The Pierre Auger Observatory open data
Adila Abdul HalimUniversity of AdelaideP. AbreuUniversidade de Lisboa–ULM. AgliettaINFN, Sezione di TorinoI. AllekotteCentro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET)Kévin Almeida CheminantRadboud University NijmegenA. AlmelaFacultad Regional Buenos Aires, Universidad Tecnológica Nacional, Buenos Aires, ArgentinaRoberto AloisioGran Sasso Science InstituteJaime Álvarez-MuñizUniversidade de Santiago de CompostelaAntonio AmbrosoneGran Sasso Science InstituteJuan Ammerman YebraUniversidade de Santiago de CompostelaGioacchino Alex AnastasiUniversità di CataniaL. AnchordoquiCity University of New YorkB. AndradaUNSAM)Luciana Andrade DouradoINFN Laboratori Nazionali del Gran SassoS. AndringaLaboratório de Instrumentação e Física Experimental de Partículas–LIP, Instituto Superior Técnico–IST, Universidade de Lisboa–UL, Lisbon, PortugalL. ApollonioINFN, Sezione di MilanoC. AramoINFN, Sezione di NapoliP. R. Araújo FerreiraRWTH Aachen UniversityE. ArnoneINFN, Sezione di TorinoJ. C. Arteaga VelázquezUniversidad Michoacana de San Nicolás de HidalgoP. AssisLaboratório de Instrumentação e Física Experimental de Partículas–LIP, Instituto Superior Técnico–IST, Universidade de Lisboa–UL, Lisbon, PortugalGualberto AvilaObservatorio Pierre Auger and Comisión Nacional de Energía AtómicaEmanuele AvoconeINFN Laboratori Nazionali del Gran SassoAlena BakalováInstitute of Physics of the Czech Academy of SciencesFelicia BarbatoINFN Laboratori Nazionali del Gran SassoAdriel Bartz MocellinColorado School of MinesJ. A. BellidoUniversity of AdelaideCorinne BératUniv. Grenoble AlpesM. E. BertainaUniversità TorinoX. BertouCentro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET), San Carlos de Bariloche, ArgentinaMarta BianciottoUniversità TorinoPeter L. BiermannMax-Planck-Institut für RadioastronomieV. BinetInstituto de Física de Rosario (IFIR)–CONICET/U.N.R., Facultad de Ciencias Bioquímicas y Farmacéuticas U.N.R., Rosario, ArgentinaKathrin BismarkInstitute for Experimental Particle PhysicsTeresa BisterNationaal Instituut voor Kernfysica en Hoge Energie Fysica (NIKHEF), Science ParkJ. BiteauInstitut Universitaire de France (IUF), Paris, FranceJ. BlazekInstitute of Physics of the Czech Academy of SciencesC. BleveUniv. Grenoble AlpesJ. BlümerInstitute for Astroparticle PhysicsM. BoháčováInstitute of Physics of the Czech Academy of SciencesDenise BoncioliINFN Laboratori Nazionali del Gran SassoC. BonifaziECyT-UNSAM and CONICET, Campus Miguelete – San MartínL. Bonneau ArbeletcheUniversidade Estadual de Campinas (UNICAMP), IFGWNataliia BorodaiInstitute of Nuclear Physics PANJ. BrackColorado State UniversityP. G. Brichetto OrcheraUNSAM)F. L. BriechleRWTH Aachen UniversityA. BuenoUniversidad de Granada and C.A.F.P.ES. BuitinkVrije Universiteit BrusselsM. BuscemiUniversità di CataniaMax BüskenUNSAM)Anthony BwembyaRadboud University NijmegenK. S. Caballero‐MoraUniversidad Autónoma de ChiapasS. Cabana-FreireUniversidade de Santiago de CompostelaLorenzo CaccianigaINFN, Sezione di MilanoF. CampuzanoInstituto de Tecnologías en Detección y AstropartículasR. CarusoUniversità di CataniaA. CastellinaINFN, Sezione di TorinoF. CatalaniUniversidade de São PauloG. CataldiINFN, Sezione di LecceLorenzo CazonUniversidade de Santiago de CompostelaM. CerdaObservatorio Pierre AugerBerenika ČermákováInstitute for Astroparticle PhysicsA. CermenatiINFN Laboratori Nazionali del Gran SassoJ. ChinellatoUniversidade Estadual de Campinas (UNICAMP), IFGWJ. ChudobaInstitute of Physics of the Czech Academy of SciencesL. ChytkaPalacky UniversityR. W. ClayUniversity of AdelaideA. C. Cobos CeruttiNational University of General San MartínRoberta ColalilloUniversità di Napoli “Federico II”R. ConceiçãoUniversidade de Lisboa–ULA. CondorelliIJCLab, CNRS/IN2P3, Université Paris-Saclay, Orsay, FranceGiovanni ConsolatiPolitecnico di Milano, Dipartimento di Scienze e Tecnologie AerospazialiM. ConteINFN, Sezione di LecceFabio ConvengaUniversità dell’AquilaDiego Correia dos SantosUniversidade Federal do Rio de JaneiroPaulo J. CostaUniversidade de Lisboa–ULC. E. CovaultCase Western Reserve UniversityM. CristinzianiUniversität SiegenCarlo Salvattore Cruz SanchezUniversidad Nacional de La Plata and CONICETS. DassoCONICET-UBA)K. DaumillerInstitute for Astroparticle PhysicsB. R. DawsonUniversity of AdelaideR. M. de AlmeidaUniversidade Federal do Rio de JaneiroBeatriz de ErricoUniversidade Federal do Rio de JaneiroJoaquín de JesúsUNSAM)S. J. de JongNationaal Instituut voor Kernfysica en Hoge Energie Fysica (NIKHEF), Science ParkJ. R. T. de Mello NetoUniversidade Federal do Rio de JaneiroI. De MitriINFN Laboratori Nazionali del Gran SassoJ. de OliveiraInstituto Federal de Educação, Ciência e Tecnologia do Rio de Janeiro (IFRJ)Danelise de Oliveira FrancoINFN, Sezione di LecceF. de PalmaINFN, Sezione di LecceV. de SouzaUniversidade de São PauloEmanuele De VitoUniversità del SalentoA. Del PopoloUniversità di CataniaO. DelignyCNRS/IN2P3, IJCLab, Université Paris-Saclay, Orsay, FranceN. DennerInstitute of Physics of the Czech Academy of SciencesL. DevalInstituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM), Buenos Aires, ArgentinaA. di MatteoINFN, Sezione di TorinoC. DobrigkeitUniversidade Estadual de Campinas (UNICAMP), IFGW
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Abstract The Pierre Auger Collaboration has embraced the concept of open access to their research data since its foundation, with the aim of giving access to the widest possible community. A gradual process of release began as early as 2007 when 1% of the cosmic-ray data was made public, along with 100% of the space-weather information. In February 2021, a portal was released containing 10% of cosmic-ray data collected by the Pierre Auger Observatory from 2004 to 2018, during the first phase of operation of the Observatory. The Open Data Portal includes detailed documentation about the detection and reconstruction procedures, analysis codes that can be easily used and modified and, additionally, visualization tools. Since then, the Portal has been updated and extended. In 2023, a catalog of the highest-energy cosmic-ray events examined in depth has been included. A specific section dedicated to educational use has been developed with the expectation that these data will be explored by a wide and diverse community, including professional and citizen scientists, and used for educational and outreach initiatives. This paper describes the context, the spirit, and the technical implementation of the release of data by the largest cosmic-ray detector ever built and anticipates its future developments.
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