\begin{table}%t1
%\centering
\par
\caption{SCUBA 850~$\mu$m core positions, names and references, peak
850~$\mu$m fluxes and C$^{18}$O integrated intensity at the submm peak
position.\label{tbl:sourcelist}} 
\begin{tabular}{ccclllcc} 
\hline\hline
\noalign{\smallskip}
No. & \multicolumn{1}{c}{RA$_{2000}$} &
\multicolumn{1}{c}{Dec$_{2000}$} &
Cluster$^{(1)}$ & Name & Reference$^{(2)}$ & $F_{850}^{(3)}$ & 
$I(\hbox{C}^{18}\hbox{O})^{(4)}$\\
 &\multicolumn{1}{c}{hh:mm:ss} & \multicolumn{1}{c}{dd:mm:ss}& & & &
mJy/bm &    K~km~s$^{-1}$ \\
\hline
 1&03:33:17.9&31:09:33&B1&B1-c&\citet{matthews02}&1638&4.0\\ 
 2&03:33:21.4&31:07:31&B1&B1-bS&\citet{hirano99,matthews02}&1554&4.8\\ 
 3&03:33:21.1&31:07:40&B1&B1-bN&\citet{hirano99,matthews02}&1200&4.8\\ 
 4&03:33:16.3&31:06:54&B1&B1-d&\citet{matthews02}&514&4.1\\ 
 5&03:33:01.9&31:04:23&B1&None&&218&3.3\\ 
 6&03:33:05.6&31:05:06&B1&None&&207&2.8\\ 
 7&03:33:16.5&31:07:51&B1&B1-a&\citet{hirano99,matthews02}&202&4.5\\ 
 8&03:33:04.0&31:04:56&B1&None&&202&2.9\\ 
 9&03:33:03.0&31:04:38&B1&None&&196&3.4\\ 
10&03:33:27.3&31:07:10&B1&None&&179&4.2\\ 
11&03:33:00.3&31:04:17&B1&None&&160&3.4\\ 
%%
12&03:43:56.5&32:00:50&HH211&HH211&\citet{mccaughrean04,chandlerricher00}&1494&2.5\\ 
%%
13&03:43:56.9&32:03:05&HH211&IC~348 MMS&\citet{eisloeffel03}&1032&3.1\\ 
14&03:44:43.9&32:01:32&HH211&None&&623&2.0\\ 
15&03:43:50.8&32:03:24&HH211&No SMM/MM source&&358&2.2\\ 
16&03:44:01.0&32:01:55&HH211&None&&296&2.4\\ 
17&03:43:57.9&32:04:01&HH211&None&&247&3.0\\ 
18&03:44:03.0&32:02:24&HH211&No SMM/MM source&&237&2.5\\ 
19&03:44:36.8&31:58:49&HH211&None&&234&1.8\\ 
20&03:44:05.5&32:01:57&HH211&No SMM/MM source&&209&2.4\\ 
21&03:44:02.3&32:02:48&HH211&None&&207&2.9\\ 
22&03:44:06.2&32:02:12&HH211&None&&204&2.4\\ 
23&03:43:37.8&32:03:06&HH211&None&&170&1.5\\ 
24&03:43:42.5&32:03:23&HH211&None&&168&2.3\\ 
25&03:44:48.5&32:00:31&HH211&None&&153&2.0\\ 
26&03:43:44.4&32:02:56&HH211&None&&153&2.5\\ 
27&03:25:35.9&30:45:30&L1448&L1448NW	 &\citet{looney00,barsony98}&2300&2.9\\ 
28&03:25:36.4&30:45:15&L1448&L1448N B  &\citet{looney00,barsony98}&2243&2.7\\ 
29&03:25:38.8&30:44:04&L1448&L1448 C&\citet{bachiller91,barsony98}&1737&2.3\\ 
30&03:25:22.4&30:45:11&L1448&L1448-IRS2  &\citet{olinger99}&1316&2.2\\ 
31&03:25:25.9&30:45:03&L1448&None&&429&2.4\\ 
