IVOA Interoperability Meeting – Victoria, BC – 18 May 2006 Data Discovery and Metadata Query Using Characterisation DM Igor Chilingarian (CRAL Observatoire.

Slides:

Advertisements

Similar presentations

European Space Astronomy Centre (ESAC) Villafranca del Castillo, MADRID (SPAIN) Pedro OSUNA ESAC ADT Team VOSpec IVOA Poona Sep 2004 VOSpec: A Tool to.

Advertisements

Characterisation of observations François Bonnarel, Mireille Louys, Anita Richards, Alberto Micol, Jonathan McDowell, Igor Chilingarian, et al.

IVOA Interop, Cambridge UK, IVOA Data Access Layer Table Access Protocol Analysis Doug Tody (NRAO/NVO ) I NTERNATIONAL V IRTUAL O BSERVATORY A LLIANCE.

European Space Astronomy Centre (ESAC) Villafranca del Castillo, MADRID (SPAIN) Jesús Salgado SLAP Implementations Sep 2006, Moscow, Russia Simple Line.

May 14, 2007TIG, opening plenary Beijing 2007 Theory IG plans Editors: Claudio Gheller, Patrizia Manzato, Laurie Shaw, Herve Wozniak, GL Other participants:

IVOA, Pune India September Data Access Layer Working Group Pune Workshop Summary Doug Tody National Radio Astronomy Observatory International.

28 October 2008 IVOA Interoperability Meeting -- Baltimore T HE I NTERNATIONAL V IRTUAL O BSERVATORY ALLIANCE TAP/VOTable Registry Interface Reg 1 – G.

DM WORKING GROUP MADRID OCT WG STATUS Spectral DM: document updated and reformatted Spectral DM Java library prototype nearly ready Characterization:

Victoria, May Session III Theory Interest Group Session III Victoria, May

May 18, 2007TIG, closing plenary Conclusions from theory IG sessions, Beijing 2007.

European Space Astronomy Centre (ESAC) Villafranca del Castillo, MADRID (SPAIN) Alberto Micol ISO & CharDM IVOA Cambridge, The Characterisation.

SSA Query Interface M. Dolensky, ESO Data Access Layer Working Group Interoperability Workshop, Pune, India 27-Sep-2004.

Characterization 2 and Provenance data models. Use cases and first roadmap F.Bonnarel (CDS)

IVOA, Pune September Data Access Layer Working Group SSA Overview and Status Doug Tody National Radio Astronomy Observatory International V.

MEx Metadata extraction. IVOA Interop, Moscow, 19-Sep-2006 Metadata extraction The problem The problem Data centres need their data described homogeneously.

IVOA Interop meeting 05/17/2006 Victoria F.Bonnarel (CDS) Generic Data discovery, Cube acces: CGPS Archive browser F.Bonnarel,T.Boch,D.Durand (CDS, CADC)

SLAP: Simple Line Access Protocol v0.5

IVOA, Kyoto May Data Access Layer Working Group Working Group Report and Summary Doug Tody National Radio Astronomy Observatory International.

A.Micol IVOA Registry REGISTRY WG Mar 2003 A Science Case (and 1000 Questions) for the IVOA Registry.

6 September 2008NVO Summer School 2008 – Santa Fe1 DAL Clients: Scripting Data Access with Python Ray Plante T HE US N ATIONAL V IRTUAL O BSERVATORY.

2008 NVO Summer School1 Data Access Layer Services Doug Tody (NRAO) T HE US N ATIONAL V IRTUAL O BSERVATORY.

Spectroscopic Data ASTR 3010 Lecture 15 Textbook Ch.11.

Lessons learnt with Aladin and characterization experience for SIA2.0 F.Bonnarel, CDS (credit to Aladin developpers, CADC,ECF,ESAC, ESO VO people, DAL.

The hydrogen atom Energy is measured in eV, or electron volts Light (photon) is electromagnetic energy Since only permitted electron orbits (energies),

Atomic Spectra. Continuous Spectra The (Visible) Hydrogen Spectrum.

S. Derriere et al., ESSW03 Budapest, 2003 May 20 UCDs - metadata for astronomy Sébastien Derriere François Ochsenbein Thomas Boch CDS, Observatoire astronomique.

IVOA Interop Beijing, DM I Analysis of Characterisation in Domain Model Context With application to (SNAP) simulations Gerard Lemson DWith feedback.

