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Related papers: The ANTARES Neutrino Telescope

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Large underwater telescopes have been proposed as a challenging method to measure high energy neutrinos from astrophysical objects. In recent years, The Antares collaboration has designed and realized the first detector of this type in the…

Instrumentation and Methods for Astrophysics · Physics 2026-05-21 K. Gracheva , M. Anghinolfi , V. Kulikovskiy , E. Shirokov , Y. Yakovenko

The ANTARES experiment is currently the largest underwater neutrino telescope in the Northern Hemisphere. It is taking high quality data since 2007. Its main scientific goal is to search for high energy neutrinos that are expected from the…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Salvatore Mangano

The observation of high energy extraterrestrial neutrinos can be an invaluable source of information about the most energetic phenomena in the Universe. Neutrinos can shed light on the processes that accelerate charge particles in an…

High Energy Astrophysical Phenomena · Physics 2019-08-15 Juan José Hernández-Rey

ANTARES is the first undersea neutrino detector ever built and presently the neutrino telescope with the largest effective area operating in the Northern Hemisphere. A three- dimensional array of photomultiplier tubes detects the Cherenkov…

High Energy Astrophysical Phenomena · Physics 2015-06-04 Ciro Bigongiari

The ANTARES collaboration completed the installation of the first neutrino detector in the sea in 2008. It consists of a three dimensional array of 885 photomultipliers to gather the Cherenkov photons induced by relativistic muons produced…

High Energy Physics - Experiment · Physics 2012-10-11 Juan de Dios Zornoza , Juan Zúñiga

The ANTARES project aims to build a deep underwater Cherenkov neutrino telescope in the Mediterranean Sea. Currently the experiment is in the construction phase and has recently achieved two important milestones. The electro-optical cable…

Astrophysics · Physics 2019-08-14 I. Sokalski

The ANTARES experiment is currently the largest underwater neutrino telescope. It is taking high quality data since 2007 and aims to detect high energy neutrinos that are expected from the acceleration of cosmic rays from astrophysical…

High Energy Astrophysical Phenomena · Physics 2019-08-13 S. Mangano

The ANTARES collaboration is building a deep sea neutrino telescope in the Mediterranean Sea. This detector will cover a sensitive area of typically 0.1 km-squared and will be equipped with about 1000 optical modules. Each of these optical…

Astrophysics · Physics 2012-08-27 The ANTARES Collaboration

In this paper, we illustrate the main features of the electronics and data acquisition systems of the ANTARES apparatus, a large volume, deep-sea neutrino telescope under construction in the Mediterranean Sea off the coast of Toulon,…

Astrophysics · Physics 2019-08-13 M. Circella

The ANTARES high energy neutrino telescope is a three-dimensional array of about 900 photomultipliers distributed over 12 mooring lines installed in the Mediterranean Sea. Between February and November 2007 it acquired data in a 5-line…

High Energy Astrophysical Phenomena · Physics 2012-08-27 ANTARES Collaboration

The ANTARES detector, completed in 2008, is the largest neutrino telescope in the Northern hemisphere. Located at a depth of 2.5 km in the Mediterranean Sea, 40 km off the Toulon shore, its main goal is the search for astrophysical high…

High Energy Astrophysical Phenomena · Physics 2015-11-11 The ANTARES Collaboration

The ANTARES neutrino telescope is a large photomultiplier array designed to detect neutrino-induced upward-going muons by their Cherenkov radiation. Understanding the absorption and scattering of light in the deep Mediterranean is…

Astrophysics · Physics 2012-08-27 ANTARES collaboration

Several projects are concentrating their efforts on opening the high energy neutrino window on the Universe with km-scale detectors. The detection principle relies on the observation, using photomultipliers, of the Cherenkov light emitted…

High Energy Astrophysical Phenomena · Physics 2009-12-08 Antoine Kouchner

The ANTARES neutrino telescope is presently being built in the Mediterranean Sea at a depth of 2500 m. The primary aim of the experiment is the detection of high energy cosmic muon neutrinos, which are identified by the muons that are…

Astrophysics · Physics 2019-08-13 S. Mangano

The ANTARES neutrino telescope is currently being constructed in the Mediterranean Sea. The complete detector will consist of 12 strings, supplemented by an additional instrumentation line. Nine strings are at present deployed of which five…

Astrophysics · Physics 2019-08-13 Felix Fehr

In May 2008, the Antares neutrino telescope was completed at 2.5 km depth in the Mediterranean Sea; data taking has been going on since. A prerequisite for neutrino astronomy is an accurate reconstruction of the neutrino events, as well as…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 Aart Heijboer

A new method for the measurement of the muon flux in the deep-sea ANTARES neutrino telescope and its dependence on the depth is presented. The method is based on the observation of coincidence signals in adjacent storeys of the detector.…

High Energy Astrophysical Phenomena · Physics 2012-08-27 ANTARES collaboration

The ANTARES Neutrino Telescope was completed in May 2008 and is the first operational Neutrino Telescope in the Mediterranean Sea. The main purpose of the detector is to perform neutrino astronomy and the apparatus also offers facilities…

Instrumentation and Methods for Astrophysics · Physics 2015-05-27 ANTARES Collaboration

The ANTARES deep-sea neutrino telescope comprises a three-dimensional array of photomultipliers to detect the Cherenkov light induced by upgoing relativistic charged particles originating from neutrino interactions in the vicinity of the…

