ABSTRACT
ICALEPCS 2001

Abstracts



THAP051 (Poster)

Presenter: Dario Mancini (Osservatorio Astronomico di Capodimonte)
email: schipani@na.astro.it
Review Status: Proceedings Ready - 03/12/02
FullText: pdf
Eprint: astro-ph/0111139

The VST Telescope Control Software in the ESO VLT Environment

P. Schipani, M. Brescia, D. Mancini, L. Marty, G. Spirito (OAC)

The VST (VLT Survey Telescope) is a 2.6 m class Alt-Az telescope to be installed at Mount Paranal in 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. This paper will focus mainly on control software aspects, describing the VST software architecture in the context of the whole ESO VLT control concept. The general architecture and the main components of the control software will be described.
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ICALEPCS 2001

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