DR2 completeness with respect to HST deep imaging sample. Completeness is computed as the number of galaxies with a MUSE redshift in a 0.31 HST AB F775W magnitude (left panel) or 0.5 photometric redshift interval (right panel). The measurements have been performed for the deep MXDF (+100-h depth, orange bars) and MOSAIC (+10-h depth, blue bars) data sets and corresponding areas.