activity
20002026
most citedObservation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above eV

409 citations · 7.6k across the 148 of their papers we have counts for

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8 papers · 1 filter

astro-ph2008★ 38 cited

Scaler Mode Technique for the ARGO-YBJ Detector

G. Aielli et al.

The ARGO-YBJ experiment has been designed to study the Extensive Air Showers with an energy threshold lower than that of the existing arrays by exploiting the high altitude locatio…

astro-ph2007★ 374 cited

Correlation of the highest-energy cosmic rays with the positions of nearby active galactic nuclei

The Pierre Auger Collaboration

Data collected by the Pierre Auger Observatory provide evidence for anisotropy in the arrival directions of the cosmic rays with the highest energies, which are correlated with the…

astro-ph2007★ 11 cited

Measurement of the UHECR energy spectrum from hybrid data of the Pierre Auger Observatory

Lorenzo Perrone

More than two years of fluorescence detector data collected in coincidence with at least one station of the surface detector array (``hybrid data'') are used to measure the flux an…

astro-ph2005★ 1 cited

Validation of the Real and Simulated Data of the Pierre Auger Fluorescence Telescopes

The Pierre Auger Collaboration, L. Perrone

The fluorescence detector (FD) of the Pierre Auger Observatory is currently operating 18 fluorescence telescopes of the 24 that will be employed in the completed detector. These te…

astro-ph2005★ 2 cited

Fluorescence and Hybrid Detection Aperture of the Pierre Auger Observatory

J. A. Bellido, D. D'Urso, H. Geenen +5

The aperture of the Fluorescence Detector (FD) of the Pierre Auger Observatory is evaluated from simulated events using different detector configurations: mono, stereo, 3-FD and 4-…

astro-ph2004★ 3 cited

Ultra High Energy nu_tau detection at Pierre Auger Observatory

G. Miele, L. Perrone, O. Pisanti

Earth--skimming UHE tau neutrinos have a chance to be detected by the Fluorescence Detector (FD) of Pierre Auger Observatory if their astrophysical flux is large enough. A detailed…