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The fluorescence-detection techniques of cosmic-ray air-shower experiments require precise knowledge of atmospheric properties to reconstruct air-shower energies. Up to now, the atmosphere in desert-like areas was assumed to be stable…

The Pierre Auger Observatory is a``hybrid'' UHECR detector. The surface detector (SD) and air fluorescence detector (FD) of the observatory are designed for observation of cosmic ray showers in coincidence, with a 10% duty cycle. The…

Astrophysics · Physics 2019-08-14 B. Fick

The Pierre Auger Observatory, a hybrid detector for the study of ultra-high energy cosmic rays (UHECRs), is now approaching completion. After describing Auger present status and performance, with an emphasis on the advantages provided by…

Astrophysics · Physics 2019-08-13 Veronique Van Elewyck

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

The Pierre Auger Observatory detects ultra-high energy cosmic rays by implementing two complementary air-shower techniques. The combination of a large ground array and fluorescence detectors, known as the hybrid concept, means that a rich…

Astrophysics · Physics 2008-11-26 Miguel Mostafa

The Surface Detector of the Pierre Auger Observatory will consist of 1600 water Cherenkov tanks sampling ground particles of air showers produced by energetic cosmic rays. The arrival times are obtained from GPS and power is provided by…

Astrophysics · Physics 2019-08-14 Tiina Suomijarvi

The Pierre Auger Observatory is a detector for ultra-high energy cosmic rays. It consists of a surface array to measure secondary particles at ground level and a fluorescence detector to measure the development of air showers in the…

High Energy Astrophysical Phenomena · Physics 2012-08-27 The Pierre Auger Collaboration

The High Elevation Auger Telescopes (HEAT) are three tiltable fluorescence telescopes which represent a low energy enhancement of the fluorescence telescope system of the southern site of the Pierre Auger Observatory in Argentina. The…

Instrumentation and Methods for Astrophysics · Physics 2019-08-14 C. Meurer , N. Scharf

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 Observatory has been designed to investigate the most energetic particles known, the ultra high energy cosmic rays. The observatory, covering an area of 3000 km^2, combines two different detection techniques to study the…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Ruben Conceição

The Pierre Auger Observatory has been operating in Malargue, Province of Mendoza, western Argentina, for over two decades, significantly advancing our understanding of cosmic rays. Beyond its scientific mission, the installation and…

Instrumentation and Methods for Astrophysics · Physics 2025-07-22 Ingomar Allekotte , Alejandra Calvo

The focus of this article is on recent results on ultra-high energy cosmic rays obtained with the Pierre Auger Observatory. The world's largest instrument of this type and its performance are described. The observations presented here…

Astrophysics · Physics 2019-08-13 Johannes Bluemer

The Pierre Auger Observatory is currently the largest observatory of Ultra High Energy Cosmic Rays. Having more data collected than any previous experiment and using a hybrid technique, it can provide important information to unveil the…

High Energy Astrophysical Phenomena · Physics 2019-08-13 R. Conceição

The Pierre Auger Observatory is the world's largest cosmic ray observatory. Our current exposure reaches nearly 40,000 km$^2$ str and provides us with an unprecedented quality data set. The performance and stability of the detectors and…

