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Recently different experiments mention to have observed a large scalecosmic-ray anisotropy at TeV energies, e.g. Milagro, Tibet andSuper-Kamiokande. For these energies the cosmic-rays are expected to be nearlyisotropic. Any measurements of cosmic-rays anisotropy could bring someinformation about propagation and origin of cosmic-rays. Though the primary aimof the ANTARES neutrino telescope is the detection of high energy cosmicneutrinos, the detector measures mainly down-doing muons, which are decayproducts of cosmic-rays collisions in the Earth's atmosphere. This proceedingdescribes an anlaysis method for the first year measurement of down-goingatmospheric muons at TeV energies in the ANTARES experiment, when five out ofthe final number of twelve lines were taking data.

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