@Article{ANTARESCollaborationAguilar_etal2011,
author="ANTARES Collaboration (Aguilar, J. A. et al
and Bigongiari, C.
and Dornic, D.
and Emanuele, U.
and Gomez-Gonzalez, J. P.
and Hernandez-Rey, J. J.
and Mangano, S.
and Salesa, F.
and Toscano, S.
and Yepes, H.
and Zornoza, J. D.
and Zu{\~{n}}iga, J.",
title="Time calibration of the ANTARES neutrino telescope",
journal="Astroparticle Physics",
year="2011",
publisher="Elsevier Science Bv",
volume="34",
number="7",
pages="539--549",
optkeywords="Time calibration; Neutrino telescopes; ANTARES",
abstract="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 similar to 1 ns. The methods developed to attain this level of precision are described.",
optnote="ISI:000287955500004",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=560), last updated on Thu, 09 Jul 2020 11:13:20 +0000",
issn="0927-6505",
doi="10.1016/j.astropartphys.2010.12.004",
opturl="http://arxiv.org/abs/arXiv:1012.2204",
opturl="https://doi.org/10.1016/j.astropartphys.2010.12.004",
archivePrefix="arXiv",
eprint="arXiv:1012.2204",
language="English"
}