Author: "Shoichi, Ogio" / Topic: telescope - Searchworks@Jio Institute Digital Library Search Results

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1. Observations of Ultra-high Energy Cosmic Rays with Telescope Array Experiment—From the Discoveries of Indications to Detailed Observations

Author: Shoichi Ogio, Hiroyuki Sagawa, and Yoshiki Tsunesada
Subjects: Physics, Telescope, Radiation, law, Astronomy, Ultra-high-energy cosmic ray, law.invention
Published: 2019
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2. Anisotropy search in the Ultra High Energy Cosmic Ray Spectrum in the Northern Hemisphere using latest data obtained with Telescope Array surface detector

Author: Grigory Rubtsov, John Matthews, Norimichi Shibata, Y. Omura, J. Yang, Fumiya Shibata, Shingo Kawana, M. Ohnishi, Taichi Inadomi, Matt Potts, William Hanlon, Monica Allen, Bokkyun Shin, Fugo Yoshida, Yuma Shibasaki, ByongGu Cheon, Ben Stokes, Douglas Bergman, Jyunsei Chiba, Dongsu Ryu, Toshihiro Fujii, Koki Sato, Yasunori Saito, M. Yamamoto, Hirokazu Iwakura, Y. Takagi, Ryuhei Arimura, Hideyuki Ohoka, Yuto Kubota, Federico R. Urban, Nobuyuki Sakurai, Kengo Sano, Mikhail Kuznetsov, Heungsu Shin, Ivan Kharuk, Yukio Uchihori, Keitaro Fujita, K. H. Lee, Jihee Kim, Yoshiki Tsunesada, Daisuke Ikeda, Hirotaka Ito, Sergey Troitsky, Yuto Arai, Ryota Onogi, J. H. Kim, Maxim Pshirkov, Takeshi Okuda, Y. Nakamura, Kohei Yada, Charlie Jui, BayarJon Paul Lubsandorzhiev, Mayuko Minamino, Hiroyuki Matsumiya, Igor Tkachev, R. Mayta, Hideki Tanaka, Naohiro Sone, Ryosuke Tsuda, Tiffany Wong, Taka Tomida, J. Remington, Masaki Fukushima, Takafumi Uehama, Aoi Iwasaki, Daiki Shinto, Hideaki Shimodaira, Hyoming Jeong, Shoichi Kishigami, Soomin Jeong, Shigeharu Udo, Eiji Kido, Hiroyuki Sagawa, Takashi Sako, Ryo Higuchi, Hisono Tokuno, H. Oda, Gordon Thomson, Tom Stroman, Priti Shah, Ryo Nakamura, Robert Cady, Kazuhiro Machida, Masahiro Takeda, Pierre Sokolsky, Naoaki Hayashida, Ken Honda, Tatsunobu Shibata, T. Seki, G. Furlich, Takaaki Ishii, R. Sahara, Fumio Kakimoto, Naoya Inoue, Akitoshi Oshima, Vladim Kuzmin, Ryuji Takeishi, Ryota Fukushima, Shigehiro Nagataki, Shunsuke Ozawa, K. Yamazaki, Masaomi Ono, Elliott Barcikowski, Toshiyuki Nonaka, Saori Kasami, Tareq Abu-Zayyad, Zach Zundel, Yana Zhezher, Kenta Yashiro, Dmitri Ivanov, D. C. Rodriguez, Ricardo Gonzalez, Samuel Blake, Sang Woo Kim, Kinya Hibino, Shoichi Ogio, Keijiro Mukai, HangBae Kim, Yusuke Kimura, Rasha Abbasi, Koichi Tanaka, Yuya Oku, Michiyuki Chikawa, Jon Paul Lundquist, Katsuaki Kasahara, Stanton Thomas, Katsumasa Kawata, Oleg Kalashev, Yuichiro Tameda, Tomoyuki Nakamura, Tsubasa Yoshioka, Arata Nakazawa, Masato Takita, Toru Nakamura, Telescope Array, Min Hyo Kim, Toshio Matsuyama, Kei Nakai, Ryota Fujiwara, Kenichi Kadota, Manobu Tanaka, Il Hung Park, Naoto Sakaki, S. Kawakami, Akimichi Taketa, Eiji Nishio, Hideyuki Kawai, Shinnosuke Kurisu, Jeremy Smith, Isaac Myers, Youngjoon Kwon, John Belz, Koichi Sekino, P. Tinyakov, Y. Takahashi, Mai Takamura, Yuta Tanoue, Motoki Hayashi, and Kozo Fujisue
Subjects: Surface (mathematics), Telescope, Physics, law, Detector, Northern Hemisphere, Astrophysics, Ultra-high-energy cosmic ray, Anisotropy, law.invention
Published: 2021
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3. High-resolution two-dimensional map of the solar-time anisotropy obtained by the GRAPES-3 large-area muon telescope

Author: Tatsumi Koi, Hiroshi Kojima, Shakeel Ahmad, Medha Chakraborty, Anuj Chandra, Shashi Dugad, Snil K. Gupta, Balakrishnan Hariharan, Yoshio Hayashi, Paranjothi Jagadeesan, Atul Jain, Pankaj Jain, Vuta B. Jhansi, Saburo Kawakami, Swapna Mahapatra, Toshio Matsuyama, Pravata Mohanty, Isao Morishita, Sumuel D. Morris, Yasushi Muraki, Toru Nakamura, Pranaba K. Nayak, Toshiyuki Nonaka, Shoichi Ogio, Akitoshi Oshima, Diptiranjan Pattanaik, Pankaj S. Rakshe, Kaviti Ramesh, Bellam S. Rao, Lakki V. Reddy, Shoichi Shibata, Hisanori Takamaru, Koichi Tanaka, Fahim Varsi, Katsuya Yamazaki, and Meeran Zuberi
Subjects: Physics, Telescope, Muon, law, Astrophysics::High Energy Astrophysical Phenomena, Solar time, Cosmic ray, Astrophysics, Anisotropy, Intensity (heat transfer), GRAPES-3, Zenith, law.invention
Abstract: In the analysis of the anisotropy of the galactic cosmic rays caused by the solar modulation below 1 TeV, time series graphs with time on the horizontal axis and cosmic ray intensity as the vertical axis had been widely adopted and other style of the graphs called harmonic vector diagrams had also been used. These methods are the time series analyses, and because of the horizontal axis (time), the graph is often misinterpreted as a “temporal variation,” even though it must be regarded as an intrinsically “spatial distribution.” This paper presents a high-resolution two-dimensional map of the solar time anisotropy using the GRAPES-3 large-area muon telescope at Ooty, south India, which has an excellent capability of observing the muon intensity in 169 directions within a 50 degree zenith angle.
Published: 2021
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4. The measurements of the cosmic ray energy spectrum and the depth of maximum shower development of Telescope Array Hybrid trigger events

Author: Katsuaki Kasahara, Shinnosuke Kurisu, Katsumasa Kawata, Shingo Kawana, William Hanlon, Tsubasa Yoshioka, R. Sahara, Hideaki Shimodaira, Hyoming Jeong, Ryo Higuchi, Norimichi Shibata, Monica Allen, Bokkyun Shin, Jeremy Smith, Y. Omura, Vladim Kuzmin, G. Furlich, Takaaki Ishii, Akimichi Taketa, Toshio Matsuyama, Eiji Nishio, ByongGu Cheon, K. Yamazaki, Tareq Abu-Zayyad, Toshiyuki Nonaka, Hideyuki Ohoka, D. C. Rodriguez, Fumiya Shibata, Hiroyuki Matsumiya, Fugo Yoshida, HangBae Kim, Hiroyuki Sagawa, Ricardo Gonzalez, Pierre Sokolsky, Tatsunobu Shibata, Hideyuki Kawai, Takafumi Uehama, Manobu Tanaka, Rasha Abbasi, Takeshi Okuda, Youngjoon Kwon, John Belz, Yuma Shibasaki, Shigehiro Nagataki, Matt Potts, Yana Zhezher, Mikhail Kuznetsov, Akitoshi Oshima, Igor Tkachev, Sang Woo Kim, Eiji Kido, Koichi Tanaka, K. H. Lee, Jihee Kim, Kazuhiro Machida, Isaac Myers, Naohiro Sone, Shunsuke Ozawa, Hideki Tanaka, Heungsu Shin, Douglas Bergman, Gordon Thomson, Ryo Nakamura, Jon Paul Lundquist, Tom Stroman, Robert Cady, Yuta Tanoue, Ben Stokes, H. Oda, Grigory Rubtsov, Tomoyuki Nakamura, Yasunori Saito, Yuto Arai, Motoki Hayashi, Ryota Fujiwara, Federico R. Urban, Nobuyuki Sakurai, Ryosuke Tsuda, Hirotaka Ito, Hisono Tokuno, Elliott Barcikowski, Charlie Jui, Soomin Jeong, Naoto Sakaki, Kozo Fujisue, BayarJon Paul Lubsandorzhiev, Mayuko Minamino, Yuya Oku, Oleg Kalashev, Dmitri Ivanov, Fumio Kakimoto, Arata Nakazawa, Kenta Yashiro, Kei Nakai, T. Seki, Naoya Inoue, Keijiro Mukai, Min Hyo Kim, Yusuke Kimura, S. Kawakami, Stanton Thomas, M. Ohnishi, Taichi Inadomi, Koki Sato, Sergey Troitsky, Kengo Sano, Aoi Iwasaki, Toshihiro Fujii, Michiyuki Chikawa, Toru Nakamura, Taka Tomida, J. Remington, Kenichi Kadota, Yuto Kubota, Il Hung Park, Saori Kasami, Y. Nakamura, Kohei Yada, Koichi Sekino, Naoaki Hayashida, P. Tinyakov, Ryuji Takeishi, Ryuhei Arimura, Yoshiki Tsunesada, Daisuke Ikeda, Tiffany Wong, Masaki Fukushima, Takashi Sako, Zach Zundel, John Matthews, J. Yang, Daiki Shinto, Priti Shah, Jyunsei Chiba, Dongsu Ryu, Masahiro Takeda, Ken Honda, Hirokazu Iwakura, Y. Takagi, Shigeharu Udo, Keitaro Fujita, Ryota Fukushima, Ivan Kharuk, M. Yamamoto, Yukio Uchihori, Ryota Onogi, J. H. Kim, R. Mayta, Kinya Hibino, Yuichiro Tameda, Masato Takita, Shoichi Kishigami, Y. Takahashi, Mai Takamura, Masaomi Ono, Telescope Array, Samuel Blake, Shoichi Ogio, and Maxim Pshirkov
Subjects: Telescope, Physics, Shower, law, Energy spectrum, Astronomy, Cosmic ray, law.invention
Published: 2021
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5. Mass composition of Telescope Array's surface detectors events using deep learning

Author: Hideaki Shimodaira, Hyoming Jeong, Hiroyuki Sagawa, Fumiya Shibata, Ryuji Takeishi, Ryo Higuchi, Youngjoon Kwon, John Belz, Hideyuki Ohoka, Ryo Nakamura, Rasha Abbasi, Daiki Shinto, Ryuhei Arimura, Koichi Tanaka, Yoshiki Tsunesada, Daisuke Ikeda, Michiyuki Chikawa, Tiffany Wong, Masaki Fukushima, Matt Potts, Yuma Shibasaki, Priti Shah, Jon Paul Lundquist, K. Yamazaki, Pierre Sokolsky, Katsuaki Kasahara, Katsumasa Kawata, Tareq Abu-Zayyad, Fugo Yoshida, Masahiro Takeda, Takashi Sako, Ken Honda, Zach Zundel, Shigehiro Nagataki, Yana Zhezher, Ben Stokes, Tsubasa Yoshioka, Kenta Yashiro, Sergey Troitsky, R. Sahara, Douglas Bergman, Sang Woo Kim, Taka Tomida, Shingo Kawana, Charlie Jui, BayarJon Paul Lubsandorzhiev, J. Remington, Mayuko Minamino, Mikhail Kuznetsov, Min Hyo Kim, Shinnosuke Kurisu, William Hanlon, Ryota Fujiwara, Elliott Barcikowski, Dmitri Ivanov, Monica Allen, Naoto Sakaki, Tomoyuki Nakamura, G. Furlich, Takaaki Ishii, Federico R. Urban, Nobuyuki Sakurai, Saori Kasami, Keijiro Mukai, Bokkyun Shin, Toshio Matsuyama, K. H. Lee, Jihee Kim, Gordon Thomson, Ryota Fukushima, Samuel Blake, Shoichi Ogio, Hirotaka Ito, Yusuke Kimura, Tom Stroman, Robert Cady, Naoaki Hayashida, Norimichi Shibata, Y. Omura, S. Kawakami, D. C. Rodriguez, Keitaro Fujita, Jeremy Smith, HangBae Kim, Takeshi Okuda, Igor Tkachev, Akimichi Taketa, Hideki Tanaka, Stanton Thomas, Naohiro Sone, Isaac Myers, Eiji Nishio, Yuya Oku, Aoi Iwasaki, Oleg Kalashev, Hiroyuki Matsumiya, Toshihiro Fujii, Hisono Tokuno, H. Oda, Jyunsei Chiba, Grigory Rubtsov, Dongsu Ryu, Manobu Tanaka, Yuto Kubota, Koichi Sekino, Takafumi Uehama, Maxim Pshirkov, Hideyuki Kawai, P. Tinyakov, Toru Nakamura, Kenichi Kadota, M. Ohnishi, Y. Nakamura, Il Hung Park, Kohei Yada, Hirokazu Iwakura, Taichi Inadomi, Y. Takagi, Y. Takahashi, Mai Takamura, Eiji Kido, Kazuhiro Machida, Arata Nakazawa, Koki Sato, John Matthews, Toshiyuki Nonaka, Kei Nakai, Ivan Kharuk, J. Yang, Ricardo Gonzalez, Kengo Sano, Yasunori Saito, Yuta Tanoue, Fumio Kakimoto, Motoki Hayashi, Yuichiro Tameda, Kozo Fujisue, Shoichi Kishigami, Masaomi Ono, Masato Takita, Telescope Array, Shigeharu Udo, Kinya Hibino, M. Yamamoto, Yukio Uchihori, Ryota Onogi, J. H. Kim, R. Mayta, Vladim Kuzmin, Ryosuke Tsuda, Soomin Jeong, T. Seki, Naoya Inoue, Heungsu Shin, Yuto Arai, Tatsunobu Shibata, Akitoshi Oshima, Shunsuke Ozawa, and ByongGu Cheon
Subjects: Surface (mathematics), Telescope, Physics, Optics, business.industry, law, Deep learning, Detector, Artificial intelligence, Mass composition, business, law.invention
Published: 2021
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6. UHECR mass composition from anisotropy of their arrival directions with the Telescope Array SD

Author: Katsuaki Kasahara, Ryota Fukushima, Takeshi Okuda, Igor Tkachev, Katsumasa Kawata, Daiki Shinto, Naohiro Sone, ByongGu Cheon, Shoichi Kishigami, Norimichi Shibata, Manobu Tanaka, Grigory Rubtsov, Ryuhei Arimura, M. Yamamoto, H. Oda, Masaomi Ono, Priti Shah, Y. Omura, Yoshiki Tsunesada, Tsubasa Yoshioka, Daisuke Ikeda, Masahiro Takeda, Tiffany Wong, Mikhail Kuznetsov, Ken Honda, K. H. Lee, Jihee Kim, Kenta Yashiro, Gordon Thomson, Hideyuki Ohoka, Yuichiro Tameda, Yukio Uchihori, Masaki Fukushima, Hiroyuki Sagawa, R. Sahara, Charlie Jui, Jyunsei Chiba, Dongsu Ryu, Tom Stroman, Fugo Yoshida, Robert Cady, Ryota Onogi, J. H. Kim, Shinnosuke Kurisu, Shingo Kawana, Ryota Fujiwara, BayarJon Paul Lubsandorzhiev, William Hanlon, Hirokazu Iwakura, Y. Takagi, R. Mayta, Hiroyuki Matsumiya, Koichi Tanaka, Mayuko Minamino, Vladim Kuzmin, Hideaki Shimodaira, Ivan Kharuk, Jon Paul Lundquist, Naoto Sakaki, Youngjoon Kwon, Kinya Hibino, John Belz, Ryo Nakamura, Hyoming Jeong, Michiyuki Chikawa, Keitaro Fujita, Takafumi Uehama, Saori Kasami, Fumiya Shibata, Ryo Higuchi, Yuya Oku, M. Ohnishi, Takashi Sako, Masato Takita, Eiji Kido, Toshiyuki Nonaka, Taichi Inadomi, Oleg Kalashev, Ryosuke Tsuda, Soomin Jeong, Ricardo Gonzalez, Rasha Abbasi, Kazuhiro Machida, Toshio Matsuyama, Min Hyo Kim, Matt Potts, Koki Sato, Kengo Sano, K. Yamazaki, Tareq Abu-Zayyad, Hideki Tanaka, Zach Zundel, S. Kawakami, Yasunori Saito, Peter Tinyakov, Samuel Blake, Shoichi Ogio, Shigeharu Udo, T. Seki, Toru Nakamura, Naoya Inoue, Jeremy Smith, John Matthews, J. Yang, Monica Allen, Kenichi Kadota, Hisono Tokuno, Yuta Tanoue, Akimichi Taketa, Bokkyun Shin, Eiji Nishio, Il Hung Park, Motoki Hayashi, Ben Stokes, Kozo Fujisue, Heungsu Shin, Federico R. Urban, Nobuyuki Sakurai, Hideyuki Kawai, Yuma Shibasaki, Koichi Sekino, Yuto Arai, Douglas Bergman, Tatsunobu Shibata, Y. Takahashi, Mai Takamura, Akitoshi Oshima, Shunsuke Ozawa, Maxim Pshirkov, Fumio Kakimoto, Sergey Troitsky, Taka Tomida, J. Remington, Naoaki Hayashida, Toshihiro Fujii, Yuto Kubota, Y. Nakamura, Kohei Yada, Elliott Barcikowski, Dmitri Ivanov, Keijiro Mukai, Yusuke Kimura, Stanton Thomas, Aoi Iwasaki, Tomoyuki Nakamura, Ryuji Takeishi, Pierre Sokolsky, Shigehiro Nagataki, Yana Zhezher, Isaac Myers, Sang Woo Kim, Hirotaka Ito, G. Furlich, Takaaki Ishii, D. C. Rodriguez, HangBae Kim, Arata Nakazawa, and Kei Nakai
Subjects: Telescope, Physics, law, Astrophysics, Mass composition, Anisotropy, law.invention
Published: 2021
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7. Gamma Ray Showers Observed at Ground Level in Coincidence With Downward Lightning Leaders

Author: Fumiya Shibata, R. W. Springer, Maxim Pshirkov, John Belz, Akitoshi Oshima, Hiroyuki Sagawa, Fumio Kakimoto, D. R. Bergman, Zach Zundel, K. Hibino, Koichi Sekino, K. Kasahara, Y. Tsunesada, Hideaki Shimodaira, Ryo Nakamura, R. LeVon, Hongsu Kim, Kazuo Saito, Shoichi Kishigami, Heungsu Shin, Shunsuke Ozawa, Mayuko Minamino, K. Honda, Hidemi Ito, K. Martens, Toshitsugu Fujii, M. Yamamoto, Y. Yoneda, N. Inoue, G. Vasiloff, Ryuji Takeishi, Masato Takita, Nobuyuki Sakurai, Masaomi Ono, Priti Shah, Hideki Tanaka, Grigory Rubtsov, M. Ohnishi, H. Yoshii, Ryota Onogi, Ben Stokes, Daisuke Ikeda, Elliott Barcikowski, Sergey Troitsky, Masaaki Tanaka, T. Matuyama, Vladim Kuzmin, Jyunsei Chiba, Dongsu Ryu, M. Allen, Helio Takai, Takayuki Tomida, Dmitri Ivanov, Tiffany Wong, B. G. Cheon, Keijiro Mukai, S. Jeong, Masaki Fukushima, B. K. Shin, K. Oki, Federico R. Urban, J. Remington, S. Udo, C. C. H. Jui, Tareq Abu-Zayyad, R. Yamane, Peter Tinyakov, Samuel Blake, Shoichi Ogio, Rasha Abbasi, William Rison, H. Kawai, Michiyuki Chikawa, M. Byrne, Naoaki Hayashida, S. Kawakami, Kiyoshi Tanaka, S. B. Thomas, Akimichi Taketa, Y. Hayashi, Toru Nakamura, K. Kawata, T. Seki, Kenichi Kadota, J. Lan, Igor Tkachev, R. Cady, J. P. Lundquist, G. Furlich, Takaaki Ishii, D. Rodeheffer, Toshiyuki Nonaka, T.-A. Shibata, Gordon Thomson, S. Yoshida, Hiroshi Yamaoka, Tom Stroman, Naoto Sakaki, Kenta Yashiro, D. C. Rodriguez, Isaac Myers, Inkyu Park, Y. Uchihori, H. Tokuno, K. Yamazaki, J. D. Smith, Yuichiro Tameda, John N. Matthews, William Hanlon, T. Okuda, J. H. Kim, J. Yang, Y. J. Kwon, Hideyuki Ohoka, Paul R. Krehbiel, T. Goto, Eiji Kido, Pierre Sokolsky, Kazuhiro Machida, M. Takeda, Shigehiro Nagataki, R. J. Thomas, and O. Kalashev
Subjects: Atmospheric Science, 010504 meteorology & atmospheric sciences, Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Astrophysics, Radiation, 01 natural sciences, High Energy Physics - Experiment, law.invention, Telescope, High Energy Physics - Experiment (hep-ex), Electron avalanche, law, 0103 physical sciences, Earth and Planetary Sciences (miscellaneous), Cosmic-ray observatory, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Lightning detection, Astrophysics::Instrumentation and Methods for Astrophysics, Gamma ray, Lightning, Physics - Atmospheric and Oceanic Physics, Geophysics, 13. Climate action, Space and Planetary Science, Atmospheric and Oceanic Physics (physics.ao-ph), Satellite, Astrophysics - High Energy Astrophysical Phenomena
Abstract: Bursts of gamma ray showers have been observed in coincidence with downward propagating negative leaders in lightning flashes by the Telescope Array Surface Detector (TASD). The TASD is a 700~square kilometer cosmic ray observatory located in southwestern Utah, U.S.A. In data collected between 2014 and 2016, correlated observations showing the structure and temporal development of three shower-producing flashes were obtained with a 3D lightning mapping array, and electric field change measurements were obtained for an additional seven flashes, in both cases co-located with the TASD. National Lightning Detection Network (NLDN) information was also used throughout. The showers arrived in a sequence of 2--5 short-duration ($\le$10~$\mu$s) bursts over time intervals of several hundred microseconds, and originated at an altitude of $\simeq$3--5 kilometers above ground level during the first 1--2 ms of downward negative leader breakdown at the beginning of cloud-to-ground lightning flashes. The shower footprints, associated waveforms and the effect of atmospheric propagation indicate that the showers consist primarily of downward-beamed gamma radiation. This has been supported by GEANT simulation studies, which indicate primary source fluxes of $\simeq$$10^{12}$--$10^{14}$ photons for $16^{\circ}$ half-angle beams. We conclude that the showers are terrestrial gamma-ray flashes (TGFs), similar to those observed by satellites, but that the ground-based observations are more representative of the temporal source activity and are also more sensitive than satellite observations, which detect only the most powerful TGFs.
Published: 2018
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8. The bursts of high energy events observed by the telescope array surface detector

Author: Hiroshi Yamaoka, T. Suzawa, Robert M. Anderson, Hideaki Shimodaira, Isaac Myers, M. Abe, Kenta Yashiro, T. Goto, Elliott Barcikowski, Dmitri Ivanov, Keijiro Mukai, Maxim Pshirkov, Sergey Troitsky, A. L. Sampson, Takaaki Ishii, Kanako Yamazaki, Priti Shah, K. Tsutsumi, S. Kitamura, Fumiya Shibata, D. C. Rodriguez, Hidemi Ito, S. Kawakami, J. P. Lundquist, Keiji Saito, Igor Tkachev, R. Ishimori, John Belz, R. W. Springer, Pierre Sokolsky, Naoaki Hayashida, Akimichi Taketa, Ben Stokes, K. Oki, Koichi Sekino, H. Yoshii, Tareq Abu-Zayyad, R. Yamane, Federico R. Urban, Kiyoshi Tanaka, Y. Yoneda, N. Inoue, M. Ohnishi, Michiyuki Chikawa, Hiroyuki Sagawa, R. Zollinger, S. Udo, C. C. H. Jui, Heungsu Shin, M. Takeda, Shigehiro Nagataki, Ryuji Takeishi, Akitoshi Oshima, Y. Uchihori, Y. J. Kwon, Hideyuki Ohoka, K. Nagasawa, S. B. Thomas, Tomohiro Matsuda, H. Kawai, Mai Takamura, T.-A. Shibata, Fumio Kakimoto, Peter Tinyakov, Gordon Thomson, K. Hibino, Samuel Blake, Byung Gu Cheon, Tom Stroman, Robert Cady, Shoichi Ogio, Zach Zundel, Hang Bae Kim, G. Vasiloff, L. M. Scott, J. Ogura, K. Martens, Hideki Tanaka, Jyunsei Chiba, Dongsu Ryu, B. K. Shin, Takayuki Tomida, Masato Takita, Mayuko Minamino, K. Honda, Yasunori Kitamura, Rasha Abbasi, A. Nozato, Y. Hayashi, Yoshiki Tsunesada, Daisuke Ikeda, M. Allen, Inkyu Park, S. R. Stratton, K. Kawata, Masaaki Tanaka, Nobuyuki Sakurai, Tiffany Wong, Masaki Fukushima, Douglas Bergman, Takahiro Fujii, V. Kuzmin, Ryota Onogi, J. H. Kim, S. Yoshida, Naoto Sakaki, O. Kalashev, Toru Nakamura, Eiji Kido, Kazuhiro Machida, Kenichi Kadota, T. Matsuyama, S. Ozawa, Yasunori Saito, K. Kasahara, Shoichi Kishigami, R. Azuma, Yuichiro Tameda, John N. Matthews, Masaomi Ono, G. Rubtsov, Shingo Kawana, William Hanlon, T. Okuda, J. Yang, H. Tokuno, J. D. Smith, J. Lan, and Toshiyuki Nonaka
Subjects: Physics, 010504 meteorology & atmospheric sciences, Gamma ray, General Physics and Astronomy, Astronomy, Cosmic ray, Astrophysics, 01 natural sciences, Lightning, Particle detector, law.invention, Telescope, Air shower, law, 0103 physical sciences, Ultra-high-energy cosmic ray, 010306 general physics, 0105 earth and related environmental sciences, Terrestrial gamma-ray flash
Abstract: The Telescope Array (TA) experiment is designed to detect air showers induced by ultra high energy cosmic rays. The TA ground Surface particle Detector (TASD) observed several short-time bursts of air shower like events. These bursts are not likely due to chance coincidence between single shower events. The expectation of chance coincidence is less than 10 − 4 for five-year's observation. We checked the correlation between these bursts of events and lightning data, and found evidence for correlations in timing and position. Some features of the burst events are similar to those of a normal cosmic ray air shower, and some are not. On this paper, we report the observed bursts of air shower like events and their correlation with lightning.
Published: 2017
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9. Search for Large-scale Anisotropy on Arrival Directions of Ultra-high-energy Cosmic Rays Observed with the Telescope Array Experiment

Author: Takashi Sako, Hideaki Shimodaira, Hyoming Jeong, Ryo Higuchi, Inkyu Park, Kenta Yashiro, R. U. Abbasi, Tareq Abu-Zayyad, R. Azuma, Fumiya Shibata, F. Kakimoto, R. Ishimori, Daisuke Ikeda, K. Yamazaki, H. Kawai, Tiffany Wong, R. Takeishi, Masaki Fukushima, Maxim Pshirkov, Hongsu Kim, B. K. Shin, Hideki Tanaka, Toshiyuki Fujii, B. G. Cheon, T. Seki, John Belz, K. Kawata, BayarJon Paul Lubsandorzhiev, Akimichi Taketa, Min Hyo Kim, G. Furlich, Takaaki Ishii, Mayuko Minamino, K. Honda, Takayuki Tomida, Seok Ho Jeong, K. H. Lee, Yuta Tanoue, Masaaki Tanaka, D. C. Rodriguez, T.-A. Shibata, S. Kawakami, Motoki Hayashi, Zach Zundel, Peter Tinyakov, Samuel Blake, Gordon Thomson, Ben Stokes, Tom Stroman, Robert Cady, J. P. Lundquist, Shoichi Ogio, Kozo Fujisue, Hiroyuki Sagawa, M. Yamamoto, M. Yosei, Hidemi Ito, Grigory Rubtsov, Koichi Sekino, Kiyoshi Tanaka, D. R. Bergman, T. Suzawa, Y. Zhezher, Heungsu Shin, Isaac Myers, Katsuaki Kasahara, Y. Takahashi, Mai Takamura, Nobuyuki Sakurai, Yuya Oku, Oleg Kalashev, K. Hibino, Shoichi Kishigami, M. Allen, Sergey Troitsky, Toru Nakamura, Kenichi Kadota, T. Matsuyama, S. Ozawa, Masaomi Ono, Toshiyuki Nonaka, Y. Uchihori, Kei Nakai, Ryota Onogi, A. Di Matteo, J. Remington, Hideyuki Ohoka, R. Mayta, Vladim Kuzmin, Ryota Fujiwara, Keitaro Fujita, Saori Kasami, Shingo Kawana, Naoto Sakaki, Naoaki Hayashida, Yoshihiko Nakamura, William Hanlon, Priti Shah, T. Okuda, J. Yang, Masato Takita, R. Sahara, Pierre Sokolsky, M. Takeda, Shigehiro Nagataki, M. Abe, Akitoshi Oshima, Y. Tsunesada, H. Tokuno, Younghoon Kwon, J. D. Smith, J. H. Kim, Elliott Barcikowski, Dmitri Ivanov, Keijiro Mukai, Jyunsei Chiba, Dongsu Ryu, Hirokazu Iwakura, Y. Takagi, Kohei Yada, Y. Omura, Igor Tkachev, Naohiro Sone, H. Oda, N. Inoue, M. Ohnishi, Taichi Inadomi, Federico R. Urban, S. Udo, C. C. H. Jui, Kengo Sano, S. B. Thomas, Yasunori Saito, Yuichiro Tameda, John N. Matthews, S. W. Kim, Hiroyuki Matsumiya, M. Chikawa, Takafumi Uehama, Eiji Kido, M. V. Kuznetsov, Kazuhiro Machida, and Ryo Nakamura
Subjects: Physics, Pierre Auger Observatory, High Energy Astrophysical Phenomena (astro-ph.HE), 010504 meteorology & atmospheric sciences, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, FOS: Physical sciences, Astronomy and Astrophysics, Cosmic ray, 01 natural sciences, Auger, Computational physics, law.invention, Telescope, Dipole, Amplitude, Space and Planetary Science, law, 0103 physical sciences, Ultra-high-energy cosmic ray, Astrophysics - High Energy Astrophysical Phenomena, Anisotropy, 010303 astronomy & astrophysics, 0105 earth and related environmental sciences
Abstract: Motivated by the detection of a significant dipole structure in the arrival directions of ultrahigh-energy cosmic rays above 8 EeV reported by the Pierre Auger Observatory (Auger), we search for a large-scale anisotropy using data collected with the surface detector array of the Telescope Array Experiment (TA). With 11 years of TA data, a dipole structure in a projection of the right ascension is fitted with an amplitude of 3.3+- 1.9% and a phase of 131 +- 33 degrees. The corresponding 99% confidence-level upper limit on the amplitude is 7.3%. At the current level of statistics, the fitted result is compatible with both an isotropic distribution and the dipole structure reported by Auger., Comment: 6 pages, 3 figures, 1 table, Proofed title. Added journal reference and DOI
Published: 2020
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10. Long distance network link for TAx4 expansion

Author: Stan B. Thomas, Toshiyuki Nonaka, Takeshi Okuda, Naoto Sakaki, Hiroyuki Sagawaa, Eiji Kido, Kohei Yada, John Matthews, Robert Cady, Ryota Fujiwara, and Shoichi Ogio
Subjects: Computer science, business.industry, Attenuation, Detector, Elevation, Measure (physics), Electrical engineering, Terrain, Power (physics), law.invention, Telescope, Air shower, law, business
Abstract: As a high-energy expansion of existing Telescope Array (TA) experiment, TAx4 SDs have been deployed and operated from Apr.2019. Network communication for inter-site and each detector also have been expanded to longer distance. Communication towers are located in off-grid. Those are operated by solar panel and batteries. In this report we describe hardware configuration and installation as well as operation status after the installation. We measure reception signals at communication towers and each detector sites. The reception depends on condition of terrain. There are several models and tools those are used for predicting received power considering elevation model. For future ground experiment of air shower observation, it is useful if attenuation of signal strength and communication quality could be estimated quantitatively. In this report, we present observed signal strength and its comparison with available attenuation models also.
Published: 2019
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11. Telescope Array Low energy Extension(TALE) Hybrid

Author: Shoichi Ogio
Subjects: Telescope, Low energy, Data acquisition, law, Computer science, Conjunction (astronomy), Detector, Extension (predicate logic), Hybrid data, Preliminary analysis, Remote sensing, law.invention
Abstract: Routine hybrid observations of the surface detectors (SD) in conjunction with the fluorescence detectors (FD) of the Telescope Array Low-energy Extension (TALE) began in November 2018. In this presentation, we will describe the data acquisition system, including the design of the SD array, as well as the FD-to-SD cross-trigger. We will report on the status of operations, and on the preliminary analysis of the TALE hybrid data.
Published: 2019
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12. Highlights from the Telescope Array experiment

