Fig. 11.
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AGN frequency in mergers vs non-mergers. Top: Frequency of AGNs (MIR AGN: red; X-ray AGN: blue; SED AGN: orange) in mergers (filled symbols) and non-mergers (empty symbols) per z-bin. Errors are calculated using binomial statistics. Bottom: Ratio of AGN frequency in mergers relative to that in non-mergers (i.e. AGN excess). The dashed line indicates no excess. Previous measurements are shown on the left. Ellison et al. (2013) found a MIR AGN excess of 13.3, shown as an arrow for readability.
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