S
S. W. Cui
Researcher at Hebei Normal University
Publications - 140
Citations - 3224
S. W. Cui is an academic researcher from Hebei Normal University. The author has contributed to research in topics: Cosmic ray & Air shower. The author has an hindex of 32, co-authored 128 publications receiving 2514 citations.
Papers
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Journal ArticleDOI
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.
Journal ArticleDOI
Knee of the cosmic hydrogen and helium spectrum below 1 PeV measured by ARGO-YBJ and a Cherenkov telescope of LHAASO
B. Bartoli,P. Bernardini,X. J. Bi,Zihuang Cao,S. Catalanotti,S. Z. Chen,T. L. Chen,S. W. Cui,B. Z. Dai,A. D'Amone,Null Danzengluobu,I. De Mitri,B. D'Ettorre Piazzoli,T. Di Girolamo,G. Di Sciascio,C. F. Feng,Zhaoyang Feng,Zhenyong Feng,Q. b. Guo,Y. Q. Guo,H. H. He,Haibing Hu,Hongbo Hu,M. Iacovacci,R. Iuppa,H. Y. Jia,Null Labaciren,H. J. Li,C. Liu,J. Liu,M. Y. Liu,Hong-peng Lu,L. L. Ma,X. H. Ma,Giovanni Mancarella,S. M. Mari,G. Marsella,S. Mastroianni,Paolo Montini,Chang-Chun Ning,L. Perrone,P. Pistilli,P. Salvini,R. Santonico,P. R. Shen,X. D. Sheng,Fudong Shi,A. Surdo,Y. H. Tan,P. Vallania,S. Vernetto,Carlo Vigorito,Huaguang Wang,C. Y. Wu,H. R. Wu,L. Xue,Q. Y. Yang,X. C. Yang,Z. G. Yao,A. F. Yuan,M. Zha,H. M. Zhang,L. Zhang,X. Y. Zhang,Y. Zhang,J. B. Zhao,Null Zhaxiciren,Null Zhaxisangzhu,X. X. Zhou,F. R. Zhu,Q. Q. Zhu,Bai Yibing,M. J. Chen,S. H. Feng,Bingshui Gao,M. H. Gu,C. Hou,Jinyao Liu,Xuelong Wang,Gary Guishan Xiao,B. k. Zhang,Shengxue Zhang,Bin Zhou,X. Zuo +83 more
TL;DR: In this paper, a measurement of the mixed proton and helium energy spectrum, obtained with the combined data of the ARGO-YBJ experiment and a wide field of view Cherenkov telescope, a prototype of the future LHAASO experiment, is reported.
Journal ArticleDOI
First Detection of Photons with Energy beyond 100 TeV from an Astrophysical Source.
M. Amenomori,Yongjun Bao,X. J. Bi,Donghong Chen,T. L. Chen,Wei Chen,Xu Chen,Yu-Lei Chen,S. W. Cui,L. K. Ding,J. Fang,K. Fang,Cunfeng Feng,Zhaoyang Feng,Z. Y. Feng,Qi Gao,Q. B. Gou,Yicheng Guo,H. H. He,Z. T. He,K. Hibino,N. Hotta,Haibing Hu,Hui Hu,Jian Huang,H. Y. Jia,L. L. Jiang,Hui-Ke Jin,F. Kajino,K. Kasahara,Y. Katayose,Chihiro Kato,Shigeaki Kato,K. Kawata,Masayoshi Kozai,Gui-Ming Le,Ang Li,Haifeng Li,Wei Li,Y. H. Lin,Bo Liu,C. X. Liu,J. S. Liu,Minghui Liu,Y. Q. Lou,H. Lu,X. R. Meng,H. Mitsui,Kazuoki Munakata,Y. Nakamura +49 more
TL;DR: This work reports on the highest energy photons from the Crab Nebula observed by the Tibet air shower array with the underground water-Cherenkov-type muon detector array, which is the first detection of photons with E>100 TeV from an astrophysical source.
Journal ArticleDOI
Are protons still dominant at the knee of the cosmic-ray energy spectrum?
