Search for TeV GRBs Using the Tibet-III ASg Data

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Scientific paper

Search for TeV GRBs was made by using the ASγ (Tib et-I I I) data taken from Nov. 1999 to July 2002. A GRB candidate was chosen as a shower cluster appearing in a given small sky window and a time interval ranging from 1 to 100 seconds. An equi-zenith-angle method was used to estimate the background. In this analysis,two methods searching for possible GRB's signals indep endently and searching for possible burst-like events coincident with satellite GRB data have been applied. No significant TeV gamma-ray bursts were detected.

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