Fig. 14
Cumulative number counts, corrected for completeness, with 1σ confidence level for SXCS (red area), compared to the log N−log S derived from the ROSAT Deep Cluster Survey (cyan area), Rosati et al. (1998). Dot-dashed and dashed lines show the fit to the 400 d (Burenin et al. 2007) and to the COSMOS (Finoguenov et al. 2007) number counts, respectively.
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