Table 4.
Open in new tab

Best-fitting parameters of the Gaussians and identification of the lines.

Gaussian*Center energy [eV]Normalization†fX‡Line identification
1|$374^{+7}_{-10}$||$11.6^{+2.8}_{-3.1}$||$7.42^{+1.79}_{1.96}$|C vi 2p to 1s (368 eV)
2|$468^{+10}_{-10}$||$2.73^{+1.00}_{-1.00}$||$2.18^{+0.80}_{-0.80}$|C vi 4p to 1s (459 eV)
3|$571^{+6}_{-5}$||$7.81^{+1.58}_{-1.48}$||$7.59^{+1.54}_{-1.44}$|O vii
4|$656^{+2}_{-6}$||$9.86^{+0.86}_{-0.95}$||$11.0^{+1.0}_{-1.1}$|O viii 2p to 1s (653 eV)
5|$814^{+7}_{-6}$||$2.20^{+0.38}_{-0.36}$||$3.05^{+0.53}_{-0.50}$|O viii or Fe xvii
6|$895^{+8}_{-10}$||$1.78^{+0.32}_{-0.33}$||$2.71^{+0.48}_{-0.50}$|Ne ix or Fe xviii
7|$1008^{+11}_{-4}$||$2.01^{+0.30}_{-1.02}$||$3.45^{+0.51}_{-1.76}$|Ne x 2p to 1s (1022 eV)
8|$1060^{+18}_{-8}$||$1.21^{+0.62}_{-0.68}$||$2.19^{+1.11}_{-1.23}$|Ne ix ?
9|$1172^{+18}_{-19}$||$0.42^{+0.13}_{-0.14}$||$0.83^{+0.27}_{-0.27}$|—
10|$1270^{+10}_{-14}$||$0.72^{+0.15}_{-0.14}$||$1.55^{+0.32}_{-0.30}$|—
11|$1339^{+7}_{-7}$||$1.04^{+0.16}_{-0.16}$||$2.37^{+0.36}_{-0.37}$|Mg xi
12|$1468^{+5}_{-5}$||$1.26^{+0.15}_{-0.14}$||$3.15^{+0.37}_{-0.36}$|Mg xii 2p to 1s (1473 eV)
13|$1564^{+20}_{-17}$||$0.28^{+0.12}_{-0.12}$||$0.75^{+0.33}_{-0.32}$|Mg xi
14|$1722^{+22}_{-25}$||$0.23^{+0.12}_{-0.10}$||$0.69^{+0.35}_{-0.29}$|Mg xii 3p to 1s (1745 eV)
15|$1836^{+3}_{-4}$||$0.55^{+0.09}_{-0.12}$||$1.72^{+0.29}_{-0.38}$|Si xiii
16|$2006^{+27}_{-27}$||$0.31^{+0.11}_{-0.11}$||$1.04^{+0.39}_{-0.39}$|Si xiv 2p to 1s (2006 eV)
17|$2616^{+23}_{-23}$||$0.33^{+0.12}_{-0.12}$||$1.46^{+0.54}_{-0.53}$|S xvi 2p to 1s (2623 eV)
Gaussian*Center energy [eV]Normalization†fX‡Line identification
1|$374^{+7}_{-10}$||$11.6^{+2.8}_{-3.1}$||$7.42^{+1.79}_{1.96}$|C vi 2p to 1s (368 eV)
2|$468^{+10}_{-10}$||$2.73^{+1.00}_{-1.00}$||$2.18^{+0.80}_{-0.80}$|C vi 4p to 1s (459 eV)
3|$571^{+6}_{-5}$||$7.81^{+1.58}_{-1.48}$||$7.59^{+1.54}_{-1.44}$|O vii
4|$656^{+2}_{-6}$||$9.86^{+0.86}_{-0.95}$||$11.0^{+1.0}_{-1.1}$|O viii 2p to 1s (653 eV)
5|$814^{+7}_{-6}$||$2.20^{+0.38}_{-0.36}$||$3.05^{+0.53}_{-0.50}$|O viii or Fe xvii
6|$895^{+8}_{-10}$||$1.78^{+0.32}_{-0.33}$||$2.71^{+0.48}_{-0.50}$|Ne ix or Fe xviii
7|$1008^{+11}_{-4}$||$2.01^{+0.30}_{-1.02}$||$3.45^{+0.51}_{-1.76}$|Ne x 2p to 1s (1022 eV)
8|$1060^{+18}_{-8}$||$1.21^{+0.62}_{-0.68}$||$2.19^{+1.11}_{-1.23}$|Ne ix ?
9|$1172^{+18}_{-19}$||$0.42^{+0.13}_{-0.14}$||$0.83^{+0.27}_{-0.27}$|—
10|$1270^{+10}_{-14}$||$0.72^{+0.15}_{-0.14}$||$1.55^{+0.32}_{-0.30}$|—
11|$1339^{+7}_{-7}$||$1.04^{+0.16}_{-0.16}$||$2.37^{+0.36}_{-0.37}$|Mg xi
12|$1468^{+5}_{-5}$||$1.26^{+0.15}_{-0.14}$||$3.15^{+0.37}_{-0.36}$|Mg xii 2p to 1s (1473 eV)
13|$1564^{+20}_{-17}$||$0.28^{+0.12}_{-0.12}$||$0.75^{+0.33}_{-0.32}$|Mg xi
14|$1722^{+22}_{-25}$||$0.23^{+0.12}_{-0.10}$||$0.69^{+0.35}_{-0.29}$|Mg xii 3p to 1s (1745 eV)
15|$1836^{+3}_{-4}$||$0.55^{+0.09}_{-0.12}$||$1.72^{+0.29}_{-0.38}$|Si xiii
16|$2006^{+27}_{-27}$||$0.31^{+0.11}_{-0.11}$||$1.04^{+0.39}_{-0.39}$|Si xiv 2p to 1s (2006 eV)
17|$2616^{+23}_{-23}$||$0.33^{+0.12}_{-0.12}$||$1.46^{+0.54}_{-0.53}$|S xvi 2p to 1s (2623 eV)
*

