Astronomy and Astrophysics – Astrophysics – High Energy Astrophysical Phenomena
Scientist
Astronomy and Astrophysics
Astrophysics
High Energy Astrophysical Phenomena
Scientist
The ARGO-YBJ Collaboration
Department of Mathematics and Physics, Tibet University, Lhasa 850000, China
Department of Physics, Hirosaki University, Hirosaki, 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 University, Kobe, JapanZ. Z.ShiInstitute of High Energy Physics, Chinese Academy of Sciences, Beijing, ChinaM.ShibataFaculty of Education, Yokohama Nat
A Wide Sky Survey to search for TeV gamma-ray sources by the Tibet air shower array
ARGO-YBJ detects a VHE gamma-ray flare from Mrk501
Correlation between Sun shadows of 10 TeV cosmic rays and solar activity.
Cosmic-ray deficit from the directions of the Moon and the Sun detected with the Tibet air-shower array
Detection of TeV gamma rays from Mrk 501 at high flaring state of activity in 1997 with the Tibet air shower array
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