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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
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
Fomalont, E.B., Goss, W.G., Lyne, A.G., Manchester, R. N., R.N., , & Justtanont, K.
1992, MNRAS, 258, 497.Google Scholar
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