Diversity of domain descriptions in natural science: virtual observatory as a case study Briukhov D.O., Kalinichenko L.A., Zakharov V.N. Institute of Informatics.

3D Spectroscopy in the Virtual Observatory: Current Status Igor Chilingarian (Observatoire de Paris, France/SAI MSU, Russia) Ivan Zolotukhin (SAI MSU,

Characterisation Data Model applied to simulated data Mireille Louys, CDS and LSIIT Strasbourg.

F. Genova, VOTECH kickoff meeting, 2004/11/ Interoperability standards F. Genova, M. Allen, T. Boch, F. Bonnarel, S. Derriere, P. Fernique, F. Ochsenbein,

IVOA Interop, Victoria Canada, May IVOA Data Access Layer Closing Plenary Summary, Victoria May 2006 Doug Tody (NRAO/NVO/IVOA) I NTERNATIONAL V IRTUAL.

16-17 Oct 2003IVOA Data Access Layer, Strasbourg IVOA Data Access Layer (DAL) Working Group Doug Tody National Radio Astronomy Observatory International.

29-30 April 2004NVO Team Meeting NCSA1 Data Access Layer (DAL) SSA, SIA Enhancement Doug Tody National Radio Astronomy Observatory National Virtual Observatory.

European Space Astronomy Centre (ESAC) Villafranca del Castillo, MADRID (SPAIN) Jesús Salgado SLAP Implementations May 2007, Beijing, China Simple Line.

Handling 3D Data in the Virtual Observatory

SimDB and DM WG Summary SimDB session this morning.

European Space Astronomy Centre (ESAC) Villafranca del Castillo, MADRID (SPAIN) Jesús Salgado Spectroscopic lines in the VO context Mar 2007, ESAC, Madrid,

IVOA Interop, SL de El Escorial, Oct IVOA DAL - Madrid DAL WG Summary October 7, 2005.

ESAVO/European Space Astronomy Centre (ESAC) Villafranca del Castillo, MADRID (SPAIN) Isa Barbarisi Beijing, May 2007 VOSpec new functionalities.

 The Bohr model was proposed:  1913  by Neils Bohr  After observing the H line emission spectrum.

IVOA, Kyoto May Data Access Layer Working Group Status and Plans for this Workshop Doug Tody National Radio Astronomy Observatory International.

October 7, 2005VOQL-Madrid1 IVOA – VOQL WG session ESAC Villafranca del Castillo Madrid, Spain Friday, October 7th, 9: :00 Yuji Shirasaki Maria Nieto-Santisteban.

European Space Astronomy Centre (ESAC) Villafranca del Castillo, MADRID (SPAIN) Jesús Salgado IVOA Interop meeting Strasbourg, May 2009 (1/12) SLAP v0.9.

European Space Astronomy Centre (ESAC) Villafranca del Castillo, MADRID (SPAIN) Pedro OSUNA ESAC ADT Team VO-tech Cambridge 2004 VOSpec: A Tool to Handle.

AstroGrid Solar/STP planning meeting Agenda: Helioscope Preparing for Solar-B Time-series viewing application IVOA and time series A PPARC funded project.

VOTECH meeting 03/06-09/2006 Sorrento F.Bonnarel (CDS) CDS DS6 cycle 3 plans F.Bonnarel In behalf of CDS team.

CMU-CS lunch talk, Gerard Lemson1 Computational and statistical problems for the Virtual Observatory With contributions from/thanks to: GAVO.

PhotDM implementation feedback | Jesus Salgado | ESAC | 18 October 2011 | IVOA Pune 2011 | Pag. 1 Photometry DM implementation feedback Jesus.

Workshop on How to Publish Data in VO ESAC, June 25-June DAL (Data Access Layer) protocols Jesus Salgado

21-jun-2009 IVOA Standards Pedro Osuna ESA-VO Project Science Archives and Computer Support Engineering Unit (SRE-OE) Science Operations Department (SRE-O)

12 Oct 2003VO Tutorial, ADASS Strasbourg, Data Access Layer (DAL) Tutorial Doug Tody, National Radio Astronomy Observatory T HE US N ATIONAL V IRTUAL.

Obscore DM v 1.1 Mireille Louys, Doug Tody, Patrick Dowler, Daniel Durand, Laurent Michel, François Bonnarel, Alberto Micol and the IVOA DataModel working.

TCG Meeting, May 15, IVOA Science Requirements - 1/14 Science Requirements and IVOA Standards Paolo Padovani on behalf of the Take-Up Committee.

