Table 6.
Open in new tab

Best-fitting parameters in model fitting with the fixed-center-energy Gaussians.

Gaussian*Center energy [eV]Normalization†Line identification
1299|$33.6^{+20.0}_{-20.0}$|C v
2367|$8.71^{+2.87}_{-2.89}$|C vi
3420—N vi
4500|$1.30^{+0.86}_{-0.87}$|N vii
5561|$5.15^{+1.03}_{-1.04}$|O vii
6653|$9.57^{+0.93}_{-0.93}$|O viii
7730|$0.60^{+0.47}_{-0.47}$|Fe xvii
8820|$0.52^{+0.43}_{-0.43}$|Fe xvii
9870|$0.90^{+0.38}_{-0.38}$|Fe xviii
10920|$1.04^{+0.39}_{-0.39}$|Ne ix
11960|$0.39^{+0.29}_{-0.29}$|Fe xx
121022|$2.53^{+0.26}_{-0.26}$|Ne x
131100|$0.60^{+0.16}_{-0.16}$|Ne ix
141220|$0.56^{+0.14}_{-0.14}$|Ne x
151330|$1.32^{+0.15}_{-0.15}$|Mg xi
161470|$1.31^{+0.15}_{-0.15}$|Mg xii
171600|$0.20^{+0.11}_{-0.11}$|Mg xi
181730|$0.26^{+0.11}_{-0.11}$|Al xiii
191850|$0.69^{+0.15}_{-0.15}$|Si xiii
202000|$0.30^{+0.12}_{-0.12}$|Si xiv
212623|$0.32^{+0.12}_{-0.12}$|S xvi
Gaussian*Center energy [eV]Normalization†Line identification
1299|$33.6^{+20.0}_{-20.0}$|C v
2367|$8.71^{+2.87}_{-2.89}$|C vi
3420—N vi
4500|$1.30^{+0.86}_{-0.87}$|N vii
5561|$5.15^{+1.03}_{-1.04}$|O vii
6653|$9.57^{+0.93}_{-0.93}$|O viii
7730|$0.60^{+0.47}_{-0.47}$|Fe xvii
8820|$0.52^{+0.43}_{-0.43}$|Fe xvii
9870|$0.90^{+0.38}_{-0.38}$|Fe xviii
10920|$1.04^{+0.39}_{-0.39}$|Ne ix
11960|$0.39^{+0.29}_{-0.29}$|Fe xx
121022|$2.53^{+0.26}_{-0.26}$|Ne x
131100|$0.60^{+0.16}_{-0.16}$|Ne ix
141220|$0.56^{+0.14}_{-0.14}$|Ne x
151330|$1.32^{+0.15}_{-0.15}$|Mg xi
161470|$1.31^{+0.15}_{-0.15}$|Mg xii
171600|$0.20^{+0.11}_{-0.11}$|Mg xi
181730|$0.26^{+0.11}_{-0.11}$|Al xiii
191850|$0.69^{+0.15}_{-0.15}$|Si xiii
202000|$0.30^{+0.12}_{-0.12}$|Si xiv
212623|$0.32^{+0.12}_{-0.12}$|S xvi
*

The width of the lines are fixed to 0.

†

In units of photons cm−2 s−1 str−1.

Table 6.
Open in new tab

Best-fitting parameters in model fitting with the fixed-center-energy Gaussians.

Gaussian*Center energy [eV]Normalization†Line identification
1299|$33.6^{+20.0}_{-20.0}$|C v
2367|$8.71^{+2.87}_{-2.89}$|C vi
3420—N vi
4500|$1.30^{+0.86}_{-0.87}$|N vii
5561|$5.15^{+1.03}_{-1.04}$|O vii
6653|$9.57^{+0.93}_{-0.93}$|O viii
7730|$0.60^{+0.47}_{-0.47}$|Fe xvii
8820|$0.52^{+0.43}_{-0.43}$|Fe xvii
9870|$0.90^{+0.38}_{-0.38}$|Fe xviii
10920|$1.04^{+0.39}_{-0.39}$|Ne ix
11960|$0.39^{+0.29}_{-0.29}$|Fe xx
121022|$2.53^{+0.26}_{-0.26}$|Ne x
131100|$0.60^{+0.16}_{-0.16}$|Ne ix
141220|$0.56^{+0.14}_{-0.14}$|Ne x
151330|$1.32^{+0.15}_{-0.15}$|Mg xi
161470|$1.31^{+0.15}_{-0.15}$|Mg xii
171600|$0.20^{+0.11}_{-0.11}$|Mg xi
181730|$0.26^{+0.11}_{-0.11}$|Al xiii
191850|$0.69^{+0.15}_{-0.15}$|Si xiii
202000|$0.30^{+0.12}_{-0.12}$|Si xiv
212623|$0.32^{+0.12}_{-0.12}$|S xvi
Gaussian*Center energy [eV]Normalization†Line identification
1299|$33.6^{+20.0}_{-20.0}$|C v
2367|$8.71^{+2.87}_{-2.89}$|C vi
3420—N vi
4500|$1.30^{+0.86}_{-0.87}$|N vii
5561|$5.15^{+1.03}_{-1.04}$|O vii
6653|$9.57^{+0.93}_{-0.93}$|O viii
7730|$0.60^{+0.47}_{-0.47}$|Fe xvii
8820|$0.52^{+0.43}_{-0.43}$|Fe xvii
9870|$0.90^{+0.38}_{-0.38}$|Fe xviii
10920|$1.04^{+0.39}_{-0.39}$|Ne ix
11960|$0.39^{+0.29}_{-0.29}$|Fe xx
121022|$2.53^{+0.26}_{-0.26}$|Ne x
131100|$0.60^{+0.16}_{-0.16}$|Ne ix
141220|$0.56^{+0.14}_{-0.14}$|Ne x
151330|$1.32^{+0.15}_{-0.15}$|Mg xi
161470|$1.31^{+0.15}_{-0.15}$|Mg xii
171600|$0.20^{+0.11}_{-0.11}$|Mg xi
181730|$0.26^{+0.11}_{-0.11}$|Al xiii
191850|$0.69^{+0.15}_{-0.15}$|Si xiii
202000|$0.30^{+0.12}_{-0.12}$|Si xiv
212623|$0.32^{+0.12}_{-0.12}$|S xvi
*

The width of the lines are fixed to 0.

†

In units of photons cm−2 s−1 str−1.

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