Comparison between SFRIR + UV and SFRHα when varying the dust correction for the Hα emission. The lower panel shows the case where LHα are corrected for dust attenuation by using the classical prescription of Calzetti (f = 0.58) while in the upper panel the Hα luminosities are corrected with our dust correction (f = 0.93). The black solid line is the 1:1 correlation line and the different colors indicate the stellar masses, as indicated in the vertical color bar. The lowest part of each panel also shows the median errors on the SFR measurements.
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