Evidence of Cosmic-Ray Acceleration up to Sub-PeV Energies in the Supernova Remnant IC 443.

Z. Cao(Chinese Academy of Sciences), G.H Chen(Guangzhou University), S. W. Cui(Hebei Normal University), Kai Fang(Chinese Academy of Sciences), W Bian(Shanghai Jiao Tong University), F Aharonian(Dublin Institute For Advanced Studies), X. H. Cui(Chinese Academy of Sciences), D. Bastieri(University of Padua), Weiling Cao(University of Science and Technology of China), Yiwang Bao(China Building Materials Academy), A.M Chen(Shanghai Jiao Tong University), Y Chen(Nanjing University), M.L Chen(Chinese Academy of Sciences), Zhe Cao(Harbin University), S. Z. Chen(Yunnan University), Xiao-Jun Bi(Ningxia Hui Autonomous Region Peoples Hospital), Z. G. Dai(University of Science and Technology of China), Hua-Xing Chen(Zhejiang Lab), Shaw H. Chen(Southwest Jiaotong University), T. L. Chen(Tibet University), Y. Z. Fan(Purple Mountain Observatory), A.V Bukevich(Institute for Nuclear Research), Liang Chen(Shanghai Astronomical Observatory), Qin Chen(Shanghai University), Yuting Bai(Chinese Academy of Sciences), J. Fang(Yunnan University), Shaomin Chen, Ning Cheng(Chinese Academy of Sciences), Long Chen(Southwest Jiaotong University), Jiang Chang, Y.J Bi(Campbell Collaboration), J. F. Chang(Nankai University), M.J Chen(Chinese Academy of Sciences), Chang Cai(Southwest Jiaotong University), E.S Chen(Chinese Academy of Sciences)
PubMed
April 24, 2026
Cited by 0


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