Fig. 2

Aberrations upstream (φu (WFE = 80 nm),
top) and downstream (φd
(WFE = 20 nm), bottom) of the coronagraph: reconstruction error
(solid red line) as a function of the incoming flux α. For
comparison,
(cyan dashed line) and
(magenta dashed line) theoretical behaviours are plotted for detector noise only and
photon noise only (respectively).
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