2025ApJS..280...61A

We combine absolute astrometry from Hipparcos and Gaia with archival radial velocities from the Keck/HIRES and ESO/HARPS spectrographs, as well as relative astrometry (when available), to derive masses and orbits for 156 companions around main-sequence stars, including 111 stellar companions, 12 brown dwarfs, and 33 planets. Although this sample is not compiled for occurrence rate statistics due to systematic biases in nonuniform target selection and varied observing strategies, we nonetheless clearly detect the brown dwarf desert in the distribution of companion masses (as well as in mass ratio), out to separations of ≳10 au. This work also enables a validation of Gaia DR3 non-single-star solutions by predicting Gaia's measured R.A. and decl. acceleration terms. For stars with Gaia astrometric acceleration solutions, we find qualitative agreement with Gaia DR3 results. Our predicted accelerations agree with the Gaia DR3 values overall, showing a median offset of 1.85σ, with a tail extending to ≈10σ. These residuals suggest modestly underestimated uncertainties, broadly consistent with previous results for parallaxes and proper motions. Three of our systems have full Gaia orbital fits; however, their true orbital periods are long, and all three Gaia solutions are spurious. Gaia DR4 will provide individual astrometric measurements and enable more detailed and extensive investigations of accelerating and orbital fits.