J/ApJ/692/556ivo://CDS.VizieR/J/ApJ/692/556doi:10.26093/cds/vizier.16920556CDSRieke G.H.Alonso-Herrero A.Weiner B.J.Perez-Gonzalez P.G.,Blaylock M.Donley J.L.Marcillac D.2017-07-05T06:59:10Z2011-04-11T09:37:44ZCDS support team

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

cds-question@unistra.frgalaxiesinfrared-sourcesspectral-energy-distributionWe show that measures of star formation rates (SFRs) for infrared galaxies using either single-band 24um or extinction-corrected Pa{alpha} luminosities are consistent in the total infrared luminosity =L(IR)~10^10^L_{{sun}}_ range. As a part of this work, we constructed spectral energy distribution templates for eleven luminous and ultraluminous purely star forming infrared galaxies and over the spectral range 0.4um to 30cm. We use these templates and the SINGS data to construct average templates from 5um to 30cm for infrared galaxies with L(IR)=5x10^9^ to 10^13^L_{{sun}}_.2009ApJ...692..556Rhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/692/556CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/ApJ/701/1398 : SFR for starburst galaxies (Sargsyan+, 2009)J/ApJ/656/770 : Mid-IR spectrum of star-forming galaxies (Smith+, 2007)J/ApJ/619/755 : Modeling starburst SEDs (Dopita+, 2005)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/692/556https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/692/556http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/692/556https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/692/556https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/692/556http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/692/556GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapInfrareddefaultJ/ApJ/692/556/table3Individual galaxy templatesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelengthumem.wldoubleN1614NGC 1614 flux densityJyphot.flux.densityfloatN2369NGC 2369 flux densityJyphot.flux.densityfloatN3256NGC 3256 flux densityJyphot.flux.densitydoubleN4194NGC 4194 flux densityJyphot.flux.densityfloatI12112IRAS 12112+0305 flux densityJyphot.flux.densitydoubleI14348IRAS 14348-1447 flux densityJyphot.flux.densitydoubleI17208IRAS 17208-0018 flux density (1)Jyphot.flux.densitydoubleI22491IRAS 22491-1808 flux densityJyphot.flux.densitydoubleArp220Arp 220 flux densityJyphot.flux.densitydoubleESO320ESO 320-G30 flux densityJyphot.flux.densityfloatZ49-57Zw 049-057 flux densityJyphot.flux.densitydoubleJ/ApJ/692/556/table4Average templatesrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambdaWavelengthumem.wldoubleF09.75Flux density for logL(IR)=9.75L_{sun}_ (1)Jyphot.flux.densityfloatF10.00Flux density for logL(IR)=10.00L_{sun}_ (1)Jyphot.flux.densitydoubleF10.25Flux density for logL(IR)=10.25L_{sun}_ (1)Jyphot.flux.densitydoubleF10.50Flux density for logL(IR)=10.50L_{sun}_ (1)Jyphot.flux.densitydoubleF10.75Flux density for logL(IR)=10.75L_{sun}_ (1)Jyphot.flux.densitydoubleF11.00Flux density for logL(IR)=11.00L_{sun}_ (1)Jyphot.flux.densitydoubleF11.25Flux density for logL(IR)=11.25L_{sun}_ (1)Jyphot.flux.densitydoubleF11.50Flux density for logL(IR)=11.50L_{sun}_ (1)Jyphot.flux.densitydoubleF11.75Flux density for logL(IR)=11.75L_{sun}_ (1)Jyphot.flux.densitydoubleF12.00Flux density for logL(IR)=12.00L_{sun}_ (1)Jyphot.flux.densitydoubleF12.25Flux density for logL(IR)=12.25L_{sun}_ (1)Jyphot.flux.densitydoubleF12.50Flux density for logL(IR)=12.50L_{sun}_ (1)Jyphot.flux.densitydoubleF12.75Flux density for logL(IR)=12.75L_{sun}_ (1)Jyphot.flux.densitydoubleF13.00Flux density for logL(IR)=13.00L_{sun}_ (1)Jyphot.flux.densitydouble