From owner-ucd-sci@eso.org Tue May 31 19:59:33 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 j4VHxQVZ027584 for ; Tue, 31 May 2005 19:59:26 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4VHxQ0q027582 for ucd-sci-outgoing; Tue, 31 May 2005 19:59:26 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-sci@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 j4VHxGVZ027552; Tue, 31 May 2005 19:59:16 +0200 (MEST) Received: from [134.171.30.4] (nb008487.ads.eso.org [134.171.30.4]) by serapis.hq.eso.org (8.11.7+Sun/8.11.7) with ESMTP id j4VHxGE13935; Tue, 31 May 2005 19:59:16 +0200 (MEST) Message-ID: <429CA60B.1070008@eso.org> Date: Mon, 30 May 2005 11:50:49 +0200 From: Andrea Preite Martinez User-Agent: Mozilla Thunderbird 1.0 X-Accept-Language: en-us, en MIME-Version: 1.0 To: ucd-sci@ivoa.net, ucd-tech@ivoa.net Subject: Sci-Board-1 Content-Type: multipart/alternative; boundary="------------000003040703050701070400" 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 --------------000003040703050701070400 Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit Dear colleagues, this first message is for setting up our roadmap and organizing the Board and our work on the UCD-vocabulary.. A. Roadmap. Our goal is very simple: we need to stabilize (which means adding, deleting, transforming ) the present draft list of ucd-words, that you can find at http://cdsweb.u-strasbg.fr/UCD/ucd1p-words.txt (just the list) http://www.ivoa.net/internal/IVOA/IvoaUCD/WD-UCDlist-20050429.pdf (the WD document) in order to (i) reach consensus, and (ii) be able to promote the list (and the associated document) to the level of IVOA Proposed Recommendation as soon as possible (within June). B. The Board 1. Duration. There will be a Sci-Board as long as UCDs will be in use in the VO, in order to maintain the vocabulary. The mission of the board is described in the main UCD document, that you can find at http://www.ivoa.net/Documents/latest/UCD.html now under minor revisions as suggested during the Exec Meeting in Kyoto. It is possible that in the future the Exec could change the mission to suit new needs of the VO. 2. Participation. Participation is on a voluntary basis. Colleagues can ask the chair of the Board to be inserted in (or deleted from) the mailing list of the Board, and to work for a specific task (see below). 3. Chair For the transition period required to set up the Board and let it run, I will act as chair person of the Board (by the way, setting up the Board and upgrading the present list of UCD-words to the level of IVOA PR is a formal action for the chairman of the UCD-WG). I propose to go for an election of the chairman of the Board in a month from now. C. Organization 1. What (Tasks) Time is very short, at least for this first phase of our work. I propose then to define a number of key tasks and form task-groups on different aspects of the vocabulary. The most urgent cases were well pinned down during the last InterOp Meeting. My first draft proposal is to organize our work around the following tasks: T1: the "velocity" and the resolution(s) problems T2: theory and simulations (sim ?) T3: at/mol physics T4: curation (humans, organizations) and other "meta"-likes T5: flux (total, net, backgr. and various "flux densities") and time (period of, instant of) T6: solar system Txx : ?? T0: Coordination, general issues, not included in the above Ts. Like the Board, tasks are not "closed". The discussion is open ("plenary") and contributions are welcome from every member of the Board. It will help people with an analytical mind (like mine!) to see "T5" appear in the subject of your message, if dealing with "net flux" or mid-time of exposure. We need a coordinator for each task, with the responsibility to make a final proposal to the Board. There is nothing formal in the following list of people, I'm just asking them to pay more attention to the discussion relevant to the corresponding task, and summarize the discussion to the Board in due time. Making use of the list of members (as of today) I propose the following coordinators: T0 General Andrea T1 Velocity/resolution Alberto Micol T2 Theory/simulations Volunteer(?) T3 At/Mol physics Marie-Lise Dubernet T4 Meta Sébastien D. T5 flux/time Jonathan MD T6 Solar system Pierre Didelon 2. How Through the Board's mailing list. Always "reply to all". The chair will record all messages. In this first phase of our work time is very short. So please answer within the given deadlines. We won't wait for late messages. 3. When FIRST ACTION: please comment on the above organization/rules/tasks within Thursday the 2nd of June. This message is sent (for the last time) also to the wider interop@ivoa.net community to ask the laziest to join in. Best regards Andrea --------------000003040703050701070400 Return-Path: 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 j517KZaJ011127 for ; Wed, 1 Jun 2005 09:20:35 +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 j517KX73014322 for ; Wed, 1 Jun 2005 09:20:33 +0200 (CEST) Received: from (150.146.129.253) by e1000.artov.rm.cnr.it via smtp id 3bf1_98c091e0_d26d_11d9_99fc_0002b3da0f69; Wed, 01 Jun 2005 09:20:13 +0200 (CEST) Received: (qmail 23411 invoked by uid 508); 1 Jun 2005 07:20:27 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.031986 secs); 01 Jun 2005 07:20:27 -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 ; 1 Jun 2005 07:20:27 -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 ; Wed, 1 Jun 2005 09:20:27 +0200 Message-ID: <20050601092027.76sgk0xwxkn4484g@webmail.sic.rm.cnr.it> Date: Wed, 1 Jun 2005 09:20:27 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Sci-Board-2 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) Reply-To: ucd-sci@ivoa.net X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.31.45 X-Virus-Scanned: by amavisd-new Dear colleagues, I see from the first answers to Sci-Board-1 that thinks are not clear for everybody: 1. Please, REPLY TO ALL the members of the Board, not to the ucd-list nor to my address. Remember that not all the members of the Board are also members of the UCD-WG. You can "cc" to your pet-list, I don't care, but make sure that at least the Board can read your message. 2. When suggesting new UCD-words, please ask yourself which kind of "quantity" you want to describe or, if not a quantity, which kind of attribute (qualifier/modifier). By the way, our mission is to stabilize and maintain a list of "words", NOT a list of UCDs. Syntax will take care of how to build UCDs, based on the classification of the word (e.g. P/Q/S syntactic flag). 3. For what VOEvent is concerned, please have a look at the conclusions of the joint session UCD/VOEvent at http://www.ivoa.net/twiki/bin/view/IVOA/InterOpMay2005UCD We will discuss Event vocabulary at the end of the year, when a first bottom-up list of terms will be available. 4. Sorry, there isn't such a thing as Solar System UCDs. I remind you that the IVOA (Proposed) Recommendation on UCDs explicitly forbids UCDs like "star", "galaxy", or "Sun", "my_pet_object", and so on. On the contrary, qualifiers like "stellar", "galactic", "solar" can be valid atoms. Regards Andrea From owner-ucd-sci@eso.org Return-Path: 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 j517X9aJ014129 for ; Wed, 1 Jun 2005 09:33:09 +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 j517X773014680 for ; Wed, 1 Jun 2005 09:33:08 +0200 (CEST) Received: from (150.146.129.253) by e1000.artov.rm.cnr.it via smtp id 3cbd_5a5bfa46_d26f_11d9_8d3c_0002b3da0f69; Wed, 01 Jun 2005 09:32:48 +0200 (CEST) Received: (qmail 26538 invoked by uid 508); 1 Jun 2005 07:33:01 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.029113 secs); 01 Jun 2005 07:33:01 -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 ; 1 Jun 2005 07:33:01 -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 ; Wed, 1 Jun 2005 09:33:01 +0200 Message-ID: <20050601093301.ijvm3jky0w740cc0@webmail.sic.rm.cnr.it> Date: Mon, 30 May 2005 16:06:59 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: T2 & T0: Theory & "coments on UCDs" page MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1 Content-Disposition: inline User-Agent: Internet Messaging Program (IMP) H3 (4.0.1) Reply-To: ucd-sci@ivoa.net X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.31.44 X-Virus-Scanned: by amavisd-new Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id j517X9aJ014129 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear all, I can try to help in the UCD-vocabulary for theory/simulations. Maybe others in the theory group would be also interested, there was some discussion in the list about the subject of UCDs... If there is no more voluntieers, I can try to coordinate it, Additionally, should be the UCDs posted at: http://cdsweb.u-strasbg.fr/UCD/cgi-bin/comment/ucdComments?sort=C included in the draft-list? Cheers Miguel (mcs@iaa.es IAA; SVO) From owner-ucd-sci@eso.org Wed Jun 1 09:24:19 2005 Return-Path: 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 j517cwaJ015245 for ; Wed, 1 Jun 2005 09:38:58 +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 j517cuXW015536 for ; Wed, 1 Jun 2005 09:38:57 +0200 (CEST) Received: from (150.146.129.253) by e1000.artov.rm.cnr.it via smtp id 3d72_2a692718_d270_11d9_9e45_0002b3da0f69; Wed, 01 Jun 2005 09:38:37 +0200 (CEST) Received: (qmail 27434 invoked by uid 508); 1 Jun 2005 07:38:50 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.037544 secs); 01 Jun 2005 07:38:50 -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 ; 1 Jun 2005 07:38:50 -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 ; Wed, 1 Jun 2005 09:38:50 +0200 Message-ID: <20050601093850.rs4dtxts10n4scsg@webmail.sic.rm.cnr.it> Date: Mon, 30 May 2005 16:06:59 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Format of concatenated UCD's 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) Reply-To: ucd-sci@ivoa.net X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.31.44 X-Virus-Scanned: by amavisd-new X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Up until now, it hasn't been possible to check the syntax of a UCD list using XML Schema: there's no way (yet) to express a list of elements separated by semi-colons. This is a shame, since it means that somebody else has to do this work - work which could have been delegated to the XML parser. Fortunately, XML Schema recognizes lists of elements separated by white spaces, i.e. not "phot.calib;src.class" but "phot.calib src.class" If the official syntax of UCD lists included the latter possibility, then the entire content of a VO XML document could be parsed at once in a single pass. Yes, it's too late for VOTable, but many other schemata are still in their infancy and would benefit dramatically from this possibility. While the use of UCD in VOTable has - up to now - been mostly in the form of documentation, VOEvent needs to be able to permit direct interpretation of the meaning of elements identified by UCD's (e.g. your robotic telescope only wants to look at GRB's and not vanilla SN). Either all subgroups like VOEvent wil be forced to define their own ontology or we enable all VO schemata to be able to interpret UCD's directly without any extra effort. The present syntax prevents this. Schema examples of how this might work can be found at http://monet.uni-sw.gwdg.de/twiki/bin/view/VOEvent/ SchemaContentUCDListType (for the formal UCD list element type) and http://monet.uni-sw.gwdg.de/twiki/bin/view/UCD/SchemaContentUCD for an example of the current UCD placed in a schema which could be concatenated in a UCD list element. In the short term, we can easily afford to let the two forms exists side by side (well, VOTable uses the old syntax, and new ones like VOEvent use the newer one). Those who have added parsers to read the old UCD lists will easily be able to adopt their code to read the new format, and those of us still working on the first versions of VO schemata can immediately benefit from being able to parse the ENTIRE document. F. Hessman C. Hettlage ------------------------------------------------------------------------ ------------------------ 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 ------------------------------------------------------------------------ ------------------------- ----- Fine messaggio inoltrato. ----- ============================================================================== 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-sci@eso.org Wed Jun 1 09:24:19 2005 Return-Path: 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 j517eDaJ015383 for ; Wed, 1 Jun 2005 09:40:13 +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 j517eAXW015567 for ; Wed, 1 Jun 2005 09:40:11 +0200 (CEST) Received: from (150.146.129.253) by e1000.artov.rm.cnr.it via smtp id 3daf_56b1a052_d270_11d9_9630_0002b3da0f69; Wed, 01 Jun 2005 09:39:52 +0200 (CEST) Received: (qmail 27654 invoked by uid 508); 1 Jun 2005 07:40:05 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.03922 secs); 01 Jun 2005 07:40:05 -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 ; 1 Jun 2005 07:40:04 -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 ; Wed, 1 Jun 2005 09:40:04 +0200 Message-ID: <20050601094004.k0cjj2a80o80o0g0@webmail.sic.rm.cnr.it> Date: Mon, 30 May 2005 16:06:59 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Fwd: Re: Sci-Board-1 -> T6/T0 MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1 Content-Disposition: inline User-Agent: Internet Messaging Program (IMP) H3 (4.0.1) Reply-To: ucd-sci@ivoa.net X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.31.44 X-Virus-Scanned: by amavisd-new Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id j517eDaJ015383 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Hi everybody, I am member of another unformal group working on planetary data in France (ASOV-Planéto), actually mainly grouping people from the region near paris, but establishing contact with the european community through EuroPlanet project. This group ASOV-Planéto is willing to submit proposition for additions and modifications of the actual UCD1+ list to the board! See the actual ;-) status of the reflexion at http://portail.imcce.fr/fr/expert/ssvo/wgovp/propucd.html, done mainly by Jérôme Berthier from IMCCE. Is there a formal/official way to do this? Can people who are not part of the board submit modifications? How? Is there an entry point for the community outside the board? What is the "good" submission path or procedure? Four questions for the same pb is perhaps enough! :-D Cordially, Pierre Andrea Preite Martinez wrote: > Dear colleagues, > > this first message is for setting up our roadmap and organizing the Board > and our work on the UCD-vocabulary.. > > A. Roadmap. > Our goal is very simple: we need to stabilize (which means adding, deleting, > transforming ) the present draft list of ucd-words, that you can find at > > http://cdsweb.u-strasbg.fr/UCD/ucd1p-words.txt (just the list) > http://www.ivoa.net/internal/IVOA/IvoaUCD/WD-UCDlist-20050429.pdf (the WD > document) > > in order to (i) reach consensus, and (ii) be able to promote the list (and > the associated document) to the level of IVOA Proposed Recommendation as > soon as possible (within June). > > B. The Board > 1. Duration. > There will be a Sci-Board as long as UCDs will be in use in the VO, in order > to maintain the vocabulary. The mission of the board is described in the > main UCD document, that you can find at > > http://www.ivoa.net/Documents/latest/UCD.html > > now under minor revisions as suggested during the Exec Meeting in Kyoto. > It is possible that in the future the Exec could change the mission to suit > new needs of the VO. > > 2. Participation. > Participation is on a voluntary basis. Colleagues can ask the chair of the > Board to be inserted in (or deleted from) the mailing list of the Board, > and to work for a specific task (see below). > > 3. Chair > For the transition period required to set up the Board and let it run, I > will act as chair person of the Board (by the way, setting up the Board > and upgrading the present list of UCD-words to the level of IVOA PR is a > formal action for the chairman of the UCD-WG). I propose to go for an > election of the chairman of the Board in a month from now. > > C. Organization > 1. What (Tasks) > Time is very short, at least for this first phase of our work. I propose > then to define a number of key tasks and form task-groups on different > aspects of the vocabulary. The most urgent cases were well pinned down > during the last InterOp Meeting. My first draft proposal is to organize our > work around the following tasks: > > T1: the "velocity" and the resolution(s) problems > T2: theory and simulations (sim ?) > T3: at/mol physics > T4: curation (humans, organizations) and other "meta"-likes > T5: flux (total, net, backgr. and various "flux densities") and time (period > of, instant of) > T6: solar system > Txx : ?? > > T0: Coordination, general issues, not included in the above Ts. > Like the Board, tasks are not "closed". The discussion is open ("plenary") > and contributions are welcome from every member of the Board. It will help > people with an analytical mind (like mine!) to see "T5" appear in the > subject of your message, if dealing with "net flux" or mid-time of > exposure. > > We need a coordinator for each task, with the responsibility to make a final > proposal to the Board. > There is nothing formal in the following list of people, I'm just asking > them to pay more attention to the discussion relevant to the corresponding > task, and summarize the discussion to the Board in due time. > Making use of the list of members (as of today) I propose the following > coordinators: > > T0 General Andrea > T1 Velocity/resolution Alberto Micol > T2 Theory/simulations Volunteer(?) > T3 At/Mol physics Marie-Lise Dubernet > T4 Meta Sébastien D. > T5 flux/time Jonathan MD > T6 Solar system Pierre Didelon > > > 2. How > Through the Board's mailing list. Always "reply to all". The chair will > record all messages. > In this first phase of our work time is very short. So please answer within > the given deadlines. We won't wait for late messages. > > 3. When > FIRST ACTION: please comment on the above organization/rules/tasks within > Thursday the 2nd of June. > > This message is sent (for the last time) also to the wider interop@ivoa.net > community to ask the laziest to join in. > > 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 > ============================================================================== > > -- 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 ------------------------------------------------------------------ ----- Fine messaggio inoltrato. ----- ============================================================================== 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-sci@eso.org Wed Jun 1 09:24:19 2005 Return-Path: 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 j517emaJ015451 for ; Wed, 1 Jun 2005 09:40:48 +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 j517ekXW015596 for ; Wed, 1 Jun 2005 09:40:46 +0200 (CEST) Received: from (150.146.129.253) by e1000.artov.rm.cnr.it via smtp id 3d76_6bb82d7c_d270_11d9_97aa_0002b3da0f69; Wed, 01 Jun 2005 09:40:27 +0200 (CEST) Received: (qmail 27763 invoked by uid 508); 1 Jun 2005 07:40:40 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.032082 secs); 01 Jun 2005 07:40:40 -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 ; 1 Jun 2005 07:40:40 -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 ; Wed, 1 Jun 2005 09:40:40 +0200 Message-ID: <20050601094040.oj6ribznn2ucks4g@webmail.sic.rm.cnr.it> Date: Mon, 30 May 2005 16:06:59 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Fwd: Re: Sci-Board-1 -> T6/T0 MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1 Content-Disposition: inline User-Agent: Internet Messaging Program (IMP) H3 (4.0.1) Reply-To: ucd-sci@ivoa.net X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.31.45 X-Virus-Scanned: by amavisd-new Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id j517emaJ015451 X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Pierre Didelon wrote: Can people who are not part of the board submit modifications? How? Is there an entry point for the community outside the board? What is the "good" submission path or procedure? Dear Pierre, The entry point of that community is YOU. By the way, you just followed the "good" submission path !! Now the discussion on Task-6 is open. Note: I asked M.Leoni at eso to generate a ucd-sci list under the "forum" page of IVOA. It will be much more practical for everybody ! The list will be ready soon. 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 ============================================================================== ----- Fine messaggio inoltrato. ----- ============================================================================== 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-sci@eso.org Wed Jun 1 09:24:19 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 j517ODaJ011655 for ; Wed, 1 Jun 2005 09:24:13 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j517ODpT011654 for ucd-sci-outgoing; Wed, 1 Jun 2005 09:24:13 +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 j517O9aJ011643 for ; Wed, 1 Jun 2005 09:24:09 +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 j517O773014428 for ; Wed, 1 Jun 2005 09:24:07 +0200 (CEST) Received: from (150.146.129.253) by e1000.artov.rm.cnr.it via smtp id 3bb8_185c54fc_d26e_11d9_8787_0002b3da0f69; Wed, 01 Jun 2005 09:23:48 +0200 (CEST) Received: (qmail 24583 invoked by uid 508); 1 Jun 2005 07:24:01 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.036856 secs); 01 Jun 2005 07:24:01 -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 ; 1 Jun 2005 07:24:01 -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 ; Wed, 1 Jun 2005 09:24:01 +0200 Message-ID: <20050601092401.q3m7lpliuw84sssw@webmail.sic.rm.cnr.it> Date: Wed, 1 Jun 2005 09:24:01 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: T0 : extensions to em, obs, spect, instr 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: 2005.5.31.44 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 Msg sent by: Data: Mon, 30 May 2005 13:06:23 +0200 Da: "Frederic V. \\Rick\\ Hessman" Rispondi-A: "Frederic V. \\Rick\\ Hessman" Oggetto: T0 : extensions to em, obs, spect, instr A: ucd@ivoa.net 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 ------------------------------------------------------------------------ ------------------------- ----- End of forwarded mail. ----- ============================================================================== 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-sci@eso.org Wed Jun 1 09:25:04 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 j517OxaJ012067 for ; Wed, 1 Jun 2005 09:24:59 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j517Oxiq012065 for ucd-sci-outgoing; Wed, 1 Jun 2005 09:24:59 +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 j517OsaJ012012 for ; Wed, 1 Jun 2005 09:24:54 +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 j517OpXW015111 for ; Wed, 1 Jun 2005 09:24:52 +0200 (CEST) Received: from (150.146.129.253) by e1000.artov.rm.cnr.it via smtp id 3d98_32e4e852_d26e_11d9_81ca_0002b3da0f69; Wed, 01 Jun 2005 09:24:32 +0200 (CEST) Received: (qmail 24878 invoked by uid 508); 1 Jun 2005 07:24:41 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.032081 secs); 01 Jun 2005 07:24:41 -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 ; 1 Jun 2005 07:24:41 -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 ; Wed, 1 Jun 2005 09:24:41 +0200 Message-ID: <20050601092441.99iuzngajagowosc@webmail.sic.rm.cnr.it> Date: Wed, 1 Jun 2005 09:24:41 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Fwd: Txx 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: 2005.5.31.45 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 ----- Messaggio inoltrato da Hessman@Astro.physik.Uni-Goettingen.DE ----- Data: Mon, 30 May 2005 13:23:44 +0200 Da: "Frederic V. \\Rick\\ Hessman" Rispondi-A: "Frederic V. \\Rick\\ Hessman" Oggetto: Txx A: ucd@ivoa.net 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 ------------------------------------------------------------------------ ------------------------- ----- Fine messaggio inoltrato. ----- ============================================================================== 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-sci@eso.org Wed Jun 1 09:27:22 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 j517RHaJ013232 for ; Wed, 1 Jun 2005 09:27:17 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j517RHaS013231 for ucd-sci-outgoing; Wed, 1 Jun 2005 09:27:17 +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 j517RCaJ013224 for ; Wed, 1 Jun 2005 09:27:13 +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 j517RAXW015166 for ; Wed, 1 Jun 2005 09:27:11 +0200 (CEST) Received: from (150.146.129.253) by e1000.artov.rm.cnr.it via smtp id 3d44_859f77a6_d26e_11d9_9410_0002b3da0f69; Wed, 01 Jun 2005 09:26:51 +0200 (CEST) Received: (qmail 25524 invoked by uid 508); 1 Jun 2005 07:27:04 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.037663 secs); 01 Jun 2005 07:27:04 -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 ; 1 Jun 2005 07:27:04 -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 ; Wed, 1 Jun 2005 09:27:04 +0200 Message-ID: <20050601092704.10nrsjdzawis0gog@webmail.sic.rm.cnr.it> Date: Wed, 1 Jun 2005 09:27:04 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Inoltro: SciBoard MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1 Content-Disposition: inline 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: 2005.5.31.44 X-Virus-Scanned: by amavisd-new Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id j517RGaJ013228 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 ----- Messaggio inoltrato da jcm@head.cfa.harvard.edu ----- Data: Mon, 30 May 2005 15:38:49 -0400 (EDT) Da: Jonathan McDowell Rispondi-A: Jonathan McDowell Oggetto: SciBoard A: andrea@rm.iasf.cnr.it Andrea. very slow email connection here at aas.. > > A. Roadmap. > Our goal is very simple: we need to stabilize (which means adding, deleting, > transforming ) the present draft list of ucd-words, that you can find at > > http://cdsweb.u-strasbg.fr/UCD/ucd1p-words.txt (just the list) > http://www.ivoa.net/internal/IVOA/IvoaUCD/WD-UCDlist-20050429.pdf (the WD > document) > > in order to (i) reach consensus, and (ii) be able to promote the list (and > the associated document) to the level of IVOA Proposed Recommendation as > soon as possible (within June). OK. Doesn't need to be complete right?: in other words deleting and transforming are more important than adding, which can be done later. > > B. The Board > 1. Duration. > There will be a Sci-Board as long as UCDs will be in use in the VO, in order > to maintain the vocabulary. The mission of the board is described in the > main UCD document, that you can find at > > http://www.ivoa.net/Documents/latest/UCD.html > > now under minor revisions as suggested during the Exec Meeting in Kyoto. > It is possible that in the future the Exec could change the mission to suit > new needs of the VO. Agreed. > > 2. Participation. > Participation is on a voluntary basis. Colleagues can ask the chair of the > Board to be inserted in (or deleted from) the mailing list of the Board, > and to work for a specific task (see below). > > 3. Chair > For the transition period required to set up the Board and let it run, I > will act as chair person of the Board (by the way, setting up the Board > and upgrading the present list of UCD-words to the level of IVOA PR is a > formal action for the chairman of the UCD-WG). I propose to go for an > election of the chairman of the Board in a month from now. > > C. Organization > 1. What (Tasks) > Time is very short, at least for this first phase of our work. I propose > then to define a number of key tasks and form task-groups on different > aspects of the vocabulary. The most urgent cases were well pinned down > during the last InterOp Meeting. My first draft proposal is to organize our > work around the following tasks: > > T1: the "velocity" and the resolution(s) problems > T2: theory and simulations (sim ?) > T3: at/mol physics > T4: curation (humans, organizations) and other "meta"-likes > T5: flux (total, net, backgr. and various "flux densities") and time (period > of, instant of) > T6: solar system > Txx : ?? OK > T0: Coordination, general issues, not included in the above Ts. > Like the Board, tasks are not "closed". The discussion is open ("plenary") > and contributions are welcome from every member of the Board. It will help > people with an analytical mind (like mine!) to see "T5" appear in the > subject of your message, if dealing with "net flux" or mid-time of > exposure. > > We need a coordinator for each task, with the responsibility to make a final > proposal to the Board. > There is nothing formal in the following list of people, I'm just asking > them to pay more attention to the discussion relevant to the corresponding > task, and summarize the discussion to the Board in due time. > Making use of the list of members (as of today) I propose the following > coordinators: > > T0 General Andrea > T1 Velocity/resolution Alberto Micol > T2 Theory/simulations Volunteer(?) > T3 At/Mol physics Marie-Lise Dubernet > T4 Meta Sébastien D. > T5 flux/time Jonathan MD > T6 Solar system Pierre Didelon > Agreed. Gerard, or Laurie Shaw maybe, as theory? > 2. How > Through the Board's mailing list. Always "reply to all". The chair will > record all messages. > In this first phase of our work time is very short. So please answer within > the given deadlines. We won't wait for late messages. You need to make a "ucd-board@ivoa.net" mailing list so we don't have to all rely on 'reply' working right. I guess Markus or Marco can help with that? > > 3. When > FIRST ACTION: please comment on the above organization/rules/tasks within > Thursday the 2nd of June. Comments above. Basically fine. Jonathan > > This message is sent (for the last time) also to the wider interop@ivoa.net > community to ask the laziest to join in. > > Best regards > > Andrea Solar System UCDs (really Astronomical Object UCDs): they will not be UCDs per the PR. But IVOA may need such a list and a UCD-compatible syntax may be appropriate. If the UCD/Semantics group doesn't want to take that work on, the DM group should probably do it. I think either group could do it, provided we keep the distinction between the two lists (UCDs, as semantics for astronomical non-object concepts, and the other list, as semantics for astronomical objects). - Jonathan ----- Fine messaggio inoltrato. ----- ============================================================================== 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-sci@eso.org Wed Jun 1 09:28:13 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 j517S7aJ013387 for ; Wed, 1 Jun 2005 09:28:07 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j517S7iX013386 for ucd-sci-outgoing; Wed, 1 Jun 2005 09:28:07 +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 j517S3aJ013371 for ; Wed, 1 Jun 2005 09:28:03 +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 j517S1XW015195 for ; Wed, 1 Jun 2005 09:28:02 +0200 (CEST) Received: from (150.146.129.253) by e1000.artov.rm.cnr.it via smtp id 3bb8_a3dfc7c0_d26e_11d9_8787_0002b3da0f69; Wed, 01 Jun 2005 09:27:42 +0200 (CEST) Received: (qmail 25598 invoked by uid 508); 1 Jun 2005 07:27:55 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.036998 secs); 01 Jun 2005 07:27:55 -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 ; 1 Jun 2005 07:27:55 -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 ; Wed, 1 Jun 2005 09:27:55 +0200 Message-ID: <20050601092755.aupeljrjs9pcg04o@webmail.sic.rm.cnr.it> Date: Wed, 1 Jun 2005 09:27:55 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Fwd: SciBoard 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: 2005.5.31.44 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 ----- Messaggio inoltrato da derriere@newb6.u-strasbg.fr ----- Data: Tue, 31 May 2005 10:35:14 +0200 Da: Sebastien Derriere Rispondi-A: Sebastien Derriere Oggetto: Re: Inoltro: SciBoard A: Andrea Preite Martinez , jcm@head.cfa.harvard.edu > > Solar System UCDs (really Astronomical Object UCDs): > they will not be UCDs per the PR. But IVOA may need such a list > and a UCD-compatible syntax may be appropriate. If the UCD/Semantics > group doesn't want to take that work on, the DM group should > probably do it. I think either group could do it, provided we > keep the distinction between the two lists (UCDs, as semantics > for astronomical non-object concepts, and the other list, > as semantics for astronomical objects). > Hi Jonathan, There might be a slight misunderstanding on this. The planetary system community has worked on their needs to express the quantities they are measuring in their field with proper UCDs. You can see the result of this reflexion here: http://portail.imcce.fr/fr/expert/ssvo/wgovp/propucd.html I think these suggestions are worth examining, and they seem quite mature: why not taking them into account for the PR. I am less confident that we can incorporate in the PR all the astronomical object types/phenomenons that were discussed for VOEvent (is this what you call "semantics for astronomical objects"?). 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 ----- Fine messaggio inoltrato. ----- ============================================================================== 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 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 13:19:00 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 j51BIqaJ026484 for ; Wed, 1 Jun 2005 13:18:52 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j51BIq06026468 for ucd-sci-outgoing; Wed, 1 Jun 2005 13:18:52 +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 j51BIjaJ026429 for ; Wed, 1 Jun 2005 13:18:46 +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 j51BIi73021737 for ; Wed, 1 Jun 2005 13:18:44 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1DdRF8-0022DY-Gs; Wed, 01 Jun 2005 13:18:38 +0200 In-Reply-To: <20050601092755.aupeljrjs9pcg04o@webmail.sic.rm.cnr.it> References: <20050601092755.aupeljrjs9pcg04o@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: <214afc13b7e2902af7d44d1b6a062131@Astro.physik.Uni-Goettingen.DE> Content-Transfer-Encoding: 7bit Cc: Roy Williams From: "Frederic V. \"Rick\" Hessman" Subject: Re: SciBoard Date: Wed, 1 Jun 2005 13:21:04 +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: 2005.6.1.6 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 Sebastien Derriere said: > Solar System UCDs (really Astronomical Object UCDs): > they will not be UCDs per the PR. But IVOA may need such a list > and a UCD-compatible syntax may be appropriate. If the UCD/Semantics > group doesn't want to take that work on, the DM group should > probably do it. I think either group could do it, provided we > keep the distinction between the two lists (UCDs, as semantics > for astronomical non-object concepts, and the other list, > as semantics for astronomical objects). The reason for separating "astronomical non-object concepts" and "sematics for astronomical objects" escapes me entirely, even if it were possible to do so (which it isn't). At least someone agrees that a natural but major extension to UCD "may be appropriate"..... :-) The UCD group has already done a fine job of starting the listing of astronomical concepts (object and non-object). Do we really want DM (or even worse, VOEvent) to do the other job, even if there's no "model" behind the data model? The non-table extensions to UCD are so obvious, relatively limited in number, and totally driven by the requirement in a variety of VO-related efforts, i.e. can't wait for a year-long discussion of whether we want to proceed beyond VOTable. If the consenus within the ucd-sci board is that we only need a few more (or less) table labels, then VOEvent or RTML will be forced to do the job which naturally should be done by UCD and the IVOA efforts to make VO tools as integrated as possible will suffer a major and utterly unnecessary setback. Don't worry - my blood pressure has returned to normal and I'll shut up. 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 13:45:59 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 j51BjlaJ001026 for ; Wed, 1 Jun 2005 13:45:47 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j51BjltT001025 for ucd-outgoing; Wed, 1 Jun 2005 13:45:47 +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 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@eso.org Precedence: bulk Reply-To: "Patricio F. Ortiz" 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-sci@eso.org Wed Jun 1 15:55:00 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 j51DsnaJ026751 for ; Wed, 1 Jun 2005 15:54:49 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j51DsnlB026747 for ucd-sci-outgoing; Wed, 1 Jun 2005 15:54:49 +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 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-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net 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 15:56:35 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 j51DuNaJ027547 for ; Wed, 1 Jun 2005 15:56:23 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j51DuNi3027546 for ucd-sci-outgoing; Wed, 1 Jun 2005 15:56:23 +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 j51DuGaJ027524 for ; Wed, 1 Jun 2005 15:56:16 +0200 (MEST) Received: from mailhost.u-strasbg.fr (mailhost.u-strasbg.fr [130.79.200.155]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51DuEXW027123 for ; Wed, 1 Jun 2005 15:56:14 +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 j51Du7nv086616 ; Wed, 1 Jun 2005 15:56:07 +0200 (CEST) Message-ID: <429DBE76.DD411C81@astro.u-strasbg.fr> Date: Wed, 01 Jun 2005 15:56:06 +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-sci@ivoa.net Subject: ucdComments page Content-Type: text/plain; charset=iso-8859-1 Content-Transfer-Encoding: 8bit X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-1.6 (mailhost.u-strasbg.fr [130.79.200.155]); Wed, 01 Jun 2005 15:56:08 +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: 2005.6.1.11 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 Hi all, An answer to both Pierre and Miguel: Pierre Didelon wrote: > > Is there a formal/official way to do this? > Can people who are not part of the board submit modifications? How? > Is there an entry point for the community outside the board? > What is the "good" submission path or procedure? > Four questions for the same pb is perhaps enough! :-D > Cordially, > Pierre Miguel Cerviño wrote: > > Additionally, should be the UCDs posted at: > > http://cdsweb.u-strasbg.fr/UCD/cgi-bin/comment/ucdComments?sort=C > > included in the draft-list? Now that we have a proper scientific board, with a mailing-list that is archived (1), etc... we might close submissions on the aforementioned web page, and redirect instead people from the community to the ucd-sci@ivoa.net for their comments/suggestions. This would avoid confusion: the sci-board would clearly be the only entry point for UCD curation. If noone disagrees, I'll disable posting on the ucdComments page, and invite submissions by email to ucd-sci@ivoa.net. And we can discuss some of the suggestions that are still unanswered on that page! Sebastien. 1: http://www.ivoa.net/forum/ucd-sci/ -- _______ / ~ /, 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-sci@eso.org Wed Jun 1 16:50:45 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 j51EocaJ009293 for ; Wed, 1 Jun 2005 16:50:39 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j51EocMA009290 for ucd-sci-outgoing; Wed, 1 Jun 2005 16:50:38 +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 j51EoWaJ009264 for ; Wed, 1 Jun 2005 16:50:32 +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 j51EoU73029472 for ; Wed, 1 Jun 2005 16:50:31 +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 j51EoPsS037470 for ; Wed, 1 Jun 2005 16:50:25 +0200 (CEST) Message-ID: <429DCB30.C9F96D0E@astro.u-strasbg.fr> Date: Wed, 01 Jun 2005 16:50:24 +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-sci@ivoa.net Subject: Re: T0 : extensions to em, obs, spect, instr References: <429C61EF.4020300@cea.fr> 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]); Wed, 01 Jun 2005 16:50:25 +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: 2005.6.1.13 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 Pierre Didelon wrote: > > UCD must define preferentially concept I suppose, isn't it? "Frederic V. \"Rick\" Hessman" wrote: > > The reason for separating "astronomical non-object concepts" and > "sematics for astronomical objects" escapes me entirely, even if it > were possible to do so (which it isn't). At least someone agrees that > a natural but major extension to UCD "may be appropriate"..... :-) Hi, Reading the last messages, I realize that we must be *very* careful with the vocabulary we use (especially as members of a board aiming at describing semantic contents!). I have already experienced how words like "objects", "concepts" and "types" can be (mis)understood when discussing across (and even within) different domains (mainly astronomy and computer science). Let me explain a few points that don't seem clear: Concept / properties : Following the ontology vocabulary, a *concept* is something abstract (can be seen as a class in object-oriented programming). This concept can have *properties*. When you define an *instance* of a concept, you associate values to the various properties. example: "telescope" can be seen as a concept (something abstract). Several properties can be associated to the concept of a telescope (its name, size, mass, location, ...). A particular telescope (one that you can see, or observe with) will be an instance of the concept "telescope". In the UCD vocabulary, most of the words correspond to *properties*. Because some properties are common to different concepts, we also created some UCD-words corresponding to *concepts*, and we can build complete UCDs by writing: "property;concept". This was done to reduce the number of words: for M properties and N concepts, this leads to N+M words instead of N*M. For the example above, we have the concept of telescope: "instr.tel". It can have a name: ucd="meta.id;instr.tel", a size: ucd="phys.size.diameter;instr.tel", a location, eg: ucd="pos.earth.lon;instr.tel" and ucd="pos.earth.lat;instr.tel", ... Basically, concepts were only introduced in the vocabulary for allowing re-usability of words. But the most important UCD-words are those describing properties: they are used to say what a quantity (can be a number or a string) is. Objects / non-objects : I'm confused with the "astronomical non-object concepts" and "sematics for astronomical objects" expressions. Astronomical objects (I understand sources detected in the sky, here) are named individually according to a controlled Nomenclature. The UCD have no role to play in this nomenclature. But there is one UCD word to say that a quantity is an object's name: meta.id : Identifier, name or designation Or maybe we can write: "meta.id;src" e.g. Currently, most of the existing UCD words are used to identify the *properties* of the astronomical objects (detected sources). 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-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-sci@eso.org Wed Jun 1 17:55:07 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 j51Ft0aJ024462 for ; Wed, 1 Jun 2005 17:55:00 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j51Ft0n4024460 for ucd-sci-outgoing; Wed, 1 Jun 2005 17:55:00 +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 j51FsuaJ024398 for ; Wed, 1 Jun 2005 17:54:56 +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 j51FssXW002646 for ; Wed, 1 Jun 2005 17:54:54 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1DdVYP-0027dc-47 for ucd-sci@ivoa.net; Wed, 01 Jun 2005 17:54:49 +0200 Mime-Version: 1.0 (Apple Message framework v622) In-Reply-To: <429DCB30.C9F96D0E@astro.u-strasbg.fr> References: <429C61EF.4020300@cea.fr> <429DCB30.C9F96D0E@astro.u-strasbg.fr> Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <868c9786a97ac1836b54c4783c304dc7@Astro.physik.Uni-Goettingen.DE> Content-Transfer-Encoding: 7bit From: "Frederic V. \"Rick\" Hessman" Subject: Re: T0 : extensions to em, obs, spect, instr Date: Wed, 1 Jun 2005 17:57:15 +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: 2005.6.1.16 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 3:54 pm, Pierre Didelon wrote: > 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, No problem at all :-) > 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! This is why I probably sound somewhat exasperated: I keep feeling that something which sounds so simple, so necessary, and so obvious is meeting such resistance. I didn't join to partake in abstract philosophical discussions about ontological problems but to be able to teach my software how to handle events and observing requests. Thus, the whole goal has to be defining something which is exactly what you want: "good (enough) level of abstraction", "widely re-useable" and certainly "precise enough to be useful at all". On 1 Jun 2005, at 4:50 pm, Sebastien Derriere wrote: > Basically, concepts were only introduced in the vocabulary for > allowing > re-usability of words. But the most important UCD-words are those > describing properties: they are used to say what a quantity (can be a > number or a string) is. Exactly. Now just abstract that idea to include not just numbers or strings but anything which the VO can deal with: images, spectra, astronomical events, generic classifications,.... Saying "what a quantity... is" is just naming it, so anything which needs to be identified deserves an official VO "name" (not to be confused with names like "Sebastien" or "NGC1234"). UCD has done this for table-like quantities, so why not extend it for the rest of us? > I'm confused with the "astronomical non-object concepts" and > "sematics for astronomical objects" expressions. > Astronomical objects (I understand sources detected in the sky, here) > are > named individually according to a controlled Nomenclature. The UCD have > no role to > play in this nomenclature. ... and no one is saying that it should. I want to name concepts, not objects. > Currently, most of the existing UCD words are used to identify > the *properties* of the astronomical objects (detected sources). Exactly, except properties like "being a spiral galaxy" are not yet allowed even though properties like "being the rotation rate" are. Being a spiral galaxy in the VO universe shouldn't be tied to the string "spiral galaxy" but to an official VO concept, e.g. src.class.galaxy.spiral. On 1 Jun 2005, at 1:44 pm, Patricio F. Ortiz wrote: > 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. If the present UCD weren't handy for other purposes, we frankly wouldn't be interested in extending it. Much more important, though, is the idea that a general UCD naming all the needed VO concepts forms the lingua franca by which VO tools, apps, processes, data, interactions,... can at least agree about what they're talking about. If UCD doesn't do this, then someone else will and you'll be forced in the long run to abandon UCD, because we don't need two ways of expressing ourselves and maintaining two or more dictionaries will never work. > 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. But this is exactly what tools like sextractor do: they tell you what it thinks zillions of objects are. Yes, the primitive versions just give you things like phot.mag and pos.eq.ra, but the more "intelligent" ones will tell you if the object is a spiral or an elliptical galaxy. If the large surveys don't start identifying objects this explicitly, then they'll only produce petabytes of useless garbage. Add the time domain (eg LSST) and you'll have a problem if there isn't also something like src.class.star.variable and event.eclipse, because otherwise they'll have to use strings. > 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? This is getting away from "concepts" and toward "processes" and "models". Don't want to touch this can of worms! Suffice it to say that something like obs.image.calibrated obs.image.uncalibrated would be handy, but connecting this to the correct obs.calib.flatfield isn't the job of UCD. > 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). The point is that naming in the sense of "RXJ 1234-567" is fine if that's what you want, but often one couldn't care less what the official name is as long as one knows what the object is generically. > 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 :-) That's exactly what VOEvent is and why I'm here fighting ;-) > 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. Putting it in "phys" makes more sense to me: while "gw" is ok, having "nd" means adding "ad" (axion detection), "crd" (cosmic-ray detection),.... If "em" is just the physical concept of electromagnetic radiation, then one could argue that it belongs in phys too. If "em" is there to descibe the means by which an observation was made, then "em=emission" could include gravitational waves and neutrinos and other things. I know, I know, there are probably endless discussions about where a concept belongs (lower level, higher level,..). I'd argue that naming the concepts in the long run is enough: the people who will do the ontologies won't care what we've called it officially. There will never be the perfect set of concept names but concepts are so heterogeneous and infinitely useful. Still, better to have ANY name at all than NO name at all. 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 18:09:00 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 j51G8saJ027247 for ; Wed, 1 Jun 2005 18:08:54 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j51G8sQF027246 for ucd-sci-outgoing; Wed, 1 Jun 2005 18:08:54 +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 j51G8oaJ027241 for ; Wed, 1 Jun 2005 18:08:50 +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 j51G8lXW003179 for ; Wed, 1 Jun 2005 18:08:48 +0200 (CEST) Received: from (150.146.129.253) by e1000.artov.rm.cnr.it via smtp id 7d58_654ef938_d2b7_11d9_97c3_0002b3da0f69; Wed, 01 Jun 2005 18:08:30 +0200 (CEST) Received: (qmail 27609 invoked by uid 508); 1 Jun 2005 16:08:41 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.03028 secs); 01 Jun 2005 16:08:41 -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 ; 1 Jun 2005 16:08:41 -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 ; Wed, 1 Jun 2005 18:08:41 +0200 Message-ID: <20050601180841.chccno54i8g7ksog@webmail.sic.rm.cnr.it> Date: Wed, 1 Jun 2005 18:08:41 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: cross-posting!! 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: 2005.6.1.17 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 Dear all, could you please STOP cross-posting your messages? The manager of the IVOA mailing list was so kind to open for the discussion two new mailing lists. After half a day he is already asking himself if that was of any use, because people continues to send discussion mails also to ucd/voevents/... lists!! Thank you for your attention. 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-sci@eso.org Wed Jun 1 18:44:10 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 j51Gi4aJ002814 for ; Wed, 1 Jun 2005 18:44:04 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j51Gi4WZ002813 for ucd-sci-outgoing; Wed, 1 Jun 2005 18:44:04 +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 j51Gi0aJ002785 for ; Wed, 1 Jun 2005 18:44:00 +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 j51Ghw73004128 for ; Wed, 1 Jun 2005 18:43:58 +0200 (CEST) Received: from argiope.saclay.cea.fr (argiope.saclay.cea.fr [132.166.192.108]) by cirse.extra.cea.fr (8.13.4/8.13.4/CEAnet-Internet.5.0) with ESMTP id j51GhrMe007594 for ; Wed, 1 Jun 2005 18:43:53 +0200 (MEST) Received: from pisaure.intra.cea.fr (unverified) by argiope.saclay.cea.fr (Content Technologies SMTPRS 4.3.17) with ESMTP id for ; Wed, 1 Jun 2005 18:43:52 +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 j51GfJBd024759 for ; Wed, 1 Jun 2005 18:41:19 +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 j51GhpbG013948 for ; Wed, 1 Jun 2005 18:43:51 +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 j51GiOe5027027 for ; Wed, 1 Jun 2005 18:44:25 +0200 (MEST) Message-ID: <429DE5C6.40809@cea.fr> Date: Wed, 01 Jun 2005 18:43:50 +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: ucd-sci@ivoa.net Subject: Re: T0 : extensions to em, obs, spect, instr References: <429C61EF.4020300@cea.fr> <429DCB30.C9F96D0E@astro.u-strasbg.fr> <868c9786a97ac1836b54c4783c304dc7@Astro.physik.Uni-Goettingen.DE> In-Reply-To: <868c9786a97ac1836b54c4783c304dc7@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: 2005.6.1.16 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 Frederic V. "Rick" Hessman wrote: > On 1 Jun 2005, at 3:54 pm, Pierre Didelon wrote: > >> 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, > > > No problem at all :-) Ouf/Ah! > >> 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! > > > This is why I probably sound somewhat exasperated: I keep feeling that > something > which sounds so simple, so necessary, and so obvious is meeting such > resistance. > I didn't join to partake in abstract philosophical discussions about > ontological > problems but to be able to teach my software how to handle events and > observing > requests. Thus, the whole goal has to be defining something which is > exactly > what you want: "good (enough) level of abstraction", "widely > re-useable" and > certainly "precise enough to be useful at all". ;-) But something obvious or "natural" for somebody in a specific context can have diff. meaning for somebody else in another context. That's also why trying to convince colleagues of the usefullness of terms is important, it force to express the implicit part of the definition. See comment below on calib. The pb of galaxy.spiral is diff. I agree. > On 1 Jun 2005, at 4:50 pm, Sebastien Derriere wrote: [SNIP] >> Currently, most of the existing UCD words are used to identify >> the *properties* of the astronomical objects (detected sources). > > > Exactly, except properties like "being a spiral galaxy" are not yet > allowed > even though properties like "being the rotation rate" are. > > Being a spiral galaxy in the VO universe shouldn't be tied to the string > "spiral galaxy" but to an official VO concept, e.g. > src.class.galaxy.spiral. > :-( src.class.galaxy is perhaps ok (if I understand correctly the mail of Rob Seaman http://www.ivoa.net/forum/ucd-sci/0506/0015.htm) then spiral can be an "additional" property extracted from an enumerated list... official or project specific? Not clear for me. > [snipp] > > This is getting away from "concepts" and toward "processes" and "models". > Don't want to touch this can of worms! Suffice it to say that something > like > > obs.image.calibrated > obs.image.uncalibrated Calibrated means astrometrically and/or phtometrically calibrated? Relative or absolute? in which reference system? ... What about spectral data, interferogramm, cosmic ray and neutrino detection? All these data have diff. level of calibration, completly diff. one from the other. Do we need to define all these in UCD, or something more general like meta.dataset.status a property which can take values like raw, astrom.calib, photomCalib... or whatever needed by a project or a context. > > would be handy, but connecting this to the correct > > obs.calib.flatfield > > isn't the job of UCD. > Agree ;-). SY PiR From owner-ucd-sci@eso.org Wed Jun 1 19:26:26 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 j51HQGaJ010030 for ; Wed, 1 Jun 2005 19:26:16 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j51HQGhK010029 for ucd-sci-outgoing; Wed, 1 Jun 2005 19:26:16 +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 j51HQBaJ010015 for ; Wed, 1 Jun 2005 19:26:11 +0200 (MEST) Received: from mailhost.u-strasbg.fr (mailhost.u-strasbg.fr [130.79.200.158]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j51HQ9XW005956 for ; Wed, 1 Jun 2005 19:26:10 +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 j51HQ0pA046205 ; Wed, 1 Jun 2005 19:26:01 +0200 (CEST) Message-ID: <429DEFA7.197122FF@astro.u-strasbg.fr> Date: Wed, 01 Jun 2005 19:25:59 +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-sci@ivoa.net CC: Williams Roy 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> 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 [130.79.200.158]); Wed, 01 Jun 2005 19:26:01 +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: 2005.6.1.19 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 "Frederic V. \"Rick\" Hessman" wrote: > > 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!) > > I agree with you that nobody wants the first expression :o) But I'm also scared by the second one, because there is a lot of implicit knowledge in it: because I am human (and astronomer), I can understand it, but what would a computer understand? You are trying to express that the observation target has a name which is "NGC12345", and that it is a galaxy with a spiral Hubble type (right?). During the discussions in Kyoto, we discussed several ways of expressing all these informations, and we came with the following: Maybe that could also be ? > 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. Not quite. When you say: you indicate that the value 12.3 represents a magnitude. Whereas is ambiguous: you implicitly conceptualize a property of the source (the morphological type), and you use an attribute ("name") to give a value ("NGC12345") that refers to the contents of the "ucd" attribute. As we speak, we often make the simplification name-of-a-thing=thing, but machines won't like it... > What we have now is the possibility > > > spiral galaxy > In this example, does "type" mean something precise? In fact, the contents of the "ucd" attribute gives the semantic type of the value that is associated. That is why you can use neutral tags (param) in the schema with ucd attributes: . If you already give special names to your schema elements, then you implicitly give the semantic type of their contents: no need for ucd! 12.3 instead of 12.3 Basically, if all elements of your xml schema are already strongly semantically typed... you don't need UCDs - but you can do a mapping from your schema's elements to the corresponding UCDs. > 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"? Now we come to the crucial point of the discussion: how to standardize the writing of possible values of astronomical object types (in the sense of object classification)? Which I agree we do need in the VO. Note however that instead of saying: "This object is a spiral galaxy", I'd rather say "The result of the classification process gives for this object the value [galaxy] for the source class, and the value [spiral] for the morphological type". Which is quite different, and hopefully much easier for a computer to understand. > 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. We must be very careful on the role that we choose for those the words we create. If we start creating words for each "concept" that we can name, we go the wrong direction.I'd create a UCD word for objects in the constellation Draco, or to see things like "pos.eq.dec.north". I think the best would be to come with a series of practical use cases where we need to manipulate information like that of "spiral galaxy", then see how we (humans+software) can handle it. > 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? I think the whole point is that "instrumental bandwidth" can readily be associated to a value. But what kind of value do you associate with "spiral galaxy"? Or would this "concept" be used to characterize a set of measures? If "src.class.galaxy.spiral" is only used to indicate without ambiguity to a software the morphological type of a source, then we could live with a value of (src.class) picked from an enumerated list of stadardized tokens (new UCD branch, pointer to a DM, or ontology distinguishing properly subtleties between Hubble and deVaucouleur classification, etc...) 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-sci@eso.org Wed Jun 1 20:04:13 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 j51I44aJ015232 for ; Wed, 1 Jun 2005 20:04:04 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j51I446n015229 for ucd-sci-outgoing; Wed, 1 Jun 2005 20:04:04 +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 j51I3jaJ015178 for ; Wed, 1 Jun 2005 20:03:46 +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 j51I3hXW006968 for ; Wed, 1 Jun 2005 20:03:43 +0200 (CEST) X-Spam-Checker-Version: SpamAssassin 3.0.3 (2005-04-27) 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=3.0.3 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 4.3.4) with ESMTPSA id 18524915; Wed, 01 Jun 2005 11:03:29 -0700 In-Reply-To: <429DEFA7.197122FF@astro.u-strasbg.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> <429DEFA7.197122FF@astro.u-strasbg.fr> Mime-Version: 1.0 (Apple Message framework v730) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: Content-Transfer-Encoding: 7bit From: Rob Seaman Subject: Re: T0 : extensions to em, obs, spect, instr Date: Wed, 1 Jun 2005 11:03:16 -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: 2005.6.1.19 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 Jun 1, 2005, at 10:25 AM, Sebastien Derriere wrote: > > > > > This is similar to how I was envisioning VOEvent usage. Rick should speak up (on whatever mailing list :-) if he sees this much differently. That said, I question whether these specific UCDs will survive our discussions. > instead of saying: "This object is a spiral galaxy", I'd rather say > "The result of the classification process gives for this object the > value [galaxy] for the source class, and the value [spiral] for the > morphological type". I think we need support for both. A name is sometimes both an enumerated value and a hierarchical classification. This is particularly true when the words express some underlying physics (or merely physical description) that is still plastic. We think we have a pretty good idea now what a "spiral galaxy" is. It wasn't so very long ago that we hadn't the slightest idea of its true nature. As long as astronomy is a living subject, there will be names with fluid meanings. Another concern is that a "src.class" expression would cover vast expanses of phase space - dozens of orders of magnitude in size (from chunks of rock in the solar system to cosmological structure) and having to distinguish between objects and processes with every possible physical/chemical/even biological property in play. Imagine a UCD-like expression of some field of biology - human anatomy, for instance. The corresponding sci.class would only have to distinguish a modest size range and modest variety of entities. (There are something like 200 cell types in the body.) What we're looking for is a reasonable way to separate the equivalent of cell biology from tissue biology from physiology at the level of organs. In particular, the allowed values for different UCDs become interrelated. (This seems likely to be something you folks have previously considered.) There are different values for src.morph.type depending on the value of src.class - and there are even different sets of UCDs entirely that are pertinent depending on the class. In short, Sebastien's view and Rick's view need to be synthesized into a common vision. > If we start creating words for each "concept" that we can name, we > go the wrong direction.I'd create a UCD word for objects > in the constellation Draco, But this is precisely what is done all the time. An astronomer pursues a new line of research and invents new terminology. Those terms may be representative of universal phenomena or may be specific to some area of study. We're hundreds of years past caring about constellations scientifically, but the details of some specific galaxy or cluster (M13, the Hyades) may be very important to describe accurately and precisely. To borrow a page from Rick, if UCDs don't support project specific glossaries, these will be expressed in some other fashion. Rob Seaman NOAO 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-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-sci@eso.org Thu Jun 2 10:48:06 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 j528luH8021343 for ; Thu, 2 Jun 2005 10:47:56 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j528lun8021342 for ucd-sci-outgoing; Thu, 2 Jun 2005 10:47:56 +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 j528lmH8021332 for ; Thu, 2 Jun 2005 10:47:49 +0200 (MEST) Received: from iaa13u.iaa.csic.es (iaa13u.iaa.csic.es [193.146.145.13]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j528llXW027576 for ; Thu, 2 Jun 2005 10:47:47 +0200 (CEST) Received: from [161.111.166.190] (wep50.iaa.csic.es [161.111.166.190]) by iaa13u.iaa.csic.es (8.9.3/8.9.1) with ESMTP id KAA05724 for ; Thu, 2 Jun 2005 10:47:41 +0200 (MET DST) Mime-Version: 1.0 (Apple Message framework v730) In-Reply-To: References: <20050531150728.fn26pj7v9fa8okc8@webmail.sic.rm.cnr.it> <94643280d46f33e5c88952d520f13f55@Astro.physik.Uni-Goettingen.DE> <429D79B3.3@cea.fr> <0a75e9e971886f955bcd71d196c35f79@Astro.physik.Uni-Goettingen.DE> <429DEFA7.197122FF@astro.u-strasbg.fr> Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: Content-Transfer-Encoding: 7bit From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Re: T0 : extensions to em, obs, spect, instr Date: Thu, 2 Jun 2005 10:48:01 +0200 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: 2005.6.2.1 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 Hello all, I give you my opinion in the present discussion from a naif point of view :) Something that has been rounding my mind when I think about UCDs is how much "detailed" it must be and what are the implications for others "fields" (I mean, value, units, datatype, etc...) in a "param" tag. I post some cases and latter my opinion below. - A given UCD would imply something for the "data type"?: Implies that this UCD has a value with datatype="float". It means that only in cases where it will be ambiguity the datatype should be defined? - Would be used a UCD alone without an associated value? It would be the case of: obs.image.uncalibrated that defines by itself a property of the image, what would be the "value" in that case? Yes, No? src.class.galaxy.spiral is a similar situation. - Should an UCD give some information about the zero-points or the units? phy.abund.X means implicitly abundance by mass or by number? It has sense phys.abund.X.byMass? Would a UDC distinguish between log Luminosity or Luminosity? (phot.flux and pho.mag have sense if this distinction is the work to do by the UCD; they are redundant if such a work must be done by "units") - Should an UCD be a "standard" assignation of the "name" filed? Well, now comes my point of view: I think that UDCs words are only valid if they do imply NO inference in the other possible "fileds", a ucd-tag have sense only as a complement of "value" or "datatype" fields (sometimes also units etc..., I am not compltly sure about "name") As an example which would be the UDC in a VOtable with this line: My Eliptical (E0) galaxies ........... ?? In this case I am not sure it it would be required an UDC of It would more useful a line with Any casee I aggre that there is a problem in how the "value" is spelling (Elliptical, E0,....) that would difficult any direct search, I think that it is a un-soluble problem: Each astronomer/VO developer etc has their own preferences (that is great, by the way).... and any machine program will have the preferences of its "owner" etc... Summing up. If we agree that every possible "field" in a "tag" must do their own job, I think that the UCDs definition becomes more simple (and in some way most useful)..... I do not know.... but maybe asked to each UCDs which range of values they my have would be useful.... Now, for practical issues :) I think that most of the discussion has been focus in the UCD "length": Or, UCD words-like vs. UCD-sentence-like. Here comes My suggestion. May be we can began in an atomized way: 1- Are all the "1st-atoms" in the list valid? (or it is needed more?, or less?) 2- Are the present words that contain two atoms valid? ......... In this case, I think, most of the present discussion would be related with the lower levels (words with many atoms), and whatever the final result we will have at least a list of really valid words :) cheers Miguel From owner-ucd-sci@eso.org Thu Jun 2 14:39:18 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 j52CdAH8002368 for ; Thu, 2 Jun 2005 14:39:11 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j52CdAXM002367 for ucd-sci-outgoing; Thu, 2 Jun 2005 14:39:10 +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 j52Cd4H8002352 for ; Thu, 2 Jun 2005 14:39:04 +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 j52Cd2XW004008 for ; Thu, 2 Jun 2005 14:39:02 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1DdoyP-000D0L-2n for ucd-sci@ivoa.net; Thu, 02 Jun 2005 14:38:57 +0200 Mime-Version: 1.0 (Apple Message framework v622) In-Reply-To: References: <20050531150728.fn26pj7v9fa8okc8@webmail.sic.rm.cnr.it> <94643280d46f33e5c88952d520f13f55@Astro.physik.Uni-Goettingen.DE> <429D79B3.3@cea.fr> <0a75e9e971886f955bcd71d196c35f79@Astro.physik.Uni-Goettingen.DE> <429DEFA7.197122FF@astro.u-strasbg.fr> Content-Type: text/plain; charset=ISO-8859-1; delsp=yes; format=flowed Message-Id: <3921b09bd80d7ddf22e0e6f24b9a7103@Astro.physik.Uni-Goettingen.DE> From: "Frederic V. \"Rick\" Hessman" Subject: Re: T0 : extensions to em, obs, spect, instr - FINAL COMMENT? Date: Thu, 2 Jun 2005 14:41:23 +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: 2005.6.2.8 X-Virus-Scanned: by amavisd-new Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id j52CdAH8002364 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 8:03 pm, Rob Seaman wrote: > On Jun 1, 2005, at 10:25 AM, Sebastien Derriere wrote: > >> >> >> >> >> > > This is similar to how I was envisioning VOEvent usage. Rick should > speak up (on whatever mailing list :-) if he sees this much > differently. That said, I question whether these specific UCDs will > survive our discussions. This is fine for VOTable, where "value" is really rather diffuse scientifically ("the thing in the table row and column with some scientific meaning given by the ucd") and where the main purpose is to recreate the non-astronomical thing "table" into an astronomical unit which can be processed. You really don't care if you have or or As soon as you get away from tables, things become more complex, since the "value" can - and SHOULD - take on more meaning. In VOEvent, the point is NOT to have a string which someone used to randomly label an object (the VOTable equivalent task), but to tell stupid computers that the object is something in particular. With there's no way to know if the class is "galaxies in general" or even "The Milky Way" unless the VO has an official dictionary saying that the "value" of "src.class" for galaxies in general should be "Galaxy" (a poor choice if you ask me, but...). Thus, I personally find the present model good for random information (non-classification tasks) but extremely bad for particular information (classification tasks). If the only way to express "spiral galaxy" is to use "src.class" = "Galaxy" and "src.morph" = "SC", then someone (i.e. a programmer) with have to deal with the fact that "src.morph" - a concept used for zillions of other astronomical objects not related to galaxies - may or may not be applicable to the object in question. That forces her/him to use an ontology :-( While I applaud those willing to tackle such, it'll be a long while until we have one which can be used in real applications. And all of this work simply because we don't have "src.galaxies.spiral" (note I've dropped "class" to reduce the number of hierarchies). > We think we have a pretty good idea now what a "spiral galaxy" is. It > wasn't so very long ago that we hadn't the slightest idea of its true > nature. As long as astronomy is a living subject, there will be names > with fluid meanings. True enough, but the point is we DO know what a "spiral galaxy" is right now, we already know of billions of them, and survey projects need NOW to be able to tell us that they've found one. Let's worry about the concepts we haven't developed when they appear. On 2 Jun 2005, at 10:48 am, Miguel Cerviño wrote: > In this case I am not sure it it would be required an UDC of It would > more useful a line with > > > Any casee I aggre that there is a problem in how the "value" is > spelling (Elliptical, E0,....) that would difficult any direct search, > I think that it is a un-soluble problem: Each astronomer/VO developer > etc has their own > preferences (that is great, by the way).... and any machine program > will have the preferences of its "owner" > etc... NO!!! The VO apps of the future will "know" how to express the concept of "elliptical galaxy" in a common fashion (otherwise they're too stupid to be able to talk to each other about them) but the human user see's what the human equivalent is supposed to be in terms s/he WANTS to see (e.g. in english, in french, or for a 3rd grade student in Malaysia,...). The ONLY question now is how difficult we want to make the life of VO programmers - nothing else! An astronomer who refuses to accept that somewhere buried in the VO software architecture there's a "src.galaxies.elliptical" or a "src.class"="Galaxy" + "src.morph"="elliptical" instead of the string "elliptische Galaxie" simply won't (and shouldn't) use the VO. Miguel's comment does raise a totally different issue which may explain why there's no confluence of ideas: do we want a VO architecture which is simply a more elegant means of letting a human user deal with complex sets of VO data and VO apps - in which case "Elliptical" will be fine to describe the galaxy since a human in there to interpret what it means - or do we want to use things like UCD's to permit computers to deal with this information without ANY human involved IN PRINCIPLE (e.g. automatic classification of zillions of LSST sources triggering robotic observations). My feeling is that the work on VOTable and UCD has been based largely on the former and I know that the work on VOEvent is largely based on the latter. Yes, this is oversimplified, but it would help to explain why we don't seem to be talking about the same thing...... Don't get me wrong - I think UCD's in their present form are great - but if this list is just about last-minute refining of the present list using the present limited set of officially allowed concepts, then please remove me so you won't have to be bothered by my rantings anymore. I'm sure you'll do a great job and we'll certainly use UCDs all over the place, but I'm then personally interested in something else and would then try to find a IVOA group doing the next - and unfortunately officially defined as different - task of teaching computers a minimal set of concepts needed to do automatic processing of VO information NOW without the use of ontologies (we just barely got our GRB colleagues to accept XML - wait until I tell them they're going to have to use OWL!). Seems a shame, but then the IVOA has historically been a pretty heterogeneous bunch and so yet another group doing some of the same work using a totally different approach won't be noticed. Computers are fast, databases can be linked, cross-references can be made, translators and parsers can be written, generations of students need to be given work, .... :-) 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 Thu Jun 2 15:25:09 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 j52DOxH8011068 for ; Thu, 2 Jun 2005 15:24:59 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j52DOxXj011058 for ucd-sci-outgoing; Thu, 2 Jun 2005 15:24:59 +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 j52DOlH8010956 for ; Thu, 2 Jun 2005 15:24:47 +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 j52DOj73007183 for ; Thu, 2 Jun 2005 15:24:45 +0200 (CEST) Received: from (150.146.129.253) by e1000.artov.rm.cnr.it via smtp id 15fe_a7638494_d369_11d9_8486_0002b3da0f69; Thu, 02 Jun 2005 15:24:32 +0200 (CEST) Received: (qmail 11993 invoked by uid 508); 2 Jun 2005 13:24:39 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.039207 secs); 02 Jun 2005 13:24:39 -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 Jun 2005 13:24:39 -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 ; Thu, 2 Jun 2005 15:24:38 +0200 Message-ID: <20050602152438.fdmq7yxtgdcgg40k@webmail.sic.rm.cnr.it> Date: Thu, 2 Jun 2005 15:24:38 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Sci-Board-3 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: 2005.6.2.10 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 ***Sci-Board-3 Dear all, I think it is time to remind you what the goal of the Sci-Board on a short time-scale is: we (eg: IVOA project and people) urgently need a stabilized version of the UCD vocabulary. Adds-on are possible in this phase, but in the short term (<1 month) the main job is to get a basic ?kernel? of ?stable? words that can be immediately used by data providers. The starting point is the list of words already available as an IVOA-WD. If the present version of the list is too much ?table/catalogue?-like for somebody's tastes, I remind that at CDS (just to quote one of the data centers) about 150.000 columns wait for a ?stable? ucd-vocabulary in order to be treated (e.g.: to have an ucd assigned to them), their number growing at the rate of 1000 per month. What I mean is: they are already there. This is why at the joint UCD-VOEvent session we decided to postpone the discussion on (to be precise, on the schema only, because actual UCDs are usable in other Event contexts/schemas) : to gather a real working vocabulary on events and associated hypothesis. The situation is not very simple : on one hand we have now a way (a way) to define -enough UCDs, on the other hand we need to have within the IVOA community (DM, Theory, VOEvent, ..) the possibility to express the same concepts using the same words. And, why not, using the same syntax already used for the UCDs. A way out is to be rigorous and at the same time. I remind you that in the actual version of UCDs we do have : in the sense that we do (we can) distinguish between the temperature of a star (its effective temperature) and that of a detector or instrument. We do distinguish between the name/identifier of an astronomical object and that of a telescope, instrument, or even a fov. In all these cases we use ucd-words describing as . While today an UCD like : src.galaxies.S0 would be meaningless, meta.id;src.galaxies.S0 would not. In the UCD context src.galaxies.S0 is only a secondary word, but in another context it could be used as primary. We can (I would say: we have to) work in this direction. I totally agree with Rick's final statement on ontologies: we need standards NOW, not in 30-40 man-years time! 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 ============================================================================== From owner-ucd-sci@eso.org Thu Jun 2 17:19:16 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 j52FJ9H8006505 for ; Thu, 2 Jun 2005 17:19:09 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j52FJ9B0006504 for ucd-sci-outgoing; Thu, 2 Jun 2005 17:19:09 +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 j52FIvH8006430 for ; Thu, 2 Jun 2005 17:18:57 +0200 (MEST) Received: from fed1rmmtao10.cox.net (fed1rmmtao10.cox.net [68.230.241.29]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j52FIs73011973 for ; Thu, 2 Jun 2005 17:18:55 +0200 (CEST) Received: from [10.0.1.32] (really [68.231.133.145]) by fed1rmmtao10.cox.net (InterMail vM.6.01.04.00 201-2131-118-20041027) with ESMTP id <20050602151844.XQRU20235.fed1rmmtao10.cox.net@[10.0.1.32]>; Thu, 2 Jun 2005 11:18:44 -0400 In-Reply-To: <20050602152438.fdmq7yxtgdcgg40k@webmail.sic.rm.cnr.it> References: <20050602152438.fdmq7yxtgdcgg40k@webmail.sic.rm.cnr.it> Mime-Version: 1.0 (Apple Message framework v730) Content-Type: multipart/alternative; boundary=Apple-Mail-2--168114231 Message-Id: <18AB023D-4017-4716-BA26-6642EA40EC36@noao.edu> Cc: Rob Seaman From: Rob Seaman Subject: Re: Sci-Board-3 Date: Thu, 2 Jun 2005 08:18:42 -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: 2005.6.2.14 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 --Apple-Mail-2--168114231 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed This is why I prefer separate threads on a single mailing list to attempts to segregate discussions up front into conceptually different mailing lists. There appear to be at least four different places to talk about UCDs/Ontologies. Either the members of those mailing lists overlap strongly - or they don't. In the former case, why have separate lists? In the latter case, some folks miss large parts of the conversation. In either case, administrivia messages proliferate trying to keep everybody in line. Oh, well...shall we take the more conceptual discussions over to ucd-tech? On Jun 2, 2005, at 6:24 AM, Andrea Preite Martinez wrote: > we (eg: IVOA project and people) urgently need a stabilized version > of the UCD vocabulary. Fine. (Although one might read discussion to date as an expression of a sense that this goal will not be trivial.) If the ucd-sci board is to focus exclusively on generating vocabulary, what we need is a structured discussion, not a free-for-all. Is there a specific action item on the table? "Provide vocabulary" ain't gonna cut it. > The starting point is the list of words already available as an > IVOA-WD. Reminder where that is? > we decided to postpone the discussion on I remind you that in the actual version of UCDs we do have > : in the sense that we do (we can) distinguish between the > temperature of a star (its effective temperature) and that of a > detector or instrument. We do distinguish between the name/ > identifier of an astronomical object and that of a telescope, > instrument, or even a fov. In all these cases we use ucd-words > describing as . It would be useful to those of us now joining the UCD conversation from outside to see such examples expressed in in their full and gory detail. > I totally agree with Rick's final statement on ontologies: we need > standards NOW, not in 30-40 man-years time! Rather, we need prototype solutions now. A standard itself cannot be reached via a short-cut. The ontologies will inevitably form the long term standards. UCDs and other semantic constructs will inevitably ultimately flow from the formalized ontologies. Astronomy is the oldest of the sciences - we have all the time in the world for these academic pursuits. In the mean time, pilot projects will produce prototype solutions that will serve the community's needs for a season before being supplanted by better technology layered on our always evolving understanding of the issues. Rob Seaman NOAO --Apple-Mail-2--168114231 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1 This is why I prefer separate = threads on a single mailing list to attempts to segregate discussions up = front into conceptually different mailing lists.=A0 There appear to be = at least four different places to talk about UCDs/Ontologies.=A0 Either = the members of those mailing lists overlap strongly - or they don't.=A0 = In the former case, why have separate lists?=A0 In the latter case, some = folks miss large parts of the conversation.=A0 In either case, = administrivia messages proliferate trying to keep everybody in line.=A0 = Oh, well...shall we take the more conceptual discussions over to = ucd-tech?

On Jun 2, 2005, at 6:24 AM, Andrea Preite = Martinez wrote:

we (eg: IVOA project and people) = urgently need a stabilized version of the=A0UCD = vocabulary.

Fine.=A0 (Although one might = read discussion to date as an expression of a sense that this goal will = not be trivial.)=A0 If the ucd-sci board is to focus exclusively on = generating vocabulary, what we need is a structured discussion, not a = free-for-all.=A0 Is there a specific action item on the table?=A0 = "Provide vocabulary" ain't gonna cut it.

The starting point is the list of words=A0already = available as an IVOA-WD.

Reminder where that = is?

we = decided to postpone the discussion on <UCDs and the = VOEvent

Define "postpone".=A0 The = VOEvent WG certainly intends that its prototypes be = fast-tracked.

I remind you that in the actual version of UCDs we = do have <objects>: in the=A0sense that we do (we can) distinguish = between the temperature of a star (its=A0effective temperature) and that = of a detector or instrument. We do=A0distinguish between the = name/identifier of an astronomical object and that=A0of a telescope, = instrument, or even a fov. In all these cases we use=A0ucd-words = describing <objects> as = <qualifiers>.

It would be useful to those of = us now joining the UCD conversation from outside to see such examples = expressed in in their full and gory detail.

I totally agree with Rick's = final statement on ontologies: we need standards=A0NOW, not in 30-40 = man-years time!

Rather, we need prototype = solutions now.=A0 A standard itself cannot be reached via a short-cut.=A0 = The ontologies will inevitably form the long term standards.=A0 UCDs and = other semantic constructs will inevitably ultimately flow from the = formalized ontologies.=A0 Astronomy is the oldest of the sciences - we = have all the time in the world for these academic pursuits.=A0 In the = mean time, pilot projects will produce prototype solutions that will = serve the community's needs for a season before being supplanted by = better technology layered on our always evolving understanding of the = issues.

Rob = Seaman
NOAO
= --Apple-Mail-2--168114231-- From owner-ucd-sci@eso.org Thu Jun 2 17:43:00 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 j52FgkH8011793 for ; Thu, 2 Jun 2005 17:42:47 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j52Fgkii011790 for ucd-sci-outgoing; Thu, 2 Jun 2005 17:42:46 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-sci@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 j52FggH8011782 for ; Thu, 2 Jun 2005 17:42:43 +0200 (MEST) Received: from [134.171.30.4] (nb008487.ads.eso.org [134.171.30.4]) by serapis.hq.eso.org (8.11.7+Sun/8.11.7) with ESMTP id j52FggE01716 for ; Thu, 2 Jun 2005 17:42:42 +0200 (MEST) Message-ID: <429F2907.1010201@eso.org> Date: Thu, 02 Jun 2005 17:43:03 +0200 From: "Marco C. Leoni" Organization: European Virtual Observatory @ESO User-Agent: Mozilla Thunderbird 1.0.2 (Windows/20050317) X-Accept-Language: en-us, en MIME-Version: 1.0 To: ucd-sci@ivoa.net Subject: Re: Sci-Board-3 References: <20050602152438.fdmq7yxtgdcgg40k@webmail.sic.rm.cnr.it> <18AB023D-4017-4716-BA26-6642EA40EC36@noao.edu> In-Reply-To: <18AB023D-4017-4716-BA26-6642EA40EC36@noao.edu> Content-Type: multipart/alternative; boundary="------------090606020208050507020105" 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 This is a multi-part message in MIME format. --------------090606020208050507020105 Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit Rob Seaman wrote: > [...] > >> The starting point is the list of words already available as an IVOA-WD. > > > Reminder where that is? It should be this one: http://www.ivoa.net/Documents/latest/UCDlist.html Cheers, Marco --------------090606020208050507020105 Content-Type: text/html; charset=ISO-8859-1 Content-Transfer-Encoding: 7bit Rob Seaman wrote:
[...]

The starting point is the list of words already available as an IVOA-WD.

Reminder where that is?

