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High energy neutrinos produced in astrophysical processes will allow for a new way of studying the universe. In order to detect the expected flux of high energy neutrinos from specific astrophysical sources, neutrino telescopes of a scale…

Astrophysics · Physics 2019-08-14 P. A. Rapidis

The observation of high-energy extraterrestrial neutrinos is one of the most promising future options to increase our knowledge on non-thermal processes in the universe. Neutrinos are e.g. unavoidably produced in environments where…

Astrophysics · Physics 2009-11-11 Ulrich F. Katz

To complement the IceCube neutrino telescope currently under construction at the South Pole, the three Mediterranean neutrino telescope projects ANTARES, NEMO and NESTOR have joined forces to develop, construct and operate a km^3-scale…

Astrophysics · Physics 2019-08-14 A. Kappes

Theoretical predictions for neutrino fluxes indicate that km$^{3}$ scale detectors are needed to detect certain astrophysical sources. The three Mediterranean experiments, ANTARES, NEMO and NESTOR are working together on a design study,…

Astrophysics · Physics 2019-08-14 J. Carr , D. Dornic , F. Jouvenot , G. Maurin

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

KM3NeT is a deep-sea research infrastructure being constructed in the Mediterranean Sea. It will host the next generation Cherenkov neutrino telescope and nodes for a deep sea multidisciplinary observatory, providing oceanographers, marine…

Instrumentation and Methods for Astrophysics · Physics 2014-08-08 Annarita Margiotta

The high energy neutrino detection by a km^3 Neutrino Telescope placed in the Mediterranean sea provides a unique tool to both determine the diffuse astrophysical neutrino flux and the neutrino-nucleon cross section in the extreme…

Astrophysics · Physics 2007-09-24 E. Borriello , A. Cuoco , G. Mangano , G. Miele , S. Pastor , O. Pisanti , P. D. Serpico

The KM3NeT/ARCA high energy neutrino telescope is currently under construction in the Mediterranean sea. The detector will consist of two blocks of instrumented structures and will have a size of the order of a cubic-kilometer. In this work…

Instrumentation and Methods for Astrophysics · Physics 2017-01-23 R. Coniglione

The observation of high-energy neutrinos from astrophysical sources would substantially improve our knowledge and understanding of the non-thermal processes in these sources, and would in particular pinpoint the accelerators of cosmic rays.…

Astrophysics · Physics 2019-08-14 J. Carr , D. Dornic , F. Jouvenot , U. F. Katz , S. Kuch , G. Maurin , R. Shanidze

We perform a study of the ultra high energy neutrino detection performances of a km^3 Neutrino Telescope sitting at the three proposed sites for ANTARES, NEMO and NESTOR in the Mediterranean sea. We focus on the effect of the underwater…

Astrophysics · Physics 2010-10-27 A. Cuoco , G. Mangano , G. Miele , S. Pastor , L. Perrone , O. Pisanti , P. D. Serpico

KM3NeT is a future research infrastructure in the Mediterranean Sea, hosting a multi-cubic-kilometre neutrino telescope and nodes for Earth and Sea sciences. In this report we shortly summarise the genesis of the KM3NeT project and present…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Ulrich F. Katz

Neutrino astronomy has entered an exciting time with the completion of the first km3-scale neutrino telescope at the South Pole (IceCube) and the successful operation of the first under-sea neutrino telescope in the Mediterranean (Antares).…

High Energy Astrophysical Phenomena · Physics 2012-09-18 V. Van Elewyck

KM3NeT is a new generation neutrino telescope currently under construction at two sites in the Mediterranean Sea. At the Capo Passero site, 100 km off-shore Sicily, Italy, a volume of more than one cubic kilometre of water will be…

High Energy Physics - Experiment · Physics 2018-07-01 Dmitry Zaborov

Neutrino astrophysics offers new perspectives on the Universe investigation: high energy neutrinos, produced by the most energetic phenomena in our Galaxy and in the Universe, carry complementary (if not exclusive) information about the…

