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Table 1
Stars with validated rotation periods.
KIC | νmax [μHz] | Δν [μHz] | Teff [K] | log g [dex] | M [M⊙] | Prot [day] | Crowding | Tcrit [day] | vsini [km s-1] | ||||||||
|
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1161618 | 34.25 ± 1.88 | 4.09 ± 0.14 | 4855 ± 161 | 1.29 ± 0.16 | 2.45 ± 0.03 | 158.34 ± 7.90 | 0.990 | 7.26 | 0.00 ± 0.00 | ||||||||
1162746 | 27.58 ± 1.81 | 3.64 ± 0.13 | 5141 ± 308 | 1.17 ± 0.18 | 2.37 ± 0.04 | 46.74 ± 4.72 | 1.000 | 8.16 | 0.00 ± 0.00 | ||||||||
1871631 | 29.29 ± 2.15 | 3.71 ± 0.11 | 4823 ± 108 | 1.18 ± 0.17 | 2.38 ± 0.03 | 44.54 ± 3.08 | 0.990 | 8.01 | 0.00 ± 0.00 | ||||||||
2018667 | 30.73 ± 1.80 | 3.83 ± 0.14 | 4773 ± 123 | 1.19 ± 0.15 | 2.40 ± 0.03 | 65.67 ± 3.52 | 0.990 | 7.75 | 0.00 ± 0.00 | ||||||||
2019396 | 37.98 ± 1.89 | 4.16 ± 0.13 | 4790 ± 100 | 1.62 ± 0.18 | 2.49 ± 0.02 | 63.86 ± 8.70 | 0.990 | 7.14 | 0.00 ± 0.00 | ||||||||
2156178 | 29.08 ± 1.87 | 3.93 ± 1.91 | 5099 ± 225 | 1.00 ± 0.98 | 2.39 ± 0.03 | 40.98 ± 3.18 | 1.000 | 7.56 | 0.00 ± 0.00 | ||||||||
2305930 | 28.27 ± 1.78 | 3.97 ± 0.14 | 4924 ± 173 | 0.84 ± 0.11 | 2.37 ± 0.03 | 33.75 ± 2.52 | 0.990 | 7.48 | 13.09 ± 0.88 | ||||||||
2436732 | 30.34 ± 1.76 | 3.70 ± 0.11 | 4719 ± 147 | 1.29 ± 0.16 | 2.39 ± 0.03 | 109.63 ± 5.17 | 0.980 | 8.03 | 0.00 ± 0.00 | ||||||||
2447529 | 106.95 ± 4.87 | 8.38 ± 0.18 | 5186 ± 247 | 2.47 ± 0.26 | 2.96 ± 0.03 | 98.83 ± 5.49 | 0.990 | 3.54 | 0.00 ± 0.00 | ||||||||
2716214 | 30.26 ± 1.95 | 3.91 ± 0.12 | 5120 ± 279 | 1.16 ± 0.17 | 2.41 ± 0.03 | 41.31 ± 2.07 | 0.990 | 7.60 | 0.00 ± 0.00 | ||||||||
2845408 | 74.76 ± 3.95 | 6.38 ± 0.12 | 5058 ± 185 | 2.42 ± 0.26 | 2.80 ± 0.03 | 142.71 ± 14.66 | 0.990 | 4.66 | 0.00 ± 0.00 | ||||||||
2845610 | 90.10 ± 5.20 | 6.97 ± 0.14 | 5095 ± 151 | 3.00 ± 0.34 | 2.88 ± 0.03 | 79.72 ± 8.51 | 1.000 | 4.26 | 0.00 ± 0.00 | ||||||||
2854994 | 133.16 ± 10.78 | 10.26 ± 0.21 | 5003 ± 117 | 2.01 ± 0.30 | 3.05 ± 0.04 | 132.27 ± 6.54 | 1.000 | 2.89 | 0.00 ± 0.00 | ||||||||
2856412 | 35.67 ± 2.05 | 4.23 ± 0.58 | 4904 ± 222 | 1.30 ± 0.39 | 2.47 ± 0.03 | 9.77 ± 0.52 | 0.990 | 7.02 | 0.00 ± 0.00 | ||||||||
2860936 | 102.01 ± 5.63 | 7.59 ± 0.84 | 5062 ± 144 | 3.07 ± 0.75 | 2.93 ± 0.03 | 114.32 ± 5.55 | 1.000 | 3.91 | 0.00 ± 0.00 | ||||||||
2988655 | 30.63 ± 1.70 | 3.87 ± 0.61 | 5158 ± 313 | 1.27 ± 0.43 | 2.42 ± 0.03 | 71.85 ± 6.93 | 0.990 | 7.67 | 0.00 ± 0.00 | ||||||||
3102990 | 29.77 ± 1.86 | 3.79 ± 0.56 | 4835 ± 177 | 1.15 ± 0.36 | 2.39 ± 0.03 | 85.44 ± 7.84 | 1.000 | 7.84 | 0.00 ± 0.00 | ||||||||
