J/MNRAS/488/1519ivo://CDS.VizieR/J/MNRAS/488/1519doi:10.26093/cds/vizier.74881519CDSYu L.-M.Bian W.-H.Wang C.Zhao B.-X.Ge X.2024-08-19T20:19:26Z2023-02-02T14:33:45ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleiquasarsseyfert-galaxiesgalaxy-kinematicsvisible-astronomyspectroscopynarrow-band-photometryatomic-spectroscopyUsing a compiled sample of 34 broad-line active galactic nuclei (AGNs) with measured H{beta} time lags from the reverberation mapping (RM) method and measured bulge stellar velocity dispersions {sigma}_*_, we calculate the virial factor f by assuming that the RM AGNs intrinsically obey the same M_BH_-{sigma}_*_ relation as quiescent galaxies, where M_BH_ is the mass of the supermassive black hole (SMBH). Considering four tracers of the velocity of the broad-line regions (BLRs), i.e. the H{beta} line width or line dispersion from the mean or rms spectrum, there are four kinds of the factor f. Using the H{beta} full width at half-maximum (FWHM) to trace the BLRs velocity, we find significant correlations between the factor f and some observational parameters, e.g. FWHM, the line dispersion. Using the line dispersion to trace the BLRs velocity, these relations disappear or become weaker. It implies the effect of inclination in BLRs geometry. It also suggests that the variable f in M_BH_ estimated from luminosity and FWHM in a single-epoch spectrum is not negligible. Using a simple model of thick-disc BLRs, we also find that, as the tracer of the BLRs velocity, H{beta} FWHM has some dependence on the inclination, while the line dispersion {sigma}_H{beta}_ is insensitive to the inclination. Considering the calibrated FWHM-based factor f from the mean spectrum, the scatter of the SMBH mass is 0.39dex for our sample of 34 low-redshift RM AGNs. For a high-redshift sample of 30 Sloan Digital Sky Survey RM AGNs with measured stellar velocity dispersions, we find that the SMBH mass scatter is larger than that for our sample of 34 low-redshift RM AGNs. It implies the possibility of evolution of the M_BH_-{sigma}_*_ relation from high-redshift to low-redshift AGNs.2019MNRAS.488.1519Yhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/488/1519CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/488/1519https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/488/1519http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/488/1519https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/488/1519https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/488/1519http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/488/1519GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/488/1519/table1 (The low-z RM AGNs with measured {sigma}_*_ for the calibration of f)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/488/1519/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/488/1519/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/488/1519/table1?GETtext/xml+votable180.050000true68.29623195.35433860.005555555555555556Cone search capability for table J/MNRAS/488/1519/table2 (The high-z RM AGNs observed by SDSS with measured {sigma}_*_)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/488/1519/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/488/1519/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/488/1519/table2?GETtext/xml+votable180.050000true213.3511453.09081220.005555555555555556Cone search capability for table J/MNRAS/488/1519/table6 (The factor f derived from the BLRs dynamical model, X-ray variability, resolved Pa {alpha} emission region for 19 AGNs)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/488/1519/table6?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/488/1519/table6?