J/A+A/535/A80ivo://CDS.VizieR/J/A+A/535/A80doi:10.26093/cds/vizier.35350080CDSMainieri V.Bongiorno A.Merloni A.Aller M.Carollo M.Iwasawa K.,Koekemoer A.M.Mignoli M.Silverman J.D.Bolzonella M.Brusa M.,Comastri A.Gilli R.Halliday C.Ilbert O.Lusso E.Salvato M.,Vignali C.Zamorani G.Contini T.Kneib J.-P.Le Fevre O.Lilly S.,Renzini A.Scodeggio M.Balestra I.Bardelli S.Caputi K.Coppa G.,Cucciati O.De La Torre S.De Ravel L.Franzetti P.Garilli B.,Iovino A.Kampczyk P.Knobel C.Kovac K.Lamareille F.,Le Borgne J.-F.Le Brun V.Maier C.Nair P.Pello R.Peng Y.,Perez Montero E.Pozzetti L.Ricciardelli E.Tanaka M.Tasca L.,Tresse L.Vergani D.Zucca E.Aussel H.Capak P.Cappelluti N.,Elvis M.Fiore F.Hasinger G.Impey C.Le Floc'h E.Scoville N.,Taniguchi Y.Trump J.2017-12-05T05:09:51Z2012-03-16T15:03:12ZCDS support team

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

cds-question@unistra.frquasarsx-ray-sourcesgalaxy-classification-systemsWe explore the connection between black hole growth at the center of obscured quasars selected from the XMM-COSMOS survey and the physical properties of their host galaxies. We study a bolometric regime (<Lbol>=8x10^45^erg/s) where several theoretical models invoke major galaxy mergers as the main fueling channel for black hole accretion. To derive robust estimates of the host galaxy properties, we use an SED fitting technique to distinguish the AGN and host galaxy emission. We evaluate the effect on galaxy properties estimates of being unable to remove the nuclear emission from the SED. The superb multi-wavelength coverage of the COSMOS field allows us to obtain reliable estimates of the total stellar masses and star formation rates (SFRs) of the hosts. We supplement this information with a morphological analysis of the ACS/HST images, optical spectroscopy, and an X-ray spectral analysis.2011A&A...535A..80Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/535/A80CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJS/172/29 : XMM-Newton survey in COSMOS field. I. (Hasinger+, 2007)J/A+A/497/635 : XMM-Newton wide-field survey in COSMOS field (Cappelluti+ 2009)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/535/A80https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/535/A80http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/535/A80https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/535/A80https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/535/A80http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/535/A80GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/535/A80/table1 (SED of type-2 QSOs)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/535/A80/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/535/A80/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/535/A80/table1?GETtext/xml+votable180.050000true150.105552.126360.0055555555555555565/6814 6/27245 27247 27344https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/535/A80?format=asciiX-rayOpticaldefaultJ/A+A/535/A80/table1SED of type-2 QSOsCOSMOSDisplay the XMMC datameta.ref.urlcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintMSimbad column added by the CDSmeta.ref.urlcharXMMCXMMC designationmeta.id;meta.mainintprimaryn_XMMC[a-f] Individual note (1)meta.notecharlogLXX-ray luminosity in the 0.5-10keV bandlog(1e-07W)phys.luminosity;em.X-rayfloatlogNHHydrogen column densitylog(cm**-2)phys.columnDensityfloatB_logNH? Upper limit for logNHlog(cm**-2)phys.columnDensity;stat.maxfloatnullableb_logNHLower limit for logNHlog(cm**-2)phys.columnDensity;stat.minfloatzRedshiftsrc.redshiftfloatf_z[sp] spectroscopic or photometric redshiftmeta.codecharlogM*? Stellar masslog(solMass)phys.massfloatnullableB_logM*? Upper limit on logM*log(solMass)phys.mass;stat.maxfloatnullableb_logM*? Lower limit on logM*log(solMass)phys.mass;stat.minfloatnullableSFR? Stellar formation ratesolMass/yrarith.rate;phys.SFRfloatnullableB_SFR? Upper limit on SFRsolMass/yrphys.SFR;stat.maxfloatnullableb_SFR? Lower limit on SFRsolMass/yrphys.SFR;stat.minfloatnullableUMAG? Absolute U magnitude in AB systemmagphys.magAbsfloatnullableBMAG? Absolute B magnitude in AB systemmagphys.magAbsfloatnullableSimbadSimbad column added by the CDSchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainJ/A+A/535/A80/table2Morphological parameters of type-2 QSO hosts at z<=1.2recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintXMMCXMMC designationmeta.id;meta.mainintzRedshiftsrc.redshiftfloatImagI magnitude (in AB system)magphot.mag;em.opt.IfloatClass[1/3] Classification code (1)meta.code.classintr1/2Half-light radius (1pix=0.03")pixphys.angSize;srcfloatRpPetrosian radius (1pix=0.03")pixphys.angSize;srcfloatepsEllipticitysrc.ellipticityfloatCConcentration indexmeta.code;spect.indexfloatAAsymmetry indexmeta.code;spect.indexfloatGGini coefficient (2)stat.fit.paramfloatM20M20 index (3)stat.fit.paramfloat