Table 1.
Our sample of Mount Wilson stars.
Star | ncyc | ![]() |
Teff [K] | Prot [d] | Pcyc [yr] | ⟨γ⟩ | σ | ⟨tr⟩/⟨td⟩ | nbin | FAP | MS/G | Data |
---|---|---|---|---|---|---|---|---|---|---|---|---|
HD 3651 | 1 | −5.040 | 5280 | 37.0 | 15.06 | 0.368 | ... | 0.594 | 10 | G | MS | 1995 |
HD 4628 | 2 | −4.874 | 5014 | 37.14 | 8.21 ± 0.41 | 0.096 | 0.145 | 0.905 | 10 | E | MS | 1995 |
HD 16160 | 1 | −4.902 | 4762 | 48.58 | 12.18 | 0.074 | ... | 1.023 | 10 | E | MS | 1995 |
HD 26965 | 2 | −4.919 | 5196 | 38.65 | 10.34 ± 0.07 | 0.076 | 0.131 | 0.864 | 10 | E | MS | 1995 |
HD 32147 | 1 | −4.939 | 4703 | 33.7 | 10.40 | 0.127 | ... | 0.758 | 10 | E | MS | 1995 |
HD 166620 | 1 | −4.975 | 5007 | 42.1 | 15.33 | 0.146 | ... | 0.723 | 10 | E | MS | 1995 |
HD 219834A | 2 | −5.098 | 5705 | 43.4 | 6.16 ± 1.78 | 0.364 | 0.133 | 0.429 | 7 | G | G | 1995 |
HD 219834B | 3 | −4.919 | 5136 | 34.78 | 8.86 ± 1.25 | 0.319 | 0.144 | 0.672 | 8 | E | G | 1995 |
Sun | 3 | −4.911 | 5780 | 26.09 | 10.90 ± 1.23 | 0.394 | 0.161 | 0.625 | 10 | E | MS | 1995+SP |
HD 10476 | 3 | −4.962 | 5489 | 35.6 | 10.23 ± 0.16 | 0.111 | 0.273 | 0.697 | 10 | E | MS | 2001 |
HD 81809 | 3 | −4.940 | 5889 | 41.66 | 7.94 ± 0.59 | 0.222 | 0.074 | 0.740 | 9 | E | G | 2001 |
HD 103095 | 3 | −4.939 | 5265 | 34.03 | 6.94 ± 0.42 | 0.202 | 0.133 | 0.917 | 10 | E | MS | 2001 |
HD 114710 | 3 | −4.738 | 6098 | 11.99 | 5.44 ± 0.34 | 0.107 | 0.463 | 0.676 | 8 | G | MS | 2001 |
HD 115404 | 2 | −4.502 | 4976 | 18.03 | 10.62 ± 1.99 | 0.158 | 0.028 | 0.742 | 10 | G | MS | 2001 |
HD 149661 | 6 | −4.625 | 5265 | 20.76 | 4.68 ± 1.25 | −0.013 | 0.361 | 0.916 | 5 | G | MS | 2001 |
HD 152391 | 3 | −4.469 | 5461 | 10.62 | 8.67 ± 2.19 | −0.040 | 0.342 | 0.959 | 8 | E | MS | 2001 |
HD 160346 | 4 | −4.818 | 4897 | 32.0 | 7.15 ± 0.26 | 0.109 | 0.071 | 0.772 | 7 | E | MS | 2001 |
HD 201091 | 4 | −4.588 | 4177 | 35.54 | 7.05 ± 0.70 | −0.033 | 0.072 | 0.873 | 9 | E | MS | 2001 |
Notes. FAP = E/G (excellent/good) as defined by Baliunas et al. (1995). MS = main-sequence star, G = giant. Pcyc is given with its standard deviation; thus there are no ‘error bars’ for stars with only one detected cycle. γ for the Sun was calculated from solar cycles 21–23, for which MW+SP data are available, but to calculate ⟨tr⟩/⟨td⟩, cycles 1–20 were also included, where all tmin and tmax are from the dates listed in Hathaway (2015). Source of Teff for the Sun: Cox (2000).
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