Unidentified GeV Sources as a Cosmological Population

Details Unidentified GeV Sources as a Cosmological Population Unidentified GeV Sources as a Cosmological Population

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21335504p&link_type=abstract

American Astronomical Society, AAS Meeting #213, #355.04; Bulletin of the American Astronomical Society, Vol. 41, p.497

Mathematics

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Scientific paper

The faint, marginally resolved, poorly-localized end of the distribution of Fermi point sources is guaranteed to include, as was the case for EGRET, an appreciable fraction unidentified sources. Most high-latitude Fermi unidentified sources will likely be extragalactic. I discuss how we can use the GeV properties of these objects, in combination with constraints placed by the extragalactic gamma-ray background, to derive clues about the nature of a cosmological population of unidentified sources, even without positional associations with lower-energy counterparts.

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