\begin{table}%t1
\caption{\label{tab1}$^{13}$CO(3--2) Observations and results.}
%\centering
\par
\begin{tabular}{lc}
\hline\hline\noalign{\smallskip}
{Parameter}&{$^{13}$CO(3--2)}\\
\hline
\multicolumn{2}{l}{{\it Observed CO(3--2) quantities:}}
\\
RA (J2000)              &14$^{\rm h}$ 15$^{\rm m}$ 46\ffs28 $\pm$ 0\ffs03\\
Dec (J2000)              &+11$^{\circ}$ 29$'$ 44\ffas0 $\pm$ 0\ffas4 \\
Center frequency (GHz)    &92.91816         \\
Redshift (LSR)\tablefootmark{a}   &$2.55784\pm 0.00003$   \\
Continuum flux density (mJy)\tablefootmark{b} &$0.3\pm 0.1$ \\
Integrated $^{13}$CO flux (Jy~\kms)\tablefootmark{b} &$0.3\pm 0.1$    \\
\\
\multicolumn{2}{l}{{\it Derived CO(3--2) quantities:}}
\\
$L^\prime$($^{13}$CO (\Kkmspc )\tablefootmark{c}     &($1.1\pm 0.3$)$\times 10^{10}$  \\
$L^\prime$($^{12}$CO (\Kkmspc )\tablefootmark{c}       &($45.9\pm 3$)$\times 10^{10}$  \\
$L^\prime$ ratio $^{12}$CO/$^{13}$CO(3--2)   &40$^{+25}_{-8}$    \\
\hline
\end{tabular}
\tablefoot{\tablefoottext{a}{Adopted from $^{12}$CO (Weiss et~al. \cite{Weiss2003}).}
\tablefoottext{b}{In a beam of 6\ffas$1\times5$\ffas4.}
\tablefoottext{c}{This is the lens-amplified value for a luminosity distance of 
$D_L = 21.28$~Gpc ($H_0 =71$~\kms~Mpc$^{-1}$, $\Omega_{\rm m} = 0.27$, 
$\Omega_{\rm vac} = 0.73$) and an angular diameter distance of $D_{\rm A} = 1.682$~Gpc; 
linear scale: $1'' \leftrightarrow 8152$~pc (Wright \cite{Wright2006}).}}
\end{table}