J/MNRAS/499/4325ivo://CDS.VizieR/J/MNRAS/499/4325doi:10.26093/cds/vizier.74994325CDSRamos Padilla A.F.Ashby M.L.N.Smith H.A.Martinez-Galarza J.R.,Beverage A.G.Dietrich J.Higuera-G. M.-A.Weiner A.S.2024-08-21T20:16:28Z2020-11-27T09:57:00ZCDS support team

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

cds-question@unistra.frgalaxiesphotometryactive-galactic-nucleiEmission from active galactic nuclei (AGNs) is known to play an important role in the evolution of many galaxies including luminous and ultraluminous systems (U/LIRGs), as well as merging systems. However, the extent, duration, and exact effects of its influence are still imperfectly understood, as are the conditions that lead to it dominating the IR emission, and then fading again after coalescence. To assess the impact of AGNs on interacting systems, we present a Spectral Energy Distribution (SED) analysis of a sample of 188 nearby galaxies We gather and systematically re-reduce archival broad-band imaging mosaics from the ultraviolet to the far-infrared using data from GALEX, SDSS, 2MASS, IRAS, WISE, Spitzer, and Herschel. We use spectroscopy from Spitzer/IRS to obtain fluxes from fine-structure lines that trace star formation and AGN activity. Utilizing the SED modelling and fitting tool CIGALE, we derive the physical conditions of the interstellar medium, both in star-forming regions and in nuclear regions dominated by the AGN in these galaxies. We investigate how the star formation rates (SFRs) and the fractional AGN contributions (fAGN) depend on stellar mass, galaxy type, and merger stage. We find that luminous galaxies more massive than about 10^10M* are likely to deviate significantly from the conventional galaxy main-sequence relation. Interestingly, infrared AGN luminosity and stellar mass in this set of objects are much tighter than SFR and stellar mass. We find that buried AGNs may occupy a locus between bright starbursts and pure AGNs in the fAGN-[NeV]/[NeII] plane. We identify a modest correlation between fAGN and mergers in their later stages.2020MNRAS.499.4325Rhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/499/4325CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJS/218/6 : Spitzer Interacting Galaxies Survey (SIGS) (Brassington+, 2015)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/499/4325https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/499/4325http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/499/4325https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/499/4325https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/499/4325http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/499/4325GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/499/4325/tablea1 (Basic data for the SIGS galaxies)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/499/4325/tablea1?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/499/4325/tablea1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/499/4325/tablea1?GETtext/xml+votable180.050000true12.756667-7.0563060.005555555555555556Cone search capability for table J/MNRAS/499/4325/tablea2 (Basic data for the SB galaxies)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/499/4325/tablea2?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/499/4325/tablea2?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/499/4325/tablea2?GETtext/xml+votable180.050000true2.472525.9237780.005555555555555556Cone search capability for table J/MNRAS/499/4325/tablea3 (Basic data for the AGN galaxies)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/499/4325/tablea3?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/499/4325/tablea3?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/499/4325/tablea3?GETtext/xml+votable180.050000true1.5812520.2029170.005555555555555556Cone search capability for table J/MNRAS/499/4325/tablea4 (Basic data for the LSM galaxies)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/499/4325/tablea4?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/499/4325/tablea4?