The present status of the Telescope Array experiment

T. Nonaka; T. Abu-Zayyad; M. Allen; R. Azuma; J. W. Belz; D. R. Bergman; S. A. Blake; O. Brusova; R. Cady; Z. Cao; J. Chiba; M. Chikawa; I. S. Cho; H. Fujii; T. Fujii; T. Fukuda; M. Fukushima; K. Hayashi; N. Hayashida; K. Hibino; K. Honda; P. Huentemeyer; G. Hughes; D. Ikeda; N. Inoue; D. Ivanov; S. Iwamoto; C. H. Jui; K. Kadota; F. Kakimoto; H. Kang; K. Kasahara; H. Kawai; S. Kawana; E. Kido; A. Kitshugi; K. Kobayashi; Y. Kondo; Y. J. Kwon; K. Martens; T. Matsuda; J. N. Matthews; T. Nakamura; S. Nam; S. Ogio; H. Ohoka; T. Okuda; M. Ohnishi; A. Oshima; Shunsuke Ozawa; I. H. Park; D. Rodriguez; D. Ryu; H. Sagawa; N. Sakurai; L. Scott; P. Shah; T. Shibata; H. Shimodaira; J. D. Smith; P. Sokolsky; R. W. Springer; S. Stratton; M. Takeda; A. Taketa; M. Takita; Y. Tameda; K. Tanaka; M. Tanaka; M. Teshima; S. B. Thomas; G. B. Thomson; H. Tokuno; T. Tomida; R. Torii; Y. Tsunesada; Y. Tsuyuguchi; Y. Uchihori; S. Udo; L. R. Wiencke; T. Yamakawa; Y. Yamakawa; K. Yamamoto; J. Yang; S. Yoshida; N. Yoshii

doi:10.1016/j.nuclphysbps.2009.03.064

The present status of the Telescope Array experiment

T. Nonaka^*, T. Abu-Zayyad, M. Allen, R. Azuma, J. W. Belz, D. R. Bergman, S. A. Blake, O. Brusova, R. Cady, Z. Cao, J. Chiba, M. Chikawa, I. S. Cho, H. Fujii, T. Fujii, T. Fukuda, M. Fukushima, K. Hayashi, N. Hayashida, K. HibinoK. Honda, P. Huentemeyer, G. Hughes, D. Ikeda, N. Inoue, D. Ivanov, S. Iwamoto, C. H. Jui, K. Kadota, F. Kakimoto, H. Kang, K. Kasahara, H. Kawai, S. Kawana, E. Kido, A. Kitshugi, K. Kobayashi, Y. Kondo, Y. J. Kwon, K. Martens, T. Matsuda, J. N. Matthews, T. Nakamura, S. Nam, S. Ogio, H. Ohoka, T. Okuda, M. Ohnishi, A. Oshima, Shunsuke Ozawa, I. H. Park, D. Rodriguez, D. Ryu, H. Sagawa, N. Sakurai, L. Scott, P. Shah, T. Shibata, H. Shimodaira, J. D. Smith, P. Sokolsky, R. W. Springer, S. Stratton, M. Takeda, A. Taketa, M. Takita, Y. Tameda, K. Tanaka, M. Tanaka, M. Teshima, S. B. Thomas, G. B. Thomson, H. Tokuno, T. Tomida, R. Torii, Y. Tsunesada, Y. Tsuyuguchi, Y. Uchihori, S. Udo, L. R. Wiencke, T. Yamakawa, Y. Yamakawa, K. Yamamoto, J. Yang, S. Yoshida, N. Yoshii

^*Corresponding author for this work

Waseda Research Institute for Science and Engineering

Research output: Contribution to journal › Article › peer-review

8 Citations (Scopus)

Abstract

The Telescope Array(TA) experiment located at western desert in Utah USA (N39.3,W112.9) is designed for observation of air shower from extreme high energy cosmic rays. The TA detector consists of 2 types of detector to enable a cross check on systematic difference from the two main methods of observation for the energy region. One is a Fluorescence detector (FD) for detecting fluorescence light from air shower and another is surface detector (SD) array for detecting air shower particles at ground level. Each SD consists of 2 layers of plastic scintillator with 3m² of surface and more sensitive to electromagnetic component in air shower. The full operation using 3FD stations and full SD array has started. Here we present the updated status of Telescope Array experiment.

