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Table 9

Leaky/Leaky+line fit results.

Source Type z Γ NH Ratio E σ EW f 2−10   keV Log L2−10   keV χ2/d.o.f. Probability Sample
1022 10-13
cm-2 keV eV eV erg cm-2 s-1 erg s-1 %
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11) (12) (13) (14)

XBSJ021822.2–050615p AGN2e 0.044 1.97 22.20 0.004 6.28 210 370 2.81 42.57 112/79 0.8 HBSS
XBSJ033845.7–352253 AGN2 0.113 1.99 31.30 0.024 ... ... ... 1.70 43.26 42/36 22.3 HBSS
XBSJ040758.9–712833 AGN2 0.134 1.90 f 21.90 0.032 ... ... ... 2.23 43.43 11/11 42.7 HBSS
XBSJ091828.4+513931 AGN1 0.185 1.85 6.41 0.045 ... ... ... 2.56 43.58 12/15 67.8 HBSS, BSS
XBSJ095218.9–013643 AGN1 0.020 3.38 49.00 0.007 0.92 50 150 9.96 43.03 60/54 27.0 HBSS, BSS
XBSJ112026.7+431520 AGN2 e 0.146 1.88 8.25 0.021 ... ... ... 1.88 43.26 20/15 15.8 HBSS

Notes. Columns: (1) source name; (2) class; (3) redshift; (4) photon index; (5) intrinsic column density; (6) scattered component to direct component ratio; (7) emission line central energy; (8) emission line width; (9) emission line equivalent width; (10) observed flux in the 2 − 10 keV band, de-absorbed by our Galaxy; (11) intrinsic luminosity in the 2 − 10 keV band; (12) χ2 to number of degrees of freedom; (13) null hypothesis probability; (14) sample the source belongs to.

(p)

Null hypothesis probability  <  10%;

(e)

elusive AGN;

(f)

fixed parameter. Source and parameters in bold face indicates that this model is considered as our best-fit model. Note: errors and upper limits are at 90% confidence level. Fluxes and luminosities refer to the MOS2 calibration.

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