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Table 1

List of sources detected in the 3−10 keV band in the field of view of the XMM-Newton observation of the Kes 69 SNR.

Src Name Count rate N H Γ χ2/d.o.f. 10-14F2−10 keV Possible association
PN cnt ks-1 1022 cm-2 erg cm-2 s-1 in SIMBAD within 15′′

1 XMMU J183331.4-101616 9.8 ± 2.0 1.1
2 XMMU J183257.1-101426 8.1 ± 0.8 0.82 IRAS 18302-1016 (13″)
3 XMMU J183312.4-101349 10.6 ± 0.9 0.47 1XMM J183312.5-101351 (1′′)
4 XMMU J183254.0-101259 4.2 ± 0.6 0.82
5 XMMU J183236.4-101146 35.3 ± 2.3 1.1 XGPS-I J183236-101144 (3″)
6 XMMU J183303.8-100928 4.0 ± 0.5 1.2
7 XMMU J183308.4-100909 3.2 ± 0.5 0.84
8 XMMU J183247.2-100606 4.3 ± 0.6 1.2
9 XMMU J183234.3-100434 10.9 ± 1.1 1.1 2MASS J18323431-1004360 (1″)a
10 XMMU J183225.2-100159 6.2 ± 0.7 0.86 XGPS-I J183225-100158 (0.5″)
11 XMMU J183215.3-100125 5.7 ± 0.8  <3.5 0.57
12 XMMU J183251.6-100105 5.8 ± 1.4 0.97 XGPS-I J183251-100106 (1″)b
13 XMMU J183307.2-100050 3.0 ± 0.5 0.42
14 XMMU J183210.8-100029 9.2 ± 1.1  <9.0 c 1.35 XGPS-I J183210-100031 (1″)
15 XMMU J183255.4-095920 6.3 ± 0.7 1.4
16 XMMU J183219.6-095843 8.0 ± 1.0 0.79
17 XMMU J183222.5-095708 9.0 ± 1.0 1.1
18 XMMU J183236.7-095556 20.0 ± 1.4  <0.7 1.0

Notes. 

(a)

mJ = 16.1.

(b)

An mR = 21.6 star, according to Motch et al. (2010).

(c)

1σ errors.

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