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The Status of the Telescope Array experiment

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.Scott, 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
May-2011
Publisher
IOP Publishing Ltd.
Citation
Journal of Physics: Conference Series, v.293, no.1, pp 1 - 6
Pages
6
Indexed
SCOPUS
Journal Title
Journal of Physics: Conference Series
Volume
293
Number
1
Start Page
1
End Page
6
URI
https://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/151298
DOI
10.1088/1742-6596/293/1/012035
ISSN
1742-6588
1742-6596
Abstract
The purpose of The Telescope Array experiment is to identify origin of the ultra high energy cosmic rays. The Telescope Array is a hybrid detector consists of a surface detector array and air fluorescence detectors. This hybrid detector is observing extensive air showers to measure the energy spectrum, anisotropy and composition of Ultra High Energy Cosmic Rays. The detector construction has been completed in March 2008, and the hybrid observation with the full configuration has been running since that time. In this talk, the status of observation and our prospects are described.
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