Fig. 4.
Numerical simulations: final coronagraphic images accounting for AO residuals from the current AO system, SAXO (left) and for AO residuals with a faster AO system, SAXO+ (right). Images on the top row are obtained with the APLC alone, while images on the bottom row are obtained after minimization of the stellar speckle intensity using PW+EFC. The HDH region is delimited by the white dashed rectangular box.
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