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Fig. 8.

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Best-fit values for , F and rbulge for galaxies in our datasets, divided in bins of μ*. We compare the fitted values for rbulge to the average and 32–68th percentile of the bulge-to-total distribution of the selected samples, labeled with the subscript “data”. The results show an increase for an increase in μ*, similar to Grootes et al. (2013), given by the black dashed line and gray. The GAMA and COSMOS surveys do not contain enough high surface density galaxies to describe a clear magnitude-inclination relation, resulting in the model not obtaining fitting results at log(μ) ∼ 8.7 M kpc−2.

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