J/ApJ/910/124ivo://CDS.VizieR/J/ApJ/910/124doi:10.26093/cds/vizier.19100124CDSXie Y.Ho L.C.Zhuang M.-Y.Shangguan J.2022-10-12T12:19:49Z2022-10-10T08:37:19ZCDS support team

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

cds-question@unistra.frquasarsactive-galactic-nucleiredshiftedchemical-abundancesinfrared-astronomyinterstellar-mediumThe star formation activity of the host galaxies of active galactic nuclei provides valuable insights into the complex interconnections between black hole growth and galaxy evolution. A major obstacle arises from the difficulty of estimating accurate star formation rates (SFRs) in the presence of a strong active galactic nucleus. Analyzing the 1-500{mu}m spectral energy distributions and high-resolution mid-infrared spectra of low-redshift (z<0.5) Palomar-Green quasars with bolometric luminosity of ~10^44.5^-10^47.5^erg/s, we find, from comparison with an independent SFR indicator based on [NeII]12.81{mu}m and [NeIII]15.56{mu}m, that the torus-subtracted, total infrared (8-1000{mu}m) emission yields robust SFRs in the range of ~1-250M_{sun}_/yr. Combined with available stellar mass estimates, the vast majority (~75%-90%) of the quasars lie on or above the main sequence of local star-forming galaxies, including a significant fraction (~50%-70%) that would qualify as starburst systems. This is further supported by the high star formation efficiencies derived from the gas content inferred from the dust masses. Inspection of high-resolution Hubble Space Telescope images reveals a wide diversity of morphological types, including a number of starbursting hosts that have not experienced significant recent dynamical perturbations. The origin of the high star formation efficiency is unknown.2021ApJ...910..124Xhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/910/124CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJ/269/352 : Quasar evolution (Schmidt+, 1983)J/ApJS/143/277 : IRAS 1Jy sample of ultraluminous galaxies. I. (Kim+, 2002)J/ApJS/143/315 : IRAS 1Jy sample of ultraluminous gal. II. (Veilleux+, 2002)J/ApJ/666/806 : SED of Spitzer quasars (QUEST) (Netzer+, 2007)J/ApJS/177/103 : HI survey of AGNs (Ho+, 2008)J/ApJ/703/1672 : Far-IR and H{alpha} fluxes in galaxies (Kennicutt+, 2009)J/A+A/533/A119 : GOODS-Herschel North and South catalogs (Elbaz+, 2011)J/ApJS/214/23 : IR spectra and photometry of z<0.5 quasars (Shi+, 2014)J/A+A/578/A11 : Spectrum of QSO XMMC 2028 (Brusa+, 2015)J/ApJS/219/18 : LIRAS: LoCuSS IR AGN survey (Xu+, 2015)J/ApJ/817/118 : SFR-M_*_ relation from ZFOURGE (Tomczak+, 2016)J/ApJ/819/L27 : Stellar masses of optical & IR QSO hosts (Zhang+, 2016)J/ApJ/848/87 : CALIFA SFRs. II. Bulges & disks (Catalan-Torrecilla+, 2017)J/MNRAS/471/59 : Intrinsic AGN SEDs in PG quasars (Lani+, 2017)J/A+A/602/A123 : AGN vs. host galaxy data in COSMOS field (Lanzuisi+, 2017)J/ApJ/841/76 : Intrinsic far-IR SED of luminous AGNs (Lyu+, 2017)J/ApJS/233/22 : xCOLD GASS catalog (Saintonge+, 2017)J/MNRAS/466/3161 : AGN global star-forming properties (Shimizu+, 2017)J/ApJ/841/102 : Type 2 AGN host galaxies in Chandra-COSMOS (Suh+, 2017)J/MNRAS/478/4238 : Properties of IR-bright AGNs (Dai+, 2018)J/ApJ/854/158 : z<0.5 PG quasars IR energy distributions (Shangguan+, 2018)J/ApJ/870/104 : 1-500um obs. of nearby luminous IR gal. (Shangguan+, 2019)J/ApJ/884/136 : PAH features of star-forming gal. using Spitzer (Xie+, 2019)J/ApJ/888/78 : The ACS-AGN Catalog: AGN luminosity vs SFR (Stemo+, 2020)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/910/124https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/910/124http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/910/124https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/910/124https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/910/124http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/910/124GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/910/124/pgqsos (Physical properties of PG quasars (table 1) and SFRs of quasar host galaxies (Table 2))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/910/124/pgqsos?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/910/124/pgqsos?