Telescope array; status and prospects

H. Kawai; T. Nunomura; N. Sakurai; S. Yoshida; H. Yoshii; K. Tanaka; F. Cohen; M. Fukushima; N. Hayashida; M. Ohnishi; H. Ohoka; Shunsuke Ozawa; H. Sagawa; T. Shibata; H. Shimodaira; M. Takeda; A. Taketa; M. Takita; H. Tokuno; R. Torii; S. Udo; H. Fujii; T. Matsuda; M. Tanaka; H. Yamaoka; K. Hibino; T. Benno; M. Chikawa; T. Nakamura; M. Teshima; K. Kadota; Y. Uchihori; Y. Hayashi; K. Matsumoto; Y. Matsumoto; T. Matsuyama; S. Ogio; A. Ohshima; T. Okuda; D. R. Bergman; G. Hughes; S. Stratton; G. B. Thomson; N. Inoue; Y. Wada; K. Kasahara; M. Fukuda; T. Iguchi; F. Kakimoto; R. Minagawa; Y. Tameda; Y. Tsunesada; J. W. Belz; J. A J Matthews; T. Abu-Zayyad; R. Cady; Z. Cao; P. Huentemeyer; C. C H Jui; K. Martens; J. N. Matthews; J. D. Smith; P. Sokolsky; R. W. Springer; S. B. Thomas; L. R. Wiencke; T. Doyle; M. J. Taylor; V. B. Wickwar; T. D. Wilkerson; K. Hashimoto; K. Honda; T. Ishii; T. Kanbe

Telescope array; status and prospects

H. Kawai, T. Nunomura, N. Sakurai, S. Yoshida, H. Yoshii, K. Tanaka, F. Cohen, M. Fukushima, N. Hayashida, M. Ohnishi, H. Ohoka, Shunsuke Ozawa, H. Sagawa, T. Shibata, H. Shimodaira, M. Takeda, A. Taketa, M. Takita, H. Tokuno, R. ToriiS. Udo, H. Fujii, T. Matsuda, M. Tanaka, H. Yamaoka, K. Hibino, T. Benno, M. Chikawa, T. Nakamura, M. Teshima, K. Kadota, Y. Uchihori, Y. Hayashi, K. Matsumoto, Y. Matsumoto, T. Matsuyama, S. Ogio, A. Ohshima, T. Okuda, D. R. Bergman, G. Hughes, S. Stratton, G. B. Thomson, N. Inoue, Y. Wada, K. Kasahara, M. Fukuda, T. Iguchi, F. Kakimoto, R. Minagawa, Y. Tameda, Y. Tsunesada, J. W. Belz, J. A J Matthews, T. Abu-Zayyad, R. Cady, Z. Cao, P. Huentemeyer, C. C H Jui, K. Martens, J. N. Matthews, J. D. Smith, P. Sokolsky, R. W. Springer, S. B. Thomas, L. R. Wiencke, T. Doyle, M. J. Taylor, V. B. Wickwar, T. D. Wilkerson, K. Hashimoto, K. Honda, T. Ishii, T. Kanbe

研究成果: Conference contribution

3 引用（Scopus）

抜粋

The Telescope Array (TA) is the air shower experiment designed for observing extremely high energy cosmic rays. It consists of an array of scintillation counters covering the ground area of 760 km² and 3 sets of air fluorescence telescopes placed in the perimeter of the array. The TA aims at making a decisive measurement of the cosmic ray spectrum in the GZK cutoff region, and pinning down the nature of cosmic rays exceeding 10 ²⁰ eV, which have been the subject of extensive studies by AGASA, HiRes and other air shower experiments. The TA is being constructed in Utah, USA, and the commissioning is expected in the spring of 2007. An extension of hybrid measurement is planned down to 10^17.5 eV in order to elucidate the galactic to extra-galactic transition of cosmic ray sources (TALE proposal).

