J/MNRAS/492/315ivo://CDS.VizieR/J/MNRAS/492/315doi:10.26093/cds/vizier.74920315CDSGupta M.Sikora M.Rusinek K.2024-08-20T20:15:40Z2023-05-23T13:18:53ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleiaccretionradio-sourcesx-ray-sourcesinfrared-photometryultraviolet-photometryThe main objective of this work is to establish and interpret the dominant spectral components and their differences in radio-loud (RL) and radio-quiet (RQ) AGN with very massive black holes, and accreting at moderate rates. Such a sample is selected from the Swift/BAT catalogue of AGN having determined optical spectra types and hosting black holes with masses >10^8.5^M_{sun}_. We confirm our previous results, that radio loudness distribution of Swift/BAT AGN is bimodal and that radio galaxies are about two times X-ray louder than their RQ counterparts. We show that the average X-ray loudness (defined as a ratio of luminosity in the 14-195keV band to that at 12{mu}m) of Type 1 and Type 2 AGN is very similar. This similarity holds for both RL and RQ subsamples and indicates negligible dependence of the observed X-ray luminosities on the inclination angle in both populations. In both the radiative output is dominated by mid-IR and hard X-ray components, and relatively weak UV luminosities indicate large amounts of dust in polar regions.2020MNRAS.492..315Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/492/315CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJS/233/17 : Swift/BAT AGN spectroscopic survey. V. X-ray dataJ/ApJ/850/74 : Swift/BAT AGN Spectroscopic Survey. I. (Koss+, 2017)J/ApJS/207/19 : Hard X-ray survey from Swift-BAT 2004-2010VIII/65 : 1.4GHz NRAO VLA Sky Survey (NVSS) (Condon+ 1998)VIII/81B : Sydney University Molonglo Sky Survey (SUMSS V2.1)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/492/315https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/492/315http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/492/315https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/492/315https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/492/315http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/492/315GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/492/315/tabled1 (RL & RQ catalogue)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/492/315/tabled1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/492/315/tabled1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/492/315/tabled1?GETtext/xml+votable180.050000true206.535173.3480.0055555555555555566/43 406 815 879 941 953 1405 1526 1919 2004 2147 2206 2216 2251 2531 3233 3502 3771 4369 4535 4540 4589 4784 4834 5018 5097 5284 5395 5463 5996 6113 6212 6386 6502 6583 6920 6923 6928 6977 7166 7422 7502 7628 7713 7728 7815 7959 8030 8071 8216 8641 8658 8812 8845 8868 9099 9231 9375 9490 9665 9942 10141 10348 10707 10788 10847 10991 11158 11490 11615 11658 11668 11683 11898 11991 12025 12251 12254 12547 12921 13079 13179 13273 13511 13541 13707 13720 14744 14858 15135 15331 15351 16100 16184 16301 16690 16805 16853 17075 17448 17525 17548 17727 17748 17795 17814 17964 17992 18365 18402 18524 18683 18769 18794 19070 19283 19373 19433 19499 19746 19932 20079 20107 20309 20489 20556 20676 20750 21016 21186 21245 21905 21953 22365 22626 22632 22890 23167 23476 24022 24228 24288 24699 24842 24848 25035 25403 25553 25580 25619 25676 25742 25965 26071 26148 26375 26393 26509 26547 26650 26767 26861 26874 27382 27477 27504 27699 27767 27803 27815 27976 28060 28153 28259 28275 28352 28471 28545 28609 28626 30140 31401 31940 32028 32143 32279 32344 32447 32456 32658 32931 33038 33239 33282 33394 33398 33571 33716 33924 33928 33930 34190 34412 34414 34430 34499 34531 34669 34726 34768 34812 34881 34907 34983 35038 35085 35246 35263 35608 35741 35934 36005 36158 36216 36382 36396 36595 36786 36890 37054 38113 38129 38205 38479 38704 38923 38948 39149 39295 39322 39717 39722 39778 40838 41014 41087 41499 41982 42012 42179 43452 43634 43667 43695 43768 43877 43983 44448 44507 44517 44526 44551 44790 45220 45222 45258 45446 45500 45985 46005 46101 46281 46544 47027 47064 47074 47169 47308 47971 48022 48394 48491 48614 48798 49042https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/492/315?format=asciiX-rayUVInfraredRadiodefaultJ/MNRAS/492/315/tabled1RL & RQ catalogueNameAGN name from Swift/BAT cataloguemeta.id;meta.maincharSimbadNameSimbad column added by the CDSmeta.idcharnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right ascension (J2000)degpos.eq.ra;meta.mainDEJ2000Declination (J2000)degpos.eq.dec;meta.mainzRedshiftsrc.redshiftdoublelogRLogarithm of the radio loudnessphys.luminosity;arith.ratiodoubleRClassRadio classification of object (1)meta.code.classcharOTypeOptical classificationmeta.code.classcharlogMBHLogarithm of the black hole mass determined from K-band luminositylog(solMass)phys.massdoublelogEdd? Logarithm of the Eddington ratiophys.luminosity;arith.ratiodoublenullablelogNHLogarithm of the Hydrogen column densitylog(cm**-2)phys.columnDensityfloatlogLW1Logarithm of WISE W1 luminositylog(1e-07W)phys.luminosity;em.IRdoublelogLW2Logarithm of WISE W2 luminositylog(1e-07W)phys.luminosity;em.IRdoublelogLW3Logarithm of WISE W3 luminositylog(1e-07W)phys.luminosity;em.IR.8-15umdoublelogLW4Logarithm of WISE W4 luminositylog(1e-07W)phys.luminosity;em.IR.15-30umdoublelogLJLogarithm of 2MASS J-band luminositylog(1e-07W)phys.luminosity;em.IR.JdoublelogLHLogarithm of 2MASS H-band luminositylog(1e-07W)phys.luminosity;em.IR.HdoublelogLKLogarithm of 2MASS K-band luminositylog(1e-07W)phys.luminosity;em.IR.KdoublelogLFUVLogarithm of GALEX FUV luminositylog(1e-07W)phys.luminosity;em.UVdoublen_logLFUV[Yes/No ] Indicates if logLFUV is an upper limitmeta.notecharlogLNUVLogarithm of GALEX NUV luminositylog(1e-07W)phys.luminosity;em.UVdoublen_logLNUV[Yes/No ] Indicates if logLNUV is an upper limitmeta.notecharlogL2keVLogarithm of the X-ray luminosity in the 2-10keV bandlog(1e-07W)phys.luminosity;em.X-rayfloatlogL14keVLogarithm of the X-ray luminosity in the 14-195keV bandlog(1e-07W)phys.luminosity;em.X-rayfloatGammaPhoton index in the X-ray band 14-195 keVinstr.bandpassfloat