J/MNRAS/491/5881ivo://CDS.VizieR/J/MNRAS/491/5881doi:10.26093/cds/vizier.74915881CDSYu L.-M.Zhao B.-X.Bian W.-H.Wang C.Ge X.2024-08-20T20:15:10Z2023-04-28T14:54:14ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleiseyfert-galaxiesaccretionvisible-astronomyspectroscopyFor a compiled sample of 120 reverberation-mapped AGNs, the bivariate correlations of the broad-line region (BLR) size (R_BLR_) with the continuum luminosity at 5100{AA} (L_5100_) and the dimensionless accretion rates (dM/dt) are investigated. Using our recently calibrated virial factor f, and the velocity tracer from the H{beta} full width at half-maximum (FWHM(H{beta})) or the line dispersion ({sigma}_H{beta}_) measured in the mean spectra, three kinds of supermassive black hole (SMBH) masses and dM/dt are calculated. An extended R_BLR_(H{beta})-L_5100_ relation including dM/dt is found to be stronger than the canonical R_BLR_(H{beta})-L_5100_ relation, showing smaller scatters. The observational parameters, R_Fe_ (the ratio of optical FeII to H{beta} line flux) and the line profile parameter D_H{beta}_ (D_H{beta}_=FWHM(H{beta})/{sigma}_H{beta}_), have relations with three kinds of dM/dt. Using R_Fe_ and D_H{beta}_ to substitute dM/dt, extended empirical R_BLR_(H{beta})-L_5100_ relations are presented. R_Fe_ is a better 'fix' for the R_BLR_(H{beta})-L_5100_ offset than the H{beta} shape D_H{beta}_. The extended empirical R_BLR_(H{beta})-L_5100_ relation including R_Fe_ can be used to calculate R_BLR_, and thus the single-epoch SMBH mass M_BH_. Our measured accretion rate dependence is not consistent with the simple model of the accretion disc instability leading the BLR formation. The BLR may instead form from the inner edge of the torus, or from some other means in which BLR size is positively correlated with accretion rate and the SMBH mass.2020MNRAS.491.5881Yhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/491/5881CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJ/851/21 : SDSS RM project first year of observations (Grier+, 2017)J/ApJ/806/22 : SEAMBHs IV. H{beta} time lags (Du+, 2015)J/ApJ/856/6 : SEAMBHs IX. 10 new H{beta} light curves (Du+, 2018)J/ApJS/217/26 : Lick AGN monitoring 2011: light curves (Barth+, 2015)J/ApJ/840/97 : Optical reverberation mapping campaign of 5 AGNshttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/491/5881https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/491/5881http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/491/5881https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/491/5881https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/491/5881http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/491/5881GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/491/5881/table1 (The properties of 120 RM AGNs)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/491/5881/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/491/5881/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/491/5881/table1?GETtext/xml+votable180.050000true1.581405320.20294920.0055555555555555565/2856 6/1405 4226 4439 4754 4803 4924 5091 5262 5274 5671 5731 5776 5989 6028 6030 6087 6165 6218 6223 6260 6441 6534 6977 7061 7209 7246 7331 7642 8029 8071 8261 8528 8922 9750 10039 10454 10483 10691 10741 10743 10749 10761 10912 10927 11191 11354 11388 11402 11428 11430 11432-11433 11490 11668 11898 12380 14858 15147 16301 17727 19283 19746 19883 19932 21824 22890 23323 23418 25054 25585 25965 26148 26292 26300 26509 27862 28060 28517 28605 29795 34881 36775 38268 49042https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/491/5881?format=asciiOpticaldefaultJ/MNRAS/491/5881/table1The properties of 120 RM AGNse_logMBHsLower error on logMBHslog(solMass)stat.errorfloatlogMBHcLogarithm of the black hole mass derived from FWHM and f_BLR_{prop.to}FWHM^-1.11^log(solMass)phys.massfloatE_logMBHcUpper error on logMBHclog(solMass)stat.error;stat.maxfloate_logMBHcLower error on logMBHclog(solMass)stat.errorfloatlogMdotFLogarithm of the accretion rate associated to logMBHFphys.mass.lossfloatE_logMdotFUpper error on logMdotFstat.error;stat.maxfloate_logMdotFLower error on logMdotFstat.errorfloatlogMdotsLogarithm of the accretion rate associated to logMBHsphys.mass.lossfloatE_logMdotsUpper error on logMdotsstat.error;stat.maxfloate_logMdotsLower error on logMdotsstat.errorfloatlogMdotcLogarithm of the accretion rate associated to logMBHcphys.mass.lossfloatE_logMdotcUpper error on logMdotcstat.error;stat.maxfloate_logMdotcLower error on logMdotcstat.errorfloatNote[*] Asterisk means that the MCMC black hole mass is used to calculate the dimensionless accretion ratemeta.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.mainSimbadNameSimbad column added by the CDSmeta.idcharnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSampleSample name (SEAMBH, SDSS-RM or BentzSample)meta.id;src.samplecharNameSource namemeta.id;meta.maincharf_Name[*] Flag on Name (1)meta.codechartauRest-frame H{beta} lag (2)dtime;arith.difffloatE_tauUpper error on taudstat.error;stat.maxfloate_tauLower error on taudstat.errorfloatlogL5100Logarithm of the host-corrected monochromatic luminosity at 5100{AA} (3)log(1e-07W)phys.luminosity;em.optfloate_logL5100Error on logL5100log(1e-07W)stat.errorfloatFWHMBroad H{beta} FWHM measured from the mean spectrum (2)km/sspect.line.widthinte_FWHMError on FWHMkm/sstat.error;phys.angSizeintsigHbBroad H{beta} line dispersion {sigma}_H{beta}_ measured from the mean spectrum (2)km/sphys.veloc.dispersioninte_sigHbError on sigHbkm/sstat.errorintDHbLine profile parameter D_H{beta}_=FWHM/sigHbspect.line.width;arith.ratiofloate_DHbError on DHbstat.errorfloatRFe? Ratio of optical FeII to H{beta} line flux (4)phot.flux;arith.ratiofloatnullablee_RFe? Error on RFestat.errorfloatnullablelogMBHFLogarithm of the black hole mass derived from the FWHM and f_BLR_=1log(solMass)phys.massfloatE_logMBHFUpper error on logMBHFlog(solMass)stat.error;stat.maxfloate_logMBHFLower error on logMBHFlog(solMass)stat.errorfloatlogMBHsLogarithm of the black hole mass derived from sigHb and f_BLR_=4.47log(solMass)phys.massfloatE_logMBHsUpper error on logMBHslog(solMass)stat.error;stat.maxfloatRefReferencesmeta.refcharJ/MNRAS/491/5881/refsReferences for Table 1recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRef[1/29] Rference numbermeta.id;meta.mainintBibCodeBibCodemeta.bib.bibcodecharAutAuthor's namemeta.bib.authorcharComCommentsmeta.notechar