元の言語	English
ホスト出版物のタイトル	29th International Cosmic Ray Conference, ICRC 2005
出版者	Tata Institute of Fundamental Research
ページ	141-144
ページ数	4
巻	8
出版物ステータス	Published - 2005
外部発表	Yes
イベント	29th International Cosmic Ray Conference, ICRC 2005 - Pune, India 継続期間: 2005 8 3 → 2005 8 10

Other

Other	29th International Cosmic Ray Conference, ICRC 2005
国	India
市	Pune
期間	05/8/3 → 05/8/10

ASJC Scopus subject areas

Nuclear and High Energy Physics

文献にアクセス

フィンガープリント Telescope array; status and prospects' の研究トピックを掘り下げます。これらはともに一意のフィンガープリントを構成します。

これを引用

Kawai, H., Nunomura, T., Sakurai, N., Yoshida, S., Yoshii, H., Tanaka, K., Cohen, F., Fukushima, M., Hayashida, N., Ohnishi, M., Ohoka, H., Ozawa, S., Sagawa, H., Shibata, T., Shimodaira, H., Takeda, M., Taketa, A., Takita, M., Tokuno, H., ... Kanbe, T. (2005). Telescope array; status and prospects. ： 29th International Cosmic Ray Conference, ICRC 2005 (巻 8, pp. 141-144). Tata Institute of Fundamental Research.

Telescope array; status and prospects. / Kawai, H.; Nunomura, T.; Sakurai, N.; Yoshida, S.; Yoshii, H.; Tanaka, K.; Cohen, F.; Fukushima, M.; Hayashida, N.; Ohnishi, M.; Ohoka, H.; Ozawa, Shunsuke; Sagawa, H.; Shibata, T.; Shimodaira, H.; Takeda, M.; Taketa, A.; Takita, M.; Tokuno, H.; Torii, R.; Udo, S.; Fujii, H.; Matsuda, T.; Tanaka, M.; Yamaoka, H.; Hibino, K.; Benno, T.; Chikawa, M.; Nakamura, T.; Teshima, M.; Kadota, K.; Uchihori, Y.; Hayashi, Y.; Matsumoto, K.; Matsumoto, Y.; Matsuyama, T.; Ogio, S.; Ohshima, A.; Okuda, T.; Bergman, D. R.; Hughes, G.; Stratton, S.; Thomson, G. B.; Inoue, N.; Wada, Y.; Kasahara, K.; Fukuda, M.; Iguchi, T.; Kakimoto, F.; Minagawa, R.; Tameda, Y.; Tsunesada, Y.; Belz, J. W.; Matthews, J. A J; Abu-Zayyad, T.; Cady, R.; Cao, Z.; Huentemeyer, P.; Jui, C. C H; Martens, K.; Matthews, J. N.; Smith, J. D.; Sokolsky, P.; Springer, R. W.; Thomas, S. B.; Wiencke, L. R.; Doyle, T.; Taylor, M. J.; Wickwar, V. B.; Wilkerson, T. D.; Hashimoto, K.; Honda, K.; Ishii, T.; Kanbe, T.

29th International Cosmic Ray Conference, ICRC 2005. 巻 8 Tata Institute of Fundamental Research, 2005. p. 141-144.

研究成果: Conference contribution

Kawai, H, Nunomura, T, Sakurai, N, Yoshida, S, Yoshii, H, Tanaka, K, Cohen, F, Fukushima, M, Hayashida, N, Ohnishi, M, Ohoka, H, Ozawa, S, Sagawa, H, Shibata, T, Shimodaira, H, Takeda, M, Taketa, A, Takita, M, Tokuno, H, Torii, R, Udo, S, Fujii, H, Matsuda, T, Tanaka, M, Yamaoka, H, Hibino, K, Benno, T, Chikawa, M, Nakamura, T, Teshima, M, Kadota, K, Uchihori, Y, Hayashi, Y, Matsumoto, K, Matsumoto, Y, Matsuyama, T, Ogio, S, Ohshima, A, Okuda, T, Bergman, DR, Hughes, G, Stratton, S, Thomson, GB, Inoue, N, Wada, Y, Kasahara, K, Fukuda, M, Iguchi, T, Kakimoto, F, Minagawa, R, Tameda, Y, Tsunesada, Y, Belz, JW, Matthews, JAJ, Abu-Zayyad, T, Cady, R, Cao, Z, Huentemeyer, P, Jui, CCH, Martens, K, Matthews, JN, Smith, JD, Sokolsky, P, Springer, RW, Thomas, SB, Wiencke, LR, Doyle, T, Taylor, MJ, Wickwar, VB, Wilkerson, TD, Hashimoto, K, Honda, K, Ishii, T & Kanbe, T 2005, Telescope array; status and prospects. ： 29th International Cosmic Ray Conference, ICRC 2005. 巻. 8, Tata Institute of Fundamental Research, pp. 141-144, 29th International Cosmic Ray Conference, ICRC 2005, Pune, India, 05/8/3.

