Presentation + Paper
16 December 2022 Preliminary design of a superconducting heterodyne array receiver for Leighton Chajnantor Telescope
Author Affiliations +
Abstract
The Leighton Chajnantor Telescope (LCT) project, sponsored by Shanghai Normal University in collaboration with Caltech and the University of Concepción, 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 3×3 beams and quantum-limited sensitivity. Based on superconducting Nb/Al-AlOx/Nb tunnel junction (SIS) mixers, we have developed a compact 1×3 array as one unit of the new heterodyne array receiver. Detailed design and measurement results will be presented.
Conference Presentation
© (2022) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
S. Q. Wang, D. Liu, B. L. Liu, M. Yao, D. Cao, F. Liu, W. Z. Shi, C. G. Shu, and S. C. Shi "Preliminary design of a superconducting heterodyne array receiver for Leighton Chajnantor Telescope", Proc. SPIE 12324, Infrared, Millimeter-Wave, and Terahertz Technologies IX, 1232404 (16 December 2022); https://doi.org/10.1117/12.2641392
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KEYWORDS
Waveguides

Receivers

Superconductors

Heterodyning

Directional couplers

Signal attenuation

Telescopes

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