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.
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The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals
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.