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Proceedings Paper

National Optical Astronomy Observatories (NOAO) IR Adaptive Optics Program III: Criteria For The Wavefront Sensor Selection
Author(s): L. Goad; F. Roddier; J. Beckers; P. Eisenhardt
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Paper Abstract

In the NOAO IR Adaptive Optics Program, we have elected to develop a system to use the visual light from an object to sense the wavefront errors and generate the corrections re-quired to give diffraction-limited imaging in the near-IR (2-10 microns). We have evaluated the performance of a variety of possible sensor systems, computing both their ideal performance and their expected performance with available detectors. A major consideration in this evaluation is the ability of the sensor to measure mean wavefront tilts of the visual wavefront over subapertures corresponding to the (larger) IR wavefront scale lengths. We have chosen to use a Hartmann-Shack sensor with red-sensitive image intensifiers and a Reticon detector.

Paper Details

Date Published: 20 August 1986
PDF: 9 pages
Proc. SPIE 0628, Advanced Technology Optical Telescopes III, (20 August 1986); doi: 10.1117/12.963546
Show Author Affiliations
L. Goad, National Optical Astronomy Observatories (United States)
F. Roddier, National Optical Astronomy Observatories (United States)
J. Beckers, National Optical Astronomy Observatories (United States)
P. Eisenhardt, National Optical Astronomy Observatories (United States)


Published in SPIE Proceedings Vol. 0628:
Advanced Technology Optical Telescopes III
Lawrence D. Barr, Editor(s)

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