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  • A Catalog of the Highest-en...
    Abdul Halim, A.; Allekotte, I.; Almeida Cheminant, K.; Almela, A.; Andrada, B.; Asorey, H.; Avila, G.; Bakalova, A.; Berat, C.; Biermann, P. L.; Bismark, K.; Bleve, C.; Boháčová, M.; Bwembya, A.; Clay, R. W.; Cobos Cerutti, A. C.; Coleman, A.; Coluccia, M. R.; Conceição, R.; Covault, C. E.; Dasso, S.; de Oliveira Franco, D.; de Palma, F.; di Matteo, A.; Dobrigkeit, C.; dos Anjos, R. C.; Eman, M.; Farrar, G.; Feldbusch, F.; Flaggs, B.; Fodran, T.; García, B.; Gemmeke, H.; Glombitza, J.; Gobbi, F.; Golup, G.; Gómez Berisso, M.; Gongora, J. P.; González, J. M.; Góra, D.; Gottowik, M.; Guarino, F.; Hamal, P.; Hebbeker, T.; Isar, P. G.; Janecek, P.; Jurysek, J.; Kizakke Covilakam, V. V.; Kleifges, M.; Lachaud, C.; Lago, B. L.; Leigui de Oliveira, M. A.; Lo Presti, D.; López, R.; Machado Payeras, A.; Mariazzi, A. G.; Mariş, I. C.; Matthews, J.; Meinert, J.; Michal, S.; Mollerach, S.; Montanet, F.; Morello, C.; Muzio, M.; Namasaka, W. M.; Nasr-Esfahani, A.; Nellen, L.; Nicora, G.; Niechciol, M.; Nucita, A; Parra, A.; Pȩkala, J.; Pereira Martins, E. E.; Perez Armand, J.; Pérez Bertolli, C.; Pimenta, M.; Prouza, M.; Rizi, V.; Rodrigues de Carvalho, W.; Rodriguez Rojo, J.; Saftoiu, A.; Saharan, M.; Salamida, F.; Sanabria Gomez, J. D.; Schäfer, C. M.; Schieler, H.; Schmidt, D.; Scornavacche, M.; Silli, G.; Sommers, P.; Stadelmaier, M.; Straub, M.; Suomijärvi, T.; Taricco, C.; Tkachenko, O.; Tobiska, P.; Torrès, Z.; Valore, L.; Wiencke, L.; Wittkowski, D.

    The Astrophysical journal. Supplement series, 02/2023, Letnik: 264, Številka: 2
    Journal Article

    Abstract A catalog containing details of the highest-energy cosmic rays recorded through the detection of extensive air showers at the Pierre Auger Observatory is presented with the aim of opening the data to detailed examination. Descriptions of the 100 showers created by the highest-energy particles recorded between 2004 January 1 and 2020 December 31 are given for cosmic rays that have energies in the range 78–166 EeV. Details are also given on a further nine very energetic events that have been used in the calibration procedure adopted to determine the energy of each primary. A sky plot of the arrival directions of the most energetic particles is shown. No interpretations of the data are offered.