Z. K. Zeng
Chinese Academy of Sciences
15 Papers
63 Citations
Z. K. Zeng is an academic researcher from Chinese Academy of Sciences. The author has contributed to research in topics: Air shower & Cosmic ray. The author has an hindex of 3, co-authored 15 publications.
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Papers
Ultrahigh-energy photons up to 1.4 petaelectronvolts from 12 γ-ray Galactic sources
Zhengguo Cao,Felix Aharonian,Felix Aharonian,Q. An,Axikegu,L. X. Bai,Bai Yibing,Y. W. Bao,D. Bastieri,X. J. Bi,Y. J. Bi,H. Cai,J. T. Cai,Zhe Cao,J. F. Chang,J. F. Chang,X. C. Chang,B. M. Chen,J. Chen,L. Chen,Liang Chen,Long Chen,M. J. Chen,M. L. Chen,Q. H. Chen,S.H. Chen,S. Z. Chen,T. L. Chen,Xuliang Chen,Yi Chen,N. Cheng,Y. D. Cheng,S. W. Cui,X. H. Cui,Y. D. Cui,B. Z. Dai,H. L. Dai,Z. G. Dai,Danzengluobu,D. della Volpe,B D Ettorre Piazzoli,X. J. Dong,Jun-Hui Fan,Y. Z. Fan,Z. X. Fan,J. Fang,Kun Fang,C. F. Feng,L. Feng,S. H. Feng,Y. L. Feng,Bingshui Gao,C. D. Gao,Q. Gao,W. Gao,M. M. Ge,Li-Sheng Geng,G. H. Gong,Q. B. Gou,M. H. Gu,J. G. Guo,X. L. Guo,Y. Q. Guo,Y. Y. Guo,Y. A. Han,H. H. He,H. N. He,J. C. He,S. L. He,Xinbo He,Y. He,M. Heller,Y. K. Hor,C. Hou,Xing-Yuan Hou,H. B. Hu,S. Hu,Shi-Qi Hu,X. J. Hu,D. H. Huang,Qizhi Huang,W. H. Huang,X. T. Huang,Z. C. Huang,F. Ji,X. L. Ji,H. Y. Jia,K. Jiang,Z. J. Jiang,Chiming Jin,D.A. Kuleshov,K. Levochkin,B. B. Li,Cong Li,Cheng Li,F. Y. Li,H. B. Li,H. C. Li,Hefan Li,Hefan Li,Jixia Li,K. Li,W. L. Li,Xuejiao Li,X. R. Li,Xufang Li,Youping Li,Y. Z. Li,Zhe Li,Zhuo Li,E. W. Liang,Yun-Feng Liang,Shuibin Lin,B. Liu,C. X. Liu,Dong Liu,H. Liu,H. D. Liu,J. Liu,Jinyao Liu,Jun Liu,J. Y. Liu,Minghui Liu,R. Liu,Shujuan Liu,W. Liu,Yunchao Liu,Z. X. Liu,W. J. Long,R. Lu,H. K. Lv,Bin Ma,L. L. Ma,X. H. Ma,Junjie Mao,A. Masood,Warit Mitthumsiri,T. Montaruli,Y. C. Nan,B. Y. Pang,P. Pattarakijwanich,Z. Y. Pei,Minghao Qi,David Ruffolo,V. Rulev,Alejandro Sáiz,Lang Shao,Oleg Shchegolev,Oleg Shchegolev,X. D. Sheng,J. R. Shi,H. C. Song,Yu. V. Stenkin,Yu. V. Stenkin,V. I. Stepanov,Qie Sun,X. N. Sun,Z. B. Sun,Pak-Hin Thomas Tam,Zebo Tang,Wenwu