Distribution of Lyα emission luminosities for our sample (thick cyan), LAEs (magenta), and radio galaxies (filled yellow). Cross-hatched magenta shading denotes LAEs that have an AGN contribution (3). Cyan shading indicates quasars in our sample that are also radio-loud (4). The inset shows the K-S test cumulative fraction out to 120 × 10⁴²  erg  s^-1 with the same color scheme. The cumulative fraction distribution is scaled for a comparison between our sample and LAEs and is truncated for the radio galaxies.