Author: Shoichi Ogio
Subjects: Physics, Range (particle radiation), Physics::Instrumentation and Detectors, business.industry, Astrophysics::High Energy Astrophysical Phenomena, media_common.quotation_subject, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, law.invention, Telescope, Optics, Air shower, Sky, law, Scintillation counter, High Energy Physics::Experiment, Anisotropy, business, media_common
Abstract: The Telescope Array is the largest hybrid cosmic ray detector in the Northern hemisphere designed to measure primary particles in 4 PeV to 100 EeV range. TA is a hybrid detector. The main TA detector consists of 507 plastic scintillation counters on a 1.2km square grid and and fluorescence detectors at three stations overlooking the sky above the surface detector array. Recently the construction of the TA low energy Extension (TALE) detectors, which consists of an additional ten fluorescence telescopes and 80 infill surface detectors with 400m and 600 m spacing, was finished. TALE lowers the energy threshold of TA down to 4 PeV. We are also constructing the TAx4 air shower array to increase statistics in particular at the highest energies. The current status and the future prospects of experiments and their recent measurements - spectrum, composition, and anisotropy - will be reviewed.
Published: 2019
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13. Time structure analysis of extensive air showers using the Telescope Array Data

Author: Shoichi Ogio, Rosa Mayta Palacios, and Yoshiki Tsunesada
Subjects: Physics, Physics::Instrumentation and Detectors, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Front (oceanography), Curvature, law.invention, Telescope, Shower, Optics, law, Waveform, High Energy Physics::Experiment, business, Energy (signal processing), Zenith
Abstract: In this paper, we report results of the study of temporal shower front structure based on the data taken by the Telescope Array Surface Detector from 2008 to 2019. By analyzing the waveforms measured by FADCs, we defined two quantities characterizing the shower structure, the curvature of the shower front and the thickness of the shower disk. These analyses were performed by selecting the data sample of high-quality events at zenith angles up to 60 degrees. Firstly we used an empirical form of the shower front curvature in term of residual time, and found a clear zenith angle dependence but no significant energy dependence based on the 3 energy intervals in log(E/eV) bins from 18.90 to 20.00. Secondly, the thickness of the disk is analyzed by the rising time of the FADC waveform. We found that the thickness of the shower disk has a dependency on angles and energy.
Published: 2019
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14. Search for Ultra-High-Energy Neutrinos with the Telescope Array Surface Detector

Author: Koichi Sekino, Y. Takahashi, Mai Takamura, S. Kitamura, Hidemi Ito, K. Martens, Yuta Tanoue, Motoki Hayashi, J. P. Lundquist, K. Tsutsumi, John Belz, Heungsu Shin, Vladim Kuzmin, Takashi Sako, Toru Nakamura, Inkyu Park, Kenichi Kadota, Yana Zhezher, Hiroyuki Sagawa, D. R. Bergman, Maxim Pshirkov, Charlie Jui, BayarJon Paul Lubsandorzhiev, Mayuko Minamino, K. Yamazaki, M. Abe, K. H. Lee, K. Honda, Daisuke Ikeda, S. R. Stratton, Yasunori Kitamura, T.-A. Shibata, Gordon Thomson, Toshiyuki Fujii, Ryo Nakamura, Tom Stroman, Robert Cady, Masaaki Tanaka, Fumiya Shibata, M. Yamamoto, Nobuyuki Sakurai, Tiffany Wong, R. Takeishi, L. M. Scott, Hongsu Kim, Y. Hayashi, R. Ishimori, Masaki Fukushima, Kazuo Saito, Ben Stokes, N. Inoue, M. Ohnishi, Y. J. Kwon, Akimichi Taketa, Eiji Kido, B. G. Cheon, H. Kawai, K. Kawata, Federico R. Urban, M. V. Kuznetsov, Ryota Onogi, Hideyuki Ohoka, Pierre Sokolsky, A. Di Matteo, H. Yoshii, S. Udo, Kazuhiro Machida, Hideaki Shimodaira, Hyoming Jeong, M. Takeda, Shigehiro Nagataki, R. Mayta, T. Seki, Seok Ho Jeong, S. B. Thomas, Peter Tinyakov, Samuel Blake, Oleg Kalashev, Shoichi Ogio, Priti Shah, Igor Tkachev, Zach Zundel, S. Kawakami, Fumio Kakimoto, Tareq Abu-Zayyad, K. Nagasawa, H. Oda, H. Tokuno, R. Azuma, Toshiyuki Nonaka, K. Hibino, Kenta Yashiro, Akitoshi Oshima, Y. Tsunesada, Keitaro Fujita, B. K. Shin, H. Yamaoka, Michiyuki Chikawa, Masato Takita, J. D. Smith, Sergey Troitsky, Y. Omura, J. Remington, J. H. Kim, Elliott Barcikowski, Dmitri Ivanov, Jyunsei Chiba, Keijiro Mukai, Naoaki Hayashida, Shingo Kawana, Dongsu Ryu, Y. Takagi, Yasunori Saito, William Hanlon, T. Okuda, J. Yang, Yuichiro Tameda, John N. Matthews, Kohei Yada, Hideki Tanaka, Takayuki Tomida, K. Kasahara, Shoichi Kishigami, Kiyoshi Tanaka, Grigory Rubtsov, M. Allen, Masaomi Ono, R. Sahara, Ryota Fujiwara, Naoto Sakaki, Y. Uchihori, Kei Nakai, Rasha Abbasi, T. Matsuyama, S. Ozawa, T. Suzawa, J. Ogura, Isaac Myers, G. Furlich, Takaaki Ishii, and D. C. Rodriguez
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Detector, FOS: Physical sciences, General Physics and Astronomy, Flux, Observable, Cosmic ray, 01 natural sciences, law.invention, Telescope, Optics, Distribution function, law, 0103 physical sciences, Alternating decision tree, High Energy Physics::Experiment, Neutrino, 010306 general physics, business, Astrophysics - High Energy Astrophysical Phenomena
Abstract: We present an upper limit on the flux of ultra-high-energy down-going neutrinos for $E > 10^{18}\ \mbox{eV}$ derived with the nine years of data collected by the Telescope Array surface detector (05-11-2008 -- 05-10-2017). The method is based on the multivariate analysis technique, so-called Boosted Decision Trees (BDT). Proton-neutrino classifier is built upon 16 observables related to both the properties of the shower front and the lateral distribution function., 10 pages, 4 figures, accepted to JETP
Published: 2019

15. Search for EeV protons of galactic origin

Author: R. Ishimori, R. Zollinger, Kenta Yashiro, Yasunori Saito, Yuichiro Tameda, John N. Matthews, K. Nagasawa, J. Yang, Y. J. Kwon, Eiji Kido, Hideyuki Ohoka, Kazuhiro Machida, J. Lan, S. Kitamura, Masato Takita, M. Abe, Byung Gu Cheon, Hidemi Ito, John Belz, Toshiyuki Nonaka, Elliott Barcikowski, Takayuki Tomida, Igor Tkachev, R. Cady, Motoki Hayashi, J. P. Lundquist, Ryuji Takeishi, BayarJon Paul Lubsandorzhiev, K. Hibino, Ben Stokes, Inkyu Park, T. Matsuyama, L. M. Scott, S. Ozawa, Dmitri Ivanov, Keijiro Mukai, Hiroshi Yamaoka, Tomohiro Matsuda, Mayuko Minamino, K. Honda, Y. Yoneda, N. Inoue, Federico R. Urban, A. Nozato, Y. Hayashi, K. Oki, M. Ohnishi, Yasunori Kitamura, T. Goto, S. Udo, C. C. H. Jui, K. Kawata, M. Allen, Douglas Bergman, Yoshiki Tsunesada, Nobuyuki Sakurai, Masaaki Tanaka, Sergey Troitsky, Daisuke Ikeda, Hideaki Shimodaira, Toru Nakamura, Kenichi Kadota, S. R. Stratton, H. Kawai, K. Kasahara, Akitoshi Oshima, S. B. Thomas, O. Kalashev, Shoichi Kishigami, Koichi Sekino, Kanako Yamazaki, Takahiro Fujii, Tiffany Wong, Priti Shah, K. Saito, Masaki Fukushima, Masaomi Ono, Jyunsei Chiba, Dongsu Ryu, B. K. Shin, Grigory Rubtsov, K. Martens, Hideki Tanaka, S. Yoshida, Y. Takahashi, Mai Takamura, Ryota Onogi, J. H. Kim, Vladim Kuzmin, H. Yoshii, Tareq Abu-Zayyad, A. H. Tirone, R. Yamane, Kiyoshi Tanaka, J. Ogura, Naoto Sakaki, Naoaki Hayashida, Peter Tinyakov, Samuel Blake, Maxim Pshirkov, Shoichi Ogio, T.-A. Shibata, Gordon Thomson, Tom Stroman, Zach Zundel, Pierre Sokolsky, Hang Bae Kim, Akimichi Taketa, Heungsu Shin, Rasha Abbasi, M. Takeda, Fumio Kakimoto, Shigehiro Nagataki, Michiyuki Chikawa, K. Tsutsumi, R. Azuma, S. Kawakami, Hiroyuki Sagawa, Y. Uchihori, T. Suzawa, Isaac Myers, Takaaki Ishii, D. C. Rodriguez, Shingo Kawana, William Hanlon, T. Okuda, H. Tokuno, J. D. Smith, and Fumiya Shibata
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Galactic anticenter, FOS: Physical sciences, Astronomy, Astronomy and Astrophysics, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Astrophysics, Galactic plane, 01 natural sciences, Galactic tide, law.invention, Telescope, law, 0103 physical sciences, Galactic corona, Astrophysics - High Energy Astrophysical Phenomena, Anisotropy, Longitude, 010303 astronomy & astrophysics, Astrophysics::Galaxy Astrophysics
Abstract: Cosmic rays in the energy range $10^{18.0}$ - $10^{18.5}$ eV are thought to have a light, probably protonic, composition. To study their origin one can search for anisotropy in their arrival directions. Extragalactic cosmic rays should be isotropic, but galactic cosmic rays of this type should be seen mostly along the galactic plane, and there should be a shortage of events coming from directions near the galactic anticenter. This is due to the fact that, under the influence of the galactic magnetic field, the transition from ballistic to diffusive behavior is well advanced, and this qualitative picture persists over the whole energy range. Guided by models of the galactic magnetic field that indicate that the enhancement along the galactic plane should have a standard deviation of about 20$^\circ$ in galactic latitude, and the deficit in the galactic anticenter direction should have a standard deviation of about 50$^\circ$ in galactic longitude, we use the data of the Telescope Array surface detector in $10^{18.0}$ to $10^{18.5}$ eV energy range to search for these effects. The data are isotropic. Neither an enhancement along the galactic plane nor a deficit in the galactic anticenter direction is found. Using these data we place an upper limit on the fraction of EeV cosmic rays of galactic origin at 1.3% at 95% confidence level.
Published: 2017
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16. TA Anisotropy Summary

Author: Gordon Thomson, C. C. H. Jui, Hiroyuki Sagawa, Peter Tinyakov, A. Di Matteo, Shoichi Ogio, Igor Tkachev, John N. Matthews, K. Kawata, J. P. Lundquist, Sergey Troitsky, Dmitri Ivanov, and Toshihiro Fujii
Subjects: Physics, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, QC1-999, Detector, Northern Hemisphere, Astrophysics::Instrumentation and Methods for Astrophysics, Astrophysics, 01 natural sciences, law.invention, Physics::Geophysics, Telescope, Sky, law, 0103 physical sciences, 010306 general physics, Anisotropy, 010303 astronomy & astrophysics, Astrophysique, Directional anisotropy, media_common
Abstract: The Telescope Array (TA) is the largest ultra-high-energy cosmic-ray (UHECR) detector in the northern hemisphere. It consists of an array of 507 surface detectors (SD) covering a total 700 km 2 and three fluorescence detector stations overlooking the SD array. In this proceedings, we summarize recent results on the search for directional anisotropy of UHECRs using the latest dataset collected by the TA SD array. We obtained hints of the anisotropy of the UHECRs in the northern sky from the various analyses., info:eu-repo/semantics/published
Published: 2019

17. Testing a reported correlation between arrival directions of ultrahigh-energy cosmic rays and a flux pattern from nearby starburst galaxies using Telescope Array data

Author: H. Kawai, Grigory Rubtsov, T. Seki, Hideaki Shimodaira, Hyoming Jeong, Toshitsugu Fujii, Shingo Kawana, G. Furlich, Takaaki Ishii, Oleg Kalashev, William Hanlon, T. Goto, K. Martens, T. Okuda, J. Yang, D. C. Rodriguez, K. Tsutsumi, M. Abe, Y. Uchihori, Elliott Barcikowski, S. Kitamura, Dmitri Ivanov, Hidemi Ito, T. Suzawa, Keijiro Mukai, Hiroyuki Sagawa, Tareq Abu-Zayyad, Maxim Pshirkov, Kenta Yashiro, Yasunori Saito, Toru Nakamura, Isaac Myers, Kenichi Kadota, R. Yamane, R. Sahara, K. Nagasawa, Heungsu Shin, Yuichiro Tameda, John N. Matthews, Ben Stokes, Fumio Kakimoto, M. Allen, L. M. Scott, Y. Hayashi, K. Yamazaki, Vladim Kuzmin, Y. J. Kwon, M. Yamamoto, K. Hibino, K. Kawata, S. Jeong, B. G. Cheon, Hideyuki Ohoka, Charlie Jui, Ryo Nakamura, K. H. Lee, T.-A. Shibata, Gordon Thomson, Nobuyuki Sakurai, Sergey Troitsky, Tom Stroman, Akimichi Taketa, Robert Cady, Kazuo Saito, J. H. Kim, Igor Tkachev, BayarJon Paul Lubsandorzhiev, J. Remington, Mayuko Minamino, K. Honda, John Belz, Yasunori Kitamura, Y. Omura, S. Kawakami, H. Oda, D. R. Bergman, H. Yoshii, Masaaki Tanaka, A. Di Matteo, Inkyu Park, Fumiya Shibata, Ryota Onogi, R. Ishimori, Kiyoshi Tanaka, Naoaki Hayashida, Takayuki Tomida, Y. Yoneda, N. Inoue, M. Ohnishi, Federico R. Urban, Akitoshi Oshima, Y. Tsunesada, Pierre Sokolsky, S. Udo, Hongsu Kim, R. Mayta, M. Takeda, S. B. Thomas, J. Ogura, Shigehiro Nagataki, Yana Zhezher, Eiji Kido, M. V. Kuznetsov, Kazuhiro Machida, K. Kasahara, Shoichi Kishigami, Hideki Tanaka, Zach Zundel, Daisuke Ikeda, R. Azuma, S. R. Stratton, Tiffany Wong, R. Takeishi, Masaki Fukushima, H. Yamaoka, Michiyuki Chikawa, Masaomi Ono, Toshiyuki Nonaka, Keitaro Fujita, B. K. Shin, Priti Shah, Peter Tinyakov, Samuel Blake, Shoichi Ogio, Masato Takita, Motoki Hayashi, J. P. Lundquist, Koichi Sekino, Y. Takahashi, Mai Takamura, Jyunsei Chiba, Dongsu Ryu, Y. Takagi, T. Matsuyama, S. Ozawa, Rasha Abbasi, S. Yoshida, Naoto Sakaki, H. Tokuno, and J. D. Smith
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, 010308 nuclear & particles physics, FOS: Physical sciences, Sigma, Flux, Astronomy and Astrophysics, Cosmic ray, Astrophysics, 01 natural sciences, Galaxy, Auger, law.invention, Telescope, Space and Planetary Science, law, 0103 physical sciences, Anisotropy, Astrophysics - High Energy Astrophysical Phenomena, 010303 astronomy & astrophysics, Energy (signal processing)
Abstract: The Pierre Auger Collaboration (Auger) recently reported a correlation between the arrival directions of cosmic rays with energies above 39 EeV and the flux pattern of 23 nearby starburst galaxies (SBGs). In this Letter, we tested the same hypothesis using cosmic rays detected by the Telescope Array experiment (TA) in the 9-year period from May 2008 to May 2017. Unlike the Auger analysis, we did not optimize the parameter values but kept them fixed to the best-fit values found by Auger, namely 9.7% for the anisotropic fraction of cosmic rays assumed to originate from the SBGs in the list and 12.9{\deg} for the angular scale of the correlations. The energy threshold we adopted is 43 EeV, corresponding to 39 EeV in Auger when taking into account the energy-scale difference between two experiments. We find that the TA data is compatible with isotropy to within 1.1{\sigma} and with the Auger result to within 1.4{\sigma}, meaning that it is not capable to discriminate between these two hypotheses., Comment: More accurate title, fixed an inconsistency in the declination range used, with a few figures slightly changing as a result, other minor revisions
Published: 2018

18. Study of muons from ultrahigh energy cosmic ray air showers measured with the Telescope Array experiment

Author: S. Kitamura, Hidemi Ito, Kenta Yashiro, Eiji Kido, M. V. Kuznetsov, Kazuhiro Machida, Jyunsei Chiba, Dongsu Ryu, Y. Takagi, Douglas Bergman, Toshiyuki Nonaka, K. Nagasawa, Hideki Tanaka, Elliott Barcikowski, J. H. Kim, T. Goto, G. Furlich, Takaaki Ishii, Y. Omura, Keitaro Fujita, Dmitri Ivanov, Pierre Sokolsky, J. Ogura, Yasunori Saito, B. K. Shin, Igor Tkachev, D. C. Rodriguez, R. Sahara, M. Takeda, Shigehiro Nagataki, Keijiro Mukai, Yuichiro Tameda, John N. Matthews, Akimichi Taketa, Rasha Abbasi, H. Oda, K. Yamazaki, M. Yamamoto, L. M. Scott, Nobuyuki Sakurai, T. Suzawa, Y. Yoneda, N. Inoue, M. Ohnishi, Sergey Troitsky, J. Remington, Y. Hayashi, Inkyu Park, Federico R. Urban, S. Udo, C. C. H. Jui, Isaac Myers, Y. J. Kwon, Hideyuki Ohoka, K. Kawata, Ryota Onogi, Koichi Sekino, A. Di Matteo, K. H. Lee, S. B. Thomas, T.-A. Shibata, Naoaki Hayashida, Takayuki Tomida, Gordon Thomson, T. Matsuyama, S. Ozawa, R. Mayta, Hongsu Kim, Priti Shah, Tom Stroman, Robert Cady, Y. Zhezher, Grigory Rubtsov, Hideaki Shimodaira, Hyoming Jeong, Y. Takahashi, Mai Takamura, K. Kasahara, Y. Uchihori, Shoichi Kishigami, S. Yoshida, Naoto Sakaki, R. Azuma, Masaomi Ono, Tareq Abu-Zayyad, R. Yamane, Kiyoshi Tanaka, Motoki Hayashi, J. P. Lundquist, Shingo Kawana, William Hanlon, M. Allen, H. Kawai, T. Okuda, J. Yang, H. Tokuno, J. D. Smith, Daisuke Ikeda, S. R. Stratton, Tiffany Wong, R. Takeishi, T. Seki, Masaki Fukushima, Masato Takita, K. Martens, K. Tsutsumi, Peter Tinyakov, Samuel Blake, Shoichi Ogio, Zach Zundel, Fumiya Shibata, R. Ishimori, Toshitsugu Fujii, Oleg Kalashev, H. Yamaoka, Michiyuki Chikawa, Ryo Nakamura, Kazuo Saito, H. Yoshii, Heungsu Shin, Toru Nakamura, K. Hibino, Kenichi Kadota, BayarJon Paul Lubsandorzhiev, Mayuko Minamino, K. Honda, Yasunori Kitamura, Masaaki Tanaka, John Belz, Hiroyuki Sagawa, Ben Stokes, B. G. Cheon, S. Kawakami, Maxim Pshirkov, Akitoshi Oshima, Y. Tsunesada, M. Abe, Fumio Kakimoto, Vladim Kuzmin, and S. Jeong
Subjects: High Energy Astrophysical Phenomena (astro-ph.HE), Physics, Muon, COSMIC cancer database, Particle number, Physics::Instrumentation and Detectors, 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Monte Carlo method, Hadron, FOS: Physical sciences, Cosmic ray, 01 natural sciences, law.invention, Telescope, Nuclear physics, Air shower, 13. Climate action, law, 0103 physical sciences, High Energy Physics::Experiment, Astrophysics - High Energy Astrophysical Phenomena, 010306 general physics
Abstract: One of the uncertainties in interpretation of ultra-high energy cosmic ray (UHECR) data comes from the hadronic interaction models used for air shower Monte Carlo (MC) simulations. The number of muons observed at the ground from UHECR-induced air showers is expected to depend upon the hadronic interaction model. One may therefore test the hadronic interaction models by comparing the measured number of muons with the MC prediction. In this paper, we present the results of studies of muon densities in UHE extensive air showers obtained by analyzing the signal of surface detector stations which should have high $\it{muon \, purity}$. The muon purity of a station will depend on both the inclination of the shower and the relative position of the station. In 7 years' data from the Telescope Array experiment, we find that the number of particles observed for signals with an expected muon purity of $\sim$65% at a lateral distance of 2000 m from the shower core is $1.72 \pm 0.10{\rm (stat.)} \pm 0.37 {\rm (syst.)}$ times larger than the MC prediction value using the QGSJET II-03 model for proton-induced showers. A similar effect is also seen in comparisons with other hadronic models such as QGSJET II-04, which shows a $1.67 \pm 0.10 \pm 0.36$ excess. We also studied the dependence of these excesses on lateral distances and found a slower decrease of the lateral distribution of muons in the data as compared to the MC, causing larger discrepancy at larger lateral distances.
Published: 2018
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19. Measurement of microwave radiation from electron beam in the atmosphere

Author: T. K. Sako, Tatsunobu Shibata, Daisuke Ikeda, Tokonatsu Yamamoto, Masaki Fukushima, Hiroyuki Sagawa, Izumi I.S. Ohta, John N. Matthews, Shoichi Ogio, Y. Inome, and Hidetoshi Akimune
Subjects: Physics, Nuclear and High Energy Physics, 010308 nuclear & particles physics, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Electron, Astrophysics, 01 natural sciences, law.invention, Telescope, Optics, Air shower, law, Observatory, 0103 physical sciences, Cathode ray, Antenna (radio), 010306 general physics, business, Instrumentation, Microwave
Abstract: We report the use of an electron light source (ELS) located at the Telescope Array Observatory in Utah, USA, to measure the isotropic microwave radiation from air showers. To simulate extensive air showers, the ELS emits an electron beam into the atmosphere and a parabola antenna system for the satellite communication is used to measure the microwave radiation from the electron beam. Based on this measurement, an upper limit on the intensity of a 12.5 GHz microwave radiation at 0.5 m from a 10 18 eV air shower was estimated to be 3.96×10 −16 W m −2 Hz −1 with a 95% confidence level.
Published: 2016
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20. Telescope Array Low energy Extension: TALE

Author: Shoichi Ogio
Subjects: Telescope, Physics, Extension (metaphysics), Low energy, law, Scintillation counter, Astronomy, law.invention
Published: 2018
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21. Calibration of Photo-Multiplier Tubes in Fluorescence Detectors of the Telescope Array

Author: B. K. Shin, Yoshiki Tsunesada, Masaki Fukushima, and Shoichi Ogio
Subjects: Telescope, Physics, Optics, law, business.industry, Detector, Calibration, Multiplier (economics), business, Fluorescence, law.invention
Published: 2018
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22. Depth of Ultra High Energy Cosmic Ray Induced Air Shower Maxima Measured by the Telescope Array Black Rock and Long Ridge FADC Fluorescence Detectors and Surface Array in Hybrid Mode

Author: R. Azuma, M. Yamamoto, Nobuyuki Sakurai, Ryota Onogi, A. Di Matteo, R. Mayta, B. G. Cheon, Fumiya Shibata, K. Martens, Hideki Tanaka, R. Ishimori, K. H. Lee, M. Abe, T.-A. Shibata, Gordon Thomson, Tom Stroman, Robert Cady, H. Tokuno, S. Kitamura, Priti Shah, T. Goto, K. Tsutsumi, Hideaki Shimodaira, Hyoming Jeong, Rasha Abbasi, S. Kawakami, Akimichi Taketa, Hidemi Ito, Jyunsei Chiba, Dongsu Ryu, J. D. Smith, J. Ogura, Toshiyuki Nonaka, Kiyoshi Tanaka, Akitoshi Oshima, Y. Takagi, G. Furlich, Takaaki Ishii, Shunsuke Ozawa, O. Kalashev, BayarJon Paul Lubsandorzhiev, Hiroshi Yamaoka, Mayuko Minamino, K. Honda, Y. Zhezher, Hiroyuki Sagawa, Keitaro Fujita, Yasunori Kitamura, Peter Tinyakov, Samuel Blake, D. C. Rodriguez, Shoichi Ogio, Ben Stokes, Toshitsugu Fujii, T. Matsuyama, Elliott Barcikowski, B. K. Shin, K. Yamazaki, Dmitri Ivanov, T. Suzawa, M. Allen, Masaaki Tanaka, K. Hibino, R. Sahara, Heungsu Shin, Zach Zundel, Ryo Nakamura, Keijiro Mukai, Isaac Myers, Kazuo Saito, Inkyu Park, Hongsu Kim, Pierre Sokolsky, S. Yoshida, Eiji Kido, Naoto Sakaki, Grigory Rubtsov, M. V. Kuznetsov, M. Takeda, John Belz, Vladim Kuzmin, H. Yoshii, Kazuhiro Machida, Shigehiro Nagataki, S. Jeong, Michiyuki Chikawa, H. Kawai, Tareq Abu-Zayyad, R. Yamane, K. Nagasawa, Douglas Bergman, Y. J. Kwon, Hideyuki Ohoka, Yasunori Saito, T. Seki, Yoshiki Tsunesada, Daisuke Ikeda, S. R. Stratton, Y. Uchihori, L. M. Scott, Tiffany Wong, R. Takeishi, Masaki Fukushima, Toru Nakamura, Y. Hayashi, Yuichiro Tameda, K. Kawata, John N. Matthews, Masato Takita, Kenichi Kadota, Sergey Troitsky, J. H. Kim, Y. Omura, Shingo Kawana, Naoaki Hayashida, William Hanlon, Igor Tkachev, T. Okuda, J. Yang, H. Oda, Kenta Yashiro, Y. Yoneda, N. Inoue, M. Ohnishi, Federico R. Urban, S. Udo, C. C. H. Jui, S. B. Thomas, Takayuki Tomida, K. Kasahara, Shoichi Kishigami, Masaomi Ono, Maxim Pshirkov, Motoki Hayashi, J. P. Lundquist, Koichi Sekino, Y. Takahashi, Mai Takamura, and Fumio Kakimoto
Subjects: Astrophysics::High Energy Astrophysical Phenomena, chemistry.chemical_element, FOS: Physical sciences, Cosmic ray, 7. Clean energy, 01 natural sciences, law.invention, Telescope, Optics, Observatory, law, 0103 physical sciences, Ultra-high-energy cosmic ray, 010303 astronomy & astrophysics, Helium, Astroparticle physics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), 010308 nuclear & particles physics, business.industry, Astronomy and Astrophysics, Air shower, chemistry, 13. Climate action, Space and Planetary Science, Ridge (meteorology), Astrophysics - High Energy Astrophysical Phenomena, business
Abstract: The Telescope Array observatory utilizes fluorescence detectors and surface detectors to observe air showers produced by ultra high energy cosmic rays in the Earth's atmosphere. Cosmic ray events observed in this way are termed hybrid data. The depth of air shower maximum is related to the mass of the primary particle that generates the shower. This paper reports on shower maxima data collected over 8.5 years using the Black Rock Mesa and Long Ridge fluorescence detectors in conjunction with the array of surface detectors. We compare the means and standard deviations of the observed $X_{\mathrm{max}}$ distributions with Monte Carlo $X_{\mathrm{max}}$ distributions of unmixed protons, helium, nitrogen, and iron, all generated using the QGSJet~II-04 hadronic model. We also perform an unbinned maximum likelihood test of the observed data, which is subjected to variable systematic shifting of the data $X_{\mathrm{max}}$ distributions to allow us to test the full distributions, and compare them to the Monte Carlo to see which elements are not compatible with the observed data. For all energy bins, QGSJet~II-04 protons are found to be compatible with Telescope Array hybrid data at the 95% confidence level after some systematic $X_{\mathrm{max}}$ shifting of the data. Three other QGSJet~II-04 elements are found to be compatible using the same test procedure in an energy range limited to the highest energies where data statistics are sparse., Comment: 39 pages, 18 figures, 5 tables, published in The Astrophysical Journal. This is a peer-reviewed, un-copyedited version of an article published in The Astrophysical Journal. IOP Publishing Ltd is not responsible for any errors or omissions in this version of the manuscript or any version derived from it. The Version of Record is available online at https://doi.org/10.3847/1538-4357/aabad7
Published: 2018
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23. Evidence of Intermediate-Scale Energy Spectrum Anisotropy of Cosmic Rays E$\geq$10$^{19.2}$ eV with the Telescope Array Surface Detector

Author: N. Inoue, M. Ohnishi, R. Sahara, Toru Nakamura, S. Udo, Kenichi Kadota, Maxim Pshirkov, K. Kasahara, M. Abe, Shoichi Kishigami, T. Goto, Toshiyuki Nonaka, Zach Zundel, S. B. Thomas, Fumio Kakimoto, Masaomi Ono, Jyunsei Chiba, Charlie Jui, Dongsu Ryu, B. K. Shin, Hiroshi Yamaoka, Yoshiki Tsunesada, Daisuke Ikeda, Kenta Yashiro, Keitaro Fujita, BayarJon Paul Lubsandorzhiev, Ben Stokes, S. R. Stratton, Y. Takagi, Tiffany Wong, Mayuko Minamino, K. Honda, Masaki Fukushima, H. Tokuno, Yasunori Kitamura, K. Martens, Masato Takita, Hideki Tanaka, Takayuki Tomida, Masaaki Tanaka, J. D. Smith, Fumiya Shibata, Sergey Troitsky, S. Kitamura, R. Ishimori, Keiji Saito, Igor Tkachev, Michiyuki Chikawa, Eiji Kido, M. V. Kuznetsov, D. R. Bergman, H. Oda, Kazuhiro Machida, Hidemi Ito, Pierre Sokolsky, Y. Uchihori, Y. J. Kwon, Hideyuki Ohoka, R. Takeishi, Yasunori Saito, Shigehiro Nagataki, Akitoshi Oshima, T. Matsuyama, Yana Zhezher, T. Suzawa, Shunsuke Ozawa, Shingo Kawana, Yuichiro Tameda, John N. Matthews, Priti Shah, O. Kalashev, Vladim Kuzmin, William Hanlon, J. Ogura, F. Urban, S. Jeong, Isaac Myers, Motoki Hayashi, Peter Tinyakov, J. P. Lundquist, Samuel Blake, Shoichi Ogio, T. Okuda, J. Yang, M. Allen, Y. Omura, Naoaki Hayashida, Koichi Sekino, Elliott Barcikowski, K. Nagasawa, Dmitri Ivanov, Y. Takahashi, Mai Takamura, G. Furlich, Takaaki Ishii, Keijiro Mukai, D. C. Rodriguez, S. Yoshida, Naoto Sakaki, Rasha Abbasi, Kiyoshi Tanaka, John Belz, R. Azuma, Inkyu Park, L. M. Scott, A. Nozato, Y. Hayashi, K. Kawata, Hideaki Shimodaira, Hyoming Jeong, K. H. Lee, Tareq Abu-Zayyad, Hiroyuki Sagawa, T.-A. Shibata, R. Yamane, Gordon Thomson, Ryo Nakamura, Tom Stroman, Robert Cady, Hongsu Kim, Akimichi Taketa, Grigory Rubtsov, M. Yamamoto, H. Yoshii, Nobuyuki Sakurai, K. Yamazaki, Takahiro Fujii, Ryota Onogi, J. H. Kim, A. Di Matteo, B. G. Cheon, R. Mayta, K. Hibino, S. Kawakami, Heungsu Shin, K. Tsutsumi, H. Kawai, T. Seki, and Y. Yoneda
Subjects: Astroparticle physics, Physics, High Energy Astrophysical Phenomena (astro-ph.HE), 010308 nuclear & particles physics, Detector, Monte Carlo method, Isotropy, FOS: Physical sciences, Astronomy and Astrophysics, Cosmic ray, Astrophysics, Poisson distribution, 01 natural sciences, law.invention, Telescope, symbols.namesake, Space and Planetary Science, law, 0103 physical sciences, symbols, Anisotropy, Astrophysics - High Energy Astrophysical Phenomena, 010303 astronomy & astrophysics
Abstract: An intermediate-scale energy spectrum anisotropy has been found in the arrival directions of ultra-high energy cosmic rays of energies above $10^{19.2}$ eV in the northern hemisphere, using 7 years of data from the Telescope Array surface detector. A relative energy distribution test is done comparing events inside oversampled spherical caps of equal exposure, to those outside, using the Poisson likelihood ratio. The center of maximum significance is at $9^h$$16^m$, $45^{\circ}$. and has a deficit of events with energies $10^{19.2}$$\leq$$E$$
Published: 2018
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24. Constraints on the diffuse photon flux with energies above $10^{18}$ eV using the surface detector of the Telescope Array experiment

