J/MNRAS/513/1175ivo://CDS.VizieR/J/MNRAS/513/1175doi:10.26093/cds/vizier.75131175CDSEspino-Briones N.Perez-Gonzalez P.G.Zamorano J.Rodriguez-Munoz L.2025-03-07T20:14:32Z2025-02-24T15:25:53ZCDS support team

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

cds-question@unistra.frgalaxiescatalogsastrometryredshiftedapparent-magnitudestar-forming-regionsphotometryspectroscopyultraviolet-astronomyvisible-astronomyinfrared-astronomystellar-massesextinctionstellar-agesWe study in detail the properties of the stellar populations of 111 massive [log(M*/M_{sun}_) => 10] dusty [far-infrared (FIR)-selected] starburst (SFR/SFRMS > 2) galaxies at 0.7 < z < 1.2. For that purpose, we use self-consistent methods that analyse the UV-to-FIR broad-band observations in terms of the stellar light and dust re-emission with energy-balance techniques. We find that the emission of our starburst galaxies can be interpreted as a recent star formation episode superimposed on a more evolved stellar population. On average, the burst age is ~80 Myr and its attenuation ~2.4 mag. Assuming our starburst galaxies at half their lifetimes, we infer a duration of the starburst phase of ~160 Myr. The median stellar mass and star formation rate (SFR) are log (M*/M_{sun}_) ~ 10.6 and ~220 M_{sun}_/yr. Assuming this SFR and the inferred duration of the starburst phase, the stellar mass added during this phase corresponds to ~40 per cent the median stellar mass of our sample. The young-population age determines the position of our galaxies in the M*-SFR plane. Galaxies located at the largest distances of the MS present shorter young-population ages. The properties of the underlying stellar population cannot be constrained accurately with our broad-band data. We also discuss the impact of including the FIR data and energy-balance techniques in the analysis of the properties of the stellar populations in starburst galaxies.2022MNRAS.513.1175Ehttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/513/1175CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toJ/ApJS/176/1 : Subaru/XMM-Newton deep survey (SXDS). II. (Furusawa+, 2008)II/319 : UKIDSS-DR9 LAS, GCS and DXS Surveys (Lawrence+ 2012)J/AJ/138/1261 : Spitzer/MIPS observations of the COSMOS field (Frayer+, 2009)J/ApJ/675/234 : Stellar mass functions for galaxies 0<z<4VIII/112 : Herschel/SPIRE point source catalog (HSPSC)VIII/106 : Herschel/PACS Point Source Catalogs (Herschel team, 2017)II/335 : Revised catalog of GALEX UV sources (GUVcat_AIS GR6+7)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/513/1175https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/513/1175http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/513/1175https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/513/1175https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/513/1175http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/513/1175GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/MNRAS/513/1175/table2ms (Dusty-starburst main- multiband photometry)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/513/1175/table2ms?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/513/1175/table2ms?