21 July 2014 Tomography and calibration for Raven: from simulations to laboratory results
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This paper discusses static and dynamic tomographic wave-front (WF) reconstructors tailored to Multi-Object Adaptive Optics (MOAO) for Raven, the first MOAO science and technology demonstrator recently installed on an 8m telescope. We show the results of a new minimum mean- square error (MMSE) solution based on spatio-angular (SA) correlation functions, which extends previous work in Correia et al, JOSA-A 20131 to adopt a zonal representation of the wave-front and its associated signals. This solution is outlined for the static reconstruction and then extended for the use of stand-alone temporal prediction and as a prediction model in a pupil plane based Linear Quadratic Gaussian (LQG) algorithm. We have fully tested our algorithms in the lab and compared the results to simulations of the Raven system. These simulations have shown that an increase in limiting magnitude of up to one magnitude can be expected when prediction is implemented and up to two magnitudes when the LQG is used.
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Kate Jackson, Kate Jackson, Carlos Correia, Carlos Correia, Olivier Lardière, Olivier Lardière, Dave Andersen, Dave Andersen, Colin Bradley, Colin Bradley, Laurie Pham, Laurie Pham, Célia Blain, Célia Blain, Reston Nash, Reston Nash, Darryl Gamroth, Darryl Gamroth, Jean-Pierre Véran, Jean-Pierre Véran, } "Tomography and calibration for Raven: from simulations to laboratory results", Proc. SPIE 9148, Adaptive Optics Systems IV, 91482K (21 July 2014); doi: 10.1117/12.2057034; https://doi.org/10.1117/12.2057034


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