Table B.1.
Energy Binning for Varying Bin Counts
| Nb | Bin Boundaries (eV) |
|---|---|
| 4 | 7.9, 13.6, 24.4, 54.4, 77.0 |
| 8 | 7.9, 13.6, 16.2, 24.4, 35.1, 47.9, 54.4, 63.4, 77.0 |
| 15 | 7.9, 11.3, 13.6, 14.5, 16.2, 21.6, 24.4, 29.6, 30.7, 35.1, |
| 41.0, 45.1, 47.9, 54.5, 63.4, 77.0 | |
| 28 | 7.9, 11.3, 13.6, 14.5, 16.2, 19.0, 21.6, 24.4, 27.0, 29.6, |
| 30.7, 33.0, 35.1, 38.0, 41.0, 43.0, 45.1, 47.9, 52.0, 54.5, | |
| 57.0, 60.0, 63.4, 66.0, 69.0, 72.0, 74.0, 77.0 | |
| 64 | 7.9, 11.3, 13.6, 14.5, 16.0, 17.0, 18.0, …, 75.0, 76.0, 77.0 |
Notes. Energy bins for the radiation field used in photoionisation calculations to assess convergence with energy resolution. For Nb energy bins, the Nb + 1 boundaries correspond to the bin boundaries. The bins are chosen to align with ionisation thresholds of the most abundant ions wherever possible. Not all significant digits are shown; for example, the bin threshold at 13.6 eV matches exactly with the ionisation energy of H used in the photoionisation cross-section.
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