%0 Journal Article
%T Zenith distribution and flux of atmospheric muons measured with the 5-line ANTARES detector
%A ANTARES Collaboration (Aguilar, J. A. et al
%A Bigongiari, C.
%A Dornic, D.
%A Emanuele, U.
%A Gomez-Gonzalez, J. P.
%A Hernandez-Rey, J. J.
%A Mangano, S.
%A Salesa, F.
%A Toscano, S.
%A Yepes, H.
%A Zornoza, J. D.
%A Zuñiga, J.
%J Astroparticle Physics
%D 2010
%V 34
%N 3
%I Elsevier Science Bv
%@ 0927-6505
%G English
%F ANTARESCollaborationAguilar_etal2010
%O ISI:000282496000005
%O exported from refbase (https://references.ific.uv.es/refbase/show.php?record=373), last updated on Thu, 09 Jul 2020 11:12:51 +0000
%X 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.
%K Atmospheric muons
%K Neutrino telescope
%K Depth-intensity relation
%R 10.1016/j.astropartphys.2010.07.001
%U http://arxiv.org/abs/1007.1777
%U https://doi.org/10.1016/j.astropartphys.2010.07.001
%P 179-184