\begin{table}%t3
  \caption{Properties of candidate \lya\ emission lines. Columns~2--4 list the offsets of the candidate in RA and Dec and in projected kpc at the \lya~emission redshifts (in Col.~5),
respectively. Column~6 lists the integrated \lya~flux in units of
$10^{-17}$~\ecs, and Col.~7 the velocity offset from the DLA~redshift. Column~8 lists the integrated signal-to-noise ratio of the \lya~emission line, and Col.~9 gives the line width of the
emission lines. Fluxes have not been corrected for Galactic extinction. Column~10 lists the significance class of the detections as described in Sect.~\ref{sect:hiz_notes}. "Conf.''
implies candidates that were confirmed previously \citep{moller98,djorgovski96}.}
  \label{tab:hiz_cand_prop}
%\centering
\small
  \begin{tabular}{llllllllll}
   \hline \hline
QSO  &  $\Delta$RA& $\Delta$Dec &  $b$ & $z$ &
   $f_{\lambda}$ &  $\Delta ~ v$  & {\it S/N}$_{\rm int}$ & \textit{FWHM}  & significance\\
     &  (\arcsec) &  (\arcsec) & (kpc) & & & (km s$^{-1}$) & & (km
s$^{-1}$) & class \\
(1)  & (2) & (3) & (4) & (5) & (6) & (7) & (8) & (9) & (10)\\
   \hline
Q0151+048A & 2.5:0.4 & --2.5:1.7 & 3.3:25.4 & 1.9363 & (150 $\pm$ 70) & +225 & 7  & 280 $\pm$ 220 & conf.\\
Q0953+4749 & --1.2 &  --0.2& 9.0 & 3.4041 & (6.6 $\pm$ 2.9)  & 0  & 15 &   290 $\pm$ 260 & 2 \\
           & --0.5 & 1.8  & 11.1 & 3.9029 & (4.9 $\pm$ 2.1)  & +730& 16&   570 $\pm$ 230 & 3\\
Q1347+112 & --2.0 & 1.5  & 20.2  & 2.4835 & (3.5 $\pm$ 1.9)  & +1080 & 8 &   190 $\pm$ 370 & 3\\
          & --4.1 & 0.4  & 34.3  & 2.0568 & (4.2 $\pm$ 3.0)   &
   +670  & 7 & 610 $\pm$ 210& 1 \\
Q1425+606 &  --4.1& 0.4  & 32.3  & 2.8280 & (8.5 $\pm$ 3.1) &
   +80 & 14 & 590 $\pm$ 220 & 3\\
Q1451+1223 & --3.0 & 3.8 & 39.2  & 2.4764 & (5.8 $\pm$ 2.6)   &
   +640  & 10 & 320 $\pm$ 260 & 3\\
           & --1.0 & 2.8 & 22.5  & 3.1739 & (3.1 $\pm$ 2.0) &
   +210  & 7 & $<$100 & 3\\
Q1759+7539 & --1.4 & 3.5  & 30.0 & 2.6377 & (5.8 $\pm$ 3.0)   &
   +1050 & 10 & 290 $\pm$ 220 & 2\\
         & 0.1     & --1.2& 9.4  & 2.9090 & (6.0 $\pm$ 2.9)  &
           --80 & 21 & 240 $\pm$ 260 & 1 \\
Q1802+5616 & --0.2 & --2.0  & 14.9 & 3.3820 & (3.5 $\pm$ 0.9) &
           --610 & 10 & 180 $\pm$ 90 & 4\\
           & 0.2  & 1.8 & 12.9 & 3.7652 & (4.6 $\pm$ 1.9) & +200 & 7 & $<$100 & 2 \\
Q2155+1358 & 0.7  &  1.2 & 10.2 & 3.3174 & (9.4 $\pm$ 3.0)  &
           +100  & 9 & 780 $\pm$ 210 & 3\\
& 1.7  &  1.9 & 19.4 & 3.1461 & (4.1 $\pm$ 2.4)  &
           +290  & 7 & 260 $\pm$ 220 & 3\\
Q2233+131 &  0.6  &  2.3 & 18.0 & 3.1543 & (9.6 $\pm$ 2.5)    &
           +90  & 9 & 230 $\pm$ 110 & conf.\\
   \hline
  \end{tabular}
\end{table}