CARS_sourcesivo://org.gavo.dc/cars/q/catThe GAVO DC teamErben, T.Hildebrandt, H.Lerchster, M.Hudelot, P.Benjamin, J.van Waerbeke, L.Schrabback, T.Brimioulle, F.Cordes, O.Dietrich, J. P.Holhjem, K.Schirmer, M.Schneider, P.2026-01-16T10:33:56ZGAVO Data Centre Team

Mönchhofstrasse 12-14, D-69120 Heidelberg

gavo@ari.uni-heidelberg.de+49 6221 54 1837catalogssurface-photometrygalaxy-distancesobservational-cosmologyImages and data from from the CFHTLS archive research survey, a multi-band dataset spanning 37 square degrees of sky in high galactic latitudes.2009A&A...493.1197Ehttp://dc.g-vo.org/cars/q/cat/infoIsServedByGAVO Data Center TAP serviceIf you use the CARS products for your own research, please give proper acknowledgment to `CADC <http://www4.cadc-ccda.hia-iha.nrc-cnrc.gc.ca/>`_, the `CFHTLS project <http://www.cfht.hawaii.edu/Science/CFHLS/cfhtlspublitext.html>`_ and the publication 2009A&A...493.1197Ehttp://dc.g-vo.org/cars/q/cat/formhttps://dc.g-vo.org/cars/q/cat/formhttp://dc.g-vo.org/cars/q/cat/scs.xml?https://dc.g-vo.org/cars/q/cat/scs.xml?GETapplication/x-votable+xmlRARight Ascension (ICRS decimal)degpos.eq.rarealDECDeclination (ICRS decimal)degpos.eq.decrealSRSearch radiusdegrealmagAutoKron-like elliptical aperture magnitudemagphot.magrealsgclassS/G classifier output (0..1)src.class.starGalaxyrealresponseformatFile format requested for output.meta.code.mimecharmaxrecMaximum number of records returned. Pass 0 to retrieve service parameters.integerverbExhaustiveness of column selection. VERB=1 only returns the most important columns, VERB=2 selects the columns deemed useful to the average user, VERB=3 returns a table with all available columns.integer180100000true36-60.01http://dc.g-vo.org/cars/q/cat/capabilitieshttps://dc.g-vo.org/cars/q/cat/capabilitieshttp://dc.g-vo.org/cars/q/cat/availabilityhttps://dc.g-vo.org/cars/q/cat/availabilityhttp://dc.g-vo.org/cars/q/cat/tableMetadatahttps://dc.g-vo.org/cars/q/cat/tableMetadatahttp://dc.g-vo.org/taphttps://dc.g-vo.org/tap3/276,297 4/669-671,692-693,712,714,1093,1108,1110,1166-1167,1200,1202,2287,2298-2299,23021.65537e-19 6.01953e-19http://dc.g-vo.org/cars/q/cat/coverageOpticalInfraredcarsImages and data from from the CFHTLS archive research survey, a multi-band dataset spanning 37 square degrees of sky in high galactic latitudes.outputImages and data from from the CFHTLS archive research survey, a multi-band dataset spanning 37 square degrees of sky in high galactic latitudes._rDistance to cone centerdegpos.angDistancedoublenullableraj2000Right ascension of barycenter (J2000)degpos.eq.ra;meta.main33.039133.402338.5181335.428335.7191doublenullabledej2000Declination of barycenter (J2000)degpos.eq.dec;meta.main-8.45327-7.43634-3.8526152.776253.17111doublenullablesgclassS/G classifier output (0..1)src.class.starGalaxy4.62885e-050.0003019550.1763220.9788520.999911floatnullablemagautoKron-like elliptical aperture magnitudemagphot.mag10.580819.644123.809425.34833.16480.999771floatnullablemagerrautoError in Kron-like elliptical aperture magnitudemagstat.error;phot.mag2.9648e-050.002989890.0804720.177188316.1780.999771floatnullablemagapruFixed aperture magnitude in the u* bandmagphot.mag;em.opt16.168822.803525.52828.284235.56190.933742floatnullablemagaprgFixed aperture magnitude in the g' bandmagphot.mag;em.opt16.409421.612924.884426.947836.23920.985983floatnullablemagaprrFixed aperture magnitude in the r' bandmagphot.mag;em.opt15.378520.800424.419426.246535.75460.959629floatnullablemagapriFixed aperture magnitude in the i' bandmagphot.mag;em.opt16.052420.186323.915325.210335.08390.997653floatnullablemagaprzFixed aperture magnitude in the z' bandmagphot.mag;em.opt14.458819.691723.510625.791433.50170.962883floatnullablefwhmFull width half max assuming a gaussian coredegphys.angSize-0.03157460.0001595550.0002919460.0006498650.09718711floatnullablefieldkeyCARS field designationmeta.idcharnullablecutoutView the generating images in Aladin. The applet version of aladin might run out of memory for these links. The script links gives you an Aladin script for cut'n'paste.floatnullable