AV 80         This star is included in the CDF for SMC evolved stars in accord
AV 80          with the individual notes in Walborn et al.
AV 80          (2000PASP..112.1243W), who state that its absolute visual
AV 80          magnitude and the strength of its UV wind features correspond to
AV 80          a luminosity class of III.
AV 177        The CCF has a double-peaked appearance, however the velocity
AV 177         separation is not large enough for a double Gaussian fit. The
AV 177         Vsini value listed is of both peaks together.
AV 332        Known as a double-lined spectroscopic binary classified as
AV 332         WN3+O6.5I (Massey et al. 2000, Cat. J/AJ/119/2214). Only one peak
AV 332         is seen in the CCFs, probably that of the O6.5I component, which
AV 332         moves in Vr by 45km/s between the observations taken six months
AV 332         apart.
AV 476        Classified as O2-3V+companion by Massey et al.
AV 476         (2005ApJ...627..477M), we see two peaks, separated by Vr of
AV 476         363km/s.
NGC346-MPG324 The peak in the two observations moves by 110km/s and changes
NGC346-MPG324  width.
SK -65 21     There are four observations taken in sequence over 15hr. All CCFs
SK -65 21      show double peaks that appear to be near or at maximum velocity
SK -65 21      separation of 350km/s. The peaks first move slightly farther
SK -65 21      apart and then closer over the four observations.
SK -66 172    Classified as O2III(f*)+OB (Walborn et al. 2002ApJS..141..443W),
SK -66 172     we do not see any sign of a companion in the CCF.
SK -67 18     Koenigsberger et al. (2003RMxAA..39..213K) classified this system
SK -67 18      as O3+O8-B0I. We see both peaks in the CCF.
SK -67 166    Observed 63 times with FUSE over approximately a 5 week period,
SK -67 166     the peak does not move.
SK -68 52     A weak second peak is stronger in the CCF with AV327 than with
SK -68 52      SK -66 100. The peaks are separated by 350km/s.
SK -69 94     The FUSE spectrum of S Dor is contaminated by the visual companion
SK -69 94      13" away which is classified as a B1I (Wolf et al. 
SK -69 94      1980A&A....88...15W). The CCF here is almost certainly
SK -69 94      representative of this star, not S Dor.
SK -69 223    Classified WC4(+OB) by Bartzakos et al. (2001, 
SK -69 223     Cat. J/MNRAS/324/33), we do not see any sign of a second peak in
SK -69 223     the CCFs. However, the main peak does move slightly between the
SK -69 223     two available observations taken 50 minutes apart.
SK -70 91     Classified as O2III(f*)+OB by Walborn et al. 
SK -70 91      (2002ApJS..141..443W), both stars have peaks in CCF. The peaks
SK -70 91      are separated by 255km/s.
BI 173        In the two observations taken two months apart, the main peak
BI 173         moves by 53km/s. There is a low-level second peak, but it is
BI 173         difficult to distinguish it from the surrounding noise.
HV 2241       A known binary, we do not see any sign of the secondary,
HV 2241        classified as early B (Mokiem et al. 2006A&A...456.1131M), in
HV 2241        the CCF.
LMC X-4       This spectrum is of the O8III companion in this X-ray binary.
PGMW 3209     Only one extremely noisy observation is available from FUSE. We do
PGMW 3209      not see any sign of a second peak in the CCF.