1. A 350GHz radial-probe SIS mixer for astronomical imaging arrays
- Author
-
Withington, S, Leech, J, Yassin, G, Isaak, KG, Jackson, BD, Gao, JR, and Klapwijk, TM
- Subjects
Astrophysics::Instrumentation and Methods for Astrophysics ,Physics::Optics - Abstract
We have developed a 330-370GHz SIS mixer for small-format, heterodyne, astronomical imaging arrays. Fixed-tuned broadband operation is achieved by means of a superconducting radial waveguide probe. A horn-reflector antenna provides high-efficiency optical coupling. Using a variable-temperature cryogenic noise source, we measured a DSB system noise temperature of 32±1K. The mixer contributes 3±3K, supporting the theoretically-predicted result that the noise temperature of a DSB mixer can be less than (Latin small letter hwith stroke)ω/2k (8.6K). © 2001 Plenum Publishing Corporation.
- Published
- 2016