Upper limits on TeV gamma-rays from Neutralino Annihilation in the Galactic Center

Details Upper limits on TeV gamma-rays from Neutralino Annihilation in the Galactic Center Upper limits on TeV gamma-rays from Neutralino Annihilation in the Galactic Center

Aug 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....7.2989k&link_type=abstract

Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int

Physics

Scientific paper

We present results of recent observations of the galactic center (Sagittarius A*) with the Whipple High Energy Gamma-Ray Telescope. The new high resolution camera and a new data analysis technique which is re-optimized to include zenith angle corrections, provide improved sensitivity at large zenith angles. The upper limit presented here can be used to give a new constraint on the flux of TeV gamma-rays produced by neutralino annihilation near the galactic center. A preliminary upper-limit on the gammaray line flux is 1.86 · 10-12 cm-2 sec-1 .

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