Fig. 17
Metallicity distribution for the excess galaxies in black. The colours mark the presence of an excess at 500 μm and code the intensity of this excess: R(500)/ΔR(500). The metallicity distribution for the DGS & KINGFISH galaxies detected at 500 μm is outlined in grey. The grey cells mark all of the galaxies for which no detection is available at 500 μm.
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