Author: Rasha Abbasi, Fumiya Shibata, S. Yoshida, T. Matsuyama, S. Ozawa, Naoto Sakaki, Yasunori Saito, John Belz, K. Nagasawa, R. Ishimori, S. Kitamura, Hidemi Ito, Ryo Nakamura, Motoki Hayashi, Toshiyuki Nonaka, Hideki Tanaka, Kazuo Saito, J. P. Lundquist, M. Yamamoto, Ben Stokes, B. G. Cheon, Heungsu Shin, T. Suzawa, Yuichiro Tameda, Isaac Myers, Inkyu Park, John N. Matthews, Douglas Bergman, Nobuyuki Sakurai, Ryota Onogi, A. Di Matteo, Koichi Sekino, M. Allen, R. Mayta, Y. Zhezher, Grigory Rubtsov, Kenta Yashiro, K. Martens, K. Tsutsumi, Keitaro Fujita, Y. Takahashi, Mai Takamura, L. M. Scott, H. Yoshii, Daisuke Ikeda, Eiji Kido, M. V. Kuznetsov, S. Kawakami, Y. Uchihori, R. Azuma, Toshitsugu Fujii, Kazuhiro Machida, S. R. Stratton, Y. Hayashi, Sergey Troitsky, B. K. Shin, Oleg Kalashev, Hongsu Kim, Hiroyuki Sagawa, Tiffany Wong, R. Takeishi, Charlie Jui, J. Remington, Pierre Sokolsky, K. Kawata, Masaki Fukushima, Akimichi Taketa, G. Furlich, Takaaki Ishii, J. H. Kim, BayarJon Paul Lubsandorzhiev, M. Takeda, Shigehiro Nagataki, Mayuko Minamino, Hideaki Shimodaira, Hyoming Jeong, D. C. Rodriguez, H. Kawai, Y. Omura, Kiyoshi Tanaka, K. Kasahara, K. Honda, Akitoshi Oshima, Y. Tsunesada, Shoichi Kishigami, Yasunori Kitamura, Naoaki Hayashida, Masaaki Tanaka, T. Seki, Masato Takita, J. Ogura, H. Yamaoka, Masaomi Ono, R. Sahara, Michiyuki Chikawa, Y. Yoneda, N. Inoue, Jyunsei Chiba, K. Hibino, Shingo Kawana, Fumio Kakimoto, Dongsu Ryu, K. Yamazaki, Tareq Abu-Zayyad, R. Yamane, Maksim Piskunov, William Hanlon, M. Ohnishi, Takayuki Tomida, Y. Takagi, T. Okuda, J. Yang, Federico R. Urban, Toru Nakamura, S. Udo, K. H. Lee, Kenichi Kadota, T.-A. Shibata, H. Tokuno, Zach Zundel, J. D. Smith, Priti Shah, Gordon Thomson, S. B. Thomas, Tom Stroman, Robert Cady, Igor Tkachev, Maxim Pshirkov, Elliott Barcikowski, Dmitri Ivanov, H. Oda, Keijiro Mukai, Peter Tinyakov, Samuel Blake, Shoichi Ogio, Vladim Kuzmin, T. Goto, S. Jeong, M. Abe, Y. J. Kwon, and Hideyuki Ohoka
Subjects: Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Muon, Photon, 010308 nuclear & particles physics, Detector, FOS: Physical sciences, Astronomy and Astrophysics, Curvature, 01 natural sciences, Computational physics, law.invention, High Energy Physics - Experiment, Telescope, High Energy Physics - Phenomenology, High Energy Physics - Experiment (hep-ex), Air shower, Distribution function, High Energy Physics - Phenomenology (hep-ph), law, 0103 physical sciences, Waveform, Astrophysics - High Energy Astrophysical Phenomena, 010303 astronomy & astrophysics
Abstract: We present the results of the search for ultra-high-energy photons with nine years of data from the Telescope Array surface detector. A multivariate classifier is built upon 16 reconstructed parameters of the extensive air shower. These parameters are related to the curvature and the width of the shower front, the steepness of the lateral distribution function, and the timing parameters of the waveforms sensitive to the shower muon content. A total number of two photon candidates found in the search is fully compatible with the expected background. The $95\%\,$CL limits on the diffuse flux of the photons with energies greater than $10^{18.0}$, $10^{18.5}$, $10^{19.0}$, $10^{19.5}$ and $10^{20.0}$ eV are set at the level of $0.067$, $0.012$, $0.0036$, $0.0013$, $0.0013~\mbox{km}^{-2}\mbox{yr}^{-1}\mbox{sr}^{-1}$ correspondingly., Comment: 7 pages, 2 figures
Published: 2018
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25. EUSO-TA - First results from a ground-based EUSO telescope

Author: N. Inoue, L. del Peral, A. Franceschi, E. Parizot, Pavol Bobik, M. Haiduc, Lech Wiktor Piotrowski, S. Bartocci, J. A. Morales de los Ríos, N. Belkhalfa, Susumu Inoue, S. Yoshida, J. Szabelski, S. B. Thomas, K. Kudela, M. D. Rodríguez Frías, Naoto Sakaki, Z. Plebaniak, Thomas Schanz, Michiyuki Chikawa, M. Di Martino, A. Marini, Toshikazu Ebisuzaki, G. Roudil, B. Harlov, J. F. Valdés-Galicia, G. Osteria, Carlo Vigorito, L. G. Tkachev, Josef Jochum, S. Naitamor, G. Vankova, A. Caramete, Livio Conti, K. Martens, D. Maravilla, L. López Campano, J. Fernández-Soriano, R. Matev, Yoshihiko Mizumoto, Sebastián Franchini, S. Biktemerova, A. Ebersoldt, Daisuke Ikeda, A. Zuccaro Marchi, Hajime Takami, Masaki Fukushima, E. G. Judd, O. Larsson, H. J. Crawford, M. Serra, Jörn Wilms, J. Karczmarczyk, M. Ave Pernas, D. Kolev, H. Krantz, Mohammed Bakiri, Luis A. Anchordoqui, I. Kaneko, O. A. Saprykin, Estíbaliz Gascón, S. Turriziani, A. Belov, Valerie Connaughton, L. Marcelli, Konstantin Belov, A. Anzalone, T. Napolitano, Toshitaka Kajino, Francesco Fenu, N. Tone, Christer Fuglesang, Humberto Ibarguen Salazar, K. Benmessai, A. Guzmán, C. Lachaud, Daisuke Yonetoku, J. Blecki, José Meseguer, Angel Sanz-Andrés, Shinsuke Abe, P. Galeotti, R. Attallah, J. Hernández Carretero, H. Tokuno, B. Beldjilali, Takayuki Tomida, Santiago Pindado, S. Jeong, T. Shirahama, Y. Tsunesada, Junpei Fujimoto, M. Yu. Zotov, Silvia Ferrarese, Katsuaki Asano, Alfonso Monaco, H. Attoui, E. M. Popescu, B. A. Khrenov, A. Pagliaro, J. Genci, L. Villaseñor, C. Tenzer, T. Sugiyama, Piergiorgio Picozza, R. Tsenov, Satoshi Wada, N. Mebarki, W. Painter, Piotr Orleanski, T. Paul, A. Pollini, Pavel Klimov, B. Panico, Y. Karadzhov, Isabel Pérez-Grande, F. Sarazin, Zbigniew Wlodarczyk, Marc Weber, F. Bisconti, C. González Alvarado, Tokonatsu Yamamoto, E. Bozzo, T. Ogawa, M. C. Talai, J.N. Capdevielle, G. Sáez Cano, Angela V. Olinto, Javier Licandro, M. Rezazadeh, Andrea Santangelo, A. Kusenko, Katsuhiko Tsuno, Yoshio Arai, I. Kreykenbohm, Pierre Sokolsky, G. Masciantonio, Y. Martín, S. Selmane, John Belz, L. Placidi, M. Kleifges, P. L. Biermann, Tomás Belenguer, Yoshitaka Itow, N. Tajima, Giuseppe Giraudo, M. Takeda, M. A. Mendoza, G. Medina-Tanco, Shigehiro Nagataki, Barbara Szabelska, T. Peter, O. Martinez, Gordon Thomson, Toshiyuki Nonaka, F. Ronga, Gustavo Alonso, J. Watanabe, J. Tubbs, I. Rusinov, I. V. Yashin, M. Fouka, Osvaldo Catalano, M. Martucci, Fausto Guarino, J. Yang, P. von Ballmoos, M. Ricci, H. Miyamoto, M. Sanz Palomino, S. E. Csorna, Amine Ahriche, Simona Toscano, A. Bruno, Jeong-Sook Kim, Kenji Shinozaki, L. Caramete, Marcos Reyes, Roberto Bellotti, K. Mase, Gali Garipov, Joowon Lee, M. Flamini, B. Vlcek, T. Patzak, James H. Adams, H. Prieto, N. Blanc, R. Cremonini, S. Dagoret-Campagne, Francesca Capel, Y. Takizawa, S. Mackovjak, J. L. Marcos, E. Kuznetsov, G. Puehlhofer, D. Supanitsky, R. Weigand Muñoz, P. Gorodetzky, Shoichi Ogio, Johannes Eser, P. Baragatti, Austin Cummings, M. Wille, Y. Uchihori, A. La Barbera, Guillaume Prévôt, S. Blin-Bondil, R. Greg, I. Stan, G. Cordero, Malek Mustafa, J. Mimouni, M. Bogomilov, Z. Polonski, D. Campana, H. Khales, L. Allen, F. Lakhdari, F. Kajino, Maciej Rybczyński, Inkyu Park, M. Putis, S. S. Meyer, A. Weindl, Mark Christl, O. Tibolla, S. Pliego, K. Kawai, Akinori Saito, Ovidiu Vaduvescu, Claudio Cassardo, Dmitri Semikoz, Andrés Merino, P. Carlson, Yuichiro Tameda, John N. Matthews, M. Traïche, F. Cafagna, E. Joven, Y. Hachisu, F. Perfetto, Bruno Spataro, B. Pastirčák, Pierre Barrillon, Eduardo García-Ortega, Sergei A. Sharakin, Piero Vallania, R. Young, Yukihiro Takahashi, José Luis Sánchez, M. D. Sabau, M. Suzuki, Marco Casolino, Claudio Fornaro, Mikhail Panasyuk, A. Neronov, Sergio Fernández-González, J. Bayer, M. C. Maccarone, Valentina Scotti, C. de la Taille, A. Kedadra, I. Dutan, I. S. Zgura, G. Cotto, K. Katahira, M. Mahdi, C. De Donato, Soon-Wook Kim, Yoshimasa Kurihara, G. Chiritoi, H. Schieler, A. Jung, A. Haungs, S. Piraino, H. Lahmar, Antonella Castellina, Mitsuteru Sato, T. Jammer, J. Rabanal, G. Abdellaoui, Hajime Yano, Heungsu Shin, R. Nava, Ralph Engel, Takahiro Fujii, Rossella Caruso, Toshiki Tajima, Hitoshi Ohmori, K. S. Caballero, Hiroyuki Sagawa, Yoshiya Kawasaki, A. Radu, A. Menshikov, Hirohiko M. Shimizu, T. Djemil, D. Allard, Alberto Cellino, S. Kalli, J. Watts, M. E. Bertaina, C. De Santis, L. R. Wiencke, M. Vrabel, P. Prat, Ken'ichi Nomoto, Z. Sahnoune, W. Hidber Cruz, S. Bacholle, Francesco Isgrò, W. Marszał, J. C. Sanchez Balanzar, AstroParticule et Cosmologie (APC (UMR_7164)), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Organisation de Micro-Électronique Générale Avancée (OMEGA), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Centre National de la Recherche Scientifique (CNRS)-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Abdellaoui, G., Abe, S., Adams, J., Ahriche, A., Allard, D., Allen, L., Alonso, G., Anchordoqui, L., Anzalone, A., Arai, Y., Asano, K., Attallah, R., Attoui, H., Ave Pernas, M., Bacholle, S., Bakiri, M., Baragatti, P., Barrillon, P., Bartocci, S., Bayer, J., Beldjilali, B., Belenguer, T., Belkhalfa, N., Bellotti, R., Belov, A., Belov, K., Belz, J. W., Benmessai, K., Bertaina, M., Biermann, P. L., Biktemerova, S., Bisconti, F., Blanc, N., Blecki, J., Blin-Bondil, S., Bobik, P., Bogomilov, M., Bozzo, E., Bruno, A., Caballero, K. S., Cafagna, F., Campana, D., Capdevielle, J-N., Capel, F., Caramete, A., Caramete, L., Carlson, P., Caruso, R., Casolino, M., Cassardo, C., Castellina, A., Catalano, O., Cellino, A., Chikawa, M., Chiritoi, G., Christl, M. J., Connaughton, V., Conti, L., Cordero, G., Cotto, G., Crawford, H. J., Cremonini, R., Csorna, S., Cummings, A., Dagoret-Campagne, S., De Donato, C., de la Taille, C., De Santis, C., del Peral, L., Di Martino, M., Djemil, T., Dutan, I., Ebersoldt, A., Ebisuzaki, T., Engel, R., Eser, J., Fenu, F., Fernández-González, S., Fernández-Soriano, J., Ferrarese, S., Flamini, M., Fornaro, C., Fouka, M., Franceschi, A., Franchini, S., Fuglesang, C., Fujii, T., Fujimoto, J., Fukushima, M., Galeotti, P., García-Ortega, E., Garipov, G., Gascón, E., Genci, J., Giraudo, G., González Alvarado, C., Gorodetzky, P., Greg, R., Guarino, F., Guzmán, A., Hachisu, Y., Haiduc, M., Harlov, B., Haungs, A., Hernández Carretero, J., Hidber Cruz, W., Ikeda, D., Inoue, N., Inoue, S., Isgrò, F., Itow, Y., Jammer, T., Jeong, S., Joven, E., Judd, E., Jung, A., Jochum, J., Kajino, F., Kajino, T., Kalli, S., Kaneko, I., Karadzhov, Y., Karczmarczyk, J., Katahira, K., Kawai, K., Kawasaki, Y., Kedadra, A., Khales, H., Khrenov, B. A., Kim, Jeong-Sook, Kim, Soon-Wook, Kleifges, M., Klimov, P. A., Kolev, D., Krantz, H., Kreykenbohm, I., Kudela, K., Kurihara, Y., Kusenko, A., Kuznetsov, E., La Barbera, A., Lachaud, C., Lahmar, H., Lakhdari, F., Larsson, O., Lee, J., Licandro, J., López Campano, L., Maccarone, M. C., Mackovjak, S., Mahdi, M., Maravilla, D., Marcelli, L., Marcos, J., Marini, A., Marszal, W., Martens, K., Martín, Y., Martinez, O., Martucci, M., Masciantonio, G., Mase, K., Mustafa, M., Matev, R., Matthews, J., Mebarki, N., Medina-Tanco, G., Mendoza, M. A., Menshikov, A., Merino, A., Meseguer, J., Meyer, S. S., Mimouni, J., Miyamoto, H., Mizumoto, Y., Monaco, A., Morales de los Ríos, J. A., Nagataki, S., Naitamor, S., Napolitano, T., Nava, R., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A. V., Orleański, P., Osteria, G., Pagliaro, A., Painter, W., Panasyuk, M. I., Panico, B., Parizot, E., Park, I. H., Pastircak, B., Patzak, T., Paul, T., Pérez-Grande, I., Perfetto, F., Peter, T., Picozza, P., Pindado, S., Piotrowski, L. W., Piraino, S., Placidi, L., Plebaniak, Z., Pliego, S., Pollini, A., Polonski, Z., Popescu, E. M., Prat, P., Prévôt, G., Prieto, H., Puehlhofer, G., Putis, M., Rabanal, J., Radu, A. A., Reyes, M., Rezazadeh, M., Ricci, M., Rodríguez Frías, M. D., Ronga, F., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M., Sáez Cano, G., Sagawa, H., Sahnoune, Z., Saito, A., Sakaki, N., Salazar, H., Sanchez Balanzar, J. C., Sánchez, J. L., Santangelo, A., Sanz-Andrés, A., Sanz Palomino, M., Saprykin, O., Sarazin, F., Sato, M., Schanz, T., Schieler, H., Scotti, V., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shimizu, H. M., Shin, H. S., Shinozaki, K., Shirahama, T., Sokolsky, P., Spataro, B., Stan, I., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Talai, M. C., Tameda, Y., Tenzer, C., Thomas, S. B., Thomson, G. B., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Traïche, M., Tsenov, R., Tsunesada, Y., Tsuno, K., Tubbs, J., Turriziani, S., Uchihori, Y., Vaduvescu, O., Valdés-Galicia, J. F., Vallania, P., Vankova, G., Vigorito, C., Villaseñor, L., Vlcek, B., von Ballmoos, P., Vrabel, M., Wada, S., Watanabe, J., Watts, J., Weber, M., Weigand Muñoz, R., Weindl, A., Wiencke, L., Wille, M., Wilms, J., Włodarczyk, Z., Yamamoto, T., Yang, J., Yano, H., Yashin, I. V., Yonetoku, D., Yoshida, S., Young, R., Zgura, I. S., Zotov, M. Yu., Zuccaro Marchi, A., Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)
Subjects: Fresnel lens, Photomultiplier, Physics::Instrumentation and Detectors, Astrophysics::High Energy Astrophysical Phenomena, Night sky, JEM-EUSO, Cosmic ray, Field of view, Astrophysics::Cosmology and Extragalactic Astrophysics, 7. Clean energy, 01 natural sciences, cosmic rays, EAS, UHECR, Astronomy and Astrophysics, Aeronáutica, law.invention, Telescope, law, 0103 physical sciences, Ultra-high-energy cosmic ray, 010303 astronomy & astrophysics, cosmic ray, Astrophysique, Physics, Fresnel len, 010308 nuclear & particles physics, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, Astronomie, Astronomía, Limiting magnitude, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: EUSO-TA is a ground-based telescope, installed at the Telescope Array (TA) site in Black Rock Mesa, Utah, USA. This is the first detector to successfully use a Fresnel lens based optical system and multi-anode photomultipliers (64 channels per tube, 2304 channels encompassing a 10.6° × 10.6° field of view) for detection of Ultra High Energy Cosmic Rays (UHECR). The telescope is located in front of one of the fluorescence detectors of the TA experiment. Since its installation in 2013, the detector has observed several ultra-high energy cosmic ray events and, in addition, meteors. The limiting magnitude of 5.5 on summed frames (∼ 3 ms) has been established. Measurements of the UV night sky emission in different conditions and moon phases and positions have been completed. The performed observations serve as a proof of concept for the future application of this detector technology., 0, SCOPUS: ar.j, info:eu-repo/semantics/published
Published: 2018
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26. A NORTHERN SKY SURVEY FOR POINT-LIKE SOURCES OF EeV NEUTRAL PARTICLES WITH THE TELESCOPE ARRAY EXPERIMENT

Author: R. Ishimori, R. W. Springer, John Belz, Gordon Thomson, Federico R. Urban, K. Hibino, W. R. Cho, Nobuyuki Sakurai, Tomohiro Matsuda, Pierre Sokolsky, Sergey Troitsky, Masayuki Tanaka, ByongGu Cheon, Yuichiro Tameda, John N. Matthews, Younghoon Kwon, M. J. Chae, K. Martens, Y. Yoneda, S. I. Lim, Thomas Stroman, M. Ohnishi, S. Kawana, Kenichi Kadota, M. Abe, Il Hung Park, Douglas Bergman, H. Yoshii, S. Kitamura, Tomoyuki Nakamura, Fumio Kakimoto, H. Kawai, S. Udo, C. C. H. Jui, Mayuko Minamino, S. Nagataki, S. Kawakami, A. L. Sampson, K. Oki, Yasunori Kitamura, A. Oshima, Takaaki Ishii, S. B. Thomas, Elliott Barcikowski, Hirotaka Ito, Maxim Pshirkov, Masaomi Ono, K. Nagasawa, Dmitri Ivanov, Tatsunobu Shibata, Toshio Matsuyama, H. Shimodaira, HangBae Kim, Kenta Yashiro, Kenichi Tanaka, T. Suzawa, H. Tanaka, Isaac Myers, T. Goto, M. Takamura, Hiroyuki Sagawa, Shunsuke Ozawa, Naoya Inoue, K. Tsutsumi, J. Ogura, Priti Shah, B. T. Stokes, Igor Tkachev, Jon Paul Lundquist, Grigory Rubtsov, Akimichi Taketa, Oleg Kalashev, Takayuki Tomida, Masahiro Takeda, Naoaki Hayashida, L. M. Scott, H. Yamaoka, Ken Honda, A. Nozato, Y. Hayashi, V.A. Kuzmin, Zach Zundel, K. Machida, K. Yamazaki, Tareq Abu-Zayyad, R. Yamane, K. Mukai, H. Ohoka, J. Yang, J. Lan, R. Zollinger, B. K. Shin, Yoshiki Tsunesada, Daisuke Ikeda, S. R. Stratton, S. Yoshida, Katsuaki Kasahara, Tiffany Wong, R. Takeishi, Masaki Fukushima, Mark Allen, Masato Takita, Michiyuki Chikawa, Yukio Uchihori, Takahiro Fujii, Peter Tinyakov, Samuel Blake, Shoichi Ogio, J. H. Kim, Kazumasa Kawata, R. Azuma, J. D. Smith, D. Rodriguez, H. Tokuno, Eiji Kido, Toshiyuki Nonaka, Ruth A. Anderson, William Hanlon, Rasha Abbasi, Robert Cady, T. Okuda, G. Vasiloff, Jyunsei Chiba, Dongsu Ryu, and Fumiya Shibata
Subjects: Physics, High Energy Astrophysical Phenomena (astro-ph.HE), media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, Astrophysics::Instrumentation and Methods for Astrophysics, Flux, FOS: Physical sciences, Astronomy and Astrophysics, Astrophysics, Astrophysics::Cosmology and Extragalactic Astrophysics, Scintillator, Coincidence, law.invention, Telescope, Space and Planetary Science, Neutron flux, Sky, law, Astrophysics - High Energy Astrophysical Phenomena, Order of magnitude, Astrophysics::Galaxy Astrophysics, Fermi Gamma-ray Space Telescope, media_common
Abstract: We report on the search for steady point-like sources of neutral particles around 10$^{18}$ eV between 2008 May and 2013 May with the scintillator surface detector of the Telescope Array experiment. We found overall no significant point-like excess above 0.5 EeV in the northern sky. Subsequently, we also searched for coincidence with the Fermi bright Galactic sources. No significant coincidence was found within the statistical uncertainty. Hence, we set an upper limit on the neutron flux that corresponds to an averaged flux of 0.07 km$^{-2}$ yr$^{-1}$ for $E>1$ EeV in the northern sky at the 95% confidence level. This is the most stringent flux upper limit in a northern sky survey assuming point-like sources. The upper limit at the 95% confidence level on the neutron flux from Cygnus X-3 is also set to 0.2 km$^{-2}$ yr$^{-1}$ for $E>0.5$ EeV. This is an order of magnitude lower than previous flux measurements., 27 pages, 10 figures, 3 tables, accepted for publication in the Astrophysical Journal
Published: 2015

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

Author: S. Y. Roh, S. Yoshida, T. Kanbe, John Belz, Y. Murano, Thomas Stroman, Akitoshi Oshima, R. Zollinger, S. Kitamura, K. Nagasawa, Takayuki Tomida, Michiyuki Chikawa, Isaac Myers, H. Tokuno, K. Kitamoto, R. W. Springer, Igor Tkachev, R. Cady, Elliott Barcikowski, R. Aida, Eiji Kido, Toshiyuki Nonaka, Dmitri Ivanov, H. Fujii, H. Tanaka, Byung Gu Cheon, Yukio Uchihori, J. H. Kim, Pierre Sokolsky, Naoya Inoue, T. Fujii, Mayuko Minamino, Tatsunobu Shibata, Tomohiro Matsuda, Ross Anderson, Peter Tinyakov, Yasunori Kitamura, Samuel Blake, Shoichi Ogio, Toshio Matsuyama, K. Kobayashi, X. Zhou, Y. Yoneda, K. Tsutsumi, S. I. Lim, Zach Zundel, Sergey Troitsky, S. Machida, K. Martens, Hirotaka Ito, Younghoon Kwon, Shunsuke Ozawa, Mark Allen, S. Udo, C. C. H. Jui, Hiroyuki Sagawa, S. Kawana, H. Kawai, E. J. Cho, H. Shimodaira, M. Tanaka, S. Iwamoto, Y. Kondo, K. Oki, Tomoyuki Nakamura, S. Kawakami, Masaomi Ono, S. B. Thomas, S. Nagataki, Naoaki Hayashida, K. Miyata, R. Azuma, T. Matsuura, Fumiya Shibata, Y. Tsuyuguchi, Jon Paul Lundquist, Yoji Kobayashi, Kiyoshi Kuramoto, T. Shirahama, Takaaki Ishii, Gordon Thomson, B. T. Stokes, Yoshiki Tsunesada, K. Hibino, R. Ishimori, Daisuke Ikeda, S. R. Stratton, H. Yamaoka, Grigory Rubtsov, K. Hayashi, Hang Bae Kim, Katsuaki Kasahara, Akimichi Taketa, Tiffany Wong, T. Fukuda, Kenichi Tanaka, Masaki Fukushima, A. L. Sampson, S. Suzuki, Hyun-Il Kim, Douglas Bergman, Federico R. Urban, Masato Takita, Nobuyuki Sakurai, D. Oku, K. Hiyama, H. Yoshii, William Hanlon, Yukio Takahashi, G. Vasiloff, K. Ikuta, J. I. Shin, T. Okuda, Jyunsei Chiba, Maxim Pshirkov, Dongsu Ryu, Fumio Kakimoto, Y. Yamakawa, S. W. Nam, H. Ukai, Priti Shah, T. Iguchi, J. D. Smith, D. Rodriguez, Masahiro Takeda, Ken Honda, Yuichiro Tameda, John N. Matthews, M. Ohnishi, L. M. Scott, Y. Hayashi, V.A. Kuzmin, B. K. Shin, K. Yamazaki, Tareq Abu-Zayyad, R. Yamane, H. Ohoka, J. Yang, J. Lan, W. R. Cho, Kenichi Kadota, Il Hung Park, Y. Wada, and Oleg Kalashev
Subjects: Physics, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astronomy and Astrophysics, Cosmic ray, Astrophysics, 7. Clean energy, Spectral line, Computational physics, law.invention, Telescope, Air shower, law, Energy spectrum, Ultra-high-energy cosmic ray
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.
Published: 2015

28. The Telescope Array Low-energy Extension

Author: Hiroyuki Sagawa, Ryosuke Saharaa, Yoshiki Tsunesada, S. Udo, Toshiyuki Nonaka, Yuichi Takahashia, Shoichi Kishigamia, Masahiro Takeda, and Shoichi Ogio
Subjects: Telescope, Physics, Scintillation, Low energy, Air shower, Optics, law, business.industry, Detector, Ultra-high-energy cosmic ray, business, law.invention
Abstract: The Telescope Array Low-energy Extension (TALE) experiment is a hybrid air shower detector for observation of air showers produced by very high energy cosmic rays above $10^{16.5}$~eV. TALE is located at the Telescope Array (TA) experiment site in the weste rn desert of Utah, USA. TALE has a Surface Detector (SD) array made up of 103 scintillation coun ters (40 with 400 m spacing, 36 with 600 m spacing and 27 with 1.2 km spacing) a nd a Fluorescence Detector (FD) station consisting of 10 FD telescopes located a t the Telescope Array Middle Drum FD station, which is made up of 14 telescopes. TALE-FD full operation started in 2013. The deployment of the 103 SDs was completed in March 2017, and to date a bout 70~$\%$ of the array is in operation with a full triggering and DAQ system. Here we report an overview of the experiment, its capabilities and the t echnical details of the TALE SD trigger and DAQ system from 4 month's operation.
Published: 2017
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29. Gain monitoring of telescope array photomultiplier cameras for the first 4 years of operation

Author: Y. Uchihori, X. Zhou, B. G. Cheon, Takaaki Ishii, T. Kanbe, Robert M. Anderson, J. Martineau, D. C. Rodriguez, Grigory Rubtsov, Isaac Myers, Y. Kobayashi, A. L. Sampson, S. Kawakami, H. Yoshii, K. Tsutsumi, H. Tokuno, Yuichiro Tameda, John N. Matthews, L. M. Scott, Y. Hayashi, Hiroyuki Sagawa, J. D. Smith, Takayuki Tomida, K. Kitamoto, R. Azuma, T. Matsuura, Mayuko Minamino, K. Honda, Yasunori Kitamura, S. Yoshida, Vladim Kuzmin, R. Zollinger, R. Aida, Masaaki Tanaka, Hideaki Shimodaira, K. Hibino, Yoshiki Tsunesada, K. Yamazaki, Daisuke Ikeda, Fumiya Shibata, Tareq Abu-Zayyad, R. Yamane, R. Ishimori, S. R. Stratton, Ben Stokes, Tiffany Wong, T.-A. Shibata, Gordon Thomson, Tom Stroman, Robert Cady, T. Fukuda, Takeshi Okuda, Igor Tkachev, Masaki Fukushima, T. Shirahama, S. Y. Roh, Hyun-Il Kim, S. Kitamura, M. Allen, T. Matsuyama, Samuel Blake, E. J. Cho, Y. Kondo, Shoichi Ogio, K. Oki, Michiyuki Chikawa, Inkyu Park, K. Nagasawa, Shingo Kawana, T. Fujii, Eiji Kido, William Hanlon, Sergey Troitsky, S. Machida, R. W. Springer, J. I. Shin, Naoaki Hayashida, Y. Tsuyuguchi, Maxim Pshirkov, Kiyoshi Tanaka, Elliott Barcikowski, Dmitri Ivanov, H. Fujii, K. Hayashi, H. Kawai, K. Kasahara, Fumio Kakimoto, Tomohiro Matsuda, K. Ikuta, Nobuyuki Sakurai, Akitoshi Oshima, K. Kobayashi, Shunsuke Ozawa, John Belz, Y. Murano, Pierre Sokolsky, M. Takeda, Shigehiro Nagataki, K. Kuramoto, Yasuhiro H. Takahashi, Masato Takita, Zach Zundel, O. Kalashev, T. Iguchi, M. Wood, P. Tinyakov, Y. Yamakawa, K. Martens, Hideki Tanaka, Y. J. Kwon, Toshiyuki Nonaka, Hiroshi Yamaoka, Hideyuki Ohoka, J. Yang, H. Ukai, Priti Shah, K. Miyata, Hongsu Kim, Bokkyun Shin, Akimichi Taketa, S. Suzuki, Douglas Bergman, D. Oku, K. Hiyama, Y. Yoneda, N. Inoue, S. I. Lim, M. Ohnishi, S. Udo, C. C. H. Jui, S. B. Thomas, S. W. Nam, W. R. Cho, Toru Nakamura, Kenichi Kadota, Y. Wada, T. J. Sonley, S. Iwamoto, G. Vasiloff, Jyunsei Chiba, Dongsu Ryu, and J. H. Kim
Subjects: Physics, Telescope, Nuclear and High Energy Physics, Photomultiplier, Optics, business.industry, law, Night sky, Optoelectronics, Scintillator, business, Instrumentation, law.invention
Abstract: The stability of the gain of the photomultiplier (PMT) camera for the Fluorescence Detector (FD) of the Telescope Array experiment was monitored using an 241 Am loaded scintillator pulsers (YAP) and a diffused xenon flasher (TXF) for a selected set of 35 PMT-readout channels. From the monitoring of YAP pulses over four years of FD operation, we found slow monotonic drifts of PMT gains at a rate of −1.7~+1.7%/year. An average of the PMT gains over the 35 channels stayed nearly constant with a rate of change measured at −0.01±0.31(stat)±0.21(sys)%/year. No systematic decrease of the PMT gain caused by the night sky background was observed. Monitoring by the TXF also tracked the PMT gain drift of the YAP at 0.88±0.14(stat)%/year.
Published: 2014
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30. The energy spectrum of ultra-high-energy cosmic rays measured by the Telescope Array FADC fluorescence detectors in monocular mode

