Comparison of centroid computation algorithms in a Shack-Hartmann sensor

被引:230
作者
Thomas, S.
Fusco, T.
Tokovinin, A.
Nicolle, M.
Michau, V.
Rousset, G.
机构
[1] Cerro Tololo Interamer Observ, La Serena, Chile
[2] Off Natl Etud & Rech Aerosp, F-92322 Chatillon, France
关键词
turbulence; instrumentation : adaptive optics;
D O I
10.1111/j.1365-2966.2006.10661.x
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Analytical theory is combined with extensive numerical simulations to compare different flavours of centroiding algorithms: thresholding, weighted centroid, correlation, quad cell (QC). For each method, optimal parameters are defined in function of photon flux, readout noise and turbulence level. We find that at very low flux the noise of QC and weighted centroid leads the best result, but the latter method can provide linear and optimal response if the weight follows spot displacements. Both methods can work with average flux as low as 10 photons per subaperture under a readout noise of three electrons. At high-flux levels, the dominant errors come from non-linearity of response, from spot truncations and distortions and from detector pixel sampling. It is shown that at high flux, centre of gravity approaches and correlation methods are equivalent (and provide better results than QC estimator) as soon as their parameters are optimized. Finally, examples of applications are given to illustrate the results obtained in the paper.
引用
收藏
页码:323 / 336
页数:14
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