High Energy Astrophysical Phenomena · Physics 2019-08-15 Antoine Letessier-Selvon , A. Aab , P. Abreu , M. Aglietta , M. Ahlers , E. J. Ahn , I. F. M. Albuquerque , I. Allekotte , J. Allen , P. Allison , A. Almela , J. Alvarez Castillo , J. Alvarez-Muniz , R. Alves Batista , M. Ambrosio , A. Aminaei , L. Anchordoqui , S. Andringa , T. Antivcic , C. Aramo , F. Arqueros , H. Asorey , P. Assis , J. Aublin , M. Ave , M. Avenier , G. Avila , A. M. Badescu , K. B. Barber , R. Bardenet , J. Baeuml , C. Baus , J. J. Beatty , K. H. Becker , A. Belletoile , J. A. Bellido , S. BenZvi , C. Berat , X. Bertou , P. L. Biermann , P. Billoir , F. Blanco , M. Blanco , C. Bleve , H. Blumer , M. Bohacova , D. Boncioli , C. Bonifazi , R. Bonino , N. Borodai , J. Brack , I. Brancus , P. Brogueira , W. C. Brown , P. Buchholz , A. Bueno , R. E. Burton , M. Buscemi , K. S. Caballero-Mora , B. Caccianiga , L. Caccianiga , M. Candusso , L. Caramete , R. Caruso , A. Castellina , G. Cataldi , L. Cazon , R. Cester , S. H. Cheng , A. Chiavassa , J. A. Chinellato , J. Chudoba , M. Cilmo , R. W. Clay , G. Cocciolo , R. Colalillo , L. Collica , M. R. Coluccia , R. Conceicao , F. Contreras , H. Cook , M. J. Cooper , S. Coutu , C. E. Covault , A. Criss , J. Cronin , A. Curutiu , R. Dallier , B. Daniel , S. Dasso , K. Daumiller , B. R. Dawson , R. M. de Almeida , M. De Domenico , 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 , L. del Peral , O. Deligny , H. Dembinski , N. Dhital , C. Di Giulio , J. C. Diaz , M. L. Diaz Castro , P. N. Diep , F. Diogo , C. Dobrigkeit , W. Docters , J. C. D'Olivo , P. N. Dong , A. Dorofeev , J. C. dos Anjos , M. T. Dova , J. Ebr , R. Engel , M. Erdmann , C. O. Escobar , J. Espadanal , A. Etchegoyen , P. Facal San Luis , H. Falcke , K. Fang , G. Farrar , A. C. Fauth , N. Fazzini , A. P. Ferguson , B. Fick , J. M. Figueira , A. Filevich , A. Filipcic , N. Foerster , B. D. Fox , C. E. Fracchiolla , E. D. Fraenkel , O. Fratu , U. Frohlich , B. Fuchs , R. Gaior , R. F. Gamarra , S. Gambetta , B. Garcia , S. T. Garcia Roca , D. Garcia-Gamez , D. Garcia-Pinto , G. Garilli , A. Gascon Bravo , H. Gemmeke , P. L. Ghia , M. Giller , J. Gitto , C. Glaser , H. Glass , F. Gomez Albarracin , M. Gomez Berisso , P. F. Gomez Vitale , P. Goncalves , J. G. Gonzalez , B. Gookin , A. Gorgi , P. Gorham , P. Gouffon , S. Grebe , N. Griffith , A. F. Grillo , T. D. Grubb , Y. Guardincerri , F. Guarino , G. P. Guedes , P. Hansen , D. Harari , T. A. Harrison , J. L. Harton , A. Haungs , T. Hebbeker , D. Heck , A. E. Herve , G. C. Hill , C. Hojvat , N. Hollon , P. Homola , J. R. Hoerandel , P. Horvath , M. Hrabovsky , D. Huber , T. Huege , A. Insolia , P. G. Isar , S. Jansen , C. Jarne , M. Josebachuili , K. Kadija , O. Kambeitz , K. H. Kampert , P. Karhan , P. Kasper , I. Katkov , B. Kegl , B. Keilhauer , A. Keivani , E. Kemp , R. M. Kieckhafer , H. O. Klages , M. Kleifges , J. Kleinfeller , J. Knapp d , R. Krause , N. Krohm , O. Kroemer , D. Kruppke-Hansen , D. Kuempel , N. Kunka , G. La Rosa , D. LaHurd , L. Latronico , R. Lauer , M. Lauscher , P. Lautridou , S. Le Coz , M. S. A. B. Leao , D. Lebrun , P. Lebrun , M. A. Leigui de Oliveira , I. Lhenry-Yvon , K. Link , R. Lopez , A. Lopez Aguera , K. Louedec , J. Lozano Bahilo , L. Lu , A. Lucero , M. Ludwig , H. Lyberis , M. C. Maccarone , C. Macolino , M. Malacari , S. Maldera , J. Maller , D. Mandat , P. Mantsch , A. G. Mariazzi , V. Marin , I. C. Maris , H. R. Marquez Falcon , G. Marsella , D. Martello , L. Martin , H. Martinez , O. Martinez Bravo , D. Martraire , J. J. Masias Meza , H. J. Mathes , J. Matthews , J. A. J. Matthews , G. Matthiae , D. Maurel , D. Maurizio , E. Mayotte , P. O. Mazur , C. Medina , G. Medina-Tanco , M. Melissas , D. Melo , E. Menichetti , A. Menshikov , S. Messina , R. Meyhandan , S. Micanovic , M. I. Micheletti , L. Middendorf , I. A. Minaya , L. Miramonti , B. Mitrica , L. Molina-Bueno , S. Mollerach , M. Monasor , D. Monnier Ragaigne , F. Montanet , B. Morales , C. Morello , J. C. Moreno , M. Mostafa , C. A. Moura , M. A. Muller , G. Muller , M. Munchmeyer , R. Mussa , G. Navarra , J. L. Navarro , S. Navas , P. Necesal , L. Nellen , A. Nelles , J. Neuser , P. T. Nhung , M. Niechciol , L. Niemietz , T. Niggemann , D. Nitz , D. Nosek , L. Novzka , J. Oehlschlager , A. Olinto , M. Oliveira , M. Ortiz , N. Pacheco , D. Pakk Selmi-Dei , M. Palatka , J. Pallotta , N. Palmieri , G. Parente , A. Parra , S. Pastor , T. Paul , M. Pech , J. Pekala , R. Pelayo , I. M. Pepe , L. Perrone , R. Pesce , E. Petermann , S. Petrera , A. Petrolini , Y. Petrov , R. Piegaia , T. Pierog , P. Pieroni , M. Pimenta , V. Pirronello , M. Platino , M. Plum , M. Pontz , A. Porcelli , T. Preda , P. Privitera , M. Prouza , E. J. Quel , S. Querchfeld , S. Quinn , J. Rautenberg , O. Ravel , D. Ravignani , B. Revenu , J. Ridky , S. Riggi , M. Risse , P. Ristori , H. Rivera , V. Rizi , J. Roberts , W. Rodrigues de Carvalho , I. Rodriguez Cabo , G. Rodriguez Fernandez , J. Rodriguez Martino , J. Rodriguez Rojo , M. D. Rodriguez-Frias , G. Ros , J. Rosado , T. Rossler , M. Roth , B. Rouille-d'Orfeuil , E. Roulet , A. C. Rovero , C. Ruhle , S. J. Saffi , A. Saftoiu , F. Salamida , H. Salazar , F. Salesa Greus , G. Salina , F. Sanchez , P. Sanchez-Lucas , C. E. Santo , E. Santos , E. M. Santos , F. Sarazin , B. Sarkar , R. Sato , N. Scharf , V. Scherini , H. Schieler , P. Schiffer , A. Schmidt , O. Scholten , H. Schoorlemmer , P. Schovanek , F. G. Schroeder , A. Schulz , J. Schulz , S. J. Sciutto , M. Scuderi , A. Segreto , M. Settimo , A. Shadkam , R. C. Shellard , I. Sidelnik , G. Sigl , O. Sima , A. Smialkowski , R. Smida , G. R. Snow , P. Sommers , J. Sorokin , H. Spinka , R. Squartini , Y. N. Srivastava , S. Stanic , J. Stapleton , J. Stasielak , M. Stephan , M. Straub , A. Stutz , F. Suarez , T. Suomijarvi , A. D. Supanitsky , T. Susa , M. S. Sutherland , J. Swain , Z. Szadkowski , M. Szuba , A. Tapia , M. Tartare , O. Tacscuau , R. Tcaciuc , N. T. Thao , J. Tiffenberg , C. Timmermans , W. Tkaczyk , C. J. Todero Peixoto , G. Toma , L. Tomankova , B. Tome , A. Tonachini , G. Torralba Elipe , D. Torres Machado , P. Travnicek , D. B. Tridapalli , E. Trovato , M. Tueros , R. Ulrich , M. Unger , J. F. Valdes Galicia , I. Valino , L. Valore , G. van Aar , A. M. van den Berg , S. van Velzen , A. van Vliet , E. Varela , B. Vargas Cardenas , G. Varner , J. R. Vazquez , R. A. Vazquez , D. Veberic , V. Verzi , J. Vicha , M. Videla , L. Villasenor , H. Wahlberg , P. Wahrlich , O. Wainberg , D. Walz , A. A. Watson , M. Weber , K. Weidenhaupt , A. Weindl , F. Werner , S. Westerhoff , B. J. Whelan , A. Widom , G. Wieczorek , L. Wiencke , B. Wilczynska , H. Wilczynski , M. Will , C. Williams , T. Winchen , B. Wundheiler , S. Wykes , T. Yamamoto , T. Yapici , P. Younk , G. Yuan , A. Yushkov , B. Zamorano , E. Zas , D. Zavrtanik , M. Zavrtanik , I. Zaw , A. Zepeda , J. Zhou , Y. Zhu , M. Zimbres Silva , M. Ziolkowski

