Global physical properties of the simulated, UDF and LLAMAS LAEs. From left to right: redshift, Lyman-α luminositie, UV magnitude, and SFR distributions. The Lyman-α luminosity and UV magnitude of the LLAMAS galaxies are intrinsic values measured (i.e., unlensed values). LLAMAS galaxies represented here are only the objects selected for spatial fitting (see Sect. 2.5). All values are measured following the same procedure on UV and NB Lyman-α images.