Fig. B.4.

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Examples of synthetic nucleated galaxies with M*, galaxy = 107 M⊙ and various M*, nuc (see the middle rows of Fig. B.3). The first column shows the surface brightness profiles, where the grey points denote the surface brightness from individual pixels of the images. The galaxy (black), nucleus (red), and combined (white) profiles come from the Sérsic+PSF models. The second column shows the inner Re of the galaxy with 27 > μ > 22 mag arcsec−2, with the nucleus contrast (Eq. B.1) annotated. The third and fourth columns show the residual images from subtracting the single Sérsic and Sérsic+PSF models, respectively. The BIC values for each model are annotated in the images. The detection limits for the BIC, visual inspection, and BICres are estimated as 104.2 M⊙, 104.5 M⊙, and 104.8 M⊙, respectively.
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