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The Pierre Auger Observatory is designed to study cosmic rays with energies greater than 10^{19} eV.
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D. Allard et. al. for the Pierre Auger Collaboration, “Aperture calculation of the Pierre Auger Observatory surface detector”, Proceedings of the 29th International Cosmic Ray Conference, Pune, India, 7
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2007
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2007
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2005
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C. Bonifazi for the Pierre Auger Collaboration, “Angular Resolution of the Pierre Auger Observatory”, Proceedings of the 29th International Cosmic Ray Conference, Pune, India, 7
2005
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M. Aglietta et. al. for the Pierre Auger Collaboration, “Response of the Pierre Auger Observatory Water Cherenkov Detectors to Muons”, Proceedings of the 29th International Cosmic Ray Conference, Pune, India, 7
2005
Cited alongside, same era.
I. Allekotte et. al. for the Pierre Auger Collaboration, “Observation of the Long Term Stability of Water Stations in the Pierre Auger Surface Detector”, Proceedings of the 29th International Cosmic Ray Conference, Pune, India, 8
2005
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T. Suomijarvi et. al. for the Pierre Auger Collaboration, “The Electronics System of the Surface Detectors of the Pierre Auger Observatory”, in preparation
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P. Facal San Luis for the Pierre Auger Collaboration, “Measurement of the UHECR spectrum above 10 19
2007
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M. Ave et. al. for the Pierre Auger Collaboration, Nucl. Inst. & Meth. A578
2007
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C. Bonifazi, A. Letessier-Selvon and E. M. Santos, accepted in Astrop. Phys. (2007), astro-ph 0705.1856
2007
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M. Ave for the Pierre Auger Collaboration, “Reconstruction accuracy of the surface detector array of the Pierre Auger Observatory”, Proceedings of the 30th International Cosmic Ray Conference, Merida, Mexico (2007), H.E. 1.4.A - 297
2007
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