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Luis A. Anchordoqui

Researcher at City University of New York

Publications -  169
Citations -  11271

Luis A. Anchordoqui is an academic researcher from City University of New York. The author has contributed to research in topics: Cosmic ray & Pierre Auger Observatory. The author has an hindex of 52, co-authored 169 publications receiving 10322 citations. Previous affiliations of Luis A. Anchordoqui include University of Wisconsin–Milwaukee & University of Grenoble.

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The Pierre Auger Collaboration

Martin Will, +494 more
TL;DR: In this article, the Pierre Auger Collaboration has reported evidence for anisotropies in the arrival directions of cosmic rays with energies larger thanEth = 55 EeV and showed that there is a correlation above the isotropic expectation with nearby active galaxies and the largest excess is in a celestial region around the position of the radio galaxy Cen A.
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Properties and performance of the prototype instrument for the Pierre Auger Observatory

J. Abraham, +356 more
TL;DR: The first phase of the Pierre Auger Observatory has been completed and all of the sub-systems that will be used in the full instrument to be tested under field conditions as discussed by the authors.
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The Pierre Auger Cosmic Ray Observatory

A. Aab, +643 more
TL;DR: The Pierre Auger Observatory as mentioned in this paper, the world's largest cosmic ray observatory, has been in successful operation since completion in 2008 and has recorded data from an exposure exceeding 40,000 km$^2$ sr yr.
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Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nuclei

J. Abraham, +483 more
TL;DR: In this paper, the Pierre Auger Observatory data was used to confirm the anisotropy of the arrival direction of the highest-energy cosmic rays with the highest energy, which are correlated with the positions of relatively nearby active galactic nuclei (AGN) at a confidence level of more than 99%.
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Update on the correlation of the highest energy cosmic rays with nearby extragalactic matter

P. Abreu, +495 more
TL;DR: In this paper, anisotropy was measured by the fraction of arrival directions that are less than 3.1 degrees from the position of an active galactic nucleus within 75 Mpc (using the Veron-Cetty and Veron 12th catalog).