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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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