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The Antares neutrino telescope, operating at 2.5 km depth in theMediterranean Sea, 40 km off the Toulon shore, represents the world's largestoperational underwater neutrino telescope, optimized for the detection ofCerenkov light produced by neutrino-induced muons. The main goal of Antares isthe search of high energy neutrinos from astrophysical point or transientsources. Antares is taking data in its full 12 lines configuration since May2008: in this paper we collect the 16 contributions by the ANTAREScollaboration that were submitted to the 31th International Cosmic RayConference ICRC 2009.  These contributions includes the detector performances, the first preliminaryresults on neutrino events and the current physics analysis including thesensitivity to point like sources, the possibility to detect high energyneutrinos in coincidence with GRB, the search for dark matter or exoticparticles.

The ANTARES Collaboration: contributions to the 31st International Cosmic Ray Conference (ICRC 2009), Lodz, Poland, July 2009