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Fig. A.1


FIR properties of some of our galaxies with individual FIR detections. All these galaxies have 1010.8 < M  [M]  < 1011. In the first column, galaxies have − 0.1 < Δlog (SSFR)MS < 0.1 while in the second column they have Δlog (SSFR)MS > MAX [Δlog (SSFR)MS]  − 0.1. Black lines show the DH SED templates best-fitting these FIR flux densities. From these fits, we inferred the infrared luminosities and dust temperatures of our galaxies.

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