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Selection of stable sources from VLBI observations from 1984 to 2006

Published online by Cambridge University Press:  01 October 2007

S. B. Qiao
Affiliation:
Shanghai Astronomical Observatory, Shanghai 200030, China Surveying and Mapping Institute, Zhengzhou 450052, China email: [email protected]
J. L. Li
Affiliation:
Shanghai Astronomical Observatory, Shanghai 200030, China
B. Zhang
Affiliation:
Shanghai Astronomical Observatory, Shanghai 200030, China
F. Tian
Affiliation:
Shanghai Astronomical Observatory, Shanghai 200030, China
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Abstract

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Based on the Calc/Solve system and aiming at the selection of stable sources, we have obtained a series of global solutions to astrometric/geodetic VLBI observations from 1984 to 2006 by changing the settings of the control parameters. After comparing the solutions and performing statistical analysis we proposed a list of 173 candidate stable sources. We also compared the list with those recommended by others authors.

Type
Contributed Papers
Copyright
Copyright © International Astronomical Union 2008

References

Feissel-Vernier, M. 2003, A&A, 403, 105Google Scholar
Fey, A. L. & Charlot, P. 1997, ApJS, 111, 95CrossRefGoogle Scholar
Fey, A. L., Ma, C., Arias, E. F., Charlot, P., Feissel-Vernier, M., Gontier, A. M., Jacobs, C. S., Li, J., & MacMillan, D. S. 2004, AJ, 127, 3587CrossRefGoogle Scholar
Ma, C., Arias, E. F., Eubanks, T. M., Fey, A. L., Gontier, A.-M., Jacobs, C. S., Sovers, O. J., Archinal, B. A., & Charlot, P. 1998, AJ, 116, 516CrossRefGoogle Scholar