From owner-theory@eso.org Wed Apr 21 09:50:53 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i3L7ofBq026966 for ; Wed, 21 Apr 2004 09:50:41 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i3L7oejS026965 for theory-outgoing; Wed, 21 Apr 2004 09:50:40 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i3L7obBq026959 for ; Wed, 21 Apr 2004 09:50:37 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i3L7oaXe012655 for ; Wed, 21 Apr 2004 09:50:36 +0200 (CEST) Received: from localhost (glemson@localhost) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with ESMTP id JAA08670 for ; Wed, 21 Apr 2004 09:50:36 +0200 (METDST) Date: Wed, 21 Apr 2004 09:50:36 +0200 (METDST) From: Lemson Gerard To: theory@ivoa.net Subject: IVOA Theory Interest Group Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: Lemson Gerard X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: During the last IVOA executive meeting, the IVOA Theory Interest Group was formed with the goal of ensuring that theoretical data and services are taken into account in the IVOA standards process. In a whitepaper published on the IVOA site (see http://www.ivoa.net/pub/papers/TheoryInTheVO.pdf) issues specific to theory are discussed. The document also summarizes tasks that a possible theory working group should accomplish, listed here as a proposed charter for the group. The IVOA Theory Interest Group will: - Provide a forum for discussing theory specific issues in a VO context. - Contribute to other IVOA working groups to ensure that theory specific requirements are included. - Incorporate standard approaches defined in these groups when designing and implementing services on theoretical archives. - Define standard services relevant for theoretical archives. - Define relevant milestones and assign specific tasks to interested parties. In the short term, we plan to define a roadmap for activities over the remainder of this year, hopefully including proposals for implementing theory specific demonstrations to be delivered early 2005. This roadmap will be discussed and finalized at the next interoperability meeting in Cambridge, MA. Please subscribe to the Theory mailing list at http://www.ivoa.net/forum/ if you are interested in contributing to this group. A Twiki page has been made available at http://www.ivoa.net/twiki/bin/view/IVOA/IvoaTheory. Please also inform theorists whom you think may be interested in contributing to this effort. We are planning to have a section of the Twiki pages reserved for a registry of existing and planned VO-like theory efforts and would welcome links to such sites. Regards, Gerard Lemson From owner-theory@eso.org Tue May 11 18:39:06 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i4BGcs5t002775 for ; Tue, 11 May 2004 18:38:54 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i4BGcsJ7002774 for theory-outgoing; Tue, 11 May 2004 18:38:54 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i4BGco5t002769; Tue, 11 May 2004 18:38:50 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i4BGcmXe016196; Tue, 11 May 2004 18:38:48 +0200 (CEST) Received: from gavopc1 (gavopc1.xray.mpe.mpg.de [130.183.72.204]) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with SMTP id SAA04319; Tue, 11 May 2004 18:38:47 +0200 (METDST) From: "Gerard Lemson" To: Cc: "Robert Hanisch" , "Rick Harnden" , "Peter Quinn" , "Roy Williams" , "Francois Ochsenbein" , "Doug Tody" , "Masatoshi Ohishi" , "Jonathan McDowell" , "Tony Linde" , "Guy Rixon" , "Nic Walton" , "Tom McGlynn" , "Francoise Genova" Subject: Agenda for Interop Theory Session Date: Tue, 11 May 2004 18:39:20 +0200 Message-ID: MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 8bit X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook IMO, Build 9.0.6604 (9.0.2911.0) In-Reply-To: <026a01c436b4$106d7ac0$7deca782@stsci.edu> X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1409 Importance: Normal X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: "Gerard Lemson" X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Please find below a first proposal for an agenda for the session of the IVOA theory interest group during the interoperability meeting in Cambridge, MA. This session will be held on Tuesday morning, 8:30 – 12:00. I would like to ask the chair persons of the working groups and other interest groups if they are willing to present their thoughts (if they have any) on what it takes to incorporate theoretical datasets or services in their process, if they think this is relevant. I think the groups listed below should have something to say about this, but others are welcome. I think it would be good if representatives of the national VOs could give a short presentation about existing or planned theory projects in their “constituency”, or at least send me links to projects they think are relevant. I would like to add these to the TWiki page (http://www.ivoa.net/twiki/bin/view/IVOA/IvoaTheory) before the meeting starts and btw feel free to do so yourself. If anyone wishes to present a short demo that would be nice. We need to define some concrete projects as well and hopefully we can decide on some during this meeting. We could try to follow the IVOA pattern and define one or more demos and maybe find volunteers to implement these. Please send me your comments on this agenda, if you have any. Thanks Gerard Lemson Agenda 1. Introduction to the theory interest group - why was the group founded ? - what issues are there for theory in the IVOA process ? - discussion of the charter. 2. Relation with working groups. Short presentations by working group chairs on what they think should/could happen on the subject of theory in their group. - DAL : theory specific protocols ? (cone searches or XMatch are not relevant in general) - DM : incorporation of theory (meta-)data in modeling process - UCD : how is theory represented in the UCD list now and how can extensions be made. - Others please. 3. Relation with the astronomical community. - Overview of existing or planned theory related projects. Hopefully representatives of national VOs can give a presentation, possibly with a demo. - Discussion on how we can use the existing projects in the group’s process. Maybe extend into demos ? How can the working groups use these results? - How can we bring the theoretical and observational astronomical community together and create applications that combine theory and observational data ? 4. Discussion of a roadmap for the next year: - Discussion about the interaction between the interest group and the working groups. How can theory issues be incorporated in their process. - How can the theory group be effective in acting as a forum for discussing theory specific aspects and as a source of information for groups building theory related services in a VO compatible manner. - Define one or more theory VO projects to be implemented as demo for next year. - More. From owner-theory@eso.org Fri May 21 21:48:41 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i4LJmQU4011204 for ; Fri, 21 May 2004 21:48:26 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i4LJmQ7n011203 for theory-outgoing; Fri, 21 May 2004 21:48:26 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i4LJmNU4011195 for ; Fri, 21 May 2004 21:48:23 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i4LJmLTY010695 for ; Fri, 21 May 2004 21:48:22 +0200 (CEST) Received: from localhost (glemson@localhost) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with ESMTP id VAA04123; Fri, 21 May 2004 21:48:21 +0200 (METDST) X-Authentication-Warning: mpehp1.mpe-garching.mpg.de: glemson owned process doing -bs Date: Fri, 21 May 2004 21:48:21 +0200 (METDST) From: Gerard Lemson X-Sender: glemson@mpehp1.mpe-garching.mpg.de To: theory@ivoa.net cc: interop@ivoa.met Subject: Agenda theory session Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: Gerard Lemson X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Hi Here an updated version of the agenda for the session of the theory interest group. Review foundation Theory IG - History - Whitepaper - Charter - IVOA Twiki pages Relation to working groups, 10-15 minute presentations - DM : Jonathan McDowell - Application : Tom McGlynn - Not here: DAL, UCD, others ? Concrete TVO efforts, 10-15 minute presentations - NVO : Dave De Young - AstroGrid : Nic Walton - VO France : Francoise Genova - GAVO : Gerard Lemson - Others Discussion/planning - Use cases !!! - How to contact and enthuse astronomical community - WG involvement: where/how should TIG get involved - Define demo(s), who volunteers to implement them ? - Roadmap, dates: next interop in India Sep/Oct 2004, Jan 2005 See you in Cambridge. Gerard Lemson From owner-theory@eso.org Sat May 22 09:15:53 2004 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i4M7FaU3019388 for ; Sat, 22 May 2004 09:15:36 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.6/8.12.6/Submit) id i4M7FacX019387 for theory-outgoing; Sat, 22 May 2004 09:15:36 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.12.6/8.12.6) with ESMTP id i4M7FWU3019381 for ; Sat, 22 May 2004 09:15:32 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id i4M7FVXe001780 for ; Sat, 22 May 2004 09:15:31 +0200 (CEST) Received: from localhost (glemson@localhost) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with ESMTP id JAA22996; Sat, 22 May 2004 09:15:30 +0200 (METDST) X-Authentication-Warning: mpehp1.mpe-garching.mpg.de: glemson owned process doing -bs Date: Sat, 22 May 2004 09:15:30 +0200 (METDST) From: Gerard Lemson X-Sender: glemson@mpehp1.mpe-garching.mpg.de To: theory@ivoa.net cc: interop@ivoa.met Subject: Re: Agenda theory session In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.1.0.84332 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: Gerard Lemson X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Hi again I noticed I forgot to mention the theory session's TWiki page. Please find it at http://www.ivoa.net/twiki/bin/view/IVOA/InterOpMay2004Theory It contains the latest version of the agenda as well as a first list with some reading material. Those of you who are giving a presentation can put any material they have on that page as well. Th page will(should) eventually also contain the material used during the presentations. Thanks Gerard From owner-theory@eso.org Wed Feb 16 18:21:01 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 j1GHKpCA019065 for ; Wed, 16 Feb 2005 18:20:52 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j1GHKpj7019064 for theory-outgoing; Wed, 16 Feb 2005 18:20:51 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 j1GHKmCA019056 for ; Wed, 16 Feb 2005 18:20:48 +0100 (MET) Received: from ppsw-4.csi.cam.ac.uk (ppsw-4.csi.cam.ac.uk [131.111.8.134]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j1GHKkhA001632 for ; Wed, 16 Feb 2005 18:20:46 +0100 (CET) Received: from cass41.ast.cam.ac.uk ([131.111.69.186]:54274) by ppsw-4.csi.cam.ac.uk (ppsw.cam.ac.uk [131.111.8.134]:25) with esmtp id 1D1Sqh-0003KD-FZ (Exim 4.44) for theory@ivoa.net (return-path ); Wed, 16 Feb 2005 17:20:27 +0000 Received: from cass25.ast.cam.ac.uk (cass25 [IPv6:2001:630:200:4240:203:baff:fe24:314]) by cass41.ast.cam.ac.uk (8.12.10+Sun/8.12.10) with ESMTP id j1GHKRoL017245 for ; Wed, 16 Feb 2005 17:20:27 GMT Received: from cass25.ast.cam.ac.uk (localhost [127.0.0.1]) by cass25.ast.cam.ac.uk (8.12.10+Sun/8.12.10) with ESMTP id j1GHKRA1024306 for ; Wed, 16 Feb 2005 17:20:27 GMT Received: from localhost (lds@localhost) by cass25.ast.cam.ac.uk (8.12.10+Sun/8.12.10/Submit) with ESMTP id j1GHKQH6024302 for ; Wed, 16 Feb 2005 17:20:27 GMT X-Authentication-Warning: cass25.ast.cam.ac.uk: lds owned process doing -bs Date: Wed, 16 Feb 2005 17:20:26 +0000 (GMT) From: Laurie Shaw X-X-Sender: lds@cass25 To: theory@ivoa.net Subject: UCDs for simulations Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Cam-ScannerInfo: http://www.cam.ac.uk/cs/email/scanner/ X-Cam-AntiVirus: No virus found X-Cam-SpamDetails: Not scanned X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.0.111621, Antispam-Engine: 2.0.1.0, Antispam-Data: 2005.2.16.8 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: Laurie Shaw X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Hi everyone, I've uploaded a short paper describing my experiences in trying to assign some UCDs (using the UCD1+ definition) to a simulated dataset and associated parameters to the theory interest twiki page. It would be great to get some feedback on this (including other peoples experiences) and to kick-off some discussions on simulated data formats and associated metadata. Thanks, Laurie ---------------- Laurie Shaw Research Student Institute of Astronomy, Univ. of Cambridge From owner-theory@eso.org Fri Feb 18 12:54:52 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 j1IBshmD022631 for ; Fri, 18 Feb 2005 12:54:43 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j1IBshW4022630 for theory-outgoing; Fri, 18 Feb 2005 12:54:43 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 j1IBscmD022620 for ; Fri, 18 Feb 2005 12:54:39 +0100 (MET) Received: from ppsw-4.csi.cam.ac.uk (ppsw-4.csi.cam.ac.uk [131.111.8.134]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j1IBsahA021898 for ; Fri, 18 Feb 2005 12:54:37 +0100 (CET) Received: from cass41.ast.cam.ac.uk ([131.111.69.186]:60335) by ppsw-4.csi.cam.ac.uk (ppsw.cam.ac.uk [131.111.8.134]:25) with esmtp id 1D26iG-0006iH-Dl (Exim 4.44) (return-path ); Fri, 18 Feb 2005 11:54:24 +0000 Received: from cass25.ast.cam.ac.uk (cass25 [IPv6:2001:630:200:4240:203:baff:fe24:314]) by cass41.ast.cam.ac.uk (8.12.10+Sun/8.12.10) with ESMTP id j1IBsLoL013842; Fri, 18 Feb 2005 11:54:21 GMT Received: from cass25.ast.cam.ac.uk (localhost [127.0.0.1]) by cass25.ast.cam.ac.uk (8.12.10+Sun/8.12.10) with ESMTP id j1IBsLA1011042; Fri, 18 Feb 2005 11:54:21 GMT Received: from localhost (lds@localhost) by cass25.ast.cam.ac.uk (8.12.10+Sun/8.12.10/Submit) with ESMTP id j1IBsLk3011039; Fri, 18 Feb 2005 11:54:21 GMT X-Authentication-Warning: cass25.ast.cam.ac.uk: lds owned process doing -bs Date: Fri, 18 Feb 2005 11:54:21 +0000 (GMT) From: Laurie Shaw X-X-Sender: lds@cass25 To: Bernard Debray cc: theory@ivoa.net Subject: Re: UCDs for simulations In-Reply-To: <4215D1A9.9010403@obs-besancon.fr> Message-ID: References: <4215D1A9.9010403@obs-besancon.fr> MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=ISO-8859-1 X-Cam-ScannerInfo: http://www.cam.ac.uk/cs/email/scanner/ X-Cam-AntiVirus: No virus found X-Cam-SpamDetails: Not scanned X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.0.111621, Antispam-Engine: 2.0.1.0, Antispam-Data: 2005.2.18.3 X-Virus-Scanned: by amavisd-new Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from QUOTED-PRINTABLE to 8bit by mercury.hq.eso.org id j1IBshmD022627 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Laurie Shaw X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Dear Bernard, Sorry about that - I forgot to move it on the twiki page. Its now on the IVOA theory page (http://www.ivoa.net/twiki/bin/view/IVOA/IvoaTheory) under 'Papers'. Cheers, Laurie On Fri, 18 Feb 2005, Bernard Debray wrote: > Dear Laurie, > > being interested in reading your document, I have tried to locate it in > the IVOA Twiki forest but I have not been able to find it so far (I have > only found a document by you, Nick Walton and J. Ostriker dating from > June 2004). > So please, could you indicate the URL where I can download your paper ? > Many thanks in advance; with best regards, > Bernard Debray > Observatoire de Besançon > France > > Laurie Shaw wrote: > > >Hi everyone, > > > >I've uploaded a short paper describing my experiences in trying to > >assign some UCDs (using the UCD1+ definition) to a simulated dataset and > >associated parameters to the theory interest twiki page. It would be great > >to get some feedback on this (including other peoples experiences) and to > >kick-off some discussions on simulated data formats and associated > >metadata. > > > >Thanks, > > > >Laurie > > > >---------------- > >Laurie Shaw > >Research Student > >Institute of Astronomy, Univ. of Cambridge > > > > > > > > > From owner-theory@eso.org Thu Mar 10 11:17:30 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 j2AAHDR5016389 for ; Thu, 10 Mar 2005 11:17:14 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j2AAHDRP016388 for theory-outgoing; Thu, 10 Mar 2005 11:17:13 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 j2AAH9R5016377 for ; Thu, 10 Mar 2005 11:17:10 +0100 (MET) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j2AAH8pB028053 for ; Thu, 10 Mar 2005 11:17:08 +0100 (CET) Received: from gavopc1 (gavopc1.xray.mpe.mpg.de [130.183.72.204]) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with SMTP id LAA09192 for ; Thu, 10 Mar 2005 11:17:02 +0100 (MET) From: "Gerard Lemson" To: Subject: IVOA theory sessions in Kyoto Date: Thu, 10 Mar 2005 11:18:43 +0100 Message-ID: MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 8bit X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook IMO, Build 9.0.6604 (9.0.2911.0) Importance: Normal X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1441 X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.0, Antispam-Data: 2005.3.10.0 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: "Gerard Lemson" X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Dear colleagues I would like to know about the plans of any of you to go to the next IVOA meeting in Kyoto and your interest in partaking in one or more sessions of the theory interest group. In particular I would like to know whether you have anything you might like to contribute there, be it a demo or a presentation. Also, do you have any ideas about specific subjects that you would like to see discussed? I think that we should at least have one session there, hopefully two. And as a first proposal I would like to suggest the subjects in the list below to be discussed. The goal should be the construction of some demos that are designed and implemented according to the IVOA philosophy, such as the use of common standards, the registration of datasets and services, solutions promoting interoperability between different sites, promoting the interaction of observers and theorists. I know that some of you have started projects on theory VO issues and I think it would be useful for us to see some of the results already before the meeting. GAVO has made some theory services available on its website (http://www.g-vo.org, in particular http://www.g-vo.org/planck and http://www.g-vo.org/mpasims) and is creating more that will be published there soon, at least in a preliminary fashion. Please submit any links to result to the TVO wiki page or send them to the mailing list. The list of subjects I propose we discuss is: 1. Availability of simulations online. One of the goals of the theory group is to promote the publication of simulation results according to standards developed in the IVOA working groups. A prerequisite for this is that simulation results are actually available online in some form. We need to have examples of this and look at different ways in which simulations results are currently made available online, which kinds of simulations are there, what services are provided for accessing them. From this we can select a first category for which we can look at ... 2. IVOA compatible publication of simulations. We should choose a small set of existing examples which we want to further develop and propose as use cases for the standards process. The further development should consist of work along the lines of the IVOA working groups. In particular: we want it to be possible to register data sets and services in an IVOA registry, we want to be able to describe simulations according to IVOA standard data models, we want to come up with standards for data exchange formats (VOTable?, UCD), we may want to see where the VO query language could be implemented and maybe there are some standard data access services we can define. Some proposals have been made, for example Laurie Shaw’s contributions on a simulation data model and a list of UCDs for simulation data. It would be good if these and other proposals can be discussed in the forum already before the actual meeting in Kyoto, so that we may come up with some proposals we can make to the other working groups. 3. Theory/observational interface. As has often been stated before, the holy grail of the theory work in the IVOA is to promote and facilitate the interaction between observers and theorists by defining and implementing services that make it easy for observers to evaluate and use the results of simulations. The standard example that is consistently mentioned is the "virtual telescope". A software component that can "observe" a simulation and produce mock images that can be directly compared to real observations. GAVO is collaborating with a number of groups who have created such tools which GAVO is publishing on its webpage. The planck simulator is one, others are observations of hydro simulations of galaxy clusters and mock pencil beams through a large scale cosmological simulation. Based on the various examples, it seems to me that this virtual telescope concept offers a nice opportunity to come up with a modularized design specification that allows explicit interoperability between components designed and implemented by experts on their field. I am writing up a proposal on this that I will submit to the mailing list in the coming week (I hope). Please send your comments, criticisms, additions to this proposal to this theory mailing list. Especially send links to examples and other contributions to start some discussion on these items, in particular about the requirements on the IVOA working groups. Cheers Gerard Lemson -- * Gerard Lemson * Tel: +49 (0)89 30000-3316 * * MPI fuer extraterrestische Physik * Fax: +49 (0)89 30000-3569 * * Giessenbachstrasse * * * Postfach 1312 * * * D-85741 Garching, GERMANY * email: gerard.lemson@mpe.mpg.de * From owner-theory@eso.org Fri Mar 25 14:56:07 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 j2PDtx2m010626 for ; Fri, 25 Mar 2005 14:55:59 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j2PDtx4Q010625 for theory-outgoing; Fri, 25 Mar 2005 14:55:59 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 j2PDtt2m010620 for ; Fri, 25 Mar 2005 14:55:55 +0100 (MET) Received: from smtpsortant.univ-lyon1.fr (smtpsortant.univ-lyon1.fr [134.214.100.5]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j2PDtrkW007035 for ; Fri, 25 Mar 2005 14:55:54 +0100 (CET) Received: from pop.univ-lyon1.fr (pop.univ-lyon1.fr [134.214.100.7]) by smtpsortant_no_amavis_spam (Postfix) with ESMTP id 7206335DEF for ; Fri, 25 Mar 2005 15:01:42 +0100 (CET) Received: from pop (localhost [127.0.0.1]) by pop.univ-lyon1.fr (Postfix) with ESMTP id 2F9CB33E74 for ; Fri, 25 Mar 2005 14:55:48 +0100 (CET) Received: from [134.214.4.13] (pc-prugniel.univ-lyon1.fr [134.214.4.13]) by pop.univ-lyon1.fr (Postfix) with ESMTP id B278133E73 for ; Fri, 25 Mar 2005 14:55:47 +0100 (CET) Message-ID: <42441862.8030500@obs.univ-lyon1.fr> Date: Fri, 25 Mar 2005 14:55:46 +0100 From: Philippe Prugniel User-Agent: Mozilla/5.0 (Macintosh; U; PPC Mac OS X Mach-O; en-US; rv:1.7) Gecko/20040616 X-Accept-Language: en-us, en MIME-Version: 1.0 To: theory@ivoa.net Subject: Re: IVOA theory sessions in Kyoto Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit X-Virus-Scanned: by amavisd-new X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.0, Antispam-Data: 2005.3.25.4 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Philippe Prugniel X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: >Dear colleagues <>> >I would like to know about the plans of any of you to go to the next IVOA meeting in Kyoto and your interest in partaking in one or more sessions of >the theory interest group. In particular I would like to know whether you have anything you might like to contribute there, be it a demo or a >presentation. >Also, do you have any ideas about specific subjects that you would like to see >discussed? Hello Gerard and dear colleagues, Thank you for this proposition of TVO-IG session in Kyoto, I agree with the goals you are defining and I will normally attend. I would like to add comments about a specific field of simulated data: SED or more generally spectra. In the recent AVO/EURO-VO science demo (in January in Madrid), two science-cases presented 'fits' of observed SEDs of galaxies against theroretical SEDs (in this case, models of stellar populations). The need for (i) having such theoretical data available and (ii) to fit them to observations was clearly expressed as a priority in the scientific discussions. These applications are a first interesting example of introducing Theory. It is indeed easier to directly fit, or compare, observed and modelled spectra than comparing images (comparing spectra can be almost as simple as subtracting them). Though during this demo it was possible to overplot models to observations, a number of important issues were left open, for example: 1) The current observational DM (Observation or SED) make mandatory informations like the position on the sky (or exposure time...), which are not relevant to modelled data. For this reason it is not possible to express a synthetic spectrum using the SED DM (so the demo was not based on 'pure-standards'). 2) To compare models with observations, we have to take into account the transfert between the source and the observer (which is usually not considered as part of the model): So we need, for example, to tell if a spectrum is corrected for Galactic extinction, internal extinction (within the source)... It seems that the current SED-DM could almost be used for a large range of modelled spectra (except the problems of point my (1)). And the question (2) could concern as well observation or model (we may like either to correct the observation, or to apply some effect to the model). However, other components of the DM are specific of the model: as described in the Provenance object of the excellent paper by L. Shaw and collaborators (on the TVO site). I do not know how we should proceed, either include the theory specification in the more general Observation DM, make a T-DM covering everything from N-body simulations to spectrosopy or make distinct DM for each scientific case... But I can work on the requirements for various applications of model of spectra, trying to connect them with the propositions of L. Shaw. And we could discuss it in Kyoto. Philippe Prugniel. From owner-theory@eso.org Fri Mar 25 15:35:13 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 j2PEZ42m013007 for ; Fri, 25 Mar 2005 15:35:04 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j2PEZ4QM013006 for theory-outgoing; Fri, 25 Mar 2005 15:35:04 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 j2PEYx2m012993 for ; Fri, 25 Mar 2005 15:34:59 +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 j2PEYvkW007759 for ; Fri, 25 Mar 2005 15:34:58 +0100 (CET) Received: from urania.cfa.harvard.edu (urania [131.142.52.147]) by head.cfa.harvard.edu (d/w) with ESMTP id j2PEYpWD011647 for ; Fri, 25 Mar 2005 09:34:51 -0500 (EST) From: Jonathan McDowell Received: (from jcm@localhost) by urania.cfa.harvard.edu (8.12.8p1/8.12.8) id j2PEYn2a018444 for theory@ivoa.net; Fri, 25 Mar 2005 09:34:49 -0500 (EST) Date: Fri, 25 Mar 2005 09:34:49 -0500 (EST) Message-Id: <200503251434.j2PEYn2a018444@urania.cfa.harvard.edu> To: theory@ivoa.net Subject: Re: IVOA theory sessions in Kyoto X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.0, Antispam-Data: 2005.3.25.4 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: Jonathan McDowell X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Phillipe's comments on the SED DM are well taken. I think this really goes to the Characterization model that the CDS team are working on, and the STC model - which already has 'relocatable' options for theory data. So it would be useful in Kyoto to elaborate a Characterization example for such model spectra. - Jonathan McDowell From owner-theory@eso.org Wed Mar 30 19:41:31 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 j2UHfN5D028935 for ; Wed, 30 Mar 2005 19:41:23 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j2UHfNZI028934 for theory-outgoing; Wed, 30 Mar 2005 19:41:23 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 j2UHfJ5D028925 for ; Wed, 30 Mar 2005 19:41:19 +0200 (MEST) Received: from sn.sai.msu.ru (sn.sai.msu.ru [195.208.220.215]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j2UHfIpB005841 for ; Wed, 30 Mar 2005 19:41:18 +0200 (CEST) Received: from sn.sai.msu.ru (localhost [127.0.0.1]) by sn.sai.msu.ru (8.12.8/8.12.8) with ESMTP id j2UHfCWj018519 for ; Wed, 30 Mar 2005 21:41:12 +0400 Received: from localhost (chil@localhost) by sn.sai.msu.ru (8.12.8/8.12.8/Submit) with ESMTP id j2UHfCs4018516 for ; Wed, 30 Mar 2005 21:41:12 +0400 X-Authentication-Warning: sn.sai.msu.ru: chil owned process doing -bs Date: Wed, 30 Mar 2005 21:41:12 +0400 (MSD) From: Igor Chilingarian X-X-Sender: chil@sn.sai.msu.ru To: theory@ivoa.net Subject: experimental SSA-like access to PEGASE.HR 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: 2.0.3.0, Antispam-Data: 2005.3.30.8 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: Igor Chilingarian X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Dear colleagues, I'd like to present an experimental access to PEGASE.HR synthetic spectra of galaxies. We tried to adapt the SSAP response format in order to be able to access synthetic spectra with SSA protocol and, for example display them with the ESA VOSpec tool. The CGI interface is availbale here: http://vo.obspm.fr/cgi-bin/siap/pegasehr.pl See brief description of usage at the same page. The present access is a simple demonstration of embedding Pegase in a service similar to SSA. It is not intended to be used for scientific research. The service is not registered. With best regards, Igor From owner-apps@eso.org Mon Apr 18 13:57:37 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3IBvLlP015794 for ; Mon, 18 Apr 2005 13:57:21 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3IBvL2g015793 for apps-outgoing; Mon, 18 Apr 2005 13:57:21 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-apps@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 j3IBvElP015772; Mon, 18 Apr 2005 13:57:14 +0200 (MEST) Received: from esacom51.vilspa.esa.int (esacom51-ext.vilspa.esa.int [192.171.2.19]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3IBvCsi025553; Mon, 18 Apr 2005 13:57:13 +0200 (CEST) Received: from esacom65.vilspa.esa.int (esacom65.vilspa.esa.int [131.176.121.32]) by esacom51.vilspa.esa.int (8.12.10/8.12.10/ESA-External-v3.2) with ESMTP id j3IBuwHY022393; Mon, 18 Apr 2005 13:56:58 +0200 (MET DST) Received: from vilspamail2.vilspa.esa.int (vilspamail2.vilspa.esa.int [131.176.121.241]) by esacom65.vilspa.esa.int (8.12.9/8.12.9/ESA-Internal-v3.2) with ESMTP id j3IBuvO9017515; Mon, 18 Apr 2005 13:56:57 +0200 (MET DST) Subject: Comparison between observational and theoretical SEDs in VO. To: theory@ivoa.net, apps@ivoa.net Cc: Gerard.Lemson@mpe.mpg.de X-Mailer: Lotus Notes Release 5.0.3 (Intl) 21 March 2000 Message-ID: From: Enrique.Solano@esa.int Date: Mon, 18 Apr 2005 13:56:56 +0200 X-MIMETrack: Serialize by Router on vilspamail2/vilspa/ESA(Release 5.0.13a |April 8, 2004) at 04/18/2005 01:56:58 PM 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: 2.0.3.0, Antispam-Data: 2005.4.18.3 X-Virus-Scanned: by amavisd-new Sender: owner-apps@eso.org Precedence: bulk Reply-To: Enrique.Solano@esa.int X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Dear all, This is to let you know that, in the context of a collaborative framework between the Spanish virtual Observatory (SVO) and ESA-VO, we are developing a service to handle theoretical data (presently, stellar spectral data). The service uses VOSpec ( http://pma.standby.vilspa.esa.es:8080/vospec/index.html) as a plotting utility. There is already a prototype version of the system that will be presented in the Kyoto interop. during the Theory session. The system works in a SSA-like way in a "two-steps" process: using the "format=metadata" option, the system returns a list of parameters that can be used for the query. Then, a proper consult can be done and the system returns a VOTable including a link to the data and that follows as close as possible the spectral data model. In the near future we plan to implement a proper fitting tool between theoretical and observational SEDs. This will require passing the observed SED to the theoretical server. On the other hand, we also plan to make a short presentation of PGos3, a collaboration between the Mexico-VO and SVO. PGos3 is a service that provides synthetic spectra, evolutionary tracks, isochrones and photoionization models. A preliminary version of the system can be found at: http://ov.inaoep.mx Cheers, Enrique Solano (SVO) & Pedro Osuna (ESA-VO) From owner-apps@eso.org Mon Apr 18 14:34:44 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 j3ICYRlP023107 for ; Mon, 18 Apr 2005 14:34:27 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j3ICYRi3023106 for apps-outgoing; Mon, 18 Apr 2005 14:34:27 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-apps@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 j3ICYElP023081; Mon, 18 Apr 2005 14:34:14 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j3ICYCsi027374; Mon, 18 Apr 2005 14:34:12 +0200 (CEST) Received: from [130.183.72.144] (gavopc2.xray.mpe.mpg.de [130.183.72.144]) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with ESMTP id OAA15360; Mon, 18 Apr 2005 14:33:44 +0200 (METDST) Message-ID: <4263A92B.90806@mpe.mpg.de> Date: Mon, 18 Apr 2005 14:33:47 +0200 From: Hans-Martin Adorf Organization: MPE User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.0; en-US; rv:1.7.2) Gecko/20040804 Netscape/7.2 (ax) X-Accept-Language: en-us, en MIME-Version: 1.0 To: Enrique.Solano@esa.int CC: theory@ivoa.net, apps@ivoa.net, Gerard.Lemson@mpe.mpg.de, Wolfgang Voges , Harry Enke Subject: Re: Comparison between observational and theoretical SEDs in VO. References: In-Reply-To: Content-Type: multipart/alternative; boundary="------------050209020404050507030903" X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.0.111621, Antispam-Engine: 2.0.1.0, Antispam-Data: 2005.4.18.3 X-Virus-Scanned: by amavisd-new Sender: owner-apps@eso.org Precedence: bulk Reply-To: Hans-Martin Adorf X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: This is a multi-part message in MIME format. --------------050209020404050507030903 Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 8bit Hi Enrique, I'm intrigued by your announcement. The one thing I'd like to add is that since quite a while we, at the German Astrophysical Virtual Observatory, have been working on a tool that can be used for comparing observed with theoretical SEDs. The tool implements a statistical classifier and is available on our Web (http://www.g-vo.org/portal/tile/products/services/sedclassifier/index.jsp). It is currently being used in a scientific project. So far we have not incorporated any VOTable or VOSpec into our SED classifier, but are looking forward to doing so at some suitable point. May be we could join forces. Unfortunately, none of us will be participating in the Kyoto event, so we will have to look for another opportunity, in case you're interested. I myself am certainly open to discussions, also over the phone, at least to get started. Cheers Hans-Martin Enrique.Solano@esa.int wrote: >Dear all, > >This is to let you know that, in the context of a collaborative framework >between the Spanish virtual Observatory (SVO) and ESA-VO, we >are developing a service to handle theoretical data (presently, stellar >spectral data). The service uses VOSpec ( >http://pma.standby.vilspa.esa.es:8080/vospec/index.html) as a plotting >utility. There is already a prototype version of the system that will be >presented in the Kyoto interop. during the Theory session. > >The system works in a SSA-like way in a "two-steps" process: using the >"format=metadata" option, the system returns a list of parameters that can be >used for the query. Then, a proper consult can be done and the system returns >a VOTable including a link to the data and that follows as close as possible >the spectral data model. > >In the near future we plan to implement a proper fitting tool between >theoretical and observational SEDs. This will require passing the observed >SED to the theoretical server. > >On the other hand, we also plan to make a short presentation of PGos3, a >collaboration between the Mexico-VO and SVO. PGos3 is a service that >provides synthetic spectra, evolutionary tracks, isochrones and >photoionization models. A preliminary version of the system can be found at: >http://ov.inaoep.mx > >Cheers, > >Enrique Solano (SVO) & Pedro Osuna (ESA-VO) > > > > > > -- Dr. Hans-Martin Adorf . Max-Planck-Institut f. extraterrestrische Physik . Giessenbachstr. 1 . D-85741 Garching b. München . Germany Phone: +49-89-30000-3352 . Fax: +49-89-30000-3404 . E-Mail: adorf@mpe.mpg.de . WWW: http://www.g-vo.org --------------050209020404050507030903 Content-Type: text/html; charset=us-ascii Content-Transfer-Encoding: 7bit Hi Enrique,

I'm intrigued by your announcement. The one thing I'd like to add is that since quite a while we, at the German Astrophysical Virtual Observatory, have been working on a tool that can be used for comparing observed with theoretical SEDs. The tool implements a statistical classifier and is available on our Web (http://www.g-vo.org/portal/tile/products/services/sedclassifier/index.jsp). It is currently being used in a scientific project.

So far we have not incorporated any VOTable or VOSpec into our SED classifier, but are looking forward to doing so at some suitable point. May be we could join forces. Unfortunately, none of us will be participating in the Kyoto event, so we will have to look for another opportunity, in case you're interested. I myself am certainly open to discussions, also over the phone, at least to get started.

Cheers
Hans-Martin


Enrique.Solano@esa.int wrote:
Dear all,

This is to let you know that, in the context of a collaborative framework
between the Spanish virtual Observatory (SVO) and ESA-VO, we
are developing a service to handle theoretical data (presently, stellar
spectral data). The service uses VOSpec (
http://pma.standby.vilspa.esa.es:8080/vospec/index.html)  as a plotting
utility. There is already a prototype version of the system that will be
presented  in the Kyoto interop. during the Theory session.

The system works in a SSA-like way in a "two-steps" process: using the
"format=metadata" option, the system returns a list of parameters that can be
used for the query. Then, a proper consult can be done and the system returns
a VOTable including a link to the data and that follows as close as possible
the spectral data model.

In the near future we plan to implement a proper fitting tool between
theoretical and observational SEDs. This will require passing the observed
SED to the theoretical server.

On the other hand, we also plan to make a short presentation of PGos3,  a
collaboration between the Mexico-VO and SVO. PGos3 is a service that
provides synthetic spectra, evolutionary tracks, isochrones and
photoionization models. A preliminary version of the system can be found at:
http://ov.inaoep.mx

Cheers,

Enrique Solano (SVO) & Pedro Osuna (ESA-VO)

