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Table 3.

Similar to Table 2 but for 2019-12-05.

Model M1 M2 M3 M4
Statistics

Cstat 3600.1 3580.5 3608.3 3497.5
Cexpt 3383 ± 81 3384 ± 81 3384 ± 81 3388 ± 81
d.o.f. 3054 3054 3054 3051

Disk blackbody

Norm (cm−2) 4.0 × 1026 (f) 4.0 × 1026 (f) 4.0 × 1026 (f) 4.0 × 1026 (f)
T (eV) 10.2 (f) 10.2 (f) 10.2 (f) 10.2 (f)

Comptonisation

Norm (ph s−1 keV−1)
Tseed (eV) 10.2 (c) 10.2 (c) 10.2 (c) 10.2 (c)
Tc (keV) 0.06 (f) 0.06 (f) 0.06 (f) 0.06 (f)
τ 30 (f) 30 (f) 30 (f) 30 (f)

Power-law

Norm (ph s−1 keV−1) (9.0 ± 0.4)×1049 (6.7 ± 0.4)×1049 (7.3 ± 0.5)×1049 (22.4 ± 3.7)×1049
Γ 1.82 ± 0.03 1.69 ± 0.03 1.70 ± 0.03 2.02 ± 0.04

Reflection

Norm (ph s−1 keV−1) 9.0 × 1049 (c) 38.7 × 1049 (f) 29.9 × 1049 (f) 22.4 × 1049 (c)
Γ 1.82 (c) 1.83 (f) 1.74 (f) 2.02 (c)
scale 1.41 ± 0.14 0.30 ± 0.02 0.29 ± 0.02 0.83 ± 0.11

Obscurer

NH (1022 cm−2) 10.5 ± 0.1 ,
log ξ (erg s−1 cm) 2.6 ± 0.2 2.0 ± 0.6 ,
0.72 ± 0.02 0.64 ± 0.04 0.67 ± 0.04 0.54 ± 0.05, 0.75 ± 0.02

Notes. Models M1, M2, and M3 use one photoionized component for the obscurer, while Model M4 uses two photoionized components. The continuum of the reflection component is coupled to that of the power-law component observed on 2019-12-05 for Model M1 and M4, 2016-12-05 for Model M2 (as in Paper I), and 2019-11-15 for Model M3.

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