Stellar mass–SFR relation, as derived from the photometric data using the LePhare code, for all galaxies analysed in this study. The symbols are the same as in as in Fig. 4, but in addition, we also plot here the M0416 star-forming cluster members from Maier et al. (2016), observed with the VLT/VIMOS, as light grey crosses. The black solid and dashed lines represent the star-forming MS at z = 0.4 and its ∼0.3 dex scatter, as derived by Peng et al. (2010b). The grey cross in the lower right corner of the plot shows the measurement errors for the SFRs and stellar masses.