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The telescope array experiment: Status and prospectsopen access

Authors
Tokuno, H.Abu-Zayyad, T.Aida, R.Allen, M.Azuma, R.Barcikowski, E.Belz, J.W.Benno, T.Bergman, D.R.Blake, S.A.Brusova, O.Cady, R.Cheon, B.G.Chiba, J.Chikawa, M.Cho, E.J.Cho, L.S.Cho, W.R.Cohen, F.Doura, K.Ebeling, C.Fujii, H.Fujii, T.Fukuda, T.Fukushima, M.Gorbunov, D.Hanlon, W.Hayashi, K.Hayashi, Y.Hayashida, N.Hibino, K.Hiyama, K.Honda, K.Hughes, G.Iguchi, T.Ikeda, D.Ikuta, K.Innemee, S.J.J.Inoue, N.Ishii, T.Ishimori, R.Ivanov, D.Iwamoto, S.Jui, C.C.H.Kadota, K.Kakimoto, F.Kalashev, O.Kanbe, T.Kang, H.Kasahara, K.Kawai, H.Kawakami, S.Kawana, S.Kido, E.Kim, B.G.Kim, H.B.Kim, J.H.Kim, J.H.Kitsugi, A.Kobayashi, K.Koers, H.Kondo, Y.Kuzmin, V.Kwon, Y.J.Lim, J.H.Lim, S.I.Machida, S.Martens, K.Martineau, J.Matsuda, T.Matsuyama, T.Matthews, J.N.Minamino, M.Miyata, K.Miyauchi, H.Murano, Y.Nakamura, T.Nam, S.W.Nonaka, T.Ogio, S.Ohnishi, M.Ohoka, H.Okuda, T.Oshima, A.Ozawa, S.Park, I.H.Rodriguez, D.Roh, S.Y.Rubtsov, G.Ryu, D.Sagawa, H.Sakurai, N.Scot, L.M.Shah, P.D.Shibata, T.Shimodaira, H.Shin, B.K.Smith, J.D.Sokolsky, P.Sonley, T.J.Springer, R.W.Stokes, B.T.Stratton, S.R.Suzuki, S.Takahashi, Y.Takeda, M.Taketa, A.Takita, M.Tameda, Y.Tanaka, H.Tanaka, K.Tanaka, M.Thomas, J.R.Thomas, S.B.Thomson, G.B.Tinyakov, P.Tkachev, I.Tomida, T.Torii, R.Troitsky, S.Tsunesada, Y.Tsuyuguchi, Y.Uchihori, Y.Udo, S.Ukai, H.Vanklaveren, B.Wada, Y.Wood, M.Yamakawa, T.Yamakawa, Y.Yamaoka, H.Yang, J.Yoshida, S.Yoshii, H.Zundel, Z.
Issue Date
Jun-2010
Publisher
AIP
Keywords
Extensive air shower; Ultra high energy cosmic rays
Citation
AIP Conference Proceedings, v.1238, pp.365 - 368
Indexed
SCOPUS
Journal Title
AIP Conference Proceedings
Volume
1238
Start Page
365
End Page
368
URI
https://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/174827
DOI
10.1063/1.3455968
ISSN
0094-243X
Abstract
The Telescope Array is a detector of extensive air shower produced by ultra High energy cosmic ray. This detector is located on Utah, USA. The construction have been completed and the full operation has been running from March 2008. In this talk, the status of observation and our prospects are described.
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