Agreement between Hα and SFR predictions with empirical measurements. Top: predicted intrinsic Hα emission vs. measured Hα corrected for Galactic extinction from (Rémy-Ruyer et al. 2015, and references therein). Bottom: predicted SFR vs. SFR(Hα+L_TIR) from Rémy-Ruyer et al. (2015). The 1σ contours of the SUEs are calculated by simulating mock data for the y-axis with a dispersion corresponding to the measured uncertainty. For 4 galaxies (HS 0017+1055, HS 0052+2536, HS 1319+3224 and HS 2352+2733) no Hα measurements are available. For 2 of those galaxies (5: HS 0052+2536 and 9: HS 1319+3224), their measured SFR is derived in using diagnostics based on FUV.