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/499/4325/tablea4?GETtext/xml+votable180.050000true5.1108330.8296390.0055555555555555566/556 614 941 3506 4215 4439 4447 4469 4681 4718 4742 4993 5040 5082 5097 5241 5244 5348 5463 5634-5635 5950 5995 6034 6037 6047 6057 6090 6098 6539 7584 7602 7604 7606 7642 7869 7986 8106 8173 8196 8299 8373 8492 8556 8922 8973 8997 9402 9470 9507 9882 10515 10544 10628 10637 10691 10739 10752 10847 10900-10901 10912 10949 10991 11027 11049 11180 11372 11389 11434 11463 11908 12380 16655 17492 17754 17927 18013 18073 18098 18209 18212 18387 18683 18731 18809 19619 19730 19883 20254 20489 22721 22792 23171 23178 25344 25610 25739 25772 25790 25841 25888 25890 25907 25965 26035 26267 26515 26971 27255 27339 27426 27446 27620 27741 27760 27767 27907 28045 28060 28184 28225 28269 28393 28542 28593 33034 34531 36716 36831 36861 38139 38704 39836 43233 43806 43877 45883 47078 471693.972892068905477e-22 1.4134638842407062e-18https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/499/4325?format=asciidefaultJ/MNRAS/499/4325/tablea1Basic data for the SIGS galaxiesSimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGrp[1-48] Group ID for the SIGS samplemeta.id;meta.mainintGalaxyGalaxy IDmeta.id;src.class.starGalaxycharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainzRedshiftsrc.redshiftfloatSample[CA] C or A indicates objects belonging to the Keel-Complete sample or the Arp sample, respectivelysrc.samplecharStage[2/5] Merger stage as defined by Dopita et al. (2002ApJS..143...47D)meta.codeintSize1Angular sizearcsecphys.angSizefloatSize2Angular sizearcsecphys.angSizefloatAngleInclination angle used in photutilsdegsrc.orbital.inclinationfloatJ/MNRAS/499/4325/tablea2Basic data for the SB galaxiesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGalaxyGalaxy IDmeta.id;src.class.starGalaxycharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainzRedshiftsrc.redshiftfloatSample[BS ] B or S indicates B wheter the objects belong to Brand et al. (2006ApJ...641..140B, Cat. J/ApJ/641/140) or added as well known local starbursts, respectivelymeta.idcharSize1Angular sizearcsecphys.angSizefloatSize2Angular sizearcsecphys.angSizefloatAngleInclination angle used in photutilsdegsrc.orbital.inclinationfloatSimbadSimbad column added by the CDSmeta.ref.urlcharJ/MNRAS/499/4325/tablea3Basic data for the AGN galaxiesSize2Angular sizearcsecphys.angSizefloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGalaxyGalaxy IDmeta.id;src.class.starGalaxycharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainzRedshiftsrc.redshiftfloatSample[GHS R] G, H or S indicates whether objects belong to the GOALS sample (G), Higuera-G. & Ramos P. (2013,HR) or taken from SIMBAD (S), respectivelysrc.samplecharSize1Angular sizearcsecphys.angSizefloatAngleInclination angle used in photutilsdegsrc.orbital.inclinationfloatSimbadSimbad column added by the CDSmeta.ref.urlcharJ/MNRAS/499/4325/tablea4Basic data for the LSM galaxiesSimbadNameSimbad column added by the CDSmeta.idcharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGalaxyGalaxy IDmeta.id;src.class.starGalaxycharRAJ2000Right ascension (J2000)pos.eq.ra;meta.mainDEJ2000Declination (J2000)pos.eq.dec;meta.mainzRedshiftsrc.redshiftfloatlog(LIR)log IR luminosity taken from Wang et al. (2014AJ....148....4W, Cat. J/AJ/148/4)solLumphys.luminosity;em.IRfloatStageMerger stage as defined by Dopita et al. (2002)meta.codefloatSize1Angular sizearcsecphys.angSizefloatSize2Angular sizearcsecphys.angSizefloatAngleInclination angle used in photutilsdegsrc.orbital.inclinationfloatJ/MNRAS/499/4325/photomPhotometry for all galaxies (tables A6-A9)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGalaxyGalaxy IDmeta.id;src.class.starGalaxycharFUV? Flux FUV band (GALEX 0.152um)mJyphot.flux;em.UVfloatnullablee_FUV? Flux uncertainty FUV bandmJystat.errorfloatnullableNUV? Flux NUV band (GALEX 0.227um)mJyphot.flux;em.UVfloatnullablee_NUV? Flux uncertainty NUV