Choosing a control system for CCAT
2010
The Cornell Caltech Atacama Telescope1 is a 25m aperture sub-millimeter wavelength telescope to be built in northern
Chile at an altitude of 5600m. Like any modern telescope, CCAT will require a powerful and comprehensive control
system; writing one from scratch is not affordable, so the CCAT TCS must be based, at least in part, on existing
software. This paper describes how the search for a suitable system (or systems) was carried out, looks at the criteria
used to judge the feasibility of various approaches to developing the new system, and suggests the further studies needed
to validate the choices. Although the purpose of the study was to find a control system for a specific telescope with its
own particular technical requirements, many of the factors considered, such as maintainability, the ability to adapt to new
requirements in the future and so on, are of concern to all telescopes. Consequently, the processes used to select the
system for CCAT are relevant to other projects faced with the same decision, even if the conclusions turn out to be
different.
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