YNAO OpenIR  > 星系类星体研究组
Study of Energy Measurement of Cosmic Ray Nuclei with LHAASO
Bai, Lu1; Liu, Hu1; Cao, Zhen2,3,4; Aharonian, F.5,6; An, Q.7,8; Axikegu9; Bai, L. X.10; Bai, Y. X.2,4; Bai, L. X.10; Bai, Y. X.2,4; Bao, Y. W.11; Bastieri, D.12; Bi, X. J.2,3,4; Bi, Y. J.2,4; Cai, H.13; Cai, J. T.12; Cao, Zhe7,8; Chang, J.14; Chang, J. F.2,4,7; Chen, B. M.15; Chen, E. S.2,3,4; Chen, J.10; Chen, Liang2,3,4; Chen, Liang16; Chen, Long9; Chen, M. J.2,4; Chen, M. L.2,4,7; Chen, Q. H.9; Chen, S. H.2,3,4; Chen, S. Z.2,4; Chen, T. L.17; Chen, X. L.2,3,4; Chen, Y.11; Cheng, N.2,4; Cheng, Y. D.2,4; Cui, S. W.15; Cui, X. H.18; Cui, Y. D.19; D’Ettorre Piazzoli, B.20; Dai, B. Z.21; Dai, H. L.2,4,7; Dai, Z. G.8; Danzengluobu17; della Volpe, D.22; Dong, X. J.2,4; Duan, K. K.14; Fan, J. H.12; Fan, Y. Z.14; Fan, Z. X.2,4; Fang, J.21; Fang, K.2,4; Feng, C. F.23; Feng, L.14; Feng, S. H.2,4; Feng, Y. L.14; Gao, B.2,4; Gao, C. D.23; Gao, L. Q.2,3,4; Gao, Q.17; Gao, W.23; Ge, M. M.21; Geng, L. S.2,4; Gong, G. H.24; Gou, Q. B.2,4; Gu, M. H.2,4,7; Guo, F. L.16; Guo, J. G.2,3,4; Guo, X. L.9; Guo, Y. Q.2,4; Guo, Y. Y.2,3,4,14; Han, Y. A.25; He, H. H.2,3,4; He, H. N.14; He, J. C.2,3,4; He, S. L.12; He, X. B.19; He, Y.9; Heller, M.22; Hor, Y. K.19; Hou, C.2,4; Hu, H. B.2,3,4; Hu, S.10; Hu, S. C.2,3,4; Hu, X. J.24; Huang, D. H.9; Huang, Q. L.2,4; Huang, W. H.23; Huang, X. T.23; Huang, X. Y.14; Huang, Z. C.9; Ji, F.2,4; Ji, X. L.2,4,7; Jia, H. Y.9; Jiang, K.7,8; Jiang, Z. J.21; Jin, C.2,3,4; Ke, T.2,4; Kuleshov, D.26; Levochkin, K.26; Li, B. B.15; Li, Cheng7,8; Li, Cong2,4; Li, F.2,4,7; Li, H. B.2,4; Li, H. C.2,4; Li, H. Y.8,14; Li, J.2,4,7; Li, K.2,4; Li, W. L.23; Li, X. R.2,4; Li, Xin7,8; Li, Xin9; Li, Y.10; Li, Y. Z.2,3,4; Li, Zhe2,4; Li, Zhuo27; Liang, E. W.28; Liang, Y. F.28; Lin, S. J.19; Liu, B.8; Liu, C.2,4; Liu, D.23; Liu, H.9; Liu, H. D.25; Liu, J.2,4; Liu, J. L.29; Liu, J. S.19; Liu, J. Y.2,4; Liu, M. Y.17; Liu, R. Y.11; Liu, S. M.9; Liu, W.2,4; Liu, Y.12; Liu, Y. N.24; Liu, Z. X.10; Long, W. J.9; Lu, R.21; Lv, H. K.2,4; Ma, B. Q.27; Ma, L. L.2,4; Ma, X. H.2,4; Mao JR(毛基荣)30; Masood, A.9; Min, Z.2,4; Mitthumsiri, W.31; Montaruli, T.22; Nan, Y. C.23; Pang, B. Y.9; Pattarakijwanich, P.31; Pei, Z. Y.12; Qi, M. Y.2,4; Qi, Y. Q.15; Qiao, B. Q.2,4; Qin, J. J.8; Ruffolo, D.31; Rulev, V.26; Sáiz, A.31; Shao, L.15; Shchegolev, O.26,32; Sheng, X. D.2,4; Shi, J. Y.2,4; Song, H. C.27; Stenkin, Yu. V.26,32; Stepanov, V.26; Su, Y.33; Sun, Q. N.9; Sun, X. N.28; Sun, Z. B.34; Tam, P. H.19; Tang, Z. B.7,8; Tian, W. W.3,18; Wang, B. D.2,4
会议录名称Proceedings of Science
2022-03-18
卷号395
DOI10.22323/1.395.0246
产权排序第30完成单位
收录类别EI
会议名称37th International Cosmic Ray Conference, ICRC 2021
会议日期2021-07-12
会议地点Virtual, Berlin, Germany
摘要

The Large High Altitude Air Shower Observatory (LHAASO) is a hybrid extensive air shower (EAS) array with an area of about 1 km2 at an altitude of 4410 m a.s.l. in Sichuan province, China. It contains three sub-detectors: 1 km2 array (KM2A) composed of 5195 electromagnetic particle detector (ED) and muon detector (MD); water Cerenkov detector array (WCDA) and 18 Wide Field-of-view Cerenkov Telescope Array (WFCTA). One of the main scientific goals is measuring the individual energy spectra of cosmic rays from ~30 TeV to a couple of EeV. The construction of the whole observatory will be completed by the end of 2021. In this paper, a new energy reconstruction method and result based on KM2A simulated nuclei events will be shown. © Copyright owned by the author(s).

