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Table 4.
Outcomes of the best-fit model for each available data set.
Telescope | ObsID | kT | ΓWC | kWC | Γ | k | I | ![]() |
---|---|---|---|---|---|---|---|---|
[keV] | [10−3
![]() |
[10−3
![]() |
[10−6
![]() |
|||||
XMM-Newton | 0201090201 | 0.46![]() |
2.69![]() |
1.11![]() |
1.62![]() |
2.26![]() |
9.5![]() |
0.96 |
Swift-XRT | Combined | 0.70![]() |
2.82![]() |
0.92![]() |
1.62![]() |
2.65![]() |
< 19.0 | 0.95 |
XMM-Newton | 0554920301 | 0.43![]() |
2.60![]() |
1.60![]() |
1.69![]() |
3.14![]() |
10.4![]() |
1.10 |
Chandra | 12868 | 0.26![]() |
1.62![]() |
1.66![]() |
1.88![]() |
4.78![]() |
< 17.0 | 1.22 |
NuSTAR | 60160087001 | – | – | – | 1.77![]() |
0.49![]() |
6.1![]() |
0.67 |
NuSTAR | 60160087002 | – | – | – | 1.69![]() |
0.51![]() |
3.11![]() |
1.11 |
NuSTAR | 60301022003 | – | – | – | 1.73![]() |
0.40![]() |
1.06![]() |
1.00 |
Chandra | Combined | 0.19![]() |
< 3.42 | 0.03![]() |
1.60![]() |
0.44![]() |
3.5![]() |
1.07 |
Swift-XRT | Combined | 0.21 (fix) | 1.85 (fix) | < 0.03 | 1.58![]() |
0.37![]() |
7.0![]() |
0.89 |
NuSTAR | 60301022005 | – | – | – | 1.69![]() |
0.51![]() |
3.6![]() |
1.09 |
XMM-Newton | 0821240201 | 0.21![]() |
1.85![]() |
0.07![]() |
1.62![]() |
0.52![]() |
6.6![]() |
1.09 |
XMM-Newton | 0821240301 | 0.14![]() |
< 1.68 | 0.07![]() |
1.63![]() |
0.26![]() |
2.9![]() |
1.02 |
Notes. kT is the warm corona temperature, ΓWC the WC power-law spectral index, kWC the WC power-law normalization, Γ the primary power-law spectral index related to the HC, k the primary power-law normalization, and is I the Fe Kα emission line intensity.
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