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.
| Original language | English |
|---|---|
| Pages (from-to) | 179-184 |
| Number of pages | 6 |
| Journal | Astroparticle Physics |
| Volume | 34 |
| Issue number | 3 |
| DOIs | |
| State | Published - Oct 2010 |
| Externally published | Yes |
Keywords
- Atmospheric muons
- Depth-intensity relation
- Neutrino telescope
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