Table 1: XMM-Newton sources detected within the half mass radius. A flag indicates whether the source belongs to the core. Most sources were detected by the most sensitive EPIC-PN camera (a flag indicates whether it is detected also by MOS1 and MOS2). The ones which were missed by EPIC-PN are labeled as MOS in that table. The source ID increases with decreasing maximum likelihood. The sources are sorted in declination. The statistical error on the position is given at the 90% confidence level, as estimated from the srcmatch task, and is given in arcseconds. For PN sources, the rates are from the PN data. For MOS sources, the rates are an average between the MOS1 and MOS2 cameras. All rates are corrected for the vignetting of the mirrors and are given in units of 10^-2 count s^-1. In EPIC-PN, for indications a count rate of 10^-2 counts s^-1 corresponds to an unabsorbed flux of $\sim$ $2.7\times 10^{-14}$ ergs s^-1 cm^-2 for a 0.6 keV blackbody model absorbed through the cluster $N_{\rm H}$ ( $8.4\times 10^{20}$ cm^-2). This flux translates to a luminosity of $\sim$ 10³² ergs s^-1 at the distance of $\omega$ Cen (5.3 kpc).
Instrument Source RA Dec Position Rate MOS1 MOS2 Core

ID h m s $\hbox{$^\circ$ }$ $\hbox{$^\prime$ }$ $\hbox{$^{\prime\prime}$ }$ Error ( $^{\prime\prime}$ ) detection detection source

PN 122 13: 26: 48.9 -47: 24: 52.2 7.32 0.13 $\pm$ 0.03 No No No

PN 80 13: 26: 30.7 -47: 26: 04.4 4.76 0.14 $\pm$ 0.03 Yes No No

PN 49 13: 26: 28.7 -47: 26: 33.3 5.28 0.15 $\pm$ 0.03 No Yes No

PN 103 13: 26: 45.4 -47: 26: 53.6 4.92 0.15 $\pm$ 0.03 No No Yes

PN 44 13: 26: 52.6 -47: 27: 15.9 3.89 0.25 $\pm$ 0.04 Yes Yes Yes

PN 24 13: 26: 40.8 -47: 27: 38.6 2.35 0.54 $\pm$ 0.05 Yes Yes Yes

PN 61 13: 26: 52.5 -47: 27: 39.1 4.08 0.18 $\pm$ 0.03 Yes Yes Yes

PN 42 13: 26: 59.2 -47: 28: 16.5 4.41 0.35 $\pm$ 0.04 Yes Yes Yes

PN 111 13: 26: 50.2 -47: 28: 40.1 4.47 0.14 $\pm$ 0.03 No No Yes

PN 92 13: 26: 44.3 -47: 28: 57.4 4.89 0.17 $\pm$ 0.03 No No Yes

PN 5 13: 26: 53.5 -47: 29: 01.3 1.17 1.74 $\pm$ 0.08 Yes Yes Yes

PN 101 13: 26: 37.9 -47: 29: 11.3 5.06 0.16 $\pm$ 0.03 No No Yes

PN 2 13: 26: 52.2 -47: 29: 36.1 0.74 3.56 $\pm$ 0.11 Yes Yes Yes

PN 72 13: 26: 34.5 -47: 29: 57.3 3.84 0.25 $\pm$ 0.04 No No Yes

PN 60 13: 26: 34.2 -47: 30: 34.7 4.08 0.25 $\pm$ 0.04 Yes No No

PN 127 13: 27: 04.5 -47: 30: 38.2 5.43 0.12 $\pm$ 0.03 No No No

PN 20 13: 26: 37.4 -47: 30: 52.9 2.32 0.53 $\pm$ 0.05 Yes Yes No

PN 88 13: 27: 04.9 -47: 31: 10.2 6.88 0.13 $\pm$ 0.03 Yes No No

PN 38 13: 26: 55.0 -47: 31: 13.2 3.73 0.29 $\pm$ 0.04 Yes Yes No

PN 9 13: 26: 48.7 -47: 31: 26.2 1.72 1.46 $\pm$ 0.10 Yes Yes No

PN 108 13: 26: 46.6 -47: 31: 40.5 5.79 0.16 $\pm$ 0.03 No No No

PN 36 13: 26: 50.8 -47: 31: 47.5 3.91 0.33 $\pm$ 0.04 Yes Yes No

PN 35 13: 26: 49.6 -47: 31: 53.2 7.26 0.17 $\pm$ 0.03 Yes Yes No

PN 57 13: 26: 49.6 -47: 32: 13.4 2.95 0.35 $\pm$ 0.05 No No No

PN 16 13: 26: 43.9 -47: 32: 31.0 2.71 0.68 $\pm$ 0.07 Yes Yes No

MOS 96 13: 26: 47.7 -47: 25: 52.6 4.71 0.05 $\pm$ 0.02 Yes Yes No

MOS 50 13: 26: 29.2 -47: 28: 13.8 2.99 0.13 $\pm$ 0.02 Yes Yes No

**Table 1:** XMM-Newton sources detected within the half mass radius. A flag indicates whether the source belongs to the core. Most sources were detected by the most sensitive EPIC-PN camera (a flag indicates whether it is detected also by MOS1 and MOS2). The ones which were missed by EPIC-PN are labeled as MOS in that table. The source ID increases with decreasing maximum likelihood. The sources are sorted in declination. The statistical error on the position is given at the 90% confidence level, as estimated from the *srcmatch* task, and is given in arcseconds. For PN sources, the rates are from the PN data. For MOS sources, the rates are an average between the MOS1 and MOS2 cameras. All rates are corrected for the vignetting of the mirrors and are given in units of 10^-2 count s^-1. In EPIC-PN, for indications a count rate of 10^-2 counts s^-1 corresponds to an unabsorbed flux of $\sim$ $2.7\times 10^{-14}$ ergs s^-1 cm^-2 for a 0.6 keV blackbody model absorbed through the cluster $N_{\rm H}$ ( $8.4\times 10^{20}$ cm^-2). This flux translates to a luminosity of $\sim$ 10³² ergs s^-1 at the distance of $\omega$ Cen (5.3 kpc).
Instrument	Source	RA	Dec	Position	Rate	MOS1	MOS2	Core
	ID	h m s	$\hbox{$^\circ$ }$ $\hbox{$^\prime$ }$ $\hbox{$^{\prime\prime}$ }$	Error ( $^{\prime\prime}$ )		detection	detection	source
PN	122	13: 26: 48.9	-47: 24: 52.2	7.32	0.13 $\pm$ 0.03	No	No	No
PN	80	13: 26: 30.7	-47: 26: 04.4	4.76	0.14 $\pm$ 0.03	Yes	No	No
PN	49	13: 26: 28.7	-47: 26: 33.3	5.28	0.15 $\pm$ 0.03	No	Yes	No
PN	103	13: 26: 45.4	-47: 26: 53.6	4.92	0.15 $\pm$ 0.03	No	No	Yes
PN	44	13: 26: 52.6	-47: 27: 15.9	3.89	0.25 $\pm$ 0.04	Yes	Yes	Yes
PN	24	13: 26: 40.8	-47: 27: 38.6	2.35	0.54 $\pm$ 0.05	Yes	Yes	Yes
PN	61	13: 26: 52.5	-47: 27: 39.1	4.08	0.18 $\pm$ 0.03	Yes	Yes	Yes
PN	42	13: 26: 59.2	-47: 28: 16.5	4.41	0.35 $\pm$ 0.04	Yes	Yes	Yes
PN	111	13: 26: 50.2	-47: 28: 40.1	4.47	0.14 $\pm$ 0.03	No	No	Yes
PN	92	13: 26: 44.3	-47: 28: 57.4	4.89	0.17 $\pm$ 0.03	No	No	Yes
PN	5	13: 26: 53.5	-47: 29: 01.3	1.17	1.74 $\pm$ 0.08	Yes	Yes	Yes
PN	101	13: 26: 37.9	-47: 29: 11.3	5.06	0.16 $\pm$ 0.03	No	No	Yes
PN	2	13: 26: 52.2	-47: 29: 36.1	0.74	3.56 $\pm$ 0.11	Yes	Yes	Yes
PN	72	13: 26: 34.5	-47: 29: 57.3	3.84	0.25 $\pm$ 0.04	No	No	Yes
PN	60	13: 26: 34.2	-47: 30: 34.7	4.08	0.25 $\pm$ 0.04	Yes	No	No
PN	127	13: 27: 04.5	-47: 30: 38.2	5.43	0.12 $\pm$ 0.03	No	No	No
PN	20	13: 26: 37.4	-47: 30: 52.9	2.32	0.53 $\pm$ 0.05	Yes	Yes	No
PN	88	13: 27: 04.9	-47: 31: 10.2	6.88	0.13 $\pm$ 0.03	Yes	No	No
PN	38	13: 26: 55.0	-47: 31: 13.2	3.73	0.29 $\pm$ 0.04	Yes	Yes	No
PN	9	13: 26: 48.7	-47: 31: 26.2	1.72	1.46 $\pm$ 0.10	Yes	Yes	No
PN	108	13: 26: 46.6	-47: 31: 40.5	5.79	0.16 $\pm$ 0.03	No	No	No
PN	36	13: 26: 50.8	-47: 31: 47.5	3.91	0.33 $\pm$ 0.04	Yes	Yes	No
PN	35	13: 26: 49.6	-47: 31: 53.2	7.26	0.17 $\pm$ 0.03	Yes	Yes	No
PN	57	13: 26: 49.6	-47: 32: 13.4	2.95	0.35 $\pm$ 0.05	No	No	No
PN	16	13: 26: 43.9	-47: 32: 31.0	2.71	0.68 $\pm$ 0.07	Yes	Yes	No
MOS	96	13: 26: 47.7	-47: 25: 52.6	4.71	0.05 $\pm$ 0.02	Yes	Yes	No
MOS	50	13: 26: 29.2	-47: 28: 13.8	2.99	0.13 $\pm$ 0.02	Yes	Yes	No