bandmJystat.errorfloatnullableuprime? Flux u_prime band (SDSS DR12 0.354um)mJyphot.mag;em.opt.Ufloatnullablee_uprime? Flux uncertainty u_prime bandmJystat.errorfloatnullablegprime? Flux g_prime band (SDSS DR12 0.477um)mJyphot.mag;em.opt.Bfloatnullablee_gprime? Flux uncertainty g_prime bandmJystat.errorfloatnullablerprime? Flux r_prime band (SDSS DR12 0.623um)mJyphot.mag;em.opt.Rfloatnullablee_rprime? Flux uncertainty r_prime bandmJystat.errorfloatnullableiprime? Flux i_prime band (SDSS DR12 0.762um)mJyphot.mag;em.opt.Idoublenullablee_iprime? Flux uncertainty i_prime bandmJystat.errorfloatnullablezprime? Flux z_prime band (SDSS DR12 0.913um)mJyphot.mag;em.opt.Idoublenullablee_zprime? Flux uncertainty z_prime bandmJystat.errorfloatnullableJ2mass? Flux J_2mass band (2MASS 1.25um)mJyphot.flux.density;em.IR.Jdoublenullablee_J2mass? Flux uncertainty J_2mass bandmJystat.errorfloatnullableH2mass? Flux H_2mass band (2MASS 1.65um)mJyphot.flux.density;em.IR.Hdoublenullablee_H2mass? Flux uncertainty H_2mass bandmJystat.errorfloatnullableKs2mass? Flux Ks_2mass band (2MASS 2.17um)mJyphot.mag;em.IR.Kdoublenullablee_Ks2mass? Flux uncertainty Ks_2mass bandmJystat.errorfloatnullableWISE1? Flux WISE1 band (WISE 3.4um)mJyphot.mag;em.IR.3-4umdoublenullablee_WISE1? Flux uncertainty WISE1 bandmJystat.errorfloatnullableIRAC1? Flux IRAC1 band (IRAC 3.6um)mJyphot.mag;em.IR.3-4umdoublenullablee_IRAC1? Flux uncertainty IRAC1 bandmJystat.errorfloatnullableIRAC2? Flux IRAC2 band (IRAC 4.5um)mJyphot.mag;em.IR.4-8umdoublenullablee_IRAC2? Flux uncertainty IRAC2 bandmJystat.errorfloatnullableWISE2? Flux WISE2 band (WISE 4.5um)mJyphot.mag;em.IR.4-8umdoublenullablee_WISE2? Flux uncertainty WISE2 bandmJystat.errorfloatnullableIRAC3? Flux IRAC3 band (IRAC 5.8um)mJyphot.flux.density;em.IR.4-8umdoublenullablee_IRAC3? Flux uncertainty IRAC3 bandmJystat.errorfloatnullableIRAC4? Flux IRAC4 band (IRAC 8.0um)mJyphot.flux.density;em.IR.8-15umdoublenullablee_IRAC4? Flux uncertainty IRAC4 bandmJystat.errorfloatnullableIRAS1? Flux IRAS1 band (IRAS 12um)mJyphot.flux.density;em.IR.8-15umdoublenullablee_IRAS1? Flux uncertainty IRAS1 bandmJystat.errorfloatnullableWISE3? Flux WISE3 band (WISE 12um)mJyphot.flux.density;em.IR.8-15umdoublenullablee_WISE3? Flux uncertainty WISE3 bandmJystat.errordoublenullableWISE4? Flux WISE4 band (WISE 22um)mJyphot.flux.density;em.IR.15-30umdoublenullablee_WISE4? Flux uncertainty WISE4 bandmJystat.errordoublenullableMIPS1? Flux MIPS1 band (MPIS 24um)mJyphot.flux.density;em.IR.15-30umdoublenullablee_MIPS1? Flux uncertainty MIPS1 bandmJystat.errordoublenullableIRAS2? Flux IRAS2 band (IRAS 25um)mJyphot.flux.density;em.IR.15-30umdoublenullablee_IRAS2? Flux uncertainty IRAS2 bandmJystat.errordoublenullableIRAS3? Flux IRAS3 band (IRAS 60um)Jyphot.flux.density;em.IR.30-60umfloatnullablee_IRAS3? Flux uncertainty IRAS3 bandJystat.errorfloatnullablePACSblue? Flux PACS_blue band (PACS 70um)Jyphot.flux.density;em.IR.30-60umfloatnullablee_PACSblue? Flux uncertainty PACS_blue bandJystat.errorfloatnullableMIPS2? Flux MIPS2 band (MIPS 70um)Jyphot.flux.density;em.IR.30-60umfloatnullablee_MIPS2? Flux uncertainty MIPS2 bandJystat.errorfloatnullableIRAS4? Flux IRAS4 band (IRAS 100um)Jyphot.flux.density;em.IR.60-100umfloatnullablee_IRAS4? Flux uncertainty IRAS4 bandJystat.errorfloatnullablePACSgreen? Flux PACS_green band (PACS 100um)Jyphot.flux.density;em.IR.60-100umfloatnullablee_PACSgreen? Flux uncertainty PACS_green bandJystat.errorfloatnullableMIPS3? Flux MIPS3 band (MIPS 160um)Jyphot.flux.density;em.mm.1500-3000GHzfloatnullablee_MIPS3? Flux uncertainty MIPS3 bandJystat.errorfloatnullablePACSred? Flux PACS_red band (PACS 180um)Jyphot.flux.density;em.mm.1500-3000GHzfloatnullablee_PACSred? Flux uncertainty PACS_red bandJystat.errorfloatnullablePSW? Flux PSW_ext band (SPIRE 250um)Jyphot.flux.density;em.mm.750-1500GHzfloatnullablee_PSW? Flux uncertainty PSW_ext bandJystat.errorfloatnullablePMW? Flux PMW_ext band (SPIRE 350um)Jyphot.flux.density;em.mm.750-1500GHzfloatnullablee_PMW? Flux