Basden, A. G. and Chemla, F. and Dipper, N. and Gendron, E. and Henry, D. and Morris, T. and Rousset, G. and Vidal, F. (2014) 'Real-time correlation reference update for astronomical adaptive optics.', Monthly notices of the Royal Astronomical Society., 439 (1). pp. 968-976.
The use of laser guide stars in astronomical adaptive optics results in elongated Shack–Hartmann wavefront sensor image patterns. Image correlation techniques can be used to determine local wavefront slope by correlating each sub-aperture image with its expected elongated shape, or reference image. Here, we present a technique which allows the correlation reference images to be updated while the adaptive optics loop is closed. We show that this can be done without affecting the resulting point spread functions. On-sky demonstration is reported. We compare different techniques for obtaining the reference images, and investigate performance over a wide range of adaptive optics system parameters. We find that image correlation techniques perform better than the standard centre-of-gravity algorithm and are highly suited for use with open-loop multiple object adaptive optics systems.
|Keywords:||Instrumentation: adaptive optics, Instrumentation: high angular resolution, Techniques: image processing.|
|Full text:||(VoR) Version of Record|
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|Publisher Web site:||http://dx.doi.org/10.1093/mnras/stu027|
|Publisher statement:||This article has been accepted for publication in Monthly Notices of the Royal Astronomical Society © 2014 The Author Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.|
|Date accepted:||04 January 2014|
|Date deposited:||24 October 2014|
|Date of first online publication:||31 January 2014|
|Date first made open access:||No date available|
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