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Data analysis and key science results of LHAASO-WCDA
Zha, Min1; Gao, Chuandong2; Hu, Shicong1,2; Lin, Shujie3; Wang, Zhen5; Xiang, Guangman2,4,6; Yao, Zhiguo1,6; Zhou, Hao5; Aharonian, F.30,31; An, Q.9,10; Axikegu24; Bai, L. X.25; Bai, Y. X.6,8; Bao, Y. W.20; Bastieri, D.15; Bi, X. J.6,7,8; Bi, Y. J.6,8; Cai, H.27; Cai, J. T.15; Cao, Z.6,7,8,9,10; Zhou, J. N.22; Chang, J.21; Chang, J. F.6,8,9; Chang, X. C.6,8; Chen, B. M.18; Chen, J.25; Chen, L.6,7,8,22,24; Zhou, X. X.24; Zhu, C. G.2; Chen, M. J.6,8; Chen, M. L.6,8,9; Chen, Q. H.24; Chen, S. H.6,7,8; Chen, S. Z.6,8; Chen, T. L.26; Chen, X. L.6,7,8; Chen, Y.20; Cheng, N.6,8; Cheng, Y. D.6,8; Cui, S. W.18; Cui, X. H.12; Cui, Y. D.16; Dai, B. Z.28; Dai, H. L.6,8,9; Dai, Z. G.20; Danzengluobu26; della Volpe, D.35; D’Ettorre Piazzoli, B.32; Dong, X. J.6,8; Fan, J. H.15; Fan, Y. Z.21; Fan, Z. X.6,8; Fang, J.28; Fang, K.6,8; Feng, C. F.2; Feng, L.21; Feng, S. H.6,8; Feng, Y. L.21; Gao, B.6,8; Goa, C. D.2; Gao, Q.26; Gao, W.2; Ge, M. M.28; Geng, L. S.6,8; Gong, G. H.11; Gou, Q. B.6,8; Gu, M. H.6,8,9; Guo, J. G.6,7,8; Guo, X. L.24; Guo, Y. Q.6,8; Guo, Y. Y.6,7,8,21; Han, Y. A.19; He, H. H.6,7,8; He, H. N.21; He, J. C.6,7,8; He, S. L.15; He, X. B.16; He, Y.24; Heller, M.35; Hor, Y. K.16; Hou, C.6,8; Hou X(侯贤)29; Hu, H. B.6,7,8; Hu, S.25; Zheng, Y.24; Hu, X. J.11; Huang, D. H.24; Huang, Q. L.6,8; Huang, W. H.2; Huang, X. T.2; Huang, Z. C.24; Ji, F.6,8; Ji, X. L.6,8,9; Jia, H. Y.24; Jiang, K.9,10; Jiang, Z. J.28; Jin, C.6,7,8; Kuleshov, D.33; Levochkin, K.33; Li, B. B.18; Li, C.6,8,9,10; Zhou, P.20; Li, F.6,8,9; Li, H. B.6,8; Li, H. C.6,8; Li, H. Y.10,21; Li, J.6,8,9; Li, K.6,8; Li, W. L.2; Li, X.9,10,24; Zhu, H.12; Li, X. R.6,8; Li, Y.25; Li, Y. Z.6,7,8; Li, Z.6,8,14; Zhou, R.25; Liang, E. W.17; Liang, Y. F.17; Lin, S. J.16; Liu, B.10; Liu, C.6,8; Liu, D.2; Liu, H.24; Liu, H. D.19; Liu, J.6,8; Liu, J. L.23; Liu, J. S.16; Liu, J. Y.6,8; Liu, M. Y.26; Liu, R. Y.20; Liu, S. M.21; Liu, W.6,8; Liu, Y. N.11; Liu, Z. X.25; Long, W. J.24; Lu, R.28; Lv, H. K.6,8; Ma, B. Q.14; Ma, L. L.6,8; Ma, X. H.6,8; Mao JR(毛基荣)29; Masood, A.24; Mitthumsiri, W.36; Montaruli, T.35; Nan, Y. C.2; Pang, B. Y.24; Pattarakijwanich, P.36; Pei, Z. Y.15; Qi, M. Y.6,8; Qiao, B. Q.6; Ruffolo, D.36; Rulev, V.33; Sáiz, A.36; Shao, L.18; Shchegolev, O.33,34; Sheng, X. D.6,8; Shi, J. R.6,8; Song, H. C.14; Stenkin, Yu. V.33,34; Stepanov, V.33; Sun, Q. N.24; Sun, X. N.17; Sun, Z. B.13; Tam, P. H.16; Tang, Z. B.9,10; Tian, W. W.7,12; Wang, B. D.6,8; Wang, C.13; Wang, H.24; Wang, H. G.15; Wang JC(王建成)29
会议录名称Proceedings of Science
2022-03-18
卷号395
DOI10.22323/1.395.0860
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

The Water Cherenkov Detector Array (WCDA) is an important component of Large High Altitude Air Shower Observatory (LHAASO). The main scientific target of WCDA is continuously surveying the northern sky at the level of few percent of Crab unit. In this proceeding, based on its first year data of WCDA-1 data, the result about the Crab Nebular observation and its energy spectrum measurment have been presented. And with WCDA full array data taking since Mar. 2021, some preliminary results have been reported. © Copyright owned by the author(s).

