Paper
27 July 2016 Speckle nulling wavefront control for Palomar and Keck
Michael Bottom, Bruno Femenia, Elsa Huby, Dimitri Mawet, Richard Dekany, Jennifer Milburn, Eugene Serabyn
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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.
© (2016) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Michael Bottom, Bruno Femenia, Elsa Huby, Dimitri Mawet, Richard Dekany, Jennifer Milburn, and Eugene Serabyn "Speckle nulling wavefront control for Palomar and Keck", Proc. SPIE 9909, Adaptive Optics Systems V, 990955 (27 July 2016); https://doi.org/10.1117/12.2233025
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CITATIONS
Cited by 16 scholarly publications.
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KEYWORDS
Speckle

Deformable mirrors

Adaptive optics

Nulling interferometry

Calibration

Imaging systems

Coronagraphy

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