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Table 2.

Lines extracted from the SPROUTS dataset.

Spectral lines logT (K) FIP (eV) Transition Sub-windows (Å)
O I 988.6 4.2 13.6 2s2 2p43P2 – 2s2 2p32D0 987.4–989.1
H I 972.5 4.5 13.6 1s22S1/2 – 5p 2P1/2 969.0–974.5
O II 718 (mult.) 4.7 13.6 2s2 2p32D5/2 – 2s 2p42D5/2 716.3–720.9
C III 977 4.8 11.3 2s21S0 – 2s 2p 1P1 974.5–980.3
N III 989 * 4.8 14.5 2s2 2p 2P1/2 – 2s 2p22D3/2 989.1–990.6
N III 991 * 4.8 14.5 2s2 2p 2P3/2 – 2s 2p22D3/2 990.6–993.4
O III 702.8 * 4.9 13.6 2s2 2p23P1 – 2s 2p33P0 700.3–703.1
O III 703.8 * 4.9 13.6 2s2 2p23P2 – 2s 2p33P1 703.1–704.8
S IV 750 * 5.0 10.4 3s2 3p 2P3/2 – 3s 3p22P3/2 749.8–752.5
S V 786 * 5.2 10.4 3s21S0 – 3s 3p 1P1 784.2–787.0
O IV 787 * 5.2 13.6 2s2 2p 2P1/2 – 2s 2p22D3/2 787.0–789.8
O VI 1032 * 5.4 13.6 1s2 2s 2S1/2 – 1s2 2p 2P3/2 1029.1–1034.9
Ne VIII 770 * 5.8 21.6 1s2 2s 2S1/2 – 1s2 2p 2P3/2 767.2–771.5
Mg VIII 772 5.9 7.6 2s2 2p 2P3/2 – 2s2p24P5/2 771.5–775.2
Mg IX 749 6.0 7.6 2s2 2p 1P1 – 2p21D2 747.8–749.8
Mg IX 706 6.0 7.6 2s21S0 – 2s 2p 3P1 704.85–708.1

Notes. Estimated temperature of formation for each spectral line and the wavelength window used to determine the Gaussian fitting parameters. The lines marked with * have been used in the DEM computation.

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