Prototype. Towards an AVO Interoperability. Mark Allen Françoise Genova CDS & the AVO Work Area 2 team:
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1 Towards an AVO Interoperability Prototype Mark Allen Françoise Genova CDS & the AVO Work Area 2 team: C. Arviset (ESA) P. Didelon (SAP/Terapix) S. Garrington (Jodrell Bank) R. Mann (ROE) A. Micol (ESO-ECF) A. Richards (Jodrell Bank) G. Rixon (Cambridge UK) A. Wicenec (ESO) + C. Benoit (OCA Nice) J. Lewis (Cambridge UK)
2 Outline AVO Interoperability prototype Goals, Metadata and Interoperability Target archives Interoperability demonstration Query by UCD, prototype wavelength query Example: multi images + catalog overlays Practical recommendations for interoperability
3 AVO interoperability prototype Goals: Federate a set of archives into CDS interoperability service Early science usage New VO functionalities Standards (UCDs, VOTable Ochsenbein, Derriere) see contributions from Build set of recommendations for archive providers Evaluate interoperability tools
4 Metadata Building blocks for interoperability UCDs, keywords, units UCDs encode semantics i.e. meaning of contents, not just a label Hierarchical tree structure Efficient searching Combine relevant information (Table-joins)
5 Basic interoperability goals Seamless interoperability at: Coordinates level overlays, mosaics Units level : combining measurements Custom merged datasets data fusion Building blocks for Concept level Data mining
6 Why &? Existing interoperating system Semi-centralised meta-data Links to distributed archival data Units and UCDs already defined for every column of every table and archive in Vizier Evaluation of metadata definitions Develop and test high level meta-data concepts [ in parallel with development of distributed metadata systems]
7 Target Archives MERLIN EIS (ESO) VLT NTT HST/ECF Wide field UK e.g. INT XMM ISO CFHT 12k Representative of SPACE/GROUND-BASED, and wide range of wavelength
8 Available for science usage NOW MERLIN EIS (ESO) ISO soon XMM (log incl.) INT + already implemented: HST Chandra CFHT VLA: NVSS 2MASS DSS GSC, UNSO + soon TNG, IRAM
9 Archive/Catalog integration Driver for new developments in interoperability tools e.g. ALADIN for radio images Astrometric registration UCD tool development Ways to use the semantics, e.g. search by UCD and UCD wavelength map for photometry searches
10 HST archive + user images
11
12 Registration In development
13 Search by UCD To address common features of science scenario questions posed for prototype VOs e.g. Find B-band photometry... in a particular region of the sky, or... of a particular type of object Possible via: wavelength map of UCDs and CDS database tools
14 Search by photometry Select wavlength range Interpreted by UCD wavelength map Combine with object name or sky region
15
16 Identified UCDs Tables including UCD column Table column matching object and wavelength selected UCD
17 Chandra Deep Field South
18
19
20
21
22 Archive/catalog implementations Systematic approach Archive holders know their data best Best when archives participate in defining metadata Human interaction required at this stage. Issues: Access, proprietry periods Maintenance -- update mechanisms
23 Interactions with archive providers Stimulating review of archive exposure mechanisms Metadata definitions What information is required to decribe their data holdings?
24 Building practical recommendations for interoperability Metadata layer structure and functionality Efficiencies of distributed/semi-centralized metadata Immediate practicalities: Standards, UCDs, archive exposure Detailed interoperability eg. Photometry Make filter system characteristics accessible Transmission curves can be integrated
25 Conclusions CDS interoperability test bed available for Metadata development Early science usage. feedback welcome Available now Efficient semi-centralized system for high level demo and testing - development in concert with distributed system architecture
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