mailto: [email protected]
DESCRIPTION
F. Bonnarel 1 , M. Louys 1 , Igor Chilingarian 2,3 , Ivan Zolothukin 3 , Brice Gassmann 1 (1) CDS, Strasbourg, (2) LERMA , Paris, (3) SAI, Moscow. Navigation within VO collections using XML metadata descriptions - PowerPoint PPT PresentationTRANSCRIPT
characterizationaxis[axisframe/ucd=''pos'']/coverage/bounds/limits/stc:lolimit2vec/stc:c1/text() --> 308.512238
characterizationaxis[axisframe/ucd=''pos'']/coverage/bounds/limits/stc:lolimit2vec/stc:c2/text() --> 60.069312
characterizationaxis[axisframe/ucd=''pos'']/coverage/bounds/limits/stc:hilimit2vec/stc:c1/text() --> 308.798321
characterizationaxis[axisframe/ucd=''pos'']/coverage/bounds/limits/stc:hilimit2vec/stc:c2/text() --> 60.353806
characterizationaxis[axisframe/ucd='‘em'']/coverage/bounds/limits/stc:lolimit/text() --> 2.02 E10-6
mailto: [email protected]
Navigation within VO collections using XML metadata descriptions
Astronomical Spectroscopy and the Virtual Observatory Workshop,ESAC, March 2007
While studying a given observation the user wants to explore other VO data collections and request for other observations with similar or complementary properties.
• We offer a cross query mecanism based on the Characterisation metadata that can support various scenarii
oFrom an image look for IFU compatible data (this scenario)
oFrom a spectrum, search for images containing the observation position and with filters centered on some specific WL range (Ha), for instance
o From a 2D image search for other 2D images on different VO servers with fine selection criteria
1: Retrieve characterisation of an
Observation from a VO server and
visualise it using the CAMEA tool (*)
SELECT * FROM processed_data WHERE '//Chaxis[axisframe/ucd=''pos'']/coverage/location/coord/stc:position2d/value2/c1/text()‘ <= 308.798321
AND'//Chaxis[axisframe/ucd=''pos'']/coverage/location/coord/stc:position2d/value2/c1/text()‘ >= 308.512238
AND '//Chaxis[axisframe/ucd=''pos'']/coverage/location/coord/stc:position2d/value2/c2/text()‘ <= +60.353806
AND'//Chaxis[axisframe/ucd=''pos'']/coverage/location/coord/stc:position2d/value2/c1/text()‘ >= +60.069312
AND'//Chaxis[axisframe/ucd=''pos'']/axisframe/numbins2/i1/text()‘>1 AND'//Chaxis[axisframe/ucd=''pos'']/axisframe/numbins2/i2/text()‘>1 AND'//Chaxis[axisframe/ucd=''em'']/axisframe/numbins1/text()‘>1 AND'//Chaxis[axisframe/ucd=''em'']/coverage/location/coord/stc:spectral/stc:value/text()‘ <2.02e-06 ;
(*) Characterisation editing tool: (CAMEA: Characterisation for astronomical metadata Editing Application) : build up by CDS within the framework of VOTECH DS5) This application offers a user-friendly interface to browse, create or edit an XML metadata file compliant to the Characterisation schema. It supports all predefined axes: spatial, spectral, time, observable, but also allows for new axis definition.(#) http://alcor.sao.ru/php/search
F. Bonnarel 1, M. Louys 1, Igor Chilingarian 2,3, Ivan Zolothukin 3 , Brice Gassmann 1
(1) CDS, Strasbourg, (2) LERMA , Paris, (3) SAI, Moscow
Services supporting Characterisation Data Model can build a description of the physical content of their data. They express how Observations data values are spanned along physical axes and provide for each of these axes, assessments of properties of the data like the location, the limits or bounds, the resolution, etc. These metadata allow seeking for similar or complementary data in services supporting the same description.
2: Identify relevant metadata to search and filter out interesting data
3: Build up a request on these
criteria to Characterisation
compliant services
Derive proper Utypes to select other
observations
Define a metadata mask for query composition using Xpath syntax
Conclusion: Indexing the content of observational data of any dimension is now feasible in the VO, using existing data models such as the Characterisation and Spectrum data model via their Utypes representations
4: Get results from ASPID-SR database (#)
Characterisation of a 2MASS J image
3D-Spectroscopy
Bounds
2.16e 10-6
File
List XML
CharacterisationFITS
Headers
Spatial
Spectral
Find out 3D spectroscopy data falling within the bounds of our 2D image at shorter wavelength
Spectral Bounds
CAMEA : Characterisation editing tool