Expanding the Pierre Auger Observatory Open Data program
The Pierre Auger Collaboration,
A. Abdul Halim,
P. Abreu,
M. Aglietta,
I. Allekotte,
K. Almeida Cheminant,
A. Almela, R. Aloisio, J. Alvarez-Muñiz, A. Ambrosone, J. Ammerman Yebra, G.A. Anastasi, L.A. Anchordoqui, B. Andrada, L. Andrade Dourado, S. Andringa, L. Apollonio, C. Aramo, E. Arnone, J.C. Arteaga Velazquez, P. Assis, G. Avila, E. Avocone, A. Bakalova, F. Barbato, A. Bartz Mocellin, J.A. Bellido, C. Berat, M.E. Bertaina, M. Bianciotto, P.L. Biermann, V. Binet, K. Bismark, T. Bister, J. Biteau, J. Blazek, J. Blümer, M. Bohacova, D. Boncioli, C. Bonifazi, L. Bonneau Arbeletche, N. Borodai, J. Brack, P.G. Brichetto Orchera, F.L. Briechle, A. Bueno, S. Buitink, M. Buscemi, M. Büsken, A. Bwembya, K.S. Caballero-Mora, S. Cabana-Freire, L. Caccianiga, F. Campuzano, J. Caraça-Valente, R. Caruso, A. Castellina, F. Catalani, G. Cataldi, L. Cazon, M. Cerda, B. Čermáková, A. Cermenati, J.A. Chinellato, J. Chudoba, L. Chytka, R.W. Clay, A. Cobos Cerutti, R. Colalillo, R. Conceição, G. Consolati, M. Conte, F. Convenga, D. Correia dos Santos, P.J. Costa, C. Covault, M. Cristinziani, C.S. Cruz Sanchez, S. Dasso, K. Daumiller, B.R. Dawson, R.M. de Almeida, E.T. de Boone, B. de Errico, J. de Jesús, S.J. de Jong, J. 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, N. Denner, L. Deval, A. di Matteo, C. Dobrigkeit, J.C. D'Olivo, L.M. Domingues Mendes, Q. Dorosti, J. dos Anjos, R.C. dos Anjos, J. Ebr, F.H. Ellwanger, R. Engel, I. Epicoco, M. Erdmann, A. Etchegoyen, C. Evoli, H. Falcke, G.R. Farrar, A. Fauth, T. Fehler, F. Feldbusch, A. Fernandes, M. Fernandez, B. Fick, J.M. Figueira, P. Filip, A. Filipcic, T. Fitoussi, B. Flaggs, T. Fodran, A. Franco, M. Freitas, T. Fujii, A. Fuster, C. Galea, B. Garcia, C. Gaudu, P.L. Ghia, U. Giaccari, F. Gobbi, F. Gollan, G. Golup, M. Gómez Berisso, P.F. Gómez Vitale, J.P. Gongora, J.M. Gonzalez, N.M. Gonzalez, D. Gora, A. Gorgi, M. Gottowik, F. Guarino, G. Guedes, L. Gülzow, S. Hahn, P. Hamal, M.R. Hampel, P.M. Hansen, V.M. Harvey, A. Haungs, T. Hebbeker, C. Hojvat, J. Hörandel, P. Horvath, M. Hrabovsky, T. Huege, A. Insolia, P.G. Isar, M. Ismaiel, P. Janecek, V. Jilek, K.H. Kampert, B. Keilhauer, A. Khakurdikar, V.V. Kizakke Covilakam, H. Klages, M. Kleifges, J. Köhler, F. Krieger, M. Kubatova, N. Kunka, B.L. Lago, N. Langner, N. Leal, M.A. Leigui de Oliveira, Y. Lema-Capeans, A. Letessier-Selvon, I. Lhenry-Yvon, L. Lopes, J.P. Lundquist, M. Mallamaci, D. Mandat, P. Mantsch, F.M. Mariani, A. Mariazzi, I.C. Maris, G. Marsella, D. Martello, S. Martinelli, M.A. Martins, H.J. Mathes, J. Matthews, G. Matthiae, E.W. Mayotte, S. Mayotte, P. Mazur, G. Medina-Tanco, J. Meinert, D. Melo, A. Menshikov, C. Merx, S. Michal, M.I. Micheletti, L. Miramonti, M. Mogarkar, S. Mollerach, F. Montanet, L. Morejon, K. Mulrey, R. Mussa, W.M. Namasaka, S. Negi, L. Nellen, K. Nguyen, G. Nicora, M. Niechciol, D. Nitz, D. Nosek, A. Novikov, V. Novotný, L. Nozka, A. Nucita, L.A. Nunez, J. Ochoa, C. Oliveira, L. Östman, M. Palatka, J. Pallotta, S. Panja, G. Parente, T. Paulsen, J. Pawlowsky, M. Pech, J. Pękala, R. Pelayo, V. Pelgrims, L.A. Pereira, E.E. Pereira Martins, C. Pérez Bertolli, L. Perrone, S. Petrera, C. Petrucci, T. Pierog, M. Pimenta, M. Platino, B. Pont, M. Pourmohammad Shahvar, P. Privitera, C. Priyadarshi, M. Prouza, K. Pytel, S. Querchfeld, J. Rautenberg, D. Ravignani, J.V. Reginatto