The Development of Q-Band HEMT Receiver for VLBI

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...

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Main Authors: Do-Heung Je, Seog-Tae Han, Tae-Sung Kim, Hyun-Joo Kim, Kang-Dong Kim, Moon-Hee Chung, Chang-Hoon Lee, Duk-Goo Roh
Format: Article
Language:English
Published: The Korean Space Science Society 2004-03-01
Series:Journal of Astronomy and Space Sciences
Subjects:
Online Access:http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2004/v21n1/OJOOBS_2004_v21n1_29.pdf
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author Do-Heung Je
Seog-Tae Han
Tae-Sung Kim
Hyun-Joo Kim
Kang-Dong Kim
Moon-Hee Chung
Chang-Hoon Lee
Duk-Goo Roh
author_facet Do-Heung Je
Seog-Tae Han
Tae-Sung Kim
Hyun-Joo Kim
Kang-Dong Kim
Moon-Hee Chung
Chang-Hoon Lee
Duk-Goo Roh
author_sort Do-Heung Je
collection DOAJ
description 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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2093-1409
language English
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spelling doaj.art-ad08c1246956489cbad06239a46d5c952024-01-02T04:18:13ZengThe Korean Space Science SocietyJournal of Astronomy and Space Sciences2093-55872093-14092004-03-01211293810.5140/JASS.2004.21.1.029The Development of Q-Band HEMT Receiver for VLBIDo-Heung Je0Seog-Tae Han1Tae-Sung Kim2Hyun-Joo Kim3Kang-Dong Kim4Moon-Hee Chung5Chang-Hoon Lee6Duk-Goo Roh7Division of Radio Astronomy, Korea Astronomy Observatory 36-1 Whaamdong, Yousunggu, Daejeon Korea, 305-348Division of Radio Astronomy, Korea Astronomy Observatory 36-1 Whaamdong, Yousunggu, Daejeon Korea, 305-348Division of Radio Astronomy, Korea Astronomy Observatory 36-1 Whaamdong, Yousunggu, Daejeon Korea, 305-348Division of Radio Astronomy, Korea Astronomy Observatory 36-1 Whaamdong, Yousunggu, Daejeon Korea, 305-348Division of Radio Astronomy, Korea Astronomy Observatory 36-1 Whaamdong, Yousunggu, Daejeon Korea, 305-348Division of Radio Astronomy, Korea Astronomy Observatory 36-1 Whaamdong, Yousunggu, Daejeon Korea, 305-348Division of Radio Astronomy, Korea Astronomy Observatory 36-1 Whaamdong, Yousunggu, Daejeon Korea, 305-348Division of Radio Astronomy, Korea Astronomy Observatory 36-1 Whaamdong, Yousunggu, Daejeon Korea, 305-348A 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.http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2004/v21n1/OJOOBS_2004_v21n1_29.pdflow noise receiverHEMTVLBI
spellingShingle Do-Heung Je
Seog-Tae Han
Tae-Sung Kim
Hyun-Joo Kim
Kang-Dong Kim
Moon-Hee Chung
Chang-Hoon Lee
Duk-Goo Roh
The Development of Q-Band HEMT Receiver for VLBI
Journal of Astronomy and Space Sciences
low noise receiver
HEMT
VLBI
title The Development of Q-Band HEMT Receiver for VLBI
title_full The Development of Q-Band HEMT Receiver for VLBI
title_fullStr The Development of Q-Band HEMT Receiver for VLBI
title_full_unstemmed The Development of Q-Band HEMT Receiver for VLBI
title_short The Development of Q-Band HEMT Receiver for VLBI
title_sort development of q band hemt receiver for vlbi
topic low noise receiver
HEMT
VLBI
url http://ocean.kisti.re.kr/downfile/volume/kosss/OJOOBS/2004/v21n1/OJOOBS_2004_v21n1_29.pdf
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