The width of the lines are fixed to 0.

†

In units of photons cm−2 s−1 str−1.

‡

fX is energy flux in units of 10−13 erg s−1 cm−2.

Table 4.
Open in new tab

Best-fitting parameters of the Gaussians and identification of the lines.

Gaussian*Center energy [eV]Normalization†fX‡Line identification
1|$374^{+7}_{-10}$||$11.6^{+2.8}_{-3.1}$||$7.42^{+1.79}_{1.96}$|C vi 2p to 1s (368 eV)
2|$468^{+10}_{-10}$||$2.73^{+1.00}_{-1.00}$||$2.18^{+0.80}_{-0.80}$|C vi 4p to 1s (459 eV)
3|$571^{+6}_{-5}$||$7.81^{+1.58}_{-1.48}$||$7.59^{+1.54}_{-1.44}$|O vii
4|$656^{+2}_{-6}$||$9.86^{+0.86}_{-0.95}$||$11.0^{+1.0}_{-1.1}$|O viii 2p to 1s (653 eV)
5|$814^{+7}_{-6}$||$2.20^{+0.38}_{-0.36}$||$3.05^{+0.53}_{-0.50}$|O viii or Fe xvii
6|$895^{+8}_{-10}$||$1.78^{+0.32}_{-0.33}$||$2.71^{+0.48}_{-0.50}$|Ne ix or Fe xviii
7|$1008^{+11}_{-4}$||$2.01^{+0.30}_{-1.02}$||$3.45^{+0.51}_{-1.76}$|Ne x 2p to 1s (1022 eV)
8|$1060^{+18}_{-8}$||$1.21^{+0.62}_{-0.68}$||$2.19^{+1.11}_{-1.23}$|Ne ix ?
9|$1172^{+18}_{-19}$||$0.42^{+0.13}_{-0.14}$||$0.83^{+0.27}_{-0.27}$|—
10|$1270^{+10}_{-14}$||$0.72^{+0.15}_{-0.14}$||$1.55^{+0.32}_{-0.30}$|—
11|$1339^{+7}_{-7}$||$1.04^{+0.16}_{-0.16}$||$2.37^{+0.36}_{-0.37}$|Mg xi
12|$1468^{+5}_{-5}$||$1.26^{+0.15}_{-0.14}$||$3.15^{+0.37}_{-0.36}$|Mg xii 2p to 1s (1473 eV)
13|$1564^{+20}_{-17}$||$0.28^{+0.12}_{-0.12}$||$0.75^{+0.33}_{-0.32}$|Mg xi
14|$1722^{+22}_{-25}$||$0.23^{+0.12}_{-0.10}$||$0.69^{+0.35}_{-0.29}$|Mg xii 3p to 1s (1745 eV)
15|$1836^{+3}_{-4}$||$0.55^{+0.09}_{-0.12}$||$1.72^{+0.29}_{-0.38}$|Si xiii
16|$2006^{+27}_{-27}$||$0.31^{+0.11}_{-0.11}$||$1.04^{+0.39}_{-0.39}$|Si xiv 2p to 1s (2006 eV)
17|$2616^{+23}_{-23}$||$0.33^{+0.12}_{-0.12}$||$1.46^{+0.54}_{-0.53}$|S xvi 2p to 1s (2623 eV)
