Fig. 10.

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Same as in Fig. 9 but for relics (95% > M⋆ ≥ 75% at tBB = 3 Gyr and t75% < 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.
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