Searching for TeV Counterparts to BATSE GRBs
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摘要: 利用西藏ASγ实验三期阵列的重建数据，对25个BATSEγ暴的TeV能区伴随γ暴进行了符合寻找。在BATSEγ暴方向的90％误差范围内，找出在给定的小天区和时间间隔内出现的显著性较高的TeV事例团，并采用“等天顶角方法”来估计背景。发现少量事例团对背景有明显超出，考虑试验次数后，其超出还不足以认定为γ暴。通过Monte Carlo模拟给出了95％置信水平下流强上限的估计值为7．1×10^-9photons／（cm^2·s）。Searching for TeV burst-like events coincident with the BATSE GRBs data was made by using the ASγ （Tibet-Ⅲ） data. In the period we analysed, there were 25 BATSE GRBs in the field view of Tibet. A search region was defined by the BATSE 90% confidence level positioning error. A GRB candidate was chosen as a shower cluster appearing in a given small sky window and a given time interval. An equi-zenith-angle method was used to estimate the background. No significant TeV GRBs were detected. The flux upper limit at the 95% confidence level was estimated to be about 7.1×10^-9 γ（cm^2·s） by Monte Carlo simulation.Abstract: Searching for TeV burst-like events coincident with the BATSE GRBs data was made by using the ASγ （Tibet-Ⅲ） data. In the period we analysed, there were 25 BATSE GRBs in the field view of Tibet. A search region was defined by the BATSE 90% confidence level positioning error. A GRB candidate was chosen as a shower cluster appearing in a given small sky window and a given time interval. An equi-zenith-angle method was used to estimate the background. No significant TeV GRBs were detected. The flux upper limit at the 95% confidence level was estimated to be about 7.1×10^-9 γ（cm^2·s） by Monte Carlo simulation.
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Key words:
- cosmic ray /
- γ-ray burst /
- TeV energy region
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