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Proceedings Paper

Speckle nulling wavefront control for Palomar and Keck
Author(s): Michael Bottom; Bruno Femenia; Elsa Huby; Dimitri Mawet; Richard Dekany; Jennifer Milburn; Eugene Serabyn
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Paper Abstract

We present a speckle nulling code currently being used for high contrast imaging at the Palomar and Keck telescopes. The code can operate in open and closed loop and is self-calibrating, requiring no system model and minimal hand-coded parameters. Written in a modular fashion, it is straightforward to port to different instruments. It has been used with systems operating in the optical through thermal infrared, and can deliver nearly an order of magnitude improvement in raw contrast. We will be releasing this code to the public in the near future.

Paper Details

Date Published: 27 July 2016
PDF: 16 pages
Proc. SPIE 9909, Adaptive Optics Systems V, 990955 (27 July 2016); doi: 10.1117/12.2233025
Show Author Affiliations
Michael Bottom, California Institute of Technology (United States)
Bruno Femenia, W.M. Keck Observatory (United States)
Elsa Huby, Univ. de Liège (Belgium)
Dimitri Mawet, California Institute of Technology (United States)
Richard Dekany, California Institute of Technology (United States)
Jennifer Milburn, California Institute of Technology (United States)
Eugene Serabyn, Jet Propulsion Lab. (United States)


Published in SPIE Proceedings Vol. 9909:
Adaptive Optics Systems V
Enrico Marchetti; Laird M. Close; Jean-Pierre Véran, Editor(s)

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