J/MNRAS/478/4238ivo://CDS.VizieR/J/MNRAS/478/4238doi:10.26093/cds/vizier.74784238CDSDai Y.S.Wilkes B.J.Bergeron J.Kuraszkiewicz J.Omont A.Atanas A.,Teplitz H.I.2024-08-18T20:20:06Z2021-12-10T13:55:05ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleigalaxiesinfrared-sourcesx-ray-sourcesWe report the relationship between the luminosities of active galactic nuclei (AGNs) and the rates of star formation (SF) for a sample of 323 far-infrared (FIR)-detected AGNs. This sample has a redshift range of 0.2<z<2.5, and spans three orders of magnitude in luminosity, L_X_~10^42-45^erg/s. We find that in AGN hosts, the total infrared (IR) luminosity (8-1000um) has a significant AGN contribution (average ~20 per cent), and we suggest using the FIR luminosity (30-1000um) as a more reliable star formation rate (SFR) estimator. We conclude that monochromatic luminosities at 60 and 100um are also good SFR indicators with negligible AGN contributions, being less sensitive than integrated IR luminosities to the shape of the AGN spectral energy distribution (SED), which is uncertain at {lambda}>100um. Significant bivariate L_X_-L_IR_ correlations are found, which remain significant in the combined sample when using residual partial correlation analysis to account for the inherent redshift dependence. No redshift or mass dependence is found for the ratio between SFR and black hole accretion rate (BHAR), which has a mean and scatter of log(SFR/BHAR)=3.1+/-0.5, agreeing with the local mass ratio between supermassive black hole and host galaxies. The large scatter in this ratio and the strong AGN-SF correlation found in these IR-bright AGNs are consistent with the scenario of an AGN-SF dependence on a common gas supply, regardless of the evolutionary model.2018MNRAS.478.4238Dhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/478/4238CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/MNRAS/429/1652 : XMM-LSS catalogue. Version II. (Chiappetti+, 2013)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/478/4238https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/478/4238http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/478/4238https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/478/4238https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/478/4238http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/478/4238GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/478/4238/table2 (Derived properties for IR-bright AGNs)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/478/4238/table2?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/478/4238/table2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/478/4238/table2?GETtext/xml+votable180.050000true33.35271-3.586710.0055555555555555565/4422-4423 4428 6/17671 17677 17679 17681-17683 17686 17716-17717https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/478/4238?format=asciiX-rayInfrareddefaultJ/MNRAS/478/4238/table2Derived properties for IR-bright AGNsSimbadSimbad column added by the CDSmeta.ref.urlcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordint2XLSSdObject identification same as in Chiappetti et al. (2013MNRAS.429.1652C, Cat. J/MNRAS/429/1652) (JHHMMSS.s+DDMMSS)meta.id;meta.maincharzRedshiftsrc.redshiftfloatf_z[1/2] Redshift flag, 1 for spec-z, 2 for photo-zmeta.codeintTdustPeak dust temperatureKphys.temperaturefloate_TdustPeak dust temperature errorKstat.errorfloatalphaPower-law indexspect.indexfloate_alphaPower-law index errorstat.error;pos.eq.rafloatHRX-ray Hardness ratio [HR=(H-S)/(H+S)] based on net count ratesphot.flux;arith.ratiofloatNHintIntrinsic column density derived from redshift and HRlog(cm**-2)phys.columnDensitydoublelogLX(2-10)Obscuration corrected rest-frame X-ray luminosity (2-10keV)log(1e-07W)phys.luminosity;em.X-rayfloatlogLIRAGNAGN contributed IR luminosity (8-1000um) (1)log(1e-07W)phys.luminosity;em.IRfloatlogLIRSFAGN-subtracted IR luminosity (8-1000um) (2)log(1e-07W)phys.luminosity;em.IRfloatSFRIRSFR derived from logLIRSF using the Kennicutt (1998ARA&A..36..189K) relation (2)Myr/yrphys.SFRintlogMdustDust mass derived from FIR photometrylog(solMass)phys.massfloate_logMdustDust mass derived from FIR photometry errorlog(solMass)stat.errorfloatlogMBH? SMBH mass derived for the subsample with optical broad emission lineslog(solMass)phys.massfloatnullableFlag[1/3] Sample flag (3)meta.code.errorint_RARight Ascension (J2000) from J/MNRAS/429/1652/2xlssddegpos.eq.ra;meta.main_DEDeclination (J2000) from J/MNRAS/429/1652/2xlssddegpos.eq.dec;meta.main