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; Spirito, G; Valentino, M; Sedmak, G. - (2004), pp. 303-304. (Intervento presentato al convegno Thinking, Observing And Mining The Universe tenutosi a Sorrento (Napoli) nel 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 | |
---|---|---|---|
15-16-Belfiore-TOMU.pdf
solo utenti autorizzati
Tipologia:
Versione Editoriale (PDF)
Licenza:
Copyright dell'editore
Dimensione
392 kB
Formato
Adobe PDF
|
392 kB | Adobe PDF | Visualizza/Apri Richiedi una copia |
I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.