\begin{table}
%\centering
\par
\caption{The XMM-Newton Catalogue of sources in the region of X1832-330.}
\label{sources}
\small\begin{tabular}[c]{ccccccccccccc}
\hline
(1) &  (2) & 	(3) &  (4) 	&  (5)			&  (6) & 	(7) & 	(8)		 & 	(9) & 	(10)			& 	(11) & 	(12)	&	(13)	\\
SRC 	&	Source name		&	ERR	& 	Rate 1			&	Rate 2			&	Rate 3			& 	Rate 4			& 	HR1			&	HR2			& 	Flux			&	OBS		&	VAR	&	CTP	\\
ID	&				& ($''$) & ($10^{-3}$~c~s$^{-1}$) & ($10^{-3}$~c~s$^{-1}$) ($10^{-3}$~c~s$^{-1}$)		& ($10^{-3}$~c~s$^{-1}$) &  &  & 	($10^{-14}$~cgs)	& & & \\ \hline
1	&	XMMU J183516.1-330602	&	1.02	&	2.85	$\pm$	0.18	&	4.42	$\pm$	0.21	&	1.77	$\pm$	0.14	&	0.22	$\pm$	0.09	&	0.22	$\pm$	0.04	&	--0.77	$\pm$	0.08	&	11.98	$\pm$	0.56	&	I, II, I+II	&	/	&	0; 0; 0	\\
2	&	XMMU J183619.4-330357	&	1.03	&	2.46	$\pm$	0.17	&	3.37	$\pm$	0.19	&	1.29	$\pm$	0.13	&	0.15	$\pm$	0.09	&	0.18	$\pm$	0.04	&	--0.85	$\pm$	0.09	&	10.45	$\pm$	0.53	&	I, II, I+II	&	/	&	1; 0; 1	\\
3	&	XMMU J183502.4-330257	&	1.03	&	1.47	$\pm$	0.13	&	3.52	$\pm$	0.19	&	2.09	$\pm$	0.15	&	0.31	$\pm$	0.10	&	0.42	$\pm$	0.04	&	--0.73	$\pm$	0.07	&	8.99	$\pm$	0.50	&	I, II, I+II	&	/	&	0; 0; 0	\\
4	&	XMMU J183546.9-330617	&	1.06	&	1.22	$\pm$	0.16	&	2.63	$\pm$	0.22	&	1.36	$\pm$	0.17	&	0.38	$\pm$	0.12	&	0.37	$\pm$	0.07	&	--0.57	$\pm$	0.11	&	7.23	$\pm$	0.57	&	I, II, I+II &	/	&	1; 0; 0	\\
5 & XMMU J183619.7-330714 &	1.05	&	2.37	$\pm$	0.18	&	2.66	$\pm$	0.19	&	0.38	$\pm$	0.09	& \textit{0.00	$\pm$	0.04}	&	0.06	$\pm$	0.05	&	--1.00$^{+0.09}_{-0.00}$	&	7.22	$\pm$	0.53	&	I, II, I+II &	/	&	0; 0; 0	\\
6	&	XMMU J183628.0-330001	&	1.10	&	0.07	$\pm$	0.06	&	1.26	$\pm$	0.14	&	1.54	$\pm$	0.15	&	1.14	$\pm$	0.17	&	0.90	$\pm$	0.08	&	--0.17	$\pm$	0.08	&	3.97	$\pm$	0.40	&	I, II, I+II &	/	&	1; 0; 0	\\
7 &	XMMU J183446.9-330143	&	1.19	&	0.55	$\pm$	0.12	&	1.00	$\pm$	0.13	&	0.93	$\pm$	0.13	& \textit{0.06	$\pm$	0.08}	&	0.31	$\pm$	0.11	&	-0.83	$\pm$	0.16	&	3.25	$\pm$ 0.41 & I, II, I+II	&	/	&	0; 2; 0	\\
8	&	XMMU J183613.6-330039	&	1.11	&	0.38	$\pm$	0.08	&	1.27	$\pm$	0.11	&	0.68	$\pm$	0.09	&	0.19	$\pm$	0.07	&	0.54	$\pm$	0.08	&	--0.56	$\pm$	0.14	&	2.93	$\pm$	0.30	&	I, II, I+II	&	/	&	0; 0; 0	\\ 
