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Correlation of the highest-energy cosmic rays with nearby extragalactic objects

Journal article published in 2007 by J.; Abreu P.; Aglietta M.; Aguirre C.; Allard D.; Allekotte I.; Allen J.; Allison P.; Alvarez C.; Alvarez-Muniz J.; Ambrosio M.; /Balseiro Inst San Carlos de Bariloche /Buenos Aires CONICET /CNEA Buenos Aires /Pierre Auger Observ. /La Plata U. /Natl Tech Abraham, P. Abreu, M. Aglietta, C. Aguirre, D. Allard, I. Allekotte, J. C. D’olivo, J. Allen, P. Allison, C. Alvarez, J. Alvarez-muñiz, M. Ambrosio, J. R. T. de Mello Neto, L. Anchordoqui, S. Andringa and other authors.
This paper is available in a repository.
This paper is available in a repository.

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Abstract

Using data collected at the Pierre Auger Observatory during the past 3.7 years, we demonstrated a correlation between the arrival directions of cosmic rays with energy above 6 x 1019 electron volts and the positions of active galactic nuclei (AGN) lying within 75 megaparsecs. We rejected the hypothesis of an isotropic distribution of these cosmic rays with at least a 99% confidence level from a prescribed a priori test. The correlation we observed is compatible with the hypothesis that the highest-energy particles originate from nearby extragalactic sources whose flux has not been substantially reduced by interaction with the cosmic background radiation. AGN or objects having a similar spatial distribution are possible sources. ; © 2007 American Association for the Advancement of Science