Left: NUVrJ color-color diagram for all our selected galaxies. The value of Mg_UV galaxies in our sample is color-coded. We identify the galaxies selected as passive using the Mg_UV index only by empty black squares. The passive region (black solid and dashed line) is taken from Davidzon et al. (2017). Right: position of our galaxies in the M-SFR diagram. We show in gray all the galaxies from VVDS deep and ultra deep sample (at all redshift) for comparison. We also show the main sequence fit at z ∼ 1 and 2 from Elbaz et al. (2007) and Daddi et al. (2007), respectively. Our selected galaxies are shown in color representing the Mg_UV strength.