Including the metal-richer, triaxial GSE halo alters chirp-mass and distance distributions of LISA-resolved DWDs while leaving the DWD gravitational-wave foreground strength unchanged.
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LISA's view of the Galactic Halo: forecasts for the Galactic double white dwarf population using Gaia data
Including the metal-richer, triaxial GSE halo alters chirp-mass and distance distributions of LISA-resolved DWDs while leaving the DWD gravitational-wave foreground strength unchanged.