SFR vs. stellar mass for the galaxies in our sample. Sources are color-coded according to their redshift, while the different symbols correspond to the different WISE classes (AGN as circles, starbursts as triangles, and intermediate disks as squares), as in Fig. 1. Upper limits to the SFRs are indicated with arrows. The diagonal lines correspond to the MS model prescriptions by Speagle et al. (2014) at z = 0.2, 1, and 2. The red cross in the bottom right corner shows the typical uncertainties of ∼0.3 dex for both SFRs and stellar masses.