The Fluorescence Detector of the Pierre Auger Observatory (2009)
Abreu, P., Aglietta, M., Aguirre, C., Ahn, E. J., Allard, D., ...
The Pierre Auger Observatory is a hybrid detector for ultra-high energy cosmic rays. It combines a surface array to measure secondary particles at ground level together with a fluorescence detector...
Abreu, P., Aglietta, M., Aguirre, C., Ahn, E. J., Allard, D., ...
Studies of the correlations of ultra-high energy cosmic ray directions with extra-Galactic objects, of general anisotropy, of photons and neutrinos, and of other astrophysical effects, with the...
Operations of and Future Plans for the Pierre Auger Observatory (2009)
Abreu, P., Aglietta, M., Aguirre, C., Ahn, E. J., Allard, D., ...
Technical reports on operations and features of the Pierre Auger Observatory, including ongoing and planned enhancements and the status of the future northern hemisphere portion of the Observatory....
Calibration and Monitoring of the Pierre Auger Observatory (2009)
Abreu, P., Aglietta, M., Aguirre, C., Ahn, E. J., Allard, D., ...
Reports on the atmospheric monitoring, calibration, and other operating systems of the Pierre Auger Observatory. Contributions to the 31st International Cosmic Ray Conference, Lodz, Poland, July 2009.
The Cosmic Ray Energy Spectrum and Related Measurements with the Pierre Auger Observatory (2009)
Abreu, P., Aglietta, M., Aguirre, C., Ahn, E. J., Allard, D., ...
Studies of the cosmic ray energy spectrum at the highest energies with the Pierre Auger Observatory.
Studies of Cosmic Ray Composition and Air Shower Structure with the Pierre Auger Observatory (2009)
Abreu, P., Aglietta, M., Aguirre, C., Ahn, E. J., Allard, D., ...
Studies of the composition of the highest energy cosmic rays with the Pierre Auger Observatory, including examination of hadronic physics effects on the structure of extensive air showers....
First buried muon counter prototype for the Auger Observatory (2009)
Sidelnik, I. P., Wundheiler, B., Colombo, E., Etchegoyen, A., Ferrero, A., Platino, M., ...
AMIGA (Auger Muons and Infill for the Ground Array) constitutes an enhancement for the Pierre Auger Observatory. It consists of a denser array of surface detectors and muon counters whose objective...
On the possibility of primary identification of individual cosmic ray showers (2008)
Supanitsky, A. D., Medina-Tanco, G., Etchegoyen, A.
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 are several models of...
A New Numerical Technique to Determine Primary Cosmic Ray Composition in the Ankle Region (2008)
Supanitsky, A. D., Medina-Tanco, G., Etchegoyen, A.
In this paper we introduce a new multiparametric technique that attempts to tackle simultaneously the problems of composition determination and hadronic interaction uncertainty. Employing simulations...
30th International Cosmic Ray Conference AMIGA, Auger Muons and Infill for the Ground (2008)
gentina
RevMexAA (Serie de Conferencias), 14, 98--98 (2002) (2008)
Estado Del Observatorio, A. Etchegoyen, El Proyecto, Pierre Auger
ndoza, Argentina, y se extiende a lo largo de la regi'on denominada "Pampa Amarilla", nombre que ha sido asignado al Observatorio. Ya se ha completado la primera etapa del Proyecto,...
RevMexAA (Serie de Conferencias), 14, 98--98 (2002) (2007)
Estado Del Observatorio, Estado Del, Observatorio Pierre Auger, El Proyecto, Pierre Auger, A. Etchegoyen
inada "Pampa Amarilla", nombre que ha sido asignado al Observatorio. Ya se ha completado la primera etapa del Proyecto, llamada Prototipo de Ingeniera, consistente en la instalaci on de 40...
Calibration of the surface array of the Pierre Auger Observatory (2006)
Bertou, X., Allison, P.S., Bonifazi, C., Bauleo, P., Grunfeld, C.M., Aglietta, M., ...
The Pierre Auger Observatory is designed to study cosmic rays of the highest energies (>$10^{19}$eV). The ground array of the Observatory will consist of 1600 water Cherenkov detectors deployed over...
Calibration of the surface array of the Pierre Auger Observatory (2006)
Bertou, X., Allison, P.S., Bonifazi, C., Bauleo, P., Grunfeld, C.M., Aglietta, M., ...
The Pierre Auger Observatory is designed to study cosmic rays of the highest energies (>$10^{19}$eV). The ground array of the Observatory will consist of 1600 water Cherenkov detectors deployed over...
Calibration of the surface array of the Pierre Auger Observatory (2006)
Bertou, X., Allison, P.S., Bonifazi, C., Bauleo, P., Grunfeld, C.M., Aglietta, M., ...
The Pierre Auger Observatory is designed to study cosmic rays of the highest energies (>$10^{19}$eV). The ground array of the Observatory will consist of 1600 water Cherenkov detectors deployed over...