Search for a Dark Matter Annihilation Signal in the TeV Range with H.E.S.S.

Details Search for a Dark Matter Annihilation Signal in the TeV Range with H.E.S.S. Search for a Dark Matter Annihilation Signal in the TeV Range with H.E.S.S.

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007idm..conf..115m&link_type=abstract

THE IDENTIFICATION OF DARK MATTER. Proceedings of the Sixth International Workshop. Held 11-16 September 2006 in Rhodes, Greece.

Astronomy and Astrophysics

Astronomy

Dark Matter, Gamma Ray Astronomy

Scientific paper

The H.E.S.S. (High Energy Stereoscopic System) array of imaging atmospheric Cherenkov telescopes is designed to detect very high energy (Eγ>100GeV) γ-rays in the TeV range. A strong signal from the high energy source HESS J1745-290 has been detected in the direction of the Galactic Center. Constraints have been derived on a possible component due to dark matter particles annihilation. Diffuse γ-ray emission has been highlighted along the Galactic plane. Prospects of detection from Sagittarius Dwarf galaxy scheduled for observations will be discussed.

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