J/ApJ/921/40ivo://CDS.VizieR/J/ApJ/921/40doi:10.26093/cds/vizier.19210040CDSKokorev V.I.Magdis G.E.Davidzon I.Brammer G.Valentino F.,Daddi E.Ciesla L.Liu D.Jin S.Cortzen I.Delvecchio I.,Gimenez-Arteaga C.Gomez-Guijarro C.Sargent M.Toft S.Weaver J.R.2023-06-15T09:14:41Z2023-03-22T11:15:35ZCDS support team

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

cds-question@unistra.frgalaxiesinfrared-sourcesredshiftedactive-galactic-nucleiWe analyze the far-infrared (FIR) properties of ~5000 star-forming galaxies at z<4.5, drawn from the deepest, super-deblended catalogs in the GOODS-N and COSMOS fields. We develop a novel panchromatic spectral energy distribution fitting algorithm, Stardust, that models the emission from stars, active galactic nuclei (AGNs), and infrared dust emission, without relying on energy balance assumptions. Our code provides robust estimates of the UV- optical and FIR physical parameters, such as the stellar mass (M*), dust mass (Mdust), infrared luminosities (LIR) arising from AGN and star formation activity, and the average intensity of the interstellar radiation field (<U>). Through a set of simulations we quantify the completeness of our data in terms of Mdust, LIR, and <U> and subsequently characterize the distribution and evolution of these parameters with redshift. We focus on the dust-to-stellar mass ratio (fdust), which we parameterize as a function of cosmic age, stellar mass, and specific star formation rate. The fdust is found to increase by a factor of 10 from z=0 to z=2 and appears to remain flat at higher z, mirroring the evolution of the gas fraction. We also find a growing fraction of warm to cold dust with increasing distance from the main sequence, indicative of more intense interstellar radiation fields, higher star formation efficiencies, and more compact star-forming regions for starburst galaxies. Finally, we construct the dust mass functions (DMFs) of star-forming galaxies up to z=1 by transforming the stellar mass function to DMF through the scaling relations derived here. The evolution of fdust and the recovered DMFs are in good agreement with the theoretical predictions of the Horizon-AGN and IllustrisTNG simulations.2021ApJ...921...40Khttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/921/40CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toII/284 : COSMOS Multi-Wavelength Photometry Catalog (Capak+, 2007)II/373 : The fourth UltraVISTA data release (DR4) (Moneti+, 2019)VIII/95 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)VIII/103 : Herschel Multi-tiered Extragalactic Survey (Oliver+, 2012)J/A+A/504/751 : GOODS-MUSIC catalog updated version (Santini+, 2009)J/AJ/142/111 : Total infrared brightness and SFR in M33 (Boquien+, 2011)J/A+A/533/A119 : GOODS-Herschel North and South catalogs (Elbaz+, 2011)J/A+A/532/A90 : PACS Evolutionary Probe (PEP-DR1) catalogs (Lutz+, 2011)J/ApJ/738/69 : SEDs of galaxies at 3.8<z<5 in GOODS (Shim+, 2011)J/MNRAS/423/197 : MIPS photometry for Herschel SAG2 Programs (Bendo+, 2012)J/ApJ/761/140 : Spectroscopy of Herschel-SPIRE galaxies (Casey+, 2012)J/ApJ/745/95 : Herschel FIR & submm phot. of KINGFISH sample (Dale+, 2012)J/A+A/544/A156 : UltraVISTA Catalogue Release DR1 (McCracken+, 2012)J/A+A/551/A100 : Panchromatic SED of Herschel sources (Berta+, 2013)J/ApJ/777/18 : Stellar mass functions of galaxies to z=4 (Muzzin+, 2013)J/ApJ/768/74 : PHIBSS: CO obs. of star-forming galaxies (Tacconi+, 2013)J/ApJS/214/24 : 3D-HST+CANDELS catalog (Skelton+, 2014)J/ApJS/224/24 : The COSMOS2015 catalog (Laigle+, 2016)J/ApJ/820/83 : ALMA galaxies in the COSMOS survey field (Scoville+, 2016)J/MNRAS/465/1789 : SCUBA-2 Cosmology Legacy Survey (Geach+, 2017)J/ApJS/233/22 : xCOLD GASS catalog (Saintonge+, 2017)J/ApJ/853/172 : "Super-deblended" dust emission in galaxies. I. (Liu+, 2018)J/ApJ/864/56 : "Super-deblended" dust em. in gal. II. COSMOS (Jin+, 2018)J/ApJS/236/30 : Herschel-ATLAS (H-ATLAS) DR2 (Maddox+, 2018)J/ApJS/235/34 : Deep JVLA imaging of GOODS-N at 20cm (Owen, 2018)J/A+A/609/A30 : Monochromatic conversion factors to LIR (Schreiber+, 2018)J/A+A/627/A132 : GAS II. UV luminosity functions & IR excess (Cousin+, 2019)J/ApJS/244/40 : A3COSMOS. I. ALMA continuum photometry catalogs (Liu+, 2019)J/A+A/643/A2 : ALPINE DR1 merged catalog (Bethermin+, 2020)J/A+A/644/A144 : Dusty star-forming galaxies (Donevski+, 2020)J/ApJ/909/56 : A galaxy sample with CO detections (Liu+, 2021)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/921/40https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/921/40http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/921/40https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/921/40https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/921/40http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/921/40GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/921/40/table3 (Structure of the best-fit catalog)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/921/40/table3?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/921/40/table3?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/921/40/table3?GETtext/xml+votable180.050000true189.397628862.28646850.0055555555555555565/6814 6/11230 11249 11252 27245 27247 27344https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/921/40?format=asciiInfrareddefaultJ/ApJ/921/40/table3Structure of the best-fit catalogf_fgasFMRi=infinite valuemeta.codecharUmin[0.1/50] Best fit U_min_ valuespect.line.intensity;arith.ratio;stat.minfloatgamma[0/0.5] Best fit {gamma} valuestat.fit.paramfloatqpah[0/10] Index of the best fit q_PAH_ valuemeta.code;spect.index;meta.modelledintU[0/373] Average radiation field intensityspect.line.intensity;arith.ratiodoublee_U[0/219] Uncertainty in Ustat.error;spect.line.intensity;arith.ratiodoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintCat[1/2] Catalog identifier (1)meta.codeintID[6/20010955] Object identifier in Catmeta.id;meta.mainintRAJ2000[149.3/189.6] Right Ascension (J2000)degpos.eq.ra;meta.mainDEJ2000[1.6/62.5] Declination (J2000)degpos.eq.dec;meta.mainArea[0/1] The goodArea flag in the parent catalogsmeta.codeintz[0.005/7.5] Redshift used in fittingsrc.redshiftfloatf_z[0/2]? Redshift type (2)meta.codeintnullableLIR[0/4.04e+13] Total FIR luminosity (3)solLumphys.luminosity;em.IRdoublee_LIR[0/8.1e+12]? Uncertainty in LIRsolLumstat.errordoublenullableLAGN[0/2e+13] AGN luminositysolLumphys.luminosity;em.IRdoublee_LAGN[0/8.3e+12]? Uncertainty in LAGNsolLumstat.errordoublenullableLIRdr[0/3.3e+13] Luminosity from DL07 (Draine & Li 2007ApJ...657..810D) templatesolLumphys.luminosity;em.IRdoublee_LIRdr[0/5.5e+12]? Uncertainty in LIRdrsolLumstat.errordoublenullableMdust[0/4.4e+10] Dust mass predicted by best-fit DL07 (Draine & Li 2007ApJ...657..810D) templatesolMassphys.massdoublee_Mdust[1/7.7e+21]? Uncertainty in MdustsolMassstat.errordoublenullabledelGDR[53.4/9.8e+20]? Gas-to-dust-ratiophys.mass;arith.ratiodoublenullablelamLast[53.2/1180.5] Last band that has an S/N>3 detection ({lambda}_last_) given in rest frameumem.wlfloatchi2[0/1988] The {chi}^2^ of best-fit coefficientsstat.fit.chi2;meta.modelledfloatfAGN[0/0.92] AGN fraction, LAGN/LIRphys.luminosity;arith.ratiodoublee_fAGN[0/1.8]? Uncertainty in fAGNstat.errordoublenullablefgas[0/18400]? Gas fraction computed as Mgas/Mdustphys.mass;arith.ratiodoublenullablefgasFMR[-0.00022/1.1e+20]? Gas fraction assuming delGDR=100phys.mass;arith.ratiodoublenullabledelMS[0/4590] Star formation ratio (5)phys.SFR;arith.ratiodoublee_delMS[0/207]? Uncertainty in delMSstat.errordoublenullablef_delGDRi=infinite valuemeta.codecharf_Mgasi=infinite valuemeta.codecharMgas[0/6.5e+26]? Gas mass computed from DelGDR & MdustsolMassphys.massdoublenullablee_Mgas[0/1.4e+25]? Uncertainty in MgassolMassstat.errordoublenullableMstar[0/1.9e+14]? Stellar mass (4)solMassphys.massdoublenullable