Sensitivity of ground-based Cherenkov telescopes for anisotropics in the cosmic gamma-ray background

Details Sensitivity of ground-based Cherenkov telescopes for anisotropics in the cosmic gamma-ray background Sensitivity of ground-based Cherenkov telescopes for anisotropics in the cosmic gamma-ray background

Dec 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008aipc.1085..767r&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: Proceedings of the 4th International Meeting on High Energy Gamma-Ray Astronomy. AIP Conferenc

Astronomy and Astrophysics

Astronomy

X- And Gamma-Ray Telescopes And Instrumentation, Gamma-Ray, Numerical Approximation And Analysis

Scientific paper

Self-annihilating dark matter contributes to the extra galactic very high-energy γ-ray background. This contribution is expected to be anisotropic following the density distribution of non-baryonic dark matter. We explore the possibilities to search for these anisotropies with present and future ground-based gamma-ray experiments like H.E.S.S., MAGIC, or CTA. A multipole-expansion of simulated events is used to investigate the sensitivity for anisotropies detectable with narrow field of view observations.

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