85-115-GHz receivers for radio astronomy

Details 85-115-GHz receivers for radio astronomy 85-115-GHz receivers for radio astronomy

Feb 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985itmtt..33...90w&link_type=abstract

IEEE Transactions on Microwave Theory and Techniques (ISSN 0018-9480), vol. MTT-33, Feb. 1985, p. 90-95.

Astronomy and Astrophysics

Astronomy

40

Josephson Junctions, Millimeter Waves, Mixing Circuits, Radio Astronomy, Superconductors, Superheterodyne Receivers, Lead Alloys, Low Noise, Microwave Circuits, Noise Temperature, Sidebands, Signal Mixing, Volt-Ampere Characteristics

Scientific paper

Low-noise receivers for radio astronomy have been built using Pb alloy
superconducting tunnel junction mixers operating at 4.5 K. They have
been used for 85-115-GHz astronomy with double-sideband receiver noise
temperature between 70 and 200 K. Junction fabrication and receiver
construction, operation, and performance are described herein.

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