We describe design of a sideband-separating superconductor-insulator-superconductor (SIS) mixer for the APEX telescope Band 3, 385 – 500 GHz. The mixer design combines waveguide components and on-chip local oscillator (LO) injection. The receiver used quadrature scheme where the RF signal is divided equally with a 90-phase shift by a waveguide 3 dB hybrid with novel design using several microstrip probes. The LO is divided using an in-phase or 180degree waveguide E-plane Y-junction. The output waveguides of the hybrid are coupled to the mixer SIS junctions through an E-probe based on waveguide-to-microstrip transition with integrated bias-T. A directional coupler for the LO and RF signals, the SIS junction, the tuning circuitry lines and the biasT are integrated on a single mixer chip. We use a novel component, an ellipse termination to provide easy and highperformance on-chip LO injection. Index Terms — SIS mixer, sideband separating receiver, waveguide-to-microstrip transition.
[1]
V. Vassilev,et al.
High quality microstrip termination for MMIC and millimeter-wave applications
,
2005,
IEEE MTT-S International Microwave Symposium Digest, 2005..
[2]
J. Mangum,et al.
System Temperatures, Single Versus Double Sideband Operation, and Optimum Receiver Performance
,
1999
.
[3]
V. Vassilev,et al.
High performance of resistive thin-film terminations for microstrip lines
,
2004,
Infrared and Millimeter Waves, Conference Digest of the 2004 Joint 29th International Conference on 2004 and 12th International Conference on Terahertz Electronics, 2004..
[4]
V. Vassilev.
Design of Sideband Separation SIS Mixer for 3 mm Band
,
2001
.