J/A+A/654/A165ivo://CDS.VizieR/J/A+A/654/A165doi:10.26093/cds/vizier.36540165CDSValentino F.Daddi E.Puglisi A.Magdis G.E.Kokorev V.I.Liu D.,Madden S.C.Gomez-Guijarro C.Lee M.-Y.Cortzen I.Circosta C.,Delvecchio I.Mullaney J.R.Gao Y.Gobat R.Aravena M.Jin S.,Fujimoto S.Silverman J.D.Dannerbauer H.2023-03-16T14:16:50Z2021-10-27T09:01:57ZCDS support team

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

cds-question@unistra.frgalaxiescatalogsinfrared-sourcesspectroscopyinterferometryIn the framework of a systematic study with the ALMA interferometer of infrared (IR)-selected main sequence and starburst galaxies at z~1-1.7 at typical ~1" resolution, we report on the effects of mid-IR and X-ray detected active galactic nuclei (AGN) on the reservoirs and excitation of molecular gas in a sample of 55 objects. We find widespread detectable nuclear activity in ~30% of the sample. The presence of dusty tori influences the IR spectral energy distribution of galaxies, as highlighted by the strong correlation among the AGN contribution to the total IR luminosity budget (fAGN=LIR_AGN_/LIR), its hard X-ray emission, and the Rayleigh-Jeans to mid-IR (S_1.2mm_/S_24um_) observed color with evident consequences on the ensuing empirical star formation rate estimates. Nevertheless, we find only marginal effects of the presence and strength of AGN on the carbon monoxide CO (J=2,4,5,7) or neutral carbon ([CI](3P1-3P0), [CI](3P2-3P1)) line luminosities and on the derived molecular gas excitation as gauged by line ratios and the full spectral line energy distributions. The [CI] and CO emission up to J=5,7 thus primarily traces the properties of the host in typical IR luminous galaxies. However, our analysis highlights the existence of a large variety of line luminosities and ratios despite the homogeneous selection. In particular, we find a sparse group of AGN-dominated sources with the highest LIR_AGN_/LIR_SFR_>=3 ratios that are more luminous in CO(5-4) than what predicted by the L_CO(5-4)_-LIR_SFR_ relation, which might be the result of the nuclear activity. For the general population, our findings translate into AGN having minimal effects on quantities such as gas and dust fractions and star formation efficiencies. If anything, we find hints of a marginal tendency of AGN hosts to be compact at far-IR wavelengths and to display 1.8x larger dust optical depths. In general, this is consistent with a marginal impact of the nuclear activity on the gas reservoirs and star formation in average star-forming AGN hosts with LIR>5x10^11^L_{sun}_, typically under-represented in surveys of quasars and sub-millimeter galaxies.2021A&A...654A.165Vhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/654/A165CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/641/A155 : CO+[CI] emission in distant galaxies (Valentino+, 2020)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/654/A165https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/654/A165http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/654/A165https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/654/A165https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/654/A165http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/654/A165GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/654/A165/tablea1 (ALMA+Far-IR+Optical AGN data table)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/654/A165/tablea1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/654/A165/tablea1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/654/A165/tablea1?GETtext/xml+votable180.050000true150.38954172.255850.0055555555555555565/6814 6/https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/654/A165?format=asciiInfrareddefaultJ/A+A/654/A165/tablea1ALMA+Far-IR+Optical AGN data tableSimbadNameSimbad column added by the CDSmeta.idcharnullablee_U? Error on U (DU)stat.error;pos.cartesian.xdoublenullableIDIdentifier (ID) (1)meta.id;meta.mainintWidthCO21? Velocity width of CO21 line (WIDTH_CO21)km/sspect.line.widthdoublenullableSNRCO76? S/N of the CO76 line flux (SNR_CO76)stat.snrdoublenullable1sigCO76? 