Corrected individual parallaxes as a function of G for the Villafranca O-021 (NGC 2362) stars selected by the membership algorithm using parallaxes from (left) Gaia DR2 with Z_DR2 = −40 μas, (middle) Gaia EDR3 with the Lindegren Z_EDR3 and the k from Maíz Apellániz et al. (2021e), and (right) Gaia EDR3 with the new Z_EDR3 and the k from the companion paper. Red symbols are used for the eight stars used to calculate the distance to the cluster in Maíz Apellániz & Barbá (2020). The green point with the large error bar near the left edge in the Gaia EDR3 plots corresponds to (the not selected) τ CMa Aa,Ab (the star is not present in Gaia DR2). The horizontal blue lines show the (corrected) group parallax (with the one sigma range plotted with dotted lines) calculated with each dataset.