Image Details
Caption: Figure 5.
Face-value distribution of the WD sample members in the ﹩{N}_{{ \mathcal C }}({M}_{G},(B-R))﹩ plane, after all the selection function cuts summarized in Equation (8) have been applied. The units of this distribution are the number of objects/mag2.
© 2021. The Author(s). Published by the American Astronomical Society.