Fig. 5.
Comparison between our I-band effective radius from single Sérsic fits and the Griffith et al. (2012) effective radius, in kpc. The two objects deviating from the one-to-one line relation are very challenging galaxies to fit in the I band: LTGb 37194 exhibits prominent spiral arms and a nuclear bar, whereas ETG 25781 also appears to have some spiral features evident in the residuals.
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