检索结果：
返回 35 结果。
排序：
- 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
- 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
- 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
- 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
- 作者： Zhang, Zhiman，Lin, Fawei，Xiang, Li，Yu, Hongdi，Wang, Zhihua，Yan, Beibei，Chen, Guanyi （ 1 School of Environmental Science and Engineering, Tianjin University/Tianjin Engineering Research Center of Organic Solid Waste Safety Disposal and Energy Utilization, Tianjin 300072, PR China 2 State Key Laboratory of Clean Energy Utilization, Zhejiang University, Hangzhou 310027, PR China 3 School of Mechanical Engineering, Tianjin University of Commerce, Tianjin 300134, PR China 4 School of Science, Tibet University, Lhasa 850012, PR China ）
- 出处： Chemical Engineering Journal 2022 Vol.427
- 关键词： Catalytic ozonation CB MnCo-I NOx Simultaneous removal
- 摘要： [Display omitted] • CB conversion reached 90% at 120 °C with O 3 /CB of 10.0 over 3D sphere-like MnCoO x. • NO presence accelerated transformation of
期刊
- 作者： Zhiman Zhang，Fawei Lin，Li Xiang，Hongdi Yu，Zhihua Wang，Beibei Yan，Guanyi Chen （ 1 School of Environmental Science and Engineering, Tianjin University/Tianjin Engineering Research Center of Organic Solid Waste Safety Disposal and Energy Utilization, Tianjin 300072, PR China; 2 ORCID: https://orcid.org/0000-0001-5461-8277.; 3 State Key Laboratory of Clean Energy Utilization, Zhejiang University, Hangzhou 310027, PR China; 4 School of Mechanical Engineering, Tianjin University of Commerce, Tianjin 300134, PR China; 5 School of Science, Tibet University, Lhasa 850012, PR China ）
- 出处： Chemical Engineering Journal 2022 Vol.427 P130929
- 关键词： CB NO Simultaneous removal Catalytic ozonation MnCo-I
- 摘要： This paper synthesized bimetallic MnCoO x catalysts for efficient synergistic ozonation of chlorobenzene and NO with presence of complicated compone
-
点击量：1
- 作者： 郭洁，王志华 （ 西藏大学文学院 ）
- 出处： 佳木斯大学社会科学学报 2022 第40卷 第5期 P99-103
- 关键词： 次仁罗布 短篇小说 城市 乡村 精神气脉
- 摘要： 次仁罗布的短篇小说聚焦了现代化、城市化进程中藏域地区如何承袭过往、顺应时代的问题。其短篇小说尽览青藏高原的人文风光并展现市井人物的生存困境。作家对藏地城、村的变化及文化焦虑提出了自己的哲思，现实主义文风背后尽显其悲悯、温暖的精神气脉。
-
点击量：1
期刊
- 作者： Zhang, Zhiman，Lin, Fawei，Xiang, Li，Yu, Hongdi，Wang, Zhihua，Yan, Beibei，Chen, Guanyi （ 1School of Environmental Science and Engineering, Tianjin University/Tianjin Engineering Research Center of Organic Solid Waste Safety Disposal and Energy Utilization, Tianjin, 300072, China;2State Key Laboratory of Clean Energy Utilization, Zhejiang University, Hangzhou, 310027, China;3School of Mechanical Engineering, Tianjin University of Commerce, Tianjin, 300134, China;4School of Science, Tibet University, Lhasa, 850012, China ）
- 出处： Chemical Engineering Journal 2022 Vol.427
- 摘要： This paper synthesized bimetallic MnCoOx catalysts for efficient synergistic ozonation of chlorobenzene and NO with presence of complicated component
期刊
- 作者： Zhang, Zhiman，Lin, Fawei，Xiang, Li，Yu, Hongdi，Wang, Zhihua，Yan, Beibei，Chen, Guanyi （ 1School of Environmental Science and Engineering, Tianjin University/Tianjin Engineering Research Center of Organic Solid Waste Safety Disposal and Energy Utilization, Tianjin, 300072, China;2State Key Laboratory of Clean Energy Utilization, Zhejiang University, Hangzhou, 310027, China;3School of Mechanical Engineering, Tianjin University of Commerce, Tianjin, 300134, China;4School of Science, Tibet University, Lhasa, 850012, China ）
- 出处： Chemical Engineering Journal 2022 Vol.427
- 摘要： This paper synthesized bimetallic MnCoOx catalysts for efficient synergistic ozonation of chlorobenzene and NO with presence of complicated component
期刊
- 作者： Zhang, Zhiman，Lin, Fawei，Xiang, Li，Yu, Hongdi，Wang, Zhihua，Yan, Beibei，Chen, Guanyi （ 1School of Environmental Science and Engineering, Tianjin University/Tianjin Engineering Research Center of Organic Solid Waste Safety Disposal and Energy Utilization, Tianjin, 300072, China;2State Key Laboratory of Clean Energy Utilization, Zhejiang University, Hangzhou, 310027, China;3School of Mechanical Engineering, Tianjin University of Commerce, Tianjin, 300134, China;4School of Science, Tibet University, Lhasa, 850012, China ）
- 出处： Chemical Engineering Journal 2022 Vol.427
- 摘要： This paper synthesized bimetallic MnCoOx catalysts for efficient synergistic ozonation of chlorobenzene and NO with presence of complicated component