  ANTARES is the largest neutrino telescope in the Northern hemisphere. The
main scientific goal is the search for cosmic neutrinos coming from galactic
and extragalactic sources. Neutrinos are detected through the Cherenkov light
emitted along the path of charged particles produced in neutrino interactions
inside or in the vicinity of the detector. ANTARES is sensitive to all flavors
though it is optimized for muon neutrinos. The detector has been taking data in
its complete configuration since May 2008.
  Using data collected in the period 2007-2010, the first analysis devoted to
the search for neutrinos from the Fermi Bubbles is presented. The Fermi Bubbles
are characterized by gamma emission with a E^{-2} spectrum and a relatively
constant intensity all over the space. According to a proposed hadronic
mechanism for this gamma-ray emission, the Fermi Bubbles can be a source of
high-energy neutrinos. No evidence of a neutrino signal is found in the ANTARES
data. Therefore upper limits are calculated for neutrino fluxes with different
energy cutoffs.

High Energy Astrophysical Phenomena