9	&	XMMU J183535.3-330808	&	1.14	&	0.84	$\pm$	0.15	&	1.24	$\pm$	0.17	&	0.93	$\pm$	0.15	&	0.23	$\pm$	0.12	&	0.19	$\pm$	0.11	&	--0.56	$\pm$	0.17	&	4.05	$\pm$	0.49	&	I, II, I+II	&	/	&	0;2;0	\\
10	&	XMMU J183515.5-330637	&	1.12	&	0.43	$\pm$	0.09	&	0.87	$\pm$	0.11	&	0.88	$\pm$	0.11	&	0.27	$\pm$	0.10	&	0.32	$\pm$	0.11	&	--0.52	$\pm$	0.13	&	2.99	$\pm$	0.34	&	I, II, I+II	&	/	&	0;0;0	\\
11	&	XMMU J183458.3-330548	&	1.17	&	0.58	$\pm$	0.12	&	0.83	$\pm$	0.13	&	0.35	$\pm$	0.10	& \textit{0.02	$\pm$	0.07}	&	0.17	$\pm$	0.13	&	--0.88$^{+0.35}_{-0.12}$	&	2.35	$\pm$	0.35	&	II, I+II		&	/	&	0; 1; 0	\\
12	&	XMMU J183509.6-325607	&	1.19	&	0.43	$\pm$	0.10	&	0.43	$\pm$	0.09	&	0.62	$\pm$	0.10	& \textit{0.02	$\pm$	0.05}	&	--0.04	$\pm$	0.15	&	--0.91$^{+0.16}_{-0.09}$	&	1.74	$\pm$	0.26	&	I,I+II		&	V	&	0;0;0	\\
13	&	XMMU J183536.7-325217	&	1.19	&	0.51	$\pm$	0.09	&	0.75	$\pm$	0.10	&	0.35	$\pm$	0.08	&	0.14	$\pm$	0.08	&	0.19	$\pm$	0.11	&	--0.43	$\pm$	0.24	&	2.35	$\pm$	0.30	&	I, II, I+II	&	/	&	0; 0; 0	\\
14	&	XMMU J183507.4-325911	&	1.18	&	0.16	$\pm$	0.06	&	0.54	$\pm$	0.08	&	0.51	$\pm$	0.08	& \textit{0.01	$\pm$	0.03}	&	0.55	$\pm$	0.14	&	--0.98$^{+0.11}_{-0.02}$	&	1.45	$\pm$	0.24	&	I, II, I+II	&	/	&	0;0;0	\\
15	&	XMMU J183526.9-325422	&	1.27	&	0.16	$\pm$	0.12	&	0.37	$\pm$	0.17	&	1.31	$\pm$	0.25	&	0.94	$\pm$	0.25	&	0.35	$\pm$	0.37	&	--0.17	$\pm$	0.16	&	3.46	$\pm$	0.68	&	I, I+II		&	/	&	0;0;0	\\
16	&	XMMU J183638.7-325144	&	1.27	&	1.49	$\pm$	0.30	&	1.57	$\pm$	0.30	&	0.98	$\pm$	0.28	& \textit{0.11	$\pm$	0.26}	&	0.08	$\pm$	0.13	&	--0.45	$\pm$	0.33	&	5.88	$\pm$	1.05	&	I, II, I+II	&	/	&	0; 0; 0	\\
17	&	XMMU J183526.1-330933	&	1.34	&	0.53	$\pm$	0.16	&	1.01	$\pm$	0.20	&	1.20	$\pm$	0.21	& \textit{0.13	$\pm$	0.13}	&	0.31	$\pm$	0.16	&	--0.81	$\pm$	0.17	&	3.11	$\pm$	0.49	&	I, I+II		&	V	&	0;1;0	\\
18	&	XMMU J183455.9-324948	&	1.31	&	0.79	$\pm$	0.17	&	0.64	$\pm$	0.16	&	0.66	$\pm$	0.15	&	0.20	$\pm$	0.18	&	-0.11	$\pm$	0.16	&	--0.53	$\pm$	0.33	&	2.79	$\pm$	0.46	&	I, I+II		&	/	&	0;0;0	\\
19	&	XMMU J183629.8-330208	&	1.28	&	0.46	$\pm$	0.12	&	0.43	$\pm$	0.11	&	0.66	$\pm$	0.13	&	0.30	$\pm$	0.14	&	--0.05	$\pm$	0.17	&	--0.34	$\pm$	0.21	&	1.88	$\pm$	0.33	&	II,I+II		&	/	&	0;0;0	\\
