Journal of Astronomy and Space Sciences (Mar 2004)

The Development of Q-Band HEMT Receiver for VLBI

  • Do-Heung Je,
  • Seog-Tae Han,
  • Tae-Sung Kim,
  • Hyun-Joo Kim,
  • Kang-Dong Kim,
  • Moon-Hee Chung,
  • Chang-Hoon Lee,
  • Duk-Goo Roh

DOI
https://doi.org/10.5140/JASS.2004.21.1.029
Journal volume & issue
Vol. 21, no. 1
pp. 29 – 38

Abstract

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A ultra low noise Q-band HEMT receiver for VLBI has been developed using a local oscillator with a very high phase stability. The performance of receiver was verified by comparison with receivers which were developed at the other countries. The receiver noise temperature shows 65 K in the frequency ragne from 42 GHz to 44 GHz, less than 100 K from 39 GHz to 46 GHz, respectively. A receiver noise temperature at SiO major line of 43GHz which will be mainly observed by using this receiver has been optimized.

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