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Table 1

Seventeen emission lines from the four IRIS spectral windows used in the multi-Gaussian fit.

IRIS window Wavelength Ion Width Intensity Ratio
(Å) (mÅ) tied to

1333.451 H2 31
C ii 1333.791 H2, S i 41

1343 1342.771 H2 31

1348.321 41
1348.641 31
Fe xii 1349.631 41
1350.06 Si ii 260

1352.742 Si ii 260 Si ii 1350.06 0.54
1353.021 Fe ii 41 Fe ii 1354.76 1.85
1353.321 88 H2 1342.77 0.79
1353.391 31 H2 1342.77 1.50
O i 1353.722 Si ii 260 Si ii 1350.06 0.49
1354.011 Fe ii 41 Fe ii 1354.76 3.43
1354.08 Fe xxi 230
1354.29 C i 130
1354.761 Fe ii 42
1354.851 H2 31 H2 1342.77 2.0

Notes. 1: The emission lines with fixed positions in the multi-Gaussian fit. 2: The emission lines with constrained positions in the multi-Gaussian fit.

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