Paper
23 July 2008 The VST secondary mirror support system
P. Schipani, F. Perrotta, C. Molfese, O. Caputi, L. Ferragina, L. Marty, M. Capaccioli, D. Gallieni, P. Fumi, E. Anaclerio, P. Lazzarini, G. De Paris
Author Affiliations +
Abstract
The VST telescope is equipped with an active optics system based on a wavefront sensor, a set of axial actuators to change the primary mirror shape and a secondary mirror positioner stage. The secondary mirror positioning capability allows the correction of defocus and coma optical aberrations, mainly caused by incorrect relative positions of the optics. The secondary mirror positioner is a 6-6 Stewart platform (also called "hexapod"). It is a parallel robot with a mobile platform moved by 6 linear actuators acting simultaneously. This paper describes the secondary mirror support system and the current status of the work.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
P. Schipani, F. Perrotta, C. Molfese, O. Caputi, L. Ferragina, L. Marty, M. Capaccioli, D. Gallieni, P. Fumi, E. Anaclerio, P. Lazzarini, and G. De Paris "The VST secondary mirror support system", Proc. SPIE 7018, Advanced Optical and Mechanical Technologies in Telescopes and Instrumentation, 701845 (23 July 2008); https://doi.org/10.1117/12.787925
Lens.org Logo
CITATIONS
Cited by 13 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Mirrors

Monochromatic aberrations

Telescopes

Active optics

Actuators

Image analysis

Kinematics

Back to Top