It should be this one:
    http://www.ivoa.net/Documents/latest/UCDlist.html


Cheers,
    Marco
--------------090606020208050507020105-- From owner-ucd-sci@eso.org Fri Jun 3 10:11:52 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 j538BgcT007003 for ; Fri, 3 Jun 2005 10:11:42 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j538BfFS007002 for ucd-sci-outgoing; Fri, 3 Jun 2005 10:11:41 +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 j538BbcT006994 for ; Fri, 3 Jun 2005 10:11:38 +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 j538BZXW005695 for ; Fri, 3 Jun 2005 10:11:35 +0200 (CEST) Received: from (150.146.129.253) by e1000.artov.rm.cnr.it via smtp id 65d8_1457b28a_d407_11d9_9325_0002b3da0f69; Fri, 03 Jun 2005 10:11:25 +0200 (CEST) Received: (qmail 13454 invoked by uid 508); 3 Jun 2005 08:11:29 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.055722 secs); 03 Jun 2005 08:11:29 -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 Jun 2005 08:11:29 -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 ; Fri, 3 Jun 2005 10:11:29 +0200 Message-ID: <20050603101129.diyu1dvr2wj4sg4g@webmail.sic.rm.cnr.it> Date: Fri, 3 Jun 2005 10:11:29 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Re: Sci-Board-3 References: <20050602152438.fdmq7yxtgdcgg40k@webmail.sic.rm.cnr.it> <18AB023D-4017-4716-BA26-6642EA40EC36@noao.edu> In-Reply-To: <18AB023D-4017-4716-BA26-6642EA40EC36@noao.edu> MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1; format="flowed" Content-Disposition: inline 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: 2005.6.2.45 X-Virus-Scanned: by amavisd-new Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id j538BfcT006999 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Quoting Rob Seaman : > On Jun 2, 2005, at 6:24 AM, Andrea Preite Martinez wrote: > >> we (eg: IVOA project and people) urgently need a stabilized version >> of the UCD vocabulary. > > Fine. (Although one might read discussion to date as an expression > of a sense that this goal will not be trivial.) If the ucd-sci board > is to focus exclusively on generating vocabulary, what we need is a > structured discussion, not a free-for-all. Is there a specific > action item on the table? "Provide vocabulary" ain't gonna cut it. Of course there is. You were probably late in joining the sci-board, and you missed it. The list was created , so the first messages were inserted in the list by hand. For reasons that I do not understand the message I'm talking about (Sci-Board-1) is there as subject, but not as content. I copy it here for you and those that joined late our list. ==========================Sci-Board-1=================================== Dear colleagues, this first message is for setting up our roadmap and organizing the Board and our work on the UCD-vocabulary.. A. Roadmap. Our goal is very simple: we need to stabilize (which means adding, deleting, transforming ) the present draft list of ucd-words, that you can find at http://cdsweb.u-strasbg.fr/UCD/ucd1p-words.txt (just the list) http://www.ivoa.net/internal/IVOA/IvoaUCD/WD-UCDlist-20050429.pdf (the WD document) in order to (i) reach consensus, and (ii) be able to promote the list (and the associated document) to the level of IVOA Proposed Recommendation as soon as possible (within June). B. The Board 1. Duration. There will be a Sci-Board as long as UCDs will be in use in the VO, in order to maintain the vocabulary. The mission of the board is described in the main UCD document, that you can find at http://www.ivoa.net/Documents/latest/UCD.html now under minor revisions as suggested during the Exec Meeting in Kyoto. It is possible that in the future the Exec could change the mission to suit new needs of the VO. 2. Participation. Participation is on a voluntary basis. Colleagues can ask the chair of the Board to be inserted in (or deleted from) the mailing list of the Board, and to work for a specific task (see below). 3. Chair For the transition period required to set up the Board and let it run, I will act as chair person of the Board (by the way, setting up the Board and upgrading the present list of UCD-words to the level of IVOA PR is a formal action for the chairman of the UCD-WG). I propose to go for an election of the chairman of the Board in a month from now. C. Organization 1. What (Tasks) Time is very short, at least for this first phase of our work. I propose then to define a number of key tasks and form task-groups on different aspects of the vocabulary. The most urgent cases were well pinned down during the last InterOp Meeting. My first draft proposal is to organize our work around the following tasks: T1: the "velocity" and the resolution(s) problems T2: theory and simulations (sim ?) T3: at/mol physics T4: curation (humans, organizations) and other "meta"-likes T5: flux (total, net, backgr. and various "flux densities") and time (period of, instant of) T6: solar system Txx : ?? T0: Coordination, general issues, not included in the above Ts. Like the Board, tasks are not "closed". The discussion is open ("plenary") and contributions are welcome from every member of the Board. It will help people with an analytical mind (like mine!) to see "T5" appear in the subject of your message, if dealing with "net flux" or mid-time of exposure. We need a coordinator for each task, with the responsibility to make a final proposal to the Board. There is nothing formal in the following list of people, I'm just asking them to pay more attention to the discussion relevant to the corresponding task, and summarize the discussion to the Board in due time. Making use of the list of members (as of today) I propose the following coordinators: T0 General Andrea T1 Velocity/resolution Alberto Micol T2 Theory/simulations Volunteer(?) T3 At/Mol physics Marie-Lise Dubernet T4 Meta Sébastien D. T5 flux/time Jonathan MD T6 Solar system Pierre Didelon 2. How Through the Board's mailing list. Always "reply to all". The chair will record all messages. In this first phase of our work time is very short. So please answer within the given deadlines. We won't wait for late messages. 3. When FIRST ACTION: please comment on the above organization/rules/tasks within Thursday the 2nd of June. This message is sent (for the last time) also to the wider interop@ivoa.net community to ask the laziest to join in. Best regards Andrea ============== end of Sci-Board-1======================================= >> we decided to postpone the discussion on Define "postpone". The VOEvent WG certainly intends that its > prototypes be fast-tracked. As above, I copy for you my second message Sci-Board-2. ======================Sci-Board-2========================================= Dear colleagues, I see from the first answers to Sci-Board-1 that thinks are not clear for everybody: 1. Please, REPLY TO ALL the members of the Board, not to the ucd-list nor to my address. Remember that not all the members of the Board are also members of the UCD-WG. You can "cc" to your pet-list, I don't care, but make sure that at least the Board can read your message. 2. When suggesting new UCD-words, please ask yourself which kind of "quantity" you want to describe or, if not a quantity, which kind of attribute (qualifier/modifier). By the way, our mission is to stabilize and maintain a list of "words", NOT a list of UCDs. Syntax will take care of how to build UCDs, based on the classification of the word (e.g. P/Q/S syntactic flag). 3. For what VOEvent is concerned, please have a look at the conclusions of the joint session UCD/VOEvent at http://www.ivoa.net/twiki/bin/view/IVOA/InterOpMay2005UCD We will discuss Event vocabulary at the end of the year, when a first bottom-up list of terms will be available. 4. Sorry, there isn't such a thing as Solar System UCDs. I remind you that the IVOA (Proposed) Recommendation on UCDs explicitly forbids UCDs like "star", "galaxy", or "Sun", "my_pet_object", and so on. On the contrary, qualifiers like "stellar", "galactic", "solar" can be valid atoms. Regards Andrea =======================end of Sci-Board-2================================= >> I remind you that in the actual version of UCDs we do have >> : in the sense that we do (we can) distinguish between the >> temperature of a star (its effective temperature) and that of a >> detector or instrument. We do distinguish between the name/ >> identifier of an astronomical object and that of a telescope, >> instrument, or even a fov. In all these cases we use ucd-words >> describing as . > > It would be useful to those of us now joining the UCD conversation > from outside to see such examples expressed in in their full and gory > detail. You can use the UCD builder on line at: http://vizier.u-strasbg.fr/UCD/cgi-bin/descr2ucd >> I totally agree with Rick's final statement on ontologies: we need >> standards NOW, not in 30-40 man-years time! > > Rather, we need prototype solutions now. I don't see why you say . There is not contradiction. I'm talking about STANDARDS NOW. STANDARDS LATER > ... The ontologies will inevitably form the long term standards... need prototyping now. > Rob Seaman > NOAO Andrea From owner-ucd-sci@eso.org Mon Jun 6 19:22:30 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 j56HMNoS028235 for ; Mon, 6 Jun 2005 19:22:23 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j56HMNtB028234 for ucd-sci-outgoing; Mon, 6 Jun 2005 19:22:23 +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 j56HMHoS028217 for ; Mon, 6 Jun 2005 19:22:18 +0200 (MEST) Received: from iaa13u.iaa.csic.es (iaa13u.iaa.csic.es [193.146.145.13]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j56HMG73002021 for ; Mon, 6 Jun 2005 19:22:16 +0200 (CEST) Received: from [161.111.166.190] (wep50.iaa.csic.es [161.111.166.190]) by iaa13u.iaa.csic.es (8.9.3/8.9.1) with ESMTP id TAA06352 for ; Mon, 6 Jun 2005 19:22:10 +0200 (MET DST) Mime-Version: 1.0 (Apple Message framework v730) In-Reply-To: <20050603101129.diyu1dvr2wj4sg4g@webmail.sic.rm.cnr.it> References: <20050602152438.fdmq7yxtgdcgg40k@webmail.sic.rm.cnr.it> <18AB023D-4017-4716-BA26-6642EA40EC36@noao.edu> <20050603101129.diyu1dvr2wj4sg4g@webmail.sic.rm.cnr.it> Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: Content-Transfer-Encoding: 7bit From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: T0: UCDs for "em" Date: Mon, 6 Jun 2005 19:22:29 +0200 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: 2005.6.6.18 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 Dear all, I just revised the "em" UDCs and I post here some suggestions. I had just rewriten the whole "Q" list and added some entries, taken from the 27-Feb 2005 Working Draft on IVOA SED Data Model (marked with *). For clarity I has put together "Q" UCDs and "S" UCDs, the latter writen in increasing energy order. First I center in "Q" UCDs, and I propose to keep: Q|em.energy |Energy value in the em frame Q|em.freq |Frequency value in the em frame Q|em.wavenumber |Wavenumber value in the em frame Q|em.wl |Wavelength value in the em frame - Include: Q|em.wl.air* |Wavelength value in the em frame in air frame somewhere it should be established default is vacuum? In most optical observation default is air and in UV vacuum as example, but SLOAN data release gives optical wl en vacuum... - Other suggestions in IVOA SED DM WD: Q|em.veloc* |Apparent radial velocity Q|em.veloc.radio* |radio velocity Q|em.veloc.optical* |optical velocity Q|em.veloc.beta* |velocity/cr - Changue from Q to E? Q|em.wl.central |Central wavelength Q|em.wl.effective |Effective wavelength I think that this UDCs does not corresponds to the EM but more important for photometric characterizations. I do not know About the characterization of the em spectrum by their energy ranges as proposed at: http://www.ivoa.net/internal/IVOA/IvoaUCD/NoteEMSpectrum-20040520.html I completely agree :) however, for clarity purpose and hogenity the UDCs I would suggest the following changues: em.IR.K --> em.IR.2-3um em.IR.H --> em.IR1500-2000nm em.IR.J --> em.IR1000-1500nm em.opt.I --> em.opt.750-1000nm em.opt.R --> em.opt.600-750nm em.opt.V --> em.opt.500-600nm em.opt.B --> em.opt.400-500nm em.opt.U --> em.opt.300-400nm so there no will be confusion with fotometry bands (and machines always will found em.string.(number - number unit) that, I do not know, but may be is more easier) Analogously, for high energy: em.X-ray.soft --> em.X.120-2000eV em.X-ray.medium --> em.X.2-12keV em.X-ray.hard --> em.X.12-120keV em.gamma.soft --> em.gamma.120-500keV em.gamma.hard --> em.gamma.500-1000keV em.gamma.1-20MeV em.VHgamma (Very-high gamma: 20Mev-10GeV) em.VHgamma.20-100MeV em.VHgamma.100-1000MeV em.VHgamma.1-10GeV em.UHgamma (Ultra high gamma rays, cosmic ray- domain) em.UHgama.10-30GeV em.UHgama.30+GeV Here, the definitions for gamma-ray is a bit lossy, and I have not found a clear consensus between very-high and ultra-high gamma in the literature.... :( Finally, I think that the inclusion of em.line would be useful, but only for a very sort list of lines (like there is irregular verbs in any language that, by the way, corresponds to the most commonly used verbs) so (with a strong background of visual astronomy) I would agree with Hydrogen lines, but I do think that em.line.OIII should be depreciated (there is several OIII lines!, and if OIII is here, by not, O I, or H+K Ca II etc...? so I propose depreciate em.line.OIII ... so the list would be: S |em.line.HI |21cm hydrogen line S |em.line.Brgamma |Bracket gamma line S |em.line.Halpha |H-alpha line S |em.line.Hbeta |H-beta line S |em.line.Hgamma |H-gamma line Depreciated: S |em.line.OIII |[OIII] line Cheers Miguel From owner-ucd-sci@eso.org Thu Jun 9 20:45:08 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 j59Iixlj023765 for ; Thu, 9 Jun 2005 20:44:59 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j59Iixx0023764 for ucd-sci-outgoing; Thu, 9 Jun 2005 20:44:59 +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 j59Iirlj023748 for ; Thu, 9 Jun 2005 20:44:53 +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 j59Iip73000570 for ; Thu, 9 Jun 2005 20:44:52 +0200 (CEST) Received: from urania.cfa.harvard.edu (urania [131.142.52.147]) by head.cfa.harvard.edu (d/w) with ESMTP id j59IijKE002570 for ; Thu, 9 Jun 2005 14:44:46 -0400 (EDT) From: Jonathan McDowell Received: (from jcm@localhost) by urania.cfa.harvard.edu (8.12.8p1/8.12.8) id j59IijxU002921 for ucd-sci@ivoa.net; Thu, 9 Jun 2005 14:44:45 -0400 (EDT) Date: Thu, 9 Jun 2005 14:44:45 -0400 (EDT) Message-Id: <200506091844.j59IijxU002921@urania.cfa.harvard.edu> To: ucd-sci@ivoa.net Subject: Re: SciBoard X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.6.9.21 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 UCD board, Sorry, I've been on travel and then sick. I've tried to catch up on the emails. About the solar system UCDs, Seb. said: > Hi Jonathan, > > There might be a slight misunderstanding on this. > The planetary system community has worked on their needs > to express the quantities they are measuring in their field > with proper UCDs. You can see the result of this reflexion > here: > http://portail.imcce.fr/fr/expert/ssvo/wgovp/propucd.html > I think these suggestions are worth examining, and they seem I have no major problems with this list, I was talking about suggestions that were raised for object types like asteroid, comet, etc. > quite mature: why not taking them into account for the PR. I had assumed in Kyoto that we would go for the PR as is, on the basis that the current list is not too bad, and then use the board to make modifications shortly afterwards. I think everyone is happy with the syntax and the methodology, while we can spend ages arguing about the actual list. It sounds like we want to add lots of things to the list before going to PR, which I worry will unnecessarily delay the PR. See Andrea's message of Jun 3 - my view is that we should look for any things in the current list that are BAD, and get rid of them; there are many things that are MISSING, but we can easily add them later. The list will be stable in the sense that valid UCDs should rarely become invalid, but it will never be stable in the sense that it will always grow. Which doesn't mean the board should delay discussing additions to the list (just that I don't think we have to agree on them before approving the PR). I'll give my comments on the planetary list below. > I am less confident that we can incorporate in the PR all the > astronomical object types/phenomenons that were discussed > for VOEvent (is this what you call "semantics for astronomical > objects"?). Yes, particularly the tree of object types: galaxy.Seyfert2 etc. I'm not so worried about the phenomena (outburst, glitch, etc..), and I thought Rick's list was quite good. But I've heard you and others say that you are worried about putting the object types in UCD, whereas it's becoming clear that the object types do need to be somewhere in the VO fairly soon. OK, now for the particular UCDs: * meta.id.(x,y,z) Hmm. I thought meta.id was more for names, how about arith.cpt.x, etc.? * obs.atm instead of obs.air I agree * obs.atm.refraction, phys.refraction - one the angle, the other the index. I guess I agree, but maybe obs.atm.refractAngle and phys.refractIndex is more explicit? * obs.elongation, obs.phaseAng - these are both angles. How about pos.angle.elongation, pos.angle.phase ? * pos.az.azi and pos.eq.ha I agree. * pos.brc.* In STC and I think in WCS-III the word 'topocentric' is being used for some of this, but body is fine too. I'd prefer pos.body.* which I find more obvious. * pos.eop.* I like, although as we become more active on other worlds isn't it likely that we'll be needing similar parameters for Mars, etc.? But maybe it's fine for now. * pos.precess Perhaps pos.eq.precess if we are talking specifically about the effect of terrestrial precession on coordinate systems (as opposed to the precession of the pole of (433)Eros or something) * phys.magAbs.G Isn't there an H as well? My asteroid friends keep talking about H.... * src.orbital.*, src.veloc.* I agree, with the possible exception of src.veloc.tan. Perhaps 'transverse' rather than 'tangential' is more clear? - Jonathan From owner-ucd-sci@eso.org Thu Jun 9 20:46:24 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 j59IkGlj024077 for ; Thu, 9 Jun 2005 20:46:17 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j59IkGZ6024076 for ucd-sci-outgoing; Thu, 9 Jun 2005 20:46:16 +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 j59IkClj024057 for ; Thu, 9 Jun 2005 20:46:12 +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 j59IkAXW022541 for ; Thu, 9 Jun 2005 20:46:11 +0200 (CEST) Received: from urania.cfa.harvard.edu (urania [131.142.52.147]) by head.cfa.harvard.edu (d/w) with ESMTP id j59Ik5KE002745 for ; Thu, 9 Jun 2005 14:46:05 -0400 (EDT) From: Jonathan McDowell Received: (from jcm@localhost) by urania.cfa.harvard.edu (8.12.8p1/8.12.8) id j59Ik5kY003131 for ucd-sci@ivoa.net; Thu, 9 Jun 2005 14:46:05 -0400 (EDT) Date: Thu, 9 Jun 2005 14:46:05 -0400 (EDT) Message-Id: <200506091846.j59Ik5kY003131@urania.cfa.harvard.edu> To: ucd-sci@ivoa.net Subject: Re: T0 : extensions to em, obs, spect, instr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.6.9.21 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 UCD comments 2: Rick's suggestions Hi UCD board, Rick Hessman proposed a number of UCDs (May 30) and I wanted to comment on them. One was spect.cont spectral continuum I endorse adding this, it's very useful for my own data. Rick suggested either em.grav-wave em.neutrino with 'em' redefined as 'emission', or else phys.grav-wave phys.particle.{cosmic-ray,neutrino} I like both. If you are comparing the light curves of the SN1987a neutrino flux and the optical flux, it makes sense to me to have phot.flux;em.neutrino even though 'photometry' strictly doesn't apply to non-photons, or maybe better phys.flux;em.neutrino but I think that phys.flux;phys.particle.neutrino is more generalizable, so I suggest we go with that. He also proposed an obs.calib tree to describe many different kinds of observation. I feel many of these are better handled with secondary words, for instance obs.calib;phot.flux instead of obs.calib.flux I know that some people feel excessive use of secondary words means that a simple search returns too many false positives - but I am convinced that alternative is an explosion of the vocabulary that will overwhelm us, and that a mild increase in search query sophistication will solve the perceived problem. We already have instr.calib, but many calibrations are not just for the instrument per se but for the observation as a whole (e.g. for ground based photometric calibrations it's usually not the instrument but the sky that is changing and needs calibration). So I think obs.calib is a better UCD. So here's my proposal for Rick's list, in which proposed new UCDs are marked by a * (sort of the paleolinguistics convention of marking hypothetical word forms with a *). Rick Jonathan phys.grav-wave/em.grav-wave *phys.wave.gravitational phys.particle.neutrino/em.neutrino *phys.particle.neutrino (note that phys.wave is a good subtree for other things like phys.wave.Alfven or phys.wave.dispersionRrelation) instr.calib *obs.calib [Calibration observation] phot.calib obs.image;*obs.calib;phot.flux [It's an image; it's for calibration; what are we calibrating - flux.] spect;*obs.calib;phot.flux [or, it's a spectrum...] obs.calib.dome-flat obs.image;obs.calib;*instr.det.flat;*instr.tel.dome [We're calibrating the flatness of the detector; we're using the dome to do it] obs.calib.flux obs.image;*obs.calib;phot.flux obs.calib.freq spect;*obs.calib;em.freq [It's a spectrum; it's for calibration; we're calibrating freq] obs.calib.guide-star meta.id;*obs.calib;*pos.astrometry [If this is the name of the guide star used..] obs.calib.phot [What's the difference with obs.calib.flux?] obs.calib.pos obs.image;*obs.calib;*pos.astrometry (?) obs.calib.sky-flat obs.image;obs.calib;*instr.det.flat obs.calib.slit-mask *instr.spect.slit obs.calib.spect spect;*obs.calib;em.wl [If you mean by this an arc spectrum; what diff from obs.calib.wl?] obs.calib.veloc spect;*obs.calib;src.veloc obs.calib.wl spect;*obs.calib;em.wl phot.calib.flux [same as obs.calib.flux?] phot.calib.mag *obs.calib;em.opt.B (etc.) pos.calib *obs.calib;pos spect.calib spect;*obs.calib spect.calib.wl spect;*obs.calib;em.wl spect.calib.freq spect;*obs.calib;em.freq Rick's next message on May 30 proposed an 'event' tree. All his events are things that happen to sources, so we might want to make this a src.event subtree. Also, it's "occultation", not "occulation". Otherwise I like it. But as we agreed in Kyoto, let's wait a while on this subject. - Jonathan From owner-ucd-sci@eso.org Thu Jun 9 20:47:47 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 j59Ilflj024983 for ; Thu, 9 Jun 2005 20:47:41 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j59IlfO9024981 for ucd-sci-outgoing; Thu, 9 Jun 2005 20:47:41 +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 j59IlXlj024931 for ; Thu, 9 Jun 2005 20:47:34 +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 j59IlVXW022649 for ; Thu, 9 Jun 2005 20:47:32 +0200 (CEST) Received: from urania.cfa.harvard.edu (urania [131.142.52.147]) by head.cfa.harvard.edu (d/w) with ESMTP id j59IlMKE002958 for ; Thu, 9 Jun 2005 14:47:25 -0400 (EDT) From: Jonathan McDowell Received: (from jcm@localhost) by urania.cfa.harvard.edu (8.12.8p1/8.12.8) id j59IlLcR003225 for ucd-sci@ivoa.net; Thu, 9 Jun 2005 14:47:21 -0400 (EDT) Date: Thu, 9 Jun 2005 14:47:21 -0400 (EDT) Message-Id: <200506091847.j59IlLcR003225@urania.cfa.harvard.edu> To: ucd-sci@ivoa.net Subject: Re: T0 : extensions to em, obs, spect, instr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.6.9.22 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 UCD comments 3: the standard vocabulary for the universe Rick Hessman said: : : Sebastien Derriere said: : > Solar System UCDs (really Astronomical Object UCDs): : > they will not be UCDs per the PR. But IVOA may need such a list : > and a UCD-compatible syntax may be appropriate. If the UCD/Semantics : > group doesn't want to take that work on, the DM group should : > probably do it. I think either group could do it, provided we : > keep the distinction between the two lists (UCDs, as semantics : > for astronomical non-object concepts, and the other list, : > as semantics for astronomical objects). : Actually, it was me who said this, Sebastien's message quoted me. At the time I wrote this, I actually agreed with Rick; I was trying to find a compromise approach since it seemed that Sebastien (and I think Patricio and other originators of the UCDs) do want to make such a distinction. Someone is going to have to list object-classification concepts. I would prefer it was the UCD board, but if not, it'll have to be the DM group or the vo-semantics folks. However, after the discussion I take a more nuanced (i.e. confused) position. I do now think there is some real justification for a separate list using the ucd = src.class value = galaxy.spiral approach: the other approach with ucd = src.class.galaxy.spiral might be ok, but very quickly we want ucd = src.class.galaxy.spiral.SB(r)cd... ucd = src.class.star.binary.O7e+PNe/LMXB ucd = src.class.comet.sungrazer ucd = src.class.body.feature.rupes In other words, 'galaxy' is not just a concept, it's a classification, and the coarsest bin in a complicated tree of classifications. (Sebastien made a distinction between classification and morphological type which I don't think is a real one in practice; morph type, variable star class, spectral type, etc. are all part of the classification of what this object is). I don't think the classification's really quite the same as distinguishing between radial velocity and some other kind of velocity. And as my examples above show, once you get down to the detailed classification the UCD syntax doesn't actually make a good match. Rick will probably argue that it still makes sense to have UCDs which go down as far as the less detailed level (star.binary etc) and I could buy that. Like Rick, I focus on the data-header applications more than the Vizier-catalog applications, and I take it as a clue that in FITS headers, "spiral galaxy" is always a keyword value, not a keyword name. This suggested to me that in fact UCD may not be the right controlled vocab for this set of concepts. But then Sebastien reminded us of the 'concept/property' way of looking at UCDs, where the question becomes: are there specific properties we need to describe? To be more specific: radial.velocity;src.class.galaxy would be the radial velocity of a galaxy. Does having this add anything to just saying radial.velocity;src - do you really care that it's a galaxy and not a star. This leads to a data model question: what properties do a galaxy and a star *not* share? For example: object.galaxy.spiral.HolmbergRadius object.star.convectionParameter This, to my mind, is the correct role of object types in UCD and argues for a tree of this kind. Right now, these kind of properties go in the phys or src list without the 'object..' prefix. - Jonathan - Jonathan From owner-ucd-sci@eso.org Thu Jun 9 20:48:05 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 j59Ilxlj025145 for ; Thu, 9 Jun 2005 20:48:00 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j59IlxoD025144 for ucd-sci-outgoing; Thu, 9 Jun 2005 20:47:59 +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 j59Ilslj025128 for ; Thu, 9 Jun 2005 20:47:54 +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 j59Ilq73000792 for ; Thu, 9 Jun 2005 20:47:53 +0200 (CEST) Received: from urania.cfa.harvard.edu (urania [131.142.52.147]) by head.cfa.harvard.edu (d/w) with ESMTP id j59IlhKE003020 for ; Thu, 9 Jun 2005 14:47:46 -0400 (EDT) From: Jonathan McDowell Received: (from jcm@localhost) by urania.cfa.harvard.edu (8.12.8p1/8.12.8) id j59IldO1003229 for ucd-sci@ivoa.net; Thu, 9 Jun 2005 14:47:39 -0400 (EDT) Date: Thu, 9 Jun 2005 14:47:39 -0400 (EDT) Message-Id: <200506091847.j59IldO1003229@urania.cfa.harvard.edu> To: ucd-sci@ivoa.net Subject: T0: basic UCD tree X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.6.9.21 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 * UCD comments 4: overall UCD tree Hi UCD board, I looked again at the UCD primary concepts and tried to group them. The one I am most worried about is "spect". time,pos,em,phot Fundamental astro concepts, fine. obs, phys Also good basic concepts arith a good basic tree, although "math" might be better. stat Maybe should be under arith? src Another fundamental concept, although as usual I would argue for a distinction between "src" (2D on the sky, results of observation) and "object" (real 3D thing in space). instr Fairly fundamental but one could argue should be under obs spect I worry about spect - this is a kind of data. If spect, why not image? I predict a few years from now we will have to change spec and instr.image to data.spect, data.image, etc. Despite this worry, I am willing to endorse the current list for the PR. - Jonathan From owner-ucd-sci@eso.org Fri Jun 10 11:00:44 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 j5A90Vq9027213 for ; Fri, 10 Jun 2005 11:00:31 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5A90VVv027212 for ucd-sci-outgoing; Fri, 10 Jun 2005 11:00:31 +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 j5A90Rq9027204 for ; Fri, 10 Jun 2005 11:00:27 +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 j5A90P73024955 for ; Fri, 10 Jun 2005 11:00:25 +0200 (CEST) Received: from (150.146.129.253) by e1000.artov.rm.cnr.it via smtp id 289f_22fce9ae_d98e_11d9_8e1b_0002b3da0f69; Fri, 10 Jun 2005 11:00:47 +0200 (CEST) Received: (qmail 18005 invoked by uid 508); 10 Jun 2005 09:00:19 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.033378 secs); 10 Jun 2005 09:00:19 -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 ; 10 Jun 2005 09:00:19 -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 ; Fri, 10 Jun 2005 11:00:19 +0200 Message-ID: <20050610110019.0nl83m6u32zkks0w@webmail.sic.rm.cnr.it> Date: Fri, 10 Jun 2005 11:00:19 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Re: T0: UCDs for "em" References: <20050602152438.fdmq7yxtgdcgg40k@webmail.sic.rm.cnr.it> <18AB023D-4017-4716-BA26-6642EA40EC36@noao.edu> <20050603101129.diyu1dvr2wj4sg4g@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: 2005.6.10.2 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 Miguel Cervino wrote: > First I center in "Q" UCDs, and I propose to keep: > > Q|em.energy |Energy value in the em frame > Q|em.freq |Frequency value in the em frame > Q|em.wavenumber |Wavenumber value in the em frame > Q|em.wl |Wavelength value in the em frame The point is that: 1. It would be clearer to use the em branch just to describe the electro-magnetic axis (radio, ir,opt,...,line,..) and move energy, freq, wl to the phys branch. 2. We now have phys.energy and em.energy If you ask the assign tool http://vizier.u-strasbg.fr/UCD/cgi-bin/descr2ucd the word energy is translated always into phys.energy : correct. You only get em.energy if you type photon energy : correct too. But we are describing the same quantity with two ucd-words! > Q|em.wl.air* |Wavelength value in the em frame in air frame > > somewhere it should be established default is vacuum? > In most optical observation default is air and > in UV vacuum as example, but SLOAN data release > gives optical wl en vacuum... yes, things are complicated: you often find which, I suspect, are wl.air in the optical and, obviously, wl.vacuum in the UV! > Q|em.veloc* |Apparent radial velocity > Q|em.veloc.radio* |radio velocity > Q|em.veloc.optical* |optical velocity > Q|em.veloc.beta* |velocity/cr somebody proposed already velocRadio, velocOpt. I ask him/her to re-submit that proposal > > - Change from Q to E: > Q|em.wl.central |Central wavelength > Q|em.wl.effective |Effective wavelength Yes, with the flag set to Q and a description like: central wl of Halpha you'll get only wl.central . > ... for clarity purpose and hogenity > the UDCs I would suggest the following changues: > > em.IR.K --> em.IR.2-3um > em.IR.H --> em.IR1500-2000nm > em.IR.J --> em.IR1000-1500nm > > em.opt.I --> em.opt.750-1000nm > em.opt.R --> em.opt.600-750nm > em.opt.V --> em.opt.500-600nm > em.opt.B --> em.opt.400-500nm > em.opt.U --> em.opt.300-400nm > > so there no will be confusion with fotometry bands may be we should go this way, because the names of those bands can be misleading. In the case of x- and gamma-rays though there is no confusion, so I would keep the existing names... > Finally, I think that the inclusion of em.line would be useful, but > only for a very sort list of lines so ... I would agree with > Hydrogen lines, but I do think that em.line.OIII should be > depreciated (there is several OIII lines!, and if OIII is here, by > not, O I, or H+K Ca II etc...? so I propose depreciate em.line.OIII ... the reason for the inclusion of the OIII line is that the doublet 4959+5007 is one of the strongest lines in emission-line objects (second only to Halpha in most cases). There are surveys in Halpha/beta and in OIII, not in OI. My point is: today em.line.OIII is used/useful. The day we'll find other lines useful we'll propose their inclusion. By the way: em.line.XXX is not a quantity: it is a qualifier of some other quantity, e.g. intensity, flux, etc.. Cheers Andrea From owner-ucd-sci@eso.org Fri Jun 10 12:09:12 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 j5AA96q9013533 for ; Fri, 10 Jun 2005 12:09:06 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5AA96WN013532 for ucd-sci-outgoing; Fri, 10 Jun 2005 12:09:06 +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 j5AA8xq9013519 for ; Fri, 10 Jun 2005 12:08:59 +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 j5AA8vXW018578 for ; Fri, 10 Jun 2005 12:08:58 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1DggRX-000Fj9-HS for ucd-sci@ivoa.net; Fri, 10 Jun 2005 12:08:51 +0200 Mime-Version: 1.0 (Apple Message framework v622) In-Reply-To: <200506091847.j59IldO1003229@urania.cfa.harvard.edu> References: <200506091847.j59IldO1003229@urania.cfa.harvard.edu> Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <25d39d6a9dc407818d6d6b228334efae@Astro.physik.Uni-Goettingen.DE> Content-Transfer-Encoding: 7bit From: "Frederic V. \"Rick\" Hessman" Subject: Re: T0: basic UCD tree Date: Fri, 10 Jun 2005 12:11:08 +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: 2005.6.10.4 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 9 Jun 2005, at 8:47 pm, Jonathan McDowell wrote: > arith a good basic tree, although "math" might be better. > stat Maybe should be under arith? I agree : math covers arith and stat. *math.arith *math.stat > src Another fundamental concept, although as usual I would argue > for > a distinction between "src" (2D on the sky, results of > observation) and > "object" (real 3D thing in space). Now, now: don't try to bring "concepts" into the UCD world ;-) ! We have to agree that "src" means "object on the sky" (where the definition of "sky" is, of course, relative to an observer, e.g. a spacecraft), since everything that UCD describes is for observations or observed properties. Otherwise, the whole "concept" (or, God-forbid, "ontology") discussion comes up again! Right now, the official UCD description of "src" is "Source" - not very helpful. I suggest using "Observed source viewed on the sky". > instr Fairly fundamental but one could argue should be under obs No!: "obs" is an observation thing made with an instrument "inst". The focal length of a telescope isn't (in our present sense) an observation, but a property of an instrument and so doesn't at ALL belong to "obs". > spect I worry about spect - this is a kind of data. > If spect, why not image? I predict a few years from now > we will have to change spec and instr.image to data.spect, > data.image, etc. I agree that data.image and data.spec is a much better model, at least for observations. After all, what UCD often does is to provide generalized "keywords" a la FITS. On the other hand, the VO theory people might complain that their "images" and "spectra" are not really "data". Sounds like a problem which has to be put off until later. > But then Sebastien reminded us of the 'concept/property' way of looking > at UCDs, where the question becomes: are there specific properties we > need to describe? To be more specific: > > radial.velocity;src.class.galaxy > > would be the radial velocity of a galaxy. Does having this add > anything to > just saying > > radial.velocity;src > > - do you really care that it's a galaxy and not a star. > This leads to a data model question: what properties do a galaxy and a > star > *not* share? For example: > object.galaxy.spiral.HolmbergRadius > object.star.convectionParameter > > This, to my mind, is the correct role of object types in UCD and > argues for a tree > of this kind. Right now, these kind of properties go in the phys or src > list without the 'object..' prefix. This can of worms obviously won't be solved using UCD alone: that's why I'm pushing the development of a parallel system which LOOKS like UCD and can be treated/ manipulated/concatenated like UCD but addresses this concept/property problem. Simply put: one person's property is another's concept and vice versa, so we need a system which can be used in both directions. > instr.calib *obs.calib [Calibration observation] > phot.calib obs.image;*obs.calib;phot.flux > obs.calib.dome-flat > obs.image;obs.calib;*instr.det.flat;*instr.tel.dome > obs.calib.flux obs.image;*obs.calib;phot.flux > obs.calib.freq spect;*obs.calib;em.freq > obs.calib.guide-star meta.id;*obs.calib;*pos.astrometry > obs.calib.phot [What's the difference with obs.calib.flux?] > obs.calib.pos obs.image;*obs.calib;*pos.astrometry (?) > obs.calib.sky-flat obs.image;obs.calib;*instr.det.flat > obs.calib.slit-mask *instr.spect.slit > obs.calib.spect spect;*obs.calib;em.wl > obs.calib.veloc spect;*obs.calib;src.veloc > obs.calib.wl spect;*obs.calib;em.wl > phot.calib.flux [same as obs.calib.flux?] > phot.calib.mag *obs.calib;em.opt.B (etc.) > pos.calib *obs.calib;pos > spect.calib spect;*obs.calib > spect.calib.wl spect;*obs.calib;em.wl > spect.calib.freq spect;*obs.calib;em.freq I basically think this is a very good compromise. See my other mail about problems with instr and others. 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 Fri Jun 10 12:09:17 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 j5AA9Cq9013544 for ; Fri, 10 Jun 2005 12:09:12 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5AA9C8P013543 for ucd-sci-outgoing; Fri, 10 Jun 2005 12:09:12 +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 j5AA8xq9013520 for ; Fri, 10 Jun 2005 12:08:59 +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 j5AA8vXW018577 for ; Fri, 10 Jun 2005 12:08:58 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1DggRW-000Fj9-KB for ucd-sci@ivoa.net; Fri, 10 Jun 2005 12:08:50 +0200 Mime-Version: 1.0 (Apple Message framework v622) Content-Transfer-Encoding: 7bit Message-Id: <12358f5050de60892fe99445a10af612@Astro.physik.Uni-Goettingen.DE> Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed To: ucd-sci@ivoa.net From: "Frederic V. \"Rick\" Hessman" Subject: T0: needed last minute changes Date: Fri, 10 Jun 2005 12:10:44 +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: 2005.6.10.4 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 After reading Jonathon's comments and re-reading the UCD vocabulary document again, I realized that we definitely need a few changes: 1. I first stumbled over instr.obsty.site.seeing Does this mean we need... instr.obsty.site.temperature instr.obsty.site.humidity Seem like a better solution would be to introduce "weather", which permits the concatenation instr.obsty.site;weather.seeing which would open a new handy family weather | meteorological condition weather.seeing | atmospheric image quality weather.temp | local temperature weather.humidity | relative humidity weather.dewpoint | dewpoint temperature weather.precipitation | presence of rain/snow/sleet (boolean?) This would be VERY helpful for VOEvent/RTML. I won't open up a new discussion of the uneven choice of contractions (e.g. "temp" instead of "temperature" but "wavenumber" instead of "wavenum" - sigh!). The topic "space weather" comes into mind as well , but I'll let others worry about that. 2. instr First of all, a trivial but needed addition: instr.det.temp | temperature of detector Next: we presently have "instr.tel.focus" and "instr.fov" which are quantities which refer to the "end-users" - no info about how the fov or focus came into being. The problem is whether to assign something like "focus" to the telescope or to the instrument. Generally, the fov of an instrument (e.g. CCD camera) is very different from that of the telescope. Do we then interpret "instr" things as being from a black box or from a specific instrument hanging on a telescope? If it's the latter, then one may need double entries. In any case there's a need for something like instr.tel.aperture | geometric diameter of telescope optics instr.tel.area | (effective?) collecting area of telescope optics instr.tel.focallength | focal length (effective?) of telescope instr.tel.fRatio | ratio of focal length to aperture diameter instr.tel.temp | temperature of telescope After all, we already have instr.focus, which is a much less needed number than the above! Sounds to me as if we need to distinguish between generic instr = e.g. telescope+filterwheel+CCD or telescope+spectrograph+CCD and "device" (can't think of a better name) which could be just the instrument part of the above (e.g. just the imaging camera or just the spectrograph). This would also imply that we need to make tel a primary key, since the telescope doesn't "belong" to the generic instrument - it's an associated thing. This would solve Jonathon's suggested of using obs.image;obs.calib;instr.det.flat;instr.tel.dome (i.e. using proposed UCDs obs.calib and instr.tel.dome) by permitting obs.image;obs.calib;inst.det.flat;tel.dome and would permit the differentiation between e.g. instr.focallength and tel.focallength. On the other hand, this means a lot of double entries which could only be gotten rid of using something like instr;optics.focallength tel;optics.focallength (unfortunately, "opt" is already taken: if we would be using "optical" for wavelength band and "optics" for optics, there wouldn't be any confusion). In summary, we need to get rid of instr.tel instr.tel.focus and add optics optics.focus optics.focallength optics.aperture optics.area optics.fRatio tel tel.dome (instr.obsty.dome is no good if there are lots of domes at the site) tel.mount (e.g. "alt-az", "equatorial", "english",....) 3. PLEASE PLEASE PLEASE change src.class.struct -> src.class.struct.BautzMorgan src.class.distance -> src.class.distance.Abell src.class.richness -> src.class.richness.Abell src.spType -> src.class.spectral.MK src.morph.type -> src.morph.Hubble The present definitions associating general class descriptions with very particular versions of mostly extragalactic classifications are absolutely insane! Or, the description has to be changed to something like src.class.struct | structure classification, e.g. Bautz-Morgan galaxy type src.class.distance | distance classification, e.g. Abell galaxy cluster src.class.richness | richness classification, e.g. Abell galaxy cluster src.class.spectral | spectral classification, e.g. MK spectral class which results in a loss of specificity. There are other spectral classes beyond MK stellar, other richness classifications other than Abell (e.g. open stellar clusters), .... 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 Fri Jun 10 15:01:42 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 j5AD1Rq9018517 for ; Fri, 10 Jun 2005 15:01:27 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5AD1RPv018516 for ucd-sci-outgoing; Fri, 10 Jun 2005 15:01:27 +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 j5AD0xq9018428 for ; Fri, 10 Jun 2005 15:00:59 +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 j5AD0v73001348 for ; Fri, 10 Jun 2005 15:00:58 +0200 (CEST) Received: from (150.146.129.253) by e1000.artov.rm.cnr.it via smtp id 275a_bda27408_d9af_11d9_9fd8_0002b3da0f69; Fri, 10 Jun 2005 15:01:21 +0200 (CEST) Received: (qmail 4849 invoked by uid 508); 10 Jun 2005 13:00:51 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. 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Processed in 0.037452 secs); 10 Jun 2005 13:00:51 -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 ; 10 Jun 2005 13:00:51 -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 ; Fri, 10 Jun 2005 15:00:51 +0200 Message-ID: <20050610150051.dq8plmskejc4cso8@webmail.sic.rm.cnr.it> Date: Fri, 10 Jun 2005 15:00:51 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: T6 - solar system UCDs References: <200506091844.j59IijxU002921@urania.cfa.harvard.edu> In-Reply-To: <200506091844.j59IijxU002921@urania.cfa.harvard.edu> 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: 2005.6.10.10 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 Here are my comments on the UCDs proposed by SS people, see: http://portail.imcce.fr/fr/expert/ssvo/wgovp/propucd.html 1. meta.id.(x,y,z) Cartesian component of a vector In the present list of ucd-words you find S|pos.cartesian |Cartesian (rectangular) coordinates Q|pos.cartesian.x |Cartesian coordinate along the x-axis Q|pos.cartesian.y |Cartesian coordinate along the y-axis Q|pos.cartesian.z |Cartesian coordinate along the z-axis The keywords used for assigning these ucd-words are: Q|pos.cartesian.(x,y,z) |(x,y,z) axis coordinate position (U,V,W) component projected so that the description: y component of any-V-quantity leads to the ucd: any-V-quantity;pos.cartesian.y where vectorial quantities are, for the moment, V|phys.electField V|phys.magField V|pos.distance V|pos.pm V|pos.precess V|src.veloc On the other hand, pos.cartesian.x/y/z is a quantity (position on axis x/y/z), so that the description : Xpos on detector yields pos.cartesian.x;instr.det My suggestion is: keep pos.cartesian.x/y/z 2. obs.air suppress 3. replace with: obs.atm I agree. But then we need to change air into atm in: S|obs.air |Atmosphere Q|obs.air.extinction |Atmospheric extinction and Q|obs.air.mass |Airmass could become Q|obs.airMass 4. obs.atm.refraction / phys.refraction I support Jonathan suggestion: change into obs.atm.refractAngle phys.refractIndex 5. obs.elongation The elongation of a celestial body its the angular separation from the body around which it orbits The UCD for this quantity already exists: pos.angDistance 6. obs.phaseAng as above 7. pos.az.ha, pos.az.azi, pos.eq.ha I agree with the proposal. 8. pos.brc.(), pos.earth() I basically agree. I also totally agree with Jonathan's comment. 9. pos.eop.() OK 10. pos.precess No, the description is all right: just Equatorial precession ==> pos.precess;pos.eq I prefer this, its more flexible. 11. phys.magAbs.G I'm only aware of the H mag (which is actually a visual mag!!) I remind you that phys.magAbs has E-flag: if you just need to specify the phot band, you can say: phys.magAbs;em.opt.V 12. src.orbital.meanMotion I suppose it is an average angular velocity (src.veloc.ang;stat.mean). No strong feelings about it. 13. ...veloc... to be revised (not only in the framwork of SS!! 14. src.veloc.compon Not in the present list. Cheers, 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-sci@eso.org Fri Jun 10 16:00:05 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 j5ADxtq9001082 for ; Fri, 10 Jun 2005 15:59:56 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5ADxtIt001081 for ucd-sci-outgoing; Fri, 10 Jun 2005 15:59:55 +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 j5ADxoq9001063 for ; Fri, 10 Jun 2005 15:59:50 +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 j5ADxmXW024911 for ; Fri, 10 Jun 2005 15:59:49 +0200 (CEST) Received: from argiope.saclay.cea.fr (argiope.saclay.cea.fr [132.166.192.108]) by cirse.extra.cea.fr (8.13.4/8.13.4/CEAnet-Internet.5.0) with ESMTP id j5ADxhbU016550 for ; Fri, 10 Jun 2005 15:59:43 +0200 (MEST) Received: from pisaure.intra.cea.fr (unverified) by argiope.saclay.cea.fr (Content Technologies SMTPRS 4.3.17) with ESMTP id ; Fri, 10 Jun 2005 15:59:43 +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 j5ADxPeg005250; Fri, 10 Jun 2005 15:59:26 +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 j5ADxfoN013718; Fri, 10 Jun 2005 15:59:41 +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 j5AE0Ae5017363 ; Fri, 10 Jun 2005 16:00:19 +0200 (MEST) Message-ID: <42A99CC5.4070601@cea.fr> Date: Fri, 10 Jun 2005 15:59:33 +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: ucd-sci@ivoa.net Subject: Re: T6 - solar system UCDs References: <200506091844.j59IijxU002921@urania.cfa.harvard.edu> <20050610150051.dq8plmskejc4cso8@webmail.sic.rm.cnr.it> In-Reply-To: <20050610150051.dq8plmskejc4cso8@webmail.sic.rm.cnr.it> 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: 2005.6.10.11 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 Nice ;-) Andrea Preite Martinez wrote: > Here are my comments on the UCDs proposed by SS people, see: > http://portail.imcce.fr/fr/expert/ssvo/wgovp/propucd.html > > 1. meta.id.(x,y,z) Cartesian component of a vector > > In the present list of ucd-words you find > S|pos.cartesian |Cartesian (rectangular) coordinates > Q|pos.cartesian.x |Cartesian coordinate along the x-axis > Q|pos.cartesian.y |Cartesian coordinate along the y-axis > Q|pos.cartesian.z |Cartesian coordinate along the z-axis > > The keywords used for assigning these ucd-words are: > Q|pos.cartesian.(x,y,z) |(x,y,z) axis coordinate position (U,V,W) > component projected > > so that the description: y component of any-V-quantity > leads to the ucd: any-V-quantity;pos.cartesian.y > > where vectorial quantities are, for the moment, > > V|phys.electField > V|phys.magField > V|pos.distance > V|pos.pm > V|pos.precess > V|src.veloc > > On the other hand, pos.cartesian.x/y/z is a quantity (position on axis > x/y/z), so that the description : > > Xpos on detector yields pos.cartesian.x;instr.det > > My suggestion is: keep pos.cartesian.x/y/z I think that we introduce this meta.id when working on previous versions where pos.cartesian did not exists. > > 2. obs.air suppress > 3. replace with: obs.atm > I agree. > But then we need to change air into atm in: > S|obs.air |Atmosphere > Q|obs.air.extinction |Atmospheric extinction > and > Q|obs.air.mass |Airmass could become > Q|obs.airMass > > 4. obs.atm.refraction / phys.refraction > I support Jonathan suggestion: change into > obs.atm.refractAngle > phys.refractIndex > > 5. obs.elongation > The elongation of a celestial body its the angular separation from the body > around which it orbits > The UCD for this quantity already exists: pos.angDistance Not really! Unless we do not need src.veloc.* because src.veloc exists. ( joke ;-) ) elongation is a "special/specific" parameter in planetology, why not then pos.angDistance.elongation > > 6. obs.phaseAng > as above It is even less true here because pos.angDistance is the angular distance betwwen two points (on a sphere) from the observer point of view and obs.phaseAng gives the angle between the sun and the observer from the observed spot point of view and is related to illumination, light incidence and re-emission... > > 7. pos.az.ha, pos.az.azi, pos.eq.ha > I agree with the proposal. > > 8. pos.brc.(), pos.earth() > I basically agree. I also totally agree with Jonathan's comment. > > 9. pos.eop.() > OK > > 10. pos.precess > No, the description is all right: just > Equatorial precession ==> pos.precess;pos.eq > I prefer this, its more flexible. but perhaps not sufficient to "describe completly" precession in some case! > > 11. phys.magAbs.G > I'm only aware of the H mag (which is actually a visual mag!!) > I remind you that phys.magAbs has E-flag: if you just need to specify the > phot band, you can say: phys.magAbs;em.opt.V ~ phys.magAbs.G is a parameter for the derivation of the absolute magnitude of asteroids > > 12. src.orbital.meanMotion > I suppose it is an average angular velocity (src.veloc.ang;stat.mean). > No strong feelings about it. > > 13. ...veloc... > to be revised (not only in the framwork of SS!! sure > > 14. src.veloc.compon > Not in the present list. > > Cheers, > > 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 > ============================================================================== > > -- 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-ucd-sci@eso.org Fri Jun 10 18:01:18 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 j5AG1Cq9025328 for ; Fri, 10 Jun 2005 18:01:13 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5AG1Cpr025327 for ucd-sci-outgoing; Fri, 10 Jun 2005 18:01:12 +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 j5AG14q9025314 for ; Fri, 10 Jun 2005 18:01:04 +0200 (MEST) Received: from iaa13u.iaa.csic.es (iaa13u.iaa.csic.es [193.146.145.13]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j5AG12XW028913 for ; Fri, 10 Jun 2005 18:01:02 +0200 (CEST) Received: from [161.111.166.190] (wep50.iaa.csic.es [161.111.166.190]) by iaa13u.iaa.csic.es (8.9.3/8.9.1) with ESMTP id SAA00311 for ; Fri, 10 Jun 2005 18:00:57 +0200 (MET DST) Mime-Version: 1.0 (Apple Message framework v730) In-Reply-To: <20050610110019.0nl83m6u32zkks0w@webmail.sic.rm.cnr.it> References: <20050602152438.fdmq7yxtgdcgg40k@webmail.sic.rm.cnr.it> <18AB023D-4017-4716-BA26-6642EA40EC36@noao.edu> <20050603101129.diyu1dvr2wj4sg4g@webmail.sic.rm.cnr.it> <20050610110019.0nl83m6u32zkks0w@webmail.sic.rm.cnr.it> Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <872B0715-B051-49A2-9DE8-E23200EE41D3@iaa.es> Content-Transfer-Encoding: 7bit From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Re: T0: UCDs for "em" & "spect" Date: Fri, 10 Jun 2005 18:01:14 +0200 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: 2005.6.10.16 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 again :) >> ... for clarity purpose and hogenity >> the UDCs I would suggest the following changues: >> >> em.IR.K --> em.IR.2-3um >> em.IR.H --> em.IR1500-2000nm >> em.IR.J --> em.IR1000-1500nm >> .... > may be we should go this way, because the names of those bands can be > misleading. > In the case of x- and gamma-rays though there is no confusion, so I > would > keep the existing names... > Uhmm, for X-ray and gamma-rays I was asking X-ray and gamma-ray people.... I know that UCDs are not for humans, but asking about what soft and hard X-rays mean, the answer is highly dependent on the asked astronomer. Usually they talk only about soft and hard. "medium-Xrays" is not understood. In fact, most people I asked consider hard X-ray as aprox 4-10 keV band (from maximmun energy from ROSAT/ EINSTEIN to max energy by CHANDRA/ASCA/XMM)..... I do not know, but I think that keep em.X-ray.soft medium and hard is misunderstanding for X-ray people. Another example, ROSAT has a "hardness" ratio that is 0.2 keV-1.5keV (soft) vs. 1-4kev (hard) (I do not remember exactly the energies, sorry) where "soft" and "hard" refers to the detectors in ROSAT (but they are used in thsi way in the articles).... In gamma ray, the situation is similar. You can take a look the INTEGRAL instruments, or CGRO ones. The problem is that each energy range use techniques completely different (due to the physics of the process) and em.gamma.hard is to wide! It includes from only space instruments to only ground based instruments (using the atmosphere as detector). In fact some gamma- ray people make distinction between gamma-ray VeryHigh gamma-rays and Ultra-High gamma rays as clearly different parts of the electromagnetic spectrum.... (I was also thinking about INTEGRAL where a more defined bands would be and asset). >> Finally, I think that the inclusion of em.line would be useful, but >> only for a very sort list of lines so ... I would agree with >> Hydrogen lines, but I do think that em.line.OIII should be >> depreciated (there is several OIII lines!, and if OIII is here, by >> not, O I, or H+K Ca II etc...? so I propose depreciate >> em.line.OIII ... >> > the reason for the inclusion of the OIII line is that the doublet > 4959+5007 > is one of the strongest lines in emission-line objects (second only to > Halpha in most cases). There are surveys in Halpha/beta and in > OIII, not in > OI. ok :) About other issues. I also agree with include arith and stat in "math". I also suggest math.stat.moment that means the order moment of the statistical distribution, i.e. mean is 1, variance is 2, skewness 3, and kurtosis 4....), so allows to include more statistical information (e.j. there is some published data in skewness distributions of globular cluster, also are useful for some synthesis models) In the case of: > >> spect I worry about spect - this is a kind of data. >> If spect, why not image? I predict a few years from now >> we will have to change spec and instr.image to >> data.spect, data.image, etc. >> > > I agree that data.image and data.spec is a much better model, at > least for observations. After all, what UCD > often does is to provide generalized "keywords" a la FITS. > > On the other hand, the VO theory people might complain that their > "images" and "spectra" are not really "data". > > Sounds like a problem which has to be put off until later. Form a theoretical point of view (mine) theory results can be considered as "data", produced by a computer instead a telescope but.... (any case the results of theory will be also under a tag isn't it? (it is my very particular opinion). (any case there is also a S UCD called "meta.modelled" Finally, about the "line" atom used in "spect"... Uhmm, I do not know if there is a more usefull atom. I mean, some lick indices, as example, are obtained from "bands" and no lines.... there is no problem is it is explicti in the definition that it would refers not only to lines but also to bands... In the same way, I think that spect.line.intensity ---> spect.line; phot.fluxDens Atoms like: profile. width, eqwidth sound ok, but spect.line.asymmetry is not included in spect.line.profile? also for spect.line.broad? (this last I am not sure) Nice weekend Miguel From owner-ucd-sci@eso.org Mon Jun 13 11:49:11 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 j5D9n2q2009725 for ; Mon, 13 Jun 2005 11:49:02 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5D9n2XX009724 for ucd-sci-outgoing; Mon, 13 Jun 2005 11:49:02 +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 j5D9muq2009713 for ; Mon, 13 Jun 2005 11:48:56 +0200 (MEST) Received: from esa-av-smtp2.gmessaging.net (esa-av-smtp2.gmessaging.net [194.51.201.23]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j5D9msXW010920 for ; Mon, 13 Jun 2005 11:48:54 +0200 (CEST) Received: from esa-spas2.gmessaging.net (relay2 [172.24.21.39]) by esa-av-smtp2.gmessaging.net (iPlanet Messaging Server 5.2 Patch 2 (built Jul 14 2004)) with ESMTP id <0II0007W6OL7RG@esa-av-smtp2.gmessaging.net> for ucd-sci@ivoa.net; Mon, 13 Jun 2005 11:48:43 +0200 (MEST) Received: from localhost (esa-spas2 [127.0.0.1]) by esa-spas2.gmessaging.net (Postfix) with ESMTP id 644B8219E49 for ; Mon, 13 Jun 2005 11:48:44 +0200 (CEST) Received: from esa-spas2.gmessaging.net ([127.0.0.1]) by localhost (esa-spas2 [127.0.0.1]) (amavisd-new, port 10024) with ESMTP id 11970-05 for ; Mon, 13 Jun 2005 11:48:41 +0200 (CEST) Received: from sciops-mailgw.vilspa.esa.int (sciops-mailgw.vilspa.esa.int [193.147.152.105]) by esa-spas2.gmessaging.net (Postfix) with ESMTP id C5D68219E46 for ; Mon, 13 Jun 2005 11:48:41 +0200 (CEST) Received: from xvsas01.vilspa.esa.es (xvsas01.vilspa.esa.es [193.147.152.101]) by sciops-mailgw.vilspa.esa.int (Postfix) with ESMTP id 96D4111F703 for ; Mon, 13 Jun 2005 11:48:41 +0200 (CEST) Received: from sciops.esa.int (xmmwl31.xsci.lan [192.168.1.61]) by xvsas01.vilspa.esa.es (8.12.10/8.12.10) with ESMTP id j5D9mfLo007180 for ; Mon, 13 Jun 2005 09:48:41 +0000 (GMT) Date: Mon, 13 Jun 2005 09:48:40 +0000 From: Matteo Guainazzi Subject: Re: T0: UCDs for "em" & "spect" In-reply-to: <872B0715-B051-49A2-9DE8-E23200EE41D3@iaa.es> To: ucd-sci@ivoa.net Message-id: <42AD5678.9010707@sciops.esa.int> MIME-version: 1.0 Content-type: text/plain; charset=ISO-8859-1; format=flowed Content-transfer-encoding: 7BIT X-Accept-Language: en-us, en User-Agent: Mozilla/5.0 (X11; U; Linux i686; en-US; rv:1.6) Gecko/20040115 X-Spam-Score: Content analysis details: (-1.2 points, 4.5 points required to be considered as spam) -1.2 BAYES_00 BODY: Bayesian spam probability is 0 to 1% [score: 0.0000] References: <20050602152438.fdmq7yxtgdcgg40k@webmail.sic.rm.cnr.it> <18AB023D-4017-4716-BA26-6642EA40EC36@noao.edu> <20050603101129.diyu1dvr2wj4sg4g@webmail.sic.rm.cnr.it> <20050610110019.0nl83m6u32zkks0w@webmail.sic.rm.cnr.it> <872B0715-B051-49A2-9DE8-E23200EE41D3@iaa.es> X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.6.13.3 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 Dear Miguel, dear Andrea, from the X-ray perspective, I confirm basically Miguel's findings. The terms "soft", "medium", "hard" X-rays have been and are being used with very different meanings in different papers. What is "hard" for XMM-Newton and Chandra (2 to 8, 10 or 15 keV), was called sometimes "intermediate" in BeppoSAX papers. Moreover, I have almost never seen "medium" in a published paper. There are two possible ways out: * to substitute words with explicit energy ranges, as suggested for the optical bands. "Soft" may become "0.1-2.4 keV" (the energy range of the ROSAT All Sky-Survey); "hard" becomes "2-10 keV" (the energy range of ASCA surveys), or "2-8 keV" (if we want to follow the typical range being used in Chandra surveys), or "2-12 keV" (if one wants to follow the typical range used in XMM-Newton source catalogues); "medium" may become "0.5-4.5 keV" (the energy range of the Einstein Slew Survey). "Very hard" (it does not currently exist, but it should if gamma-ray astronomers agree) may become "15-200 keV" (typical BeppoSAX/PDS range). * to substitute explicit survey bands and sub-bands (ROSAT has, for instance, a "soft soft band, 0.1-0.4 keV, and a "hard soft band", 0.4-2.4 keV) for qualitative qualifiers; e.g.: "Einstein Slew Survey band" (".emss"), or "ROSAT All Sky Survey soft" (".rasss"), "PDS energy range" (".pds") instead of "soft", ... The consequences of either choice are clear: in the former, we risk mis-understanding old surveys (those done when I was not born, but still in use), in the latter we multiply we number of UCD endlessly. None of the above solutions is therefore satisfactory, from my point of view. As often in the VO context we are trying to extract order from chaos, i.e. one to derive standards where standards have never been applied in the past. My favorite (and surely controversial) solution? A more conservative and radical (!) approach: we remove "soft", "medium" and "hard", and keep only "em.X-rays". Regards, Matteo -- Matteo Guainazzi XMM-Newton SOC Matteo.Guainazzi@sciops.esa.int European Space Astronomy Center of ESA Phone: +34 91 8131 176 VILSPA, Apartado 50727, E-28080 Madrid Fax: +34 91 8131 172 From owner-ucd-sci@eso.org Mon Jun 13 12:10:54 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 j5DAAjq2014543 for ; Mon, 13 Jun 2005 12:10:46 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5DAAjKt014541 for ucd-sci-outgoing; Mon, 13 Jun 2005 12:10:45 +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 j5DAAeq2014462 for ; Mon, 13 Jun 2005 12:10:40 +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 j5DAAc73015596 for ; Mon, 13 Jun 2005 12:10:38 +0200 (CEST) Received: from (150.146.129.253) by e1000.artov.rm.cnr.it via smtp id 3594_75443278_dbf3_11d9_8f23_0002b3da0f69; Mon, 13 Jun 2005 12:11:07 +0200 Received: (qmail 3144 invoked by uid 508); 13 Jun 2005 10:10:32 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.032655 secs); 13 Jun 2005 10:10:32 -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 ; 13 Jun 2005 10:10:32 -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, 13 Jun 2005 12:10:31 +0200 Message-ID: <20050613121031.r4m3ie1qsyxw44cg@webmail.sic.rm.cnr.it> Date: Mon, 13 Jun 2005 12:10:31 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Re: T0: UCDs for "em" & "spect" References: <20050602152438.fdmq7yxtgdcgg40k@webmail.sic.rm.cnr.it> <18AB023D-4017-4716-BA26-6642EA40EC36@noao.edu> <20050603101129.diyu1dvr2wj4sg4g@webmail.sic.rm.cnr.it> <20050610110019.0nl83m6u32zkks0w@webmail.sic.rm.cnr.it> <872B0715-B051-49A2-9DE8-E23200EE41D3@iaa.es> In-Reply-To: <872B0715-B051-49A2-9DE8-E23200EE41D3@iaa.es> 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: 2005.6.13.5 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 Hi Miguel: >> In the case of x- and gamma-rays though there is no confusion, so I >> would keep the existing names... > Uhmm, for X-ray and gamma-rays I was asking X-ray and gamma-ray > people.... I gave those bands the names soft/medium/hard x-rays because I'm an x-ray man and I'm coming from an x/gamma-ray institute... > I know that UCDs are not for humans, but asking about what soft and > hard X-rays mean, > the answer is highly dependent on the asked astronomer. Usually they > talk only about > soft and hard. "medium-Xrays" is not understood. In fact, most people > I asked consider > hard X-ray as aprox 4-10 keV band (from maximmun energy from ROSAT/ > EINSTEIN to max energy by CHANDRA/ASCA/XMM)..... I do not know, but I > think that > keep em.X-ray.soft medium and hard is misunderstanding for X-ray > people. Another example, > ROSAT has a "hardness" ratio that is 0.2 keV-1.5keV (soft) vs. 1-4kev > (hard) (I do not remember exactly the > energies, sorry) where "soft" and "hard" refers to the detectors in > ROSAT (but they are used in this way in the articles).... You are perfectly right, usually they think in terms of the bandpass of their instrument. 4 keV are hard for ROSAT people because 4keV is hardER than 0.2 keV (their soft limit). For XMM people 10keV are hard. For BeppoSAX people 10 keV are medium, because the bandpass reaches 2-300 keV. We should not forget that we are parsing the em spectrum, we have to describe it, not the bandpasses of instruments. So, to avoid a narrow-minded interpretation of the ucd-words em.X-ray.* your suggestion (use energies instead of labels) is the safest one. > In gamma ray, the situation is similar. You can take a look the > INTEGRAL instruments, or CGRO ones. > The problem is that each energy range use techniques completely > different (due to the physics of the process) and em.gamma.hard is to > wide! It includes from only space instruments to only ground based > instruments (using the atmosphere as detector). In fact some gamma- > ray people make distinction between gamma-ray VeryHigh gamma-rays and > Ultra-High gamma rays as clearly different parts of the > electromagnetic spectrum.... I agree that gamma.hard is rather wide!! Probably we should go for at least three bands: hard/high VeryHigh UltraHigh 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-sci@eso.org Mon Jun 13 15:09:58 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 j5DD9iq2013807 for ; Mon, 13 Jun 2005 15:09:45 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5DD9iNv013806 for ucd-sci-outgoing; Mon, 13 Jun 2005 15:09:44 +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 j5DD9Iq2013671 for ; Mon, 13 Jun 2005 15:09:18 +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 j5DD9GXW016779 for ; Mon, 13 Jun 2005 15:09:16 +0200 (CEST) Received: from (150.146.129.253) by e1000.artov.rm.cnr.it via smtp id 15c6_69f3dbc6_dc0c_11d9_9d0f_0002b3da0f69; Mon, 13 Jun 2005 15:09:46 +0200 Received: (qmail 9956 invoked by uid 508); 13 Jun 2005 13:09:10 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.030497 secs); 13 Jun 2005 13:09:10 -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 ; 13 Jun 2005 13:09:09 -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, 13 Jun 2005 15:09:09 +0200 Message-ID: <20050613150909.dc3n3n7vynswgkkk@webmail.sic.rm.cnr.it> Date: Mon, 13 Jun 2005 15:09:09 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Re: T0: UCDs for "em" & "spect" References: <20050602152438.fdmq7yxtgdcgg40k@webmail.sic.rm.cnr.it> <18AB023D-4017-4716-BA26-6642EA40EC36@noao.edu> <20050603101129.diyu1dvr2wj4sg4g@webmail.sic.rm.cnr.it> <20050610110019.0nl83m6u32zkks0w@webmail.sic.rm.cnr.it> <872B0715-B051-49A2-9DE8-E23200EE41D3@iaa.es> <42AD5678.9010707@sciops.esa.int> In-Reply-To: <42AD5678.9010707@sciops.esa.int> 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: 2005.6.13.10 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 Quoting Matteo Guainazzi: > Dear Miguel, dear Andrea, > My favorite (and surely controversial) solution? A more conservative > and radical (!) approach: we remove "soft", "medium" and "hard", and > keep only "em.X-rays". No way, Matteo!! How do you define the beginning and the end energies of what you call x-ray :) ? The only solution is to decouple energies from sub-bands, and to describe "regions" of the em spectrum by numbers and not by labels. 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 ============================================================================== From owner-ucd-sci@eso.org Mon Jun 13 15:20:10 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 j5DDJpq2015305 for ; Mon, 13 Jun 2005 15:19:51 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5DDJpal015304 for ucd-sci-outgoing; Mon, 13 Jun 2005 15:19:51 +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 j5DDJiq2015286 for ; Mon, 13 Jun 2005 15:19:45 +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 j5DDJh73022211 for ; Mon, 13 Jun 2005 15:19:43 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1Dhoqm-0001Qf-IG for ucd-sci@ivoa.net; Mon, 13 Jun 2005 15:19:36 +0200 Mime-Version: 1.0 (Apple Message framework v622) In-Reply-To: <20050613121031.r4m3ie1qsyxw44cg@webmail.sic.rm.cnr.it> References: <20050602152438.fdmq7yxtgdcgg40k@webmail.sic.rm.cnr.it> <18AB023D-4017-4716-BA26-6642EA40EC36@noao.edu> <20050603101129.diyu1dvr2wj4sg4g@webmail.sic.rm.cnr.it> <20050610110019.0nl83m6u32zkks0w@webmail.sic.rm.cnr.it> <872B0715-B051-49A2-9DE8-E23200EE41D3@iaa.es> <20050613121031.r4m3ie1qsyxw44cg@webmail.sic.rm.cnr.it> Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: Content-Transfer-Encoding: 7bit From: "Frederic V. \"Rick\" Hessman" Subject: Re: T0: UCDs for "em" & "spect" Date: Mon, 13 Jun 2005 15:22:10 +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: 2005.6.13.10 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 >> In gamma ray, the situation is similar. You can take a look the >> INTEGRAL instruments, or CGRO ones. >> The problem is that each energy range use techniques completely >> different (due to the physics of the process) and em.gamma.hard is to >> wide! It includes from only space instruments to only ground based >> instruments (using the atmosphere as detector). In fact some gamma- >> ray people make distinction between gamma-ray VeryHigh gamma-rays and >> Ultra-High gamma rays as clearly different parts of the >> electromagnetic spectrum.... > > I agree that gamma.hard is rather wide!! Probably we should go for > at least three bands: > hard/high > VeryHigh > UltraHigh But the problem remains that "hard" and "very" and "ultra" are undefined. If the band is so wide, then use more than 3 bands, just like the present use in the radio (which is also wide). 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 Mon Jun 13 18:01:17 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 j5DG19q2029665 for ; Mon, 13 Jun 2005 18:01:09 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5DG19wx029664 for ucd-sci-outgoing; Mon, 13 Jun 2005 18:01:09 +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 j5DG14q2029645 for ; Mon, 13 Jun 2005 18:01:04 +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 j5DG11XW000097 for ; Mon, 13 Jun 2005 18:01:02 +0200 (CEST) Received: from (150.146.129.253) by e1000.artov.rm.cnr.it via smtp id 154a_68f47178_dc24_11d9_87fb_0002b3da0f69; Mon, 13 Jun 2005 18:01:32 +0200 Received: (qmail 13259 invoked by uid 508); 13 Jun 2005 16:00:55 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.034525 secs); 13 Jun 2005 16:00:55 -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 ; 13 Jun 2005 16:00:55 -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, 13 Jun 2005 18:00:55 +0200 Message-ID: <20050613180055.cwxyf7fm3u88css4@webmail.sic.rm.cnr.it> Date: Mon, 13 Jun 2005 18:00:55 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Re: T0 : extensions to em, obs, spect, instr References: <200506091846.j59Ik5kY003131@urania.cfa.harvard.edu> In-Reply-To: <200506091846.j59Ik5kY003131@urania.cfa.harvard.edu> 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: 2005.6.13.15 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 Quoting Jonathan McDowell : > Rick Hessman proposed a number of UCDs (May 30) and I wanted to > comment on them. > One was > spect.cont spectral continuum > I endorse adding this, it's very useful for my own data. If you mean that spect.cont is a sort of flux per unit something, than it'll be better to wait for a revision of the fluxDensity word > So here's my proposal for Rick's list, in which proposed new UCDs > are marked by a * (sort of the paleolinguistics convention of > marking hypothetical word forms with a *). > > Rick Jonathan > phys.grav-wave/em.grav-wave *phys.wave.gravitational > phys.particle.neutrino/em.neutrino *phys.particle.neutrino > instr.calib *obs.calib [Calibration observation] Yes, we could introduce the three sub-trees: S | phys.wave.* S | phys.particle.* (starting for the already present electron) S | obs.calib(.*) A few comments on the following list: > phot.calib obs.image;*obs.calib;phot.flux > [It's an image; it's for calibration; what are we calibrating - flux.] > spect;*obs.calib;phot.flux > [or, it's a spectrum...] > obs.calib.dome-flat > obs.image;obs.calib;*instr.det.flat;*instr.tel.dome > [We're calibrating the flatness of the detector; we're using > the dome to do it] > obs.calib.flux obs.image;*obs.calib;phot.flux > obs.calib.freq spect;*obs.calib;em.freq > [It's a spectrum; it's for calibration; we're calibrating freq] > obs.calib.guide-star meta.id;*obs.calib;*pos.astrometry > [If this is the name of the guide star used..] > obs.calib.phot [What's the difference with obs.calib.flux?] > obs.calib.pos obs.image;*obs.calib;*pos.astrometry (?) > obs.calib.sky-flat obs.image;obs.calib;*instr.det.flat > obs.calib.slit-mask *instr.spect.slit > obs.calib.spect spect;*obs.calib;em.wl > [If you mean by this an arc spectrum; what diff from obs.calib.wl?] > obs.calib.veloc spect;*obs.calib;src.veloc > obs.calib.wl spect;*obs.calib;em.wl > phot.calib.flux [same as obs.calib.flux?] > phot.calib.mag *obs.calib;em.opt.B (etc.) > pos.calib *obs.calib;pos > spect.calib spect;*obs.calib > spect.calib.wl spect;*obs.calib;em.wl > spect.calib.freq spect;*obs.calib;em.freq 1. the order is inverted: e.g. obs.image;*obs.calib;phot.flux ==> phot.flux;obs.calib spect;*obs.calib;src.veloc ==> src.veloc;obs.calib *obs.calib;em.opt.B ==> phot.mag;em.opt.B;obs.calib The same for Rick's suggestions: instr/tel;optics.focallength ==> optics.focallength;instr/tel 2. We have to maintain UCD-words, not UCDs 3. Saying: [It's an image; it's for calibration; what are we calibrating - flux.] means that you are probably describing a detaset, so an alternative description could be: [name (or url, or ...) of an image used for flux-calibrating other images of raw data] that could translate into : meta.id;obs.image;obs.calib We probably need a deeper discussion before introducing new trees. I agree with Jonathan: let's move quickly from WD to PR, and continue at the same time the discussion on new words, object types, events, etc... 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-sci@eso.org Tue Jun 14 04:27:54 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 j5E2Rl3v010503 for ; Tue, 14 Jun 2005 04:27:47 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5E2RlNx010501 for ucd-sci-outgoing; Tue, 14 Jun 2005 04:27:47 +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 j5E2Rh3v010484 for ; Tue, 14 Jun 2005 04:27:44 +0200 (MEST) Received: from fed1rmmtao04.cox.net (fed1rmmtao04.cox.net [68.230.241.35]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j5E2RfXW027874 for ; Tue, 14 Jun 2005 04:27:42 +0200 (CEST) Received: from [10.0.1.128] (really [68.231.133.145]) by fed1rmmtao04.cox.net (InterMail vM.6.01.04.00 201-2131-118-20041027) with ESMTP id <20050614022726.CUDZ23392.fed1rmmtao04.cox.net@[10.0.1.128]>; Mon, 13 Jun 2005 22:27:26 -0400 Mime-Version: 1.0 (Apple Message framework v730) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <18E084E6-5413-49C6-ABB0-CFAD3CFA1D80@noao.edu> Cc: Rob Seaman Content-Transfer-Encoding: 7bit From: Rob Seaman Subject: VOConcepts Date: Mon, 13 Jun 2005 19:27:31 -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: 2005.6.13.36 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 Howdy, I picked this list as the most appropriate place for this conversation. Please comment if you've got a different idea. This discussion is being driven by VOEvent issues, but the implications are broader. Some observations, assumptions, and conclusions: 1) UCDs appear to be the near term VO solution for semantic nomenclature. 2) VOEVENT will soon require a VOConcept style mechanism. 3) It seems obvious that VOConcept will borrow UCD syntax. 4) There seems to be significant delay implicit with establishing VOConcept as an official offshoot of UCDland. 5) Thus it seems that there will be significant pressure to establish VOConcept as a separate namespace of some sort under UCD. Operating under that assumption, the question is what that namespace will look like. The current snapshot is available at http:// monet.uni-sw.gwdg.de/twiki/bin/view/VOEvent/UnifiedContentDescriptors Here are my comments; 1) Proper names don't belong under the VOConcept namespace. Whether this is a separate namespace of its own, or whether proper names are handled by a completely separate mechanism, there is no need to specify something like "solar_system.Sun". Call me a radical, but I think the Sun should simply be called "Sun". In any event, a proper name of an object or process is distinct from any sort of classification of that particular object or process. 2) A "coronal mass ejection" is not equivalent to stars.corona;process.mass-loss.ejection, whether or not this precisely describes the physical event. My point is that just as with proper names, the astronomical community has chosen to assign "proper class names" to certain phenomena: CMEs, GRBs, KBOs, etc. We will fail if we seek to provide a namespace that usefully predicts what new class names will be needed in the future. Rather, we need a mechanism for adding new identifiers. 3) Which is it? Sun;process.pulsation or Sun;seismology? Again, "helioseismology" is an identifier distinct from the latter classification. 4) We need neither stars;planets nor stars.planets - just planets. I think we can assume for most purposes that if you are describing a planet that a star is somewhere in the neighborhood. 5) How about both stars.multiple and stars.binary? These are just two out of several clustering options, such as stars.cluster, for that matter. 6) It's interesting what stars.nearby is trying to describe, but this seems pretty parochial. There are a lot of "neighborhoods" scattered throughout astronomical semantics. Maybe there is some way to generalize this as some kind of operator notation. (On the other hand, that seems a bit precious.) 7) stars.supernova seems redundant. What else would it be? This is just the "planet" comment revisited. This is distinct from the star.variable family precisely because a SN is rather emphatic. 8) VOConcept (however constituted under whatever name) needs to represent stars, galaxies, and other objects. It isn't so obvious that "cosmology" is useful classification for VOEvent purposes. It isn't obvious what VO-wide purposes this classification would be used for in general. 9) VOEvent provides a good testbed for a number of VO technologies. It seems to me that a VOConcept list targeted precisely at VOEvent needs, perhaps augmented by some carefully selected concepts to fill in just a few missing items is a good place to start. Rob Seaman NOAO From owner-ucd-sci@eso.org Tue Jun 14 09:45:31 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 j5E7jP3v002908 for ; Tue, 14 Jun 2005 09:45:25 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5E7jPFe002907 for ucd-sci-outgoing; Tue, 14 Jun 2005 09:45:25 +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 j5E7jJ3v002889 for ; Tue, 14 Jun 2005 09:45:20 +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 j5E7jI73008811 for ; Tue, 14 Jun 2005 09:45:18 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1Di66g-000JES-RD for ucd-sci@ivoa.net; Tue, 14 Jun 2005 09:45:10 +0200 Mime-Version: 1.0 (Apple Message framework v622) In-Reply-To: <18E084E6-5413-49C6-ABB0-CFAD3CFA1D80@noao.edu> References: <18E084E6-5413-49C6-ABB0-CFAD3CFA1D80@noao.edu> Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <6e48c566b5bd5a515f17edbe25223fbd@Astro.physik.Uni-Goettingen.DE> Content-Transfer-Encoding: 7bit From: "Frederic V. \"Rick\" Hessman" Subject: Re: VOConcepts Date: Tue, 14 Jun 2005 09:47:45 +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: 2005.6.13.46 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 I think we'd all appreciate a general comment on whether ucd-sci is the right place for a discussion of what we have tenatively called VOConcept. Yes, there are lots of potential relations between VOCocept and UCD - see the Kyoto papers by S. Derriere and A. Allan - so there are lots of reasons to include both communities right now, but the ultimate connections will be indirect by popular demand within the UCD community, since the UCD design documents as they are currently written don't foresee any deviations beyond the VOTable-ish uses of UCDs. You might ask us to please shut up and worry about this later, but we're in the final throes of finishing VOEvent 1.0 and need to make a short-term decision about whether we ignore the problem of naming for now (at the cost of a loss of naming capability) or make an initial plunge in the direction of a UCD-like VOConcept (whatever you want to call it). Please vote: ___ Please stop talking about VOConcept in this list - we have enough to worry about as it is. ___ I think the two issues are still related enough to warrant inclusion in the ucd-sci discussion list for now. Based upon the tally, we can decide to continue (at least now and then) or to start a new list. If you vote for stopping, then please ignore the rest of this message and "have a nice day." :-) On 14 Jun 2005, at 4:27 am, Rob Seaman wrote: > I picked this list as the most appropriate place for this > conversation. Please comment if you've got a different idea. This > discussion is being driven by VOEvent issues, but the implications are > broader. Some observations, assumptions, and conclusions: > > 1) UCDs appear to be the near term VO solution for semantic > nomenclature. SOME semantic nomenclature. My feeling is that there is lots of resistance to a generalization and not just because of short-term release pressures. > 2) VOEVENT will soon require a VOConcept style mechanism. VOEvent needs it NOW. > 3) It seems obvious that VOConcept will borrow UCD syntax. > 4) There seems to be significant delay implicit with establishing > VOConcept as an official offshoot of UCDland. > 5) Thus it seems that there will be significant pressure to establish > VOConcept as a separate namespace of some sort under UCD. or, more likely, parallel to UCD. > Operating under that assumption, the question is what that namespace > will look like. The current snapshot is available at > http://monet.uni-sw.gwdg.de/twiki/bin/view/VOEvent/ > UnifiedContentDescriptors > > Here are my comments; > > 1) Proper names don't belong under the VOConcept namespace. Whether > this is a separate namespace of its own, or whether proper names are > handled by a completely separate mechanism, there is no need to > specify something like "solar_system.Sun". Call me a radical, but I > think the Sun should simply be called "Sun". In any event, a proper > name of an object or process is distinct from any sort of > classification of that particular object or process. I agree. For those cases (and not just the Sun) we need Jupiter RXJ1234+567 NGC12345 GRB12345 Note the combination of UCD and VOConcept in the last case and note that is fine for simple things but isn't necessarily the same thing for more complex naming purposes. > 2) A "coronal mass ejection" is not equivalent to > stars.corona;process.mass-loss.ejection, whether or not this precisely > describes the physical event. My point is that just as with proper > names, the astronomical community has chosen to assign "proper class > names" to certain phenomena: CMEs, GRBs, KBOs, etc. We will fail if > we seek to provide a namespace that usefully predicts what new class > names will be needed in the future. Rather, we need a mechanism for > adding new identifiers. Both. The complex naming will enable VO-technology to combine information in new ways maybe we haven't thought of. On the other hand, there has to be a human interface so that the user can use terms like "GRB" or "KBO". Yes, by combining UCD-like elements, we're getting close to starting an ontological analysis, but just barely and not necessarily because we WANT an ontology. Thus, CME = stars.corona;process.mass-loss.ejection is fine - one for the human, one for the computer. > 3) Which is it? Sun;process.pulsation or Sun;seismology? Again, > "helioseismology" is an identifier distinct from the latter > classification. Neither if "Sun" is kept as a proper name ;-) Sun ..... > 4) We need neither stars;planets nor stars.planets - just planets. I > think we can assume for most purposes that if you are describing a > planet that a star is somewhere in the neighborhood. > > 5) How about both stars.multiple and stars.binary? These are just two > out of several clustering options, such as stars.cluster, for that > matter. > > 6) It's interesting what stars.nearby is trying to describe, but this > seems pretty parochial. There are a lot of "neighborhoods" scattered > throughout astronomical semantics. Maybe there is some way to > generalize this as some kind of operator notation. (On the other > hand, that seems a bit precious.) No - this type of inclusion is exactly what is needed for a totally different VO application: education and public outreach. See http://www.communicatingastronomy.org/index.html for a VO-related group which is interested in such concepts. Nearby stars are interesting because they move on the sky. "Nearby" to a professional is perhaps not an interesting concept - just go to Sinbad and get the latest catalogue to pick out what you want - but identifying images available to the public as being interesting for studying proper motion and parallax is a great thing and it would be nice to have a universal identifier for that purpose. The names themselves are what's important - it's the need for a name which should drive the list. > 7) stars.supernova seems redundant. What else would it be? This is > just the "planet" comment revisited. This is distinct from the > star.variable family precisely because a SN is rather emphatic. The problem of hierarchical naming (and hence implict primitive ontologies) came up early in RTML: our first list was a random collection of names - "star", "supernova", "cepheid",... - but it became difficult to manage simply because of the danger of muliple entries. A minimum amount of hierarchy insures that the administration of the names is straight-forward and even eases their use in GUIs and other more mundane uses. > 8) VOConcept (however constituted under whatever name) needs to > represent stars, galaxies, and other objects. It isn't so obvious > that "cosmology" is useful classification for VOEvent purposes. It > isn't obvious what VO-wide purposes this classification would be used > for in general. I dropped "cosmology" from the original VOConcept list because my VOEvent colleagues were taken somewhat aback with how quickly such a list can grow and because there's no immediate need for "cosmology" in VOEvent. 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 Tue Jun 14 15:06:59 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 j5ED6q3v021239 for ; Tue, 14 Jun 2005 15:06:52 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5ED6qkI021238 for ucd-sci-outgoing; Tue, 14 Jun 2005 15:06:52 +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 j5ED6m3v021218 for ; Tue, 14 Jun 2005 15:06:48 +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 j5ED6k73018826 for ; Tue, 14 Jun 2005 15:06:47 +0200 (CEST) Received: (qmail 18200 invoked by uid 508); 14 Jun 2005 13:06:40 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.033231 secs); 14 Jun 2005 13:06:40 -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 ; 14 Jun 2005 13:06:40 -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 ; Tue, 14 Jun 2005 15:06:39 +0200 Message-ID: <20050614150639.qgep7mgcut1cskg8@webmail.sic.rm.cnr.it> Date: Tue, 14 Jun 2005 15:06:39 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Re: VOConcepts References: <18E084E6-5413-49C6-ABB0-CFAD3CFA1D80@noao.edu> <6e48c566b5bd5a515f17edbe25223fbd@Astro.physik.Uni-Goettingen.DE> In-Reply-To: <6e48c566b5bd5a515f17edbe25223fbd@Astro.physik.Uni-Goettingen.DE> 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: 2005.6.14.10 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 Dear Rick, I think I will not vote. I find the discussion (any discussion) among people with different ideas very stimulating. And sometimes also more useful than perfect agreement. Reducing the size of the group until you can feel eventually "among us" is not good at all in real life, certainly not in the VO. Just to show you that you are not the only one "uneasy" with somebody else's point of view, I'll make an example of how "uneasy" could feel an UCD-folk like me. Take for instance the UCD you proposed few days ago: instr.obsty.site;weather.seeing just to express "seeing" When I saw it I made a jump on my chair: why? In inverse order of importance: 1. The UCD-like syntax is wrong: first the "quantity", then the "qualifier" it should read: weather.seeing;instr.obsty.site 2. We are proposing UCD-words, not UCDs. If you propose an independent word for "seeing", ok, it's :weather.seeing 3. My mind works in terms of "how to assign ucd-words starting from a description, and then build an UCD" e.g. in term of the process to build an UCD from one or more keyword(s): the "keywords => ucd-words => UCDs" chain. It is impossible (in this framework) to go from the single keyword "seeing" to an UCD composed of two UCD-words (each one of these UCD-words needs its own description). Let's reverse the roles: you jump on the chair when you see the description of the src.class.* words. You are perfectly right. What is not said is that I do not use the description field to assign words/ucds: I use a series of words (keywords derived from the description) that are OR-ed, which is exactly equivalent to the loosier description you suggest. As I already said, the ucd vocabulary is not only composed of words that are "quantities". More and more "objects" are creeping in, and I can imagine the development of two sub-lists : a "q-list" slowly evolving (or even stabilized; after all the number of new (astro-)physical quantities per year is probably very easy to control!!) and an "o-list" (or whatever name we decide for it!!) for "non-quantities", both lists with the same syntax (just for simplicity and "interoperability" (!!), so that we can continue to build UCDs of the form: word[q-list];word[o-list] ... as we do today without knowing that we are actually doing 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-ucd-sci@eso.org Tue Jun 14 17:48:24 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 j5EFmF3v004529 for ; Tue, 14 Jun 2005 17:48:15 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5EFmF0w004528 for ucd-sci-outgoing; Tue, 14 Jun 2005 17:48:15 +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 j5EFmA3v004507 for ; Tue, 14 Jun 2005 17:48:11 +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 j5EFm873025219 for ; Tue, 14 Jun 2005 17:48:09 +0200 (CEST) Received: from [131.215.146.143] ([131.215.146.143]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id j5EFm6Qn019087 (version=TLSv1/SSLv3 cipher=RC4-SHA bits=128 verify=NO); Tue, 14 Jun 2005 08:48:06 -0700 In-Reply-To: <6e48c566b5bd5a515f17edbe25223fbd@Astro.physik.Uni-Goettingen.DE> References: <18E084E6-5413-49C6-ABB0-CFAD3CFA1D80@noao.edu> <6e48c566b5bd5a515f17edbe25223fbd@Astro.physik.Uni-Goettingen.DE> Mime-Version: 1.0 (Apple Message framework v622) Content-Type: text/plain; charset=US-ASCII; format=flowed Message-Id: <90d425de570af37c027e96fc39d04638@cacr.caltech.edu> Content-Transfer-Encoding: 7bit Cc: Roy Williams From: Roy Williams Subject: Re: VOConcepts Date: Tue, 14 Jun 2005 08:47:54 -0700 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: 2005.6.14.14 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 Jun 14, 2005, at 12:47 AM, Frederic V. "Rick" Hessman wrote: > I think we'd all appreciate a general comment on whether ucd-sci is > the right place for a discussion > of what we have tenatively called VOConcept. Rick It says in the UCD document "UCD describe astronomical quantities", meaning that they are "semantic meaning of data quantities", for example "phys.temperature". The implication is that UCD is NOT something like "satellite.Phobos;planet.Mars" and it is NOT something like "image.jpeg;human.JacquesChirac". I believe that the scope here is correct, and that extensions in to these other areas of knowledge will slow down the well-developed and sophisticated UCD effort. One of the best things about UCD is that it has been mined from thousands of table instances written by hundreds of astronomers, and therefore has unimpeachable credentials as a representation of the astronomical community. However, we should tackle wider questions when supported by use cases from the community. I believe the UCD effort should become part of a wider "semantics" effort, which may use UCD syntax for other areas of knowledge (eg. astrophysical events), or it may use OWL or RDF or other syntax. Frankly I don't care about the syntax part, that comes later: what is important in these semantics efforts is formalizing some branch of knowledge so that computers can record, compare, and deduce. > Yes, there are lots of potential relations between VOConcept and UCD I would prefer not to use the term "VOConcept", as it is too vague. I think the Semantics WG should concentrate on small, well-defined, areas. > You might ask us to please shut up and worry about this later, but > we're in the final throes of finishing VOEvent 1.0 and need to make a > short-term decision about whether we ignore the problem of naming for > now (at the cost of a loss of naming capability) or make an initial > plunge in the direction of a UCD-like VOConcept (whatever you want to > call it). I think that VOEvent should be published as version 1.0 Working Draft without any formal semantics for describing events, but rather describe events in natural language: "Looks like an exploding square galaxy" would be a typical description. Then in VOEvent 1.1 we can tackle formal semantics and other matters. And that formal description of astronomical events should not be called "VOConcept", but something more specific, such as "Unified Event Description", or "VOEventDescription". The first task of that discussion group is define what is the area of knowledge that is being covered, and agree to a short paragraph expressing what is an is not being formalized into syntax. For example, in VOEventDescription, is it an event when Michael Jackson is acquitted? How about when a new planet is discovered? How about a flare from a star that flares every 2 weeks? I believe that defining scope is the key to progress here, and that the tighter that scope, the better chances for agreement. Otherwise we are caught in a morass of ontological questions. In the words of Bill Clinton, "It depends upon what the meaning of the word is means. " > Please vote: > ___ Please stop talking about VOConcept in this list - we have enough > to worry about as it is. > ___ I think the two issues are still related enough to warrant > inclusion in the ucd-sci discussion list for now. > > Based upon the tally, we can decide to continue (at least now and > then) or to start a new list. I think the discussion of VOEventDescription should take place in the VOEvent mailing list, perhaps copying the entire Semantics WG when wider issues come up. Roy From owner-ucd-sci@eso.org Tue Jun 14 18:54:36 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 j5EGsT3v018620 for ; Tue, 14 Jun 2005 18:54:29 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5EGsTOw018619 for ucd-sci-outgoing; Tue, 14 Jun 2005 18:54:29 +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 j5EGsK3v018606 for ; Tue, 14 Jun 2005 18:54:21 +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 j5EGsIXW022921 for ; Tue, 14 Jun 2005 18:54:18 +0200 (CEST) X-Spam-Checker-Version: SpamAssassin 3.0.4 (2005-06-05) 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=3.0.4 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 4.3.4) with ESMTPSA id 18731820; Tue, 14 Jun 2005 09:54:06 -0700 In-Reply-To: <90d425de570af37c027e96fc39d04638@cacr.caltech.edu> References: <18E084E6-5413-49C6-ABB0-CFAD3CFA1D80@noao.edu> <6e48c566b5bd5a515f17edbe25223fbd@Astro.physik.Uni-Goettingen.DE> <90d425de570af37c027e96fc39d04638@cacr.caltech.edu> Mime-Version: 1.0 (Apple Message framework v730) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: Content-Transfer-Encoding: 7bit From: Rob Seaman Subject: Re: VOConcepts Date: Tue, 14 Jun 2005 09:54:03 -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: 2005.6.14.18 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 Roy says: > I think the discussion of VOEventDescription should take place in > the VOEvent mailing list, perhaps copying the entire Semantics WG > when wider issues come up. I've forwarded the last few messages to VOEvent. Further discussion will continue over there. Rob Seaman NOAO From owner-ucd-sci@eso.org Wed Jun 15 09:22:35 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 j5F7MRNm005724 for ; Wed, 15 Jun 2005 09:22:28 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5F7MRti005723 for ucd-sci-outgoing; Wed, 15 Jun 2005 09:22:27 +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 j5F7MHNm005692 for ; Wed, 15 Jun 2005 09:22:18 +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 j5F7MG73018864 for ; Wed, 15 Jun 2005 09:22:16 +0200 (CEST) Received: from sisley.uni-sw.gwdg.de ([134.76.205.209]) by alpha.uni-sw.gwdg.de with esmtp (Exim) id 1DiSDw-000g6j-LH for ucd-sci@ivoa.net; Wed, 15 Jun 2005 09:22:08 +0200 Mime-Version: 1.0 (Apple Message framework v622) In-Reply-To: <20050614150639.qgep7mgcut1cskg8@webmail.sic.rm.cnr.it> References: <18E084E6-5413-49C6-ABB0-CFAD3CFA1D80@noao.edu> <6e48c566b5bd5a515f17edbe25223fbd@Astro.physik.Uni-Goettingen.DE> <20050614150639.qgep7mgcut1cskg8@webmail.sic.rm.cnr.it> Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <25e0156b6e8fe2c7269c22897f2887f8@Astro.physik.Uni-Goettingen.DE> Content-Transfer-Encoding: 7bit From: "Frederic V. \"Rick\" Hessman" Subject: Re: src.class.* and weather.* Date: Wed, 15 Jun 2005 09:24:44 +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: 2005.6.14.46 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 > Just to show you that you are not the only one "uneasy" with somebody > else's point of view, I'll make an example of how "uneasy" could feel > an > UCD-folk like me. > Take for instance the UCD you proposed few days ago: > instr.obsty.site;weather.seeing just to express "seeing" > > When I saw it I made a jump on my chair: why? > In inverse order of importance: > > 1. The UCD-like syntax is wrong: first the "quantity", then the > "qualifier" > it should read: weather.seeing;instr.obsty.site Sorry - I confess that I haven't been worrying AT ALL about things like order, since the examples I've been worrying about don't depend upon it: is there really a fundamental difference between "seeing at an observatory"=weather.seeing;instr.obsty.site and "observatory's seeing"=intr.obsty.site;weather.seeing. Maybe for some extreme examples and onotolgy folks, but otherwise...... > 2. We are proposing UCD-words, not UCDs. If you propose an independent > word > for "seeing", ok, it's :weather.seeing True, but my bottom line is how to use them to express something. The UCD words are defined not just to be there but to be used. I forgot to distinguish between words and atoms - excuse moi! > 3. My mind works in terms of "how to assign ucd-words starting from a > description, and then build an UCD" e.g. in term of the process to > build an UCD from one or more keyword(s): > the "keywords => ucd-words => UCDs" chain. > It is impossible (in this framework) to go from the single keyword > "seeing" to an UCD composed of two UCD-words > (each one of these UCD-words needs its own description). Hmmm.... don't quite get that. My approach has been - I want to express something - look at the official UCD list to see what comes closest - if there's no exact/good match, look for related things to see if composing works - if there are no matches/composing solutions at all, think of new atoms or words, worrying about whether one needs a single atom/family of words or just additions to present families Not obvious that we're talking about a different process, but just my laziness in atom/word order, no specification of the "syntax code" and too few descriptions. > Let's reverse the roles: you jump on the chair when you see the > description > of the src.class.* words. > You are perfectly right. What is not said is that I do not use the > description > field to assign words/ucds: I use a series of words (keywords > derived from the description) that are OR-ed, > which is exactly equivalent to the loosier description you suggest. Sorry - still don't get this..... Are you saying that src.class.richness DOESN'T mean Abell class (even though that's what the official list says) or not? If it DOES mean that, then we need to rename the word. If it DOESN'T mean that, we need to change the description. Either way, we need to change something, because leaving it as it is will forever prevent someone from using richness for anything else with a good conscience. It's perfectly valid for someone to suggest a word based on their own needs (indeed, this is the BEST way), but the UCD community should make sure that the necessary generalizations are made when needed, and in the case of my list, I feel they are needed. > As I already said, the ucd vocabulary is not only composed of words > that are "quantities". More and more "objects" are creeping in, and I > can > imagine the development of two sub-lists : > > a "q-list" slowly evolving (or even stabilized; after all the number of > new (astro-)physical quantities per year is probably very easy > to control!!) > > and an "o-list" (or whatever name we decide for it!!) for > "non-quantities", > > both lists with the same syntax (just for simplicity and > "interoperability" (!!), > so that we can continue to build UCDs of the form: > > word[q-list];word[o-list] ... > > as we do today without knowing that we are actually doing it (!) I'm have been arguing for exactly this solution, but I have been getting the impression that others aren't so happy with it. I've trimmed down the VOConcept list to a bit more than 100 words/compositions to include only those which are needed by VOEvent. I'd be very happy to add "syntax codes" and formal descriptions, trim the list even further, mail everyone a down-to-earth ASCII file, and drop the whole issue of XML Schema integration if the UCD community would absorb VOConcept. 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 15 10:29:25 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 j5F8TINm019269 for ; Wed, 15 Jun 2005 10:29:18 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5F8TINc019268 for ucd-sci-outgoing; Wed, 15 Jun 2005 10:29:18 +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 j5F8TENm019257 for ; Wed, 15 Jun 2005 10:29:14 +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 j5F8TCXW017901 for ; Wed, 15 Jun 2005 10:29:12 +0200 (CEST) Received: (qmail 31232 invoked by uid 508); 15 Jun 2005 08:29:06 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.033055 secs); 15 Jun 2005 08:29:06 -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 ; 15 Jun 2005 08:29:06 -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 ; Wed, 15 Jun 2005 10:29:05 +0200 Message-ID: <20050615102905.vk0zlgvdmmlck4sc@webmail.sic.rm.cnr.it> Date: Wed, 15 Jun 2005 10:29:05 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Re: src.class.* and weather.* References: <18E084E6-5413-49C6-ABB0-CFAD3CFA1D80@noao.edu> <6e48c566b5bd5a515f17edbe25223fbd@Astro.physik.Uni-Goettingen.DE> <20050614150639.qgep7mgcut1cskg8@webmail.sic.rm.cnr.it> <25e0156b6e8fe2c7269c22897f2887f8@Astro.physik.Uni-Goettingen.DE> In-Reply-To: <25e0156b6e8fe2c7269c22897f2887f8@Astro.physik.Uni-Goettingen.DE> 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: 2005.6.14.46 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 >> In inverse order of importance: >> 1. The UCD-like syntax is wrong: first the "quantity", then the "qualifier" >> it should read: weather.seeing;instr.obsty.site > > Sorry - I confess that I haven't been worrying AT ALL about things like > order... That's why I said it's the least important thing :) >> 3. My mind works in terms of "how to assign ucd-words starting from a >> description, and then build an UCD" ... >> It is impossible (in this framework) to go from the single keyword >> "seeing" to an UCD composed of two UCD-words >> (each one of these UCD-words needs its own description). > > Hmmm.... don't quite get that. My approach has been > - I want to express something > - look at the official UCD list to see what comes closest > - if there's no exact/good match, look for related things to see if > composing works The above points correspond to the action: - find the ucd-word(s) that best match what you "want to express" which is followed by the action of - "building" the ucd from the words just found and according to ucd-syntax. These two actions together are performed by the "UCD-builder" that you can find, in its "beta-version", at http://vizier.u-strasbg.fr/UCD/cgi-bin/descr2ucd >> Let's reverse the roles: you jump on the chair when you see the description >> of the src.class.* words. >> You are perfectly right. What is not said is that I do not use the >> description >> field to assign words/ucds: I use a series of words (keywords >> derived from the description) that are OR-ed, >> which is exactly equivalent to the loosier description you suggest. > > Sorry - still don't get this..... Are you saying that > src.class.richness DOESN'T mean > Abell class (even though that's what the official list says) or not? It actually means : richness class e.g. Abell richness class (by the way, ther is also a "Abell distance class" !! Try "Abell class" as input for the builder...) > If it DOES mean > that, then we need to rename the word. If it DOESN'T mean that, we > need to change the description. Either way, we need to change > something, because leaving it as > it is will forever prevent someone from using richness for anything > else with a good conscience. Yes, we need to change the descriptions of all src.class.*, and this thanks to the discussion that is going on!! Andrea From owner-ucd-sci@eso.org Fri Jun 24 14:54:18 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 j5OCs54f014055 for ; Fri, 24 Jun 2005 14:54:05 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5OCs5wP014053 for ucd-sci-outgoing; Fri, 24 Jun 2005 14:54:05 +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 j5OCrv4f014029 for ; Fri, 24 Jun 2005 14:53:57 +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 j5OCrrXW009302 for ; Fri, 24 Jun 2005 14:53:55 +0200 (CEST) Received: (qmail 8285 invoked by uid 508); 24 Jun 2005 12:53:47 -0000 Received: from 10.1.1.2 by smtp1 (envelope-from , uid 500) with qmail-scanner-1.25-st-qms (clamdscan: 0.85. spamassassin: 3. perlscan: 1.25. Clear:RC:1(10.1.1.2):. Processed in 0.164369 secs); 24 Jun 2005 12:53:47 -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 ; 24 Jun 2005 12:53:46 -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 ; Fri, 24 Jun 2005 14:53:46 +0200 Message-ID: <20050624145346.xxa5qiwl0ri8wgsw@webmail.sic.rm.cnr.it> Date: Fri, 24 Jun 2005 14:53:46 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Draft list of ucd-words MIME-Version: 1.0 Content-Type: multipart/mixed; boundary="=_5ccufo2ecsqo" 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: 2005.6.24.5 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 This message is in MIME format. --=_5ccufo2ecsqo Content-Type: text/plain; charset=ISO-8859-1 Content-Disposition: inline Content-Transfer-Encoding: 7bit Dear all, after 26 days of discussion and contributions from many of you, I decided to sum up things and to modify the list of words according to my personal feelings. You can find the proposed list in the txt file appended. Of course the discussion is not over, but unfortunately we need a rather "stable" version soon. The PR-version of the document (the text accompanying the list) will be sent around after the meeting in Garching. A list of all (I hope !!) the modifications is shown below (Descr=changes in the description Canc=word erased Added= word added) : < S | em.IR.H |Descr < S | em.IR.J |Descr < S | em.IR.K |Descr < S | em.X-ray.hard |Descr < S | em.X-ray.medium |Descr < S | em.X-ray.soft |Descr < S | em.gamma.hard |Descr < S | em.gamma.soft |Descr < S | em.opt.B |Descr < S | em.opt.I |Descr < S | em.opt.R |Descr < S | em.opt.U |Descr < S | em.opt.V |Descr < | instr.angRes |Canc < Q | instr.bandpass |Descr < Q | instr.dispersion |Added < Q | instr.order |Added < | instr.spect |Canc < | instr.spect.dispersion |Canc < | instr.spect.order |Canc < | instr.spect.resolution |Canc < | instr.tel.focus |Canc < Q | instr.tel.focalLength |Added < P | meta.curation |Added < P | meta.version |Added < Q | obs.airMass |Added < S | obs.atmos |Added < Q | obs.atmos.extinction |Added < Q | obs.atmos.refractAngle |Added < S | obs.calib |Added < Q | phys.density |Descr < Q | phys.energy |Descr < Q | phys.energyDensity |Added < Q | phys.refractIndex |Added < Q | phys.transmission |Added < V | phys.veloc |Added < Q | phys.veloc.ang |Added < Q | phys.veloc.cmb |Added < Q | phys.veloc.dispersion |Added < Q | phys.veloc.escape |Added < Q | phys.veloc.expansion |Added < Q | phys.veloc.lg |Added < Q | phys.veloc.lsr |Added < Q | phys.veloc.microTurb |Added < Q | phys.veloc.orbital |Added < Q | phys.veloc.pulsat |Added < Q | phys.veloc.rotat |Added < Q | phys.veloc.transverse |Added < Q | pos.angDistance |Descr < Q | pos.az.azi |Added < S | pos.bodyrc |Added < | pos.earth.nutation |Canc < S | pos.earthop |Added < Q | pos.earthop.nutation |Added < Q | pos.eq.ha |Added < Q | pos.phaseAng |Added < V | pos.precess |Descr < Q | pos.resolution |Added < Q | spect.resolution |Added < | spect.veloc |Canc < E | spect.dopplerVeloc |Added < E | spect.dopplerVeloc.radio |Added < E | spect.dopplerVeloc.optic |Added < S | src |Descr < Q | src.class.distance |Descr < Q | src.class.richness |Descr < Q | src.class.starGalaxy |Descr < Q | src.class.struct |Descr < | src.orbital.veloc |Canc < | src.veloc |Canc < | src.veloc.ang |Canc < | src.veloc.cmb |Canc < | src.veloc.dispersion |Canc < | src.veloc.escape |Canc < | src.veloc.expansion |Canc < | src.veloc.lg |Canc < | src.veloc.lsr |Canc < | src.veloc.microTurb |Canc < | src.veloc.pulsat |Canc < | src.veloc.rotat |Canc < Q | time.obs |Added < Q | time.obs.end |Added < Q | time.obs.start |Added 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 ============================================================================== --=_5ccufo2ecsqo Content-Type: application/octet-stream; name="master_sent" Content-Disposition: attachment; filename="master_sent" Content-Transfer-Encoding: 7bit Q | arith | Arithmetic quantities S | arith.diff | Difference between two quantities described by the same UCD P | arith.factor | Numerical factor P | arith.grad | Gradient P | arith.rate | Rate (per time unit) S | arith.ratio | Ratio between two quantities described by the same UCD Q | arith.zp | Zero point S | em | Electromagnetic spectrum S | em.IR | Infrared part of the spectrum S | em.IR.15-30um | Infrared between 15 and 30 micron S | em.IR.3-4um | Infrared between 3 and 4 micron S | em.IR.30-60um | Infrared between 30 and 60 micron S | em.IR.4-8um | Infrared between 4 and 8 micron S | em.IR.60-100um | Infrared between 60 and 100 micron S | em.IR.8-15um | Infrared between 8 and 15 micron S | em.IR.H | Infrared between 1.5 and 2 micron S | em.IR.J | Infrared between 1.0 and 1.5 micron S | em.IR.K | Infrared between 2 and 3 micron S | em.UV | Ultraviolet part of the spectrum S | em.UV.10-50nm | Ultraviolet between 10 and 50 nm S | em.UV.100-200nm | Ultraviolet between 100 and 200 nm S | em.UV.200-300nm | Ultraviolet between 200 and 300 nm S | em.UV.50-100nm | Ultraviolet between 50 and 100 nm S | em.X-ray | X-ray part of the spectrum S | em.X-ray.hard | Hard X-ray (12 - 120 keV) S | em.X-ray.medium | Medium X-ray (2 - 12 keV) S | em.X-ray.soft | Soft X-ray (0.2 - 2 keV) Q | em.energy | Energy value in the em frame Q | em.freq | Frequency value in the em frame S | em.gamma | Gamma rays part of the spectrum S | em.gamma.hard | Hard gamma ray (>500 keV) S | em.gamma.soft | Soft gamma ray (120 - 500 keV) S | em.line | Designation of major atomic and molecular lines S | em.line.HI | 21cm hydrogen line S | em.line.Brgamma | Bracket gamma line S | em.line.Halpha | H-alpha line S | em.line.Hbeta | H-beta line S | em.line.Hgamma | H-gamma line S | em.line.OIII | [OIII] line S | em.mm | Millimetric part of the spectrum S | em.mm.100-200GHz | Millimetric between 100 and 200 GHz S | em.mm.1500-3000GHz | Millimetric between 1500 and 3000 GHz S | em.mm.200-400GHz | Millimetric between 200 and 400 GHz S | em.mm.30-50GHz | Millimetric between 30 and 50 GHz S | em.mm.400-750GHz | Millimetric between 400 and 750 GHz S | em.mm.50-100GHz | Millimetric between 50 and 100 GHz S | em.mm.750-1500GHz | Millimetric between 750 and 1500 GHz S | em.opt | Optical part of the spectrum S | em.opt.B | Optical band between 400 and 500 nm S | em.opt.I | Optical band between 750 and 1000 nm S | em.opt.R | Optical band between 600 and 750 nm S | em.opt.U | Optical band between 300 and 400 nm S | em.opt.V | Optical band between 500 and 600 nm S | em.radio | Radio part of the spectrum S | em.radio.100-200MHz | Radio between 100 and 200 MHz S | em.radio.12-30GHz | Radio between 12 and 30 GHz S | em.radio.1500-3000MHz | Radio between 1500 and 3000 MHz S | em.radio.20-100MHz | Radio between 20 and 100 MHz S | em.radio.200-400MHz | Radio between 200 and 400 MHz S | em.radio.3-6GHz | Radio between 3 and 6 GHz S | em.radio.400-750MHz | Radio between 400 and 750 MHz S | em.radio.6-12GHz | Radio between 6 and 12 GHz S | em.radio.750-1500MHz | Radio between 750 and 1500 MHz Q | em.wavenumber | Wavenumber value in the em frame Q | em.wl | Wavelength value in the em frame Q | em.wl.central | Central wavelength Q | em.wl.effective | Effective wavelength Q | instr | Instrument E | instr.background | Instrumental background Q | instr.bandpass | Bandpass (e.g.: band name) of instrument Q | instr.bandwidth | Bandwidth of the instrument Q | instr.baseline | Baseline for interferometry S | instr.beam | Beam Q | instr.calib | Calibration parameter S | instr.det | Detector Q | instr.det.noise | Instrument noise Q | instr.det.psf | Point Spread Function Q | instr.det.qe | Quantum efficiency Q | instr.dispersion | Dispersion of a spectrograph Q | instr.filter | Filter Q | instr.filter.transm | Filter transmission S | instr.fov | Field of view S | instr.obsty | Observatory satellite mission Q | instr.obsty.site.seeing | Seeing Q | instr.offset | Offset angle respect to main direction of observation Q | instr.order | Spectral order in a spectrograph Q | instr.param | Various instrumental parameters S | instr.pixel | Pixel S | instr.plate | Photographic plate Q | instr.plate.emulsion | Plate emulsion Q | instr.precision | Instrument precision Q | instr.saturation | Instrument saturation threshold Q | instr.scale | Instrument scale (for CCD, plate, image) Q | instr.sensitivity | Instrument sensitivity, detection threshold Q | instr.setup | Instrument configuration or setup Q | instr.skyLevel | Sky level Q | instr.skyTemp | Sky temperature Q | instr.tel | Telescope Q | instr.tel.focalLength | Telescope focal length P | meta | Metadata P | meta.bib | Bibliographic reference P | meta.bib.author | Author name P | meta.bib.bibcode | Bibcode P | meta.bib.fig | Figure in a paper P | meta.bib.journal | Journal name P | meta.bib.page | Page number P | meta.bib.volume | Volume number P | meta.code | Code or flag P | meta.code.class | Classification code P | meta.code.error | limit uncertainty error flag P | meta.code.member | Membership code P | meta.code.mime | MIME type P | meta.code.multip | Multiplicity or binarity flag P | meta.code.qual | Quality, precision, reliability flag or code P | meta.cryptic | Unknown or impossible to understand quantity P | meta.curation | Identity of man/organization responsible for the data Q | meta.dataset | Dataset S | meta.file | File S | meta.fits | FITS standard Q | meta.fits.software | Software used in generating FITS file P | meta.id | Identifier, name or designation P | meta.id.assoc | Identifier of associated counterpart P | meta.id.cross | Cross identification P | meta.id.parent | Identification of parent source P | meta.id.part | Part of identifier, suffix or sub-component S | meta.main | Main value of something S | meta.modelled | Quantity was produced by a model P | meta.note | Note or remark (longer than a code or flag) P | meta.number | Number (of things; e.g. nb of object in an image) P | meta.record | Record number P | meta.ref | Reference, or origin P | meta.ref.url | URL, web address S | meta.table | Table or catalogue P | meta.title | Title or explanation Q | meta.ucd | UCD P | meta.unit | Unit P | meta.version | Version S | obs | Observation Q | obs.airMass | Airmass S | obs.atmos | Atmosphere Q | obs.atmos.extinction | Atmospheric extinction Q | obs.atmos.refractAngle | Atmospheric refraction angle S | obs.calib | Calibration observation S | obs.field | Region covered by the observation S | obs.image | Image Q | obs.observer | Observer, discoverer Q | obs.param | Various observation or reduction parameter E | phot | Photometry E | phot.antennaTemp | Antenna temperature Q | phot.calib | Photometric calibration C | phot.color | Color index or magnitude difference Q | phot.color.excess | color excess Q | phot.color.reddFree | Dereddened color E | phot.count | Flux expressed in counts E | phot.fluence | fluence E | phot.flux | Photon flux Q | phot.flux.bol | Bolometric flux E | phot.flux.sb | Flux surface brightness E | phot.fluxDens | Flux density (per wl/freq/energy interval) E | phot.fluxDens.sb | Flux density surface brightness E | phot.limbDark | Limb-darkening coefficients E | phot.mag | Photometric magnitude Q | phot.mag.bc | Bolometric correction Q | phot.mag.bol | Bolometric magnitude Q | phot.mag.distMod | Distance modulus E | phot.mag.reddFree | Dereddened magnitude E | phot.mag.sb | Surface brightness in magnitude units E | phot.sb | Surface brightness Q | phys | Physical quantities Q | phys.SFR | Star formation rate E | phys.absorption | Extinction or absorption Q | phys.absorption.coeff | Absorption coefficient Q | phys.absorption.gal | Galactic extinction Q | phys.absorption.opticalDepth | Optical depth Q | phys.abund | Abundance Q | phys.abund.Fe | Fe/H abundance Q | phys.abund.X | Hydrogen abundance Q | phys.abund.Y | Helium abundance Q | phys.abund.Z | Metallicity abundance Q | phys.acceleration | Acceleration Q | phys.albedo | Albedo or reflectance Q | phys.angArea | Angular area Q | phys.angMomentum | Angular momentum V | phys.angSize | Angular size width diameter dimension extension major minor axis extraction radius Q | phys.angSize.smajAxis | angular size extent or extension of semi-major axis Q | phys.angSize.sminAxis | angular size extent or extension of semi-minor axis Q | phys.area | Area (in linear units) Q | phys.at | Atomic physics Q | phys.at.branchingRatio | Branching ratio Q | phys.at.collStrength | Collisional strength Q | phys.at.crossSection | Atomic cross-section Q | phys.at.damping | Atomic damping quantities (van der Waals) Q | phys.at.lande | Lande factor Q | phys.at.lineShift | Line shifting coefficient Q | phys.at.moment | Atomic momentum Q | phys.at.moment.electric | Electric momentum Q | phys.at.moment.magnetic | Magnetic momentum Q | phys.at.number | Atomic number Z Q | phys.at.oscStrength | Oscillator strength Q | phys.at.qn | Atomic quantum number Q | phys.at.qn.I | Nuclear spin quantum number Q | phys.at.qn.S | Electronic spin quantum number Q | phys.at.qn.L | Electronic L quantum number Q | phys.at.qn.J | Coupling of S and L qn Q | phys.at.qn.F | Coupling of J and I qn Q | phys.at.term | Atomic term Q | phys.at.transProb | Atomic transition probability, Einstein A coefficient Q | phys.at.wOscStrength | Weighted oscillator strength Q | phys.at.weight | Atomic weight Q | phys.atmol | Atomic and molecular physics (shared properties) Q | phys.atmol.coll | Related to collisions Q | phys.atmol.configuration | Configuration Q | phys.atmol.element | Element Q | phys.atmol.excitation | Atomic molecular excitation parameter Q | phys.atmol.ion | Ion S | phys.atmol.ionization | Related to ionization S | phys.atmol.level | Atomic level Q | phys.atmol.parity | Parity Q | phys.atmol.state.final | Quantity refers to atomic molecular final/ground state Q | phys.atmol.state.initial | Quantity refers to initial state Q | phys.atmol.sweight | Statistical weight S | phys.atmol.trans | Transition between states Q | phys.columnDensity | Column density Q | phys.density | Density (of mass, electron, ...) Q | phys.dielectric | Complex dielectric function Q | phys.dispMeasure | Dispersion measure V | phys.electField | Electric field S | phys.electron | Electron Q | phys.electron.degen | Electron degeneracy parameter Q | phys.emissMeasure | Emission measure Q | phys.emissivity | Emissivity Q | phys.energy | Energy Q | phys.energyDensity | Energy-density Q | phys.eos | Equation of state Q | phys.excitParam | Excitation parameter U Q | phys.gauntFactor | Gaunt factor/correction Q | phys.gravity | Surface gravity Q | phys.ionizParam | Ionization parameter Q | phys.ionizParam.coll | Collisional ionization Q | phys.ionizParam.rad | Radiative ionization E | phys.luminosity | Luminosity Q | phys.luminosity.fun | Luminosity function E | phys.magAbs | Absolute magnitude Q | phys.magAbs.bol | Bolometric absolute magnitude V | phys.magField | Magnetic field Q | phys.mass | Mass Q | phys.mass.light | Mass to light ratio Q | phys.mass.loss | Mass loss Q | phys.massYield | Mass yield Q | phys.mol | Molecular data Q | phys.mol.dipole | Molecular dipole Q | phys.mol.dipole.electric | Electric molecular dipole Q | phys.mol.dipole.magnetic | Magnetic molecular dipole Q | phys.mol.dissociation | Molecular dissociation Q | phys.mol.formationHeat | Formation heat for molecules Q | phys.mol.qn | Molecular quantum numbers Q | phys.mol.quadrupole | Molecular quadrupole Q | phys.mol.quadrupole.electric | Electric molecular quadrupole Q | phys.mol.quadrupole.magnetic | Magnetic molecular quadrupole S | phys.mol.rotation | Molecular rotation S | phys.mol.vibration | Molecular vibration Q | phys.polarization | Polarization Q | phys.polarization.rotMeasure | Rotation measure polarization Q | phys.polarization.stokes | Stokes polarization Q | phys.pressure | Pressure Q | phys.recombination.coeff | Recombination coefficient Q | phys.refractIndex | Refraction index Q | phys.size | Size (not angular) Q | phys.size.diameter | Diameter Q | phys.size.radius | Radius Q | phys.size.smajAxis | Linear semi major axis Q | phys.size.sminAxis | Linear semi minor axis Q | phys.temperature | Temperature Q | phys.temperature.effective | Effective temperature Q | phys.temperature.electron | Electron temperature Q | phys.transmission | Transmission (of filter, instrument, ...) V | phys.veloc | Space velocity Q | phys.veloc.ang | Angular velocity Q | phys.veloc.cmb | CMB velocity Q | phys.veloc.dispersion | Velocity dispersion Q | phys.veloc.escape | Escape velocity Q | phys.veloc.expansion | Expansion velocity Q | phys.veloc.lg | Local Group radial velocity Q | phys.veloc.lsr | Local Standard of Rest radial velocity Q | phys.veloc.microTurb | Microturbulence velocity Q | phys.veloc.orbital | Orbital velocity Q | phys.veloc.pulsat | Pulsational velocity Q | phys.veloc.rotat | Rotational velocity Q | phys.veloc.transverse | Transverse / tangential velocity Q | pos | Position and coordinates Q | pos.angDistance | Angular distance, elongation Q | pos.az | Position in alt-azimutal frame Q | pos.az.alt | Alt-azimutal altitude Q | pos.az.azi | Alt-azimutal azimut Q | pos.az.zd | Alt-azimutal zenith distance S | pos.barycenter | Barycenter S | pos.bodyrc | Body related coordinates S | pos.cartesian | Cartesian (rectangular) coordinates Q | pos.cartesian.x | Cartesian coordinate along the x-axis Q | pos.cartesian.y | Cartesian coordinate along the y-axis Q | pos.cartesian.z | Cartesian coordinate along the z-axis Q | pos.dirCos | Direction cosine V | pos.distance | Linear distance S | pos.earth | Coordinates related to Earth Q | pos.earth.altitude | Altitude on Earth Q | pos.earth.lon | Longitude on Earth S | pos.earthop | Earth orientation parameters Q | pos.earthop.nutation | Earth nutation S | pos.ecliptic | Ecliptic coordinates Q | pos.ecliptic.lat | Ecliptic latitude Q | pos.ecliptic.lon | Ecliptic longitude S | pos.errorEllipse | Positional error ellipse Q | pos.ephem | Ephemeris S | pos.eq | Equatorial coordinates Q | pos.eq.dec | Declination in equatorial coordinates Q | pos.eq.ha | Hour-angle Q | pos.eq.ra | Right ascension in equatorial coordinates Q | pos.eq.spd | South polar distance in equatorial coordinates Q | pos.frame | Reference frame used for positions S | pos.galactic | Galactic coordinates Q | pos.galactic.lat | Latitude in galactic coordinates Q | pos.galactic.lon | Longitude in galactic coordinates S | pos.galactocentric | Galactocentric coordinate system S | pos.geocentric | Geocentric coordinate system Q | pos.healpix | Hierarchical Equal Area IsoLatitude Pixelization S | pos.heliocentric | Heliocentric position coordinate (solar system bodies) Q | pos.htm | Hierarchical Triangular Mesh S | pos.lambert | Lambert projection Q | pos.lunar | Lunar coordinates Q | pos.lunar.occult | Occultation by lunar limb Q | pos.parallax | Parallax Q | pos.parallax.dyn | Dynamical parallax Q | pos.parallax.phot | Photometric parallaxes Q | pos.parallax.spect | Spectroscopic parallax Q | pos.parallax.trig | Trigonometric parallax Q | pos.phaseAng | Phase angle, e.g. elongation of earth from sun as seen from a third cel. object V | pos.pm | Proper motion Q | pos.posAng | Position angle of a given vector V | pos.precess | Precession (in equatorial coordinates) Q | pos.resolution | Angular resolution Q | pos.satellite | Position/coordinates of satellite or planet S | pos.supergalactic | Supergalactic coordinates Q | pos.supergalactic.lat | Latitude in supergalactic coordinates Q | pos.supergalactic.lon | Longitude in supergalactic coordinates P | pos.wcs | WCS keywords P | pos.wcs.cdmatrix | WCS CDMATRIX P | pos.wcs.crpix | WCS CRPIX P | pos.wcs.crval | WCS CRVAL P | pos.wcs.ctype | WCS CTYPE P | pos.wcs.naxes | WCS NAXES P | pos.wcs.naxis | WCS NAXIS P | pos.wcs.scale | WCS scale or scale of an image Q | spect | Spectroscopy Q | spect.doppler | Doppler parameter b E | spect.index | Spectral index E | spect.line | Spectral line E | spect.line.asymmetry | Line asymmetry E | spect.line.broad | Spectral line broadening Q | spect.line.broad.Stark | Stark line broadening coefficient E | spect.line.broad.Zeeman | Zeeman broadening E | spect.line.eqwidth | Line equivalent width E | spect.line.intensity | Line intensity E | spect.line.profile | Line profile E | spect.line.width | Spectral line fwhm Q | spect.resolution | Spectral (or velocity) resolution E | spect.dopplerVeloc | Radial velocity, derived from the shift of some spectral feature E | spect.dopplerVeloc.radio | Radial velocity derived from a frequency shift using the radio convention E | spect.dopplerVeloc.optic | Radial velocity derived from a wavelength shift using the optical convention S | src | Observed source viewed on the sky Q | src.class | Source classification (star, galaxy, cluster...) Q | src.class.color | Color classification Q | src.class.distance | Distance class e.g. Abell Q | src.class.luminosity | Luminosity class Q | src.class.richness | Richness class e.g. Abell Q | src.class.starGalaxy | Star/galaxy discriminator, stellarity index Q | src.class.struct | Structure classification e.g. Bautz-Morgan Q | src.density | Density of sources Q | src.ellipticity | Source ellipticity Q | src.impactParam | Impact parameter Q | src.morph | Morphology structure Q | src.morph.param | Morphological parameter Q | src.morph.scLength | Scale length for a galactic component (disc or bulge) Q | src.morph.type | Hubble morphological type (galaxies) Q | src.orbital | Orbital parameters Q | src.orbital.eccentricity | Orbit eccentricity Q | src.orbital.inclination | Orbit inclination Q | src.orbital.meanAnomaly | Orbit mean anomaly Q | src.orbital.node | Ascending node Q | src.orbital.periastron | Periastron Q | src.redshift | Redshift Q | src.redshift.phot | Photometric redshift Q | src.sample | Sample Q | src.spType | Spectral type MK Q | src.var | Variability of source E | src.var.amplitude | Amplitude of variation Q | src.var.index | Variability index Q | src.var.pulse | Pulse Q | stat | Statistical parameters Q | stat.Fourier | Fourier coefficient Q | stat.Fourier.amplitude | Amplitude Fourier coefficient P | stat.correlation | Correlation between two parameters P | stat.covariance | Covariance between two parameters P | stat.error | Statistical error P | stat.error.sys | Systematic error Q | stat.fit | Fit P | stat.fit.chi2 | Chi2 P | stat.fit.dof | Degrees of freedom P | stat.fit.goodness | Goodness or significance of fit S | stat.fit.omc | Observed minus computed Q | stat.fit.param | Parameter of fit P | stat.fit.residual | Residual fit P | stat.likelihood | Likelihood S | stat.max | Maximum or upper limit S | stat.mean | Mean, average value S | stat.median | Median value S | stat.min | Minimum or lowest limit Q | stat.param | Parameter P | stat.snr | Signal to noise ratio P | stat.stdev | Standard deviation Q | stat.value | Miscellaneous value P | stat.variance | Variance P | stat.weight | Statistical weight Q | time | Time Q | time.age | Age Q | time.crossing | Crossing time Q | time.epoch | Epoch, julian date Q | time.equinox | Equinox Q | time.expo | Exposure on-time, duration Q | time.expo.end | End time of exposure Q | time.expo.start | Start time of exposure Q | time.interval | Interval of time Q | time.lifetime | Lifetime Q | time.obs | Observation on-time, duration Q | time.obs.end | End time of observation Q | time.obs.start | Start time of observation Q | time.period | Period Q | time.phase | Phase Q | time.relax | Relaxation time Q | time.resolution | Time resolution Q | time.scale | Timescale --=_5ccufo2ecsqo-- From owner-ucd-sci@eso.org Tue Jun 28 15:17:02 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 j5SDGpHa004999 for ; Tue, 28 Jun 2005 15:16:51 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5SDGpmC004998 for ucd-sci-outgoing; Tue, 28 Jun 2005 15:16:51 +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 j5SDGjHa004971 for ; Tue, 28 Jun 2005 15:16:45 +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 j5SDGhXW016845 for ; Tue, 28 Jun 2005 15:16:43 +0200 (CEST) Received: from argiope.saclay.cea.fr (argiope.saclay.cea.fr [132.166.192.108]) by cirse.extra.cea.fr (8.13.4/8.13.4/CEAnet-Internet.5.0) with ESMTP id j5SDGXhr006577 for ; Tue, 28 Jun 2005 15:16:33 +0200 (MEST) Received: from pisaure.intra.cea.fr (unverified) by argiope.saclay.cea.fr (Content Technologies SMTPRS 4.3.17) with ESMTP id ; Tue, 28 Jun 2005 15:16:33 +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 j5SDFblZ031983; Tue, 28 Jun 2005 15:15:37 +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 j5SDGSed026250; Tue, 28 Jun 2005 15:16:28 +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 j5SDHBe5028856 ; Tue, 28 Jun 2005 15:17:12 +0200 (MEST) Message-ID: <42C14DAA.2020400@cea.fr> Date: Tue, 28 Jun 2005 15:16:26 +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: ucd-sci@ivoa.net CC: Andrea Preite Martinez Subject: Re: Draft list of ucd-words References: <20050624145346.xxa5qiwl0ri8wgsw@webmail.sic.rm.cnr.it> In-Reply-To: <20050624145346.xxa5qiwl0ri8wgsw@webmail.sic.rm.cnr.it> 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: 2005.6.28.10 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 everybody, some comments... A) global comments A.0 instr.obsty - S | instr.obsty | Observatory satellite mission you mean Observatory or satellite mission -> Observatory / satellite mission ? - Q | instr.obsty.site.seeing | Seeing Is this the global seeing resulting of detector, instrument, atmosphere... or does it concern only the instrumental part? If so, did we need a obs.seeing? Not clear for me. A.1 phys.veloc.trans - Q | phys.veloc.transverse | Transverse / tangential velocity I am not sure that these two definitions are (allways?) compatible. Moreover, transverse is perhaps not the right word. It isn't tangential, as opposed to radial? Or do we need two definitions? But velocity transverse to the mouvment seems strange/unappropriate? A.2 radial velocities they are now spread in 3 separate group - phys.veloc.[lg|lsr] - spect.dopplerVeloc.* - src.redshift.* Is spect.dopplerVeloc.* equivalent to radial velocity? Some "reduced" RV, to the earth center, to the sun are not defined/available, ( see gc, geoc and hc in src.veloc.radial at http://www.imcce.fr/fr/expert/ssvo/wgovp/ucdtree.html ) and the frame corresponding to spect.dopplerVeloc is not defined. So, phys.veloc.hc for heliocentric value is not available, while the corresponding position pos.heliocentric is. I suggest to complete RV and clearly identify them using phys.veloc.radial.[gc|geoc|hc|lg|lsr] and to change description of spect.dopplerVeloc.* to clearly define the information about the "place of measurement" : ObsLocation (in case of spacecraft it can be tricky) or referential frame. A.3 pos.* the big case/issue already clarified but still some inhomogeneity or confusion (at least in my head). A.3.1 pos.earth Q | pos.earth.lon | Longitude on Earth exists but not latitude! Q | pos.earth.altitude | Altitude on Earth exists but not distance which give the distance to the center A.3.2 lon/lat/alt/dist For any coordinate system (pos.*centric and mainly pos.bodyrc) the four informations can be usefull, and if pos.distance is available the others don't exist, and can be used to construct composed words. I suggest introduction of pos.[alt|lat|lon] (at least the two last ones) to be able to used composed words like pos.lat;pos.bodyrc or to introduce [dist|lat|lon] for all coordinate system and alt for some of them. A.3.3 Some subdivision are not sufficients. pos.bodyrc as mentionned above ;-) but also : pos.precess, pos.earthop.nutation and pos.earthop too see corresponding needs at http://www.imcce.fr/fr/expert/ssvo/wgovp/ucdtree.html B additional comments mainly related to (small?) solar system objects ( or extra solar system sytem and not only planetary one ;-) ) B.1 Mean motion >>>>> Andrea Preite Martinez wrote: >>>>> >>>>>> 12. src.orbital.meanMotion >>>>>> I suppose it is an average angular velocity (src.veloc.ang;stat.mean). >>>>>> No strong feelings about it. >>>>> No, the mean motion is not an average angular velocity. It is given by the third Kepler's law: n2 * a3 = cste with n the mean motion and a the semi-major axis of the orbit. So it is a corner stone of the computation of orbits: we need it as a proper UCD. B.2 asteroid Absolute Magnitude H is the absolute magnitude which already exist in the UCD (phys.magAbs) for asteroids we need also the slope parameter usually called G : phys.magAbs.G but seen as a kind of "calibration" parameter may be a better place somewhere else in the UCD tree is perhaps possible? B.3 pos.precess I guess pos.precess could be more generic because it could be used both for the equatorial and ecliptic precessions. Perhaps we should change .ra and .dec to .lon and .lat and, in the same way, .dzeta, .z and ,theta should be change because they usually refer to the equatorial precession when the ecliptic precession parameters are expressed with other letters. B.4 pos.eop.* Jonathan McDowell wrote: > * pos.eop.* I like, although as we become more active on other worlds isn't it likely > that we'll be needing similar parameters for Mars, etc.? But maybe it's fine for now. yes, SolarSystem people mind about this. But the Earth is a special case which is used often in ephemeris computation. I guess that first this UCD should be created and then a more generic one should be added ? That's all for the moment. sincerely yours, Pierre Andrea Preite Martinez wrote: > Dear all, > > after 26 days of discussion and contributions from many of you, I decided to > sum up things and to modify the list of words according to my personal > feelings. > > You can find the proposed list in the txt file appended. > Of course the discussion is not over, but unfortunately we need a rather > "stable" version soon. > The PR-version of the document (the text accompanying the list) will be sent > around after the meeting in Garching. ... > > 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 > ============================================================================== ------------------------------------------------------------------ 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-ucd-sci@eso.org Wed Jun 29 00:13:36 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 j5SMDPmK025683 for ; Wed, 29 Jun 2005 00:13:25 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5SMDPC3025682 for ucd-sci-outgoing; Wed, 29 Jun 2005 00:13:25 +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 j5SMDLmK025674 for ; Wed, 29 Jun 2005 00:13:21 +0200 (MEST) Received: from smtp.ucolick.org (santo.ucolick.org [128.114.23.204]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j5SMDI73011344 for ; Wed, 29 Jun 2005 00:13:19 +0200 (CEST) Received: from localhost (localhost [127.0.0.1]) by smtp.ucolick.org (Postfix) with ESMTP id 152F55D714 for ; Tue, 28 Jun 2005 15:13:13 -0700 (PDT) Received: from geneva.ucolick.org (geneva.ucolick.org [128.114.23.183]) (using TLSv1 with cipher DHE-RSA-AES256-SHA (256/256 bits)) (No client certificate requested) by smtp.ucolick.org (Postfix) with ESMTP id B538E11406 for ; Tue, 28 Jun 2005 15:13:12 -0700 (PDT) Received: from geneva.ucolick.org (localhost [127.0.0.1]) by geneva.ucolick.org (8.13.1/8.12.10) with ESMTP id j5SMDC7S012280 for ; Tue, 28 Jun 2005 15:13:12 -0700 Received: (from sla@localhost) by geneva.ucolick.org (8.13.1/8.13.1/Submit) id j5SMDBWj012279 for ucd-sci@ivoa.net; Tue, 28 Jun 2005 15:13:11 -0700 Date: Tue, 28 Jun 2005 15:13:11 -0700 From: Steve Allen To: ucd-sci@ivoa.net Subject: Re: Draft list of ucd-words Message-ID: <20050628221311.GA12268@ucolick.org> References: <20050624145346.xxa5qiwl0ri8wgsw@webmail.sic.rm.cnr.it> Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii Content-Disposition: inline In-Reply-To: <20050624145346.xxa5qiwl0ri8wgsw@webmail.sic.rm.cnr.it> User-Agent: Mutt/1.4.2.1i X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.6.28.24 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 Fri 2005-06-24T14:53:46 +0200, Andrea Preite Martinez hath writ: > < Q | obs.atmos.refractAngle |Added I am a bit mystified by the utility of this quantity. In actual practice it is usually impossible to distinguish the amount of refraction from the amount of unmodelled telescope flexure. It is a rare situation when it is actually possible to make a measurement of the refraction angle. Any error is simply accommodated by the ever-requisite fine pointing adjustment of the telescope. Under what circumstances is refractAngle actually used? What drives any requirements for it to be accurate or precise? On the other hand, the differential refraction, which is to say both the change in the amount of refraction over a field of view and the atmospheric dispersion due to refraction are quantities which are often calculated and used. The differential refraction and the atmospheric dispersion are needed for designing and manufacturing focal plane constructs for multi object spectrographs. The dispersion enters directly into the decision about the position angle at which a slit spectrograph should be oriented. A map of the differential refraction is necessary for multi-slit spectrographs and for fiber-fed spectrographs. In my experience these two are needed far more often, and to greater precision, than the absolute amount of refraction. > S | pos.earthop | Earth orientation parameters > Q | pos.earthop.nutation | Earth nutation These specifications seem incomplete, but I'm not sure what they are supposed to be communicating. As a starter for discussion, does nutation refer to IAU 2000A model, IAU 2000B model, or the models resulting from the FK5-based revision performed between 1976/1984, or the nutation based on the older Newcomb models of precession, or what? Is polar motion and UT1 relevant? Do they use the IAU 2000 models, or one of the older forms used in previous versions of the IERS conventions, or the even older FK5 forms, or what? > Q | pos.eq.ha | Hour-angle > Q | pos.az | Position in alt-azimutal frame > Q | pos.az.alt | Alt-azimutal altitude > Q | pos.az.azi | Alt-azimutal azimut > Q | pos.az.zd | Alt-azimutal zenith distance If I understand the work of the general relativists who have been contributing to various IAU initiatives over the past two decades then all of the above quantities do not have precisely-defined meanings. There is no mathematical framework for a rigorous mapping of celestial sphere to observation angles which is valid at the microarcsecond level. The meaning of hour angle has been called into question at a precision much less tight by the IAU 2000 redefinition of UT1 and the introduction of the CIO/CEO- and TIO/TEO- based expressions. There is an active IAU committee trying to work out nomenclature for the "classical" vs. the "CIO-based" versions of these sorts of quantities. Should the definitions of these admit that they may not be meaningful at the milliarcsecond level and give references to the draft documents which explain why? On Tue 2005-06-28T15:16:26 +0200, Pierre Didelon hath writ: > A.3.1 pos.earth > Q | pos.earth.lon | Longitude on Earth > exists but not latitude! > Q | pos.earth.altitude | Altitude on Earth > exists but not distance which give the distance to the center > > A.3.2 lon/lat/alt/dist In the context of FITS WCS Paper III we decided that it was not a good idea to admit the concepts of latitude, longitude, and height into the standard. (Note, by the way that I strongly prefer to use the term "height" rather than "altitude" or "elevation". The geodetic community also uses "height" at least in part to avoid confusion with the other two, which may be angles.) Unless there is also a UCD word something like pos.earth.geodatum it is not possible to associate a precise meaning with .lon, .lat, and .alt As we point out in FITS WCS Paper III, there are something like 1000 different geodetic datums in use, and some of their positions differ from each other by kilometers. Rather than burden FITS with the need to recognize even a small subset of those datums we decided to omit angular body coordinates and stick to Cartesian coordinates only. True, even Cartesian coordinates technically require the specification of a datum, but in current usage all the Cartesian terrestrial datums differ by only about 0.1 m. I recognize that there is a very strong tradition for the use of angular body coordinates, but if precise meaning is required they are not a good idea. -- Steve Allen WGS-84 (GPS) UCO/Lick Observatory Natural Sciences II, Room 165 Lat +36.99858 University of California Voice: +1 831 459 3046 Lng -122.06014 Santa Cruz, CA 95064 http://www.ucolick.org/~sla/ Hgt +250 m From owner-ucd-sci@eso.org Wed Jun 29 05:25:59 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 j5T3PnmK019759 for ; Wed, 29 Jun 2005 05:25:49 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5T3PnFb019757 for ucd-sci-outgoing; Wed, 29 Jun 2005 05:25:49 +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 j5T3PjmK019751 for ; Wed, 29 Jun 2005 05:25:45 +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 j5T3PgXW012164 for ; Wed, 29 Jun 2005 05:25:43 +0200 (CEST) X-Spam-Checker-Version: SpamAssassin 3.0.4 (2005-06-05) on noao.edu X-Spam-Level: X-Spam-Status: No, score=-2.6 required=4.5 tests=AWL,BAYES_00 autolearn=ham version=3.0.4 X-TFF-CGPSA-Version: 1.4f1 X-TFF-CGPSA-Filter: Scanned Received: from [72.254.6.5] (account seaman HELO [10.5.95.225]) by noao.edu (CommuniGate Pro SMTP 4.3.5) with ESMTPSA id 18991210; Tue, 28 Jun 2005 20:25:30 -0700 In-Reply-To: <20050624145346.xxa5qiwl0ri8wgsw@webmail.sic.rm.cnr.it> References: <20050624145346.xxa5qiwl0ri8wgsw@webmail.sic.rm.cnr.it> Mime-Version: 1.0 (Apple Message framework v730) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <4B410189-D4C3-4D71-8F7E-3B0ADA7A2CD5@noao.edu> Cc: Rob Seaman Content-Transfer-Encoding: 7bit From: Rob Seaman Subject: Re: Draft list of ucd-words Date: Tue, 28 Jun 2005 20:25:31 -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: 2005.6.28.32 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 Jun 24, 2005, at 5:53 AM, Andrea Preite Martinez wrote: > Of course the discussion is not over, but unfortunately we need a > rather "stable" version soon. > I'm concerned about the general nature of the UCDs in the list. It seems to me that the most useful quantities are those such as em.opt. [UBVRI] that have the broadest or most empirically determined definitions. Steve points out the shortcomings of several of the more precisely definable quantities. Many of these require some more complicated data structure to even attempt to describe the underlying physics. A simple scalar will never suffice. For instance, Steve picks apart several of the WCS related UCDs. What is the precise benefit to the VO or its users of selecting UCDs to convey these quantities rather than STC elements? Note that I'm not seeking to reopen the "UCDs are not XML" discussion - rather, in a loose analogy in which XML represents a variety of data types and UCDs represent names, what is the point of providing names for scalar quantities that are of no utility standing by themselves? I suppose you could attach a UCD to a more complicated XML (or other kind of) data structure - but how would that work exactly? Wouldn't this possibility need to be reflected within the UCD mechanism itself? The other thing about "em.opt.B" is that it represents a quantity whose definition is completely within the control of the international astronomical community. Other than additionally specifying exactly what it is whose measured Johnson B magnitude is being quoted (some object through some aperture), there is no intrinsic ambiguity. Some of the other quantities "belong" to non- astronomical constituencies at least as much as they belong to us. Not trying to make trouble - please point me to a document or discussion thread if such carping is old news. Rob Seaman NOAO From owner-ucd-sci@eso.org Wed Jun 29 10:15:45 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 j5T8FamK025789 for ; Wed, 29 Jun 2005 10:15:36 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5T8Fax6025788 for ucd-sci-outgoing; Wed, 29 Jun 2005 10:15:36 +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 j5T8FVmK025773 for ; Wed, 29 Jun 2005 10:15:31 +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 j5T8FT73024722 for ; Wed, 29 Jun 2005 10:15:29 +0200 (CEST) Received: from argiope.saclay.cea.fr (argiope.saclay.cea.fr [132.166.192.108]) by cirse.extra.cea.fr (8.13.4/8.13.4/CEAnet-Internet.5.0) with ESMTP id j5T8FOJM006487 for ; Wed, 29 Jun 2005 10:15:24 +0200 (MEST) Received: from pisaure.intra.cea.fr (unverified) by argiope.saclay.cea.fr (Content Technologies SMTPRS 4.3.17) with ESMTP id ; Wed, 29 Jun 2005 10:15:23 +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 j5T8ESWu030628; Wed, 29 Jun 2005 10:14:28 +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 j5T8FMCl003185; Wed, 29 Jun 2005 10:15:22 +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 j5T8EkSO004026 ; Wed, 29 Jun 2005 10:15:22 +0200 (MEST) Message-ID: <42C25875.80501@cea.fr> Date: Wed, 29 Jun 2005 10:14:45 +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: ucd-sci@ivoa.net CC: sla@ucolick.org Subject: Re: Draft list of ucd-words References: <20050624145346.xxa5qiwl0ri8wgsw@webmail.sic.rm.cnr.it> <20050628221311.GA12268@ucolick.org> In-Reply-To: <20050628221311.GA12268@ucolick.org> 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: 2005.6.29.1 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 Steve Allen wrote: > On Fri 2005-06-24T14:53:46 +0200, Andrea Preite Martinez hath writ: ... >>S | pos.earthop | Earth orientation parameters >>Q | pos.earthop.nutation | Earth nutation > > These specifications seem incomplete, but I'm not sure what > they are supposed to be communicating. open corresponding items ( pos.eop, pos.eop.nutation, pos.eop.pole ) at http://www.imcce.fr/fr/expert/ssvo/wgovp/ucdtree.html to see more possible elements. Passing the mouse over the proposed UCD display a few words meaning in the upper part of the window ;-) > > As a starter for discussion, does nutation refer to > IAU 2000A model, IAU 2000B model, or the models resulting from > the FK5-based revision performed between 1976/1984, or > the nutation based on the older Newcomb models of precession, or what? > > Is polar motion and UT1 relevant? Do they use the IAU 2000 models, or > one of the older forms used in previous versions of the IERS > conventions, or the even older FK5 forms, or what? > > >>Q | pos.eq.ha | Hour-angle > > >>Q | pos.az | Position in alt-azimutal frame >>Q | pos.az.alt | Alt-azimutal altitude >>Q | pos.az.azi | Alt-azimutal azimut >>Q | pos.az.zd | Alt-azimutal zenith distance > > > If I understand the work of the general relativists who have been > contributing to various IAU initiatives over the past two decades then > all of the above quantities do not have precisely-defined meanings. > There is no mathematical framework for a rigorous mapping of celestial > sphere to observation angles which is valid at the microarcsecond > level. Perhaps, but a lot of measurements with much less accuracy exist. UCD has not the goal to replace STC or any equivalent, only give some (not all) informations about used quantity. > > The meaning of hour angle has been called into question at > a precision much less tight by the IAU 2000 redefinition of UT1 > and the introduction of the CIO/CEO- and TIO/TEO- based > expressions. There is an active IAU committee trying to work > out nomenclature for the "classical" vs. the "CIO-based" > versions of these sorts of quantities. > > Should the definitions of these admit that they may > not be meaningful at the milliarcsecond level and give > references to the draft documents which explain why? > > On Tue 2005-06-28T15:16:26 +0200, Pierre Didelon hath writ: > > >>A.3.1 pos.earth >> Q | pos.earth.lon | Longitude on Earth >>exists but not latitude! >>Q | pos.earth.altitude | Altitude on Earth >>exists but not distance which give the distance to the center >> >>A.3.2 lon/lat/alt/dist > > > In the context of FITS WCS Paper III we decided that it was not a good idea > to admit the concepts of latitude, longitude, and height into the > standard. > > (Note, by the way that I strongly prefer to use the term "height" rather > than "altitude" or "elevation". The geodetic community also uses "height" > at least in part to avoid confusion with the other two, which may be angles.) Whatever is the choosen term, it is needed, even in STC, at least to specify the altitude of the observing place. > > Unless there is also a UCD word something like pos.earth.geodatum it is not > possible to associate a precise meaning with .lon, .lat, and .alt > > As we point out in FITS WCS Paper III, there are something like 1000 > different geodetic datums in use, and some of their positions differ > from each other by kilometers. Rather than burden FITS with the need > to recognize even a small subset of those datums we decided to omit > angular body coordinates and stick to Cartesian coordinates only. > > True, even Cartesian coordinates technically require the specification > of a datum, but in current usage all the Cartesian terrestrial datums > differ by only about 0.1 m. > > I recognize that there is a very strong tradition for the use of > angular body coordinates, but if precise meaning is required they > are not a good idea. > > -- > Steve Allen WGS-84 (GPS) > UCO/Lick Observatory Natural Sciences II, Room 165 Lat +36.99858 > University of California Voice: +1 831 459 3046 Lng -122.06014 > Santa Cruz, CA 95064 http://www.ucolick.org/~sla/ Hgt +250 m ^ | perhaps not precise enough, but nevertheless usefull quantities ;-) -- 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/ ------------------------------------------------------------------ Puissé-je toujours marcher avec la beauté devant moi. Dicton Navajo Tony Hillerman - Les clowns sacrés ------------------------------------------------------------------ From owner-ucd-sci@eso.org Wed Jun 29 12:19:21 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 j5TAJFmK023360 for ; Wed, 29 Jun 2005 12:19:15 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5TAJFiL023359 for ucd-sci-outgoing; Wed, 29 Jun 2005 12:19:15 +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 j5TAJAmK023353 for ; Wed, 29 Jun 2005 12:19:11 +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 j5TAJ8XW024039 for ; Wed, 29 Jun 2005 12:19:09 +0200 (CEST) Received: from [192.168.1.100] (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 j5TAJ6Qn028372 (version=TLSv1/SSLv3 cipher=RC4-SHA bits=128 verify=NO); Wed, 29 Jun 2005 03:19:07 -0700 In-Reply-To: <42C25875.80501@cea.fr> References: <20050624145346.xxa5qiwl0ri8wgsw@webmail.sic.rm.cnr.it> <20050628221311.GA12268@ucolick.org> <42C25875.80501@cea.fr> Mime-Version: 1.0 (Apple Message framework v622) Content-Type: multipart/alternative; boundary=Apple-Mail-24--779777 Message-Id: <1055be75840525c23e851cc2b61bfe2b@cacr.caltech.edu> Cc: Roy Williams , sla@ucolick.org From: Roy Williams Subject: Re: Draft list of ucd-words Date: Wed, 29 Jun 2005 03:19:00 -0700 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: 2005.6.29.5 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 --Apple-Mail-24--779777 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; format=flowed I see questions on this list about precise definitions of UCD, and I do not think it is relevant. We are not building a self-consistent data model of astronomy, but rather we are pragmatically taking the list of quantities that real astronomers have used in 5000 real tables at Vizier. If a table is published in ApJ that defines the "altitude" of their observatory (pos.earth.altitude), it is not for us to say the writer was a fool, it is for us to make sure there is a UCD for that concept. Similarly, the STC is irrelevant here. If astronomical tables contain RA and Dec, then there should be pos.eq.ra and pos.eq.dec. It is not for us to say that RA and Dec do not always have unambiguous definitions. California Institute of Technology 626 395 3670 --Apple-Mail-24--779777 Content-Transfer-Encoding: 7bit Content-Type: text/enriched; charset=US-ASCII I see questions on this list about precise definitions of UCD, and I do not think it is relevant. We are not building a self-consistent data model of astronomy, but rather we are pragmatically taking the list of quantities that real astronomers have used in 5000 real tables at Vizier. If a table is published in ApJ that defines the "altitude" of their observatory (pos.earth.altitude), it is not for us to say the writer was a fool, it is for us to make sure there is a UCD for that concept. Similarly, the STC is irrelevant here. If astronomical tables contain RA and Dec, then there should be pos.eq.ra and pos.eq.dec. It is not for us to say that RA and Dec do not always have unambiguous definitions. HelveticaCalifornia Institute of Technology 626 395 3670 --Apple-Mail-24--779777-- From owner-ucd-sci@eso.org Wed Jun 29 17:48:06 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 j5TFlomK026615 for ; Wed, 29 Jun 2005 17:47:50 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5TFlocr026614 for ucd-sci-outgoing; Wed, 29 Jun 2005 17:47:50 +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 j5TFlWmK026562 for ; Wed, 29 Jun 2005 17:47:32 +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 j5TFlTXW006096 for ; Wed, 29 Jun 2005 17:47:30 +0200 (CEST) X-Spam-Checker-Version: SpamAssassin 3.0.4 (2005-06-05) on noao.edu X-Spam-Level: X-Spam-Status: No, score=-2.5 required=4.5 tests=AWL,BAYES_00,HTML_20_30, HTML_MESSAGE autolearn=no version=3.0.4 X-TFF-CGPSA-Version: 1.4f1 X-TFF-CGPSA-Filter: Scanned Received: from [72.254.55.195] (account seaman HELO [10.5.95.219]) by noao.edu (CommuniGate Pro SMTP 4.3.5) with ESMTPSA id 19000242; Wed, 29 Jun 2005 08:47:15 -0700 In-Reply-To: <1055be75840525c23e851cc2b61bfe2b@cacr.caltech.edu> References: <20050624145346.xxa5qiwl0ri8wgsw@webmail.sic.rm.cnr.it> <20050628221311.GA12268@ucolick.org> <42C25875.80501@cea.fr> <1055be75840525c23e851cc2b61bfe2b@cacr.caltech.edu> Mime-Version: 1.0 (Apple Message framework v730) Content-Type: multipart/alternative; boundary=Apple-Mail-3-18916721 Message-Id: <8DAB1A37-2372-40F0-B2D5-46DD5250C0A7@noao.edu> Cc: Rob Seaman , Roy Williams , sla@ucolick.org From: Rob Seaman Subject: Re: Draft list of ucd-words Date: Wed, 29 Jun 2005 08:47:17 -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: 2005.6.29.15 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 --Apple-Mail-3-18916721 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Hi Roy, > I see questions on this list about precise definitions of UCD, and > I do not think it is relevant. We are not building a self- > consistent data model of astronomy, but rather we are pragmatically > taking the list of quantities that real astronomers have used in > 5000 real tables at Vizier. That's precisely my point. If the idea is merely to construct a complete (and indeed, consistent) list of the minimal number of identifiers necessary to capture some large (and growing) set of tables from the astronomical literature - well, then, what is the point of discussion at all? Harvest all the identifiers, correct typos, remove synonyms and you're done. Rather, we appear to be chartered to do something different - to construct a poor man's ontology. Certainly UCDs are often offered up as the pragmatic path out of ontological jungles. > If a table is published in ApJ that defines the "altitude" of > their observatory (pos.earth.altitude), it is not for us to say the > writer was a fool, it is for us to make sure there is a UCD for > that concept. Right - and I agree with Steve that this should rather be called "height". But this begs the question of whether we need to provide UCDs for *both* height above the Earth's surface *and* distance from its center. And dozens of other questions for this one little identifier such as how (or whether) to express the shape of the earth such that "height" from one table means even approximately the same thing as "altitude" from another. > Similarly, the STC is irrelevant here. If astronomical tables > contain RA and Dec, then there should be pos.eq.ra and pos.eq.dec. > It is not for us to say that RA and Dec do not always have > unambiguous definitions. But naming has the implication of defining. By attaching the same UCD to values from two different tables we are asserting that for [all | most | many | some | any] purposes that these values represent identical "things". Certainly VO users will take it this way. Why else provide common class identifiers other than to assert a common class? We are clearly seeking some semantic middle ground between instantiating a separate UCD for each column of each table (e.g., Hertzsprung.1947.fig_1.pos.eq.ra) and the evanescent dream of a full astronomical ontology. If that is not the case, I would argue that rather than seat a committee to decide these issues that some purely mechanical process be sought to convert the column headings from each month's new batch of tables from the literature into UCDs. I think we are precisely building a simple kind of data model of astronomy. It is indeed intended to be self-consistent, but certainly not to be complete (either in extent or expressive ability). Ideally we will understand the holes in the data model as well as the consensus descriptors. In general, holes should be left where simple UCD expressions don't suffice. We will fail if we aim too close to completeness. We will also fail if the UCD "data model" (or whatever folks want to call it) diverges too far from a coherent expression of the domain of astronomy. The quickest way to wrap up the current exercise is to severely limit the list of UCDs to only contain the least controversial. If columns from 5000 tables have left holes in the list of UCDs, one might expect that this reflects underlying difficulties of astronomical semantics that we will not more easily overcome. The way to extend a robust UCD process into the future is to provide an explicit namespace mechanism from the start. This will allow capturing controversial or peripheral identifiers such as VOConcept, but will also allow us to wipe the etch-a-sketch clean with new version(s) of subject dependent list(s) of UCDs. If later we decide that v1:pos.earth.height should indeed have been v2:pos.earth.altitude, there needs to be a lightweight way to make the transition. This is also the way to ensure a speedy process in the future. The alternative is a heavyweight process such as FITS standardization - talk about it for ten years and still leave some folks unhappy and eager to violate the standard. Better an incomplete list of UCDs than an incorrect one. Better two lists than one. Rob Seaman NOAO --Apple-Mail-3-18916721 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1
Hi Roy,