Kawai, H. ; Nunomura, T. ; Sakurai, N. ; Yoshida, S. ; Yoshii, H. ; Tanaka, K. ; Cohen, F. ; Fukushima, M. ; Hayashida, N. ; Ohnishi, M. ; Ohoka, H. ; Ozawa, Shunsuke ; Sagawa, H. ; Shibata, T. ; Shimodaira, H. ; Takeda, M. ; Taketa, A. ; Takita, M. ; Tokuno, H. ; Torii, R. ; Udo, S. ; Fujii, H. ; Matsuda, T. ; Tanaka, M. ; Yamaoka, H. ; Hibino, K. ; Benno, T. ; Chikawa, M. ; Nakamura, T. ; Teshima, M. ; Kadota, K. ; Uchihori, Y. ; Hayashi, Y. ; Matsumoto, K. ; Matsumoto, Y. ; Matsuyama, T. ; Ogio, S. ; Ohshima, A. ; Okuda, T. ; Bergman, D. R. ; Hughes, G. ; Stratton, S. ; Thomson, G. B. ; Inoue, N. ; Wada, Y. ; Kasahara, K. ; Fukuda, M. ; Iguchi, T. ; Kakimoto, F. ; Minagawa, R. ; Tameda, Y. ; Tsunesada, Y. ; Belz, J. W. ; Matthews, J. A J ; Abu-Zayyad, T. ; Cady, R. ; Cao, Z. ; Huentemeyer, P. ; Jui, C. C H ; Martens, K. ; Matthews, J. N. ; Smith, J. D. ; Sokolsky, P. ; Springer, R. W. ; Thomas, S. B. ; Wiencke, L. R. ; Doyle, T. ; Taylor, M. J. ; Wickwar, V. B. ; Wilkerson, T. D. ; Hashimoto, K. ; Honda, K. ; Ishii, T. ; Kanbe, T. / Telescope array; status and prospects. 29th International Cosmic Ray Conference, ICRC 2005. 巻 8 Tata Institute of Fundamental Research, 2005. pp. 141-144

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title = "Telescope array; status and prospects",

abstract = "The Telescope Array (TA) is the air shower experiment designed for observing extremely high energy cosmic rays. It consists of an array of scintillation counters covering the ground area of 760 km2 and 3 sets of air fluorescence telescopes placed in the perimeter of the array. The TA aims at making a decisive measurement of the cosmic ray spectrum in the GZK cutoff region, and pinning down the nature of cosmic rays exceeding 10 20 eV, which have been the subject of extensive studies by AGASA, HiRes and other air shower experiments. The TA is being constructed in Utah, USA, and the commissioning is expected in the spring of 2007. An extension of hybrid measurement is planned down to 1017.5 eV in order to elucidate the galactic to extra-galactic transition of cosmic ray sources (TALE proposal).",

author = "H. Kawai and T. Nunomura and N. Sakurai and S. Yoshida and H. Yoshii and K. Tanaka and F. Cohen and M. Fukushima and N. Hayashida and M. Ohnishi and H. Ohoka and Shunsuke Ozawa and H. Sagawa and T. Shibata and H. Shimodaira and M. Takeda and A. Taketa and M. Takita and H. Tokuno and R. Torii and S. Udo and H. Fujii and T. Matsuda and M. Tanaka and H. Yamaoka and K. Hibino and T. Benno and M. Chikawa and T. Nakamura and M. Teshima and K. Kadota and Y. Uchihori and Y. Hayashi and K. Matsumoto and Y. Matsumoto and T. Matsuyama and S. Ogio and A. Ohshima and T. Okuda and Bergman, {D. R.} and G. Hughes and S. Stratton and Thomson, {G. B.} and N. Inoue and Y. Wada and K. Kasahara and M. Fukuda and T. Iguchi and F. Kakimoto and R. Minagawa and Y. Tameda and Y. Tsunesada and Belz, {J. W.} and Matthews, {J. A J} and T. Abu-Zayyad and R. Cady and Z. Cao and P. Huentemeyer and Jui, {C. C H} and K. Martens and Matthews, {J. N.} and Smith, {J. D.} and P. Sokolsky and Springer, {R. W.} and Thomas, {S. B.} and Wiencke, {L. R.} and T. Doyle and Taylor, {M. J.} and Wickwar, {V. B.} and Wilkerson, {T. D.} and K. Hashimoto and K. Honda and T. Ishii and T. Kanbe",

year = "2005",

language = "English",

volume = "8",

pages = "141--144",

booktitle = "29th International Cosmic Ray Conference, ICRC 2005",

publisher = "Tata Institute of Fundamental Research",

note = "29th International Cosmic Ray Conference, ICRC 2005 ; Conference date: 03-08-2005 Through 10-08-2005",

}

TY - GEN

T1 - Telescope array; status and prospects

AU - Kawai, H.

