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Table 4

Rotation periods, (BV)0 colors, and gyrochronology ages using different calibrations.

KIC Rvar Teff (BV)0 Δ(BV)0 P ΔP tB07 ΔtB07 tMH08 ΔtMH08 tM09 ΔtM09 Flag
(%) (K) (mag) (mag) (d) (d) (Myr) (Myr) (Myr) (Myr) (Myr) (Myr)

7799260 2.14 5437 0.671 0.010 23.837 0.000 ev
11135449 1.20 4731 1.032 0.010 31.783 0.775 2197 162 3154 364 2370 313
3751292 4.21 6089 0.556 0.010 3.656 0.000 172 16 241 35 279 48
8481446 0.39 5699 0.628 0.010 15.115 0.000 1710 134 1892 222 2213 259
3757951 6.17 5345 0.677 0.010 1.918 0.006 vs

Notes. If no ages are provided, either the period or the color lies outside the valid calibration range (see Table 3). Super-stable and very stable stars (flagged as “ss” and “vs”, respectively) were discarded from the stellar ages sample. Furthermore, stars with log g< 4.2 may have evolved off the main sequence (flagged as “ev”). For these stars we provide a rotation period but no ages since gyrochronology relations are not calibrated for evolved stars. Further table entries are the KIC number, the variability range Rvar, and the effective temperature Teff. The full table is available at the CDS.

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