Abstract
CCAT will be a 25m diameter sub-millimeter telescope capable of operating in the 0.2 to 2.1mm wavelength range. It will be located at an altitude of 5600m on Cerro Chajnantor in northern Chile near the ALMA site. The anticipated first generation instruments include large format (60,000) kinetic inductance detector (KID) cameras, a large format heterodyne array and a direct detection multi-object spectrometer. The paper describes the architecture of the CCAT software and the development strategy. © 2014 SPIE.
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CITATION STYLE
Jenness, T., Shepherd, M. C., Schaaf, R., Sayers, J., Ossenkopf, V., Nikola, T., … Brazier, A. (2014). An overview of the planned CCAT software system. In Software and Cyberinfrastructure for Astronomy III (Vol. 9152, p. 91522W). SPIE. https://doi.org/10.1117/12.2056516
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