Table 2: XMM-Newton sources detected outside the half mass radius. As in Table 1 most sources were detected by the most sensitive EPIC-PN camera (a flag indicates whether it is detected also by MOS1 and MOS2). The ones which were missed by EPIC-PN are labeled as MOS in that table. The source ID increases with decreasing maximum likelihood. The sources are sorted in declination. The statistical error on the position is given at the 90% confidence level, as estimated from the srcmatch task and is given in arcseconds. For PN sources, the rates are from the PN data. For MOS sources, the rates are an average between the MOS1 and MOS2 cameras. All rates are corrected for the vignetting of the mirrors and are given in units of 10^-2 count s^-1. In EPIC-PN, for indications a count rate of 10^-2 counts s^-1 corresponds to an unabsorbed flux of $\sim$ $2.7\times 10^{-14}$ ergs s^-1 cm^-2 for a 0.6 keV blackbody model absorbed through the cluster $N_{\rm H}$ ( $8.4\times 10^{20}$ cm^-2). This flux translates to a luminosity of $\sim$ 10³² ergs s^-1 at the distance of $\omega$ Cen (5.3 kpc).
Instrument Source RA Dec Position Rate MOS1 MOS2

ID h m s $\hbox{$^\circ$ }$ $\hbox{$^\prime$ }$ $\hbox{$^{\prime\prime}$ }$ Error ( $^{\prime\prime}$ ) detection detection

