Development of high QE, fast Avalanche Photodiodes for Astronomical Adaptive Optics

D. Bonaccini; S. Cova; M. Ghioni; R. Gheser; F. Zappa

doi:10.1364/ADOP.1995.TuA53

Adaptive Optics
Technical Digest Series (Optica Publishing Group, 1995),
paper TuA53
•https://doi.org/10.1364/ADOP.1995.TuA53

Development of high QE, fast Avalanche Photodiodes for Astronomical Adaptive Optics

D. Bonaccini, S. Cova, M. Ghioni, R. Gheser, and F. Zappa

Adaptive Optics 1995

Garching Germany
2–6 October 1995
ISBN:

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D. Bonaccini, S. Cova, M. Ghioni, R. Gheser, and F. Zappa, "Development of high QE, fast Avalanche Photodiodes for Astronomical Adaptive Optics," in Adaptive Optics, Technical Digest Series (Optica Publishing Group, 1995), paper TuA53.

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Abstract

Considering adaptive optics servosystems (AOS) in astronomical applications, a number of error sources have been identified in the wavefront sensor, which provides the reference signal of the servo-loop. These errors impair the system performance, especially with usually faint sources such as Natural Guide Stars (NGS).

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