J/ApJ/881/154ivo://CDS.VizieR/J/ApJ/881/154doi:10.26093/cds/vizier.18810154CDSPaliya V.S.Koss M.Trakhtenbrot B.Ricci C.Oh K.Ajello M.Stern D.,Powell M.C.Urry C.M.Harrison F.Lamperti I.Mushotzky R.,Marcotulli L.Mejia-Restrepo J.Hartmann D.2021-07-05T07:47:48Z2021-02-15T10:21:44ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleigamma-ray-astronomyx-ray-sourcesredshiftedmagnetic-fieldsvisible-astronomyspectroscopyThe recently released 105-month Swift-Burst Alert Telescope (BAT) all-sky hard X-ray survey catalog presents an opportunity to study astrophysical objects detected in the deepest look at the entire hard X-ray (14-195keV) sky. Here we report the results of a multifrequency study of 146 blazars from this catalog, quadrupling the number compared to past studies, by utilizing recent data from the Fermi-Large Area Telescope (LAT), Swift-BAT, and archival measurements. In our {gamma}-ray analysis of ~10yr of the LAT data, 101 are found as {gamma}-ray emitters, whereas, 45 remains LAT undetected. We model the broadband spectral energy distributions with a synchrotron-inverse Compton radiative model. On average, BAT detected sources host massive black holes (M_bh_~10^9^M_{sun}_) and luminous accretion disks (L_d_~10^46^erg/s). At high redshifts (z>2), BAT blazars host more powerful jets with luminous accretion disks compared to those detected only with Fermi-LAT. We find good agreement in the black hole masses derived from the single-epoch optical spectroscopic measurements and standard accretion disk modeling approaches. Other physical properties of BAT blazars are similar to those known for Fermi-LAT detected objects.2019ApJ...881..154Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/881/154CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toVIII/40 : GB6 catalog of radio sources (Gregory+ 1996)VII/258 : Quasars and Active Galactic Nuclei (13th Ed.) (Veron+ 2010)VII/274 : The Roma BZCAT - 5th edition (Massaro+, 2015)J/AJ/130/896 : SUMSS Giant Radio Sources (Saripalli+, 2005)J/ApJS/171/61 : All-Sky Survey of Flat-Spectrum Radio Sources (Healey+, 2007)J/ApJ/699/603 : Evolution of Swift/BAT blazars (Ajello+, 2009)J/ApJ/716/30 : SED of Fermi bright blazars (Abdo+, 2010)J/ApJS/194/45 : QSO properties from SDSS-DR7 (Shen+, 2011)J/ApJ/748/49 : Optical spectroscopy of 1LAC broad-line blazars (Shaw+, 2012)J/other/RMxAA/48.9 : Opt. spec. atlas of MOJAVE AGNs (Torrealba+, 2012)J/ApJ/764/135 : Spectroscopic redshifts of BL Lac objects (Shaw+, 2013)J/ApJ/780/73 : Redshifts of BL Lac objects from Fermi (Ajello+, 2014)J/other/Nat/515.376 : Power of relativistic jets in blazars (Ghisellini+, 2014)J/ApJS/218/23 : Fermi LAT third source catalog (3FGL) (Acero+, 2015)J/ApJ/850/74 : Swift/BAT AGN Spectroscopic Survey. I. (Koss+, 2017)J/ApJ/851/33 : Multi-wavelength analysis of CGRaBS blazars (Paliya+, 2017)J/ApJS/233/17 : Swift/BAT AGN spectroscopic survey. V. X-ray (Ricci+, 2017)J/ApJS/235/4 : The 105-month Swift-BAT all-sky hard X-ray survey (Oh+, 2018)http://www.bass-survey.com/ : BASS project home pagehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/881/154https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/881/154http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/881/154https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/881/154https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/881/154http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/881/154GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/881/154/blazars (The SED parameters associated with the modeling of the broadband emission of BAT blazars (Table 4) and various jet powers (Table 5))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/881/154/blazars?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/881/154/blazars?