\begin{table}%t3
\caption {Sources observed during the first observing run only. Columns~6--9
give the peak of each line or the rms level of the spectrum, both in K.}
\label{tab_sou_2}
%\centerline
{\begin{tabular}{lllllllll}
\hline \hline
IRAS & RA (J2000) & Dec. (J2000) & \Vlsr\ & $d_{\rm kin}$ & \H\ (1--0) & \H\ (3--2) & \D\ (2--1) & \D\ (3--2) \\
Source & (h m s) & ($^{\circ}$ $'$  $''$) & (\kms ) & (kpc) & & & \\
\hline
IRAS 05490+2658$^{2}$ & 05 52 12.9 &  26 59 33 & 0.8 & 2.1 & 0.4 & ${\leq} 0.9$ & ${\leq} 0.19$ & ${\leq} 0.3$ \\
IRAS 18567+0700$^{1}$ & 18 59 13.6 &  07 04 47 & 29.4 & 2.16 & 0.5 & ${\leq} 0.4$ & ${\leq} 0.13$ & ${\leq} 0.2$\\
IRAS 20106+3545$^{1}$ & 20 12 31.2 &  35 54 46 & 7.8 & 1.6 & 0.5 & 0.45 & ${\leq} 0.05$ & ${\leq} 0.05$ \\
IRAS 20205+3948$^{2}$ & 20 22 21.9 &  39 58 05 & $-$1.7 & 4.5 & $\leq$0.03 & ${\leq} 0.1$ & ${\leq} 0.05$ & ${\leq} 0.05$ \\
IRAS 20278+3521$^{1}$ & 20 29 46.9 &  35 31 39 & $-$4.5 & 5.0 & 0.3 & ${\leq} 0.2$ & ${\leq} 0.06$ & ${\leq} 0.08$ \\
IRAS 22134+5834$^{2}$ & 22 15 09.1 &  58 49 09 & $-$18.3 & 2.6 & 1.2 & 1.6 & ${\leq} 0.06$ & ${\leq} 0.08$ \\
IRAS 23139+5939$^{2}$ & 23 16 09.3 &  59 55 23 & $-$44.7 & 4.8 & 0.9 & 1.5 & ${\leq} 0.16$ & ${\leq} 0.3$ \\
IRAS 23151+5912$^{2}$ & 23 17 21.0 &  59 28 49 & $-$54.4 & 5.7 & ${\leq} 0.08$ & ${\leq} 0.5$ & ${\leq} 0.13$& ${\leq} 0.36$ \\
%IRAS 23385+6053$^\dagger$ & 23 40 54.498 &  61 10 28.01 & 5.8 & 4.9 & ${\leq} 0.08$ & ${\leq} 0.9$ & ${\leq} 0.19$ & ${\leq} 0.45$ \\
IRAS 23545+6508$^{2}$ & 23 57 05.2 &  65 25 11 & $-$18.4 & 0.8 & ${\leq} 0.07$ & ${\leq} 0.8$ & ${\leq} 0.15$ & ${\leq} 0.42$\\
\hline
\end{tabular}
}
\par
\footnotesize
$^{ 1}$  \Vlsr\ and $d_{\rm kin}$ from \AMM\ observations (Molinari et~al.~\cite{mol96}). $^{ 2}$  \Vlsr\ and $d_{\rm kin}$ from \AMM\ observations (Sridharan et~al.~\cite{sridharan}). 
\normalsize
\end{table}