Fig. 4
Top panel: NGC 3783 EPIC-pn data fit residuals without absorption by a high-ionisation component (HC), showing new Fe xxv and Fe xxvi absorption lines in the 2016 obscured epoch. Middle panel: line transmission of the blue-shifted HC Fe xxv and Fe xxvi absorption lines (solid lines), shown with respect to the Fe Kα and Fe Kβ emission lines and the continuum unaffected by the HC line absorption (dotted lines). Bottom panel: EPIC-pn data and their best-fit model (dotted lines).
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