Tian,B. D. Wang,Cunguo Wang,H. Wang,Hong-Guang Wang,J. C. Wang,J. S. Wang,L. P. Wang,L. Y. Wang,R. N. Wang,W. Wang,X. G. Wang,Xuelong Wang,Xiang-Yu Wang,Yongchun Wang,Y. J. Wang,Y. P. Wang,Zheng Wang,Zhen Wang,Z. H. Wang,Z. X. Wang,D. M. Wei,Jun-Jie Wei,Y. J. Wei,T. Wen,C. Y. Wu,H. R. Wu,S. Wu,W. X. Wu,X. F. Wu,S. Q. Xi,J.W. Xia,J.W. Xia,J. J. Xia,G. M. Xiang,G. C. Xiao,H. B. Xiao,G. G. Xin,Y. L. Xin,Y. M. Xing,Donglian Xu,Rong Xu,L. Xue,Duo Yan,C. W. Yang,Fan Yang,J. Y. Yang,Linbin Yang,M. J. Yang,Ruizhi Yang,S. B. Yang,Y. H. Yao,Z. G. Yao,Y. M. Ye,L. Q. Yin,N. Yin,X. H. You,Z. Y. You,Y. H. Yu,Q. Yuan,Houdun Zeng,Tao Zeng,W. Zeng,Z. K. Zeng,M. Zha,X. X. Zhai,Bo Zhang,H. M. Zhang,He Zhang,Jie Zhang,J. W. Zhang,Lu Zhang,Li Zhang,L. X. Zhang,P. F. Zhang,P. P. Zhang,Rui Zhang,Rui Zhang,S. R. Zhang,Shengxue Zhang,Xiang Zhang,Xiaofei Zhang,Yong Zhang,Yi Zhang,Ying Zhang,Yugang Zhang,Binyu Zhao,J. B. Zhao,Lei Zhao,L. Z. Zhao,S. P. Zhao,S. P. Zhao,F. Zheng,Y. Zheng,Bin Zhou,Hao Zhou,Jianeng Zhou,Ping Zhou,R. Zhou,X. X. Zhou,Cheng Guang Zhu,F. R. Zhu,H. Zhu,K. J. Zhu,X. Zuo +264 more
TL;DR: In this article, the authors reported the detection of more than 530 photons at energies above 100 teraelectronvolts and up to 1.4 PeV from 12 sources in the Galaxy.
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The observation of the Crab Nebula with LHAASO-KM2A for the performance study
Felix Aharonian,Q. An,Axikegu,L. X. Bai,Bai Yibing,Y. W. Bao,D. Bastieri,X. J. Bi,Y. J. Bi,H. Cai,J. T. Cai,Zihuang Cao,J. F. Chang,J. F. Chang,X. C. Chang,B. M. Chen,J. Chen,L. Chen,M. J. Chen,M. L. Chen,Q. H. Chen,S.H. Chen,S. Z. Chen,T. L. Chen,Xuliang Chen,Y. B. Chen,N. Cheng,Y. D. Cheng,S. W. Cui,X. H. Cui,Y. D. Cui,B. Z. Dai,H. L. Dai,Z. G. Dai,Danzengluobu,D. della Volpe,B. D'Ettorre Piazzoli,X. J. Dong,Jun-Hui Fan,Y. Z. Fan,Z. X. Fan,J. Fang,Kun Fang,C. F. Feng,L. Feng,S. H. Feng,Y. L. Feng,Bingshui Gao,C. D. Gao,Q. Gao,W. Gao,M. M. Ge,Li-Sheng Geng,G. H. Gong,Q. B. Gou,M. H. Gu,J. G. Guo,X. L. Guo,Y. Q. Guo,Y. Y. Guo,Y. A. Han,H. H. He,H. N. He,J. C. He,S. L. He,Xinbo