\begin{table}%tB.5
\caption{\label{tab_par95GHz}Same as Table~\ref{par_classI} for the 95~GHz \METH\ maser (Class~I) detected with the Nobeyama 45-m telescope.}
%\centering
\par
\begin{tabular}{cccccc}
\hline \hline
\noalign{\smallskip}
Source\tablefootmark{a} & \Vlsr\ & $\int F_{\nu} {\rm d}V$ &    $V$     &      $\Delta V$    &     $F_{\nu}^{\rm peak}$  \\
        & (km s$^{-1}$)  &  (Jy km s$^{-1}$)  & (km s$^{-1}$)  &  (km s$^{-1}$)  &  (Jy)  \\
\hline\\[-3.2mm]
 H05480+2545  &    --9.3\tablefootmark{b}  & 3.1 $\pm$ 0.6      & --10.6 $\pm$ 0.1     &    1.3 $\pm$ 0.3      &   2.2  \\
 H18089-1732    &   32.9 &  2.7 $\pm$ 0.4    &     31.38 $\pm$ 0.02  &        0.45 $\pm$ 0.05  &       5.5 \\  
    &    &  14 $\pm$ 2      &   32.4 $\pm$ 0.2  &       3.2 $\pm$ 0.4   &      4.2   \\
 H18159-1648   &  22.1 &  4.7 $\pm$ 0.8      &    20.1 $\pm$ 0.1       &   1.6 $\pm$ 0.4       &   2.7   \\
    &   &  7.6 $\pm$ 0.6       &   22.56 $\pm$ 0.06 &     1.4 $\pm$ 0.1     &    5.2  \\   
 H18316-0602   &  42.2 &  1.1 $\pm$ 0.2 &     41.63 $\pm$ 0.05 &    0.5 $\pm$ 0.1 &        2.1 \\  
 H18360-0537   &  102.3 &  13.2 $\pm$ 0.8      &   102.5 $\pm$ 0.1      &  4.1 $\pm$ 0.4       &   4.0    \\ 
 H20126+4104  & --3.9  &  6.0 $\pm$ 0.4       & --2.75 $\pm$ 0.08    &  2.3 $\pm$ 0.2       &   2.5   \\
 H21391+5802  &   0.4   & 2.5 $\pm$ 0.6      &   12.1 $\pm$ 0.1        &  1.2 $\pm$ 0.5      &   2.0    \\
 H22506+5944  & --51.5 &  5 $\pm$ 1    & --47.1 $\pm$ 0.2      &    2.4 $\pm$ 0.6    &     2.0   \\
 L18018-2426    &  10.5  & 33.5 $\pm$ 0.4    &     10.800 $\pm$ 0.004 &    0.622 $\pm$ 0.009 &    50  \\  
 L18144-1723   &   47.3 &  26.4 $\pm$ 0.6     &     47.91 $\pm$ 0.03    &  2.07 $\pm$ 0.08  &    12   \\
 L18396-0431  &  97.3  & 3.8 $\pm$ 0.4    &     50.37 $\pm$ 0.08  &    1.24 $\pm$ 0.2   &       2.9   \\
    &    & 14 $\pm$ 2       &   57.4 $\pm$ 0.6    &      7 $\pm$ 1     &    1.9   \\
     &   & 4 $\pm$ 1      &    61.5 $\pm$ 0.1   &       1.3 $\pm$ 0.4  &        2.5   \\
    &   &  8.0 $\pm$ 0.8   &     71.3 $\pm$ 0.2   &        3.4 $\pm$ 0.6 &         2.2   \\
     &    &  1.6 $\pm$ 0.2     &     130.50 $\pm$ 0.08 &    0.7 $\pm$ 0.1 &        2.1 \\ 
\hline
\end{tabular}
\tablefoot{
\tablefoottext{a}{``L'' and ``H'' indicate if the source belongs to the \low\ or \high\ sample;}
\tablefoottext{b}{from \AMM\ observations performed with the Nobeyama 45-m telescope.}
}
\end{table}