  The ANTARES deep sea neutrino telescope has been taking data continuously
since its completion in 2008. With its excellent view of the Galactic plane and
good angular resolution the telescope can constrain the origin of the diffuse
astrophysical neutrino flux reported by IceCube. Assuming various spectral
indices for the energy spectrum of neutrino emitters, the Southern sky and in
particular central regions of our Galaxy have been studied searching for
point-like objects, for extended regions of emission, and for signal from
transient objects selected through multi-messenger observations. For the first
time, cascade events are used for these searches.
  ANTARES has also provided results on searches for hypothetical particles
(such as magnetic monopoles and nuclearites in the cosmic radiation), and
multi-messenger studies of the sky in combination with various detectors. Of
particular note are the searches for dark matter: the limits obtained for the
spin-dependent WIMP-nucleon cross section surpassing those of current
direct-detection experiments.