He,Y. He,M. Heller,Y. K. Hor,C. Hou,Xing-Yuan Hou,H. B. Hu,Shi-Qi Hu,S. Hu,X. J. Hu,D. H. Huang,Qizhi Huang,W. H. Huang,X. T. Huang,Z. C. Huang,F. Ji,X. L. Ji,H. Y. Jia,K. Jiang,Z. J. Jiang,Chiming Jin,D.A. Kuleshov,K. Levochkin,Bing Li,C-Q. Li,F. Li,H. B. Li,H. C. Li,Hefan Li,Jixia Li,K. Li,W. L. Li,X. X. Li,Xufang Li,Youping Li,Y. Z. Li,Z. Li,E. W. Liang,Yun-Feng Liang,Shuibin Lin,B. J. Liu,C. X. Liu,Dong Liu,H. M. Liu,H. D. Liu,J. Liu,Jinyao Liu,J. S. Liu,J. Y. Liu,Minghui Liu,R. Liu,Shujuan Liu,W. Liu,Yunchao Liu,Z. X. Liu,W. J. Long,R. Lu,H. K. Lv,Bin Ma,L. L. Ma,X. H. Ma,Junjie Mao,A. Masood,Warit Mitthumsiri,T. Montaruli,Y. C. Nan,B. Y. Pang,P. Pattarakijwanich,Z. Y. Pei,Minghao Qi,David Ruffolo,V. Rulev,Alejandro Sáiz,Lang Shao,Oleg Shchegolev,X. D. Sheng,J. R. Shi,H. C. Song,Yu. V. Stenkin,V. I. Stepanov,Qie Sun,X. N. Sun,Z. B. Sun,Pak-Hin Thomas Tam,Zebo Tang,Wenwu Tian,B. D. Wang,Cunguo Wang,Hui Wang,Haiyan Wang,J. C. Wang,J. S. Wang,L. P. Wang,L. Y. Wang,R. N. Wang,W. Wang,X. G. Wang,Xuelong Wang,Xiang-Yu Wang,Yongchun Wang,Y. J. Wang,Y. P. Wang,Zujian Wang,Z. H. Wang,Zheng Wang,D. M. Wei,Jun-Jie Wei,Y. J. Wei,T. Wen,C. Y. Wu,H. R. Wu,S. Wu,W. X. Wu,X. F. Wu,S. Q. Xi,J.W. Xia,J. J. Xia,G. M. Xiang,G. C. Xiao,H. B. Xiao,G. G. Xin,Y. L. Xin,Y. M. Xing,Da Xu,Rong Xu,L. Xue,Duo Yan,C. W. Yang,Fan Yang,J. Y. Yang,Linbin Yang,M. J. Yang,Ruizhi Yang,S. B. Yang,Yu-Hua Yao,Z. G. Yao,Y. M. Ye,L. Q. Yin,N. Yin,X. H. You,Z. Y. You,Y. H. Yu,Q. Yuan,Houdun Zeng,Tao Zeng,W. Zeng,Z. K. Zeng,M. Zha,X. X. Zhai,Bo Zhang,H. M. Zhang,Honghao Zhang,Jia Zhang,Jiawen Zhang,L. Zhang,L. Zhang,P. F. Zhang,P. P. Zhang,Rui Zhang,S. R. Zhang,Shengxue Zhang,X. Y. Zhang,Xuan Zhang,Y. Zhang,Yi Zhang,Yugang Zhang,Binyu Zhao,J. B. Zhao,Ling Zhao,Lei Zhao,S. P. Zhao,F. Zheng,Yangheng Zheng,Bin Zhou,Hao Zhou,Jianeng Zhou,Ping Zhou,R. Zhou,X. X. Zhou,Cheng Guang Zhu,F. R. Zhu,H. Zhu,K. J. Zhu,X. Zuo +248 more
TL;DR: In this paper, the authors presented the pipeline of KM2A data analysis and the first observation on the Crab Nebula, a standard candle in very high energy gamma-ray astronomy.
