FIR properties of some of our SFR–M∗ bins, as inferred from our stacking analysis. These SFR–M∗ bins have 1010.8 < 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).
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