[引用][C] Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory

P Abreu, M Aglietta, JM Albury, I Allekotte, A Cheminant… - 2022 - repository.udem.edu.co

[引用][C] Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory

P Abreu, IC Maris, O Zapparrata… - The Astrophysical …, 2022 - difusion.ulb.ac.be

Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory

P Abreu, M Aglietta, JM Albury… - The Astrophysical …, 2022 - ui.adsabs.harvard.edu
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 …

Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory

P Abreu, M Aglietta, JM Albury, I Allekotte… - THE ASTROPHYSICAL …, 2022 - air.unimi.it
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 …

Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory

P Abreu, M Aglietta, J Albury, I Allekotte… - THE …, 2022 - airus.unisalento.it
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 …

Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory

P Abreu, M Aglietta, JM Albury, I Allekotte… - Astrophys. J., 2022 - hal.science
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 …

Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory

P Abreu, M Aglietta, JM Albury, I Allekotte… - THE ASTROPHYSICAL …, 2022 - iris.unina.it
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 …

Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory

P Abreu, M Aglietta, JM Albury… - The …, 2022 - publikationen.bibliothek.kit.edu
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 …

Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory

P Abreu, M Aglietta, JM Albury, I Allekotte… - Astrophys. J., 2022 - inria.hal.science
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 …

Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger Observatory

P Abreu, J Ammerman Yebra, J Álvarez Muñiz… - minerva.usc.es
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 …