Energy spectrum of ultra-high energy cosmic rays observed with the Telescope Array using a hybrid technique

T. Abu-Zayyad; R. Aida; M. Allen; R. Anderson; R. Azuma; E. Barcikowski; J. W. Belz; D. R. Bergman; S. A. Blake; R. Cady; B. G. Cheon; J. Chiba; M. Chikawa; E. J. Cho; W. R. Cho; H. Fujii; T. Fujii; T. Fukuda; M. Fukushima; W. Hanlon; K. Hayashi; Y. Hayashi; N. Hayashida; K. Hibino; K. Hiyama; K. Honda; T. Iguchi; D. Ikeda; K. Ikuta; N. Inoue; T. Ishii; R. Ishimori; H. Ito; D. Ivanov; S. Iwamoto; C. C.H. Jui; K. Kadota; F. Kakimoto; O. Kalashev; T. Kanbe; K. Kasahara; H. Kawai; S. Kawakami; S. Kawana; E. Kido; H. B. Kim; H. K. Kim; J. H. Kim; J. H. Kim; K. Kitamoto; S. Kitamura; Y. Kitamura; K. Kobayashi; Y. Kobayashi; Y. Kondo; K. Kuramoto; V. Kuzmin; Y. J. Kwon; J. Lan; S. I. Lim; J. P. Lundquist; S. Machida; K. Martens; T. Matsuda; T. Matsuura; T. Matsuyama; J. N. Matthews; M. Minamino; K. Miyata; Y. Murano; I. Myers; K. Nagasawa; S. Nagataki; T. Nakamura; S. W. Nam; T. Nonaka; S. Ogio; M. Ohnishi; H. Ohoka; K. Oki; D. Oku; T. Okuda; M. Ono; A. Oshima; S. Ozawa; I. H. Park; M. S. Pshirkov; D. C. Rodriguez; S. Y. Roh; G. Rubtsov; D. Ryu; H. Sagawa; N. Sakurai; A. L. Sampson; L. M. Scott; P. D. Shah; F. Shibata; T. Shibata; H. Shimodaira; B. K. Shin; J. I. Shin; T. Shirahama; J. D. Smith; P. Sokolsky; R. W. Springer; B. T. Stokes; S. R. Stratton; T. Stroman; S. Suzuki; Y. Takahashi; M. Takeda; A. Taketa; M. Takita; Y. Tameda; H. Tanaka; K. Tanaka; M. Tanaka; S. B. Thomas; G. B. Thomson; P. Tinyakov; I. Tkachev; H. Tokuno; T. Tomida; S. Troitsky; Y. Tsunesada; K. Tsutsumi; Y. Tsuyuguchi; Y. Uchihori; S. Udo; H. Ukai; F. Urban; G. Vasiloff; Y. Wada; T. Wong; Y. Yamakawa; R. Yamane; H. Yamaoka; K. Yamazaki; J. Yang; Y. Yoneda; S. Yoshida; H. Yoshii; X. Zhou; R. Zollinger; Z. Zundel

doi:10.1016/j.astropartphys.2014.05.002

Energy spectrum of ultra-high energy cosmic rays observed with the Telescope Array using a hybrid technique

