Table 1.

Results of SXS spectral fitting.*

Model parameterFe xxv fitS xv fit
No broadeningWith broadeningNo broadeningWith broadening
N 132 D CIE plasma (vapec)
kT (keV)……………………0.7……………………
ZSi (solar)……………………0.6……………………
ZS (solar)……………………0.9……………………
ZFe (solar)……………………0.4……………………
vhelio (km s−1)……………………0……………………210380+370520620+770
 σ (km s−1)……………………0……………………0520340+780
 Flux, 2–10 keV……………………8.8……………………5.61.9+2.95.51.8+3.1
Flux, fitting band……………………0.006……………………1.30.2+0.41.30.2+0.4
N 132 D NEI plasma (vrnei)
kT (keV)……………………1.5……………………
kTinit (keV)……………………80……………………
net (1012 s cm−3)……………………0.9……………………
ZSi (solar)……………………0.4……………………
ZS (solar)……………………0.4……………………
ZFe (solar)……………………0.5……………………
vhelio (km s−1)14401000+1001140810+64014401140
 σ (km s−1)0510330+10600510
 Flux, 2–10 keV9.53.0+4.59.73.2+4.26.16.2
Flux, fitting band0.480.16+0.250.490.16+0.240.340.34
CXB power law
 Γ……………………1.54……………………
 Flux, 2–10 keV……………………0.040……………………
 Flux, fitting band……………………0.0016…………………………………………0.0006……………………
Spectral fitting band……………………6.45–6.80 keV…………………………………………2.40–2.48 keV……………………
C-stat/d.o.f.107.9/696106.5/69561.0/15759.1/156
Goodness-of-fit (KS)§24%20%62%31%
Goodness-of-fit (CvM)§35%21%62%46%
Model parameterFe xxv fitS xv fit
No broadeningWith broadeningNo broadeningWith broadening
N 132 D CIE plasma (vapec)
kT (keV)……………………0.7……………………
ZSi (solar)……………………0.6……………………
ZS (solar)……………………0.9……………………
ZFe (solar)……………………0.4……………………
vhelio (km s−1)……………………0……………………210380+370520620+770
 σ (km s−1)……………………0……………………0520340+780
 Flux, 2–10 keV……………………8.8……………………5.61.9+2.95.51.8+3.1
Flux, fitting band……………………0.006……………………1.30.2+0.41.30.2+0.4
N 132 D NEI plasma (vrnei)
kT (keV)……………………1.5……………………
kTinit (keV)……………………80……………………
net (1012 s cm−3)……………………0.9……………………
ZSi (solar)……………………0.4……………………
ZS (solar)……………………0.4……………………
ZFe (solar)……………………0.5……………………
vhelio (km s−1)14401000+1001140810+64014401140
 σ (km s−1)0510330+10600510
 Flux, 2–10 keV9.53.0+4.59.73.2+4.26.16.2
Flux, fitting band0.480.16+0.250.490.16+0.240.340.34
CXB power law
 Γ……………………1.54……………………
 Flux, 2–10 keV……………………0.040……………………
 Flux, fitting band……………………0.0016…………………………………………0.0006……………………
Spectral fitting band……………………6.45–6.80 keV…………………………………………2.40–2.48 keV……………………
C-stat/d.o.f.107.9/696106.5/69561.0/15759.1/156
Goodness-of-fit (KS)§24%20%62%31%
Goodness-of-fit (CvM)§35%21%62%46%

*Unless noted otherwise, values without quoted uncertainties are fixed. Uncertainties are 90% confidence limits.

Results with broadening assume a Gaussian prior with σ = 1000 km s−1.

Flux is given in units of 10−12 erg cm−2 s−1. The ratio of the vapec and vrnei component normalizations was fixed to that in Bamba et al. (2017).

§“Goodness-of-fit” is the percentage of simulated observations with lower fit statistics than the real data, as described in subsection 3.1.