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/488/1519/table6?GETtext/xml+votable180.050000true180.3098044-3.67805970.0055555555555555565/2856 6/893 4439 5989 6028 6087 6977 7246 7484 7642 8261 8528 8922 10454 10691 10741 10743 10912 10927 11191 11388 11402 11428 11430 11432-11433 11490 11898 12380 14960 16301 17727 19283 19567 19883 22890 23323 25054 25585 25735 25965 26148 26292 26300 28060 28517 28605 29795 34881 38268 49042https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/488/1519?format=asciiOpticaldefaultJ/MNRAS/488/1519/table1The low-z RM AGNs with measured {sigma}_*_ for the calibration of fSimbadNameSimbad column added by the CDSmeta.idcharnullabler_sigHbReference for sigHb (1)meta.ref;pos.framecharONameOther namemeta.idcharRFe? Ratio of optical FeII and H{beta} flux from Du et al. (2016ApJ...818L..14D, Cat. J/ApJ/818/L14)phot.flux;spect.line;arith.ratiofloatnullablesigmaStellar velocity dispersionkm/sphys.veloc.dispersioninte_sigmaError on sigmakm/sstat.errorintr_sigmaReference for sigma (1)meta.ref;pos.framecharBTypeBulge type (G1)src.classcharlambdaLHost-corrected monochromatic luminosity at 5100{AA}1e-07Wphys.luminosityfloate_lambdaLError on lambdaL1e-07Wstat.errorfloatr_lambdaLReference for lambdaL (1)meta.ref;pos.framechartauRest-frame H{beta} time lagdtime;arith.difffloatE_tauUpper error on taudstat.error;stat.maxfloate_tauLower error on taudstat.errorfloatr_tauReference for tau (1)meta.ref;pos.framecharFWHMmean? Broad H{beta} FWHM_mean_ from the mean spectrumkm/sspect.line.widthintnullablee_FWHMmean? Error on FWHMmeankm/sstat.errorintnullabler_FWHMmeanReference for FWHMmean (1)meta.ref;pos.framecharFWHMrms? Broad H{beta} FWHM_rms_ from the rms spectrumkm/sspect.line.widthintnullablee_FWHMrms? Error on FWHMrmskm/sstat.errorintnullabler_FWHMrmsReference for FWHMrms (1)meta.ref;pos.framecharsigHb? Broad H{beta} line dispersion {sigma}_H{beta},mean_ from the mean spectrumkm/sphys.veloc.dispersionintnullablee_sigHb? Error on sigHbkm/sstat.errorintnullablesigHbrms? Broad H{beta} line dispersion {sigma}_H{beta},rms_ from the rms spectrumkm/sphys.veloc.dispersionintnullablee_sigHbrms? Error on sigHbrmskm/sstat.errorintnullabler_sigHbrmsReference for sigHbrms (1)meta.ref;pos.framecharVPFm? Virial product calculated based on FWHMmean1e+06solMassphys.massfloatnullableE_VPFm? Upper error on VPFm1e+06solMassstat.error;stat.maxfloatnullablee_VPFm? Lower error on VPFm1e+06solMassstat.errorfloatnullableVPsm? Virial product calculated based on sigHb1e+06solMassphys.massfloatnullableE_VPsm? Upper error on VPsm1e+06solMassstat.error;stat.maxfloatnullablee_VPsm? Lower error on VPsm1e+06solMassstat.errorfloatnullableVPFrms? Virial product calculated based on FWHMrms1e+06solMassphys.massfloatnullableE_VPFrms? Upper error on VPFrms1e+06solMassstat.error;stat.maxfloatnullablee_VPFrms? Lower error on VPFrms1e+06solMassstat.errorfloatnullableVPsrms? Virial product calculated based on sigHbrms1e+06solMassphys.massfloatnullableE_VPsrms? Upper error on VPsrms1e+06solMassstat.error;stat.maxfloatnullablee_VPsrms? Lower error on VPsrms1e+06solMassstat.errorfloatnullablerefsReferences (2)meta.ref;pos.framechar_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.mainrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameAGN namemeta.id;meta.maincharJ/MNRAS/488/1519/table2The high-z RM AGNs observed by SDSS with measured {sigma}_*_SimbadNameSimbad column added by the CDSmeta.idcharnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameAGN namemeta.id;meta.maincharzRedshiftsrc.redshiftfloatsigmaStar velocity dispersionkm/sphys.veloc.dispersionfloate_sigmaError on sigmakm/sstat.errorfloatFWHMmeanBroad line FWHM_mean_ from the mean spectrumkm/sspect.line.widthinte_FWHMmeanError on FWHMmeankm/sstat.errorintFWHMrmsBroad line FWHM_rms_ from the rms spectrumkm/sspect.line.widthinte_FWHMrmsError on FWHMrmskm/sstat.errorintsigmeanBroad line dispersion from the mean spectrumkm/sphys.veloc.dispersioninte_sigmeanError on sigmeankm/sstat.errorintsigrmsBroad line dispersion from the rms spectrumkm/sphys.veloc.dispersioninte_sigrmsError on sigrmskm/sstat.errorintVPFmVirial product calculated based on FWHMmean (1)1e+06solMassphys.massfloatE_VPFmUpper error on VPFm1e+06solMassstat.error;stat.maxfloate_VPFmLower error on VPFm1e+06solMassstat.errorfloatVPsmVirial product calculated based on sigmean (1)1e+06solMassphys.massfloatE_VPsmUpper error on VPsm1e+06solMassstat.error;stat.maxfloate_VPsmLower error on VPsm1e+06solMassstat.errorfloatVPsrmsVirial product calculated based on sigrms (1)1e+06solMassphys.massfloatE_VPsrmsUpper error on VPsrms1e+06solMassstat.error;stat.maxfloate_VPsrmsLower