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.
VST – VLT Survey Telescope Integration Status / Belfiore, C., Brescia, M., Capaccioli, M., Caputi, O., Castiello, G., Cortecchia, F., Ferragina, L., Fierro, D., Fiume, V., Mancini, D., Mancini, G., Marra, G., Marty, L., Mazzola, G., Parisi, L., Pellone, L., Perrotta, F., Porzio, V., Schipani, P., Sciarretta, G., et al.. - (2004), pp. 303-304. (Thinking, Observing And Mining The Universe Sorrento (Napoli) Settembre 2003) [10.1142/9789812702999_0036].
VST – VLT Survey Telescope Integration Status
Brescia M
Writing – Original Draft Preparation
;Capaccioli M;
2004
Abstract
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.| File | Dimensione | Formato | |
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