T. Abu-Zayyad, R. Aida, M. Allen, R. Anderson, R. Azuma, E. Barcikowski, J. W. Belz, D. R. Bergman, S. A. Blake, R. Cady, B. G. Cheon, J. Chiba, M. Chikawa, E. J. Cho, W. R. Cho, H. Fujii, T. Fujii, T. Fukuda, M. Fukushima, W. HanlonK. Hayashi, Y. Hayashi, N. Hayashida, K. Hibino, K. Hiyama, K. Honda, T. Iguchi, D. Ikeda, K. Ikuta, N. Inoue, T. Ishii, R. Ishimori, H. Ito, D. Ivanov, S. Iwamoto, C. C.H. Jui, K. Kadota, F. Kakimoto, O. Kalashev, T. Kanbe, K. Kasahara, H. Kawai, S. Kawakami, S. Kawana, E. Kido, H. B. Kim, H. K. Kim, J. H. Kim, J. H. Kim, K. Kitamoto, S. Kitamura, Y. Kitamura, K. Kobayashi, Y. Kobayashi, Y. Kondo, K. Kuramoto, V. Kuzmin, Y. J. Kwon, J. Lan, S. I. Lim, J. P. Lundquist, S. Machida, K. Martens, T. Matsuda, T. Matsuura, T. Matsuyama, J. N. Matthews, M. Minamino, K. Miyata, Y. Murano, I. Myers, K. Nagasawa, S. Nagataki, T. Nakamura, S. W. Nam, T. Nonaka, S. Ogio, M. Ohnishi, H. Ohoka, K. Oki, D. Oku, T. Okuda, M. Ono, A. Oshima, S. Ozawa, I. H. Park, M. S. Pshirkov, D. C. Rodriguez, S. Y. Roh, G. Rubtsov, D. Ryu, H. Sagawa, N. Sakurai, A. L. Sampson, L. M. Scott, P. D. Shah, F. Shibata, T. Shibata, H. Shimodaira, B. K. Shin, J. I. Shin, T. Shirahama, J. D. Smith, P. Sokolsky, R. W. Springer, B. T. Stokes, S. R. Stratton, T. Stroman, S. Suzuki, Y. Takahashi, M. Takeda, A. Taketa, M. Takita, Y. Tameda, H. Tanaka, K. Tanaka, M. Tanaka, S. B. Thomas, G. B. Thomson, P. Tinyakov, I. Tkachev, H. Tokuno, T. Tomida, S. Troitsky, Y. Tsunesada, K. Tsutsumi, Y. Tsuyuguchi, Y. Uchihori, S. Udo, H. Ukai, F. Urban, G. Vasiloff, Y. Wada, T. Wong, Y. Yamakawa, R. Yamane, H. Yamaoka, K. Yamazaki, J. Yang, Y. Yoneda, S. Yoshida, H. Yoshii, X. Zhou, R. Zollinger, Z. Zundel

Department of Physics

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48 Citations (Scopus)

Abstract

We measure the spectrum of cosmic rays with energies greater than 10 ^18.2 eV with the fluorescence detectors (FDs) and the surface detectors (SDs) of the Telescope Array Experiment using the data taken in our first 2.3-year observation from May 27, 2008 to September 7, 2010. A hybrid air shower reconstruction technique is employed to improve accuracies in determination of arrival directions and primary energies of cosmic rays using both FD and SD data. The energy spectrum presented here is in agreement with our previously published spectra and the HiRes results.

Original language	English
Pages (from-to)	93-101
Number of pages	9
Journal	Astroparticle Physics
Volume	61
DOIs	https://doi.org/10.1016/j.astropartphys.2014.05.002
Publication status	Published - 2015 Feb

Bibliographical note

Funding Information:
The Telescope Array Experiment is supported by the Japan Society for the Promotion of Science through Grants-in-Aid for Scientific Research on Specially Promoted Research (21000002) “Extreme Phenomena in the Universe Explored by Highest Energy Cosmic Rays”, and the Inter-University Research Program of the Institute for Cosmic Ray Research; by the U.S. National Science Foundation awards PHY-0307098, PHY-0601915, PHY-0703893, PHY-0758342, PHY-0848320, PHY-1069280, and PHY-1069286 (Utah) and PHY-0649681 (Rutgers); by the National Research Foundation of Korea ( 2006-0050031 , 2007-0056005 , 2007-0093860 , 2010-0011378 , 2010-0028071 , R32-10130 ); by the Russian Academy of Sciences , RFBR Grants 10-02-01406a and 11-02-01528a (INR), IISN project No. 4.4509.10 and Belgian Science Policy under IUAP VI/11 (ULB). The foundations of Dr. Ezekiel R. and Edna Wattis Dumke, Willard L. Eccles and the George S. and Dolores Dore Eccles all helped with generous donations. The State of Utah supported the project through its Economic Development Board, and the University of Utah through the Office of the Vice President for Research. The experimental site became available through the cooperation of the Utah School and Institutional Trust Lands Administration (SITLA), U.S. Bureau of Land Management and the U.S. Air Force. We also wish to thank the people and the officials of Millard County, Utah, for their steadfast and warm support. We gratefully acknowledge the contributions from the technical staffs of our home institutions as well as the University of Utah Center for High Performance Computing (CHPC).

