The Energy Scale Calibration Using the Moon Shadow of LHAASO-WCDA Detector

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【作者】Wang, Yanjin，Cao, Zhen，Zeng, Zongkang，Ma, Lingling，Nan, Yuncheng，Aharonian, F.，An, Q.，Axikegu，Bai, L.X.，Bai, Y.X.，Bao, Y.W.，Bastieri, D.，Bi, X.J.，Bi, Y.J.，Cai, H.，Cai, J.T.，Cao, Zhen，Cao, Zhe，Chang, J.，Chang, J.F.，Chen, B.M.，Chen, E.S.，Chen, J.，Chen, Liang，Chen, Long，Chen, M.J.，Chen, M.L.，Chen, Q.H.，Chen, S.H.，Chen, S.Z.，Chen, T.L.，Chen, X.L.，Chen, Y.，Cheng, N.，Cheng, Y.D.，Cui, S.W.，Cui, X.H.，Cui, Y.D.，Dai, B.Z.，Dai, H.L.，Dai, Z.G.，Danzengluobu，della Volpe, D.，DEttorre Piazzoli, B.，Dong, X.J.，Duan, K.K.，Fan, J.H.，Fan, Y.Z.，Fan, Z.X.，Fang, J.，Fang, K.，Feng, C.F.，Feng, L.，Feng, S.H.，Feng, Y.L.，Gao, B.，Gao, C.D.，Gao, L.Q.，Gao, Q.，Gao, W.，Ge, M.M.，Geng, L.S.，Gong, G.H.，Gou, Q.B.，Gu, M.H.，Guo, F.L.，Guo, J.G.，Guo, X.L.，Guo, Y.Q.，Guo, Y.Y.，Han, Y.A.，He, H.H.，He, H.N.，He, J.C.，He, S.L.，He, X.B.，He, Y.，Heller, M.，Hor, Y.K.，Hou, C.，Hu, H.B.4
【作者单位】¹College of Sciences, Northeastern University, Liaoning, Shenyang; 110819, China;²Key Laboratory of Particle Astrophysics, Experimental Physics Division, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing; 100049, China;³Institute of Frontier and Interdisciplinary Science, Shandong University, Shandong, Qingdao; 266237, China;⁴Key Laboratory of Particle Astrophyics, Experimental Physics Division, Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing; 100049, China;⁵University of Chinese Academy of Sciences, Beijing; 100049, China;⁶TIANFU Cosmic Ray Research Center, Sichuan, Chengdu, China;⁷State Key Laboratory of Particle Detection and Electronics, China;⁸University of Science and Technology of China, Anhui, Hefei; 230026, China;⁹Department of Engineering Physics, Tsinghua University, Beijing; 100084, China;¹⁰National Astronomical Observatories, Chinese Academy of Sciences, Beijing; 100101, China;¹¹National Space Science Center, Chinese Academy of Sciences, Beijing; 100190, China;¹²School of Physics, Peking University, Beijing; 100871, China;¹³Center for Astrophysics, Guangzhou University, Guangdong, Guangzhou; 510006, China;¹⁴School of Physics and Astronomy, School of Physics (Guangzhou), Sun Yat-Sen University, Guangdong, Zhuhai; 519082, China;¹⁵School of Physical Science and Technology, Guangxi University, Guangxi, Nanning; 530004, China;¹⁶Hebei Normal University, Hebei, Shijiazhuang; 050024, China;¹⁷School of Physics and Microelectronics, Zhengzhou University, Henan, Zhengzhou; 450001, China;¹⁸School of Astronomy and Space Science, Nanjing University, Jiangsu, Nanjing; 210023, China;¹⁹Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing; 210023, China;²⁰Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai; 200030, China;²¹Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai; 200240, China;²²School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Sichuan, Chengdu; 610031, China;²³College of Physics, Sichuan University, Sichuan, Chengdu; 610065, China;²⁴Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Tibet, Lhasa; 850000, China;²⁵School of Physics and Technology, Wuhan University, Hubei, Wuhan; 430072, China;²⁶School of Physics and Astronomy, Yunnan University, Yunnan, Kunming; 650091, China;²⁷Yunnan Observatories, Chinese Academy of Sciences, Yunnan, Kunming; 650216, China;²⁸Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2, Dublin, Ireland;²⁹Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg; 69029, Germany;³⁰Dipartimento di Fisica, Università di Napoli 'Federico II', Complesso Universitario di Monte SantAngelo, via Cinthia, Napoli; 80126, Italy;³¹Institute for Nuclear Research of Russian Academy of Sciences, Moscow; 117312, Russia;³²Moscow Institute of Physics and Technology, Moscow; 141700, Russia;³³Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, Geneva; 1211, Switzerland;³⁴Department of Physics, Faculty of Science, Mahidol University, Bangkok; 10400, Thailand
【召开年】2021
【会议地点】Virtual, Berlin, Germany
【摘要】 The Water Cherenkov Detector Array of LHAASO are designed to work in combination for measuring the energy spectra of the cosmic ray species over a very wide energy range from a few TeV to 10 PeV. The energy calibration can be achieved with a proven ...
【文献类型】会议论文

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