--
Dr. Hans-Martin Adorf Dr. Hans-Martin Adorf • Max-Planck-Institut f. extraterrestrische Physik • Giessenbachstr. 1 • D-85741 Garching b. München • Germany
Phone: +49-89-30000-3352 • Fax: +49-89-30000-3404 • E-Mail: adorf@mpe.mpg.de • WWW: http://www.g-vo.org
--------------050209020404050507030903-- From owner-theory@eso.org Tue May 10 12:20:27 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 j4AAKG1u014574 for ; Tue, 10 May 2005 12:20:17 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4AAKGYf014573 for theory-outgoing; Tue, 10 May 2005 12:20:16 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 j4AAKA1u014537 for ; Tue, 10 May 2005 12:20:11 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4AAK9XW005406 for ; Tue, 10 May 2005 12:20:09 +0200 (CEST) Received: from gavopc1 (gavopc1.xray.mpe.mpg.de [130.183.72.204]) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with SMTP id MAA09689; Tue, 10 May 2005 12:20:03 +0200 (METDST) From: "Gerard Lemson" To: Cc: , , , , , , Subject: agenda theory session Kyoto Date: Tue, 10 May 2005 12:23:03 +0200 Message-ID: MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 8bit X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook IMO, Build 9.0.6604 (9.0.2911.0) Importance: Normal X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1441 X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.10.4 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: "Gerard Lemson" X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Dear Collegues After receiving some feedback to the email reproduced below I propose the following agenda for the theory session in Kyoto, which is scheduled for wednesday morening. First we'll have some presentations, each about 15 minutes: 1. Dave De Young on activities regarding a data repository for theory simulations in the USA. 2. Enrique Solano: PGos3, a prototype for synthetic spectra and evolutionary model computation in the VO (see http://ov.inaoep.mx/) 3. Laurie Shaw on data model and UCDs for theory (see his papers at the theory TWiki site http://www.ivoa.net/twiki/bin/view/IVOA/IvoaTheory) and/or webservices for producing SZ maps and comparig them to observations. 4. Gerard Lemson: theory VO activities in Germany(see www.g-vo.org/mpasims, www.g-vo.org/planck, www.g-vo.org/hydrosims, or http://gavows2.xray.mpe.mpg.de:8080/hydrosims in case the public site is not up yet). Upon request I will also present work done by the groups at JHU/Hungary on theory spectra These presentations about cover the subjects proposed in the email below, with some emphasis on theory spectra, which clearly is of interest for a number of people. I propose to have discussions about these subjects in the remainder of the session. In particular we should discuss: 1. Publishing theory datasets:, how to archive them, how to wrap them with web services them available. 2. Models for metadata describing these datasets. Here we may pay special attention to theory spectra, as it is closest to the data model that is developed furthest in the DM/DAL working groups, but offers different requirements. It would be good if representatives of these working groups could attend this meeting. 3. Making theory services/application available online, both for analysing/visualising these datasets and simulators for creating new ones. Here we should address interoperability, how to tie different services together. And we should pay special attention to the interaction between observational and theoretical services. I can discuss efforts that GAVO is involved in with both theorists and observers around Munich and in various collaborations that have this as their goal. It would be good if within the IVOA we could organize some similar projects. I hope that members of working groups can attend these discussions. Please send any comments to the mailing list. Thanks and see you in Kyoto Gerard -- * Gerard Lemson * Tel: +49 (0)89 30000-3316 * * MPI fuer extraterrestische Physik * Fax: +49 (0)89 30000-3569 * * Giessenbachstrasse * * * Postfach 1312 * * * D-85741 Garching, GERMANY * email: gerard.lemson@mpe.mpg.de * > Dear colleagues > > I would like to know about the plans of any of you to go to the next IVOA > meeting in Kyoto and your interest in partaking in one or more sessions of > the theory interest group. In particular I would like to know whether you > have anything you might like to contribute there, be it a demo or a > presentation. > Also, do you have any ideas about specific subjects that you would like to > see > discussed? > > I think that we should at least have one session there, hopefully two. > And as a first proposal I would like to suggest the subjects in the list > below to be discussed. The goal should be the construction of some demos > that are designed and implemented according to the IVOA philosophy, such > as the use of common standards, the registration of datasets and services, > solutions promoting interoperability between different sites, promoting > the interaction of observers and theorists. > > I know that some of you have started projects on theory VO issues and I > think it would be useful for us to see some of the results already before > the meeting. GAVO has made some theory services available on its website > (http://www.g-vo.org, in particular http://www.g-vo.org/planck and > http://www.g-vo.org/mpasims) and is creating more that will be published > there soon, at least in a preliminary fashion. Please submit any links > to result to the TVO wiki page or send them to the mailing list. > > The list of subjects I propose we discuss is: > 1. Availability of simulations online. > One of the goals of the theory group is to promote the publication of > simulation results according to standards developed in the IVOA working > groups. A prerequisite for this is that simulation results are actually > available online in some form. We need to have examples of this and look at > different ways in which simulations results are currently made available > online, which kinds of simulations are there, what services are provided > for accessing them. From this we can select a first category for which > we can look at ... > > 2. IVOA compatible publication of simulations. > We should choose a small set of existing examples which we want to further > develop and propose as use cases for the standards process. The further > development > should consist of work along the lines of the IVOA working groups. In > particular: > we want it to be possible to register data sets and services in an IVOA > registry, > we want to be able to describe simulations according to IVOA standard data > models, > we want to come up with standards for data exchange formats (VOTable?, UCD), > we > may want to see where the VO query language could be implemented and maybe > there > are some standard data access services we can define. Some proposals have > been > made, for example Laurie Shaw’s contributions on a simulation data model and > a > list of UCDs for simulation data. It would be good if these and other > proposals > can be discussed in the forum already before the actual meeting in Kyoto, so > that we may come up with some proposals we can make to the other working > groups. > > 3. Theory/observational interface. > As has often been stated before, the holy grail of the theory work in the > IVOA > is to promote and facilitate the interaction between observers and theorists > by > defining and implementing services that make it easy for observers to > evaluate > and use the results of simulations. The standard example that is > consistently > mentioned is the "virtual telescope". A software component that can > "observe" > a simulation and produce mock images that can be directly compared to real > observations. GAVO is collaborating with a number of groups who have created > such tools which GAVO is publishing on its webpage. The planck simulator is > one, others are observations of hydro simulations of galaxy clusters and > mock > pencil beams through a large scale cosmological simulation. Based on the > various examples, it seems to me that this virtual telescope concept offers > a nice opportunity to come up with a modularized design specification that > allows explicit interoperability between components designed and implemented > by experts on their field. I am writing up a proposal on this that I will > submit to the mailing list in the coming week (I hope). > > Please send your comments, criticisms, additions to this proposal to this > theory mailing list. Especially send links to examples and other > contributions > to start some discussion on these items, in particular about the > requirements > on the IVOA working groups. > > Cheers > > Gerard Lemson From owner-theory@eso.org Wed May 11 04:55:23 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 j4B2tFnt015107 for ; Wed, 11 May 2005 04:55:15 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4B2tFU3015106 for theory-outgoing; Wed, 11 May 2005 04:55:15 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 j4B2tAnt015100 for ; Wed, 11 May 2005 04:55:10 +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 j4B2t873004302 for ; Wed, 11 May 2005 04:55:09 +0200 (CEST) Received: from urania.cfa.harvard.edu (urania [131.142.52.147]) by head.cfa.harvard.edu (d/w) with ESMTP id j4B2t2Ci014766 for ; Tue, 10 May 2005 22:55:02 -0400 (EDT) From: Jonathan McDowell Received: (from jcm@localhost) by urania.cfa.harvard.edu (8.12.8p1/8.12.8) id j4B2t288015793 for theory@ivoa.net; Tue, 10 May 2005 22:55:02 -0400 (EDT) Date: Tue, 10 May 2005 22:55:02 -0400 (EDT) Message-Id: <200505110255.j4B2t288015793@urania.cfa.harvard.edu> To: theory@ivoa.net Subject: Laurie's UCD paper X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.10.36 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: Jonathan McDowell X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Dear IVOA theory, after recent work on UCDs I've gone back to look at Laurie's paper on UCDs for simulations. In general I like the sim.* tree, but I don't like the sim.param.* and phys.param.* trees. It seems to me that the things listed in those trees are quantities that could simply be in the phys.* trees, and might appear in other contexts than simulations. I suggest instead sim.* as "UCD secondary words", and so UCDs like phys.cosmology.hubble time.step;sim.param phys.size;sim.extent;sim.param and so on. "What is this? First of all, it's a physical size. What kind of physical size? It's the extent of a simulation, and it's one of the parameters to the simulation". Similarly, rather than sim.obj.star I'd say "src.class.star;sim.obj" ("It's a star; oh by the way it's a simulated star") and "pos.frame.cartesian" instead of "sim.coordsys.cart" (nothing particularly "sim" about it, except that it's what STC calls a 'relocatable' frame - if you insist, "pos.frame.cartesian;pos.sim.relocatable") In contrast, the sim.alg and sim.resource trees don't correspond to to astronomical things, but sim.resource UCDs could equally well correspond to observation reduction pipeline things. An earlier attempt to propose a software tree got shot down, but I think it has to come back at some point, e.g. soft.processors or meta.compute.processors or something. For the phys.param, how about phys.cosmology.omega;phys.matter phys.cosmology.omega;phys.darkEnergy on the principle that different kinds of omega are basically the same concept and should be distinguished by secondary UCDs... Along the same lines, we might want to record other kinds of algorithms like smoothing algorithms applied to data, so soft.alg.sim.nbody might be better than sim.alg.nbody. In the above I have taken as a general principle: What's most important is the concept, not whether it's simulated or not. In many cases what you're simulating has a counterpart in the real universe; in those cases the "sim.something" should be a qualifying adjective, not the main concept. So things like sim.obj.particle, which are truly simulation specific, should stay as Laurie has proposed. I'm not sure about sim.obj.halo, I guess that's a sim-specific thing, but sim.obj.gal sure isn't. (Note that the whole issue of a UCD tree for an astronomical object ontology has recently come up again for the nth time. I'm sure it will eventually happen despite the naysayers.) - Jonathan McDowell From owner-theory@eso.org Thu May 12 10:59:02 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 j4C8wqWX025626 for ; Thu, 12 May 2005 10:58:53 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4C8wqDq025625 for theory-outgoing; Thu, 12 May 2005 10:58:52 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 j4C8wlWX025609 for ; Thu, 12 May 2005 10:58:47 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4C8wjXW015997 for ; Thu, 12 May 2005 10:58:45 +0200 (CEST) Received: from gavopc1 (gavopc1.xray.mpe.mpg.de [130.183.72.204]) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with SMTP id KAA16839; Thu, 12 May 2005 10:58:39 +0200 (METDST) From: "Gerard Lemson" To: Cc: , , , , , , Subject: RE: agenda theory session Kyoto Date: Thu, 12 May 2005 11:01:41 +0200 Message-ID: MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 8bit X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook IMO, Build 9.0.6604 (9.0.2911.0) X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1441 In-Reply-To: Importance: Normal X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.12.2 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: "Gerard Lemson" X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: There is an update to the agenda of the theory session (which should end of this day be available on TWiki). There is an extra presentation by Philippe Prugniel title: Model and Access requirement for spectral-modelling services: Projects in VO-France -- * Gerard Lemson * Tel: +49 (0)89 30000-3316 * * MPI fuer extraterrestische Physik * Fax: +49 (0)89 30000-3569 * * Giessenbachstrasse * * * Postfach 1312 * * * D-85741 Garching, GERMANY * email: gerard.lemson@mpe.mpg.de * > -----Original Message----- > From: Gerard Lemson [mailto:gerard.lemson@mpe.mpg.de] > Sent: Tuesday, May 10, 2005 12:23 PM > To: theory@ivoa.net > Cc: lds@ast.cam.ac.uk; prugniel@obs.univ-lyon1.fr; > jcm@head.cfa.harvard.edu; deyoung@noao.edu; Enrique.Solano@esa.int; > mcs@iaa.es; herve.wozniak@obs.univ-lyon1.fr > Subject: agenda theory session Kyoto > > > > > Dear Collegues > After receiving some feedback to the email reproduced below I > propose the following > agenda for the theory session in Kyoto, which is scheduled for > wednesday morening. > > First we'll have some presentations, each about 15 minutes: > > 1. Dave De Young on activities regarding a data repository for > theory simulations in the USA. > 2. Enrique Solano: PGos3, a prototype for synthetic spectra and > evolutionary model computation in the VO > (see http://ov.inaoep.mx/) > 3. Laurie Shaw on data model and UCDs for theory (see his papers > at the theory TWiki site > http://www.ivoa.net/twiki/bin/view/IVOA/IvoaTheory) and/or > webservices for producing SZ maps and comparig them to observations. > 4. Gerard Lemson: theory VO activities in Germany(see > www.g-vo.org/mpasims, www.g-vo.org/planck, > www.g-vo.org/hydrosims, or > http://gavows2.xray.mpe.mpg.de:8080/hydrosims in case the public site > is not up yet). > Upon request I will also present work done by the groups at > JHU/Hungary on theory spectra > > These presentations about cover the subjects proposed in the > email below, with some emphasis > on theory spectra, which clearly is of interest for a number of people. > I propose to have discussions about these subjects in the > remainder of the session. > In particular we should discuss: > > 1. Publishing theory datasets:, how to archive them, how to wrap > them with web services them available. > 2. Models for metadata describing these datasets. > Here we may pay special attention to theory spectra, as it is > closest to the data model that > is developed furthest in the DM/DAL working groups, but offers > different requirements. > It would be good if representatives of these working groups > could attend this meeting. > 3. Making theory services/application available online, both for > analysing/visualising > these datasets and simulators for creating new ones. Here we > should address interoperability, > how to tie different services together. And we should pay > special attention to the interaction > between observational and theoretical services. I can discuss > efforts that GAVO is involved in > with both theorists and observers around Munich and in various > collaborations that have this > as their goal. It would be good if within the IVOA we could > organize some similar projects. > > I hope that members of working groups can attend these discussions. > > Please send any comments to the mailing list. > > Thanks and see you in Kyoto > > Gerard > > > > -- > * Gerard Lemson * Tel: +49 (0)89 30000-3316 > * > * MPI fuer extraterrestische Physik * Fax: +49 (0)89 30000-3569 > * > * Giessenbachstrasse * > * > * Postfach 1312 * > * > * D-85741 Garching, GERMANY * email: > gerard.lemson@mpe.mpg.de * > > > Dear colleagues > > > > I would like to know about the plans of any of you to go to the > next IVOA > > meeting in Kyoto and your interest in partaking in one or more > sessions of > > the theory interest group. In particular I would like to know > whether you > > have anything you might like to contribute there, be it a demo or a > > presentation. > > Also, do you have any ideas about specific subjects that you > would like to > > see > > discussed? > > > > I think that we should at least have one session there, hopefully two. > > And as a first proposal I would like to suggest the subjects in the list > > below to be discussed. The goal should be the construction of some demos > > that are designed and implemented according to the IVOA philosophy, such > > as the use of common standards, the registration of datasets > and services, > > solutions promoting interoperability between different sites, promoting > > the interaction of observers and theorists. > > > > I know that some of you have started projects on theory VO issues and I > > think it would be useful for us to see some of the results > already before > > the meeting. GAVO has made some theory services available on its website > > (http://www.g-vo.org, in particular http://www.g-vo.org/planck and > > http://www.g-vo.org/mpasims) and is creating more that will be published > > there soon, at least in a preliminary fashion. Please submit any links > > to result to the TVO wiki page or send them to the mailing list. > > > > The list of subjects I propose we discuss is: > > 1. Availability of simulations online. > > One of the goals of the theory group is to promote the publication of > > simulation results according to standards developed in the IVOA working > > groups. A prerequisite for this is that simulation results are actually > > available online in some form. We need to have examples of this > and look at > > different ways in which simulations results are currently made available > > online, which kinds of simulations are there, what services are provided > > for accessing them. From this we can select a first category for which > > we can look at ... > > > > 2. IVOA compatible publication of simulations. > > We should choose a small set of existing examples which we want > to further > > develop and propose as use cases for the standards process. The further > > development > > should consist of work along the lines of the IVOA working groups. In > > particular: > > we want it to be possible to register data sets and services in an IVOA > > registry, > > we want to be able to describe simulations according to IVOA > standard data > > models, > > we want to come up with standards for data exchange formats > (VOTable?, UCD), > > we > > may want to see where the VO query language could be > implemented and maybe > > there > > are some standard data access services we can define. Some > proposals have > > been > > made, for example Laurie Shaw’s contributions on a simulation > data model and > > a > > list of UCDs for simulation data. It would be good if these and other > > proposals > > can be discussed in the forum already before the actual meeting > in Kyoto, so > > that we may come up with some proposals we can make to the other working > > groups. > > > > 3. Theory/observational interface. > > As has often been stated before, the holy grail of the theory > work in the > > IVOA > > is to promote and facilitate the interaction between observers > and theorists > > by > > defining and implementing services that make it easy for observers to > > evaluate > > and use the results of simulations. The standard example that is > > consistently > > mentioned is the "virtual telescope". A software component that can > > "observe" > > a simulation and produce mock images that can be directly > compared to real > > observations. GAVO is collaborating with a number of groups who > have created > > such tools which GAVO is publishing on its webpage. The planck > simulator is > > one, others are observations of hydro simulations of galaxy clusters and > > mock > > pencil beams through a large scale cosmological simulation. Based on the > > various examples, it seems to me that this virtual telescope > concept offers > > a nice opportunity to come up with a modularized design > specification that > > allows explicit interoperability between components designed > and implemented > > by experts on their field. I am writing up a proposal on this > that I will > > submit to the mailing list in the coming week (I hope). > > > > Please send your comments, criticisms, additions to this > proposal to this > > theory mailing list. Especially send links to examples and other > > contributions > > to start some discussion on these items, in particular about the > > requirements > > on the IVOA working groups. > > > > Cheers > > > > Gerard Lemson From owner-theory@eso.org Tue May 17 03:21:04 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 j4H1KubO025217 for ; Tue, 17 May 2005 03:20:56 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4H1Kuu9025216 for theory-outgoing; Tue, 17 May 2005 03:20:56 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 j4H1KqbO025210 for ; Tue, 17 May 2005 03:20:52 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4H1KpXW003918 for ; Tue, 17 May 2005 03:20:51 +0200 (CEST) Received: from localhost (glemson@localhost) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with ESMTP id DAA04197; Tue, 17 May 2005 03:20:45 +0200 (METDST) X-Authentication-Warning: mpehp1.mpe-garching.mpg.de: glemson owned process doing -bs Date: Tue, 17 May 2005 03:20:44 +0200 (METDST) From: Gerard Lemson X-Sender: glemson@mpehp1.mpe-garching.mpg.de To: Enrique.Solano@esa.int cc: theory@ivoa.net Subject: RE: agenda theory session Kyoto In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=X-UNKNOWN X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.16.39 X-Virus-Scanned: by amavisd-new Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from QUOTED-PRINTABLE to 8bit by mercury.hq.eso.org id j4H1KubO025212 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Gerard Lemson X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: A slight update to the agenda of the theory session to accomodate Enrique's request is made to the session agenda on the twiki page. Gerard On Thu, 12 May 2005 Enrique.Solano@esa.int wrote: > > Hi Gerard, > > I would like to change the title of my contribution. It should be: > > "TSAP: a VO-protocol to access theoretical data. Application to PGos3" > > Many thanks in advance. > > Cheers, > ________________________ > Enrique Solano Márquez > LAEFF/INTA > Spanish Virtual Observatory > P.O. BOX 50727 > 28080 Madrid > Spain > e-mail: esm@laeff.esa.es > Phone: 34 - 91 813 11 00 > Fax: 34 - 91 813 11 60 > ------------------------- > > From owner-theory@eso.org Tue May 24 09:09:44 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 j4O79VMi017765 for ; Tue, 24 May 2005 09:09:32 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4O79VBx017764 for theory-outgoing; Tue, 24 May 2005 09:09:31 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 j4O79QMi017749 for ; Tue, 24 May 2005 09:09:26 +0200 (MEST) Received: from ppsw-0.csi.cam.ac.uk (ppsw-0.csi.cam.ac.uk [131.111.8.130]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j4O79OXW020773 for ; Tue, 24 May 2005 09:09:24 +0200 (CEST) X-Cam-SpamDetails: Not scanned X-Cam-AntiVirus: No virus found X-Cam-ScannerInfo: http://www.cam.ac.uk/cs/email/scanner/ Received: from cass41.ast.cam.ac.uk ([131.111.69.186]:35515) by ppsw-0.csi.cam.ac.uk (ppsw.cam.ac.uk [131.111.8.130]:25) with esmtp id 1DaTXR-0008Ex-20 (Exim 4.51) (return-path ); Tue, 24 May 2005 08:09:17 +0100 Received: from cass25.ast.cam.ac.uk (cass25 [IPv6:2001:630:200:4240:203:baff:fe24:314]) by cass41.ast.cam.ac.uk (8.12.10+Sun/8.12.10) with ESMTP id j4O79HoL010313; Tue, 24 May 2005 08:09:17 +0100 (BST) Received: from cass25.ast.cam.ac.uk (localhost [127.0.0.1]) by cass25.ast.cam.ac.uk (8.12.10+Sun/8.12.10) with ESMTP id j4O79GSQ016515; Tue, 24 May 2005 08:09:16 +0100 (BST) Received: from localhost (lds@localhost) by cass25.ast.cam.ac.uk (8.12.10+Sun/8.12.10/Submit) with ESMTP id j4O79G4k016512; Tue, 24 May 2005 08:09:16 +0100 (BST) X-Authentication-Warning: cass25.ast.cam.ac.uk: lds owned process doing -bs Date: Tue, 24 May 2005 08:09:16 +0100 (BST) From: Laurie Shaw X-X-Sender: lds@cass25 To: Gerard Lemson cc: theory@ivoa.net Subject: Simulation data model working draft In-Reply-To: Message-ID: References: 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: 2005.5.23.45 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: Laurie Shaw X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Hi everyone, I've now added the latest draft of the simulation data model to the IVOA theory twiki page [Simulation.v.0.2.doc]. Comments and feedback would be great! Thanks, Laurie From owner-theory@eso.org Tue May 24 11:16:44 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 j4O9GWMi011616 for ; Tue, 24 May 2005 11:16:32 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4O9GWfW011615 for theory-outgoing; Tue, 24 May 2005 11:16:32 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 j4O9GSMi011600 for ; Tue, 24 May 2005 11:16:28 +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 j4O9GQ73019223 for ; Tue, 24 May 2005 11:16:26 +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 LAA02448; Tue, 24 May 2005 11:16:11 +0200 (MET DST) In-Reply-To: References: Mime-Version: 1.0 (Apple Message framework v622) Content-Type: text/plain; charset=ISO-8859-1; format=flowed Message-Id: <893802e097f3f70a21469e5e2d482749@iaa.es> Cc: Enrique.Solano@esa.int, theory@ivoa.net, Gerard Lemson , =?ISO-8859-1?Q?Miguel_Cervi=F1o?= From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Re: Simulation data model working draft Date: Tue, 24 May 2005 11:16:33 +0200 To: Laurie Shaw X-Mailer: Apple Mail (2.622) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.24.2 X-Virus-Scanned: by amavisd-new Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id j4O9GWMi011609 Sender: owner-theory@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Dear all, I just provide some feedback to the just posted document by Laurie. My point of view is more focussed in the data model that refers to: - Spectral Energy distributions (atmosphere models + results of synthesis models) - Stellar evolution (evolutionary tracks, isochrones and Color Magnitude Diagrams) - The interrelation (pipe-line) between both in a VO environment So, my suggestions are oriented to include these kind of theoretical data in the proposed working draft. My suggestions concern to the next points in the posted document: 4.2. Characterisation: I would let the characterisation items in the simulations the most similar to the ones in observations as possible. And include some additional "objects" for simulations (like "physical parameters" and something like "Model Resolution" instead reuse "Resolution"). Here comes my reasons: In the case of synthesis models, several times the results have been obtained by the use of observed objects (e.j. observational stellar libraries as commonly used in some synthesis models like STEBLIB in Bruzual & Charlot, HST data in Starburst 99 or ELODIE in PEGASE-HR). In this situation, the results of the models, are not purely theoretical, but based in observations: results depends on: - Bounds and Resolution "classes" from the observations - "model resolution" class in the used algorimths inside the code. Summing up: I would propose that the theoretical data model "includes" the observational one, PLUS some extensions (e.g.: physical parameters or model resolution), instead to re-use the objects used in observations with a different meaning. 4.3. Provenance: I have an additional items to be added to provenance, and an extension of 4.3.5. Resources Here are some possible text to be added: In 4.3.5:Resources: Additionally to the technical details in the computation, Resources would include the list of steps and hyperlinks needed to recover the simulation in a VO environment if possible, in such a way that, in the case that the model would be: a) Directly recovered in the case that it constitute a final result b) Directly computed and used as an intermediate step for further developments. Such a object in the data model would allow the intrinsic pipe-line characteristic of some theoretical models. As an example, a stellar library (that can be obtained by a VOtool by a selection of stellar spectrum either observational and/or theoretical), which would be a final product by itself, would be used by a synthesis model to obtain the SED of a galaxy. In that case it is not needed to obtain first the whole library, but to know "how to obtain some elements" in the library and what is the parameter space (log g, Teff, metallicity and so on) covered by the library. 4.5.7.: Credits and Executive Summary? It is worth to note that no lost of the corresponding credits will occur. In opposite to observational data, managed by institutions, most of theoretical model are managed and developed by small groups, and sometimes by individual persons (examples would be the extensive use of Kurucz atmosphere models or the photoionization code Cloudy, by G. Ferland, by the community). If the data model is not able to recover the corresponding credits, it would produce that some groups will not join the theoretical VO iniciative, since they would considered that their work will receive no credit. From a metadata perspective it would be required some additional text fieds that sumarize in a univocally way the model by its ingredients, and the cautions for its use. It would be quite useful (from a final-user point of view) if such fields are writen in a "latex-ready" format including bibitem references and the corresponding fields with the \bibitem references in ADS/CDS format, in such a way that it can be used by "cut and paste" the corresponding fileds of the VOTable. Well, sorry for this long e-mail. I hope that it would be useful Miguel El 24/05/2005, a las 9:09, Laurie Shaw escribió: > > Hi everyone, > > I've now added the latest draft of the simulation data model to the > IVOA > theory twiki page [Simulation.v.0.2.doc]. Comments and feedback would > be > great! > > Thanks, > > Laurie > > From owner-theory@eso.org Mon May 30 14:19:03 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 j4UCIj4L028430 for ; Mon, 30 May 2005 14:18:46 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j4UCIjod028429 for theory-outgoing; Mon, 30 May 2005 14:18:45 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 j4UCIc4L028408 for ; Mon, 30 May 2005 14:18:38 +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 j4UCIaXW014596 for ; Mon, 30 May 2005 14:18:36 +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 OAA18738; Mon, 30 May 2005 14:18:30 +0200 (MET DST) In-Reply-To: <20050530115049.2qoe5rsg22gwko4k@webmail.sic.rm.cnr.it> References: <20050530115049.2qoe5rsg22gwko4k@webmail.sic.rm.cnr.it> Mime-Version: 1.0 (Apple Message framework v622) Content-Type: text/plain; charset=ISO-8859-1; delsp=yes; format=flowed Message-Id: <02bc559471c6e5e4758480419eb1384d@iaa.es> Cc: theory@ivoa.net, =?ISO-8859-1?Q?Miguel_Cervi=F1o?= From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Re: Sci-Board-1 Date: Mon, 30 May 2005 14:18:52 +0200 To: Andrea Preite Martinez X-Mailer: Apple Mail (2.622) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.5.30.8 X-Virus-Scanned: by amavisd-new Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id j4UCIj4L028423 Sender: owner-theory@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= X-Mozilla-Status: 8011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Dear Andrea I can try to help in the UCD-vocabulary for theory/simulations. May be others in the theory group would be also interested, there was some discussion in the list about the subject of UCDs... (I just made a carbon copy to the theory group of this mail and your anterior e-mail) If there is no more voluntieers, I can try to coordinate it, Cheers Miguel (mcs@iaa.es IAA; SVO) > 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 > ======================================================================= > ======= > From owner-theory@eso.org Wed Jun 8 10:31:13 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 j588V3kX029107 for ; Wed, 8 Jun 2005 10:31:03 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j588V3rZ029106 for theory-outgoing; Wed, 8 Jun 2005 10:31:03 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 j588UxkX029100 for ; Wed, 8 Jun 2005 10:30:59 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j588UvXW006032 for ; Wed, 8 Jun 2005 10:30:58 +0200 (CEST) Received: from gavopc1 (gavopc1.xray.mpe.mpg.de [130.183.72.204]) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with SMTP id KAA08276 for ; Wed, 8 Jun 2005 10:30:52 +0200 (METDST) From: "Gerard Lemson" To: Subject: plans from Kyoto meeting Date: Wed, 8 Jun 2005 10:34:29 +0200 Message-ID: MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook IMO, Build 9.0.6604 (9.0.2911.0) Importance: Normal X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1441 X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.1, Antispam-Data: 2005.6.8.1 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: theory@ivoa.net X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Dear Collegues During the session of the theory interest group in the Kyoto interop meeting it was decided that several groups would write up scientific use cases for the theory-VO like activities they have so far been involved in. The use cases should pay particular attention to those areas where IVOA standards and implementations can or should be used, giving opinions on whether existing products suffice, or detailing discrepancies. >From these use cases we will extract requirements on the various IVOA working group activities, to see whether existing results can be used in current or slightly modified form, or whether new activities are necessary. The goal is to discuss these requirements at the next interop meeting in Spain in October. It was decided that 4 different areas would be investigated: large scale cosomological simulations, medium scale (galaxy merger, jets) ones, theory spectra and atomic and molecular scale. The following groups/individuals volunteered to write use cases: - Large scale: Laurie Shaw; Gerard Lemson - Medium scale: Dave De Young, who will try to get contributions from Peter Teuben/Piet Hut - theory spectra: Enrique Solano and Pedro Osuna; JHU/HVO - atomic scales: Marie Lise Dubernet I propose the following time scales for this work, based on the goal that by the next interop we have a first Working Draft with requirements: - "Note" from each groups with use cases by mid August. This gives 2 months. - Start of writing of requirements "Working Draft" (a group effort) by beginning of September. - Version 0.1 of WD ready by next interop for discussion in theory session and in relevant working groups. >From the volunteers I would like to get comments on whether the proposed schedule seems doable and adequate. Everyone else please mail your comments to the theory mailing list which c/should also be used for discussions about the contents of notes once they are put forward to the theory TWiki page. Thanks Gerard -- * Gerard Lemson * Tel: +49 (0)89 30000-3316 * * MPI fuer extraterrestische Physik * Fax: +49 (0)89 30000-3569 * * Giessenbachstrasse * * * Postfach 1312 * * * D-85741 Garching, GERMANY * email: gerard.lemson@mpe.mpg.de * From owner-theory@eso.org Wed Sep 21 10:54:49 2005 Return-Path: Received: from mercury.hq.eso.org (localhost [127.0.0.1]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j8L8sZ91017586 for ; Wed, 21 Sep 2005 10:54:35 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j8L8sZUF017585 for theory-outgoing; Wed, 21 Sep 2005 10:54:35 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 j8L8sT91017515 for ; Wed, 21 Sep 2005 10:54:29 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j8L8sSin011735 for ; Wed, 21 Sep 2005 10:54:28 +0200 (CEST) Received: from gavopc1 (gavopc1.xray.mpe.mpg.de [130.183.72.204]) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with SMTP id KAA10321; Wed, 21 Sep 2005 10:54:19 +0200 (METDST) From: "Gerard Lemson" To: Cc: , , , , , "Tamas Budavari" , "Gerard Lemson" Subject: theory session Date: Wed, 21 Sep 2005 10:59:58 +0200 Message-ID: MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook IMO, Build 9.0.6604 (9.0.2911.0) X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1506 Importance: Normal X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.0.3.2, Antispam-Data: 2005.9.21.2 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: theory@ivoa.net X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Dear collegues During the interop mneeting in Madrid there wil be 1 2-hour session of the theory interest group, on Thursday afternoon, 16:45-18:30. The subject of this was basically defined at the end of the last meeting. We'll be discussing use cases defined by some of us and try to match these to the efforts of the IVOA working groups to define requirements for them. To have something to talk about I urge those who volunteered to write up such use cases, to put the results of this on the theory TWiki pages. To this end I have created an index page at http://www.ivoa.net/twiki/bin/viewauth/IVOA/IvoaTheoryUseCases where you can add the title of your use case and link it to a page where you describe it in more detail. The format of the use case is not prescribed (so far). I have as an example started writing up one of my use cases following the AstroGrid format, but feel free to use your own. I would also hope that these same volunteers can introduce the use cases during the session. Please you let me know whether this is possible, or, if not, whether you will be able to produce the use case. If others wish to make contributions, please let me know as it may well be that there is time available. Thanks and hope to see you in Madrid. Regards Gerard -- * Gerard Lemson * Tel: +49 (0)89 30000-3316 * * MPI fuer extraterrestische Physik * Fax: +49 (0)89 30000-3569 * * Giessenbachstrasse * * * Postfach 1312 * * * D-85741 Garching, GERMANY * email: gerard.lemson@mpe.mpg.de * From owner-theory@eso.org Wed Oct 5 12:48:41 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 j95Am89S000836 for ; Wed, 5 Oct 2005 12:48:08 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id j95Am8qY000835 for theory-outgoing; Wed, 5 Oct 2005 12:48:08 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 j95Am39S000824 for ; Wed, 5 Oct 2005 12:48:04 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id j95Am2in016810 for ; Wed, 5 Oct 2005 12:48:02 +0200 (CEST) Received: from localhost (glemson@localhost) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with ESMTP id MAA13207 for ; Wed, 5 Oct 2005 12:47:56 +0200 (METDST) X-Authentication-Warning: mpehp1.mpe-garching.mpg.de: glemson owned process doing -bs Date: Wed, 5 Oct 2005 12:47:56 +0200 (METDST) From: Gerard Lemson X-Sender: glemson@mpehp1.mpe-garching.mpg.de To: theory@ivoa.net Subject: theory session at interop Madrid 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: 2005.10.5.6 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: theory@ivoa.net X-Mozilla-Status: 8001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: Dear Collegues A propsed outline for tomorrow's theory interest group session has been posted on the interop meetings twiki page at http://ivoa.net/twiki/bin/view/IVOA/InterOpOct2005Theory It will be updated later today. If you have any comments please let me know Cheers Gerard Lemson From owner-theory@eso.org Fri Dec 23 10:36:22 2005 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 jBN9a5gF020333 for ; Fri, 23 Dec 2005 10:36:06 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id jBN9a5wt020332 for theory-outgoing; Fri, 23 Dec 2005 10:36:05 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 jBN9a0gF020313; Fri, 23 Dec 2005 10:36:00 +0100 (MET) Received: from ppsw-0.csi.cam.ac.uk (ppsw-0.csi.cam.ac.uk [131.111.8.130]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id jBN9ZwA1017415; Fri, 23 Dec 2005 10:35:58 +0100 (CET) X-Cam-SpamDetails: Not scanned X-Cam-AntiVirus: No virus found X-Cam-ScannerInfo: http://www.cam.ac.uk/cs/email/scanner/ Received: from cass41.ast.cam.ac.uk ([131.111.69.186]:54286) by ppsw-0.csi.cam.ac.uk (ppsw.cam.ac.uk [131.111.8.130]:25) with esmtp id 1EpjKz-0003X4-01 (Exim 4.54) (return-path ); Fri, 23 Dec 2005 09:35:45 +0000 Received: from cass54.ast.cam.ac.uk (cass54 [IPv6:2001:630:200:4240:203:baff:fed8:66d9]) by cass41.ast.cam.ac.uk (8.13.4+Sun/8.13.4) with ESMTP id jBN9ZekI010449; Fri, 23 Dec 2005 09:35:40 GMT Received: from cass54.ast.cam.ac.uk (localhost [127.0.0.1]) by cass54.ast.cam.ac.uk (8.13.4+Sun/8.13.3) with ESMTP id jBN9ZeMg016880; Fri, 23 Dec 2005 09:35:40 GMT Received: from localhost (naw@localhost) by cass54.ast.cam.ac.uk (8.13.4+Sun/8.13.3/Submit) with ESMTP id jBN9ZdPG016877; Fri, 23 Dec 2005 09:35:39 GMT X-Authentication-Warning: cass54.ast.cam.ac.uk: naw owned process doing -bs Date: Fri, 23 Dec 2005 09:35:39 +0000 (GMT) From: Nicholas Walton X-X-Sender: naw@cass54 To: theory@ivoa.net, ivoa@ivoa.net, teuben@astro.umd.edu, blaizot@MPA-Garching.MPG.DE, J.C.Helly@dur.ac.uk, tom.theuns@durham.ac.uk cc: Nicholas Walton , Laurie Shaw , Gerard Lemson Subject: IVOA Theory-Interest Group: Particle Simulations Workshop: Cambridge, UK: 27-28 Feb 2006 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: 2005.12.23.1 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: theory@ivoa.net Dear All, We would like to invite you to participate in a two-day workshop on the 27th-28th February, 2006, at the Institute of Astronomy, Cambridge University, aimed at discussing and proposing solutions to the main issues regarding the successful integration of simulated data into the Virtual Observatory. Specifically, as discussed at the ESAC Oct 2005 Interoperability meeting theory session, the focus of this workshop will be on the requirements of data extracted from 'particle' (Nbody, SPH) simulations. The workshop will aim to address the following specific topics: * proposing and determining a standard data format and file structure for simulated data * development of meta-data models for discovery and querying of published data * identifying the main requirements of simulated data on the other IVOA working groups, especially with regard to data discovery, querying, and retrieval, and the registration of selected data products and services. * identifying the type of services to be made available for the analysis/visualisation of simulated data (e.g. virtual telescopes, online semi-analytical galaxy formation) >From the outcome of this workshop, we hope to enable the publication of simulated data using a standard prototype data format, the success of which can be discussed at the IVOA InterOperability meeting in Victoria in May 2006 (http://www.ivoa.net/twiki/bin/view/IVOA/InterOpMay2006). We also aim to be able to present a list of requirements of the IVOA working groups, based on a selection of theory 'use-cases'. Details of logistics and registration for the workshop can be found at http://ag01.ast.cam.ac.uk:8080/twiki/bin/view/Community/TheoryMeetFeb06 We hope very much to see you in Cambridge in February 2006. Yours, and best wishes for Xmas and the New Year, Nic Walton, Laurie Shaw and Gerard Lemson. ======================================================================== Dr N. A. Walton (AstroGrid Project Scientist http://www.astrogrid.org) (Euro-VO VOTC Project Scientist http://www.euro-vo.org) Institute of Astronomy Tel: +44 1223 337503 University of Cambridge Fax: +44 1223 337523 Madingley Road WWW: http://www.ast.cam.ac.uk/~naw Cambridge, CB3 0HA email: naw@ast.cam.ac.uk ======================================================================== From owner-ivoa@eso.org Fri Dec 23 10:36:36 2005 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 jBN9aHgF020362 for ; Fri, 23 Dec 2005 10:36:18 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id jBN9aHTK020361 for ivoa-outgoing; Fri, 23 Dec 2005 10:36:17 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ivoa@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 jBN9a0gF020313; Fri, 23 Dec 2005 10:36:00 +0100 (MET) Received: from ppsw-0.csi.cam.ac.uk (ppsw-0.csi.cam.ac.uk [131.111.8.130]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id jBN9ZwA1017415; Fri, 23 Dec 2005 10:35:58 +0100 (CET) X-Cam-SpamDetails: Not scanned X-Cam-AntiVirus: No virus found X-Cam-ScannerInfo: http://www.cam.ac.uk/cs/email/scanner/ Received: from cass41.ast.cam.ac.uk ([131.111.69.186]:54286) by ppsw-0.csi.cam.ac.uk (ppsw.cam.ac.uk [131.111.8.130]:25) with esmtp id 1EpjKz-0003X4-01 (Exim 4.54) (return-path ); Fri, 23 Dec 2005 09:35:45 +0000 Received: from cass54.ast.cam.ac.uk (cass54 [IPv6:2001:630:200:4240:203:baff:fed8:66d9]) by cass41.ast.cam.ac.uk (8.13.4+Sun/8.13.4) with ESMTP id jBN9ZekI010449; Fri, 23 Dec 2005 09:35:40 GMT Received: from cass54.ast.cam.ac.uk (localhost [127.0.0.1]) by cass54.ast.cam.ac.uk (8.13.4+Sun/8.13.3) with ESMTP id jBN9ZeMg016880; Fri, 23 Dec 2005 09:35:40 GMT Received: from localhost (naw@localhost) by cass54.ast.cam.ac.uk (8.13.4+Sun/8.13.3/Submit) with ESMTP id jBN9ZdPG016877; Fri, 23 Dec 2005 09:35:39 GMT X-Authentication-Warning: cass54.ast.cam.ac.uk: naw owned process doing -bs Date: Fri, 23 Dec 2005 09:35:39 +0000 (GMT) From: Nicholas Walton X-X-Sender: naw@cass54 To: theory@ivoa.net, ivoa@ivoa.net, teuben@astro.umd.edu, blaizot@MPA-Garching.MPG.DE, J.C.Helly@dur.ac.uk, tom.theuns@durham.ac.uk cc: Nicholas Walton , Laurie Shaw , Gerard Lemson Subject: IVOA Theory-Interest Group: Particle Simulations Workshop: Cambridge, UK: 27-28 Feb 2006 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: 2005.12.23.1 X-Virus-Scanned: by amavisd-new Sender: owner-ivoa@eso.org Precedence: bulk Reply-To: ivoa@ivoa.net Dear All, We would like to invite you to participate in a two-day workshop on the 27th-28th February, 2006, at the Institute of Astronomy, Cambridge University, aimed at discussing and proposing solutions to the main issues regarding the successful integration of simulated data into the Virtual Observatory. Specifically, as discussed at the ESAC Oct 2005 Interoperability meeting theory session, the focus of this workshop will be on the requirements of data extracted from 'particle' (Nbody, SPH) simulations. The workshop will aim to address the following specific topics: * proposing and determining a standard data format and file structure for simulated data * development of meta-data models for discovery and querying of published data * identifying the main requirements of simulated data on the other IVOA working groups, especially with regard to data discovery, querying, and retrieval, and the registration of selected data products and services. * identifying the type of services to be made available for the analysis/visualisation of simulated data (e.g. virtual telescopes, online semi-analytical galaxy formation) >From the outcome of this workshop, we hope to enable the publication of simulated data using a standard prototype data format, the success of which can be discussed at the IVOA InterOperability meeting in Victoria in May 2006 (http://www.ivoa.net/twiki/bin/view/IVOA/InterOpMay2006). We also aim to be able to present a list of requirements of the IVOA working groups, based on a selection of theory 'use-cases'. Details of logistics and registration for the workshop can be found at http://ag01.ast.cam.ac.uk:8080/twiki/bin/view/Community/TheoryMeetFeb06 We hope very much to see you in Cambridge in February 2006. Yours, and best wishes for Xmas and the New Year, Nic Walton, Laurie Shaw and Gerard Lemson. ======================================================================== Dr N. A. Walton (AstroGrid Project Scientist http://www.astrogrid.org) (Euro-VO VOTC Project Scientist http://www.euro-vo.org) Institute of Astronomy Tel: +44 1223 337503 University of Cambridge Fax: +44 1223 337523 Madingley Road WWW: http://www.ast.cam.ac.uk/~naw Cambridge, CB3 0HA email: naw@ast.cam.ac.uk ======================================================================== From owner-theory@eso.org Tue Jan 3 11:05:38 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k03A5OK4028785 for ; Tue, 3 Jan 2006 11:05:24 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k03A5OUv028784 for theory-outgoing; Tue, 3 Jan 2006 11:05:24 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k03A51K4028727 for ; Tue, 3 Jan 2006 11:05:02 +0100 (MET) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k03A501r011921 for ; Tue, 3 Jan 2006 11:05:00 +0100 (CET) Received: from gavopc1 (gavopc1.xray.mpe.mpg.de [130.183.72.204]) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with SMTP id LAA02058; Tue, 3 Jan 2006 11:03:18 +0100 (MET) From: "Gerard Lemson" To: "Dave DeYoung" , "Enrique Solana" , "Franck LePetit" , "Gerard Lemson" , "Laurie Shaw" , "Pedro Osuna" , "Tamas Budavari" Cc: , "Gerard Lemson" , "Dave De Young" , "Dr. Kokubo" , "Dr. Matumoto" , =?iso-8859-1?Q?Herv=E9_Wozniak_?= , "Jongsoo Kim" , =?iso-8859-1?Q?Miguel_Cervi=F1o?= , "Nicholas Walton" , "Sarah Maddison " , "Ugo Becciani " Subject: use cases Date: Tue, 3 Jan 2006 11:05:03 +0100 Message-ID: MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook IMO, Build 9.0.6604 (9.0.2911.0) X-MIMEOLE: Produced By Microsoft MimeOLE V6.00.2800.1506 Importance: Normal X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2006.1.3.1 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: theory@ivoa.net Dear Collegues First a happy new year to all of you. By the end of this month I would like to start the process of extracting requirements from the theory use cases. As you may have gathered from the email sent out by Nic Walton and Laurie Shaw, for the particular case of N-body simulation results we will do part of that work during a workshop in Cambridge, UK (see http://ag01.ast.cam.ac.uk:8080/twiki/bin/view/Community/TheoryMeetFeb06). For the other use cases this will (at first) be done via the mailing list. I hope that those of you who already contributed to the process will have the opportunity to update the existing use cases on the theory Wiki page so that they contain explicit descriptions of the VO components required for their execution as agreed at the ESAC meeting. I would also like to invite everyone to add others. Thanks, Gerard -- * Gerard Lemson * Tel: +49 (0)89 30000-3316 * * MPI fuer extraterrestische Physik * Fax: +49 (0)89 30000-3569 * * Giessenbachstrasse * * * Postfach 1312 * * * D-85741 Garching, GERMANY * email: gerard.lemson@mpe.mpg.de * From owner-theory@eso.org Thu Feb 23 04:46:59 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k1N3kiaR002715 for ; Thu, 23 Feb 2006 04:46:44 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k1N3kiNq002713 for theory-outgoing; Thu, 23 Feb 2006 04:46:44 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k1N3kcaR002706 for ; Thu, 23 Feb 2006 04:46:38 +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 k1N3kZkD025082 for ; Thu, 23 Feb 2006 04:46:36 +0100 (CET) X-Spam-Checker-Version: SpamAssassin 3.1.0 (2005-09-13) on noao.edu X-Spam-Level: X-Spam-Status: No, score=-137.4 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 orion.tuc.noao.edu ([140.252.1.22] verified) by noao.edu (CommuniGate Pro SMTP 5.0.6) with ESMTP id 23971804; Wed, 22 Feb 2006 20:46:26 -0700 Received: (from deyoung@localhost) by orion.tuc.noao.edu (8.11.6p2-20030918/8.11.3/SAG-04Apr12) id k1N3kOW23049; Wed, 22 Feb 2006 20:46:24 -0700 (MST) Date: Wed, 22 Feb 2006 20:46:24 -0700 (MST) From: Dave De Young Message-Id: <200602230346.k1N3kOW23049@orion.tuc.noao.edu> To: glemson@xray.mpe.mpg.de, naw@ast.cam.ac.uk Subject: IVOA Theory IG Meeting Cc: hanisch@stci.edu, teuben@astro.umd.edu, theory@ivoa.net X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.1.0.0, Antispam-Data: 2006.02.22.184606 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: Dave De Young Dear Nic, Gerard, et al. I am sorry that I will be unable to attend the forthcoming Theory IG meeting next week; it sounds like a very important meeting. However, I did have a discussion with Bob Hanisch at our NVO Advisory Committee meeting last week about "next steps" for the Theory IG as seen from the IVOA "Process". It seems that the topics described for next week's meeting are very much on track for moving the Theory IG into the areas of interest covered by other IVOA working groups and eventually for the Theory IG to become a Theory Working Group. Once the topics to be discussed at Cambridge are reasonably well defined, the next step seems to be an informal "note" to the IVOA Exec that characterises the major problems, outlines the initial definitions of the metadata required, and describes the next steps to be taken. A clear area of interest is the use of large scale simulations by observers, and hence a description of what would be needed to make such simulations accessible to observers, including the basic metadata, would be very relevant. Some simulations have made a lot of progress in this area, while others have done very little, as all of you know. Also of interest are some descriptions of the interaction with, and requirements from, other IVOA working groups such as DAL, Registry, etc. I notice that the Workshop announcement specifically describes large scale cosmological simulations as an area of emphasis. These calculations are very complex, often with many assumptions (e.g., "feedback"), and they can be very high profile (e.g., Millennium). But I urge the workshop to also include the problems involved in other classes of complex simulations that are used by a large fraction of the community. These have been discussed before at our meetings, and they include areas such as radiation transfer, binary systems evolution including general relativity, relativistic hydrodynamics, and 3D MHD simulations with turbulence and radiation. I suspect the metadata issues for these classes of simulations may be very different that those for the cosmology or purely N body calculations. Again, my apologies for being unable to attend. If at the end of the workshop there are issues that need further development, particularly in the area of MHD and hydrodynamic simulations, I would be happy to assist. Please let me know. Best wishes for a successful meeting. Dave From owner-theory@eso.org Tue Feb 28 16:19:39 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k1SFJ7mF017346 for ; Tue, 28 Feb 2006 16:19:07 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k1SFJ6Nw017345 for theory-outgoing; Tue, 28 Feb 2006 16:19:06 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k1SFIjmF017237 for ; Tue, 28 Feb 2006 16:18:46 +0100 (MET) Received: from ppsw-9.csi.cam.ac.uk (ppsw-9.csi.cam.ac.uk [131.111.8.139]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k1SFIh22005814 for ; Tue, 28 Feb 2006 16:18:44 +0100 (CET) X-Cam-SpamDetails: Not scanned X-Cam-AntiVirus: No virus found X-Cam-ScannerInfo: http://www.cam.ac.uk/cs/email/scanner/ Received: from cass41.ast.cam.ac.uk ([131.111.69.186]:42081) by ppsw-9.csi.cam.ac.uk (ppsw.cam.ac.uk [131.111.8.139]:25) with esmtp id 1FE6cK-0008AH-Um (Exim 4.54) (return-path ); Tue, 28 Feb 2006 15:18:24 +0000 Received: from cass54.ast.cam.ac.uk (cass54 [IPv6:2001:630:200:4240:203:baff:fed8:66d9]) by cass41.ast.cam.ac.uk (8.13.4+Sun/8.13.4) with ESMTP id k1SFILaJ014116; Tue, 28 Feb 2006 15:18:21 GMT Received: from cass54.ast.cam.ac.uk (localhost [127.0.0.1]) by cass54.ast.cam.ac.uk (8.13.4+Sun/8.13.3) with ESMTP id k1SFHvEn009045; Tue, 28 Feb 2006 15:17:57 GMT Received: from localhost (naw@localhost) by cass54.ast.cam.ac.uk (8.13.4+Sun/8.13.3/Submit) with ESMTP id k1SFHufY009042; Tue, 28 Feb 2006 15:17:56 GMT X-Authentication-Warning: cass54.ast.cam.ac.uk: naw owned process doing -bs Date: Tue, 28 Feb 2006 15:17:56 +0000 (GMT) From: Nicholas Walton X-X-Sender: naw@cass54 To: Dave De Young cc: glemson@xray.mpe.mpg.de, hanisch@stci.edu, teuben@astro.umd.edu, theory@ivoa.net, Nicholas Walton , j.c.helly@durham.ac.uk, c.gheller@cineca.it Subject: Re: IVOA Theory IG Meeting In-Reply-To: <200602230346.k1N3kOW23049@orion.tuc.noao.edu> Message-ID: References: <200602230346.k1N3kOW23049@orion.tuc.noao.edu> 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: 2006.02.28.062606 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: Nicholas Walton hi dave we did indeed look at the issue of moving to a Theory-WG and a proposal will be generating a position note on this at the May interop. focus of that would be work on SNAP - simple numerical access protocol. i'll be circulating a fuller summary of key outcomes of the meeting early next week. in the mean time - please take a look at the meeting wiki page at http://www.ivoa.net/twiki/bin/view/IVOA/CambridgeTheoryWorkshopFeb06 cheers, nic ======================================================================== Dr N. A. Walton (AstroGrid Project Scientist http://www.astrogrid.org) (Euro-VO VOTC Project Scientist http://www.euro-vo.org) Institute of Astronomy Tel: +44 1223 337503 University of Cambridge Fax: +44 1223 337523 Madingley Road WWW: http://www.ast.cam.ac.uk/~naw Cambridge, CB3 0HA email: naw@ast.cam.ac.uk ======================================================================== On Wed, 22 Feb 2006, Dave De Young wrote: > > Dear Nic, Gerard, et al. > > I am sorry that I will be unable to attend the forthcoming Theory > IG meeting next week; it sounds like a very important meeting. > However, I did have a discussion with Bob Hanisch at our NVO > Advisory Committee meeting last week about "next steps" for the > Theory IG as seen from the IVOA "Process". It seems that the topics > described for next week's meeting are very much on track for moving > the Theory IG into the areas of interest covered by other IVOA > working groups and eventually for the Theory IG to become a Theory > Working Group. Once the topics to be discussed at Cambridge are > reasonably well defined, the next step seems to be an informal > "note" to the IVOA Exec that characterises the major problems, > outlines the initial definitions of the metadata required, and > describes the next steps to be taken. A clear area of interest is > the use of large scale simulations by observers, and hence a > description of what would be needed to make such simulations > accessible to observers, including the basic metadata, would be > very relevant. Some simulations have made a lot of progress in > this area, while others have done very little, as all of you know. > Also of interest are some descriptions of the interaction with, > and requirements from, other IVOA working groups such as DAL, > Registry, etc. > > I notice that the Workshop announcement specifically describes > large scale cosmological simulations as an area of emphasis. These > calculations are very complex, often with many assumptions (e.g., > "feedback"), and they can be very high profile (e.g., Millennium). > But I urge the workshop to also include the problems involved in > other classes of complex simulations that are used by a large > fraction of the community. These have been discussed before at > our meetings, and they include areas such as radiation transfer, > binary systems evolution including general relativity, relativistic > hydrodynamics, and 3D MHD simulations with turbulence and radiation. > I suspect the metadata issues for these classes of simulations may > be very different that those for the cosmology or purely N body > calculations. > > Again, my apologies for being unable to attend. If at the end of > the workshop there are issues that need further development, > particularly in the area of MHD and hydrodynamic simulations, I > would be happy to assist. Please let me know. > > Best wishes for a successful meeting. > > Dave > > > From owner-theory@eso.org Fri Apr 14 23:49:50 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k3ELnMP6008296 for ; Fri, 14 Apr 2006 23:49:22 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k3ELnMpg008295 for theory-outgoing; Fri, 14 Apr 2006 23:49:22 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k3ELnCP6008286; Fri, 14 Apr 2006 23:49:12 +0200 (MEST) Received: from ppsw-7.csi.cam.ac.uk (ppsw-7.csi.cam.ac.uk [131.111.8.137]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k3ELn9k5001979; Fri, 14 Apr 2006 23:49:09 +0200 (CEST) X-Cam-SpamDetails: Not scanned X-Cam-AntiVirus: No virus found X-Cam-ScannerInfo: http://www.cam.ac.uk/cs/email/scanner/ Received: from cass41.ast.cam.ac.uk ([131.111.69.186]:41641) by ppsw-7.csi.cam.ac.uk (ppsw.cam.ac.uk [131.111.8.137]:25) with esmtp id 1FUWA0-0004AM-OE (Exim 4.54) (return-path ); Fri, 14 Apr 2006 22:49:00 +0100 Received: from cass25.ast.cam.ac.uk (cass25 [IPv6:2001:630:200:4240:203:baff:fe24:314]) by cass41.ast.cam.ac.uk (8.13.6+Sun/8.13.6) with ESMTP id k3ELmuHu013196; Fri, 14 Apr 2006 22:48:56 +0100 (BST) Received: from cass25.ast.cam.ac.uk (localhost [127.0.0.1]) by cass25.ast.cam.ac.uk (8.13.6+Sun/8.13.6) with ESMTP id k3ELmurs007140; Fri, 14 Apr 2006 22:48:56 +0100 (BST) Received: from localhost (lds@localhost) by cass25.ast.cam.ac.uk (8.13.6+Sun/8.13.6/Submit) with ESMTP id k3ELmtOm007137; Fri, 14 Apr 2006 22:48:55 +0100 (BST) X-Authentication-Warning: cass25.ast.cam.ac.uk: lds owned process doing -bs Date: Fri, 14 Apr 2006 22:48:55 +0100 (BST) From: Laurie Shaw X-X-Sender: lds@cass25 To: Gerard Lemson , Nicholas Walton , Laurie Shaw cc: ucd@ivoa.net, theory@ivoa.net Subject: UCD's for simulations In-Reply-To: Message-ID: References: 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: 2.3.0.1, Antispam-Data: 2006.04.13.165108 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: Laurie Shaw Dear All, I've recently been experimenting with assigning UCDs to the results of some cosmological simulations -- specifically to catalogues of dark matter halos and their associated subhalos. In general, i've found that the existing UCD tree is able to describe most of the properties of these objects that are typically analysed in the literature, albeit with a few exceptions. However, it is not currently possible to describe the properties and parameters of the simulations themselves. This includes some input physical parameters (i.e. cosmological parameters) that define the theoretical context of the simulation, and technical parameters that define its size,scope and resolution (e.g number of particles, length of simulation box side, gravitational softening length, time/redshift of a simulation output). Therefore, for the latter, I propose a new branch of the UCD tree to encompass computatational techniques in astronomy: 'comp'. This branch can be used to describe both astrophysical (and cosmological) simulations, and data reduction and post-processing algorithms for both simulation and observational data. It is roughly a computing analogue of the 'instr' branch. For the case of simulations I propose the following sub-branches comp.sim (computational simulation) comp.sim.nbody (Nbody simulation) comp.sim.sph (Smoothed Particle Hydrodynamics simulation) comp.sim.boxside (Simulation box) comp.sim.gravsoft (gravitational softening) comp.sim.particles (simulation particles (for Nbody and SPH simulations)) comp.sim.snapshot (output of a simulation box at a particular instant) comp.sim.grid (simulation grid (for hydro simulations)) The number of particles in the simulation box, number of grid points, particle mass, gravitational softening length and simulation box side length would therefore be: meta.num;comp.sim.particles meta.num;comp.sim.grid phys.mass;comp.sim.particles phys.size;comp.sim.gravsoft phys.size;comp.sim.boxside (For the last two, introduction of a phys.size.length UCD might provide a more accurate description.) The mass of an object in terms of the number of particles it contains: phys.mass;meta.num;comp.sim.particles Other possible sub-branches could be comp.resourse (computational resources used in simulation/data processing) comp.resource.processors (processors used) comp.resource.memory (total size of a data file) plus those that are more specific to data-reduction/post-processing of observational data. Algorithms that might apply to both simulated and observed data (e.g. smoothing of images or particle densities) would be listed directly under the comp branch: phys.size;comp.smooth (or, with the introduction of a phys.size.length UCD: phys.size.length;comp.smooth) Physical Parameters --------------------- Currently, there exists no UCDs for the main cosmological parameters. In terms of simulations, it is very important to be able define the assumed cosmology, when interpreting the results. To describe these parameters I propose a 'cosmology' sub-branch of the phys branch. So, phys.cosmology (cosmology) phys.cosmology.omega (matter/energy density of universe) phys.cosmology.hubble (hubble constant) phys.cosmology.sigma8 (Normalisation of matter power-spectrum) and also: phys.matter.dark (dark matter tag) phys.matter.baryon (baryonic matter tag) phys.DarkEnergy (dark energy tag) So, Omega_Lambda, Omega_DM, Omega_baryon would be phys.cosmology.omega;phys.DarkEnery, phys.cosmology.omega;phys.matter.dark phys.comsology.omega;phys.matter.baryonic Now we can also describe the number of dark matter (gas particles) in an SPH simulation, or a simulated object (star/galaxy/halo) using: meta.num;comp.sim.particles;phys.matter.dark(/baryonic) Furthermore, the mass and radius of dark matter halos in cosmological simulations are frequently defined in terms of a virial overdensity. Hence a phys.virial UCD would be usefull in specifying what is meant by the mass and radius of a halo: phys.mass;phys.virial (virial mass) phys.size.radius;phys.virial (virial radius) Time in Simulations ------------------ People frequently analyse the output of simulations, or snapshots, at a series of different timesteps. This is often quoted in terms of the redshift of the snapshot. At the moment, redshift exists under the 'src' branch. Maybe it might be better under the `phys' branch as it is a measure of both distance and time, and can therefore be used to label both the distance of observed objects and to label a time-stamp for simulation snapshots: phys.redshift;comp.sim.snapshot Astrophysical Objects -------------------- Another problem is the listing of astronomical objects types under the 'src' branch. This introduces confusion when trying to describe a simulated astrophysical object. For example, the first word in src.class.galaxy;comp.sim (simulated galaxy) implies that this is an observed astrophysical source, the second that it is simulated. Additionally, objects such as halos and subhalos are not typically observed (though i guess people do make estimates of their mass/size through gravitational lensing). It seems strange to have halo and subhalo listed under the src.class sub-branch. I therefore suggest that an object branch be introduced in which astrophysical (and theoretical) objects can be listed (as also proposed by others on the UCD suggestion page): object.galaxy;comp.sim (a simulated galaxy) object.galaxy.spiral;comp.sim (a simulated spiral galaxy) One example that I encountered of an actual quantity where this was useful is describing the mass in substructure, or the number of subhalos, in a simulated halo: phys.mass;object.DMhalo.subhalo meta.num;onject.DMhalo.subhalo It would be great to hear everyones thoughts, or ideas for alternative approaches, for all these. Cheers, Laurie List of Proposed UCDs --------------------- comp (computational astronomy) comp.sim (simulations) comp.sim.nbody (Nbody simulation) comp.sim.sph (Smoothed Particle Hydrodynamics simulation) comp.sim.boxside (Simulation box) comp.sim.gravsoft (gravitational softening) comp.sim.particles (simulation particles (for Nbody and SPH simulations)) comp.sim.snapshot (output of a simulation box at a particular instant) comp.sim.grid (simulation grid (for hydro simulations)) comp.resourse (to describe computational resources used in simulation/data processing) comp.resource.processors (processors used) comp.resource.memory (total size on disk of data) (comp.dataReduct ? comp.algorithm (general algorithms applied to sim/obs data) ) phys.cosmology phys.cosmology.omega (matter/energy density of universe) phys.cosmology.hubble (hubble constant) phys.cosmology.sigma8 (Normalisation of matter power-spectrum) phys.matter.dark (dark matter tag) phys.matter.baryon (baryonic matter tag) phys.DarkEnergy (dark energy tag) phys.virial phys.size.length object (astophysical object) object.planet (planet) object.satellite object.star (star) object.galaxy (galaxy) object.DMhalo (DM halo) Object.DMhalo.subhalo (DM subhalo) etc From owner-ucd@eso.org Fri Apr 14 23:49:54 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k3ELnHP6008291 for ; Fri, 14 Apr 2006 23:49:17 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k3ELnHJ2008290 for ucd-outgoing; Fri, 14 Apr 2006 23:49:17 +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 k3ELnCP6008286; Fri, 14 Apr 2006 23:49:12 +0200 (MEST) Received: from ppsw-7.csi.cam.ac.uk (ppsw-7.csi.cam.ac.uk [131.111.8.137]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k3ELn9k5001979; Fri, 14 Apr 2006 23:49:09 +0200 (CEST) X-Cam-SpamDetails: Not scanned X-Cam-AntiVirus: No virus found X-Cam-ScannerInfo: http://www.cam.ac.uk/cs/email/scanner/ Received: from cass41.ast.cam.ac.uk ([131.111.69.186]:41641) by ppsw-7.csi.cam.ac.uk (ppsw.cam.ac.uk [131.111.8.137]:25) with esmtp id 1FUWA0-0004AM-OE (Exim 4.54) (return-path ); Fri, 14 Apr 2006 22:49:00 +0100 Received: from cass25.ast.cam.ac.uk (cass25 [IPv6:2001:630:200:4240:203:baff:fe24:314]) by cass41.ast.cam.ac.uk (8.13.6+Sun/8.13.6) with ESMTP id k3ELmuHu013196; Fri, 14 Apr 2006 22:48:56 +0100 (BST) Received: from cass25.ast.cam.ac.uk (localhost [127.0.0.1]) by cass25.ast.cam.ac.uk (8.13.6+Sun/8.13.6) with ESMTP id k3ELmurs007140; Fri, 14 Apr 2006 22:48:56 +0100 (BST) Received: from localhost (lds@localhost) by cass25.ast.cam.ac.uk (8.13.6+Sun/8.13.6/Submit) with ESMTP id k3ELmtOm007137; Fri, 14 Apr 2006 22:48:55 +0100 (BST) X-Authentication-Warning: cass25.ast.cam.ac.uk: lds owned process doing -bs Date: Fri, 14 Apr 2006 22:48:55 +0100 (BST) From: Laurie Shaw X-X-Sender: lds@cass25 To: Gerard Lemson , Nicholas Walton , Laurie Shaw cc: ucd@ivoa.net, theory@ivoa.net Subject: UCD's for simulations In-Reply-To: Message-ID: References: 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: 2.3.0.1, Antispam-Data: 2006.04.13.165108 X-Virus-Scanned: by amavisd-new Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Laurie Shaw Dear All, I've recently been experimenting with assigning UCDs to the results of some cosmological simulations -- specifically to catalogues of dark matter halos and their associated subhalos. In general, i've found that the existing UCD tree is able to describe most of the properties of these objects that are typically analysed in the literature, albeit with a few exceptions. However, it is not currently possible to describe the properties and parameters of the simulations themselves. This includes some input physical parameters (i.e. cosmological parameters) that define the theoretical context of the simulation, and technical parameters that define its size,scope and resolution (e.g number of particles, length of simulation box side, gravitational softening length, time/redshift of a simulation output). Therefore, for the latter, I propose a new branch of the UCD tree to encompass computatational techniques in astronomy: 'comp'. This branch can be used to describe both astrophysical (and cosmological) simulations, and data reduction and post-processing algorithms for both simulation and observational data. It is roughly a computing analogue of the 'instr' branch. For the case of simulations I propose the following sub-branches comp.sim (computational simulation) comp.sim.nbody (Nbody simulation) comp.sim.sph (Smoothed Particle Hydrodynamics simulation) comp.sim.boxside (Simulation box) comp.sim.gravsoft (gravitational softening) comp.sim.particles (simulation particles (for Nbody and SPH simulations)) comp.sim.snapshot (output of a simulation box at a particular instant) comp.sim.grid (simulation grid (for hydro simulations)) The number of particles in the simulation box, number of grid points, particle mass, gravitational softening length and simulation box side length would therefore be: meta.num;comp.sim.particles meta.num;comp.sim.grid phys.mass;comp.sim.particles phys.size;comp.sim.gravsoft phys.size;comp.sim.boxside (For the last two, introduction of a phys.size.length UCD might provide a more accurate description.) The mass of an object in terms of the number of particles it contains: phys.mass;meta.num;comp.sim.particles Other possible sub-branches could be comp.resourse (computational resources used in simulation/data processing) comp.resource.processors (processors used) comp.resource.memory (total size of a data file) plus those that are more specific to data-reduction/post-processing of observational data. Algorithms that might apply to both simulated and observed data (e.g. smoothing of images or particle densities) would be listed directly under the comp branch: phys.size;comp.smooth (or, with the introduction of a phys.size.length UCD: phys.size.length;comp.smooth) Physical Parameters --------------------- Currently, there exists no UCDs for the main cosmological parameters. In terms of simulations, it is very important to be able define the assumed cosmology, when interpreting the results. To describe these parameters I propose a 'cosmology' sub-branch of the phys branch. So, phys.cosmology (cosmology) phys.cosmology.omega (matter/energy density of universe) phys.cosmology.hubble (hubble constant) phys.cosmology.sigma8 (Normalisation of matter power-spectrum) and also: phys.matter.dark (dark matter tag) phys.matter.baryon (baryonic matter tag) phys.DarkEnergy (dark energy tag) So, Omega_Lambda, Omega_DM, Omega_baryon would be phys.cosmology.omega;phys.DarkEnery, phys.cosmology.omega;phys.matter.dark phys.comsology.omega;phys.matter.baryonic Now we can also describe the number of dark matter (gas particles) in an SPH simulation, or a simulated object (star/galaxy/halo) using: meta.num;comp.sim.particles;phys.matter.dark(/baryonic) Furthermore, the mass and radius of dark matter halos in cosmological simulations are frequently defined in terms of a virial overdensity. Hence a phys.virial UCD would be usefull in specifying what is meant by the mass and radius of a halo: phys.mass;phys.virial (virial mass) phys.size.radius;phys.virial (virial radius) Time in Simulations ------------------ People frequently analyse the output of simulations, or snapshots, at a series of different timesteps. This is often quoted in terms of the redshift of the snapshot. At the moment, redshift exists under the 'src' branch. Maybe it might be better under the `phys' branch as it is a measure of both distance and time, and can therefore be used to label both the distance of observed objects and to label a time-stamp for simulation snapshots: phys.redshift;comp.sim.snapshot Astrophysical Objects -------------------- Another problem is the listing of astronomical objects types under the 'src' branch. This introduces confusion when trying to describe a simulated astrophysical object. For example, the first word in src.class.galaxy;comp.sim (simulated galaxy) implies that this is an observed astrophysical source, the second that it is simulated. Additionally, objects such as halos and subhalos are not typically observed (though i guess people do make estimates of their mass/size through gravitational lensing). It seems strange to have halo and subhalo listed under the src.class sub-branch. I therefore suggest that an object branch be introduced in which astrophysical (and theoretical) objects can be listed (as also proposed by others on the UCD suggestion page): object.galaxy;comp.sim (a simulated galaxy) object.galaxy.spiral;comp.sim (a simulated spiral galaxy) One example that I encountered of an actual quantity where this was useful is describing the mass in substructure, or the number of subhalos, in a simulated halo: phys.mass;object.DMhalo.subhalo meta.num;onject.DMhalo.subhalo It would be great to hear everyones thoughts, or ideas for alternative approaches, for all these. Cheers, Laurie List of Proposed UCDs --------------------- comp (computational astronomy) comp.sim (simulations) comp.sim.nbody (Nbody simulation) comp.sim.sph (Smoothed Particle Hydrodynamics simulation) comp.sim.boxside (Simulation box) comp.sim.gravsoft (gravitational softening) comp.sim.particles (simulation particles (for Nbody and SPH simulations)) comp.sim.snapshot (output of a simulation box at a particular instant) comp.sim.grid (simulation grid (for hydro simulations)) comp.resourse (to describe computational resources used in simulation/data processing) comp.resource.processors (processors used) comp.resource.memory (total size on disk of data) (comp.dataReduct ? comp.algorithm (general algorithms applied to sim/obs data) ) phys.cosmology phys.cosmology.omega (matter/energy density of universe) phys.cosmology.hubble (hubble constant) phys.cosmology.sigma8 (Normalisation of matter power-spectrum) phys.matter.dark (dark matter tag) phys.matter.baryon (baryonic matter tag) phys.DarkEnergy (dark energy tag) phys.virial phys.size.length object (astophysical object) object.planet (planet) object.satellite object.star (star) object.galaxy (galaxy) object.DMhalo (DM halo) Object.DMhalo.subhalo (DM subhalo) etc From owner-theory@eso.org Mon Apr 24 17:14:16 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k3OFE0WB018412 for ; Mon, 24 Apr 2006 17:14:01 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k3OFE0mk018407 for theory-outgoing; Mon, 24 Apr 2006 17:14:00 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k3OFDgWB018333 for ; Mon, 24 Apr 2006 17:13:44 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k3OFDer9005106 for ; Mon, 24 Apr 2006 17:13:41 +0200 (CEST) Received: from gavopc1 (gavopc1.xray.mpe.mpg.de [130.183.72.204]) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with SMTP id RAA19718; Mon, 24 Apr 2006 17:13:31 +0200 (METDST) From: "Gerard Lemson" To: Cc: "Dave De Young" , "Dr. Kokubo" , "Dr. Matumoto" , "Gerard Lemson" , =?iso-8859-1?Q?Herv=E9_Wozniak_?= , "Jongsoo Kim" , =?iso-8859-1?Q?Miguel_Cervi=F1o?= , "Nicholas Walton" , "Sarah Maddison " , "Ugo Becciani " , "Dave DeYoung" , "Enrique Solana" , "Franck LePetit" , "Laurie Shaw" , "Pedro Osuna" , "Tamas Budavari" Subject: Theory IG agenda Date: Mon, 24 Apr 2006 17:15:44 +0200 Message-ID: MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" Content-Transfer-Encoding: 7bit X-Priority: 3 (Normal) X-MSMail-Priority: Normal X-Mailer: Microsoft Outlook IMO, Build 9.0.6604 (9.0.2911.0) X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2800.1506 Importance: Normal X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.03.26.223108 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: "Gerard Lemson" Dear collegues I have asked the organising committee of the coming IVOA interop meeting for two sessions of the theory interest group. I think the goals should be to reach consensus and progress on the requirements document and on some proposals for standards that have recently emerged. In order to create an agenda I would like to ask for comments on the following proposal, and for volunteers for contributions. During the first session I propose to evaluate where we are wrt the use case scenarios we started one year ago. In particular I think we should discuss requirements extracted from the use cases which are to be posed to the WGs. I will submit a first draft of a Note containing such requirements by next week. During the meeting I would like to discuss this further and complete it as much as possible. To this end if anyone has still things to add to the use cases on the TWiki pages please do so, particularly paying attention to listing requirements on the standards as you see them I hope we can find time duringthe week to continue working on these issues in some more detail, possibly in smaller groups. The recent theory workshops in Cambridge and Paris show that it is easier to get results when people can sit together and discuss things face to face. I understand there are smaller rooms available where such meetings can take place. During these meetings we should take the chance to discuss some actual proposals that have been produced in the last few months. In particular the meeting in Cambridge has produced useful discussions about a SNAP DAL protocol (see the minutes at http://www.ivoa.net/twiki/bin/view/IVOA/CambridgeTheoryWorkshopFeb06) and Laurie is working on a draft of this. Laurie has also produced work on UCDs which we should discuss and turn into a full. This all deals with n-body simulations mainly. I think it would be good therefore to also discuss in more detail what requirements can be derived from synthetic spectra, especially in the context of the SSA protocol and SED data model, thta are under develoment in the DAL and DM groups respectively. As suggested in Paris, we may want to look how the recent draft for the characterisation data model can be used for characterising the footprint etc of simulations. The results of these efforts will be discussed in the second session, likely on Thursday afternoon, hopefully with attendance of relevant WG members. Dave DeYoung has suggested the interest group could/should morph into a working group. Maybe this can be discussed during this session. The final results will be presented during the closing plenary session. Please your comments, a note whether you will attend the meeting, whether you are willing to contribute anything to these sessions, or suggestions for more specific topics to talk about within the context described above. Best regards Gerard Lemson PS My appologies if you get this mail multiple times. There is no doubt some overlap between the various mailing lists I am using. -- * Gerard Lemson * Tel: +49 (0)89 30000-3316 * * MPI fuer extraterrestische Physik * Fax: +49 (0)89 30000-3569 * * Giessenbachstrasse * * * Postfach 1312 * * * D-85741 Garching, GERMANY * email: gerard.lemson@mpe.mpg.de * From owner-theory@eso.org Thu May 4 14:43:13 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k44Ch1Lc004217 for ; Thu, 4 May 2006 14:43:01 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k44Ch1ce004216 for theory-outgoing; Thu, 4 May 2006 14:43:01 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k44Ch0Lc004212; Thu, 4 May 2006 14:43:00 +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 k44CgwxF010081; Thu, 4 May 2006 14:42:59 +0200 (CEST) Received: from [161.111.165.119] (dae-d19.iaa.csic.es [161.111.165.119]) by iaa13u.iaa.csic.es (8.9.3/8.9.1) with ESMTP id OAA15244; Thu, 4 May 2006 14:42:52 +0200 (MET DST) Mime-Version: 1.0 (Apple Message framework v749.3) Content-Type: text/plain; charset=ISO-8859-1; delsp=yes; format=flowed Message-Id: <83BB6883-226C-40EC-B266-280310C48E3D@iaa.es> Cc: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: tehoretical SEDs in VO applications Date: Thu, 4 May 2006 14:42:34 +0200 To: theory@ivoa.net, apps@ivoa.net X-Mailer: Apple Mail (2.749.3) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.4.42617 Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id k44Ch1Lc004213 Sender: owner-theory@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Dear all, I just send this comments that may be discussed in the next meeting. It is just a comparison about how different VO applications manage a SED building following the SED data model requirements. The applications compared are VOSpec, specview, topcat, and VOplot. (Note that topcat and VOplot are general propose tools and VOSpec and specview are specific for SEDs). I had find that more or less the current SED data model is fine for theory, and may be, model parameters should be specified in ... fields for characterization or provenance (it is an issue to be defined in the theory group). Note that in the theoretical domain, the parameters that define the model are equally relevant than the model results themselves. However, for the case of applications, (visualization tools mainly) I had found some inconsistence/problems with a VOTable designed in such a way, and also internal inconsistency between different tools. I summarize them here: a) problem with units nomenclature: There is no recommendation about the use of units in the VOTable fields. In particular, VOSpec and specview use different ways to define the units for the flux e.j. cm**2 vs. cm2 to define the $cm^2$ (in latex). Would it be possible to define any recommendation about that? Otherwise the same VOTable would not be used for both applications! b) Metadata and saved files: As pointed before, metadata in theoretical models are fundamental to understand and perform any posterior analysis or comparison with real data (or "pipeline" process for datamining as example). Again, metadata are sometimes equal in importance than the simulation result. However: - the VOTable metadata are not visualized by VOSpec, sepcview and VOPlot - metadata otuside are visualized by Topcat, but not metadata in ... (so may be the use of a for characterization of the model is not a good idea after all...) About the VOTables that can be saved by VOSpec, specview and Topcat (VOPlot do not save VOTables) it is found that metadata is systematically lost!! (it means, such type of applications are not completely suitable to retrieve theoretical models thought the VO registry for their posterior use!). In particular: - specview: do not include niether the original VOTable of but include their own and 's - VOSpec do not include the original metadata - and VOTables saved by topcat include table metadata but all parameters are lost. c) Columns to be plotted: c.1) specview needs 3 requirements to plot a VOTable: i.- the Table must have a name (only VOTables with looks to work ii.- utype in x and y coordinates in FIELD must be specified c.2) VOSpec needs two (non-standard) lines to specify the columns and only two columns can be plotted (i.e. do not include for example a column with errors that would be useful for both observations and theoretical data. Finally, for theoretical SEDs, they are some times stored in a multicolumn format, I have not tested with spectview, but it is not supported by VOSpec. d) A final comment, it looks that only VOSpec is able to manage a Theoretical spectral acces protocol: It means, perform the query to a server that gives back a table with the parameter space covered by the models that the server provides, and perform a "second" query over a subsample of the parameter space covered. I hope that this comments would help to improve the applications and for the theory group best regards Miguel Cerviño From owner-apps@eso.org Thu May 4 14:43:18 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k44Ch2Lc004222 for ; Thu, 4 May 2006 14:43:02 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k44Ch1K2004221 for apps-outgoing; Thu, 4 May 2006 14:43:01 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-apps@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 k44Ch0Lc004212; Thu, 4 May 2006 14:43:00 +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 k44CgwxF010081; Thu, 4 May 2006 14:42:59 +0200 (CEST) Received: from [161.111.165.119] (dae-d19.iaa.csic.es [161.111.165.119]) by iaa13u.iaa.csic.es (8.9.3/8.9.1) with ESMTP id OAA15244; Thu, 4 May 2006 14:42:52 +0200 (MET DST) Mime-Version: 1.0 (Apple Message framework v749.3) Content-Type: text/plain; charset=ISO-8859-1; delsp=yes; format=flowed Message-Id: <83BB6883-226C-40EC-B266-280310C48E3D@iaa.es> Cc: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: tehoretical SEDs in VO applications Date: Thu, 4 May 2006 14:42:34 +0200 To: theory@ivoa.net, apps@ivoa.net X-Mailer: Apple Mail (2.749.3) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.4.42617 Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id k44Ch1Lc004213 Sender: owner-apps@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Dear all, I just send this comments that may be discussed in the next meeting. It is just a comparison about how different VO applications manage a SED building following the SED data model requirements. The applications compared are VOSpec, specview, topcat, and VOplot. (Note that topcat and VOplot are general propose tools and VOSpec and specview are specific for SEDs). I had find that more or less the current SED data model is fine for theory, and may be, model parameters should be specified in ... fields for characterization or provenance (it is an issue to be defined in the theory group). Note that in the theoretical domain, the parameters that define the model are equally relevant than the model results themselves. However, for the case of applications, (visualization tools mainly) I had found some inconsistence/problems with a VOTable designed in such a way, and also internal inconsistency between different tools. I summarize them here: a) problem with units nomenclature: There is no recommendation about the use of units in the VOTable fields. In particular, VOSpec and specview use different ways to define the units for the flux e.j. cm**2 vs. cm2 to define the $cm^2$ (in latex). Would it be possible to define any recommendation about that? Otherwise the same VOTable would not be used for both applications! b) Metadata and saved files: As pointed before, metadata in theoretical models are fundamental to understand and perform any posterior analysis or comparison with real data (or "pipeline" process for datamining as example). Again, metadata are sometimes equal in importance than the simulation result. However: - the VOTable metadata are not visualized by VOSpec, sepcview and VOPlot - metadata otuside are visualized by Topcat, but not metadata in ... (so may be the use of a for characterization of the model is not a good idea after all...) About the VOTables that can be saved by VOSpec, specview and Topcat (VOPlot do not save VOTables) it is found that metadata is systematically lost!! (it means, such type of applications are not completely suitable to retrieve theoretical models thought the VO registry for their posterior use!). In particular: - specview: do not include niether the original VOTable of but include their own and 's - VOSpec do not include the original metadata - and VOTables saved by topcat include table metadata but all parameters are lost. c) Columns to be plotted: c.1) specview needs 3 requirements to plot a VOTable: i.- the Table must have a name (only VOTables with
looks to work ii.- utype in x and y coordinates in FIELD must be specified c.2) VOSpec needs two (non-standard) lines to specify the columns and only two columns can be plotted (i.e. do not include for example a column with errors that would be useful for both observations and theoretical data. Finally, for theoretical SEDs, they are some times stored in a multicolumn format, I have not tested with spectview, but it is not supported by VOSpec. d) A final comment, it looks that only VOSpec is able to manage a Theoretical spectral acces protocol: It means, perform the query to a server that gives back a table with the parameter space covered by the models that the server provides, and perform a "second" query over a subsample of the parameter space covered. I hope that this comments would help to improve the applications and for the theory group best regards Miguel Cerviño From owner-theory@eso.org Thu May 4 15:17:29 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k44DHMLc011448 for ; Thu, 4 May 2006 15:17:22 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k44DHMAR011447 for theory-outgoing; Thu, 4 May 2006 15:17:22 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k44DHILc011428; Thu, 4 May 2006 15:17:18 +0200 (MEST) Received: from mailhost.u-strasbg.fr (mailhost.u-strasbg.fr [130.79.200.151]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k44DHFr9008777; Thu, 4 May 2006 15:17:16 +0200 (CEST) Received: from vizir.u-strasbg.fr (vizir.u-strasbg.fr [130.79.128.13]) by mailhost.u-strasbg.fr (8.13.4/jtpda-5.5pre1) with ESMTP id k44DH9ua067520 ; Thu, 4 May 2006 15:17:09 +0200 (CEST) Received: from newb6.u-strasbg.fr (localhost [127.0.0.1]) by vizir.u-strasbg.fr (8.11.6+Sun/8.9.1) with ESMTP id k44DIcQ13515; Thu, 4 May 2006 15:18:38 +0200 (MET DST) Message-ID: <4459FF2E.A38836FB@newb6.u-strasbg.fr> Date: Thu, 04 May 2006 15:18:38 +0200 From: Thomas Boch Organization: CDS - Observatoire astronomique de Strasbourg X-Mailer: Mozilla 4.7 [en] (X11; I; SunOS 5.7 sun4u) X-Accept-Language: en MIME-Version: 1.0 To: Miguel =?iso-8859-1?Q?Cervi=F1o?= CC: theory@ivoa.net, apps@ivoa.net Subject: Re: tehoretical SEDs in VO applications References: <83BB6883-226C-40EC-B266-280310C48E3D@iaa.es> Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-2.0.2 (mailhost.u-strasbg.fr [130.79.200.151]); Thu, 04 May 2006 15:17:09 +0200 (CEST) X-Virus-Scanned: ClamAV 0.88.1/1439/Thu May 4 09:33:29 2006 on mr1.u-strasbg.fr X-Virus-Status: Clean X-Spam-Status: No, score=-1.4 required=5.0 tests=ALL_TRUSTED,AWL autolearn=disabled version=3.1.1 X-Spam-Checker-Version: SpamAssassin 3.1.1 (2006-03-10) on mr1.u-strasbg.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.4.53212 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Thomas Boch Dear Miguel, I'd like to comment your first point. > > a) problem with units nomenclature: There is no recommendation about > the use of units in the VOTable > fields. In particular, VOSpec and specview use different ways to > define the units for the flux > e.j. cm**2 vs. cm2 to define the $cm^2$ (in latex). Would it be > possible to define any > recommendation about that? Otherwise the same VOTable would not be > used for both applications! Section 4.3 of the VOTable document ( http://www.ivoa.net/Documents/latest/VOT.html ) gives a reference ( http://vizier.u-strasbg.fr/doc/catstd-3.2.htx ) about how units should be expressed. According to this section, $cm^2$ should be defined in a VOTable field as unit="cm2" Cheers, Thomas From owner-apps@eso.org Thu May 4 15:17:36 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k44DHLLc011441 for ; Thu, 4 May 2006 15:17:21 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k44DHLK8011438 for apps-outgoing; Thu, 4 May 2006 15:17:21 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-apps@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 k44DHILc011428; Thu, 4 May 2006 15:17:18 +0200 (MEST) Received: from mailhost.u-strasbg.fr (mailhost.u-strasbg.fr [130.79.200.151]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k44DHFr9008777; Thu, 4 May 2006 15:17:16 +0200 (CEST) Received: from vizir.u-strasbg.fr (vizir.u-strasbg.fr [130.79.128.13]) by mailhost.u-strasbg.fr (8.13.4/jtpda-5.5pre1) with ESMTP id k44DH9ua067520 ; Thu, 4 May 2006 15:17:09 +0200 (CEST) Received: from newb6.u-strasbg.fr (localhost [127.0.0.1]) by vizir.u-strasbg.fr (8.11.6+Sun/8.9.1) with ESMTP id k44DIcQ13515; Thu, 4 May 2006 15:18:38 +0200 (MET DST) Message-ID: <4459FF2E.A38836FB@newb6.u-strasbg.fr> Date: Thu, 04 May 2006 15:18:38 +0200 From: Thomas Boch Organization: CDS - Observatoire astronomique de Strasbourg X-Mailer: Mozilla 4.7 [en] (X11; I; SunOS 5.7 sun4u) X-Accept-Language: en MIME-Version: 1.0 To: Miguel =?iso-8859-1?Q?Cervi=F1o?= CC: theory@ivoa.net, apps@ivoa.net Subject: Re: tehoretical SEDs in VO applications References: <83BB6883-226C-40EC-B266-280310C48E3D@iaa.es> Content-Type: text/plain; charset=us-ascii Content-Transfer-Encoding: 7bit X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-2.0.2 (mailhost.u-strasbg.fr [130.79.200.151]); Thu, 04 May 2006 15:17:09 +0200 (CEST) X-Virus-Scanned: ClamAV 0.88.1/1439/Thu May 4 09:33:29 2006 on mr1.u-strasbg.fr X-Virus-Status: Clean X-Spam-Status: No, score=-1.4 required=5.0 tests=ALL_TRUSTED,AWL autolearn=disabled version=3.1.1 X-Spam-Checker-Version: SpamAssassin 3.1.1 (2006-03-10) on mr1.u-strasbg.