10.4's Spotlight -- extremely nice). I was trying to discourage folk from using FITS keywords as general metadata, and encourage them to use UCDs instead. As part of this, I produced a set of UCD equivalents for a candidate list of FITS keywords. There were some gaps, however, and I wasn't sure how to go about filling them. Is there a better way than looking through the one-line descriptions in the current list at ? There are two UCD tree browsers on the UCD page, of course, but they're really just a more attractive presentation of the text list and don't, for example, have more discursive documentation. The other UCD tools didn't produce any useful suggestions for `BITPIX' or `number of axes' What would be _really_ nice, of course, is a tool which allowed you to enter one of a subset of FITS keywords and produced one of a few possible UCDs to use instead. So my question is, am I missing something (much more likely than I wish it were)? Such a thing would require an injection of Copious Free Time, of course, but I found myself in a rather awkward place, recommending UCDs over FITS keywords, to an audience which is familiar with FITS, but for whom the UCD list is opaque and rather thinly documented. All the best, Norman -- ---------------------------------------------------------------------- Norman Gray : Physics & Astronomy, Glasgow University, UK http://www.astro.gla.ac.uk/users/norman/ : www.starlink.ac.uk From owner-ucd@eso.org Tue May 3 16:41:41 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j43EfRYH010810 for ; Tue, 3 May 2005 16:41:27 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j43EfRFg010809 for ucd-outgoing; Tue, 3 May 2005 16:41:27 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j43EfMYH010800 for ; Tue, 3 May 2005 16:41:22 +0200 (MEST) Received: from smtp1.sic.rm.cnr.it (smtp1.sic.rm.cnr.it [150.146.129.253]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j43EfK73015259 for ; Tue, 3 May 2005 16:41:21 +0200 (CEST) Received: (qmail 25193 invoked by uid 508); 3 May 2005 14:41:14 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.84. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.061412 secs); 03 May 2005 14:41:14 -0000 Received: from unknown (HELO localhost) ([10.1.1.2]) (envelope-sender ) by smtp1.sic.rm.cnr.it (qmail-ldap-1.03) with SMTP for ; 3 May 2005 14:41:14 -0000 Received: from eddington.rm.iasf.cnr.it (eddington.rm.iasf.cnr.it [150.146.136.118]) by webmail.sic.rm.cnr.it (Horde) with HTTP for ; Tue, 3 May 2005 16:41:14 +0200 Message-ID: <20050503164114.gxpb53ye89ygogo4@webmail.sic.rm.cnr.it> Date: Tue, 3 May 2005 16:41:14 +0200 From: Andrea Preite Martinez To: Norman Gray Cc: ucd@ivoa.net Subject: Re: UCD name documentation References: <1eff2d5b2ed291becf05825cb37fd8e6@astro.gla.ac.uk> In-Reply-To: <1eff2d5b2ed291becf05825cb37fd8e6@astro.gla.ac.uk> MIME-Version: 1.0 Content-Type: multipart/mixed; boundary="=_1ey860p5kkg0" Content-Transfer-Encoding: 7bit User-Agent: Internet Messaging Program (IMP) H3 (4.0.1) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.3.12 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Andrea Preite Martinez X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 This message is in MIME format. --=_1ey860p5kkg0 Content-Type: text/plain; charset=ISO-8859-1; format="flowed" Content-Disposition: inline Content-Transfer-Encoding: 7bit Dear Norman, > As part of this, I produced a set of UCD equivalents for a candidate > list of FITS keywords. I did the same exactly a year ago. UCDs have evolved since then, and the list I'm appending was not revised according to the new list now on-line. The list was generated merging the headers produced by 7 observatories/data_producers (with data in all ranges of wl). > There were some gaps, however, and I wasn't > sure how to go about filling them. Is there a better way than looking > through the one-line descriptions in the current list at > ? There are two UCD > tree browsers on the UCD page, of course, but they're really just a > more attractive presentation of the text list and don't, for example, > have more discursive documentation. The other UCD tools didn't produce > any useful suggestions for `BITPIX' or `number of axes' I agree, even the "builder" will not be of great help with BITPIX! > What would be _really_ nice, of course, is a tool which allowed you to > enter one of a subset of FITS keywords and produced one of a few > possible UCDs to use instead. If you think that the appended list (better, an updated version of it) could be the base for such a tool, I'll do it (the tool, I mean) All the best, Andrea --=_1ey860p5kkg0 Content-Type: text/plain; charset=UTF-8; name="fits-ucd1p.txt" Content-Disposition: attachment; filename="fits-ucd1p.txt" Content-Transfer-Encoding: 7bit #FITS Keyword | Description | Proposed UCD1+ #Andrea, 10/10/2003 | Rev.17/05/2004 | # | | AIRMASS | air mass | obs.air.mass AIRT_EOS | air temperature at End of Scan | phys.temperature;obs.air AIRT_SOS | air temperature at Start of Scan | phys.temperature;obs.air AMASS_FC | approximate air mass at image center | obs.air.mass AM_EOS | air mass at End of Scan | obs.air.mass AM_SOS | air mass at Start of Scan | obs.air.mass APERTURE | name of field of view aperture | meta.id;instr.fov ARCFILE | archive file name | meta.id;meta.file ARYT_EOS | array temperature at End of Scan | phys.temperature;instr AUTHOR | author of the data | meta.bib.author BANDPASS | GSSS bandpass code | instr.bandpass BANDW | total bandwidth of observation | instr.bandwidth BAR_EOS | barometric pressure at End of Scan | phys.pressure;obs.air BAR_SOS | barometric pressure at Start of Scan | phys.pressure;obs.air BASE | pixel dwell time | time;instr.pixel BITPIX | bits per data value | meta.fits.bitpix BLANK | value used for undefined array elements | meta.code;meta.table BLOCKED | is physical blocksize a multiple of 2880? | meta.code;meta.fits BSCALE | linear factor in scaling equation | arith.factor BUNIT | physical units of the array values | meta.unit BZERO | zero point in scaling equation | arith.zp CALID | calibration identifiers for image | meta.id;phot.calib CDELTia | coordinate increment along axis ia | pos.wcs CDi_ja | linear transformation matrix (with scale) | pos.wcs CHECKSUM | checksum for the current HDU | meta.fits.software CHECKVER | version of checksum algorithm | meta.fits.software COMMENT | descriptive comment | meta.note CONFIGUR | s/w configuration used to process the data | meta.fits.software CONTINUE | denotes the CONTINUE long string keyword convention | meta.note CREATOR | name of software task that created the file | meta.id;meta.fits.software CROTAn | coordinate system rotation angle | pos.wcs CRPIXja | pixel coordinate of the reference point | pos.wcs CRVALia | coordinate system value at reference point | pos.wcs CTYPEa | axis type | pos.wcs CUNITia | units of CRVALia and CDELTia | pos.wcs DATAMAX | maximum data value | stat.max DATAMEAN | mean data value | stat.mean DATAMED | median data value | stat.median DATAMIN | minimum data value | stat.min DATAMODE | pre-processor dat mode | meta.fits.software DATARMS | RMS of data values | stat.stdev DATASUM | checksum of the dat records | meta.fits.software DATE | date of file creation | time.epoch;meta.fits DATE-END | date of the end of observation | time.end DATE-OBS | date of the observation | time.epoch DATE_EOS | U.T. date at End of Scan | time.end DATE_SOS | U.T. date at Start of Scan | time.start DAYNUM | sequential survey day number | time.epoch DEC | declination of the observed object | pos.eq.dec DEC_EOS | scan reference declination J2000 | pos.eq.dec DEC_NOM | nominal declination of the observation | pos.eq.dec DEC_OBJ | declination of the observed object | pos.eq.dec DEC_PNT | dec of the pointed direction of the instrument | pos.eq.dec DEC_SCX | declination of the X spacecraft axis | pos.eq.dec;instr DEC_SCY | declination of the Y spacecraft axis | pos.eq.dec;instr DEC_SCZ | declination of the Z spacecraft axis | pos.eq.dec;instr DEC_SOS | scan reference declination J2000 | pos.eq.dec DETNAM | name of detector used to make the observation | meta.id;instr.det DXFS | cross-scan frame step for image | # DYFS | in-scan frame step for image | # ELAPTIME | elapsed time of the observation | time.expo END | marks the end of the header keywords | meta.note EPOCH | equinox of celestial coordinate system | time.equinox EQUINOX | equinox of celestial coordinate system | time.equinox EXPOSURE | exposure time | time.expo EXPTIME | exposure time | time.expo EXTEND | may the FITS file contain extensions? | meta.code EXTLEVEL | hierarchical level of the extension | meta.code EXTNAME | name of the extension | meta.id;meta.code EXTVER | version of the extension | meta.id;meta.code FILENAME | name of the file | meta.id;meta.file FILETYPE | type of file | meta.code;meta.file FILTER | name of filter used during the observation | meta.id;instr.filter FILTERn | name of filters used during the observation | meta.id;instr.filter FLXSCALE | relative flux scale | arith.factor;phot.flux FN_PRNX | observatory filename prefix | meta.id;meta.file FOCUS | telescope focus setting | meta.code;instr.tel.focus FREQ0 | rest frequency | em.freq FREQR | reference frequency | em.freq GCOUNT | group count | meta.number;meta.fits GRATING | name of the grating used during observation | meta.id;instr.grating GRATINGn | name of the grating used during observation | meta.id;instr.grating GROUPS | indicates random groups structure | meta.note HA_EOS | hour angle at End of Scan | pos.az.ha HA_SOS | hour angle at Start of Scan | pos.az.ha HDUCLASS | general identifier for the classification of the data | meta.fits.hdu HDUCLASn | hierarchical classification of the data | meta.fits.hdu HDUDOC | reference to document describing the data format | meta.fits.hdu HDULEVEL | hierarchical level of the HDU | meta.fits.hdu HDUNAME | descriptive name of the HDU | meta.fits.hdu HDUVER | version number of the HDU | meta.fits.hdu HDUVERS | specific version of the document referenced by "HDUDOC" | meta.fits.hdu HIERARCH | denotes the HIERARCH keyword convention at ESO | meta.fits.eso HISTORY | processing history of the data | meta.note;meta.fits ICSVERSN | "ics" script version | meta.fits.software INHERIT | denotes the INHERIT keyword convention | meta.note;meta.fits INSTRUME | name of instrument | meta.id;instr IS_OFF1 | in-scan offset - SOS to frame 1 | # IS_OFF2 | in-scan offset - SOS to end frame | # JD-END | Julian Day at end | time.end JD-START | Julian Day at start | time.start JDAY | Julian Day of observation | time.epoch LATITUDE | geographic latitude of the observation | pos.earth.lat LIVETIME | exposure time after deadtime correction | time.expo MAGZP | calibrated zero point for image (magnitudes) | arith.zp;phot.calib MAPLAB | label of the map | meta.id;obs.field MISSION | mission name | meta.id;instr.obsty MJD-OBS | modified Julian Day at start | time.start MJDREF | modified Julian Day zero point for times | time.epoch MOONANGL | angle between the observation and the moon | pos.posAng NAXIS | number of axes | phys.dimens;meta.table NAXISn | size of the axis n | phys.size;meta.table.axis NEXTEND | Number of standard extensions | meta.number NOISE | noise value in map | instr.det.noise NORM | normalization factor in "fast fourier transform" | arith.factor;stat.Fourier NUMFRMS | number of frames in scan | meta.number OBJECT | name of observed object | meta.id;src OBJNAME | IAU name of observed object | meta.id;src OBSERVER | observer who acquired the data | obs.observer OBS_ID | unique observation ID | meta.id;obs OBS_MODE | instrumental mode of the observation | meta.code;instr.setup ONTIME | integration time during the observation | time.expo ORDATE | observation reference date | time.epoch ORIENTAT | position angle of image y axis (deg. E of N) | pos.posAng ORIGFILE | original file name | meta.id;meta.file ORIGIN | organization responsible for the data | meta.id;instr.obsty PA_PNT | position angle of the pointing | pos.posAng PCDEC | pointing center declination | pos.eq.dec;obs PCOUNT | parameter count | meta.number PCRA | pointing center R.A. | pos.eq.ra;obs PCi_ja | linear transformation matrix | pos.wcs PIXNAM | "pixphot" processing namelist configuration id | meta.fits.software PLATEID | GSSS plate id | meta.id;instr.plate PLTDECD | Dec (degrees) of plate center | pos.eq.dec.degrees;instr.plate PLTDECM | Dec (arcmin) of plate center | pos.eq.dec.arcmin;instr.plate PLTDECS | Dec (arcsec) of plate center | pos.eq.dec.arcsec;instr.plate PLTDECSN | Dec (sign) of plate center | pos.eq.dec.sign;instr.plate PLTGRADE | plate quality grade | meta.code;instr.plate PLTLABEL | observatory plate label | meta.id;instr.plate PLTRAH | R.A. (hours) of plate center | pos.eq.ra.hours;instr.plate PLTRAM | R.A. (minutes) of plate center | pos.eq.ra.minutes;instr.plate PLTRAS | R.A. (seconds) of plate center | pos.eq.ra.seconds;instr.plate PLTSCALE | plate scale (arcsec per mm) | instr.scale POSITNID | observatory scan position identifier | meta.id;pos,obs.field PROGRAM | the name of the s/w task that created the file | meta.id;meta.fits.software PSCALn | parameter scaling factor axis n | arith.factor PSi_ma | coordinate parameter m (char) | pos.wcs PTYPEn | name of random groups parameter | #meta.id PVi_ma | coordinate parameter m (float) | pos.wcs PZEROn | parameter scaling zero point | arith.zp RA | R.A. of the observation | pos.eq.ra;obs RADECSYS | coordinate reference frame | pos.frame RA_EOS | scan reference R.A. J2000 | pos.eq.ra;obs RA_NOM | nominal R.A. of the observation | pos.eq.ra;obs RA_OBJ | R.A. of the observed object | pos.eq.ra RA_PNT | R.A. of the pointed direction of the instrument | pos.eq.ra;instr RA_SCX | R.A. of the X spacecraft axis | pos.eq.ra;instr RA_SCY | R.A. of the Y spacecraft axis | pos.eq.ra;instr RA_SCZ | R.A. of the Z spacecraft axis | pos.eq.ra;instr RA_SOS | scan reference R.A. J2000 | pos.eq.ra;obs REFERENC | bibliographic reference | meta.bib REGION | GSSS region name | meta.id;instr.plate ROOTNAME | rootname of the file | meta.id;meta.file SATURATE | Data value at which saturation occurs | # SCANDIR | scan direction | # SCANIMG | name of original scan | meta.id;obs SCANNO | nightly scan number | meta.number;obs SCANNUM | identifies scan of the plate | meta.id;instr.plate SCHEDVER | scan scheduled version | meta.code;obs SCRPTFN | script template file name | meta.fits.software SCRPTVER | script template version | meta.fits.software SEESH | seeing shape parameter for image | instr.obsty.site.seeing SEE_EOS | seeing at End of Scan | instr.obsty.site.seeing SEE_SOS | seeing at Start of Scan | instr.obsty.site.seeing SIMPLE | does file conform to the Standard? | meta.code;meta.fits SITELAT | latitude of observatory | pos.earth.lat SITELONG | longitude of observatory | pos.earth.lon SKIPRDOS | number of frames skipped at start of scan | meta.number SKYSIG | point source filtered noise estimate for image | instr.det.noise SKYVAL | modal sky estimate for image | instr.det.noise STRIP_ID | 2MASS tile number | meta.id;obs.field ST_EOS | sidereal time at End of Scan | time.end ST_SOS | sidereal time at Start of Scan | time.start SUNANGLE | angle between the observation and the sun | pos.posAng TBCOLn | beginning column number | meta.id;meta.table.column TDBINn | default histogram bin size for the column | # TDIMn | dimensionality of the array | phys.dimens;meta.table.column TDISPn | display format | meta.code;meta.fits TDMAXn | maximum physical value in the column | stat.max TDMINn | minimum physical value in the column | stat.min TELAPSE | elapsed time of the observation | time.expo TELESCOP | name of telescope | meta.id;instr.tel TELNAME | telescope location (name of site) | instr.obsty.site TELT_EOS | telescope temperature at End of Scan | phys.temperature;instr.tel TELT_SOS | telescope temperature at Start of Scan | phys.temperature;instr.tel TFIELDS | number of columns in the table | meta.number;meta.table.column TFORMn | column data format | meta.code;meta.table.column THEAP | offset to starting data heap address | arith.diff;phys.size;meta.fits TIME-END | time at the end of the observation | time.end TIME-OBS | time at the start of the observation | time.start TIMEDEL | time resolution of data | time.resolution TIMER0 | read1 time | time;instr.setup TIMER1 | read2-read1 time | time;instr.setup TIMER2 | secondary settling time | time;instr.setup TIMEREF | time reference (barycenter/local) | meta.ref;time TIMESYS | time system | meta.ref;time TIMEUNIT | time unit | meta.unit;time TIMEZERO | clock correction | arith.factor;time TIMVERSN | timing system definition | meta.ref;time TITLE | title for the observation or data | meta.id;obs TLMAXn | maximum legal value in the column | stat.max TLMINn | minimum legal value in the column | stat.min TNULLn | value used to indicate undefined table element | meta.code;meta.table TOT-EXPT | total cumulative exposure time | time.expo TOT-IMAG | total number of images | meta.number;obs.image TSCALn | linear data scaling factor | arith.factor TSORTKEY | defines the sort order of a table | # TSTART | start time of observation | time.start TSTOP | end time of observation | time.end TTYPEn | column name | meta.id;meta.table.column TUNITn | column units | meta.unit;meta.table.column TYPE | scan type | meta.code;obs TYPEn | name of random groups parameter | # TZEROn | column scaling zero point | arith.zp;meta.table.column USXREF | 2MASS U-scan X coordinate at image center | # USYREF | 2MASS U-scan Y coordinate at image center | # UT | U.T. time at start | time.start UT_DATE | U.T. date of scan | time.epoch UT_EOS | U.T. at End of Scan | time.end UT_OFF1 | U.T. offset - Start Of Scan to frame 1 | arith.diff;time.start UT_SOS | U.T. at Start of Scan | time.start VEL | center velocity | src.veloc VELCODE | code for center velocity | meta.code;src.veloc VELR | reference velocity | src.veloc WAVEF_P | secondary waveform data file | meta.id;meta.file WCSAXESa | number of axes in WCS description | pos.wcs WDIR_EOS | wind direction at End of Scan | obs.air.wind WDIR_SOS | wind direction at Start of Scan | obs.air.wind WSPD_EOS | wind speed at End of Scan | obs.air.wind WSPD_SOS | wind speed at Start of Scan | obs.air.wind XPIXELSZ | x pixel size | phys.size;instr.pixel XS_OFF1 | x-scan offet - SOS to frame 1 | # XS_OFF2 | x-scan offet - SOS to end frame | # XTENSION | marks beginning of new HDU | meta.note;meta.fits.hdu YPIXELSZ | y pixel size | phys.size;instr.pixel ZD_EOS | zenith distance at End of Scan | pos.az.zd ZD_SOS | zenith distance at Start of Scan | pos.az.zd ZP | zero point calibration | arith.zp;phot.calib ZP_ERR | error in zero point | stat.error;arith.zp;phot.calib --=_1ey860p5kkg0-- From owner-ucd@eso.org Tue May 3 18:22:06 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j43GLsYH000433 for ; Tue, 3 May 2005 18:21:54 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j43GLska000431 for ucd-outgoing; Tue, 3 May 2005 18:21:54 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j43GLmYH000411 for ; Tue, 3 May 2005 18:21:48 +0200 (MEST) Received: from othello.physics.gla.ac.uk (othello.physics.gla.ac.uk [130.209.204.200]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j43GLk73019132 for ; Tue, 3 May 2005 18:21:46 +0200 (CEST) Received: from gw-trusted.physics.gla.ac.uk ([130.209.204.195] helo=[192.168.78.115]) by othello.physics.gla.ac.uk:587 with asmtp (TLS-1.0:RSA_ARCFOUR_SHA:16) (Exim 4.34) id 1DT09T-0004hR-RD for ucd@ivoa.net; Tue, 03 May 2005 17:21:41 +0100 Mime-Version: 1.0 (Apple Message framework v622) In-Reply-To: <20050503164114.gxpb53ye89ygogo4@webmail.sic.rm.cnr.it> References: <1eff2d5b2ed291becf05825cb37fd8e6@astro.gla.ac.uk> <20050503164114.gxpb53ye89ygogo4@webmail.sic.rm.cnr.it> Content-Type: text/plain; charset=US-ASCII; format=flowed Message-Id: Content-Transfer-Encoding: 7bit From: Norman Gray Subject: Re: UCD name documentation Date: Tue, 3 May 2005 17:21:39 +0100 To: ucd@ivoa.net X-Mailer: Apple Mail (2.622) X-PHYSCI-Spam-Score: 0.0 (/) X-PHYSCI-Spam-Report: 0.0/5.0 X-Othello-SMTP: True X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.3.15 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Norman Gray X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Andrea, On 2005 May 3 , at 15.41, Andrea Preite Martinez wrote: > If you think that the appended list (better, an updated version of it) > could be the base for such a tool, I'll do it (the tool, I mean) Thanks -- that's just the thing I was looking for. Will this appear on the UCD pages at some point? If anyone's interested, this came up on a `osxastro' list (OS X for astronomy applications). The thread is `Tiger's Spotlight & FITS files' at . All the best, Norman -- ---------------------------------------------------------------------- Norman Gray : Physics & Astronomy, Glasgow University, UK http://www.astro.gla.ac.uk/users/norman/ : www.starlink.ac.uk From owner-voevent@eso.org Tue May 3 23:10:07 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j43L9qYH029594 for ; Tue, 3 May 2005 23:09:52 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j43L9qUJ029593 for voevent-outgoing; Tue, 3 May 2005 23:09:52 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-voevent@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j43L9mYH029585; Tue, 3 May 2005 23:09:48 +0200 (MEST) Received: from earth.astro.umd.edu (earth.astro.umd.edu [129.2.14.2]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j43L9kXW025175; Tue, 3 May 2005 23:09:46 +0200 (CEST) Received: from [129.2.15.131] (lap31.astro.umd.edu [129.2.15.131]) by earth.astro.umd.edu (Postfix) with ESMTP id 95900109A6; Tue, 3 May 2005 17:09:36 -0400 (EDT) Message-ID: <4277E88B.7030305@gsfc.nasa.gov> Date: Tue, 03 May 2005 17:09:31 -0400 From: Ed Shaya User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.7.6) Gecko/20050319 X-Accept-Language: en-us, en MIME-Version: 1.0 To: "Frederic V. \"Rick\" Hessman" Cc: IVOA List VOEvent , ucd@ivoa.net Subject: Re: New UCDs for VOEvent please References: <32fd4a5efbfd9d3afbbae300411c0379@Astro.physik.Uni-Goettingen.DE> <426FBAC9.2050600@cacr.caltech.edu> <4272824B.7010900@gsfc.nasa.gov> <71e0852515f7c6122fe60632c6efb16d@Astro.physik.Uni-Goettingen.DE> In-Reply-To: <71e0852515f7c6122fe60632c6efb16d@Astro.physik.Uni-Goettingen.DE> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.3.22 X-Virus-Scanned: by amavisd-new Sender: owner-voevent@eso.org Precedence: bulk Reply-To: Ed Shaya X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Fred, Actually, I've been slaving away at an ontology for several months. It is still quite broad and far from complete. But if you are interested and have the facility to examine OWL, then have a look. I am open to any and all comments.: http://archive.astro.umd.edu/ont/ (an svn archive) Ed Frederic V. "Rick" Hessman wrote: > > On 29 Apr 2005, at 8:51 pm, Ed Shaya wrote: > >> But we can also be keeping another eye on the longer time scale >> where we want to be able to put data in machine understandable terms >> so that applications can do the most possible on our behalf. This >> requires something a bit more sophisticated than just a simple class >> hierarchy of terms. An ontology would be more complete but probably >> not even an order of magnitude (factor 10) more than the UCD is >> now. In fact, given the requests and requirements to augment UCDs, >> with time, the UCD will probably grow to the size of an ontology >> anyway. So, it is probably wise to start doing some thinking in >> terms of the formal OWL standard now. What we do with the ontology >> can vary greatly. >> 1. Use it as a string identifier, exactly as UCDs are. The >> advantage is that one can read the Ontology at that point to get >> more context for the meaning of the term. >> 2. Use it as one more model builder for developing schemas. This >> is like UML but more in tune with knowledge/information structures. >> I think this is what Mathew had in mind. >> 3. Use it to test completeness and consistency of terms. This would >> not be on the fly, but rather as one adds new terms one can see >> whether it is clashing with other terms and Venn diagrams let you >> see something about completeness. This then makes it more >> acceptable for groups to be adding terms into their namespace >> without going to the VO heads or the IAU. >> 4. One can use it as the defining structure of all information being >> exchanged. Sounds daring but in fact several other related science >> fields are preparing to do just that, including space physics. >> 5. One can use it to reason out pathways to converting, pipelining, >> and analysing data. It should be possible to automatically find the >> transformation and queries needed to satisfy an arbitrary stated >> goal or request. Our group at UMD has an NASA/AISRP grant to >> figure out the basics of how this might be done using OWL. > > > Ummm.... maybe my googling didn't go quite as far or I'm missing > something: the "ontology" I found was a "low-level" (no - that sounds > too negative - let's say "very fundamental") means of describing > scientific quantities - nothing particularly "astronomical" about > it. If this is as far as anyone has gotten, then I vote for a > mid-term temporary solution - what I've called "VOThings" - which > someone else can turn into a full astronomical ontology in the > future. Thus, > > - Small, multiple, overlapping, incompatible lists within > different schemata will be an unnecessary pain, so we need a minimal > common-ground list. > > - A formal development of a real astronomical ontology will take > many years and we can't wait that long. > > - We should resist the temptation to make VOThings "complete" > since it won't ever be such and we'd waste time in trying. Maybe > having such a terrible name will be a good thing - let's get it over > quickly knowing that some day somebody else will get it right. > > Rick > > ------------------------------------------------------------------------ > ------------------------ > Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE > Universitaets-Sternwarte Tel. +49-551-39-5052 > Geismarlandstr. 