Fig. 9.
Top: merger fractions in AGNs and non-AGNs as stellar mass increases for the GAMA sample. For the GAMA OPT AGNs, the merger fraction increases as stellar mass increases in the mass complete regime in different redshift bins (indicated in the bottom right corner in each panel). Bottom: same as the top panel, but with stricter merger identification. Errors are calculated through binomial statistics. We find an increase of the merger fractions in AGNs as stellar mass increases.
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