The 2.6 m VST telescope is going to be installed at Cerro Paranal (Chile) as a powerful instrument for optical surveys. It is a joint project between the INAF - Osservatorio Astronomico di Capodimonte (OAC) and ESO. This paper deals with Telescope Control Software (TCS) technical aspects and software engineering design and development strategies.
Software reverse engineering and development: the VST TCS case / Schipani, P.; Brescia, M.; Mancini, D.; Marty, L.; Spirito, G.. - 314:(2004), pp. 697-701. ( Astronomical Data Analysis Software and Systems XIII Strasburgo, Francia Ottobre 2003).
Software reverse engineering and development: the VST TCS case
Brescia, M.
Co-primo
Membro del Collaboration Group
;
2004
Abstract
The 2.6 m VST telescope is going to be installed at Cerro Paranal (Chile) as a powerful instrument for optical surveys. It is a joint project between the INAF - Osservatorio Astronomico di Capodimonte (OAC) and ESO. This paper deals with Telescope Control Software (TCS) technical aspects and software engineering design and development strategies.File in questo prodotto:
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