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

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

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ANTARES Collaboration; Aguilar Sánchez, Juan Antonio; Bigongiari, C.; Dornic, Damien; Emanuele, U.; Gómez González, Juan Pablo; Hernández Rey, Juan José; Mangano, Salvatore; Salesa Greus, Francisco; Toscano, S.; Yepes Ramírez, Harold; Zornoza Gómez, Juan de Dios; Zúñiga Román, Juan

Aquest document és un/a article, creat/da en: 2010

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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