A large underground water Cherenkov muon detector array with the Tibet air shower array for the Gamma-ray astronomy in the 100 TeV region: Overview and physics goal
【作者单位】1 Department of Physics, Hirosaki University, Hirosaki 036-8561, Japan 2 Department of Physics, Saitama University, Saitama 338-8570, Japan 3 Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China 4 Faculty of Engineering, Yokohama National University, Yokohama 240-8501, Japan 5 Department of Physics, Hebei Normal University, Shijiazhuang 050016 6 Department of Mathematics and Physics, Tibet University, Lhasa 850000, China 7 Department of Physics, Shandong University, Jinan 250100, China 8 Institute of Modern Physics, South West Jiaotong University, Chengdu 610031, China 9 Department of Physics, Yunnan University, Kunming 650091, China 10 Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan 11 Faculty of Education, Utsunomiya University, Utsunomiya 321-8505, Japan
【年份】2008
【卷号】Vol.175-176
【页码】476-479
【ISSN】0920-5632
【摘要】 The Tibet air shower array with effective area 37,000 m 2 located at 4300m in altitude, in Tibet, China, is sensitive to celestial gamma rays with energies above a few TeV. We have a plan to add a large underground muon detector array to it in order...