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.4.53212 Sender: owner-apps@eso.org Precedence: bulk Reply-To: Thomas Boch Dear Miguel, I'd like to comment your first point. > > a) problem with units nomenclature: There is no recommendation about > the use of units in the VOTable > fields. In particular, VOSpec and specview use different ways to > define the units for the flux > e.j. cm**2 vs. cm2 to define the $cm^2$ (in latex). Would it be > possible to define any > recommendation about that? Otherwise the same VOTable would not be > used for both applications! Section 4.3 of the VOTable document ( http://www.ivoa.net/Documents/latest/VOT.html ) gives a reference ( http://vizier.u-strasbg.fr/doc/catstd-3.2.htx ) about how units should be expressed. According to this section, $cm^2$ should be defined in a VOTable field as unit="cm2" Cheers, Thomas From owner-theory@eso.org Thu May 4 17:57:25 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k44FvIO5011905 for ; Thu, 4 May 2006 17:57:18 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k44FvIUw011903 for theory-outgoing; Thu, 4 May 2006 17:57:18 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k44FvHO5011893; Thu, 4 May 2006 17:57:17 +0200 (MEST) Received: from mail.ncsa.uiuc.edu (mail.ncsa.uiuc.edu [141.142.2.28]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k44FvEr9017566; Thu, 4 May 2006 17:57:15 +0200 (CEST) X-Envelope-From: rplante@poplar.ncsa.uiuc.edu Received: from poplar.ncsa.uiuc.edu (poplar.ncsa.uiuc.edu [141.142.240.13]) by mail.ncsa.uiuc.edu (8.11.7/8.11.7) with ESMTP id k44Fv4014902; Thu, 4 May 2006 10:57:04 -0500 Received: from poplar.ncsa.uiuc.edu (localhost.localdomain [127.0.0.1]) by poplar.ncsa.uiuc.edu (8.12.8/8.12.8) with ESMTP id k44Fv5qU004903; Thu, 4 May 2006 10:57:05 -0500 Received: from localhost (rplante@localhost) by poplar.ncsa.uiuc.edu (8.12.8/8.12.8/Submit) with ESMTP id k44Fv4fn004899; Thu, 4 May 2006 10:57:05 -0500 Date: Thu, 4 May 2006 10:57:04 -0500 (CDT) From: Ray Plante To: theory@ivoa.net cc: registry@ivoa.net Subject: How to Publish to the NVO Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-NCSA-MailScanner-Information: Please contact help@ncsa.uiuc.edu for more information, mail.ncsa.uiuc.edu X-NCSA-MailScanner: Found to be clean X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.4.82629 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Ray Plante Gentle Theorists, During a recent chat, Sebastien Derriere reported on a meeting of VOTheorists in which there was some discussion of how one should publish simulation data and/or services to the VO. I thought that I would mention a document I wrote for the NVO called "How to Publish to the NVO". It's meant to be a brief introduction to VO publishing with pointers to how to get started. It's a little out of date at the moment (an update is in the works), but it is not inaccurate. I would be interested to get some feedback from your group about how applicable you feel it is to theory-related resources. In particular, if you have suggestions for addressing the theory community, this would get a great time to get those. In the VO, we talk a lot about registering standard services like SIA and SkyNodes. However you may not be aware that it is currently possible to register general data collections and non-standard services, including those that have a web-page interface. While I'm sure that you will benefit from some standards that are specifically targetted to the theory community in the future, you may find the generic resource descriptions useful today. In fact, I would encourage you to visit the registry at NCSA (http://nvo.ncsa.uiuc.edu/nvoregistration.html) and try registering somethings. This site provides a sandbox version that allows you to try out the interface without actually publishing anything. Finally, to the Registry WG, it's been suggested that we take a look at this document and see if there is an IVOA version we might publish as a note. Your feedback is welcome as well. cheers, Ray From owner-registry@eso.org Thu May 4 17:57:33 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k44FvIO5011914 for ; Thu, 4 May 2006 17:57:18 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k44FvI1Y011913 for registry-outgoing; Thu, 4 May 2006 17:57:18 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-registry@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k44FvHO5011893; Thu, 4 May 2006 17:57:17 +0200 (MEST) Received: from mail.ncsa.uiuc.edu (mail.ncsa.uiuc.edu [141.142.2.28]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k44FvEr9017566; Thu, 4 May 2006 17:57:15 +0200 (CEST) X-Envelope-From: rplante@poplar.ncsa.uiuc.edu Received: from poplar.ncsa.uiuc.edu (poplar.ncsa.uiuc.edu [141.142.240.13]) by mail.ncsa.uiuc.edu (8.11.7/8.11.7) with ESMTP id k44Fv4014902; Thu, 4 May 2006 10:57:04 -0500 Received: from poplar.ncsa.uiuc.edu (localhost.localdomain [127.0.0.1]) by poplar.ncsa.uiuc.edu (8.12.8/8.12.8) with ESMTP id k44Fv5qU004903; Thu, 4 May 2006 10:57:05 -0500 Received: from localhost (rplante@localhost) by poplar.ncsa.uiuc.edu (8.12.8/8.12.8/Submit) with ESMTP id k44Fv4fn004899; Thu, 4 May 2006 10:57:05 -0500 Date: Thu, 4 May 2006 10:57:04 -0500 (CDT) From: Ray Plante To: theory@ivoa.net cc: registry@ivoa.net Subject: How to Publish to the NVO Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-NCSA-MailScanner-Information: Please contact help@ncsa.uiuc.edu for more information, mail.ncsa.uiuc.edu X-NCSA-MailScanner: Found to be clean X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.4.82629 Sender: owner-registry@eso.org Precedence: bulk Reply-To: Ray Plante Gentle Theorists, During a recent chat, Sebastien Derriere reported on a meeting of VOTheorists in which there was some discussion of how one should publish simulation data and/or services to the VO. I thought that I would mention a document I wrote for the NVO called "How to Publish to the NVO". It's meant to be a brief introduction to VO publishing with pointers to how to get started. It's a little out of date at the moment (an update is in the works), but it is not inaccurate. I would be interested to get some feedback from your group about how applicable you feel it is to theory-related resources. In particular, if you have suggestions for addressing the theory community, this would get a great time to get those. In the VO, we talk a lot about registering standard services like SIA and SkyNodes. However you may not be aware that it is currently possible to register general data collections and non-standard services, including those that have a web-page interface. While I'm sure that you will benefit from some standards that are specifically targetted to the theory community in the future, you may find the generic resource descriptions useful today. In fact, I would encourage you to visit the registry at NCSA (http://nvo.ncsa.uiuc.edu/nvoregistration.html) and try registering somethings. This site provides a sandbox version that allows you to try out the interface without actually publishing anything. Finally, to the Registry WG, it's been suggested that we take a look at this document and see if there is an IVOA version we might publish as a note. Your feedback is welcome as well. cheers, Ray From owner-theory@eso.org Thu May 4 18:17:05 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k44GH0O5015381 for ; Thu, 4 May 2006 18:17:00 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k44GH0WC015379 for theory-outgoing; Thu, 4 May 2006 18:17:00 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k44GGxO5015370; Thu, 4 May 2006 18:16:59 +0200 (MEST) Received: from mail.ncsa.uiuc.edu (mail.ncsa.uiuc.edu [141.142.2.28]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k44GGvr9018577; Thu, 4 May 2006 18:16:57 +0200 (CEST) X-Envelope-From: rplante@poplar.ncsa.uiuc.edu Received: from poplar.ncsa.uiuc.edu (poplar.ncsa.uiuc.edu [141.142.240.13]) by mail.ncsa.uiuc.edu (8.11.7/8.11.7) with ESMTP id k44GGV005752; Thu, 4 May 2006 11:16:32 -0500 Received: from poplar.ncsa.uiuc.edu (localhost.localdomain [127.0.0.1]) by poplar.ncsa.uiuc.edu (8.12.8/8.12.8) with ESMTP id k44GGWqU009946; Thu, 4 May 2006 11:16:32 -0500 Received: from localhost (rplante@localhost) by poplar.ncsa.uiuc.edu (8.12.8/8.12.8/Submit) with ESMTP id k44GGWRc009942; Thu, 4 May 2006 11:16:32 -0500 Date: Thu, 4 May 2006 11:16:32 -0500 (CDT) From: Ray Plante To: theory@ivoa.net cc: registry@ivoa.net Subject: Re: How to Publish to the NVO In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-NCSA-MailScanner-Information: Please contact help@ncsa.uiuc.edu for more information, mail.ncsa.uiuc.edu X-NCSA-MailScanner: Found to be clean X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.4.85115 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Ray Plante On Thu, 4 May 2006, Ray Plante wrote: > Gentle Theorists, > > I thought that I would mention > a document I wrote for the NVO called "How to Publish to the NVO". I guess I should provide you with an actual pointer to the document, right? http://us-vo.org/pubs/files/PublishHowTo.html cheers, Ray From owner-registry@eso.org Thu May 4 18:17:12 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k44GH0O5015388 for ; Thu, 4 May 2006 18:17:00 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k44GH0B1015387 for registry-outgoing; Thu, 4 May 2006 18:17:00 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-registry@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k44GGxO5015370; Thu, 4 May 2006 18:16:59 +0200 (MEST) Received: from mail.ncsa.uiuc.edu (mail.ncsa.uiuc.edu [141.142.2.28]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k44GGvr9018577; Thu, 4 May 2006 18:16:57 +0200 (CEST) X-Envelope-From: rplante@poplar.ncsa.uiuc.edu Received: from poplar.ncsa.uiuc.edu (poplar.ncsa.uiuc.edu [141.142.240.13]) by mail.ncsa.uiuc.edu (8.11.7/8.11.7) with ESMTP id k44GGV005752; Thu, 4 May 2006 11:16:32 -0500 Received: from poplar.ncsa.uiuc.edu (localhost.localdomain [127.0.0.1]) by poplar.ncsa.uiuc.edu (8.12.8/8.12.8) with ESMTP id k44GGWqU009946; Thu, 4 May 2006 11:16:32 -0500 Received: from localhost (rplante@localhost) by poplar.ncsa.uiuc.edu (8.12.8/8.12.8/Submit) with ESMTP id k44GGWRc009942; Thu, 4 May 2006 11:16:32 -0500 Date: Thu, 4 May 2006 11:16:32 -0500 (CDT) From: Ray Plante To: theory@ivoa.net cc: registry@ivoa.net Subject: Re: How to Publish to the NVO In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-NCSA-MailScanner-Information: Please contact help@ncsa.uiuc.edu for more information, mail.ncsa.uiuc.edu X-NCSA-MailScanner: Found to be clean X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.4.85115 Sender: owner-registry@eso.org Precedence: bulk Reply-To: Ray Plante On Thu, 4 May 2006, Ray Plante wrote: > Gentle Theorists, > > I thought that I would mention > a document I wrote for the NVO called "How to Publish to the NVO". I guess I should provide you with an actual pointer to the document, right? http://us-vo.org/pubs/files/PublishHowTo.html cheers, Ray From owner-theory@eso.org Thu May 4 20:02:36 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k44I2SO5029457 for ; Thu, 4 May 2006 20:02:28 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k44I2Svp029456 for theory-outgoing; Thu, 4 May 2006 20:02:28 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k44I2RO5029442; Thu, 4 May 2006 20:02:27 +0200 (MEST) Received: from sol.star.bris.ac.uk (sol.star.bris.ac.uk [137.222.58.39]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k44I2PxF029394; Thu, 4 May 2006 20:02:26 +0200 (CEST) Received: from andromeda.star.bris.ac.uk ([137.222.58.155] ident=root) by sol.star.bris.ac.uk with esmtp (Exim 3.35 #1) id 1Fbi9c-000464-00; Thu, 04 May 2006 19:02:20 +0100 Received: from mbt (helo=localhost) by andromeda.star.bris.ac.uk with local-esmtp (Exim 3.36 #1) id 1Fbi9Y-0008CH-00; Thu, 04 May 2006 19:02:16 +0100 Date: Thu, 4 May 2006 19:02:16 +0100 (BST) From: Mark Taylor X-X-Sender: mbt@andromeda.star.bris.ac.uk To: theory@ivoa.net, Subject: Re: tehoretical SEDs in VO applications In-Reply-To: <83BB6883-226C-40EC-B266-280310C48E3D@iaa.es> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=ISO-8859-1 X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.4.103150 Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from QUOTED-PRINTABLE to 8bit by mercury.hq.eso.org id k44I2RO5029444 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Mark Taylor On Thu, 4 May 2006, Miguel Cerviño wrote: > Dear all, > > I just send this comments that may be discussed in the next meeting. > It is just a comparison about how different VO applications manage > a SED building following the SED data model requirements. > The applications compared are VOSpec, specview, topcat, and VOplot. > (Note that topcat and VOplot are general propose tools and VOSpec and > specview are specific for SEDs). Miguel, thanks for this posting. This kind of detailed feedback on what does and doesn't work, and what you want to see, is useful for application developers (well, I speak for myself in any case). As you say, TOPCAT doesn't pay much attention to GROUP elements at present. I believe what it does is to behave as if GROUP elements (though not their contents) are not there, so the grouping will be lost, but columns and parameters within the group will not. It also ignores table structure (for instance RESOURCEs within RESOURCEs) in a similar way. Trying to do improve this kind of table metadata retention for VOTables is on the to-do list, but not currently very near the top (there are some technical difficulties which I will forbear to explain). However, if it's something which the theory community (and others?) see as important I can see about prioritising it. Ranking on the to-do list is influenced by user requests; I have had a few requests for this in the past but not that many. Mark -- Mark Taylor Astronomical Programmer Physics, Bristol University, UK m.b.taylor@bris.ac.uk +44-117-928-8776 http://www.star.bris.ac.uk/~mbt/ From owner-apps@eso.org Thu May 4 20:02:48 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k44I2SO5029450 for ; Thu, 4 May 2006 20:02:28 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k44I2Sm1029449 for apps-outgoing; Thu, 4 May 2006 20:02:28 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-apps@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 k44I2RO5029442; Thu, 4 May 2006 20:02:27 +0200 (MEST) Received: from sol.star.bris.ac.uk (sol.star.bris.ac.uk [137.222.58.39]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k44I2PxF029394; Thu, 4 May 2006 20:02:26 +0200 (CEST) Received: from andromeda.star.bris.ac.uk ([137.222.58.155] ident=root) by sol.star.bris.ac.uk with esmtp (Exim 3.35 #1) id 1Fbi9c-000464-00; Thu, 04 May 2006 19:02:20 +0100 Received: from mbt (helo=localhost) by andromeda.star.bris.ac.uk with local-esmtp (Exim 3.36 #1) id 1Fbi9Y-0008CH-00; Thu, 04 May 2006 19:02:16 +0100 Date: Thu, 4 May 2006 19:02:16 +0100 (BST) From: Mark Taylor X-X-Sender: mbt@andromeda.star.bris.ac.uk To: theory@ivoa.net, Subject: Re: tehoretical SEDs in VO applications In-Reply-To: <83BB6883-226C-40EC-B266-280310C48E3D@iaa.es> Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=ISO-8859-1 X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.4.103150 Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from QUOTED-PRINTABLE to 8bit by mercury.hq.eso.org id k44I2RO5029444 Sender: owner-apps@eso.org Precedence: bulk Reply-To: Mark Taylor On Thu, 4 May 2006, Miguel Cerviño wrote: > Dear all, > > I just send this comments that may be discussed in the next meeting. > It is just a comparison about how different VO applications manage > a SED building following the SED data model requirements. > The applications compared are VOSpec, specview, topcat, and VOplot. > (Note that topcat and VOplot are general propose tools and VOSpec and > specview are specific for SEDs). Miguel, thanks for this posting. This kind of detailed feedback on what does and doesn't work, and what you want to see, is useful for application developers (well, I speak for myself in any case). As you say, TOPCAT doesn't pay much attention to GROUP elements at present. I believe what it does is to behave as if GROUP elements (though not their contents) are not there, so the grouping will be lost, but columns and parameters within the group will not. It also ignores table structure (for instance RESOURCEs within RESOURCEs) in a similar way. Trying to do improve this kind of table metadata retention for VOTables is on the to-do list, but not currently very near the top (there are some technical difficulties which I will forbear to explain). However, if it's something which the theory community (and others?) see as important I can see about prioritising it. Ranking on the to-do list is influenced by user requests; I have had a few requests for this in the past but not that many. Mark -- Mark Taylor Astronomical Programmer Physics, Bristol University, UK m.b.taylor@bris.ac.uk +44-117-928-8776 http://www.star.bris.ac.uk/~mbt/ From owner-theory@eso.org Thu May 4 20:14:45 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k44IEdO5001277 for ; Thu, 4 May 2006 20:14:40 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k44IEdVQ001276 for theory-outgoing; Thu, 4 May 2006 20:14:39 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k44IEdO5001271 for ; Thu, 4 May 2006 20:14:39 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k44IEbxF000006 for ; Thu, 4 May 2006 20:14:38 +0200 (CEST) Received: from localhost (glemson@localhost) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with ESMTP id UAA02365; Thu, 4 May 2006 20:14:28 +0200 (METDST) X-Authentication-Warning: mpehp1.mpe-garching.mpg.de: glemson owned process doing -bs Date: Thu, 4 May 2006 20:14:28 +0200 (METDST) From: Gerard Lemson X-Sender: glemson@mpehp1.mpe-garching.mpg.de To: Ray Plante cc: theory@ivoa.net Subject: Re: How to Publish to the NVO In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.4.105107 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Gerard Lemson Hi Ray We did indeed came to the conclusion that it should be possible to register resources without there being a fitting standard specification/protocol. I would actually like to try to register some such theory specific services and datasets during the interop, as there we could benefit from interaction with registry connaiseurs such as you. Would you be willing and to make a contribution to one of the theory sessions on Monday to explain this in some more detail ? Cheers Gerard On Thu, 4 May 2006, Ray Plante wrote: > Gentle Theorists, > > During a recent chat, Sebastien Derriere reported on a meeting of > VOTheorists in which there was some discussion of how one should publish > simulation data and/or services to the VO. I thought that I would mention > a document I wrote for the NVO called "How to Publish to the NVO". It's > meant to be a brief introduction to VO publishing with pointers to how to > get started. It's a little out of date at the moment (an update is in the > works), but it is not inaccurate. I would be interested to get some > feedback from your group about how applicable you feel it is to > theory-related resources. In particular, if you have suggestions for > addressing the theory community, this would get a great time to get those. > > In the VO, we talk a lot about registering standard services like SIA and > SkyNodes. However you may not be aware that it is currently possible to > register general data collections and non-standard services, including > those that have a web-page interface. While I'm sure that you will > benefit from some standards that are specifically targetted to the theory > community in the future, you may find the generic resource descriptions > useful today. In fact, I would encourage you to visit the registry at > NCSA (http://nvo.ncsa.uiuc.edu/nvoregistration.html) and try registering > somethings. This site provides a sandbox version that allows you to try > out the interface without actually publishing anything. > > Finally, to the Registry WG, it's been suggested that we take a look at > this document and see if there is an IVOA version we might publish as a > note. Your feedback is welcome as well. > > cheers, > Ray > > From owner-theory@eso.org Thu May 4 20:20:44 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k44IKcO5002311 for ; Thu, 4 May 2006 20:20:38 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k44IKbCF002310 for theory-outgoing; Thu, 4 May 2006 20:20:37 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k44IKbO5002306 for ; Thu, 4 May 2006 20:20:37 +0200 (MEST) Received: from mail.ncsa.uiuc.edu (mail.ncsa.uiuc.edu [141.142.2.28]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k44IKYxF000297 for ; Thu, 4 May 2006 20:20:35 +0200 (CEST) X-Envelope-From: rplante@poplar.ncsa.uiuc.edu Received: from poplar.ncsa.uiuc.edu (poplar.ncsa.uiuc.edu [141.142.240.13]) by mail.ncsa.uiuc.edu (8.11.7/8.11.7) with ESMTP id k44IK6009493; Thu, 4 May 2006 13:20:06 -0500 Received: from poplar.ncsa.uiuc.edu (localhost.localdomain [127.0.0.1]) by poplar.ncsa.uiuc.edu (8.12.8/8.12.8) with ESMTP id k44IK7qU017021; Thu, 4 May 2006 13:20:07 -0500 Received: from localhost (rplante@localhost) by poplar.ncsa.uiuc.edu (8.12.8/8.12.8/Submit) with ESMTP id k44IK6P3017017; Thu, 4 May 2006 13:20:07 -0500 Date: Thu, 4 May 2006 13:20:06 -0500 (CDT) From: Ray Plante To: Gerard Lemson cc: theory@ivoa.net Subject: Re: How to Publish to the NVO In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-NCSA-MailScanner-Information: Please contact help@ncsa.uiuc.edu for more information, mail.ncsa.uiuc.edu X-NCSA-MailScanner: Found to be clean X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.4.103150 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Ray Plante On Thu, 4 May 2006, Gerard Lemson wrote: > Would you be willing and to make a contribution to one of the theory > sessions on Monday to explain this in some more detail ? Sure. There's the usual juggling of parallel sessions. I'm slated to give a talk at one of the GWS sessions but I'm not sure which, yet. cheers, Ray From owner-theory@eso.org Thu May 4 23:09:43 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k44L9cO5028424 for ; Thu, 4 May 2006 23:09:38 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k44L9cuj028423 for theory-outgoing; Thu, 4 May 2006 23:09:38 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k44L9bO5028418 for ; Thu, 4 May 2006 23:09:37 +0200 (MEST) Received: from mesiob.obspm.fr (mesiob.obspm.fr [145.238.2.2]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k44L9Zr9005281 for ; Thu, 4 May 2006 23:09:35 +0200 (CEST) Received: from [145.238.18.175] (achille.obspm.fr [145.238.18.175]) by mesiob.obspm.fr (8.13.4/8.13.4/SIO Observatoire de Paris) with ESMTP id k44L9T6o010963; Thu, 4 May 2006 23:09:29 +0200 In-Reply-To: References: Mime-Version: 1.0 (Apple Message framework v749.3) Content-Type: text/plain; charset=ISO-8859-1; delsp=yes; format=flowed Message-Id: <68D040F3-2B11-46FA-93C1-12A1AF6236B2@obspm.fr> Cc: Ray Plante , theory@ivoa.net From: Franck Le Petit Subject: Re: How to Publish to the NVO Date: Thu, 4 May 2006 23:01:36 +0200 To: Gerard Lemson X-Mailer: Apple Mail (2.749.3) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-2.0.2 (mesiob.obspm.fr [145.238.2.2]); Thu, 04 May 2006 23:09:29 +0200 (CEST) X-Virus-Scanned: ClamAV version 0.88.2, clamav-milter version 0.88.2 on mesiob.obspm.fr X-Virus-Status: Clean X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.4.133105 Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id k44L9bO5028419 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Franck Le Petit Dear Gerard, dear Ray and dear members of VO-Theory I followed Ray informations to register my PDR simulation code in the NVO registry. I did some mistakes (as the creation of an organization and an authority which do not want to disappear from the registry. I hope this will be solved soon) but succeeded very easily to register it as a service (marked as a skyservice - another little problem) It is extremely simple to do. Once registered, I tried several searches in the NVO as somebody looking for a simulation code of interstellar clouds would do. Each time, the NVO search system has been able to find it. So, even if there are some points to improve, as Ray said, the way the inscription in registries is done can be used for simulations with a web interface (webservices as well I guess). Best regards and see you in Victoria. Franck PS : For those who wonder, PDR codes are the codes which model the physics and the chemistry of interstellar clouds. PPS: If you try to access the code, you will be blocked by a login and password. This is because it gives access to computing facilities of the Observatory of Paris. We need a bit more computing power before opening completely the access to the codes. ------------------------------------ Franck Le Petit LUTH Observatoire de Meudon 5 Place Jules Janssen 92190 Meudon France Tel: (33) 1 45 07 75 66 ------------------------------------ Le 4 mai 06 à 20:14, Gerard Lemson a écrit : > Hi Ray > > We did indeed came to the conclusion that it should be possible to > register resources without there being a fitting standard > specification/protocol. I would actually like to try to register some > such theory specific services and datasets during the interop, as > there we > could benefit from interaction with registry connaiseurs such as you. > Would you be willing and to make a contribution to one of the theory > sessions on Monday to explain this in some more detail ? > > Cheers > Gerard > > On Thu, 4 May 2006, Ray Plante wrote: > >> Gentle Theorists, >> >> During a recent chat, Sebastien Derriere reported on a meeting of >> VOTheorists in which there was some discussion of how one should >> publish >> simulation data and/or services to the VO. I thought that I would >> mention >> a document I wrote for the NVO called "How to Publish to the >> NVO". It's >> meant to be a brief introduction to VO publishing with pointers to >> how to >> get started. It's a little out of date at the moment (an update >> is in the >> works), but it is not inaccurate. I would be interested to get some >> feedback from your group about how applicable you feel it is to >> theory-related resources. In particular, if you have suggestions for >> addressing the theory community, this would get a great time to >> get those. >> >> In the VO, we talk a lot about registering standard services like >> SIA and >> SkyNodes. However you may not be aware that it is currently >> possible to >> register general data collections and non-standard services, >> including >> those that have a web-page interface. While I'm sure that you will >> benefit from some standards that are specifically targetted to the >> theory >> community in the future, you may find the generic resource >> descriptions >> useful today. In fact, I would encourage you to visit the >> registry at >> NCSA (http://nvo.ncsa.uiuc.edu/nvoregistration.html) and try >> registering >> somethings. This site provides a sandbox version that allows you >> to try >> out the interface without actually publishing anything. >> >> Finally, to the Registry WG, it's been suggested that we take a >> look at >> this document and see if there is an IVOA version we might publish >> as a >> note. Your feedback is welcome as well. >> >> cheers, >> Ray >> >> > From owner-theory@eso.org Fri May 5 12:48:36 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k45AmSl7003406 for ; Fri, 5 May 2006 12:48:28 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k45AmR4n003405 for theory-outgoing; Fri, 5 May 2006 12:48:27 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k45AmRl7003399; Fri, 5 May 2006 12:48:27 +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 k45AmOr9004569; Fri, 5 May 2006 12:48:25 +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 <0IYS00AYUGOEWU@esa-av-smtp2.gmessaging.net>; Fri, 05 May 2006 12:48:14 +0200 (MEST) Received: from localhost (esa-spas2 [127.0.0.1]) by esa-spas2.gmessaging.net (Postfix) with ESMTP id 191E0219E46; Fri, 05 May 2006 12:48:14 +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 12477-05; Fri, 05 May 2006 12:48:12 +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 4EC9E219E59; Fri, 05 May 2006 12:48:12 +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 734E011F8EF; Fri, 05 May 2006 12:48:12 +0200 (CEST) Received: from isol11.vilspa.esa.int (IDENT:U2FsdGVkX18MOLaQx+/7dKNrSXypIzoD5XtzJzgOhE8@isol11.vilspa.esa.int [193.147.153.45]) by iso.vilspa.esa.es (8.12.10/8.12.10) with ESMTP id k45AmCl2024232; Fri, 05 May 2006 12:48:12 +0200 (MEST) Date: Fri, 05 May 2006 12:48:11 +0200 From: Jesus Salgado Subject: Re: tehoretical SEDs in VO applications To: theory@ivoa.net, apps@ivoa.net Cc: Jesus.Salgado@sciops.esa.int Message-id: <1146826091.4221.24.camel@isol11.vilspa.esa.int> MIME-version: 1.0 X-Mailer: Evolution 2.0.2 (2.0.2-27) Content-type: text/plain; charset=UTF-8 Content-transfer-encoding: 8BIT 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: 2.3.0.1, Antispam-Data: 2006.5.5.25104 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Jesus Salgado Dear Miguel, Just some comments about your applications benchmark. Units: ------ > 1. problem with units nomenclature: There is no recommendation about the use of units in the VOTable fields. In particular, > VOSpec and specview use different ways to define the units for the flux e.j. cm**2 vs. cm2 to define the $cm^2$ (in latex). > Would it be possible to define any recommendation about that? Otherwise the same VOTable would not be used for both > applications! As you probably know, VOSpec is not using the units string definition for the units handling but the scaleq and dimeq fields. We made the proposal to include this dimensional analysis data to prevent the problems of multiple unit string convections (among other things) You have read it in the SED document, (point 3.2 Units) http://hea-www.harvard.edu/~jcm/vo/docs/spec0.93.html The definition of the scaleq and dimeq syntax is (hopefully) uniform for all the services, following our recommendation. In any case, same VOTables are currently used for both applications, so it looks that the problem has been solved at application level (for us, using the dimensional analysis information instead of the unit strings, for others using aliases and string conversions) Metadata in VOTable ------------------- About the VOTable metadata issue, in our view, the information inside the VOTable response is to be used automatically by the client application (except for the VOTable editors). In case there is no implementation to use specific information in the VOTable response, there is a risk to lose it. VOSpec is taking the information for the row where the spectrum is described and it is shown to the user if the user double-click on one spectrum in the result tree. This should not be enough in the future, as any essential information included in the VOTable response should be protocolized in some way to be properly treated in the client (not only shown). If there is some information only to be shown to the user linked to one result, probably the best way to do it for the time being could be to include a link to a dynamically generated page (in a format readable by humans). About the columns for errors, this will be included in VOSpec quite soon for all the services that can provide them. The only constraint would be the order of the columns in the “columns†field. TSAP: ----- > d) A final comment, it looks that only VOSpec is able to manage a Theoretical spectral acces protocol: > It means, perform the query to a server that gives back a table with the parameter space covered by the > models that the server provides, and perform a "second" query over a subsample of the parameter space covered. This is not quite surprising as we were the ones to propose the theoretical spectral access protocol in the IVOA. As you probably know, we proposed the creation of this kind of server to the SVO coordinator (Enrique Solano) for the Kurucz models and we implemented the client part in VOSpec. Some other services were created later related to SVO and Mexican VO, and we have contacted some others to create similar services (as the ones from the French VO), so all the services have been created more or less under our coordination. We think it is a good first step to include theoretical SEDs in the VO, and easy to be implemented for SED VO applications. Best Regards, Jesus Salgado ESA-VO team e-mail: Jesus.Salgado@sciops.esa.int Tel + 34 91 8131271 European Space Agency/European Space Astronomy Centre VILLAFRANCA Satellites Tracking Station P.O. Box 50727 E-28080 Villafranca del Castillo MADRID - SPAIN From owner-apps@eso.org Fri May 5 12:48:52 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k45AmSl7003411 for ; Fri, 5 May 2006 12:48:28 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k45AmSqD003410 for apps-outgoing; Fri, 5 May 2006 12:48:28 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-apps@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 k45AmRl7003399; Fri, 5 May 2006 12:48:27 +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 k45AmOr9004569; Fri, 5 May 2006 12:48:25 +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 <0IYS00AYUGOEWU@esa-av-smtp2.gmessaging.net>; Fri, 05 May 2006 12:48:14 +0200 (MEST) Received: from localhost (esa-spas2 [127.0.0.1]) by esa-spas2.gmessaging.net (Postfix) with ESMTP id 191E0219E46; Fri, 05 May 2006 12:48:14 +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 12477-05; Fri, 05 May 2006 12:48:12 +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 4EC9E219E59; Fri, 05 May 2006 12:48:12 +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 734E011F8EF; Fri, 05 May 2006 12:48:12 +0200 (CEST) Received: from isol11.vilspa.esa.int (IDENT:U2FsdGVkX18MOLaQx+/7dKNrSXypIzoD5XtzJzgOhE8@isol11.vilspa.esa.int [193.147.153.45]) by iso.vilspa.esa.es (8.12.10/8.12.10) with ESMTP id k45AmCl2024232; Fri, 05 May 2006 12:48:12 +0200 (MEST) Date: Fri, 05 May 2006 12:48:11 +0200 From: Jesus Salgado Subject: Re: tehoretical SEDs in VO applications To: theory@ivoa.net, apps@ivoa.net Cc: Jesus.Salgado@sciops.esa.int Message-id: <1146826091.4221.24.camel@isol11.vilspa.esa.int> MIME-version: 1.0 X-Mailer: Evolution 2.0.2 (2.0.2-27) Content-type: text/plain; charset=UTF-8 Content-transfer-encoding: 8BIT 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: 2.3.0.1, Antispam-Data: 2006.5.5.25104 Sender: owner-apps@eso.org Precedence: bulk Reply-To: Jesus Salgado Dear Miguel, Just some comments about your applications benchmark. Units: ------ > 1. problem with units nomenclature: There is no recommendation about the use of units in the VOTable fields. In particular, > VOSpec and specview use different ways to define the units for the flux e.j. cm**2 vs. cm2 to define the $cm^2$ (in latex). > Would it be possible to define any recommendation about that? Otherwise the same VOTable would not be used for both > applications! As you probably know, VOSpec is not using the units string definition for the units handling but the scaleq and dimeq fields. We made the proposal to include this dimensional analysis data to prevent the problems of multiple unit string convections (among other things) You have read it in the SED document, (point 3.2 Units) http://hea-www.harvard.edu/~jcm/vo/docs/spec0.93.html The definition of the scaleq and dimeq syntax is (hopefully) uniform for all the services, following our recommendation. In any case, same VOTables are currently used for both applications, so it looks that the problem has been solved at application level (for us, using the dimensional analysis information instead of the unit strings, for others using aliases and string conversions) Metadata in VOTable ------------------- About the VOTable metadata issue, in our view, the information inside the VOTable response is to be used automatically by the client application (except for the VOTable editors). In case there is no implementation to use specific information in the VOTable response, there is a risk to lose it. VOSpec is taking the information for the row where the spectrum is described and it is shown to the user if the user double-click on one spectrum in the result tree. This should not be enough in the future, as any essential information included in the VOTable response should be protocolized in some way to be properly treated in the client (not only shown). If there is some information only to be shown to the user linked to one result, probably the best way to do it for the time being could be to include a link to a dynamically generated page (in a format readable by humans). About the columns for errors, this will be included in VOSpec quite soon for all the services that can provide them. The only constraint would be the order of the columns in the “columns†field. TSAP: ----- > d) A final comment, it looks that only VOSpec is able to manage a Theoretical spectral acces protocol: > It means, perform the query to a server that gives back a table with the parameter space covered by the > models that the server provides, and perform a "second" query over a subsample of the parameter space covered. This is not quite surprising as we were the ones to propose the theoretical spectral access protocol in the IVOA. As you probably know, we proposed the creation of this kind of server to the SVO coordinator (Enrique Solano) for the Kurucz models and we implemented the client part in VOSpec. Some other services were created later related to SVO and Mexican VO, and we have contacted some others to create similar services (as the ones from the French VO), so all the services have been created more or less under our coordination. We think it is a good first step to include theoretical SEDs in the VO, and easy to be implemented for SED VO applications. Best Regards, Jesus Salgado ESA-VO team e-mail: Jesus.Salgado@sciops.esa.int Tel + 34 91 8131271 European Space Agency/European Space Astronomy Centre VILLAFRANCA Satellites Tracking Station P.O. Box 50727 E-28080 Villafranca del Castillo MADRID - SPAIN From owner-apps@eso.org Fri May 5 15:38:29 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k45Dc9l7002586 for ; Fri, 5 May 2006 15:38:09 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k45Dc9x0002585 for apps-outgoing; Fri, 5 May 2006 15:38:09 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-apps@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 k45Dc8l7002575; Fri, 5 May 2006 15:38:08 +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 k45Dc6r9012178; Fri, 5 May 2006 15:38:07 +0200 (CEST) Received: from [161.111.165.119] (dae-d19.iaa.csic.es [161.111.165.119]) by iaa13u.iaa.csic.es (8.9.3/8.9.1) with ESMTP id PAA12183; Fri, 5 May 2006 15:38:00 +0200 (MET DST) In-Reply-To: <1146826091.4221.24.camel@isol11.vilspa.esa.int> References: <1146826091.4221.24.camel@isol11.vilspa.esa.int> Mime-Version: 1.0 (Apple Message framework v749.3) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: Cc: theory@ivoa.net, apps@ivoa.net Content-Transfer-Encoding: 7bit From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Re: tehoretical SEDs in VO applications Date: Fri, 5 May 2006 15:37:42 +0200 To: Jesus Salgado X-Mailer: Apple Mail (2.749.3) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.5.55109 Sender: owner-apps@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Thanks a lot Jesus, I completely agree with you points, but only for "increasing" the discussion: About metadata in the VO table, there is two particular issues specifically related with theory, and any analysis tool: Suppouse that you overplot real data and several theoretical models. And you obtain a good fit of a particular model. If the application is not able to show the model parameters (that should be included somewhere in the VOTable metadata), how can you recover them for, for example, a publication? I would agree that an link to a generated page would be fine, but it would only works for catalogs, and it would not work if the teoretical data is generated by the use of diferent aplications (example a virtual telescope machine). Since model parameters should be included in the VOtable, I think is more easy, and safer, that the applications would be able to show the information that is yet included in the VOTable they manage instead to refer to an external link. Additionally, an external link will make not possible to work with downloaded data without internet conexion.... (An specific comment about that is that the providers of synthesis models would not be very happy and may be will not join actively the VO iniciative if they do not obtain credits for the use of their models, and metadata is the only place where such a credit can be written explicitelly, including references to the models papers etc...) And about TSAP, yes, I know (I had been also working) it ;) However, most of VOtools applications are not designed to support a TSAP-like protocol: Obtain a parameter VOTable and process it before access the data.... Maybe is time that other applications also will think about this kind of implementation, isn't it? cheers miguel From owner-theory@eso.org Fri May 5 15:38:31 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k45Dc9l7002581 for ; Fri, 5 May 2006 15:38:09 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k45Dc99e002579 for theory-outgoing; Fri, 5 May 2006 15:38:09 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k45Dc8l7002575; Fri, 5 May 2006 15:38:08 +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 k45Dc6r9012178; Fri, 5 May 2006 15:38:07 +0200 (CEST) Received: from [161.111.165.119] (dae-d19.iaa.csic.es [161.111.165.119]) by iaa13u.iaa.csic.es (8.9.3/8.9.1) with ESMTP id PAA12183; Fri, 5 May 2006 15:38:00 +0200 (MET DST) In-Reply-To: <1146826091.4221.24.camel@isol11.vilspa.esa.int> References: <1146826091.4221.24.camel@isol11.vilspa.esa.int> Mime-Version: 1.0 (Apple Message framework v749.3) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: Cc: theory@ivoa.net, apps@ivoa.net Content-Transfer-Encoding: 7bit From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Re: tehoretical SEDs in VO applications Date: Fri, 5 May 2006 15:37:42 +0200 To: Jesus Salgado X-Mailer: Apple Mail (2.749.3) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.5.55109 Sender: owner-theory@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Thanks a lot Jesus, I completely agree with you points, but only for "increasing" the discussion: About metadata in the VO table, there is two particular issues specifically related with theory, and any analysis tool: Suppouse that you overplot real data and several theoretical models. And you obtain a good fit of a particular model. If the application is not able to show the model parameters (that should be included somewhere in the VOTable metadata), how can you recover them for, for example, a publication? I would agree that an link to a generated page would be fine, but it would only works for catalogs, and it would not work if the teoretical data is generated by the use of diferent aplications (example a virtual telescope machine). Since model parameters should be included in the VOtable, I think is more easy, and safer, that the applications would be able to show the information that is yet included in the VOTable they manage instead to refer to an external link. Additionally, an external link will make not possible to work with downloaded data without internet conexion.... (An specific comment about that is that the providers of synthesis models would not be very happy and may be will not join actively the VO iniciative if they do not obtain credits for the use of their models, and metadata is the only place where such a credit can be written explicitelly, including references to the models papers etc...) And about TSAP, yes, I know (I had been also working) it ;) However, most of VOtools applications are not designed to support a TSAP-like protocol: Obtain a parameter VOTable and process it before access the data.... Maybe is time that other applications also will think about this kind of implementation, isn't it? cheers miguel From owner-theory@eso.org Fri May 5 16:37:09 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k45Eb5l7013874 for ; Fri, 5 May 2006 16:37:05 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k45Eb5Pq013871 for theory-outgoing; Fri, 5 May 2006 16:37:05 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k45Eb4l7013866; Fri, 5 May 2006 16:37:04 +0200 (MEST) Received: from esa-av-smtp1.gmessaging.net (esa-av-smtp1.gmessaging.net [194.51.201.22]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k45Eb1r9015523; Fri, 5 May 2006 16:37:02 +0200 (CEST) Received: from esa-spas1.gmessaging.net (relay [172.24.21.38]) by esa-av-smtp1.gmessaging.net (iPlanet Messaging Server 5.2 Patch 2 (built Jul 14 2004)) with ESMTP id <0IYS00E4LR6JW4@esa-av-smtp1.gmessaging.net>; Fri, 05 May 2006 16:35:08 +0200 (MEST) Received: from localhost (localhost.localdomain [127.0.0.1]) by esa-spas1.gmessaging.net (Postfix) with ESMTP id 8382B229DAA; Fri, 05 May 2006 16:35:07 +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 27618-10; Fri, 05 May 2006 16:35:05 +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 AFAEE229DB5; Fri, 05 May 2006 16:35:05 +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 7C38F11F8EF; Fri, 05 May 2006 16:35:05 +0200 (CEST) Received: from isol11.vilspa.esa.int (IDENT:U2FsdGVkX18q+hkBPBFpguvGTDcw0IGMv5AmS3hoDLA@isol11.vilspa.esa.int [193.147.153.45]) by iso.vilspa.esa.es (8.12.10/8.12.10) with ESMTP id k45EZ5l2023816; Fri, 05 May 2006 16:35:05 +0200 (MEST) Date: Fri, 05 May 2006 16:35:04 +0200 From: Jesus Salgado Subject: Re: tehoretical SEDs in VO applications In-reply-to: To: Miguel =?ISO-8859-1?Q?Cervi=F1o?= Cc: Jesus.Salgado@sciops.esa.int, theory@ivoa.net, apps@ivoa.net Message-id: <1146839704.4221.66.camel@isol11.vilspa.esa.int> MIME-version: 1.0 X-Mailer: Evolution 2.0.2 (2.0.2-27) Content-type: text/plain; charset=utf-8 Content-transfer-encoding: 8BIT 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: <1146826091.4221.24.camel@isol11.vilspa.esa.int> X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.5.65105 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Jesus Salgado Hi Miguel, On Fri, 2006-05-05 at 15:37 +0200, Miguel Cerviño wrote: > Thanks a lot Jesus, > > I completely agree with you points, but > only for "increasing" the discussion: > > About metadata in the VO table, there is two particular issues > specifically related with theory, and any analysis tool: > Suppouse that you overplot real data and several theoretical models. > And you obtain a good fit of a particular model. If the application > is not able to show the > model parameters (that should be included somewhere in the VOTable > metadata), how > can you recover them for, for example, a publication? I would agree > that an > link to a generated page would be fine, but it would only works for > catalogs, > and it would not work if the teoretical data is generated by the use > of diferent > aplications (example a virtual telescope machine). Since model > parameters should > be included in the VOtable, I think is more easy, and safer, that the > applications > would be able to show the information that is yet included in the > VOTable > they manage instead to refer to an external link. Additionally, an > external link > will make not possible to work with downloaded data without internet > conexion.... > In this particular case, I would put the metadata to identify the spectrum inside the spectrum itself, e.g., inside the header in case of a fits or inside the votable spectrum in case of a votable spectrum. In this case, the file downloaded would be self-consistent and the model provider will be sure that all the information to properly "understand" the spectrum is there after saving the file. If I remember correctly, all the applications have a save function for the file itself, so this approach would work for all the VO applications. (in the case of VOSpec, clicking twice on one spectrum, a window appears with a Save button) Probably, there is room to more specific metadata in the VOTable response (in particular publications links should be understood better in the clients) but, except for the VOTable editors, many of the metadata will be ignored by the VO clients. On the other hand, and probably because of the same reason, the VO clients do not save the VOTable responses but only the data link files. There is a problem added to save VOTable responses. For the client, the result is a combination of several VOTables from different servers, so the only two ways that I see to save the metadata is either saving every single VOTable or to create a VOTable as a combination of several heterogeneous VOTables (really a mess if we want to maintain this result VOTable as something usable as input for future e.g. VOSpec sessions) > (An specific comment about that is that the providers of synthesis > models > would not be very happy and may be will not join actively the VO > iniciative if > they do not obtain credits for the use of their models, and metadata > is the > only place where such a credit can be written explicitelly, including > references to > the models papers etc...) > > And about TSAP, yes, I know (I had been also working) it ;) > However, most of VOtools applications are not designed to > support a TSAP-like protocol: Obtain a parameter VOTable and > process it before access the data.... Maybe is time that other > applications also will think about this kind of implementation, isn't > it? > I agree with you as the implementation of TSAP for a VO SED client application is quite easy and can be done for other applications. During the presentation in Kyoto, it was agreed to include TSAP as a particular case of SSAP. The only thing to be changed in the SSAP was to demote the position compulsory input to optional, as "position" is meaningless for most of the model servers. The call to the format=metadata was something standard to create specific queries to servers and it should be already implemented in the clients, but most of the VO applications create "blind" queries using only the compulsory parameters (what it represents a problem for the TSAP implementations) In any case, the creation of on-the-fly query forms using the format=metadata VOTables (or other more complex response in the future, in case of evolution) should not be a major problem. > cheers > > miguel > > Best Regards, -- Jesus J. Salgado ESA-VO team e-mail: Jesus.Salgado@sciops.esa.int Tel + 34 91 8131271 European Space Agency/European Space Astronomy Centre VILLAFRANCA Satellites Tracking Station P.O. Box 50727 E-28080 Villafranca del Castillo MADRID - SPAIN From owner-apps@eso.org Fri May 5 16:37:19 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k45Eb5l7013880 for ; Fri, 5 May 2006 16:37:05 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k45Eb5n4013878 for apps-outgoing; Fri, 5 May 2006 16:37:05 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-apps@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 k45Eb4l7013866; Fri, 5 May 2006 16:37:04 +0200 (MEST) Received: from esa-av-smtp1.gmessaging.net (esa-av-smtp1.gmessaging.net [194.51.201.22]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k45Eb1r9015523; Fri, 5 May 2006 16:37:02 +0200 (CEST) Received: from esa-spas1.gmessaging.net (relay [172.24.21.38]) by esa-av-smtp1.gmessaging.net (iPlanet Messaging Server 5.2 Patch 2 (built Jul 14 2004)) with ESMTP id <0IYS00E4LR6JW4@esa-av-smtp1.gmessaging.net>; Fri, 05 May 2006 16:35:08 +0200 (MEST) Received: from localhost (localhost.localdomain [127.0.0.1]) by esa-spas1.gmessaging.net (Postfix) with ESMTP id 8382B229DAA; Fri, 05 May 2006 16:35:07 +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 27618-10; Fri, 05 May 2006 16:35:05 +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 AFAEE229DB5; Fri, 05 May 2006 16:35:05 +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 7C38F11F8EF; Fri, 05 May 2006 16:35:05 +0200 (CEST) Received: from isol11.vilspa.esa.int (IDENT:U2FsdGVkX18q+hkBPBFpguvGTDcw0IGMv5AmS3hoDLA@isol11.vilspa.esa.int [193.147.153.45]) by iso.vilspa.esa.es (8.12.10/8.12.10) with ESMTP id k45EZ5l2023816; Fri, 05 May 2006 16:35:05 +0200 (MEST) Date: Fri, 05 May 2006 16:35:04 +0200 From: Jesus Salgado Subject: Re: tehoretical SEDs in VO applications In-reply-to: To: Miguel =?ISO-8859-1?Q?Cervi=F1o?= Cc: Jesus.Salgado@sciops.esa.int, theory@ivoa.net, apps@ivoa.net Message-id: <1146839704.4221.66.camel@isol11.vilspa.esa.int> MIME-version: 1.0 X-Mailer: Evolution 2.0.2 (2.0.2-27) Content-type: text/plain; charset=utf-8 Content-transfer-encoding: 8BIT 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: <1146826091.4221.24.camel@isol11.vilspa.esa.int> X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.5.65105 Sender: owner-apps@eso.org Precedence: bulk Reply-To: Jesus Salgado Hi Miguel, On Fri, 2006-05-05 at 15:37 +0200, Miguel Cerviño wrote: > Thanks a lot Jesus, > > I completely agree with you points, but > only for "increasing" the discussion: > > About metadata in the VO table, there is two particular issues > specifically related with theory, and any analysis tool: > Suppouse that you overplot real data and several theoretical models. > And you obtain a good fit of a particular model. If the application > is not able to show the > model parameters (that should be included somewhere in the VOTable > metadata), how > can you recover them for, for example, a publication? I would agree > that an > link to a generated page would be fine, but it would only works for > catalogs, > and it would not work if the teoretical data is generated by the use > of diferent > aplications (example a virtual telescope machine). Since model > parameters should > be included in the VOtable, I think is more easy, and safer, that the > applications > would be able to show the information that is yet included in the > VOTable > they manage instead to refer to an external link. Additionally, an > external link > will make not possible to work with downloaded data without internet > conexion.... > In this particular case, I would put the metadata to identify the spectrum inside the spectrum itself, e.g., inside the header in case of a fits or inside the votable spectrum in case of a votable spectrum. In this case, the file downloaded would be self-consistent and the model provider will be sure that all the information to properly "understand" the spectrum is there after saving the file. If I remember correctly, all the applications have a save function for the file itself, so this approach would work for all the VO applications. (in the case of VOSpec, clicking twice on one spectrum, a window appears with a Save button) Probably, there is room to more specific metadata in the VOTable response (in particular publications links should be understood better in the clients) but, except for the VOTable editors, many of the metadata will be ignored by the VO clients. On the other hand, and probably because of the same reason, the VO clients do not save the VOTable responses but only the data link files. There is a problem added to save VOTable responses. For the client, the result is a combination of several VOTables from different servers, so the only two ways that I see to save the metadata is either saving every single VOTable or to create a VOTable as a combination of several heterogeneous VOTables (really a mess if we want to maintain this result VOTable as something usable as input for future e.g. VOSpec sessions) > (An specific comment about that is that the providers of synthesis > models > would not be very happy and may be will not join actively the VO > iniciative if > they do not obtain credits for the use of their models, and metadata > is the > only place where such a credit can be written explicitelly, including > references to > the models papers etc...) > > And about TSAP, yes, I know (I had been also working) it ;) > However, most of VOtools applications are not designed to > support a TSAP-like protocol: Obtain a parameter VOTable and > process it before access the data.... Maybe is time that other > applications also will think about this kind of implementation, isn't > it? > I agree with you as the implementation of TSAP for a VO SED client application is quite easy and can be done for other applications. During the presentation in Kyoto, it was agreed to include TSAP as a particular case of SSAP. The only thing to be changed in the SSAP was to demote the position compulsory input to optional, as "position" is meaningless for most of the model servers. The call to the format=metadata was something standard to create specific queries to servers and it should be already implemented in the clients, but most of the VO applications create "blind" queries using only the compulsory parameters (what it represents a problem for the TSAP implementations) In any case, the creation of on-the-fly query forms using the format=metadata VOTables (or other more complex response in the future, in case of evolution) should not be a major problem. > cheers > > miguel > > Best Regards, -- Jesus J. Salgado ESA-VO team e-mail: Jesus.Salgado@sciops.esa.int Tel + 34 91 8131271 European Space Agency/European Space Astronomy Centre VILLAFRANCA Satellites Tracking Station P.O. Box 50727 E-28080 Villafranca del Castillo MADRID - SPAIN From owner-theory@eso.org Wed May 10 05:24:16 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k4A3O35K021015 for ; Wed, 10 May 2006 05:24:03 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k4A3O3VI021014 for theory-outgoing; Wed, 10 May 2006 05:24:03 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k4A3O25K021008 for ; Wed, 10 May 2006 05:24:02 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k4A3O1xF017077 for ; Wed, 10 May 2006 05:24:01 +0200 (CEST) Received: from localhost (glemson@localhost) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with ESMTP id FAA15501 for ; Wed, 10 May 2006 05:23:55 +0200 (METDST) X-Authentication-Warning: mpehp1.mpe-garching.mpg.de: glemson owned process doing -bs Date: Wed, 10 May 2006 05:23:55 +0200 (METDST) From: Gerard Lemson X-Sender: glemson@mpehp1.mpe-garching.mpg.de To: theory@ivoa.net Subject: agenda 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: 2.3.0.1, Antispam-Data: 2006.5.9.193116 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Gerard Lemson Dear collegues The current agenda for the theory sessions is posted on the meeting's theory site, http://www.ivoa.net/twiki/bin/view/IVOA/InterOpMay2006Theory. It is not final as I am still waiting for some replies to requests. But please let me know any questions you have already. Note that I am currently already in Victoria, thus 9 hours out of synch with Middle-European time. Regards Gerard From owner-theory@eso.org Mon May 15 07:47:37 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k4F5lRb7001691 for ; Mon, 15 May 2006 07:47:27 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k4F5lRr6001690 for theory-outgoing; Mon, 15 May 2006 07:47:27 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k4F5lQb7001681; Mon, 15 May 2006 07:47:26 +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 k4F5lMQk027850; Mon, 15 May 2006 07:47:23 +0200 (CEST) Received: from localhost (localhost.localdomain [127.0.0.1]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP id 9030BC7475; Mon, 15 May 2006 07:47:14 +0200 (CEST) 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 11617-10; Mon, 15 May 2006 07:47:14 +0200 (CEST) Received: from localhost (unknown [10.1.0.18]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP; Mon, 15 May 2006 07:47:14 +0200 (CEST) Received: from 204.50.11.162 ([204.50.11.162]) by webmail.sic.rm.cnr.it (Horde MIME library) with HTTP; Mon, 15 May 2006 08:48:36 +0200 Message-ID: <20060515084836.7xzmd39g4gk0c8ww@webmail.sic.rm.cnr.it> Date: Mon, 15 May 2006 08:48:36 +0200 From: Andrea Preite Martinez To: Laurie Shaw Cc: Gerard Lemson , Nicholas Walton , ucd@ivoa.net, theory@ivoa.net Subject: Re: UCD's for simulations References: In-Reply-To: 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 (4.1.1) X-Virus-Scanned: amavisd-new at sic.rm.cnr.it X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.14.213115 Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id k4F5lRb7001682 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Andrea Preite Martinez Dear Laurie, I've been collecting various proposal for upgrading the list of UCD-words, and I'll present these proposal for discussion (including yours) during the UCD/Semantic session (thu 18, 9.00-10.30). The list of proposed modifications and the agenda can be found at http://ivoa.net/twiki/bin/view/IVOA/InterOpMay2006UCD Regards, 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 :+39.339.38.17.355 =================================================================================== Quoting Laurie Shaw : > > Dear All, > > I've recently been experimenting with assigning UCDs to the results of > some cosmological simulations -- specifically to catalogues of dark > matter halos and their associated subhalos. In general, i've found > that the existing UCD tree is able to describe most of the properties of > these objects that are typically analysed in the literature, albeit with a > few exceptions. > > However, it is not currently possible to describe the properties and > parameters of the simulations themselves. This includes some input > physical parameters (i.e. cosmological parameters) that define the > theoretical context of the simulation, and technical > parameters that define its size,scope and resolution (e.g number of > particles, length of simulation box side, gravitational > softening length, time/redshift of a simulation output). > > Therefore, for the latter, I propose a new branch of the UCD tree to > encompass computatational techniques in astronomy: 'comp'. This > branch can be used to describe both astrophysical (and cosmological) > simulations, and data reduction and post-processing algorithms for > both simulation and observational data. It is roughly a computing > analogue of the 'instr' branch. For the case of simulations I propose > the following sub-branches > > comp.sim (computational simulation) > comp.sim.nbody (Nbody simulation) > comp.sim.sph (Smoothed Particle Hydrodynamics simulation) > comp.sim.boxside (Simulation box) > comp.sim.gravsoft (gravitational softening) > comp.sim.particles (simulation particles (for Nbody and SPH > simulations)) > comp.sim.snapshot (output of a simulation box at a particular > instant) > comp.sim.grid (simulation grid (for hydro simulations)) > > The number of particles in the simulation box, number of grid points, > particle mass, gravitational softening length and simulation box side > length would therefore be: > > meta.num;comp.sim.particles > meta.num;comp.sim.grid > phys.mass;comp.sim.particles > phys.size;comp.sim.gravsoft > phys.size;comp.sim.boxside > > (For the last two, introduction of a phys.size.length UCD might provide a > more accurate description.) > > The mass of an object in terms of the number of particles it contains: > > phys.mass;meta.num;comp.sim.particles > > Other possible sub-branches could be > > comp.resourse (computational resources used in simulation/data > processing) > comp.resource.processors (processors used) > comp.resource.memory (total size of a data file) > > plus those that are more specific to data-reduction/post-processing of > observational data. Algorithms that might apply to both simulated and > observed data (e.g. smoothing of images or particle densities) would > be listed directly under the comp branch: > > phys.size;comp.smooth > (or, with the introduction of a phys.size.length UCD: > phys.size.length;comp.smooth) > > Physical Parameters > --------------------- > Currently, there exists no UCDs for the main cosmological > parameters. In terms of simulations, it is very important to be able > define the assumed cosmology, when interpreting the results. To > describe these parameters I propose a 'cosmology' sub-branch of > the phys branch. So, > > phys.cosmology (cosmology) > phys.cosmology.omega (matter/energy density of universe) > phys.cosmology.hubble (hubble constant) > phys.cosmology.sigma8 (Normalisation of matter power-spectrum) > > and also: > > phys.matter.dark (dark matter tag) > phys.matter.baryon (baryonic matter tag) > phys.DarkEnergy (dark energy tag) > > So, Omega_Lambda, Omega_DM, Omega_baryon would be > > phys.cosmology.omega;phys.DarkEnery, > phys.cosmology.omega;phys.matter.dark > phys.comsology.omega;phys.matter.baryonic > > Now we can also describe the number of dark matter (gas particles) in > an SPH simulation, or a simulated object (star/galaxy/halo) using: > > meta.num;comp.sim.particles;phys.matter.dark(/baryonic) > > Furthermore, the mass and radius of dark matter halos in cosmological > simulations are frequently defined in terms of a virial > overdensity. Hence a phys.virial UCD would be usefull in specifying > what is meant by the mass and radius of a halo: > > phys.mass;phys.virial (virial mass) > phys.size.radius;phys.virial (virial radius) > > Time in Simulations > ------------------ > People frequently analyse the output of simulations, or snapshots, at > a series of different timesteps. This is often quoted in terms of the > redshift of > the snapshot. At the moment, redshift exists under the 'src' > branch. Maybe it might be better under the `phys' branch as it is a > measure of both distance and time, and can therefore be used to label > both the distance of observed objects and to label a time-stamp for > simulation snapshots: > > phys.redshift;comp.sim.snapshot > > Astrophysical Objects > -------------------- > Another problem is the listing of astronomical objects types under the > 'src' branch. This introduces confusion when trying to describe a > simulated astrophysical object. For example, the first word in > src.class.galaxy;comp.sim (simulated galaxy) implies that this is an > observed astrophysical source, the second that it is simulated. > > Additionally, objects such as halos and subhalos are not typically > observed (though i guess people do make estimates of their mass/size > through > gravitational lensing). It seems strange to have halo and subhalo > listed under the src.class sub-branch. I therefore suggest that an > object branch be introduced in which astrophysical (and theoretical) > objects can be listed (as also proposed by others on the UCD suggestion > page): > > object.galaxy;comp.sim (a simulated galaxy) > object.galaxy.spiral;comp.sim (a simulated spiral galaxy) > > One example that I encountered of an actual quantity where this was > useful is describing the mass in substructure, or the number of > subhalos, in a simulated halo: > > phys.mass;object.DMhalo.subhalo > meta.num;onject.DMhalo.subhalo > > It would be great to hear everyones thoughts, or ideas for alternative > approaches, for all these. > > Cheers, > > Laurie > > > List of Proposed UCDs > --------------------- > comp (computational astronomy) > comp.sim (simulations) > comp.sim.nbody (Nbody simulation) > comp.sim.sph (Smoothed Particle Hydrodynamics simulation) > comp.sim.boxside (Simulation box) > comp.sim.gravsoft (gravitational softening) > comp.sim.particles (simulation particles (for Nbody and SPH simulations)) > comp.sim.snapshot (output of a simulation box at a particular instant) > comp.sim.grid (simulation grid (for hydro simulations)) > comp.resourse (to describe computational resources used in simulation/data > processing) > comp.resource.processors (processors used) > comp.resource.memory (total size on disk of data) > (comp.dataReduct ? > comp.algorithm (general algorithms applied to sim/obs data) ) > > phys.cosmology > phys.cosmology.omega (matter/energy density of universe) > phys.cosmology.hubble (hubble constant) > phys.cosmology.sigma8 (Normalisation of matter power-spectrum) > phys.matter.dark (dark matter tag) > phys.matter.baryon (baryonic matter tag) > phys.DarkEnergy (dark energy tag) > phys.virial > phys.size.length > > object (astophysical object) > object.planet (planet) > object.satellite > object.star (star) > object.galaxy (galaxy) > object.DMhalo (DM halo) > Object.DMhalo.subhalo (DM subhalo) > etc > > > From owner-ucd@eso.org Mon May 15 07:47:39 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k4F5lRb7001686 for ; Mon, 15 May 2006 07:47:27 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k4F5lR7R001685 for ucd-outgoing; Mon, 15 May 2006 07:47:27 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-ucd@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k4F5lQb7001681; Mon, 15 May 2006 07:47:26 +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 k4F5lMQk027850; Mon, 15 May 2006 07:47:23 +0200 (CEST) Received: from localhost (localhost.localdomain [127.0.0.1]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP id 9030BC7475; Mon, 15 May 2006 07:47:14 +0200 (CEST) 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 11617-10; Mon, 15 May 2006 07:47:14 +0200 (CEST) Received: from localhost (unknown [10.1.0.18]) by smtp1.sic.rm.cnr.it (Postfix) with ESMTP; Mon, 15 May 2006 07:47:14 +0200 (CEST) Received: from 204.50.11.162 ([204.50.11.162]) by webmail.sic.rm.cnr.it (Horde MIME library) with HTTP; Mon, 15 May 2006 08:48:36 +0200 Message-ID: <20060515084836.7xzmd39g4gk0c8ww@webmail.sic.rm.cnr.it> Date: Mon, 15 May 2006 08:48:36 +0200 From: Andrea Preite Martinez To: Laurie Shaw Cc: Gerard Lemson , Nicholas Walton , ucd@ivoa.net, theory@ivoa.net Subject: Re: UCD's for simulations References: In-Reply-To: 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 (4.1.1) X-Virus-Scanned: amavisd-new at sic.rm.cnr.it X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.14.213115 Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id k4F5lRb7001682 Sender: owner-ucd@eso.org Precedence: bulk Reply-To: Andrea Preite Martinez Dear Laurie, I've been collecting various proposal for upgrading the list of UCD-words, and I'll present these proposal for discussion (including yours) during the UCD/Semantic session (thu 18, 9.00-10.30). The list of proposed modifications and the agenda can be found at http://ivoa.net/twiki/bin/view/IVOA/InterOpMay2006UCD Regards, 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 :+39.339.38.17.355 =================================================================================== Quoting Laurie Shaw : > > Dear All, > > I've recently been experimenting with assigning UCDs to the results of > some cosmological simulations -- specifically to catalogues of dark > matter halos and their associated subhalos. In general, i've found > that the existing UCD tree is able to describe most of the properties of > these objects that are typically analysed in the literature, albeit with a > few exceptions. > > However, it is not currently possible to describe the properties and > parameters of the simulations themselves. This includes some input > physical parameters (i.e. cosmological parameters) that define the > theoretical context of the simulation, and technical > parameters that define its size,scope and resolution (e.g number of > particles, length of simulation box side, gravitational > softening length, time/redshift of a simulation output). > > Therefore, for the latter, I propose a new branch of the UCD tree to > encompass computatational techniques in astronomy: 'comp'. This > branch can be used to describe both astrophysical (and cosmological) > simulations, and data reduction and post-processing algorithms for > both simulation and observational data. It is roughly a computing > analogue of the 'instr' branch. For the case of simulations I propose > the following sub-branches > > comp.sim (computational simulation) > comp.sim.nbody (Nbody simulation) > comp.sim.sph (Smoothed Particle Hydrodynamics simulation) > comp.sim.boxside (Simulation box) > comp.sim.gravsoft (gravitational softening) > comp.sim.particles (simulation particles (for Nbody and SPH > simulations)) > comp.sim.snapshot (output of a simulation box at a particular > instant) > comp.sim.grid (simulation grid (for hydro simulations)) > > The number of particles in the simulation box, number of grid points, > particle mass, gravitational softening length and simulation box side > length would therefore be: > > meta.num;comp.sim.particles > meta.num;comp.sim.grid > phys.mass;comp.sim.particles > phys.size;comp.sim.gravsoft > phys.size;comp.sim.boxside > > (For the last two, introduction of a phys.size.length UCD might provide a > more accurate description.) > > The mass of an object in terms of the number of particles it contains: > > phys.mass;meta.num;comp.sim.particles > > Other possible sub-branches could be > > comp.resourse (computational resources used in simulation/data > processing) > comp.resource.processors (processors used) > comp.resource.memory (total size of a data file) > > plus those that are more specific to data-reduction/post-processing of > observational data. Algorithms that might apply to both simulated and > observed data (e.g. smoothing of images or particle densities) would > be listed directly under the comp branch: > > phys.size;comp.smooth > (or, with the introduction of a phys.size.length UCD: > phys.size.length;comp.smooth) > > Physical Parameters > --------------------- > Currently, there exists no UCDs for the main cosmological > parameters. In terms of simulations, it is very important to be able > define the assumed cosmology, when interpreting the results. To > describe these parameters I propose a 'cosmology' sub-branch of > the phys branch. So, > > phys.cosmology (cosmology) > phys.cosmology.omega (matter/energy density of universe) > phys.cosmology.hubble (hubble constant) > phys.cosmology.sigma8 (Normalisation of matter power-spectrum) > > and also: > > phys.matter.dark (dark matter tag) > phys.matter.baryon (baryonic matter tag) > phys.DarkEnergy (dark energy tag) > > So, Omega_Lambda, Omega_DM, Omega_baryon would be > > phys.cosmology.omega;phys.DarkEnery, > phys.cosmology.omega;phys.matter.dark > phys.comsology.omega;phys.matter.baryonic > > Now we can also describe the number of dark matter (gas particles) in > an SPH simulation, or a simulated object (star/galaxy/halo) using: > > meta.num;comp.sim.particles;phys.matter.dark(/baryonic) > > Furthermore, the mass and radius of dark matter halos in cosmological > simulations are frequently defined in terms of a virial > overdensity. Hence a phys.virial UCD would be usefull in specifying > what is meant by the mass and radius of a halo: > > phys.mass;phys.virial (virial mass) > phys.size.radius;phys.virial (virial radius) > > Time in Simulations > ------------------ > People frequently analyse the output of simulations, or snapshots, at > a series of different timesteps. This is often quoted in terms of the > redshift of > the snapshot. At the moment, redshift exists under the 'src' > branch. Maybe it might be better under the `phys' branch as it is a > measure of both distance and time, and can therefore be used to label > both the distance of observed objects and to label a time-stamp for > simulation snapshots: > > phys.redshift;comp.sim.snapshot > > Astrophysical Objects > -------------------- > Another problem is the listing of astronomical objects types under the > 'src' branch. This introduces confusion when trying to describe a > simulated astrophysical object. For example, the first word in > src.class.galaxy;comp.sim (simulated galaxy) implies that this is an > observed astrophysical source, the second that it is simulated. > > Additionally, objects such as halos and subhalos are not typically > observed (though i guess people do make estimates of their mass/size > through > gravitational lensing). It seems strange to have halo and subhalo > listed under the src.class sub-branch. I therefore suggest that an > object branch be introduced in which astrophysical (and theoretical) > objects can be listed (as also proposed by others on the UCD suggestion > page): > > object.galaxy;comp.sim (a simulated galaxy) > object.galaxy.spiral;comp.sim (a simulated spiral galaxy) > > One example that I encountered of an actual quantity where this was > useful is describing the mass in substructure, or the number of > subhalos, in a simulated halo: > > phys.mass;object.DMhalo.subhalo > meta.num;onject.DMhalo.subhalo > > It would be great to hear everyones thoughts, or ideas for alternative > approaches, for all these. > > Cheers, > > Laurie > > > List of Proposed UCDs > --------------------- > comp (computational astronomy) > comp.sim (simulations) > comp.sim.nbody (Nbody simulation) > comp.sim.sph (Smoothed Particle Hydrodynamics simulation) > comp.sim.boxside (Simulation box) > comp.sim.gravsoft (gravitational softening) > comp.sim.particles (simulation particles (for Nbody and SPH simulations)) > comp.sim.snapshot (output of a simulation box at a particular instant) > comp.sim.grid (simulation grid (for hydro simulations)) > comp.resourse (to describe computational resources used in simulation/data > processing) > comp.resource.processors (processors used) > comp.resource.memory (total size on disk of data) > (comp.dataReduct ? > comp.algorithm (general algorithms applied to sim/obs data) ) > > phys.cosmology > phys.cosmology.omega (matter/energy density of universe) > phys.cosmology.hubble (hubble constant) > phys.cosmology.sigma8 (Normalisation of matter power-spectrum) > phys.matter.dark (dark matter tag) > phys.matter.baryon (baryonic matter tag) > phys.DarkEnergy (dark energy tag) > phys.virial > phys.size.length > > object (astophysical object) > object.planet (planet) > object.satellite > object.star (star) > object.galaxy (galaxy) > object.DMhalo (DM halo) > Object.DMhalo.subhalo (DM subhalo) > etc > > > From owner-theory@eso.org Tue May 16 18:29:38 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k4GGTVQ8014209 for ; Tue, 16 May 2006 18:29:31 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k4GGTV8V014208 for theory-outgoing; Tue, 16 May 2006 18:29:31 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k4GGTUQ8014203 for ; Tue, 16 May 2006 18:29:30 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k4GGTSQk004549 for ; Tue, 16 May 2006 18:29:29 +0200 (CEST) Received: from localhost (glemson@localhost) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with ESMTP id SAA15316 for ; Tue, 16 May 2006 18:29:23 +0200 (METDST) X-Authentication-Warning: mpehp1.mpe-garching.mpg.de: glemson owned process doing -bs Date: Tue, 16 May 2006 18:29:21 +0200 (METDST) From: Gerard Lemson X-Sender: glemson@mpehp1.mpe-garching.mpg.de To: theory@ivoa.net Subject: theory sessions 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: 2.3.0.1, Antispam-Data: 2006.5.16.85111 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Gerard Lemson Dear all In the first theory sessions we decided that the following subjects deserve more detailed attention during this Interop: data formats, UCDs,metadata and SNAP. On the meeting's TWiki page (http://www.ivoa.net/twiki/bin/view/IVOA/InterOpMay2006Theory I have added some structure to these proposals. Please mail me if you would like to contribute to one of these discussions and when you would have time to do so wrt the other sessions going on. If possible I would like to start this afternoon. Cheers Gerard From owner-theory@eso.org Tue May 16 20:30:23 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k4GIUIQ8002155 for ; Tue, 16 May 2006 20:30:18 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k4GIUIXA002154 for theory-outgoing; Tue, 16 May 2006 20:30:18 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k4GIUFQ8002145; Tue, 16 May 2006 20:30:15 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k4GIUEsR004671; Tue, 16 May 2006 20:30:14 +0200 (CEST) Received: from localhost (glemson@localhost) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with ESMTP id UAA19966; Tue, 16 May 2006 20:30:08 +0200 (METDST) X-Authentication-Warning: mpehp1.mpe-garching.mpg.de: glemson owned process doing -bs Date: Tue, 16 May 2006 20:30:08 +0200 (METDST) From: Gerard Lemson X-Sender: glemson@mpehp1.mpe-garching.mpg.de To: theory@ivoa.net cc: flepetit@mesiog.obspm.fr, herve.wozniak@obs.univ-lyon1.fr, c.gheller@cineca.it, ndelmott@eso.org, deyoung-at-noao.edu@xray.mpe.mpg.de, andrea.preitemartinez@iasf-roma.inaf.it, gerard.lemson@mpe.mpg.de Subject: theory UCD session 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: 2.3.0.1, Antispam-Data: 2006.5.16.103106 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Gerard Lemson Dear collegues Taking into account replies to the email I suggest we meet this afternoon after lunch, 2PM to discuss the UCDs for theory. Andrea, If you can not make this I will report to you later. Cheers Gerard PS I will mail about a location later. From owner-theory@eso.org Tue May 16 20:58:02 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k4GIvvQ8006148 for ; Tue, 16 May 2006 20:57:57 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k4GIvvTW006147 for theory-outgoing; Tue, 16 May 2006 20:57:57 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k4GIvuQ8006141; Tue, 16 May 2006 20:57:56 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k4GIvssR005953; Tue, 16 May 2006 20:57:55 +0200 (CEST) Received: from localhost (glemson@localhost) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with ESMTP id UAA20914; Tue, 16 May 2006 20:57:49 +0200 (METDST) X-Authentication-Warning: mpehp1.mpe-garching.mpg.de: glemson owned process doing -bs Date: Tue, 16 May 2006 20:57:48 +0200 (METDST) From: Gerard Lemson X-Sender: glemson@mpehp1.mpe-garching.mpg.de To: theory@ivoa.net cc: flepetit@mesiog.obspm.fr, herve.wozniak@obs.univ-lyon1.fr, c.gheller@cineca.it, ndelmott@eso.org, deyoung-at-noao.edu@xray.mpe.mpg.de, andrea.preitemartinez@iasf-roma.inaf.it, gerard.lemson@mpe.mpg.de Subject: Re: theory UCD session In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.16.105108 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Gerard Lemson The meeting will be in Boardroom B, up the stairs at the back of the main meeting rooms. We will start discussing UCDs, but hopefully we can deal with other issues as well, for example a discussion how to approach the question of data formats, which may not need too much time. Gerard On Tue, 16 May 2006, Gerard Lemson wrote: > Dear collegues > Taking into account replies to the email I suggest we meet this afternoon > after lunch, 2PM to discuss the UCDs for theory. > Andrea, If you can not make this I will report to you later. > Cheers > Gerard > PS > I will mail about a location later. > From owner-theory@eso.org Wed May 17 01:51:23 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k4GNpFWr012772 for ; Wed, 17 May 2006 01:51:15 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k4GNpFVW012771 for theory-outgoing; Wed, 17 May 2006 01:51:15 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k4GNpEWr012766; Wed, 17 May 2006 01:51:14 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k4GNpCsR020571; Wed, 17 May 2006 01:51:13 +0200 (CEST) Received: from localhost (glemson@localhost) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with ESMTP id BAA00339; Wed, 17 May 2006 01:51:07 +0200 (METDST) X-Authentication-Warning: mpehp1.mpe-garching.mpg.de: glemson owned process doing -bs Date: Wed, 17 May 2006 01:51:06 +0200 (METDST) From: Gerard Lemson X-Sender: glemson@mpehp1.mpe-garching.mpg.de To: theory@ivoa.net cc: flepetit@mesiog.obspm.fr, herve.wozniak@obs.univ-lyon1.fr, c.gheller@cineca.it, ndelmott@eso.org, deyoung-at-noao.edu@xray.mpe.mpg.de, andrea.preitemartinez@iasf-roma.inaf.it, gerard.lemson@mpe.mpg.de Subject: Re: theory UCD session In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.16.155107 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Gerard Lemson Dear collegues Today the Cc:-s above met for a discussion about concepts that we need to describe simulations. It started based on the email by Laurie Shaw with a proposal for new UCDs. We realised that whereas some of the proposals were properties, others were values. The former might be used to construct a UCD, the latter to words in a/the standard vocabulary. We decided that we first wanted to create a more comprehensive list of these concepts, and only afterwards subdivide them into their apropriate class, after weeding out concepts already existing in UCD list and/or vocabulary. To this end the first attempt is posted on the Twik pages, http://www.ivoa.net/twiki/bin/view/IVOA/TheorySemanticVocabulary. Please add concepts and possible values. It may be somewhat cryptic at the moment, this should improve. The result will be discussed Thursday morning, first in UCD session I, then in theory session III. Regards Gerard From owner-theory@eso.org Wed May 17 17:00:48 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k4HExKCb012942 for ; Wed, 17 May 2006 16:59:20 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k4HExK3i012941 for theory-outgoing; Wed, 17 May 2006 16:59:20 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k4HExJCb012933; Wed, 17 May 2006 16:59:19 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k4HExDQk002815; Wed, 17 May 2006 16:59:13 +0200 (CEST) Received: from localhost (glemson@localhost) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with ESMTP id QAA09952; Wed, 17 May 2006 16:59:05 +0200 (METDST) X-Authentication-Warning: mpehp1.mpe-garching.mpg.de: glemson owned process doing -bs Date: Wed, 17 May 2006 16:59:02 +0200 (METDST) From: Gerard Lemson X-Sender: glemson@mpehp1.mpe-garching.mpg.de To: theory@ivoa.net cc: flepetit@mesiog.obspm.fr, francois@vizir.u-strasbg.fr, m.b.taylor@bristol.ac.uk, herve.wozniak@obs.univ-lyon1.fr, c.gheller@cineca.it, ndelmott@eso.org, deyoung-at-noao.edu@xray.mpe.mpg.de, andrea.preitemartinez@iasf-roma.inaf.it, gerard.lemson@mpe.mpg.de Subject: theory data formats and SNAP session In-Reply-To: Message-ID: MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.17.65111 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Gerard Lemson Dear Collegues As discussed earlier, today we will continue our discussions. We'd like to talk about data formats and SNAP in particular. As the exec meeting is actually planned to last until 15:30, and takes up the Boardroom B where we'd be meeting, lets plan to meet at 16:00 there after all. Regards Gerard From owner-theory@eso.org Thu May 18 10:28:08 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k4I8S0KG001013 for ; Thu, 18 May 2006 10:28:00 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k4I8S0XW001012 for theory-outgoing; Thu, 18 May 2006 10:28:00 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k4I8RxKG001008 for ; Thu, 18 May 2006 10:27:59 +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 k4I8RvQk003752 for ; Thu, 18 May 2006 10:27:58 +0200 (CEST) Received: from [161.111.165.116] (dae-d16.iaa.csic.es [161.111.165.116]) by iaa13u.iaa.csic.es (8.9.3/8.9.1) with ESMTP id KAA16563 for ; Thu, 18 May 2006 10:27:51 +0200 (MET DST) Mime-Version: 1.0 (Apple Message framework v749.3) Content-Transfer-Encoding: 7bit Message-Id: <523EFBF4-4FE2-4296-8103-F9F2C086F94D@iaa.es> Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed To: theory@ivoa.net From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: FoV in Aladin and Virtual Telescopes Date: Thu, 18 May 2006 10:27:48 +0200 X-Mailer: Apple Mail (2.749.3) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.18.3108 Sender: owner-theory@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Dear all, I am not in Victoria but I am following the session in the wiki pages. I just see that Aladin provides now an implementation of any FoV, that is described in a xml file (at least it is in the abstract). I just realized that maybe it would be quite useful for future virtual telescope developments, but it would need: - the xml file with the FoV would be a VOTable - there would be a "repository" or registry of FoV (may be provided by particular telescopes, or simple, a place where different FoV would be added by particular users that has done the work to define it for their observational proporsal) (i.e. the FoV is just another item in all the VO environment) Well it is just a comment :) cheers Miguel From owner-theory@eso.org Thu May 18 17:34:20 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k4IFY1KG011943 for ; Thu, 18 May 2006 17:34:01 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k4IFY1AJ011942 for theory-outgoing; Thu, 18 May 2006 17:34:01 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k4IFY0KG011927 for ; Thu, 18 May 2006 17:34:00 +0200 (MEST) Received: from smtpsortant.univ-lyon1.fr (smtpsortant.univ-lyon1.fr [134.214.100.5]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k4IFXwQk024785 for ; Thu, 18 May 2006 17:33:58 +0200 (CEST) Received: from smtpsortant (localhost [127.0.0.1]) by smtpsortant.univ-lyon1.fr (Postfix) with ESMTP id A5B9334416; Thu, 18 May 2006 17:33:52 +0200 (CEST) Received: from cisrweb.univ-lyon1.fr (cisrweb.univ-lyon1.fr [193.48.219.23]) by smtpsortant_amavis_only (Postfix) with ESMTP id 0CFD634404; Thu, 18 May 2006 17:33:52 +0200 (CEST) Received: by cisrweb.univ-lyon1.fr (Postfix, from userid 33) id 04C2A530002; Thu, 18 May 2006 17:33:52 +0200 (CEST) Received: from 204.50.11.162 ([204.50.11.162]) by webmail.univ-lyon1.fr (IMP) with HTTP for ; Thu, 18 May 2006 17:33:51 +0200 Message-ID: <1147966431.446c93dfe5179@webmail.univ-lyon1.fr> Date: Thu, 18 May 2006 17:33:51 +0200 From: Herve Wozniak To: theory@ivoa.net Cc: mcs@iaa.es, flepetit@mesiog.obspm.fr, c.gheller@cineca.it, glemson@xray.mpe.mpg.de, ndelmott@eso.org, deyoung@noao.edu, andrea.preitemartinez@iasf-roma.inaf.it, gerard.lemson@mpe.mpg.de Subject: semantics MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1 Content-Transfer-Encoding: 8bit User-Agent: Internet Messaging Program (IMP) 3.2.6 X-Originating-IP: 204.50.11.162 X-Virus-Scanned: by AMaViS snapshot-20020222 X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.18.75108 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Herve Wozniak Hello, I just have a look to the vocabulary list (http://www.ivoa.net/twiki/bin/view/IVOA/TheorySemanticVocabulary) that has been recently increased by Miguel. Thanks to fill the gap with all the necessary tools for stellar population evolution. I'm wondering however whether we need or not to introduce a second level of 'physical processes' (as suggested by Miguel, I guess). I understand that the problem comes from stellar evolution and stellar population synthesis since the real physical processes involved in such modelling are very embedded in several shells of code. It could be difficult to classify PEGASE, GALAXEV etc. in the 'radiative transfer' or 'photoionization' boxes! I could also anticipate that if I want to classify my own chemodynamical codes, I will need more or less every keywords of the 'physical process' list (apart from GR!)!!! Keeping in mind that these keywords are possible values of an UCD, I would describe my chemodyn code as 'gravitational dynamics + hydrodynamics' at the minimum, but how to describe star formation recipes, feedback, stellar population evolution etc. which form the 'chemo' part of the code ? Anyway, in my opinion, 'stellar evolution', 'stellar population synthesis', but also 'stellar structure' and so on (still many gaps to be filled!), should be also (or only?) listed in the 'subject'. I suggest to include photoionization and photodissociation in 'physical process' to be able to describe e.g. cloudy,mappings, Meudon code, etc., should we keep or not the 'primary/secondary' distinction. I would like to propose that hydrostatic is a particular case of hydrodynamics since a growing number of star/planet/exo-planet atmosphere models includes atmospheric circulation. Cheers, Herve _______________________________________________________________ Herve WOZNIAK Centre de Recherche Astronomique de Lyon (UMR 5574 UCBL/CNRS/ENS-Lyon) 9, avenue Charles Andre, F-69561 Saint Genis Laval cedex Phone: (+33) (0) 478 868 388 Fax: (+33) (0) 478 868 386 http://www-obs.univ-lyon1.fr/herve.wozniak/ -------------------------------------------------------------------------- Ce message a été envoyé depuis le webmail IMP (Internet Messaging Program) From owner-theory@eso.org Thu May 18 19:23:41 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k4IHNZKG027516 for ; Thu, 18 May 2006 19:23:35 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k4IHNYno027515 for theory-outgoing; Thu, 18 May 2006 19:23:34 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k4IHNXKG027506 for ; Thu, 18 May 2006 19:23:33 +0200 (MEST) Received: from mesiob.obspm.fr (mesiob.obspm.fr [145.238.2.2]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k4IHNVQk000140 for ; Thu, 18 May 2006 19:23:31 +0200 (CEST) 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) with ESMTP id k4IHMT2U014392; Thu, 18 May 2006 19:22:29 +0200 Date: Thu, 18 May 2006 19:22:29 +0200 (CEST) From: Franck.LePetit@obspm.fr X-X-Sender: flepetit@mesioq.obspm.fr To: Herve Wozniak cc: theory@ivoa.net, mcs@iaa.es, flepetit@mesiog.obspm.fr, c.gheller@cineca.it, glemson@xray.mpe.mpg.de, ndelmott@eso.org, deyoung@noao.edu, andrea.preitemartinez@iasf-roma.inaf.it, gerard.lemson@mpe.mpg.de Subject: Re: semantics In-Reply-To: <1147966431.446c93dfe5179@webmail.univ-lyon1.fr> Message-ID: References: <1147966431.446c93dfe5179@webmail.univ-lyon1.fr> MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=ISO-8859-1 X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-2.0.2 (mesiob.obspm.fr [145.238.2.2]); Thu, 18 May 2006 19:22:29 +0200 (CEST) X-Virus-Scanned: ClamAV version 0.88.2, clamav-milter version 0.88.2 on mesiob.obspm.fr X-Virus-Status: Clean X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.18.93105 Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from QUOTED-PRINTABLE to 8bit by mercury.hq.eso.org id k4IHNYKG027511 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Franck.LePetit@obspm.fr Hello, We thought a bit to this problem of definition we had on tuesday afternoon. I put below my notes. My conclusions are : - we have to add an entry for the name of the developper or the developping team. during the registration. - The tag physical process will be our main problem. We will have to describe far more our codes that we said on tuesday. Below I give the example of somebody who would looked for a PDR code to compute vibrationnal excitation of H2. It will require to describe codes in all the details. - On the other hand, as mentionned during the discussion on tuesday and in last Herve's mail, registration of some codes would require to use far too much "physical processes" values. An efficient search in registries need to group them with more common names. Ex: photoionization region code (cloudy type), PDR code. Best regards Franck Le Petit and Fabrice Roy ---------------------------------------------------------- Note about UCDs for the descrition of codes in registries ---------------------------------------------------------- First we have to precise if we try to caracterize a code or a result from a simulation. They should be considered as two different categories in the registries. A metadata should be associated to simulation results to say from which code it comes from. A search on this metadata should be possible. Example : I want all simulation results from Zeus. ********************************************** UCDs required FOR CODES ********************************************** A search in the registries has to find a code. Example of searches : 0) I want the wonderful code developped by the Albert E. 1) I want the Cloudy code. (search by name) 2) I want the version of 1999 of the Cloudy code (add the version) 3) I want a radiative transfer code (category of code) 4) I want a radiative transfer code using the Ali method (method specification) 5) I want a radiative transfer code able to deal with X-Rays in optically thick media. (that is a tough one) 6) I want a radiative transfer code for interstellar clouds in the millimetric producing spectra. (add a specification on the output) 8) I want an MHD code using characteristics methods for boundary conditions. (method about boundary conditions - should be covered by algorithm) 10) I want a stationnary (or time dependent) MHD shock model Note : We could find very difficult queries. Ex: I want a PDR code computing the vibrational excitation of H2. Such queries would require to describe a lot the code in the registries (excitation of H2). I think that in a first step we do not have to go to this level but, at a point, it may be necessary. It will require to have many possibilities in the "physical process" tag (far more than in the thesaurus). 0 --- Team / developper --------------------------------------- (Example 0) A search on the name of a team or of a developper name should be possible. It is frequent, we choose a code because we are confident in a team... Required for registration : yes 1 --- Name -------------------------------------------------- (Example 1) A UCD is required to tag the name of the code Required for registration : yes Multiple possibilities : no Choice from a list : no 2 --- Version ----------------------------------------------- (Ex. 2) A UCD is required to tag the number version of the code. Required : yes Multiple possibilities : no Choice from a list : should follow common standards for versionning (Hervé knows that) 3 --- Physical Process (Type of code) ----------------------- (Ex. 3) A UCD is required to specify the physical processes the code can deal with. Most of the possibilities can be found in the "thesaurus". We should add some possibilities which are the common name given to codes dealing with many physical processes. Example : PDR code, Photoionization region code. Multiple choice possible : yes Defined list of possibilities : yes(?) List of choices : Thesaurus (plus a few more to reflect the usual way these codes are called ? ) Note: If we want to find a solution as the request :"search for a PDR code computing the H2 excitation", the thesaurus will no more be sufficient. Other solutions will have to be found. Examples : - radiative transfer - MHD - gravitationnal dynamics (not in thesaurus) - photoionization (cover many physical processes) - PDR (cover many physical processes) 4 --- Subject --------------------------------------------- (Ex. 6-7) This UCD would precise the kinds of objects the code can simulate. Example : - Accretion disk - Molecular clouds - Galaxies ... Multiple choice : yes Defined list of possibilities : yes List : Thesaurus Note : Example 5 is a problem. The request requires a code able to deal with optically thick media. Such characterization is not found in the thesaurus. Note : A search using "Physical process" and "Subject" should succeed most of the time excepted for specific researches 5 --- Algorithm ---------------------------------------- (Example : 4,8) This UCD is required to specify an algorithm. Example : N-body, SPH, Ali, ..., Problem : The same algorithm can have different names. Possible solution : Add as many values as it has of names. The list should not be limited. Reason : New algorithms can be found. Should this field be filled for all codes ? Not sure if such classification is relevant for physico-chemistry codes. There are so many physical processes that nobody care how they are done (excepted for radiative transfer). 6 --- Time Evolution algorithm ---------------------------- Is it a necessity to separate the time algorithm with the other algorithms ? The main interest is that this UCD could help to discriminate between stationnary and time dependent codes. (7 --- Algorithmic parameters) --------------------------- To be suppressed for the definition of codes in the VO. Only relevant for the definition of results of simulations. 8 --- Result type ----------------------------------------- (Ex: 6) A UCD is required for result type as seen in Ex. 6. Multiple possibilities : yes Defined list of possibilities : yes List : - snapshot - animation - table - fits 9 --- Result parameters I do not see the purpose of this UCD. From owner-theory@eso.org Fri May 19 02:06:15 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k4J069Ed025071 for ; Fri, 19 May 2006 02:06:09 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k4J069O1025070 for theory-outgoing; Fri, 19 May 2006 02:06:09 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k4J067Ed025057; Fri, 19 May 2006 02:06:07 +0200 (MEST) Received: from newb6.u-strasbg.fr (newb6.u-strasbg.fr [130.79.128.16]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k4J065Qk018096; Fri, 19 May 2006 02:06:05 +0200 (CEST) Received: from localhost (www-data@astron [130.79.128.15]) by newb6.u-strasbg.fr (8.9.3/8.9.3) with ESMTP id CAA25384; Fri, 19 May 2006 02:05:52 +0200 (MET DST) Received: from 204.50.11.162 ([204.50.11.162]) by astron.u-strasbg.fr (Horde MIME library) with HTTP; Fri, 19 May 2006 02:00:21 +0200 Message-ID: <20060519020021.o1fqwxilb9344k40@astron.u-strasbg.fr> Date: Fri, 19 May 2006 02:00:21 +0200 From: derriere@newb6.u-strasbg.fr To: Franck.LePetit@obspm.fr Cc: Herve Wozniak , theory@ivoa.net, mcs@iaa.es, flepetit@mesiog.obspm.fr, c.gheller@cineca.it, glemson@xray.mpe.mpg.de, ndelmott@eso.org, deyoung@noao.edu, andrea.preitemartinez@iasf-roma.inaf.it, gerard.lemson@mpe.mpg.de Subject: Re: semantics References: <1147966431.446c93dfe5179@webmail.univ-lyon1.fr> In-Reply-To: MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1; format="flowed" Content-Disposition: inline User-Agent: Internet Messaging Program (IMP) H3 (4.0.4) X-MailScanner-Astro: Message analyse non infecte par sophos sur astro.u-strasbg.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.18.155111 Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id k4J068Ed025062 Sender: owner-theory@eso.org Precedence: bulk Reply-To: derriere@newb6.u-strasbg.fr Hello, You can find the presentation that I did during Registry session 5 on the meeting page: http://www.ivoa.net/twiki/bin/view/IVOA/InterOpMay2006ResReg Especially, on the last slide, I tried to identify the metadata tags from the Registry ResourceMetadata document that could correspond to the main categories that you identified. Comments are welcome. By the way, I'm a bit uncomfortable with the usage of the UCD term in your mail. For example, I totally agree that we need a UCD meaning "algorithm". But the different possible values described by this UCD are not UCDs. They can be words in a normalized vocabulary, you can write them using a "a la UCD" syntax, but they really are not UCDs. To tell it in a few words, we can have a UCD for each ResourceMetadata element. The UCD is used to give a name to the empty box, and this name is not specific to a given schema, unlike the name of the XML element. The values you put in the box can be issued from a normalized vocabulary, but they are not UCDs in the original sense. Sebastien. From owner-theory@eso.org Fri May 19 18:44:23 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k4JGi7Ed014032 for ; Fri, 19 May 2006 18:44:07 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k4JGi7Wk014031 for theory-outgoing; Fri, 19 May 2006 18:44:07 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k4JGi7Ed014025 for ; Fri, 19 May 2006 18:44:07 +0200 (MEST) Received: from mpehp1.mpe-garching.mpg.de (mpehp1.mpe-garching.mpg.de [130.183.70.10]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k4JGi5Qk029103 for ; Fri, 19 May 2006 18:44:05 +0200 (CEST) Received: from localhost (glemson@localhost) by mpehp1.mpe-garching.mpg.de (8.9.3 (PHNE_25183+JAGae58098)/8.9.3) with ESMTP id SAA27218 for ; Fri, 19 May 2006 18:44:00 +0200 (METDST) X-Authentication-Warning: mpehp1.mpe-garching.mpg.de: glemson owned process doing -bs Date: Fri, 19 May 2006 18:44:00 +0200 (METDST) From: Gerard Lemson X-Sender: glemson@mpehp1.mpe-garching.mpg.de To: theory@ivoa.net Subject: metadata modeling 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: 2.3.0.1, Antispam-Data: 2006.5.19.83106 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Gerard Lemson Dear collegues Today at 11 we will try to meet in Boardroom B, upstairs, to discuss the approach to modeling metadata for discovering interesting simulations. See you there Gerard From owner-theory@eso.org Fri May 19 19:42:15 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k4JHg8Ed021595 for ; Fri, 19 May 2006 19:42:08 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k4JHg8cN021593 for theory-outgoing; Fri, 19 May 2006 19:42:08 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k4JHg8Ed021589; Fri, 19 May 2006 19:42:08 +0200 (MEST) Received: from mail.globalsuite.net (mail.globalsuite.net [69.46.103.201]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k4JHg5sR010797; Fri, 19 May 2006 19:42:06 +0200 (CEST) Received: from localhost.localdomain (unknown [204.50.11.162]) by mail.globalsuite.net (Symantec Mail Security) with ESMTP id 4CF8BC2F; Fri, 19 May 2006 11:41:58 -0600 (MDT) Received: from localhost.localdomain (localhost [127.0.0.1]) by localhost.localdomain (8.13.6/8.13.4) with ESMTP id k4JHgFBM006439; Fri, 19 May 2006 13:42:15 -0400 Received: from localhost (localhost [[UNIX: localhost]]) by localhost.localdomain (8.13.6/8.13.5/Submit) id k4JHgFbH006436; Fri, 19 May 2006 13:42:15 -0400 X-Authentication-Warning: localhost.localdomain: thomas set sender to brian_thomas@earthlink.net using -f From: Brian Thomas To: dm@ivoa.net, theory@ivoa.net Subject: Links to W3C workflow/processing models Date: Fri, 19 May 2006 13:42:15 -0400 User-Agent: KMail/1.9.1 Cc: grid@ivoa.net MIME-Version: 1.0 Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 7bit Content-Disposition: inline Message-Id: <200605191342.15312.brian_thomas@earthlink.net> X-Brightmail-Tracker: AAAAAA== X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.19.95111 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Brian Thomas As I mentioned in the DM session today there are a number of W3C efforts which should be considered (or at least mined for the 'good stuff') in terms of doing distributed workflows and processing descriptions. (at Mark Taylor's suggestion I have cross posted to theory and grid-ws groups..don't shoot the messenger!!) =brian Links: http://www.w3.org/TR/proc-model-req/ http://www.w3.org/TR/xml-pipeline/ (older) http://www.w3.org/Submission/OWL-S/ Software : http://www.mindswap.org/2004/owl-s/api/ (OWL-S API/execution environment) From owner-dm@eso.org Fri May 19 19:42:32 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k4JHgAEd021610 for ; Fri, 19 May 2006 19:42:10 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k4JHgAYO021609 for dm-outgoing; Fri, 19 May 2006 19:42:10 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dm@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 k4JHg8Ed021589; Fri, 19 May 2006 19:42:08 +0200 (MEST) Received: from mail.globalsuite.net (mail.globalsuite.net [69.46.103.201]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k4JHg5sR010797; Fri, 19 May 2006 19:42:06 +0200 (CEST) Received: from localhost.localdomain (unknown [204.50.11.162]) by mail.globalsuite.net (Symantec Mail Security) with ESMTP id 4CF8BC2F; Fri, 19 May 2006 11:41:58 -0600 (MDT) Received: from localhost.localdomain (localhost [127.0.0.1]) by localhost.localdomain (8.13.6/8.13.4) with ESMTP id k4JHgFBM006439; Fri, 19 May 2006 13:42:15 -0400 Received: from localhost (localhost [[UNIX: localhost]]) by localhost.localdomain (8.13.6/8.13.5/Submit) id k4JHgFbH006436; Fri, 19 May 2006 13:42:15 -0400 X-Authentication-Warning: localhost.localdomain: thomas set sender to brian_thomas@earthlink.net using -f From: Brian Thomas To: dm@ivoa.net, theory@ivoa.net Subject: Links to W3C workflow/processing models Date: Fri, 19 May 2006 13:42:15 -0400 User-Agent: KMail/1.9.1 Cc: grid@ivoa.net MIME-Version: 1.0 Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 7bit Content-Disposition: inline Message-Id: <200605191342.15312.brian_thomas@earthlink.net> X-Brightmail-Tracker: AAAAAA== X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.19.95111 Sender: owner-dm@eso.org Precedence: bulk Reply-To: Brian Thomas As I mentioned in the DM session today there are a number of W3C efforts which should be considered (or at least mined for the 'good stuff') in terms of doing distributed workflows and processing descriptions. (at Mark Taylor's suggestion I have cross posted to theory and grid-ws groups..don't shoot the messenger!!) =brian Links: http://www.w3.org/TR/proc-model-req/ http://www.w3.org/TR/xml-pipeline/ (older) http://www.w3.org/Submission/OWL-S/ Software : http://www.mindswap.org/2004/owl-s/api/ (OWL-S API/execution environment) From owner-grid@eso.org Fri May 19 19:42:33 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k4JHg9Ed021603 for ; Fri, 19 May 2006 19:42:09 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k4JHg9p0021601 for grid-outgoing; Fri, 19 May 2006 19:42:09 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-grid@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 k4JHg8Ed021589; Fri, 19 May 2006 19:42:08 +0200 (MEST) Received: from mail.globalsuite.net (mail.globalsuite.net [69.46.103.201]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k4JHg5sR010797; Fri, 19 May 2006 19:42:06 +0200 (CEST) Received: from localhost.localdomain (unknown [204.50.11.162]) by mail.globalsuite.net (Symantec Mail Security) with ESMTP id 4CF8BC2F; Fri, 19 May 2006 11:41:58 -0600 (MDT) Received: from localhost.localdomain (localhost [127.0.0.1]) by localhost.localdomain (8.13.6/8.13.4) with ESMTP id k4JHgFBM006439; Fri, 19 May 2006 13:42:15 -0400 Received: from localhost (localhost [[UNIX: localhost]]) by localhost.localdomain (8.13.6/8.13.5/Submit) id k4JHgFbH006436; Fri, 19 May 2006 13:42:15 -0400 X-Authentication-Warning: localhost.localdomain: thomas set sender to brian_thomas@earthlink.net using -f From: Brian Thomas To: dm@ivoa.net, theory@ivoa.net Subject: Links to W3C workflow/processing models Date: Fri, 19 May 2006 13:42:15 -0400 User-Agent: KMail/1.9.1 Cc: grid@ivoa.net MIME-Version: 1.0 Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 7bit Content-Disposition: inline Message-Id: <200605191342.15312.brian_thomas@earthlink.net> X-Brightmail-Tracker: AAAAAA== X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.3.0.1, Antispam-Data: 2006.5.19.95111 Sender: owner-grid@eso.org Precedence: bulk Reply-To: Brian Thomas As I mentioned in the DM session today there are a number of W3C efforts which should be considered (or at least mined for the 'good stuff') in terms of doing distributed workflows and processing descriptions. (at Mark Taylor's suggestion I have cross posted to theory and grid-ws groups..don't shoot the messenger!!) =brian Links: http://www.w3.org/TR/proc-model-req/ http://www.w3.org/TR/xml-pipeline/ (older) http://www.w3.org/Submission/OWL-S/ Software : http://www.mindswap.org/2004/owl-s/api/ (OWL-S API/execution environment) From owner-theory@eso.org Thu Jun 1 14:22:26 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k51CMAap028260 for ; Thu, 1 Jun 2006 14:22:11 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k51CMAJF028259 for theory-outgoing; Thu, 1 Jun 2006 14:22:10 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k51CM1ap028229 for ; Thu, 1 Jun 2006 14:22:01 +0200 (MEST) Received: from mpemail.mpe.mpg.de (mpemail.mpe-garching.mpg.de [130.183.137.110]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k51CLxsR000223 for ; Thu, 1 Jun 2006 14:21:59 +0200 (CEST) Received: from gavopc1.xray.mpe.mpg.de ([130.183.72.204] helo=gavopc1) by mpemail.mpe.mpg.de with esmtp (Exim 4.50) id 1FlmC9-0000Td-B2 for theory@ivoa.net; Thu, 01 Jun 2006 14:22:33 +0200 From: "Gerard" To: Subject: results victoria meeting and roadmap Date: Thu, 1 Jun 2006 14:24:19 +0200 Message-ID: <000f01c68576$4e901b60$cc48b782@gavopc1> MIME-Version: 1.0 Content-Type: multipart/alternative; boundary="----=_NextPart_000_0010_01C68587.1218EB60" X-Mailer: Microsoft Office Outlook 11 Thread-Index: AcaFdk4WpkzmZzDdQWKnt9SLa5WFuA== X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2869 X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.6.1.43408 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: "Gerard" This is a multi-part message in MIME format. ------=_NextPart_000_0010_01C68587.1218EB60 Content-Type: text/plain; charset="US-ASCII" Content-Transfer-Encoding: 7bit Dear collegues To all of you who participated during the interop in Victoria: thank you very much for your contributions during a rather busy week. I think we accomplished quite a lot, on which we can now build during the time till the next interop in Moscow. In particular, I want to list here the projects that we started, the time scales on which we want to see results, as well as the people who volunteered to participate. NB. My memory of precisely who volunteered during the meeting is patchy. I am sure there may have been more hands raised than I remember. Please mail me if you feel left out. ---------- Semantics: ---------- Following early work by Laurie on UCDs for simulations, we started compiling a list of concepts on the meeting's TWiki page. This list will be open for editing by everyone for two weeks starting today. After this period a number of us will translate this list into a request to the Semantics WG for additions to the list of UCDs and words to the Semantic Vocabulary. This we want to be finished in about a month (i.e. mid July) so that we can send it to the Semantics group and have it discusssed by Moscow Interop. Everyone is invited to add to the list of words on the TWiki page. Please see that page for how to proceed to add these. The following persons volunteered for adding structure to this list. We should start discussing how to do so via the email list. Following practice in other groups I suggest to prefix the subject with [SEMANTICS] : Laurie Shaw Dave De Young Peter Teuben Claudio Gheller Herve Wozniak Frank LePetit GL . ----- SNAP: ----- We decided to move ahead with the Simple Numerical Access Protocol (SNAP) that was initiated during the workshop in Cambridge, early this year. There was discussion about whether the protocol should incorporate both N-Body and mesh simulations. The majority opinion was that we should do this. We decided to follow the SSA approach, not the (old) SIAP approach that SNAP was originally based on. This implies that apart from a specification of the query protocol and data formats, we need a data model for the metadata of the data products. This model will determine what is returned by the query protocol, the protocol itself, and likely also the metadata accompanying the final delivered data products. The project for this is described separately below. Also the tasks surrounding data formats is described separately. We discussed the functionality described by the protocol. It was decided that apart from (in principle) allowing retrieval of complete data sets, there should be options for retrieving subsets. These can be sub volumes/slices etc, but possibly also random sampling. A problem is how we can let a user decide which subset they want. Possibilities such as querying for a "thumbnail" small version of the complete set were shown by Claudio in his demo of VisIVO which already has SNAP like functionality. This will need to be worked out further. Volunteers for working on the SNAP protocol are Claudio Gheller Laurie Shaw Herve Wozniak Peter Teuben (?) GL . Let's use [SNAP] as prefix for emails about this subject on the theory mailing list. Mails could be Cc-ed to the dal mailing list. We want to have a version 0.1 document containing descriptions of the functionality for SNAP as well as the data formats we propose for the results to be ready for discussion in Moscow. After this we should start incorporating the results of the data modeling project and progress to a version 0.5 or further by the China interop, 2007. ------------- Data Formats: ------------- We discussed the formats for data products sent from theory specific services, such as the SNAP discussed above. The concensus was that we'd for now stick to VOTable where appropriate, likely using the BINARY form for the data itself. It was realised this may require some selling to the community, as well as further polling into what data formats are actually being used and how translators can be written to the proposed standard. Dave Zurek volunteered to start this, Dave De Young will participate, GL in Europe. Results of this poll will be communicated by the next interop. Claudio Gheller volunteered to write example translator modules for some of the data formats he deals with in VisIVO. GL will do so for some of the Gadget postprocessed data sets. These will be shown next interop. Discussion about this could be prefixed with [DATAFORMATS] Mails could be Cc-ed to the dal mailing list. -------------- Data modeling: -------------- We had a special session about data modeling for simulation data. It was decided we would start working on this according to the following plan: - Agree on the problem domain (focus on discovery as use case) - Define conceptual or analysis model of the problem domain(s) (Physics, characterisation, computational details) - Define a fully detailed logical model for the particular problem area (SNAP) - Define binding to particular languages: XML, Java/C#, relational model See the PPT on "Data modeling for simulations" at the meeting's TWiki page for some more details. Volunteers for working further on this subject were: Gerard Lemson Herve Woznaik Dave De Young Frank LePetit Laurie Shaw Mireille Louys Brian Thomas . Time scale is that by Moscow we should have the conceptual model ready for discussion. The model should then be tied in with SNAP, with a logical model for SNAP incorporated in the SNAP 0.5 version. When mailing the theory list use something like [SIMULATION DM] as prefix. I guess the DM list could be included in such mails. ----------------- Summary, roadmap: ----------------- Summarising these developments is the following road map for the theory interest group. Note that some of these tasks really fall under the responsibility of particular working groups, in particular DAL and DM. Their chairmen have agreed with our plans and we will keep them in the loop. ---------------------------------------------------------------------------- ----------------- Description When finished ---------------------------------------------------------------------------- ----------------- Semantics: Collect unstructured list of words and concepts for use in - June 16 2006 registration of non-standard theory services/datasets and data model. Result: TWiki page Add structure to the list, divide in UCD and Semantic - July 14 2006 Vocabulary, cross check with VOEvent and other such lists Result: Note Discuss Note within IG, update and - July 31 2006 send to Semanticsa working group as request Data modeling: Create analysis model for simulations containing: - Interop Moscow 2006 characterisation physics numerical algorithm experiment Result: WD Logcial model included in SNAP - Interop China 2007 Result: WD Data formats: Poll theorists about the data formats they use in their - Moscow Interop 2006 simulations, and their wilingness to assist in translating these to VOTable. Result: Note Example code for translating some popular data formats - Moscow Interop 2006 into binary votable SNAP: Write WD about SNAP, focusing on functionality and data formats - Moscow Interop 2006 of different types of simulations: N-Body, regular mesh, AMR Result: WD version 0.1 Incorporate data models - China Interop 2007 Result: WD version 0.5 Prototpye applications using following possible serialisations - After China Interop, before Autumn Interop of data model XML Java, C# relational model Result: applications that "do" something with the model Propose as PR - Autumn interop 2007 Various: Outreach to theorists to register their services - June 5 2006 Result: email to representatives of national projects This mail will be added as a Projects page on the TWiki of the theory group. Please send comments to the theory mailing list. Best regards Gerard Lemson ------=_NextPart_000_0010_01C68587.1218EB60 Content-Type: text/html; charset="US-ASCII" Content-Transfer-Encoding: quoted-printable