error on VPsrms1e+06solMassstat.errorfloat_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.mainVPFrmsVirial product calculated based on FWHMrms (1)1e+06solMassphys.massfloatE_VPFrmsUpper error on VPFrms1e+06solMassstat.error;stat.maxfloate_VPFrmsLower error on VPFrms1e+06solMassstat.errorfloatLineObserved linemeta.id;spect.linecharJ/MNRAS/488/1519/table3The M_BH_ and four kinds factor of the low-z RM AGNs in Table 1recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameAGN namemeta.id;meta.maincharf_NameFlag on Name (1)meta.codecharBTypeBulge type (G1)src.classcharlogMBH1Logarithm of the black hole mass derived from method 1 (2)log(solMass)phys.massfloate_logMBH1Error on logMBH1log(solMass)stat.errorfloatlogMBH2? Logarithm of the black hole mass derived from method 2 (3)log(solMass)phys.massfloatnullablee_logMBH2? Error on logMBH2log(solMass)stat.errorfloatnullablelogfFm1? Logarithm of the virial factor derived using the virial product VP_F,mean_ and logMBH1stat.fit.paramfloatnullableE_logfFm1? Upper error on logfFm1stat.error;stat.maxfloatnullablee_logfFm1? Lower error on logfFm1stat.errorfloatnullablelogfFm2? Logarithm of the virial factor derived using the virial product VP_F,mean_ and logMBH2stat.fit.paramfloatnullablee_logfsr2? Lower error on logfsr2stat.errorfloatnullableE_logfFm2? Upper error on logfFm2stat.error;stat.maxfloatnullablee_logfFm2? Lower error on logfFm2stat.errorfloatnullablelogfsm1? Logarithm of the virial factor derived using the virial product VP_{sigma},mean_ and logMBH1stat.fit.paramfloatnullableE_logfsm1? Upper error on logfsm1stat.error;stat.maxfloatnullablee_logfsm1? Lower error on logfsm1stat.errorfloatnullablelogfsm2? Logarithm of the virial factor derived using the virial product VP_{sigma},mean_ and logMBH2stat.fit.paramfloatnullableE_logfsm2? Upper error on logfsm2stat.error;stat.maxfloatnullablee_logfsm2? Lower error on logfsm2stat.errorfloatnullablelogfFr1? Logarithm of the virial factor derived using the virial product VP_F,rms_ and logMBH1stat.fit.paramfloatnullableE_logfFr1? Upper error on logfFr1stat.error;stat.maxfloatnullablee_logfFr1? Lower error on logfFr1stat.errorfloatnullablelogfFr2? Logarithm of the virial factor derived using the virial product VP_F,rms_ and logMBH2stat.fit.paramfloatnullableE_logfFr2? Upper error on logfFr2stat.error;stat.maxfloatnullablee_logfFr2? Lower error on logfFr2stat.errorfloatnullablelogfsr1? Logarithm of the virial factor derived using the virial product VP_{sigma},rms_ and logMBH1stat.fit.paramfloatnullableE_logfsr1? Upper error on logfsr1stat.error;stat.maxfloatnullablee_logfsr1? Lower error on logfsr1stat.errorfloatnullablelogfsr2? Logarithm of the virial factor derived using the virial product VP_{sigma},rms_ and logMBH2stat.fit.paramfloatnullableE_logfsr2? Upper error on logfsr2stat.error;stat.maxfloatnullableJ/MNRAS/488/1519/table6The factor f derived from the BLRs dynamical model, X-ray variability, resolved Pa {alpha} emission region for 19 AGNsSimbadNameSimbad column added by the CDSmeta.idcharnullabletauRest-frame H{beta} time lagdtime;arith.difffloatE_tauUpper error on taudstat.error;stat.maxfloate_tauLower error on taudstat.errorfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintr_tauReference for tau and FWHMmean (2)meta.ref;pos.frameintFWHMmeanBroad line FWHM_mean_ from the mean spectrumkm/sspect.line.widthinte_FWHMmeanError on FWHMmeankm/sstat.errorintlogVPFmLogarithm of the virial product calculated based on FWHMmeanlog(solMass)phys.massfloatE_logVPFmUpper error on logVPFmlog(solMass)stat.error;stat.maxfloate_logVPFmLower error on logVPFmlog(solMass)stat.errorfloatlogMBHLogarithm of the black hole masslog(solMass)phys.massfloatE_logMBHUpper error on logMBHlog(solMass)stat.error;stat.maxfloate_logMBHLower error on logMBHlog(solMass)stat.errorfloatlogfFmLogarithm of the virial factor derived using logVPFmstat.fit.paramfloatE_logfFmUpper error on logfFmstat.error;stat.maxfloate_logfFmLower error on logfFmstat.errorfloatr_logMBHReference for logMBH (1)meta.ref;pos.framechar_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.mainNameAGN namemeta.id;meta.mainchar