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Fig. 5.
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Unfolded spectra and model fits along with the data-to-model ratio for const*TBabs(xillverCP) fits to epoch G (left), epoch H (middle), and epoch I (right) of NGC 3227. For epochs G, H, and I, zTBabs was added to the model. Blue and yellow data points refer to FPMA and FPMB, respectively.
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