Table A.1.
Times of minima and maxima for the MW stars and the time intervals we used to derive these as upper and lower index, and period and skewness for each cycle.
| HD | #cyc | tmin | tmax | Pcyc [yr] | γ |
|---|---|---|---|---|---|
| 3651 | 1 | −2600 , 2900 |
−550 |
15.06 | 0.368 |
| 4628 | 1 | −2450 , 400 |
−1000 |
7.80 | −0.049 |
| 4628 | 2 | 400, 3550 |
1800 |
8.62 | 0.242 |
| 16160 | 1 | −900 , 3550 |
1350 |
12.18 | 0.074 |
| 26965 | 1 | −2050 , 1700 |
−300 |
10.27 | −0.055 |
| 26965 | 2 | 1700, 5500 |
3450 |
10.40 | 0.207 |
| 32147 | 1 | −1050 , 2750 |
−3150 , 300 , 4850 |
10.40 | 0.127 |
| 166620 | 1 | −2200 , 3400 |
150 |
15.33 | 0.146 |
| 219834A | 1 | 150 , 3050 |
1000 |
7.94 | 0.231 |
| 219834A | 2 | 3050, 4650 |
3550 |
4.38 | 0.496 |
| 219834B | 1 | −3950 , −500 |
−2700 |
9.45 | 0.521 |
| 219834B | 2 | −500, 3150 |
1100 |
9.99 | 0.197 |
| 219834B | 3 | 3150, 5750 |
4200 |
7.12 | 0.238 |
| Sun | 1 | −1150, 2650 | 200 | 10.40 | 0.338 |
| Sun | 2 | 2650, 6200 | 3700 | 9.72 | 0.231 |
| Sun | 3 | 6200, 10800 | 7650 | 12.59 | 0.614 |
| 10476 | 3 | −2900 , 900 |
−1350 |
10.40 | 0.109 |
| 10476 | 2 | 900, 4550 |
2100 |
9.99 | 0.446 |
| 10476 | 3 | 4550, 8300 |
6400 |
10.27 | −0.224 |
| 81809 | 1 | −2650 , 350 |
−1250 |
8.21 | 0.128 |
| 81809 | 2 | 350, 3450 |
1600 |
8.49 | 0.310 |
| 81809 | 3 | 3450, 6050 |
4500 |
7.12 | 0.228 |
| 103095 | 1 | −1700 , 750 |
−600 |
6.71 | 0.260 |
| 103095 | 2 | 750, 3500 |
2100 |
7.53 | 0.018 |
| 103095 | 3 | 3500, 5900 |
4600 ,7300 |
6.57 | 0.328 |
| 114710 | 1 | 1200 , 3350 |
1750 |
5.89 | 0.761 |
| 114710 | 2 | 3350, 5300 |
4300 |
5.34 | −0.248 |
| 114710 | 3 | 5300, 7150 |
6200 |
5.07 | −0.193 |
| 115404 | 1 | −1100 , 3500 |
400 |
12.59 | 0.130 |
| 115404 | 2 | 3500, 6650 |
5300 |
8.62 | 0.186 |
| 149661 | 1 | −3350 , −1700 |
−2400 |
4.52 | 0.006 |
| 149661 | 2 | −1700, −400 |
−1300 |
3.56 | 0.524 |
| 149661 | 3 | −400, 1300 |
400 |
4.65 | −0.123 |
| 149661 | 4 | 1300, 2500 |
2000 |
3.29 | −0.114 |
| 149661 | 5 | 2500, 5100 |
3400 |
7.12 | 0.268 |
| 149661 | 6 | 5100, 6900 |
6250 |
4.93 | −0.638 |
| 152391 | 1 | −1800 , 2100 |
200 |
10.68 | −0.460 |
| 152391 | 2 | 2100, 5650 |
4050 |
9.72 | −0.038 |
| 152391 | 3 | 5650, 7700 |
6350 |
5.61 | 0.379 |
| 160346 | 1 | −3750 , −1100 |
−2700 |
7.26 | 0.008 |
| 160346 | 2 | −1100, 1400 |
150 |
6.84 | 0.178 |
| 160346 | 3 | 1400, 3950 |
2350 |
6.98 | 0.077 |
| 160346 | 4 | 3950, 6700 |
5250 |
7.53 | 0.175 |
| 201091 | 1 | −3400 , −850 |
−2300 |
6.98 | −0.085 |
| 201091 | 2 | −850, 2150 |
400 |
8.21 | −0.004 |
| 201091 | 3 | 2150, 4500 |
3400 |
6.43 | 0.071 |
| 201091 | 4 | 4500, 6900 |
5700 |
6.57 | −0.113 |
Notes. [tmin/max] = JD-2444000. tmin and tmax for the Sun are from Hathaway (2015). Intervals used in the fitting of minima are only listed once for each minimum. With HD 32147 and HD 103095, the additional maxima were used in to increase statistics in the calculation of ⟨tr⟩/⟨td⟩.
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