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相关论文: Multi-messenger Astrophysics with the Pierre Auger…

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An overview of the multi-messenger capabilities of the Pierre Auger Observatory is presented. The techniques and performance of searching for Ultra-High Energy neutrinos, photons and neutrons are described. Some of the most relevant results…

高能天体物理现象 · 物理学 2019-04-29 The Pierre Auger Collaboration , A. Aab , P. Abreu , M. Aglietta , I. F. M. Albuquerque , J. M. Albury , I. Allekotte , A. Almela , J. Alvarez Castillo , J. Alvarez-Muñiz , G. A. Anastasi , L. Anchordoqui , B. Andrada , S. Andringa , C. Aramo , H. Asorey , P. Assis , G. Avila , A. M. Badescu , A. Bakalova , A. Balaceanu , F. Barbato , R. J. Barreira Luz , S. Baur , K. H. Becker , J. A. Bellido , C. Berat , M. E. Bertaina , X. Bertou , P. L. Biermann , J. Biteau , S. G. Blaess , A. Blanco , J. Blazek , C. Bleve , M. Boháčová , D. Boncioli , C. Bonifazi , N. Borodai , A. M. Botti , J. Brack , T. Bretz , A. Bridgeman , F. L. Briechle , P. Buchholz , A. Bueno , S. Buitink , M. Buscemi , K. S. Caballero-Mora , L. Caccianiga , L. Calcagni , A. Cancio , F. Canfora , J. M. Carceller , R. Caruso , A. Castellina , F. Catalani , G. Cataldi , L. Cazon , M. Cerda , J. A. Chinellato , J. Chudoba , L. Chytka , R. W. Clay , A. C. Cobos Cerutti , R. Colalillo , A. Coleman , M. R. Coluccia , R. Conceição , A. Condorelli , G. Consolati , F. Contreras , F. Convenga , M. J. Cooper , S. Coutu , C. E. Covault , B. Daniel , S. Dasso , K. Daumiller , B. R. Dawson , J. A. Day , R. M. de Almeida , S. J. de Jong , G. De Mauro , J. R. T. de Mello Neto , I. De Mitri , J. de Oliveira , F. O. de Oliveira Salles , V. de Souza , J. Debatin , M. del Río , O. Deligny , N. Dhital , M. L. Díaz Castro , F. Diogo , C. Dobrigkeit , J. C. D'Olivo , Q. Dorosti , R. C. dos Anjos , M. T. Dova , A. Dundovic , J. Ebr , R. Engel , M. Erdmann , C. O. Escobar , A. Etchegoyen , H. Falcke , J. Farmer , G. Farrar , A. C. Fauth , N. Fazzini , F. Feldbusch , F. Fenu , L. P. Ferreyro , J. M. Figueira , A. Filipčič , M. M. Freire , T. Fujii , A. Fuster , B. García , H. Gemmeke , A. Gherghel-Lascu , P. L. Ghia , U. Giaccari , M. Giammarchi , M. Giller , D. Głas , J. Glombitza , F. Gobbi , G. Golup , M. Gómez Berisso , P. F. Gómez Vitale , J. P. Gongora , N. González , I. Goos , D. Góra , A. Gorgi , M. Gottowik , T. D. Grubb , F. Guarino , G. P. Guedes , E. Guido , R. Halliday , M. R. Hampel , P. Hansen , D. Harari , T. A. Harrison , V. M. Harvey , A. Haungs , T. Hebbeker , D. Heck , P. Heimann , G. C. Hill , C. Hojvat , E. M. Holt , P. Homola , J. R. Hörandel , P. Horvath , M. Hrabovský , T. Huege , J. Hulsman , A. Insolia , P. G. Isar , I. Jandt , J. A. Johnsen , M. Josebachuili , J. Jurysek , A. Kääpä , K. H. Kampert , B. Keilhauer , N. Kemmerich , J. Kemp , H. O. Klages , M. Kleifges , J. Kleinfeller , R. Krause , D. Kuempel , G. Kukec Mezek , A. Kuotb Awad , B. L. Lago , D. LaHurd , R. G. Lang , R. Legumina , M. A. Leigui de Oliveira , V. Lenok , A. Letessier-Selvon , I. Lhenry-Yvon , O. C. Lippmann , D. Lo Presti , L. Lopes , R. López , A. López Casado , R. Lorek , Q. Luce , A. Lucero , M. Malacari , G. Mancarella , D. Mandat , B. C. Manning , P. Mantsch , A. G. Mariazzi , I. C. Mariş , G. Marsella , D. Martello , H. Martinez , O. Martínez Bravo , M. Mastrodicasa , H. J. Mathes , S. Mathys , J. Matthews , G. Matthiae , E. Mayotte , P. O. Mazur , G. Medina-Tanco , D. Melo , A. Menshikov , K. -D. Merenda , S. Michal , M. I. Micheletti , L. Middendorf , L. Miramonti , B. Mitrica , D. Mockler , S. Mollerach , F. Montanet , C. Morello , G. Morlino , M. Mostafá , A. L. Müller , M. A. Muller , S. Müller , R. Mussa , L. Nellen , P. H. Nguyen , M. Niculescu-Oglinzanu , M. Niechciol , D. Nitz , D. Nosek , V. Novotny , L. Nožka , A Nucita , L. A. Núñez , F. Oikonomou , A. Olinto , M. Palatka , J. Pallotta , M. P. Panetta , P. Papenbreer , G. Parente , A. Parra , M. Pech , F. Pedreira , J. Pękala , R. Pelayo , J. Peña-Rodriguez , L. A. S. Pereira , M. Perlin , L. Perrone , C. Peters , S. Petrera , J. Phuntsok , T. Pierog , M. Pimenta , V. Pirronello , M. Platino , J. Poh , B. Pont , C. Porowski , R. R. Prado , P. Privitera , M. Prouza , A. Puyleart , S. Querchfeld , S. Quinn , R. Ramos-Pollan , J. Rautenberg , D. Ravignani , M. Reininghaus , J. Ridky , F. Riehn , M. Risse , P. Ristori , V. Rizi , W. Rodrigues de Carvalho , J. Rodriguez Rojo , M. J. Roncoroni , M. Roth , E. Roulet , A. C. Rovero , P. Ruehl , S. J. Saffi , A. Saftoiu , F. Salamida , H. Salazar , G. Salina , J. D. Sanabria Gomez , F. Sánchez , E. M. Santos , E. Santos , F. Sarazin , R. Sarmento , C. Sarmiento-Cano , R. Sato , P. Savina , M. Schauer , V. Scherini , H. Schieler , M. Schimassek , M. Schimp , F. Schlüter , D. Schmidt , O. Scholten , P. Schovánek , F. G. Schröder , S. Schröder , J. Schumacher , S. J. Sciutto , M. Scornavacche , R. C. Shellard , G. Sigl , G. Silli , O. Sima , R. Šmída , G. R. Snow , P. Sommers , J. F. Soriano , J. Souchard , R. Squartini , D. Stanca , S. Stanič , J. Stasielak , P. Stassi , M. Stolpovskiy , A. Streich , F. Suarez , M. Suárez-Durán , T. Sudholz , T. Suomijärvi , A. D. Supanitsky , J. Šupík , Z. Szadkowski , A. Taboada , O. A. Taborda , A. Tapia , C. Timmermans , C. J. Todero Peixoto , B. Tomé , G. Torralba Elipe , A. Travaini , P. Travnicek , M. Trini , M. Tueros , R. Ulrich , M. Unger , M. Urban , J. F. Valdés Galicia , I. Valiño , L. Valore , P. van Bodegom , A. M. van den Berg , A. van Vliet , E. Varela , B. Vargas Cárdenas , D. Veberič , C. Ventura , I. D. Vergara Quispe , V. Verzi , J. Vicha , L. Villaseñor , J. Vink , S. Vorobiov , H. Wahlberg , A. A. Watson , M. Weber , A. Weindl , M. Wiedeński , L. Wiencke , H. Wilczyński , T. Winchen , M. Wirtz , D. Wittkowski , B. Wundheiler , L. Yang , A. Yushkov , E. Zas , D. Zavrtanik , M. Zavrtanik , L. Zehrer , A. Zepeda , B. Zimmermann , M. Ziolkowski , Z. Zong , F. Zuccarello

