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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】M. Amenomori,S. Ayabe,D. Chen,S. W. Cui,Danzengluobu,L. K. Ding,X. H. Ding,C. F. Feng,Z. Y. Feng,X. Y. Gao,Q. X. Geng,H. W. Guo,H. H. He,M. He,K. Hibino,N. Hotta,Haibing Hu,H. B. Hu,J. Huang,Q. Huang,H. Y. Jia,F. Kajino,K. Kasahara,Y. Katayose,C. Kato,K. Kawata,Labaciren,G. M. Le,J. Y. Li,H. Lu,S. L. Lu,X. R. Meng,K. Mizutani,J. Mu,K. Munakata,A. Nagai,H. Nanjo,M. Nishizawa,M. Ohnishi,I. Ohta,H. Onuma,T. Ouchi,S. Ozawa,J. R. Ren,T. Saito,M. Sakata,T. Sasaki,M. Shibata,A. Shiomi,T. Shirai,H. Sugimoto,M. Takashima,M. Takita,Y. H. Tan,N. Tateyama,S. Torii,H. Tsuchiya,S. Udo,T. Utsugi,H. Wang,X. Wang,Y. G. Wang,H. R. Wu,L. Xue,Y. Yamamoto,C. T. Yan,X. C. Yang,S. Yasue,Z. H. Ye,G. C. Yu,A. F. Yuan,T. Yuda,H. M. Zhang,J. L. Zhang,N. J. Zhang,X. Y. Zhang,Yi Zhang,Y. Zhang,Zhaxisangzhu,X. X. Zhou,
  • 【DOI】10.1086/491612
  • 【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】1005-1012
  • 【ISSN】0004-637X
  • 【关键词】gamma rays : observations surveys 
  • 【摘要】 Results of a steady TeV gamma-ray point-source search using data taken from the Tibet HD ( 1997 February - 1999 September) and Tibet III ( 1999 November - 2001 October) arrays are presented. From 0 degrees to 60 degrees in declination, significant ex...
  • 【文献类型】 期刊
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