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arXiv · 1607.05170

Natural guide-star processing for wide-field laser-assisted AO systems

Carlos M. Correia·Benoit Neichel·Jean-Marc Conan·Cyril Petit·Jean-Francois Sauvage·Thierry Fusco·Joel D. R. Vernet·Niranjan Thatte
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Abstract

Sky-coverage in laser-assisted AO observations largely depends on the system's capability to guide on the faintest natural guide-stars possible. Here we give an up-to-date status of our natural guide-star processing tailored to the European-ELT's visible and near-infrared (0.47 to 2.45 {\mu}m) integral field spectrograph - Harmoni. We tour the processing of both the isoplanatic and anisoplanatic tilt modes using the spatio-angular approach whereby the wave-front is estimated directly in the pupil plane avoiding a cumbersome explicit layered estimation on the 35-layer profiles we're currently using. Taking the case of Harmoni, we cover the choice of wave-front sensors, the number and field location of guide-stars, the optimised algorithms to beat down angular anisoplanatism and the performance obtained with different temporal controllers under split high-order/low-order tomography or joint tomography. We consider both atmospheric and far greater telescope wind buffeting disturbances. In addition we provide the sky-coverage estimates thus obtained.

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Carlos M. Correia, Benoit Neichel, Jean-Marc Conan, Cyril Petit, Jean-Francois Sauvage, Thierry Fusco, Joel D. R. Vernet, Niranjan Thatte. 2016-07-18. Natural guide-star processing for wide-field laser-assisted AO systems. https://doi.org/10.1117/12.2232918

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