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Search for the Anomalous Events Detected by ANITA Using the Pierre Auger Observatory

Adila Abdul HalimUniversity of AdelaideP. AbreuUniversidade de Lisboa—ULM. AgliettaINFNI. AllekotteCentro Atómico Bariloche and Instituto Balseiro (CNEA-UNCuyo-CONICET)Kévin Almeida CheminantInstitute of Nuclear Physics PAN, Krakow, PolandA. AlmelaInstituto de Tecnologías en Detección y Astropartículas (CNEA, CONICET, UNSAM)Roberto AloisioGran Sasso Science InstituteJaime Álvarez-MuñizUniversidade de Santiago de CompostelaJuan Ammerman YebraUniversidade de Santiago de CompostelaGioacchino Alex AnastasiINFNL. AnchordoquiDepartment of Physics and Astronomy, Lehman College, City University of New York, Bronx, New York, USAB. AndradaInstituto de Tecnologías en Detección y AstropartículasS. AndringaUniversidade de Lisboa—ULL. ApollonioINFNC. AramoINFNPaulo Ricardo Araújo FerreiraRWTH Aachen UniversityE. ArnoneINFNJ. C. Arteaga VelázquezUniversidad Michoacana de San Nicolás de HidalgoP. AssisUniversidade de Lisboa—ULG. ÁvilaObservatorio Pierre Auger and Comisión Nacional de Energía AtómicaEmanuele AvoconeUniversità dell’AquilaAlena BakalováInstitute of Physics of the Czech Academy of SciencesFelicia BarbatoINFN Laboratori Nazionali del Gran SassoAdriel Bartz MocellinColorado School of MinesJ. A. BellidoUniversidad Nacional de San Agustin de ArequipaCorinne BératUniv. Grenoble AlpesM. E. BertainaINFNGopal BhattaInstitute of Nuclear Physics PAN, Krakow, PolandMarta BianciottoUniversità TorinoPeter L. BiermannUniversidade de São Paulo, Escola de Engenharia de Lorena, Lorena, Sao Paulo, BrazilV. BinetFacultad de Ciencias Bioquímicas y Farmacéuticas U.N.RKathrin BismarkKarlsruhe Institute of Technology (KIT), Institute for Experimental Particle Physics, Karlsruhe, GermanyTeresa BisterRadboud University NijmegenJonathan BiteauUniversité Paris-SaclayJiří BlažekInstitute of Physics of the Czech Academy of SciencesC. BleveUniv. Grenoble AlpesJ. BlümerKarlsruhe Institute of Technology (KIT)M. BoháčováInstitute of Physics of the Czech Academy of SciencesDenise BoncioliINFN Laboratori Nazionali del Gran SassoC. BonifaziUniversidade Federal do Rio de JaneiroL. Bonneau ArbeletcheUniversidade Estadual de Campinas (UNICAMP)Nataliia BorodaiInstitute of Nuclear Physics PAN, Krakow, PolandJ. BrackInstituto de Física de Rosario (IFIR)-CONICET/U.N.R. and Facultad de Ciencias Bioquímicas y Farmacéuticas U.N.R., Rosario, ArgentinaP. G. Brichetto OrcheraInstituto de Tecnologías en Detección y AstropartículasF. L. BriechleRWTH Aachen UniversityA. BuenoUniversidad de GranadaS. BuitinkVrije Universiteit BrusselsM. BuscemiINFNM. BüskenKarlsruhe Institute of Technology (KIT)Anthony BwembyaRadboud University NijmegenK. S. Caballero‐MoraUniversidad Autónoma de ChiapasS. Cabana-FreireUniversidade de Santiago de CompostelaLorenzo CaccianigaUniversità di MilanoF. CampuzanoConsejo Nacional de Investigaciones Científicas y TécnicasI. CaracasBergische Universität WuppertalR. CarusoUniversità di CataniaA. CastellinaOsservatorio Astrofisico di Torino (INAF)F. CatalaniUniversidade de São PauloG. CataldiINFNLorenzo CazonUniversidade de Santiago de CompostelaM. CerdaObservatorio Pierre AugerA. CermenatiGran Sasso Science InstituteJ. ChudobaInstitute of Physics of the Czech Academy of SciencesL. ChytkaPalacky UniversityR. W. ClayUniversity of AdelaideA. C. Cobos CeruttiConsejo Nacional de Investigaciones Científicas y TécnicasRoberta ColalilloUniversità di Napoli “Federico IIM.R. ColucciaINFNR. ConceiçãoUniversidade de Lisboa—ULA. CondorelliUniversité Paris-SaclayGiovanni ConsolatiPolitecnico di Milano, Dipartimento di Scienze e Tecnologie AerospazialiMarcelo ConteUniversità del SalentoFabio ConvengaINFN Laboratori Nazionali del Gran SassoD. Correia dos SantosUniversidade Federal FluminensePedro J. CostaUniversidade de Lisboa—ULC. E. CovaultCase Western Reserve UniversityM. CristinzianiUniversität SiegenCarlo Salvattore Cruz SanchezUniversidad Nacional de La Plata and CONICETS. DassoInstitute of Astronomy and Space PhysicsK. DaumillerKarlsruhe Institute of Technology (KIT)B. R. DawsonUniversity of AdelaideR. M. de AlmeidaUniversidade Federal FluminenseJoaquín de JesúsKarlsruhe Institute of Technology (KIT), Institute for Astroparticle Physics, Karlsruhe, GermanyS. J. de JongNationaal Instituut voor Kernfysica en Hoge Energie Fysica (NIKHEF)J. R. T. de Mello NetoUniversidade Federal do Rio de JaneiroI. De MitriINFN Laboratori Nazionali del Gran SassoJ. de OliveiraDanelise de Oliveira FrancoINFNF. de PalmaUniversità del SalentoV. de SouzaUniversidade de São PauloBeatriz de ErricoUniversidade Federal do Rio de JaneiroEmanuele De VitoUniversità del SalentoA. Del PopoloINFNO. DelignyUniversité Paris-SaclayN. DennerInstitute of Physics of the Czech Academy of SciencesL. DevalKarlsruhe Institute of Technology (KIT)A. di MatteoINFNM. Dobre“Horia Hulubei” National Institute for Physics and Nuclear EngineeringC. DobrigkeitUniversidade Estadual de Campinas (UNICAMP)
Physical Review Lettersjournal2025en
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A dedicated search for upward-going air showers at zenith angles exceeding 110° and energies E>0.1 EeV has been performed using the Fluorescence Detector of the Pierre Auger Observatory. The search is motivated by two "anomalous" radio pulses observed by the ANITA flights I and III that appear inconsistent with the standard model of particle physics. Using simulations of both regular cosmic-ray showers and upward-going events, a selection procedure has been defined to separate potential upward-going candidate events and the corresponding exposure has been calculated in the energy range [0.1-33] EeV. One event has been found in the search period between January 1, 2004, and December 31, 2018, consistent with an expected background of 0.27±0.12 events from misreconstructed cosmic-ray showers. This translates to an upper bound on the integral flux of (7.2±0.2)×10^{-21} cm^{-2} sr^{-1} y^{-1} and (3.6±0.2)×10^{-20} cm^{-2} sr^{-1} y^{-1} for an E^{-1} and E^{-2} spectrum, respectively. An upward-going flux of showers normalized to the ANITA observations is shown to predict over 34 events for an E^{-3} spectrum and over 8.1 events for a conservative E^{-5} spectrum, in strong disagreement with the interpretation of the anomalous events as upward-going showers.

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