I see questions on this list = about precise definitions of UCD, and I do not think it is relevant. We = are not building a self-consistent data model of astronomy, but rather = we are pragmatically taking the list of quantities that real astronomers = have used in 5000 real tables at Vizier.=A0
<= BR class=3D"khtml-block-placeholder">
That's precisely my point.=A0 = If the idea is merely to construct a complete (and indeed, consistent) = list of the minimal number of identifiers necessary to capture some = large (and growing) set of tables from the astronomical literature - = well, then, what is the point of discussion at all? =A0Harvest all the = identifiers, correct typos, remove synonyms and you're done. =A0Rather, = we appear to be chartered to do something different - to construct a = poor man's ontology.=A0 Certainly UCDs are often offered up as the = pragmatic path out of ontological jungles.

=A0If a table is published in ApJ = that defines the "altitude" of their observatory (pos.earth.altitude), = it is not for us to say the writer was a fool, it is for us to make sure = there is a UCD for that concept.

Right - and I agree with Steve = that this should rather be called "height".=A0 But this begs the = question of whether we need to provide UCDs for *both* height above the = Earth's surface *and* distance from its center.=A0 And dozens of other = questions for this one little identifier such as how (or whether) to = express the shape of the earth such that "height" from one table means = even approximately the same thing as "altitude" from = another.

Similarly, the STC is irrelevant here. If astronomical tables = contain RA and Dec, then there should be pos.eq.ra and pos.eq.dec. It is = not for us to say that RA and Dec do not always have unambiguous = definitions.

But naming has the = implication of defining.=A0 By attaching the same UCD to values from two = different tables we are asserting that for [all | most | many | some | = any] purposes that these values represent identical "things".=A0 = Certainly VO users will take it this way.=A0 Why else provide common = class identifiers other than to assert a common = class?

We are clearly seeking some = semantic middle ground between instantiating a separate UCD for each = column of each table (e.g., Hertzsprung.1947.fig_1.pos.eq.ra) and the = evanescent dream of a full astronomical ontology.=A0 If that is not the = case, I would argue that rather than seat a committee to decide these = issues that some purely mechanical process be sought to convert the = column headings from each month's new batch of tables from the = literature into UCDs.

I think we are precisely = building a simple kind of data model of astronomy.=A0 It is indeed = intended to be=A0self-consistent, but certainly not to be complete = (either in extent or expressive ability).=A0 Ideally we will understand = the holes in the data model as well as the consensus descriptors.=A0 In = general, holes should be left where simple UCD expressions don't = suffice.=A0 We will fail if we aim too close to completeness.=A0 We will = also fail if the UCD "data model" (or whatever folks want to call it) = diverges too far from a coherent expression of the domain of = astronomy.

The = quickest way to wrap up the current exercise is to severely limit the = list of UCDs to only contain the least controversial.=A0 If columns from = 5000 tables have left holes in the list of UCDs, one might expect that = this reflects underlying difficulties of astronomical semantics that we = will not more easily overcome.

The way to extend a robust = UCD process into the future is to provide an explicit namespace = mechanism from the start.=A0 This will allow capturing controversial or = peripheral identifiers such as VOConcept, but will also allow us to wipe = the etch-a-sketch clean with new version(s) of subject dependent list(s) = of UCDs.=A0 If later we decide that v1:pos.earth.height should indeed = have been v2:pos.earth.altitude, there needs to be a lightweight way to = make the transition.=A0 This is also the way to ensure a speedy process = in the future.=A0 The alternative is a heavyweight process such as FITS = standardization - talk about it for ten years and still leave some folks = unhappy and eager to violate the standard.

Better an incomplete list = of UCDs than an incorrect one.=A0 Better two lists than = one.

Rob = Seaman
NOAO
= --Apple-Mail-3-18916721-- From owner-ucd-sci@eso.org Wed Jun 29 18:28:21 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 j5TGSFmK004851 for ; Wed, 29 Jun 2005 18:28:15 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5TGSFmG004850 for ucd-sci-outgoing; Wed, 29 Jun 2005 18:28:15 +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 j5TGS5mK004821 for ; Wed, 29 Jun 2005 18:28:06 +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 j5TGS3XW007762 for ; Wed, 29 Jun 2005 18:28:04 +0200 (CEST) Received: from [131.215.146.143] ([131.215.146.143]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id j5TGS2Qn023112 (version=TLSv1/SSLv3 cipher=RC4-SHA bits=128 verify=NO); Wed, 29 Jun 2005 09:28:02 -0700 In-Reply-To: <8DAB1A37-2372-40F0-B2D5-46DD5250C0A7@noao.edu> References: <20050624145346.xxa5qiwl0ri8wgsw@webmail.sic.rm.cnr.it> <20050628221311.GA12268@ucolick.org> <42C25875.80501@cea.fr> <1055be75840525c23e851cc2b61bfe2b@cacr.caltech.edu> <8DAB1A37-2372-40F0-B2D5-46DD5250C0A7@noao.edu> Mime-Version: 1.0 (Apple Message framework v622) Content-Type: text/plain; charset=ISO-8859-1; format=flowed Message-Id: <0f37cba6a09192ef4c0f597ce6aa4349@cacr.caltech.edu> Cc: ucd-sci@ivoa.net, sla@ucolick.org From: Roy Williams Subject: Re: Draft list of ucd-words Date: Wed, 29 Jun 2005 09:27:51 -0700 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: 2005.6.29.17 X-Virus-Scanned: by amavisd-new Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id j5TGSEmK004846 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 > By attaching the same UCD to values from two different tables we are > asserting that ..... these values represent identical "things".  We are asserting that there exists a context in which they are the same. Question: In what context is an R-magnitude and a B-magnitude the same thing? Answer: when you count photons without regard to their wavelength. > some purely mechanical process be sought to convert the column > headings from each month's new batch of tables from the literature > into UCDs. That was the original conception. The only structure was some grouping. Then we tried to get clever, and replaced the single UCD "magnitude error" by two components ("magnitude" and "error"). That was the slippery slope towards a data model. And here we are up to our asses in ontological alligators! > ..... building a simple kind of data model of astronomy. > ..... evanescent dream of a full astronomical ontology I don't think these things are possible. Everyone has their own opinion. It would be too complex and unwieldy. > The way to extend a robust UCD process into the future is to provide > an explicit namespace mechanism from the start.  We tried this before about 2 years ago, but it was vetoed. The problem with namespace is that it reduces interoperability -- there was a fear that everyone would simply use their own namespace. Roy From owner-ucd-sci@eso.org Wed Jun 29 18:56:16 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 j5TGu9mK009379 for ; Wed, 29 Jun 2005 18:56:09 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5TGu91c009378 for ucd-sci-outgoing; Wed, 29 Jun 2005 18:56:09 +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 j5TGu5mK009374 for ; Wed, 29 Jun 2005 18:56:05 +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 j5TGu2XW008606 for ; Wed, 29 Jun 2005 18:56:03 +0200 (CEST) X-Spam-Checker-Version: SpamAssassin 3.0.4 (2005-06-05) on noao.edu X-Spam-Level: X-Spam-Status: No, score=-2.6 required=4.5 tests=AWL,BAYES_00,HTML_40_50, HTML_MESSAGE autolearn=ham version=3.0.4 X-TFF-CGPSA-Version: 1.4f1 X-TFF-CGPSA-Filter: Scanned Received: from [72.254.55.195] (account seaman HELO [10.5.95.219]) by noao.edu (CommuniGate Pro SMTP 4.3.5) with ESMTPSA id 19001586; Wed, 29 Jun 2005 09:55:48 -0700 In-Reply-To: <0f37cba6a09192ef4c0f597ce6aa4349@cacr.caltech.edu> References: <20050624145346.xxa5qiwl0ri8wgsw@webmail.sic.rm.cnr.it> <20050628221311.GA12268@ucolick.org> <42C25875.80501@cea.fr> <1055be75840525c23e851cc2b61bfe2b@cacr.caltech.edu> <8DAB1A37-2372-40F0-B2D5-46DD5250C0A7@noao.edu> <0f37cba6a09192ef4c0f597ce6aa4349@cacr.caltech.edu> Mime-Version: 1.0 (Apple Message framework v730) Content-Type: multipart/alternative; boundary=Apple-Mail-4-23029817 Message-Id: Cc: Rob Seaman From: Rob Seaman Subject: Re: Draft list of ucd-words Date: Wed, 29 Jun 2005 09:55:50 -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: 2005.6.29.18 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 --Apple-Mail-4-23029817 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Roy says; > We are asserting that there exists a context in which they are the > same. Question: In what context is an R-magnitude and a B-magnitude > the same thing? Answer: when you count photons without regard to > their wavelength. Photon counting and the logarithmic ratios of the magnitude scale are very different beasts. If you are going to pursue photon counting you are likely to end up with something resembling IRAF's QPOE interface. Similarly with expressing world coordinates - there is an irreducible core of complexity. The way to deal with this is to embrace the complexity, not attempt to implement false simplicity. > The problem with namespace is that it reduces interoperability -- > there was a fear that everyone would simply use their own namespace. There are 340+ sessions here at JavaOne - and something like 340 different - and differently named - java class libraries and other "thingies" being discussed. Many of these overlap each other. It hasn't seemed to hurt the 15,000 attendees any. Folks may well define utilitarian namespaces willy-nilly for purposes internal to their own projects. They will, however, gravitate toward a few standard choices for any expressions that need to be shared with the larger VO community. You aren't describing a problem - you describe an opportunity. Rob --Apple-Mail-4-23029817 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1
Roy = says;

We are = asserting that there exists a context in which they are the same. = Question: In what context is an R-magnitude and a B-magnitude the same = thing? Answer: when you count photons without regard to their = wavelength.