Author: T. Kanbe, Y. Kobayashi, Fumiya Shibata, S. Kitamura, Robert M. Anderson, R. Ishimori, Hidemi Ito, Sergey Troitsky, Grigory Rubtsov, Isaac Myers, T. Matsuyama, Y. Yamakawa, S. Yoshida, H. Ukai, Priti Shah, Yuichiro Tameda, S. Suzuki, Taka Tomida, T. Shirahama, John N. Matthews, Douglas Bergman, Pierre Sokolsky, R. Zollinger, D. Oku, K. Hiyama, Y. J. Kwon, Hiroyuki Sagawa, K. Ikuta, Hideyuki Ohoka, Hideaki Shimodaira, M. Takeda, J. H. Kim, M. Allen, T. J. Sonley, Shigehiro Nagataki, K. Oki, Charlie Jui, J. Ogura, Y. Kondo, Akimichi Taketa, Naoaki Hayashida, Y. Tsuyuguchi, K. Kasahara, K. Kitamoto, J. P. Lundquist, Takaaki Ishii, Toshiyuki Nonaka, Mayuko Minamino, K. Honda, S. Y. Roh, B. G. Cheon, Takeshi Okuda, Igor Tkachev, T. Iguchi, A. L. Sampson, D. C. Rodriguez, S. Iwamoto, John Belz, Inkyu Park, K. Miyata, Masaomi Ono, J. I. Shin, Yasunori Kitamura, K. Yamazaki, Bokkyun Shin, S. Kawakami, Y. Murano, Tareq Abu-Zayyad, Vladim Kuzmin, R. Yamane, T. Fujii, K. Tsutsumi, Hiroshi Yamaoka, R. Aida, Masaaki Tanaka, G. Vasiloff, R. Azuma, T. Matsuura, Elliott Barcikowski, T.-A. Shibata, L. M. Scott, K. Hibino, Jyunsei Chiba, Dongsu Ryu, Gordon Thomson, Tom Stroman, Robert Cady, Y. Hayashi, Hongsu Kim, Dmitri Ivanov, H. Fujii, Y. Uchihori, O. Kalashev, W. R. Cho, H. Kawai, Hyun-Il Kim, Kiyoshi Tanaka, H. Yoshii, Eiji Kido, Yoshiki Tsunesada, K. Kuramoto, Y. Yoneda, N. Inoue, S. I. Lim, Daisuke Ikeda, Toru Nakamura, Kenichi Kadota, S. R. Stratton, M. Ohnishi, S. Machida, S. Udo, J. Yang, Y. Wada, Tiffany Wong, J. Lan, S. B. Thomas, Nobuyuki Sakurai, S. W. Nam, T. Fukuda, Masaki Fukushima, Peter Tinyakov, Samuel Blake, Shoichi Ogio, E. J. Cho, Michiyuki Chikawa, Yasuhiro H. Takahashi, Zach Zundel, Masato Takita, K. Martens, Hideki Tanaka, H. Tokuno, J. D. Smith, R. W. Springer, Tomohiro Matsuda, K. Kobayashi, Shingo Kawana, William Hanlon, Maxim Pshirkov, K. Hayashi, Fumio Kakimoto, Akitoshi Oshima, Shunsuke Ozawa, and Ben Stokes
Subjects: Astroparticle physics, Physics, business.industry, Aperture, Monte Carlo method, Detector, Astronomy and Astrophysics, Cosmic ray, law.invention, Telescope, Optics, law, Ultra-high-energy cosmic ray, business, Event reconstruction
Abstract: We present a measurement of the energy spectrum of ultra-high-energy cosmic rays performed by the Telescope Array experiment using monocular observations from its two new FADC-based fluorescence detectors. After a short description of the experiment, we describe the data analysis and event reconstruction procedures. Since the aperture of the experiment must be calculated by Monte Carlo simulation, we describe this calculation and the comparisons of simulated and real data used to verify the validity of the aperture calculation. Finally, we present the energy spectrum calculated from the merged monocular data sets of the two FADC-based detectors, and also the combination of this merged spectrum with an independent, previously published monocular spectrum measurement performed by Telescope Array’s third fluorescence detector [T. Abu-Zayyad et al., The energy spectrum of Telescope Array’s middle drum detector and the direct comparison to the high resolution fly’s eye experiment, Astroparticle Physics 39 (2012) 109-119, http://dx.doi.org/10.1016/j.astropartphys.2012.05.012 , Available from: ]. This combined spectrum corroborates the recently published Telescope Array surface detector spectrum [T. Abu-Zayyad, et al., The cosmic-ray energy spectrum observed with the surface detector of the Telescope Array experiment, ApJ 768 (2013) L1, http://dx.doi.org/10.1088/2041-8205/768/1/L1 , Available from: ] with independent systematic uncertainties.
Published: 2013
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31. Cosmic ray oriented performance studies for the JEM-EUSO first level trigger

Author: H. Sato, T. Djemil, Alberto Cellino, Octavian Micu, Javier Licandro, M. D. Rodríguez Frías, Z. Plebaniak, N. Guardone, Katsuhiko Tsuno, A. Belov, L. R. Wiencke, N. Tone, G. Cordero, A. Anzalone, T. Napolitano, Michiyuki Chikawa, Katsuaki Asano, A. Ebersoldt, Daisuke Yonetoku, I. S. Zgura, Roberto Bellotti, M. Mahdi, T. Pierog, Yoshimasa Kurihara, H. Schieler, E. M. Popescu, Antonella Castellina, Mitsuteru Sato, T. Jammer, K. S. Caballero, Hiroyuki Sagawa, Christer Fuglesang, J. Watanabe, G. Roudil, K. Mase, Graciela B. Gelmini, G. Chiritoi, Y. Hachisu, F. Perfetto, Y. Yamamoto, B. Pastirčák, J. Geary, H. Khales, José Meseguer, Angel Sanz-Andrés, Osvaldo Catalano, Santiago Pindado, Junpei Fujimoto, B. A. Khrenov, S. Pliego, Thomas J. Weiler, Pierre Barrillon, Eduardo García-Ortega, Sergei A. Sharakin, Massimiliano Bonamente, James H. Adams, Y. Tsunesada, H. Lahmar, Patrick J. Reardon, Toshiki Tajima, G. Siemieniec-Oziȩbło, Satoshi Wada, T. Ogawa, M. Yu. Zotov, J. Genci, Piergiorgio Picozza, N. Mebarki, Mohammed Bakiri, C. Catalano, K. Benmessai, M. Suzuki, Valentina Scotti, Hitoshi Ohmori, G. Abdellaoui, Francesco Isgrò, Daisuke Ikeda, Belkacem Benadda, W. Painter, P. Gorodetzky, Yoshiya Kawasaki, E. Kuznetsov, Yoshihiko Mizumoto, R. Bechini, M. C. Talai, C. De La Taille, K. Shinozaki, A. Radu, F.J. Ronga, Alfonso Monaco, Shinsuke Abe, B. Nadji, E. Parizot, A. Guzmán, Toshitaka Kajino, K. Kawai, Ralph Engel, I. Kreykenbohm, Hajime Takami, Angela V. Olinto, Andrea Santangelo, D. Maravilla, S. Blin-Bondil, D. Allard, Vladimir Andreev, Masaki Fukushima, R. Nava, V. S. Morozenko, Akinori Saito, Maxim Gonchar, Hirohiko M. Shimizu, M. A. Mendoza, E. G. Judd, D. Kang, G. Castellini, Andreas A. Berlind, M. Rezazadeh, S. Selmane, Alexander Kusenko, K. Higashide, C. Moretto, P. Galeotti, Y. Martín, M. E. Bertaina, L. Villaseñor, C. De Santis, J. Yang, Rossella Caruso, J. Karczmarczyk, Shigeto Watanabe, Ken'ichi Nomoto, K. Słomińska, H. Attoui, C. Tenzer, F Dulucq, N. Inoue, S. Bacholle, John N. Matthews, Francesca Capel, J. F. Valdés-Galicia, L. G. Tkachev, H. Tahi, G. Vankova, Tokonatsu Yamamoto, Guillaume Prévôt, L. del Peral, A. Franceschi, Pavol Bobik, T. Sugiyama, Hajime Yano, Tadeusz Wibig, B. Mot, S. Dagoret-Campagne, S. Bartocci, E. Bozzo, M. Serra, Luis A. Anchordoqui, T. Shibata, M. Traïche, S. Mackovjak, J. Fernández-Soriano, D. Supanitsky, T. Batsch, Toshio Murakami, R. Young, M. Sakata, S. Biktemerova, Toshikazu Ebisuzaki, Yukihiro Takahashi, José Luis Sánchez, S. Ahmad, C. Lachaud, F. Cafagna, H. J. Crawford, O. Larsson, S. Messaoud, K. Kudela, G. Modestino, E. Joven, M. Rahmani, Giuseppe Giraudo, R. Weigand Muñoz, T. Shirahama, S. A. Djenas, S. Kalli, I. Kaneko, A. Haungs, S. Piraino, J. Watts, Hanna Rothkaehl, J. Mimouni, J. A. Morales de los Ríos, Toshiyuki Nonaka, Ovidiu Vaduvescu, M. Karus, L. Santiago Crúz, M. Bogomilov, Josef Jochum, F. Bisconti, M. Lacombe, Claudio Cassardo, Shoichi Ogio, M. Flamini, Silvia Ferrarese, C. Pennypacker, Marco Casolino, Claudio Fornaro, Susumu Inoue, Tomás Belenguer, J. Błȩcki, L. Mehrad, M. Vrabel, P. Prat, Piotr Orleanski, Ke Fang, Mikhail Panasyuk, F. Kajino, Andrés Merino, Y. Takizawa, M. Fouka, P. L. Biermann, Z. Sahnoune, D. Kolev, H. Lim, J. C. Sanchez, Maciej Rybczyński, G. Sáez Cano, D. Monnier-Ragaigne, A. Segreto, W. Aouimeur, A. Neronov, M. C. Maccarone, B. Harlov, I. Rusinov, P. Carlson, T. Mernik, A. Jung, H. W. Park, R. Boudaoud, M. Dupieux, I. V. Yashin, Carlo Vigorito, Domenico Finco, A. Kedadra, T. Paul, Valerie Connaughton, Marcos Reyes, R. Guehaz, N. Blanc, M. Ave Pernas, T. Nakamura, Yoshio Arai, L. Marcelli, I. Dutan, L. Placidi, A. Sobey, Francesco Fenu, Piero Vallania, S. E. Csorna, G. Masciantonio, G. Medina-Tanco, J. L. Marcos, M. D. Sabau, Johannes Eser, H. Prieto, R. Cremonini, H. Ikeda, Naoto Sakaki, G. Cotto, Markus Roth, C. De Donato, L. López Campano, Sergio Fernández-González, Takayuki Tomida, Nicusor Arsene, J. Bayer, A. Insolia, M. Kleifges, N. Tajima, M. Takeda, Soon-Wook Kim, J. Rabanal, J. Hernández Carretero, Fausto Guarino, P. von Ballmoos, M. Ricci, A. Bruno, M. Unger, Shigehiro Nagataki, K. Katahira, Isabel Pérez-Grande, F. Sarazin, Zbigniew Wlodarczyk, Marc Weber, R. Matev, Simona Toscano, Michael S. Briggs, M. Haiduc, Lech Wiktor Piotrowski, S. Yoshida, J. Szabelski, Estíbaliz Gascón, O. Martinez, T. Patzak, M. Nagata, Dmitry V. Naumov, J.N. Capdevielle, I. Stan, A. Caramete, K. Martens, Konstantin Belov, Joowon Lee, F. Tajima, A. Acheli, J. N. Albert, Thomas Schanz, M. Wille, Livio Conti, Y. Uchihori, A. Zuccaro Marchi, Jörn Wilms, O. A. Saprykin, Sug Whan Kim, F. Kanouni, Sebastián Franchini, Gali Garipov, R. Attallah, D. Campana, F. Lakhdari, Barbara Szabelska, Inkyu Park, M. Putis, Y. Miyazaki, A. Weindl, T. Peter, B. Vlcek, Mark Christl, Gustavo Alonso, O. Tibolla, Jeong Sook Kim, C. González Alvarado, P. Baragatti, H. Miyamoto, M. Manfrin, Yoshitaka Itow, L. Caramete, M. Sanz Palomino, Y. Karadzhov, Amine Ahriche, Humberto Ibarguen Salazar, G. Contino, H. Tokuno, W. Hidber, R. Tsenov, R. Forza, A. Pollini, Pavel Klimov, B. Panico, M. Mignone, M. Di Martino, A. Marini, G. Osteria, D.V. Semikoz, T. Tymieniecka, J. Sledd, M. Nagano, Abdellaoui, G., Abe, S., Acheli, A., Adams, J. H., Ahmad, S., Ahriche, A., Albert, J. N., Allard, D., Alonso, G., Anchordoqui, L., Andreev, V., Anzalone, A., Aouimeur, W., Arai, Y., Arsene, N., Asano, K., Attallah, R., Attoui, H., Ave pernas, M., Bacholle, S., Bakiri, M., Baragatti, P., Barrillon, P., Bartocci, S., Batsch, T., Bayer, J., Bechini, R., Belenguer, T., Bellotti, R., Belov, A., Belov, K., Benadda, B., Benmessai, K., Berlind, A. A., Bertaina, M., Biermann, P. L., Biktemerova, S., Bisconti, F., Blanc, N., Błȩcki, J., Blin Bondil, S., Bobik, P., Bogomilov, M., Bonamente, M., Boudaoud, R., Bozzo, E., Briggs, M. S., Bruno, A., Caballero, K. S., Cafagna, F., Campana, D., Capdevielle, J. N., Capel, F., Caramete, A., Caramete, L., Carlson, P., Caruso, R., Casolino, M., Cassardo, C., Castellina, A., Castellini, G., Catalano, C., Catalano, O., Cellino, A., Chikawa, M., Chiritoi, G., Christl, M. J., Connaughton, V., Conti, L., Contino, G., Cordero, G., Cotto, G., Crawford, H. J., Cremonini, R., Csorna, S., Dagoret Campagne, S., De donato, C., De la taille, C., De santis, C., Del peral, L., Di martino, M., Djemil, T., Djenas, S. A., Dulucq, F., Dupieux, M., Dutan, I., Ebersoldt, A., Ebisuzaki, T., Engel, R., Eser, J., Fang, K., Fenu, F., Fernández González, S., Fernández Soriano, J., Ferrarese, S., Finco, D., Flamini, M., Fornaro, C., Forza, R., Fouka, M., Franceschi, A., Franchini, S., Fuglesang, C., Fujimoto, J., Fukushima, M., Galeotti, P., García Ortega, E., Garipov, G., Gascón, E., Geary, J., Gelmini, G., Genci, J., Giraudo, G., Gonchar, M., González alvarado, C., Gorodetzky, P., Guardone, N., Guarino, Fausto, Guehaz, R., Guzmán, A., Hachisu, Y., Haiduc, M., Harlov, B., Haungs, A., Hernández carretero, J., Hidber, W., Higashide, K., Ikeda, D., Ikeda, H., Inoue, N., Inoue, S., Insolia, A., Isgro', Francesco, Itow, Y., Jammer, T., Joven, E., Judd, E. G., Jung, A., Jochum, J., Kajino, F., Kajino, T., Kalli, S., Kaneko, I., Kang, D., Kanouni, F., Karadzhov, Y., Karczmarczyk, J., Karus, M., Katahira, K., Kawai, K., Kawasaki, Y., Kedadra, A., Khales, H., Khrenov, B. A., Kim, Jeong Sook, Kim, Soon Wook, Kim, Sug Whan, Kleifges, M., Klimov, P. A., Kolev, D., Kreykenbohm, I., Kudela, K., Kurihara, Y., Kusenko, A., Kuznetsov, E., Lacombe, M., Lachaud, C., Lahmar, H., Lakhdari, F., Larsson, O., Lee, J., Licandro, J., Lim, H., López campano, L., Maccarone, M. C., Mackovjak, S., Mahdi, M., Manfrin, M., Maravilla, D., Marcelli, L., Marcos, J. L., Marini, A., Martens, K., Martín, Y., Martinez, O., Masciantonio, G., Mase, K., Matev, R., Matthews, J. N., Mebarki, N., Medina Tanco, G., Mehrad, L., Mendoza, M. A., Merino, A., Mernik, T., Meseguer, J., Messaoud, S., Micu, O., Mignone, M., Mimouni, J., Miyamoto, H., Miyazaki, Y., Mizumoto, Y., Modestino, G., Monaco, A., Monnier Ragaigne, D., Morales de los ríos, J. A., Moretto, C., Morozenko, V. S., Mot, B., Murakami, T., Nadji, B., Nagano, M., Nagata, M., Nagataki, S., Nakamura, T., Napolitano, T., Naumov, D., Nava, R., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A. V., Orleański, P., Osteria, G., Painter, W., Panasyuk, M. I., Panico, B., Parizot, E., Park, I. H., Park, H. W., Pastircak, B., Patzak, T., Paul, T., Pennypacker, C., Pérez Grande, I., Perfetto, Francesco, Peter, T., Picozza, P., Pierog, T., Pindado, S., Piotrowski, L. W., Piraino, S., Placidi, L., Plebaniak, Z., Pliego, S., Pollini, A., Popescu, E. M., Prat, P., Prévôt, G., Prieto, H., Putis, M., Rabanal, J., Radu, A. A., Rahmani, M., Reardon, P., Reyes, M., Rezazadeh, M., Ricci, M., Rodríguez frías, M. D., Ronga, F., Roth, M., Rothkaehl, H., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M. D., Sáez cano, G., Sagawa, H., Sahnoune, Z., Saito, A., Sakaki, N., Sakata, M., Salazar, H., Sanchez, J. C., Sánchez, J. L., Santangelo, A., Santiago crúz, L., Sanz Andrés, A., Sanz palomino, M., Saprykin, O., Sarazin, F., Sato, H., Sato, M., Schanz, T., Schieler, H., Scotti, Valentina, Segreto, A., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shibata, T., Shimizu, H. M., Shinozaki, K., Shirahama, T., Siemieniec Oziȩbło, G., Sledd, J., Słomińska, K., Sobey, A., Stan, I., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tahi, H., Tajima, F., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Talai, M. C., Tenzer, C., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Traïche, M., Tsenov, R., Tsunesada, Y., Tsuno, K., Tymieniecka, T., Uchihori, Y., Unger, M., Vaduvescu, O., Valdés Galicia, J. F., Vallania, P., Vankova, G., Vigorito, C., Villaseñor, L., Vlcek, B., Von ballmoos, P., Vrabel, M., Wada, S., Watanabe, J., Watanabe, S., Watts, J., Weber, M., Weigand muñoz, R., Weindl, A., Weiler, T. J., Wibig, T., Wiencke, L., Wille, M., Wilms, J., Włodarczyk, Z., Yamamoto, T., Yamamoto, Y., Yang, J., Yano, H., Yashin, I. V., Yonetoku, D., Yoshida, S., Young, R., Zgura, I. S., Zotov, M. Y. u., Zuccaro marchi, A., Laboratoire Leprince-Ringuet (LLR), Centre National de la Recherche Scientifique (CNRS)-École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Laboratoire de l'Accélérateur Linéaire (LAL), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut de recherche en astrophysique et planétologie (IRAP), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)
Subjects: Nuclear and High Energy Physics, data analysis method, Instrumentation, Astrophysics::High Energy Astrophysical Phenomena, Night sky, measurement methods, satellite, JEM-EUSO, FPGA, Nightglow background, Trigger system, Cosmic ray, 01 natural sciences, law.invention, Aeronáutica, Telescope, nightglow background, law, 0103 physical sciences, International Space Station, cosmic radiation: UHE, [PHYS.PHYS.PHYS-INS-DET]Physics [physics]/Physics [physics]/Instrumentation and Detectors [physics.ins-det], 010303 astronomy & astrophysics, background: suppression, Remote sensing, Physics, detector: wide-angle, trigger system, laser: pulsed, showers: atmosphere, 010308 nuclear & particles physics, Astrophysics::Instrumentation and Methods for Astrophysics, trigger, Astronomía, Satellite, background: fluctuation, FPGA, JEM-EUSO, Nightglow background, Trigger system, Nuclear and High Energy Physics, Instrumentation, Neutrino, Energy (signal processing), performance
Abstract: 著者人数: 368名 (JAXA職員: 池田, 博一 ; 鈴木, 睦 ; 矢野, 創), Accepted: 2017-05-29, 資料番号: SA1170117000
Published: 2017
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32. Study of Microwave Radiation from the Electron Beam at the Telescope Array Site

Author: Takao Kuwabara, Krijn de Vries, Hiroyuki Sagawa, Aongus Ó Murchadha, Romain Gaïor, B. K. Shin, Tokonatsu Yamamoto, A. Ishihara, Thomas Meures, S. Yoshida, Izumi I.S. Ohta, Kael Hanson, John N. Matthews, Gordon Thomson, Daisuke Ikeda, Shoichi Ogio, K. Mase, Masaki Fukushima, Tatsunobu Shibata, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE (UMR_7585)), and Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS)
Subjects: electron beam, accelerator, Cosmic ray, Electron, Radiation, 01 natural sciences, Radio spectrum, microwaves, electron: accelerator, law.invention, detector: fluorescence, Telescope, Optics, law, 0103 physical sciences, site, electron: beam, 010306 general physics, Physics, radio wave, 010308 nuclear & particles physics, business.industry, Particle accelerator, calibration, cosmic radiation, frequency, atmosphere, Physics::Accelerator Physics, business, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], radio emission, Microwave, Radio wave
Abstract: International audience; The Telescope Array (TA) experiment installed the electron accelerator in order to calibrate the fluorescence detector by shooting 40 MeV electrons into the atmosphere. This accelerator also works to investigate the radio detection techniques used for the cosmic ray observations. Using this accelerator, four experimental groups have studied individual radio detection methods at different frequency bands ranging from 50 MHz to 12 GHz. All of these experiments have observed the microwave radiation from the electron beam itself. We have studied the radiation by combining all the measured results and constructed a model of this phenomena. Results of four experiments and model expectation are in good agreement within the systematic uncertainty.
Published: 2016
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33. Auger at the Telescope Array: Recent Progress Toward a Direct Cross-Calibration of Surface-Detector Stations

Author: R. Cady, P. Mantsch, R. Halliday, Toshiyuki Nonaka, L. Guglielmi, Corbin Covault, John Matthews, T. Trung, Fred Sarazin, Ryan Lorek, P. Lebrun, S. Colognes, B. Genolini, Hiroyuki Sagawa, E. Rauly, Ricardo Sato, B. Courty, John N. Matthews, Shoichi Ogio, M. Marton, O. Wolf, R. Takeishi, P.O. Mazur, Jeffrey A. Johnsen, S. Quinn, Toshihiro Fujii, AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université de Paris (UP), Institut de Physique Nucléaire d'Orsay (IPNO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP ), Université Grenoble Alpes (UGA), Pierre Auger, Telescope Array, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Centre National de la Recherche Scientifique (CNRS)-Université Paris Cité (UPCité), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes [2016-2019] (UGA [2016-2019]), Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, and PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)
Subjects: air, data acquisition, Auger, law.invention, detector: fluorescence, Telescope, Data acquisition, Observatory, law, Calibration, hardware, (cross) calibration, Remote sensing, Pierre Auger Observatory, Physics, instrumentation, cosmic radiation: energy spectrum, hybrid, showers: atmosphere, detector: surface, Detector, sensitivity, calibration, laser, observatory, Central Laser Facility, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: International audience; Since 2007 the Telescope Array Project (TA) and the Pierre Auger Observatory (Auger) have collected extensive data sets spanning several orders of magnitude in energy of the cosmic-ray spectrum. In both experiments the bulk of data is generated from the surface-detector (SD) array, which is energetically calibrated with fluorescence detectors using a hybrid approach. However, each experiment has implemented a different SD station design, resulting in different sensitivities of extensive air-shower channels. Understanding these differences and any potential unforeseen systematic errors is essential for future joint analyses. In this paper we present an update on the progress of an in-situ cross-calibration program. We focus on recent hardware installations which enable the read out of co-located Auger and TA SD stations at the TA central laser facility (CLF). We also present a preliminary analysis of event signals observed at the CLF.
Published: 2016
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34. Performance and Operational Status of Muon Detectors in the Telescope Array Experiment

Author: Takeshi Okuda, Hiroyuki Sagawa, Naoki Sakurai, Dmitri Ivanov, Toshiyuki Nonaka, Ben Stokes, Shoichi Ogio, Robert Cady, John N. Matthews, and R. Takeishi
Subjects: Telescope, Physics, Optics, law, business.industry, business, law.invention, Muon detector
Published: 2016
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35. Calibration of photomultiplier tubes for the fluorescence detector of telescope array experiment using a Rayleigh scattered laser beam

Author: S. Udo, Nobuyuki Sakurai, Hiroyuki Sagawa, N. Inoue, Akimichi Taketa, Lawrence Wiencke, Stan B. Thomas, Toshihiro Fujii, John N. Matthews, S. Kawana, Shoichi Ogio, Masato Takita, Yoshiki Tsunesada, Masaki Fukushima, and H. Tokuno
Subjects: Nuclear and High Energy Physics, Photomultiplier, Physics - Instrumentation and Detectors, Photon, Physics::Instrumentation and Detectors, FOS: Physical sciences, 01 natural sciences, law.invention, Telescope, symbols.namesake, Optics, law, 0103 physical sciences, Calibration, Rayleigh scattering, 010306 general physics, Instrumentation and Methods for Astrophysics (astro-ph.IM), Instrumentation, Physics, 010308 nuclear & particles physics, business.industry, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Instrumentation and Detectors (physics.ins-det), symbols, Nitrogen laser, Astrophysics - Instrumentation and Methods for Astrophysics, business, Beam (structure)
Abstract: We performed photometric calibration of the PhotoMultiplier Tube (PMT) and readout electronics used for the new fluorescence detectors of the Telescope Array (TA) experiment using Rayleigh scattered photons from a pulsed nitrogen laser beam. The experimental setup, measurement procedure, and results of calibration are described. The total systematic uncertainty of the calibration is estimated to be 7.2%. An additional uncertainty of 3.7% is introduced by the transport of the calibrated PMTs from the laboratory to the TA experimental site., 43 pages, 15 figures
Published: 2012
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36. Telescope Array Experiment

Author: Shoichi Ogio
Subjects: Physics::Instrumentation and Detectors, QC1-999, Astrophysics::High Energy Astrophysical Phenomena, media_common.quotation_subject, Cosmic ray, 01 natural sciences, law.invention, Telescope, Optics, law, 0103 physical sciences, Anisotropy, 010303 astronomy & astrophysics, media_common, Physics, Range (particle radiation), 010308 nuclear & particles physics, business.industry, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Air shower, Sky, Scintillation counter, High Energy Physics::Experiment, business
Abstract: The Telescope Array is the largest hybrid cosmic ray detector in the Northern hemisphere designed to measure primary particles in 4 PeV to 100 EeV range. The main TA detector consists of an air shower array of 507 plastic scintillation counters on a 1.2 km square grid and fluorescence detectors at three stations overlooking the sky above the air shower array. The experiment and its recent measurements - spectrum, composition, and anisotropy - is reviewed. Recently the construction of the TA Low energy Extension (TALE) detector, which consists of an additional fluorescence detector and an infill array, was finished. TALE lowers the energy threshold of TA down to 4 PeV. We are also constructing the TAx4 detector to increase statistics in particular at the highest energies. The current status and the future prospects of these new TAx4 experiments is reported.
Published: 2019
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37. Trigger electronics of the new Fluorescence Detectors of the Telescope Array Experiment

Author: H. Tokuno, Hiroyuki Sagawa, Yuichiro Tameda, John N. Matthews, Nobuyuki Sakurai, Jeremy Smith, Manobu Tanaka, Takeshi Matsuda, Tatsunobu Shibata, S. Udo, C. C. H. Jui, K. Kadota, Masahiro Takeda, Yoshiki Tsunesada, Shoichi Ogio, Masaki Fukushima, Akimichi Taketa, Stanton B. Thomas, and Fumio Kakimoto
Subjects: Physics, Nuclear and High Energy Physics, Photon, Physics::Instrumentation and Detectors, business.industry, Detector, Night sky, Astrophysics::Instrumentation and Methods for Astrophysics, Scintillator, Fluorescence, law.invention, Telescope, Optics, law, Electronics, Ultra-high-energy cosmic ray, business, Instrumentation
Abstract: The Telescope Array Project is an experiment designed to observe Ultra High Energy Cosmic Rays via a “hybrid” detection technique utilizing both fluorescence light detectors (FDs) and scintillator surface particle detectors (SDs). We have installed three FD stations and 507 SDs in the Utah desert, and initiated observations from March 2008. The northern FD station reuses 14 telescopes from the High Resolution Fly's Eye, HiRes-I station. Each of the two southern FD stations contains 12 new telescopes utilizing new FADC electronics. Each telescope is instrumented with a camera composed of 256 PMTs. Since the detectors are composed of many PMTs and each PMT detects fluorescence photons together with the vast amount of night sky background, a sophisticated triggering system is required. In this paper, we describe the trigger electronics of these new FD stations. We also discuss performance of the FDs with this triggering system, in terms of efficiencies and apertures for various detector configurations.
Published: 2009
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38. The present status of the Telescope Array experiment

Author: K. Kasahara, John N. Matthews, T.-A. Shibata, Lawrence Wiencke, Gordon Thomson, Z. Cao, Robert Cady, Dmitri Ivanov, Toshiyuki Nonaka, H. Fujii, Douglas Bergman, K. Hibino, Masahiro Teshima, Pierre Sokolsky, K. Yamamoto, Taka Tomida, Naoaki Hayashida, O. A. Brusova, P. Huentemeyer, Takeshi Okuda, John Belz, M. Takeda, Akitoshi Oshima, Shingo Kawana, T. Yamakawa, Shunsuke Ozawa, Eiji Kido, Y. Kondo, Charlie Jui, Samuel Blake, Shoichi Ogio, Akimichi Taketa, Y. Tsuyuguchi, J. Yang, I. S. Cho, Yuichiro Tameda, K. Honda, Inkyu Park, Hiroyuki Sagawa, T. Fujii, Priti Shah, J. D. Smith, H. Kawai, M. Allen, Masaaki Tanaka, Y. J. Kwon, Hideyuki Ohoka, Toru Nakamura, Kenichi Kadota, Masato Takita, R. Azuma, N. Inoue, M. Ohnishi, Hyesung Kang, S. Udo, S. B. Thomas, S. W. Nam, S. Yoshida, A. Kitshugi, Y. Yamakawa, N. Yoshii, Kiyoshi Tanaka, K. Hayashi, Fumio Kakimoto, K. Martens, D. C. Rodriguez, Nobuyuki Sakurai, Y. Uchihori, Hideaki Shimodaira, R. Torii, Gareth Hughes, Tareq Abu-Zayyad, L. M. Scott, Hisono Tokuno, R. W. Springer, Tomohiro Matsuda, K. Kobayashi, Jyunsei Chiba, Dongsu Ryu, Michiyuki Chikawa, S. Iwamoto, Yoshiki Tsunesada, Daisuke Ikeda, S. R. Stratton, T. Fukuda, and Masaki Fukushima
Subjects: Physics, Nuclear and High Energy Physics, Systematic difference, business.industry, Detector, Scintillator, Atomic and Molecular Physics, and Optics, law.invention, Ground level, Telescope, Optics, Air shower, law, Ultra-high-energy cosmic ray, business
Abstract: The Telescope Array(TA) experiment located at western desert in Utah USA (N39.3,W112.9) is designed for observation of air shower from extreme high energy cosmic rays. The TA detector consists of 2 types of detector to enable a cross check on systematic difference from the two main methods of observation for the energy region. One is a Fluorescence detector (FD) for detecting fluorescence light from air shower and another is surface detector (SD) array for detecting air shower particles at ground level. Each SD consists of 2 layers of plastic scintillator with 3m 2 of surface and more sensitive to electromagnetic component in air shower. The full operation using 3FD stations and full SD array has started. Here we present the updated status of Telescope Array experiment.
Published: 2009
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39. On site calibration for new fluorescence detectors of the telescope array experiment

Author: H. Tokuno, Yoshiki Tsunesada, Daisuke Ikeda, Nobuyuki Sakurai, S. Kawana, Masaki Fukushima, T.-A. Shibata, Yuichiro Tameda, Hiroyuki Sagawa, Akimichi Taketa, K. Kadota, Masahiro Takeda, R. Azuma, M. Fukuda, Y. Murano, Shoichi Ogio, N. Inoue, S. Udo, and Fumio Kakimoto
Subjects: Physics, Systematic error, Nuclear and High Energy Physics, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Astrophysics::Cosmology and Extragalactic Astrophysics, Fluorescence, law.invention, Telescope, Optics, law, Calibration, business, Instrumentation, Energy (signal processing)
Abstract: The Telescope Array experiment is searching for the origin of ultra-high energy cosmic rays using a ground array of particle detectors and three fluorescence telescope stations. The precise calibration of the fluorescence detectors is important for small systematic errors in shower reconstruction. This paper details the process of calibrating cameras for two of the fluorescence telescope stations. This paper provides the operational results of these camera calibrations.
Published: 2009
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40. Telescope Array Experiment

