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Fig. 10.

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Predictions of UVLF out to z = 13 from our model constrained on z < 8 data and compared to measurements from the literature. The solid lines correspond to the model evaluated at different redshifts from the best-fit linear redshift dependence of the model parameters fit on 4 ≲ z ≲ 8 data. The dashed and dotted lines illustrate the two extreme scenarios of increasing SFE versus increasing stochasticity and show the model where we tune by hand ϵ0 and σUV to approximately match the observations, while keeping the other parameters nominal. The filled area shows the effect of dust attenuation on the UVLF, with the upper thin lines marking the unatenuated UVLF.

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