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Table 8

Power law plus reflected component fit results.

Source Type z Γ NH R f2−10   keV Log L2−10   keV χ2/d.o.f. Probability Sample
1022 10-13
cm-2 erg cm-2 s-1 erg s-1 %
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
XBSJ021808.3–045845p AGN1 0.712 2.38  < 0.04 0.3(< 0.5) 2.67 44.80 459/417 7.8 HBSS, BSS
XBSJ023713.5–522734 AGN1 0.193 2.80  < 0.017 2(< 7) 2.95 43.53 75/88 84.4 HBSS, BSS
XBSJ031311.7–765428 AGN1 1.274 2.16  < 0.25  < 0.10 1.11 44.94 60/50 17.2 BSS
XBSJ043448.3–775329 AGN1 e 0.097 1.9 f 0.20 0.4( < 0.6) 4.00 43.00 9/11 62.1 BSS
XBSJ052108.5–251913 AGN1 1.196 2.22  < 0.17 0.6( < 1.20) 2.73 45.28 78/64 11.2 HBSS, BSS
XBSJ074312.1+742937 AGN1 0.312 2.51  < 0.006 1.3(< 1.6) 10.6 44.56 199/192 35.2 HBSS, BSS
XBSJ101922.6+412049 AGN1 0.239 2.12  < 0.03 0.3( < 0.6 2.97 43.65 102/110 69.0 HBSS, BSS
XBSJ141736.3+523028 AGN1 0.985 2.16  < 0.14 0.3(< 1.7) 0.89 44.60 112/97 15.0 BSS
XBSJ223547.9–255836 AGN1 0.304 2.88 0.08 1.7(< 5) 0.86 43.42 32/32 47.7 BSS
XBSJ231601.7–424038 AGN1 0.383 3.05  < 0.072 2(< 5.5) 0.73 43.59 56/52 33.9 BSS

Notes. Columns: (1) source name; (2) class; (3) redshift; (4) photon index; (5) intrinsic column density; (6) reflection scaling factor and upper limit at 90% confidence (between parenthesis); (7) observed flux in the 2 − 10 keV band, de-absorbed by our Galaxy; (8) intrinsic luminosity in the 2 − 10 keV band; (9) χ2 to number of degrees of freedom; (10) null hypothesis probability; (11) 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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