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Discovery of a New Gamma-Ray Source, LHAASO J0341+5258, with Emission up to 200 TeV
Zhengguo Cao,Felix Aharonian,Felix Aharonian,Q. An,Axikegu,L. X. Bai,Y. Bai,Y. W. Bao,D. Bastieri,X. J. Bi,Y. J. Bi,H. Cai,J. T. Cai,Zhe Cao,J. F. Chang,J. F. Chang,B. M. Chen,E. S. Chen,J. Chen,Liang Chen,Long Chen,M. J. Chen,M. L. Chen,Q. H. Chen,Sina Chen,S. Z. Chen,T. L. Chen,Xuliang Chen,Yi Chen,N. Cheng,Y. D. Cheng,S. W. Cui,X. H. Cui,Y. D. Cui,B. D'Ettorre Piazzoli,B. Z. Dai,H. L. Dai,Z. G. Dai,Danzengluobu,D. della Volpe,Xiang-Kun Dong,Kai-Kai Duan,Jun-Hui Fan,Y. Z. Fan,Z. X. Fan,J. Fang,Kun Fang,C. F. Feng,L. Feng,S. H. Feng,Y. L. Feng,Bingshui Gao,C. D. Gao,Long Gao,Q. Gao,W. Gao,M. M. Ge,Li-Sheng Geng,G. H. Gong,Q. B. Gou,M. H. Gu,Fulai Guo,J. G. Guo,X. L. Guo,Y. Q. Guo,Y. Y. Guo,Y. A. Han,H. H. He,H. N. He,Jiangang He,S. L. He,Xinbo He,Y. He,M. Heller,Y. K. Hor,C. Hou,H. B. Hu,S. Hu,Shi-Qi Hu,X. J. Hu,D. H. Huang,Qizhi Huang,W. H. Huang,X. T. Huang,X. Y. Huang,Z. C. Huang,F. Ji,X. L. Ji,H. Y. Jia,K. Jiang,Z. J. Jiang,Chiming Jin,T. Ke,D.A. Kuleshov,K. Levochkin,B. B. Li,Cheng Li,Cong Li,F. Y. Li,H. B. Li,H. C. Li,Hefan Li,Hefan Li,Jixia Li,K. Li,W. L. Li,Xufang Li,Xin Li,Yulong Li,Y. Z. Li,Zhe Li,Zhuo Li,E. W. Liang,Yun-Feng Liang,S. J. Lin,B. Liu,C. X. Liu,Dong Liu,H. Liu,H. D. Liu,J. Liu,Jinmei Liu,Jun Liu,J. Y. Liu,Minghui Liu,R. Liu,S. M. Liu,W. Liu,Yi Liu,Yunchao Liu,Z. X. Liu,W. J. Long,R. Lu,H. K. Lv,B. Q. Ma,L. L. Ma,X. H. Ma,Junjie Mao,A. Masood,Z. Min,Warit Mitthumsiri,T. Montaruli,Y. C. Nan,B. Y. Pang,P. Pattarakijwanich,Z. Y. Pei,Minghao Qi,Y. Q. Qi,B. Q. Qiao,Jiajun Qin,David Ruffolo,V. Rulev,Alejandro Sáiz,Lang Shao,Oleg Shchegolev,Oleg Shchegolev,X. D. Sheng,J. Y. Shi,H. C. Song,Yu. V. Stenkin,Yu. V. Stenkin,V. I. Stepanov,Y. Su,Qie Sun,X. N. Sun,Z. B. Sun,Pak-Hin Thomas Tam,Zebo Tang,Wenwu Tian,Boyang Wang,Cunguo Wang,H. Wang,Hong-Guang Wang,Jian Wang,J. S. Wang,L. P. Wang,L. Y. Wang,R. N. Wang,W. Wang,X. G. Wang,Xuelong Wang,Xiang-Yu Wang,Y. Wang,Yonggang Wang,Yuan-Hao Wang,Y. P. Wang,Zhao-Qi Wang,Z. X. Wang,Zhen Wang,Zheng Wang,D. M. Wei,Jun-Jie Wei,Y. J. Wei,T. Wen,C. Y. Wu,H. R. Wu,S. Wu,W. X. Wu,X. F. Wu,S. Q. Xi,J.W. Xia,J.W. Xia,J. J. Xia,G. M. Xiang,D. X. Xiao,G. C. Xiao,H. B. Xiao,G. G. Xin,Y. L. Xin,Y. M. Xing,Donglian Xu,Rong Xu,L. Xue,Duo Yan,Jingzhi Yan,C. W. Yang,Fan Yang,J. Y. Yang,L. L. Yang,M. J. Yang,Ruizhi Yang,S. B. Yang,Y. H. Yao,Z. G. Yao,Y. M. Ye,L. Q. Yin,N. Yin,X. H. You,Z. Y. You,Y. H. Yu,Q. Yuan,Houdun Zeng,Tao Zeng,W. Zeng,Z. K. Zeng,M. Zha,X. X. Zhai,Bo Zhang,H. M. Zhang,Hanzhong Zhang,Jia Zhang,J. W. Zhang,L. X. Zhang,Li Zhang,Lu Zhang,P. F. Zhang,P. P. Zhang,Rui Zhang,Rui Zhang,S. R. Zhang,Shengxue Zhang,Xiang Zhang,Xiao-Hu Zhang,Ying Zhang,Yugang Zhang,Yi Zhang,Yong Zhang,Binyu Zhao,J. B. Zhao,Lei Zhao,L. Z. Zhao,S. P. Zhao,S. P. Zhao,F. Zheng,Y. Zheng,Binbin Zhou,H. Zhou,Jianeng Zhou,Ping Zhou,R. Zhou,X. X. Zhou,Cheng Guang Zhu,F. R. Zhu,H. Zhu,K. J. Zhu,X. Zuo +275 more
TL;DR: In this paper, the authors reported the discovery of a new extended gamma-ray source in the Galactic plane named LHAASO J0341+5258 with a pretrial significance of 8.2 standard deviations above 25 TeV.
