Study of longitudinal development of cosmic-ray induced air showers with LHAASO-WFCTA

doi:10.22323/1.395.0245

YNAO OpenIR > 星系类星体研究组

	Study of longitudinal development of cosmic-ray induced air showers with LHAASO-WFCTA
	Liu, Hu 1; Cao, Zhen 2,3,4; Aharonian, F.5,6; An, Q.7,8; Axikegu 9; Bai, L. X.10; Bai, Y. X.2,4; Zhu, H.18; Zhu, K. J.2,3,4,7; 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, Zhe 7,8; Chang, J.14; Chang, J. F.2,4,7; Chen, B. M.15; Chen, E. S.2,3,4; Chen, J.10; Chen, Liang 2,3,4,16; Zhu, F. R.9; Chen, Long 9; 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; Danzengluobu 17; 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, Cheng 7,8; Li, Cong 2,4; 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, Xin 7,8,9; Zuo, X.2,4; Li, Y.10; Li, Y. Z.2,3,4; Li, Zhe 2,4; Li, Zhuo 27; Liang, E. W.28; Liang, Y. F.28; Lin, S. J.19; Liu, B.8; Liu, C.2,4; Liu, D.23; Lia, 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; Wang, C.34
会议录名称	Proceedings of Science
	2022-03-18
卷号	395
DOI	10.22323/1.395.0245
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 Wide Field-of-view Cerenkov Telescope Array (WFCTA) is an important component of Large High Altitude Air Shower Observatory (LHAASO), which aims to measure the individual energy spectra of cosmic rays from ~30 TeV to a couple of EeV. The longitudinal development is one of the main tools to distinguish nuclei from each other. WFCTA is composed of 18 imaging air Cerenkov telescopes, each telescope has 32 × 32 pixels, covers a field of view 16o × 16o (each pixel corresponding to 0.5o × 0.5o). The first telescope started in operation since February 2019, up to now, there are 18 telescopes in operation. Cerenkov photon detected by different pixels were generated at different height (or different traversed material). The distribution of dN/dθ (θ is the angle between the direction of Cerenkov photon and the direction of primary particle) is reconstructed from the image of WFCTA to study the longitudinal development of the shower (similar to dN/dX). In this paper, the dN/dθ reconstructing method and the preliminary result on the particle identification power based on this method 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	20230213348371
EI主题词	Pixels
EI分类号	657 Space Physics - 657.2 Extraterrestrial Physics and Stellar Phenomena - 931.3 Atomic and Molecular Physics
引用统计
文献类型	会议论文
条目标识符	http://ir.ynao.ac.cn/handle/114a53/25744
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, 2, 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	Liu, Hu,Cao, Zhen,Aharonian, F.,et al. Study of longitudinal development of cosmic-ray induced air showers with LHAASO-WFCTA[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 longitudina（1448KB）	会议论文		开放获取	CC BY-NC-SA	浏览请求全文