J/MNRAS/482/560ivo://CDS.VizieR/J/MNRAS/482/560doi:10.26093/cds/vizier.74820560CDSMahajan S.Ashby M.L.N.Willner S.P.Barmby P.Fazio G.G.,Maragkoudakis A.Raychaudhury S.Zezas A.2024-08-19T20:15:17Z2022-01-18T14:29:18ZCDS support team

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

cds-question@unistra.frgalaxiesphotometryultraviolet-photometryWe present multiwavelength global star formation rate (SFR) estimates for 326 galaxies from the Star Formation Reference Survey in order to determine the mutual scatter and range of validity of different indicators. The widely used empirical SFR recipes based on 1.4GHz continuum, 8.0um polycyclic aromatic hydrocarbons (PAHs), and a combination of far-infrared (FIR) plus ultraviolet (UV) emission are mutually consistent with scatter of <~0.3dex. The scatter is even smaller, <~0.24dex, in the intermediate luminosity range 9.3<log(L_60um_/L_{sun}_)<10.7. The data prefer a non-linear relation between 1.4GHz luminosity and other SFR measures. PAH luminosity underestimates SFR for galaxies with strong UV emission. A bolometric extinction correction to far-UV luminosity yields SFR within 0.2dex of the total SFR estimate, but extinction corrections based on UV spectral slope or nuclear Balmer decrement give SFRs that may differ from the total SFR by up to 2dex. However, for the minority of galaxies with UV luminosity >5x10^9^L_{sun}_ or with implied far-UV extinction <1mag, the UV spectral slope gives extinction corrections with 0.22dex uncertainty.2019MNRAS.482..560Mhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/482/560CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/PASP/123/1011 : Star Formation Reference Survey (SFRS) (Ashby+, 2011)J/MNRAS/504/3831 : Stellar mass distribution of local star-forming galaxiesJ/MNRAS/506/3079 : Halpha and other SFR indicators (Kouroumpatzakis+, 2021)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/482/560https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/482/560http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/482/560https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/482/560https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/482/560http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/482/560GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapUVdefaultJ/MNRAS/482/560/table12GALEX data (table 1 ) and SFR measures (table 2) for SFRS galaxiesSimbadNameSimbad column added by the CDSmeta.idcharnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintSFRSGalaxy ID from Paper I (G1)meta.idintNameGalaxy namemeta.id;meta.maincharDistGalaxy distance from Paper I (G1)Mpcpos.distancefloatFUVGalex FUV magnitude (AB)magphot.mag;em.UV.100-200nmfloate_FUVFUV magnitude statistical uncertaintymagstat.errorfloatNUVGalex NUV magnitude (AB)magphot.mag;em.UVfloate_NUVNUV magnitude statistical uncertaintymagstat.errorfloatE(B-V)Milky Way colour excess (2)magphot.color.excessfloatlogSFRFUVlog SFR from FUV luminosity (2)log(solMass.yr**-1)phys.SFRfloatlogSFRNUVlog SFR from NUV luminosity (2)log(solMass.yr**-1)phys.SFRfloatlogSFR1.4GHzllog SFR from 1.4GHz linear relation (2)log(solMass.yr**-1)phys.SFRfloatlogSFR1.4GHznllog SFR from 1.4GHz non-linear relation (2)log(solMass.yr**-1)phys.SFRfloatlogSFRFIRlog SFR from FIR luminosity (2)log(solMass.yr**-1)phys.SFRfloatlogSFRPAHlog SFR from PAH luminosity (2)log(solMass.yr**-1)phys.SFRfloatlogSFRtotlog SFR from combined FIR and FUV (2)log(solMass.yr**-1)phys.SFRfloat