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Table 2.

Fitting results for X3 with Kerrbb+reflection+gauss model.

Model relxill+cutpl relxillNS+cutpl
Parameters
constLE 1 . 054 0.024 + 0.029 $ 1.054^{+0.029}_{-0.024} $ 1 . 058 0.028 0.032 $ 1.058^{0.032}_{-0.028} $
a 0.998 * 0.998 *
Incl(°) < 4.98 < 8.12
M(M) 6 . 28 0.09 + 0.07 $ 6.28^{+0.07}_{-0.09} $ 5 . 52 0.60 + 0.43 $ 5.52^{+0.43}_{-0.60} $
(× 10−2) 54 . 95 1.47 + 1.71 $ 54.95^{+1.71}_{-1.47} $ 41 . 20 5.17 + 5.42 $ 41.20^{+5.42}_{-5.17} $
Tin (keV) 0 . 747 0.44 + 0.052 $ 0.747^{+0.052}_{-0.44} $
Γ 2.79 ± 0.07 2 . 00 0.09 + 0.08 $ 2.00^{+0.08}_{-0.09} $
Log(ξ) < 1.96 2 . 16 0.07 0.11 $ 2.16^{0.11}_{0.07} $
§AFe 2 . 35 1.07 + 0.26 $ 2.35^{+0.26}_{-1.07} $ 4 . 84 0.55 1.16 $ 4.84^{1.16}_{-0.55} $
Ecut/kTe (keV) 60.00 * 60.00 *
Log (n) 15 * 19 *
Normr(×10−3) 81 . 01 37.70 + 25.85 $ 81.01^{+25.85}_{-37.70} $ 30 . 73 7.79 + 5.72 $ 30.73^{+5.72}_{-7.79} $
NormPL/NormCP(×10−2) < 0.82 6 . 72 1.02 + 1.26 $ 6.72^{+1.26}_{-1.02} $
Egau(keV) 6 . 75 0.04 + 0.03 $ 6.75^{+0.03}_{-0.04} $ 6.79 ± 0.04
σgau(keV) 0 . 11 0.07 + 0.05 $ 0.11^{+0.05}_{-0.07} $ 0 . 14 0.07 + 0.05 $ 0.14^{+0.05}_{-0.07} $
Normgau(10−3) 1 . 09 0.21 + 0.22 $ 1.09^{+0.22}_{-0.21} $ 1 . 20 0.25 + 0.31 $ 1.20^{+0.31}_{-0.25} $
χ2/ν 1134.74/1000 1104.78/999

(1.13) (1.10)
AIC 1159.052 1131.145

Notes.

*

A parameter fixed in the fit.

Ecut corresponds to the relxill and cutoff power-law, while kTe corresponds to the relxillNS and NthComp.

§

iron abundance in solar units.

(★)

logarithmic value of the disk density (in cm−3).

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