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Search For Gamma-Ray Bursts With The Tibet Air Shower Array

M Amenomori,S Ayabe,L K Ding,Z Y Feng,Yu Fu,H W Guo,M He,K Hibino,N Hotta,Jingyi Huang,Q Huang,A X Huo,K Izu,H Y Jia,F Kajino,K Kasahara,Y Katayose,K Kawata,J Y Li,Honghai Lu,S L Lu,G X Luo,X R Meng, Kazuyoshi Mizutani,Jianbing Mu,H Nanjo, Masato Nishizawa,Masami Ohnishi,I Ohta,Toshihiko Ouchi,S Ozawa,Z R Peng,J R Ren,T Saito,M Sakata,Takashi Sasaki,Z Z Shi,M Shibata,A Shiomi,Toshikazu Shirai,H Sugimoto,Hitoshi Sugiyama,K Taira,Y H Tan,N Tateyama,Shoji Torii,T Utsugi,C R Wang,Huiping Wang,X W Xu, Y L Yamamoto,G C Yu,A F Yuan,T Yuda,C S Zhang,H M Zhang,J L Zhang,N J Zhang,Xue Ying Zhang

HIGH ENERGY GAMMA-RAY ASTRONOMY（2001）

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Abstract
We searched for multi-TeV counterparts to the gamma-ray bursts (GRBs) at keV energies detected by BATSE during the period from October 2, 1995 to March 18, 1999 using the data of the Tibet Air Shower Array. In the field of view of the array there were 70 GRBs detected by BATSE in this period. The search was done based on the sky survey within error circles of BATSE bursts and with time scales during 10 to several hundred seconds. No significant signals of counterparts to the GRBs were detected.
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Key words
gamma ray burst,field of view,gamma ray
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