Related Researcher

Author's Photo

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


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

DC Field Value Language Abu-Zayyad, T. ko Aida, R. ko Allen, M. ko Anderson, R. ko Azuma, R. ko Barcikowski, E. ko Belz, J. W. ko Bergman, D. R. ko Blake, S. A. ko Cady, R. ko Cheond, B. G. ko Chiba, J. ko Chikawa, M. ko Cho, E. J. ko Cho, W. R. ko Fujii, H. ko Fujii, T. ko Fukuda, T. ko Fukushima, M. ko Hanlon, W. ko Hayashi, K. ko Hayashi, Y. ko Hayashida, N. ko Hibino, K. ko Hiyama, K. ko Honda, K. ko Iguchi, T. ko Ikeda, D. ko Ikuta, K. ko Inoue, N. ko Ishii, T. ko Ishimori, R. ko Ito, H. ko Ivanov, D. ko Iwamoto, S. ko Jui, C. C. H. ko Kadota, K. ko Kakimoto, F. ko Kalashev, O. ko Kanbe, T. ko Kasahara, K. ko Kawai, H. ko Kawakami, S. ko Kawana, S. ko Kido, E. ko Kim, H. B. ko Kim, H. K. ko Kim, J. H. ko Kim, J. H. ko Kitamoto, K. ko Kitamura, S. ko Kitamura, Y. ko Kobayashi, K. ko Kobayashi, Y. ko Kondo, Y. ko Kuramoto, K. ko Kuzmin, V. ko Kwong, Y. J. ko Lan, J. ko Lim, S. I. ko Lundquist, J. P. ko Machida, S. ko Martens, K. ko Matsuda, T. ko Matsuura, T. ko Matsuyama, T. ko Matthews, J. N. ko Minamino, M. ko Miyata, K. ko Murano, Y. ko Myers, I. ko Nagasawa, K. ko Nagataki, S. ko Nakamura, T. ko Nam, S. W. ko Nonaka, T. ko Ogio, S. ko Ohnishi, M. ko Ohoka, H. ko Oki, K. ko Oku, D. ko Okuda, T. ko Ono, M. ko Oshima, A. ko Ozawa, S. ko Park, I. H. ko Pshirkov, M. S. ko Rodriguez, D. C. ko Roh, S. Y. ko Rubtsov, G. ko Ryu, Dongsu ko Sagawa, H. ko Sakurai, N. ko Sampson, A. L. ko Scott, L. M. ko Shah, P. D. ko Shibata, F. ko Shibata, T. ko Shimodaira, H. ko Shin, B. K. ko Shin, J. I. ko Shirahama, T. ko Smith, J. D. ko Sokolsky, P. ko Springer, R. W. ko Stokes, B. T. ko Stratton, S. R. ko Stroman, T. ko Suzuki, S. ko Takahashi, Y. ko Takeda, M. ko Taketa, A. ko Takita, M. ko Tameda, Y. ko Tanaka, H. ko Tanaka, K. ko Tanaka, M. ko Thomas, S. B. ko Thomson, G. B. ko Tinyakov, P. ko Tkachev, I. ko Tokuno, H. ko Tomida, T. ko Troitsky, S. ko Tsunesada, Y. ko Tsutsumi, K. ko Tsuyuguchi, Y. ko Uchihori, Y. ko Udo, S. ko Ukai, H. ko Urban, F. ko Vasiloff, G. ko Wada, Y. ko Wong, T. ko Yamakawa, Y. ko Yamane, R. ko Yamaoka, H. ko Yamazaki, K. ko Yang, J. ko Yoneda, Y. ko Yoshida, S. ko Yoshii, H. ko Zhou, X. ko Zollinger, R. ko Zundel, Z. ko 2015-02-10T00:07:25Z - 2015-02-09 ko 2015-02 -
dc.identifier.citation ASTROPARTICLE PHYSICS, v.61, no., pp.93 - 101 ko
dc.identifier.issn 0927-6505 ko
dc.identifier.uri -
dc.identifier.uri 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 * 2015-12-28 *
dc.identifier.doi 10.1016/j.astropartphys.2014.05.002 ko
Appears in Collections:
PHY_Journal Papers

find_unist can give you direct access to the published full text of this article. (UNISTARs only)

Show simple item record


  • mendeley


Items in DSpace are protected by copyright, with all rights reserved, unless otherwise indicated.