Search Results - "Komae, I."

Isotropy of Cosmic Rays beyond 10 20 eV Favors Their Heavy Mass Composition by Abbasi, R. U., Abe, Y., Abu-Zayyad, T., Allen, M., Arai, Y., Arimura, R., Barcikowski, E., Belz, J. W., Bergman, D. R., Blake, S. A., Buckland, I., Cheon, B. G., Chikawa, M., Fujii, T., Fujisue, K., Fujita, K., Fujiwara, R., Fukushima, M., Furlich, G., Globus, N., Gonzalez, R., Hanlon, W., Hayashida, N., He, H., Hibi, R., Hibino, K., Higuchi, R., Honda, K., Ikeda, D., Inoue, N., Ishii, T., Ito, H., Ivanov, D., Iwasaki, A., Jeong, H. M., Jeong, S., Jui, C. C. H., Kadota, K., Kakimoto, F., Kalashev, O., Kasahara, K., Kasami, S., Kawakami, S., Kawata, K., Kharuk, I., Kido, E., Kim, H. B., Kim, J. H., Kim, S. W., Kimura, Y., Komae, I., Kuzmin, V., Kuznetsov, M., Kwon, Y. J., Lee, K. H., Lubsandorzhiev, B., Lundquist, J. P., Matsumiya, H., Matsuyama, T., Matthews, J. N., Mayta, R., Mizuno, K., Murakami, M., Myers, I., Lee, K. H., Nagataki, S., Nakai, K., Nakamura, T., Nishio, E., Nonaka, T., Oda, H., Ogio, S., Onishi, M., Ohoka, H., Okazaki, N., Oku, Y., Okuda, T., Omura, Y., Ono, M., Oshima, A., Oshima, H., Ozawa, S., Park, I. H., Park, K. Y., Potts, M., Pshirkov, M. S., Remington, J., Rodriguez, D. C., Rott, C., Rubtsov, G. I., Ryu, D., Sagawa, H., Saito, R., Sakaki, N., Sako, T., Sakurai, N., Sato, D., Sato, K., Sato, S., Sekino, K.

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Isotropy of cosmic rays beyond $10^{20}$ eV favors their heavy mass composition by Abbasi, R. U, Abu-Zayyad, T, Arai, Y, Barcikowski, E, Belz, J. W, Bergman, D. R, Blake, S. A, Cheon, B. G, Fujii, T, Fujisue, K, Fujiwara, R, Fukushima, M, Furlich, G, Globus, N, Gonzalez, R, Hanlon, W, Hayashida, N, He, H, Hibi, R, Hibino, K, Higuchi, R, Honda, K, Ikeda, D, Inoue, N, Ishii, T, Ivanov, D, Iwasaki, A, Jeong, S, Jui, C. C. H, Kakimoto, F, Kasami, S, Kawakami, S, Kawata, K, Kharuk, I, Kido, E, Kim, H. B, Kim, J. H, Kim, S. W, Kimura, Y, Kuzmin, V, Lee, K. H, Lundquist, J. P, Matsumiya, H, Matsuyama, T, Mayta, R, Mizuno, K, Murakami, M, Myers, I, Nagataki, S, Nakai, K, Nishio, E, Nonaka, T, Ogio, S, Ohoka, H, Okazaki, N, Oku, Y, Okuda, T, Ono, M, Oshima, A, Oshima, H, Park, I. H, Potts, M, Pshirkov, M. S, Remington, J, Rodriguez, D. C, Rott, C, Rubtsov, G. I, Saito, R, Sakaki, N, Sakurai, N, Sato, S, Sekino, K, Shah, P. D, Shibata, N, Shibata, T, Shikita, J, Shin, H. S, Shinto, D, Sokolsky, P, Stroman, T. A, Takahashi, K, Takeda, M, Taketa, A, Takita, M, Tameda, Y, Tanaka, K, Tanaka, M, Tanoue, Y, Thomson, G. B, Tinyakov, P, Tokuno, H, Tomida, T, Troitsky, S, Udo, S, Urban, F, Wong, T, Yamazaki, K, Yoshida, F, Zhezher, Y, Zundel, Z

