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The all-particle spectrum and mean logarithmic mass of cosmic rays in the knee region by LHAASO-KM2A | |
Zhang, Hengying1,3; He, Huihai1,2,3; Feng, Cunfeng4; Cao, Zhen2,3,5; Aharonian, F.6,7; An, Q.8,9; Axikegu10; Bai, Y. X.3,5; Bao, Y. W.11; Bastieri, D.12; Bi, X. J.2,3,5; Bi, Y. J.3,5; Cai, J. T.12; Cao, Q.13; Cao, W. Y.9; Cao, Zhe8,9; Chang, J.14; Chang, J. F.3,5,8; Chen, A. M.15; Chen, E. S.2,3,5; Chen, Liang16; Chen, Lin10; Chen, Long10; Chen, M. J.3,5; Chen, M. L.3,5,8; Chen, Q. H.10; Chen, S. H.2,3,5; Chen, S. Z.3,5; Chen, T. L.17; Chen, Y.11; Cheng, N.3,5; Cheng, Y. D.3,5; Cui, M. Y.14; Cui, S. W.13; Cui, X. H.18; Cui, Y. D.19; Dai, B. Z.20; Dai, H. L.3,5,8; Dai, Z. G.9; Danzengluobu17; della Volpe, D.21; Dong, X. Q.2,3,5; Duan, K. K.14; Fan, J. H.12; Fan, Y. Z.14; Fang, J.20; Fang, K.3,5; Feng, C. F.4; Feng, L.14; Feng, S. H.3,5; Feng, X. T.4; Feng, Y. L.17; Gabici, S.22; Gao, B.3,5; Gao, C. D.4; Gao, L. Q.2,3,5; Gao, Q.17; Gao, W.3,5; Gao, W. K.2,3,5; Ge, M. M.20; Geng, L. S.3,5; Giacinti, G.15; Gong, G. H.23; Gou, Q. B.3,5; Gu, M. H.3,5,8; Guo, F. L.16; Guo, X. L.10; Guo, Y. Q.3,5; Guo, Y. Y.14; Han, Y. A.24; He, H. H.2,3,5; He, H. N.14; He, J. Y.14; He, X. B.19; He, Y.10; Heller, M.21; Hor, Y. K.19; Hou, B. W.2,3,5; Hou, C.3,5; Hou X(侯贤)25![]() ![]() | |
会议录名称 | Proceedings of Science |
2024-09-27 | |
卷号 | 444 |
DOI | 10.22323/1.444.0461 |
产权排序 | 第25完成单位 |
收录类别 | EI |
会议名称 | 38th International Cosmic Ray Conference, ICRC 2023 |
会议日期 | 2023-07-26 |
会议地点 | Nagoya, Japan |
会议赞助商 | et al.; Institute for Cosmic Ray Research (ICRR) Univeristy of Tokyo; International Union of Pure and Applied Physics (IUPAP); JPS; Nagoya Convention and Visitors Bureau; Nagoya University |
摘要 | The kilometer-square array (KM2A) of the Large High Altitude Air Shower Observatory (LHAASO, located at 4410 m above sea level with an atmospheric depth of 600 g/cm2) can simultaneously measure air shower sizes of both electromagnetic particles and muon contents with high precision for cosmic rays with energies in the knee region. The energy is reconstructed by combining parameters of muons and electromagnetic particles, which is weakly dependent on the mass composition of cosmic rays. We study the measurement method of the all particle spectrum and mean logarithmic mass through the simulation data, and discuss the corresponding systematic errors. © Copyright owned by the author(s) under the terms of the Creative Commons. |
资助项目 | National Key Research and Development Program of China[2018YFA0404202];National Key Research and Development Program of China[2018YFA0404203];National Key Research and Development Program of China[2018YFA0404204];National Key Research and Development Program of China[2018YFA0404201];National Natural Science Foundation of China[12175121];National Natural Science Foundation of China[12105301];National Natural Science Foundation of China[12022502];National Natural Science Foundation of China[12275280];National Natural Science Foundation of China[12261160362];National Natural Science Foundation of China[12205314];National Natural Science Foundation of China[12105294] |
项目资助者 | National Key Research and Development Program of China[2018YFA0404202, 2018YFA0404203, 2018YFA0404204, 2018YFA0404201] ; National Natural Science Foundation of China[12175121, 12105301, 12022502, 12275280, 12261160362, 12205314, 12105294] |
