Fig. B.1.
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Left to right: SFR comparisons of Hα versus SFR10 Myr, [C II] at 158 μm versus SFR100 Myr, IR versus SFR 100Myr, and (UV + IR) versus SFR 100Myr for galaxies in the NEWCLUSTER (black squares) and NEWHORIZON (red circles) simulations. Each row corresponds to the different viewing angles: face-on, 30°, 60°, and edge-on (top to bottom). The solid gray line is the identity line, while the dashed, dotted and dash-dot lines indicate offsets of ±0.3, ±0.7, and ±1 dex, respectively. On the top left corner of each plot, the dispersion of the entire sample is shown.
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