Distribution of the SFR as a function of the stellar mass for the sample of spatially resolved continuum galaxies (red markers). Galaxies suitable for the analysis of spatially resolved gas kinematics (C16; Contini et al., and in prep.) are indicated by the grey symbols. The sample galaxies fall along the “normal” star-forming sequence of galaxies and extend to the lowest stellar mass regime (~10^8.5 M_⊙) probed so far with IFS surveys. UDF10-ID #5, indicated by its ID number, shows no ionised gas in the MUSE data cube (except a weak [OII] line) and deviates from the “normal” star-forming sequence.