Fig. 8
From top to bottom: normalised distributions (solid line for LAMOST DA/M binaries, dashed line for SDSS DA/M binaries) of distance, white dwarf mass, effective temperature and surface gravity, spectral type of the companion star and g − r colour. Kolmogorov-Smirnov probabilities resulting from comparing the stellar parameter determinations from both samples are indicated in the right panels.
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