Non-Gaussian timing residual skewness in pulsar timing arrays
gr-qc, astro-ph.CO
Submitted: 2026-10-02
Updated: 2026-10-02
Terminology
Sources
- 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 second data release from the European Pulsar Timing Array III. Search for gravitational wave signals
- Searching for the nano-Hertz stochastic gravitational wave background with the Chinese Pulsar Timing Array Data Release I
- Comparing recent PTA results on the nanohertz stochastic gravitational wave background
- The MeerKAT Pulsar Timing Array: The first search for gravitational waves with the MeerKAT radio telescope
- Status Report on Global Pulsar-Timing-Array Efforts to Detect Gravitational Waves
- GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo During the Second Part of the Third Observing Run
- Tests of General Relativity with GWTC-3
- The Science of the Einstein Telescope
- New Horizons for Fundamental Physics with LISA
- Progress of the TianQin project
- Low-frequency gravitational radiation from coalescing massive black hole binaries in hierarchical cosmologies
- The stochastic gravitational-wave background from massive black hole binary systems: implications for observations with Pulsar Timing Arrays
- The Distribution of Coalescing Compact Binaries in the Local Universe: Prospects for Gravitational-Wave Observations
- Massive Black Hole Binary Mergers in Dynamical Galactic Environments
- The Gravitational Wave Background from Massive Black Hole Binaries in Illustris: spectral features and time to detection with pulsar timing arrays
- The Astrophysics of Nanohertz Gravitational Waves
- Exploring realistic nanohertz gravitational-wave backgrounds
- Signals of merging supermassive primordial black holes in pulsar timing arrays
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