Histograms of Lyα and LyC emission of our sample of 1933 galaxies. Top row: Lyα properties of our sample with intrinsic luminosity (left), escaping luminosity (middle), and escape fraction (right). Bottom row: same properties but for LyC radiation. In the middle panel of the top row, we also show the distribution of of galaxies observed in MUSE GTO surveys (MUSE galaxies are shown in green or, where at z > 6, in pink). The dashed lines show their respective median values. The luminosities have a peaked distribution, has a bi-modal distribution with a strong peak at 1, and in most galaxies is very low.