Comparison of the estimated stellar masses via CIGALE according to different attenuation laws. The left panel shows the stellar masses calculated via CIGALE with the Calzetti et al. (2000) attenuation law, M_C00, with those calculated by the VIPERS team using the Le Phare tool (Arnouts et al. 1999; Ilbert et al. 2006), M_VIPERS, for 36 157 galaxies in the pure sample. The right panel shows the stellar masses calculated with CIGALE using the Calzetti et al. (2000) and Charlot & Fall (2000)M_CF00 attenuation laws for the same pure sample of galaxies. In both plots the one-to-one relation is shown with an orange line.