Paper
1 September 2021 Implementation of a broadband focal plane estimator for high-contrast dark zones
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Abstract
The characterization of exoplanets’ atmospheres using direct imaging spectroscopy requires high-contrast over a wide wavelength range. We study a recently proposed focal plane wavefront estimation algorithm that exclusively uses broadband images to estimate the electric field. This approach therefore reduces the complexity and observational overheads compared to traditional single wavelength approaches. The electric field is estimated as an incoherent sum of monochromatic intensities with the pair-wise probing technique. This paper covers the detailed implementation of the algorithm and an application to the High-contrast Imager for Complex Aperture Telescopes (HiCAT) testbed with the goal to compare the performance between the broadband and traditional narrowband filter approaches.
© (2021) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Susan F. Redmond, Laurent Pueyo, Leonid Pogorelyuk, James Noss, Scott D. Will, Iva Laginja, N. Jeremy Kasdin, Marshall D. Perrin, and Rémi Soummer "Implementation of a broadband focal plane estimator for high-contrast dark zones", Proc. SPIE 11823, Techniques and Instrumentation for Detection of Exoplanets X, 118231Q (1 September 2021); https://doi.org/10.1117/12.2594620
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KEYWORDS
Image analysis

Exoplanets

Spectroscopy

Stars

Wavefronts

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