Author: A. Ohshima, Shigeharu Udo, Shoichi Ogio, K. Ikuta, Hideaki Shimodaira, Michael J. Taylor, R. Azuma, Kiyoshi Tanaka, Y. Yamakawa, Hiroyuki Sagawa, T. Iguchi, J. D. Smith, H. Fujii, Yukio Uchihori, K. Hayashi, Yuichiro Tameda, R. Torii, Gareth Hughes, Z. Cao, K. Kadota, Nobuyuki Sakurai, K. Hashimoto, K. Hibino, M. Mostofa, Tareq Abu-Zayyad, H. Yamaoka, Fumio Kakimoto, Y. Kondo, John Belz, Y. Murano, Shunsuke Ozawa, Hideyuki Ohoka, Takayuki Tomida, Hisono Tokuno, M. Chikawa, H. Yoshii, T. Kanbe, T.-A. Shibata, Gordon Thomson, Akira Endo, K. Martens, T. Benno, Robert Cady, J. R. Thomas, Eiji Kido, Vincent B Wickwar, Y. Hayashi, R. W. Springer, Masato Takita, K. Doura, N. Hayashida, K. Miyata, Yoshiki Tsunesada, Daisuke Ikeda, Takaaki Ishii, S. R. Stratton, Tomohiro Matsuda, F. Cohen, Shingo Kawana, Masaki Fukushima, Thomas D. Wilkerson, S. Machida, John N. Matthews, Mayuko Minamino, Pierre Sokolsky, Noritaka Shimizu, M. Takeda, Masaaki Tanaka, Toshiyuki Nonaka, H. Kawai, Jyunsei Chiba, K. Misumi, S. Kawakami, P. Huentemeyer, N. Inoue, M. Ohnishi, C. C. H. Jui, S. B. Thomas, Takeshi Okuda, T. Doyle, Akimichi Taketa, Y. Wada, Lawrence Wiencke, Douglas Bergman, S. Yoshida, Katsuaki Kasahara, K. Hiyama, K. Honda, H. Tanaka, T. Matsuyama, Masahiro Teshima, and Toru Nakamura
Subjects: Physics, Nuclear and High Energy Physics, Physics::Instrumentation and Detectors, business.industry, Astrophysics::High Energy Astrophysical Phenomena, Detector, Astrophysics::Instrumentation and Methods for Astrophysics, Cosmic ray, Atomic and Molecular Physics, and Optics, law.invention, Telescope, Optics, law, Observatory, High Energy Physics::Experiment, Detector array, Anisotropy, business, Hybrid data, Energy (signal processing)
Abstract: The TA observatory is a hybrid detector system consisting of both a surface detector array as well as a set of fluorescence detectors. The observatory will measure the energy spectrum, anisotropy and composition of ultra-high energy cosmic rays. The surface detectors are being deployed and the array should be complete by the end of February, 2007. We will soon be collecting hybrid data at the Telecope Array.
Published: 2008
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41. Trigger system for the TA fluorescence detector

Author: Akimichi Taketa, Fumio Kakimoto, K. Hiyama, K. Kadota, H. Tokuno, J. D. Smith, S.B. Thomas, Takeshi Matsuda, Yoshiki Tsunesada, Masaki Fukushima, Yuichiro Tameda, Shoichi Ogio, Manobu Tanaka, and Ryuji Azuma
Subjects: Physics, business.industry, Instrumentation, Detector, Condensed Matter Physics, Signal, Atomic and Molecular Physics, and Optics, Electronic, Optical and Magnetic Materials, law.invention, Telescope, Optics, Air shower, Data acquisition, law, CTD, Ultra-high-energy cosmic ray, business
Abstract: The Telescope Array (TA) is a hybrid detector system consisting of fluorescence detectors (FDs) and a surface detector (SD) array to study ultra high energy cosmic rays. In this paper, we describe the development and status of the trigger system for the TA FDs. The trigger system consists of three components, those are the Signal Digitizer and Finder (SDF) module, the Track Finder (TF) module and the Central Trigger Distributor (CTD) module. The SDF module recognizes the fluorescence signal, TF finds air shower tracks and CTD controls data acquisition. We also report the first engineering run carried out in 2007.
Published: 2007

42. The Energy Spectrum of Cosmic Rays above 10$^{17.2}$ eV Measured by the Fluorescence Detectors of the Telescope Array Experiment in Seven Years

Author: K. Hibino, T. Goto, Grigory Rubtsov, H. Yoshii, Akitoshi Oshima, Ben Stokes, Kazumasa Kawata, R. Azuma, H. Kawai, K. Nagasawa, Kenta Yashiro, M. Abe, T.-A. Shibata, Gordon Thomson, Tom Stroman, Robert Cady, K. Martens, Federico R. Urban, Mayuko Minamino, T. Suzawa, John Belz, K. Honda, S. Kitamura, Hang Bae Kim, Priti Shah, Hideki Tanaka, Yasunori Kitamura, Mai Takamura, Hidemi Ito, Isaac Myers, K. Tsutsumi, Byung Gu Cheon, Masaaki Tanaka, Nobuyuki Sakurai, Bokkyun Shin, Eiji Kido, Fumiya Shibata, Igor Tkachev, Pierre Sokolsky, J. H. Kim, Kazuhiro Machida, Y. Tsunesada, Zach Zundel, S. Kawakami, Douglas Bergman, Fumio Kakimoto, R. Ishimori, K. Kasahara, Kanako Yamazaki, K. Oki, Toshiyuki Nonaka, J. P. Lundquist, M. Takeda, Sergey Troitsky, Inkyu Park, R. W. Springer, Shigehiro Nagataki, G. Vasiloff, Heungsu Shin, Y. Mukai, Y. J. Kwon, Hideyuki Ohoka, Hiroyuki Sagawa, Jyunsei Chiba, Y. Yoneda, Akimichi Taketa, Kiyoshi Tanaka, Dongsu Ryu, Hiroshi Yamaoka, N. Inoue, M. Ohnishi, Masaomi Ono, Ryuji Takeishi, S. Udo, C. C. H. Jui, Tomohiro Matsuda, S. B. Thomas, Toshihiro Fujii, Naoaki Hayashida, M. Allen, Shingo Kawana, O. Kalashev, W. R. Cho, Y. Uchihori, William Hanlon, Toru Nakamura, T. Okuda, J. Ogura, Kenichi Kadota, Takayuki Tomida, Elliott Barcikowski, Dmitri Ivanov, H. Tokuno, Takaaki Ishii, J. D. Smith, D. C. Rodriguez, J. Yang, Yuichiro Tameda, John N. Matthews, J. Lan, Masato Takita, Peter Tinyakov, Samuel Blake, Shoichi Ogio, L. M. Scott, A. Nozato, Y. Hayashi, Hideaki Shimodaira, Vladim Kuzmin, T. Matsuyama, S. Ozawa, Tareq Abu-Zayyad, R. Yamane, Maxim Pshirkov, Michiyuki Chikawa, S. Yoshida, Daisuke Ikeda, S. R. Stratton, Rasha Abbasi, Tiffany Wong, Masaki Fukushima, and R. Zollinger
Subjects: Physics, High Energy Astrophysical Phenomena (astro-ph.HE), Range (particle radiation), 010308 nuclear & particles physics, Astrophysics::High Energy Astrophysical Phenomena, Detector, FOS: Physical sciences, Astronomy and Astrophysics, Cosmic ray, Astrophysics, 7. Clean energy, 01 natural sciences, Fluorescence, law.invention, Telescope, Orders of magnitude (time), law, 0103 physical sciences, Energy spectrum, Astrophysics - High Energy Astrophysical Phenomena, 010303 astronomy & astrophysics, Energy (signal processing)
Abstract: The Telescope Array (TA) experiment is the largest detector to observe ultra-high-energy cosmic rays in the northern hemisphere. The fluorescence detectors at southern two stations of TA are newly constructed and have now completed seven years of steady operation. One advantage of monocular analysis of the fluorescence detectors is a lower energy threshold for cosmic rays than that of other techniques like stereoscopic observations or coincidences with the surface detector array, allowing the measurement of an energy spectrum covering three orders of magnitude in energy. Analyzing data collected during those seven years, we report the energy spectrum of cosmic rays covering a broad range of energies above 10$^{17.2}$ eV measured by the fluorescence detectors and a comparison with previously published results., Submitted to Astroparticle Physics
Published: 2015

43. The EUSO-Balloon pathfinder

Author: N. Tone, Daisuke Yonetoku, H. Ikeda, K. Mase, Francesco Isgrò, B. Keilhauer, Francesco Fenu, I. V. Yashin, Frederic Jean Ronga, L. Santiago Crúz, M. Yu. Zotov, Silvia Ferrarese, L. Marcelli, Susana Briz, I. Kreykenbohm, Vladimir Andreev, F. Dulucq, D. Ikeda, F. Sarazin, Andreas A. Berlind, A. Bruno, Patrick J. Reardon, Toshiki Tajima, G. Siemieniec-Oziȩbło, D. Kolev, Karl Mannheim, Valerie Connaughton, H. H. Silva Lopez, Marc Weber, K. Shinozaki, G. Masciantonio, Hitoshi Ohmori, Tomás Belenguer, G. Castellinic, H. Prieto, R. Cremonini, P. L. Biermann, Yoshiya Kawasaki, R. Nava, Michael S. Briggs, A. J. de Castro, N. Sakaki, I. Rusinov, S. Ahmad, Markus Roth, M. D. Rodríguez Frías, Alberto Cellino, Fausto Guarino, P. von Ballmoos, M. Ricci, L. Valore, I. Rodríguez, D. Allard, Rossella Caruso, T. Patzak, Toshiyuki Nonaka, Alfonso Monaco, M. E. Bertaina, Thomas J. Weiler, Yoshihiko Mizumoto, Taka Tomida, Z. Plebaniak, J. Blümer, Marcos Reyes, Tokonatsu Yamamoto, G. Roudil, M. Putis, A. Sobey, T. Murakami, O. Martinez, T. Shirahama, S. Sánchez, G. Catalano, Ken'ichi Nomoto, J. Karczmarczyk, J. N. Albert, Thomas Schanz, B. A. Khrenov, H. Miyamoto, S. Perez Cano, H. J. Crawford, L. R. Wiencke, G. Giraudo, A. Insolia, M. Kleifges, Humberto Ibarguen Salazar, C. De Santis, H. Tokuno, M. Flamini, Hanna Rothkaehl, Michiyuki Chikawa, Y. Takizawa, Livio Conti, M. Serra, A. Haungs, C. De Donato, Soon-Wook Kim, B. Harlov, Luis A. Anchordoqui, S. Piraino, Carlo Vigorito, T. Batsch, Hajime Yano, S. Falk, K. Kudela, Yoshimasa Kurihara, H. Schieler, M. Nagata, Piotr Orleanski, J. Geary, J. S. Kim, T. Shibata, I. Kaneko, K. Kawai, Akinori Saito, A. Zuccaro Marchi, V. S. Morozenko, Jörn Wilms, Roberto Bellotti, Dmitry V. Naumov, Y. Karadzhov, Mitsuteru Sato, N. De Simone, R. Young, O. A. Saprykin, M. Sakata, B. Mot, Javier Licandro, J.N. Capdevielle, Z. Włodarczyk, P. Picozza, Andrii Neronov, J. Lee, James H. Adams, J. Błȩcki, G. Distratis, A. Ebersoldt, J. F. Valdés-Galicia, L. Villaseñor, Yukihiro Takahashi, R. Bechini, Piero Vallania, R. Tsenov, H. Lim, N. Tajima, M. C. Maccarone, M. D. Sabau, Toshikazu Ebisuzaki, M. Suzuki, L. G. Tkachev, G. Sáez-Cano, A. Jung, S. Csorna, T. Pierog, J. Watanabe, Gali Garipov, Shigehiro Nagataki, Yoshiki Tsunesada, Simona Toscano, A. Pollini, Pavel Klimov, D. Supanitsky, M. Takeda, F. Cafagna, T. Paul, K. Yoshida, Marco Casolino, Claudio Fornaro, J. Bayer, G. Modestino, E. Joven, K. Higashide, Lech Wiktor Piotrowski, G. Vankova, Shigeto Watanabe, C. de la Taille, Ovidiu Vaduvescu, M. Lacombe, K. Katahira, Claudio Cassardo, Massimiliano Bonamente, M. Rybczyński, Valentina Scotti, H. Sato, Shoichi Ogio, Dmitri Semikoz, Yoshitaka Itow, Graciela B. Gelmini, Hajime Takami, A. Guzman, Jianyi Yang, Masaki Fukushima, C. Lachaud, E. Kuznetsov, G. Medina-Tanco, S. Biktemerova, T. Mernik, Y. Hachisu, Y. Arai, S. Dagoret-Campagne, D. Maravilla, G. Cordero, N. Inoue, L. del Peral, A. Franceschi, E. Parizot, David B. Cline, T. Nakamura, Y. Yamamoto, Katsuaki Asano, Alexander Kusenko, C. González Alvarado, J. A. Morales de los Ríos, Pierre Barrillon, S. Yoshida, J. Szabelski, K. Słomińska, E. G. Judd, Sergei A. Sharakin, Katsuhiko Tsuno, Susumu Inoue, Guillaume Prévôt, Satoshi Wada, M. Di Martino, A. Marini, A. Dell’Oro, Toshitaka Kajino, T. Ogawa, G. Osteria, C. Blaksley, T. Tymieniecka, J. Sledd, M. Sanz Palomino, Angela V. Olinto, Fernando López, Andrea Santangelo, R. Matev, M. Bogomilov, F. Tajima, F. Kajino, Ralph Engel, C. Moretto, P. Galeotti, M. Ave Pernas, H. W. Park, P. Gorodetzky, C. Tenzer, T. Sugiyama, Tadeusz Wibig, Ke Fang, Frederic Trillaud, M. Wille, M. Nagano Murakami, Y. Uchihori, J. Hernández Carretero, M. Unger, M. Dupieux, Barbara Szabelska, T. Peter, M. I. Panasyuk, S. Selmane, A. Anzalone, T. Napolitano, K. Belov, C. Catalano, D. Monnier-Ragaigne, A. Segreto, N. Blanc, S. Blin-Bondil, J. Fujimoto, P. Bobik, Hiroyuki Sagawa, Maxim Gonchar, Hirohiko M. Shimizu, P. Baragatti, J. Watts, C. Pennypacker, B. Pastircak, P. Prat, I. Fernández-Gómez, M. Karus, Domenico Finco, D. Campana, Inkyu Park, Y. Miyazaki, Mark Christl, O. Tibolla, APC - Astrophysique des Hautes Energies (APC - AHE), AstroParticule et Cosmologie (APC (UMR_7164)), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Università di Bologna [Bologna] (UNIBO)-Università di Bologna [Bologna] (UNIBO), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Dipartimento di Astronomia, Universita degli Studi di Bologna, Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO), Adams, J. H., Ahmad, S., Albert, J. N., Allard, D., Anchordoqui, L., Andreev, V., Anzalone, A., Arai, Y., Asano, K., Ave Pernas, M., Baragatti, P., Barrillon, P., Batsch, T., Bayer, J., Bechini, R., Belenguer, T., Bellotti, R., Belov, K., Berlind, A. A., Bertaina, M., Biermann, P. L., Biktemerova, S., Blaksley, C., Blanc, N., Błȩcki, J., Blin Bondil, S., Blã¼mer, J., Bobik, P., Bogomilov, M., Bonamente, M., Briggs, M. S., Briz, S., Bruno, A., Cafagna, F., Campana, D., Capdevielle, J. N., Caruso, R., Casolino, M., Cassardo, C., Castellinic, G., Catalano, C., Catalano, G., Cellino, A., Chikawa, M., Christl, M. J., Cline, D., Connaughton, V., Conti, L., Cordero, G., Crawford, H. J., Cremonini, R., Csorna, S., Dagoret Campagne, S., de Castro, A. J., De Donato, C., de la Taille, C., De Santis, C., del Peral, L., Dell’Oro, A., De Simone, N., Di Martino, M., Distratis, G., Dulucq, F., Dupieux, M., Ebersoldt, A., Ebisuzaki, T., Engel, R., Falk, S., Fang, K., Fenu, F., FernÃ¡ndez GÃ³mez, I., Ferrarese, S., Finco, D., Flamini, M., Fornaro, C., Franceschi, A., Fujimoto, J., Fukushima, M., Galeotti, P., Garipov, G., Geary, J., Gelmini, G., Giraudo, G., Gonchar, M., GonzÃ¡lez Alvarado, C., Gorodetzky, P., Guarino, Fausto, Guzmã¡n, A., Hachisu, Y., Harlov, B., Haungs, A., HernÃ¡ndez Carretero, J., Higashide, K., Ikeda, D., Ikeda, H., Inoue, N., Inoue, S., Insolia, A., Isgro', Francesco, Itow, Y., Joven, E., Judd, E. G., Jung, A., Kajino, F., Kajino, T., Kaneko, I., Karadzhov, Y., Karczmarczyk, J., Karus, M., Katahira, K., Kawai, K., Kawasaki, Y., Keilhauer, B., Khrenov, B. A., Kim, J. S., Kim, S. W., Kleifges, M., Klimov, P. A., Kolev, D., Kreykenbohm, I., Kudela, K., Kurihara, Y., Kusenko, A., Kuznetsov, E., Lacombe, M., Lachaud, C., Lee, J., Licandro, J., Lim, H., Lã³pez, F., Maccarone, M. C., Mannheim, K., Maravilla, D., Marcelli, L., Marini, A., Martinez, O., Masciantonio, G., Mase, K., Matev, R., Medina Tanco, G., Mernik, T., Miyamoto, H., Miyazaki, Y., Mizumoto, Y., Modestino, G., Monaco, A., Monnier Ragaigne, D., Morales de los RÃos, J. A., Moretto, C., Morozenko, V. S., Mot, B., Murakami, T., Murakami, M. Nagano, Nagata, M., Nagataki, S., Nakamura, T., Napolitano, T., Naumov, D., Nava, R., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A. V., Orleański, P., Osteria, G., Panasyuk, M. I., Parizot, E., Park, I. H., Park, H. W., Pastircak, B., Patzak, T., Paul, T., Pennypacker, C., Perez Cano, S., Peter, T., Picozza, P., Pierog, T., Piotrowski, L. W., Piraino, S., Plebaniak, Z., Pollini, A., Prat, P., Prã©vã´t, G., Prieto, H., Putis, M., Reardon, P., Reyes, M., Ricci, M., Rodrãguez, I., RodrÃguez FrÃas, M. D., Ronga, F., Roth, M., Rothkaehl, H., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M. D., SÃ¡ez Cano, G., Sagawa, H., Saito, A., Sakaki, N., Sakata, M., Salazar, H., Sã¡nchez, S., Santangelo, A., Santiago CrÃºz, L., Sanz Palomino, M., Saprykin, O., Sarazin, F., Sato, H., Sato, M., Schanz, T., Schieler, H., Scotti, V., Segreto, A., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shibata, T., Shimizu, H. M., Shinozaki, K., Shirahama, T., Siemieniec Oziȩbło, G., Silva LÃ³pez, H. H., Sledd, J., Słomińska, K., Sobey, A., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tajima, F., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Tenzer, C., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Trillaud, F., Tsenov, R., Tsunesada, Y., Tsuno, K., Tymieniecka, T., Uchihori, Y., Unger, M., Vaduvescu, O., ValdÃ©s Galicia, J. F., Vallania, P., Valore, Laura, Vankova, G., Vigorito, C., Villaseã±or, L., von Ballmoos, P., Wada, S., Watanabe, J., Watanabe, S., Watts, J., Weber, M., Weiler, T. J., Wibig, T., Wiencke, L., Wille, M., Wilms, J., Włodarczyk, Z., Yamamoto, T., Yamamoto, Y., Yang, J., Yano, H., Yashin, I. V., Yonetoku, D., Yoshida, K., Yoshida, S., Young, R., Zotov, M. Y. u., Zuccaro Marchi, A., Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Alma Mater Studiorum Università di Bologna [Bologna] (UNIBO)
Subjects: Ciencias Físicas, JEM-EUSO, cosmic-rays, Cosmic ray, 01 natural sciences, law.invention, Telescope, Observatory, law, 0103 physical sciences, International Space Station, Ultraviolet light, Air-fluorescence, Balloon experiment, UHECR, Astronomy and Astrophysics, Space and Planetary Science, 010303 astronomy & astrophysics, Remote sensing, Physics, 010308 nuclear & particles physics, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astronomy, Astronomy and Astrophysic, Near space, Astronomía, Pathfinder, [SDU]Sciences of the Universe [physics], Temporal resolution, UHECR, Air-fluorescence, JEM-EUSO, Balloon experiment, EUSO-Balloon, CIENCIAS NATURALES Y EXACTAS
Abstract: 注記: The JEM-EUSO Collaboration 289名 [所属. 宇宙航空研究開発機構宇宙科学研究所 (JAXA)(ISAS) 池田, 博一; 鈴木, 睦; 矢野, 創], Accepted: 2015-06-11, Note: The JEM-EUSO Collaboration 289members [Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) Ikeda, Hirokazu; Suzuki, Makoto; Yano, Hajime], 資料番号: SA1150237000
Published: 2015
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44. Publisher’s Note: Measurement of the proton-air cross section with Telescope Array’s Middle Drum detector and surface array in hybrid mode [Phys. Rev. D92, 032007 (2015)]

Author: Hideki Tanaka, K. Nagasawa, R. Zollinger, Hisono Tokuno, L. M. Scott, Pierre Sokolsky, A. Nozato, Y. Hayashi, M. Takeda, Shigehiro Nagataki, K. Kawata, K. Hibino, Hidemi Ito, P. Tinyakov, Mai Takamura, Dmitri Ivanov, Rasha Abbasi, M. Takita, Inkyu Park, Daisuke Ikeda, S. R. Stratton, O. Kalashev, B. G. Cheon, Akitoshi Oshima, Y. Tsunesada, Kalen Martens, R. W. Springer, Hideaki Shimodaira, Tiffany Wong, T. Goto, Charlie Jui, Ryuji Takeishi, Maxim Pshirkov, Sergey Troitsky, Mayuko Minamino, Yuichiro Tameda, K. Oki, K. Honda, Masaki Fukushima, Shunsuke Ozawa, Grigory Rubtsov, K. Yamazaki, T.-A. Shibata, Yasunori Kitamura, J. D. Smith, Takeshi Okuda, Vladim Kuzmin, Gordon Thomson, Igor Tkachev, Tom Stroman, H. Yoshii, Masaaki Tanaka, Robert Cady, Fumiya Shibata, Tomohiro Matsuda, Taka Tomida, Akimichi Taketa, R. Ishimori, M. Allen, S. B. Thomas, S. Kawakami, T. Matsuyama, Bokkyun Shin, John Belz, G. Vasiloff, Tareq Abu-Zayyad, R. Yamane, J. Ogura, Eiji Kido, Kazuhiro Machida, Elliott Barcikowski, M. J. Chae, Hiroyuki Sagawa, Shingo Kawana, K. Kadota, Jyunsei Chiba, Dongsu Ryu, D. R. Bergman, Naoaki Hayashida, Heungsu Shin, Y. Uchihori, William Hanlon, S. Yoshida, Y. J. Kwon, Toshitsugu Fujii, J. Yang, K. Kasahara, Nobuyuki Sakurai, Hideyuki Ohoka, John N. Matthews, Samuel Blake, Shoichi Ogio, Kiyoshi Tanaka, Fumio Kakimoto, Zach Zundel, M. Abe, Y. Yoneda, N. Inoue, S. I. Lim, Masaomi Ono, W. R. Cho, J. H. Kim, M. Ohnishi, Takaaki Ishii, Ben Stokes, Hongsu Kim, Federico R. Urban, D. C. Rodriguez, T. Suzawa, Toru Nakamura, H. Kawai, Isaac Myers, S. Kitamura, Kenta Yashiro, K. Tsutsumi, Priti Shah, Toshiyuki Nonaka, Michiyuki Chikawa, Y. Mukai, Hiroshi Yamaoka, Shigeharu Udo, R. Azuma, J. P. Lundquist, and J. Lan
Subjects: Physics, Surface (mathematics), Nuclear and High Energy Physics, Proton, business.industry, Detector, Drum, Astrophysics, Cosmology, law.invention, Gravitation, Telescope, Cross section (physics), Optics, law, business
Published: 2015
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45. The JEM-EUSO mission : an introduction

Author: J. Karczmarczyk, A. Haungs, T. Murakami, Tomás Belenguer, Piero Vallania, M. D. Sabau, M. Serra, J. Bayer, C. de la Taille, K. Katahira, Luis A. Anchordoqui, T. Batsch, D. Supanitsky, Hanna Rothkaehl, R. Nava, N. Sakaki, Y. Karadzhov, I. Kaneko, K. Mase, J. Watts, L. Valore, Rossella Caruso, H. J. Crawford, C. Pennypacker, I. Rodríguez, Shoichi Ogio, Patrick J. Reardon, Toshiki Tajima, G. Siemieniec-Oziȩbło, G. Masciantonio, Hitoshi Ohmori, Yoshiya Kawasaki, D. Allard, G. Castellini, M. E. Bertaina, Ken'ichi Nomoto, Silvia Ferrarese, Toshiyuki Nonaka, P. Prat, R. Young, M. Sakata, A. Guzmán, I. V. Yashin, T. Shirahama, T. Shibata, Alberto Cellino, P. Picozza, J. Lee, I. Fernández-Gómez, P. Baragatti, L. Marcelli, Ralph Engel, M. Karus, G. Sáez Cano, M. Nagata, A. Ebersoldt, L. Villaseñor, A. Bruno, Jeong-Sook Kim, L. R. Wiencke, J. Błȩcki, Karl Mannheim, D. Ikeda, D. Monnier-Ragaigne, A. Segreto, F. Tajima, Lech Wiktor Piotrowski, M. Rybczyński, Michael S. Briggs, A. J. de Castro, F. Sarazin, Domenico Finco, H. Lim, Frederic Trillaud, P. Gorodetzky, Dmitry V. Naumov, R. Bechini, Marc Weber, Katsuaki Asano, G. Cordero, M. C. Maccarone, Piotr Orleanski, N. Blanc, S. Piraino, J.N. Capdevielle, T. Patzak, S. Yoshida, J. Szabelski, Francesco Fenu, Yoshiki Tsunesada, Hiroyuki Sagawa, M. Wille, Andrii Neronov, Y. Uchihori, R. Matev, G. Giraudo, M. Suzuki, Satoshi Wada, H. Sato, C. De Donato, Markus Roth, J. N. Albert, T. Ogawa, Hajime Takami, B. A. Khrenov, G. Distratis, Fausto Guarino, O. Martinez, Masaki Fukushima, Thomas Schanz, Soon-Wook Kim, Takuji Nakamura, Jianyi Yang, Yoshitaka Itow, Shigeto Watanabe, H. Miyamoto, D. Maravilla, P. von Ballmoos, M. Ricci, K. Shinozaki, Angela V. Olinto, Fernando López, Andrea Santangelo, S. Selmane, Livio Conti, J. Fujimoto, A. Anzalone, Barbara Szabelska, T. Peter, David B. Cline, A. Zuccaro Marchi, Maxim Gonchar, Hirohiko M. Shimizu, M. D. Rodríguez Frías, F. Cafagna, G. Modestino, E. Joven, D. Campana, Francesco Isgrò, F. Dulucq, Z. Plebaniak, J. Blümer, Valentina Scotti, B. Keilhauer, Graciela B. Gelmini, M. Flamini, P. L. Biermann, Jörn Wilms, Javier Licandro, M. I. Panasyuk, J. F. Valdés-Galicia, L. G. Tkachev, O. A. Saprykin, Michiyuki Chikawa, B. Mot, Y. Hachisu, Inkyu Park, Frederic Jean Ronga, M. Dupieux, S. Csorna, T. Napolitano, S. Perez Cano, Y. Takizawa, L. Santiago Crúz, M. Putis, Humberto Ibarguen Salazar, Y. Arai, G. Vankova, I. Rusinov, A. Sobey, Y. Miyazaki, S. Blin-Bondil, C. De Santis, H. Tokuno, Y. Yamamoto, A. Insolia, M. Kleifges, Yukihiro Takahashi, B. Pastirčák, E. G. Judd, T. Pierog, M. Ave Pernas, Katsuhiko Tsuno, H. Prieto, R. Cremonini, S. Biktemerova, J. Watanabe, Pierre Barrillon, Mark Christl, O. Tibolla, Osvaldo Catalano, Gali Garipov, K. Kawai, I. Kreykenbohm, Sergei A. Sharakin, R. Tsenov, Vladimir Andreev, Marcos Reyes, Marco Casolino, Claudio Fornaro, K. Belov, C. Catalano, A. Pollini, J. Hernández Carretero, Pavel Klimov, M. Unger, C. Lachaud, S. Dagoret-Campagne, M. Di Martino, A. Marini, Toshikazu Ebisuzaki, T. J. Weiler, G. Osteria, S. Sánchez, S. Ahmad, Yoshimasa Kurihara, T. Tymieniecka, J. Sledd, H. Schieler, Mitsuteru Sato, C. González Alvarado, Alfonso Monaco, C. Blaksley, N. Tone, Ke Fang, M. Nagano, Taka Tomida, Daisuke Yonetoku, Roberto Bellotti, Andreas A. Berlind, M. Sanz Palomino, Tokonatsu Yamamoto, James H. Adams, M. Yu. Zotov, D. Kolev, Valerie Connaughton, H. H. Silva Lopez, Susana Briz, S. Falk, H. Ikeda, V. S. Morozenko, Hajime Yano, A. Dell’Oro, Toshitaka Kajino, K. Higashide, C. Moretto, P. Galeotti, C. Tenzer, T. Sugiyama, Tadeusz Wibig, K. Kudela, G. Roudil, B. Harlov, Carlo Vigorito, N. Tajima, M. Takeda, Shigehiro Nagataki, Guillaume Prévôt, M. Bogomilov, F. Kajino, H. W. Park, Massimiliano Bonamente, E. Kuznetsov, Alexander Kusenko, K. Słomińska, Akinori Saito, Ovidiu Vaduvescu, M. Lacombe, Claudio Cassardo, Dmitri Semikoz, Sug-Whan Kim, T. Mernik, Z. Włodarczyk, Simona Toscano, N. Inoue, L. del Peral, A. Franceschi, E. Parizot, Pavol Bobik, J. A. Morales de los Ríos, Susumu Inoue, A. Jung, T. Paul, K. Yoshida, G. Medina-Tanco, J. Geary, N. De Simone, Yoshihiko Mizumoto, Organisation de Micro-Électronique Générale Avancée (OMEGA), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), AstroParticule et Cosmologie (APC (UMR_7164)), Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratori Nazionali del Sud (LNS), Istituto Nazionale di Fisica Nucleare (INFN), Division of Biology, Kansas State University, Kansas State University, CTC, Università degli studi di Bari Aldo Moro = University of Bari Aldo Moro (UNIBA), Institut de recherche en astrophysique et planétologie (IRAP), Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Institut de Recherche pour le Développement (IRD)-Université Toulouse III - Paul Sabatier (UT3), Université de Toulouse (UT)-Université de Toulouse (UT)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Institut de Recherche pour le Développement (IRD)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Météo-France -Centre National de la Recherche Scientifique (CNRS), INAF - Osservatorio Astrofisico di Torino (OATo), Istituto Nazionale di Astrofisica (INAF), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology [Zürich] (ETH Zürich), Universities Space Research Association (USRA), Regione Emilia Romagna, Servizio Tecnico Bacini Enza e sinistra Secchia, Institute for Data Processing and Electronics (IPE), Karlsruhe Institute of Technology (KIT), Institute for Ecology, Universität Greifswald - University of Greifswald, Tokushima research center, Department of Physics and Astronomy [UCLA, Los Angeles], University of California [Los Angeles] (UCLA), University of California (UC)-University of California (UC), Istituto Nazionale di Fisica Nucleare, Sezione di Torino (INFN, Sezione di Torino), Institute of Applied Biotechnology and Basic Sciences, Rzeszow University, Department of Mechanical System (Hiroshima University), Hiroshima University, Nagoya University, Department of Pathology, Ludwig-Maximilians-Universität München (LMU), Friedrich-Alexander Universität Erlangen-Nürnberg (FAU), Institute of Experimental Physics of Kosice, Slovak Academy of Sciences (SAS), KEK (High energy accelerator research organization), iMagX/MIRO, Université Catholique de Louvain = Catholic University of Louvain (UCL), Instituto de Astrofisica de Canarias (IAC), The Open University of Japan [Chiba] (OUJ), Tohoku University [Sendai], Department of Earth and Planetary Science [Tokyo], Graduate School of Science [Tokyo], The University of Tokyo (UTokyo)-The University of Tokyo (UTokyo), Department of Electrical Engineering and Computer Sciences, University of Hyogo, INTEGRAL Science Data Center (ISDC), Geneva Observatory, Université de Genève = University of Geneva (UNIGE)-Université de Genève = University of Geneva (UNIGE), Service de dermatologie et vénéréologie (CHUV Lausanne), Centre Hospitalier Universitaire Vaudois [Lausanne] (CHUV), Laboratoire de Physique Théorique et Modèles Statistiques (LPTMS), Université Paris-Sud - Paris 11 (UP11)-Centre National de la Recherche Scientifique (CNRS), Institute for Surgical Technology and Biomechanics [Bern] (ISTB), University of Bern, Centre IRMf de Marseille, Université de la Méditerranée - Aix-Marseille 2, Space Research Centre of Polish Academy of Sciences (CBK), Polska Akademia Nauk = Polish Academy of Sciences (PAN), Centre d'étude spatiale des rayonnements (CESR), Center for Mathematics and Physics, University of Aizu, Centre de recherche sur la Paléobiodiversité et les Paléoenvironnements (CR2P), Muséum national d'Histoire naturelle (MNHN)-Université Pierre et Marie Curie - Paris 6 (UPMC)-Centre National de la Recherche Scientifique (CNRS), Colorado School of Mines, Department of Physics (Department of Physics), Tokyo Metropolitan University [Tokyo] (TMU), Department of Radiation-Oncology, Università degli Studi di Firenze = University of Florence (UniFI), Graduate School of Materials Science, Nara Institute os Science and Technology, Observatoire océanologique de Banyuls (OOB), Sorbonne Université (SU)-Centre National de la Recherche Scientifique (CNRS), Max-Planck-Institut für Kernphysik (MPIK), Max-Planck-Gesellschaft, Vrije Universiteit Brussel (VUB), Laboratoire de Génie Electrique de Grenoble (G2ELab), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Institute of Sensor and Actuator Systems, Vienna University of Technology (TU Wien), Institut de Mécanique Céleste et de Calcul des Ephémérides (IMCCE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université de Lille-Centre National de la Recherche Scientifique (CNRS), Luxembourg Institute of Science and Technology (LIST), Dr. Karl-Remeis-Sternwarte, Erlangen Centre for Astroparticle Physics (ECAP), Friedrich-Alexander Universität Erlangen-Nürnberg (FAU)-Friedrich-Alexander Universität Erlangen-Nürnberg (FAU), Kyoto University, University of Connecticut (UCONN), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-École polytechnique (X), Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Observatoire de Paris, PSL Research University (PSL)-PSL Research University (PSL)-Université Paris Diderot - Paris 7 (UPD7), National Institute for Nuclear Physics (INFN), University of Bari and INFN section of Bari, Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Observatoire Midi-Pyrénées (OMP), Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS), Eidgenössische Technische Hochschule - Swiss Federal Institute of Technology in Zürich [Zürich] (ETH Zürich), University of California-University of California, Université Catholique de Louvain (UCL), The University of Tokyo, University of Geneva [Switzerland]-University of Geneva [Switzerland], Polska Akademia Nauk (PAN), Université Fédérale Toulouse Midi-Pyrénées-Université Fédérale Toulouse Midi-Pyrénées-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire Midi-Pyrénées (OMP), Université Pierre et Marie Curie - Paris 6 (UPMC)-Muséum national d'Histoire naturelle (MNHN)-Centre National de la Recherche Scientifique (CNRS), Tokyo Metropolitan University [Tokyo], University of Florence (UNIFI), High Energy Accelerator Research Organization (KEK), University of Tsukuba, Vrije Universiteit [Brussels] (VUB), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS)-Université Grenoble Alpes (UGA), Technical University of Vienna [Vienna] (TU WIEN), PSL Research University (PSL)-PSL Research University (PSL)-Université de Lille-Centre National de la Recherche Scientifique (CNRS), Kyoto University [Kyoto], Adams, J. H., Ahmad, S., Albert, J. N., Allard, D., Anchordoqui, L., Andreev, V., Anzalone, A., Arai, Y., Asano, K., Ave Pernas, M., Baragatti, P., Barrillon, P., Batsch, T., Bayer, J., Bechini, R., Belenguer, T., Bellotti, R., Belov, K., Berlind, A. A., Bertaina, M., Biermann, P. L., Biktemerova, S., Blaksley, C., Blanc, N., Błȩcki, J., Blin Bondil, S., Blã¼mer, J., Bobik, P., Bogomilov, M., Bonamente, M., Briggs, M. S., Briz, S., Bruno, A., Cafagna, F., Campana, D., Capdevielle, J. N., Caruso, R., Casolino, M., Cassardo, C., Castellini, G., Catalano, C., Catalano, O., Cellino, A., Chikawa, M., Christl, M. J., Cline, D., Connaughton, V., Conti, L., Cordero, G., Crawford, H. J., Cremonini, R., Csorna, S., Dagoret Campagne, S., de Castro, A. J., De Donato, C., de la Taille, C., De Santis, C., del Peral, L., Dell’Oro, A., De Simone, N., Di Martino, M., Distratis, G., Dulucq, F., Dupieux, M., Ebersoldt, A., Ebisuzaki, T., Engel, R., Falk, S., Fang, K., Fenu, F., FernÃ¡ndez GÃ³mez, I., Ferrarese, S., Finco, D., Flamini, M., Fornaro, C., Franceschi, A., Fujimoto, J., Fukushima, M., Galeotti, P., Garipov, G., Geary, J., Gelmini, G., Giraudo, G., Gonchar, M., GonzÃ¡lez Alvarado, C., Gorodetzky, P., Guarino, Fausto, Guzmã¡n, A., Hachisu, Y., Harlov, B., Haungs, A., HernÃ¡ndez Carretero, J., Higashide, K., Ikeda, D., Ikeda, H., Inoue, N., Inoue, S., Insolia, A., Isgro', Francesco, Itow, Y., Joven, E., Judd, E. G., Jung, A., Kajino, F., Kajino, T., Kaneko, I., Karadzhov, Y., Karczmarczyk, J., Karus, M., Katahira, K., Kawai, K., Kawasaki, Y., Keilhauer, B., Khrenov, B. A., Kim, Jeong Sook, Kim, Soon Wook, Kim, Sug Whan, Kleifges, M., Klimov, P. A., Kolev, D., Kreykenbohm, I., Kudela, K., Kurihara, Y., Kusenko, A., Kuznetsov, E., Lacombe, M., Lachaud, C., Lee, J., Licandro, J., Lim, H., Lã³pez, F., Maccarone, M. C., Mannheim, K., Maravilla, D., Marcelli, L., Marini, A., Martinez, O., Masciantonio, G., Mase, K., Matev, R., Medina Tanco, G., Mernik, T., Miyamoto, H., Miyazaki, Y., Mizumoto, Y., Modestino, G., Monaco, A., Monnier Ragaigne, D., Morales de los RÃos, J. A., Moretto, C., Morozenko, V. S., Mot, B., Murakami, T., Nagano, M., Nagata, M., Nagataki, S., Nakamura, T., Napolitano, T., Naumov, D., Nava, R., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A. V., Orleański, P., Osteria, G., Panasyuk, M. I., Parizot, E., Park, I. H., Park, H. W., Pastircak, B., Patzak, T., Paul, T., Pennypacker, C., Perez Cano, S., Peter, T., Picozza, P., Pierog, T., Piotrowski, L. W., Piraino, S., Plebaniak, Z., Pollini, A., Prat, P., Prã©vã´t, G., Prieto, H., Putis, M., Reardon, P., Reyes, M., Ricci, M., Rodrãguez, I., Frãas, M. D. RodrÃguez, Ronga, F., Roth, M., Rothkaehl, H., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M. D., SÃ¡ez Cano, G., Sagawa, H., Saito, A., Sakaki, N., Sakata, M., Salazar, H., Sã¡nchez, S., Santangelo, A, Santiago CrÃºz, L., Sanz Palomino, M., Saprykin, O., Sarazin, F., Sato, H., Sato, M., Schanz, T., Schieler, H., Scotti, V., Segreto, A., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shibata, T., Shimizu, H. M., Shinozaki, K., Shirahama, T., Siemieniec Oziȩbło, G., Silva LÃ³pez, H. H., Sledd, J., Słomińska, K., Sobey, A., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tajima, F., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Tenzer, C., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Trillaud, F., Tsenov, R., Tsunesada, Y., Tsuno, K., Tymieniecka, T., Uchihori, Y., Unger, M., Vaduvescu, O., ValdÃ©s Galicia, J. F., Vallania, P., Valore, Laura, Vankova, G., Vigorito, C., Villaseã±or, L., von Ballmoos, P., Wada, S., Watanabe, J., Watanabe, S., Watts, J., Weber, M., Weiler, T. J., Wibig, T., Wiencke, L., Wille, M., Wilms, J., Włodarczyk, Z., Yamamoto, T., Yamamoto, Y., Yang, J., Yano, H., Yashin, I. V., Yonetoku, D., Yoshida, K., Yoshida, S., Young, R., Zotov, M. Y. u., Zuccaro Marchi, A., École polytechnique (X)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Commissariat à l'énergie atomique et aux énergies alternatives (CEA)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3), Università degli studi di Bari Aldo Moro (UNIBA), Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS), The University of Tokyo (UTokyo), Centre National de la Recherche Scientifique (CNRS)-Université Paris-Sud - Paris 11 (UP11), Observatoire Midi-Pyrénées (OMP), Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Météo France-Centre National d'Études Spatiales [Toulouse] (CNES)-Université Fédérale Toulouse Midi-Pyrénées-Centre National de la Recherche Scientifique (CNRS)-Institut de Recherche pour le Développement (IRD)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Toulouse III - Paul Sabatier (UT3), Université Fédérale Toulouse Midi-Pyrénées, Università degli Studi di Firenze = University of Florence [Firenze] (UNIFI), Centre National de la Recherche Scientifique (CNRS)-Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology, Centre National de la Recherche Scientifique (CNRS)-Université de Lille-Observatoire de Paris, and Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Université Pierre et Marie Curie - Paris 6 (UPMC)
Subjects: Photon, Aperture, Ciencias Físicas, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, Cosmic ray, ultra-high energy cosmic rays, Astrophysics, law.invention, Telescope, Atmosphere, law, International Space Station, Neutrino, Ultra-high energy cosmic rays, Neutrinos, Neutrinos, Ultra-high energy cosmic ray, ComputingMilieux_MISCELLANEOUS, media_common, Physics, [PHYS]Physics [physics], Astrophysics::Instrumentation and Methods for Astrophysics, Astronomy, neutrinos, Astronomy and Astrophysics, Ultra-high energy cosmic rays, Astronomy and Astrophysic, Universe, Astronomía, Space and Planetary Science, Physics::Space Physics, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph], CIENCIAS NATURALES Y EXACTAS
Abstract: 注記: The JEM-EUSO Collaboration 288名 [所属. 宇宙航空研究開発機構宇宙科学研究所 (JAXA)(ISAS) 池田, 博一; 鈴木, 睦; 矢野, 創], Accepted: 2015-10-19, Note: The JEM-EUSO Collaboration 288members [Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) Ikeda, Hirokazu; Suzuki, Makoto; Yano, Hajime], 資料番号: SA1150231000
Published: 2015
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46. Calibration aspects of the JEM-EUSO mission

