Pulsar Timing Noise

Details Pulsar Timing Noise Pulsar Timing Noise

Dec 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006chjas...6b.169h&link_type=abstract

Chinese Journal of Astronomy and Astrophysics, Supplement, Volume 6, Issue S2, Proceedings of the 2005 Lake Hanas International

Astronomy and Astrophysics

Astrophysics

Pulsars: General

Scientific paper

Pulsar timing techniques allow a pulsar's rotational, astrometric and binary parameters to be measured to high precision. Any features that remain in the timing residuals after fitting for the expected pulsar parameters are suggestive of unmodelled physics such as binary companions, free precession or glitch events. In this paper we provide an overview of the features observed in the timing residuals that collectively are referred to as ``pulsar timing noise''. We use results obtained from the literature and from the Jodrell Bank observatory archive of timing residuals.

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