Astronomy and Astrophysics – Astrophysics
Scientific paper
2001-11-07
eConf C011127 (2001) WEAP061
Astronomy and Astrophysics
Astrophysics
3 pages, 5 figures, ICALEPCS 2001 Conference, PSN#WEAP061
Scientific paper
The VST (VLT Survey Telescope) is a 2.6 m class Alt-Az telescope to be installed on Cerro Paranal in the Atacama desert, Northern Chile, in the European Southern Observatory (ESO) site. The VST is a wide-field imaging facility planned to supply databases for the ESO Very Large Telescope (VLT) science and carry out stand-alone observations in the UV to I spectral range. So far no telescope has been dedicated entirely to surveys; the VST will be the first survey telescope to start the operation, as a powerful survey facility for the VLT observatory. This paper will focus on the axes motion control system. The dynamic model of the telescope will be analyzed, as well as the effect of the wind disturbance on the telescope performance. Some algorithms for the telescope position control will be briefly discussed.
Mancini Dario
Schipani Pietro
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