Multi-zone warm and cold clumpy absorbers in three Seyfert galaxies

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Table 4:

Results obtained from the X-ray spectral analysis of UGC 3142.
Instruments	Energy	$\chi^{2}$ (d.o.f.)	$\Gamma$	$N_{\rm H}$	$N_{\rm H}^1$	f¹	$N_{\rm H}^2$	f²
	[keV]			[ $10^{20}\rm ~cm^{-2}$ ]	[ $10^{22}\rm ~cm^{-2}$ ]		[ $10^{22}\rm ~cm^{-2}$ ]
EPIC^a	0.3-10	1488 (1028)	$0.9^{\rm +0.1}_{-0.1}$	$1.4^{\rm +0.1}_{-0.1}$	-	-	-	-
EPIC^b	0.3-10	1080 (1027)	$1.13^{\rm +0.04}_{-0.05}$	0.19	$2.1^{\rm +0.1}_{-0.1}$	$0.92^{\rm +0.01}_{-0.01}$	-	-
EPIC^c	0.3-10	994 (1022)	$1.4^{\rm +0.1}_{-0.1}$	0.19	$1.4^{\rm +0.2}_{-0.2}$	$0.92^{\rm +0.01}_{-0.02}$	$5^{\rm +1}_{-1}$	$0.57^{\rm +0.08}_{-0.09}$
(EPIC + ISGRI + BAT)^c	0.3-110	1011 (1034)	$1.5^{\rm +0.1}_{-0.1}$	0.19	$1.4^{\rm +0.3}_{-0.4}$	$0.92^{\rm +0.02}_{-0.06}$	$4^{\rm +2}_{-1}$	$0.6^{\rm +0.2}_{-0.1}$

Notes. The data were modeled with an absorbed power law model (a), a power law absorbed by Galactic cold matter plus a layer of partially absorbing neutral material (b), and a power law absorbed by Galactic cold matter and two layers of partially absorbing neutral material, plus a Gaussian K $\alpha$ iron line (c). EPIC includes PN, MOS1 and MOS2 data.

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