Fig. 7
Comparison between the MIR (22 μm) and the Balmer-corrected Hα SFR tracers; recipes from Calzetti (2013); see Eqs. (6) and (4). Solid line corresponds to the 1:1 line. Orange points show type-2 AGN galaxies and blue points represent star-forming galaxies. The legend gives the number of objects available in both cases. Residuals appear in the bottom part of this figure as a function of the Balmer-corrected Hα SFR tracer. Solid line shows the mean value of −0.08 when all the galaxies are included and the dashed lines are referred to the 1σ dispersion (±0.29 dex) around it. For SF galaxies, the mean values is −0.15, while for type-2 AGN host galaxies is 0.03.
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