Table 5: Best-fit parameters for the X-ray spectral analysis (extragalactic objects).
name id Model $\Gamma$ $N_{\rm H}$ kT red $\chi^2$/d.o.f. $f_{2{-}10~\rm keV}$ Log $L_{2{-}10~\rm keV}$
        ($\times$1022)     ($\times$10-13)  
XBS J002618.5+105019 BEL AGN PL $\rm 2.02^{+ 0.07}_{-0.06}$ < 0.011 ... 1.15 / 97 2.8 44.44
XBS J013240.1-133307 NEL AGN PL 1.9 (frozen) $\rm 2.54^{+ 0.71}_{ -0.56}$ ... 1.11 / 19 1.7 44.41
XBS J013944.0-674909 BEL AGN PL $\rm 1.94^{+ 0.14}_{-0.12}$ < 0.018 ... 0.91 / 34 1.2 42.56
XBS J015957.5+003309 BEL AGN PL $\rm 2.14^{+ 0.09}_{-0.09}$ < 0.010 ... 1.19 / 99 2.9 44.03
XBS J021640.7-044404 BEL AGN PL $\rm 2.24^{+ 0.08}_{-0.09}$ < 0.020 ... 1.17 / 67 1.1 44.74
XBS J021808.3-045845 BEL AGN PL + BB $\rm 2.01^{+ 0.04}_{-0.04}$ < 0.007 $\rm0.16^{+ 0.01}_{ -0.01}$ 1.07 / 527 2.3 44.79
XBS J021817.4-045113 BEL AGN PL $\rm 1.84^{+ 0.04}_{-0.03}$ <0.04 ... 1.07 / 346 2.7 45.22
$\rm XBS~J021822.2$-050615a NEL AGN Leaky $\rm 1.66^{+ 0.34}_{-0.36}$ $\rm 20.54^{+ 0.36}_{ -0.44}$ ... 1.41 / 63 3.0 42.76
XBS J023713.5-522734 NLSy1 PL + BB $\rm 1.90^{+ 0.18}_{-0.13}$ < 0.18 $\rm0.11^{+ 0.02}_{ -0.02}$ 0.86 / 80 2.7 43.52
XBS J030206.8-000121 BEL AGN PL $\rm 1.90^{+ 0.06}_{-0.06}$ < 0.015 ... 1.14 / 125 2.2 44.63
$\rm XBS~J030614.1$-284019b BEL AGN PL $\rm 1.56^{+ 0.26}_{-0.13}$ < 0.048 ... 1.15 / 16 2.9 43.87
XBS J031015.5-765131 BEL AGN PL $\rm 1.92^{+ 0.04}_{-0.04}$ < 0.022 ... 0.90 / 189 3.4 45.47
XBS J031146.1-550702 Sy1.9 PL $\rm 2.08^{+ 0.13}_{-0.12}$ < 0.013 ... 0.93 / 44 2.8 43.37
XBS J031859.2-441627 BEL AGN PL $\rm 1.58^{+ 0.29}_{-0.29}$ $\rm0.33^{+0.43}_{-0.19}$ ... 0.73 / 18 1.7 42.99
XBS J033845.7-352253 NEL AGN Leaky + RS 1.9 (frozen) $\rm 28.5^{+ 6.7}_{-10.0}$ $\rm0.16^{+ 0.04}_{ -0.08}$ 0.83 / 29 1.7 43.21
XBS J040658.8-712457 Sy1.9 PL 1.9 (frozen) $\rm 21.97^{+ 17.67}_{ -12.78}$ ... 1.25 / 4 1.6 43.56
XBS J040758.9-712833 NEL AGN Leaky 1.9 (frozen) $\rm 28.23^{+21.96}_{-14.64}$ ... 1.13 / 5 2.5 43.44
XBS J041108.1-711341 BEL AGN PL $\rm 1.95^{+ 0.48}_{-0.36}$ < 0.61 ... 0.99 / 6 0.8 44.59
XBS J185613.7-462239 BEL AGN PL $\rm 2.18^{+ 0.27}_{-0.24}$ < 0.058 ... 1.15 / 26 1.4 44.69
XBS J193248.8-723355 ELG PL 1.9 (frozen) $\rm 1.14^{+ 0.25}_{ -0.21}$ ... 1.06 / 35 1.9 43.76
XBS J204043.4-004548 NEL AGN PL 1.9 (frozen) $\rm 3.00^{+ 1.15}_{ -0.90}$ ... 1.35 / 16 1.7 44.50
XBS J205635.7-044717 BEL AGN PL + BB $\rm 1.91^{+ 0.51}_{-0.35}$ < 0.56 $\rm0.15^{+ 0.03}_{ -0.03}$ 1.18 / 21 1.7 43.42
XBS J205829.9-423634 NLSy1 PL $\rm 1.91^{+ 0.09}_{-0.09}$ $\rm0.09^{+ 0.04}_{ -0.03}$ ... 0.76 / 120 3.2 43.76
XBS J213002.3-153414 BEL AGN PL $\rm 2.10^{+ 0.23}_{-0.21}$ $\rm0.08^{+ 0.12}_{ -0.08}$ ... 0.82 / 26 1.8 44.45
$\rm XBS~J213824.0$-423019c BEL AGN PL $\rm 2.14^{+ 0.25}_{-0.17}$ < 0.057 ... 0.86 / 26 1.6 43.60
XBS J214041.4-234720 BEL AGN PL $\rm 2.19^{+ 0.10}_{-0.10}$ < 0.012 ... 1.06 / 93 1.7 44.28
XBS J220601.5-015346 BEL AGN PL + BB $\rm 1.56^{+ 0.16}_{-0.09}$ <0.670 $\rm0.06^{+ 0.01}_{ -0.04}$ 0.72 / 15 1.7 43.36
Column 1: source name;

Col. 2: optical identification;

Col. 3: best-fit model (PL = absorbed power-law; Leaky = leaky absorbed power-law; PL + BB = absorbed power-law plus
Black-Body spectrum; Leaky + RS = leaky absorbed power-law plus a Raymond-Smith spectrum)

Col. 4: best-fit photon index of the power-law component;

Col. 5: best-fit intrinsic hydrogen column density [cm-2];

Col. 6: temperature of the thermal component (if present) [keV];

Col. 7: reduced Chi-squared and degrees of freedom of the best-fit;

Col. 8: observed 2-10 keV flux (corrected for the Galactic absorption) [erg s-1 cm-1];

Col. 9: logarithm of the intrinsic luminosity in the 2-10 keV energy range [erg s-1];

a results from the X-ray analysis taken from Severgnini et al. (2003);

b in this object the presence of an emission line at 1.9 keV (source rest frame, consistent with the Si XIII at 1.86 keV) is required;

c in this object the presence of an emission line at 6.4 keV (source rest frame, consistent with the Fe I K$\alpha$) is required.


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