Show simple item record

dc.contributor.authorKeith, M.J.
dc.contributor.authorColes, W.
dc.contributor.authorShannon, R.M.
dc.contributor.authorHobbs, G.B.
dc.contributor.authorManchester, R.N.
dc.contributor.authorBailes, M.
dc.contributor.authorBhat, Ramesh
dc.contributor.authorBurke-Spolaor, S.
dc.contributor.authorChampion, D.J.
dc.contributor.authorChaudhary, A.
dc.contributor.authorHotan, A.W.
dc.contributor.authorKhoo, J.
dc.contributor.authorKocz, J.
dc.contributor.authorOstowski, S.
dc.contributor.authorRavi, V.
dc.contributor.authorReynolds, J.E.
dc.contributor.authorSarkissian, J.
dc.contributor.authorvan Straten, W.
dc.contributor.authorYardley, D.R.B.
dc.identifier.citationKeith, M.J. and Coles, W. and Shannon, R.M. and Hobbs, G.B. and Manchester, R.N. and Bailes, M. and Bhat, N.D.R. et al. 2013. Measurement and correction of variations in interstellar dispersion in high-precision pulsar timing. Monthly Notices of the Royal Astronomical Society. 429 (3): pp. 2161-2174.

Signals from radio pulsars show a wavelength-dependent delay due to dispersion in the interstellar plasma. At a typical observing wavelength, this delay can vary by tens of microseconds on 5-yr time-scales, far in excess of signals of interest to pulsar timing arrays, such as that induced by a gravitational wave background. Measurement of these delay variations is not only crucial for the detection of such signals, but also provides an unparalleled measurement of the turbulent interstellar plasma at astronomical unit (au) scales. In this paper we demonstrate that without consideration of wavelength-independent red noise, ‘simple’ algorithms to correct for interstellar dispersion can attenuate signals of interest to pulsar timing arrays. We present a robust method for this correction, which we validate through simulations, and apply it to observations from the Parkes Pulsar Timing Array. Correction for dispersion variations comes at a cost of increased band-limited white noise. We discuss scheduling to minimize this additional noise, and factors, such as scintillation, that can exacerbate the problem. Comparison with scintillation measurements confirms previous results that the spectral exponent of electron density variations in the interstellar medium often appears steeper than expected. We also find a discrete change in dispersion measure of PSR J1603−7202 of ∼2 × 10−3 cm−3 pc for about 250 d. We speculate that this has a similar origin to the ‘extreme scattering events’ seen in other sources. In addition, we find that four pulsars show a wavelength-dependent annual variation, indicating a persistent gradient of electron density on an au spatial scale, which has not been reported previously.

dc.publisherOxford University Press
dc.subjectISM: structure
dc.subjectpulsars: general
dc.subjectmethods: data analysis
dc.titleMeasurement and correction of variations in interstellar dispersion in high-precision pulsar timing
dc.typeJournal Article
dcterms.source.titleMonthly Notices of the Royal Astronomical Society

This article has been published in Monthly Notices of the Royal Astronomical Society. © 2013 The Authors. Published by Oxford University Press on behalf of Royal Astronomical Society. All rights reserved.

curtin.accessStatusOpen access

Files in this item


This item appears in the following Collection(s)

Show simple item record