Stellar masses based on the da Cunha et al. (2008) model (hereafter M_DCE08) are plotted as a function of the ones derived from Bell et al. (2003) relation based on Ks luminosity (M_Ks) after applying the corrections discussed in the text. Vertical error bars indicate the 16–84 percentile ranges in the recovered probability distributions, while the horizontal error bars are the 30% errors as described by Bell et al. (2003) determined from the scatter in the models. The blue dashed line represents the one-to-one relation.