Paper
11 September 2015 Optimized focal and pupil plane masks for vortex coronagraphs on telescopes with obstructed apertures
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Abstract
We present methods for optimizing pupil and focal plane optical elements that improve the performance of vortex coronagraphs on telescopes with obstructed or segmented apertures. Phase-only and complex masks are designed for the entrance pupil, focal plane, and the plane of the Lyot stop. Optimal masks are obtained using both analytical and numerical methods. The latter makes use of an iterative error reduction algorithm to calculate "correcting" optics that mitigate unwanted diffraction from aperture obstructions. We analyze the achieved performance in terms of starlight suppression, contrast, off-axis image quality, and chromatic dependence. Manufacturing considerations and sensitivity to aberrations are also discussed. This work provides a path to joint optimization of multiple coronagraph planes to maximize sensitivity to exoplanets and other faint companions.
© (2015) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Garreth J. Ruane, Olivier Absil, Elsa Huby, Dimitri Mawet, Christian Delacroix, Brunella Carlomagno, Pierre Piron, and Grover A. Swartzlander Jr. "Optimized focal and pupil plane masks for vortex coronagraphs on telescopes with obstructed apertures", Proc. SPIE 9605, Techniques and Instrumentation for Detection of Exoplanets VII, 96051I (11 September 2015); https://doi.org/10.1117/12.2187236
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Cited by 9 scholarly publications.
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KEYWORDS
Coronagraphy

Point spread functions

Electroluminescent displays

Telescopes

Virtual colonoscopy

Light

Optical components

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