Fig. 9
Planet-to-starlight ratio spectrum. Same as Fig. 8 but for a multi-axial (Fizeau) setting. The integration has been performed by means of a single mode cylindrical fibre optics of radius λ0 / D, where D is separation of the two mirrors. The abrupt cut-off at approximately 16.5μm is the long wavelength cut of the fibre optics.
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