Instrumentation and Methods for Astrophysics · Physics 2011-02-18 The ANTARES Collaboration , J. A. Aguilar , I. Al Samarai , A. Albert , M. André , M. Anghinolfi , G. Anton , S. Anvar , M. Ardid , A. C. Assis Jesus , T. Astraatmadja , J. J. Aubert , R. Auer , B. Baret , S. Basa , M. Bazzotti , V. Bertin , S. Biagi , C. Bigongiari , M. Bou-Cabo , M. C. Bouwhuis , A. M. Brown , J. Brunner , J. Busto , F. Camarena , A. Capone , C. Carloganu , G. Carminati , J. Carr , S. Cecchini , Ph. Charvis , T. Chiarusi , M. Circella , H. Costantini , N. Cottini , P. Coyle , C. Curtil , M. P. Decowski , I. Dekeyser , A. Deschamps , C. Distefano , C. Donzaud , D. Dornic , D. Drouhin , T. Eberl , U. Emanuele , J. P. Ernenwein , S. Escoffier , F. Fehr , V. Flaminio , U. Fritsch , J. L. Fuda , S. Galata , P. Gay , G. Giacomelli , J. P. Gómez-González , K. Graf , G. Guillard , G. Halladjian , G. Hallewell , H. van Haren , A. J. Heijboer , Y. Hello , J. J. Hernández-Rey , B. Herold , J. Hössl , C. C. Hsu , M. de Jong , M. Kadler , N. Kalantar-Nayestanaki , O. Kalekin , A. Kappes , U. Katz , P. Kooijman , C. Kopper , A. Kouchner , V. Kulikovskiy , R. Lahmann , P. Lamare , G. Larosa , D. Lefèvre , G. Lim , D. Lo Presti , H. Loehner , S. Loucatos , F. Lucarelli , S. Mangano , M. Marcelin , A. Margiotta , J. A. Martinez-Mora , A. Mazure , T. Montaruli , M. Morganti , L. Moscoso , H. Motz , C. Naumann , M. Neff , D. Palioselitis , G. E. Pavalas , P. Payre , J. Petrovic , P. Piattelli , N. Picot-Clemente , C. Picq , V. Popa , T. Pradier , E. Presani , C. Racca , C. Reed , G. Riccobene , C. Richardt , M. Rujoiu , G. V. Russo , F. Salesa , P. Sapienza , F. Schöck , J. P. Schuller , R. Shanidze , F. Simeone , A. Spies , M. Spurio , J. J. M. Steijger , Th. Stolarczyk , M. Taiuti , C. Tamburini , L. Tasca , S. Toscano , B. Vallage , V. Van Elewyck , G. Vannoni , M. Vecchi , P. Vernin , G. Wijnker , E. de Wolf , H. Yepes , D. Zaborov , J. D. Zornoza , J. Zúñiga

Interest for studying cosmic neutrinos using deep-sea detectors has increase after the discovery of a diffuse flux of cosmic neutrinos by the IceCube collaboration and the possibility of wider multi-messenger studies with the observations…

High Energy Physics - Experiment · Physics 2025-05-13 A. Albert , S. Alves , M. André , M. Ardid , S. Ardid , J. -J. Aubert , J. Aublin , B. Baret , S. Basa , Y. Becherini , B. Belhorma , F. Benfenati , V. Bertin , S. Biagi , J. Boumaaza , M. Bouta , M. C. Bouwhuis , H. Branzas , R. Bruijn , J. Brunner , J. Busto , B. Caiffi , D. Calvo , S. Campion , A. Capone , F. Carenini , J. Carr , V. Carretero , T. Cartraud , S. Celli , L. Cerisy , M. Chabab , R. Cherkaoui El Moursli , T. Chiarusi , M. Circella , J. A. B. Coelho , A. Coleiro , R. Coniglione , P. Coyle , A. Creusot , A. F. Dìaz , B. De Martino , I. Del Rosso , C. Distefano , I. Di Palma , C. Donzaud , D. Dornic , D. Drouhin , T. Eberl , A. Eddymaoui , T. van Eeden , D. van Eijk , S. El Hedri , N. El Khayati , A. Enzenhöfer , P. Fermani , G. Ferrara , F. Filippini , L. Fusco , S. Gagliardini , J. Garcìa-Méndez , C. Gatius Oliver , P. Gay , N. Geisselbrecht , H. Glotin , R. Gozzini , R. Gracia Ruiz , K. Graf , C. Guidi , L. Haegel , H. van Haren , A. J. Heijboer , Y. Hello , L. Hennig , J. J. Hernàndez-Rey , J. Hössl , F. Huang , G. Illuminati , B. Jisse-Jung , M. de Jong , P. de Jong , M. Kadler , O. Kalekin , U. Katz , A. Kouchner , I. Kreykenbohm , V. Kulikovskiy , R. Lahmann , M. Lamoureux , A. Lazo , D. Lefèvre , E. Leonora , G. Levi , S. Le Stum , S. Loucatos , J. Manczak , M. Marcelin , A. Margiotta , A. Marinelli , J. A. Martìnez-Mora , P. Migliozzi , A. Moussa , R. Muller , S. Navas , E. Nezri , B. 'O Fearraigh , E. Oukacha , A. M. Paun , G. E. Pavalas , S. Pena-Martìnez , M. Perrin-Terrin , P. Piattelli , C. Poirè , V. Popa , T. Pradier , N. Randazzo , D. Real , G. Riccobene , A. Romanov , A. Sànchez Losa , A. Saina , F. Salesa Greus , D. F. E. Samtleben , M. Sanguineti , P. Sapienza , F. Schüssler , J. Seneca , M. Spurio , Th. Stolarczyk , M. Taiuti , Y. Tayalati , B. Vallage , G. Vannoye , V. Van Elewyck , S. Viola , D. Vivolo , J. Wilms , S. Zavatarelli , A. Zegarelli , J. D. Zornoza , J. Zúniga