J/A+A/664/A73ivo://CDS.VizieR/J/A+A/664/A73doi:10.26093/cds/vizier.36640073CDSBurgarella D.Bogdanoska J.Nanni A.Bardelli S.Bethermin M.,Boquien M.Buat V.Faisst A.L.Dessauges-Zavadsky M.Fudamoto Y.,Fujimoto S.Giavalisco M.Ginolfi M.Gruppioni C.Hathi N.P.Ibar E.,Jones G.C.Koekemoer A.M.Kohno K.Lemaux B.C.Narayanan D.Oesch P.,Ouchi M.Riechers D.A.Pozzi F.Romano M.Schaerer D.Talia M.,Theule P.Vergani D.Zamorani G.Zucca E.Cassata P.ALPINE team2023-12-21T16:07:36Z2022-08-05T12:20:31ZCDS support team

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

cds-question@unistra.frgalaxiesstar-forming-regionsastronomical-modelsStar-forming galaxies are composed of various types of galaxies. However, the luminosity functions at z>~4-5 suggest that most galaxies have a relatively low stellar mass (logMstar~10) and a low dust attenuation (A_FUV_~1.0). The physical properties of these objects are quite homogeneous. We used an approach where we combined their rest-frame far-infrared and submillimeter emissions and utilized the universe and the redshift as a spectrograph to increase the amount of information in a collective way. From a subsample of 27 ALMA-detected galaxies at z>4.5, we built an infrared spectral energy distribution composite template. It was used to fit, with CIGALE, the 105 galaxies (detections and upper limits) in the sample from the far-ultraviolet to the far-infrared. The derived physical parameters provide information to decipher the nature of the dust cycle and of the stellar populations in these galaxies. The derived IR composite template is consistent with the galaxies in the studied sample. A delayed star formation history with {tau}_main_=500Myrs is slightly favored by the statistical analysis as compared to a delayed with a final burst or a continuous star formation history. The position of the sample in the star formation rate (SFR) versus Mstar diagram is consistent with previous papers. The redshift evolution of the log Mstar versus AFUV relation is in agreement with an evolution in redshift of this relation. This evolution is necessary to explain the cosmic evolution of the average dust attenuation of galaxies. Evolution is also observed in the Ldust/LFUV (IRX) versus UV slope {beta}_FUV_ diagram: younger galaxies have bluer {beta}_FUV_. We modeled the shift of galaxies in the IRX versus the {beta}_FUV_ diagram with the mass-weighted age as a free parameter, and we provide an equation to make predictions. The large sample studied in this paper is generally consistent with models that assume rapid dust formation from supernovae and removal of dust by outflows and supernovae blasts. However, we find that high mass dusty star-forming galaxies cannot be explained by the models.2022A&A...664A..73Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/664/A73CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/A+A/643/A2 : ALPINE DR1 merged catalog (Bethermin+, 2020)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/664/A73https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/664/A73http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/664/A73https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/664/A73https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/664/A73http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/664/A73GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/A+A/664/A73/tablee1 (Physical parameters from PL+OTMBB (Physical_parameters_plotmbb_final_21Oct))https://vizier.cds.unistra.fr/viz-bin/conesearch/J/A+A/664/A73/tablee1?https://vizier.iucaa.in/viz-bin/conesearch/J/A+A/664/A73/tablee1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/A+A/664/A73/tablee1?GETtext/xml+votable180.050000true53.2251-27.833560.0055555555555555566/17683 17692 27256 27258-27259 35935https://cdsarc.cds.unistra.fr/viz-bin/moc/J/A+A/664/A73?format=asciidefaultJ/A+A/664/A73/tabled1IR template for each of the models, normalized to 200umrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelengthumem.wlfloatFnu(DL2014)/F200umDL2014 flux, normalized to 200umphot.flux;arith.ratiofloatFnu(PL+OTMBB)/F200umPL+OTMBB flux, normalized to 200umphot.flux;arith.ratiofloatFnu(PL+GMBB)/F200umPL+GMBB flux, normalized to 200umphot.flux;arith.ratiofloatJ/A+A/664/A73/tablee1Physical parameters from PL+OTMBB (Physical_parameters_plotmbb_final_21Oct)SimbadNameSimbad column added by the CDSmeta.idcharnullableNameSource namemeta.id;meta.maincharrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintz? Redshiftsrc.redshiftdoublenullablebetaFUVUV slope, {beta}_FUV_meta.crypticdoublee_betaFUVUV slope errorstat.errordoublesSFRSpecific star formation rateyr**-1meta.iddoublee_sSFRSpecific star formation rate erroryr**-1stat.errordoublesMdustdl2014Specific dust mass from DL2014phys.mass;arith.ratiodoublee_sMdustdl2014Specific dust mass from DL2014 errorstat.errordoublesMdustpre-shockPre-shock specific dust massphys.mass;arith.ratiodoublee_sMdustpre-shockPre-shock specific dust mass errorstat.errordoublesMdustpost-shockPost-shock specific dust massphys.mass;arith.ratiodoublee_sMdustpost-shockPost-shock specific dust mass errorstat.errordoubleMdustdl2014Dust mass from dl2014phys.massdoublee_Mdustdl2014Dust mass from dl2014 errorstat.errordoubleMdustpre-shockPre-shock dust massphys.massdoublee_Mdustpre-shockPre-shock dust mass errorstat.errordoubleMdustpost-shockPre-shock dust massphys.massdoublee_Mdustpost-shockPre-shock dust mass errorstat.errordoubleAFUVFUV dust attenuationphys.luminosity;arith.ratiodoublee_AFUVFUV dust attenuation errorstat.errordoubleIRXLdust/LFUV ratiophot.flux;arith.ratiodoublee_IRXLdust/LFUV ratio errorstat.errordoubleAgeMain ageMyrtime.age;meta.maindoublee_AgeMain age errorMyrstat.error;time.agedoubleLdustDust luminositysolLumphys.luminositydoublee_LdustDust luminosity errorsolLumstat.errordoubleLFUVFUV luminositysolLumphys.luminosity;em.UVdoublee_LFUVFUV luminosity errorsolLumstat.errordoubleSFRStar formation ratesolMass/yrphys.SFRdoublee_SFRStar formation rate errorsolMass/yrstat.error;phys.SFRdoubleMstarStar masssolMassphys.massdoublee_MstarStar mass errorsolMassstat.errordouble_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.mainJ/A+A/664/A73/tablee2Physical parameters from DL2014 (Physical_parameters_dl2014_final_21Oc)z? Redshiftsrc.redshiftdoublenullablee_AFUVFUV dust attenuation errorstat.errordoubleIRXLdust/LFUX ratiophot.flux;arith.ratiodoublee_IRXLdust/LFUX ratio errorstat.errordoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintNameSource namemeta.id;meta.maincharbetaFUVUV slope, {beta}_FUV_meta.crypticdoublee_betaFUVUV slope errorstat.errordoublesSFRSpecific star formation rateyr**-1meta.iddoublee_sSFRSpecific star formation rate erroryr**-1stat.errordoublesMdustSpecific dust massphys.mass;arith.ratiodoublee_sMdustSpecific dust mass errorstat.errordoubleAFUVFUV dust attenuationphys.luminosity;arith.ratiodoubleAgeMain ageMyrtime.age;meta.maindoublee_AgeMain age errorMyrstat.error;time.agedoubleLdustDust luminositysolLumphys.luminositydoublee_LdustDust luminosity errorsolLumstat.errordoubleMdustDust masssolMassphys.massdoublee_MdustDust mass errorsolMassstat.errordoubleLFUVFUV luminositysolLumphys.luminosity;em.UVdoublee_LFUVFUV luminosity errorsolLumstat.errordoubleSFRStar formation ratephys.SFRdoublee_SFRStar formation rate errorstat.error;phys.SFRdoubleMstarStar masssolMassphys.massdoublee_MstarStar mass errorsolMassstat.errordoubleJ/A+A/664/A73/lbghizIR composite built from the of ALMA-detected objectsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIdIdentifiermeta.id;stat.fitcharlambdaWavelengthumem.wlfloatFnu/F200um? Flux, normalized to 200umphot.flux;arith.ratiodoublenullablel_Fnu/F200um[-] - indicates upper limit for Fnu/F200ummeta.code.errorchare_Fnu/F200um? Error on Fnu/F200umstat.errordoublenullableS/N? Signal-to-noise ratio (1)stat.snrdoublenullable