Table 3: Best fit spectral parameters using an absorbed power-law, a soft thermal component and a Gaussian narrow line.

Name
$N_{\rm H, int}$ $\Gamma $ $E_\alpha$ $EW_\alpha$ C kT/ $\Gamma_{\rm soft}$ $F_{\rm 2-10}$ $F_{\rm 20-100}$ $\chi^{2}$/d.o.f.
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10)
LEDA 168563 - $\rm 1.68^{+0.05}_{-0.05}$ $\rm 6.44^{+0.09}_{-0.11}$ <52 $\rm0.6^{+0.2}_{-0.2}$ $\rm 3.8^{+0.2}_{-0.2}$ 1.46 5.6 507/488
IGR J07597-3842 - $\rm 1.57^{+0.01}_{-0.02}$ $\rm 6.44^{+0.04}_{-0.06}$ $\rm 48^{+39}_{-13}$ $\rm0.8^{+0.1}_{-0.1}$ $\rm0.09^{+0.01}_{-0.01}$ 1.56 3.6 352/339
ESO 209-12 - $\rm 1.73^{+0.02}_{-0.03}$ $\rm 6.39^{+0.04}_{-0.05}$ $\rm 163^{+57}_{-62}$ $\rm 1.2^{+0.3}_{-0.2}$ $\rm0.05^{+0.01}_{-0.01}$ 0.83 1.9 500/508
FRL 1146(AO3) $\rm0.36^{+0.05}_{-0.05}$ $\rm 1.84^{+0.05}_{-0.05}$ $\rm 6.39^{+0.07}_{-0.07}$ <146 $\rm 1.1^{+0.3}_{-0.3}$ $\rm0.15^{+0.02}_{-0.01}$ 1.15 2.0 418/421
FRL 1146(AO4)$^{\dag }$ $\rm0.28^{+0.04}_{-0.04}$ $\rm 1.69^{+0.04}_{-0.06}$ $\rm 6.37^{+0.03}_{-0.03}$ $\rm 111^{+37}_{-38}$ $\rm0.7^{+0.2}_{-0.2}$ $\rm0.16^{+0.01}_{-0.01}$ 1.21 2.0 424/438
$\rm 4U~1344-60^{\dag }$ $\rm0.98^{+0.14}_{-0.17}$ $\rm 2.04^{+0.08}_{-0.09}$ $\rm 6.41^{+0.03}_{-0.04}$ $\rm 51^{+20}_{-19}$ $\rm0.9^{+0.1}_{-0.1}$ - 3.58 6.6 706/638
IGR J16482-3036 $\rm0.09^{+0.01}_{-0.01}$ $\rm 1.59^{+0.02}_{-0.03}$ $\rm 6.46^{+0.06}_{-0.06}$ $\rm 96^{+32}_{-72}$ $\rm0.5^{+0.1}_{-0.1}$ - 1.97 1.9 607/563
IGR J16558-5203$^{\dag }$ - $\rm 2.25^{+0.03}_{-0.03}$ $\rm 6.48^{+0.05}_{-0.06}$ $\rm 61^{+50}_{-34}$ $\rm 2.7^{+0.5}_{-0.5}$ - 1.05 2.8 540/592
IGR J17418-1212$^{\dag }$ $\rm0.13^{+0.01}_{-0.01}$ $\rm 1.98^{+0.01}_{-0.02}$ $\rm 6.28^{+0.04}_{-0.05}$ $\rm 51^{+37}_{-20}$ $\rm 1.5^{+0.3}_{-0.3}$ - 1.29 2.1 651/606
IGR J18027-1455$^{\dag }$ $\rm0.41^{+0.05}_{-0.05}$ $\rm 1.61^{+0.04}_{-0.04}$ $\rm 6.39^{+0.01}_{-0.03}$ $\rm 134^{+33}_{-34}$ $\rm 2.9^{+0.4}_{-0.3}$ $\rm0.19^{+0.08}_{-0.07}$ 0.61 4.6 363/316
Note: (1): Galaxy name. (2): Intrinsic fully-covering column density in units of 1022 cm-2. (3): Power-law photon index. (4): Energy of the FeK line, in keV. (5): Equivalent width of the FeK line, in eV. (6): Value of the XMM-Newton/INTEGRAL cross-calibration constant. (7): Temperature of the thermal component (kT in keV) or photon index of the soft power-law component ( $\Gamma_{\rm soft}$) in the case of LEDA 168563. (8-9): Model fluxes in the 2-10 keV and 20-100 keV bands in units of 10-11 erg cm-2 s-1. (10): Chi-squared and degrees of freedom. $\dag $: Sources with extra spectral components (see Sect. 4).

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