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Related papers: Astronomy potential of KM3NeT/ARCA

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Studying atmospheric neutrino oscillations in the few-GeV range with a multimegaton detector promises to determine the neutrino mass hierarchy. This is the main science goal pursued by the future KM3NeT/ORCA water Cherenkov detector in the…

Instrumentation and Detectors · Physics 2017-05-22 S. Adrián-Martínez , M. Ageron , S. Aiello , A. Albert , F. Ameli , E. G. Anassontzis , M. Andre , G. Androulakis , M. Anghinolfi , G. Anton , M. Ardid , T. Avgitas , G. Barbarino , E. Barbarito , B. Baret , J. Barrios-Martí , A. Belias , E. Berbee , A. van den Berg , V. Bertin , S. Beurthey , V. van Beveren , N. Beverini , S. Biagi , A. Biagioni , M. Billault , M. Bondì , R. Bormuth , B. Bouhadef , G. Bourlis , S. Bourret , C. Boutonnet , M. Bouwhuis , C. Bozza , R. Bruijn , J. Brunner , E. Buis , R. Buompane , J. Busto , G. Cacopardo , L. Caillat , M. Calamai , D. Calvo , A. Capone , L. Caramete , S. Cecchini , S. Celli , C. Champion , S. Cherubini , V. Chiarella , T. Chiarusi , M. Circella , L. Classen , D. Cobas , R. Cocimano , J. A. B. Coelho , A. Coleiro , S. Colonges , R. Coniglione , M. Cordelli , A. Cosquer , P. Coyle , A. Creusot , G. Cuttone , C. D'Amato , A. D'Amico , A. D'Onofrio , G. De Bonis , C. De Sio , I. Di Palma , A. F. Díaz , C. Distefano , C. Donzaud , D. Dornic , Q. Dorosti-Hasankiadeh , E. Drakopoulou , D. Drouhin , M. Durocher , T. Eberl , S. Eichie , D. van Eijk , I. El Bojaddaini , D. Elsaesser , A. Enzenhöfer , M. Favaro , P. Fermani , G. Ferrara , G. Frascadore , L. A. Fusco , T. Gal , S. Galatà , F. Garufi , P. Gay , M. Gebyehu , F. Giacomini , L. Gialanella , V. Giordano , N. Gizani , R. Gracia , K. Graf , T. Grégoire , G. Grella , A. Grmek , 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 , M. Kreter , V. Kulikovskiy , R. Lahmann , P. Lamare , G. Larosa , A. Leisos , F. Leone , 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 , M. Manzali , A. Margiotta , A. Marinelli , O. Mariş , C. Markou , J. A. Martínez-Mora , A. Martini , F. Marzaioli , 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. Orzelli , A. Papaikonomou , R. Papaleo , G. E. Păvălaş , H. Peek , G. Pellegrini , C. Pellegrino , C. Perrina , M. Pfutzner , P. Piattelli , K. Pikounis , M. -O. Pleinert , G. E. Poma , V. Popa , T. Pradier , F. Pratolongo , G. Pühlhofer , S. Pulvirenti , L. Quinn , C. Racca , F. Raffaelli , N. Randazzo , T. Rauch , 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 , J. Schnabel , V. Sciacca , M. Sedita , T. Seitz , I. Sgura , F. Simeone , V. Sipala , B. Spisso , M. Spurio , G. Stavropoulos , J. Steijger , S. M. Stellacci , D. Stransky , M. Taiuti , Y. Tayalati , F. Terrasi , D. Tézier , S. Theraube , P. Timmer , C. Tönnis , L. Trasatti , R. Travaglini , A. Trovato , A. Tsirigotis , S. Tzamarias , E. Tzamariudaki , B. Vallage , V. Van Elewyck , J. Vermeulen , P. Vicini , S. Viola , D. Vivolo , M. Volkert , L. Wiggers , J. Wilms , E. de Wolf , K. Zachariadou , J. D. Zornoza , J. Zúñiga

On the 13th February 2023 the KM3NeT/ARCA telescope observed a track-like event compatible with a ultra-high-energy muon with an estimated energy of 120 PeV, produced by a neutrino with an even higher energy, making it the most energetic…

High Energy Astrophysical Phenomena · Physics 2025-02-13 The KM3NeT collaboration

The ANTARES Collaboration has completed in 2008 the deployment of what is currently the largest high energy neutrino detector in the Northern hemisphere. The search for cosmic neutrinos in the energy range between tens of GeV and tens of…

High Energy Astrophysical Phenomena · Physics 2019-08-14 Manuela Vecchi

The main goal of the ANTARES neutrino telescope is the identification of neutrinos from cosmic accelerators. The good visibility towards the Southern sky for neutrino energies below 100 TeV and the good angular resolution for reconstructed…

High Energy Astrophysical Phenomena · Physics 2019-08-23 Julien Aublin , Giulia Illuminati , Sergio Navas

The ANTARES collaboration propose to observe High Energy Cosmic Neutrinos using a Deep Sea Cherenkov detector. The sky survey with high energy neutrinos is complementary to the observations with photons. It is expected that this will shed a…

