FIR properties of some of our SFR–M_∗ bins, as inferred from our stacking analysis. These SFR–M_∗ bins have 10^10.8 < M_∗  [M_⊙]  < 10¹¹. In the first column, SFR–M_∗ bins have − 0.1 < Δlog (SSFR)_MS < 0.1, while in the second column they have Δlog (SSFR)_MS = max [Δlog (SSFR)_MS]. Black lines show the DH SED templates best-fitting these FIR flux densities. From these fits, we inferred the mean dust temperatures of galaxies in these SFR–M_∗ bins. We also verified that the infrared luminosities inferred from these fits agree, within 0.3 dex, with the mean infrared luminosities inferred from our “ladder of SFR indicators” (see Sect. 2.6).