Table 2: Spectral fit results.

Source		 $\gamma$ kT $N_{\rm H}$ SM4 Flux5 Luminosity6
XMMU J05...   [keV] [1021cm-2]   [erg cm-2 s-1 [erg s-1]

2924.3-655724		   $ 0.68\pm0.08 $ <0.1 MK 6.6 $~\times 10^{-14}$  
2940.5-655318 $\rm 2.33^{+0.13}_{-0.20}$   $\rm 1.3^{+0.2}_{-0.4}$ PL 9.6 $~\times 10^{-14}$  
2947.4-655639 $1.31 \pm 0.17 $   $2.6 \pm 1.0 $ PL 2.2 $~\times 10^{-13}$ 7.7 $~\times 10^{34}$
3011.2-655122 $1.07 \pm 0.06 $   $6.9 \pm 0.3 $ PL 1.2 $~\times 10^{-12}$ 3.9 $~\times 10^{35}$
3034.9-655653   0.7 fixed $\rm 1.9^{+0.8}_{-0.6}$ MK 1.9 $~\times 10^{-14}$ 1.2 $~\times 10^{34}$

3041.0-660532		 $\rm 1.40^{+0.14}_{-0.11}$   $\rm 2.7^{+0.9}_{-0.7}$ PL 2.9 $~\times 10^{-13}$  
3049.9-655522 $\rm 2.00^{+0.20}_{-0.21}$   $\rm 1.4^{+0.5}_{-0.5}$ PL 5.1 $~\times 10^{-14}$  
3056.2-6548091   $\rm0.049^{+0.006}_{-0.012}$ <0.3 BB 4.2 $~\times 10^{-14}$ 1.3 $~\times 10^{34}$
3102.5-6606492 $\rm 1.81^{+0.09}_{-0.07}$   <0.1 PL 2.3 $~\times 10^{-13}$  
3113.3-660705 $\rm 1.67^{+0.12}_{-0.13}$ $ 0.10\pm0.02$ $\rm 6.9^{+0.7}_{-1.3}$ / $\rm 97^{+3}_{-7}$ MC 7.0 $~\times 10^{-12}$ 4.6 $~\times 10^{37}$

3137.2-660131		   $0.66\pm0.16$ <1.0 MK 1.6 $~\times 10^{-14}$  
3150.9-655616 $\rm 1.92^{+0.14}_{-0.07}$   $\rm 5.3^{+0.9}_{-0.7}$ PL 1.6 $~\times 10^{-13}$  
3153.8-660217 $\rm 2.07^{+0.20}_{-0.17}$   $2.8\pm0.6$ PL 1.0 $~\times 10^{-13}$  
3153.9-654959 $\rm 1.88^{+0.30}_{-0.26}$   $\rm 3.8^{+1.8}_{-1.2}$ PL 1.1 $~\times 10^{-13}$  
3157.1-660233 $\rm 1.62^{+0.14}_{-0.17}$   $\rm 3.8^{+1.0}_{-1.2}$ PL 1.4 $~\times 10^{-13}$  

3226.2-655352		   $0.68\pm0.06$ $\rm 2.1^{+0.9}_{-0.6}$ MK 5.5 $~\times 10^{-14}$ 3.6 $~\times 10^{34}$
3230.2-6557353 $\rm 2.23^{+0.20}_{-0.13}$   $\rm0.7^{+0.3}_{-0.5}$ PL 6.3 $~\times 10^{-14}$  
3232.4-655139 $\rm 1.18^{+0.25}_{-0.29}$   $\rm 2.5^{+2.2}_{-1.5}$ PL 1.2 $~\times 10^{-13}$ 4.1 $~\times 10^{34}$
3236.7-655551 $\rm 2.02^{+0.19}_{-0.16}$   $\rm 1.3^{+0.5}_{-0.4}$ PL 1.1 $~\times 10^{-13}$  
3243.9-660258   $0.52\pm0.18 $ <0.4 MK 1.0 $~\times 10^{-14}$  
1 Spectral fit to pn spectrum only.
2 The low absorption indicates a low energy excess which is probably caused by contamination from EXO 053109-6609.2.
3 Located in arc structure caused by single reflected photons from nearby bright SNR which probably causes contamination.
4 Spectral model; MC: multi-component (see text), PL: power-law, BB: blackbody, MK: thermal emission from plasma in collisional equilibrium (Mewe-Kaastra, Mewe et al. 1985).
5 0.2-10 keV, determined from the pn spectrum except for EXO 053109-6609.2 (MOS1) which is located on a CCD gap in the pn.
6 0.2-10 keV, intrinsic luminosity with $N_{\rm H}$ set to 0 for sources located in the LMC assuming a distance of 50 kpc.


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