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Fig. 5.


Average Sérsic n value as a function of ellipticity for galaxies with 20 <  F814W <  24.5 in COSMOS (black points; Griffith et al. 2012) and the UDF (red points; Coe et al. 2006). The solid line indicates the average n as a function of ϵ used in the image simulations (for galaxies with 20 <  mr <  25), whereas the dashed lines is for the case we scramble the ellipticities to resemble the FC17 results more closely.

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