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International Symposium on Astronomy and Astrophysics of the Extreme Universe, Tokyo : Japon (2007)
The Pierre Auger Observatory: status, results and perspective
E. Parizot1
PIERRE AUGER Collaboration(s)
(2007)

While the completion of the Pierre Auger Observatory (or simply "Auger'') is still underway, the 5165 km^2.sr.yr integrated acceptance accumulated since the January 1st, 2004 is now significantly larger than what was gathered by the previous experiments dedicated to the detection of ultra-high-energy cosmic rays (UHECRs). We report on the development status of Auger and present some results related to the cosmic-ray energy spectrum, composition and anisotropies, and the photon fraction at ultra-high energy. We briefly discuss the importance of the ankle region to understand the overall phenomenology of cosmic-rays, and mention future enhancements of Auger focusing on this energy range.
1 :  APC - UMR 7164 - AstroParticule et Cosmologie
APC - AHE
Physique/Astrophysique/Cosmologie et astrophysique extra-galactique

Planète et Univers/Astrophysique/Cosmologie et astrophysique extra-galactique

Planète et Univers/Astrophysique
Astrophysics
Lien vers le texte intégral : 
http://fr.arXiv.org/abs/0709.2500