Table A.4.
Time-integrated flare flux (erg per square centimetre) in HST-COS FUV.
| Temporal flux evolution | AU Mic F1 | AU Mic F2 | AU Mic F3 | AU Mic F4 | 2MASS...168 F1 | Karmn...+035 F1 | 2MASS...036 F1 | 2MASS...441 F1 |
|---|---|---|---|---|---|---|---|---|
| Mendoza model | 1.2787×10−9 | 7.0657×10−10 | 3.2834×10−10 | 1.8946×10−10 | 8.8510×10−11 | 7.1278×10−10 | 1.5559×10−9 | 6.3635×10−11 |
| Davenport model | 1.2769×10−9 | 7.1558×10−10 | 3.2823×10−10 | 1.9141×10−10 | 8.9296×10−11 | 7.2030×10−10 | 1.6056×10−9 | 6.5371×10−11 |
| Feinstein model | 6.3695×10−10 | 4.2002×10−10 | 2.2379×10−10 | 2.1785×10−10 | 8.1210×10−11 | 4.0197×10−10 | 7.3248×10−10 | 6.0898×10−11 |
| Inverse H model | 1.2908×10−9 | 6.4422×10−10 | 3.1229×10−10 | 2.2236×10−10 | 8.6776×10−11 | 5.4157×10−10 | 1.6026×10−9 | 7.2716×10−11 |
| Inverse HCIII model | 1.4917×10−9 | 7.1842×10−10 | 3.5056×10−10 | 2.7133×10−10 | 9.2140×10−11 | 5.3430×10−10 | 1.4785×10−9 | 7.2198×10−11 |
| ‘Fiducial flare’ model | 2.5810×10−9 | 8.4980×10−10 | 5.0288×10−10 | 3.5072×10−10 | - | - | - | - |
| Observed | 1.2793×10−9 | 6.7371×10−10 | 3.2174×10−10 | 1.9310×10−10 | 8.5826×10−11 | 5.9483×10−10 | 1.4291×10−9 | 6.8553×10−11 |
Notes. The time-integrated flare flux is calculated across FUV-A and FUV-B segments consistent with detector gaps specific to the observation (see Appendix A.4) in all temporally spectrally resolved models, including ‘fiducial flare’. 2MASS...168, Karmn...+035, 2MASS...036 and 2MASS...441 stand for 2MASS J01521830-5950168, Karmn J07446+0352MASS, J02365171-5203036 and 2MASS J22025453-6440441, respectively.
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