Preliminary design of a superconducting heterodyne array receiver for Leighton Chajnantor Telescope
Infrared, Millimeter-Wave, and Terahertz Technologies IX(2022)
Abstract
The Leighton Chajnantor Telescope (LCT) project, sponsored by Shanghai Normal University in collaboration with Caltech and the University of Concepcion, is seeking to relocate the Caltech Submillimeter Observatory (CSO)[1] from Mauna Kea, Hawaii to Llano de Chajnantor Observatory on the Chajnantor Plateau in Chile. The LCT will be equipped with a new 345-GHz band heterodyne array receiver of 3x3 beams and quantum-limited sensitivity. Based on superconducting Nb/Al-AlOx/Nb tunnel junction (SIS) mixers, we have developed a compact 1x3 array as one unit of the new heterodyne array receiver. Detailed design and measurement results will be presented.
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