Fig. 3.
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Fraction of cluster galaxies (
) hosting an X-ray AGN (LX[0.5 − 10 keV] > 1042 erg s−1). The results are plotted as a function of distance from the cluster centre. Error bars indicate the 1σ confidence limits for small numbers of events (Gehrels 1986). For comparison, we plot the results from previous analyses on clusters of similar mass and redshift.
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