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/513/1175/table2ms?GETtext/xml+votable180.050000true34.51972694-5.057373060.005555555555555556Cone search capability for table J/MNRAS/513/1175/table2cs (Dusty-starburst complementary- multiband photometry)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/MNRAS/513/1175/table2cs?https://vizier.iucaa.in/viz-bin/conesearch/J/MNRAS/513/1175/table2cs?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/MNRAS/513/1175/table2cs?GETtext/xml+votable180.050000true34.70662611-4.782121940.0055555555555555566/17677 17679 17688 176903.972892068905477e-22 1.4134638842407062e-18https://cdsarc.cds.unistra.fr/viz-bin/moc/J/MNRAS/513/1175?format=asciiUVOpticalInfrareddefaultJ/MNRAS/513/1175/table2msDusty-starburst main- multiband photometryzRedshift (redshift) (2)src.redshiftfloate_S160? PACS 160um flux uncertainty (dS160)mJystat.errorfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right ascension (J2000) (ra) (1)degpos.eq.ra;meta.mainDEJ2000Declination (J2000) (dec) (1)degpos.eq.dec;meta.mainFUVmag? FUV GALEX band at 153.9 nm observed AB magnitude (FUV_mag) (3)magphot.mag;em.UV.100-200nmfloatnullablee_FUVmag? Mean uncertainty on FUVmag (FUV_magerr) (3)magstat.error;phot.magfloatnullableNUVmag? NUV GALEX band at 231.6 nm observed AB magnitude (NUV_mag) (3)magphot.mag;em.UV.200-300nmfloatnullablee_NUVmag? Mean uncertainty on NUVmag (NUV_magerr) (3)magstat.error;phot.magfloatnullableBmag? B Subaru band at 441.9 nm observed AB magnitude (B_mag) (3)magphot.mag;em.opt.Bfloatnullablee_Bmag? Mean uncertainty on Bmag (B_magerr) (3)magstat.error;phot.magfloatnullableVmag? V Subaru band at 545.6 nm observed AB magnitude (V_mag) (3)magphot.mag;em.opt.Vfloatnullablee_Vmag? Mean uncertainty on Vmag (V_magerr) (3)magstat.error;phot.magfloatnullableRcmag? R_c_ Subaru band at 651.8 nm observed AB magnitude (R_mag) (3)magphot.mag;em.opt.Rfloatnullablee_Rcmag? Mean uncertainty on Rcmag (R_magerr) (3)magstat.error;phot.magfloatnullableimag? I' Subaru band at 766.9 nm observed AB magnitude (i_mag) (3)magphot.mag;em.opt.Ifloatnullablee_imag? Mean uncertainty on imag (i_magerr) (3)magstat.error;phot.magfloatnullablezmag? Z' Subaru band at 906.8 nm observed AB magnitude (z_mag) (3)magphot.mag;em.opt.Ifloatnullablee_zmag? Mean uncertainty on zmag (z_magerr) (3)magstat.error;phot.magfloatnullableJmag? J UKIRT/WFCAM band at 1.25 {mu}m observed AB magnitude (J_mag) (3)magphot.mag;em.IR.Jfloatnullablee_Jmag? Mean uncertainty on Jmag (J_magerr) (3)magstat.error;phot.magfloatnullableHmag? H UKIRT/WFCAM band at 1.64 {mu}m observed AB magnitude (H_mag) (3)magphot.mag;em.IR.Hfloatnullablee_Hmag? Mean uncertainty on Hmag (H_magerr) (3)magstat.error;phot.magfloatnullableKmag? K UKIRT/WFCAM band at 2.21 {mu}m observed AB magnitude (H_magerr) (3)magphot.mag;em.IR.Kfloatnullablee_Kmag? Mean uncertainty on Kmag (K_magerr) (3)magstat.error;phot.magfloatnullable3.6mag? 3.6 {mu}m IRAC/Spitzer band at 3.56 {mu}m observed AB magnitude (I1_mag) (3)magphot.mag;em.IR.3-4umfloatnullablee_3.6mag? Mean uncertainty on 3.6mag (I1_magerr) (3)magstat.errorfloatnullable4.5mag? 