SFR vs. M_⋆ plot for the DWALIN galaxy sample. Green squares, brown triangles, and blue circles indicate galaxies whose SFR measurements come from the combination of UV and MIR data, MIR data alone, or UV data alone, respectively (see text for details). ID numbers are shown for the DWALIN-19 sample studied with MUSE in this work. Gray dots show the sample of ≈15 750 nearby galaxies studied by Leroy et al. (2019). We also show the SFR–M_⋆ trends at z ≃ 0 from the SDSS (Chang et al. 2015, dashed line), from the LMLVL sample (Berg et al. 2012, dotted line), and the relation derived by McGaugh et al. (2017) for a sample of low-surface brightness galaxies (dot-dashed line).