All Science Journal Classification (ASJC) codes

Astronomy and Astrophysics

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10.1016/j.astropartphys.2014.05.002

Cite this

Abu-Zayyad, T., Aida, R., Allen, M., Anderson, R., Azuma, R., Barcikowski, E., Belz, J. W., Bergman, D. R., Blake, S. A., Cady, R., Cheon, B. G., Chiba, J., Chikawa, M., Cho, E. J., Cho, W. R., Fujii, H., Fujii, T., Fukuda, T., Fukushima, M., ... Zundel, Z. (2015). Energy spectrum of ultra-high energy cosmic rays observed with the Telescope Array using a hybrid technique. Astroparticle Physics, 61, 93-101. https://doi.org/10.1016/j.astropartphys.2014.05.002

@article{a51a67f607f54e2680461db49cbb433b,

title = "Energy spectrum of ultra-high energy cosmic rays observed with the Telescope Array using a hybrid technique",

abstract = "We measure the spectrum of cosmic rays with energies greater than 10 18.2 eV with the fluorescence detectors (FDs) and the surface detectors (SDs) of the Telescope Array Experiment using the data taken in our first 2.3-year observation from May 27, 2008 to September 7, 2010. A hybrid air shower reconstruction technique is employed to improve accuracies in determination of arrival directions and primary energies of cosmic rays using both FD and SD data. The energy spectrum presented here is in agreement with our previously published spectra and the HiRes results.",

author = "T. Abu-Zayyad and R. Aida and M. Allen and R. Anderson and R. Azuma and E. Barcikowski and Belz, {J. W.} and Bergman, {D. R.} and Blake, {S. A.} and R. Cady and Cheon, {B. G.} and J. Chiba and M. Chikawa and Cho, {E. J.} and Cho, {W. R.} and H. Fujii and T. Fujii and T. Fukuda and M. Fukushima and W. Hanlon and K. Hayashi and Y. Hayashi and N. Hayashida and K. Hibino and K. Hiyama and K. Honda and T. Iguchi and D. Ikeda and K. Ikuta and N. Inoue and T. Ishii and R. Ishimori and H. Ito and D. Ivanov and S. Iwamoto and Jui, {C. C.H.} and K. Kadota and F. Kakimoto and O. Kalashev and T. Kanbe and K. Kasahara and H. Kawai and S. Kawakami and S. Kawana and E. Kido and Kim, {H. B.} and Kim, {H. K.} and Kim, {J. H.} and Kim, {J. H.} and K. Kitamoto and S. Kitamura and Y. Kitamura and K. Kobayashi and Y. Kobayashi and Y. Kondo and K. Kuramoto and V. Kuzmin and Kwon, {Y. J.} and J. Lan and Lim, {S. I.} and Lundquist, {J. P.} and S. Machida and K. Martens and T. Matsuda and T. Matsuura and T. Matsuyama and Matthews, {J. N.} and M. Minamino and K. Miyata and Y. Murano and I. Myers and K. Nagasawa and S. Nagataki and T. Nakamura and Nam, {S. W.} and T. Nonaka and S. Ogio and M. Ohnishi and H. Ohoka and K. Oki and D. Oku and T. Okuda and M. Ono and A. Oshima and S. Ozawa and Park, {I. H.} and Pshirkov, {M. S.} and Rodriguez, {D. C.} and Roh, {S. Y.} and G. Rubtsov and D. Ryu and H. Sagawa and N. Sakurai and Sampson, {A. L.} and Scott, {L. M.} and Shah, {P. D.} and F. Shibata and T. Shibata and H. Shimodaira and Shin, {B. K.} and Shin, {J. I.} and T. Shirahama and Smith, {J. D.} and P. Sokolsky and Springer, {R. W.} and Stokes, {B. T.} and Stratton, {S. R.} and T. Stroman and S. Suzuki and Y. Takahashi and M. Takeda and A. Taketa and M. Takita and Y. Tameda and H. Tanaka and K. Tanaka and M. Tanaka and Thomas, {S. B.} and Thomson, {G. B.} and P. Tinyakov and I. Tkachev and H. Tokuno and T. Tomida and S. Troitsky and Y. Tsunesada and K. Tsutsumi and Y. Tsuyuguchi and Y. Uchihori and S. Udo and H. Ukai and F. Urban and G. Vasiloff and Y. Wada and T. Wong and Y. Yamakawa and R. Yamane and H. Yamaoka and K. Yamazaki and J. Yang and Y. Yoneda and S. Yoshida and H. Yoshii and X. Zhou and R. Zollinger and Z. Zundel",

