YNAO OpenIR  > 星系类星体研究组
Method to measure muon content of extensive air showers with LHAASO KM2A-WCDA synergy
Cao, Zhen1; Aharonian, F.4,5; An, Q.6,7; Axikegu8; Bai, L.X.9; Bai, Y.X.1,3; Bao, Y.W.10; Bastieri, D.11; Bi, X.J.1,2,3; Bi, Y.J.1,3; Cai, J.T.11; Cao, Q.12; Cao, W.Y.7; Cao, Zhe6,7; Chang, J.13; Chang, J.F.1,3,6; Chen, E.S.1,2,3; Chen, Liang13; Chen, Lin8; Chen, Long8; Chen, M.J.1,3; Chen, M.L.1,3,6; Chen, Q.H.8; Chen, S.H.1,2,3; Chen, S.Z.1,3; Chen, T.L.14; Chen, Y.10; Cheng, H.L.2,14,15; Cheng, N.1,3; Cheng, Y.D.1,3; Cui, S.W.12; Cui, X.H.15; Cui, Y.D.16; Dai, B.Z.17; Dai, H.L.1,3,6; Dai, Z.G.7; Danzengluobu14; della Volpe, D.18; Dong, X.Q.1,2,3; Duan, K.K.13; Fan, J.H.11; Fan, Y.Z.13; Fang, J.17; Fang, K.1,3; Feng, C.F.19; Feng, L.13; Feng, S.H.1,3; Feng, X.T.19; Feng, Y.L.14; Gao, B.1,3; Gao, C.D.19; Gao, L.Q.1,2,3; Gao, Q.14; Gao, W.1,3; Gao, W.K.1,2,3; Ge, M.M.17; Geng, L.S.1,3; Gong, G.H.20; Gou, Q.B.1,3; Gu, M.H.1,3,6; Guo, F.L.13; Guo, X.L.8; Guo, Y.Q.1,3; Guo, Y.Y.13; Han, Y.A.21; He, H.H.1,2,3; He, H.N.13; He, J.Y.13; He, X.B.16; He, Y.8; Heller, M.18; Hor, Y.K.16; Hou, B.W.1,2,3; Hou, C.1,3; Hou X(侯贤)22; Hu, H.B.1,2,3; Hu, Q.7,13; Hu, S.C.1,2,3; Huang, D.H.8; Huang, T.Q.1,3; Huang, W.J.16; Huang, X.T.19; Huang, X.Y.13; Huang, Y.1,2,3; Huang, Z.C.8; Ji, X.L.1,3,6; Jia, H.Y.8; Jia, K.19; Jiang, K.6,7; Jiang, X.W.1,3; Jiang, Z.J.17; Jin, M.8; Kang, M.M.9; Ke, T.1,3; Kuleshov, D.23; Kurinov, K.23; Li, B.B.12; Li, Cheng6,7; Li, Cong1,3; Li, D.1,2,3; Li, F.1,3,6; Li, H.B.1,3; Li, H.C.1,3; Li, H.Y.7,13; Li, J.7,13; Li, Jian7; Li, Jie1,3,6; Li, K.1,3; Li, W.L.19; Li, W.L.24; Li, X.R.1,3; Li, Xin6,7; Li, Y.Z.1,2,3; Li, Zhe1,3; Li, Zhuo25; Liang, E.W.26; Liang, Y.F.26; Lin, S.J.16; Liu, B.7; Liu, C.1,3; Liu, D.19; Liu, H.8; Liu, H.D.21; Liu, J.1,3; Liu, J.L.1,3; Liu, J.L.24; Liu, J.S.16; Liu, J.Y.1,3; Liu, M.Y.14; Liu, R.Y.10; Liu, S.M.8; Liu, W.1,3; Liu, Y.11; Liu, Y.N.20; Long, W.J.8; Lu, R.17; Luo, Q.16; Lv, H.K.1,3; Ma, B.Q.25; Ma, L.L.1,3; Ma, X.H.1,3; Mao JR(毛基荣)22; Min, Z.1,3; Mitthumsiri, W.27; Nan, Y.C.1,3; Ou, Z.W.16; Pang, B.Y.8; Pattarakijwanich, P.27; Pei, Z.Y.11; Qi, M.Y.1,3; Qi, Y.Q.12; Qiao, B.Q.1,3; Qin, J.J.7; Ruffolo, D.27; Sáiz, A.27; Shao, C.Y.16; Shao, L.12; Shchegolev, O.23,28; Sheng, X.D.1,3; Song, H.C.25; Stenkin, Yu.V.23,28; Stepanov, V.23; Su, Y.13; Sun, Q.N.8; Sun, X.N.26; Sun, Z.B.29; Tam, P.H.T.16; Tang, Z.B.6,7; Tian, W.W.2,15; Wang, C.29; Wang, C.B.8; Wang, G.W.7; Wang, H.G.11; Wang, H.H.16; Wang