PN 119 13: 26: 37.8 -47: 16: 00.8 7.59 0.31 $\pm$ 0.06 No No

PN 54 13: 26: 56.4 -47: 17: 15.4 3.77 0.53 $\pm$ 0.07 No Yes

PN 65 13: 26: 18.3 -47: 17: 28.6 5.31 0.43 $\pm$ 0.07 Yes Yes

PN 29 13: 26: 53.3 -47: 18: 24.4 3.60 0.63 $\pm$ 0.07 Yes Yes

PN 97 13: 27: 05.8 -47: 18: 35.1 5.02 0.30 $\pm$ 0.05 No No

PN 132 13: 26: 31.0 -47: 18: 48.5 26.59 0.21 $\pm$ 0.05 No No

PN 3 13: 27: 27.7 -47: 19: 08.8 0.83 7.39 $\pm$ 0.24 Yes Yes

PN 17 13: 26: 23.5 -47: 19: 27.9 3.00 0.89 $\pm$ 0.08 Yes Yes

PN 56 13: 27: 02.8 -47: 19: 29.9 5.59 0.38 $\pm$ 0.06 Yes Yes

PN 28 13: 26: 46.3 -47: 19: 47.4 2.64 0.80 $\pm$ 0.07 Yes Yes

PN 31 13: 26: 38.5 -47: 20: 01.7 2.43 0.66 $\pm$ 0.07 Yes Yes

PN 95 13: 27: 08.4 -47: 20: 25.9 7.41 0.16 $\pm$ 0.04 Yes No

PN 43 13: 26: 03.8 -47: 20: 42.9 3.86 0.54 $\pm$ 0.07 Yes Yes

PN 73 13: 26: 35.7 -47: 20: 57.4 9.14 0.26 $\pm$ 0.05 No Yes

PN 68 13: 27: 10.2 -47: 21: 29.2 4.06 0.31 $\pm$ 0.05 Yes No

PN 145 13: 28: 08.7 -47: 21: 36.8 48.16 0.54 $\pm$ 0.09 No No

PN 133 13: 27: 58.4 -47: 22: 03.6 24.29 0.30 $\pm$ 0.06 No No

PN 32 13: 26: 54.5 -47: 22: 04.7 2.73 0.46 $\pm$ 0.06 Yes Yes

PN 15 13: 26: 41.5 -47: 22: 16.5 2.34 0.66 $\pm$ 0.06 Yes Yes

PN 77 13: 26: 48.6 -47: 22: 18.7 4.95 0.15 $\pm$ 0.03 No Yes

PN 129 13: 27: 33.3 -47: 22: 48.1 6.29 0.18 $\pm$ 0.04 No No

PN 39 13: 26: 23.2 -47: 22: 52.7 2.70 0.52 $\pm$ 0.06 Yes No

PN 70 13: 28: 01.9 -47: 23: 16.5 4.68 0.68 $\pm$ 0.09 No No

PN 18 13: 27: 21.2 -47: 23: 24.4 1.92 0.92 $\pm$ 0.08 Yes Yes

PN 41 13: 27: 07.9 -47: 23: 35.3 3.28 0.42 $\pm$ 0.05 Yes Yes

PN 99 13: 25: 51.0 -47: 23: 40.6 5.60 0.33 $\pm$ 0.06 No No

PN 118 13: 26: 27.3 -47: 24: 00.2 17.34 0.20 $\pm$ 0.04 No No

PN 67 13: 26: 41.3 -47: 24: 05.0 6.67 0.17 $\pm$ 0.03 Yes Yes

PN 79 13: 26: 12.8 -47: 24: 16.6 5.92 0.19 $\pm$ 0.04 No Yes

PN 110 13: 27: 12.1 -47: 24: 22.9 5.66 0.17 $\pm$ 0.04 No No

PN 94 13: 27: 28.5 -47: 24: 25.2 4.86 0.23 $\pm$ 0.04 No No

PN 126 13: 26: 37.0 -47: 24: 30.5 6.26 0.12 $\pm$ 0.03 No No

PN 59 13: 26: 31.4 -47: 24: 43.6 5.14 0.24 $\pm$ 0.04 Yes Yes

PN 86 13: 27: 57.9 -47: 25: 12.0 6.47 0.29 $\pm$ 0.06 No Yes

PN 75 13: 25: 39.7 -47: 25: 23.4 6.02 0.35 $\pm$ 0.06 No Yes

PN 82 13: 27: 06.3 -47: 25: 37.8 7.52 0.17 $\pm$ 0.03 No Yes

PN 106 13: 25: 44.8 -47: 25: 54.7 7.58 0.31 $\pm$ 0.06 No No

PN 6 13: 27: 29.4 -47: 25: 55.4 1.18 2.35 $\pm$ 0.11 Yes Yes

PN 146 13: 27: 39.3 -47: 25: 57.1 7.76 0.15 $\pm$ 0.04 No No

PN 144 13: 27: 59.4 -47: 26: 09.5 7.58 0.22 $\pm$ 0.05 No No

PN 26 13: 25: 55.9 -47: 26: 19.6 2.53 0.85 $\pm$ 0.08 Yes Yes

PN 131 13: 25: 42.3 -47: 26: 36.1 9.30 0.25 $\pm$ 0.05 No No

PN 105 13: 25: 51.3 -47: 26: 44.9 5.92 0.26 $\pm$ 0.05 No No

PN 115 13: 26: 21.3 -47: 27: 08.2 4.93 0.14 $\pm$ 0.03 No No

PN 138 13: 25: 58.0 -47: 27: 32.0 6.95 0.16 $\pm$ 0.04 No No

PN 135 13: 25: 32.6 -47: 27: 37.8 8.22 0.25 $\pm$ 0.06 No No

PN 76 13: 26: 04.2 -47: 27: 41.6 7.24 0.15 $\pm$ 0.04 No Yes

PN 140 13: 27: 48.5 -47: 28: 01.0 47.60 0.20 $\pm$ 0.04 No No

PN 102 13: 27: 17.0 -47: 28: 18.7 5.41 0.12 $\pm$ 0.03 Yes No

PN 136 13: 26: 00.8 -47: 28: 21.5 10.83 0.17 $\pm$ 0.04 No No

**Table 2:** XMM-Newton sources detected outside the half mass radius. As in Table 1 most sources were detected by the most sensitive EPIC-PN camera (a flag indicates whether it is detected also by MOS1 and MOS2). The ones which were missed by EPIC-PN are labeled as MOS in that table. The source ID increases with decreasing maximum likelihood. The sources are sorted in declination. The statistical error on the position is given at the 90% confidence level, as estimated from the *srcmatch* task and is given in arcseconds. For PN sources, the rates are from the PN data. For MOS sources, the rates are an average between the MOS1 and MOS2 cameras. All rates are corrected for the vignetting of the mirrors and are given in units of 10^-2 count s^-1. In EPIC-PN, for indications a count rate of 10^-2 counts s^-1 corresponds to an unabsorbed flux of $\sim$ $2.7\times 10^{-14}$ ergs s^-1 cm^-2 for a 0.6 keV blackbody model absorbed through the cluster $N_{\rm H}$ ( $8.4\times 10^{20}$ cm^-2). This flux translates to a luminosity of $\sim$ 10³² ergs s^-1 at the distance of $\omega$ Cen (5.3 kpc).
Instrument	Source	RA	Dec	Position	Rate	MOS1	MOS2
	ID	h m s	$\hbox{$^\circ$ }$ $\hbox{$^\prime$ }$ $\hbox{$^{\prime\prime}$ }$	Error ( $^{\prime\prime}$ )		detection	detection
PN	119	13: 26: 37.8	-47: 16: 00.8	7.59	0.31 $\pm$ 0.06	No	No
PN	54	13: 26: 56.4	-47: 17: 15.4	3.77	0.53 $\pm$ 0.07	No	Yes
PN	65	13: 26: 18.3	-47: 17: 28.6	5.31	0.43 $\pm$ 0.07	Yes	Yes
PN	29	13: 26: 53.3	-47: 18: 24.4	3.60	0.63 $\pm$ 0.07	Yes	Yes
PN	97	13: 27: 05.8	-47: 18: 35.1	5.02	0.30 $\pm$ 0.05	No	No
PN	132	13: 26: 31.0	-47: 18: 48.5	26.59	0.21 $\pm$ 0.05	No	No
PN	3	13: 27: 27.7	-47: 19: 08.8	0.83	7.39 $\pm$ 0.24	Yes	Yes
PN	17	13: 26: 23.5	-47: 19: 27.9	3.00	0.89 $\pm$ 0.08	Yes	Yes
PN	56	13: 27: 02.8	-47: 19: 29.9	5.59	0.38 $\pm$ 0.06	Yes	Yes
PN	28	13: 26: 46.3	-47: 19: 47.4	2.64	0.80 $\pm$ 0.07	Yes	Yes
PN	31	13: 26: 38.5	-47: 20: 01.7	2.43	0.66 $\pm$ 0.07	Yes	Yes
PN	95	13: 27: 08.4	-47: 20: 25.9	7.41	0.16 $\pm$ 0.04	Yes	No
PN	43	13: 26: 03.8	-47: 20: 42.9	3.86	0.54 $\pm$ 0.07	Yes	Yes
PN	73	13: 26: 35.7	-47: 20: 57.4	9.14	0.26 $\pm$ 0.05	No	Yes
PN	68	13: 27: 10.2	-47: 21: 29.2	4.06	0.31 $\pm$ 0.05	Yes	No
PN	145	13: 28: 08.7	-47: 21: 36.8	48.16	0.54 $\pm$ 0.09	No	No
PN	133	13: 27: 58.4	-47: 22: 03.6	24.29	0.30 $\pm$ 0.06	No	No
PN	32	13: 26: 54.5	-47: 22: 04.7	2.73	0.46 $\pm$ 0.06	Yes	Yes
PN	15	13: 26: 41.5	-47: 22: 16.5	2.34	0.66 $\pm$ 0.06	Yes	Yes
PN	77	13: 26: 48.6	-47: 22: 18.7	4.95	0.15 $\pm$ 0.03	No	Yes
PN	129	13: 27: 33.3	-47: 22: 48.1	6.29	0.18 $\pm$ 0.04	No	No
PN	39	13: 26: 23.2	-47: 22: 52.7	2.70	0.52 $\pm$ 0.06	Yes	No
PN	70	13: 28: 01.9	-47: 23: 16.5	4.68	0.68 $\pm$ 0.09	No	No
PN	18	13: 27: 21.2	-47: 23: 24.4	1.92	0.92 $\pm$ 0.08	Yes	Yes
PN	41	13: 27: 07.9	-47: 23: 35.3	3.28	0.42 $\pm$ 0.05	Yes	Yes
PN	99	13: 25: 51.0	-47: 23: 40.6	5.60	0.33 $\pm$ 0.06	No	No
PN	118	13: 26: 27.3	-47: 24: 00.2	17.34	0.20 $\pm$ 0.04	No	No
PN	67	13: 26: 41.3	-47: 24: 05.0	6.67	0.17 $\pm$ 0.03	Yes	Yes
PN	79	13: 26: 12.8	-47: 24: 16.6	5.92	0.19 $\pm$ 0.04	No	Yes
PN	110	13: 27: 12.1	-47: 24: 22.9	5.66	0.17 $\pm$ 0.04	No	No
PN	94	13: 27: 28.5	-47: 24: 25.2	4.86	0.23 $\pm$ 0.04	No	No
PN	126	13: 26: 37.0	-47: 24: 30.5	6.26	0.12 $\pm$ 0.03	No	No
PN	59	13: 26: 31.4	-47: 24: 43.6	5.14	0.24 $\pm$ 0.04	Yes	Yes
PN	86	13: 27: 57.9	-47: 25: 12.0	6.47	0.29 $\pm$ 0.06	No	Yes
PN	75	13: 25: 39.7	-47: 25: 23.4	6.02	0.35 $\pm$ 0.06	No	Yes
PN	82	13: 27: 06.3	-47: 25: 37.8	7.52	0.17 $\pm$ 0.03	No	Yes
PN	106	13: 25: 44.8	-47: 25: 54.7	7.58	0.31 $\pm$ 0.06	No	No
PN	6	13: 27: 29.4	-47: 25: 55.4	1.18	2.35 $\pm$ 0.11	Yes	Yes
PN	146	13: 27: 39.3	-47: 25: 57.1	7.76	0.15 $\pm$ 0.04	No	No
PN	144	13: 27: 59.4	-47: 26: 09.5	7.58	0.22 $\pm$ 0.05	No	No
PN	26	13: 25: 55.9	-47: 26: 19.6	2.53	0.85 $\pm$ 0.08	Yes	Yes
PN	131	13: 25: 42.3	-47: 26: 36.1	9.30	0.25 $\pm$ 0.05	No	No
PN	105	13: 25: 51.3	-47: 26: 44.9	5.92	0.26 $\pm$ 0.05	No	No
PN	115	13: 26: 21.3	-47: 27: 08.2	4.93	0.14 $\pm$ 0.03	No	No
PN	138	13: 25: 58.0	-47: 27: 32.0	6.95	0.16 $\pm$ 0.04	No	No
PN	135	13: 25: 32.6	-47: 27: 37.8	8.22	0.25 $\pm$ 0.06	No	No
PN	76	13: 26: 04.2	-47: 27: 41.6	7.24	0.15 $\pm$ 0.04	No	Yes
PN	140	13: 27: 48.5	-47: 28: 01.0	47.60	0.20 $\pm$ 0.04	No	No
PN	102	13: 27: 17.0	-47: 28: 18.7	5.41	0.12 $\pm$ 0.03	Yes	No
PN	136	13: 26: 00.8	-47: 28: 21.5	10.83	0.17 $\pm$ 0.04	No	No

