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A Northern Sky Survey for Steady Tera-Electron Volt Gamma-Ray Point Sources Using the Tibet Air Shower Array

  • 【作者】Amenomori, M ,Ayabe, S ,Chen, D ,Cui, SW ,Danzengluobu ,Ding, LK ,Ding, XH ,Feng, CF ,Feng, ZY ,Gao, XY
  • 【作者单位】Department of Physics, Hirosaki University, Hirosaki 036-8561, Japan;Department of Physics, Saitama University, Saitama 338-8570, Japan;Faculty of Engineering, Yokohama National University, Yokohama 240-8501, Japan;Department of Physics, HeBei Normal University, Shijiazhuang 050016, China;Department of Mathematics and Physics, Tibet University, Lhasa 850000, China;Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China;Department of Mathematics and Physics, Tibet University, Lhasa 850000, China;Department of Physics, Shandong University, Jinan 250100, China;Institute of Modern Physics, South West Jiaotong University, Chengdu 610031, China;Department of Physics, Yunnan University, Kunming 650091, China;Department of Physics, Yunnan University, Kunming 650091, China;Department of Mathematics and Physics, Tibet University, Lhasa 850000, China;Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China;Department of Physics, Shandong University, Jinan 250100, China;Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan;Faculty of Education, Utsunomiya University, Utsunomiya 321-8505, Japan;Department of Mathematics and Physics, Tibet University, Lhasa 850000, China;Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China;Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan;Institute of Modern Physics, South West Jiaotong University, Chengdu 610031, China;Institute of Modern Physics, South West Jiaotong University, Chengdu 610031, China;Department of Physics, Konan University, Kobe 658-8501, Japan;Faculty of Systems Engineering, Shibaura Institute of Technology, Saitama 330-8570, Japan;Faculty of Engineering, Yokohama National University, Yokohama 240-8501, Japan;Department of Physics, Shinshu University, Matsumoto 390-8621, Japan;Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan;Department of Mathematics and Physics, Tibet University, Lhasa 850000, China;Center of Space Science and Application Research, Chinese Academy of Sciences, Beijing 100080, China;Department of Physics, Shandong University, Jinan 250100, China;Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China;Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China;Department of Mathematics and Physics, Tibet University, Lhasa 850000, China;Department of Physics, Saitama University, Saitama 338-8570, Japan;Department of Physics, Yunnan University, Kunming 650091, China;Department of Physics, Shinshu University, Matsumoto 390-8621, Japan;Advanced Media Network Center, Utsunomiya University, Utsunomiya 321-8585, Japan;Department of Physics, Hirosaki University, Hirosaki 036-8561, Japan;National Institute for Informatics, Tokyo 101-8430, Japan;Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan;Faculty of Education, Utsunomiya University, Utsunomiya 321-8505, Japan;Department of Physics, Saitama University, Saitama 338-8570, Japan;Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan;Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan;Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China;Tokyo Metropolitan College of Aeronautical Engineering, Tokyo 116-0003, Japan;Department of Physics, Konan University, Kobe 658-8501, Japan;Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan;Faculty of Engineering, Yokohama National University, Yokohama 240-8501, Japan;Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan;Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan;Shonan Institute of Technology, Fujisawa 251-8511, Japan;Department of Physics, Konan University, Kobe 658-8501, Japan;Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan;Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China;Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan;Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan;Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan;Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan;Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan;Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China;Department of Physics, Saitama University, Saitama 338-8570, Japan;Department of Physics, Shandong University, Jinan 250100, China;Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China;Department of Physics, Shandong University, Jinan 250100, China;Department of Physics, Konan University, Kobe 658-8501, Japan;Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China;Department of Physics, Yunnan University, Kunming 650091, China;Department of Physics, Shinshu University, Matsumoto 390-8621, Japan;Center of Space Science and Application Research, Chinese Academy of Sciences, Beijing 100080, China;Institute of Modern Physics, South West Jiaotong University, Chengdu 610031, China;Department of Mathematics and Physics, Tibet University, Lhasa 850000, China;Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan;Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China;Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China;Department of Physics, Shandong University, Jinan 250100, China;Department of Physics, Shandong University, Jinan 250100, China;Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China;Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China;Department of Mathematics and Physics, Tibet University, Lhasa 850000, China;Institute of Modern Physics, South West Jiaotong University, Chengdu 610031, China
  • 【年份】2005
  • 【卷号】Vol.633 No.2
  • 【页码】1005
  • 【ISSN】0004-637X
  • 【关键词】CRAB-NEBULA GALACTIC PLANE MARKARIAN 501 TEV SEARCH EMISSION PERFORMANCE RADIATION 
  • 【摘要】 Results of a steady TeV γ-ray point-source search using data taken from the Tibet HD and Tibet III arrays are presented. From 0° to 60° in declination, significant excesses from the well-known steady source Crab Nebula and the high state of the fla...
  • 【文献类型】 期刊
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