Stellar mass function for all (black), star-forming (blue), and quiescent (red) galaxies in four redshift bins. The solid lines show the best parametric form of our SMF measurements (stars), while the shaded areas represent the systematic uncertainty due to the SF/Q separation (cf. Sect. 5.1). The dashed lines show the parametric forms obtained if a single-Schechter function is assumed to fit the SF population. The measurements of Tomczak et al. (2014, squares) and Ilbert et al. (2013, circles) are plotted for comparison.