Fig. 5.

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Dust-attenuated UV luminosity function in SPHINX-SN (red) and SPHINX-CR (dark blue), with Poissonian error-bars. From the top left to the bottom right panel, we show increasing redshift from 5 to 10. The references of the observations shown in each panel are written in the legend. At any time, the UV luminosity functions of the two simulations are very similar and consistent with the observational constraints.
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