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Proceedings Paper

A visible/infra-red low noise fast readout wavefront sensor for all-sky adaptive optics
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Paper Abstract

Current adaptive optic systems are limited by the read noise and sensitivity of their wavefront cameras. Recent advances in substrate thinning are producing focal plane arrays with high quantum efficiencies and extended spectral response over 0.5 to 1.6 microns. Infra Red Laboratories have developed and tested a new ultra-low noise readout integrated circuit (ROIC) that has a performance of 2 electrons (r.m.s.) per pixel read. We combine these two technologies to produce a new detector capable of dramatically increasing the number of available natural guide stars across the sky (and hence increased sky coverage), even in heavily obscured regions near the Galactic plane.

Paper Details

Date Published: 15 June 2006
PDF: 10 pages
Proc. SPIE 6276, High Energy, Optical, and Infrared Detectors for Astronomy II, 62760V (15 June 2006); doi: 10.1117/12.672593
Show Author Affiliations
Matthew A. Kenworthy, Steward Observatory (United States)
Philip M. Hinz, Steward Observatory (United States)
Suresh Sivanandam, Steward Observatory (United States)
Andrew H. Breuninger, Steward Observatory (United States)
Frank J. Low, IRLabs, Inc. (United States)

Published in SPIE Proceedings Vol. 6276:
High Energy, Optical, and Infrared Detectors for Astronomy II
David A. Dorn; Andrew D. Holland, Editor(s)

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