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相关论文: Highlights from the Pierre Auger Observatory (ICRC…

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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

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 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…

高能天体物理现象 · 物理学 2023-03-01 Olivier Deligny

Ultra-high energy cosmic rays (UHECRs) are particles, likely protons and/or nuclei, with energies up to $10^{20}$ eV that are observed through the giant air showers they produce in the atmosphere. These particles carry the information on…

高能天体物理现象 · 物理学 2017-02-24 O. Deligny , K. Kawata , P. Tinyakov

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…

高能天体物理现象 · 物理学 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…

高能天体物理现象 · 物理学 2019-08-17 L. Cazon

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…

高能天体物理现象 · 物理学 2023-09-06 Olivier Deligny

In this contribution we summarize the highlights from the Pierre Auger Observatory presented at the 35th International Cosmic Ray Conference. We discuss the update of the measurement of the energy spectrum of cosmic rays over a wide range…

高能天体物理现象 · 物理学 2018-11-02 Michael Unger

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 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…

天体物理学 · 物理学 2007-05-23 Serguei Vorobiov

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 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

The Pierre Auger Observatory has driven the field of ultra-high-energy cosmic ray (UHECR) physics, producing several groundbreaking observations over the last 20 years. One of the most striking findings has been the complex evolution of…

高能天体物理现象 · 物理学 2025-07-22 Eric Mayotte

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…

高能天体物理现象 · 物理学 2022-05-04 Jaroslaw Stasielak

Ultra-High Energy Cosmic Rays (UHECRs) are charged particles of energies above $10^{18}$ eV that originate outside of the Galaxy. Because the flux of the UHECRs at Earth is very small, the only practical way of observing UHECRs is by…

高能天体物理现象 · 物理学 2017-05-26 Valerio Verzi , Dmitri Ivanov , Yoshiki Tsunesada

The energy spectrum of ultra-high energy cosmic rays (UHECRs) provides essential information on the most energetic phenomena in the Universe. Beyond EeV energies, the Telescope Array and Pierre Auger Observatory have the largest exposures…

高能天体物理现象 · 物理学 2020-01-27 O. Deligny

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…

高能天体物理现象 · 物理学 2019-08-13 R. Conceição

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

高能天体物理现象 · 物理学 2016-06-22 João 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…

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

In its Phase I, the Pierre Auger Observatory has led to several observations, driving the field of ultra-high-energy cosmic ray (UHECR) research over the last 20 years. Major achievements obtained so far include the unprecedented precise…

高能天体物理现象 · 物理学 2025-09-22 Denise Boncioli
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