Left: comparison between the Hα luminosity corrected for dust attenuation derived using the 24μm Spitzer/MIPS emission (L(Hα)_24μm) and that derived using the Balmer decrement (L(Hα)_BD), as described in the text. Both luminosities are corrected for [NII] contamination. Different symbols indicate different galaxies. Filled symbols are for Hα narrow-band data, and open symbols represent MUSE data. The dotted line shows the one-to-one relation. Right: same comparison for the star formation rates derived using the Kennicutt (1998a) calibration adapted for a Chabrier (2003) IMF.