SFR mass plane color-coded by reddening E(B-V) of the stellar populations, inferred with a PPXF fitting of stellar populations convolved with a Calzetti et al. (1994) dust attenuation law with E(B-V) as a free parameter in three different redshift bins. Each data point represents a single galaxy. The galaxies for which no SFR could be measured are plotted with upper limits. Some are below the quenching threshold and clearly quiescent, while some residual star formation cannot be ruled out for others. More details are given in Fig. 2.