Paper
8 October 2007 The VST telescope optomechatronic control system
P. Schipani, M. Brescia, M. Capaccioli, D. Mancini, L. Marty, C. Molfese, F. Perrotta
Author Affiliations +
Proceedings Volume 6719, Optomechatronic Systems Control III; 67190D (2007) https://doi.org/10.1117/12.754604
Event: International Symposium on Optomechatronic Technologies, 2007, Lausanne, Switzerland
Abstract
The VST (VLT Survey Telescope) is a 2.6m optical ground-based telescope to be installed in the Cerro Paranal (Chile) observational station of the European Southern Observatory (ESO). It is a joint project of INAF-Osservatorio Astronomico di Capodimonte, responsible of the telescope design and realization, and ESO, responsible for the civil infrastructures and the daily operation of the instrument. The control system of the telescope is by definition an opto-mechatronic system. It combines mechatronic and optical disciplines together with the final aim to produce sharp images of star objects. Feedback control systems are partially based on mechatronic conventional sensors like position transducers, but also optical feedbacks coming from two separate technical CCD sensors are used to implement outer control loops for the compensation of optical aberrations e.g. introduced by the gravity, by shape imperfections or flexures in the mirrors, by thermal effects, by a not perfect alignment of the telescope axes.
© (2007) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
P. Schipani, M. Brescia, M. Capaccioli, D. Mancini, L. Marty, C. Molfese, and F. Perrotta "The VST telescope optomechatronic control system", Proc. SPIE 6719, Optomechatronic Systems Control III, 67190D (8 October 2007); https://doi.org/10.1117/12.754604
Lens.org Logo
CITATIONS
Cited by 3 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Telescopes

Mirrors

Control systems

Active optics

Stars

Wavefront sensors

Opto mechatronics

RELATED CONTENT

Commissioning telescopes from 20 cm to 8.2 m
Proceedings of SPIE (February 04 2003)
Network control system of LAMOST telescope (Invited Paper)
Proceedings of SPIE (December 06 2005)
The 3,6 m optical telescope for ARIES the control...
Proceedings of SPIE (September 24 2012)
Gemini wavefront sensing subsystems
Proceedings of SPIE (February 04 2003)
Commissioning results from the Large Binocular Telescope
Proceedings of SPIE (September 17 2012)
Field stabilization on the ESO VLT telescopes
Proceedings of SPIE (June 16 2000)

Back to Top