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19932022
most citedOrigin and Propagation of Extremely High Energy Cosmic Rays

648 citations · 7.8k across the 137 of their papers we have counts for

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Showing 2011 · astro-ph.HEShow all

6 papers · 2 filters

astro-ph.HE2011★ 40 cited

Search for signatures of magnetically-induced alignment in the arrival directions measured by the Pierre Auger Observatory

The Pierre Auger Collaboration, P. Abreu, M. Aglietta +496

We present the results of an analysis of data recorded at the Pierre Auger Observatory in which we search for groups of directionally-aligned events (or `multiplets') which exhibit…

astro-ph.HE2011★ 60 cited

The Pierre Auger Observatory I: The Cosmic Ray Energy Spectrum and Related Measurements

The Pierre Auger Collaboration, P. Abreu, M. Aglietta +493

Studies of the cosmic ray energy spectrum at the highest energies with the Pierre Auger Observatory

astro-ph.HE2011★ 25 cited

The Pierre Auger Observatory III: Other Astrophysical Observations

The Pierre Auger Collaboration, P. Abreu, M. Aglietta +493

Astrophysical observations of ultra-high-energy cosmic rays with the Pierre Auger Observatory

astro-ph.HE2011★ 51 cited

The Pierre Auger Observatory II: Studies of Cosmic Ray Composition and Hadronic Interaction models

The Pierre Auger Collaboration, P. Abreu, M. Aglietta +493

Studies of the composition of the highest energy cosmic rays with the Pierre Auger Observatory, including examination of hadronic physics effects on the structure of extensive air…

astro-ph.HE2011

Interdisciplinary Aspects of High-Energy Astrophysics

Guenter Sigl

Modern astrophysics, especially at GeV energy scales and above is a typical example where several disciplines meet: The location and distribution of the sources is the domain of as…

astro-ph.HE2011★ 45 cited

Lorentz Invariance Violation and Chemical Composition of Ultra High Energy Cosmic Rays

Andrey Saveliev, Luca Maccione, Guenter Sigl

Motivated by experimental indications of a significant presence of heavy nuclei in the cosmic ray flux at ultra high energies ($\gtrsim 10^{19} \eV$), we consider the effects of Pl…