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    Optimal interpolation and prediction in pulsar timing

    Access Status
    Open access via publisher
    Authors
    Deng, X.
    Coles, W.
    Hobbs, G.
    Keith, M.
    Manchester, R.
    Shannon, Ryan
    Zheng, J.
    Date
    2012
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Deng, 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.
    Source Title
    Monthly Notices of the Royal Astronomical Society
    DOI
    10.1111/j.1365-2966.2012.21189.x
    ISSN
    0035-8711
    School
    Curtin Institute of Radio Astronomy (Physics)
    URI
    http://hdl.handle.net/20.500.11937/39340
    Collection
    • Curtin Research Publications
    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.

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