\begin{table}%t4
      \caption{\label{tab:glob}Column densities integrated over the sightlines. H\1~and H$_2$ measurements are from A2003.
      The \textit{FUSE} determination of the P\2~column density makes use of the $\lambda1125$ line while the
       HST/\textit{STIS} determination makes use of the $\lambda1533$ line. O\1~is analyzed through the
       $\lambda1356$ transition.}
                  %\centerline
{
         \begin{tabular}{lcccccc}
            \hline\hline
         Sightline  &  $\log N${\rm (H\1)} &   {\rm $f$(H$_2$)} &    $\log N${\rm (P\2)}  &  $\log N${\rm (P\2)}  &   $\log N${\rm (O\1)}  &  $\log$~{\rm P\2/O\1}\\
      &                          &                  &     $[$FUSE$]$     &     $[$STIS$]$             &  $[$STIS$]$             &  $[$STIS$]$                         \\
           \hline
HD~24534 &    /     &      0.76     &     /        & $14.42\pm0.05$ & $17.82\pm0.06$ &  $-3.40\pm0.08$ \\
         &          &        &        &                   &                   (/)$^{{a}}$ &       \\
HD~93222& $21.40$ &  $0.05$ &  $14.79\pm0.06$ & $14.82\pm0.01$ & $18.12\pm0.03$ & $-3.30\pm0.03$ \\
         &          &        &        &                   &                   ($18.13\pm0.02$)$^{{a}}$ &       \\
HD~99857&  $21.24$ &  $0.24$ &  $14.67\pm0.06$ & $14.64\pm0.02$ & $17.90\pm0.03$ & $-3.26\pm0.03$ \\
         &          &        &        &                   &                   ($17.89\pm0.03$)$^{{a}}$ &       \\
HD~104705 & $21.10$ &  $0.16$ &  $14.75 \pm 0.04$ & $14.54 \pm 0.04$ & $17.77\pm 0.04$ &$-3.23 \pm 0.06$ \\
         &          &        &        &                   &                   ($17.81\pm0.02$)$^{{a}}$ &       \\
HD~121968 &    /      &     /    &  $14.04\pm0.09$ & $14.02\pm0.09$ & $17.10\pm0.11$ &$-3.08\pm0.15$ \\
         &          &        &        &                   &                   (/)$^{{a}}$ &       \\
HD~124314 & $21.41$ &  $0.20$ &  $14.81 \pm 0.04$ & $14.96 \pm 0.24$ & $18.24 \pm 0.11$ &$-3.28 \pm 0.28$ \\
         &          &        &        &                   &                   ($18.18\pm0.02$)$^{{a}}$ &       \\
HD~177989& $20.96$ &  $0.25$ &  $14.43 \pm 0.04$ & $14.47 \pm 0.07$ & $17.80 \pm 0.05$ &$-3.33 \pm 0.09$ \\
         &          &        &        &                   &                   ($17.79\pm0.03$)$^{{a}}$ &       \\
HD~202347 & $20.94$ &  $0.17$ &  $14.34\pm0.17$ & $14.33\pm0.07$ & $17.58 \pm 0.10$ &$-3.26\pm0.13$ \\
         &          &        &        &                   &                   ($17.58\pm0.06$)$^{{a}}$ &       \\
HD~218915 & $21.17$ & $0.18$ &  $14.37\pm0.10$ & $14.53\pm0.09$ & $17.83\pm0.05$ &$-3.30\pm0.11$ \\
         &          &        &        &                   &                   ($17.82\pm0.03$)$^{{a}}$ &       \\
HD~224151 & $21.32$ &  $0.28$ & /                  & $14.87\pm0.09$ & $18.10\pm0.05$ & $-3.23\pm0.11$ \\
         &          &        &        &                   &                   ($18.06\pm0.03$)$^{{a}}$ &       \\
            \hline
\multicolumn{7}{l}{$^{{a}}$ When measured, O\1~column densities derived in A2003.}           
         \end{tabular}}
%\smallskip
   \end{table}