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Fig. 3.
Left panel: X-ray flux (in units of 10−11 erg cm−2 s−1 in the energy range of 0.2–12 keV) distribution of the sample; right panel: redshift distribution of the sample, where known (in red), and redshift distribution of all AGN with known z (in blue) within the XMM-Newton SMC survey from (Secrest et al. 2015).
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