Photon counting and the = logarithmic ratios of the magnitude scale are very different beasts.=A0 = If you are going to pursue photon counting you are likely to end up with = something resembling IRAF's QPOE interface.=A0 Similarly with expressing = world coordinates - there is an irreducible core of complexity.=A0 The = way to deal with this is to embrace the complexity, not attempt to = implement false simplicity.

The problem with namespace is that it reduces = interoperability -- there was a fear that everyone would simply use = their own namespace.

There are 340+ sessions = here at JavaOne - and something like 340 different - and differently = named - java class libraries and other "thingies" being discussed.=A0 = Many of these overlap each other.=A0 It hasn't seemed to hurt the 15,000 = attendees any.=A0 Folks may well define utilitarian namespaces = willy-nilly for purposes internal to their own projects.=A0 They will, = however, gravitate toward a few standard choices for any expressions = that need to be shared with the larger VO = community.

You aren't describing a = problem - you describe an opportunity.

Rob
= --Apple-Mail-4-23029817-- From owner-ucd-sci@eso.org Wed Jun 29 19:20:17 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 j5THKAmK013068 for ; Wed, 29 Jun 2005 19:20:10 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5THKATH013065 for ucd-sci-outgoing; Wed, 29 Jun 2005 19:20:10 +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 j5THK1mK012963 for ; Wed, 29 Jun 2005 19:20:01 +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 j5THJx73014798 for ; Wed, 29 Jun 2005 19:19:59 +0200 (CEST) Received: from [131.215.146.143] ([131.215.146.143]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-6.6) with ESMTP id j5THJwQn000889 (version=TLSv1/SSLv3 cipher=RC4-SHA bits=128 verify=NO); Wed, 29 Jun 2005 10:19:58 -0700 In-Reply-To: References: <20050624145346.xxa5qiwl0ri8wgsw@webmail.sic.rm.cnr.it> <20050628221311.GA12268@ucolick.org> <42C25875.80501@cea.fr> <1055be75840525c23e851cc2b61bfe2b@cacr.caltech.edu> <8DAB1A37-2372-40F0-B2D5-46DD5250C0A7@noao.edu> <0f37cba6a09192ef4c0f597ce6aa4349@cacr.caltech.edu> Mime-Version: 1.0 (Apple Message framework v622) Content-Type: text/plain; charset=ISO-8859-1; format=flowed Message-Id: Cc: ucd-sci@ivoa.net From: Roy Williams Subject: Re: Draft list of ucd-words Date: Wed, 29 Jun 2005 10:19:47 -0700 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: 2005.6.29.18 X-Virus-Scanned: by amavisd-new Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id j5THKAmK013057 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 >> We are asserting that there exists a context in which they are the >> same. Question: In what context is an R-magnitude and a B-magnitude >> the same thing? Answer: when you count photons without regard to >> their wavelength. > Photon counting and the logarithmic ratios of the magnitude scale are > very different beasts.  If you are going to pursue photon counting you > are likely to end up with something resembling IRAF's QPOE interface.  > Similarly with expressing world coordinates - there is an irreducible > core of complexity.  The way to deal with this is to embrace the > complexity, not attempt to implement false simplicity. OK I am showing my ignorance of what magnitude exactly means. But it sounds like you are taking a hard line that the concept of "magnitude" is meaningless by itself, and has no place in the UCD list. Surely it has some rigorous definition in terms of photons or flux or energy or SOMETHING? And therefore a context in which they can be compared. And what is wrong with world coordinates? We have UCDs for CRVAL and CRPIX and CTYPE and all those good WCS keywords. Are they also so poorly defined as to be useless? They are well-defined in the Calabretta papers, aren't they? >> The problem with namespace is that it reduces interoperability -- >> there was a fear that everyone would simply use their own namespace. > > You aren't describing a problem - you describe an opportunity. The namespaces for UCD was my suggestion. I was voted down. From owner-ucd-sci@eso.org Wed Jun 29 19:32:41 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 j5THWXmK015070 for ; Wed, 29 Jun 2005 19:32:33 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5THWXvq015069 for ucd-sci-outgoing; Wed, 29 Jun 2005 19:32:33 +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 j5THWSmK015061 for ; Wed, 29 Jun 2005 19:32:28 +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 j5THWQ73015164 for ; Wed, 29 Jun 2005 19:32:27 +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 1DngQ3-00048L-PP; Wed, 29 Jun 2005 18:32:17 +0100 In-Reply-To: <8DAB1A37-2372-40F0-B2D5-46DD5250C0A7@noao.edu> References: <20050624145346.xxa5qiwl0ri8wgsw@webmail.sic.rm.cnr.it> <20050628221311.GA12268@ucolick.org> <42C25875.80501@cea.fr> <1055be75840525c23e851cc2b61bfe2b@cacr.caltech.edu> <8DAB1A37-2372-40F0-B2D5-46DD5250C0A7@noao.edu> Mime-Version: 1.0 (Apple Message framework v730) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <578357BE-8513-488B-BF49-EB57A6E8415C@astro.gla.ac.uk> Cc: Rob Seaman , Roy Williams , sla@ucolick.org Content-Transfer-Encoding: 7bit From: Norman Gray Subject: Re: Draft list of ucd-words Date: Wed, 29 Jun 2005 18:32:14 +0100 To: ucd-sci@ivoa.net X-Mailer: Apple Mail (2.730) 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: 2005.6.29.19 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 Greetings, On 2005 Jun 29 , at 16.47, Rob Seaman wrote: >> If a table is published in ApJ that defines the "altitude" of >> their observatory (pos.earth.altitude), it is not for us to say >> the writer was a fool, it is for us to make sure there is a UCD >> for that concept. > > Right - and I agree with Steve that this should rather be called > "height". The Gene Ontology folk have described a few key ideas that helped them create a big and very successful ontology. Though GO has problems -- some quite fundamental -- non-ontologists do actually use it to do actual science. Some of these `rules' are rather obvious, such as `involve users', but Rob's message is a hook for a couple of the non-obvious ones. GO uses opaque labels for every concept, so that pos.earth.altitude and pos.earth.height would both be ucd12345 or something. They do this (i) to avoid arguments about which noun it should be, (ii) so they can version them easily (when are we going to have fight about replacing pos.earth.height with pos.earth.height2? whereas no-one has a sentimental attachment to ucd12345), (iii) so users aren't tempted to use their intuition about what the labels mean, and are forced to use the project's tools to discover and resolve labels, and (iiia) to make it transparently clear to everyone that the label really doesn't matter -- it's just a string which keys to a careful description elsewhere. I'm not suggesting replacing all the UCDs with numbers (don't worry), but suggesting that it might be best to avoid `obvious' names, and even that it might be a virtue than a vice to have names which are mnemonic but still vague enough to force folk to look up careful definitions _before_ they use them. > But this begs the question of whether we need to provide UCDs for > *both* height above the Earth's surface *and* distance from its > center. Agreeing with what I take to be Rob's argument, I think this is settled by an observation that these distinct concepts do or do not appear in multiple published tables, where `multiple' represents some vague threshold number less than ten but definitely more than one. > And dozens of other questions for this one little identifier such > as how (or whether) to express the shape of the earth such that > "height" from one table means even approximately the same thing as > "altitude" from another. However I think any discussion about the geoid implies an attempt to push UCDs well beyond what I believe to be their valuably constrained scope. Thus the description of pos.earth.height should carefully _not_ say which datum it is relative to, and draw attention to the fact that it is not saying this! This is because... > By attaching the same UCD to values from two different tables we > are asserting that for [all | most | many | some | any] purposes > that these values represent identical "things". It seems to me that the purpose in question is `find tables I might be interested in', and that the equivalence relation here is not one of identity. My perception is that the UCD word set has been successful, and should remain successful, to the extent that it abides by two principles: that the word list is small enough and mnemonic enough that folk are likely to remember a respectable proportion of the words, and that it service those use-cases where false positives are good. That set includes searching for tables, and excludes driving processing. It might be a bit late to edit things now, but I have said before that I feel the UCD document would benefit from a bolder statement of its scope, and of its non-goals. > The way to extend a robust UCD process into the future is to > provide an explicit namespace mechanism from the start. This will > allow capturing controversial or peripheral identifiers such as > VOConcept, but will also allow us to wipe the etch-a-sketch clean > with new version(s) of subject dependent list(s) of UCDs. If later > we decide that v1:pos.earth.height should indeed have been > v2:pos.earth.altitude, there needs to be a lightweight way to make > the transition. Hear, hear. One of the other GO maxims -- up there with `involve the users' -- was `version the ontology'. It seems the GO is in more-or- less continuous flux, but this simply doesn't matter, because they recognised at the outset that they were going to have to do this, and so designed their formalism and tools to cope/help with it. I hope this helps. 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-sci@eso.org Wed Jun 29 19:52:41 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 j5THqWmK018479 for ; Wed, 29 Jun 2005 19:52:32 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5THqWVY018478 for ucd-sci-outgoing; Wed, 29 Jun 2005 19:52:32 +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 j5THqRmK018471 for ; Wed, 29 Jun 2005 19:52:27 +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 j5THqOXW010596 for ; Wed, 29 Jun 2005 19:52:25 +0200 (CEST) X-Spam-Checker-Version: SpamAssassin 3.0.4 (2005-06-05) on noao.edu X-Spam-Level: X-Spam-Status: No, score=-2.5 required=4.5 tests=AWL,BAYES_00,HTML_40_50, HTML_MESSAGE autolearn=ham version=3.0.4 X-TFF-CGPSA-Version: 1.4f1 X-TFF-CGPSA-Filter: Scanned Received: from [216.111.165.59] (account seaman HELO [10.0.5.23]) by noao.edu (CommuniGate Pro SMTP 4.3.5) with ESMTPSA id 19002813; Wed, 29 Jun 2005 10:52:04 -0700 In-Reply-To: References: <20050624145346.xxa5qiwl0ri8wgsw@webmail.sic.rm.cnr.it> <20050628221311.GA12268@ucolick.org> <42C25875.80501@cea.fr> <1055be75840525c23e851cc2b61bfe2b@cacr.caltech.edu> <8DAB1A37-2372-40F0-B2D5-46DD5250C0A7@noao.edu> <0f37cba6a09192ef4c0f597ce6aa4349@cacr.caltech.edu> Mime-Version: 1.0 (Apple Message framework v730) Content-Type: multipart/alternative; boundary=Apple-Mail-10-26394698 Message-Id: <50C96AD6-350E-4D76-AEED-A3C088197FA0@noao.edu> Cc: Rob Seaman , ucd-sci@ivoa.net From: Rob Seaman Subject: Re: Draft list of ucd-words Date: Wed, 29 Jun 2005 10:51:55 -0700 To: Roy Williams 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: 2005.6.29.20 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 --Apple-Mail-10-26394698 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Roy says: > OK I am showing my ignorance of what magnitude exactly means. But > it sounds like you are taking a hard line that the concept of > "magnitude" is meaningless by itself, and has no place in the UCD > list. Surely it has some rigorous definition in terms of photons or > flux or energy or SOMETHING? And therefore a context in which they > can be compared. No, magnitudes are fine - precisely because they have a fuzzy definition. What I was apparently arguing only poorly was that more interesting things like photon counting are harder to represent using simple scalar quantities/names or lists (even hierarchical lists) of same. > And what is wrong with world coordinates? We have UCDs for CRVAL > and CRPIX and CTYPE and all those good WCS keywords. Are they also > so poorly defined as to be useless? They are well-defined in the > Calabretta papers, aren't they? I'm situated in a rather awkward location in the Moscone Center and the wifi keeps cutting out, so I won't try to reply in detail, but surely it would be better to provide a single identifier to a complete WCS data structure than to label each separate piece of same? But fundamentally I was just attempting so add a "me, too" to Steve's much more cogently worded reply. If he isn't panicking - neither am I. > The namespaces for UCD was my suggestion. I was voted down. Maybe it's time to have another vote. Rob --Apple-Mail-10-26394698 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1
Roy says:

OK I am showing my ignorance of = what magnitude exactly means. But it sounds like you are taking a hard = line that the concept of "magnitude" is meaningless by itself, and has = no place in the UCD list. Surely it has some rigorous definition in = terms of photons or flux or energy or SOMETHING? And therefore a context = in which they can be compared.

No, magnitudes are fine - = precisely because they have a fuzzy definition.=A0 What I was apparently = arguing only poorly was that more interesting things like photon = counting are harder to represent using simple scalar quantities/names or = lists (even hierarchical lists) of same.

And what is wrong with world = coordinates? We have UCDs for CRVAL and CRPIX and CTYPE and all those = good WCS keywords.=A0 Are = they also so poorly defined as to be useless? They are well-defined in = the Calabretta papers, aren't they?

I'm situated in a rather awkward = location in the Moscone Center and the wifi keeps cutting out, so I = won't try to reply in detail, but surely it would be better to provide a = single identifier to a complete WCS data structure than to label each = separate piece of same?=A0 But fundamentally I was just attempting so = add a "me, too" to Steve's much more cogently worded reply.=A0 If he = isn't panicking - neither am I.

The namespaces for UCD was my = suggestion. I was voted down.

Maybe it's time to have = another vote.