4.5 {mu}m IRAC/Spitzer band at 4.50 {mu}m observed AB magnitude (I2_mag) (3)magphot.mag;em.IR.4-8umfloatnullablee_4.5mag? Mean uncertainty on 4.5mag (I2_magerr) (3)magstat.errorfloatnullable5.8mag? 5.8 {mu}m IRAC/Spitzer band at 5.74 {mu}m observed AB magnitude (I3_mag) (3)magphot.flux.density;em.IR.4-8umfloatnullablee_5.8mag? Mean uncertainty on 5.8mag (I3_magerr) (3)magstat.errorfloatnullable8.0mag? 8.0 {mu}m IRAC/Spitzer band at 7.93 {mu}m observed AB magnitude (I4_mag) (3)magphot.flux.density;em.IR.8-15umfloatnullablee_8.0mag? Mean uncertainty on 8.0mag (I4_magerr) (3)magstat.errorfloatnullableS24? Spitzer/MIPS 24um band flux density at 23.8 {mu}m (S24)mJyphot.flux.density;em.IR.15-30umfloatnullablee_S24? MIPS 24um flux uncertainty (dS24)mJystat.errorfloatnullableS70? Spitzer/MIPS 70um band flux density at 72.5 {mu}m (S70)mJyphot.flux.density;em.IR.30-60umfloatnullablee_S70? MIPS 70um flux uncertainty (dS70)mJystat.errorfloatnullableS100? PACS/Herschel 100um band flux density at 102.4 {mu}m (S100)mJyphot.flux.density;em.IR.60-100umfloatnullablee_S100? PACS 100um flux uncertainty (dS100)mJystat.errorfloatnullableS160? PACS/Herschel 160um band flux density at 165.6 {mu}m (S160)mJyphot.flux.density;em.mm.1500-3000GHzfloatnullableS250? SPIRE/Herschel 250um band flux density at 253.2 {mu}m (S250)mJyphot.flux.density;em.mm.750-1500GHzfloatnullablee_S250? SPIRE 250um flux uncertainty (dS250)mJystat.errorfloatnullableS350? SPIRE/Herschel 350um band flux density at 355.9 {mu}m (S350)mJyphot.flux.density;em.mm.750-1500GHzfloatnullablee_S350? SPIRE 350um flux uncertainty (dS350)mJystat.errorfloatnullableS500? SPIRE/Herschel 500um band flux uncertainty at 511.3 {mu}m (S500)mJyphot.flux.density;em.mm.400-750GHzfloatnullablee_S500? SPIRE 500um flux uncertainty (S500)mJystat.errorfloatnullableIDSpitzer/MIPS-24 ID designation (ID)meta.id;meta.maincharJ/MNRAS/513/1175/table2csDusty-starburst complementary- multiband photometryimag? I' Subaru band at 766.9 nm observed AB magnitude (i_mag) (3)magphot.mag;em.opt.Ifloatnullablee_imag? Mean uncertainty on imag (i_magerr) (3)magstat.error;phot.magfloatnullablezmag? Z' Subaru band at 906.8 nm observed AB magnitude (z_mag) (3)magphot.mag;em.opt.Ifloatnullablee_zmag? Mean uncertainty on zmag (z_magerr) (3)magstat.error;phot.magfloatnullableJmag? J UKIRT/WFCAM band at 1.25 {mu}m observed AB magnitude (J_mag) (3)magphot.mag;em.IR.Jfloatnullablee_Jmag? Mean uncertainty on Jmag (J_magerr) (3)magstat.error;phot.magfloatnullableHmag? H UKIRT/WFCAM band at 1.64 {mu}m observed AB magnitude (H_mag) (3)magphot.mag;em.IR.Hfloatnullablee_Hmag? Mean uncertainty on Hmag (H_magerr) (3)magstat.error;phot.magfloatnullableKmag? K UKIRT/WFCAM band at 2.21 {mu}m observed AB magnitude (H_magerr) (3)magphot.mag;em.IR.Kfloatnullablee_Kmag? Mean uncertainty on Kmag (K_magerr) (3)magstat.error;phot.magfloatnullable3.6mag? 3.6 {mu}m IRAC/Spitzer band at 3.56 {mu}m observed AB magnitude (I1_mag) (3)magphot.mag;em.IR.3-4umfloatnullablee_3.6mag? Mean uncertainty on 3.6mag (I1_magerr) (3)magstat.errorfloatnullable4.5mag? 4.5 {mu}m IRAC/Spitzer band at 4.50 {mu}m