Table A.2
The Ca II H and K analysis for the HARPS M dwarf sample (minimal; full version available at the CDS).
| Name | V | B−V | V−K | π | σ π | Ref. | M | N | S | σ S |
|
|
P rot | S / N VR |
| [mas] | [mas] | Phot, π | M / M ⊙ | × 105 | [d] | |||||||||
|
|
||||||||||||||
| Gl551 | 11.09 | 1.90 | 6.730 | 771.64 | 2.60 | (1), (3) | 0.12 | 76 | 11.265 | 9.641 | –5.003 | 0.915 | 42 | 7.5 |
| Gl388 | 9.32 | 1.53 | 4.710 | 204.60 | 2.80 | (1), (3) | 0.42 | 41 | 8.690 | 1.089 | –4.191 | 0.834 | 12 | 28.3 |
| LHS3746 | 11.82 | 1.54 | 5.078 | 134.29 | 1.31 | (2), (5) | 0.24 | 6 | 0.783 | 0.109 | –5.610 | 0.058 | 107 | 7.2 |
| HIP 74261 | 10.73 | 1.28 | 3.558 | 41.26 | 2.31 | (2), (3) | 0.60 | 5 | 1.685 | 0.079 | –4.473 | 0.182 | 19 | 12.4 |
| HD 329868 | 10.81 | 1.21 | 3.698 | 46.39 | 3.65 | (2), (3) | 0.56 | 6 | 1.452 | 0.154 | –4.609 | 0.308 | 23 | 10.4 |
| HD 329879 | 11.25 | 1.34 | 3.731 | 36.84 | 2.45 | (2), (3) | 0.58 | 12 | 1.506 | 0.202 | –4.604 | 0.391 | 23 | 10.1 |
| LHS1134 | 13.05 | 1.59 | 5.316 | 113.90 | 34.20 | (2), (3) | 0.17 | 4 | 0.665 | 0.452 | –5.733 | 0.034 | 129 | 3.2 |
| GJ163 | 11.82 | 1.52 | 4.680 | 66.69 | 1.82 | (1), (3) | 0.40 | 179 | 0.703 | 0.135 | –5.480 | 0.106 | 87 | 9.4 |
| HIP 19394 | 11.90 | 1.37 | 4.741 | 66.69 | 1.82 | (2), (3) | 0.40 | 20 | 0.684 | 0.094 | –5.532 | 0.070 | 95 | 9.3 |
| BD–120662 | 10.12 | 1.25 | 3.648 | 45.28 | 1.97 | (2), (3) | 0.71 | 8 | 1.846 | 0.069 | –4.467 | 0.144 | 19 | 17.4 |
Notes. We listed: i) the V magnitude, B−V, V−K color-indexes, and their references (Ref. Phot., see below); ii) the parallax (π), its uncertainty (σπ), and the references (Ref. π, see below); iii) the stellar masses; iv) the number of spectra used in the analysis for a given target (N); vi) the median of the S-index and its dispersion (σS); vii) the median of the 
and its dispersion (); viii) the rotation period derived from Eq. (12); and ix) the averaged S/N in the violet and red bands.
Reference. (1) Leggett (1992); (2) Gaidos et al. (2014); (3) van Leeuwen (2007); (4) van Altena et al. (1995); (5) RECONS; (6) Lépine & Gaidos (2011).
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