Table 3
Stars for which we derived a reliable rotation period Prot.
KID | Prot [days] | error Prot [days] | ⟨ Sph,k = 5 ⟩ | error ⟨ Sph,k = 5 ⟩ | Type of detection | Source of Prot |
|
||||||
1430163 | 4.16 | 0.92 | 223.79 | 8.18 | A | KADACS |
1435467 | 6.68 | 0.89 | 208.99 | 5.81 | A | KADACS |
2450729 | 53.00 | 5.32 | 164.74 | 1.78 | A | KADACS⋆ |
2837475 | 3.68 | 0.36 | 85.68 | 3.46 | A | KADACS |
2852862 | 10.13 | 0.63 | 123.90 | 3.33 | A | KADACS |
2865774 | 6.22 | 0.56 | 141.49 | 5.49 | V | PDC |
2998253 | 6.79 | 0.53 | 180.04 | 5.90 | A | KADACS |
3112152 | 15.48 | 1.19 | 180.25 | 4.11 | V | KADACS |
3123191 | 20.33 | 1.38 | 332.06 | 5.29 | A | KADACS |
3223000 | 4.85 | 0.39 | 1096.52 | 34.88 | A | KADACS |
3236382 | 3.66 | 0.42 | 99.56 | 4.40 | V | PDC |
3241581 | 26.26 | 2.01 | 177.18 | 2.65 | V | KADACS |
3344897 | 5.66 | 0.94 | 268.28 | 8.52 | A | KADACS |
3424541 | 3.46 | 0.33 | 322.94 | 12.57 | A | KADACS |
3430893 | 8.29 | 0.69 | 123.11 | 3.65 | A | KADACS |
3632418 | 12.89 | 1.38 | 133.50 | 2.71 | A | KADACS |
3633847 | 10.96 | 1.03 | 122.10 | 3.01 | A | KADACS |
3633889 | 4.23 | 0.30 | 52.90 | 2.71 | A | KADACS |
3642422 | 48.73 | -8.19 | 259.91 | 2.92 | V | PDC |
3643774 | 14.40 | 1.56 | 223.65 | 4.36 | A | KADACS |
3656476 | 31.67 | 3.53 | 80.90 | 1.48 | A | KADACS |
3657002 | 16.02 | 1.54 | 201.59 | 4.00 | A | KADACS |
3661135 | 28.39 | 4.83 | 174.53 | 3.10 | A | KADACS |
3733735 | 2.56 | 0.19 | 251.21 | 11.65 | A | KADACS |
... |
Notes. KOIs are identified by a (†) in the KID (Kepler IDentification number). The column “Type of detection” explains whether Prot has been determined automatically (A) or after a visual check (V). The column “Source of Prot” gives the set of data – KADACS or PDC – from which the final Prot has been obtained. The (⋆) indicates when the KADACS datasets were filtered at 100 days instead of the standard 30 days. This table is available in its entirety in a machine-readable form at the CDS. A portion is shown here for guidance regarding its form and content.
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