Updated version of the normalised, cumulative radial distributions as a function of the dynamical age (Figure 15 from Leitinger et al. (2023)), including the two additional GCs, NGC 104 and NGC 6656. We have used updated dynamical ages from Baumgardt et al. (2023b), that change the sample of the ‘dynamically young’ clusters of our sample by removing NGC 2808 and NGC 7078, as the updated dynamical ages of these clusters now exceed age/T_rh > 4.5. Please note that the colour-coding of the clusters in this figure do not correspond to the same colour-coding in Figure 15 of Leitinger et al. (2023).