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• W596898119 abstract "We present a new method to characterize unresolved point sources (PSs), generalizing traditional template fits to account for non-Poissonian photon statistics. We apply this method to Fermi Large Area Telescope gamma-ray data to characterize PS populations at high latitudes and in the Inner Galaxy. We find that PSs (resolved and unresolved) account for ~50% of the total extragalactic gamma-ray background in the energy range ~1.9 to 11.9 GeV. Within 10$^circ$ of the Galactic Center with $|b| geq 2^circ$, we find that ~5-10% of the flux can be accounted for by a population of unresolved PSs, distributed consistently with the observed ~GeV gamma-ray excess in this region. The excess is fully absorbed by such a population, in preference to dark-matter annihilation. The inferred source population is dominated by near-threshold sources, which may be detectable in future searches." @default.
• W596898119 created "2016-06-24" @default.
• W596898119 creator A5015553898 @default.
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• W596898119 date "2016-02-04" @default.
• W596898119 modified "2023-10-17" @default.
• W596898119 title "Evidence for Unresolved<mml:math xmlns:mml=http://www.w3.org/1998/Math/MathML display=inline><mml:mi>γ</mml:mi></mml:math>-Ray Point Sources in the Inner Galaxy" @default.
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• W596898119 doi "https://doi.org/10.1103/physrevlett.116.051103" @default.
• W596898119 hasPubMedId "https://pubmed.ncbi.nlm.nih.gov/26894697" @default.
• W596898119 hasPublicationYear "2016" @default.
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