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A Catalog of the Highest-Energy Cosmic Rays Recorded During Phase I of Operation of the Pierre Auger Observatory

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arxiv 2211.16020 v1 pith:DDIICX7H submitted 2022-11-29 astro-ph.HE astro-ph.IM

The Pierre Auger Collaboration: A. Abdul Halim , P. Abreu , M. Aglietta , I. Allekotte , P. Allison , K. Almeida Cheminant , A. Almela , J. Alvarez-Muñiz
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J. Ammerman Yebra G.A. Anastasi L. Anchordoqui B. Andrada S. Andringa C. Aramo P.R. Araújo Ferreira E. Arnone J. C. Arteaga Velázquez H. Asorey P. Assis M. Ave G. Avila E. Avocone A.M. Badescu A. Bakalova A. Balaceanu F. Barbato J. Beatty J.A. Bellido C. Berat M.E. Bertaina X. Bertou G. Bhatta P.L. Biermann P. Billoir V. Binet K. Bismark T. Bister J. Biteau J. Blazek C. Bleve J. Blümer M. Boháčová D. Boncioli C. Bonifazi L. Bonneau Arbeletche N. Borodai J. Brack T. Bretz P.G. Brichetto Orchera F.L. Briechle P. Buchholz A. Bueno S. Buitink M. Buscemi M. Büsken A. Bwembya K.S. Caballero-Mora L. Caccianiga I. Caracas R. Caruso A. Castellina F. Catalani G. Cataldi L. Cazon M. Cerda R. Cester J.A. Chinellato J. Chirinos J. Chudoba L. Chytka R.W. Clay A.C. Cobos Cerutti R. Colalillo A. Coleman M.R. Coluccia R. Conceição A. Condorelli G. Consolati F. Contreras F. Convenga D. Correia dos Santos C.E. Covault M. Cristinziani C.S. Cruz Sanchez S. Dasso K. Daumiller B.R. Dawson R.M. de Almeida J. de Jesús S.J. de Jong J.R.T. de Mello Neto I. De Mitri J. de Oliveira D. de Oliveira Franco F. de Palma V. de Souza E. De Vito A. Del Popolo O. Deligny L. Deval A. di Matteo M. Dobre C. Dobrigkeit J.C. D'Olivo L.M. Domingues Mendes A. Dorofeev R.C. dos Anjos J. Ebr M. Eman R. Engel I. Epicoco M. Erdmann A. Etchegoyen H. Falcke J. Farmer G. Farrar A.C. Fauth N. Fazzini F. Feldbusch F. Fenu B. Fick J.M. Figueira A. Filipčič T. Fitoussi B. Flaggs T. Fodran T. Fujii A. Fuster C. Galea C. Galelli B. García H. Gemmeke F. Gesualdi A. Gherghel-Lascu P.L. Ghia U. Giaccari M. Giammarchi J. Glombitza F. Gobbi F. Gollan G. Golup M. Gómez Berisso P.F. Gómez Vitale J.P. Gongora J.M. González N. González I. Goos D. Góra A. Gorgi M. Gottowik T.D. Grubb F. Guarino G.P. Guedes E. Guido S. Hahn P. Hamal M.R. Hampel P. Hansen D. Harari J. Harton V.M. Harvey A. Haungs T. Hebbeker D. Heck C. Hojvat J.R. Hörandel P. Horvath M. Hrabovský T. Huege A. Insolia P.G. Isar P. Janecek J.A. Johnsen J. Jurysek A. Kääpä K.H. Kampert B. Keilhauer A. Khakurdikar V.V. Kizakke Covilakam H.O. Klages M. Kleifges J. Kleinfeller F. Knapp J. Knapp N. Kunka C. Lachaud B.L. Lago N. Langner M.A. Leigui de Oliveira V. Lenok A. Letessier-Selvon I. Lhenry-Yvon D. Lo Presti L. Lopes R. López L. Lu Q. Luce J.P. Lundquist A. Machado Payeras D. Mandat B.C. Manning J. Manshanden P. Mantsch S. Marafico F.M. Mariani A.G. Mariazzi I.C. Mariş G. Marsella D. Martello S. Martinelli O. Martínez Bravo M.A. Martins M. Mastrodicasa H.J. Mathes J. Matthews G. Matthiae E. Mayotte