Table 2.

Best-fitting parameters for a power-law model for the XIS spectra and the PIN spectrum.*

ParameterXISHXD-PIN
Photon index2.93 ± 0.02|$3.15^{+1.18}_{-1.14}$|
Flux4.43 ± 0.03 × 10−11§8.26 ± 1.44 × 10−12
[erg cm−2 s−1]
χ2/d.o.f.732.16/6580.87/4
ParameterXISHXD-PIN
Photon index2.93 ± 0.02|$3.15^{+1.18}_{-1.14}$|
Flux4.43 ± 0.03 × 10−11§8.26 ± 1.44 × 10−12
[erg cm−2 s−1]
χ2/d.o.f.732.16/6580.87/4

*Errors are for a single parameter of interest in 90% confidence.

The absorbing column density is set to be 6.7 × 1021 cm−2, referring to Hiraga et al. (2009).

The model contains the fixed GRXE component and the normalization is corrected (see text).

§The flux at the range of 2–10 keV.

The flux at the range of 12–22 keV.

Table 2.

Best-fitting parameters for a power-law model for the XIS spectra and the PIN spectrum.*

ParameterXISHXD-PIN
Photon index2.93 ± 0.02|$3.15^{+1.18}_{-1.14}$|
Flux4.43 ± 0.03 × 10−11§8.26 ± 1.44 × 10−12
[erg cm−2 s−1]
χ2/d.o.f.732.16/6580.87/4
ParameterXISHXD-PIN
Photon index2.93 ± 0.02|$3.15^{+1.18}_{-1.14}$|
Flux4.43 ± 0.03 × 10−11§8.26 ± 1.44 × 10−12
[erg cm−2 s−1]
χ2/d.o.f.732.16/6580.87/4

*Errors are for a single parameter of interest in 90% confidence.

The absorbing column density is set to be 6.7 × 1021 cm−2, referring to Hiraga et al. (2009).

The model contains the fixed GRXE component and the normalization is corrected (see text).

§The flux at the range of 2–10 keV.

The flux at the range of 12–22 keV.

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