Astrophysics · Physics 2012-08-27 ANTARES collaboration

The acoustic neutrino detection technique is a promising approach for future large-scale detectors with the aim of measuring the small expected flux of neutrinos at energies in the EeV-range and above. The technique is based on the…

Instrumentation and Methods for Astrophysics · Physics 2018-11-30 Robert Lahmann

The ANTARES neutrino telescope is installed at a depth of 2.5 km of the Mediterranean Sea and consists of a three-dimensional array of 885 photomultipliers arranged on twelve detector lines. The prime objective is to detect high-energy…

High Energy Astrophysical Phenomena · Physics 2019-08-21 Salvatore Mangano

Recent measurements of ultra-high energy cosmic rays and neutrinos are briefly reviewed. With several new large scale observatories nearing completion or becoming fully operational only very recently, a large body of high quality and high…

High Energy Astrophysical Phenomena · Physics 2014-11-20 Karl-Heinz Kampert

The NEMO project aims at the search, development and validation of key technologies for the construction, deployment and mantainance of an underwater Cherenkov km3 neutrino telescope in the Mediterranean Sea. Moreover, the NEMO…

Astrophysics · Physics 2007-05-23 Piera Sapienza

The objective of neutrino astronomy, born with the identification of thermonuclear fusion in the sun and the particle processes controlling the fate of a nearby supernova, is to build instruments which reach throughout and far beyond our…

Astrophysics · Physics 2007-05-23 F. Halzen

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

The ANTARES telescope is being built in the Mediterranean Sea. The detector consists of a 3D array of photomultipliers (PMTs) that detects the Cherenkov light induced by the muons produced in neutrino interactions. Other signatures can also…

Astrophysics · Physics 2019-08-13 J. A. Aguilar

The discrimination of the two possible options for the neutrino mass ordering (normal or inverted) is a major goal for current and future neutrino oscillation experiments. Such goal might be reached by observing high-statistics energy-angle…

High Energy Physics - Phenomenology · Physics 2018-02-14 Francesco Capozzi , Eligio Lisi , Antonio Marrone

Multi-messenger astronomy requires real-time systems capable of rapidly responding to external alerts and sharing significant detections with partner observatories. KM3NeT, a deep-sea Cherenkov neutrino telescope in the Mediterranean Sea,…

High Energy Astrophysical Phenomena · Physics 2026-04-30 Martina Marconi

The KM3NeT project is a common European effort for the design of a km3-scale deep-sea neutrino telescope in the Mediterranean. For the upcoming Design Study simulations have been done using modified ANTARES software. Several concepts and…

Astrophysics · Physics 2009-11-11 S. Kuch

The NEMO Collaboration is conducting an R&D activity towards the construction of a Mediterranean km3 neutrino telescope. In this work, we present the results of Monte Carlo simulation studies on the capability of the proposed NEMO telescope…

Astrophysics · Physics 2008-11-26 C. Distefano

The recent detection of the ultra-high energy neutrino KM3-230213A by KM3NeT/ARCA marks the first observation of an astrophysical neutrino with energy above 100 PeV, opening a new window to the ultra-high energy Universe. In this…

High Energy Astrophysical Phenomena · Physics 2026-05-11 Per Arne Sevle Myhr

With the KM3NeT experiment, which is presently under construction in the Mediterranean Sea, a new neutrino telescope will be installed to study both the neutrino properties as well as the cosmic origin of these particles. To do so, about…

Instrumentation and Methods for Astrophysics · Physics 2019-10-23 Rasa Muller , Sander von Benda-Beckmann , Ed Doppenberg , Robert Lahmann , Ernst-Jan Buis

The KM3NeT neutrino telescope is currently being deployed at two different sites in the Mediterranean Sea. First searches for astrophysical neutrinos have been performed using data taken with the partial detector configuration already in…