Table 2: Continued.
Instrument Source RA Dec Position Rate MOS1 MOS2

ID h m s $\hbox{$^\circ$ }$ $\hbox{$^\prime$ }$ $\hbox{$^{\prime\prime}$ }$ Error ( $^{\prime\prime}$ ) detection detection

PN 47 13: 27: 14.5 -47: 28: 31.3 4.40 0.28 $\pm$ 0.04 Yes Yes

PN 33 13: 25: 52.7 -47: 28: 55.4 3.11 0.71 $\pm$ 0.08 Yes Yes

PN 98 13: 25: 57.3 -47: 28: 58.6 6.54 0.27 $\pm$ 0.05 No No

PN 4 13: 26: 19.7 -47: 29: 11.5 0.78 3.42 $\pm$ 0.12 Yes Yes

PN 91 13: 26: 13.5 -47: 29: 13.5 6.09 0.21 $\pm$ 0.04 No No

PN 62 13: 26: 01.0 -47: 29: 13.2 5.70 0.31 $\pm$ 0.05 No Yes

PN 51 13: 26: 06.2 -47: 29: 18.7 5.21 0.53 $\pm$ 0.06 No No

PN 64 13: 28: 14.1 -47: 29: 24.0 5.99 0.92 $\pm$ 0.10 No No

PN 123 13: 25: 54.7 -47: 29: 32.9 11.31 0.20 $\pm$ 0.04 No No

PN 78 13: 26: 07.9 -47: 29: 55.1 4.43 0.27 $\pm$ 0.04 No No

PN 27 13: 25: 44.7 -47: 29: 58.5 3.42 0.67 $\pm$ 0.08 Yes Yes

PN 107 13: 27: 16.1 -47: 29: 59.7 5.76 0.17 $\pm$ 0.04 No No

PN 100 13: 27: 45.8 -47: 30: 00.8 7.85 0.17 $\pm$ 0.04 Yes No

PN 137 13: 26: 15.5 -47: 30: 15.1 47.94 0.13 $\pm$ 0.03 No No

PN 104 13: 26: 13.3 -47: 30: 19.8 5.20 0.18 $\pm$ 0.04 No No

PN 84 13: 27: 40.0 -47: 30: 24.0 5.91 0.22 $\pm$ 0.04 Yes No

PN 109 13: 27: 48.5 -47: 30: 26.0 4.44 0.23 $\pm$ 0.05 No No

PN 87 13: 26: 07.4 -47: 30: 26.8 5.88 0.25 $\pm$ 0.04 No No

PN 117 13: 26: 23.5 -47: 30: 49.4 6.53 0.15 $\pm$ 0.03 No No

PN 124 13: 26: 10.2 -47: 31: 13.8 27.02 0.16 $\pm$ 0.04 No No

PN 12 13: 27: 27.4 -47: 31: 33.7 2.14 0.93 $\pm$ 0.08 Yes Yes

PN 121 13: 25: 50.9 -47: 31: 38.9 25.26 0.23 $\pm$ 0.05 No No

PN 114 13: 27: 14.9 -47: 31: 50.0 5.49 0.15 $\pm$ 0.03 No No

PN 74 13: 27: 21.7 -47: 32: 07.3 7.32 0.15 $\pm$ 0.04 No Yes

PN 139 13: 26: 18.9 -47: 32: 07.2 15.62 0.28 $\pm$ 0.04 No No

PN 8 13: 26: 25.1 -47: 32: 28.7 1.12 2.10 $\pm$ 0.10 Yes Yes

PN 11 13: 27: 11.9 -47: 32: 41.4 1.86 0.82 $\pm$ 0.07 Yes Yes

PN 21 13: 25: 57.2 -47: 32: 51.6 2.34 0.86 $\pm$ 0.08 Yes Yes

PN 116 13: 27: 23.0 -47: 33: 05.4 7.07 0.18 $\pm$ 0.04 No No

PN 1 13: 26: 01.5 -47: 33: 07.4 0.69 6.94 $\pm$ 0.20 Yes Yes

PN 34 13: 27: 10.0 -47: 33: 21.8 3.34 0.36 $\pm$ 0.05 Yes Yes

PN 14 13: 28: 09.1 -47: 33: 27.0 2.42 2.39 $\pm$ 0.16 Yes No

PN 130 13: 25: 58.9 -47: 33: 48.2 46.71 0.22 $\pm$ 0.05 No No

PN 37 13: 25: 53.5 -47: 33: 49.3 3.58 0.62 $\pm$ 0.07 Yes Yes

PN 90 13: 25: 41.3 -47: 33: 58.0 8.28 0.28 $\pm$ 0.06 Yes No

PN 25 13: 26: 11.5 -47: 34: 04.2 2.43 0.78 $\pm$ 0.07 Yes Yes

PN 40 13: 26: 26.9 -47: 34: 09.1 3.88 0.33 $\pm$ 0.05 Yes Yes

PN 22 13: 26: 13.6 -47: 34: 43.2 2.44 0.88 $\pm$ 0.08 Yes Yes

PN 30 13: 26: 27.4 -47: 34: 54.9 2.94 0.50 $\pm$ 0.06 Yes Yes

PN 23 13: 27: 12.7 -47: 34: 56.4 2.38 0.77 $\pm$ 0.07 Yes Yes

PN 52 13: 26: 59.2 -47: 34: 59.0 3.58 0.31 $\pm$ 0.05 Yes Yes

PN 93 13: 26: 10.8 -47: 35: 07.3 4.89 0.27 $\pm$ 0.05 No No

PN 85 13: 27: 53.7 -47: 35: 07.6 6.17 0.28 $\pm$ 0.06 Yes No

PN 141 13: 27: 23.4 -47: 35: 22.2 8.37 0.16 $\pm$ 0.04 No No

PN 120 13: 26: 13.0 -47: 35: 56.3 8.64 0.22 $\pm$ 0.04 No No

PN 143 13: 25: 52.5 -47: 36: 12.2 6.88 0.19 $\pm$ 0.05 No No

PN 46 13: 26: 23.8 -47: 36: 13.5 4.16 0.36 $\pm$ 0.05 Yes Yes

PN 45 13: 26: 39.1 -47: 36: 33.5 3.76 0.33 $\pm$ 0.05 Yes Yes

PN 10 13: 26: 11.4 -47: 37: 11.3 1.35 2.51 $\pm$ 0.13 Yes Yes

PN 142 13: 26: 26.6 -47: 37: 12.7 9.22 0.17 $\pm$ 0.04 No No

PN 134 13: 27: 25.0 -47: 37: 15.1 11.10 0.21 $\pm$ 0.05 No No

PN 113 13: 27: 00.3 -47: 37: 15.2 7.51 0.15 $\pm$ 0.04 No Yes

PN 81 13: 26: 36.4 -47: 37: 30.2 5.59 0.25 $\pm$ 0.05 Yes No

**Table 2:** Continued.
Instrument	Source	RA	Dec	Position	Rate	MOS1	MOS2
	ID	h m s	$\hbox{$^\circ$ }$ $\hbox{$^\prime$ }$ $\hbox{$^{\prime\prime}$ }$	Error ( $^{\prime\prime}$ )		detection	detection
PN	47	13: 27: 14.5	-47: 28: 31.3	4.40	0.28 $\pm$ 0.04	Yes	Yes
PN	33	13: 25: 52.7	-47: 28: 55.4	3.11	0.71 $\pm$ 0.08	Yes	Yes
PN	98	13: 25: 57.3	-47: 28: 58.6	6.54	0.27 $\pm$ 0.05	No	No
PN	4	13: 26: 19.7	-47: 29: 11.5	0.78	3.42 $\pm$ 0.12	Yes	Yes
PN	91	13: 26: 13.5	-47: 29: 13.5	6.09	0.21 $\pm$ 0.04	No	No
PN	62	13: 26: 01.0	-47: 29: 13.2	5.70	0.31 $\pm$ 0.05	No	Yes
PN	51	13: 26: 06.2	-47: 29: 18.7	5.21	0.53 $\pm$ 0.06	No	No
PN	64	13: 28: 14.1	-47: 29: 24.0	5.99	0.92 $\pm$ 0.10	No	No
PN	123	13: 25: 54.7	-47: 29: 32.9	11.31	0.20 $\pm$ 0.04	No	No
PN	78	13: 26: 07.9	-47: 29: 55.1	4.43	0.27 $\pm$ 0.04	No	No
PN	27	13: 25: 44.7	-47: 29: 58.5	3.42	0.67 $\pm$ 0.08	Yes	Yes
PN	107	13: 27: 16.1	-47: 29: 59.7	5.76	0.17 $\pm$ 0.04	No	No
PN	100	13: 27: 45.8	-47: 30: 00.8	7.85	0.17 $\pm$ 0.04	Yes	No
