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Fig. 6.

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Variation in Ecut and kTe with the observation epochs as obtained from the xillver and xillverCP model fits, respectively, to the spectra of NGC 3227. The plotted errors were calculated using the χ2 = 2.71 criterion, i.e. 90% confidence range. The dashed black lines in each panel are fits of constant (mean of Ecut and kTe) to the data points. For the fitting, epochs in which we were unable to constrain Ecut and kTe were dropped (indicated with red diamonds).

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