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Table 3

Missing AGNs: results of fitting the spectral data with both a power law in the hard X-ray energy band (2−10 keV) and an absorbed power-law model across the whole X-ray spectrum (0.3−10 keV).

ID Notes Γ d.o.f.

Power-Law model over 2 − 10 keV

26 1.020/3
42 0.680/20
53 a 1.306/11
63 a 0.829/7
65 1.156/54
71 c 2.080/112
100 1.182/47
104 0.581/9
111 b,1
125 b,2 0.655/6
129 1.270/3
161
171 0.811/3
191 1.195/217
195 1.021/299
203 0.817/4
204 a 0.220/3
214 0.958/4
241 0.810/19
275 0.897/213
318 b,1
329 c 1.910/3
338 0.802/7
355 0.008/1
357 0.556/11
ID Notes Γ d.o.f.

Absorbed Power-Law model over 0.3 − 10 keV

26 1.213/63
42 0.933/161
53 a 1.154/43
63 a 1.500/18
65 1.370/316
71 c
100 1.360/301
104 1.350/170
111 b,1 0.676/31
125 b,2 0.993/85
129 1.294/39
161 1.762/8
171 1.437/81
191 1.475/562
195 2.021/587
203 0.949/41
204 a 0.367/13
214 1.052/32
241 0.899/102
275 1.657/558
318 b,1 0.894/30
329 c
338 0.979/63
355 1.002/13
357 1.231/66

Notes. (a) The hard photon index was obtained in the energy band 1−10 keV due to low statistics; (b) the pn data is dominated by the background: (1) above 2 − 3 keV, (2) above 6 keV; (c) The soft excess is far strong (ratio  > 30) invalidating the application of PL fit across the whole X-ray spectra.

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