Solar wind plasma noise correlated between LISA and Taiji can bias stochastic gravitational wave background parameter estimates by up to 19% of Fisher uncertainty under large-scale correlation assumptions.
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Finite source number and finite observation time make PTA gravitational-wave-background Fourier coefficients non-Gaussian, with an analytically computed excess kurtosis and a Cauchy-distributed argument probe.
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Effects of Solar Wind Plasma Noise on Stochastic Gravitational Wave Background Searches with the LISA-Taiji Network
Solar wind plasma noise correlated between LISA and Taiji can bias stochastic gravitational wave background parameter estimates by up to 19% of Fisher uncertainty under large-scale correlation assumptions.
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Finite Populations & Finite Time: The Non-Gaussianity of a Gravitational Wave Background
Finite source number and finite observation time make PTA gravitational-wave-background Fourier coefficients non-Gaussian, with an analytically computed excess kurtosis and a Cauchy-distributed argument probe.