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Ryu, Dongsu
Astrophysics Lab
Research Interests
  • Shock waves and turbulence in clusters of galaxies
  • Origin and evolution of magnetic fields and cosmic rays in the universe
  • Plasma astrophysical phenomena in the large-scale structure of the universe

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

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dc.contributor.author Abu-Zayyad, T. ko
dc.contributor.author Aida, R. ko
dc.contributor.author Allen, M. ko
dc.contributor.author Anderson, R. ko
dc.contributor.author Azuma, R. ko
dc.contributor.author Barcikowski, E. ko
dc.contributor.author Belz, J. W. ko
dc.contributor.author Bergman, D. R. ko
dc.contributor.author Blake, S. A. ko
dc.contributor.author Cady, R. ko
dc.contributor.author Cheond, B. G. ko
dc.contributor.author Chiba, J. ko
dc.contributor.author Chikawa, M. ko
dc.contributor.author Cho, E. J. ko
dc.contributor.author Cho, W. R. ko
dc.contributor.author Fujii, H. ko
dc.contributor.author Fujii, T. ko
dc.contributor.author Fukuda, T. ko
dc.contributor.author Fukushima, M. ko
dc.contributor.author Hanlon, W. ko
dc.contributor.author Hayashi, K. ko
dc.contributor.author Hayashi, Y. ko
dc.contributor.author Hayashida, N. ko
dc.contributor.author Hibino, K. ko
dc.contributor.author Hiyama, K. ko
dc.contributor.author Honda, K. ko
dc.contributor.author Iguchi, T. ko
dc.contributor.author Ikeda, D. ko
dc.contributor.author Ikuta, K. ko
dc.contributor.author Inoue, N. ko
dc.contributor.author Ishii, T. ko
dc.contributor.author Ishimori, R. ko
dc.contributor.author Ito, H. ko
dc.contributor.author Ivanov, D. ko
dc.contributor.author Iwamoto, S. ko
dc.contributor.author Jui, C. C. H. ko
dc.contributor.author Kadota, K. ko
dc.contributor.author Kakimoto, F. ko
dc.contributor.author Kalashev, O. ko
dc.contributor.author Kanbe, T. ko
dc.contributor.author Kasahara, K. ko
dc.contributor.author Kawai, H. ko
dc.contributor.author Kawakami, S. ko
dc.contributor.author Kawana, S. ko
dc.contributor.author Kido, E. ko
dc.contributor.author Kim, H. B. ko
dc.contributor.author Kim, H. K. ko
dc.contributor.author Kim, J. H. ko
dc.contributor.author Kim, J. H. ko
dc.contributor.author Kitamoto, K. ko
dc.contributor.author Kitamura, S. ko
dc.contributor.author Kitamura, Y. ko
dc.contributor.author Kobayashi, K. ko
dc.contributor.author Kobayashi, Y. ko
dc.contributor.author Kondo, Y. ko
dc.contributor.author Kuramoto, K. ko
dc.contributor.author Kuzmin, V. ko
dc.contributor.author Kwong, Y. J. ko
dc.contributor.author Lan, J. ko
dc.contributor.author Lim, S. I. ko
dc.contributor.author Lundquist, J. P. ko
dc.contributor.author Machida, S. ko
dc.contributor.author Martens, K. ko
dc.contributor.author Matsuda, T. ko
dc.contributor.author Matsuura, T. ko
dc.contributor.author Matsuyama, T. ko
dc.contributor.author Matthews, J. N. ko
dc.contributor.author Minamino, M. ko
dc.contributor.author Miyata, K. ko
dc.contributor.author Murano, Y. ko
dc.contributor.author Myers, I. ko
dc.contributor.author Nagasawa, K. ko
dc.contributor.author Nagataki, S. ko
dc.contributor.author Nakamura, T. ko
dc.contributor.author Nam, S. W. ko
dc.contributor.author Nonaka, T. ko
dc.contributor.author Ogio, S. ko
dc.contributor.author Ohnishi, M. ko
dc.contributor.author Ohoka, H. ko
dc.contributor.author Oki, K. ko
dc.contributor.author Oku, D. ko