11 Fax +49-551-39-5043 > 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman > ------------------------------------------------------------------------ > ------------------------- > MONET: a MOnitoring NEtwork of Telescopes > http://monet.uni-goettingen.de > ------------------------------------------------------------------------ > ------------------------- > > From owner-ucd@eso.org Fri May 6 12:15:20 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j46AF2DV024547 for ; Fri, 6 May 2005 12:15:02 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j46AF2hN024545 for ucd-outgoing; Fri, 6 May 2005 12:15:02 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j46AEvDV024534 for ; Fri, 6 May 2005 12:14:57 +0200 (MEST) Received: from alpha.uni-sw.gwdg.de (alpha.uni-sw.gwdg.de [134.76.205.222]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j46AEu73007613 for ; Fri, 6 May 2005 12:14:56 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1DTzr8-000HCH-R2; Fri, 06 May 2005 12:14:50 +0200 In-Reply-To: <011EA67F-8093-408A-A5C5-AF6BC33A70A3@noao.edu> References: <427A7DAB.3010102@cacr.caltech.edu> <011EA67F-8093-408A-A5C5-AF6BC33A70A3@noao.edu> Mime-Version: 1.0 (Apple Message framework v622) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <4cd59db0ee26584cabeaaece611a1fcd@Astro.physik.Uni-Goettingen.DE> Content-Transfer-Encoding: 7bit Cc: ucd@ivoa.net, voevent-core@us-vo.org From: "Frederic V. \"Rick\" Hessman" Subject: Re: [Voevent-core] Draft v0.6, VOThings & UCD usage Date: Fri, 6 May 2005 12:17:02 +0200 To: Rob Seaman X-Mailer: Apple Mail (2.622) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.6.5 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Frederic V. \"Rick\" Hessman" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 > - It seems to me that VOThing is unlikely to be embraced as a name. > Suggestions? Perhaps this facility should exist underneath VOEvent > itself in some fashion. Other VO projects needing access would then > simply reference us in return. Remember: I purposefully used this terrible name to emphasize the need for a VO-wide solution. How about "VOConcept"? It seems that the UCD community will also have to address the usefuless of the present UCD usage: one requires a separate parser to disentagle what "em.X-ray;phot.count;obs.image" is supposed to mean, whereas parsing something like em.X-rayphot.countobs.image would fall out of the normal processing of the XML document with no real additional effort. This is why I've been playing with UCDType and VOThingType in the experimental VOEvent schema (http://monet.uni-sw.gwdg.de/twiki/bin/view/VOEvent/ SchemaTableOfContents). This is a good chance to force our VO colleagues to think a bit more about how different VO projects can be made more compatible (at least) and more useful (we hope) in the near future. I'd like to see VOEvent's and turn into something like ("concept" <--> "VOConcept" = "VOThing") em.opt process.burst phot.flux em.opt.R supernova.Type_Ia NGC 1234 galaxies The whole point of XML, after all, is to do as much as possible in XML, othewise one can stick to old ASCII formats. > - There appears to be no purpose for the "type" attribute of the > VOEvent element. This functionality is encapsulated under the > citations. Comments on section 3.2 would be quite welcome. I think it's a bit tricky that the ultimate purpose of the document is hidden in the cite attributes in a lower-level element. Yes, we can agree what everything is supposed to mean, but you certainly can't call it elegant. And no, I don't really have a better suggestion..... > - Timestamp? I vote for subelement of Curation, not attribute of > VOEvent. Unless I get some immediate support for my suggestion, I assume we keep the original syntax. > - There is no error attribute for a VOTable Param, so there should be > none for VOEvent. I FIRMLY disagree with this. With VOTable, the syntax is designed to describe rows and columns in a table and errors are often kept in separate entries. VOEvent needs to be able to describe a measurement, and I've always told my students that a measurement without an error and some units isn't a measurement. It's artificially cumbersome to force people to use s in order to attach an error by adding another element which is identical with the partner element except for the ".error" appendix on the ucd. > - I think all elements of a packet should be optional. A completely > empty VOEvent should be acceptable, for instance, for testing. It is > not our job to try to limit usage only to sensible packets. The first > thing any subscribing client will do is to perform a reality check on > the semantics of the message *from the point of view of the needs of > the client itself*. If a client driving a robotic telescope receives > a discovery packet with no WhereWhen, it will be a simple matter to > reject it. It would, on the other hand, be a hellaciously complicated > job to try to construct a protocol/language in which no nonsense could > be spoken. (See the Sunday morning talk shows for examples.) I started to say that a packet without a is anonymous, but that's not entirely true: if the packet HAS to have a unique ivo: ID, then there's at least somebody who knows where the message came from. Is this enough? What if your system gets a message with the id "ivo://other/message12345678"? Do you assume that somebody within the IVOA was wise in letting somebody who knows what s/he's doing insert a nearly blank message claiming to have found a optical transient? > - We are relying on STC and RTML (and other stuff like UCD). How > should we mandate (or not) what versions of each standard are > acceptable for a packet conforming to VOEvent vM.n? Should we > constrain the usage to the latest stable version of each dependency at > the time of our own releases? Surely the VO must have run into this > before? When STC and RTML is inserted in the schema, one is forced to specify a particular version. As the schema is updated, the appended schemata can also be updated. A performance issue is implicit here: if extremely fast processing times are required, either your system will have to forget about formal schema-based parsing or probably should force the parser to use local copies of the schemata (e.g. updated regularly from the IVOA). > - I think How should continue to live at the top level (not underneath > Curation). It should, however, typically only correspond to a pointer > to an RMTL document or earlier VOEvent packet. (This is the > equivalent of the familiar "N more" syntax for commanding additional > exposures under a variety of data acquisition systems.) In many > cases, How will be omitted entirely. Hear! Hear! If somethings comes from Raptor or a similarly trustworthy source, for instance, we won't need to have the grimy details in the message. Good practice should dictate, however, that there really should be a useful link (a , for example) which permits one to take a look if needed. Rick ------------------------------------------------------------------------ ------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Universitaets-Sternwarte Tel. +49-551-39-5052 Geismarlandstr. 11 Fax +49-551-39-5043 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman ------------------------------------------------------------------------ ------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.uni-goettingen.de ------------------------------------------------------------------------ ------------------------- From owner-ucd@eso.org Fri May 6 12:39:58 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j46AdjDV027081 for ; Fri, 6 May 2005 12:39:45 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j46Adj7E027080 for ucd-outgoing; Fri, 6 May 2005 12:39:45 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j46AdUDV027061 for ; Fri, 6 May 2005 12:39:31 +0200 (MEST) Received: from apollo.le.ac.uk (ntp2b.le.ac.uk [143.210.16.125]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j46AdTXW004168 for ; Fri, 6 May 2005 12:39:29 +0200 (CEST) Received: from [143.210.36.63] (helo=mail.star.le.ac.uk) by apollo.le.ac.uk with esmtp (Exim 4.44) id 1DU0Ep-0005kh-Gl; Fri, 06 May 2005 11:39:19 +0100 Received: from barbara.star.le.ac.uk (barbara.star.le.ac.uk [143.210.36.88]) by mail.star.le.ac.uk (Postfix) with ESMTP id E4CA2271A03; Fri, 6 May 2005 11:39:10 +0100 (BST) Date: Fri, 6 May 2005 11:37:07 +0100 (BST) From: "Patricio F. Ortiz" To: "Frederic V. \"Rick\" Hessman" Cc: Rob Seaman , , Subject: Re: [Voevent-core] Draft v0.6, VOThings & UCD usage In-Reply-To: <4cd59db0ee26584cabeaaece611a1fcd@Astro.physik.Uni-Goettingen.DE> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-UoL-Id: 9968641ad51498f592f89315acb5c628@1DU0Ep-0005kh-Gl@apollo.le.ac.uk X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.6.5 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Patricio F. Ortiz" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi Frederick, On Fri, 6 May 2005, Frederic V. "Rick" Hessman wrote: > > - It seems to me that VOThing is unlikely to be embraced as a name. > > Suggestions? Perhaps this facility should exist underneath VOEvent > > itself in some fashion. Other VO projects needing access would then > > simply reference us in return. > > Remember: I purposefully used this terrible name to emphasize the need > for a VO-wide solution. How about "VOConcept"? > > It seems that the UCD community will also have to address the usefuless > of the present UCD usage: one requires a separate parser to disentagle > what "em.X-ray;phot.count;obs.image" is supposed to mean, whereas > parsing something like > > em.X-rayphot.countobs.image ucd> > > would fall out of the normal processing of the XML document with no > real additional effort. Possibly, but that makes UCDs tied to a particular representation (XML), which I don't believe should be the way to go. If UCDs are to be used widely, they should remain as independent of the "way to write them" as possible. Some people (include me) would like to use UCDs in a non XML context, and build our own tools. Furthermore, which usages do you have in mind where a piece of software would be required to "understand" the meaning of a UCD? (other than just compare with other UCDs, either completely or partially) Cheers, Patricio --- Patricio F. Ortiz pfo@star.le.ac.uk Department of Physics & Astronomy Phone: +44 (0)116 252 2015 University of Leicester Leicester, LE1 7RH, UK From owner-ucd@eso.org Fri May 6 12:57:34 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j46AvADV028763 for ; Fri, 6 May 2005 12:57:11 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j46AvAOm028761 for ucd-outgoing; Fri, 6 May 2005 12:57:10 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j46Av6DV028755 for ; Fri, 6 May 2005 12:57:06 +0200 (MEST) Received: from alpha.uni-sw.gwdg.de (alpha.uni-sw.gwdg.de [134.76.205.222]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j46Av473008556 for ; Fri, 6 May 2005 12:57:05 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1DU0Vv-000Hcz-KD; Fri, 06 May 2005 12:56:59 +0200 In-Reply-To: References: Mime-Version: 1.0 (Apple Message framework v622) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: Content-Transfer-Encoding: 7bit Cc: , , Rob Seaman From: "Frederic V. \"Rick\" Hessman" Subject: Re: [Voevent-core] Draft v0.6, VOThings & UCD usage Date: Fri, 6 May 2005 12:59:11 +0200 To: "Patricio F. Ortiz" X-Mailer: Apple Mail (2.622) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.6.6 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Frederic V. \"Rick\" Hessman" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 On 6 May 2005, at 12:37 pm, Patricio F. Ortiz wrote: >>> - It seems to me that VOThing is unlikely to be embraced as a name. >>> Suggestions? Perhaps this facility should exist underneath VOEvent >>> itself in some fashion. Other VO projects needing access would then >>> simply reference us in return. >> >> Remember: I purposefully used this terrible name to emphasize the need >> for a VO-wide solution. How about "VOConcept"? >> >> It seems that the UCD community will also have to address the >> usefuless >> of the present UCD usage: one requires a separate parser to disentagle >> what "em.X-ray;phot.count;obs.image" is supposed to mean, whereas >> parsing something like >> >> em.X-rayphot.countobs.image> ucd> >> >> would fall out of the normal processing of the XML document with no >> real additional effort. > > Possibly, but that makes UCDs tied to a particular representation > (XML), > which I don't believe should be the way to go. If UCDs are to be used > widely, they should remain as independent of the "way to write them" > as possible. Some people (include me) would like to use UCDs in a non > XML context, and build our own tools. Furthermore, which usages do you > have in mind where a piece of software would be required to > "understand" > the meaning of a UCD? (other than just compare with other UCDs, either > completely or partially) I don't see any problem: in produing the UCDType (not to be confused with VOTable's "ucdType", which just says what a ucd should look like lexographically), I simply took the official list and put it in a schema enumeration so that it could be checked syntactically. This certainly doesn't preclude someone else using the list for totally different purposes. The whole point of UCD's was, at least as I understood it, that one could use an official label for a concept which a computer could then process. The UCD tags aren't for people - they're for computers. By making the UCD list available within a schema, we can make the list simpler for computers to process. Rick ------------------------------------------------------------------------ ------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Universitaets-Sternwarte Tel. +49-551-39-5052 Geismarlandstr. 11 Fax +49-551-39-5043 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman ------------------------------------------------------------------------ ------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.uni-goettingen.de ------------------------------------------------------------------------ ------------------------- From owner-ucd@eso.org Fri May 6 13:16:14 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j46BG0DV000683 for ; Fri, 6 May 2005 13:16:01 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j46BG0f6000682 for ucd-outgoing; Fri, 6 May 2005 13:16:00 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j46BFvDV000659 for ; Fri, 6 May 2005 13:15:57 +0200 (MEST) Received: from artemis.le.ac.uk (mailsend.le.ac.uk [143.210.4.129]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j46BFtXW005039 for ; Fri, 6 May 2005 13:15:56 +0200 (CEST) Received: from [143.210.36.63] (helo=mail.star.le.ac.uk) by artemis.le.ac.uk with esmtp (Exim 4.44) id 1DU0oA-00051k-2x; Fri, 06 May 2005 12:15:50 +0100 Received: from barbara.star.le.ac.uk (barbara.star.le.ac.uk [143.210.36.88]) by mail.star.le.ac.uk (Postfix) with ESMTP id E4E11271A03; Fri, 6 May 2005 12:15:49 +0100 (BST) Date: Fri, 6 May 2005 12:13:46 +0100 (BST) From: "Patricio F. Ortiz" To: "Frederic V.Rick Hessman" Cc: ucd@ivoa.net Subject: Re: [Voevent-core] Draft v0.6, VOThings & UCD usage In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-UoL-Id: f41c81d3706211017d30c5cb6654600e@1DU0oA-00051k-2x@artemis.le.ac.uk X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.6.6 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Patricio F. Ortiz" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 On Fri, 6 May 2005, Frederic V.Rick Hessman wrote: > On 6 May 2005, at 12:37 pm, Patricio F. Ortiz wrote: > > >>> - It seems to me that VOThing is unlikely to be embraced as a name. > >>> Suggestions? Perhaps this facility should exist underneath VOEvent > >>> itself in some fashion. Other VO projects needing access would then > >>> simply reference us in return. > >> > >> Remember: I purposefully used this terrible name to emphasize the need > >> for a VO-wide solution. How about "VOConcept"? > >> > >> It seems that the UCD community will also have to address the > >> usefuless > >> of the present UCD usage: one requires a separate parser to disentagle > >> what "em.X-ray;phot.count;obs.image" is supposed to mean, whereas > >> parsing something like > >> > >> em.X-rayphot.countobs.image >> ucd> > >> > >> would fall out of the normal processing of the XML document with no > >> real additional effort. > > > > Possibly, but that makes UCDs tied to a particular representation > > (XML), > > which I don't believe should be the way to go. If UCDs are to be used > > widely, they should remain as independent of the "way to write them" > > as possible. Some people (include me) would like to use UCDs in a non > > XML context, and build our own tools. Furthermore, which usages do you > > have in mind where a piece of software would be required to > > "understand" > > the meaning of a UCD? (other than just compare with other UCDs, either > > completely or partially) > > I don't see any problem: in produing the UCDType (not to be confused > with VOTable's "ucdType", which just says what a ucd should look like > lexographically), I simply took the official list and put it in a > schema enumeration so that it could be checked syntactically. This > certainly doesn't preclude someone else using the list for totally > different purposes. Perhaps, I can see it from your point of view. That means that anyone getting an XML document adopting that convention and wanting to use "total" UCDs needs to append these elements into a new element which will look like the original. Non-XML representations will remain as originally proposed, right? > The whole point of UCD's was, at least as I understood it, that one > could use an official label for a concept which a computer could then > process. The UCD tags aren't for people - they're for computers. By > making the UCD list available within a schema, we can make the list > simpler for computers to process. In an ideal world, yes, UCDs should be for computers, but in a few cases the information for a given column is so "cryptic" that a human would get more information from the UCD than from an explanation/column-name combination. Besides, I can think of cases in which users are faced with a choice between a number of "things" (to use that term :-) :-) in which the UCD will play an important role to understand what they are dealing with. Searches launched by users will not always return "precise answers", (eg, a registry query) so one of the discriminating elements may well be the UCD. > Rick Cheers, Patricio --- Patricio F. Ortiz pfo@star.le.ac.uk Department of Physics & Astronomy Phone: +44 (0)116 252 2015 University of Leicester Leicester, LE1 7RH, UK From owner-ucd@eso.org Fri May 6 17:05:42 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j46F5ADV006997 for ; Fri, 6 May 2005 17:05:10 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j46F5Aat006996 for ucd-outgoing; Fri, 6 May 2005 17:05:10 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j46F4xDV006951 for ; Fri, 6 May 2005 17:04:59 +0200 (MEST) Received: from alpha.uni-sw.gwdg.de (alpha.uni-sw.gwdg.de [134.76.205.222]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j46F4v73017898 for ; Fri, 6 May 2005 17:04:57 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1DU4No-000Khl-7W; Fri, 06 May 2005 17:04:52 +0200 In-Reply-To: References: Mime-Version: 1.0 (Apple Message framework v622) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <09edf63bac6eaf3722da225c046d3a4f@Astro.physik.Uni-Goettingen.DE> Content-Transfer-Encoding: 7bit Cc: ucd@ivoa.net From: "Frederic V. \"Rick\" Hessman" Subject: Re: [Voevent-core] Draft v0.6, VOThings & UCD usage Date: Fri, 6 May 2005 17:06:54 +0200 To: "Patricio F. Ortiz" X-Mailer: Apple Mail (2.622) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.6.13 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Frederic V. \"Rick\" Hessman" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 >>>>> - It seems to me that VOThing is unlikely to be embraced as a name. >>>>> Suggestions? Perhaps this facility should exist underneath VOEvent >>>>> itself in some fashion. Other VO projects needing access would >>>>> then >>>>> simply reference us in return. >>>> >>>> Remember: I purposefully used this terrible name to emphasize the >>>> need >>>> for a VO-wide solution. How about "VOConcept"? >>>> >>>> It seems that the UCD community will also have to address the >>>> usefuless >>>> of the present UCD usage: one requires a separate parser to >>>> disentagle >>>> what "em.X-ray;phot.count;obs.image" is supposed to mean, whereas >>>> parsing something like >>>> >>>> em.X-rayphot.countobs.image>>> ucd> >>>> >>>> would fall out of the normal processing of the XML document with no >>>> real additional effort. >>> >>> Possibly, but that makes UCDs tied to a particular representation >>> (XML), >>> which I don't believe should be the way to go. If UCDs are to be used >>> widely, they should remain as independent of the "way to write them" >>> as possible. Some people (include me) would like to use UCDs in a non >>> XML context, and build our own tools. Furthermore, which usages do >>> you >>> have in mind where a piece of software would be required to >>> "understand" >>> the meaning of a UCD? (other than just compare with other UCDs, >>> either >>> completely or partially) >> >> I don't see any problem: in produing the UCDType (not to be confused >> with VOTable's "ucdType", which just says what a ucd should look like >> lexographically), I simply took the official list and put it in a >> schema enumeration so that it could be checked syntactically. This >> certainly doesn't preclude someone else using the list for totally >> different purposes. > > Perhaps, I can see it from your point of view. That means that anyone > getting an XML document adopting that convention and wanting to use > "total" UCDs needs to append these elements into a new element which > will look like the original. I'm not sure what you mean by "total" - "original"? UCD information which gets passed via its XML representation can be turned into any format you want: e.g. em.opt.Rphot.flux... is the same as in a VOTable, and we hope the human at the end only sees "R-band optical flux of 1.234e-4 W/m^2" (or something similarly intelligent) and neither of the above computer representations! > Non-XML representations will remain as originally proposed, right? My point is that UCDs will have a life of their own as an official representation of astronomical quantities and concepts - to be used for whatever purposes people find them useful for - but that their use as a means of communication between computers and between people and computers will be much simpler if there is an official XML representation. The current model of simple string concatenation is a cumbersome one for computers given that everything else is cast in XML. Thus, the creation of an official UCD standard list should be accompanied (not replaced!) by an attempt to make the list XML-enabled. My suggestion of using concatenated elements instead of concatenated UCD content is just one obivous way to achieve this functionality. >> The whole point of UCD's was, at least as I understood it, that one >> could use an official label for a concept which a computer could then >> process. The UCD tags aren't for people - they're for computers. By >> making the UCD list available within a schema, we can make the list >> simpler for computers to process. > > In an ideal world, yes, UCDs should be for computers, but in a few > cases > the information for a given column is so "cryptic" that a human would > get > more information from the UCD than from an explanation/column-name > combination. Besides, I can think of cases in which users are faced > with > a choice between a number of "things" (to use that term :-) :-) in > which > the UCD will play an important role to understand what they are dealing > with. Searches launched by users will not always return "precise > answers", (eg, a registry query) so one of the discriminating elements > may > well be the UCD. Absolutely - the UCD can be the syntactical glue by which the human users are finally able to communicate with the external VO world. All the more reasons to invest (1) in a more useful parallel version of the UCD list (XML) and (2) in extensions to the now still VOTable-ish UCD list (a la but not necessarily exactly like VOThing). Rick ------------------------------------------------------------------------ ------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Universitaets-Sternwarte Tel. +49-551-39-5052 Geismarlandstr. 11 Fax +49-551-39-5043 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman ------------------------------------------------------------------------ ------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.uni-goettingen.de ------------------------------------------------------------------------ ------------------------- From owner-ucd@eso.org Mon May 9 08:06:32 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4964wdw022979 for ; Mon, 9 May 2005 08:04:59 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4964wT7022978 for ucd-outgoing; Mon, 9 May 2005 08:04:58 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4964tdw022968 for ; Mon, 9 May 2005 08:04:55 +0200 (MEST) Received: from head.cfa.harvard.edu (head.cfa.harvard.edu [131.142.41.8]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4964rXW018817 for ; Mon, 9 May 2005 08:04:54 +0200 (CEST) Received: from urania.cfa.harvard.edu (urania [131.142.52.147]) by head.cfa.harvard.edu (d/w) with ESMTP id j4964lAv003001 for ; Mon, 9 May 2005 02:04:47 -0400 (EDT) From: Jonathan McDowell Received: (from jcm@localhost) by urania.cfa.harvard.edu (8.12.8p1/8.12.8) id j4964lFb012041 for ucd@ivoa.net; Mon, 9 May 2005 02:04:47 -0400 (EDT) Date: Mon, 9 May 2005 02:04:47 -0400 (EDT) Message-Id: <200505090604.j4964lFb012041@urania.cfa.harvard.edu> To: ucd@ivoa.net Subject: New UCD list X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.8.42 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Jonathan McDowell X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear Andrea, I've been looking at the new UCD list. I have a question, some comments and a concern. question: I assume that the suggestion I made in Aug 2004 for "phot.flux.beam" should now be handled by "phot.flux;instr.beam" using the new "instr.beam" UCD? comment: I applaud the simplification of phot.color. How are you handling this in the Vizier tables with more than one color? Adding secondary pairs of "em.