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The ANTARES project aims to build a deep-sea Cherenkov Telescope for High Energy Neutrino Astronomy located in the Mediterranean Sea. The experiment, currently in the construction phase, has recently achieved an important milestone : the…

天体物理学 · 物理学 2019-08-14 Thierry Pradier

The Surface Detector array of the Pierre Auger Observatory can detect neutrinos with energy between 10^17 eV and 10^20 eV from point-like sources across the sky south of +55 deg and north of -65 deg declinations. A search has been performed…

高能天体物理现象 · 物理学 2012-10-12 Pierre Auger Collaboration

IceCube is a km^3 scale neutrino detector being constructed deep in the Antarctic ice. When complete, IceCube will consist of 4800 optical modules deployed on 80 strings between 1450 and 2450 m of depth. During the 2007-2008 data taking…

高能天体物理现象 · 物理学 2019-08-13 Erik Strahler

The ANTARES Neutrino Telescope is a water Cherenkov detector currently under construction in the Mediterranean Sea. It is also designed to serve as a platform for investigations of the deep-sea environment. In this context, the ANTARES…

天体物理学 · 物理学 2008-11-26 K Graf , G Anton , J Hoessl , A Kappes , U F Katz , R Lahmann , C Naumann , K Salomon

Neutrinos may offer a unique opportunity to explore the far Universe at high energy. The ANTARES collaboration aims at building a large undersea neutrino detector able to observe astrophysical sources (AGNs, X-ray binary systems, ...) and…

天体物理学 · 物理学 2016-08-30 S. Basa

Neutrino telescopes offer an alternative way to explore the Universe. Several projects are in operation or under construction. A detector under the ocean is very promising because of the very accurate angular resolution that it provides.…

高能物理 - 实验 · 物理学 2009-10-31 L. Moscoso

Analysis of the Fermi-LAT data has revealed two extended structures above and below the Galactic Centre emitting gamma rays with a hard spectrum, the so-called Fermi bubbles. Hadronic models attempting to explain the origin of the Fermi…

高能天体物理现象 · 物理学 2016-10-19 ANTARES Collaboration , S. Adrián-Martínez , A. Albert , I. Al Samarai , M. André , G. Anton , S. Anvar , M. Ardid , T. Astraatmadja , J-J. Aubert , B. Baret , J. Barrios-Martí , S. Basa , V. Bertin , S. Biagi , C. Bigongiari , C. Bogazzi , B. Bouhou , M. C. Bouwhuis , J. Brunner , J. Busto , A. Capone , L. Caramete , C. Cârloganu , J. Carr , S. Cecchini , Z. Charif , Ph. Charvis , T. Chiarusi , M. Circella , F. Classen , R. Coniglione , L. Core , H. Costantini , P. Coyle , A. Creusot , C. Curtil , G. De Bonis , I. Dekeyser , A. Deschamps , C. Donzaud , D. Dornic , Q. Dorosti , D. Drouhin , A. Dumas , T. Eberl , U. Emanuele , A. Enzenhöfer , J-P. Ernenwein , S. Escoffier , K. Fehn , P. Fermani , V. Flaminio , F. Folger , U. Fritsch , L. A. Fusco , S. Galatà , P. Gay , S. Geißelsöder , K. Geyer , G. Giacomelli , V. Giordano , A. Gleixner , J. P. Gómez-González , K. Graf , G. Guillard , H. van Haren , A. J. Heijboer , Y. Hello , J. J. Hernández-Rey , B. Herold , J. Hößl , C. Hugon , C. W. James , M. de Jong , M. Kadler , O. Kalekin , A. Kappes , U. Katz , P. Kooijman , A. Kouchner , I. Kreykenbohm , V. Kulikovskiy , R. Lahmann , E. Lambard , G. Lambard , G. Larosa , D. Lattuada , D. Lefèvre , E. Leonora , D. Lo Presti , H. Loehner , S. Loucatos , F. Louis , S. Mangano , M. Marcelin , A. Margiotta , J. A. Martínez-Mora , S. Martini , T. Michael , T. Montaruli , M. Morganti , C. Müller , M. Neff , E. Nezri , D. Palioselitis , G. E. Păvălaş , C. Perrina , V. Popa , T. Pradier , C. Racca , G. Riccobene , R. Richter , C. Rivière , A. Robert , K. Roensch , A. Rostovtsev , D. F. E. Samtleben , M. Sanguineti , P. Sapienza , J. Schmid , J. Schnabel , S. Schulte , F. Schüssler , T. Seitz , R. Shanidze , C. Sieger , F. Simeone , A. Spies , M. Spurio , J. J. M. Steijger , Th. Stolarczyk , A. Sánchez-Losa , M. Taiuti , C. Tamburini , Y. Tayalati , A. Trovato , B. Vallage , C. Vallée , V. Van Elewyck , M. Vecchi , P. Vernin , E. Visser , S. Wagner , J. Wilms , E. de Wolf , K. Yatkin , H. Yepes , J. D. Zornoza , J. Zúñiga

