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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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 Perfil; 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.

    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 2010 Zenith distribution and flux of atmospheric muons measured with the 5-line ANTARES detector Astroparticle Physics 34 3 179 184
http://dx.doi.org/10.1016/j.astropartphys.2010.07.001
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