Fig. 3.
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Best-fit model (Model M1 in Tables 2 and 3) to the XMM-Newton (EPIC/pn and RGS) and NuSTAR spectra of NGC 3227 in late 2019. The top panels are the transmission of the X-ray obscurer (XO), de-ionized warm absorber (de-WA), and the Galactic absorption (MW). Data (colored curves with 1σ uncertainties in gray) and model (black curves) of each instrument are rebinned for clarity.
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