\begin{table}%t1
\caption{\label{f10214-table}Observed CO and $\mbox{\rm C {\scriptsize I}}$ line
parameters towards F10214.}
\small%\centerline
 {
\begin{tabular}{c c c c c c c c}
\hline \hline
Line & Telescope & $\nu_{\rm obs}$ & $S_\nu$$^{{a}}$ & $\Delta$$V_{\rm FWHM}$$^{{b}}$ & $I^{{a}}$ &
$V^{{b}}$ & $L'$/10$^{\rm 10}$$^{{~ c}}$ \\
& & [GHz] & [mJy] & [\kms] & [Jy \kms] & [\kms] & [\kkmspc] \\
\hline
avg. profile  & IRAM 30 m & ... & ... & 246 $\pm$ 10 & ... & 20 $\pm$ 4 & ... \\
CO(3$-$2)  & IRAM 30 m & 105.25230 & 15.5 $\pm$ 3.5 & 174 $\pm$ 23 & 3.80 $\pm$ 0.45 & 25 $\pm$ 11 & 10.83 $\pm$ 1.28 \\
CO(3$-$2)  & PdBI & 105.25160  & 13.5 $\pm$ 0.6 & 224 $\pm$ 12 & 3.40 $\pm$ 0.19 & 4 $\pm$ 4 & 9.70 $\pm$ 0.54 \\
CO(4$-$3)  & IRAM 30 m & 140.33020 & 21.7 $\pm$ 4.0 & 245 $\pm$ 28 & 5.32 $\pm$ 0.51 & 17 $\pm$ 11 & 8.53 $\pm$ 0.82 \\
CO(6$-$5)  & IRAM 30 m & 210.46850 & 28.8 $\pm$ 3.3 & 203 $\pm$ 16 & 7.09 $\pm$ 0.47 & 20 $\pm$ 7 & 5.06 $\pm$ 0.34 \\
CO(7$-$6)  & IRAM 30 m & 245.52621 & 22.1 $\pm$ 4.6 & 248 $\pm$ 30 & 5.43 $\pm$ 0.56 & 18 $\pm$ 14 & 2.84 $\pm$ 0.29 \\
\cone & IRAM 30 m & 149.80235 & 8.3 $\pm$ 2.4  & 156 $\pm$ 26 & 2.03 $\pm$ 0.36 & -5 $\pm$ 14 & 2.86 $\pm$ 0.51$^{{d}}$ \\
\ctwo & PdBI & 246.34500  & 18.7 $\pm$ 2.3 & 182 $\pm$ 30 & 4.59 $\pm$ 0.66 & -6 $\pm$ 10 & 2.39 $\pm$ 0.34 \\
\hline
\end{tabular}}
\medskip
$^{{a}}$ The values are derived from Gaussian fits with the fixed line width and center velocity of the averaged CO line profile. \\
$^{{b}}$ The values are obtained from Gaussian fits to each spectrum. The velocity offsets are
centered at a redshift of 2.2854 (Downes et~al. \cite{Down95}). \\
$^{{c}}$ We use a $\Lambda$ cosmology with $H_{\rm0}$~= 73~$\rm \kms~Mpc^{-1}$, $\rm \Omega_\Lambda$~= 0.74 and $\rm \Omega_{\rm m}$~= 0.26 (Spergel et~al. \cite{Sper07}). \\
$^{{d}}$ The data are from Wei\ss\ et~al. (\cite{Weis05a}), but fitted with the fixed line width and central velocity.
\end{table}