Affiliation
University of Arizona, Steward ObservatoryWyant College of Optical Science, University of Arizona
Issue Date
2023-10-05Keywords
Coronagraphyexoplanets
integrated wavefront sensing and coronagraphy
phase induced amplitude apodization complex mask coronagraph
PIAACMC
Zernike wavefront sensor
Metadata
Show full item recordPublisher
SPIECitation
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/10.1117/12.2677825Rights
© 2023 SPIE. (2023) Published by SPIE.Collection Information
This item from the UA Faculty Publications collection is made available by the University of Arizona with support from the University of Arizona Libraries. If you have questions, please contact us at repository@u.library.arizona.edu.Abstract
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 SPIE.Note
Immediate accessISSN
0277-786XISBN
978-151066574-3Version
Final Published Versionae974a485f413a2113503eed53cd6c53
10.1117/12.2677825