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Search for Point Sources of Ultra–High‐Energy Cosmic Rays above 4.0 x 1019eV Using a Maximum Likelihood Ratio Test

R. U. Abbasi,T. Abu‐Zayyad,J. F. Amann,G. Archbold,R. Atkins,J. A. Bellido,K. Belov,J. W. Belz,S. Y. Ben‐Zvi,D. R. Bergman,J. H. Boyer,G. W. Burt,Z. Cao,R. W. Clay,B. M. Connolly,B. R. Dawson,W. Deng,G. R. Farrar,Y. Fedorova,J. Findlay,C. B. Finley,W. F. Hanlon,C. M. Hoffman,M. H. Holzscheiter,G. A. Hughes,P. Huntemeyer,C. C. H. Jui, K. Kim,M. A. Kirn,B. C. Knapp,E. C. Loh,M. M. Maestas,N. Manago,E. J. Mannel,L. J. Marek,K. Martens,J. A. J. Matthews,J. N. Matthews,A. O’Neill,C. A. Painter,L. Perera,K. Reil,R. Riehle,M. D. Roberts,M. Sasaki,S. R. Schnetzer,M. Seman,K. M. Simpson,G. Sinnis,J. D. Smith,R. Snow,P. Sokolsky,C. Song,R. W. Springer,B. T. Stokes,J. R. Thomas,S. B. Thomas,G. B. Thomson,D. Tupa,S. Westerhoff,L. R. Wiencke,A. Zech

ASTROPHYSICAL JOURNAL（2005）

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关键词
acceleration of particles,cosmic rays,large-scale structure of universe
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