Poster + Presentation
13 December 2020 Infrared wavefront sensing for adaptive optics assisted galactic center observations with GRAVITY
Author Affiliations +
Conference Poster
Abstract
We describe the operation of the infrared wavefront sensing based Adaptive Optics system CIAO. The Coudé Infrared Adaptive Optics (CIAO) system is a central auxiliary component of the Very Large Telescope interferometer (VLTI). It enables in particular Galactic Center observations using the GRAVITY interferometric instrument. CIAO compensates for phase disturbances caused by atmospheric turbulence, which all four 8 m Unit Telescopes (UT) experience during observation. Each of the four CIAO units generates an almost diffraction-limited image quality at its UT, which ensures that maximum flux of the observed stellar object enters the input fibers of GRAVITY. We present CIAO performance data obtained in the first 3 years of operation. We describe how CIAO is configured and used for observations with GRAVITY. We focus on the outstanding features of the infrared sensitive Saphira detector, which is used for the first time on Paranal, and show how it works as a wavefront sensor detector.
Conference Presentation
© (2020) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Stefan Hippler, Wolfgang Brandner, Silvia Scheithauer, Martin Kulas, Johana Panduro, Peter Bizenberger, Henri Bonnet, Casey Deen, Françoise Delplancke-Ströbele, Frank Eisenhauer, Gert Finger, Zoltan Hubert, Johann Kolb, Eric Müller, Laurent Pallanca, Julien Woillez, and Gérard Zins "Infrared wavefront sensing for adaptive optics assisted galactic center observations with GRAVITY", Proc. SPIE 11448, Adaptive Optics Systems VII, 114484K (13 December 2020); https://doi.org/10.1117/12.2560222
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KEYWORDS
Adaptive optics

Wavefront sensors

Infrared radiation

Interferometers

Infrared sensors

Infrared telescopes

Sensors

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