【作者单位】1School of Physical Science and Technology, Southwest Jiaotong University, Chengdu; 611756, China;2Graduate School of Tangshan, Southwest Jiaotong University, Tangshan; 063000, China;3School of Information Science and Technology, Southwest Jiaotong University, Chengdu; 611756, China;4Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Beijing; 100049, China;5Key Laboratory of Particle Astrophyics, Experimental Physics Division, Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing; 100049, China;6University of Chinese Academy of Sciences, Beijing; 100049, China;7TIANFU Cosmic Ray Research Center, Sichuan, Chengdu, China;8Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland;9Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg; 69029, Germany;10State Key Laboratory of Particle Detection and Electronics, China;11University of Science and Technology of China, Anhui, Hefei; 230026, China;12School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Sichuan, Chengdu; 610031, China;13College of Physics, Sichuan University, Sichuan, Chengdu; 610065, China;14School of Astronomy and Space Science, Nanjing University, Jiangsu, Nanjing; 210023, China;15Center for Astrophysics, Guangzhou University, Guangdong, Guangzhou; 510006, China;16School of Physics and Technology, Wuhan University, Hubei, Wuhan; 430072, China;17Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing; 210023, China;18Hebei Normal University, Hebei, Shijiazhuang; 050024, China;19Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai; 200030, China;20Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Tibet, Lhasa; 850000, China;21National Astronomical Observatories, Chinese Academy of Sciences, Beijing; 100101, China;22School of Physics and Astronomy, School of Physics (Guangzhou), Sun Yat-sen University, Guangdong, Zhuhai; 519000, China;23Dipartimento di Fisica, Università di Napoli 'Federico II', Complesso Universitario di Monte Sant'Angelo, via Cinthia, Napoli; 80126, Italy;24School of Physics and Astronomy, Yunnan University, Yunnan, Kunming; 650091, China;25D'epartement de Physique Nucl'eaire et Corpusculaire, Facult'e de Sciences, Universit'e de Gen'eve, 24 Quai Ernest Ansermet, Geneva; 1211, Switzerland;26Institute of Frontier and Interdisciplinary Science, Shandong University, Shandong, Qingdao; 266237, China;27Department of Engineering Physics, Tsinghua University, Beijing; 100084, China;28School of Physics and Microelectronics, Zhengzhou University, Henan, Zhengzhou; 450001, China;29Institute for Nuclear Research of Russian Academy of Sciences, Moscow; 117312, Russia;30School of Physics, Peking University, Beijing; 100871, China;31School of Physical Science and Technology, Guangxi University, Guangxi, Nanning; 530004, China;32Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai; 200240, China;33Yunnan Observatories, Chinese Academy of Sciences, Yunnan, Kunming; 650216, China;34Department of Physics, Faculty of Science, Mahidol University, Bangkok; 10400, Thailand;35Moscow Institute of Physics and Technology, Moscow; 141700, Russia;36Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing; 210023, China;37National Space Science Center, Chinese Academy of Sciences, Beijing; 100190, China
【召开年】2021
【会议地点】Virtual, Berlin, Germany
【摘要】 Identification of proton and gamma plays an essential role in ultra-high energy gamma-ray astronomy with LHAASO-KM2A. In this work, two neural networks and graph neural networks ) are applied to distinguish proton and gamma in the LHAASOKM2A simulat...