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The Radio Reference Frame

Published online by Cambridge University Press:  12 April 2016

R. A. Gaume  and
A. L. Fey
R. A. Gaume
Affiliation:
United States Naval Observatory, Washington, D.C, U.S.A.
A. L. Fey
Affiliation:
United States Naval Observatory, Washington, D.C, U.S.A.

Abstract

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The Radio Reference Frame, defined by the radio positions of a large number of extragalactic sources, marks a milestone in the production of a global, self-consistent, quasi–inertial celestial reference frame accurate at the milliarcsecond level. A brief review of the current status and future direction of the project is presented.

Type
Research Article
Information
International Astronomical Union Colloquium , Volume 164: Radio Emission from Galactic and Extragalactic Compact Sources , 1998 , pp. 383 - 384
Copyright
Copyright © Astronomical Society of the Pacific 1998

References

Fey, A.L., & Charlot, P. 1997. ApJS, 111, 95–142.CrossRefGoogle Scholar
Fey, A.L., Clegg, A.W., & Fomalont, E.B. 1996. ApJS, 105, 299–330.Google Scholar
Johnston, K.J., et al. 1995. AJ, 110, 880–915.Google Scholar