  The ANTARES neutrino telescope is installed at a depth of 2.5 km of the
Mediterranean Sea and consists of a three-dimensional array of 885
photomultipliers arranged on twelve detector lines. The prime objective is to
detect high-energy neutrinos from extraterrestrial origin. Relativistic muons
emerging from charged-current muon neutrino interactions in the detector
surroundings produce a cone of Cerenkov light which allows the reconstruction
of the original neutrino direction. The collaboration has implemented different
methods to search for neutrino point sources in the data collected since 2007.
Results obtained with these methods as well as the sensitivity of the telescope
are presented.
