Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory
A promising energy range to look for angular correlations between cosmic rays of extragalactic origin and their sources is at the highest energies, above a few tens of EeV (1 EeV ≡ 1018 eV). Despite the flux of these particles being extremely low, the area of ∼3000 km2 covered at the Pierre Auger Ob...
Guardado en:
| Autores principales: | Micheletti, M. I., Binet, V., The Pierre Auger collaboration |
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| Formato: | article artículo publishedVersion |
| Lenguaje: | Inglés |
| Publicado: |
Institute of Physics
2023
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| Materias: | |
| Acceso en línea: | http://hdl.handle.net/2133/25269 http://hdl.handle.net/2133/25269 |
| Aporte de: |
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