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Table 3

Relative RV for spectra with significant nebular contamination but which estimates were possible from combining the spectra from each night (see Sect. 3.2).

VFTS MJD Relative radial velocities [km s-1]
He i He i He i He i
λ4388 λ4144 λ4026 λ4471
004∗ (S) 54 767 0.39 0.44 0.29 −1.42
004 54 827 −14.28 −15.10 −12.47 −71.61
004 54 828 −39.97 −59.7 −23.65 −14.02
004 54 860 −10.62 −3.45 17.85 0.37
004 54 886 −60.14 −40.36 −12.47 −23.02
004 55 114 53.58 −3.45 −58.75 −28.42
010 54 767 26.80 5.19 −14.43 6.94
010 54 827 9.20 −12.24 −26.21 −32.39
010∗ (S) 54 860 −0.28 0.44 −1.17 −0.34
010 54 886 −39.55 40.07 −8.54 ...
010 55 114 4.88 41.65 −17.38 ...
054∗ (S) 54 767 −0.28 −0.27 6.93 −0.28
054 54 827 20.03 −28.95 −15.16 −18.88
054 54 860 49.82 24.11 8.40 19.64
054 54 886 −21.94 −23.22 −60.82 −37.47
054 55 114 −21.94 31.28 −65.24 −33.49

Notes. Celestial coordinates and optical photometry for the VFTS stars are given in Table 5 of Paper I. Observations indicated by the ∗ qualifier to the first column were the template spectra for the RV estimates. The subsequent letters in parentheses indicate the binary status from this work: (B) = binary; (S) = single; (V) = RV variable; see Sect. 3.3 for further details. Values for the first three entries are shown; the full table is available at the CDS.

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