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
Lens.org Logo
CITATIONS
Cited by 3 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Mirrors

Telescopes

Active optics

Wavefront sensors

Monochromatic aberrations

Safety

Image quality

RELATED CONTENT

Mt ABU 2.5m Telescope: design and fabrication
Proceedings of SPIE (July 06 2018)
Active optics system for the CTIO 4-m telescope
Proceedings of SPIE (June 08 1995)
The 3,6 m optical telescope for ARIES the control...
Proceedings of SPIE (September 24 2012)
WIYN telescope active optics system
Proceedings of SPIE (June 08 1995)
Gemini prime focus wavefront sensor
Proceedings of SPIE (July 07 2000)

Back to Top