S. Mayotte P.O. Mazur G. Medina-Tanco J. Meinert D. Melo A. Menshikov S. Michal M.I. Micheletti L. Miramonti S. Mollerach F. Montanet L. Morejon C. Morello A.L. Müller K. Mulrey R. Mussa M. Muzio W.M. Namasaka A. Nasr-Esfahani L. Nellen G. Nicora M. Niculescu-Oglinzanu M. Niechciol D. Nitz I. Norwood D. Nosek V. Novotny L. Nožka A Nucita L.A. Núñez C. Oliveira M. Palatka J. Pallotta G. Parente A. Parra J. Pawlowsky M. Pech J. Pękala R. Pelayo E.E. Pereira Martins J. Perez Armand C. Pérez Bertolli L. Perrone S. Petrera C. Petrucci T. Pierog M. Pimenta M. Platino B. Pont M. Pothast M. Pourmohammad Shavar P. Privitera M. Prouza A. Puyleart S. Querchfeld J. Rautenberg D. Ravignani M. Reininghaus J. Ridky F. Riehn M. Risse V. Rizi W. Rodrigues de Carvalho J. Rodriguez Rojo M.J. Roncoroni S. Rossoni M. Roth E. Roulet A.C. Rovero P. Ruehl A. Saftoiu M. Saharan F. Salamida H. Salazar G. Salina J.D. Sanabria Gomez F. Sánchez E.M. Santos E. Santos F. Sarazin R. Sarmento R. Sato P. Savina C.M. Schäfer V. Scherini H. Schieler M. Schimassek M. Schimp F. Schlüter D. Schmidt O. Scholten H. Schoorlemmer P. Schovánek F.G. Schröder J. Schulte T. Schulz S.J. Sciutto M. Scornavacche A. Segreto S. Sehgal S.U. Shivashankara G. Sigl G. Silli O. Sima R. Smau R. Šmída P. Sommers J.F. Soriano R. Squartini M. Stadelmaier D. Stanca S. Stanič J. Stasielak P. Stassi M. Straub A. Streich M. Suárez-Durán T. Suomijärvi A.D. Supanitsky Z. Szadkowski A. Tapia C. Taricco C. Timmermans O. Tkachenko P. Tobiska C.J. Todero Peixoto B. Tomé Z. Torrès A. Travaini P. Travnicek C. Trimarelli M. Tueros R. Ulrich M. Unger L. Vaclavek M. Vacula J.F. Valdés Galicia L. Valore E. Varela A. Vásquez-Ramírez D. Veberič C. Ventura I.D. Vergara Quispe V. Verzi J. Vicha L.M. Villaseñor Cendejas J. Vink S. Vorobiov C. Watanabe A.A. Watson A. Weindl L. Wiencke H. Wilczyński D. Wittkowski B. Wundheiler P. Younk A. Yushkov O. Zapparrata E. Zas D. Zavrtanik M. Zavrtanik
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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 1 January 2004 and 31 December 2020 are given for cosmic rays that have energies in the range 78 EeV to 166 EeV. Details are also given of 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.

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Cited by 2 Pith papers

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  1. The Large Magellanic Cloud as a source of the highest energy cosmic rays

    astro-ph.HE 2025-07 conditional novelty 5.0 of 10

    The five most energetic Auger cosmic rays cluster in a small sky region, and the Large Magellanic Cloud is a closer angular match than Centaurus A to that cluster.

  2. Consequences of a Heavy-Metal Scenario of Ultra-High-Energy Cosmic Rays

    astro-ph.HE 2025-02 conditional novelty 5.0 of 10

    Assuming pure iron cosmic rays above 40 EeV, the paper derives constant Xmax scale shifts for QGSJet II-04 and Sibyll 2.3d, yielding a consistent mass-composition model for Auger data.

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