Table 1.
NuSTAR + Swift and Suzaku X-ray spectral fitting results.
| constant×TBabs×(partcov×TBabs)×(partcov×TBabs)×(vmcflow+gauss) | |||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| Suzaku | Count rate | nH (1022 cm−2) | covering fraction | kTmax keV | Fe/Fe⊙ | λFeKα keV | EW (Fe Kα) eV | FX | LX | Ṁ 10−9M⊙ yr−1 |
 /d.o.f |
| 402040010 | XIS0+3:0.65 | 0.12 ± 0.07a | 53 | 0.67 ± 0.01 | 6.39 ± 0.01 | 230 ± 10 | 1091 ± 10 | 5220 ± 50 | 3.7 ± 0.1 | 1.04/2116 | |
| XIS1: 0.62 | 1.4 ± 0.1b | 0.87 ± 0.03 | |||||||||
| HXD: 0.13 | 12 ± 1b | 0.60 ± 0.02 | |||||||||
| 906007010 | XIS0+3:0.61 | 0.06 ± 0.04a | 53 | 0.48 ± 0.06 | 6.41 ± 0.01 | 350 ± 10 | 1983 ± 14 | 9486 ± 60 | 6.7 ± 0.3 | 1.05/1660 | |
| XIS1:0.54 | 4.8 ± 0.4b | 0.90 ± 0.01 | |||||||||
| HXD:0.21 | 28 ± 3b | 0.74 ± 0.02 | |||||||||
| constant×TBabs×(partcov×TBabs)×(vmcflow+gauss) | |||||||||||
| Count rate | nH | Covering Fraction | kTmax | Fe/Fe⊙ | FX | LX | Ṁ |
 /d.o.f |
|||
| NuSTAR + Swift | FPMA: 0.55 | 1.7 ± 0.2a | 64 ± 5 | 0.44 ± 0.07 | 1376 ± 10 | 6582 ± 50 | 4.3 ± 0.4 | 1.12/977 | |||
| FPMB: 0.59 | 29 ± 5 | 0.51 ± 0.03 | |||||||||
| XRT: 0.19 | |||||||||||
| constant×TBabs×(partcov×TBabs)×(reflect×vmcflow+gauss) | |||||||||||
| Count rate | nH | Covering fraction | kTmax | Fe/Fe⊙ | Ref. Amplitude | FX | LX | Ṁ |
 /d.o.f. |
||
| 1.3 ± 0.3a | 53 ± 4 | 0.46 ± 0.06 | 0.77 ± 0.21 | 1030 ± 7 | 4925 ± 30 | 4.1 ± 0.2 | 1.07/976 | ||||
| 12 + 5 | 0.6 ± 0.1 | ||||||||||
Notes. X-ray flux and luminosity, in units of 10−13 ergs s−1 cm−2 and 1031 ergs s−1, respectively, are calculated in the 0.3−80.0keV energy band. Iron abundances in units of abundances from Wilms et al. (2000). Luminosities and Ṁ are determined assuming a distance of 2kpc.
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