Table C.1.
Error on the estimation of the age provided by the gyrochronology analysis in the case of |δP| = 0.5.
| Mass | Pinit | SMAinit | Age50% | Δt50% | Prot, 50% | Porb, 50% | Prot, isol.,50% | Agegyro | Agegyro, isol. |
|---|---|---|---|---|---|---|---|---|---|
| (M⊙) | (days) | (au) | (Myr) | (Myr) | (days) | (days) | (days) | (Myr) | (Myr) |
| 0.7 | 6.00 | 0.0258 | 164/624 | 40/80 | 4.16/7.72 | –/– | 8.25/11.86 | 84/256 | 288/549 |
| 0.7 | 7.00 | 0.0286 | 965/4155 | 140/1550 | 10.05/17.94 | –/0.2630 | 15.59/36.71 | 409/1151 | 895/4133 |
| 0.7 | 8.00 | 0.0209 | 1655/1655 | 250/250 | 13.11/13.11 | –/– | 21.19/21.19 | 657/657 | 1549/1549 |
| 0.7 | 9.00 | 0.0226 | 3856/3856 | 1350/1350 | 18.46/18.46 | 0.2639/0.2633 | 34.86/34.86 | 1211/1211 | 3770/3770 |
| 0.7 | 10.40 | 0.0248 | 8707/8707 | 3400/3400 | 19.48/19.48 | 0.2642/0.2637 | 50.55/50.55 | 1333/1333 | 7319/7319 |
Notes. Here we consider a 0.7 M⊙ star around which orbits a 2 Mjup planet and for ⟨𝒟⟩=⟨𝒟⟩*100. We adopted a dissipation that is two orders of magnitude higher ⟨𝒟⟩*100 than the frequency-averaged tidal dissipation used in this article. The listed data are for ⟨𝒟⟩*100 (left) and ⟨𝒟⟩ (right) and in the case of |δP|=0.50. We only show data that are in common between the two datasets.
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