Notes. The first, second, and third columns list the identifier as well as coordinates. The column ‘F814W’ lists the F814 magnitude from (Milone et al. 2018). The column ‘SpT’ lists the derived spectral types. The column ‘lines’ indicates which spectral lines among He Iλλ 4713.15, 4921.93, 5015.68, 5047.74, 6678.15, 7065.19 Å were used to measure RVs (an ‘x’ indicates that the line was used, while ‘–’ indicates that it was not used). We then give an overview over the measured RVs and associated errors for each epoch. The next column indicates whether the star was flagged as binary (‘–’ indicates that no RV measurements were possible, ‘sin’ means no significant RV shifts were detected, ‘SB1’ means it was flagged as binary based on RV variability, ‘SB2’ indicates a composite SB2 spectrum). The last column lists possible comments. A full version of this table is available at the CDS. The first few lines are shown as an example.