Dear collegues

 

To all of you who participated during the interop in = Victoria:

thank you very much for your contributions during a = rather busy

week. I think we accomplished quite a lot, on which = we can now

build during the time till the next interop in = Moscow. =

 

In particular, I want to list here the projects that = we started,

the time scales on which we want to see results, as = well as

the people who volunteered to participate. =

NB.

My memory of precisely who volunteered during the = meeting is patchy.

I am sure there may have been more hands raised than = I remember.

Please mail me if you feel left = out.

 

 

----------

Semantics:

----------

Following early work by Laurie on UCDs for = simulations,

we started compiling a list of concepts on the = meeting's TWiki page.

This list will be open for editing by everyone for = two weeks starting today.

After this period a number of us will translate this = list

into a request to the Semantics WG for additions to = the list of UCDs and

words to the Semantic = Vocabulary.

This we want to be finished in about a month (i.e. = mid July) so that we

can send it to the Semantics group and have it = discusssed by Moscow Interop.

 

Everyone is invited to add to the list of words on = the TWiki page.

Please see that page for how to proceed to add = these.

 

The following persons volunteered for adding = structure to this list.

We should start discussing how to do so via the email = list.

Following practice in other groups I suggest to = prefix the subject with

[SEMANTICS] :

Laurie Shaw

Dave De Young

Peter Teuben

Claudio Gheller

Herve Wozniak

Frank LePetit

GL

…

 

-----

SNAP:

-----

We decided to move ahead with the Simple Numerical = Access Protocol (SNAP) that was initiated

during the workshop in Cambridge, early this year. There was discussion about whether the =

protocol should incorporate both N-Body and mesh simulations. The majority opinion was that = we

should do this.

 

We decided to follow the SSA approach, not the (old) = SIAP approach that SNAP

was originally based on. This implies that apart from = a specification of the query protocol and

data formats, we need a data model for the metadata = of the data products. This model will determine

what is returned by the query protocol, the protocol = itself, and likely also the metadata

accompanying the final delivered data products. The = project for this is described separately below.

Also the tasks surrounding data formats is described separately.

 

We discussed the functionality described by the = protocol. It was decided that apart from (in principle)

allowing retrieval of complete data sets, there = should be options for retrieving subsets. These

can be sub volumes/slices etc, but possibly also = random sampling.

A problem is how we can let a user decide which = subset they want. Possibilities such as querying

for a "thumbnail" small version of the = complete set were shown

by Claudio in his demo of VisIVO which already has = SNAP like functionality. This will need

to be worked out = further.

 

 

Volunteers for working on the SNAP protocol = are

Claudio Gheller

Laurie Shaw

Herve Wozniak

Peter Teuben (?)

GL

…

 

Let's use [SNAP] as prefix for emails about this = subject on the theory mailing list.

Mails could be Cc-ed to the dal mailing = list.

 

We want to have a version 0.1 document containing descriptions of the functionality for SNAP

as well as the data formats we propose for the = results to be ready for discussion in Moscow.

After this we should start incorporating the results = of the data modeling project and

progress to a version 0.5 or further by the = China interop, 2007.

 

 

-------------

Data Formats:

-------------

We discussed the formats for data products sent from = theory specific services,

such as the SNAP discussed = above.

The concensus was that we'd for now stick to VOTable = where appropriate, likely using

the BINARY form for the data = itself.

It was realised this may require some selling to the community, as well as further polling

into what data formats are actually being used and = how translators can be written to

the proposed standard.

 

Dave Zurek volunteered to start this, Dave De Young = will participate, GL in Europe.

Results of this poll will be communicated by the next interop.

 

Claudio Gheller volunteered to write example = translator modules for some of the data formats

he deals with in VisIVO.

GL will do so for some of the Gadget postprocessed = data sets.

These will be shown next = interop.

 

Discussion about this could be prefixed with = [DATAFORMATS]

Mails could be Cc-ed to the dal mailing = list.

 

--------------

Data modeling:

--------------

We had a special session about data modeling for = simulation data.

It was decided we would start working on this = according to the following plan:

- Agree on the problem domain (focus on discovery as = use case)

- Define conceptual or analysis model of the problem domain(s)

  (Physics, characterisation, computational = details)

- Define a fully detailed logical model for the = particular problem area (SNAP)

- Define binding to particular languages: XML, = Java/C#, relational model

 

See the PPT on "Data modeling for = simulations" at the meeting's TWiki page

for some more details.

 

Volunteers for working further on this subject = were:

Gerard = Lemson

Herve Woznaik

Dave De Young

Frank LePetit

Laurie Shaw

Mireille Louys

Brian Thomas

…

 

Time scale is that by Moscow we should have the conceptual model ready for = discussion.

The model should then be tied in with SNAP, with a = logical model for SNAP

incorporated in the SNAP 0.5 = version.

 

When mailing the theory list use something like = [SIMULATION DM] as prefix.

I guess the DM list could be included in such = mails.

 

 

-----------------

Summary, roadmap:

-----------------

Summarising these developments is the following road = map for the theory

interest group. Note that some of these tasks really = fall under the responsibility

of particular working groups, in particular DAL and = DM. Their chairmen have agreed

with our plans and we will keep them in the = loop.

 

 

------------------------------------------------------= ---------------------------------------

   =          = Description          &n= bsp;           &nb= sp;           &nbs= p;            = ;            =             &= nbsp;           &n= bsp;        When finished

------------------------------------------------------= ---------------------------------------

Semantics:

         =    Collect unstructured list of words and concepts for use in = -           June 16 = 2006

         =    registration of non-standard theory services/datasets

         =    and data model.

         =    Result: TWiki page

 

         =    Add structure to the list, divide in UCD and Semantic =             &= nbsp;      = -           July 14 = 2006

         =    Vocabulary, cross check with VOEvent and other such lists

         =    Result: Note

 

         =    Discuss Note within IG, update = and           &nbs= p;            = ;            =          -           July 31 = 2006

         =    send to Semanticsa working group as = request           =             &= nbsp;     

 

 

Data modeling:

         =    Create analysis model for simulations containing: =             &= nbsp;           - =           Interop Moscow = 2006

         =             &= nbsp;  characterisation

         =             &= nbsp;  physics

         =             &= nbsp;  numerical algorithm

         =             &= nbsp;  experiment

         =    Result: WD

 

         =    Logcial model included in = SNAP           &nb= sp;           &nbs= p;            = ;            =   -           = Interop China 2007

         =    Result: WD

 

 

Data formats:

         =    Poll theorists about the data formats they use in their       - =           Moscow Interop = 2006

         =    simulations, and their wilingness to assist in translating

         =    these to VOTable.

         =    Result: Note

 

         =    Example code for translating some popular data formats           =     = -           Moscow = Interop 2006

         =    into binary votable

 

SNAP:

         =    Write WD about SNAP, focusing on functionality and data formats = -           Moscow = Interop 2006

         =    of different types of simulations: N-Body, regular mesh, AMR         =

         =    Result: WD version 0.1

 

         =    Incorporate data = models           &= nbsp;           &n= bsp;           &nb= sp;           &nbs= p;            = ; -           China Interop 2007

         =    Result: WD version 0.5

 

         =    Prototpye applications using following possible serialisations         = -           After = China Interop, before Autumn Interop

         =    of data model

         =             &= nbsp;  XML

         =             &= nbsp;  Java, C#

         =             &= nbsp;  relational model

         =    Result: applications that "do" something with the model

 

         =    Propose as = PR            = ;            =             &= nbsp;           &n= bsp;           &nb= sp;           &nbs= p; -           Autumn interop 2007

 

Various:

         =    Outreach to theorists to register their = services           = ;       = -           June 5 2006

         =    Result: email to representatives of national projects

 

 

 

This mail will be added as a Projects page on the = TWiki of the theory group.

Please send comments to the theory mailing = list.

