The contribution of blazars to the extragalactic diffuse γ-ray background

Details The contribution of blazars to the extragalactic diffuse γ-ray background The contribution of blazars to the extragalactic diffuse γ-ray background

May 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997aipc..410.1233m&link_type=abstract

The fourth compton symposium. AIP Conference Proceedings, Volume 410, pp. 1233-1237 (1997).

Computer Science

1

Active And Peculiar Galaxies And Related Systems, Background Radiations, Gamma-Ray Sources, Gamma-Ray Bursts

Scientific paper

We present results of a calculation of the blazar contribution to the extragalactic diffuse γ-ray background (EGRB) in the EGRET-energy range. Our model is based on the non-thermal emission processes known to be important in blazar jets, and on the unification scheme of radio-loud AGN. The background calculations place a lower limit of 5-16% AGN-contribution to the EGRB.

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