\begin{table}%T2
\caption{\label{clusters}Results for cluster detection.}
\small%\centerline
{
\begin{tabular}{lccccccccccc}  
\hline\hline\noalign{\smallskip}
 Sou. & $d^a$ & $I_{\rm c}$ & $N_{\rm obs}$ & $R_{\rm clu}$ & \multicolumn{2}{c}{Pre-MS} & $M_{\rm gas}$ & $L_{\rm bol}$ & $A_V$ $_{\rm peak}$ & \multicolumn{2}{c}{Cluster Center} \\
 Mol & kpc & & & pc & \% & \% & \msun & 10$^3$\lsun & mag & $\alpha$(J2000) & $\delta$(J2000) \\
 &  & & &  & \textit{CC} & \textit{CM} &  &  & \\ \hline
3    & 2.17 & 78   & 78   & 1.7 & 34 & 99 & 910 & 12.4 & 18 &	00:44:57.4	&	+55:47:20.0 \\
8A    & 11.5 & 25  & 30   & 1.3 & 37 & 27 & 1650 & 57.0 & 18 &	05:17:13.8	&	+39:22:29.7 \\
8B    & 11.5 & 27  & 24   & 1.3 & 9 & 4 & 1780 & 5.5 & 8 &	05:17:12.0	&	+39:21:51.8 \\
9    & 6.2 & 7   & 7   & 0.6 & 16 & $-^g$ & $-$ & 24 & $-$ &	05:20:16.9	&	+36:37:22.0 \\
11   & 2.1 & 51   & 48   & 0.5 & 12 & 41 & 360 & 4.6 & 35 &	05:37:47.7	&	+31:59:24.0 \\
12   & 1.6 & 12   & 13   & 0.3 & 0    & 30 & 72 & 1.6 & 46 &	05:40:24.4	&	+23:51:54.8 \\
15  & 1.5 & 64   & 61   & 0.3 & 34  & $-^g$ & $-$ & 5.8 & $-$ &	06:08:41.0	&	+21:31:00.0 \\
28   & 4.5 & 75   & 75   & 1.0 & 58 & 95  & 220 & 9.1 & 4 &	07:00:51.5	&	$-$08:56:18.2 \\
30   & 0.3 &  200$^e$ & \multicolumn{4}{c}{no cluster detected$^b$} & -- & 0.14 & $-$ & $-$ & $-$ \\
38   & 0.5 & $-$5 & \multicolumn{4}{c}{no cluster detected$^c$} & --$^h$ & 0.19 & 40 & $-$ & $-$ \\
45   & 4.3 & 28   & 27   & 0.5 & 68 & 19   & 1340 & 21.2 & 77 &	18:17:24.1	&	$-$17:22:12.3 \\
50   & 4.9 & 46   & 43 & 0.6 & 36 & 41 & 80 & 17.3 & 25 & 18:19:07.6 & $-$16:11:21.0 \\
59   & 5.7 & 0 & \multicolumn{4}{c}{no cluster detected$^c$} & --$^h$ & 11 & 29 & $-$ & $-$ \\
75   & 3.9 & 8     & 7     & 0.7 & 37 & 24 & 1310 & 13.3 & 38 &	18:53:38.1	&	+01:50:26.5 \\
82   & 6.8 & 8 & 10 & 0.3 & 0 & 52 & 590 & 15.4 & 52 &	18:59:03.2	&	+03:53:16.7 \\
84   & 2.2 & 21   & 21   & 0.3 & 0 & 54 & 28 & 4.3 & 15 &	18:59:14.3	&	+07:04:52.3 \\
98   & 4.5 & 6 & \multicolumn{4}{c}{no cluster detected$^f$} & --$^h$ & 9.2 & 68 &	$-$ & $-$  \\
99  & 6.1 & 45   & 38   & 0.9 & 49 & $-^g$ & $-$ & 37.3 & $-$ &	19:11:51.4	&	+09:49:35.4 \\
103 & 4.1 & 105 & 107 & 0.7 & 46 & 87 & 510 & 28.2 & 42 &	19:23:36.2	&	+17:28:58.1 \\
109 & 4.3 & 19   & 17   & 0.5 & $^d$ & $^d$ & 1030 & 26.7 & 90 &	19:39:33.0	&	+24:00:21.3 \\
110 & 4.3 & 23   & 20   & 0.5 & $^d$ & $^d$ & 400 & 14.8 & 55 &	19:40:58.5	&	+24:04:36.3 \\
136  & 3.6 & 21   & 19   & 0.6 & 18 & 52 & 230 & 4 & 21 &	21:32:31.4	&	+51:02:23.1 \\
139 & 7.3 & 25   & 24   & 1.2 & 10 & 31 & 1870 & 1.35 & 20 &	21:53:39.2	&	+56:27:50.7 \\
143  & 5.0 & 25   & 22   & 0.8 & 10 & 76 & 630 & 7.8 & 26 &	22:19:09.0	&	+56:04:58.7 \\
148 & 5.1 & 43 & 41 & 0.9 & 43 & 64 & 22 & 7.8 & 13 &	22:32:23.4	&	+58:19:01.3 \\
151 & 5.4 & 15   & 14   & 0.9 & 12 & 30 & 2020 & 25 & 40 &	22:52:38.3	&	+60:00:44.6 \\
160  & 5.0 & 36   & 34   & 1.3 & 30 & 76 & 1830 & 16 & 32 &	23:40:53.1	&	+61:10:21.0 \\ \hline
\end{tabular} }
\smallskip
 $^a$ Kinetic distance using the rotation curve from Brand \& Blitz (\cite{BrBl}). \\
 $^b$ Stellar density analysis inconclusive due to extreme
crowdedness of this field. \\
 $^c$ Stellar density reveales no peaks close to the IRAS
position or the submm peak. \\
 $^d$ Only observed in \ks. \\
 $^e$ Detection refused due to extreme field complexity (see text). \\
 $^f$ Detection refused because only 1 annulus in the radial density profile is above background (see text). \\
 $^g$ No extinction estimate is available due to lack of submm information to evaluate de-reddening correction. \\
 $^h$ Extinction estimate is available from single-pointing submillimeter data (Molinari et~al. \cite{Metal00}) but not from maps, so that a reliable clump mass estimate is not possible. 
\end{table}