Systematic shift of the average mass and radii dispersion for different groups of stars. The first row reports the non-shifted values, which are also reported as transparent points in each panel. Each row past the first one explores the effects of a shift in a given parameter of its 1σ interval, as labelled. The last two rows report the non-corrected mass and dispersion average values, and what happens when the Temperatures coming from the B − V bands are used. The dashed lines represent the mass derived from the EB results in Kaluzny et al. (2013, 0.85M_⊙, first column); the mass of the 1G, the 2G, and the HB from; Tailo et al. (2019, the values are 0.85M_⊙, 0.833M_⊙, and 0.64M_⊙ for the second to fourth columns, respectively); and the shaded areas mark their 1σ intervals.