资助项目National Natural Science Foundation of China[11635011] ; National Natural Science Foundation of China[11675187] ; National Natural Science Foundation of China[11761141001] ; National Natural Science Foundation of China[11905227] ; National Natural Science Foundation of China[12022502] ; National Natural Science Foundation of China[RTA6280002] ; National Natural Science Foundation of China[U1831208] ; National Natural Science Foundation of China[U1931111] ; National Natural Science Foundation of China[U1931112] ; National Natural Science Foundation of China[Y811A35]
项目资助者National Natural Science Foundation of China[11635011, 11675187, 11761141001, 11905227, 12022502, RTA6280002, U1831208, U1931111, U1931112, Y811A35]
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20230213367599
EI主题词Cosmology
EI分类号461.9 Biology - 657 Space Physics - 657.2 Extraterrestrial Physics and Stellar Phenomena
引用统计
文献类型会议论文
条目标识符http://ir.ynao.ac.cn/handle/114a53/25736
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, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, 100049, China;
2.Institute of Frontier and Interdisciplinary Science, Shandong University, Shandong, Qingdao, 266237, China;
3.School of Physies and Astronomy, School of Physics (Guangzhou), Sun Yat-sen University, Guangdong, Zhuhai, 519082, China;
4.Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China;
5.Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, China;
6.Key Laboratory of Particle Astrophyics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, 100049, China;
7.University of Chinese Academy of Sciences, Beijing, 100049, China;
8.TIANFU Cosmic Ray Research Center, Sichuan, Chengdu, China;
9.State Key Laboratory of Particle Detection and Electronics, China;
10.University of Science and Technology of China, Anhui, Hefei, 230026, China;
11.Department of Engineering Physics, Tsinghua University, Beijing, 100084, China;
12.National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China;
13.National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China;
14.School of Physics, Peking University, Beijing, 100871, China;
15.Center for Astrophysics, Guangzhou University, Guangdong, Guangzhou, 510006, China;
16.School of Physics and Astronomy, School of Physics (Guangzhou), Sun Yat-sen University, Guangdong, Zhuhai, 519082, China;
17.School of Physical Science and Technology, Guangxi University, Guangxi, Nanning, 530004, China;
18.Hebei Normal University, Hebei, Shijiazhuang, 050024, China;
19.School of Physics and Microelectronics, Zhengzhou University, Henan, Zhengzhou, 450001, China;
20.School of Astronomy and Space Science, Nanjing University, Jiangsu, Nanjing, 210023, China;
21.Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing, 210023, China;
22.Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China;
23.Tsung Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, China;
24.School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Sichuan, Chengdu, 610031, China;
25.College of Physics, Sichuan University, Sichuan, Chengdu, 610065, China;
26.Key Laboratory of Cosmic Rays (Tibet University, Ministry of Education, Tibet, Lhasa, 850000, China;
27.School of Physics and Technology, Wuhan University, Hubei, Wuhan, 430072, China;
28.School of Physics and Astronomy, Yunnan University, Yunnan, Kunming, 650091, China;
29.Yunnan Observatories, Chinese Academy of Sciences, Yunnan, Kunming, 650216, China;
30.Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2 Dublin, Ireland;
31.Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg, 69029, Germany;
32.Dipartimento di Fisica dell’Università di Napoli
33.Institute for Nuclear Research of Russian Academy of Sciences, Moscow, 117312, Russia;
34.Moscow Institute of Physics and Technology, Moscow, 141700, Russia;
35.Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université deGenève, 24 Quai Ernest Ansermet, Geneva, 1211, Switzerland;
36.Department of Physics, Faculty of Science, Mahidol University, Bangkok, 10400, Thailand
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Zha, Min,Gao, Chuandong,Hu, Shicong,et al. Data analysis and key science results of LHAASO-WCDA[C]:Sissa Medialab Srl,2022.
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