Original language	English
Pages (from-to)	26-31
Number of pages	6
Journal	Nuclear Physics B - Proceedings Supplements
Volume	190
Issue number	C
DOIs	https://doi.org/10.1016/j.nuclphysbps.2009.03.064
Publication status	Published - 2009 May

ASJC Scopus subject areas

Nuclear and High Energy Physics

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10.1016/j.nuclphysbps.2009.03.064

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Nonaka, T., Abu-Zayyad, T., Allen, M., Azuma, R., Belz, J. W., Bergman, D. R., Blake, S. A., Brusova, O., Cady, R., Cao, Z., Chiba, J., Chikawa, M., Cho, I. S., Fujii, H., Fujii, T., Fukuda, T., Fukushima, M., Hayashi, K., Hayashida, N., ... Yoshii, N. (2009). The present status of the Telescope Array experiment. Nuclear Physics B - Proceedings Supplements, 190(C), 26-31. https://doi.org/10.1016/j.nuclphysbps.2009.03.064

Nonaka, T, Abu-Zayyad, T, Allen, M, Azuma, R, Belz, JW, Bergman, DR, Blake, SA, Brusova, O, Cady, R, Cao, Z, Chiba, J, Chikawa, M, Cho, IS, Fujii, H, Fujii, T, Fukuda, T, Fukushima, M, Hayashi, K, Hayashida, N, Hibino, K, Honda, K, Huentemeyer, P, Hughes, G, Ikeda, D, Inoue, N, Ivanov, D, Iwamoto, S, Jui, CH, Kadota, K, Kakimoto, F, Kang, H, Kasahara, K, Kawai, H, Kawana, S, Kido, E, Kitshugi, A, Kobayashi, K, Kondo, Y, Kwon, YJ, Martens, K, Matsuda, T, Matthews, JN, Nakamura, T, Nam, S, Ogio, S, Ohoka, H, Okuda, T, Ohnishi, M, Oshima, A, Ozawa, S, Park, IH, Rodriguez, D, Ryu, D, Sagawa, H, Sakurai, N, Scott, L, Shah, P, Shibata, T, Shimodaira, H, Smith, JD, Sokolsky, P, Springer, RW, Stratton, S, Takeda, M, Taketa, A, Takita, M, Tameda, Y, Tanaka, K, Tanaka, M, Teshima, M, Thomas, SB, Thomson, GB, Tokuno, H, Tomida, T, Torii, R, Tsunesada, Y, Tsuyuguchi, Y, Uchihori, Y, Udo, S, Wiencke, LR, Yamakawa, T, Yamakawa, Y, Yamamoto, K, Yang, J, Yoshida, S & Yoshii, N 2009, 'The present status of the Telescope Array experiment', Nuclear Physics B - Proceedings Supplements, vol. 190, no. C, pp. 26-31. https://doi.org/10.1016/j.nuclphysbps.2009.03.064

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title = "The present status of the Telescope Array experiment",

abstract = "The Telescope Array(TA) experiment located at western desert in Utah USA (N39.3,W112.9) is designed for observation of air shower from extreme high energy cosmic rays. The TA detector consists of 2 types of detector to enable a cross check on systematic difference from the two main methods of observation for the energy region. One is a Fluorescence detector (FD) for detecting fluorescence light from air shower and another is surface detector (SD) array for detecting air shower particles at ground level. Each SD consists of 2 layers of plastic scintillator with 3m2 of surface and more sensitive to electromagnetic component in air shower. The full operation using 3FD stations and full SD array has started. Here we present the updated status of Telescope Array experiment.",

author = "T. Nonaka and T. Abu-Zayyad and M. Allen and R. Azuma and Belz, {J. W.} and Bergman, {D. R.} and Blake, {S. A.} and O. Brusova and R. Cady and Z. Cao and J. Chiba and M. Chikawa and Cho, {I. S.} and H. Fujii and T. Fujii and T. Fukuda and M. Fukushima and K. Hayashi and N. Hayashida and K. Hibino and K. Honda and P. Huentemeyer and G. Hughes and D. Ikeda and N. Inoue and D. Ivanov and S. Iwamoto and Jui, {C. H.} and K. Kadota and F. Kakimoto and H. Kang and K. Kasahara and H. Kawai and S. Kawana and E. Kido and A. Kitshugi and K. Kobayashi and Y. Kondo and Kwon, {Y. J.} and K. Martens and T. Matsuda and Matthews, {J. N.} and T. Nakamura and S. Nam and S. Ogio and H. Ohoka and T. Okuda and M. Ohnishi and A. Oshima and Shunsuke Ozawa and Park, {I. H.} and D. Rodriguez and D. Ryu and H. Sagawa and N. Sakurai and L. Scott and P. Shah and T. Shibata and H. Shimodaira and Smith, {J. D.} and P. Sokolsky and Springer, {R. W.} and S. Stratton and M. Takeda and A. Taketa and M. Takita and Y. Tameda and K. Tanaka and M. Tanaka and M. Teshima and Thomas, {S. B.} and Thomson, {G. B.} and H. Tokuno and T. Tomida and R. Torii and Y. Tsunesada and Y. Tsuyuguchi and Y. Uchihori and S. Udo and Wiencke, {L. R.} and T. Yamakawa and Y. Yamakawa and K. Yamamoto and J. Yang and S. Yoshida and N. Yoshii",

year = "2009",

month = may,

doi = "10.1016/j.nuclphysbps.2009.03.064",

language = "English",

volume = "190",

pages = "26--31",

journal = "Nuclear Physics B - Proceedings Supplements",

issn = "0920-5632",

publisher = "Elsevier",

number = "C",

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TY - JOUR

T1 - The present status of the Telescope Array experiment

AU - Nonaka, T.

