Milky Way GCs coverage with MOCCA models for 2D N_SG/N_TOT (Milone et al. 2017a) ratios computed as a cumulative value for different radii (scaled to r_hl). Every line correspond to one MOCCA simulation. The selected MOCCA models are the same as in Figures 2 and A.1. The N_SG/N_TOT ratios are colored according to whether they were initially TF or TuF. Only for a few models is there a large difference for N_SG/N_TOT ratios between small and large radial distances (for those closer to dissolution). For the majority of the models there is no significant difference for N_SG/N_TOT ratios between those measured in the very center and those measured around r_hl radius. For details see Section 4.