J/MNRAS/448/1060ivo://CDS.VizieR/J/MNRAS/448/1060doi:10.26093/cds/vizier.74481060CDSGhisellini G.Tavecchio F.2024-08-14T20:19:53Z2015-12-04T15:39:58ZCDS support team

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

cds-question@unistra.frbl-lacertae-objectsWe study the broad emission line blazars detected in the {gamma}-ray band by the Large Area Telescope onboard the Fermi satellite and with the optical spectrum studied by Shaw et al. (2012, Cat. J/ApJ/748/49, hereafter S12, and 2013, Cat. J/ApJ/764/135, hereafter S13). The observed broad line strength provides a measure of the ionizing luminosity of the accretion disc, while the {gamma}-luminosity is a proxy for the bolometric non-thermal beamed jet emission. The resulting sample, composed by 217 blazars, is the best suited to study the connection between accretion and jet properties. We compare the broad emission line properties of these blazars with those of radio-quiet and radio-loud quasars present in the Sloan Digital Sky Survey, to asses differences and similarities of the disc luminosity and the virial black hole mass. For most sources, we could derive the black hole mass by reproducing the IR-optical-UV data with a standard accretion disc spectrum, and we compared the black hole masses derived with the two methods. The distributions of the masses estimated in the two ways agree satisfactorily. We then apply a simple, one-zone, leptonic model to all the 217 objects of our sample. The knowledge of the black hole mass and disc luminosity helps to constrain the jet parameters. On average, they are similar to what found by previous studies of smaller samples of sources.2015MNRAS.448.1060Ghttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/448/1060CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJ/748/49 : Optical spectroscopy of 1LAC broad-line blazars (Shaw+, 2012)J/ApJ/764/135 : Spectroscopic redshifts of BL Lac objects (Shaw+, 2013)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/448/1060https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/448/1060http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/448/1060https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/448/1060https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/448/1060http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/448/1060GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/448/1060/tablea1 (The FSRQs in our sample)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/448/1060/tablea1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/448/1060/tablea1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/448/1060/tablea1?GETtext/xml+votable180.050000true1.1485647-47.60544560.005555555555555556Cone search capability for table J/MNRAS/448/1060/tablea2 (The BL Lac objects considered in this paper, drawn from the S13)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/448/1060/tablea2?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/448/1060/tablea2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/448/1060/tablea2?GETtext/xml+votable180.050000true3.484902819.17831060.0055555555555555566/172 438 808 911 1222 1509 2140 2234 2574 2661 2741 3024 3128 4285 4352 4394 4407 4572 4601 4820 4866 4880 4940 5139 5162 5201 5284 5353 5371 5390 5458 5775 5795 5817 5870 6101 6167 6292 6777 7045 7131 7346 7389 7426 7446 7452 7709 8199 8299 8466 8487 8699 8830 9003 9075 9442 9460 9545 9629 9633 9773 9853 9914 9998-9999 10020 10249-10250 10352 10422 10426 10466 10561 10681 10910 10971 10996 11081 11177 11242 11430 11777 11787 12173 12386 12466 12475 12599 12625 12687 12842 13352 13410 13485 13572 13729 14641 14854 15286 15761 16532 16661 16971 17186 17364 17665 17944 18092 18109 18624 18853 19023 19109 19493 19593 19622 19850 19878 19910 19918 20888 21160 21266 21358 21437 21458 21972 22305 22501 22558 22730 23383 23416 23436 23691 23897 25501 25649 26303 26340 26983 27060 27124 27243 27310 27433 28066 28083 28352 28370 28479 28492 28517 28673 29772 29925 30193 30446 30923 31430 31451 31664 31757 31844 31875 32808 32832 33549 33560 33611 33774 33825 33827 33964 34038 34086 34461 34637 34767 35119 35370 36090 36665 36708 36944 37512 38355 38766 39077 40174 