[HTML][HTML] Arrival directions of cosmic rays above 32 EeV from phase one of the Pierre Auger Observatory

KA Cheminant, RA Batista, JA Yebra… - The Astrophysical …, 2022 - iopscience.iop.org
Cosmic rays are observed up to the astounding energies of more than 1020 eV, making
them the most energetic particles known in the universe. However, the origin of these …

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

P Abreu, M Aglietta, JM Albury, I Allekotte… - 2022 - datosdeinvestigacion.conicet.gov.ar
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 - osti.gov
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 …

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

S Buitink, O Scholten, T Huege - researchportal.vub.be
ABSTRACT A promising energy range to look for angular correlation between cosmic rays of
extragalactic origin and their sources is at the highest energies, above few tens of EeV (1 …

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

P Abreu, M Aglietta, JM Albury, R Alves Batista… - 2022 - repository.ubn.ru.nl
Cosmic rays are observed up to the astounding energies of more than 1020 eV, making
them the most energetic particles known in the universe. However, the origin of these …

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

P Abreu, M Aglietta, JM Albury, I Allekotte… - 2022 - ri.conicet.gov.ar
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… - 2022 - notablesdelaciencia.conicet.gov.ar
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 …

[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, PL Biermann - \apj, 2022 - pure.mpg.de
Arrival Directions of Cosmic Rays above 32 EeV from Phase One of the Pierre Auger
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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 …, 2022 - re.public.polimi.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 - inspirehep.net
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 …