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Table 7
X-ray and EUV fluxes and the corresponding mass-loss rates derived from the three proxy spectra for both planets.
| Spectrum | FXUV (W/m2) | Ṁ˙ (g/s) |
|---|---|---|
| TOI-5108 b HD 108147 | 0.297 | (1.00 ± 0.19) × 109 |
| Sun | 0.560 | (1.89 ± 0.35) × 109 |
| WASP 17 TOI-5786 b | 2.891 | (9.8 ± 1.8) × 109 |
| HD 108147 | 0.114 | (3.6 ± 0.4) × 108 |
| Sun | 0.216 | (6.8 ± 0.8) × 108 |
| WASP 17 | 1.114 | (3.5 ± 0.4) × 109 |
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