J/ApJ/690/20ivo://CDS.VizieR/J/ApJ/690/20doi:10.26093/cds/vizier.16900020CDSShankar F.Weinberg D.H.Miralda-Escude J.2017-06-22T14:29:32Z2011-03-07T12:37:19ZCDS support team

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

cds-question@unistra.frstellar-evolutionary-modelsactive-galactic-nucleiredshiftedWe construct evolutionary models of the populations of active galactic nuclei (AGNs) and supermassive black holes, in which the black hole mass function grows at the rate implied by the observed luminosity function, given assumptions about the radiative efficiency and the luminosity in Eddington units. We draw on a variety of recent X-ray and optical measurements to estimate the bolometric AGN luminosity function and compare to X-ray background data and the independent estimate of Hopkins et al. to assess remaining systematic uncertainties. The integrated AGN emissivity closely tracks the cosmic star-formation history, suggesting that star formation and black hole growth are closely linked at all redshifts.2009ApJ...690...20Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/690/20CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/ApJ/667/131 : Mass function of active black holes (Greene+, 2007)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/690/20https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/690/20http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/690/20https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/690/20https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/690/20http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/690/20GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/ApJ/690/20/table2AGN bolometric luminosity functionsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzRedshiftsrc.redshiftfloatlogLLog of the luminosity in units of erg/slog(1e-07W)phys.luminosityfloatlogFLog reference bolometric AGN luminosity function log{Phi}log(Mpc**-3)phys.luminosity.funfloatlogFnoCtLog reference bolometric AGN luminosity function with no Compton-thick sources (G1)log(Mpc**-3)phys.luminosity.funfloatlogFdCtLog reference bolometric AGN luminosity function with double Compton-thick sources (G2)log(Mpc**-3)phys.luminosity.funfloatlogFHRHLog reference bolometric AGN luminosity function from Hopkins et al. 2007ApJ...654..731Hlog(Mpc**-3)phys.luminosity.funfloatJ/ApJ/690/20/bhBlack Hole mass functions and duty cycleszRedshiftsrc.redshiftfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlogMLog of black hole masslog(solMass)phys.massfloatlogFLog reference black hole mass function log{Phi}log(Mpc**-3)phys.luminosity.funfloatlogFnoCtLog reference black hole mass function with no Compton-thick sources (G1)log(Mpc**-3)phys.luminosity.funfloatlogFdCtLog reference black hole mass function with double Compton-thick sources (G2)log(Mpc**-3)phys.luminosity.funfloatlogFHRHLog reference black hole mass function with HRH07 luminosity function (G3)log(Mpc**-3)phys.luminosity.funfloatlogFExtLog reference black hole mass function with modified HRH07 (G4)log(Mpc**-3)phys.luminosity.funfloatPo[0,1] Duty cycle for reference model (1)stat.fit.paramdoublePonoCtDuty cycle for reference model with no Compton-thick sources (G1)stat.fit.paramdoublePodCtDuty cycle for reference model with double Compton-thick sources (G2)stat.fit.paramdoublePoHRH07Duty cycle for reference model with HRH07 luminosity function (G3)stat.fit.paramdoublePoExtDuty cycle for reference model with modified HRH07 luminosity function (G4)stat.fit.paramdouble