【作者】Aharonian, Felix A.，An, Q.，Axikegu，Bai, Lixin，Bai, Yunxiang，Bao, Yiwei，Bastieri, D.，Bi, Xiaojun，Bi, Yujiang，Cai, Hao，Cai, J. T.，Cao, Zhen，Cao, Zhe，Chang, Jin，Chang, J. F.，Chang, Xiaochuan，Chen, B. M.，Chen, Jian，Chen, Lin，Chen, Liang，Chen, Mingjun，Chen, M. L.，Chen, Qihui，Chen, Shanhong，Chen, Songzhan，Chen, Tianlu，Chen, X. L.，Chen, Yang，Cheng, Ning，Cheng, Y. D.，Cui, Shuwang，Cui, Xiaohong，Cui, Yudong，Dai, Benzhong，Dai, H. L.，Dai, Zigao，Danzengluobu，Volpe, Domenico Della，Piazzoli, Benedetto Dettorre，Dong, X. J.，Fan, Junhui，Fan, Yizhong，Fan, Z. X.，Fang, Jinghong，Fang, Kun，Feng, Cunfeng，Feng, Lei，Feng, Shaohui，Feng, Youliang，Gao, Bo，Gao, C. D.，Gao, Qi，Gao, Wei，Ge, Maomao，Geng, L. S.，Gong, Guanghua，Gou, Quanbu，Gu, M. H.，Guo, Junguang，Guo, X. L.，Guo, Yiqing，Guo, Yingying，Han, Y. A.，He, Huihai，He, Haoning，He, Jiancheng，He, S. L.，He, Xinbo，He, Yu，Heller, Matthieu，Hor, Yuen Keung，Hou, Chao，Hou, Xian，Hu, Hongbo，Hu, S.，Hu, S. C.，Hu, X. J.，Huang, Daihui，Huang, Qiulan，Huang, Wenhao，Huang, Xingtao，Huang, Z. C.，Ji, F.，Ji, Xia
【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;4State Key Laboratory of Particle Detection and Electronics, Beijing, China;5University of Science and Technology of China, 230026, Hefei, Anhui, China;6Department of Engineering Physics, Tsinghua University, 100084, Beijing, China;7National Astronomical Observatories, Chinese Academy of Sciences, 100101, Beijing, China;8National Space Science Center, Chinese Academy of Sciences, 100190, Beijing, China;9School of Physics, Peking University, 100871, Beijing, China;10Center for Astrophysics, Guangzhou University, 510006, Guangzhou, Guangdong, China;11School of Physics and Astronomy & School of Physics (Guangzhou), Sun Yat-sen University, 519000, Zhuhai, Guangdong, China;12School of Physical Science and Technology, Guangxi University, 530004, Nanning, Guangxi, China;13Hebei Normal University, 050024, Shijiazhuang, Hebei, China;14School of Physics and Microelectronics, Zhengzhou University, 450001, Zhengzhou, Henan, China;15School of Astronomy and Space Science, Nanjing University, 210023, Nanjing, Jiangsu, China;16Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, 210023, Nanjing, Jiangsu, China;17Institute of Frontier and Interdisciplinary Science, Shandong University, 266237, Qingdao, Shandong, China;18Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 200030, Shanghai, China;19Tsung-Dao Lee Institute & School of Physics and Astronomy, Shanghai Jiao Tong University, 200240, Shanghai, China;20School of Physical Science and Technology & School of Information Science and Technology, Southwest Jiaotong University, 610031, Chengdu, Sichuan, China;21College of Physics, Sichuan University, 610065, Chengdu, Sichuan, China;22Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, 850000, Lhasa, Tibet, China;23School of Physics and Technology, Wuhan University, 430072, Wuhan, Hubei, China;24School of Physics and Astronomy, Yunnan University, 650091, Kunming, Yunnan, China;25Yunnan Observatories, Chinese Academy of Sciences, 650216, Kunming, Yunnan, China;26Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin, Ireland;27Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, 69029, Heidelberg, Germany;28Dipartimento di Fisica dell’Università di Napoli “Federico II”, Complesso Universitario di Monte Sant’Angelo, via Cinthia, 80126, Napoli, Italy;29Institute for Nuclear Research of Russian Academy of Sciences, 117312, Moscow, Russia;30Moscow Institute of Physics and Technology, 141700, Moscow, Russia;31Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, 1211, Geneva, Switzerland;32Department of Physics, Faculty of Science, Mahidol University, 10400, Bangkok, Thailand
【年份】2021
【卷号】Vol.5 No.4
【页码】531-541
【ISSN】2509-9930
【关键词】LHAASO WCDA GRB
【摘要】 Purpose Observation of high energy and very high emission from Gamma Ray Bursts is crucial to study the gigantic explosion and the underline processes. With a large field-of-view and almost full duty cycle, the Water Cherenkov Detector Array , a su...
