J/A+A/467/73ivo://CDS.VizieR/J/A+A/467/73doi:10.26093/cds/vizier.34670073CDSTajer M.Polletta M.Chiappetti L.Maraschi L.Trinchieri G.,Maccagni D.Andreon S.Garcet O.Surdej J.Pierre M.Le Fevre O.,Franceschini A.Lonsdale C.J.Surace J.A.Shupe D.L.Fang F.,Rowan-Robinson M.Smith H.E.Tresse L.2007-11-07T21:49:21Z2007-11-07T22:43:58ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frsurveysactive-galactic-nucleix-ray-sourcesinfrared-sourcesredshiftedinfrared-photometryvisible-astronomybroad-band-photometryOur goal is to probe the populations of obscured and unobscured AGN investigating their optical-IR and X-ray properties as a function of X-ray flux, luminosity and redshift within a hard X-ray selected sample with wide multiwavelength coverage. We selected a sample of 136 X-ray sources detected at a significance of >=3{sigma} in the 2-10keV band (F_2-10_>~10^-14^erg/cm^2^/s) in a ~1deg^2^ area in the XMM Medium Deep Survey (XMDS, Cat. <J/A+A/439/413>). The XMDS area is covered with optical photometry from the VVDS and CFHTLS surveys and infrared Spitzer data from the SWIRE survey. Based on the X-ray luminosity and X-ray to optical ratio, 132 sources are likely AGN, of which 122 have unambiguous optical - IR identification. The observed optical and IR spectral energy distributions of all identified sources are fitted with AGN/galaxy templates in order to classify them and compute photometric redshifts. X-ray spectral analysis is performed individually for sources with a sufficient number of counts and using a stacking technique for subsamples of sources at different flux levels. Hardness ratios are used to estimate X-ray absorption in individual weak sources.2007A&A...467...73Thttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/467/73CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toIII/250 : The VIMOS VLT deep survey (VVDS-DEEP) (Le Fevre+ 2005)J/A+A/461/81 : Galaxy clusters in the CFHTLS (Olsen+, 2007)J/A+A/403/857 : VLA-VIRMOS Deep Field (Bondi+, 2003)J/ApJ/591/640 : XMM-LSS low-frequency radio counterparts (Cohen+, 2003)J/A+A/439/413 : XMDS/VVDS 4{sigma} catalogue (Chiappetti+, 2005)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/467/73https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/467/73http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/467/73https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/467/73https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/467/73http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/467/73GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/467/73/tablea1 (The 3{sigma} hard sample)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/467/73/tablea1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/467/73/tablea1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/467/73/tablea1?GETtext/xml+votable180.050000true36.33782917-4.663465560.0055555555555555566/17683 17686 17689 17692 17694https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/467/73?format=asciiX-rayOpticalInfrareddefaultJ/A+A/467/73/tablea1The 3{sigma} hard samplerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSeqSequential number, XMDS NNNN in Simbadmeta.recordintXMDSXMDS designation (JHHMMSS.s+DDMMSS)meta.id;meta.maincharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainF2-10keVFlux in the 2-10keV band1e-17W.m**-2phot.flux;em.X-ray.mediumfloatHRHardness ratio between the 2-10 and 0.5-2keV bandsphot.flux;em.X-ray.soft;arith.ratiofloatX-O? Distance between the X-ray and optical VVDS positionsarcsecpos;arith.difffloatnullableBmag? VVDS B magnitude (in AB system)magfloatnullableImag? VVDS I magnitude (in AB system)magfloatnullableCol[BR-] Color classification (1)src.class.colorchari'mag? CFHTLS i' magnitude (in AB system)magphot.mag;em.opt.IfloatnullableF3.6um? SWIRE flux at 3.6umuJyphot.flux.density;em.IR.3-4umintnullablel_F24umLimit flag on F24ummeta.code.errorcharF24um? SWIRE flux at 24umuJyphot.flux.density;em.IR.15-30umintnullablezsp? Spectroscopic redshiftsrc.redshiftfloatnullablezph? Photometric redshiftsrc.redshiftfloatnullableTypeSED classificationsrc.classcharlogLX? Absorption corrected X-ray luminosity in the 2-10keV bandlog(1e-07W)phys.luminosity;em.X-rayfloatnullable