The VST telescope control software in the ESO VLT environment

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dc.creatorSchipani, P.
dc.creatorBrescia, M.
dc.creatorMancini, D.
dc.creatorMarty, L.
dc.creatorSpirito, G.
dc.date2001-11-07
dc.date2001-12-06
dc.date.accessioned2026-07-07T02:01:16Z
dc.date.available2026-07-07T02:01:16Z
dc.descriptionThe VST (VLT Survey Telescope) is a 2.6 m 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.
dc.description3 pages, 2 figures, ICALEPCS 2001 Conference, PSN#THAP051
dc.identifierhttps://arxiv.org/abs/astro-ph/0111139
dc.identifierhttp://arxiv.org/abs/astro-ph/0111139
dc.identifiereConf C011127 (2001) THAP051
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/3683
dc.subjectAstrophysics
dc.titleThe VST telescope control software in the ESO VLT environment
dc.typetext

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