J/A+A/534/A54ivo://CDS.VizieR/J/A+A/534/A54doi:10.26093/cds/vizier.35340054CDSStrong A.W.Orlando E.Jaffe T.R.CDS support team

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

cds-question@unistra.frastronomical-modelsgamma-ray-astronomyWe exploit synchrotron radiation to constrain the low-energy interstellar electron spectrum, using various radio surveys and connecting with electron data from Fermi-LAT and other experiments. The GALPROP programme for cosmic-ray propagation, gamma-ray and synchrotron radiation is used. Secondary electrons and positrons are included. Propagation models based on cosmic-ray and gamma-ray data are tested against synchrotron data from 22MHz to 94GHz.2011A&A...534A..54Shttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/534/A54CatalogResearchIsServedByTAP VizieR generic servicehttps://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/A+A/534/A54https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/A+A/534/A54http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/A+A/534/A54https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/A+A/534/A54https://vizier.iucaa.in/viz-bin/votable?-source=J/A+A/534/A54http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/A+A/534/A54GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapGamma-raydefault