Multiwavelength properties of changing-state active galactic nuclei - I. The evolution of soft excess and X-ray continuum

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Table B.5.

Broadband X-ray properties of IRAS 23226–3843

Epoch	$log L_{PC}^{2 - 10}$ $Mathematical equation: $ \log L_{\mathrm{PC}}^{\mathrm{2-10}} $$	$log L_{SE}^{0.5 - 2}$ $Mathematical equation: $ \log L_{\mathrm{SE}}^{\mathrm{0.5-2}} $$	Γ	E_cut	log R_S	kT_BB	log Q	log λ_Edd	χ²/dof
				(keV)		(eV)
(1)	(2)	(3)	(4)	(5)	(6)	(7)	(8)	(9)	(10)
E1	42.49 ± 0.06	< 41.14	1.89 ± 0.03	> 51	−0.44 ± 0.09	120^*	−1.35 ± 0.06	−2.34 ± 0.08	158/201
E2	42.10 ± 0.03	< 41.10	1.94 ± 0.05	200^*	−	120^*	< − 1.00	−2.74 ± 0.06	86/85
E3	42.02 ± 0.03	41.03 ± 0.43	2.04 ± 0.03	> 55	−1.74 ± 0.19	112 ± 19	−0.99 ± 0.43	−2.82 ± 0.06	157/168
E4	43.10 ± 0.01	42.06 ± 0.14	1.91 ± 0.02	$136_{- 84}^{+ 99}$ $Mathematical equation: $ 136 ^{+99}_{-84} $$	−0.40 ± 0.09	133 ± 13	−1.04 ± 0.14	−1.66 ± 0.05	1569/1489

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