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  5. Modeling noise propagation in Fourier-filtering wavefront sensing, fundamental limits, and quantitative comparison
 

Modeling noise propagation in Fourier-filtering wavefront sensing, fundamental limits, and quantitative comparison

Journal
ASTRONOMY & ASTROPHYSICS  
Date Issued
2023
Author(s)
Chambouleyron, V.
•
Fauvarque, O.
•
PLANTET, Cedric Antoine Adrien Gabriel  
•
Sauvage, J. -F.
•
Levraud, N.
•
Cissé, M.
•
Neichel, B.
•
Fusco, T.
DOI
10.1051/0004-6361/202245351
Abstract
Context. Adaptive optics (AO) is a technique allowing for ground-based telescopes' angular resolution to be improved drastically. The wavefront sensor (WFS) is one of the key components of such systems, driving the fundamental performance limitations.
Aims: In this paper, we focus on a specific class of WFS: the Fourier-filtering wavefront sensors (FFWFSs). This class is known for its extremely high sensitivity. However, a clear and comprehensive noise propagation model for any kind of FFWFS is lacking.
Methods: Considering read-out noise and photon noise, we derived a simple and comprehensive model allowing us to understand how these noises propagate in the phase reconstruction in the linear framework.
Results: This new noise propagation model works for any kind of FFWFS, and it allows one to revisit the fundamental sensitivity limit of these sensors. Furthermore, a new comparison between widely used FFWFSs is held. We focus on the two main FFWFS classes used: the Zernike WFS (ZWFS) and the pyramid WFS (PWFS), bringing new understanding of their behavior....
Volume
670
Start page
A153
Uri
http://hdl.handle.net/20.500.12386/35815
Url
http://arxiv.org/abs/2212.13577v2
https://www.aanda.org/articles/aa/full_html/2023/02/aa45351-22/aa45351-22.html
Issn Identifier
0004-6361
Rights
open.access
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