How to represent coverage: temporal, spectral, positional Clive Page AstroGrid Project University of Leicester 2003 March 19.

Publishing Combined Image & Spectral Data Packages Introduction to MEx M. Sierra, J.-C. Malapert, B. Rino VO ESO - Garching Virtual Observatory Info-Workshop.

The Virtual Solar Observatory – An Operational Resource for Heliophysics Informatics Frank Hill & The VSO Team.

Describing 3D Datasets Igor Chilingarian (CRAL Observatoire de Lyon/Sternberg Astronomical Institute of the Moscow State University) IVOA DM & DAL WG –

VO Data Access Layer IVOA Cambridge, UK 12 May 2003 Doug Tody, NRAO.

Registry workgroup: Final summary IVOA Interop Plenary Kyoto May 16-20, 2005 Tony Linde IVOA Registry workgroup chair AstroGrid Programme Manager VOTech.

9/Dec/2010Interoperability meeting, Nara, Japan Characterisation v.2 use-cases Update on the full spectrum fitting Igor Chilingarian (CDS) on behalf of.

Is non-unicity of utype/ucds a problem? The problem: is it possible to query some IVOA database directly from UCDs or Utypes? Select * from ivoa_table.

ESAC 2017 JWST Workshop JWST User Documentation Hands on experience

Analysis of Characterisation in Domain Model Context

UVIS Calibration Update

S3 from the point of view of SimDB

IVOA – VOQL WG session ESAC Villafranca del Castillo Madrid, Spain Friday, October 7th, 9: :00 Yuji Shirasaki Maria Nieto-Santisteban VOQL-Madrid.

Utypes for Model Referencing

Before Bell Rings Grab 2 Papers From The Side Table Have your Electron Energy and Light Packet out for me to Check.

Presentation transcript:

IVOA Interoperability Meeting – Victoria, BC – 18 May 2006 Data Discovery and Metadata Query Using Characterisation DM Igor Chilingarian (CRAL Observatoire de Lyon, France/SAI MSU, Russia) on behalf of Characterisaton subgroup of DM WG

IVOA Interoperability Meeting – Victoria, BC – 18 May 2006 Commonalities of DAL protocols Query interfaces of: SIAPSSAPSLAP STAP (Astrogrid) In all the cases query is constructed using “mnemonic” parameter names, for example POS=180,10&SIZE=1.0&BAND=4e-7/5e-7 In all cases “mandatory” query parameters correspond to the characterisation DM elements

IVOA Interoperability Meeting – Victoria, BC – 18 May 2006 Using Characterisation DM Query interface we propose: Usage of the “axis” concept to “universalize” the queries on different physical parameters. Usage of at least first and at most second level of the characterisation metadata Axes are identified by their UCDs list of available axes should be given by the getCapabilities query (or its analogue) Usage of complete characterisation UTYPEs as http-get (post) parameter names Additional parameters (not covered by characterisation DM) should be given by the getCapabilities query

IVOA Interoperability Meeting – Victoria, BC – 18 May 2006 Example 1. Accessing Spectra spectral: give me all the flux calibrated data from the archive with the central wavelength between 4500A and 4900A, with a starting wavelength not longer than 4200A, with a finishing wavelength not shorter than 6000A, having FWHM spectral resolution between 1A and 2A, axis1.ucd=em&axis1.calibrationStatus=1&axis1.unit=um& axis1.ucd=em&axis1.calibrationStatus=1&axis1.unit=um& axis1.coverage.location.Coord.Coordinate.value=0.45/0.49& axis1.coverage.location.Coord.Coordinate.value=0.45/0.49& axis1.coverage.bounds.limits.LoLimit=/0.42& axis1.coverage.bounds.limits.LoLimit=/0.42& axis1.coverage.bounds.limits.HiLimit=0.6/& axis1.coverage.bounds.limits.HiLimit=0.6/& axis1.resolution.refval=0.0001/0.0002& axis1.resolution.refval=0.0001/0.0002& axis2.ucd=phot&axis2.calibrationStatus=1 axis2.ucd=phot&axis2.calibrationStatus=1

