Table 3
Ratios between the reference spectra described in the text and the time-averaged flux of this work.
| Spectrum E. range | [1, 100] Å | [1, 2.5] Å | [2.5, 5] Å | [5, 10] Å | [10, 20] Å | [20, 50] Å | [50, 100] Å |
|---|---|---|---|---|---|---|---|
| (this work) Average (erg cm−2 s−1) at 1 AU | ![]() |
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| DA+25 Minimum | ![]() |
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| DA+25 Median | ![]() |
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| DA+25 80th percentile | ![]() |
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| DA+25 Maximum | ![]() |
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| BI+24 Quiescent | ![]() |
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| BI+24 Elevated | ![]() |
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| BI+24 Rising | ![]() |
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| BI+24 Descending | ![]() |
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| BI+24 Flare | ![]() |
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| SF+25 Average | ![]() |
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| RI+17 Average | ![]() |
– | – | ![]() |
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| LO+18 MUSCLES APEC | ![]() |
– | – | ![]() |
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| LO+18 MUSCLES Multi | ![]() |
– | ![]() |
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Notes. DA+25: this work; BI+24: Binder et al. (2024); SF+25: Sanz-Forcada et al. (2025); RI+17: Ribas et al. (2017); LO+18: Loyd et al. (2018). The first row shows the total flux values in the different wavelength ranges for the average. Absolute 1 σ errors are propagated considering only the uncertainties of the references from this work. For example, the value
indicates that in that band the referenced spectrum is
times fainter than our time-averaged spectrum (first row, same column), whereas the value
indicates that the referenced spectrum is
times brighter than our time-averaged spectrum (first row, same column). (*) The reference spectrum for this value is integrated over [7, 100] Å instead of [5, 100] Å.
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