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The IceCube collaboration is building a cubic kilometer scale neutrino telescope at a depth of 2 km at the geographic South Pole, utilizing the clear Antarctic ice as a Cherenkov medium to detect cosmic neutrinos. The IceCube observatory is…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Timo Karg

The IceCube Neutrino Observatory is a kilometer-scale detector currently under construction at the South Pole. In its final configuration the detector will comprise 5160 Digital Optical Modules (DOMs) deployed on 86 strings between 1.5-2.5…

High Energy Astrophysical Phenomena · Physics 2019-08-21 S. Toscano

IceCube is a 1 km$^3$ neutrino detector now being built at the South Pole. Its 4800 optical modules will detect Cherenkov radiation from charged particles produced in neutrino interactions. IceCube will search for neutrinos of astrophysical…

Astrophysics · Physics 2019-08-13 Spencer R. Klein

The IceCube Neutrino Observatory at the South Pole has been completed in December 2010. In this paper we describe the final detector and report results on physics and performance using data taken at different stages of the yet incomplete…

High Energy Astrophysical Phenomena · Physics 2012-08-27 The IceCube Collaboration

IceCube is a 1 km^3 neutrino detector now being built at the Amundsen-Scott South Pole Station. It consists of 4800 Digital Optical Modules (DOMs) which detect Cherenkov radiation from the charged particles produced in neutrino…

Instrumentation and Detectors · Physics 2019-08-13 Spencer R. Klein

The IceCube Observatory is a km^3 neutrino telescope currently under construction at the geographic South Pole. It will comprise 4800 optical sensors deployed on 80 vertical strings between 1450 and 2450 meters under the ice surface.…

Astrophysics · Physics 2019-08-13 Paolo Desiati

IceCube is a 1 km3 neutrino telescope currently under construction at the South Pole. The detector will consist of 4800 optical sensors deployed at depths between 1450 m and 2450 m in clear Antarctic ice evenly distributed over 80 strings.…

Astrophysics · Physics 2019-08-13 Albrecht Karle

IceCube is a 1 km$^3$ neutrino observatory being built to study neutrino production in active galactic nuclei, gamma-ray bursts, supernova remnants, and a host of other astrophysical sources. High-energy neutrinos may signal the sources of…

Astrophysics · Physics 2019-08-14 Spencer R. Klein

IceCube is a 1 km^3 neutrino telescope currently under construction at the South Pole. The detector will consist of 5160 optical sensors deployed at depths between 1450 m and 2450 m in clear Antarctic ice distributed over 86 strings. An air…

High Energy Astrophysical Phenomena · Physics 2019-08-13 A. Karle

The IceCube observatory located at the South Pole is a cubic-kilometre optical Cherenkov telescope primarily designed for the detection of high-energy astrophysical neutrinos. IceCube became fully operational in 2010, after a seven-year…

High Energy Astrophysical Phenomena · Physics 2018-11-20 Markus Ahlers , Klaus Helbing , Carlos Pérez de los Heros

Construction of the cubic-kilometer neutrino detector IceCube at the South Pole has been completed in December 2010. It forms a lattice of 5160 photomultiplier tubes monitoring a gigaton of the deep Antarctic ice for particle induced…

High Energy Physics - Experiment · Physics 2019-08-13 K. Helbing

The IceCube Neutrino Observatory is a cubic-kilometer-scale high-energy neutrino detector built into the ice at the South Pole. Construction of IceCube, the largest neutrino detector built to date, was completed in 2011 and enabled the…