PN	137	13: 26: 15.5	-47: 30: 15.1	47.94	0.13 $\pm$ 0.03	No	No
PN	104	13: 26: 13.3	-47: 30: 19.8	5.20	0.18 $\pm$ 0.04	No	No
PN	84	13: 27: 40.0	-47: 30: 24.0	5.91	0.22 $\pm$ 0.04	Yes	No
PN	109	13: 27: 48.5	-47: 30: 26.0	4.44	0.23 $\pm$ 0.05	No	No
PN	87	13: 26: 07.4	-47: 30: 26.8	5.88	0.25 $\pm$ 0.04	No	No
PN	117	13: 26: 23.5	-47: 30: 49.4	6.53	0.15 $\pm$ 0.03	No	No
PN	124	13: 26: 10.2	-47: 31: 13.8	27.02	0.16 $\pm$ 0.04	No	No
PN	12	13: 27: 27.4	-47: 31: 33.7	2.14	0.93 $\pm$ 0.08	Yes	Yes
PN	121	13: 25: 50.9	-47: 31: 38.9	25.26	0.23 $\pm$ 0.05	No	No
PN	114	13: 27: 14.9	-47: 31: 50.0	5.49	0.15 $\pm$ 0.03	No	No
PN	74	13: 27: 21.7	-47: 32: 07.3	7.32	0.15 $\pm$ 0.04	No	Yes
PN	139	13: 26: 18.9	-47: 32: 07.2	15.62	0.28 $\pm$ 0.04	No	No
PN	8	13: 26: 25.1	-47: 32: 28.7	1.12	2.10 $\pm$ 0.10	Yes	Yes
PN	11	13: 27: 11.9	-47: 32: 41.4	1.86	0.82 $\pm$ 0.07	Yes	Yes
PN	21	13: 25: 57.2	-47: 32: 51.6	2.34	0.86 $\pm$ 0.08	Yes	Yes
PN	116	13: 27: 23.0	-47: 33: 05.4	7.07	0.18 $\pm$ 0.04	No	No
PN	1	13: 26: 01.5	-47: 33: 07.4	0.69	6.94 $\pm$ 0.20	Yes	Yes
PN	34	13: 27: 10.0	-47: 33: 21.8	3.34	0.36 $\pm$ 0.05	Yes	Yes
PN	14	13: 28: 09.1	-47: 33: 27.0	2.42	2.39 $\pm$ 0.16	Yes	No
PN	130	13: 25: 58.9	-47: 33: 48.2	46.71	0.22 $\pm$ 0.05	No	No
PN	37	13: 25: 53.5	-47: 33: 49.3	3.58	0.62 $\pm$ 0.07	Yes	Yes
PN	90	13: 25: 41.3	-47: 33: 58.0	8.28	0.28 $\pm$ 0.06	Yes	No
PN	25	13: 26: 11.5	-47: 34: 04.2	2.43	0.78 $\pm$ 0.07	Yes	Yes
PN	40	13: 26: 26.9	-47: 34: 09.1	3.88	0.33 $\pm$ 0.05	Yes	Yes
PN	22	13: 26: 13.6	-47: 34: 43.2	2.44	0.88 $\pm$ 0.08	Yes	Yes
PN	30	13: 26: 27.4	-47: 34: 54.9	2.94	0.50 $\pm$ 0.06	Yes	Yes
PN	23	13: 27: 12.7	-47: 34: 56.4	2.38	0.77 $\pm$ 0.07	Yes	Yes
PN	52	13: 26: 59.2	-47: 34: 59.0	3.58	0.31 $\pm$ 0.05	Yes	Yes
PN	93	13: 26: 10.8	-47: 35: 07.3	4.89	0.27 $\pm$ 0.05	No	No
PN	85	13: 27: 53.7	-47: 35: 07.6	6.17	0.28 $\pm$ 0.06	Yes	No
PN	141	13: 27: 23.4	-47: 35: 22.2	8.37	0.16 $\pm$ 0.04	No	No
PN	120	13: 26: 13.0	-47: 35: 56.3	8.64	0.22 $\pm$ 0.04	No	No
PN	143	13: 25: 52.5	-47: 36: 12.2	6.88	0.19 $\pm$ 0.05	No	No
PN	46	13: 26: 23.8	-47: 36: 13.5	4.16	0.36 $\pm$ 0.05	Yes	Yes
PN	45	13: 26: 39.1	-47: 36: 33.5	3.76	0.33 $\pm$ 0.05	Yes	Yes
PN	10	13: 26: 11.4	-47: 37: 11.3	1.35	2.51 $\pm$ 0.13	Yes	Yes
PN	142	13: 26: 26.6	-47: 37: 12.7	9.22	0.17 $\pm$ 0.04	No	No
PN	134	13: 27: 25.0	-47: 37: 15.1	11.10	0.21 $\pm$ 0.05	No	No
PN	113	13: 27: 00.3	-47: 37: 15.2	7.51	0.15 $\pm$ 0.04	No	Yes
PN	81	13: 26: 36.4	-47: 37: 30.2	5.59	0.25 $\pm$ 0.05	Yes	No

**Table 2:** Continued.
Instrument	Source	RA	Dec	Position	Rate	MOS1	MOS2
	ID	h m s	$\hbox{$^\circ$ }$ $\hbox{$^\prime$ }$ $\hbox{$^{\prime\prime}$ }$	Error ( $^{\prime\prime}$ )		detection	detection
PN	128	13: 26: 24.1	-47: 37: 45.7	9.76	0.23 $\pm$ 0.05	No	No
PN	19	13: 26: 07.4	-47: 38: 01.3	2.31	1.15 $\pm$ 0.10	Yes	Yes
PN	69	13: 27: 33.4	-47: 38: 35.0	5.55	0.48 $\pm$ 0.07	Yes	No
PN	58	13: 26: 32.4	-47: 38: 50.7	4.94	0.38 $\pm$ 0.06	No	Yes
PN	83	13: 27: 22.5	-47: 39: 46.4	5.07	0.45 $\pm$ 0.07	No	No
PN	53	13: 27: 01.2	-47: 40: 55.9	4.34	0.57 $\pm$ 0.07	Yes	Yes
PN	66	13: 26: 57.9	-47: 41: 22.4	6.22	0.54 $\pm$ 0.07	No	Yes
PN	125	13: 26: 33.1	-47: 41: 29.2	49.94	0.29 $\pm$ 0.06	No	No
PN	112	13: 27: 03.3	-47: 42: 41.9	8.30	0.46 $\pm$ 0.07	No	No
MOS	7	13: 25: 52.1	-47: 19: 09.5	0.91	2.30 $\pm$ 0.09	Yes	Yes
MOS	63	13: 25: 40.6	-47: 22: 08.4	4.28	0.23 $\pm$ 0.04	Yes	Yes
MOS	48	13: 25: 34.5	-47: 25: 58.5	3.58	0.28 $\pm$ 0.04	Yes	Yes
MOS	13	13: 26: 20.4	-47: 30: 03.8	1.57	0.40 $\pm$ 0.03	Yes	Yes
MOS	89	13: 26: 25.7	-47: 39: 04.5	4.63	0.12 $\pm$ 0.03	Yes	Yes
MOS	55	13: 26: 10.4	-47: 39: 10.8	3.67	0.27 $\pm$ 0.04	Yes	Yes
MOS	71	13: 26: 10.6	-47: 40: 28.5	5.08	0.21 $\pm$ 0.04	Yes	Yes

Table 3: The XMM-Newton sources correlated with the Chandra and ROSAT sources. The error on the Chandra position is given at the 90% confidence level, as provided by the wavdetect task. The ROSAT source numbers are taken from Johnston et al. (1994); Verbunt & Johnston (2000). The EINSTEIN sources are labeled as in Hertz & Grindlay (1983). The source list is declination sorted.
Source RA Dec Chandra Chandra Position Previous

ID RA Dec error ( $^{\prime\prime}$ ) ID

h m s $\hbox{$^\circ$ }$ $\hbox{$^\prime$ }$ $\hbox{$^{\prime\prime}$ }$ h m s $\hbox{$^\circ$ }$ $\hbox{$^\prime$ }$ $\hbox{$^{\prime\prime}$ }$ (RA/Dec)

3 13: 27: 27.7 -47: 19: 08.8 ... ... ... 4,D

7 13: 25: 52.1 -47: 19: 09.5 ... ... ... 3,A

17 13: 26: 23.5 -47: 19: 27.9 13: 26: 23.5 -47: 19: 24.1 0.52/0.45 ...

