A 210?280 GHz sis heterodyne receiver for the James Clerk Maxwell Telescope part I: Design and performance
- 1 May 1992
- journal article
- Published by Springer Nature in International Journal of Infrared and Millimeter Waves
- Vol. 13 (5) , 647-658
- https://doi.org/10.1007/bf01010688
Abstract
No abstract availableKeywords
This publication has 12 references indexed in Scilit:
- A 210?280 GHz sis heterodyne receiver for the James Clerk Maxwell Telescope part II: CalibrationInternational Journal of Infrared and Millimeter Waves, 1992
- Quality and performance of tunable waveguide backshortsElectronics Letters, 1991
- A 345GHz SIS receiver for radio astronomyInternational Journal of Infrared and Millimeter Waves, 1989
- A low noise SIS receiver covering the frequency range 215?250 GHzInternational Journal of Infrared and Millimeter Waves, 1988
- Low-noise SIS heterodyne receiver at 230 GHzElectronics Letters, 1987
- Scaled model measurements of embedding impedances for SIS waveguide mixersInternational Journal of Infrared and Millimeter Waves, 1985
- All Solid-State Low-Noise Receivers for 210-240 GHzIEEE Transactions on Microwave Theory and Techniques, 1982
- Dual-Harmonic Noncontacting Millimeter Waveguide Backshorts: Theory, Design, and TestIEEE Transactions on Microwave Theory and Techniques, 1982
- Offset masks for lift-off photoprocessingApplied Physics Letters, 1977
- Theoretical and Experimental Analysis of a Waveguide Mounting StructureIEEE Transactions on Microwave Theory and Techniques, 1971