41110 41335 41426 41460 41988 43246 43451 44730 44840 45081 45196 45454 45713 45943 46204 46835 46852 47512 48300https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/448/1060?format=asciidefaultJ/MNRAS/448/1060/tablea1The FSRQs in our sampleSimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameName (HHMM+DDMM), from S12meta.id;meta.maincharONameOther name, from NEDmeta.idcharzRedshiftsrc.redshiftfloatlogMHb? Black hole mass calculated through the virial method by S12 using the H{beta} linelog(solMass)phys.massfloatnullablelogMMgII? Black hole mass calculated through the virial method by S12 using the MgII linelog(solMass)phys.massfloatnullablelogMCIV? Black hole mass calculated through the virial method by S12 using the CIV linelog(solMass)phys.massfloatnullablelogMfitBlack hole mass estimated in this paper through the disc-fitting methodlog(solMass)phys.massfloatf_logMfit[)] ) for values that could not be evaluated through the disc-fitting methodmeta.codecharn_logMfitNote on logMfit (1)meta.notechar_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/MNRAS/448/1060/tablea2The BL Lac objects considered in this paper, drawn from the S13SimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameName (HHMM+DDMM), from S13meta.id;meta.maincharONameOther name, from NEDmeta.idcharzRedshiftsrc.redshiftfloatlogMfitMass used in the fitting modellog(solMass)phys.massfloat_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/MNRAS/448/1060/tablea3Parameters used to model the SEDNameName (HHMM_DDMM)meta.id;meta.maincharzRedshiftsrc.redshiftfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSampleSample (S12 or S13)src.samplecharLd45Accretion disk luminosity1e+38Wphys.luminosityfloatPpe45Power injected in the blob calculated in the comoving frame (P'e,45)1e+38Wpos.frame;obs.field;meta.modelleddoubleBMagnetic fieldGphys.magFieldfloatRdissDissipation radius in units of RSphys.size.radius;arith.ratiointGammaBulk Lorentz factor at Rdissstat.fit.paramfloatn_GammaNote on vewing angle if not set to 3 (1)meta.notechargammamaxMaximum random Lorentz factor of the injected electronsstat.fit.paramdoublegammabBreak random Lorentz factor of the injected electronsstat.fit.paramintgammapeakRandom Lorentz factor of the electrons emitting at the peak of the SEDstat.fit.paramdoublegammacoolRandom Lorentz factor of the electrons cooling in one dynamical time R=cstat.fit.paramfloatUpTotal (magnetic+radiative) energy density in the comoving frame (U')1e-07J.cm**-3phys.energy.densityfloats1Slope of the injected electron distributionstat.fit.paramfloats2Slope of the injected electron distributionstat.fit.paramfloatdM/dtinMass accretion ratesolMass/yrphys.mass.lossdoubledM/dtoutMass outflowing ratesolMass/yrphys.mass.lossdoublelogLdDisc luminosity according to S12log(solLum)phys.luminosityfloatJ/MNRAS/448/1060/tablea4Parameters for BL Lac objects in S13BMagnetic fieldGphys.magFieldfloatGammaBulk Lorentz factor at Rdissstat.fit.paramfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSampleSample (S12 or S13)src.samplecharNameName (HHMM_DDMM)meta.id;meta.maincharzRedshiftsrc.redshiftfloatLd45Accretion disk luminosity1e+38Wphys.luminosityfloatPpe45Power injected in the blob calculated in the comoving frame (P'e,45)1e+38Wpos.frame;obs.field;meta.modelleddoubleRdissDissipation radius in units of RSphys.size.radius;arith.ratiointn_GammaNote on vewing angle if not set to 3 (1)meta.notechargammamaxMaximum random Lorentz factor of the injected electronsstat.fit.paramdoublegammabBreak random Lorentz factor of the injected electronsstat.fit.paramintgammapeakRandom Lorentz factor of the electrons emitting at the peak of the SEDstat.fit.paramdoublegammacoolRandom Lorentz factor of the electrons cooling in one dynamical time R=cstat.fit.paramfloatUpTotal (magnetic+radiative) energy density in the comoving frame (U')1e-07J.cm**-3phys.energy.densityfloats1Slope of the injected electron distributionstat.fit.paramfloats2Slope of the injected electron distributionstat.fit.paramfloatdM/dtinMass accretion ratesolMass/yrphys.mass.lossdoubledM/dtoutMass outflowing ratesolMass/yrphys.mass.lossdoublelogLdDisc luminosity according to S12log(solLum)phys.luminosityfloat