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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…

天体物理学 · 物理学 2019-08-13 Serguei Vorobiov

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…

天体物理学 · 物理学 2010-04-15 M. C. Medina , M. Gomez Berisso , I. Allekotte , A. Etchegoyen , G. Medina-Tanco , A. D. Supanitsky

The Pierre Auger Observatory is designed to study cosmic rays of the highest energies ($>10^{19}$ eV). The ground array of the Observatory will consist of 1600 water Cherenkov detectors deployed over 3000 km^2. The remoteness and large…

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…

天体物理学 · 物理学 2019-08-15 Miguel Mostafa

The Southern part of the Pierre Auger Observatory is nearing completion, and has been in stable operation since January 2004 while it has grown in size. The large sample of data collected so far has led to a significant improvement in the…

天体物理学 · 物理学 2019-08-13 T. Yamamoto

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…

高能天体物理现象 · 物理学 2025-09-16 Fabio Convenga

The Pierre Auger Observatory is the world's largest operating detection system for the observation of ultra high energy cosmic rays (UHECRs). The detector allows detailed measurements of their energy spectrum, mass composition and arrival…

天体物理仪器与方法 · 物理学 2018-11-27 Dariusz Gora

A key feature of the Pierre Auger Observatory is its hybrid design, in which ultra high energy cosmic rays are detected simultaneously by fluorescence telescopes and a ground array. The two techniques see air showers in complementary ways,…

天体物理学 · 物理学 2019-08-13 B. R. Dawson

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…

天体物理仪器与方法 · 物理学 2014-07-03 Pierre Auger Collaboration

The Pierre Auger Observatory, the world's largest observatory of ultra-high-energy cosmic rays (UHECR), offers a unique insight into the properties of hadronic interactions occurring in air showers at energies well above those reached at…

高能天体物理现象 · 物理学 2024-12-05 Jan Ebr

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…

高能天体物理现象 · 物理学 2020-12-25 Joao de Mello Neto

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…

The Pierre Auger Observatory has begun a major Upgrade of its already impressive capabilities, with an emphasis on improved mass composition determination using the surface detectors of the Observatory. Known as AugerPrime, the upgrade will…

