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Research ArticlesCorrelation of the Highest-Energy Cosmic Rays with Nearby Extragalactic ObjectsThe Pierre Auger Collaboration*
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
* The full list of authors and their affiliations appears at the end of this paper. 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.
Observatorio Pierre Auger, Avenida San Martín Norte 304, (5613) Malargüe, Mendoza, Argentina. E-mail: auger_collaboration2{at}fnal.gov
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Science. ISSN 0036-8075 (print), 1095-9203 (online)
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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.