Averaged MIR and FIR SED fitting of galaxy subsamples at 0.3 < z < 0.55 (left panel) and 1.3 < z < 1.6 (right panel), based on fluxes derived from the mean stacking technique described in Appendix A. For each redshift range, SED fits are illustrated for two different bins of stellar mass and two bins of NRK color. The best SED fits are shown with the solid blue curves, while the red curves represent SEDs extrapolated from the 24 μm flux. Downward filled triangles depict upper limits for the stacked fluxes at 500 μm.