Fig. 4
The bulge fraction (upper-left), the disc scalelength (lower-left), the effective radius of the bulge (upper-right) and the half-light radius of the galaxy (lower-right) in the i and r bands are plotted against each other for the 1638 galaxies (in the photometric sample) modelled in both bands by fitting a de Vaucouleurs profile to the bulge and an exponential to the disc.
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