The ANTARES optical beacon system

M. Ageron,J.A. Aguilar,A. Albert,F. Ameli, M. Anghinolfi,G. Anton,S. Anvar,F. Ardellier-Desages,E. Aslanides, J-J. Aubert,R. Auer,E. Barbarito, S. Basa,M. Battaglieri,Y. Becherini,J. Beltramelli,V. Bertin,A. Bigi,M. Billault,R. Blaes,N. de Botton,M.C. Bouwhuis,S.M. Bradbury,R. Bruijn,J. Brunner,G.F. Burgio,J. Busto,F. Cafagna,L. Caillat,A. Calzas,A. Capone,L. Caponetto,Edward A Carmona,J. Carr,S.L. Cartwright,D. Castel,E. Castorina,V. Cavasinni,S. Cecchini,A. Ceres,P. Charvis,P. Chauchot,T. Chiarusi, M. Circella,C. Colnard,Chantal Compere,R. Coniglione,N. Cottini,P. Coyle,S. Cuneo,A-S. Cussatlegras,G. Damy,R. van Dantzig,G. De Bonis,C. De Marzo,R. De Vita,I. Dekeyser,E. Delagnes,D. Denans,A. Deschamps,J-J. Destelle,B. Dinkespieler,C. Distefano,C. Donzaud,J-F. Drogou,F. Druillole,Dominique M Durand,J-P. Ernenwein,S. Escoffier,E. Falchini,S. Favard,F. Fehr,F. Feinstein,S. Ferry,Catherine A Fiorello,V. Flaminio,K. Fratini,J-L. Fuda,S. Galeotti,J-M. Gallone,G. Giacomelli,N. Girard,C. Gojak,Ph. Goret,K. Graf,G D Hallewell,M.N. Harakeh,B. Hartmann,A. Heijboer,E. Heine,Y. Hello,J.J. Hernández-Rey,J. Hößl,C M Hoffman,J. Hogenbirk,J.R. Hubbard,M. Jaquet,Monique W M Jaspers,M. de Jong,F. Jouvenot,N. Kalantar-Nayestanaki,A. Kappes,T. Karg,U F Katz,Pernille Keller,E. Kok,H. Kok,P P Kooijman,C. Kopper,E.V. Korolkova,A. Kouchner,W. Kretschmer,A. Kruijer,S. Kuch,V.A. Kudryavstev,P. Lagier,R. Lahmann,G. Lamanna,P. Lamare,G. Lambard,J-C. Languillat,H. Laschinsky,Julien Lavalle,Y. Le Guen,H. Le Provost,A. Le Van Suu,D. Lefèvre,Thierry Legou,G. Lelaizant,Gordon Lim,D. Lo Presti,H. Loehner,S. Loucatos,F. Louis,F. Lucarelli,V. Lyashuk,M. Marcelin,A. Margiotta,R. Masullo,F. Mazéas,A. Mazure,J.E. McMillan,R. Megna,M. Melissas,E. Migneco,A. Milovanovic,M. Mongelli,T. Montaruli,M. Morganti,L. Moscoso,M. Musumeci,M. Naumann-Godo,C L Naumann,V. Niess,Tommy A Noble,C. Olivetto,R. Ostasch,N. Palanque-Delabrouille,P. Payre,H. Peek,A. Perez,C. Petta,P. Piattelli,R. Pillet,J-P. Pineau,J. Poinsignon,V. Popa,T. Pradier,C. Racca,N. Randazzo,J. van Randwijk,D E Real,B. van Rens,F. Réthoré,P. Rewiersma,G. Riccobene,Vincent Rigaud,M. Ripani,V. Roca, C. Roda,J.F. Rolin,H.J. Rose,A. Rostovtsev,Jakobus A Le Roux,M. Ruppi,G.V. Russo,G. Rusydi,F. Salesa,K. Salomon,P. Sapienza,Felix Schmitt,J-P. Schuller,R. Shanidze,I A Sokalski,T. Spona,M. Spurio,G. van der Steenhoven,T. Stolarczyk,K. Streeb,L. Sulak,M. Taiuti,Christian Tamburini,C. Tao,G. Terreni,L.F. Thompson,F. Urbano,P. Valdy,Vera L S Valente,B. Vallage,G. Vaudaine,G. Venekamp,B. Verlaat,P. Vernin, G. de Vries-Uiterweerd,R. van Wijk,G. Wijnker,P. de Witt Huberts,G. Wobbe,E. de Wolf,A-F. Yao,D. Zaborov,H. Zaccone,J.D. Zornoza,J. Zúñiga

Nuclear Instruments and Methods in Physics Research Section A: Accelerators, Spectrometers, Detectors and Associated Equipment(2007)

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摘要
ANTARES is a neutrino telescope being deployed in the Mediterranean Sea. It consists of a three-dimensional array of photomultiplier tubes that can detect the Cherenkov light induced by charged particles produced in the interactions of neutrinos with the surrounding medium. High angular resolution can be achieved, in particular, when a muon is produced, provided that the Cherenkov photons are detected with sufficient timing precision. Considerations of the intrinsic time uncertainties stemming from the transit time spread in the photomultiplier tubes and the mechanism of transmission of light in sea water lead to the conclusion that a relative time accuracy of the order of 0.5ns is desirable. Accordingly, different time calibration systems have been developed for the ANTARES telescope. In this article, a system based on Optical Beacons, a set of external and well-controlled pulsed light sources located throughout the detector, is described. This calibration system takes into account the optical properties of sea water, which is used as the detection volume of the ANTARES telescope. The design, tests, construction and first results of the two types of beacons, LED and laser-based, are presented.
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95.55.Vj,95.85.Ry
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