Mildly obscured active galaxies and the cosmic X-ray background

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Table 4

Compton-thick estimates obtained using BAT spectral templates derived from the samples based on absorption, fitting only the CTK density, for various combination of XLFs and N_H distributions.

XLF	N _H	Flux^a	f _CTK ^b

H05	G07	3.0 ± 0.5	24%	2.12
U03	T09		< 5%	1.92
U14	U14	11.5 ± 0.5	47%	1.92
M15	U14	8.0 ± 0.5	47%	1.64

Notes. The datasets used in the fitting process are ROSAT, Swift/XRT, Swift/BAT, and INTEGRAL.

^(a)

Flux at the peak of the CTK component in the synthesis, in unit of keV cm^-2 s^-1 Str^-1.

^(b)

Fraction of CTK (log (N_H)> 24) over all AGN (any N_H, CTK themselves included).

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