1{sigma} limit on CO76 flux (ONESIGMA_CO76)Jy.km/sphot.flux.densityfloatnullableWidthCO76? Velocity width of CO76 line (WIDTH_CO76)km/sspect.line.widthdoublenullablefCO76? Quality and usage flag for CO76 (FLAG_CO76) (1)meta.code.qualfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right ascension (J2000) (RAh)pos.eq.ra;meta.mainDEJ2000Declination (J2000) (DEd)pos.eq.dec;meta.mainzspOptMIROptical/near-IR redshift (ZSPEC_OPTICALNIR) (2)src.redshift;pos.heliocentricfloatzspsubmmALMA submillimeter redshift (ZSPEC_SUBMM)src.redshift;pos.heliocentricdoublee_zspsubmm? Error on the ALMA redshift (DZSPEC_SUBMM)stat.errordoublenullablelogM*? logarithm of stellar mass (LOG_STELLARMASS) (3)log(solMass)phys.massdoublenullableLLIRtot? Total 8-1000um IR luminosity (TOTAL_LIR) (4)solLumphys.luminosity;em.IRdoublenullablee_LLIRtot? Error on the total IR luminosity (DTOTAL_LIR)solLumstat.errordoublenullableSFLIR? IR luminosity due to star formation (SF_LIR)solLumphys.luminosity;em.IRdoublenullablee_SFLIR? Error on IR luminosity due to star formation (DSF_LIR)solLumstat.errordoublenullableAGNLIR? IR luminosity from the AGN component (AGN_LIR)solLumphys.luminosity;em.IRdoublenullablee_AGNLIR? Error on IR luminosity from the AGN component (DAGN_LIR)solLumstat.errordoublenullablefAGN? Fraction of total LIR due to the AGN (F_AGN) (5)phys.luminosity;em.IRdoublenullablee_fAGN? Error on the fraction of total LIR due to the AGN (DF_AGN)stat.errordoublenullableMdust? Dust mass (MDUST) (6)solMassphys.massdoublenullablee_Mdust? Error on the dust mass (DMDUST)solMassstat.errordoublenullableU? Mean intensity of the interstellar radiation field (U) (6)phot.mag;em.opt.UdoublenullableDistMS? Distance from the main sequence (DISTANCEMS) (7)stat.fit.paramdoublenullableSize? Source angular size from ALMA (SIZE)arcsecphys.angSizefloatnullablee_Size? Error on the source angular size from ALMA (DSIZE)arcsecstat.error;phys.angSizefloatnullable1sigsize? 1{sigma} upper limit on the size (ONESIGMA_SIZE)arcsecphys.angSize;stat.maxfloatnullableFCO54? Velocity integrated CO54 flux (FLUX_LINECO54)Jy.km/sphot.flux.densitydoublenullableSNRCO54? S/N of the CO54 line flux (SNR_CO54)stat.snrdoublenullable1sigCO54? 1{sigma} limit on CO54 flux (ONESIGMA_CO54)Jy.km/sphot.flux.densitydoublenullableWidthCO54? Velocity width of CO54 line (WIDTH_CO54)km/sspect.line.widthdoublenullablefCO54? Quality and usage flag for CO54 (FLAG_CO54) (1)meta.code.qualfloatnullableFCO21? Velocity integrated CO21 flux (FLUX_LINECO21)Jy.km/sphot.flux.densitydoublenullableSNRCO21? S/N of the CO21 line flux (SNR_CO21)stat.snrdoublenullable1sigCO21? 1{sigma} limit on CO21 flux (ONESIGMA_CO21)Jy.km/sphot.flux.densitydoublenullablefCO21? Quality and usage flag for CO21 (FLAG_CO21) (1)meta.code.qualfloatnullableFCO76? Velocity integrated CO76 flux (FLUX_LINECO76)Jy.km/sphot.flux.densitydoublenullableFCI21? Velocity integrated CI21 flux (FLUX_LINECI21)Jy.km/sphot.flux.densitydoublenullableSNRCI21? S/N of the CI21 line flux (SNR_CI21)stat.snrdoublenullable1sigCI21? 1{sigma} limit on CI21 flux (ONESIGMA_CI21)Jy.km/sphot.flux.densityfloatnullableWIDTHCI21? Velocity width of CI21 line (WIDTHCI21)km/sspect.line.widthdoublenullablefCI21? Quality and usage flag for CI21 (FLAG_CI21) (1)meta.code.qualfloatnullableFCI10? Velocity integrated CI10 flux (FLUX_LINECI10)Jy.km/sphot.flux.densitydoublenullableSNRCI10? S/N of the CI10 line flux (SNR_CI10)stat.snrdoublenullable1sigCI10? 1{sigma} limit on CI10 flux (ONESIGMA_CI10)Jy.km/sphot.flux.densitydoublenullableWidthCI10? Velocity width of CI10 line (WIDTH_CI10)km/sspect.line.widthfloatnullablefCI10? Quality and usage flag for CI10 (FLAG_CI10) (1)meta.code.qualfloatnullableFCO43? Velocity integrated CO43 flux (FLUX_LINECO43)Jy.km/sphot.flux.densitydoublenullableSNRCO43? S/N of the CO43 line flux (SNR_CO43)stat.snrdoublenullable1sigCO43? 1{sigma} limit on CO43 flux (ONESIGMA_CO43)Jy.km/sphot.flux.densityfloatnullableWidthCO43? Velocity width of CO43 line (WIDTH_CO43)km/sspect.line.widthfloatnullablefCO43? Quality and usage flag for CO43 (FLAG_CO43) (1)meta.code.qualfloatnullableLX? 2-10 keV rest frame log-luminosity (Lx_210) (8)erg/sphys.luminosity;em.X-rayfloatnullablefD12[0/1] Donley et al., 2012ApJ...748..142D AGN classification (FLAG_DONLEY2012) (9)meta.codechar