31 July 1998 Characterization of a 200-GHz SIS mixer
Author Affiliations +
We report on the status of SIS mixers being constructed at the Institute of Astronomy and Astrophysics, Academia Sinica. These mixers will later be integrated into the receiver systems used on the ASIAA supplied antennas for the SMA project. We have reproduced the SAO design for these mixers at the 200 GHz band. We achieve acceptable noise performance across the tuning band of the mixers.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Chi Chung Chin, Sung-Shiou Shen, Robert Hu, Shun-Cheng Yang, Robert N. Martin, "Characterization of a 200-GHz SIS mixer", Proc. SPIE 3357, Advanced Technology MMW, Radio, and Terahertz Telescopes, (31 July 1998); doi: 10.1117/12.317393; https://doi.org/10.1117/12.317393


A 100 115 GHz SIS receiver for radio...
Proceedings of SPIE (October 01 1991)
8-1000 GHz vector network analyzer
Proceedings of SPIE (December 01 1990)
A wideband 240 GHz receiver for the submillimeter array
Proceedings of SPIE (July 19 2016)
A combined 3mm and 1.3mm bands SIS receiver for the...
Proceedings of SPIE (August 30 1993)
Receiver-beam characterization for the SMA
Proceedings of SPIE (July 31 1998)

Back to Top