Disentangled spectra of the broad-lined, Be star companion. The figure compares spectra disentangled using the shift-and-add method for assumed Be star radial-velocity semi-amplitudes of 5, 10, and 20 km/s shown in dark, medium and light grey, respectively. The cyan line shows the Be star spectrum obtained via the singular value decomposition (SVD) method of Seeburger et al. (2024). Unlike the shift-and-add method, this technique determines RVs as part of the disentangling process and does not require an input value of K_Be. The inferred RVs imply a semi-amplitude of approximately K_Be ≃ 5 km/s.