902 citations · 5.9k across the 124 of their papers we have counts for
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On the possibility of primary identification of individual cosmic ray showers
A. D. Supanitsky, G. Medina-Tanco, A. Etchegoyen
The transition between the Galactic and extragalactic cosmic ray components could take place either in the region of the spectrum known as the second knee or in the ankle. There ar…
A New Numerical Technique to Determine Primary Cosmic Ray Composition in the Ankle Region
A. D. Supanitsky, G. Medina-Tanco, A. Etchegoyen
In this paper we introduce a new multiparametric technique that attempts to tackle simultaneously the problems of composition determination and hadronic interaction uncertainty. Em…
Sites for Gamma-ray Astronomy in Argentina
A. C. Rovero, G. E. Romero, I. Allekotte +9
We have searched for possible sites in Argentina for the installation of large air Cherenkov telescope arrays and water Cherenkov systems. At present seven candidates are identifie…
Underground Muon Counters as a Tool for Composition Analyses
A. D. Supanitsky, A. Etchegoyen, G. Medina-Tanco +3
The transition energy from galactic to extragalactic cosmic ray sources is still uncertain, but it should be associated either with the region of the spectrum known as the second k…
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…
Enhancing the Pierre Auger Observatory to the 10^{17} to 10^{18.5} eV Range: Capabilities of an Infill Surface Array
M. C. Medina, M. Gomez Berisso, I. Allekotte +3
The Pierre Auger Observatory has been designed to study the highest-energy cosmic rays in nature (E > 10^{18.5} eV). The determination of their arrival direction, energy and compos…