Author: Humberto Ibarguen Salazar, C. De Santis, H. Tokuno, Katsuaki Asano, Alfonso Monaco, M. Rybczyński, Alberto Cellino, R. Tsenov, Taka Tomida, H. Sato, P. Baragatti, Gali Garipov, A. Pollini, Pavel Klimov, G. Cordero, L. R. Wiencke, Tokonatsu Yamamoto, Barbara Szabelska, David B. Cline, Yoshimasa Kurihara, H. Schieler, Mitsuteru Sato, Silvia Ferrarese, M. Di Martino, G. Giraudo, A. Marini, T. Peter, Satoshi Wada, R. Matev, T. Ogawa, E. G. Judd, G. Catalano, Katsuhiko Tsuno, G. Osteria, T. Tymieniecka, J. Sledd, C. Lachaud, M. I. Panasyuk, B. A. Khrenov, H. Miyamoto, M. Suzuki, S. Dagoret-Campagne, D. Campana, Valentina Scotti, Ovidiu Vaduvescu, M. Lacombe, Claudio Cassardo, M. Ave Pernas, S. Falk, Graciela B. Gelmini, Y. Hachisu, Inkyu Park, F. Dulucq, Angela V. Olinto, Y. Arai, Fernando López, Andrea Santangelo, Massimiliano Bonamente, Y. Yamamoto, Francesco Isgrò, A. Guzmán, B. Keilhauer, J. N. Albert, Dmitri Semikoz, Pierre Barrillon, Sergei A. Sharakin, Y. Miyazaki, Thomas Schanz, J. Geary, Y. Karadzhov, Roberto Bellotti, R. Young, J. Watts, M. Sakata, Yoshitaka Itow, Andreas A. Berlind, M. D. Rodríguez Frías, E. Kuznetsov, Toshikazu Ebisuzaki, C. Pennypacker, Frederic Jean Ronga, Toshiyuki Nonaka, Z. Plebaniak, James H. Adams, B. Pastircak, N. De Simone, J. Blümer, M. Putis, Mark Christl, O. Tibolla, Livio Conti, P. Prat, L. Villaseñor, A. Zuccaro Marchi, P. L. Biermann, T. Mernik, I. Kreykenbohm, H. Ikeda, M. Flamini, Vladimir Andreev, F. Tajima, Michiyuki Chikawa, J. Hernández Carretero, P. Gorodetzky, I. Rusinov, I. Fernández-Gómez, A. Sobey, Ralph Engel, Yoshihiko Mizumoto, M. Unger, A. Insolia, M. Kleifges, Alexander Kusenko, Thomas J. Weiler, C. Blaksley, G. Sáez-Cano, Y. Takizawa, M. Wille, Jörn Wilms, D. Kolev, I. V. Yashin, S. Perez Cano, M. Nagano Murakami, Y. Uchihori, M. Karus, O. A. Saprykin, S. Ahmad, T. Shibata, L. Marcelli, K. Słomińska, Marcos Reyes, J. F. Valdés-Galicia, L. G. Tkachev, Domenico Finco, T. Murakami, Kenji Shinozaki, J. Karczmarczyk, R. Bechini, M. Serra, N. Inoue, Luis A. Anchordoqui, Ke Fang, J. Błȩcki, L. del Peral, A. Franceschi, E. Parizot, S. Sánchez, Pavol Bobik, Valerie Connaughton, H. H. Silva Lopez, S. Csorna, T. Batsch, A. Bruno, G. Vankova, Frederic Trillaud, Hiroyuki Sagawa, K. Mase, Karl Mannheim, Michael S. Briggs, A. J. de Castro, D. Maravilla, H. Lim, K. Kawai, Akinori Saito, S. Biktemerova, Francesco Fenu, M. C. Maccarone, Shigeto Watanabe, T. Patzak, I. Kaneko, Hajime Yano, Z. Włodarczyk, Piero Vallania, J. A. Morales de los Ríos, M. D. Sabau, M. Dupieux, Tomás Belenguer, Hanna Rothkaehl, Maxim Gonchar, Hirohiko M. Shimizu, G. Distratis, D. Supanitsky, Susumu Inoue, D. Ikeda, Lech Wiktor Piotrowski, D. Monnier-Ragaigne, A. Segreto, C. González Alvarado, N. Tone, F. Sarazin, Simona Toscano, J. Bayer, A. Ebersoldt, S. Selmane, Marc Weber, Daisuke Yonetoku, F. Cafagna, G. Modestino, E. Joven, Shoichi Ogio, P. Picozza, J. Lee, Guillaume Prévôt, S. Yoshida, J. Szabelski, C. de la Taille, M. Yu. Zotov, A. Jung, Javier Licandro, Susana Briz, A. Anzalone, T. Napolitano, H. J. Crawford, Yoshiki Tsunesada, T. Paul, K. Katahira, K. Yoshida, O. Martinez, B. Mot, Yukihiro Takahashi, N. Blanc, G. Castellinic, Markus Roth, R. Nava, Hajime Takami, M. Bogomilov, N. Sakaki, Patrick J. Reardon, T. Pierog, J. Watanabe, Toshiki Tajima, G. Siemieniec-Oziȩbło, Fausto Guarino, P. von Ballmoos, M. Ricci, L. Valore, Masaki Fukushima, M. Sanz Palomino, T. Nakamura, G. Medina-Tanco, M. Takeda, K. Belov, Marco Casolino, Claudio Fornaro, C. Catalano, Rossella Caruso, F. Kajino, G. Masciantonio, Hitoshi Ohmori, Yoshiya Kawasaki, I. Rodríguez, H. W. Park, T. Shirahama, D. Allard, M. E. Bertaina, Piotr Orleanski, C. De Donato, Soon-Wook Kim, Ken'ichi Nomoto, J. S. Kim, V. S. Morozenko, A. Haungs, S. Piraino, J. Fujimoto, S. Blin-Bondil, L. Santiago Crúz, H. Prieto, R. Cremonini, Jianyi Yang, M. Nagata, Dmitry V. Naumov, J.N. Capdevielle, Andrii Neronov, G. Roudil, B. Harlov, Carlo Vigorito, K. Kudela, N. Tajima, Shigehiro Nagataki, A. Dell’Oro, Toshitaka Kajino, K. Higashide, C. Moretto, P. Galeotti, C. Tenzer, T. Sugiyama, Tadeusz Wibig, Adams, J. H., Ahmad, S., Albert, J. N., Allard, D., Anchordoqui, L., Andreev, V., Anzalone, A., Arai, Y., Asano, K., Ave Pernas, M., Baragatti, P., Barrillon, P., Batsch, T., Bayer, J., Bechini, R., Belenguer, T., Bellotti, R., Belov, K., Berlind, A. A., Bertaina, M., Biermann, P. L., Biktemerova, S., Blaksley, C., Blanc, N., Błȩcki, J., Blin Bondil, S., Blã¼mer, J., Bobik, P., Bogomilov, M., Bonamente, M., Briggs, M. S., Briz, S., Bruno, A., Cafagna, F., Campana, D., Capdevielle, J. N., Caruso, R., Casolino, M., Cassardo, C., Castellinic, G., Catalano, C., Catalano, G., Cellino, A., Chikawa, M., Christl, M. J., Cline, D., Connaughton, V., Conti, L., Cordero, G., Crawford, H. J., Cremonini, R., Csorna, S., Dagoret Campagne, S., de Castro, A. J., De Donato, C., de la Taille, C., De Santis, C., del Peral, L., Dell’Oro, A., De Simone, N., Di Martino, M., Distratis, G., Dulucq, F., Dupieux, M., Ebersoldt, A., Ebisuzaki, T., Engel, R., Falk, S., Fang, K., Fenu, F., FernÃ¡ndez GÃ³mez, I., Ferrarese, S., Finco, D., Flamini, M., Fornaro, C., Franceschi, A., Fujimoto, J., Fukushima, M., Galeotti, P., Garipov, G., Geary, J., Gelmini, G., Giraudo, G., Gonchar, M., GonzÃ¡lez Alvarado, C., Gorodetzky, P., Guarino, Fausto, Guzmã¡n, A., Hachisu, Y., Harlov, B., Haungs, A., HernÃ¡ndez Carretero, J., Higashide, K., Ikeda, D., Ikeda, H., Inoue, N., Inoue, S., Insolia, A., Isgro', Francesco, Itow, Y., Joven, E., Judd, E. G., Jung, A., Kajino, F., Kajino, T., Kaneko, I., Karadzhov, Y., Karczmarczyk, J., Karus, M., Katahira, K., Kawai, K., Kawasaki, Y., Keilhauer, B., Khrenov, B. A., Kim, J. S., Kim, S. W., Kleifges, M., Klimov, P. A., Kolev, D., Kreykenbohm, I., Kudela, K., Kurihara, Y., Kusenko, A., Kuznetsov, E., Lacombe, M., Lachaud, C., Lee, J., Licandro, J., Lim, H., Lã³pez, F., Maccarone, M. C., Mannheim, K., Maravilla, D., Marcelli, L., Marini, A., Martinez, O., Masciantonio, G., Mase, K., Matev, R., Medina Tanco, G., Mernik, T., Miyamoto, H., Miyazaki, Y., Mizumoto, Y., Modestino, G., Monaco, A., Monnier Ragaigne, D., Morales de los RÃos, J. A., Moretto, C., Morozenko, V. S., Mot, B., Murakami, T., Murakami, M. Nagano, Nagata, M., Nagataki, S., Nakamura, T., Napolitano, T., Naumov, D., Nava, R., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A. V., Orleański, P., Osteria, G., Panasyuk, M. I., Parizot, E., Park, I. H., Park, H. W., Pastircak, B., Patzak, T., Paul, T., Pennypacker, C., Perez Cano, S., Peter, T., Picozza, P., Pierog, T., Piotrowski, L. W., Piraino, S., Plebaniak, Z., Pollini, A., Prat, P., Prã©vã´t, G., Prieto, H., Putis, M., Reardon, P., Reyes, M., Ricci, M., Rodrãguez, I., RodrÃguez FrÃas, M. D., Ronga, F., Roth, M., Rothkaehl, H., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M. D., SÃ¡ez Cano, G., Sagawa, H., Saito, A., Sakaki, N., Sakata, M., Salazar, H., Sã¡nchez, S., Santangelo, A., Santiago CrÃºz, L., Sanz Palomino, M., Saprykin, O., Sarazin, F., Sato, H., Sato, M., Schanz, T., Schieler, H., Scotti, V., Segreto, A., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shibata, T., Shimizu, H. M., Shinozaki, K., Shirahama, T., Siemieniec Oziȩbło, G., Silva LÃ³pez, H. H., Sledd, J., Słomińska, K., Sobey, A., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tajima, F., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Tenzer, C., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Trillaud, F., Tsenov, R., Tsunesada, Y., Tsuno, K., Tymieniecka, T., Uchihori, Y., Unger, M., Vaduvescu, O., ValdÃ©s Galicia, J. F., Vallania, P., Valore, Laura, Vankova, G., Vigorito, C., Villaseã±or, L., von Ballmoos, P., Wada, S., Watanabe, J., Watanabe, S., Watts, J., Weber, M., Weiler, T. J., Wibig, T., Wiencke, L., Wille, M., Wilms, J., Włodarczyk, Z., Yamamoto, T., Yamamoto, Y., Yang, J., Yano, H., Yashin, I. V., Yonetoku, D., Yoshida, K., Yoshida, S., Young, R., Zotov, M. Y. u., and Zuccaro Marchi, A.
Subjects: Photon, Ciencias Físicas, JEM-EUSO, Phase (waves), Air-Shower fluorescence telescope, Calibration, Space-Based experiment, Astronomy and Astrophysics, Space and Planetary Science, computer science, law.invention, Telescope, Optics, law, Transmittance, observations and techniques, space-based experiment, Remote sensing, Physics, business.industry, Detector, air-shower fluorescence telescope, Albedo, Astronomy and Astrophysic, calibration, chemistry and earth sciences, Air-Shower fluorescence telescope, JEM-EUSO, Calibration, Space-Based experiment, Astronomía, astronomy, statistics for engineering, Focal surface, business, physics, CIENCIAS NATURALES Y EXACTAS
Abstract: he JEM-EUSO telescope will be, after calibration, a very accurate instrument which yields the number of received photons from the number of measured photo-electrons. The project is in phase A (demonstration of the concept) including already operating prototype instruments, i.e. many parts of the instrument have been constructed and tested. Calibration is a crucial part of the instrument and its use. The focal surface (FS) of the JEM-EUSO telescope will consist of about 5000 photo-multiplier tubes (PMTs), which have to be well calibrated to reach the required accuracy in reconstructing the air-shower parameters. The optics system consists of 3 plastic Fresnel (double-sided) lenses of 2.5 m diameter. Theaim of the calibration system is to measure the efficiencies (transmittances) of the optics and absolute efficiencies of the entire focal surface detector. The system consists of 3 main components: (i) Pre-flight calibration devices on ground, where the efficiency and gain of the PMTs will be measured absolutely and also the transmittance of the optics will be. (ii) On-board relative calibration system applying twomethods: a) operating during the day when the JEM-EUSO lid will be closed with small light sources on board. b) operating during the night, together with data taking: the monitoring of the background rate over identical sites. (iii) Absolute in-flight calibration, again, applying two methods: a) measurement of the moon light, reflected on high altitude, high albedo clouds. b) measurements of calibrated flashes and tracks produced by the Global Light System (GLS). Some details of each calibration method will be described in this paper. Fil: Adams, J. H.. University of Alabama in Huntsville; Estados Unidos Fil: Ahmad, S.. Ecole Polytechnique; Francia Fil: Albert, J. N.. Univ Paris-Sud; Francia Fil: Allard, D.. Univ Paris Diderot; Francia Fil: Anchordoqui, L.. University of Wisconsin-Milwaukee; Estados Unidos Fil: Andreev, V.. University of California; Estados Unidos Fil: Anzalone, A.. INAF - Istituto di Astrofisica Spaziale e Fisica Cosmica di Palermo; Italia Fil: Arai, Y.. High Energy Accelerator Research Organization (KEK); Japón Fil: Asano, K.. Tokyo Institute of Technology; Japón Fil: Ave Pernas, M.. Universidad de Alcala (UAH); España Fil: Barrillon, P.. Univ Paris-Sud; Francia Fil: Batsch, T.. National Centre for Nuclear Research; Polonia Fil: Bayer, J.. University of Tubingen; Alemania Fil: Bechini, R.. Universita’ di Torino; Italia Fil: Belenguer, T.. Instituto Nacional de Tecnica Aeroespacial (INTA); España Fil: Bellotti, R.. Istituto Nazionale di Fisica Nucleare; Italia Fil: Belov, K.. University of California; Estados Unidos Fil: Berlind, A. A.. Vanderbilt University; Estados Unidos Fil: Bertaina, M.. Istituto Nazionale di Fisica Nucleare; Italia Fil: Biermann, P. L.. Karlsruhe Institute of Technology (KIT); Alemania Fil: Biktemerova, S.. Joint Institute for Nuclear Research; Rusia Fil: Blaksley, C.. Univ Paris Diderot; Francia Fil: Blanc. N.. Swiss Center for Electronics and Microtechnology (CSEM); Suiza Fil: Blecki, J.. Space Research Centre of the Polish Academy of Sciences (CBK); Polonia Fil: Blin-Bondil, S.. Ecole Polytechnique; Francia Fil: Blumer, J.. Karlsruhe Institute of Technology (KIT); Alemania Fil: Bobik, P.. Institute of Experimental Physics; Eslovaquia Fil: Bogomilov, M.. University of Sofia; Bulgaria Fil: Bonamente, M.. University of Alabama in Huntsville; Estados Unidos Fil: Supanitsky, Alberto Daniel. Consejo Nacional de Investigaciónes Científicas y Técnicas. Oficina de Coordinación Administrativa Ciudad Universitaria. Instituto de Astronomía y Física del Espacio. - Universidad de Buenos Aires. Facultad de Ciencias Exactas y Naturales. Instituto de Astronomía y Física del Espacio; Argentina Fil: The JEM-EUSO Collaboration.
Published: 2015
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47. Performances of JEM–EUSO : energy and X_{max} reconstruction

Author: I. V. Yashin, L. Marcelli, B. A. Khrenov, H. Miyamoto, Kenji Shinozaki, A. Bruno, Karl Mannheim, Michael S. Briggs, A. J. de Castro, D. Supanitsky, Shoichi Ogio, M. Rybczyński, F. Dulucq, Graciela B. Gelmini, Andreas A. Berlind, A. Jung, Massimiliano Bonamente, Javier Licandro, T. Paul, N. Tone, Daisuke Yonetoku, M. Ave Pernas, F. Tajima, H. Sato, David B. Cline, Gali Garipov, C. De Donato, Soon-Wook Kim, G. Cordero, M. Yu. Zotov, K. Yoshida, Susana Briz, S. Selmane, Y. Hachisu, Y. Arai, Y. Yamamoto, Piero Vallania, M. D. Sabau, Alfonso Monaco, Taka Tomida, J. Bayer, E. Kuznetsov, J. Hernández Carretero, P. Baragatti, Hiroyuki Sagawa, D. Kolev, J. S. Kim, M. Putis, A. Sobey, A. Insolia, M. Kleifges, C. de la Taille, E. G. Judd, K. Katahira, M. Unger, T. Pierog, J. Watanabe, M. Wille, M. Nagano Murakami, Y. Uchihori, M. Takeda, J. F. Valdés-Galicia, P. Gorodetzky, G. Distratis, V. S. Morozenko, C. Lachaud, Katsuhiko Tsuno, G. Castellinic, Katsuaki Asano, J. Fujimoto, Tokonatsu Yamamoto, Patrick J. Reardon, Toshiki Tajima, G. Siemieniec-Oziȩbło, G. Masciantonio, Hitoshi Ohmori, Yoshiya Kawasaki, S. Dagoret-Campagne, Pierre Barrillon, L. G. Tkachev, S. Csorna, Valerie Connaughton, Toshikazu Ebisuzaki, T. Shibata, I. Kreykenbohm, D. Allard, M. E. Bertaina, Alexander Kusenko, G. Vankova, H. H. Silva Lopez, Jianyi Yang, Vladimir Andreev, R. Matev, J. N. Albert, M. Di Martino, Markus Roth, G. Medina-Tanco, Ken'ichi Nomoto, Francesco Isgrò, A. Marini, D. Campana, M. Nagata, Thomas Schanz, Hajime Yano, Fausto Guarino, P. von Ballmoos, M. Ricci, Satoshi Wada, G. Catalano, P. Prat, A. Haungs, S. Piraino, K. Słomińska, B. Keilhauer, G. Prévôt, S. Biktemerova, T. Ogawa, Yoshihiko Mizumoto, T. Patzak, Lech Wiktor Piotrowski, R. Nava, Inkyu Park, Dmitry V. Naumov, R. Bechini, N. Sakaki, Livio Conti, Ke Fang, S. Ahmad, T. Murakami, J. Karczmarczyk, A. Zuccaro Marchi, Y. Karadzhov, L. Valore, F. Cafagna, Frederic Jean Ronga, Sergei A. Sharakin, G. Modestino, Rossella Caruso, Angela V. Olinto, Fernando López, Jörn Wilms, E. Joven, G. Osteria, Andrea Santangelo, T. Tymieniecka, J. Sledd, D. Maravilla, Y. Miyazaki, A. Dell’Oro, Toshitaka Kajino, S. Yoshida, J. Szabelski, Silvia Ferrarese, O. A. Saprykin, P. L. Biermann, Maxim Gonchar, S. Falk, S. Blin-Bondil, Hirohiko M. Shimizu, R. Young, M. Sakata, I. Rusinov, M. Dupieux, Z. Włodarczyk, Hanna Rothkaehl, Shigeto Watanabe, Mark Christl, O. Tibolla, J. N. Capdevielle, L. Santiago Crúz, A. Anzalone, T. Napolitano, Thomas J. Weiler, K. Higashide, C. Moretto, J. Geary, P. Galeotti, Alberto Cellino, A. Guzmán, S. Perez Cano, C. González Alvarado, Marcos Reyes, P. Picozza, J. Błȩcki, Roberto Bellotti, H. Prieto, J. Lee, Simona Toscano, Barbara Szabelska, T. Peter, C. Tenzer, I. Rodríguez, H. Lim, L. R. Wiencke, R. Cremonini, M. C. Maccarone, N. De Simone, T. Sugiyama, J. Watts, S. Sánchez, Tadeusz Wibig, T. Shirahama, Toshiyuki Nonaka, C. Pennypacker, James H. Adams, Andrii Neronov, B. Pastircak, H. Ikeda, L. Villaseñor, G. Giraudo, G. Sáez-Cano, N. Inoue, I. Fernández-Gómez, K. Kawai, L. del Peral, A. Franceschi, E. Parizot, Pavol Bobik, M. Sanz Palomino, M. Bogomilov, D. Monnier-Ragaigne, A. Segreto, M. Karus, M. I. Panasyuk, Akinori Saito, M. Suzuki, Piotr Orleanski, Domenico Finco, K. Belov, C. Catalano, F. Kajino, J. A. Morales de los Ríos, Yoshitaka Itow, Ovidiu Vaduvescu, G. Roudil, M. Lacombe, Tomás Belenguer, Claudio Cassardo, B. Harlov, Susumu Inoue, H. W. Park, Carlo Vigorito, K. Kudela, H. J. Crawford, Valentina Scotti, Humberto Ibarguen Salazar, C. De Santis, H. Tokuno, N. Tajima, T. Mernik, Shigehiro Nagataki, R. Tsenov, A. Pollini, Pavel Klimov, Yoshimasa Kurihara, H. Schieler, Ralph Engel, Mitsuteru Sato, Frederic Trillaud, B. Mot, Yukihiro Takahashi, Marco Casolino, Claudio Fornaro, M. Flamini, Y. Takizawa, C. Blaksley, K. Mase, M. D. Rodríguez Frías, Z. Plebaniak, J. Blümer, Michiyuki Chikawa, D. Ikeda, A. Ebersoldt, F. Sarazin, Marc Weber, Yoshiki Tsunesada, O. Martinez, N. Blanc, Francesco Fenu, D. Semikoz, Hajime Takami, Masaki Fukushima, T. Nakamura, M. Serra, Luis A. Anchordoqui, T. Batsch, I. Kaneko, Adams, J. H., Ahmad, S., Albert, J. N., Allard, D., Anchordoqui, L., Andreev, V., Anzalone, A., Arai, Y., Asano, K., Ave Pernas, M., Baragatti, P., Barrillon, P., Batsch, T., Bayer, J., Bechini, R., Belenguer, T., Bellotti, R., Belov, K., Berlind, A. A., Bertaina, M., Biermann, P. L., Biktemerova, S., Blaksley, C., Blanc, N., Błȩcki, J., Blin Bondil, S., Blümer, J., Bobik, P., Bogomilov, M., Bonamente, M., Briggs, M. S., Briz, S., Bruno, A., Cafagna, F., Campana, D., Capdevielle, J. N., Caruso, R., Casolino, M., Cassardo, C., Castellinic, G., Catalano, C., Catalano, G., Cellino, A., Chikawa, M., Christl, M. J., Cline, D., Connaughton, V., Conti, L., Cordero, G., Crawford, H. J., Cremonini, R., Csorna, S., Dagoret Campagne, S., de Castro, A. J., De Donato, C., de la Taille, C., De Santis, C., del Peral, L., Dell’Oro, A., De Simone, N., Di Martino, M., Distratis, G., Dulucq, F., Dupieux, M., Ebersoldt, A., Ebisuzaki, T., Engel, R., Falk, S., Fang, K., Fenu, F., Fernández Gómez, I., Ferrarese, S., Finco, D., Flamini, M., Fornaro, C., Franceschi, A., Fujimoto, J., Fukushima, M., Galeotti, P., Garipov, G., Geary, J., Gelmini, G., Giraudo, G., Gonchar, M., González Alvarado, C., Gorodetzky, P., Guarino, Fausto, Guzmán, A., Hachisu, Y., Harlov, B., Haungs, A., Hernández Carretero, J., Higashide, K., Ikeda, D., Ikeda, H., Inoue, N., Inoue, S., Insolia, A., Isgro', Francesco, Itow, Y., Joven, E., Judd, E. G., Jung, A., Kajino, F., Kajino, T., Kaneko, I., Karadzhov, Y., Karczmarczyk, J., Karus, M., Katahira, K., Kawai, K., Kawasaki, Y., Keilhauer, B., Khrenov, B. A., Kim, J. S., Kim, S. W., Kleifges, M., Klimov, P. A., Kolev, D., Kreykenbohm, I., Kudela, K., Kurihara, Y., Kusenko, A., Kuznetsov, E., Lacombe, M., Lachaud, C., Lee, J., Licandro, J., Lim, H., López, F., Maccarone, M. C., Mannheim, K., Maravilla, D., Marcelli, L., Marini, A., Martinez, O., Masciantonio, G., Mase, K., Matev, R., Medina Tanco, G., Mernik, T., Miyamoto, H., Miyazaki, Y., Mizumoto, Y., Modestino, G., Monaco, A., Monnier Ragaigne, D., Morales de los Ríos, J. A., Moretto, C., Morozenko, V. S., Mot, B., Murakami, T., Murakami, M. Nagano, Nagata, M., Nagataki, S., Nakamura, T., Napolitano, T., Naumov, D., Nava, R., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A. V., Orleański, P., Osteria, G., Panasyuk, M. I., Parizot, E., Park, I. H., Park, H. W., Pastircak, B., Patzak, T., Paul, T., Pennypacker, C., Perez Cano, S., Peter, T., Picozza, P., Pierog, T., Piotrowski, L. W., Piraino, S., Plebaniak, Z., Pollini, A., Prat, P., Prévôt, G., Prieto, H., Putis, M., Reardon, P., Reyes, M., Ricci, M., Rodríguez, I., Rodríguez Frías, M. D., Ronga, F., Roth, M., Rothkaehl, H., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M. D., Sáez Cano, G., Sagawa, H., Saito, A., Sakaki, N., Sakata, M., Salazar, H., Sánchez, S., Santangelo, A., Santiago Crúz, L., Sanz Palomino, M., Saprykin, O., Sarazin, F., Sato, H., Sato, M., Schanz, T., Schieler, H., Scotti, V., Segreto, A., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shibata, T., Shimizu, H. M., Shinozaki, K., Shirahama, T., Siemieniec Oziȩbło, G., Silva López, H. H., Sledd, J., Słomińska, K., Sobey, A., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tajima, F., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Tenzer, C., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Trillaud, F., Tsenov, R., Tsunesada, Y., Tsuno, K., Tymieniecka, T., Uchihori, Y., Unger, M., Vaduvescu, O., Valdés Galicia, J. F., Vallania, P., Valore, Laura, Vankova, G., Vigorito, C., Villaseñor, L., von Ballmoos, P., Wada, S., Watanabe, J., Watanabe, S., Watts, J., Weber, M., Weiler, T. J., Wibig, T., Wiencke, L., Wille, M., Wilms, J., Włodarczyk, Z., Yamamoto, T., Yamamoto, Y., Yang, J., Yano, H., Yashin, I. V., Yonetoku, D., Yoshida, K., Yoshida, S., Young, R., Zotov, M. Y. u., and Zuccaro Marchi, A.
Subjects: reconstruction, Ciencias Físicas, media_common.quotation_subject, Astrophysics::High Energy Astrophysical Phenomena, JEM-EUSO, X (max) reconstruction, ComputingMethodologies_IMAGEPROCESSINGANDCOMPUTERVISION, Cosmic ray, X_{max} reconstruction, Astrophysics, law.invention, Energy reconstruction, JEM–EUSO, Xmax reconstruction, Astronomy and Astrophysics, Space and Planetary Science, Telescope, law, International Space Station, Ultra-high-energy cosmic ray, max, media_common, energy reconstruction, Physics, Resolution (electron density), Astrophysics::Instrumentation and Methods for Astrophysics, X-max reconstruction, Astronomy, Universe, Astronomía, JEM-EUSO, Energy reconstruction, X-max reconstruction, Event (particle physics), CIENCIAS NATURALES Y EXACTAS, Energy (signal processing)
Abstract: 注記: The JEM-EUSO Collaboration 288名 [所属. 宇宙航空研究開発機構宇宙科学研究所 (JAXA)(ISAS) 池田, 博一; 鈴木, 睦; 矢野, 創], Accepted: 2014-10-13, Note: The JEM-EUSO Collaboration 288members [Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) Ikeda, Hirokazu; Suzuki, Makoto; Yano, Hajime], 資料番号: SA1150235000
Published: 2015
Full Text: View/download PDF

