Model parameter . | Fe xxv fit . | S xv fit . | ||
---|---|---|---|---|
. | No broadening . | With broadening† . | No broadening . | With 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…………………… | 210 | 520 | |
σ (km s−1) | ……………………0…………………… | 0 | 520 | |
Flux, 2–10 keV‡ | ……………………8.8…………………… | 5.6 | 5.5 | |
Flux, fitting band‡ | ……………………0.006…………………… | 1.3 | 1.3 | |
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) | 1440 | 1140 | 1440 | 1140 |
σ (km s−1) | 0 | 510 | 0 | 510 |
Flux, 2–10 keV‡ | 9.5 | 9.7 | 6.1 | 6.2 |
Flux, fitting band‡ | 0.48 | 0.49 | 0.34 | 0.34 |
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 | 107.9 | 106.5 | 61.0 | 59.1 |
Goodness-of-fit (KS)§ | 24% | 20% | 62% | 31% |
Goodness-of-fit (CvM)§ | 35% | 21% | 62% | 46% |
Model parameter . | Fe xxv fit . | S xv fit . | ||
---|---|---|---|---|
. | No broadening . | With broadening† . | No broadening . | With 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…………………… | 210 | 520 | |
σ (km s−1) | ……………………0…………………… | 0 | 520 | |
Flux, 2–10 keV‡ | ……………………8.8…………………… | 5.6 | 5.5 | |
Flux, fitting band‡ | ……………………0.006…………………… | 1.3 | 1.3 | |
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) | 1440 | 1140 | 1440 | 1140 |
σ (km s−1) | 0 | 510 | 0 | 510 |
Flux, 2–10 keV‡ | 9.5 | 9.7 | 6.1 | 6.2 |
Flux, fitting band‡ | 0.48 | 0.49 | 0.34 | 0.34 |
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 | 107.9 | 106.5 | 61.0 | 59.1 |
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.
Model parameter . | Fe xxv fit . | S xv fit . | ||
---|---|---|---|---|
. | No broadening . | With broadening† . | No broadening . | With 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…………………… | 210 | 520 | |
σ (km s−1) | ……………………0…………………… | 0 | 520 | |
Flux, 2–10 keV‡ | ……………………8.8…………………… | 5.6 | 5.5 | |
Flux, fitting band‡ | ……………………0.006…………………… | 1.3 | 1.3 | |
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) | 1440 | 1140 | 1440 | 1140 |
σ (km s−1) | 0 | 510 | 0 | 510 |
Flux, 2–10 keV‡ | 9.5 | 9.7 | 6.1 | 6.2 |
Flux, fitting band‡ | 0.48 | 0.49 | 0.34 | 0.34 |
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 | 107.9 | 106.5 | 61.0 | 59.1 |
Goodness-of-fit (KS)§ | 24% | 20% | 62% | 31% |
Goodness-of-fit (CvM)§ | 35% | 21% | 62% | 46% |
Model parameter . | Fe xxv fit . | S xv fit . | ||
---|---|---|---|---|
. | No broadening . | With broadening† . | No broadening . | With 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…………………… | 210 | 520 | |
σ (km s−1) | ……………………0…………………… | 0 | 520 | |
Flux, 2–10 keV‡ | ……………………8.8…………………… | 5.6 | 5.5 | |
Flux, fitting band‡ | ……………………0.006…………………… | 1.3 | 1.3 | |
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) | 1440 | 1140 | 1440 | 1140 |
σ (km s−1) | 0 | 510 | 0 | 510 |
Flux, 2–10 keV‡ | 9.5 | 9.7 | 6.1 | 6.2 |
Flux, fitting band‡ | 0.48 | 0.49 | 0.34 | 0.34 |
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 | 107.9 | 106.5 | 61.0 | 59.1 |
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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