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P. Padovani, September 15, 2009 - ESO VO Day - 1/15 The Virtual Observatory Paolo Padovani Head, Virtual Observatory Project Office, ESO EURO-VO Facility.

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Presentation on theme: "P. Padovani, September 15, 2009 - ESO VO Day - 1/15 The Virtual Observatory Paolo Padovani Head, Virtual Observatory Project Office, ESO EURO-VO Facility."— Presentation transcript:

1 P. Padovani, September 15, 2009 - ESO VO Day - 1/15 The Virtual Observatory Paolo Padovani Head, Virtual Observatory Project Office, ESO EURO-VO Facility Centre Scientist

2 P. Padovani, September 15, 2009 - ESO VO Day - 2/15 The way Astronomy works Telescopes (ground- and space-based, covering the full electromagnetic spectrum)  Observatories Instruments (telescope/band dependent)  Observatories/Consortia Publications  Journals Data curation (metadata + tables & catalogues)  Data curators Data analysis software (instrument dependent)  Observatories/Consortia/Researchers Active Archives  Observatories/Agencies … and Public Outreach  Observatories/Agencies

3 P. Padovani, September 15, 2009 - ESO VO Day - 3/15 Information Avalanche Huge surveys:100 million sources at 100 years to identify them Ever fainter sources routinely surpassing the identification limits of 8 - 10m telescopes [R ≈ 25]25 Huge data collections: download and data analysis on desktop problematic/impossible. Example: downloading Sloan Digital Sky Survey (SDSS) DR6 data: images (10 Terabytes)  ~ 3 months at 10 Mbps (ESO’s speed) catalogues (2 Terabytes)  ~ 3 weeks on DVDs  ~ 2,100 of them And data analysis?? (similar size for MACHO, 2MASS etc …)

4 R ~ 25.5, VLT/FORS2, t exp ~ 2.5 hrs (Szokoly et al. 2004)

5 P. Padovani, September 15, 2009 - ESO VO Day - 5/15 Instruments Data Headers Telescope control Logs Observatories Outreach Products Calibrations Raw Data Processed Data Analysis Data Products Catalogues Software Computing Publications Papers Tables Figures courtesy of P. Quinn

6 P. Padovani, September 15, 2009 - ESO VO Day - 6/15 The Virtual Observatory The Virtual Observatory (VO) is an innovative, still evolving, system to:  take advantage of astronomical data explosion  allow astronomers to interrogate multiple data centres in a seamless and transparent way and to utilize at best astronomical data  permit remote computing and data analysis  foster new science Web: all documents inside PC; VO: all astronomical databases inside PC VO  democratization of astronomy! All of the above requires the various players to speak the same language  VO standards and protocols defined and adopted within the IVOA (International Virtual Observatory Alliance), which includes 17 projects world-wide

7 P. Padovani, September 15, 2009 - ESO VO Day - 7/15 17 China India Canada Spain Italy Armenia France Germany Hungary Japan Korea USA Russia UK AustraliaEurope (Brazil joined recently)

8 P. Padovani, September 15, 2009 - ESO VO Day - 8/15 The European View: the EURO-VO http://www.euro-vo.org http://www.euro-vo.org Successor to the Astrophysical Virtual Observatory (AVO), which was a 5 M€, Phase A study (2001 - 2004/5) on the scientific requirements and technology for building the VO in Europe, 50% funded by European Community (Fifth Framework Programme [FP5]) Includes 8 partners: ESO, European Space Agency (ESA), plus six national nodes: INAF (Italy), INSU (France), INTA (Spain), NOVA (Netherlands), PPARC (UK), and RDS (Germany) Has three components: Data Centre Alliance, Technology Centre, Facility Centre Partly funded by the EC but substantial (> 50%) partner support

