Of all the methods used for the detection of extra-solar planets, the radial velocity technique is still the dominant source of extra-solar planet discoveries. Furthermore, many of the planets discovered are hot Jupiters in 3-5 day orbits with ~10% chance of transiting their parent star. Thus many of the hot Jupiters discovered via radial velocity surveys are expected to also exhibit a photometric transit signature.

I will be presenting simulations of the expected results from a generic multi-object survey based on calculated noise models and sensitivity for the instrument and the known distribution of exoplanetary system parameters. Code has been developed for automatically sifting and fitting the planet candidates produced by the survey to allow for fast follow-up observations to be conducted. Considering the expected high number of hot Jupiters from the survey, a transit ephemeris is automatically calculated by the radial velocity code for each candidate and updated when new data becomes available. Early photometric follow-up of planet candidates during the predicted transit windows will indicate whether or not the planet's orbit is favourably inclined for transits to be visible. The techniques presented here may be applied to a wide range of radial velocity planet surveys.