【作者单位】1The Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Lhasa 850000, Tibet, People's Republic of China;chentl@utibet.edu.cn, fengyouliang@utibet.edu.cn;2Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, People's Republic of China;3University of Chinese Academy of Sciences, 19 A Yuquan Road, Shijingshan District, Beijing 100049, People's Republic of China;4College of Physics, Chongqing University, No. 55 Daxuecheng South Road, High-tech District, Chongqing 401331, People's Republic of China;5College of Physics, Sichuan University, Chengdu 610064, People's Republic of China;6Suzhou Aerospace Information Research Institute, Suzhou 215123, People's Republic of China;7Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210008, People's Republic of China
【年份】2024
【卷号】Vol.967 No.1
【页码】31
【ISSN】0004-637X
【摘要】 The High Altitude Detection of Astronomical Radiation is a novel wide-field Cherenkov Telescope. It is designed for gamma-ray astronomy in the energy range of 10 GeV to 100 TeV, with gamma-ray bursts being one of its primary research focuses. To as...
