Paper
17 September 2012 The active optics system of the VST: concepts and results
Author Affiliations +
Abstract
The active optics system of the VLT Survey Telescope (VST) adopts a positioning system for the secondary mirror, a system to support and modify the shape of the 2.6-m primary mirror, and a Shack-Hartmann wavefront sensor. This paper describes the concepts of the VST active optics and the commissioning of the whole system on the ESO's Paranal Observatory.
© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Pietro Schipani, Demetrio Magrin, Lothar Noethe, Carmelo Arcidiacono, Javier Argomedo, Massimo Dall'Ora, Sergio D'Orsi, Jacopo Farinato, Laurent Marty, Roberto Ragazzoni, and Gabriele Umbriaco "The active optics system of the VST: concepts and results", Proc. SPIE 8444, Ground-based and Airborne Telescopes IV, 84444Z (17 September 2012); https://doi.org/10.1117/12.925493
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Cited by 3 scholarly publications.
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KEYWORDS
Mirrors

Telescopes

Active optics

Wavefront sensors

Monochromatic aberrations

Safety

Image quality

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