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Table 1.
Best-fit parameters of the 3−10 keV fit of the joint XMM+NuSTAR data.
Parameter | Value | Value |
---|---|---|
(XMM) | (NuSTAR) | |
Γ | 1.66 ± 0.02 | |
Normalization | (1.29 ± 0.05)×10−3 | |
Cpn-MOS12 | 1.061 ± 0.014 | |
Cpn-FPMA | 0.89 ± 0.02 | |
Cpn-FPMB | 0.94 ± 0.02 | |
Fe Kα line (Δχ2/d.o.f. = −137/−3) | ||
E (keV) |
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|
N (ph cm−2 s−1) | (4.5 ± 0.6)×10−6 | (3.3 ± 2.5)×10−6 |
EW (eV) | 55 ± 6 | 38 ± 30 |
Fe XXV He-α line (Δχ2/d.o.f. = −9/−3) | ||
E (keV) |
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|
N (ph cm−2 s−1) | (0.9 ± 0.6)×10−6 | < 1.5 × 10−6 |
EW (eV) | 12 ± 8 | < 18 |
Fe Kβ line (Δχ2/d.o.f. = −6/−3) | ||
E (keV) | 7.04 ± 0.08 | |
N (ph cm−2 s−1) | (0.7 ± 0.5)×10−6 | < 1.0 × 10−6 |
EW (eV) | 11 ± 8 | < 13 |
Notes. The normalization of the nuclear power law is in ph cm−2 s−1 keV−1 units at 1 keV. All reported values are in the rest frame of the source and the statistical improvements are referred to a model without the emission line.
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