J/A+A/653/A149ivo://CDS.VizieR/J/A+A/653/A149doi:10.26093/cds/vizier.36530149CDSBoquien M.Salim S.2022-01-19T09:14:51Z2021-09-24T08:00:59ZCDS support team

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

cds-question@unistra.frgalaxiesinfrared-sourcesastronomical-modelsphotometryThe infrared (IR) emission of dust heated by stars provides critical information for galaxy evolution studies. Unfortunately, observations are often limited to the mid-IR, making templates a necessity. Previously published templates were based on small samples of luminous galaxies, which are not necessarily representative of normal star-forming galaxies. We constructed new-generation dust templates, including instrument-specific relations and software tools that facilitate the estimation of the total IR (TIR) luminosity as well as obscured and unobscured star formation rate (SFR) based on one or several fluxes up to z=4. For the first time, the templates include a dependence on both TIR luminosity and the specific SFR (sSFR), thereby increasing their reliability and utility for a wide range of galaxies. We also provide formulae for calculating TIR luminosities and SFR from JWST F2100W observations at 0<z<2. Our templates are based on 2584 normal star-forming galaxies spanning a wide range of stellar mass and sSFR, including sSFRs typical at higher redshifts. IR spectra and properties were obtained using cigale and the physically motivated Draine & Li (2007ApJ...657..810D) dust models. The photometry from the GALEX-SDSS-WISE Legacy Catalog was supplemented with 2MASS and Herschel-ATLAS, up to 19 bands from FUV to 500um. The shape of the dust spectrum varies with TIR luminosity, but also independently with sSFR. Remarkably precise estimates of the dust luminosity are possible with a single band over the rest-frame 12-17um and 55-130um. We validate single-band estimates on diverse populations, including local luminous IR galaxies, and find no significant systematic errors. Using two or more bands simultaneously yields the unbiased estimation of the TIR luminosity, even of star-forming dwarfs. We obtain fresh insights regarding the interplay between monochromatic IR luminosities, spectral shapes, and physical properties, and we constructed new templates and estimators of the dust luminosity and SFR. We provide software for generating templates and estimating these quantities based on 1-4 bands from WISE, JWST, Spitzer, and Herschel, up to z=4.2021A&A...653A.149Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/653/A149CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/653/A149https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/653/A149http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/653/A149https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/653/A149https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/653/A149http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/653/A149GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapInfrareddefaultJ/A+A/653/A149/table1Coefficients to estimate LTIR and the SFR from one up to four bands up to z=4recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintzRedshift (redshift)src.redshiftfloatmLTIRIRAC4? Coefficient for band spitzer.irac.ch4 to estimate LTIR (m_LTIR[spitzer.irac.ch4])stat.fit.paramdoublenullablemLTIRF2550W? Coefficient for band jwst.miri.F2550W to estimate LTIR (m_LTIR[jwst.miri.F2550W])stat.fit.paramdoublenullablemLTIRF2100W? Coefficient for band jwst.miri.F2100W to estimate LTIR (m_LTIR[jwst.miri.F2100W])stat.fit.paramdoublenullablemLTIRF1800W? Coefficient for band jwst.miri.F1800W to estimate LTIR (m_LTIR[jwst.miri.F1800W])stat.fit.paramdoublenullablemLTIRF1500W? Coefficient for band jwst.miri.F1500W to estimate LTIR (m_LTIR[jwst.miri.F1500W])stat.fit.paramdoublenullablemLTIRF1280W? Coefficient for band jwst.miri.F1280W to estimate LTIR (m_LTIR[jwst.miri.F1280W])stat.fit.paramdoublenullablemLTIRF1130W? Coefficient for band jwst.miri.F1130W to estimate LTIR (m_LTIR[jwst.miri.F1130W])stat.fit.paramdoublenullablemLTIRF1000W? Coefficient for band jwst.miri.F1000W to estimate LTIR (m_LTIR[jwst.miri.F1000W])stat.fit.paramdoublenullablemLTIRF770W? Coefficient