uncertainty PMW_ext bandJystat.errorfloatnullablePLW? Flux PLW_ext band (SPIRE 500um)Jyphot.flux.density;em.mm.400-750GHzfloatnullablee_PLW? Flux uncertainty PLW_ext bandJystat.errorfloatnullableJ/MNRAS/499/4325/paramCIGALE (bayes) derived parameters for all galaxies with good fits (tables A6-A9)GalaxyGalaxy IDmeta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintagn.fAGNAGN fractionphys.luminosity;arith.ratiofloate_agn.fAGNAGN fraction errorstat.errorfloatagn.lumlog AGN luminosity of the three AGN components by Fritz et al. (2006MNRAS.366..767F)log(solLum)phys.luminosityfloate_agn.lumlog AGN luminosity error of the three components by Fritz et al. (2006MNRAS.366..767F)log(solLum)stat.errorfloatatt.stel.oldlog old attenuation from the old stellar populationlog(solLum)stat.fit.paramfloate_att.stel.oldlog old attenuation error from the old stellar populationlog(solLum)stat.errorfloatatt.stel.younglog young attenuation from the old stellar populationlog(solLum)stat.fit.paramfloate_att.stel.younglog young attenuation error from the old stellar populationlog(solLum)stat.errorfloatdust.alphaParameter that defines the contribution of the local heating intensity in the duststat.fit.paramfloate_dust.alphaError on dust.alphastat.errorfloatdust.lumlog dust luminositylog(solLum)phys.luminosityfloate_dust.lumlog dust luminosity errorlog(solLum)stat.errorfloatsfh.sfrlog star formation ratelog(solMass.yr**-1)meta.idfloate_sfh.sfrlog star formation rate errorlog(solMass.yr**-1)stat.errorfloatsfh.tau-mainlog e-folding time of the main stellar population modellog(yr)stat.fit.paramfloate_sfh.tau-mainlog e-folding time of the main stellar population model errorlog(yr)stat.errorfloatstel.age.m-starlog age of the oldest stars in the galaxylog(yr)time.agefloate_stel.age.m-starlog age of the oldest stars in the galaxy errorlog(yr)stat.errorfloatstel.m-gaslog gas masslog(solMass)phys.massfloate_stel.m-gaslog gas mass errorlog(solMass)stat.errorfloatstel.m-starlog stellar masslog(solMass)phys.massfloate_stel.m-starlog stellar mass errorlog(solMass)stat.errorfloatJ/MNRAS/499/4325/parampsiCIGALE (bayes) derived parameters for six AGN galaxies with different Psi (tables A10-13)recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintGalaxyGalaxy IDmeta.id;meta.maincharagn.fAGNAGN fractionphys.luminosity;arith.ratiofloate_agn.fAGNAGN fraction errorstat.errorfloatagn.lumlog AGN luminosity of the three AGN components by Fritz et al. (2006MNRAS.366..767F)log(solLum)phys.luminosityfloate_agn.lumlog AGN luminosity error of the three components by Fritz et al. (2006MNRAS.366..767F)log(solLum)stat.errorfloatatt.stel.oldlog old attenuation from the old stellar populationlog(solLum)stat.fit.paramfloate_att.stel.oldlog old attenuation error from the old stellar populationlog(solLum)stat.errorfloatatt.stel.younglog young attenuation from the old stellar populationlog(solLum)stat.fit.paramfloate_att.stel.younglog young attenuation error from the old stellar populationlog(solLum)stat.errorfloatdust.alphaParameter that defines the contribution of the local heating intensity in the duststat.fit.paramfloate_dust.alphaError on dust.alphastat.errorfloatdust.lumlog dust luminositylog(solLum)phys.luminosityfloate_dust.lumlog dust luminosity errorlog(solLum)stat.errorfloatsfh.sfrlog star formation ratelog(solMass.yr**-1)meta.idfloate_sfh.sfrlog star formation rate errorlog(solMass.yr**-1)stat.errorfloatsfh.tau-mainlog e-folding time of the main stellar population modellog(yr)stat.fit.paramfloate_sfh.tau-mainlog e-folding time of the main stellar population model errorlog(yr)stat.errorfloatstel.age.m-starlog age of the oldest stars in the galaxylog(yr)time.agefloate_stel.age.m-starlog age of the oldest stars in the galaxy errorlog(yr)stat.errorfloatstel.m-gaslog gas masslog(solMass)phys.massfloate_stel.m-gaslog gas mass errorlog(solMass)stat.errorfloatstel.m-starlog stellar masslog(solMass)phys.massfloate_stel.m-starlog stellar mass errorlog(solMass)stat.errorfloat