Same as in Fig. 9 but for relics (95% > M_⋆ ≥ 75% at t_{BB = 3 Gyr} and t_75% <  3 Gyr). The systems are plotted in order of decreasing degree of relicness from top-left to bottom-right. Some indication for the presence of a second stellar population with younger ages and/or lower metallicity is visible in the density plots, especially in the bottom row, although the mass is still dominated by the pristine stars.