*" UCDs? comment: The UCD desc for 'phot.count' still includes the comment "count (/s)" even though on Oct 19 you agreed on the feedback form that we drop the "/s". comment: I second Alberto's suggestions on homogenization of things like resolution. comment: However, On attempting to map the WCS keywords with things like arith.1_1, I think this is trying to take UCDs beyond where they should go (something I've been accused of myself!). That's what a UTYPE is for, to map it to a data model. All the components of cdmatrix are the same kind of thing and should have the same ucd. concern: On the comments page I also asked in August-Sept. 2004 for feedback on the following proposed UCDs: em.veloc.radio meta.curation phys.energy-density src.net I'm a bit disappointed that many months later a new list has emerged without none of these being addressed, even with a "well, I don't think this is sensible for a UCD". These were proposed not just for fun, but as things needed for the spectral data model document. I also still think that it would be a good idea if new UCDs were circulated for comment to the UCD WG "board" before the web page was updated, the process still seems a bit opaque and over-centralized. (by the way, the automated emails we get with "A suggestion has been made for a new UCD" would I think be much more useful if the text of the suggestion was included, removing one step in the process, since I have the impression few WG members have been responding to them). Best wishes, Jonathan McDowell From owner-ucd@eso.org Mon May 9 15:46:03 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j49Djkdw001791 for ; Mon, 9 May 2005 15:45:46 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j49Djjnu001790 for ucd-outgoing; Mon, 9 May 2005 15:45:45 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j49DjIdw001645 for ; Mon, 9 May 2005 15:45:18 +0200 (MEST) Received: from othello.physics.gla.ac.uk (othello.physics.gla.ac.uk [130.209.204.200]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j49DjGXW002289 for ; Mon, 9 May 2005 15:45:16 +0200 (CEST) Received: from gw-trusted.physics.gla.ac.uk ([130.209.204.195] helo=[192.168.78.115]) by othello.physics.gla.ac.uk:587 with asmtp (TLS-1.0:RSA_ARCFOUR_SHA:16) (Exim 4.34) id 1DV8ZD-0007xM-NJ; Mon, 09 May 2005 14:45:04 +0100 In-Reply-To: <200505090604.j4964lFb012041@urania.cfa.harvard.edu> References: <200505090604.j4964lFb012041@urania.cfa.harvard.edu> Mime-Version: 1.0 (Apple Message framework v622) Content-Type: text/plain; charset=US-ASCII; format=flowed Message-Id: Content-Transfer-Encoding: 7bit From: Norman Gray Subject: Re: New UCD list Date: Mon, 9 May 2005 14:45:02 +0100 To: ucd@ivoa.net X-Mailer: Apple Mail (2.622) X-PHYSCI-Spam-Score: 0.0 (/) X-PHYSCI-Spam-Report: 0.0/5.0 X-Othello-SMTP: True X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.9.11 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Norman Gray X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Greetings, On 2005 May 9 , at 07.04, Jonathan McDowell wrote: > (by the way, the automated emails we get with "A suggestion has been > made for > a new UCD" would I think be much more useful if the text of the > suggestion > was included, removing one step in the process, since I have the > impression > few WG members have been responding to them). Who is the `we', here? Is this the CDS panel for discussing new UCDs, or the list of folk on the WG, which I take to be approximately coextensive with the list of authors of the UCD1+ proposal? I understood I was still on the WG, though I don't recall any such automated emails. Norman -- ---------------------------------------------------------------------- Norman Gray : Physics & Astronomy, Glasgow University, UK http://www.astro.gla.ac.uk/users/norman/ : www.starlink.ac.uk From owner-ucd@eso.org Mon May 9 17:07:16 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j49F71dw017012 for ; Mon, 9 May 2005 17:07:02 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j49F71E4017011 for ucd-outgoing; Mon, 9 May 2005 17:07:01 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j49F6vdw016981 for ; Mon, 9 May 2005 17:06:58 +0200 (MEST) Received: from smtp1.sic.rm.cnr.it (mailrelay.artov.rm.cnr.it [150.146.129.253]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j49F6uXW005735 for ; Mon, 9 May 2005 17:06:56 +0200 (CEST) Received: (qmail 5630 invoked by uid 508); 9 May 2005 15:06:49 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.84. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.034899 secs); 09 May 2005 15:06:49 -0000 Received: from unknown (HELO localhost) ([10.1.1.2]) (envelope-sender ) by smtp1.sic.rm.cnr.it (qmail-ldap-1.03) with SMTP for ; 9 May 2005 15:06:49 -0000 Received: from eddington.u-strasbg.fr (eddington.u-strasbg.fr [130.79.129.110]) by webmail.sic.rm.cnr.it (Horde) with HTTP for ; Mon, 9 May 2005 17:06:49 +0200 Message-ID: <20050509170649.srzz6v0z3gkgossw@webmail.sic.rm.cnr.it> Date: Mon, 9 May 2005 17:06:49 +0200 From: Andrea Preite Martinez To: ucd@ivoa.net Subject: Re: New UCD list MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1 Content-Disposition: inline Content-Transfer-Encoding: 7bit User-Agent: Internet Messaging Program (IMP) H3 (4.0.1) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.9.13 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Andrea Preite Martinez X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Dear Jonathan, > question: I assume that the suggestion I made in Aug 2004 for "phot.flux.beam" > should now be handled by "phot.flux;instr.beam" using the new "instr.beam" > UCD? You're right, that was the idea. > comment: I applaud the simplification of phot.color. How are you handling > this in the Vizier tables with more than one color? Adding secondary pairs of > "em.*" UCDs? Yes, if U-B and V-K are present, we would simply have phot.color;em.opt.U;em.opt.B phot.color;em.opt.V;em.IR.K > comment: The UCD desc for 'phot.count' still includes the comment "count (/s)" > even though on Oct 19 you agreed on the feedback form that we drop the "/s". Thanks, this will be fixed in version 1.01 of the list. > comment: I second Alberto's suggestions on homogenization of things like > resolution. Yes, I agree. Anyone opposing the following changes ? instr.angRes -> pos.resolution (angular resolution) instr.spect.resolution -> spect.resolution (spectral resolution) > comment: However, On attempting to map the WCS keywords with things like > arith.1_1, I think this is trying to take UCDs beyond where they should > go (something I've been accused of myself!). That's what a UTYPE is for, > to map it to a data model. All the components of cdmatrix are the same > kind of thing and should have the same ucd. I also agree with you. > concern: > > On the comments page I also asked in August-Sept. 2004 for feedback on the > following proposed UCDs: > em.veloc.radio There are several things at stake with this one. You can now describe velocities with the following combinations: For radial velocities derived from a spectrum: spect.veloc -- which can be followed by a word em.* : spect.veloc;em.opt or spect.veloc;em.radio or spect.veloc;em.line.HI ... For other velocities : src.veloc (by the way, the definition is wrong in the list! It should not read "radial velocity", but simply "Velocity"). You first suggested em.veloc.radio to account for the 2 conventions to derive velocities from spectra (optical and radio conventions). If nobody ever applies the optical convention to a radio spectrum (or vice versa), then we can live with spect.veloc;em.opt and spect.veloc;em.radio What do you think? > meta.curation What about having a few specific words to describe the elements of VOResource metadata: meta.entity (or meta.identity and meta.organization) meta.version ... > phys.energy-density Yes, but spelled phys.energyDensity ? > src.net You suggested three words to distinguish total source flux, background flux, and net source flux. I don't feel comfortable with src.net, because net values should be the default... The background could be described by a qualifier, e.g. renaming instr.background to stat.background. "Total" is too general a word. Can you suggest a more specific word to describe source+background? Would this be the same as aperture photometry in the optical (i.e. total flux measured within some radius). > I also still > think that it would be a good idea if new UCDs were circulated for > comment to the UCD WG "board" before the web page was updated, the > process still seems a bit opaque and over-centralized. I think the role of the Kyoto session will also be to formalize the existence of the board. Emails like yours contribute to make the process less opaque! > (by the way, the automated emails we get with "A suggestion has been made for > a new UCD" would I think be much more useful if the text of the suggestion > was included, removing one step in the process, since I have the impression > few WG members have been responding to them). Okay, it can be done! Andrea. ============================================================================== Andrea Preite Martinez andrea@rm.iasf.cnr.it Istituto di Astrofisica Spaziale Tel.:+39.06.4993.4641 Area di Ricerca di Tor Vergata Fax.:+39.06.2066.0188 Via del Fosso del Cavaliere 100 Cell:+39.339.3817355 00133 Roma ============================================================================== From owner-ucd@eso.org Mon May 9 17:38:47 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j49Fcadw022481 for ; Mon, 9 May 2005 17:38:36 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j49Fca8m022480 for ucd-outgoing; Mon, 9 May 2005 17:38:36 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j49FcWdw022475 for ; Mon, 9 May 2005 17:38:32 +0200 (MEST) Received: from head.cfa.harvard.edu (head.cfa.harvard.edu [131.142.41.8]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j49FcUXW007020 for ; Mon, 9 May 2005 17:38:31 +0200 (CEST) Received: from xebec.cfa.harvard.edu (xebec [131.142.52.100]) by head.cfa.harvard.edu (d/w) with ESMTP id j49FcOCi002128; Mon, 9 May 2005 11:38:24 -0400 (EDT) From: Arnold Rots Received: (from arots@localhost) by xebec.cfa.harvard.edu (8.12.8p1/8.12.8) id j49FcOfq024961; Mon, 9 May 2005 11:38:24 -0400 (EDT) Message-Id: <200505091538.j49FcOfq024961@xebec.cfa.harvard.edu> Subject: Re: New UCD list In-Reply-To: <20050509170649.srzz6v0z3gkgossw@webmail.sic.rm.cnr.it> To: Andrea Preite Martinez Date: Mon, 9 May 2005 11:38:24 -0400 (EDT) CC: ucd@ivoa.net X-Mailer: ELM [version 2.4ME+ PL99 (25)] MIME-Version: 1.0 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.9.14 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Arnold Rots X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Andrea Preite Martinez wrote: > ... > You first suggested em.veloc.radio to account for the 2 conventions to > derive velocities from spectra (optical and radio conventions). If > nobody > ever applies the optical convention to a radio spectrum (or vice versa), > then we can live with spect.veloc;em.opt and spect.veloc;em.radio > What do you think? > O yes! The optical definition needs to be (and is) used for plenty of radio observations. Do you distinguish between LSR, geocenter, barycenter, topocenter, Galactic center (to name the most popular ones)? > ... -------------------------------------------------------------------------- Arnold H. Rots Chandra X-ray Science Center Smithsonian Astrophysical Observatory tel: +1 617 496 7701 60 Garden Street, MS 67 fax: +1 617 495 7356 Cambridge, MA 02138 arots@head.cfa.harvard.edu USA http://hea-www.harvard.edu/~arots/ -------------------------------------------------------------------------- From owner-ucd@eso.org Mon May 9 20:42:07 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j49Ifsdw015861 for ; Mon, 9 May 2005 20:41:55 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j49IfsOu015860 for ucd-outgoing; Mon, 9 May 2005 20:41:54 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j49Ifndw015853 for ; Mon, 9 May 2005 20:41:50 +0200 (MEST) Received: from serv1.obs-besancon.fr (serv1.obs-besancon.fr [193.52.185.11]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j49Ifm73013846 for ; Mon, 9 May 2005 20:41:48 +0200 (CEST) Received: from services3.obs-besancon.fr ([193.52.184.204] ident=mail) by serv1.obs-besancon.fr with esmtp (Exim 3.35 #1 (Debian)) id 1DVDBs-00023P-00 for ; Mon, 09 May 2005 20:41:16 +0200 Received: from bd.obs-besancon.fr ([193.52.184.161] helo=obs-besancon.fr) by services3.obs-besancon.fr with esmtp (Exim 3.35 #1 (Debian)) id 1DVDFz-0003Hw-00; Mon, 09 May 2005 20:45:32 +0200 Message-ID: <427FAEB0.1040507@obs-besancon.fr> Date: Mon, 09 May 2005 20:40:48 +0200 From: Bernard Debray User-Agent: Mozilla/5.0 (X11; U; Linux i686; en-US; rv:1.0.2) Gecko/20030208 Netscape/7.02 X-Accept-Language: fr, en MIME-Version: 1.0 To: ucd@ivoa.net CC: modele@obs-besancon.fr Subject: UCDs and optical and near-infrared bandpasses References: <20050502071545.o2qry3nmgtcgok8s@webmail.sic.rm.cnr.it> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-MailScanner: Found to be clean, Found to be clean X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.9.21 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Bernard Debray X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear UCD list members, I apologize if the subject of the remarks below has already been addressed or this turns out eventually to be outside the scope of the UCD field. This is both a remark on the UCD electromagnetic spectrum scheme and a question about the use of UCDs. I have browsed the archive of the UCD mailing list and found only one message, by Patricio Ortiz, already a long time ago (October 2003, http://www.ivoa.net/forum/ucd/0310/0067.htm) that fits this topic and looked quite sound to me. One of the claimed aims of UCDs is interoperability. Therefore, they should serve, for instance, the purpose of comparing magnitudes from different catalogues in given filters. Therefore, one should be able to identify unambiguously through which filter, photometric system, ... a magnitude is supplied in a catalogue or by a simulation tool. In the division of the electromagnetic spectrum in the UCD document, optical and near-infrared subparts of the spectrum where given names which are the ones of filters in the Johnson, ... photometric system, whereas they designate contiguous portions of the electromagnetic spectrum. While Johnson filters do fit in the subparts so defined, this is not always the case for filters from other photometric systems. For instance, the g filter of the SDSS photometric system has an effective wavelength of 482.5 nm but the flux in this band encompasses widely both the em.opt.B and em.opt.V domains. On the other hand, there seems to be,as far as I can see, no UCD which refers to the specification of a photometric system which could complement the UCD for the description of the electromagnetic spectrum subpart. Alternatively, the UCDs for specific filters such as those of SDSS' system, which could become more widespread that Johnson's in the future, could be handed over to particular namespaces. But it then still seems to me that, in order to release ambiguity in the meaning of optical and near-infrared parts of the spectrum, the corresponding UCDs should be named slightly differently, not simply U, B, V, ... Finally, if the desired achievement of identifications of data columns in the purpose of comparaison is beyond the scope of UCDs, should the cross-comparaison process be handed over to VO tools at more sophisticated levels ? Thanks in advance for your remarks and comments. Best regards, Bernard Debray Bernard Debray bernard.debray@obs-besancon.fr Observatoire de Besançon http://www.obs-besancon.fr/ BP 1615 25010 Besançon Cedex France Andrea Preite Martinez wrote: >Dear member of the UCD_wg, > >since last Friday (20050429) an updated list of UCD words is available at: > >http://vizier.u-strasbg.fr/UCD/ucd1p-words.txt > >at the UCD page: > >http://vizier.u-strasbg.fr/UCD/ > >The new list of words has been edited according to the very valuable >comments coming from the community and also thanks to the (almost!) every >day use of them made by Sebastien and myself. > >The most important differences with the previous version (20040823) concern > >- distances and sizes (linear/angular) >- the introduction of a rectangular/cartesian reference frame >- the phot.color section, much simplified >- spelling, abbreviations, syntax ... > > >At the UCD page you can also find un updated version of the UCD_tree >browser(s) >and a new tool, the ucd_builder: > >http://vizier.u-strasbg.fr/UCD/cgi-bin/descr2ucd > >that uses a description in "natural" language to find the relevant >ucd_words, and then tries to build a valid ucd out of them. > >In these two weeks before Kyoto please explore the list, use the tools and >send back comments. >A more "formal" comment page is available to suggest changes in the list of >words at: >http://vizier.u-strasbg.fr/UCD/cgi-bin/comment/ucdComments > >Have fun. >Andrea > > From owner-ucd@eso.org Mon May 9 22:32:17 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j49KW5dw028182 for ; Mon, 9 May 2005 22:32:05 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j49KW5ab028180 for ucd-outgoing; Mon, 9 May 2005 22:32:05 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j49KW1dw028173 for ; Mon, 9 May 2005 22:32:01 +0200 (MEST) Received: from apollo.le.ac.uk (mailsend.le.ac.uk [143.210.16.125]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j49KVvXW017404 for ; Mon, 9 May 2005 22:31:58 +0200 (CEST) Received: from [143.210.36.63] (helo=mail.star.le.ac.uk) by apollo.le.ac.uk with esmtp (Exim 4.44) id 1DVEuq-0001jH-63; Mon, 09 May 2005 21:31:48 +0100 Received: from barbara.star.le.ac.uk (barbara.star.le.ac.uk [143.210.36.88]) by mail.star.le.ac.uk (Postfix) with ESMTP id F1285271A00; Mon, 9 May 2005 21:31:45 +0100 (BST) Date: Mon, 9 May 2005 21:29:14 +0100 (BST) From: "Patricio F. Ortiz" To: Bernard Debray Cc: ucd@ivoa.net, Subject: Re: UCDs and optical and near-infrared bandpasses In-Reply-To: <427FAEB0.1040507@obs-besancon.fr> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=ISO-8859-1 Content-Transfer-Encoding: 8BIT X-UoL-Id: 85de7ab74c5d26c3a8d0c0e35bc78b63@1DVEuq-0001jH-63@apollo.le.ac.uk X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.9.25 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Patricio F. Ortiz" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi Andrea, Bernard, et al, I've been sitting on my hands to see if there was any reaction to the way UCDs are heading, but as I was mentioned in the last post, I feel I can free my hands and re-phrase my concerns again. I fully agree with Bernard's position, which something isn't quite right with the way UCD1+ are heading, particularly in the photometry section, which comprises and will comprise the bulk of the data in astronomy. We should ask ourselves why we want to attach a UCD to a column's metadata, and how we intend to use it. To the first question, the initial answer (pre-historic UCDs :-) was that we wanted to be able to recognize the content of any given column in as accurate a way as possible in order to compare it with others (we had datamining in mind); we wished not to mix apples, pears, oranges or lemmons, so, there would be different UCDs for apples, lemmons and oranges (to follow Roy's way of exemplifying things) :-) Now, we have reached a point in which we're lucky to have one ucd for apples and pears and one for lemmons and oranges (citrics). Perhaps we only have one UCD for fruits.which.grow.on.trees.of.more.than.two.metres.high :-) Which leads us to the second question... How do we intend to use them? Do we want to find "things" using ucds? Sure, 1- I(*) want to find all catalogues containing observations with the gunn g filter (enough of fruits, we're astronomers :-). Perhaps I'd like to compare observations done by different observers? (*) replace I by "user" or "users". 2- Another possibility is that I want to find observations in the optical blue section of the em-spectrum? Fine, I may be just interested in discovering resources rather than comparing on a very accurate level. 3- I want to discover which objects have been observed in the radio regime of the CO emission at 3.whatever mm [go back to normal use of 'I'] As far as I can see, ucd1+ allows us to answer [2] accurately and possibly completely, while [1] and [3] will give us a lot of answers with a low S/N, ie, correct answers combined with irrelevant information (to the person questioning). One of the initial ideas of UCDs (mine at least) was to tag columns accurately (including filter/photometric systems), but having "virtual UCDs", ie, UCDs which will be accessible to those querying, but never (or rarely) attached to columns. Translation tables would take care of interpreting that if I asked for "blue magnitude" I would get Johnsons' B, Stroemgrem, gunn, washington, HST, Sloan, etc, etc. However accurate querying was possible. The problem of UCD1+ is that if I want HST Blue observations I have to weed through all the other systems which were put in the same box!! Somehow I feel as if I went to a supermarket to buy AAA alkaline batteries and I'm told "Ah! batteries, they are all in this box (AAA, AA, C, D, N, etc., alkaline, zn, li, new-tech, etc.), here, help yourself" I don't think I'll go back to buy batteries there again! OK, so what can be done? I'm not just complaining here! :-) UCD1+ have already the broad classification, *I* think we need to add the fine structure, so no information is lost and needs to be re-discovered time after time For instance, S|em.opt.B should be left for a magnitude for which we have no idea how it was measured (old catalogues), while a Johnson's B should be something like S|em.opt.B:phot.jhn.B Yes, the ucd tree will grow again (or we'll have to handle this with UTYPE or some other meta-data element), but the example just given gives an accurate description of the quantity, yet can be used in fuzzy searches. Alternatively, we could have phot.jhn.B by itself as the UCD, but have something like S|em.opt.B -> (S|em.opt.B, phot.jhn.B, phot.HST.B, ....... ) That means that in the context of a query, whenever a tool finds the left term it should look for columns which contain a UCD listed in the right hand side. If no list is associated with a "virtual UCD", exact matches should be performed (which should not prevent us from searching for 'phot.HST' regarding of the filter observed! I've implemented tools like this, that's why I'm voicing this proposition. To finish, I just took a quick look at the 'em.line' section... well, absorption and emission lines exist across the spectrum: Ly-alpha, CIV (QSOs), molecular lines, (CO, H20) in Radio, FeXIV in X, etc. By not leaving room for accurate description with UCDs we are making UCDs less useful as accurate descriptors and discovery tools. I feel more threatened by a lack of accuracy in the description of a column than for a largish set of terms (which only reflects our trade). Cheers, Patricio On Mon, 9 May 2005, Bernard Debray wrote: > Dear UCD list members, > > I apologize if the subject of the remarks below has already been > addressed or this turns out eventually to be outside the scope of the > UCD field. This is both a remark on the UCD electromagnetic spectrum > scheme and a question about the use of UCDs. > > I have browsed the archive of the UCD mailing list and found only one > message, by Patricio Ortiz, already a long time ago (October 2003, > http://www.ivoa.net/forum/ucd/0310/0067.htm) that fits this topic and > looked quite sound to me. > > One of the claimed aims of UCDs is interoperability. Therefore, they > should serve, for instance, the purpose of comparing magnitudes from > different catalogues in given filters. Therefore, one should be able to > identify unambiguously through which filter, photometric system, ... a > magnitude is supplied in a catalogue or by a simulation tool. > > In the division of the electromagnetic spectrum in the UCD document, > optical and near-infrared subparts of the spectrum where given names > which are the ones of filters in the Johnson, ... photometric system, > whereas they designate contiguous portions of the electromagnetic spectrum. > > While Johnson filters do fit in the subparts so defined, this is not > always the case for filters from other photometric systems. For > instance, the g filter of the SDSS photometric system has an effective > wavelength of 482.5 nm but the flux in this band encompasses widely both > the em.opt.B and em.opt.V domains. > On the other hand, there seems to be,as far as I can see, no UCD which > refers to the specification of a photometric system which could > complement the UCD for the description of the electromagnetic spectrum > subpart. > > Alternatively, the UCDs for specific filters such as those of SDSS' > system, which could become more widespread that Johnson's in the future, > could be handed over to particular namespaces. But it then still seems > to me that, in order to release ambiguity in the meaning of optical and > near-infrared parts of the spectrum, the corresponding UCDs should be > named slightly differently, not simply U, B, V, ... > > Finally, if the desired achievement of identifications of data columns > in the purpose of comparaison is beyond the scope of UCDs, should the > cross-comparaison process be handed over to VO tools at more > sophisticated levels ? > > Thanks in advance for your remarks and comments. > > Best regards, > Bernard Debray > > Bernard Debray bernard.debray@obs-besancon.fr > Observatoire de Besançon http://www.obs-besancon.fr/ > BP 1615 > 25010 Besançon Cedex > France > > > Andrea Preite Martinez wrote: > > >Dear member of the UCD_wg, > > > >since last Friday (20050429) an updated list of UCD words is available at: > > > >http://vizier.u-strasbg.fr/UCD/ucd1p-words.txt > > > >at the UCD page: > > > >http://vizier.u-strasbg.fr/UCD/ > > > >The new list of words has been edited according to the very valuable > >comments coming from the community and also thanks to the (almost!) every > >day use of them made by Sebastien and myself. > > > >The most important differences with the previous version (20040823) concern > > > >- distances and sizes (linear/angular) > >- the introduction of a rectangular/cartesian reference frame > >- the phot.color section, much simplified > >- spelling, abbreviations, syntax ... > > > > > >At the UCD page you can also find un updated version of the UCD_tree > >browser(s) > >and a new tool, the ucd_builder: > > > >http://vizier.u-strasbg.fr/UCD/cgi-bin/descr2ucd > > > >that uses a description in "natural" language to find the relevant > >ucd_words, and then tries to build a valid ucd out of them. > > > >In these two weeks before Kyoto please explore the list, use the tools and > >send back comments. > >A more "formal" comment page is available to suggest changes in the list of > >words at: > >http://vizier.u-strasbg.fr/UCD/cgi-bin/comment/ucdComments > > > >Have fun. > >Andrea > > > > > > --- Patricio F. Ortiz pfo@star.le.ac.uk Department of Physics & Astronomy Phone: +44 (0)116 252 2015 University of Leicester Leicester, LE1 7RH, UK From owner-ucd@eso.org Tue May 10 09:53:31 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4A7q01u021948 for ; Tue, 10 May 2005 09:52:00 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4A7q0W2021947 for ucd-outgoing; Tue, 10 May 2005 09:52:00 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4A7pu1u021937 for ; Tue, 10 May 2005 09:51:56 +0200 (MEST) Received: from mailhost.u-strasbg.fr (mailhost.u-strasbg.fr [130.79.200.154]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4A7pt73001605 for ; Tue, 10 May 2005 09:51:55 +0200 (CEST) Received: from vizir.u-strasbg.fr (vizir.u-strasbg.fr [130.79.128.13]) by mailhost.u-strasbg.fr (8.13.1/jtpda-5.5pre1) with ESMTP id j4A7pnel028337 for ; Tue, 10 May 2005 09:51:49 +0200 (CEST) Received: from vizier (localhost [127.0.0.1]) by vizir.u-strasbg.fr (8.11.6+Sun/8.9.1) with ESMTP id j4A7qdE20199; Tue, 10 May 2005 09:52:39 +0200 (MET DST) Message-Id: <200505100752.j4A7qdE20199@vizir.u-strasbg.fr> To: ucd@ivoa.net cc: francois@vizir.u-strasbg.fr Date: Tue, 10 May 2005 09:52:39 +0200 From: Francois Ochsenbein X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-1.6 (mailhost.u-strasbg.fr [130.79.200.154]); Tue, 10 May 2005 09:51:49 +0200 (CEST) X-Antivirus: scanned by sophos at u-strasbg.