J/ApJS/252/29ivo://CDS.VizieR/J/ApJS/252/29doi:10.26093/cds/vizier.22520029CDSKoss M.J.Strittmatter B.Lamperti I.Shimizu T.Trakhtenbrot B.,Saintonge A.Treister E.Cicone C.Mushotzky R.Oh K.Ricci C.,Stern D.Ananna T.T.Bauer F.E.Privon G.C.Bar R.E.De Breuck C.,Harrison F.Ichikawa K.Powell M.C.Rosario D.Sanders D.B.,Schawinski K.Shao LiMegan Urry C.Veilleux S.2021-07-05T12:18:14Z2021-05-26T13:14:56ZCDS support team

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

cds-question@unistra.fractive-galactic-nucleico-line-emissionredshiftedmolecular-physicssurveysseyfert-galaxiesWe present the host-galaxy molecular gas properties of a sample of 213 nearby (0.01<z<0.05) hard-X-ray-selected active galactic nucleus (AGN) galaxies, drawn from the 70-month catalog of Swift's Burst Alert Telescope (BAT), with 200 new CO(2-1) line measurements obtained with the James Clerk Maxwell Telescope and the Atacama Pathfinder Experiment telescope. We find that AGN in massive galaxies (log(M_*_/M_{sun}_)>10.5) tend to have more molecular gas and higher gas fractions than inactive galaxies matched in stellar mass. When matched in star formation, we find AGN galaxies show no difference from inactive galaxies, with no evidence that AGN feedback affects the molecular gas. The higher molecular gas content is related to AGN galaxies hosting a population of gas-rich early types with an order of magnitude more molecular gas and a smaller fraction of quenched, passive galaxies (~5% versus 49%) compared to inactive galaxies. The likelihood of a given galaxy hosting an AGN (L_bol_>10^44^erg/s) increases by ~10-100 between a molecular gas mass of 10^8.7^M_{sun}_ and 10^10.2^M_{sun}_. AGN galaxies with a higher Eddington ratio (log(L/L_Edd_)>-1.3) tend to have higher molecular gas masses and gas fractions. The log(NH/cm^-2^)>23.4) of AGN galaxies with higher column densities are associated with lower depletion timescales and may prefer hosts with more gas centrally concentrated in the bulge that may be more prone to quenching than galaxy-wide molecular gas. The significant average link of host-galaxy molecular gas supply to supermassive black hole (SMBH) growth may naturally lead to the general correlations found between SMBHs and their host galaxies, such as the correlations between SMBH mass and bulge properties, and the redshift evolution of star formation and SMBH growth.2021ApJS..252...29Khttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJS/252/29CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/swift : Swift Master Catalog (HEASARC, 2004-)VII/258 : Quasars and Active Galactic Nuclei (13th Ed.) (Veron+ 2010)J/ApJS/146/353 : Circumnuclear dust in galaxies (Martini+, 2003)J/AJ/136/2782 : Star formation efficiency in nearby galaxies (Leroy+, 2008)J/ApJ/701/587 : HST H-band imaging survey. II. QUEST QSOs (Veilleux+, 2009)J/MNRAS/413/813 : ATLAS3D project. I. (Cappellari+, 2011)J/ApJ/739/57 : Ultra hard X-ray AGNs in the Swift/BAT survey (Koss+, 2011)J/MNRAS/415/32 : COLD GASS survey (Saintonge+, 2011)J/MNRAS/414/940 : ATLAS3D project. IV. (Young+, 2011)J/MNRAS/421/1569 : Properties of 18286 SDSS radio galaxies (Best+, 2012)J/ApJ/746/L22 : Dual AGNs in the nearby Universe (Koss+, 2012)J/MNRAS/426/2601 : CO lines in luminous IR galaxies (Papadopoulos+, 2012)J/A+A/541/A118 : AGN-Host Galaxy Connection (Povic+, 2012)J/ApJS/207/19 : Hard X-ray survey from Swift-BAT 6yrs (Baumgartner+, 2013)J/ApJ/765/L26 : Swift/BAT X-ray data from GOALS LIRGs (Koss+, 2013)J/A+A/564/A65 : Cold gas data of Herschel Reference Survey (Boselli+, 2014)J/ApJ/794/152 : PACS observations of Herschel-BAT sample (Melendez+, 2014)J/ApJS/219/1 : Catalog of Type-1 AGNs from SDSS-DR7 (Oh+, 2015)J/ApJ/815/L13 : Compton-thick AGNs from 70-month Swift/BAT (Ricci+, 2015)J/MNRAS/458/2221 : ATLAS3D Project. XXXI (Nyland+, 2016)J/MNRAS/457/2703 : Local SDSS galaxies in Herschel Stripe 82 (Rosario+, 2016)J/MNRAS/456/3335 : SPIRE observations of Herschel-BAT sample (Shimizu+, 2016)J/A+A/604/A53 : ALLSMOG final DR. A new APEX CO survey (Cicone+, 2017)J/ApJ/835/74 : IR phot. of AGNs in Swift/BAT 70 month (Ichikawa+, 2017)J/ApJ/850/74 : Swift/BAT AGN Spectroscopic Survey. I. (Koss+, 2017)J/ApJS/233/17 : Swift/BAT AGN spectroscopic survey. V. X-ray (Ricci+, 2017)J/ApJS/233/22 : xCOLD GASS catalog (Saintonge+, 2017)J/MNRAS/466/3161 : AGN global star-forming properties (Shimizu+, 2017)J/A+A/609/A9 : Local Swift-BAT AGN observed with Herschel (Lutz+, 2018)J/ApJ/870/31 : BAT AGN spectroscopic survey. XI. IR phot. (Ichikawa+, 2019)J/ApJ/881/154 : BAT AGN spectroscopic survey. XVI. Blazars (Paliya+, 2019)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJS/252/29https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJS/252/29http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJS/252/29https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJS/252/29https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJS/252/29http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJS/252/29GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJS/252/29/agns (Multiwavelength properties of the BAT AGN (Table 1) and CO(2-1) measurements (Table 2))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJS/252/29/agns?