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| Paper: |
Limits on pulsar planetary systems from the Jodrell Bank timimg database |
| Volume: |
36, Planets Around Pulsars |
| Page: |
19 |
| Authors: |
Bailes, M.; Lyne, A. G.; Shemar, S. L. |
| Abstract: |
The Jodrell Bank timing database is used to verify the existence of a sinusoidal feature with a period of about 1,100 days in the pulse timing residuals of the pulsar PSR 0329+54, claimed by Demianski and Proszynski (1979). Data obtained indicate that there are no obvious signatures of planetary systems. The pulsar PSR 1828-11 contains a large amount of timing noise, and has postfit residuals that can be modelled quite successfully by two sinusoids, but only after the removal of a significant period second derivative. |
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