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.9.47 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Francois Ochsenbein X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi Patricio, et al., This question of accurate/inaccurate description was discussed many times --- and one of the results was the definition of 2 different entities : -- the UCDs which have the role of broad classification -- the "utype" was introduced to fulfil the role of the accurate description -- the "utype" being in principle connected to a data model which gives the necessary level of detail. In the photometric domain, each of the two entities has its role: -- from a ucd: 2 quantities showing the same UCD can be compared at least in a statistical way; -- from a utype: the accurate specification of each filter must be accessible; quantities can then be combined. In practice however the required level of details is frequently not fully known. There is exactly the same problem in the astrometric domain: while UCDs can be used to define the RA and Dec, an accurate definition of these values requires a lot of extra parameters -- have a look at Arnold's Space-Time model and be sure you have specified everything if you want to be accurate... In many practical cases -- e.g. for statistical cross-matching -- a full description is not required, and then the UCDs have their place. --francois ================================================================================ Francois Ochsenbein ------ Observatoire Astronomique de Strasbourg 11, rue de l'Universite F-67000 STRASBOURG Phone: +33-(0)390 24 24 29 Email: francois@astro.u-strasbg.fr (France) Fax: +33-(0)390 24 24 17 ================================================================================ From owner-ucd@eso.org Tue May 10 14:07:15 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4AC6J1u000984 for ; Tue, 10 May 2005 14:06:19 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4AC6Ijc000983 for ucd-outgoing; Tue, 10 May 2005 14:06:18 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4AC6F1u000970 for ; Tue, 10 May 2005 14:06:15 +0200 (MEST) Received: from head.cfa.harvard.edu (head.cfa.harvard.edu [131.142.41.8]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4AC6D73008502 for ; Tue, 10 May 2005 14:06:14 +0200 (CEST) Received: from urania.cfa.harvard.edu (urania [131.142.52.147]) by head.cfa.harvard.edu (d/w) with ESMTP id j4AC67Ci004629 for ; Tue, 10 May 2005 08:06:07 -0400 (EDT) From: Jonathan McDowell Received: (from jcm@localhost) by urania.cfa.harvard.edu (8.12.8p1/8.12.8) id j4AC67oh015174 for ucd@ivoa.net; Tue, 10 May 2005 08:06:07 -0400 (EDT) Date: Tue, 10 May 2005 08:06:07 -0400 (EDT) Message-Id: <200505101206.j4AC67oh015174@urania.cfa.harvard.edu> To: ucd@ivoa.net Subject: How precise should UCDs be? X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.10.7 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Jonathan McDowell X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Francois wrote: > This question of accurate/inaccurate description was discussed > many times --- and one of the results was the definition of 2 > different entities : > -- the UCDs which have the role of broad classification > -- the "utype" was introduced to fulfil the role of the accurate > description -- the "utype" being in principle connected to a > data model which gives the necessary level of detail. My own thoughts on the relation between UCD and utype/DM have evolved a little (although it comes to essentially the same answer as Francois). I believe that the UCD should have a precise and accurate definition, but that when you need metadata, or parameters, i.e. you need to refer to other UCDs, the utype/DM is needed. It's not a question of level of detail or "accurate", it's a question of "complete" - do you need more than one number of value to describe the idea? Thus, flux.photDens.sb and flux.photDens;instr.beam are different physical concepts - subtly different, and we are going to a high level of detail, but it's necessary to do so. But RA2000 and RA1950 are the same basic concept differing only by a parameter. The concept 'RA' and the concept 'equinox' are the two different concepts here: pos.eq.ra (value = 12:26:03.4) and time.equinox (value = 2000.0) and these are related to each other in the context of a coordinate frame (e.g. STC) data model. RA1950 and RA2000 are really the same physical concept simply with different metadata. pos.eq.ra is PRECISELY defined, it's just not COMPLETELY defined without tying it to the STC metadata. In contrast, you can't really say that about "surface brightness" and "flux density per beam", there's no associated metadata to distinguish them. (I guess you could use instr.scale or instr.pixel and tie it to the spatially variable beam size in the second case but I think implicitly using an algorithm to connect two concepts is cheating.) Of course for pragmatic reasons we do break this paradigm for the "phot.*;em.*" UCDs where the "em.IR" is really metadata for the "phot.*" concept. But in general I think this is a good rule of thumb for deciding whether you need a new UCD, or whether you need to relate two different UCDs via a data model. > while UCDs can be used to define the RA and Dec, an accurate > definition of these values requires a lot of extra parameters > -- have a look at Arnold's Space-Time model and be sure you > have specified everything if you want to be accurate... > In many practical cases -- e.g. for statistical cross-matching -- > a full description is not required, and then the UCDs have their > place. The key phrase here is "requires a lot of extra parameters". In some other practical cases, a full description *is* required: so you need the parameters and a data model to relate them to each other. But if the data model is very generic you still need the UCDs to describe precisely what the individual parameters are. This is of course fuzzy, since sometimes - as in parts of STC - the utype implies what the UCD must be. But sometimes the utype describes only the precise relationship between two concepts, and the UCDs describe the precise identity of the concepts - both precise, but doing different jobs. Thus you might use utypes to link a velocity and its standard of rest, but you still need to use UCDs to explain that this is the escape velocity from the star (src.veloc.escape) and not the expansion velocity of the wind (src.veloc.expansion) that you're talking about. If you look at the src.veloc tree I see three different kinds of UCD: Group 1 - different kinds of velocity src.veloc src.veloc.ang (src.veloc means radial velocity, we're missing a way to say "(norm of) 3D space velocity", I suggest src.veloc.space or src.veloc.total) Group 2 - the velocity of what? (distinguishing different physics concepts): src.veloc.dispersion src.veloc.escape src.veloc.expansion src.veloc.microTurb src.veloc.pulsat src.veloc.rotat Group 3 - shortcuts for giving parameter values of the STC frames: src.veloc.cmb src.veloc.lg src.veloc.lsr Do other people see the same distinction I'm seeing here? I suggest that instead of Group 3 we should have pos.frame.cmb, pos.frame.lg, pos.frame.lsr, pos.frame.src and allow combinations like src.veloc;pos.frame.lsr src.veloc.space;pos.frame.lsr to make more clear that the concept that's changing is the frame, not the velocity. - Jonathan From owner-ucd@eso.org Tue May 10 14:59:53 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4ACxe1u009640 for ; Tue, 10 May 2005 14:59:40 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4ACxeGC009639 for ucd-outgoing; Tue, 10 May 2005 14:59:40 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from clyde.hq.eso.org (clyde.hq.eso.org [134.171.45.17]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4ACxR1u009584; Tue, 10 May 2005 14:59:28 +0200 (MEST) Received: from [134.171.10.12] (ma008861.hq.eso.org [134.171.10.12]) (authenticated bits=0) by clyde.hq.eso.org (8.12.8/8.12.8) with ESMTP id j4ACxRfF028969 (version=TLSv1/SSLv3 cipher=RC4-SHA bits=128 verify=NOT); Tue, 10 May 2005 14:59:27 +0200 In-Reply-To: <200505101206.j4AC67oh015174@urania.cfa.harvard.edu> References: <200505101206.j4AC67oh015174@urania.cfa.harvard.edu> Mime-Version: 1.0 (Apple Message framework v622) Content-Type: text/plain; charset=US-ASCII; format=flowed Message-Id: <536c867aa5ebeae2ff9af6b55dc312a5@eso.org> Content-Transfer-Encoding: 7bit Cc: ucd@ivoa.net From: Alberto Micol Subject: Re: How precise should UCDs be? Date: Tue, 10 May 2005 14:59:29 +0200 To: Jonathan McDowell X-Mailer: Apple Mail (2.622) X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Alberto Micol X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 On May 10, 2005, at 14:06, Jonathan McDowell wrote: > > The key phrase here is "requires a lot of extra parameters". In some > other practical cases, a full description *is* required: so you need > the > parameters and a data model to relate them to each other. But if the > data model is very generic you still need the UCDs to describe > precisely > what the individual parameters are. > > This is of course fuzzy, since sometimes - as in parts of STC - the > utype implies what the UCD must be. But sometimes the utype describes > only the precise relationship between two concepts, and the UCDs > describe the precise identity of the concepts - both precise, but > doing different jobs. Thus you might use utypes to > link a velocity and its standard of rest, but you still need to > use UCDs to explain that this is the escape velocity from the > star (src.veloc.escape) and not the expansion velocity of the > wind (src.veloc.expansion) that you're talking about. > [...] > Group 2 > - the velocity of what? (distinguishing different physics concepts): > src.veloc.dispersion > src.veloc.escape > src.veloc.expansion > src.veloc.microTurb > src.veloc.pulsat > src.veloc.rotat > Devil's advocate point of view It looks to me as if you are trying to model a generic astronomical source by using UCDs. Wouldn't that be the role of a "Generic Astronomical Source Data Model" instead? That is, the UCD could be src.veloc leaving to the utype of the GAS-DM to tell which part of the source is being described. Drawing a line between UCDs and UTYPEs is something we have not achieved yet. The fact is that we have never really tried. I have never seen a VOTABLE using both UCDs and UTYPEs; until we see one and we experiment with it I fear we could philosophically talk about it for ages. We need real examples (self-criticism: hence we need some DM :-) ). In my view, precise UCDs means: a pragmatic, though incomplete, approach; an approach that is useful to fill a gap: the absence of a DM. To counter-balance such sentence I can certainly add that on the other hand, we will never have all the DMs we would need. Help! :-) Alberto From owner-ucd@eso.org Tue May 10 15:11:35 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4ADBC1u011901 for ; Tue, 10 May 2005 15:11:13 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4ADBCSN011900 for ucd-outgoing; Tue, 10 May 2005 15:11:12 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4ADB71u011877 for ; Tue, 10 May 2005 15:11:08 +0200 (MEST) Received: from mailhost.u-strasbg.fr (mailhost.u-strasbg.fr [130.79.200.153]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4ADB573011028 for ; Tue, 10 May 2005 15:11:06 +0200 (CEST) Received: from astro.u-strasbg.fr (newb6.u-strasbg.fr [130.79.128.16]) by mailhost.u-strasbg.fr (8.13.1/jtpda-5.5pre1) with ESMTP id j4ADAtLW072772 ; Tue, 10 May 2005 15:10:55 +0200 (CEST) Message-ID: <4280B2DF.400C25E2@astro.u-strasbg.fr> Date: Tue, 10 May 2005 15:10:55 +0200 From: Sebastien Derriere Organization: Observatoire de Strasbourg X-Mailer: Mozilla 4.7 [en] (X11; I; SunOS 5.6 sun4u) X-Accept-Language: en MIME-Version: 1.0 To: Norman Gray CC: ucd@ivoa.net Subject: Re: New UCD list References: <200505090604.j4964lFb012041@urania.cfa.harvard.edu> Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-1.6 (mailhost.u-strasbg.fr [130.79.200.153]); Tue, 10 May 2005 15:10:56 +0200 (CEST) X-Antivirus: scanned by sophos at u-strasbg.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.10.9 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Sebastien Derriere X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Norman Gray wrote: > > > Who is the `we', here? Is this the CDS panel for discussing new UCDs, > or the list of folk on the WG, which I take to be approximately > coextensive with the list of authors of the UCD1+ proposal? I > understood I was still on the WG, though I don't recall any such > automated emails. Hi Norman, You are still on the WG. People who receive these emails are those who explicitly asked to receive automated notifications for additions made on the following page: http://vizier.u-strasbg.fr/UCD/cgi-bin/comment/ucdComments Currently, this means: Sebastien Derriere, Bob Mann, Anita Richards, Jonathan McDowell, Pedro Osuna, Andrea Preite-Martinez, and Nausicaa Delmotte. I can add you if you want. From now on, automated messages should include the explanation of the suggested change (previously you had to check details on the web page). Sebastien. -- _______ / ~ /, Sebastien Derriere mailto:derriere@astro.u-strasbg.fr / ~~~~ // Observatoire de Strasbourg Phone +33 (0) 390 242 444 /______// 11, rue de l'universite Telefax +33 (0) 390 242 417 (______(/ F-67000 Strasbourg France From owner-ucd@eso.org Tue May 10 15:19:17 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4ADJ6kw013295 for ; Tue, 10 May 2005 15:19:06 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4ADJ6wj013293 for ucd-outgoing; Tue, 10 May 2005 15:19:06 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4ADJ1kw013280; Tue, 10 May 2005 15:19:01 +0200 (MEST) Received: from athena.le.ac.uk (athena.le.ac.uk [143.210.16.127]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4ADIx73011381; Tue, 10 May 2005 15:19:00 +0200 (CEST) Received: from [143.210.36.63] (helo=mail.star.le.ac.uk) by athena.le.ac.uk with esmtp (Exim 4.44) id 1DVUdS-0000RQ-Fq; Tue, 10 May 2005 14:18:54 +0100 Received: from barbara.star.le.ac.uk (barbara.star.le.ac.uk [143.210.36.88]) by mail.star.le.ac.uk (Postfix) with ESMTP id 26FF7271A08; Tue, 10 May 2005 14:18:54 +0100 (BST) Date: Tue, 10 May 2005 14:16:19 +0100 (BST) From: "Patricio F. Ortiz" To: Alberto Micol Cc: ucd@ivoa.net Subject: Re: How precise should UCDs be? In-Reply-To: <536c867aa5ebeae2ff9af6b55dc312a5@eso.org> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-UoL-Id: 71f0601656df495020ce566fcf5c5c61@1DVUdS-0000RQ-Fq@athena.le.ac.uk X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.10.11 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Patricio F. Ortiz" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 On Tue, 10 May 2005, Alberto Micol wrote: > On May 10, 2005, at 14:06, Jonathan McDowell wrote: > > The key phrase here is "requires a lot of extra parameters". In some > > other practical cases, a full description *is* required: so you need > > the > > parameters and a data model to relate them to each other. But if the > > data model is very generic you still need the UCDs to describe > > precisely > > what the individual parameters are. > > > > This is of course fuzzy, since sometimes - as in parts of STC - the > > utype implies what the UCD must be. But sometimes the utype describes > > only the precise relationship between two concepts, and the UCDs > > describe the precise identity of the concepts - both precise, but > > doing different jobs. Thus you might use utypes to > > link a velocity and its standard of rest, but you still need to > > use UCDs to explain that this is the escape velocity from the > > star (src.veloc.escape) and not the expansion velocity of the > > wind (src.veloc.expansion) that you're talking about. > > [...] > > Group 2 > > - the velocity of what? (distinguishing different physics concepts): > > src.veloc.dispersion > > src.veloc.escape > > src.veloc.expansion > > src.veloc.microTurb > > src.veloc.pulsat > > src.veloc.rotat > > > > Devil's advocate point of view > > It looks to me as if you are trying to model a generic astronomical > source > by using UCDs. Wouldn't that be the role of a "Generic Astronomical > Source Data Model" > instead? > That is, the UCD could be src.veloc leaving to the utype of the GAS-DM > to tell which part of the source is being described. > > Drawing a line between UCDs and UTYPEs is something we have not > achieved yet. > > The fact is that we have never really tried. I have never seen a VOTABLE > using both UCDs and UTYPEs; until we see one and we experiment with it > I fear we could philosophically talk about it for ages. > We need real examples (self-criticism: hence we need some DM :-) ). > > In my view, precise UCDs means: a pragmatic, though incomplete, > approach; > an approach that is useful to fill a gap: the absence of a DM. > > To counter-balance such sentence I can certainly add that > on the other hand, we will never have all the DMs we would need. > > Help! > :-) > > Alberto Alberto, that's exactly my problem! I've never seen any VOT with both ucds and utype that would allow me to think how to identify quantities which are "kind of equivalent" or "equivalent enough" so the user has a short list to pick what is of his/her interest. Whether that line exists, or how it will be defined is quite important. We have already a number of people (astronomers and non-astronomers) wondering why we bother with UCDs (let alone utype!). I second your position that we need practical examples, not just philosophical discussions on how we should write this or that. In my case, the clash with reality comes when consulting a registry (or the META tables in vizier) trying to retrieve resources of a particular type. Personally if I want to get catalogues with HST blue data, I'd like to get back a list with as little overhead as possible, not five times larger, poluted by all other observations in the blue bands which fall into the same box... again, I haven't seen utype widely used yet. If I could narrow down the search using utype + ucd or utype alone, fine, we can always write a piece of software to perform this task. My complaints last night had to do with the fact that up to this point in time, using only ucd1+ our searches would bring back too much overhead. Cheers, Patricio --- Patricio F. Ortiz pfo@star.le.ac.uk Department of Physics & Astronomy Phone: +44 (0)116 252 2015 University of Leicester Leicester, LE1 7RH, UK From owner-ucd@eso.org Tue May 10 15:21:25 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4ADLCkw013666 for ; Tue, 10 May 2005 15:21:13 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4ADLCcM013665 for ucd-outgoing; Tue, 10 May 2005 15:21:12 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4ADL7kw013651 for ; Tue, 10 May 2005 15:21:07 +0200 (MEST) Received: from eso.org (pc003499.hq.eso.org [134.171.40.117]) by serapis.hq.eso.org (8.11.7+Sun/8.11.7) with ESMTP id j4ADL7D24256 for ; Tue, 10 May 2005 15:21:07 +0200 (MEST) Message-ID: <4280B544.2010503@eso.org> Date: Tue, 10 May 2005 15:21:08 +0200 From: Markus Dolensky Organization: European Southern Observatory User-Agent: Mozilla/5.0 (X11; U; Linux i686; en-US; rv:1.4) Gecko/20030624 Netscape/7.1 X-Accept-Language: en, de-AT MIME-Version: 1.0 To: ucd@ivoa.net Subject: Re: How precise should UCDs be? References: <200505101206.j4AC67oh015174@urania.cfa.harvard.edu> <536c867aa5ebeae2ff9af6b55dc312a5@eso.org> In-Reply-To: <536c867aa5ebeae2ff9af6b55dc312a5@eso.org> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Markus Dolensky X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Alberto Micol wrote: > I have never seen a VOTABLE using both UCDs and UTYPEs; Alberto, Here you are: http://www.ivoa.net/internal/IVOA/IvoaDAL/ssample20041021.xml The lack of examples is due to the fact that the utype attribute is new to version 1.1 of VOTable, but more importantly that we are just starting to write services that produce data model compliant data (chicken & egg thing). BEWARE: Above example is obsolete as far as the used data model is concerned, but it should be a valid VOTabled doc nonetheless. - Markus From owner-ucd@eso.org Tue May 10 20:58:03 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4AIvnXa002300 for ; Tue, 10 May 2005 20:57:49 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4AIvnra002299 for ucd-outgoing; Tue, 10 May 2005 20:57:49 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4AIviXa002286 for ; Tue, 10 May 2005 20:57:45 +0200 (MEST) Received: from serv1.obs-besancon.fr (serv1.obs-besancon.fr [193.52.185.11]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4AIvhXW021858 for ; Tue, 10 May 2005 20:57:43 +0200 (CEST) Received: from services3.obs-besancon.fr ([193.52.184.204] ident=mail) by serv1.obs-besancon.fr with esmtp (Exim 3.35 #1 (Debian)) id 1DVZuh-0005G5-00 for ; Tue, 10 May 2005 20:57:03 +0200 Received: from bd.obs-besancon.fr ([193.52.184.161] helo=obs-besancon.fr) by services3.obs-besancon.fr with esmtp (Exim 3.35 #1 (Debian)) id 1DVZz1-0002FZ-00 for ; Tue, 10 May 2005 21:01:31 +0200 Message-ID: <428103EB.5030205@obs-besancon.fr> Date: Tue, 10 May 2005 20:56:43 +0200 From: Bernard Debray User-Agent: Mozilla/5.0 (X11; U; Linux i686; en-US; rv:1.0.2) Gecko/20030208 Netscape/7.02 X-Accept-Language: fr, en MIME-Version: 1.0 To: ucd@ivoa.net Subject: Re: How precise should UCDs be? References: <200505101206.j4AC67oh015174@urania.cfa.harvard.edu> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-MailScanner: Found to be clean, Found to be clean X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.10.22 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Bernard Debray X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Dear all, Jonathan McDowell wrote: >Francois Ochsenbein wrote: > >>This question of accurate/inaccurate description was discussed >>many times --- and one of the results was the definition of 2 >>different entities : >>-- the UCDs which have the role of broad classification >>-- the "utype" was introduced to fulfil the role of the accurate >> description -- the "utype" being in principle connected to a >> data model which gives the necessary level of detail. >> >>In the photometric domain, each of the two entities has its role: >>-- from a ucd: 2 quantities showing the same UCD can be compared >> at least in a statistical way; >>-- from a utype: the accurate specification of each filter must be >> accessible; quantities can then be combined. >> In practice however the required level of details is frequently >> not fully known. >> >>There is exactly the same problem in the astrometric domain: >>while UCDs can be used to define the RA and Dec, an accurate >>definition of these values requires a lot of extra parameters >>-- have a look at Arnold's Space-Time model and be sure you >>have specified everything if you want to be accurate... >>In many practical cases -- e.g. for statistical cross-matching -- >>a full description is not required, and then the UCDs have their >>place. >> >>--francois > >My own thoughts on the relation between UCD and utype/DM have evolved a >little (although it comes to essentially the same answer as Francois). I >believe that the UCD should have a precise and accurate definition, but >that when you need metadata, or parameters, i.e. you need to refer to >other UCDs, the utype/DM is needed. It's not a question of level of >detail or "accurate", it's a question of "complete" - do you need >more than one number of value to describe the idea? > >... >But > RA2000 and RA1950 are the same basic concept differing only by a parameter. > The concept 'RA' and the concept 'equinox' are the two different concepts > here: > pos.eq.ra (value = 12:26:03.4) and > time.equinox (value = 2000.0) > >and these are related to each other in the context of a coordinate frame >(e.g. STC) data model. RA1950 and RA2000 are really the same physical >concept simply with different metadata. pos.eq.ra is PRECISELY defined, >it's just not COMPLETELY defined without tying it to the STC metadata. > >... > >Of course for pragmatic reasons we do break this paradigm for >the "phot.*;em.*" UCDs where the "em.IR" is really metadata for the >"phot.*" concept. But in general I think this is a good rule of thumb >for deciding whether you need a new UCD, or whether you need to >relate two different UCDs via a data model. > >>while UCDs can be used to define the RA and Dec, an accurate >>definition of these values requires a lot of extra parameters >>-- have a look at Arnold's Space-Time model and be sure you >>have specified everything if you want to be accurate... >>In many practical cases -- e.g. for statistical cross-matching -- >>a full description is not required, and then the UCDs have their >>place. >> >> >The key phrase here is "requires a lot of extra parameters". In some >other practical cases, a full description *is* required: so you need the >parameters and a data model to relate them to each other. But if the >data model is very generic you still need the UCDs to describe precisely >what the individual parameters are. > >... > - Jonathan > Yes, definitely. If I go back to my particular initial concern about photometric bandpasses, I pointed that the definition of the UCDs for electromagnetic spectrum in the document NoteEMSpectrum-2004052-3.pdf which is still referred in the last version of the UCD1+ Working Draft Document (2005-04-29) is somewhat ambiguous for the optical and near-infrared parts. For example, the note in the table for em.opt.U says "B band" which, I think, for the average astronomer is Johnson B filter bandpass. On the other hand, there is no ucd to define a photometric system. Therefore in this case, the definition is not "precise" in the sense that it can be confusing. On the other hand, I would tend to think that in order to be used in registries, UCDs should allow a more complete description than for being used in statistical cross-matching (e.g. "I need a resource which has g magnitude in the SDSS photometric system for a given part of the sky"). Does that mean this should be envisaged through data modelling as well ? Bernard Debray bernard.debray@obs-besancon.fr Observatoire de Besançon http://www.obs-besancon.fr/ BP 1615 25010 Besançon Cedex France From owner-ucd@eso.org Wed May 11 00:22:03 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4AMLmnt024963 for ; Wed, 11 May 2005 00:21:48 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4AMLmia024962 for ucd-outgoing; Wed, 11 May 2005 00:21:48 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4AMLjnt024954 for ; Wed, 11 May 2005 00:21:45 +0200 (MEST) Received: from head.cfa.harvard.edu (head.cfa.harvard.edu [131.142.41.8]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4AMLh73029373 for ; Wed, 11 May 2005 00:21:44 +0200 (CEST) Received: from urania.cfa.harvard.edu (urania [131.142.52.147]) by head.cfa.harvard.edu (d/w) with ESMTP id j4AMLbCi027684 for ; Tue, 10 May 2005 18:21:37 -0400 (EDT) From: Jonathan McDowell Received: (from jcm@localhost) by urania.cfa.harvard.edu (8.12.8p1/8.12.8) id j4AMLb3d015644 for ucd@ivoa.net; Tue, 10 May 2005 18:21:37 -0400 (EDT) Date: Tue, 10 May 2005 18:21:37 -0400 (EDT) Message-Id: <200505102221.j4AMLb3d015644@urania.cfa.harvard.edu> To: ucd@ivoa.net Subject: Re: New UCD list X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.10.29 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Jonathan McDowell X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Andrea, Just a couple of followups to your reply to me on Monday: - I agree with your spelling change: phys.energyDensity - spec.veloc; em.opt: I agree if the implication of this is agreed to be "optical method for determining velocity" rather than "velocity measured from the optical spectrum". (Following Arnold's point that yes, alas, all methods are used for all kinds of data) - meta.entity etc as "a few specific words to describe VOResource" Yes... although we should be careful to define them in a general way. I'll try and propose some specifics at Kyoto. - I'm not sure "stat.background" is quite right - to me, background is an astronomical/physical rather than statistical concept. Let me be clear about my proposal: the src.