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Fig. 6.

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Example light curve realizations of the continuum (red) and reflected light (blue), which correspond to the power-spectral models plotted in Fig. 5. The reflected light curve reduces variability amplitude and is delayed by 50 days. Increasing the size of the reflector further reduces the amplitude of the reflected light curve and shifts it further forward in time. A random selection of observing epochs are plotted, representing measurements of the continuum (black dots) and Fe Kα line (cyan stars) fluxes. The sampled light curves are not obviously correlated, although the parent light curves are.

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