Main properties of obtained A_FUV priors. Panel a shows the distributions of original A_FUV from the Salim et al. (2018) work obtained from careful SED fitting based on measurements from UV to mid-IR (A_FUV, blue left hatched histogram), and A_FUVp calculated based on Eq. (4) (orange right hatched histogram). Panel b presents the distribution of the difference between A_FUV and A_FUVp and denotes its median value. In panel c, the difference between A_FUV and A_FUVp is shown as a function of redshift. We removed for clarity from panel a 426 galaxies, for which calculated A_FUVp was lower than 0.