J/A+A/590/A80ivo://CDS.VizieR/J/A+A/590/A80doi:10.26093/cds/vizier.35900080CDSRanalli P.Koulouridis E.Georgantopoulos I.Fotopoulou S.Hsu L.-T.,Salvato M.Comastri A.Pierre M.Cappelluti N.Carrera F.J.,Chiappetti L.Clerc N.Gilli R.Iwasawa K.Pacaud F.Paltani S.,Plionis E.Vignali C.2016-05-16T15:01:27Z2016-05-16T16:00:56ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleix-ray-sourcesastronomical-modelsThe XMM-Large scale structure (XMM-LSS), XMM-Cosmological evolution survey (XMM-COSMOS), and XMM-Chandra deep field south (XMM-CDFS) surveys are complementary in terms of sky coverage and depth. Together, they form a clean sample with the least possible variance in instrument effective areas and point spread function. Therefore this is one of the best samples available to determine the 2-10keV luminosity function of active galactic nuclei (AGN) and their evolution. The samples and the relevant corrections for incompleteness are described. A total of 2887 AGN is used to build the LF in the luminosity interval 10^42^-10^46^erg/s and in the redshift interval 0.001-4. A new method to correct for absorption by considering the probability distribution for the column density conditioned on the hardness ratio is presented.2016A&A...590A..80Rhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/590/A80CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/590/A80https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/590/A80http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/590/A80https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/590/A80https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/590/A80http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/590/A80GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapX-raydefaultJ/A+A/590/A80/lade-lLF samples from XMM-LSS, LADE modelnormNormalisation (1)stat.fit.paramdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintgamma1Exponent of the first branch of the power-lawarith.factordoublegamma2Exponent of the second branch of the power-lawarith.factordoubleLstarKnee luminosity of the LFlog(1e-07W)phys.luminositydoublezcCritical redshiftsrc.redshiftdoublep1First luminosity evolution slopephys.luminosity.fundoublep2Second luminosity evolution slopephys.luminosity.fundoubledDensity evolution slopestat.fit.paramdoubleJ/A+A/590/A80/lade-lckLF samples from all surveys together, LADE modelrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintnormNormalisation (1)stat.fit.paramdoublegamma1Exponent of the first branch of the power-lawarith.factordoublegamma2Exponent of the second branch of the power-lawarith.factordoubleLstarKnee luminosity of the LFlog(1e-07W)phys.luminositydoublezcCritical redshiftsrc.redshiftdoublep1First luminosity evolution slopephys.luminosity.fundoublep2Second luminosity evolution slopephys.luminosity.fundoubledDensity evolution slopestat.fit.paramdoubleJ/A+A/590/A80/ldde-cLF samples from XMM-CDFS, LDDE modelrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintnormNormalisation (1)stat.fit.paramdoublegamma1Exponent of the first branch of the power-lawarith.factordoublegamma2Exponent of the second branch of the power-lawarith.factordoubleLstarKnee luminosity of the LFlog(1e-07W)phys.luminositydoublezcCritical redshiftsrc.redshiftdoublep1First luminosity evolution slopephys.luminosity.fundoublep2Second luminosity evolution slopephys.luminosity.fundoubledDensity evolution slopestat.fit.paramdoubleJ/A+A/590/A80/ldde-kLF samples from XMM-COSMOS, LDDE modelrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintnormNormalisation (1)stat.fit.paramdoublegamma1Exponent of the first branch of the power-lawarith.factordoublegamma2Exponent of the second branch of the power-lawarith.factordoubleLstarKnee luminosity of the LFlog(1e-07W)phys.luminositydoublezcCritical redshiftsrc.redshiftdoublep1First luminosity evolution slopephys.luminosity.fundoublep2Second luminosity evolution slopephys.luminosity.fundoubledDensity evolution slopestat.fit.paramdoubleJ/A+A/590/A80/ldde-lLF samples from XMM-LSS, LDDE modelrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintnormNormalisation (1)stat.fit.paramdoublegamma1Exponent of the first branch of the power-lawarith.factordoublegamma2Exponent of the second branch of the power-lawarith.factordoubleLstarKnee luminosity of the LFlog(1e-07W)phys.luminositydoublezcCritical redshiftsrc.redshiftdoublep1First luminosity evolution slopephys.luminosity.fundoublep2Second luminosity evolution slopephys.luminosity.fundoubledDensity evolution slopestat.fit.paramdoubleJ/A+A/590/A80/ldde-lckLF samples from all surveys together, LDDE modelrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintnormNormalisation (1)stat.fit.paramdoublegamma1Exponent of the first branch of the power-lawarith.factordoublegamma2Exponent of the second branch of the power-lawarith.factordoubleLstarKnee luminosity of the LFlog(1e-07W)phys.luminositydoublezcCritical redshiftsrc.redshiftdoublep1First luminosity evolution slopephys.luminosity.fundoublep2Second luminosity evolution slopephys.luminosity.fundoubledDensity evolution slopestat.fit.paramdoubleJ/A+A/590/A80/lade-cLF samples from XMM-CDFS, LADE modelrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintnormNormalisation (1)stat.fit.paramdoublegamma1Exponent of the first branch of the power-lawarith.factordoublegamma2Exponent of the second branch of the power-lawarith.factordoubleLstarKnee luminosity of the LFlog(1e-07W)phys.luminositydoublezcCritical redshiftsrc.redshiftdoublep1First luminosity evolution slopephys.luminosity.fundoublep2Second luminosity evolution slopephys.luminosity.fundoubledDensity evolution slopestat.fit.paramdoubleJ/A+A/590/A80/lade-kLF samples from XMM-COSMOS, LADE modelzcCritical redshiftsrc.redshiftdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintnormNormalisation (1)stat.fit.paramdoublegamma1Exponent of the first branch of the power-lawarith.factordoublegamma2Exponent of the second branch of the power-lawarith.factordoubleLstarKnee luminosity of the LFlog(1e-07W)phys.luminositydoublep1First luminosity evolution slopephys.luminosity.fundoublep2Second luminosity evolution slopephys.luminosity.fundoubledDensity evolution slopestat.fit.paramdouble