JC(王建成)22; Wang, J.S.24; Wang, K.10; Wang, L.P.19; Wang, L.Y.1,3; Wang, P.H.8; Wang, R.19; Wang, W.16; Wang, X.G.26; Wang, X.Y.10; Wang, Y.8; Wang, Y.D.1,3; Wang, Y.J.1,3; Wang, Z.H.9; Wang, Z.X.17; Wang, Zhen24; Wang, Zheng1,3,6; Wei, D.M.13; Wei, J.J.13; Wei, Y.J.1,2,3; Wen, T.17; Wu, C.Y.1,3; Wu, H.R.1,3; Wu, S.1,3; Wu, X.F.13; Wu, Y.S.7; Xi, S.Q.1,3; Xia, J.7,13; Xia, J.J.8; Xiang, G.M.2,13; Xiao, D.X.12; Xiao, G.1,3; Xin, G.G.1,3; Xin, Y.L.8; Xing, Y.13; Xiong, Z.1,2,3; Xu, D.L.24; Xu, R.F.1,2,3; Xu, R.X.25; Xue, L.19; Yan, D.H.17; Yan, J.Z.13; Yan, T.1,3; Yang, C.W.9; Yang, F.12; Yang, F.F.1,3,6; Yang, H.W.16; Yang, J.Y.16; Yang, L.L.16; Yang, M.J.1,3; Yang, R.Z.7; Yang, S.B.17; Yao, Y.H.9; Yao, Z.G.1,3; Ye, Y.M.20; Yin, L.Q.1,3; Yin, N.19; You, X.H.1,3; You, Z.Y.1,2,3; Yu, Y.H.7; Yuan, Q.13; Yue, H.1,2,3; Zeng, H.D.13; Zeng, T.X.1,3,6; Zeng, W.17; Zeng, Z.K.1,2,3; Zha, M.1,3; Zhang, B.B.10; Zhang, F.8; Zhang, H.M.10; Zhang, H.Y.1,3; Zhang, J.L.15; Zhang, L.X.11; Zhang, Li17; Zhang, P.F.17; Zhang, P.P.7,13; Zhang, R.7,13; Zhang, S.B.2,15; Zhang, S.R.12; Zhang, S.S.1,3; Zhang, X.10; Zhang, X.P.1,3; Zhang, Y.F.8; Zhang, Yi1,13; Zhang, Yong1,3; Zhao, B.8; Zhao, J.1,3; Zhao, L.6,7; Zhao, L.Z.12; Zhao, S.P.13,19; Zheng, F.29; Zheng, Y.8; Zhou, B.1,3; Zhou, H.24; Zhou, J.N.13; Zhou, P.10; Zhou, R.9; Zhou, X.X.8; Zhu, C.G.19; Zhu, F.R.8; Zhu, H.15; Zhu, K.J.1,2,3,6; Zuo, X.1,3
发表期刊NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT
2024-02
卷号1059
DOI10.1016/j.nima.2023.168958
产权排序第22完成单位
收录类别SCI ; EI
关键词Muon measurement Water Cherenkov Detector LHAASO
摘要The measurement of shower muons on an event-by-event basis offers a potent tool for conducting ground-based experiments on gamma rays and cosmic rays due to its sensitivity to primary mass and interaction models. In recent years, underground water Cherenkov detectors as large-area muon counters provide the most powerful way of rejecting cosmic ray background when searching for TeV-PeV gamma rays and cosmic ray electrons, an unprecedented rejection power of 104-105 is achieved. Unburied water Cherenkov detectors are widely used in ground-based gamma astronomy experiments, e.g, Milagro, HAWC, LHAASO-WCDA, etc. However, due to the presence of electromagnetic components, their deployment as event-by-event muon counters has encountered considerable challenges. All the experiments mentioned above reconstruct lateral-distribution -function related parameters to tell a gamma from hadrons. In this work, we first developed a method to utilize the WCDA, to specify muon content in each shower with LHAASO KM2A-WCDA synergy and help LHAASO to gain approximately a 37,650-meter-square effective area as a muon counter.
