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Fig. 6.

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GALFIT fitting results using mock images generated by GALAXEV and SKIRT, in both dust-free (dashed lines) and dusty (solid lines) conditions. The upper panel shows the variation in bulge fraction fbulge, p with stellar mass. The lower panel illustrates how the scale length of the disk hR. Dashed and solid lines represent the median values, whose error bars correspond to the 1σ range.

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