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJS/252/29/agns?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJS/252/29/agns?GETtext/xml+votable180.050000true0.61013.351910.0055555555555555566/134 723 745 1121 1405 1677 2251 4215 4488 4834 5149 5463 6212 6752 7157 7386 7552 8216 8870 8921 8922 10788 11490 13021 13720 16690 16892 17350 17408 17525 17548 17727 17795 18307 18402 18419 18484 18524 18695 18794 18897 18918 19283 19296 19318 19373 19376 19400 19469 19797 19883 19940 20171 20201 20489 20556 20750 21016 21036 21088 21186 21237 21245 21378 21785 21996 22365 22585 22626 22632 22637 22890 22912 22975 23010 23081 23224 23278 23323 24120 24123 24381 24748 24842 25054 25090 25273 25572 25585 25610 25742 25773 26071 26300 26375 26393 26547 26861 27143 27477 27699 27803 28075 28275 28350 28517 28609 29906 30026 31158 31509 31833 32986 33034 33038 33716 33953 34070 34104 34125 34294 34318 34499 34861 34913 35049 35052 35071 35085 35106 35263 35284 35407 35447 35623 35638 35717 35899 36062 36073 36158 36216 36323 36618 36668 36765 36775 36786 36861 37054 37287 37458 38129 38314 38479 38526 38696 38704 38817 38948 39138 39149 39182 39613 39717 40013 40250 40258 40818 41423 41435 41982 42012 43412 43520 43546 43634 43649 43677 43825 43860 43877 43983 44448 44507 44551 44698 44722 44892 45220 45222 45446 45735 45779 45883 46544 46811 46831 46865 47027 47064 47120 47154 47169 47222 47245 47597 48321 48798 49001 49042https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJS/252/29?format=asciiRadiodefaultJ/ApJS/252/29/agnsMultiwavelength properties of the BAT AGN (Table 1) and CO(2-1) measurements (Table 2)SimbadNameSimbad column added by the CDSmeta.idcharTypeAGN typesrc.classcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintBAT[1/1413] Catalog ID in the BAT surveymeta.idintNameGalaxy Name, optical/IR counterpart to AGNmeta.id;meta.maincharRAJ2000[0.2/352.3] Counterpart Right Ascension (J2000)degpos.eq.ra;meta.mainDEJ2000[-78.9/63.7] Counterpart declination (J2000)degpos.eq.dec;meta.mainzspec[0.01/0.05] Redshift (1)src.redshiftfloatrk20fe[5/82] Isophotal radius (2)arcsecphys.angSizefloatIncl[18/89] Inclination angle (3)degsrc.orbital.inclination;pos.posAngintMorphMorphological classification (4)src.morphcharlogM*[9.4/11.4] log of stellar masses of the BAT AGN host galaxies (5)log(solMass)phys.massfloatl_SFRLimit flag on SFRmeta.code.error;phys.SFRcharSFR[0/132]? Star formation rate (6)solMass/yrphys.SFRfloatnullablel_D(MS)Limit flag on DMSmeta.code.errorcharD(MS)[-10.3/2.2]? Offset from the Main Sequence of star-formation (7)stat.fit.residualfloatnullableTelTelescope used for the CO observation (1)instr.setup;obscharHPBW[20/32] Associated beam sizearcsecphys.angSize;instr.beamintFlagCO21[0/1] Detection flag for the CO(2-1) line (1=detection) (2)meta.codeintsigma-CO21[0.4/17.1]? RMS noise achieved around the CO(1-0) line (3)mKinstr.det.noisefloatnullableC-aper[1.0/8.71] Beam correction factor (4)instr.paramfloatSN-inte[-3/39.5] Signal-to-noise, integrated linestat.snrfloatL-inte[0.2/105.5] Total CO(2-1) line luminosity from integrated line (5)1e+08K.km.s**-1.pc**2phys.luminosityfloatlogMH2[8/10.7] Log of total molecular gas mass (6)log(solMass)phys.massfloatlogtdepH2[7.5/20.1]? Log of gas depletion timescale (7)log(yr)time.scalefloatnullablePro[-1/2]? Fit type (8)meta.codeintnullableL-pro[0.2/132.1]? Total CO(2-1) line luminosity from the profile fit (9)1e+08K.km.s**-1.pc**2phys.luminosityfloatnullableSN-pro[1.5/55.1]? Signal-to-noise, CO profilestat.snrfloatnullableW50[41/658]? FWHM of the CO line from profile fitkm/sspect.line.widthintnullablee_W50[18/953]? Uncertainty in W50km/sstat.errorintnullablezCO[3151/14928]? Redshift from the central CO velocitykm/ssrc.redshift;pos.heliocentricintnullablee_zCO[2/327]? Uncertainty in zCOkm/sstat.errorintnullableK17Display data from Koss+, 2017, J/ApJ/850/74meta.ref.urlintnullableNEDNED column added by the CDSmeta.ref.urlchar