Chin. Phys. Lett.  2005, Vol. 22 Issue (6): 1560-1562    DOI:
Original Articles |
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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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.
Keywords: 96.40.Pq      98.38.Mz      98.38.Dq     
Published: 01 June 2005
PACS:  96.40.Pq  
  98.38.Mz (Supernova remnants)  
  98.38.Dq (Molecular clouds, H2 clouds, dense clouds, and dark clouds)  
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https://cpl.iphy.ac.cn/       OR      https://cpl.iphy.ac.cn/Y2005/V22/I6/01560
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ZHANG Ji-Long
TAN You-Hen
LU Hong
WANG Hui
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