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,…

高能天体物理现象 · 物理学 2021-02-02 Lukas Zehrer

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…

天体物理学 · 物理学 2019-08-13 Veronique Van Elewyck

The Pierre Auger Observatory is the largest astroparticle experiment in operation. Complementary to the measurements of the charged ultra-high energy (UHE) cosmic rays, it provides a very good sensitivity to the detection of UHE photons and…

高能天体物理现象 · 物理学 2022-12-15 Nicolás Martín González

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 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

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

Astroparticles offer a new path for research in the field of particle physics, allowing investigations at energies above those accesible with accelerators. Ultra-high energy cosmic rays can be studied via the observation of the showers they…

高能天体物理现象 · 物理学 2019-08-21 Analisa Mariazzi

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

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

The Pierre Auger Observatory stands as the largest detector for ultra-high-energy (UHE) cosmic rays. The Observatory is also sensitive to UHE photons and neutrinos that can be produced along with UHE cosmic rays or in top-down processes,…

高能天体物理现象 · 物理学 2025-01-08 Nicolas M. Gonzalez

Data taken at the Pierre Auger Observatory are used to search for air showers initiated by ultra-high energy (UHE) photons. Results of searches are reported from hybrid observations where events are measured with both fluorescence and array…

天体物理学 · 物理学 2019-08-13 M. D. Healy

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…

高能天体物理现象 · 物理学 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…

高能物理 - 实验 · 物理学 2019-08-17 S. Andringa

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 scientific achievements of the Pierre Auger Collaboration cover diverse and complementary fields of research. The search for the origin of ultra-high energy cosmic rays (UHECRs) is based on the measurement of the energy spectrum and…

高能天体物理现象 · 物理学 2022-12-02 Antonella Castellina

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

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 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…

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