Left: Absolute UV magnitude as a function of redshift in the UDS sample. The 73 galaxies with robust S/N > 3 Lyα detection are shown in blue, while the rest of the population is shown in red. Right: Distribution of Lyα EW₀ as a function of M_UV. Galaxies in the UDS with S/N > 3 are shown as circles, while upper limits EW_0, lim are shown as triangles. They are color-coded by spectroscopic redshift. For comparison, we report CEERS-EGS emitters (gray squares) and upper limits (gray triangles) from Napolitano et al. (2024). The dashed black lines at M_UV = –20.25 and –18.75 define the bright and faint regimes. The UDS sample is complete down to M_UV = –18.25, indicated by the solid red line.