胡海冰_西藏大学机构知识库

检索banner

胡海冰

职称：讲师
研究方向：物理学
学科领域：物理学，无线电电子学、电信技术，教育，天文学，信息与知识传播
所属二级机构：理学院
成果数量：139条 ,属于理学院数量为:22条

检索结果：返回 139 结果。

排序：

期刊

Research on the knee region of cosmic ray by using a novel type of electron–neutron detector array 统计源期刊(中信所)

作者： Bing-Bing Li，Xin-Hua Ma，Shu-Wang Cui，Hao-Kun Chen，Tian-Lu Chen，Danzengluobu，Wei Gao，Hai-Bing Hu，Denis Kuleshov，Kirill Kurinov，Hu Liu，Mao-Yuan Liu，Ye Liu，Da-Yu Peng，Yao-Hui Qi，Oleg Shchegolev，Yuri Stenkin，Li-Qiao Yin，Heng-Yu Zhang，Liang-Wei Zhang （ ¹College of Physics, Hebei Normal University, 050024, Shijiazhuang, China;²Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, 100049, Beijing, China;³TIANFU Cosmic Ray Research Center, 610000, Chengdu, China;⁴College of Science, Tibet University, 850000, Lhasa, China;⁵Key Laboratory of Comic Rays, Ministry of Education, Tibet University, 850000, Lhasa, China;⁶Institute for Nuclear Research of the Russian Academy of Sciences, 117312, Moscow, Russia;⁷School of Physical Science and Technology, Southwest Jiaotong University, 610031, Chengdu, China;⁸School of Management Science and Engineering, Hebei University of Economics and Business, 050061, Shijiazhuang, China;⁹Moscow Institute of Physics and Technology, 141700, Moscow, Russia ）
出处： Frontiers of Physics 2024 Vol.19 No.4
关键词： cosmic ray EAS knee region LHAASO ENDA
摘要： By accurately measuring composition and energy spectrum of cosmic ray, the origin problem of so called “knee” region can be solved. However, up to th

期刊

Stringent Tests of Lorentz Invariance Violation from LHAASO Observations of GRB 221009A EI工程索引(美)

作者： Cao, Zhen， Aharonian, F.， Axikegu， Bai, Y.X.， Bao, Y.W.， Bastieri, D.， Bi, X.J.， Bi, Y.J.， Bian, W.， Bukevich, A.V.， Cao, Q.， Cao, W.Y.， Cao, Zhe， Chang, J.， Chang, J.F.， Chen, A.M.， Chen, E.S.， Chen, H.X.， Chen, Liang， Chen, Lin， Chen, Long， Chen, M.J.， Chen, M.L.， Chen, Q.H.， Chen, S.， Chen, S.H.， Chen, S.Z.， Chen, T.L.， Chen, Y.， Cheng, N.， Cheng, Y.D.， Cui, M.Y.， Cui, S.W.， Cui, X.H.， Cui, Y.D.， Dai, B.Z.， Dai, H.L.， Dai, Z.G.， Danzengluobu， Dong, X.Q.， Duan, K.K.， Fan, J.H.， Fan, Y.Z.， Fang, J.， Fang, J.H.， Fang, K.， Feng, C.F.， Feng, H.， Feng, L.， Feng, S.H.， Feng, X.T.， Feng, Y.， Feng, Y.L.， Gabici, S.， Gao, B.， Gao, C.D.， Gao, Q.， Gao, W.， Gao, W.K.， Ge, M.M.， Geng, L.S.， Giacinti, G.， Gong, G.H.， Gou, Q.B.， Gu, M.H.， Guo, F.L.， Guo, X.L.， Guo, Y.Q.， Guo, Y.Y.， Han, Y.A.， Hasan, M.， He, H.H.， He, H.N.， He, J.Y.， He, Y.， Hor, Y.K.， Hou, B.W.， Hou, C.， Hou, X.， Hu, H.B.， Hu, Q.， Hu, S.C.， Huang, D.H.， Huang, T.Q.， Huang, W.J.， Huang, X.T.， Huang, X.Y.， Huang, Y.， Ji, X.L.， Jia, H.Y.， Jia, K.， Jiang, K.， Jiang, X.W.， Jiang, Z.J.， Jin, M.， Kang, M.M.， Karpikov, I.， Kuleshov, D.， Kurinov, K.， Li, B.B.， Li, C.M.， Li, Cheng， Li, Cong， Li, D.， Li, F.， Li, H.B.， Li, H.C.， Li, Jian， Li, Jie， Li, K.， Li, S.D.， Li, W.L.， Li, W.L.， Li, X.R.， Li, Xin， Li, Y.Z.， Li, Zhe， Li, Zhuo， Liang, E.W.， Liang, Y.F.， Lin, S.J.， Liu, B.， Liu, C.， Liu, D.， Liu, D.B.， Liu, H.， Liu, H.D.， Liu, J.， Liu, J.L.， Liu, M.Y.， Liu, R.Y.， Liu, S.M.， Liu, W.， Liu, Y.， Liu, Y.N.， Luo, Q.， Luo, Y.， Lv, H.K.， Ma, B.Q.， Ma, L.L.， Ma, X.H.， Mao, J.R.， Min, Z.， Mitthumsiri, W.， Mu, H.J.， Nan, Y.C.， Neronov, A.， Ou, L.J.， Pattarakijwanich, P.， Pei, Z.Y.， Qi, J.C.， Qi, M.Y.， Qiao, B.Q.， Qin, J.J.， Raza, A.， Ruffolo, D.， Sáiz, A.， Saeed, M.， Semikoz, D.， Shao, L.， Shchegolev, O.， Sheng, X.D.， Shu, F.W.， Song, H.C.， Stenkin, Yu.V.， Stepanov, V.， Su, Y.， Sun, D.X.， Sun, Q.N.， Sun, X.N.， Sun, Z.B.， Takata, J.， Tam, P.H.T. （ ¹Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute 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, Sichuan, Chengdu; 610000, China;⁴Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2, Dublin, Ireland;⁵Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg; 69029, Germany;⁶School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Sichuan, Chengdu; 610031, China;⁷School of Astronomy and Space Science, Nanjing University, Jiangsu, Nanjing; 210023, China;⁸Center for Astrophysics, Guangzhou University, Guangdong, Guangzhou; 510006, China;⁹Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai; 200240, China;¹⁰Institute for Nuclear Research, Russian Academy of Sciences, Moscow; 117312, Russia;¹¹Hebei Normal University, Hebei, Shijiazhuang; 050024, China;¹²University of Science and Technology of China, Anhui, Hefei; 230026, China;¹³State Key Laboratory of Particle Detection and Electronics, China;¹⁴Key Laboratory of Dark Matter and Space Astronomy, Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing; 210023, China;¹⁵Research Center for Astronomical Computing, Zhejiang Laboratory, Zhejiang, Hangzhou; 311121, China;¹⁶Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai; 200030, China;¹⁷School of Physics and Astronomy, Yunnan University, Yunnan, Kunming; 650091, China;¹⁸Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Tibet, Lhasa; 850000, China;¹⁹National Astronomical Observatories, Chinese Academy of Sciences, Beijing; 100101, China;²⁰School of Physics and Astronomy (Zhuhai), School of Physics (Guangzhou), Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, Zhuhai; 519000, China;²¹School of Physics and Astronomy (Zhuhai), School of Physics (Guangzhou), Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, Guangdong, Guangzhou; 510275, China;²²Institute of Frontier and Interdisciplinary Science, Shandong University, Shandong, Qingdao; 266237, China;²³APC, Université Paris Cité, CNRS, IN2P3, CEA, IRFU, Observatoire de Paris, 119, Paris; 75205, France;²⁴Department of Engineering Physics, Tsinghua University, Beijing; 100084, China;²⁵School of Physics and Microelectronics, Zhengzhou University, Henan, Zhengzhou; 450001, China;²⁶Yunnan Observatories, Chinese Academy of Sciences, Yunnan, Kunming; 650216, China;²⁷China Center of Advanced Science and Technology, Beijing; 100190, China;²⁸College of Physics, Sichuan University, Sichuan, Chengdu; 610065, China;²⁹School of Physics, Peking University, Beijing; 100871, China;³⁰Guangxi Key Laboratory for Relativistic Astrophysics, School of Physical Science and Technology, Guangxi University, Guangxi, Nanning; 530004, China;³¹Department of Physics, Faculty of Science, Mahidol University, Bangkok; 10400, Thailand;³²Moscow Institute of Physics and Technology, Moscow; 141700, Russia;³³Center for Relativistic Astrophysics and High Energy Physics, School of Physics and Materials Science, Institute of Space Science and Technology, Nanchang University, Jiangxi, Nanchang; 330031, China;³⁴National Space Science Center, Chinese Academy of Sciences, Beijing; 100190, China;³⁵School of Physics, Huazhong University of Science and Technology, Hubei, Wuhan; 430074, China ）
出处： arXiv 2024
摘要： Very recently, the Large High Altitude Air Shower Observatory reported the observation of the very early TeV afterglow of the brightest-of-all-time G

