Warm absorber outflows in radio-loud active galactic nucleus 3C 59

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Table 1.

Best-fit parameters of SED models and warm absorbers for 3C 59.

Component	Model	Parameter	Symbol	Value
Disk blackbody component	`dbb`	Normalization	A (10²⁵ m²)	1.34 (scaled)
(NIR-optical-UV)		Temperature	kT_BB (eV)	3.4 (fixed)

Warm Comptonization component	`comt`	Normalization	A (10⁵⁶ ph s⁻¹ keV⁻¹)	$4 . 01_{- 1.17}^{+ 1.71}$ $4.01^{+1.71}_{-1.17}$
(soft X-ray excess)		Seed photons temperature	kT₀ (eV)	3.4 (fixed)
		Plasma temperature	kT₁ (eV)	$89 . 00_{- 4.71}^{+ 4.86}$ $89.00^{+4.86}_{-4.71}$
		Optical depth	τ	30 (fixed)

X-ray power-law component	`pow`	Normalization	A (10⁵² ph s⁻¹ keV⁻¹)	$5 . 93_{- 0.16}^{+ 0.21}$ $5.93^{+0.21}_{-0.16}$
		Photon index	Γ	1.63 ± 0.02

Neutral reflection component	`refl`	Incident power-law normalization	A (10⁵² ph s⁻¹ keV⁻¹)	5.94 (coupled)
		Incident power-law photon index	Γ	1.63 (coupled)
		Reflection scale	s	0.21 ± 0.06

Galactic neutral gas	`hot`	Hydrogen column density	N_H (10²⁰ cm⁻²)	6.59 (fixed)
		Electron temperature	kT_e (eV)	0.001 (fixed)

High-ionization warm absorber (WA_H)	`pion`	Hydrogen column density	N_H (10²² cm⁻²)	$0 . 69_{- 0.17}^{+ 0.31}$ $0.69^{+0.31}_{-0.17}$
		log of ionization parameter	log [ξ (erg cm s⁻¹)]	$2 . 65_{- 0.09}^{+ 0.10}$ $2.65^{+0.10}_{-0.09}$
		Turbulent velocity	σ_v	$175_{- 87}^{+ 93}$ $175^{+93}_{-87}$
		Outflowing velocity	v_out (km s⁻¹)	$- 528_{- 222}^{+ 163}$ $-528^{+163}_{-222}$

Low-ionization warm absorber (WA_L)	`pion`	Hydrogen column density	N_H (10²² cm⁻²)	$0 . 31_{- 0.03}^{+ 0.04}$ $0.31^{+0.04}_{-0.03}$
		log of ionization parameter	log [ξ (erg cm s⁻¹)]	1.65 ± 0.11
		Turbulent velocity	σ_v	$94_{- 30}^{+ 36}$ $94^{+36}_{-30}$
		Outflowing velocity	v_out (km s⁻¹)	$- 228_{- 122}^{+ 121}$ $-228^{+121}_{-122}$

Statistical results		Best-fit Cash statistic	C-stat	2076.9
		Expected Cash statistic	C-expt	1755.9
		Degree of freedom	DoF	1699

Intrinsic luminosity		0.3−10 keV luminosity	L_{0.3 − 10 keV} (erg s⁻¹)	5.19 × 10⁴⁴
		2−10 keV luminosity	L_{2 − 10 keV} (erg s⁻¹)	2.82 × 10⁴⁴
		1−1000 Ryd ionizing luminosity	L_ion (erg s⁻¹)	1.79 × 10⁴⁵
		Bolometric luminosity	L_bol (erg s⁻¹)	3.45 × 10⁴⁵

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