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Table 10

Power law plus thermal component fit results.

Source Type z Γ NH kT E σ EW f2−10   keV Log L2−10   keV χ2/d.o.f. Probability Sample
1022 10-13
cm-2 keV 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)

XBSJ012654.3+191246 AGN e 0.043 1.90 f 0.066 1.04 ... ... ... 0.29 41.17 7/11 83.0 BSS
XBSJ021822.2–050615p AGN2 0.044 1.67 19.6 1.8 6.28 210 360 2.93 42.51 109/78 1.2 HBSS
XBSJ033845.7–322253p AGN2 0.113 1.9f 24.1 0.21 ... ... ... 1.61 43.17 49/36 7.3 HBSS
XBSJ040758.9–712833 AGN2 0.134 1.9f 11.0 0.24 ... ... ... 1.80 43.22 14/10 16.3 HBSS
XBSJ112026.7+431520 AGN2 0.146 1.9f 7.5 0.87 ... ... ... 1.87 43.26 18/15 25.5 HBSS
XBSJ231546.5–590313 AGN2 0.0446 1.90 f 1.25 0.46 ... ... ... 1.49 41.95 15/14 35.9 BSS

Notes. Columns: (1) source name; (2) class; (3) redshift; (4) photon index; (5) intrinsic column density; (6) plasma temperature; (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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