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Search for the Multi-TeV Gamma Rays from the Shell-Like SNR G40.5-0.5 Using the Tibet Air Shower Array |
ZHANG Ji-Long;TAN You-Hen;LU Hong;WANG Hui |
Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences,
Beijing 100049 |
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Cite this article: |
ZHANG Ji-Long, TAN You-Hen, LU Hong et al 2005 Chin. Phys. Lett. 22 1560-1562 |
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Abstract Using observation data of the Tibet air shower array in different periods, a region with the highest excess of 4.4σ in the multi-TeV was detected from the SNR G40.5-0.5 direction, although statistically insignificant yet. The position of the highest excess is located around the EGRET unidentified source 3EG J1903+0550.
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Keywords:
96.40.Pq
98.38.Mz
98.38.Dq
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Published: 01 June 2005
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