AGN Triggering in the Infall Regions of Distant X-Ray Luminous Galaxy Clusters at
Figure 5
Cumulative number count distributions starting from an off-center angle of 8′ inwards. (a) Total cumulative counts for cluster fields (solid lines) in comparison to the median background models (dashed lines) for the soft-band (black) and full-band detection (red). (b) Cumulative distribution of excess counts after subtraction of the background model for the soft band (black) and full-band (red). Dotted lines show the original measured distribution, whereas solid lines depict the smoothed trends after boxcar filtering. Average cluster radii (dashed) and (solid) for the distant cluster sample are marked by the blue vertical lines.
