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Related papers: The Pierre Auger Cosmic Ray Observatory

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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 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

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

High Energy Astrophysical Phenomena · Physics 2011-07-26 The Pierre Auger Collaboration , P. Abreu , M. Aglietta , E. J. Ahn , I. F. M. Albuquerque , D. Allard , I. Allekotte , J. Allen , P. Allison , J. Alvarez Castillo , J. Alvarez-Muñiz , M. Ambrosio , A. Aminaei , L. Anchordoqui , S. Andringa , T. Antičić , A. Anzalone , C. Aramo , E. Arganda , F. Arqueros , H. Asorey , P. Assis , J. Aublin , M. Ave , M. Avenier , G. Avila , T. Bäcker , M. Balzer , K. B. Barber , A. F. Barbosa , R. Bardenet , S. L. C. Barroso , B. Baughman , J. Bäuml , J. J. Beatty , B. R. Becker , K. H. Becker , A. Bellétoile , J. A. Bellido , S. BenZvi , C. Berat , X. Bertou , P. L. Biermann , P. Billoir , F. Blanco , M. 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 , K. S. Caballero-Mora , L. Caramete , R. Caruso , A. Castellina , O. Catalano , G. Cataldi , L. Cazon , R. Cester , J. Chauvin , S. H. Cheng , A. Chiavassa , J. A. Chinellato , A. Chou , J. Chudoba , R. W. Clay , M. R. Coluccia , R. Conceição , F. Contreras , H. Cook , M. J. Cooper , J. Coppens , A. Cordier , U. Cotti , S. Coutu , C. E. Covault , A. Creusot , A. Criss , J. Cronin , A. Curutiu , S. Dagoret-Campagne , R. Dallier , S. Dasso , 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 , H. Dembinski , N. Dhital , C. Di Giulio , J. C. Diaz , M. L. Díaz Castro , P. N. Diep , C. Dobrigkeit , W. Docters , J. C. D'Olivo , P. N. Dong , A. Dorofeev , J. C. dos Anjos , M. T. Dova , D. D'Urso , I. Dutan , J. Ebr , R. Engel , M. Erdmann , C. O. Escobar , A. Etchegoyen , P. Facal San Luis , I. Fajardo Tapia , H. Falcke , G. Farrar , A. C. Fauth , N. Fazzini , A. P. Ferguson , A. Ferrero , B. Fick , A. Filevich , A. Filipčič , S. Fliescher , C. E. Fracchiolla , E. D. Fraenkel , U. Fröhlich , B. Fuchs , R. Gaior , R. F. Gamarra , S. Gambetta , B. García , D. García Gámez , D. Garcia-Pinto , A. Gascon , H. Gemmeke , K. Gesterling , P. L. Ghia , U. Giaccari , M. Giller , H. Glass , M. S. Gold , G. Golup , F. Gomez Albarracin , M. Gómez Berisso , P. Gonçalves , D. Gonzalez , J. G. Gonzalez , B. Gookin , D. Góra , A. Gorgi , P. Gouffon , S. R. Gozzini , E. Grashorn , S. Grebe , N. Griffith , M. Grigat , A. F. Grillo , Y. Guardincerri , F. Guarino , G. P. Guedes , A. Guzman , J. D. Hague , P. Hansen , D. Harari , S. Harmsma , J. L. Harton , A. Haungs , T. Hebbeker , D. Heck , A. E. Herve , C. Hojvat , N. Hollon , V. C. Holmes , P. Homola , J. R. Hörandel , A. Horneffer , M. Hrabovský , T. Huege , A. Insolia , F. Ionita , A. Italiano , C. Jarne , S. Jiraskova , M. Josebachuili , K. Kadija , K. -H. Kampert , P. Karhan , P. Kasper , B. Kégl , B. Keilhauer , A. Keivani , J. L. Kelley , E. Kemp , R. M. Kieckhafer , H. O. Klages , M. Kleifges , J. Kleinfeller , J. Knapp , D. -H. Koang , K. Kotera , N. Krohm , O. Krömer , D. Kruppke-Hansen , F. Kuehn , D. Kuempel , J. K. Kulbartz , N. Kunka , G. La Rosa , C. Lachaud , P. Lautridou , M. S. A. B. Leão , D. Lebrun , P. Lebrun , M. A. Leigui de Oliveira , A. Lemiere , A. Letessier-Selvon , I. Lhenry-Yvon , K. Link , R. López , A. Lopez Agüera , K. Louedec , J. Lozano Bahilo , A. Lucero , M. Ludwig , H. Lyberis , M. C. Maccarone , C. Macolino , S. Maldera , D. Mandat , P. Mantsch , A. G. Mariazzi , J. Marin , V. Marin , I. C. Maris , H. R. Marquez Falcon , G. Marsella , D. Martello , L. Martin , H. Martinez , O. Martínez Bravo , H. J. Mathes , J. Matthews , J. A. J. Matthews , G. Matthiae , D. Maurizio , P. O. Mazur , G. Medina-Tanco , M. Melissas , D. Melo , E. Menichetti , A. Menshikov , P. Mertsch , C. Meurer , S. Mićanović , M. I. Micheletti , W. Miller , L. Miramonti , S. Mollerach , M. Monasor , D. Monnier Ragaigne , F. Montanet , B. Morales , C. Morello , E. Moreno , J. C. Moreno , C. Morris , M. Mostafá , C. A. Moura , S. Mueller , M. A. Muller , G. Müller , M. Münchmeyer , R. Mussa , G. Navarra , J. L. Navarro , S. Navas , P. Necesal , L. Nellen , A. Nelles , J. Neuser , P. T. Nhung , L. Niemietz , N. Nierstenhoefer , D. Nitz , D. Nosek , L. Nožka , M. Nyklicek , J. Oehlschläger , A. Olinto , V. M. Olmos-Gilbaja , M. Ortiz , N. Pacheco , D. Pakk Selmi-Dei , M. Palatka , J. Pallotta , N. Palmieri , G. Parente , E. Parizot , A. Parra , R. D. Parsons , S. Pastor , T. Paul , M. Pech , J. Pȩkala , R. Pelayo , I. M. Pepe , L. Perrone , R. Pesce , E. Petermann , S. Petrera , P. Petrinca , A. Petrolini , Y. Petrov , J. Petrovic , C. Pfendner , N. Phan , R. Piegaia , T. Pierog , P. Pieroni , M. Pimenta , V. Pirronello , M. Platino , V. H. Ponce , M. Pontz , P. Privitera , M. Prouza , E. J. Quel , S. Querchfeld , J. Rautenberg , O. Ravel , D. Ravignani , B. Revenu , J. Ridky , S. Riggi , M. Risse , P. Ristori , H. Rivera , V. Rizi , J. Roberts , C. Robledo , W. Rodrigues de Carvalho , 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 , C. Rühle , F. Salamida , H. Salazar , G. Salina , F. Sánchez , M. Santander , C. E. Santo , E. Santos , E. M. Santos , F. Sarazin , B. Sarkar , S. Sarkar , R. Sato , N. Scharf , V. Scherini , H. Schieler , P. Schiffer , A. Schmidt , F. Schmidt , O. Scholten , H. Schoorlemmer , J. Schovancova , P. Schovánek , F. Schröder , S. Schulte , D. Schuster , S. J. Sciutto , M. Scuderi , A. Segreto , M. Settimo , A. Shadkam , R. C. Shellard , I. Sidelnik , G. Sigl , H. H. Silva Lopez , A. Śmiał kowski , R. Šmída , G. R. Snow , P. Sommers , J. Sorokin , H. Spinka , R. Squartini , S. Stanic , J. Stapleton , J. Stasielak , M. Stephan , E. Strazzeri , A. Stutz , F. Suarez , T. Suomijärvi , A. D. Supanitsky , T. Šuša , M. S. Sutherland , J. Swain , Z. Szadkowski , M. Szuba , A. Tamashiro , A. Tapia , M. Tartare , O. Taşcău , C. G. Tavera Ruiz , R. Tcaciuc , D. Tegolo , N. T. Thao , D. Thomas , J. Tiffenberg , C. Timmermans D. K. Tiwari , W. Tkaczyk , C. J. Todero Peixoto , B. Tomé , A. Tonachini , 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. van den Berg , E. Varela , B. Vargas Cárdenas , J. R. Vázquez , R. A. Vázquez , D. Veberič , V. Verzi , J. Vicha , M. Videla , L. Villaseñor , H. Wahlberg , P. Wahrlich , O. Wainberg , D. Walz , D. Warner , A. A. Watson , M. Weber , K. Weidenhaupt , A. Weindl , S. Westerhoff , B. J. Whelan , G. Wieczorek , L. Wiencke , B. Wilczyńska , H. Wilczyński , M. Will , C. Williams , T. Winchen , L. Winders , M. G. Winnick , M. Wommer , B. Wundheiler , T. Yamamoto , T. Yapici , P. Younk , G. Yuan , A. Yushkov , B. Zamorano , E. Zas , D. Zavrtanik , M. Zavrtnik , I. Zaw , A. Zepeda , M. Zimbres-Silva , M. Ziolkowski

