By injecting eccentric binary signals into simulated PTA data, the paper shows individual masses are recoverable at high frequencies, while low-frequency signals can be confused with the stochastic background and yield Bayes factors near unity.
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Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays
By injecting eccentric binary signals into simulated PTA data, the paper shows individual masses are recoverable at high frequencies, while low-frequency signals can be confused with the stochastic background and yield Bayes factors near unity.