Extended
Sources
Giacconi
et al. 2002, ApJS, 139, 369
A search for extended sources in
the 1 Ms exposure yield
19 candidates. For relatively rare objects like groups and clusters of
galaxies,
the CDFS probes the very faint end of their X-ray luminosity function.
XID
|
RA(J2000)
|
Dec
(J2000)
|
counts
[0.5-2] keV
|
Flux
[0.5-2] keV
|
S/N
|
FWHM
|
Off
Axis
|
HR
|
eHR
|
37
|
3:32:22.21
|
-27:41:56.22
|
89.8
|
5.03e-16
|
8.0
|
5.6
|
6.77
|
-0.23
|
0.11
|
116
|
3:32:30.07
|
-27:44:05.35
|
93.0
|
5,29e-16
|
8.8
|
3.9
|
4.58
|
-0.56
|
0.11
|
132
|
3:32:44.09
|
-27:54:56.12
|
40.9
|
2.19e-16
|
4.8
|
6.9
|
7.17
|
-0.05
|
0.17
|
138
|
3:32:50.11
|
-27:41:35.30
|
51.8
|
9.13e-16
|
5.9
|
7.3
|
8.54
|
-1.00
|
0.00
|
147
|
3:32:46.43
|
-27:46:32.74
|
25.9
|
1.49e-16
|
4.0
|
4.1
|
4.50
|
0.65
|
0.08
|
240
|
3:32:59.20
|
-27:51:40.43
|
43.8
|
2.46e-16
|
4.9
|
7.4
|
7.43
|
-0.15
|
0.19
|
249
|
3:32:19.49
|
-27:54:06.55
|
27.4
|
1.46e-16
|
3.7
|
8.2
|
5.80
|
-0.12
|
0.22
|
507
|
3:33:00.12
|
-27:49:25.50
|
23.3
|
1.43e-16
|
3.0
|
5.7
|
7.04
|
0.10
|
0.23
|
511
|
3:32:36.63
|
-27:46:31.30
|
22.6
|
1.27e-16
|
3.5
|
5.8
|
2.79
|
-0.24
|
0.27
|
514
|
3:32:33.56
|
-27:43:12.40
|
27.1
|
1.57e-16
|
4.1
|
5.0
|
5.56
|
-0.14
|
0.21
|
522
|
3:32:21.50
|
-27:55:50.99
|
68.2
|
3.78e-16
|
6.6
|
6.1
|
7.36
|
-0.34
|
0.16
|
527
|
3:32:18.59
|
-27:54:14.40
|
36.6
|
1.97e-16
|
4.4
|
6.6
|
6.00
|
-0.29
|
0.21
|
529
|
3:32:16.32
|
-27:55:25.97
|
23.4
|
1.32e-16
|
3.0
|
9.0
|
7.29
|
0.11
|
0.25
|
544
|
3:31:54.64
|
-27:51:04.75
|
34.7
|
1.90e-16
|
3.9
|
6.5
|
7.86
|
0.05
|
0.22
|
560
|
3:32:06.27
|
-27:45:38.02
|
23.2
|
1.26e-16
|
3.6
|
5.5
|
5.77
|
-1.00
|
0.00
|
566
|
3:32:18.11
|
-27:47:19.50
|
30.9
|
2.33e-16
|
4.5
|
3.4
|
2.65
|
-1.00
|
0.00
|
581
|
3:32:07.47
|
-27:49:43.68
|
17.6
|
9.51e-17
|
3.0
|
3.8
|
4.77
|
-1.00
|
0.00
|
594
|
3:32:09.83
|
-27:42:49.68
|
237.0
|
1.36e-15
|
12.0
|
8.1
|
7.14
|
-1.00
|
0.00
|
645
|
3:31:49.95
|
-27:49:41.74
|
262.0
|
1.75e-15
|
9.0
|
----
|
8.58
|
-1.00
|
0.00
|
