Physics
Scientific paper
Aug 2001
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001icrc....7.2753a&link_type=abstract
Proceedings of the 27th International Cosmic Ray Conference. 07-15 August, 2001. Hamburg, Germany. Under the auspices of the Int
Physics
2
Scientific paper
Our study is made for a search for TeV counterparts to GRBs observed by BATSE using the Tibet II/HD air-shower data set. Analysed Tibet data are taken during the period October 1995 through September 1999. BATSE detected 67 GRBs within the field of view of Tibet array during this period. Six kinds of time durations, 5, 10, 20, 30, 40 and 50 sec just after BATSE trig-ger, are employed for the examination. GRB971115a is found to be the most prominent GRB having Power value of 6.05. The probability that Power value is greater than 6.05 is occurred by the statistical uctuation is estimated by Monte Carlo simulation, and was found to be 2 × 10-1 . Therefore, such Power value can be understood as consistent with statistical uctuation. So, no clearly significant TeV gamma-ray bursts of employed time durations were detected from our analysis of Tibet II data set.
Amenomori Michihiro
Ayabe S.
Cui Shu-Wen
Ding Lin-Kai
Ding Xue-Yong
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