\begin{table}%T2
\setcounter{table}{1}
\caption{The 34.6~$\mu$m and 1612~MHz line parameters for the three supergiants
which are used to estimate the OH~maser radiative pump rate. 
The integrated fluxes $F^{\rm int}_{34.6}$ is in [$10^{-19}$~W/cm$^2$], 
$F^{\rm int,blue}_{\rm OH}$ is in [$10^{-26}$~W/cm$^2$] while the equivalent
widths $EW_{34.6}$ is in [$10^{-4}~\mu$m]. Negative
values mean that the line is in absorption.}
\label{LineOHpump}
%\centerline
{
\begin{tabular}{l@{~~~ }l@{ ~~~ }l@{ ~~~ }l@{~~~ }l@{~~~  }l@{~~~  }l@{~~~  }l@{ ~~~ }l@{~~~}}
\hline\hline
\noalign{\smallskip}
Name &TDT$^{*}$  &$F^{\rm int}_{34.6}$ &$EW_{34.6}$ &$F^{\rm int,blue}_{\rm OH}$ &Pump rate &References1 &$F^{\rm int,lit}_{34.6}$ & References2$^{**}$ \\
(1)       &(2)        &(3)                  &(4)         &(5)                         &(6)       &(7)         &(8)                      &(9)            \\
\noalign{\smallskip}
\hline
\noalign{\smallskip}
IRAS~07209$-$2540~~~    &73103039~~~               &$-18.7~~~      $       &$-18.0~~~      $        &$1751~~~        $ &$0.052 ~~~ $ &tL-H(fig)$^{\#\#}$~~~     &--21.0~~~               &NEU99~~~   \\
                         &73402218               &$-21.4      $       &$-20.9      $        &               &          &              &                    &        \\
                         &$\underline{73601963}$ &$\underline{-17.6}$ &$\underline{-16.2}$  &               &          &              &                    &        \\
IRAS~19244$+$1115    &31600936               &$-4.12      $       &$-12.6      $        &$662         $ &$0.042$   &SYL97         &--4.8                & SYL97  \\
                         &$\underline{36401613}$ &$\underline{-8.10}$ &$\underline{-21.0}$  &               &          &              &                    &        \\
                         &36401631               &$-3.31      $       &$-10.3      $        &               &          &              &                    &        \\
                         &72400804               &$-6.49      $       &$-15.9      $        &               &          &              &                    &        \\
NML~Cyg         &05200726               &$-34.7      $       &$-54.4      $        &$1154        $ &$0.052  $ &priv(fig)$^{\#\#}$      &                    &        \\
                         &34201475               &$-8.74^{\#} $       &$-14.7^{\#} $        &               &          &              &                    &        \\
                         &$\underline{52200201}$ &$\underline{-11.5}$ &$\underline{-16.0}$  &               &          &              &                    &        \\
                         &52200719               &$-8.34      $       &$-16.8      $        &               &          &              &                    &        \\
                         &52200720               &$-5.01      $       &$-9.34      $        &               &          &              &                    &        \\
                         &53001311               &$-5.86      $       &$-11.0      $        &               &          &              &                    &        \\
                         &74103105               &$-34.8      $       &$-49.3      $        &               &          &              &                    &        \\
              \noalign{\smallskip}               
\hline 
\end{tabular}}
\medskip
* The best spectrum together with its parameters are underlined for each source. 
  They are used to estimate the pump rate.\\
{**} The reference codes in Col.~(9):
NEU99: Neufeld et~al. (\cite{neu99});
SYL97: Sylvester et~al. (\cite{syl97}).\\
\# Only the sub-line No.~10 of 34201475 
spectrum are used.\\
\#\# (fig) means the integrated 1612~MHz OH~maser fluxes are measured by us from the figure in the literature.
\end{table}