Fig. 5.
Upper panel: results of the best fit for the EPIC PN phase-averaged spectrum of observation C (red line) obtained with a gabs*TBabs*(pegpwrlw + bbodyrad) model. The blackbody (blue line) and power-law (green line) components are plotted, as well as the spectrum of the background (magenta). Lower panels: residuals (in standard deviation units) for the best fit obtained without (top) and with (bottom) the gabs component. A factor 10 graphic rebin is used.
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