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Fig. 4.

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Results of fitting the T04 model for galaxies in the GAMA, SDSS, and COSMOS datasets. The fitted parameters are the (top), F (middle), and rbulge (bottom). We compare the fitted values of and F to the ones found in Leslie et al. (2018a), Driver et al. (2007), and Andrae et al. (2012), and 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”. Our best-fit values are in line with the literature values. We see that and F increase with redshift.

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