Fig. B.1
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Offset between the uncalibrated Gaia XP radial velocities and reference ones as a function of BP − RP colour. We split the dwarfs and the giants using the log g measurements from Zhang et al. (2023). The dashed vertical line shows the limit above which we used two bins in log g for our calibration model. The figure only includes sources with E(B−V) < 0.1 and 12 < G < 13.
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