High Energy Astrophysical Phenomena · Physics 2024-05-08 KM3NeT Collaboration , S. Aiello , A. Albert , S. Alves Garre , Z. Aly , A. Ambrosone , F. Ameli , M. Andre , E. Androutsou , M. Anguita , L. Aphecetche , M. Ardid , S. Ardid , H. Atmani , J. Aublin , L. Bailly-Salins , Z. Bardačová , B. Baret , A. Bariego-Quintana , S. Basegmez du Pree , Y. Becherini , M. Bendahman , F. Benfenati , M. Benhassi , D. M. Benoit , E. Berbee , V. Bertin , S. Biagi , M. Boettcher , D. Bonanno , J. Boumaaza , M. Bouta , M. Bouwhuis , C. Bozza , R. M. Bozza , H. Brânzaş , F. Bretaudeau , R. Bruijn , J. Brunner , R. Bruno , E. Buis , R. Buompane , J. Busto , B. Caiffi , D. Calvo , S. Campion , A. Capone , F. Carenini , V. Carretero , T. Cartraud , P. Castaldi , V. Cecchini , S. Celli , L. Cerisy , M. Chabab , M. Chadolias , A. Chen , S. Cherubini , T. Chiarusi , M. Circella , R. Cocimano , J. A. B. Coelho , A. Coleiro , R. Coniglione , P. Coyle , A. Creusot , G. Cuttone , R. Dallier , Y. Darras , A. De Benedittis , B. De Martino , G. De Wasseige , V. Decoene , R. Del Burgo , I. Del Rosso , U. M. Di Cerbo , L. S. Di Mauro , I. Di Palma , A. F. Díaz , C. Diaz , D. Diego-Tortosa , C. Distefano , A. Domi , C. Donzaud , D. Dornic , M. Dörr , E. Drakopoulou , D. Drouhin , R. Dvornický , T. Eberl , E. Eckerová , A. Eddymaoui , T. van Eeden , M. Eff , D. van Eijk , I. El Bojaddaini , S. El Hedri , A. Enzenhöfer , G. Ferrara , M. D. Filipović , F. Filippini , D. Franciotti , L. A. Fusco , J. Gabriel , S. Gagliardini , T. Gal , J. García Méndez , A. Garcia Soto , C. Gatius Oliver , N. Geißelbrecht , H. Ghaddari , L. Gialanella , B. K. Gibson , E. Giorgio , I. Goos , P. Goswami , D. Goupilliere , S. R. Gozzini , R. Gracia , K. Graf , C. Guidi , B. Guillon , M. Gutiérrez , H. van Haren , A. Heijboer , A. Hekalo , L. Hennig , J. J. Hernández-Rey , W. Idrissi Ibnsalih , G. Illuminati , M. de Jong , P. de Jong , B. J. Jung , P. Kalaczyński , O. Kalekin , U. F. Katz , A. Khatun , G. Kistauri , C. Kopper , A. Kouchner , V. Kueviakoe , V. Kulikovskiy , R. Kvatadze , M. Labalme , R. Lahmann , M. Lamoureux , G. Larosa , C. Lastoria , A. Lazo , S. Le Stum , G. Lehaut , E. Leonora , N. Lessing , G. Levi , M. Lindsey Clark , F. Longhitano , J. Majumdar , L. Malerba , F. Mamedov , J. Mańczak , A. Manfreda , M. Marconi , A. Margiotta , A. Marinelli , C. Markou , L. Martin , J. A. Martínez-Mora , F. Marzaioli , M. Mastrodicasa , S. Mastroianni , S. Miccichè , G. Miele , P. Migliozzi , E. Migneco , M. L. Mitsou , C. M. Mollo , L. Morales-Gallegos , M. Morga , A. Moussa , I. Mozun Mateo , R. Muller , M. R. Musone , M. Musumeci , S. Navas , A. Nayerhoda , C. A. Nicolau , B. Nkosi , B. Ó Fearraigh , V. Oliviero , A. Orlando , E. Oukacha , D. Paesani , J. Palacios González , G. Papalashvili , V. Parisi , E. J. Pastor Gomez , A. M. Păun , G. E. Păvălaş , S. Peña Martínez , M. Perrin-Terrin , J. Perronnel , V. Pestel , R. Pestes , P. Piattelli , C. Poirè , V. Popa , T. Pradier , J. Prado , S. Pulvirenti , G. Quéméner , C. A. Quiroz-Rangel , U. Rahaman , N. Randazzo , R. Randriatoamanana , S. Razzaque , I. C. Rea , D. Real , G. Riccobene , J. Robinson , A. Romanov , A. Šaina , F. Salesa Greus , D. F. E. Samtleben , A. Sánchez Losa , S. Sanfilippo , M. Sanguineti , C. Santonastaso , D. Santonocito , P. Sapienza , J. Schnabel , J. Schumann , H. M. Schutte , J. Seneca , N. Sennan , B. Setter , I. Sgura , R. Shanidze , A. Sharma , Y. Shitov , F. Šimkovic , A. Simonelli , A. Sinopoulou , M. V. Smirnov , B. Spisso , M. Spurio , D. Stavropoulos , I. Štekl , M. Taiuti , Y. Tayalati , H. Thiersen , I. Tosta e Melo , E. Tragia , B. Trocmé , V. Tsourapis , E. Tzamariudaki , A. Vacheret , A. Valer Melchor , V. Valsecchi , V. Van Elewyck , G. Vannoye , G. Vasileiadis , F. Vazquez de Sola , C. Verilhac , A. Veutro , S. Viola , D. Vivolo , J. Wilms , E. de Wolf , H. Yepes-Ramirez , G. Zarpapis , S. Zavatarelli , A. Zegarelli , D. Zito , J. D. Zornoza , J. Zúñiga , N. Zywucka

The ANTARES neutrino telescope, located in the Mediterranean Sea, and the IceCube neutrino observatory, located at the geographic South Pole, both search for cosmic neutrino events with an instantaneous full-sky field of view. The different…

High Energy Astrophysical Phenomena · Physics 2019-08-21 Giulia Illuminati