Fig. 3.
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Cumulative number of counts in the soft (left) and hard (2–10 keV; right) energy band, derived within a distance of 6 arcmin from the aim point in the Chandra data of MQN01. The red shaded area shows the uncertainties within 1σ due to photometric errors. The black line shows the number of counts predicted for the field from the AGN+Galaxy models developed in Gilli et al. (2007).
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