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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