48. Science of atmospheric phenomena with JEM-EUSO

Author: Yoshihiko Mizumoto, Toshiyuki Nonaka, T. Murakami, A. Guzmán, J. Karczmarczyk, J. Watts, C. Pennypacker, B. Pastircak, P. Prat, I. Fernández-Gómez, M. Karus, Domenico Finco, Hiroyuki Sagawa, M. Suzuki, M. Flamini, Hanna Rothkaehl, D. Monnier-Ragaigne, A. Segreto, Maxim Gonchar, Hirohiko M. Shimizu, L. Villaseñor, Y. Takizawa, Javier Licandro, P. Picozza, Alberto Cellino, Roberto Bellotti, J. Lee, F. Dulucq, Lech Wiktor Piotrowski, Valentina Scotti, J. N. Albert, N. Blanc, Thomas Schanz, Toshikazu Ebisuzaki, G. Sáez-Cano, M. Rybczyński, Andreas A. Berlind, L. R. Wiencke, James H. Adams, H. Ikeda, M. Di Martino, S. Yoshida, J. Szabelski, A. Marini, T. Pierog, J. Watanabe, G. Cordero, M. Takeda, G. Castellinic, Livio Conti, C. De Donato, A. Zuccaro Marchi, G. Giraudo, Soon-Wook Kim, Katsuaki Asano, S. Blin-Bondil, Markus Roth, A. Dell’Oro, Toshitaka Kajino, A. Haungs, S. Piraino, Jörn Wilms, D. Kolev, G. Osteria, Massimiliano Bonamente, O. A. Saprykin, Fausto Guarino, P. von Ballmoos, M. Ricci, J. Słomiński, T. Tymieniecka, H. Sato, J. Sledd, Valerie Connaughton, H. H. Silva Lopez, E. Kuznetsov, M. Putis, P. Baragatti, K. Higashide, C. Moretto, P. Galeotti, A. Sobey, Barbara Szabelska, R. Matev, Satoshi Wada, M. Nagata, T. Ogawa, Alexander Kusenko, A. Insolia, M. Kleifges, Gali Garipov, Ralph Engel, David B. Cline, J. F. Valdés-Galicia, L. G. Tkachev, S. Csorna, C. Tenzer, J. S. Kim, D. Maravilla, Yoshimasa Kurihara, T. Peter, H. Schieler, T. Sugiyama, G. Vankova, O. Martinez, K. Słomińska, V. S. Morozenko, Mitsuteru Sato, Francesco Isgrò, Angela V. Olinto, Tadeusz Wibig, Fernando López, Andrea Santangelo, E. G. Judd, B. Keilhauer, Katsuhiko Tsuno, Alfonso Monaco, Graciela B. Gelmini, D. Campana, T. Shibata, Taka Tomida, C. Blaksley, Frederic Trillaud, Y. Hachisu, Dmitry V. Naumov, Y. Arai, I. Kreykenbohm, Vladimir Andreev, Tokonatsu Yamamoto, K. Mase, R. Young, Frederic Jean Ronga, I. Rodríguez, Tomás Belenguer, S. Biktemerova, M. Sakata, C. Lachaud, Inkyu Park, S. Dagoret-Campagne, B. Mot, Y. Yamamoto, T. Shirahama, J.N. Capdevielle, Francesco Fenu, G. Catalano, S. Ahmad, N. Tajima, Piero Vallania, Y. Miyazaki, M. D. Sabau, Shigehiro Nagataki, J. Fujimoto, S. Falk, R. Bechini, Yukihiro Takahashi, M. Ave Pernas, C. González Alvarado, Pierre Barrillon, Ke Fang, Mark Christl, O. Tibolla, Marco Casolino, Claudio Fornaro, Z. Włodarczyk, Humberto Ibarguen Salazar, D. Ikeda, F. Sarazin, Piotr Orleanski, Silvia Ferrarese, H. J. Crawford, J. Bayer, Sergei A. Sharakin, J. Hernández Carretero, Mikhail Panasyuk, M. Unger, C. De Santis, Marc Weber, Shigeto Watanabe, J. Błȩcki, H. Tokuno, C. de la Taille, G. Roudil, B. Harlov, H. Lim, Carlo Vigorito, M. C. Maccarone, K. Kudela, M. Sanz Palomino, K. Katahira, L. Santiago Crúz, Jianyi Yang, M. Dupieux, Patrick J. Reardon, Toshiki Tajima, G. Siemieniec-Oziȩbło, G. Masciantonio, Hitoshi Ohmori, R. Nava, Y. Karadzhov, N. Sakaki, M. Serra, Luis A. Anchordoqui, L. Valore, Rossella Caruso, Yoshiya Kawasaki, Simona Toscano, T. Batsch, H. Prieto, R. Cremonini, R. Tsenov, D. Allard, Guillaume Prévôt, Andrii Neronov, S. Selmane, M. E. Bertaina, A. Pollini, Pavel Klimov, I. Kaneko, Ken'ichi Nomoto, F. Tajima, Yoshitaka Itow, P. Gorodetzky, A. Anzalone, M. Bogomilov, T. Napolitano, M. Wille, M. Nagano Murakami, Y. Uchihori, K. Belov, F. Kajino, A. Ebersoldt, C. Catalano, H. W. Park, Yoshiki Tsunesada, Hajime Takami, Masaki Fukushima, T. Nakamura, N. Tone, Daisuke Yonetoku, M. Yu. Zotov, Susana Briz, M. D. Rodríguez Frías, Z. Plebaniak, J. Blümer, Michiyuki Chikawa, Hajime Yano, P. L. Biermann, D. Supanitsky, I. Rusinov, J. Geary, N. De Simone, Marcos Reyes, Shoichi Ogio, A. Jung, T. Paul, K. Yoshida, S. Sánchez, B. A. Khrenov, H. Miyamoto, G. Medina-Tanco, N. Inoue, L. del Peral, A. Franceschi, E. Parizot, Pavol Bobik, J. A. Morales de los Ríos, Susumu Inoue, Ovidiu Vaduvescu, M. Lacombe, Claudio Cassardo, Dmitri Semikoz, T. Mernik, I. V. Yashin, L. Marcelli, Thomas J. Weiler, S. Perez Cano, Kenji Shinozaki, A. Bruno, Karl Mannheim, Michael S. Briggs, A. J. de Castro, K. Kawai, T. Patzak, Akinori Saito, G. Distratis, F. Cafagna, G. Modestino, E. Joven, Adams, J. H., Ahmad, S., Albert, J. N., Allard, D., Anchordoqui, L., Andreev, V., Anzalone, A., Arai, Y., Asano, K., Ave Pernas, M., Baragatti, P., Barrillon, P., Batsch, T., Bayer, J., Bechini, R., Belenguer, T., Bellotti, R., Belov, K., Berlind, A. A., Bertaina, M., Biermann, P. L., Biktemerova, S., Blaksley, C., Blanc, N., Błȩcki, J., Blin Bondil, S., Blã¼mer, J., Bobik, P., Bogomilov, M., Bonamente, M., Briggs, M. S., Briz, S., Bruno, A., Cafagna, F., Campana, D., Capdevielle, J. N., Caruso, R., Casolino, M., Cassardo, C., Castellinic, G., Catalano, C., Catalano, G., Cellino, A., Chikawa, M., Christl, M. J., Cline, D., Connaughton, V., Conti, L., Cordero, G., Crawford, H. J., Cremonini, R., Csorna, S., Dagoret Campagne, S., de Castro, A. J., De Donato, C., de la Taille, C., De Santis, C., del Peral, L., Dell’Oro, A., De Simone, N., Di Martino, M., Distratis, G., Dulucq, F., Dupieux, M., Ebersoldt, A., Ebisuzaki, T., Engel, R., Falk, S., Fang, K., Fenu, F., FernÃ¡ndez GÃ³mez, I., Ferrarese, S., Finco, D., Flamini, M., Fornaro, C., Franceschi, A., Fujimoto, J., Fukushima, M., Galeotti, P., Garipov, G., Geary, J., Gelmini, G., Giraudo, G., Gonchar, M., GonzÃ¡lez Alvarado, C., Gorodetzky, P., Guarino, Fausto, Guzmã¡n, A., Hachisu, Y., Harlov, B., Haungs, A., HernÃ¡ndez Carretero, J., Higashide, K., Ikeda, D., Ikeda, H., Inoue, N., Inoue, S., Insolia, A., Isgro', Francesco, Itow, Y., Joven, E., Judd, E. G., Jung, A., Kajino, F., Kajino, T., Kaneko, I., Karadzhov, Y., Karczmarczyk, J., Karus, M., Katahira, K., Kawai, K., Kawasaki, Y., Keilhauer, B., Khrenov, B. A., Kim, J. S., Kim, S. W., Kleifges, M., Klimov, P. A., Kolev, D., Kreykenbohm, I., Kudela, K., Kurihara, Y., Kusenko, A., Kuznetsov, E., Lacombe, M., Lachaud, C., Lee, J., Licandro, J., Lim, H., Lã³pez, F., Maccarone, M. C., Mannheim, K., Maravilla, D., Marcelli, L., Marini, A., Martinez, O., Masciantonio, G., Mase, K., Matev, R., Medina Tanco, G., Mernik, T., Miyamoto, H., Miyazaki, Y., Mizumoto, Y., Modestino, G., Monaco, A., Monnier Ragaigne, D., Morales de los RÃos, J. A., Moretto, C., Morozenko, V. S., Mot, B., Murakami, T., Murakami, M. Nagano, Nagata, M., Nagataki, S., Nakamura, T., Napolitano, T., Naumov, D., Nava, R., Neronov, A., Nomoto, K., Nonaka, T., Ogawa, T., Ogio, S., Ohmori, H., Olinto, A. V., Orleański, P., Osteria, G., Panasyuk, M. I., Parizot, E., Park, I. H., Park, H. W., Pastircak, B., Patzak, T., Paul, T., Pennypacker, C., Perez Cano, S., Peter, T., Picozza, P., Pierog, T., Piotrowski, L. W., Piraino, S., Plebaniak, Z., Pollini, A., Prat, P., Prã©vã´t, G., Prieto, H., Putis, M., Reardon, P., Reyes, M., Ricci, M., Rodrãguez, I., RodrÃguez FrÃas, M. D., Ronga, F., Roth, M., Rothkaehl, H., Roudil, G., Rusinov, I., Rybczyński, M., Sabau, M. D., SÃ¡ez Cano, G., Sagawa, H., Saito, A., Sakaki, N., Sakata, M., Salazar, H., Sã¡nchez, S., Santangelo, A., Santiago CrÃºz, L., Sanz Palomino, M., Saprykin, O., Sarazin, F., Sato, H., Sato, M., Schanz, T., Schieler, H., Scotti, V., Segreto, A., Selmane, S., Semikoz, D., Serra, M., Sharakin, S., Shibata, T., Shimizu, H. M., Shinozaki, K., Shirahama, T., Siemieniec Oziȩbło, G., Silva LÃ³pez, H. H., Sledd, J., Słomińska, K., Sobey, A., Sugiyama, T., Supanitsky, D., Suzuki, M., Szabelska, B., Szabelski, J., Tajima, F., Tajima, N., Tajima, T., Takahashi, Y., Takami, H., Takeda, M., Takizawa, Y., Tenzer, C., Tibolla, O., Tkachev, L., Tokuno, H., Tomida, T., Tone, N., Toscano, S., Trillaud, F., Tsenov, R., Tsunesada, Y., Tsuno, K., Tymieniecka, T., Uchihori, Y., Unger, M., Vaduvescu, O., ValdÃ©s Galicia, J. F., Vallania, P., Valore, Laura, Vankova, G., Vigorito, C., Villaseã±or, L., von Ballmoos, P., Wada, S., Watanabe, J., Watanabe, S., Watts, J., Weber, M., Weiler, T. J., Wibig, T., Wiencke, L., Wille, M., Wilms, J., Włodarczyk, Z., Yamamoto, T., Yamamoto, Y., Yang, J., Yano, H., Yashin, I. V., Yonetoku, D., Yoshida, K., Yoshida, S., Young, R., Zotov, M. Y. u., Zuccaro Marchi, A., and Słomiński, J.
Subjects: Atmospheric physics, Ciencias Físicas, Space Shuttle, Cosmic ray, Elves, Jets - Atmospheric phenomena, Sprites, Transient Luminous Events, Astronomy and Astrophysics, Space and Planetary Science, Astrophysics, ELVES, Elve, Transient Luminous Events, Elves, Sprites, Jets - Atmospheric phenomena, law.invention, Telescope, purl.org/becyt/ford/1 [https], law, International Space Station, Ultra-high-energy cosmic ray, Astrophysique, Physics, Astronomy, purl.org/becyt/ford/1.3 [https], Astronomie, Astronomy and Astrophysic, Sciences de l'espace, Astronomía, Moment (physics), Sprite, Satellite, Transient Luminous Event, CIENCIAS NATURALES Y EXACTAS
Abstract: 注記: The JEM-EUSO Collaboration 289名 [所属. 宇宙航空研究開発機構宇宙科学研究所 (JAXA)(ISAS) 池田, 博一; 鈴木, 睦; 矢野, 創], Accepted: 2014-11-17, Note: The JEM-EUSO Collaboration 289members [Affiliation. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency (JAXA)(ISAS) Ikeda, Hirokazu; Suzuki, Makoto; Yano, Hajime], 資料番号: SA1150236000
Published: 2015
Full Text: View/download PDF

49. Searches for Large-Scale Anisotropy in the Arrival Directions of Cosmic Rays Detected above Energy of $10^{19}$ eV at the Pierre Auger Observatory and the Telescope Array

