Table F.1
Lines with significant rotation period detections common to Gl 581 and Proxima.
| Gl 581 | Proxima | ||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|
| λ0,med [Å] | Sp. | P [d] | FAP | Param | ⟨depth⟩ [1 − F / Fc] | ⟨F W H M⟩ [km/s] | P [d] | FAP | Param | ⟨depth⟩ [1 − F / Fc] | ⟨F W H M⟩ [km/s] |
| 9790.368 | Ti I | 141.32 | 4e-09 | F W H M | 0.66 | 8.6 | 79.24 | 8e-21 | F W H M | 0.63 | 12.2 |
| 10433.372 | − | 148.28 | 5e-05 | F W H M | 0.17 | 6.0 | 78.41 | 2e-12 | F W H M | 0.36 | 7.9 |
| 10908.741 | Cr I | 138.20 | 2e-04 | depth | 0.17 | 8.8 | 78.33 | 3e-06 | pEW | 0.14 | 12.3 |
| 11641.442 | Fe I | 140.26 | 6e-05 | F W H M | 0.49 | 9.4 | 78.29 | 2e-18 | F W H M | 0.49 | 14.2 |
| 11772.861 | K I | 134.01 | 2e-09 | pEW | 0.51 | 8.8 | 79.95 | 3e-34 | F W H M | 0.72 | 21.5 |
| 11786.493 | Fe I | 131.21 | 8e-04 | pEW | 0.44 | 7.7 | 78.82 | 6e-24 | depth | 0.37 | 10.1 |
| 11887.328 | Fe I | 141.45 | 2e-06 | pEW | 0.53 | 9.5 | 79.49 | 2e-14 | F W H M | 0.54 | 13.7 |
| 12435.644 | K I | 135.46 | 6e-12 | F W H M | 0.54 | 9.5 | 81.42 | 2e-25 | depth | 0.70 | 26.4 |
| 12525.528 | K I | 140.79 | 4e-06 | F W H M | 0.59 | 13.1 | 79.11 | 3e-26 | F W H M | 0.75 | 31.5 |
| 12825.188 | Ti I | 140.66 | 2e-07 | F W H M | 0.48 | 8.7 | 79.21 | 3e-18 | depth | 0.39 | 12.7 |
| 12903.288 | Mn I | 138.33 | 6e-10 | F W H M | 0.54 | 12.1 | 79.61 | 2e-26 | depth | 0.52 | 17.2 |
| 13322.620 | Mn I | 140.52 | 7e-06 | F W H M | 0.46 | 10.5 | 79.61 | 4e-13 | pEW | 0.43 | 15.4 |
| 15061.215 | Ca I | 138.97 | 8e-04 | F W H M | 0.24 | 7.9 | 78.99 | 3e-11 | pEW | 0.21 | 16.4 |
| 15339.017 | Ti I | 131.44 | 7e-04 | centre | 0.34 | 12.6 | 78.78 | 3e-21 | depth | 0.20 | 19.9 |
| 15792.876 | − | 134.49 | 2e-04 | centre | 0.05 | 4.0 | 92.20 | 1e-07 | depth | 0.12 | 5.2 |
| 16062.960 | − | 130.53 | 9e-04 | depth | 0.17 | 6.1 | 96.21 | 5e-05 | pEW | 0.27 | 6.7 |
| 17701.334 | − | 146.26 | 8e-10 | depth | 0.30 | 5.4 | 91.42 | 7e-05 | pEW | 0.45 | 5.9 |
Notes. λ0,med is the median of the line centres measured for both stars; Sp. is the species of the line obtained from the VALD3 database (Ryabchikova et al. 2015); P, FAP, Param, ⟨depth⟩, and ⟨F W H M⟩ correspond to the detected period, FAP for the detected period, line parameter responsible for the detected period, median line FWHM, and median line depth, respectively. All wavelength values are in vacuum.
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