Astronomy and Astrophysics – Astrophysics
Scientist
Astronomy and Astrophysics
Astrophysics
Scientist
The Tibet AS gamma Collaboration
The Tibet ASgamma Collaboration
National Astronomical Observatoires / Yunnan Observatory, CAS;, Graduate School of CAS
University of Saskatchewan, Saskatoon, Canada
Department of Physics, Yunnan University, Kunming 650091, China
Department of Physics, Hirosaki University, Hirosaki, Japan
School of Graduate, Chinese Academy of Sciences, Beijing, China
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, Chin
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 Northern Sky Survey for Steady Tera-Electron Volt Gamma-Ray Point Sources Using the Tibet Air Shower Array
A Wide Sky Survey to search for TeV gamma-ray sources by the Tibet air shower array
Activity cycle of solar filaments
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