\begin{table}%t2
\caption{Redshifts for the first 10 galaxies$^{{\rm *}}$ in the
sample of 143 measured with 2dF in the cluster A3667 and falling in
the redshift range $0.044 \leq z \leq 0.068$.\label{tab:z}}
%\centerline
 {\begin{tabular}{ccccccccc}
\hline\hline
\noalign{\smallskip}
 {\rm ID} & {\rm RA }     & {\rm Dec}    & $m_{\rm B}$ &
$z_{\rm abs}$ & $z_{\rm em}$  &    $z_{\rm ave}$ & $z_{\rm lit}$& {\rm morphological} \\
&  {\rm (J2000)}&  {\rm (J2000)} & & & & & & {\rm type}\\
\hline
1  & 20~05~37.49  &  $-$56~41~06.1 & 16.89 & 0.0558 &	 &         & & 2\\
2  & 20~06~26.98  &  $-$56~19~50.9 & 18.16 & 0.0586 &	 &         & & 3\\
3  & 20~07~22.03  &  $-$56~39~44.0 & 16.41 & 0.0535 &	 &         & & 2\\
4  & 20~07~29.09  &  $-$57~28~46.2 & 18.09 & 0.0553 & 0.0553 & 0.0553  & & 5\\
5  & 20~07~30.08  &  $-$57~22~58.6 & 16.75 & 0.0521 & 0.0518 & 0.0520  & & 3\\
6  & 20~07~32.50  &  $-$56~34~45.9 & 17.43 & 0.0560 & 0.0557 & 0.0559  & & 4\\
7  & 20~07~56.06  &  $-$56~16~01.3 & 16.65 & 0.0543 & 0.0545 & 0.0544  & 0.0535 & 5\\
8  & 20~08~01.56  &  $-$56~06~07.6 & 17.60 & 0.0594 & 0.0594 & 0.0594  & & 3\\
9  & 20~08~09.17  &  $-$56~30~21.7 & 16.80 & 0.0523 &	 &         & 0.0524 & 2\\
10 & 20~08~27.61  &  $-$56~20~42.5 & 17.79 & 0.0572 & 0.0569 & 0.05705 & & 3\\
\noalign{\smallskip}
\hline
\end{tabular} }
\par
\smallskip
$^{{\rm *}}$
The full data table contains 143 objects and is available in electronic
form at CDS via anonymous ftp to {\tt cdsarc.u-strasbg.fr (130.79.128.5)}
or via {\tt http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/479/1}. Column~1
gives the source ID number; Cols.~2 and~3 are the Right Ascension and 
Declination in J2000 coordinates; Col.~4 is the blue magnitude; Cols.~6 
and~7 are the redshifts as determined by absorption and emission features,
respectively, and Col.~8 is the average redshift for cases where a redshift
could be determined by both emission and absoprtion features; Col.~9 is
the previously published redshift and Col.~10 is the morphological type 
determined by the best correlation to the spectral templates used by
2dfdr, numbers correspond to those listed in \cite{colless01}.
\end{table}