\begin{table}%t11
\par
\caption{\label{mrvi}Catalogue of mean radial and rotational velocities.}
%\centerline
 {\begin{tabular}{lrlrrrrrrrrrrrl}
\noalign{\smallskip}\hline\hline\noalign{\smallskip}
Cluster & \multicolumn{1}{c}{No.} & \multicolumn{1}{c}{ID} & \multicolumn{1}{c}{RA(J2000)} & \multicolumn{1}{c}{Dec(J2000)} & \multicolumn{1}{c}{$\bar{RV}$} & \multicolumn{1}{c}{$\epsilon$} & \multicolumn{1}{c}{$\sigma$} & \multicolumn{1}{c}{$E/I$} & 
$N$ & $V$ sin~$i$ & Error & \multicolumn{1}{c}{$\Delta T$} & $P(\chi^2)$ & Notes\\
\noalign{\smallskip}\hline\noalign{\smallskip}
Blanco 1 & 0008 & SA140 66 & 23 59 26.73 & --28 51 13.9 & 4.74 & 0.25 & 0.48 & 0.80 & 6 & 14.9 & 0.7 & 4737 & 0.675 & NM \\
Blanco 1 & 0015 & ZS 3     &  0 00 11.33 & --29 50 42.5 & --8.32 & 1.66 & 3.71 & 7.65 & 5 &  4.1 & 1.5 &  350 & 0.000 & NM, SB \\
Blanco 1 & 0016 & ZS 9     &  0 00 12.04 & --30 20 50.4 & --6.08 & 0.20 & 0.20 & 0.47 & 5 &  6.0 & 1.0 & 3989 & 0.930 & NM \\
Blanco 1 & 0018 & SA140 91 &  0 00 35.38 & --29 15 48.3 & 11.42 & 0.56 & 0.56 &      & 1 &  6.2 & 2.9 &      &       & NM \\
Blanco 1 & 0019 & W 19     &  0 00 45.02 & --29 06 30.2 &  6.31 & 0.36 & 0.81 & 1.88 & 5 &  0.0 & 0.0 & 3971 & 0.008 & SB2? \\
Blanco 1 & 0020 & SA140 97 &  0 00 46.60 & --29 08 05.6 &  6.63 & 0.16 & 0.34 & 0.85 & 6 &  4.8 & 0.9 & 3985 & 0.613 & \\
\hline
\end{tabular}}
\par
 \smallskip
{Note:} the columns contain the cluster name, the star identification according to the 
numbering system used in WEBDA, the original identification (ID), the mean radial velocity ($\bar{RV}$), the uncertainty on the mean
($\epsilon$), the formal standard deviation, ($\sigma$), of radial velocities, all three in km~s$^{-1}$, the 
external  to internal error ratio, $E/I  =  \sigma$/$\epsilon$, the number of observations used in the 
computation of the mean velocity ($N$), the rotational velocity ($V \sin i$) and its error, the time span in [days] covered by observations, 
($\Delta T$), the probability that the scatter is due to random noise ($P(\chi^2)$), and notes on membership (NM for non members), 
binarity (SB1: spectroscopic binary, SB1O: binary with an orbit, SB2 and SB2O: double-lined binary. 
The full table is available in electronic form at the CDS.
\end{table}