On the driver of relativistic effect strength in Seyfert galaxies

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Table 3

Summary of spectral fit results for the GREDOS sample: continuum components.

Source	Γ	N_H,1	N_H,2	log (ξ)/C_f^a	R_nr^b	R_r^c	Abs. Model^d
		(10²² cm^-2)	(10²² cm^-2)

NGC 4507		d	7 ± 3	< 2.1		< 0.1	CW
NGC 4388			4 ± 3		0.8 ± 0.3		CW
Mrk 6			...	0.85 ± 0.02	< 0.4	< 2.9	PC
NGC 2110				...	0.9 ± 0.5	3.4 ± 0.7	DC
NGC 5252				...	< 0.1	0.4	DC
NGC 7172		13.3 ± 0.2	...	...	< 0.1		SC
1ES0241+622			...	...	< 0.6	< 0.1	SC
GRS1734-292		1.41 ± 0.02	...	...	< 0.1	< 0.4	SC
NGC 5506				< –0.27	< 0.1	< 0.1	CW
NGC 4151			...	0.853 ± 0.004		< 0.1	PC
NGC 526A			...	...	< 0.06	< 0.12	SC
MCG-05-23-016			...	...	< 0.64	< 0.10	SC

Notes.

^(a)

Ionisation parameter for the warm absorber component for model CW or covering fraction of the patchy absorber for model PC.

^(b)

Ratio of the normalisation of the non-relativistic reflection component to the primary power-law.

^(c)

Ratio of the normalisation of the relativistic reflection component to the primary power-law.

^(d)

Absorption model. Legenda: SC = single cold absorber; DC = double cold absorber; PC = partial covering; CW = cold and warm absorber.

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