Mildly obscured active galaxies and the cosmic X-ray background

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Table 3

Comparison of Compton-thick estimates with previous works using BAT spectral templates derived from the samples based on N_H.

Paper	XLF^a	N _H ^b	Templates	CTKR^c	Datasets^d	Flux^e

G07	H05	G07	G07	24 ÷ 26	ASCA SIS, HEAO1	10
			BAT			< 0.3	>2

T09	U03	T09	T09	24 ÷ 25	XMM, Chandra, BAT, INTEGRAL	4
			BAT			< 1	>2

U14	U14	U14	U14	24 ÷ 26	ASCA SIS, BAT, INTEGRAL	9 ± 4
			BAT			9.5 ± 0.5	1.74

Notes. For each paper we report both the CTK flux estimated in the original paper and the one estimated with the BAT templates, togheter with the of the fit.

^(a)

XLF used in the corresponding paper.

^(b)

N_H distribution used in the corresponding paper.

^(c)

log (N_H) range of CTK AGN considered in the synthesis.

^(d)

Datasets used to compare with the CXB synthesis.

^(e)

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

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