Adding a prior linking GW frequency f to its derivative ḏ from detached white dwarf mass limits to the GBSIEVER iterative pipeline raises resolved DWD sources by ~7.3% for LISA and ~14.6% for the LISA-Taiji network on simulated data.
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Improving the resolution of double white dwarf systems with spaceborne gravitational wave observatories using a robust astrophysical prior
Adding a prior linking GW frequency f to its derivative ḏ from detached white dwarf mass limits to the GBSIEVER iterative pipeline raises resolved DWD sources by ~7.3% for LISA and ~14.6% for the LISA-Taiji network on simulated data.