* would be secondary words, so you'd write phot.flux;em.IR;src.total I agree src.net should be the default, but maybe it's helpful for clarity in some cases. instr.background seems not right, because the background can be of cosmic rather than instrumental origin. Thanks, Jonathan From owner-ucd@eso.org Wed May 11 15:38:10 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4BDbqnt006857 for ; Wed, 11 May 2005 15:37:53 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4BDbqMx006856 for ucd-outgoing; Wed, 11 May 2005 15:37:52 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4BDbjnt006821 for ; Wed, 11 May 2005 15:37:45 +0200 (MEST) Received: from mailhost.u-strasbg.fr (mailhost.u-strasbg.fr [130.79.200.153]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4BDbh73020676 for ; Wed, 11 May 2005 15:37:43 +0200 (CEST) Received: from astro.u-strasbg.fr (newb6.u-strasbg.fr [130.79.128.16]) by mailhost.u-strasbg.fr (8.13.1/jtpda-5.5pre1) with ESMTP id j4BDbb8m005148 ; Wed, 11 May 2005 15:37:37 +0200 (CEST) Message-ID: <42820AA0.A5821669@astro.u-strasbg.fr> Date: Wed, 11 May 2005 15:37:36 +0200 From: Sebastien Derriere Organization: Observatoire de Strasbourg X-Mailer: Mozilla 4.7 [en] (X11; I; SunOS 5.6 sun4u) X-Accept-Language: en MIME-Version: 1.0 To: ucd@ivoa.net Subject: UCD simple tools Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-1.6 (mailhost.u-strasbg.fr [130.79.200.153]); Wed, 11 May 2005 15:37:38 +0200 (CEST) X-Antivirus: scanned by sophos at u-strasbg.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.11.11 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Sebastien Derriere X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hello, I just released a series of basic tools to ease manipulation of the UCD1+. They are described here, with simple CGI forms: http://cdsweb.u-strasbg.fr/UCD/tools.htx A Web Service access is also available, and documented here: http://cdsweb.u-strasbg.fr/cdsws/ucdClient.gml These tools allow: translate: convert UCD1 into default corresponding UCD1+ explain: get the description of a UCD1+ word/combination validate: check whether a UCD1+ is well-formed upgrade: convert deprecated UCD1+ to a valid expression assign: attempt to find the best UCD1+ corresponding to a plain text description They will be presented to those of you attending the meeting in Kyoto, during the UCD session! Sebastien. -- _______ / ~ /, Sebastien Derriere mailto:derriere@astro.u-strasbg.fr / ~~~~ // Observatoire de Strasbourg Phone +33 (0) 390 242 444 /______// 11, rue de l'universite Telefax +33 (0) 390 242 417 (______(/ F-67000 Strasbourg France From owner-ucd@eso.org Thu May 12 21:09:19 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4CJ8Mq6026155 for ; Thu, 12 May 2005 21:08:22 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4CJ8MWk026154 for ucd-outgoing; Thu, 12 May 2005 21:08:22 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4CJ8Gq6026122 for ; Thu, 12 May 2005 21:08:16 +0200 (MEST) Received: from mailhost.u-strasbg.fr (mailhost.u-strasbg.fr [130.79.200.154]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4CJ8EXW004414 for ; Thu, 12 May 2005 21:08:15 +0200 (CEST) Received: from astro.u-strasbg.fr (newb6.u-strasbg.fr [130.79.128.16]) by mailhost.u-strasbg.fr (8.13.1/jtpda-5.5pre1) with ESMTP id j4CJ83Ar046262 ; Thu, 12 May 2005 21:08:03 +0200 (CEST) Message-ID: <4283A991.2A3EED5F@astro.u-strasbg.fr> Date: Thu, 12 May 2005 21:08:01 +0200 From: Sebastien Derriere Organization: Observatoire de Strasbourg X-Mailer: Mozilla 4.7 [en] (X11; I; SunOS 5.6 sun4u) X-Accept-Language: en MIME-Version: 1.0 To: Arnold Rots CC: ucd@ivoa.net Subject: Re: New UCD list References: <200505091538.j49FcOfq024961@xebec.cfa.harvard.edu> Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-1.6 (mailhost.u-strasbg.fr [130.79.200.154]); Thu, 12 May 2005 21:08:03 +0200 (CEST) X-Antivirus: scanned by sophos at u-strasbg.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.12.22 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Sebastien Derriere X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Arnold Rots wrote: > > Andrea Preite Martinez wrote: > > ... > > You first suggested em.veloc.radio to account for the 2 conventions to > > derive velocities from spectra (optical and radio conventions). If > > nobody > > ever applies the optical convention to a radio spectrum (or vice versa), > > then we can live with spect.veloc;em.opt and spect.veloc;em.radio > > What do you think? > > > > O yes! The optical definition needs to be (and is) used for plenty of > radio observations. Hi, In order to find the relevant UCD, we need an accurate description/ explanation of the quantity we want to describe. My understanding is the following: there are 3 kinds of velocities 1. physical velocities (ratio of a distance and a time) 2. radio "velocity" representing a frequency shift 3. optical "velocity" representing a wavelength shift 2 and 3 have no physical meaning, they only correspond to a physical radial velocity for motions << c (speed of light). The difference is that (2) depends on the rest frequency, while (3) depends on the observing frequency. But (2) seems to be deprecated by the IAU. In the UCD, you have the word "src.veloc" for case (1). - Again, the description of this word should read simply "Velocity", not "Radial velocity" sorry for the confusion. There is also a word "spect.veloc" for so-called velocities derived from a spectrum. We had in mind that it could be complemented by a word indicating what kind of spectra was used, e.g : spect.veloc;em.opt -> radial "velocity" derived from optical spectrum spect.veloc;em.line.HI -> radial "velocity" derived from a shift of the HI line With your input, I understand that we should have two words, for cases (2) and (3), for example: spect.opticalVeloc and spect.radioVeloc , and we could say: "spect.opticalVeloc;em.radio" for a measurement-of-a-frequency-shift-in a-radio-spectrum-expressed-as-a-velocity-with-the-optical-convention ?! My concern with this is that if someone asks the proper UCD for a "radio velocity", the answer could be "spect.opticalVeloc;em.radio" or "spect.radioVeloc", because the description given by the user is ambiguous. > Do you distinguish between LSR, geocenter, barycenter, topocenter, > Galactic center (to name the most popular ones)? There are a few UCD words which describe some reference frames: pos.geocentric pos.heliocentric pos.galactocentric You are allowed to append them to indicate in which frame the velocity was measured: src.veloc;pos.geocentric src.veloc;pos.cartesian.y;pos.galactocentric (to indicate one component of the velocity) In 3 cases where the frame was only used for velocities, some specific words exist, as noted by Jonathan: src.veloc.cmb src.veloc.lsr src.veloc.lg Sebastien. -- _______ / ~ /, Sebastien Derriere mailto:derriere@astro.u-strasbg.fr / ~~~~ // Observatoire de Strasbourg Phone +33 (0) 390 242 444 /______// 11, rue de l'universite Telefax +33 (0) 390 242 417 (______(/ F-67000 Strasbourg France From owner-ucd@eso.org Thu May 12 21:43:40 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4CJhSq6029530 for ; Thu, 12 May 2005 21:43:28 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4CJhS5J029529 for ucd-outgoing; Thu, 12 May 2005 21:43:28 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4CJhOq6029520 for ; Thu, 12 May 2005 21:43:24 +0200 (MEST) Received: from head.cfa.harvard.edu (head.cfa.harvard.edu [131.142.41.8]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4CJhMXW005191 for ; Thu, 12 May 2005 21:43:22 +0200 (CEST) Received: from xebec.cfa.harvard.edu (xebec [131.142.52.100]) by head.cfa.harvard.edu (d/w) with ESMTP id j4CJhGRm000415 for ; Thu, 12 May 2005 15:43:16 -0400 (EDT) From: Arnold Rots Received: (from arots@localhost) by xebec.cfa.harvard.edu (8.12.8p1/8.12.8) id j4CJhEkY024567 for ucd@ivoa.net; Thu, 12 May 2005 15:43:14 -0400 (EDT) Message-Id: <200505121943.j4CJhEkY024567@xebec.cfa.harvard.edu> Subject: Re: New UCD list In-Reply-To: <4283A991.2A3EED5F@astro.u-strasbg.fr> To: ucd@ivoa.net Date: Thu, 12 May 2005 15:43:14 -0400 (EDT) X-Mailer: ELM [version 2.4ME+ PL99 (25)] MIME-Version: 1.0 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.12.22 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Arnold Rots X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 You may want to look the gory detail up in the STC document. I'd much rather tie "radial velocities" to redshift and, yes, they are basically just formalisms, not physical velocities; but your description is not entirely accurate. - Arnold Sebastien Derriere wrote: > Arnold Rots wrote: > > > > Andrea Preite Martinez wrote: > > > ... > > > You first suggested em.veloc.radio to account for the 2 conventions to > > > derive velocities from spectra (optical and radio conventions). If > > > nobody > > > ever applies the optical convention to a radio spectrum (or vice versa), > > > then we can live with spect.veloc;em.opt and spect.veloc;em.radio > > > What do you think? > > > > > > > O yes! The optical definition needs to be (and is) used for plenty of > > radio observations. > > Hi, > > In order to find the relevant UCD, we need an accurate description/ > explanation of the quantity we want to describe. > My understanding is the following: there are 3 kinds of velocities > 1. physical velocities (ratio of a distance and a time) > 2. radio "velocity" representing a frequency shift > 3. optical "velocity" representing a wavelength shift > > 2 and 3 have no physical meaning, they only correspond to a physical > radial > velocity for motions << c (speed of light). The difference is that (2) > depends > on the rest frequency, while (3) depends on the observing frequency. But > (2) > seems to be deprecated by the IAU. > > In the UCD, you have the word "src.veloc" for case (1). - Again, the > description of this word should read simply "Velocity", not "Radial > velocity" > sorry for the confusion. > > There is also a word "spect.veloc" for so-called velocities derived > from a spectrum. We had in mind that it could be complemented by a word > indicating what kind of spectra was used, e.g : > spect.veloc;em.opt -> radial "velocity" derived from optical > spectrum > spect.veloc;em.line.HI -> radial "velocity" derived from a shift of the > HI line > > With your input, I understand that we should have two words, for cases > (2) > and (3), for example: spect.opticalVeloc and spect.radioVeloc , and we > could > say: "spect.opticalVeloc;em.radio" for a > measurement-of-a-frequency-shift-in > a-radio-spectrum-expressed-as-a-velocity-with-the-optical-convention ?! > My concern with this is that if someone asks the proper UCD for a > "radio velocity", > the answer could be "spect.opticalVeloc;em.radio" or "spect.radioVeloc", > because > the description given by the user is ambiguous. > > > > Do you distinguish between LSR, geocenter, barycenter, topocenter, > > Galactic center (to name the most popular ones)? > > There are a few UCD words which describe some reference frames: > pos.geocentric > pos.heliocentric > pos.galactocentric > > You are allowed to append them to indicate in which frame the velocity > was measured: > src.veloc;pos.geocentric > src.veloc;pos.cartesian.y;pos.galactocentric (to indicate one > component of the velocity) > > In 3 cases where the frame was only used for velocities, some specific > words exist, as noted by Jonathan: > src.veloc.cmb > src.veloc.lsr > src.veloc.lg > > Sebastien. > -- > _______ > / ~ /, Sebastien Derriere mailto:derriere@astro.u-strasbg.fr > / ~~~~ // Observatoire de Strasbourg Phone +33 (0) 390 242 444 > /______// 11, rue de l'universite Telefax +33 (0) 390 242 417 > (______(/ F-67000 Strasbourg France > -------------------------------------------------------------------------- Arnold H. Rots Chandra X-ray Science Center Smithsonian Astrophysical Observatory tel: +1 617 496 7701 60 Garden Street, MS 67 fax: +1 617 495 7356 Cambridge, MA 02138 arots@head.cfa.harvard.edu USA http://hea-www.harvard.edu/~arots/ -------------------------------------------------------------------------- From owner-ucd@eso.org Fri May 13 16:33:30 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4DEWtsE000661 for ; Fri, 13 May 2005 16:32:55 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4DEWser000660 for ucd-outgoing; Fri, 13 May 2005 16:32:54 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4DEWnsE000634 for ; Fri, 13 May 2005 16:32:49 +0200 (MEST) Received: from mailhost.u-strasbg.fr (mailhost.u-strasbg.fr [130.79.200.157]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4DEWlXW001133 for ; Fri, 13 May 2005 16:32:48 +0200 (CEST) Received: from astro.u-strasbg.fr (newb6.u-strasbg.fr [130.79.128.16]) by mailhost.u-strasbg.fr (8.13.1/jtpda-5.5pre1) with ESMTP id j4DEWgtx083366 ; Fri, 13 May 2005 16:32:42 +0200 (CEST) Message-ID: <4284BA89.EAC5A4EB@astro.u-strasbg.fr> Date: Fri, 13 May 2005 16:32:41 +0200 From: Sebastien Derriere Organization: Observatoire de Strasbourg X-Mailer: Mozilla 4.7 [en] (X11; I; SunOS 5.6 sun4u) X-Accept-Language: en MIME-Version: 1.0 To: ucd@ivoa.net Subject: Re: New UCD list References: <200505121943.j4CJhEkY024567@xebec.cfa.harvard.edu> Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-1.6 (mailhost.u-strasbg.fr [130.79.200.157]); Fri, 13 May 2005 16:32:42 +0200 (CEST) X-Antivirus: scanned by sophos at u-strasbg.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.13.13 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Sebastien Derriere X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Arnold Rots wrote: > > You may want to look the gory detail up in the STC document. > I'd much rather tie "radial velocities" to redshift and, yes, they are > basically just formalisms, not physical velocities; but your > description is not entirely accurate. Hi, I had looked at the FITS spectral coordinates paper, as this is what Jonathan originally referenced to in his suggestion. See http://pan-starrs.ifa.hawaii.edu/ project/IPP/wcs_paper3_20050126.pdf I read there that there are 4 different quantities: 1. apparent radial velocity 2. "radio" velocity 3. "optical" velocity 4. redshift My last mail was just to suggest that we could have 2 ucd words for quantities 2 and 3 (I suggest spect.radioVeloc and spect.opticalVeloc), instead of the single spect.veloc existing now, which is not accurate enough for some people. I don't pretend we can/need be as accurate as STC with a few UCD words - leave this to specific stc:utypes. At least we must try to describe the basic existing quantities with UCD. Sebastien. -- _______ / ~ /, Sebastien Derriere mailto:derriere@astro.u-strasbg.fr / ~~~~ // Observatoire de Strasbourg Phone +33 (0) 390 242 444 /______// 11, rue de l'universite Telefax +33 (0) 390 242 417 (______(/ F-67000 Strasbourg France From owner-ucd@eso.org Mon May 30 13:04:26 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4UB484L014504 for ; Mon, 30 May 2005 13:04:08 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4UB48Nd014503 for ucd-outgoing; Mon, 30 May 2005 13:04:08 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4UB444L014496 for ; Mon, 30 May 2005 13:04:04 +0200 (MEST) Received: from alpha.uni-sw.gwdg.de (alpha.uni-sw.gwdg.de [134.76.205.222]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4UB43XW012392 for ; Mon, 30 May 2005 13:04:03 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1Dci3p-001TNx-NM for ucd@ivoa.net; Mon, 30 May 2005 13:03:57 +0200 Mime-Version: 1.0 (Apple Message framework v622) Content-Transfer-Encoding: 7bit Message-Id: Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed To: ucd@ivoa.net From: "Frederic V. \"Rick\" Hessman" Subject: T0 : extensions to em, obs, spect, instr Date: Mon, 30 May 2005 13:06:23 +0200 X-Mailer: Apple Mail (2.622) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.30.6 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Frederic V. \"Rick\" Hessman" X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 1. I suggest we rename em from "electromagnetic spectrum" to "emission" and add em.grav-wave (gravitational wave) em.neutrino (neutrino) Alternatively, add phys.grav-wave (gravitational wave) phys.particle (particle emission) phys.particle.cosmic-ray phys.particle.neutrino ...? 2. I suggest we add UCD's for describing calibration observations. Presently, they are few mentions of calibrations at all in the official list: instr.calib (calibration parameter) phot.calib (photometric calibration) and they are sorely needed for things like VOEvent and RTML. It's trivial to say that there's a big different between calibrations (see above) and calibration observations, so new UCD's are needed and it seems the likely candidates would be: obs.calib (calibration observation) obs.calib.dome-flat (dome-flat observation) obs.calib.flux (flux calibration observation) obs.calib.freq (frequency calibration observation) obs.calib.guide-star (guide-star observation, e.g. for intial setup) obs.calib.phot (photometric calibration observation) obs.calib.pos (astrometric calibration observation obs.calib.sky-flat (sky-flat observation) obs.calib.slit-mask (slit-mask calibration observation) obs.calib.spect (spectral type calibration observation) obs.calib.veloc (radial velocity calibration observation, e.g. standard star) obs.calib.wl (wavelength calibration observation) For completeness, one should then also add phot.calib.flux (photometric flux calibration) phot.calib.mag (photometric magnitude calibration) pos.calib (astrometric calibration) spect.calib (spectroscopic calibration) spect.calib.wl (" " in wavelength) spect.calib.freq (" " in frequency) 3. Suggested addition to spect (Spectroscopy) spect.cont (spectral continuum) We already have spect.line. Rick ------------------------------------------------------------------------ ------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Universitaets-Sternwarte Tel. +49-551-39-5052 Geismarlandstr. 11 Fax +49-551-39-5043 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman ------------------------------------------------------------------------ ------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.uni-goettingen.de ------------------------------------------------------------------------ ------------------------- From owner-ucd@eso.org Mon May 30 13:40:07 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4UBdl4L019911 for ; Mon, 30 May 2005 13:39:48 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4UBdleq019910 for ucd-outgoing; Mon, 30 May 2005 13:39:47 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4UBdf4L019895 for ; Mon, 30 May 2005 13:39:41 +0200 (MEST) Received: from alpha.uni-sw.gwdg.de (alpha.uni-sw.gwdg.de [134.76.205.222]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4UBLPXW012824 for ; Mon, 30 May 2005 13:21:25 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1DciKc-001TaL-NM for ucd@ivoa.net; Mon, 30 May 2005 13:21:18 +0200 Mime-Version: 1.0 (Apple Message framework v622) Content-Transfer-Encoding: 7bit Message-Id: <84bb0f6cc51a46b0499a99dc75f16b0a@Astro.physik.Uni-Goettingen.DE> Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed To: ucd@ivoa.net From: "Frederic V. \"Rick\" Hessman" Subject: Txx Date: Mon, 30 May 2005 13:23:44 +0200 X-Mailer: Apple Mail (2.622) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.30.7 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Frederic V. \"Rick\" Hessman" X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Again, because of VOEvent and RTML, I'd like to suggest we include at least event (physical or observational event) event.burst ("sudden" observed change in state) event.chirp (continuous change in frequency) event.discovery (discovery of previously unknown object) event.eclipse (intrinsic eclipse of physically related objects) event.eruption ("sudden" physical change in state resulting in more/less observed emission) event.explosion (physical explosion) event.glitch (discontinuous change in frequency) event.occulation (extrinsic occulation of physically unrelated objects) event.variation (variation in some observable property) event.variation.phot (photometric variation) event.variation.pos (astrometric shift in position) event.variation.spect (spectroscopic variation) If we're going to have solar system UCD's, then it's only fair to have stellar and extragalactic ones: I suggest looking at http://monet.uni-sw.gwdg.de/twiki/bin/view/VOEvent/ UnifiedContentDescriptors were there are unit UCD's like "stars", "ism", "galaxy" (as in milky way), "galaxies", and "cosmology". Yes, we don't have to adopt ALL of them, but it would help to have the basic ones. Rick ------------------------------------------------------------------------ ------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Universitaets-Sternwarte Tel. +49-551-39-5052 Geismarlandstr. 11 Fax +49-551-39-5043 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman ------------------------------------------------------------------------ ------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.uni-goettingen.de ------------------------------------------------------------------------ ------------------------- From owner-ucd@eso.org Tue May 31 15:09:36 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4VD9LVZ015501 for ; Tue, 31 May 2005 15:09:21 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4VD9LGB015500 for ucd-outgoing; Tue, 31 May 2005 15:09:21 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4VD9GVZ015486 for ; Tue, 31 May 2005 15:09:16 +0200 (MEST) Received: from cirse.extra.cea.fr (cirse.extra.cea.fr [132.166.172.102]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4VD9EXW026108 for ; Tue, 31 May 2005 15:09:14 +0200 (CEST) Received: from cincidele.saclay.cea.fr (cincidele.saclay.cea.fr [132.166.192.111]) by cirse.extra.cea.fr (8.13.4/8.13.4/CEAnet-Internet.5.0) with ESMTP id j4VD95lc011371 for ; Tue, 31 May 2005 15:09:05 +0200 (MEST) Received: from pisaure.intra.cea.fr (unverified) by cincidele.saclay.cea.fr (Content Technologies SMTPRS 4.3.17) with ESMTP id ; Tue, 31 May 2005 15:09:05 +0200 Received: from nenuphar.saclay.cea.fr (nenuphar.saclay.cea.fr [132.166.192.7]) by pisaure.intra.cea.fr (8.12.11/8.12.11) with ESMTP id j4VD6XkP009029; Tue, 31 May 2005 15:06:33 +0200 (envelope-from pdidelon@cea.fr) Received: from discovery.saclay.cea.fr (discovery.saclay.cea.fr [132.166.26.121]) by nenuphar.saclay.cea.fr (8.12.10/8.12.10/CEAnet-internes.4.0) with ESMTP id j4VD93mG010790; Tue, 31 May 2005 15:09:03 +0200 (MEST) Received: from cea.fr (sappcj122.extra.cea.fr [132.166.9.122]) by discovery.saclay.cea.fr (8.12.10/jtpda-5.3.2) with ESMTP id j4VD9ae5021763 ; Tue, 31 May 2005 15:09:37 +0200 (MEST) Message-ID: <429C61EF.4020300@cea.fr> Date: Tue, 31 May 2005 15:09:03 +0200 From: Pierre Didelon Organization: CEA User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.4) Gecko/20030624 Netscape/7.1 (ax) X-Accept-Language: en-us, en MIME-Version: 1.0 To: "Frederic V. \"Rick\" Hessman" CC: ucd@ivoa.net Subject: Re: T0 : extensions to em, obs, spect, instr References: In-Reply-To: Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.31.8 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Pierre Didelon X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi, Frederic V. "Rick" Hessman wrote: > 1. I suggest we rename em from "electromagnetic spectrum" to "emission" electromagnetic spectrum can concern absorption! > and add > > em.grav-wave (gravitational wave) > em.neutrino (neutrino) > > Alternatively, add > > phys.grav-wave (gravitational wave) > phys.particle (particle emission) > phys.particle.cosmic-ray > phys.particle.neutrino why not electron, proton, neutron.... UCD must define preferentially concept I suppose, isn't it? Enumerated lists must be handle with other mechanisms! Keyword (<=>UCD) and the corresponding values...Y/N? > ...? > > 2. I suggest we add UCD's for describing calibration observations. > Presently, they are > few mentions of calibrations at all in the official list: > > instr.calib (calibration parameter) > phot.calib (photometric calibration) > > and they are sorely needed for things like VOEvent and RTML. > > It's trivial to say that there's a big different between > calibrations (see above) and calibration > observations, so new UCD's are needed and it seems the likely > candidates would be: > > obs.calib (calibration observation) > obs.calib.dome-flat (dome-flat observation) > obs.calib.flux (flux calibration observation) > obs.calib.freq (frequency calibration observation) > obs.calib.guide-star (guide-star observation, e.g. for > intial setup) > obs.calib.phot (photometric calibration observation) > obs.calib.pos (astrometric calibration observation > obs.calib.sky-flat (sky-flat observation) > obs.calib.slit-mask (slit-mask calibration observation) > obs.calib.spect (spectral type calibration observation) > obs.calib.veloc (radial velocity calibration > observation, e.g. standard star) > obs.calib.wl (wavelength calibration observation) Looks like you are trying to define a data model for observation and data reduction with UCD... which is perhaps not the best way to go? > > For completeness, one should then also add > > phot.calib.flux (photometric flux calibration) > phot.calib.mag (photometric magnitude calibration) > pos.calib (astrometric calibration) > spect.calib (spectroscopic calibration) > spect.calib.wl (" " in wavelength) > spect.calib.freq (" " in frequency) > > 3. Suggested addition to spect (Spectroscopy) > > spect.cont (spectral continuum) I like it (personnaly), but why not then spect.background.... > > We already have spect.line. > > > Rick > > ------------------------------------------------------------------------ > ------------------------ > Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE > Universitaets-Sternwarte Tel. +49-551-39-5052 > Geismarlandstr. 