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VLBI Astrometry

Published online by Cambridge University Press:  19 July 2016

J. E. Reynolds*
Affiliation:
Australia Telescope National Facility, CSIRO

Abstract

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VLBI is at present the most accurate technique for measuring radiosource positions and the only method capable of high precision for a reasonable number of sources. The applications of VLBI astrometry in stellar, Galactic and extra-Galactic regimes are reviewed. In particular, substantial progress has been made in the last few years towards a global reference frame of extragalactic radiosource positions. The status of this frame, and of the link to the optical reference frames is also described.

Type
Astrometry
Copyright
Copyright © Kluwer 1994 

References

Bailes, M. & Johnston, S.: 1993, in URSI Review of Radio Science, ed. Stone, W. R. (in press).Google Scholar
Bartel, N. et al.: 1986, Nature, 319, 733.Google Scholar
Davis, J.L. et al.: 1985, Radio Science, 20, 1593.Google Scholar
Fey, A.L. et al.: 1992, Astron. J., 104, 891.Google Scholar
Harvey, B.R. et al.: 1992, Astron. J., 103, 229.Google Scholar
Jacobs, C.S.: 1993, in Proc. IAU Symp. 156, Developments in Astrometry & Their Impacts on Astrophysics & Geodynamics, Shanghai, 1992 (in press).Google Scholar
Jauncey, D.L.: 1991, Aust. J. Phys., 44, 785.Google Scholar
Johnston, K.J. et al.: 1985, Astron. J., 90, 1343.Google Scholar
Johnston, K.J. et al.: 1988, in Proc. IAU Symp. 129, The Impact of VLBI on Astrophysics and Geophysics, eds. Reid, M. & Moran, J., Reidel:Dordrecht, p317.Google Scholar
Johnston, S. et al.: 1993, Nature, 361, 613.Google Scholar
Lestrade, J.F. et al.: 1990, Astron. J., 99, 1663.Google Scholar
Lestrade, J.F. et al.: 1992, Astron. & Astrophys., 258, 112.Google Scholar
Lowe, S.T.: 1993, in Proc. IAU Symp. 156, Developments in Astrometry & and Their Impacts on Astrophysics & Geodynamics, Shanghai, 1992 (in press).Google Scholar
Ma, C. et al.: 1986, Astron. J., 92, 1020.Google Scholar
Moran, J.M.: 1993 in Proc. Symp. on Sub-Arcsecond Radio Astronomy, Manchester, 1992 (in press).Google Scholar
Reid, et al.: 1988, Astrophys. J., 330, 809.CrossRefGoogle Scholar
Reynolds, J.E. et al.: 1993, Astron, J., (to be submitted).Google Scholar
Robertson, D.S., Carter, W.E. & Dillinger, W.H.: 1991, Nature, 349, 768.Google Scholar
Rogers, A.E.E.: 1976, in Methods of Experimental Physics Vol 12C, ed. Meeks, M. L., Academic Press:New York, p139.Google Scholar
Rogers, A.E.E. et al.: 1983, Science, 219, 51.Google Scholar
Russell, J.L. et al.: 1992, Astron. J., 103, 2090.Google Scholar
Russell, J.L. et al.: 1993, in Proc. Symp. on Sub-Arcsecond Radio Astronomy, Manchester, 1992 (in press).Google Scholar
Shapiro, I.I.: 1976, in Methods of Experimental Physics Vol 12C, ed. Meeks, M. L., Academic Press:New York, p261.Google Scholar
Sovers, O.J.: 1991, JPL Publication 83–39, Rev. 4.Google Scholar
Sovers, O.J. et al.: 1988, Astron J., 95, 1647.Google Scholar
Staveley-Smith, L.S. et al.: 1992, Nature, 355, 147.Google Scholar
Thompson, A.R., Moran, J.M. & Swenson, G.W.: 1986, Interferometry and Synthesis in Radio Astronomy, Wiley:New York.Google Scholar
Wade, C.M. & Johnston, K.J.: 1976, Astron. J., 82, 791.Google Scholar
Walter, H.: 1993, in Proc. IAU Symp. 156, Developments in Astrometry & Their Impacts on Astrophysics & Geodynamics, Shanghai, 1992 (in press).Google Scholar
White, G.L. et al.: 1990, Astron. J., 99, 405.Google Scholar
Whitney, A.R. et al.: 1991, NOAA Technical Report NOS 137 NGS 49, Proc. of the AGU Chapman Conference on Geodetic VLBI: Monitoring Global Change, U.S. Department of Commerce, Rockville, Maryland.Google Scholar