Hostname: page-component-848d4c4894-x5gtn Total loading time: 0 Render date: 2024-05-20T12:33:55.617Z Has data issue: false hasContentIssue false
  • English
  • Français

Linking the Radio and Optical Frames with Merlin

Published online by Cambridge University Press:  25 May 2016

S.T. Garrington ,
R.J. Davis ,
L.V. Morrison  and
R.W. Argyle
S.T. Garrington
Affiliation:
Nuffield Radio Astronomy Laboratories, Jodrell Bank, UK
R.J. Davis
Affiliation:
Nuffield Radio Astronomy Laboratories, Jodrell Bank, UK
L.V. Morrison
Affiliation:
Royal Greenwich Observatory, UK
R.W. Argyle
Affiliation:
Royal Greenwich Observatory, UK

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

MERLIN positions of 12 radio stars are used to link the provisional Hipparcos reference frame to the International Celestial Reference Frame. The accuracy of the link using these radio stars is 2.3 milliarcseconds. Further observations are planned to check the accuracy of the link in the future.

Type
Part 7. Data Processing Techniques
Information
Symposium - International Astronomical Union , Volume 179: New Horizons from Multi-Wavelength Sky Surveys , 1998 , pp. 389 - 391
Copyright
Copyright © Kluwer 1998 

References

Kovalevsky, J and Lindegren, L. 1996 Astron. Astrophys. (in prep).Google Scholar
Lestrade, J.-F., et al. 1994 IAU Symp.166, pp 119–126.Google Scholar
Lindegren, L. and Kovalevsky, J. 1995 Astron. Astrophys. 304, 189.Google Scholar
Pan, X., Shao, M. and Colavita, M.M., 1993, Astrophys. J. Lett. 413, L129.Google Scholar