Abstract
We consider the emission of high-energy to very-high-energy gamma -rays in radio-quiet active Galactic nuclei (AGN) or the central regions of radio-loud AGN. We use our results to estimate the gamma -ray flux from the central regions of nearby AGN and then to calculate the contribution to the diffuse gamma -ray flux from unresolved AGN.
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More From: Journal of Physics G: Nuclear and Particle Physics
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