Comparison of our mass estimates on the AstroSpectro300 sample when not using the spectroscopic measurement with mass estimates from Gaia Collaboration (2023a), which adopted a primary mass and then used the astrometry and the spectroscopy to estimate the secondary mass. The two panels show the primaries (left) and secondaries (right), both with 9674 stars. The horizontal and vertical axes do not span a common range in each panel.