Bayesian characterization of circumbinary sub-stellar objects with <i>LISA</i>
Bayesian characterization of circumbinary sub-stellar objects with <i>LISA</i>
The Laser Interferometer Space Antenna (LISA) will detect and characterize $\sim10^4$ Galactic Binaries consisting predominantly of two White Dwarfs (WD). An interesting prospect within this population is a third object--another WD star, a Circumbinary Exoplanet (CBP), or a Brown Dwarf (BD)--in orbit about the inner WD pair. We present the …