【作者单位】1Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing; 100049, China;2University of Chinese Academy of Sciences, Beijing; 100049, China;3Tianfu Cosmic Ray Research Center, Sichuan, Chengdu; 610000, China;4Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2, Dublin, Ireland;5Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg; 69029, Germany;6School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Sichuan, Chengdu; 610031, China;7School of Astronomy and Space Science, Nanjing University, Jiangsu, Nanjing; 210023, China;8Center for Astrophysics, Guangzhou University, Guangdong, Guangzhou; 510006, China;9Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai; 200240, China;10Institute for Nuclear Research, Russian Academy of Sciences, Moscow; 117312, Russia;11Hebei Normal University, Hebei, Shijiazhuang; 050024, China;12University of Science and Technology of China, Anhui, Hefei; 230026, China;13State Key Laboratory of Particle Detection and Electronics, China;14Key Laboratory of Dark Matter and Space Astronomy, Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing; 210023, China;15Research Center for Astronomical Computing, Zhejiang Laboratory, Zhejiang, Hangzhou; 311121, China;16Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai; 200030, China;17School of Physics and Astronomy, Yunnan University, Yunnan, Kunming; 650091, China;18Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Tibet, Lhasa; 850000, China;19National Astronomical Observatories, Chinese Academy of Sciences, Beijing; 100101, China;20School of Physics and Astronomy (Zhuhai), School of Physics (Guangzhou), Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, Zhuhai; 519000, China;21School of Physics and Astronomy (Zhuhai), School of Physics (Guangzhou), Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, Guangdong, Guangzhou; 510275, China;22Institute of Frontier and Interdisciplinary Science, Shandong University, Shandong, Qingdao; 266237, China;23APC, Université Paris Cité, CNRS, IN2P3, CEA, IRFU, Observatoire de Paris, 119, Paris; 75205, France;24Department of Engineering Physics, Tsinghua University, Beijing; 100084, China;25School of Physics and Microelectronics, Zhengzhou University, Henan, Zhengzhou; 450001, China;26Yunnan Observatories, Chinese Academy of Sciences, Yunnan, Kunming; 650216, China;27China Center of Advanced Science and Technology, Beijing; 100190, China;28College of Physics, Sichuan University, Sichuan, Chengdu; 610065, China;29School of Physics, Peking University, Beijing; 100871, China;30Guangxi Key Laboratory for Relativistic Astrophysics, School of Physical Science and Technology, Guangxi University, Guangxi, Nanning; 530004, China;31Department of Physics, Faculty of Science, Mahidol University, Bangkok; 10400, Thailand;32Moscow Institute of Physics and Technology, Moscow; 141700, Russia;33Center for Relativistic Astrophysics and High Energy Physics, School of Physics and Materials Science, Institute of Space Science and Technology, Nanchang University, Jiangxi, Nanchang; 330031, China;34National Space Science Center, Chinese Academy of Sciences, Beijing; 100190, China;35School of Physics, Huazhong University of Science and Technology, Hubei, Wuhan; 430074, China
【年份】2024
【摘要】 Very recently, the Large High Altitude Air Shower Observatory reported the observation of the very early TeV afterglow of the brightest-of-all-time GRB 221009A, recording the highest photon statistics in the TeV band ever from a gamma-ray burst. We ...