期刊

Modeling of TeV Galactic Cosmic-ray Anisotropy based on Intensity Mapping in an MHD Model Heliosphere EI工程索引(美)

作者： M. Amenomori，Y. W. Bao，X. J. Bi，D. Chen，T. L. Chen，W. Y. Chen，Xu Chen，Y. Chen，Cirennima，S. W. Cui，Danzengluobu，L. K. Ding，J. H. Fang，K. Fang，C. F. Feng，Zhaoyang Feng，Z. Y. Feng，Qi Gao，Q. B. Gou，Y. Q. Guo，Y. Y. Guo，Y. Hayashi，H. H. He，Z. T. He，K. Hibino，N. Hotta，Haibing Hu，H. B. Hu，K. Y. Hu，J. Huang，H. Y. Jia，L. Jiang，P. Jiang，H. B. Jin，K. Kasahara，Y. Katayose，C. Kato，S. Kato，I. Kawahara，T. Kawashima，K. Kawata，M. Kozai，Labaciren，G. M. Le，A. F. Li，H. J. Li，W. J. Li，Y. Li，Y. H. Lin，B. Liu，C. Liu，J. S. Liu，L. Y. Liu，M. Y. Liu，W. Liu，H. Lu，T. Makishima，Y. Masuda，S. Matsuhashi，M. Matsumoto，X. R. Meng，Y. Meng，A. Mizuno，K. Munakata，Y. Nakamura，H. Nanjo，C. C. Ning，M. Nishizawa，R. Noguchi，M. Ohnishi，S. Okukawa，S. Ozawa，X. Qian，X. L. Qian，X. B. Qu，T. Saito，M. Sakata，T. Sako，T. K. Sako，T. Sasaki，J. Shao，T. Shibasaki，M. Shibata，A. Shiomi，H. Sugimoto，W. Takano，M. Takita，Y. H. Tan，N. Tateyama，S. Torii，H. Tsuchiya，S. Udo，R. Usui，H. Wang，S. F. Wang，Y. P. Wang，Wangdui，H. R. Wu，Q. Wu，J. L. Xu，L. Xue，Z. Yang，Y. Q. Yao，J. Yin，Y. Yokoe，Y. L. Yu，A. F. Yuan，L. M. Zhai，H. M. Zhang，J. L. Zhang，X. Zhang，X. Y. Zhang，Y. Zhang，Yi Zhang，Ying Zhang，S. P. Zhao，Zhaxisangzhu，X. X. Zhou，Y. H. Zou，N. V. Pogorelov （ ¹Department of Physics, Hirosaki University, Hirosaki 036-8561, Japan.;²School of Astronomy and Space Science, Nanjing University, Nanjing 210093, China.;³Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China.;⁴National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China.;⁵Department of Mathematics and Physics, Tibet University, Lhasa 850000, China.;⁶Department of Physics, Hebei Normal University, Shijiazhuang 050016, China.;⁷University of Chinese Academy of Sciences, Beijing 100049, China.;⁸Institute of Frontier and Interdisciplinary Science and Key Laboratory of Particle Physics and Particle Irradiation (MOE), Shandong University, Qingdao 266237, China.;⁹Institute of Modern Physics, SouthWest Jiaotong University, Chengdu 610031, China.;¹⁰Department of Physics, Shinshu University, Matsumoto 390-8621, Japan.;¹¹Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan.;¹²Faculty of Education, Utsunomiya University, Utsunomiya 321-8505, Japan.;¹³Faculty of Systems Engineering, Shibaura Institute of Technology, Omiya 330-8570, Japan.;¹⁴Faculty of Engineering, Yokohama National University, Yokohama 240-8501, Japan.;¹⁵Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan.;¹⁶Polar Environment Data Science Center, Joint Support-Center for Data Science Research, Research Organization of Information and Systems, Tachikawa 190-0014, Japan.;¹⁷National Center for Space Weather, China Meteorological Administration, Beijing 100081, China.;¹⁸School of Information Science and Engineering, Shandong Agriculture University, Taian 271018, China.;¹⁹Department of Astronomy, School of Physical Sciences, University of Science and Technology of China, Hefei 230026, China.;²⁰National Institute of Informatics, Tokyo 101-8430, Japan.;²¹National Institute of Information and Communications Technology, Tokyo 184-8795, Japan.;²²Department of Mechanical and Electrical Engineering, Shangdong Management University, Jinan 250357, China.;²³College of Science, China University of Petroleum, Qingdao 266555, China.;²⁴Tokyo Metropolitan College of Industrial Technology, Tokyo 116-8523, Japan.;²⁵Department of Physics, Konan University, Kobe 658-8501, Japan.;²⁶College of Industrial Technology, Nihon University, Narashino 275-8575, Japan.;²⁷Shonan Institute of Technology, Fujisawa 251-8511, Japan.;²⁸Research Institute for Science and Engineering, Waseda University, Tokyo 162-0044, Japan.;²⁹Japan Atomic Energy Agency, Tokai-mura 319-1195, Japan.;³⁰Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210034, China.;³¹Department of Space Science and Center for Space Plasma and Aeronomic Research, University of Alabama in Huntsville, 320 Sparkman Drive, Huntsville, AL 35899, USA. ）
出处： Journal of Physics: Conference Series 2024 Vol.2742 P012014
摘要： Cosmic rays do not arrive at the Earth uniformly. Recent experiments have consistently observed small anisotropies with amplitudes of ∼0.2% in the arr

期刊

Optimization of performance of the KM2A full array using the Crab Nebula Scopus文摘索引数据库(荷)