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Absolute calibration of LHAASO WFCTA camera based on LED
Felix Aharonian,Felix Aharonian,Q. An,Axikegu,L. X. Bai,Bai Yibing,Y. W. Bao,D. Bastieri,X. J. Bi,Y. J. Bi,H. Cai,J. T. Cai,Zhengguo Cao,Zhe Cao,J. F. Chang,J. F. Chang,B. M. Chen,E. S. Chen,J. Chen,Liang Chen,Long Chen,M. J. Chen,M. L. Chen,Q. H. Chen,Sina Chen,S. Z. Chen,T. L. Chen,Xuliang Chen,Yi Chen,N. Cheng,Y. D. Cheng,S. W. Cui,X. H. Cui,Y. D. Cui,B. Z. Dai,H. L. Dai,Z. G. Dai,Danzengluobu,D. della Volpe,B. D'Ettorre Piazzoli,X. J. Dong,Kai-Kai Duan,Jun-Hui Fan,Y. Z. Fan,Z. X. Fan,J. Fang,Kun Fang,C. F. Feng,L. Feng,S. H. Feng,Y. L. Feng,Y.T. Fu,H.Y. Gan,Bingshui Gao,C. D. Gao,Lidan Gao,Q. Gao,W. Gao,M. M. Ge,Li-Sheng Geng,G. H. Gong,Q. B. Gou,M. H. Gu,Fengqin Guo,J. G. Guo,X. L. Guo,Y. Q. Guo,Y. Y. Guo,Y. A. Han,H. H. He,H. N. He,J. C. He,S. L. He,Xinbo He,Y. He,M. Heller,Y. K. Hor,C. Hou,H. B. Hu,S. Hu,Shi-Qi Hu,X. J. Hu,D. H. Huang,Qizhi Huang,W. H. Huang,X. T. Huang,X. Y. Huang,Z. C. Huang,F. Ji,X. L. Ji,H. Y. Jia,K. Jiang,Z. J. Jiang,Chiming Jin,T. Ke,D.A. Kuleshov,K. Levochkin,B. B. Li,Cong Li,Cheng Li,F. Y. Li,H. B. Li,H. C. Li,Hefan Li,Hefan Li,Jixia Li,K. Li,W. L. Li,Xin Li,Xufang Li,Youping Li,Y. Z. Li,Zhe Li,Zhuo Li,E. W. Liang,Yun-Feng Liang,Shuibin Lin,B. Liu,C. X. Liu,Dong Liu,H. Liu,H. D. Liu,J. Liu,Jinyao Liu,Jun Liu,J. Y. Liu,Minghui Liu,R. Liu,S. M. Liu,W. Liu,Yi Liu,Yunchao Liu,Z. X. Liu,W. J. Long,R. Lu,H. K. Lv,Bin Ma,L. L. Ma,X. H. Ma,Junjie Mao,A. Masood,Z. Min,Warit Mitthumsiri,T. Montaruli,Y. C. Nan,B. Y. Pang,P. Pattarakijwanich,Z. Y. Pei,Minghao Qi,Y. Q. Qi,B. Q. Qiao,Jianguo Qin,David Ruffolo,V. Rulev,Alejandro Sáiz,Lang Shao,Oleg Shchegolev,Oleg Shchegolev,X. D. Sheng,J. Y. Shi,H. C. Song,Yu. V. Stenkin,Yu. V. Stenkin,V. I. Stepanov,Y. Su,Qie Sun,X. N. Sun,Z. B. Sun,Pak-Hin Thomas Tam,Zebo Tang,Wenwu Tian,B. D. Wang,Cunguo Wang,H. Wang,Hong-Guang Wang,Jian Wang,J. S. Wang,L. P. Wang,L. Y. Wang,R. N. Wang,W. Wang,X. G. Wang,Xuelong Wang,Xiang-Yu Wang,Y. Wang,Yongchun Wang,Y. J. Wang,Y. P. Wang,Z. H. Wang,Z. X. Wang,Zhen Wang,Zheng Wang,D. M. Wei,Jun-Jie