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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

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 has by now achieved an exposure of order $10^5~{\rm km}^2$ sr yr, exploring about 85% of the sky. In this talk, I will review some of the recent results, including the detailed measurements of the features in…

High Energy Astrophysical Phenomena · Physics 2021-10-11 Esteban Roulet

I describe some of the results on ultrahigh-energy cosmic rays that have been obtained with the Pierre Auger Observatory. These include measurements of the spectrum, composition and anisotropies. Possible astrophysical scenarios that…

High Energy Astrophysical Phenomena · Physics 2019-06-12 Esteban Roulet

Recent results obtained with the Pierre Auger Observatory are described. These include measurements of the spectrum, anisotropies and composition of ultra-high energy cosmic rays. The ankle of the spectrum is measured at $4\times…

High Energy Astrophysical Phenomena · Physics 2015-03-17 Esteban Roulet

We review in these notes the status of the construction of the Pierre Auger Observatory and present the first Physics results, based on the data collected during the first year and a half of operation. These results are preliminary, once…

Astrophysics · Physics 2015-06-24 R. C. Shellard

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 Southern Pierre Auger Observatory is now nearing completion and the accumulating data sample has already allowed to extract scientific results of relevance for ultra-high energy cosmic-ray (UHECR) physics. This lecture focuses on the…

Astrophysics · Physics 2019-08-14 V. Van Elewyck

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 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 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

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

We report on studies of the composition of ultra high energy cosmic rays with the Pierre Auger Observatory. The detection of longitudinal air shower profiles with the fluorescence detector is described and the measurement of the average…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Michael Unger

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 aims to determine the nature and origin of the ultra-high energy cosmic rays (UHECR). The Auger hybrid detector combines fluorescence observations of extended air showers, initiated in the atmosphere by these…

Astrophysics · Physics 2007-05-23 Serguei Vorobiov

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…

Astrophysics · Physics 2019-08-13 T. Yamamoto

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 goal of the Pierre Auger Observatory is to determine the still unknown nature and origin of ultra-high energy cosmic rays. The study of these elusive particles probes astrophysical sites of particle acceleration as well as fundamental…

Astrophysics · Physics 2007-05-23 Andreas Zech

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
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