3216467 | 31.47 ± 1.96 | 3.83 ± 0.12 | 4623 ± 154 | 1.21 ± 0.16 | 2.40 ± 0.03 | 151.87 ± 8.36 | 0.990 | 7.75 | 0.00 ± 0.00 | ||||||||
3220837 | 132.56 ± 20.10 | 13.21 ± 0.31 | 5294 ± 260 | 0.79 ± 0.21 | 3.06 ± 0.07 | 79.73 ± 7.54 | 0.990 | 2.25 | 0.00 ± 0.00 | ||||||||
3240280 | 29.19 ± 1.71 | 3.78 ± 1.71 | 4810 ± 121 | 1.08 ± 0.99 | 2.38 ± 0.03 | 103.83 ± 5.30 | 0.990 | 7.86 | 0.00 ± 0.00 | ||||||||
3324186 | 32.44 ± 2.20 | 3.91 ± 0.09 | 4724 ± 110 | 1.26 ± 0.16 | 2.42 ± 0.03 | 51.87 ± 4.32 | 0.980 | 7.60 | 0.00 ± 0.00 | ||||||||
3432732 | 80.48 ± 3.81 | 6.45 ± 0.13 | 5015 ± 150 | 2.85 ± 0.28 | 2.83 ± 0.02 | 121.75 ± 5.62 | 1.000 | 4.60 | 0.00 ± 0.00 | ||||||||
3437031 | 63.45 ± 2.74 | 5.60 ± 0.18 | 5059 ± 214 | 2.49 ± 0.28 | 2.73 ± 0.02 | 138.77 ± 7.22 | 0.990 | 5.30 | 0.00 ± 0.00 | ||||||||
3439466 | 29.33 ± 1.65 | 3.91 ± 0.11 | 4991 ± 235 | 1.01 ± 0.13 | 2.39 ± 0.03 | 46.75 ± 4.41 | 0.990 | 7.60 | 0.00 ± 0.00 | ||||||||
3448282 | 30.45 ± 1.54 | 3.59 ± 0.09 | 4891 ± 241 | 1.55 ± 0.18 | 2.40 ± 0.03 | 55.98 ± 4.69 | 0.990 | 8.27 | 0.00 ± 0.00 | ||||||||
3526625 | 34.35 ± 2.51 | 4.18 ± 0.15 | 4883 ± 184 | 1.21 ± 0.18 | 2.45 ± 0.04 | 125.11 ± 5.95 | 1.000 | 7.11 | 0.00 ± 0.00 | ||||||||
3532985 | 94.84 ± 10.80 | 7.92 ± 0.27 | 4752 ± 122 | 1.89 ± 0.40 | 2.89 ± 0.05 | 6.03 ± 0.29 | 0.990 | 3.75 | 0.00 ± 0.00 | ||||||||
3557606 | 100.96 ± 6.24 | 8.09 ± 0.24 | 5044 ± 118 | 2.29 ± 0.29 | 2.93 ± 0.03 | 26.34 ± 2.99 | 0.990 | 3.67 | 0.00 ± 0.00 | ||||||||
3642135 | 51.25 ± 2.53 | 4.96 ± 0.15 | 5060 ± 175 | 2.13 ± 0.24 | 2.64 ± 0.02 | 144.72 ± 7.10 | 1.000 | 5.99 | 0.00 ± 0.00 | ||||||||
3750783 | 110.02 ± 4.91 | 8.68 ± 0.20 | 5249 ± 300 | 2.38 ± 0.27 | 2.97 ± 0.03 | 6.79 ± 0.45 | 0.990 | 3.42 | 0.00 ± 0.00 | ||||||||
3758731 | 74.83 ± 5.98 | 6.28 ± 0.18 | 5119 ± 248 | 2.63 ± 0.42 | 2.80 ± 0.04 | 115.12 ± 3.69 | 1.000 | 4.73 | 0.00 ± 0.00 | ||||||||
3937217 | 30.06 ± 1.94 | 3.76 ± 0.11 | 4887 ± 185 | 1.24 ± 0.17 | 2.40 ± 0.03 | 54.08 ± 4.43 | 1.000 | 7.90 | 9.08 ± 1.42 | ||||||||
3956210 | 29.67 ± 3.21 | 3.85 ± 0.50 | 5015 ± 214 | 1.13 ± 0.37 | 2.40 ± 0.05 | 54.83 ± 4.94 | 0.990 | 7.71 | 0.00 ± 0.00 | ||||||||
4041075 | 32.20 ± 2.00 | 3.78 ± 0.13 | 4290 ± 156 | 1.23 ± 0.17 | 2.40 ± 0.03 | 111.25 ± 5.14 | 1.000 | 7.86 | 0.00 ± 0.00 | ||||||||
... | ... | ... | ... | ... | ... | ... | ... | ... |
Notes. The crowding value represents the amount of the integrated flux belonging to the targeted star. Hence, it is equal to 1 when only the targeted star is in the aperture. The full table is available at the CDS.
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