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Table A.2.

Simultaneous fits of the two XMM-Newton and NuSTAR spectra with three different relativistic reflection models. The column density along the line-of-sight was fixed at the Galactic one, i.e. 1.27×1020 cm−2, and the inclination angle at 9.9 degrees. (a) Velocity of primary source. (b) Index of the ionisation gradient with a power-law shape. (c) The breaking radius Rbr and the height of the primary source are both expressed in ISCO units, except for the REFLKERR model for which Rbr is expressed in gravitational radius units. The data-to-model ratio for each model is reported in Fig. A.2.

Parameters RELXILLD RELXILLLPION REFLKERRD
a 0.993±0.001 0.997±0.001 ≥0.991
AFe 4.5±0.1 2.1 2.9±0.2
log Ndisc (cm−3) 17.0±0.1 17.1±0.1
β (v/c) (a) 0.07±0.01
ξ − index(b) ≤0.02

2019 Nov

q1 8.3±0.1 4.8±0.1
q2 3.4±0.1 2.3±0.1
Rbr (c) 2.6±0.1 13.4
h(c) ≤1.2
Γ 1.92±0.01 2.01±0.01
kThot (keV) 88±2
y 0.44±0.01
Ecut (keV) 300 (f) ≥872
log ξ (erg cm s−1) 3.0±0.1 2.7±0.1 2.6±0.1
3.8±0.1 1.2±0.1
normrel 9.0±0.1×10−5 0.28±0.1 6.6±0.1×10−3

2020 April

q1 8.0±0.1 4.5±0.1
q2 3.3±0.1 2.1±0.1
Rbr (c) 2.7±0.1 10.3
h(c) ≤1.1
Γ 1.84±0.01 1.88±0.01
kThot (keV) 76±2
y 0.37±0.01
Ecut (keV) 300 (f) 451
log ξ (erg cm s−1) 3.0±0.1 2.9±0.1 0.3±0.1
2.6±0.1 2.2±0.1
normrel 9.3±0.1×10−5 0.42 7.3±0.1×10−3

χ2/d.o.f. 2001.7/1618 2045.9/1621 2065.4/1616
1.24 1.26 1.28

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