资助项目Chengdu Management Committee of Tianfu New Area; National Key R&D program of China[2018YFA0404201]; National Science Foundation of China, NSFC[12205314]; National Science Foundation of China, NSFC[12022502]; National Science Foundation of China, NSFC[12105294]; Youth Innovation Promotion Association CAS[2022010]; National Science and Technology Develop-ment Agency (NSTDA); National Research Council of Thailand (NRCT) : High-Potential Research Team Grant Program[N42A650868]
项目资助者Chengdu Management Committee of Tianfu New Area ; National Key R&D program of China[2018YFA0404201] ; National Science Foundation of China, NSFC[12205314, 12022502, 12105294] ; Youth Innovation Promotion Association CAS[2022010] ; National Science and Technology Develop-ment Agency (NSTDA) ; National Research Council of Thailand (NRCT) : High-Potential Research Team Grant Program[N42A650868]
语种英语
学科领域天文学
文章类型Article
出版者ELSEVIER
出版地RADARWEG 29, 1043 NX AMSTERDAM, NETHERLANDS
ISSN0168-9002
URL查看原文
WOS记录号WOS:001141700900001
WOS研究方向Instruments & Instrumentation ; Nuclear Science & Technology ; Physics
WOS类目Instruments & Instrumentation ; Nuclear Science & Technology ; Physics, Nuclear ; Physics, Particles & Fields
关键词[WOS]GAMMA-RAY EMISSION ; COSMIC-RAYS
EI入藏号20234915184981
EI主题词Gamma rays
EI分类号444.2 Groundwater - 657 Space Physics - 657.2 Extraterrestrial Physics and Stellar Phenomena - 922.1 Probability Theory - 931.3 Atomic and Molecular Physics - 932.1 High Energy Physics - 944.7 Radiation Measuring Instruments
引用统计
文献类型期刊论文
版本出版稿
条目标识符http://ir.ynao.ac.cn/handle/114a53/26513
专题星系类星体研究组
高能天体物理研究组
作者单位1.Key Laboratory of Particle Astrophyics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Beijing, 100049, China;
2.University of Chinese Academy of Sciences, Beijing, 100049, China;
3.TIANFU Cosmic Ray Research Center, Chengdu, Sichuan, China;
4.Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2 Dublin, Ireland;
5.Max–Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg, 69029, Germany;
6.State Key Laboratory of Particle Detection and Electronics, China;
7.University of Science and Technology of China, Hefei, 230026, Anhui, China;
8.School of Physical Science and Technology & School of Information Science and Technology, Southwest Jiaotong University, Chengdu, 610031, Sichuan, China;
9.College of Physics, Sichuan University, Chengdu, 610065, Sichuan, China;
10.School of Astronomy and Space Science, Nanjing University, Nanjing, 210023, Jiangsu, China;
11.Center for Astrophysics, Guangzhou University, Guangzhou, 510006, Guangdong, China;
12.Hebei Normal University, Shijiazhuang, 050024, Hebei, China;
13.Key Laboratory of Dark Matter and Space Astronomy & Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, 210023, Jiangsu, China;
14.Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Lhasa, 850000, Tibet, China;
15.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China;
16.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 & 510275 Guangzhou, Guangdong, China;
17.School of Physics and Astronomy, Yunnan University, Kunming, 650091, Yunnan, China;
18.Departement de Physique Nucleaire et Corpusculaire, Faculte de Sciences, Universite de Geneave, 24 Quai Ernest Ansermet, 1211 Geneva, Switzerland;
19.Institute of Frontier and Interdisciplinary Science, Shandong University, Qingdao, 266237, Shandong, China;
20.Department of Engineering Physics, Tsinghua University, Beijing, 100084, China;
21.School of Physics and Microelectronics, Zhengzhou University, Zhengzhou, 450001, Henan, China;
22.Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, Yunnan, China;
23.Institute for Nuclear Research of Russian Academy of Sciences, Moscow, 117312, Russia;
24.Tsung-Dao Lee Institute & School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, China;
25.School of Physics, Peking University, Beijing, 100871, China;
26.School of Physical Science and Technology, Guangxi University, Nanning, 530004, Guangxi, China;
27.Department of Physics, Faculty of Science, Mahidol University, Bangkok, 10400, Thailand;
28.Moscow Institute of Physics and Technology, Moscow, 141700, Russia;
29.National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China
推荐引用方式
GB/T 7714
Cao, Zhen,Aharonian, F.,An, Q.,et al. Method to measure muon content of extensive air showers with LHAASO KM2A-WCDA synergy[J]. NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT,2024,1059.
APA Cao, Zhen.,Aharonian, F..,An, Q..,Axikegu.,Bai, L.X..,...&Zuo, X..(2024).Method to measure muon content of extensive air showers with LHAASO KM2A-WCDA synergy.NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT,1059.
MLA Cao, Zhen,et al."Method to measure muon content of extensive air showers with LHAASO KM2A-WCDA synergy".NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT 1059(2024).
条目包含的文件
文件名称/大小 文献类型 版本类型 开放类型 使用许可
Method to measure mu(1177KB)期刊论文出版稿开放获取CC BY-NC-SA浏览 请求全文
个性服务
推荐该条目
保存到收藏夹
查看访问统计
导出为Endnote文件
谷歌学术
谷歌学术中相似的文章
[Cao, Zhen]的文章
[Aharonian, F.]的文章
[An, Q.]的文章
百度学术
百度学术中相似的文章
[Cao, Zhen]的文章
[Aharonian, F.]的文章
[An, Q.]的文章
必应学术
必应学术中相似的文章
[Cao, Zhen]的文章
[Aharonian, F.]的文章
[An, Q.]的文章
相关权益政策
暂无数据
收藏/分享
文件名: Method to measure muon content of extensive air showers with LHAASO KM2A-WCDA synergy.pdf
格式: Adobe PDF
所有评论 (0)
暂无评论
 

除非特别说明,本系统中所有内容都受版权保护,并保留所有权利。