作者： Zhen Cao ，F. Aharonian，Q. An ，Axikegu ，Y.X. Bai ，Y.W. Bao ，D. Bastieri，X.J. Bi ，Y.J. Bi ，J.T. Cai ，Q. Cao ，W.Y. Cao ，Zhe Cao ，J. Chang ，J.F. Chang ，A.M. Chen ，E.S. Chen ，Liang Chen ，Lin Chen ，Long Chen ，M.J. Chen ，M.L. Chen ，Q.H. Chen ，S.H. Chen ，T.L. Chen ，Y. Chen ，N. Cheng ，Y.D. Cheng ，M.Y. Cui ，S.W. Cui ，X.H. Cui ，Y.D. Cui ，B.Z. Dai ，H.L. Dai ，Z.G. Dai ，Danzengluobu ，D. della Volpe，X.Q. Dong ，K.K. Duan ，J.H. Fan ，Y.Z. Fan ，J. Fang ，K. Fang ，C.F. Feng ，L. Feng ，S.H. Feng ，X.T. Feng ，Y.L. Feng ，S. Gabici，B. Gao ，C.D. Gao ，L.Q. Gao ，Q. Gao ，W. Gao ，W.K. Gao ，M.M. Ge ，L.S. Geng ，G. Giacinti，G.H. Gong ，Q.B. Gou ，M.H. Gu ，F.L. Guo ，X.L. Guo ，Y.Q. Guo ，Y.Y. Guo ，Y.A. Han ，H.H. He ，H.N. He ，J.Y. He ，X.B. He ，Y. He ，M. Heller，Y.K. Hor ，B.W. Hou ，C. Hou ，X. Hou ，H.B. Hu ，Q. Hu ，S.C. Hu ，D.H. Huang ，T.Q. Huang ，W.J. Huang ，X.T. Huang ，X.Y. Huang ，Y. Huang ，Z.C. Huang ，X.L. Ji ，H.Y. Jia ，K. Jia ，K. Jiang ，X.W. Jiang ，Z.J. Jiang ，M. Jin ，M.M. Kang ，T. Ke ，D. Kuleshov，K. Kurinov，B.B. Li ，Cheng Li ，Cong Li ，D. Li ，F. Li ，H.B. Li ，H.C. Li ，H.Y. Li ，J. Li ，Jian Li ，Jie Li ，K. Li ，W.L. Li ，W.L. Li ，X.R. Li ，Xin Li ，Y.Z. Li ，Zhe Li ，Zhuo Li ，E.W. Liang ，Y.F. Liang ，S.J. Lin ，B. Liu ，C. Liu ，D. Liu ，H. Liu ，H.D. Liu ，J. Liu ，J.L. Liu ，J.Y. Liu ，M.Y. Liu ，R.Y. Liu ，S.M. Liu ，W. Liu ，Y. Liu ，Y.N. Liu ，R. Lu ，Q. Luo ，H.K. Lv ，B.Q. Ma ，L.L. Ma ，X.H. Ma ，J.R. Mao ，Z. Min ，W. Mitthumsiri，H.J. Mu ，Y.C. Nan ，A. Neronov，Z.W. Ou ，B.Y. Pang ，P. Pattarakijwanich，Z.Y. Pei ，M.Y. Qi ，Y.Q. Qi ，B.Q. Qiao ，J.J. Qin ，D. Ruffolo，A. Sáiz，D. Semikoz，C.Y. Shao ，L. Shao ，O. Shchegolev，X.D. Sheng ，F.W. Shu ，H.C. Song ，Yu.V. Stenkin，V. Stepanov，Y. Su ，Q.N. Sun ，X.N. Sun ，Z.B. Sun ，P.H.T. Tam ，Q.W. Tang ，Z.B. Tang ，W.W. Tian ，C. Wang ，C.B. Wang ，G.W. Wang ，H.G. Wang ，H.H. Wang ，J.C. Wang ，K. Wang ，L.P. Wang ，L.Y. Wang ，P.H. Wang ，R. Wang ，W. Wang ，X.G. Wang ，X.Y. Wang ，Y. Wang ，Y.D. Wang ，Y.J. Wang ，Z.H. Wang ，Z.X. Wang ，Zhen Wang ，Zheng Wang ，D.M. Wei ，J.J. Wei ，Y.J. Wei ，T. Wen ，C.Y. Wu ，H.R. Wu ，S. Wu ，X.F. Wu ，Y.S. Wu ，S.Q. Xi ，J. Xia ，J.J. Xia ，G.M. Xiang ，D.X. Xiao ，G. Xiao ，G.G. Xin ，Y.L. Xin ，Y. Xing ，Z. Xiong ，D.L. Xu ，R.F. Xu ，R.X. Xu ，W.L. Xu ，L. Xue ，D.H. Yan ，J.Z. Yan ，T. Yan ，C.W. Yang ，F. Yang ，F.F. Yang ，H.W. Yang ，J.Y. Yang ，L.L. Yang ，M.J. Yang ，R.Z. 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. Yue ，H.D. Zeng ，T.X. Zeng ，W. Zeng ，M. Zha ，B.B. Zhang ，F. Zhang ，H.M. Zhang ，H.Y. Zhang ，J.L. Zhang ，L.X. Zhang ，Li Zhang ，P.F. Zhang ，P.P. Zhang ，R. Zhang ，S.B. Zhang ，S.R. Zhang ，S.S. Zhang ，X. Zhang ，X.P. Zhang ，Y.F. Zhang ，Yi Zhang ，Yong Zhang ，B. Zhao ，J. Zhao ，L. Zhao ，L.Z. Zhao ，S.P. Zhao ，F. Zheng ，B. Zhou ，H. Zhou ，J.N. Zhou ，M. Zhou ，P. Zhou ，R. Zhou ，X.X. Zhou ，C.G. Zhu ，F.R. Zhu ，H. Zhu ，K.J. Zhu ，X. Zuo ，（ ¹Key Laboratory of Particle Astrophyics &Experimental Physics Division &Computing Center, Institute 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, Chengdu 610000, China;⁴Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2 Dublin, Ireland;⁵Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, 69029 Heidelberg, Germany;⁶State Key Laboratory of Particle Detection and Electronics, China;⁷University of Science and Technology of China, Hefei 230026, China;⁸School of Physical Science and Technology &School of Information Science and Technology, Southwest Jiaotong University, Chengdu 610031, China;⁹School of Astronomy and Space Science, Nanjing University, Nanjing 210023, China;¹⁰Center for Astrophysics, Guangzhou University, Guangzhou 510006, China;¹¹Hebei Normal University, Shijiazhuang 050024, China;¹²Key Laboratory of Dark Matter and Space Astronomy &Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023, China;¹³Tsung-Dao Lee Institute &School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China;¹⁴Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China;¹⁵Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Lhasa 850000, Tibet, China;¹⁶National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;¹⁷School of Physics and Astronomy (Zhuhai) &School of Physics (Guangzhou) &Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, Zhuhai 519000 &Guangzhou 510275, China;¹⁸School of Physics and Astronomy, Yunnan University, Kunming 650091, China;¹⁹Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, 1211 Geneva, Switzerland;²⁰Institute of Frontier and Interdisciplinary Science, Shandong University, Qingdao 266237, China;²¹APC, Universit'e Paris Cit'e, CNRS/IN2P3, CEA/IRFU, Observatoire de Paris, 119 75205 Paris, France;²²Department of Engineering Physics, Tsinghua University, Beijing 100084, China;²³School of Physics and Microelectronics, Zhengzhou University, Zhengzhou 450001, China;²⁴Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, China;²⁵College of Physics, Sichuan University, Chengdu 610065, China;²⁶Institute for Nuclear Research of Russian Academy of Sciences, Moscow 117312, Russia;²⁷Moscow Institute of Physics and Technology, Moscow 141700, Russia;²⁸School of Physics, Peking University, Beijing 100871, China;²⁹School of Physical Science and Technology, Guangxi University, Nanning 530004, China;³⁰Department of Physics, Faculty of Science, Mahidol University, Bangkok 10400, Thailand;³¹Center for Relativistic Astrophysics and High Energy Physics, School of Physics and Materials Science &Institute of Space Science and Technology, Nanchang University, Nanchang 330031, China;³²National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China ）
出处： Chinese Physics C 2024 Vol.48 No.6 P065001
摘要： The full array of the Large High Altitude Air Shower Observatory has been in operation since July 2021. For its kilometer-square array , we optimized

期刊

Measurement of ultra-high-energy diffuse gamma-ray emission of the Galactic plane from 10 TeV to 1 PeV with LHAASO-KM2A

