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[ascl:2410.018] fastPTA: Constraining power of PTA configurations forecaster

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.

Code site:
https://github.com/mauropieroni/fastpta
Used in:
https://ui.adsabs.harvard.edu/abs/2024PhRvD.110f3022B
Described in:
https://ui.adsabs.harvard.edu/abs/2024arXiv240714460D
Bibcode:
2024ascl.soft10018D

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ascl:2410.018
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