The stars in Table D.2 are a mix of rejected spectra because of various problems and also those objects that were identified as υ_los non-members by the VLT/FLAMES spectroscopy and confirmed by DR3 astrometry and removed from further analysis. The membership likelihood (mem) is given as M (member), NM (non-member), LM (likely member) and sometimes M and LM have a p after, which suggests that the star maybe (or is) a member but it is peculiar (a C-star or a double star, for example). The velocities in this table can be reliable if the stars are members, but are advised to be used with caution, if at all. They are not used in this paper. Some stars have other better FLAMES spectra as part of this survey and are thus listed in Table. D.1 with those values (which may differ from what is here).