ANTARES is a project leading towards the construction and deployment of a neutrino telescope in the deep Mediterranean Sea. The telescope will use an array of photomultiplier tubes to detect the Cherenkov light emitted by muons resulting…

天体物理学 · 物理学 2012-08-27 ANTARES collaboration

The ANTARES telescope is well-suited for detecting astrophysical transient neutrino sources as it can observe a full hemisphere of the sky at all times with a high duty cycle. The background due to atmospheric particles can be drastically…

高能天体物理现象 · 物理学 2016-08-08 S. Adrián-Martínez , A. Albert , M. André , G. Anton , M. Ardid , J. -J. Aubert , B. Baret , J. Barrios-Martí , S. Basa , V. Bertin , S. Biagi , C. Bogazzi , R. Bormuth , M. Bou-Cabo , M. C. Bouwhuis , R. Bruijn , J. Brunner , J. Busto , A. Capone , L. Caramete , J. Carr , T. Chiarusi , M. Circella , R. Coniglione , H. Costantini , P. Coyle , A. Creusot , I. Dekeyser , A. Deschamps , G. De Bonis , C. Distefano , C. Donzaud , D. Dornic , D. Drouhin , A. Dumas , T. Eberl , D. Elsässer , A. Enzenhöfer , K. Fehn , I. Felis , P. Fermani , F. Folger , L. A. Fusco , S. Galatà , P. Gay , S. Geißelsöder , K. Geyer , V. Giordano , A. Gleixner , R. Gracia-Ruiz , K. Graf , H. van Haren , A. J. Heijboer , Y. Hello , J. J. Hernández-Rey , A. Herrero , J. Hößl , J. Hofestädt , C. Hugon , C. W James , M. de Jong , M. Kadler , O. Kalekin , U. Katz , D. Kießling , P. Kooijman , A. Kouchner , I. Kreykenbohm , V. Kulikovskiy , R. Lahmann , G. Lambard , D. Lattuada , D. Lefèvre , E. Leonora , S. Loucatos , S. Mangano , A. Margiotta , J. A. Martínez-Mora , S. Martini , A. Mathieu , T. Michael , P. Migliozzi , A. Moussa , C. Mueller , M. Neff , E. Nezri , G. E. Păvălaş , C. Pellegrino , C. Perrina , P. Piattelli , V. Popa , T. Pradier , C. Racca , G. Riccobene , R. Richter , K. Roensch , A. Rostovtsev , M. Saldaña , D. F. E. Samtleben , M. Sanguineti , P. Sapienza , J. Schmid , J. Schnabel , S. Schulte , F. Schüssler , T. Seitz , C. Sieger , M. Spurio , J. J. M. Steijger , Th. Stolarczyk , A. Sánchez-Losa , M. Taiuti , C. Tamburini , A. Trovato , M. Tselengidou , C. Tönnis , D. Turpin , B. Vallage , C. Vallée , V. Van Elewyck , E. Visser , D. Vivolo , S. Wagner , J. Wilms , J. D. Zornoza , J. Zúñiga

The ANTARES project aims at the construction of an underwater neutrino telescope at the scale of 0.1 km^2 2400 m deep in the Mediterranean Sea. After a 4-year R&D program, the ANTARES project has entered the construction phase which will be…

高能物理 - 实验 · 物理学 2015-06-25 T. Montaruli , for ANTARES Collaboration

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…

天体物理仪器与方法 · 物理学 2019-08-13 Aart Heijboer

High-energy neutrinos could be produced in the interaction of charged cosmic rays with matter or radiation surrounding astrophysical sources. To look for transient sources associated with neutrino emission, a follow-up program of neutrino…

