Table A.2
Long-term cycles and rotation periods for the stars in our sample.
| Star | P cycle | A cycle | FAP | P rot | A rot | FAP | Prot Lit | Ref. | |||
| (years) | (mmag) | (%) | (d) | (mmag) | (%) | (d) | |||||
|
|
|||||||||||
| HD 1388 | 13.4 ± 6.0 | 8.1 ± 2.2 | <0.1 | 19.9 ± 1.4 | 1 | ||||||
| 19.7 ± 2.8 | 4 | ||||||||||
| HD 10180 | 4.1 ± 0.4 | 3.3 ± 0.9 | 1.7 | 29.5 ± 0.1 | 3.3 ± 0.9 | 3.7 | 24.1 ± 3.0 | 4 | |||
| HD 21019 | 29.5 ± 0.1 | 5.9 ± 1.3 | 0.7 | 38.4 ± 3.5 | 4 | ||||||
| HD 2071 | 11.2 ± 3.6 | 4.9 ± 1.3 | <0.1 | 29.6 ± 0.1 | 3.1 ± 0.9 | <0.1 | 22.8 ± 0.7 | 1 | |||
| HD 1320 | 3.3 ± 0.2 | 2.6 ± 0.8 | 2.1 | 29.6 ± 0.1 | 2.5 ± 0.8 | 2.7 | 28.4 ± 8.7 | 1 | |||
| HD 63765 | 12.9 ± 4.9 | 3.9 ± 0.9 | <0.1 | 29.5 ± 0.1 | 2.7 ± 1.0 | 0.2 | 26.7 ± 6.7 | 1 | |||
| HD 82558* | 2.5 ± 0.1 | 13.6 ± 1.1 | 0.3 | 1.6 ± 0.1 | 28.7 ± 0.9 | <0.1 | 1.60 ± 0.0 | 6 | |||
| HD 155885 | 6.2 ± 0.1 | 36.9 ± 1.0 | <0.1 | 21.1± 2.1a | 7 | ||||||
| HD 224789 | 7.1 ± 0.9 | 6.7 ± 1.3 | <0.1 | 16.6 ± 0.1 | 6.8 ± 1.2 | <0.1 | 16.9 ± 1.8 | 1 | |||
| 11.8 ± 4.7 | 4 | ||||||||||
| V660 Tau | 7.1 ± 0.2 | 31.7 ± 1.5 | <0.1 | 0.2 ± 0.0 | 35.9 ± 1.5 | <0.1 | 0.23 ± 0.02a | 8 | |||
| HD 176986 | 7.3 ± 0.7 | 4.8 ± 1.2 | <0.1 | 33.4 ± 0.2 | 1 | ||||||
| 39.0 ± 5.3 | 4 | ||||||||||
| HD 32147 | 5.8 ± 0.5 | 7.5 ± 1.3 | <0.1 | 47.4 ± 4.7a | 10 | ||||||
| HD 45088* | 7.0 ± 0.1 | 14.2 ± 1.2 | <0.1 | 7.4 ± 0.7a | 9 | ||||||
| HD 104067 | 7.7 ± 1.3 | 4.1 ± 0.7 | <0.1 | 27.4 ± 0.1 | 2.8 ± 0.7 | 5.0 | 29.8 ± 3.1 | 1 | |||
| HD 215152* | 29.8 ± 0.1 | 2.4 ± 1.1 | 3.0 | 36.5 ± 1.6 | 1 | ||||||
| 41.8 ± 5.6 | 4 | ||||||||||
| V410 Tau | 1.9 ± 0.1 | 253.2 ± 2.7 | <0.1 | 1.9 ± 0.2a | 12 | ||||||
| HD 131977 | 5.1 ± 0.2 | 34.5 ± 1.8 | <0.1 | ||||||||
| HD 125595 | 5.9 ± 0.6 | 4.1 ± 0.9 | <0.1 | 29.4 ± 0.1 | 2.9 ± 0.9 | 10.3 | 37.2 ± 2.0 | 1 | |||
| HD 118100 | 9.3 ± 0.4 | 17.3 ± 1.1 | <0.1 | 3.9 ± 0.1 | 30.4 ± 0.9 | <0.1 | |||||
| GJ9482 | 10.1 ± 1.4 | 6.9 ± 0.9 | <0.1 | ||||||||
| HD 113538 | 6.6 ± 0.6 | 4.9 ± 0.9 | <0.1 | 43.9 ± 0.2 | 4.6 ± 0.8 | 2.5 | |||||
| GJ846 | 8.5 ± 1.1 | 7.3 ± 1.2 | <0.1 | 31.0 ± 0.1 | 1 | ||||||
| GJ676A | 7.5 ± 0.6 | 8.2 ± 1.0 | <0.1 | 41.2 ± 3.8 | 1 | ||||||
| GJ229 | 8.4 ± 0.3 | 12.8 ± 0.9 | <0.1 | 27.3 ± 0.1 | 2.9 ± 0.9 | 11.4 | |||||
| HD 197481 | 7.6 ± 0.4 | 14.4 ± 1.7 | <0.1 | 4.9 ± 0.1 | 18.6 ± 1.1 | <0.1 | |||||
| GJ514 | 9.9 ± 3.8 | 5.8 ± 1.4 | <0.1 | 28.0 ± 2.9 | 1 | ||||||
| GJ239 | 4.9 ± 0.4 | 5.2 ± 1.0 | <0.1 | ||||||||
| GJ205 | 10.8 ± 1.1 | 9.3 ± 0.8 | <0.1 | 33.4 ± 0.1 | 4.8 ± 0.8 | <0.1 | 35.0 ± 0.1 | 1 | |||
| 3.9 ± 0.3 | 6.9 ± 1.4 | <0.1 | |||||||||
