Table 5: Summary of best-fitting parameters of the SEDs of the sources. We give the total galactic extinctions in magnitudes  $A_{H {\sc i}}$ and $A_{\rm H_2}$, the X-ray extinction of the source in magnitudes $A_{\rm x}$ and then the parameters themselves: the extinction in the optical $A_{\rm v}$, the temperature $T_\ast $ and the $\frac{{R}_\ast}{{D}_{\ast}}$ ratio of the companion and the temperature and radius $T_{\rm D}$ and ${R}_{{\rm D}}$ (in ${R}_{\ast }$ unit) of the dust component when needed. We also add the reduced $\chi ^2$ we reach for each fit.
Sources $A_{H {\sc i}}$ $A_{\rm H_2}$ $A_{\rm x}$ $A_{\rm v}$ $T_{\ast} ({\rm K})$ $\frac{{R}_\ast}{{D}_{\ast}}$ $T_{\rm D} ({\rm K})$ ${R}_{\rm D} \left({R}_{\ast}\right)$ $\chi^2/{\rm d.o.f.}$
IGR J16195-4945 11.7 28.6 37.4 15.5 23 800 $5.96\times 10^{-{11}}$ 1160 5.1 3.9/2
IGR J16207-5129 9.3 11.8 19.8 10.5 33 800 $9.42\times10^{-{11}}$     28.5/9
IGR J16318-4848 11.0 19.2 1069.5 17.0 22 200 $3.74\times 10^{-{10}}$ 1100 10.0 6.6/6
IGR J16320-4751 11.4 23.6 112.2 35.4 33 000 $1.38\times 10^{-{10}}$     7.7/6
IGR J16358-4726 11.8 39.4 176.4 17.6 24 500 $3.16\times 10^{-{11}}$ 810 10.1 3.6/2
IGR J16418-4532 10.1 19.3 53.5 14.5 32 800 $3.77\times 10^{-{11}}$     1.4/4
IGR J16465-4507 11.3 31.4 320.7 5.9 25 000 $6.40\times 10^{-{11}}$     13.9/7
IGR J16479-4514 11.4 43.8 41.2 18.5 32 800 $1.00\times 10^{-{10}}$     7.4/6
IGR J17252-3616 8.3 20.1 80.2 20.8 32 600 $7.57\times 10^{-{11}}$     3.8/5
IGR J17391-3021 7.3 23.9 160.4 9.2 31 400 $1.80\times 10^{-{10}}$     11.7/10
IGR J17544-2619 7.7 41.5 7.70 6.1 31 000 $1.27\times10^{-{10}}$     6.1/8
IGR J19140+0951 9.0 14.0 32.1 16.5 22 500 $1.92\times10^{-{10}}$     14.4/6

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