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Published online by Cambridge University Press: 13 October 2006
The existing high contrast imaging techniques cannot be applieddirectly to the telescope of the diameter 30–100 m without takinginto account the specific characteristics of a segmented surface.While the increase in telescope diameter is an advantage for thehigh contrast range science, the segmentation sets a limit on theperformance of the coronagraph. In particular, diffraction fromintersegment gaps sets a floor to the achievable extinction of thestarlight. Masking out the gaps in the Lyot plane although helpsincreasing the contrast, does not solve completely the problem: thehigh spatial frequency component of the diffractive light remains.In the paper I suggest using a Lyot stop which produces aphase-amplitude modulation in order to reduce the effect ofsegmentation.