Published 2015
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A new HDF5 based raw data model for CCAT
Abstract
CCAT will be a large sub-millimeter telescope to be built near the ALMA site in northern Chile. The telescope must support a varied set of instrumentation including large format KID cameras, a large heterodyne array and a KID-based direct detection multi-object spectrometer. We are developing a new raw data model based on HDF5 that can cope with the expected data rates of order Gbit/s and is flexible enough to hold raw data from all planned instruments.
Additional Information
© 2015 Astronomical Society of the Pacific.Attached Files
Published - 495-0543.pdf
Submitted - 1410.8788v1.pdf
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Additional details
- Eprint ID
- 52507
- Resolver ID
- CaltechAUTHORS:20141209-141450484
- Created
-
2014-12-09Created from EPrint's datestamp field
- Updated
-
2023-06-02Created from EPrint's last_modified field
- Series Name
- Astronomical Society of the Pacific conference series
- Series Volume or Issue Number
- 495