High Energy Astrophysical Phenomena · Physics 2010-02-11 T. Chiarusi , M. Spurio

The identification of cosmic objects emitting high energy neutrinos could provide new insights about the Universe and its active sources. The existence of these cosmic neutrinos has been proven by the IceCube collaboration, but the big…

Instrumentation and Methods for Astrophysics · Physics 2021-09-06 Rasa Muller , Aart Heijboer , Alfonso Garcia Soto , Barbara Caiffi , Matteo Sanguineti , Vladimir Kulikovskiy

Neutrinos are unique cosmic messengers. Present attempts are directed to extend the window of cosmic neutrino observation from low energies (Sun, supernovae) to much higher energies. The aim is to study the most violent processes in the…

High Energy Astrophysical Phenomena · Physics 2015-06-03 Ulrich F. Katz , Christian Spiering

A next-generation neutrino telescope infrastructure, the Kilometer Cube Neutrino Telescope KM3NeT, is currently under construction in the Mediterranean Sea. Its low energy configuration ORCA is optimised for the detection of atmospheric…

High Energy Physics - Experiment · Physics 2022-09-21 Piotr Kalaczyński

The main objectives of the KM3NeT Collaboration are i) the discovery and subsequent observation of high-energy neutrino sources in the Universe and ii) the determination of the mass hierarchy of neutrinos. These objectives are strongly…

Instrumentation and Methods for Astrophysics · Physics 2016-07-27 S. Adrián-Martínez , M. Ageron , F. Aharonian , S. Aiello , A. Albert , F. Ameli , E. Anassontzis , M. Andre , G. Androulakis , M. Anghinolfi , G. Anton , M. Ardid , T. Avgitas , G. Barbarino , E. Barbarito , B. Baret , J. Barrios-Martí , B. Belhorma , A. Belias , E. Berbee , A. van den Berg , V. Bertin , S. Beurthey , V. van Beveren , N. Beverini , S. Biagi , A. Biagioni , M. Billault , M. Bond , R. Bormuth , B. Bouhadef , G. Bourlis , S. Bourret , C. Boutonnet , M. Bouwhuis , C. Bozza , R. Bruijn , J. Brunner , E. Buis , J. Busto , G. Cacopardo , L. Caillat , M. Calamai , D. Calvo , A. Capone , L. Caramete , S. Cecchini , S. Celli , C. Champion , R. Cherkaoui El Moursli , S. Cherubini , T. Chiarusi , M. Circella , L. Classen , R. Cocimano , J. A. B. Coelho , A. Coleiro , S. Colonges , R. Coniglione , M. Cordelli , A. Cosquer , P. Coyle , A. Creusot , G. Cuttone , A. D'Amico , G. De Bonis , G. De Rosa , C. De Sio , F. Di Capua , I. Di Palma , A. F. Díaz García , C. Distefano , C. Donzaud , D. Dornic , Q. Dorosti-Hasankiadeh , E. Drakopoulou , D. Drouhin , L. Drury , M. Durocher , T. Eberl , S. Eichie , D. van Eijk , I. El Bojaddaini , N. El Khayati , D. Elsaesser , A. Enzenhöfer , F. Fassi , P. Favali , P. Fermani , G. Ferrara , G. Frascadore , C. Filippidis , L. A. Fusco , T. Gal , S. Galatà , F. Garufi , P. Gay , M. Gebyehu , V. Giordano , N. Gizani , R. Gracia , K. Graf , T. Grégoire , G. Grella , R. Habel , S. Hallmann , H. van Haren , S. Harissopulos , T. Heid , A. Heijboer , E. Heine , S. Henry , J. J. Hernández-Rey , M. Hevinga , J. Hofestädt , C. M. F. Hugon , G. Illuminati , C. W. James , P. Jansweijer , M. Jongen , M. de Jong , M. Kadler , O. Kalekin , A. Kappes , U. F. Katz , P. Keller , G. Kieft , D. Kießling , E. N. Koffeman , P. Kooijman , A. Kouchner , V. Kulikovskiy , R. Lahmann , P. Lamare , A. Leisos , E. Leonora , M. Lindsey Clark , A. Liolios , C. D. Llorens Alvarez , D. Lo Presti , H. Löhner , A. Lonardo , M. Lotze , S. Loucatos , E. Maccioni , K. Mannheim , A. Margiotta , A. Marinelli , O. Mariş , C. Markou , J. A. Martínez-Mora , A. Martini , R. Mele , K. W. Melis , T. Michael , P. Migliozzi , E. Migneco , P. Mijakowski , A. Miraglia , C. M. Mollo , M. Mongelli , M. Morganti , A. Moussa , P. Musico , M. Musumeci , S. Navas , C. A. Nicolau , I. Olcina , C. Olivetto , A. Orlando , A. Papaikonomou , R. Papaleo , G. E. Păvălaş , H. Peek , C. Pellegrino , C. Perrina , M. Pfutzner , P. Piattelli , K. Pikounis , G. E. Poma , V. Popa , T. Pradier , F. Pratolongo , G. Pühlhofer , S. Pulvirenti , L. Quinn , C. Racca , F. Raffaelli , N. Randazzo , P. Rapidis , P. Razis , D. Real , L. Resvanis , J. Reubelt , G. Riccobene , C. Rossi , A. Rovelli , M. Saldaña , I. Salvadori , D. F. E. Samtleben , A. Sánchez García , A. Sánchez Losa , M. Sanguineti , A. Santangelo , D. Santonocito , P. Sapienza , F. Schimmel , J. Schmelling , V. Sciacca , M. Sedita , T. Seitz , I. Sgura , F. Simeone , I. Siotis , V. Sipala , B. Spisso , M. Spurio , G. Stavropoulos , J. Steijger , S. M. Stellacci , D. Stransky , M. Taiuti , Y. Tayalati , D. Tézier , S. Theraube , L. Thompson , P. Timmer , C. Tönnis , L. Trasatti , A. Trovato , A. Tsirigotis , S. Tzamarias , E. Tzamariudaki , B. Vallage , V. Van Elewyck , J. Vermeulen , P. Vicini , S. Viola , D. Vivolo , M. Volkert , G. Voulgaris , L. Wiggers , J. Wilms , E. de Wolf , K. Zachariadou , J. D. Zornoza , J. Zúñiga