20	&	XMMU J183542.4-331107	&	1.29	&	1.14	$\pm$	0.22	&	1.07	$\pm$	0.20	&	0.31	$\pm$	0.14	&	0.61	$\pm$	0.24	&	0.00	$\pm$	0.13	&	0.28	$\pm$	0.26	&	3.02	$\pm$	0.51	&	I, I+II		&	/	&	1;0;0	\\
21	&	XMMU J183459.5-325430	&	1.46	&	0.30	$\pm$	0.12	&	0.52	$\pm$	0.13	&	0.42	$\pm$	0.13	&	0.23	$\pm$	0.15	&	0.26	$\pm$	0.22	&	--0.28	$\pm$	0.34	&	1.73	$\pm$	0.30	&	I+II		&	/	&	0;0;0	\\
22	&	XMMU J183632.8-330509	&	1.20	&	0.81	$\pm$	0.16	&	0.84	$\pm$	0.16	&	0.73	$\pm$	0.15	& \textit{0.06	$\pm$	0.11}	&	0.06	$\pm$	0.14	&	--0.76$^{+0.26}_{-0.24}$	&	2.61	$\pm$	0.43	&	I, I+II		&	V	&	1; 0; 1	\\
23	&	XMMU J183539.1-324747	&	1.90	&	0.82	$\pm$	0.20	&	0.66	$\pm$	0.18	& \textit{0.00	$\pm$	0.09}	& \textit{0.03	$\pm$	0.11}	&	--0.11	$\pm$	0.18	&	--			&	2.15	$\pm$	0.40	&	I+II		&	/	&	3; 0; 1	\\
24	&	XMMU J183450.7-325705	&	1.52	&	0.27	$\pm$	0.12	&	0.57	$\pm$	0.15	&	0.33	$\pm$	0.13	& \textit{0.13	$\pm$	0.15}	&	0.35	$\pm$	0.23	&	-0.44	$\pm$	0.48	&	1.57	$\pm$	0.31	&	I+II		&	/	&	0;2;0	\\
25	&	XMMU J183514.8-325354	&	1.27	&	0.36	$\pm$	0.10	&	0.47	$\pm$	0.11	&	0.62	$\pm$	0.12	&	0.14	$\pm$	0.11	&	0.11	$\pm$	0.18	&	--0.64	$\pm$	0.24	&	1.90	$\pm$	0.33	&	II, I+II &	/	&	0; 0; 0	\\
26	&	XMMU J183453.2-325851	&	1.27	&	0.75	$\pm$	0.12	&	0.40	$\pm$	0.10	& \textit{0.00	$\pm$	0.02}	& \textit{0.03	$\pm$	0.07}	&	--0.29	$\pm$	0.13	&	-			&	1.29	$\pm$	0.28	&	II, I+II		&	/	&	0; 0; 0	\\
27	&	XMMU J183611.0-330725	&	1.53	& \textit{0.00	$\pm$	0.04}	& \textit{0.11	$\pm$	0.11}	&	0.67	$\pm$	0.17	&	0.55	$\pm$	0.21	&	1.00$^{+0.00}_{-0.70}$	&	--0.10	$\pm$	0.23	&	1.34	$\pm$	0.32	&	I+II		&	/	&	0; 0; 0	\\
28	&	XMMU J183512.1-330324	&	1.18	&	0.74	$\pm$	0.10	&	0.43	$\pm$	0.08	&	0.11	$\pm$	0.05	&	0.11	$\pm$	0.06	&	--0.26	$\pm$	0.11	&	--0.03	$\pm$	0.37	&	1.70	$\pm$	0.26	&	I, II, I+II	&	/	&	0; 1; 1	\\
29	&	XMMU J183523.7-324836	&	1.68	&	0.91	$\pm$	0.20	&	0.35	$\pm$	0.13	& \textit{0.02	$\pm$	0.06}	& \textit{0.00	$\pm$	0.11}	&	--0.44	$\pm$	0.18	&	-			&	1.82	$\pm$	0.35	&	I+II		&	/	&	0;1;0	\\
30	&	XMMU J183448.4-330107	&	1.79	&	0.91	$\pm$	0.19	&	0.48	$\pm$	0.15	& \textit{0.00	$\pm$	0.04}	& \textit{0.09	$\pm$	0.14}	&	--0.30	$\pm$	0.17	&	-			&	1.68	$\pm$	0.34	&	I+II		&	/	&	0;0;0	\\
