Hostname: page-component-586b7cd67f-r5fsc Total loading time: 0 Render date: 2024-11-26T22:18:21.720Z Has data issue: false hasContentIssue false

Errors in high precision source position determination

Published online by Cambridge University Press:  12 April 2016

Pedro Elosegui
Affiliation:
Instituto de Astrofísica de Andalucía, Apdo. 2144, E-18080 Granada, Spain
Juan-Maria Marcaide
Affiliation:
Instituto de Astrofísica de Andalucía, Apdo. 2144, E-18080 Granada, Spain
Irwin I. Shapiro
Affiliation:
Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, U.S.A.

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.

We have made a detailed analysis of the systematic errors in the determination, from two sets of VLBI observations, of the position of the quasar 1038+528 A relative to the quasar 1038+528 B. This analysis confirms an apparent proper motion at λ=3.6cm of 26±8 μas/yr of the core of the quasar 1038+528 A relative to the quasar 1038+528 B.

Type
VLBI Imaging
Copyright
Copyright © Astronomical Society of the Pacific 1991

References

Bartel, N., Herring, T.A., Ratner, M.I., Shapiro, I.I., and Corey, B.E. 1986, Nature, 319, 733.Google Scholar
Marcaide, J.M., Shapiro, I.I., Corey, B.E., Cotton, W.D., Gorenstein, M.V., Rogers, A.E.E., Romney, J.D., Schild, R.E., Bååth, L., Bartel, N., Cohen, N.L., Clark, T.A., Preston, R.A., Ratner, M.I., and Whitney, A.R. 1985, Astr. Ap., 142, 71.Google Scholar
Marcaide, J.M., Elósegui, P., and Shapiro, I.I. 1990, In Parsec Scale Radio Jets, ed. Zensus, J.A. and Pearson, T.J., Cambridge University Press, p. 43.Google Scholar
Morabito, D.D., Niell, A.E., Preston, R.A., Linfield, R.P., Wehrle, A.E., and Faulkner, J. 1986, Astron. J., 91, 1038.Google Scholar