Capaccioli, Massimo (2006) Software Design Aspects and First Test Results of VLT Survey Telescope Control System. In: 26th meeting of the IAU, Special Session 1, 6-17 Agosto, 2006, Prague, Czech Republic.Full text not available from this repository.
The 2.6 m VLT Survey Telescope (VST) is going to be installed at Cerro Paranal (Chile) as a powerful survey instrument for the ESO VLT. The tightest requirements to be respected for such a telescope, (large field of view of 1°x1°, pixel scale of 0.21 arcs
|Item Type:||Conference or Workshop Item (UNSPECIFIED)|
|Depositing User:||ing Paolo Nicastro|
|Date Deposited:||18 Oct 2010 08:15|
|Last Modified:||30 Apr 2014 19:41|
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