Upper panel: position of our sBzK sources in the SFR-M_⋆ plane. The purple contours indicate sources with only UV-detection (i.e., having no mid/far-IR), the orange dots the MIPS-but-not-PACS-detected sources, and the red stars the PACS-detected sources. The vertical dotted line indicates the stellar mass where the sample becomes strongly incomplete. The horizontal dot-dash and three-dot-dash lines represents the completeness limits in SFR of the UV and MIPS subsamples. Lower panel: distance between our sBzK sources and the center of the main sequence. The horizontal long-dash line corresponds to the limit between the galaxies classified as main sequence of starburst. The vertical short-dash line shows the mass cut that defines a complete mass-selected sample of starburst galaxies detected by PACS.