Observation of Multi-TeV Gamma Rays from the Shell-Like SNR GC40.5-0.5 Using the Tibet Air Shower Array

Details Observation of Multi-TeV Gamma Rays from the Shell-Like SNR GC40.5-0.5 Using the Tibet Air Shower Array Observation of Multi-TeV Gamma Rays from the Shell-Like SNR GC40.5-0.5 Using the Tibet Air Shower Array

Jul 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003icrc....4.2405z&link_type=abstract

Proceedings of the 28th International Cosmic Ray Conference. July 31-August 7, 2003. Trukuba, Japan. Under the auspices of the I

Physics

1

Scientific paper

Using observation data of the Tibet air shower array in different
periods, an excess of events in the multi-TeV region was detected from
the SNR GC40.50.5 direction, although statistically not significant yet.
The position of the highest excess is around the EGRET unidentified
source 3EG J1903+0550.

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