Wei,Y. J. Wei,T. Wen,C. Y. Wu,H. R. Wu,S. Wu,W. X. Wu,X. F. Wu,S. Q. Xi,J.W. Xia,J.W. Xia,J. J. Xia,G. M. Xiang,D. X. Xiao,G. C. Xiao,H. B. Xiao,G. G. Xin,Y. L. Xin,Y. M. Xing,Donglian Xu,Rong Xu,L. Xue,Duo Yan,Jiawei Yan,C. W. Yang,Fan Yang,J. Y. Yang,Linbin Yang,M. J. Yang,Ruizhi Yang,S. B. Yang,Y. H. Yao,Z. G. Yao,Y. M. Ye,L. Q. Yin,N. Yin,X. H. You,Z. Y. You,Y. H. Yu,Q. Yuan,Houdun Zeng,Tao Zeng,W. Zeng,Z. K. Zeng,M. Zha,X. X. Zhai,Bo Zhang,H. M. Zhang,He Zhang,Jia Zhang,J. W. Zhang,Lu Zhang,Li Zhang,L. X. Zhang,P. F. Zhang,P. P. Zhang,Rui Zhang,Rui Zhang,S. R. Zhang,Shengxue Zhang,Xiang Zhang,Xiaofei Zhang,Ying Zhang,Yugang Zhang,Yong Zhang,Yi Zhang,Binyu Zhao,J. B. Zhao,Lei Zhao,L. Z. Zhao,S. P. Zhao,S. P. Zhao,F. Zheng,Y. Zheng,Bin Zhou,Hao Zhou,Jianeng Zhou,Ping Zhou,R. Zhou,X. X. Zhou,Cheng Guang Zhu,F. R. Zhu,H. Zhu,K. J. Zhu,X. Zuo +277 more
TL;DR: In this paper, a multi-wavelength cylindrical illuminator based on LEDs is developed and mounted inside the telescope to calibrate and monitor the camera, and the illuminators stability is better than 0.5% under the temperature variation from -26 to 26 ˚ C.
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Performance test of the electromagnetic particle detectors for the LHAASO experiment
Felix Aharonian,Felix Aharonian,Q. An,Axikegu,L. X. Bai,Y. Bai,Yongjun Bao,D. Bastieri,X. J. Bi,Y. J. Bi,H. Cai,J. T. Cai,Zihuang Cao,J. F. Chang,J. F. Chang,X. C. Chang,B. M. Chen,J. Chen,L. Chen,M. J. Chen,M. L. Chen,Q. H. Chen,Sina Chen,S. Z. Chen,T. L. Chen,Xuliang Chen,Yi Chen,N. Cheng,Y. D. Cheng,S. W. Cui,Xiaoling Cui,Y. D. Cui,B. Z. Dai,H. L. Dai,Z. G. Dai,Danzengluobu,D. della Volpe,B. D'Ettorre Piazzoli,Xiang-Kun Dong,J. H. Fan,Y. Z. Fan,Z. X. Fan,J. Fang,K. Fang,C. F. Feng,L. Feng,S. H. Feng,Y. L. Feng,Bingshui Gao,C. D. Gao,Q. Gao,W. Gao,M. M. Ge,Li-Sheng Geng,G. H. Gong,Q. B. Gou,M. H. Gu,J. G. Guo,X. L. Guo,Y. Q. Guo,Y. Y. Guo,Y. A. Han,H. H. He,H. N. He,Jiangang He,S. L. He,Xin-Tao He,Y. He,M. Heller,Y. K. Hor,C. Hou,Xing-Yuan Hou,H. B. Hu,S. Hu,Shi-Qi Hu,X. J. Hu,D. H. Huang,Huang Qiyan,W. H. Huang,X. T. Huang,Z. C. Huang,F. Ji,X. L. Ji,H. Y. Jia,K. Jia,K. Jiang,Z. J. Jiang,Chiming Jin,D.A. Kuleshov,K. Levochkin,B. Li,B. B. Li,Chunlong