  While the number of exoplanets discovered continues to increase at a rapid
rate, we are still to discover any system that truly resembles the Solar
system. Existing and near future surveys will likely continue this trend of
rapid discovery. To see if these systems are Solar system analogues, we will
need to efficiently allocate resources to carry out intensive follow-up
observations. We seek to uncover the properties and trends across systems that
indicate how much of the habitable zone is stable in each system to provide
focus for planet hunters. We study the dynamics of all known single Jovian
planetary systems, to assess the dynamical stability of the habitable zone
around their host stars. We perform a suite of simulations of all systems where
the Jovian planet will interact gravitationally with the habitable zone, and
broadly classify these systems. Besides the system's mass ratio (Mpl/Mstar),
and the Jovian planet's semi-major axis (apl) and eccentricity (epl), we find
that there are no underlying system properties which are observable that
indicate the potential for planets to survive within the system's habitable
zone. We use Mpl/Mstar, apl and epl to generate a parameter space over which
the unstable systems cluster, thus allowing us to predict which systems to
exclude from future observational or numerical searches for habitable
exoplanets. We also provide a candidate list of 20 systems that have completely
stable habitable zones and Jovian planets orbiting beyond the habitable zone as
potential first order Solar system analogues.
