This talk is based on the work Donevski et al. , to be submitted - we aim to tackle one of existing challenges in dusty, galaxy formation and evolution by estimating the evolution of \(M_{\rm dust}/M_{\star}\)over cosmic time. I explain how to take particular care of understanding the eventual systematics of estimated physical properties. I show how we model and interpret our results in the context of galaxy formation and evolution by confronting the findings to the newest generation of galaxy models and simulations that include self-consistent dust growth. We find that the ratio between dust and stellar mass can be used as a great diagnostics to disentangle MS and SB galaxies over all redshifts.