  The ANTARES detector, completed in 2008, is the largest neutrino telescope in
the Northern hemisphere. It is located at a depth of 2.5 km in the
Mediterranean Sea, 40 km off the Toulon shore. The scientific scope of the
experiment is very broad, being the search for astrophysical neutrinos the main
goal. In this paper we collect the 22 contributions of the ANTARES
collaboration to the 32nd International Cosmic Ray Conference (ICRC 2011). At
this stage of the experiment the scientific output is very rich and the
contributions included in these proceedings cover the main physics results
(steady point sources, correlations with GRBs, diffuse fluxes, target of
opportunity programs, dark matter, exotic physics, oscillations, etc.) and some
relevant detector studies (water optical properties, energy reconstruction,
moon shadow, accoustic detection, etc.)
