Finite populations of inspiralling supermassive black hole binaries plus finite observation windows introduce non-Gaussian statistics in the pulsar timing array signal that are absent from the Gaussian approximation used in current analyses.
Manchester, The international pulsar timing array, Classical and Quantum Gravity30, 224010 (2013)
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Finite Populations & Finite Time: The Non-Gaussianity of a Gravitational Wave Background
Finite populations of inspiralling supermassive black hole binaries plus finite observation windows introduce non-Gaussian statistics in the pulsar timing array signal that are absent from the Gaussian approximation used in current analyses.