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Mark-III VLBI astrometry of pulsars

Published online by Cambridge University Press:  12 April 2016

Dayton L. Jones ,
Rachel J. Dewey ,
Carl R. Gwinn  and
Michael M. Davis
Dayton L. Jones
Affiliation:
Jet Propulsion Laboratory, Mail Code 238-700, California Institute of Technology, Pasadena, CA. 91109
Rachel J. Dewey
Affiliation:
Jet Propulsion Laboratory, Mail Code 238-700, California Institute of Technology, Pasadena, CA. 91109
Carl R. Gwinn
Affiliation:
Dept. of Physics, University of California, Santa Barbara, CA. 93106
Michael M. Davis
Affiliation:
National Astronomy and Ionosphere Center, Arecibo Observatory, P. 0. Box 995, Arecibo, P.R. 00613

Abstract

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Differential 18-cm VLBI measurements of the position of PSR 1937+214 with respect to the quasar 1923+210 have been made to improve our knowledge of the offset between the planetary ephemeris reference frame and the extragalactic radio reference frame. Our preliminary frame-tie result (VLBI – Timing position) is +21 ± 2 milli-arcseconds in right ascension and +14 ± 9 milli-arcseconds in declination. We describe the data analysis methods used and compare our results with other radio interferometric position measurements of PSR 1937+214. Our results illustrate the value of combining the large collecting area of the Arecibo telescope with the Mk-III VLBI recording system.

Type
VLBI Imaging
Information
International Astronomical Union Colloquium , Volume 131: Radio Interferometry: Theory, Techniques, and Applications , 1991 , pp. 346 - 349
Copyright
Copyright © Astronomical Society of the Pacific 1991

References

Backer, D.C., et al. 1985, A. J., 90, 2275.CrossRefGoogle Scholar
Bartel, N., et al. 1985, A. J., 90, 318.Google Scholar
Bartel, N., et al. 1990, In Workshop on the Impact of Pulsar Timing on Relativity and Cosmology (Berkeley, June 1990), p. X1.Google Scholar
Davis, M.M., et al. 1985, Nature, 315, 547.Google Scholar
Rawley, L.A., Taylor, J.H., and Davis, M.,M. 1988, Ap. J. 326, 947.Google Scholar