Measurement of the cosmic-ray energy spectrum above 2.5×1018 eV using the Pierre Auger Observatory

Keyphrases

• Anisotropy 50%
• Ankle 100%
• Cosmic Ray Energy Spectrum 100%
• Cosmic Rays 50%
• Declination 50%
• Energy Spectrum 50%
• Hadronic Physics 50%
• Particle Flux 50%
• Pierre Auger Observatory 100%
• Primary Mass Composition 50%
• Southern Hemisphere 50%
• Spectral Indices 50%
• Systematic Uncertainty 50%
• Zenith Angle 50%

Physics

• Anisotropy 50%
• Energy Spectra 100%
• Flattening 50%
• Flux (Rate) 50%
• Hadronic Physics 50%
• Observatory 100%
• Spectral Index 50%