28 13: 26: 46.3 -47: 19: 47.4 13: 26: 46.2 -47: 19: 45.9 0.68/0.39 18

31 13: 26: 38.5 -47: 20: 01.7 13: 26: 38.5 -47: 19: 58.3 0.68/0.48 ...

73 13: 26: 35.7 -47: 20: 57.4 13: 26: 35.2 -47: 20: 52.8 1.28/0.64 ...

68 13: 27: 10.2 -47: 21: 29.2 13: 27: 09.9 -47: 21: 27.7 0.78/0.47 ...

32 13: 26: 54.5 -47: 22: 04.7 13: 26: 54.5 -47: 22: 04.6 0.24/0.10 ...

15 13: 26: 41.5 -47: 22: 16.5 13: 26: 41.5 -47: 22: 16.3 0.52/0.31 ...

39 13: 26: 23.2 -47: 22: 52.7 13: 26: 23.1 -47: 22: 51.2 0.73/0.80 ...

18 13: 27: 21.2 -47: 23: 24.4 13: 27: 21.1 -47: 23: 24.5 0.63/0.38 19

41 13: 27: 07.9 -47: 23: 35.3 13: 27: 08.0 -47: 23: 33.6 0.65/0.39 ...

67 13: 26: 41.3 -47: 24: 05.0 13: 26: 41.2 -47: 24: 00.9 0.87/0.58 ...

79 13: 26: 12.8 -47: 24: 16.6 13: 26: 12.8 -47: 24: 13.6 0.79/0.59 ...

110 13: 27: 12.1 -47: 24: 22.9 13: 27: 12.4 -47: 24: 24.9 1.04/0.78 ...

94 13: 27: 28.5 -47: 24: 25.2 13: 27: 28.4 -47: 24: 22.2 0.89/0.58 ...

126 13: 26: 37.0 -47: 24: 30.5 13: 26: 37.3 -47: 24: 31.3 1.07/0.62 ...

59 13: 26: 31.4 -47: 24: 43.6 13: 26: 31.3 -47: 24: 39.4 0.62/0.53 ...

82 13: 27: 06.3 -47: 25: 37.8 13: 27: 06.4 -47: 25: 39.5 0.56/0.69 ...

6 13: 27: 29.4 -47: 25: 55.4 13: 27: 29.3 -47: 25: 54.8 0.28/0.15 6

49 13: 26: 28.7 -47: 26: 33.3 13: 26: 28.7 -47: 26: 27.3 0.64/0.23 ...

103 13: 26: 45.4 -47: 26: 53.6 13: 26: 45.4 -47: 26: 52.4 1.05/0.65 ...

44 13: 26: 52.6 -47: 27: 15.9 13: 26: 52.9 -47: 27: 15.7 1.17/0.52 ...

24 13: 26: 40.8 -47: 27: 38.6 13: 26: 40.5 -47: 27: 38.7 1.60/0.91 ...

61 13: 26: 52.5 -47: 27: 39.1 13: 26: 52.6 -47: 27: 38.5 1.01/0.50 ...

76 13: 26: 04.2 -47: 27: 41.6 13: 26: 04.4 -47: 27: 42.1 0.65/0.78 ...

47 13: 27: 14.5 -47: 28: 31.3 13: 27: 14.5 -47: 28: 28.8 1.01/0.77 ...

33 13: 25: 52.7 -47: 28: 55.4 ... ... ... 8

92 13: 26: 44.3 -47: 28: 57.4 13: 26: 44.3 -47: 28: 56.2 0.71/0.68 ...

5 13: 26: 53.5 -47: 29: 01.3 13: 26: 53.5 -47: 29: 00.8 0.16/0.07 9a,C

4 13: 26: 19.7 -47: 29: 11.5 13: 26: 19.7 -47: 29: 11.2 0.15/0.12 7,B

101 13: 26: 37.9 -47: 29: 11.3 13: 26: 38.0 -47: 29: 10.7 1.28/0.79 ...

51 13: 26: 06.2 -47: 29: 18.7 13: 26: 05.9 -47: 29: 22.3 0.70/0.74 ...

2 13: 26: 52.2 -47: 29: 36.1 13: 26: 52.2 -47: 29: 36.1 0.15/0.04 9b,C

72 13: 26: 34.5 -47: 29: 57.3 13: 26: 34.4 -47: 29: 55.8 0.20/0.18 ...

13 13: 26: 20.4 -47: 30: 03.8 13: 26: 20.4 -47: 30: 04.0 0.19/0.19 ...

137 13: 26: 15.5 -47: 30: 15.1 13: 26: 16.7 -47: 30: 56.3 1.42/0.52 ...

84 13: 27: 40.0 -47: 30: 24.0 13: 27: 39.6 -47: 30: 24.4 1.30/0.90 ...

60 13: 26: 34.2 -47: 30: 34.7 13: 26: 34.4 -47: 30: 34.5 0.46/0.33 ...

127 13: 27: 04.5 -47: 30: 38.2 13: 27: 04.6 -47: 30: 37.0 0.78/0.68 ...

117 13: 26: 23.5 -47: 30: 49.4 13: 26: 23.5 -47: 30: 44.2 0.70/0.59 ...

20 13: 26: 37.4 -47: 30: 52.9 13: 26: 37.4 -47: 30: 54.5 0.38/0.22 ...

38 13: 26: 55.0 -47: 31: 13.2 13: 26: 55.0 -47: 31: 13.7 0.59/0.28 ...

9 13: 26: 48.7 -47: 31: 26.2 13: 26: 48.8 -47: 31: 26.0 0.43/0.20 21

12 13: 27: 27.4 -47: 31: 33.7 13: 27: 27.4 -47: 31: 33.2 0.41/0.43 ...

121 13: 25: 50.9 -47: 31: 38.9 13: 25: 48.9 -47: 31: 27.4 0.66/0.66 ...

108 13: 26: 46.6 -47: 31: 40.5 13: 26: 46.5 -47: 31: 44.4 1.25/0.70 ...

36 13: 26: 50.8 -47: 31: 47.5 13: 26: 51.1 -47: 31: 45.8 0.27/0.28 ...

114 13: 27: 14.9 -47: 31: 50.0 13: 27: 14.7 -47: 31: 49.6 1.09/0.46 ...

74 13: 27: 21.7 -47: 32: 07.3 13: 27: 21.5 -47: 32: 05.9 1.20/0.40 ...

35 13: 26: 49.6 -47: 31: 53.2 13: 26: 49.5 -47: 31: 47.8 1.22/0.46 ...

57 13: 26: 49.6 -47: 32: 13.4 13: 26: 49.5 -47: 32: 13.6 0.43/0.15 ...

