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Redundant apodization for direct imaging of exoplanets
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APODIZED PUPIL LYOT CORONAGRAPHS FOR ARBITRARY APERTURES. IV. REDUCED INNER WORKING ANGLE AND INCREASED ROBUSTNESS TO LOW-ORDER ABERRATIONS
Direct detection of exoplanets in the 3–10 μm range with E-ELT/METIS
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Combining high-dispersion spectroscopy with high contrast imaging: Probing rocky planets around our nearest neighbors
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Performance characterization of a broadband vector Apodizing Phase Plate coronagraph
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Successes and challenges of the APP Coronagraph
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