Total infrared brightness and SFR in M33J/AJ/142/111ivo://CDS.VizieR/J/AJ/142/111doi:10.26093/cds/vizier.51420111CDSBoquien M.Calzetti D.Combes F.Henkel C.Israel F.Kramer C.,Relano M.Verley S.Van Der Werf P.Xilouris E.M.HERM33ES Team2013-02-19T11:31:49Z2013-02-01T15:30:25ZCDS support teamCDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, Francecds-question@unistra.frgalaxiesinfrared-sourcesextinctionIn the context of the Herschel HERM33ES open time key project, we are studying the moderately inclined Scd local group galaxy M33 which is located only 840kpc away. In this article, using Spitzer and Herschel data ranging from 3.6um to 500um, along with HI, H{alpha} maps, and Galaxy Evolution Explorer ultraviolet data, we have studied the emission of the dust at the high spatial resolution of 150pc. Combining Spitzer and Herschel bands, we have provided new, inclination-corrected, resolved estimators of the total infrared brightness and of the star formation rate from any combination of these bands. ---------------------------------------------------------- RA (2000) DE Designation(s) ---------------------------------------------------------- 01 33 50.90 +30 39 35.8 M33 = NGC 598 ----------------------------------------------------------2011AJ....142..111Bhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/142/111CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/142/111https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/142/111http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/142/111https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/142/111https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/142/111http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/142/111GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapInfrareddefault
J/AJ/142/111/table1Coefficients of the fit of the combination of any number of Spitzer and Herschel bands from 8.0um to 500um to estimate the total IR luminositynNumber of bandsmeta.numberintc160? Coefficient for best fit to Herschel/PACS 160 micron band (1)stat.fit.paramfloatnullablee_c160? Uncertainty in c160stat.errorfloatnullablec250? Coefficient for best fit to Herschel/SPIRE 250 micron band (1)stat.fit.paramfloatnullablee_c250? Uncertainty in c250stat.errorfloatnullablec350? Coefficient for best fit to Herschel/SPIRE 350 micron band (1)stat.fit.paramfloatnullablee_c350? Uncertainty in c350stat.errorfloatnullablec500? Coefficient for best fit to Herschel/SPIRE 500 micron band (1)stat.fit.paramfloatnullablee_c500? Uncertainty in c500stat.errorfloatnullablebRelationship constant (1)stat.fit.paramfloate_b? Uncertainty in bstat.errorfloatnullablesigmaStandard deviation of the total IR luminosity (table1) or SFR (table2) around best fitstat.stdev;phys.luminosity;em.IRfloatrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintc8? Coefficient for best fit to Spitzer/IRAC 8 micron band (1)stat.fit.paramfloatnullablee_c8? Uncertainty in c8stat.errorfloatnullablec24? Coefficient for best fit to Spitzer/MIPS 24 micron band (1)stat.fit.paramfloatnullablee_c24? Uncertainty in c24stat.errorfloatnullablec70? Coefficient for best fit to Spitzer/MIPS 70 micron band (1)stat.fit.paramfloatnullablee_c70? Uncertainty in c70stat.errorfloatnullablec100? Coefficient for best fit to Herschel/PACS 100 micron band (1)stat.fit.paramfloatnullablee_c100? Uncertainty in c100stat.errorfloatnullable
J/AJ/142/111/table2Coefficients of the fit of the combination of any number of Spitzer and Herschel bands from 8.0um to 500um to estimate the SFR in M_{sun}_/yr/kpc^2recnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintc8? Coefficient for best fit to Spitzer/IRAC 8 micron band (1)stat.fit.paramfloatnullablee_c8? Uncertainty in c8stat.errorfloatnullablec24? Coefficient for best fit to Spitzer/MIPS 24 micron band (1)stat.fit.paramfloatnullablee_c24? Uncertainty in c24stat.errorfloatnullablenNumber of bandsmeta.numberintc70? Coefficient for best fit to Spitzer/MIPS 70 micron band (1)stat.fit.paramfloatnullablee_c70? Uncertainty in c70stat.errorfloatnullablec100? Coefficient for best fit to Herschel/PACS 100 micron band (1)stat.fit.paramfloatnullablee_c100? Uncertainty in c100stat.errorfloatnullablec160? Coefficient for best fit to Herschel/PACS 160 micron band (1)stat.fit.paramfloatnullablee_c160? Uncertainty in c160stat.errorfloatnullablec250? Coefficient for best fit to Herschel/SPIRE 250 micron band (1)stat.fit.paramfloatnullablee_c250? Uncertainty in c250stat.errorfloatnullablec350? Coefficient for best fit to Herschel/SPIRE 350 micron band (1)stat.fit.paramfloatnullablee_c350? Uncertainty in c350stat.errorfloatnullablec500? Coefficient for best fit to Herschel/SPIRE 500 micron band (1)stat.fit.paramfloatnullablee_c500? Uncertainty in c500stat.errorfloatnullablebRelationship constant (1)stat.fit.paramfloate_b? Uncertainty in bstat.errorfloatnullablesigmaStandard deviation of the total IR luminosity (table1) or SFR (table2) around best fitstat.stdev;phys.luminosity;em.IRfloat