A Gibbs sampling technique marginalizes over photon-to-Gaussian assignments to fit timing and noise models to discrete gamma-ray arrival times while accounting for pulse-profile uncertainty.
A., Vallisneri, M., Taylor, S
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EPTA second data release reports Bayes factor of 60 for an isotropic nanohertz GWB in the 10.3-year subset, with amplitude (2.5±0.7)×10^{-15} at 1 yr^{-1} when spectral index is fixed at 13/3.
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Timing Gamma-ray Pulsars using Gibbs Sampling
A Gibbs sampling technique marginalizes over photon-to-Gaussian assignments to fit timing and noise models to discrete gamma-ray arrival times while accounting for pulse-profile uncertainty.