语种 | 英语 |
学科领域 | 天文学 ; 天体物理学 ; 高能天体物理学 ; 星系与宇宙学 |
文章类型 | Conference article (CA) |
URL | 查看原文 |
EI入藏号 | 20245117556015 |
EI主题词 | Systematic errors |
EI分类号 | 1301.1.3 - 1302.1 - 1303.1 - 731.1.1 - 941.9 |
引用统计 | |
文献类型 | 会议论文 |
条目标识符 | http://ir.ynao.ac.cn/handle/114a53/27926 |
专题 | 星系类星体研究组 |
作者单位 | 1.Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, 100049, China; 2.University of Chinese Academy of Sciences, Beijing, 100049, China; 3.TIANFU Cosmic Ray Research Center, Sichuan, Chengdu, China; 4.Institute of Frontier and Interdisciplinary Science, Shandong University, Shandong, Qingdao, 266237, China; 5.Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, 100049, China; 6.Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland; 7.Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg, 69029, Germany; 8.State Key Laboratory of Particle Detection and Electronics, China; 9.University of Science and Technology of China, Anhui, Hefei, 230026, China; 10.School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Sichuan, Chengdu, 610031, China; 11.School of Astronomy and Space Science, Nanjing University, Jiangsu, Nanjing, 210023, China; 12.Center for Astrophysics, Guangzhou University, Guangdong, Guangzhou, 510006, China; 13.Hebei Normal University, Hebei, Shijiazhuang, 050024, China; 14.Key Laboratory of Dark Matter and Space Astronomy, Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing, 210023, China; 15.Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, China; 16.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China; 17.Key Laboratory of Cosmic Rays (Tibet University, Ministry of Education, Tibet, Lhasa, 850000, China; 18.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China; 19.School of Physics and Astronomy (Zhuhai), School of Physics (Guangzhou), Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, 519000 Zhuhai, Guangdong, Guangzhou, 510275, China; 20.School of Physics and Astronomy, Yunnan University, Yunnan, Kunming, 650091, China; 21.Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, Geneva, 1211, Switzerland; 22.APC, Universit’e Paris Cit’e, CNRS, IN2P3, CEA, IRFU, Observatoire de Paris, Paris, 119 75205, France; 23.Department of Engineering Physics, Tsinghua University, Beijing, 100084, China; 24.School of Physics and Microelectronics, Zhengzhou University, Henan, Zhengzhou, 450001, China; 25.Yunnan Observatories, Chinese Academy of Sciences, Yunnan, Kunming, 650216, China; 26.College of Physics, Sichuan University, Sichuan, Chengdu, 610065, China; 27.Institute for Nuclear Research of Russian Academy of Sciences, Moscow, 117312, Russia; 28.Moscow Institute of Physics and Technology, Moscow, 141700, Russia; 29.School of Physics, Peking University, Beijing, 100871, China; 30.School of Physical Science and Technology, Guangxi University, Guangxi, Nanning, 530004, China; 31.Department of Physics, Faculty of Science, Mahidol University, Bangkok, 10400, Thailand; 32.Center 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; 33.National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China |
推荐引用方式 GB/T 7714 | Zhang, Hengying,He, Huihai,Feng, Cunfeng,et al. The all-particle spectrum and mean logarithmic mass of cosmic rays in the knee region by LHAASO-KM2A[C],2024. |
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