Abstract

Phase apodization coronagraphs are implemented in a pupil plane to create a dark hole in the science camera focal plane. They are successfully created as "Apodizing Phase Plates" (APPs) using classical optical manufacturing, and as "vector-APPs" using liquid-crystal patterning with essentially achromatic performance. This type of coronagraph currently delivers excellent broadband contrast (∼\sim10−5^{-5}) at small angular separations (few λ/Dλ/D) at ground-based telescopes, owing to their insensitivity to tip/tilt errors.

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