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Related papers: The prototype string for the km3-scale Baikal neut…

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A prototype detection unit of the KM3NeT deep-sea neutrino telescope has been installed at 3500m depth 80km offshore the Italian coast. KM3NeT in its final configuration will contain several hundreds of detection units. Each detection unit…

Instrumentation and Methods for Astrophysics · Physics 2016-04-06 KM3NeT Collaboration , S. Adrián-Martínez , M. Ageron , F. Aharonian , S. Aiello , A. Albert , F. Ameli , E. G. Anassontzis , G. C. Androulakis , M. Anghinolfi , G. Anton , S. Anvar , M. Ardid , T. Avgitas , K. Balasi , H. Band , G. Barbarino , E. Barbarito , F. Barbato , B. Baret , S. Baron , J. Barrios , A. Belias , E. Berbee , A. M. van den Berg , A. Berkien , V. Bertin , S. Beurthey , V. van Beveren , N. Beverini , S. Biagi , A. Biagioni , S. Bianucci , M. Billault , A. Birbas , H. Boer Rookhuizen , R. Bormuth , V. Bouché , B. Bouhadef , G. Bourlis , C. Boutonnet , M. Bouwhuis , C. Bozza , R. Bruijn , J. Brunner , G. Cacopardo , L. Caillat , M. Calamai , D. Calvo , A. Capone , L. Caramete , F. Caruso , S. Cecchini , A. Ceres , R. Cereseto , C. Champion , F. Château , T. Chiarusi , B. Christopoulou , M. Circella , L. Classen , R. Cocimano , A. Coleiro , S. Colonges , R. Coniglione , A. Cosquer , M. Costa , P. Coyle , A. Creusot , G. Cuttone , C. D'Amato , A. D'Amico , G. De Bonis , G. De Rosa , N. Deniskina , J. -J. Destelle , C. Distefano , F. Di Capua , C. Donzaud , D. Dornic , Q. Dorosti-Hasankiadeh , E. Drakopoulou , D. Drouhin , L. Drury , D. Durand , T. Eberl , D. Elsaesser , A. Enzenhöfer , P. Fermani , L. A. Fusco , D. Gajanana , T. Gal , S. Galatà , F. Garufi , M. Gebyehu , V. Giordano , N. Gizani , R. GraciaRuiz , K. Graf , R. Grasso , G. Grella , A. Grmek , R. Habel , H. van Haren , T. Heid , A. Heijboer , E. Heine , S. Henry , J. J. Hernández-Rey , B. Herold , M. A. Hevinga , M. van der Hoek , J. Hofestädt , J. Hogenbirk , C. Hugon , J. Hößl , M. Imbesi , C. W. James , P. Jansweijer , J. Jochum , M. de Jong , M. Jongen , M. Kadler , O. Kalekin , A. Kappes , E. Kappos , U. Katz , O. Kavatsyuk , P. Keller , G. Kieft , E. Koffeman , H. Kok , P. Kooijman , J. Koopstra , A. Korporaal , A. Kouchner , I. Kreykenbohm , V. Kulikovskiy , R. Lahmann , P. Lamare , G. Larosa , D. Lattuada , H. Le Provost , K. P. Leismüller , A. Leisos , D. Lenis , E. Leonora , M. LindseyClark , C. D. Llorens Alvarez , H. Löhner , A. Lonardo , S. Loucatos , F. Louis , E. Maccioni , K. Mannheim , K. Manolopoulos , A. Margiotta , O. Mariş , C. Markou , J. A. Martínez-Mora , A. Martini , R. Masullo , K. W. Melis , T. Michael , P. Migliozzi , E. Migneco , A. Miraglia , C. M. Mollo , M. Mongelli , M. Morganti , S. Mos , Y. Moudden , P. Musico , M. Musumeci , C. Nicolaou , C. A. Nicolau , A. Orlando , A. Orzelli , A. Papaikonomou , R. Papaleo , G. E. Păvălaş , H. Peek , C. Pellegrino , M. G. Pellegriti , C. Perrina , P. Piattelli , K. Pikounis , V. Popa , Th. Pradier , M. Priede , G. Pühlhofer , S. Pulvirenti , C. Racca , F. Raffaelli , N. Randazzo , P. A. Rapidis , P. Razis , D. Real , L. Resvanis , J. Reubelt , G. Riccobene , A. Rovelli , M. Saldaña , D. F. E. Samtleben , M. Sanguineti , A. Santangelo , P. Sapienza , J. Schmelling , J. Schnabel , V. Sciacca , M. Sedita , T. Seitz , I. Sgura , F. Simeone , V. Sipala , A. Spitaleri , M. Spurio , G. Stavropoulos , J. Steijger , T. Stolarczyk , D. Stransky , M. Taiuti , G. Terreni , D. Tézier , S. Théraube , L. F. Thompson , P. Timmer , L. Trasatti , A. Trovato , M. Tselengidou , A. Tsirigotis , S. Tzamarias , E. Tzamariudaki , B. Vallage , V. Van Elewyck , J. Vermeulen , P. Vernin , P. Vicini , S. Viola , D. Vivolo , P. Werneke , L. Wiggers , J. Wilms , E. de Wolf , R. H. L. van Wooning , E. Zonca , J. D. Zornoza , J. Zúñiga , A. Zwart

