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Fig. 1

image

PID 203 and PID 319 (large filled squares) are plotted along with various AGN samples on the LXz plane: XMM-CDFS (filled squares, Comastri et al., in prep.; Ranalli et al. 2013), PG quasars (open circles, Piconcelli et al. 2005), SDSS quasars (crosses, Strateva et al. 2005), and CAIXA (filled circles, Bianchi et al. 2009). The LX is the rest-frame 210 keV luminosity. The monochromatic 2 keV luminosities in Strateva et al. (2005) were converted to 210 keV luminosities assuming a power-law spectrum of Γ = 1.8.

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