Rotation periods, (B−V)0 colors, and gyrochronology ages using different calibrations.
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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