Skymap for atmospheric muons at TeV energies measured in deep-sea neutrino telescope ANTARES

Astronomy and Astrophysics – Astrophysics – Instrumentation and Methods for Astrophysics

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Proceedings of the 31st ICRC conference, Lodz 2009, 3 pages, 2 figures

Scientific paper

Recently different experiments mention to have observed a large scale cosmic-ray anisotropy at TeV energies, e.g. Milagro, Tibet and Super-Kamiokande. For these energies the cosmic-rays are expected to be nearly isotropic. Any measurements of cosmic-rays anisotropy could bring some information about propagation and origin of cosmic-rays. Though the primary aim of the ANTARES neutrino telescope is the detection of high energy cosmic neutrinos, the detector measures mainly down-doing muons, which are decay products of cosmic-rays collisions in the Earth's atmosphere. This proceeding describes an anlaysis method for the first year measurement of down-going atmospheric muons at TeV energies in the ANTARES experiment, when five out of the final number of twelve lines were taking data.

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