J/MNRAS/466/3161ivo://CDS.VizieR/J/MNRAS/466/3161doi:10.26093/cds/vizier.74663161CDSShimizu T.T.Mushotzky R.F.Melendez M.Koss M.J.Barger A.J.,Cowie L.L.2024-08-17T20:17:53Z2019-11-27T16:24:16ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleiinfrared-sourcesWe combine the HerschelSpace Observatory PACS (Photoconductor Array Camera and Spectrometer) and SPIRE (Spectral and Photometric Imaging Receiver) photometry with archival WISE (Wide-field Infrared Survey Explorer) photometry to construct the spectral energy distributions (SEDs) for over 300 local (z<0.05), ultrahard X-ray (14-195keV) selected active galactic nuclei (AGN) from the Swift Burst Alert Telescope (BAT) 58-month catalogue. Using a simple analytical model that combines an exponentially cutoff power law with a single temperature modified blackbody, we decompose the SEDs into a host galaxy and AGN component. We calculate dust masses, dust temperatures, and star formation rates (SFRs) for our entire sample and compare them to a stellar mass-matched sample of local non-AGN galaxies. We find AGN host galaxies have systematically higher dust masses, dust temperatures, and SFRs due to the higher prevalence of late-type galaxies to host an AGN, in agreement with previous studies of the Swift/BAT AGN. We provide a scaling to convert X-ray luminosities into 8-1000{mu}m AGN luminosities, as well as determine the best mid-to-far IR colours for identifying AGN-dominated galaxies in the IR regime. We find that for nearly 30 per cent of our sample, the 70{mu}m emission contains a significant contribution from the AGN (>0.5), especially at higher luminosities (L_14-195keV_>10^42.5^erg/s). Finally, we measure the local SFR-AGN luminosity relationship, finding a slope of 0.18, large scatter (0.37 dex), and no evidence for an upturn at high AGN luminosity. We conclude with a discussion on the implications of our results within the context of galaxy evolution with and without AGN2017MNRAS.466.3161Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/466/3161CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/ApJ/794/152 : PACS observations of Herschel-BAT sample (Melendez+, 2014)J/MNRAS/456/3335 : SPIRE observations of Herschel-BAT sample (Shimizu+, 2016)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/466/3161https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/466/3161http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/466/3161https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/466/3161https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/466/3161http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/466/3161GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapInfrareddefaultJ/MNRAS/466/3161/table1Best Fit C12 Model Parameters, Luminosities, and AGN FractionsSimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameGalaxy namemeta.id;meta.maincharl_logMdustLimit flag on logMdustmeta.code.errorcharlogMdust? Dust masslog(solMass)phys.massfloatnullableE_logMdust? Error on logMdust (upper value)log(solMass)stat.error;stat.maxfloatnullablee_logMdust? Error on logMdust (lower value)log(solMass)stat.errorfloatnullableTdust? Dust temperature for the MBB component (1)Kphys.temperaturefloatnullableE_Tdust? Error on Tdust (upper value)Kstat.error;stat.maxfloatnullablee_Tdust? Error on Tdust (lower value)Kstat.errorfloatnullablealpha? Slope of the power-law componentspect.indexfloatnullableE_alpha? Error on alpha (upper value)stat.error;stat.maxfloatnullablee_alpha? Error on alpha (lower value)stat.error;pos.eq.rafloatnullablelambdac? Turnover wavelengthumem.wlfloatnullableE_lambdac? Error on lambdac (upper value)umstat.error;stat.maxfloatnullablee_lambdac? Error on lambdac (lower value)umstat.errorfloatnullablel_logLIRLimit flag on logLIRmeta.code.errorcharlogLIR? Total infrared luminosity from 8 to 1000umlog(solLum)phys.luminosity;em.IRfloatnullableE_logLIR? Error on logLIR (upper value)log(solLum)stat.error;stat.maxfloatnullablee_logLIR? Error on logLIR (lower value)log(solLum)stat.errorfloatnullablel_logLSFLimit flag on logLSFmeta.code.errorcharlogLSF? MBB component luminositylog(solLum)phys.luminosityfloatnullableE_logLSF? Error on logLSF (upper value)log(solLum)stat.error;stat.maxfloatnullablee_logLSF? Error on logLSF (lower value)log(solLum)stat.errorfloatnullablel_logLAGNIRLimit on logLAGNIRmeta.code.errorcharlogLAGNIR? Power-law component luminositylog(solLum)phys.luminosity;em.IRfloatnullableE_logLAGNIR? Error on logLAGNIR (upper value)log(solLum)stat.error;stat.maxfloatnullablee_logLAGNIR? Error on logLAGNIR (lower value)log(solLum)stat.errorfloatnullablel_fAGNC12Limit flag on fAGNC12meta.code.errorcharfAGNC12? Fractional contribution of the AGN to the total infrared luminosityphys.luminosity;arith.ratiofloatnullableE_fAGNC12? Error on fAGNC12 (upper value)stat.error;stat.maxfloatnullablee_fAGNC12? Error on fAGNC12 (upper value)stat.errorfloatnullableNEDNED column added by the CDSmeta.ref.urlchar