 

 

Best regards

 

Gerard = Lemson

 

------=_NextPart_000_0010_01C68587.1218EB60-- From owner-theory@eso.org Fri Jun 2 10:50:34 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k528oIPn029934 for ; Fri, 2 Jun 2006 10:50:18 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k528oIYV029932 for theory-outgoing; Fri, 2 Jun 2006 10:50:18 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k528o1Pn028290 for ; Fri, 2 Jun 2006 10:50:01 +0200 (MEST) Received: from [134.171.10.74] (ma011930.hq.eso.org [134.171.10.74]) (authenticated bits=0) by clyde.hq.eso.org (8.12.8/8.12.8) with ESMTP id k528o148023642 (version=TLSv1/SSLv3 cipher=RC4-SHA bits=128 verify=NOT) for ; Fri, 2 Jun 2006 10:50:01 +0200 Mime-Version: 1.0 (Apple Message framework v749.3) In-Reply-To: <000f01c68576$4e901b60$cc48b782@gavopc1> References: <000f01c68576$4e901b60$cc48b782@gavopc1> Content-Type: text/plain; charset=ISO-8859-1; delsp=yes; format=flowed Message-Id: <59BBE49D-16FE-44C7-9E5C-7A2CDACF57AF@eso.org> From: Paul Harrison Subject: Re: results victoria meeting and roadmap [SNAP] parameter data model Date: Fri, 2 Jun 2006 10:50:08 +0200 To: theory@ivoa.net X-Mailer: Apple Mail (2.749.3) X-Virus-Scanned: by amavisd-new Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id k528oHPn029917 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Paul Harrison Hi, I did not attend any of the theory sessions in Victoria, but Gerard's summary has prompted me to draw your attention to some possible crossover with the work of the Registry and Grid WGs. The most obvious overlap is in the area described by Frédéric Boone's presentation on a parameter data model, where the Registry WG is defining a general model of an "application" including its parameters http://www.ivoa.net/twiki/bin/view/IVOA/RegDMApplications, which is based on the Common Execution Architecture (CEA) work within Astrogrid. CEA was originally designed to "wrap" legacy code as asynchronously callable web services (following the UWS pattern of the Grid WG http://www.ivoa.net/twiki/bin/view/IVOA/ IvoaGridAndWebServices#Asynchronous_activities_proposal) with parameter lists that were described in the registry so that user interfaces could be dynamically generated. Astrogrid has a mature implementation of CEA which includes * servers that can quickly be used to wrap a legacy commandline application - http://software.astrogrid.org/components/cea/index.html * a workflow component that can be used to run CEA applications - http://software.astrogrid.org/components/jes/index.html * a desktop client that can call the (remote) applications via a dynamic GUI or via your favourite scripting language - http:// software.astrogrid.org/userdocs/workbench.html The CEA parameter model was intended to be as general as possible and I think that it would already be suitable for use as part of SNAP, though I would be interested in working with you to add any features that you thought necessary. In addition, whilst the access to pre- computed theoretical data sets might be considered to be "Data Access", I can see that there are use cases where the theoretician wants to instruct a service to run a program to generate new data with new parameters, which would fit better with the "Execution" pattern being developed as UWS from the Grid WG. Paul Harrison From owner-theory@eso.org Fri Jun 16 17:37:37 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k5GFbLpO028513 for ; Fri, 16 Jun 2006 17:37:21 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k5GFbLhd028512 for theory-outgoing; Fri, 16 Jun 2006 17:37:21 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k5GFbGpO028502 for ; Fri, 16 Jun 2006 17:37:16 +0200 (MEST) Received: from serv2.obs-besancon.fr (serv2.obs-besancon.fr [193.52.185.12]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k5GFbEQk023346 for ; Fri, 16 Jun 2006 17:37:14 +0200 (CEST) Received: from services3.obs-besancon.fr ([193.52.184.204] ident=mail) by serv2.obs-besancon.fr with esmtp (Exim 3.36 #1 (Debian)) id 1FrG2z-00023h-00 for ; Fri, 16 Jun 2006 17:15:45 +0200 Received: from serv2.obs-besancon.fr ([193.52.185.12] helo=localhost) by services3.obs-besancon.fr with esmtp (Exim 3.36 #1 (Debian)) id 1FrFtm-0006cQ-00; Fri, 16 Jun 2006 17:06:14 +0200 Received: from dhcp241.iap.fr (dhcp241.iap.fr [193.49.4.241]) by webmail.obs-besancon.fr (Horde MIME library) with HTTP for ; Fri, 16 Jun 2006 17:05:27 +0200 Message-ID: <20060616170527.f8on5ycrqrvkkg88@webmail.obs-besancon.fr> Date: Fri, 16 Jun 2006 17:05:27 +0200 From: debray@obs-besancon.fr To: theory@ivoa.net Cc: bernard.debray@obs-besancon.fr Subject: [SEMANTICS] Re: semantics MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1 Content-Disposition: inline User-Agent: Internet Messaging Program (IMP) H3 (4.0.2) X-Observatoire-Besancon-MailScanner: Found to be clean, Found to be clean X-Observatoire-Besancon-MailScanner-From: debray@obs-besancon.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.6.16.75432 X-Virus-Scanned: by amavisd-new Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id k5GFbLpO028509 Sender: owner-theory@eso.org Precedence: bulk Reply-To: debray@obs-besancon.fr Dear members of the "theory" mailing list, as the deadline for collecting list of words and concepts (http://www.ivoa.net/twiki/bin/view/IVOA/TheorySemanticVocabulary) is approaching at high speed, I am just sending some comments coming from our view with the model of the Galaxy developed in Besançon (see http://www.ivoa.net/twiki/bin/view/IVOA/GalacticStellarContentSimulator). I have added some items on the twiki page and give some comments thereafter. The additions are : 1. add Galactic model to "name of code" 2. add "stars" to "subject" comment: in our mind, this is different from "star" ; "star" as a simulation subject can be understood as modelling the structure, interior, ... of a star, whereas "stars" infers modelling stellar population(s). Note that, may be in a different context, VOEvent does not make some difference between both (http://www.ivoa.net/internal/IVOA/VOEventVocabulary/objects.html). 3. add "Monte Carlo" and "Stellar population synthesis" to "type of algorithm" 4. add "catalogue of objects" and "object statistics" to "result type" ; Some further comments/possible additions: 5. can "nuclear reactions" be added to "physical process" ? 6. in "result type", may be "table" should be specified a bit more ? 7. should not we distinguish between result "type" (which could be "snapshot", "animation", " catalogue of objects", "object statistics", ...) and result "format" (which could then be: "FITS", "VOTable", "MPEG", "CSV", ...) 8. "algorithmic parameters" understood as initial and boundary conditions can be virtually any physical or astronomical quantity ; we have added some among the most important input parameters for the model of the Galaxy 9. I agree with Franck's remark about "Result parameters": Franck.LePetit@obspm.fr wrote: > ... > > 9 --- Result parameters > > I do not see the purpose of this UCD. With best regards, Bernard Debray -- Observatoire de Besançon | http://www.obs-besancon.fr/ 41 bis, avenue de l'Observatoire | bernard.debray@obs-besancon.fr BP 1615 | Tel : (33) 3 81 66 69 28 25010 Besançon cedex | Fax : (33) 3 81 66 69 44 France | ---------------------------------------------------------------- This message was sent using IMP, the Internet Messaging Program. From owner-theory@eso.org Mon Jun 19 18:04:11 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k5JG3v4V023535 for ; Mon, 19 Jun 2006 18:03:57 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k5JG3vam023534 for theory-outgoing; Mon, 19 Jun 2006 18:03:57 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k5JG3o4V023520 for ; Mon, 19 Jun 2006 18:03:50 +0200 (MEST) Received: from mesiob.obspm.fr (mesiob.obspm.fr [145.238.2.2]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k5JG3lQk026446 for ; Mon, 19 Jun 2006 18:03:47 +0200 (CEST) Received: from [145.238.18.175] (achille.obspm.fr [145.238.18.175]) by mesiob.obspm.fr (8.13.4/8.13.4/SIO Observatoire de Paris) with ESMTP id k5JG3Ztn016742 for ; Mon, 19 Jun 2006 18:03:35 +0200 Mime-Version: 1.0 (Apple Message framework v750) To: theory@ivoa.net Message-Id: <80909CA7-81A7-424F-9712-481D7E57E743@obspm.fr> Content-Type: multipart/alternative; boundary=Apple-Mail-18-626540190 From: Franck Le Petit Subject: [SEMANTICS] Re: semantics Date: Mon, 19 Jun 2006 17:53:51 +0200 X-Mailer: Apple Mail (2.750) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-2.0.2 (mesiob.obspm.fr [145.238.2.2]); Mon, 19 Jun 2006 18:03:35 +0200 (CEST) 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: 2.4.0.264935, Antispam-Data: 2006.6.19.75432 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Franck Le Petit --Apple-Mail-18-626540190 Content-Transfer-Encoding: quoted-printable Content-Type: text/plain; charset=ISO-8859-1; delsp=yes; format=flowed Dear members of the theory group. Now that the deadline of the 16th of june is behind us, we would = =20 like to suggest a modification of the Twiki page concerning Semantics =20= to continue the structuration of the informations. We would like to add to the main items further informations = which =20 should be required when we will ask to the semantic group to add UCDs =20= as : - Is the item a required information or an optinal one for =20 registration ? - Are multiple choice possible or not ? - Do the values associated to the UCDs have to be choosen from a = =20 given list or not and if yes, from which list ? =09 You will find below what we suggest for the presentation (a = mixture =20 of our previous email with some new inputs as well as Bernard =20 Debray's last comments). The list of words on the present twiki page =20 could be found at the end. Apart these modifications we see several difficulties up to now = : 1 - for the algorithms, the list may become very very long = and so =20 unusable for an efficient search in the registries. A solution has to =20= be find... 2 - Bernard Debray mentionned a very nice problem adding to = the =20 twiki page "Stellar synthesis Populations" in "physical processes". This is neither a "physical process", nor an = "algorithm", nor a =20 "subject". But that is the way everybody call such codes. It may be possible to cover such codes with "subject =3D = =20 Galaxies:Content" (if we want to use the thesaurus.). But who would =20 think to do a search this way ? I think I mentionned this difficulty with "PDR codes" = which, as =20 stellar synthesis populations codes cover many physical processes. Should not we add a new item "Category of code" to cover = large =20 domains of codes with a finite list of possibilities as : - Large structures formation - Hydrodynamic - MHD - Stellar synthesis populations - PDR - Numerical Relativity - Radiative transfer - ... In some cases, the value associated could be the same as = in =20 "physical processes" but not always as for "stellar population =20 synthesis". It would help a lot the search in registries. 3 - The item "Result parameters" seems unuseful for the =20 registration of codes. It may be useful for the registration of =20 simulation results but it is completly linked to the datamodel =20 describing the simulation results. So I suggest to forget it for the =20 moment. 4 - I added a new item "Description" where it would be = possible to =20 add an ASCII text describing the code. This exist yet in the =20 registration of any VO service in the present registries. I do not =20 know if the registries will allow to search by words in such =20 description. Does anybody know if we plan to have in the VO a tool =20 as "spotlight" in the Mac OS X which is able to find any document =20 when we give it a few words contained in this document ? Best regards Franck Le Petit & Fabrice Roy = ------------------------------------------------------------------- Observatoire of Paris LUTH - Laboratory Universe and Theories =20 -------------------------------------------------------------------- =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=20 =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D Suggestion for the new twiki page =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=20 =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D For each main items : - Description of the content of the UCD - Information on the content : - Is it a required information or an optional one - Are multiple choices possible - Do the informations have to be choosed in a list and = if yes, =20 from which list - Note : a place where to discuss on the twiki page each main = item. Note : need to specify the differences between what is required to =20 register codes and results from simulation. Remark : Required informations to register a code or a simulation =20 result are not exactly the same. In the latter case, parameters of =20 the simulation have to be specified which is not true for the =20 registration of the code. =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=20 =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D Main Items =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=20 =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D Items required to register a code : 1 - Name of the code 2 - Name of the developper / team / contact 3 - Version of the code 4 - Description of the code 5 - Physical processes 6 - Subject 7 - Algorithm 8 - Time evolution 9 - Type of results 10 - Results format 11 - Associated tools 12 - Web address Items required to register simulation results : 1 - Name of the dataset 2 - Name of the developpers / team / contact 3 - Version of the dataset 4 - Description 5 - Physical processes 6 - Subject 7 - Algorithm 8 - Time evolution 9 - Type of results 10 - Results formats 11 - Associated tools 12 - Web address 13 - Provenance 14 - Results parameters =46rom 1 to 12 it is similar to the registration of codes. 13 - Provenance : should give access to the code used to produce the =20 dataset (optional in case of simulation results coming from a code =20 not described in the VO) 14 - Result parameters : should give the parameters corresponding to =20 the production of the simulation results. It is difficult to discuss =20 this item now since it is directly linked to datamodels that we do =20 not have now. 1 --- Name of the code =20 ------------------------------------------------------------------------=20= --------------------------- Description : Give the name of the code Required : YES Multiple choice : NO List : NO Examples : Zeus, Ramses, Cloudy , .... Note : A UCD seems to exist : meta.id 2 --- Name of the developpers / team / contact =20 ------------------------------------------------------------------- Description : Give the name of the developpers Required : Yes Multiple choice : yes List : no Examples : Albert E. Note : 1 - Implementation done. UCD is meta.curation 3 --- Version of the code =20 ------------------------------------------------------------------------=20= ---------------------- Type: Required : yes Multiple choice : no List : no Examples : Note : - Herv=E9 suggested to use common standards for = versionning - A UCD seems to exist for that : meta.version 4 --- Description of the code =20 ------------------------------------------------------------------------=20= --------------- Description : ASCII text describing the code / the simulation = results Required : yes Multiple choice : no List : no list Note : Should be covered by the UCD meta.note (?) 5 --- Physical Process =20 ------------------------------------------------------------------------=20= ------------------------- Description : General keywords to describe the physical =20 processes that the code deal with Required : yes Multiple choice : yes List : MNRAS keywords, section "Physical data and processes" : =20= http://www.blackwellpublishing.com/pdf/mnraskey.pdf Examples : MHD, radiative transfer, molecular processes, =20 gravitation, ... Note : To avoid problems of synonyms during the search a list = may be =20 required. In the list on the former twiki page, nearly all words can =20 be found in the thesaurus but sometimes the meaning is not as precise =20= as we would wish. Does it seem sufficient ? 6 --- Subject =20 ------------------------------------------------------------------------=20= ------------------------------------- Description : General keywords describing the kind of objects =20= the code can deal with Required : yes Multiple choice : yes List : MNRAS keywords : http://www.blackwellpublishing.com/pdf/=20= mnraskey.pdf Examples : Star, Galaxy, Large scale structures, Molecular = clouds, ... Note : 1 - Advange to use a list is that the search should be =20= easier since it will avoid synonyms 2 - All words can be found in the thesaurus. 7 ---- =20 Algorithm = --------------------------------------------------------------=20 ------------------------------------------ Description : Most important algorithms in the code Required : optional Multiple choice : yes List : Yes but has to be defined Examples : nbody, tree, sph, Ali, ... Note : 1 - A list is necessary for an efficient search or we = will =20 have troubles with specific numerical methods and synonyms 2 - On the other hand, new algorithms can be found = and a fixed =20 list is a problem. Example :In radiative transfer it is necessary = to specify =20 algorithm. Up to now the main ones were : LVG, Monte-Carlo and Ali. =20 But recently Moshe Elitzur for Kentucky university has just found a =20 new revolutionnary method called CEP. How would it be possible to add =20= this to a fixed list ? 3 - I choosed to group algorithm and time =20 evolution algorithm. As numericians we clearly do the difference =20 between the two, but this separation may not be required in the =20 registries. Since multiple-choice are possible for this item, the =20 time evolution algorithm should be 8 ---- Time evolution =20 ------------------------------------------------------------------------=20= ------------------------- Description : Flag saying if the code is stationnar or time = dependant Required : yes Multiple choice : yes List : 2 possibilities : yes or no 9 ---- Type of result =20 ------------------------------------------------------------------------=20= --------------------------- Description : Give the type of results : Required : yes Multiple choice : yes List : yes - table - VO-table - spectre - VO-spectre - snapshot - animation - fits - catalog - statistics Note : 1 - The list has to be completed. 2 - Should we add to the list : "rawdata" for =20 binary results from a simulation ? 10 --- Results formats =20 ------------------------------------------------------------------------=20= ------------------------- Description : Give the format of the results Required : yes Multiple choice : yes List : yes - ASCII / binary - HDF5 - giff, jpeg, ... - mpeg4, quicktime, ... Note : This information could be usefull to find a code = producing =20 outputs in a specific format to be plug in a workflow.=09 11 --- Associated tools =20 ------------------------------------------------------------------------=20= ---------------------- Description : give the name in the VO registries of associated = tools =20 to the code Required : no Multiple choice : yes List : no Note : 1 - This would be usefull if a user looking for a code = could =20 find with the description of the code, associated VO-service for this =20= code. For example the name/acess to a theoretical database of results =20= produced by this code, or the name of another code used to analyse =20 the results of the first code. 12 --- Web Adress =20 ------------------------------------------------------------------------=20= ---------------------------- Description : give the web address where to access the code / =20= simulation result Required : yes Multiple choice : no List : no Note : A UCD exists for that : meta.ref.url =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D Simulation results =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D 13 - Provenance Description : Give the name of the code used to produce the =20 theoretical data Required : Optional Multiple : No (yes for results from the combination of 2 codes ? = ) List : no Note : 1 - Optional since the code used to produce the data may = not =20 be registered 14 - Results parameters Description : Give the parameters used to produce the data Required : yes Mutliple : yes List : no Note: 1 - Maybe it is too early to know how to deal with this = item =20 since it is directly linked to datamodel(s) =09 =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=20 =3D=3D=3D=3D=3D=3D B **** Thesaurus Keywords =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=20 =3D=3D=3D=3D=3D=3D Do the keywords of the thesaurus cover all the physical processes : Thesaurus radiative =20 transfer Yes gravitational =20 dynamics Gravitation GR What does GR means ? (General Relat. ?) =20 relativity =20 hydrodynamics =20= Yes fluid =20 dynamics W=20= hat is the difference with hydro ? plasma =20 physics =20 Plasma magneto-=20 hydrodynamics Yes stellar =20 evolution =20 No --- see subject below stellar population =20 synthesis No --- see subject below =20 photoionization =20= atomic processes / molecular processes =20 photodissociation =20= molecular processes physical process (secondary?) hydrostatic equilibrium (atmosphere?) No (but = may =20 be covered by an hydrodynamics physical process and a stationnary =20 algorithm) =09 =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D subject =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D =20 Subject =20= Thesaurus =20 star =20= star:individual: =20 stars =20= stars: stellar =20 clusters =20 galaxies: star clusters =20 galaxy =20= galaxies : volume of space accretion disc(k) =20 jet =20= ISM: jets and outflows interstellar =20 medium ISM molecular =20 cloud ISM : =20= clouds atmosphere (of planet, exo-planet, star...) =20 stars:atmosphere, nothing for planet atmosphere stellar evolution stars: = evolution stellar population =20 synthesis stars: evolution / =20 galaxy: evolution (?) =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D Algorithm =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D * nbody (What does it mean ? particle-particle ? ) * mesh * collisionless (not an algorithm ? - just a physical =20= approach ? ) * eulerian grid * lagrangian grid * tree * adaptive refinement mesh * adaptive refinement tree * sph * tree-sph * pppm * pm * pp (What is "nbody" compare to pp ? ) * fokker-planck codes * vlasov solvers * orbit solver * pic (particle in cell) * tree-pm * scf (self consistent field) * ffm (fast multipole method) * schwarzschild * ppm (piecewise parabolic method) * plm (piecewise linear method =3D godunov) * Isochrone synthesis * Fuel consuption theorem * Spectral method * Radiative transfer code : * ETL * LVG * Monte-Carlo * ALI * CEP =09 o leap frog o individual timesteps o static o adaptative timesteps o runge-kutta o symplectic integrator Gear Predictor/Corrector --Apple-Mail-18-626540190 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1

Dear members of the theory group.

Now that the deadline of the 16th of june is = behind us, we would like to suggest a modification of the Twiki page = concerning Semantics to continue the structuration of the = informations.
We would like to add to the main items = further informations which should be required when we will ask to the = semantic group to add UCDs as :
- = Is the item a required information or an optinal one for registration = ?
- = Are multiple choice possible or not ?
- = Do the values associated to the UCDs have to be choosen from a given = list or not and if yes, from which list ? =A0 =A0 =A0


You will find below what we suggest for the presentation (a = mixture of our previous email with some new inputs as well as Bernard = Debray's last comments). The list of words on the present twiki page = could be found at the end.=A0

Apart these modifications we see several difficulties up to now = :
1 = - = for the = algorithms, the list may become very very long and so unusable for an = efficient search in the registries. A solution has to be = find...

2 = - = Bernard Debray = mentionned a very nice problem adding to the twiki page "Stellar = synthesis Populations" in "physical processes".=A0
This is neither a "physical process", nor an "algorithm", nor a = "subject". But that is the way everybody call such = codes.=A0
It may be possible to cover such codes = with=A0 = "subject =3D = Galaxies:Content" (if we want to use the thesaurus.). But who would = think to do a search this way ?=A0
I = think I mentionned this difficulty with "PDR codes" which, as stellar = synthesis populations codes cover many physical = processes.=A0
Should not we add a new item "Category of = code" to cover large domains of codes with a finite list of = possibilities as :
- Large structures = formation
- Hydrodynamic
- = MHD
- = Stellar synthesis populations
- PDR
- = Numerical Relativity
- Radiative transfer
- = ...

In some cases, the value associated could be the same as in = "physical processes" but not always as for "stellar population = synthesis".=A0 =A0It would = help a lot the search in registries.

=A0

3 = - = The item "Result = parameters" seems unuseful for the registration of codes. It may be = useful for the registration of simulation results but it is completly = linked to the datamodel describing the simulation results. So I suggest = to forget it for the moment.
4 = - I = added a new item "Description" where it would be possible to add an = ASCII text describing the code. This exist yet in the registration of = any VO service in the present registries. I do not know if the = registries will allow to search by words in such description. Does = anybody know if we plan to have in the VO=A0 a tool as "spotlight" in the Mac OS X which = is able to find any document when we give it a few words contained in = this document ?=A0


Best regards
Franck Le Petit & Fabrice Roy

=A0 = =A0-------------------------------------------------------------------
Observatoire of Paris
LUTH = -=A0Laboratory = Universe and Theories
=A0 =A0=A0 =A0=A0 =A0=A0 = --------------------------------------------------------------------=A0




=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D
Suggestion for the new twiki = page
=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D


For each main items :
- = Description of the content of the UCD
- = Information on the content :
- Is it a required information or an optional = one
- = Are multiple choices possible
- Do=A0 the informations have to be choosed in a list = and if yes, from which list
- Note : a place where to discuss on the = twiki page each main item.
Note : need to specify the differences between what is required = to register codes and results from simulation.

Remark :=A0 Required informations to register a code or a = simulation result are not exactly the same. In the latter case, = parameters of the simulation have to be specified which is not true for = the registration of the code.

=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D
Main Items
=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=A0


Items required to register a code = :
1 = - Name of the code
2 - Name of the developper / team / = contact
3 - Version of the = code
4 - Description of the = code
5 - Physical = processes
6 - Subject
7 = -=A0 = Algorithm
8 - Time evolution
9 - Type of = results
10 - Results format
11 - Associated = tools
12 - Web address

Items required to register simulation results = :
1 = - Name of the dataset=A0
2 - Name of the developpers / team / = contact=A0
3 - Version of the dataset=A0
4 - = Description
5 - Physical = processes
6 - Subject
7 - = Algorithm
8 - Time evolution
9 - Type of = results
10 - Results formats
11 - Associated = tools
12 - Web address
13 - = Provenance=A0
14 - Results parameters =A0


=46rom 1 to 12 it = is similar to the registration of codes.=A0
13 - Provenance : = should give access to the code used to produce the dataset (optional in = case of simulation results coming from a code not described in the = VO)
14 - Result parameters : should give the parameters corresponding = to the production of the simulation results. It is difficult to discuss = this item now since it is directly linked to datamodels that we do not = have now.



1 --- Name of the = code = --------------------------------------------------------------------------= -------------------------
Description : Give the name of the = code
Required : YES
Multiple choice : NO
List : NO
Examples : Zeus, Ramses, Cloudy , ....=A0
Note : A UCD seems to exist : meta.id


2 --- Name of the = developpers / team / contact = -------------------------------------------------------------------=
Description : Give the name of the developpers = =A0
Required : Yes
Multiple choice : yes
List : no=A0
Examples : Albert E.
Note : 1 - Implementation done. UCD is = meta.curation

3 --- Version of = the code = --------------------------------------------------------------------------= --------------------
Type:
Required : yes
Multiple choice : no
List : no=A0
Examples :=A0
Note :=A0= =A0
- Herv=E9 suggested to use common standards = for versionning
- A UCD seems to exist for that : = meta.version

4 --- Description = of the code = --------------------------------------------------------------------------= -------------
Description : ASCII text describing the code = / the simulation results
Required : yes
Multiple choice : no
List : no list
Note : Should be covered by the UCD meta.note = (?)


5 --- Physical Process = --------------------------------------------------------------------------= -----------------------=A0
=A0 =A0 =A0 Description :=A0 General keywords to describe the physical = processes that the code deal with=A0
Required : yes
Multiple choice : yes=A0
List : MNRAS keywords, section "Physical data and processes" = :=A0 = http://www.bl= ackwellpublishing.com/pdf/mnraskey.pdf
Examples : MHD, radiative transfer, molecular processes, = gravitation, ...
Note : To avoid problems of synonyms during = the search a list may be required. In the list on the former twiki page, = nearly all words can be found in the thesaurus but sometimes the meaning = is not as precise as we would wish. Does it seem sufficient ? = =A0


6 --- Subject = --------------------------------------------------------------------------= -----------------------------------
=A0 =A0 =A0 = = Description : = General keywords describing the kind of objects the code can deal = with
Required : yes
Multiple choice : yes
Examples : Star, Galaxy, Large scale structures, Molecular = clouds, ...=A0
Note :=A0 1 -=A0 Advange to use a list is that the search = should be easier since it will avoid synonyms
=A0=A0 = =A0 2 = -=A0 = All words can be = found in the thesaurus.
7 = ---- Algorithm -------------------------------------------------------------------= -------------------------------------
Description : Most important algorithms in the = code=A0
Required : optional
Multiple choice : yes
List : Yes but has to be = defined
Examples : nbody, tree, sph, Ali, = ...
Note :=A0= 1 - A list is = necessary for an efficient search or we will have troubles with specific = numerical methods and synonyms
= =A0 = 2 - On the other = hand, new algorithms can be found and a fixed list is a = problem.=A0
Example :In radiative transfer it is = necessary to specify algorithm. Up to now the main ones were : LVG, = Monte-Carlo and Ali.=A0= But recently Moshe = Elitzur for Kentucky university has just found a new revolutionnary = method called CEP. How would it be possible to add this to a fixed list = ?=A0
=A0=A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = 3 - I choosed to = group algorithm and time evolution algorithm. As numericians we clearly = do the difference between the two, but this separation may not be = required in the registries. Since multiple-choice are possible for this = item, the time evolution algorithm should be=A0 =A0 =A0 =A0

8 ---- Time evolution = --------------------------------------------------------------------------= -----------------------
Description : Flag saying if the code is = stationnar or time dependant
Required : yes
Multiple choice : yes
List : 2 possibilities : yes or = no=A0


9 ---- Type of result = --------------------------------------------------------------------------= -------------------------
Description : Give the type of results :
Required : yes
Multiple choice : yes
List : yes
- table
- = VO-table
- spectre
- = VO-spectre
- snapshot
- = animation
- fits
- = catalog
=A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0= =A0 =A0 - = statistics
=A0 =A0 =A0 =A0 Note : 1 - The list has to be = completed.
=A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = 2 - Should we add = to the list : "rawdata" for binary results from a simulation = ?


10 --- Results formats = --------------------------------------------------------------------------= -----------------------
Description : Give the format of the = results
Required : yes
Multiple choice : yes
List : yes
- = ASCII / binary
- HDF5
- = giff, jpeg, ...
- mpeg4, quicktime, = ...
Note : This information could be usefull to find a code producing = outputs in a specific format to be plug in a = workflow.
11 --- Associated tools = --------------------------------------------------------------------------= --------------------
Description : give the name in the VO = registries of associated tools to the code
Required : no
Multiple choice : yes
List : no
Note : 1 - This would be usefull if a user = looking for a code could find with the description of the code, = associated VO-service for this code. For example the name/acess to a = theoretical database of results produced by this code, or the name of = another code used to analyse the results of the first = code.=A0


12 --- Web Adress = --------------------------------------------------------------------------= --------------------------
Description : give the web address where to = access the code / simulation result
Required : yes
Multiple choice : no
List : no
Note : A UCD exists for that : = meta.ref.url

=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D
Simulation = results
=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D


13 - = Provenance=A0
Description : Give the name of the code used = to produce the theoretical data
Required : Optional=A0
Multiple : No (yes for results from the = combination of 2 codes ? )
List : no
Note : 1 - Optional since the code used to produce the data may = not be registered


14 - Results = parameters
Description : Give the parameters used to = produce the data
Required : yes
Mutliple : yes
List : no
Note: 1 - Maybe it is too early to know how to deal with this = item since it is directly linked to datamodel(s)



=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D
B **** Thesaurus = Keywords
=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D

Do the keywords of = the thesaurus cover all the physical processes :

=A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0= =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 Thesaurus
  • =A0=A0 =A0 =A0 =A0 =A0 =A0 =A0 radiative transfer =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0= =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = Yes
  • =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 gravitational dynamics=A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0= =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 Gravitation
  • =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 GR What does GR means ? (General Relat. ?) = =A0 =A0 = relativity
  • =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 hydrodynamics =A0= =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 Yes
  • =A0 =A0 =A0 =A0 =A0= =A0 =A0 =A0 fluid dynamics =A0= =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 What is the difference with hydro = ?
  • =A0=A0 =A0 =A0 =A0 =A0 =A0 =A0 = plasma = physics=A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 Plasma
  • =A0=A0 =A0 =A0 =A0 = =A0 =A0 =A0 magneto-hydrodynamics=A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0= =A0 =A0 =A0 =A0 =A0 Yes
  • =A0=A0 =A0 =A0 =A0 = =A0 =A0 =A0 stellar evolution=A0= =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 No --- see subject = below
  • =A0=A0 =A0 =A0 =A0 = =A0 =A0 =A0 stellar population synthesis =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0= =A0 =A0 =A0 =A0 =A0 =A0 =A0 No --- see subject = below
  • =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 photoionization=A0= =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 atomic processes / molecular = processes
  • =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 photodissociation=A0= =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 molecular = processes
  • physical process = (secondary?)
    • = hydrostatic = equilibrium (atmosphere?)=A0= =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 No (but may be covered by an hydrodynamics = physical process and a stationnary algorithm)=A0



=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D

subject

=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D


=A0=A0 =A0 =A0 =A0 = =A0 Subject = =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 Thesaurus=A0

  • =A0 =A0 =A0 =A0 =A0= star=A0 =A0 =A0 =A0 =A0= =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = star:individual:
  • =A0=A0 =A0 =A0 =A0 = =A0 stars=A0= =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = =A0 =A0 stars:
  • =A0=A0 =A0 =A0 =A0 = =A0 stellar = clusters=A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 galaxies: star clusters
  • =A0=A0 =A0 =A0 =A0 = =A0 galaxy=A0= =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = galaxies = :
  • =A0 =A0 =A0 =A0 =A0 volume of space=A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0= =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = =A0
  • =A0 =A0 =A0 =A0 =A0 = accretion = disc(k)=A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0
  • =A0 =A0 =A0 =A0 =A0 = jet=A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = =A0 ISM: jets and = outflows
  • =A0 =A0 =A0 =A0 =A0 = interstellar = medium =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 ISM
  • =A0 =A0 =A0 =A0 =A0 = molecular cloud = =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 ISM : clouds
  • =A0 =A0 =A0 =A0 =A0 = atmosphere (of = planet, exo-planet, star...)=A0 =A0 =A0 =A0 =A0 =A0 =A0 stars:atmosphere, nothing for planet = atmosphere
  • =A0 =A0 =A0 =A0 =A0 = stellar = evolution =A0= stars: = evolution
  • =A0=A0 =A0 =A0 =A0 = stellar population = synthesis=A0 =A0 =A0 =A0 =A0 = =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = stars: evolution / = galaxy: evolution (?)

=A0

=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D
Algorithm
=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D= =3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D=3D

=A0 =A0 *=A0 nbody (What does = it mean ? particle-particle ? )
=A0 =A0 = = = * = mesh
=A0 =A0 * collisionless (not an algorithm ? - just a = physical approach ? )
=A0 =A0 * eulerian grid
=A0 =A0 = = = * lagrangian = grid
=A0 =A0 * tree
=A0 =A0 = = = * adaptive = refinement mesh
=A0 =A0 * adaptive refinement = tree
=A0 =A0 * sph
=A0 =A0 = = = * = tree-sph
=A0 =A0 * pppm
=A0 =A0 = = = * = pm
=A0= =A0 * = pp (What is "nbody" compare to pp ? )
=A0 =A0 = = = * fokker-planck = codes
=A0 =A0 * vlasov solvers
=A0 =A0 = = = * orbit = solver
=A0 =A0 * pic (particle in = cell)
=A0 =A0 * tree-pm
=A0 =A0 = = = * scf (self = consistent field)
=A0 =A0 * ffm (fast multipole = method)
=A0 =A0 * schwarzschild
=A0 =A0 = = = * ppm (piecewise = parabolic method)
=A0 =A0 * plm (piecewise linear method =3D = godunov)
=A0 =A0 * Isochrone synthesis
=A0 =A0 = = = * Fuel consuption = theorem
=A0=A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 =A0 = * Spectral = method

* = Radiative transfer code :
* ETL
* = LVG
* = Monte-Carlo
* ALI
* = CEP


=A0=A0 =A0 =A0 =A0 = =A0 =A0 o leap = frog
=A0 =A0 =A0 =A0 =A0 o individual = timesteps
=A0 =A0 =A0 =A0 =A0 o static
=A0 =A0 =A0 = = =A0 =A0 = o adaptative = timesteps
=A0 =A0 =A0 =A0 =A0 =A0 o runge-kutta
=A0=A0 =A0 =A0 = =A0= =A0 = o symplectic = integrator
=A0=A0 =A0 =A0 =A0 =A0 =A0 =A0 = Gear
=A0 =A0 =A0 Predictor/Corrector

= --Apple-Mail-18-626540190-- From owner-theory@eso.org Tue Jun 20 10:32:18 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k5K8W7P0004961 for ; Tue, 20 Jun 2006 10:32:07 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k5K8W72C004960 for theory-outgoing; Tue, 20 Jun 2006 10:32:07 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k5K8W1P0004934 for ; Tue, 20 Jun 2006 10:32:02 +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 k5K8VwQk024408 for ; Tue, 20 Jun 2006 10:31:59 +0200 (CEST) Received: from [161.111.165.126] (dae-d26.iaa.csic.es [161.111.165.126]) by iaa13u.iaa.csic.es (8.9.3/8.9.1) with ESMTP id KAA04574; Tue, 20 Jun 2006 10:31:44 +0200 (MET DST) In-Reply-To: <80909CA7-81A7-424F-9712-481D7E57E743@obspm.fr> References: <80909CA7-81A7-424F-9712-481D7E57E743@obspm.fr> Mime-Version: 1.0 (Apple Message framework v750) Content-Type: multipart/alternative; boundary=Apple-Mail-1-686402058 Message-Id: <3F000330-506F-4C7B-8A04-00BF08ED5584@iaa.es> Cc: theory@ivoa.net From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Re: [SEMANTICS] Re: semantics Date: Tue, 20 Jun 2006 10:31:33 +0200 To: Franck Le Petit X-Mailer: Apple Mail (2.750) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.6.20.5432 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= --Apple-Mail-1-686402058 Content-Transfer-Encoding: quoted-printable Content-Type: text/plain; charset=ISO-8859-1; delsp=yes; format=flowed Dear theory group, I just want to make two comments about previous e-mails regarding semantics and population synthesis issues =20 mainly. Respecting Franck e-mail, As far as I understand UDCs, > - Is the item a required information or an optinal one for =20 > registration ? It should used for describe the data (the model =20= in our case), the registration of services is a different issue: It is not needed any UDC for a =20 registration! The register only provides the possible services, but it do not carry too much about =20 what is inside the service (data types, udcs, etc), but what is the protocol that you use to =20 access it: TSAP, SSAP, etc... I just revised previous e-mails, and I think =20 that, for the moment, it will not possible to ask the registry for a " radiative transfer code using the Ali =20= method" as example, as well as it is not possible to ask to the register for a IUE spectra of =20 NGC 1068 taken during 1994... (the register do not search in each VOService, only says =20 which VOService are aviable...) (Any case, although the registry do not work in such a =20 way, the exercise will we an interesting effort for the future, and I think =20 that it is interesting to build services that would work sometime in this way) In the other hand, UCD is a list of "concepts", =20 but not a list of manes! i.e.: Cloudy whould be a "value" of a field with given UCD words. > - Are multiple choice possible or not ? =BFwhat do you mean? > - Do the values associated to the UCDs have to be choosen from a = =20 > given list or not and if yes, from which list ? You can find the current list of UCDs at: http://www.ivoa.net/Documents/latest/=20 UCDlist.html And the process to add UCDs in the list at (IVOA =20= recomendation): http://www.ivoa.net/Documents/latest/=20 UCDlistMaintenance.html However, THERE IS NO LIST of the values associated =20= with it: the same UCD would have different values (that will depends at the end on =20 the developer of the service). The UCD only tries to delimiter the "concept", but not its =20= value. Any search in UCDs aims to look for concepts (example theory) Note about "synthesis model" in "algorithm": I do not know exactly =20 were synthesis models (or an isocrhone, or an atmosphere models) =20 would fit I think that may be it is good as value related with the SUBJECT: =20 "stars" for isochrones, and "stellar clusters" (or may be better, =20 "stellar populations") for synthesis models. Any case, the types of algorithms used in =20 synthesis models are: Isocrone synthesis or Fuel Comsuption theorem =20 (that was yet included). In the other side, Monte Carlo simulations =20 are a "way" to use the algorithm. (Althought Monte Carlo simulations =20 has their own meaning as a particular algorithm). Any case, from the UCD point of view, there will be no problem, since =20= the algorimth is a posterior characterzation of the main class, subject. > > Apart these modifications we see several difficulties up to now = : > 1 - for the algorithms, the list may become very very long = and so =20 > unusable for an efficient search in the registries. A solution has =20 > to be find... > I think that the final goal is not to include all the =20 "algorithms" as UDCs words. The idea of the list would be better =20 understood as a list of possible values where we must try to classify in a =20 few classes of concepts (that will be the final UCD) > 2 - Bernard Debray mentionned a very nice problem adding to = the =20 > twiki page "Stellar synthesis Populations" in "physical processes". > This is neither a "physical process", nor an = "algorithm", nor a =20 > "subject". But that is the way everybody call such codes. I think that whatever people would cal it, =20 correct or incorrectly, the issue here is how a "machine" will =20 recognize it ;) No human will examine the register, but =20 machines... The important point (that is a different issue) is how a =20 machine translate the human words (natural language) =20 to the VOServices, etc... Maybe it is ussefull to visit the UCD builder =20 at ADS to understand the point: http://cdsweb.u-strasbg.fr/UCD/cgi-bin/=20 descr2ucd > Should not we add a new item "Category of code" to cover = large =20 > domains of codes with a finite list of possibilities as : I completely aggre, I think that it is just =20 the things we need now: to find class of concepts this case, the UCD =20 will be "category of code" and the list below, the =20 possible values (an important note: In the list, some =20 developer would give a value of the category "hydrodynamic" and other, "hydrodynamic simulation" of =20 "simulaci=F3n hidrodin=E1mica", and I think that IVOA do not care about =20= these issues..., but I am not completely sure) > - Large structures formation > - Hydrodynamic > - MHD > - Stellar synthesis populations > - PDR > - Numerical Relativity > - Radiative transfer > - ... > > In some cases, the value associated could be the same as = in =20 > "physical processes" but not always as for "stellar population =20 > synthesis". It would help a lot the search in registries. > 3 - The item "Result parameters" seems unuseful for the =20 > registration of codes. It may be useful for the registration of =20 > simulation results but it is completly linked to the datamodel =20 > describing the simulation results. So I suggest to forget it for =20 > the moment. I agree, but before to register a code, I think that is =20 more important to define what the code do! What is the goal? include codes in the register that only =20= the code developers will use? define the data model? or try to define =20= both at the same time, given that they are intrinsically related? (by the way, I just included an item called "output", =20 with subitems like photometric evolution, spectral energy =20 distribution or luminosity distribution function... I think we have forgot that most of possible search will =20 be done looking for the final result!, may be it was some way =20 included in the other items, but not explicitly) > > 4 - I added a new item "Description" where it would be = possible =20 > to add an ASCII text describing the code. This exist yet in the =20 > registration of any VO service in the present registries. I do not =20 > know if the registries will allow to search by words in such =20 > description. Does anybody know if we plan to have in the VO a tool =20= > as "spotlight" in the Mac OS X which is able to find any document =20 > when we give it a few words contained in this document ? > In the VOTable definition, there is a FIELD called =20 DESCRIPTION for this propose. However, I think that you refer to an =20 "human readable" text more suitable for publications, isn't it? After Victoria meeting I was wondering a bout a =20 similar issue, but more focused in have some "latex ready tex" that =20 can be directly cut&paste in scientific production. In particular, it is also =20 related with "credits" and it also affects the modification of =20 VOtables by any application. I think that the issue is in fact to define a field that should be =20 "human redeable". In UCDs, there is the word "meta", and I have seen =20= in any VOTable someting like "meta.human". Any case, completely agree with the =20 point, although I would prefer to include in such UCD a detailed =20 scientific descriptions, that means, also references. Any case it is intimately connected with the =20 Application group: At the end, users will not look inside VOTables, =20 but they will use applications to work with them, so any attempt in this direction will have no =20 result if we are not coordinate with the App. group... Cheers Miguel= --Apple-Mail-1-686402058 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1 Dear theory group, I just want = to make two comments about=A0
previous e-mails regarding semantics = and population synthesis issues mainly.

Respecting Franck = e-mail,
As far as I understand UDCs,

- = Is the item a required information or an optinal one for registration = ?
=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 = =A0=A0 =A0=A0 =A0It should used for describe the data (the model in our = case), the registration of services is
=A0 =A0 =A0=A0 =A0=A0 = =A0=A0 =A0a different issue: It is not needed any UDC for a = registration! The register only provides the=A0
=A0 =A0 =A0=A0 = =A0=A0 =A0=A0 =A0possible services, but it do not carry too much about = what is inside the service (data types,
=A0 =A0=A0 =A0=A0 =A0=A0= =A0=A0 udcs, etc), but what is the protocol that you use to access it: = TSAP, SSAP, etc...
=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0= I just revised previous e-mails, and I think that, for the moment, it = will not possible to ask the
=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 = registry for a " radiative transfer code using the Ali method" as = example, as well as it is not
=A0 =A0 =A0=A0 =A0=A0 =A0=A0 = =A0possible to ask to the register for a IUE spectra of NGC 1068 taken = during 1994... (the
=A0 =A0 =A0=A0 =A0=A0 =A0=A0 =A0register = do not search in each VOService, only says which VOService are = aviable...)
=A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0(Any case, although = the registry do not work in such a way, the exercise will
=A0=A0= =A0=A0 =A0=A0 =A0=A0 =A0we an interesting effort for the future, and I = think that it is interesting to build services
=A0=A0 =A0=A0 = =A0=A0 =A0=A0 =A0that would work sometime in this way)
=A0=A0 = =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0In the other hand, UCD is a list = of "concepts", but not a list of manes! i.e.: Cloudy
=A0 =A0 = =A0=A0 =A0=A0 =A0=A0 =A0whould be a "value" of a field with given UCD = words.
=A0=A0

- = Are multiple choice possible or not = ?
=A0 =A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0= =A0=BFwhat do you mean?=A0
=A0=A0 =A0

- = Do the values associated to the UCDs have to be choosen from a given = list or not and if yes, from which list ? =A0 =A0 = =A0
=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 = =A0=A0 =A0You can find the current list of UCDs at:
=A0=A0 =A0=A0= =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0http://www.ivoa= .net/Documents/latest/UCDlist.html
=A0 =A0=A0 =A0=A0 =A0=A0 = =A0=A0 =A0=A0 =A0And the process to add=A0 UCDs in=A0 the list at (IVOA = recomendation):
=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 = =A0=A0 =A0=A0 =A0http= ://www.ivoa.net/Documents/latest/UCDlistMaintenance.html
=A0= =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0However, THERE IS NO LIST of the = values associated with it: the same UCD would have
=A0 =A0=A0 = =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0different values (that will depends at = the end on the developer of the service). The UCD
=A0 =A0=A0 = =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0only tries to delimiter the "concept", = but not its value. Any search in UCDs aims to
=A0 =A0=A0 =A0=A0 = =A0=A0 =A0=A0 =A0=A0 =A0look for concepts (example theory)

Note about "synthesis = model" in "algorithm": I do not know exactly were synthesis models (or = an isocrhone, or an atmosphere models) would fit
I think that = may be it is good as value related with the SUBJECT:=A0 "stars" for = isochrones, and "stellar clusters" (or may be better, "stellar = populations")
for synthesis models.=A0Any case, the types of = algorithms used in synthesis models are: Isocrone synthesis or Fuel = Comsuption theorem (that was yet included). In the other side,=A0Monte = Carlo simulations are a "way" to use the algorithm. (Althought Monte = Carlo simulations has their own meaning as a particular = algorithm).
Any case, from the UCD point of view, there will = be no problem, since the algorimth is a posterior characterzation of the = main class, subject.=A0


Apart these modifications we see several = difficulties up to now :
1 - for the algorithms, the list may become very very long and so = unusable for an efficient search in the registries. A solution has to be = find...
=A0 =A0 =A0=A0 =A0=A0 =A0=A0 = =A0I think that the final goal is not to include all the "algorithms" as = UDCs words. The idea of the list would be better understood as a = list
=A0 =A0 =A0=A0 =A0=A0 =A0=A0 =A0of possible values where = we must try to classify in a few classes of concepts (that will be the = final UCD)


2 = - = Bernard Debray = mentionned a very nice problem adding to the twiki page "Stellar = synthesis Populations" in "physical processes".=A0
This is neither a "physical process", nor an "algorithm", nor a = "subject". But that is the way everybody call such = codes.=A0

=A0=A0 =A0=A0 =A0=A0 =A0=A0 = =A0=A0 =A0=A0 =A0=A0 =A0I think that whatever people would cal it, = correct or incorrectly, the issue here is how a "machine" will recognize = it ;)
=A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0No = human will examine the register, but machines... The important point = (that is a different issue) is how a machine
=A0=A0 =A0=A0 =A0=A0= =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0translate the human words (natural = language) to the VOServices, etc...
=A0=A0 =A0=A0 =A0=A0 =A0=A0 = =A0=A0 =A0=A0 =A0=A0 =A0
=A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0= =A0=A0 =A0Maybe it is ussefull to visit the UCD builder at ADS to = understand the point:

=A0 =A0 =A0=A0 =A0=A0 =A0=A0 = =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0http://cdsweb.u-= strasbg.fr/UCD/cgi-bin/descr2ucd=A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 = =A0=A0 =A0

Should not we add a new item "Category of code" to cover large = domains of codes with a finite list of possibilities as = :
=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 = =A0=A0 =A0=A0 =A0=A0 =A0I completely aggre, I think that it is just the = things we need now: to find class of concepts=A0this case, the UCD will = be=A0
=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 = =A0"category of code" and the list below, the possible = values
=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 = =A0(an important note: In the list, some developer would give a value of = the category "hydrodynamic" and
=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 = =A0=A0 =A0=A0 =A0=A0 =A0other, "hydrodynamic simulation" of "simulaci=F3n = hidrodin=E1mica", and I think that IVOA do not care about these = issues...,
=A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0= but I am not completely sure)
=A0=A0
- = Large structures formation
- Hydrodynamic
- = MHD
- = Stellar synthesis populations
- PDR
- = Numerical Relativity
- Radiative transfer
- = ...

In some cases, the value associated could be the same as in = "physical processes" but not always as for "stellar population = synthesis".=A0 =A0It would = help a lot the search in = registries.


3 = - = The item "Result = parameters" seems unuseful for the registration of codes. It may be = useful for the registration of simulation results but it is completly = linked to the datamodel describing the simulation results. So I suggest = to forget it for the moment.

=A0 =A0 =A0=A0 =A0=A0 =A0I = agree, but before to register a code, I think that is more important to = define what the code do!=A0
=A0 =A0 =A0=A0 =A0=A0 =A0What is = the goal? include codes in the register that only the code developers = will use? define the data model? or try to define both at the = same
=A0 =A0 =A0=A0 =A0=A0 =A0time, given that they are = intrinsically related?
=A0 =A0 =A0=A0 =A0=A0 =A0(by the way, I = just included an item called "output", with subitems like photometric = evolution,=A0 spectral energy distribution or luminosity distribution = function...
=A0 =A0 =A0=A0 =A0=A0 =A0I think we have forgot = that most of possible search will be done looking for the final result!, = may be it was some way included in the other items, but
=A0 =A0 = =A0=A0 =A0=A0 =A0not explicitly)


4 = - I = added a new item "Description" where it would be possible to add an = ASCII text describing the code. This exist yet in the registration of = any VO service in the present registries. I do not know if the = registries will allow to search by words in such description. Does = anybody know if we plan to have in the VO=A0 a tool as "spotlight" in the Mac OS X which = is able to find any document when we give it a few words contained in = this document ?=A0
=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 suitable for = publications, isn't it?
=A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 =A0After = Victoria meeting I was wondering a bout a similar issue, but more = focused in have some "latex ready tex" that can be directly = cut&paste
=A0 =A0=A0 =A0=A0 =A0=A0 =A0in scientific = production. In particular, it is also related with "credits" and it also = affects the modification of VOtables by any application. I think = that=A0
=A0=A0 =A0=A0 =A0=A0 =A0=A0 the issue is in fact to = define a field that should be "human redeable". In UCDs, there is the = word =A0"meta", and I have seen in any VOTable someting
=A0=A0 = =A0=A0 =A0=A0 =A0=A0 like "meta.human". Any case, completely agree with = the point, although I would prefer to include in such UCD a detailed = scientific descriptions, that
=A0 =A0=A0 =A0=A0 =A0=A0 =A0means,= also references.
=A0 =A0 =A0=A0 =A0=A0 =A0=A0 =A0=A0 Any case = it is intimately connected with the Application group: At the end, users = will not look inside VOTables, but they will use applications to = work=A0
=A0 =A0 =A0=A0 =A0=A0 =A0with them, so any attempt in = this direction will have no result if we are not coordinate with the = App. group...


Cheers

= Miguel
= --Apple-Mail-1-686402058-- From owner-theory@eso.org Thu Jun 22 01:30:26 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k5LNUFeA025550 for ; Thu, 22 Jun 2006 01:30:15 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.12.10+Sun/8.12.10/Submit) id k5LNUFfG025549 for theory-outgoing; Thu, 22 Jun 2006 01:30:15 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k5LNU6eA025519 for ; Thu, 22 Jun 2006 01:30:06 +0200 (MEST) Received: from noao.edu (noao.edu [140.252.1.54]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k5LNU1Qk006785 for ; Thu, 22 Jun 2006 01:30:02 +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 [140.252.1.227] (account deyoung@noao.edu) by noao.edu (CommuniGate Pro WebUser 5.0.9) with HTTP id 27824483; Wed, 21 Jun 2006 16:29:54 -0700 From: "Dave DeYoung" Subject: Re: [SEMANTICS] Re: semantics To: Franck Le Petit Cc: theory@ivoa.net X-Mailer: CommuniGate Pro WebUser v5.0.9 Date: Wed, 21 Jun 2006 16:29:54 -0700 Message-ID: In-Reply-To: <80909CA7-81A7-424F-9712-481D7E57E743@obspm.fr> References: <80909CA7-81A7-424F-9712-481D7E57E743@obspm.fr> 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: 2.4.0.264935, Antispam-Data: 2006.6.21.153432 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: "Dave DeYoung" Dear Franck and Fabrice; I think you have done an excellent job in your carefully prepared proposal. There is a great deal of detail in the description of your 14 items that will require careful consideration by all of us. I note in passing that the thesarus is still rather incomplete, especially in the area of subject and somewhat in the area of physical processes. However, this is easily addressed. Thanks for your proposal. Dave De Young From owner-theory@eso.org Fri Jul 21 20:48:31 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k6LImAdo007996 for ; Fri, 21 Jul 2006 20:48:10 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6LImAJ8007995 for theory-outgoing; Fri, 21 Jul 2006 20:48:10 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k6LIm61h007989 for ; Fri, 21 Jul 2006 20:48:06 +0200 (MEST) Received: from ppsw-0.csi.cam.ac.uk (ppsw-0.csi.cam.ac.uk [131.111.8.130]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k6LIm1um017761 for ; Fri, 21 Jul 2006 20:48:04 +0200 (CEST) X-Cam-SpamDetails: Not scanned X-Cam-AntiVirus: No virus found X-Cam-ScannerInfo: http://www.cam.ac.uk/cs/email/scanner/ Received: from cass41.ast.cam.ac.uk ([131.111.69.186]:46127) by ppsw-0.csi.cam.ac.uk (ppsw.cam.ac.uk [131.111.8.130]:25) with esmtp id 1G402I-0000C5-1f (Exim 4.54) for theory@ivoa.net (return-path ); Fri, 21 Jul 2006 19:47:42 +0100 Received: from cass25.ast.cam.ac.uk (cass25 [IPv6:2001:630:200:4240:203:baff:fe24:314]) by cass41.ast.cam.ac.uk (8.13.6+Sun/8.13.6) with ESMTP id k6LIlgU6019160 for ; Fri, 21 Jul 2006 19:47:42 +0100 (BST) Received: from cass25.ast.cam.ac.uk (localhost [127.0.0.1]) by cass25.ast.cam.ac.uk (8.13.7+Sun/8.13.7) with ESMTP id k6LIlgxi013184 for ; Fri, 21 Jul 2006 19:47:42 +0100 (BST) Received: from localhost (lds@localhost) by cass25.ast.cam.ac.uk (8.13.7+Sun/8.13.7/Submit) with ESMTP id k6LIlfqH013181 for ; Fri, 21 Jul 2006 19:47:42 +0100 (BST) X-Authentication-Warning: cass25.ast.cam.ac.uk: lds owned process doing -bs Date: Fri, 21 Jul 2006 19:47:41 +0100 (BST) From: Laurie Shaw X-X-Sender: lds@cass25 To: theory@ivoa.net Subject: [SEMANTICS] Simulation Categories and Standard Vocab words 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: 2.4.0.264935, Antispam-Data: 2006.7.21.105432 X-Virus-Scanned: by amavisd-new Sender: owner-theory@eso.org Precedence: bulk Reply-To: Laurie Shaw Dear theory group, I would just like to make a few comments (rather belatedly) on the Semantics discussion, especially the emails by Frank, Herve and Miguel. I've listed my points by topic. UCDs vs Standard Vocabulary ---- It seems that there is a little confusion on whether we are trying to define new UCDs or words for the Standard Vocabulary. Initially, on the twiki page (http://www.ivoa.net/twiki/bin/view/IVOA/TheorySemanticVocabulary) we outlined lists of words under various categories (e.g. physical process, subject, algorithm, etc) describing various different types of simulation properties. In his email, Frank Le Petit then defined a specific set of categories that must be filled in in order to describe the purpose and operation of a piece of simulation code (to be published in the VO) adequately. As far as I understand it, we will require there to be a UCD describing each of the categories that we eventually come up with. However, the words that we use to populate a category will come from the IVOA standard vocabulary (a vocabulary that encompasses the set of words that can be used as UCDs, plus all standard terms that are currently in use in astronomy (in UCD syntax)). So, eventually, once we have decided on a set of categories, we will need to propose a UCD for each category, plus words for the standard vocabulary that will be used within these categories that we identify as being necessary in order to ensure that most astrophysical simulation codes can be adequately represented. Simulation Categories ---- The set of simulation categories that must be filled in order to fully describe a simulation that were proposed by Franck are as follows: 1 - Name of the code 2 - Name of the developer / team / contact 3 - Version of the code 4 - Description of the code (ASCII text) 5 - Physical processes 6 - Subject 7 - Algorithm 8 - Time evolution 9 - Type of results 10 - Results format So far, it seems like no-one has any problems with the first three, each of which I think there already exists a UCD (meta.id, meta.curation, meta.version, meta.note). I don.t think that we need define any new standard vocabulary (SV) words for these as they are all fairly specific to each simulation, although, it could be argued that the .Name. be part of the SV as simulated datasets may point to this tag.?? The next four categories on the hand seem to be the most important (at least in terms of defining new SV words) as they entirely describe what the code is trying to do and how it does it. Taking the .Subject. category first, which describes the astrophysical objects that the code is primarily dealing with, looking at the IVOA standard vocabulary as it is now (http://www.ivoa.net/internal/IVOA/IvoaUCD/VO-standard-vocabulary_8.pdf) it seems like many of the objects are already roughly accounted for (I.ve only had a quick glance at this though). The only things that I can see that are not there are Dark matter halo (and subhalo) and volume of space. Note that we can still use the UCD syntax and structure for SV words, so .stellar cluster. is .stars.globular.cluster. or .stars.cluster.. The .physical process. and .algorithm. categories are by far the most complicated due to the sheer range of physical processes that are modelled, in how much detail (approximations or exactly), their relative impact on the results (does a process, e.g. stellar feedback, have a major or minor effect on whatever is being simulated) and how it is incorporated. It seems to me that .physical process. could mean two things here . 1) the overall phenomenon that is being simulated (e.g. galaxy *formation*, stellar *evolution*) 2) the physics that is accounted for in doing so, (e.g. radiative transfer, GR, etc) We could either go the way of having two separate categories, one for .process. and one for .physics., or just keep .physical process. and have multiple entries that together define what is going on, and the physics that is making it happen. It should be noted here that there is already a .process. field in the SV (e.g. procees.accretion, process.emission, etc), so I guess we have to propose those that are missing, e.g. process.radtransfer, process.evolution). So for stellar evolution we might have, .stars. in the Subject category and .process.evolution. and .process.radTransfer. in the Physical Processes category (or, alternatively, have the last two in separate Process and Physics categories). I.m wondering whether this approach gets past the Process or Subject? category problem for .stellar evolution. and .stellar population synthesis. that Herve pointed out. Algorithm ---- As others have pointed out, for this category I think we have to be careful not to be too specific else there will end up being millions of words in the SV list for .comp.algorithm. (or whatever it ends up being called). I think that the words required for this category should only refer to the top-most level algorithm. Looking at the list on the twiki, it seems that some of the words suggested are almost code Names or Physical Processes -- I don.t think .collisionless. or .Fuel consumption theorem. are algorithms (although I could be wrong). Furthermore, tpm, pppm, pm, pp, etc, are all types of Nbody code, so the word for tpm might be .comp.alg.Nbody.tpm., whilst I.m guessing .adaptive refinement mesh. would be .comp.alg.mesh.adaptive-refinement. , or something like that. I.m thinking that in the near term most of the entries for algorithm will be under .mesh., .hyrdo (including sph). or .nbody. with a few extras. If we decide to get more specific than this, then the number of words we.ll require to describe different simulations to the same degree with increase exponentially. If someone was to need more detail, they could always look at the .Description. category, or even a paper that that points to, having before rounded down the search to tree-sph, etc. Time Evolution -- Do we really actually need this? In terms of methods like .leap frog., etc, it seems like this is more for the Algorithm category (and a very specific detail at that). I would have though that the temporal resolution, included under some kind of Parameters category for individual simulated datasets might be more relevant. I agree with Franck that this should at most be a YES or NO flag with regards to whether the code is time dependant or not. Type of Results and Results Format --- I totally agree with Franck.s suggestion here.. Code language and .parallelism. --- I also propose a new category (Language?) for the language (c++, fortran, etc) in which the code is written and whether it is designed for use on multi-processor machines or clusters. I guess these could also be under two separate categories. Parallism could be either by protocol (mpi, openMP) or by a flag (yes/no). Single or Multiple Entries in each Category ---- I think that we should not place limits on any of the categories (except for maybe Version and Time Evolution) to just one entry. Could cause problems down the road as simulations get more and more powerful in size and especially scope. Would be great to hear peoples thoughts on these topics, and to make some decisions so that I can write a proposal that we agree on! Sorry for the long email, Cheers, Laurie From owner-theory@eso.org Wed Jul 26 20:03:32 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k6QI3FFC002950 for ; Wed, 26 Jul 2006 20:03:15 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k6QI3FRw002949 for theory-outgoing; Wed, 26 Jul 2006 20:03:15 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k6QI3B3C002937 for ; Wed, 26 Jul 2006 20:03:11 +0200 (MEST) Received: from tonali.inaoep.mx (tonali.inaoep.mx [192.100.172.5]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k6QI36um027428 for ; Wed, 26 Jul 2006 20:03:08 +0200 (CEST) Received: from calmecac.inaoep.mx (calmecac.inaoep.mx [192.100.172.51]) by tonali.inaoep.mx (Postfix) with ESMTP id 143987BB3; Wed, 26 Jul 2006 13:03:03 -0500 (CDT) Received: from localhost (localhost [127.0.0.1]) by calmecac.inaoep.mx (Postfix) with ESMTP id 4E923EB29; Wed, 26 Jul 2006 13:02:54 -0500 (CDT) X-Virus-Scanned: by amavisd-new Received: from calmecac.inaoep.mx ([127.0.0.1]) by localhost (calmecac.inaoep.mx [127.0.0.1]) (amavisd-new, port 10024) with ESMTP id QX3xpjIAq47V; Wed, 26 Jul 2006 13:02:50 -0500 (CDT) Received: from [192.168.13.234] (unknown [192.168.13.234]) by calmecac.inaoep.mx (Postfix) with ESMTP id D6D64EB20; Wed, 26 Jul 2006 13:02:50 -0500 (CDT) In-Reply-To: References: Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <0F0C5C0F-FDC1-4E99-90C6-C0244EFEA1DD@iaa.es> Cc: theory@ivoa.net Content-Transfer-Encoding: 7bit From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Re: [SEMANTICS] Simulation Categories and Standard Vocab words Date: Wed, 26 Jul 2006 13:02:52 -0500 To: Laurie Shaw 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: 2006.7.26.103432 Sender: owner-theory@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Dear Laurie, and all About your previous e-mail, I agree with you in most items :), however I have some comments: About the use of the "meta" atom to define the UDCs for theory for the first four items: 1 - Name of the code 2 - Name of the developer / team / contact 3 - Version of the code 4 - Description of the code (ASCII text) there has been a discussion in ucd-sci mailling list that would be interesting: http://www.ivoa.net/forum/ucd-sci/0607/0133.htm Anycase, about the use of meta.name vs. meta.id to describe the "name of the code" I think that meta.id makes a better job, since some times a code is identified not by its name, but by a reference (example: Bruzual & Charlot 1991 code is called GRISEL, but almost nobody knows it!) So, meta.id can be either the name of the code (if any) or a reference to a paper or web page that identifies the code. About the use of meta.curation for describe the "name of developer team", I am not sure to be a good solution: currently I am implementing a VO service with synthesis models (in agreement with several groups of model developers). In this situation I would we the responsable of the curation of the database, but I am not the developer of the models included in the service (this description should be in the provenance field of the VOTable, but not necessarelly in a service registry) I think that meta.curation has a very specific role in the VO. so, many be, the name of developer would be described better by "meta.ref". It also includes "meta.ref.url" for possible www pages of the developer, that would be different than the group that put the results in the VO, (may this solution would be useful for the additional items included in Franck's mail: 12 Web Adress and 13 Provenance) About the distinction between "physics" and "process", I think that Laurie'ssuggestion about keep two different categories for physics and process is quite good. And it helps to describe stellar population synthesis-like codes. However, I would be a bit more specific for some process like: process.evolution.spectrophotometric process.evolution.chemical However, I do not find place for an UCD for the Star Formation History or the Initial Mass Function (phys.SFH, phys.IMF?) as example. Any suggestion? > 7 - Algorithm Just a coment: Fuel Consumption theorem is a recipe (as well as isochrone synthesis) to perform the isochrone integration (a exchange of variable from mass in isochrones to time in tracks for fast evolutionary phases). Any case, it is not relevant now and I think that comp.algorithm without more detail is enough for population synthesis... > Code language and .parallelism. > --- I totally agree about the "protocol" atom. It would be also useful for the Web&Grid service group. Anyone knows how they would handle the possible Grid services? About the language.... It is really needed? I mean, it is an useful information for VO or it would define a code? I think that language aspects would be relevant for interop, but any case it should be used when in the registry of the service, not in the VOTable with the results of the code. May be I am wrong.... > Single or Multiple Entries in each Category > ---- > > I think that we should not place limits on any of the categories > (except > for maybe Version and Time Evolution) to just one entry. Could cause > problems down the road as simulations get more and more powerful in > size > and especially scope. I also agree. Multiple entries are needed for example for synthesis codes (that use the results of other codes like atmosphere libraries and evolutionary tracks) of SED fitting tools (that would use different synthesis models). Also it is useful for the description of pipeline process, isn't it? cheers Miguel From owner-theory@eso.org Tue Aug 29 18:58:27 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k7TGwD9Z020175 for ; Tue, 29 Aug 2006 18:58:13 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k7TGwDnG020174 for theory-outgoing; Tue, 29 Aug 2006 18:58:13 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k7TGwD0d020169 for ; Tue, 29 Aug 2006 18:58:13 +0200 (MEST) Received: from mpemail.mpe.mpg.de (mpemail.mpe-garching.mpg.de [130.183.137.110]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k7TGwBum005788 for ; Tue, 29 Aug 2006 18:58:11 +0200 (CEST) Received: from gavopc1.xray.mpe.mpg.de ([130.183.72.204] helo=gavopc1) by mpemail.mpe.mpg.de with esmtp (Exim 4.50) id 1GI6uW-0006Bo-TH; Tue, 29 Aug 2006 18:58:00 +0200 From: "Gerard" To: "'Claudio Gheller'" Cc: Subject: RE: VOTable for simulations Date: Tue, 29 Aug 2006 19:01:58 +0200 Message-ID: <003c01c6cb8c$d6ca7410$cc48b782@gavopc1> MIME-Version: 1.0 Content-Type: text/plain; charset="US-ASCII" Content-Transfer-Encoding: 7bit X-Mailer: Microsoft Office Outlook 11 Thread-index: Acar6HknwXcjAvi4RR2XVtNU67aSeQfovuEA X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2962 In-Reply-To: <44BF5CC4.6070006@cineca.it> X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.8.29.91442 Sender: owner-theory@eso.org Precedence: bulk Reply-To: "Gerard" Hi Claudio Sorry for the late reply to this email. I'm Cc-ing the theory group as well I gather you are thinking of grid simulation data here, so this mail does not apply to N-body. Anyway, for that I think we can use the VOTable spec as it stands, in particular section 5.3 dealing with binary serialisation (see http://www.ivoa.net/Documents/REC/VOTable/VOTable-20040811.pdf ). In the case you address, would it make sense to try to mimick FITS in the naming of key words, so use NAXIS for rank, and NAXIS1 for size0, NAXIS2 for size1 etc for the dimensions ? If I am not mistaken VOTable itself is based on the FITS binary table spec, so your proposal might be seen as a translation of a FITS datacube (IMAGE). Did we actually not think about using FITS as is for (uniform) grid simulations ? In that case your proposal could also be used I guess, where iso STREAM we'd have FITS as in standard VOTable usage (though I don't know whether votable presumes that the FITS file contains a table). I am not sure whether FITS images/datacubes allow multiple values per cell (i.,e. have an array size), but don't think so. Otherwise we could probbaly generalise in that direction. Do you propose to follow the VOTable/FITS directions on little-vs big-endian ? Cheers Gerard > -----Original Message----- > From: Claudio Gheller [mailto:c.gheller@cineca.it] > Sent: Thursday, July 20, 2006 12:37 PM > To: Gerard Lemson; Ugo Becciani; Alessandro Costa; Marco Comparato; R. > Smareglia > Subject: VOTable for simulations > > Dear friends, > > I have tried to figure out the structure of a VOTable for simulated > data. In the following the result. > I made the following assumptions: > > 1. data are binary > 2. the binary file is a raw stream of byte, with no structure (no fits, > no hdf...). It is external to the VOTable (at the moment I've not > considered base64 conversion for performance reasons) > 3. Each file has an XML descriptor associated. The descriptor at > present gives only the necessary infos to deal with the file. > 4. Each file contains ONE variable. This is suggested for the following > reasons > - data rank and size can change from variable to variable. > - complex description > - The association direct XML header file - bin file - variable, is > easier to handle. > - smaller files > - files easier to handle by external applications (also not VO-compliant) > - drawback: proliferation in the number of files > However we can consider the support to more complex files or even > formats, like FITS or HDF5. But let's start with something simple. > > At this point I made the Snap program create binary files (at present > still HDF5, but just for backward compatibility) and associated XMLs. > For example: > test.h5 ----> snapped data > test.h5.xml ----> associated VOTable: > > > xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" > xmlns="http://vizier.u-strasbg.fr/xml/VOTable-1.1.xsd > "> > >
> ucd="" datatype="float" arraysize="41x41x41" unit="Kelvin" /> > > > > > > > >
> > > > Notice that the rank and size of the dataset is expressed in the > arraysize keyword of FIELD. It is also written in the 4 PARAM fields. > This is just to avoid the parsing of the string to get the basic info of > rank and size and to have them directly as numbers (with their precise > type). At present there are no UCD and no reference to the SNAP > protocol, since both are not yet defined. I'm working on the latter... > > This is the very first attempt!!! Let me know all your comments. > Claudio > > -- > ------------------------------------ > Dr. Claudio Gheller, Ph.D. > High Performance System Division > CINECA - Bologna - Italy > Tel. +39-051-6171560 > Fax. +39-051-6137273 > ------------------------------------ From owner-theory@eso.org Thu Aug 31 14:55:49 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k7VCtdBE014800 for ; Thu, 31 Aug 2006 14:55:40 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k7VCtdkN014799 for theory-outgoing; Thu, 31 Aug 2006 14:55:39 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k7VCtdPY014795 for ; Thu, 31 Aug 2006 14:55:39 +0200 (MEST) Received: from as2.cineca.com (as2.cineca.com [130.186.84.242]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k7VCtaum016691 for ; Thu, 31 Aug 2006 14:55:36 +0200 (CEST) Received: from localhost (localhost.localdomain [127.0.0.1]) by as2.cineca.com (Postfix) with ESMTP id 9CE8A1D7; Thu, 31 Aug 2006 14:55:25 +0200 (CEST) Received: from cineca.mm.cineca.it (cineca.mm.cineca.it [130.186.10.200]) by as2.cineca.com (Postfix) with ESMTP id 98B49373; Thu, 31 Aug 2006 14:55:15 +0200 (CEST) Received: from [130.186.7.201] (dhcp7-201.cineca.it [130.186.7.201]) (using TLSv1 with cipher DHE-RSA-AES256-SHA (256/256 bits)) (No client certificate requested) as user c.gheller@cineca.it by cineca.mm.cineca.it (Postfix) with ESMTP id 390D57B65CC; Thu, 31 Aug 2006 14:55:13 +0200 (MEST) Message-ID: <44F6DC31.4030009@cineca.it> From: Claudio Gheller User-Agent: Mozilla Thunderbird 1.0.7 (Windows/20050923) X-Accept-Language: en-us, en MIME-Version: 1.0 To: Gerard Cc: theory@ivoa.net, Ugo Becciani , "R. Smareglia" Subject: Re: VOTable for simulations References: <003c01c6cb8c$d6ca7410$cc48b782@gavopc1> In-Reply-To: <003c01c6cb8c$d6ca7410$cc48b782@gavopc1> Content-Type: multipart/alternative; boundary="------------060503090303030205020201" Date: Thu, 31 Aug 2006 14:55:13 +0200 (MEST) X-Virus-Scanned: Cineca AppOs 0.99 at as2.cineca.com X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.8.31.53443 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Claudio Gheller This is a multi-part message in MIME format. --------------060503090303030205020201 Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit Ciao Gerard, in the meantime I had thought a litlle about possible formats for the VOTable. In fact I come to the conclusion that there is little new to add to the already existing VOTable specification, both for grids and for particles. The only parameters that I think we have to add is the "rank" parameter (it may already exist, but I could have missed it). Rank is the only parameter that makes grids different from particles, scalars from vectors. For the rest, particles are completely the same as grids. NO different approaches are needed. In practice: Rank = 1 --> scalar on particles (a sequence of scalar values associated to the N particles, one info per particle, N values) Rank = 2 --> vector on particles (sets of three values per particles, Nx3) Rank = 3 --> scalar on grids (one value per grid point, NxNxN - assuming a cubic grid for simplicity) Rank = 4 --> vector on grids (set of three values per grid point, NxNxNx3) At the moment let's consider only 3D simulations. From the example belowe you can notice that "rank" is a ridondant info that can be obtained also directly from the "arraysize" parameter. But you must go through a parsing and therefore it could be useful to keep it highlighted in a specific parameter. In this version, more variables, of different sizes, can be stored in the SAME file. The file could have different formats (fits, hdf... that must be specified properly). I assume, for the moment, a raw binary file, where variables are written one after the other (the standard table structure in row and colums is not efficient or even possible). The entry point for each variable can be easily calculated using the "arraysize" and "datatype" parameters. Furthermore, the order in which they are sotred must be specified. And this could be the order in which the FIELDs are stored in the VOTable. Example: our data file contains a scalar field on a mesh, a vector field on a mesh, a scalar and a vector fields on particles:
Let me know your opinion. Claudio Gerard wrote: >Hi Claudio >Sorry for the late reply to this email. I'm Cc-ing the theory group as well > >I gather you are thinking of grid simulation data here, so this mail does >not apply to N-body. Anyway, for that I think we can use the VOTable spec as >it stands, in particular section 5.3 dealing with binary serialisation (see >http://www.ivoa.net/Documents/REC/VOTable/VOTable-20040811.pdf ). > >In the case you address, would it make sense to try to mimick FITS in the >naming of key words, so use NAXIS for rank, and NAXIS1 for size0, NAXIS2 for >size1 etc for the dimensions ? If I am not mistaken VOTable itself is based >on the FITS binary table spec, so your proposal might be seen as a >translation of a FITS datacube (IMAGE). Did we actually not think about >using FITS as is for (uniform) grid simulations ? In that case your proposal >could also be used I guess, where iso STREAM we'd have FITS as in standard >VOTable usage (though I don't know whether votable presumes that the FITS >file contains a table). > >I am not sure whether FITS images/datacubes allow multiple values per cell >(i.,e. have an array size), but don't think so. Otherwise we could probbaly >generalise in that direction. >Do you propose to follow the VOTable/FITS directions on little-vs big-endian >? > >Cheers > >Gerard > > > > > >>-----Original Message----- >>From: Claudio Gheller [mailto:c.gheller@cineca.it] >>Sent: Thursday, July 20, 2006 12:37 PM >>To: Gerard Lemson; Ugo Becciani; Alessandro Costa; Marco Comparato; R. >>Smareglia >>Subject: VOTable for simulations >> >>Dear friends, >> >>I have tried to figure out the structure of a VOTable for simulated >>data. In the following the result. >>I made the following assumptions: >> >>1. data are binary >>2. the binary file is a raw stream of byte, with no structure (no fits, >>no hdf...). It is external to the VOTable (at the moment I've not >>considered base64 conversion for performance reasons) >>3. Each file has an XML descriptor associated. The descriptor at >>present gives only the necessary infos to deal with the file. >>4. Each file contains ONE variable. This is suggested for the following >>reasons >>- data rank and size can change from variable to variable. >>- complex description >>- The association direct XML header file - bin file - variable, is >>easier to handle. >>- smaller files >>- files easier to handle by external applications (also not VO-compliant) >>- drawback: proliferation in the number of files >>However we can consider the support to more complex files or even >>formats, like FITS or HDF5. But let's start with something simple. >> >>At this point I made the Snap program create binary files (at present >>still HDF5, but just for backward compatibility) and associated XMLs. >>For example: >>test.h5 ----> snapped data >>test.h5.xml ----> associated VOTable: >> >> >>>xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" >>xmlns="http://vizier.u-strasbg.fr/xml/VOTable-1.1.xsd >>"> >> >> >> >ucd="" datatype="float" arraysize="41x41x41" unit="Kelvin" /> >> >> >> >> >> >> >> >>
>> >> >> >>Notice that the rank and size of the dataset is expressed in the >>arraysize keyword of FIELD. It is also written in the 4 PARAM fields. >>This is just to avoid the parsing of the string to get the basic info of >>rank and size and to have them directly as numbers (with their precise >>type). At present there are no UCD and no reference to the SNAP >>protocol, since both are not yet defined. I'm working on the latter... >> >>This is the very first attempt!!! Let me know all your comments. >>Claudio >> >>-- >>------------------------------------ >>Dr. Claudio Gheller, Ph.D. >>High Performance System Division >>CINECA - Bologna - Italy >>Tel. +39-051-6171560 >>Fax. +39-051-6137273 >>------------------------------------ >> >> > > > > > > -- ------------------------------------ Dr. Claudio Gheller, Ph.D. High Performance System Division CINECA - Bologna - Italy Tel. +39-051-6171560 Fax. +39-051-6137273 ------------------------------------ --------------060503090303030205020201 Content-Type: text/html; charset=ISO-8859-1 Content-Transfer-Encoding: 7bit Ciao Gerard,
in the meantime I had thought a litlle about possible formats for the VOTable. In fact I come to the conclusion that there is little new to add to the already existing VOTable specification, both for grids and for particles.
The only parameters that I think we have to add is the "rank" parameter (it may already exist, but I could have missed it).
Rank is the only parameter that makes grids different from particles, scalars from vectors. For the rest, particles are completely the same as grids. NO different approaches are needed.

