Table 4
Rotation periods, (B−V)0 colors, and gyrochronology ages using different calibrations.
| KIC | Rvar | Teff | (B−V)0 | Δ(B−V)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.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.