Fig. 1
Simulated XMM-Newton images and source detection. Top: X-ray photon map from cosmo-OWLS overplotted with red (cyan) circles that mark the position and redshift of the input dark matter haloes (secondary haloes). The radius of each circle represents the r500 radius. Middle: same as top overplotted with the X-ray contours (10 ks exposure) and the position of the input simulated AGN (blacksquares). Bottom: same as top after including XMM-Newton instrumental effects and background. Green squares (circles) mark significant detections of point-like (extended) sources by the detection algorithm.
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