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Table A.1.

Baseline model used for simulations of Fvar spectra.

U1-U3 O1 O2
log NH, Gal 20.98(f)

Scattered emission

log NH1 23.78(f) 23.4(f)
log ξ1 2.60(f) 2.58(f)
log NH2 22.72(f) 22.48(f)
log ξ2 1.35(f) 1.03(f)

Warm absorber

log NH1 22.40 ± 0.04
log ξ1 3.08 ± 0.01
log NH2 21.74 ± 0.01 22.33 ± 0.04
log ξ2
log NH3 22.32 ± 0.02
log ξ3 2.56 ± 0.02

cutoffpl

Γ 1.75 ± 0.01 1.90 ± 0.02 1.94 ± 0.03
Ecut 340
0.3–2 keV
Fobsc 1.1 2.2
Funobsc 4.1 4.1 5.3
2–10 keV
Fobsc 2.6 3.4
Funobsc 5.3 4.1 4.9

compTT

Tseed 1.47(f) 1.08(f)
Tc 0.54(f) 0.13(f)
τdepth 9.9(f) 22(f)
0.3–2 keV
Fobsc 0.3 0.8
2–10 keV
Funobsc 1.5 1.0 2.0

Obscurer #1

Cf1 0.47(f) 0.38(f)
log NH1 22.92 ± 0.04 22.17 ± 0.13
log ξ1 1.84(f) 1.84(f)

Obscurer #2

Cf2 0.51(f) 0.48(f)
log NH2 23.32 ± 0.03 23.40 ± 0.04
log ξ2 1.84(f) 1.84(f)

χ2/d.o.f. 2676/1883 3965/3662

Notes. Fluxes are in units of 10−11 erg s−1 cm−2 (Fobsc and Funobsc refer, respectively, to fluxes with and without the effects of the obscurer), power-law cut-off (Ecut) in units of keV, seed photon temperature (Tseed) in units of eV, plasma temperature (Tc) in units of keV, column densities (NH) in units of cm−2, ionisation parameters (defined as ξ = L1 − 1000 Ryd/ner2, where ne is the electron density, r the distance of the absorbing gas, and L1 − 1000 Ryd the ionising luminosity) in units of erg cm s−1, (f) fixed to values obtained by Mao19 and M17.

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