C. Bonifazi

Publication List Details

Period

2006 - 2009

Number

12

Co-Authors

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...

Astrophysical Sources of Cosmic Rays and Related Measurements with the Pierre Auger Observatory (2009)

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....

The angular resolution of the Pierre Auger Observatory (2009)

Bonifazi, C.

We discuss the angular resolution obtained for events registered with the surface detector alone and for hybrid events, i.e., those observed simultaneously by both the surface and fluorescence...

The Surface Detector System of the Pierre Auger Observatory (2007)

Allekotte, I., Barbosa, A. F., Bauleo, P., Bonifazi, C., Civit, B., Escobar, C. O., ...

The Pierre Auger Observatory is designed to study cosmic rays with energies greater than 10^{19} eV. Two sites are envisaged for the observatory, one in each hemisphere, for complete sky coverage....

A model for the time uncertainty measurements in the Auger surface detector array (2007)

Bonifazi, C., Letessier-Selvon, A., Santos, E. M.

The precise determination of the arrival direction of cosmic rays is a fundamental prerequisite for the search for sources or the study of their anisotropies on the sky. One of the most important...

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...