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Table 2

GPS outcome values.

(1) (2) (3) (4)
KIC PHFIP σ PHFIP α σ α Prot GPS Prot GLS Prot ACF log g [Fe/H] Var Teff
(d) (d) (d) (d) (d) (ppm) (K)
10070928 3.78 0.108 0.173 0.0050 19.894 22.132 21.747 4.594 −0.46 4688 5706
10080186 3.67 0.131 0.207 0.0074 19.315 18.239 17.747 4.547 −0.10 7472 5749
10080239 2.96 0.084 0.184 0.0052 15.578 16.577 16.131 4.547 −0.14 7174 5792
10083970 3.08 0.097 0.188 0.0059 16.210 16.308 16.374 4.559 −0.20 11 418 5745
10089777 3.65 0.066 0.188 0.0034 19.210 19.437 19.381 4.541 0.07 3752 5713
10091612 2.90 0.078 0.130 0.0035 15.263 22.214 4.550 −0.18 1760 5804
10125510 3.78 0.180 0.161 0.0076 19.894 23.427 4.372 −0.64 0608 5838
10129857 4.69 0.235 0.162 0.0081 24.684 28.859 4.536 −0.06 1488 5757
10136417 4.46 0.276 0.169 0.0105 23.473 27.541 26.288 4.303 0.16 2690 5849
10140949 4.12 0.127 0.182 0.0056 21.684 22.636 4.501 0.02 1999 5874
10146308 3.69 0.191 0.174 0.0090 19.421 21.193 4.591 −0.52 3340 5804
10064358 3.82 0.078 0.231 0.0047 20.105 16.526 16.533 4.486 −0.22 2526 5772

Notes. This table contains an example of the GPS outputs, the compared rotation period values from GLS & ACF, and stellar parameters for 12 randomly selected objects from samples A and B. (1) GPS outcome: in Col. 2, the PHFIP is given, in Col. 3, its 2-sigma uncertainty, σ PHFIP, defined from individual inflection points for each Kepler observing quarter. In Cols. 4 and 5, values of α-factor and its 2-sigma uncertainty are reported, respectively. Prot GPS values in Col. 6, as result of applying Eq. (1) using the factor α = 0.19. (2) Col. 7 shows the Prot reported by Reinhold & Gizon (2015). (3) Prot and variability values reported by McQuillan et al. (2014) in Col. 8. (4) Cols. 10, 11 and 12 show the log g, [Fe/H] and Teff, respectively,taken from Huber et al. (2014). A complete table for the 1047 objects is available at the CDS.

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