11 Fax +49-551-39-5043 > 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman > ------------------------------------------------------------------------ > ------------------------- > MONET: a MOnitoring NEtwork of Telescopes > http://monet.uni-goettingen.de > ------------------------------------------------------------------------ > ------------------------- > -- Pierre ------------------------------------------------------------------ DIDELON :@: pdidelon_at_cea.fr Phone : 33 (0)1 69 08 58 89 CEA SACLAY - Service d'Astrophysique 91191 Gif-Sur-Yvette Cedex ------------------------------------------------------------------ Aidez les enfants Tibétains : http://www.a-e-t.org/jcparrain.htm ou d'autres : http://www.sosesf.org/ ------------------------------------------------------------------ Seule compte la démarche. Car c'est elle qui dure et non le but qui n'est qu'illusion du voyageur... Saint Exupery - Citadelle ------------------------------------------------------------------ From owner-ucd@eso.org Tue May 31 17:04:35 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4VF4IVZ019605 for ; Tue, 31 May 2005 17:04:18 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4VF4IDr019604 for ucd-outgoing; Tue, 31 May 2005 17:04:18 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4VF4AVZ019576; Tue, 31 May 2005 17:04:10 +0200 (MEST) Received: from alpha.uni-sw.gwdg.de (alpha.uni-sw.gwdg.de [134.76.205.222]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4VF4773005599; Tue, 31 May 2005 17:04:07 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1Dd8Hd-001o0N-HM; Tue, 31 May 2005 17:03:57 +0200 In-Reply-To: <20050531150728.fn26pj7v9fa8okc8@webmail.sic.rm.cnr.it> References: <20050531150728.fn26pj7v9fa8okc8@webmail.sic.rm.cnr.it> Mime-Version: 1.0 (Apple Message framework v622) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <94643280d46f33e5c88952d520f13f55@Astro.physik.Uni-Goettingen.DE> Content-Transfer-Encoding: 7bit Cc: Steve Allen , Ana Ines Gomez de Castro , Pierre Didelon , Marie-Lise Dubernet-Tuckey , Alberto Micol , Sebastien Derriere , Nausicaa Delmotte , Jonathan McDowell , Allan Alasdair , Francois Ochsenbein , Roy Williams , =?ISO-8859-1?Q?Miguel_Cervi=C3=B1o?= , Matteo Guainazzi , Bob Mann , Scott Barthelmy , Rob Seaman , Andrea Preite Martinez , Dick Shaw , ucd@ivoa.net From: "Frederic V. \"Rick\" Hessman" Subject: Re: T0 : extensions to em, obs, spect, instr Date: Tue, 31 May 2005 17:06:22 +0200 To: Pierre Didelon X-Mailer: Apple Mail (2.622) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.31.12 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Frederic V. \"Rick\" Hessman" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 On 31 May 2005, at 3:09 pm, Pierre Didelon wrote: > Frederic V. "Rick" Hessman wrote: > >> 1. I suggest we rename em from "electromagnetic spectrum" to >> "emission" and add >> em.grav-wave (gravitational wave) >> em.neutrino (neutrino) > electromagnetic spectrum can concern absorption! Yes, but if you see anything at all, it's ultimately emission (even if attenuated). Admittedly, the better solution is... >> Alternatively, add >> phys.grav-wave (gravitational wave) >> phys.particle (particle emission) >> phys.particle.cosmic-ray >> phys.particle.neutrino > why not electron, proton, neutron.... If people are detecting them, why not? The whole point of em is to describe by what means we observe something, and photons are only one of many ways. I'm sure my LIGO colleagues would be happy with phys.grav-wave and my HESS/MAGIC friends phys.particle.neutrino. The present UCD isn't complete and we probably won't need phys.particle.axion for a long while, so the (other) missing entries aren't a problem, but right now there are some glaring holes..... > UCD must define preferentially concept I suppose, isn't it? > Enumerated lists must be handle with other mechanisms! > Keyword (<=>UCD) and the corresponding values...Y/N? I'm not sure what you mean.... >> ...? >> 2. I suggest we add UCD's for describing calibration observations. >> Presently, they are >> few mentions of calibrations at all in the official list: >> instr.calib (calibration parameter) >> phot.calib (photometric calibration) >> and they are sorely needed for things like VOEvent and RTML. >> It's trivial to say that there's a big different between >> calibrations (see above) and calibration >> observations, so new UCD's are needed and it seems the likely >> candidates would be: >> obs.calib (calibration observation) >> obs.calib.dome-flat (dome-flat observation) >> obs.calib.flux (flux calibration observation) >> obs.calib.freq (frequency calibration observation) >> obs.calib.guide-star (guide-star observation, e.g. for >> intial setup) >> obs.calib.phot (photometric calibration >> observation) >> obs.calib.pos (astrometric calibration observation >> obs.calib.sky-flat (sky-flat observation) >> obs.calib.slit-mask (slit-mask calibration observation) >> obs.calib.spect (spectral type calibration >> observation) >> obs.calib.veloc (radial velocity calibration >> observation, e.g. standard star) >> obs.calib.wl (wavelength calibration observation) > Looks like you are trying to define a data model for observation > and data reduction with UCD... which is perhaps not the best way to go? Absolutely NOT!!!! I just want to be able to say what something is, just like the original VOTable types who wanted to describe their catalogue entries. There's nothing fundamentally different in a VO sense between a calibration image (say, an obs.calib.phot) and a table entry of the resulting calibration (say, phot.calib). Right now, UCD is mainly (some but not me might say only) useful for tables, which is why it needs to be extended to non-table standard VO uses. A "data model for observation and data reduction" looks very different indeed, though it must ultimately use elements for which the VO has a primitive description. UCD is our VO dictionary and data/observation/reduction models are VO prose or poetry: do you want us to write a VO poem using words no one (i.e. no app) understands? >> For completeness, one should then also add >> phot.calib.flux (photometric flux calibration) >> phot.calib.mag (photometric magnitude calibration) >> pos.calib (astrometric calibration) >> spect.calib (spectroscopic calibration) >> spect.calib.wl (" " in wavelength) >> spect.calib.freq (" " in frequency) >> 3. Suggested addition to spect (Spectroscopy) >> spect.cont (spectral continuum) > I like it (personnaly), but why not then spect.background.... If it's needed, why not? Your favorite VO app should be able to know the difference between a spectral line and a spectral contiinuum and, in the real world, between the spectrum in the background (sky). Again, we have spect.line right now only because there are spectral line catalogues out there but few spectral continuum catalogues. No, I'm not trying to get a VO ontology through the back door: ontologies tell us what the intimate relations between objects are, whereas UCD simply gives us the ability to name things. We're still in the VO Neadertaler age where we've only agreed that "Ugga" means "rock". I'm worrying about how we ultimately want to transmit the knowledge of turning a rock into a spear. I hope that the problem now isn't going to be getting our colleagues to agree that we need a word for "stick".... Rick ------------------------------------------------------------------------ ------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Universitaets-Sternwarte Tel. +49-551-39-5052 Geismarlandstr. 11 Fax +49-551-39-5043 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman ------------------------------------------------------------------------ ------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.uni-goettingen.de ------------------------------------------------------------------------ ------------------------- From owner-ucd@eso.org Wed Jun 1 11:03:21 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51936aJ001817 for ; Wed, 1 Jun 2005 11:03:07 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j51936wc001816 for ucd-outgoing; Wed, 1 Jun 2005 11:03:06 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j5192raJ001759; Wed, 1 Jun 2005 11:02:53 +0200 (MEST) Received: from cirse.extra.cea.fr (cirse.extra.cea.fr [132.166.172.102]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j5192p73017570; Wed, 1 Jun 2005 11:02:51 +0200 (CEST) Received: from cincidele.saclay.cea.fr (cincidele.saclay.cea.fr [132.166.192.111]) by cirse.extra.cea.fr (8.13.4/8.13.4/CEAnet-Internet.5.0) with ESMTP id j5192jYJ025370; Wed, 1 Jun 2005 11:02:45 +0200 (MEST) Received: from pisaure.intra.cea.fr (unverified) by cincidele.saclay.cea.fr (Content Technologies SMTPRS 4.3.17) with ESMTP id ; Wed, 1 Jun 2005 11:02:45 +0200 Received: from nenuphar.saclay.cea.fr (nenuphar.saclay.cea.fr [132.166.192.7]) by pisaure.intra.cea.fr (8.12.11/8.12.11) with ESMTP id j5190Clj027549; Wed, 1 Jun 2005 11:00:12 +0200 (envelope-from pdidelon@cea.fr) Received: from discovery.saclay.cea.fr (discovery.saclay.cea.fr [132.166.26.121]) by nenuphar.saclay.cea.fr (8.12.10/8.12.10/CEAnet-internes.4.0) with ESMTP id j5192imG010027; Wed, 1 Jun 2005 11:02:44 +0200 (MEST) Received: from cea.fr (sappcj122.extra.cea.fr [132.166.9.122]) by discovery.saclay.cea.fr (8.12.10/jtpda-5.3.2) with ESMTP id j5193He5013874 ; Wed, 1 Jun 2005 11:03:17 +0200 (MEST) Message-ID: <429D79B3.3@cea.fr> Date: Wed, 01 Jun 2005 11:02:43 +0200 From: Pierre Didelon Organization: CEA User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.4) Gecko/20030624 Netscape/7.1 (ax) X-Accept-Language: en-us, en MIME-Version: 1.0 To: "Frederic V. \"Rick\" Hessman" CC: ucd@ivoa.net, ucd-sci@ivoa.net Subject: Re: T0 : extensions to em, obs, spect, instr References: <20050531150728.fn26pj7v9fa8okc8@webmail.sic.rm.cnr.it> <94643280d46f33e5c88952d520f13f55@Astro.physik.Uni-Goettingen.DE> In-Reply-To: <94643280d46f33e5c88952d520f13f55@Astro.physik.Uni-Goettingen.DE> Content-Type: text/plain; charset=us-ascii; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.6.1.2 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Pierre Didelon X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi Rick, (apologies for cross posting, i will try to avoid it in the future ;-) ) Frederic V. "Rick" Hessman wrote: > On 31 May 2005, at 3:09 pm, Pierre Didelon wrote: > >> Frederic V. "Rick" Hessman wrote: >> SNIP >> UCD must define preferentially concept I suppose, isn't it? >> Enumerated lists must be handle with other mechanisms! >> Keyword (<=>UCD) and the corresponding values...Y/N? > > > I'm not sure what you mean.... I will try to explain what I mean with two or three examples... if I have time, in an other mail. ;-) It is related with the pb of describing things (not really naming them!?) (for bandpass see http://www.ivoa.net/forum/ucd/0505/0197.htm) and how precise UCD must be (http://www.ivoa.net/forum/ucd/0505/0202.htm). The two mails of P.Ortiz give a clear insight of the basic pb. To make it brief, if we can perhaps admit to have bandpass "names" in UCD vocabulary it become very very difficult to have solar system object names, and certainly inacceptable to have all astronomical object names... I hope :-D This last purpose is handle by name resolvers : NED,SIMBAD... > >>> ...? >>> 2. I suggest we add UCD's for describing calibration observations. >>> Presently, they are >>> few mentions of calibrations at all in the official list: >>> instr.calib (calibration parameter) >>> phot.calib (photometric calibration) >>> and they are sorely needed for things like VOEvent and RTML. >>> It's trivial to say that there's a big different between >>> calibrations (see above) and calibration >>> observations, so new UCD's are needed and it seems the likely >>> candidates would be: >>> obs.calib (calibration observation) >>> obs.calib.dome-flat (dome-flat observation) >>> obs.calib.flux (flux calibration observation) >>> obs.calib.freq (frequency calibration observation) >>> obs.calib.guide-star (guide-star observation, e.g. >>> for intial setup) >>> obs.calib.phot (photometric calibration observation) >>> obs.calib.pos (astrometric calibration observation >>> obs.calib.sky-flat (sky-flat observation) >>> obs.calib.slit-mask (slit-mask calibration observation) >>> obs.calib.spect (spectral type calibration >>> observation) >>> obs.calib.veloc (radial velocity calibration >>> observation, e.g. standard star) >>> obs.calib.wl (wavelength calibration observation) >> >> Looks like you are trying to define a data model for observation >> and data reduction with UCD... which is perhaps not the best way to go? > > > Absolutely NOT!!!! I just want to be able to say what something is, Not only! For example obs.calib.dome-flat is certainly an image (or may be a spectra?) which have been obtained under specific conditions and used in a precise context to derive reduced data. It describe only a "personnal" point of view of the way a piece of data can be used! But take an image obs.calib.sky-flat (sky-flat observation), although its main usage will be calibration nobody can assert that some project can use these data for other purposes, even scientific ones : variability event follow up, historical tracing back, proper motion detection... or whatever else we are not already thinking or aware of. obs.calib.freq or obs.calib.spectcan certainly be better defined with another syntax, and first of all what is the kind of observed data concerned, image, spectra, linelist...? ... > just like the original > VOTable types who wanted to describe their catalogue entries. There's > nothing fundamentally > different in a VO sense between a calibration image (say, an > obs.calib.phot) and a table entry > of the resulting calibration (say, phot.calib). Right now, UCD is > mainly (some but not me might > say only) useful for tables, which is why it needs to be extended to > non-table standard VO uses. Yes but it is not the goal of the SCI-Board, at least from the point of view of the structure, it is only concern by the content, and I am not sure that all the UCD problems can be resolve only by content "handling". Worthwhile for ucd@ivoa.net perhaps not for ucd-sci@ivoa.net. > > A "data model for observation and data reduction" looks very different > indeed, though it must > ultimately use elements for which the VO has a primitive description. > UCD is our VO dictionary But dictionnary of what? All the words in astronomy (so it is related to ontology and semantic I suppose) or a dictionary of concepts, these ones beeing able to "take" values or can be instanciate in more precise description. UCD is only a part (conceptuel one AFAI understand) of a "parameter" description which can be more precisely define by "values" (restricted by enumerated lists, obtained from name resolver....), others "attributes" or even others "parameters". > and data/observation/reduction models are VO prose or poetry: do you > want us to write a VO poem > using words no one (i.e. no app) understands? > >>> For completeness, one should then also add >>> phot.calib.flux (photometric flux calibration) >>> phot.calib.mag (photometric magnitude calibration) >>> pos.calib (astrometric calibration) >>> spect.calib (spectroscopic calibration) >>> spect.calib.wl (" " in wavelength) >>> spect.calib.freq (" " in frequency) >>> 3. Suggested addition to spect (Spectroscopy) >>> spect.cont (spectral continuum) >> >> I like it (personnaly), but why not then spect.background.... > > > If it's needed, why not? Your favorite VO app should be able to know the > difference between a spectral line and a spectral contiinuum and, in the > real world, between the spectrum in the background (sky). Again, we have > spect.line right now only because there are spectral line catalogues > out there but > few spectral continuum catalogues. > > No, I'm not trying to get a VO ontology through the back door: > ontologies tell us > what the intimate relations between objects are, whereas UCD simply > gives us > the ability to name things. Hmmm. Same comments as above concerning concepts vs things. > We're still in the VO Neadertaler age where we've > only agreed that "Ugga" means "rock". I'm worrying about how we > ultimately > want to transmit the knowledge of turning a rock into a spear. I hope > that the problem now isn't going to be getting our colleagues to agree > that we > need a word for "stick".... > > Rick SY PiR From owner-ucd-sci@eso.org Wed Jun 1 13:04:16 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51B4AaJ023853 for ; Wed, 1 Jun 2005 13:04:10 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j51B4ABZ023852 for ucd-sci-outgoing; Wed, 1 Jun 2005 13:04:10 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-sci@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51B46aJ023842; Wed, 1 Jun 2005 13:04:06 +0200 (MEST) Received: from alpha.uni-sw.gwdg.de (alpha.uni-sw.gwdg.de [134.76.205.222]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51B44XW021787; Wed, 1 Jun 2005 13:04:04 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1DdR0x-0022CO-9Z; Wed, 01 Jun 2005 13:03:59 +0200 In-Reply-To: <429D79B3.3@cea.fr> References: <20050531150728.fn26pj7v9fa8okc8@webmail.sic.rm.cnr.it> <94643280d46f33e5c88952d520f13f55@Astro.physik.Uni-Goettingen.DE> <429D79B3.3@cea.fr> Mime-Version: 1.0 (Apple Message framework v622) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <0a75e9e971886f955bcd71d196c35f79@Astro.physik.Uni-Goettingen.DE> Content-Transfer-Encoding: 7bit Cc: ucd@ivoa.net, Roy Williams From: "Frederic V. \"Rick\" Hessman" Subject: Re: T0 : extensions to em, obs, spect, instr Date: Wed, 1 Jun 2005 13:06:24 +0200 To: ucd-sci@ivoa.net X-Mailer: Apple Mail (2.622) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.6.1.5 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 On 1 Jun 2005, at 11:02 am, Pierre Didelon wrote: >>> UCD must define preferentially concept I suppose, isn't it? >>> Enumerated lists must be handle with other mechanisms! >>> Keyword (<=>UCD) and the corresponding values...Y/N? >> I'm not sure what you mean.... > > I will try to explain what I mean with two or three examples... > if I have time, in an other mail. ;-) > It is related with the pb of describing things (not really naming > them!?) > (for bandpass see http://www.ivoa.net/forum/ucd/0505/0197.htm) > and how precise UCD must be > (http://www.ivoa.net/forum/ucd/0505/0202.htm). > The two mails of P.Ortiz give a clear insight of the basic pb. > To make it brief, if we can perhaps admit to have bandpass "names" in > UCD vocabulary > it become very very difficult to have solar system object names, > and certainly inacceptable to have all astronomical object names... I > hope :-D > This last purpose is handle by name resolvers : NED,SIMBAD... Let's leave the solar system out of the way at first. If we just take stellar+extragalactic astronomy, then - of course - NOBODY wants a UCD which says src.class.galaxy.spiral.virgocluster.northern-part.opt.name.NGC12345 What VOEvent DOES needs, however, is something generic like (ignore the actual XML tag names!) This use is ENTIRELY EQUIVALENT in its VO meaning, scope, and usefulness to having a VOTable which contains some entry identified as meaning some physical property. This is totally different from having a DM/ontology which says what it means to have a spiral galaxy or what properties are associated with a spiral galaxy or whether the name makes any sense. Of course UCD isn't a name resolver, but if isn't a concept resolver, what is it? Why are some concepts more equal than others? What we have now is the possibility spiral galaxy and who says what "spiral galaxy" means? Who has to parse a different object where the type is "galaxy, spiral" or "galaxy of type spiral" or "spiralgalaxy" or.... Wouldn't life be so easy if we could just say that there is a UCD "src.class.galaxy.spiral"? To say that UCD should NOT do the first (say that something is a spiral galaxy) but should do the latter (say that a table entry is a radial velocity) means that UCD is only intended to be used for tables and catalogues. If this is the foundation of this list, then please remove me. Yes, we shouldn't throw together a list of random concepts and declare our work done. So, please complain if you don't like my suggestions. But isn't the whole point of ucd-sci to determine what astronomical concepts need to be expressable? >>> Looks like you are trying to define a data model for observation >>> and data reduction with UCD... which is perhaps not the best way to >>> go? >> Absolutely NOT!!!! I just want to be able to say what something is, > Not only! > For example obs.calib.dome-flat is certainly an image (or may be a > spectra?) > which have been obtained under specific conditions and used in a > precise context > to derive reduced data. It describe only a "personnal" point of view > of the way a > piece of data can be used! But the point is that the original purpose of the observation has been expressed. Whether it's an image, a spectrum, or simply a number can be extracted from all the other metadata. If you don't have "obs.calib.dome-flat", then you're left with scanning the FITS header for OBJECT="DOMEFLT", OBJECT="DFLAT", OBJECT="DOMFLAT", OBJECT="FLAT-DOME", .... > But take an image obs.calib.sky-flat (sky-flat observation), although > its main > usage will be calibration nobody can assert that some project can use > these data > for other purposes, even scientific ones : variability event follow > up, historical > tracing back, proper motion detection... or whatever else we are not > already > thinking or aware of. Ah, but if I'm looking for a bright GRB in daytime observations, knowing that the image is an obs.calib.sky-flat makes tremendous difference: it could have been an obs.calib.dome-flat (which wouldn't be of any use)! > obs.calib.freq or obs.calib.spectcan certainly be better defined with > another syntax, > and first of all what is the kind of observed data concerned, image, > spectra, linelist...? Since UCDs can be concatenated, this isn't important: the role of the observation has been named as a concept - the rest comes from the data and metadata. A trivial example of how useful this could be would be in a data pipeline: if all the images had things attached like obs.calib.dome-flat, obs.calib.wl then there would be a universal and trivial method for determining just what the data are, independent of FITS keywords and local systems (e.g. ESO.DET.CCD.PAR.TEMP......). >> just like the original >> VOTable types who wanted to describe their catalogue entries. >> There's nothing fundamentally >> different in a VO sense between a calibration image (say, an >> obs.calib.phot) and a table entry >> of the resulting calibration (say, phot.calib). Right now, UCD is >> mainly (some but not me might >> say only) useful for tables, which is why it needs to be extended to >> non-table standard VO uses. > Yes but it is not the goal of the SCI-Board, at least from the point > of view > of the structure, it is only concern by the content, and I am not sure > that all the UCD problems can be resolve only by content "handling". > Worthwhile for ucd@ivoa.net perhaps not for ucd-sci@ivoa.net. I disagree: the WHOLE point of ucd-sci is to make high-level decisions of what is needed scientifically. Otherwise, what's the "sci" in ucd-sci for? >> A "data model for observation and data reduction" looks very >> different indeed, though it must >> ultimately use elements for which the VO has a primitive description. >> UCD is our VO dictionary > But dictionnary of what? > All the words in astronomy (so it is related to ontology and semantic > I suppose) > or a dictionary of concepts, these ones beeing able to "take" values > or can be > instanciate in more precise description. > UCD is only a part (conceptuel one AFAI understand) of a "parameter" > description > which can be more precisely define by "values" (restricted by > enumerated lists, > obtained from name resolver....), others "attributes" or even others > "parameters". This is a particularly VOTable-ish view of the VO and of the role of UCDs. You want to have instr.bandwidth in order to identify that the number in a table is the instrumental bandwidth. I want to have src.class.galaxy.spiral in order to be able to identify that the VOEvent happened next to a spiral galaxy. Where's the difference? What one calls "values", "attributes" and "parameters" is just a question of semantics. Why do I have to use spiral galaxy rather than src.class.galaxy.spiral but you don't have to use instrumental bandwidth instead of instr.bandwidth? Rick ------------------------------------------------------------------------ ------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Universitaets-Sternwarte Tel. +49-551-39-5052 Geismarlandstr. 