Proceedings Paper
Next generation heterodyne array for JCMT| Format | Member Price | Non-Member Price |
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Paper Abstract
As part of the JCMT Future Instrumentation Project, the EAO looks to optimize the premier niche of the facility as the
go-to telescope for fast, deep wide-field mapping of the universe at 345 GHz (850 um). The next generation heterodyne
array for JCMT will be designed to provide deep ultra-fast mapping capabilities that takes advantage of the full field-of-view
available to the telescope, and an array of 90 SIS mixers. This paper presents a preliminary design options and the
critical science drivers for the project.
Paper Details
Date Published: 19 July 2016
PDF: 6 pages
Proc. SPIE 9914, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII, 991429 (19 July 2016);
Published in SPIE Proceedings Vol. 9914:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII
Wayne S. Holland; Jonas Zmuidzinas, Editor(s)
PDF: 6 pages
Proc. SPIE 9914, Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII, 991429 (19 July 2016);
Show Author Affiliations
M.-T. Chen, Academia Sinica (Taiwan)
J. Dempsey, East Asian Observatory (United States)
P. T. P. Ho, Academia Sinica (Taiwan)
East Asian Observatory (United States)
J. Dempsey, East Asian Observatory (United States)
P. T. P. Ho, Academia Sinica (Taiwan)
East Asian Observatory (United States)
P. Friberg, East Asian Observatory (United States)
D. Bintley, East Asian Observatory (United States)
C. Walther, East Asian Observatory (United States)
D. Bintley, East Asian Observatory (United States)
C. Walther, East Asian Observatory (United States)
Published in SPIE Proceedings Vol. 9914:
Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy VIII
Wayne S. Holland; Jonas Zmuidzinas, Editor(s)
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