【作者单位】Institute of High Energy Physics，Chinese Academy of Sciences(CAS)，Key Laboratory of Particle Astrophysics；University of Chinese Academy of Sciences(UCAS)；College of Physics，Sichuan University；Tsung-Dao Lee Institute，Shanghai Jiao Tong University；Physics Department of Science School，Tibet University；Institute of Frontier and Interdisciplinary Science，Shandong University；Purple Mountain Observatory，Chinese Academy of Sciences(CAS)，Key Laboratory of Dark Matter and Space Astronomy；Department of Physics，University of Wisconsin-Madison，1150 University ave Madison；School of Physics and Technology，Wuhan University
【年份】2020
【卷号】第4卷
【期号】 第3期
【页码】392-398
【关键词】Cosmic rays Diffuse γ-rays YBJ-HA EAS
【摘要】 Purpose Cosmic rays up to PeV energy are believed to be generated in our galaxy.γ-rays at 100TeV energies are important probe to identify PeVtrons.Besides, γ-rays contain additional information on the propagation of the galactic cosmic rays.Methods D...
