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Proceedings Paper

National Optical Astronomy Observatories (NOAO) Infrared Adaptive Optics Program Iv: Ir Background Speckle Noise Induced By Adaptive Optics In Astronomical Telescopes
Author(s): Francois Roddier; Peter Eisenhardt
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Paper Abstract

The infrared emission of astronomical sources is buried in a large background due to the thermal emission of the telescope. The real time deformations of an adaptive flexible mirror are likely to produce a spurious modulation of this background, adding noise to the signal. We estimate here the amount of noise introduced by such a mirror.

Paper Details

Date Published: 20 August 1986
PDF: 9 pages
Proc. SPIE 0628, Advanced Technology Optical Telescopes III, (20 August 1986); doi: 10.1117/12.963547
Show Author Affiliations
Francois Roddier, National Optical Astronomy Observatories (United States)
Peter 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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