Figure to replace Fig. 7a–c in Moehler et al. (2000b, NGC 6752). Temperatures and masses (derived from Buonanno et al.’s photometry) of the programme stars in NGC 6752. a) Determined using model atmospheres with cluster metallicity ([M/H] = −1.5), b) adopting a solar metallicity ([M/H] = 0) for the model atmospheres, c) adopting a super–solar metallicity ([M/H] = +0.5) for the model atmospheres. For more details see Sect. 4.1 [of the original paper]. The dashed resp. solid lines mark the ZAHB masses for a metallicity [M/H] = −1.54, as computed with and without mixing, respectively. (see Sect. 4.2 and Fig. 4 [of the original paper] for details).