Fig. 14.
Difference between PSF and cmodel magnitudes plotted against absorption-corrected 2–10 keV luminosity. The short and long bars in the lower right corner are typical errors of mPSF − mcmodel for i = 24 and 25, respectively. Filled circles: AGN 1; Open circles: AGN 2; Crosses: SF.

Difference between PSF and cmodel magnitudes plotted against absorption-corrected 2–10 keV luminosity. The short and long bars in the lower right corner are typical errors of mPSF − mcmodel for i = 24 and 25, respectively. Filled circles: AGN 1; Open circles: AGN 2; Crosses: SF.

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