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A New 4–8 GHz Receiver for Kunming Station

Wen Chen, Longfei Hao, Zhixuan Li, Yonghua Xu, Min Wang

Труды ИПА РАН, вып. 41, 41–44 (2017)

Ключевые слова: VLBI, Astrometry, C-Band

Аннотация

Yunnan Astronomical Observatories (YNAO) is located in Kunming, Yunnan province, has a 40 m Radio Telescope which is part of the Chinese VLBI Network (CVN). Kunming station have installed a new C-Band receiver, so we can carry on more international VLBI observations in C-band, and will soon to be one of EVN stations. We got the first fringes with EVN fringe-test experiment in C-band last month. The Kunming station shows its good compatibility to work with the EVN in C-band.

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Wen Chen, Longfei Hao, Zhixuan Li, Yonghua Xu, Min Wang. A New 4–8 GHz Receiver for Kunming Station // Труды ИПА РАН. — 2017. — Вып. 41. — С. 41–44.

@article{chen2017,
  abstract = {Yunnan Astronomical Observatories (YNAO) is located in Kunming, Yunnan province, has a 40 m Radio Telescope which is part of the Chinese VLBI Network (CVN). Kunming station have installed a new C-Band receiver, so we can carry on more international VLBI observations in C-band, and will soon to be one of EVN stations. We got the first fringes with EVN fringe-test experiment in C-band last month. The Kunming station shows its good compatibility to work with the EVN in C-band.},
  author = {Wen Chen and Longfei Hao and Zhixuan Li and Yonghua Xu and Min Wang},
  issue = {41},
  journal = {Труды ИПА РАН},
  keyword = {VLBI, Astrometry, C-Band},
  pages = {41--44},
  title = {A New 4–8 GHz Receiver for Kunming Station},
  url = {http://iaaras.ru/library/paper/1700/},
  year = {2017}
}

TY  - JOUR
TI  - A New 4–8 GHz Receiver for Kunming Station
AU  - Chen, Wen
AU  - Hao, Longfei
AU  - Li, Zhixuan
AU  - Xu, Yonghua
AU  - Wang, Min
PY  - 2017
T2  - Труды ИПА РАН
IS  - 41
SP  - 41
AB  - Yunnan Astronomical Observatories (YNAO) is located in Kunming,
Yunnan province, has a 40 m Radio Telescope which is part of the
Chinese VLBI Network (CVN). Kunming station have installed a new
C-Band receiver, so we can carry on more international VLBI
observations in C-band, and will soon to be one of EVN stations. We
got the first fringes with EVN fringe-test experiment in C-band last
month. The Kunming station shows its good compatibility to work with
the EVN in C-band.
UR  - http://iaaras.ru/library/paper/1700/
ER  -