32&03:25:49.0&30:42:25&L1448&None&&364&2.0\\ 
33&03:25:50.6&30:42:01&L1448&None&&306&2.1\\ 
34&03:25:30.8&30:45:07&L1448&None&&231&2.6\\ 
35&03:27:39.1&30:13:01&L1455&RNO 15 FIR&\citet{rengel02}&556&1.4\\ 
36&03:27:42.9&30:12:28&L1455&None&&402&0.9\\ 
\hline
37&03:27:48.4&30:12:09&L1455&No SMM/MM source&&324&0.8\\ 
38&03:27:46.6&30:12:05&L1455&No SMM/MM source&&272&0.9\\ 
39&03:27:38.1&30:13:57&L1455&No SMM/MM source&&238&1.4\\ 
40&03:27:39.9&30:12:10&L1455&None&&232&1.4\\ 
41&03:29:10.4&31:13:30&NGC~1333&IRAS 4A&\citet{sandell91}&7000&3.7\\ 
42&03:29:12.0&31:13:10&NGC~1333&IRAS 4B; SK-3&\citet{sandell91,sandellknee01}&3025&3.4\\ 
43&03:29:03.2&31:15:59&NGC~1333&HH7-11 MMS 1; SK-12/13&\citet{chini97}&2831&4.0\\ 
44&03:28:55.3&31:14:36&NGC~1333&IRAS 2A; SK-8&\citet{sandell94,sandellknee01}&2355&3.8\\ 
45&03:29:01.4&31:20:29&NGC~1333&SK-24&\citet{sandellknee01}&1119&3.7\\ 
46&03:29:10.9&31:18:27&NGC~1333&SK-20&\citet{sandellknee01}&1061&3.6\\ 
47&03:28:59.7&31:21:34&NGC~1333&SK-31&\citet{sandellknee01}&770&4.9\\ 
48&03:29:13.6&31:13:55&NGC~1333&IRAS 4C; SK-5&\citet{looney00,sandellknee01}&667&3.3\\ 
49&03:28:36.7&31:13:30&NGC~1333&SK-6&\citet{sandellknee01}&621&2.0\\ 
50&03:29:06.5&31:15:39&NGC~1333&HH 7-11 MMS 4; SK-15&\citet{chini01,sandellknee01}&619&3.2\\ 
51&03:29:08.8&31:15:18&NGC~1333&SK-16&\citet{sandellknee01}&574&2.8\\ 
52&03:29:03.7&31:14:53&NGC~1333&HH7-11 MMS 6; SK-14&\citet{chini01,sandellknee01}&517&3.8\\ 
53&03:29:04.5&31:20:59&NGC~1333&SK-26&\citet{sandellknee01}&513&4.8\\ 
54&03:29:10.7&31:21:45&NGC~1333&SK-28&\citet{sandellknee01}&420&3.6\\ 
55&03:28:40.4&31:17:51&NGC~1333&None&&410&1.9\\ 
56&03:29:07.7&31:21:57&NGC~1333&SK-29&\citet{sandellknee01}&394&4.3\\ 
57&03:29:18.2&31:25:11&NGC~1333&SK-33&\citet{sandellknee01}&376&4.1\\ 
58&03:29:24.0&31:33:21&NGC~1333&None&&371&0.9\\ 
59&03:29:16.5&31:12:35&NGC~1333&None&&371&3.2\\ 
60&03:28:39.3&31:18:27&NGC~1333&None&&354&2.9\\ 
61&03:29:17.3&31:27:50&NGC~1333&None&&349&2.3\\ 
62&03:29:07.1&31:17:24&NGC~1333&SK-18&\citet{sandellknee01}&318&4.0\\ 
63&03:29:18.8&31:23:17&NGC~1333&SK-32&\citet{sandellknee01}&308&3.8\\ 
64&03:29:25.5&31:28:18&NGC~1333&None&&292&1.4\\ 
65&03:29:00.4&31:12:01&NGC~1333&SK-1&\citet{sandellknee01}&288&2.3\\ 
66&03:29:05.3&31:22:11&NGC~1333&SK-30&\citet{sandellknee01}&228&5.1\\ 
67&03:29:19.7&31:23:56&NGC~1333&None&&223&4.7\\ 
