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Time Calibration of the ANTARES Neutrino Telescope

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arxiv 1012.2204 v1 pith:C7YLQJJJ submitted 2010-12-10 astro-ph.IM hep-exphysics.ins-det

Time Calibration of the ANTARES Neutrino Telescope

The ANTARES Collaboration: J.A. Aguilar , I. Al Samarai , A. Albert , M. Andr\'e , M. Anghinolfi , G. Anton , S. Anvar , M. Ardid
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A.C. Assis Jesus T. Astraatmadja J.J. Aubert R. Auer B. Baret S. Basa M. Bazzotti V. Bertin S. Biagi C. Bigongiari M. Bou-Cabo M.C. Bouwhuis A. M. Brown J. Brunner J. Busto F. Camarena A. Capone C.Carloganu G. Carminati J. Carr S. Cecchini Ph. Charvis T. Chiarusi M. Circella H. Costantini N. Cottini P. Coyle C. Curtil M.P. Decowski I. Dekeyser A. Deschamps C. Distefano C. Donzaud D. Dornic D. Drouhin T. Eberl U. Emanuele J.P. Ernenwein S. Escoffier F. Fehr V. Flaminio U. Fritsch J.L. Fuda S. Galata P. Gay G. Giacomelli J.P. G\'omez-Gonz\'alez K. Graf G. Guillard G. Halladjian G. Hallewell H. van Haren A.J. Heijboer Y. Hello J.J. Hern\'andez-Rey B. Herold J. H\"ossl C.C. Hsu M. de Jong M. Kadler N. Kalantar-Nayestanaki O. Kalekin A. Kappes U. Katz P. Kooijman C. Kopper A. Kouchner V. Kulikovskiy R. Lahmann P. Lamare G. Larosa D. Lef\`evre G. Lim D. Lo Presti H. Loehner S. Loucatos F. Lucarelli S. Mangano M. Marcelin A. Margiotta J.A. Martinez-Mora A. Mazure T. Montaruli M. Morganti L. Moscoso H. Motz C. Naumann M. Neff D. Palioselitis G.E.Pavalas P. Payre J. Petrovic P. Piattelli N. Picot-Clemente C. Picq V. Popa T. Pradier E. Presani C. Racca C. Reed G. Riccobene C. Richardt M. Rujoiu G.V. Russo F. Salesa P. Sapienza F. Sch\"ock J.P. Schuller R. Shanidze F. Simeone A. Spies M. Spurio J.J.M. Steijger Th. Stolarczyk M. Taiuti C. Tamburini L. Tasca S. Toscano B. Vallage V. Van Elewyck G. Vannoni M. Vecchi P. Vernin G. Wijnker E. de Wolf H. Yepes D. Zaborov J.D. Zornoza J. Z\'u\~niga
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classification astro-ph.IM hep-exphysics.ins-det
keywords neutrinocalibrationtimeantareslevellightphotomultiplierstelescope
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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The ANTARES deep-sea neutrino telescope comprises a three-dimensional array of photomultipliers to detect the Cherenkov light induced by upgoing relativistic charged particles originating from neutrino interactions in the vicinity of the detector. The large scattering length of light in the deep sea facilitates an angular resolution of a few tenths of a degree for neutrino energies exceeding 10 TeV. In order to achieve this optimal performance, the time calibration procedures should ensure a relative time calibration between the photomultipliers at the level of about 1ns. The methods developed to attain this level of precision are described.

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