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The TIBET AS+MD project; progress report 2015

Abstract:

We plan to build a large (approximately 10,000 m-2) water Cherenkov- type muon detector array under the existing Tibet air shower array at 4,300 m above sea level, to observe 10-1000 TeV gamma rays from cosmic-ray accelerators in our Galaxy with wide field of view at very low background level. A gamma-ray induced air shower has significantly less muons compared with a cosmic-ray induced one. Therefore, we can effectively discriminate between primary gamma rays and cosmic-ray background events by means of counting number of muons in an air shower event by the muon detector array. We will make a progress report on the project, as some part of it started data-taking in 2014.

Año de publicación:

2015

Keywords:

    Fuente:

    scopusscopus

    Tipo de documento:

    Conference Object

    Estado:

    Acceso restringido

    Áreas de conocimiento:

      Áreas temáticas:

      • Conocimiento
      • Organizaciones generales y museología
      • Gestión y servicios auxiliares

      Contribuidores:

      Shibata M.Shibata M.
      Labaciren Labaciren
      Hotta N.Hotta N.
      Jia H.Y.Jia H.Y.
      Chen T.L.Chen T.L.
      Kasahara K.Kasahara K.
      Sakata M.Sakata M.
      Lu H.Lu H.
      Nakamura Y.Nakamura Y.
      Bi X.J.Bi X.J.
      Amenomori M.Amenomori M.
      Danzengluobu Danzengluobu
      Zhaxisangzhu Zhaxisangzhu
      Yuan A.F.Yuan A.F.
      Zhou X.X.Zhou X.X.
      Gou Q.B.Gou Q.B.
      Tsuchiya H.Tsuchiya H.
      Liu C.Liu C.
      Ding L.K.Ding L.K.
      Huang J.Huang J.
      Qu X.B.Qu X.B.
      Li H.J.Li H.J.
      Cui S.W.Cui S.W.
      Zhang H.M.Zhang H.M.
      Hibino K.Hibino K.
      Udo S.Udo S.
      Li W.J.Li W.J.
      Xue L.Xue L.
      Nanjo H.Nanjo H.
      Li A.F.Li A.F.
      Mizutani K.Mizutani K.
      Wu H.R.Wu H.R.
      Tan Y.H.Tan Y.H.
      Niwa T.Niwa T.
      Chen D.Chen D.
      Guo Y.Q.Guo Y.Q.
      Hu H.B.Hu H.B.
      T. K. SakoT. K. Sako
      Kajino F.Kajino F.
      Takita M.Takita M.
      Hu H.B.Hu H.B.
      Miyazaki T.Miyazaki T.
      Torii S.Torii S.
      Zhai L.M.Zhai L.M.
      Shirai T.Shirai T.
      Ohnishi M.Ohnishi M.
      Wang H.Wang H.
      Yamamoto Y.Yamamoto Y.
      Feng Z.Y.Feng Z.Y.
      Kozai M.Kozai M.
      Feng Z.Y.Feng Z.Y.
      Nishizawa M.Nishizawa M.
      Yasue S.Yasue S.
      Feng C.F.Feng C.F.
      Kato C.Kato C.
      Zhang J.L.Zhang J.L.
      Zhang X.Y.Zhang X.Y.
      Liu M.Y.Liu M.Y.
      Chen W.Y.Chen W.Y.
      Yang Z.Yang Z.
      Zhang Y.Zhang Y.
      Meng X.R.Meng X.R.
      Zhang Y.Zhang Y.
      Qian X.L.Qian X.L.
      Yuda T.Yuda T.
      He H.H.He H.H.
      Shiomi A.Shiomi A.
      Zhang Y.Zhang Y.
      Le G.M.Le G.M.
      Tateyama N.Tateyama N.
      Saito T.Y.Saito T.Y.
      Ozawa S.Ozawa S.
      Nakajima T.Nakajima T.
      Katayose Y.Katayose Y.
      He Z.T.He Z.T.
      Saito T.Saito T.
      Jiang L.Jiang L.
      Munakata K.Munakata K.
      Sugimoto H.Sugimoto H.
      Ohta I.Ohta I.
      Shao J.Shao J.
      Yamauchi K.Yamauchi K.
      Kawata K.Kawata K.
      Liu J.S.Liu J.S.