Parameter Estimation for Eccentric Supermassive Black Hole Binaries with Pulsar Timing Arrays
Sara Manzini, Stanislav Babak
astro-ph.HE
Submitted: 2026-08-07
Updated: 2026-08-10
Code: https://github.com/nanograv/discovery
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- The second data release from the European Pulsar Timing Array III. Search for gravitational wave signals
- The NANOGrav 15-year Data Set: Evidence for a Gravitational-Wave Background
- Search for an isotropic gravitational-wave background with the Parkes Pulsar Timing Array
- The International Pulsar Timing Array: First Data Release
- Massive BH Binaries as Periodically-Variable AGN
- Expected properties of the first gravitational wave signal detected with pulsar timing arrays
- Resolving the nano-Hz gravitational wave sky: the detectability of eccentric binaries with PTA experiments
- Lighting up the nano-hertz gravitational wave sky: opportunities and challenges of multimessenger astronomy with PTA experiments
- Effective-one-body modelling of eccentric supermassive black hole binaries for Pulsar Timing Array
- Rapid parameter estimation for pulsar-timing-array datasets with variational inference and normalizing flows
- Understanding and analysing time-correlated stochastic signals in pulsar timing
- Noise analysis in the European Pulsar Timing Array data release 2 and its implications on the gravitational-wave background search
- From Spin Noise to Systematics: Stochastic Processes in the First International Pulsar Timing Array Data Release
- Hyper-efficient model-independent Bayesian method for the analysis of pulsar timing data
- New advances in the Gaussian-process approach to pulsar-timing data analysis
- Beyond diagonal approximations: improved covariance modeling for pulsar timing array data analysis
- Prototype Global Analysis of LISA Data with Multiple Source Types
- Eryn : A multi-purpose sampler for Bayesian inference
- Bayesian model selection without evidences: application to the dark energy equation-of-state
- Common-red-signal analysis with 24-yr high-precision timing of the European Pulsar Timing Array: Inferences in the stochastic gravitational-wave background search
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