J/AJ/135/2245ivo://CDS.VizieR/J/AJ/135/2245doi:10.26093/cds/vizier.51352245CDSRieke G.H.Blaylock M.Decin L.Engelbracht C.Ogle P.Avrett E.,Carpenter J.Cutri R.M.Armus L.Gordon K.Gray R.O.Hinz J.Su K.,Willmer C.N.A.2017-06-19T07:57:12Z2011-02-04T12:27:37ZCDS support team

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

cds-question@unistra.frthe-suninfrared-astronomyspectroscopystandard-starsWe determine an absolute calibration for the Multiband Imaging Photometer for Spitzer 24um band and recommend adjustments to the published calibrations for Two Micron All Sky Survey (2MASS), Infrared Array Camera (IRAC), and IRAS photometry to put them on the same scale. We show that consistent results are obtained by basing the calibration on either an average A0V star spectral energy distribution (SED), or by using the absolutely calibrated SED of the Sun in comparison with solar-type stellar photometry (the solar analog method).2008AJ....135.2245Rhttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/AJ/135/2245CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+AS/113/237 : Ultraviolet Spectrum of the Sun (Samain, 1995)J/ApJS/181/351 : Solar flux model in 30-1300nm wavelength range (Killen+, 2009)J/A+A/525/A74 : Solar Atlas (Molaro+, 2011)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/AJ/135/2245https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/AJ/135/2245http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/AJ/135/2245https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/AJ/135/2245https://vizier.iucaa.in/viz-bin/votable?-source=J/AJ/135/2245http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/AJ/135/2245GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapInfrareddefaultJ/AJ/135/2245/table7Reference spectral energy distributions of the Sun and VegarecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintlambda[0.2/30] Wavelengthumem.wlfloatSunFlux density of the SunW.m**-2.nm**-1phot.flux.densitydoubleVegaFlux density of VegaW.m**-2.nm**-1phot.flux.densitydouble