observed AB magnitude (I2_mag) (3)magphot.mag;em.IR.4-8umfloatnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintRAJ2000Right ascension (J2000) (ra) (1)degpos.eq.ra;meta.mainDEJ2000Declination (J2000) (dec) (1)degpos.eq.dec;meta.mainzRedshift (redshift) (2)src.redshiftfloatFUVmag? FUV GALEX band at 153.9 nm observed AB magnitude (FUV_mag) (3)magphot.mag;em.UV.100-200nmfloatnullablee_FUVmag? Mean uncertainty on FUVmag (FUV_magerr) (3)magstat.error;phot.magfloatnullableNUVmag? NUV GALEX band at 231.6 nm observed AB magnitude (NUV_mag) (3)magphot.mag;em.UV.200-300nmfloatnullablee_NUVmag? Mean uncertainty on NUVmag (NUV_magerr) (3)magstat.error;phot.magfloatnullableBmag? B Subaru band at 441.9 nm observed AB magnitude (B_mag) (3)magphot.mag;em.opt.Bfloatnullablee_Bmag? Mean uncertainty on Bmag (B_magerr) (3)magstat.error;phot.magfloatnullableVmag? V Subaru band at 545.6 nm observed AB magnitude (V_mag) (3)magphot.mag;em.opt.Vfloatnullablee_Vmag? Mean uncertainty on Vmag (V_magerr) (3)magstat.error;phot.magfloatnullableRcmag? R_c_ Subaru band at 651.8 nm observed AB magnitude (R_mag) (3)magphot.mag;em.opt.Rfloatnullablee_Rcmag? Mean uncertainty on Rcmag (R_magerr) (3)magstat.error;phot.magfloatnullablee_4.5mag? Mean uncertainty on 4.5mag (I2_magerr) (3)magstat.errorfloatnullable5.8mag? 5.8 {mu}m IRAC/Spitzer band at 5.74 {mu}m observed AB magnitude (I3_mag) (3)magphot.flux.density;em.IR.4-8umfloatnullablee_5.8mag? Mean uncertainty on 5.8mag (I3_magerr) (3)magstat.errorfloatnullable8.0mag? 8.0 {mu}m IRAC/Spitzer band at 7.93 {mu}m observed AB magnitude (I4_mag) (3)magphot.flux.density;em.IR.8-15umfloatnullablee_8.0mag? Mean uncertainty on 8.0mag (I4_magerr) (3)magstat.errorfloatnullableS24? Spitzer/MIPS 24um band flux density at 23.8 {mu}m (S24)mJyphot.flux.density;em.IR.15-30umfloatnullablee_S24? MIPS 24um flux uncertainty (dS24)mJystat.errorfloatnullableS70? Spitzer/MIPS 70um band flux density at 72.5 {mu}m (S70)mJyphot.flux.density;em.IR.30-60umfloatnullablee_S70? MIPS 70um flux uncertainty (dS70)mJystat.errorfloatnullableS100? PACS/Herschel 100um band flux density at 102.4 {mu}m (S100)mJyphot.flux.density;em.IR.60-100umfloatnullablee_S100? PACS 100um flux uncertainty (dS100)mJystat.errorfloatnullableS160? PACS/Herschel 160um band flux density at 165.6 {mu}m (S160)mJyphot.flux.density;em.mm.1500-3000GHzfloatnullablee_S160? PACS 160um flux uncertainty (dS160)mJystat.errorfloatnullableS250? SPIRE/Herschel 250um band flux density at 253.2 {mu}m (S250)mJyphot.flux.density;em.mm.750-1500GHzfloatnullablee_S250? SPIRE 250um flux uncertainty (dS250)mJystat.errorfloatnullableS350? SPIRE/Herschel 350um band flux density at 355.9 {mu}m (S350)mJyphot.flux.density;em.mm.750-1500GHzfloatnullablee_S350? SPIRE 350um flux uncertainty (dS350)mJystat.errorfloatnullableS500? SPIRE/Herschel 500um band flux uncertainty at 511.3 {mu}m (S500)mJyphot.flux.density;em.mm.400-750GHzfloatnullablee_S500? SPIRE 500um flux uncertainty (S500)mJystat.errorfloatnullableIDSpitzer/MIPS-24 ID designation (ID)meta.id;meta.maincharJ/MNRAS/513/1175/table5msStellar population synthesis physical property results for main- dusty starburstsrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzRedshift (redshift) (1)src.redshiftfloatlogLtirTotal IR luminosity (Ltir) (2)log(solLum)phys.luminosity;em.IRfloate_logLtirMean uncertainty of logLtir (dLtir)log(solLum)stat.errorfloatlogM*syStellar Mass derived with Synthesizer code (Ms_sy)log(solMass)phys.massfloate_logM*syMean uncertainty of logM*sy (dMs_sy)log(solMass)stat.errorfloatlogM*ciStellar Mass derived with CIGALE code (Ms_ci)log(solMass)phys.massfloate_logM*ciMean uncertainty of logM*ci (dMs_ci)log(solMass)stat.errorfloatlogSFRsySFR averaged over 10 Myr derived with Synthesizer code (SFR_sy)log(solMass.yr**-1)phys.SFRfloate_logSFRsyMean uncertainty of logSFRsy (dSFR_sy)log(solMass.yr**-1)stat.errorfloatlogSFRciSFR averaged over 10 Myr derived with CIGALE code (SFR_ci)log(solMass.yr**-1)phys.SFRfloate_logSFRciMean uncertainty of logSFRci (dSFR_ci)log(solMass.yr**-1)stat.errorfloatAVysyThe attenuation in V band of the young population A^you^_V_ derived with Synthesizer code (Avy_sy)magphys.absorptionfloate_AVysyMean uncertainty of AVysy (dAvy_sy)magstat.errorfloatAVyciThe attenuation in V band of the young population A^you^_V_ derived with CIGALE code (Avy_ci)magphys.absorptionfloate_AVyciMean uncertainty of AVyci (dAvy_ci)magstat.errorfloatAgeysyEstimated age of the young population t_you_ derived with Synthesizer code (Agy_sy)Myrtime.ageinte_AgeysyMean uncertainty of Ageysy (dAgy_sy)Myrstat.errorintAgeyciEstimated age of the young population t_you_ derived with CIGALE code (Agy_ci)Myrtime.ageinte_AgeyciMean uncertainty of Ageyci (dAgy_ci)Myrstat.errorintTauysyYoung population e-folding time derived with Synthesizer code (Tay_sy)Gyrtime.scalefloate_TauysyMean uncertainty of Tauysy (dTay_sy)Gyrstat.errorfloatbsyBurst intensity as M*_you_/M* derived with Synthesizer code (bu_sy)phys.mass;arith.ratiointe_bsyMean uncertainty of bsy (dbu_sy)stat.errorintbciBurst intensity as M*_you_/M* derived with CIGALE code (bu_ci)phys.mass;arith.ratiointe_bciMean uncertainty of bci (dbu_ci)stat.errorintAVosyThe attenuation in V band of the old population A^old^_V_ derived with Synthesizer code (Avo_sy)magphys.absorptionfloate_AVosyMean uncertainty of AVosy (dAvo_sy)magstat.errorfloatAVociThe attenuation in V band of the old population A^old^_V_ derived with CIGALE code (Avo_ci)magphys.absorptionfloate_AVociMean uncertainty of AVoci (dAvo_ci)magstat.errorfloatAgeosyEstimated age of the old population t_old_ derived with Synthesizer code (Ago_sy)Gyrtime.agefloate_AgeosyMean uncertainty of Ageosy (dAgo_sy)Gyrstat.errorfloatAgeociEstimated age of the old population t_old_ derived with CIGALE code (Ago_ci)Gyrtime.agefloate_AgeociMean uncertainty of Ageoci (dAgo_ci)Gyrstat.errorfloatTauosyOld population e-folding time derived with Synthesizer code (Tao_sy)Myrtime.scaleinte_TauosyMean uncertainty of Tauosy (dTao_sy)Myrstat.errorintTauociOld population e-folding time derived with CIGALE code (Tao_ci)Myrtime.scaleinte_TauociMean uncertainty of Tauoci (dTao_ci)Myrstat.errorintIDSpitzer/MIPS-24 ID designation (ID)meta.id;meta.maincharJ/MNRAS/513/1175/table5csStellar population