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The Central Laser Facility is located near the middle of the Pierre Auger Observatory in Argentina. It features a UV laser and optics that direct a beam of calibrated pulsed light into the sky. Light scattered from this beam produces tracks…

Measurements of air showers are accumulating at an increasing rate while construction proceeds at the Pierre Auger Observatory. Although the southern site is only half complete, the cumulative exposure is already similar to those achieved…

Astrophysics · Physics 2012-08-27 The Pierre Auger Collaboration

With the knowledge and statistical precision derived from two decades of measurement, the Pierre Auger Observatory has significantly deepened our understanding of ultra-high-energy cosmic rays while unearthing an increasingly complex…

Instrumentation and Methods for Astrophysics · Physics 2025-08-12 David Schmidt

Air fluorescence detectors measure the energy of ultra-high energy cosmic rays by collecting fluorescence light emitted from nitrogen molecules along the extensive air shower cascade. To ensure a reliable energy determination, the light…

Astrophysics · Physics 2008-11-26 S. Y. BenZvi , B. M. Connolly , J. A. J. Matthews , M. Prouza , E. F. Visbal , S. Westerhoff

This paper summarizes the status and the recent measurements from the Pierre Auger Observatory. The energy spectrum is described and its features discussed. We report searches for anisotropy of cosmic ray arrival directions on large scales…

High Energy Astrophysical Phenomena · Physics 2013-09-06 J. R. T. de Mello Neto

The Pierre Auger Observatory is the largest extensive air shower detector. Based on a hybrid system, this experiment measures the longitudinal shower development and the particles at the ground. This detection system allows the extraction…

High Energy Astrophysical Phenomena · Physics 2021-08-23 Matias Perlin

The Pierre Auger Cosmic-Ray Observatory uses the earth's atmosphere as a calorimeter to measure extensive air-showers created by particles of astrophysical origin. Some of these particles carry joules of energy. At these extreme energies,…

Astrophysics · Physics 2019-08-13 L. Wiencke

The Pierre Auger Observatory is designed to elucidate the origin and nature of Ultra High Energy Cosmic Rays using a hybrid detection technique. A first run of data taking with a prototype version of both detectors (the so called…

Astrophysics · Physics 2007-05-23 Stefano Argiro

In this paper some recent results from the Pierre Auger Collaboration are presented. These are the measurement of the energy spectrum of cosmic rays over a wide range of energies ($10^{17.5}$ to above $10^{20}$ eV), studies of the…

High Energy Astrophysical Phenomena · Physics 2019-05-22 Sergio Petrera

The Pierre Auger Observatory is the largest air-shower detector in the world, offering unparalleled exposure to photons with energies above $5 \times 10^{16}$ eV. Since the start of data collection almost two decades ago, numerous searches…

High Energy Astrophysical Phenomena · Physics 2025-09-08 Pierpaolo Savina

Ultra-high-energy cosmic rays (UHECRs) are the highest energy messengers in the universe, with energies up to $10^{20}$ eV. Studies of astrophysical particles (nuclei, electrons, neutrinos and photons) at their highest observed energies…

High Energy Astrophysical Phenomena · Physics 2020-12-25 Joao de Mello Neto

Data taken at the Pierre Auger Observatory are used to search for air showers initiated by ultra-high energy (UHE) photons. Results of searches are reported from hybrid observations where events are measured with both fluorescence and array…

Astrophysics · Physics 2019-08-13 M. D. Healy

Studies of the cosmic ray energy spectrum at the highest energies with the Pierre Auger Observatory.

