【作者】Aharonian, Felix A.，Alekseenko, Victor V.，AN, Qi，Axikegu，Bai, Lixin，Bao, Yiwei，Bastieri, D.，Bi, Xiaojun，Cai, Hao，Cao, Zhe，Cao, Zhen，Chang, Jin，Chang, J. F.，Chang, Xiaochuan，Chao, S. P.，Chen, B. M.，Chen, Jian，Chen, Lin，Chen, Liang，Chen, M. L.，Chen, Mingjun，Chen, Qihui，Chen, Shanhong，Chen, Songzhan，Chen, Tianlu，Chen, X. L.，Chen, Yang，Cheng, Ning，Cheng, Y. D.，Cui, Shuwang，Cui, Xiaohong，Cui, Yudong，Dai, Benzhong，Dai, H. L.，Dai, Zigao，Danzengluobu，D'Ettorre-Piazzoli, Benedetto，Fang, Jinghong，Fan, Junhui，Fan, Yizhong，Feng, Cunfeng，Feng, Li，Feng, Shaohui，Feng, Youliang，Gao, Bo，Gao, Qi，Gao, Wei，Ge, Maomao，Geng, Lisheng，Gong, Guanghua，Gou, Quanbu，Gu, Minhao，Guo, Yiqing，Guo, Yingying，Han, Y. A.，He, Huihai，He, Jiancheng，Heller, Matthieu，He, S. L.，He, Yu，Hou, Chao，Huang, Daihui，Huang, Qiulan，Huang, Wenhao，Huang, Xingtao，Hu, Hongbo，Hu, S.，Jia, Huanyu，Jiang, Kun，Ji, F.，Jin, Chao，Ji, Xiaolu，Levochkin, Kirill R.，Liang, Enwei，Liang, Yunfeng，Li, Cheng，Li, Cong，Li, Fei，Li, H. Y.，Li, Haibo，Li, Huicai，Li, Huiling，Li, Jiajun，Li, K
【作者单位】1Institute of High Energy Physics, Chinese Academy of Sciences, Beijing, 100049, China;2University of Chinese Academy of Sciences, Beijing, 100049, China;3TIANFU Cosmic Ray Research Center, Shichuan Chengdu, China;4University of Science and Technology of China, Hefei, Anhui, 230026, China;5Tsinghua University, Beijing, 100084, China;6National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China;7National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China;8School of Physics, Peking University, Beijing, 100871, China;9Center for Astrophysics, Guangzhou University, Guangzhou, Guangdong, 510006, China;10Sun Yat-sen University, Zhuhai, Guangdong, 519000, China;11Shool of Physics and Technology, Guangxi University, Nanning, Guangxi, 530004, China;12Hebei Normal University, Shijiazhuang, Hebei, 050024, China;13School of Physics and Engineering, Zhengzhou University, Zhengzhou, Henan, 450001, China;14Nanjing University, Nanjing, Jiangsu, 210023, China;15Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, Jiangsu, 210034, China;16Institute of Frontier and Interdisciplinary Science, Shandong University, Qingdao, Shandong, 266237, China;17Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China;18School of Physical Science and Technology, Southwest Jiaotong University, Chengdu, Sichuan, 610031, China;19Sichuan University, Chengdu, Sichuan, 610065, China;20Key Laboratory of Cosmic Rays, Tibet University, Ministry of Education, Lhasa, Tibet, 850000, China;21School of Physics and Technology, Wuhan University, Wuhan, 430072, China;22Yunnan University, Kunming, Yunnan, 650091, China;23Yunnan Astronomical Observatories, Chinese Academy of Sciences, Kunming, Yunnan, 650216, China;24Institute for Nuclear Research, Russian Academy of Sciences, Moscow, Russian Federation;25Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genéve, Geneva, Switzerland;26Department of Physics, Faculty of Science, Mahidol University, Bangkok, Thailand;27Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland;28Max-Planck-Institut Fijr Kernphysik, P.O. Box 103980, Heidelberg, 69029, Germany;29Dipartimento di Fisica Dell'Universit\'a di Napoli "federico II", Complesso Universitario di Monte Sant'Angelo, via Cinthia, Napoli, 80126, Italy
【年份】2020
【卷号】Vol.44 No.6
【ISSN】1674-1137
【摘要】 The Water Cherenkov Detector Array is a major component of the Large High Altitude Air Shower Array Observatory , a new generation cosmic-ray experiment with unprecedented sensitivity, currently under construction. WCDA is aimed at the study of TeV ...