31	&	XMMU J183516.1-325724	&	1.31	&	0.29	$\pm$	0.09	&	0.44	$\pm$	0.10	&	0.34	$\pm$	0.09	& \textit{0.02	$\pm$	0.05}	&	0.21	$\pm$	0.19	&	--0.87$^{+0.24}_{-0.13}$	&	1.46	$\pm$	0.30	&	II, I+II		&	/	&	0; 2; 0	\\
32	&	XMMU J183514.1-325623	&	1.90	&	0.43	$\pm$	0.11	&	0.32	$\pm$	0.10	&	0.16	$\pm$	0.08	& \textit{0.00	$\pm$	0.05}	&	--0.15	$\pm$	0.20	&	--1.00$^{+0.58}_{-0.00}$	&	1.15	$\pm$	0.23	&	I+II		&	/	&	1; 1; 1	\\
33	&	XMMU J183541.1-325339	&	1.39	&	0.18	$\pm$	0.08	&	0.58	$\pm$	0.11	&	0.35	$\pm$	0.09	&	0.08	$\pm$	0.06	&	0.53	$\pm$	0.16	&	--0.55	$\pm$	0.23	&	1.22	$\pm$	0.24	&	I, I+II		&	V	&	1; 0; 0	\\
34	&	XMMU J183622.4-325338	&	1.69	&	0.22	$\pm$	0.12	&	0.63	$\pm$	0.17	&	0.38	$\pm$	0.14	& \textit{0.00	$\pm$	0.07}	&	0.48	$\pm$	0.23	&	--1.00$^{+0.38}_{-0.00}$	&	1.60	$\pm$	0.34	&	I+II		&	/	&	0;0;0	\\
35	&	XMMU J183630.2-330708	&	1.32	&	0.40	$\pm$	0.13	&	1.09	$\pm$	0.18	&	0.43	$\pm$	0.13	& \textit{0.01	$\pm$	0.06}	&	0.46	$\pm$	0.15	&	--0.93$^{+0.26}_{-0.07}$	&	2.32	$\pm$	0.41	&	I, I+II		&	/	&	0; 0; 0	\\ \hline
36	&	XMMU J183515.1-325016	&	1.83	&	0.97	$\pm$	0.19	& \textit{0.00	$\pm$	0.10}	& \textit{0.00	$\pm$	0.04}	& \textit{0.02	$\pm$	0.10}	&	--1.00$^{+0.20}_{-0.00}$	&	--			&	1.39	$\pm$	0.33	&	I+II	&	/	&	2;5;1	\\
37	&	XMMU J183628.7-330409	&	1.36	&	0.60	$\pm$	0.13	&	0.65	$\pm$	0.13	&	0.30	$\pm$	0.10	&	0.19	$\pm$	0.15	&	0.04	$\pm$	0.14	&	--0.04	$\pm$	0.38	&	1.75	$\pm$	0.34	&	II, I+II	&	$V$	&	0; 0; 0	\\
38	&	XMMU J183442.8-325840	&	2.01	&	0.26	$\pm$	0.14	&	0.62	$\pm$	0.17	&	0.46	$\pm$	0.16	& \textit{0.06	$\pm$	0.13}	&	0.40	$\pm$	0.25	&	--0.75$^{+0.45}_{-0.25}$	&	1.74	$\pm$	0.37	&	I+II	&	/	&	1;2;1	\\
39	&	XMMU J183614.3-325949	&	1.71	&	0.10	$\pm$	0.08	&	0.40	$\pm$	0.11	&	0.21	$\pm$	0.09	&	0.12	$\pm$	0.10	&	0.61	$\pm$	0.28	&	--0.26	$\pm$	0.44	&	1.11	$\pm$	0.23	&	I+II	&	/	&	1; 0; 0	\\
40	&	XMMU J183538.4-324701	&	1.99	&	0.35	$\pm$	0.18	&	0.60	$\pm$	0.17	&	0.23	$\pm$	0.14	&	0.28	$\pm$	0.24	&	0.27	$\pm$	0.28	&	0.11	$\pm$	0.52	&	2.17	$\pm$	0.44	&	I+II	&	/	&	0; 0; 0	\\
