\begin{table}%t4
\caption{Lines from Systems E--K detected in the Keck spectrum.
\label{tab:sysek}}
%\centerline
 {\begin{tabular}{lcccc}
\hline\hline
No.Line ID & \zabs & $b$ & $\log N$ & M05 ID \\
   & & (\kms) & (\cmsq) &\\
\hline
\multicolumn{5}{c}{System E $\zabs = 1.89$} \\
1.\HI  & (a) &&&\\
1.\CIV  & 1.88805\err0.00001 & 10.00 (fixed) & 13.873\err0.032 & 1; \CIV\\
1.\SiIV\ \sh& 1.88805\err0.00001 & 6.50 (fixed) & 13.036\err0.064 &	\\
\hline
2.\HI  & (a) &&&\\
2.\CIV  & 1.88851\err0.00007 & 10.00 (fixed) & 13.576\err0.034 & 2; \CIV\\
2.\SiIV\ \sh & (a) & & & \\
\hline 
\multicolumn{5}{c}{System J (new system) $\zabs = 1.93$} \\
1.\HI   & (a) &&&\\
2.\CIV\ $\ddag$& 1.92658\err0.00001 & 10.00 (fixed) & 13.727\err0.081 &	\\
\hline
\multicolumn{5}{c}{System F $\zabs = 1.97$} \\
1.\HI  & (a) &&&\\
1.\CIV & 1.96399\err0.00002 & 10.00 (fixed) & 13.699\err0.213 & 1; \CIV\\
\hline
2.\HI  & (a) &&&\\
2.\CIV & 1.96420\err0.00002 & 10.00 (fixed) & 14.185\err0.179 & 2, 3; \CIV\\
\hline
3.\HI  & (a) &&&\\
3.\CIV & 1.96519\err0.00001 & 10.00 (fixed) & 14.241\err0.030 & 4, 5; \CIV\\
\hline
4.\HI  & (a) &&&\\
4.\CIV & 1.96572\err0.00001 & 10.00 (fixed) & 13.574\err0.026 & 6; \CIV\\
\hline
\multicolumn{5}{c}{System G $\zabs = 2.07$} \\
1.\HI  & (a) &&&\\
1.\CIV  & 2.07061\err0.00005 & 10.00 (fixed) & 14.385\err0.576 & 1; \CIV\\
1.\SiIV\ \sh& 2.07061\err0.00005 & 6.50 (fixed) & 12.887\err0.307 & 1; \SiIV\\
\hline
2.\HI  & (a) &&&\\
2.\CIV  & 2.07091\err0.00005 & 10.00 (fixed) & 14.487\err0.575 & 2; \CIV\\
2.\SiIV\ \sh& 2.07091\err0.00005 & 6.50 (fixed) & 13.491\err0.188 & 2; \SiIV\\
\hline 
\multicolumn{5}{c}{System I $\zabs = 2.18$} \\
1.\HI     & (a) & & &    \\
1.\CIV    & 2.17560\err0.00002 & 10.00 (fixed) & 13.295\err0.036 & \\
1.\SiIV   & 2.17560\err0.00002 &  6.50 (fixed) & 12.359\err0.069 & \\
\hline
2.\HI     & (a) & & &    \\
2.\CIV    & 2.17606\err0.00005 & 10.00 (fixed) & 13.066\err0.056 & \\
2.\SiIV   & 2.17606\err0.00005 &  6.50 (fixed) & 12.107\err0.123 & \\
\hline
3.\HI     & (a) & & &    \\
3.\CIV    & 2.17645\err0.00001 & 10.00 (fixed) & 13.741\err0.033 & \\
3.\SiIV   & 2.17645\err0.00001 &  6.50 (fixed) & 12.750\err0.040 & \\
\hline
\multicolumn{5}{c}{System K (new system) $\zabs = 2.26$} \\
1.\HI\ \P & 2.26214\err0.00005 & 25.00 (fixed) & 14.850\err0.615 &	\\
1.\CIV & 2.26214\err0.00005 & 10.00 (fixed) & 12.827\err0.332 & 	\\
\hline
\multicolumn{5}{c}{System H $\zabs = 2.27$} \\
1.\HI\ \P & 2.26613\err0.00002 & 25.00 (fixed) & 14.075\err0.570 &	\\
1.\CIV & 2.26613\err0.00002 & 10.00 (fixed) & 13.200\err0.035 & 1; \CIV\\
1.\SiIV & 2.26613\err0.00002 & 6.50 (fixed) & 12.527\err0.053 &	\\
1.\SiIII\ \sh& 2.26613\err0.00002 & 6.50 (fixed) & 12.784\err0.085 & 1; \SiIII\\
\hline
\end{tabular}}
\par
\smallskip
$\sharp$ -- Heavy-element line in \Lya\ forest region of the spectrum;   
$\ddag$ -- line blended with identified line (\CIV\ in System J
is blended with \OI\ from System B);  
\P\ -- saturated line;  
(a) -- \HI\ lines are not observable in Systems E, J, F, I and G, in
either MMT or Keck spectra. \HI\ lines in System~I and 2.\SiIV\ lines in System~E
are seen in the MMT spectrum.
\end{table}