Akim, A. Reuzki, J. Ridky, F. Riehn, M. Risse, V. Rizi, E. Rodriguez, G. Rodriguez Fernandez, J.R. Rodriguez Rojo, S. Rossoni, M. Roth, E. Roulet, A. Rovero, A. Saftoiu, M. Saharan, F. Salamida, H.I. Salazar, G. Salina, P. Sampathkumar, N. San Martin, J. Sanabria Gomez, F.A. Sánchez, E.M. Santos, E. Santos, F. Sarazin, R. Sarmento, R. Sato, P. Savina, V. Scherini*, H. Schieler, M. Schimassek, M. Schimp, D. Schmidt, O. Scholten, H. Schoorlemmer, P. Schovanek, F.G. Schröder, J. Schulte, T. Schulz, S.J. Sciutto, M. Scornavacche, A. Sedoski, A. Segreto, S. Sehgal, S.U. Shivashankara, G. Sigl, K. Simkova, F. Simon, R. Smida, P. Sommers, R. Squartini, M. Stadelmaier, S. Stanič, J. Stasielak, P. Stassi, S. Strähnz, M. Straub, T. Suomijarvi, A.D. Supanitsky, Z. Svozilikova, K. Syrokvas, Z. Szadkowski, F. Tairli, M. Tambone, A. Tapia, C. Taricco, C. Timmermans, O. Tkachenko, P. Tobiska, C.J. Todero Peixoto, B. Tomé, A. Travaini, P. Travnicek, M.J. Tueros, M. Unger, R. Uzeiroska, L. Vaclavek, M. Vacula, I. Vaiman, J.F. Valdés Galicia, L. Valore, P. van Dillen, E. Varela, V. Vašíčková, A. Vásquez-Ramírez, D. Veberic, I.D. Vergara Quispe, S. Verpoest, V. Verzi, J. Vicha, J. Vink, S. Vorobiov, J.B. Vuta, C.K.O. Watanabe, A. Watson, A. Weindl, M. Weitz, L. Wiencke, H. Wilczyński, B. Wundheiler, B. Yue, A. Yushkov, E. Zas, D. Zavrtanik and M. Zavrtaniket al. (click to show)*: corresponding author
Pre-published on:
September 23, 2025
Published on:
December 30, 2025
Abstract
Since 2021, the Open Data Portal has provided access to the Pierre Auger Observatory’s data for both the scientific community and the general public. The data release process has been in place since the Observatory’s foundation. It continues to be strengthened as outlined in the approved policy and the Observatory’s Data Management Plan. More than 80 000 cosmic-ray events above $10^{17}$ eV, detected with the surface and fluorescence detectors, have been released at various levels, from calibrated traces to high-level reconstruction parameters. Additionally, atmospheric data and low-energy particle counting rates have been made available for space weather studies.
The Collaboration is committed to releasing FAIR (Findable, Accessible, Interoperable, and Reusable) data, along with accompanying software and detailed documentation, enabling users
to perform their own queries and analyses for both research and educational purposes. These datasets have already served as a basis for several scientific papers and have been widely used in
various outreach activities.
After 20 years of stable data acquisition, the Pierre Auger Collaboration will disclose 30% of the cosmic ray events above 2.5 · $10^{18}$ eV collected with the main surface detector array between
2004 and 2022, corresponding to an exposure of about 24 000 km$^2$ sr yr, together with events detected with the fluorescence detector and used for energy calibration. This release will provide an unprecedented public dataset for ultra-high-energy cosmic rays, enabling in-depth studies of their properties.
Together with the published catalog of the 100 most energetic events recorded, this initiative represents the Pierre Auger Collaboration’s strong commitment to distributed and collective knowledge,
sharing progress with the entire scientific community.
DOI: https://doi.org/10.22323/1.501.1251
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