Physics
Scientist
Sagami Inst. of Technology
Sagami Institute of Technology, Japan
Sagami Institute of Technology, Fujisawa, Japan
Shonan Institute of Technology, Fujisawa 251-8511, Japan
Shonan Institute of Technology, Fujisawa 252-8511, 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, University of Tokyo, Tanashi, JapanM.SakataDepartment of Physics, Konan U
A new project to search for high energy gamma ray point souces in Tibet
A Wide Sky Survey to search for TeV gamma-ray sources by the Tibet air shower array
An Upper Limit on Cosmic-Ray overline p/p Flux Ratio Estimated by the Moon's Shadow with the Tibet-III Air Shower Array
Analysis of Emulsion Chambers in Tibet Hybrid Experiment Using the Image Scanner
Behavior and Structure of Super-Families Observed with the Emulsion Chambers at Mts. Fuji and Kanbala
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