J/MNRAS/470/2539ivo://CDS.VizieR/J/MNRAS/470/2539doi:10.26093/cds/vizier.74702539CDSPopescu C.C.Yang R.Tuffs R.J.Natale G.Rushton M.Aharonian F.2024-08-17T20:19:49Z2017-07-13T08:45:02ZCDS support team

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

cds-question@unistra.frastronomical-modelsgalaxiesphotometryWe provide a library for the ultraviolet - submillimetre (submm) interstellar radiation fields (ISRFs) of the Milky Way (MW), derived from modelling COBE, IRAS and Planck maps of the all-sky emission in the near-, mid-, far-infrared and submm. The library was produced using the axisymmetric radiative transfer model that we have previously implemented to model the panchromatic spectral energy distributions (SEDs) of star-forming galaxies in the nearby universe, but with a new methodology allowing for optimization of the radial and vertical geometry of stellar emissivity and dust opacity, as deduced from the highly resolved emission seen from the vantage point of the Sun.2017MNRAS.470.2539Phttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/MNRAS/470/2539CatalogResearchIsServedByTAP VizieR generic servicerelated-toJ/A+A/527/A109 : Dust and PAH emission SEDs of disk galaxies (Popescu+, 2011)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/MNRAS/470/2539https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/MNRAS/470/2539http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/MNRAS/470/2539https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/MNRAS/470/2539https://vizier.iucaa.in/viz-bin/votable?-source=J/MNRAS/470/2539http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/MNRAS/470/2539GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapOpticaldefaultJ/MNRAS/470/2539/modelsModels for RFs in direct stellar lightrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintBandBand (1)instr.bandpasscharr(pc)[0/24000] Galactocentric radial positionpcpos.distance;pos.galactocentricintz(pc)[0/10000] Galactocentric vertical positionpcpos.distance;pos.cartesian.z;pos.galactocentricinturadEnergy density of radiation fields (erg/pc^3^/{AA})uJ.pc**-3.nm**-1phys.energy.densitydoubleEabsEnergy absorbed (erg/s/pc^3^/{AA})uW.pc**-3.nm**-1phys.emissivitydouble