Z
Z. T. He
Researcher at Hebei Normal University
Publications - 25
Citations - 468
Z. T. He 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 9, co-authored 25 publications receiving 296 citations.
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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
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.
Journal ArticleDOI
Probe of the Solar Magnetic Field Using the “Cosmic-Ray Shadow” of the Sun
M. Amenomori,X. J. Bi,Donghong Chen,T. L. Chen,W. Y. Chen,S. W. Cui,Danzengluobu,L. K. Ding,C. F. Feng,Zhaoyang Feng,Zhenyong Feng,Q. B. Gou,Y. Q. Guo,K. Hakamada,Huihai He,Z. T. He,K. Hibino,N. Hotta,Haibing Hu,H. B. Hu,Jing Huang,H. Y. Jia,L. L. Jiang,F. Kajino,K. Kasahara,Y. Katayose,Chihiro Kato,Kazumasa Kawata,Labaciren,Gui-Ming Le,A. F. Li,A. F. Li,Haifeng Li,W. J. Li,C. X. Liu,J. S. Liu,Minghui Liu,Hsiao-Chi Lu,X. R. Meng,K. Mizutani,Kazuoki Munakata,H. Nanjo,Masaki Nishizawa,M. Ohnishi,I. Ohta,H. Onuma,Shunsuke Ozawa,X. L. Qian,X. B. Qu,Takeshi Saito,Takashi Saito,M. Sakata,T. K. Sako,J. Shao,M. Shibata,A. Shiomi,T. Shirai,H. Sugimoto,Masato Takita,Y. H. Tan,N. Tateyama,Shoji Torii,Harufumi Tsuchiya,S. Udo,Huaguang Wang,H. R. Wu,L. Xue,Y. Yamamoto,Zicai Yang,S. Yasue,A. F. Yuan,T. Yuda,L. M. Zhai,H. M. Zhang,Jia Zhang,X. Y. Zhang,Y. Zhang,Yi Zhang,Ying Zhang,Zhaxisangzhu,X. X. Zhou +80 more
TL;DR: This is the first successful attempt to evaluate the coronal magnetic field models by using the Sun's shadow observed in the TeV cosmic-ray flux, and it is found that the intensity deficit in the simulated Sun’s shadow is very sensitive to the corona magnetic field structure.
Journal ArticleDOI
Northern Sky Galactic Cosmic Ray Anisotropy between 10 and 1000 TeV with the Tibet Air Shower Array
M. Amenomori,X. J. Bi,Donghong Chen,T. L. Chen,Wei Chen,S. W. Cui,Danzengluobu,Liming Ding,C. F. Feng,Zhaoyang Feng,Zhenyong Feng,Q. B. Gou,Y. Q. Guo,H. H. He,Z. T. He,K. Hibino,N. Hotta,Haibing Hu,Hailan Hu,Jing Huang,H. Y. Jia,LuHua Jiang,F. Kajino,K. Kasahara,Y. Katayose,Chihiro Kato,Kazumasa Kawata,Masayoshi Kozai,Labaciren,Gui-Ming Le,Ang Li,Ang Li,H. J. Li,Wei Li,Wei Li,C. X. Liu,Jiren Liu,Minghui Liu,Hong-peng Lu,X. R. Meng,T. Miyazaki,K. Mizutani,K. Mizutani,Kazuoki Munakata,T. Nakajima,Yoshihiko Nakamura,H. Nanjo,Masaki Nishizawa,T. Niwa,M. Ohnishi,I. Ohta,S. Ozawa,X. L. Qian,X. L. Qian,X. B. Qu,To. Saito,Takashi Saito,M. Sakata,Takashi Sako,J. Shao,J. Shao,M. Shibata,A. Shiomi,T. Shirai,H. Sugimoto,Masato Takita,Y. H. Tan,N. Tateyama,Shoji Torii,Harufumi Tsuchiya,S. Udo,H. W. Wang,H. R. Wu,L. Xue,Y. Yamamoto,K. Yamauchi,Zicai Yang,A. F. Yuan,T. Yuda,L. M. Zhai,H. M. Zhang,Jia Zhang,X. Y. Zhang,Y. Zhang,Yi Zhang,Ying Zhang,Zhaxisangzhu,X. X. Zhou +87 more
TL;DR: In this paper, the authors report on the analysis of the 10-1000 TeV sidereal anisotropy of GCRs with the data collected by the Tibet Air Shower Array from 1995 October to 2010 February.
Journal ArticleDOI
Potential PeVatron supernova remnant G106.3+2.7 seen in the highest-energy gamma rays
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,Kun 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,K. Kasahara,Y. Katayose,Chihiro Kato,Shigeaki Kato,K. Kawata,W. Kihara,Y. Ko,Masayoshi Kozai,Labaciren,Gui-Ming Le,Ang Li,H. J. Li,W. J. Li,Y. H. Lin,B. Liu,C. X. Liu,J. S. Liu,Minghui Liu,Wenwei Liu,Y. Q. Lou,Hsiao-Chi 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,Takeshi Saito,M. Sakata,T. K. Sako,J. Shao,M. Shibata,A. Shiomi,H. Sugimoto,W. Takano,M. Takita,Y. H. Tan,N. Tateyama,S. 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,X. Y. Zhang,Xuan Zhang,Y. Zhang,Yi Zhang,Ying Zhang,Shi-Ping Zhao,Zhaxisangzhu,X. X. Zhou +94 more
TL;DR: In this article, the gamma-ray emission from the supernova remnant G106.3+2.7 above 10 teraelectronvolts (TeV) has been observed and it was shown that the very high-energy gamma ray emission above 10 TeV is well correlated with a molecular cloud rather than the pulsar PSR J2229+6114.