KM3NeT is a deep-sea research infrastructure being constructed in the Mediterranean Sea. It will be installed at three sites: KM3NeT-Fr, offshore Toulon, France, KM3NeT-It, offshore Portopalo di Capo Passero, Sicily (Italy) and KM3NeT-Gr,…

Instrumentation and Methods for Astrophysics · Physics 2014-08-07 A. Margiotta

The KM3NeT Collaboration is currently constructing a multi-site high-energy neutrino telescope in the Mediterranean Sea consisting of matrices of pressure-resistant glass spheres, each holding a set of 31 small-area photomultipliers. The…

Instrumentation and Methods for Astrophysics · Physics 2022-07-27 S. Aiello , A. Albert , M. Alshamsi , S. Alves Garre , Z. Aly , A. Ambrosone , F. Ameli , M. Andre , G. Androulakis , M. Anghinolfi , M. Anguita , M. Ardid , S. Ardid , J. Aublin , C. Bagatelas , B. Baret , S. Basegmez du Pree , M. Bendahman , F. Benfenati , E. Berbee , A. M. van den Berg , V. Bertine , S. Biagi , M. Boettcher , M. Bou Cabo , J. Boumaaza , M. Bouta , M. Bouwhuis , C. Bozza , H. Branza , R. Bruijn , J. Brunner , R. Bruno , E. Buis , R. Buompane , J. Busto , B. Caiffi , D. Calvo , S. Campion , A. Capone , V. Carretero , P. Castaldi , S. Celli , M. Chabab , N. Chau , A. Chena , S. Cherubini , V. Chiarella , T. Chiarusi , M. Circella , R. Cocimano , J. A. B. Coelho , A. Coleiro , M. Colomer Molla , R. Coniglione , P. Coyle , A. Creusot , A. Cruza , G. Cuttone , R. Dalliera , B. De Martino , I. Di Palma , A. F. Diaz , D. Diego Tortosa , C. Distefano , A. Domi , C. Donzau , D. Dornic , M. Dorra , D. Drouhin , T. Eberla , A. Eddyamoui , T. van Eeden , D. van Eijk , I. El Bojaddaini , S. El Hedri , A. Enzenhofer , V. Espinosa , P. Fermani , G. Ferrara , M. D. Filipovic , F. Filippini , L. A. Fusco , T. Gala , J. Garcia Mendez , F. Garufi , Y. Gatelet , C. Gatius Oliver , N. Geisselbrecht , L. Gialanella , E. Giorgio , S. R. Gozzini , R. Gracia , K. Grafa , G. Grella , D. Guderian , C. Guidi , B. Guillon , M. Gutierrez , J. Haefner , S. Hallmann , H. Hamdaoui , H. van Harena , A. Heijboer , A. Hekaloa , L. Henniga , J. J. Hernandez-Rey , J. Hofestadt , F. Huang , W. Idrissi Ibnsalih , G. Illuminati , C. W. James , D. Janezashvili , M. de Jong , P. de Jong , B. J. Jung , P. Kalaczynski , O. Kalekin , U. F. Katz , N. R. Khan Chowdhury , G. Kistauri , F. van der Knaap , P. Kooijman , A. Kouchner , V. Kulikovskiy , M. Labalme , R. Lahmann , M. Lamoureux , G. Larosa , C. Lastori , A. Lazo , R. Le Breton , S. Le Stum , G. Lehaut , O. Leonardi , F. Leone , E. Leonora , N. Lessing , G. Levi , M. Lincetto , M. Lindsey Clark , T. Lipreau , C. LLorens Alvarez , F. Longhitano , D. Lopez-Coto , L. Maderer , J. Majumdar , J. Manczak , A. Margiotta , A. Marinelli , C. Markou , L. Martina , J. A. Martinez-Mora , A. Martini , F. Marzaioli , S. Mastroianni , K. W. Melis , G. Miele , P. Migliozzi , E. Migneco , P. Mijakowski , L. S. Miranda , C. M. Mollo , M. Moser , A. Moussa , R. Muller , M. Musumeci , L. Nauta , S. Navas , C. A. Nicolau , B. Nkosi , B. OFearraigh , M. OSullivan , M. Organokov , A. Orlando , J. Palacios Gonzalez , G. Papalashvilia , R. Papaleo , A. M. Paun , G. E. Pavala , C. Pellegrino , M. Perrin-Terrin , V. Pestel , P. Piattelli , C. Pieterse , O. Pisanti , C. Poire , V. Popa , T. Pradier , I. Probsta , S. Pulvirenti , G. Quemenera , N. Randazzo , S. Razzaquea , D. Real , S. Recka , G. Riccobene , A. Romanov , A. Rovelli , F. Salesa Greus , D. F. E. Samtlebe , A. Sanchez Losa , M. Sanguineti , D. Santonocito , P. Sapienza , J. Schnabel , M. F. Schneidera , J. Schumann , H. M. Schutte , J. Seneca , I. Sgura , R. Shanidze , A. Sharma , A. Sinopoulou , B. Spisso , M. Spurio , D. Stavropoulos , S. M. Stellaccian , M. Taiutik , Y. Tayalati , H. Thiersen , S. Tingay , S. Tsagkli , V. Tsourapis , E. Tzamariudaki , D. Tzanetatos , V. Van Elewyck , G. Vasileiadis , F. Versari , D. Vivolo , G. de Wasseige , J. Wilmsa , R. Wojaczynski , E. de Wolf , T. Yousfi , S. Zavatarelli , A. Zegarelli , D. Zito , J. D. Zornoza , J. Zuniga , N. Zywucka
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