41	&	XMMU J183548.1-331137	&	1.78	& \textit{0.17	$\pm$	0.20}	&	1.06	$\pm$	0.32	&	0.92	$\pm$	0.33	&	0.69	$\pm$	0.40	&	0.73$^{+0.27}_{-0.29}$	&	--0.15	$\pm$	0.33	&	3.04	$\pm$	0.69	&	I+II	&	/	&	0;0;0	\\
42	&	XMMU J183538.5-325139	&	1.74	&	0.82	$\pm$	0.23	& \textit{0.07	$\pm$	0.11}	&	0.29	$\pm$	0.15	& \textit{0.13	$\pm$	0.15}	&	--0.83$^{+0.23}_{-0.17}$	&	--0.39	$\pm$	0.56	&	1.89	$\pm$	0.42	&	I	&	V	&	0; 0; 1	\\
43	&	XMMU J183512.8-324755	&	1.66	&	1.83	$\pm$	0.50	& \textit{0.15	$\pm$	0.23}	& \textit{0.19	$\pm$	0.26}	& \textit{0.00	$\pm$	0.19}	&	--0.85$^{+0.22}_{-0.15}$	&	--			&	3.81	$\pm$	0.93	&	$I$	&	$V$	&	0; 0; 0	\\
44	&	XMMU J183529.7-324734	&	2.34	&	1.19	$\pm$	0.36	& \textit{0.18	$\pm$	0.19}	& \textit{0.08	$\pm$	0.15}	& \textit{0.04	$\pm$	0.19}	&	--0.74	$\pm$	0.24	&	--			&	2.78	$\pm$	0.66	&	I	&	V	&	3; 3; 1	\\
45	&	XMMU J183632.9-325653	&	1.61	&	0.71	$\pm$	0.22	&	0.76	$\pm$	0.24	& \textit{0.15	$\pm$	0.16}	& \textit{0.00	$\pm$	0.07}	&	0.04	$\pm$	0.22	&	--			&	2.13	$\pm$	0.49	&	II	&	V	&	0;0;0	\\
46	&	XMMU J183515.9-324703	&	2.11	&	1.31	$\pm$	0.49	&	0.61	$\pm$	0.37	& \textit{0.06	$\pm$	0.18}	&	1.24	$\pm$	0.66	&	--0.36	$\pm$	0.31	&	0.91$^{+0.09}_{-0.27}$	&	4.74	$\pm$	1.10	&	II	&	/	&	0; 1; 0	\\ \hline
\end{tabular}
\medskip
Key to table:\\
Column~(1) = Source ID number; Col.~(2) = source XMM name; Col.~(3) = position error; Cols.~(4)--(7) = MOS1+MOS2 count rates in the energy ranges 0.5--1, 1--2, 2--5, and 4 = 5--10~keV, respectively (rates consistent with false detections are reported in italic); Cols.~(8),(9) = count rate hardness ratios, defined as HR1 = (2--1)/(2+1) and HR2 = (4--3)/(4+3) (values are omitted when in both energy ranges the measured count rates are consistent with a false detection); Col.~(10) = flux in the 0.5--10~keV energy range, in units of 10$^{-14}$~erg~cm$^{-2}$~s$^{-1}$, calculated as reported in the text; Col.~(11) = XMM observation with a positive source detection; Col.~(12) = flag indicating a source variability; Col.~(13) = number of GSC, USNO--NOMAD and 2MASS counterparts, respectively, found considering a circular uncertainty region with a radius of three times the source position error.
\end{table}