Distribution of the 96 individual LAEs used in this study in redshift and absolute UV magnitude, colour-coded by lensing magnification. Redshifts quoted are spectroscopic from MUSE and magnitude values are derived from the filter that covers the rest frame 1500 Å emission. Horizontal dashed lines denote relevant limits: red denotes the M_UV limit in an equivalent blank field study (Kusakabe et al. 2020) and black denotes the integration limit used when calculating the star formation rate density from the UV luminosity function (LF) in the latest study (Bouwens et al. 2022b).