TY - JOUR
T1 - Highlights from the Pierre Auger Observatory
AU - Pierre Auger Collaboration
AU - Salamida, Francesco
AU - Abdul Halim, A.
AU - Abreu, P.
AU - Aglietta, M.
AU - Allekotte, I.
AU - Almeida Cheminant, K.
AU - Almela, A.
AU - Aloisio, R.
AU - Alvarez-Muñiz, J.
AU - Ammerman Yebra, J.
AU - Anastasi, G. A.
AU - Anchordoqui, L.
AU - Andrada, B.
AU - Andringa, S.
AU - Aramo, C.
AU - Araújo Ferreira, P. R.
AU - Arnone, E.
AU - Arteaga Velázquez, J. C.
AU - Asorey, H.
AU - Assis, P.
AU - Avila, G.
AU - Avocone, E.
AU - Badescu, A. M.
AU - Bakalova, A.
AU - Balaceanu, A.
AU - Barbato, F.
AU - Bartz Mocellin, A.
AU - Bellido, J. A.
AU - Berat, C.
AU - Bertaina, M. E.
AU - Bhatta, G.
AU - Bianciotto, M.
AU - Biermannh, P. L.
AU - Binet, V.
AU - Bismark, K.
AU - Bister, T.
AU - Biteau, J.
AU - Blazek, J.
AU - Bleve, C.
AU - Blümer, J.
AU - Bohácová, M.
AU - Boncioli, D.
AU - Bonifazi, C.
AU - Bonneau Arbeletche, L.
AU - Borodai, N.
AU - Brack, J.
AU - Brichetto Orchera, P. G.
AU - Briechle, F. L.
AU - Bueno, A.
AU - Ventura, C.
N1 - Publisher Copyright:
© Copyright owned by the author(s) under the terms of the Creative Commons.
PY - 2024/9/27
Y1 - 2024/9/27
N2 - The Pierre Auger Observatory is a unique facility designed to study ultra-high energy cosmic rays, with energies up to 1020 eV and beyond. The Observatory is located in Argentina and comprises more than 1600 water Cherenkov detectors spread over an area of 3000 square kilometers overlooked by Fluorescence detectors. The first phase of the Observatory's data-taking began in 2004 and continued until the end of 2021. In this contribution, the results from the Phase I data analysis of the Pierre Auger Observatory are presented. They include, among others, measurements of the cosmic-ray energy spectrum, composition, and arrival direction anisotropy. The Phase I results from the Pierre Auger Observatory provide major advances in the understanding of the ultra-high energy cosmic ray phenomena and lay the foundation for second-phase studies with the upgraded AugerPrime detector. The status of the AugerPrime upgrade and its performance will be also discussed.
AB - The Pierre Auger Observatory is a unique facility designed to study ultra-high energy cosmic rays, with energies up to 1020 eV and beyond. The Observatory is located in Argentina and comprises more than 1600 water Cherenkov detectors spread over an area of 3000 square kilometers overlooked by Fluorescence detectors. The first phase of the Observatory's data-taking began in 2004 and continued until the end of 2021. In this contribution, the results from the Phase I data analysis of the Pierre Auger Observatory are presented. They include, among others, measurements of the cosmic-ray energy spectrum, composition, and arrival direction anisotropy. The Phase I results from the Pierre Auger Observatory provide major advances in the understanding of the ultra-high energy cosmic ray phenomena and lay the foundation for second-phase studies with the upgraded AugerPrime detector. The status of the AugerPrime upgrade and its performance will be also discussed.
UR - http://www.scopus.com/inward/record.url?scp=85183358310&partnerID=8YFLogxK
M3 - Conference article
AN - SCOPUS:85183358310
SN - 1824-8039
VL - 444
JO - Proceedings of Science
JF - Proceedings of Science
M1 - 016
T2 - 38th International Cosmic Ray Conference, ICRC 2023
Y2 - 26 July 2023 through 3 August 2023
ER -