Author: Telescope, Array, Pierre Auger Collaborations (Alexander Aab, Pedro, Abreu, Marco, Aglietta, Eun Joo Ahn, Imen Al Samarai, Ivone, Albuquerque, Ingomar, Allekotte, Jeff, Allen, Patrick, Allison, Alejandro, Almela, Jesus Alvarez Castillo, Jaime Alvarez Muñiz, Rafael Alves Batista, Michelangelo, Ambrosio, Amin, Aminaei, Luis, Anchordoqui, Sofia, Andringa, Carla, Aramo, Victor Manuel Aranda, Fernando, Arqueros, Hernán Gonzalo Asorey, Pedro, Assis, Julien, Aublin, Maximo, Ave, Michel, Avenier, Gualberto, Avila, Nafiun, Awal, Alina Mihaela Badescu, Barber, Kerri B., Julia, Bäuml, Colin, Baus, Jim, Beatty, Karl Heinz Becker, Bellido, Jose A., Corinne, Berat, Mario Edoardo Bertania, Xavier, Bertou, Peter, Biermann, Pierre, Billoir, Blaess, Simon G., Miguel, Blanco, Carla, Bleve, Hans, Blümer, Martina, Boháčová, Denise, Boncioli, Carla, Bonifazi, Raffaella, Bonino, Nataliia, Borodai, Jeffrey, Brack, Iliana, Brancus, Ariel, Bridgeman, Pedro, Brogueira, Brown, William C., Peter, Buchholz, Antonio, Bueno, Stijn, Buitink, Buscemi, Mario, Caballero Mora, Karen S., Barbara, Caccianiga, Lorenzo, Caccianiga, Marina, Candusso, Laurentiu, Caramete, Caruso, Rossella, Antonella, Castellina, Gabriella, Cataldi, Lorenzo, Cazon, Rosanna, Cester, Chavez, Alan G., Andrea, Chiavassa, Jose Augusto Chinellato, Jiri, Chudoba, Marco, Cilmo, Clay, Roger W., Giuseppe, Cocciolo, Roberta, Colalillo, Alan, Coleman, Laura, Collica, Maria Rita Coluccia, Ruben, Conceição, Fernando, Contreras, Cooper, Mathew J., Alain, Cordier, Stephane, Coutu, Corbin, Covault, James, Cronin, Alex, Curutiu, Richard, Dallier, Bruno, Daniel, Sergio, Dasso, Kai, Daumiller, Dawson, Bruce R., de Almeida, Rogerio M., Manlio De Domenico, de Jong, Sijbrand J., Joao de Mello Neto, Ivan De Mitri, Jaime de Oliveira, Vitor de Souza, Luis del Peral, Olivier, Deligny, Hans, Dembinski, Niraj, Dhital, Claudio Di Giulio, Armando Di Matteo, Johana Chirinos Diaz, Mary Lucia Díaz Castro, Francisco, Diogo, Carola, Dobrigkeit, Wendy, Docters, Juan Carlos D'Olivo, Alexei, Dorofeev, Qader Dorosti Hasankiadeh, Maria Teresa Dova, Jan, Ebr, Ralph, Engel, Martin, Erdmann, Mona, Erfani, Escobar, Carlos O., Joao, Espadanal, Alberto, Etchegoyen, Pedro Facal San Luis, Heino, Falcke, Fang, Ke, Glennys, Farrar, Anderson, Fauth, Norberto, Fazzini, Ferguson, Andrew P., Mateus, Fernandes, Brian, Fick, Juan Manuel Figueira, Alberto, Filevich, Andrej, Filipčič, Brendan, Fox, Octavian, Fratu, Uwe, Fröhlich, Benjamin, Fuchs, Toshihiro, Fujii, Romain, Gaior, Beatriz, García, Sayri Tupac Garcia Roca, Diego Garcia Gamez, Diego Garcia Pinto, Gianpaolo, Garilli, Alberto Gascon Bravo, Florian, Gate, Hartmut, Gemmeke, Piera Luisa Ghia, Ugo, Giaccari, Marco, Giammarchi, Maria, Giller, Christian, Glaser, Henry, Glass, Mariano Gómez Berisso, Gómez Vitale, Primo F., Patrícia, Gonçalves, Gonzalez, Javier G., Nicolás, González, Ben, Gookin, Jacob, Gordon, Alessio, Gorgi, Peter, Gorham, Philippe, Gouffon, Stefan, Grebe, Nathan, Griffith, Aurelio, Grillo, Grubb, Trent D., Fausto, Guarino, Germano, Guedes, Matías Rolf Hampel, Patricia, Hansen, Diego, Harari, Harrison, Thomas A., Sebastian, Hartmann, John, Harton, Andreas, Haungs, Thomas, Hebbeker, Dieter, Heck, Philipp, Heimann, Herve, Alexander E., Hill, Gary C., Carlos, Hojvat, Nicholas, Hollon, Ewa, Holt, Piotr, Homola, Jörg, Hörandel, Pavel, Horvath, Miroslav, Hrabovský, Daniel, Huber, Tim, Huege, Antonio, Insolia, Paula Gina Isar, Ingolf, Jandt, Stefan, Jansen, Cecilia, Jarne, Mariela, Josebachuili, Alex, Kääpä, Olga, Kambeitz, Karl Heinz Kampert, Peter, Kasper, Igor, Katkov, Balazs, Kégl, Bianca, Keilhauer, Azadeh, Keivani, Ernesto, Kemp, Roger, Kieckhafer, Hans, Klages, Matthias, Kleifges, Jonny, Kleinfeller, Raphael, Krause, Nicole, Krohm, Oliver, Krömer, Daniel Kruppke Hansen, Daniel, Kuempel, Norbert, Kunka, Danielle, Lahurd, Luca, Latronico, Robert, Lauer, Markus, Lauscher, Pascal, Lautridou, Sandra Le Coz, Milton, Leão, Didier, Lebrun, Paul, Lebrun, Marcelo Augusto Leigui de Oliveira, Antoine Letessier Selvon, Isabelle Lhenry Yvon, Katrin, Link, Rebeca, López, Angeles Lopez Agüera, Karim, Louedec, Julio Lozano Bahilo, Lu, Lu, Agustin, Lucero, Marianne, Ludwig, Max, Malacari, Simone, Maldera, Manuela, Mallamaci, Jennifer, Maller, Dusan, Mandat, Paul, Mantsch, Analisa, Mariazzi, Vincent, Marin, Ioana, Mariş, Giovanni, Marsella, Daniele, Martello, Lilian, Martin, Humberto, Martinez, Oscar Martínez Bravo, Diane, Martraire, Jimmy Masías Meza, Hermann Josef Mathes, Sebastian, Mathys, James, Matthews, John, Matthews, Giorgio, Matthiae, Detlef, Maurel, Daniela, Maurizio, Eric, Mayotte, Peter, Mazur, Carlos, Medina, Gustavo Medina Tanco, Rebecca, Meissner, Maximilien, Melissas, Diego, Melo, Alexander, Menshikov, Stefano, Messina, Rishi, Meyhandan, Saša, Mićanović, Maria Isabel Micheletti, Lukas, Middendorf, Minaya, Ignacio A., Lino, Miramonti, Bogdan, Mitrica, Laura Molina Bueno, Silvia, Mollerach, Maria, Monasor, Delphine Monnier Ragaigne, François, Montanet, Carlo, Morello, Miguel, Mostafá, Moura, Celio A., Marcio Aparecido Muller, Gero, Müller, Sarah, Müller, Moritz, Münchmeyer, Roberto, Mussa, Gianni, Navarra, Sergio, Navas, Petr, Necesal, Lukas, Nellen, Anna, Nelles, Jens, Neuser, Nguyen, Phong H., Marcus, Niechciol, Lukas, Niemietz, Tim, Niggemann, Dave, Nitz, Dalibor, Nosek, Vladimir, Novotny, Lyberis, Nožka, Livingstone, Ochilo, Angela, Olinto, Micael, Oliveira, Noelia, Pacheco, Daniel Pakk Selmi Dei, Miroslav, Palatka, Juan, Pallotta, Nunzia, Palmieri, Philipp, Papenbreer, Gonzalo, Parente, Alejandra, Parra, Thomas, Paul, Miroslav, Pech, Jan, Pękala, Rodrigo, Pelayo, Iuri, Pepe, Lorenzo, Perrone, Emily, Petermann, Christine, Peters, Sergio, Petrera, Yevgeniy, Petrov, Jamyang, Phuntsok, Ricardo, Piegaia, Tanguy, Pierog, Pablo, Pieroni, Mário, Pimenta, Valerio, Pirronello, Manuel, Platino, Matthias, Plum, Alessio, Porcelli, Czeslaw, Porowski, Raul Ribeiro Prado, Paolo, Privitera, Michael, Prouza, Victor, Purrello, Quel, Eduardo J., Sven, Querchfeld, Sean, Quinn, Julian, Rautenberg, Olivier, Ravel, Diego, Ravignani, Benoît, Revenu, Jan, Ridky, Simone, Riggi, Markus, Risse, Pablo, Ristori, Vincenzo, Rizi, Washington Rodrigues de Carvalho, Iago Rodriguez Cabo, Gonzalo Rodriguez Fernandez, Jorge Rubén Rodriguez Rojo, Maria Dolores Rodríguez Frías, Dmytro, Rogozin, Germán, Ros, Jaime, Rosado, Tomas, Rossler, Markus, Roth, Esteban, Roulet, Adrian, Rovero, Saffi, Steven J., Alexandra, Saftoiu, Francesco, Salamida, Humberto, Salazar, Ahmed, Saleh, Francisco Salesa Greus, Gaetano, Salina, Federico, Sánchez, Patricia Sanchez Lucas, Santo, Catarina E., Edivaldo Moura Santos, Eva, Santos, Fred, Sarazin, Biswaijt, Sarkar, Raul, Sarmento, Ricardo, Sato, Nils, Scharf, Viviana, Scherini, Harald, Schieler, Peter, Schiffer, David, Schmidt, Olaf, Scholten, Harm, Schoorlemmer, Petr, Schovánek, Alexander, Schulz, Johannes, Schulz, Johannes, Schumacher, Sergio, Sciutto, Alberto, Segreto, Mariangela, Settimo, Amir, Shadkam, Shellard, Ronald C., Iván, Sidelnik, Guenter, Sigl, Octavian, Sima, Andrzej, Śmiałkowski, Radomir, Šmída, Gregory, Snow, Paul, Sommers, Sorokin, J., Ruben, Squartini, Srivastava, Yogendra N., Samo, Stanič, James, Stapleton, Jaroslaw, Stasielak, Maurice, Stephan, Anne, Stutz, Federico, Suarez, Tiina, Suomijärvi, Daniel Supanitsky, A., Michael, Sutherland, John, Swain, Zbigniew, Szadkowski, Marek, Szuba, Oscar Alejandro Taborda, Alex, Tapia, Mathieu, Tartare, Andreas, Tepe, Vanessa Menezes Theodoro, Charles, Timmermans, Todero Peixoto, Carlos J., Gabriel, Toma, Lenka, Tomankova, Bernardo, Tomé, Aurelio, Tonachini, Guillermo Torralba Elipe, Diego Torres Machado, Petr, Travnicek, Enrica, Trovato, Matias, Tueros, Ralf, Ulrich, Michael, Unger, Martin, Urban, Valdés Galicia, Jose F., Ines, Valiño, Laura, Valore, Guus van Aar, Patrick van Bodegom, van den Berg, Ad M., Sjoert van Velzen, Arjen van Vliet, Enrique, Varela, Bernardo Vargas Cárdenas, Gary, Varner, Vázquez, Jose R., Ricardo, Vázquez, Darko, Veberič, Valerio, Verzi, Jakub, Vicha, Mariela, Videla, Luis, Villaseñor, Brian, Vlcek, Serguei, Vorobiov, Hernan, Wahlberg, Oscar, Wainberg, David, Walz, Alan, Watson, Marc, Weber, Klaus, Weidenhaupt, Andreas, Weindl, Felix, Werner, Allan, Widom, Lawrence, Wiencke, Barbara, Wilczyńska, Henryk, Wilczyński, Martin, Will, Christopher, Williams, Tobias, Winchen, David, Wittkowski, Brian, Wundheiler, Sarka, Wykes, Tokonatsu, Yamamoto, Tolga, Yapici, Guofeng, Yuan, Alexey, Yushkov, Bruno, Zamorano, Enrique, Zas, Danilo, Zavrtanik, Marko, Zavrtanik, Ingyin, Zaw, Arnulfo, Zepeda, Jing, Zhou, Yue, Zhu, Marcelo Zimbres Silva, Michael, Ziolkowski, Francesca, Zuccarello, Rasha, Abbasi, Michihiko, Abe, Tareq Abu Zayyad, Monica, Allen, Robyn, Anderson, Ryuji, Azuma, Elliott, Barcikowski, Belz, John W., Bergman, Douglas R., Samuel Adam Blake, Robert, Cady, Min Jung Chae, Byung Gu Cheon, Junsei, Chiba, Michiyuki, Chikawa, Woo Ram Cho, Masaki, Fukushima, Takashi, Goto, William, Hanlon, Yoshio, Hayashi, Naoaki, Hayashida, Kinya, Hibino, Ken, Honda, Daisuke, Ikeda, Naoya, Inoue, Takaaki, Ishii, Rie, Ishimori, Hideo Ito (Utah, U., Riken, Dmitri, Ivanov, Jui, Charles C. H., Kenichi, Kadota, Fumio, Kakimoto, Oleg, Kalashev, Katsuaki, Kasahara, Hideyuki, Kawai, Saburo, Kawakami, Shingo, Kawana, Kazumasa, Kawata, Eiji, Kido, Hang Bae Kim, Ji Hee Kim, Ji Hyun Kim, Seiji, Kitamura, Yuki, Kitamura, Vadim, Kuzmin, Young Joon Kwon, Jian, Lan, Sun In Lim, Jon Paul Lundquist, Kazuhiro, Machida, Kai, Martens, Takeshi, Matsuda, Toshio, Matsuyama, Matthews, John N., Mayuko, Minamino, Keijiro, Mukai, Isaac, Myers, Keisuke, Nagasawa, Shigehiro, Nagataki, Toru, Nakamura, Toshiyuki, Nonaka, Asuka, Nozato, Shoichi, Ogio, Jun, Ogura, Munehiro, Ohnishi, Hideyuki, Ohoka, Kaoru, Oki, Takeshi, Okuda, Masaomi, Ono, Akitoshi, Oshima, Shunsuke, Ozawa, Park, Il H., Pshirkov, Maxim S., Douglas Chase Rodriguez, Grigory, Rubtsov, Dongsu, Ryu, Hiroyuki, Sagawa, Nobuyuki, Sakurai, Sampson, Amanda L., Scott, Lauren M., Priti Dhanesh Shah, Fumiya, Shibata, Tatsunobu, Shibata, Hideaki, Shimodaira, Bok Kyun Shin, Smith, Jeremy D., Pierre, Sokolsky, Wayne Springer, R., Benjamin Taylor Stokes, Stratton, Sean R., Thomas, Stroman, Takumi, Suzawa, Mai, Takamura, Masahiro, Takeda, Ryuji, Takeishi, Akimichi, Taketa, Masato, Takita, Yuichiro, Tameda, Hideki, Tanaka, Koichi, Tanaka, Manobu, Tanaka, Thomas, Stanton B., Thomson, Gordon B., Peter, Tinyakov, Igor, Tkachev, Hisao, Tokuno, Takayuki, Tomida, Sergey, Troitsky, Yoshiki, Tsunesada, Kazuki, Tsutsumi, Yukio, Uchihori, Shigeharu, Udo, Federico, Urban, Gina, Vasiloff, Tiffany, Wong, Hiroshi, Yamaoka, Katsuya, Yamazaki, Jongmann, Yang, Kenta, Yashiro, Shigeru, Yoshida, Hisashi, Yoshii, Rhett, Zollinger, Zachary, Zundel, Shogo, Konishi, Shingo, Wachi, Yoshiki, Nishimoto, Heungsu, Shin, Mai, Tsujimoto, Tomoya, Matsuhira, Laboratoire de Physique Nucléaire et de Hautes Énergies (LPNHE), Université Pierre et Marie Curie - Paris 6 (UPMC)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris Diderot - Paris 7 (UPD7)-Centre National de la Recherche Scientifique (CNRS), Laboratoire SUBATECH Nantes (SUBATECH), Mines Nantes (Mines Nantes)-Université de Nantes (UN)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Unité Scientifique de la Station de Nançay (USN), Observatoire des Sciences de l'Univers en région Centre (OSUC), Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de l'Accélérateur Linéaire (LAL), Université Paris-Sud - Paris 11 (UP11)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Centre National de la Recherche Scientifique (CNRS), Laboratoire de Physique Subatomique et de Cosmologie (LPSC), Université Joseph Fourier - Grenoble 1 (UJF)-Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Centre National de la Recherche Scientifique (CNRS), Institut de Physique Nucléaire d'Orsay (IPNO), PIERRE AUGER, Centre National de la Recherche Scientifique (CNRS)-Université Paris Diderot - Paris 7 (UPD7)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Pierre et Marie Curie - Paris 6 (UPMC), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université de Nantes (UN)-Mines Nantes (Mines Nantes), Centre National de la Recherche Scientifique (CNRS)-Observatoire de Paris, Université Paris sciences et lettres (PSL)-Université Paris sciences et lettres (PSL)-Institut national des sciences de l'Univers (INSU - CNRS)-Observatoire des Sciences de l'Univers en région Centre (OSUC), Université Paris sciences et lettres (PSL)-Université d'Orléans (UO)-Centre National de la Recherche Scientifique (CNRS)-Université d'Orléans (UO), Centre National de la Recherche Scientifique (CNRS)-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Paris-Sud - Paris 11 (UP11), Institut polytechnique de Grenoble - Grenoble Institute of Technology (Grenoble INP )-Institut Polytechnique de Grenoble - Grenoble Institute of Technology-Institut National de Physique Nucléaire et de Physique des Particules du CNRS (IN2P3)-Université Joseph Fourier - Grenoble 1 (UJF)-Centre National de la Recherche Scientifique (CNRS), A., Aab, P., Abreu, M., Aglietta, E. J., Ahn, I., Al Samarai, I. F. M., Albuquerque, I., Allekotte, J., Allen, P., Allison, A., Almela, J., Alvarez Castillo, J., Alvarez Mu?iz, R., Alves Batista, M., Ambrosio, A., Aminaei, L., Anchordoqui, S., Andringa, Aramo, Carla, F., Arquero, H., Asorey, P., Assi, J., Aublin, M., Ave, M., Avenier, G., Avila, A. M., Badescu, K. B., Barber, J., B?uml, C., Bau, J. J., Beatty, K. H., Becker, J. A., Bellido, C., Berat, M. E., Bertaina, X., Bertou, P. L., Biermann, P., Billoir, M., Blanco, C., Bleve, H., Bl?mer, M., Boh??ov?, D., Boncioli, C., Bonifazi, R., Bonino, N., Borodai, J., Brack, I., Brancu, P., Brogueira, W. C., Brown, P., Buchholz, A., Bueno, S., Buitink, Buscemi, Mario, K. S., Caballero Mora, B., Caccianiga, L., Caccianiga, M., Candusso, L., Caramete, R., Caruso, A., Castellina, G., Cataldi, L., Cazon, R., Cester, A. G., Chavez, A., Chiavassa, J. A., Chinellato, J., Chudoba, Cilmo, Marco, R. W., Clay, G., Cocciolo, Colalillo, Roberta, A., Coleman, L., Collica, M. R., Coluccia, R., Concei??o, F., Contrera, M. J., Cooper, A., Cordier, S., Coutu, C. E., Covault, J., Cronin, A., Curutiu, R., Dallier, B., Daniel, S., Dasso, K., Daumiller, B. R., Dawson, R. M., de Almeida, M., De Domenico, S. J., de Jong, J. R. T., de Mello Neto, I., De Mitri, J., de Oliveira, V., de Souza, L., del Peral, O., Deligny, H., Dembinski, N., Dhital, C., Di Giulio, A., Di Matteo, J. C., Diaz, M. L., D?az Castro, F., Diogo, C., Dobrigkeit, W., Docter, J. C., D'Olivo, A., Dorofeev, Q., Dorosti Hasankiadeh, M. T., Dova, J., Ebr, R., Engel, M., Erdmann, M., Erfani, C. O., Escobar, J., Espadanal, A., Etchegoyen, P., Facal San Lui, H., Falcke, K., Fang, G., Farrar, A. C., Fauth, N., Fazzini, A. P., Ferguson, M., Fernande, B., Fick, J. M., Figueira, A., Filevich, A., Filip?i?, B. D., Fox, O., Fratu, U., Fr?hlich, B., Fuch, T., Fuji, R., Gaior, B., Garc?a, S. T., Garcia Roca, D., Garcia Gamez, D., Garcia Pinto, G., Garilli, A., Gascon Bravo, F., Gate, H., Gemmeke, P. L., Ghia, U., Giaccari, M., Giammarchi, M., Giller, C., Glaser, H., Gla, M., G?mez Berisso, P. F., G?mez Vitale, P., Gon?alve, J. G., Gonzalez, N., Gonz?lez, B., Gookin, A., Gorgi, P., Gorham, P., Gouffon, S., Grebe, N., Griffith, A. F., Grillo, T. D., Grubb, Y., Guardincerri, Guarino, Fausto, G. P., Guede, M. R., Hampel, P., Hansen, D., Harari, T. A., Harrison, S., Hartmann, J. L., Harton, A., Haung, T., Hebbeker, D., Heck, P., Heimann, A. E., Herve, G. C., Hill, C., Hojvat, N., Hollon, E., Holt, P., Homola, J. R., H?randel, P., Horvath, M., Hrabovsk?, D., Huber, T., Huege, A., Insolia, P. G., Isar, K., Islo, I., Jandt, S., Jansen, C., Jarne, M., Josebachuili, A., K??p?, O., Kambeitz, K. H., Kampert, P., Kasper, I., Katkov, B., K?gl, B., Keilhauer, A., Keivani, E., Kemp, R. M., Kieckhafer, H. O., Klage, M., Kleifge, J., Kleinfeller, R., Krause, N., Krohm, O., Kr?mer, D., Kruppke Hansen, D., Kuempel, N., Kunka, G., La Rosa, D., Lahurd, L., Latronico, R., Lauer, M., Lauscher, P., Lautridou, S., Le Coz, M. S. A. B., Le?o, D., Lebrun, P., Lebrun, M. A., Leigui de Oliveira, A., Letessier Selvon, I., Lhenry Yvon, K., Link, R., L?pez, A., Lopez Ag?era, K., Louedec, J., Lozano Bahilo, L., Lu, A., Lucero, M., Ludwig, M. C., Maccarone, M., Malacari, S., Maldera, M., Mallamaci, J., Maller, D., Mandat, P., Mantsch, A. G., Mariazzi, V., Marin, I. C., Mari?, G., Marsella, D., Martello, L., Martin, H., Martinez, O., Mart?nez Bravo, D., Martraire, J. J., Mas?as Meza, H. J., Mathe, S., Mathy, J. A. J., Matthew, J., Matthew, G., Matthiae, D., Maurel, D., Maurizio, E., Mayotte, P. O., Mazur, C., Medina, G., Medina Tanco, M., Melissa, D., Melo, E., Menichetti, A., Menshikov, S., Messina, R., Meyhandan, S., Mi?anovi?, M. I., Micheletti, L., Middendorf, I. A., Minaya, L., Miramonti, B., Mitrica, L., Molina Bueno, S., Mollerach, M., Monasor, D., Monnier Ragaigne, F., Montanet, C., Morello, M., Mostaf?, C. A., Moura, M. A., Muller, G., M?ller, M., M?nchmeyer, R., Mussa, G., Navarra, S., Nava, P., Necesal, L., Nellen, A., Nelle, J., Neuser, M., Niechciol, L., Niemietz, T., Niggemann, D., Nitz, D., Nosek, V., Novotny, L., No?ka, L., Ochilo, A., Olinto, M., Oliveira, N., Pacheco, D., Pakk Selmi Dei, M., Palatka, J., Pallotta, N., Palmieri, P., Papenbreer, G., Parente, A., Parra, T., Paul, M., Pech, J., P?kala, R., Pelayo, I. M., Pepe, L., Perrone, R., Pesce, E., Petermann, C., Peter, S., Petrera, A., Petrolini, Y., Petrov, J., Phuntsok, R., Piegaia, T., Pierog, P., Pieroni, M., Pimenta, V., Pirronello, M., Platino, M., Plum, A., Porcelli, C., Porowski, R. R., Prado, P., Privitera, M., Prouza, V., Purrello, E. J., Quel, S., Querchfeld, S., Quinn, J., Rautenberg, O., Ravel, D., Ravignani, B., Revenu, J., Ridky, S., Riggi, M., Risse, P., Ristori, V., Rizi, J., Robert, W., Rodrigues de Carvalho, I., Rodriguez Cabo, G., Rodriguez Fernandez, J., Rodriguez Rojo, M. D., Rodr?guez Fr?a, G., Ro, J., Rosado, T., Rossler, M., Roth, E., Roulet, A. C., Rovero, S. J., Saffi, A., Saftoiu, F., Salamida, H., Salazar, A., Saleh, F., Salesa Greu, G., Salina, F., S?nchez, P., Sanchez Luca, C. E., Santo, E., Santo, E. M., Santo, F., Sarazin, B., Sarkar, R., Sarmento, R., Sato, N., Scharf, V., Scherini, H., Schieler, P., Schiffer, O., Scholten, H., Schoorlemmer, P., Schov?nek, A., Schulz, J., Schulz, J., Schumacher, S. J., Sciutto, A., Segreto, M., Settimo, A., Shadkam, R. C., Shellard, I., Sidelnik, G., Sigl, O., Sima, A., ?mia?kowski, R., ?m?da, G. R., Snow, P., Sommer, J., Sorokin, R., Squartini, Y. N., Srivastava, S., Stani?, J., Stapleton, J., Stasielak, M., Stephan, A., Stutz, F., Suarez, T., Suomij?rvi, A. D., Supanitsky, M. S., Sutherland, J., Swain, Z., Szadkowski, M., Szuba, O. A., Taborda, A., Tapia, M., Tartare, V. M., Theodoro, C., Timmerman, C. J., Todero Peixoto, G., Toma, L., Tomankova, B., Tom?, A., Tonachini, G., Torralba Elipe, D., Torres Machado, P., Travnicek, E., Trovato, M., Tuero, R., Ulrich, M., Unger, M., Urban, Galicia, J. F. Vald?s., I., Vali?o, Valore, Laura, G., van Aar, A. M., van den Berg, S., van Velzen, A., van Vliet, E., Varela, B., Vargas C?rdena, G., Varner, J. R., V?zquez, R. A., V?zquez, D., Veberi?, V., Verzi, J., Vicha, M., Videla, L., Villase?or, B., Vlcek, S., Vorobiov, H., Wahlberg, O., Wainberg, D., Walz, A. A., Watson, M., Weber, K., Weidenhaupt, A., Weindl, F., Werner, A., Widom, L., Wiencke, B., Wilczy?ska, H., Wilczy?ski, M., Will, C., William, T., Winchen, D., Wittkowski, B., Wundheiler, S., Wyke, T., Yamamoto, T., Yapici, P., Younk, G., Yuan, A., Yushkov, B., Zamorano, E., Za, D., Zavrtanik, M., Zavrtanik, I., Zaw, A., Zepeda, J., Zhou, Y., Zhu, M., Zimbres Silva, M., Ziolkowski, R. U., Abbasi, M., Abe, T., Abu Zayyad, M., Allen, R., Anderson, R., Azuma, E., Barcikowski, J. W., Belz, D. R., Bergman, S. A., Blake, R., Cady, M. J., Chae, B. G., Cheon, J., Chiba, M., Chikawa, W. R., Cho, T., Fujii, M., Fukushima, T., Goto, W., Hanlon, Y., Hayashi, N., Hayashida, K., Hibino, K., Honda, D., Ikeda, N., Inoue, T., Ishii, R., Ishimori, H., Ito, D., Ivanov, C. C. H., Jui, K., Kadota, F., Kakimoto, O., Kalashev, K., Kasahara, H., Kawai, S., Kawakami, S., Kawana, K., Kawata, E., Kido, H. B., Kim, J. H., Kim, S., Kitamura, Y., Kitamura, V., Kuzmin, Y. J., Kwon, J., Lan, S. I., Lim, J. 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B., Thomson, P., Tinyakov, I., Tkachev, H., Tokuno, T., Tomida, S., Troitsky, Y., Tsunesada, K., Tsutsumi, Y., Uchihori, S., Udo, F., Urban, G., Vasiloff, T., Wong, R., Yamane, H., Yamaoka, K., Yamazaki, J., Yang, K., Yashiro, Y., Yoneda, S., Yoshida, H., Yoshii, R., Zollinger, Z., Zundel, I. A., Samarai, I. F., M., J. A., Castillo, J., Alvarez Muñiz, R. A., Batista, C., Aramo, J., Bäuml, Bleve, Carla, H., Blümer, M., Boháčová, M., Buscemi, M., Cilmo, Cocciolo, Giuseppe, R., Colalillo, Coluccia, MARIA RITA, R., Conceição, R. M., De, M. D., Domenico, S. J., De, J. R., T., DE MITRI, Ivan, J. d., Oliveira, V. d., Souza, L. d., Peral, C. D., Giulio, A. D., Matteo, M. L., Díaz, Q. D., Hasankiadeh, P. F., San, A., Filipčič, U., Fröhlich, B., García, S. T., Garcia, A. G., Bravo, M. G., Berisso, P. F., Gómez, P., Gonçalve, N., González, F., Guarino, J. R., Hörandel, M., Hrabovský, A., Kääpä, B., Kégl, O., Krömer, G. L., Rosa, S. L., Coz, M. S., A., M. A., Leigui, R., López, A. L., Agüera, J. L., Bahilo, I. C., Mariş, Marsella, Giovanni, Martello, Daniele, O. M., Bravo, J. J., Masía, J. A., J., S., Mićanović, D. M., Ragaigne, M., Mostafá, G., Müller, M., Münchmeyer, L., Nožka, D. P., Selmi Dei, J., Pękala, Perrone, Lorenzo, W. R., De, I. R., Cabo, G. R., Fernandez, J. R., Rojo, M. D., Rodríguez Fría, F. S., Greu, F., Sánchez, Scherini, Viviana, P., Schovánek, A., Śmiałkowski, R., Šmída, S., Stanič, T., Suomijärvi, C. J., Todero, B., Tomé, G. T., Elipe, D. T., Machado, J. F., Valdé, I., Valiño, L., Valore, G. v., Aar, A. M., Van, S. v., Velzen, A. v., Vliet, B. V., Cárdena, J. R., Vázquez, R. A., Vázquez, D., Veberič, L., Villaseñor, B., Wilczyńska, H., Wilczyński, M. Z., Silva, T. P., Auger, C. C., H., T. T., Array, A. Aab, P. Abreu, M. Aglietta, E. J. Ahn, I. A. Samarai, I. F. M., I. Allekotte, J. Allen, P. Allison, A. Almela, J. A. Castillo, J. Alvarez-Muñiz, R. A. Batista, M. Ambrosio, A. Aminaei, L. Anchordoqui, S. Andringa, C. Aramo, F. Arquero, H. Asorey, P. Assi, J. Aublin, M. Ave, M. Avenier, G. Avila, A. M. Badescu, K. B. Barber, J. Bäuml, C. Bau, J. J. Beatty, K. H. Becker, J. A. Bellido, C. Berat, M. E. Bertaina, X. Bertou, P. L. Biermann, P. Billoir, M. Blanco, C. Bleve, H. Blümer, M. Boháčová, D. Boncioli, C. Bonifazi, R. Bonino, N. Borodai, J. Brack, I. Brancu, P. Brogueira, W. C. Brown, P. Buchholz, A. Bueno, S. Buitink, M. Buscemi, K. S. Caballero-Mora, B. Caccianiga, L. Caccianiga, M. Candusso, L. Caramete, R. Caruso, A. Castellina, G. Cataldi, L. Cazon, R. Cester, A. G. Chavez, A. Chiavassa, J. A. Chinellato, J. Chudoba, M. Cilmo, R. W. Clay, G. Cocciolo, R. Colalillo, A. Coleman, L. Collica, M. R. Coluccia, R. Conceição, F. Contrera, M. J. Cooper, A. Cordier, S. Coutu, C. E. Covault, J. Cronin, A. Curutiu, R. Dallier, B. Daniel, S. Dasso, K. Daumiller, B. R. Dawson, R. M. de, M. D. Domenico, S. J. de, J. R. T., I. D. Mitri, J. d. Oliveira, V. d. Souza, L. d. Peral, O. Deligny, H. Dembinski, N. Dhital, C. D. Giulio, A. D. Matteo, J. C. Diaz, M. L. Díaz, F. Diogo, C. Dobrigkeit, W. Docter, J. C. D'Olivo, A. Dorofeev, Q. D. Hasankiadeh, M. T. Dova, J. Ebr, R. Engel, M. Erdmann, M. Erfani, C. O. Escobar, J. Espadanal, A. Etchegoyen, P. F. San, H. Falcke, K. Fang, G. Farrar, A. C. Fauth, N. Fazzini, A. P. Ferguson, M. Fernande, B. Fick, J. M. Figueira, A. Filevich, A. Filipčič, B. D. Fox, O. Fratu, U. Fröhlich, B. Fuch, T. Fuji, R. Gaior, B. García, S. T. Garcia, D. Garcia-Gamez, D. Garcia-Pinto, G. Garilli, A. G. Bravo, F. Gate, H. Gemmeke, P. L. Ghia, U. Giaccari, M. Giammarchi, M. Giller, C. Glaser, H. Gla, M. G. Berisso, P. F. Gómez, P. Gonçalve, J. G. Gonzalez, N. González, B. Gookin, A. Gorgi, P. Gorham, P. Gouffon, S. Grebe, N. Griffith, A. F. Grillo, T. D. Grubb, Y. Guardincerri, F. Guarino, G. P. Guede, M. R. Hampel, P. Hansen, D. Harari, T. A. Harrison, S. Hartmann, J. L. Harton, A. Haung, T. Hebbeker, D. Heck, P. Heimann, A. E. Herve, G. C. Hill, C. Hojvat, N. Hollon, E. Holt, P. Homola, J. R. Hörandel, P. Horvath, M. Hrabovský, D. Huber, T. Huege, A. Insolia, P. G. Isar, K. Islo, I. Jandt, S. Jansen, C. Jarne, M. Josebachuili, A. Kääpä, O. Kambeitz, K. H. Kampert, P. Kasper, I. Katkov, B. Kégl, B. Keilhauer, A. Keivani, E. Kemp, R. M. Kieckhafer, H. O. Klage, M. Kleifge, J. Kleinfeller, R. Krause, N. Krohm, O. Krömer, D. Kruppke-Hansen, D. Kuempel, N. Kunka, G. L. Rosa, D. LaHurd, L. Latronico, R. Lauer, M. Lauscher, P. Lautridou, S. L. Coz, M. S. A., D. Lebrun, P. Lebrun, M. A. Leigui, A. Letessier-Selvon, I. Lhenry-Yvon, K. Link, R. López, A. L. Agüera, K. Louedec, J. L. Bahilo, L. Lu, A. Lucero, M. Ludwig, M. C. Maccarone, M. Malacari, S. Maldera, M. Mallamaci, J. Maller, D. Mandat, P. Mantsch, A. G. Mariazzi, V. Marin, I. C. Mariş, G. Marsella, D. Martello, L. Martin, H. Martinez, O. M. Bravo, D. Martraire, J. J. Masía, H. J. Mathe, S. Mathy, J. A. J., J. Matthew, G. Matthiae, D. Maurel, D. Maurizio, E. Mayotte, P. O. Mazur, C. Medina, G. Medina-Tanco, M. Melissa, D. Melo, E. Menichetti, A. Menshikov, S. Messina, R. Meyhandan, S. Mićanović, M. I. Micheletti, L. Middendorf, I. A. Minaya, L. Miramonti, B. Mitrica, L. Molina-Bueno, S. Mollerach, M. Monasor, D. M. Ragaigne, F. Montanet, C. Morello, M. Mostafá, C. A. Moura, M. A. Muller, G. Müller, M. Münchmeyer, R. Mussa, G. Navarra, S. Nava, P. Necesal, L. Nellen, A. Nelle, J. Neuser, M. Niechciol, L. Niemietz, T. Niggemann, D. Nitz, D. Nosek, V. Novotny, L. Nožka, L. Ochilo, A. Olinto, M. Oliveira, N. Pacheco, D. P. Selmi-Dei, M. Palatka, J. Pallotta, N. Palmieri, P. Papenbreer, G. Parente, A. Parra, T. Paul, M. Pech, J. Pękala, R. Pelayo, I. M. Pepe, L. Perrone, R. Pesce, E. Petermann, C. Peter, S. Petrera, A. Petrolini, Y. Petrov, J. Phuntsok, R. Piegaia, T. Pierog, P. Pieroni, M. Pimenta, V. Pirronello, M. Platino, M. Plum, A. Porcelli, C. Porowski, R. R. Prado, P. Privitera, M. Prouza, V. Purrello, E. J. Quel, S. Querchfeld, S. Quinn, J. Rautenberg, O. Ravel, D. Ravignani, B. Revenu, J. Ridky, S. Riggi, M. Risse, P. Ristori, V. Rizi, J. Robert, W. R. de, I. R. Cabo, G. R. Fernandez, J. R. Rojo, M. D. Rodríguez-Fría, G. Ro, J. Rosado, T. Rossler, M. Roth, E. Roulet, A. C. Rovero, S. J. Saffi, A. Saftoiu, F. Salamida, H. Salazar, A. Saleh, F. S. Greu, G. Salina, F. Sánchez, P. Sanchez-Luca, C. E. Santo, E. Santo, E. M. Santo, F. Sarazin, B. Sarkar, R. Sarmento, R. Sato, N. Scharf, V. Scherini, H. Schieler, P. Schiffer, O. Scholten, H. Schoorlemmer, P. Schovánek, A. Schulz, J. Schulz, J. Schumacher, S. J. Sciutto, A. Segreto, M. Settimo, A. Shadkam, R. C. Shellard, I. Sidelnik, G. Sigl, O. Sima, A. Śmiałkowski, R. Šmída, G. R. Snow, P. Sommer, J. Sorokin, R. Squartini, Y. N. Srivastava, S. Stanič, J. Stapleton, J. Stasielak, M. Stephan, A. Stutz, F. Suarez, T. Suomijärvi, A. D. Supanitsky, M. S. Sutherland, J. Swain, Z. Szadkowski, M. Szuba, O. A. Taborda, A. Tapia, M. Tartare, V. M. Theodoro, C. Timmerman, C. J. Todero, G. Toma, L. Tomankova, B. Tomé, A. Tonachini, G. T. Elipe, D. T. Machado, P. Travnicek, E. Trovato, M. Tuero, R. Ulrich, M. Unger, M. Urban, J. F. Valdé, I. Valiño, L. Valore, G. v. Aar, A. M. van, S. v. Velzen, A. v. Vliet, E. Varela, B. V. Cárdena, G. Varner, J. R. Vázquez, R. A. Vázquez, D. Veberič, V. Verzi, J. Vicha, M. Videla, L. Villaseñor, B. Vlcek, S. Vorobiov, H. Wahlberg, O. Wainberg, D. Walz, A. A. Watson, M. Weber, K. Weidenhaupt, A. Weindl, F. Werner, A. Widom, L. Wiencke, B. Wilczyńska, H. Wilczyński, M. Will, C. William, T. Winchen, D. Wittkowski, B. Wundheiler, S. Wyke, T. Yamamoto, T. Yapici, P. Younk, G. Yuan, A. Yushkov, B. Zamorano, E. Za, D. Zavrtanik, M. Zavrtanik, I. Zaw, A. Zepeda, J. Zhou, Y. Zhu, M. Z. Silva, M. Ziolkowski, T. P. Auger, R. U. Abbasi, M. Abe, T. Abu-Zayyad, M. Allen, R. Anderson, R. Azuma, E. Barcikowski, J. W. Belz, D. R. Bergman, S. A. Blake, R. Cady, M. J. Chae, B. G. Cheon, J. Chiba, M. Chikawa, W. R. Cho, T. Fujii, M. Fukushima, T. Goto, W. Hanlon, Y. Hayashi, N. Hayashida, K. Hibino, K. Honda, D. Ikeda, N. Inoue, T. Ishii, R. Ishimori, H. Ito, D. Ivanov, C. C. H., K. Kadota, F. Kakimoto, O. Kalashev, K. Kasahara, H. Kawai, S. Kawakami, S. Kawana, K. Kawata, E. Kido, H. B. Kim, J. H. Kim, S. Kitamura, Y. Kitamura, V. Kuzmin, Y. J. Kwon, J. Lan, S. I. Lim, J. P. Lundquist, K. Machida, K. Marten, T. Matsuda, T. Matsuyama, J. N. Matthew, M. Minamino, K. Mukai, I. Myer, K. Nagasawa, S. Nagataki, T. Nakamura, T. Nonaka, A. Nozato, S. Ogio, J. Ogura, M. Ohnishi, H. Ohoka, K. Oki, T. Okuda, M. Ono, A. Oshima, S. Ozawa, I. H. Park, M. S. Pshirkov, D. C. Rodriguez, 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. D. Smith, P. Sokolsky, R. W. Springer, B. T. Stoke, S. R. Stratton, T. A. Stroman, T. Suzawa, M. Takamura, M. Takeda, R. Takeishi, A. Taketa, M. Takita, Y. Tameda, H. Tanaka, K. Tanaka, M. Tanaka, S. B. Thoma, G. B. Thomson, P. Tinyakov, I. Tkachev, H. Tokuno, T. Tomida, S. Troitsky, Y. Tsunesada, K. Tsutsumi, Y. Uchihori, S. Udo, F. Urban, G. Vasiloff, T. Wong, R. Yamane, H. Yamaoka, K. Yamazaki, J. Yang, K. Yashiro, Y. Yoneda, S. Yoshida, H. Yoshii, R. Zollinger, Z. Zundel, T. T. Array, and Research unit Astroparticle Physics
Subjects: Ciencias Físicas, Astronomy, Rays, Astrophysics, Astroparticle physics, Cosmic rays, 01 natural sciences, law.invention, Pierre, law, Anisotropy, Telescope, 010303 astronomy & astrophysics, High Energy Astrophysical Phenomena (astro-ph.HE), Physics, [PHYS]Physics [physics], Energy, [SDU.ASTR.HE]Sciences of the Universe [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], Astrophysics::Instrumentation and Methods for Astrophysics, astroparticle physic, Radiación cósmica, Auger, Cosmic, Arrival, ComputingMethodologies_DOCUMENTANDTEXTPROCESSING, Física nuclear, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, CIENCIAS NATURALES Y EXACTAS, High, [PHYS.ASTR.HE]Physics [physics]/Astrophysics [astro-ph]/High Energy Astrophysical Phenomena [astro-ph.HE], [PHYS.ASTR.IM]Physics [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Astrophysics::High Energy Astrophysical Phenomena, FOS: Physical sciences, Cosmic ray, SURFACE DETECTOR, ICECUBE, AIR-SHOWER ARRAY, Directions, cosmic rays, 0103 physical sciences, Instrumentation and Methods for Astrophysics (astro-ph.IM), Ciencias Exactas, Pierre Auger Observatory, SPECTRUM, 010308 nuclear & particles physics, Array, Spectral density, Spherical harmonics, Física, Astronomy and Astrophysics, ASTROFÍSICA, Ultra, [SDU.ASTR.IM]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Instrumentation and Methods for Astrophysic [astro-ph.IM], Astronomía, Dipole, RESOLUTION, Space and Planetary Science, Experimental High Energy Physics, Quadrupole, Observatory, [PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Abstract: Spherical harmonic moments are well-suited for capturing anisotropy at any scale in the flux of cosmic rays. An unambiguous measurement of the full set of spherical harmonic coefficients requires full-sky coverage. This can be achieved by combining data from observatories located in both the northern and southern hemispheres. To this end, a joint analysis using data recorded at the Telescope Array and the Pierre Auger Observatory above 1019 eV is presented in this work. The resulting multipolar expansion of the flux of cosmic rays allows us to perform a series of anisotropy searches, and in particular to report on the angular power spectrum of cosmic rays above 1019 eV. No significant deviation from isotropic expectations is found throughout the analyses performed. Upper limits on the amplitudes of the dipole and quadrupole moments are derived as a function of the direction in the sky, varying between 7% and 13% for the dipole and between 7% and 10% for a symmetric quadrupole., Facultad de Ciencias Exactas
Published: 2014
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50. Study of Ultra-High Energy Cosmic Ray Composition Using Telescope Array's Middle Drum Detector and Surface Array in Hybrid Mode

Author: J. D. Smith, Michiyuki Chikawa, Hideaki Shimodaira, Y. J. Kwon, Hideyuki Ohoka, Mayuko Minamino, Inkyu Park, K. Honda, Yasunori Kitamura, Igor Tkachev, Douglas Bergman, Kazumasa Kawata, R. Azuma, Masaaki Tanaka, S. Kitamura, Hidemi Ito, Rasha Abbasi, K. Yamazaki, Tareq Abu-Zayyad, R. Yamane, Hiroyuki Sagawa, Vladim Kuzmin, K. Martens, K. Oki, T. Goto, M. J. Chae, Y. Yoneda, N. Inoue, S. I. Lim, M. Ohnishi, Nobuyuki Sakurai, Takahiro Fujii, J. H. Kim, T.-A. Shibata, Gordon Thomson, S. Udo, C. C. H. Jui, Tom Stroman, Robert Cady, Elliott Barcikowski, Grigory Rubtsov, F. Kakimoto, L. M. Scott, S. B. Thomas, Kenta Yashiro, Dmitri Ivanov, A. Nozato, Y. Hayashi, Sergey Troitsky, H. Yoshii, Masato Takita, Akimichi Taketa, Bokkyun Shin, Mai Takamura, Fumiya Shibata, R. W. Springer, M. Abe, Takayuki Tomida, B. G. Cheon, R. Ishimori, R. Zollinger, A. L. Sampson, S. Yoshida, Tomohiro Matsuda, S. Kawakami, Zach Zundel, J. P. Lundquist, J. Yang, Hideki Tanaka, G. Vasiloff, Yoshiki Tsunesada, T. Matsuyama, Daisuke Ikeda, Hongsu Kim, J. Lan, Jyunsei Chiba, Dongsu Ryu, S. R. Stratton, K. Hibino, Tiffany Wong, Masaki Fukushima, Federico R. Urban, Takaaki Ishii, Peter Tinyakov, Samuel Blake, Shoichi Ogio, Maxim Pshirkov, K. Kasahara, Priti Shah, D. C. Rodriguez, Akitoshi Oshima, Masaomi Ono, Shunsuke Ozawa, Naoaki Hayashida, Toshiyuki Nonaka, T. Suzawa, Robert M. Anderson, Oleg Kalashev, W. R. Cho, K. Nagasawa, Y. Mukai, Hiroshi Yamaoka, Toru Nakamura, Isaac Myers, Kiyoshi Tanaka, Kenichi Kadota, Shingo Kawana, William Hanlon, T. Okuda, Y. Uchihori, H. Tokuno, Heungsu Shin, Ryuji Takeishi, M. Allen, Yuichiro Tameda, John N. Matthews, H. Kawai, John Belz, Eiji Kido, Kazuhiro Machida, K. Tsutsumi, Pierre Sokolsky, M. Takeda, Shigehiro Nagataki, J. Ogura, and B. T. Stokes
Subjects: Physics, Pierre Auger Observatory, High Energy Astrophysical Phenomena (astro-ph.HE), Resolution (electron density), Detector, FOS: Physical sciences, Astronomy and Astrophysics, Cosmic ray, Astrophysics, Auger, law.invention, Computational physics, Telescope, Observatory, law, Ultra-high-energy cosmic ray, Astrophysics - High Energy Astrophysical Phenomena, Astrophysics - Instrumentation and Methods for Astrophysics, Instrumentation and Methods for Astrophysics (astro-ph.IM)
Abstract: Previous measurements of the composition of Ultra-High Energy Cosmic Rays(UHECRs) made by the High Resolution Fly's Eye(HiRes) and Pierre Auger Observatory(PAO) are seemingly contradictory, but utilize different detection methods, as HiRes was a stereo detector and PAO is a hybrid detector. The five year Telescope Array(TA) Middle Drum hybrid composition measurement is similar in some, but not all, respects in methodology to PAO, and good agreement is evident between data and a light, largely protonic, composition when comparing the measurements to predictions obtained with the QGSJetII-03 and QGSJet-01c models. These models are also in agreement with previous HiRes stereo measurements, confirming the equivalence of the stereo and hybrid methods. The data is incompatible with a pure iron composition, for all models examined, over the available range of energies. The elongation rate and mean values of Xmax are in good agreement with Pierre Auger Observatory data. This analysis is presented using two methods: data cuts using simple geometrical variables and a new pattern recognition technique., Comment: 23 pages, 30 figures
Published: 2014
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