Fig. 13.
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Figure showing the MZR predicted by the EAGLE and TNG hydrodynamical simulations. Left: stellar MZR of star-forming galaxies at z ∼ 3 selected from the Eagle hydrodynamical simulation sets (Ref. L0100N1504) as a function of the total mass of their host haloes from 1010 to 1014 M⊙. Right: same as the left panel, but for the Illustris-TNG100 simulation.
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