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/910/124/pgqsos?GETtext/xml+votable180.050000true1.496824416.16361720.0055555555555555566/4215 4506 5091 5244 5437 5481 5576 5687 5731 6028 7246 7998 8017 8071 8299 8528 8636 8641 8845 8881 8893 8906 8927 8941 9018 9181 9194 9262 9959 10039 10162 10217 10269 10472 10578 10691 10694 10709 11217 11354 11388 11668 11829 11924 12317 12380 12632 17819 18127 18918 19287 19315 19416 19433 19567 19700 19730 19746 19767 19883 19932 25403 25735 25742 25965 26310 26509 26736 26859 26902 27023 27025 27227 27293 27349 27580 27720 27848 27862 28060 28164 28356 28471 31650 44785 44988https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/910/124?format=asciiInfrareddefaultJ/ApJ/910/124/pgqsosPhysical properties of PG quasars (table 1) and SFRs of quasar host galaxies (Table 2)r_MorphReference code for Morph (5)meta.ref;pos.framecharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDObject identifiermeta.id;meta.maincharSimbadSimbad column added by the CDSmeta.ref.urlcharuplogSFRNe[0.14/1.51]? Upper uncertainty/limit in logSFRNe (6)log(solMass.yr**-1)stat.errorfloatnullablel_logLIRLimit flag on logLIRmeta.code.errorcharlogLIR[42.66/45.85] Log IR luminosity in erg/s (7)log(1e-07W)phys.luminosity;em.IRfloatNEDNED column added by the CDSmeta.ref.urlcharz[0.025/0.472] Spectroscopic redshift from Shangguan+ (2018, J/ApJ/854/158)src.redshiftfloatDL[113/2723] Luminosity distance from Shangguan+ (2018, J/ApJ/854/158)Mpcpos.distanceintlogL5100[43.6/46.2] log monochromatic AGN luminosity at 5100{AA} from Shangguan+ (2018, J/ApJ/854/158)log(1e-07W)phys.luminosity;em.optfloatlogMBH[6.6/10] log blackhole mass from Shangguan+ (2018, J/ApJ/854/158)log(solMass)phys.massfloatZ16Display data from Zhang+, 2016, J/ApJ/819/L27meta.ref.urlcharlogM*[9.7/12.1] log stellar mass (1)log(solMass)phys.massfloatf_logM*[*] Flag on logM* (2)meta.codecharO/H[8.7/8.9] Oxygen abundance; 12+log(O/H) (3)log(Sun)phys.abundfloate_O/H[0.1/0.14] Lower uncertainty in O/Hlog(Sun)stat.error;phys.abundfloatE_O/H[0.1/0.14] Upper uncertainty in O/Hlog(Sun)stat.error;stat.maxfloatl_logMgasLimit flag on logMgasmeta.code.errorcharlogMgas[8.3/11] log gas mass from Shangguan+ (2018, J/ApJ/854/158)log(solMass)phys.massfloate_logMgas[0.2/0.5]? Lower uncertainty in logMgaslog(solMass)stat.errorfloatnullableE_logMgas[0.2/0.5]? Upper uncertainty in logMgaslog(solMass)stat.error;stat.maxfloatnullableMorphMorphology flag(s) of host galaxy (4)meta.code;src.morphcharl_logL[NeII]Limit flag on logL[NeII]meta.code.errorcharlogL[NeII][40.2/42.81]? Log [NeII]12.81um luminosity in erg/slog(1e-07W)phys.luminosity;em.IR.8-15umfloatnullablee_logL[NeII][0.02/0.3]? Lower uncertainty in logL[NeII]log(1e-07W)stat.errorfloatnullableE_logL[NeII][0.02/0.3]? Upper uncertainty in logL[NeII]log(1e-07W)stat.error;stat.maxfloatnullablel_logL[NeIII]Limit flag on logL[NeIII]meta.code.errorcharlogL[NeIII][40.6/43]? Log [NeIII]15.56um luminosity in erg/slog(1e-07W)phys.luminosity;em.IR.15-30umfloatnullablee_logL[NeIII][0.02/0.3]? Lower uncertainty in logL[NeIII]log(1e-07W)stat.errorfloatnullableE_logL[NeIII][0.02/0.3]? Upper uncertainty in logL[NeIII]log(1e-07W)stat.error;stat.maxfloatnullablel_logL[NeV]Limit flag on logL[NeV]meta.code.errorcharlogL[NeV][40.43/42.62]? Log [NeV]14.32um luminosity in erg/slog(1e-07W)phys.luminosity;em.IR.8-15umfloatnullablee_logL[NeV][0.02/0.35]? Lower uncertainty in logL[NeV]log(1e-07W)stat.errorfloatnullableE_logL[NeV][0.02/0.35]? Upper uncertainty in logL[NeV]log(1e-07W)stat.error;stat.maxfloatnullablef+[0.05/0.76]? Fractional abundances of singly ionized Neonphys.abund;arith.ratiofloatnullablee_f+[0.03/0.24]? Lower uncertainty in f+stat.errorfloatnullableE_f+[0.03/0.24]? Upper uncertainty in f+stat.error;stat.maxfloatnullablef2+[0.18/0.97]? Fractional abundances of doubly ionized Neonphys.abund;arith.ratiofloatnullablee_f2+[0.02/0.25]? Lower uncertainty in f2+stat.errorfloatnullableE_f2+[0.02/0.25]? Upper uncertainty in f2+stat.error;stat.maxfloatnullablel_logSFRNe[l] Limit flag on logSFRNe (6)stat.errorcharlogSFRNe[0.19/2.38]? Log star formation rate from neon luminositylog(solMass.yr**-1)phys.SFR;em.IRfloatnullablelologSFRNe[-0.13/1.25]? Lower uncertainty/limit in logSFRNe (6)log(solMass.yr**-1)stat.errorfloatnullablee_logLIR[0.01/0.16]? Lower uncertainty in logLIRlog(1e-07W)stat.errorfloatnullableE_logLIR[0.01/0.18]? Upper uncertainty in logLIRlog(1e-07W)stat.error;stat.maxfloatnullablel_logSFRIRLimit flag on logSFRIRmeta.code.errorcharlogSFRIR[-0.69/2.5] Log star formation rate from IR (7)log(solMass.yr**-1)phys.SFR;em.IRfloate_logSFRIR[0.01/0.16]? Lower uncertainty in logSFRIRlog(solMass.yr**-1)stat.errorfloatnullableE_logSFRIR[0.01/0.18]? Upper uncertainty in logSFRIRlog(solMass.yr**-1)stat.error;stat.maxfloatnullable_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.mainS18Display data from Shangguan+, 2018, J/ApJ/854/158meta.ref.urlchar