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dc.contributor.authorDeng, X.
dc.contributor.authorColes, W.
dc.contributor.authorHobbs, G.
dc.contributor.authorKeith, M.
dc.contributor.authorManchester, R.
dc.contributor.authorShannon, Ryan
dc.contributor.authorZheng, J.
dc.date.accessioned2017-01-30T14:32:53Z
dc.date.available2017-01-30T14:32:53Z
dc.date.created2016-01-11T20:00:25Z
dc.date.issued2012
dc.identifier.citationDeng, X. and Coles, W. and Hobbs, G. and Keith, M. and Manchester, R. and Shannon, R. and Zheng, J. 2012. Optimal interpolation and prediction in pulsar timing. Monthly Notices of the Royal Astronomical Society. 424 (1): pp. 244-251.
dc.identifier.urihttp://hdl.handle.net/20.500.11937/39340
dc.identifier.doi10.1111/j.1365-2966.2012.21189.x
dc.description.abstract

For pulsar projects it is often necessary to predict the pulse phase in advance, for example when preparing for new observations. Interpolation of the pulse phase between existing measurements is also often required, for example when folding X-ray or gamma-ray observations according to the radio pulse phase. Until now these procedures have been done using various ad hoc methods. The purpose of this paper is to show how to interpolate or predict the pulse phase optimally using statistical models of the various noise processes and the phase measurement uncertainty.

dc.titleOptimal interpolation and prediction in pulsar timing
dc.typeJournal Article
dcterms.source.volume424
dcterms.source.number1
dcterms.source.startPage244
dcterms.source.endPage251
dcterms.source.issn0035-8711
dcterms.source.titleMonthly Notices of the Royal Astronomical Society
curtin.departmentCurtin Institute of Radio Astronomy (Physics)
curtin.accessStatusOpen access via publisher


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