资助项目National Natural Science Foundation of China[11947404] ; Department of Science and Technology of Sichuan Province[2020YFSY0016] ; Department of Science and Technology of Sichuan Province[2021YFSY0031]
项目资助者National Natural Science Foundation of China[11947404] ; Department of Science and Technology of Sichuan Province[2020YFSY0016,2021YFSY0031]
语种英语
学科领域天文学 ; 天体物理学 ; 高能天体物理学 ; 核科学技术
文章类型Conference article (CA)
出版者Sissa Medialab Srl
URL查看原文
EI入藏号20225213290503
EI主题词Observatories
EI分类号657 Space Physics - 657.2 Extraterrestrial Physics and Stellar Phenomena - 944.7 Radiation Measuring Instruments
引用统计
文献类型会议论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/25686
专题星系类星体研究组
作者单位1.Southwest Jiaotong University, Xipu Campus, Southwest Jiaotong University, Chengdu, 611756, China;
2.Key Laboratory of Particle Astrophyics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, 100049, China;
3.University of Chinese Academy of Sciences, Beijing, 100049, China;
4.TIANFU Cosmic Ray Research Center, Sichuan, Chengdu, China;
5.Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin, Ireland;
6.Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg, 69029, Germany;
7.State Key Laboratory of Particle Detection and Electronics, China;
8.University of Science and Technology of China, Anhui, Hefei, 230026, China;
9.School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Sichuan, Chengdu, 610031, China;
10.College of Physics, Sichuan University, Sichuan, Chengdu, 610065, 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.School of Physics and Technology, Wuhan University, Hubei, Wuhan, 430072, China;
14.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing, 210023, China;
15.Hebei Normal University, Hebei, Shijiazhuang, 050024, 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, School of Physics (Guangzhou), Sun Yat-sen University, Guangdong, Zhuhai, 519000, China;
20.Dipartimento di Fisica dell’Università di Napoli `‘Federico II
21.School of Physics and Astronomy, Yunnan University, Yunnan, Kunming, 650091, China;
22.D¡¯epartement de Physique Nucl¡¯eaire et Corpusculaire, Facult¡¯e de Sciences, Universit¡¯e de Gen‘eve, 24 Quai Ernest Ansermet, Geneva, 1211, Switzerland;
23.Institute of Frontier and Interdisciplinary Science, Shandong University, Shandong, Qingdao, 266237, China;
24.Department of Engineering Physics, Tsinghua University, Beijing, 100084, China;
25.School of Physics and Microelectronics, Zhengzhou University, Henan, Zhengzhou, 450001, China;
26.Institute for Nuclear Research of Russian Academy of Sciences, Moscow, 117312, Russia;
27.School of Physics, Peking University, Beijing, 100871, China;
28.School of Physical Science and Technology, Guangxi University, Guangxi, Nanning, 530004, China;
29.Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, China;
30.Yunnan Observatories, Chinese Academy of Sciences, Yunnan, Kunming, 650216, China;
31.Department of Physics, Faculty of Science, Mahidol University, Bangkok, 10400, Thailand;
32.Moscow Institute of Physics and Technology, Moscow, 141700, Russia;
33.Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing, 210023, China;
34.National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China
推荐引用方式
GB/T 7714
Bai, Lu,Liu, Hu,Cao, Zhen,et al. Study of Energy Measurement of Cosmic Ray Nuclei with LHAASO[C]:Sissa Medialab Srl,2022.
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
Study of Energy Meas(2247KB)会议论文 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
[Bai, Lu]的文章
[Liu, Hu]的文章
[Cao, Zhen]的文章
百度学术
百度学术中相似的文章
[Bai, Lu]的文章
[Liu, Hu]的文章
[Cao, Zhen]的文章
必应学术
必应学术中相似的文章
[Bai, Lu]的文章
[Liu, Hu]的文章
[Cao, Zhen]的文章
相关权益政策
暂无数据
收藏/分享
文件名: Study of Energy Measurement of Cosmic Ray Nuclei with LHAASO.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。