Abstract
The Atacama Large Millimeter Array (ALMA) is a collaboration between Europe,
North America, and Japan to build an aperture synthesis telescope with more
than 50 12-m antennas at 5000 m altitude in Chile. In its full configuration,
ALMA will observe in 10 bands between 30 and 950 GHz, and will provide
astronomers with unprecedented sensitivity and spatial resolution at
millimetre and sub-millimetre wavelengths. Band 9, covering 602-720 GHz, is
the highest frequency band in the baseline ALMA project, and will thus offer
the telescope's highest spatial resolutions. This paper describes the
design of the Band 9 receiver cartridges for the Atacama Large Millimeter
Array (ALMA). These are field-replaceable heterodyne front-ends offering high
sensitivity, 602-720 GHz frequency coverage, 4-12 GHz IF bandwidth, and high
quasioptical efficiencies. Because the project will ultimately require up
to 64 cartridges to fully populate the ALMA array, two key aspects of the
design of the Band 9 cartridge have been to take advantage of commercial
manufacturing capabilities and to simplify the assembly of the cartridge.
Original language | English |
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Title of host publication | Proceedings of the Ninteenth International Symposium on Space Terahertz Technology, held April 28-30, 2008, in Groningen |
Editors | Wolfgang Wild |
Pages | 258-262 |
Publication status | Published - 1-Apr-2008 |
Event | 19th International Symposium on Space Terahertz Technology 2008 - Groningen, Netherlands Duration: 28-Apr-2008 → 30-Apr-2008 |
Conference
Conference | 19th International Symposium on Space Terahertz Technology 2008 |
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Country/Territory | Netherlands |
City | Groningen |
Period | 28/04/2008 → 30/04/2008 |