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Estimating phase errors from pupil discontinuities from simulated on sky data: examples with VLT and Keck

Authors :
Lamb, Masen
Correia, Carlos
Sauvage, Jean-François
Véran, Jean-Pierre
Andersen, David
Vigan, Arthur
Wizinowich, Peter
Van Dam, Marcos
Mugnier, Laurent
Bond, Charlotte
Marchetti, Enrico
Close, Laird
ONERA - The French Aerospace Lab [Châtillon]
ONERA-Université Paris Saclay (COmUE)
DOTA, ONERA, Université Paris Saclay (COmUE) [Châtillon]
NRC Herzberg Institute of Astrophysics
National Research Council of Canada (NRC)
Department of Public Administration
University at Albany [SUNY]
State University of New York (SUNY)-State University of New York (SUNY)
Laboratoire d'Astrophysique de Marseille (LAM)
Centre National de la Recherche Scientifique (CNRS)-Institut national des sciences de l'Univers (INSU - CNRS)-Aix Marseille Université (AMU)-Centre National d'Études Spatiales [Toulouse] (CNES)
W.M. Keck Observatory
Aix Marseille Université (AMU)-Institut national des sciences de l'Univers (INSU - CNRS)-Centre National d'Études Spatiales [Toulouse] (CNES)-Centre National de la Recherche Scientifique (CNRS)
Source :
SPIE Astronomical Telescopes + Instrumentation, SPIE Astronomical Telescopes + Instrumentation, Jul 2016, Edinburgh, United Kingdom. pp.99096D, ⟨10.1117/12.2233093⟩
Publication Year :
2016
Publisher :
HAL CCSD, 2016.

Abstract

International audience; We propose and apply two methods for estimating phase discontinuities for two realistic scenarios on VLT and Keck. The methods use both phase diversity and a form of image sharpening. For the case of VLT, we simulate the `low wind effect' (LWE) which is responsible for focal plane errors in low wind and good seeing conditions. We successfully estimate the LWE using both methods, and show that using both methods both independently and together yields promising results. We also show the use of single image phase diversity in the LWE estimation, and show that it too yields promising results. Finally, we simulate segmented piston effects on Keck/NIRC2 images and successfully recover the induced phase errors using single image phase diversity. We also show that on Keck we can estimate both the segmented piston errors and any Zernike modes affiliated with the non-common path.

Details

Language :
English
Database :
OpenAIRE
Journal :
SPIE Astronomical Telescopes + Instrumentation, SPIE Astronomical Telescopes + Instrumentation, Jul 2016, Edinburgh, United Kingdom. pp.99096D, ⟨10.1117/12.2233093⟩
Accession number :
edsair.doi.dedup.....a76c778d6bb395faf9c111d094da9136
Full Text :
https://doi.org/10.1117/12.2233093⟩