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检索条件"机构=Key Laboratory of Particle Astrophysics and Experimental Physics Division and Computing Center"
572 条 记 录,以下是11-20 订阅
排序:
The First LHAASO Catalog of Gamma-ray Sources below 25TeV  38
The First LHAASO Catalog of Gamma-ray Sources below 25TeV
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38th International Cosmic Ray Conference, ICRC 2023
作者: Hu, S.C. Xiang, G.M. Zha, M. Yao, Z.G. Key Laboratory of Particle Astrophyics & Experimental Physics Division & Computing Center Institute of High Energy Physics Chinese Academy of Sciences Beijing100049 China University of Chinese Academy of Sciences Beijing100049 China Tianfu Cosmic Ray Research Center Sichuan Chengdu610000 China Key Laboratory for Research in Galaxies and Cosmology Shanghai Astronomical Observatory Chinese Academy of Sciences Shanghai200030 China
We report the first catalog of TeV gamma-ray sources realized with the most sensitive wide field-of-view TeV telescope ever built. Since March 2021, it continuously surveys the northern sky with field of view ∼ 2 sr ... 详细信息
来源: 评论
Design and Test of SiPM Readout Circuit  38
Design and Test of SiPM Readout Circuit
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38th International Cosmic Ray Conference, ICRC 2023
作者: Li, Kefan Yang, Mingjie Zhang, Shoushan Chen, Long Zhu, Fengrong Southwest Jiaotong University School of Physical Science and Technology No. 999 Xi’an Road Chengdu China Institute of High Energy Physics Chinese Academy of Sciences Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center No. 19B Yuquan Road Beijing China Institute of High Energy Physics Chinese Academy of Sciences TIANFU Cosmic Ray Research Center No. 1500 Kezhi Road Chengdu China
Silicon photomultiplier (SiPM) have several advantages such as high photon detection efficiency, wide spectral response range, high gain at low bias voltage and compact structure. In addition, SiPM is not damaged by h... 详细信息
来源: 评论
Discovery of the Ultra-High-Energy gamma-ray source LHAASO J2002+3238 spatially associated with SNR G69.7+1.0  38
Discovery of the Ultra-High-Energy gamma-ray source LHAASO J...
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38th International Cosmic Ray Conference, ICRC 2023
作者: Hou, B.W. Zhang, R. Xi, S.Q. Chen, S.Z. He, H.N. Xia, Z.Q. Key Laboratory of Particle Astrophyics & Experimental Physics Division & Computing Center Institute of High Energy Physics Chinese Academy of Sciences Beijing100049 China University of Chinese Academy of Sciences Beijing100049 China Tianfu Cosmic Ray Research Center Sichuan Chengdu610000 China University of Science and Technology of China Hefei230026 China Key Laboratory of Dark Matter and Space Astronomy Key Laboratory of Radio Astronomy Purple Mountain Observatory Chinese Academy of Sciences Nanjing210023 China
The origin of Galactic PeV cosmic rays is still under debate. Shell-type supernova remnants (SNRs) are proposed to be one of the candidate sources of Galactic PeV cosmic rays, but observational evidence is lacking. He... 详细信息
来源: 评论
Detection of a new GeV source in the outer region of the Coma cluster: a signature of external accretion shock ?
arXiv
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arXiv 2024年
作者: Chen, Xiao-Bin Wang, Kai Huang, yi-Yun Zhang, Hai-Ming Xi, Shao-Qiang Liu, Ruo-Yu Wang, Xiang-Yu School of Astronomy and Space Science Nanjing University Nanjing210023 China Ministry of Education Nanjing210023 China Guangxi Key Laboratory for Relativistic Astrophysics School of Physical Science and Technology Guangxi University Nanning530004 China Key Laboratory of Particle Astrophysics & Experimental Physics Division & Computing Center Institute of High Energy Physics Chinese Academy of Sciences Beijing100049 China
The supersonic flow motions associated with infall of baryonic gas toward sheets and filaments, as well as cluster mergers, produces large-scale shock waves. The shocks associated with galaxy clusters can be classifie... 详细信息
来源: 评论
Search for neutrino emission from the Cygnus Bubble based on LHAASO γ-ray observations
arXiv
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arXiv 2024年
作者: Li, Wenlian Huang, Tian-Qi Xu, Donglian He, Huihai Tsung-Dao Lee Institute Shanghai Jiao Tong University Shanghai201210 China Key Laboratory of Particle Astrophysics and Experimental Physics Division and Computing Center Institute of High Energy Physics Chinese Academy of Sciences Beijing100049 China TIANFU Cosmic Ray Research Center Sichuan Chengdu China Shanghai Key Laboratory for Particle Physics and Cosmology Shanghai200240 China University of Chinese Academy of Sciences Beijing100049 China
The Cygnus region, which contains massive molecular and atomic clouds and young stars, is a promising Galactic neutrino source candidate. Cosmic rays transport in the region can produce neutrinos and γ-rays. Recently... 详细信息