作者： Cao, Zhen， Aharonian, F.， An, Q.， Axikegu， Bai, Y.X.， Bao, Y.W.， Bastieri, D.， Bi, X.J.， Bi, Y.J.， Cai, J.T.， Cao, Q.， Cao, W.Y.， Cao, Zhe， Chang, J.， Chang, J.F.， Chen, A.M.， Chen, E.S.， Chen, Liang， Chen, Lin， Chen, Long， Chen, M.J.， M.L., Chen， Q.H., Chen， S.H., Chen， S.Z., Chen， T.L., Chen， Y., Chen， N., Cheng， Y.D., Cheng， M.Y., Cui， S.W., Cui， X.H., Cui， Y.D., Cui， B.Z., Dai， H.L., Dai， Z.G., Dai， 15， D., della Volpe， X.Q., Dong， K.K., Duan， J.H., Fan， Y.Z., Fan， J., Fang， K., Fang， C.F., Feng， L., Feng， S.H., Feng， X.T., Feng， Y.L., Feng， S., Gabici， B., Gao， C.D., Gao， L.Q., Gao， Q., Gao， W., Gao， W.K., Gao， M.M., Ge， L.S., Geng， G., Giacinti， G.H., Gong， Q.B., Gou， M.H., Gu， F.L., Guo， X.L., Guo， Y.Q., Guo， Y.Y., Guo， Y.A., Han， H.H., He， H.N., He， J.Y., He， X.B., He， Y., He， M., Heller， Y.K., Hor， B.W., Hou， C., Hou， X., Hou， H.B., Hu， Q., Hu， S.C., Hu， D.H., Huang， T.Q., Huang， W.J., Huang， X.T., Huang， X.Y., Huang， Y., Huang， Z.C., Huang， X.L., Ji， H.Y., Jia， K., Jia， K., Jiang， X.W., Jiang， Z.J., Jiang， M., Jin， M.M., Kang， T., Ke， D., Kuleshov， K., Kurinov， B.B., Li， C., Li， C., Li， D., Li， F., Li， H.B., Li， H.C., Li， H.Y., Li， J., Li， J., Li， J., Li， K., Li， W.L., Li， W.L., Li， X.R., Li， X., Li， Y.Z., Li， Z., Li， Z., Li， E.W., Liang， Y.F., Liang， S.J., Lin， B., Liu， C., Liu， D., Liu， H., Liu， H.D., Liu， J., Liu， J.L., Liu， J.Y., Liu， M.Y., Liu， R.Y., Liu， S.M., Liu， W., Liu， Y., Liu， Y.N., Liu， R., Lu， Q., Luo， H.K., Lv， B.Q., Ma， L.L., Ma， X.H., Ma， J.R., Mao， Z., Min， W., Mitthumsiri， H.J., Mu， Y.C., Nan， A., Neronov， Z.W., Ou， B.Y., Pang， P., Pattarakijwanich， Z.Y., Pei， M.Y., Qi， Y.Q., Qi， B.Q., Qiao， J.J., Qin， D., Ruffolo， A., Sáiz， D., Semikoz， C.Y., Shao， L., Shao， O., Shchegolev， X.D., Sheng， F.W., Shu， H.C., Song， Y.V., Stenkin， V., Stepanov， Y., Su， Q.N., Sun， X.N., Sun， Z.B., Sun， P.H.T., Tam （ ¹Key Laboratory of Particle Astrophyics & Experimental Physics Division & Computing Center, Institute 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, Sichuan, Chengdu; 610000, China;⁴Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland;⁵Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg; 69029, Germany;⁶State Key Laboratory of Particle Detection and Electronics, China;⁷University of Science and Technology of China, Anhui, Hefei; 230026, China;⁸School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Sichuan, Chengdu; 610031, China;⁹School of Astronomy and Space Science, Nanjing University, Jiangsu, Nanjing; 210023, China;¹⁰Center for Astrophysics, Guangzhou University, Guangdong, Guangzhou; 510006, China;¹¹Hebei Normal University, Hebei, Shijiazhuang; 050024, China;¹²Key Laboratory of Dark Matter and Space Astronomy, Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Jiangsu, Nanjing; 210023, China;¹³Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai; 200240, China;¹⁴Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai; 200030, China;¹⁵Key Laboratory of Cosmic Rays (Tibet University, Ministry of Education, Tibet, Lhasa; 850000, China;¹⁶National Astronomical Observatories, Chinese Academy of Sciences, Beijing; 100101, China;¹⁷School of Physics and Astronomy (Zhuhai), School of Physics (Guangzhou), Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, Guangdong, Guangzhou; 510275, China;¹⁸School of Physics and Astronomy, Yunnan University, Yunnan, Kunming; 650091, China;¹⁹Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, Geneva; 1211, Switzerland;²⁰Institute of Frontier and Interdisciplinary Science, Shandong University, Shandong, Qingdao; 266237, China;²¹APC, Universite Paris Cite, CNRS, IN2P3, CEA/IRFU, Observatoire de Paris, Paris; 119 75205, France;²²Department of Engineering Physics, Tsinghua University, Beijing; 100084, China;²³School of Physics and Microelectronics, Zhengzhou University, Henan, Zhengzhou; 450001, China;²⁴Yunnan Observatories, Chinese Academy of Sciences, Yunnan, Kunming; 650216, China;²⁵College of Physics, Sichuan University, Sichuan, Chengdu; 610065, China;²⁶Institute for Nuclear Research of Russian Academy of Sciences, Moscow; 117312, Russia;²⁷Moscow Institute of Physics and Technology, Moscow; 141700, Russia;²⁸School of Physics, Peking University, Beijing; 100871, China;²⁹School of Physical Science and Technology, Guangxi University, Guangxi, Nanning; 530004, China;³⁰Department of Physics, Faculty of Science, Mahidol University, Bangkok; 10400, Thailand;³¹Center for Relativistic Astrophysics and High Energy Physics, School of Physics and Materials Science, Institute of Space Science and Technology, Nanchang University, Jiangxi, Nanchang; 330031, China;³²National Space Science Center, Chinese Academy of Sciences, Beijing; 100190, China ）
出处： arXiv 2023
摘要： The diffuse Galactic γ-ray emission, mainly produced via interactions between cosmic rays and the diffuse interstellar medium, is a very important pro

期刊

Flux variations of cosmic ray air showers detected by LHAASO-KM2A during a thunderstorm on June 10, 2021* * Supported in China by National Key R&D program of China , NSFC and in Thailand by RTA6280002 from Thailand Science Research and Innovation

作者： Aharonian, Felix，An, Q.，None, Axikegu，Bai, Lixin，Bai, Yunxiang，Bao, Yiwei，Bastieri, D.，Bi, X. J.，Bi, Yujiang，Cai, J. T.，Cao, Zhe，Cao, Zhen，Chang, J.，Chang, J. F.，Chen, E. S.，Chen, Liang，Chen, Lin，Chen, Minjun，Chen, M. L.，Chen, Shanhong，Chen, S. Z.，Chen, T. L.，Chen, X. J.，Chen, Yao，Cheng, H. L.，Cheng, Ning，Cheng, Y. D.，Cui, Sh W.，Cui, Xiaohong，Cui, Y. D.，Dai, B. Z.，Dai, H. L.，Dai, Z. G.，None, Danzengluobu，Volpe, Domenico Della，Duan, K. K.，Fan, J. H.，Fan, Y. Z.，Fan, Z. X.，Fang, Jinghong，Fang, K.，Feng, C. F.，Feng, L.，Feng, Shaohui，Feng, X. T.，Feng, Youliang，Gao, Bo，Gao, C. D.，Gao, L. Q.，Gao, Q.，Gao, Wei，Gao, W. K.，Ge, Maomao，Geng, L. S.，Gong, G. H.，Gou, Q. B.，Gu, Minhao，Guo, F. L.，Guo, Junguang，Guo, X. L.，Guo, Yiqin，Guo, Yingying，Han, Y. A.，He, H. H.，He, Haoning，He, S. L.，He, Xinbo，He, Yu，Heller, M.，Hor, Yuen Keung，Hou, Chao，Hou, X.，Hu, Haibing，Hu, Qingqing，Hu, S.，Hu, S. C.，Hu, X. J.，Huang, Daihui，Huang, Wenhao，Huang, X. T.，Huang, Xiaoyuan，Huang, Yan，Huang, Z. C.，Ji, X. L.，Jia, H. Y.，Jia, K.，Jiang, K.，Jiang, Zej （ ¹Key Laboratory of Particle Astrophyics, Experimental Physics Division, Computing Center, Institute 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, Sichuan, Chengdu, China;⁴Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, Dublin 2, Ireland;⁵Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg, 69029, Germany;⁶State Key Laboratory of Particle Detection and Electronics, China;⁷University of Science and Technology of China, Hefei, 230026, China;⁸School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Chengdu, 610031, China;⁹College of Physics, Sichuan University, Chengdu, 610065, China;¹⁰School of Astronomy and Space Science, Nanjing University, Nanjing, 210023, China;¹¹Center for Astrophysics, Guangzhou University, Guangzhou, 510006, China;¹²Key Laboratory of Dark Matter and Space Astronomy, Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, 210023, China;¹³Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China;¹⁴Key Laboratory of Cosmic Rays, Tibet University, Ministry of Education, Tibet, Lhasa, 850000, China;¹⁵National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China;¹⁶Hebei Normal University, Shijiazhuang, 050024, China;¹⁷School of Physics and Astronomy (Zhuhai), School of Physics (Guangzhou), Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, Zhuhai, 510275, China;¹⁸School of Physics and Astronomy, Yunnan University, Kunming, 650091, China;¹⁹D′epartement de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, Geneva, 1211, Switzerland;²⁰Institute of Frontier and Interdisciplinary Science, Shandong University, Qingdao, 266237, China;²¹Department of Engineering Physics, Tsinghua University, Beijing, 100084, China;²²School of Physics and Microelectronics, Zhengzhou University, Zhengzhou, 450001, China;²³Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, China;²⁴Institute for Nuclear Research, Russian Academy of Sciences, Moscow, 117312, Russian Federation;²⁵School of Physics, Peking University, Beijing, 100871, China;²⁶School of Physical Science and Technology, Guangxi University, Nanning, 530004, China;²⁷Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, China ）
出处： Chinese Physics C 2023 Vol.47 No.1
摘要： The Large High Altitude Air Shower Observatory has three sub-arrays, KM2A, WCDA, and WFCTA. The flux variations of cosmic ray air showers were studie

