Fig. 7
Left: representative sample images of one AGN in our sample in HST/ACS F850LP band, HST/ACS F850LP band (after PSF-matched) and WFC3/IR F160W images. The green circles represent the apertures we used to assess the AGN contribution on host colors. Right: redshift vs. Δ(U−V) for AGN hosts and non-AGN galaxies in GOODS-South. The red and black lines denote the sliding median for AGN hosts and non-AGN galaxies, respectively.
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