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Table C.1.

Parameter GTI 1 (soft HR) GTI 2 (hard HR) Hard HR average spectrum
NuSTAR + XMM-Newton + XRISM NuSTAR + XRISM XRISM
CFPMA fixed to 1 fixed to 1
CFPMB 1.011 ± 0.003 1.010 ± 0.005
CEPIC − pn 0.879 ± 0.003
CResolve 0.943 ± 0.005 1 . 003 0.007 + 0.007 $ 1.003^{+0.007}_{-0.007} $ fixed to 1
NH, ISM(1022cm−2) fixed to 0.371 fixed to 0.371 fixed to 0.371
NH(1022cm−2) 7 . 46 0.17 + 0.18 $ 7.46^{+0.18}_{-0.17} $ 25 . 04 0.96 + 1.00 $ 25.04^{+1.00}_{-0.96} $ 31 . 15 1.07 + 1.10 $ 31.15^{+1.10}_{-1.07} $
CF 0 . 912 0.003 + 0.004 $ 0.912^{+0.004}_{-0.003} $ 0.882 ± 0.008 0.876 ± 0.007
Γ 0.91 ± 0.01 1.15 ± 0.02 0.90 ± 0.04
K ( ph keV 1 cm 2 s 1 ) $ K \ (\rm{ph \ keV^{-1} cm^{-2} s^{-1}}) $ 0.322 ± 0.011 0.245 ± 0.013 0.096 ± 0.007
Ecut (keV) 19 . 87 1.13 + 1.07 $ 19.87^{+1.07}_{-1.13} $ 20 . 02 1.39 + 1.47 $ 20.02^{+1.47}_{-1.39} $
Efold (keV) 13 . 12 0.42 + 0.46 $ 13.12^{+0.46}_{-0.42} $ 13 . 14 0.35 + 0.38 $ 13.14^{+0.38}_{-0.35} $
E10 keV(keV) 9.5 ± 0.2 10.3 ± 0.2 9.3 ± 0.2
d10 keV(keV) 4 . 63 0.25 + 0.26 $ 4.63^{+0.26}_{-0.25} $ 0 . 69 0.13 + 0.12 $ 0.69^{+0.12}_{-0.13} $ 0 . 87 0.21 + 0.20 $ 0.87^{+0.20}_{-0.21} $
σ10 keV (keV) 4 . 85 0.24 + 0.26 $ 4.85^{+0.26}_{-0.24} $ 2.77 ± 0.29 1 . 42 0.21 + 0.21 $ 1.42^{+0.21}_{-0.21} $
ECRSF, F (keV) 23 . 01 0.32 + 0.30 $ 23.01^{+0.30}_{-0.32} $ 24 . 34 0.88 + 0.82 $ 24.34^{+0.82}_{-0.88} $
σCRSF, F (keV) 0.5 × σCRSF, H 0.5 × σCRSF, H
dCRSF, F (keV) 8 . 92 0.40 + 0.41 $ 8.92^{+0.41}_{-0.40} $ 0 . 84 0.28 + 0.27 $ 0.84^{+0.27}_{-0.28} $
ECRSF, H (keV) 55 . 67 0.63 + 0.62 $ 55.67^{+0.62}_{-0.63} $ 53 . 14 0.87 + 0.97 $ 53.14^{+0.97}_{-0.87} $
σCRSF, H (keV) 14 . 79 0.40 + 0.38 $ 14.79^{+0.38}_{-0.40} $ 8 . 41 0.77 + 0.79 $ 8.41^{+0.79}_{-0.77} $
dCRSF, H(keV) 68 . 3 4.8 + 5.0 $ 68.3^{+5.0}_{-4.8} $ 17 . 5 2.1 + 1.9 $ 17.5^{+1.9}_{-2.1} $
ENe(keV) 1.18 ± 0.01
A Ne ( ph s 1 cm 2 ) $ A_{{\mathrm{Ne}}} (\rm{ph \, s^{-1} \, cm^{-2}}) $ 0 . 357 0.018 + 0.015 $ 0.357^{+0.015}_{-0.018} $
σNe(keV) 0 . 993 0.007 + 0.005 $ 0.993^{+0.005}_{-0.007} $
EMg(keV) 1.30 ± 0.01
AMg (ph s−1 cm−2) 0 . 506 0.031 + 0.033 $ 0.506^{+0.033}_{-0.031} $