note = "Funding Information: The Telescope Array Experiment is supported by the Japan Society for the Promotion of Science through Grants-in-Aid for Scientific Research on Specially Promoted Research (21000002) “Extreme Phenomena in the Universe Explored by Highest Energy Cosmic Rays”, and the Inter-University Research Program of the Institute for Cosmic Ray Research; by the U.S. National Science Foundation awards PHY-0307098, PHY-0601915, PHY-0703893, PHY-0758342, PHY-0848320, PHY-1069280, and PHY-1069286 (Utah) and PHY-0649681 (Rutgers); by the National Research Foundation of Korea ( 2006-0050031 , 2007-0056005 , 2007-0093860 , 2010-0011378 , 2010-0028071 , R32-10130 ); by the Russian Academy of Sciences , RFBR Grants 10-02-01406a and 11-02-01528a (INR), IISN project No. 4.4509.10 and Belgian Science Policy under IUAP VI/11 (ULB). The foundations of Dr. Ezekiel R. and Edna Wattis Dumke, Willard L. Eccles and the George S. and Dolores Dore Eccles all helped with generous donations. The State of Utah supported the project through its Economic Development Board, and the University of Utah through the Office of the Vice President for Research. The experimental site became available through the cooperation of the Utah School and Institutional Trust Lands Administration (SITLA), U.S. Bureau of Land Management and the U.S. Air Force. We also wish to thank the people and the officials of Millard County, Utah, for their steadfast and warm support. We gratefully acknowledge the contributions from the technical staffs of our home institutions as well as the University of Utah Center for High Performance Computing (CHPC). ",

year = "2015",

month = feb,

doi = "10.1016/j.astropartphys.2014.05.002",

language = "English",

volume = "61",

pages = "93--101",

journal = "Astroparticle Physics",

issn = "0927-6505",

publisher = "Elsevier",

}

Abu-Zayyad, T, Aida, R, Allen, M, Anderson, R, Azuma, R, Barcikowski, E, Belz, JW, Bergman, DR, Blake, SA, Cady, R, Cheon, BG, Chiba, J, Chikawa, M, Cho, EJ, Cho, WR, Fujii, H, Fujii, T, Fukuda, T, Fukushima, M, Hanlon, W, Hayashi, K, Hayashi, Y, Hayashida, N, Hibino, K, Hiyama, K, Honda, K, Iguchi, T, Ikeda, D, Ikuta, K, Inoue, N, Ishii, T, Ishimori, R, Ito, H, Ivanov, D, Iwamoto, S, Jui, CCH, Kadota, K, Kakimoto, F, Kalashev, O, Kanbe, T, Kasahara, K, Kawai, H, Kawakami, S, Kawana, S, Kido, E, Kim, HB, Kim, HK, Kim, JH, Kim, JH, Kitamoto, K, Kitamura, S, Kitamura, Y, Kobayashi, K, Kobayashi, Y, Kondo, Y, Kuramoto, K, Kuzmin, V, Kwon, YJ, Lan, J, Lim, SI, Lundquist, JP, Machida, S, Martens, K, Matsuda, T, Matsuura, T, Matsuyama, T, Matthews, JN, Minamino, M, Miyata, K, Murano, Y, Myers, I, Nagasawa, K, Nagataki, S, Nakamura, T, Nam, SW, Nonaka, T, Ogio, S, Ohnishi, M, Ohoka, H, Oki, K, Oku, D, Okuda, T, Ono, M, Oshima, A, Ozawa, S, Park, IH, Pshirkov, MS, Rodriguez, DC, Roh, SY, Rubtsov, G, Ryu, D, Sagawa, H, Sakurai, N, Sampson, AL, Scott, LM, Shah, PD, Shibata, F, Shibata, T, Shimodaira, H, Shin, BK, Shin, JI, Shirahama, T, Smith, JD, Sokolsky, P, Springer, RW, Stokes, BT, Stratton, SR, Stroman, T, Suzuki, S, Takahashi, Y, Takeda, M, Taketa, A, Takita, M, Tameda, Y, Tanaka, H, Tanaka, K, Tanaka, M, Thomas, SB, Thomson, GB, Tinyakov, P, Tkachev, I, Tokuno, H, Tomida, T, Troitsky, S, Tsunesada, Y, Tsutsumi, K, Tsuyuguchi, Y, Uchihori, Y, Udo, S, Ukai, H, Urban, F, Vasiloff, G, Wada, Y, Wong, T, Yamakawa, Y, Yamane, R, Yamaoka, H, Yamazaki, K, Yang, J, Yoneda, Y, Yoshida, S, Yoshii, H, Zhou, X, Zollinger, R & Zundel, Z 2015, 'Energy spectrum of ultra-high energy cosmic rays observed with the Telescope Array using a hybrid technique', Astroparticle Physics, vol. 61, pp. 93-101. https://doi.org/10.1016/j.astropartphys.2014.05.002

