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001     85076
005     20250731122843.0
024 7 _ |a 10.1126/science.1151124
|2 doi
024 7 _ |a WOS:000250788500033
|2 WOS
024 7 _ |a altmetric:113347
|2 altmetric
024 7 _ |a pmid:17991855
|2 pmid
024 7 _ |a arXiv:0711.2256
|2 arXiv
024 7 _ |a inspire:767631
|2 inspire
024 7 _ |a openalex:W2147633035
|2 openalex
037 _ _ |a PHPPUBDB-7509
082 _ _ |a 500
088 1 _ |a arXiv:0711.2256; FERMILAB-PUB-07-579-AD-CD-E-TD
088 _ _ |a arXiv:0711.2256
|2 arXiv
088 _ _ |a FERMILAB-PUB-07-579-AD-CD-E-TD
|2 Fermilab
100 1 _ |a Abraham, J.
|0 INSPIRE-00148984
|b 0
110 1 _ |a DESY
|b Theorie
245 _ _ |a Correlation of the Highest Energy Cosmic Rays with Nearby Extragalactic Objects.
260 _ _ |a Washington, DC [u.a.]
|c 2008
|b American Association for the Advancement of Science16205
300 _ _ |a 938
336 7 _ |a article
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336 7 _ |a Output Types/Journal article
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336 7 _ |a Report
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|2 PUB:(DE-HGF)
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336 7 _ |a Journal Article
|b journal
|m journal
|0 PUB:(DE-HGF)16
|s 1521105238_26382
|2 PUB:(DE-HGF)
336 7 _ |a ARTICLE
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336 7 _ |a JOURNAL_ARTICLE
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336 7 _ |a Journal Article
|0 0
|2 EndNote
440 _ 0 |a Science
|0 PERI:(DE-600)2060783-0
|v 318
|x 0036-8075
500 _ _ |3 Converted on 2013-05-30 12:21
500 _ _ |3 Converted on 2013-06-21 19:20
520 _ _ |a 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 ~ 6x10^{19} 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.
536 _ _ |a 520 - Astroteilchenphysik (POF1-500)
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588 _ _ |a Dataset connected to CrossRef
650 _ 7 |a cosmic radiation: particle source
|2 INSPIRE
650 _ 7 |a cosmic radiation: angular dependence
|2 INSPIRE
650 _ 7 |a experimental results
|2 INSPIRE
650 _ 7 |a anisotropy
|2 INSPIRE
693 _ _ |0 EXP:(DE-MLZ)NOSPEC-20140101
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