Instrumentation and Methods for Astrophysics · Physics 2024-02-08 IceCube Collaboration , M. G. Aartsen , M. Ackermann , J. Adams , J. A. Aguilar , M. Ahlers , M. Ahrens , D. Altmann , K. Andeen , T. Anderson , I. Ansseau , G. Anton , M. Archinger , C. Argüelles , R. Auer , J. Auffenberg , S. Axani , J. Baccus , X. Bai , S. Barnet , S. W. Barwick , V. Baum , R. Bay , K. Beattie , J. J. Beatty , J. Becker Tjus , K. -H. Becker , T. Bendfelt , S. BenZvi , D. Berley , E. Bernardini , A. Bernhard , D. Z. Besson , G. Binder , D. Bindig , M. Bissok , E. Blaufuss , S. Blot , D. Boersma , C. Bohm , M. Börner , F. Bos , D. Bose , S. Böser , O. Botner , A. Bouchta , J. Braun , L. Brayeur , H. -P. Bretz , S. Bron , A. Burgman , C. Burreson , T. Carver , M. Casier , E. Cheung , D. Chirkin , A. Christov , K. Clark , L. Classen , S. Coenders , G. H. Collin , J. M. Conrad , D. F. Cowen , R. Cross , C. Day , M. Day , J. P. A. M. de André , C. De Clercq , E. del Pino Rosendo , H. Dembinski , S. De Ridder , F. Descamps , P. Desiati , K. D. de Vries , G. de Wasseige , M. de With , T. DeYoung , J. C. Díaz-Vélez , V. di Lorenzo , H. Dujmovic , J. P. Dumm , M. Dunkman , B. Eberhardt , W. R. Edwards , T. Ehrhardt , B. Eichmann , P. Eller , S. Euler , P. A. Evenson , S. Fahey , A. R. Fazely , J. Feintzeig , J. Felde , K. Filimonov , C. Finley , S. Flis , C. -C. Fösig , A. Franckowiak , M. Frère , E. Friedman , T. Fuchs , T. K. Gaisser , J. Gallagher , L. Gerhardt , K. Ghorbani , W. Giang , L. Gladstone , T. Glauch , D. Glowacki , T. Glüsenkamp , A. Goldschmidt , J. G. Gonzalez , D. Grant , Z. Griffith , L. Gustafsson , C. Haack , A. Hallgren , F. Halzen , E. Hansen , T. Hansmann , K. Hanson , J. Haugen , D. Hebecker , D. Heereman , K. Helbing , R. Hellauer , R. Heller , S. Hickford , J. Hignight , G. C. Hill , K. D. Hoffman , R. Hoffmann , K. Hoshina , F. Huang , M. Huber , P. O. Hulth , K. Hultqvist , S. In , M. Inaba , A. Ishihara , E. Jacobi , J. Jacobsen , G. S. Japaridze , M. Jeong , K. Jero , A. Jones , B. J. P. Jones , J. Joseph , W. Kang , A. Kappes , T. Karg , A. Karle , U. Katz , M. Kauer , A. Keivani , J. L. Kelley , J. Kemp , A. Kheirandish , J. Kim , M. Kim , T. Kintscher , J. Kiryluk , N. Kitamura , T. Kittler , S. R. Klein , S. Kleinfelder , M. Kleist , G. Kohnen , R. Koirala , H. Kolanoski , R. Konietz , L. Köpke , C. Kopper , S. Kopper , D. J. Koskinen , M. Kowalski , M. Krasberg , K. Krings , M. Kroll , G. Krückl , C. Krüger , J. Kunnen , S. Kunwar , N. Kurahashi , T. Kuwabara , M. Labare , K. Laihem , H. Landsman , J. L. Lanfranchi , M. J. Larson , F. Lauber , A. Laundrie , D. Lennarz , H. Leich , M. Lesiak-Bzdak , M. Leuermann , L. Lu , J. Ludwig , J. Lünemann , C. Mackenzie , J. Madsen , G. Maggi , K. B. M. Mahn , S. Mancina , M. Mandelartz , R. Maruyama , K. Mase , H. Matis , R. Maunu , F. McNally , C. P. McParland , P. Meade , K. Meagher , M. Medici , M. Meier , A. Meli , T. Menne , G. Merino , T. Meures , S. Miarecki , R. H. Minor , T. Montaruli , M. Moulai , T. Murray , R. Nahnhauer , U. Naumann , G. Neer , M. Newcomb , H. Niederhausen , S. C. Nowicki , D. R. Nygren , A. Obertacke Pollmann , A. Olivas , A. O'Murchadha , T. Palczewski , H. Pandya , D. V. Pankova , S. Patton , P. Peiffer , Ö. Penek , J. A. Pepper , C. Pérez de los Heros , C. Pettersen , D. Pieloth , E. Pinat , P. B. Price , G. T. Przybylski , M. Quinnan , C. Raab , L. Rädel , M. Rameez , K. Rawlins , R. Reimann , B. Relethford , M. Relich , E. Resconi , W. Rhode , M. Richman , B. Riedel , S. Robertson , M. Rongen , C. Roucelle , C. Rott , T. Ruhe , D. Ryckbosch , D. Rysewyk , L. Sabbatini , S. E. Sanchez Herrera , A. Sandrock , J. Sandroos , P. Sandstrom , S. Sarkar , K. Satalecka , P. Schlunder , T. Schmidt , S. Schoenen , S. Schöneberg , A. Schukraft , L. Schumacher , D. Seckel , S. Seunarine , M. Solarz , D. Soldin , M. Song , G. M. Spiczak , C. Spiering , T. Stanev , A. Stasik , J. Stettner , A. Steuer , T. Stezelberger , R. G. Stokstad , A. Stößl , R. Ström , N. L. Strotjohann , K. -H. Sulanke , G. W. Sullivan , M. Sutherland , H. Taavola , I. Taboada , J. Tatar , F. Tenholt , S. Ter-Antonyan , A. Terliuk , G. Tešić , L. Thollander , S. Tilav , P. A. Toale , M. N. Tobin , S. Toscano , D. Tosi , M. Tselengidou , A. Turcati , E. Unger , M. Usner , J. Vandenbroucke , N. van Eijndhoven , S. Vanheule , M. van Rossem , J. van Santen , M. Vehring , M. Voge , E. Vogel , M. Vraeghe , D. Wahl , C. Walck , A. Wallace , M. Wallraff , N. Wandkowsky , Ch. Weaver , M. J. Weiss , C. Wendt , S. Westerhoff , D. Wharton , B. J. Whelan , S. Wickmann , K. Wiebe , C. H. Wiebusch , L. Wille , D. R. Williams , L. Wills , P. Wisniewski , M. Wolf , T. R. Wood , E. Woolsey , K. Woschnagg , D. L. Xu , X. W. Xu , Y. Xu , J. P. Yanez , G. Yodh , S. Yoshida , M. Zoll

