Fig. E.1.
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Same quantities as in the lower-left panel of Fig. 6 for the starburst/MS ratio, but after averaging 1000 realisations of randomised LIR values. This corresponds to selecting random galaxies from the fiducial catalogue, restricted to sources with S/N ≥ 3 in at least three bands, and repeating this process 1000 times, then taking the average ratio values.
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