Table 2
Synthesis of the characterisation and long-term activity analysis developed in this work.
Star | # Spectra | Time span (d) | ⟨S⟩ | σS/⟨S⟩ | log ![]() |
σlog ![]() |
Pcyc (d) | FAP (%) IB 19 | Bootstrap |
---|---|---|---|---|---|---|---|---|
GJ 1 | 68 | 5238 | 0.399 | 0.140 | −5.537 | 0.145 | 4286 ± 479 | 0.01 | 0.04 |
GJ 15 A | 13 | 15 | 0.427 | 0.046 | −5.513 | 0.041 | − | − |
GJ 79 | 22 | 6589 | 1.703 | 0.064 | −4.497 | 0.032 | − | − |
GJ 169 | 3 | 9 | 1.287 | 0.036 | −4.524 | 0.018 | − | − |
GJ 176 | 112 | 4813 | 1.477 | 0.137 | −4.823 | 0.070 | − | − |
GJ 205 | 102 | 7675 | 1.801 | 0.175 | −4.614 | 0.088 | 5313 ± 862 | <0.1 | <0.01 |
GJ 229 A | 86 | 7698 | 1.487 | 0.130 | −4.665 | 0.066 | 4949 ± 423 | <0.1 | <0.01 |
GJ 273 | 172 | 4490 | 0.752 | 0.094 | −5.491 | 0.063 | − | − |
GJ 338 B | 7 | 2958 | 1.765 | 0.077 | −4.393 | 0.037 | − | − |
GJ 393 | 154 | 5121 | 0.939 | 0.081 | −5.066 | 0.045 | 1124 ± 29 | 0.003 | 0.02 |
GJ 406 | 33 | 3733 | 155.893 | 0.902 | −3.986 | 0.402 | − | − |
GJ 411 | 1 | − | 0.397 | − | −5.615 | − | − | − |
GJ 412 A | 12 | 1742 | 0.350 | 0.115 | −5.675 | 0.121 | − | − |
GJ 447 | 65 | 4331 | 1.211 | 0.190 | −5.406 | 0.107 | 1956 ± 98 IB | 0.0002 |
GJ 488 | 67 | 5232 | 1.603 | 0.097 | −4.480 | 0.048 | − | − |
GJ 526 | 47 | 6232 | 0.736 | 0.090 | −5.106 | 0.056 | 3739 ± 288 | 0.013 | 0.08 |
GJ 536 | 216 | 5842 | 1.120 | 0.116 | −4.840 | 0.061 | 1643 ± 58 | 0.008 | 0.06 |
4044 ± 443 | 0.05 | 0.1 | |||||||
GJ 551 | 140 | 5495 | 11.994 | 0.399 | −4.807 | 0.160 | 4121 ± 321 | 0.02 | 0.05 |
GJ 570 B | 129 | 1859 | 1.394 | 0.099 | −4.821 | 0.049 | − | − |
GJ 581 | 30 | 1883 | 0.537 | 0.106 | −5.606 | 0.082 | − | − |
GJ 628 | 154 | 4998 | 0.715 | 0.139 | −5.518 | 0.094 | 4498 ± 607 | 0.004 | 0.01 |
GJ 674 | 74 | 5470 | 1.585 | 0.165 | −4.869 | 0.082 | − | − |
GJ 687 | 98 | 4 | 0.558 | 0.030 | −5.519 | 0.023 | − | − |
GJ 699 | 72 | 5834 | 0.695 | 0.319 | −5.533 | 0.185 | 3281 ± 255 | 0.001 | 0.02 |
GJ 725 A | 21 | 3 | 0.454 | 0.088 | −5.642 | 0.076 | − | − |
GJ 725 B | 50 | 612 | 0.752 | 0.643 | −5.387 | 0.277 | − | − |
GJ 729 | 103 | 7603 | 7.418 | 0.274 | −4.335 | 0.116 | 1521 ± 20 IB2 | <0.1 |
GJ 752 A | 305 | 5892 | 1.004 | 0.124 | −5.070 | 0.069 | 4416 ± 462 | <0.01 | 0.02 |
GJ 809 | 61 | 5152 | 1.545 | 0.148 | −4.647 | 0.076 | 2898 ± 273 | 0.001 | 0.03 |
GJ 825 | 37 | 5474 | 1.094 | 0.101 | −4.673 | 0.051 | 2593 ± 137 | 0.04 | 0.1 |
7038 ± 2700 | 0.0002 | 0.01 | |||||||
GJ 832 | 172 | 5632 | 0.699 | 0.118 | −5.175 | 0.072 | 2297 ± 54 | <0.1 | <0.01 |
GJ 876 | 96 | 3261 | 0.918 | 0.112 | −5.435 | 0.073 | − | − |
GJ 880 | 125 | 4450 | 1.635 | 0.072 | −4.681 | 0.036 | − | − |
GJ 887 | 79 | 2120 | 1.131 | 0.114 | −4.797 | 0.060 | − | − |
GJ 908 | 39 | 3525 | 0.490 | 0.124 | −5.326 | 0.095 | − | − |
Notes. In Cols. 4 and 5 we show, respectively, the S index obtained for each star in the sample and its variability. In Cols. 6 and 7 we show the chromospheric activity levels measured from the log indicator and their standard deviation. Finally, we report the detected magnetic activity cycles with their FAPs in Cols. 8 and 9, respectively. With IB and IB2 we highlight the cycles extracted from Ibañez Bustos et al. (2019b) and Ibañez Bustos et al. (2020), respectively.
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