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Table 2:

Summary of the results of the spectral fitting of the type-1 AGN stacked spectra.

${\langle z \rangle}$
${\rm\Gamma_{best-fit}}$ ${\it kT}_{{\rm best-fit}}$ ${\rm\Gamma_{2-10~keV}}$
(1) (2) (3) (4)
0.31 1.69 $\pm$ 0.03 0.11 $\pm$ 0.01 1.60 $\pm$ 0.07
0.74 2.02 $\pm$ 0.04 0.09 $\pm$ 0.01 1.83 $\pm$ 0.10
0.94 1.97 $\pm$ 0.03 - 1.96 $\pm$ 0.08
1.19 2.01 $\pm$ 0.03 - 1.93 $\pm$ 0.04
1.45 1.93 $\pm$ 0.06 - 2.01 $\pm$ 0.17
1.74 1.99 $\pm$ 0.05 - 1.91 $\pm$ 0.11
2.01 1.81 $\pm$ 0.05 - 1.81 $\pm$ 0.12
2.56 1.81 $\pm$ 0.05 - 1.77 $\pm$ 0.20

Notes. (1) Mean redshift in bin. (2) Best-fit ${\Gamma }$ value. (3) Rest-frame temperature of the blackbody model (in keV) used to fit the soft excess component. (4) Best-fit ${\Gamma }$ from a power-law fitting in the 2-10 keV rest-frame band. Errors are 90% confidence.


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