Gaussian*Center energy [eV]Normalization†fX‡Line identification
1|$374^{+7}_{-10}$||$11.6^{+2.8}_{-3.1}$||$7.42^{+1.79}_{1.96}$|C vi 2p to 1s (368 eV)
2|$468^{+10}_{-10}$||$2.73^{+1.00}_{-1.00}$||$2.18^{+0.80}_{-0.80}$|C vi 4p to 1s (459 eV)
3|$571^{+6}_{-5}$||$7.81^{+1.58}_{-1.48}$||$7.59^{+1.54}_{-1.44}$|O vii
4|$656^{+2}_{-6}$||$9.86^{+0.86}_{-0.95}$||$11.0^{+1.0}_{-1.1}$|O viii 2p to 1s (653 eV)
5|$814^{+7}_{-6}$||$2.20^{+0.38}_{-0.36}$||$3.05^{+0.53}_{-0.50}$|O viii or Fe xvii
6|$895^{+8}_{-10}$||$1.78^{+0.32}_{-0.33}$||$2.71^{+0.48}_{-0.50}$|Ne ix or Fe xviii
7|$1008^{+11}_{-4}$||$2.01^{+0.30}_{-1.02}$||$3.45^{+0.51}_{-1.76}$|Ne x 2p to 1s (1022 eV)
8|$1060^{+18}_{-8}$||$1.21^{+0.62}_{-0.68}$||$2.19^{+1.11}_{-1.23}$|Ne ix ?
9|$1172^{+18}_{-19}$||$0.42^{+0.13}_{-0.14}$||$0.83^{+0.27}_{-0.27}$|—
10|$1270^{+10}_{-14}$||$0.72^{+0.15}_{-0.14}$||$1.55^{+0.32}_{-0.30}$|—
11|$1339^{+7}_{-7}$||$1.04^{+0.16}_{-0.16}$||$2.37^{+0.36}_{-0.37}$|Mg xi
12|$1468^{+5}_{-5}$||$1.26^{+0.15}_{-0.14}$||$3.15^{+0.37}_{-0.36}$|Mg xii 2p to 1s (1473 eV)
13|$1564^{+20}_{-17}$||$0.28^{+0.12}_{-0.12}$||$0.75^{+0.33}_{-0.32}$|Mg xi
14|$1722^{+22}_{-25}$||$0.23^{+0.12}_{-0.10}$||$0.69^{+0.35}_{-0.29}$|Mg xii 3p to 1s (1745 eV)
15|$1836^{+3}_{-4}$||$0.55^{+0.09}_{-0.12}$||$1.72^{+0.29}_{-0.38}$|Si xiii
16|$2006^{+27}_{-27}$||$0.31^{+0.11}_{-0.11}$||$1.04^{+0.39}_{-0.39}$|Si xiv 2p to 1s (2006 eV)
17|$2616^{+23}_{-23}$||$0.33^{+0.12}_{-0.12}$||$1.46^{+0.54}_{-0.53}$|S xvi 2p to 1s (2623 eV)
*

The width of the lines are fixed to 0.

†

In units of photons cm−2 s−1 str−1.

‡

fX is energy flux in units of 10−13 erg s−1 cm−2.

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