Francesca Calore, Mattia Di Mauro, Fiorenza Donato
Published 2014-12-16Version 1
Gamma rays from young pulsars and milli-second pulsars are expected to contribute to the diffuse gamma-ray emission measured by the {\it Fermi} Large Area Telescope (LAT) at high latitudes. We derive the contribution of the pulsars undetected counterpart by using information from radio to gamma rays and we show that they explain only a small fraction of the isotropic diffuse gamma-ray background.
Comments: Proceeding of the Neutrino Oscillation Workshop, NOW 2014. 3 pages, 2 figures
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