Best-fit double power-law parameters for the UV LF in bins of redshift. We show the results obtained by leaving all four parameters free (green squares) and fixing the faint-end slope (β = −1.25, shown as a horizontal dashed blue line; blue circles). We compare our results with those of Kulkarni et al. (2019). Our results show a clear decrease in the value of the normalization parameter Φ^* with redshift, in line with the fitted Schechter parameter for the Lyα LF. The faint-end slope β also shows hints of a declining evolution, while the bright-end slope γ is poorly constrained by our data.