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Fermi–LAT Observations toward the Galactic Center

Published online by Cambridge University Press:  09 February 2017

Simona Murgia
Simona Murgia*
Affiliation:
Department of Physics and Astronomy, University of California, Irvine, CA 92697, USA email: smurgia@uci.edu
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Abstract

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The inner region of the Milky Way is one of the most interesting and complex regions of the γ-ray sky. Intense interstellar emission and point sources contribute to it, as well as other potential components such as an unresolved population of point sources and dark matter. In recent years, claims have been made of an excess consistent with a dark matter annihilation signal in the data collected with the Fermi Large Area Telescope (Fermi–LAT). Although these results are intriguing, the complexity involved in modeling the foreground and background emission from conventional astrophysical sources of γ-rays makes a conclusive interpretation of these results challenging. In these proceedings, I discuss Fermi–LAT observations of the Galactic center region, the methodology for point source detection and treatment of the interstellar emission, the characterization of the GeV excess, and implications for dark matter.

Keywords

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Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 11 , Symposium S322: The Multi-Messenger Astrophysics of the Galactic Centre , July 2016 , pp. 11 - 20
Copyright
Copyright © International Astronomical Union 2017 

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