VST - VLT Survey Telescope Integration Status

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dc.creatorBelfiore, C.
dc.creatorBrescia, M.
dc.creatorCapaccioli, M.
dc.creatorCaputi, O.
dc.creatorCastiello, G.
dc.creatorCortecchia, F.
dc.creatorFerragina, L.
dc.creatorFierro, D.
dc.creatorFiume, V.
dc.creatorMancini, D.
dc.creatorMancini, G.
dc.creatorMarra, G.
dc.creatorMarty, L.
dc.creatorMazzola, G.
dc.creatorParisi, L.
dc.creatorPellone, L.
dc.creatorPerrotta, F.
dc.creatorPorzio, V.
dc.creatorSchipani, P.
dc.creatorSciarretta, G.
dc.creatorSpirito, G.
dc.creatorValentino, M.
dc.creatorSedmak, G.
dc.date2005-01-27
dc.date.accessioned2026-07-07T02:16:52Z
dc.date.available2026-07-07T02:16:52Z
dc.descriptionThe VLT Survey Telescope (VST) is a 2.6m aperture, wide field, UV to I facility, to be installed at the European Southern Observatory (ESO) on the Cerro Paranal Chile. VST was primarily intended to complement the observing capabilities of VLT with wide-angle imaging for detecting and pre-characterising sources for further observations with the VLT.
dc.description2 pages, 2 figures, conference
dc.identifierhttps://arxiv.org/abs/astro-ph/0501598
dc.identifierhttp://arxiv.org/abs/astro-ph/0501598
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/8957
dc.subjectAstrophysics
dc.titleVST - VLT Survey Telescope Integration Status
dc.typetext

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