Paper
13 September 2012 LIFT, a noise-effective low order focal-plane sensor: from theory to full experimental validation
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Abstract
Laser Tomographic systems, such as ATLAS, will rely on natural guide stars to sense low order aberrations. LIFT is a novel focal plane wavefront sensor (WFS), performing a maximum likelihood phase retrieval on a single image, with better sensitivity than a 2x2 Hartmann-Shack WFS. We first present a characterization of LIFT’s noise propagation performance and working domain by means of simulations. We then show the results of experiments on ONERA’s test bench for LIFT. These experiments validate the estimation of tip/tilt and focus, in monochromatic light and in large bandwidth (for a spectral resolution of 3), as well as the expected noise propagation. They also confirm the validity of the imaging models used for simulations. Finally, we focus on the preparation of an on-sky validation based on Gemini Multi-conjugate adaptive optics System (GeMS) calibration data at Gemini Southern Observatory.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Cédric Plantet, Benoit Neichel, Serge Meimon, Thierry Fusco, and Jean-Marc Conan "LIFT, a noise-effective low order focal-plane sensor: from theory to full experimental validation", Proc. SPIE 8447, Adaptive Optics Systems III, 84471O (13 September 2012); https://doi.org/10.1117/12.926895
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Cited by 3 scholarly publications.
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KEYWORDS
Monochromatic aberrations

Sensors

Wavefront sensors

Error analysis

Calibration

Stars

Turbulence

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