High Energy Astrophysical Phenomena · Physics 2009-07-10 The Pierre Auger Collaboration , J. Abraham , P. Abreu , M. Aglietta , C. Aguirre , E. J. Ahn , D. Allard , I. Allekotte , J. Allen , J. Alvarez-Muñiz , M. Ambrosio , L. Anchordoqui , S. Andringa , A. Anzalone , C. Aramo , E. Arganda , S. Argirò , K. Arisaka , F. Arneodo , F. Arqueros , T. Asch , H. Asorey , P. Assis , J. Aublin , M. Ave , G. Avila , T. Bäcker , D. Badagnani , K. B. Barber , A. F. Barbosa , S. L. C. Barroso , B. Baughman , P. Bauleo , J. J. Beatty , T. Beau , B. R. Becker , K. H. Becker , A. Bellétoile , J. A. Bellido , S. BenZvi , C. Berat , P. Bernardini , X. Bertou , P. L. Biermann , P. Billoir , O. Blanch-Bigas , F. Blanco , C. Bleve , H. Blümer , M. Boháčová , D. Boncioli , C. Bonifazi , R. Bonino , N. Borodai , J. Brack , P. Brogueira , W. C. Brown , R. Bruijn , P. Buchholz , A. Bueno , R. E. Burton , N. G. Busca , K. S. Caballero-Mora , L. Caramete , R. Caruso , W. Carvalho , A. Castellina , O. Catalano , L. Cazon , R. Cester , J. Chauvin , A. Chiavassa , J. A. Chinellato , A. Chou , J. Chudoba , J. Chye , R. W. Clay , E. Colombo , R. Conceição , B. Connolly , F. Contreras , J. Coppens , A. Cordier , U. Cotti , S. Coutu , C. E. Covault , A. Creusot , A. Criss , J. Cronin , A. Curutiu , S. Dagoret-Campagne , R. Dallier , K. Daumiller , B. R. Dawson , R. M. de Almeida , M. De Domenico , C. De Donato , S. J. de Jong , G. De La Vega , W. J. M. de Mello Junior , J. R. T. de Mello Neto , I. De Mitri , V. de Souza , K. D. de Vries , G. Decerprit , L. del Peral , O. Deligny , A. Della Selva , C. Delle Fratte , H. Dembinski , C. DiGiulio , J. C. Diaz , P. N. Diep , C. Dobrigkeit , J. C. D'Olivo , P. N. Dong , A. Dorofeev , J. C. dos Anjos , M. T. Dova , D. D'Urso , I. Dutan , M. A. DuVernois , R. Engel , M. Erdmann , C. O. Escobar , A. Etchegoyen , P. Facal San Luis , H. Falcke , G. Farrar , A. C. Fauth , N. Fazzini , F. Ferrer , A. Ferrero , B. Fick , A. Filevich , A. Filipčič , I. Fleck , S. Fliescher , C. E. Fracchiolla , E. D. Fraenkel , W. Fulgione , R. F. Gamarra , S. Gambetta , B. García , D. GarcíaGámez , D. Garcia-Pinto , X. Garrido , G. Gelmini , H. Gemmeke , P. L. Ghia , U. Giaccari , M. Giller , H. Glass , L. M. Goggin , M. S. Gold , G. Golup , F. Gomez Albarracin , M. Gómez Berisso , P. Gonçalves , M. Gonçalves do Amaral , D. Gonzalez , J. G. Gonzalez , D. Góra , A. Gorgi , P. Gouffon , S. R. Gozzini , E. Grashorn , S. Grebe , M. Grigat , A. F. Grillo , Y. Guardincerri , F. Guarino , G. P. Guedes , J. Gutiérrez , J. D. Hague , V. Halenka , P. Hansen , D. Harari , S. Harmsma , J. L. Harton , A. Haungs , M. D. Healy , T. Hebbeker , G. Hebrero , D. Heck , V. C. Holmes , P. Homola , J. R. Hörandel , A. Horneffer , M. Hrabovský , T. Huege , M. Hussain , M. Iarlori , A. Insolia , F. Ionita , A. Italiano , S. Jiraskova , M. Kaducak , K. H. Kampert , T. Karova , P. Kasper , B. Kégl , B. Keilhauer , E. Kemp , R. M. Kieckhafer , H. O. Klages , M. Kleifges , J. Kleinfeller , R. Knapik , J. Knapp , D. -H. Koang , A. Krieger , O. Krömer , D. Kruppke-Hansen , F. Kuehn , D. Kuempel , K. Kulbartz , N. Kunka , A. Kusenko , G. LaRosa , C. Lachaud , B. L. Lago , P. Lautridou , M. S. A. B. Leão , D. Lebrun , P. Lebrun , J. Lee , M. A. Leigui de Oliveira , A. Lemiere , A. Letessier-Selvon , M. Leuthold , I. Lhenry-Yvon , R. López , A. Lopez Agüera , K. Louedec , J. Lozano Bahilo , A. Lucero , H. Lyberis , M. C. Maccarone , C. Macolino , S. Maldera , D. Mandat , P. Mantsch , A. G. Mariazzi , I. C. Maris , H. R. Marquez Falcon , D. Martello , O. Martínez Bravo , H. J. Mathes , J. Matthews , J. A. J. Matthews , G. Matthiae , D. Maurizio , P. O. Mazur , M. McEwen , R. R. McNeil , G. Medina-Tanco , M. Melissas , D. Melo , E. Menichetti , A. Menshikov , R. Meyhandan , M. I. Micheletti , G. Miele , W. Miller , L. Miramonti , S. Mollerach , M. Monasor , D. Monnier Ragaigne , F. Montanet , B. Morales , C. Morello , J. C. Moreno , C. Morris , M. Mostafá , C. A. Moura , S. Mueller , M. A. Muller , R. Mussa , G. Navarra , J. L. Navarro , S. Navas , P. Necesal , L. Nellen , C. Newman-Holmes , D. Newton , P. T. Nhung , N. Nierstenhoefer , D. Nitz , D. Nosek , L. Nožka , M. Nyklicek , J. Oehlschläger , A. Olinto , P. Oliva , V. M. Olmos-Gilbaja , M. Ortiz , N. Pacheco , D. Pakk Selmi-Dei , M. Palatka , J. Pallotta , G. Parente , E. Parizot , S. Parlati , S. Pastor , M. Patel , T. Paul , V. Pavlidou , K. Payet , M. Pech , J. Pȩkala , I. M. Pepe , L. Perrone , R. Pesce , E. Petermann , S. Petrera , P. Petrinca , A. Petrolini , Y. Petrov , J. Petrovic , C. Pfendner , R. Piegaia , T. Pierog , M. Pimenta , T. Pinto , V. Pirronello , O. Pisanti , M. Platino , J. Pochon , V. H. Ponce , M. Pontz , P. Privitera , M. Prouza , E. J. Quel , J. Rautenberg , O. Ravel , D. Ravignani , A. Redondo , B. Revenu , F. A. S. Rezende , J. Ridky , S. Riggi , M. Risse , C. Rivière , V. Rizi , C. Robledo , G. Rodriguez , J. Rodriguez Martino , J. Rodriguez Rojo , I. Rodriguez-Cabo , M. D. Rodríguez-Frías , G. Ros , J. Rosado , T. Rossler , M. Roth , B. Rouillé-d'Orfeuil , E. Roulet , A. C. Rovero , F. Salamida , H. Salazar , G. Salina , F. Sánchez , M. Santander , C. E. Santo , E. M. Santos , F. Sarazin , S. Sarkar , R. Sato , N. Scharf , V. Scherini , H. Schieler , P. Schiffer , A. Schmidt , F. Schmidt , T. Schmidt , O. Scholten , H. Schoorlemmer , J. Schovancova , P. Schovánek , F. Schroeder , S. Schulte , F. Schüssler , D. Schuster , S. J. Sciutto , M. Scuderi , A. Segreto , D. Semikoz , M. Settimo , R. C. Shellard , I. Sidelnik , B. B. Siffert , G. Sigl , A. Śmiałkowski , R. Šmída , B. E. Smith , G. R. Snow , P. Sommers , J. Sorokin , H. Spinka , R. Squartini , E. Strazzeri , A. Stutz , F. Suarez , T. Suomijärvi , A. D. Supanitsky , M. S. Sutherland , J. Swain , Z. Szadkowski , A. Tamashiro , A. Tamburro , T. Tarutina , O. Taşcău , R. Tcaciuc , D. Tcherniakhovski , D. Tegolo , N. T. Thao , D. Thomas , R. Ticona , J. Tiffenberg , C. Timmermans , W. Tkaczyk , C. J. Todero Peixoto , B. Tomé , A. Tonachini , I. Torres , P. Travnicek , D. B. Tridapalli , G. Tristram , E. Trovato , M. Tueros , R. Ulrich , M. Unger , M. Urban , J. F. Valdés Galicia , I. Valiño , L. Valore , A. M. vandenBerg , J. R. Vázquez , R. A. Vázquez , D. Veberič , A. Velarde , T. Venters , V. Verzi , M. Videla , L. Villaseñor , S. Vorobiov , L. Voyvodic , H. Wahlberg , P. Wahrlich , O. Wainberg , D. Warner , A. A. Watson , S. Westerhoff , B. J. Whelan , G. Wieczorek , L. Wiencke , B. Wilczyńska , H. Wilczyński , C. Wileman , M. G. Winnick , H. Wu , B. Wundheiler , T. Yamamoto , P. Younk , G. Yuan , A. Yushkov , E. Zas , D. Zavrtanik , M. Zavrtanik , I. Zaw , A. Zepeda , M. Ziolkowski