期刊

Pointing calibration of LHAASO-WFCTA telescopes using bright stars

作者： Zhen Cao，F. Aharonian，Q. An，Axikegu，Y.X. Bai，Y.W. Bao，D. Bastieri，X.J. Bi，Y.J. Bi，J.T. Cai，Q. Cao，W.Y. Cao，Zhe Cao，J. Chang，J.F. Chang，A.M. Chen，E.S. Chen，Liang Chen，Lin Chen，Long Chen，M.J. Chen，M.L. Chen，Q.H. Chen，S.H. Chen，S.Z. Chen，T.L. Chen，Y. Chen，N. Cheng，Y.D. Cheng，M.Y. Cui，S.W. Cui，X.H. Cui，Y.D. Cui，B.Z. Dai，H.L. Dai，Z.G. Dai，Danzengluobu，D. della Volpe，X.Q. Dong，K.K. Duan，J.H. Fan，Y.Z. Fan，J. Fang，K. Fang，C.F. Feng，L. Feng，S.H. Feng，X.T. Feng，Y.L. Feng，S. Gabici，B. Gao，C.D. Gao，L.Q. Gao，Q. Gao，W. Gao，W.K. Gao，M.M. Ge，L.S. Geng，G. Giacinti，G.H. Gong，Q.B. Gou，M.H. Gu，F.L. Guo，X.L. Guo，Y.Q. Guo，Y.Y. Guo，Y.A. Han，H.H. He，H.N. He，J.Y. He，X.B. He，Y. He，M. Heller，Y.K. Hor，B.W. Hou，C. Hou，X. Hou，H.B. Hu，Q. Hu，S.C. Hu，D.H. Huang，T.Q. Huang，W.J. Huang，X.T. Huang，X.Y. Huang，Y. Huang，Z.C. Huang，X.L. Ji，H.Y. Jia，K. Jia，K. Jiang，X.W. Jiang，Z.J. Jiang，M. Jin，M.M. Kang，T. Ke，D. Kuleshov，K. Kurinov，B.B. Li，Cheng Li，Cong Li，D. Li，F. Li，H.B. Li，H.C. Li，H.Y. Li，J. Li，Jian Li，Jie Li，K. Li，W.L. Li，W.L. Li，X.R. Li，Xin Li，Y.Z. Li，Zhe Li，Zhuo Li，E.W. Liang，Y.F. Liang，S.J. Lin，B. Liu，C. Liu，D. Liu，H. Liu，H.D. Liu，J. Liu，J.L. Liu，J.Y. Liu，M.Y. Liu，R.Y. Liu，S.M. Liu，W. Liu，Y. Liu，Y.N. Liu，R. Lu，Q. Luo，H.K. Lv，B.Q. Ma，L.L. Ma，X.H. Ma，J.R. Mao，Z. Min，W. Mitthumsiri，H.J. Mu，Y.C. Nan，A. Neronov，Z.W. Ou，B.Y. Pang，P. Pattarakijwanich，Z.Y. Pei，M.Y. Qi，Y.Q. Qi，B.Q. Qiao，J.J. Qin，D. Ruffolo，A. Sáiz，D. Semikoz，C.Y. Shao，L. Shao，O. Shchegolev，X.D. Sheng，F.W. Shu，H.C. Song，Yu.V. Stenkin，V. Stepanov，Y. Su，Q.N. Sun，X.N. Sun，Z.B. Sun，P.H.T. Tam，Q.W. Tang，Z.B. Tang，W.W. Tian，C. Wang，C.B. Wang，G.W. Wang，H.G. Wang，H.H. Wang，J.C. Wang，K. Wang，L.P. Wang，L.Y. Wang，P.H. Wang，R. Wang，W. Wang，X.G. Wang，X.Y. Wang，Y. Wang，Y.D. Wang，Y.J. Wang，Z.H. Wang，Z.X. Wang，Zhen Wang，Zheng Wang，D.M. Wei，J.J. Wei，Y.J. Wei，T. Wen，C.Y. Wu，H.R. Wu，S. Wu，X.F. Wu，Y.S. Wu，S.Q. Xi，J. Xia，J.J. Xia，G.M. Xiang，D.X. Xiao，G. Xiao，G.G. Xin，Y.L. Xin，Y. Xing，Z. Xiong，D.L. Xu，R.F. Xu，R.X. Xu，W.L. Xu，L. Xue，D.H. Yan，J.Z. Yan，T. Yan，C.W. Yang，F. Yang，F.F. Yang，H.W. Yang，J.Y. Yang，L.L. Yang，M.J. Yang，R.Z. 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. Yue，H.D. Zeng，T.X. Zeng，W. Zeng，M. Zha，B.B. Zhang，F. Zhang，H.M. Zhang，H.Y. Zhang，J.L. Zhang，L.X. Zhang，Li Zhang，P.F. Zhang，P.P. Zhang，R. Zhang，S.B. Zhang，S.R. Zhang，S.S. Zhang，X. Zhang，X.P. Zhang，Y.F. Zhang，Yi Zhang，Yong Zhang，B. Zhao，J. Zhao，L. Zhao，L.Z. Zhao，S.P. Zhao，F. Zheng，B. Zhou，H. Zhou，J.N. Zhou，M. Zhou，P. Zhou，R. Zhou，X.X. Zhou，C.G. Zhu，F.R. Zhu，H. Zhu，K.J. Zhu，X. Zuo，LHAASO Collaboration （ ¹Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049 Beijing, China;²University of Chinese Academy of Sciences, 100049 Beijing, China;³TIANFU Cosmic Ray Research Center, Chengdu, Sichuan, China;⁴Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2 Dublin, Ireland;⁵Max–Planck-Institute for Nuclear Physics, P.O. Box 103980, 69029 Heidelberg, Germany;⁶State Key Laboratory of Particle Detection and Electronics, China;⁷University of Science and Technology of China, 230026 Hefei, Anhui, China;⁸School of Physical Science and Technology & School of Information Science and Technology, Southwest Jiaotong University, 610031 Chengdu, Sichuan, China;⁹School of Astronomy and Space Science, Nanjing University, 210023 Nanjing, Jiangsu, China;¹⁰Center for Astrophysics, Guangzhou University, 510006 Guangzhou, Guangdong, China;¹¹Hebei Normal University, 050024 Shijiazhuang, Hebei, China;¹²Key Laboratory of Dark Matter and Space Astronomy & Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, 210023 Nanjing, Jiangsu, China;¹³Tsung-Dao Lee Institute & School of Physics and Astronomy, Shanghai Jiao Tong University, 200240 Shanghai, China;¹⁴Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 200030 Shanghai, China;¹⁵Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, 850000 Lhasa, Tibet, China;¹⁶National Astronomical Observatories, Chinese Academy of Sciences, 100101 Beijing, China;¹⁷School of Physics and Astronomy (Zhuhai) & School of Physics (Guangzhou) & Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, 519000 Zhuhai & 510275 Guangzhou, Guangdong, China;¹⁸School of Physics and Astronomy, Yunnan University, 650091 Kunming, Yunnan, China;¹⁹Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, 1211 Geneva, Switzerland;²⁰Institute of Frontier and Interdisciplinary Science, Shandong University, 266237 Qingdao, Shandong, China;²¹APC, Université Paris Cité, CNRS/IN2P3, CEA/IRFU, Observatoire de Paris, 119 75205 Paris, France;²²Department of Engineering Physics, Tsinghua University, 100084 Beijing, China;²³School of Physics and Microelectronics, Zhengzhou University, 450001 Zhengzhou, Henan, China;²⁴Yunnan Observatories, Chinese Academy of Sciences, 650216 Kunming, Yunnan, China;²⁵College of Physics, Sichuan University, 610065 Chengdu, Sichuan, China;²⁶Institute for Nuclear Research of Russian Academy of Sciences, 117312 Moscow, Russia;²⁷School of Physics, Peking University, 100871 Beijing, China;²⁸School of Physical Science and Technology, Guangxi University, 530004 Nanning, Guangxi, China;²⁹Department of Physics, Faculty of Science, Mahidol University, Bangkok 10400, Thailand;³⁰Moscow Institute of Physics and Technology, 141700 Moscow, Russia;³¹Center for Relativistic Astrophysics and High Energy Physics, School of Physics and Materials Science & Institute of Space Science and Technology, Nanchang University, 330031 Nanchang, Jiangxi, China;³²National Space Science Center, Chinese Academy of Sciences, 100190 Beijing, China ）
出处： Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 2023 Vol.1056 P168662
摘要： One of the main scientific objectives of the Large High Altitude Air Shower Observatory is to perform accurate measurements of the energy spectra for
点击量：2

