[1]
Z. B Zhang, G.L. Wang, X. Liu, Z.H. Tang, Analysis of EOP Determination via Chinese VLBI Network, Geomatics and Information Science of Wuhan University, 38 (8): 911, (2013).
Google Scholar
[2]
G.L. Wang and M. H Xu. An Analysis of UT1 Determined by IVS Intensive Observations. Chinese Astronomy and Astrophysics, 36(4): 408{416, (2012).
DOI: 10.1016/j.chinastron.2012.10.006
Google Scholar
[3]
Qian Zhihan, Wu Linda, Very Long Baseline Interferometry, Mapping Publishing Company, (1983).
Google Scholar
[4]
K. Baver, D. MacMillan, L. Petrov, and et al. Analysis of the VLBI intensive sessions. International VLBI Service for Geodesy and Astrometry 2004 General Meeting Proceedings. NASA/CP-2004-212255, pages 394-398, (2004).
Google Scholar
[5]
K.D. Baver, J.M. Gipson, and D.S. MacMillan. Strategies for Improving the IVS-INT01 UT1 Estimates: Preliminary Results of RD0907 through RD0910. (2009).
Google Scholar
[6]
M. Vennebusch. Investigations on European Baseline Rates. In Proceedings of the 16th Working Meeting on European VLBI for Geodesy and Astrometry, held at Leipzig, May, volume 9, (2003).
Google Scholar
[7]
M. Vennebusch, A. Nothnagel, and H. Kutterer. Singular value decomposition and cluster analysis as regression diagnostics tools for geodetic applications. Journal of Geodesy, 83(9): 877- 891, (2009).
DOI: 10.1007/s00190-009-0306-5
Google Scholar
[8]
M. Uunila, A. Nothnagel, and J. Leek. In ence of Source Constellations on UT1 Derived from IVS INT1 Sessions. In IVS 2012 General Meeting Proceedings, pp.395-399, volume 1, pages 395-399, (2013).
Google Scholar
[9]
Z.B. Zhang, X. Liu, and J. N Gao. ZenithWet Delay Estimation and Radio Source Sky Coverage. Advanced Materials Research, 718: 593-599, (2013).
DOI: 10.4028/www.scientific.net/amr.718-720.593
Google Scholar
[10]
I. Jurkevich. A method of computing periods of cyclic phenomena. Astrophysics and Space Science, 13(1): 154-167, (1971).
DOI: 10.1007/bf00656321
Google Scholar
[11]
D.N. Swingler. A comparison of the fourier, jurkevich, and stellingwerf methods of period estimation. The Astronomical Journal, 97: 280-287, (1989).
DOI: 10.1086/114981
Google Scholar