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Fig. 9.


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Results of 2D Sérsic fits to the surface brightness distributions of bulge components. In every panel, the orange points and histograms represent the results for the FVAE galaxies and the blue for the analytic galaxies. Each panel represents a different parameter, as labelled. For each parameter the true value of the parameter is plotted as a function of the inferred one from the best-fit model. A perfect fit corresponds to the diagonal. In addition, above and to the right of each plot are the projected distributions of the scatter plot. Finally, the inset plot shows the distribution of the error (fitted value minus true value). To make the scatter plot less crowded, only half the galaxies are plotted, but the error histograms and the projected distributions are computed on the entire field (for more details of the error distributions, see Table 1).

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