【作者单位】Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China>University of Chinese Academy of Sciences, Beijing, 100049, China>Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China>National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China>National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China>Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China>University of Chinese Academy of Sciences, Beijing, 100049, China>Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China>Department of Physics, Shandong University, Jinan 250100, China>Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China>University of Chinese Academy of Sciences, Beijing, 100049, China>National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100012, China>Department of Physics, Shandong University, Jinan 250100, China>Department of Physics, Shandong University, Jinan 250100, China>Institute of Modern Physics, Southwest Jiaotong University, Chengdu 610031, China>Institute of Modern Physics, Southwest Jiaotong University, Chengdu 610031, China>Physics Department of Science School, Tibet University, Lhasa 850000, China>Physics Department of Science School, Tibet University, Lhasa 850000, China>Physics Department of Science School, Tibet University, Lhasa 850000, China>Physics Department of Science School, Tibet University, Lhasa 850000, China>Physics Department of Science School, Tibet University, Lhasa 850000, China>Physics Department of Science School, Tibet University, Lhasa 850000, China
【年份】2016
【卷号】Vol.11 No.6
【页码】P06016
【ISSN】1748-0221
【摘要】 Since 2014, a new hybrid experiment consisting of a high-energy air-shower-core array (YAC-II), a high-density air-shower array (Tibet-III) and a large underground water-Cherenkov muon-detector array (MD) has been continued by the Tibet AS γ collabor...
