Sebastiaan Y. Haffert,1 Jared R. Males,1 Oliver Guyon1,2,3
1Steward Observatory, The Univ. of Arizona (United States) 2Astrobiology Ctr., National Institutes of Natural Sciences (Japan) 3National Astronomical Observatory of Japan, Subaru Telescope (United States)
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Uncorrected wavefront errors create speckle noise in high-contrast observations at small inner-working angles. These speckles can be sensed and controlled by using coronagraph integrated wavefront sensors. Here, we will present how the Phase Induced Amplitude Apodized Complex Mask Corongraph (PIAACMC) can be integrated with both a Self-Coherent Camera (SCC) for focal plane wavefront sensing and an extremely sensitivity high-order pupil plane Zernike Wavefront Sensor (ZWFS). Non-common path aberrations can be completely erased by integrating both sensors into the PIAACMC, which is of extremely high importance in high-contrast imaging.
(2023) Published by SPIE. Downloading of the abstract is permitted for personal use only.
Sebastiaan Y. Haffert,Jared R. Males, andOliver Guyon
"Integrated coronagraphy and wavefront sensing with the PIAACMC", Proc. SPIE 12680, Techniques and Instrumentation for Detection of Exoplanets XI, 126802J (5 October 2023); https://doi.org/10.1117/12.2677825
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Sebastiaan Y. Haffert, Jared R. Males, Oliver Guyon, "Integrated coronagraphy and wavefront sensing with the PIAACMC," Proc. SPIE 12680, Techniques and Instrumentation for Detection of Exoplanets XI, 126802J (5 October 2023); https://doi.org/10.1117/12.2677825