We report theoretical and experimental results of on-going feasibility studies to detect cosmic neutrinos acoustically in Lake Baikal. In order to examine ambient noise conditions and to develop respective pulse detection techniques a…

We review the status and results of the high energy neutrino telescopes in the Northern Hemisphere, namely ANTARES and Baikal (NT200+).

High Energy Astrophysical Phenomena · Physics 2012-03-12 Juan José Hernández-Rey

Current generation neutrino telescopes cover an energy range from about 10 GeV to beyond $10^9$ GeV. IceCube sets the scale for future experiments to make improvements. Strategies for future upgrades will be discussed in three energy…

Instrumentation and Methods for Astrophysics · Physics 2015-06-11 Albrecht Karle

We rewiew the present status of the Baikal Neutrino Project and present the results of a search for high energy neutrinos with the detector intermediate stage NT-96.

Astrophysics · Physics 2008-11-26 BAIKAL Collaboration , V. Balkanov

We use likelihood approach for search for local astrophysical neutrino sources in unbinned versus binned methods with Baikal deep underwater telescopes. We analyze neutrino data sample selected with NT200 telescope for 1038 live days by…

High Energy Astrophysical Phenomena · Physics 2014-06-11 O. V. Suvorova , T. A. Ovsiannikova

The Baikal-GVD neutrino telescope currently consists of 8 clusters of 288 optical modules (photodetectors). One cluster comprises 8 strings, each of which is subdivided into 3 sections of 12 optical modules. This paper presents the methods…

High Energy Physics - Experiment · Physics 2021-07-30 D. P. Petukhov

Since the end of the 2005-2006 austral summer, the IceCube detector consists of an array of 9 strings, deployed between 1450 m and 2450 m of depth and containing 540 digital optical sensors and 16 IceTop surface stations with 64 sensors.…

Astrophysics · Physics 2019-08-14 Paolo Desiati

A deep underwater Cherenkov telescope has been operating since 1993 in stages of growing size at 1.1 km depth in Lake Baikal. The key component of the telescope is the Optical Module (OM) which houses the highly sensitive phototube…

Astrophysics · Physics 2008-11-26 R. I. Bagduev

We review the present status of the lake Baikal Neutrino Experiment and present selected physical results gained with the consequetive stages of the stepwise increasing detector: from NT-36 to NT-96. Results cover atmospheric muons,…

Astrophysics · Physics 2008-11-26 BAIKAL Collaboration , V. Balkanov

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