Comparison of our mass estimates on the Orbital300 sample using astrometry and photometry with those from Gaia Collaboration (2023a), which adopted a mass for the primary and then inferred the mass of the secondary from a variety of data (in many cases there is no secondary mass estimate). The two panels show the primaries (left, 19 603 stars) and secondaries (right, 1574 stars). A few sources lie outside the range of the plots.