J/A+A/666/A11ivo://CDS.VizieR/J/A+A/666/A11doi:10.26093/cds/vizier.36660011CDSPapadakis I.E.Dovciak M.Kammoun E.S.2023-07-03T14:12:38Z2022-09-27T10:58:05ZCDS support team

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

cds-question@unistra.fraccretionactive-galactic-nucleiastronomical-modelsWe present the results of a study of the half-light radius-vs-black hole mass and the luminosity-vs-black hole mass relations in active galactic nuclei (AGN), when the disc is illuminated by the X-ray corona. We use KYNSED, which is a recently developed spectral model for the broad-band spectral energy distribution in AGN. We consider non-illuminated Novikov-Thorne discs, and X-ray illuminated discs with a Novikov-Thorne temperature radial profile, and a temperature profile modified by a colour correction factor. We assume that the X-ray luminosity is equal to the accretion power that is dissipated to the disc below a transition radius, and we compute the half-light radius and the disc luminosity for many black hole masses, and a wide range of accretion rates, black hole spins, X-ray corona luminosity and height. Non-illuminated discs are not consistent with the observations, while X-ray illuminated discs can explain both the half-light radius veresus black hole mass and the luminosity versus black hole mass relation in AGN, for a wide range of physical parameters. X-ray illuminated discs can explain the data if we observe the gravitationally lensed quasars mainly face-on, but also if the mean inclination angle is 60 degrees.2022A&A...666A..11Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/666/A11CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/666/A11https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/666/A11http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/666/A11https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/666/A11https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/666/A11http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/666/A11GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapdefaultJ/A+A/666/A11/table4The half-light radius datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintAllDisplay Half-light radius and Luminosity at 3000{AA} for model parametersmeta.ref.urlcharBHMBlack hole mass (0.32, 1.00, 3.16, 10.00 or 31.60)1e+08solMassphys.massfloatInclInclination (30 or 60)degsrc.orbital.inclinationintSpinBlack hole mass spin (0.00, 0.30, 0.50, 0.80 or 1.00)stat.paramfloatMdotAccretion rate in Eddington units (0.05, 0.10, 0.20, 0.30, 0.50 or 0.80)arith.ratefloatRtrTransition radius (in Risco) (1.00, 1.50, 2.00, 3.00, 6.00 or 12.00)phys.size.radius;arith.ratiofloatHeightCorona height, in Rg (0 for non illuminated disc) (0.00, 5.00, 10.00, 20.00, 40.00, 60.00, 80.00 or 100.00)pos.cartesian.zfloatR1/2-NTHalf-light radius for non illuminated NT discs1e+14cmphys.size.radiusfloatR1/2-NT+fcolHalf-light radius for non illuminated NT discs with colour correction1e+14cmphys.size.radiusfloatR1/2-NT/XHalf-light radius for illuminated NT discs1e+14cmphys.size.radiusfloatR1/2-NT/X+fcolHalf-light radius for illuminated NT discs with colour correction1e+14cmphys.size.radiusfloatJ/A+A/666/A11/table5The luminosity datarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintAllDisplay Half-light radius and Luminosity at 3000{AA} for model parametersmeta.ref.urlcharBHMBlack hole mass (0.32, 1.00, 3.16, 10.00 or 31.60)1e+08solMassphys.massfloatInclInclination (30 or 60)degsrc.orbital.inclinationintSpinBHM spin (0.00, 0.30, 0.50, 0.80 or 1.00)stat.paramfloatMdotAccretion rate in Eddington units (0.05, 0.10, 0.20, 0.30, 0.50 or 0.80)arith.ratefloatRtrTransition radius (in Risco) (1.00, 1.50, 2.00, 3.00, 6.00 or 12.00)phys.size.radius;arith.ratiofloatHeightCorona height, in Rg (0 for non illuminated disc) (0.00, 5.00, 10.00, 20.00, 40.00, 60.00, 80.00 or 100.00)pos.cartesian.zfloatlog(L-NT)Logarithm of Luminosity at 3000{AA} of non-illuminated NT discslog(1e-07W)phys.luminosityfloatlog(L-NT+fcol)Logarithm of Luminosity at 3000{AA} of non-illuminated NT discs with colour correctionlog(1e-07W)phys.luminosityfloatlog(L-NT/X)Logarithm of Luminosity at 3000{AA} of illuminated NT discslog(1e-07W)phys.luminosityfloatlog(L-NT/X+fcol)Logarithm of Luminosity at 3000{AA} of illuminated NT discs with colour correctionlog(1e-07W)phys.luminosityfloat