Suzaku and SWIFT-BAT observations of a newly discovered Compton-thick AGN

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Table 1

Best-fit values of the mildly and heavily Compton-thick AGN models.

Mildly Compton-thick AGN models
Model	Γ	N_H	Refl.	Scatt.	E₁	σ	E₂	σ	χ²/d.o.f.	L(2–10 keV)
		[10²² cm^-2]	frac.	frac.	keV	eV	keV	eV		10⁴² erg s^-1

One line	2.4 ± 0.5	145 ± 10	0.7	<1%	6.37 ± 0.01	<50	–	–	265.5/190	70
Two lines	2.4 ± 0.5	146	0.7	<1%	6.37 ± 0.01	<50	6.92	<50	255.9/188	70

Model	Γ	N_H	ξ	E₂	σ	χ²/d.o.f.	L(2–10 keV)
		[10²² cm^-2]	erg cm s^-1	keV	eV		10⁴² erg s^-1

Reflionx	2.5 ± 0.5	130 ± 30	29	6.91	< 50	226.3/190	50

Heavily Compton-thick AGN model
Model	Γ	N_H	ξ	E₂	σ	χ²/d.o.f.	L(2–10 keV)
		[10²² cm^-2]	erg cm s^-1	keV	eV		10⁴² erg s^-1

Reflionx	2.2 ± 0.5	> 1000^a	66	6.93	<50	218.9/189	>10³^b

Notes.

^(a)

This value of N_H is not an output of the fit, but it is an assumption that we made in this model.

^(b)

This value of L(2–10 keV) has been derived assuming that the observed luminosity is less than few percents of the intrinsic one.

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