| GJ832 | 13.2 ± 4.2 | 6.8 ± 1.5 | <0.1 | 45.7 ± 9.3 | 1 | ||||||
| GJ536 | 43.3 ± 0.1 | 4.8 ± 1.1 | <0.1 | 43.8 ± 0.1 | 1 | ||||||
| GJ382 | 13.6 ± 1.7 | 15.1 ± 1.0 | <0.1 | 21.2 ± 0.1 | 5.7 ± 0.9 | <0.1 | 21.7 ± 0.1 | 1 | |||
| 21.6 ± 2.2a | 2 | ||||||||||
| GJ588 | 5.2 ± 0.7 | 3.1 ± 1.2 | 0.5 | 43.1 ± 0.2 | 2.7 ± 1.1 | 2.3 | 61.3 ± 6.5 | 1 | |||
| GJ176 | 5.9 ± 0.7 | 6.5 ± 1.6 | 1.5 | 40.8 ± 0.1 | 7.0 ± 1.3 | <0.1 | 39.3 ± 0.1 | 1 | |||
| 38.9 ± 3.9a | 2 | ||||||||||
| GJ752A | 9.3 ± 1.9 | 7.7 ± 3.2 | <0.1 | 46.0 ± 0.2 | 4.5 ± 1.1 | <0.1 | 46.5 ± 0.3 | 1 | |||
| GJ674 | 10.1 ± 0.8 | 17.7 ± 1.2 | <0.1 | 35.0 ± 0.1 | 5.5 ± 1.1 | <0.1 | 32.9 ± 0.1 | 1 | |||
| 33.3 ± 3.3a | 2 | ||||||||||
| GJ680 | 5.0 ± 0.2 | 8.4 ± 0.9 | <0.1 | ||||||||
| GJ408 | 5.3 ± 0.6 | 6.4 ± 1.5 | 2 | ||||||||
| GJ877 | 52.8 ± 0.1 | 7.8 ± 0.7 | <0.1 | 116.1 ± 0.7 | 1 | ||||||
| GJ479 | 2.0 ± 0.1 | 5.7 ± 1.1 | <0.1 | 22.5 ± 0.1 | 4.9 ± 1.1 | 1.2 | |||||
| GJ358* | 4.9 ± 0.1 | 20.5 ± 0.9 | <0.1 | 25.2 ± 0.1 | 12.1 ± 0.7 | <0.1 | 16.8 ± 1.6 | 1 | |||
| 25.0 ± 2.5a | 2 | ||||||||||
| GJ273 | 6.6 ± 1.3 | 7.7 ± 1.5 | <0.1 | 115.9 ± 19.4 | 1 | ||||||
| GJ849 | 10.2 ± 0.9 | 12.4 ± 1.0 | <0.1 | 39.2 ± 6.3 | 1 | ||||||
| GJ729 | 7.1 ± 0.1 | 5.3 ± 0.7 | <0.1 | 2.9 ± 0.1 | 8.8 ± 0.9 | <0.1 | 2.87 | 2 | |||
| 2.1 ± 0.1 | 7.9 ± 0.5 | <0.1 | |||||||||
| GJ896A | 15.3 ± 0.1 | 25.2 ± 1.3 | <0.1 | ||||||||
| GJ317 | 5.2 ± 0.3 | 12.4 ± 1.1 | <0.1 | ||||||||
| GJ526 | 9.9 ± 2.8 | 6.9 ± 1.0 | <0.1 | 52.3 ± 1.7 | 1 | ||||||
| GJ234 | 5.9 ± 0.5 | 10.1 ± 1.4 | <0.1 | 8.1 ± 0.1 | 7.7 ± 1.3 | 0.3 | |||||
| GJ54.1 | 69.2 ± 0.1 | 15.6 ± 1.1 | <0.1 | ||||||||
Notes.
Reference. For rotation periods in the literature: 1) Suárez Mascareño et al. (2015) using periodic variations of CaII H&K and Hα emission lines. 2) Kiraga & Stepien (2007) using periodic variations in the photometry of the ASAS survey. 3) Robertson et al. (2014) using periodic variations of Hα emission line. 4) Lovis et al. (2011) using Mamajek & Hillenbrand (2008) age-activity-rotation relationship. 5) Olmedo et al. (2013) using their own activity-rotation relationship based on the MgII H&K emission lines. 6) Jetsu (1993) using periodic variations in photometry. 7) Donahue et al. (1996) using periodic variations in photometry. 8) Wright et al. (2011) using periodic variations in photometry. 9) Strassmeier et al. (1993) using periodic variations in photometry. 10) Saar & Osten (1997) estimated from CaII H&K measurements. 11) Chugainov (1974) using periodic variations in brightness. 12) Strassmeier (2009) using periodic variations in photometry.
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