Global properties of the galaxies from the LLAMAS. From left to right: distribution of redshift, lensing magnification, UV magnitude, and SFR (both corrected from lensing magnification). The grey area in each panel represents the sources selected for the spatial fitting (see Sect. 3.4). When more than one image is detected for the same source, the values of the most magnified images are presented in panels 3 and 4. The magnifications presented in this figure are the total magnification for each source, i.e., the sum of the global magnifications of each multiple image of the same galaxy.