TY - JOUR

T1 - Energy spectrum of ultra-high energy cosmic rays observed with the Telescope Array using a hybrid technique

AU - Abu-Zayyad, T.

AU - Aida, R.

AU - Allen, M.

AU - Anderson, R.

AU - Azuma, R.

AU - Barcikowski, E.

AU - Belz, J. W.

AU - Bergman, D. R.

AU - Blake, S. A.

AU - Cady, R.

AU - Cheon, B. G.

AU - Chiba, J.

AU - Chikawa, M.

AU - Cho, E. J.

AU - Cho, W. R.

AU - Fujii, H.

AU - Fujii, T.

AU - Fukuda, T.

AU - Fukushima, M.

AU - Hanlon, W.

AU - Hayashi, K.

AU - Hayashi, Y.

AU - Hayashida, N.

AU - Hibino, K.

AU - Hiyama, K.

AU - Honda, K.

AU - Iguchi, T.

AU - Ikeda, D.

AU - Ikuta, K.

AU - Inoue, N.

AU - Ishii, T.

AU - Ishimori, R.

AU - Ito, H.

AU - Ivanov, D.

AU - Iwamoto, S.

AU - Jui, C. C.H.

AU - Kadota, K.

AU - Kakimoto, F.

AU - Kalashev, O.

AU - Kanbe, T.

AU - Kasahara, K.

AU - Kawai, H.

AU - Kawakami, S.

AU - Kawana, S.

AU - Kido, E.

AU - Kim, H. B.

AU - Kim, H. K.

AU - Kim, J. H.

AU - Kitamoto, K.

AU - Kitamura, S.

AU - Kitamura, Y.

AU - Kobayashi, K.

AU - Kobayashi, Y.

AU - Kondo, Y.

AU - Kuramoto, K.

AU - Kuzmin, V.

AU - Kwon, Y. J.

AU - Lan, J.

AU - Lim, S. I.

AU - Lundquist, J. P.

AU - Machida, S.

AU - Martens, K.

AU - Matsuda, T.

AU - Matsuura, T.

AU - Matsuyama, T.

AU - Matthews, J. N.

AU - Minamino, M.

AU - Miyata, K.

AU - Murano, Y.

AU - Myers, I.

AU - Nagasawa, K.

AU - Nagataki, S.

AU - Nakamura, T.

AU - Nam, S. W.

AU - Nonaka, T.

AU - Ogio, S.

AU - Ohnishi, M.

AU - Ohoka, H.

AU - Oki, K.

AU - Oku, D.

AU - Okuda, T.

AU - Ono, M.

AU - Oshima, A.

AU - Ozawa, S.

AU - Park, I. H.

AU - Pshirkov, M. S.

AU - Rodriguez, D. C.

AU - Roh, S. Y.

AU - Rubtsov, G.

AU - Ryu, D.

AU - Sagawa, H.

AU - Sakurai, N.

AU - Sampson, A. L.

AU - Scott, L. M.

AU - Shah, P. D.

AU - Shibata, F.

AU - Shibata, T.

AU - Shimodaira, H.

AU - Shin, B. K.

AU - Shin, J. I.

AU - Shirahama, T.

AU - Smith, J. D.

AU - Sokolsky, P.

AU - Springer, R. W.

AU - Stokes, B. T.

AU - Stratton, S. R.

AU - Stroman, T.

AU - Suzuki, S.

AU - Takahashi, Y.

