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Fig. 9.

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Relation between shape parameters at one (top row) and three (bottom row) stellar half-mass radii and the stellar mass, colored by the b-value. The black lines indicate the median values in the respective mass bins and the shaded regions the 1σ ranges (containing 68% of the galaxies above and below the median). The dashed part of the lines indicates where there may be effects caused by low number statistics.

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