Fig. 12
The log N − log S of the present sample in the 0.5 − 2.0 keV band. Fluxes are calculated in the r500 aperture. Results from several surveys are also shown: COSMOS (Finoguenov et al. 2007), RDCS (the ROSAT Deep Cluster Survey, Rosati et al. 1998), 400 deg2 survey (Burenin et al. 2007; Vikhlinin et al. 2009) and the XMM-LSS (Pacaud et al. 2007). See Sect. 5.3 for details.
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