Table 3: Spectral parameters for sufficiently bright sources.
1 2 3 4 5 6 7 8 9 10
No. ID $\Gamma$ $N_{\rm H}$ kT Abund. Thermal $\chi^{2}$ d.o.f. No.
      [cm-2] [keV] (solar) model      
05 2E 0055.6-7241 $\rm 2.59^{+0.16}_{-0.33}$ $\rm 5.3^{+1.1}_{-0.8} \times 10^{21}$ - - - 41.4 51 2
06 XMMU J005735.7-721932 $\rm 1.42^{+0.25}_{-0.20}$ $\rm 3.6^{+1.9}_{-1.5} \times 10^{21}$ - - - 84.6 63 4
07 AX J0058-720 $\rm 1.01^{+0.11}_{-0.11}$ $\rm 3.4^{+5.9}_{-3.4} \times 10^{20}$ - - - 91.6 65 3
08 RX J0057.8-7207 $\rm0.97^{+0.08}_{-0.07}$ $\rm 3.0^{+0.8}_{-0.4} \times 10^{21}$ - - - 161.9 133 3
10 RX J0059.3-7223 $\rm 1.46^{+0.12}_{-0.13}$ $\rm 1.8^{+0.7}_{-0.6} \times 10^{21}$ - - - 117.8 99 5
11 RX J0100.2-7204 $\rm 2.00^{+0.41}_{-0.26}$ $\rm 1.7^{+0.9}_{-1.0} \times 10^{21}$ - - - 28.9 26 3
14 RX J0101.3-7211 $\rm 1.14^{+0.18}_{-0.13}$ $\rm 3.3^{+2.4}_{-1.1} \times 10^{21}$ $\rm0.20^{+0.09}_{-0.06}$ $\rm0.11^{+0.10}_{-0.11}$ MEKAL 82.6 56 2
15 RX J0101.6-7204 $\rm 1.73^{+0.15}_{-0.17}$ $\rm 8.6^{+4.9}_{-5.6} \times 10^{20}$ - - - 68.0 58 6
16 AX J0103-722 $\rm 1.08_{-0.19}^{+0.12}$ $\rm 1.9_{-1.7}^{+1.9} \times 10^{21}$ $\rm0.27_{-0.07}^{+0.08}$ $\rm0.31_{-0.17}^{+0.43}$ MEKAL 172.7 155 3
17 RX J0103.6-7201 (Model 1) $\rm0.72_{-0.07}^{+0.06}$ $\rm 1.7_{-0.9}^{+1.0} \times 10^{21}$ $\rm0.27_{-0.04}^{+0.03}$ $\rm0.77_{-0.28}^{+0.17}$ MEKAL 295.1 240 3

(Model 2) $\rm0.71_{-0.06}^{+0.05}$ $\rm 2.3_{-0.8}^{+0.8} \times 10^{21}$ $\rm0.32_{-0.05}^{+0.05}$ $\rm 1.07_{-0.18}^{+0.57}$ (O) VMEKAL 272.9 238 3
          $\rm 1.61_{-0.66}^{+1.40}$ (Ne)        
Notes to Col. 4: Additional $N_{\rm H}$ to Galactic foreground $N_{\rm H, Gal}$ (see Eqs. (2) and (3)).
Notes to Col. 9: Degrees of freedom.
Notes to Col. 10: Number of used spectra.

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