Fig. 7.
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Stellar mass as a function of M200 for the central galaxies of haloes with M* ≥ 108 M⊙ for the all analysed simulations (see labels in the inset). For comparison, the relation proposed by Guo et al. (2010) (dashed line and the extrapolation for halo masses lower than 1011.5 indicated by the solid line) and trend for the L4 Auriga galaxies (Grand et al. 2024) are also included (open, black circles).
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