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Fig. 7.

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AGN fraction (in %) for the different types of AGN in different overdensity bins: coeval field (blue) intermediate overdensity (green), and highest overdensity peaks (red). Here, we only show the five categories (MIR-SED, MIR-color, X-ray-lum, X2R, and opt-sp) for which, on average, there are more than eight AGNs across all 100 MC iterations. Note: the categories are not mutually exclusive and an AGN may meet the criteria for more than one category. See Figure 11 in Lyu et al. (2022) for the overlap of sources in different AGN categories. The asymmetric 1σ errors on these AGN fractions are shown. For all categories, there is a clear trend of higher AGN fraction for galaxies in denser environments.

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