σMg(keV) 0 . 424 0.005 + 0.004 $ 0.424^{+0.004}_{-0.005} $
EFe Kα2(keV) 6 . 3970 0.0010 + 0.0009 $ 6.3970^{+0.0009}_{-0.0010} $ 6 . 3959 0.0016 + 0.0015 $ 6.3959^{+0.0015}_{-0.0016} $ 6.3905 ± 0.0008
AFe Kα2(ph s−1 cm−2) ( 1 . 54 0.09 + 0.01 ) × 10 3 $ (1.54^{+0.01}_{-0.09})\times10^{-3} $ ( 1 . 14 0.19 + 0.20 ) × 10 3 $ (1.14^{+0.20}_{-0.19})\times 10^{-3} $ (0.71 ± 0.10)×10−3
σFe Kα2(keV) ( 9 . 51 0.52 + 0.40 ) × 10 3 $ (9.51^{+0.40}_{-0.52})\times10^{-3} $ ( 8 . 39 0.96 + 0.89 ) × 10 3 $ (8.39^{+0.89}_{-0.96})\times 10^{-3} $ ( 4 . 80 0.76 + 0.78 ) × 10 3 $ (4.80^{+0.78}_{-0.76})\times 10^{-3} $
EFe Kα1(keV) 6.4048 ± 0.0007 6.4050 ± 0.0006 6.4041 ± 0.0004
AFe Kα1(ph s−1 cm−2) ( 0 . 36 0.09 + 0.10 ) × 10 3 $ (0.36^{+0.10}_{-0.09})\times10^{-3} $ (0.48 ± 0.15)×10−3 ( 1 . 14 0.10 + 0.09 ) × 10 3 $ (1.14^{+0.09}_{-0.10})\times10^{-3} $
σFe Kα1(keV) ( 1 . 81 0.55 + 0.59 ) × 10 3 $ (1.81^{+0.59}_{-0.55})\times10^{-3} $ ( 2 . 60 0.71 + 0.83 ) × 10 3 $ (2.60^{+0.83}_{-0.71})\times 10^{-3} $ ( 4 . 12 0.37 + 0.38 ) × 10 3 $ (4.12^{+0.38}_{-0.37})\times 10^{-3} $
EFe Kβ(keV) 7 . 0637 0.0026 + 0.0027 $ 7.0637^{+0.0027}_{-0.0026} $ 7 . 0634 0.0011 + 0.0010 $ 7.0634^{+0.0010}_{-0.0011} $ 7.0630 ± 0.0014
AFe Kβ(ph s−1 cm−2) (0.21 ± 0.04)×10−3 (0.09 ± 0.03)×10−3 ( 0 . 23 0.03 + 0.04 ) × 10 3 $ (0.23^{+0.04}_{-0.03})\times10^{-3} $
σFe Kβ(keV) ( 7 . 10 2.65 + 2.51 ) × 10 3 $ (7.10^{+2.51}_{-2.65}) \times 10^{-3} $ ( 0 . 84 0.82 + 1.54 ) × 10 3 $ (0.84^{+1.54}_{-0.82})\times 10^{-3} $ ( 8 . 04 1.48 + 1.35 ) × 10 3 $ (8.04^{+1.35}_{-1.48})\times10^{-3} $
ENi Kα(keV) 7.4513 ± 0.0001 7 . 4475 0.0035 + 0.0034 $ 7.4475^{+0.0034}_{-0.0035} $ 7.4771 ± 0.0019
ANi Kα(ph s−1 cm−2) ≤0.04 × 10−3 ≤3 × 10−6 ( 0 . 06 0.02 + 0.03 ) × 10 3 $ (0.06^{+0.03}_{-0.02})\times10^{-3} $
σNi Kα (keV) ≤0.26 × 10−3 ≤0.63 × 10−3 ( 3 . 63 2.65 + 2.85 ) × 10 3 $ (3.63^{+2.85}_{-2.65})\times10^{-3} $
C-stat(a) 1.37 1.21 1.17

(a) The parameters derived from our variational inference analysis with jaxspec were loaded in ISIS to compute the equivalent C-stat to allow for frequentist goodness of fit assessment.

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