\begin{table}%t5
\caption{\label{co_lines}Fitted fluxes for the CO~lines observed above 120~$\mu$m for \object{VY~CMa}.}
%\centering
 \small \begin{tabular}{ccccc|c}
\hline \hline\noalign{\smallskip}
Transition  & Wavelength & Auto & Manual  \\
&  ($\mu$m)  & fit flux &  fit flux\tablefootmark{a}\\
&           & (10$^{-19}$ W cm$^{-2}$) & (10$^{-19}$~W~cm$^{-2}$) \\
\hline
$J = 14$--13 & 185.999 & 1.72  & $1.96 \pm 0.4$  \\
$J = 15$--14 & 173.631 & 1.35  & $1.88 \pm 1.3$  \\
$J = 16$--15 & 162.812 & 2.37  & $2.69 \pm 1.4$  \\
$J = 17$--16 & 153.267 & 1.54  & $2.00 \pm 0.6$ \\
$J = 18$--17 & 144.784 & -Blend- & -Blend-  \\
$J = 19$--18 & 137.196 & 1.06  & $1.31 \pm 1.1$  \\
$J = 20$--19 & 130.369 & -Blend- & -Blend-  \\
$J = 21$--20 & 124.193 & 1.60  & $0.92 \pm 2.0$ \\
\hline
\end{tabular}
\tablefoot{\tablefoottext{a}{Errors do not include systematic uncertainty in the baseline subtraction ($\sim$30\%)}.}
\vspace*{-3mm}
\end{table}