11 Fax +49-551-39-5043 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman ------------------------------------------------------------------------ ------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.uni-goettingen.de ------------------------------------------------------------------------ ------------------------- From owner-ucd-sci@eso.org Wed Jun 1 13:45:57 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51BjpaJ001036 for ; Wed, 1 Jun 2005 13:45:51 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j51Bjp2I001035 for ucd-sci-outgoing; Wed, 1 Jun 2005 13:45:51 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-sci@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51BjgaJ001019; Wed, 1 Jun 2005 13:45:43 +0200 (MEST) Received: from artemis.le.ac.uk (mailsend.le.ac.uk [143.210.4.129]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51BjfXW022819; Wed, 1 Jun 2005 13:45:41 +0200 (CEST) Received: from [143.210.36.63] (helo=mail.star.le.ac.uk) by artemis.le.ac.uk with esmtp (Exim 4.44) id 1DdRf6-0005wZ-MG; Wed, 01 Jun 2005 12:45:29 +0100 Received: from barbara.star.le.ac.uk (barbara.star.le.ac.uk [143.210.36.88]) by mail.star.le.ac.uk (Postfix) with ESMTP id F13F7271A05; Wed, 1 Jun 2005 12:45:27 +0100 (BST) Date: Wed, 1 Jun 2005 12:44:33 +0100 (BST) From: "Patricio F. Ortiz" To: "Frederic V. \"Rick\" Hessman" Cc: ucd-sci@ivoa.net, , Roy Williams Subject: Re: T0 : extensions to em, obs, spect, instr In-Reply-To: <0a75e9e971886f955bcd71d196c35f79@Astro.physik.Uni-Goettingen.DE> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-UoL-Id: b1d4ea7a57c3fbadbaf035999a5acb6d@1DdRf6-0005wZ-MG@artemis.le.ac.uk X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.6.1.7 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi Pierre & Frederic, Seems to me that you both have some good points in your arguments. I'll just try to put things in a different light here. As far as I can see it, we are dealing with three (or more) "parallel universes": - table metadata (the raw material we used to develop UCDs) - image metadata - VOevents metadata Looks like the structure suggested by UCDs in the 'table metadata' could fit well into the other two cases. I see no reason not to use it. It's unlikely that elements from one domain could be openly used in the other, eg, adding an object type to a list of objects in a catalogue using its "type-ucd". Maybe someone would like to do so, but it won't happen in the large surveys. Image metadata is something I haven't thought much, but it is true that if one could immediately recognize a dome-flat by looking at just one element on the metadata it would be great! People handling archives would likely be very interested in exploring this domain and propose their set of standardized descriptors (ucd-like or image-ucd). How can I handle it now if I want to find an image (processed with bias subtraction and flat-fielded?) How do I locate the adequate flat fields for a given image? I could've located the object images in an archive by the pointing position, but their accompaning calibration images? I just launched a lot of (to me at least) open questions. Back to the VOevent case, handling a few concepts and attaching them to short descriptors seems to be quite necesary. Quite likely this list will evolve with time (everything does). VOevent seems to require description of an object and perhaps naming, but I see naming as a way to locate the object (at a given time). You will shoot me if I'm wrong, I'm sure :-) but this seems very much like how to build a IAU telegram to notify a supernova in a way which the description elements could be easily recognized and processed by automated agents (and possibly humans :-) Finally, I think Frederic mentioned why we don't have ucds with neutrino or gravity waves observations... well, 6 or 7 years ago there was nearly nothing (tables) in the literature... I agree, they should be there, and as the observation methods are likely to be quite different from night-astronomy, we could think of having em. electromagnetic spectrum gw. gravity wave detection nd. neutrino detection as base sections within the UCD schemes, just as we have at. to denote atomic transitions usually measured in the lab. Cheers, Patricio On Wed, 1 Jun 2005, Frederic V. "Rick" Hessman wrote: > > On 1 Jun 2005, at 11:02 am, Pierre Didelon wrote: > > >>> UCD must define preferentially concept I suppose, isn't it? > >>> Enumerated lists must be handle with other mechanisms! > >>> Keyword (<=>UCD) and the corresponding values...Y/N? > >> I'm not sure what you mean.... > > > > I will try to explain what I mean with two or three examples... > > if I have time, in an other mail. ;-) > > It is related with the pb of describing things (not really naming > > them!?) > > (for bandpass see http://www.ivoa.net/forum/ucd/0505/0197.htm) > > and how precise UCD must be > > (http://www.ivoa.net/forum/ucd/0505/0202.htm). > > The two mails of P.Ortiz give a clear insight of the basic pb. > > To make it brief, if we can perhaps admit to have bandpass "names" in > > UCD vocabulary > > it become very very difficult to have solar system object names, > > and certainly inacceptable to have all astronomical object names... I > > hope :-D > > This last purpose is handle by name resolvers : NED,SIMBAD... > > Let's leave the solar system out of the way at first. If we just take > stellar+extragalactic > astronomy, then - of course - NOBODY wants a UCD which says > > src.class.galaxy.spiral.virgocluster.northern-part.opt.name.NGC12345 > > What VOEvent DOES needs, however, is something generic like (ignore the > actual XML tag names!) > > > > This use is ENTIRELY EQUIVALENT in its VO meaning, scope, and > usefulness to having a VOTable > which contains some entry identified as meaning some physical property. > This is totally different > from having a DM/ontology which says what it means to have a spiral > galaxy or what properties are > associated with a spiral galaxy or whether the name makes any sense. > Of course UCD isn't a name > resolver, but if isn't a concept resolver, what is it? Why are some > concepts more equal than others? > > What we have now is the possibility > > > spiral galaxy > > > and who says what "spiral galaxy" means? Who has to parse a different > object where the type is > "galaxy, spiral" or "galaxy of type spiral" or "spiralgalaxy" or.... > Wouldn't life be so easy if we could just > say that there is a UCD "src.class.galaxy.spiral"? > > To say that UCD should NOT do the first (say that something is a spiral > galaxy) but should do the latter > (say that a table entry is a radial velocity) means that UCD is only > intended to be > used for tables and catalogues. If this is the foundation of this > list, then please remove me. > > Yes, we shouldn't throw together a list of random concepts and declare > our work done. So, please > complain if you don't like my suggestions. But isn't the whole point > of ucd-sci to determine what astronomical > concepts need to be expressable? > > >>> Looks like you are trying to define a data model for observation > >>> and data reduction with UCD... which is perhaps not the best way to > >>> go? > >> Absolutely NOT!!!! I just want to be able to say what something is, > > Not only! > > For example obs.calib.dome-flat is certainly an image (or may be a > > spectra?) > > which have been obtained under specific conditions and used in a > > precise context > > to derive reduced data. It describe only a "personnal" point of view > > of the way a > > piece of data can be used! > > But the point is that the original purpose of the observation has been > expressed. > Whether it's an image, a spectrum, or simply a number can be extracted > from all the > other metadata. If you don't have "obs.calib.dome-flat", then you're > left with scanning > the FITS header for OBJECT="DOMEFLT", OBJECT="DFLAT", OBJECT="DOMFLAT", > OBJECT="FLAT-DOME", .... > > > But take an image obs.calib.sky-flat (sky-flat observation), although > > its main > > usage will be calibration nobody can assert that some project can use > > these data > > for other purposes, even scientific ones : variability event follow > > up, historical > > tracing back, proper motion detection... or whatever else we are not > > already > > thinking or aware of. > > Ah, but if I'm looking for a bright GRB in daytime observations, > knowing that the image > is an obs.calib.sky-flat makes tremendous difference: it could have > been an > obs.calib.dome-flat (which wouldn't be of any use)! > > > obs.calib.freq or obs.calib.spectcan certainly be better defined with > > another syntax, > > and first of all what is the kind of observed data concerned, image, > > spectra, linelist...? > > Since UCDs can be concatenated, this isn't important: the role of the > observation has > been named as a concept - the rest comes from the data and metadata. > > A trivial example of how useful this could be would be in a data > pipeline: if all the images > had things attached like obs.calib.dome-flat, obs.calib.wl then there > would be a universal > and trivial method for determining just what the data are, independent > of FITS keywords > and local systems (e.g. ESO.DET.CCD.PAR.TEMP......). > > >> just like the original > >> VOTable types who wanted to describe their catalogue entries. > >> There's nothing fundamentally > >> different in a VO sense between a calibration image (say, an > >> obs.calib.phot) and a table entry > >> of the resulting calibration (say, phot.calib). Right now, UCD is > >> mainly (some but not me might > >> say only) useful for tables, which is why it needs to be extended to > >> non-table standard VO uses. > > Yes but it is not the goal of the SCI-Board, at least from the point > > of view > > of the structure, it is only concern by the content, and I am not sure > > that all the UCD problems can be resolve only by content "handling". > > Worthwhile for ucd@ivoa.net perhaps not for ucd-sci@ivoa.net. > > I disagree: the WHOLE point of ucd-sci is to make high-level decisions > of what is needed scientifically. > Otherwise, what's the "sci" in ucd-sci for? > > >> A "data model for observation and data reduction" looks very > >> different indeed, though it must > >> ultimately use elements for which the VO has a primitive description. > >> UCD is our VO dictionary > > But dictionnary of what? > > All the words in astronomy (so it is related to ontology and semantic > > I suppose) > > or a dictionary of concepts, these ones beeing able to "take" values > > or can be > > instanciate in more precise description. > > UCD is only a part (conceptuel one AFAI understand) of a "parameter" > > description > > which can be more precisely define by "values" (restricted by > > enumerated lists, > > obtained from name resolver....), others "attributes" or even others > > "parameters". > > This is a particularly VOTable-ish view of the VO and of the role of > UCDs. You want to have > instr.bandwidth in order to identify that the number in a table is the > instrumental bandwidth. I want to > have src.class.galaxy.spiral in order to be able to identify that the > VOEvent happened next to a spiral > galaxy. Where's the difference? What one calls "values", > "attributes" and "parameters" is just > a question of semantics. Why do I have to use > > spiral galaxy > > rather than src.class.galaxy.spiral but you don't have to use > > instrumental bandwidth > > instead of instr.bandwidth? > > Rick > > ------------------------------------------------------------------------ > ------------------------ > Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE > Universitaets-Sternwarte Tel. +49-551-39-5052 > Geismarlandstr. 11 Fax +49-551-39-5043 > 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman > ------------------------------------------------------------------------ > ------------------------- > MONET: a MOnitoring NEtwork of Telescopes > http://monet.uni-goettingen.de > ------------------------------------------------------------------------ > ------------------------- > > --- Patricio F. Ortiz pfo@star.le.ac.uk Department of Physics & Astronomy Phone: +44 (0)116 252 2015 University of Leicester Leicester, LE1 7RH, UK From owner-ucd@eso.org Wed Jun 1 15:57:20 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51DswaJ026827 for ; Wed, 1 Jun 2005 15:54:59 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j51DswhK026825 for ucd-outgoing; Wed, 1 Jun 2005 15:54:58 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51DsiaJ026685; Wed, 1 Jun 2005 15:54:44 +0200 (MEST) Received: from cirse.extra.cea.fr (cirse.extra.cea.fr [132.166.172.102]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51Dsf73026571; Wed, 1 Jun 2005 15:54:42 +0200 (CEST) Received: from cincidele.saclay.cea.fr (cincidele.saclay.cea.fr [132.166.192.111]) by cirse.extra.cea.fr (8.13.4/8.13.4/CEAnet-Internet.5.0) with ESMTP id j51DsahP025645; Wed, 1 Jun 2005 15:54:36 +0200 (MEST) Received: from pisaure.intra.cea.fr (unverified) by cincidele.saclay.cea.fr (Content Technologies SMTPRS 4.3.17) with ESMTP id ; Wed, 1 Jun 2005 15:54:36 +0200 Received: from muguet.saclay.cea.fr (muguet.saclay.cea.fr [132.166.192.6]) by pisaure.intra.cea.fr (8.12.11/8.12.11) with ESMTP id j51Dq2ws020266; Wed, 1 Jun 2005 15:52:02 +0200 (envelope-from pdidelon@cea.fr) Received: from discovery.saclay.cea.fr (discovery.saclay.cea.fr [132.166.26.121]) by muguet.saclay.cea.fr (8.12.10/8.12.10/CEAnet-internes.4.0) with ESMTP id j51DsUwZ001657; Wed, 1 Jun 2005 15:54:30 +0200 (MEST) Received: from cea.fr (sappcj122.extra.cea.fr [132.166.9.122]) by discovery.saclay.cea.fr (8.12.10/jtpda-5.3.2) with ESMTP id j51Dsse5021220 ; Wed, 1 Jun 2005 15:55:03 +0200 (MEST) Message-ID: <429DBE0C.7060905@cea.fr> Date: Wed, 01 Jun 2005 15:54:20 +0200 From: Pierre Didelon Organization: CEA User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.4) Gecko/20030624 Netscape/7.1 (ax) X-Accept-Language: en-us, en MIME-Version: 1.0 To: Hessman@astro.physik.uni-goettingen.de CC: ucd-sci@ivoa.net, Roy Williams , ucd@ivoa.net Subject: Re: T0 : extensions to em, obs, spect, instr References: <20050531150728.fn26pj7v9fa8okc8@webmail.sic.rm.cnr.it> <94643280d46f33e5c88952d520f13f55@Astro.physik.Uni-Goettingen.DE> <429D79B3.3@cea.fr> <0a75e9e971886f955bcd71d196c35f79@Astro.physik.Uni-Goettingen.DE> In-Reply-To: <0a75e9e971886f955bcd71d196c35f79@Astro.physik.Uni-Goettingen.DE> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.6.1.11 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Pierre Didelon X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi, First a precision. It was only my point of view (friendly i assume, at least when writing it) and certainly not "THE" UCD-SCI board pov, and I didn't want to hurt you, just express a (my?) difficulty when defining new UCD (similar to the one we had when trying to define UCD for planetology) which is related to the definition of the "good level of abstraction" to be enoughly high to be widely re-usable but at the same time enoughly precise to be usable at all! Some small comments... only to try to precise "my" pov. Frederic V. "Rick" Hessman wrote: > > On 1 Jun 2005, at 11:02 am, Pierre Didelon wrote: > >>>> UCD must define preferentially concept I suppose, isn't it? >>>> Enumerated lists must be handle with other mechanisms! >>>> Keyword (<=>UCD) and the corresponding values...Y/N? >>> >>> I'm not sure what you mean.... >> >> >> I will try to explain what I mean with two or three examples... >> if I have time, in an other mail. ;-) >> It is related with the pb of describing things (not really naming >> them!?) >> (for bandpass see http://www.ivoa.net/forum/ucd/0505/0197.htm) >> and how precise UCD must be >> (http://www.ivoa.net/forum/ucd/0505/0202.htm). >> The two mails of P.Ortiz give a clear insight of the basic pb. >> To make it brief, if we can perhaps admit to have bandpass "names" in >> UCD vocabulary >> it become very very difficult to have solar system object names, >> and certainly inacceptable to have all astronomical object names... I >> hope :-D >> This last purpose is handle by name resolvers : NED,SIMBAD... > > > Let's leave the solar system out of the way at first. If we just take > stellar+extragalactic > astronomy, then - of course - NOBODY wants a UCD which says > > src.class.galaxy.spiral.virgocluster.northern-part.opt.name.NGC12345 > > What VOEvent DOES needs, however, is something generic like (ignore the > actual XML tag names!) > > > > This use is ENTIRELY EQUIVALENT in its VO meaning, scope, and > usefulness to having a VOTable > which contains some entry identified as meaning some physical property. > This is totally different > from having a DM/ontology which says what it means to have a spiral > galaxy or what properties are > associated with a spiral galaxy or whether the name makes any sense. > Of course UCD isn't a name > resolver, but if isn't a concept resolver, what is it? Why are some > concepts more equal than others? > > What we have now is the possibility > > > spiral galaxy > > > and who says what "spiral galaxy" means? Who has to parse a different > object where the type is > "galaxy, spiral" or "galaxy of type spiral" or "spiralgalaxy" or.... > Wouldn't life be so easy if we could just > say that there is a UCD "src.class.galaxy.spiral"? OK! But do/must UCD be the solution to (all?) natural langage parsing? It seems to be a general pb of enumerated lists and classifications. must UCD integrate all the existing ones of every astro fields? > > To say that UCD should NOT do the first (say that something is a spiral > galaxy) but should do the latter > (say that a table entry is a radial velocity) means that UCD is only > intended to be > used for tables and catalogues. Why? Using already existing terms and definitions we could write as you begin to do galaxy spiral The nice part of this view is that as NGC12345 can be resolved by simbad/ned... galaxy and spiral can be handle by separated services, living their own live and evolutionary track. Unfortunately, it does not resolve "immediatly" the nomenclature and parsing problem... I agree. And may be it is not the good way? Once again... only "my" pov. > If this is the foundation of this > list, then please remove me. Perhaps it's me who must be removed! ;-) > > Yes, we shouldn't throw together a list of random concepts and declare > our work done. So, please > complain if you don't like my suggestions. > But isn't the whole point > of ucd-sci to determine what astronomical > concepts need to be expressable? > >>>> Looks like you are trying to define a data model for observation >>>> and data reduction with UCD... which is perhaps not the best way to >>>> go? >>> >>> Absolutely NOT!!!! I just want to be able to say what something is, >> >> Not only! >> For example obs.calib.dome-flat is certainly an image (or may be a >> spectra?) >> which have been obtained under specific conditions and used in a >> precise context >> to derive reduced data. It describe only a "personnal" point of view >> of the way a >> piece of data can be used! > > > But the point is that the original purpose of the observation has been > expressed. > Whether it's an image, a spectrum, or simply a number can be extracted > from all the > other metadata. If you don't have "obs.calib.dome-flat", then you're > left with scanning > the FITS header for OBJECT="DOMEFLT", OBJECT="DFLAT", OBJECT="DOMFLAT", > OBJECT="FLAT-DOME", .... Same remarks as above! all this is related with DM Observation definition and may be utype will perhaps be of some help? > >> But take an image obs.calib.sky-flat (sky-flat observation), although >> its main >> usage will be calibration nobody can assert that some project can use >> these data >> for other purposes, even scientific ones : variability event follow >> up, historical >> tracing back, proper motion detection... or whatever else we are not >> already >> thinking or aware of. > > > Ah, but if I'm looking for a bright GRB in daytime observations, > knowing that the image > is an obs.calib.sky-flat makes tremendous difference: it could have > been an > obs.calib.dome-flat (which wouldn't be of any use)! > >> obs.calib.freq or obs.calib.spectcan certainly be better defined with >> another syntax, >> and first of all what is the kind of observed data concerned, image, >> spectra, linelist...? > > > Since UCDs can be concatenated, this isn't important: the role of the > observation has > been named as a concept - the rest comes from the data and metadata. > > A trivial example of how useful this could be would be in a data > pipeline: if all the images > had things attached like obs.calib.dome-flat, obs.calib.wl then there > would be a universal > and trivial method for determining just what the data are, independent > of FITS keywords > and local systems (e.g. ESO.DET.CCD.PAR.TEMP......). Yes certainly! But perhaps another organizing way with a UCD defining a data kind and/or purpose and then the corresponding parameters (not FIELD ;-), so not restricted to VOTable) can take the desired values. I don't think that UCD purpose is to solve nomenclature pb or definitions but I am perhaps (certainly?) wrong. > >>> just like the original >>> VOTable types who wanted to describe their catalogue entries. >>> There's nothing fundamentally >>> different in a VO sense between a calibration image (say, an >>> obs.calib.phot) and a table entry >>> of the resulting calibration (say, phot.calib). Right now, UCD is >>> mainly (some but not me might >>> say only) useful for tables, which is why it needs to be extended >>> to non-table standard VO uses. >> >> Yes but it is not the goal of the SCI-Board, at least from the point >> of view >> of the structure, it is only concern by the content, and I am not sure >> that all the UCD problems can be resolve only by content "handling". >> Worthwhile for ucd@ivoa.net perhaps not for ucd-sci@ivoa.net. > > > I disagree: the WHOLE point of ucd-sci is to make high-level decisions > of what is needed scientifically. > Otherwise, what's the "sci" in ucd-sci for? > >>> A "data model for observation and data reduction" looks very >>> different indeed, though it must >>> ultimately use elements for which the VO has a primitive >>> description. UCD is our VO dictionary >> >> But dictionnary of what? >> All the words in astronomy (so it is related to ontology and semantic >> I suppose) >> or a dictionary of concepts, these ones beeing able to "take" values >> or can be >> instanciate in more precise description. >> UCD is only a part (conceptuel one AFAI understand) of a "parameter" >> description >> which can be more precisely define by "values" (restricted by >> enumerated lists, >> obtained from name resolver....), others "attributes" or even others >> "parameters". > > > This is a particularly VOTable-ish view of the VO and of the role of > UCDs. I don't catch the point! > You want to have > instr.bandwidth in order to identify that the number in a table or anywhere else! > is the > instrumental bandwidth. I want to > have src.class.galaxy.spiral in order to be able to identify that the > VOEvent happened next to a spiral > galaxy. Where's the difference? What one calls "values", > "attributes" and "parameters" is just > a question of semantics. and corresponding level of abstraction. > Why do I have to use > > spiral galaxy > > rather than src.class.galaxy.spiral but you don't have to use > > instrumental bandwidth > > instead of instr.bandwidth? From my pov ( once again :-( ), instr.bandwidth is a concept realised in a lot of diff items (all existing filters) while spiral galaxy is a classification schema realisation. But I may be wrong, and the usefullness of some usage requires perhaps the introduction of at least some classification schema! including MK spectral type for stars? > > Rick > > ------------------------------------------------------------------------ > ------------------------ > Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE > Universitaets-Sternwarte Tel. +49-551-39-5052 > Geismarlandstr. 11 Fax +49-551-39-5043 > 37083 Goettingen http://www.uni-sw.gwdg.de/~hessman > ------------------------------------------------------------------------ > ------------------------- > MONET: a MOnitoring NEtwork of Telescopes > http://monet.uni-goettingen.de > ------------------------------------------------------------------------ > ------------------------- > -- Pierre ------------------------------------------------------------------ DIDELON :@: pdidelon_at_cea.fr Phone : 33 (0)1 69 08 58 89 CEA SACLAY - Service d'Astrophysique 91191 Gif-Sur-Yvette Cedex ------------------------------------------------------------------ Aidez les enfants Tibétains : http://www.a-e-t.org/jcparrain.htm ou d'autres : http://www.sosesf.org/ ------------------------------------------------------------------ Seule compte la démarche. Car c'est elle qui dure et non le but qui n'est qu'illusion du voyageur... Saint Exupery - Citadelle ------------------------------------------------------------------ From owner-ucd-sci@eso.org Wed Jun 1 17:33:04 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51FWvaJ019133 for ; Wed, 1 Jun 2005 17:32:57 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j51FWvQI019132 for ucd-sci-outgoing; Wed, 1 Jun 2005 17:32:57 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-sci@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51FWgaJ019102; Wed, 1 Jun 2005 17:32:43 +0200 (MEST) Received: from fed1rmmtao12.cox.net (fed1rmmtao12.cox.net [68.230.241.27]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51FWdXW001697; Wed, 1 Jun 2005 17:32:40 +0200 (CEST) Received: from [10.0.1.24] (really [68.231.133.145]) by fed1rmmtao12.cox.net (InterMail vM.6.01.04.00 201-2131-118-20041027) with ESMTP id <20050601153216.NIIV550.fed1rmmtao12.cox.net@[10.0.1.24]>; Wed, 1 Jun 2005 11:32:16 -0400 In-Reply-To: <429DBE0C.7060905@cea.fr> References: <20050531150728.fn26pj7v9fa8okc8@webmail.sic.rm.cnr.it> <94643280d46f33e5c88952d520f13f55@Astro.physik.Uni-Goettingen.DE> <429D79B3.3@cea.fr> <0a75e9e971886f955bcd71d196c35f79@Astro.physik.Uni-Goettingen.DE> <429DBE0C.7060905@cea.fr> Mime-Version: 1.0 (Apple Message framework v730) Content-Type: multipart/alternative; boundary=Apple-Mail-1--253680462 Message-Id: Cc: Rob Seaman , ucd@ivoa.net, ucd-tech@ivoa.net From: Rob Seaman Subject: UCDs vs ontologies? Date: Wed, 1 Jun 2005 08:32:36 -0700 To: ucd-sci@ivoa.net X-Mailer: Apple Mail (2.730) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.6.1.15 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 --Apple-Mail-1--253680462 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed On Jun 1, 2005, at 6:54 AM, Pierre Didelon wrote: > But do/must UCD be the solution to (all?) natural langage parsing? It would be premature to begin the work of the board by willy-nilly reassigning identifiers such as "em". It seems likely that we will need to be able to express the concepts of both "electromagnetism" and "emission". If there is emission, there is absorption. And sometimes we may want to express the combination of "electromagnetic emission" at the same time. On the other hand, we're told that the role of UCDs is distinct from that of ontologies. An ontology is an (attempt) at expressing the complete range of some knowledge domain. Astronomy is a big subject - its ontology will be big. Perhaps by analogy we can view an ontology as the unabridged dictionary for some subject, whereas UCDs are simply one way to build a glossary for a specific purpose. Glossaries are often small enough to be appended to a brief document. Personally, I think the VO community will need to develop several separate ontologies over time as well as several separate glossaries of UCDs or UCD-like constructs. It is not obvious that a glossary of UCDs for tabular convenience is equivalent to a glossary of UCDs for VOEvent convenience. An ontology can afford to be large and unwieldy to reach its goal of being complete and accurate. A UCD style glossary, on the other hand, will eventually reach an optimum size. Its utility will pass a point of diminishing returns. Too much precision engenders confusion. The availability of too many options results in overlapping shades of meaning. I gather the current list of UCDs was generated by looking at actual tables in the literature. This is just how the unabridged OED was created from words sieved from millions of quotations. Just like a dictionary, the work of maintaining the list of UCDs will continue indefinitely as new tabular usage is coined. I would suggest that the creation of this new list of UCD-like entities to describe astronomical "concepts" is fundamentally a different exercise. We may not be trying to generate a complete ontology with all interrelationships clearly drawn between all concepts, but we are trying to be complete in the sense of not leaving any gaps in the web of concepts. "Star" and "galaxy" will clearly make the final cut. "Star.white_dwarf" and "galaxy.spiral" most likely, too. But it won't take many levels to exhaust the utility of compiling such a list. I expect the final list to have hundreds of entries, not tens of thousands. One final point. The nature of this board is to participate in the process of certifying an official list of terms. I think the true utility of both glossaries and dictionaries will be achieved when facilities are available for creating and maintaining *unofficial* lists. For VOEvent, for instance, it seems likely that each project publishing events will adopt its own glossary pertinent to its own instrumentation and observations. We should support these activities and provide a framework for project specific glossaries. They will spring into existence whether or not we do so. At least if we support the creation of project specific glossaries, we can have some say in controlling a common semantic structure and a standardized distribution mechanism. This might also naturally lead to the next step of layering UCD glossaries on top of our emerging ontology (ies). A glossary, after all, is nothing but a well chosen list of words out of the dictionary. It is the dictionary that provides etymology, synonyms and antonyms, classification by part of speech, tenses and gender, pronunciation, ... Sorry for the cross-posting. If we can't restrain ourselves from generating all these mailing lists, I'm not sure what hope we have for a coherent set of UCD lists :-) Rob Seaman NOAO --Apple-Mail-1--253680462 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1

On Jun 1, 2005, at = 6:54 AM, Pierre Didelon wrote:

But do/must UCD be the solution to (all?) natural = langage parsing?

