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Table B.1.

Key parameters of the most relevant lines.

Spectroscopic Transition Type Energy, keV Transition
symbol probability, s−1
Fe XXV Kα − W 1s21S0 - 1s2p1P1 E1 6.700 4.57 × 1014
Fe XXV Kα − X 1s21S0 - 1s2p3P2 M2 6.682 6.64 × 109
Fe XXV Kα − Y 1s21S0 - 1s2p3P1 E1 6.668 4.42 × 1013
Fe XXV Kα − Z 1s21S0 - 1s2s3S1 M1 6.634 2.12 × 108
Fe XXVI Lyα3/2 1s2S1/2 - 2p2P3/2 E1 6.973 2.8370 × 1014
Fe XXVI Lyα1/2 1s2S1/2 - 2p2P1/2 E1 6.952 2.8731 × 1014

Notes. All data (energies rounded to 1 eV) are from NIST Atomic Spectra Database (Kramida et al. 2024).

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