Open Access
Table F.1.
Observational trends used in this work and their caveats.
| Ingredient | References | Caveats |
|---|---|---|
| Skumanich law | Skumanich (1972) | |
| Gallet & Bouvier (2015) | Uncertainty in the core-envelope coupling timescale dependency. Possible break of gyrochronology for evolved stars. | |
| van Saders et al. (2016) | ||
| Wind braking torque | Matt et al. (2015) | Slows rotators with lower stellar masses spinning too fast compared to the one observed in the Kepler field. Possible dependency on the metallicity. |
| LX − Ro relationship | Pizzolato et al. (2003) | |
| Wright et al. (2011) | Uncertainties in the trend obtained due to observational biases. | |
| Reiners et al. (2014) | ||
| ZDI studies | Reiners (2012) | |
| Vidotto et al. (2014) | Only large-scale unsigned magnetic flux can be measured, missing small-scale field, observational uncertainties. | |
| See et al. (2017) | ||
| Astrospheric wind measurements | Wood et al. (2002, 2005) | Assumed interstellar medium parameters, limited number of systems, large scatter in scaling law. |
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