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Fig. A.2


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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