Star formation rate as a function of stellar mass (M_stellar) for the VIMOS sample (blue diamonds). The solid line represents the star-forming main sequence found by Schreiber et al. (2015), and the dashed lines give the scatter of 0.4 dex. Upper limits are shown as grey diamonds. The optically selected Type II AGN from zCOSMOS survey found by Bongiorno et al. (2012) and from BOSS DR12 are shown as green circles and grey contours, respectively.