In practice:
Rank = 1  --> scalar on particles (a sequence of scalar values associated to the N particles,  one info  per particle, N values)
Rank = 2 --> vector on particles (sets of three values per particles, Nx3)
Rank = 3 --> scalar on grids (one value per grid point, NxNxN - assuming a cubic grid for simplicity)
Rank = 4 --> vector on grids (set of three values per grid point, NxNxNx3)
At the moment let's consider only 3D simulations.
>From the example belowe you can notice that "rank" is a ridondant info that can be obtained also directly from the "arraysize" parameter. But you must go through a parsing and therefore it could be useful to keep it highlighted in a specific parameter.

In this version, more variables, of different sizes, can be stored in the SAME file. The file could have different formats (fits, hdf... that must be specified properly). I assume, for the moment, a raw binary file, where variables are written one after the other (the standard table structure in row and colums is not efficient or even possible). The entry point for each variable can be easily calculated using the "arraysize" and "datatype" parameters. Furthermore, the order in which they are sotred must be specified. And this could be the order in which the FIELDs are stored in the VOTable.

Example: our data file contains a scalar field on a mesh, a vector field on a mesh, a scalar and a vector fields on particles:

<?xml version="1.0"?>
<VOTABLE xmlns:xsd="http://www.w3.org/2001/XMLSchema" xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://vizier.u-strasbg.fr/xml/VOTable-1.1.xsd
">
       <RESOURCE name=myTestResource>
               <TABLE name="BmTemperature" ID="MyTestTable" >
                       <FIELD name="BmTemperature" ID="myTestObject1" ucd="" datatype="float" rank="3" arraysize="41x41x41"   unit="K" />
                       <FIELD name="BmVelocity"    ID="myTestObject2" ucd="" datatype="float" rank="4" arraysize="41x41x41x3" unit="km/sec" />
                       <FIELD name="ParticlPos"    ID="myTestObject3" ucd="" datatype="float" rank="2" arraysize="10000x3"    unit="Mpc" />
                       <FIELD name="PartDens"      ID="myTestObject4" ucd="" datatype="float" rank="1" arraysize="10000"      unit="g/cm3" />
                       <DATA><BINARY>
                       <STREAM href="file:///scratch/myhome/test.h5"/>
                       </BINARY></DATA>
               </TABLE>
       </RESOURCE>
</VOTABLE> 

Let me know your opinion.
Claudio


Gerard wrote: 
Hi Claudio
Sorry for the late reply to this email. I'm Cc-ing the theory group as well

I gather you are thinking of grid simulation data here, so this mail does
not apply to N-body. Anyway, for that I think we can use the VOTable spec as
it stands, in particular section 5.3 dealing with binary serialisation (see
http://www.ivoa.net/Documents/REC/VOTable/VOTable-20040811.pdf ).

In the case you address, would it make sense to try to mimick FITS in the
naming of key words, so use NAXIS for rank, and NAXIS1 for size0, NAXIS2 for
size1 etc for the dimensions ? If I am not mistaken VOTable itself is based
on the FITS binary table spec, so your proposal might be seen as a
translation of a FITS datacube (IMAGE). Did we actually not think about
using FITS as is for (uniform) grid simulations ? In that case your proposal
could also be used I guess, where iso STREAM we'd have FITS as in standard
VOTable usage (though I don't know whether votable presumes that the FITS
file contains a table).

I am not sure whether FITS images/datacubes allow multiple values per cell
(i.,e. have an array size), but don't think so. Otherwise we could probbaly
generalise in that direction. 
Do you propose to follow the VOTable/FITS directions on little-vs big-endian
?

Cheers

Gerard



  
-----Original Message-----
From: Claudio Gheller [mailto:c.gheller@cineca.it]
Sent: Thursday, July 20, 2006 12:37 PM
To: Gerard Lemson; Ugo Becciani; Alessandro Costa; Marco Comparato; R.
Smareglia
Subject: VOTable for simulations

Dear friends,

I have tried to figure out the structure of a VOTable for simulated
data. In the following the result.
I made the following assumptions:

1. data are binary
2. the binary file is a raw stream of byte, with no structure (no fits,
no hdf...). It is external to the VOTable (at the moment I've not
considered base64 conversion for performance reasons)
3. Each file has an  XML descriptor associated. The descriptor at
present gives only the necessary infos to deal with the file.
4. Each file contains ONE variable. This is suggested for the following
reasons
- data rank and size can change from variable to variable.
- complex description
- The association direct XML header file - bin file - variable, is
easier to handle.
- smaller files
- files easier to handle by external applications (also not VO-compliant)
- drawback: proliferation in the number of files
However we can consider the support to more complex files or even
formats, like FITS or HDF5. But let's start with something simple.

At this point I made the Snap program create binary files (at present
still HDF5, but just for backward compatibility) and associated XMLs.
For example:
test.h5 ----> snapped data
test.h5.xml ----> associated VOTable:

<?xml version="1.0"?>
<VOTABLE xmlns:xsd="http://www.w3.org/2001/XMLSchema"
xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance"
xmlns="http://vizier.u-strasbg.fr/xml/VOTable-1.1.xsd
">
        <RESOURCE name=myTestResource>
                <TABLE name="BmTemperature" ID="MyTestTable" >
                        <FIELD name="BmTemperature" ID="myTestObject"
ucd="" datatype="float" arraysize="41x41x41" unit="Kelvin" />
                        <PARAM name="rank" datatype="int" value="3"/>
                        <PARAM name="size0" datatype="long" value="41"/>
                        <PARAM name="size1" datatype="long" value="41"/>
                        <PARAM name="size2" datatype="long" value="41"/>
                        <DATA><BINARY>
                        <STREAM href="file:///scratch/myhome/test.h5"/>
                        </BINARY></DATA>
                </TABLE>
        </RESOURCE>
</VOTABLE>

Notice that the rank and size of the dataset is expressed in the
arraysize keyword of FIELD. It is also written in the 4 PARAM fields.
This is just to avoid the parsing of the string to get the basic info of
rank and size and to have them directly as numbers (with their precise
type). At present there are no UCD and no reference to the SNAP
protocol, since both are not yet defined. I'm working on the latter...

This is the very first attempt!!! Let me know all your comments.
Claudio

--
------------------------------------
Dr. Claudio Gheller, Ph.D.
High Performance System Division
CINECA - Bologna - Italy
Tel. +39-051-6171560
Fax. +39-051-6137273
------------------------------------
    




  


-- 
------------------------------------
Dr. Claudio Gheller, Ph.D.
High Performance System Division
CINECA - Bologna - Italy
Tel. +39-051-6171560
Fax. +39-051-6137273
------------------------------------
--------------060503090303030205020201-- From owner-theory@eso.org Thu Aug 31 18:59:51 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k7VGxgfq026304 for ; Thu, 31 Aug 2006 18:59:42 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k7VGxgdM026303 for theory-outgoing; Thu, 31 Aug 2006 18:59:42 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k7VGxaVX026283 for ; Thu, 31 Aug 2006 18:59:37 +0200 (MEST) Received: from mpemail.mpe.mpg.de (mpemail.mpe-garching.mpg.de [130.183.137.110]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k7VFFVum028526 for ; Thu, 31 Aug 2006 17:15:31 +0200 (CEST) Received: from gavopc1.xray.mpe.mpg.de ([130.183.72.204] helo=gavopc1) by mpemail.mpe.mpg.de with esmtp (Exim 4.50) id 1GIoGL-0003Ew-MX; Thu, 31 Aug 2006 17:15:25 +0200 From: "Gerard" To: "'Claudio Gheller'" Cc: , "'Ugo Becciani'" , "'R. Smareglia'" Subject: RE: VOTable for simulations Date: Thu, 31 Aug 2006 17:19:25 +0200 Message-ID: <001c01c6cd10$d869c8e0$cc48b782@gavopc1> MIME-Version: 1.0 Content-Type: text/plain; charset="iso-8859-1" X-Mailer: Microsoft Office Outlook 11 In-Reply-To: <44F6DC31.4030009@cineca.it> X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2962 Thread-Index: AcbM/McN2NFHgGaTRLihMMT4ULovtwADmGvw X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.8.31.75443 Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id k7VGxcVV026288 Sender: owner-theory@eso.org Precedence: bulk Reply-To: "Gerard" Dear Claudio >From the VOTable spec, in particular section 2.2, I gather that they indeed already included support for multi-dimensional arrays. This seems then indeed the natural way to support at least uniform grids coming from simulations as well. Some comments: >From their example I gather that arraysize="41x41x41x3" means "three data cubes of dimensions 41x41x41", not "one 3D-vector valued datacube of dimensions 41x41x41". "41x41x41" would mean "41 2D datafields of dimension 41x41". I think that therefore a 3D vector field could/has to be encoded as (for example)
This makes the content of the individual field components more explicit. Each gets it own UCD for example. I have removed the rank attribute for the moment. There is no way yet to specify the spatial coordinates of the grid cells. For a grid one can specify the spatial coordinates in general in a shorthand way, for example using a set of standard parameters as in the FITS array keywords (see http://fits.gsfc.nasa.gov/standard21b/fits_standard.pdf 5.4.2.5), CRPIXn, CDELTn etc. I think we need to specify something like that here as well, it is definitly more efficient than having separate cubes with the coordinates. Luckily in general our coordinate system will not require the full WCS like formalism in general. Still I also liked your original approach, which, as I commented in my earlier reply, seemed to lead to a kind of equivalence in XML of the FITS image specification. I wonder whether the VOTable group has considered to put image data in an XML form of FITS just as they did for the FITS binary table. I'll pose the question on their mailing list. Tough we can use the multi-dimensional array, it seems not as natural. Then, though it is possible to use this same formalism for particle data as well, I think there the tabular approach is more natural in many circumstances. In particular in the work that I have been doing with databases, the natural representation of more complex individual objects is as a table, with all the properties, including now the positions, in a row. The way to store such tabular datasets in binary form is specified exactly in the the existing VOTable spec, in section 5.3. An equivalent C-struct oriented format in binary files is what I have encountered consistently for more complex objects coming for example from the postprocessing of cosmological simulations at the MPA in Garching. But you're right that many people also store particle data in individual arrays for each particle property. That is more naturally mapped in the sense of your rank 1/2 examples. Making the same adjustment as above for the datacubes I would propose to allow also something as in the following example:
I would advocate supporting both representations for particle data, tabular and (1D) array. In the latter case we still need something to distinguish between particle data and image data. Your rank basically does that, just the name might be unfortunate. We might want to be more explicit about the kind of data that is stored, an attribute with values MESH, N_BODY maybe ? In your example you use an HDF5 binary file. VOTable does not support that, though it does support FITS, I suppose as BINARY table (see VOTable spec section 5.2). Is there a natural mapping from VOTable key words to HDF metadata structures ? Or shall we first concetrate on the binary serialisations specified in VOTable ? Cheers Gerard ________________________________________ From: Claudio Gheller [mailto:c.gheller@cineca.it] Sent: Thursday, August 31, 2006 2:55 PM To: Gerard Cc: theory@ivoa.net; Ugo Becciani; R. Smareglia Subject: Re: VOTable for simulations Ciao Gerard, in the meantime I had thought a litlle about possible formats for the VOTable. In fact I come to the conclusion that there is little new to add to the already existing VOTable specification, both for grids and for particles. The only parameters that I think we have to add is the "rank" parameter (it may already exist, but I could have missed it). Rank is the only parameter that makes grids different from particles, scalars from vectors. For the rest, particles are completely the same as grids. NO different approaches are needed. In practice: Rank = 1  --> scalar on particles (a sequence of scalar values associated to the N particles,  one info  per particle, N values) Rank = 2 --> vector on particles (sets of three values per particles, Nx3) Rank = 3 --> scalar on grids (one value per grid point, NxNxN - assuming a cubic grid for simplicity) Rank = 4 --> vector on grids (set of three values per grid point, NxNxNx3) At the moment let's consider only 3D simulations. >From the example belowe you can notice that "rank" is a ridondant info that can be obtained also directly from the "arraysize" parameter. But you must go through a parsing and therefore it could be useful to keep it highlighted in a specific parameter. In this version, more variables, of different sizes, can be stored in the SAME file. The file could have different formats (fits, hdf... that must be specified properly). I assume, for the moment, a raw binary file, where variables are written one after the other (the standard table structure in row and colums is not efficient or even possible). The entry point for each variable can be easily calculated using the "arraysize" and "datatype" parameters. Furthermore, the order in which they are sotred must be specified. And this could be the order in which the FIELDs are stored in the VOTable. Example: our data file contains a scalar field on a mesh, a vector field on a mesh, a scalar and a vector fields on particles:                                                                                                                                                                                                      
         Let me know your opinion. Claudio Gerard wrote: Hi Claudio Sorry for the late reply to this email. I'm Cc-ing the theory group as well I gather you are thinking of grid simulation data here, so this mail does not apply to N-body. Anyway, for that I think we can use the VOTable spec as it stands, in particular section 5.3 dealing with binary serialisation (see http://www.ivoa.net/Documents/REC/VOTable/VOTable-20040811.pdf ). In the case you address, would it make sense to try to mimick FITS in the naming of key words, so use NAXIS for rank, and NAXIS1 for size0, NAXIS2 for size1 etc for the dimensions ? If I am not mistaken VOTable itself is based on the FITS binary table spec, so your proposal might be seen as a translation of a FITS datacube (IMAGE). Did we actually not think about using FITS as is for (uniform) grid simulations ? In that case your proposal could also be used I guess, where iso STREAM we'd have FITS as in standard VOTable usage (though I don't know whether votable presumes that the FITS file contains a table). I am not sure whether FITS images/datacubes allow multiple values per cell (i.,e. have an array size), but don't think so. Otherwise we could probbaly generalise in that direction. Do you propose to follow the VOTable/FITS directions on little-vs big-endian ? Cheers Gerard -----Original Message----- From: Claudio Gheller [mailto:c.gheller@cineca.it] Sent: Thursday, July 20, 2006 12:37 PM To: Gerard Lemson; Ugo Becciani; Alessandro Costa; Marco Comparato; R. Smareglia Subject: VOTable for simulations Dear friends, I have tried to figure out the structure of a VOTable for simulated data. In the following the result. I made the following assumptions: 1. data are binary 2. the binary file is a raw stream of byte, with no structure (no fits, no hdf...). It is external to the VOTable (at the moment I've not considered base64 conversion for performance reasons) 3. Each file has an XML descriptor associated. The descriptor at present gives only the necessary infos to deal with the file. 4. Each file contains ONE variable. This is suggested for the following reasons - data rank and size can change from variable to variable. - complex description - The association direct XML header file - bin file - variable, is easier to handle. - smaller files - files easier to handle by external applications (also not VO-compliant) - drawback: proliferation in the number of files However we can consider the support to more complex files or even formats, like FITS or HDF5. But let's start with something simple. At this point I made the Snap program create binary files (at present still HDF5, but just for backward compatibility) and associated XMLs. For example: test.h5 ----> snapped data test.h5.xml ----> associated VOTable:
Notice that the rank and size of the dataset is expressed in the arraysize keyword of FIELD. It is also written in the 4 PARAM fields. This is just to avoid the parsing of the string to get the basic info of rank and size and to have them directly as numbers (with their precise type). At present there are no UCD and no reference to the SNAP protocol, since both are not yet defined. I'm working on the latter... This is the very first attempt!!! Let me know all your comments. Claudio -- ------------------------------------ Dr. Claudio Gheller, Ph.D. High Performance System Division CINECA - Bologna - Italy Tel. +39-051-6171560 Fax. +39-051-6137273 ------------------------------------ -- ------------------------------------ Dr. Claudio Gheller, Ph.D. High Performance System Division CINECA - Bologna - Italy Tel. +39-051-6171560 Fax. +39-051-6137273 ------------------------------------ From owner-theory@eso.org Fri Sep 1 11:43:41 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k819hWaC027641 for ; Fri, 1 Sep 2006 11:43:32 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k819hW6o027640 for theory-outgoing; Fri, 1 Sep 2006 11:43:32 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k819hVm7027627 for ; Fri, 1 Sep 2006 11:43:31 +0200 (MEST) Received: from as2.cineca.com (as2.cineca.com [130.186.84.242]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k819hSum016139 for ; Fri, 1 Sep 2006 11:43:29 +0200 (CEST) Received: from localhost (localhost.localdomain [127.0.0.1]) by as2.cineca.com (Postfix) with ESMTP id 4856032E; Fri, 1 Sep 2006 11:43:21 +0200 (CEST) Received: from cineca.mm.cineca.it (cineca.mm.cineca.it [130.186.10.200]) by as2.cineca.com (Postfix) with ESMTP id B4413304; Fri, 1 Sep 2006 11:43:16 +0200 (CEST) Received: from [130.186.7.201] (dhcp7-201.cineca.it [130.186.7.201]) (using TLSv1 with cipher DHE-RSA-AES256-SHA (256/256 bits)) (No client certificate requested) as user c.gheller@cineca.it by cineca.mm.cineca.it (Postfix) with ESMTP id 4422A7B9340; Fri, 1 Sep 2006 11:43:16 +0200 (MEST) Message-ID: <44F800B3.9090404@cineca.it> From: Claudio Gheller User-Agent: Mozilla Thunderbird 1.0.7 (Windows/20050923) X-Accept-Language: en-us, en MIME-Version: 1.0 To: Gerard Cc: theory@ivoa.net, "'Ugo Becciani'" , "'R. Smareglia'" Subject: Re: VOTable for simulations References: <001c01c6cd10$d869c8e0$cc48b782@gavopc1> In-Reply-To: <001c01c6cd10$d869c8e0$cc48b782@gavopc1> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 7bit Date: Fri, 1 Sep 2006 11:43:16 +0200 (MEST) X-Virus-Scanned: Cineca AppOs 0.99 at as2.cineca.com X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.9.1.21443 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Claudio Gheller Ciao Gerard, > >>From their example I gather that arraysize="41x41x41x3" means "three data >cubes of dimensions 41x41x41", >not "one 3D-vector valued datacube of dimensions 41x41x41". >"41x41x41" would mean "41 2D datafields of dimension 41x41". I think that >therefore a 3D vector field >could/has to be encoded as (for example) > > Ok, in order to keep alligned with VOTable standards let's adopt this solution. EACH CONTAINS ONLY a SCALAR FIELD, that can be both a real scalar quantity and a component of a multidimensional array. In this way we could lose the "nature" of the quantity (scalar or vector), but this could be recovered by the associated UCD. > > xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" > xmlns="http://vizier.u-strasbg.fr/xml/VOTable-1.1.xsd"> > > > datatype="float" > arraysize="41x41x41x1" unit="km/s" /> > datatype="float" > arraysize="41x41x41x1" unit="km/s" /> > datatype="float" > arraysize="41x41x41x1" unit="km/s" /> > > > > > >
> > > >This makes the content of the individual field components more explicit. >Each gets it own UCD for example. > > >I have removed the rank attribute for the moment. > > Fine, we can get the associated information from the "arraysize" >There is no way yet to specify the spatial coordinates of the grid cells. >For a grid one can specify >the spatial coordinates in general in a shorthand way, for example using a >set of standard parameters >as in the FITS array keywords (see >http://fits.gsfc.nasa.gov/standard21b/fits_standard.pdf 5.4.2.5), >CRPIXn, CDELTn etc. I think we need to specify something like that here as >well, it is definitly more >efficient than having separate cubes with the coordinates. >Luckily in general our coordinate system will not require the full WCS like >formalism in general. > > I will take a look at these FITS standards. Obvioulsly, for a regular grid we do not need to specify the grid points but only the number of points and the mesh resolution per each dimension. I guess this information can be specified at the level of the element (but I'm not sure it is the right place). Obviously if data are mixed, mesh and particles in the same file, the information refers only to the mesh components. >Then, though it is possible to use this same formalism for particle data as >well, I think there the tabular approach is more natural in many >circumstances. In particular in the work that I have been doing with >databases, >the natural representation of more complex individual objects is as a table, >with all the properties, including >now the positions, in a row. The way to store such tabular datasets in >binary form is specified exactly in the >the existing VOTable spec, in section 5.3. An equivalent C-struct oriented >format in binary files is what I have encountered consistently for more >complex objects coming for example from the postprocessing of cosmological >simulations at the MPA in Garching. > >But you're right that many people also store particle data in individual >arrays for each particle property. > > I agree that we should support both the approaches. The tabular approach is more natural, since you can find "close to each other" all the information related to a particle. However, often the user needs to select only one (or few) of the properties of the particles. For example, for visualization you may need to load only the position. For the mass functions, the positions and the masses. For the velocity dispersion, the three component of the velocity. In this cases, it is much faster and more efficient to store each variable separately (you load all the data in a single contiguous read operation). Furthermore, many codes use this kind of storage technique (e.g. Gadget and Enzo, between the most popular). >That is more naturally mapped in the sense of your rank 1/2 examples. Making >the same adjustment as above for >the datacubes I would propose to allow also something as in the following >example: > > > xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" > xmlns="http://vizier.u-strasbg.fr/xml/VOTable-1.1.xsd"> > > > datatype="float" > arraysize="100000x1" unit="Mpc" /> > datatype="float" > arraysize="100000x1" unit="Mpc" /> > datatype="float" > arraysize="100000x1" unit="Mpc" /> > datatype="float" > arraysize="100000x1" unit="km/s" /> > datatype="float" > arraysize="100000x1" unit="km/s" /> > datatype="float" > arraysize="100000x1" unit="km/s" /> > > > > >
> > > > > > At this point, I would drop the "x1" in the "arraysize". >In the latter case we still need something to distinguish between particle >data and image data. >Your rank basically does that, just the name might be unfortunate. We might >want to be more explicit >about the kind of data that is stored, an attribute with values MESH, N_BODY >maybe ? > > ok... name of the attribute? maybe "geometry"... >In your example you use an HDF5 binary file. VOTable does not support that, >though it does support FITS, >I suppose as BINARY table (see VOTable spec section 5.2). Is there a natural >mapping from VOTable key words >to HDF metadata structures ? Or shall we first concetrate on the binary >serialisations specified in VOTable ? > > At the moment I would focus on "pure" binaries. HDF5 was cited only as an example. I go on... Thanks a lot for all the comments!!! C. -- ------------------------------------ Dr. Claudio Gheller, Ph.D. High Performance System Division CINECA - Bologna - Italy Tel. +39-051-6171560 Fax. +39-051-6137273 ------------------------------------ From owner-theory@eso.org Mon Sep 4 11:04:37 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k8493oqt029685 for ; Mon, 4 Sep 2006 11:03:50 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k8493o0K029684 for theory-outgoing; Mon, 4 Sep 2006 11:03:50 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k8493nH2029680 for ; Mon, 4 Sep 2006 11:03:49 +0200 (MEST) Received: from mpemail.mpe.mpg.de (mpemail.mpe-garching.mpg.de [130.183.137.110]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k8493mum012641 for ; Mon, 4 Sep 2006 11:03:48 +0200 (CEST) Received: from gavopc1.xray.mpe.mpg.de ([130.183.72.204] helo=gavopc1) by mpemail.mpe.mpg.de with esmtp (Exim 4.50) id 1GKAMk-0001Yc-2s for theory@ivoa.net; Mon, 04 Sep 2006 11:03:38 +0200 From: "Gerard" To: Subject: Moscow Date: Mon, 4 Sep 2006 11:07:38 +0200 Message-ID: <002a01c6d001$91d7edf0$cc48b782@gavopc1> MIME-Version: 1.0 Content-Type: multipart/alternative; boundary="----=_NextPart_000_002B_01C6D012.5560BDF0" X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.2962 thread-index: AcbQAZG0xDISjXPlTZmI3VQL7umCaA== X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.9.4.13442 Sender: owner-theory@eso.org Precedence: bulk Reply-To: "Gerard" This is a multi-part message in MIME format. ------=_NextPart_000_002B_01C6D012.5560BDF0 Content-Type: text/plain; charset="US-ASCII" Content-Transfer-Encoding: 7bit Dear collegues I will not be able to attend the Moscow interop meeting. However, there will be a session, which Herve Wozniak will chair. We are currently discussing the program and will notify you of an agenda later this week. If you feel that there are certain things that should be on the agenda, please let us know. Best regards Gerard Lemson ------=_NextPart_000_002B_01C6D012.5560BDF0 Content-Type: text/html; charset="US-ASCII" Content-Transfer-Encoding: quoted-printable

Dear collegues

 

I will not be able to attend the Moscow interop = meeting.

However, there will be a session, which Herve Wozniak = will chair.

We are currently discussing the program and will = notify you of an agenda later this week.

If you feel that there are certain things that should = be on the agenda, please let us know.

 

Best regards

 

Gerard Lemson

------=_NextPart_000_002B_01C6D012.5560BDF0-- From owner-theory@eso.org Mon Sep 11 14:51:46 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 10000000 X-Mozilla-Keys: 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 k8BCpcrG016904 for ; Mon, 11 Sep 2006 14:51:38 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k8BCpcfB016903 for theory-outgoing; Mon, 11 Sep 2006 14:51:38 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k8BCpbdC016899 for ; Mon, 11 Sep 2006 14:51:37 +0200 (MEST) Received: from ppsw-7.csi.cam.ac.uk (ppsw-7.csi.cam.ac.uk [131.111.8.137]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k8BCpYum026992 for ; Mon, 11 Sep 2006 14:51:34 +0200 (CEST) X-Cam-SpamDetails: Not scanned X-Cam-AntiVirus: No virus found X-Cam-ScannerInfo: http://www.cam.ac.uk/cs/email/scanner/ Received: from cass41.ast.cam.ac.uk ([131.111.69.186]:50758) by ppsw-7.csi.cam.ac.uk (ppsw.cam.ac.uk [131.111.8.137]:25) with esmtp id 1GMlFS-0008Td-NK (Exim 4.54) (return-path ); Mon, 11 Sep 2006 13:50:50 +0100 Received: from cass25.ast.cam.ac.uk (cass25 [IPv6:2001:630:200:4240:203:baff:fe24:314]) by cass41.ast.cam.ac.uk (8.13.7+Sun/8.13.7) with ESMTP id k8BCon8c012542; Mon, 11 Sep 2006 13:50:49 +0100 (BST) Received: from cass25.ast.cam.ac.uk (localhost [127.0.0.1]) by cass25.ast.cam.ac.uk (8.13.7+Sun/8.13.7) with ESMTP id k8BConrY002758; Mon, 11 Sep 2006 13:50:49 +0100 (BST) Received: from localhost (lds@localhost) by cass25.ast.cam.ac.uk (8.13.7+Sun/8.13.7/Submit) with ESMTP id k8BComCO002755; Mon, 11 Sep 2006 13:50:48 +0100 (BST) X-Authentication-Warning: cass25.ast.cam.ac.uk: lds owned process doing -bs Date: Mon, 11 Sep 2006 13:50:48 +0100 (BST) From: Laurie Shaw X-X-Sender: lds@cass25 To: Claudio Gheller cc: Gerard Lemson , Herve Wozniak , theory@ivoa.net Subject: Re: draft and meeting In-Reply-To: <44FD899B.5030503@cineca.it> Message-ID: References: <44FD899B.5030503@cineca.it> MIME-Version: 1.0 Content-Type: MULTIPART/MIXED; BOUNDARY="-559023410-851401618-1157979048=:2630" X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.9.11.52946 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Laurie Shaw This message is in MIME format. The first part should be readable text, while the remaining parts are likely unreadable without MIME-aware tools. Send mail to mime@docserver.cac.washington.edu for more info. ---559023410-851401618-1157979048=:2630 Content-Type: TEXT/PLAIN; charset=US-ASCII Hi Everyone, Attached is a first draft of the technical note that I have been writing for simulation Semantics. Based on the discussions at and after the Victoria meeting, and on early work on the Simulation data models, I break down the meta-data requirements to describe simulations into a set of categories. Each category itself must be labelled by a UCD, for which have made initial suggestions. The typical contents of a category varies between single characters or numbers, ascii text (or urls, names etc) and words from the standard vocabulary (which is still largely to be defined). I've attached the doc in both ms word and pdf formats. Would be great to have a brief discussion about this before the Moscow meeting -- I still have time to make lots of changes, if needed! Thanks, Laurie ---559023410-851401618-1157979048=:2630 Content-Type: APPLICATION/pdf; name="Sim_UCD_Note.pdf" Content-Transfer-Encoding: BASE64 Content-ID: Content-Description: Content-Disposition: attachment; filename="Sim_UCD_Note.pdf" JVBERi0xLjQNJeLjz9MNCjg5NSAwIG9iaiA8PC9MaW5lYXJpemVkIDEvTCA5 NDc3Ny9PIDg5Ny9FIDIxOTU2L04gMTIvVCA3NjgyOS9IIFsgNjY5IDU4Ml0+ Pg1lbmRvYmoNICAgICAgICAgICAgICAgDQp4cmVmDQo4OTUgMTgNCjAwMDAw MDAwMTYgMDAwMDAgbg0KMDAwMDAwMTQ0OSAwMDAwMCBuDQowMDAwMDAxNzI3 IDAwMDAwIG4NCjAwMDAwMDIwMzIgMDAwMDAgbg0KMDAwMDAwMjU2NyAwMDAw MCBuDQowMDAwMDAyOTk3IDAwMDAwIG4NCjAwMDAwMDMzOTMgMDAwMDAgbg0K MDAwMDAwMzQyOSAwMDAwMCBuDQowMDAwMDAzNjYzIDAwMDAwIG4NCjAwMDAw MDM4ODUgMDAwMDAgbg0KMDAwMDAwMzk2MiAwMDAwMCBuDQowMDAwMDA0MjAx IDAwMDAwIG4NCjAwMDAwMDU1NzAgMDAwMDAgbg0KMDAwMDAwNTk5OCAwMDAw MCBuDQowMDAwMDA2MjI2IDAwMDAwIG4NCjAwMDAwMDg4OTYgMDAwMDAgbg0K MDAwMDAwMTI1MSAwMDAwMCBuDQowMDAwMDAwNjY5IDAwMDAwIG4NCnRyYWls ZXINCjw8L1NpemUgOTEzL1ByZXYgNzY4MTcvWFJlZlN0bSAxMjUxL1Jvb3Qg 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10:00:34 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k8C80Xol012218 for theory-outgoing; Tue, 12 Sep 2006 10:00:33 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k8C80WYl012214 for ; Tue, 12 Sep 2006 10:00:32 +0200 (MEST) Received: from smtpsortant1.univ-lyon1.fr (smtpsortant1.univ-lyon1.fr [134.214.100.90]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k8C80Tum013453 for ; Tue, 12 Sep 2006 10:00:30 +0200 (CEST) Received: from localhost (localhost [127.0.0.1]) by smtpsortant1.univ-lyon1.fr (Postfix) with ESMTP id 82B12439E98; Tue, 12 Sep 2006 10:00:24 +0200 (CEST) Received: from smtpsortant1.univ-lyon1.fr ([127.0.0.1]) by localhost (smtpsortant1.univ-lyon1.fr [127.0.0.1]) (amavisd-new, port 10024) with ESMTP id 01212-03; Tue, 12 Sep 2006 10:00:23 +0200 (CEST) Received: from obs.univ-lyon1.fr (obs.univ-lyon1.fr [134.214.4.140]) by smtpsortant1.univ-lyon1.fr (Postfix) with ESMTP id C0211439F57; Tue, 12 Sep 2006 10:00:23 +0200 (CEST) Received: from [127.0.0.1] (canicule.univ-lyon1.fr [134.214.4.20]) by obs.univ-lyon1.fr (Postfix) with ESMTP id D9DAD4BB4F; Tue, 12 Sep 2006 10:00:26 +0200 (CEST) Message-ID: <4506690E.7030507@obs.univ-lyon1.fr> Date: Tue, 12 Sep 2006 10:00:14 +0200 From: Herve Wozniak Organization: Centre de Recherche Astronomique de Lyon User-Agent: Thunderbird 1.5.0.5 (Windows/20060719) MIME-Version: 1.0 To: Laurie Shaw Cc: Claudio Gheller , Gerard Lemson , theory@ivoa.net Subject: Re: draft and meeting References: <44FD899B.5030503@cineca.it> In-Reply-To: Content-Type: multipart/mixed; boundary="------------090800060806040209010700" X-Virus-Scanned: by amavisd-new-20030616-p10 (Debian) at univ-lyon1.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.9.12.3443 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Herve Wozniak This is a multi-part message in MIME format. --------------090800060806040209010700 Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 8bit Hello Laurie, thanks for your draft. my first (and quick) comments are included in the document using word revision tool. For discussions. Regards, Herve Laurie Shaw a écrit : > Hi Everyone, > > Attached is a first draft of the technical note that I have been writing > for simulation Semantics. Based on the discussions at and after the > Victoria meeting, and on early work on the Simulation data models, I break > down the meta-data requirements to describe simulations into a set of > categories. Each category itself must be labelled by a UCD, for which have > made initial suggestions. The typical contents of a category varies > between single characters or numbers, ascii text (or urls, names etc) and > words from the standard vocabulary (which is still largely to be defined). > > I've attached the doc in both ms word and pdf formats. Would be great to > have a brief discussion about this before the Moscow meeting -- I still > have time to make lots of changes, if needed! > > Thanks, > > Laurie -- _______________________________________________________________ Herve WOZNIAK Centre de Recherche Astronomique de Lyon UMR 5574 Université Lyon I - CNRS - ENS-Lyon 9, avenue Charles Andre, F-69561 Saint Genis Laval cedex Phone: (+33) (0) 478 868 388 Fax: (+33) (0) 478 868 386 http://www-obs.univ-lyon1.fr/herve.wozniak/ --------------090800060806040209010700 Content-Type: application/msword; name="Sim_UCD_Note_HW.doc" Content-Transfer-Encoding: base64 Content-Disposition: inline; filename="Sim_UCD_Note_HW.doc" 0M8R4KGxGuEAAAAAAAAAAAAAAAAAAAAAPgADAP7/CQAGAAAAAAAAAAAAAAADAAAAHAEAAAAA AAAAEAAAHgEAAAEAAAD+////AAAAABkBAAAaAQAAGwEAAP////////////////////////// //////////////////////////////////////////////////////////////////////// //////////////////////////////////////////////////////////////////////// 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(8.13.6+Sun/8.12.10) with ESMTP id k8DK54Es009112 for ; Wed, 13 Sep 2006 22:05:04 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k8DK54Og009110 for theory-outgoing; Wed, 13 Sep 2006 22:05:04 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k8DK53uI009102 for ; Wed, 13 Sep 2006 22:05:04 +0200 (MEST) 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 k8DK511x024230 for ; Wed, 13 Sep 2006 22:05:01 +0200 (CEST) Received: from [145.238.18.175] (achille.obspm.fr [145.238.18.175]) by mesiob.obspm.fr (8.13.4/8.13.4/SIO Observatoire de Paris) with ESMTP id k8DK4lYe026736; Wed, 13 Sep 2006 22:04:47 +0200 In-Reply-To: References: <44FD899B.5030503@cineca.it> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: multipart/alternative; boundary=Apple-Mail-24--518021972 Message-Id: Cc: Claudio Gheller , Gerard Lemson , Herve Wozniak , theory@ivoa.net From: Franck Le Petit Subject: Re: draft and meeting Date: Wed, 13 Sep 2006 22:03:24 +0200 To: Laurie Shaw X-Mailer: Apple Mail (2.752.2) X-Greylist: Sender IP whitelisted, not delayed by milter-greylist-2.0.2 (mesiob.obspm.fr [145.238.2.2]); Wed, 13 Sep 2006 22:04:47 +0200 (CEST) X-Virus-Scanned: ClamAV version 0.88.4, clamav-milter version 0.88.4 on mesiob.obspm.fr X-Virus-Status: Clean X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.9.13.123443 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Franck Le Petit --Apple-Mail-24--518021972 Content-Transfer-Encoding: quoted-printable Content-Type: text/plain; charset=ISO-8859-1; delsp=yes; format=flowed Dear Laurie, Fabrice and I had a look at the draft for simulation semantic. We think it is a very good draft and just have a few comments : 1 - In part 4 : Physics of the code We think that in the three cases: Physical Objective, = Physical =20 Processes and Subject, le list of possible values have to be =20 perfectly defined or a search in the registries will be unable to =20 succeed because of synonyms. MNRAS keywords and some words used in VO-=20= events should cover most of the possibilities. If you agree we should explicitely add this in the text = as it is =20 done for Physical Objective. 2 - In part 5.1 : Algorithm As you say, here we will have a tough work to define the = list =20 beeing precise enough without getting lost in the details. Up to now, =20= the list consider only keywords for hydrodynamical keywords, N-body, =20 etc. I wonder if we could add to this list ETL, LVG, Monte-Carlo, =20 Ali to cover algorithm used in radiative transfer codes. It should be =20= easy to cover all the numerical methods for rad. transf. codes =20 easily. This is a point we should talk about in Moscow. 3 - In part 5-3 : Protocol This section is indeed usefull in the case of the search = for a =20 service to be used on grids. In this case we should provide not only =20 informations about parallelisation but all the technical requirements =20= to run the code. For exemple compilers, libraries (Blas, Lapack, =20 NAG, ...). This makes me think to another problem. In the case of a = code =20 launched on a grid via a VO-service such as Astrogrid, do we plan at =20 any level to describe the requirements in hardware: memory, =20 processor... I think that may be useful at a point but maybe it is =20 not required at this level of our work. 4 - In part 6-3 : Algorithm Parameters I think we should not focus too much on this part yet = since it is =20 linked to the datamodel to describe results. This part is fine as it =20 is presently. Best regards Franck & Fabrice. ------------------------------------ Franck Le Petit LUTH Observatoire de Paris 5 Place Jules Janssen 92190 Meudon France Tel: (33) 1 45 07 75 66 ------------------------------------ Le 11 sept. 06 =E0 14:50, Laurie Shaw a =E9crit : > > Hi Everyone, > > Attached is a first draft of the technical note that I have been =20 > writing > for simulation Semantics. Based on the discussions at and after the > Victoria meeting, and on early work on the Simulation data models, =20 > I break > down the meta-data requirements to describe simulations into a set of > categories. Each category itself must be labelled by a UCD, for =20 > which have > made initial suggestions. The typical contents of a category varies > between single characters or numbers, ascii text (or urls, names =20 > etc) and > words from the standard vocabulary (which is still largely to be =20 > defined). > > I've attached the doc in both ms word and pdf formats. Would be =20 > great to > have a brief discussion about this before the Moscow meeting -- I =20 > still > have time to make lots of changes, if needed! > > Thanks, > > Laurie > > --Apple-Mail-24--518021972 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1

Dear = Laurie,

Fabrice = and I had a look at the draft for simulation semantic.
We think = it is a very good draft and just have a few comments :

1 - In = part 4 : Physics of the code
We think that in the = three cases: Physical Objective, Physical Processes and Subject, le list = of possible values have to be perfectly defined or a search in the = registries will be unable to succeed because of synonyms. MNRAS keywords = and some words used in VO-events should cover most of the = possibilities.=A0
If you agree we should = explicitely add this in the text as it is done for Physical = Objective.

2 - In = part 5.1 : Algorithm
As you say, here we will = have a tough work to define the list beeing precise enough without = getting lost in the details. Up to now, the list consider only keywords = for hydrodynamical keywords, N-body, etc. =A0 I wonder if we could add = to this list ETL, LVG, Monte-Carlo, Ali to cover algorithm used in = radiative transfer codes. It should be easy to cover all the numerical = methods for rad. transf. codes easily. This is a point we should talk = about in Moscow.

3 - In = part 5-3 : Protocol
This section is indeed = usefull in the case of the search for a service to be used on grids. In = this case we should provide not only informations about parallelisation = but all the technical requirements to run the code. For exemple = compilers, libraries (Blas, Lapack, NAG, ...).=A0
= This makes me think to another problem. In the case of a code = launched on a grid via a VO-service such as Astrogrid, do we plan at any = level to describe the requirements in hardware: memory, processor... I = think that may be useful at a point but maybe it is not required at this = level of our work.

4 - In = part 6-3 : Algorithm Parameters
I think we should not = focus too much on this part yet since it is linked to the datamodel to = describe results. This part is fine as it is presently.

Best = regards
Franck & = Fabrice.

=A0 = =A0------------------------------------
=A0 =A0Franck Le = Petit
=A0 =A0LUTH
=A0 =A0Observatoire de = Paris
=A0 =A05 Place Jules Janssen
=A0 =A092190 = Meudon
=A0 =A0France
=A0 =A0Tel: (33) 1 45 07 75 = 66
=A0 =A0------------------------------------

Le 11 = sept. 06 =E0 14:50, Laurie Shaw a =E9crit :


Hi = Everyone,

Attached is a first draft of the technical note that = I have been writing
for simulation Semantics. = Based on the discussions at and after the
Victoria = meeting, and on early work on the Simulation data models, I = break
down the meta-data requirements = to describe simulations into a set of
made initial suggestions. The = typical contents of a category varies
between = single characters or numbers, ascii text (or urls, names etc) = and
words from the standard = vocabulary (which is still largely to be defined).

I've = attached the doc in both ms word and pdf formats. Would be great = to
have a brief discussion about this before the = Moscow meeting -- I still
have time to = make lots of changes, if needed!

