【作者单位】a Department of Physics, Hirosaki University, Japan; b Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, China; c National Astronomical Observatories, Chinese Academy of Sciences, China; d Department of Mathematics and Physics, Tibet University, China; e Department of Physics, Hebei Normal University, China; f Department of Physics, Shandong University, China; g Institute of Modern Physics, SouthWest Jiaotong University, China; h Faculty of Engineering, Kanagawa University, Japan; i Faculty of Education, Utsunomiya University, Japan; j Department of Physics, Konan University, Japan; k Research Institute for Science and Engineering, Waseda University, Japan; l Faculty of Engineering, Yokohama National University, Japan; m Department of Physics, Shinshu University, Japan; n Institute for Cosmic Ray Research, University of Tokyo, Japan; o Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (ISAS/JAXA), Japan; p National Center for Space Weather, China Meteorological Administration, China; q School of Information Science and Engineering, Shandong Agriculture University, China; r Saitama University, Japan; s National Institute of Informatics, Japan; t Sakushin Gakuin University, Japan; u College of Science, China University of Petroleum, China; v Tokyo Metropolitan College of Industrial Technology, Japan; w Max-Planck-Institut für Physik, Germany; x Escuela de Ciencias Físicas y Nanotechnología, Yachay Tech., Ecuador; y College of Industrial Technology, Nihon University, Japan; z Shonan Institute of Technology, Japan; aa Japan Atomic Energy Agency, Japan
【年份】2017
【ISSN】1824-8039;1824-8039
【摘要】 We built a large water Cherenkov-type muon detector array under the existing Tibet air shower array at 4,300 m above sea level, to observe 10-1000 TeV gamma rays from cosmic-ray accelerators in our Galaxy with wide field of view at very low backgrou...
