Hostname: page-component-6bf8c574d5-vmclg Total loading time: 0 Render date: 2025-02-17T17:03:59.337Z Has data issue: false hasContentIssue false
  • English
  • Français

Pulsar timing array

Published online by Cambridge University Press:  21 October 2010

Alexander E. Rodin
Alexander E. Rodin*
Affiliation:
Pushchino Radio Astronomy Observatory of the Lebedev Physical Institute, Pushchino, Moscow region, 142290, Russia email: [email protected]
Rights & Permissions [Opens in a new window]

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Simultaneous timing of several pulsars distributed over the sky, so called Pulsar Timing Array (PTA), is used for a variety of metrological and astronomical applications. Three examples of PTA application are presented: link between celestial reference frames, ensemble pulsar time scale and detection of gravitational waves.

Keywords

pulsar timingreference systemstimegravitational waves
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 5 , Highlights H15: Highlights of Astronomy , November 2009 , pp. 229 - 230
Copyright
Copyright © International Astronomical Union 2010

References

Golyandina, N., Nekrutkin, V., & Zhigljavsky, A., Analysis of Time Series Structure SSA and Related Techniques. CHAPMAN & HALL/CRC, 2001CrossRefGoogle Scholar
Jenet, F., Hobbs, G., Lee, K. J., & Manchester, R. N., 2005, ApJ, 625L, 123CrossRefGoogle Scholar
Rodin, A. E. & Sekido, M. 2002, in Ros, E., Porcas, R. W., Lobanov, A. P., & Zensus, J. A. (eds.), Proc. 6th European VLBI Network Symposium (Bonn, Germany), p. 247Google Scholar
Rodin, A. E., 2008, MNRAS, 387, 1583–1588CrossRefGoogle Scholar