来源: 评论
由超拍电子伏特加速器产生的超高能伽马射线气泡
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Science Bulletin 2024年 第4期69卷 449-457页
作者: LHAASO Collaboration Zhen Cao Chuandong Gao Cong Li Ruo-Yu Liu Ruizhi Yang 不详 Key Laboratory of Particle Astrophyics&Experimental Physics Division&Computing Center Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China University of Chinese Academy of Sciences Beijing 100049China TIANFU Cosmic Ray Research Center ChengduChina Institute of Frontier and Interdisciplinary Science Shandong UniversityQingdao 266237China School of Astronomy and Space Science Nanjing UniversityNanjing 210023China University of Science and Technology of China Hefei 230026China
We report the detection of aγ-ray bubble spanning at least 100deg2 in ultra-high energy(UHE)up to a few PeV in the direction of the star-forming region Cygnus X,implying the presence super PeVatron(s)accelerating pro... 详细信息
来源: 评论
Determining the Origin of Very-high-energy Gamma Rays from Galactic Sources by Future Neutrino Observations
arXiv
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arXiv 2023年
作者: Song, Bo-Heng Huang, Tian-Qi Wang, Kai Department of Astronomy School of Physics Huazhong University of Science and Technology Wuhan430074 China Key Laboratory of Particle Astrophysics and Experimental Physics Division Computing Center Institute of High Energy Physics Chinese Academy of Sciences Beijing100049 China Tianfu Cosmic Ray Research Center Sichuan Chengdu610000 China
Recently, the Large High Altitude Air Shower Observatory (LHAASO) identified 12 γ-ray sources emitting gamma rays with energies above 100 TeV, making them potential PeV cosmic-ray accelerators (PeVatrons). Neutrino o... 详细信息
来源: 评论
Chapter 1 LHAASO Instruments and Detector technology
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Chinese physics C 2022年 第3期46卷 1-35页
作者: Xin-Hua Ma Yu-Jiang Bi Zhen Cao Ming-Jun Chen Song-Zhan Chen Yao-Dong Cheng Guang-Hua Gong Min-Hao Gu Hui-Hai He Chao Hou Wen-Hao Huang Xing-Tao Huang Cheng Liu Oleg Shchegolev Xiang-Dong Sheng Yuri Stenkin Chao-Yong Wu Han-Rong Wu Sha Wu Gang Xiao Zhi-Guo Yao Shou-Shan Zhang Yi Zhang Xiong Zuo Key Laboratory of Particle Astrophyics&Experimental Physics Division&Computing Center Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China TIANFU Cosmic Ray Research Center ChengduSichuanChina University of Chinese Academy of Sciences Beijing 100049China Department of Engineering Physics Tsinghua UniversityBeijing 100084China Institute of Frontier and Interdisciplinary Science Shandong UniversityQingdao 266237ShandongChina Institute for Nuclear Research of Russian Academy of Sciences Moscow 117312Russia Moscow Institute of Physics and Technology Moscow 141700Russia Key Laboratory of Dark Matter and Space Astronomy Purple Mountain ObservatoryChinese Academy of SciencesNanjing 210023JiangsuChina
The Large High Altitude Air Shower Observatory(LHAASO)(Fig.1)is located at ***(4410 m a.s.l.,600 g/cm^(2),29°21'27.56"N,100°08'19.66"E)in Daocheng,Sichuan province,*** consists of 1.3 km^(2... 详细信息
来源: 评论
Testing and analysis of the plastic scintillator units for LHAASO-ED
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Radiation Detection Technology and Methods 2021年 第4期5卷 513-519页
作者: Ya-Ping Wang Chao Hou Xiang-Dong Sheng Shao-Hui Feng Hong-Kui Lv Jia Liu Jing Zhao Xiao-Peng Zhang Quan-Bu Gou Key Laboratory of Particle Astrophyics&Experimental Physics Division&Computing Center Institute of High Energy PhysicsChinese Academy of SciencesBeijing 100049China University of Chinese Academy of Sciences Beijing 100049China TIANFU Cosmic Ray Research Center ChengduSichuanChina
Background A total of 5195 electromagnetic particle detectors(EDs)are used in the 1-square-kilometer extensive air shower array(KM2A),which is a subarray of the Large High Altitude Air Shower Observatory(LHAASO).Purpo... 详细信息
来源: 评论
Search for neutrino signals correlated with LHAASO diffuse Galactic emission
arXiv
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arXiv 2024年
作者: Li, Wenlian Huang, Tian-Qi Xu, Donglian He, Huihai Tsung-Dao Lee Institute Shanghai Jiao Tong University Shanghai201210 China Shanghai Key Laboratory for Particle Physics and Cosmology Shanghai200240 China Key Laboratory of Particle Astrophysics and Experimental Physics Division and Computing Center Institute of High Energy Physics Chinese Academy of Sciences Beijing100049 China TIANFU Cosmic Ray Research Center Sichuan Chengdu China School of Physics and Astronomy Shanghai Jiao Tong University Shanghai200240 China University of Chinese Academy of Sciences Beijing100049 China
The diffuse Galactic γ-ray emission originates from the interactions between cosmic rays and the interstellar medium or radiation fields within our Galaxy, where the production of neutrinos is also anticipated. Recen... 详细信息
来源: 评论