A deep X-ray look to the most obscured quasar at z ∼ 3.6 and its environment

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Table 2.

Best-fit parameters derived from the empirical models.

Model	Γ	C-stat/d.o.f.	N_H	Flux_{0.5 − 2}	Flux_2 − 10	L_2 − 10
			(10²⁴ cm⁻²)	(10⁻¹⁶ erg cm⁻² s⁻¹)	(10⁻¹⁵ erg cm⁻² s⁻¹)	(10⁴⁵ erg s⁻¹)
POW^(a)	${0.2}_{- 0.3}^{+ 0.3}$ ${0.2}_{-0.3}^{+0.3}$	46.1/48	–	${5.4}_{- 2.4}^{+ 0.5}$ ${5.4}_{-2.4}^{+0.5}$	${10.9}_{- 4.8}^{+ 0.7}$ ${10.9}_{-4.8}^{+0.7}$	${0.09}_{- 0.04}^{+ 0.08}$ ${0.09}_{-0.04}^{+0.08}$
CABSPOW^(b)	(1.9)	54.8/48	${0.9}_{- 0.2}^{+ 0.2}$ ${0.9}_{-0.2}^{+0.2}$	${4.3}_{- 1.0}^{+ 0.9}$ ${4.3}_{-1.0}^{+0.9}$	${6.2}_{- 1.0}^{+ 0.8}$ ${6.2}_{-1.0}^{+0.8}$	${1.7}_{- 0.4}^{+ 0.6}$ ${1.7}_{-0.4}^{+0.6}$
REFLDOM^(c)	(1.9)	48.8/49	–	${6.3}_{- 0.7}^{+ 0.8}$ ${6.3}_{-0.7}^{+0.8}$	${6.5}_{- 0.8}^{+ 0.8}$ ${6.5}_{-0.8}^{+0.8}$	${0.10}_{- 0.01}^{+ 0.01}$ ${0.10}_{-0.01}^{+0.01}$ ^(d)

Notes. The parameters in brackets were held constant at the specified value.

^(a)

TBABS*ZPOW.

^(b)

TBABS*ZTBABS*CABS*ZPOW.

^(c)

TBABS*PEXMON.

^(d)

Luminosity of the reflected component.

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