\begin{table} %t5
\caption{\label{tbl:msx_ps}The properties of MSX~point sources associated with the BRC sample.} 
\small%\centerline
{
\begin{tabular}{lccccccccc}
 \hline \hline & & & &   &\multicolumn{4}{c}{Mid-infrared fluxes} &
\\ \cline{6-9} SFO~Id. & MSX~name & RA & Dec &  \multicolumn{1}{c}{Offset} & \multicolumn{1}{c}{8
$\mu$m} & \multicolumn{1}{c}{12 $\mu$m}& \multicolumn{1}{c}{14 $\mu$m}& \multicolumn{1}{c}{21
$\mu$m} & Quality flag$^a$\\
&			&	(J2000)&(J2000)	   &  \multicolumn{1}{c}{(\arcsec)} & 
\multicolumn{1}{c}{(Jy)}&  \multicolumn{1}{c}{(Jy)}&  \multicolumn{1}{c}{(Jy)}& 
\multicolumn{1}{c}{(Jy)}& \\
\hline
 47&G234.7617$-$00.2766& 07:31:49.0&  $-$19:27:34.2& 1.3	&2.5  & 3.5   &3.4	&11.9   &4444 
\\ 49&G234.6358+00.8281& 07:35:38.9&  $-$18:48:50.4& 27.0  &3.4  & 4.6   &3.3	&27.2   &4444\\
51&G253.2934$-$01.6114& 08:09:33.1&  $-$36:04:59.5& 3.8	&0.5  & 0.9   &1.2	&2.3    &4121\\
54&G259.9395$-$00.0419& 08:35:31.0&  $-$40:38:25.8& 8.5	&0.5  & 1.1   &3.4	&30.0   &4444\\
55&G260.7658+00.6604& 08:41:06.7&  $-$40:52:16.7& 72.4  &1.5  & 2.3   &1.9	&3.4    &4443\\
60&G268.0574$-$00.9515& 09:00:01.2&  $-$47:31:46.2& 9.4	&2.8  & 5.8   &2.3	&7.2    &4444\\
64&G290.3745+01.6615& 11:12:18.2&  $-$58:46:19.9& 2.0	&0.8  & 2.8   &10.0  &51.2   &4444\\
65&G294.2815$-$01.9124& 11:32:48.7&  $-$63:27:21.6 & 56.9  &0.2  & \multicolumn{1}{c}{$-$0.7}  &1.1	&4.2
&3023\\ 68&G294.5117$-$01.6205& 11:35:32.4&  $-$63:14:41.3& 10.4  &0.8  & 1.3   &2.5	&13.9   &4244\\
69&G295.1622$-$01.5825& 11:41:11.8&  $-$63:23:23.3& 11.1  &--0.0 & \multicolumn{1}{c}{$-$0.6}  &0.9	&2.8
&0022\\ 
71&G304.8872+00.6356& 13:08:12.2&  $-$62:10:21.0& 6.2	&0.1  & \multicolumn{1}{c}{$-$0.6} 
&1.1	&5.2    &1024\\ 
72&G306.1160+00.1386& 13:19:07.9&  $-$62:33:42.8& 1.9	&3.1  & 4.6  
&5.5	&10.1   &4444\\ 
74&G313.2850$-$00.3350& 14:19:42.0&  $-$61:25:12.0  & 5.0	&0.5  & 1.7  
&2.1	&8.5    &4344\\ 
75&G327.5761$-$00.8497& 15:55:50.6&  $-$54:38:47.4& 10.7  &4.6  & 5.9  
&2.3	&7.1    &4444\\ 
76&G332.9565+01.8035& 16:10:38.6&  $-$49:05:52.1& 1.0	&6.2  & 10.0 
&9.3	&22.4   &4444\\ 
79&G336.4917$-$01.4741& 16:40:00.0    & $-$48:51:41.4 &3.7    &58.2 & 147.3
&264.2 &1796.3 &4444\\
80&G336.6568$-$01.4099& 16:40:22.6&  $-$48:41:43.4& 69.1  &0.1  &
\multicolumn{1}{c}{$-$0.6}  &1.1	&4.7    &1023\\ 82&G343.0500+02.6094& 16:46:53.5&  $-$41:13:59.5& 39.6
&2.1  & 2.3   &1.5	&4.1    &4433\\ 85&G343.3516$-$00.0786& 16:59:07.0&  $-$42:42:07.2& 5.8	&74.4 &
75.4  &46.3  &119.0  &4444\\ 
\hline 
\end{tabular} }
\smallskip
$^a$ Each of the four numbers (starting on the left) are associated with the  the 8, 12, 14 and 21~\mum\ flux values and indicate the quality of each flux value as follows: 0 = not detected, 1 = upper-limit, 2 = fair, 3 = good, 4 = excellent. 
\end{table}