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Table 5:

Results of the X-ray spectral analysis. Errors and upper limits are all given at the 90% level.

Name 		Net number Galactic $N_{\rm H}$ $^{\dagger}$ $N_{\rm H}$ $\Gamma$ 2-10 keV flux $^{\ddagger}$ 20-40 keV flux
(IGR)   of counts $\times10^{22}$ cm-2 $\times10^{22}$ cm-2   erg cm-2 s-1 erg cm-2 s-1
            Extrapolated IBIS source
J02086-1742 931 0.01 <0.017 $1.55_{\rm -0.08}^{+0.1}$ $6.4\times10^{-12}$ $6.3\times10^{-12}$ $6.8\times10^{-12}$
J02524-0829$^{\star}$ 617 0.04 $12\pm3$ $2.4\pm0.6$ $1.2\times10^{-11}$ $4.7\times10^{-12}$ 3.1 $\times10^{-11}$
J03184-0014 22 0.05 <1.1 $1.4_{\rm -0.9}^{+1.5}$ $1.5\times10^{-13}$ $2.0\times10^{-13}$ $2.9\times10^{-11}$
J11457-1827$^\P$ 4020 0.03 $1.298_{\rm -0.003}^{+0.01}$ $1.91_{\rm -0.04}^{+0.08}$ $1.4\times10^{-11}$ $1.1\times10^{-11}$ $3.3\times10^{-11}$
J12060+3818$^\P$ 48 0.016 <0.13 $2.4_{\rm -0.9}^{+1.2}$ $1.5\times10^{-13}$ $5.6\times10^{-14}$ $3.1\times10^{-11}$
J12070+2535$^\P$ 74 0.016 $0.3\pm0.2$ $1.9_{\rm -0.5}^{+0.6}$ $1.4\times10^{-12}$ $1.1\times10^{-12}$ $1.4\times10^{-11}$
J13042-1020a 268 0.033 $29_{\rm -6}^{+8}$ $2\pm0.2$ $4.0\times10^{-12}$ $1.7\times10^{-12}$ $7.5\times10^{-12}$
J13412+3022a 90 0.014 $30_{\rm -8}^{+11}$ $1.4_{\rm -0.6}^{+0.2}$ $8.0\times10^{-12}$ $9.5\times10^{-12}$ $9.1\times10^{-12}$
J14488-5942#1 344 1.8 $13_{\rm -4}^{+6}$ $2.8_{\rm -0.9}^{+1.1}$ $7.9\times10^{-12}$ $7.1\times10^{-13}$ $3.8\times10^{-12}$
'' #2 22 '' <2.4 $2.2_{\rm -1.6}^{+2.2}$ $4.7\times10^{-14}$ $7.9\times10^{-15}$ ''
J23130+8608 20 0.052 - $1.4_{\rm -0.9}^{+0.7}$ $7.0\times10^{-14}$ $9.4\times10^{-14}$ $1.4\times10^{-11}$

Notes.  $^{(\dagger)}$ Value obtained from the LAB survey (Kalberla et al. 2005). $^{(\ddagger)}$ Flux corrected for the absorption. $^{(\star)}$ Hard fluxes are estimated over the 17-60 keV ranges. $^{(\P)}$ Hard fluxes are estimated over the 20-60 keV ranges. (a) Spectra fitted with a partial covering absorber and a power-law.


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