  The ANTARES collaboration completed the installation of the first neutrino
detector in the sea in 2008. It consists of a three dimensional array of 885
photomultipliers to gather the Cherenkov photons induced by relativistic muons
produced in charged-current interactions of high energy neutrinos close to/in
the detector. The scientific scope of neutrino telescopes is very broad: the
origin of cosmic rays, the origin of the TeV photons observed in many
astrophysical sources or the nature of dark matter. The data collected up to
now have allowed us to produce a rich output of physics results, including the
map of the neutrino sky of the Southern hemisphere, search for correlations
with GRBs, flaring sources, gravitational waves, limits on the flux produced by
dark matter self-annihilations, etc. In this paper a review of these results is
presented.
