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Timing noise as a source of discrepancy between timing and VLBI pulsar positions

Published online by Cambridge University Press:  12 April 2016

A. E. Rodin ,
Yu. P. Ilyasov ,
V. V. Oreshko  and
M. Sekido
A. E. Rodin
Affiliation:
PRAO ASC LPI, Pushchino, Moscow region, 142292, Russia
Yu. P. Ilyasov
Affiliation:
PRAO ASC LPI, Pushchino, Moscow region, 142292, Russia
V. V. Oreshko
Affiliation:
PRAO ASC LPI, Pushchino, Moscow region, 142292, Russia
M. Sekido
Affiliation:
KSRC CRL, 893-1, Hirai, Kashima, Ibaraki, 314, Japan

Abstract

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Pulsar positions obtained by VLBI and timing are compared. The difference between these positions is proven to be mainly due to timing noise. A new method which significantly reduces the difference have been developed.

Type
Part 2. Timing, General Relativity and Astrometry
Information
International Astronomical Union Colloquium , Volume 177: Pulsar Astronomy - 2000 and Beyond , 2000 , pp. 145 - 146
Copyright
Copyright © Astronomical Society of the Pacific 2000

References

Doroshenko, O.V., & Kopeikin, S.M. 1990, Sov. Astr., 34, 496.Google Scholar
Downs, G.S., Reichly, P.E. 1983, ApJ, 53, 169.Google Scholar
Fomalont, E.B., Goss, W.G., Lyne, A.G., Manchester, R. N., R.N., , & Justtanont, K. 1992, MNRAS, 258, 497.Google Scholar
Ilyasov, Yu. P., Potapov, V.A., & Rodin, A.E. 1999, This proceedings.Google Scholar
Rodin, A.E. 2000, PhD thesis, P. N. Lebedev Physical Institute.Google Scholar
Taylor, J.H., & Weisberg, J.M. 1989, ApJ, 345, 434.Google Scholar