The Pierre Auger Observatory is the largest facility in the world to study ultra-high-energy cosmic rays. It has a hybrid detection technique that combines the observation of the longitudinal development of extensive air showers and the…

High Energy Astrophysical Phenomena · Physics 2021-10-28 B. Andrada

We report on the observations of cosmic rays with energies > 1.0 EeV from Jan 2004 to April 2009 by the Pierre Auger Observatory. During this period the Observatory has grown from about 300 surface detectors to about 1600 upon its…

High Energy Astrophysical Phenomena · Physics 2009-11-25 James W. Cronin

The Pierre Auger Observatory has been designed to study the highest-energy cosmic rays in nature (E > 10^{18.5} eV). The determination of their arrival direction, energy and composition is performed by the analysis of the atmospheric…

Ultra-high energy cosmic rays (UHECRs) have been studied with the data of the Pierre Auger Observatory for more than fifteen years. An essential feature of the Observatory is its hybrid design: UHECRs are detected through the observation of…

High Energy Astrophysical Phenomena · Physics 2023-09-06 Olivier Deligny

The Pierre Auger Observatory in Malarg\"ue, Argentina, is designed to study the properties of ultra-high energy cosmic rays with energies above 1018 eV. It is a hybrid facility that employs a Fluorescence Detector to perform nearly…

Instrumentation and Methods for Astrophysics · Physics 2014-07-03 Pierre Auger Collaboration

Ultra high energy particles arrive at Earth constantly. They provide a beam at energies higher than any man-made accelerator, but at a very low rate. Two large experiments, the Pierre Auger Observatory and the Telescope Array experiment,…

High Energy Astrophysical Phenomena · Physics 2011-11-14 Miguel Mostafa

The Pierre Auger Observatory has been detecting ultra-high energy cosmic rays (UHECRs) for more than fifteen years. An essential feature of the Observatory is its hybrid design: cosmic rays above $100~$PeV are detected through the…

High Energy Astrophysical Phenomena · Physics 2023-03-01 Olivier Deligny