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Home All issues Volume 691 (November 2024) A&A, 691 (2024) A228 Full HTML
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Table B.4.

Same as Table B.3, but here we jointly fit all data from Epochs 2 to 6.

Model Parameter Epoch 1 Epoch 2 Epoch 3 Epoch 4 Epoch 5 Epoch 6
Constant CFPMB 0.96 ± 0.02 1.01 ± 0.03 0.92 ± 0.04 1.00 ± 0.06 - -
CSwift 1.00 ± 0.05 0.95 ± 0.07 0.46 ± 0.08 0.9 ± 0.1 - -
CXMM − Newton - - - 0.79 ± 0.04 - -
TBabs NH (1020 cm−2) [5.0]
powerlaw Γ - 1.38 ± 0.02 1.52 ± 0.05 1.51 ± 0.05 0 . 9 − 1.1 + 0.6 $ 0.9_{-1.1}^{+0.6} $ -
norm (keV−1cm−2s−1) - (10.0 ± 0.5)×10−4 (4.2 ± 0.4)×10−4 (2.7 ± 0.3)×10−4 (2.1 ± 1.5)×10−6 -
slimdz ṁ ( m ˙ Edd $ \dot{m}_{\mathrm{Edd}} $) - < 4.9 < 18 > 4.8 < 0.23 < 0.17
θ (°) - < 76
log(M•/M⊙) - 2 . 4 − 0.1 + 0.6 $ 2.4_{-0.1}^{+0.6} $
a• - 0 . 4 − 0.9 + 0.5 $ 0.4_{-0.9}^{+0.5} $
relxillCp θ (°) 74 ± 2 - - - - -
a• 0.98 ± 0.01 - - - - -
kTe (keV) 28 ± 8 - - - - -
Γ 1.22 ± 0.02 - - - - -
q 4 ± 2 - - - - -
log(ξ) 3.45 ± 0.06 - - - - -
AFe > 8.0 - - - - -
Reflfrac 11 − 4 + 21 $ 11_{-4}^{+21} $ - - - - -
log(ρ/cm−3) < 15.2 - - - - -
norm (erg cm−2s−1) (3 ± 2)×10−5 - - - - -
C-stat/d.o.f. 279.5/275 688.5/691

Notes. We force the slim-disk component in each epoch to have the same inclination, θ, BH mass, M•, and BH spin, a•. Since statistically the slim-disk component is not needed for Epochs 2, 3, and 5, only an upper limit on the disk accretion rate was obtained for these epochs.

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