VST - VLT Survey Telescope Integration Status

C. Belfiore; D. Fierro; D. Mancini; F. Cortecchia; F. Perrotta; G. Castiello; G. Mancini; G. Marra; G. Mazzola; G. Sciarretta

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VST - VLT Survey Telescope Integration Status

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arxiv astro-ph/0501598 v1 pith:LOZJVQ2F submitted 2005-01-27 astro-ph

C. Belfiore , M. Brescia , M. Capaccioli , O. Caputi , G. Castiello , F. Cortecchia , L. Ferragina , D. Fierro

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V. Fiume D. Mancini G. Mancini G. Marra L. Marty G. Mazzola L. Parisi L. Pellone F. Perrotta V. Porzio P. Schipani G. Sciarretta G. Spirito M. Valentino G. Sedmak

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The 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.

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