Institutional Repository System Of Yunnan Observatories, CAS
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 |
DOI | 10.22323/1.395.0860 |
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 |
推荐引用方式 GB/T 7714 | Zha, Min,Gao, Chuandong,Hu, Shicong,et al. Data analysis and key science results of LHAASO-WCDA[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 | ||
Data analysis and ke(4001KB) | 会议论文 | 开放获取 | CC BY-NC-SA | 浏览 请求全文 |
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。
修改评论