Thanks,

Subject: Re: draft and meeting To: Laurie Shaw , Claudio Gheller Cc: Gerard Lemson , Herve Wozniak , theory@ivoa.net X-Mailer: CommuniGate Pro WebUser v5.1c.3 Date: Wed, 13 Sep 2006 14:44:22 -0700 Message-ID: In-Reply-To: References: <44FD899B.5030503@cineca.it> 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: 2.4.0.264935, Antispam-Data: 2006.9.13.141443 Sender: owner-theory@eso.org Precedence: bulk Reply-To: "Dave DeYoung" Dear Laurie et al.; This seems like a very good start on this problem. I have a few comments to add to those of the others. First, in general we are not considering just "simulations" if one wants to be precise. Codes such as CLOUDY and various radiative transfer codes clearly need to be included, but they are not strictly simulations. It's all theoretical astrophysics, so perhaps a more general term is needed. More specifically: 3.2 Name of Code - Not all codes have names. e.g., MHD-TVD codes used here are not yet "named" because the authors think it is frivolous. How should these be included? 4.2 Physical Processes - The vocabulary here is very incomplete, as was noted by Laurie. 4.3 Subject - There seems to be a lot of overlap or redundancy here with section 4.1, which is supposed to give a description of the phenomenon being simulated. 5.3 I agree with others that the specification of the library is useful. 6.3 Algorithm Parameters - Here there is also a lot of overlap with section 5.1, Algortithm. Perhaps these two should be merged or at least placed in the same general section. I am sorry I will be unable to attend the Moscow meeting. I hope you have a very productive set of discussions there. Best wishes, Dave De Young From owner-theory@eso.org Thu Sep 14 00:46:21 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 10000000 X-Mozilla-Keys: 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 k8DMkDNp004410 for ; Thu, 14 Sep 2006 00:46:13 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k8DMkDFt004409 for theory-outgoing; Thu, 14 Sep 2006 00:46:13 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k8DMkC0n004403 for ; Thu, 14 Sep 2006 00:46:12 +0200 (MEST) Received: from smtp.iaa.es (smtp.iaa.csic.es [193.146.145.11]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k8DMk8L5021687 for ; Thu, 14 Sep 2006 00:46:08 +0200 (CEST) Received: from [132.248.230.73] ([132.248.230.73]) (authenticated bits=0) by smtp.iaa.es (8.13.1/8.13.1) with ESMTP id k8DMjY7J005651; Thu, 14 Sep 2006 00:45:36 +0200 In-Reply-To: References: <44FD899B.5030503@cineca.it> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: multipart/mixed; boundary=Apple-Mail-1--508301633 Message-Id: <7C7CFC36-75F5-48B3-AEA2-E39A11B701DC@iaa.es> Cc: Laurie Shaw , Claudio Gheller , Gerard , Dave DeYoung , Herve Wozniak , =?ISO-8859-1?Q?Miguel_Cervi=F1o?= From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Re: draft and meeting Date: Wed, 13 Sep 2006 17:45:24 -0500 To: theory@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: 2006.9.13.151443 Sender: owner-theory@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= --Apple-Mail-1--508301633 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Dear all, I just edited the doc file by Herve and I have included some text and my own coments. I also have included the coments by Frank, Fabribrice and Dave. (I don not know what would be the best way to modify the document, but in any case I just do it in this way). In general I agree with all comments. Laurie, thanks alot for the document, I think that in general very good Best regards miguel P.D: I am sorry but I will not be in Moscow meeting P.D.2: There has been a draft about characterization in the DM group. I think that most of the things they point out there are addressed in some way here. However, in the characteriztion draft there has been an special enfasis in define the "bounds" of the data included in the table (in the case of an spectrum it would be the limits where the spectrum is defined) I do not know if the current draft on smenatics also cover the bounds of theoretical models for n-body simulations etc... --Apple-Mail-1--508301633 Content-Transfer-Encoding: base64 Content-Type: application/octet-stream; x-mac-type=5738424E; x-unix-mode=0644; x-mac-creator=4D535744; name=Sim_UCD_Note_v2.doc Content-Disposition: attachment; filename=Sim_UCD_Note_v2.doc 0M8R4KGxGuEAAAAAAAAAAAAAAAAAAAAAPgADAP7/CQAGAAAAAAAAAAAAAAADAAAAVAEAAAAAAAAA EAAAVgEAAAEAAAD+////AAAAAFEBAABSAQAAUwEAAP////////////////////////////////// //////////////////////////////////////////////////////////////////////////// //////////////////////////////////////////////////////////////////////////// //////////////////////////////////////////////////////////////////////////// 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majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k8F1GIen025991 for theory-outgoing; Fri, 15 Sep 2006 03:16:18 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k8F1GHaI025984 for ; Fri, 15 Sep 2006 03:16:17 +0200 (MEST) Received: from serv2.obs-besancon.fr (serv2.obs-besancon.fr [193.52.185.12]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k8F1GE1x023714 for ; Fri, 15 Sep 2006 03:16:15 +0200 (CEST) Received: from services3.obs-besancon.fr ([193.52.184.204] ident=mail) by serv2.obs-besancon.fr with esmtp (Exim 3.36 #1 (Debian)) id 1GO25O-0000UH-00; Fri, 15 Sep 2006 03:01:42 +0200 Received: from serv2.obs-besancon.fr ([193.52.185.12] helo=localhost) by services3.obs-besancon.fr with esmtp (Exim 3.36 #1 (Debian)) id 1GO20M-0006ji-00; Fri, 15 Sep 2006 02:56:30 +0200 Received: from c5850-a2-1-62-147-0-48.dial.proxad.net (c5850-a2-1-62-147-0-48.dial.proxad.net [62.147.0.48]) by webmail.obs-besancon.fr (Horde MIME library) with HTTP for ; Fri, 15 Sep 2006 02:56:27 +0200 Message-ID: <20060915025627.uodcx2giypsg8cgc@webmail.obs-besancon.fr> Date: Fri, 15 Sep 2006 02:56:27 +0200 From: debray@obs-besancon.fr To: theory@ivoa.net Cc: Laurie Shaw Subject: Re: draft MIME-Version: 1.0 Content-Type: text/plain; charset=ISO-8859-1 Content-Disposition: inline User-Agent: Internet Messaging Program (IMP) H3 (4.0.2) X-Observatoire-Besancon-MailScanner: Found to be clean, Found to be clean X-Observatoire-Besancon-MailScanner-From: debray@obs-besancon.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 4.7.1.128075, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.9.14.175443 Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id k8F1GHaI025987 Sender: owner-theory@eso.org Precedence: bulk Reply-To: debray@obs-besancon.fr Dear Laurie, dear members of the Theory Interest Group, First, thanks to Laurie for the setting up of the "Theory Semantics" technical note. I would also like to make a few further comments: - in the "Introduction", should not the registration of "theoretical on-line services" be mentionned as well as of codes and simulation data sets, in accordance with Sébastien Derrière's talk at the Registry session of the last interop meeting ? - In 2 "List of Categories" : * I would suggest to list here the complete list of Categories, therefore corresponding exactly to the subparagraphs of paragraphs 3 to 6 of the "Contents" ; "Type of Results" and Algorithm Parameters" are missing. * "Type of results" would be "d,c", similarly to "result format" * "Algorithm parameters" would be "d,c" * "Version of code" could be significant also for data (therefore should be "d,c") ; a simulation can be very (at least somewhat) different when obtained with a new version of a code ; so one has to know which version of the code it refers to. - 3.2 Name of code : As Dave de Young stated it, the word "name" is probably not the best one to refer to the code here. May be a vaguer word (appellation ?) should be used instead ; the associated ucd would then point to what the "appelation" is actually: * meta.id: identifier or name, although the recent discussion on the ucd-sci list, that Miguel mentionned in a previous mail, could make think that "id" refering to "identifier", could be considered in the future as something very specific (it has to be unique) and therefore should be distinguished from a name or a designation (but there is no meta.name at the moment), * meta.bib.xxx (author, bibcode) if the code is referred to by a publication reference * meta.ref.url in case of a reference to a web page * ... Notice that the second ucd word "comp.code" is not mentionned in the list of suggested UCDs at the end of the document. Two questions here: * can the atom "code" be used with a meaning different from what it has in other ucd words (meta.code) ? * is not it possible to use the already existing ucd "meta.software" instead ? - 3.3 Version of code : requiring the version to be a number may seem constraining ; it could be any string, especially the month or date of the release of the version ("jul2006", "2005-11-23", ...) ; I then agree with the precisions added by Miguel. - 4. Physics of Code : I think it would be more natural to put "Subject" before "Physical Objective" and "Physical Processes" ("which object ?", "what ?", "how ?") - 4.1 Physical Objective : there is probably no need to add the word "meta.main" at the end of the ucd as Laurie suggested to leave the possibility of multiple entries for (almost) all categories. - 5.3 Protocol the name of this category comes from the initial suggestion by Laurie but this name seems now unrelevant given all the related additional proposals. May be a broader category should be thought of here ("Computing" ?) under which several more specific informations are possibly supplied : * parallelisation (yes/no), vectorisation * if parallelisation, library used : OpenMP, MPI; way memory is used, ... * language(s) of the code : C, C++, Fortran77, Fortran90, ... * ... The above are relevant for codes, but some informative parameters could possibly be added for simulation data under a "Computing" header : * cpu time needed to compute the simulation (+ info on processor) * size of the simulation These informations could may be be useful in worflows: "given the size and cpu time needed, is it worth rerunning the program ?" - could have to do with SNAP as well - 6.2 Results Formats why not adding VOTable here which was agreed after Victoria to be data format used by theory specific services to send data products ? Very minor supplementary comments : - the "Abstract" should probably be more explicit in the final version - adding the page numbers on each page of the document would ease its reading - in par. 1 (Introduction), why talking about "snip of simulation code" whereas the aim is certainly to register very big codes ? (a wink ;-) in a tough text ?...) Finally, I have a suggestion which may be worth being discussed : as a goal of the present technical note is to provide clues to register codes and simulations and if the content of the note is more or less agreed in Moscow, would it be worth setting up a tentative "theory registry" (or ask people managing one of the registries to implement the theory extensions); the aim of it would be to have a testbench for trying to register existing simulation codes and data in the framework of the technical note and for simulating queries aiming at locating simulation codes/data. May be this would have to be discussed with big projects such as VO-Tech. With best regards, Bernard Debray -- Observatoire de Besançon | http://www.obs-besancon.fr/ 41 bis, avenue de l'Observatoire | bernard.debray@obs-besancon.fr BP 1615 | Tel : (33) 3 81 66 69 28 25010 Besançon cedex | Fax : (33) 3 81 66 69 44 France | Laurie Shaw wrote: >Hi Everyone, > >Attached is a first draft of the technical note that I have been writing >for simulation Semantics. Based on the discussions at and after the >Victoria meeting, and on early work on the Simulation data models, I break >down the meta-data requirements to describe simulations into a set of >categories. Each category itself must be labelled by a UCD, for which have >made initial suggestions. The typical contents of a category varies >between single characters or numbers, ascii text (or urls, names etc) and >words from the standard vocabulary (which is still largely to be defined). > >I've attached the doc in both ms word and pdf formats. Would be great to >have a brief discussion about this before the Moscow meeting -- I still >have time to make lots of changes, if needed! > >Thanks, > >Laurie ---------------------------------------------------------------- This message was sent using IMP, the Internet Messaging Program. From owner-theory@eso.org Fri Sep 15 19:25:34 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k8FHPTCW008008 for ; Fri, 15 Sep 2006 19:25:29 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k8FHPTI9008006 for theory-outgoing; Fri, 15 Sep 2006 19:25:29 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k8FHPSe0008000 for ; Fri, 15 Sep 2006 19:25:28 +0200 (MEST) Received: from smtp.iaa.es (smtp.iaa.csic.es [193.146.145.11]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k8FHPQL5026927 for ; Fri, 15 Sep 2006 19:25:26 +0200 (CEST) Received: from [132.248.230.73] ([132.248.230.73]) (authenticated bits=0) by smtp.iaa.es (8.13.1/8.13.1) with ESMTP id k8FHPF6B032604; Fri, 15 Sep 2006 19:25:16 +0200 In-Reply-To: <20060915025627.uodcx2giypsg8cgc@webmail.obs-besancon.fr> References: <20060915025627.uodcx2giypsg8cgc@webmail.obs-besancon.fr> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <3A281F2A-E677-4579-BF86-60322FEF00CE@iaa.es> Cc: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Content-Transfer-Encoding: 7bit From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Re: draft Date: Fri, 15 Sep 2006 12:25:14 -0500 To: debray@obs-besancon.fr, theory@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: 2006.9.15.95442 Sender: owner-theory@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= hello, I agree with the coments by Bernard, in particular > Notice that the second ucd word "comp.code" is not mentionned in > the list of > suggested UCDs at the end of the document. Two questions here: > * can the atom "code" be used with a meaning different from what > it has in > other ucd words (meta.code) ? > * is not it possible to use the already existing ucd > "meta.software" instead? Yes! I think that meta.software could do a quite better job: - it avoid collisions with "codification" or other flags - it also allows to reuse the same fileds (name, parameters etc..) for VOTables describing pipe-lines (data reduction and simulations) that would be useful for future virtual telescopes... > 6.2 Results Formats > why not adding VOTable here which was agreed after Victoria to > be data > format used by theory specific services to send data products ? > Also agree. However, it is supposed that at the end, whatever the data-format, it should be included in a VOTable, isn't it? Any case, the "theoretical results" i am produced for synthesis models are in ascii-VOTable. > Finally, I have a suggestion which may be worth being discussed : > as a goal of the present technical note is to provide clues to > register codes > and simulations and if the content of the note is more or less > agreed in > Moscow, would it be worth setting up a tentative "theory > registry" (or ask > people managing one of the registries to implement the theory > extensions); the > aim of it would be to have a testbench for trying to register existing > simulation codes and data in the framework of the technical note > and for > simulating queries aiming at locating simulation codes/data. > May be this would have to be discussed with big projects such as VO- > Tech. I aslo aggree :) Since I will not be in moscow, here there is some comments: At the ESA-registry there is and area for register TSAP (theoretical simple access protocol) services. The problem is that there is no services registered there and there is no application that uses this registry at the moment (as far as I know, VOSpec use their own registry) I think that the real problem is to define the protocol to access theoretical data since: a) Theoretical data usually do not make use of COOSYS (that I think, is mandatory in VOTables with data) b) The parameter space of simulations is different that the one of observations (mainly defined by possitions or object names) So it is need to make a first query about the parameter space of the service before to make the query over the service, and before retrieve the desired simulations (3 steps are involved instead two). I do not exactly remenber, but in victoria meeting Pedro Osuna was going present a version of TSAP?. Any case, I think that it would be better to define the access protocol and then use this protocol for "identify" theoretical services. I think that it has the additional advantage that Applications would began to implement this kind of protocol even if there is no theoretical databases/workflows... so, once the theoretical services will be ready, it will be not needed to wait too much time before theoretical results can be accessible from VO Applications... (it is my suggestion). cheers miguel From owner-theory@eso.org Tue Sep 19 15:42:32 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k8JDgPl5017998 for ; Tue, 19 Sep 2006 15:42:25 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k8JDgPC5017997 for theory-outgoing; Tue, 19 Sep 2006 15:42:25 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k8JDgOEN017992 for ; Tue, 19 Sep 2006 15:42:24 +0200 (MEST) Received: from smtpsortant1.univ-lyon1.fr (smtpsortant1.univ-lyon1.fr [134.214.100.90]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k8JDg61x011524 for ; Tue, 19 Sep 2006 15:42:23 +0200 (CEST) Received: from localhost (localhost [127.0.0.1]) by smtpsortant1.univ-lyon1.fr (Postfix) with ESMTP id 7D51243A5B2 for ; Tue, 19 Sep 2006 15:00:18 +0200 (CEST) Received: from smtpsortant1.univ-lyon1.fr ([127.0.0.1]) by localhost (smtpsortant1.univ-lyon1.fr [127.0.0.1]) (amavisd-new, port 10024) with ESMTP id 08162-07 for ; Tue, 19 Sep 2006 15:00:17 +0200 (CEST) Received: from obs.univ-lyon1.fr (obs.univ-lyon1.fr [134.214.4.140]) by smtpsortant1.univ-lyon1.fr (Postfix) with ESMTP id 1BCCF43A1BA for ; Tue, 19 Sep 2006 14:56:54 +0200 (CEST) Received: from [127.0.0.1] (foehn.univ-lyon1.fr [134.214.4.21]) by obs.univ-lyon1.fr (Postfix) with ESMTP id 17FEE4BB4F; Tue, 19 Sep 2006 14:56:58 +0200 (CEST) Message-ID: <450FE906.2090306@obs.univ-lyon1.fr> Date: Tue, 19 Sep 2006 14:56:38 +0200 From: Herve Wozniak User-Agent: Thunderbird 1.5.0.7 (Windows/20060909) MIME-Version: 1.0 To: theory@ivoa.net Subject: theory session in Moscow Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Virus-Scanned: by amavisd-new-20030616-p10 (Debian) at univ-lyon1.fr X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.0.266434, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.9.19.61942 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Herve Wozniak Hi theorists, I've uploaded the two documents that have been discussed in Moscow today and the minutes of the session taken by Franck (thanks Franck for this tricky task!). it includes questions and interesting suggestions. See the dedicated page: http://www.ivoa.net/twiki/bin/view/IVOA/InterOpSep2006Theory I will try to elaborate on a more detailed document, maybe in ppt format, later on. Regards, Herve -- _______________________________________________________________ Herve WOZNIAK Centre de Recherche Astronomique de Lyon UMR 5574 Université Lyon I - CNRS - ENS-Lyon 9, avenue Charles Andre, F-69561 Saint Genis Laval cedex Phone: (+33) (0) 478 868 388 Fax: (+33) (0) 478 868 386 http://www-obs.univ-lyon1.fr/herve.wozniak/ From owner-theory@eso.org Mon Oct 2 09:49:45 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 k927mDtw009053 for ; Mon, 2 Oct 2006 09:48:13 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id k927mDvG009052 for theory-outgoing; Mon, 2 Oct 2006 09:48:13 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 k927mCe5009048 for ; Mon, 2 Oct 2006 09:48:12 +0200 (MEST) Received: from smtp.iaa.es (smtp.iaa.csic.es [193.146.145.11]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id k927mASL010771 for ; Mon, 2 Oct 2006 09:48:11 +0200 (CEST) Received: from [161.111.166.120] (dfe-d20.iaa.csic.es [161.111.166.120]) (authenticated bits=0) by smtp.iaa.es (8.13.1/8.13.1) with ESMTP id k927m56O018108; Mon, 2 Oct 2006 09:48:05 +0200 Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=WINDOWS-1252; delsp=yes; format=flowed Message-Id: <4F7920F5-C41B-450E-B967-209D3A40D517@iaa.es> Cc: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Theory meetining? Date: Mon, 2 Oct 2006 09:48:04 +0200 To: theory@ivoa.net X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.0.266434, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.10.2.1943 Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id k927mCe5009049 Sender: owner-theory@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Dear all, I was just reading the wiki documents from the Moscow Interop. meeting and I have seen that it is proposed a mid-term meeting on Dec 2006 or Jan 2007 http://www.ivoa.net/internal/IVOA/InterOpSep2006Plenary/TIG_closing.pdf where it is written: • Need a ‘Mid-term meeting’ before next INTEROP – likely in GarchingDecember 06 or January 07 – 1 ‘theory’ representative of each national VO – Work breakdown between people really willing to participate to developments/implementations Where I would find more info about the mid-term meeting? Additionally, there will be a conference in December in Canary Islands about stelar population synthesis. It was scheduled in the original program a round-table about VO, but from science and code developers point of view, so there will be a pool of people potencialy interested in theory developments in the VO. I was thinking to ask there about the output data format for synthesis models and also about some points about characterization (in particular I would like to obtain feedback about the "code of codes" issue implicit in synthesis models). If there is another questions that would be relevant for the theory group (at this moment or for the near future), please, let me know (I will try to push that some people in evolutionary synthesis get involved in the IVOA theory group, but I am not too optimistic about this issue at this moment) cheers miguel From owner-theory@eso.org Wed Nov 15 22:25:52 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 kAFLPkkT003775 for ; Wed, 15 Nov 2006 22:25:46 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id kAFLPkOZ003774 for theory-outgoing; Wed, 15 Nov 2006 22:25:46 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 kAFLHXoU002875; Wed, 15 Nov 2006 22:17:34 +0100 (MET) Received: from [10.0.1.2] (p5496F46A.dip.t-dialin.net [84.150.244.106]) (authenticated bits=0) by clyde.hq.eso.org (8.12.8/8.12.8) with ESMTP id kAFLHWfj031424 (version=TLSv1/SSLv3 cipher=AES128-SHA bits=128 verify=NOT); Wed, 15 Nov 2006 22:17:33 +0100 In-Reply-To: <83BB6883-226C-40EC-B266-280310C48E3D@iaa.es> References: <83BB6883-226C-40EC-B266-280310C48E3D@iaa.es> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=ISO-8859-1; delsp=yes; format=flowed Message-Id: <5BB3D771-5E22-4182-859C-33ECF41990CE@eso.org> Cc: theory@ivoa.net, apps@ivoa.net From: Alberto Micol Subject: Re: tehoretical SEDs in VO applications Date: Wed, 15 Nov 2006 22:17:29 +0100 To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= X-Mailer: Apple Mail (2.752.2) Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id kAFLHYoU002876 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Alberto Micol Dear Miguel, I found your comparison an incredibly useful and interesting exercise. I think there should be a specific VO body to thoroughly perform this kind of investigations and comparison, including applications, protocol, data model or registry compliancy, etc. because the lessons that can be learned should be considered of paramount importance in the development of the VO. But that is already known. So, let me ask you just a question regarding your point (c.1): you mention 3 specview requirements, but then only 2 points (i and ii) are given (unless you count c1 ii as two requirements, one for x and one for y). I found any lesson learned so valuable that I prefer to ask what is maybe obvious. Was (ii) to be counted twice or (iii) was left in your fingertips? Thanks, Alberto On May 4, 2006, at 14:42, Miguel Cerviño wrote: > Dear all, > > I just send this comments that may be discussed in the next meeting. > It is just a comparison about how different VO applications manage > a SED building following the SED data model requirements. > [...] > c) Columns to be plotted: > > c.1) specview needs 3 requirements to plot a VOTable: > > i.- the Table must have a name (only VOTables with name="whatever"> looks to work > ii.- utype in x and y coordinates in FIELD must be specified > > c.2) VOSpec needs two (non-standard) lines to > specify the columns and only > two columns can be plotted (i.e. do not include for > example a column with errors that would be > useful for both observations and theoretical data. > [...] > I hope that this comments would help to improve the applications > and for the theory group > > best regards > > Miguel Cerviño > > From owner-apps@eso.org Wed Nov 15 22:26:03 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 kAFLPkCC003770 for ; Wed, 15 Nov 2006 22:25:46 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id kAFLPkEq003769 for apps-outgoing; Wed, 15 Nov 2006 22:25:46 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-apps@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 kAFLHXoU002875; Wed, 15 Nov 2006 22:17:34 +0100 (MET) Received: from [10.0.1.2] (p5496F46A.dip.t-dialin.net [84.150.244.106]) (authenticated bits=0) by clyde.hq.eso.org (8.12.8/8.12.8) with ESMTP id kAFLHWfj031424 (version=TLSv1/SSLv3 cipher=AES128-SHA bits=128 verify=NOT); Wed, 15 Nov 2006 22:17:33 +0100 In-Reply-To: <83BB6883-226C-40EC-B266-280310C48E3D@iaa.es> References: <83BB6883-226C-40EC-B266-280310C48E3D@iaa.es> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=ISO-8859-1; delsp=yes; format=flowed Message-Id: <5BB3D771-5E22-4182-859C-33ECF41990CE@eso.org> Cc: theory@ivoa.net, apps@ivoa.net From: Alberto Micol Subject: Re: tehoretical SEDs in VO applications Date: Wed, 15 Nov 2006 22:17:29 +0100 To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= X-Mailer: Apple Mail (2.752.2) Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id kAFLHYoU002876 Sender: owner-apps@eso.org Precedence: bulk Reply-To: Alberto Micol Dear Miguel, I found your comparison an incredibly useful and interesting exercise. I think there should be a specific VO body to thoroughly perform this kind of investigations and comparison, including applications, protocol, data model or registry compliancy, etc. because the lessons that can be learned should be considered of paramount importance in the development of the VO. But that is already known. So, let me ask you just a question regarding your point (c.1): you mention 3 specview requirements, but then only 2 points (i and ii) are given (unless you count c1 ii as two requirements, one for x and one for y). I found any lesson learned so valuable that I prefer to ask what is maybe obvious. Was (ii) to be counted twice or (iii) was left in your fingertips? Thanks, Alberto On May 4, 2006, at 14:42, Miguel Cerviño wrote: > Dear all, > > I just send this comments that may be discussed in the next meeting. > It is just a comparison about how different VO applications manage > a SED building following the SED data model requirements. > [...] > c) Columns to be plotted: > > c.1) specview needs 3 requirements to plot a VOTable: > > i.- the Table must have a name (only VOTables with
name="whatever"> looks to work > ii.- utype in x and y coordinates in FIELD must be specified > > c.2) VOSpec needs two (non-standard) lines to > specify the columns and only > two columns can be plotted (i.e. do not include for > example a column with errors that would be > useful for both observations and theoretical data. > [...] > I hope that this comments would help to improve the applications > and for the theory group > > best regards > > Miguel Cerviño > > From owner-theory@eso.org Thu Nov 16 12:19:31 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 kAGBJINP007159 for ; Thu, 16 Nov 2006 12:19:18 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id kAGBJISC007158 for theory-outgoing; Thu, 16 Nov 2006 12:19:18 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 kAGBJIfE007154; Thu, 16 Nov 2006 12:19:18 +0100 (MET) Received: from smtp.iaa.es (smtp.iaa.csic.es [193.146.145.11]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id kAGBJGXh000606; Thu, 16 Nov 2006 12:19:16 +0100 (CET) Received: from [161.111.165.12] (dae2.iaa.csic.es [161.111.165.12]) (authenticated bits=0) by smtp.iaa.es (8.13.1/8.13.1) with ESMTP id kAGBJ9Pb023510; Thu, 16 Nov 2006 12:19:10 +0100 In-Reply-To: <5BB3D771-5E22-4182-859C-33ECF41990CE@eso.org> References: <83BB6883-226C-40EC-B266-280310C48E3D@iaa.es> <5BB3D771-5E22-4182-859C-33ECF41990CE@eso.org> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=ISO-8859-1; delsp=yes; format=flowed Message-Id: Cc: theory@ivoa.net, apps@ivoa.net From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Re: tehoretical SEDs in VO applications Date: Thu, 16 Nov 2006 12:19:14 +0100 To: Alberto Micol X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.0.266434, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.11.16.30434 Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id kAGBJIfE007155 Sender: owner-theory@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Dear Alberto and all, I just tested with specview (2.12.2) to answer the question by Alberto. (I didn´t remeber if I had lost something in item (iii) The answer is about specview: i) it is needed a "name" in the table tag (or maybe in any other place) ii) it is needed the utype in X iii) it is needed the utype in Y so > Was (ii) to be counted twice or (iii) was left in your fingertips? The minimal VOTable it manage is:
..... Surprisely I had found that specview is not able to manage the VOTables generated by itself at least in ascii!! At leats for the table i had donwload (first HTS data from I zw 18), the VOTable that is obtained when it is saved produce two
elements, and specview only manage the first one with observational metadata. I had need to load the table in TopCat and save it again with topcat to obtain a VOTable that spceview reads. Any case I will try to repeat the exercise again in some weeks ... cheers Miguel From owner-apps@eso.org Thu Nov 16 12:19:32 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 kAGBJJt4007165 for ; Thu, 16 Nov 2006 12:19:19 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id kAGBJJh8007163 for apps-outgoing; Thu, 16 Nov 2006 12:19:19 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-apps@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 kAGBJIfE007154; Thu, 16 Nov 2006 12:19:18 +0100 (MET) Received: from smtp.iaa.es (smtp.iaa.csic.es [193.146.145.11]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id kAGBJGXh000606; Thu, 16 Nov 2006 12:19:16 +0100 (CET) Received: from [161.111.165.12] (dae2.iaa.csic.es [161.111.165.12]) (authenticated bits=0) by smtp.iaa.es (8.13.1/8.13.1) with ESMTP id kAGBJ9Pb023510; Thu, 16 Nov 2006 12:19:10 +0100 In-Reply-To: <5BB3D771-5E22-4182-859C-33ECF41990CE@eso.org> References: <83BB6883-226C-40EC-B266-280310C48E3D@iaa.es> <5BB3D771-5E22-4182-859C-33ECF41990CE@eso.org> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=ISO-8859-1; delsp=yes; format=flowed Message-Id: Cc: theory@ivoa.net, apps@ivoa.net From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Re: tehoretical SEDs in VO applications Date: Thu, 16 Nov 2006 12:19:14 +0100 To: Alberto Micol X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.0.266434, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.11.16.30434 Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from quoted-printable to 8bit by mercury.hq.eso.org id kAGBJIfE007155 Sender: owner-apps@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Dear Alberto and all, I just tested with specview (2.12.2) to answer the question by Alberto. (I didn´t remeber if I had lost something in item (iii) The answer is about specview: i) it is needed a "name" in the table tag (or maybe in any other place) ii) it is needed the utype in X iii) it is needed the utype in Y so > Was (ii) to be counted twice or (iii) was left in your fingertips? The minimal VOTable it manage is:
..... Surprisely I had found that specview is not able to manage the VOTables generated by itself at least in ascii!! At leats for the table i had donwload (first HTS data from I zw 18), the VOTable that is obtained when it is saved produce two
elements, and specview only manage the first one with observational metadata. I had need to load the table in TopCat and save it again with topcat to obtain a VOTable that spceview reads. Any case I will try to repeat the exercise again in some weeks ... cheers Miguel From owner-theory@eso.org Thu Nov 16 14:36:59 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 kAGDamqb000768 for ; Thu, 16 Nov 2006 14:36:48 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id kAGDamIu000767 for theory-outgoing; Thu, 16 Nov 2006 14:36:48 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 kAGDal16000763; Thu, 16 Nov 2006 14:36:47 +0100 (MET) Received: from donner.stsci.edu (donner.stsci.edu [130.167.251.65]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id kAGDaiXh011751; Thu, 16 Nov 2006 14:36:45 +0100 (CET) Received: from stsci.edu (obiwan.stsci.edu [130.167.236.123]) by donner.stsci.edu (MOS 3.7.2-GA) with ESMTP id EHA60323; Thu, 16 Nov 2006 08:35:09 -0500 (EST) Message-ID: <455C690D.3070501@stsci.edu> Date: Thu, 16 Nov 2006 08:35:09 -0500 From: Ivo Busko User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.0; en-US; rv:1.0.1) Gecko/20020823 Netscape/7.0 (CK-STScI-CPT) X-Accept-Language: en-us, en MIME-Version: 1.0 To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= CC: Alberto Micol , theory@ivoa.net, apps@ivoa.net Subject: Re: tehoretical SEDs in VO applications References: <83BB6883-226C-40EC-B266-280310C48E3D@iaa.es> <5BB3D771-5E22-4182-859C-33ECF41990CE@eso.org> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Junkmail-Whitelist: YES (by domain whitelist at donner.stsci.edu) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.0.266434, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.11.16.52432 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Ivo Busko Hi, Miguel and all As the specview developer, I would like to add my 0.02 cents to the discussion. In fact, I would like to warn about the use of specview to generate "valid" VO-compliant files. The "Save as" and "Save" options write data in xml files (no FITS support yet) following the standards set by the Spectrum Data Model in its 0.92 incarnation. But the code is still incomplete as far as metadata goes. Not all valid metadata described in 0.92 is actually passed thru and ends up in the output xml file. Other errors and inconsistencies may exiist as well. My poiny is, don't take specview's output as a well rounded, finished example of a VO-compliant file. It's work in progress. Besides, there were significant developments in the Data Model model since 0.92, and none of these are implemented in specview yet. Miguel, could you please provide me with a copy of the HTS data from I zw 18? I would like to see what is going on. In the examples I have, the entire file generated by specview is read back, even when multiple tables are present. And, what exactly do you mean by "at least in ascii"? Specview supports a simple ascii table format, but that has nothing to do with the VO xml format. Cheers, -Ivo ********************************************************************* * Ivo C. Busko, PhD e-mail: busko@stsci.edu * * Senior Systems Software Engineer Voice: (410)338-4472 * * Astronomy Tools and Applications FAX: (410)338-4767 * * Engineering and Software Services Division * * Space Telescope Science Institute http://www.stsci.edu * * 3700 San Martin Drive * * Baltimore MD 21218-2410 USA * ********************************************************************* Miguel Cerviño wrote: > Dear Alberto and all, > > I just tested with specview (2.12.2) to answer the question by Alberto. > (I didn´t remeber if I had lost something in item (iii) > The answer is about specview: > > i) it is needed a "name" in the table tag (or maybe in any other place) > ii) it is needed the utype in X > iii) it is needed the utype in Y > > so > >> Was (ii) to be counted twice or (iii) was left in your fingertips? > > > The minimal VOTable it manage is: > > > xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" > xsi:schemaLocation="http://www.ivoa.net/xml/VOTable/v1.1 http:// > www.ivoa.net/xml/VOTable/v1.1" > xmlns="http://www.ivoa.net/xml/VOTable/v1.1"> > >
> utype="sed:Segment.Points.SpectralCoord.Value"/> > utype="sed:Segment.Points.Flux.Value"/> > > > ..... > > > Surprisely I had found that specview is not able to manage the VOTables > generated by itself at least in ascii!! > At leats for the table i had donwload (first HTS data from I zw 18), > the VOTable that is obtained when it is saved produce two
> elements, and specview only manage the first one with observational > metadata. I had need to load the table in TopCat and save it again with > topcat to obtain a VOTable that spceview reads. > > > Any case I will try to repeat the exercise again in some weeks ... > > cheers > > Miguel > > From owner-apps@eso.org Thu Nov 16 14:37:02 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 kAGDamY0000773 for ; Thu, 16 Nov 2006 14:36:48 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id kAGDamxu000772 for apps-outgoing; Thu, 16 Nov 2006 14:36:48 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-apps@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 kAGDal16000763; Thu, 16 Nov 2006 14:36:47 +0100 (MET) Received: from donner.stsci.edu (donner.stsci.edu [130.167.251.65]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id kAGDaiXh011751; Thu, 16 Nov 2006 14:36:45 +0100 (CET) Received: from stsci.edu (obiwan.stsci.edu [130.167.236.123]) by donner.stsci.edu (MOS 3.7.2-GA) with ESMTP id EHA60323; Thu, 16 Nov 2006 08:35:09 -0500 (EST) Message-ID: <455C690D.3070501@stsci.edu> Date: Thu, 16 Nov 2006 08:35:09 -0500 From: Ivo Busko User-Agent: Mozilla/5.0 (Windows; U; Windows NT 5.0; en-US; rv:1.0.1) Gecko/20020823 Netscape/7.0 (CK-STScI-CPT) X-Accept-Language: en-us, en MIME-Version: 1.0 To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= CC: Alberto Micol , theory@ivoa.net, apps@ivoa.net Subject: Re: tehoretical SEDs in VO applications References: <83BB6883-226C-40EC-B266-280310C48E3D@iaa.es> <5BB3D771-5E22-4182-859C-33ECF41990CE@eso.org> Content-Type: text/plain; charset=ISO-8859-1; format=flowed Content-Transfer-Encoding: 8bit X-Junkmail-Whitelist: YES (by domain whitelist at donner.stsci.edu) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.0.266434, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.11.16.52432 Sender: owner-apps@eso.org Precedence: bulk Reply-To: Ivo Busko Hi, Miguel and all As the specview developer, I would like to add my 0.02 cents to the discussion. In fact, I would like to warn about the use of specview to generate "valid" VO-compliant files. The "Save as" and "Save" options write data in xml files (no FITS support yet) following the standards set by the Spectrum Data Model in its 0.92 incarnation. But the code is still incomplete as far as metadata goes. Not all valid metadata described in 0.92 is actually passed thru and ends up in the output xml file. Other errors and inconsistencies may exiist as well. My poiny is, don't take specview's output as a well rounded, finished example of a VO-compliant file. It's work in progress. Besides, there were significant developments in the Data Model model since 0.92, and none of these are implemented in specview yet. Miguel, could you please provide me with a copy of the HTS data from I zw 18? I would like to see what is going on. In the examples I have, the entire file generated by specview is read back, even when multiple tables are present. And, what exactly do you mean by "at least in ascii"? Specview supports a simple ascii table format, but that has nothing to do with the VO xml format. Cheers, -Ivo ********************************************************************* * Ivo C. Busko, PhD e-mail: busko@stsci.edu * * Senior Systems Software Engineer Voice: (410)338-4472 * * Astronomy Tools and Applications FAX: (410)338-4767 * * Engineering and Software Services Division * * Space Telescope Science Institute http://www.stsci.edu * * 3700 San Martin Drive * * Baltimore MD 21218-2410 USA * ********************************************************************* Miguel Cerviño wrote: > Dear Alberto and all, > > I just tested with specview (2.12.2) to answer the question by Alberto. > (I didn´t remeber if I had lost something in item (iii) > The answer is about specview: > > i) it is needed a "name" in the table tag (or maybe in any other place) > ii) it is needed the utype in X > iii) it is needed the utype in Y > > so > >> Was (ii) to be counted twice or (iii) was left in your fingertips? > > > The minimal VOTable it manage is: > > > xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" > xsi:schemaLocation="http://www.ivoa.net/xml/VOTable/v1.1 http:// > www.ivoa.net/xml/VOTable/v1.1" > xmlns="http://www.ivoa.net/xml/VOTable/v1.1"> > >
> utype="sed:Segment.Points.SpectralCoord.Value"/> > utype="sed:Segment.Points.Flux.Value"/> > > > ..... > > > Surprisely I had found that specview is not able to manage the VOTables > generated by itself at least in ascii!! > At leats for the table i had donwload (first HTS data from I zw 18), > the VOTable that is obtained when it is saved produce two
> elements, and specview only manage the first one with observational > metadata. I had need to load the table in TopCat and save it again with > topcat to obtain a VOTable that spceview reads. > > > Any case I will try to repeat the exercise again in some weeks ... > > cheers > > Miguel > > From owner-theory@eso.org Fri Nov 17 16:33:47 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 kAHFXe0P012581 for ; Fri, 17 Nov 2006 16:33:40 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id kAHFXe9f012580 for theory-outgoing; Fri, 17 Nov 2006 16:33:40 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 kAHFXdnE012570; Fri, 17 Nov 2006 16:33:39 +0100 (MET) Received: from donner.stsci.edu (donner.stsci.edu [130.167.251.65]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id kAHFXaXh016569; Fri, 17 Nov 2006 16:33:36 +0100 (CET) Received: from comet.stsci.edu (comet.stsci.edu [130.167.251.67]) by donner.stsci.edu (MOS 3.7.2-GA) with ESMTP id EHJ58790; Fri, 17 Nov 2006 10:28:53 -0500 (EST) Received: (from comet.stsci.edu [68.54.166.247]) by comet.stsci.edu (MOS 3.7.2-GA) with HTTPS/1.1 id CMI06997 (AUTH busko); Fri, 17 Nov 2006 10:28:52 -0500 (EST) From: Ivo Busko Subject: Re: tehoretical SEDs in VO applications To: =?iso-8859-1?Q?Miguel=20Cervi=F1o?= Cc: theory@ivoa.net, apps@ivoa.net X-Mailer: Mirapoint Webmail Direct 3.7.2-GA MIME-Version: 1.0 Content-Type: text/plain; charset=UTF-8 Content-Transfer-Encoding: 7bit Message-Id: <20061117102852.CMI06997@comet.stsci.edu> Date: Fri, 17 Nov 2006 10:28:52 -0500 (EST) X-Junkmail-Whitelist: YES (by domain whitelist at donner.stsci.edu) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.0.266434, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.11.17.71932 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Ivo Busko Hi Miguel The ArrayIndexOutOfBoundsException error in specview is caused by a misspelled attribute in the input VOTable file. The target position must be specified as two values, for RA and DEC, and in the file you sent me there is only one value, like this: The "value" and "arraysize" attributes are inconsistent, thus the error. Now, I don't understand how this is possible, since the FITS header doesn't have any positional information from where the TargetPos field could be composed from. I run specview using FOS data retrieved from the STScI archive, which have an almost identical FITS header with the 1zw18 header, and the generated VOTable does not have any TargetPos field, as it should be. So I wonder if the original file you used as specview input is any different from STScI archive files, or if you edited the file, or something on those lines. Cheers, -Ivo From owner-apps@eso.org Fri Nov 17 16:33:51 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 kAHFXd0E012576 for ; Fri, 17 Nov 2006 16:33:39 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id kAHFXdK9012575 for apps-outgoing; Fri, 17 Nov 2006 16:33:39 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-apps@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 kAHFXdnE012570; Fri, 17 Nov 2006 16:33:39 +0100 (MET) Received: from donner.stsci.edu (donner.stsci.edu [130.167.251.65]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id kAHFXaXh016569; Fri, 17 Nov 2006 16:33:36 +0100 (CET) Received: from comet.stsci.edu (comet.stsci.edu [130.167.251.67]) by donner.stsci.edu (MOS 3.7.2-GA) with ESMTP id EHJ58790; Fri, 17 Nov 2006 10:28:53 -0500 (EST) Received: (from comet.stsci.edu [68.54.166.247]) by comet.stsci.edu (MOS 3.7.2-GA) with HTTPS/1.1 id CMI06997 (AUTH busko); Fri, 17 Nov 2006 10:28:52 -0500 (EST) From: Ivo Busko Subject: Re: tehoretical SEDs in VO applications To: =?iso-8859-1?Q?Miguel=20Cervi=F1o?= Cc: theory@ivoa.net, apps@ivoa.net X-Mailer: Mirapoint Webmail Direct 3.7.2-GA MIME-Version: 1.0 Content-Type: text/plain; charset=UTF-8 Content-Transfer-Encoding: 7bit Message-Id: <20061117102852.CMI06997@comet.stsci.edu> Date: Fri, 17 Nov 2006 10:28:52 -0500 (EST) X-Junkmail-Whitelist: YES (by domain whitelist at donner.stsci.edu) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.0.266434, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.11.17.71932 Sender: owner-apps@eso.org Precedence: bulk Reply-To: Ivo Busko Hi Miguel The ArrayIndexOutOfBoundsException error in specview is caused by a misspelled attribute in the input VOTable file. The target position must be specified as two values, for RA and DEC, and in the file you sent me there is only one value, like this: The "value" and "arraysize" attributes are inconsistent, thus the error. Now, I don't understand how this is possible, since the FITS header doesn't have any positional information from where the TargetPos field could be composed from. I run specview using FOS data retrieved from the STScI archive, which have an almost identical FITS header with the 1zw18 header, and the generated VOTable does not have any TargetPos field, as it should be. So I wonder if the original file you used as specview input is any different from STScI archive files, or if you edited the file, or something on those lines. Cheers, -Ivo From owner-theory@eso.org Fri Nov 17 17:29:25 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 kAHGTJPE021693 for ; Fri, 17 Nov 2006 17:29:19 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id kAHGTJnp021692 for theory-outgoing; Fri, 17 Nov 2006 17:29:19 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 kAHGTI8s021683; Fri, 17 Nov 2006 17:29:19 +0100 (MET) Received: from smtp.iaa.es (smtp.iaa.csic.es [193.146.145.11]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id kAHGTEJQ017996; Fri, 17 Nov 2006 17:29:15 +0100 (CET) Received: from [192.168.1.12] (126.30.217.87.dynamic.jazztel.es [87.217.30.126] (may be forged)) (authenticated bits=0) by smtp.iaa.es (8.13.1/8.13.1) with ESMTP id kAHGRi43008775; Fri, 17 Nov 2006 17:27:50 +0100 In-Reply-To: <20061117102852.CMI06997@comet.stsci.edu> References: <20061117102852.CMI06997@comet.stsci.edu> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <838B256F-CA78-4616-BBAA-C370AF80F4EF@iaa.es> Cc: theory@ivoa.net, apps@ivoa.net Content-Transfer-Encoding: 7bit From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Re: tehoretical SEDs in VO applications Date: Fri, 17 Nov 2006 17:27:49 +0100 To: busko@stsci.edu X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.0.266434, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.11.17.81433 Sender: owner-theory@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= uhmm, I had not modified the file... I just make the proof again ... and I obtain the same result I reported. The procces I use is: a) resolve I zw 18 coordinates with NED using the form in specview b) performe the search once the position is resolved Here is the data of the image I obtain: (it was "HST spectra" in the app, not "HST/FOS/SSAP") HST Spectra YES z0wp0104m MAST.HST.GHRS 143.50845833333 55.240944444444 http:// archive.stsci.edu/pub/vospectra/ghrs/z0wp0104m_vo.fits IZW18 1000 48734.779 48734.721 1992-04-22 17:17:00 1992-04-23 05:06:00 spectrum/ fits FK5 2000.000 G160M n n 1285.330 1321.280 WAVELENGTH FLUX SIGMA L ML-1T-3 ML-1T-3 1E-10 1E+7 1E+7 ANGSTROMS ERGS/CM^2/S/A ERGS/CM^2/S/ A IZW18 I found 3 possible alternatives: a) I am running spectview incorectly (I am ussing java -jar spectview.jar instead the distribution script) b) The different services that provide the spectra are different or provide different information in the FITS header, and specview manage it in a different way: In case (b) it shoud needed to answer if 1.- it would be an issue related to the application 2.- It would be an issue related with the service... (I can try to obtain the data from the same server with other applications and see what happens... but during next week) Cheers and nice weekend Miguel From owner-apps@eso.org Fri Nov 17 17:29:30 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 kAHGTK7Q021700 for ; Fri, 17 Nov 2006 17:29:20 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id kAHGTKak021699 for apps-outgoing; Fri, 17 Nov 2006 17:29:20 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-apps@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 kAHGTI8s021683; Fri, 17 Nov 2006 17:29:19 +0100 (MET) Received: from smtp.iaa.es (smtp.iaa.csic.es [193.146.145.11]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id kAHGTEJQ017996; Fri, 17 Nov 2006 17:29:15 +0100 (CET) Received: from [192.168.1.12] (126.30.217.87.dynamic.jazztel.es [87.217.30.126] (may be forged)) (authenticated bits=0) by smtp.iaa.es (8.13.1/8.13.1) with ESMTP id kAHGRi43008775; Fri, 17 Nov 2006 17:27:50 +0100 In-Reply-To: <20061117102852.CMI06997@comet.stsci.edu> References: <20061117102852.CMI06997@comet.stsci.edu> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <838B256F-CA78-4616-BBAA-C370AF80F4EF@iaa.es> Cc: theory@ivoa.net, apps@ivoa.net Content-Transfer-Encoding: 7bit From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Re: tehoretical SEDs in VO applications Date: Fri, 17 Nov 2006 17:27:49 +0100 To: busko@stsci.edu X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.0.266434, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.11.17.81433 Sender: owner-apps@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= uhmm, I had not modified the file... I just make the proof again ... and I obtain the same result I reported. The procces I use is: a) resolve I zw 18 coordinates with NED using the form in specview b) performe the search once the position is resolved Here is the data of the image I obtain: (it was "HST spectra" in the app, not "HST/FOS/SSAP") HST Spectra YES z0wp0104m MAST.HST.GHRS 143.50845833333 55.240944444444 http:// archive.stsci.edu/pub/vospectra/ghrs/z0wp0104m_vo.fits IZW18 1000 48734.779 48734.721 1992-04-22 17:17:00 1992-04-23 05:06:00 spectrum/ fits FK5 2000.000 G160M n n 1285.330 1321.280 WAVELENGTH FLUX SIGMA L ML-1T-3 ML-1T-3 1E-10 1E+7 1E+7 ANGSTROMS ERGS/CM^2/S/A ERGS/CM^2/S/ A IZW18 I found 3 possible alternatives: a) I am running spectview incorectly (I am ussing java -jar spectview.jar instead the distribution script) b) The different services that provide the spectra are different or provide different information in the FITS header, and specview manage it in a different way: In case (b) it shoud needed to answer if 1.- it would be an issue related to the application 2.- It would be an issue related with the service... (I can try to obtain the data from the same server with other applications and see what happens... but during next week) Cheers and nice weekend Miguel From owner-theory@eso.org Fri Nov 17 18:20:02 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 kAHHJu9g028560 for ; Fri, 17 Nov 2006 18:19:56 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id kAHHJuB9028559 for theory-outgoing; Fri, 17 Nov 2006 18:19:56 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 kAHHJtfV028555; Fri, 17 Nov 2006 18:19:55 +0100 (MET) Received: from smtp.iaa.es (smtp.iaa.csic.es [193.146.145.11]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id kAHHJrJQ022019; Fri, 17 Nov 2006 18:19:54 +0100 (CET) Received: from [192.168.1.131] (118.31.217.87.dynamic.jazztel.es [87.217.31.118] (may be forged)) (authenticated bits=0) by smtp.iaa.es (8.13.1/8.13.1) with ESMTP id kAHHJkrk014338; Fri, 17 Nov 2006 18:19:47 +0100 In-Reply-To: <838B256F-CA78-4616-BBAA-C370AF80F4EF@iaa.es> References: <20061117102852.CMI06997@comet.stsci.edu> <838B256F-CA78-4616-BBAA-C370AF80F4EF@iaa.es> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: Cc: busko@stsci.edu, theory@ivoa.net, apps@ivoa.net Content-Transfer-Encoding: 7bit From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Re: tehoretical SEDs in VO applications Date: Fri, 17 Nov 2006 18:19:51 +0100 To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.0.266434, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.11.17.90932 Sender: owner-theory@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= sorry, To avoid misunderstandings: 3 possible alternatives: a) I am running spectview incorrectly b) There is a problem in specview (when retrieve from "HST spectra" or write the VOTable) c) There is a problem with the service that provide the "HST spectra" sorry for my typing errors miguel > I found 3 possible alternatives: > > a) I am running spectview incorectly (I am ussing java -jar > spectview.jar instead the distribution script) > b) The different services that provide the spectra are different or > provide different information in the FITS header, and specview > manage it in a different way: > > In case (b) it shoud needed to answer if > 1.- it would be an issue related to the application > 2.- It would be an issue related with the service... (I can try > to obtain the data from the same server with other applications and > see what happens... but during next week) > > > Cheers and nice weekend > > Miguel > From owner-apps@eso.org Fri Nov 17 18:20:07 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 kAHHJuwr028565 for ; Fri, 17 Nov 2006 18:19:56 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id kAHHJuga028564 for apps-outgoing; Fri, 17 Nov 2006 18:19:56 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-apps@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 kAHHJtfV028555; Fri, 17 Nov 2006 18:19:55 +0100 (MET) Received: from smtp.iaa.es (smtp.iaa.csic.es [193.146.145.11]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id kAHHJrJQ022019; Fri, 17 Nov 2006 18:19:54 +0100 (CET) Received: from [192.168.1.131] (118.31.217.87.dynamic.jazztel.es [87.217.31.118] (may be forged)) (authenticated bits=0) by smtp.iaa.es (8.13.1/8.13.1) with ESMTP id kAHHJkrk014338; Fri, 17 Nov 2006 18:19:47 +0100 In-Reply-To: <838B256F-CA78-4616-BBAA-C370AF80F4EF@iaa.es> References: <20061117102852.CMI06997@comet.stsci.edu> <838B256F-CA78-4616-BBAA-C370AF80F4EF@iaa.es> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: Cc: busko@stsci.edu, theory@ivoa.net, apps@ivoa.net Content-Transfer-Encoding: 7bit From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Re: tehoretical SEDs in VO applications Date: Fri, 17 Nov 2006 18:19:51 +0100 To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.0.266434, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.11.17.90932 Sender: owner-apps@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= sorry, To avoid misunderstandings: 3 possible alternatives: a) I am running spectview incorrectly b) There is a problem in specview (when retrieve from "HST spectra" or write the VOTable) c) There is a problem with the service that provide the "HST spectra" sorry for my typing errors miguel > I found 3 possible alternatives: > > a) I am running spectview incorectly (I am ussing java -jar > spectview.jar instead the distribution script) > b) The different services that provide the spectra are different or > provide different information in the FITS header, and specview > manage it in a different way: > > In case (b) it shoud needed to answer if > 1.- it would be an issue related to the application > 2.- It would be an issue related with the service... (I can try > to obtain the data from the same server with other applications and > see what happens... but during next week) > > > Cheers and nice weekend > > Miguel > From owner-theory@eso.org Fri Nov 17 19:09:01 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 kAHI8uIw004831 for ; Fri, 17 Nov 2006 19:08:56 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id kAHI8u33004830 for theory-outgoing; Fri, 17 Nov 2006 19:08:56 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 kAHI8tiQ004821; Fri, 17 Nov 2006 19:08:55 +0100 (MET) Received: from donner.stsci.edu (donner.stsci.edu [130.167.251.65]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id kAHI8qXh027535; Fri, 17 Nov 2006 19:08:53 +0100 (CET) Received: from comet.stsci.edu (comet.stsci.edu [130.167.251.67]) by donner.stsci.edu (MOS 3.7.2-GA) with ESMTP id EHK24912; Fri, 17 Nov 2006 13:08:47 -0500 (EST) Received: (from comet.stsci.edu [68.54.166.247]) by comet.stsci.edu (MOS 3.7.2-GA) with HTTPS/1.1 id CMI15037 (AUTH busko); Fri, 17 Nov 2006 13:08:46 -0500 (EST) From: Ivo Busko Subject: Re: tehoretical SEDs in VO applications To: =?iso-8859-1?Q?Miguel=20Cervi=F1o?= Cc: theory@ivoa.net, apps@ivoa.net X-Mailer: Mirapoint Webmail Direct 3.7.2-GA MIME-Version: 1.0 Content-Type: text/plain; charset=UTF-8 Message-Id: <20061117130846.CMI15037@comet.stsci.edu> Date: Fri, 17 Nov 2006 13:08:46 -0500 (EST) X-Junkmail-Whitelist: YES (by domain whitelist at donner.stsci.edu) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.0.266434, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.11.17.95432 Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from base64 to 8bit by mercury.hq.eso.org id kAHI8uiQ004822 Sender: owner-theory@eso.org Precedence: bulk Reply-To: Ivo Busko Hi, Miguel Ah, you are reading directly from a SSAP service... OK, so it is a bug in specview after all. A good example of how the code is not yet propely tested. I fixed this particular bug, but other bugs are sure to surface sooner or later. The bug fix should be available on the next release. And thanks for providing the test case! -Ivo ---- Original message ---- >Date: Fri, 17 Nov 2006 18:19:51 +0100 >From: Miguel Cerviño >Subject: Re: tehoretical SEDs in VO applications >To: Miguel Cerviño >Cc: busko@stsci.edu, theory@ivoa.net, apps@ivoa.net > >sorry, > >To avoid misunderstandings: > >3 possible alternatives: > >a) I am running spectview incorrectly >b) There is a problem in specview (when retrieve from "HST spectra" >or write the VOTable) >c) There is a problem with the service that provide the "HST spectra" > >sorry for my typing errors > >miguel > >> I found 3 possible alternatives: >> >> a) I am running spectview incorectly (I am ussing java -jar >> spectview.jar instead the distribution script) >> b) The different services that provide the spectra are different or >> provide different information in the FITS header, and specview >> manage it in a different way: >> >> In case (b) it shoud needed to answer if >> 1.- it would be an issue related to the application >> 2.- It would be an issue related with the service... (I can try >> to obtain the data from the same server with other applications and >> see what happens... but during next week) >> >> >> Cheers and nice weekend >> >> Miguel >> > From owner-apps@eso.org Fri Nov 17 19:09:06 2006 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 kAHI8umn004826 for ; Fri, 17 Nov 2006 19:08:56 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id kAHI8u3G004825 for apps-outgoing; Fri, 17 Nov 2006 19:08:56 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-apps@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 kAHI8tiQ004821; Fri, 17 Nov 2006 19:08:55 +0100 (MET) Received: from donner.stsci.edu (donner.stsci.edu [130.167.251.65]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id kAHI8qXh027535; Fri, 17 Nov 2006 19:08:53 +0100 (CET) Received: from comet.stsci.edu (comet.stsci.edu [130.167.251.67]) by donner.stsci.edu (MOS 3.7.2-GA) with ESMTP id EHK24912; Fri, 17 Nov 2006 13:08:47 -0500 (EST) Received: (from comet.stsci.edu [68.54.166.247]) by comet.stsci.edu (MOS 3.7.2-GA) with HTTPS/1.1 id CMI15037 (AUTH busko); Fri, 17 Nov 2006 13:08:46 -0500 (EST) From: Ivo Busko Subject: Re: tehoretical SEDs in VO applications To: =?iso-8859-1?Q?Miguel=20Cervi=F1o?= Cc: theory@ivoa.net, apps@ivoa.net X-Mailer: Mirapoint Webmail Direct 3.7.2-GA MIME-Version: 1.0 Content-Type: text/plain; charset=UTF-8 Message-Id: <20061117130846.CMI15037@comet.stsci.edu> Date: Fri, 17 Nov 2006 13:08:46 -0500 (EST) X-Junkmail-Whitelist: YES (by domain whitelist at donner.stsci.edu) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.0.266434, Antispam-Engine: 2.4.0.264935, Antispam-Data: 2006.11.17.95432 Content-Transfer-Encoding: 8bit X-MIME-Autoconverted: from base64 to 8bit by mercury.hq.eso.org id kAHI8uiQ004822 Sender: owner-apps@eso.org Precedence: bulk Reply-To: Ivo Busko Hi, Miguel Ah, you are reading directly from a SSAP service... OK, so it is a bug in specview after all. A good example of how the code is not yet propely tested. I fixed this particular bug, but other bugs are sure to surface sooner or later. The bug fix should be available on the next release. And thanks for providing the test case! -Ivo ---- Original message ---- >Date: Fri, 17 Nov 2006 18:19:51 +0100 >From: Miguel Cerviño >Subject: Re: tehoretical SEDs in VO applications >To: Miguel Cerviño >Cc: busko@stsci.edu, theory@ivoa.net, apps@ivoa.net > >sorry, > >To avoid misunderstandings: > >3 possible alternatives: > >a) I am running spectview incorrectly >b) There is a problem in specview (when retrieve from "HST spectra" >or write the VOTable) >c) There is a problem with the service that provide the "HST spectra" > >sorry for my typing errors > >miguel > >> I found 3 possible alternatives: >> >> a) I am running spectview incorectly (I am ussing java -jar >> spectview.jar instead the distribution script) >> b) The different services that provide the spectra are different or >> provide different information in the FITS header, and specview >> manage it in a different way: >> >> In case (b) it shoud needed to answer if >> 1.- it would be an issue related to the application >> 2.- It would be an issue related with the service... (I can try >> to obtain the data from the same server with other applications and >> see what happens... but during next week) >> >> >> Cheers and nice weekend >> >> Miguel >> > From owner-theory@eso.org Wed Dec 20 11:08:50 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 kBKA8XVM029017 for ; Wed, 20 Dec 2006 11:08:33 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id kBKA8XgA029016 for theory-outgoing; Wed, 20 Dec 2006 11:08:33 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 kBKA8W1i029010; Wed, 20 Dec 2006 11:08:32 +0100 (MET) Received: from smtp.iaa.es (smtp.iaa.csic.es [193.146.145.11]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id kBKA8Ug8010673; Wed, 20 Dec 2006 11:08:31 +0100 (CET) Received: from [161.111.165.12] (dae2.iaa.csic.es [161.111.165.12]) (authenticated bits=0) by smtp.iaa.es (8.13.1/8.13.1) with ESMTP id kBKA8M3j022468; Wed, 20 Dec 2006 11:08:22 +0100 Mime-Version: 1.0 (Apple Message framework v752.2) Content-Transfer-Encoding: 7bit Message-Id: <6D993361-4961-478C-8608-BB4AA04DA941@iaa.es> Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed To: theory@ivoa.net, apps@ivoa.net From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Report IAUSymp 241: Stellar Populations Date: Wed, 20 Dec 2006 11:08:22 +0100 X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.2.285561, Antispam-Engine: 2.5.0.283055, Antispam-Data: 2006.12.20.15433 Sender: owner-theory@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Hello all, There as been a meeting about Stellar populations (IAUSymp 241) where some issues related to the VO (theory and applications) has been discussed. The meeting was focus in science, and there was only few people was involve in VO activities, so it was a "preliminary contact" between VO and "real world" I send here a very draft about my impressions about this meeting that can be discussed in the list (there was other people in the metting, like Santi Cassisi, Herve Wozniak, Philippe Prugniel, Licai Deng (VOChina) and some people from VOIndia) that may be have a different impressions. 1) In general there was a strong interest of model developers to provide their results in the VO 2) They do not have any "guide" to do that. I had the feeling that, in general, they do not know how VO works, in particular the issues related with registry and about the role of national VO host and how to coordinate their activities. My impression is that they understand the VO as "another paper", in the sense that, systematically, when I asked if they had asked to their "national VO contact" for support, they didn't contact! Maybe more publicity about that is needed. A very simple guide that can be posted in astro-ph... 3) There was some confusion about issues related about the use of the codes in the VO. Some of them was thinking about "open source" codes (that is not necessarily the case) instead to make public their results. 4) In general, most of code developers was STRONGLY worried about how to keep the credits of their work. I think that it can be done in the PROVENANCE fileds of the tables, but, in any case, most of the applications does not hand provenance fields in a particular way (and sometimes, these fields are erased by the application when the final VOTable is saved).... I think that it will be the main issue to solve if we want convince "standard" astronomers to include their result in the VO (independently if the implementation is done by themselves following a guide or by third parties). 5) In the particular case of synthesis models results (and some case for atmosphere libraries and stellar tracks/isochrones) it would be interesting to make a "mail-list" where non-VO people would define what these object are and how it can be described in a unique way (i.e. produce a data model from the model developers but explained and described in a science context without VO words ;) 6) (Also a personal opinion) There is no way to access VOTables referenced inside VOTables (or at least, I know no application able do that). It will be useful since, synthesis models, or galaxy fitting models make use of "collections" of other theoretical/observational data (atmospheres libraries and isochrones in the first case or collections of synthesis models results in the second). Well, It is all, I any one have more ideas/suggestions/comments about this will be great :) Merry Xtmas Miguel From owner-apps@eso.org Wed Dec 20 11:08:59 2006 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 kBKA8Xb8029022 for ; Wed, 20 Dec 2006 11:08:33 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id kBKA8XTu029021 for apps-outgoing; Wed, 20 Dec 2006 11:08:33 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-apps@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 kBKA8W1i029010; Wed, 20 Dec 2006 11:08:32 +0100 (MET) Received: from smtp.iaa.es (smtp.iaa.csic.es [193.146.145.11]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id kBKA8Ug8010673; Wed, 20 Dec 2006 11:08:31 +0100 (CET) Received: from [161.111.165.12] (dae2.iaa.csic.es [161.111.165.12]) (authenticated bits=0) by smtp.iaa.es (8.13.1/8.13.1) with ESMTP id kBKA8M3j022468; Wed, 20 Dec 2006 11:08:22 +0100 Mime-Version: 1.0 (Apple Message framework v752.2) Content-Transfer-Encoding: 7bit Message-Id: <6D993361-4961-478C-8608-BB4AA04DA941@iaa.es> Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed To: theory@ivoa.net, apps@ivoa.net From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Report IAUSymp 241: Stellar Populations Date: Wed, 20 Dec 2006 11:08:22 +0100 X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.2.285561, Antispam-Engine: 2.5.0.283055, Antispam-Data: 2006.12.20.15433 Sender: owner-apps@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Hello all, There as been a meeting about Stellar populations (IAUSymp 241) where some issues related to the VO (theory and applications) has been discussed. The meeting was focus in science, and there was only few people was involve in VO activities, so it was a "preliminary contact" between VO and "real world" I send here a very draft about my impressions about this meeting that can be discussed in the list (there was other people in the metting, like Santi Cassisi, Herve Wozniak, Philippe Prugniel, Licai Deng (VOChina) and some people from VOIndia) that may be have a different impressions. 1) In general there was a strong interest of model developers to provide their results in the VO 2) They do not have any "guide" to do that. I had the feeling that, in general, they do not know how VO works, in particular the issues related with registry and about the role of national VO host and how to coordinate their activities. My impression is that they understand the VO as "another paper", in the sense that, systematically, when I asked if they had asked to their "national VO contact" for support, they didn't contact! Maybe more publicity about that is needed. A very simple guide that can be posted in astro-ph... 3) There was some confusion about issues related about the use of the codes in the VO. Some of them was thinking about "open source" codes (that is not necessarily the case) instead to make public their results. 4) In general, most of code developers was STRONGLY worried about how to keep the credits of their work. I think that it can be done in the PROVENANCE fileds of the tables, but, in any case, most of the applications does not hand provenance fields in a particular way (and sometimes, these fields are erased by the application when the final VOTable is saved).... I think that it will be the main issue to solve if we want convince "standard" astronomers to include their result in the VO (independently if the implementation is done by themselves following a guide or by third parties). 5) In the particular case of synthesis models results (and some case for atmosphere libraries and stellar tracks/isochrones) it would be interesting to make a "mail-list" where non-VO people would define what these object are and how it can be described in a unique way (i.e. produce a data model from the model developers but explained and described in a science context without VO words ;) 6) (Also a personal opinion) There is no way to access VOTables referenced inside VOTables (or at least, I know no application able do that). It will be useful since, synthesis models, or galaxy fitting models make use of "collections" of other theoretical/observational data (atmospheres libraries and isochrones in the first case or collections of synthesis models results in the second). Well, It is all, I any one have more ideas/suggestions/comments about this will be great :) Merry Xtmas Miguel From owner-theory@eso.org Fri Jan 26 10:14:45 2007 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 l0Q9Ebn0022326 for ; Fri, 26 Jan 2007 10:14:37 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id l0Q9EbY8022325 for theory-outgoing; Fri, 26 Jan 2007 10:14:37 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 l0Q9EajP022321; Fri, 26 Jan 2007 10:14:36 +0100 (MET) Received: from mpemail.mpe.mpg.de (mpemail.mpe-garching.mpg.de [130.183.137.110]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id l0Q9EZej003829; Fri, 26 Jan 2007 10:14:36 +0100 (CET) Received: from gavopc1.xray.mpe.mpg.de ([130.183.72.204] helo=gavopc1) by mpemail.mpe.mpg.de with esmtp (Exim 4.50) id 1HANAE-0007Eb-60; Fri, 26 Jan 2007 10:14:30 +0100 From: "Gerard" To: , Subject: simulation data models Date: Fri, 26 Jan 2007 10:14:48 +0100 Message-ID: <000501c7412a$6d5de390$cc48b782@gavopc1> MIME-Version: 1.0 Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 7bit X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.3028 Thread-Index: AcdBKm0+IjkfNybwSju9kBSwS7sAzA== X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.2.285561, Antispam-Engine: 2.5.0.283055, Antispam-Data: 2007.1.26.10433 X-Perl-Spam: Gauge=IIIIIII, Probability=7%, Report='__CT 0, __CTE 0, __CTYPE_CHARSET_QUOTED 0, __CT_TEXT_PLAIN 0, __HAS_MSGID 0, __HAS_X_MAILER 0, __MIME_TEXT_ONLY 0, __MIME_VERSION 0, __SANE_MSGID 0, __USER_AGENT_MS_GENERIC 0' Sender: owner-theory@eso.org Precedence: bulk Reply-To: "Gerard" Dear colleagues The theory interest group has been working on a project to create a data model describing the results of numerical simulations. The concrete focus of this model is that it should assist the simple numerical access protocol (SNAP, another theory IG project) in a similar way as the spectral data model assists the simple spectral access protocol. As defined in Victoria, SNAP is supposed to deal with systems existing and evolving in 3 dimensional space. A scale is not prescribed, the simulations can range from full cosmological simulations down to formation of planets and everything in between. The first goal of the modeling exercise was to create a so called analysis model, which describes the domain we're interested in, without too much emphasis on the final use and implementations. We have a skeleton available, based on the patterns in the domain model I proposed with Pat Dowler some years ago (see the DM pages). To test this model out it would be good to have some concrete data models that people have used in their work. These may be explicit, such as models for a database storing simulation (meta-)data, some may be implicit, as in a description of attributes and data in HDF(5) files. We would like to get a hold of examples of such models, with the aim of investigating whether they can be described using the elements in the current model and to find out whether new features should be added. So my request is that if you own or know of the existence of such data models, and these are or can be made public, please mail me about this, so that we can take those models into account in this exercise. Thanks in advance Gerard Lemson From owner-dm@eso.org Fri Jan 26 10:14:53 2007 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 l0Q9EcXR022332 for ; Fri, 26 Jan 2007 10:14:38 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id l0Q9EbKv022331 for dm-outgoing; Fri, 26 Jan 2007 10:14:37 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dm@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.13.6+Sun/8.12.10) with ESMTP id l0Q9EajP022321; Fri, 26 Jan 2007 10:14:36 +0100 (MET) Received: from mpemail.mpe.mpg.de (mpemail.mpe-garching.mpg.de [130.183.137.110]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id l0Q9EZej003829; Fri, 26 Jan 2007 10:14:36 +0100 (CET) Received: from gavopc1.xray.mpe.mpg.de ([130.183.72.204] helo=gavopc1) by mpemail.mpe.mpg.de with esmtp (Exim 4.50) id 1HANAE-0007Eb-60; Fri, 26 Jan 2007 10:14:30 +0100 From: "Gerard" To: , Subject: simulation data models Date: Fri, 26 Jan 2007 10:14:48 +0100 Message-ID: <000501c7412a$6d5de390$cc48b782@gavopc1> MIME-Version: 1.0 Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 7bit X-Mailer: Microsoft Office Outlook 11 X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.3028 Thread-Index: AcdBKm0+IjkfNybwSju9kBSwS7sAzA== X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.2.285561, Antispam-Engine: 2.5.0.283055, Antispam-Data: 2007.1.26.10433 X-Perl-Spam: Gauge=IIIIIII, Probability=7%, Report='__CT 0, __CTE 0, __CTYPE_CHARSET_QUOTED 0, __CT_TEXT_PLAIN 0, __HAS_MSGID 0, __HAS_X_MAILER 0, __MIME_TEXT_ONLY 0, __MIME_VERSION 0, __SANE_MSGID 0, __USER_AGENT_MS_GENERIC 0' Sender: owner-dm@eso.org Precedence: bulk Reply-To: "Gerard" Dear colleagues The theory interest group has been working on a project to create a data model describing the results of numerical simulations. The concrete focus of this model is that it should assist the simple numerical access protocol (SNAP, another theory IG project) in a similar way as the spectral data model assists the simple spectral access protocol. As defined in Victoria, SNAP is supposed to deal with systems existing and evolving in 3 dimensional space. A scale is not prescribed, the simulations can range from full cosmological simulations down to formation of planets and everything in between. The first goal of the modeling exercise was to create a so called analysis model, which describes the domain we're interested in, without too much emphasis on the final use and implementations. We have a skeleton available, based on the patterns in the domain model I proposed with Pat Dowler some years ago (see the DM pages). To test this model out it would be good to have some concrete data models that people have used in their work. These may be explicit, such as models for a database storing simulation (meta-)data, some may be implicit, as in a description of attributes and data in HDF(5) files. We would like to get a hold of examples of such models, with the aim of investigating whether they can be described using the elements in the current model and to find out whether new features should be added. So my request is that if you own or know of the existence of such data models, and these are or can be made public, please mail me about this, so that we can take those models into account in this exercise. Thanks in advance Gerard Lemson From owner-theory@eso.org Fri Jan 26 23:36:56 2007 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 l0QMaiBg003804 for ; Fri, 26 Jan 2007 23:36:44 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id l0QMahFu003803 for theory-outgoing; Fri, 26 Jan 2007 23:36:43 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 l0QMafhP003791; Fri, 26 Jan 2007 23:36:42 +0100 (MET) Received: from pro.abac.com (pro.abac.com [66.226.64.2]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id l0QMadej000327; Fri, 26 Jan 2007 23:36:40 +0100 (CET) Received: from [132.239.66.176] (cassx176.ucsd.edu [132.239.66.176]) (authenticated bits=0) by pro.abac.com (8.13.8/8.13.8) with ESMTP id l0QMaTLJ011826; Fri, 26 Jan 2007 14:36:30 -0800 (PST) (envelope-from rwagner@physics.ucsd.edu) In-Reply-To: <000501c7412a$6d5de390$cc48b782@gavopc1> References: <000501c7412a$6d5de390$cc48b782@gavopc1> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: multipart/alternative; boundary=Apple-Mail-2-417750898 Message-Id: Cc: theory@ivoa.net, dm@ivoa.net, Mike Norman , evrard@umich.edu X-Mailer: Apple Mail (2.752.2) From: Rick Wagner Subject: Re: simulation data models Date: Fri, 26 Jan 2007 14:36:35 -0800 To: "Gerard" X-Spam-Score: 0.101 (HTML_MESSAGE) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.2.285561, Antispam-Engine: 2.5.0.283055, Antispam-Data: 2007.1.26.142433 X-Perl-Spam: Gauge=IIIIIII, Probability=7%, Report='HTML_50_70 0.1, __C230066_P5 0, __CP_URI_IN_BODY 0, __CT 0, __CTYPE_HAS_BOUNDARY 0, __CTYPE_MULTIPART 0, __CTYPE_MULTIPART_ALT 0, __FRAUD_419_INTRO 0, __HAS_MSGID 0, __HAS_X_MAILER 0, __MIME_HTML 0, __MIME_VERSION 0, __SANE_MSGID 0, __TAG_EXISTS_HTML 0' Sender: owner-theory@eso.org Precedence: bulk Reply-To: Rick Wagner --Apple-Mail-2-417750898 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Hello Gerard, Your message comes at a good time for me to introduce myself. I'm a graduate student working with Mike Norman at UCSD, and I attended the NVO Summer School this year to learn more about the IVOA, in the hopes of publishing the results of our simulations to the NVO. While at the Summer School, I implemented a SkyNode based on a use case you wrote up a while ago, the Theory SkyNode. I've been following the work of the Theory Interest Group from the sidelines, and am planning to go with whatever standards arise. Which is why the database tables exposed via the SkyNode are minimal, and only provide summary information on X-ray clusters identified in an existing archive. I am assuming I'll have to change things later, so I'm taking things slow. With that said, I've put some thought into how to organize our simulation data with the goal of it being published to the NVO. I'd be happy to organize my notes into a draft document, if you think it would be of use. Further, as a result of the Summer School, I was able to presented my work at AAS in Seattle. You can view a copy of my poster here: http://lca.ucsd.edu/Members/rpwagner/PosterRickWagner.pdf I spoke with Gus Evrard at AAS, and he expressed an interest to work on a common data model for galaxy clusters to enable code comparison. All three or our groups have built databases containing tabulated properties of simulated objects, and there may be enough common properties to the database schemas to draft a data model for clusters. Sincerely, Rick --------------------------------------------------------------- Rick Wagner, Graduate Student Researcher UCSD Physics 9500 Gilman Drive La Jolla, CA 92093-0424 Email: rwagner@physics.ucsd.edu WWW: http://lca.ucsd.edu (858) 822-4784 Phone --------------------------------------------------------------- --Apple-Mail-2-417750898 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1
Hello Gerard,

Your message comes at a = good time for me to introduce myself. I'm a graduate student working = with Mike Norman at UCSD, and I attended the NVO Summer School this year = to learn more about the IVOA, in the hopes of publishing the results of = our simulations to the NVO.

