Hostname: page-component-cd9895bd7-hc48f Total loading time: 0 Render date: 2024-12-12T14:31:50.609Z Has data issue: false hasContentIssue false

Development of a Radio-Astrometric Catalog by Means of Very Long Baseline Interferometry Observations*

Published online by Cambridge University Press:  12 April 2016

J. L. Fanselow
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91103
O. J. Sovers
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91103
J. B. Thomas
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91103
F. R. Bletzacker
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91103
T. J. Kearns
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91103
E. J. Cohen
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91103
G. H. Purcell Jr.
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91103
D. H. Rogstad
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91103
L. J. Skjerve
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91103
L. E. Young
Affiliation:
Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91103

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.

The Jet Propulsion Laboratory of the California Institute of Technology has been developing a radio-astrometric catalogue for use in the application of radio interferometry to interplanetary navigation and geodesy. The catalogue consists of approximately 100 compact extragalactic radio sources whose relative positions have formal uncertainties of the order of 0”.01. The sources cover nearly all of the celestial sphere above -40° declination. By using the optical counterparts of many of these radio sources, we have tied this radio reference frame to the FK4 optical system with a global accuracy of approximately 0”.01. This paper describes the status of this work.

Type
Research Article
Copyright
Copyright © Reidel 1981

Footnotes

*

This paper presents the results of one phase of research carried out at the Jet Propulsion Laboratory, California Institute of Technology, under Contract No. NAS 7-100, sponsored by t h e National Aeronautics and Space Administration.

References

* This paper presents the results of one phase of research carried out at the Jet Propulsion Laboratory, California Institute of Technology, under Contract No. NAS 7-100, sponsored by t h e National Aeronautics and Space Administration.