VST-VLT Survey Telescope Integration Status
- Belfiore,C.
- BRESCIA, Massimo
- Capaccioli,M.
- Caputi,O.
- Castiello, G.
- CORTECCHIA, Fausto
- Ferragina, L.
- FIERRO, Davide
- Fiume, V.
- MANCINI, Dario
- Mancini, G.
- Marra, G.
- MARTY, Laurent
- Mazzola, G.
- Parisi, L.
- Pellone, L.
- PERROTTA, Francesco
- Porzio, V.
- SCHIPANI, Pietro
- Sciarretta, G.
- Spirito, G.
- Valentino, M.
Publication date
January 2004
DOI Publisher
World Scientific Publishing and Mainland PressAbstract
The VLT Survey Telescope (VST) is a 2.6 m aperture, wide-field (1°1°), 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
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