arXiv (All)
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Red noise and evolving signals: a complete frequentist approach to supermassive black hole binary searches with pulsar timing arrays
cosmology-and-nongalactic-astrophysicsgeneral-relativity-and-quantum-cosmologyhigh-energy-astrophysical-phenomena
Searches for gravitational waves (GWs) from isolated supermassive black hole binaries (SMBHBs) in pulsar timing array (PTA) data require simultaneous estimation of signal and noise parameters, so the dimensionality of the fit scales with the number of observed pulsars. This computational difficulty
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