Fig. 16.
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Ratio of intrinsic sizes (main figure) as well mock observations (inset figure) at 1500 Å with observations like ALMA configuration is shown for UV and IR spectrum in stellar mass bins of 0.5 dex, with median values plotted as data-points. The error bars denote the 16th and 84th percentile values. Only sufficiently populated bins (N > 20) have been used to plot the lines.
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