This catalogue accompanies our article (Naik & Widmark, 2022), in which we demonstrate the use of Bayesian neural networks for predicting the missing radial (line-of-sight) velocities of stars obs
Gaia astrometry of nearby stars is precise enough to detect the tiny displacements induced by substellar companions, but radial velocity (RV) data are needed for definitive...
The Hundred-Thousand-Proper-Motion (HTPM) project will determine the proper motions of ~113500 stars using a ~23-year baseline. The proper motions will be based on space-based...
