Fig. D.1.
Stellar-to-dark matter ratios at higher redshifts. Top: f⋆ vs. M⋆ for Auriga, EAGLE, and Illustris disc galaxies at z = 0.5. The dotted blue line denotes the relation determined using the Moster et al. (2018) abundance matching relation, and the shaded region denotes the 1σ scatter around the relation. Bottom: V⋆/Vtot for the galaxies shown in the top panel. Auriga is already locally more baryon-dominated than EAGLE and Illustris at higher redshifts.
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