期刊

A tera-electron volt afterglow from a narrow jet in an extremely bright gamma-ray burst Scopus文摘索引数据库(荷)

作者： Cao,Zhen，Aharonian,F.，An,Q.，Axikegu，Bai,L.X.，Bai,Y.X.，Bao,Y.W.，Bastieri,D.，Bi,X.J.，Bi,Y.J.，Cai,J.T.，Cao,Q.，Cao,W.Y.，Cao,Zhe，Chang,J.，Chang,J.F.，Chen,E.S.，Chen,Liang，Chen,Lin，Chen,Long，Chen,M.J.，Chen,M.L.，Chen,Q.H.，Chen,S.H.，Chen,S.Z.，Chen,T.L.，Chen,Y.，Cheng,H.L.，Cheng,N.，Cheng,Y.D.，Cui,S.W.，Cui,X.H.，Cui,Y.D.，Dai,B.Z.，Dai,H.L.，Dai,Z.G.，Danzengluobu，Della Volpe,D.，Dong,X.Q.，Duan,K.K.，Fan,J.H.，Fan,Y.Z.，Fang,J.，Fang,K.，Feng,C.F.，Feng,L.，Feng,S.H.，Feng,X.T.，Feng,Y.L.，Gao,B.，Gao,C.D.，Gao,L.Q.，Gao,Q.，Gao,W.，Gao,W.K.，Ge,M.M.，Geng,L.S.，Gong,G.H.，Gou,Q.B.，Gu,M.H.，Guo,F.L.，Guo,X.L.，Guo,Y.Q.，Guo,Y.Y.，Han,Y.A.，He,H.H.，He,H.N.，He,J.Y.，He,X.B.，He,Y.，Heller,M.，Hor,Y.K.，Hou,B.W.，Hou,C.，Hou,X.，Hu,H.B.，Hu,Q.，Hu,S.C.，Huang,D.H.，Huang,T.Q.，Huang,W.J.，Huang,X.T.，Huang,X.Y.，Huang,Y.，Huang,Z.C.，Ji,X.L.，Jia,H.Y.，Jia,K.，Jiang,K.，Jiang,X.W.，Jiang,Z.J.，Jin,M.，Kang,M.M.，Ke,T.，Kuleshov,D.，Kurinov,K.，Li,B.B.，Li,Cheng，Li,Cong，Li,D.，Li,F.，Li,H.B.，Li,H.C.，Li,H.Y.，Li,J.，Li,Jian，Li,Jie，Li,K.，Li,W.L.，Li,W.L.，Li,X.R.，Li,Xin，Li,Y.Z.，Li,Zhe，Li,Zhuo，Liang,E.W.，Liang,Y.F.，Lin,S.J.，Liu,B.，Liu,C.，Liu,D.，Liu,H.，Liu,H.D.，Liu,J.，Liu,J.L.，Liu,J.L.，Liu,J.S.，Liu,J.Y.，Liu,M.Y.，Liu,R.Y.，Liu,S.M.，Liu,W.，Liu,Y.，Liu,Y.N.，Long,W.J.，Lu,R.，Luo,Q.，Lv,H.K.，Ma,B.Q.，Ma,L.L.，Ma,X.H.，Mao,J.R.，Min,Z.，Mitthumsiri,W.，Nan,Y.C.，Ou,Z.W.，Pang,B.Y.，Pattarakijwanich,P.，Pei,Z.Y.，Qi,M.Y.，Qi,Y.Q.，Qiao,B.Q.，Qin,J.J.，Ruffolo,D.，Sáiz,A.，Shao,C.Y.，Shao,L.，Shchegolev,O.，Sheng,X.D.，Song,H.C.，Stenkin,Y.V.，Stepanov,V.，Su,Y.，Sun,Q.N.，Sun,X.N.，Sun,Z.B.，Tam,P.H.T.，Tang,Z.B.，Tian,W.W.，Wang,C.，Wang,C.B.，Wang,G.W.，Wang,H.G.，Wang,H.H.，Wang,J.C.，Wang,J.S.，Wang,K.，Wang,L.P.，Wang,L.Y.，Wang,P.H.，Wang,R.，Wang,W.，Wang,X.G.，Wang,X.Y.，Wang,Y.，Wang,Y.D.，Wang,Y.J.，Wang,Z.H.，Wang,Z.X.，Wang,Zhen，Wang,Zheng，Wei,D.M.，Wei,J.J.，Wei,Y.J.，Wen,T.，Wu,C.Y.，Wu,H.R.，Wu,S.，Wu,X.F.，Wu,Y.S.，Xi,S.Q.，Xia,J.，Xia,J.J.，Xiang,G.M.，Xiao,D.X.，Xiao,G.，Xin,G.G.，Xin,Y.L.，Xing,Y.，Xiong,Z.，Xu,D.L.，Xu,R.F.，Xu,R.X.，Xue,L.，Yan,D.H.，Yan,J.Z.，Yan,T.，Yang,C.W.，Yang,F.，Yang,F.F.，Yang,H.W.，Yang,J.Y.，Yang,L.L.，Yang,M.J.，Yang,R.Z.，Yang,S.B.，Yao,Y.H.，Yao,Z.G.，Ye,Y.M.，Yin,L.Q.，Yin,N.，You,X.H.，You,Z.Y.，Yu,Y.H.，Yuan,Q.，Yue,H.，Zeng,H.D.，Zeng,T.X.，Zeng,W.，Zeng,Z.K.，Zha,M.，Zhang,B.，Zhang,B.B.，Zhang,F.，Zhang,H.M.，Zhang,H.Y.，Zhang,J.L.，Zhang,L.X.，Zhang,L.，Zhang,P.F.，Zhang,P.P.，Zhang,R.，Zhang,S.B.，Zhang,S.R.，Zhang,S.S.，Zhang,X.，Zhang,X.P.，Zhang,Y.F.，Zhang,Y.，Zhang,Yong，Zhao,B.，Zhao,J.，Zhao,L.，Zhao,L.Z.，Zhao,S.P.，Zheng,F.，Zheng,J.H.，Zhou,B.，Zhou,H.，Zhou,J.N.，Zhou,P.，Zhou,R.，Zhou,X.X.，Zhu,C.G.，Zhu,F.R.，Zhu,H.，Zhu,K.J.，Zuo,X. （ ¹Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute of High Energy Physics, Chinese Academy of Sciences, 100049, Beijing, China;²University of Chinese Academy of Sciences, 100049, Beijing, China;³Tianfu Cosmic Ray Research Center, Chengdu, 610000, Sichuan, China;⁴Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2 Dublin, Ireland;⁵Max-Planck-Institute for Nuclear Physics, P.O. Box 103980, Heidelberg, 69029, Germany;⁶State Key Laboratory of Particle Detection and Electronics, China;⁷University of Science and Technology of China, Hefei, 230026, Anhui, China;⁸School of Physical Science and Technology & School of Information Science and Technology, Southwest Jiaotong University, Chengdu, 610031, Sichuan, China;⁹College of Physics, Sichuan University, Chengdu, 610065, Sichuan, China;¹⁰School of Astronomy and Space Science, Nanjing University, Nanjing, 210023, Jiangsu, China;¹¹Key Laboratory of Modern Astronomy and Astrophysics (Nanjing University), Ministry of Education, Nanjing, 210023, China;¹²Center for Astrophysics, Guangzhou University, Guangzhou, 510006, Guangdong, China;¹³Hebei Normal University, Shijiazhuang, 050024, Hebei, China;¹⁴Key Laboratory of Dark Matter and Space Astronomy & Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, 210023, Jiangsu, China;¹⁵Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, 200030, Shanghai, China;¹⁶Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Lhasa, 850000, Tibet, China;¹⁷National Astronomical Observatories, Chinese Academy of Sciences, 100101, Beijing, China;¹⁸School of Physics and Astronomy (Zhuhai) & School of Physics (Guangzhou) & Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, Guangdong, China;¹⁹School of Physics and Astronomy, Yunnan University, Kunming, 650091, Yunnan, China;²⁰Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, 1211, Geneva, Switzerland;²¹Institute of Frontier and Interdisciplinary Science, Shandong University, Qingdao, 266237, Shandong, China;²²Department of Engineering Physics, Tsinghua University, 100084, Beijing, China;²³School of Physics and Microelectronics, Zhengzhou University, Zhengzhou, 450001, Henan, China;²⁴Yunnan Observatories, Chinese Academy of Sciences, Kunming, 650216, Yunnan, China;²⁵Institute for Nuclear Research of Russian Academy of Sciences, 117312, Moscow, Russian Federation;²⁶Moscow Institute of Physics and Technology, 141700, Moscow, Russian Federation;²⁷Shanghai Jiao Tong University, Tsung-Dao Lee Institute & School of Physics and Astronomy, 200240, Shanghai, China;²⁸School of Physics, Peking University, 100871, Beijing, China;²⁹School of Physical Science and Technology, Guangxi University, Nanning, 530004, Guangxi, China;³⁰Department of Physics, Faculty of Science, Mahidol University, 10400, Bangkok, Thailand;³¹Chinese Academy of Sciences, National Space Science Center, 100190, Beijing, China;³²Nevada Center for Astrophysics, University of Nevada, Las Vegas, United States;³³Department of Physics and Astronomy, University of Nevada, Las Vegas, United States; ）
出处： Science (New York, N.Y.) 2023 Vol.380 No.6652 P1390-1396
摘要： Some gamma-ray bursts have a tera-electron volt afterglow, but the early onset of this has not been observed. We report observations with the Large
点击量：5

