  Our knowledge of the Solar System, encourages us to beleive that we might
expect exomoons to be present around some of the known exoplanets. With present
hardware and existing optical astronomy methods we shall not be able to find
exomoons at least 10 years from now and even then, it will be a hard task to
detect them. Using data from the Exoplanet Orbit Database (EOD) we find stars
with Jovian exoplanets within 50 light years. Most of them will be fully
accessible by the new radio telescope, The Five-hundred-meter Aperture
Spherical radio Telescope (FAST) under construction, now in the test phase. We
suggest radio astronomy based methods to search for possible exomoons around
two exoplanets.
