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| Paper: |
The CCAT Software System |
| Volume: |
485, Astronomical Data Analysis Software and Systems XXIII |
| Page: |
49 |
| Authors: |
Jenness, T.; Brazier, A.; Edwards, K.; Marsden, G.; Nikola, T.; Ossenkopf, V.; Padin, S.; Sayers, J.; Schaaf, R.; Shepherd, M. |
| Abstract: |
CCAT will be a 25-meter telescope for submillimeter astronomy
located at 5600 m altitude on Cerro Chajnantor in northern Chile.
CCAT will combine high sensitivity, a wide field of view, and a
broad wavelength range (0.35 to 2.1 mm) to provide an unprecedented
capability for deep, large-area multicolor submillimeter. It
is planned to have a suite of instruments including large format KID
cameras, a large heterodyne array and a KID-based
direct detection multi-object spectrometer. The remote location
drives a desire for fully autonomous observing coupled with data
reduction pipelines and fast feedback to principal investigators. |
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