Fig. 16.
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Evolution of z-GAL apparent dust mass (upper panel) and apparent FIR luminosity (lower panel) with redshift for the optically thin MBB, shown in black squares. The BEARS sample (Bendo et al. 2023) is over-plotted in orange diamonds. In the lower panel, the black dashed line shows the lower limit resulting from the 500 μm flux density selection.
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