An overview of the planned CCAT software system
T Jenness, MC Shepherd, R Schaaf… - … for Astronomy III, 2014 - spiedigitallibrary.org
T Jenness, MC Shepherd, R Schaaf, J Sayers, V Ossenkopf, T Nikola, G Marsden, R Higgins…
Software and Cyberinfrastructure for Astronomy III, 2014•spiedigitallibrary.orgCCAT will be a 25m diameter sub-millimeter telescope capable of operating in the 0.2 to 2.1
mm 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.
mm 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.
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.
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