Red noise and evolving signals: a complete frequentist approach to supermassive black hole binary searches with pulsar timing arrays
gr-qc, astro-ph.CO, astro-ph.HE, astro-ph.IM
Submitted: 2026-06-05
Updated: 2026-09-23
Code: https://github.com/mfalxa/fakepta
Terminology
Sources
- Extending the frequency reach of pulsar timing array based gravitational wave search without high cadence observations
- Detection and parameter estimation of supermassive black hole ringdown signals using a pulsar timing array
- Pulsar Timing Array Observations of Massive Black Hole Binaries
- Pulsar Timing Array Based Search for Supermassive Black Hole Binaries in the Square Kilometer Array Era
- Hierarchical search method for gravitational waves from stellar-mass binary black holes in noisy space-based detector data
Related papers
- Tests of General Relativity with Einstein Telescope
- Unitary quantum matter-bounce in a universe with a positive cosmological constant
- Quasi-pole quintessential inflation in metric-affine gravity
- Dynamical tidal response of neutron stars: From effective field theory to gravitational waveforms
- Limits of the Rastall--Einstein Equivalence: Matter-Action Compatibility, FLRW Dynamics, and Exceptional Sectors
- Boson star-black hole binaries: initial data and head-on collisions