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The ANTARES telescope is being built in the Mediterranean Sea. The detectorconsists of a 3D array of photomultipliers (PMTs) that detects the Cherenkovlight induced by the muons produced in neutrino interactions. Other signaturescan also be detected. Since the neutrino fluxes from point-like sources areexpected to be small, it is of the utmost importance to take advantage of theANTARES pointing accuracy (angular resolution better than 0.3 degrees for muonevents above 10 TeV) to disentangle a possible signal from the unavoidableatmospheric neutrino background. In order to distinguish an excess of neutrinoevents from the background, several searching algorithms have been developedwithin the ANTARES collaboration. In this contribution, the discovery potentialand sensitivity to point-like sources of the ANTARES neutrino telescope arepresented.

Expected discovery potential and sensitivity of the ANTARES neutrino telescope to neutrino point-like sources