Astronomy and Astrophysics – Astronomy
Scientific paper
Jun 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ijimw..10..579v&link_type=abstract
International Journal of Infrared and Millimeter Waves (ISSN 0195-9271), vol. 10, June 1989, p. 579-593.
Astronomy and Astrophysics
Astronomy
1
Closed Cycles, Cryogenic Cooling, Radio Telescopes, Receivers, Sis (Superconductors), Intermediate Frequency Amplifiers, Liquid Helium, Microwave Oscillators, Mixing Circuits, Noise Temperature, Refrigerating Machinery
Scientific paper
A mechanically tunable SIS receiver covering the frequency range from 125 to 170 GHz is described. For cooling at 2.8 K, a closed cycle refrigeration system has been developed that has a cooling power of 350 mW at 2.8 K. The IF is centered at 1.4 GHz, with a bandwidth of 600 MHz. For preamplification, a cryogenic two-stage HEMT amplifier has been developed that has a noise temperature of about 7 K. Typical broadband (600 MHz) values are between 50 and 200 K, depending on the frequency. The receiver is used for radioastronomical measurements at the Cologne 3-m radio-telescope.
Eigler K.
Hilberath W.
Jacobs Karl
Mueller Ph.
Vowinkel Bernd
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