Recent measurements of the properties of cosmic rays above 10^17 eV are summarized and implications on our contemporary understanding of their origin are discussed. Cosmic rays with energies exceeding 10^20 eV have been measured, they are…

Astrophysics · Physics 2015-05-13 Joerg R. Hoerandel

Ultra High Energy Cosmic Rays are the most energetic particles directly measured, reaching orders of magnitude above those attained in the LHC. The Pierre Auger Observatory is shedding light onto the long-standing mysteries of their nature…

High Energy Astrophysical Phenomena · Physics 2019-08-17 L. Cazon

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, located in Argentina, provides an unprecedented integrated aperture for the search of photons with energy above 100 PeV. In this contribution recent results are presented including the diffuse search for…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Daniel Kuempel

The Pierre Auger Observatory is a hybrid detector designed to observe and study ultra-high-energy particles of extraterrestrial origin. With its 27 fluorescence telescopes and over 1600 autonomously operating water-Cherenkov detectors…

Instrumentation and Methods for Astrophysics · Physics 2025-07-22 Paul Filip

The Auger Engineering Radio Array (AERA) complements the Pierre Auger Observatory with 150 radio-antenna stations measuring in the frequency range from 30 to 80 MHz. With an instrumented area of 17 km$^2$, the array constitutes the largest…

Instrumentation and Methods for Astrophysics · Physics 2019-06-12 Tim Huege

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

Ultra-high-energy cosmic rays (UHECR), of energy >10 EeV, arrive at the Earth regularly, but their sources, acceleration mechanisms, details of propagation through the universe, and particle composition remain mysteries. In addition, their…

Instrumentation and Methods for Astrophysics · Physics 2020-12-10 Sijbrand de Jong

The Pierre Auger Observatory is the largest operating cosmic ray observatory ever built. Calorimetric measurements of extensive air showers induced by cosmic rays are performed with a fluorescence detector. Thus, one of the main challenges…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 K. Louedec

This paper presents the highlights from the recent measurements of the energy spectrum, mass composition, and arrival directions of the ultra-high energy ($> 10^{17}$ eV = 0.1 EeV) cosmic rays (UHECR) by the Pierre Auger Observatory. The…

Astrophysics · Physics 2019-08-13 Serguei Vorobiov

The world largest exposure to ultra-high energy cosmic rays accumulated by the Pierre Auger Observatory led to major advances in our understanding of their properties, but the many unknowns about the nature and distribution of the sources,…

High Energy Astrophysical Phenomena · Physics 2019-06-12 Antonella Castellina

Ultra-high-energy cosmic rays (UHECRs) are studied with giant ground-based detector systems recording extensive air showers, induced by cosmic ray particles in the atmosphere. Research at the Pierre Auger Observatory - the largest of such…

High Energy Astrophysical Phenomena · Physics 2022-05-04 Jaroslaw Stasielak

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

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 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, dedicated to measuring ultra-high energy cosmic rays, has been promoting for more than two decades educational and scientific outreach activities to make its results known in an understandable language to…

High Energy Astrophysical Phenomena · Physics 2025-09-16 Fabio Convenga

We report a measurement of the flux of cosmic rays with unprecedented precision and statistics using data from the Pierre Auger Observatory. Based on fluorescence observations in coincidence with at least one station of the surface detector…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Ioana C. Maris