Rob
= --Apple-Mail-10-26394698-- From owner-ucd-sci@eso.org Thu Jun 30 08:10:57 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 j5U6ApGH010486 for ; Thu, 30 Jun 2005 08:10:51 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5U6ApT3010485 for ucd-sci-outgoing; Thu, 30 Jun 2005 08:10:51 +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 j5U6AlGH010464 for ; Thu, 30 Jun 2005 08:10:47 +0200 (MEST) Received: from ms0.astro.physik.uni-goettingen.de (ms0.astro.physik.uni-goettingen.de [134.76.204.32]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j5U6Aj73005570 for ; Thu, 30 Jun 2005 08:10:46 +0200 (CEST) Received: from sisley.astro.physik.uni-goettingen.de ([134.76.205.209]) by ms0.astro.physik.uni-goettingen.de with esmtp (Exim 4.44) id 1DnsFx-0003bW-MP for ucd-sci@ivoa.net; Thu, 30 Jun 2005 08:10:37 +0200 Mime-Version: 1.0 (Apple Message framework v622) In-Reply-To: <578357BE-8513-488B-BF49-EB57A6E8415C@astro.gla.ac.uk> References: <20050624145346.xxa5qiwl0ri8wgsw@webmail.sic.rm.cnr.it> <20050628221311.GA12268@ucolick.org> <42C25875.80501@cea.fr> <1055be75840525c23e851cc2b61bfe2b@cacr.caltech.edu> <8DAB1A37-2372-40F0-B2D5-46DD5250C0A7@noao.edu> <578357BE-8513-488B-BF49-EB57A6E8415C@astro.gla.ac.uk> Content-Type: text/plain; charset=ISO-8859-1; delsp=yes; format=flowed Message-Id: <8421f512d315809626d3b4cc3bc809a3@astro.physik.uni-goettingen.de> From: "Frederic V. Hessman" Subject: Re: Draft list of ucd-words Date: Thu, 30 Jun 2005 08:13:22 +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: 2005.6.29.44 X-Virus-Scanned: by amavisd-new Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id j5U6AoGH010481 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 >> The way to extend a robust UCD process into the future is to provide >> an explicit namespace mechanism from the start. This will allow >> capturing controversial or peripheral identifiers such as VOConcept, >> but will also allow us to wipe the etch-a-sketch clean with new >> version(s) of subject dependent list(s) of UCDs. If later we decide >> that v1:pos.earth.height should indeed have been >> v2:pos.earth.altitude, there needs to be a lightweight way to make >> the transition. > > Hear, hear. One of the other GO maxims -- up there with `involve the > users' -- was `version the ontology'. It seems the GO is in > more-or-less continuous flux, but this simply doesn't matter, because > they recognised at the outset that they were going to have to do this, > and so designed their formalism and tools to cope/help with it. (back on-line after a painful move of our entire institute) I confess that even I can see the advantages of this in principle - and I was the most vociferous complainer about opaque UCD's. However, I'm not crazy about numbering the concepts - yet another layer of naming, this time utterly random in appearance - and I'm not quite sure how versioning is going to function in practice. On the other hand, if GO works, then what can one say? Rick ------------------------------------------------------------------------ ------------------------ NEW ADDRESS!!! ------------------------------------------------------------------------ ------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Institut für Astrophysik Tel. +49-551-39-5052 Friedrich-Hund-Platz 1 Fax +49-551-39-5043 37077 Goettingen http://www.Astro.physik.Uni-Goettingen.de/~hessman ------------------------------------------------------------------------ ------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.Uni-Goettingen.de ------------------------------------------------------------------------ ------------------------- From owner-ucd-sci@eso.org Thu Jun 30 10:14:10 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 j5U8E3GH002817 for ; Thu, 30 Jun 2005 10:14:04 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j5U8E3lV002816 for ucd-sci-outgoing; Thu, 30 Jun 2005 10:14:03 +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 j5U8DwGH002804 for ; Thu, 30 Jun 2005 10:13:58 +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 j5U8DuXW004385 for ; Thu, 30 Jun 2005 10:13:56 +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 j5U8DoJd028602 for ; Thu, 30 Jun 2005 10:13:50 +0200 (MEST) Received: from pisaure.intra.cea.fr (unverified) by cincidele.saclay.cea.fr (Content Technologies SMTPRS 4.3.17) with ESMTP id ; Thu, 30 Jun 2005 10:13:50 +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 j5U8CrT5003007; Thu, 30 Jun 2005 10:12:53 +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 j5U8Dned021677; Thu, 30 Jun 2005 10:13:49 +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 j5U8Dmbh018165 ; Thu, 30 Jun 2005 10:13:49 +0200 (MEST) Message-ID: <42C3A9BC.3050009@cea.fr> Date: Thu, 30 Jun 2005 10:13:48 +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: norman@astro.gla.ac.uk CC: ucd-sci@ivoa.net Subject: Re: Draft list of ucd-words References: <20050624145346.xxa5qiwl0ri8wgsw@webmail.sic.rm.cnr.it> <20050628221311.GA12268@ucolick.org> <42C25875.80501@cea.fr> <1055be75840525c23e851cc2b61bfe2b@cacr.caltech.edu> <8DAB1A37-2372-40F0-B2D5-46DD5250C0A7@noao.edu> <578357BE-8513-488B-BF49-EB57A6E8415C@astro.gla.ac.uk> In-Reply-To: <578357BE-8513-488B-BF49-EB57A6E8415C@astro.gla.ac.uk> 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: 2005.6.30.0 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 Norman Gray wrote: > > Greetings, > > On 2005 Jun 29 , at 16.47, Rob Seaman wrote: > >>> If a table is published in ApJ that defines the "altitude" of their >>> observatory (pos.earth.altitude), it is not for us to say the writer >>> was a fool, it is for us to make sure there is a UCD for that concept. >> >> >> Right - and I agree with Steve that this should rather be called >> "height". > > > The Gene Ontology folk have described a few key ideas that helped them > create a big and very successful ontology. Though GO has problems -- > some quite fundamental -- non-ontologists do actually use it to do > actual science. Some of these `rules' are rather obvious, such as > `involve users', but Rob's message is a hook for a couple of the > non-obvious ones. > > GO uses opaque labels for every concept, so that pos.earth.altitude and > pos.earth.height would both be ucd12345 or something. They do this (i) > to avoid arguments about which noun it should be, (ii) so they can > version them easily (when are we going to have fight about replacing > pos.earth.height with pos.earth.height2? whereas no-one has a > sentimental attachment to ucd12345), (iii) so users aren't tempted to > use their intuition about what the labels mean, and are forced to use > the project's tools to discover and resolve labels, and (iiia) to make > it transparently clear to everyone that the label really doesn't matter > -- it's just a string which keys to a careful description elsewhere. > > I'm not suggesting replacing all the UCDs with numbers (don't worry), > but suggesting that it might be best to avoid `obvious' names, and even > that it might be a virtue than a vice to have names which are mnemonic > but still vague enough to force folk to look up careful definitions > _before_ they use them. > Agree ;-) "the Word is not the Thing it represents" (Science and Sanity: An Introduction to Non-Aristotelian Systems and General Semantics, 1933, Alfred KORZYBSKI) or "the word dog doesn't bite". The words didn't really matter if we agree about the descriptions/definitions. >> The way to extend a robust UCD process into the future is to provide >> an explicit namespace mechanism from the start. This will allow >> capturing controversial or peripheral identifiers such as VOConcept, >> but will also allow us to wipe the etch-a-sketch clean with new >> version(s) of subject dependent list(s) of UCDs. If later we decide >> that v1:pos.earth.height should indeed have been >> v2:pos.earth.altitude, there needs to be a lightweight way to make >> the transition. > > > Hear, hear. One of the other GO maxims -- up there with `involve the > users' -- was `version the ontology'. It seems the GO is in more-or- > less continuous flux, but this simply doesn't matter, because they > recognised at the outset that they were going to have to do this, and > so designed their formalism and tools to cope/help with it. Descriptions can change, as a lot of things... including our minds :-) > > I hope this helps. All the best, I allways appreciate your interventions. > > Norman > > -- Pierre ------------------------------------------------------------------ DIDELON :@: pdidelon_at_cea.fr Phone : 33 (0)1 69 08 58 89 CEA SACLAY - Service d'Astrophysique 91191 Gif-Sur-Yvette Cedex ------------------------------------------------------------------ La carte n'est pas le territoire - Alfred KORZYBSKI ------------------------------------------------------------------ From owner-ucd-sci@eso.org Mon Jul 11 17:01:39 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 j6BF1Q1b008581 for ; Mon, 11 Jul 2005 17:01:26 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j6BF1PEM008580 for ucd-sci-outgoing; Mon, 11 Jul 2005 17:01:25 +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 j6BF1H1b008550 for ; Mon, 11 Jul 2005 17:01:17 +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 j6BF1Bin008452 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-sci@eso.org Precedence: bulk Reply-To: ucd-sci@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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28.83 c 0 13.94 0.85 28.99 18.2 28.99 c 11.19 0 15.84 -2.96 22.04 -8.5 c 2.07 -1.89 2.41 -1.89 3.1 -1.89 c 1.72 0 2.07 1.55 2.24 2.24 c 0.34 1.38 2.07 11.02 2.07 11.88 c 0 1.55 -1.21 2.24 -4.13 3.62 c -8.26 3.79 -13.43 5.66 -25.48 5.66 c -25.65 0 -41.03 -12.1 -41.03 -42.33 c 0 -28.58 14.58 -41.49 40.17 -41.49 c 4.65 0 14.98 0.17 26.51 6.03 c 4.82 2.58 4.99 2.75 4.99 4.48 c h f* 2131 6452.73 m 0 28.23 -13.71 43.19 -41.66 43.19 c -28.75 0 -41.34 -15.38 -41.34 -43.19 c 0 -28.06 14.57 -40.63 41.17 -40.63 c 27.03 0 41.83 12.39 41.83 40.63 c h 2089.34 6425.11 m -18.59 0 -18.34 15.72 -18.34 29.69 c 0 13.26 -0.25 29.13 18.17 29.13 c 18.59 0 18.83 -15.44 18.83 -29.13 c 0 -13.6 0 -29.69 -18.66 -29.69 c h f* 2223 6469.95 m 0 17.73 -7.55 24.95 -25.06 24.95 c -18.08 0 -25.82 -13.2 -28.06 -17.89 c 0.09 0 0 8.61 p 0 5.51 -1.24 8.42 -8.52 8.42 c -5.85 0 p -6.2 0 -7.59 -1.93 -7.59 -8.42 c 0 -63.35 p 0 -6.2 1.74 -8.26 7.59 -8.26 c 6.89 0 p 6.54 0 8.52 2.24 8.52 8.26 c 0 38.05 p 0 14.98 9.85 22.59 18.68 22.59 c 8.26 0 10.32 -4.13 10.32 -13.29 c 0 -47.34 p 0 -5.51 1.16 -8.26 7.93 -8.26 c 6.89 0 p 6.54 0 8.19 2.24 8.19 8.26 c h f* 2270 6481 15.85 0 P 2.07 0 8.26 -0.55 8.26 5.65 c 0 6.2 -6.2 6.35 -8.26 6.35 c -15.85 0 0 14.13 p 0 5.51 -1.13 7.87 -7.73 7.87 c -5.34 0 p -6.2 0 -8.41 -1.8 -8.41 -7.87 c 0 -14.13 -3.81 0 p -1.89 0 -8.26 -0.16 -8.26 -6.35 c 0 -6.2 6.2 -5.65 8.26 -5.65 c 3.29 0 0 -44.1 p 0 -17.39 6.25 -24.79 18.23 -24.79 c 1.55 0 9.12 0 18.08 2.75 c 2.93 0.86 12.91 3.96 12.91 7.23 c 0 0.52 -0.34 1.72 -1.38 5.34 c -0.86 3.44 -1.21 4.48 -2.75 4.48 c -0.86 0 -1.03 -0.17 -2.07 -1.21 c -1.89 -1.38 -6.54 -5.59 -13.77 -5.59 c -4.13 0 -7.24 3.01 -7.24 14.72 c h f* 2336 6453.59 m 0 16.35 13.82 23.07 24.84 23.76 c 3.1 0.17 3.44 0.17 3.44 4.65 c 0 8.09 p 0 3.44 0 4.65 -3.1 4.65 c -4.82 0 -17.39 -1.72 -25.48 -20.31 c -0.57 0 0 11.19 p 0 5.51 -1.15 8.42 -7.87 8.42 c -5.51 0 p -6.2 0 -8.76 -1.93 -8.76 -8.42 c 0 -63.35 p 0 -6.2 2.01 -8.26 8.76 -8.26 c 6.37 0 p 6.54 0 7.87 2.24 7.87 8.26 c h 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1.13 -8.26 7.73 -8.26 c 6.37 0 p 6.54 0 8.39 2.24 8.39 8.26 c h 3452 6440.51 m 0 -16.01 -16.87 -16.4 -17.41 -16.4 c -7.23 0 -11.59 6.39 -11.59 13.13 c 0 16.87 24.14 18.08 29 18.25 c h f* 3513 6453.59 m 0 16.35 13.82 23.07 24.84 23.76 c 3.1 0.17 3.44 0.17 3.44 4.65 c 0 8.09 p 0 3.44 0 4.65 -3.1 4.65 c -4.82 0 -17.39 -1.72 -25.48 -20.31 c -0.57 0 0 11.19 p 0 5.51 -1.15 8.42 -7.87 8.42 c -5.51 0 p -6.2 0 -8.76 -1.93 -8.76 -8.42 c 0 -63.35 p 0 -6.2 2.01 -8.26 8.76 -8.26 c 6.37 0 p 6.54 0 7.87 2.24 7.87 8.26 c h f* 3624.57 6484.75 m 0.86 2.24 0.43 2.58 0.43 3.44 c 0 4.65 -4.36 4.8 -6.46 4.8 c -3.79 0 p -2.75 0 -6.54 -0.16 -9.12 -4.11 c -0.52 -0.86 -14.46 -38.91 -15.32 -50.44 c -0.17 0 p -0.86 8.44 -7.92 24.45 -15.32 40.97 c -4.82 10.85 -6.03 13.58 -14.63 13.58 c -4.48 0 p -2.41 0 -6.71 -0.16 -6.71 -4.63 c 0 -0.69 0.52 -1.89 0.86 -2.75 c 32.54 -71.61 p -1.38 -3.62 -1.89 -5.51 -2.41 -7.23 c -2.07 -5.68 -4.99 -12.66 -14.29 -12.66 c -5.68 0 -9.64 1.9 -11.53 2.85 c -0.86 0.52 -1.21 0.69 -1.72 0.69 c -0.86 0 -2.44 -0.52 -2.44 -2.58 c 0 -1.38 1.16 -13.26 1.75 -13.94 c 1.55 -2.07 10.85 -2.01 13.6 -2.01 c 21.35 0 29.78 19.98 31.16 24.05 c h f* 1009.5 6307.73 m 0.69 2.07 0.86 2.24 0.86 3.1 c 0 4.65 -4.3 4.18 -6.71 4.18 c -6.71 0 p -3.62 0 -8.61 0.47 -11.36 -7.1 c -23.24 -63.87 -8.95 -26.51 p -0.17 0.52 -2.07 6.54 -4.65 13.6 c -27.89 76.95 p -2.75 7.4 -7.57 6.93 -11.19 6.93 c -9.3 0 p -2.41 0 -6.71 0.47 -6.71 -4.18 c 0 -0.86 0.17 -1.03 0.86 -3.1 c 38.56 -104.49 p 2.58 -7.23 7.57 -7.23 11.02 -7.23 c 15.84 0 p 3.62 0 8.44 0 11.19 7.57 c h f* 1084.2 6233 m 3.96 0 7.8 0.17 7.8 7.76 c 0 22.21 -10.2 37.17 -35.52 37.17 c -27.54 0 -41.48 -15.55 -41.48 -41.82 c 0 -28.23 16.48 -42 43.72 -42 c 6.54 0 16.35 0.86 27.72 6.54 c 3.79 1.89 4.53 2.41 4.53 4.48 c 0 1.21 -0.17 6.2 -0.23 7.57 c -0.69 5.34 -0.86 5.51 -2.41 5.51 c -0.69 0 -1.03 0 -2.93 -1.72 c -10.16 -8.78 -20.49 -10.38 -25.99 -10.38 c -19.45 0 -21.52 15.64 -22.03 26.89 c h 1037 6242 m 0.53 10.49 4.07 23.93 19.48 23.93 c 13.77 0 16.35 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-2.41 -12.22 -2.41 -13.94 c 0 -3.1 12.74 -7.06 12.91 -7.23 c 9.47 -2.93 16.53 -2.93 19.45 -2.93 c 8.78 0 30.3 0.69 30.3 26.17 c h f* 1252.56 6315 m -5.51 0 -8.26 -0.95 -8.26 -7.27 c 0 -7.92 p 0 -5.51 1.72 -8.81 8.09 -8.81 c 8.95 0 p 8.26 0 8.26 3.94 8.26 12.77 c 0 8.26 0 11.23 -8.26 11.23 c h 1268 6266.58 m 0 5.51 -1.15 8.42 -7.87 8.42 c -6.37 0 p -6.2 0 -8.76 -1.93 -8.76 -8.42 c 0 -62.32 p 0 -6.2 2.01 -8.26 8.76 -8.26 c 6.37 0 p 6.54 0 7.87 2.24 7.87 8.26 c h f* 1368 6234.73 m 0 28.23 -13.71 43.19 -41.66 43.19 c -28.75 0 -41.34 -15.38 -41.34 -43.19 c 0 -28.06 14.57 -40.63 41.17 -40.63 c 27.03 0 41.83 12.39 41.83 40.63 c h 1326.34 6207.11 m -18.59 0 -18.34 15.72 -18.34 29.69 c 0 13.26 -0.25 29.13 18.17 29.13 c 18.59 0 18.83 -15.44 18.83 -29.13 c 0 -13.6 0 -29.69 -18.66 -29.69 c h f* 1460 6251.95 m 0 17.73 -7.55 24.95 -25.06 24.95 c -18.08 0 -25.82 -13.2 -28.06 -17.89 c 0.09 0 0 8.61 p 0 5.51 -1.24 8.42 -8.52 8.42 c -5.85 0 p -6.2 0 -7.59 -1.93 -7.59 -8.42 c 0 -63.35 p 0 -6.2 1.74 -8.26 7.59 -8.26 c 6.89 0 p 6.54 0 8.52 2.24 8.52 8.26 c 0 38.05 p 0 14.98 9.85 22.59 18.68 22.59 c 8.26 0 10.32 -4.13 10.32 -13.29 c 0 -47.34 p 0 -5.51 1.16 -8.26 7.93 -8.26 c 6.89 0 p 6.54 0 8.19 2.24 8.19 8.26 c h f* 1594 6311 m 0 3.27 0.11 7.79 -7.46 7.79 c -3.44 0 -4.13 -0.28 -6.2 -1.94 c -3.1 -2.75 -9.64 -9.12 -26.68 -9.47 c -3.1 0 -7.57 -1.21 -7.57 -6.2 c 0 -6.2 6.03 -6.2 8.26 -6.2 c 5.31 0 11.52 0.86 16.65 2.24 c 0 -89.22 -13.9 0 p -2.24 0 -8.26 0.39 -8.26 -5.8 c 0 -6.2 6.03 -6.2 8.26 -6.2 c 49.06 0 p 1.89 0 8.26 0 8.26 6.2 c 0 6.2 -6.37 5.8 -8.26 5.8 c -12.16 0 h f* 1666 6213.9 m 0 4.48 -0.19 5.1 -5.12 5.1 c -13.26 0 p -4.48 0 -4.62 -0.19 -4.62 -5.1 c 0 -13.26 p 0 -4.48 0.17 -4.65 4.63 -4.65 c 13.26 0 p 4.48 0 5.12 0.17 5.12 4.65 c h f* 1768 6255.05 m 0 23.58 0.11 63.74 -39.66 63.74 c -39.94 0 -39.34 -39.99 -39.34 -63.74 c 0 -23.58 -0.6 -62.83 39.17 -62.83 c 39.94 0 39.83 38.91 39.83 62.83 c h 1728.17 6204.21 m -12.74 0 -14.63 16.14 -15.15 20.88 c -1.21 9.12 -1.02 25.31 -1.02 32.36 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3670 0W , 3291 3670 1A , 3327 3670 0A , 3372 3640 1E , 1001 3530 80 82 /4U $C /d;VPf<"a#_Z[3\>@1T-rk3g5YPRq_&:[@=qYFQ+f@'Np^6ekroY:>XYNtG$IpYk7qYFQ+f@'Np ^6dIEp%i%!YL , 1089 3529 4M , 1147 3530 0A , 1193 3530 3S , 1290 3529 0E , 1349 3530 7L , 1453 3527 83 88 /1Y $C -(KjF&iKpP&6s0e:'cX&XTA\F_?`'(Jdngbgg^=q=J[eO:+52&eK-.loo0[f;APJ[S1-\ap,_Vi?[ O\j(ER(r~> , 1545 3530 0A , 1590 3529 0E , 1638 3506 65 76 /4Y $C 3XZ'2'B_Xc*F$F-\$l22mFpqd+5?Mfp[/!ln(2^>TL=:c-hmI5mZ[OOVZ06df@,5FronjGdXQAQ hs!A:?Z5S?otPWFG6fmRc[g%dr.]cU0b=~> , 1754 3500 3O , 1792 3530 7L , 1857 3529 4M , 1915 3530 0A , 1961 3530 3S , 2058 3529 0E , 2117 3530 7L , 2182 3529 0S , 2273 3529 0E , 2332 3529 3W , 2370 3529 3I , 2423 3530 0A , 2469 3529 4M , 2527 3530 0W , 2560 3506 1U , 2618 3530 27 83 /2C $C ,DK9l"GX%.s8W-!s8W-!s8W-!s8W-!s8W-!s8W-!s7NIR%"I>iJ,~> , 2651 3529 0E , 2709 3530 0W , 2742 3529 0E , 2801 3529 4A , 2853 3530 0W , 2885 3529 1Q , 2950 3530 57 83 /5C $C 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1001 3112 77 81 /2S $C .Dors!s0U]?XNj5s8W-!s8W-!s8W-!s8W+]ln>RB^]494s'K.5p](6)qs2#nmp&"plm7aA"$2$C 5Mu~> , 1085 3112 2K , 1151 3111 4M , 1209 3112 3S , 1307 3111 0E , 1365 3111 3W , 1450 3112 99 82 @C , /f@)?;hJ0JH15/d_;N.o`#%as8Q=%5M,nllh]N'rkJ@/5M,ims8(X;rkJ1,?e56Q p&Eq6rkJ1,?e56Qp&DMtrkI^4YQ"Ptp&DMtrkI^4YPl5fp&@bdrjV`RYPl5fp&@bbJ+rehYPl5f p&@b]riP%k(PaUPfT=Hqo\]~> 1558 3111 4A , 1649 3109 1Y , 1740 3112 2C , 1765 3088 4Y , 1835 3112 7L , 1900 3112 7L , 2012 3082 3O , 2049 3112 2S , 2134 3112 2K , 2199 3111 4M , 2258 3112 3S , 2355 3111 0E , 2414 3111 3W , 2460 3112 0W , 2492 3112 81 85 /2S $C ,D(N/)F)ju-j3>$$n,hj9jb8on*MY*g/n#SDsk3oh-GN;YQ#>eQB>P3d_E3_IqaB2d_GaWJ,;k< p6G[F/-"=)p[kZWY.r[ls0T!0'n<:_?g@XBJ,~> , 2580 3112 0W , 2612 3112 99 82 @C , /f@)?;hJ0JH15/d_;N.o`#%as8Q=%5M,nllh]N'rkJ@/5M,ims8(X;rkJ1,?e56Q p&Eq6rkJ1,?e56Qp&DMtrkI^4YQ"Ptp&DMtrkI^4YPl5fp&@bdrjV`RYPl5fp&@bbJ+rehYPl5f p&@b]riP%k(PaUPfT=Hqo\]~> 2720 3111 4A , 2772 3109 1Y , 2864 3112 2C , 2888 3088 4Y , 2958 3112 7L , 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1554 3590 5O , 1597 3591 4E , 1657 3590 5E , 1737 3590 4I , 1788 3590 1M , 1843 3591 5M , 1926 3590 5E , 2014 3590 1M , 2061 3590 5O , 2103 3590 2C , 2166 3591 5M , 2288 3591 5M , 2371 3590 5E , 2428 3590 1M , 2474 3591 1O , 2535 3590 4I , 2617 3590 1M , 2672 3591 5S , 2694 3590 6A , 2778 3590 1M , 2821 3569 6E , 2879 3590 4I , 2954 3590 5O , 2996 3591 4E , 3057 3590 5E , 3137 3590 4I , 3188 3590 1M , 3242 3591 5M , 3325 3590 5E , 3405 3590 5O , 3448 3591 4E , 3516 3591 1I , 3539 3591 1O , 3599 3569 3I , 3662 3570 5W , 3717 3590 5E , 3765 3590 2S , 3820 3590 5E , 3868 3591 1O , 3969 3591 1I , 3999 3591 2Y , 4056 3590 3A , 4116 3590 4I , 4160 3590 5E , 4216 3590 2I , 4308 3591 1I , 4331 3591 1O , 4431 3590 41 50 /2M $C .Din+#``?1#T.ZQKG/HsX6I2if;.<-:PQVas8W,us*TKD#X@'>p\3M2eZebbnq)[Iqu#sj@q 0Mh~> , 4471 3590 2C , 4534 3591 5M , 4614 3590 2W , 4682 3591 1I , 4705 3591 1O , 4773 3590 1M , 4820 3590 5O , 4870 3591 1I , 4893 3590 2C , 4947 3591 1O , 5039 3590 6A , 5126 3591 1I , 5148 3590 5O , 5191 3591 4E , 724 3454 2I , 785 3455 1I , 807 3455 73 77 /3M $C 4pB7:?iM:).DskSdpN.Ts8W-!s8W-!s8W-!s8W-!s8W-!s3H7'o;JH%^]4?6s8W-!s7a+t3\@9q mqM5brO^g4[b\1D6OY/V_be5V+PO^I`$d<)_LM~> , 871 3454 5E , 919 3455 4Y , 962 3454 5E , 1010 3455 1O , 1068 3454 5O , 1147 3454 2C , 1201 3454 5O , 1244 3455 4E , 1304 3454 5E , 1353 3455 4Y , 1440 3454 1M , 1486 3454 5O , 1529 3454 2C , 1591 3455 5M , 1674 3454 4I , 1725 3455 3E , 0 81 156 rG 896 3163 50 86 /0Q $C 4:SY^BUgPkUs8W-!s8W-!s8W-!s8W-!s8W-!s-jPGli4ZZi*pF0n9B2)hUF6P~> , 962 3163 19 16 /3Q $C 0FRp\s8D~> , 999 3163 0Q , 1196 3163 81 83 /0U $C 4<&6q.?fCWG^+SQhXUdOI&$iA2oG.BDng5"hu1=`s8N#ts7cQ.s8W-!s8W,brI=kDs'PWgrg-tt H , 1283 3162 58 58 /3U $C ,f,s6nkA=82^J?adR=_d"lf`Eq)n @9SC"(fF$K~> , 1344 3163 64 84 /0Y $C +bqPadm;GiJ,fQKs8W-!s8W-!s8W-!s8W-!s6%4n60mG.X-pUm*js)!)j Z1%SY;#E-e:gjb~> , 1422 3163 53 56 /3Y $C /f^o"9a=BWs8W-!s8W-!s8W-!s8W-!qu?-"m:7n4p)76Up-.)Wf5%d5esK:N"r%~> , 1481 3163 25 83 /1C $C -P&tEs8W-!s8W-!s8W-!s8W-!s8Tg,W;lZQ,U^9Ts*gZ?~> , 1512 3162 46 71 /4C $C ,68r!c>\?mkW4&`j;@lKe2?,Ns8W-!s8W-!s8W-!kCZMCh0o7&;Li-Ss8Vup6Vm~> , 1560 3163 1C , 1591 3162 63 58 /1G $C ._pln),NW9%YLYce(kS\GLqBiD/;&10M , 1664 3163 3Y , 1767 3162 1G , 1833 3163 47 84 /4G $C +busks8W-!s8W-!s8W-!s8W-!4rL^JGQ+dS8caGAs8W,ur"@`>3+5q`G7N+D$kr~> , 1917 3162 56 58 /1K $C 2$\dCO;8C93Y'Wf<:ofC%.g-Cl06aarVulkrOor=*Z05/L-\8G(iik , 1980 3162 4C , 2028 3162 1G , 2102 3163 89 56 /4K $C /f^o! , 2197 3162 48 58 /1O $C .D^kf$pkF1_K>&2j;12"#Jtgo'6Vo2=K8;t9K#Eq0e(!u&qu">8sZD-:fo1iTO`T\+L&9Hb(nSa FkBuRYe`GG]rMJW:r,\Q8,~> , K 716 2957 4U , 795 2956 5O , 837 2956 2C , 900 2957 5M , 983 2956 4I , 1062 2956 6A , 1138 2956 5E , 1186 2957 4Y , 1229 2956 5E , 1322 2956 2I , 1374 2956 5E , 1423 2957 61 77 /4O $C 4pB75J+=FsS3 , 1484 2957 62 48 /1O $C 4pDMuJ+K=RS3 , 1544 2956 5E , 1601 2956 2I , 1698 2957 2Y , 1723 2956 2C , 1786 2957 5S , 1816 2957 5S , 1838 2956 2C , 1890 2956 6A , 1976 2957 1I , 1999 2957 1O , 2059 2935 3I , 2150 2956 5O , 2193 2957 4E , 2253 2956 5E , 2302 2956 4I , 2345 2956 5E , 2430 2935 3I , 2484 2956 3A , 2553 2957 1I , 2583 2956 2I , 2636 2956 5E , 2692 2957 5S , 2723 2957 1I , 2745 2957 1O , 2805 2956 5E , 2854 2956 4I , 2905 2957 17 47 /3A $C 1iS)F[Jd:D(fC>5rb16q:Xf:-e27~> , 893 2822 0K , 948 2822 3E , 1025 2821 1M , 1072 2821 2W , 1133 2821 2W , 1193 2822 4Y , 1236 2821 5E , 1284 2821 2S , 1350 2822 1I , 1380 2821 1M , 1427 2821 5O , 1477 2822 1I , 1500 2821 2C , 1554 2822 1O , 1615 2821 4I , 1698 2821 1M , 1745 2822 4Y , 1788 2821 5E , 1869 2822 60 76 /7D $C 4pB8bJ+=FqA02X_?5KeNI<<'sl#a\gl$oP:[[-lgO[j,/4rWg3]D(^dpi!D6ID4TW_sR( , 1923 2821 5E , 1972 2801 2E , 2032 2821 5O , 2107 2821 5O , 2150 2821 2C , 2245 2821 1M , 2332 2822 5M , 2423 2822 1I , 2445 2822 1O , 2514 2822 1I , 2544 2822 5M , 2624 2821 62 49 /5Y $C ,f5uQJd3F/W'k`R6+nW;Ruj2M<1'l_EV5C-s53kVs8W-!s8W-!s8W-!s8W$uX$-q4!It.@TL'bH~> , 2693 2822 5M , 2783 2801 5W , 2847 2821 1M , 2894 2822 1O , 2962 2821 2I , 3047 2821 2C , 3102 2822 1O , 3171 2822 5S , 3193 2800 6E , 3291 2822 1I , 3321 2822 2Y , 3379 2821 5O , 3422 2822 4E , 3482 2821 5E , 3563 2822 4Y , 3606 2821 5E , 3655 2821 4I , 3698 2821 5Y , 3766 2822 5S , 3789 2821 5O , 3872 2822 1I , 3894 2821 4I , 3969 2822 1O , 4030 2821 2C , 4085 2821 5O , 4168 2821 1M , 4222 2822 5M , 4302 2821 2W , 4371 2822 1I , 4393 2800 3I , 4447 2821 5Y , 4508 2821 2C , 4563 2821 5Y , 4623 2821 4I , 4707 2795 7J , 204 51 0 rG 4745 2822 39 51 /1S $C 1CHsMs8W-!s8W-!s82hCqq`A[`t-#[6#leZJ)>\052h/)~> , 4786 2821 51 53 /4S $C 3X(0FS1Gf3Ve@q`:IC4RkTG1tFaEf^s)7W.gXpaZm"U"E0]b8OOC=SCJ[lL(J**AL%5%JHd_f=A rhri`-u'/=0VfO2~> , K 4847 2801 5W , 204 51 0 rG 4907 2821 55 77 /1W $C ,6Paa1CFMBkW9+8k^"Aj.0kMH?Fk:Zlh1;Xs8W-!rVsY2^YA-[$OeO)]-3J'XbDB8"r9H's8W-! [;#~> , 4968 2821 52 53 /4W $C +Ti?2'L;hS%YKH#=s--k5kGUN-d[1RT8bN&I_J*RmsiD<:]'ncQ2U`kQIabjf*2km=1&K>:gl]u , 5024 2821 50 53 /2A $C +Mi=u"lT[l3Xu^:WZXUk,>^uA;@f\o8:T0>s8W-!hs]H68(4oY$Z%F('=$Eg[1"Hl6%YA1hu~> , K 5114 2821 1M , 5160 2822 4Y , 5203 2821 5E , 724 2684 1U , 809 2686 76 75 /5A $C -D8k'%+"N!_#b&7csWtWCTjpIH="2T\mDu?]liRcldGIXV7PCJ/_35uf=%#`]5-.o[p?E.=)3Q& p:FW-pA5B0g[4_3ID4TW\(gC`Jmr:g_HJaJ`2~> , 894 2665 5W , 952 2685 2W , 1013 2685 5Y , 1074 2685 5O , 204 51 0 rG 1156 2685 41 65 /2E $C 22-]LMBI!NKA+qO$i`NfCIA.%s8W-!s8W-!s360r#@7:7e=7W\s8Vu]e,~> , K 1241 2686 1I , 1263 2685 4I , 1351 2685 1M , 1405 2686 5M , 1485 2685 2W , 1554 2686 1I , 1576 2664 3I , 1630 2685 5Y , 1691 2685 2C , 1746 2685 5Y , 1806 2685 4I , 1857 2686 3A , 1928 2685 6A , 2004 2685 5E , 2089 2685 5Y , 2149 2685 4I , 2192 2685 5E , 204 51 0 rG 2281 2685 2E , 2325 2686 22 76 /5E $C 1CHsMs8W-!s8W-!s8W-!s8W-!qbYdlq3ZJMs8W%u:]~> , 2353 2686 88 51 /2I $C 1C?GO+Tg+YVbK#Js8W-!s8W-!s8W-!s8W-!s8W-!s8Vu2s6fd`q$.q;]uXT*?&#f$L([nGZ*@T4 mal0U_@9ZX0WbE[$kr~> , 2448 2685 4W , K 2544 2685 1M , 2590 2686 1O , 2659 2685 53 77 /5G $C 22*jn#TSHYTb , 204 51 0 rG 2752 2685 2E , 2796 2685 4W , 2852 2686 2I , 2946 2665 57 72 /2K $C 1^d'Ns8W-!s8V9"n:C(]kWYRkHcTih_@NFEgs8Vfms8W-!s8QE?rkI]7G*WOh/*g=H3n%.> =@%WP@%[~> , 3011 2685 4W , 3067 2686 1S , 3107 2685 4S , 3164 2685 2E , 3208 2685 55 51 /5K $C 2$:Ys1^aVf6/$(GH6Bcs#!LC_s*t"Is8W-!s8W-!s8W-!s8W,QC=>u~> , 3270 2686 1S , 3310 2685 4W , K 3406 2686 1I , 3429 2686 1O , 3489 2685 4I , 3532 2685 5O , 3575 2685 50 50 /2G $C .`0"(KLPCo&2<&ch'VAF8\.]%Uu%]PkroQ*]mp(C2M\gSTARE^df$r2f6ur<=7)i$.qr+"6OY*2 Lf-oK~> , 3631 2685 1M , 3686 2685 5G , 3746 2659 7N , 3789 2686 3E , 893 2551 45 73 /5M $C /e+HMGJ3@b2So-2hVW7\gO",#hUjoomG#*fh7J$CDVjd8h7_]hrV-6K[M/+*s8T7%dcN:`d_E/k e^nM>Wsg:k"Ul4o@MCMha@+q~> , 948 2551 3E , 1024 2550 1M , 1070 2550 5O , 1113 2550 2C , 1175 2551 85 48 /2O $C -D4W5(d&!%r:"_\3DLXE9Iih%s8W-!s8W-!s8W-!s8W-!s8W-!s8W,nJ,fEGFb1jqoLA<:mB'Uh X(aJVRYDcY+59iElki"m(e]T4Lf;.p#T+r~> , 1258 2550 4I , 1337 2550 1M , 1384 2551 4Y , 1426 2550 2G , 1503 2551 1O , 1563 2550 2C , 1618 2550 5O , 1688 2551 4E , 1746 2529 6E , 1803 2530 61 69 /5C $C 4pF65_qMNus8W-!o0AfW4qTf-kTJbK0`")J;gl>cS*fP/s5/VQRQ#RhC~> , 1864 2551 4E , 1925 2550 2G , 1973 2551 1O , 2042 2550 1M , 2088 2550 5O , 2131 2550 2G , 2187 2550 5G , 2248 2551 3E , 2324 2551 1E , 2395 2551 4E , 2455 2550 2G , 2532 2550 4I , 2575 2550 2G , 2623 2530 5C , 2692 2550 1M , 2738 2551 4Y , 2789 2550 1M , 2835 2550 5O , 2886 2551 1I , 2908 2550 2C , 2963 2551 1O , 3059 2551 1I , 3081 2550 4I , 3160 2551 2O , 3251 2550 1M , 3298 2551 4Y , 3341 2551 7D , 3395 2550 2G , 3452 2550 5G , 3532 2550 2W , 3590 2529 6E , 3683 2550 1M , 3765 2550 2M , 3814 2550 1M , 3861 2530 5C , 3929 2551 1I , 3951 2550 5O , 4002 2550 1M , 4056 2551 5S , 4115 2551 5S , 4137 2550 2G , 4185 2550 5O , 4228 2550 5O , 4270 2550 2G , 4319 2551 4Y , 4389 2550 5O , 4432 2550 2C , 4514 2551 4E , 4575 2550 2G , 4631 2551 5S , 4654 2530 5C , 4742 2551 4Y , 4785 2550 2G , 4841 2550 1M , 4896 2550 5G , 4956 2550 1M , 5003 2550 2W , 5071 2551 1I , 5102 2551 5S , 5132 2551 1I , 5154 2550 5O , 5194 2529 6E , 724 2388 7J , 758 2394 5C , 822 2414 2C , 877 2414 4I , 928 2415 1I , 950 2414 5O , 1000 2415 1I , 1023 2414 2C , 1077 2415 1O , 1177 2414 1M , 1224 2415 1O , 1284 2393 3I , 1347 2415 5S , 1369 2414 2G , 1457 2430 75 25 /2Q $C /dI7#8,rQr%img3~> , 204 51 0 rG 1569 2394 2K , 1633 2414 57 53 /5Q $C +Mi=u"lOsKF<*>9T'1_1F:`@d8\I@Q2ui..J,fQKs8VOprn$nJgL""5Bindo$l9Xn)R,p6@%i9( "2F~> , 1693 2414 43 53 /2U $C 2$P=VDZh%&iAu+j]Ruu2%u#,l0"TcU<%1WH8AJ(`L0Q#48sO'>>+i*!6Xk , 1739 2415 75 76 /5U $C 4:m+"TYbleC[YJ7hR:24D1,dFiii$)C\o7>(>&;_YO>\&=8'A3m , 1819 2415 55 51 /2Y $C 1C?GPVO]RDs8W-!s8W-!s8W-!s8W)u^[Jm&a(r,ML:rYUhmM1M=puf5JV&C~> , 1881 2393 58 73 /5Y $C .DWU[%8]@-%YLZSSIf$n_@Jp;ds^ohs4ZtN_/+FQ[1>o0[=s4,)HFk4FfSlA"Qfet_?Z"'l-nH" ?hcpu:YXK.rVuotrI9 , K 1944 2388 7N , 2010 2414 62 49 /3A $C ,f5uQJd3F/W'k`R6+nW;Ruj2M<1'l_EV5C-s53kVs8W-!s8W-!s8W-!s8W$uX$-q4!It.@TL'bH~> , 2071 2415 1O , 2139 2415 5S , 2162 2414 2G , 2210 2414 4I , 2253 2414 4I , 2327 2414 5O , 2370 2415 4E , 2430 2414 2G , 2518 2414 2M , 2559 2414 2C , 2621 2415 2O , 2704 2394 5C , 2768 2414 2C , 2822 2414 4I , 2865 2414 2G , 2922 2414 5G , 3005 2414 6A , 3081 2414 2C , 3136 2415 4Y , 3187 2414 5G , 3270 2415 4E , 3339 2414 1M , 3386 2414 4I , 3468 2414 1M , 3545 2414 6A , 3621 2414 2G , 3678 2415 5S , 3708 2415 5S , 3761 2415 7D , 3819 2415 1O , 3880 2414 2C , 3931 2414 6A , 4010 2415 1O , 4110 2414 1M , 4164 2414 2M , 4205 2415 4Y , 4248 2414 2C , 4302 2415 1O , 4360 2393 6E , 4425 2415 2O , 4547 2388 7J , 4582 2414 4I , 4633 2415 1I , 4655 2393 3I , 4710 2415 1O , 4778 2414 1M , 4833 2415 5S , 4886 2414 5O , 4929 2414 2C , 5014 2415 1O , 5075 2414 2C , 5138 2415 1I , 5160 2414 4I , 5203 2414 2G , 716 2280 4Y , 767 2279 1M , 813 2279 5O , 864 2280 1I , 886 2279 2C , 985 2295 2Q , 204 51 0 rG 1102 2279 2U , 1148 2280 2Y , 1209 2280 1S , K 1254 2253 7N , 1325 2279 2C , 1379 2280 4Y , 1458 2279 4I , 1501 2280 4E , 1562 2279 2C , 1617 2280 4Y , 1659 2279 5O , 1746 2280 35 77 /5W $C -D?_&n9\3Ns8W-!s8W-!s8W-!s7nM\cfS^:s8W-!s50%Ve%1"cmCR4>C)^@gT[W~> , 1771 2279 2C , 1826 2280 4Y , 1877 2280 2O , 2004 2253 7J , 2038 2279 4I , 2081 2279 5O , 2132 2279 1M , 2178 2280 1O , 2247 2279 5G , 2308 2279 1M , 2354 2280 4Y , 2405 2279 5G , 2502 2279 5G , 2554 2279 2G , 2603 2279 2S , 2669 2280 1I , 2699 2279 1M , 2745 2279 5O , 2796 2280 1I , 2818 2279 2C , 2873 2280 1O , 2978 2295 2Q , 204 51 0 rG 3095 2279 2U , 3141 2279 2E , 3185 2279 1W , 3246 2279 4W , 3302 2280 52 50 /3C $C +p/CI4kK,:Fo.mC5Pi+eomQ/kqq'HSYHPEB?Z*Tlh0j^_qYPF.p?V`QrAt=a~> , K 3360 2253 7N , 0 81 156 rG 896 1988 0Q , 962 1988 3Q , 991 1988 60 86 /6C $C -O*1bs8R8D.j;l9[r1$6HadnK]6#doGh9[/QBiXgGMP _b12M$eVL`[;+6j@9SBm$n26+~> , 1196 1988 0U , 1283 1987 3U , 1344 1988 0Y , 1422 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5X , 1117 2262 2T , K 1204 2236 1J , 1238 2242 2V , 1302 2262 7C , 1356 2262 6I , 1407 2263 6G , 1430 2262 1T , 1480 2263 6G , 1502 2262 7C , 1557 2263 6M , 1625 2262 2R , 1680 2263 6A , 1747 2262 7G , 1807 2262 2R , 1854 2262 1T , 1904 2262 2R , 1959 2236 4J , 989 2128 1H , 1079 2128 6A , 1109 2128 6A , 1165 2107 2X , 1215 2127 7K , 1283 2127 2R , 1330 2128 6M , 1387 2127 1T , 1438 2128 6G , 1460 2127 1T , 1511 2128 6G , 1533 2127 1L , 1581 2127 6I , 1650 2128 2N , 1693 2127 1L , 1750 2128 6A , 1780 2127 2R , 1826 2127 1T , 1869 2127 1L , 1925 2127 7G , 2004 2127 1T , 2046 2127 7C , 2127 2127 1T , 2169 2128 3H , 2230 2127 1L , 2304 2107 2V , 2368 2127 7C , 2423 2127 6I , 2474 2128 6G , 2496 2127 1T , 2546 2128 6G , 2569 2127 7C , 2623 2128 6M , 2710 2127 7C , 2772 2128 3P , 2832 2127 2R , 2878 2128 6M , 2965 2127 7C , 3019 2127 0L , 3086 2106 27 95 /1T $C 4sV7iM=[Bm%YMI.473(*HX , 3119 2127 1L , 3176 2127 0D , 3216 2127 40 68 /1T $C .KkDE,!L+ , 3267 2107 0T , 3325 2128 6G , 3347 2128 6M , 3434 2106 6O , 3489 2127 1L , 3537 2128 6M , 3598 2127 1L , 3646 2128 2N , 3697 2127 2R , 3751 2128 6A , 3800 2127 7C , 3854 2128 6M , 3941 2127 1T , 3983 2128 3H , 4044 2127 1L , 4118 2127 6I , 4161 2128 3V , 4219 2106 3L , 4275 2128 3D , 4343 2128 1H , 4425 2128 6M , 4485 2106 6O , 4540 2127 7K , 4608 2128 6A , 4639 2127 2R , 4685 2128 2N , 4762 2107 2X , 4811 2127 7K , 4880 2127 2R , 4927 2128 6M , 4984 2127 1T , 5035 2128 6G , 5057 2127 1T , 5107 2128 6G , 5130 2127 1L , 5178 2127 6I , 5229 2107 0T , 989 1991 2J , 1075 1992 6G , 1098 1991 1T , 1140 1992 3H , 1251 1991 1T , 1293 1992 3H , 1354 1991 1L , 1453 1991 1L , 1501 1992 6E , 1567 1991 0D , 1607 1991 1L , 1656 1971 2V , 1716 1991 1T , 1767 1992 6G , 1789 1991 7C , 1843 1992 6M , 1954 1991 7C , 2017 1992 3P , 2092 1971 2V , 2153 1992 2N , 2195 1991 7C , 2256 1970 27 95 /1T $C 4sV7iM=[Bm%YMI.473(*HX , 2289 1991 1L , 2346 1991 0D , 2386 1991 40 68 /1T $C .KkDE,!L+ , 2437 1992 6G , 2459 1991 7C , 2514 1992 6M , 2574 1991 6I 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/7F $C ,R8o+6,Fj+F9jguh'VW.dr0HbmJjY2^"?'"pAY*cjZ'p:(uZ)(kTJah#43c0Y=\D*9D13W=7tn: fD`Pbs8Vb7s/l%o?eXA? , 912 1586 3D , 204 51 0 rG 993 1585 2T , 1039 1565 6F , 1103 1585 1X , 1159 1585 50 53 /4J $C +Mi=u"lT[l3Xu^:WZXUk,>^uA;@f\o8:T0>s8W-!hs]H68(4oY$Z%F('=$Eg[1"Hl6%YA1hu~> , 1212 1585 1F , K 1297 1559 1J , 1331 1585 6I , 1374 1565 2V , 1438 1585 1L , 1494 1585 0D , 1535 1585 1T , 1577 1586 2N , 1628 1585 2R , 1683 1586 6A , 1749 1585 7G , 1810 1585 2R , 1856 1585 1T , 1907 1585 2R , 1961 1559 27 109 /4J $C 0B(ZpDV_pJpNq8$mJD@i\+b=Jn,)SRDu]jHs8W-!s&K+!Y@$tgp$8ee='h5iWp6t!9"LikPq#b;TE~> , 997 1450 4F , 1051 1449 7C , 1105 1450 2N , 1184 1450 3H , 1252 1450 6G , 1275 1449 6I , 1318 1449 1T , 1360 1449 7C , 1415 1450 2N , 1465 1450 6G , 1496 1449 0D , 1544 1449 2R , 1599 1450 6A , 1656 1450 2N , 1699 1449 1L , 1756 1449 2R , 1802 1449 6I , 1845 1449 7C , 1900 1450 6M , 1960 1449 6I , 2011 1429 0T , 2069 1429 2V , 2130 1450 3H , 2191 1449 7C , 2245 1449 1T , 2288 1449 7C , 2350 1450 2Z , 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2@]]%~> , 2343 6005 4I , 2404 6006 4Q , 2428 6005 4A , 2475 6005 6W , 2508 6006 0F , 2976 5991 6O , 3023 6006 0F , 3067 5990 4Y , 3112 6005 4M , 3153 6006 4U , 3169 6005 3W , 3211 6006 7M , 3258 5990 0B , 3309 6004 37 58 /0R $C -E,Eu-jSBIpd@l(7"Z!]6+o41qRo,,5P9O+?G7piX , 3348 6006 4Q , 3371 6006 37 34 /5K $C 3"8(F94#Nj%r\oNp@dme^&-Ogh7_\#rnhYOIbriHmecCa)gK!~> , 3409 6005 3O , 3455 5991 0J , 3470 6006 4Q , 3494 6006 7M , 3541 6005 4M , 3574 6005 6W , 3607 6006 3S , 3648 6006 4U , 3664 6005 5C , 3713 6005 3O , 3751 6005 3W , 3793 6006 0N , 1921 5912 0N , 1992 5911 3O , 2030 5911 6W , 2062 5911 3W , 2113 5912 4U , 2128 5911 6W , 2161 5911 3W , 2204 5911 5C , 2251 5912 24 55 /0V $C 49Tpp[_MkBs8W-!s8W-!s8W-!s8UYp5PK[~> , 2274 5911 3O , 2320 5912 4U , 2335 5911 3W , 2378 5912 46 34 /5O $C 2AdhGs31]UM1Oq5Y*HArf$_-1f%O0Q[oP"cQ$5WedVb?#kr5L(2bNBG(?Yc**md-e~> , 2422 5912 4Q , 2446 5911 4M , 2976 5897 6O , 3023 5912 0F , 3067 5896 4Y , 3112 5911 4M , 3154 5912 4U , 3169 5911 4M , 3202 5912 4Q , 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5438 7I , 2058 5438 6W , 2099 5439 4U , 2114 5438 6S , 2152 5438 7I , 2194 5439 0V , 2218 5438 7I , 2260 5439 3S , 2301 5439 4U , 2325 5437 0R , 2364 5439 61 53 /1H $C ,6=S80GYL4s8W-!s8W-!s8W+jY[@G1p]%A]s8M]k]m$Ug0O.+m~> , 2425 5437 65 56 /6A $C ,c<,#B>Hi$=+(2jkr1X/YA%pYrEoR8YQ+Y&rI=c!oX\9R_H;Ec*h`9^pgNmnID:3Fqu?]rqYs4e /qW%3JdQlA/fHGP+Oj'~> , 2976 5424 6O , 3023 5439 0F , 3070 5438 7I , 3112 5438 6W , 3153 5439 4U , 3169 5438 6S , 3206 5438 7I , 3249 5439 0V , 3272 5438 7I , 3314 5439 3S , 1921 5329 6O , 1968 5344 0F , 2015 5343 7I , 2058 5343 6W , 2099 5344 4U , 2114 5343 6S , 2152 5343 7I , 2194 5344 0V , 2218 5343 7I , 2260 5344 3S , 2301 5344 4U , 2325 5342 0R , 2364 5344 1H , 2425 5342 6A , 2495 5344 4U , 2511 5343 6S , 2556 5344 31 53 /1L $C 0H$HQ#n/Kes8W-!s8W-!s8W-!s7q<<,Os"[_;XAA~> , 2976 5329 6O , 3023 5344 0F , 3070 5343 7I , 3112 5343 6W , 3153 5344 4U , 3169 5343 6S , 3206 5343 7I , 3249 5344 0V , 3272 5343 7I , 3314 5344 3S , 1921 5234 6O , 1968 5249 0F , 2015 5248 7I , 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4rUs9e&.^[,6HX>mIpF*qg\#5s8V>5f3XfH''LqR/4.EheK_#M7LVHtID4TWrP/(+s8W$NoXa\+ < , 2405 5060 3S , 2438 5059 7I , 2480 5059 3W , 2523 5059 4A , 2976 5059 4M , 3009 5045 6O , 3058 5059 3O , 3096 5059 6S , 3134 5059 6W , 3175 5060 4U , 3190 5060 0V , 3214 5060 4Q , 3237 5060 7M , 3284 5059 3O , 3330 5060 4U , 3345 5059 5C , 3392 5060 3S , 3425 5059 7I , 3468 5059 3W , 3510 5059 4A , 1921 4950 6O , 1968 4965 0F , 2013 4949 4Y , 2058 4964 4M , 2099 4965 4U , 2115 4964 4A , 2162 4965 4Q , 2185 4964 4M , 2219 4964 6W , 2252 4964 3W , 2294 4965 7M , 2341 4964 6S , 2379 4964 3O , 2424 4965 4U , 2440 4964 6S , 2477 4964 7I , 2520 4965 0N , 2590 4950 6O , 2640 4964 7I , 2682 4965 7M , 2976 4950 6O , 3025 4964 7I , 3067 4964 4M , 3109 4965 4U , 3124 4964 4A , 3171 4965 4Q , 3195 4964 4M , 3228 4964 6W , 3261 4964 3W , 3304 4965 7M , 3351 4964 6S , 3388 4964 3O , 3434 4950 0J , 3449 4950 6O , 3499 4964 7I , 3541 4964 4M , 3583 4965 4U , 3598 4964 6S , 3636 4964 3W , 3678 4965 3S , 3711 4964 6W , 3744 4964 3O , 3782 4964 4M , 3815 4965 4Q , 3839 4964 3W , 3881 4965 7M , 3936 4965 4U , 3951 4965 5O , 4034 4945 21 80 /1Q $C $DAqKWD`Af;Y7XPldo/5YPPI& , 4057 4964 7I , 4100 4965 3S , 4161 4949 4Y , 4206 4950 12 24 /6J $X )upHK#64u/"+UEf!5JTm!8mib!,qpW!&+C,!&+qf+7LBA5O^o,5N!XA+2AD;~> , 4250 4965 5K , 4295 4945 21 80 /1V $C ,Q"rfh7J$CDYpp1qgWhe^A\'2p\Y!js7F)+ , 1921 4856 6O , 1968 4871 0F , 2013 4855 4Y , 2058 4870 4M , 2099 4871 4U , 2115 4870 4A , 2162 4871 4Q , 2185 4870 4M , 2219 4870 6W , 2252 4870 3W , 2294 4871 7M , 2341 4870 6S , 2379 4870 3O , 2424 4871 4U , 2440 4855 0B , 2482 4870 6S , 2976 4856 6O , 3025 4870 7I , 3067 4870 4M , 3109 4871 4U , 3124 4870 4A , 3171 4871 4Q , 3195 4870 4M , 3228 4870 6W , 3261 4870 3W , 3304 4871 7M , 3351 4870 6S , 3388 4870 3O , 3434 4856 0J , 3449 4856 6O , 3499 4870 7I , 3541 4870 4M , 3583 4871 4U , 3598 4855 0B , 3640 4870 3W , 3683 4871 0V , 3706 4870 3W , 3749 4870 6S , 3786 4870 6W , 3819 4870 7I , 3864 4870 6S , 3902 4870 3O , 3939 4871 7M , 3984 4870 6W , 4017 4871 3S , 4050 4871 4Q , 4073 4870 6S , 1921 4761 6O , 1968 4776 0F , 2013 4760 4Y , 2058 4775 4M , 2099 4776 4U , 2115 4775 3O , 2152 4776 0V , 2176 4775 3O , 2213 4775 6S , 2251 4775 6W , 2284 4776 3S , 2317 4775 7I , 2359 4776 7M , 2414 4776 4U , 2430 4775 3O , 2468 4776 7M , 2515 4775 3O , 2552 4776 3S , 2585 4760 0B , 2628 4760 4Y , 2976 4761 6O , 3023 4776 0F , 3067 4760 4Y , 3112 4775 4M , 3153 4776 4U , 3169 4775 3O , 3207 4776 7M , 3254 4775 3O , 3291 4776 3S , 3324 4760 0B , 3367 4760 4Y , 3419 4761 0J , 3435 4761 6O , 3482 4776 0F , 3527 4760 4Y , 3571 4775 4M , 3613 4776 4U , 3628 4775 3O , 3666 4776 0V , 3689 4775 3O , 3727 4775 6S , 3765 4775 6W , 3798 4776 3S , 3831 4775 7I , 3873 4776 7M , 1921 4666 6O , 1968 4681 0F , 2013 4665 4Y , 2058 4680 4M , 2099 4681 4U , 2115 4680 3O , 2152 4681 5O , 2197 4680 6W , 2230 4680 3O , 2268 4681 7M , 2315 4680 4M , 2348 4681 4Q , 2372 4680 7I , 2414 4681 7M , 2976 4666 6O , 3023 4681 0F , 3067 4665 4Y , 3112 4680 4M , 3154 4681 4U , 3169 4680 3W , 3211 4681 7M , 3258 4665 0B , 3309 4679 0R , 3348 4681 4Q , 3371 4681 5K , 3409 4680 3O , 3475 4680 7I , 3517 4681 3S , 3578 4666 6O , 3625 4681 0F , 3670 4665 4Y , 3715 4680 4M , 3756 4681 4U , 3772 4680 4M , 3805 4681 4Q , 3829 4681 5K , 3866 4680 3O , 1921 4572 6O , 1968 4587 0F , 2013 4571 4Y , 2058 4586 4M , 2099 4587 4U , 2115 4587 0N , 2185 4586 3W , 2228 4586 4M , 2261 4586 4M , 2302 4587 4U , 2318 4587 33 56 /6O $C 4;pGK$Z#eBs8W-!s8W,pi,AOT?iU0+s)UQ]Dr0@*:r@Ne'GsX~> , 2344 4587 3S , 2377 4586 3W , 2419 4586 6S , 2457 4586 6W , 2490 4587 4Q , 2513 4586 7I , 2556 4587 7M , 2976 4572 47 50 /6O $C 49U-Z(]XO8r:mo95)\@o5mHicLSjrpI5gW0^]1eCs8W%?s/s)E]1ZjT-mBel_GF(I0%:jX-i~> , 3023 4587 0F , 3067 4571 4Y , 3112 4586 4M , 3154 4587 4U , 3169 4587 0N , 3240 4586 3W , 3282 4586 4M , 3315 4586 4M , 3357 4572 0J , 3372 4586 3W , 3415 4587 3S , 3448 4587 4Q , 3471 4586 6W , 3504 4587 0F , 3559 4587 4U , 3575 4587 3S , 3608 4586 3W , 3650 4586 6W , 3683 4587 4Q , 3706 4586 7I , 1921 4477 6O , 1968 4492 0F , 2013 4476 4Y , 2058 4491 4M , 2099 4492 4U , 2115 4477 6O , 2164 4491 7I , 2206 4492 0V , 2230 4491 3W , 2272 4492 3S , 2305 4492 4Q , 2329 4492 5K , 2366 4491 3W , 2409 4491 6W , 2442 4492 4Q , 2465 4491 7I , 2508 4492 7M , 2563 4492 4U , 2578 4477 6O , 2628 4491 7I , 2670 4491 4M , 2703 4492 63 57 /6Q $C 4:DgQZi$=:8.lb6?aWs@f3 , 2767 4492 7M , 2814 4476 0B , 2976 4477 6O , 3025 4491 7I , 3067 4491 4M , 3109 4492 4U , 3124 4477 6O , 3174 4491 7I , 3216 4491 4M , 3249 4492 6Q , 3313 4492 7M , 3360 4476 0B , 3410 4477 0J , 3426 4477 6O , 3473 4492 0F , 3518 4476 4Y , 3562 4491 4M , 3604 4492 4U , 3619 4477 6O , 3669 4491 7I , 3711 4492 0V , 3734 4491 3W , 3777 4492 3S , 3810 4492 4Q , 3833 4492 5K , 3871 4491 3W , 3913 4491 6W , 3946 4492 4Q , 3970 4491 7I , 4012 4492 7M , 1921 4382 6O , 1971 4396 7I , 2013 4396 4M , 2054 4397 4U , 2070 4396 3W , 2112 4397 7M , 2159 4381 0B , 1921 4288 6O , 1971 4302 7I , 2013 4302 4M , 2054 4303 4U , 2070 4302 4A , 2117 4302 3O , 2155 4302 6W , 2976 4288 6O , 3025 4302 7I , 3067 4302 4M , 3109 4303 4U , 3124 4302 6S , 3162 4302 3W , 3204 4303 3S , 3237 4302 6W , 3270 4302 3O , 3308 4302 4M , 3341 4303 4Q , 3365 4302 3W , 3407 4303 7M , 3462 4288 0J , 3478 4303 4Q , 3501 4303 7M , 3548 4302 4M , 3582 4302 6W , 3615 4303 3S , 3656 4303 4U , 3671 4302 4A , 3718 4302 3O , 3756 4302 6W , 1921 4193 6O , 1971 4207 7I , 2013 4207 4M , 2054 4208 4U , 2070 4207 3O , 2108 4193 47 50 /2B $C +@&GZ6N@)cr^79K#Jqe'n:D,AK7,(-:KQ.Lf3eC?s8W-!qtpDCCN&NW[Z((l-.lWY(oN+u0M_~> , 2160 4208 4U , 2176 4207 4A , 2223 4207 3O , 2261 4207 6S , 2306 4208 4U , 2322 4207 3W , 2364 4208 3S , 2397 4207 6S , 2435 4207 4M , 2468 4207 3O , 2506 4207 6S , 1921 4099 6O , 1971 4113 7I , 2013 4113 4M , 2054 4114 4U , 2070 4113 3O , 2108 4099 2B , 2160 4114 4U , 2176 4114 3S , 2209 4113 3W , 2259 4114 4U , 2275 4114 0N , 2345 4114 4Q , 2369 4114 7M , 2413 4113 0Z , 2461 4113 6W , 2493 4113 3O , 2531 4113 4M , 1921 4004 6O , 1971 4018 7I , 2013 4018 4M , 2054 4019 4U , 2070 4018 3O , 2108 4004 2B , 2160 4019 4U , 2176 4019 3S , 2209 4018 3W , 2259 4019 4U , 2275 4018 4M , 2308 4018 3O , 2346 4018 6S , 2383 4018 7I , 2426 4019 7M , 2473 4018 4A , 2520 4018 4M , 1921 3909 6O , 1971 3923 7I , 2013 3923 4M , 2054 3924 4U , 2070 3908 0B , 2112 3923 3W , 2155 3924 0V , 2186 3924 4U , 2202 3923 6S , 2239 3923 7I , 2282 3924 0N , 2352 3909 6O , 2402 3923 7I , 2444 3924 7M , 2976 3909 6O , 3025 3923 7I , 3067 3923 4M , 3109 3924 4U , 3124 3923 6S , 3162 3923 3W , 3204 3924 3S , 3237 3923 6W , 3270 3923 3O , 3308 3923 4M , 3341 3924 4Q , 3365 3923 3W , 3407 3924 7M , 3462 3909 0J , 3478 3909 6O , 3527 3923 7I , 3569 3923 4M , 3611 3924 4U , 3626 3908 0B , 3669 3923 3W , 3711 3924 0V , 3735 3923 3W , 3777 3923 6S , 3815 3923 6W , 3847 3924 4Q , 3871 3923 6S , 1921 3815 6O , 1971 3829 7I , 2013 3829 4M , 2054 3830 4U , 2070 3815 6O , 2117 3830 0N , 2196 3830 4U , 2211 3829 4A , 2258 3829 3O , 2296 3829 6S , 2976 3815 6O , 3025 3829 7I , 3067 3829 4M , 3109 3830 4U , 3124 3815 6O , 3171 3830 0N , 3250 3815 0J , 3265 3815 6O , 3315 3829 7I , 3357 3829 4M , 3399 3830 4U , 3414 3829 3O , 3452 3815 2B , 3504 3830 4U , 3520 3829 4A , 3567 3829 3O , 3605 3829 6S , 1921 3720 6O , 1971 3734 7I , 2013 3734 4M , 2054 3735 4U , 2070 3720 6O , 2117 3735 0N , 2196 3735 4U , 2211 3735 3S , 2244 3734 3W , 2976 3720 6O , 3025 3734 7I , 3067 3734 4M , 3109 3735 4U , 3124 3720 6O , 3171 3735 0N , 3250 3720 0J , 3265 3720 6O , 3315 3734 7I , 3357 3734 4M , 3399 3735 4U , 3414 3734 3O , 3452 3720 2B , 3504 3735 4U , 3520 3735 3S , 3553 3734 3W , 1921 3625 6O , 1971 3639 7I , 2013 3639 4M , 2054 3640 4U , 2070 3625 6O , 2117 3640 3S , 2150 3639 3O , 2188 3639 6S , 2225 3639 3O , 2263 3639 4M , 2296 3639 4M , 2338 3640 4U , 2353 3639 4A , 2400 3639 3O , 2438 3639 6S , 2976 3625 6O , 3025 3639 7I , 3067 3639 4M , 3109 3640 4U , 3124 3625 6O , 3171 3640 3S , 3204 3639 3O , 3242 3639 6S , 3280 3639 3O , 3317 3639 4M , 3351 3639 4M , 3392 3625 0J , 3408 3625 6O , 3457 3639 7I , 3499 3639 4M , 3541 3640 4U , 3556 3639 3O , 3594 3625 2B , 3647 3640 4U , 3662 3639 4A , 3709 3639 3O , 3747 3639 6S , 1921 3531 6O , 1971 3545 7I , 2013 3545 4M , 2054 3546 4U , 2070 3531 6O , 2117 3546 3S , 2150 3545 3O , 2188 3545 6S , 2225 3545 3O , 2263 3545 4M , 2296 3545 4M , 2338 3546 4U , 2353 3546 3S , 2386 3545 3W , 2976 3531 6O , 3025 3545 7I , 3067 3545 4M , 3109 3546 4U , 3124 3531 6O , 3171 3546 3S , 3204 3545 3O , 3242 3545 6S , 3280 3545 3O , 3317 3545 4M , 3351 3545 4M , 3392 3531 0J , 3408 3531 6O , 3457 3545 7I , 3499 3545 4M , 3541 3546 4U , 3556 3545 3O , 3594 3531 2B , 3647 3546 4U , 3662 3546 3S , 3695 3545 3W , 1921 3436 6O , 1971 3450 7I , 2013 3450 4M , 2054 3451 4U , 2070 3436 6O , 2117 3451 3S , 2150 3450 7I , 2197 3435 21 70 /6V $C 3%Q39]FLXHGMh;)?)o(Is8W-!s8W,l1_8O*\8VC.*BgU6iIq~> , 1921 3341 6O , 1971 3355 7I , 2013 3355 4M , 2054 3356 4U , 2070 3355 4M , 2103 3340 0B , 2154 3356 4U , 2169 3355 6S , 2207 3355 7I , 2249 3356 0N , 2320 3341 6O , 2369 3355 7I , 2412 3356 7M , 2976 3341 6O , 3025 3355 7I , 3067 3355 4M , 3109 3356 4U , 3124 3355 6S , 3162 3355 3W , 3204 3356 3S , 3237 3355 6W , 3270 3355 3O , 3308 3355 4M , 3341 3356 4Q , 3365 3355 3W , 3407 3356 7M , 3462 3341 0J , 3478 3341 6O , 3527 3355 7I , 3569 3355 4M , 3611 3356 4U , 3626 3355 4M , 3660 3355 0Z , 3707 3341 6O , 3756 3355 3O , 3794 3356 3S , 3827 3340 0B , 3869 3355 3W , 3912 3356 0V , 3935 3355 3W , 3977 3355 6S , 4015 3355 6W , 4048 3356 4Q , 4072 3355 6S , 1921 3261 4M , 1955 3262 3S , 1988 3261 6S , 2033 3262 4U , 2049 3261 7I , 2091 3262 3S , 2124 3261 5C , 2171 3262 4Q , 2195 3261 6W , 2228 3261 3W , 2270 3262 0V , 2302 3262 4U , 2317 3261 3O , 2355 3262 7M , 2402 3261 3O , 2439 3262 3S , 2472 3246 0B , 2515 3246 4Y , 2976 3247 6O , 3023 3262 0F , 3067 3246 4Y , 3112 3261 4M , 3153 3262 4U , 3169 3261 3O , 3207 3262 7M , 3254 3261 3O , 3291 3262 3S , 3324 3246 0B , 3367 3246 4Y , 3419 3247 0J , 3435 3261 4M , 3468 3262 3S , 3501 3261 6S , 3547 3262 4U , 3562 3261 7I , 3605 3262 3S , 3638 3261 5C , 3685 3262 4Q , 3708 3261 6W , 3741 3261 3W , 3784 3262 0V , 1921 3166 4M , 1955 3167 3S , 1988 3166 6S , 2033 3167 4U , 2049 3166 7I , 2091 3167 3S , 2124 3166 5C , 2171 3167 4Q , 2195 3166 6W , 2228 3166 3W , 2270 3167 0V , 2302 3167 4U , 2317 3166 4M , 2350 3166 3O , 2388 3152 6O , 2435 3166 3W , 2478 3167 3S , 2511 3166 3W , 2553 3166 6W , 2586 3167 4Q , 2609 3166 7I , 2652 3167 7M , 2976 3152 6O , 3025 3166 7I , 3067 3166 4M , 3109 3167 4U , 3124 3166 3W , 3167 3167 7M , 3214 3151 0B , 3256 3167 6K , 3321 3167 4Q , 3344 3166 4M , 3378 3166 6W , 3411 3166 3W , 3453 3167 7M , 3500 3166 6S , 3538 3166 3O , 3583 3152 0J , 3599 3166 4M , 3632 3167 3S , 3665 3166 6S , 3711 3167 4U , 3726 3166 7I , 3769 3167 3S , 3802 3166 5C , 3849 3167 4Q , 3872 3166 6W , 3905 3166 3W , 3948 3167 0V , 1921 3071 4M , 1955 3072 3S , 1988 3071 6S , 2033 3072 4U , 2049 3071 7I , 2091 3072 3S , 2124 3071 5C , 2171 3072 4Q , 2195 3071 6W , 2228 3071 3W , 2270 3072 0V , 2302 3072 4U , 2317 3071 4M , 2350 3072 4Q , 2374 3072 5K , 2412 3071 3O , 2976 3057 6O , 3023 3072 0F , 3067 3056 4Y , 3112 3071 4M , 3153 3072 4U , 3169 3071 4M , 3202 3072 4Q , 3226 3072 5K , 3264 3071 3O , 3309 3057 0J , 3325 3071 4M , 3358 3072 3S , 3391 3071 6S , 3437 3072 4U , 3452 3071 7I , 3495 3072 3S , 3528 3071 5C , 3575 3072 4Q , 3598 3071 6W , 3631 3071 3W , 3674 3072 0V , 1921 2977 4M , 1955 2978 3S , 1988 2977 6S , 2033 2978 4U , 2049 2977 4M , 2082 2977 3O , 2120 2963 6O , 2167 2977 3W , 2209 2978 3S , 2242 2977 3W , 2285 2977 6W , 2318 2978 4Q , 2341 2977 7I , 2383 2978 7M , 2976 2963 6O , 3025 2977 7I , 3067 2977 4M , 3109 2978 4U , 3124 2977 3W , 3167 2978 7M , 3214 2962 0B , 3256 2978 6K , 3321 2978 4Q , 3344 2977 4M , 3378 2977 6W , 3411 2977 3W , 3453 2978 7M , 3500 2977 6S , 3538 2977 3O , 3583 2963 0J , 3599 2977 4M , 3632 2978 3S , 3665 2977 6S , 1921 2882 4M , 1955 2883 3S , 1988 2882 6S , 2033 2883 4U , 2049 2882 46 35 /2G $C .Oskup"]ZoqRZNAomL+Q='n]$PP_EGlfl14Is&GDW&_Xu+T+G~> , 2091 2882 3O , 2129 2883 0V , 2152 2882 7I , 2197 2882 6S , 2243 2883 4U , 2258 2882 6S , 2296 2882 7I , 2338 2883 0N , 2409 2868 6O , 2458 2882 7I , 2500 2883 7M , 2976 2882 4M , 3009 2883 3S , 3042 2882 6S , 3088 2883 4U , 3103 2882 2G , 3146 2882 3O , 3183 2883 0V , 3207 2882 7I , 3251 2882 6S , 3297 2868 0J , 3313 2868 6O , 3362 2882 7I , 3404 2882 4M , 3446 2883 4U , 3461 2882 6S , 3499 2882 3W , 3541 2883 3S , 3574 2882 6W , 3607 2882 3O , 3645 2882 4M , 3678 2883 4Q , 3702 2882 3W , 3744 2883 7M , 1921 2788 4M , 1955 2789 3S , 1988 2788 6S , 2033 2789 4U , 2049 2788 2G , 2091 2788 3O , 2129 2789 0V , 2152 2788 7I , 2197 2788 6S , 2243 2789 4U , 2258 2773 0B , 2301 2788 6S , 2976 2788 4M , 3009 2789 3S , 3042 2788 6S , 3088 2789 4U , 3103 2788 2G , 3146 2788 3O , 3183 2789 0V , 3207 2788 7I , 3251 2788 6S , 3297 2774 0J , 3313 2774 6O , 3362 2788 7I , 3404 2788 4M , 3446 2789 4U , 3461 2773 0B 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5668 2Y , 3299 5668 2I , 3341 5669 2Q , 3356 5668 1S , 3398 5668 6L , 3431 5669 3K , 3502 5668 6X , 3544 5668 2I , 1965 5573 6X , 2008 5573 2Y , 2055 5573 2I , 2096 5574 2Q , 2112 5573 1S , 2154 5574 2M , 2177 5574 1O , 2218 5574 2Q , 2234 5573 1K , 2272 5574 46 34 /3O $C 2AdhGs31]UM1Oq5Y*HArf$_-1f%O0Q[oP"cQ$5WedVb?#kr5L(2bNBG(?Yc**md-e~> , 2316 5573 6L , 2349 5574 2M , 2373 5574 7B , 2420 5573 6H , 2457 5573 6L , 2490 5574 2M , 2514 5573 6X , 2556 5574 7B , 3210 5573 6X , 3252 5573 2Y , 3299 5573 2I , 3341 5574 2Q , 3356 5573 1S , 3398 5573 6L , 3431 5574 3K , 3502 5573 6X , 3544 5573 2I , 3586 5574 2Q , 3601 5573 1K , 3639 5574 3O , 3683 5573 6L , 3716 5574 2M , 3740 5574 7B , 3787 5573 6H , 3825 5573 6L , 3858 5574 2M , 3881 5573 6X , 3923 5574 7B , 1965 5478 6X , 2008 5478 2Y , 2055 5478 2I , 2096 5479 2Q , 2112 5478 1S , 2154 5479 2M , 2177 5479 1O , 2218 5479 2Q , 2234 5479 3K , 2305 5478 1S , 2347 5478 2I , 2380 5478 2I , 3210 5478 6X , 3252 5478 2Y , 3299 5478 2I , 3341 5479 2Q , 3356 5478 1S , 3398 5479 2M , 3422 5479 1O , 3455 5479 77 54 /0S $C 4rMFe$l!LOPQXl<87>^0le;Ag5`#I6rkIdq\,--6oY:.nJ(OY6V>n<2rkIk!0E(iVp&AspJ(sg, qte(nrnl0(hpqa6pAUEXric1u\+IH0j*m>9i560E26Us~> , 3532 5478 1S , 3575 5478 2I , 3608 5478 2I , 1965 5370 6D , 2012 5385 3C , 2059 5384 6X , 2102 5384 6L , 2143 5385 2Q , 2158 5385 47 56 /3S $C 49QW*5KX-jMeTBps8W-!s8W-!s8W-!s8W(;2*[60emJIWs8W-!n*djV\(fks_]ndkjWKW~> , 2205 5384 7N , 2252 5385 3O , 2297 5385 5Z , 2362 5384 1K , 2399 5385 7B , 2446 5384 2I , 3210 5370 6D , 3257 5385 3C , 3304 5384 6X , 3346 5384 6L , 3387 5385 2Q , 3403 5385 3S , 3450 5384 7N , 3497 5385 5Z , 3561 5384 1K , 3599 5385 7B , 3646 5384 2I , 1965 5275 6D , 2012 5290 3C , 2059 5289 6X , 2102 5289 6L , 2143 5290 2Q , 2158 5290 3S , 2205 5289 7N , 2252 5290 3O , 2297 5290 5Z , 2362 5289 1K , 2399 5290 7B , 2446 5289 2I , 2488 5290 2Q , 2503 5289 2I , 2537 5289 2Y , 3210 5275 6D , 3257 5290 3C , 3304 5289 6X , 3346 5289 6L , 3387 5290 2Q , 3403 5290 3S , 3450 5289 7N , 3497 5290 5Z , 3561 5289 1K , 3599 5290 7B , 3646 5289 2I , 3687 5290 2Q , 3703 5289 2I , 3736 5289 2Y , 1965 5180 6D , 2012 5195 3C , 2059 5194 6X , 2102 5194 6L , 2143 5195 2Q , 2158 5194 2I , 2192 5194 2Y , 3210 5180 6D , 3257 5195 3C , 3304 5194 6X , 3346 5194 6L , 3387 5195 2Q , 3403 5195 3K , 3473 5194 1S , 3516 5179 7F , 3566 5195 2Q , 3581 5194 2I , 3615 5194 2Y , 1965 5086 6D , 2012 5101 3C , 2057 5085 0C , 2102 5100 2I , 2143 5101 2Q , 2159 5100 1S , 2201 5100 6L , 2242 5101 2Q , 2257 5100 2Y , 2304 5101 1O , 2337 5100 1S , 2380 5101 7B , 2427 5100 6H , 2462 5101 3C , 2509 5101 2M , 2533 5101 7B , 2580 5085 7F , 2622 5099 7J , 2684 5100 1S , 2727 5100 6L , 2760 5101 2M , 2783 5100 6X , 3210 5086 6D , 3257 5101 3C , 3301 5085 0C , 3346 5100 2I , 3388 5101 2Q , 3403 5100 1S , 3445 5100 6L , 3478 5101 3K , 3549 5100 6X , 3591 5101 2U , 3623 5101 2Q , 3638 5100 2Y , 3685 5101 1O , 3718 5100 1S , 3761 5101 7B , 3808 5100 6H , 3843 5101 3C , 3890 5101 2M , 3914 5101 7B , 3961 5085 7F , 4003 5099 7J , 4065 5100 1S , 4108 5100 6L , 4141 5101 2M , 4164 5100 6X , 1965 4991 6D , 2012 5006 3C , 2057 4990 0C , 2102 5005 2I , 2143 5006 2Q , 2159 5005 1S , 2201 5005 6L , 2242 5006 2Q , 2257 5005 6H , 2295 5006 1O , 2328 5005 6X , 2370 5005 2I , 2404 5005 2I , 2445 5004 37 58 /0W $C -E,Eu-jSBIpd@l(7"Z!]6+o41qRo,,5P9O+?G7piX , 2484 5005 1K , 2522 5005 6H , 2559 5005 6L , 2592 5006 2M , 2616 5005 6X , 2658 5006 7B , 3210 4991 6D , 3257 5006 3C , 3301 4990 0C , 3346 5005 2I , 3388 5006 2Q , 3403 5005 1S , 3445 5005 6L , 3478 5006 3K , 3549 5005 6X , 3591 5006 2U , 3623 5006 2Q , 3638 5005 6H , 3676 5006 1O , 3709 5005 6X , 3751 5005 2I , 3785 5005 2I , 3826 5004 0W , 3865 5005 1K , 3903 5005 6H , 3940 5005 6L , 3973 5006 2M , 3997 5005 6X , 4039 5006 7B , 1965 4897 6D , 2012 4912 3C , 2057 4896 0C , 2102 4911 2I , 2143 4912 2Q , 2159 4911 1S , 2201 4911 6L , 2242 4912 2Q , 2257 4912 2U , 2281 4912 2M , 2304 4912 7B , 2351 4911 1K , 2397 4910 0W , 2436 4912 3C , 2483 4912 2M , 2507 4912 3G , 2533 4911 6L , 3210 4897 6D , 3257 4912 3C , 3301 4896 0C , 3346 4911 2I , 3388 4912 2Q , 3403 4911 1S , 3445 4911 6L , 3478 4912 3K , 3549 4911 6X , 3591 4912 2U , 3623 4912 2Q , 3638 4912 2U , 3662 4912 2M , 3685 4912 7B , 3732 4911 1K , 3778 4910 0W , 3817 4912 3C , 3864 4912 2M , 3888 4912 3G , 3914 4911 6L , 1965 4802 6D , 2012 4817 3C , 2057 4801 0C , 2102 4816 2I , 2143 4817 2Q , 2159 4816 1S , 2201 4816 6L , 2242 4817 2Q , 2257 4817 3K , 2328 4816 6X , 2370 4817 3K , 2441 4816 1K , 2479 4817 7B , 2523 4816 6L , 1965 4707 6D , 2012 4722 3C , 2057 4706 0C , 2102 4721 2I , 2143 4722 2Q , 2159 4721 1S , 2201 4721 6L , 2242 4722 2Q , 2257 4722 3K , 2328 4721 6X , 2370 4722 3K , 2441 4721 1K , 2479 4722 7B , 2523 4721 6L , 2564 4722 2Q , 2580 4721 1K , 2617 4722 2U , 2641 4721 1K , 2678 4721 6H , 2716 4721 6L , 2749 4722 1O , 2782 4722 2M , 2806 4721 6H , 3210 4707 6D , 3257 4722 3C , 3301 4706 0C , 3346 4721 2I , 3388 4722 2Q , 3403 4721 1S , 3445 4721 6L , 3486 4722 2Q , 3502 4722 1O , 3535 4721 1S , 3577 4721 1W , 3624 4722 2M , 3648 4721 1S , 3690 4721 6L , 3723 4722 2M , 3747 4721 6X , 3789 4722 7B , 3836 4722 61 53 /3W $C ,6=S80GYL4s8W-!s8W-!s8W+jY[@G1p]%A]s8M]k]m$Ug0O.+m~> , 3895 4706 0C , 3939 4707 6D , 3989 4721 1K , 1965 4613 6D , 2012 4628 3C , 2057 4612 0C , 2102 4627 2I , 2143 4628 2Q , 2159 4627 1S , 2201 4627 6L , 2242 4628 2Q , 2257 4628 3K , 2328 4627 6X , 2370 4628 3K , 2441 4627 1K , 2479 4628 7B , 2523 4627 6L , 2564 4628 2Q , 2580 4628 3K , 2650 4627 1S , 2693 4612 7F , 2735 4628 7B , 2782 4627 1K , 2820 4627 6L , 2853 4628 2M , 2876 4627 6H , 3210 4613 6D , 3257 4628 3C , 3301 4612 0C , 3346 4627 2I , 3388 4628 2Q , 3403 4627 1S , 3445 4627 6L , 3486 4628 2Q , 3502 4628 1O , 3535 4627 1S , 3577 4627 1W , 3624 4628 2M , 3648 4627 1S , 3690 4627 6L , 3723 4628 2M , 3747 4627 6X , 3789 4628 7B , 3836 4628 3W , 3895 4612 0C , 3939 4613 6D , 3989 4627 1K , 1965 4518 6D , 2012 4533 3C , 2057 4517 0C , 2102 4532 2I , 2143 4533 2Q , 2159 4532 1S , 2201 4532 6L , 2242 4533 2Q , 2257 4518 47 50 /1A $C +@&GZ6N@)cr^79K#Jqe'n:D,AK7,(-:KQ.Lf3eC?s8W-!qtpDCCN&NW[Z((l-.lWY(oN+u0M_~> , 2302 4533 7B , 2357 4533 2Q , 2381 4531 0W , 3210 4518 6D , 3257 4533 3C , 3301 4517 0C , 3346 4532 2I , 3388 4533 2Q , 3403 4532 1S , 3445 4532 6L , 3486 4533 2Q , 3502 4518 1A , 3547 4533 7B , 1965 4423 6D , 2012 4438 3C , 2057 4422 0C , 2102 4437 2I , 2143 4438 2Q , 2159 4437 1S , 2201 4437 6L , 2242 4438 2Q , 2257 4423 1A , 2302 4438 7B , 2357 4438 2Q , 2373 4438 0K , 3210 4423 6D , 3257 4438 3C , 3301 4422 0C , 3346 4437 2I , 3388 4438 2Q , 3403 4437 1S , 3445 4437 6L , 3486 4438 2Q , 3502 4423 1A , 3547 4438 7B , 1965 4329 6D , 2012 4344 3C , 2057 4328 0C , 2102 4343 2I , 2143 4344 2Q , 2159 4343 1S , 2201 4343 6L , 2242 4344 2Q , 2257 4329 1A , 2302 4344 7B , 2357 4344 2Q , 2373 4342 42 56 /4A $C .F*#fs8W-!s8W-!s8W+QPi,oa~> , 3210 4329 6D , 3257 4344 3C , 3301 4328 0C , 3346 4343 2I , 3388 4344 2Q , 3403 4343 1S , 3445 4343 6L , 3486 4344 2Q , 3502 4329 1A , 3547 4344 7B , 1965 4234 6D , 2012 4249 3C , 2057 4233 0C , 2102 4248 2I , 2143 4249 2Q , 2159 4248 1S , 2201 4248 6L , 2242 4249 2Q , 2257 4234 1A , 2302 4249 7B , 2357 4249 2Q , 2373 4249 55 54 /1E $C 4pF6B!a&h0s8W(5s8W,tJ(KCpr^KD5n,E@e_1&ooli7!gY.]/SW=Thm't)s~> , 3210 4234 6D , 3257 4249 3C , 3301 4233 0C , 3346 4248 2I , 3388 4249 2Q , 3403 4248 1S , 3445 4248 6L , 3486 4249 2Q , 3502 4234 1A , 3547 4249 7B , 1965 4139 6D , 2012 4154 3C , 2057 4138 0C , 2102 4153 2I , 2143 4154 2Q , 2159 4153 1S , 2201 4153 6L , 2234 4154 3K , 2304 4153 6X , 2347 4154 2U , 2378 4154 2Q , 2394 4153 2I , 2427 4153 6L , 2460 4153 1S , 2503 4153 6L , 2535 4153 1K , 2581 4154 2Q , 2597 4154 0O , 2644 4154 7B , 2691 4153 1S , 2733 4154 2U , 3210 4139 6D , 3257 4154 3C , 3301 4138 0C , 3346 4153 2I , 3388 4154 2Q , 3403 4153 1S , 3445 4153 6L , 3478 4154 3K , 3549 4153 6X , 3591 4154 2U , 3623 4154 2Q , 3638 4154 0O , 3685 4154 7B , 3732 4153 1S , 3775 4154 2U , 1965 4045 6D , 2012 4060 3C , 2057 4044 0C , 2102 4059 2I , 2143 4060 2Q , 2159 4059 1S , 2201 4059 6L , 2234 4060 3K , 2304 4059 6X , 2347 4060 2U , 2378 4060 2Q , 2394 4059 2I , 2427 4059 6L , 2460 4059 1S , 2503 4059 6L , 2535 4059 1K , 2581 4060 2Q , 2597 4060 2M , 2620 4060 7B , 2667 4060 2M , 2691 4059 6L , 2724 4060 2M , 2747 4059 1S , 2790 4060 2U , 3210 4045 6D , 3257 4060 3C , 3301 4044 0C , 3346 4059 2I , 3388 4060 2Q , 3403 4059 1S , 3445 4059 6L , 3478 4060 3K , 3549 4059 6X , 3591 4060 2U , 3623 4060 2Q , 3638 4060 2M , 3662 4060 7B , 3709 4060 2M , 3732 4059 6L , 3765 4060 2M , 3789 4059 1S , 3831 4060 2U , 1965 3950 6D , 2012 3965 3C , 2057 3949 0C , 2102 3964 2I , 2143 3965 2Q , 2159 3965 3K , 2229 3964 1S , 2272 3964 2I , 2305 3964 2I , 2338 3965 65 54 /4E $C +TY+("spJQs8W-!s68"K&c,R0o\D.%l+1/)dr`11VWi5A:"&=`S#+ZK2bNDaLK*EP\0-52^]~> , 2402 3965 2M , 2425 3964 1K , 2463 3965 2U , 2486 3964 1W , 3210 3950 6D , 3257 3965 3C , 3301 3949 0C , 3346 3964 2I , 3388 3965 2Q , 3403 3965 3K , 3474 3965 4E , 3537 3965 2M , 3561 3964 1K , 3598 3965 2U , 3622 3964 1W , 1965 3855 6D , 2012 3870 3C , 2057 3854 0C , 2102 3869 2I , 2143 3870 2Q , 2159 3870 3K , 2229 3869 6X , 2272 3870 2U , 2303 3870 2Q , 2319 3855 1A , 2363 3869 7N , 2410 3869 1S , 2453 3869 1W , 2500 3870 1O , 2533 3869 7N , 2580 3855 6D , 2629 3869 6X , 2671 3870 2U , 2695 3869 1K , 2741 3870 2Q , 2756 3870 3K , 2827 3869 1S , 2869 3854 7F , 2911 3870 7B , 2958 3869 1K , 2996 3869 6L , 3029 3870 2M , 3053 3869 6H , 3210 3855 6D , 3257 3870 3C , 3301 3854 0C , 3346 3869 2I , 3388 3870 2Q , 3403 3869 1S , 3445 3869 6L , 3486 3870 2Q , 3502 3870 1O , 3535 3869 1S , 3577 3869 1W , 3624 3870 2M , 3648 3869 1S , 3690 3869 6L , 3723 3870 2M , 3747 3869 6X , 3789 3870 7B , 3836 3870 3W , 3895 3854 0C , 3939 3855 6D , 3989 3869 1K , 1965 3761 6D , 2012 3776 3C , 2057 3760 0C , 2102 3775 2I , 2143 3776 2Q , 2159 3776 1O , 2192 3775 1K , 2229 3776 3G , 2255 3776 1O , 2288 3775 1S , 2330 3775 6H , 2368 3775 6L , 2401 3776 2M , 2425 3775 6X , 2467 3776 7B , 3210 3761 6D , 3257 3776 3C , 3301 3760 0C , 3346 3775 2I , 3388 3776 2Q , 3403 3776 1O , 3436 3775 1K , 3474 3776 3G , 3500 3776 1O , 3533 3775 1S , 3575 3775 6H , 3613 3775 6L , 3646 3776 30 54 /1I $C 49bZH-*R@Ks8W-!s8W-!s8W-!s8V`SJA6U~> , 3676 3776 7B , 3723 3775 1W , 3770 3775 1K , 3808 3776 3O , 1965 3666 6D , 2015 3680 6X , 2057 3680 2I , 2098 3681 2Q , 2114 3680 1S , 2156 3681 37 34 /4I $C 3"8(F94#Nj%r\oNp@dme^&-Ogh7_\#rnhYOIbriHmecCa)gK!~> , 2202 3681 2Q , 2217 3681 3C , 2264 3680 1S , 3210 3666 6D , 3259 3680 6X , 3301 3680 2I , 3343 3681 2Q , 3358 3680 1K , 3396 3666 1A , 3449 3681 2Q , 3464 3681 3C , 3511 3680 1S , 1965 3572 6D , 2015 3586 6X , 2057 3586 2I , 2098 3587 2Q , 2114 3586 1K , 2152 3586 1S , 2194 3587 1O , 2227 3586 6L , 2260 3587 3C , 2315 3587 2Q , 2330 3587 7B , 2375 3586 7N , 2422 3586 6L , 2455 3586 1S , 2497 3586 6L , 2530 3587 2M , 2554 3586 6X , 2596 3587 7B , 3210 3572 6D , 3259 3586 6X , 3301 3586 2I , 3343 3587 2Q , 3358 3586 1K , 3396 3586 6X , 3438 3572 6D , 3493 3587 2Q , 3509 3587 7B , 3554 3586 7N , 3601 3586 6L , 3634 3586 1S , 3676 3586 6L , 3709 3587 2M , 3732 3586 6X , 3775 3587 7B , 1965 3491 2I , 1999 3477 6D , 2048 3491 1K , 2086 3491 6H , 2123 3491 6L , 2164 3492 2Q , 2180 3491 46 35 /1M $C .Oskup"]ZoqRZNAomL+Q='n]$PP_EGlfl14Is&GDW&_Xu+T+G~> , 2222 3491 1K , 2260 3492 2U , 2283 3491 6X , 2328 3491 6H , 3210 3491 2I , 3243 3477 6D , 3293 3491 1K , 3330 3491 6H , 3368 3491 6L , 3409 3492 2Q , 3424 3491 1W , 3471 3491 6X , 3514 3477 6D , 3561 3477 6D , 3608 3492 2U , 3631 3491 1K , 3669 3492 1O , 3702 3490 65 56 /4M $C ,(2NKIs(D_7de!^\)17o:"Sj7YGUX[V16s:qpN7D])$ , 3758 3491 1K , 3796 3492 2U , 3819 3491 6X , 3864 3491 6H , 1965 3396 2I , 1999 3397 1O , 2032 3396 6H , 2077 3397 2Q , 2093 3397 3G , 2119 3396 2E , 2180 3397 3C , 2227 3397 3K , 3210 3382 6D , 3257 3397 3C , 3301 3381 0C , 3346 3396 2I , 3388 3397 2Q , 3403 3396 1S , 3445 3397 7B , 3493 3381 7F , 3543 3395 0W , 3582 3397 2M , 3605 3397 4I , 3643 3396 1K , 3689 3382 0G , 3704 3396 2I , 3738 3397 1O , 3771 3396 6H , 1965 3302 2I , 1999 3303 1O , 2032 3302 6H , 2077 3303 2Q , 2093 3302 6X , 2135 3303 1O , 2168 3302 2Y , 2215 3303 2M , 2239 3302 6L , 2272 3302 1S , 2314 3303 2U , 2346 3303 2Q , 2361 3302 1M , 2403 3302 1K , 2441 3303 2U , 2465 3302 6X , 2509 3302 6H , 3210 3288 6D , 3257 3303 3C , 3301 3287 0C , 3346 3302 2I , 3388 3303 2Q , 3403 3302 1M , 3445 3302 1K , 3483 3303 2U , 3507 3302 6X , 3551 3302 6H , 3597 3303 2Q , 3612 3302 6X , 3655 3303 1O , 3688 3302 2Y , 3735 3303 2M , 3758 3302 6L , 3791 3302 1S , 3834 3303 2U , 1965 3207 2I , 1999 3208 1O , 2032 3207 6H , 2077 3208 2Q , 2093 3207 1M , 2135 3207 1K , 2173 3208 2U , 2196 3207 6X , 2241 3207 6H , 3210 3193 6D , 3257 3208 3C , 3301 3192 0C , 3346 3207 2I , 3388 3208 2Q , 3403 3207 1M , 3445 3207 1K , 3483 3208 2U , 3507 3207 6X , 3551 3207 6H , 1965 3112 2I , 1999 3113 1O , 2032 3112 6H , 2077 3113 2Q , 2093 3112 1M , 2135 3112 1K , 2173 3113 2U , 2196 3112 6X , 2241 3112 6H , 2287 3113 2Q , 2302 3112 1S , 2345 3113 7B , 2392 3097 7F , 3210 3098 6D , 3257 3113 3C , 3301 3097 0C , 3346 3112 2I , 3388 3113 2Q , 3403 3112 1M , 3445 3112 1K , 3483 3113 2U , 3507 3112 6X , 3551 3112 6H , 3597 3113 2Q , 3612 3112 1S , 3655 3113 7B , 3702 3097 7F , 1965 3018 2I , 1999 3019 1O , 2032 3018 6H , 2077 3019 2Q , 2093 3018 1M , 2135 3018 1K , 2173 3019 2U , 2196 3018 6X , 2241 3018 6H , 2287 3019 2Q , 2302 3018 6H , 2340 3019 3K , 2408 3018 2Y , 3210 3004 6D , 3257 3019 3C , 3301 3003 0C , 3346 3018 2I , 3388 3019 2Q , 3403 3018 1M , 3445 3018 1K , 3483 3019 2U , 3507 3018 6X , 3551 3018 6H , 3597 3004 0G , 3612 3004 6D , 3662 3018 6X , 3704 3018 2I , 3746 3019 2Q , 3761 3018 6H , 3799 3019 3K , 3867 3018 2Y , 1965 2923 2I , 1999 2924 1O , 2032 2923 6H , 2077 2924 2Q , 2093 2923 1M , 2135 2923 1K , 2173 2924 2U , 2196 2923 6X , 2241 2923 6H , 2287 2924 2Q , 2302 2923 1W , 2349 2924 2M , 2373 2923 2I , 2406 2909 6D , 2456 2923 1K , 2493 2924 1O , 2526 2923 2I , 2560 2924 2M , 2583 2923 6X , 2625 2924 7B , 3210 2909 6D , 3257 2924 3C , 3301 2908 0C , 3346 2923 2I , 3388 2924 2Q , 3403 2923 1M , 3445 2923 1K , 3483 2924 2U , 3507 2923 6X , 3551 2923 6H , 3597 2924 2Q , 3612 2923 1W , 3660 2924 2M , 3683 2923 2I , 3716 2909 6D , 3766 2923 1K , 3803 2924 1O , 3836 2923 2I , 3870 2924 2M , 3893 2923 6X , 3936 2924 7B , 1965 2828 2I , 1999 2829 1O , 2032 2828 6H , 2077 2829 2Q , 2093 2828 1M , 2135 2828 1K , 2173 2829 2U , 2196 2828 6X , 2241 2828 6H , 2287 2829 2Q , 2302 2828 1K , 2340 2828 2I , 2373 2828 6H , 2411 2828 1S , 2453 2814 6D , 2503 2828 1K , 3210 2814 6D , 3257 2829 3C , 3301 2813 0C , 3346 2828 2I , 3388 2829 2Q , 3403 2828 1M , 3445 2828 1K , 3483 2829 2U , 3507 2828 6X , 3551 2828 6H , 3597 2829 2Q , 3612 2828 1K , 3650 2828 2I , 3683 2828 6H , 3721 2828 1S , 3764 2814 6D , 3813 2828 1K , 1965 2734 2I , 1999 2735 1O , 2032 2734 6H , 2077 2735 2Q , 2093 2734 1M , 2135 2734 1K , 2173 2735 2U , 2196 2734 6X , 2241 2734 6H , 2287 2735 2Q , 2302 2734 1K , 2340 2735 3O , 2384 2720 6D , 2432 2734 1S , 2474 2735 7B , 2521 2734 2I , 2554 2735 2M , 2578 2734 6X , 2620 2735 7B , 3210 2720 6D , 3257 2735 3C , 3301 2719 0C , 3346 2734 2I , 3388 2735 2Q , 3403 2734 1M , 3445 2734 1K , 3483 2735 2U , 3507 2734 6X , 3551 2734 6H , 3597 2735 2Q , 3612 2734 1K , 3650 2735 3O , 3695 2720 6D , 3742 2734 1S , 3784 2735 7B , 3831 2734 2I , 3865 2735 2M , 3888 2734 6X , 3930 2735 7B , 1965 2639 2I , 1999 2640 1O , 2032 2639 6H , 2077 2640 2Q , 2093 2639 1M , 2135 2639 1K , 2173 2640 2U , 2196 2639 6X , 2241 2639 6H , 2287 2640 2Q , 2302 2640 2U , 2326 2624 7F , 3210 2625 6D , 3257 2640 3C , 3301 2624 0C , 3346 2639 2I , 3388 2640 2Q , 3403 2639 1M , 3445 2639 1K , 3483 2640 2U , 3507 2639 6X , 3551 2639 6H , 3597 2625 0G , 3612 2625 6D , 3662 2639 6X , 3704 2639 2I , 3746 2640 2Q , 3761 2640 2U , 3785 2624 7F , 1965 2544 2I , 1999 2545 1O , 2032 2544 6H , 2077 2545 2Q , 2093 2544 1M , 2135 2544 1K , 2173 2545 2U , 2196 2544 6X , 2241 2544 6H , 2287 2545 2Q , 2302 2545 2U , 2326 2544 2I , 2359 2545 1O , 3210 2530 6D , 3257 2545 3C , 3301 2529 0C , 3346 2544 2I , 3388 2545 2Q , 3403 2544 1M , 3445 2544 1K , 3483 2545 2U , 3507 2544 6X , 3551 2544 6H , 3597 2530 0G , 3612 2530 6D , 3662 2544 6X , 3704 2544 2I , 3746 2545 2Q , 3761 2545 2U , 3785 2544 2I , 3818 2545 1O , 1965 2450 2I , 1999 2451 1O , 2032 2450 6H , 2077 2451 2Q , 2093 2450 1M , 2135 2450 1K , 2173 2451 2U , 2196 2450 6X , 2241 2450 6H , 2287 2451 2Q , 2302 2451 3K , 2373 2451 2M , 2396 2450 6H , 2434 2451 1O , 2467 2450 6X , 2509 2451 3W , 2563 2450 7N , 2610 2451 1O , 2643 2450 2Y , 3210 2436 6D , 3257 2451 3C , 3301 2435 0C , 3346 2450 2I , 3388 2451 2Q , 3403 2450 1M , 3445 2450 1K , 3483 2451 2U , 3507 2450 6X , 3551 2450 6H , 3597 2451 2Q , 3612 2451 3K , 3683 2451 2M , 3707 2450 6H , 3744 2451 1O , 3777 2450 6X , 3820 2451 3W , 3874 2450 7N , 3921 2451 1O , 3954 2450 2Y , 1965 2355 2I , 1999 2356 1O , 2032 2355 6H , 2077 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5716 6I , 1166 5715 3M , 1206 5716 36 34 /0Y $C /e)pSG"!!]Ddi&#]50!-DV_pJiOa:#gUAlkVShfpqfom0J,~> , 1263 5716 6I , 1293 5715 3M , 1333 5716 0Y , 1380 5716 7G , 2519 5716 6M , 2565 5716 7G , 2602 5716 3Q , 2648 5716 3U , 2702 5716 6I , 2733 5716 3D , 2772 5716 6E , 2819 5716 3I , 994 5604 6Q , 1039 5622 3D , 1083 5622 3I , 1136 5622 6I , 1163 5622 6E , 1208 5622 3D , 1250 5622 3Y , 1291 5604 4W , 1333 5622 4C , 1380 5622 6U , 2519 5622 6M , 2565 5622 7G , 2602 5622 3Q , 2648 5622 3U , 2702 5622 6I , 2733 5622 3D , 2772 5622 6E , 2819 5622 3I , 2872 5622 6I , 2902 5622 3U , 2941 5622 4K , 2986 5622 3Y , 994 5509 6Q , 1039 5527 3D , 1083 5527 3I , 1136 5527 6I , 1168 5527 6U , 1204 5527 3Q , 1248 5527 6E , 2519 5527 6M , 2565 5527 7G , 2602 5527 3Q , 2648 5527 3U , 2702 5527 6I , 2733 5527 3D , 2772 5527 6E , 2819 5527 3I , 2872 5527 6I , 2904 5527 3I , 2942 5527 6M , 2987 5526 3M , 3027 5527 4C , 3069 5527 6M , 994 5414 6Q , 1039 5432 3D , 1083 5432 3I , 1136 5432 6I , 1166 5432 3U , 1208 5431 3M , 1249 5432 4C , 1291 5432 6M , 1332 5432 0D , 1390 5432 6I , 1420 5431 3M , 1462 5432 6Y , 1503 5432 6M , 1549 5432 7G , 1588 5432 6M , 1629 5432 0P , 1673 5432 3Y , 1716 5432 3U , 994 5320 6Q , 1039 5338 3D , 1083 5338 3I , 1136 5338 6I , 1166 5338 3U , 1208 5338 3D , 1248 5320 6Q , 2937 474 42 73 /5T $C 4;sf+$pfS_s8W-!s8W-!s8W-!s8W-!s8W-!rcl)/^(6G1' , 2984 474 55 74 /1E $C .`%n$O?>5!J,fQKr:i$paU$8N^AYfpqgSG9rV,^Z\(gq$\,P9'rP/('J*lt0g[5$Mg])3,^;k_M qqp90~> , cleartomark end end pagesave restore showpage %%PageTrailer %%Trailer %%Pages: 14 %%EOF --=_5j4gqpybq3y8-- From owner-ucd-sci@eso.org Mon Jul 11 18:37:03 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 j6BGap1b027113 for ; Mon, 11 Jul 2005 18:36:51 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j6BGaoqD027110 for ucd-sci-outgoing; Mon, 11 Jul 2005 18:36:50 +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 j6BGai1b027100; Mon, 11 Jul 2005 18:36:45 +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 ESMTP id j6BGafhx006062; Mon, 11 Jul 2005 18:36:42 +0200 (CEST) Received: from dropbox.aoc.nrao.edu (dropbox [146.88.1.13]) by revere.aoc.nrao.edu (8.11.6/8.11.6) with ESMTP id j6BGaQH05687; Mon, 11 Jul 2005 10:36:26 -0600 Received: from oak.aoc.nrao.edu (oak.aoc.nrao.edu [146.88.3.232]) by dropbox.aoc.nrao.edu (8.12.8/8.12.8/smtp-gateway) with ESMTP id j6BGaPen019660; Mon, 11 Jul 2005 10:36:25 -0600 Date: Mon, 11 Jul 2005 10:36:25 -0600 (MDT) From: Doug Tody X-X-Sender: dtody@oak To: ucd@ivoa.net cc: ucd-sci@ivoa.net Subject: Re: draft PR doc on ucd-words In-Reply-To: <20050711170103.buzzas2dadesw8cs@webmail.sic.rm.cnr.it> 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=-1, required 7, EMAIL_ATTRIBUTION -0.50, IN_REP_TO -0.50, USER_AGENT_PINE 0.00) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.2, Antispam-Data: 2005.7.11.16 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 Mon, 11 Jul 2005, Andrea Preite Martinez wrote: > 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 I haven't been following the UCD discussions, and while I am sure there is some reason for this change, these name changes do not look like an improvement. The "old" version is clearly preferable here. - Doug From owner-ucd-sci@eso.org Mon Jul 11 19:25:07 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 j6BHP01b005201 for ; Mon, 11 Jul 2005 19:25:01 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j6BHP0mp005200 for ucd-sci-outgoing; Mon, 11 Jul 2005 19:25:00 +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 j6BHOv1b005193 for ; Mon, 11 Jul 2005 19:24:57 +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 j6BHOtin014161 for ; Mon, 11 Jul 2005 19:24:56 +0200 (CEST) Received: from sothis.cfa.harvard.edu (sothis [131.142.52.147]) by head.cfa.harvard.edu (d/w) with ESMTP id j6BHOnRY028721 for ; Mon, 11 Jul 2005 13:24:49 -0400 (EDT) From: Jonathan McDowell Received: (from jcm@localhost) by sothis.cfa.harvard.edu (8.12.8p1/8.12.8) id j6BHOnJa000739 for ucd-sci@ivoa.net; Mon, 11 Jul 2005 13:24:49 -0400 (EDT) Date: Mon, 11 Jul 2005 13:24:49 -0400 (EDT) Message-Id: <200507111724.j6BHOnJa000739@sothis.cfa.harvard.edu> To: ucd-sci@ivoa.net Subject: Re: draft PR doc on ucd-words X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.2, Antispam-Data: 2005.7.11.18 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 Mon, 11 Jul 2005, Andrea Preite Martinez wrote: > 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 I agree with Doug. I hate the new versions. I think the "can't be a starting substring" was put in to make some kinds of searching easier, but I never found the argument convincing and would argue that we should instead remove this restriction from the UCD-Rec document. - Jonathan From owner-ucd-sci@eso.org Mon Jul 11 19:56:19 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 j6BHuB1b009576 for ; Mon, 11 Jul 2005 19:56:11 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j6BHuBtb009575 for ucd-sci-outgoing; Mon, 11 Jul 2005 19:56:11 +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 j6BHu41b009561 for ; Mon, 11 Jul 2005 19:56:05 +0200 (MEST) Received: from smtp.ucolick.org (santo.ucolick.org [128.114.23.204]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j6BHu2in015377 for ; Mon, 11 Jul 2005 19:56:03 +0200 (CEST) Received: from localhost (localhost [127.0.0.1]) by smtp.ucolick.org (Postfix) with ESMTP id 7BAED5D714 for ; Mon, 11 Jul 2005 10:55:56 -0700 (PDT) Received: from geneva.ucolick.org (geneva.ucolick.org [128.114.23.183]) (using TLSv1 with cipher DHE-RSA-AES256-SHA (256/256 bits)) (No client certificate requested) by smtp.ucolick.org (Postfix) with ESMTP id 1EEA011406 for ; Mon, 11 Jul 2005 10:55:56 -0700 (PDT) Received: from geneva.ucolick.org (localhost [127.0.0.1]) by geneva.ucolick.org (8.13.1/8.12.10) with ESMTP id j6BHtt2K026926 for ; Mon, 11 Jul 2005 10:55:55 -0700 Received: (from sla@localhost) by geneva.ucolick.org (8.13.1/8.13.1/Submit) id j6BHttZ7026925 for ucd-sci@ivoa.net; Mon, 11 Jul 2005 10:55:55 -0700 Date: Mon, 11 Jul 2005 10:55:54 -0700 From: Steve Allen To: ucd-sci@ivoa.net Subject: Re: draft PR doc on ucd-words Message-ID: <20050711175554.GD26543@ucolick.org> References: <20050711170103.buzzas2dadesw8cs@webmail.sic.rm.cnr.it> Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii Content-Disposition: inline In-Reply-To: User-Agent: Mutt/1.4.2.1i X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.2, Antispam-Data: 2005.7.11.20 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 Mon 2005-07-11T10:36:25 -0600, Doug Tody hath writ: > > old version =============> new version > > pos.earthop pos.eop In this one case the new version is actually more mnemonic for those of us who look at such data regularly. -- Steve Allen WGS-84 (GPS) UCO/Lick Observatory Natural Sciences II, Room 165 Lat +36.99858 University of California Voice: +1 831 459 3046 Lng -122.06014 Santa Cruz, CA 95064 http://www.ucolick.org/~sla/ Hgt +250 m From owner-ucd-sci@eso.org Tue Jul 12 15:33:09 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 j6CDX0d5003590 for ; Tue, 12 Jul 2005 15:33:00 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j6CDX0Ub003589 for ucd-sci-outgoing; Tue, 12 Jul 2005 15:33:00 +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 j6CDWrd5003527 for ; Tue, 12 Jul 2005 15:32:54 +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 j6CDWqin024471 for ; Tue, 12 Jul 2005 15:32:52 +0200 (CEST) Received: (qmail 25029 invoked by uid 508); 12 Jul 2005 13:32:45 -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 0.031783 secs); 12 Jul 2005 13:32:45 -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 ; 12 Jul 2005 13:32:45 -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 ; Tue, 12 Jul 2005 15:32:45 +0200 Message-ID: <20050712153245.dzuvuukco8hwkw0s@webmail.sic.rm.cnr.it> Date: Tue, 12 Jul 2005 15:32:45 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Cc: ucd@ivoa.net Subject: UCD-list: pdf/html file 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: 2.0.3.2, Antispam-Data: 2005.7.12.10 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 Sorry for yersteday, the attached file had extension ".pdf" but it was a .ps!! As for the content of the document, I agree with Doug and Jonathan, so it is a pleasure for me to come back to the old spelling "phot.fluxDens" ! I keep "pos.eop" (by the way, this was the spelling proposed by planetary people!) I added a note in the doc explaining that a few words are not complying with one of the recs in the main document. I uploaded the document in the ivoa doc repository http://www.ivoa.net/Documents. I hope it'll be made available soon. 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-sci@eso.org Wed Jul 13 09:45:56 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 j6D7jjU6005788 for ; Wed, 13 Jul 2005 09:45:45 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j6D7jilX005787 for ucd-sci-outgoing; Wed, 13 Jul 2005 09:45:44 +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 j6D7jeU6005778 for ; Wed, 13 Jul 2005 09:45:40 +0200 (MEST) Received: from esa-av-smtp2.gmessaging.net (esa-av-smtp2.gmessaging.net [194.51.201.23]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j6D7jahx023045 for ; Wed, 13 Jul 2005 09:45:37 +0200 (CEST) Received: from esa-spas1.gmessaging.net (relay2 [172.24.21.39]) by esa-av-smtp2.gmessaging.net (iPlanet Messaging Server 5.2 Patch 2 (built Jul 14 2004)) with ESMTP id <0IJK00GKD2VUBM@esa-av-smtp2.gmessaging.net> for ucd-sci@ivoa.net; Wed, 13 Jul 2005 09:45:30 +0200 (MEST) Received: from localhost (localhost.localdomain [127.0.0.1]) by esa-spas1.gmessaging.net (Postfix) with ESMTP id 23E5C229DAB for ; Wed, 13 Jul 2005 09:45:31 +0200 (CEST) Received: from esa-spas1.gmessaging.net ([127.0.0.1]) by localhost (esa-spas1 [127.0.0.1]) (amavisd-new, port 10024) with ESMTP id 05711-03 for ; Wed, 13 Jul 2005 09:45:29 +0200 (CEST) Received: from sciops-mailgw.vilspa.esa.int (sciops-mailgw.vilspa.esa.int [193.147.152.105]) by esa-spas1.gmessaging.net (Postfix) with ESMTP id 038C9229DA9 for ; Wed, 13 Jul 2005 09:45:29 +0200 (CEST) Received: from xvsas01.vilspa.esa.es (xvsas01.vilspa.esa.es [193.147.152.101]) by sciops-mailgw.vilspa.esa.int (Postfix) with ESMTP id C29F511F8EF for ; Wed, 13 Jul 2005 09:45:28 +0200 (CEST) Received: from sciops.esa.int (xmmwl31.xsci.lan [192.168.1.61]) by xvsas01.vilspa.esa.es (8.12.10/8.12.10) with ESMTP id j6D7jSrv019717 for ; Wed, 13 Jul 2005 07:45:28 +0000 (GMT) Date: Wed, 13 Jul 2005 07:45:28 +0000 From: Matteo Guainazzi Subject: Late comments (mainly) on the UCD word list To: ucd-sci@ivoa.net Message-id: <42D4C698.70908@sciops.esa.int> MIME-version: 1.0 Content-type: text/plain; charset=us-ascii; format=flowed Content-transfer-encoding: 7BIT X-Accept-Language: en-us, en User-Agent: Mozilla/5.0 (X11; U; Linux i686; en-US; rv:1.6) Gecko/20040115 X-Spam-Score: Content analysis details: (-1.2 points, 4.5 points required to be considered as spam) -1.2 BAYES_00 BODY: Bayesian spam probability is 0 to 1% [score: 0.0000] X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.2, Antispam-Data: 2005.7.12.45 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 Dear Andrea et al., you will find below some comments, mainly on the current UCD list, prepared by Ana and myself. If I interpret correctly your last message to the UCD SciBoard, we have passed the deadline, when the contributions from the UCD SciBoard were expected to come. If so, we have obviously missed some important information about the time-line. We apologize for that. Should our comment be arrived beyond the time horizon, feel free to ignore them for the time being, and to postpone them for the next round of comments, if anyhow interesting: 1. we propose to remove all the words containing an explicit specification of the wavelength or frequency range. They should be replaced by words of the type: "em.wl.start; em.wl.end" (these words do not exist, and should be added). Rationale: the current method lacks flexibility, and is very likely not to cover all the interesting wavelengths ranges in existing catalogues, where "standard" wavelength ranges do not exist (e.g., high-energy) 2. we propose to substitute "instr.${band}" for all words of the type "em.${band}". Rationale: the sensitive bandpass is a property of the detector 3. we propose to add the words "em.wl.start" and "em.wl.stop". Rationale: they may be useful and flexible characterizations of the bandpass 4. we propose to move "instr.obsty.site.seeing" to "obs.seeing". Rationale: this is a property of an observation rather than of an instrument 5. we propose to unify "instr.beam" and "instr.det.psf" into "instr.psf". Rationale: in most cases, users are interested in the overall PSF (optics+detector). "Beam" is the radio jargon for PSF. Should the detector PSF be necessary, one could use: "instr.psf; instr.det" 6. we propose to remove "instr.precision". Rationale: too generic, probably useless 7. we propose to add the following radio-related words: "instr.interferometry", and "instr.resolution". Rationale: the former is self-explaining; the latter indicates the spatial resolution 8. we propose to change the word code of "instr.filter.transm" and "instr.spect.resolution" to "V". Rationale: the filter transmission is an intrinsically vectorial quantity; the spectral resolution as well (dependence on energy and/or order) 9. we propose to add a further atom to the "Multiplicity of binarity flag": "meta.code.multip.star", "meta.code.multip.planet". Rationale: self-explaining 10. we propose to add a further "meta" atom: "meta.subexp". Rationale: this will allow to characterize the rank of sub-exposures in a multi-exposure observations, whenever useful for, e.g., variability studies 11. we propose to add a further "meta" atom: "meta.rank". Rationale: useful to indicate an element in an intrinsically vectorial quantity 12. we propose to move "meta.id" and "meta.id.assoc" to "src.id" and "src.id.assoc". Rationale: they belong to "sources" rather then to "metadata" 13. we believe that the following "phys" word should be moved to "src": "phys.angArea", "phys.AngSize" (and associated words), "phys.area", "phys.size" (and associated words). Rationale: the same as #12 above 14. we believe that words belonging to the following categories: "phot", "pos", "spec", should be placed under the category "src" (e.g.: "phot.antennaTemp" -> "src.phot.antennaTemp", "pos.angDistance" -> "src.pos.angDistance"; "spect.Doppler" -> "src.spect.Doppler". Rationale: all these words ultimately describe source properties 15. the words for coupling of quantum numbers do not cover all the possible coupling cases. A more general method is needed, and the Data Line Model sub-group is indeed working on this. We propose to wait for the conclusion of their work, before this issue is ultimately addressed 16. a new word "pos.offaxis" should be added. Rationale: the off-axis angle may be a useful quantity is some catalogs 17. "pos.earth", "pos.earth.lat", "pos.earth.lon" should be placed under the "obs" category. Rationale: these quantity belongs logically to an observation, not to (the position of) a source 18. "pos.earth.nutation" should be removed. Rationale: it is no longer consistent with the IAU specification 19. a new word "src.ephem" should be added. Rationale: it is necessary to separate "observatory" from "source" ephemeris 20. "spect.veloc" should be replaced by "src.radial.vel". Rationale: it is a property of the source, rather than of a spectrum 21. we propose to add "src.stellarityIndex". Rationale: it may be useful to easily discriminate point-like from extended sources 22. we propose to add the following words in the "stat" category: "stat.distribution", "stat.fit.model". Rationale: without them, the information on the statistical quantities and/or the fit are incomplete 23. we propose to replace "stat.moment" (as a vectorial quantity) for "stat.mean" and "stat.stdev". Any of the statistical moments could be therefore indicated by the UCD: "stat.moment; meta.rank". Rationale: the proposed method is more flexible, and could avoid the proliferation of new words to indicate skewness, kurtosis ... 24. the following words should be moved from the category "time" to "src": "time.age", "time.crossing", "time.period", "time.phase", "time.relax". E.g.: "time.age" -> "src.time.age". Rationale: they logically belong to a source rather them to the 4th dimension 25. we propose to add the following word: "time.deadtime". Rationale: useful for photon-counting devices based catalogues An additional point that we have discussed concerns the units in which interferometric data shall be provided. Is it accepted that data providers have to convert them in physical units at the server level? If not, we need probably to include specific UCD words to deal with "images" in the Fourier space. I again apologize for the long and late message. Thanks for your attention. Regards, Matteo & Ana -- Matteo Guainazzi XMM-Newton SOC Matteo.Guainazzi@sciops.esa.int European Space Astronomy Center of ESA Phone: +34 91 8131 176 VILSPA, Apartado 50727, E-28080 Madrid Fax: +34 91 8131 172 From owner-ucd-sci@eso.org Wed Jul 13 15:40:27 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 j6DDe4Q8019574 for ; Wed, 13 Jul 2005 15:40:04 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j6DDe3w6019571 for ucd-sci-outgoing; Wed, 13 Jul 2005 15:40:03 +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 j6DDduQ8019536 for ; Wed, 13 Jul 2005 15:39:56 +0200 (MEST) Received: from smtp.ucolick.org (santo.ucolick.org [128.114.23.204]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j6DDdrin012832 for ; Wed, 13 Jul 2005 15:39:54 +0200 (CEST) Received: from localhost (localhost [127.0.0.1]) by smtp.ucolick.org (Postfix) with ESMTP id 1775A5D714 for ; Wed, 13 Jul 2005 06:39:48 -0700 (PDT) Received: from geneva.ucolick.org (geneva.ucolick.org [128.114.23.183]) (using TLSv1 with cipher DHE-RSA-AES256-SHA (256/256 bits)) (No client certificate requested) by smtp.ucolick.org (Postfix) with ESMTP id ADCC111406 for ; Wed, 13 Jul 2005 06:39:47 -0700 (PDT) Received: from geneva.ucolick.org (localhost [127.0.0.1]) by geneva.ucolick.org (8.13.1/8.12.10) with ESMTP id j6DDdlDN018023 for ; Wed, 13 Jul 2005 06:39:47 -0700 Received: (from sla@localhost) by geneva.ucolick.org (8.13.1/8.13.1/Submit) id j6DDdkZU018022 for ucd-sci@ivoa.net; Wed, 13 Jul 2005 06:39:46 -0700 Date: Wed, 13 Jul 2005 06:39:46 -0700 From: Steve Allen To: ucd-sci@ivoa.net Subject: Re: Late comments (mainly) on the UCD word list Message-ID: <20050713133946.GA17964@ucolick.org> References: <42D4C698.70908@sciops.esa.int> Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii Content-Disposition: inline In-Reply-To: <42D4C698.70908@sciops.esa.int> User-Agent: Mutt/1.4.2.1i X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.2, Antispam-Data: 2005.7.13.10 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 Wed 2005-07-13T07:45:28 +0000, Matteo Guainazzi hath writ: > 20. "spect.veloc" should be replaced by "src.radial.vel". Rationale: it > is a property of the source, rather than of a spectrum This is quite contrary to the notions clearly espoused by Lindegren and Dravins (2003) A&A 401, 1185. Without a model there is no way to assign a radial velocity to a source. The measurable quantity, is a spectral shift for which any apparent radial velocity is merely conventional. That said, it remains the case that many instances of conventional radial velocity measures exist in the literature. -- Steve Allen WGS-84 (GPS) UCO/Lick Observatory Natural Sciences II, Room 165 Lat +36.99858 University of California Voice: +1 831 459 3046 Lng -122.06014 Santa Cruz, CA 95064 http://www.ucolick.org/~sla/ Hgt +250 m From owner-ucd-sci@eso.org Thu Jul 14 11:42:55 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 j6E9gnil008579 for ; Thu, 14 Jul 2005 11:42:49 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j6E9gnav008578 for ucd-sci-outgoing; Thu, 14 Jul 2005 11:42:49 +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 j6E9gjil008569 for ; Thu, 14 Jul 2005 11:42:45 +0200 (MEST) Received: from ms0.astro.physik.uni-goettingen.de (ms0.astro.physik.uni-goettingen.de [134.76.204.32]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j6E9ghhx016204 for ; Thu, 14 Jul 2005 11:42:43 +0200 (CEST) Received: from sisley.astro.physik.uni-goettingen.de ([134.76.205.209]) by ms0.astro.physik.uni-goettingen.de with esmtp (Exim 4.44) id 1Dt0El-0001dI-L4 for ucd-sci@ivoa.net; Thu, 14 Jul 2005 11:42:35 +0200 Mime-Version: 1.0 (Apple Message framework v622) In-Reply-To: <42D4C698.70908@sciops.esa.int> References: <42D4C698.70908@sciops.esa.int> Content-Type: text/plain; charset=ISO-8859-1; delsp=yes; format=flowed Message-Id: <6180f164fbf9daa4f9084e652f649cc6@astro.physik.uni-goettingen.de> From: "Frederic V. Hessman" Subject: Re: Late comments (mainly) on the UCD word list Date: Thu, 14 Jul 2005 11:45:30 +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: 2.0.3.2, Antispam-Data: 2005.7.14.2 X-Virus-Scanned: by amavisd-new Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id j6E9gmil008575 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 > 2. we propose to substitute "instr.${band}" for all words of the type > "em.${band}". Rationale: the sensitive bandpass is a property of the > detector I agree that we'll never have a complete list of useful wavelength regions, but there is still a difference between "an instrument with the bandpass of a Bessel V filter" (instr.opt.V) and "photons with wavelength corresponding to the peak of a Bessel V filter" (em.opt.V). Although I see arguments for both, I personally prefer the old form. > 4. we propose to move "instr.obsty.site.seeing" to "obs.seeing". > Rationale: this is a property of an observation rather than of an > instrument Did anyone ever respond to my suggestion of using the primary word "weather"? Seeing is only the property of an observation if used to describe image properties. If one is careful, it's not even the property of an observatory but simply part of the "weather". We need other weather words anyway, so weather.seeing weather.temp weather.humidity weather.precipitation which permits the weather generally or the "weather" inside a dome to be described. If you want the seeing within an image (which is implied by "instr.obsty.site.seeing" since it's tied to an instr), then you need things like > 9. we propose to add a further atom to the "Multiplicity of binarity > flag": "meta.code.multip.star", "meta.code.multip.planet". Rationale: > self-explaining YUK! I propose to DROP meta.code.multip ALTOGETHER : why single out this one property of objects when there are zillions of others? The other meta.codes are tolerable because they're very general and inspecific (e.g. "quality" or "class") or at the very worst boolean ("membership"). > 10. we propose to add a further "meta" atom: "meta.subexp". Rationale: > this will allow to characterize the rank of sub-exposures in a > multi-exposure observations, whenever useful for, e.g., variability > studies Sorry - another YUK! This is even worse than using src.class.distance officially only for Abell distance class. The only reasonable solution is a general-purpose hierarchy structure word: meta.pos or maybe meta.hierarch, where one can easily recognize that, e.g., the value "0" or "A" is the top level, "1" or "B" the next, etc. Then one could use this for all kinds of things. > 11. we propose to add a further "meta" atom: "meta.rank". Rationale: > useful to indicate an element in an intrinsically vectorial quantity See above. > 12. we propose to move "meta.id" and "meta.id.assoc" to "src.id" and > "src.id.assoc". Rationale: they belong to "sources" rather then to > "metadata" Only if one is applying them to sources: when applying them to other things (e.g. XML document id's), one would have a problem with src. > 13. we believe that the following "phys" word should be moved to > "src": > "phys.angArea", "phys.AngSize" (and associated words), "phys.area", > "phys.size" (and associated words). Rationale: the same as #12 above Ibid. > 14. we believe that words belonging to the following categories: > "phot", > "pos", "spec", should be placed under the category "src" (e.g.: > "phot.antennaTemp" -> "src.phot.antennaTemp", "pos.angDistance" -> > "src.pos.angDistance"; "spect.Doppler" -> "src.spect.Doppler". > Rationale: all these words ultimately describe source properties Just as you argued above to place the words appropriately, antennaTemp is DEFINITELY not a property of a src but of an obs or instr. > 15. the words for coupling of quantum numbers do not cover all the > possible coupling cases. A more general method is needed, and the Data > Line Model sub-group is indeed working on this. We propose to wait for > the conclusion of their work, before this issue is ultimately addressed > > 16. a new word "pos.offaxis" should be added. Rationale: the off-axis > angle may be a useful quantity is some catalogs A better and more general choice would be "pos.relative". > 21. we propose to add "src.stellarityIndex". Rationale: it may be > useful > to easily discriminate point-like from extended sources Too specific. The current "src.class.starGalaxy" is just as bad or worse (as if there are only stars and galaxies out there!). A MUCH better solution is "src.class.resolved". Please dump src.class.starGalaxy!!!! Finally, there are still two corrections to the descriptions to remove narrow applications of general concepts: src.morph.type | morphological type, e.g. Hubble (there are others!!!) src.morph.scLength | scale length, e.g. of disk or bulge in a galaxy (there are others!!!) src.spType | spectral type, e.g. MK (there are others!!!!) Otherwise, OK. I'm still not enthusiastic about the inconsistant use of contractions ("lg" is OK for "local group" but "sg" is not OK for "supergalactic"???), but there are obviously too many of us old people who grew up worrying about to get our data into 4k of computer memory or (like myself) wrote their disserations at home using an acoustic modem at 300 baud and so don't trust computers and networks to handle strings longer than about 8 characters. ;-) Rick ------------------------------------------------------------------------ ------------------------ NEW ADDRESS!!! ------------------------------------------------------------------------ ------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Institut für Astrophysik Tel. +49-551-39-5052 Friedrich-Hund-Platz 1 Fax +49-551-39-5043 37077 Goettingen Room F04-133 http://www.Astro.physik.Uni-Goettingen.de/~hessman ------------------------------------------------------------------------ ------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.Uni-Goettingen.de ------------------------------------------------------------------------ ------------------------- From owner-ucd-sci@eso.org Fri Jul 15 13:55:24 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 j6FBtFfJ013181 for ; Fri, 15 Jul 2005 13:55:15 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j6FBtFFf013180 for ucd-sci-outgoing; Fri, 15 Jul 2005 13:55:15 +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 j6FBt8fJ013118 for ; Fri, 15 Jul 2005 13:55:08 +0200 (MEST) Received: from smtp1.sic.rm.cnr.it (smtp1.sic.rm.cnr.it [150.146.129.253]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j6FBt5hx026567 for ; Fri, 15 Jul 2005 13:55:06 +0200 (CEST) Received: (qmail 17890 invoked by uid 508); 15 Jul 2005 11:54:59 -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 0.039559 secs); 15 Jul 2005 11:54:59 -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 ; 15 Jul 2005 11:54:59 -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 ; Fri, 15 Jul 2005 13:54:59 +0200 Message-ID: <20050715135459.s5rkrvu5rp4wcgs8@webmail.sic.rm.cnr.it> Date: Fri, 15 Jul 2005 13:54:59 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Re: Late comments (mainly) on the UCD word list References: <42D4C698.70908@sciops.esa.int> In-Reply-To: <42D4C698.70908@sciops.esa.int> 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: 2.0.3.2, Antispam-Data: 2005.7.15.8 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 > 1. we propose to remove all the words containing an explicit > specification of the wavelength or frequency range... > 2. we propose to substitute "instr.${band}" for all words of the type > "em.${band}". Rationale: the sensitive bandpass is a property of the > detector This has been a problem since the very beginning of the ucd's history. The pros and cons of different possible solutions were carefully considered, and at the end it was decided to consider that words were only a way to describe the wl/freq axis, NOT the properties of an instrument, and that the spelling was only mnemonic. The job of assigning the right em-word to a point or interval on that axis is done by a script, who takes care of units, band codes, intervals, difference of intervals (i.e.: colours in astronomy), so that, for example: 2.456mm is translated into em.mm.100-200GHz L em.IR.3-4um 0.1eV em.IR.8-15um 0.001nm em.gamma.hard V-N em.opt.V;em.IR.8-15um , and even F439W em.opt.B (Warning: the on-line script needs a quantity to assign an ucd. em-words are not, so add mag/flux... to your wl/freq/energy to get an answer) > 3. we propose to add the words "em.wl.start" and "em.wl.stop". > Rationale: they may be useful and flexible characterizations of the > bandpass In many cases I found a data/column description saying: beginning/minimum wl, ending/maximum wl, that I translated using stat.min, stat.max. On the other hand, beginning/ending of observation/exposure deserved wholly new ucd-words! So I'm in favour of introducing these concepts, but as generic qualifiers that can be applied to any axis (time, wl, freq, ..) > 4. we propose to move "instr.obsty.site.seeing" to "obs.seeing". > Rationale: this is a property of an observation rather than of an instrument I whould say seeing is a property of a . I also agree with Rick's suggestion, it's a property of the at a given site. > 5. we propose to unify "instr.beam" and "instr.det.psf" into > "instr.psf"... > 6. we propose to remove "instr.precision". Rationale: too generic, > probably useless A good occasion to repeat that the list of words was initially built entirely bottom-up, i.e. from data description. If "instr.precision" exists, it means that the description "precision", although too generic, has been used by some author. > 7. we propose to add the following radio-related words: > "instr.interferometry", and "instr.resolution". Rationale: the former is > self-explaining; the latter indicates the spatial resolution The former can be one of the many with syntax-flag S. As for the latter, at present: instrument resolution => pos.resolution image resolution => pos.resolution;obs.image spatial resolution => pos.resolution > 8. we propose to change the word code of "instr.filter.transm" and > "instr.spect.resolution" to "V". Rationale: the filter transmission is > an intrinsically vectorial quantity; the spectral resolution as well > (dependence on energy and/or order) The V-flag indicates a vector in space > 9. we propose to add a further atom to the "Multiplicity of binarity > flag": "meta.code.multip.star", "meta.code.multip.planet". Rationale: > self-explaining I think that is tolerable because it's sufficiently generic, and because it is used. > 10. we propose to add a further "meta" atom: "meta.subexp"... > 11. we propose to add a further "meta" atom: "meta.rank"... I need a use-case to make-up my mind > 12. we propose to move "xxx" to "src.xxx" > 13. as above > 14. as above > 20. as above > 24. as above In doing this, I think we would narrow the meaning of those words. > 16. a new word "pos.offaxis" should be added. Rationale: the off-axis > angle may be a useful quantity is some catalogs I agree. > 17. "pos.earth", "pos.earth.lat", "pos.earth.lon" should be placed under > the "obs" category. Rationale: these quantity belongs logically to an > observation, not to (the position of) a source I can assure you that pos.earth means position ON the earth, not source position on some earth-based coordinate frame!! > 18. "pos.earth.nutation" should be removed. Rationale: it is no longer > consistent with the IAU specification Changed. > 21. we propose to add "src.stellarityIndex". Rationale: it may be useful > to easily discriminate point-like from extended sources A word with the description ?stellarity index? already exists. > 22. we propose to add the following words in the "stat" category... > 23. Yes, I think a revision of the "stat" category is probably necessary. > 25. we propose to add the following word: "time.deadtime". Rationale: > useful for photon-counting devices based catalogues I agree. > An additional point that we have discussed concerns the units in which > interferometric data shall be provided... ?? UCDs do not care about units.. > Finally, there are still two corrections to the descriptions to > remove narrow applications of general concepts: > src.morph.type | morphological type, e.g. Hubble (there are others!!!) > src.morph.scLength | scale length, e.g. of disk or bulge in a > galaxy (there are others!!!) > src.spType | spectral type, e.g. MK (there are others!!!!) Sorry, but I did not study english at school. I studied latin. When you write: i.e. = id est, you mean: that is e.g. = exempli gratia, which means: for example (i.e., of course, there are others!!!) > I'm still not enthusiastic about the inconsistant use of contractions > ("lg" is OK for "local group" but "sg" is not OK for > "supergalactic"???), > but there are obviously too many of us old > people who grew up worrying about to get our > data into 4k of > computer memory... Indeed!!! I still feel that changing to ?supergalactic? was a terrible waste of memory!! :-) 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-sci@eso.org Fri Jul 15 17:16:19 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 j6FFGBI4000803 for ; Fri, 15 Jul 2005 17:16:11 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j6FFGBPS000802 for ucd-sci-outgoing; Fri, 15 Jul 2005 17:16:11 +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 j6FFG3I4000749 for ; Fri, 15 Jul 2005 17:16:04 +0200 (MEST) Received: from parker.sim.ucm.es (parker.sim.ucm.es [147.96.1.105]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j6FFG1hx004989 for ; Fri, 15 Jul 2005 17:16:01 +0200 (CEST) Received: from parker.sim.ucm.es (parker.sim.ucm.es [127.0.0.1]) by localhost.ucm.es (Postfix) with ESMTP id 659B32F481B for ; Fri, 15 Jul 2005 17:15:53 +0200 (CEST) Received: from ODISEO.sim.ucm.es (unknown [10.150.1.32]) by parker.sim.ucm.es (Postfix) with ESMTP id 52C082F4127 for ; Fri, 15 Jul 2005 17:15:53 +0200 (CEST) Received: from taurus.mat.ucm.es ([147.96.19.251]) by ODISEO.sim.ucm.es (Sun Java System Messaging Server 6.1 HotFix 0.11 (built Jan 28 2005)) with ESMTP id <0IJO00BPID2KED70@ODISEO.sim.ucm.es> for ucd-sci@ivoa.net; Fri, 15 Jul 2005 17:15:56 +0200 (CEST) Date: Fri, 15 Jul 2005 19:14:29 +0200 (CEST) From: Ana Ines Gomez de Castro Subject: Re: Late comments (mainly) on the UCD word list In-reply-to: <20050715135459.s5rkrvu5rp4wcgs8@webmail.sic.rm.cnr.it> To: ucd-sci@ivoa.net Message-id: 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: 2.0.3.2, Antispam-Data: 2005.7.15.13 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, On Fri, 15 Jul 2005, Andrea Preite Martinez wrote: > > > 1. we propose to remove all the words containing an explicit > > specification of the wavelength or frequency range... > > 2. we propose to substitute "instr.${band}" for all words of the type > > "em.${band}". Rationale: the sensitive bandpass is a property of the > > detector > > This has been a problem since the very beginning of the ucd's history. The > pros and cons of different possible solutions were carefully considered, > and at the end it was decided to consider that words were only a way > to describe the wl/freq axis, NOT the properties of an instrument, and that > the spelling was only mnemonic. > The job of assigning the right em-word to a point or interval on that axis > is done by a script, who takes care of units, band codes, intervals, > difference of intervals (i.e.: colours in astronomy), so that, for example: > > 2.456mm is translated into em.mm.100-200GHz > L em.IR.3-4um > 0.1eV em.IR.8-15um > 0.001nm em.gamma.hard > V-N em.opt.V;em.IR.8-15um , and even > F439W em.opt.B > > (Warning: the on-line script needs a quantity to assign an ucd. em-words are > not, so add mag/flux... to your wl/freq/energy to get an answer) > Fine! How are you planing to deal with E230M, F28x50LP, F25CN2700 "filters" or GRISM? (these are standard optical elements in HST/STIS or ACS) > > 3. we propose to add the words "em.wl.start" and "em.wl.stop". > > Rationale: they may be useful and flexible characterizations of the > > bandpass > > In many cases I found a data/column description saying: beginning/minimum > wl, ending/maximum wl, that I translated using stat.min, stat.max. On the > other hand, beginning/ending of observation/exposure deserved wholly new > ucd-words! So I'm in favour of introducing these concepts, but as generic > qualifiers that can be applied to any axis (time, wl, freq, ..) > Fine! > > 4. we propose to move "instr.obsty.site.seeing" to "obs.seeing". > > Rationale: this is a property of an observation rather than of an instrument > > I whould say seeing is a property of a . > I also agree with Rick's suggestion, it's a property of the at a > given site. Fine. Should there also be some UCD for transparency? > > > 5. we propose to unify "instr.beam" and "instr.det.psf" into > > "instr.psf"... > > 6. we propose to remove "instr.precision". Rationale: too generic, > > probably useless > > A good occasion to repeat that the list of words was initially built > entirely bottom-up, i.e. from data description. If "instr.precision" > exists, it means that the description "precision", although too generic, > has been used by some author. > Could you ask the author what did he mean? > > 7. we propose to add the following radio-related words: > > "instr.interferometry", and "instr.resolution". Rationale: the former is > > self-explaining; the latter indicates the spatial resolution > > The former can be one of the many with syntax-flag S. > As for the latter, at present: > instrument resolution => pos.resolution > image resolution => pos.resolution;obs.image > spatial resolution => pos.resolution > > > 8. we propose to change the word code of "instr.filter.transm" and > > "instr.spect.resolution" to "V". Rationale: the filter transmission is > > an intrinsically vectorial quantity; the spectral resolution as well > > (dependence on energy and/or order) > > The V-flag indicates a vector in space > At the very first AVO meeting organized by Piero in Garching there was a long discussion about this issue. To fully understand the meaning of an image obtained with a given filter you need the Transmittance function of the filter ( T(lambda) ). Unless you force all the observatories to use exactly the same filters and qualify them, specifying the transmittance function is the easiest way to qualify them and allow proper comparisons between observations obtained with different instruments. Are "functions" allowed as UCDs > > 9. we propose to add a further atom to the "Multiplicity of binarity > > flag": "meta.code.multip.star", "meta.code.multip.planet". Rationale: > > self-explaining > > I think that is tolerable because it's sufficiently > generic, and because it is used. In the coming years, planets are going to be searched for in basically all stars around. There will be searched for not only on "single" star systems but on multiple systems. How are you planing to classify them? > > > 10. we propose to add a further "meta" atom: "meta.subexp"... > > 11. we propose to add a further "meta" atom: "meta.rank"... > HST is divides the exposure time into subexposures. For each sub-exposure an "image" is produced and archived within a single "archive record" that corresponds to the "exposure". In rapidly variable objects, it is relevant to make use of the "sub-exposures". If you wish to see a direct application where this relevance is oustanding take a glance to Gomez de Castro, 2002 (MNRAS). The target is AB Dor and the spectra where obtained with HST/HRS. > I need a use-case to make-up my mind > > > 12. we propose to move "xxx" to "src.xxx" > > 13. as above > > 14. as above > > 20. as above > > 24. as above I think that they are self-explanatory > > In doing this, I think we would narrow the meaning of those words. > Why? > > 16. a new word "pos.offaxis" should be added. Rationale: the off-axis > > angle may be a useful quantity is some catalogs > I agree. > > > 17. "pos.earth", "pos.earth.lat", "pos.earth.lon" should be placed under > > the "obs" category. Rationale: these quantity belongs logically to an > > observation, not to (the position of) a source > > I can assure you that pos.earth means position ON the earth, not source > position on some earth-based coordinate frame!! Then, why are them within the "pos" category? I thought that "pos" is related with "source" and "obs" with the observation/observatory. Doesn't it look more natural, obs.pos.earth.lat? > > > 18. "pos.earth.nutation" should be removed. Rationale: it is no longer > > consistent with the IAU specification > Changed. > > > 21. we propose to add "src.stellarityIndex". Rationale: it may be useful > > to easily discriminate point-like from extended sources > > A word with the description ?stellarity index? already exists. > > > 22. we propose to add the following words in the "stat" category... > > 23. > > Yes, I think a revision of the "stat" category is probably necessary. > > > 25. we propose to add the following word: "time.deadtime". Rationale: > > useful for photon-counting devices based catalogues > I agree. > > > An additional point that we have discussed concerns the units in which > > interferometric data shall be provided... Matteo and I were dicussing about how interferometric data were going to be provided to VO's from the observatories. Interferometric data are basically images in the "Fourier space" and not in the "physical space". During the AVO experience, Joddrell Bank provided directly "physical images" since they carried out the Inverse Fourier Tranform before given access to the data through the web. So, our question is a generic issue. Interferometric data are going to become more and more common in Astronomy. The "measuring space" of interferometric data is the "Fourier- I mean , space frequencies - space". Are the interferometric data providers going to release their products in the "physical" or in the "Fourier" space? Has this issue be discussed?, has been discussed how does it affect UCD's? Finally, I've kept thinking about UCD's for "simulations" and this is very tricky. As important as the method, resolution, time-scales etcc. is to describe the boundary and the initial conditions. I still wonder how!!! Cheers, Ana Prof. Ana I. Gomez de Castro Instituto de Astronomia y Geodesia (CSIC-UCM) Fac. de CC Matematicas Universidad Complutense de Madrid 28040 Madrid, Spain Ph. 34-913944578 (office) 34-659783338 (mobile) Email: aig@mat.ucm.es From owner-ucd-sci@eso.org Fri Jul 15 17:42:38 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 j6FFgTI4005849 for ; Fri, 15 Jul 2005 17:42:29 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j6FFgTej005848 for ucd-sci-outgoing; Fri, 15 Jul 2005 17:42:29 +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 j6FFgMI4005806 for ; Fri, 15 Jul 2005 17:42:23 +0200 (MEST) Received: from fed1rmmtao02.cox.net (fed1rmmtao02.cox.net [68.230.241.37]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j6FFgJin008373 for ; Fri, 15 Jul 2005 17:42:20 +0200 (CEST) Received: from [10.0.1.21] (really [68.231.133.145]) by fed1rmmtao02.cox.net (InterMail vM.6.01.04.00 201-2131-118-20041027) with ESMTP id <20050715154206.XYID22430.fed1rmmtao02.cox.net@[10.0.1.21]>; Fri, 15 Jul 2005 11:42:06 -0400 In-Reply-To: <20050715135459.s5rkrvu5rp4wcgs8@webmail.sic.rm.cnr.it> References: <42D4C698.70908@sciops.esa.int> <20050715135459.s5rkrvu5rp4wcgs8@webmail.sic.rm.cnr.it> Mime-Version: 1.0 (Apple Message framework v730) Content-Type: multipart/alternative; boundary=Apple-Mail-18--746470585 Message-Id: <6A441722-CBE8-42C9-AE85-9EAD58AD711D@noao.edu> From: Rob Seaman Subject: Re: Late comments (mainly) on the UCD word list Date: Fri, 15 Jul 2005 08:42:13 -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: 2.0.3.2, Antispam-Data: 2005.7.15.13 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 --Apple-Mail-18--746470585 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed On Jul 15, 2005, at 4:54 AM, Andrea Preite Martinez wrote: > I whould say seeing is a property of a . > I also agree with Rick's suggestion, it's a property of the > at a > given site. For any given tabular example, the concept of "seeing" likely includes effects local to the dome and telescope, which often dominate the resulting measured PSF, independent of the theoretical diffraction limit of the telescope. Rarely will seeing strictly derived from the weather be measured or recorded. > A good occasion to repeat that the list of words was initially built > entirely bottom-up, i.e. from data description. If "instr.precision" > exists, it means that the description "precision", although too > generic, > has been used by some author. This is a good way to build such a list. It is not the only way one might proceed. If namespaces (or the potential for same) are not introduced early in the process, there will be much more trouble later when the VO inevitably finds some way to squeeze them in. > I need a use-case to make-up my mind A single use-case is not much point. The idea is to assemble a range of use-cases such that all the potential behaviors of the system or model are elucidated. > ?? UCDs do not care about units.. Indeed, but sometimes a preference is implicit. Seeing is likely in arcseconds, dates are likely ISO 8601, and so forth. Rob Seaman NOAO --Apple-Mail-18--746470585 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1
On Jul 15, 2005, at = 4:54 AM, Andrea Preite Martinez wrote:

I whould say seeing is a property of a = <site>.
I also agree with Rick's = suggestion, it's a property of the <weather> at a
given site.