9 An alliance of European data centres who will populate the EURO-VO with data, provide the physical storage and computational fabric and who will publish data, metadata and services to the EURO-VO using VO technologies A distributed organization that coordinates a set of research and development projects on the advancement of VO technology, systems and tools in response to scientific and community requirements An operational organization, that provides the EURO-VO with a persistent, centralized registry for resources, standards and certification mechanisms as well as community support for VO technology take-up and scientific programs. EURO- VO’s “public face” @ ESO managed by ESO and ESA

10 P. Padovani, September 15, 2009 - ESO VO Day - 10/15 The EURO-VO Project: AIDA The “Astronomical Infrastructure for Data Access (AIDA)” project is funded by the EC FP7 through the Infrastructure call INFRA-2007-1.2.1 “Scientific Digital Repositories” AIDA has the same partners as the EURO-VO Project started on Feb. 1, 2008, which ensures continuation of European-wide VO activities at least until mid-2010 AIDA is a combination of DCA, VOTC, and FC activities AIDA aims at unifying the digital data collection of European astronomy, integrating their access mechanisms with evolving e- technologies and enhancing the science extracted from these data-sets One of AIDA’s main goals is to support the European astronomical community in their exploitation of astronomical data through VO tools

11 P. Padovani, September 15, 2009 - ESO VO Day - 11/15 ESO and the VO ESO operates one of the largest astronomical archives in the world ESO is committed to becoming a key provider of data and resources in the Virtual Observatory:  Founding member of IVOA  Lead partner of Astrophysical Virtual Observatory  Lead partner of EURO-VO To this aim, ESO has created (Nov. 2004) the Virtual Observatory Systems Dept., which then evolved (June 2008) into the Virtual Observatory Project (VOP) Office to manage ESO’s VO activities and make sure ESO data are VO compliant In practice: we make sure that ESO’s data products are “interoperable” and “up- to-date” and that ESO’s voice is heard at the international level when data access and exchange standards are discussed VOP includes 5 people: PP, Fabien Chereau, EH, Alberto Micol, and Bruno Rino

12 P. Padovani, September 15, 2009 - ESO VO Day - 12/15 Science and the Virtual Observatory The ultimate goal of the VO is to facilitate the work of astronomers and foster new science. This is done directly by: allowing easier/better access to (ever larger amounts of) data providing new/improved research tools (see http://www.euro- vo.org/pub/fc/software.html) http://www.euro- vo.org/pub/fc/software.html And indirectly by: motivating data centres to: 1.agree on common standards (esp. for information exchange) 2.provide homogeneous meta-data (data about data) and quality flags 3.produce and/or collect science-ready data Indirect ways not easily linkable to the VO!

13 P. Padovani, September 15, 2009 - ESO VO Day - 13/15 The VO and science-ready data Astronomical research nowadays needs a variety of multi- wavelength data Access to individual archives is time-consuming and not easy: different astronomical archives have widely different access/search interfaces and standards/conventions Data reduction requires widely specialized, complex analysis software for various bands (radio, IR, optical, X-ray, etc.) Astronomers need and want reduced data! The VO provides access to science-ready data. But only if: they exist! the data provider has gone through the (often small) effort of “publishing them” to the VO (= following VO standards)

14 P. Padovani, September 15, 2009 - ESO VO Day - 14/15 ESO VO Day Goal: expose ESO astronomers to VO tools and services so that they can use them efficiently for their own research; based on our experience, this is the most effective way to introduce astronomers to the VO Methods: –lecture and tutor the participants on the usage of such tools –give real life examples of scientific applications –hands-on exercises Participants: 27 (+ 4 tutors: PP, EH, Mark Allen [CDS, Strasbourg] and Mark Taylor [AstroGrid, UK])

15 P. Padovani, September 15, 2009 - ESO VO Day - 15/15 VO Day Programme General introduction to VO tools Three use cases in increasing order of complexity Lunch will be provided in front of the Auditorium Important: some tools are still “shaky”, so please be patient! use cases might seem easy to do now, but have required quite some work on the tutors’ side VO science still requires astrophysical judgement! Time for feedback at the end


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