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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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THE COSMIC-RAY ENERGY SPECTRUM OBSERVED WITH THE SURFACE DETECTOR OF THE TELESCOPE ARRAY EXPERIMENT

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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 Cheon, 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 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 Kwon, Y. J. ko
dc.contributor.author Lan, J. ko
dc.contributor.author Lim, S. I. 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 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 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 Vasiloff, G. ko
dc.contributor.author Wada, Y. ko
dc.contributor.author Wong, T. ko
dc.contributor.author Wood, M. 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 2014-09-16T06:54:22Z -
dc.date.created 2014-09-15 ko
dc.date.issued 2013-05 -
dc.identifier.citation ASTROPHYSICAL JOURNAL LETTERS, v.768, no.1, pp.1 - 5 ko
dc.identifier.issn 2041-8205 ko
dc.identifier.uri https://scholarworks.unist.ac.kr/handle/201301/5968 -
dc.identifier.uri http://www.scopus.com/inward/record.url?partnerID=HzOxMe3b&scp=84876530151 ko
dc.description.abstract The Telescope Array (TA) collaboration has measured the energy spectrum of ultra-high energy cosmic rays (UHECRs) with primary energies above 1.6 x 10(18) eV. This measurement is based upon four years of observation by the surface detector component of TA. The spectrum shows a dip at an energy of 4.6x10(18) eV and a steepening at 5.4x10(19) eV which is consistent with the expectation from the GZK cutoff. We present the results of a technique, new to the analysis of UHECR surface detector data, that involves generating a complete simulation of UHECRs striking the TA surface detector. The procedure starts with shower simulations using the CORSIKA Monte Carlo program where we have solved the problems caused by use of the "thinning" approximation. This simulation method allows us to make an accurate calculation of the acceptance of the detector for the energies concerned. ko
dc.description.statementofresponsibility open -
dc.language ENG ko
dc.publisher IOP PUBLISHING LTD ko
dc.subject astroparticle physics ko
dc.subject cosmic rays ko
dc.subject methods: data analysis ko
dc.title THE COSMIC-RAY ENERGY SPECTRUM OBSERVED WITH THE SURFACE DETECTOR OF THE TELESCOPE ARRAY EXPERIMENT ko
dc.type ARTICLE ko
dc.identifier.scopusid 2-s2.0-84876530151 ko
dc.identifier.wosid 000317912900001 ko
dc.type.rims ART ko
dc.description.wostc 31 *
dc.description.scopustc 23 *
dc.date.tcdate 2015-05-06 *
dc.date.scptcdate 2014-09-15 *
dc.identifier.doi 10.1088/2041-8205/768/1/L1 ko
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