【作者单位】1Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China;2University of Chinese Academy of Sciences, 100049 Beijing, China;3TIANFU Cosmic Ray Research Center, Chengdu, Sichuan, China;4Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2 Dublin, Ireland;5Max–Planck-Institute for Nuclear Physics, P.O. Box 103980, 69029 Heidelberg, Germany;6State Key Laboratory of Particle Detection and Electronics, China;7University of Science and Technology of China, 230026 Hefei, Anhui, China;8School of Physical Science and Technology & School of Information Science and Technology, Southwest Jiaotong University, 610031 Chengdu, Sichuan, China;9School of Astronomy and Space Science, Nanjing University, 210023 Nanjing, Jiangsu, China;10Center for Astrophysics, Guangzhou University, 510006 Guangzhou, Guangdong, China;11Hebei Normal University, 050024 Shijiazhuang, Hebei, China;12Key Laboratory of Dark Matter and Space Astronomy & Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, 210023 Nanjing, Jiangsu, China;13Tsung-Dao Lee Institute & School of Physics and Astronomy, Shanghai Jiao Tong University, 200240 Shanghai, China;14Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 200030 Shanghai, China;15Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, 850000 Lhasa, Tibet, China;16National Astronomical Observatories, Chinese Academy of Sciences, 100101 Beijing, China;17School of Physics and Astronomy (Zhuhai) & School of Physics (Guangzhou) & Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, 519000 Zhuhai & 510275 Guangzhou, Guangdong, China;18School of Physics and Astronomy, Yunnan University, 650091 Kunming, Yunnan, China;19Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, 1211 Geneva, Switzerland;20Institute of Frontier and Interdisciplinary Science, Shandong University, 266237 Qingdao, Shandong, China;21APC, Université Paris Cité, CNRS/IN2P3, CEA/IRFU, Observatoire de Paris, 119 75205 Paris, France;22Department of Engineering Physics, Tsinghua University, 100084 Beijing, China;23School of Physics and Microelectronics, Zhengzhou University, 450001 Zhengzhou, Henan, China;24Yunnan Observatories, Chinese Academy of Sciences, 650216 Kunming, Yunnan, China;25College of Physics, Sichuan University, 610065 Chengdu, Sichuan, China;26Institute for Nuclear Research of Russian Academy of Sciences, 117312 Moscow, Russia;27School of Physics, Peking University, 100871 Beijing, China;28School of Physical Science and Technology, Guangxi University, 530004 Nanning, Guangxi, China;29Department of Physics, Faculty of Science, Mahidol University, Bangkok 10400, Thailand;30Moscow Institute of Physics and Technology, 141700 Moscow, Russia;31Center for Relativistic Astrophysics and High Energy Physics, School of Physics and Materials Science & Institute of Space Science and Technology, Nanchang University, 330031 Nanchang, Jiangxi, China;32National Space Science Center, Chinese Academy of Sciences, 100190 Beijing, China
【年份】2023
【卷号】Vol.1056
【页码】168662
【ISSN】0168-9002
【摘要】 One of the main scientific objectives of the Large High Altitude Air Shower Observatory is to perform accurate measurements of the energy spectra for different cosmic ray masses, from a few TeV to 100 PeV. As one of the main sub-arrays of LHAASO, th...