期刊

An ultrahigh-energy γ -ray bubble powered by a super PeVatron EI工程索引(美)

作者： Z. Cao，F. Aharonian，Q An，Axikegu，Y.X Bai，Y.W Bao，D Bastieri，X.J Bi，Y.J Bi，J.T Cai，Q Cao，W.Y Cao，Zhe Cao，J Chang，J.F Chang，A.M Chen，E.S Chen，Liang Chen，Lin Chen，Long Chen，M.J Chen，M.L Chen，Q.H Chen，S.H Chen，S.Z Chen，T.L Chen，Y Chen，N Cheng，Y.D Cheng，M.Y Cui，S.W Cui，X.H Cui，Y.D Cui，B.Z Dai，H.L Dai，Z.G Dai，Danzengluobu，D della Volpe，X.Q Dong，K.K Duan，J.H Fan，Y.Z Fan，J Fang，K Fang，C.F Feng，L Feng，S.H Feng，X.T Feng，Y.L Feng，S Gabici，B Gao，C.D Gao，L.Q Gao，Q Gao，W Gao，W.K Gao，M.M Ge，L.S Geng，G Giacinti，G.H Gong，Q.B Gou，M.H Gu，F.L Guo，X.L Guo，Y.Q Guo，Y.Y Guo，Y.A Han，H.H He，H.N He，J.Y He，X.B He，Y He，M Heller，Y.K Hor，B.W Hou，C Hou，X Hou，H.B Hu，Q Hu，S.C Hu，D.H Huang，T.Q Huang，W.J Huang，X.T Huang，X.Y Huang，Y Huang，Z.C Huang，X.L Ji，H.Y Jia，K Jia，K Jiang，X.W Jiang，Z.J Jiang，M Jin，M.M Kang，T Ke，D Kuleshov，K Kurinov，B.B Li，Cheng Li，Cong Li，D Li，F Li，H.B Li，H.C Li，H.Y Li，J Li，Jian Li，Jie Li，K Li，W.L Li，W.L Li，X.R Li，Xin Li，Y.Z Li，Zhe Li，Zhuo Li，E.W Liang，Y.F Liang，S.J Lin，B Liu，C Liu，D Liu，H Liu，H.D Liu，J Liu，J.L Liu，J.Y Liu，M.Y Liu，R.Y Liu，S.M Liu，W Liu，Y Liu，Y.N Liu，R Lu，Q Luo，H.K Lv，B.Q Ma，L.L Ma，X.H Ma，J.R Mao，Z Min，W Mitthumsiri，H.J Mu，Y.C Nan，A Neronov，Z.W Ou，B.Y Pang，P Pattarakijwanich，Z.Y Pei，M.Y Qi，Y.Q Qi，B.Q Qiao，J.J Qin，D Ruffolo，A Sáiz，D Semikoz，C.Y Shao，L Shao，O Shchegolev，X.D Sheng，F.W Shu，H.C Song，Yu.V Stenkin，V Stepanov，Y Su，Q.N Sun，X.N Sun，Z.B Sun，P.H.T Tam，Q.W Tang，Z.B Tang，W.W Tian，C Wang，C.B Wang，G.W Wang，H.G Wang，H.H Wang，J.C Wang，K Wang，L.P Wang，L.Y Wang，P.H Wang，R Wang，W Wang，X.G Wang，X.Y Wang，Y Wang，Y.D Wang，Y.J Wang，Z.H Wang，Z.X Wang，Zhen Wang，Zheng Wang，D.M Wei，J.J Wei，Y.J Wei，T Wen，C.Y Wu，H.R Wu，S Wu，X.F Wu，Y.S Wu，S.Q Xi，J Xia，J.J Xia，G.M Xiang，D.X Xiao，G Xiao，G.G Xin，Y.L Xin，Y Xing，Z Xiong，D.L Xu，R.F Xu，R.X Xu，W.L Xu，L Xue，D.H Yan，J.Z Yan，T Yan，C.W Yang，F Yang，F.F Yang，H.W Yang，J.Y Yang，L.L Yang，M.J Yang，R.Z 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 Yue，H.D Zeng，T.X Zeng，W Zeng，M Zha，B.B Zhang，F Zhang，H.M Zhang，H.Y Zhang，J.L Zhang，L.X Zhang，Li Zhang，P.F Zhang，P.P Zhang，R Zhang，S.B Zhang，S.R Zhang，S.S Zhang，X Zhang，X.P Zhang，Y.F Zhang，Yi Zhang，Yong Zhang，B Zhao，J Zhao，L Zhao，L.Z Zhao，S.P Zhao，F Zheng，B Zhou，H Zhou，J.N Zhou，M Zhou，P Zhou，R Zhou，X.X Zhou，C.G Zhu，F.R Zhu，H Zhu，K.J Zhu，X Zuo （ ¹Key Laboratory of Particle Astrophyics & Experimental Physics Division & Computing Center, Institute 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, Chengdu 610000, China;⁴Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2 Dublin, Ireland;⁵Max-Planck-Institut for Nuclear Physics, Heidelberg 69026, Germany;⁶State Key Laboratory of Particle Detection and Electronics, China;⁷University of Science and Technology of China, Hefei 230026, China;⁸School of Physical Science and Technology, School of Information Science and Technology, Southwest Jiaotong University, Chengdu 610031, China;⁹School of Astronomy and Space Science, Nanjing University, Nanjing 210023, China;¹⁰Center for Astrophysics, Guangzhou University, Guangzhou 510006, China;¹¹Hebei Normal University, Shijiazhuang 050024, China;¹²Key Laboratory of Dark Matter and Space Astronomy, Key Laboratory of Radio Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing 210023, China;¹³Tsung-Dao Lee Institute, School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai 200240, China;¹⁴Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai 200030, China;¹⁵Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Lhasa 850000, China;¹⁶National Astronomical Observatories, Chinese Academy of Sciences, Beijing 100101, China;¹⁷School of Physics and Astronomy (Zhuhai), School of Physics (Guangzhou) & Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, Zhuhai 519000 & Guangzhou 510275, China;¹⁸School of Physics and Astronomy, Yunnan University, Kunming 650091, China;¹⁹Département de Physique Nucléaire et Corpusculaire, Faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, 1211 Geneva, Switzerland;²⁰Institute of Frontier and Interdisciplinary Science, Shandong University, Qingdao 266237, China;²¹APC, Universit’e Paris Cit’e, CNRS/IN2P3, CEA/IRFU, Observatoire de Paris, Paris 119 75205, France;²²Department of Engineering Physics, Tsinghua University, Beijing 100084, China;²³School of Physics and Microelectronics, Zhengzhou University, Zhengzhou 450001, China;²⁴Yunnan Observatories, Chinese Academy of Sciences, Kunming 650216, China;²⁵College of Physics, Sichuan University, Chengdu 610065, China;²⁶Institute for Nuclear Research of Russian Academy of Sciences, Moscow 117312, Russia;²⁷Moscow Institute of Physics and Technology, Moscow 141700, Russia;²⁸School of Physics, Peking University, Beijing 100871 China;²⁹School of Physical Science and Technology, Guangxi University, Nanning 530004, China;³⁰Department of Physics, Faculty of Science, Mahidol University, Bangkok 10400, Thailand;³¹Center for Relativistic Astrophysics and High Energy Physics, School of Physics and Materials Science, Institute of Space Science and Technology, Nanchang University, Nanchang 330031, China;³²National Space Science Center, Chinese Academy of Sciences, Beijing 100190, China ）
出处： Science Bulletin 2023
摘要： We report the detection of a γ -ray bubble spanning at least 100 deg 2 in ultra high energy up to a few PeV in the direction of the star-forming regi

