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Fig. A.2

image

Distributions of the flux ratio of the Sérsic component to the PSF component (in magnitudes) from two component GALFIT fits to AGNs and inactive galaxies in the WFC3/F160W band. 1000 draws of a mass-matched control sample are analyzed to determine the 1σ/2σ scatter in the n distributions for inactive galaxies, shown as dark/light grey zones in the histograms. Red open histograms show the distributions for the AGNs. The dashed black line is the distribution for the full inactive galaxy sample for which two component fits were performed, including many lower mass galaxies not widely found among AGN hosts. This histogram has been scaled down to overlap with the peak of the AGN histogram, to allow a simple visual comparison of the distributions.

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