dc.contributor.author Okuda, T. ko
dc.contributor.author Ono, M. ko
dc.contributor.author Oshima, A. ko
dc.contributor.author Ozawa, S. ko
dc.contributor.author Park, I. H. ko
dc.contributor.author Pshirkov, M. S. ko
dc.contributor.author Rodriguez, D. C. ko
dc.contributor.author Roh, S. Y. ko
dc.contributor.author Rubtsov, G. ko
dc.contributor.author Ryu, Dongsu ko
dc.contributor.author Sagawa, H. ko
dc.contributor.author Sakurai, N. ko
dc.contributor.author Sampson, A. L. ko
dc.contributor.author Scott, L. M. ko
dc.contributor.author Shah, P. D. ko
dc.contributor.author Shibata, F. ko
dc.contributor.author Shibata, T. ko
dc.contributor.author Shimodaira, H. ko
dc.contributor.author Shin, B. K. ko
dc.contributor.author Shin, J. I. ko
dc.contributor.author Shirahama, T. ko
dc.contributor.author Smith, J. D. ko
dc.contributor.author Sokolsky, P. ko
dc.contributor.author Springer, R. W. ko
dc.contributor.author Stokes, B. T. ko
dc.contributor.author Stratton, S. R. ko
dc.contributor.author Stroman, T. ko
dc.contributor.author Suzuki, S. ko
dc.contributor.author Takahashi, Y. ko
dc.contributor.author Takeda, M. ko
dc.contributor.author Taketa, A. ko
dc.contributor.author Takita, M. ko
dc.contributor.author Tameda, Y. ko
dc.contributor.author Tanaka, H. ko
dc.contributor.author Tanaka, K. ko
dc.contributor.author Tanaka, M. ko
dc.contributor.author Thomas, S. B. ko
dc.contributor.author Thomson, G. B. ko
dc.contributor.author Tinyakov, P. ko
dc.contributor.author Tkachev, I. ko
dc.contributor.author Tokuno, H. ko
dc.contributor.author Tomida, T. ko
dc.contributor.author Troitsky, S. ko
dc.contributor.author Tsunesada, Y. ko
dc.contributor.author Tsutsumi, K. ko
dc.contributor.author Tsuyuguchi, Y. ko
dc.contributor.author Uchihori, Y. ko
dc.contributor.author Udo, S. ko
dc.contributor.author Ukai, H. ko
dc.contributor.author Urban, F. ko
dc.contributor.author Vasiloff, G. ko
dc.contributor.author Wada, Y. ko
dc.contributor.author Wong, T. ko
dc.contributor.author Yamakawa, Y. ko
dc.contributor.author Yamane, R. ko
dc.contributor.author Yamaoka, H. ko
dc.contributor.author Yamazaki, K. ko
dc.contributor.author Yang, J. ko
dc.contributor.author Yoneda, Y. ko
dc.contributor.author Yoshida, S. ko
dc.contributor.author Yoshii, H. ko
dc.contributor.author Zhou, X. ko
dc.contributor.author Zollinger, R. ko
dc.contributor.author Zundel, Z. ko
dc.date.available 2015-02-10T00:07:25Z -
dc.date.created 2015-02-09 ko
dc.date.issued 2015-02 -
dc.identifier.citation ASTROPARTICLE PHYSICS, v.61, no., pp.93 - 101 ko
dc.identifier.issn 0927-6505 ko
dc.identifier.uri https://scholarworks.unist.ac.kr/handle/201301/10502 -
dc.identifier.uri http://www.sciencedirect.com/science/article/pii/S0927650514000668 ko
dc.description.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. (C) 2014 Elsevier B.V. All rights reserved. ko
dc.description.statementofresponsibility close -
dc.language ENG ko
dc.publisher ELSEVIER SCIENCE BV ko
dc.title Energy spectrum of ultra-high energy cosmic rays observed with the Telescope Array using a hybrid technique ko
dc.type ARTICLE ko
dc.identifier.scopusid 2-s2.0-84907599683 ko
dc.identifier.wosid 000343391200013 ko
dc.type.rims ART ko
dc.description.wostc 5 *
dc.date.tcdate 2015-12-28 *
dc.identifier.doi 10.1016/j.astropartphys.2014.05.002 ko
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