Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
The Tibet AS gamma Collaboration
CANGAROO-III
The Tibet ASgamma Collaboration
Department of Physics, Konan University, Kobe, Hyogo 658-8501, Japan
Department of Physics, Konan University, Kobe 658-8501, Japan
Department of Physics, Konan University, Okamoto 8-9-1, Higashinada, Kobe 658-8501, Japan
Department of Physics, Hirosaki University, Hirosaki, Japan
Konan Univ., Kobe, Japan
Department of Physics, Hirosaki University, Hirosaki, JapanZ.CaoL. K.DingInstitute of High Energy Physics, Chinese Academy of Sciences, Beijing, ChinaZ. Y.FengDepartment of Physics, South West Jiaotong University, Chengdu, ChinaK.HibinoInstitute for Cosmic Ray Research, University of Tokyo, Tanashi, JapanN.HottaFaculty of Education, Utsunomiya University, Utsunomiya, JapanQ.HuangDepartment of Physics, South Jiaotong University, Chengdu, ChinaA. X.HuoInstitute of High Energy Physics, Chinese Academy of Sciences, Beijing, ChinaH. Y.JiaG. Z.JiangS. Q.JiaoDepartment of Physics, South West Jiaotong University, Chengdu, ChinaF.KajinoDepartment of Physics, Konan University, Kobe, JapanK.KasaharaFaculty of Engineering, Kanagawa University, Yokohama, JapanLabacirenD. M.MeiDepartment of Mathematics and Physics, Tibet Universityk Lhasa, ChinaL.MengInstitute of High Energy Physics, Chinese Academy of Sciences, Beijing, ChinaX. R.MengMimacirenDepartment of Mathematics and Physics, Tibet University, Lhasa, ChinaK.MizutaniDepartment of Physics, Saitama University, Urawa, JapanJ.MuDepartment of Physics, Yunnan University, Kunming, ChinaH.NanjoDepartment of Physics, Hirosaki University, Horosaki, JapanM.NishizawaDepartment of Physics, Konan University, Kobe, JapanNusangDepartment of Mathematics and Physics, Tibet University, Lhasa, ChinaA.OguroDepartment of Physics, Saitama University, Urawa, JapanM.OhnishiDepartment of Physics, Konan University, Kobe, JapanI.OhtaFaculty of Education, Utsunomiya University, Utsunomiya, JapanJ. R.RenInstitute of High Energy Physics, Chinese Academy of Sciences, Beijing, ChinaTo.SaitoInstitute for Cosmic Ray Research, Uni
10, 000 M**2 Cosmic Ray Muon Detection System Located at Rather Shallow Underground
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 the Gamma-ray astronomy in the 100 TeV region: Overview and physics goal
A new method to search for high energy gamma rays by track-calorimeter detectors at a high mountain
A new project to search for high energy gamma ray point souces in Tibet
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