**Table 3:** Continued.
Source	RA	Dec	Chandra	Chandra	Position	Previous
ID			RA	Dec	error ( $^{\prime\prime}$ )	ID
	h m s	$\hbox{$^\circ$ }$ $\hbox{$^\prime$ }$ $\hbox{$^{\prime\prime}$ }$	h m s	$\hbox{$^\circ$ }$ $\hbox{$^\prime$ }$ $\hbox{$^{\prime\prime}$ }$	(RA/Dec)
8	13: 26: 25.1	-47: 32: 28.7	13: 26: 25.1	-47: 32: 28.3	0.229/0.20	10
16	13: 26: 43.9	-47: 32: 31.0	13: 26: 44.1	-47: 32: 32.3	0.315/0.23	...
11	13: 27: 11.9	-47: 32: 41.4	13: 27: 11.7	-47: 32: 41.6	0.249/0.22	...
21	13: 25: 57.2	-47: 32: 51.6	13: 25: 57.2	-47: 32: 50.8	0.373/0.38	...
1	13: 26: 01.5	-47: 33: 07.4	13: 26: 01.5	-47: 33: 06.3	0.164/0.15	11
34	13: 27: 10.0	-47: 33: 21.8	13: 27: 10.0	-47: 33: 21.8	0.568/0.34	...
14	13: 28: 09.1	-47: 33: 27.0	...	...	...	12
25	13: 26: 11.5	-47: 34: 04.2	13: 26: 11.5	-47: 34: 03.4	0.401/0.34	...
40	13: 26: 26.9	-47: 34: 09.1	13: 26: 26.7	-47: 34: 09.5	0.794/0.45	...
22	13: 26: 13.6	-47: 34: 43.2	13: 26: 13.6	-47: 34: 41.5	0.561/0.44	...
30	13: 26: 27.4	-47: 34: 54.9	13: 26: 27.6	-47: 34: 56.9	0.361/0.29	...
23	13: 27: 12.7	-47: 34: 56.4	13: 27: 12.9	-47: 34: 57.1	0.324/0.19	...
52	13: 26: 59.2	-47: 34: 59.0	13: 26: 59.3	-47: 34: 58.2	0.744/0.48	...
45	13: 26: 39.1	-47: 36: 33.5	13: 26: 39.2	-47: 36: 32.3	0.727/0.46	...
10	13: 26: 11.4	-47: 37: 11.3	...	...	...	13
113	13: 27: 00.3	-47: 37: 15.2	13: 27: 00.4	-47: 37: 15.2	0.998/0.64	...

Note - We have indicated in this table only the sources correlated with other X-ray observations. There are three OGLEGC sources which are associated with X-ray sources (OGLEGC 15 and 22 with two Chandra sources, OGLEGC 30 with XMM-Newton source 29). Their positions from Kaluzny et al. (1996) are:
OGLEGC15 13^h 26^m 47.42^s -47 $\hbox{$^\circ$ }$ 36 $^\prime$ 00.4 $^{\prime\prime}$
OGLEGC22 13^h 26^m 08.33^s -47 $\hbox{$^\circ$ }$ 30 $^\prime$ 33.0 $^{\prime\prime}$
OGLEGC30 13^h 26^m 53.33^s -47 $\hbox{$^\circ$ }$ 18 $^\prime$ 22.9 $^{\prime\prime}$ .

Table 5: Best fit spectral parameters for the brightest sources of the field of view. We have selected those sources which have more than 100 net counts in EPIC-PN and limited our analysis to the 16 sources within twice the half mass radius. Simple models have been used: Power Law (PL), Blackbody (BB), Thermal Bremsstrahlung (TB). For source 3, which has an optical counterpart (Cool et al. 1995), we used a two temperature Raymond-Smith model (2T). The model parameters are either the photon index or the temperature in keV. Whenever allowed by the statistics, we left the $N_{\rm H}$ as a free parameter of the fit. Otherwise it was frozen at the optical value ( $8.4\times 10^{20}$ cm^-2). We used either the $\chi ^{\scriptscriptstyle 2}$ or Cash statistics in the fit. The bolometric luminosity is computed between 0.5 and 10 keV and is given in units of 10³¹ ergs s^-1.
Source Best fit $N_{\rm H}$ Model $\chi^{\scriptscriptstyle 2}_{\scriptscriptstyle \nu}$ Degree of Bolometric

ID model (10²⁰ cm^-2) parameter freedom luminosity

1 BB $62^{\scriptscriptstyle +21}_{\scriptscriptstyle -21}$ $1.2^{\scriptscriptstyle +0.1}_{\scriptscriptstyle -0.1}$ 1.08 55 191 $\pm$ 7

TB $167^{\scriptscriptstyle +31}_{\scriptscriptstyle -31}$ $10.7^{\scriptscriptstyle +11.1}_{\scriptscriptstyle -4.0}$ 1.00 55 302 $\pm$ 11

PL $183^{\scriptscriptstyle +35}_{\scriptscriptstyle -35}$ $1.7^{\scriptscriptstyle +0.3}_{\scriptscriptstyle -0.3}$ 1.03 55 339 $\pm$ 12

2 TB (8.4) $23.0^{\scriptscriptstyle +29.9}_{\scriptscriptstyle -10.1}$ 0.72 31 67 $\pm$ 3

PL (8.4) $1.4^{\scriptscriptstyle +0.2}_{\scriptscriptstyle -0.2}$ 0.68 31 72 $\pm$ 3

3 2T $30^{\scriptscriptstyle +11}_{\scriptscriptstyle -17}$ $0.2^{\scriptscriptstyle +0.1}_{\scriptscriptstyle -0.1}$ 1.08 28 136 $\pm$ 7

$0.9^{\scriptscriptstyle +0.1}_{\scriptscriptstyle -0.2}$

5 TB (8.4) $18.7^{\scriptscriptstyle +65.2}_{\scriptscriptstyle -10.0}$ 0.78 17 27 $\pm$ 2

PL (8.4) $1.4^{\scriptscriptstyle +0.2}_{\scriptscriptstyle -0.2}$ 0.80 31 30 $\pm$ 2

6 TB (8.4) $4.5^{\scriptscriptstyle +4.7}_{\scriptscriptstyle -1.9}$ 0.83 17 27 $\pm$ 3

PL (8.4) $1.7^{\scriptscriptstyle +0.3}_{\scriptscriptstyle -0.3}$ 0.81 17 32 $\pm$ 3

8 TB (8.4) $5.8^{\scriptscriptstyle +7.2}_{\scriptscriptstyle -2.5}$ 0.98 19 28 $\pm$ 2

PL (8.4) $1.7^{\scriptscriptstyle +0.3}_{\scriptscriptstyle -0.3}$ 0.81 19 32 $\pm$ 3

9 TB $21^{\scriptscriptstyle +16}_{\scriptscriptstyle -16}$ $4.4^{\scriptscriptstyle +6.3}_{\scriptscriptstyle -2.1}$ 0.58 10 23 $\pm$ 3

TB (8.4) $8.3^{\scriptscriptstyle +17.0}_{\scriptscriptstyle -3.9}$ 0.79 11 23 $\pm$ 3

PL $31^{\scriptscriptstyle +24}_{\scriptscriptstyle -13}$ 2.0 $\pm$ 0.6 0.51 10 29 $\pm$ 4

PL (8.4) $1.5^{\scriptscriptstyle +0.2}_{\scriptscriptstyle -0.2}$ 0.96 11 29 $\pm$ 4

12 BB (8.4) $0.3^{\scriptscriptstyle +0.1}_{\scriptscriptstyle -0.1}$ 1.54 9 5 $\pm$ 1

TB (8.4) $1.2^{\scriptscriptstyle +1.7}_{\scriptscriptstyle -0.6}$ 1.22 9 7 $\pm$ 2

PL (8.4) $2.4^{\scriptscriptstyle +0.6}_{\scriptscriptstyle -0.6}$ 1.10 9 9 $\pm$ 2

15 PL (8.4) $1.0^{\scriptscriptstyle +0.5}_{\scriptscriptstyle -0.5}$ 0.42 6 21 $\pm$ 4

18 TB (8.4) $3.7^{\scriptscriptstyle +11.0}_{\scriptscriptstyle -2.1}$ 1.12 5 10 $\pm$ 2

PL (8.4) $1.8^{\scriptscriptstyle +0.5}_{\scriptscriptstyle -0.5}$ 1.01 5 12 $\pm$ 2

Source Best fit $N_{\rm H}$ Model C statistic Number of Bolometric

ID model (10²⁰ cm^-2) parameter PHA bins luminosity

11 TB (8.4) $3.2^{\scriptscriptstyle +7.7}_{\scriptscriptstyle -3.2}$ C 8.29 11 8 $\pm$ 2

PL (8.4) $1.9^{\scriptscriptstyle +0.7}_{\scriptscriptstyle -0.7}$ C 8.96 11 10 $\pm$ 2

