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Fig. 9

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Simulated images at λ = 950nm. a) Simulated object map and b) associated image in the focal plane. The following planets are simulated: one with a star-over-planet contrast of 105 at a separation of 0.2 arcsec (planet 1), two with star-over-planet contrast of 106 at separations of 0.2 (planet 2) and 0.4 (planet 3), respectively, and one with a star-over-planet contrast of 107 at a separation of 0.4 arcsec (planet 4). The image in the focal plane is obtained by convolving the object map oλ by the non-coronagraphic psf . c) Simulated aberrations and d) associated image of the speckle field in the image focal plane. The image is given by the coronagraphic PSF .

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