\begin{table}%t3
%  %%\centering
\par
 \caption{Lines detected above 5$\sigma$ in the low- (lr) and high-resolution (hr) spectra. \label{tab:lines}}
 %%\centerline
\par
 { \begin{tabular}{ccccrc}
    \hline\hline
    \rm $\lambda$(lr)  &
     ${\it EW}_{\rm rest}$(lr) &
    $\lambda$(hr) &
    ${\it EW}_{\rm rest}$(hr) &
    ID$^{{b,c}}$ &
    $z$ \\
    \hline
 4484 &   9 (1)$^{{a}}$ & &                 &            \lyb~$\lambda$1025.7  & 3.3715\\
 5317 &               & 5316.9  &                 &       \lya~em.~$\lambda$1215.6  & 3.3736\\
      &               & 5415.8  & 0.31 (3)      &         \ion{N}{v}~$\lambda$1238.8  & 3.3717\\
      &               & 5433.5  & 0.20 (2)      &         \ion{N}{v}~$\lambda$1242.8  & 3.3720\\
      &               & 5465.4  & 0.15 (2)      & 	               &	   \\
      &               & 5467.4  & 0.21 (3)      &        \ion{S}{ii}~$\lambda$1250.5  & 3.3719\\ 
 5483 & 0.44 (6)      & 5481.1  & 0.29 (2)      &        \ion{S}{ii}~$\lambda$1253.8  & 3.3716\\
 5511 & 1.07 (5)      & 5505.0  & 0.33 (2)      &        \ion{S}{ii}~$\lambda$1259.5  & 3.3707\\
      &               & 5509.7  & 1.00 (2)      &       \ion{Si}{ii}~$\lambda$1260.4  & 3.3713\\
      &               &         &                 &\  or~ \ion{Fe}{ii}~$\lambda$1260.5  & 3.3709\\
 5530 & 0.76 (5)      & 5529.2  & 0.75 (2)      &   \ion{Si}{ii}{*}~$\lambda$1264.7  & 3.3718\\
      &               & 5591.5  & 0.11 (2)      &$\oplus$, \rm \ion{C}{i}~$\lambda$1280.1? & 3.3679\\
      &               & 5595.7  & 0.10 (2)      &                             &       \\   
      &               & 5624.4  & 0.11 (2)      &                             &       \\  
 5637 & 0.33 (5)      & 5634.7  & 0.16 (2)      &                             &       \\  
      &               & 5649.2  & 0.16 (1)      &                             &       \\
      &               & 5652.0  & 0.15 (1)      &      \ion{Fe}{ii}~$\lambda$2344.2? & 1.4110\\
 5692 & 0.75 (6)      & 5692.5  & 0.69 (2)      &         \ion{O}{i}~$\lambda$1302.1  & 3.3716\\
 5706 & 1.08 (6)      & 5702.4  & 0.70 (2)      &       \ion{Si}{ii}~$\lambda$1304.3  & 3.3718\\
      &               &         &               & and~\ion{O}{i}{*}~$\lambda$1304.8?& 3.3702\\
 5706 & 1.08 (6)      & 5709.7  & 0.32 (2)      &    \ion{O}{i}{**}~$\lambda$1306.0? & 3.3718\\
 5727 & 0.26 (5)      & 5723.9  & 0.29 (2)      &   \ion{Si}{ii}{*}~$\lambda$1309.2  & 3.3718\\
 5838 & 1.71 (7)      & 5833.7  & 0.84 (3)      &        \ion{C}{ii}~$\lambda$1334.5  & 3.3713\\
      &               & 5838.9  & 0.79 (2)      &    \ion{C}{ii}{*}~$\lambda$1335.7  & 3.3714\\
 6095 & 1.19 (6)      & 6092.9  & 1.08 (4)      &       \ion{Si}{iv}~$\lambda$1393.7  & 3.3716\\
 6135 & 0.98 (6)      & 6132.4  & 1.15 (4)      &       \ion{Si}{iv}~$\lambda$1402.7  & 3.3716\\
 6280 & 0.51 (3)      & 6278.0  & 0.42 (3)      &$\oplus$, \rm \ion{Fe}{ii}$\lambda$2600.1? & 1.4145\\
      &               & 6629.2  & 0.14 (2)      &                             &       \\
 6676 & 0.69 (4)      & 6673.8  & 0.75 (3)      &        \ion{Si}{ii}~$\lambda$1526.7  & 3.3714\\
