Preliminary design of a superconducting heterodyne array receiver for Leighton Chajnantor Telescope

Shuqin Wang,Dong Liu,Bo-Liang Liu, Ming Yao,Duo Cao, Feng Liu,Wangzhou Shi, Chenggang Shu,Shengcai Shi

Infrared, Millimeter-Wave, and Terahertz Technologies IX(2022)

Cited 0|Views0
No score
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.
More
Translated text
AI Read Science
Must-Reading Tree
Example
Generate MRT to find the research sequence of this paper
Chat Paper
Summary is being generated by the instructions you defined