LISA's response to the kinematic dipole in the GWB is governed by one symmetry-fixed frequency-dependent function, with Fisher forecasts showing detectability for h²Ω_GW above 5×10^{-8} (fiducial) or 5×10^{-10} (improved noise) for scale-invariant signals.
The NANOGrav 15 yr Data Set: Search for Anisotropy in the Gravitational-wave 28 Background.Astrophys
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Probing the Kinematic Dipole with LISA: an analytical treatment
LISA's response to the kinematic dipole in the GWB is governed by one symmetry-fixed frequency-dependent function, with Fisher forecasts showing detectability for h²Ω_GW above 5×10^{-8} (fiducial) or 5×10^{-10} (improved noise) for scale-invariant signals.