Radial velocities compared to their reference values, where ReDetermineApHotStars has been applied to the hotter stars. Top left panel: bias of the radial velocity of the stars (RVS value minus reference value). It should be compared to the equivalent plot in Fig. 4 to see the improvement due to ReDetermineApHotStars. The dashed blue lines indicate ±3 km s⁻¹. Top right panel: median of the radial velocity bias of stars in the T_eff = 8500 − 14 500 K range, binned in one-magnitude-wide (grvs_mag) bins. The relation between the two is fitted linearly (red line). Applying the magnitude-related correction leads to an improved set of radial velocities, which are once again compared to their reference values (bottom left panel). The precision of these improved values is shown in the bottom right panel. Similarly to Fig. 4, the blue symbols give the external precision, and the red symbols give the internal precision. All plots include only stars with grvs_mag ≤ 12 mag.