A new time-domain method using the annual modulation of the unresolved and resolved double white dwarf gravitational wave foreground constrains the Galactic thin disk scale height and length and bulge scale radius to 10-40% accuracy in mock LISA/Taiji observations.
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Constraining the Galactic Structure using Time Domain Gravitational Wave Signal from Double White Dwarfs Detected by Space Gravitational Wave Detectors
A new time-domain method using the annual modulation of the unresolved and resolved double white dwarf gravitational wave foreground constrains the Galactic thin disk scale height and length and bulge scale radius to 10-40% accuracy in mock LISA/Taiji observations.