Following the discovery of 51 Pegasi b, the CORALIE spectrograph on the 1.2 meter Leonhard Euler telescope was commissioned in 1998, order to continue searching for exoplanets around Sun-like stars. Since then, CORALIE has continually measured the radial velocities (RVs) of over 1600 FGK-type stars. This 25+ year baseline of RV data provides orbital coverage for exoplanets and brown dwarfs that lie at wide separations (10s of AU) from their host stars. Such companions also induce astrometric perturbations on their host stars, that can be detected in astrometry surveys such as Hipparcos and Gaia. By combining RV and Hipparcos-Gaia proper motion anomaly (PMa) data in orbit fits, we are able to overcome the mass-inclination degeneracy inherent to RV data. We therefore present the precise dynamical masses of 5 gas giant exoplanets, 3 of which are in multiplanetary systems. Additionally, with the results from our RV + PMa orbit fits for all 1600+ targets, we are able to determine the feasibility of detecting numerous companions in direct imaging. This includes companions we have already imaged with SPHERE on VLT, as well as prospects for other direct imaging instruments.