\begin{table}%tB.1
\caption{\label{Odin table}Observed transitions and their parameters$^{{a}}$ in S140 with the Odin satellite in a five point NE-SW strip.}
\small%\centerline
 {
 {
\begin{tabular}{ l l l l l l l r r r  rl}
\hline
\hline
%&&&&&&&&&&& \\[-8pt]
Species		& Transition 	 & Freq  	& $E_{\rm u}$	&$A$-coeff & $\Delta \upsilon$&	Pos. & $\upsilon_{{\rm LSR}}$ & $T_{\rm peak}$
& $\int$ $T^{~*}_{{\rm A}}$ d$\upsilon$       &rms   &note  \\
	                      &	          & [GHz]	 &	[K] 	& [s$^{-1}$] &[kms$^{-1}$] &&[kms$^{-1}$]& [mK] & [K kms$^{-1}$]&[mK]  &\\
\hline
 H$_2$O	& 1$_{1,0}$--1$_{0,1}$& 556.936&61.0&3.46e-3 &0.27      
      &  1      &--8.0 & 207 &  0.64&39&  \\ 
&&&&&&2& --6.9 & 517 & 2.74&68&\\ 
&&&&&&3& --6.6 & 632 &3.34 &19&\\ 
&&&&&&4& --7.0 & 379 &1.84 &57&\\ 
&&&&&&5&  --  &--   &   -- & 44& No detection. \\ 
H$_2^{18}$O 	& 1$_{1,0}$--1$_{0,1}$& 	547.676	&60.5	&3.29e-3&0.34&3&-- &-- &-- &$\sim$8 &	 No detection.\\ 
CO 	& 5--4& 	576.258		&83.0 &1.22e-5&0.32&1&--5.4 &6680& 47.1&67 &	\\
&&&&&&2& --5.0 &11~760  &94.2 &47&\\
&&&&&&3& --5.5 & 13~240 &108.8 &43&\\
&&&&&&4& --6.6 & 8690 & 60.1 &50&\\
&&&&&&5& --6.9 & 2220 & 10.1 &160&\\
$^{13}$CO 	& 5--4& 	550.926	&79.3	&1.10e-5&0.27&1&  --7.8 & 2~740& 8.29 &115& \\  
&&&&&&2& --7.4 & 5930 & 21.4&81&\\
&&&&&&3& --7.4 & 7110 & 27.7&61&\\
&&&&&&4& --7.6 & 3640 & 13.2&119&\\
&&&&&&5& --8.5 & 1190  &2.5&291&\\ 
NH$_3$ 	& 1$_{0}$--0$_{0}$& 	572.498		&27.5& 1.61e-3&0.32&1&
                       --8.0 &  444  & 1.18&99&	 \\
&&&&&&2& --7.4  & 467 & 1.83 &33&\\
&&&&&&3& --7.4 & 588 & 2.66 &29&\\
&&&&&&4& --7.3  & 381  & 1.86 &36&\\
&&&&&&5& --  & --  &--  &91&No detection\\
\hline
\end{tabular}}}
\medskip
$^{{a}}$ Transition = the quantum numbers for the transition; Freq~= rest frequency of the transition;   $E_{\rm u}$~= the upper state energy; $A$-coeff~= the Einstein $A$-coefficient; $\Delta \upsilon$~= the velocity resolution; Pos~= the strip position from NE to SW. $\upsilon_{\rm LSR}$~= the peak LSR~velocity;  $T_{\rm peak}$~= the observed peak temperature of the transition;   $\int$~$T^{~*}_{{\rm A}}$~d$\upsilon$~= the integrated intensity from the observed spectra not corrected for beam-efficiency or beam-filling; rms~=~noise.
\end{table}