Fig. A.2.

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Fractions of each component from the MCMC modelling, described in Section 3.1, for objects with −0.3 < (g − r) < − 0.05 and −0.14 < grz < 0.07 in the LSDR9-Gaia EDR3 crossmatch. The BHB Gaussian component has a hard prior for the mean and standard deviation. The dark/light markers are the fractions for a given g interval when white dwarf candidates are excluded/included. The white dwarf contamination in the BHB fractions is negligible throughout g.
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