Effects of different dust corrections on the star-formation rate evolution for luminous (on the left) and less luminous (on the right) galaxies. Black asterisks and filled green squares represent, respectively, the observed and corrected star-formation rate (along with the corresponding errors) by Bouwens et al. (2009), assuming the β−A₁₆₀₀ relation by Meurer et al. (1999). The red dashed lines report the corrected star-formation rate, obtained taking into account the results of this study.