Cryogenically cooled K‐band high electron mobility transistor receiver for radio astronomical observation-Reference-Cited by-同舟云学术

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Cryogenically cooled K‐band high electron mobility transistor receiver for radio astronomical observation

Published:1987-03 Issue:3 Volume:58 Page:379-382
ISSN:0034-6748
Container-title:Review of Scientific Instruments
language:en
Short-container-title:Review of Scientific Instruments

Author:

Kasuga T.,Kawabe R.,Ishiguro M.,Yamada K.,Kurihara H.,Niori M.,Hirachi Y.

Publisher

AIP Publishing

Subject

Instrumentation

Link

http://aip.scitation.org/doi/pdf/10.1063/1.1139292

Reference9 articles.

1. Masers

2. Interstellar Ammonia

3. Ultra-Low-Noise 1.2- to 1.7-GHz Cooled GaAsFET Amplifiers

4. A New Field-Effect Transistor with Selectively Doped GaAs/n-AlxGa1-xAs Heterojunctions

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1. The potential for a K-band receiver on the Large Millimeter Telescope;Millimeter, Submillimeter, and Far-Infrared Detectors and Instrumentation for Astronomy X;2020-12-13

2. A 22-GHz-band low-noise down-converter for satellite broadcast receivers;IEEE Transactions on Microwave Theory and Techniques;1991-06

3. Aperture synthesis observations of NH3 in OMC-1 - Filamentary structures around Orion-KL;The Astrophysical Journal;1990-08

4. New H2O masers in the NGC 7538 region;The Astrophysical Journal;1990-06

5. Aperture synthesis observations of the molecular environment of the SGR A complex. I - The M-0.13-0.08 molecular cloud;The Astrophysical Journal;1989-12

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