高能天体物理现象 · 物理学 2024-02-27 A. Albert , S. Alves , M. André , M. Ardid , S. Ardid , J. -J. Aubert , J. Aublin , B. Baret , S. Basa , Y. Becherini , B. Belhorma , M. Bendahman , F. Benfenati , V. Bertin , S. Biagi , M. Bissinger , J. Boumaaza , M. Bouta , M. C. Bouwhuis , H. Brânzas , R. Bruijn , J. Brunner , J. Busto , B. Caiffi , D. Calvo , S. Campion , A. Capone , L. Caramete , F. Carenini , J. Carr , V. Carretero , 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. S. M. Cruz , A. F. Díaz , B. De Martino , C. Distefano , I. Di Palma , C. Donzaud , D. Dornic , D. Drouhin , T. Eberl , 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. García , C. Gatius Oliver , P. Gay , N. Geißelbrecht , H. Glotin , R. Gozzini , R. Gracia Ruiz , K. Graf , C. Guidi , L. Haegel , S. Hallmann , H. van Haren , A. J. Heijboer , Y. Hello , L. Hennig , J. J. Hernández-Rey , J. Hößl , J. Hofestädt , F. Huang , G. Illuminati , C. W. James , 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 , L. Maderer , J. Manczak , M. Marcelin , A. Margiotta , A. Marinelli , J. A. Martínez-Mora , P. Migliozzi , A. Moussa , R. Muller , S. Navas , E. Nezri , B. Ó Fearraigh , E. Oukacha , A. Pāun , G. E. Pāvālas , S. Peña-Martínez , M. Perrin-Terrin , P. Piattelli , V. Popa , T. Pradier , N. Randazzo , D. Real , G. Riccobene , A. Romanov , A. Sánchez-Losa , A. Saina , F. Salesa Greus , D. F. E. Samtleben , M. Sanguineti , P. Sapienza , J. Schnabel , J. Schumann , F. Schüssler , J. Seneca , M. Spurio , Th. Stolarczyk , M. Taiuti , Y. Tayalati , S. J. Tingay , B. Vallage , G. Vannoye , V. Van Elewyck , S. Viola , D. Vivolo , J. Wilms , S. Zavatarelli , A. Zegarelli , J. D. Zornoza , J. Zúñiga , V. Lipunov , G. Antipov , P. Balanutsa , D. Buckley , N. Budnev , A. Chasovnikov , D. Cheryasov , C. Francile , A. Gabovich , E. Gorbovskoy , I. Gorbunov , O. Gress , V. Kornilov , A. Kuznetsov , A. Iyudin , R. Podesta , F. Podesta , R. Rebolo Lopez , V. Senik , M. Sierra-Rucart , S. Svertilov , N. Tiurina , D. Vlasenko , I. Yashin , K. Zhirkov , S. Croft , D. L. Kaplan , G. E. Anderson , A. Williams , D. Dobie , K. W. Bannister , P. J. Hancock , P. A. Evans , J. A. Kennea , J. P. Osborne , S. B. Cenko , S. Antier , J. L. Atteia , M. Boër , A. Klotz , S. Chaty , K. Hodapp , V. Savchenko

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.…

高能天体物理现象 · 物理学 2012-08-27 ANTARES collaboration

A method to search for neutrino induced showers from gamma-ray bursts in the ANTARES detector is presented. ANTARES consists of a three-dimensional array of photosensitive devices that measure Cherenkov light induced by charged particles…

高能天体物理现象 · 物理学 2015-05-27 Eleonora Presani

This paper briefly summarizes the search for astronomical sources of high-energy neutrinos using the AMANDA-B10 detector. The complete data set from 1997 was analyzed. For E_mu>10 TeV, the detector exceeds 10,000 m^2 in effective area…

天体物理学 · 物理学 2014-10-13 E. Andres , P. Askebjer , X. Bai , G. Barouch , S. W. Barwick

Recently different experiments mention to have observed a large scale cosmic-ray anisotropy at TeV energies, e.g. Milagro, Tibet and Super-Kamiokande. For these energies the cosmic-rays are expected to be nearly isotropic. Any measurements…

天体物理仪器与方法 · 物理学 2019-08-13 Salvatore Mangano

This paper describes the search for astronomical sources of high-energy neutrinos using the AMANDA-B10 detector, an array of 302 photomultiplier tubes, used for the detection of Cherenkov light from upward traveling neutrino-induced muons,…

天体物理学 · 物理学 2008-11-26 J. Ahrens , X. Bai , G. Barouch , S. W. Barwick

Relic neutralinos produced after the Big Bang are favoured candidates for Dark Matter. They can accumulate at the centre of massive celestial objects like our Sun. Their annihilation can result in a high-energy neutrino flux that could be…

天体物理学 · 物理学 2019-08-13 Gordon Lim

AMANDA-II is the largest neutrino telescope collecting data at the moment, and its main goal is to search for sources of high energy extra-terrestrial neutrinos. The detection of such sources could give non-controversial evidence for the…

天体物理学 · 物理学 2019-08-14 Paolo Desiati

The ANTARES neutrino telescope is being constructed at a site off the French Mediterranean coast at a depth of 2400m. When high energy neutrinos interact in water, the charged secondary particles produce Cherenkov light which can be…

天体物理学 · 物理学 2009-09-29 Bettina Hartmann