The XMM-Newton Wide Angle Survey (XWAS): the X-ray spectrum of type-1 AGN

S. Mateos; F. J. Carrera; M. J. Page; M. G. Watson; A. Corral; J. A. Tedds; J. Ebrero; M. Krumpe; A. Schwope; M. T. Ceballos

doi:10.1051/0004-6361/200913187

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Volume 510 (February 2010)

A&A, 510 (2010) A35

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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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