The Application of 20 inch MCP-PMT In LHAASO-WCDA

doi:10.22323/1.395.0696

YNAO OpenIR > 星系类星体研究组

	The Application of 20 inch MCP-PMT In LHAASO-WCDA
	You, Xiaohao 1,3; Gao, Bo 1,3; Chen, MingJun 1,3; Li, HuiCai 1,3; Liu, Cheng 1,3; Li, Kai 1,3; Cao, Zhen 1,2,3; Aharonian, F.4,5; An, Q.6,7; Axikegu 8; 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, H.12; Cai, J. T.11; Cao, Zhe 6,7; Chang, J.13; Chang, J. F.1,3,6; Chen, B. M.14; Chen, E. S.1,2,3; Chen, J.9; Chen, Liang 1,2,3; Chen, Liang 15; Chen, Long 8; Chen, M. L.1,3,6; Chen, Q. H.8; Chen, S. H.1,2,3; Chen, S. Z.1,3; Chen, T. L.16; Chen, X. L.1,2,3; Chen, Y.10; Cheng, N.1,3; Cheng, Y. D.1,3; Cui, S. W.14; Cui, X. H.17; Cui, Y. D.18; D'Ettorre Piazzoli, B.19; Dai, B. Z.20; Dai, H. L.1,3,6; Dai, Z. G.7; Danzengluobu 16; della Volpe, D.21; Dong, X. J.1,3; Duan, K. K.13; Fan, J. H.11; Fan, Y. Z.13; Fan, Z. X.1,3; Fang, J.20; Fang, K.1,3; Feng, C. F.22; Feng, L.13; Feng, S. H.1,3; Feng, Y. L.13; Gao, C. D.22; Gao, L. Q.1,2,3; Gao, Q.16; Gao, W.22; Ge, M. M.20; Geng, L. S.1,3; Gong, G. H.23; Gou, Q. B.1,3; Gu, M. H.1,3,6; Guo, F. L.15; Guo, J. G.1,2,3; Guo, X. L.8; Guo, Y. Q.1,3; Guo, Y. Y.1,2,3,13; Han, Y. A.24; He, H. H.1,2,3; He, H. N.13; He, J. C.1,2,3; He, S. L.11; He, X. B.18; He, Y.8; Heller, M.21; Hor, Y. K.18; Hou, C.1,3; Hu, H. B.1,2,3; Hu, S.9; Hu, S. C.1,2,3; Hu, X. J.23; Huang, D. H.8; Huang, Q. L.1,3; Huang, W. H.22; Huang, X. T.22; Huang, X. Y.13; Huang, Z. C.8; Ji, F.1,3; Ji, X. L.1,3,6; Jia, H. Y.8; Jiang, K.6,7; Jiang, Z. J.20; Jin, C.1,2,3; Ke, T.1,3; Kuleshov, D.25; Levochkin, K.25; Li, B. B.14; Li, Cheng 6,7; Li, Cong 1,3; Li, F.1,3,6; Li, H. B.1,3; Li, H. Y.7,13; Li, J.1,3,6; Li, W. L.22; Li, X. R.1,3; Li, Xin 6,7; Li, Xin 8; Li, Y.9; Li, Y. Z.1,2,3; Li, Zhe 1,3; Li, Zhuo 26; Liang, E. W.27; Liang, Y. F.27; Lin, S. J.18; Liu, B.7; Liu, D.22; Liu, H.8; Liu, H. D.24; Liu, J.1,3; Liu, J. L.28; Liu, J. S.18; Liu, J. Y.1,3; Liu, M. Y.16; Liu, R. Y.10; Liu, S. M.8; Liu, W.1,3; Liu, Y.11; Liu, Y. N.23; Liu, Z. X.9; Long, W. J.8; Lu, R.20; Lv, H. K.1,3; Ma, B. Q.26; Ma, L. L.1,3; Ma, X. H.1,3; Mao JR(毛基荣)29 ; Masood, A.8; Min, Z.1,3; Mitthumsiri, W.30; Montaruli, T.21; Nan, Y. C.22; Pang, B. Y.8; Pattarakijwanich, P.30; Pei, Z. Y.11; Qi, M. Y.1,3; Qi, Y. Q.14; Qiao, B. Q.1,3; Qin, J. J.7; Ruffolo, D.30; Rulev, V.25; Sáiz, A.30; Shao, L.14; Shchegolev, O.25,31; Sheng, X. D.1,3; Shi, J. Y.1,3; Song, H. C.26; Stenkin, Yu. V.25,31; Stepanov, V.25; Su, Y.32; Sun, Q. N.8; Sun, X. N.27; Sun, Z. B.33; Tam, P. H.18; Tang, Z. B.6,7; Tian, W. W.2,17; Wang, B. D.1,3; Wang, C.33; Wang, H.8; Wang, H. G.11
会议录名称	Proceedings of Science
	2022-03-18
卷号	395
DOI	10.22323/1.395.0696
产权排序	第29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	In the Large High Altitude Air Shower Observatory (LHAASO), the main physics objective of the Water Cherenkov Detector Array (WCDA) is to survey the gamma-ray sky continuously in the energy range from 100 GeV to PeV. The Water Cherenkov detector array, covering an area of about 78,000 m2 area, is constituted by 3120 detector units divided into 3 separate arrays. In the second and third array are installed 2220 20" PMTs instead of the 8 PMT used in the first 150 × 150m2 array. This type of PMT has large sensitive area, high quantum efficiency (QE), and large peak-to-valley (P/V) ratio for single photoelectron detection. In this work, we will report on the application of 20 inch MCP-PMT at LHAASO-WCDA. © Copyright owned by the author(s) under the terms of the Creative Commons Attribution-NonCommercial-NoDerivatives 4.0 International License (CC BY-NC-ND 4.0)