AU - Abu-Zayyad, T.

AU - Allen, M.

AU - Azuma, R.

AU - Belz, J. W.

AU - Bergman, D. R.

AU - Blake, S. A.

AU - Brusova, O.

AU - Cady, R.

AU - Cao, Z.

AU - Chiba, J.

AU - Chikawa, M.

AU - Cho, I. S.

AU - Fujii, H.

AU - Fujii, T.

AU - Fukuda, T.

AU - Fukushima, M.

AU - Hayashi, K.

AU - Hayashida, N.

AU - Hibino, K.

AU - Honda, K.

AU - Huentemeyer, P.

AU - Hughes, G.

AU - Ikeda, D.

AU - Inoue, N.

AU - Ivanov, D.

AU - Iwamoto, S.

AU - Jui, C. H.

AU - Kadota, K.

AU - Kakimoto, F.

AU - Kang, H.

AU - Kasahara, K.

AU - Kawai, H.

AU - Kawana, S.

AU - Kido, E.

AU - Kitshugi, A.

AU - Kobayashi, K.

AU - Kondo, Y.

AU - Kwon, Y. J.

AU - Martens, K.

AU - Matsuda, T.

AU - Matthews, J. N.

AU - Nakamura, T.

AU - Nam, S.

AU - Ogio, S.

AU - Ohoka, H.

AU - Okuda, T.

AU - Ohnishi, M.

AU - Oshima, A.

AU - Ozawa, Shunsuke

AU - Park, I. H.

AU - Rodriguez, D.

AU - Ryu, D.

AU - Sagawa, H.

AU - Sakurai, N.

AU - Scott, L.

AU - Shah, P.

AU - Shibata, T.

AU - Shimodaira, H.

AU - Smith, J. D.

AU - Sokolsky, P.

AU - Springer, R. W.

AU - Stratton, S.

AU - Takeda, M.

AU - Taketa, A.

AU - Takita, M.

AU - Tameda, Y.

AU - Tanaka, K.

AU - Tanaka, M.

AU - Teshima, M.

AU - Thomas, S. B.

AU - Thomson, G. B.

AU - Tokuno, H.

AU - Tomida, T.

AU - Torii, R.

AU - Tsunesada, Y.

AU - Tsuyuguchi, Y.

AU - Uchihori, Y.

AU - Udo, S.

AU - Wiencke, L. R.

AU - Yamakawa, T.

AU - Yamakawa, Y.

AU - Yamamoto, K.

AU - Yang, J.

AU - Yoshida, S.

AU - Yoshii, N.

PY - 2009/5

Y1 - 2009/5

N2 - The Telescope Array(TA) experiment located at western desert in Utah USA (N39.3,W112.9) is designed for observation of air shower from extreme high energy cosmic rays. The TA detector consists of 2 types of detector to enable a cross check on systematic difference from the two main methods of observation for the energy region. One is a Fluorescence detector (FD) for detecting fluorescence light from air shower and another is surface detector (SD) array for detecting air shower particles at ground level. Each SD consists of 2 layers of plastic scintillator with 3m2 of surface and more sensitive to electromagnetic component in air shower. The full operation using 3FD stations and full SD array has started. Here we present the updated status of Telescope Array experiment.

AB - The Telescope Array(TA) experiment located at western desert in Utah USA (N39.3,W112.9) is designed for observation of air shower from extreme high energy cosmic rays. The TA detector consists of 2 types of detector to enable a cross check on systematic difference from the two main methods of observation for the energy region. One is a Fluorescence detector (FD) for detecting fluorescence light from air shower and another is surface detector (SD) array for detecting air shower particles at ground level. Each SD consists of 2 layers of plastic scintillator with 3m2 of surface and more sensitive to electromagnetic component in air shower. The full operation using 3FD stations and full SD array has started. Here we present the updated status of Telescope Array experiment.

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U2 - 10.1016/j.nuclphysbps.2009.03.064

DO - 10.1016/j.nuclphysbps.2009.03.064

M3 - Article

AN - SCOPUS:65649129298

SN - 0920-5632

VL - 190

SP - 26

EP - 31

JO - Nuclear Physics B - Proceedings Supplements

JF - Nuclear Physics B - Proceedings Supplements

IS - C

ER -

The present status of the Telescope Array experiment

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