Updated calibrations for the 22 μm and TIR single-band SFR tracers anchoring them to extinction-corrected Hα luminosity (Eq. (4)). Orange points in left panels correspond to type-2 AGN, while blue points refer to star-forming galaxies. Linear fits are shown with dashed lines, while nonlinear fits are shown with dotted lines. The results for these calibrations appear in Table 2. The residuals are computed as the average value of the log[5.5 × 10^-42 × L(Hα_corr)/a × L(IR)] where L(IR) could be 22 μm or TIR for the case of the linear fits, after applying a 4σ rejection. These values are computed for all galaxies (black), star-forming (blue), and type-2 AGN host galaxies (orange).