Gaia G magnitude distribution of dwarfs with good parallax (f ≤ 0.2) removed using CaMD cuts shown in Figure 2 before applying the magnitude cut. We can see that our magnitude cut falls just before the distribution falls off due to incompleteness in magnitudes where dwarfs do not have good parallaxes (f ≤ 0.2) (in orange). Selected stars’ distribution used for the CaMD cut is shown in blue.