Similar Items: Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory
- A search for point sources of EeV neutrons
- Chemical Composition of Cosmic Ray in the 5 EeV region and upgrade of the Auger Observatory
- Probing the origin of ultra-high-energy cosmic rays with neutrinos in the EeV energy range using the Pierre Auger Observatory
- Searches for Large-Scale Anisotropy in the Arrival Directions of Cosmic Rays Detected above Energy of 1019 eV at the Pierre Auger Observatory and the Telescope Array
- Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
- Search for photons above 10^18 eV with the hybrid detector of the Pierre Auger Observatory
Author: Abreu, P.
- Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
- Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory
- Reconstruction of inclined air showers detected with the Pierre Auger Observatory
- Depth of maximum of air-shower profiles at the Pierre Auger Observatory. II. Composition implications
- Search for photons above 10^18 eV with the hybrid detector of the Pierre Auger Observatory
- Techniques for Measuring Aerosols using the Central Laser Facility at the Pierre Auger Observatory
Author: Aglietta, M.
- Search for patterns by combining cosmic-ray energy and arrival directions at the Pierre Auger Observatory
- Data-driven estimation of the invisible energy of cosmic ray showers with the Pierre Auger Observatory
- Reconstruction of inclined air showers detected with the Pierre Auger Observatory
- Depth of maximum of air-shower profiles at the Pierre Auger Observatory. II. Composition implications
- Search for photons above 10^18 eV with the hybrid detector of the Pierre Auger Observatory
- Techniques for Measuring Aerosols using the Central Laser Facility at the Pierre Auger Observatory