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

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Table 3.

Best-fit parameters derived from geometry-dependent models.

Model	C-stat/d.o.f.	N_H	Flux_{0.5 − 2}	Flux_2 − 10	L_2 − 10
		(10²⁴ cm⁻²)	(10⁻¹⁶ erg s⁻¹)	(10⁻¹⁵ erg s⁻¹)	(10⁴⁵ erg s⁻¹)
BORSPHERE^(a)	58.3/48	${1.3}_{- 0.4}^{+ 0.4}$ ${1.3}_{-0.4}^{+0.4}$	${7.1}_{- 0.6}^{+ 5.8}$ ${7.1}_{-0.6}^{+5.8}$	${5.0}_{- 1.4}^{+ 0.5}$ ${5.0}_{-1.4}^{+0.5}$	${1.4}_{- 0.3}^{+ 0.4}$ ${1.4}_{-0.3}^{+0.4}$
BORUS^(b)	54.6/48	${0.9}_{- 0.2}^{+ 0.2}$ ${0.9}_{-0.2}^{+0.2}$	${4.4}_{- 1.0}^{+ 0.9}$ ${4.4}_{-1.0}^{+0.9}$	${6.2}_{- 1.0}^{+ 0.8}$ ${6.2}_{-1.0}^{+0.8}$	${1.3}_{- 0.3}^{+ 0.4}$ ${1.3}_{-0.3}^{+0.4}$
MYTORUS^(c)	48.6/48	> 6.9	${4.3}_{- 0.3}^{+ 2.0}$ ${4.3}_{-0.3}^{+2.0}$	${10.0}_{- 1.2}^{+ 1.2}$ ${10.0}_{-1.2}^{+1.2}$ ^(d)	> 10.0 ^(e)

Notes.

^(a)

TBABS(BORSPHERE+ZTBABS*CABS*ZCUTOFFPL).

^(b)

TBABS(BORUS+ZTBABS*CABS*ZCUTOFFPL).

^(c)

TBABS(ZPOW*MYTZ+MYTS+ MYTL).

^(d)

The N_H is frozen to the best-fit value during the flux calculation.

^(e)

The value reflects the lower limit on N_H.

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