资助项目	N/A
项目资助者	N/A
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	20230113326382
EI主题词	Gamma rays
EI分类号	657 Space Physics - 657.2 Extraterrestrial Physics and Stellar Phenomena - 931.3 Atomic and Molecular Physics - 932.1 High Energy Physics - 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/114a53/25727
专题	星系类星体研究组
作者单位	1.Key Laboratory of Particle Astrophyics, Experimental Physics Division, Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 19B Yuquan Road, Shijingshan District, Beijing, 100049, China; 2.University of Chinese Academy of Sciences, Beijing, 100049, China; 3.TIANFU Cosmic Ray Research Center, Sichuan, Chengdu, 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, Anhui, Hefei, 230026, China; 8.School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Sichuan, Chengdu, 610031, China; 9.College of Physics, Sichuan University, Sichuan, Chengdu, 610065, China; 10.School of Astronomy and Space Science, Nanjing University, Jiangsu, Nanjing, 210023, China; 11.Center for Astrophysics, Guangzhou University, Guangdong, Guangzhou, 510006, China; 12.School of Physics and Technology, Wuhan University, Hubei, Wuhan, 430072, China; 13.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing, 210023, China; 14.Hebei Normal University, Hebei, Shijiazhuang, 050024, China; 15.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China; 16.Key Laboratory of Cosmic Rays, Tibet University, Ministry of Education, Tibet, Lhasa, 850000, China; 17.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China; 18.School of Physics and Astronomy, School of Physics (Guangzhou), Sun Yat-sen University, Guangdong, Zhuhai, 519000, China; 19.Dipartimento di Fisica, Università di Napoli 'Federico II 20.School of Physics and Astronomy, Yunnan University, Yunnan, Kunming, 650091, China; 21.Departement de Physique Nucleaire et Corpusculaire, Faculte de Sciences, Universite de Gen'eve, 24 Quai Ernest Ansermet, Geneva, 1211, Switzerland; 22.Institute of Frontier and Interdisciplinary Science, Shandong University, Shandong, Qingdao, 266237, China; 23.Department of Engineering Physics, Tsinghua University, Beijing, 100084, China; 24.School of Physics and Microelectronics, Zhengzhou University, Henan, Zhengzhou, 450001, China; 25.Institute for Nuclear Research of Russian Academy of Sciences, Moscow, 117312, Russia; 26.School of Physics, Peking University, Beijing, 100871, China; 27.School of Physical Science and Technology, Guangxi University, Guangxi, Nanning, 530004, China; 28.Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, China; 29.Yunnan Observatories, Chinese Academy of Sciences, Yunnan, Kunming, 650216, China; 30.Department of Physics, Faculty of Science, Mahidol University, Bangkok, 10400, Thailand; 31.Moscow Institute of Physics and Technology, Moscow, 141700, Russia; 32.Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing, 210023, China; 33.National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China
推荐引用方式 GB/T 7714	You, Xiaohao,Gao, Bo,Chen, MingJun,et al. The Application of 20 inch MCP-PMT In LHAASO-WCDA[C]:Sissa Medialab Srl,2022.

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