@Article{ANTARESCollaborationAguilar_etal2010,
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="Zenith distribution and flux of atmospheric muons measured with the 5-line ANTARES detector",
journal="Astroparticle Physics",
year="2010",
publisher="Elsevier Science Bv",
volume="34",
number="3",
pages="179--184",
optkeywords="Atmospheric muons; Neutrino telescope; Depth-intensity relation",
abstract="The ANTARES high-energy neutrino telescope is a three-dimensional array of about 900 photomultipliers distributed over 12 mooring lines installed in the Mediterranean Sea. Between February and November 2007 it acquired data in a 5-line configuration. The zenith angular distribution of the atmospheric muon flux and the associated depth-intensity relation are measured and compared with previous measurements and Monte Carlo expectations. An evaluation of the systematic effects due to uncertainties on environmental and detector parameters is presented.",
optnote="ISI:000282496000005",
optnote="exported from refbase (https://references.ific.uv.es/refbase/show.php?record=373), last updated on Thu, 09 Jul 2020 11:12:51 +0000",
issn="0927-6505",
doi="10.1016/j.astropartphys.2010.07.001",
opturl="http://arxiv.org/abs/1007.1777",
opturl="https://doi.org/10.1016/j.astropartphys.2010.07.001",
archivePrefix="arXiv",
eprint="1007.1777",
language="English"
}