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Table A.2

Cool stars with well determined activity cycles are tabulated first, followed by chaotic and multiple cycles, and finally probable cycles.

No. Name Spectype Prot Pcyc FAP Pcyc(2) FAP(2) B − V τc Branch Survey
CA: Cool stars with clear well defined solar-like activity cycles
1 Sun† G2V 25 10.7 ± 0.08 1.0e-545 .. .. .. MW
2 HD 3651† K0V 44.0 14.9 ± 0.2 4.2e-97 .. .. 0.85 20.87 I MW
3 HD 4628† K4V 38.5 8.47 ± 0.05 4.4e-194 .. .. 0.89 21.72 I MW
4 HD 10476† K1V 35.2 10.59 ± 0.1 2.6e-122 .. .. 0.836 20.51 I MW
5 HD 16160† K3V 48.0 12.7 ± 0.11 2.4e-183 .. .. 0.918 22.16 I MW
6 HD 26965† K1V 43.0 10.23 ± 0.07 1.2e-163 .. .. 0.82 20.04 I MW
7 HD 32147† K5V 48.0 10.84 ± 0.15 1.5e-60 .. .. 1.049 23.38 I MW
8 HD 81809† G2V 40.2 8.01 ± 0.05 1.8e-129 .. .. 0.655 12.27 I MW
9 HD 103095† K1V 31.0 7.06 ± 0.05 7.0e-129 .. .. 0.754 17.51 I MW
10 HD 152391† G7V 11.43 11.97 ± 0.1 6.3e-199 .. .. 0.749 17.28 A MW
11 HD 160346† K3V 36.4 7.19 ± 0.04 3.5e-173 .. .. 0.594 8.75 I MW
12 HD 166620† K2V 42.4 17.05 ± 0.2 4.8e-173 .. .. 0.876 21.46 I MW
13 HD 185144† K0V 29.0 7.07 ± 0.14 2.2e-124 .. .. 0.786 18.85 I MW
14 HD 201091† K5V 35.7 7.1 ± 0.05 4.0e-131 .. .. 1.069 23.53 I MW
15 HD 219834B† K2V 43.0 9.42 ± 0.1 2.5e-81 .. .. 0.787 18.89 I MW
CB: Cool stars with multiple cycles
1 HD 1835† G2.5V 7.78 22.0 ± 0.93 4.2e-44 9.06 ± 0.15 5.5e-39 0.659 12.51 A MW
2 HD 101501 G8V 16.68 23.2 ± 1.5 3.4e-53 4.5 ± 0.03 6.4e-39 0.723 16.02 .. MW
3 HD 149661† K2V 21.07 15.3 ± 0.4 8.5e-72 7.7 ± 0.12 1.2e-42 0.827 20.25 A MW
4 HD 190406† G1V 13.94 2.6 ± 0.02 1.1e-52 18.7 ± 0.9 8.8e-50 0.61 9.67 I MW
5 HD 20630† G5V 9.24 22.3 ± 0.98 6.3e-51 5.7 ± 0.15 2.9e-11 0.681 13.77 A MW
CC: Cool stars with probable activity cycles
1 HD 10780 K0V 21.7 10.14 ± 0.31 1.8e-43 .. .. 0.804 19.51 .. MW
2 HD 18256† FIV-V 3.0 5.89 ± 0.11 1.2e-27 .. .. 0.471 3.11 A MW
3 HD 26913† G8V 7.1 13.3 ± 0.5 2.8e-41 .. .. 0.68 13.71 A MW
4 HD 26923 G0V 60.4 8.58 ± 0.17 1.4e-32 .. .. 0.57 7.48 .. MW
5 HD 37394 K1V 10.74 3.67 ± 0.07 7.2e-13 .. .. 0.84 20.62 .. MW
6 HD 76151† G3V 15.0 18.1 ± 0.76 5.9e-80 .. .. 0.661 12.62 I MW
7 HD 78366† G0V 9.67 13.34 ± 0.38 1.4e-48 .. .. 0.585 8.26 A MW
8 HD 82443 K0V 5.37 13.84 ± 3.9 1.8e-21 .. .. 0.779 18.58 .. MW
9 HD 82885† G8IV-V 18.6 7.69 ± 0.14 4.0e-31 .. .. 0.77 18.212 A MW
10 HD 100180 F7V 14.6 3.6 ± 0.04 6.7e-33 .. .. 0.57 7.45 .. MW
11 HD 115043 G1V 5.86 1.6 ± 0.02 1.0e-13 .. .. 0.603 9.26 .. MW
