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The tibet AS+MD project; status report 2017

Abstract:

We built a large (approximately 4,000 m2) 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 make a status report on the experiment.

Año de publicación:

2017

Keywords:

    Fuente:

    scopusscopus

    Tipo de documento:

    Conference Object

    Estado:

    Acceso restringido

    Áreas de conocimiento:

      Áreas temáticas:

        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.
        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.
        Nishizawa M.Nishizawa M.
        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.