Fig. B.1.
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Overview of dust removal timescales and normalisation constants for different GAMA galaxy subsamples, compared to DD20. Panel (a): GAMA dusty galaxies. Top: Dust removal timescale as a function of redshift for GAMA dusty galaxies (Herschel SPIRE 250 μm S/N ≥ 3, redshift up to 0.9) and galaxies from DD20 (redshift from 0.9 to 5.234). Bottom: Normalisation constant as a function of redshift. Panel (b): GAMA dusty spiral galaxies + DD20. Panel (c): GAMA massive dusty spiral galaxies + DD20. Panel (d): GAMA massive DSFGs + DD20. The GAMA redshift bin with z<0.1 contains only a single galaxy, which made it impossible to obtain any fit. Panel (e): GAMA massive dusty ETGs + DD20.
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