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IVOA Executive Committee Meeting (TM52)Telecon 12 Feb 2014Contents LogisticsTelecon: 12Feb2014 @11am EST Here's a pointer to a world clock to translate the time for your location:http://www.timeanddate.com/worldclock/fixedtime.html?msg=IVOA+Exec+Telecon&iso=20140212T11&p1=43&ah=2 Agenda
Reports from the ProjectsArgentina - NOVAArVOAstroGridAustralia-VOBRAVOChina-VO
ChiVOCVOEuro-VOThe current Euro-VO project, CoSADIE, is continuing to coordinate European VO activities. In particular, a Technology Forum gathering the teams which develop the VO will be held in Trieste, 12-13 March 2014 (http://www.cosadie.eu/twiki/bin/view/CoSADIE/TechForum3). CoSADIE will participate in a VO school organised in collaboration between Poland and France in Poland in June 2014. CoSADIE other strand of work is to assess all the elements necessary in a sustainable Euro-VO. This is done in close collaboration with the Astronet European project, which gathers the European funding agencies and establishes the strategy of astronomy in Europe. The new European Framework Programme, Horizon 2020, is explored to find how Euro-VO can look for support in the new context. Liaison with the Research Data Alliance and with other European projects such as EUDAT continues.ESAVOFrance VOThe annual meeting of the Action Spécifique Observatoires Virtuels France was held in Paris, 28-29 January 2014. The meeting programme and viewgraphs presented are at http://www.france-ov.org/twiki/bin/view/ASOVFrance/ProgrammeASOV2014 (mostly in French). The meeting gathered ~40 participants from Besançon, Grenoble, Nançay, Paris, Strasbourg, working on interoperability standards for astronomy, heliospheric and space plasma physics, planetary studies, and atomic and molecular physics (with also attendents working in the CTA project). Presentations dealt with the organisation of regional centres, standards, tools and services. The meeting demonstrated once again that the work on standards and tools performed in the IVOA context is reused and customized by other disciplines - taking advantage of the huge intellectual investment put by many in the IVOA. French teams continue to be very active in the development of standards in IVOA and in the other disciplines and in the organisation of the European/international Interoperability projects. Wrt. IVOA French teams are involved in the definition of most standards recently approved or in RFC (VOTable 1.3, PhotDM, VOUnits, PDL, MOC) and being worked at (DataLink, Simple Image Access, Spectral DM, Char2). France VO continues to support participation of staff working in French labs in IVOA meetings and in similar meetings organised in other disciplines.GAVO | ||||||||
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> > | GAVO's Heidelberg and Potsdam data centers keep maintaining and developing services, e.g., a new imaging catalog of nearby AGNs in the infrared, and an improved publication of a catalog of candidate members of open clusters. We are also involved in working out the details of publishing upcoming data from Gaia. In standards, we continued preparation of the relational registry, which we see as a successor to the current interface for querying searchable registries. We also implemented a flexible prototype for datalink services, including provisions for slicing and dicing of large datasets, and started prototyping an improved method for dealing with Echelle spectra in the VO. Client support for this is provided by SPLAT, which also grew a premliminary interface to ObsCore and Datalink. We are active within the Edu IG, where we collaborate on writing a combined requirements/best practice Note and set up a subversion repository open to all IVOA members to develop and maintain educational material in; this includes recommendations on documenting the translation status. | |||||||
HVOVObs.itA national hands-on workshop on VO, with attached a session on Science gateways, took place in Catania in December (19th to 21st); workshop program, details and materials can be found here http://vobs.astro.it/vofriends/. VObs.it is starting to organize itself for the Spring 2015 Interoperability Meeting. Two locations are under evaluation: Sesto/Sexten (on the Dolomites) or Venice. Costs (both for organizers and participants) will vary greatly from one choice to the other, Venice being more expensive. If Sesto is chosen the meeting dates should be shifted to June and, since it's not easily reachable with standard means of transportation and is about 150 km from Venice, VObs.it can organize (no more than) two coaches to bring participants from Venice airport to the Interop location and back at the beginning and end of the meeting respectively. For participants not being able to take advantage of this service (or not attending the full meeting) a shuttle bus service exists (~50/60€ per person), or local transportation.Japan-VOUkraine VOVAORVOSouth Africa VOSouth African Astroinformatics Alliance (SA3)The Southern African Large Telescope (SALT) Virtual Observatory Data Archive System (VODAS) is now available. SALT-VODAS allows users to search the SALT data archive for all publicly available SALT data. This includes data from commissioning proposals, included the High Resolution Spectrograph (HRS which is still being commissioned), all calibration data taken with SALT, and data from any proposal past its proprietary period. SALT-VODAs was developed in a collaboration between SAAO, SA3 and VO-India. Users can access VODAS from http://vodas.salt.ac.za/. This is first time data from any South African telescope has been made public. SA3 and CDS, with help from SA Centre for High Performance Computing (CHPC), has installed a mirror copy of VizieR, the CDS catalogue querying service, at the CHPC in Cape Town and is the process of testing it before making a public announcement. In addition to the primary site in France, VizieR mirrors are already functioning in Japan, Canada, India, UK, Russia, China and USA, but this is the first in the southern hemisphere. Patricia Whitelock February 2014 SVO(Since Sep 2013) Manpower: 8 FTEs. The SVO Thematic Network (people from Spanish institutes with interest in the VO) is composed of almost 200 participants from more than 30 labs. Science:
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