Fig. 9.

Simulations of high resolution Fvar spectra, assuming variations of single parameters (log ξ varying by ∼24%, covering factor varying by ∼4%, and NH varying by ∼19–23%, as indicated in the upper corner of each plot) of obscurer #2 in NGC 3783. The black and light grey curves are, respectively, the Fvar spectra excluding and including the contribution from the constant scattered emission and reflection components.
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