Table A.3
Mass, radius, and density of L 98-59 derived with different approaches
| Method | M* | R* | ρ* |
|---|---|---|---|
| [M⊙] | [R⊙] | [ρ⊙] | |
| Stefan-Boltzmann law |  |
||
| log g + R* |  |
// |  |
| ρ* + R* |  |
// |  |
| VOSA | 0.273 ± 0.030 | – |  |
| Cifuentes+20 (f(L)) | 0.338 ± 0.087 | 0.343 ± 0.082 |  |
| Cifuentes+20 (f(Teff)) | 0.432 ± 0.090 | 0.433 ± 0.086 |  |
| mass-lum (Mann et al. 2019) | 0.290 ± 0.020 | – |  |
| K19 | 0.313 ± 0.014 | 0.312 ± 0.014 |  |
Notes. The adopted estimates are provided in Table H.1. // indicates that the radius estimate used as input of the method was provided by the Stefan-Boltzmann law. – indicates that the radius is not estimated by the method and that we used the estimate provided by the Stefan-Bolztmann law to compute the stellar density.
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