68&03:28:56.2&31:19:13&NGC~1333&No SMM/MM source&&201&3.9\\ 
69&03:28:34.4&31:06:59&NGC~1333&None&&201&1.3\\ 
70&03:29:15.3&31:20:31&NGC~1333&SK-22&\citet{sandellknee01}&192&4.2\\ 
71&03:28:38.7&31:05:57&NGC~1333&None&&177&1.9\\ 
72&03:29:19.1&31:11:38&NGC~1333&No SMM/MM source&&167&2.6\\ 
73&03:28:38.8&31:19:15&NGC~1333&None&&162&2.4\\ 
74&03:28:32.5&31:11:08&NGC~1333&None&&156&1.9\\ 
\hline
75&03:28:42.6&31:06:10&NGC~1333&None&&153&2.2\\ 
76&03:32:17.8&30:49:46&None&No SMM/MM source&&1916&1.7\\ 
77&03:31:21.0&30:45:28&None&I03282+3035 &\citet{bachiller94,motteandre01}&892&1.1\\ 
78&03:47:41.6&32:51:44&None$^{(5)}$&B5 IRS1&\citet{motteandre01}&424&?\\ 
79&03:47:39.1&32:52:18&None$^{(5)}$&None&&335&?\\ 
80&03:26:37.6&30:15:24&None&No SMM/MM source&&302&0.2\\ 
81&03:30:15.5&30:23:43&None&No SMM/MM source&&253&0.9\\ 
82&03:33:13.1&31:19:51&None&None&&219&2.4\\ 
83&03:32:48.9&31:09:40&None&None&&188&0.3\\ 
84&03:32:21.9&31:04:56&None$^{(6)}$&None&&184&0.2\\ 
85&03:28:32.5&31:00:53&None&03254+3050&\citet{dent98}&177&1.5\\ 
86&03:26:30.9&30:32:28&None&None&&176&1.5\\ 
87&03:32:21.5&31:05:08&None$^{(6)}$&None&&166&0.4\\ 
88&03:31:31.6&30:43:32&None&None&&165&2.2\\ 
89&03:32:25.9&30:59:05&None&None&&164&2.2\\ 
90&03:45:16.5&32:04:47&None&None&&163&0.8\\ 
91&03:29:23.3&31:36:08&None&None&&154&?\\ 
\hline
\noalign{\smallskip}
\multicolumn{8}{p{18.0cm}}{$^{(1)}$ If the core satisfies the
cluster membership criterion (Sect.~\ref{sect:clusters}) then the
cluster name is given here.}\\
\multicolumn{8}{p{18.0cm}}{$^{(2)}$ References are to the earliest
previous detection of the submillimetre source.   Full
cross-identifications with sources at other wavelengths are
non-trivial due to differing beam sizes and are left for a future
analysis, but to indicate an obvious likely counterpart (e.g., IRAS),
"No SMM/MM source'' is marked in the "Name'' column instead of "None''.}\\
\multicolumn{8}{p{18.0cm}}{$^{(3)}$ SCUBA 850~$\mu$m peak flux ($14''$ beam).}\\
\multicolumn{8}{p{18.0cm}}{$^{(4)}$ C$^{18}$O integrated intensity
($1'$ beam averaged) at the 850~$\mu$m peak.  A question mark in
this column indicates a SCUBA peak which lies outside the C$^{18}$O map.}\\
\multicolumn{8}{p{18.0cm}}{$^{(5)}$ B5 pair.}\\
\multicolumn{8}{p{18.0cm}}{$^{(6)}$ B1 west pair.}\\
\end{tabular}
\end{table}