IVOA Interoperability Meeting – Victoria, BC – 18 May 2006 Example 2: Images images: give me all the flux calibrated data from the archive with the central wavelength between 4000A and 10000A, with the right ascension of the centre between 12h and 18h, and declination of the centre >+88 deg, having FWHM spatial resolution not less than 3.6 arcsec. Interesting: this query should also return 3D spectroscopic data if they exist in the archive. axis1.ucd=em&axis1.calibrationStatus=1&axis1.unit=um& axis1.ucd=em&axis1.calibrationStatus=1&axis1.unit=um& axis1.coverage.location.Coord.Coordinate.value=0.4/1.0& axis1.coverage.location.Coord.Coordinate.value=0.4/1.0& axis2.ucd=pos&axis1.calibrationStatus=1&axis1.unit=deg& axis2.ucd=pos&axis1.calibrationStatus=1&axis1.unit=deg& axis2.coverage.location.Coord.Position2D.Value2.c1=180/270& axis2.coverage.location.Coord.Position2D.Value2.c1=180/270& axis2.coverage.location.Coord.Position2D.Value2.c2=88/90& axis2.coverage.location.Coord.Position2D.Value2.c2=88/90& axis2.resolution.refval=0.001/& axis2.resolution.refval=0.001/& axis3.ucd=phot&axis3.calibrationStatus=1 axis3.ucd=phot&axis3.calibrationStatus=1

IVOA Interoperability Meeting – Victoria, BC – 18 May 2006 Example 3: 3D data (IFU, Fabry-Perot,…) 3D spectra: give me all the flux calibrated data from the archive with the central wavelength between 4500A and 4900A, having FWHM spectral resolution between 1A and 2A, located at the area with the right ascension of the centre between 12h and 18h, and declination of the centre >+88 deg, having FWHM spatial resolution not less than 1.8 arcsec ?axis1.ucd=em&axis1.calibrationStatus=1&axis1.unit=um& ?axis1.ucd=em&axis1.calibrationStatus=1&axis1.unit=um& axis1.coverage.location.Coord.Spectral.value=0.45/0.49& axis1.coverage.location.Coord.Spectral.value=0.45/0.49& axis1.coverage.bounds.limits.LoLimit=/0.42& axis1.coverage.bounds.limits.LoLimit=/0.42& axis1.coverage.bounds.limits.HiLimit=0.6/& axis1.coverage.bounds.limits.HiLimit=0.6/& axis1.resolution.refval=0.0001/0.0002& axis1.resolution.refval=0.0001/0.0002& axis2.ucd=pos&axis1.calibrationStatus=1&axis1.unit=deg& axis2.ucd=pos&axis1.calibrationStatus=1&axis1.unit=deg& axis2.coverage.location.Position2D.Value2.c1=180/270& axis2.coverage.location.Position2D.Value2.c1=180/270& axis2.coverage.location.Position2D.Value2.c2=88/90& axis2.coverage.location.Position2D.Value2.c2=88/90& axis2.resolution.refval=0.001/& axis2.resolution.refval=0.001/& axis3.ucd=phot&axis3.calibrationStatus=1 axis3.ucd=phot&axis3.calibrationStatus=1

IVOA Interoperability Meeting – Victoria, BC – 18 May 2006 Example 4: Atomic Lines spectral lines: give me all spectral lines of Hydrogen (ssp.atomicNumber), between 900A and 1500A with the final energy level between 13.5 and 13.7 eV (get Lyman series). “ssp” means Service-Specific Parameter ?axis1.ucd=em&axis1.calibrationStatus=1&axis1.unit=um& ?axis1.ucd=em&axis1.calibrationStatus=1&axis1.unit=um& axis1.coverage.location.Coord.value=0.09/0.13& axis1.coverage.location.Coord.value=0.09/0.13& axis2.ucd=phys.energy%3Bphys.atom.final%3Bphys.atom.level& axis2.ucd=phys.energy%3Bphys.atom.final%3Bphys.atom.level& axis2.unit=eV&axis2.calibrationStatus=1& axis2.unit=eV&axis2.calibrationStatus=1& axis2.coverage.location.Coord.value=13.5/13.7& axis2.coverage.location.Coord.value=13.5/13.7& ssp.atomicNumber=1 ssp.atomicNumber=1

IVOA Interoperability Meeting – Victoria, BC – 18 May 2006Caveats UCD 1+ may contain “;” that is equivalent to “&” in the HTTP_GET Query length may exceed 4096 bytes allowed for HTTP_GET Upper/lower case issue: parameters are case- sensitive for HTTP_GET, but UTYPEs are case- insensitive

IVOA Interoperability Meeting – Victoria, BC – 18 May 2006 Useful Features Easy conversion into XQuery Logical extension: use ADQL/x instead of http-get query No more discussions on the names of the parameters!