The role of molecular gas in the nuclear regions of IRAS 00183-7111 - ALMA and X-ray investigations of an ultraluminous infrared galaxy

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Volume 616 (August 2018)

A&A, 616 (2018) A127

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Table 5.

Best-fit X-ray parameters obtained using the X ILLVER model.

	logξ^a	Γ^b	N_H^c	Luminosity^e
Chandra		1.9 (fixed)	9.0 ± 2.0
XMM-Newton		1.9 (fixed)
NuSTAR	3.2 ± 0.3	1.9 (fixed)	<10

Broad-band spectral parameters (0.5–24 keV)

	2.6 ± 0.15	1.9 (fixed)		4.2 ± 0.1

Notes.

^(a)

Ionization parameter derived from the best fit, with its errors quoted at the 90% confidence level.

^(b)

Photon index derived from the best fit with errors quoted at the 90% confidence level.

^(c)

Intrinsic N_H column density in units of 10²² cm⁻² and obtained from the best-fit model.

^(d)

Observed-frame 2–10 keV flux from the best spectral fitting in units of 10⁻¹³ erg cm⁻² s⁻¹.

^(e)

Intrinsic rest-frame 2–10 keV luminosity from the best spectral fitting in units of 10⁴³ erg s⁻¹.

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