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/881/154/blazars?GETtext/xml+votable180.050000true2.6161940510.969251990.0055555555555555566/325 611 615 893 967 1546 1696 1699 1782 2091 2273 2549 3023 3431 3724 3886 4027 4114 5423 5597 6013 6021 6167 6477 6988 7038 7233 7518 7709 7896 7969 8057 8858 8945 9612 9633 9723 9821 10598 10605 10895 11091 11160 12047 12117 12162 12632 12921 12973 13359 13496 13820 13927 14068 14608 14641 14737 15067 15218 15969 16027 16093 16447 16962 17471 17785 17890 18624 19190 19307 19398 19566 19622 19996 20099 20156 20309 20624 20657 21020 21142 21758 22066 22658 22659 24084 24571 25132 25302 25630 25742 25818 26131 26292 26297 26303 26543 27039 27815 28083 28479 28517 28538 28618 29072 31211 31399 32961 33164 33460 33583 33611 33795 34099 34123 34264 34517 34572 35706 35875 36342 37190 37388 38128 38916 40332 40351 40527 41135 41938 42822 42901 43105 44908 45178 45738 46055 46280 46924 47016 47375 48023 48610 48676 48712 48846https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/881/154?format=asciiGamma-rayX-rayOpticaldefaultJ/ApJ/881/154/blazarsThe SED parameters associated with the modeling of the broadband emission of BAT blazars (Table 4) and various jet powers (Table 5)SimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGDisplay the gamma-ray spectral parameters from Fermi-LAT (link to Table 3)meta.ref.urlcharNameSource identifiermeta.id;meta.maincharprimaryz[0.03/4.71] Redshiftsrc.redshiftfloattheta[0.7/6] Viewing angledegpos.posAngfloatlogMbh[0/10.04] log scale black hole mass (1)log(solMass)instr.scalefloatn_logMbhMethod used to derive logMbh (2)meta.notecharlogLd[0/48] log scale accretion disk luminosity (1)log(1e-07W)phys.luminosityfloatRdis[0.006/0.8] Dissipation distancepcpos.distancefloatRblr[0/1.1] Broad Line Region sizepcphys.size;spect.line;obs.fieldfloatdelta[8.6/28.1] Doppler factorspect.dopplerParamfloatGamma[5/19] Bulk Lorentz factorstat.fit.paramintB[0.1/3.2] Magnetic field in Gauss0.0001Tphys.magFieldfloatp[1.2/2.4] Spectral index before break energy (3)spect.indexfloatq[3.3/6] Spectral index after break energy (3)spect.indexfloatgammaMin[1/500] Minimum Lorentz factor (4)arith.factor;stat.minintgammab[12/1056773] Break Lorentz factor (4)arith.factorintgammaMax[700/5000000] Maximum Lorentz factor (4)arith.factor;stat.maxfloatlogUe[-3.3/-0.13] log scale particle energy density in units of erg/cm^3^log(1e-07J.cm**-3)phys.energy.densityfloatCD[0.1/363] Compton dominancestat.fit.paramfloatlogPe[42.16/45.81] log electron power (5)log(1e-07W)phys.luminosity;phys.electronfloatlogPm[41.8/46.7] log magnetic power (5)log(1e-07W)phys.magFieldfloatlogPr[42.8/48.1] log radiative power (5)log(1e-07W)phys.luminosityfloatlogPp[42.7/48.5] log proton power (5)log(1e-07W)phys.luminosityfloatlogPj[43/48.5] log total power; sum of Pe, Pm, and Pp (5)log(1e-07W)phys.luminosityfloatK17Display data from Koss+, 2017, J/ApJ/850/74meta.ref.urlintnullable_RAPositions from the 105-month Swift-BAT (Oh+, 2018, J/ApJS/235/4) (right ascension part)degpos.eq.ra;meta.main_DEPositions from the 105-month Swift-BAT (Oh+, 2018, J/ApJS/235/4) (declination part)degpos.eq.dec;meta.mainJ/ApJ/881/154/table3The {gamma}-ray spectral parameters of Fermi-LAT detected BAT blazarsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameSource identifiermeta.id;meta.maincharFlux[1.2e-6/0.0004] The 0.1-300GeV energy fluxMeV.cm**-2.s**-1phot.flux.density;em.gamma.harddoublee_Flux[2e-7/6.6e-6] Uncertainty in FluxMeV.cm**-2.s**-1stat.error;phot.fluxdoubleGamma[1.27/3.43] The 0.1-300GeV {Gamma} value (1)stat.fit.paramfloate_Gamma[0.01/0.3] Uncertainty in Gammastat.errorfloatBeta[0/0.5] log parabola model curvature parameterstat.fit.paramfloate_Beta[0/0.12] Uncertainty in Betastat.errorfloatTS[29.7/278383] Test statistic from likelihood fittingstat.likelihooddouble