13 PL (8.4) $0.9^{\scriptscriptstyle +0.3}_{\scriptscriptstyle -0.3}$ C 1.16 8 33 $\pm$ 5

20 BB (8.4) $0.6^{\scriptscriptstyle +0.2}_{\scriptscriptstyle -0.2}$ C 16.37 11 6 $\pm$ 2

TB $52^{\scriptscriptstyle +70}_{\scriptscriptstyle -40}$ $2.0^{\scriptscriptstyle +4.2}_{\scriptscriptstyle -1.3}$ C 16.70 11 9 $\pm$ 2

22 PL (8.4) $1.6^{\scriptscriptstyle +0.4}_{\scriptscriptstyle -0.4}$ C 9.18 11 12 $\pm$ 2

23 TB (8.4) $0.7^{\scriptscriptstyle +1.1}_{\scriptscriptstyle -0.4}$ C 12.58 10 5 $\pm$ 2

PL (8.4) $2.8^{\scriptscriptstyle +0.9}_{\scriptscriptstyle -0.9}$ C 12.77 10 6 $\pm$ 2

24, high state PL (8.4) $1.2^{\scriptscriptstyle +0.4}_{\scriptscriptstyle -0.4}$ C 16.2 14 18 $\pm$ 2

low state PL (8.4) $1.7^{\scriptscriptstyle +1.4}_{\scriptscriptstyle -1.4}$ C 10.2 11 4 $\pm$ 2

25 TB (8.4) $1.4^{\scriptscriptstyle +5.6}_{\scriptscriptstyle -0.8}$ C 2.50 5 6 $\pm$ 2

PL (8.4) $2.2^{\scriptscriptstyle +0.8}_{\scriptscriptstyle -0.8}$ C 1.81 5 8 $\pm$ 2

Source	Best fit	$N_{\rm H}$	Model	$\chi^{\scriptscriptstyle 2}_{\scriptscriptstyle \nu}$	Degree of	Bolometric
ID	model	(10²⁰ cm^-2)	parameter		freedom	luminosity
1	BB	$62^{\scriptscriptstyle +21}_{\scriptscriptstyle -21}$	$1.2^{\scriptscriptstyle +0.1}_{\scriptscriptstyle -0.1}$	1.08	55	191 $\pm$ 7
	TB	$167^{\scriptscriptstyle +31}_{\scriptscriptstyle -31}$	$10.7^{\scriptscriptstyle +11.1}_{\scriptscriptstyle -4.0}$	1.00	55	302 $\pm$ 11
	PL	$183^{\scriptscriptstyle +35}_{\scriptscriptstyle -35}$	$1.7^{\scriptscriptstyle +0.3}_{\scriptscriptstyle -0.3}$	1.03	55	339 $\pm$ 12

2	TB	(8.4)	$23.0^{\scriptscriptstyle +29.9}_{\scriptscriptstyle -10.1}$	0.72	31	67 $\pm$ 3
	PL	(8.4)	$1.4^{\scriptscriptstyle +0.2}_{\scriptscriptstyle -0.2}$	0.68	31	72 $\pm$ 3

3	2T	$30^{\scriptscriptstyle +11}_{\scriptscriptstyle -17}$	$0.2^{\scriptscriptstyle +0.1}_{\scriptscriptstyle -0.1}$	1.08	28	136 $\pm$ 7
			$0.9^{\scriptscriptstyle +0.1}_{\scriptscriptstyle -0.2}$
5	TB	(8.4)	$18.7^{\scriptscriptstyle +65.2}_{\scriptscriptstyle -10.0}$	0.78	17	27 $\pm$ 2
	PL	(8.4)	$1.4^{\scriptscriptstyle +0.2}_{\scriptscriptstyle -0.2}$	0.80	31	30 $\pm$ 2

6	TB	(8.4)	$4.5^{\scriptscriptstyle +4.7}_{\scriptscriptstyle -1.9}$	0.83	17	27 $\pm$ 3
	PL	(8.4)	$1.7^{\scriptscriptstyle +0.3}_{\scriptscriptstyle -0.3}$	0.81	17	32 $\pm$ 3

8	TB	(8.4)	$5.8^{\scriptscriptstyle +7.2}_{\scriptscriptstyle -2.5}$	0.98	19	28 $\pm$ 2
	PL	(8.4)	$1.7^{\scriptscriptstyle +0.3}_{\scriptscriptstyle -0.3}$	0.81	19	32 $\pm$ 3

9	TB	$21^{\scriptscriptstyle +16}_{\scriptscriptstyle -16}$	$4.4^{\scriptscriptstyle +6.3}_{\scriptscriptstyle -2.1}$	0.58	10	23 $\pm$ 3
	TB	(8.4)	$8.3^{\scriptscriptstyle +17.0}_{\scriptscriptstyle -3.9}$	0.79	11	23 $\pm$ 3
	PL	$31^{\scriptscriptstyle +24}_{\scriptscriptstyle -13}$	2.0 $\pm$ 0.6	0.51	10	29 $\pm$ 4
	PL	(8.4)	$1.5^{\scriptscriptstyle +0.2}_{\scriptscriptstyle -0.2}$	0.96	11	29 $\pm$ 4

12	BB	(8.4)	$0.3^{\scriptscriptstyle +0.1}_{\scriptscriptstyle -0.1}$	1.54	9	5 $\pm$ 1
	TB	(8.4)	$1.2^{\scriptscriptstyle +1.7}_{\scriptscriptstyle -0.6}$	1.22	9	7 $\pm$ 2
	PL	(8.4)	$2.4^{\scriptscriptstyle +0.6}_{\scriptscriptstyle -0.6}$	1.10	9	9 $\pm$ 2

15	PL	(8.4)	$1.0^{\scriptscriptstyle +0.5}_{\scriptscriptstyle -0.5}$	0.42	6	21 $\pm$ 4

18	TB	(8.4)	$3.7^{\scriptscriptstyle +11.0}_{\scriptscriptstyle -2.1}$	1.12	5	10 $\pm$ 2
	PL	(8.4)	$1.8^{\scriptscriptstyle +0.5}_{\scriptscriptstyle -0.5}$	1.01	5	12 $\pm$ 2
Source	Best fit	$N_{\rm H}$	Model	C statistic	Number of	Bolometric
ID	model	(10²⁰ cm^-2)	parameter		PHA bins	luminosity
11	TB	(8.4)	$3.2^{\scriptscriptstyle +7.7}_{\scriptscriptstyle -3.2}$	C 8.29	11	8 $\pm$ 2
	PL	(8.4)	$1.9^{\scriptscriptstyle +0.7}_{\scriptscriptstyle -0.7}$	C 8.96	11	10 $\pm$ 2

13	PL	(8.4)	$0.9^{\scriptscriptstyle +0.3}_{\scriptscriptstyle -0.3}$	C 1.16	8	33 $\pm$ 5

20	BB	(8.4)	$0.6^{\scriptscriptstyle +0.2}_{\scriptscriptstyle -0.2}$	C 16.37	11	6 $\pm$ 2
	TB	$52^{\scriptscriptstyle +70}_{\scriptscriptstyle -40}$	$2.0^{\scriptscriptstyle +4.2}_{\scriptscriptstyle -1.3}$	C 16.70	11	9 $\pm$ 2

22	PL	(8.4)	$1.6^{\scriptscriptstyle +0.4}_{\scriptscriptstyle -0.4}$	C 9.18	11	12 $\pm$ 2

23	TB	(8.4)	$0.7^{\scriptscriptstyle +1.1}_{\scriptscriptstyle -0.4}$	C 12.58	10	5 $\pm$ 2
	PL	(8.4)	$2.8^{\scriptscriptstyle +0.9}_{\scriptscriptstyle -0.9}$	C 12.77	10	6 $\pm$ 2

24, high state	PL	(8.4)	$1.2^{\scriptscriptstyle +0.4}_{\scriptscriptstyle -0.4}$	C 16.2	14	18 $\pm$ 2
low state	PL	(8.4)	$1.7^{\scriptscriptstyle +1.4}_{\scriptscriptstyle -1.4}$	C 10.2	11	4 $\pm$ 2

25	TB	(8.4)	$1.4^{\scriptscriptstyle +5.6}_{\scriptscriptstyle -0.8}$	C 2.50	5	6 $\pm$ 2
	PL	(8.4)	$2.2^{\scriptscriptstyle +0.8}_{\scriptscriptstyle -0.8}$	C 1.81	5	8 $\pm$ 2

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