for band jwst.miri.F770W to estimate LTIR (m_LTIR[jwst.miri.F770W])stat.fit.paramdoublenullablemLTIRSPIREPLW? Coefficient for band herschel.spire.PLW to estimate LTIR (m_LTIR[herschel.spire.PLW])stat.fit.paramdoublenullablemLTIRSPIREPMW? Coefficient for band herschel.spire.PLW to estimate LTIR (m_LTIR[herschel.spire.PMW])stat.fit.paramdoublenullablemLTIRSPIREPSW? Coefficient for band herschel.spire.PSW to estimate LTIR (m_LTIR[herschel.spire.PSW])stat.fit.paramdoublenullablemLTIRPACS160? Coefficient for band herschel.pacs.160 to estimate LTIR (m_LTIR[herschel.pacs.160])stat.fit.paramdoublenullablemLTIRPACS100? Coefficient for band herschel.pacs.100 to estimate LTIR (m_LTIR[herschel.pacs.100])stat.fit.paramdoublenullablemLTIRPACS70? Coefficient for band herschel.pacs.70 to estimate LTIR (m_LTIR[herschel.pacs.70])stat.fit.paramdoublenullablemLTIRMIPS24? Coefficient for band spitzer.mips.24 to estimate LTIR (m_LTIR[spitzer.mips.24])stat.fit.paramdoublenullablemLTIRWISE3? Coefficient for band WISE3 to estimate LTIR (m_LTIR[WISE3])stat.fit.paramdoublenullablemLTIRWISE4? Coefficient for band WISE4 to estimate LTIR (m_LTIR[WISE4])stat.fit.paramdoublenullablenLTIRn coefficient to estimate LTIR (n_LTIR)stat.fit.paramdoublemSFRIRAC4? Coefficient for band spitzer.irac.ch4 to estimate the SFR (m_SFR[spitzer.irac.ch4])stat.fit.paramdoublenullablemSFRF2550W? Coefficient for band jwst.miri.F2550W to estimate the SFR (m_SFR[jwst.miri.F2550W])stat.fit.paramdoublenullablemSFRF2100W? Coefficient for band jwst.miri.F2100W to estimate the SFR (m_SFR[jwst.miri.F2100W])stat.fit.paramdoublenullablemSFRF1800W? Coefficient for band jwst.miri.F1800W to estimate the SFR (m_SFR[jwst.miri.F1800W])stat.fit.paramdoublenullablemSFRF1500W? Coefficient for band jwst.miri.F1500W to estimate the SFR (m_SFR[jwst.miri.F1500W])stat.fit.paramdoublenullablemSFRF1280W? Coefficient for band jwst.miri.F1280W to estimate the SFR (m_SFR[jwst.miri.F1280W])stat.fit.paramdoublenullablemSFRF1130W? Coefficient for band jwst.miri.F1130W to estimate the SFR (m_SFR[jwst.miri.F1130W])stat.fit.paramdoublenullablemSFRF1000W? Coefficient for band jwst.miri.F1000W to estimate the SFR (m_SFR[jwst.miri.F1000W])stat.fit.paramdoublenullablemSFRF770W? Coefficient for band jwst.miri.F770W to estimate the SFR (m_SFR[jwst.miri.F770W])stat.fit.paramdoublenullablemSFRSPIREPLW? Coefficient for band herschel.spire.PLW to estimate the SFR (m_SFR[herschel.spire.PLW])stat.fit.paramdoublenullablemSFRSPIREPMW? Coefficient for band herschel.spire.PMW to estimate the SFR (m_SFR[herschel.spire.PMW])stat.fit.paramdoublenullablemSFRSPIREPSW? Coefficient for band herschel.spire.PSW to estimate the SFR (m_SFR[herschel.spire.PSW])stat.fit.paramdoublenullablemSFRPACS160? Coefficient for band herschel.pacs.160 to estimate the SFR (m_SFR[herschel.pacs.160])stat.fit.paramdoublenullablemSFRPACS100? Coefficient for band herschel.pacs.100 to estimate the SFR (m_SFR[herschel.pacs.100])stat.fit.paramdoublenullablemSFRPACS70? Coefficient for band herschel.pacs.70 to estimate the SFR (m_SFR[herschel.pacs.70])stat.fit.paramdoublenullablemSFRMIPS24? Coefficient for band spitzer.mips.24 to estimate the SFR (m_SFR[spitzer.mips.24])stat.fit.paramdoublenullablemSFRWISE3? Coefficient for band WISE3 to estimate the SFR (m_SFR[WISE3])stat.fit.paramdoublenullablemSFRWISE4? Coefficient for band WISE4 to estimate the SFR (m_SFR[WISE4])stat.fit.paramdoublenullablenSFRn coefficient to estimate the SFR (n_SFR)stat.fit.paramdoubleJ/A+A/653/A149/table3Coefficients to estimate LTIR and the SFR from a single band and the sSFR up to z=4zRedshift (redshift)src.redshiftfloatmSFRF1800W? Coefficient for band jwst.miri.F1800W to estimate the SFR (m_SFR[jwst.miri.F1800W])stat.fit.paramdoublenullablemSFRF1500W? Coefficient for band jwst.miri.F1500W to estimate the SFR (m_SFR[jwst.miri.F1500W])stat.fit.paramdoublenullablemSFRF1280W? Coefficient for band jwst.miri.F1280W to estimate the SFR (m_SFR[jwst.miri.F1280W])stat.fit.paramdoublenullablemSFRF1130W? Coefficient for band jwst.miri.F1130W to estimate the SFR (m_SFR[jwst.miri.F1130W])stat.fit.paramdoublenullablemSFRF1000W? Coefficient