Table 1.
X-ray spectral parameters of NGC 4631 X-6 in Chandra and XMM–Newton observations.
| Data label | Net Rate | NH | Γ/Tin | Γ*/T![]() |
Cstat/dof | Fx | Lx | ![]() |
![]() |
|---|---|---|---|---|---|---|---|---|---|
| (10−3 counts/s) | (1022 cm−2) | (/keV) | (/keV) | (10−13 erg cm−2 s−1) | (1039 erg s−1) | (10−13 erg cm−2 s−1) | (1039 erg s−1) | ||
| C1 | < 0.08 | ||||||||
| tbabs*tbabs*power-law | |||||||||
| C2 | 17.64 ± 0.78 | ![]() |
![]() |
![]() |
21.56/28b | ![]() |
![]() |
![]() |
![]() |
| C3 | 7.93 ± 0.59 | ![]() |
![]() |
![]() |
27.48/29 | ![]() |
![]() |
![]() |
![]() |
| C4 | 9.75 ± 0.73 | ![]() |
![]() |
![]() |
21.99/30 | ![]() |
![]() |
![]() |
![]() |
| Ccombine1 | 9.06 ± 0.47 | ![]() |
![]() |
![]() |
58.47/60 | ![]() |
![]() |
![]() |
![]() |
| C5 | 8.25 ± 0.64 | ![]() |
![]() |
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35.92/29 | ![]() |
![]() |
![]() |
![]() |
| C6 | 9.63 ± 0.81 | ![]() |
![]() |
![]() |
32.27/22 | ![]() |
![]() |
![]() |
![]() |
| C7 | 9.69 ± 0.81 | ![]() |
![]() |
![]() |
20.52/23 | ![]() |
![]() |
![]() |
![]() |
| C8 | 4.59 ± 0.39 | ![]() |
![]() |
![]() |
32.46/23 | ![]() |
![]() |
![]() |
![]() |
| Ccombine2 | 2.49 ± 0.20 | ![]() |
![]() |
![]() |
22.76/26 | ![]() |
![]() |
![]() |
![]() |
| tbabs*tbabs*diskbb | |||||||||
| C2 | ![]() |
![]() |
![]() |
17.62/28b | ![]() |
![]() |
![]() |
![]() |
|
| C3 | ![]() |
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27.22/29 | ![]() |
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![]() |
|
| C4 | ![]() |
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23.44/30 | ![]() |
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![]() |
|
| Ccombine1 | ![]() |
![]() |
![]() |
59/60 | ![]() |
![]() |
![]() |
![]() |
|
| C5 | ![]() |
![]() |
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36.04/29 | ![]() |
![]() |
![]() |
![]() |
|
| C6 | ![]() |
![]() |
![]() |
31.76/22 | ![]() |
![]() |
![]() |
![]() |
|
| C7 | ![]() |
![]() |
![]() |
17.82/23 | ![]() |
![]() |
![]() |
![]() |
|
| C8 | ![]() |
![]() |
![]() |
30.64/23 | ![]() |
![]() |
![]() |
![]() |
|
| Ccombine2 | ![]() |
![]() |
![]() |
20.85/26 | ![]() |
![]() |
![]() |
![]() |
|
| XM1 | < 2.74 | ||||||||
| XM2 | 21.57 ± 0.93 | 0.71![]() |
1.40![]() |
34.53/33 | 3.80![]() |
![]() |
– | – | |
| XM3 | < 2.11 | ||||||||
Notes. The NH of one tbabs component was fixed to the line-of-sight value of 0.013 × 1022 cm−2. The intrinsic NH (second tbabs component) was left to free to vary; for the entries marked with (*), the intrinsic NH was fixed at average values of 0.90 × 1022 cm−2 and 0.49 × 1022 cm−2 for the power-law and diskbb models, respectively. Ccombine1 and Ccombine2 correspond to combined observations C3–C4 and C9–C12, respectively. The count rate values for C9–C12 are (1.68 ± 0.38) × 10−3, (2.07 ± 0.32) × 10−3, (2.42 ± 0.35) × 10−3, and (2.57 ± 0.44)×10−3, respectively. The superscript b indicates that the corresponding spectral fits were performed using the χ2/d.o.f. statistic. Absorbed fluxes were calculated in the 0.5–8 keV energy range, while unabsorbed luminosities were derived assuming a distance of 7.6 Mpc. Quoted uncertainties correspond to the 90% confidence level for each parameter.
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