Abstract
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.
Original language | English |
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Pages (from-to) | 480-483 |
Number of pages | 4 |
Journal | Nuclear Physics B - Proceedings Supplements |
Volume | 175-176 |
Issue number | SUPPL.: COMPLETE |
DOIs | |
Publication status | Published - 2008 Jan |
ASJC Scopus subject areas
- Nuclear and High Energy Physics