Notes. Relevant properties of the target systems studied in this work, including the primary’s effective temperature T_pAGB, metallicity [Fe/H] and refractory depletion strength. In addition, we list the binary period P and eccentricity e, the Gaia DR3 luminosity L_Gaia, and the inclination i_par and primary star radius R_1, par found from previous parametric modelling. Below that, the number of selected observed spectra N_obs, and their average signal-to-noise ratio (S/N)_avg, as well as the references used. T_pAGB and [Fe/H] values (formal errors of 250 K and 0.3 dex, respectively) were based on (1) Waelkens et al. (1991), (2) Rao & Giridhar (2014), (3) Gorlova et al. (2012), (4) Giridhar et al. (2000) and (5) Giridhar et al. (2005). The refractory depletion strength classification, as well as P and e were taken from (6) Oomen et al. (2018). L_Gaia was derived from (7) Gaia Collaboration (2023), i_par and R_1, par from (8) Bollen et al. (2020), (9) Bollen et al. (2021) and (10) Bollen et al. (2022). We note that the luminosities are not fully reliable, as none of these systems were flagged as astrometric binaries in Gaia DR3.