Li,F. Y. Li,Hongliang Li,H. B. Li,H. C. Li,H. Y. Li,H. Y. Li,Jixia Li,K. Li,W. L. Li,Xuejiao Li,Xufang Li,Yulong Li,Y. Z. Li,Z. Li,En-Wei Liang,Y. F. Liang,S. J. Lin,B. Liu,C. X. Liu,Dong Liu,H. Liu,H. D. Liu,J. S. Liu,Jinmei Liu,Jun Liu,J. Y. Liu,Minghui Liu,Ruo-Yu Liu,Shujuan Liu,Weihang Liu,Yunchao Liu,Z. X. Liu,W. J. Long,R. Lu,H. K. Lv,B. Q. Ma,L. L. Ma,X. H. Ma,Jirong Mao,A. Masood,Warit Mitthumsiri,T. Montaruli,Y. C. Nan,B. Y. Pang,P. Pattarakijwanich,Z. Y. Pei,Minghao Qi,David Ruffolo,V. Rulev,Alejandro Sáiz,L. Shao,Oleg Shchegolev,Oleg Shchegolev,Xiangdong Sheng,J. R. Shi,H. C. Song,Yu. V. Stenkin,Yu. V. Stenkin,V. I. Stepanov,Qie Sun,X. N. Sun,Z. B. Sun,P. H. T. Tam,Zebo Tang,Wenwu Tian,Boyang Wang,C. Wang,Hui Wang,H. G. Wang,J. C. Wang,Junping Wang,L. P. Wang,L. Y. Wang,R. N. Wang,W. H. Wang,X. G. Wang,Xuelong Wang,Xiang-Yu Wang,Yonggang Wang,Yuan-Hao Wang,Y. P. Wang,Zujian Wang,Zhao-Qi Wang,Z. X. Wang,D. M. Wei,Jun-Jie Wei,Y. J. Wei,T. Wen,C. Y. Wu,H. R. Wu,S. Wu,W. X. Wu,X. F. Wu,S. Q. Xi,J.W. Xia,J.W. Xia,J. J. Xia,G. M. Xiang,Guang-Cheng Xiao,H. B. Xiao,G. G. Xin,Y. L. Xin,Y. M. Xing,Donglian Xu,Renxin Xu,L. Xue,Duo Yan,C. W. Yang,Fan Yang,J. Y. Yang,L. L. Yang,M. J. Yang,Ruizhi Yang,S. B. Yang,Y. H. Yao,Z. G. Yao,Y. M. Ye,L. Q. Yin,N. Yin,X. H. You,Z. Y. You,Y. H. Yu,Q. Yuan,H. D. Zeng,Tao Zeng,W. Zeng,Z. K. Zeng,M. Zha,X. X. Zhai,Bo Zhang,H. M. Zhang,Hanzhong Zhang,Jie Zhang,J. W. Zhang,Lu Zhang,L. X. Zhang,P. F. Zhang,P. P. Zhang,Rui Zhang,Rui Zhang,S. R. Zhang,Shengxue Zhang,Xiang Zhang,Xiao-Hu Zhang,Y. Zhang,Ying Zhang,Yugang Zhang,Binyu Zhao,J. B. Zhao,Lei Zhao,L. Z. Zhao,S. P. Zhao,S. P. Zhao,Xiao Zhao,F. Zheng,Y. Zheng,Binbin Zhou,H. Zhou,Jin-Jian Zhou,P. Zhou,R. Zhou,X. X. Zhou,Cheng Guang Zhu,F. R. Zhu,Huachun Zhu,K. J. Zhu,Xiong Zuo +259 more
TL;DR: In this paper, the performance of more than four thousands Electromagnetic particle Detectors (EDs) is summarized with the design requirements with the time resolution of 1.6 nns, the detection efficiency of 97.8%, charge resolution for single particle of 18.5% and count rate around 480 Hz.
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