AU - Takeda, M.

AU - Taketa, A.

AU - Takita, M.

AU - Tameda, Y.

AU - Tanaka, H.

AU - Tanaka, K.

AU - Tanaka, M.

AU - Thomas, S. B.

AU - Thomson, G. B.

AU - Tinyakov, P.

AU - Tkachev, I.

AU - Tokuno, H.

AU - Tomida, T.

AU - Troitsky, S.

AU - Tsunesada, Y.

AU - Tsutsumi, K.

AU - Tsuyuguchi, Y.

AU - Uchihori, Y.

AU - Udo, S.

AU - Ukai, H.

AU - Urban, F.

AU - Vasiloff, G.

AU - Wada, Y.

AU - Wong, T.

AU - Yamakawa, Y.

AU - Yamane, R.

AU - Yamaoka, H.

AU - Yamazaki, K.

AU - Yang, J.

AU - Yoneda, Y.

AU - Yoshida, S.

AU - Yoshii, H.

AU - Zhou, X.

AU - Zollinger, R.

AU - Zundel, Z.

N1 - Funding Information: The Telescope Array Experiment is supported by the Japan Society for the Promotion of Science through Grants-in-Aid for Scientific Research on Specially Promoted Research (21000002) “Extreme Phenomena in the Universe Explored by Highest Energy Cosmic Rays”, and the Inter-University Research Program of the Institute for Cosmic Ray Research; by the U.S. National Science Foundation awards PHY-0307098, PHY-0601915, PHY-0703893, PHY-0758342, PHY-0848320, PHY-1069280, and PHY-1069286 (Utah) and PHY-0649681 (Rutgers); by the National Research Foundation of Korea ( 2006-0050031 , 2007-0056005 , 2007-0093860 , 2010-0011378 , 2010-0028071 , R32-10130 ); by the Russian Academy of Sciences , RFBR Grants 10-02-01406a and 11-02-01528a (INR), IISN project No. 4.4509.10 and Belgian Science Policy under IUAP VI/11 (ULB). The foundations of Dr. Ezekiel R. and Edna Wattis Dumke, Willard L. Eccles and the George S. and Dolores Dore Eccles all helped with generous donations. The State of Utah supported the project through its Economic Development Board, and the University of Utah through the Office of the Vice President for Research. The experimental site became available through the cooperation of the Utah School and Institutional Trust Lands Administration (SITLA), U.S. Bureau of Land Management and the U.S. Air Force. We also wish to thank the people and the officials of Millard County, Utah, for their steadfast and warm support. We gratefully acknowledge the contributions from the technical staffs of our home institutions as well as the University of Utah Center for High Performance Computing (CHPC).

PY - 2015/2

Y1 - 2015/2

N2 - We measure the spectrum of cosmic rays with energies greater than 10 18.2 eV with the fluorescence detectors (FDs) and the surface detectors (SDs) of the Telescope Array Experiment using the data taken in our first 2.3-year observation from May 27, 2008 to September 7, 2010. A hybrid air shower reconstruction technique is employed to improve accuracies in determination of arrival directions and primary energies of cosmic rays using both FD and SD data. The energy spectrum presented here is in agreement with our previously published spectra and the HiRes results.

AB - We measure the spectrum of cosmic rays with energies greater than 10 18.2 eV with the fluorescence detectors (FDs) and the surface detectors (SDs) of the Telescope Array Experiment using the data taken in our first 2.3-year observation from May 27, 2008 to September 7, 2010. A hybrid air shower reconstruction technique is employed to improve accuracies in determination of arrival directions and primary energies of cosmic rays using both FD and SD data. The energy spectrum presented here is in agreement with our previously published spectra and the HiRes results.

UR - http://www.scopus.com/inward/record.url?scp=84907599683&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84907599683&partnerID=8YFLogxK

U2 - 10.1016/j.astropartphys.2014.05.002

DO - 10.1016/j.astropartphys.2014.05.002

M3 - Article

AN - SCOPUS:84907599683

SN - 0927-6505

VL - 61

SP - 93

EP - 101

JO - Astroparticle Physics

JF - Astroparticle Physics

ER -

Energy spectrum of ultra-high energy cosmic rays observed with the Telescope Array using a hybrid technique

Abstract

Bibliographical note

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