fastPTA forecasts the sensitivity of future Pulsar Timing Array (PTA) configurations and assesses constraints on Stochastic Gravitational Wave Background (SGWB) parameters. The code can generate mock PTA catalogs with noise levels compatible with current and future PTA experiments. These catalogs can then be used to perform Fisher forecasts of MCMC simulations.
https://ui.adsabs.harvard.edu/abs/2024PhRvD.110f3022B , https://ui.adsabs.harvard.edu/abs/2024arXiv240714460D