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Status and prospect of telescope array (TA) experiment

Authors
Kasahara, K.Kawai, H.Yoshida, S.Yoshii, H.Chung, T.Nam, S.W.Oh, S.Park, I.H.Park, J.H.Yang, J.Cheon, Byung GuUnno, Y.Yun, Y.H.Tanaka, K.Cohen, F.Fukushima, M.Hayashida, N.Hiyama, K.Ikeda, D.Kido, E.Kondo, Y.Nonaka, T.Ohnishi, M.Ohoka, H.Ozawa, S.Sagawa, H.Sakurai, N.Shibata, T.Shimodaira, H.Takeda, M.Taketa, A.Takita, M.Tokuno, H.Torii, R.Udo, S.Yamakawa, Y.Fujii, H.Matsuda, T.Tanaka, M.Yamaoka, H.Hibino, K.Benno, T.Chikawa, M.Doura, K.Nakamura, T.Huentemeyer, P.Sinnis, G.Teshima, M.Kadota, K.Uchihori, Y.Hayashi, K.Hayashi, Y.Kawakami, S.Matsuyama, T.Minamino, M.Ogio, S.Ohshima, A.Okuda, T.Shimizu, N.Tanaka, H.Bergman, D.R.Hughes, G.A.Scott, L.M.Stratton, S.R.Thomson, G.B.Endo, A.Inoue, N.Kawana, S.Wada, Y.Azuma, R.Fukuda, T.Iguchi, T.Kakimoto, F.Machida, S.Murano, Y.Tameda, Y.Tsunesada, Y.Chiba, J.Miyata, K.Ormes, J.Matthews, J.A.J.Abbasi, R.U.Abu-Zayyad, T.Belz, J.W.Blake, S.A.Brusova, O.Cady, R.Cao, Z.Jui, C.C.H.Martens, K.Mostafa, M.Matthews, J.N.Rodriguez, D.Smith, J.D.Sokolsky, P.Springer, R.W.Thomas, J.R.Thomas, S.B.Wiencke, L.R.Doyle, T.Taylor, M.J.Wickwar, V.B.Wilkerson, T.D.Honda, K.Ikuta, K.Ishii, T.Kanbe, T.Tomida, T.Cho, I.S.Kwon, Y.
Issue Date
Jul-2007
Publisher
Universidad Nacional Autonoma de Mexico
Citation
Proceedings of the 30th International Cosmic Ray Conference, ICRC 2007, v.4, no.HE PART 1, pp.417 - 420
Indexed
SCOPUS
Journal Title
Proceedings of the 30th International Cosmic Ray Conference, ICRC 2007
Volume
4
Number
HE PART 1
Start Page
417
End Page
420
URI
https://scholarworks.bwise.kr/hanyang/handle/2021.sw.hanyang/179843
ISSN
0000-0000
Abstract
Telescope Array (TA) is an air shower experiment composed of an array of ground particle detectors and 3 sets of fluorescence telescopes installed in Utah, USA. It aims at drawing a conclusion on the (non-)existence of the GZK cutoff reported controversially by AGASA and HiRes experiments. An anisotropy of the UHECR arrival directions will be studied in the northern hemisphere where the galactic disturbances are small. The plastic scintillator is useful for the determination of the air shower energy independent of the hadronic interaction model and the primary composition. Various calibration methods will be applied for the accurate determination of event energy scale. A total acceptance of the ground array and the telescope will be more than 20 times larger than that of AGASA. An operation of partial detector has started in spring 2007. The status of the experiment is reported and prospects for the physics are given.
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