“…We report an estimation of the injected mass composition of ultra-high energy cosmic rays (UHECRs) at energies higher than 10 EeV. The composition is inferred…”
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Mass composition of ultra-high energy cosmic rays from distribution of their arrival directions with the Telescope Array by Abbasi, R. U, Abu-Zayyad, T, Arai, Y, Barcikowski, E, Belz, J. W, Bergman, D. R, Blake, S. A, Cheon, B. G, Fujii, T, Fujisue, K, Fujiwara, R, Fukushima, M, Furlich, G, Globus, N, Gonzalez, R, Hanlon, W, Hayashida, N, He, H, Hibi, R, Hibino, K, Higuchi, R, Honda, K, Ikeda, D, Inoue, N, Ishii, T, Ivanov, D, Iwasaki, A, Jeong, S, Jui, C. C. H, Kakimoto, F, Kasami, S, Kawakami, S, Kawata, K, Kharuk, I, Kido, E, Kim, H. B, Kim, J. H, Kim, S. W, Kimura, Y, Kuzmin, V, Lee, K. H, Lundquist, J. P, Matsumiya, H, Matsuyama, T, Mayta, R, Mizuno, K, Murakami, M, Myers, I, Nagataki, S, Nakai, K, Nishio, E, Nonaka, T, Ogio, S, Ohoka, H, Okazaki, N, Oku, Y, Okuda, T, Ono, M, Oshima, A, Oshima, H, Park, I. H, Potts, M, Pshirkov, M. S, Remington, J, Rodriguez, D. C, Rott, C, Rubtsov, G. I, Saito, R, Sakaki, N, Sakurai, N, Sato, S, Sekino, K, Shah, P. D, Shibata, N, Shibata, T, Shikita, J, Shin, H. S, Shinto, D, Sokolsky, P, Stroman, T. A, Takahashi, K, Takeda, M, Taketa, A, Takita, M, Tameda, Y, Tanaka, K, Tanaka, M, Tanoue, Y, Thomson, G. B, Tinyakov, P, Tokuno, H, Tomida, T, Troitsky, S, Udo, S, Urban, F, Wong, T, Yamazaki, K, Yoshida, F, Zhezher, Y, Zundel, Z

“…We use a new method to estimate the injected mass composition of ultrahigh cosmic rays (UHECRs) at energies higher than 10 EeV. The method is based on…”
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Observation of Declination Dependence in the Cosmic Ray Energy Spectrum by The Telescope Array Collaboration, Abbasi, R. U, Abu-Zayyad, T, Belz, J. W, Bergman, D. R, Buckland, I, Campbell, W, Cheon, B. G, Fedynitch, A, Fujii, T, Fujisue, K, Fujita, K, Fukushima, M, Gerber, Z, Globus, N, Hanlon, W, Hayashida, N, Hibino, K, Ikeda, D, Ishii, T, Jeong, S, Jui, C. C. H, Kadota, K, Kakimoto, F, Kalashev, O, Kasahara, K, Kawachi, Y, Kharuk, I, Kido, E, Kim, J. H, Kim, S. W, Kobo, R, Komae, I, Komatsu, K, Komori, K, Koyama, C, Kudenko, M, Kusumori, Y, Kwon, Y. J, Lee, K. H, Lee, M. J, Lubsandorzhiev, B, Lundquist, J. P, Matthews, J. A, Matthews, J. N, Mizuno, K, Mori, M, Nagataki, S, Nakahara, M, Nakamura, T, Nakayama, T, Nakayama, Y, Nonaka, T, Ogio, S, Ohoka, H, Okazaki, N, Onishi, M, Oshima, H, Ozawa, S, Park, I. H, Park, K. Y, Potts, M, Remington, J, Rott, C, Rubtsov, G. I, Ryu, D, Sagawa, H, Sakaki, N, Sakamoto, R, Sako, T, Sakurai, S, Sato, D, Sekino, K, Shibata, T, Shimodaira, H, Shin, B. K, Shin, H. S, Shinozaki, K, Smith, J. D, Sokolsky, P, Stokes, B. T, Stroman, T. A, Takahashi, K, Takeda, M, Taketa, A, Tameda, Y, Tanaka, M, Thomson, G. B, Tinyakov, P, Tkachev, I, Tomida, T, Troitsky, S, Tsunesada, Y, Udo, S, Vaiman, I. A, Vrábel, M, Warren, D, Yamazaki, K, Zhezher, Y, Zundel, Z

“…We report on an observation of the difference between northern and southern skies of the ultrahigh energy cosmic ray energy spectrum with a significance of…”
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