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Fig. 8

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Stray light. Top two panels: residual stray light for a point source star and an example far-resolved 1.5 mas star. For the resolved star, 481 point sources are used, for the same total intensity as in the point source. Two bottom panels: radial cuts given in linear scale and log10 scale. Curves are for the NW2 configuration and a centrally obstructed telescope. The wavefront used is that of the apodized occulter.

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