Circularly Symmetric Apodization via Starshaped Masks
arXiv:astro-ph/0305045 · doi:10.1086/379238
Abstract
Recently, we introduced a class of shaped pupil masks, called spiderweb masks, that produce point spread functions having annular dark zones. With such masks, a single image can be used to probe a star for extrasolar planets. In this paper, we introduce a new class of shaped pupil masks that also provide annular dark zones. We call these masks starshaped masks. Given any circularly symmetric apodization function, we show how to construct a corresponding starshaped mask that has the same point-spread function (out to any given outer working distance) as obtained by the apodization.
Paper also at: http://www.orfe.princeton.edu/~rvdb/tex/starshape/ms.pdf Updated to clarify misleading statements regarding total throughput for apodizations and their corresponding starshaped masks
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- Apodized pupil Lyot coronagraphs for arbitrary apertures. V. Hybrid Shaped Pupil designs for imaging Earth-like planets with future space observatories
- Shaped Pupil Lyot Coronagraphs: High-Contrast Solutions for Restricted Focal Planes
- Analyzing the designs of planet finding missions
- Apodized Pupil Lyot Coronagraphs for Arbitrary Apertures. IV. Reduced Inner Working Angle and Increased Robustness to Low-Order Aberrations
- Optimal Asymmetric Apodizations and Shaped Pupils for Planet Finding Coronagraphy
- Demonstration of high contrast with an obscured aperture with the WFIRST-AFTA shaped pupil coronagraph
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- Coronographic Methods for the Detection of Terrestrial Planets
- Comparative study of manufacturing techniques for coronagraphic binary pupil masks: masks on substrates and free-standing masks
- Shaped pupil design for the Gemini Planet Imager
- Apodization in high-contrast long-slit spectroscopy. Closer, deeper, fainter, cooler
- Coronagraphic demonstration experiment using aluminum mirrors for space infrared astronomical observations
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