12 HD 115383† F8V 3.33 11.79 ± 0.28 5.5e-29 .. .. 0.585 8.26 A MW
13 HD 146233 G2V 22.7 11.36 ± 1.23 2.1e-02 .. .. 0.652 12.10 .. MW
14 HD 155885† K1V 21.11 5.83 ± 0.01 2.2e-33 .. .. 0.855 21.0 A MW
15 HD 155886† K1V 20.69 21.6 ± 1.2 3.23e-23 .. .. 0.855 21.0 A MW
16 HD 156026† K5V 21.0 21.3 ± 0.83 3.4-85 .. .. 1.144 24.10 .. MW
17 HD 165341A† K0V 19.7 5.07 ± 0.05 1.3e-48 .. .. 0.86 21.11 A MW
18 HD 190007 K4V 28.98 5.38 ± 0.06 9.3e-31 .. .. 1.128 23.98 .. MW
19 HD 201092† K7V 37.84 11.1 ± 0.18 3.3e-60 .. .. 1.31 25.45 I MW
20 HD 20003 G8V 37.1 7.7 ± 0.5 3.8e-09 .. .. 0.77 18.25 .. H
21 HD 20619 G1.5V 22.3 5.0 ± 0.2 1.5e-14 .. .. 0.65 12.27 .. H
22 HD 21693 G9IV-V 36.3 7.4 ± 0.3 6.9e-19 .. .. 0.71 15.35 .. H
23 HD 45184 G2V 21.4 4.9 ± 0.3 1.8e-23 .. .. 0.626 10.59 .. H
24 HD 7199 K0IV-V 41.0 4.0 ± 0.3 1.9e-11 .. .. 0.55 6.42 .. H
25 HD 82516 K2V 36.7 4.2 ± 0.1 1.1e-09 .. .. 0.93 22.28 .. H
26 HD 89454 G5V 21.1 4.0 ± 0.8 1.2e-07 .. .. 0.72 15.71 .. H
27 HD 157830 G6V 24.3 3.9 ± 0.5 3.9e-06 .. .. 0.68 13.98 .. H
28 HD 361 G1V 14.1 4.6 ± 0.2 8.6e-03 .. .. 0.624 10.48 .. H
29 HD 12617 K3V 30.7 4.5 ± 2.2 4.5e-03 .. .. 1.02 23.16 .. H
30 HD 166724 K0IV-V 30.9 2.4 ± 0.2 1.8e-04 .. .. 1.46 26.69 .. H
31 HD 21749 K4.5V 34.5 9.1 ± 6.3 3.4e-10 .. .. 1.13 23.99 .. H
32 HD 154577 K2.5V 45.8 5.9 ± 0.1 5.4e-66 .. .. 0.88 21.71 .. H
33 HD 88742 G0V 11.3 2.9 ± 0.1 1.3e-15 .. .. 0.59 8.65 .. H

Notes. The HD name of the star is shown in Col. 2, the spectral type in Col. 3 and the rotation period (days) in Col. 4. Columns 5, 6, 7 and 8 show the cycle periods (years) and FAPs of the stars determined in this work. The B − V and τc are shown in Cols. 9 and 10. Finally Cols. 11 and 12 show the Active and Inactive branch classification from Saar & Brandenburg (1999) and the corresponding surveys. MW stands for Mount Wilson and H stands for HARPS. The † symbol shows stars which were previously included in the analysis of Saar & Brandenburg (1999). The rotation periods for the Mount Wilson stars are taken from Saar & Brandenburg (1999) and Hempelmann et al. (2016), except for a few cases as follows: HD 10780, HD 26923, HD 3734 (Gaidos et al. 2000), HD 82443 (Messina et al. 1999), HD 100180 (Oláh et al. 2016), HD 146233 (Petit et al. 2008). The rotation periods for the HARPS stars are taken from Lovis et al. (2011). The τc used here is calculated based on the empirical relation of Noyes et al. (1984a), where τc is a function of B − V.

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