Predicted UV LFs at low (upper) and intermediate (lower) redshift. We show the LFs using the calibration (see Section 2.3) at z ∼ 5 from Bouwens et al. (2015a), with Planck 2015 cosmology (Planck Collaboration et al. 2015), with Planck 2015 cosmology (Planck Collaboration et al. 2015). Points show the binned UV LFs and upper limits from Arnouts et al. (2005), Alavi et al. (2014), Oesch et al. (2010), Bouwens et al. (2015a), Finkelstein et al. (2015a), Bowler et al. (2015), Atek et al. (2015a). We note that the data from Atek et al. (2015a) were made public after our model was submitted and illustrates the consistency of our model with observations even at very low luminosity. Shaded regions show the 1σ confidence range.