Fig. 3.
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Distributions of rest-MIR wavelengths probed by the sharpest MIRI band (shortest wavelength) with a detection dominated by dust emission, for our S/N > 75 (upper panel) and S/N > 10 (lower panel) samples. The colors of these stacked distributions correspond to the MIRI band used. The total number of galaxies in a given MIRI band is shown in the legend of each panel.
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