It would be premature to = begin the work of the board by willy-nilly reassigning identifiers such = as "em".=A0 It seems likely that we will need to be able to express the = concepts of both "electromagnetism" and "emission".=A0 If there is = emission, there is absorption.=A0 And sometimes we may want to express = the combination of "electromagnetic emission" at the same = time.

On= the other hand, we're told that the role of UCDs is distinct from that = of ontologies.=A0 An ontology is an (attempt) at expressing the complete = range of some knowledge domain.=A0 Astronomy is a big subject - its = ontology will be big.=A0 Perhaps by analogy we can view an ontology as = the unabridged dictionary for some subject, whereas UCDs are simply one = way to build a glossary for a specific purpose.=A0 Glossaries are often = small enough to be appended to a brief document.

Personally, I think the VO = community will need to develop several separate ontologies over time as = well as several separate glossaries of UCDs or UCD-like constructs.=A0 = It is not obvious that a glossary of UCDs for tabular convenience is = equivalent to a glossary of UCDs for VOEvent convenience.=A0 An ontology = can afford to be large and unwieldy to reach its goal of being complete = and accurate.=A0 A UCD style glossary, on the other hand, will = eventually reach an optimum size.=A0 Its utility will pass a point of = diminishing returns.=A0 Too much precision engenders confusion.=A0 The = availability of too many options results in overlapping shades of = meaning.

I = gather the current list of UCDs was generated by looking at actual = tables in the literature.=A0 This is just how the unabridged OED was = created from words sieved from millions of quotations.=A0 Just like a = dictionary, the work of maintaining the list of UCDs will continue = indefinitely as new tabular usage is coined.

I would suggest that the = creation of this new list of UCD-like entities to describe astronomical = "concepts" is fundamentally a different exercise.=A0 We may not be = trying to generate a complete ontology with all interrelationships = clearly drawn between all concepts, but we are trying to be complete in = the sense of not leaving any gaps in the web of concepts.=A0 =A0"Star" = and "galaxy" will clearly make the final cut.=A0 "Star.white_dwarf" and = "galaxy.spiral" most likely, too.=A0 But it won't take many levels to = exhaust the utility of compiling such a list.=A0 I expect the final list = to have hundreds of entries, not tens of thousands.

One final point.=A0 The = nature of this board is to participate in the process of certifying an = official list of terms.=A0 I think the true utility of both glossaries = and dictionaries will be achieved when facilities are available for = creating and maintaining *unofficial* lists.=A0 For VOEvent, for = instance, it seems likely that each project publishing events will adopt = its own glossary pertinent to its own instrumentation and observations.=A0= We should support these activities and provide a framework for project = specific glossaries.=A0 They will spring into existence whether or not = we do so.=A0 At least if we support the creation of project specific = glossaries, we can have some say in controlling a common semantic = structure and a standardized distribution mechanism.=A0 This might also = naturally lead to the next step of layering UCD glossaries on top of our = emerging ontology(ies).=A0 A glossary, after all, is nothing but a well = chosen list of words out of the dictionary.=A0 It is the dictionary that = provides etymology, synonyms and antonyms, classification by part of = speech, tenses and gender, pronunciation, ...

Sorry for the = cross-posting.=A0 If we can't restrain ourselves from generating all = these mailing lists, I'm not sure what hope we have for a coherent set = of UCD lists :-)

Rob = Seaman
NOAO
= --Apple-Mail-1--253680462-- From owner-ucd-sci@eso.org Wed Jun 1 17:42:47 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51FgfaJ021512 for ; Wed, 1 Jun 2005 17:42:42 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j51FgfUB021511 for ucd-sci-outgoing; Wed, 1 Jun 2005 17:42:41 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-sci@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51FgbaJ021500; Wed, 1 Jun 2005 17:42:37 +0200 (MEST) Received: from mssltz.mssl.ucl.ac.uk (mssltz.mssl.ucl.ac.uk [128.40.71.165]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51FgZ73001765; Wed, 1 Jun 2005 17:42:36 +0200 (CEST) Received: from msslta.mssl.ucl.ac.uk (msslta.mssl.ucl.ac.uk [128.40.71.124]) by mssltz.mssl.ucl.ac.uk (8.12.10/8.12.10) with ESMTP id j51FgPJ0005148 (version=TLSv1/SSLv3 cipher=EDH-RSA-DES-CBC3-SHA bits=168 verify=NO); Wed, 1 Jun 2005 16:42:25 +0100 Date: Wed, 1 Jun 2005 16:42:25 +0100 (BST) From: Elizabeth Auden To: Rob Seaman cc: ucd-sci@ivoa.net, ucd@ivoa.net, ucd-tech@ivoa.net Subject: Re: UCDs vs ontologies? In-Reply-To: Message-ID: References: <20050531150728.fn26pj7v9fa8okc8@webmail.sic.rm.cnr.it> <94643280d46f33e5c88952d520f13f55@Astro.physik.Uni-Goettingen.DE> <429D79B3.3@cea.fr> <0a75e9e971886f955bcd71d196c35f79@Astro.physik.Uni-Goettingen.DE> <429DBE0C.7060905@cea.fr> MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed X-MSSL-MailScanner-Information: Please contact the ISP for more information X-MSSL-MailScanner: No virus found X-MSSL-MailScanner-SpamCheck: not spam, SpamAssassin (score=-4.9, required 5, BAYES_00 -4.90) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.6.1.15 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 > On the other hand, we're told that the role of UCDs is distinct from that of > ontologies. An ontology is an (attempt) at expressing the complete range of > some knowledge domain. Astronomy is a big subject - its ontology will be > big. > Personally, I think the VO community will need to develop several separate > ontologies over time as well as several separate glossaries of UCDs or > UCD-like constructs. It is not obvious that a glossary of UCDs for tabular > convenience is equivalent to a glossary of UCDs for VOEvent convenience. An > ontology can afford to be large and unwieldy to reach its goal of being > complete and accurate. Incidentally, I've posted a first go at a VOEvent ontology (OWL-DL format) on the VOTech wiki at http://wiki.eurovotech.org/bin/view/VOTech/VoEventOntology. Any comments on the structure, concepts, and coverage of this v0.000000001 ontology would be appreciated. cheers, Elizabeth From owner-ucd-tech@eso.org Wed Jun 1 20:42:01 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51IfqaJ022928 for ; Wed, 1 Jun 2005 20:41:52 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j51IfqIG022927 for ucd-tech-outgoing; Wed, 1 Jun 2005 20:41:52 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-tech@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51IfhaJ022912; Wed, 1 Jun 2005 20:41:44 +0200 (MEST) Received: from earth.astro.umd.edu (earth.astro.umd.edu [129.2.14.2]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51IffXW008022; Wed, 1 Jun 2005 20:41:42 +0200 (CEST) Received: from [129.2.14.215] (lap5.astro.umd.edu [129.2.14.215]) (using TLSv1 with cipher DHE-RSA-AES256-SHA (256/256 bits)) (No client certificate requested) by earth.astro.umd.edu (Postfix) with ESMTP id 65B5B109A7; Wed, 1 Jun 2005 14:41:35 -0400 (EDT) Message-ID: <429E015D.1080501@gsfc.nasa.gov> Date: Wed, 01 Jun 2005 14:41:33 -0400 From: Ed Shaya User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.1; en-US; rv:1.7.6) Gecko/20050319 X-Accept-Language: en-us, en MIME-Version: 1.0 To: Elizabeth Auden Cc: Rob Seaman , ucd-sci@ivoa.net, ucd@ivoa.net, ucd-tech@ivoa.net, Data Model IVOA List Subject: Re: [Ontology] UCDs vs ontologies? References: <20050531150728.fn26pj7v9fa8okc8@webmail.sic.rm.cnr.it> <94643280d46f33e5c88952d520f13f55@Astro.physik.Uni-Goettingen.DE> <429D79B3.3@cea.fr> <0a75e9e971886f955bcd71d196c35f79@Astro.physik.Uni-Goettingen.DE> <429DBE0C.7060905@cea.fr> In-Reply-To: Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.6.1.21 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-tech@eso.org Precedence: bulk Reply-To: ucd-tech@ivoa.net X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Elizabeth, Hurray. Another ontology fan. I have taken the liberty of using OwlDoc in Protege to create a browser readable version of your ontology. It is at http://archive.astro.umd.edu/ont/Documentation/VOEVENT/index.html Would you mind if I integrate what you have into the more general ontology that I have been working on? http://archive.astro.umd.edu/ont/Documentation/index.html (And yes, Rob it does tend to get big, but one can trim it at any level. I rather see UCDs as a form of topic maps which is quite a close relative of Ontology. I prefer ontology because I believe one can do more rigorous reasoning and query with it, but many prefer topic maps because they are more loose and easy. ) Now that there are two of us interested in Ontology we can form a group. It has been suggested to me that Ontology discussions should reside in the data model group with "[Ontology]" in the subject Re:. So, I am ccing there too and will take the rest of this discussion there. I hope you are tuned in Elizabeth. Ed Elizabeth Auden wrote: > > Incidentally, I've posted a first go at a VOEvent ontology (OWL-DL > format) on the VOTech wiki at > http://wiki.eurovotech.org/bin/view/VOTech/VoEventOntology. Any > comments on the structure, concepts, and coverage of this v0.000000001 > ontology would be appreciated. > > cheers, > Elizabeth > From owner-ucd@eso.org Wed Jun 1 21:20:37 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51JKMaJ029542 for ; Wed, 1 Jun 2005 21:20:22 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j51JKMkm029541 for ucd-outgoing; Wed, 1 Jun 2005 21:20:22 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51JKHaJ029533 for ; Wed, 1 Jun 2005 21:20:17 +0200 (MEST) Received: from apollo.le.ac.uk (apollo.le.ac.uk [143.210.16.125]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51JKG73009185 for ; Wed, 1 Jun 2005 21:20:16 +0200 (CEST) Message-Id: <200506011920.j51JKG73009185@apollo.hq.eso.org> Received: from [143.210.36.14] (helo=marindi) by apollo.le.ac.uk with esmtp (Exim 4.44) id 1DdYl7-00057j-6c; Wed, 01 Jun 2005 20:20:09 +0100 From: "Tony Linde" To: "'Ed Shaya'" , "'Elizabeth Auden'" Cc: Subject: RE: [Ontology] UCDs vs ontologies? Date: Wed, 1 Jun 2005 20:20:09 +0100 MIME-Version: 1.0 Content-Type: text/plain; charset="US-ASCII" Content-Transfer-Encoding: 7bit X-Mailer: Microsoft Office Outlook, Build 11.0.6353 In-Reply-To: <429E015D.1080501@gsfc.nasa.gov> Thread-Index: AcVm2cueQYqoM/bbRmqtZQLc9T46QgABEzjg X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2527 X-UoL-Id: 11b34ef000f39a0fef8ef2218051c54b@1DdYl7-00057j-6c@apollo.le.ac.uk X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.6.1.22 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: "Tony Linde" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi Ed, Count me in too. In fact, you can count a whole sub-group of the VOTech project, DS5. Check out: http://wiki.eurovotech.org/bin/view/VOTech/ResourceDiscovery and associated. And you don't need a new group, there already is one, the semantics workgroup: semantics@ivoa.net archive at: http://ivoa.net/forum/semantics/ It was set up after discussions between variouspeople a couple of years ago but died out. I'll repost this message there (since I *HATE* cross-posting) and suggest we all adjourn to the semantics forum for ontology-like discussions. Cheers, Tony. > -----Original Message----- > From: owner-dm@eso.org [mailto:owner-dm@eso.org] On Behalf Of Ed Shaya > Sent: 01 June 2005 19:42 > To: Elizabeth Auden > Cc: Rob Seaman; ucd-sci@ivoa.net; ucd@ivoa.net; > ucd-tech@ivoa.net; Data Model IVOA List > Subject: Re: [Ontology] UCDs vs ontologies? > > Elizabeth, > > Hurray. Another ontology fan. I have taken the liberty > of using OwlDoc in Protege to create a browser readable > version of your ontology. It is at > > http://archive.astro.umd.edu/ont/Documentation/VOEVENT/index.html > > Would you mind if I integrate what you have into the more > general ontology that I have been working on? > http://archive.astro.umd.edu/ont/Documentation/index.html > (And yes, Rob it does tend to get big, but one can trim it at > any level. I rather see UCDs as a form of topic maps which > is quite a close relative of Ontology. I prefer ontology > because I believe one can do more rigorous reasoning and > query with it, but many prefer topic maps because they are > more loose and easy. ) > > Now that there are two of us interested in Ontology we can > form a group. It has been suggested to me that Ontology > discussions should reside in the data model group with > "[Ontology]" in the subject Re:. So, I am ccing there too > and will take the rest of this discussion there. I hope you > are tuned in Elizabeth. > > Ed > > > > > Elizabeth Auden wrote: > > > > > Incidentally, I've posted a first go at a VOEvent ontology (OWL-DL > > format) on the VOTech wiki at > > http://wiki.eurovotech.org/bin/view/VOTech/VoEventOntology. Any > > comments on the structure, concepts, and coverage of this > v0.000000001 > > ontology would be appreciated. > > > > cheers, > > Elizabeth > > > > From owner-ucd-tech@eso.org Wed Jun 1 21:30:32 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51JUQaJ001214 for ; Wed, 1 Jun 2005 21:30:26 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j51JUQmI001213 for ucd-tech-outgoing; Wed, 1 Jun 2005 21:30:26 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-tech@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51JUGaJ001202; Wed, 1 Jun 2005 21:30:17 +0200 (MEST) Received: from phobos.caltech.edu (phobos.caltech.edu [131.215.102.1]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51JUE73009441; Wed, 1 Jun 2005 21:30:15 +0200 (CEST) Received: from avyakta.caltech.edu (IDENT:U2FsdGVkX1/ZNn3d3vbHF6HA5XVycgfncWUk5Eq04f4@avyakta [131.215.102.12]) by phobos.caltech.edu (8.12.10/8.12.10) with ESMTP id j51JU74I027713; Wed, 1 Jun 2005 12:30:07 -0700 (PDT) Received: from localhost (localhost.localdomain [127.0.0.1]) by avyakta.caltech.edu (8.12.11/8.12.8) with ESMTP id j51JU6Ka001820; Wed, 1 Jun 2005 12:30:06 -0700 Date: Wed, 1 Jun 2005 12:30:06 -0700 (PDT) From: Ashish Mahabal X-X-Sender: aam@avyakta.caltech.edu To: Ed Shaya cc: Elizabeth Auden , Rob Seaman , ucd-sci@ivoa.net, ucd@ivoa.net, ucd-tech@ivoa.net, Data Model IVOA List Subject: Re: [Ontology] UCDs vs ontologies? In-Reply-To: <429E015D.1080501@gsfc.nasa.gov> Message-ID: References: <20050531150728.fn26pj7v9fa8okc8@webmail.sic.rm.cnr.it> <94643280d46f33e5c88952d520f13f55@Astro.physik.Uni-Goettingen.DE> <429D79B3.3@cea.fr> <0a75e9e971886f955bcd71d196c35f79@Astro.physik.Uni-Goettingen.DE> <429DBE0C.7060905@cea.fr> <429E015D.1080501@gsfc.nasa.gov> MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.6.1.22 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-tech@eso.org Precedence: bulk Reply-To: ucd-tech@ivoa.net X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi Ed, Count me in too. I am the topic maps kind of person you mentioned, but also interested in ontologies. This should provide me some new impetus to working on UCDs, topic maps and ontologies. -ashish Ashish Mahabal, Caltech Astronomy, Pasadena, CA 91125 http://www.astro.caltech.edu/~aam aam at astro.caltech.edu Backups? We doan *NEED* no steenking baX%^~,VbKx NO CARRIER From owner-ucd@eso.org Mon Jul 11 17:01:51 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j6BF1O1b008576 for ; Mon, 11 Jul 2005 17:01:25 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j6BF1OUI008575 for ucd-outgoing; Mon, 11 Jul 2005 17:01:24 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j6BF1G1b008547 for ; Mon, 11 Jul 2005 17:01:16 +0200 (MEST) Received: from smtp1.sic.rm.cnr.it (mailrelay.artov.rm.cnr.it [150.146.129.253]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j6BF1Bin008451 for ; Mon, 11 Jul 2005 17:01:12 +0200 (CEST) Received: (qmail 3568 invoked by uid 508); 11 Jul 2005 15:01:05 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.86. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.958815 secs); 11 Jul 2005 15:01:05 -0000 Received: from unknown (HELO localhost) ([10.1.1.2]) (envelope-sender ) by smtp1.sic.rm.cnr.it (qmail-ldap-1.03) with SMTP for ; 11 Jul 2005 15:01:04 -0000 Received: from eddington.u-strasbg.fr (eddington.u-strasbg.fr [130.79.129.110]) by webmail.sic.rm.cnr.it (Horde) with HTTP for ; Mon, 11 Jul 2005 17:01:03 +0200 Message-ID: <20050711170103.buzzas2dadesw8cs@webmail.sic.rm.cnr.it> Date: Mon, 11 Jul 2005 17:01:03 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Cc: ucd@ivoa.net Subject: draft PR doc on ucd-words MIME-Version: 1.0 Content-Type: multipart/mixed; boundary="=_5j4gqpybq3y8" Content-Transfer-Encoding: 7bit User-Agent: Internet Messaging Program (IMP) H3 (4.0.1) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.2, Antispam-Data: 2005.7.11.14 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: ucd@ivoa.net X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 This message is in MIME format. --=_5j4gqpybq3y8 Content-Type: text/plain; charset=ISO-8859-1 Content-Disposition: inline Content-Transfer-Encoding: 7bit After 4 weeks of discussion in the Sci-board and some extra time to set up the document, you'll find attached a draft version of the document containing the list of ucd-words. Note for the Sci-board: I included the last comments. I also had to modify a number of words to be compliant with the UCD-Rec document ("... for any two words at the same level in the hierarchy, one can't be a starting substring of the other..."), so old version =============> new version phot.fluxDensity phot.fluDensity phys.energyDensity phys.energDensity phys.massYield phys.mYield pos.earthop pos.eop Of course there is still the case of phys.at/atmol, but we can wait for the revision of the whole list of atomic and molecular ucds. I submit the document+list to the members of the UCD-WG because this is the IVOA standard procedure, and I formally ask you if we can move from the WD phase to the PR phase. In this particular case we also had to follow another "formal" procedure, estabished by the UCD main document, to generate and maintain the list of ucd-words. This is why I'm sending the draft to both mailing lists. The document is already in the PR "format" but, being a draft, the link to the RFC page is of course not yet activated. If you have major objections (on the content of the document/list of words) please let me know asap. According to our roadmap, we have to move the UCD-list document from the WD phase to the PR phase within July. This would mean asking for comments on the PR document during a holiday period. I think it would be better to issue the RFC in the second half of August. Please let me know if you disagree on that. Best regards Andrea ============================================================================== Andrea Preite Martinez andrea@rm.iasf.cnr.it Istituto di Astrofisica Spaziale Tel.:+39.06.4993.4641 Area di Ricerca di Tor Vergata Fax.:+39.06.2066.0188 Via del Fosso del Cavaliere 100 Cell:+39.339.3817355 00133 Roma ============================================================================== --=_5j4gqpybq3y8 Content-Type: application/pdf; name="UCDlist-20050711.pdf" Content-Disposition: attachment; filename="UCDlist-20050711.pdf" Content-Transfer-Encoding: 7bit %!PS-Adobe-3.0 %%Pages: (atend) %%BoundingBox: 0 0 596 758 %%HiResBoundingBox: 0.000000 0.000000 595.300000 757.700000 %......................................... %%Creator: ESP Ghostscript 707 (pswrite) %%CreationDate: 2005/07/11 16:09:12 %%DocumentData: Clean7Bit %%LanguageLevel: 2 %%EndComments %%BeginProlog % This copyright applies to everything between here and the %%EndProlog: % Copyright 2003 artofcode LLC and Easy Software Products, all rights reserved. %%BeginResource: procset GS_pswrite_2_0_1001 /GS_pswrite_2_0_1001 80 dict dup begin /PageSize 2 array def/setpagesize{ PageSize aload pop 3 index eq exch 4 index eq and{ pop pop pop}{ PageSize dup 1 5 -1 roll put 0 4 -1 roll put dup null eq {false} {dup where} ifelse{ exch get exec} { pop/setpagedevice where { pop 1 dict dup /PageSize PageSize put setpagedevice} { /setpage where{ pop PageSize aload pop pageparams 3 {exch pop} repeat setpage}if}ifelse}ifelse}ifelse} bind def /!{bind def}bind def/#{load def}!/N/counttomark # /rG{3{3 -1 roll 255 div}repeat setrgbcolor}!/G{255 div setgray}!/K{0 G}! 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