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Table 6

Black body model fit results.

Source Type z Γ NH kT f2 − 10   keV Log L2−10   keV χ2/d.o.f. Probability Sample
1022 10-13
cm-2 keV erg cm-2 s-1 erg s-1 (%)
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
XBSJ000532.7+200716 AGN1 0.119 2.31 0.02 0.10 0.60 42.42 36/35 40.7 BSS
XBSJ005031.1–520012 AGN1 0.463 2.03  < 0.26 0.11 0.94 43.95 88/78 19.7 BSS
XBSJ015957.5+003309 AGN1 0.310 2.01  < 0.15 0.07 3.18 44.06 93/80 15.3 HBSS, BSS
XBSJ021808.3–045845 AGN1 0.712 1.91  < 0.03 0.20 2.58 44.81 446/417 15.9 HBSS, BSS
XBSJ023530.2–523045 AGN1 0.429 1.9 f  < 0.125 0.059 1.10 43.91 22/18 23.1 BSS
XBSJ023713.5–522734 AGN1 0.193 1.92  < 0.06 0.11 2.71 43.52 71/87 88.9 HBSS, BSS
XBSJ030641.0–283559 AGN1 0.367 2.10  < 0.14 0.096 0.51 43.45 33/24 11.0 BSS
XBSJ031311.7–765428 AGN1 1.274 1.78  < 0.66 0.156 0.98 44.95 59/50 18.8 BSS
XBSJ031851.9–441815 AGN1 1.360 1.58 0.13 0.13 0.94 44.93 17/15 32.8 BSS
XBSJ052108.5–251913 AGN1 1.196 1.70  < 0.28 0.27 2.51 45.28 78/64 11.8 HBSS,BSS
XBSJ065839.5–560813 AGN1 0.211 1.86 0.04 0.10 0.71 43.02 66/68 54.1 BSS
XBSJ074312.1+742937 AGN1 0.312 1.98  < 0.01 0.12 9.79 44.55 190/192 51.7 HBSS, BSS
XBSJ095218.9–013643p AGN1 0.01993 1.90f 4.2 0.15 5.73 41.92 133/57 5e-6 HBSS, BSS
XBSJ100926.5+533426 AGN1 1.718 1.72 0.17 0.23 0.87 45.19 41/37 30.7 BSS
XBSJ101922.6+412049 AGN1 0.239 1.51  < 0.04 0.15 2.87 43.71 107/110 57.8 HBSS, BSS
XBSJ140100.0–110942 AGN1e 0.164 2.31 0.12 0.07 0.45 42.61 62/61 46.1 BSS
XBSJ141736.3+523028 AGN1 0.985 1.74  < 0.29 0.22 0.82 44.61 111/97 17.0 BSS
XBSJ153456.1+013033 p AGN1 0.310 2.27  < 0.30 0.09 1.13 43.65 77/62 9.7 BSS
XBSJ223547.9–255836 AGN1 0.304 1.43  < 0.03 0.19 0.91 43.43 32/32 49.5 BSS
XBSJ225118.0–175951 AGN1 0.172 2.09 0.16 0.09 1.25 43.09 95/88 28.9 BSS
XBSJ231601.7–424038 AGN1 0.383 1.74  < 0.10 0.14 0.75 43.61 56/51 29.0 BSS

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