For any given tabular = example, the concept of "seeing" likely includes effects local to the = dome and telescope, which often dominate the resulting measured PSF, = independent of the theoretical diffraction limit of the telescope.=A0 = Rarely will seeing strictly derived from the weather be measured or = recorded.

A good = occasion to repeat that the list of words was initially built
entirely bottom-up, i.e. from data description. If = "instr.precision"
exists, it means that the = description "precision", although too generic,
has been used by some = author.

This is a good way to build such = a list.=A0 It is not the only way one might proceed.=A0 If namespaces = (or the potential for same) are not introduced early in the process, = there will be much more trouble later when the VO inevitably finds some = way to squeeze them in.

I need a use-case to make-up my = mind

A = single use-case is not much point.=A0 The idea is to assemble a range of = use-cases such that all the potential behaviors of the system or model = are elucidated.

?? UCDs do not care about = units..

Indeed, but sometimes a = preference is implicit.=A0 Seeing is likely in arcseconds, dates are = likely ISO 8601, and so forth.

Rob = Seaman
NOAO
= --Apple-Mail-18--746470585-- From owner-ucd-sci@eso.org Fri Jul 15 18:33:22 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 j6FGXEI4014929 for ; Fri, 15 Jul 2005 18:33:14 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j6FGXE1Z014928 for ucd-sci-outgoing; Fri, 15 Jul 2005 18:33:14 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-sci@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 j6FGXAI4014922 for ; Fri, 15 Jul 2005 18:33:10 +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 j6FGXAE28712 for ; Fri, 15 Jul 2005 18:33:10 +0200 (MEST) Mime-Version: 1.0 (Apple Message framework v622) In-Reply-To: <42D4C698.70908@sciops.esa.int> References: <42D4C698.70908@sciops.esa.int> Content-Type: text/plain; charset=US-ASCII; format=flowed Message-Id: <0c98fa388c24f6627eccd21e02333daf@eso.org> Content-Transfer-Encoding: 7bit From: Alberto Micol Subject: What is that a UCD can be assigned to? Date: Fri, 15 Jul 2005 18:33:09 +0200 To: ucd-sci@ivoa.net X-Mailer: Apple Mail (2.622) 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 Dear All, I'm trying to catch up with UCDs, sorry to be so late. Matteo's and Ana's comments, plus my own way of reading the list of words, and especially the comments associated with each word, make me think that something is not yet properly defined, and that some ambiguity is still to be removed. While historically UCDs were assigned to *columns* in the Vizier collection of tables, I wonder if this is still true. That is, I cannot find in any document of the UCD1+ the answer to the question: What is that a UCD can be assigned to? I know that it CAN be assigned to a scalar quantity; I know that it CAN be assigned to a column in a table; but CAN it be assigned to an image, to a table, or any other piece of Astronomical Data? I cannot find the answer in any recent UCD-related document (correct me if wrong). I think we need to fill this gap, and give a clear answer. The answer can be: NO --- If the answer is that a UCD can NOT be assigned to anything else than a scalar quantity or an array of identical quantities (i.e., the column in a table), then I do not see why we should have a UCD like instr.interferometry (Thanks Matteo for the good example) YES --- If, at the contrary, UCDs can be assigned to generic, however complicated, data structures then instr.interferometry becomes a nice UCD (though I would suggest data.interferometry instead). Furthermore, if UCDs can be assigned to complex data structures then suddenly I can make sense of other UCDs (like instr.filter.transm) which are currently defined in an ambiguous way: > instr.filter.transm | Filter transmission Is it for a typical value of the transmission of my filter (e.g. 0.2)? or Does it refer to the entire array that represents the "transmission curve" ? On the other hand, if the answer is YES, then a table could have its own UCDs, (and in that case the VOTable standard will need a revision to support UCDs at the table level). But I think that the answer is NO, because otherwise the vocabulary would need to explode and include all kind of things. Hence, if the answer is NO, then I would suggest to make the comments a bit more strict to avoid confusion. A couple of examples: Current Description Possibly less ambiguous description ------------------- ----------------------------------------- Filter transmission -> Typical value for the filter transmission Spectral resolution -> Typical value of the spectral resolution Resolution -> Typical value of the angular resolution Spectral line -> Common name of the spectral line Detector -> Name of the detector Photographic Plate -> Type of emulsion etc. etc. Alberto PS: Did I get the right answer? Menace: Many more comments to come (e.g. UCDs for Characterisation DM, etc.), hopefully next week. From owner-ucd-sci@eso.org Tue Jul 19 14:10:03 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 j6JC9ttR016558 for ; Tue, 19 Jul 2005 14:09:56 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j6JC9t1m016557 for ucd-sci-outgoing; Tue, 19 Jul 2005 14:09:55 +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 j6JC9mtR016547 for ; Tue, 19 Jul 2005 14:09:48 +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 j6JC9kin024405 for ; Tue, 19 Jul 2005 14:09:46 +0200 (CEST) Received: from argiope.saclay.cea.fr (argiope.saclay.cea.fr [132.166.192.108]) by cirse.extra.cea.fr (8.13.4/8.13.4/CEAnet-Internet.5.0) with ESMTP id j6JC9a1Z018301 for ; Tue, 19 Jul 2005 14:09:36 +0200 (MEST) Received: from pisaure.intra.cea.fr (unverified) by argiope.saclay.cea.fr (Content Technologies SMTPRS 4.3.17) with ESMTP id for ; Tue, 19 Jul 2005 14:09:36 +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 j6JC85fx008638 for ; Tue, 19 Jul 2005 14:08:05 +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 j6JC9Zs5016897 for ; Tue, 19 Jul 2005 14:09:35 +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 j6JC9fbh021016 for ; Tue, 19 Jul 2005 14:09:42 +0200 (MEST) Message-ID: <42DCED7E.3010008@cea.fr> Date: Tue, 19 Jul 2005 14:09:34 +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: ucd-sci@ivoa.net Subject: Re: Late comments (mainly) on the UCD word list 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: 2.0.3.2, Antispam-Data: 2005.7.19.8 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, some comments related to DM ... ;-) SY, Pierre Ana Ines Gomez de Castro wrote: > Hi, > > On Fri, 15 Jul 2005, Andrea Preite Martinez wrote: > > >>>3. we propose to add the words "em.wl.start" and "em.wl.stop". >>>Rationale: they may be useful and flexible characterizations of the >>>bandpass >> >>In many cases I found a data/column description saying: beginning/minimum >>wl, ending/maximum wl, that I translated using stat.min, stat.max. On the >>other hand, beginning/ending of observation/exposure deserved wholly new >>ucd-words! So I'm in favour of introducing these concepts, but as generic >>qualifiers that can be applied to any axis (time, wl, freq, ..) >> > > > > Fine! > > ... >>>8. we propose to change the word code of "instr.filter.transm" and >>>"instr.spect.resolution" to "V". Rationale: the filter transmission is >>>an intrinsically vectorial quantity; the spectral resolution as well >>>(dependence on energy and/or order) >> >>The V-flag indicates a vector in space >> > > > At the very first AVO meeting organized by Piero in Garching there was > a long discussion about this issue. To fully understand the meaning of > an image obtained with a given filter you need the Transmittance > function of the filter ( T(lambda) ). Unless you force all the > observatories to use exactly the same filters and qualify them, > specifying the transmittance function is the easiest way to qualify > them and allow proper comparisons between observations obtained > with different instruments. Are "functions" allowed as UCDs > It is may be more related to DM dealing with characterization http://alinda.u-strasbg.fr/Model/Characterisation/DM_vers0.1/ to "fully" describe metadata conserning an observation, including filters and theirs properties... http://alinda.u-strasbg.fr/Model/Characterisation/DM_vers0.1/3771728084_130.html UCD is perhaps to general/generic to be complete? >> >>>17. "pos.earth", "pos.earth.lat", "pos.earth.lon" should be placed under >>>the "obs" category. Rationale: these quantity belongs logically to an >>>observation, not to (the position of) a source >> >>I can assure you that pos.earth means position ON the earth, not source >>position on some earth-based coordinate frame!! > > > Then, why are them within the "pos" category? I thought that "pos" is > related with "source" and "obs" with the observation/observatory. > Doesn't it look more natural, obs.pos.earth.lat? > but pos.earth.lat or pos.earth.* can perhaps be related to something else than observation? >> >> >>>An additional point that we have discussed concerns the units in which >>>interferometric data shall be provided... > > > Matteo and I were dicussing about how interferometric data were > going to be provided to VO's from the observatories. Interferometric > data are basically images in the "Fourier space" and not in the > "physical space". During the AVO experience, Joddrell Bank > provided directly "physical images" since they carried out > the Inverse Fourier Tranform before given access to the data > through the web. So, our question is a generic issue. > > Interferometric data are going to become more and more > common in Astronomy. The "measuring space" of interferometric > data is the "Fourier- I mean , space frequencies - space". > Are the interferometric data providers going to release their > products in the "physical" or in the "Fourier" space? > Has this issue be discussed?, has been discussed how does > it affect UCD's? What UCD did you forsee to be able to describe more precisely interferometry data. DM group working on characterization would certainly be interested also by this topic. > > > Finally, I've kept thinking about UCD's for "simulations" > and this is very tricky. As important as the method, > resolution, time-scales etcc. is to describe the > boundary and the initial conditions. I still wonder how!!! > > > Cheers, > > Ana > > > Prof. Ana I. Gomez de Castro > Instituto de Astronomia y Geodesia (CSIC-UCM) > Fac. de CC Matematicas > Universidad Complutense de Madrid > 28040 Madrid, Spain > > Ph. 34-913944578 (office) 34-659783338 (mobile) > Email: aig@mat.ucm.es > > -- 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/ ------------------------------------------------------------------ La carte n'est pas le territoire - Alfred KORZYBSKI ------------------------------------------------------------------ From owner-ucd-sci@eso.org Tue Jul 19 14:39:07 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 j6JCcwtR022701 for ; Tue, 19 Jul 2005 14:38:58 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j6JCcwV7022700 for ucd-sci-outgoing; Tue, 19 Jul 2005 14:38:58 +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 j6JCcotR022674 for ; Tue, 19 Jul 2005 14:38:50 +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 j6JCcmin025397 for ; Tue, 19 Jul 2005 14:38:48 +0200 (CEST) Received: from argiope.saclay.cea.fr (argiope.saclay.cea.fr [132.166.192.108]) by cirse.extra.cea.fr (8.13.4/8.13.4/CEAnet-Internet.5.0) with ESMTP id j6JCcgxY008379 for ; Tue, 19 Jul 2005 14:38:42 +0200 (MEST) Received: from pisaure.intra.cea.fr (unverified) by argiope.saclay.cea.fr (Content Technologies SMTPRS 4.3.17) with ESMTP id for ; Tue, 19 Jul 2005 14:38:42 +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 j6JCbBJ6013713 for ; Tue, 19 Jul 2005 14:37:11 +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 j6JCcfs5003984 for ; Tue, 19 Jul 2005 14:38:41 +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 j6JCcmbh021761 for ; Tue, 19 Jul 2005 14:38:48 +0200 (MEST) Message-ID: <42DCF450.8090709@cea.fr> Date: Tue, 19 Jul 2005 14:38:40 +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: ucd-sci@ivoa.net Subject: Re: What is that a UCD can be assigned to? References: <42D4C698.70908@sciops.esa.int> <0c98fa388c24f6627eccd21e02333daf@eso.org> In-Reply-To: <0c98fa388c24f6627eccd21e02333daf@eso.org> 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: 2.0.3.2, Antispam-Data: 2005.7.19.8 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 Alberto Micol wrote: > > Dear All, > > I'm trying to catch up with UCDs, sorry to be so late. > > Matteo's and Ana's comments, plus my own way of reading the list of words, > and especially the comments associated with each word, make me think that > something is not yet properly defined, and that some ambiguity is still > to be removed. > > While historically UCDs were assigned to *columns* in the Vizier > collection of tables, > I wonder if this is still true. That is, I cannot find in any document > of the UCD1+ > the answer to the question: > > What is that a UCD can be assigned to? > > I know that it CAN be assigned to a scalar quantity; > I know that it CAN be assigned to a column in a table; > > but > > CAN it be assigned to an image, to a table, or any other piece of > Astronomical Data? > > I cannot find the answer in any recent UCD-related document (correct me > if wrong). > I think we need to fill this gap, and give a clear answer. > > The answer can be: > > NO > --- > If the answer is that a UCD can NOT be assigned to anything else than a > scalar quantity > or an array of identical quantities (i.e., the column in a table), > then I do not see why we should have a UCD like instr.interferometry > (Thanks Matteo for the good example) > > > YES > --- > If, at the contrary, UCDs can be assigned to generic, however > complicated, data structures > then instr.interferometry becomes a nice UCD (though I would suggest > data.interferometry instead). > > Furthermore, if UCDs can be assigned to complex data structures then > suddenly I can make sense of other UCDs (like instr.filter.transm) > which are currently defined in an ambiguous way: > > > instr.filter.transm | Filter transmission > > Is it for a typical value of the transmission of my filter (e.g. 0.2)? > or > Does it refer to the entire array that represents the "transmission > curve" ? May be it can be both, depending of the context and the data decribed? But transmission curve is certainly more precisely described by SED-DM, and in this context why not associating this structure with such an UCD? > > On the other hand, if the answer is YES, then a table could have its own > UCDs, > (and in that case the VOTable standard will need a revision to support > UCDs at the table level). It is the only "special" case where ucd are allowed aside column (FIELD) or "individual" (which can contain an array nevertheless) quantity (PARAM), not speaking of column or quantity grouping (GROUP) ;-) > > > But I think that the answer is NO, because otherwise the vocabulary > would need to explode > and include all kind of things. > Hence, if the answer is NO, then I would suggest to make the comments a > bit more strict > to avoid confusion. It is perhaps neither YES nor NO. Actually the main usage is still column characterization but who can forsee all possible usefull usage... and/or try to forbid it? > A couple of examples: > > Current Description Possibly less ambiguous description > ------------------- ----------------------------------------- > Filter transmission -> Typical value for the filter transmission > Spectral resolution -> Typical value of the spectral resolution > Resolution -> Typical value of the angular resolution > Spectral line -> Common name of the spectral line > Detector -> Name of the detector > Photographic Plate -> Type of emulsion > etc. etc. > > Alberto Friendly, Pierre From owner-ucd-sci@eso.org Wed Jul 27 17:58:14 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 j6RFw8SB008272 for ; Wed, 27 Jul 2005 17:58:08 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j6RFw89M008271 for ucd-sci-outgoing; Wed, 27 Jul 2005 17:58:08 +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 j6RFvwSB008229 for ; Wed, 27 Jul 2005 17:57:58 +0200 (MEST) Received: from ms0.astro.physik.uni-goettingen.de (ms0.astro.physik.uni-goettingen.de [134.76.204.32]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j6RFvuin012091 for ; Wed, 27 Jul 2005 17:57:56 +0200 (CEST) Received: from sisley.astro.physik.uni-goettingen.de ([134.76.205.209]) by ms0.astro.physik.uni-goettingen.de with esmtp (Exim 4.44) id 1DxoI3-0000sa-Ae for ucd-sci@ivoa.net; Wed, 27 Jul 2005 17:57:51 +0200 Mime-Version: 1.0 (Apple Message framework v622) In-Reply-To: <20050715135459.s5rkrvu5rp4wcgs8@webmail.sic.rm.cnr.it> References: <42D4C698.70908@sciops.esa.int> <20050715135459.s5rkrvu5rp4wcgs8@webmail.sic.rm.cnr.it> Content-Type: text/plain; charset=ISO-8859-1; delsp=yes; format=flowed Message-Id: <94beff6f1861cfe20667d9677887ac38@astro.physik.uni-goettingen.de> From: "Frederic V. Hessman" Subject: Re: Late comments (mainly) on the UCD word list Date: Mon, 25 Jul 2005 19:02:32 +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: 2.0.3.2, Antispam-Data: 2005.7.27.16 X-Virus-Scanned: by amavisd-new Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id j6RFw8SB008267 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 >> 16. a new word "pos.offaxis" should be added. Rationale: the off-axis >> angle may be a useful quantity is some catalogs > I agree. But "pos.relative" is much more general and just as good for this particular use. >> 21. we propose to add "src.stellarityIndex". Rationale: it may be >> useful >> to easily discriminate point-like from extended sources > > A word with the description ?stellarity index? already exists. Yes, but "src.starGalaxy" is obviously not general enough for a galactic nebular catalogue: is the value in the table indicating that the object is a star, a non-stellar nebula, or really a galaxy? Thus: "src.pointlike" or "src.resolved" ! >> Finally, there are still two corrections to the descriptions to >> remove narrow applications of general concepts: >> src.morph.type | morphological type, e.g. Hubble (there are >> others!!!) >> src.morph.scLength | scale length, e.g. of disk or bulge in a >> galaxy (there are others!!!) >> src.spType | spectral type, e.g. MK (there are others!!!!) > > Sorry, but I did not study english at school. I studied latin. > When you write: > i.e. = id est, you mean: that is > e.g. = exempli gratia, which means: for example (i.e., of course, > there are > others!!!) Sorry - I obviously meant for you to edit out the "(there are others!!!)" but didn't say so. >> I'm still not enthusiastic about the inconsistant use of contractions >> ("lg" is OK for "local group" but "sg" is not OK for >> "supergalactic"???), > but there are obviously too many of us old >> people who grew up worrying about to get our > data into 4k of >> computer memory... > > Indeed!!! I still feel that changing to ?supergalactic? was a terrible > waste of memory!! :-) XML is a waste of memory in any case, but the point is that it doesn't matter. We're talking about a 5% effect in the size of documents - it's a waste of time to even think about it, so one might as well be explicit. Rick ------------------------------------------------------------------------ ------------------------ NEW ADDRESS!!! ------------------------------------------------------------------------ ------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Institut für Astrophysik Tel. +49-551-39-5052 Friedrich-Hund-Platz 1 Fax +49-551-39-5043 37077 Goettingen Room F04-133 http://www.Astro.physik.Uni-Goettingen.de/~hessman ------------------------------------------------------------------------ ------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.Uni-Goettingen.de ------------------------------------------------------------------------ ------------------------- From owner-ucd-sci@eso.org Wed Sep 28 17:05:47 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 j8SF5dYK001535 for ; Wed, 28 Sep 2005 17:05:39 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j8SF5dvt001534 for ucd-sci-outgoing; Wed, 28 Sep 2005 17:05:39 +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 j8SF5EYK001293; Wed, 28 Sep 2005 17:05:14 +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 j8SF5Chx004462; Wed, 28 Sep 2005 17:05:12 +0200 (CEST) Received: from localhost (localhost.localdomain [127.0.0.1]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP id 93B63C74A8; Wed, 28 Sep 2005 17:05:03 +0200 (CEST) Received: from smtp1.sic.rm.cnr.it ([127.0.0.1]) by localhost (smtp1 [127.0.0.1]) (amavisd-new, port 10023) with ESMTP id 00562-09; Wed, 28 Sep 2005 17:05:02 +0200 (CEST) Received: from localhost (unknown [10.1.0.7]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP; Wed, 28 Sep 2005 17:05:02 +0200 (CEST) Received: from martinez.u-strasbg.fr (martinez.u-strasbg.fr [130.79.129.134]) by webmail.sic.rm.cnr.it (Horde) with HTTP for ; Wed, 28 Sep 2005 17:05:02 +0200 Message-ID: <20050928170502.cr5855mfvtwk004o@webmail.sic.rm.cnr.it> Date: Wed, 28 Sep 2005 17:05:02 +0200 From: Andrea Preite Martinez To: ucd@ivoa.net Cc: ucd-sci@ivoa.net Subject: Call for contributions 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-Virus-Scanned: by amavisd-new X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.2, Antispam-Data: 2005.9.28.6 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 (This message is sent to the UCD and UCD-sci lists: I?m sorry, some of you will receive it twice!) Dear All, The InterOp meeting is approaching, and there is still ample room for contribution in the Agenda of the UCD session. For the moment I envisage to shortly describe the current status of UCDs and open a discussion on future perspectives. Between the present situation and the future development of ontology, I think there is the need for an intermediate step. Up to now, with the "first generation" UCDs, we tackled the problem of describing mainly "quantities" appearing in table data, with the addition of various flavours of qualifiers and modifiers. On the other hand there is an increasing need to describe other concepts within a semantic scheme unique and agreed upon by the whole community. Elements of data models or object types and phenomena of "events" are typical examples of what we might want to integrate in a "second generation" UCDs. We should keep in mind that we need to go any way through this intermediate step in order to build the ontology. By the way, this is the reason why we asked in Kyoto to add "semantics" to the name of the working group. I think it is time to discuss how to build the second generation of UCDs. Some of you already proposed ucd-words of this kind during the recent discussion on the ucd vocabulary. Next UCD session is the right place to restart the discussion. If you want to contribute, send me a title and the time required in order to update the agenda of the session. Andrea ============================================================================== Andrea Preite Martinez andrea.preitemartinez@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 CDS :+33.3.90242473 ============================================================================== From owner-ucd-sci@eso.org Wed Sep 28 18:42:31 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 j8SGgLYK019986 for ; Wed, 28 Sep 2005 18:42:21 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j8SGgLlj019985 for ucd-sci-outgoing; Wed, 28 Sep 2005 18:42:21 +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 j8SGgEYK019970; Wed, 28 Sep 2005 18:42:15 +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 j8SGgBhx008485; Wed, 28 Sep 2005 18:42:12 +0200 (CEST) X-Spam-Checker-Version: SpamAssassin 3.1.0 (2005-09-13) on noao.edu X-Spam-Level: X-Spam-Status: No, score=-4.8 required=4.5 tests=ALL_TRUSTED,AWL,BAYES_00, HTML_40_50,HTML_MESSAGE autolearn=ham version=3.1.0 X-TFF-CGPSA-Version: 1.4f1 X-TFF-CGPSA-Filter: Scanned Received: from [140.252.18.64] (account seaman HELO [140.252.18.64]) by noao.edu (CommuniGate Pro SMTP 4.3.8) with ESMTPSA id 20727546; Wed, 28 Sep 2005 09:42:03 -0700 In-Reply-To: <20050928170502.cr5855mfvtwk004o@webmail.sic.rm.cnr.it> References: <20050928170502.cr5855mfvtwk004o@webmail.sic.rm.cnr.it> Mime-Version: 1.0 (Apple Message framework v734) Content-Type: multipart/alternative; boundary=Apple-Mail-82--705330383 Message-Id: Cc: ucd@ivoa.net From: Rob Seaman Subject: Re: Call for contributions Date: Wed, 28 Sep 2005 09:42:04 -0700 To: ucd-sci@ivoa.net X-Mailer: Apple Mail (2.734) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.2, Antispam-Data: 2005.9.28.8 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 --Apple-Mail-82--705330383 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed On Sep 28, 2005, at 8:05 AM, Andrea Preite Martinez wrote: > Elements of data models or object types and phenomena of "events" > are typical examples of what we might want to integrate in a > "second generation" UCDs. Yes, indeed. I think we can all reach agreement on such things. > On the other hand there is an increasing need to describe other > concepts within a semantic scheme unique and agreed upon by the > whole community. No, not at all. A single, unique UCD namespace will never satisfy all requirements and all users. The current UCD effort has produced a worthy product. The way to protect the investment in the current UCDs, as well as to support the development of new classes of UCDs, is to recognize just that - that "VOConcepts" and other future DM specific UCDs represent separate classes of UCDs - separate namespaces. UCDs are not XML, but the concept of a purpose specific namespace is larger than either. We cannot possibly afford to wait for agreement from the whole community for every single UCD that is proposed. The solution is to recognize that UCDs live in multiple lists managed by multiple authorities, i.e., they live in namespaces (whether or not we call them that). And bear in mind that as the VO matures, the community in question will become the larger astronomy and physics (and geoscience and planetary science and exobiology and...) community, not just the current cozy coffee klatch. Terminology will inevitably collide. We should allow for that now, rather than address each name collision as some ad hoc shoehorning of concepts into nomenclature that fits badly or not at all. > We should keep in mind that we need to go any way through this > intermediate step in order to build the ontology. Yes and no. Yes this is the correct path to follow. No, I am skeptical that a single universe-girdling ontology will emerge at the end of the day. If the VO semantic efforts fail, it will be due to over-reaching and over-generalization. We need to define a process for building separate, project and purpose specific, ontologies (plural). Rob Seaman NOAO --Apple-Mail-82--705330383 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1
On Sep 28, 2005, at = 8:05 AM, Andrea Preite Martinez wrote:

Elements of data models or object types and phenomena = of "events" are=A0typical examples of what we might want to integrate in = a "second=A0generation" UCDs.

Yes, indeed.=A0 I think we can = all reach agreement on such things.

On the other hand there is an increasing need to = describe other concepts=A0within a semantic scheme unique and agreed = upon by the whole community.

No, not at = all.=A0 A single, unique UCD namespace will never satisfy all = requirements and all users.=A0 The current UCD effort has produced a = worthy product.=A0 The way to protect the investment in the current = UCDs, as well as to support the development of new classes of UCDs, is = to recognize just that - that "VOConcepts" and other future DM specific = UCDs represent separate classes of UCDs - separate = namespaces.

UCDs are not XML, but the = concept of a purpose specific namespace is larger than either.=A0 We = cannot possibly afford to wait for agreement from the whole community = for every single UCD that is proposed.=A0 The solution is to recognize = that UCDs live in multiple lists managed by multiple authorities, i.e., = they live in namespaces (whether or not we call them = that).

And = bear in mind that as the VO matures, the community in question will = become the larger astronomy and physics (and geoscience and planetary = science and exobiology and...) community, not just the current cozy = coffee klatch.=A0 Terminology will inevitably collide.=A0 We should = allow for that now, rather than address each name collision as some ad = hoc shoehorning of concepts into nomenclature that fits badly or not at = all.

We = should keep in mind that we need to go any way through this = intermediate=A0step in order to build the = ontology.

Yes and no.=A0 = Yes this is the correct path to follow.=A0 No, I am skeptical that a = single universe-girdling ontology will emerge at the end of the day.=A0 = If the VO semantic efforts fail, it will be due to over-reaching and = over-generalization.=A0 We need to define a process for building = separate, project and purpose specific, ontologies (plural).

Rob Seaman
= --Apple-Mail-3--1004063097-- From owner-ucd-sci@eso.org Tue Jul 25 11:26:57 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6P9QoAT023463 for ; Tue, 25 Jul 2006 11:26:50 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6P9Qo9c023462 for ucd-sci-outgoing; Tue, 25 Jul 2006 11:26:50 +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 (8.13.6+Sun/8.12.10) with ESMTP id k6P9QhjM023447 for ; Tue, 25 Jul 2006 11:26:43 +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 k6P9QeLY012743 for ; Tue, 25 Jul 2006 11:26:41 +0200 (CEST) Received: from localhost (smtp1 [127.0.0.1]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP id CA7101DA2D8; Tue, 25 Jul 2006 11:26:34 +0200 (CEST) X-Virus-Scanned: by amavisd-new Received: from smtp1.sic.rm.cnr.it ([127.0.0.1]) by localhost (smtp1.sic.rm.cnr.it [127.0.0.1]) (amavisd-new, port 10023) with ESMTP id TKrWNWDpf2vy; Tue, 25 Jul 2006 11:26:34 +0200 (CEST) Received: from localhost (unknown [10.1.2.2]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP; Tue, 25 Jul 2006 11:26:34 +0200 (CEST) Received: from martinez.u-strasbg.fr (martinez.u-strasbg.fr [130.79.129.134]) by webmail.sic.rm.cnr.it (Horde MIME library) with HTTP; Tue, 25 Jul 2006 11:26:34 +0200 Message-ID: <20060725112634.oz0z4tjnk4swk8kg@webmail.sic.rm.cnr.it> Date: Tue, 25 Jul 2006 11:26:34 +0200 From: Andrea Preite Martinez To: Nausicaa Delmotte Cc: ucd-sci@ivoa.net Subject: Re: observation proposal and name of the observer References: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> <44BB83C3.3010702@eso.org> In-Reply-To: <44BB83C3.3010702@eso.org> MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1; DelSp="Yes"; format="flowed" Content-Disposition: inline User-Agent: Internet Messaging Program (IMP) H3 (4.1.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.7.25.13432 Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id k6P9QnjM023457 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Andrea Preite Martinez Quoting Nausicaa Delmotte : > - What is the difference between 'title of an observation proposal' > and 'name of an observation proposal'? > > So far I would not have expected any difference but with the introduction > of the new UCD word obs.proposal, it seems it is possible to construct both > meta.title;obs.proposal > and > meta.id;obs.proposal > > Maybe someone could provide an example, in case there is a difference > of meaning > between those two UCDs? I just cannot see the difference... (given > that the proposal > code is already defined by meta.code;obs.proposal). > Don't forget catalogues! According to the Catalogue DM, a catalogue can have: - a name (in the description text)/a title (in the XML schema) - an identifier - a shortName My point of view: - The title of XYZ is a string describing the content of XYZ, as in a scientific paper (actually this is the origin of the ucd); - the name/identifier is a string uniquely identifying XYZ, as for humans (e.g.: Andrea Preite Martinez is my name/identifier); - a short name for me could be APM (and my "code" could be my social security number!). I don't see the difference between name and identifier. Another point is that a "possible" ucd is not necessarily a "good" ucd!! > By the way, what about the 'abstract of the observation proposal'? > meta.abstract;obs.proposal? > Good, why not? > - Name of the observer: so far it has been obs.observer > but if we introduce meta.id.PI, meta.id.Coi for human beings, > why not meta.id.Observer;obs? > The ucd-word obs.observer was introduced to describe the observer/discoverer of a source, then extended to PIs. By the way, not always the PI is also the Observer, so why not have both! Cheers, Andrea =================================================================================== Andrea Preite Martinez andrea.preitemartinez@iasf-roma.inaf.it IASF Tel.IASF:+39.06.4993.4651 Via del Fosso del Cavaliere 100 Tel.CDS :+33.3.90242473 I-00133 Roma Cell.1 :+39.320.43.15.383 Cell.2 :+39. =================================================================================== From owner-ucd-sci@eso.org Tue Jul 25 13:52:01 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6PBppAG017471 for ; Tue, 25 Jul 2006 13:51:51 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6PBpp2k017470 for ucd-sci-outgoing; Tue, 25 Jul 2006 13:51:51 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-sci@eso.org using -f Received: from clyde.hq.eso.org (clyde.hq.eso.org [134.171.45.17]) by mercury.hq.eso.org (8.13.6+Sun/8.12.10) with ESMTP id k6PBpdXR017442; Tue, 25 Jul 2006 13:51:39 +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 k6PBpck9010186 (version=TLSv1/SSLv3 cipher=RC4-SHA bits=128 verify=NOT); Tue, 25 Jul 2006 13:51:38 +0200 In-Reply-To: <20060725112634.oz0z4tjnk4swk8kg@webmail.sic.rm.cnr.it> References: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> <44BB83C3.3010702@eso.org> <20060725112634.oz0z4tjnk4swk8kg@webmail.sic.rm.cnr.it> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <4A0BDD99-FA55-4D89-A4EF-E7D8A4F4C44A@eso.org> Cc: Nausicaa Delmotte , ucd-sci@ivoa.net Content-Transfer-Encoding: 7bit From: Alberto Micol Subject: Re: observation proposal and name of the observer Date: Tue, 25 Jul 2006 13:51:19 +0200 To: Andrea Preite Martinez X-Mailer: Apple Mail (2.752.2) X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Alberto Micol On Jul 25, 2006, at 11:26, Andrea Preite Martinez wrote: > Quoting Nausicaa Delmotte : > > >> - What is the difference between 'title of an observation proposal' >> and 'name of an observation proposal'? >> >> So far I would not have expected any difference but with the >> introduction >> of the new UCD word obs.proposal, it seems it is possible to >> construct both >> meta.title;obs.proposal >> and >> meta.id;obs.proposal I would personally use: meta.title;obs.proposal for the title of a proposal meta.id;obs.proposal for the proposal id I do not understand what "name of an observational proposal" actually means. Where did you get this one from Nausicaa? >> Maybe someone could provide an example, in case there is a >> difference >> of meaning >> between those two UCDs? I just cannot see the difference... (given >> that the proposal >> code is already defined by meta.code;obs.proposal). >> > Don't forget catalogues! According to the Catalogue DM, a catalogue > can have: > > - a name (in the description text)/a title (in the XML schema) > - an identifier > - a shortName > Yes, in the case of catalogues there is a third quantity to consider, the shortname, which does not exist for proposals. What should we be using here? catalog title -> meta.title;meta.table catalog id -> meta.id;meta.table catalog shortname -> ??? One could think of using meta.id;meta.table also for the shortname given that shortname is an alias of the catalog id (which happens to be just more human-readable). But I am against that for the reasons given below... > My point of view: > - The title of XYZ is a string describing the content of XYZ, as in > a scientific paper (actually this is the origin of the ucd); > - the name/identifier is a string uniquely identifying XYZ, as for > humans (e.g.: Andrea Preite Martinez is my name/identifier); To me names and identifiers are quite different. The name might not be unique, while an identifier better be. In the human case, the name is not unique, but the name with the birth certificate makes that person unique. What is unique is the identifier assigned to such human when registering to whatever service, e.g. the social security number. An identifiers will differ for the same human within different services. Alike, a catalogue which is colloquially called Veron 2006, will have different IDs in different services. I think a meta.nickname could be useful here. Aside note: I would drop meta.dataset in favour of meta.id;obs > - a short name for me could be APM (and my "code" could be my > social security number!). > I don't see the difference between name and identifier. meta.code is described as: "Code or flag" Given that meta.id to me is the identifier, I am pushed to think that Code is not an identifier. Hence I always interpret meta.code as a flag. As such, as a UCD user, I am not going to assign the ucd meta.code to a social security number. I guess that after this email, I will be invited not to assign ucds any longer... ;-) But the truth is that the UCD assignment is a highly subjective matter. > Another point is that a "possible" ucd is not necessarily a "good" > ucd!! And how can a user tell wether her choice resulted into a "good" ucd? Alberto From owner-ucd-sci@eso.org Tue Jul 25 16:26:58 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6PEQh68019225 for ; Tue, 25 Jul 2006 16:26:43 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6PEQhKE019224 for ucd-sci-outgoing; Tue, 25 Jul 2006 16:26:43 +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 (8.13.6+Sun/8.12.10) with ESMTP id k6PEQVRu019187 for ; Tue, 25 Jul 2006 16:26:32 +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 k6PEQRum000057 for ; Tue, 25 Jul 2006 16:26:28 +0200 (CEST) Received: from [10.0.1.134] (really [68.231.133.145]) by fed1rmmtao08.cox.net (InterMail vM.6.01.06.01 201-2131-130-101-20060113) with ESMTP id <20060725142620.FKGZ27857.fed1rmmtao08.cox.net@[10.0.1.134]>; Tue, 25 Jul 2006 10:26:20 -0400 In-Reply-To: <4A0BDD99-FA55-4D89-A4EF-E7D8A4F4C44A@eso.org> References: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> <44BB83C3.3010702@eso.org> <20060725112634.oz0z4tjnk4swk8kg@webmail.sic.rm.cnr.it> <4A0BDD99-FA55-4D89-A4EF-E7D8A4F4C44A@eso.org> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: multipart/alternative; boundary=Apple-Mail-2--563265475 Message-Id: <4CC29EE4-F187-41B3-BC3E-99D24FC29211@noao.edu> Cc: Andrea Preite Martinez , Nausicaa Delmotte , ucd-sci@ivoa.net From: Rob Seaman Subject: Re: observation proposal and name of the observer Date: Tue, 25 Jul 2006 07:26:33 -0700 To: Alberto Micol X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.7.25.63432 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Rob Seaman --Apple-Mail-2--563265475 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed On Jul 25, 2006, at 4:51 AM, Alberto Micol wrote: > I would personally use: > > meta.title;obs.proposal for the title of a proposal > meta.id;obs.proposal for the proposal id > > I do not understand what "name of an observational proposal" > actually means. Me neither. The most obvious distinction between the title of a proposal and its ID is that the title is assigned by the proposing astronomer(s) and the ID is assigned by the observatory acting as an agent for the resources the astronomers are proposing to use. > Yes, in the case of catalogues there is a third quantity to consider, > the shortname, which does not exist for proposals. A name, including a shortname, applies to a resource - whoever assigns the name. A catalog, instrument, telescope, filter, etc., is a resource. A proposal is not. A proposal can ultimately result in the production of a resource, such as the catalogs or images published by a survey project. These may themselves have a shortname - a nickname - that might colloquially also be applied to the project or even the proposal. For example, Nick Suntzeff is the P.I. for a proposal entitled: "The w Project: Measuring the Equation of State of the Universe". NOAO assigned the ID "2002B-0007" (see http://www.noao.edu/perl/abstract? 2002B-0007). This has resulted in a survey - and the fruits of that survey - also known as "ESSENCE" (http://www.ctio.noao.edu/essence). One might then choose to refer to the "ESSENCE proposal abstract" (a casually assigned name), for instance, even though the acronym came about after the original project was proposed. > To me names and identifiers are quite different. > The name might not be unique, while an identifier better be. Agree with this, but this distinction is only the result of who assigns the token. A name can be assigned by any party involved in some resource transaction. An identifier may only be assigned by the holder of the resource. Rob Seaman NOAO --Apple-Mail-2--563265475 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1
On Jul 25, 2006, at 4:51 AM, Alberto Micol = wrote:

I = would personally use:

meta.title;obs.proposal for the title of a = proposal
meta.id;obs.proposal=A0= =A0 for the proposal id

I do not understand what "name of an = observational proposal" actually = means.

Me neither.

The most obvious distinction between the = title of a proposal and its ID is that the title is assigned by the = proposing astronomer(s) and the ID is assigned by the observatory acting = as an agent for the resources the astronomers are proposing to = use.

Yes, in the case of catalogues there is a = third quantity to consider,
the shortname, which does not exist for = proposals.

A name, including a shortname, applies to a = resource - whoever assigns the name.=A0 A catalog, instrument, = telescope, filter, etc., is a resource.=A0 A proposal is not.=A0 A = proposal can ultimately result in the production of a resource, such as = the catalogs or images published by a survey project.=A0 These may = themselves have a shortname - a nickname - that might colloquially also = be applied to the project or even the = proposal.

For example, Nick Suntzeff is the P.I. for a = proposal entitled:=A0 "The w Project: Measuring the Equation of State of = the Universe".=A0 NOAO assigned the ID "2002B-0007" (see=A0http://www.noao.edu/= perl/abstract?2002B-0007).=A0 This has resulted in a survey - and = the fruits of that survey - also known as "ESSENCE" (http://www.ctio.noao.edu/essence= ).=A0 One might then choose to refer to the "ESSENCE proposal = abstract" (a casually assigned name), for instance, even though the = acronym came about after the original project was = proposed.

To me names and identifiers are quite = different.
The name might not be unique, while an = identifier better be.

Agree with this, but this distinction is only = the result of who assigns the token.=A0 A name can be assigned by any = party involved in some resource transaction.=A0 An identifier may only = be assigned by the holder of the resource.

Rob Seaman
NOAO
= --Apple-Mail-2--563265475-- From owner-ucd-sci@eso.org Tue Jul 25 16:56:39 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6PEuUac025914 for ; Tue, 25 Jul 2006 16:56:30 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6PEuUil025912 for ucd-sci-outgoing; Tue, 25 Jul 2006 16:56:30 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-sci@eso.org using -f Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.13.6+Sun/8.12.10) with ESMTP id k6PEuLJJ025851 for ; Tue, 25 Jul 2006 16:56:21 +0200 (MEST) Received: from [134.171.27.58] (ga008899.ads.eso.org [134.171.27.58]) by serapis.hq.eso.org (8.11.7+Sun/8.11.7) with ESMTP id k6PEuLd18981 for ; Tue, 25 Jul 2006 16:56:21 +0200 (MEST) Message-ID: <44C63115.8020101@eso.org> Date: Tue, 25 Jul 2006 16:56:21 +0200 From: Nausicaa Delmotte User-Agent: Thunderbird 1.5.0.4 (X11/20060516) MIME-Version: 1.0 To: ucd-sci@ivoa.net Subject: Re: observation proposal and name of the observer References: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> <44BB83C3.3010702@eso.org> <20060725112634.oz0z4tjnk4swk8kg@webmail.sic.rm.cnr.it> <4A0BDD99-FA55-4D89-A4EF-E7D8A4F4C44A@eso.org> In-Reply-To: <4A0BDD99-FA55-4D89-A4EF-E7D8A4F4C44A@eso.org> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Nausicaa Delmotte Alberto Micol said the following on 07/25/2006 01:51 PM: > I do not understand what "name of an observational proposal" actually > means. > Where did you get this one from Nausicaa? From the list of examples at http://www.ivoa.net/twiki/bin/view/IVOA/UCDwordsRFM meta.id;obs.proposal | name of the proposal meta.code;obs.proposal | proposal code etc. > I am not going to assign the ucd meta.code to a social security number I agree that meta.code should be reserved for flags and codes but not IDs. Though for ESO proposals, the difference between code and ID is getting fuzzy since the ID is itself composed of codes, e.g. 074.D-0761 [0-2]PP.[A-Z]-NNNN [0-2] is the type of program (normal, large...) [A-Z] is the category of the proposal (cosmology, stars, galaxies...) But the whole is greater than the sum of the parts, so the proposal ID should correspond to meta.id;obs.proposal and not meta.code;obs.proposal. >> Another point is that a "possible" ucd is not necessarily a "good" ucd!! > > And how can a user tell wether her choice resulted into a "good" ucd? I would say that the more examples we give in the reference UCD document, the easiest it is for a user to be convinced that the correct UCD was assigned. Nausicaa From owner-ucd-sci@eso.org Tue Jul 25 17:18:30 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6PFILUC000369 for ; Tue, 25 Jul 2006 17:18:22 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6PFILFt000368 for ucd-sci-outgoing; Tue, 25 Jul 2006 17:18:21 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-sci@eso.org using -f Received: from clyde.hq.eso.org (clyde.hq.eso.org [134.171.45.17]) by mercury.hq.eso.org (8.13.6+Sun/8.12.10) with ESMTP id k6PFI9Ar000318; Tue, 25 Jul 2006 17:18:09 +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 k6PFI8k9015356 (version=TLSv1/SSLv3 cipher=RC4-SHA bits=128 verify=NOT); Tue, 25 Jul 2006 17:18:08 +0200 In-Reply-To: <4CC29EE4-F187-41B3-BC3E-99D24FC29211@noao.edu> References: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> <44BB83C3.3010702@eso.org> <20060725112634.oz0z4tjnk4swk8kg@webmail.sic.rm.cnr.it> <4A0BDD99-FA55-4D89-A4EF-E7D8A4F4C44A@eso.org> <4CC29EE4-F187-41B3-BC3E-99D24FC29211@noao.edu> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <20B7754A-5A0F-4ADC-92B0-B3EAC704378C@eso.org> Cc: Andrea Preite Martinez , Nausicaa Delmotte , ucd-sci@ivoa.net Content-Transfer-Encoding: 7bit From: Alberto Micol Subject: Re: observation proposal and name of the observer Date: Tue, 25 Jul 2006 17:18:06 +0200 To: Rob Seaman X-Mailer: Apple Mail (2.752.2) X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Alberto Micol On Jul 25, 2006, at 16:26, Rob Seaman wrote: > On Jul 25, 2006, at 4:51 AM, Alberto Micol wrote: > >> I would personally use: >> >> meta.title;obs.proposal for the title of a proposal >> meta.id;obs.proposal for the proposal id >> >> I do not understand what "name of an observational proposal" >> actually means. > > Me neither. > > The most obvious distinction between the title of a proposal and > its ID is that the title is assigned by the proposing astronomer(s) > and the ID is assigned by the observatory acting as an agent for > the resources the astronomers are proposing to use. > >> Yes, in the case of catalogues there is a third quantity to consider, >> the shortname, which does not exist for proposals. > > A name, including a shortname, applies to a resource - whoever > assigns the name. A catalog, instrument, telescope, filter, etc., > is a resource. A proposal is not. A proposal can ultimately > result in the production of a resource, such as the catalogs or > images published by a survey project. These may themselves have a > shortname - a nickname - that might colloquially also be applied to > the project or even the proposal. > > For example, Nick Suntzeff is the P.I. for a proposal entitled: > "The w Project: Measuring the Equation of State of the Universe". > NOAO assigned the ID "2002B-0007" (see http://www.noao.edu/perl/ > abstract?2002B-0007). This has resulted in a survey - and the > fruits of that survey - also known as "ESSENCE" (http:// > www.ctio.noao.edu/essence). One might then choose to refer to the > "ESSENCE proposal abstract" (a casually assigned name), for > instance, even though the acronym came about after the original > project was proposed. Also in the HST case short names are used (e.g. UDF, HDF, etc), and one could say "the UDF proposal" actually referring to a list of proposals that composed the entire project. (I do not actually remember now whether UDF was developed through various proposals and not only one, but the important thing is that it CAN happen). Just to say that a nickname is a loose concept, which does not necessarily map one to one with the described entity (the proposal in this case). Hence I think it would be better to have a meta.nickname ucd... >> To me names and identifiers are quite different. >> The name might not be unique, while an identifier better be. > > Agree with this, but this distinction is only the result of who > assigns the token. A name can be assigned by any party involved in > some resource transaction. An identifier may only be assigned by > the holder of the resource. Fully agreed. > Rob Seaman > NOAO Alberto -- Alberto Micol ESA/DSCI/RSSD/SNM From owner-ucd-sci@eso.org Tue Jul 25 17:37:18 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6PFb35D003754 for ; Tue, 25 Jul 2006 17:37:04 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6PFb3GT003753 for ucd-sci-outgoing; Tue, 25 Jul 2006 17:37:03 +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 (8.13.6+Sun/8.12.10) with ESMTP id k6PFacdD003685 for ; Tue, 25 Jul 2006 17:36:38 +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 k6PFaZum003940 for ; Tue, 25 Jul 2006 17:36:36 +0200 (CEST) X-Spam-Checker-Version: SpamAssassin 3.1.3 (2006-06-01) on noao.edu X-Spam-Level: X-Spam-Status: No, score=-4.4 required=4.5 tests=ALL_TRUSTED,AWL,BAYES_00, HTML_MESSAGE autolearn=ham version=3.1.3 X-TFF-CGPSA-Version: 1.4f1 X-TFF-CGPSA-Filter: Scanned Received: from [140.252.4.155] ([140.252.4.155] verified) by noao.edu (CommuniGate Pro SMTP 5.0.9) with ESMTPS id 28990609; Tue, 25 Jul 2006 08:36:23 -0700 In-Reply-To: <44C63115.8020101@eso.org> References: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> <44BB83C3.3010702@eso.org> <20060725112634.oz0z4tjnk4swk8kg@webmail.sic.rm.cnr.it> <4A0BDD99-FA55-4D89-A4EF-E7D8A4F4C44A@eso.org> <44C63115.8020101@eso.org> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: multipart/alternative; boundary=Apple-Mail-10--559079750 Message-Id: <601CD3E3-D975-4834-965E-6A75AF222AAB@noao.edu> Cc: ucd-sci@ivoa.net From: Rob Seaman Subject: Re: observation proposal and name of the observer Date: Tue, 25 Jul 2006 08:36:19 -0700 To: Nausicaa Delmotte X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.7.25.73432 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Rob Seaman --Apple-Mail-10--559079750 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed On Jul 25, 2006, at 7:56 AM, Nausicaa Delmotte wrote: > I would say that the more examples we give in the reference UCD > document, > the easiest it is for a user to be convinced that the correct UCD > was assigned. If the logic behind UCDs may only be correctly grasped by example, UCDs might just as well be opaque tokens assigned randomly. It seems to me that the whole point of the exercise is to illuminate (at least partially) the intrinsic structure that underlies astronomical nomenclature. Given a categorized value, what are the rules for constructing quantities contingent on that value? Given a complex UCD expression, how does one parse it without consulting documentation such as a master list? Users need to understand other people's UCDs - they may also need to assign their own. UCD fluency won't be established through better documentation (not that this hurts), but rather must be built into the linguistic structure of the "language". Rob Seaman NOAO --Apple-Mail-10--559079750 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1
On Jul 25, 2006, at 7:56 AM, Nausicaa = Delmotte wrote:

I = would say that the more examples we give in the reference UCD = document,
the easiest it is for a user to be convinced = that the correct UCD was = assigned.

If the logic behind UCDs may only be = correctly grasped by example, UCDs might just as well be opaque tokens = assigned randomly.=A0 It seems to me that the whole point of the = exercise is to illuminate (at least partially) the intrinsic structure = that underlies astronomical nomenclature.=A0 Given a categorized value, = what are the rules for constructing quantities contingent on that = value?=A0 Given a complex UCD expression, how does one parse it = without consulting documentation such as a master = list?

Users need to understand other people's UCDs = - they may also need to assign their own.=A0 UCD fluency won't be = established through better documentation (not that this hurts), but = rather must be built into the linguistic structure of the = "language".

Rob Seaman
NOAO
= --Apple-Mail-10--559079750-- From owner-ucd-sci@eso.org Tue Jul 25 17:56:46 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6PFuXtf007436 for ; Tue, 25 Jul 2006 17:56:33 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6PFuXae007434 for ucd-sci-outgoing; Tue, 25 Jul 2006 17:56:33 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-sci@eso.org using -f Received: from clyde.hq.eso.org (clyde.hq.eso.org [134.171.45.17]) by mercury.hq.eso.org (8.13.6+Sun/8.12.10) with ESMTP id k6PFuDu5007375; Tue, 25 Jul 2006 17:56:14 +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 k6PFuDk9016305 (version=TLSv1/SSLv3 cipher=RC4-SHA bits=128 verify=NOT); Tue, 25 Jul 2006 17:56:13 +0200 In-Reply-To: <601CD3E3-D975-4834-965E-6A75AF222AAB@noao.edu> References: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> <44BB83C3.3010702@eso.org> <20060725112634.oz0z4tjnk4swk8kg@webmail.sic.rm.cnr.it> <4A0BDD99-FA55-4D89-A4EF-E7D8A4F4C44A@eso.org> <44C63115.8020101@eso.org> <601CD3E3-D975-4834-965E-6A75AF222AAB@noao.edu> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: Cc: Nausicaa Delmotte , ucd-sci@ivoa.net Content-Transfer-Encoding: 7bit From: Alberto Micol Subject: Re: observation proposal and name of the observer Date: Tue, 25 Jul 2006 17:56:11 +0200 To: Rob Seaman X-Mailer: Apple Mail (2.752.2) X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Alberto Micol On Jul 25, 2006, at 17:36, Rob Seaman wrote: > On Jul 25, 2006, at 7:56 AM, Nausicaa Delmotte wrote: > >> I would say that the more examples we give in the reference UCD >> document, >> the easiest it is for a user to be convinced that the correct UCD >> was assigned. > > If the logic behind UCDs may only be correctly grasped by example, > UCDs might just as well be opaque tokens assigned randomly. It > seems to me that the whole point of the exercise is to illuminate > (at least partially) the intrinsic structure that underlies > astronomical nomenclature. Given a categorized value, what are the > rules for constructing quantities contingent on that value? Given > a complex UCD expression, how does one parse it without consulting > documentation such as a master list? > > Users need to understand other people's UCDs - they may also need > to assign their own. UCD fluency won't be established through > better documentation (not that this hurts), but rather must be > built into the linguistic structure of the "language". I do agree, but ... how to make it happen? I mean, a pragmatic service provider would want to read (and real fast) the existing ucd documentation and start using ucds asap. Kids learn the linguistic structure during their kindergarden phase, using the trial and error method. How can we succeed, that is make such service provider happy, and at the same time reach desired "UCD fluency" without asking the service providers to go through the kindergarden phase? I do agree with Nausicaa, we need more examples, and probably more comprehensive UCD descriptions (not just only the couple of words currently listed for each ucd); not too much, but just enough to not have anyone repeating the same errors again and again, and to avoid confusion (e.g. meta.code while one really means meta.id, meta.id while one really means meta.code, ;-) etc.) Al From owner-ucd-sci@eso.org Tue Jul 25 18:08:35 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6PG8S3X009931 for ; Tue, 25 Jul 2006 18:08:28 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6PG8SVu009929 for ucd-sci-outgoing; Tue, 25 Jul 2006 18:08:28 +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 (8.13.6+Sun/8.12.10) with ESMTP id k6PG8E7G009886 for ; Tue, 25 Jul 2006 18:08:14 +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 k6PG8Bum005601 for ; Tue, 25 Jul 2006 18:08:12 +0200 (CEST) Received: from [131.215.146.143] ([131.215.146.143]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-7.2) with ESMTP id k6PG7m3H003658 (version=TLSv1/SSLv3 cipher=RC4-SHA bits=128 verify=NO); Tue, 25 Jul 2006 09:07:48 -0700 In-Reply-To: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> References: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <65879593-BCAA-414E-BEA7-ACE2A9304141@cacr.caltech.edu> Cc: Roy Williams , ucd-sci@ivoa.net Content-Transfer-Encoding: 7bit From: Roy Williams Subject: Re: RFMs (Requests for modification) on the List of UCD-words Date: Tue, 25 Jul 2006 09:07:41 -0700 To: Andrea Preite Martinez X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.7.25.83433 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Roy Williams Andrea et al I like the new UCDs, I do not have any problem with approving the new words and the changes. But perhaps I can make a pest of myself by suggesting a couple more. I see we already have P | meta.ref | Reference, or origin P | meta.ref.url | URL, web address, service endpoint and I would like to suggest also for completeness P | meta.ref.uri | URI, universal resource identifier P | meta.ref.ivorn | IVORN, Int. Virtual Obs. Resource Name ivo:// Hope this is not too late. Indeed I have use cases for these if you would like to see that. Roy On Jul 17, 2006, at 2:01 AM, Andrea Preite Martinez wrote: > RFMs (Requests for modification) on the List of UCD-words > ========================================================= > > > Dear all, > > You can find at http://www.ivoa.net/twiki/bin/view/IVOA/ > UCDwordsRFM a list of proposed requests (RFMs) to modify/add the > present standard list of ucd-words: The UCD1+ controlled > vocabulary, Vers. 1.11 - IVOA Recommendation 31 December 2005 > ( http://www.ivoa.net/Documents/latest/UCDlist.html ). California Institute of Technology 626 395 3670 From owner-ucd-sci@eso.org Tue Jul 25 18:21:17 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6PGLAP4012666 for ; Tue, 25 Jul 2006 18:21:10 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6PGLAX5012665 for ucd-sci-outgoing; Tue, 25 Jul 2006 18:21:10 +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 (8.13.6+Sun/8.12.10) with ESMTP id k6PGL6hH012659 for ; Tue, 25 Jul 2006 18:21:07 +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 k6PGL3um006536 for ; Tue, 25 Jul 2006 18:21:04 +0200 (CEST) X-Spam-Checker-Version: SpamAssassin 3.1.3 (2006-06-01) on noao.edu X-Spam-Level: X-Spam-Status: No, score=-4.4 required=4.5 tests=ALL_TRUSTED,AWL,BAYES_00 autolearn=ham version=3.1.3 X-TFF-CGPSA-Version: 1.4f1 X-TFF-CGPSA-Filter: Scanned Received: from [140.252.4.155] ([140.252.4.155] verified) by noao.edu (CommuniGate Pro SMTP 5.0.9) with ESMTPS id 28992551; Tue, 25 Jul 2006 09:20:57 -0700 In-Reply-To: References: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> <44BB83C3.3010702@eso.org> <20060725112634.oz0z4tjnk4swk8kg@webmail.sic.rm.cnr.it> <4A0BDD99-FA55-4D89-A4EF-E7D8A4F4C44A@eso.org> <44C63115.8020101@eso.org> <601CD3E3-D975-4834-965E-6A75AF222AAB@noao.edu> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: Cc: Nausicaa Delmotte , ucd-sci@ivoa.net Content-Transfer-Encoding: 7bit From: Rob Seaman Subject: Re: observation proposal and name of the observer Date: Tue, 25 Jul 2006 09:20:53 -0700 To: Alberto Micol X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.7.25.83433 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Rob Seaman On Jul 25, 2006, at 8:56 AM, Alberto Micol wrote: > we need more examples, and probably > more comprehensive UCD descriptions (not just only the couple > of words currently listed for each ucd); not too much, but just enough > to not have anyone repeating the same errors again and again, > and to avoid confusion (e.g. meta.code while one really means meta.id, > meta.id while one really means meta.code, ;-) etc.) Well, you might start there. I still have no clue what the distinction is supposed to be between meta.code and meta.id. As a cautionary tale, I highly recommend "The Meaning of Everything" by Simon Winchester. This is the story of the Oxford English Dictionary - the prototypical project that was supposed to take five years, but took fifty - or was it 75 years? - to complete. (Only to start all over again.) UCDs are ultimately derived from the experience of the OED - both are structured word lists, compiled by reference to a body of literature. Rob From owner-ucd-sci@eso.org Tue Jul 25 18:48:40 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6PGmXX6017633 for ; Tue, 25 Jul 2006 18:48:33 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6PGmXtW017632 for ucd-sci-outgoing; Tue, 25 Jul 2006 18:48:33 +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 (8.13.6+Sun/8.12.10) with ESMTP id k6PGmQlo017621 for ; Tue, 25 Jul 2006 18:48:26 +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 k6PGmNum008172 for ; Tue, 25 Jul 2006 18:48:24 +0200 (CEST) Received: from [131.215.146.143] ([131.215.146.143]) (authenticated bits=0) by mail.cacr.caltech.edu (8.12.3/8.12.3/Debian-7.2) with ESMTP id k6PGmH3H004363 (version=TLSv1/SSLv3 cipher=RC4-SHA bits=128 verify=NO); Tue, 25 Jul 2006 09:48:17 -0700 In-Reply-To: References: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> <44BB83C3.3010702@eso.org> <20060725112634.oz0z4tjnk4swk8kg@webmail.sic.rm.cnr.it> <4A0BDD99-FA55-4D89-A4EF-E7D8A4F4C44A@eso.org> <44C63115.8020101@eso.org> <601CD3E3-D975-4834-965E-6A75AF222AAB@noao.edu> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: Cc: Roy Williams , ucd-sci@ivoa.net Content-Transfer-Encoding: 7bit From: Roy Williams Subject: Re: observation proposal and name of the observer Date: Tue, 25 Jul 2006 09:48:11 -0700 To: Rob Seaman X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.7.25.85433 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Roy Williams On Jul 25, 2006, at 9:20 AM, Rob Seaman wrote: > I still have no clue what the distinction is supposed to be between > meta.code and meta.id. My understanding: -- A code is also called an enumeration or a labeling or a classification. It is tied to a namespace. In the Hubble namespace, galaxies have codes Sa, Sb, SBa, E0 etc etc -- An ID is unique identifier for something that is strongly linked to a namespace. Within the Messier namespace, there are identifiers M31, M51, M87. -- A name is anything that identifies something, need not be unique. Thus a single galaxy can have several names, eq M87 and NGC4486 are different names for the same thing. -- A Title is a multi-word version of a name: "Center of Virgo cluster" would be a title for M87. California Institute of Technology 626 395 3670 From owner-ucd-sci@eso.org Tue Jul 25 19:44:12 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6PHi1Nk025501 for ; Tue, 25 Jul 2006 19:44:01 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6PHi0ep025484 for ucd-sci-outgoing; Tue, 25 Jul 2006 19:44:00 +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 (8.13.6+Sun/8.12.10) with ESMTP id k6PHhuNs025457 for ; Tue, 25 Jul 2006 19:43:56 +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 k6PHhrum010467 for ; Tue, 25 Jul 2006 19:43:54 +0200 (CEST) X-Spam-Checker-Version: SpamAssassin 3.1.3 (2006-06-01) on noao.edu X-Spam-Level: X-Spam-Status: No, score=-4.4 required=4.5 tests=ALL_TRUSTED,AWL,BAYES_00 autolearn=ham version=3.1.3 X-TFF-CGPSA-Version: 1.4f1 X-TFF-CGPSA-Filter: Scanned Received: from [140.252.4.155] ([140.252.4.155] verified) by noao.edu (CommuniGate Pro SMTP 5.0.9) with ESMTPS id 28996063; Tue, 25 Jul 2006 10:43:46 -0700 In-Reply-To: References: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> <44BB83C3.3010702@eso.org> <20060725112634.oz0z4tjnk4swk8kg@webmail.sic.rm.cnr.it> <4A0BDD99-FA55-4D89-A4EF-E7D8A4F4C44A@eso.org> <44C63115.8020101@eso.org> <601CD3E3-D975-4834-965E-6A75AF222AAB@noao.edu> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <674900CA-4073-41C9-AD02-BD494AF95D3C@noao.edu> Cc: ucd-sci@ivoa.net Content-Transfer-Encoding: 7bit From: Rob Seaman Subject: Re: observation proposal and name of the observer Date: Tue, 25 Jul 2006 10:43:43 -0700 To: Roy Williams X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.7.25.95432 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Rob Seaman Roy wrote: > -- A code is also called an enumeration or a labeling or a > classification. It is tied to a namespace. In the Hubble namespace, > galaxies have codes Sa, Sb, SBa, E0 etc etc > > -- An ID is unique identifier for something that is strongly linked > to a namespace. Within the Messier namespace, there are identifiers > M31, M51, M87. Ok. How about, rather, meta.classID and meta.nameID? It seems to me that the "IDness" of something is the part that will suggest to most users that this is something from a controlled namespace, whereas a class is a type of something and a name denotes a specific something, either of which might require a controlled ID. > -- A name is anything that identifies something, need not be > unique. Thus a single galaxy can have several names, eq M87 and > NGC4486 are different names for the same thing. > > -- A Title is a multi-word version of a name: "Center of Virgo > cluster" would be a title for M87. But surely a name can be multi-word and a title, e.g., "Macbeth" need not. And nicknames can indeed be "short names", such as "B" instead of "Johnson B", but can also be longer, such as "The Scottish Play". The general question of names is an issue of alias management. An ID is only unique in the sense of being guaranteed not to apply to more than one item. On the other hand, a single item may have multiple IDs - multiple aliases. Rob From owner-ucd-sci@eso.org Wed Jul 26 12:03:31 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6QA3INY001321 for ; Wed, 26 Jul 2006 12:03:18 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6QA3HPn001320 for ucd-sci-outgoing; Wed, 26 Jul 2006 12:03:17 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-sci@eso.org using -f Received: from forth.hq.eso.org (forth.hq.eso.org [134.171.45.18]) by mercury.hq.eso.org (8.13.6+Sun/8.12.10) with ESMTP id k6QA30Eb001283; Wed, 26 Jul 2006 12:03:01 +0200 (MEST) Received: from [134.171.10.12] (ma008861.hq.eso.org [134.171.10.12]) (authenticated bits=0) by forth.hq.eso.org (8.12.8/8.12.8) with ESMTP id k6QA30sC012494 (version=TLSv1/SSLv3 cipher=RC4-SHA bits=128 verify=NOT); Wed, 26 Jul 2006 12:03:00 +0200 In-Reply-To: References: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> <44BB83C3.3010702@eso.org> <20060725112634.oz0z4tjnk4swk8kg@webmail.sic.rm.cnr.it> <4A0BDD99-FA55-4D89-A4EF-E7D8A4F4C44A@eso.org> <44C63115.8020101@eso.org> <601CD3E3-D975-4834-965E-6A75AF222AAB@noao.edu> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: Cc: Rob Seaman , ucd-sci@ivoa.net Content-Transfer-Encoding: 7bit From: Alberto Micol Subject: Re: observation proposal and name of the observer Date: Wed, 26 Jul 2006 12:02:58 +0200 To: Roy Williams X-Mailer: Apple Mail (2.752.2) X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Alberto Micol On Jul 25, 2006, at 18:48, Roy Williams wrote: > > My understanding: > -- A code is also called an enumeration or a labeling or a > classification. It is tied to a namespace. In the Hubble namespace, > galaxies have codes Sa, Sb, SBa, E0 etc etc > -- An ID is unique identifier for something that is strongly linked > to a namespace. Within the Messier namespace, there are identifiers > M31, M51, M87. > > -- A name is anything that identifies something, need not be > unique. Thus a single galaxy can have several names, eq M87 and > NGC4486 are different names for the same thing. > > -- A Title is a multi-word version of a name: "Center of Virgo > cluster" would be a title for M87. > > I think that the above sentences put together by Roy are a perfect example of how to write ucd descriptions. I would not agree though on the Hubble classification because the right ucd is in that case meta.code.class, and not just meta.code P | meta.code | code is also called an enumeration or a labeling | of a flag. An example is the PixFlags in the SIAP1.0 | standard, which is a flag whose meaning is well | understood within that protocol. P | meta.code.class | Classification, tide to a namespace. | In the Hubble namespace, galaxies have codes | Sa, Sb, SBa, E0 etc P | meta.id | An ID is unique identifier for something that | is strongly linked to a namespace. Within the | Messier namespace, there are identifiers M31, M51, M87 P | meta.title | A Title is a multi-word version of a name: | "Center of Virgo cluster" would be a title for M87 P | meta.name | *** currently to be found under meta.id, *** | *** but probably it deserves its own ucd? *** It would be nice to extend the descriptions of all other ucds in a similar way, wouldn't it? Alberto From owner-ucd-sci@eso.org Wed Jul 26 16:43:14 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6QEh11v025819 for ; Wed, 26 Jul 2006 16:43:01 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6QEh1g0025818 for ucd-sci-outgoing; Wed, 26 Jul 2006 16:43:01 +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 (8.13.6+Sun/8.12.10) with ESMTP id k6QEgmuu025767 for ; Wed, 26 Jul 2006 16:42:50 +0200 (MEST) Received: from fed1rmmtao05.cox.net (fed1rmmtao05.cox.net [68.230.241.34]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k6QEgjLY006395 for ; Wed, 26 Jul 2006 16:42:45 +0200 (CEST) Received: from [10.0.1.143] (really [68.231.133.145]) by fed1rmmtao05.cox.net (InterMail vM.6.01.06.01 201-2131-130-101-20060113) with ESMTP id <20060726144239.DTND12909.fed1rmmtao05.cox.net@[10.0.1.143]>; Wed, 26 Jul 2006 10:42:39 -0400 In-Reply-To: References: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> <44BB83C3.3010702@eso.org> <20060725112634.oz0z4tjnk4swk8kg@webmail.sic.rm.cnr.it> <4A0BDD99-FA55-4D89-A4EF-E7D8A4F4C44A@eso.org> <44C63115.8020101@eso.org> <601CD3E3-D975-4834-965E-6A75AF222AAB@noao.edu> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <74599EA8-38A5-4A92-9410-1EE6AC72AE7C@noao.edu> Cc: Roy Williams , ucd-sci@ivoa.net Content-Transfer-Encoding: 7bit From: Rob Seaman Subject: Re: observation proposal and name of the observer Date: Wed, 26 Jul 2006 07:42:54 -0700 To: Alberto Micol X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.7.26.63432 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Rob Seaman On Jul 26, 2006, at 3:02 AM, Alberto Micol wrote: > I think that the above sentences put together by Roy > are a perfect example of how to write ucd descriptions. Roy certainly has a good knack for simplifying a description. But that doesn't excuse IVOA from a responsibility to simplify the things actually being described. Design elegance is a goal, not just a serendipitous occurrence. > I would not agree though on the Hubble classification because the > right ucd is in that case meta.code.class, and not just meta.code Every message in this discussion seems to bring additional nuances of usage. One suspects the latest is still not a complete list - either in the sense of capturing all ID-like meta UCD constructs that have been proposed - or in the sense of providing orthonormal basis vectors suitable for describing pertinent metadata. > P | meta.code | code is also called an > enumeration or a labeling > | of a flag. An example is > the PixFlags in the SIAP1.0 > | standard, which is a flag > whose meaning is well > | understood within that > protocol. > > P | meta.code.class | Classification, tide to a > namespace. > | In the Hubble namespace, > galaxies have codes > | Sa, Sb, SBa, E0 etc Users are not going to understand these distinctions. You will see as many instances of meta.class.code as you do of meta.code.class. You may see more meta.class instances than anything else. Users are going to have a hard enough time understanding why they need the "meta" at all - ain't all UCDs about metadata? If "code" is synonymous with "enum", why not use "enum"? The word "code" is horrifically overloaded for other purposes. Also, isn't an enumeration a modifier of the base UCD? A classification certainly could be open-ended - that is, not a code at all. How about: meta.class;enum Which opens up the possibility of constructs like: meta.id;enum Which might be used to limit the allowed values to a specific list of observing proposals, for instance - say, to those belonging to a particular investigator or pertaining to a particular telescope. > P | meta.id | An ID is unique identifier > for something that > | is strongly linked to a > namespace. Within the > | Messier namespace, there > are identifiers M31, M51, M87 If a namelike UCD ID requires only two levels, why should a classlike UCD ID require three? > P | meta.title | A Title is a multi-word > version of a name: > | "Center of Virgo cluster" > would be a title for M87 Again - multi-word is not the essence of the issue. That the title is assigned by the investigators, not by the observatory, likely is. > P | meta.name | *** currently to be found > under meta.id, *** > | *** but probably it > deserves its own ucd? *** So UCDs that don't actually exist are to be described, too? To the extent that this particular pseudo-meta-notional-concept exists, you are most closely describing a shortname here, and the title is an instance of a long name - or simply a "name". In fact, all of these concepts could be said to be subclassed from "name". > It would be nice to extend the descriptions of all other ucds > in a similar way, wouldn't it? Such descriptions certainly won't hurt, but the things being described should first be as carefully specified as anything in IVOA. From the discussion it seems obvious that no user can ever be trusted with either the generation or interpretation of a UCD. It also suggests that a UCD validator would be immediately seized upon by a grateful IVOA developer community. The question of versioning UCDs takes on new importance, too, since subtleties like those above will lead to perennial pressure to revise the roster of UCDs, not only to add new descriptors to open up new vistas of domain space, but also to clarify previous blessed descriptors. The meaning of a UCD construct seems unsettlingly unstable. Rob From owner-ucd-sci@eso.org Thu Jul 27 12:29:21 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6RATDNN022042 for ; Thu, 27 Jul 2006 12:29:14 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6RATDFu022041 for ucd-sci-outgoing; Thu, 27 Jul 2006 12:29:13 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-sci@eso.org using -f Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.13.6+Sun/8.12.10) with ESMTP id k6RAT4Rd021986 for ; Thu, 27 Jul 2006 12:29:04 +0200 (MEST) Received: from [134.171.27.58] (ga008899.ads.eso.org [134.171.27.58]) by serapis.hq.eso.org (8.11.7+Sun/8.11.7) with ESMTP id k6RAT3d10059 for ; Thu, 27 Jul 2006 12:29:03 +0200 (MEST) Message-ID: <44C8956F.9050101@eso.org> Date: Thu, 27 Jul 2006 12:29:03 +0200 From: Nausicaa Delmotte User-Agent: Thunderbird 1.5.0.4 (X11/20060516) MIME-Version: 1.0 To: ucd-sci@ivoa.net Subject: classification and code References: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> <44BB83C3.3010702@eso.org> <20060725112634.oz0z4tjnk4swk8kg@webmail.sic.rm.cnr.it> <4A0BDD99-FA55-4D89-A4EF-E7D8A4F4C44A@eso.org> <44C63115.8020101@eso.org> <601CD3E3-D975-4834-965E-6A75AF222AAB@noao.edu> <74599EA8-38A5-4A92-9410-1EE6AC72AE7C@noao.edu> In-Reply-To: <74599EA8-38A5-4A92-9410-1EE6AC72AE7C@noao.edu> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Nausicaa Delmotte Rob Seaman said the following on 07/26/2006 04:42 PM: >> P | meta.code | code is also called an >> enumeration or a labeling >> | of a flag. An example is the >> PixFlags in the SIAP1.0 >> | standard, which is a flag >> whose meaning is well >> | understood within that protocol. >> >> P | meta.code.class | Classification, tide to a >> namespace. >> | In the Hubble namespace, >> galaxies have codes >> | Sa, Sb, SBa, E0 etc > > Users are not going to understand these distinctions. You will see as > many instances of meta.class.code as you do of meta.code.class. You may > see more meta.class instances than anything else. It is true that there is some ambiguity regarding meta.code and meta.code.class According to the dictionary, a code is a coding system used for transmitting messages requiring brevity or secrecy and a classification is a group of people or things arranged by class or category Thus a classification code is a code representing a category within a classification system. Suppose a user wants to classify a list of observations according to the following categories: 'SCIENCE', 'CALIB', 'ACQUISITON', 'TEST', etc. Those categories are words, not codes. So a new UCD like meta.class is needed. Though one could argue that words are part of the language system and language is a code for human thought ;-) If you assign shortcuts to the categories ('S' for 'SCIENCE', 'C' for 'CALIB' etc), the correct UCD is meta.class.code since the UCD recommendation says that the order of the atoms induces a hierarchy. Now the question is: are there codes that are not part of a classification system? If no, I would drop meta.code and all columns previously assigned meta.code.class should be re-assigned meta.class.code. > If "code" is synonymous with "enum", why not use "enum"? The word > "code" is horrifically overloaded for other purposes. Strictly speaking, I don't think a code is an enumeration. An enumeration is a detailed account, in which each thing is specially noticed. However, 'code' and 'enumeration' are sometimes used for the same thing. It is something like a language shortcut. It is not necessarily bad to mention such words in the definition of a UCD since people are used to deal with both of them, it could even make things easier for the user but only AS LONG AS EXAMPLES ARE GIVEN since some other people might start wondering about the true meaning of words in the definition. In that case, they will have to look at the examples and that will solve the ambiguity. That is why we need to provide examples. Learning by example allows to grasp the basics more easily. > Also, isn't an > enumeration a modifier of the base UCD? A classification certainly > could be open-ended - that is, not a code at all. How about: > > meta.class;enum I would say an enumeration is a list of things (codes or not) that belong to a common category within a classification system... > Which opens up the possibility of constructs like: > > meta.id;enum > > Which might be used to limit the allowed values to a specific list of > observing proposals, for instance - say, to those belonging to a > particular investigator or pertaining to a particular telescope. ... so here I would assign meta.id;meta.class or better meta.id;meta.class.part? Cheers Nausicaa From owner-ucd-sci@eso.org Thu Jul 27 18:22:59 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6RGMaF7027709 for ; Thu, 27 Jul 2006 18:22:36 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6RGMZob027708 for ucd-sci-outgoing; Thu, 27 Jul 2006 18:22:35 +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 (8.13.6+Sun/8.12.10) with ESMTP id k6RGMSCs027695 for ; Thu, 27 Jul 2006 18:22:28 +0200 (MEST) Received: from fed1rmmtao03.cox.net (fed1rmmtao03.cox.net [68.230.241.36]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k6RGMOLY001769 for ; Thu, 27 Jul 2006 18:22:25 +0200 (CEST) Received: from [10.0.1.151] (really [68.231.133.145]) by fed1rmmtao03.cox.net (InterMail vM.6.01.06.01 201-2131-130-101-20060113) with ESMTP id <20060727162217.GOCY2704.fed1rmmtao03.cox.net@[10.0.1.151]>; Thu, 27 Jul 2006 12:22:17 -0400 In-Reply-To: <44C8956F.9050101@eso.org> References: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> <44BB83C3.3010702@eso.org> <20060725112634.oz0z4tjnk4swk8kg@webmail.sic.rm.cnr.it> <4A0BDD99-FA55-4D89-A4EF-E7D8A4F4C44A@eso.org> <44C63115.8020101@eso.org> <601CD3E3-D975-4834-965E-6A75AF222AAB@noao.edu> <74599EA8-38A5-4A92-9410-1EE6AC72AE7C@noao.edu> <44C8956F.9050101@eso.org> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: multipart/alternative; boundary=Apple-Mail-1--383504335 Message-Id: <66680684-D374-4A7F-8B7B-EFBCAAB805E6@noao.edu> Cc: ucd-sci@ivoa.net From: Rob Seaman Subject: Re: classification and code Date: Thu, 27 Jul 2006 09:22:34 -0700 To: Nausicaa Delmotte X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.7.27.83432 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Rob Seaman --Apple-Mail-1--383504335 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Hi Nausicaa, I said: >> Users are not going to understand these distinctions. and you said a bunch of stuff ending with: > ... so here I would assign meta.id;meta.class or better > meta.id;meta.class.part? This was in regard to some specific question of usage that is neither here nor there at the moment. What is both here and there is that you - an expert for some question of IVOA usage - are now arguing with yourself about the correct answer. I'll say it again - users are not going to understand how to use UCDs. This may or may not be acceptable - it depends on whether our users will ever need to either parse other people's UCDs or create their own. More generally, the question isn't whether UCDs make *any* sense - there appears to be a defensible logic behind every individual distinction that is raised. The question is whether the same logic lies behind all choices - and further, whether the logic is stable over time. I recommend: 1) UCD versioning be explicit 2) a UCD verification web service be assigned high priority (that is, beyond checking syntax and atoms) > a code is a coding system used for transmitting messages requiring > brevity or secrecy But "code" also means a way of representing a message in a new medium, e.g., ASCII. Code can be error detecting or correcting. A code can be a statute, that is, a rule. I see the "brevity or secrecy" definition at dictionary.com, but there many other entries: genetic code, a patient whose heart has stopped :-(, source code. In the latter case, we learn that the word "code" is used specifically to distinguish instructions from data ("often used in opposition to 'data'") - and yet, here we are applying it to (meta)data. I'm getting a code in my node. It isn't that I don't understand the logic behind the choice - it's that many other choices are just as logical. Why make *this* choice? And second, why specifically meta.code.class and *not* meta.class.code or meta.class;meta.code or any of the many other variations? Given the basic rules of UCDs and a list of atoms, a motivated undergraduate should be able to recreate the master list to a couple of sigma - heck, an awk script should be able to do it. But what is one to do with a rule like: "after the primary word, subsequent words are arranged by decreasing importance"? Importance to whom and for what purpose? The rule for atoms is even more ethereal: "the order of these atoms induces a hierarchy". We also have: "the only possible validation of the selected vocabulary is to check its ability to describe properly a wide range of real data". Check how? Define "properly". How about a Monte Carlo test of a canonical ensemble of alternate vocabularies? :-) Perhaps I simply don't understand the rules yet. I doubt I'm alone. I think there is reason to worry if the official list of UCDs can only be justified a posteriori. If nobody else feels the same way, by all means continue with the adoption of the new batch. In addition to versioning and a verification tool, I would then reiterate my support for retaining the ability to namespace UCDs. > If you assign shortcuts to the categories ('S' for 'SCIENCE', 'C' > for 'CALIB' etc), > the correct UCD is meta.class.code since the UCD recommendation > says that the order > of the atoms induces a hierarchy. Ok. So *both* meta.code.class and meta.class.code are to be supported? And is our software supposed to be able to understand these razor thin distinctions and do something usefully different? > Now the question is: are there codes that are not part of a > classification system? > If no, I would drop meta.code and all columns previously assigned > meta.code.class > should be re-assigned meta.class.code. Again - versioning. If our databases aren't to be held hostage to the vagaries of future drifts in UCD usage, they need to be able to refer to a specific, permanently stable, list of UCDs that was in effect when the columns were assigned. I suspect I'm not the only archivist to feel a chill at the sight of the word "re-assign" :-) > Strictly speaking, I don't think a code is an enumeration. > An enumeration is a detailed account, in which each thing is > specially noticed. > However, 'code' and 'enumeration' are sometimes used for the same > thing. > It is something like a language shortcut. Ok - I'm all for precision of expression. We have: - a code is a coding system used for transmitting messages requiring brevity or secrecy - a classification is a group of people or things arranged by class or category - an enumeration is a detailed account, in which each thing is specially noticed And we have the rule that "the order of the atoms induces a hierarchy", so each of: meta.code.class.enum, meta.code.enum.class, meta.class.code.enum, meta.class.enum.code, meta.enum.class.code, and meta.enum.code.class are distinctly different in the obvious way :-) > they will have to look at the examples and that will solve the > ambiguity. > That is why we need to provide examples. > Learning by example allows to grasp the basics more easily. I haven't heard anybody argue against providing examples, but the assertions of solving ambiguities and grasping basics should be challenged by providing IVOA beta testers with such examples and requesting they a) describe the meaning of the examples, and b) use the knowledge gained to create new UCDs representing various concepts. I suggest this worthy goal continue: "The UCD working group has tried to resist the temptation to allow the UCD syntax to be overly expressive." Rob --Apple-Mail-1--383504335 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1
Hi=A0Nausicaa,

I said:

Users are not going to understand these = distinctions.

and you said a bunch of stuff ending = with:

... so here I would assign meta.id;meta.class or better = meta.id;meta.class.part?

