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23 April 2024

» arxiv » 0710.2752

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Future plan for observation of cosmic gamma rays in the 100 TeV energy region with the Tibet air shower array : simulation and sensitivity
M. Amenomori ; X. J. Bi ; D. Chen ; S. W. Cui ; Danzengluobu ; L. K. Ding ; X. H. Ding ; C. Fan ; C. F. Feng ; Zhaoyang Feng ; Z. Y. Feng ; X. Y. Gao ; Q. X. Geng ; H. W. Guo ; H. H. He ; M. He ; K. Hibino ; N. Hotta ; Haibing Hu ; H. B. Hu ; J. Huang ; Q. Huang ; H. Y. Jia ; F. Kajino ; K. Kasahara ; Y. Katayose ; C. Kato ; K. Kawata ; Labaciren ; G. M. Le ; A. F. Li ; J. Y. Li ; Y.-Q. Lou ; H. Lu ; S. L. Lu ; X. R. Meng ; K. Mizutani ; J. Mu ; K. Munakata ; A. Nagai ; H. Nanjo ; M. Nishizawa ; M. Ohnishi ; I. Ohta ; H. Onuma ; T. Ouchi ; S. Ozawa ; J. R. Ren ; T. Saito ; T. Y. Saito ; M. Sakata ; T. K. Sako ; M. Shibata ; A. Shiomi ; T. Shirai ; H. Sugimoto ; M. Takita ; Y. H. Tan ; N. Tateyama ; S. Torii ; H. Tsuchiya ; S. Udo ; B. Wang ; H. Wang ; X. Wang ; Y. Wang ; Y. G. Wang ; H. R. Wu ; L. Xue ; Y. Yamamoto ; C. T. Yan ; X. C. Yang ; S. Yasue ; Z. H. Ye ;
Date:	15 Oct 2007
Abstract:	The Tibet air shower array, which has an effective area of 37,000 square meters and is located at 4300 m in altitude, has been observing air showers induced by cosmic rays with energies above a few TeV. We have a plan to add a large muon detector array to it for the purpose of increasing its sensitivity to cosmic gamma rays in the 100 TeV energy region by discriminating them from cosmic-ray hadrons. We have deduced the attainable sensitivity of the muon detector array using our Monte Carlo simulation. We report here on the detailed procedure of our Monte Carlo simulation.
Source:	arXiv, 0710.2752
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