Citing Articles For: Accurate pulsar timing array residual variances and correlation of the stochastic gravitational-wave background

Looking for non-Gaussianity in pulsar timing arrays through the four point correlator

Adrien Kuntz, Clemente Smarra, and Massimo Vaglio

Phys. Rev. D 114 084020 (2026)

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Finite populations and finite time: The non-Gaussianity of a gravitational wave background

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Implications of the Nanohertz Gravitational-wave Background for Galactic Feedback and Massive Black Hole Growth

Megan Taylor Tillman, Blakesley Burkhart, Chiara M. F. Mingarelli, J. Andrew Casey-Clyde, Lars Hernquist, Sownak Bose, Enikő Regős, and César Hernández-Aguayo

ApJL 1003 L50 (2026)

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Accurate pulsar timing array residual variances and correlation of the stochastic gravitational-wave background

Looking for non-Gaussianity in pulsar timing arrays through the four point correlator

Simulating a Gaussian stochastic gravitational wave background signal in pulsar timing arrays

Finite populations and finite time: The non-Gaussianity of a gravitational wave background

Implications of the Nanohertz Gravitational-wave Background for Galactic Feedback and Massive Black Hole Growth

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