Published July 18, 2014
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An overview of the planned CCAT software system
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.
Additional Information
© 2014 Society of Photo-Optical Instrumentation Engineers (SPIE). The CCAT Submillimeter Observatory (CCAT) is owned and operated by a consortium of universities and non-profit organizations located in the United States, Canada and Germany. Specifically the CCAT Consortium is comprised of: Cornell University, California Institute of Technology (Caltech), University of Colorado at Boulder, University of Cologne, University of Bonn, Dalhousie University, McGill University, McMaster University, University of British Columbia, University of Calgary, University of Toronto, University of Waterloo, University of Western Ontario and Associated Universities, Incorporated. The CCAT Engineering Design Phase was partially supported by funding from the National Science Foundation via AST-1118243. We thank William Peters for making Supercam commissioning data available to us for testing. We also thank Steve Padin, John Carpenter and Jeff Zivick for helpful comments on the manuscript. The SWCam prototype map-maker makes use of facilities provided by WestGrid and Compute Canada Calcul Canada.Attached Files
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Additional details
- Eprint ID
- 87841
- Resolver ID
- CaltechAUTHORS:20180713-135448617
- AST-1118243
- NSF
- Created
-
2018-07-13Created from EPrint's datestamp field
- Updated
-
2021-11-16Created from EPrint's last_modified field
- Series Name
- Proceedings of SPIE
- Series Volume or Issue Number
- 9152