M. Amenomori,S. Ayabe,D. Chen,S. W. Cui,Danzengluobu,L. K. Ding,X. H. Ding,Cunfeng Feng,Z. Y. Feng,X. Y. Gao,Q. X. Geng,H. W. Guo,H. H. He,M. He,K. Hibino,N. Hotta,Haibing Hu,H. B. Hu,Jing Huang,Q. Huang,H. Y. Jia,F. Kajino,Katsuaki Kasahara,Y. Katayose,Chihiro Kato,Kazumasa Kawata,Labaciren,G. M. Le,J. Y. Li,Hsiao-Chi Lu,S. L. Lu,X. R. Meng,K. Mizutani,J. Mu,Kazuoki Munakata,A. Nagai,H. Nanjo,Masaki Nishizawa,M. Ohnishi,I. Ohta,H. Onuma,T. Ouchi,Shunsuke Ozawa,Jieru Ren,Takeshi Saito,M. Sakata,T. Sasaki,M. Shibata,A. Shiomi,T. Shirai,H. Sugimoto,Masato Takita,Y. H. Tan,N. Tateyama,Shoji Torii,Harufumi Tsuchiya,S. Udo,Huaguang Wang,X. Wang,Y. G. Wang,H. R. Wu,L. Xue,Y. Yamamoto,C. T. Yan,X. C. Yang,S. Yasue,Z. H. Ye,G. C. Yu,A. F. Yuan,T. Yuda,H. M. Zhang,Jia Zhang,N. J. Zhang,Xuan Zhang,Y. Zhang,Yi Zhang,Zhaxisangzhu,X. X. Zhou +77 more
TL;DR: In this article, a hybrid experiment consisting of emulsion chambers, burst detectors and the Tibet-II air-shower array was carried out at Yangbajing (4300 m a.s.l., 606 g / cm 2 ) in Tibet to obtain the energy spectra of primary protons and heliums.
Journal ArticleDOI
First Detection of sub-PeV Diffuse Gamma Rays from the Galactic Disk: Evidence for Ubiquitous Galactic Cosmic Rays beyond PeV Energies.
M. Amenomori,Yongjun Bao,X. J. Bi,Donghong Chen,T. L. Chen,W. Y. Chen,Xu Chen,Yu-Lei Chen,Cirennima,S. W. Cui,Danzengluobu,L. K. Ding,J. Fang,K. Fang,C. F. Feng,Zhaoyang Feng,Z. Y. Feng,Qi Gao,Q. B. Gou,Y. Q. Guo,Yang Guo,H. H. He,Z. T. He,K. Hibino,N. Hotta,Haibing Hu,H. B. Hu,Jian Huang,H. Y. Jia,L. L. Jiang,H. B. Jin,Katsuaki Kasahara,Y. Katayose,Chihiro Kato,Shigeaki Kato,K. Kawata,W. Kihara,Y. Ko,Masayoshi Kozai,Labaciren,Gui-Ming Le,Ang Li,Ang Li,H. J. Li,W. J. Li,W. J. Li,Y. H. Lin,B. Liu,C. X. Liu,J. S. Liu,Minghui Liu,Wenwei Liu,Y. Q. Lou,Hong-peng Lu,X. R. Meng,Kazuoki Munakata,H. Nakada,Y. Nakamura,H. Nanjo,Masaki Nishizawa,M. Ohnishi,T. Ohura,S. Ozawa,X. L. Qian,X. B. Qu,To. Saito,M. Sakata,Takashi Sako,J. Shao,J. Shao,M. Shibata,A. Shiomi,H. Sugimoto,W. Takano,Masato Takita,Y. H. Tan,N. Tateyama,Shoji Torii,Harufumi Tsuchiya,S. Udo,Huaguang Wang,H. R. Wu,L. Xue,Y. Yamamoto,Zicai Yang,Y. Yokoe,A. F. Yuan,L. M. Zhai,H. M. Zhang,Jia Zhang,Xiang Zhang,X. Y. Zhang,Y. Zhang,Yi Zhang,Ying Zhang,Shi-Ping Zhao,Zhaxisangzhu,X. X. Zhou,mrow> γ<,mrow,msub +100 more
TL;DR: For the first time, the long-awaited detection of diffuse gamma rays with energies between 100 TeV and 1 PeV in the Galactic disk was reported in this paper, which is consistent with expectations from the hadronic emission scenario in which gamma rays originate from the decay of π 0's produced through the interaction of protons with the interstellar medium.