A large underground water Cherenkov muon detector array with the Tibet air shower array for Gamma-ray astronomy in the 100 TeV region: detector design and simulation

Details A large underground water Cherenkov muon detector array with the Tibet air shower array for Gamma-ray astronomy in the 100 TeV region: detector design and simulation A large underground water Cherenkov muon detector array with the Tibet air shower array for Gamma-ray astronomy in the 100 TeV region: detector design and simulation

Jan 2008

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008nuphs.175..480t&link_type=abstract

Nuclear Physics B Proceedings Supplements, Volume 175, p. 480-483.

Physics

Nuclear Physics

Scientific paper

We are planning to build a large water-Cherenkov-type muon detector
array around the Tibet air shower array for Gamma-ray astronomy in the
100 TeV Region. In this paper, we describe the design of the Tibet MD
array and details of the Monte Carlo simulation to demonstrate the
sensitivity of the Tibet AS+MD array.

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