Table 1.

Results of SXS spectral fitting.*

Model parameterFe xxv fitS xv fit
No broadeningWith broadeningNo broadeningWith broadening
N 132 D CIE plasma (vapec)
kT (keV)……………………0.7……………………
ZSi (solar)……………………0.6……………………
ZS (solar)……………………0.9……………………
ZFe (solar)……………………0.4……………………
vhelio (km s−1)……………………0……………………210380+370520620+770
 σ (km s−1)……………………0……………………0520340+780
 Flux, 2–10 keV……………………8.8……………………5.61.9+2.95.51.8+3.1
Flux, fitting band……………………0.006……………………1.30.2+0.41.30.2+0.4
N 132 D NEI plasma (vrnei)
kT (keV)……………………1.5……………………
kTinit (keV)……………………80……………………
net (1012 s cm−3)……………………0.9……………………
ZSi (solar)……………………0.4……………………
ZS (solar)……………………0.4……………………
ZFe (solar)……………………0.5……………………
vhelio (km s−1)14401000+1001140810+64014401140
 σ (km s−1)0510330+10600510
 Flux, 2–10 keV9.53.0+4.59.73.2+4.26.16.2
Flux, fitting band0.480.16+0.250.490.16+0.240.340.34
CXB power law
 Γ……………………1.54……………………
 Flux, 2–10 keV……………………0.040……………………
 Flux, fitting band……………………0.0016…………………………………………0.0006……………………
Spectral fitting band……………………6.45–6.80 keV…………………………………………2.40–2.48 keV……………………
C-stat/d.o.f.107.9/696106.5/69561.0/15759.1/156
Goodness-of-fit (KS)§24%20%62%31%
Goodness-of-fit (CvM)§35%21%62%46%
Model parameterFe xxv fitS xv fit
No broadeningWith broadeningNo broadeningWith broadening
N 132 D CIE plasma (vapec)
kT (keV)……………………0.7……………………
ZSi (solar)……………………0.6……………………
ZS (solar)……………………0.9……………………
ZFe (solar)……………………0.4……………………
vhelio (km s−1)……………………0……………………210380+370520620+770
 σ (km s−1)……………………0……………………0520340+780
 Flux, 2–10 keV……………………8.8……………………5.61.9+2.95.51.8+3.1
Flux, fitting band……………………0.006……………………1.30.2+0.41.30.2+0.4
N 132 D NEI plasma (vrnei)
kT (keV)……………………1.5……………………
kTinit (keV)……………………80……………………
net (1012 s cm−3)……………………0.9……………………
ZSi (solar)……………………0.4……………………
ZS (solar)……………………0.4……………………
ZFe (solar)……………………0.5……………………
vhelio (km s−1)14401000+1001140810+64014401140
 σ (km s−1)0510330+10600510
 Flux, 2–10 keV9.53.0+4.59.73.2+4.26.16.2
Flux, fitting band0.480.16+0.250.490.16+0.240.340.34
CXB power law
 Γ……………………1.54……………………
 Flux, 2–10 keV……………………0.040……………………
 Flux, fitting band……………………0.0016…………………………………………0.0006……………………
Spectral fitting band……………………6.45–6.80 keV…………………………………………2.40–2.48 keV……………………
C-stat/d.o.f.107.9/696106.5/69561.0/15759.1/156
Goodness-of-fit (KS)§24%20%62%31%
Goodness-of-fit (CvM)§35%21%62%46%

*Unless noted otherwise, values without quoted uncertainties are fixed. Uncertainties are 90% confidence limits.

Results with broadening assume a Gaussian prior with σ = 1000 km s−1.

Flux is given in units of 10−12 erg cm−2 s−1. The ratio of the vapec and vrnei component normalizations was fixed to that in Bamba et al. (2017).

§“Goodness-of-fit” is the percentage of simulated observations with lower fit statistics than the real data, as described in subsection 3.1.

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