SFR_UV0 vs. SFR_[OII]0 corrected for dust extinction using, respectively, β_phot and Eq. (11), and EW_[OII] and Eq. (14) assuming a Calzetti et al. (2000) law and f = 0.50. The black line is the 1-to-1 relation that corresponds also to a linear fit to the points. Blue and red lines show the fits with other two different assumptions of f. Blue points are IR-detected galaxies, while light blue points are galaxies with no IR detection.