Fig. 11.

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λsBHAR as a function of the distance from the central QSOs, CTS G18.01 in MQN01 (red) and PSK1138 in the Spiderweb (green) protocluster. The black dots mark the median values of λsBHAR for the AGN in both protoclusters across different bins of distance from the two central QSOs. The uncertainties correspond to the 16th and 84th percentile values within each radial bin.
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