 6706 & 0.54 (4)      & 6703.7  & 0.34 (3)      &    \ion{Si}{ii}{*}~$\lambda$1533.4  & 3.3717\\
      &               & 6743.0  & 0.14 (2)      &       \ion{Mg}{ii}~$\lambda$2796.3? & 1.4114\\
      &               & 6754.2  & 0.13 (2)      &       \ion{Mg}{ii}~$\lambda$2803.5? & 1.4092\\
      &               & 6760.6  & 0.14 (3)      & 	                &	    \\
 6770 & 1.42 (4)      & 6766.9  & 0.99 (3)      &         \ion{C}{iv}~$\lambda$1548.2  & 3.3708\\
      &               & 6769.9  & 0.51 (3)      &         \ion{C}{iv}~$\lambda$1548.2  & 3.3728\\
 6782 & 1.28 (4)      & 6778.2  & 0.84 (3)      &         \ion{C}{iv}~$\lambda$1550.7  & 3.3708\\
      &               & 6781.0  & 0.53 (3)      &         \ion{C}{iv}~$\lambda$1550.7  & 3.3727\\
 6875 &               & 6870.4  &                 &$\oplus$                    &       \\
      &               & 6876.5  &                 &$\oplus$                    &       \\
 6900 &               & 6891.9  &                 &$\oplus$                    &       \\
      &               & 6902.4  &                 &$\oplus$                    &       \\
 7034 & 0.51 (4)      & 7031.7  & 0.48 (3)      &       \ion{Fe}{ii}~$\lambda$1608.4  & 3.3717\\
      &               & 7043.6  & 0.17 (3)      &       \ion{Fe}{ii}~$\lambda$1611.2  & 3.3716\\
      &               & 7082.0  & 0.15 (3)      & 	               &	   \\
      &               & 7160.1  & 0.20 (3)      &                             &       \\
      &               & 7202.7  & 0.17 (3)      &$\oplus$                    &       \\
 7307 & 1.08 (5)      & 7303.5  & 0.99 (7)      &       \ion{Al}{ii}~$\lambda$1670.7  & 3.3713\\
 7907 & 0.58 (5)      &         &                 &        \ion{Si}{ii}~$\lambda$1808.0  & 3.3734\\
 8112 & 0.45 (5)      &         &                 &       \ion{Al}{iii}~$\lambda$1854.7  & 3.3738\\
 8145 & 0.23 (4)      &         &                 &     \ion{Al}{iii}~$\lambda$1862.7  & 3.3724\\
 8237 & 0.34 (4)      &         &                 & 	                &	    \\
 8802 & 0.55 (6)      &         &                 & 	                &	    \\
 8859 & 0.82 (9)      &         &                 &      \ion{Zn}{ii}~$\lambda$2026.1  & 3.3725\\
 8970 & 0.73 (11)     &         &                 &$\oplus$                    &       \\
 9019 & 0.77 (5)      &         &                 &$\oplus$, \rm \ion{Zn}{ii}~$\lambda$2062.6  & 3.3726\\
 \hline
  \end{tabular}}
$^{{a}}$ \lyb\ is located in the \lya\ forest, which
    causes it to be blended with forest lines, and the continuum
    placement is highly uncertain, resulting in a large {\it EW} error.\\
$^{{b}}$ The lines at $\lambda\lambda$5652.0, 6278.0,
    6743.0, and 6754.2 can in principle be identified with
    \ion{Fe}{ii} and \ion{Mg}{ii} at $z=1.41$; however, strong
    absorption is then expected from \ion{Fe}{ii} $\lambda$2382, which is
    not detected.\\
$^{{c}}$ The lines for which significant absorption
    was also detected in the standard star spectrum are marked with a
    $\oplus$.
\end{table}