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Ensemble Pulsar Time Study by Pulsar Timing Observations

Published online by Cambridge University Press:  19 July 2016

Tinggao Yang  and
Guangren Ni
Tinggao Yang
Affiliation:
National Time Service Center, Chinese Academy of Sciences, P. O. Box 18, Lintong, Shaanxi, China
Guangren Ni
Affiliation:
National Time Service Center, Chinese Academy of Sciences, P. O. Box 18, Lintong, Shaanxi, China

Abstract

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Long term timing of multiple millisecond pulsars can contribute to the study of an ensemble pulsar time scale PTens. A wavelet decomposition algorithm (WDA) was applied to define a PTens using the available millisecond pulsar timing datA. The PTens obtained from WDA is more stable than those resulting from other algorithms. The Chinese 50 m radio telescope is specially designed for PTens study and detection of gravitational wave background via millisecond pulsars timing observations. A scheme for multiple millisecond pulsar timing and ensemble pulsar time study is discussed in some detail.

Type
Part 10: Radio Pulsar Timing
Information
Symposium - International Astronomical Union , Volume 218: Young Neutrons Stars and their Environments , 2004 , pp. 439 - 440
Copyright
Copyright © Astronomical Society of the Pacific 2004 

References

Foster, R. S., & Backer, D. C. 1990, ApJ, 361, 300.CrossRefGoogle Scholar
Kaspi, V. M., Taylor, J. H., & Ryba, M. F. 1994, ApJ, 428, 713.Google Scholar
Petit, G., & Tavella, P. 1996, A&A, 308, 290.Google Scholar