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Fig. 8.

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Ratio of the (circularized) effective radius (left panel) and axis ratio (right panel) for different galaxy types to those of the parent SFG sample. Galaxies are in the redshift bin 3 < z < 5 and are massive (log(M*/M) > 10). In the case of the effective radius, ratios calculated after applying a correction to a common redshift and stellar mass are displayed with open squares. The ratios are obtained by dividing the median values of a given galaxy type by the median values of the parent SFG sample, with the error bars representing the uncertainty of the ratio of the medians.

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