Observation of TeV gamma rays from the fermi bright galactic sources with the tibet air shower array

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【作者】Amenomori, M.，Bi, X.J.，Chen, D.，Cui, S.W.，Danzengluobu，Ding, L.K.，Ding, X.H.，Fan, C.，Feng, C.F.，Feng, Z.，Feng, Z.Y.，Gao, X.Y.，Geng, Q.X.，Gou, Q.B.，Guo, H.W.，He, H.H.，He, M.，Hibino, K.，Hotta, N.，Hu, H.，Hu, H.B.，Huang, J.，Huang, Q.，Jia, H.Y.，Jiang, L.，Kajino, F.，Kasahara, K.，Katayose, Y.，Kato, C.，Kawata, K.，Labaciren，Le, G.M.，Li, A.F.，Li, H.C.，Li, J.Y.，Liu, C.，Lou, Y.-Q.，Lu, H.，Meng, X.R.，Mizutani, K.，Mu, J.，Munakata, K.，Nanjo, H.，Nishizawa, M.，Ohnishi, M.，Ohta, I.，Ozawa, S.，Saito, T.，Saito, T.Y.，Sakata, M.，Sako, T.K.，Shibata, M.，Shiomi, A.，Shirai, T.，Sugimoto, H.，Takita, M.，Tan, Y.H.，Tateyama, N.，Torii, S.，Tsuchiya, H.，Udo, S.，Wang, B.，Wang, H.，Wang, Y.，Wang, Y.G.，Wu, H.R.，Xue, L.，Yamamoto, Y.，Yan, C.T.，Yang, X.C.，Yasue, S.，Ye, Z.H.，Yu, G.C.，Yuan, A.F.，Yuda, T.，Zhang, H.M.，Zhang, J.L.，Zhang, N.J.，Zhang, X.Y.，Zhang, Y.，Zhang, Y.，Zhang, Y.，Zhaxisangzhu，Zhou, A.X.X.
【作者单位】a Department of Physics, Hirosaki University, Hirosaki 036-8561, Japan; b Key Laboratory of Particle Astrophysics, Institute of High Energy Physics, Chinese Academy of Sciences, Beijing 100049, China; c Institute for Cosmic Ray Research, University of Tokyo, Kashiwa 277-8582, Japan; d Department of Physics, Hebei Normal University, Shijiazhuang 050016, China; e Department of Mathematics and Physics, Tibet University, Lhasa 850000, China; f Department of Physics, Shandong University, Jinan 250100, China; g Institute of Modern Physics, SouthWest Jiaotong University, Chengdu 610031, China; h Department of Physics, Yunnan University, Kunming 650091, China; i Faculty of Engineering, Kanagawa University, Yokohama 221-8686, Japan; j Faculty of Education, Utsunomiya University, Utsunomiya 321-8505, Japan; k Department of Physics, Konan University, Kobe 658-8501, Japan; l Research Institute for Science and Engineering, Waseda University, Tokyo 169-8555, Japan; m Faculty of Engineering, Yokohama National University, Yokohama 240-8501, Japan; n Department of Physics, Shinshu University, Matsumoto 390-8621, Japan; o National Center for Space Weather, China Meteorological Administration, Beijing 100081, China; p Physics Department and Tsinghua Center for Astrophysics, Tsinghua University, Beijing 100084, China; q Saitama University, Saitama 338-8570, Japan; r National Institute of Informatics, Tokyo 101-8430, Japan; s Sakushin Gakuin University, Utsunomiya 321-3295, Japan; t Tokyo Metropolitan College of Industrial Technology, Tokyo 116-8523, Japan; u Max-Planck-Institut für Physik, München D-80805, Germany; v College of Industrial Technology, Nihon University, Narashino 275-8576, Japan; w Shonan Institute of Technology, Fujisawa 251-8511, Japan; x RIKEN, Wako 351-0198, Japan; y Institute of Disaster Prevention Science and Technology, Yanjiao 065201, China; z School of General Education, Shinshu University, Matsumoto 390-8621, Japan; aa Center of Space Science and Application Research, Chinese Academy of Sciences, Beijing 100080, China
【年份】2010
【卷号】Vol.709 No.1Part2
【页码】L6-L10
【ISSN】2041-8205
【关键词】Gamma rays: general ISM: supernova remnants Pulsars: general
【摘要】 Using the Tibet-III air shower array, we search for TeV γ-rays from 27 potential Galactic sources in the early list of bright sources obtained by the Fermi Large Area Telescope at energies above 100MeV. Among them, we observe seven sources instead of...
【文献类型】期刊

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