activity
19932025
most citedObservation of a Large-scale Anisotropy in the Arrival Directions of Cosmic Rays above eV

409 citations · 7.4k across the 127 of their papers we have counts for

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22 papers · 1 filter

astro-ph2008★ 12 cited

Kolmogorov-Smirnov test as a tool to study the distribution of ultra-high energy cosmic ray sources

Diego Harari, Silvia Mollerach, Esteban Roulet

We analyze in detail the two-dimensional Kolmogorov-Smirnov test as a tool to learn about the distribution of the sources of the ultra-high energy cosmic rays. We confront in parti…

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

Search for correlation of UHECRs and BL Lacs in Pierre Auger Observatory data

Diego Harari

Several analyses of the data collected by other experiments have found an excess of cosmic rays in correlation with subclasses of BL Lacs. Data from the Pierre Auger Observatory do…

astro-ph2006★ 63 cited

On the ultra-high energy cosmic ray horizon

D. Harari, S. Mollerach, E. Roulet

We compute the ultra-high energy cosmic ray horizon, i.e. the distance up to which cosmic ray sources may significantly contribute to the fluxes above a certain threshold on the ob…

astro-ph2006★ 8 cited

Detecting filaments in the ultra-high energy cosmic ray distribution

Diego Harari, Silvia Mollerach, Esteban Roulet

We propose and test new statistical tools to study the distribution of cosmic rays based on the use of the Minimal Spanning Tree. The method described is particularly sensitive to…

astro-ph2004★ 80 cited

B polarization of the CMB from Faraday rotation

Claudia Scoccola, Diego Harari, Silvia Mollerach

We study the effect of Faraday rotation due to a homogeneous magnetic field on the polarization of the cosmic microwave background (CMB). Scalar fluctuations give rise only to pari…