synthesis physical property results for complementary- dusty starburstszRedshift (redshift) (1)src.redshiftfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlogLtirTotal IR luminosity (Ltir) (2)log(solLum)phys.luminosity;em.IRfloate_logLtirMean uncertainty of logLtir (dLtir)log(solLum)stat.errorfloatlogM*syStellar Mass derived with Synthesizer code (Ms_sy)log(solMass)phys.massfloate_logM*syMean uncertainty of logM*sy (dMs_sy)log(solMass)stat.errorfloatlogM*ciStellar Mass derived with CIGALE code (Ms_ci)log(solMass)phys.massfloate_logM*ciMean uncertainty of logM*ci (dMs_ci)log(solMass)stat.errorfloatlogSFRsySFR averaged over 10 Myr derived with Synthesizer code (SFR_sy)log(solMass.yr**-1)phys.SFRfloate_logSFRsyMean uncertainty of logSFRsy (dSFR_sy)log(solMass.yr**-1)stat.errorfloatlogSFRciSFR averaged over 10 Myr derived with CIGALE code (SFR_ci)log(solMass.yr**-1)phys.SFRfloate_logSFRciMean uncertainty of logSFRci (dSFR_ci)log(solMass.yr**-1)stat.errorfloatAVysyThe attenuation in V band of the young population A^you^_V_ derived with Synthesizer code (Avy_sy)magphys.absorptionfloate_AVysyMean uncertainty of AVysy (dAvy_sy)magstat.errorfloatAVyciThe attenuation in V band of the young population A^you^_V_ derived with CIGALE code (Avy_ci)magphys.absorptionfloate_AVyciMean uncertainty of AVyci (dAvy_ci)magstat.errorfloatAgeysyEstimated age of the young population t_you_ derived with Synthesizer code (Agy_sy)Myrtime.ageinte_AgeysyMean uncertainty of Ageysy (dAgy_sy)Myrstat.errorintAgeyciEstimated age of the young population t_you_ derived with CIGALE code (Agy_ci)Myrtime.ageinte_AgeyciMean uncertainty of Ageyci (dAgy_ci)Myrstat.errorintTauysyYoung population e-folding time derived with Synthesizer code (Tay_sy)Gyrtime.scalefloatAgeosyEstimated age of the old population t_old_ derived with Synthesizer code (Ago_sy)Gyrtime.agefloate_TauysyMean uncertainty of Tauysy (dTay_sy)Gyrstat.errorfloatbsyBurst intensity as M*_you_/M* derived with Synthesizer code (bu_sy)phys.mass;arith.ratiointe_bsyMean uncertainty of bsy (dbu_sy)stat.errorintbciBurst intensity as M*_you_/M* derived with CIGALE code (bu_ci)phys.mass;arith.ratiointe_bciMean uncertainty of bci (dbu_ci)stat.errorintAVosyThe attenuation in V band of the old population A^old^_V_ derived with Synthesizer code (Avo_sy)magphys.absorptionfloate_AVosyMean uncertainty of AVosy (dAvo_sy)magstat.errorfloatAVociThe attenuation in V band of the old population A^old^_V_ derived with CIGALE code (Avo_ci)magphys.absorptionfloate_AVociMean uncertainty of AVoci (dAvo_ci)magstat.errorfloate_AgeosyMean uncertainty of Ageosy (dAgo_sy)Gyrstat.errorfloatAgeociEstimated age of the old population t_old_ derived with CIGALE code (Ago_ci)Gyrtime.agefloate_AgeociMean uncertainty of Ageoci (dAgo_ci)Gyrstat.errorfloatTauosyOld population e-folding time derived with Synthesizer code (Tao_sy)Myrtime.scaleinte_TauosyMean uncertainty of Tauosy (dTao_sy)Myrstat.errorintTauociOld population e-folding time derived with CIGALE code (Tao_ci)Myrtime.scaleinte_TauociMean uncertainty of Tauoci (dTao_ci)Myrstat.errorintIDSpitzer/MIPS-24 ID designation (ID)meta.id;meta.mainchar