Fig. 11.
High-contrast images (at the shortest wavelength, 0.966 μm) used to verify the WDH analysis procedure (logarithmic scale). Left: simulation using only the fitting and AO-servolag errors. Middle left: simulation additionally including NCPA upstream (given by the ZELDA on-sky estimate) and downstream of the APLC focal-plane mask. Middle right: simulation additionally including LOR and LWE. Right: on-sky image of the star 51 Eri taken with the VLT/SPHERE-IFS instrument.
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