TY  - JOUR
AU  - ANTARES Collaboration (Aguilar, J. A. et al
AU  - Bigongiari, C.
AU  - Dornic, D.
AU  - Emanuele, U.
AU  - Gomez-Gonzalez, J. P.
AU  - Hernandez-Rey, J. J.
AU  - Mangano, S.
AU  - Salesa, F.
AU  - Toscano, S.
AU  - Yepes, H.
AU  - Zornoza, J. D.
AU  - Zuñiga, J.
PY  - 2010
DA  - 2010//
TI  - Zenith distribution and flux of atmospheric muons measured with the 5-line ANTARES detector
T2  - Astropart Phys.
JO  - Astroparticle Physics
SP  - 179
EP  - 184
VL  - 34
IS  - 3
PB  - Elsevier Science Bv
KW  - Atmospheric muons
KW  - Neutrino telescope
KW  - Depth-intensity relation
AB  - 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.
SN  - 0927-6505
UR  - http://arxiv.org/abs/1007.1777
UR  - https://doi.org/10.1016/j.astropartphys.2010.07.001
DO  - 10.1016/j.astropartphys.2010.07.001
LA  - English
N1  - ISI:000282496000005
ID  - ANTARESCollaborationAguilar_etal2010
ER  -