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Fig. 6

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Signal-to-noise ratio in the Gaia EDR3 parallax (SNRϖEDR3${\rm{SN}}{{\rm{R}}_{{\varpi _{{\rm{EDR3}}}}}}$) used as a prior versus the de-reddened r band apparent magnitude (r^$\hat r$) for the white dwarf sample. The black dots show individual measurements. The red areas, from lighter to darker, enclose 90%, 50%, and 10% of the sources, respectively. The dashed gray line marks SNRϖEDR3=3${\rm{SN}}{{\rm{R}}_{{\varpi _{{\rm{EDR3}}}}}} = 3$.

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