Zenith distribution and flux of atmospheric muons measured with the 5-line ANTARES detector

Details Zenith distribution and flux of atmospheric muons measured with the 5-line ANTARES detector Zenith distribution and flux of atmospheric muons measured with the 5-line ANTARES detector

Oct 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aph....34..179a&link_type=abstract

Astroparticle Physics, Volume 34, Issue 3, p. 179-184.

Physics

12

Scientific paper

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.

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