The IceCube Neutrino Observatory instruments roughly one cubic kilometer of deep, glacial ice below the geographic South Pole with 5160 optical sensors to register the Cherenkov light of passing relativistic, charged particles. Since its…

Instrumentation and Methods for Astrophysics · Physics 2019-11-26 Martin Rongen

The IceCube Neutrino Observatory is a cubic kilometer neutrino telescope located at the geographic South Pole. Cherenkov radiation emitted by charged secondary particles from neutrino interactions is observed by IceCube using an array of…

High Energy Astrophysical Phenomena · Physics 2026-04-01 Kevin J. Meagher

High-energy neutrinos are uniquely suited to study a large variety of physics as they traverse the universe almost untouched, in contrast to conventional astronomical messengers like photons or cosmic rays which are limited by interactions…

Astrophysics · Physics 2019-08-14 Carsten Rott

IceCube is a kilometer-scale high energy neutrino telescope under construction at the South Pole, a second-generation instrument expanding the capabilities of the AMANDA telescope. The scientific portfolio of IceCube includes the detection…

High Energy Astrophysical Phenomena · Physics 2009-07-22 Tyce DeYoung

Encompasing a volume of ~1 km^3 of glacial ice at the South Pole, IceCube is currently the worlds largest neutrino detector. It consists of 5160 optical modules on 86 strings in a depth between 1450m and 2450m, as well as 324 optical…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Sebastian Böser

The completed IceCube Observatory, the first km^3 neutrino telescope, is already providing the most stringent limits on the flux of high energy cosmic neutrinos from point-like and diffuse galactic and extra-galactic sources. The…

High Energy Astrophysical Phenomena · Physics 2019-08-13 Paolo Desiati

The $\sim$1 km$^3$ IceCube neutrino observatory was completed in December, 2010 and is taking data on cosmic-ray muons and neutrinos, extra-terrestrial neutrinos, and setting limits on a variety of exotic phenomena. This proceeding will…

High Energy Astrophysical Phenomena · Physics 2019-08-21 Spencer R. Klein

IceCube is a cubic neutrino telescope under construction at the South Pole since the austral summer 2004/2005 with a total instrumented volume of the order of 1 km^3. At the moment it is taking data with 40 deployed strings. The full…

Astrophysics · Physics 2010-12-13 P. Berghaus
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