Presentation + Paper
13 December 2020 First on-sky results of the CAWS wavefront sensor on the CANARY experiment
Author Affiliations +
Abstract
Point-diffraction interferometers are a class of wavefront sensors which can directly measure the phase with great accuracy, regardless of defects such as vortices and disconnected apertures. Due to these properties, they have been suggested in applications such as cophasing of telescope segments, wavefront sensing impervious to the island effect and high-contrast AO and imaging. This paper presents an implementation of this class of interferometer, the Calibration & Alignment~WFS (CAWS), and the results of the first on-sky tests in the visible behind the SCAO loop of the CANARY AO experiment at the William Herschel Telescope. An initial analysis of AO residuals is performed in order to retrieve the SNR of interference fringes and assess the instrument's performance under various observing conditions. Finally, these results are used to test the validity of our models, which would allow for rapid implementation-specific modelling to find minimum-useful flux and other CAWS limits.
Conference Presentation
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Nicolas Dubost, Nazim Bharmal, Maud Langlois, Magali Loupias, Clément Schotte, Michel Tallon, Lazar Staykov, Lisa Bardou, James Osborn, Fanny Chemla, Matthieu Cohen, Tristan Buey, Éric Gendron, and Tim Morris "First on-sky results of the CAWS wavefront sensor on the CANARY experiment", Proc. SPIE 11448, Adaptive Optics Systems VII, 1144819 (13 December 2020); https://doi.org/10.1117/12.2561326
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KEYWORDS
Wavefront sensors

Adaptive optics

Interferometers

Signal to noise ratio

Demodulation

Cameras

Near infrared

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