天体物理仪器与方法 · 物理学 2016-04-14 The Pierre Auger Collaboration , A. Aab , P. Abreu , M. Aglietta , E. J. Ahn , I. Al Samarai , I. F. M. Albuquerque , I. Allekotte , P. Allison , A. Almela , J. Alvarez Castillo , J. Alvarez-Muñiz , R. Alves Batista , M. Ambrosio , A. Aminaei , L. Anchordoqui , S. Andringa , C. Aramo , F. Arqueros , N. Arsene , H. Asorey , P. Assis , J. Aublin , M. Ave , M. Avenier , G. Avila , N. Awal , A. M. Badescu , K. B. Barber , J. Bäuml , C. Baus , J. J. Beatty , K. H. Becker , J. A. Bellido , C. Berat , M. E. Bertaina , X. Bertou , P. L. Biermann , P. Billoir , S. G. Blaess , A. Blanco , M. Blanco , J. Blazek , C. Bleve , H. Blümer , M. Boháčová , D. Boncioli , C. Bonifazi , N. Borodai , J. Brack , I. Brancus , A. Bridgeman , P. Brogueira , W. C. Brown , P. Buchholz , A. Bueno , S. Buitink , M. Buscemi , K. S. Caballero-Mora , B. Caccianiga , L. Caccianiga , M. Candusso , L. Caramete , R. Caruso , A. Castellina , G. Cataldi , L. Cazon , R. Cester , A. G. Chavez , A. Chiavassa , J. A. Chinellato , J. Chudoba , M. Cilmo , R. W. Clay , G. Cocciolo , R. Colalillo , A. Coleman , L. Collica , M. R. Coluccia , R. Conceição , F. Contreras , M. J. Cooper , A. Cordier , S. Coutu , C. E. Covault , J. Cronin , R. Dallier , B. Daniel , S. Dasso , K. Daumiller , B. R. Dawson , R. M. de Almeida , S. J. de Jong , G. De Mauro , J. R. T. de Mello Neto , I. De Mitri , J. de Oliveira , V. de Souza , L. del Peral , O. Deligny , H. Dembinski , N. Dhital , C. Di Giulio , A. Di Matteo , J. C. Diaz , M. L. Díaz Castro , F. Diogo , C. Dobrigkeit , W. Docters , J. C. D'Olivo , A. Dorofeev , Q. Dorosti Hasankiadeh , M. T. Dova , J. Ebr , R. Engel , M. Erdmann , M. Erfani , C. O. Escobar , J. Espadanal , A. Etchegoyen , H. Falcke , K. Fang , G. Farrar , A. C. Fauth , N. Fazzini , A. P. Ferguson , M. Fernandes , B. Fick , J. M. Figueira , A. Filevich , A. Filipčič , B. D. Fox , O. Fratu , M. M. Freire , B. Fuchs , T. Fujii , B. García , D. Garcia-Pinto , F. Gate , H. Gemmeke , A. Gherghel-Lascu , P. L. Ghia , U. Giaccari , M. Giammarchi , M. Giller , D. Głas , C. Glaser , H. Glass , G. Golup , M. Gómez Berisso , P. F. Gómez Vitale , N. González , B. Gookin , J. Gordon , A. Gorgi , P. Gorham , P. Gouffon , N. Griffith , A. F. Grillo , T. D. Grubb , F. Guarino , G. P. Guedes , M. R. Hampel , P. Hansen , D. Harari , T. A. Harrison , S. Hartmann , J. L. Harton , A. Haungs , T. Hebbeker , D. Heck , P. Heimann , N. Hemery , A. E. Herve , G. C. Hill , C. Hojvat , N. Hollon , E. Holt , P. Homola , J. R. Hörandel , P. Horvath , M. Hrabovský , D. Huber , T. Huege , A. Insolia , P. G. Isar , I. Jandt , S. Jansen , C. Jarne , J. A. Johnsen , M. Josebachuili , A. Kääpä , O. Kambeitz , K. H. Kampert , P. Kasper , I. Katkov , B. Kégl , B. Keilhauer , A. Keivani , E. Kemp , R. M. Kieckhafer , H. O. Klages , M. Kleifges , J. Kleinfeller , R. Krause , N. Krohm , O. Krömer , D. Kuempel , G. Kukec Mezek , N. Kunka , D. LaHurd , L. Latronico , R. Lauer , M. Lauscher , P. Lautridou , S. Le Coz , D. Lebrun , P. Lebrun , M. A. Leigui de Oliveira , A. Letessier-Selvon , I. Lhenry-Yvon , K. Link , L. Lopes , R. López , A. López Casado , K. Louedec , L. Lu , A. Lucero , M. Malacari , S. Maldera , M. Mallamaci , J. Maller , D. Mandat , P. Mantsch , A. G. Mariazzi , V. Marin , I. C. Mariş , G. Marsella , D. Martello , L. Martin , H. Martinez , O. Martínez Bravo , D. Martraire , J. J. Masías Meza , H. J. Mathes , S. Mathys , J. Matthews , J. A. J. Matthews , G. Matthiae , D. Maurizio , E. Mayotte , P. O. Mazur , C. Medina , G. Medina-Tanco , R. Meissner , V. B. B. Mello , D. Melo , A. Menshikov , S. Messina , R. Meyhandan , M. I. Micheletti , L. Middendorf , I. A. Minaya , L. Miramonti , B. Mitrica , L. Molina-Bueno , S. Mollerach , F. Montanet , C. Morello , M. Mostafá , C. A. Moura , M. A. Muller , G. Müller , S. Müller , R. Mussa , G. Navarra , S. Navas , P. Necesal , L. Nellen , A. Nelles , J. Neuser , P. H. Nguyen , M. Niculescu-Oglinzanu , M. Niechciol , L. Niemietz , T. Niggemann , D. Nitz , D. Nosek , V. Novotny , L. Nožka , L. Ochilo , F. Oikonomou , A. Olinto , N. Pacheco , D. Pakk Selmi-Dei , M. Palatka , J. Pallotta , P. Papenbreer , G. Parente , A. Parra , T. Paul , M. Pech , J. Pȩkala , R. Pelayo , I. M. Pepe , L. Perrone , E. Petermann , C. Peters , S. Petrera , Y. Petrov , J. Phuntsok , R. Piegaia , T. Pierog , P. Pieroni , M. Pimenta , V. Pirronello , M. Platino , M. Plum , A. Porcelli , C. Porowski , R. R. Prado , P. Privitera , M. Prouza , V. Purrello , E. J. Quel , S. Querchfeld , S. Quinn , J. Rautenberg , O. Ravel , D. Ravignani , D. Reinert , B. Revenu , J. Ridky , S. Riggi , M. Risse , P. Ristori , V. Rizi , W. Rodrigues de Carvalho , G. Rodriguez Fernandez , J. Rodriguez Rojo , M. D. Rodríguez-Frías , D. Rogozin , J. Rosado , M. Roth , E. Roulet , A. C. Rovero , S. J. Saffi , A. Saftoiu , F. Salamida , H. Salazar , A. Saleh , F. Salesa Greus , G. Salina , F. Sánchez , P. Sanchez-Lucas , E. Santos , E. M. Santos , F. Sarazin , B. Sarkar , R. Sarmento , R. Sato , C. Scarso , M. Schauer , V. Scherini , H. Schieler , D. Schmidt , O. Scholten , H. Schoorlemmer , P. Schovánek , F. G. Schröder , A. Schulz , J. Schulz , J. Schumacher , S. J. Sciutto , A. Segreto , M. Settimo , A. Shadkam , R. C. Shellard , I. Sidelnik , G. Sigl , O. Sima , A. Śmiałkowski , R. Šmída , G. R. Snow , P. Sommers , J. Sorokin , R. Squartini , Y. N. Srivastava , D. Stanca , S. Stanič , J. Stapleton , J. Stasielak , M. Stephan , A. Stutz , F. Suarez , T. Suomijärvi , A. D. Supanitsky , M. S. Sutherland , J. Swain , Z. Szadkowski , O. A. Taborda , A. Tapia , A. Tepe , V. M. Theodoro , C. Timmermans , C. J. Todero Peixoto , G. Toma , L. Tomankova , B. Tomé , A. Tonachini , G. Torralba Elipe , D. Torres Machado , P. Travnicek , M. Trini , R. Ulrich , M. Unger , M. Urban , J. F. Valdés Galicia , I. Valiño , L. Valore , G. van Aar , P. van Bodegom , A. M. van den Berg , S. van Velzen , A. van Vliet , E. Varela , B. Vargas Cárdenas , G. Varner , R. Vasquez , J. R. Vázquez , R. A. Vázquez , D. Veberič , V. Verzi , J. Vicha , M. Videla , L. Villaseñor , B. Vlcek , S. Vorobiov , H. Wahlberg , O. Wainberg , D. Walz , A. A. Watson , M. Weber , K. Weidenhaupt , A. Weindl , F. Werner , A. Widom , L. Wiencke , H. Wilczyński , T. Winchen , D. Wittkowski , B. Wundheiler , S. Wykes , L. Yang , T. Yapici , A. Yushkov , E. Zas , D. Zavrtanik , M. Zavrtanik , A. Zepeda , Y. Zhu , B. Zimmermann , M. Ziolkowski , Z. Zong , F. Zuccarello

The Pierre Auger Observatory is the world's largest detector of ultra--high energy cosmic rays (UHECRs). It uses an array of fluorescence telescopes and particle detectors at the ground to obtain detailed measurements of the energy…

高能天体物理现象 · 物理学 2022-02-02 Dariusz Gora

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…

天体物理仪器与方法 · 物理学 2020-12-10 Sijbrand de Jong

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…

高能天体物理现象 · 物理学 2025-09-08 Pierpaolo Savina

The scale and scope of the physics studied at the Auger Observatory offer significant opportunities for original outreach work. Education, outreach, and public relations of the Auger collaboration are coordinated in a task of its own whose…

天体物理学 · 物理学 2019-08-13 Gregory R. Snow

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…

天体物理仪器与方法 · 物理学 2025-08-12 David Schmidt

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…

天体物理仪器与方法 · 物理学 2019-08-13 K. Louedec

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…

高能天体物理现象 · 物理学 2009-11-25 James W. Cronin