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SEARCH FOR ANISOTROPY OF ULTRAHIGH ENERGY COSMIC RAYS WITH THE TELESCOPE ARRAY EXPERIMENT

Author
ABU-ZAYYAD, T1 ; AIDA, R2 ; CHEON, B. G4 ; CHIBA, J5 ; CHIKAWA, M6 ; CHO, E. J4 ; CHO, W. R7 ; FUJII, H8 ; FUJII, T9 ; FUKUDA, T3 ; FUKUSHIMA, M10 11 ; HANLON, W1 ; ALLEN, M1 ; HAYASHI, K3 ; HAYASHI, Y9 ; HAYASHIDA, N10 ; HIBINO, K12 ; HIYAMA, K10 ; HONDA, K2 ; IGUCHI, T3 ; IKEDA, D10 ; IKUTA, K2 ; INOUE, N13 ; ANDERSON, R1 ; ISHII, T2 ; ISHIMORI, R3 ; IVANOV, D1 14 ; IWAMOTO, S2 ; JUI, C. C. H1 ; KADOTA, K15 ; KAKIMOTO, F3 ; KALASHEV, O16 ; KANBE, T2 ; KASAHARA, K17 ; AZUMA, R3 ; KAWAI, H18 ; KAWAKAMI, S9 ; KAWANA, S13 ; KIDO, E10 ; KIM, H. B4 ; KIM, H. K7 ; KIM, J. H4 ; KIM, J. H19 ; KITAMOTO, K6 ; KITAMURA, S3 ; BARCIKOWSKI, E1 ; KITAMURA, Y3 ; KOBAYASHI, K5 ; KOBAYASHI, Y3 ; KONDO, Y10 ; KURAMOTO, K9 ; KUZMIN, V16 ; KWON, Y. J7 ; LIM, S. I20 ; MACHIDA, S3 ; MARTENS, K11 ; BELZ, J. W1 ; BERGMAN, D. R1 ; BLAKE, S. A1 ; CADY, R1
[1] High Energy Astrophysics Institute and Department of Physics and Astronomy, University of Utah, Salt Lake City, UT, United States
[2] Interdisciplinary Graduate School of Medicine and Engineering, University of Yamanashi, Kofu, Yamanashi, Japan
[3] Graduate School of Science and Engineering, Tokyo Institute of Technology, Meguro, Tokyo, Japan
[4] Department of Physics and The Research Institute of Natural Science, Hanyang University, Seongdong-gu, Seoul, Korea, Republic of
[5] Department of Physics, Tokyo University of Science, Noda, Chiba, Japan
[6] Department of Physics, Kinki University, Higashi Osaka, Osaka, Japan
[7] Department of Physics, Yonsei University, Seodaemun-gu, Seoul, Korea, Republic of
[8] Institute of Particle and Nuclear Studies, KEK, Tsukuba, Ibaraki, Japan
[9] Graduate School of Science, Osaka City University, Osaka, Osaka, Japan
[10] Institute for Cosmic Ray Research, University of Tokyo, Kashiwa, Chiba, Japan
[11] Kavli Institute for the Physics and Mathematics of the Universe, University of Tokyo, Kashiwa, Chiba, Japan
[12] Faculty of Engineering, Kanagawa University, Yokohama, Kanagawa, Japan
[13] The Graduate School of Science and Engineering, Saitama University, Saitama, Saitama, Japan
[14] Department of Physics and Astronomy, Rutgers University, Piscataway, United States
[15] Department of Physics, Tokyo City University, Setagaya-ku, Tokyo, Japan
[16] Institute for Nuclear Research of the Russian Academy of Sciences, Moscow, Russian Federation
[17] Advanced Research Institute for Science and Engineering, Waseda University, Shinjuku-ku, Tokyo, Japan
[18] Department of Physics, Chiba University, Chiba, Chiba, Japan
[19] Department of Astronomy and Space Science, Chungnam National University, Yuseong-gu, Daejeon, Korea, Republic of
[20] Department of Physics and Institute for the Early Universe, Ewha Womans University, Seodaaemun-gu, Seoul, Korea, Republic of
Source

The Astrophysical journal. 2012, Vol 757, Num 1 ; 26.1-26.11 ; 1 ; ref : 3/4 p

CODEN
ASJOAB
ISSN
0004-637X
Scientific domain
Astronomy earth cosmic environment
Publisher
IOP, Bristol
Publication country
United Kingdom
Document type
Article
Language
Russian
Author keyword
acceleration of particles astroparticle physics cosmic rays magnetic fields methods: statistical relativistic processes
Keyword (fr)
Accélération particule Anisotropie Ascension droite Champ magnétique interstellaire Champ magnétique Corrélation Déflexion Energie seuil Galaxies actives Matrice détecteur Modèle Méthode statistique Noyau galactique actif Noyau galaxies Rayonnement cosmique Structure grande échelle
Keyword (en)
Particle acceleration Anisotropy Right ascension Interstellar magnetic fields Magnetic fields Correlations Deflection Threshold energy Active galaxies Dectector arrays Models Statistical method Active galaxy nuclei Galaxy nuclei Cosmic radiation Large-scale structure
Keyword (es)
Aceleración partícula Modelo Método estadístico
Classification
Pascal
001 Exact sciences and technology / 001E Earth, ocean, space / 001E03 Astronomy

Discipline
Astronomy
Origin
Inist-CNRS
Database
PASCAL
INIST identifier
26384544

Sauf mention contraire ci-dessus, le contenu de cette notice bibliographique peut être utilisé dans le cadre d’une licence CC BY 4.0 Inist-CNRS / Unless otherwise stated above, the content of this bibliographic record may be used under a CC BY 4.0 licence by Inist-CNRS / A menos que se haya señalado antes, el contenido de este registro bibliográfico puede ser utilizado al amparo de una licencia CC BY 4.0 Inist-CNRS

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