期刊

Absolute calibration of LHAASO WFCTA camera based on LED

作者： Aharonian, F.，An, Q.，Axikegu，Bai, Lixin，Bai, Yunxiang，Bao, Yiwei，Bastieri, D.，Bi, X. J.，Bi, Yujiang，Cai, Hui，Cai, J. T.，Cao, Zhen，Cao, Zhe，Chang, Jinfan，Chang, J. F.，Chen, B. M.，Chen, E. S.，Chen, Jian，Chen, Liang，Chen, Minjun，Chen, M. L.，Chen, Qihui，Chen, Shanhong，Chen, S. Chen，Chen, T. L.，Chen, Xiuliang，Chen, Yingcheng，Cheng, Ning，Cheng, Y. D.，Cui, Sh W.，Cui, Xiaohong，Cui, Yudong，Dai, B. Z.，Dai, Hongliang，Dai, Z. G.，Danzengluobu，Della Volpe, Danzengluobu D.，Piazzoli, Benedetto Dettorre，Dong, X. J.，Duan, Kaikai，Fan, J. H.，Fan, Y. Z.，Fan, Z. X.，Fang, Jinghong，Fang, Kun，Feng, C. F.，Feng, Lei，Feng, Shaohui，Feng, Youliang，Fu, Yangting，Gan, Haiyong，Gao, Bo，Gao, C. D.，Gao, L. Q.，Gao, Qi，Gao, Wei，Ge, Maomao，Geng, L. S.，Gong, G. H.，Gou, Q. B.，Gu, Minhao，Guo, F. L.，Guo, Junguang，Guo, X. L.，Guo, Yiqin，Guo, Yingying，Han, Y. A.，He, H. H.，He, Haoning，He, Jiancheng，He, S. L.，He, Xinbo，He, Yu，Heller, M.，Hor, Yuen Keung，Hou, Chao，Hu, H. B.，Hu, Shouyang，Hu, S. C.，Hu, X. J.，Huang, Daihui，Huang, Qiulan，Huang, Wenhao，Huang, X. T （ ¹Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center, Institute 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, Chengdu, Sichuan, China;⁴State Key Laboratory of Particle Detection and Electronics, China;⁵University of Science and Technology of China, Hefei, Anhui, 230026, China;⁶Department of Engineering Physics, Tsinghua University, Beijing, 100084, China;⁷National Astronomical Observatories, Chinese Academy of Sciences, Beijing, 100101, China;⁸National Space Science Center, Chinese Academy of Sciences, Beijing, 100190, China;⁹School of Physics, Peking University, Beijing, 100871, China;¹⁰Center for Astrophysics, Guangzhou University, Guangzhou, Guangdong, 510006, China;¹¹School of Physics and Astronomy (Zhuhai) & School of Physics (Guangzhou) & Sino-French Institute of Nuclear Engineering and Technology (Zhuhai), Sun Yat-sen University, Zhuhai & 510275 Guangzhou, Guangdong, 519000, China;¹²School of Physical Science and Technology, Guangxi University, Nanning, Guangxi, 530004, China;¹³Hebei Normal University, Shijiazhuang, Hebei, 050024, China;¹⁴School of Physics and Microelectronics, Zhengzhou University, Zhengzhou, Henan, 450001, China;¹⁵School of Astronomy and Space Science, Nanjing University, Nanjing, Jiangsu, 210023, China;¹⁶Key Laboratory of Dark Matter and Space Astronomy, Purple Mountain Observatory, Chinese Academy of Sciences, Nanjing, Jiangsu, 210023, China;¹⁷Institute of Frontier and Interdisciplinary Science, Shandong University, Qingdao, Shandong, 266237, China;¹⁸Key Laboratory for Research in Galaxies and Cosmology, Shanghai Astronomical Observatory, Chinese Academy of Sciences, Shanghai, 200030, China;¹⁹Tsung-Dao Lee Institute & School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, 200240, China;²⁰School of Physical Science and Technology & School of Information Science and Technology, Southwest Jiaotong University, Chengdu, Sichuan, 610031, China;²¹College of Physics, Sichuan University, Chengdu, Sichuan, 610065, China;²²Key Laboratory of Cosmic Rays (Tibet University), Ministry of Education, Lhasa, Tibet, 850000, China;²³School of Physics and Technology, Wuhan University, Wuhan, Hubei, 430072, China;²⁴School of Physics and Astronomy, Yunnan University, Kunming, Yunnan, 650091, China;²⁵Yunnan Observatories, Chinese Academy of Sciences, Kunming, Yunnan, 650216, China;²⁶National Institute of Metrology, Beijing, 100029, China;²⁷Dublin Institute for Advanced Studies, 31 Fitzwilliam Place, 2 Dublin, Ireland;²⁸Max-Planck-Institut for Nuclear Physics, P.O. Box 103980, Heidelberg, 69029, Germany;²⁹Dipartimento di Fisica dell'Università di Napoli “Federico II”, Complesso Universitario di Monte Sant'Angelo, via Cinthia, Napoli, 80126, Italy;³⁰Institute for Nuclear Research of Russian Academy of Sciences, Moscow, 117312, Russian Federation;³¹Moscow Institute of Physics and Technology, Moscow, 141700, Russian Federation;³²Département de Physique Nucléaire et Corpusculaire, faculté de Sciences, Université de Genève, 24 Quai Ernest Ansermet, Geneva, 1211, Switzerland;³³Department of Physics, Faculty of Science, Mahidol University, Bangkok, 10400, Thailand ）
出处： Nuclear Instruments and Methods in Physics Research, Section A: Accelerators, Spectrometers, Detectors and Associated Equipment 2022 Vol.1021
摘要： The main scientific goal of the LHAASO WFCTA experiment is to measure the cosmic ray energy spectra and composition from 10 TeV to 1 EeV. Cherenkov ph

共139条记录 1/14 第一页 [1] [2] [3] [4] [5] [6] [7] [8] [9] [10] 下一页最后一页到第页