\begin{table}%t5
\caption{\label{tbl:rms_radio}Parameters for radio sources found to be associated with RMS sources. }
\par
%
\par
%\centerline
 {
\begin{tabular}{llcrrrrlc}
\hline
\hline
RMS Name &Radio Name$^a$	& Offset &	RA	&	Dec	&	Peak 	&	Integrated	&	Source	&	Classification$^a$ 	\\
& & (\arcsec)	&	(J2000)	&	(J2000)	&	(mJy) 	&	(mJy)	&	Size (\arcsec)	&		\\
\hline
G010.4413+00.0101	&	G10.440+0.011$^\dagger$	&	4.4	&	18:08:37.93	&	$-$19:53:58.9	&	7.5	&	32.5	&	13.1 $\times$ 8.1	&	HII region	\\
G010.5975$-$00.3838	&	G10.598$-$0.384$^\dagger$	&	0.6	&	18:10:25.59	&	$-$19:57:11.0	&	66.1	&	136.6	&	7.7 $\times$ 4.7	&	HII region	\\
	&	G10.597$-$0.383$^\dagger$	&	6.0	&	18:10:25.13	&	$-$19:57:12.2	&	52.0	&	105.6	&	12.6 $\times$ 2.4	&	HII region	\\
	&	G10.601$-$0.384$^\dagger$	&	11.8	&	18:10:26.03	&	$-$19:57:01.8	&	32.9	&	78.9	&	12.5 $\times$ 4.0	&	HII region	\\
G010.6291$-$00.3385	&	G10.629$-$0.338$^\dagger$	&	1.2	&	18:10:19.25	&	$-$19:54:12.1	&	18.1	&	25.2	&	4.6 $\times$ 2.9	&	HII region	\\
G010.9592+00.0217	&	G10.959+0.022$^\dagger$	&	3.2	&	18:09:39.35	&	$-$19:26:26.9	&	178.7	&	195.0	&	2.2 $\times$ 1.0	&	HII region	\\
G010.9657+00.0083	&	G10.967+0.009$^\dagger$	&	3.6	&	18:09:43.31	&	$-$19:26:25.1	&	16.4	&	68.7	&	12.3 $\times$ 7.9	&	HII region	\\
	&	G10.965+0.010$^\dagger$	&	5.9	&	18:09:42.95	&	$-$19:26:27.8	&	34.2	&	63.8	&	5.9 $\times$ 4.7	&	HII region	\\
	&	G10.965+0.006$^\dagger$	&	8.3	&	18:09:43.64	&	$-$19:26:36.0	&	19.8	&	74.8	&	13.0 $\times$ 6.6	&	HII region	\\
G011.1109$-$00.4001	&	G11.111$-$0.400$^\dagger$	&	0.3	&	18:11:32.30	&	$-$19:30:40.7	&	18.2	&	50.0	&	9.9 $\times$ 3.4	&	HII region	\\
	&	G11.111$-$0.399$^\dagger$	&	6.0	&	18:11:31.88	&	$-$19:30:38.5	&	96.7	&	111.9	&	3.7 $\times$ 1.2	&	HII region	\\
G011.1723$-$00.0656	&	G11.172$-$0.065$^\dagger$	&	3.4	&	18:10:24.98	&	$-$19:17:46.1	&	23.5	&	71.0	&	9.8 $\times$ 6.9	&	HII region	\\
G011.4201$-$01.6815	&	G011.4201$-$01.6819	&	1.1	&	18:16:56.89	&	$-$19:51:08.1	&	0.8	&	3.2	&	1.9 $\times$ 1.5	&	HII/YSO	\\
G011.9454$-$00.0373	&	G11.946$-$0.036$^\dagger$	&	5.1	&	18:11:53.22	&	$-$18:36:14.6	&	70.2	&	623.4	&	18.3 $\times$ 14.9	&	HII region	\\
	&	G11.944$-$0.037$^\dagger$	&	5.1	&	18:11:53.20	&	$-$18:36:21.8	&	271.6	&	453.4	&	4.7 $\times$ 3.9	&	HII region	\\
G012.1177+01.1966	&	G012.1175+01.1965	&	1.2	&	18:07:41.54	&	$-$17:51:28.9	&	32.2	&	63.6	&	1.9 $\times$ 1.5	&	PN	\\
G012.1917$-$00.1029	&	G12.192$-$0.103$^\dagger$	&	1.0	&	18:12:37.95	&	$-$18:25:15.0	&	21.3	&	119.6	&	18.6 $\times$ 7.2	&	HII region	\\
	&	G12.191$-$0.101$^\dagger$	&	7.3	&	18:12:37.48	&	$-$18:25:13.3	&	9.5	&	30.1	&	12.4 $\times$ 5.7	&	HII region	\\
G012.1993$-$00.0342	&	G12.199$-$0.034$^\dagger$	&	3.0	&	18:12:23.59	&	$-$18:22:54.4	&	54.3	&	60.1	&	1.8 $\times$ 1.3	&	HII/YSO	\\
G012.4314$-$01.1117	&	G012.4317$-$01.1112	&	2.2	&	18:16:51.23	&	$-$18:41:28.4	&	8.1	&	105.2	&	3.7 $\times$ 3.1	&	HII region	\\
G012.8062$-$00.1987	&	G12.805$-$0.200$^\dagger$	&	5.3	&	18:14:13.74	&	$-$17:55:42.1	&	1748.5	&	6290.8	&	12.6 $\times$ 4.6	&	HII region	\\
G013.2097$-$00.1436	&	G13.210$-$0.144$^\dagger$	&	2.4	&	18:14:50.05	&	$-$17:32:44.7	&	317.5	&	1017.0	&	9.1 $\times$ 7.8	&	HII region	\\
G014.1742+00.0226	&	G14.175+0.024$^\dagger$	&	3.9	&	18:16:08.53	&	$-$16:37:06.1	&	21.2	&	96.4	&	11.6 $\times$ 10.0	&	HII region	\\
G014.2071$-$00.1105	&	G14.207$-$0.110$^\dagger$	&	3.3	&	18:16:41.75	&	$-$16:39:12.1	&	11.4	&	60.0	&	13.1 $\times$ 11.1	&	HII region	\\
G014.2361+00.2138	&	G14.237+0.212$^\dagger$	&	7.0	&	18:15:34.45	&	$-$16:28:27.1	&	30.2	&	35.5	&	2.3 $\times$ 2.2	&	PN	\\
\hline
\end{tabular}}
\medskip
$^a$ Matches identified from the \cite{white2005} catalogue are identified by a superscript $\dagger$ added to the end of the source's radio name.
\par
$^b$ RMS sources have been give one of five difference classifications: HII region, PN, YSO, HII/YSO and Other. The first three of these are obvious, however, the last two require a little explanation. The HII/YSO classification is give to MSX sources that appear to be associated with both an HII region and a YSO. The classification ``Other'' is given to sources that do not fit into any of the other classification. 
\par
Notes: Only a small portion of the data is provided here, the full table is available in electronic form at the CDS.
\end{table}