The X-ray warm absorber and nuclear obscuration in the Seyfert 1.8 galaxy ESO 113-G010

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Table 1

Best-fit parameters of the power-law continuum and two-phase warm absorber xabsmodel obtained from fitting the RGS spectrum as described in Sect. 4 and using SED E in Fig. 4.

Power law:	Γ^a		Norm^b
	2.62 ± 0.05		3.1 ± 0.1
xabs	log ξ^c	N_H^d	Flow v^e	RMS v^e
Phase 1:	3.2 ± 0.1	1.6 ± 1.0	−1100 ± 300	500 ± 300
Phase 2:	2.3 ± 0.1	0.5 ± 0.2	−700 ± 100	100 ± 40

Notes. The (1046 d.o.f.). The fitted parameter errors are quoted at 90% confidence for one interesting parameter. .

^(a)

Photon index.

^(b)

Normalisation in 10⁵¹ photons s^-1 keV^-1 at 1 keV.

^(c)

erg cm s^-1.

^(d)

10²² cm^-2.

^(e)

km s^-1

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