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  5. On-sky correction of non-common path aberration with the pyramid wavefront sensor
 

On-sky correction of non-common path aberration with the pyramid wavefront sensor

Journal
ASTRONOMY & ASTROPHYSICS  
Date Issued
2020
Author(s)
ESPOSITO, Simone  
•
PUGLISI, Alfio Timothy  
•
PINNA, Enrico  
•
AGAPITO, Guido  
•
Quirós-Pacheco, F.
•
Véran, J. P.
•
Herriot, G.
DOI
10.1051/0004-6361/201937033
Abstract
The paper deals with with the on-sky performance of the pyramid wavefront sensor-based Adaptive Optics (AO) systems. These wavefront sensors are of great importance, being used in all first light AO systems of the ELTs (E-ELT, GMT, and TMT), currently in design phase. In particular, non-common path aberrations (NCPAs) are a critical issue encountered when using an AO system to produce corrected images in an associated astronomical instrument. The AO wavefront sensor (WFS) and the supported scientific instrument typically use a series of different optical elements, thus experiencing different aberrations. The usual way to correct for such NCPAs is to introduce a static offset in the WFS signals. In this way, when the AO loop is closed the sensor offsets are zeroed and the deformable mirror converges to the shape required to null the NCPA. The method assumes that the WFS operation is linear and completely described by some pre-calibrated interaction matrix. This is not the case for some frequently used wavefront sensors like the Pyramid sensor or a quad-cell Shack-Hartmann sensor. Here we present a method to work in closed-loop with a pyramid wavefront sensor, or more generally a non-linear WFS, introducing a wavefront offset that remains stable when AO correction quality changes due to variations in external conditions like star brightness, seeing, and wind speed. The paper details the methods with analytical and numerical considerations. Then we present results of tests executed at the LBT telescope, in daytime and on sky, using the FLAO system and LUCI2 facility instrument. The on-sky results clearly show the successful operation of the method that completely nulls NCPA, recovering diffraction-limited images with about 70% Strehl ratio in H band in variable seeing conditions. The proposed method is suitable for application to the above-mentioned ELT AO systems.
Volume
636
Start page
A88
Uri
http://hdl.handle.net/20.500.12386/36559
Url
https://api.elsevier.com/content/abstract/scopus_id/85084280359
https://www.aanda.org/articles/aa/full_html/2020/04/aa37033-19/aa37033-19.html
Issn Identifier
0004-6361
Ads BibCode
2020A&A...636A..88E
Rights
open.access
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