Table 5: X-ray spectral analysis. Errors and upper limits are all given at the 90% level.
Name Net number Galactic $N_{\rm H}$ (LAB/DL)$^\ddagger$ $N_{\rm H}$ $\Gamma $ 2-10 keV flux
(IGR)   of counts $\times10^{22}$ cm-2 $\times10^{22}$ cm-2   erg cm-2 s-1
J03184-0014 19 0.05/0.06 0.06$^\dagger$ $\rm 1.4_{-0.7}^{+0.8}$ $\rm 5.3_{-0.3}^{+0.5}$ $\times10^{-14}$
J03532-6829 1650 0.06/0.06 $\rm0.09_{-0.04}^{+0.04}$ $\rm 1.9_{-0.1}^{+0.1}$ $\rm 1.75_{-0.18}^{+0.14}$ $\times10^{-11}$
J05319-6601 19 0.12/0.06 0.12$^\dagger$ $\rm 1.55_{-0.77}^{+0.89}$ $\rm 5_{-3}^{+4}$ $\times10^{-14}$
J05346-5759 2172 0.04/0.05 <0.05 $\rm 1.22_{-0.09}^{+0.1}$ $\rm 1.7_{-0.1}^{+0.2}$ $\times10^{-11}$
  378   <0.15 $\rm 1.75_{-0.3}^{+0.3}$ $\rm 5.7_{-1.0}^{+1.2}$ $\times10^{-12}$
  2516   $\rm0.05_{-0.03}^{+0.03}$ $\rm 1.34_{-0.09}^{+0.09}$ $\rm 1.7_{-0.1}^{+0.1}\times10^{-11}$
J09025-6814 17 0.05/0.07 $\rm 9_{-7}^{+123}$ <3.2 < $9.2\times10^{-12}$
J10101-5654 86 1.35/1.77 $\rm 3.3_{-1.7}^{+2.5}$ $\rm 1.3_{-0.8}^{+0.9}$ $\rm 1.2_{-0.6}^{+0.3}\times10^{-11}$
J13020-6359 337 1.40/1.53 2.48$^\dagger$ $\rm0.9_{-0.3}^{+0.3}$ $\rm 2.3_{-0.9}^{+0.3}\times10^{-11}$
  670   2.48$^\dagger$ $\rm 1.2_{-0.2}^{+0.2}$ $\rm 2.6_{-0.4}^{+0.2}\times10^{-11}$
  471   2.48$^\dagger$ $\rm 1.1_{-0.2}^{+0.2}$ $\rm 2.3_{-0.5}^{+0.3}\times10^{-11}$
  574   2.48$^\dagger$ $\rm 1.1_{-0.2}^{+0.2}$ $\rm 2.3_{-0.5}^{+0.3}\times10^{-11}$
J15161-3827 #1 48 0.06/0.07 22-9+17 2.0$^\dagger$ $\rm 1.2_{-0.5}^{+0.5}$ $\times10^{-12}$
#2 32 0.07/0.07 <0.2 $\rm 1.2_{-0.5}^{+0.7}$ < $1.3\times10^{-13}$
#3 18 0.07/0.07 <1.9 >2.8 <1 $\times10^{-13}$
#4 13 0.06/0.07 0.065$^\dagger$ $\rm 2.0_{-0.9}^{+1.0}$ $\rm 3_{-2}^{+5}\times10^{-14}$
J16287-5021 75 1.37/1.55 $\rm 2.6_{-1.6}^{+2.1}$ $\rm0.9_{-0.8}^{+0.8}$ $\rm 6.5_{-3.0}^{+2.2}\times10^{-12}$
J17353-3539 416 0.69/0.63 $\rm0.7_{-0.3}^{+0.4}$ $\rm 2.2_{-0.4}^{+0.4}$ $\rm 5.0_{-0.5}^{+0.9}\times10^{-12}$
  803   $\rm0.8_{-0.2}^{+0.2}$ $\rm 2.1_{-0.3}^{+0.3}$ $\rm 1.2_{-0.1}^{+0.1}\times10^{-11}$
J17476-2253 45 0.30/0.38 $\rm 1.9_{-1.1}^{+1.7}$ $\rm 2.6_{-1.0}^{+1.4}$ $\rm 5_{-3}^{+2}\times10^{-12}$
J18214-1318 1866 1.21/1.54 $\rm 3.5_{-0.5}^{+0.8}$ $\rm0.4_{-0.2}^{+0.2}$ $\rm 6.7_{-0.4}^{+0.7}\times10^{-11}$
J19267+1325 461 0.95/0.93 <0.6 1.1-0.3+0.3 $8.1_{-0.7}^{+1.6}\times10^{-12}$
J20286+2544 #1 171 0.20/0.26 $\rm 61_{-20}^{+23}$ $\rm 2.5_{-1.4}^{+1.6}$ $\rm 2.1_{-1.2}^{+1.6}\times10^{-11}$
#2 53 0.20/0.26 $\rm 93_{-61}^{+80}$ $\rm 2.7_{-3.1}^{+3.1}$ < $1.6\times10^{-11}$
J23206+6431 244 0.78/0.90 $\rm0.9_{-0.7}^{+1.0}$ $\rm 1.6_{-0.5}^{+0.7}$ $5.5_{-1.0}^{+1.3}\times10^{-12}$
$^\ddagger$ Values of weighted average Galactic $N_{\rm H}$ respectively obtained from Leiden/Argentine/Bonn (LAB) and Dickey & Lockman (DL) surveys of Galactic H I in the Galaxy; $^\dagger$ unconstrained parameter that was fixed during the spectral fit.

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