The hyperluminous Compton-thick z ∼ 2 quasar nucleus of the hot DOG W1835+4355 observed by NuSTAR

L. Zappacosta; E. Piconcelli; F. Duras; C. Vignali; R. Valiante; S. Bianchi; A. Bongiorno; F. Fiore; C. Feruglio; G. Lanzuisi; R. Maiolino; S. Mathur; G. Miniutti; C. Ricci

doi:10.1051/0004-6361/201732557

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Volume 618 (October 2018)

A&A, 618 (2018) A28

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Table 1.

X-ray spectral fitting: derived parameters.

Model^a	C-stat/d.o.f.	Γ	N_H (10²⁴ cm⁻²)	Γ_sc	f_sc(%)	L_2–10 (10⁴⁵ erg s⁻¹)	L_10–40 (10⁴⁵ erg s⁻¹)
CABSPow^b	147/154	(1.9)		(=Γ)
REFLDOM^c	149/156	(1.9)	–	(=Γ_pexmon)	(2)	0.2^f	0.6^f
MYTOR^d	149/155	(1.9)		(=Γ)
BNSPHERE^e	149/155	(1.9)		(=Γ)

Notes.

^(a)

See Sects. 3.1, 3.1.1 and 3.2.

^(b)

, where , are Gaussian lines to parametrize the neutral and ionized Fe Kα line;

^(c)

;

^(d)

WABS(ZPOWERLW_SC + ZPOWERLW*MYTZ+MYTS+MYTL);

^(e)

WABS(ZPOWERLW_sc + BNTORUS);

^(f)

observed luminosity not corrected for absorption.

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