Computed diameters as a function of measured diameters, for eight stars recently observed with interferometry and not used for the polynomial fit. Stars with increasing diameter, HD numbers: 209458 (G0V), 189733 (K1.5V), 69830 (G8), 185351 (G9III), 190658 (M2.5III), 183589 (K5I), 95687 (M3I), 97671 (M3I), (Johnson et al. 2014; Boffin et al. 2014; Tanner et al. 2015; Boyajian et al. 2015; Arroyo-Torres et al. 2015). The agreement is excellent, with a mean-squared difference between measured and computed diameters expressed in noise units of 0.5. The straight dotted line corresponds to x = y.