AU - Nunomura, T.

AU - Sakurai, N.

AU - Yoshida, S.

AU - Yoshii, H.

AU - Tanaka, K.

AU - Cohen, F.

AU - Fukushima, M.

AU - Hayashida, N.

AU - Ohnishi, M.

AU - Ohoka, H.

AU - Ozawa, Shunsuke

AU - Sagawa, H.

AU - Shibata, T.

AU - Shimodaira, H.

AU - Takeda, M.

AU - Taketa, A.

AU - Takita, M.

AU - Tokuno, H.

AU - Torii, R.

AU - Udo, S.

AU - Fujii, H.

AU - Matsuda, T.

AU - Tanaka, M.

AU - Yamaoka, H.

AU - Hibino, K.

AU - Benno, T.

AU - Chikawa, M.

AU - Nakamura, T.

AU - Teshima, M.

AU - Kadota, K.

AU - Uchihori, Y.

AU - Hayashi, Y.

AU - Matsumoto, K.

AU - Matsumoto, Y.

AU - Matsuyama, T.

AU - Ogio, S.

AU - Ohshima, A.

AU - Okuda, T.

AU - Bergman, D. R.

AU - Hughes, G.

AU - Stratton, S.

AU - Thomson, G. B.

AU - Inoue, N.

AU - Wada, Y.

AU - Kasahara, K.

AU - Fukuda, M.

AU - Iguchi, T.

AU - Kakimoto, F.

AU - Minagawa, R.

AU - Tameda, Y.

AU - Tsunesada, Y.

AU - Belz, J. W.

AU - Matthews, J. A J

AU - Abu-Zayyad, T.

AU - Cady, R.

AU - Cao, Z.

AU - Huentemeyer, P.

AU - Jui, C. C H

AU - Martens, K.

AU - Matthews, J. N.

AU - Smith, J. D.

AU - Sokolsky, P.

AU - Springer, R. W.

AU - Thomas, S. B.

AU - Wiencke, L. R.

AU - Doyle, T.

AU - Taylor, M. J.

AU - Wickwar, V. B.

AU - Wilkerson, T. D.

AU - Hashimoto, K.

AU - Honda, K.

AU - Ishii, T.

AU - Kanbe, T.

PY - 2005

Y1 - 2005

N2 - The Telescope Array (TA) is the air shower experiment designed for observing extremely high energy cosmic rays. It consists of an array of scintillation counters covering the ground area of 760 km2 and 3 sets of air fluorescence telescopes placed in the perimeter of the array. The TA aims at making a decisive measurement of the cosmic ray spectrum in the GZK cutoff region, and pinning down the nature of cosmic rays exceeding 10 20 eV, which have been the subject of extensive studies by AGASA, HiRes and other air shower experiments. The TA is being constructed in Utah, USA, and the commissioning is expected in the spring of 2007. An extension of hybrid measurement is planned down to 1017.5 eV in order to elucidate the galactic to extra-galactic transition of cosmic ray sources (TALE proposal).

AB - The Telescope Array (TA) is the air shower experiment designed for observing extremely high energy cosmic rays. It consists of an array of scintillation counters covering the ground area of 760 km2 and 3 sets of air fluorescence telescopes placed in the perimeter of the array. The TA aims at making a decisive measurement of the cosmic ray spectrum in the GZK cutoff region, and pinning down the nature of cosmic rays exceeding 10 20 eV, which have been the subject of extensive studies by AGASA, HiRes and other air shower experiments. The TA is being constructed in Utah, USA, and the commissioning is expected in the spring of 2007. An extension of hybrid measurement is planned down to 1017.5 eV in order to elucidate the galactic to extra-galactic transition of cosmic ray sources (TALE proposal).

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UR - http://www.scopus.com/inward/citedby.url?scp=74949137782&partnerID=8YFLogxK

M3 - Conference contribution

AN - SCOPUS:74949137782

VL - 8

SP - 141

EP - 144

BT - 29th International Cosmic Ray Conference, ICRC 2005

PB - Tata Institute of Fundamental Research

T2 - 29th International Cosmic Ray Conference, ICRC 2005

Y2 - 3 August 2005 through 10 August 2005

ER -