Revealing the burning and soft heart of the bright bare active galactic nucleus ESO 141-G55: X-ray broadband and SED analysis

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Volume 689 (September 2024)

A&A, 689 (2024) A336

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Table C.1.

SED fits (UV to 10 keV) of the 2007#4 XMM-Newton-pn spectrum of ESO141-G55 with the baseline model RELAGN+REFLKERRD.

Parameters	2007#4
a	0(f)
θ (degrees)	43(f)
log ṁ	−1.01 $_{- 0.02}^{+ 0.03}$ $^{+0.03}_{-0.02}$
kT_hot (keV)	136 (f)
τ_hot	0.47 $_{- 0.07}^{+ 0.13}$ $^{+0.13}_{-0.07}$
Γ_hot	2.05 $_{- 0.06}^{+ 0.05}$ $^{+0.05}_{-0.06}$
R_hot (R_g)	19 $_{- 1}^{+ 2}$ $^{+2}_{-1}$
kT_warm (keV)	0.40 $_{- 0.10}^{+ 0.14}$ $^{+0.14}_{-0.10}$
Γ_warm	2.82 $_{- 0.09}^{+ 0.13}$ $^{+0.13}_{-0.09}$
R_warm (R_g)	51 $_{- 8}^{+ 12}$ $^{+12}_{-8}$
log ξ	0.6(f)
A_Fe	1.4(f)
norm_reflkerrd (×10⁻³)	4.8 $_{- 1.3}^{+ 0.7}$ $^{+0.7}_{-1.3}$

$F_{0.001 - 100 keV}^{unabs}$ $F^{\mathrm{unabs}}_{\mathrm{0.001-100\,keV}}$ ^(a) (erg cm⁻² s⁻¹)	5.0×10⁻¹⁰
$L_{0.001 - 100 keV}^{unabs}$ $L^{\mathrm{unabs}}_{\mathrm{0.001-100\,keV}}$ ^(a) (erg s⁻¹)	1.7×10⁴⁵
χ²/d.o.f.	518.3/440

Notes.

^(a)

Source flux and luminosity corrected from Galactic absorption and reddening. (f) means that the value was fixed to that found for the 2022 observation (Table 6).

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