Paper
13 December 2020 CHARA array adaptive optics: complex operational software and performance
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Abstract
The CHARA Array is the longest baseline optical interferometer in the world. Operated with natural seeing, it has delivered landmark sub-milliarcsecond results in the areas of stellar imaging, binaries, and stellar diameters. However, to achieve ambitious observations of faint targets such as young stellar objects and active galactic nuclei, higher sensitivity is required. For that purpose, adaptive optics are developed to correct atmospheric turbulence and non-common path aberrations between each telescope and the beam combiner lab. This paper describes the AO software and its integration into the CHARA system. We also report initial on-sky tests that demonstrate an increase of scientific throughput by sensitivity gain and by extending useful observing time in worse seeing conditions. Our 6 telescopes and 12 AO systems with tens of critical alignments and control loops pose challenges in operation. We describe our methods enabling a single scientist to operate the entire system.
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Narsireddy Anugu, Theo ten Brummelaar, Nils H. Turner, Matthew D. Anderson, Jean-Baptiste Le Bouquin, Judit Sturmann, Laszlo Sturmann, Chris Farrington, Norm Vargas, Olli Majoinen, Michael J. Ireland, John D. Monnier, Denis Mourard, Gail Schaefer, Douglas R. Gies, Stephen T. Ridgway, Stefan Kraus, Cyril Petit, Michel Tallon, Caroline B. Lim, and Philippe Berio "CHARA array adaptive optics: complex operational software and performance", Proc. SPIE 11446, Optical and Infrared Interferometry and Imaging VII, 1144622 (13 December 2020); https://doi.org/10.1117/12.2561560
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Cited by 2 scholarly publications.
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KEYWORDS
Adaptive optics

Telescopes

Wavefront sensors

Cameras

Optical arrays

Deformable mirrors

Actuators

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