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HARP/ACSIS: A submillimetre spectral imaging system on the James Clerk Maxwell Telescope

Abstract:

This paper describes a new Heterodyne Array Receiver Programme (HARP) and Auto-Correlation Spectral Imaging System (ACSIS) that have recently been installed and commissioned on the James Clerk Maxwell Telescope (JCMT). The 16-element focal-plane array receiver, operating in the submillimetre from 325 to 375 GHz, offers high (three-dimensional) mapping speeds, along with significant improvements over single-detector counterparts in calibration and image quality. Receiver temperatures are $\sim...

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Publication status:
Published

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Authors


Buckle, JV More by this author
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Journal:
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
Volume:
399
Issue:
2
Pages:
1026-1043
Publication date:
2009-07-21
DOI:
EISSN:
1365-2966
ISSN:
0035-8711
URN:
uuid:58831101-a1fc-481d-8ee1-2df9b1b4150c
Source identifiers:
6188
Local pid:
pubs:6188
Keywords:

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