Fine-scale angular fluctuations in the high-energy extragalactic gamma-ray background from blazars.

Details Fine-scale angular fluctuations in the high-energy extragalactic gamma-ray background from blazars. Fine-scale angular fluctuations in the high-energy extragalactic gamma-ray background from blazars.

Dec 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996jkps...29..714h&link_type=abstract

Journal of the Korean Physical Society, Vol. 29, No. 6, p. 714 - 718

Physics

Gamma-Ray Background: Fluctuations, Gamma-Ray Background: Blazars

Scientific paper

Blazars, a class of active galactic nuclei recently discovered by the EGRET mounted on the Compton Gamma-Ray Observatory as emitting very high-energy γ-rays, have been proposed as the sources for the multi-GeV extragalactic γ-ray background. Using a relation between the radio and the γ-ray luminosities for these sources, the authors present simulated fine-scale angular fluctuation patterns in this background as functions of observational energies. They predict some features, observable by high-resolution γ-rays telescopes, which may identify blazars as the major contributors in forming the high-energy extragalactic γ-ray background.

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