Top panel: Distribution of G magnitudes for the sample of stars with distances d = 1 /ϖ < 200 pc (solid line histograms) and distances d_pg < 200 pc from Bailer-Jones et al. (2021) (shaded histograms). The blue histograms represent the S and S_pg samples. The red histograms represent the S_NYMG and S_NYMGpg samples, as explained in Sect. 2.1. Middle panel: Residuals of the number of sources between S_NYMG and S _NYMGpg (red) and between S and S_pg (blue) as a function of G. Bottom panel: Same residuals as the middle panel, shown as a function of the photometric S/N of G. All error bars correspond to the propagated Poisson error.