This was in regard to some specific question = of usage that is neither here nor there at the moment.=A0 What is both = here and there is that you - an expert for some question of IVOA usage - = are now arguing with yourself about the correct answer.=A0 I'll say it = again - users are not going to understand how to use UCDs.=A0 This may = or may not be acceptable - it depends on whether our users will ever = need to either parse other people's UCDs or create their = own.

More generally, the question isn't whether = UCDs make *any* sense - there appears to be a defensible logic behind = every individual distinction that is raised.=A0 The question is whether = the same logic lies behind all choices - and further, whether the logic = is stable over time.=A0 I recommend:

1) UCD versioning be = explicit
2) a UCD verification web service be assigned high priority (that = is, beyond checking syntax and atoms)

a code is a coding = system used for transmitting messages requiring brevity or = secrecy

But "code" also means a way of representing a = message in a new medium, e.g., ASCII.=A0 Code can be error detecting or = correcting.=A0 A code can be a statute, that is, a rule.=A0 I see the = "brevity or secrecy" definition at dictionary.com, but there many other = entries:=A0 genetic code, a patient whose heart has stopped :-(, source = code.=A0 In the latter case, we learn that the word "code" is used = specifically to distinguish instructions from data ("often used in = opposition to 'data'") - and yet, here we are applying it to (meta)data. = =A0I'm getting a code in my node.

It isn't that I don't understand the logic = behind the choice - it's that many other choices are just as logical.=A0 = Why make *this* choice?=A0 And second, why specifically meta.code.class = and *not* meta.class.code or meta.class;meta.code or any of the many = other variations?=A0 Given the basic rules of UCDs and a list of atoms, = a motivated undergraduate should be able to recreate the master list to = a couple of sigma - heck, an awk script should be able to do = it.

But what is one to do with a rule like:=A0 = "after the primary word, subsequent words are arranged by decreasing = importance"?=A0 Importance to whom and for what purpose?=A0 The rule for = atoms is even more ethereal: "the order of these atoms induces a = hierarchy".=A0 We also have:=A0 "the only possible validation of the = selected vocabulary is to check its ability to describe properly a wide = range of real data".=A0 Check how?=A0 Define "properly". =A0How about a = Monte Carlo test of a canonical ensemble of alternate vocabularies? =A0:-)= =A0Perhaps I simply don't understand the rules yet.=A0 I doubt I'm = alone.

I think there is reason to worry if the = official list of UCDs can only be justified a posteriori.=A0 If nobody = else feels the same way, by all means continue with the adoption of the = new batch.=A0 In addition to versioning and a verification tool, I would = then reiterate my support for retaining the ability to namespace = UCDs.

If you assign = shortcuts to the categories ('S' for 'SCIENCE', 'C' for 'CALIB' = etc),
the correct UCD is meta.class.code since the = UCD recommendation says that the order
of the atoms = induces a hierarchy.

Ok.=A0 So *both* meta.code.class and = meta.class.code are to be supported?=A0 And is our software supposed to = be able to understand these razor thin distinctions and do something = usefully different?

Now the question is: are there codes that are not part of a = classification system?
If no, I would drop meta.code and all columns = previously assigned meta.code.class
should be = re-assigned meta.class.code.

Again - versioning.=A0 If our databases = aren't to be held hostage to the vagaries of future drifts in UCD usage, = they need to be able to refer to a specific, permanently stable, list of = UCDs that was in effect when the columns were assigned.=A0 I suspect I'm = not the only archivist to feel a chill at the sight of the word = "re-assign" :-)

Strictly speaking, = I don't think a code is an enumeration.
An enumeration is = a detailed account, in which each thing is specially = noticed.
However, 'code' and 'enumeration' are = sometimes used for the same thing.
It is something = like a language shortcut.

Ok - I'm all for precision of expression.=A0 = We have:

-=A0a code is a coding system used for transmitting messages = requiring brevity or secrecy
-=A0a classification is a group of people or = things arranged by class or category
-=A0an enumeration is a detailed account, in which each thing is = specially noticed

And we have the = rule that "the order of the atoms induces a hierarchy", so each = of:

meta.code.class.enum,
meta.code.enum.class,
meta.class.code.enum,
meta.class.enum.code,
meta.enum.class.code, and
meta.enum.code.class

are distinctly = different in the obvious way :-)

they will have to look at the examples and that will solve the = ambiguity.
That is why we need to provide = examples.
Learning by example allows to grasp the = basics more easily.

I haven't heard anybody argue against = providing examples, but the assertions of solving ambiguities and = grasping basics should be challenged by providing IVOA beta testers with = such examples and requesting they a) describe the meaning of the = examples, and b) use the knowledge gained to create new UCDs = representing various concepts.

I suggest this worthy goal continue:=A0 "The = UCD working group has tried to resist the temptation to allow the UCD = syntax to be overly expressive."

Rob

= --Apple-Mail-1--383504335-- From owner-ucd-sci@eso.org Thu Jul 27 19:05:29 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6RH5MXH003483 for ; Thu, 27 Jul 2006 19:05:22 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6RH5MLk003482 for ucd-sci-outgoing; Thu, 27 Jul 2006 19:05:22 +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 (8.13.6+Sun/8.12.10) with ESMTP id k6RH5G5g003446; Thu, 27 Jul 2006 19:05:16 +0200 (MEST) Received: from mout0.freenet.de (mout0.freenet.de [194.97.50.131]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k6RH5Cum015907; Thu, 27 Jul 2006 19:05:13 +0200 (CEST) Received: from [194.97.50.135] (helo=mx2.freenet.de) by mout0.freenet.de with esmtpa (Exim 4.61) (envelope-from ) id 1G69IJ-0008CV-8w; Thu, 27 Jul 2006 19:05:07 +0200 Received: from p5484d77b.dip.t-dialin.net ([84.132.215.123] helo=[192.168.0.101]) by mx2.freenet.de with esmtpsa (ID frederic.hessman@freenet.de) (TLSv1:RC4-SHA:128) (Exim 4.62 #2) id 1G69II-0001lu-Cp; Thu, 27 Jul 2006 19:05:07 +0200 In-Reply-To: <66680684-D374-4A7F-8B7B-EFBCAAB805E6@noao.edu> References: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> <44BB83C3.3010702@eso.org> <20060725112634.oz0z4tjnk4swk8kg@webmail.sic.rm.cnr.it> <4A0BDD99-FA55-4D89-A4EF-E7D8A4F4C44A@eso.org> <44C63115.8020101@eso.org> <601CD3E3-D975-4834-965E-6A75AF222AAB@noao.edu> <74599EA8-38A5-4A92-9410-1EE6AC72AE7C@noao.edu> <44C8956F.9050101@eso.org> <66680684-D374-4A7F-8B7B-EFBCAAB805E6@noao.edu> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: multipart/alternative; boundary=Apple-Mail-59--380949433 Message-Id: <588E1AA5-556C-45ED-A04C-81A6FF94D77E@Astro.physik.Uni-Goettingen.DE> Cc: Nausicaa Delmotte From: Hessman Frederic Subject: Re: classification and code Date: Thu, 27 Jul 2006 19:05:09 +0200 To: ucd-sci@ivoa.net X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.7.27.85433 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Hessman Frederic --Apple-Mail-59--380949433 Content-Transfer-Encoding: quoted-printable Content-Type: text/plain; charset=ISO-8859-1; delsp=yes; format=flowed Rob Seaman said... > I'll say it again - users are not going to understand how to use =20 > UCDs. This may or may not be acceptable - it depends on whether =20 > our users will ever need to either parse other people's UCDs or =20 > create their own. > > More generally, the question isn't whether UCDs make *any* sense - =20 > there appears to be a defensible logic behind every individual =20 > distinction that is raised. The question is whether the same logic =20= > lies behind all choices - and further, whether the logic is stable =20 > over time. > It isn't that I don't understand the logic behind the choice - it's =20= > that many other choices are just as logical. Why make *this* choice? I think there is reason to worry if the official list of UCDs can =20 only be justified a posteriori. If nobody else feels the same way, =20 by all means continue with the adoption of the new batch. In =20 addition to versioning and a verification tool, I would then =20 reiterate my support for retaining the ability to namespace UCDs. > Ok. So *both* meta.code.class and meta.class.code are to be =20 > supported? And is our software supposed to be able to understand =20 > these razor thin distinctions and do something usefully different? > Hear, hear! Yes, the list grew in a historical process somewhat =20 organically, and yes we're all very glad that those who worked in the =20= initial development who had other things on their minds than the long-=20= term evolution, but THIS is the time - not later - to put the UCDs on =20= a firm symantic foundation and to clearly define how to create words =20 and how to clearly avoid naming a concept for which no one can find a =20= meaning. Thus, I concur that we need a very explicit and robust set of =20 guidelines, e.g. > I recommend: 0) UCD constructions DO NOT constitute a formal ontology and are = =20 intended to be clearly understood, chosen, and interpreted within the =20= context they are used. Thus, long _generic_ hierarchies should be =20 avoided (e.g. meta.code.class.enum). > 1) UCD versioning be explicit > 2) a UCD verification web service be assigned high priority = (that =20 > is, beyond checking syntax and atoms) 3) UCD words can be contracted if the uncontracted form is =20 cumbersome or if the contracted form constitutes a commonly =20 recognized abbreviation, but uncontracted forms are to be preferred =20 and length is per se no constraint. 4) UCD words should not be contracted if the meaning of the =20 contraction is not clearly understood outside of it's immediate context ... Rick ------------------------------------------------------------------------=20= ------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Institut f=FCr Astrophysik Tel. +49-551-39-5052 Friedrich-Hund-Platz 1 Fax +49-551-39-5043 37077 Goettingen Room F04-133 http://www.Astro.physik.Uni-Goettingen.de/~hessman ------------------------------------------------------------------------=20= ------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.Uni-Goettingen.de ------------------------------------------------------------------------=20= ------------------------- --Apple-Mail-59--380949433 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1
Rob Seaman = said...

I'll say it again - users are not going to = understand how to use UCDs.=A0 This may or may not be acceptable - it = depends on whether our users will ever need to either parse other = people's UCDs or create their own.

More generally, the question isn't whether = UCDs make *any* sense - there appears to be a defensible logic behind = every individual distinction that is raised.=A0 The question is whether = the same logic lies behind all choices - and further, whether the logic = is stable over time.

It isn't that I don't understand the logic = behind the choice - it's that many other choices are just as logical.=A0 = Why make *this* choice?=A0=A0

I think there is reason to worry if the = official list of UCDs can only be justified a posteriori.=A0 If nobody = else feels the same way, by all means continue with the adoption of the = new batch.=A0 In addition to versioning and a verification tool, I would = then reiterate my support for retaining the ability to namespace = UCDs.

Ok.=A0 So *both* meta.code.class and meta.class.code are to be = supported?=A0 And is our software supposed to be able to understand = these razor thin distinctions and do something usefully = different?

<= DIV>
Hear, hear!=A0 Yes, the = list grew in a historical process somewhat organically, and yes we're = all very glad that those who worked in the initial development who had = other things on their minds than the long-term evolution, but THIS is = the time - not later - to put the UCDs on a firm symantic foundation and = to clearly define how to create words and how to clearly avoid naming a = concept for which no one can find a meaning.

Thus, I concur that we need = a very explicit and robust set of guidelines, = e.g.

=A0 I = recommend:

= 0) UCD = constructions DO NOT constitute a formal ontology and are intended to be = clearly understood, chosen, and interpreted within the context they are = used.=A0 Thus, long _generic_ hierarchies should be avoided (e.g. = meta.code.class.enum).
1) UCD versioning be explicit
2) a UCD verification web service be assigned = high priority (that is, beyond checking syntax and = atoms)
3) UCD words can be contracted if = the uncontracted form is cumbersome or if the contracted form = constitutes a commonly recognized abbreviation, but uncontracted forms = are to be preferred and length is per se no constraint.
4) UCD = words should not be contracted if the meaning of the contraction is not = clearly understood outside of it's immediate context
= ...

Rick

Hessman@Astro.physi= k.Uni-Goettingen.DE
Institut f=FCr Astrophysik=A0 =A0 =A0 = =A0 =A0 Tel.=A0 +49-551-39-5052
Friedrich-Hund-Platz 1 =A0 =A0 = =A0 =A0 Fax +49-551-39-5043
37077 Goettingen =A0 =A0 =A0 =A0 =A0= =A0 =A0 =A0 Room F04-133
-----------------------= --------------------------------------------------------------------------=
MONET: a MOnitoring NEtwork of Telescopes
---------------------------------------------------------------= ----------------------------------

=

= --Apple-Mail-59--380949433-- From owner-ucd-tech@eso.org Fri Apr 27 14:53:03 2007 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 (8.13.6+Sun/8.12.10) with ESMTP id l3RCr1Qs020976 for ; Fri, 27 Apr 2007 14:53:01 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id l3RCr1Me020958 for ucd-tech-outgoing; Fri, 27 Apr 2007 14:53:01 +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 (8.13.6+Sun/8.12.10) with ESMTP id l3RCr0Au020943; Fri, 27 Apr 2007 14:53:00 +0200 (MEST) Received: from smtp1.sic.rm.cnr.it (smtp4.sic.rm.cnr.it [150.146.129.187]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id l3RCqwvM019460; Fri, 27 Apr 2007 14:52:58 +0200 (CEST) Received: from localhost (smtp4 [127.0.0.1]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP id 43FD7D00A7; Fri, 27 Apr 2007 14:52:52 +0200 (CEST) X-Virus-Scanned: amavisd-new at sic.rm.cnr.it Received: from smtp1.sic.rm.cnr.it ([127.0.0.1]) by localhost (smtp1.sic.rm.cnr.it [127.0.0.1]) (amavisd-new, port 10023) with ESMTP id Pxlpc7qmDfig; Fri, 27 Apr 2007 14:52:51 +0200 (CEST) Received: from localhost (unknown [10.1.0.33]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP; Fri, 27 Apr 2007 14:52:51 +0200 (CEST) Received: from martinez.u-strasbg.fr (martinez.u-strasbg.fr [130.79.129.134]) by webmail.sic.rm.cnr.it (Horde MIME library) with HTTP; Fri, 27 Apr 2007 14:52:51 +0200 Message-ID: <20070427145251.ix8xyoju8s0k00wg@webmail.sic.rm.cnr.it> Date: Fri, 27 Apr 2007 14:52:51 +0200 From: Andrea Preite Martinez To: semantics@ivoa.net, ucd-sci@ivoa.net, ucd-tech@ivoa.net Subject: Semantics news MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1; DelSp="Yes"; format="flowed" Content-Disposition: inline User-Agent: Internet Messaging Program (IMP) H3 (4.1.4) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.3.1.294258, Antispam-Engine: 2.5.1.298604, Antispam-Data: 2007.4.26.164934 X-Perl-Spam: Gauge=IIIIIII, Probability=7%, Report='__CD 0, __CP_URI_IN_BODY 0, __CT 0, __CTE 0, __CT_TEXT_PLAIN 0, __HAS_MSGID 0, __MIME_TEXT_ONLY 0, __MIME_VERSION 0, __SANE_MSGID 0, __USER_AGENT 0' Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id l3RCr0Au020944 Sender: owner-ucd-tech@eso.org Precedence: bulk Reply-To: Andrea Preite Martinez Dear all, here some news: UCDs: - The new UCD1+ list of words (Version 1.23) is an IVOA-REC since April 02. You can find the document in the IVOA Document repository. - As you can see in Appendix B of the document, 12 words have been deleted since last REC (Rec20051231). The following is the list
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 j8SILZYK006464 for ; Wed, 28 Sep 2005 20:21:36 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j8SILZ11006463 for ucd-sci-outgoing; Wed, 28 Sep 2005 20:21:35 +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 j8SILQYK006439; Wed, 28 Sep 2005 20:21:26 +0200 (MEST) Received: from msslty.mssl.ucl.ac.uk (msslty.mssl.ucl.ac.uk [128.40.71.164]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j8SILOhx011981; Wed, 28 Sep 2005 20:21:24 +0200 (CEST) Received: from msslta.mssl.ucl.ac.uk (msslta.mssl.ucl.ac.uk [128.40.71.124]) by msslty.mssl.ucl.ac.uk (8.12.10/8.12.10) with ESMTP id j8SIL6RY014774 (version=TLSv1/SSLv3 cipher=EDH-RSA-DES-CBC3-SHA bits=168 verify=NO); Wed, 28 Sep 2005 19:21:06 +0100 Date: Wed, 28 Sep 2005 19:21:06 +0100 (BST) From: Elizabeth Auden To: ucd@ivoa.net cc: Roy Williams , ucd-sci@ivoa.net Subject: Re: Call for contributions In-Reply-To: <7c91e618ae1dd30e11790017baf3f7d1@cacr.caltech.edu> Message-ID: References: <20050928170502.cr5855mfvtwk004o@webmail.sic.rm.cnr.it> <7c91e618ae1dd30e11790017baf3f7d1@cacr.caltech.edu> 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: 2.0.3.2, Antispam-Data: 2005.9.28.11 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 Roy, > efforts together: there is a great intellectual effort in representing > knowledge, but little emphasis on a fundamental question: WHAT ARE HOPING TO > ACHIEVE? What is needed is not grand plans for the far future, but rather a > small application or demo -- it can be very limited in scope -- so that Jo > Astronomer is interested, impressed, and perhaps surprised when she sees it. There's an ontology workshop at Strasbourg at the end of October - I'm giving a talk (and hopefully a demo, but so far I just have a logo) about a small ontology based application that will use an ontology based on VOEvent to correlate solar events in different catalogues. I'll let you know when I get past the logo stage. :) cheers, Elizabeth -- Elizabeth Auden, MSSL Holmbury St. Mary, Dorking RH5 6NT Tel: +44 (0)1483 204 276 eSDO Technical Lead, AstroGrid Developer From owner-ucd-sci@eso.org Thu Sep 29 15:25:17 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 j8TDP1mA002413 for ; Thu, 29 Sep 2005 15:25:01 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j8TDP0mk002412 for ucd-sci-outgoing; Thu, 29 Sep 2005 15:25:00 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-sci@eso.org using -f Received: from forth.hq.eso.org (forth.hq.eso.org [134.171.45.18]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j8TDOqmA002353; Thu, 29 Sep 2005 15:24:52 +0200 (MEST) Received: from [130.79.129.222] ([130.79.129.222]) (authenticated bits=0) by forth.hq.eso.org (8.12.8/8.12.8) with ESMTP id j8TDOpXQ017457 (version=TLSv1/SSLv3 cipher=RC4-SHA bits=128 verify=NOT); Thu, 29 Sep 2005 15:24:52 +0200 Mime-Version: 1.0 (Apple Message framework v623) Content-Type: text/plain; charset=US-ASCII; format=flowed Message-Id: Content-Transfer-Encoding: 7bit Cc: ucd@ivoa.net From: Alberto Micol Subject: Instrument related UCDs Date: Thu, 29 Sep 2005 15:24:51 +0200 To: ucd-sci@ivoa.net X-Mailer: Apple Mail (2.623) 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 Dear UCDers, I'm pretty aware that this email comes far too late, and I apologise for that. Still, for the next round, I think that some of the UCD descriptions should be improved to avoid confusion. But please keep reading, and imagine a naive user which might or might not have deep knowledge on how an instrument works; still s/he is given the task to assign ucds to different quantities. Here we go: E instr.background: Is it the signal induced by e.g. the electronics of the detector, or, another example, by the heat of the detector? Note: it is not to be confused with the readout noise (instr.det.noise). If the answer is yes, then... Q instr.skyLevel: ...Is it different than instr.background? If it is a "sky" level, why does it belong to instr? Also, why is it not marked with the syntax code "E"? Q instr.det.psf: Is this the FWHM of the PSF, or the PSF itself? Maybe a better description to clarify... And why is it associated to instr.det? Usually the PSF is the product of the convolution of various components starting from the seeing; is this just only the component induced by the instrument optics (including the telescope itself), or is it really meant to be the component coming from the fact that the detector is sampled into pixels? I would think that the ucd for PSF FWHM is: phys.size;phys.resolution;instr (but phys.resolution does not exist). instr.precision: Is it the sampling precision, or e.g. the astrometric accuracy? instr.det.qe, instr.sensitivity: At first sight one might think that those two ucds are equivalent! I would recommend to change the description of instr.sensitivity to actually explicit the fact that the sensitivity includes BOTH the detector QE AND the transmission of the optics (at least that is my guess!). Q instr.tel: Is it suppose to be the name of the telescope? Or is it just only an adjective (in which case Q should be changed to S)? Q instr.tel.focalLength exists; what about instr.tel.diameter? Let me end this with TRANSMISSION: Regarding transmission I would like to see explicited in the text that phys.transm is actually the covolution of various things, eg.: phys.transm = instr.sensitivity * instr.filter.transm (where I assume that instr.sensitivity = instr.det.qe * instr.optics.transm and notice that I invented the last one, which does not exist) I think we have to make very clear such distinctions, otherwise people will use e.g. instr.sensitivity, while they mean phys.transm, or viceversa! Alberto From owner-ucd-sci@eso.org Fri Oct 7 13:49:23 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 j97BmrC5002390 for ; Fri, 7 Oct 2005 13:48:54 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j97BmrkW002389 for ucd-sci-outgoing; Fri, 7 Oct 2005 13:48:53 +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 j97BmmC5002370 for ; Fri, 7 Oct 2005 13:48:49 +0200 (MEST) Received: from ms0.astro.physik.uni-goettingen.de (ms0.astro.physik.uni-goettingen.de [134.76.204.32]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j97Bmlin022412 for ; Fri, 7 Oct 2005 13:48:47 +0200 (CEST) Received: from sisley.astro.physik.uni-goettingen.de ([134.76.205.209]) by ms0.astro.physik.uni-goettingen.de with esmtp (Exim 4.44) id 1ENqiO-0004c6-2V for ucd-sci@ivoa.net; Fri, 07 Oct 2005 13:48:40 +0200 Mime-Version: 1.0 (Apple Message framework v728) In-Reply-To: <20050928170502.cr5855mfvtwk004o@webmail.sic.rm.cnr.it> References: <20050928170502.cr5855mfvtwk004o@webmail.sic.rm.cnr.it> Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <10BB23A9-4F20-49E4-8B11-14C4B7821A7B@astro.physik.uni-goettingen.de> Content-Transfer-Encoding: 7bit From: "Frederic V. \"Rick\" Hessman" Subject: UCDs and Ontology Workshop Date: Fri, 7 Oct 2005 13:48:39 +0200 To: ucd-sci@ivoa.net X-Mailer: Apple Mail (2.728) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.2, Antispam-Data: 2005.10.7.8 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 Dear Andrea, I noticed that the CDS is hosting an ontology workshop, but there are no details on the internet. Is this sufficiently related to our discussion of UCDs that I should be interested in attending (since I wanted to drop by anyway sometime), or is this a closed and/or technical workshop for pundits? Rick From owner-ucd-sci@eso.org Tue Oct 18 17:53:03 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 j9IFqksQ012462 for ; Tue, 18 Oct 2005 17:52:46 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j9IFqk3o012461 for ucd-sci-outgoing; Tue, 18 Oct 2005 17:52:46 +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 j9IFqasQ012426; Tue, 18 Oct 2005 17:52:36 +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 j9IFqYZq018462; Tue, 18 Oct 2005 17:52:35 +0200 (CEST) Received: from localhost (localhost.localdomain [127.0.0.1]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP id AEBE2C74AA; Tue, 18 Oct 2005 17:52:16 +0200 (CEST) Received: from smtp1.sic.rm.cnr.it ([127.0.0.1]) by localhost (smtp1 [127.0.0.1]) (amavisd-new, port 10023) with ESMTP id 08119-07; Tue, 18 Oct 2005 17:52:16 +0200 (CEST) Received: from localhost (unknown [10.1.0.7]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP; Tue, 18 Oct 2005 17:52:15 +0200 (CEST) Received: from martinez.u-strasbg.fr (martinez.u-strasbg.fr [130.79.129.134]) by webmail.sic.rm.cnr.it (Horde) with HTTP for ; Tue, 18 Oct 2005 17:52:25 +0200 Message-ID: <20051018175225.oye1p5on6kq8s84s@webmail.sic.rm.cnr.it> Date: Tue, 18 Oct 2005 17:52:25 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Cc: ucd@ivoa.net Subject: IVOA Note on UCD maintenance 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-Virus-Scanned: by amavisd-new X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2005.10.18.14 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear member, at the recent InterOp meeting in Madrid I got the action to prepare a document desribing in detail the procedure to follow in order to maintain the standard list of UCD words. Together with Sebastien we wrote a draft document that I uploaded in the IVOA document area as a Note: "Maintenance of the list of UCD words. Ver.1.0" ( http://www.ivoa.net/Documents/Notes/ ... I still don't have the link to the note) Before sending it to the TCC I'd appreciate comments on the text !! Regards Andrea ============================================================================== Andrea Preite Martinez andrea.preitemartinez@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 CDS :+33.3.90242473 ============================================================================== From owner-ucd-sci@eso.org Tue Oct 18 19:54:58 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 j9IHslsQ010514 for ; Tue, 18 Oct 2005 19:54:47 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j9IHsljh010513 for ucd-sci-outgoing; Tue, 18 Oct 2005 19:54:47 +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 j9IHsZsQ010477; Tue, 18 Oct 2005 19:54:36 +0200 (MEST) Received: from parker.sim.ucm.es (parker.sim.ucm.es [147.96.1.105]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j9IHsYe4009826; Tue, 18 Oct 2005 19:54:34 +0200 (CEST) Received: from parker.sim.ucm.es (parker.sim.ucm.es [127.0.0.1]) by localhost.ucm.es (Postfix) with ESMTP id ED1EA2F4363; Tue, 18 Oct 2005 19:54:26 +0200 (CEST) Received: from ODISEO.sim.ucm.es (unknown [10.150.1.32]) by parker.sim.ucm.es (Postfix) with ESMTP id D48C12F414D; Tue, 18 Oct 2005 19:54:26 +0200 (CEST) Received: from taurus.mat.ucm.es ([147.96.19.251]) by ODISEO.sim.ucm.es (Sun Java System Messaging Server 6.1 HotFix 0.11 (built Jan 28 2005)) with ESMTP id <0IOK002UMHQS8DE0@ODISEO.sim.ucm.es>; Tue, 18 Oct 2005 19:54:28 +0200 (CEST) Date: Tue, 18 Oct 2005 19:53:51 +0200 (CEST) From: Ana Ines Gomez de Castro Subject: Re: IVOA Note on UCD maintenance In-reply-to: <20051018175225.oye1p5on6kq8s84s@webmail.sic.rm.cnr.it> To: ucd-sci@ivoa.net Cc: ucd@ivoa.net Message-id: 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: 2.1.0.0, Antispam-Data: 2005.10.18.18 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 Dear Andrea, I've read the document and have some questions (maybe because I didn't attend the InterOp meeting). Here they are! 1. Why do you need two bodies "the scientific board" and the "semantics WG" to approve a new UCD?. Do you envission the SciBoard a "technical body" and the "Semantics WG" a "political-coordinating body"? >From our previous experience, I think that to accept a new UCD we require: - To test that the proposed new UCD cannot be made as a combination of the already existing. - To check that it is scientifically meaningful Is the SciBoard going to be responsible of both duties? 2. I assume that the rigidity in the updating of the UCD list (the list is updated during the InterOp meetings) is caused by the fact that once a new UCD is accepted the data providers have to include it in their "protocols", am I right? 3. Concerning the web based form... don't you think that it would be good to have a Comments field where the "history" of the UCD approval/disapproval is recorded?. It is feasible that a scientist, after receiving the notification of "rejection" answers to the SciBoard providing new reasons for the inclusion of the UCD word, eventually some of these reasons maybe relevant and the SciBoard may reconsider the rejection. I have not the slighlest idea about the degree of activity we might expect from the Community BUT it maybe a good policy to keep all the "rejected UCDs" in data base so, any time someone wish to propose a new UCD, the data base can be cross-checked so some time can be saved to the Chair of the SciBoard. Maybe this list could be accessible to the Community. 4. I do not understand well why on the on hand, it may be necessary to insert rapidly a new UCD (with the "temporary namespace "ivoa:"") and at the same time accept that the list of UCD's is updated in time-scales of InterOp meetings. Hope it helps!. Please, do not waste time answering the questions that have been already discussed at the InterOp meetings, just let me know. Cheers, Ana Prof. Ana I. Gomez de Castro Instituto de Astronomia y Geodesia (CSIC-UCM) Fac. de CC Matematicas Universidad Complutense de Madrid 28040 Madrid, Spain Ph. 34-913944578 (office) 34-659783338 (mobile) Email: aig@mat.ucm.es On Tue, 18 Oct 2005, Andrea Preite Martinez wrote: > Dear member, > > at the recent InterOp meeting in Madrid I got the action to prepare a > document desribing in detail the procedure to follow in order to maintain > the standard list of UCD words. > > Together with Sebastien we wrote a draft document that I uploaded in the > IVOA document area as a Note: "Maintenance of the list of UCD words. > Ver.1.0" > ( http://www.ivoa.net/Documents/Notes/ ... I still don't have the link to > the note) > > Before sending it to the TCC I'd appreciate comments on the text !! > > Regards > > Andrea > > > ============================================================================== > Andrea Preite Martinez andrea.preitemartinez@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 CDS :+33.3.90242473 > ============================================================================== > > -- Prof. Ana I. Gomez de Castro Instituto de Astronomia y Geodesia (CSIC-UCM) Fac. de CC Matematicas Universidad Complutense de Madrid 28040 Madrid, Spain Ph. 34-913944578 (office) 34-659783338 (mobile) Email: aig@mat.ucm.es From owner-ucd-sci@eso.org Wed Oct 19 08:50:40 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 j9J6oV8m011963 for ; Wed, 19 Oct 2005 08:50:32 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j9J6oVHZ011962 for ucd-sci-outgoing; Wed, 19 Oct 2005 08:50:31 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-sci@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 j9J6oH8m011925; Wed, 19 Oct 2005 08:50:17 +0200 (MEST) Received: from [134.171.27.27] (ga010247.ads.eso.org [134.171.27.27]) by serapis.hq.eso.org (8.11.7+Sun/8.11.7) with ESMTP id j9J6oHP22727; Wed, 19 Oct 2005 08:50:17 +0200 (MEST) Message-ID: <4355ECA9.1010805@eso.org> Date: Wed, 19 Oct 2005 08:50:17 +0200 From: Nausicaa Delmotte Organization: ESO User-Agent: Mozilla Thunderbird 1.0.7-1.1.fc3 (X11/20050929) X-Accept-Language: en-us, en MIME-Version: 1.0 To: ucd-sci@ivoa.net CC: ucd@ivoa.net Subject: Re: IVOA Note on UCD maintenance References: In-Reply-To: Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit 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 Dear all, Ana Ines Gomez de Castro wrote: > 3. Concerning the web based form... don't you think that it would be > good to have a Comments field where the "history" of the UCD > approval/disapproval is recorded?. It is feasible that a scientist, > after receiving the notification of "rejection" answers to the SciBoard > providing new reasons for the inclusion of the UCD word, eventually some > of these reasons maybe relevant and the SciBoard may reconsider the > rejection. > > I have not the slighlest idea about the degree of activity we might > expect from the Community BUT it maybe a good policy to keep all the > "rejected UCDs" in data base so, any time someone wish to propose a new > UCD, the data base can be cross-checked so some time can be saved to > the Chair of the SciBoard. Maybe this list could be accessible to the > Community. Yes, keeping track of the rejected UCD words in a database/file/... would be indeed very nice for future reference. Else, or in addition, maybe we could add a 'status flag' field to the form, so that we could 'sort by' status (rejected, temporary, accepted) and date. Cheers Nausicaa From owner-ucd-sci@eso.org Wed Oct 19 11:38:18 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 j9J9cA8m010656 for ; Wed, 19 Oct 2005 11:38:10 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j9J9cA1R010655 for ucd-sci-outgoing; Wed, 19 Oct 2005 11:38:10 +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 j9J9c58m010628 for ; Wed, 19 Oct 2005 11:38:05 +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 j9J9c3Zq004722 for ; Wed, 19 Oct 2005 11:38:03 +0200 (CEST) Received: from localhost (localhost.localdomain [127.0.0.1]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP id 20E08C74CD for ; Wed, 19 Oct 2005 11:37:56 +0200 (CEST) Received: from smtp1.sic.rm.cnr.it ([127.0.0.1]) by localhost (smtp1 [127.0.0.1]) (amavisd-new, port 10023) with ESMTP id 07273-01 for ; Wed, 19 Oct 2005 11:37:55 +0200 (CEST) Received: from localhost (unknown [10.1.0.7]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP for ; Wed, 19 Oct 2005 11:37:55 +0200 (CEST) Received: from martinez.u-strasbg.fr (martinez.u-strasbg.fr [130.79.129.134]) by webmail.sic.rm.cnr.it (Horde) with HTTP for ; Wed, 19 Oct 2005 11:37:55 +0200 Message-ID: <20051019113755.pyduajhv0ee1c8sw@webmail.sic.rm.cnr.it> Date: Wed, 19 Oct 2005 11:37:55 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Re: IVOA Note on UCD maintenance References: 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-Virus-Scanned: by amavisd-new X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2005.10.19.0 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Ana, let me use your comments to clarify some of the issues (especially for those not present at the last InterOp meeting): Quoting Ana Ines Gomez de Castro : > > 1. Why do you need two bodies "the scientific board" and the "semantics > WG" to approve a new UCD?. Do you envission the SciBoard a "technical > body" and the "Semantics WG" a "political-coordinating body"? > Up to now the WG "UCDs" was taking care only of UCDs. At the InterOp meeting the mission (and consequently the name) of the WG has been broadened to cover: - UCDs: Maintenance of the list of UCD words; - Semantics: definition of standard vocabulary(ies) in the fields covered by IVOA activities; - Ontologies: explore what, how, why. The Sci-Board and the WG are not two separate bodies/entities: the Sci-Board is a group working within the WG to fulfill one of the missions of the WG. The final responsibility towards the IVOA Exec and the community at large resides in the WG (the Board has been appointed by the WG, not by the Exec). > From our previous experience, I think that to accept a new UCD we require: > - To test that the proposed new UCD cannot be made as a combination of the > already existing. > - To check that it is scientifically meaningful > Is the SciBoard going to be responsible of both duties? > Right so. I'd add that the proposed modification should be considered non only meaningful, but also used/useful. The list of UCDs is not a data model. > 2. I assume that the rigidity in the updating of the UCD list (the > list is updated during the InterOp meetings) is caused by the fact > that once a new UCD is accepted the data providers have to include it > in their "protocols", am I right? > In short, yes. You probably noticed that the procedure is rather "informal" and "asynchronous" at the beginning (RFM, discussion in the Board) and it becomes more "formal" in its second part (the actual update of the list). This is because in the IVOA there is only one way to establish (or re-establish, as in this case) what is an "IVOA standard" and how. > 3. Concerning the web based form... don't you think that it would be > good to have a Comments field where the "history" of the UCD > approval/disapproval is recorded?. It is feasible that a scientist, > after receiving the notification of "rejection" answers to the SciBoard > providing new reasons for the inclusion of the UCD word, eventually some > of these reasons maybe relevant and the SciBoard may reconsider the > rejection. > First of all, let me say that the actual page at http://vizier.u-strasbg.fr/UCD/cgi-bin/comment/ucdComments is only a test page, still to be upgraded to fulfil the requested needs. But the page is already an interface to a database of ALL requests (showing the "history", as you say). The RFM form is accessible from this page. As for the case of "new reasons" for a resubmission, well why not resubmitting! You won't lose the thread (already activated by user, by date, by ucd). All this answers also your next comment: > I have not the slighlest idea about the degree of activity we might > expect from the Community BUT it maybe a good policy to keep all the > "rejected UCDs" in data base so, any time someone wish to propose a new > UCD, the data base can be cross-checked so some time can be saved to > the Chair of the SciBoard. Maybe this list could be accessible to the > Community. > > 4. I do not understand well why on the on hand, it may be necessary to > insert rapidly a new UCD (with the "temporary namespace "ivoa:"") and > at the same time accept that the list of UCD's is updated in time-scales > of InterOp meetings. > This is just because the time-scale of the process of approving an IVOA Recommendation starting from the status of WD can take a few months (>2)! > Hope it helps!. Yes, indeed! Cheers, Andrea ============================================================================== Andrea Preite Martinez andrea.preitemartinez@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 CDS :+33.3.90242473 ============================================================================== From owner-ucd-sci@eso.org Wed Oct 19 11:48:55 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 j9J9mm8m012594 for ; Wed, 19 Oct 2005 11:48:48 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j9J9mmrv012593 for ucd-sci-outgoing; Wed, 19 Oct 2005 11:48:48 +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 j9J9ma8m012562; Wed, 19 Oct 2005 11:48:37 +0200 (MEST) Received: from esa-av-smtp2.gmessaging.net (esa-av-smtp2.gmessaging.net [194.51.201.23]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j9J9mVe4015506; Wed, 19 Oct 2005 11:48:31 +0200 (CEST) Received: from esa-spas2.gmessaging.net (relay2 [172.24.21.39]) by esa-av-smtp2.gmessaging.net (iPlanet Messaging Server 5.2 Patch 2 (built Jul 14 2004)) with ESMTP id <0IOL00AEJPWLXU@esa-av-smtp2.gmessaging.net>; Wed, 19 Oct 2005 11:48:21 +0200 (MEST) Received: from localhost (esa-spas2 [127.0.0.1]) by esa-spas2.gmessaging.net (Postfix) with ESMTP id 14A3A219E4A; Wed, 19 Oct 2005 11:48:25 +0200 (CEST) Received: from esa-spas2.gmessaging.net ([127.0.0.1]) by localhost (esa-spas2 [127.0.0.1]) (amavisd-new, port 10024) with ESMTP id 09251-02; Wed, 19 Oct 2005 11:48:23 +0200 (CEST) Received: from sciops-mailgw.vilspa.esa.int (sciops-mailgw.vilspa.esa.int [193.147.152.105]) by esa-spas2.gmessaging.net (Postfix) with ESMTP id E13BC219E43; Wed, 19 Oct 2005 11:48:22 +0200 (CEST) Received: from iso.vilspa.esa.es (isous5.vilspa.esa.es [193.147.153.100]) by sciops-mailgw.vilspa.esa.int (Postfix) with ESMTP id 0764411FAC4; Wed, 19 Oct 2005 11:48:23 +0200 (CEST) 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 j9J9mMVH005411; Wed, 19 Oct 2005 11:48:22 +0200 (MEST) Date: Wed, 19 Oct 2005 11:48:22 +0200 From: Pedro Osuna Subject: Re: IVOA Note on UCD maintenance In-reply-to: <20051018175225.oye1p5on6kq8s84s@webmail.sic.rm.cnr.it> To: ucd@ivoa.net Cc: Pedro.Osuna@esa.int, ucd-sci@ivoa.net Message-id: <1129715301.23228.1769.camel@isol03.vilspa.esa.int> MIME-version: 1.0 X-Mailer: Ximian Evolution 1.4.5 (1.4.5-14) Content-type: text/plain Content-transfer-encoding: 7BIT X-Spam-Score: Content analysis details: (-1.2 points, 4.5 points required to be considered as spam) -1.2 BAYES_00 BODY: Bayesian spam probability is 0 to 1% [score: 0.0000] References: <20051018175225.oye1p5on6kq8s84s@webmail.sic.rm.cnr.it> X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2005.10.19.3 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 Dear Andrea, I think the procedure is quite thorough and reflects all the steps we suggested in the initial document on UCD. I am worried though about allowing the identifier "ivoa:" as namespace for those UCDs already approved but temporarily out of the UCD standard (as this one will only be updated once or twice a year). What this might end up is with loads of systems using not-yet-standard UCDs, different from one proposal to the other, and all of them starting with the same identifier "ivoa:". Even worse, probably the data provider will write the "ivoa:" ucd, and probably won't change it to the "real" one when the UCD is standardised. A possible solution for this problem would be to allow for specific namespaces for specific needs (let's say, like a "solar:" namespace for solar physics specific UCDs) but this again seems to go in the debate on whether this should be relegated to data models or not, which I think is not worth to retake now. Just my two cents. Cheers, P. On Tue, 2005-10-18 at 17:52, Andrea Preite Martinez wrote: > Dear member, > > at the recent InterOp meeting in Madrid I got the action to prepare a > document desribing in detail the procedure to follow in order to maintain > the standard list of UCD words. > > Together with Sebastien we wrote a draft document that I uploaded in the > IVOA document area as a Note: "Maintenance of the list of UCD words. > Ver.1.0" > ( http://www.ivoa.net/Documents/Notes/ ... I still don't have the link to > the note) > > Before sending it to the TCC I'd appreciate comments on the text !! > > Regards > > Andrea > > > ============================================================================== > Andrea Preite Martinez andrea.preitemartinez@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 CDS :+33.3.90242473 > ============================================================================== -- Pedro Osuna Alcalaya ESA Science Archives System Engineer Science Archive Team European Space Astronomy Centre (ESAC/ESA) e-mail: Pedro.Osuna@esa.int Tel + 34 91 8131314 --------------------------------- European Space Astronomy Centre European Space Agency P.O. Box 50727 E-28080 Villafranca del Castillo MADRID - SPAIN From owner-ucd-sci@eso.org Wed Oct 19 12:10:39 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 j9JAAW8m017320 for ; Wed, 19 Oct 2005 12:10:32 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j9JAAW2A017319 for ucd-sci-outgoing; Wed, 19 Oct 2005 12:10:32 +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 j9JAAK8m017209; Wed, 19 Oct 2005 12:10:21 +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 j9JAAJZq006025; Wed, 19 Oct 2005 12:10:19 +0200 (CEST) Received: from katrine.roe.ac.uk (localhost.localdomain [127.0.0.1]) by katrine.roe.ac.uk (Postfix) with ESMTP id 1D0DB1842B; Wed, 19 Oct 2005 11:10:14 +0100 (BST) Received: from somehost by katrine.roe.ac.uk (postfixilter 1.4) with SMTP id 7179; Wed, 19 Oct 2005 11:10:12 +0100 (BST) Received: from katrine (localhost.localdomain [127.0.0.1]) by localhost (Postfix) with ESMTP id C1DFF18261; Wed, 19 Oct 2005 11:10:12 +0100 (BST) Received: from localhost.localdomain ([127.0.0.1]) by katrine.roe.ac.uk (MailMonitor for SMTP v1.2.2 ) ; Wed, 19 Oct 2005 11:10:12 +0100 (BST) Received: from egilsay.roe.ac.uk (egilsay.roe.ac.uk [195.194.120.103]) by katrine.roe.ac.uk (Postfix) with ESMTP id 8FFAD18261; Wed, 19 Oct 2005 11:10:12 +0100 (BST) Date: Wed, 19 Oct 2005 11:10:12 +0100 (BST) From: Bob Mann To: ucd@ivoa.net Cc: ucd-sci@ivoa.net Subject: Re: IVOA Note on UCD maintenance In-Reply-To: <20051018175225.oye1p5on6kq8s84s@webmail.sic.rm.cnr.it> Message-ID: References: <20051018175225.oye1p5on6kq8s84s@webmail.sic.rm.cnr.it> MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed X-Spam-Checker-Version: SpamAssassin 2.62 (2004-01-11) on katrine.roe.ac.uk X-Spam-Level: X-Spam-Status: No, hits=0.0 required=1000.0 tests=none autolearn=no version=2.62 X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2005.10.19.4 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 folks, My only comment on this is to ask whether it is better to have each RFM sent out to the Scientific Board as soon as it is submitted or whether they should be collected over a period (three months?) and have the Scientific Board then debate those RFMs which have accumulated during that period. My question is really based on own experience and working habits. If I see an email arriving about a single proposed UCD amendment I'm probably unlikely to take time to consider it if I'm busy, whereas, if I know I have a few hours' work to do every quarter I'm more likely to set aside a period of time for doing that work properly. What do other people think? cheers Bob From owner-ucd-sci@eso.org Wed Oct 19 16:03:50 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 j9JE3g8m012106 for ; Wed, 19 Oct 2005 16:03:42 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j9JE3gx9012105 for ucd-sci-outgoing; Wed, 19 Oct 2005 16:03:42 +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 j9JE3V8m012063; Wed, 19 Oct 2005 16:03:31 +0200 (MEST) Received: from fed1rmmtao02.cox.net (fed1rmmtao02.cox.net [68.230.241.37]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j9JE3SZq018784; Wed, 19 Oct 2005 16:03:29 +0200 (CEST) Received: from [10.0.1.129] (really [68.231.133.145]) by fed1rmmtao02.cox.net (InterMail vM.6.01.05.02 201-2131-123-102-20050715) with ESMTP id <20051019140252.XYAB29216.fed1rmmtao02.cox.net@[10.0.1.129]>; Wed, 19 Oct 2005 10:02:52 -0400 In-Reply-To: <1129715301.23228.1769.camel@isol03.vilspa.esa.int> References: <20051018175225.oye1p5on6kq8s84s@webmail.sic.rm.cnr.it> <1129715301.23228.1769.camel@isol03.vilspa.esa.int> Mime-Version: 1.0 (Apple Message framework v734) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <14DE598C-6B6D-41EB-BDB9-CCAE567AE8B9@noao.edu> Content-Transfer-Encoding: 7bit From: Rob Seaman Subject: Re: IVOA Note on UCD maintenance Date: Wed, 19 Oct 2005 07:03:21 -0700 To: ucd-sci@ivoa.net, ucd@ivoa.net X-Mailer: Apple Mail (2.734) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2005.10.19.12 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 Pedro Osuna wrote: > I am worried though about allowing the identifier "ivoa:" as namespace > for those UCDs already approved but temporarily out of the UCD > standard > (as this one will only be updated once or twice a year). Section 2 of the v1.1 UCD standard seems to state that "ivoa;" is equivalent to the default namespace. It is unclear what distinction is being drawn here between "approved" and "not yet standard". On the other hand, I am very heartened that the UCD committee(s) have reached the point of recognizing that at least some alternative namespaces are necessary. > A possible solution for this problem would be to allow for specific > namespaces for specific needs (let's say, like a "solar:" namespace > for > solar physics specific UCDs) The standard already does: "The use of namespaces, indicated by the presence of a colon in the word, is possible..." This is also discussed in section 2, which goes on to attempt to dissuade their use: "but should be avoided as far as possible." I believe this to be a vain hope. The way to control the looming complexity of UCDs is precisely to spread the responsibility (and pain) around. This reminds me of the "image" extension specification for FITS, which tries to convince users that it is both bad - and worse, unnecessary - to create data-less primary header data units. What did the community immediately do with image extensions? I'm tempted to leave that as a rhetorical question - but what we did was to discover an excellent usage for subclassing metadata between the primary headers and the extension headers and for stuffing all the data into the extensions. UCD namespaces are inevitable. Bob Mann wrote: > My only comment on this is to ask whether it is better to have > each RFM sent out to the Scientific Board as soon as it is submitted > or whether they should be collected over a period (three months?) By all means, although I might suggest a monthly cadence. There should also be a mechanism for expedited discussions for UCDs which are needed "yesterday". Note, however, that the pressure for immediate decision-making would also be relieved by the availability of namespaces. Rob Seaman National Optical Astronomy Observatory From owner-ucd-sci@eso.org Mon Nov 7 16:48:42 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 jA7FmYaj026919 for ; Mon, 7 Nov 2005 16:48:34 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id jA7FmYBY026918 for ucd-sci-outgoing; Mon, 7 Nov 2005 16:48:34 +0100 (MET) 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 jA7FmKaj026876; Mon, 7 Nov 2005 16:48:21 +0100 (MET) Received: from smtp1.sic.rm.cnr.it (smtp1.sic.rm.cnr.it [150.146.129.253]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id jA7FmIZq005814; Mon, 7 Nov 2005 16:48:19 +0100 (CET) Received: from localhost (localhost.localdomain [127.0.0.1]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP id 18C34C7422; Mon, 7 Nov 2005 16:48:09 +0100 (CET) Received: from smtp1.sic.rm.cnr.it ([127.0.0.1]) by localhost (smtp1 [127.0.0.1]) (amavisd-new, port 10023) with ESMTP id 14673-05; Mon, 7 Nov 2005 16:48:03 +0100 (CET) Received: from localhost (unknown [10.1.0.7]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP; Mon, 7 Nov 2005 16:47:57 +0100 (CET) Received: from martinez.u-strasbg.fr (martinez.u-strasbg.fr [130.79.129.134]) by webmail.sic.rm.cnr.it (Horde MIME library) with HTTP; Mon, 07 Nov 2005 16:47:55 +0100 Message-ID: <20051107164755.cwtk98wgjvq8gkk8@webmail.sic.rm.cnr.it> Date: Mon, 07 Nov 2005 16:47:55 +0100 From: Andrea Preite Martinez To: ucd@ivoa.net, ucd-sci@ivoa.net Subject: 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 (4.0.4) X-Virus-Scanned: by amavisd-new X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2005.11.7.14 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear all, I received from the IVOA Exec a request to modify all UCD1+ words that do not conform to what is said in the standard UCD document, i.e.: UCD1+ words at the same level in the hierarchy cannot be a starting substring of another that is, we cannot have phot.flux and phot.fluxDens As you know, the document at http://www.ivoa.net/Documents/latest/UCDlist.html is in the PR status, and will be moved to IVOA Recommendation after an appropriate action on the words concerned. The rule mentioned above is violated for the following ucd1+ words: E | phot.fluxDens | Flux density (per wl/freq/energy interval) E | phot.fluxDens.sb | Flux density surface brightness Q | phys.atmol | Atomic and molecular physics (shared properties) Q | phys.atmol.branchingRatio | Branching ratio Q | phys.atmol.coll | Related to collisions Q | phys.atmol.configuration | Configuration Q | phys.atmol.crossSection | Atomic / molecular cross-section Q | phys.atmol.element | Element Q | phys.atmol.excitation | Atomic molecular excitation parameter Q | phys.atmol.final | Quantity refers to atomic/molecular final/ground state, level, ecc. Q | phys.atmol.initial | Quantity refers to atomic/molecular initial state, level, ecc. Q | phys.atmol.ion | Ion S | phys.atmol.ionization | Related to ionization S | phys.atmol.level | Atomic level Q | phys.atmol.lifetime | Lifetime of a level Q | phys.atmol.lineShift | Line shifting coefficient Q | phys.atmol.parity | Parity Q | phys.atmol.sweight | Statistical weight S | phys.atmol.trans | Transition between states Q | phys.energyDensity | Energy-density Q | phys.massToLight | Mass to light ratio Q | phys.massYield | Mass yield because of the already existing words phot.flux phys.at phys.energy phys.mass In order to reach a rapid convergence on the reformulation of these words, I?m suggesting a possible solution for each of them in the list that follows: Present Suggested new E | phot.fluxDens | phot.flux.fluxDens or: phot.flux.density E | phot.fluxDens.sb | phot.flux.fluxDens.sb or: phot.flux.density.sb Q | phys.atmol | suppress Q | phys.atmol.branchingRatio | phys.branchingRatio Q | phys.atmol.coll | phys.collision Q | phys.atmol.configuration | phys.state.configuration Q | phys.atmol.crossSection | phys.crossSection Q | phys.atmol.element | phys.element Q | phys.atmol.excitation | phys.excitation Q | phys.atmol.final | phys.state.final Q | phys.atmol.initial | phys.state.initial Q | phys.atmol.ion | phys.element.ion S | phys.atmol.ionization | phys.ionization S | phys.atmol.level | phys.level Q | phys.atmol.lifetime | phys.level.lifetime Q | phys.atmol.lineShift | phys.lineShift Q | phys.atmol.parity | phys.state.parity Q | phys.atmol.sweight | phys.state.sweight S | phys.atmol.trans | phys.state.trans Q | phys.energyDensity | phys.energy.density Q | phys.massToLight | phys.mass.light Q | phys.massYield | phys.mass.yield The other possibility for the phys.atmol.xxx group is to suppress the word phys.at Please let me know your opinion and/or your suggestions. Andrea ============================================================================== Andrea Preite Martinez andrea.preitemartinez@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:+39.320.43.15.383 00133 Roma CDS :+33.3.90242473 ============================================================================== From owner-ucd-sci@eso.org Mon Nov 7 17:35:28 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 jA7GZMaj005975 for ; Mon, 7 Nov 2005 17:35:22 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id jA7GZLQm005974 for ucd-sci-outgoing; Mon, 7 Nov 2005 17:35:21 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-sci@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 jA7GZHaj005967; Mon, 7 Nov 2005 17:35:17 +0100 (MET) 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 jA7GZH47032103 (version=TLSv1/SSLv3 cipher=RC4-SHA bits=128 verify=NOT); Mon, 7 Nov 2005 17:35:17 +0100 In-Reply-To: <20051107164755.cwtk98wgjvq8gkk8@webmail.sic.rm.cnr.it> References: <20051107164755.cwtk98wgjvq8gkk8@webmail.sic.rm.cnr.it> Mime-Version: 1.0 (Apple Message framework v623) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <718d8e4897942ec4822d14397eb0ceb2@eso.org> Content-Transfer-Encoding: 7bit Cc: ucd@ivoa.net From: Alberto Micol Subject: Re: Date: Mon, 7 Nov 2005 17:35:16 +0100 To: ucd-sci@ivoa.net X-Mailer: Apple Mail (2.623) 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 Andrea, Sorry to come back with this, but there is another possibility... If we state that each UCD word MUST end with the ';' character, -that is, even if there are no other subsequent words- then no UCD can ever be a substring of another one. Example: phot.flux; is not a substring of phot.fluxDens; The beauty of it is that no other changes are required. It is my laziness... I always prefer to change the least... Alberto PS: I send this email because I'm sure you are expecting it from me ;-) PPS: And I promise that this is the last time I mention this. On Nov 7, 2005, at 16:47, Andrea Preite Martinez wrote: > Dear all, > > I received from the IVOA Exec a request to modify all UCD1+ words that > do not conform to what is said in the standard UCD document, i.e.: > > UCD1+ words at the same level in the hierarchy cannot be a starting > substring of another > > that is, we cannot have phot.flux and phot.fluxDens > > As you know, the document at > http://www.ivoa.net/Documents/latest/UCDlist.html > is in the PR status, and will be moved to IVOA Recommendation after an > appropriate action on the words concerned. > > The rule mentioned above is violated for the following ucd1+ words: > > E | phot.fluxDens | Flux density (per wl/freq/energy > interval) > E | phot.fluxDens.sb | Flux density surface brightness > Q | phys.atmol | Atomic and molecular physics (shared > properties) > Q | phys.atmol.branchingRatio | Branching ratio > Q | phys.atmol.coll | Related to collisions > Q | phys.atmol.configuration | Configuration > Q | phys.atmol.crossSection | Atomic / molecular cross-section > Q | phys.atmol.element | Element > Q | phys.atmol.excitation | Atomic molecular excitation parameter > Q | phys.atmol.final | Quantity refers to atomic/molecular > final/ground state, level, ecc. > Q | phys.atmol.initial | Quantity refers to atomic/molecular > initial state, level, ecc. > Q | phys.atmol.ion | Ion > S | phys.atmol.ionization | Related to ionization > S | phys.atmol.level | Atomic level > Q | phys.atmol.lifetime | Lifetime of a level > Q | phys.atmol.lineShift | Line shifting coefficient > Q | phys.atmol.parity | Parity > Q | phys.atmol.sweight | Statistical weight > S | phys.atmol.trans | Transition between states > Q | phys.energyDensity | Energy-density > Q | phys.massToLight | Mass to light ratio > Q | phys.massYield | Mass yield > > because of the already existing words > phot.flux > phys.at > phys.energy > phys.mass > > In order to reach a rapid convergence on the reformulation of these > words, I?m suggesting a possible solution for each of them in the list > that follows: > > Present Suggested new > E | phot.fluxDens | phot.flux.fluxDens or: > phot.flux.density > E | phot.fluxDens.sb | phot.flux.fluxDens.sb or: > phot.flux.density.sb > Q | phys.atmol | suppress > Q | phys.atmol.branchingRatio | phys.branchingRatio > Q | phys.atmol.coll | phys.collision > Q | phys.atmol.configuration | phys.state.configuration > Q | phys.atmol.crossSection | phys.crossSection > Q | phys.atmol.element | phys.element > Q | phys.atmol.excitation | phys.excitation > Q | phys.atmol.final | phys.state.final > Q | phys.atmol.initial | phys.state.initial > Q | phys.atmol.ion | phys.element.ion S | > phys.atmol.ionization | phys.ionization > S | phys.atmol.level | phys.level > Q | phys.atmol.lifetime | phys.level.lifetime > Q | phys.atmol.lineShift | phys.lineShift > Q | phys.atmol.parity | phys.state.parity > Q | phys.atmol.sweight | phys.state.sweight > S | phys.atmol.trans | phys.state.trans Q | > phys.energyDensity | phys.energy.density > Q | phys.massToLight | phys.mass.light > Q | phys.massYield | phys.mass.yield > > The other possibility for the phys.atmol.xxx group is to suppress the > word phys.at > > Please let me know your opinion and/or your suggestions. > > Andrea > > > ======================================================================= > ======= > Andrea Preite Martinez > andrea.preitemartinez@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:+39.320.43.15.383 > 00133 Roma CDS :+33.3.90242473 > ======================================================================= > ======= > > Alberto Micol ST-ECF HST Archive Scientist From owner-ucd-sci@eso.org Mon Nov 7 17:45:12 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 jA7Gixaj007953 for ; Mon, 7 Nov 2005 17:44:59 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id jA7GixjH007952 for ucd-sci-outgoing; Mon, 7 Nov 2005 17:44:59 +0100 (MET) 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 jA7Gilaj007840; Mon, 7 Nov 2005 17:44:47 +0100 (MET) 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 jA7GijZq008368; Mon, 7 Nov 2005 17:44:45 +0100 (CET) Received: from pisaure.intra.cea.fr (pisaure.intra.cea.fr [132.166.88.38]) by cirse.extra.cea.fr (8.13.4/8.13.4/CEAnet-Internet.5.0) with ESMTP id jA7GiUGY026678; Mon, 7 Nov 2005 17:44:35 +0100 (MET) 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 jA7Gd5ga028672; Mon, 7 Nov 2005 17:39:06 +0100 (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+PROTO) with ESMTP id jA7GiTa8018180; Mon, 7 Nov 2005 17:44:29 +0100 (MET) 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 jA7GjMbh017235 ; Mon, 7 Nov 2005 17:45:22 +0100 (MET) Message-ID: <436F846C.3010009@cea.fr> Date: Mon, 07 Nov 2005 17:44:28 +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: ucd-sci@ivoa.net CC: ucd@ivoa.net Subject: Re: References: <20051107164755.cwtk98wgjvq8gkk8@webmail.sic.rm.cnr.it> In-Reply-To: <20051107164755.cwtk98wgjvq8gkk8@webmail.sic.rm.cnr.it> 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: 2.1.0.0, Antispam-Data: 2005.11.7.14 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 Andrea Preite Martinez wrote: > Dear all, > > I received from the IVOA Exec a request to modify all UCD1+ words that > do not conform to what is said in the standard UCD document, i.e.: > > UCD1+ words at the same level in the hierarchy cannot be a starting > substring of another > > that is, we cannot have phot.flux and phot.fluxDens > > As you know, the document at > http://www.ivoa.net/Documents/latest/UCDlist.html > is in the PR status, and will be moved to IVOA Recommendation after an > appropriate action on the words concerned. > > The rule mentioned above is violated for the following ucd1+ words: > > E | phot.fluxDens | Flux density (per wl/freq/energy interval) > E | phot.fluxDens.sb | Flux density surface brightness > Q | phys.atmol | Atomic and molecular physics (shared properties) [SNIP]... > Q | phys.energyDensity | Energy-density > Q | phys.massToLight | Mass to light ratio > Q | phys.massYield | Mass yield > > because of the already existing words > phot.flux > phys.at > phys.energy > phys.mass > > In order to reach a rapid convergence on the reformulation of these > words, I?m suggesting a possible solution for each of them in the list > that follows: > > Present Suggested new > E | phot.fluxDens | phot.flux.fluxDens or: phot.flux.density > E | phot.fluxDens.sb | phot.flux.fluxDens.sb or: phot.flux.density.sb The second formulation seems more logical but then fluxDens atom desapear, is this a pb? [SNIP] > > The other possibility for the phys.atmol.xxx group is to suppress the > word phys.at why not modifying phys.at.xxx group to phys.atom.xxx > > Please let me know your opinion and/or your suggestions. > > Andrea > > > ============================================================================== > > Andrea Preite Martinez > andrea.preitemartinez@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:+39.320.43.15.383 > 00133 Roma CDS :+33.3.90242473 > ============================================================================== > > > SY -- 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/ ------------------------------------------------------------------ From owner-ucd-sci@eso.org Mon Nov 7 18:27:21 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 jA7HRFaj015297 for ; Mon, 7 Nov 2005 18:27:15 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id jA7HRFK5015296 for ucd-sci-outgoing; Mon, 7 Nov 2005 18:27:15 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-sci@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 jA7HR6aj015281; Mon, 7 Nov 2005 18:27:06 +0100 (MET) Received: from [134.171.27.27] (ga010247.ads.eso.org [134.171.27.27]) by serapis.hq.eso.org (8.11.7+Sun/8.11.7) with ESMTP id jA7HR6P03513; Mon, 7 Nov 2005 18:27:06 +0100 (MET) Message-ID: <436F8E6A.3000107@eso.org> Date: Mon, 07 Nov 2005 18:27:06 +0100 From: Nausicaa Delmotte Organization: ESO User-Agent: Mozilla Thunderbird 1.0.7-1.1.fc3 (X11/20050929) X-Accept-Language: en-us, en MIME-Version: 1.0 To: ucd-sci@ivoa.net CC: ucd@ivoa.net Subject: Re: References: <20051107164755.cwtk98wgjvq8gkk8@webmail.sic.rm.cnr.it> <718d8e4897942ec4822d14397eb0ceb2@eso.org> In-Reply-To: <718d8e4897942ec4822d14397eb0ceb2@eso.org> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit 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, But what is preventing us from adding the semicolon as ending separator? I do apologize for asking a question that seems to have already been answered in the past, but I could not find the answer in the archive mailing-list and since I did not follow all the UCD developments from the very beginning, probably I missed something. Could anybody give me a pointer to a discussion or a very brief comment on it? Or is it maybe to avoid having a possible NULL word at the end when parsing a UCD, assuming the ending semicolon? Thank you Nausicaa Alberto Micol wrote: > > Hi Andrea, > > Sorry to come back with this, but there is another possibility... > If we state that each UCD word MUST end with the ';' character, > -that is, even if there are no other subsequent words- then > no UCD can ever be a substring of another one. > > Example: > > phot.flux; is not a substring of phot.fluxDens; > > The beauty of it is that no other changes are required. > > It is my laziness... I always prefer to change the least... > > Alberto > PS: I send this email because I'm sure you are expecting it from me ;-) > PPS: And I promise that this is the last time I mention this. > > On Nov 7, 2005, at 16:47, Andrea Preite Martinez wrote: > >> Dear all, >> >> I received from the IVOA Exec a request to modify all UCD1+ words >> that do not conform to what is said in the standard UCD document, i.e.: >> >> UCD1+ words at the same level in the hierarchy cannot be a starting >> substring of another >> >> that is, we cannot have phot.flux and phot.fluxDens >> >> As you know, the document at >> http://www.ivoa.net/Documents/latest/UCDlist.html >> is in the PR status, and will be moved to IVOA Recommendation after >> an appropriate action on the words concerned. >> >> The rule mentioned above is violated for the following ucd1+ words: >> >> E | phot.fluxDens | Flux density (per wl/freq/energy >> interval) >> E | phot.fluxDens.sb | Flux density surface brightness >> Q | phys.atmol | Atomic and molecular physics >> (shared properties) >> Q | phys.atmol.branchingRatio | Branching ratio >> Q | phys.atmol.coll | Related to collisions >> Q | phys.atmol.configuration | Configuration >> Q | phys.atmol.crossSection | Atomic / molecular cross-section >> Q | phys.atmol.element | Element >> Q | phys.atmol.excitation | Atomic molecular excitation parameter >> Q | phys.atmol.final | Quantity refers to atomic/molecular >> final/ground state, level, ecc. >> Q | phys.atmol.initial | Quantity refers to atomic/molecular >> initial state, level, ecc. >> Q | phys.atmol.ion | Ion >> S | phys.atmol.ionization | Related to ionization >> S | phys.atmol.level | Atomic level >> Q | phys.atmol.lifetime | Lifetime of a level >> Q | phys.atmol.lineShift | Line shifting coefficient >> Q | phys.atmol.parity | Parity >> Q | phys.atmol.sweight | Statistical weight >> S | phys.atmol.trans | Transition between states >> Q | phys.energyDensity | Energy-density >> Q | phys.massToLight | Mass to light ratio >> Q | phys.massYield | Mass yield >> >> because of the already existing words >> phot.flux >> phys.at >> phys.energy >> phys.mass >> >> In order to reach a rapid convergence on the reformulation of these >> words, I?m suggesting a possible solution for each of them in the >> list that follows: >> >> Present Suggested new >> E | phot.fluxDens | phot.flux.fluxDens or: >> phot.flux.density >> E | phot.fluxDens.sb | phot.flux.fluxDens.sb or: >> phot.flux.density.sb >> Q | phys.atmol | suppress >> Q | phys.atmol.branchingRatio | phys.branchingRatio >> Q | phys.atmol.coll | phys.collision >> Q | phys.atmol.configuration | phys.state.configuration >> Q | phys.atmol.crossSection | phys.crossSection >> Q | phys.atmol.element | phys.element >> Q | phys.atmol.excitation | phys.excitation >> Q | phys.atmol.final | phys.state.final >> Q | phys.atmol.initial | phys.state.initial >> Q | phys.atmol.ion | phys.element.ion S | >> phys.atmol.ionization | phys.ionization >> S | phys.atmol.level | phys.level >> Q | phys.atmol.lifetime | phys.level.lifetime >> Q | phys.atmol.lineShift | phys.lineShift >> Q | phys.atmol.parity | phys.state.parity >> Q | phys.atmol.sweight | phys.state.sweight >> S | phys.atmol.trans | phys.state.trans Q | >> phys.energyDensity | phys.energy.density >> Q | phys.massToLight | phys.mass.light >> Q | phys.massYield | phys.mass.yield >> >> The other possibility for the phys.atmol.xxx group is to suppress the >> word phys.at >> >> Please let me know your opinion and/or your suggestions. >> >> Andrea >> >> >> ======================================================================= >> ======= >> Andrea Preite Martinez >> andrea.preitemartinez@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:+39.320.43.15.383 >> 00133 Roma CDS :+33.3.90242473 >> ======================================================================= >> ======= >> >> > Alberto Micol > ST-ECF HST Archive Scientist -- Dr Nausicaa Delmotte @..@ ndelmott@eso.org European Southern Observatory (----) Tel: +49 (0)89 3200 6418 Karl-Schwarzschild-Str. 2 ( >__< ) Fax: +49 (0)89 3200 6480 D-85748 Garching bei Muenchen ^^ ~~ ^^ http://www.eso.org/~ndelmott/ From owner-ucd-sci@eso.org Tue Nov 8 05:21:43 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 jA84Lbhj018956 for ; Tue, 8 Nov 2005 05:21:38 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id jA84LbmU018955 for ucd-sci-outgoing; Tue, 8 Nov 2005 05:21:37 +0100 (MET) 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 jA84LThj018943; Tue, 8 Nov 2005 05:21:30 +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 jA84LRe4020350; Tue, 8 Nov 2005 05:21:28 +0100 (CET) Received: from sothis.cfa.harvard.edu (sothis [131.142.52.147]) by head.cfa.harvard.edu (d/w) with ESMTP id jA84LLrx020679; Mon, 7 Nov 2005 23:21:21 -0500 (EST) From: Jonathan McDowell Received: (from jcm@localhost) by sothis.cfa.harvard.edu (8.12.8p1/8.12.8) id jA84LL8f004051; Mon, 7 Nov 2005 23:21:21 -0500 (EST) Date: Mon, 7 Nov 2005 23:21:21 -0500 (EST) Message-Id: <200511080421.jA84LL8f004051@sothis.cfa.harvard.edu> To: ucd-sci@ivoa.net, ucd@ivoa.net Subject: Re: X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2005.11.7.38 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 Dear Andrea and others, 1) In the first place, I never liked that rule. Alberto's suggestion could be implemented in the UCD-analysing software - in other words, I don't actually bother adding a terminal semicolon to my phot.fluxDens but when you pass it to your search/comparison tool, a trailing semicolon gets added automatically phot.fluxDens; This is a classic case of wanting to avoid writing 3 lines of code, and making things annoying for human readability and comprehension. 2) Nevertheless, the rule is what we adopted. > Present Suggested new > E | phot.fluxDens | phot.flux.fluxDens or: > phot.flux.density > E | phot.fluxDens.sb | phot.flux.fluxDens.sb or: > phot.flux.density.sb I agree that the second choices phot.flux.density.* are better. (Pierre - I don't think losing the fluxDens atom is a problem.) OK: > Q | phys.energyDensity | phys.energy.density I don't like this, since it's not a mass, it's a ratio. It's really talking about the composition of the physical environment (how much baryons, how much photons, etc.) Maybe phys.composition.massLight (or phys.abund.massLight) > Q | phys.massToLight | phys.mass.light Can you remind me what this means exactly? Is it a percentage, or e.g. an SNe yield of iron in solar masses? > Q | phys.massYield | phys.mass.yield I don't like suppressing the atmol element. It makes the UCDs too flat. We could just make them all "at" and explain that "at" includes "atmol". But if we are willing to make a bigger change, we can take something from the work of the DM At/Mol team: some of these items are species (atmol, particle), some are states (levels), some are transitions and interactions. I think it's clear that states and levels are associated with particles in a way that phys.mass.yield is not, so I would be in favor of > Q | phys.atmol | suppress > Q | phys.atmol.element | phys.species.element > Q | phys.atmol.excitation | phys.species.excitation > Q | phys.atmol.ion | phys.species.ion > S | phys.atmol.ionization | phys.species.ionization Q | phys.at.number | phys.species.atomicNumber Q | phys.at.weight | phys.species.weight > Q | phys.atmol.branchingRatio | phys.transition.branchingRatio > Q | phys.atmol.coll | phys.transition.collision > Q | phys.atmol.crossSection | phys.transition.crossSection > Q | phys.atmol.lineShift | phys.transition.lineShift > S | phys.atmol.trans | phys.transition.trans Q | phys.at.collStrength | phys.transition.collStrength Q | phys.at.damping | phys.transition.damping Q | phys.at.lande | phys.transition.Lande factor Q | phys.at.oscStrength | phys.transition.oscStrength Q | phys.at.radiationType | phys.transition.radiationType Q | phys.at.term | phys.transition.term Q | phys.at.transProb | phys.transition.prob Q | phys.at.wOscStrength | phys.transition.wOscStrength > Q | phys.atmol.parity | phys.state.parity > Q | phys.atmol.sweight | phys.state.sweight > Q | phys.atmol.configuration | phys.state.configuration > Q | phys.atmol.final | phys.state.final > Q | phys.atmol.initial | phys.state.initial > S | phys.atmol.level | phys.state.level > Q | phys.atmol.lifetime | phys.state.lifetime Q | phys.at.qn | phys.state.qn Q | phys.at.qn.I | phys.state.qn.I - Jonathan From owner-ucd-sci@eso.org Tue Nov 8 10:29:18 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 jA89TBcZ004845 for ; Tue, 8 Nov 2005 10:29:11 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id jA89TBpo004844 for ucd-sci-outgoing; Tue, 8 Nov 2005 10:29:11 +0100 (MET) 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 jA89T7cZ004836; Tue, 8 Nov 2005 10:29:07 +0100 (MET) Received: from ms0.astro.physik.uni-goettingen.de (ms0.astro.physik.uni-goettingen.de [134.76.204.32]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id jA89T5Zq011406; Tue, 8 Nov 2005 10:29:05 +0100 (CET) Received: from sisley.astro.physik.uni-goettingen.de ([134.76.205.209]) by ms0.astro.physik.uni-goettingen.de with esmtp (Exim 4.44) id 1EZPml-0000g6-VN; Tue, 08 Nov 2005 10:29:00 +0100 In-Reply-To: <200511080421.jA84LL8f004051@sothis.cfa.harvard.edu> References: <200511080421.jA84LL8f004051@sothis.cfa.harvard.edu> Mime-Version: 1.0 (Apple Message framework v734) Content-Type: multipart/alternative; boundary=Apple-Mail-18-663600752 Message-Id: <0F56C61F-8EAD-4A51-AF9E-53F3504D730D@astro.physik.uni-goettingen.de> Cc: ucd@ivoa.net From: "Frederic V. \"Rick\" Hessman" Subject: Re: Re: Date: Tue, 8 Nov 2005 10:28:59 +0100 To: ucd-sci@ivoa.net X-Mailer: Apple Mail (2.734) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2005.11.8.0 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 --Apple-Mail-18-663600752 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed > >> Present Suggested new >> E | phot.fluxDens | phot.flux.fluxDens or: >> phot.flux.density >> E | phot.fluxDens.sb | phot.flux.fluxDens.sb or: >> phot.flux.density.sb >> > > I agree that the second choices phot.flux.density.* are better. > (Pierre - I don't think losing the fluxDens atom is a problem.) Don't want to step on any radio astronomer's toes, but flux density is flux. Yes, I know, it's monochromatic flux per unit frequency, but where's the distinction between bolometric flux, monochromatic flux per unit frequency, and monochromatic flux per unit wavelength? Do we also then have to support the use of candela's, lux's, and the lot - also physical (even SI!) terms for the same things? How about (see, e.g., Mihalas): phot.flux generic net rate of radiant energy flow per unit area and time phot.flux.freq monochromatic flux per unit frequency, flux density phot.flux.wave monochromatic flux per unit wavelength phot.flux.bol bolometric flux phot.flux.Eddington Eddington flux = flux / 4PI I was going to suggest adding phot.flux.astr (that terrible factor of PI or /1PI, depending upon how you look at it!), but I won't...... >>> Q | phys.massToLight | phys.mass.light >>> > I don't like this, since it's not a mass, it's a ratio. > It's really talking about the composition of the physical > environment (how much baryons, how much photons, etc.) > Maybe phys.composition.massLight (or phys.abund.massLight) I prefer phys.composition.massLightRatio Rick --Apple-Mail-18-663600752 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1

=A0=A0 Present =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = =A0 Suggested new
E | = phot.fluxDens =A0 =A0 =A0 =A0 =A0 = =A0 =A0 | phot.flux.fluxDens=A0= or: =A0
phot.flux.density
E | = phot.fluxDens.sb=A0 =A0 =A0 =A0 =A0 = =A0 | phot.flux.fluxDens.sb=A0= or: =A0
phot.flux.density.sb


I agree = that the second choices phot.flux.density.* are better.
(Pierre - I don't think losing the fluxDens atom is = a problem.)