for band jwst.miri.F1000W to estimate the SFR (m_SFR[jwst.miri.F1000W])stat.fit.paramdoublenullablemSFRF770W? Coefficient for band jwst.miri.F770W to estimate the SFR (m_SFR[jwst.miri.F770W])stat.fit.paramdoublenullablemSFRSPIREPLW? Coefficient for band herschel.spire.PLW to estimate the SFR (m_SFR[herschel.spire.PLW])stat.fit.paramdoublenullablemSFRSPIREPMW? Coefficient for band herschel.spire.PMW to estimate the SFR (m_SFR[herschel.spire.PMW])stat.fit.paramdoublenullablemSFRSPIREPSW? Coefficient for band herschel.spire.PSW to estimate the SFR (m_SFR[herschel.spire.PSW])stat.fit.paramdoublenullablemSFRPACS160? Coefficient for band herschel.pacs.160 to estimate the SFR (m_SFR[herschel.pacs.160])stat.fit.paramdoublenullablemSFRPACS100? Coefficient for band herschel.pacs.100 to estimate the SFR (m_SFR[herschel.pacs.100])stat.fit.paramdoublenullablemSFRPACS70? Coefficient for band herschel.pacs.70 to estimate the SFR (m_SFR[herschel.pacs.70])stat.fit.paramdoublenullablemSFRmips24? Coefficient for band spitzer.mips.24 to estimate the SFR (m_SFR[spitzer.mips.24])stat.fit.paramdoublenullablemSFRWISE3? Coefficient for band WISE3 to estimate the SFR (m_SFR[WISE3])stat.fit.paramdoublenullablemSFRWISE4? Coefficient for band WISE4 to estimate the SFR (m_SFR[WISE4])stat.fit.paramdoublenullablesSFRs coefficient for the sSFR to estimate the SFR (s_SFR)stat.fit.paramdoublenSFRn coefficient to estimate the SFR (n_SFR)stat.fit.paramdoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintmLTIRIRAC4? Coefficient for band spitzer.irac.ch4 to estimate LTIR (m_LTIR[spitzer.irac.ch4])stat.fit.paramdoublenullablemLTIRF2550W? Coefficient for band jwst.miri.F2550W to estimate LTIR (m_LTIR[jwst.miri.F2550W])stat.fit.paramdoublenullablemLTIRF2100W? Coefficient for band jwst.miri.F2100W to estimate LTIR (m_LTIR[jwst.miri.F2100W])stat.fit.paramdoublenullablemLTIRF1800W? Coefficient for band jwst.miri.F1800W to estimate LTIR (m_LTIR[jwst.miri.F1800W])stat.fit.paramdoublenullablemLTIRF1500W? Coefficient for band jwst.miri.F1500W to estimate LTIR (m_LTIR[jwst.miri.F1500W])stat.fit.paramdoublenullablemLTIRF1280W? Coefficient for band jwst.miri.F1280W to estimate LTIR (m_LTIR[jwst.miri.F1280W])stat.fit.paramdoublenullablemLTIRF1130W? Coefficient for band jwst.miri.F1130W to estimate LTIR (m_LTIR[jwst.miri.F1130W])stat.fit.paramdoublenullablemLTIRF1000W? Coefficient for band jwst.miri.F1000W to estimate LTIR (m_LTIR[jwst.miri.F1000W])stat.fit.paramdoublenullablemLTIRF770W? Coefficient for band jwst.miri.F770W to estimate LTIR (m_LTIR[jwst.miri.F770W])stat.fit.paramdoublenullablemLTIRSPIREPLW? Coefficient for band herschel.spire.PLW to estimate LTIR (m_LTIR[herschel.spire.PLW])stat.fit.paramdoublenullablemLTIRSPIREPMW? Coefficient for band herschel.spire.PMW to estimate LTIR (m_LTIR[herschel.spire.PMW])stat.fit.paramdoublenullablemLTIRSPIREPSW? Coefficient for band herschel.spire.PSW to estimate LTIR (m_LTIR[herschel.spire.PSW])stat.fit.paramdoublenullablemLTIRPACS160? Coefficient for band herschel.pacs.160 to estimate LTIR (m_LTIR[herschel.pacs.160])stat.fit.paramdoublenullablemLTIRPACS100? Coefficient for band herschel.pacs.100 to estimate LTIR (m_LTIR[herschel.pacs.100])stat.fit.paramdoublenullablemLTIRPACS70? Coefficient for band herschel.pacs.70 to estimate LTIR (m_LTIR[herschel.pacs.70])stat.fit.paramdoublenullablemLTIRMIPS24? Coefficient for band spitzer.mips.24 to estimate LTIR (m_LTIR[spitzer.mips.24])stat.fit.paramdoublenullablemLTIRWISE3? Coefficient for band WISE3 to estimate LTIR (m_LTIR[WISE3])stat.fit.paramdoublenullablemLTIRWISE4? Coefficient for band WISE4 to estimate LTIR (m_LTIR[WISE4])stat.fit.paramdoublenullablesLTIRs coefficient for the sSFR to estimate LTIR (s_LTIR)stat.fit.paramdoublenLTIRn coefficient to estimate LTIR (n_LTIR)stat.fit.paramdoublemSFRIRAC4? Coefficient for band spitzer.irac.ch4 to estimate the SFR (m_SFR[spitzer.irac.ch4])stat.fit.paramdoublenullablemSFRF2550W? Coefficient for band jwst.miri.F2550W to estimate the SFR (m_SFR[jwst.miri.F2550W])stat.fit.paramdoublenullablemSFRF2100W? Coefficient for band jwst.miri.F2100W to estimate the SFR (m_SFR[jwst.miri.F2100W])stat.fit.paramdoublenullable