Evaluation of the Celestial Foreground in Determination of the Extragalactic Diffuse Gamma-ray Emission

Details Evaluation of the Celestial Foreground in Determination of the Extragalactic Diffuse Gamma-ray Emission Evaluation of the Celestial Foreground in Determination of the Extragalactic Diffuse Gamma-ray Emission

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006head....9.1801m&link_type=abstract

American Astronomical Society, HEAD meeting #9, #18.01; Bulletin of the American Astronomical Society, Vol. 38, p.381

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The intensity and spectrum of the diffuse extragalactic emission in high-energy gamma rays have attracted long-standing experimental and theoretical interest. They relate to the luminosity functions of blazars and other active galaxies, as unresolved point sources, and to any truly diffuse cosmological component. Any evaluation of the extragalactic diffuse emission relies on detailed understanding of the calibration and backgrounds of the gamma-ray telescope as well as the intensities of the foreground celestial components. We evaluate the celestial sources of the foreground and their impact on determination of the true diffuse extragalactic gamma-ray emission.

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