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Miyun 232 MHz Survey and Some New Imaging Techniques

Published online by Cambridge University Press:  19 July 2016

Zhang Xizhen  and
Zheng Yijia
Zhang Xizhen
Affiliation:
Beijing Astronomical Observatory, CAS, Beijing 100080, China
Zheng Yijia
Affiliation:
Beijing Astronomical Observatory, CAS, Beijing 100080, China

Abstract

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A new meter-wave survey of sky region north of declination +30° is carried out with the Miyun 232 MHz Synthesis Radio Telescope(MSRT). The instrument, observation and some new imaging techniques are briefly described in this paper. As first result, two 8° × 8° regions centred respectively at α : 00h 41m , δ: 41°12′ and α: 07h 00m , δ: 35°00′ were observed and reduced. On the average 4 – 5 sources per square degree are recorded with position accuracy of 5′ / S(Jy). The accuracy of flux determination is limited by background fluctuation which is about 30 mJy. The catalogue is complete for sources with flux larger than 0.25 Jy.

Keywords

surveyradio sourcesimaging
Type
Imaging Results: Radio and Millimeter Waves
Information
Symposium - International Astronomical Union , Volume 158: Very High Angular Resolution Imaging , 1994 , pp. 352 - 354
Copyright
Copyright © Kluwer 1994 

References

Baldwin, J.E., Boysen, R.C., Hales, S.E.G., Jenning, J.E., Waggett, P.C., Warner, P.J., Wilson, D.M.A.: 1985, MNRAS 217, 717 CrossRefGoogle Scholar
Ficarra, A., Grueff, G., Tomassetti, G.: 1985, A. Ap. Suppl. 59, 255 Google Scholar
Shouguan, Wang: 1984, Publications of Beijing Astronomical Observatory 1, 1 Google Scholar