While at the Summer School, = I implemented a SkyNode based=A0=A0on a use case you wrote up a while = ago, the Theory SkyNode. I've been following the work of the Theory = Interest Group from the sidelines, and am planning to go with whatever = standards arise. Which is why the database tables exposed via the = SkyNode are minimal, and only provide summary information on X-ray = clusters identified in an existing archive. I am assuming I'll have to = change things later, so I'm taking things slow.=A0

With that said, I've put = some thought into how to organize our simulation data with the goal of = it being published to the NVO. I'd be happy to organize my notes into a = draft document, if you think it would be of use.=A0

Further, as a result of the = Summer School, I was able to presented my work at AAS in Seattle.=A0You = can view a copy of my poster here:

I spoke with Gus Evrard at = AAS, and he expressed an interest to work on a common data model for = galaxy clusters to enable code comparison. All three or our groups have = built databases containing tabulated properties of simulated objects, = and there may be enough common properties to the database schemas to = draft a data model for clusters.

Sincerely,
Rick
Rick Wagner, Graduate Student Researcher
UCSD Physics
9500 Gilman = Drive
La Jolla, CA=A0=A092093-0424
Email:=A0 rwagner@physics.ucsd.edu
WWW:=A0 =A0=A0http://lca.ucsd.edu
(858) 822-4784 = Phone
----------------------------------------------------------= -----

=

= --Apple-Mail-2-417750898-- From owner-dm@eso.org Fri Jan 26 23:36:58 2007 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 l0QMaivC003812 for ; Fri, 26 Jan 2007 23:36:44 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id l0QMaiPn003811 for dm-outgoing; Fri, 26 Jan 2007 23:36:44 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dm@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.13.6+Sun/8.12.10) with ESMTP id l0QMafhP003791; Fri, 26 Jan 2007 23:36:42 +0100 (MET) Received: from pro.abac.com (pro.abac.com [66.226.64.2]) by apollo.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id l0QMadej000327; Fri, 26 Jan 2007 23:36:40 +0100 (CET) Received: from [132.239.66.176] (cassx176.ucsd.edu [132.239.66.176]) (authenticated bits=0) by pro.abac.com (8.13.8/8.13.8) with ESMTP id l0QMaTLJ011826; Fri, 26 Jan 2007 14:36:30 -0800 (PST) (envelope-from rwagner@physics.ucsd.edu) In-Reply-To: <000501c7412a$6d5de390$cc48b782@gavopc1> References: <000501c7412a$6d5de390$cc48b782@gavopc1> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: multipart/alternative; boundary=Apple-Mail-2-417750898 Message-Id: Cc: theory@ivoa.net, dm@ivoa.net, Mike Norman , evrard@umich.edu X-Mailer: Apple Mail (2.752.2) From: Rick Wagner Subject: Re: simulation data models Date: Fri, 26 Jan 2007 14:36:35 -0800 To: "Gerard" X-Spam-Score: 0.101 (HTML_MESSAGE) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.2.285561, Antispam-Engine: 2.5.0.283055, Antispam-Data: 2007.1.26.142433 X-Perl-Spam: Gauge=IIIIIII, Probability=7%, Report='HTML_50_70 0.1, __C230066_P5 0, __CP_URI_IN_BODY 0, __CT 0, __CTYPE_HAS_BOUNDARY 0, __CTYPE_MULTIPART 0, __CTYPE_MULTIPART_ALT 0, __FRAUD_419_INTRO 0, __HAS_MSGID 0, __HAS_X_MAILER 0, __MIME_HTML 0, __MIME_VERSION 0, __SANE_MSGID 0, __TAG_EXISTS_HTML 0' Sender: owner-dm@eso.org Precedence: bulk Reply-To: Rick Wagner --Apple-Mail-2-417750898 Content-Transfer-Encoding: 7bit Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Hello Gerard, Your message comes at a good time for me to introduce myself. I'm a graduate student working with Mike Norman at UCSD, and I attended the NVO Summer School this year to learn more about the IVOA, in the hopes of publishing the results of our simulations to the NVO. While at the Summer School, I implemented a SkyNode based on a use case you wrote up a while ago, the Theory SkyNode. I've been following the work of the Theory Interest Group from the sidelines, and am planning to go with whatever standards arise. Which is why the database tables exposed via the SkyNode are minimal, and only provide summary information on X-ray clusters identified in an existing archive. I am assuming I'll have to change things later, so I'm taking things slow. With that said, I've put some thought into how to organize our simulation data with the goal of it being published to the NVO. I'd be happy to organize my notes into a draft document, if you think it would be of use. Further, as a result of the Summer School, I was able to presented my work at AAS in Seattle. You can view a copy of my poster here: http://lca.ucsd.edu/Members/rpwagner/PosterRickWagner.pdf I spoke with Gus Evrard at AAS, and he expressed an interest to work on a common data model for galaxy clusters to enable code comparison. All three or our groups have built databases containing tabulated properties of simulated objects, and there may be enough common properties to the database schemas to draft a data model for clusters. Sincerely, Rick --------------------------------------------------------------- Rick Wagner, Graduate Student Researcher UCSD Physics 9500 Gilman Drive La Jolla, CA 92093-0424 Email: rwagner@physics.ucsd.edu WWW: http://lca.ucsd.edu (858) 822-4784 Phone --------------------------------------------------------------- --Apple-Mail-2-417750898 Content-Transfer-Encoding: quoted-printable Content-Type: text/html; charset=ISO-8859-1
Hello Gerard,

Your message comes at a = good time for me to introduce myself. I'm a graduate student working = with Mike Norman at UCSD, and I attended the NVO Summer School this year = to learn more about the IVOA, in the hopes of publishing the results of = our simulations to the NVO.

While at the Summer School, = I implemented a SkyNode based=A0=A0on a use case you wrote up a while = ago, the Theory SkyNode. I've been following the work of the Theory = Interest Group from the sidelines, and am planning to go with whatever = standards arise. Which is why the database tables exposed via the = SkyNode are minimal, and only provide summary information on X-ray = clusters identified in an existing archive. I am assuming I'll have to = change things later, so I'm taking things slow.=A0

With that said, I've put = some thought into how to organize our simulation data with the goal of = it being published to the NVO. I'd be happy to organize my notes into a = draft document, if you think it would be of use.=A0

Further, as a result of the = Summer School, I was able to presented my work at AAS in Seattle.=A0You = can view a copy of my poster here:

I spoke with Gus Evrard at = AAS, and he expressed an interest to work on a common data model for = galaxy clusters to enable code comparison. All three or our groups have = built databases containing tabulated properties of simulated objects, = and there may be enough common properties to the database schemas to = draft a data model for clusters.

Sincerely,
Rick
Rick Wagner, Graduate Student Researcher
UCSD Physics
9500 Gilman = Drive
La Jolla, CA=A0=A092093-0424
Email:=A0 rwagner@physics.ucsd.edu
WWW:=A0 =A0=A0http://lca.ucsd.edu
(858) 822-4784 = Phone
----------------------------------------------------------= -----

=

= --Apple-Mail-2-417750898-- From owner-theory@eso.org Wed Feb 14 10:49:33 2007 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 l1E9nS4u017614 for ; Wed, 14 Feb 2007 10:49:28 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id l1E9nSvf017613 for theory-outgoing; Wed, 14 Feb 2007 10:49:28 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 l1E9nRpl017602; Wed, 14 Feb 2007 10:49:27 +0100 (MET) Received: from smtp.iaa.es (smtp.iaa.csic.es [193.146.145.11]) by apollo.hq.eso.org (8.13.8+Sun/8.12.10) with ESMTP id l1E9nQRJ024635; Wed, 14 Feb 2007 10:49:26 +0100 (CET) Received: from [161.111.165.12] (dae2.iaa.csic.es [161.111.165.12]) (authenticated bits=0) by smtp.iaa.es (8.13.1/8.13.1) with ESMTP id l1E9n91H019163; Wed, 14 Feb 2007 10:49:09 +0100 In-Reply-To: References: <200702130439.l1D4dkw0011375@urania.cfa.harvard.edu> <45D1BD61.8020701@stsci.edu> <45D1EE87.2000106@cea.fr> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <8CC04BD2-A0D5-4E42-BFE2-6732BC193E90@iaa.es> Cc: "P.Didelon" , Ivo Busko , dm@ivoa.net, Carlos Rodrigo Blanco , theory@ivoa.net Content-Transfer-Encoding: 7bit From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Re: SED serialization Date: Wed, 14 Feb 2007 10:49:08 +0100 To: Doug Tody X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.2.285561, Antispam-Engine: 2.5.0.283055, Antispam-Data: 2007.2.14.13934 X-Perl-Spam: Gauge=IIIIIII, Probability=7%, Report='__CP_MEDIA_2_BODY 0, __CP_URI_IN_BODY 0, __CT 0, __CTE 0, __CT_TEXT_PLAIN 0, __HAS_MSGID 0, __HAS_X_MAILER 0, __MIME_TEXT_ONLY 0, __MIME_VERSION 0, __SANE_MSGID 0' Sender: owner-theory@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Dear all. (I have include in the reply the theory list, since some one would be also interested in the discussion, so I also include a brief summary of it) I am working in synthesis models, which one of the main result are the spectra of a stellar population or, if you want, a set of spectrum generated each one for a different age/evolutionary conditions. I was began to implement a service with the set of models following the "spectral data model" (c.f. http://hea-www.harvard.edu/~jcm/vo/docs/spec102/specrc2.pdf) for each of the models, which I think it is almost fine for this pourpose Now, I would use the "SED data model", (http://hea-www.harvard.edu/~jcm/vo/docs/spec96/sed96.pdf) that, If I understood correctly, would allow to provide the complete dataset of models. In the dm list there is now the issue of if SED can be considered as a "specialised" case of spectrum or the opposite (with implications for applications etc...) From my point of view, I think that in fact we are dealling with two quite different issues: a) I think that an spectrum dm should be the primary description of any spectrum (as all agree) It has the advantages from service providers and users that you obtain a single usable table that can be handle yet by most applications. (In this case, SED dm is not an especial case of spectrum). b) About SED data model, I have an alternative perspective: I think that it is quite better to make a "general data model" that would include not only "segments" with collection of spectra/time series, but also other possible results that the VO would produce (e.g. arrays that describe the chemical evolution of a galaxy where each segment has information about different elements, or a set of a MonteCarlo simulations, and atmosphere library, a set of isochrones or evolutionary tracks etc...) In this context, I think that the current SED data model can be transformed in a more general data model that would describe collections of data, that also would means that produce an VOTable where elements are references to others VOTables with the specific primary data. As possible advantages: - It can include a more wide variety of situations (not the special one of spectra) without increasing the amount of data models. In my case, I would provide different model results, not only spectra, without need to include the utypes for the particular spectrum, the utypes for sets of spectra and different utypes for individual models and collections for the case of non-spectra/time-series results. - It would naturally include the issue about how to include references to, as an example, the description of photometric filters etc... - The VOTables that the applications will deal with (and also users) will be smaller in size and, hence, virtual memory (e.j. my set of high- resolution spectra results, that I would include in a single VOTable in the SED dm will have a size about 4Gb). - It allows to "explore" large databases with different types of data (e.g. actually, if you query VizieR looking for isochrones in Aladin, you obtain a sigle VOTable with all isocrones, instead the single isochrone you are interested in, you can obtain this single file from the VizieR server, but not with VO applications. - It is not necessary that apps that understand spectra makes additional implementations (the problem SED dm model issue becomes an issue related with how to query the resgistry) The disadvantage I see in this approach are: - Modules of the applications that query a service must to understand if they obtain a VOTable with references to other VOTables of a VOTable with data (or a mixing of both). Any case, I think that such issue is in someway yet included in SSAP protocol (if it include the TSAP protocol, i.e. an answer of a query ssap?FORMAT=METADATA) - Users will need to make more choices before obtain a particular result, although will depend on the model provider and in if the application would make a multiple query from the VOTable with the collection. Summing up, I think that the it would be better to have a good direct access to individual data (spectrum dm in this case) and that any access to sets of "individual data" can be more easily handle by dm that describe VOTables of VOTables (that can be a recurent process) following a general datamodel instead to provide datamodels for specific cases. It is just a suggestion :) cheers miguel From owner-dm@eso.org Wed Feb 14 10:49:38 2007 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 l1E9nSTZ017607 for ; Wed, 14 Feb 2007 10:49:28 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id l1E9nSoh017606 for dm-outgoing; Wed, 14 Feb 2007 10:49:28 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dm@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.13.6+Sun/8.12.10) with ESMTP id l1E9nRpl017602; Wed, 14 Feb 2007 10:49:27 +0100 (MET) Received: from smtp.iaa.es (smtp.iaa.csic.es [193.146.145.11]) by apollo.hq.eso.org (8.13.8+Sun/8.12.10) with ESMTP id l1E9nQRJ024635; Wed, 14 Feb 2007 10:49:26 +0100 (CET) Received: from [161.111.165.12] (dae2.iaa.csic.es [161.111.165.12]) (authenticated bits=0) by smtp.iaa.es (8.13.1/8.13.1) with ESMTP id l1E9n91H019163; Wed, 14 Feb 2007 10:49:09 +0100 In-Reply-To: References: <200702130439.l1D4dkw0011375@urania.cfa.harvard.edu> <45D1BD61.8020701@stsci.edu> <45D1EE87.2000106@cea.fr> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <8CC04BD2-A0D5-4E42-BFE2-6732BC193E90@iaa.es> Cc: "P.Didelon" , Ivo Busko , dm@ivoa.net, Carlos Rodrigo Blanco , theory@ivoa.net Content-Transfer-Encoding: 7bit From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: Re: SED serialization Date: Wed, 14 Feb 2007 10:49:08 +0100 To: Doug Tody X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.2.285561, Antispam-Engine: 2.5.0.283055, Antispam-Data: 2007.2.14.13934 X-Perl-Spam: Gauge=IIIIIII, Probability=7%, Report='__CP_MEDIA_2_BODY 0, __CP_URI_IN_BODY 0, __CT 0, __CTE 0, __CT_TEXT_PLAIN 0, __HAS_MSGID 0, __HAS_X_MAILER 0, __MIME_TEXT_ONLY 0, __MIME_VERSION 0, __SANE_MSGID 0' Sender: owner-dm@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Dear all. (I have include in the reply the theory list, since some one would be also interested in the discussion, so I also include a brief summary of it) I am working in synthesis models, which one of the main result are the spectra of a stellar population or, if you want, a set of spectrum generated each one for a different age/evolutionary conditions. I was began to implement a service with the set of models following the "spectral data model" (c.f. http://hea-www.harvard.edu/~jcm/vo/docs/spec102/specrc2.pdf) for each of the models, which I think it is almost fine for this pourpose Now, I would use the "SED data model", (http://hea-www.harvard.edu/~jcm/vo/docs/spec96/sed96.pdf) that, If I understood correctly, would allow to provide the complete dataset of models. In the dm list there is now the issue of if SED can be considered as a "specialised" case of spectrum or the opposite (with implications for applications etc...) From my point of view, I think that in fact we are dealling with two quite different issues: a) I think that an spectrum dm should be the primary description of any spectrum (as all agree) It has the advantages from service providers and users that you obtain a single usable table that can be handle yet by most applications. (In this case, SED dm is not an especial case of spectrum). b) About SED data model, I have an alternative perspective: I think that it is quite better to make a "general data model" that would include not only "segments" with collection of spectra/time series, but also other possible results that the VO would produce (e.g. arrays that describe the chemical evolution of a galaxy where each segment has information about different elements, or a set of a MonteCarlo simulations, and atmosphere library, a set of isochrones or evolutionary tracks etc...) In this context, I think that the current SED data model can be transformed in a more general data model that would describe collections of data, that also would means that produce an VOTable where elements are references to others VOTables with the specific primary data. As possible advantages: - It can include a more wide variety of situations (not the special one of spectra) without increasing the amount of data models. In my case, I would provide different model results, not only spectra, without need to include the utypes for the particular spectrum, the utypes for sets of spectra and different utypes for individual models and collections for the case of non-spectra/time-series results. - It would naturally include the issue about how to include references to, as an example, the description of photometric filters etc... - The VOTables that the applications will deal with (and also users) will be smaller in size and, hence, virtual memory (e.j. my set of high- resolution spectra results, that I would include in a single VOTable in the SED dm will have a size about 4Gb). - It allows to "explore" large databases with different types of data (e.g. actually, if you query VizieR looking for isochrones in Aladin, you obtain a sigle VOTable with all isocrones, instead the single isochrone you are interested in, you can obtain this single file from the VizieR server, but not with VO applications. - It is not necessary that apps that understand spectra makes additional implementations (the problem SED dm model issue becomes an issue related with how to query the resgistry) The disadvantage I see in this approach are: - Modules of the applications that query a service must to understand if they obtain a VOTable with references to other VOTables of a VOTable with data (or a mixing of both). Any case, I think that such issue is in someway yet included in SSAP protocol (if it include the TSAP protocol, i.e. an answer of a query ssap?FORMAT=METADATA) - Users will need to make more choices before obtain a particular result, although will depend on the model provider and in if the application would make a multiple query from the VOTable with the collection. Summing up, I think that the it would be better to have a good direct access to individual data (spectrum dm in this case) and that any access to sets of "individual data" can be more easily handle by dm that describe VOTables of VOTables (that can be a recurent process) following a general datamodel instead to provide datamodels for specific cases. It is just a suggestion :) cheers miguel From owner-theory@eso.org Wed Feb 14 18:34:08 2007 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 l1EHXHFc020664 for ; Wed, 14 Feb 2007 18:33:17 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id l1EHXHiY020663 for theory-outgoing; Wed, 14 Feb 2007 18:33:17 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 l1EHXFo7020657; Wed, 14 Feb 2007 18:33:15 +0100 (MET) Received: from revere.aoc.nrao.edu (revere.aoc.nrao.edu [146.88.1.15]) by apollo.hq.eso.org (8.13.8+Sun/8.12.10) with ESMTP id l1EHXDgB025230; Wed, 14 Feb 2007 18:33:14 +0100 (CET) Received: from dropbox.aoc.nrao.edu (dropbox.aoc.nrao.edu [146.88.1.13]) by revere.aoc.nrao.edu (8.13.1/8.13.1/cv-ws-8.12) with ESMTP id l1EHWXLG003939; Wed, 14 Feb 2007 10:32:33 -0700 Received: from oak.aoc.nrao.edu (oak.aoc.nrao.edu [146.88.3.232]) by dropbox.aoc.nrao.edu (8.13.1/8.13.1/smtp-gateway) with ESMTP id l1EHWUoe019885; Wed, 14 Feb 2007 10:32:31 -0700 Date: Wed, 14 Feb 2007 10:32:30 -0700 (MST) From: Doug Tody X-X-Sender: dtody@oak To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= cc: "P.Didelon" , Ivo Busko , dm@ivoa.net, Carlos Rodrigo Blanco , theory@ivoa.net Subject: Re: SED serialization In-Reply-To: <8CC04BD2-A0D5-4E42-BFE2-6732BC193E90@iaa.es> Message-ID: References: <200702130439.l1D4dkw0011375@urania.cfa.harvard.edu> <45D1BD61.8020701@stsci.edu> <45D1EE87.2000106@cea.fr> <8CC04BD2-A0D5-4E42-BFE2-6732BC193E90@iaa.es> MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed X-MailScanner-Information: Please contact the postmaster@aoc.nrao.edu for more information X-MailScanner: Found to be clean X-MailScanner-SpamCheck: not spam, SpamAssassin (not cached, score=-101.44, required 5, autolearn=disabled, ALL_TRUSTED -1.44, USER_IN_WHITELIST -100.00) X-MailScanner-From: dtody@nrao.edu X-Spam-Status: No X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.2.285561, Antispam-Engine: 2.5.0.283055, Antispam-Data: 2007.2.14.91933 X-Perl-Spam: Gauge=IIIIIII, Probability=7%, Report='__CP_MEDIA_BODY 0, __CT 0, __CT_TEXT_PLAIN 0, __HAS_MSGID 0, __MIME_TEXT_ONLY 0, __MIME_VERSION 0, __SANE_MSGID 0, __X_MAIL_SCANNER 0' Sender: owner-theory@eso.org Precedence: bulk Reply-To: Doug Tody Miguel - This is very useful as I think it helps illustrate how complex SEDs can be, especially if we consider heterogeneous or theory data, or dynamically computed SEDs. While a multi-segment spectrum (or time series) can be considered a special case of a SED, in general SEDs can be much more complex than this. If I understand your argument correctly, you are saying that: o Spectrum as it stands is the right approach for the case of "simple" 1-D spectra (although some more features such as for modeling photometry may be required). o For SEDs what is mainly needed is a high level description of the overall SED object. The individual observations or datasets ("segments") which contributed to the SED can be anything, and are best dealt with by pointing to primary datasets that describe these (e.g., a separate 1D-spectrum, image cutout, etc. Existing interfaces such as SSAP, SIAP, TSAP, etc. could then presumably be used to get at this data. Perhaps smaller Spectrum or whatever objects can be directly included, but this could get complicated - we should think more carefully about what this really means. The following is an especially good point: > The VOTables that the applications will deal with (and also users) > will be smaller in size and, hence, virtual memory (e.j. my set of > high-resolution spectra results, that I would include in a single > VOTable in the SED dm will have a size about 4Gb). This could also be the case for time series or theory data of course. In a case like this, there really is no way we can practically include the individual datasets directly as segments, and some means of pointing to the external data is required. Then if the analysis needs to go look at the primary data it can use an existing interface appropriate to that data to access it. - Doug From owner-dm@eso.org Wed Feb 14 18:34:30 2007 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 l1EHXHTD020669 for ; Wed, 14 Feb 2007 18:33:17 +0100 (MET) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id l1EHXHuY020668 for dm-outgoing; Wed, 14 Feb 2007 18:33:17 +0100 (MET) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dm@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.13.6+Sun/8.12.10) with ESMTP id l1EHXFo7020657; Wed, 14 Feb 2007 18:33:15 +0100 (MET) Received: from revere.aoc.nrao.edu (revere.aoc.nrao.edu [146.88.1.15]) by apollo.hq.eso.org (8.13.8+Sun/8.12.10) with ESMTP id l1EHXDgB025230; Wed, 14 Feb 2007 18:33:14 +0100 (CET) Received: from dropbox.aoc.nrao.edu (dropbox.aoc.nrao.edu [146.88.1.13]) by revere.aoc.nrao.edu (8.13.1/8.13.1/cv-ws-8.12) with ESMTP id l1EHWXLG003939; Wed, 14 Feb 2007 10:32:33 -0700 Received: from oak.aoc.nrao.edu (oak.aoc.nrao.edu [146.88.3.232]) by dropbox.aoc.nrao.edu (8.13.1/8.13.1/smtp-gateway) with ESMTP id l1EHWUoe019885; Wed, 14 Feb 2007 10:32:31 -0700 Date: Wed, 14 Feb 2007 10:32:30 -0700 (MST) From: Doug Tody X-X-Sender: dtody@oak To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= cc: "P.Didelon" , Ivo Busko , dm@ivoa.net, Carlos Rodrigo Blanco , theory@ivoa.net Subject: Re: SED serialization In-Reply-To: <8CC04BD2-A0D5-4E42-BFE2-6732BC193E90@iaa.es> Message-ID: References: <200702130439.l1D4dkw0011375@urania.cfa.harvard.edu> <45D1BD61.8020701@stsci.edu> <45D1EE87.2000106@cea.fr> <8CC04BD2-A0D5-4E42-BFE2-6732BC193E90@iaa.es> MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII; format=flowed X-MailScanner-Information: Please contact the postmaster@aoc.nrao.edu for more information X-MailScanner: Found to be clean X-MailScanner-SpamCheck: not spam, SpamAssassin (not cached, score=-101.44, required 5, autolearn=disabled, ALL_TRUSTED -1.44, USER_IN_WHITELIST -100.00) X-MailScanner-From: dtody@nrao.edu X-Spam-Status: No X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.2.2.285561, Antispam-Engine: 2.5.0.283055, Antispam-Data: 2007.2.14.91933 X-Perl-Spam: Gauge=IIIIIII, Probability=7%, Report='__CP_MEDIA_BODY 0, __CT 0, __CT_TEXT_PLAIN 0, __HAS_MSGID 0, __MIME_TEXT_ONLY 0, __MIME_VERSION 0, __SANE_MSGID 0, __X_MAIL_SCANNER 0' Sender: owner-dm@eso.org Precedence: bulk Reply-To: Doug Tody Miguel - This is very useful as I think it helps illustrate how complex SEDs can be, especially if we consider heterogeneous or theory data, or dynamically computed SEDs. While a multi-segment spectrum (or time series) can be considered a special case of a SED, in general SEDs can be much more complex than this. If I understand your argument correctly, you are saying that: o Spectrum as it stands is the right approach for the case of "simple" 1-D spectra (although some more features such as for modeling photometry may be required). o For SEDs what is mainly needed is a high level description of the overall SED object. The individual observations or datasets ("segments") which contributed to the SED can be anything, and are best dealt with by pointing to primary datasets that describe these (e.g., a separate 1D-spectrum, image cutout, etc. Existing interfaces such as SSAP, SIAP, TSAP, etc. could then presumably be used to get at this data. Perhaps smaller Spectrum or whatever objects can be directly included, but this could get complicated - we should think more carefully about what this really means. The following is an especially good point: > The VOTables that the applications will deal with (and also users) > will be smaller in size and, hence, virtual memory (e.j. my set of > high-resolution spectra results, that I would include in a single > VOTable in the SED dm will have a size about 4Gb). This could also be the case for time series or theory data of course. In a case like this, there really is no way we can practically include the individual datasets directly as segments, and some means of pointing to the external data is required. Then if the analysis needs to go look at the primary data it can use an existing interface appropriate to that data to access it. - Doug From owner-theory@eso.org Sun Apr 22 16:33:08 2007 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 l3MEWenu029805 for ; Sun, 22 Apr 2007 16:32:40 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id l3MEWdfV029804 for theory-outgoing; Sun, 22 Apr 2007 16:32:39 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 l3MEWdQ2029799 for ; Sun, 22 Apr 2007 16:32:39 +0200 (MEST) Received: from mpemail.mpe.mpg.de (mpemail.mpe.mpg.de [130.183.137.110]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id l3MEWcU4017241 for ; Sun, 22 Apr 2007 16:32:38 +0200 (CEST) Received: from gavopc1.xray.mpe.mpg.de ([130.183.72.204] helo=gavopc1) by mpemail.mpe.mpg.de with esmtp (Exim 4.50) id 1Hfd6n-00010N-EA for theory@ivoa.net; Sun, 22 Apr 2007 16:32:12 +0200 From: "Gerard" To: Subject: Beijing meeting Date: Sun, 22 Apr 2007 16:34:33 +0200 Message-ID: <000001c784eb$585e8940$cc48b782@gavopc1> MIME-Version: 1.0 Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 7bit X-Mailer: Microsoft Office Outlook 11 Thread-Index: AceE61hCVSislZgTTIq48FlBQGtAuA== X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.3028 X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.3.1.294258, Antispam-Engine: 2.5.1.298604, Antispam-Data: 2007.4.22.71834 X-Perl-Spam: Gauge=IIIIIII, Probability=7%, Report='__CT 0, __CTE 0, __CT_TEXT_PLAIN 0, __HAS_MSGID 0, __HAS_X_MAILER 0, __MIME_TEXT_ONLY 0, __MIME_VERSION 0, __SANE_MSGID 0, __USER_AGENT_MS_GENERIC 0' Sender: owner-theory@eso.org Precedence: bulk Reply-To: "Gerard" Dear colleagues There will be official three meetings of the theory interest group. Two of these will deal with simulation data model and SNAP protocol respectively and are fully scheduled. There is a third meeting on possible new projects for the interest group. For this I invite proposals for discussion items and/or presentations. Best regards Gerard Lemson From owner-theory@eso.org Fri May 11 14:17:12 2007 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 l4BCGtUC006548 for ; Fri, 11 May 2007 14:16:55 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id l4BCGtsJ006547 for theory-outgoing; Fri, 11 May 2007 14:16:55 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 l4BCGs1t006543 for ; Fri, 11 May 2007 14:16:55 +0200 (MEST) Received: from mpemail.mpe.mpg.de (mpemail.mpe.mpg.de [130.183.137.110]) by apollo.hq.eso.org (8.13.8+Sun/8.12.10) with ESMTP id l4BCGsYf009069 for ; Fri, 11 May 2007 14:16:54 +0200 (CEST) Received: from exim by mpemail.mpe.mpg.de with local (Exim 4.60) (envelope-from ) id 1HmU3F-0001YT-5S for theory@ivoa.net; Fri, 11 May 2007 14:16:49 +0200 From: "glemson" To: theory@ivoa.net Subject: theory sessions Beijing Date: Fri, 11 May 2007 14:16:49 +0200 Mime-Version: 1.0 Content-Type: text/plain; charset="utf-8"; format=flowed Content-Transfer-Encoding: 7bit Message-Id: X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.3.1.294258, Antispam-Engine: 2.5.1.298604, Antispam-Data: 2007.5.11.50034 X-Perl-Spam: Gauge=IIIIIII, Probability=7%, Report='__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' Sender: owner-theory@eso.org Precedence: bulk Reply-To: "glemson" Dear colleagues The agenda for the theory sessions during the Beijing interop next week is available on the wiki page http://www.ivoa.net/twiki/bin/view/IVOA/InterOpMay2007Theory See you soon Best regards Gerard Lemson From owner-theory@eso.org Tue Jun 26 15:28:19 2007 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 l5QDS9V6026746 for ; Tue, 26 Jun 2007 15:28:09 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id l5QDS9TN026745 for theory-outgoing; Tue, 26 Jun 2007 15:28:09 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 l5QDS7b0026734; Tue, 26 Jun 2007 15:28:07 +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 l5QDS0nO018389; Tue, 26 Jun 2007 15:28:02 +0200 (CEST) Received: from dropbox.aoc.nrao.edu (dropbox.aoc.nrao.edu [146.88.1.13]) by revere.aoc.nrao.edu (8.13.1/8.13.1/cv-ws-8.12) with ESMTP id l5QDQlAf018254; Tue, 26 Jun 2007 07:26:47 -0600 Received: from localhost (localhost [[UNIX: localhost]]) by dropbox.aoc.nrao.edu (8.13.1/8.13.1/Submit) id l5QDQkJq004188; Tue, 26 Jun 2007 07:26:46 -0600 Date: Tue, 26 Jun 2007 07:26:52 -0600 From: Doug Tody X-X-Sender: dtody@cetus To: Gerard cc: dal@ivoa.net, theory@ivoa.net Subject: RE: RFC initiated for Simple Spectral Access protocol In-Reply-To: <001401c7b7f3$eabf9af0$cc48b782@gavopc1> Message-ID: References: <20070626115750.q3gwpurl6o0ck4wc@webmail.esac.esa.int> <001401c7b7f3$eabf9af0$cc48b782@gavopc1> MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-MailScanner-Information: Please contact the postmaster@aoc.nrao.edu for more information X-MailScanner: Found to be clean X-MailScanner-SpamCheck: not spam, SpamAssassin (not cached, score=-101.44, required 5, autolearn=disabled, ALL_TRUSTED -1.44, USER_IN_WHITELIST -100.00) X-MailScanner-From: dtody@aoc.nrao.edu X-Spam-Status: No X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.3.2.304607, Antispam-Engine: 2.5.1.298604, Antispam-Data: 2007.6.25.191907 X-Perl-Spam: Gauge=IIIIIII, Probability=7%, Report='__CT 0, __CT_TEXT_PLAIN 0, __HAS_MSGID 0, __MIME_TEXT_ONLY 0, __MIME_VERSION 0, __SANE_MSGID 0, __X_MAIL_SCANNER 0' Sender: owner-theory@eso.org Precedence: bulk Reply-To: Doug Tody On Tue, 26 Jun 2007, Gerard wrote: > > > We talked to Markus yesterday (he is at ESAC because one EuroVO > > > workshop) and he mentioned a special section about FORMAT=METADATA > > > (including a better example) is being prepared but it has not been > > > included in the document because time constrains. In fact, we had the > > > action to send a description/example about the use for theoretical > > > services. As the description is decoupled from the rest of the > > > document, I do not see major problems if the section is finally > > > included. > > > > It could still be useful to have a section/example noting how to handle > > theory data (although this really should have been in the doc already > > it should be fairly independent). > > > This might be useful, even though, after repeated questioning, everyone at > the last few IVOA meetings claimed that SSA covers the needs of those > wishing to publish theory spectra. If this is not the case, adding such a > section/example might make this true anyway. We think it does cover this case already, but a use-case example at the end, for the implementor of such a service, could be useful. An example of metadata extension could also be useful. These are not high priority though, and could also appear in V1.1 this fall. - Doug From owner-dal@eso.org Tue Jun 26 15:29:46 2007 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 l5QDS9AX026741 for ; Tue, 26 Jun 2007 15:28:09 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id l5QDS9Db026740 for dal-outgoing; Tue, 26 Jun 2007 15:28:09 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dal@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.13.6+Sun/8.12.10) with ESMTP id l5QDS7b0026734; Tue, 26 Jun 2007 15:28:07 +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 l5QDS0nO018389; Tue, 26 Jun 2007 15:28:02 +0200 (CEST) Received: from dropbox.aoc.nrao.edu (dropbox.aoc.nrao.edu [146.88.1.13]) by revere.aoc.nrao.edu (8.13.1/8.13.1/cv-ws-8.12) with ESMTP id l5QDQlAf018254; Tue, 26 Jun 2007 07:26:47 -0600 Received: from localhost (localhost [[UNIX: localhost]]) by dropbox.aoc.nrao.edu (8.13.1/8.13.1/Submit) id l5QDQkJq004188; Tue, 26 Jun 2007 07:26:46 -0600 Date: Tue, 26 Jun 2007 07:26:52 -0600 From: Doug Tody X-X-Sender: dtody@cetus To: Gerard cc: dal@ivoa.net, theory@ivoa.net Subject: RE: RFC initiated for Simple Spectral Access protocol In-Reply-To: <001401c7b7f3$eabf9af0$cc48b782@gavopc1> Message-ID: References: <20070626115750.q3gwpurl6o0ck4wc@webmail.esac.esa.int> <001401c7b7f3$eabf9af0$cc48b782@gavopc1> MIME-Version: 1.0 Content-Type: TEXT/PLAIN; charset=US-ASCII X-MailScanner-Information: Please contact the postmaster@aoc.nrao.edu for more information X-MailScanner: Found to be clean X-MailScanner-SpamCheck: not spam, SpamAssassin (not cached, score=-101.44, required 5, autolearn=disabled, ALL_TRUSTED -1.44, USER_IN_WHITELIST -100.00) X-MailScanner-From: dtody@aoc.nrao.edu X-Spam-Status: No X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.3.2.304607, Antispam-Engine: 2.5.1.298604, Antispam-Data: 2007.6.25.191907 X-Perl-Spam: Gauge=IIIIIII, Probability=7%, Report='__CT 0, __CT_TEXT_PLAIN 0, __HAS_MSGID 0, __MIME_TEXT_ONLY 0, __MIME_VERSION 0, __SANE_MSGID 0, __X_MAIL_SCANNER 0' Sender: owner-dal@eso.org Precedence: bulk Reply-To: Doug Tody On Tue, 26 Jun 2007, Gerard wrote: > > > We talked to Markus yesterday (he is at ESAC because one EuroVO > > > workshop) and he mentioned a special section about FORMAT=METADATA > > > (including a better example) is being prepared but it has not been > > > included in the document because time constrains. In fact, we had the > > > action to send a description/example about the use for theoretical > > > services. As the description is decoupled from the rest of the > > > document, I do not see major problems if the section is finally > > > included. > > > > It could still be useful to have a section/example noting how to handle > > theory data (although this really should have been in the doc already > > it should be fairly independent). > > > This might be useful, even though, after repeated questioning, everyone at > the last few IVOA meetings claimed that SSA covers the needs of those > wishing to publish theory spectra. If this is not the case, adding such a > section/example might make this true anyway. We think it does cover this case already, but a use-case example at the end, for the implementor of such a service, could be useful. An example of metadata extension could also be useful. These are not high priority though, and could also appear in V1.1 this fall. - Doug From owner-theory@eso.org Tue Jun 26 15:44:23 2007 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 l5QDiHfr001595 for ; Tue, 26 Jun 2007 15:44:17 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id l5QDiHh8001594 for theory-outgoing; Tue, 26 Jun 2007 15:44:17 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 l5QDiHwG001589; Tue, 26 Jun 2007 15:44:17 +0200 (MEST) Received: from mpemail.mpe.mpg.de (mpemail.mpe.mpg.de [130.183.137.110]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id l5QDiBq8022437; Tue, 26 Jun 2007 15:44:15 +0200 (CEST) Received: from gavopc1.xray.mpe.mpg.de ([130.183.72.204] helo=gavopc1) by mpemail.mpe.mpg.de with esmtp (Exim 4.60) (envelope-from ) id 1I3Aon-00025h-71; Tue, 26 Jun 2007 15:10:53 +0200 From: "Gerard" To: "'Doug Tody'" Cc: , References: <20070626115750.q3gwpurl6o0ck4wc@webmail.esac.esa.int> Subject: RE: RFC initiated for Simple Spectral Access protocol Date: Tue, 26 Jun 2007 15:14:24 +0200 Message-ID: <001401c7b7f3$eabf9af0$cc48b782@gavopc1> MIME-Version: 1.0 Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 7bit X-Mailer: Microsoft Office Outlook 11 In-Reply-To: X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.3138 Thread-Index: Ace38ivo1gD2rXPDRAqtgoZ7+EVq5wAAKqiw X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.3.2.304607, Antispam-Engine: 2.5.1.298604, Antispam-Data: 2007.6.25.191907 X-Perl-Spam: Gauge=IIIIIII, Probability=7%, Report='__CT 0, __CTE 0, __CT_TEXT_PLAIN 0, __HAS_MSGID 0, __HAS_X_MAILER 0, __MIME_TEXT_ONLY 0, __MIME_VERSION 0, __SANE_MSGID 0, __USER_AGENT_MS_GENERIC 0' Sender: owner-theory@eso.org Precedence: bulk Reply-To: "Gerard" > > We talked to Markus yesterday (he is at ESAC because one EuroVO > > workshop) and he mentioned a special section about FORMAT=METADATA > > (including a better example) is being prepared but it has not been > > included in the document because time constrains. In fact, we had the > > action to send a description/example about the use for theoretical > > services. As the description is decoupled from the rest of the > > document, I do not see major problems if the section is finally > > included. > > It could still be useful to have a section/example noting how to handle > theory data (although this really should have been in the doc already > it should be fairly independent). > This might be useful, even though, after repeated questioning, everyone at the last few IVOA meetings claimed that SSA covers the needs of those wishing to publish theory spectra. If this is not the case, adding such a section/example might make this true anyway. For those of you listening only to the theory mailing list. It would be nice to hear from groups attempting to publish theory spectra through SSA. We know of the TSAP efforts, Herve has recently raised some issues, there may/must be more. For those who (think they) succeeded, maybe they could post some examples to this discussion trail to assist the DAL group. Best regards Gerard Lemson From owner-dal@eso.org Tue Jun 26 15:45:37 2007 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 l5QDiIl8001600 for ; Tue, 26 Jun 2007 15:44:18 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id l5QDiICf001599 for dal-outgoing; Tue, 26 Jun 2007 15:44:18 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dal@eso.org using -f Received: from rocky.hq.eso.org (rocky.hq.eso.org [134.171.42.43]) by mercury.hq.eso.org (8.13.6+Sun/8.12.10) with ESMTP id l5QDiHwG001589; Tue, 26 Jun 2007 15:44:17 +0200 (MEST) Received: from mpemail.mpe.mpg.de (mpemail.mpe.mpg.de [130.183.137.110]) by rocky.hq.eso.org (8.12.10+Sun/8.12.10) with ESMTP id l5QDiBq8022437; Tue, 26 Jun 2007 15:44:15 +0200 (CEST) Received: from gavopc1.xray.mpe.mpg.de ([130.183.72.204] helo=gavopc1) by mpemail.mpe.mpg.de with esmtp (Exim 4.60) (envelope-from ) id 1I3Aon-00025h-71; Tue, 26 Jun 2007 15:10:53 +0200 From: "Gerard" To: "'Doug Tody'" Cc: , References: <20070626115750.q3gwpurl6o0ck4wc@webmail.esac.esa.int> Subject: RE: RFC initiated for Simple Spectral Access protocol Date: Tue, 26 Jun 2007 15:14:24 +0200 Message-ID: <001401c7b7f3$eabf9af0$cc48b782@gavopc1> MIME-Version: 1.0 Content-Type: text/plain; charset="us-ascii" Content-Transfer-Encoding: 7bit X-Mailer: Microsoft Office Outlook 11 In-Reply-To: X-MimeOLE: Produced By Microsoft MimeOLE V6.00.2900.3138 Thread-Index: Ace38ivo1gD2rXPDRAqtgoZ7+EVq5wAAKqiw X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.3.2.304607, Antispam-Engine: 2.5.1.298604, Antispam-Data: 2007.6.25.191907 X-Perl-Spam: Gauge=IIIIIII, Probability=7%, Report='__CT 0, __CTE 0, __CT_TEXT_PLAIN 0, __HAS_MSGID 0, __HAS_X_MAILER 0, __MIME_TEXT_ONLY 0, __MIME_VERSION 0, __SANE_MSGID 0, __USER_AGENT_MS_GENERIC 0' Sender: owner-dal@eso.org Precedence: bulk Reply-To: "Gerard" > > We talked to Markus yesterday (he is at ESAC because one EuroVO > > workshop) and he mentioned a special section about FORMAT=METADATA > > (including a better example) is being prepared but it has not been > > included in the document because time constrains. In fact, we had the > > action to send a description/example about the use for theoretical > > services. As the description is decoupled from the rest of the > > document, I do not see major problems if the section is finally > > included. > > It could still be useful to have a section/example noting how to handle > theory data (although this really should have been in the doc already > it should be fairly independent). > This might be useful, even though, after repeated questioning, everyone at the last few IVOA meetings claimed that SSA covers the needs of those wishing to publish theory spectra. If this is not the case, adding such a section/example might make this true anyway. For those of you listening only to the theory mailing list. It would be nice to hear from groups attempting to publish theory spectra through SSA. We know of the TSAP efforts, Herve has recently raised some issues, there may/must be more. For those who (think they) succeeded, maybe they could post some examples to this discussion trail to assist the DAL group. Best regards Gerard Lemson From owner-theory@eso.org Tue Jul 3 12:32:00 2007 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 l63AVqkO015115 for ; Tue, 3 Jul 2007 12:31:52 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id l63AVq5C015114 for theory-outgoing; Tue, 3 Jul 2007 12:31:52 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 l63AVpT3015105; Tue, 3 Jul 2007 12:31:51 +0200 (MEST) Received: from smtp.iaa.es (smtp.iaa.csic.es [193.146.145.11]) by apollo.hq.eso.org (8.13.8+Sun/8.12.10) with ESMTP id l63AVo6L015057; Tue, 3 Jul 2007 12:31:50 +0200 (CEST) Received: from [161.111.165.115] (dae-d15.iaa.csic.es [161.111.165.115]) (authenticated bits=0) by smtp.iaa.es (8.13.1/8.13.1) with ESMTP id l63AVi7k031657; Tue, 3 Jul 2007 12:31:44 +0200 In-Reply-To: References: <20070626115750.q3gwpurl6o0ck4wc@webmail.esac.esa.int> <001401c7b7f3$eabf9af0$cc48b782@gavopc1> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <497429B6-C51C-43BF-8A05-7EF479482B21@iaa.es> Cc: dal@ivoa.net, theory@ivoa.net Content-Transfer-Encoding: 7bit From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: On FORMAT=METADATA Date: Tue, 3 Jul 2007 12:31:43 +0200 To: Doug Tody , Gerard , Carlos Rodrigo X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.3.2.304607, Antispam-Engine: 2.5.1.298604, Antispam-Data: 2007.7.3.31232 X-Perl-Spam: Gauge=IIIIIII, Probability=7%, Report='__CP_MEDIA_BODY 0, __CP_URI_IN_BODY 0, __CT 0, __CTE 0, __CT_TEXT_PLAIN 0, __HAS_MSGID 0, __HAS_X_MAILER 0, __MIME_TEXT_ONLY 0, __MIME_VERSION 0, __SANE_MSGID 0' Sender: owner-theory@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Hello, I was not in the "dal" mail list, so I hope do not repeat issues that may be there before. I want to comment 3 issues related with TSAP (in general the use of format=metadata) that have appeared in the list 1) About an use case of the FORMAT=METADATA usage can be found at: http://svo.laeff.inta.es/modules.php? op=modload&name=phpWikiP&file=index&pagename=TSAP (or http://svo.laeff.inta.es --> TSAP in left menu under SVO Projects) I think that it is a clear example there :) The important point in the usage of format=metadata in that pages is that it is NOT restricted to spectrum, it can be use to query any dataset (image, spectrum, time series, catalog, numerical simulation...!) Format=metadata is just a first contact with a VO service ("Hello, what do you provide?") after that, you can continue with a SSA, an image, a numerical simulation via SNAP or, why not, another format=metadata query.... 2) About the claims that SSA covers the needs of those wishing to publish theory spectra... I think that it is a confusion here.... Maybe SSA covers these needs (I would including TSAP), but the real problem is how many applications includes the format=metadata query... I only know VOSpec and VOSed.... Services adn protocol are ready, the problem is in other place... In other words, SSA theoretical enable the access to theoretical models by the use of format=metadata, but it do not allow the access to theoretical models in the VO because it is not user-friendly implemented in applications (except a few of them). Any case It is not an issue in this mailing list. Finally, It also support the claim by Jesus about TSAP as a "transitory" protocol: - TSAP is necessary NOW because it is the only way to access theoretical data proved to work, at least in the applications it has been implemented. - It is hope to have another protocol (maybe more general) in the future... In fact it the "S" of spectra in TSAP is not required since the protocol can be used for data diferent than spectra. The "T" in TSAP is also not required, since the idea of the use of format=metadata is to query a service where there is no "a priori" knowledge about its offers, and there is no a predefined way to make a query (ej: there is no RA and DEC in the data the service offers) So, it is hope to have a "general access protocol" that allow access to all possible VOTables that are no spectra or image.... 3) Finally, about possible extensions... As I point out in the first item, I think that the most natural extension is to allow a format=metadata query recursively. In the current TSAP version, the TSAP service must be able to answer queries with query: answer 1. http..... format=metadata VOTable with possible query parameters without tabledata 2. http... value1=a&valuen=b VOTable with a list of references to others VOTables that can be loaded by the specific application 3. http.... id=12312 access to a particular VOTable with data The order is 1 --> 2 --> 3, but it is imposed by current applications using TSAP. But actually, the workflow can be 1 ---> 2 --> 1+2 ---> 1+2 ---> 1+2 --- > .... ---> 3 where 1+2 means "for fixed values on some fields in the query, is there more values to choose?". It allows to explore services like, as example, VizieR, or in general, any complex databese with no regular structure... cheers Miguel From owner-dal@eso.org Tue Jul 3 12:32:18 2007 X-Mozilla-Status: 0001 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 l63AVqoB015110 for ; Tue, 3 Jul 2007 12:31:52 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id l63AVqYj015109 for dal-outgoing; Tue, 3 Jul 2007 12:31:52 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-dal@eso.org using -f Received: from apollo.hq.eso.org (apollo.hq.eso.org [134.171.42.42]) by mercury.hq.eso.org (8.13.6+Sun/8.12.10) with ESMTP id l63AVpT3015105; Tue, 3 Jul 2007 12:31:51 +0200 (MEST) Received: from smtp.iaa.es (smtp.iaa.csic.es [193.146.145.11]) by apollo.hq.eso.org (8.13.8+Sun/8.12.10) with ESMTP id l63AVo6L015057; Tue, 3 Jul 2007 12:31:50 +0200 (CEST) Received: from [161.111.165.115] (dae-d15.iaa.csic.es [161.111.165.115]) (authenticated bits=0) by smtp.iaa.es (8.13.1/8.13.1) with ESMTP id l63AVi7k031657; Tue, 3 Jul 2007 12:31:44 +0200 In-Reply-To: References: <20070626115750.q3gwpurl6o0ck4wc@webmail.esac.esa.int> <001401c7b7f3$eabf9af0$cc48b782@gavopc1> Mime-Version: 1.0 (Apple Message framework v752.2) Content-Type: text/plain; charset=US-ASCII; delsp=yes; format=flowed Message-Id: <497429B6-C51C-43BF-8A05-7EF479482B21@iaa.es> Cc: dal@ivoa.net, theory@ivoa.net Content-Transfer-Encoding: 7bit From: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Subject: On FORMAT=METADATA Date: Tue, 3 Jul 2007 12:31:43 +0200 To: Doug Tody , Gerard , Carlos Rodrigo X-Mailer: Apple Mail (2.752.2) X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.3.2.304607, Antispam-Engine: 2.5.1.298604, Antispam-Data: 2007.7.3.31232 X-Perl-Spam: Gauge=IIIIIII, Probability=7%, Report='__CP_MEDIA_BODY 0, __CP_URI_IN_BODY 0, __CT 0, __CTE 0, __CT_TEXT_PLAIN 0, __HAS_MSGID 0, __HAS_X_MAILER 0, __MIME_TEXT_ONLY 0, __MIME_VERSION 0, __SANE_MSGID 0' Sender: owner-dal@eso.org Precedence: bulk Reply-To: =?ISO-8859-1?Q?Miguel_Cervi=F1o?= Hello, I was not in the "dal" mail list, so I hope do not repeat issues that may be there before. I want to comment 3 issues related with TSAP (in general the use of format=metadata) that have appeared in the list 1) About an use case of the FORMAT=METADATA usage can be found at: http://svo.laeff.inta.es/modules.php? op=modload&name=phpWikiP&file=index&pagename=TSAP (or http://svo.laeff.inta.es --> TSAP in left menu under SVO Projects) I think that it is a clear example there :) The important point in the usage of format=metadata in that pages is that it is NOT restricted to spectrum, it can be use to query any dataset (image, spectrum, time series, catalog, numerical simulation...!) Format=metadata is just a first contact with a VO service ("Hello, what do you provide?") after that, you can continue with a SSA, an image, a numerical simulation via SNAP or, why not, another format=metadata query.... 2) About the claims that SSA covers the needs of those wishing to publish theory spectra... I think that it is a confusion here.... Maybe SSA covers these needs (I would including TSAP), but the real problem is how many applications includes the format=metadata query... I only know VOSpec and VOSed.... Services adn protocol are ready, the problem is in other place... In other words, SSA theoretical enable the access to theoretical models by the use of format=metadata, but it do not allow the access to theoretical models in the VO because it is not user-friendly implemented in applications (except a few of them). Any case It is not an issue in this mailing list. Finally, It also support the claim by Jesus about TSAP as a "transitory" protocol: - TSAP is necessary NOW because it is the only way to access theoretical data proved to work, at least in the applications it has been implemented. - It is hope to have another protocol (maybe more general) in the future... In fact it the "S" of spectra in TSAP is not required since the protocol can be used for data diferent than spectra. The "T" in TSAP is also not required, since the idea of the use of format=metadata is to query a service where there is no "a priori" knowledge about its offers, and there is no a predefined way to make a query (ej: there is no RA and DEC in the data the service offers) So, it is hope to have a "general access protocol" that allow access to all possible VOTables that are no spectra or image.... 3) Finally, about possible extensions... As I point out in the first item, I think that the most natural extension is to allow a format=metadata query recursively. In the current TSAP version, the TSAP service must be able to answer queries with query: answer 1. http..... format=metadata VOTable with possible query parameters without tabledata 2. http... value1=a&valuen=b VOTable with a list of references to others VOTables that can be loaded by the specific application 3. http.... id=12312 access to a particular VOTable with data The order is 1 --> 2 --> 3, but it is imposed by current applications using TSAP. But actually, the workflow can be 1 ---> 2 --> 1+2 ---> 1+2 ---> 1+2 --- > .... ---> 3 where 1+2 means "for fixed values on some fields in the query, is there more values to choose?". It allows to explore services like, as example, VizieR, or in general, any complex databese with no regular structure... cheers Miguel From owner-theory@eso.org Tue Jul 3 14:26:05 2007 X-Mozilla-Status: 0011 X-Mozilla-Status2: 00000000 X-Mozilla-Keys: 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 l63CPtkF004842 for ; Tue, 3 Jul 2007 14:25:55 +0200 (MEST) Received: (from majordomo@localhost) by mercury.hq.eso.org (8.13.6+Sun/8.13.6/Submit) id l63CPtbP004841 for theory-outgoing; Tue, 3 Jul 2007 14:25:55 +0200 (MEST) X-Authentication-Warning: mercury.hq.eso.org: majordomo set sender to owner-theory@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 l63CPsxD004836; Tue, 3 Jul 2007 14:25:54 +0200 (MEST) Received: from esa-av-smtp2.gmessaging.net (esa-av-smtp2.gmessaging.net [194.51.201.23]) by apollo.hq.eso.org (8.13.8+Sun/8.12.10) with ESMTP id l63CPrb7024326; Tue, 3 Jul 2007 14:25:54 +0200 (CEST) Received: from conversion-daemon.esa-relay2.cesson.gm-adm by esa-av-smtp2.gmessaging.net (iPlanet Messaging Server 5.2 HotFix 2.04 (built Feb 8 2005)) id <0JKL00A01QS6W0@esa-av-smtp2.gmessaging.net> (original mail from Pedro.Osuna@sciops.esa.int); Tue, 03 Jul 2007 14:25:39 +0200 (MEST) Received: from esa-spas2.gmessaging.net (relay2 [172.24.21.39]) by esa-av-smtp2.gmessaging.net (iPlanet Messaging Server 5.2 HotFix 2.04 (built Feb 8 2005)) with ESMTP id <0JKL00BF2RUQ36@esa-av-smtp2.gmessaging.net>; Tue, 03 Jul 2007 14:25:38 +0200 (MEST) Received: from localhost (esa-spas2 [127.0.0.1]) by localhost.esa.gmessaging.net (Postfix) with ESMTP id 2B42E219F4E; Tue, 03 Jul 2007 14:25:38 +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 05126-21-4; Tue, 03 Jul 2007 14:25:36 +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 1EC17219F50; Tue, 03 Jul 2007 14:25:36 +0200 (CEST) Received: from sciops.esac.int (scimail.esac.esa.int [193.147.152.87]) by sciops-mailgw.vilspa.esa.int (Postfix) with ESMTP id 2A83211F8ED; Tue, 03 Jul 2007 14:24:40 +0200 (CEST) Received: from satl03.net4.lan (satl03.net4.lan [10.68.182.47]) (authenticated bits=0) by sciops.esac.int (8.13.1/8.13.1) with ESMTP id l63CPZTT023911; Tue, 03 Jul 2007 14:25:36 +0200 Date: Tue, 03 Jul 2007 14:25:32 +0200 From: Pedro Osuna Subject: Re: On FORMAT=METADATA In-reply-to: <497429B6-C51C-43BF-8A05-7EF479482B21@iaa.es> To: Miguel =?ISO-8859-1?Q?Cervi=F1o?= Cc: Pedro.Osuna@sciops.esa.int, Doug Tody , Gerard , Carlos Rodrigo , dal@ivoa.net, theory@ivoa.net Message-id: <1183465532.11466.107.camel@satl03.net4.lan> MIME-version: 1.0 X-Mailer: Evolution 2.0.2 (2.0.2-27.rhel4.6) Content-type: text/plain Content-transfer-encoding: 8BIT X-Spam-Score: Content analysis details: (-1.0 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] 0.2 AWL AWL: Auto-whitelist adjustment References: <20070626115750.q3gwpurl6o0ck4wc@webmail.esac.esa.int> <001401c7b7f3$eabf9af0$cc48b782@gavopc1> <497429B6-C51C-43BF-8A05-7EF479482B21@iaa.es> X-Scanned-By: MIMEDefang 2.35 X-PMX-Version: 5.3.2.304607, Antispam-Engine: 2.5.1.298604, Antispam-Data: 2007.7.3.50840 X-Perl-Spam: Gauge=IIIIIII, Probability=7%, Report='__CP_MEDIA_BODY 0, __CP_URI_IN_BODY 0, __CT 0, __CTE 0, __CT_TEXT_PLAIN 0, __HAS_MSGID 0, __HAS_X_MAILER 0, __MIME_TEXT_ONLY 0, __MIME_VERSION 0, __SANE_MSGID 0' Sender: owner-theory@eso.org Precedence: bulk Reply-To: Pedro Osuna Dear all, I am planning to send my inputs to the comments on the SSAP doc, both from the community point of view as from my VOQL Chair hat (which I have to following the RFC). >From my working group side, I had an informal action from Doug to write a "Use Case" in the form of appendix or similar for the FORMAT=METADATA case for Theoretical spectra, and how it is currently used with -so called- Theoretical Spectrum Access Protocol services. I will write this "Use Case" and send it to Doug and the community by tomorrow. This Use Case compiles inputs from both SVO and ESAVO, who were the ones that first described the possible TSAP, now embedded in SSAP. I think the absorption of the so called TSAP in the SSAP was already agreed some time ago, and it is maybe good enough for the time being at least. Whether we will have to review it in the future depending on what type of architecture is decided for the getCapabilities is something we will have to discuss later, I believe. Other issues related to what a "General Protocol" means, its relation to TAP, its relation to the "getCapabilities", etc., are outside the scope of the FORMAT=METADATA discussion for theoretical spectra here, as it affects many other things in which we are working on different fields and groups. I will be sending the inputs by tomorrow. Cheers, P. On Tue, 2007-07-03 at 12:31 +0200, Miguel Cerviño wrote: > Hello, > I was not in the "dal" mail list, so I hope do not repeat issues that > may be there before. > I want to comment 3 issues related with TSAP (in general the use of > format=metadata) that have appeared in the list > > 1) About an use case of the FORMAT=METADATA usage can be found at: > > http://svo.laeff.inta.es/modules.php? > op=modload&name=phpWikiP&file=index&pagename=TSAP > > (or http://svo.laeff.inta.es --> TSAP in left menu under SVO Projects) > I think that it is a clear example there :) > > The important point in the usage of format=metadata in that pages is > that it is NOT > restricted to spectrum, it can be use to query any dataset (image, > spectrum, time series, catalog, numerical simulation...!) > > Format=metadata is just a first contact with a VO service ("Hello, > what do you provide?") > after that, you can continue with a SSA, an image, a numerical > simulation via SNAP or, why not, another format=metadata query.... > > > 2) About the claims that SSA covers the needs of those > wishing to publish theory spectra... I think that it is a confusion > here.... > Maybe SSA covers these needs (I would including TSAP), but the real > problem is > how many applications includes the format=metadata query... I only > know VOSpec > and VOSed.... Services adn protocol are ready, the problem is in > other place... > > In other words, SSA theoretical enable the access to theoretical > models by the use of > format=metadata, but it do not allow the access to theoretical models > in the VO because > it is not user-friendly implemented in applications (except a few of > them). > > Any case It is not an issue in this mailing list. > > Finally, It also support the claim by Jesus about TSAP as a > "transitory" protocol: > - TSAP is necessary NOW because it is the only way to access > theoretical data proved > to work, at least in the applications it has been implemented. > - It is hope to have another protocol (maybe more general) in the > future... In fact > it the "S" of spectra in TSAP is not required since the > protocol can be used for data > diferent than spectra. > The "T" in TSAP is also not required, since the idea of > the use of format=metadata > is to query a service where there is no "a priori" knowledge > about its offers, and there > is no a predefined way to make a query (ej: there is no RA > and DEC in the data the > service offers) > > So, it is hope to have a "general access protocol" that allow > access to all possible VOTables that are no spectra or image.... > > > 3) Finally, about possible extensions... As I point out in the first > item, I think that the > most natural extension is to allow a format=metadata query recursively. > > In the current TSAP version, the TSAP service must be able to answer > queries with > > query: answer > 1. http..... format=metadata VOTable with possible > query parameters without > > tabledata > > 2. http... value1=a&valuen=b VOTable with a list of > references to others VOTables > > that can be loaded by the specific application > > 3. http.... id=12312 access to a > particular VOTable with data > > > The order is 1 --> 2 --> 3, but it is imposed by current applications > using TSAP. But > actually, the workflow can be 1 ---> 2 --> 1+2 ---> 1+2 ---> 1+2 --- > > .... ---> 3 > where 1+2 means "for fixed values on some fields in the query, is > there more values to choose?". It allows to explore services like, > as example, VizieR, or in general, any > complex databese with no regular structure... > > > cheers > > Miguel > > -- Pedro Osuna Alcalaya European Space Agency (ESA) European Space Astronomy Centre (ESAC) Research and Scientific Support Department (RSSD) Astronomy Science Operations Division (SCI-SD) e-mail: Pedro.Osuna@esa.int Tel + 34 91 813 13 14 Fax: +34 91 813 11 72 ------------------------------------------------- European Space Astronomy Centre (ESAC) P.O. Box 50727 E-28080 Villafranca del Castillo MADRID - SPAIN ================================================================================================ This message and any attachments are intended for the use of the addressee or ad