Don't want to step on any radio = astronomer's toes, but flux density is flux. =A0 =A0Yes, I know, it's = monochromatic flux per unit frequency, but where's the distinction = between bolometric flux, monochromatic flux per unit frequency, and = monochromatic flux per unit wavelength?=A0 Do we also then have to = support the use of candela's, lux's, and the lot - also physical (even = SI!) terms for the same things?=A0 How about (see, e.g., = Mihalas):

=A0=A0= =A0 phot.flux =A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0generic = net rate of radiant energy flow per unit area and time
=A0=A0=A0= phot.flux.freq=A0 =A0 =A0=A0 =A0=A0 =A0=A0 =A0monochromatic flux per = unit frequency, flux density
=A0=A0=A0 phot.flux.wave=A0 =A0 = =A0=A0 =A0=A0 =A0monochromatic flux per unit wavelength
=A0=A0=A0= phot.flux.bol =A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0bolometric = flux
=A0=A0=A0 phot.flux.Eddington=A0 =A0Eddington flux =3D = flux / 4PI
=A0=A0
I was going to suggest adding=A0 = phot.flux.astr (that terrible factor of PI or /1PI, depending upon how = you look at it!), but I won't......

Q | phys.massToLight=A0 =A0 =A0 =A0 =A0 =A0 | = phys.mass.light

I don't like this, since it's not a mass, it's a = ratio.
It's really talking about the = composition of the physical
environment = (how much baryons, how much photons, etc.)
Maybe = phys.composition.massLight (or = phys.abund.massLight)

I prefer = phys.composition.massLightRatio

Rick
= --Apple-Mail-18-663600752-- From owner-ucd-sci@eso.org Tue Nov 8 11:53:59 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 jA8ArrcZ010171 for ; Tue, 8 Nov 2005 11:53:53 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id jA8ArqqH010169 for ucd-sci-outgoing; Tue, 8 Nov 2005 11:53:52 +0100 (MET) 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 jA8ArQcZ009896; Tue, 8 Nov 2005 11:53:26 +0100 (MET) Received: from ms0.astro.physik.uni-goettingen.de (ms0.astro.physik.uni-goettingen.de [134.76.204.32]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id jA8ArOe4002001; Tue, 8 Nov 2005 11:53:25 +0100 (CET) Received: from sisley.astro.physik.uni-goettingen.de ([134.76.205.209]) by ms0.astro.physik.uni-goettingen.de with esmtp (Exim 4.44) id 1EZR6N-0000zO-7Y; Tue, 08 Nov 2005 11:53:19 +0100 In-Reply-To: <0F56C61F-8EAD-4A51-AF9E-53F3504D730D@astro.physik.uni-goettingen.de> References: <200511080421.jA84LL8f004051@sothis.cfa.harvard.edu> <0F56C61F-8EAD-4A51-AF9E-53F3504D730D@astro.physik.uni-goettingen.de> Mime-Version: 1.0 (Apple Message framework v734) Content-Type: multipart/alternative; boundary=Apple-Mail-20-668659969 Message-Id: <315AEB18-8F62-4864-864D-82DEBC808069@astro.physik.uni-goettingen.de> Cc: ucd@ivoa.net From: "Frederic V. \"Rick\" Hessman" Subject: phot.flux - an Addendum Date: Tue, 8 Nov 2005 11:53:18 +0100 To: ucd-sci@ivoa.net X-Mailer: Apple Mail (2.734) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2005.11.8.3 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-20-668659969 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed > Don't want to step on any radio astronomer's toes, but flux density > is flux. Yes, I know, it's monochromatic flux per unit > frequency, but where's the distinction between bolometric flux, > monochromatic flux per unit frequency, and monochromatic flux per > unit wavelength? Do we also then have to support the use of > candela's, lux's, and the lot - also physical (even SI!) terms for > the same things? How about (see, e.g., Mihalas): > > phot.flux generic net rate of radiant > energy flow per unit area and time > phot.flux.freq monochromatic flux per unit > frequency, flux density > phot.flux.wave monochromatic flux per unit wavelength > phot.flux.bol bolometric flux > phot.flux.Eddington Eddington flux = flux / 4PI > > I was going to suggest adding phot.flux.astr (that terrible factor > of PI or /1PI, depending upon how you look at it!), but I won't...... Sorry - should have re-read the 1.02 documentation: "flux density" has been generalized beyond it's normal use. How do we then distinguish between the many different forms? By units alone, i.e. non-UCD things? That works fine for things like lengths and times and masses, since the physical quantities are well defined beyond their units, but F_nu and F_lambda are totally different quantities and this fact is utterly independent of the units. Perhaps phot.flux.perFreq phot.flux.perWave phot.flux.perEnergy phot.flux.perWavenumber phot.flux.perDecade nu*F_nu, lambda*F_lambda,... Looking at the current list, I'd also like to complain about phot.flux.sb Since when is surface brightness a flux? Surface brightness is an intensity and intensity != flux. So... phot.intensity generic directed rate of radiant energy flow per unit area, time, and solid angle, surface brightness phot.intensity.bol (not generally needed, but here for symmetry) phot.intensity.perFreq phot.intensity.perWave phot.intensity.perEnergy phot.intensity.perWavenumber phot.intensity.perDecade (Ibid.) I know this is a bit of a change, but I frankly didn't notice before.... sorry! Rick --Apple-Mail-20-668659969 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1
Don't = want to step on any radio astronomer's toes, but flux density is flux. =A0= =A0Yes, I know, it's monochromatic flux per unit frequency, but where's = the distinction between bolometric flux, monochromatic flux per unit = frequency, and monochromatic flux per unit wavelength?=A0 Do we also = then have to support the use of candela's, lux's, and the lot - also = physical (even SI!) terms for the same things?=A0 How about (see, e.g., = Mihalas):

=A0=A0= =A0 phot.flux =A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0generic = net rate of radiant energy flow per unit area and time
=A0=A0=A0= phot.flux.freq=A0 =A0 =A0=A0 =A0=A0 =A0=A0 =A0monochromatic flux per = unit frequency, flux density
=A0=A0=A0 phot.flux.wave=A0 =A0 = =A0=A0 =A0=A0 =A0monochromatic flux per unit wavelength
=A0=A0=A0= phot.flux.bol =A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0bolometric = flux
=A0=A0=A0 phot.flux.Eddington=A0 =A0Eddington flux =3D = flux / 4PI
=A0=A0
I was going to suggest adding=A0 = phot.flux.astr (that terrible factor of PI or /1PI, depending upon how = you look at it!), but I won't......

Sorry - should have re-read = the 1.02 documentation: "flux density" has been generalized beyond it's = normal use.=A0 How do we then
distinguish between the = many different forms?=A0 By units alone, i.e. non-UCD things?=A0 That = works fine for things like lengths and times and masses, since the = physical quantities are well defined beyond their units, but F_nu and = F_lambda are totally different quantities and this fact is utterly = independent of the units.

Perhaps

=A0=A0 =A0=A0 = =A0phot.flux.perFreq
=A0 =A0 =A0=A0 = =A0phot.flux.perWave
=A0 =A0 =A0=A0 = =A0phot.flux.perEnergy
=A0 =A0 =A0=A0 = =A0phot.flux.perWavenumber
=A0 =A0 =A0=A0 = =A0phot.flux.perDecade =A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0nu*F_nu, = lambda*F_lambda,...

Looking at the current = list, I'd also like to complain about

=A0=A0=A0 = phot.flux.sb

Since when is surface = brightness a flux?=A0 =A0Surface brightness is an intensity and = intensity !=3D flux.=A0 So...

=A0=A0=A0 phot.intensity=A0 = =A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 = =A0generic directed rate of radiant energy flow per unit area, time, and = solid angle, surface brightness
=A0=A0=A0 = phot.intensity.bol =A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 = =A0(not generally needed, but here for symmetry)
=A0=A0=A0 = phot.intensity.perFreq
=A0=A0=A0 = phot.intensity.perWave
=A0=A0=A0 = phot.intensity.perEnergy
=A0=A0=A0 = phot.intensity.perWavenumber
=A0=A0=A0 = phot.intensity.perDecade=A0 =A0=A0 =A0=A0 =A0=A0 = =A0(Ibid.)

I know this is a bit of a = change, but I frankly didn't notice before.... = sorry!

Rick
= --Apple-Mail-20-668659969-- From owner-ucd-sci@eso.org Tue Nov 8 14:54:39 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 jA8DsWcZ015477 for ; Tue, 8 Nov 2005 14:54:32 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id jA8DsWPu015474 for ucd-sci-outgoing; Tue, 8 Nov 2005 14:54:32 +0100 (MET) 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 jA8DrvcZ015295; Tue, 8 Nov 2005 14:53:57 +0100 (MET) 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 jA8Drte4009342; Tue, 8 Nov 2005 14:53:55 +0100 (CET) Received: from localhost (localhost.localdomain [127.0.0.1]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP id 3B34BC73F2; Tue, 8 Nov 2005 14:53:47 +0100 (CET) Received: from smtp1.sic.rm.cnr.it ([127.0.0.1]) by localhost (smtp1 [127.0.0.1]) (amavisd-new, port 10023) with ESMTP id 21628-09; Tue, 8 Nov 2005 14:53:46 +0100 (CET) Received: from localhost (unknown [10.1.0.7]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP; Tue, 8 Nov 2005 14:53:45 +0100 (CET) Received: from martinez.u-strasbg.fr (martinez.u-strasbg.fr [130.79.129.134]) by webmail.sic.rm.cnr.it (Horde MIME library) with HTTP; Tue, 08 Nov 2005 14:53:45 +0100 Message-ID: <20051108145345.trrx6vmck0oc8g8s@webmail.sic.rm.cnr.it> Date: Tue, 08 Nov 2005 14:53:45 +0100 From: Andrea Preite Martinez To: ucd@ivoa.net, ucd-sci@ivoa.net Cc: Robert Hanisch Subject: UCDlist document update 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 (4.0.4) X-Virus-Scanned: by amavisd-new X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2005.11.8.9 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 Dear all, after a first round of comments and suggestions, let me summarize: 1. I think it will be unwise to re-open the discussion on the already standard UCD main document (thus de-classing it back to WD) to ease the approval of a second standard, just because we are too lazy to find a reasonable spelling for a few words! 2. Let?s keep changes to a minimum. I found suggestions on the atmol and flux/sb words very interesting and worth discussing with more time and care. Shortly we will know how to do it ! (http://www.ivoa.net/Documents/latest/UCDmaintenance.html) 3. atmol: I think the simplest solution in this particular case is to change the words phys.at.* into phys.atomic.* 4. ?obtorto collo? (we do it, but we whould have preferred not to do it!) we go for phot.flux.density* and phys.energy.density 5. phys.massToLight can become phys.composition.massLightRatio (indeed the ratio has to do with the barionic composition of galaxies or clusters of galaxies) 6. phys.massYield can become phys.composition.yield (also in this case the new version is better than the old one - mass just indicated units) I will wait for a few more days before changing the list of words. Cheers Andrea ============================================================================== Andrea Preite Martinez andrea.preitemartinez@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 CDS :+33.3.90242473 ============================================================================== From owner-ucd-sci@eso.org Tue Nov 8 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 jA8EjncZ027783 for ; Tue, 8 Nov 2005 15:45:49 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id jA8Ejnwp027782 for ucd-sci-outgoing; Tue, 8 Nov 2005 15:45:49 +0100 (MET) 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 jA8EjZcZ027730; Tue, 8 Nov 2005 15:45:35 +0100 (MET) Received: from esa-av-smtp2.gmessaging.net (esa-av-smtp2.gmessaging.net [194.51.201.23]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id jA8EjXe4012067; Tue, 8 Nov 2005 15:45:33 +0100 (CET) Received: from esa-spas2.gmessaging.net (relay2 [172.24.21.39]) by esa-av-smtp2.gmessaging.net (iPlanet Messaging Server 5.2 Patch 2 (built Jul 14 2004)) with ESMTP id <0IPN00KRS4ZNRH@esa-av-smtp2.gmessaging.net>; Tue, 08 Nov 2005 15:45:23 +0100 (MET) Received: from localhost (esa-spas2 [127.0.0.1]) by esa-spas2.gmessaging.net (Postfix) with ESMTP id 9C25B219EDD; Tue, 08 Nov 2005 15:45:26 +0100 (CET) Received: from esa-spas2.gmessaging.net ([127.0.0.1]) by localhost (esa-spas2 [127.0.0.1]) (amavisd-new, port 10024) with ESMTP id 06259-07; Tue, 08 Nov 2005 15:45:24 +0100 (CET) Received: from sciops-mailgw.vilspa.esa.int (sciops-mailgw.vilspa.esa.int [193.147.152.105]) by esa-spas2.gmessaging.net (Postfix) with ESMTP id 67C55219ED2; Tue, 08 Nov 2005 15:45:24 +0100 (CET) Received: from iso.vilspa.esa.es (isous5.vilspa.esa.es [193.147.153.100]) by sciops-mailgw.vilspa.esa.int (Postfix) with ESMTP id C619211F8F0; Tue, 08 Nov 2005 15:45:24 +0100 (CET) Received: from isol03.vilspa.esa.int (IDENT:U2FsdGVkX19NSAMfRde+x43Yc6Nb704KCtTMMuW4kv8@isol03.vilspa.esa.int [193.147.153.17]) by iso.vilspa.esa.es (8.12.10/8.12.10) with ESMTP id jA8EjNDH018895; Tue, 08 Nov 2005 15:45:23 +0100 (MET) Date: Tue, 08 Nov 2005 15:45:23 +0100 From: Pedro Osuna Subject: Re: UCDlist document update In-reply-to: <20051108145345.trrx6vmck0oc8g8s@webmail.sic.rm.cnr.it> To: ucd@ivoa.net Cc: Pedro.Osuna@esa.int, ucd-sci@ivoa.net, Bob Hanisch Message-id: <1131461123.32035.196.camel@isol03.vilspa.esa.int> MIME-version: 1.0 X-Mailer: Evolution 2.0.2 (2.0.2-22) Content-type: text/plain Content-transfer-encoding: 7BIT X-Spam-Score: Content analysis details: (-0.0 points, 4.5 points required to be considered as spam) 0.6 J_CHICKENPOX_31 BODY: 3alpha-pock-1alpha 0.6 J_CHICKENPOX_45 BODY: 4alpha-pock-5alpha -1.2 BAYES_00 BODY: Bayesian spam probability is 0 to 1% [score: 0.0000] References: <20051108145345.trrx6vmck0oc8g8s@webmail.sic.rm.cnr.it> X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2005.11.8.10 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 Dear all, on the phys.atmol subject, I'd like to see Marie-Lise opinion before you write any changes, as she introduced many of the initial UCDs for that. In principle, Jonathan's new names look OK in view of our own work on Line DM, but I insist that she should say a word on it. Unfortunately, she does not seem to be on-line, so: Andrea, can this part wait until we know from her? Cheers, P. On Tue, 2005-11-08 at 14:53 +0100, Andrea Preite Martinez wrote: > Dear all, > > after a first round of comments and suggestions, let me summarize: > > 1. I think it will be unwise to re-open the discussion on the already > standard UCD main document (thus de-classing it back to WD) to ease the > approval of a second standard, just because we are too lazy to find a > reasonable spelling for a few words! > > 2. Let?s keep changes to a minimum. I found suggestions on the atmol > and flux/sb words very interesting and worth discussing with more time > and care. Shortly we will know how to do it ! > (http://www.ivoa.net/Documents/latest/UCDmaintenance.html) > > 3. atmol: I think the simplest solution in this particular case is to > change the words phys.at.* into phys.atomic.* > > 4. ?obtorto collo? (we do it, but we whould have preferred not to do > it!) we go for phot.flux.density* and phys.energy.density > > 5. phys.massToLight can become phys.composition.massLightRatio (indeed > the ratio has to do with the barionic composition of galaxies or > clusters of galaxies) > > 6. phys.massYield can become phys.composition.yield (also in this case > the new version is better than the old one - mass just indicated units) > > I will wait for a few more days before changing the list of words. > > Cheers > > Andrea > > > ============================================================================== > Andrea Preite Martinez andrea.preitemartinez@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 CDS :+33.3.90242473 > ============================================================================== > > From owner-ucd-sci@eso.org Tue Nov 8 15:55:35 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 jA8EtVcZ029713 for ; Tue, 8 Nov 2005 15:55:31 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id jA8EtVL5029712 for ucd-sci-outgoing; Tue, 8 Nov 2005 15:55:31 +0100 (MET) 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 jA8EsxcZ029549; Tue, 8 Nov 2005 15:54:59 +0100 (MET) 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 jA8EsvZq024255; Tue, 8 Nov 2005 15:54:57 +0100 (CET) Received: from astro.u-strasbg.fr (cluster.u-strasbg.fr [130.79.128.8]) by mailhost.u-strasbg.fr (8.13.3/jtpda-5.5pre1) with ESMTP id jA8EspD4003207 ; Tue, 8 Nov 2005 15:54:51 +0100 (CET) Received: (from genova@localhost) by astro.u-strasbg.fr (8.11.7p1+Sun/8.10.2) id jA8Esnx13829; Tue, 8 Nov 2005 15:54:49 +0100 (MET) Date: Tue, 8 Nov 2005 15:54:49 +0100 (MET) Message-Id: <200511081454.jA8Esnx13829@astro.u-strasbg.fr> From: genova@cluster.u-strasbg.fr (Francoise Genova) To: ucd@ivoa.net Cc: Pedro.Osuna@esa.int, hanisch@stsci.edu, ucd-sci@ivoa.net Subject: Re: UCDlist document update X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-2.0 (mailhost.u-strasbg.fr [130.79.200.157]); Tue, 08 Nov 2005 15:54:51 +0100 (CET) X-Virus-Scanned: by amavisd-new X-Virus-Status: Clean X-Spam-Status: No, score=-1.3 required=5.0 tests=ALL_TRUSTED,AWL autolearn=disabled version=3.1.0 X-Spam-Checker-Version: SpamAssassin 3.1.0 (2005-09-13) on mr7.u-strasbg.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2005.11.8.11 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Hi, Marie-Lise is presently chairing a session of the French VO school. She will have a look ASAP Cheers Francoise From owner-ucd-sci@eso.org Tue Nov 8 17:43:56 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 jA8GhmcZ021585 for ; Tue, 8 Nov 2005 17:43:48 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id jA8Ghml9021582 for ucd-sci-outgoing; Tue, 8 Nov 2005 17:43:48 +0100 (MET) 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 jA8GhfcZ021552; Tue, 8 Nov 2005 17:43:41 +0100 (MET) Received: from mesiob.obspm.fr (mesiob.obspm.fr [145.238.2.2]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id jA8GhdZq028708; Tue, 8 Nov 2005 17:43:39 +0100 (CET) Received: from mesioq.obspm.fr (mesioq.obspm.fr [145.238.2.57]) by mesiob.obspm.fr (8.13.4/8.13.4/SIO Observatoire de Paris - 01/01/03) with ESMTP id jA8GhX5j015910; Tue, 8 Nov 2005 17:43:33 +0100 Date: Tue, 8 Nov 2005 17:43:33 +0100 (CET) From: marie-lise.dubernet@obspm.fr X-X-Sender: dubernet@mesioq.obspm.fr To: ucd-sci@ivoa.net cc: ucd@ivoa.net, Pedro.Osuna@esa.int, Bob Hanisch Subject: Re: UCDlist document update In-Reply-To: <1131461123.32035.196.camel@isol03.vilspa.esa.int> Message-ID: References: <20051108145345.trrx6vmck0oc8g8s@webmail.sic.rm.cnr.it> <1131461123.32035.196.camel@isol03.vilspa.esa.int> MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-1.6 (mesiob.obspm.fr [145.238.2.2]); Tue, 08 Nov 2005 17:43:33 +0100 (CET) X-Virus-Scanned: by amavisd-new X-Virus-Status: Clean X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2005.11.7.33 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 dear all, sorry for delayed answer. the DM details are not final yet, therefore I would not advise to use the DM (even if UCD have no meaning without the DM). At present my view is to unify all quantities related to atomic and molecular physics under a single word phys.atmol.* "quantities related to atomic and molecular processes" A more complete list of UCD will be proposed once the DM is set "final". best regards marie lise On Tue, 8 Nov 2005, Pedro Osuna wrote: > Dear all, > > on the phys.atmol subject, I'd like to see Marie-Lise opinion before you > write any changes, as she introduced many of the initial UCDs for that. > In principle, Jonathan's new names look OK in view of our own work on > Line DM, but I insist that she should say a word on it. Unfortunately, > she does not seem to be on-line, so: Andrea, can this part wait until we > know from her? > > Cheers, > P. > > > On Tue, 2005-11-08 at 14:53 +0100, Andrea Preite Martinez wrote: > > Dear all, > > > > after a first round of comments and suggestions, let me summarize: > > > > 1. I think it will be unwise to re-open the discussion on the already > > standard UCD main document (thus de-classing it back to WD) to ease the > > approval of a second standard, just because we are too lazy to find a > > reasonable spelling for a few words! > > > > 2. Let?s keep changes to a minimum. I found suggestions on the atmol > > and flux/sb words very interesting and worth discussing with more time > > and care. Shortly we will know how to do it ! > > (http://www.ivoa.net/Documents/latest/UCDmaintenance.html) > > > > 3. atmol: I think the simplest solution in this particular case is to > > change the words phys.at.* into phys.atomic.* > > > > 4. ?obtorto collo? (we do it, but we whould have preferred not to do > > it!) we go for phot.flux.density* and phys.energy.density > > > > 5. phys.massToLight can become phys.composition.massLightRatio (indeed > > the ratio has to do with the barionic composition of galaxies or > > clusters of galaxies) > > > > 6. phys.massYield can become phys.composition.yield (also in this case > > the new version is better than the old one - mass just indicated units) > > > > I will wait for a few more days before changing the list of words. > > > > Cheers > > > > Andrea > > > > > > ============================================================================== > > Andrea Preite Martinez andrea.preitemartinez@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 CDS :+33.3.90242473 > > ============================================================================== > > > > > > From owner-ucd-sci@eso.org Tue Nov 8 22:20:34 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 jA8LKRcZ009210 for ; Tue, 8 Nov 2005 22:20:28 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id jA8LKRNS009209 for ucd-sci-outgoing; Tue, 8 Nov 2005 22:20:27 +0100 (MET) 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 jA8LKNcZ009205; Tue, 8 Nov 2005 22:20:23 +0100 (MET) 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 jA8LKKZq009400; Tue, 8 Nov 2005 22:20:21 +0100 (CET) X-Spam-Checker-Version: SpamAssassin 3.1.0 (2005-09-13) on noao.edu X-Spam-Level: X-Spam-Status: No, score=-5.0 required=4.5 tests=ALL_TRUSTED,AWL,BAYES_00 autolearn=ham version=3.1.0 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 4.3.8) with ESMTPSA id 21508239; Tue, 08 Nov 2005 14:20:03 -0700 In-Reply-To: <200511080421.jA84LL8f004051@sothis.cfa.harvard.edu> References: <200511080421.jA84LL8f004051@sothis.cfa.harvard.edu> Mime-Version: 1.0 (Apple Message framework v746.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: Cc: ucd@ivoa.net Content-Transfer-Encoding: 7bit From: Rob Seaman Subject: UCD verifier? Date: Tue, 8 Nov 2005 14:19:57 -0700 To: ucd-sci@ivoa.net X-Mailer: Apple Mail (2.746.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2005.11.8.24 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 Hi, > UCD1+ words at the same level in the hierarchy cannot be a starting > substring of another With the recent talk about the UCD1+ list not conforming to the UCD specification, I am prompted to wonder whether anyone is working on a UCD verifier - or perhaps one already exists? It seems to me that a tool would be very useful for verifying that a single token is a conforming UCD and that a list of same avoids various classes of name collisions and other errors. This will help individuals who want to suggest new UCDs as well as projects who may be developing their own namespaces. Rob Seaman NOAO From owner-ucd-sci@eso.org Wed Nov 9 09:24:18 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 jA98NvKi016656 for ; Wed, 9 Nov 2005 09:23:57 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id jA98NvX9016654 for ucd-sci-outgoing; Wed, 9 Nov 2005 09:23:57 +0100 (MET) 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 jA98NaKi016545 for ; Wed, 9 Nov 2005 09:23:36 +0100 (MET) Received: from smtp1.sic.rm.cnr.it (smtp1.sic.rm.cnr.it [150.146.129.253]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id jA98NYZq024814 for ; Wed, 9 Nov 2005 09:23:34 +0100 (CET) Received: from localhost (localhost.localdomain [127.0.0.1]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP id 25AE0C73E6 for ; Wed, 9 Nov 2005 09:23:27 +0100 (CET) Received: from smtp1.sic.rm.cnr.it ([127.0.0.1]) by localhost (smtp1 [127.0.0.1]) (amavisd-new, port 10023) with ESMTP id 27927-01 for ; Wed, 9 Nov 2005 09:23:26 +0100 (CET) Received: from localhost (unknown [10.1.0.7]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP for ; Wed, 9 Nov 2005 09:23:26 +0100 (CET) Received: from martinez.u-strasbg.fr (martinez.u-strasbg.fr [130.79.129.134]) by webmail.sic.rm.cnr.it (Horde MIME library) with HTTP; Wed, 09 Nov 2005 09:23:26 +0100 Message-ID: <20051109092326.ve3i452crb6s4wgs@webmail.sic.rm.cnr.it> Date: Wed, 09 Nov 2005 09:23:26 +0100 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Re: UCD verifier? References: <200511080421.jA84LL8f004051@sothis.cfa.harvard.edu> 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 (4.0.4) X-Virus-Scanned: by amavisd-new X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2005.11.8.46 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 Quoting Rob Seaman : > > With the recent talk about the UCD1+ list not conforming to the UCD > specification, I am prompted to wonder whether anyone is working on a > UCD verifier - or perhaps one already exists? Yes, try the validate tool at http://vizier.u-strasbg.fr/UCD/tools.htx Andrea From owner-ucd-sci@eso.org Wed Nov 9 14:55:48 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 jA9DtcKs024115 for ; Wed, 9 Nov 2005 14:55:38 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id jA9Dtcic024114 for ucd-sci-outgoing; Wed, 9 Nov 2005 14:55:38 +0100 (MET) 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 jA9DtXKs024107; Wed, 9 Nov 2005 14:55:34 +0100 (MET) Received: from fed1rmmtao03.cox.net (fed1rmmtao03.cox.net [68.230.241.36]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id jA9DtUZq007339; Wed, 9 Nov 2005 14:55:31 +0100 (CET) Received: from [10.0.1.99] (really [68.231.133.145]) by fed1rmmtao03.cox.net (InterMail vM.6.01.05.02 201-2131-123-102-20050715) with ESMTP id <20051109135454.PLHF4527.fed1rmmtao03.cox.net@[10.0.1.99]>; Wed, 9 Nov 2005 08:54:54 -0500 In-Reply-To: <20051109092326.ve3i452crb6s4wgs@webmail.sic.rm.cnr.it> References: <200511080421.jA84LL8f004051@sothis.cfa.harvard.edu> <20051109092326.ve3i452crb6s4wgs@webmail.sic.rm.cnr.it> Mime-Version: 1.0 (Apple Message framework v746.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: Cc: ucd@ivoa.net Content-Transfer-Encoding: 7bit From: Rob Seaman Subject: Re: UCD verifier? Date: Wed, 9 Nov 2005 06:55:26 -0700 To: ucd-sci@ivoa.net X-Mailer: Apple Mail (2.746.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2005.11.9.9 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 Nov 9, 2005, at 1:23 AM, Andrea Preite Martinez wrote: >> With the recent talk about the UCD1+ list not conforming to the >> UCD specification, I am prompted to wonder whether anyone is >> working on a UCD verifier - or perhaps one already exists? > > Yes, try the validate tool at > http://vizier.u-strasbg.fr/UCD/tools.htx Thanks. Other pointed me to that, too. The rules and meta-rules for UCD building imply that each UCD fills a niche in a larger semantic ecology. Each new UCD causes a potential challenge to all previously declared UCDs or lists or namespaces of same. The tool I was suggesting would not only test a single proposed UCD against the syntactical rules, but also test a list of same (e.g., representing a namespace) against the rules for building lists of UCDs. I suspect that the notion that two namespaces cannot contain identical UCDs (or more stringently, was it identical "words"?) will fall by the wayside, but if not, it would prove useful - almost mandatory - to have a tool to vet two lists against each other, or for instance, a newly proposed list against all previously registered namespaces. Which is to say that the choice of rules for assembling lists of UCDs is not a completely free design parameter. Rob Seaman NOAO From owner-ucd-sci@eso.org Tue Jan 3 10:20:40 2006 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 (8.12.10+Sun/8.12.10) with ESMTP id k039KUK4002933 for ; Tue, 3 Jan 2006 10:20:30 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k039KUm2002932 for ucd-sci-outgoing; Tue, 3 Jan 2006 10:20:30 +0100 (MET) 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 k039KKK4002912; Tue, 3 Jan 2006 10:20:20 +0100 (MET) 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 k039KG1r010154; Tue, 3 Jan 2006 10:20:18 +0100 (CET) Received: from localhost (localhost.localdomain [127.0.0.1]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP id 6AD5AC73EB; Tue, 3 Jan 2006 10:20:09 +0100 (CET) Received: from localhost (localhost.localdomain [127.0.0.1]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP id 4C465C73E6; Tue, 3 Jan 2006 10:20:09 +0100 (CET) Received: from smtp1.sic.rm.cnr.it ([127.0.0.1]) by localhost (smtp1 [127.0.0.1]) (amavisd-new, port 10023) with ESMTP id 09454-09; Tue, 3 Jan 2006 10:20:08 +0100 (CET) Received: from localhost (unknown [10.1.0.7]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP; Tue, 3 Jan 2006 10:20:08 +0100 (CET) Received: from martinez.u-strasbg.fr (martinez.u-strasbg.fr [130.79.129.134]) by webmail.sic.rm.cnr.it (Horde MIME library) with HTTP; Tue, 03 Jan 2006 10:20:08 +0100 Message-ID: <20060103102008.y85gtgkm7jf4844g@webmail.sic.rm.cnr.it> Date: Tue, 03 Jan 2006 10:20:08 +0100 From: Andrea Preite Martinez To: ucd@ivoa.net, ucd-sci@ivoa.net Subject: UCD news... 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 (4.0.4) X-Virus-Scanned: by amavisd-new X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2006.1.3.0 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net Dear members of the WG, first of all, a very happy new year to you all! For a good start, I'm pleased to annunce you that the UCD1+ word-list is an IVOA Recommendation from Dec 31 2005. You can find version 1.11 of the document at http://www.ivoa.net/Documents/latest/UCDlist.html Now that we have eventually the first standard list of words, it's time to start wondering how to change it! We already had a discussion on a Note on UCD1+ maintenance I submitted to the WG in October. I revised the Note according to some (if not all) of your remarks, and transformed the Note into the Working Draft that you can find at http://www.ivoa.net/Documents/latest/UCDlistMaintenance.html . I?m ready to move the document to the state of PR and request comments from the community, but before doing this I?d like to be sure that the discussion in our WG is over. So, if you still have comments or amendments to the text of the Working Draft, please do it soon. A reasonable schedule could be to have an RFC in February and to submit the PR to the Exec before the InterOp in spring. Cheers, Andrea ============================================================================== Andrea Preite Martinez andrea.preitemartinez@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 CDS :+33.3.90242473 ============================================================================== From owner-ucd@eso.org Tue Jan 3 10:21:38 2006 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 (8.12.10+Sun/8.12.10) with ESMTP id k039KPK4002923 for ; Tue, 3 Jan 2006 10:20:25 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k039KPLx002922 for ucd-outgoing; Tue, 3 Jan 2006 10:20:25 +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 k039KKK4002912; Tue, 3 Jan 2006 10:20:20 +0100 (MET) 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 k039KG1r010154; Tue, 3 Jan 2006 10:20:18 +0100 (CET) Received: from localhost (localhost.localdomain [127.0.0.1]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP id 6AD5AC73EB; Tue, 3 Jan 2006 10:20:09 +0100 (CET) Received: from localhost (localhost.localdomain [127.0.0.1]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP id 4C465C73E6; Tue, 3 Jan 2006 10:20:09 +0100 (CET) Received: from smtp1.sic.rm.cnr.it ([127.0.0.1]) by localhost (smtp1 [127.0.0.1]) (amavisd-new, port 10023) with ESMTP id 09454-09; Tue, 3 Jan 2006 10:20:08 +0100 (CET) Received: from localhost (unknown [10.1.0.7]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP; Tue, 3 Jan 2006 10:20:08 +0100 (CET) Received: from martinez.u-strasbg.fr (martinez.u-strasbg.fr [130.79.129.134]) by webmail.sic.rm.cnr.it (Horde MIME library) with HTTP; Tue, 03 Jan 2006 10:20:08 +0100 Message-ID: <20060103102008.y85gtgkm7jf4844g@webmail.sic.rm.cnr.it> Date: Tue, 03 Jan 2006 10:20:08 +0100 From: Andrea Preite Martinez To: ucd@ivoa.net, ucd-sci@ivoa.net Subject: UCD news... 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 (4.0.4) X-Virus-Scanned: by amavisd-new X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2006.1.3.0 Sender: owner-ucd@eso.org Precedence: bulk Reply-To: ucd@ivoa.net Dear members of the WG, first of all, a very happy new year to you all! For a good start, I'm pleased to annunce you that the UCD1+ word-list is an IVOA Recommendation from Dec 31 2005. You can find version 1.11 of the document at http://www.ivoa.net/Documents/latest/UCDlist.html Now that we have eventually the first standard list of words, it's time to start wondering how to change it! We already had a discussion on a Note on UCD1+ maintenance I submitted to the WG in October. I revised the Note according to some (if not all) of your remarks, and transformed the Note into the Working Draft that you can find at http://www.ivoa.net/Documents/latest/UCDlistMaintenance.html . I?m ready to move the document to the state of PR and request comments from the community, but before doing this I?d like to be sure that the discussion in our WG is over. So, if you still have comments or amendments to the text of the Working Draft, please do it soon. A reasonable schedule could be to have an RFC in February and to submit the PR to the Exec before the InterOp in spring. Cheers, Andrea ============================================================================== Andrea Preite Martinez andrea.preitemartinez@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 CDS :+33.3.90242473 ============================================================================== From owner-ucd-sci@eso.org Thu Jan 5 11:01:26 2006 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 (8.12.10+Sun/8.12.10) with ESMTP id k05A1G9j027754 for ; Thu, 5 Jan 2006 11:01:16 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k05A1GQe027753 for ucd-sci-outgoing; Thu, 5 Jan 2006 11:01:16 +0100 (MET) 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 k05A1B9j027736 for ; Thu, 5 Jan 2006 11:01:12 +0100 (MET) 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 k05A191r016591 for ; Thu, 5 Jan 2006 11:01:10 +0100 (CET) Received: from pisaure.intra.cea.fr (pisaure.intra.cea.fr [132.166.88.38]) by cirse.extra.cea.fr (8.13.4/8.13.4/CEAnet-Internet.5.0) with ESMTP id k05A0tOS015221 for ; Thu, 5 Jan 2006 11:01:00 +0100 (MET) 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 k059rSrm014512 for ; Thu, 5 Jan 2006 10:53:28 +0100 (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+PROTO) with ESMTP id k05A0pjd016883 for ; Thu, 5 Jan 2006 11:00:51 +0100 (MET) 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 k05A26bh009059 for ; Thu, 5 Jan 2006 11:02:09 +0100 (MET) Message-ID: <43BCEE4F.8020208@cea.fr> Date: Thu, 05 Jan 2006 11:00:47 +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: ucd-sci@ivoa.net Subject: Re: UCD news... References: <20060103102008.y85gtgkm7jf4844g@webmail.sic.rm.cnr.it> In-Reply-To: <20060103102008.y85gtgkm7jf4844g@webmail.sic.rm.cnr.it> 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: 2.1.0.0, Antispam-Data: 2006.1.5.1 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net Hi Andrea, Andrea Preite Martinez wrote: > Dear members of the WG, > > first of all, a very happy new year to you all! > > For a good start, I'm pleased to annunce you that the UCD1+ word-list is > an IVOA Recommendation from Dec 31 2005. > You can find version 1.11 of the document at :-) > > http://www.ivoa.net/Documents/latest/UCDlist.html Now that we have > eventually the first standard list of words, it's time to start > wondering how to change it! > We already had a discussion on a Note on UCD1+ maintenance I submitted > to the WG in October. I revised the Note according to some (if not all) > of your remarks, and transformed the Note into the Working Draft that > you can find at > http://www.ivoa.net/Documents/latest/UCDlistMaintenance.html . > > I?m ready to move the document to the state of PR and request comments > from the community, but before doing this I?d like to be sure that the > discussion in our WG is over. So, if you still have comments or > amendments to the text of the Working Draft, please do it soon. The procedure for ucd-list revision formalism seems to be well establish, nevertheless I have a question and a request for clarification concerning the way it will work... in real world. It concerns the end of the introduction where the differents parts involved in the procedure are listed/presented. I don't completly understand the link between the sci-board and the community. There is no mention of the UCD WG! What is the purposes and goals of this group considering the UCDlist? Are the sci-board members supposed to follow the discussions on semantic WG? For the moment I am not registered there! Because before any proposition of modifications some discussions will occurs on the WG lists and it will perhaps be of some help to follow the ideas maturation for a better understanding of the proposition!? Or are the propositions supposed to occur ab nihilo? Where are supposed to occur such discussions, UCD or semantic WG? > A reasonable schedule could be to have an RFC in February and to submit > the PR to the Exec before the InterOp in spring. Cheers, > > Andrea > > > ============================================================================== > > Andrea Preite Martinez > andrea.preitemartinez@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 CDS :+33.3.90242473 > ============================================================================== > > > -- 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/ ------------------------------------------------------------------ Le langage est l'illusion qui masque la complexité de l'esprit. Julip - Jim Harrison ------------------------------------------------------------------ Si le paraitre compte plus que l'être le faire-savoir plus que le savoir-faire la croyance est elle plus forte que la science? From owner-ucd-sci@eso.org Thu Jan 5 11:23:55 2006 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 (8.12.10+Sun/8.12.10) with ESMTP id k05ANj9j000824 for ; Thu, 5 Jan 2006 11:23:45 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k05ANjYJ000823 for ucd-sci-outgoing; Thu, 5 Jan 2006 11:23:45 +0100 (MET) 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 k05ANf9j000815 for ; Thu, 5 Jan 2006 11:23:41 +0100 (MET) 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 k05ANd1r017317 for ; Thu, 5 Jan 2006 11:23:39 +0100 (CET) Received: from localhost (localhost.localdomain [127.0.0.1]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP id 7AD5DC743A for ; Thu, 5 Jan 2006 11:23:31 +0100 (CET) Received: from localhost (localhost.localdomain [127.0.0.1]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP id 26E2EC7437 for ; Thu, 5 Jan 2006 11:23:31 +0100 (CET) Received: from smtp1.sic.rm.cnr.it ([127.0.0.1]) by localhost (smtp1 [127.0.0.1]) (amavisd-new, port 10023) with ESMTP id 03555-07 for ; Thu, 5 Jan 2006 11:23:30 +0100 (CET) Received: from localhost (unknown [10.1.0.7]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP for ; Thu, 5 Jan 2006 11:23:30 +0100 (CET) Received: from martinez.u-strasbg.fr (martinez.u-strasbg.fr [130.79.129.134]) by webmail.sic.rm.cnr.it (Horde MIME library) with HTTP; Thu, 05 Jan 2006 11:23:30 +0100 Message-ID: <20060105112330.j023ic9xmmyo0o8o@webmail.sic.rm.cnr.it> Date: Thu, 05 Jan 2006 11:23:30 +0100 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Re: UCD news... References: <20060103102008.y85gtgkm7jf4844g@webmail.sic.rm.cnr.it> <43BCEE4F.8020208@cea.fr> In-Reply-To: <43BCEE4F.8020208@cea.fr> 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 (4.0.4) X-Virus-Scanned: by amavisd-new X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2006.1.5.2 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: ucd-sci@ivoa.net Quoting Pierre Didelon : > > There is no mention of the UCD WG! What is the purposes and goals of > this group > considering the UCDlist? > Are the sci-board members supposed to follow the discussions on semantic WG? > For the moment I am not registered there! Pierre, you are right, I forgot to communicate "urbi et orbi" for those not present at last InterOp that the Exec has decided to change the name of the UCD WG into UCD/Semantic WG. For technical reasons (I've been told by the -former - IVOA Doc manager) the names of the WG and of the discussion list were left unchanged. So UCD WG and Semantic WG are indeed the same thing! Ciao Andrea ============================================================================== Andrea Preite Martinez andrea.preitemartinez@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 CDS :+33.3.90242473 ============================================================================== From owner-ucd-sci@eso.org Thu Mar 2 13:49:13 2006 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 (8.12.10+Sun/8.12.10) with ESMTP id k22Ckx4R007422 for ; Thu, 2 Mar 2006 13:46:59 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k22CkxuT007421 for ucd-sci-outgoing; Thu, 2 Mar 2006 13:46:59 +0100 (MET) 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 k22Cko4R007390 for ; Thu, 2 Mar 2006 13:46:50 +0100 (MET) Received: from serenity.mcc.ac.uk (serenity.mcc.ac.uk [130.88.200.93]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k22CkmkD022511 for ; Thu, 2 Mar 2006 13:46:49 +0100 (CET) Received: from silvia.phy.umist.ac.uk ([130.88.151.9]) by serenity.mcc.ac.uk with esmtps (TLSv1:AES256-SHA:256) (Exim 4.51 (FreeBSD)) id 1FEnCd-0008vY-FT for ucd-sci@ivoa.net; Thu, 02 Mar 2006 12:46:43 +0000 Date: Thu, 2 Mar 2006 12:52:39 +0000 (GMT) From: Silvia Dalla X-X-Sender: sdalla@silvia.phy.umist.ac.uk To: ucd-sci@ivoa.net Subject: Request for modification of UCD: time.obs Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-UoM: Scanned by the University Mail System. See http://www.itservices.manchester.ac.uk/email/filtering/information/ for details. X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2006.03.01.172607 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Silvia Dalla hi all, I propose modifying 'time.obs'. This UCD is currently defined as: 'Observation on-time, duration' However we are missing a UCD that identifies the time stamp associated with an observation: for example if data are collected between a 'time.obs.start' and a 'time.obs.end', frequently the mid point of this time interval is used to define the time of the observation. I propose that 'time.obs' should be 'time stamp associated to the observation'. A new UCD could be used to identify the duration of the observation: the obvious choice would be 'time.obs.duration'. Best wishes, Silvia ------------------------------------ Silvia Dalla School of Physics and Astronomy University of Manchester PO Box 88 Manchester M60 1QD UK Tel +44-161-306 8705 Fax +44-161-306 3941 ------------------------------------ From owner-ucd-sci@eso.org Fri Mar 3 00:13:42 2006 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 (8.12.10+Sun/8.12.10) with ESMTP id k22NDVr0005035 for ; Fri, 3 Mar 2006 00:13:31 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k22NDVln005034 for ucd-sci-outgoing; Fri, 3 Mar 2006 00:13:31 +0100 (MET) 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 k22NDQr0005028 for ; Fri, 3 Mar 2006 00:13:26 +0100 (MET) Received: from smtp.ucolick.org (santo.ucolick.org [128.114.23.204]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k22NDLkD025982 for ; Fri, 3 Mar 2006 00:13:24 +0100 (CET) Received: from localhost (localhost [127.0.0.1]) by smtp.ucolick.org (Postfix) with ESMTP id 848865D714 for ; Thu, 2 Mar 2006 15:13:15 -0800 (PST) Received: from geneva.ucolick.org (geneva.ucolick.org [128.114.23.183]) (using TLSv1 with cipher DHE-RSA-AES256-SHA (256/256 bits)) (No client certificate requested) by smtp.ucolick.org (Postfix) with ESMTP id 3052311406 for ; Thu, 2 Mar 2006 15:13:15 -0800 (PST) Received: from geneva.ucolick.org (localhost [127.0.0.1]) by geneva.ucolick.org (8.13.1/8.12.10) with ESMTP id k22NDEYi032184 for ; Thu, 2 Mar 2006 15:13:14 -0800 Received: (from sla@localhost) by geneva.ucolick.org (8.13.1/8.13.1/Submit) id k22NDETt032183 for ucd-sci@ivoa.net; Thu, 2 Mar 2006 15:13:14 -0800 Date: Thu, 2 Mar 2006 15:13:14 -0800 From: Steve Allen To: ucd-sci@ivoa.net Subject: Re: Request for modification of UCD: time.obs Message-ID: <20060302231314.GA32136@ucolick.org> References: Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii Content-Disposition: inline In-Reply-To: User-Agent: Mutt/1.4.2.1i X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2006.03.02.144604 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Steve Allen On Thu 2006-03-02T12:52:39 +0000, Silvia Dalla hath writ: > I propose modifying 'time.obs'. > > This UCD is currently defined as: 'Observation on-time, duration' > > However we are missing a UCD that identifies the time stamp associated > with an observation: for example if data are collected between a > 'time.obs.start' and a 'time.obs.end', frequently the mid point of > this time interval is used to define the time of the observation. > > I propose that 'time.obs' should be 'time stamp associated to the > observation'. > > A new UCD could be used to identify the duration of the observation: > the obvious choice would be 'time.obs.duration'. There are several FITS reserved keywords with definitions which are closely related to these UCDs. It would be dismaying if the UCDs and the FITS keywords became dissonant rather than consonant. First a quick review... >From the original Wells et al. paper there is DATE-OBS The current FITS standard asserts that this should be assume to refer to the start of an observation unless another interpretation is clearly explained in the comment field. In the original paper by Wells et al. this keyword was defined simply as "date of data acquisition". As a result not all instances of its use conform to the suggestion (added nearly two decades afterwards) that it refer to the start of an observation. FITS WCS Paper II (celestial coordinates) reserved MJD-OBS with semantics identical to DATE-OBS except for being expressed as a floating point count of days rather than as a character string indicating a calendar date. FITS WCS Paper III (spectral coordinates) reserved MJD-AVG and DATE-AVG with semantics indicating that the value should refer to an average date (of a presumably extended observation). Now I switch back to UCDs. DATE-OBS seems to correspond best to Silvia Dalla's suggestion for a change to "time.obs". DATE-AVG seems to correspond best to "time.obs;stat.mean". But that calls up a question of whether the current semantics for "time.obs", which indicate a duration, are not begging for a new UCD entry in the stat group -- should there be a UCD something like "stat.range" or "stat.span" to indicate the difference between the maximum and minimum of a quantity? I wonder why there is "time.obs.start" instead of "time.obs;stat.min" and similarly "time.obs.end" instead of "time.obs;stat.max" But upon reading closely through http://www.ivoa.net/Documents/latest/UCDlist.html I am left mystified by the distinction in semantics between the UCDs "time.obs" and "time.expo" Is there a more detailed explanation of the difference in the semantics of these two quantities? -- Steve Allen WGS-84 (GPS) UCO/Lick Observatory Natural Sciences II, Room 165 Lat +36.99858 University of California Voice: +1 831 459 3046 Lng -122.06014 Santa Cruz, CA 95064 http://www.ucolick.org/~sla/ Hgt +250 m From owner-ucd-sci@eso.org Fri Mar 3 00:38:17 2006 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 (8.12.10+Sun/8.12.10) with ESMTP id k22Nc5r0006543 for ; Fri, 3 Mar 2006 00:38:05 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k22Nc5u0006542 for ucd-sci-outgoing; Fri, 3 Mar 2006 00:38:05 +0100 (MET) 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 k22Nc0r0006537 for ; Fri, 3 Mar 2006 00:38:01 +0100 (MET) 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 k22NbwkD026833 for ; Fri, 3 Mar 2006 00:37:59 +0100 (CET) X-Spam-Checker-Version: SpamAssassin 3.1.0 (2005-09-13) on noao.edu X-Spam-Level: X-Spam-Status: No, score=-4.3 required=4.5 tests=ALL_TRUSTED,AWL,BAYES_00 autolearn=ham version=3.1.0 X-TFF-CGPSA-Version: 1.4f1 X-TFF-CGPSA-Filter: Scanned Received: from [140.252.4.21] (account shaw@noao.edu) by noao.edu (CommuniGate Pro WebUser 5.0.8) with HTTP id 24178466; Thu, 02 Mar 2006 16:37:51 -0700 From: "Dick Shaw" Subject: Re: Request for modification of UCD: time.obs To: Silvia Dalla , ucd-sci@ivoa.net X-Mailer: CommuniGate Pro WebUser v5.0.8 Date: Thu, 02 Mar 2006 16:37:51 -0700 Message-ID: In-Reply-To: References: MIME-Version: 1.0 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: 2.1.0.0, Antispam-Data: 2006.03.02.144604 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: "Dick Shaw" There is certainly merit in making a distinction among quantities such as these. For example, one needs to be able to describe the interval of time over which the data were obtained, as well as the effective duration of the exposure. For example: an integration may be started, interrupted, and then resumed. Or, multiple exposures of a region of sky may be obtained separately and later combined. This is common in ground-based IR, where sky brightness is an issue, or in the optical if the consecutive exposures are obtained to track a time-variable phenomenon, or merely to dither images spatially to remove artifacts such as seams in a large, focal plane array. In these cases the interval over which photons were collected is shorter than the difference between the start of the first exposure and the end of the last. Somehow this information needs to be recorded for high-level (i.e., combined) data products. Depending upon the degree to which one wishes to obsess about the details, a richer semantic description may be in order. Regards, Dick Shaw On Thu, 2 Mar 2006 12:52:39 +0000 (GMT) Silvia Dalla wrote: > > hi all, > > I propose modifying 'time.obs'. > > This UCD is currently defined as: 'Observation on-time, duration' > > However we are missing a UCD that identifies the time stamp associated > with an observation: for example if data are collected between a > 'time.obs.start' and a 'time.obs.end', frequently the mid point of > this time interval is used to define the time of the observation. > > I propose that 'time.obs' should be 'time stamp associated to the > observation'. > > A new UCD could be used to identify the duration of the observation: > the obvious choice would be 'time.obs.duration'. > > Best wishes, > Silvia > > ------------------------------------ > Silvia Dalla > School of Physics and Astronomy > University of Manchester > PO Box 88 > Manchester M60 1QD > UK > > Tel +44-161-306 8705 >Fax +44-161-306 3941 > ------------------------------------ #--- Dr. Richard A. Shaw, Scientist National Optical Astronomy Observatory 950 N. Cherry Avenue Tucson, AZ 85719 USA 520-318-8398 From owner-ucd-sci@eso.org Fri Mar 3 00:55:35 2006 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 (8.12.10+Sun/8.12.10) with ESMTP id k22NtKr0007480 for ; Fri, 3 Mar 2006 00:55:20 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k22NtJOV007479 for ucd-sci-outgoing; Fri, 3 Mar 2006 00:55:19 +0100 (MET) 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 k22NtFr0007475 for ; Fri, 3 Mar 2006 00:55:15 +0100 (MET) 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 k22NtAkD027412 for ; Fri, 3 Mar 2006 00:55:11 +0100 (CET) X-Spam-Checker-Version: SpamAssassin 3.1.0 (2005-09-13) on noao.edu X-Spam-Level: X-Spam-Status: No, score=-4.8 required=4.5 tests=ALL_TRUSTED,AWL,BAYES_00 autolearn=ham version=3.1.0 X-TFF-CGPSA-Version: 1.4f1 X-TFF-CGPSA-Filter: Scanned Received: from [140.252.4.155] ([140.252.4.155] verified) by noao.edu (CommuniGate Pro SMTP 5.0.8) with ESMTPS id 24178847; Thu, 02 Mar 2006 16:55:03 -0700 In-Reply-To: <20060302231314.GA32136@ucolick.org> References: <20060302231314.GA32136@ucolick.org> Mime-Version: 1.0 (Apple Message framework v746.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <3029B3F6-05D8-443B-A272-5862A9E439EE@noao.edu> Content-Transfer-Encoding: 7bit From: Rob Seaman Subject: Re: Request for modification of UCD: time.obs Date: Thu, 2 Mar 2006 16:54:57 -0700 To: ucd-sci@ivoa.net X-Mailer: Apple Mail (2.746.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2006.03.02.152605 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Rob Seaman On Mar 2, 2006, at 4:13 PM, Steve Allen wrote: > It would be dismaying if the UCDs and the FITS keywords became > dissonant rather than consonant. Most certainly agree! Wouldn't mind, however, if the FITS standards process were to be informed by VO standards, not just the other way around :-) > DATE-OBS > The current FITS standard asserts that this should be assume to refer > to the start of an observation unless another interpretation is > clearly explained in the comment field. Have also seen headers with all variations of beginning, middle, and ending timestamps (and not all provided via DATE-OBS) and even both beginning and ending time stamps with no explicit exposure duration per se. Not clear that one size can, or should, fit all. Should also point out that the syntax and semantics of DATE-OBS changed significantly due to Y2K. The original usage was to specify only a calendar date. Current usage can combine date and time into an atomic whole. > DATE-AVG seems to correspond best to "time.obs;stat.mean". Just as there are various statistical measures of central tendency, an "average" representative timestamp for an observation may reasonably mean many different things. Various instruments, for instance, allow pausing and resuming an exposure for arbitrary periods. The camera shutter (if any) may not even be open during the claimed midpoint of an observation. Other instruments, for instance drift scans, have significantly different representative timestamps for different pixels. A shuttered camera on a space platform may have one (scalar) timestamp for captured "science" photons and another (vector) timestamp for radiation events that continue to accumulate during readout. Even simple (ground-based, shuttered, etc.) observations might benefit from correcting the overt midpoint timestamp for varying airmass during the observation. (Alternately, an "effective" airmass might be computed.) Hesitate to refer folks, yet again, to STC. Rob Seaman NOAO From owner-ucd-sci@eso.org Sat Mar 4 23:44:36 2006 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 (8.12.10+Sun/8.12.10) with ESMTP id k24MiSjR004218 for ; Sat, 4 Mar 2006 23:44:28 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k24MiScC004217 for ucd-sci-outgoing; Sat, 4 Mar 2006 23:44:28 +0100 (MET) Message-Id: <200603042244.k24MiScC004217@mercury.hq.eso.org> X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-sci@eso.org using -f Date: Fri, 03 Mar 2006 11:52:27 +0100 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: Re: UCD time.obs Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Andrea Preite Martinez X-Virus-Scanned: by amavisd-new Hi Silvia, Steve, Dick, Rob, let me extract from the discussion on the UCD time.obs three points: We should not mix up a "duration" (interval of time) with an "instant" (currently date/time), or different instants during the "duration". This semantic difference is reflected in the present list of UCDs. 1. time-instant: Astronomer are used to characterize their observations by a time-stamp (a UNIQUE time-stamp) that is reasonably to consider some sort of average between the beginning and the end of an observation. This stamp/label is called EPOCH of the observation. The corresponding UCD is time.epoch . 2. time-duration: First of all we need to consider that modern observations are often (I dare say always in the case of observations from space) the result of multiple exposures. While 30 years ago there was no semantic difference between observation and exposure, today we need to be precise, one observation being the result of more than one exposure, leading to an observation-duration usually greater than a single exposure-duration The UCDs time.obs and time.expo reflect this difference. 3. start/end, and the correspondance between FITS keywords and UCDs. I'm aware of the importance that FITS keywords still have in describing our data, but I'm also aware of the fact that (expecially in the "time" domain!!) there is a tendency to force (to forge?) the initial meaning and to proliferate keywords (Rob is right!). I think that we already have the UCDs corresponding to the quoted keywords: DATE-OBS = MJD-OBS : time.obs.start (time-stamp of the beginning of the observation) DATE-AVG = MJD-AVG : time.epoch[;obs] (epoch of the observation) I also agree with Steve sentence /> It would be dismaying if the UCDs/ /> and the FITS keywords became dissonant rather than consonant/ and Rob's comment to it, but I interpret his warning as: we should not make the same mistakes! Why start/end and not min/max: First of all for esthetic reasons. Most seriously, because in my opinion min/max whould indicate a min/max DURATION, while start/end are certainly referring, correctly, to two INSTANTs of time. Finally, start/end are the words that you find in the description of the data, not min/max. Andrea ------------------------------------------------------------------------ Andrea Preite Martinez andrea.preitemartinez-at-iasf-roma.inaf.it IASF Tel.IASF:+39.06.4993.4651 Via del Fosso del Cavaliere 100 Tel.CDS :+33.3.90242473 I-00133 Roma Cell.1 :+39.320.43.15.383 Cell.2 :+39.335.38.17.355 =================================================================================== From owner-ucd-sci@eso.org Sun Mar 5 08:28:52 2006 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 (8.12.10+Sun/8.12.10) with ESMTP id k257Pdjl004556 for ; Sun, 5 Mar 2006 08:28:47 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k256wRXl029349 for ucd-sci-outgoing; Sun, 5 Mar 2006 07:58:27 +0100 (MET) 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 k256vPjR029060 for ; Sun, 5 Mar 2006 07:57:26 +0100 (MET) Received: from smtp.ucolick.org (santo.ucolick.org [128.114.23.204]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k256vN22020243 for ; Sun, 5 Mar 2006 07:57:24 +0100 (CET) Received: from localhost (localhost [127.0.0.1]) by smtp.ucolick.org (Postfix) with ESMTP id 084945D715 for ; Sat, 4 Mar 2006 22:57:17 -0800 (PST) Received: from geneva.ucolick.org (geneva.ucolick.org [128.114.23.183]) (using TLSv1 with cipher DHE-RSA-AES256-SHA (256/256 bits)) (No client certificate requested) by smtp.ucolick.org (Postfix) with ESMTP id 9C96411416 for ; Sat, 4 Mar 2006 22:57:16 -0800 (PST) Received: from geneva.ucolick.org (localhost [127.0.0.1]) by geneva.ucolick.org (8.13.1/8.12.10) with ESMTP id k256vG9v013949 for ; Sat, 4 Mar 2006 22:57:16 -0800 Received: (from sla@localhost) by geneva.ucolick.org (8.13.1/8.13.1/Submit) id k256vFgZ013948 for ucd-sci@ivoa.net; Sat, 4 Mar 2006 22:57:15 -0800 Date: Sat, 4 Mar 2006 22:57:15 -0800 From: Steve Allen To: ucd-sci@ivoa.net Subject: Re: UCD time.obs Message-ID: <20060305065715.GA13916@ucolick.org> References: <200603042244.k24MiScC004217@mercury.hq.eso.org> Mime-Version: 1.0 Content-Type: text/plain; charset=us-ascii Content-Disposition: inline In-Reply-To: <200603042244.k24MiScC004217@mercury.hq.eso.org> User-Agent: Mutt/1.4.2.1i X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2006.03.04.222605 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Steve Allen On Fri 2006-03-03T11:52:27 +0100, Andrea Preite Martinez hath writ: > We should not mix up a "duration" (interval of time) with an "instant" > (currently date/time), or different instants during the "duration". This > semantic difference is reflected in the present list of UCDs. I agree. My confusion stems from the fact that the semantic definition for all of the UCD words consists of an incomplete sentence. In the absence of detailed descriptions such as those provided in this note I did not understand which ones were instant or duration or that observation is a superset of exposure. This may be true of other, non-temporal, UCD words. For the sake of averting subsequent misinterpretations, is there a way to include richer semantic definitions as part of the document itself? Or alternatively, to include an explicit, and obvious, reference to a separate "usage" document with examples, correspondences with FITS keywords, etc? -- Steve Allen WGS-84 (GPS) UCO/Lick Observatory Natural Sciences II, Room 165 Lat +36.99858 University of California Voice: +1 831 459 3046 Lng -122.06014 Santa Cruz, CA 95064 http://www.ucolick.org/~sla/ Hgt +250 m From owner-ucd-sci@eso.org Mon Jul 17 11:01:26 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6H91NZc002330 for ; Mon, 17 Jul 2006 11:01:23 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6H91Ntb002329 for ucd-sci-outgoing; Mon, 17 Jul 2006 11:01:23 +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 (8.13.6+Sun/8.12.10) with ESMTP id k6H91Mua002319 for ; Mon, 17 Jul 2006 11:01:22 +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 k6H91KLY004388 for ; Mon, 17 Jul 2006 11:01:20 +0200 (CEST) Received: from localhost (smtp1 [127.0.0.1]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP id CF17D1DA2FA for ; Mon, 17 Jul 2006 11:01:14 +0200 (CEST) X-Virus-Scanned: amavisd-new at sic.rm.cnr.it Received: from smtp1.sic.rm.cnr.it ([127.0.0.1]) by localhost (smtp1.sic.rm.cnr.it [127.0.0.1]) (amavisd-new, port 10023) with ESMTP id JXUQI0Vqm+4O for ; Mon, 17 Jul 2006 11:01:14 +0200 (CEST) Received: from localhost (unknown [10.1.2.2]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP for ; Mon, 17 Jul 2006 11:01:14 +0200 (CEST) Received: from martinez.u-strasbg.fr (martinez.u-strasbg.fr [130.79.129.134]) by webmail.sic.rm.cnr.it (Horde MIME library) with HTTP; Mon, 17 Jul 2006 11:01:14 +0200 Message-ID: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> Date: Mon, 17 Jul 2006 11:01:14 +0200 From: Andrea Preite Martinez To: ucd-sci@ivoa.net Subject: RFMs (Requests for modification) on the List of UCD-words MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1; DelSp="Yes"; format="flowed" Content-Disposition: inline User-Agent: Internet Messaging Program (IMP) H3 (4.1.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.7.17.13433 Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id k6H91Mua002323 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Andrea Preite Martinez RFMs (Requests for modification) on the List of UCD-words ========================================================= Dear all, You can find at http://www.ivoa.net/twiki/bin/view/IVOA/UCDwordsRFM a list of proposed requests (RFMs) to modify/add the present standard list of ucd-words: The UCD1+ controlled vocabulary, Vers. 1.11 - IVOA Recommendation 31 December 2005 ( http://www.ivoa.net/Documents/latest/UCDlist.html ). The RFMs were collected over the past few month, from suggestions coming from various members of the IVOA community. The list has been presented at the UCD-session in Victoria (see the presentation of the original list at http://ivoa.net/twiki/bin/view/IVOA/InterOpMay2006UCD ), and corrected taking into account the discussions during the meeting within the WG and with the Theory IG. Other suggestions have been added to describe attributes used by some Data Models. The list is open for discussion in accordance with the approved standard procedure: Maintenance of the list of UCD words, Version 1.20 - IVOA Recommendation 28 May 2006 (http://www.ivoa.net/Documents/latest/UCDlistMaintenance.html ). Due to web security problems, for the moment we discourage the usage of the web-based form for submitting RFMs. So we can consider the present list of RFMs as a collective effort of the community, not requiring a private personal answer (see par. 2.2 and 2.3 of the maintenance document). For the time being, all the RFMs and all the corresponding answers will be grouped together in a public document. Other RFMs could be proposed during the discussion phase, so that we can consider this document as a temporary repository of all proposed RFMs. Due to the holiday period, I propose to leave the discussion (and the possibility to include other RFMs in the present list) open till August 15. Then I will propose to the WG a revised version of the UCD1+ controlled vocabulary. Cheers, Andrea =================================================================================== Andrea Preite Martinez andrea.preitemartinez@iasf-roma.inaf.it IASF Tel.IASF:+39.06.4993.4651 Via del Fosso del Cavaliere 100 Tel.CDS :+33.3.90242473 I-00133 Roma Cell.1 :+39.320.43.15.383 Cell.2 :+39. =================================================================================== From owner-ucd-sci@eso.org Mon Jul 17 14:34:28 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6HCYKGh018030 for ; Mon, 17 Jul 2006 14:34:20 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6HCYKZY018029 for ucd-sci-outgoing; Mon, 17 Jul 2006 14:34:20 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd-sci@eso.org using -f Received: from serapis.hq.eso.org (serapis.hq.eso.org [134.171.7.10]) by mercury.hq.eso.org (8.13.6+Sun/8.12.10) with ESMTP id k6HCYBvi018005; Mon, 17 Jul 2006 14:34:11 +0200 (MEST) Received: from [134.171.27.58] (ga008899.ads.eso.org [134.171.27.58]) by serapis.hq.eso.org (8.11.7+Sun/8.11.7) with ESMTP id k6HCYBd20194; Mon, 17 Jul 2006 14:34:11 +0200 (MEST) Message-ID: <44BB83C3.3010702@eso.org> Date: Mon, 17 Jul 2006 14:34:11 +0200 From: Nausicaa Delmotte User-Agent: Thunderbird 1.5.0.4 (X11/20060516) MIME-Version: 1.0 To: ucd-sci@ivoa.net CC: Andrea Preite Martinez Subject: observation proposal and name of the observer References: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> In-Reply-To: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Nausicaa Delmotte Dear Andreas, all, Thanks a lot for the new list of proposed requests. I'd like to comment on the following two points: - What is the difference between 'title of an observation proposal' and 'name of an observation proposal'? So far I would not have expected any difference but with the introduction of the new UCD word obs.proposal, it seems it is possible to construct both meta.title;obs.proposal and meta.id;obs.proposal Maybe someone could provide an example, in case there is a difference of meaning between those two UCDs? I just cannot see the difference... (given that the proposal code is already defined by meta.code;obs.proposal). By the way, what about the 'abstract of the observation proposal'? meta.abstract;obs.proposal? - Name of the observer: so far it has been obs.observer but if we introduce meta.id.PI, meta.id.Coi for human beings, why not meta.id.Observer;obs? Thanks, Cheers, Nausicaa Andrea Preite Martinez said the following on 07/17/2006 11:01 AM: > RFMs (Requests for modification) on the List of UCD-words > ========================================================= > > > Dear all, > > You can find at http://www.ivoa.net/twiki/bin/view/IVOA/UCDwordsRFM a > list of proposed requests (RFMs) to modify/add the present standard list > of ucd-words: The UCD1+ controlled vocabulary, Vers. 1.11 - IVOA > Recommendation 31 December 2005 ( > http://www.ivoa.net/Documents/latest/UCDlist.html ). > > The RFMs were collected over the past few month, from suggestions coming > from various members of the IVOA community. > > The list has been presented at the UCD-session in Victoria (see the > presentation of the original list at > http://ivoa.net/twiki/bin/view/IVOA/InterOpMay2006UCD ), and corrected > taking into account the discussions during the meeting within the WG and > with the Theory IG. Other suggestions have been added to describe > attributes used by some Data Models. > > The list is open for discussion in accordance with the approved standard > procedure: Maintenance of the list of UCD words, Version 1.20 - IVOA > Recommendation 28 May 2006 > (http://www.ivoa.net/Documents/latest/UCDlistMaintenance.html ). > > Due to web security problems, for the moment we discourage the usage of > the web-based form for submitting RFMs. So we can consider the present > list of RFMs as a collective effort of the community, not requiring a > private personal answer (see par. 2.2 and 2.3 of the maintenance > document). For the time being, all the RFMs and all the corresponding > answers will be grouped together in a public document. Other RFMs could > be proposed during the discussion phase, so that we can consider this > document as a temporary repository of all proposed RFMs. > > Due to the holiday period, I propose to leave the discussion (and the > possibility to include other RFMs in the present list) open till August 15. > > Then I will propose to the WG a revised version of the UCD1+ controlled > vocabulary. > > Cheers, > > Andrea > > =================================================================================== > > Andrea Preite Martinez > andrea.preitemartinez@iasf-roma.inaf.it > IASF Tel.IASF:+39.06.4993.4651 > Via del Fosso del Cavaliere 100 Tel.CDS :+33.3.90242473 > I-00133 Roma Cell.1 :+39.320.43.15.383 > Cell.2 :+39. > =================================================================================== > > > -- Dr Nausicaa Delmotte @..@ ndelmott@eso.org ESO Archive Service Developer (----) Tel: +49 (0)89 3200 6418 Karl-Schwarzschild-Str. 2 ( >__< ) Fax: +49 (0)89 3200 6677 D-85748 Garching bei Muenchen ^^ ~~ ^^ http://www.eso.org/~ndelmott/ From owner-ucd-sci@eso.org Mon Jul 17 17:35:33 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6HFZTx0001836 for ; Mon, 17 Jul 2006 17:35:29 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6HFZT1p001834 for ucd-sci-outgoing; Mon, 17 Jul 2006 17:35:29 +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 (8.13.6+Sun/8.12.10) with ESMTP id k6HFZSAh001823 for ; Mon, 17 Jul 2006 17:35:28 +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 k6HFZOum018989 for ; Mon, 17 Jul 2006 17:35:25 +0200 (CEST) X-Spam-Checker-Version: SpamAssassin 3.1.3 (2006-06-01) on noao.edu X-Spam-Level: X-Spam-Status: No, score=-4.4 required=4.5 tests=ALL_TRUSTED,AWL,BAYES_00, HTML_MESSAGE autolearn=ham version=3.1.3 X-TFF-CGPSA-Version: 1.4f1 X-TFF-CGPSA-Filter: Scanned Received: from [140.252.10.113] (account seaman [140.252.10.113] verified) by noao.edu (CommuniGate Pro SMTP 5.0.9) with ESMTPSA id 28703250; Mon, 17 Jul 2006 08:35:11 -0700 In-Reply-To: References: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: multipart/alternative; boundary=Apple-Mail-69-897140808 Message-Id: Cc: ucd-sci@ivoa.net From: Rob Seaman Subject: Re: RFMs (Requests for modification) on the List of UCD-words Date: Mon, 17 Jul 2006 08:35:16 -0700 To: andrea.preitemartinez@iasf-roma.inaf.it X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.7.17.75432 Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: Rob Seaman --Apple-Mail-69-897140808 Content-Transfer-Encoding: quoted-printable Content-Type: text/plain; charset=WINDOWS-1252; delsp=yes; format=flowed Hi Andrea, > proposed requests (RFMs) to modify/add the present standard list of =20= > ucd-words Should we be gratified or distressed at the large number of proposed =20 changes? :-) I understand from the maintenance agreement, that the end result here =20= will be a new list with an incremented version number. I don't see =20 any discussion for supporting older versions indefinitely in service =20 of content previously created. Comments? > Other suggestions have been added to describe attributes used by =20 > some Data Models. Does this represent a change in the original coherent genesis of the =20 UCDs as astronomical column headings? What does "some" Data Models =20 mean? Do UCDs now have a mandate to support all IVOA (or even =20 astronomical) DMs? =46rom the RFMs: >> A complete proposed revision of the time branch can be found in a =20 >> TN at the end of this document. I support drawing a clearer distinction between duration and epoch. =20 What is the benefit, however, to keep both notions under the same =20 "time" hierarchy? Why not, for example, simply "duration.event" and =20 "epoch.event"? I'm also concerned that this list is growing too =20 rapidly. Timelike modifiers will often appear in combination with =20 other UCDs - they are more like adjectives and adverbs than nouns and =20= verbs. As with other fundamental concepts, time descriptors should =20 remain elegantly simple and sparse. >> Other =93computational=94 and =93cosmological=94 words were discussed = in =20 >> Victoria, also with the Theory IG. We need an input from them in =20 >> order to revise/complete the list I have the same response to these terms as I do to VOEvent's - don't =20 these really represent a different namespace? In particular, =20 shouldn't the Theory group be maintaining this list if they are its =20 primary target? Rob Seaman NOAO= --Apple-Mail-69-897140808 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=WINDOWS-1252
Hi Andrea,

proposed requests = (RFMs) to modify/add the present standard list of = ucd-words

Should we be gratified or distressed at the = large number of proposed changes?=A0 :-)

I understand from = the maintenance agreement, that the end result here will be a new list = with an incremented version number.=A0 I don't see any discussion for = supporting older versions indefinitely in service of content previously = created.=A0 Comments?

Other suggestions = have been added to describe attributes used by some Data = Models.

Does this = represent a change in the original coherent genesis of the UCDs as = astronomical column headings?=A0 What does "some" Data Models mean?=A0 = Do UCDs now have a mandate to support all IVOA (or even astronomical) = DMs?

=46rom the RFMs:

A complete = proposed revision of the time branch can be found in a TN at the end of = this document.

I support drawing a clearer distinction = between duration and epoch.=A0 What is the benefit, however, to keep = both notions under the same "time" hierarchy?=A0 Why not, for example, = simply "duration.event" and "epoch.event"?=A0 I'm also concerned that = this list is growing too rapidly.=A0 Timelike modifiers will often = appear in combination with other UCDs - they are more like adjectives = and adverbs than nouns and verbs.=A0 As with other fundamental concepts, = time descriptors should remain elegantly simple and = sparse.

Other = =93computational=94 and =93cosmological=94 words were discussed in = Victoria, also with the Theory IG. We need an input from them in order = to revise/complete the = list

I = have the same response to these terms as I do to VOEvent's - don't these = really represent a different namespace?=A0 In particular, shouldn't the = Theory group=A0 be maintaining this list if they are its primary = target?

Rob Seaman
NOAO
= --Apple-Mail-69-897140808-- From owner-ucd-sci@eso.org Thu Jul 20 14:02:48 2006 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 (8.13.6+Sun/8.12.10) with ESMTP id k6KC0EJh003498 for ; Thu, 20 Jul 2006 14:00:15 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6KC0E34003497 for ucd-sci-outgoing; Thu, 20 Jul 2006 14:00:14 +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 (8.13.6+Sun/8.12.10) with ESMTP id k6KC068P003464 for ; Thu, 20 Jul 2006 14:00:06 +0200 (MEST) Received: from ms0.astro.physik.uni-goettingen.de (ms0.astro.physik.uni-goettingen.de [134.76.204.32]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k6KC04um014701 for ; Thu, 20 Jul 2006 14:00:04 +0200 (CEST) Received: from sisley.astro.physik.uni-goettingen.de ([134.76.205.209]) by ms0.astro.physik.uni-goettingen.de with esmtp (Exim 4.44) id 1G3XC9-0000NA-2l; Thu, 20 Jul 2006 13:59:57 +0200 In-Reply-To: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> References: <20060717110114.0gnivdi8v4c8ggwo@webmail.sic.rm.cnr.it> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: multipart/alternative; boundary=Apple-Mail-3--1004063097 Message-Id: <1EF62D83-43EB-4974-920D-56F4F625D0D8@astro.physik.uni-goettingen.de> Cc: ucd-sci@ivoa.net From: "Frederic V. Hessman" Subject: Re: RFMs (Requests for modification) on the List of UCD-words Date: Thu, 20 Jul 2006 13:59:55 +0200 To: Andrea Preite Martinez X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.7.20.43432 X-Virus-Scanned: by amavisd-new Sender: owner-ucd-sci@eso.org Precedence: bulk Reply-To: "Frederic V. Hessman" --Apple-Mail-3--1004063097 Content-Transfer-Encoding: quoted-printable Content-Type: text/plain; charset=ISO-8859-1; delsp=yes; format=flowed Just a few points: - DM/DE: Why phys.matter.dark and phys.DarkEnergy rather than phys.DarkMatter =20 and phys.energy.dark? - capitalization: I'm confused again about the question of capitalizations: e.g. why =20 phys.DarkEnergy but phys.cosmology.hubble rather than phys.darkEnergy =20= and phys.cosmology.Hubble (or phys.cosmology.hubbleConstant)? Yes, =20 this is a can of worms (e.g. em.uv instead of em.UV), but there =20 should at least be some system (e.g. if you normally write things =20 capitalized, then capitalize, e.g. UV instead of uv, Hubble instead =20 of hubble). - add: obs.calib.flat.sky obs.calib.flat.dome obs.calib.flat.internal phys.particle.neutrino (there are neutrino telescopes) - flux density: Solution (c) using composite UCD's will be cumbersome: =20 phot.flux.perDecade is then phot.flux;em.decade? - length: I'm also confused again about why we have stat.probability (11 =20 letters) and time.duration (8) but comp.sim, and time.expo rather =20 than stat.prob, time.dur, comp.simulation (10 letters) and =20 time.exposure (8). Remind me why we sometimes need to save a few =20 bytes of memory by using occational abbreviations (independent of the =20= length) and can't simply spell things out .... ;-) Rick =09 ------------------------------------------------------------------------=20= ------------------------ Dr. Frederic V. Hessman Hessman@Astro.physik.Uni-Goettingen.DE Institut f=FCr Astrophysik Tel. +49-551-39-5052 Friedrich-Hund-Platz 1 Fax +49-551-39-5043 37077 Goettingen Room F04-133 http://www.Astro.physik.Uni-Goettingen.de/~hessman ------------------------------------------------------------------------=20= ------------------------- MONET: a MOnitoring NEtwork of Telescopes http://monet.Uni-Goettingen.de ------------------------------------------------------------------------=20= ------------------------- --Apple-Mail-3--1004063097 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1 Just a few points:

- DM/DE:

Why phys.matter.dark and = phys.DarkEnergy rather than phys.DarkMatter and = phys.energy.dark?

- = capitalization:

I'm confused again about = the question of capitalizations:=A0 =A0e.g. why phys.DarkEnergy but = phys.cosmology.hubble rather than phys.darkEnergy and = phys.cosmology.Hubble (or phys.cosmology.hubbleConstant)?=A0 =A0Yes, = this is a can of worms (e.g. em.uv instead of em.UV), but there should = at least be some system (e.g. if you normally write things capitalized, = then capitalize, e.g. UV instead of uv, Hubble instead of = hubble).

- = add:

obs.calib.flat.sky
= obs.calib.flat.dome
obs.calib.flat.internal
phys.parti= cle.neutrino = (there are neutrino telescopes)

- flux = density:

Solution (c) using = composite UCD's will be cumbersome:=A0 phot.flux.perDecade is then = phot.flux;em.decade?

- length:

I'm also confused again = about why we have stat.probability (11 letters) and time.duration (8) = but comp.sim,=A0 and time.expo rather than stat.prob, time.dur, = comp.simulation (10 letters) and time.exposure (8).=A0 Remind me why we = sometimes need to save a few bytes of memory by using occational = abbreviations (independent of the length) and can't simply spell things = out ....=A0 ;-)

Rick
=
Institut f=FCr Astrophysik=A0 =A0 =A0 = =A0 =A0 Tel.=A0 +49-551-39-5052
Friedrich-Hund-Platz 1 =A0 =A0 = =A0 =A0 Fax +49-551-39-5043
37077 Goettingen =A0 =A0 =A0 =A0 =A0= =A0 =A0 =A0 Room F04-133
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MONET: a MOnitoring NEtwork of Telescopes
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