The Pierre Auger Observatory in Argentina provides the largest data sample of the cosmic ray events with energy above 10$^{18}$ eV. These high energy events can be used to test our understanding of the hadronic interactions at energies…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Petr Travnicek

The Pierre Auger Observatory advances the study of ultra-high-energy cosmic rays through a hybrid system of surface and fluorescence detectors. This paper presents recent results, including refined spectrum measurements, anisotropy…

High Energy Astrophysical Phenomena · Physics 2025-04-15 Qader Dorosti Hasankiadeh

The Pierre Auger Observatory has already collected more ultra high energy cosmic ray data than all the previous experiments. With an hybrid detection technique, it can provide coherent results on the flux, energy spectrum and arrival…

High Energy Physics - Experiment · Physics 2019-08-17 S. Andringa

The successful installation and operation of the Pierre Auger Observatory in Argentina has been a milestone in Astroparticle research in Latin America, generating new regional research opportunities in the field. In this context, the LAGO…

Instrumentation and Methods for Astrophysics · Physics 2014-07-31 Iván Sidelnik

Over the past decade the multi-messenger astrophysics has emerged as a distinct discipline, providing unique insights into the properties of high-energy phenomena in the Universe. The Pierre Auger Observatory, located in Malarg\"ue,…

High Energy Astrophysical Phenomena · Physics 2021-02-02 Lukas Zehrer

While the completion of the Pierre Auger Observatory (or simply ``Auger'') is still underway, the 5165 km^2.sr.yr integrated acceptance accumulated since the January 1st, 2004 is now significantly larger than what was gathered by the…

Astrophysics · Physics 2019-08-13 E. Parizot