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Table A.1

Targets selected for further analysis from Kepler K2 campaigns 1, 2 and 3.

EPIC C Kp P [d] D1 W1 ϕ2 D2 W2 Type Notes
201160323 1 18.23 22.18 0.34 0.008 0.385 0.21 0.010 P Rapid apsidal motion
201161715 1 14.65 59.89 0.10 0.014 0.701 0.09 0.016 P
201246763 1 11.93 43.68 0.35 0.008 0.258 0.31 0.014 P
201253025 1 12.86 6.79 0.26 0.042 0.494 0.24 0.046 P Prot = 6.5, 7.2 d
201379113 1 14.76 21.21 0.34 0.009 0.369 0.02 0.011 P
201382417 1 11.66 5.20 0.07 0.048 0.500 0.01 0.048 T Prot = 5.2 d
201408204 1 11.85 8.48 0.42 0.031 0.611 0.39 0.036 T Prot = 7.4, 8.4 d
201488365 1 8.81 6.73 0.36 0.048 0.500 0.36 0.048 P FM Leo
201576812 1 10.07 5.73 0.15 0.028 0.500 0.05 0.028 P TYC 272–458–1, Prot = 6.1 d
201648133 1 10.14 35.02 0.41 0.012 0.487 0.21 0.011 T Period constraint from WASP data
201665500 1 12.14 3.05 0.07 0.060 0.500 0.003 0.060 T Prot = 3.2 d
201705526 1 9.94 18.10 0.06 0.016 0.656 0.01 0.012 P BD +04° 2479
201723461 1 14.91 22.73 0.34 0.009 0.345 0.06 0.010 P
202674012 2 9.77 23.31 0.24 0.022 0.497 0.22 0.021 P HD 149946. FEROS spectra
202843085 2 11.80 16.50 0.38 0.030 0.448 0.38 0.034 P
203361171 2 11.92 7.32 0.11 0.038 0.489 0.11 0.038 P
203371239 2 11.74 20.36 0.35 0.025 0.500 0.35 0.022 P Pulsations
203543668 2 13.68 36.76 0.20 0.005 0.198 0.05 0.012 P Prot = 9.0 d
203610780 2 12.24 29.60 0.12 0.012 0.482 0.02 0.017 T
203636784 2 12.87 6.76 0.25 0.036 0.500 0.05 0.036 T Prot = 7.0 d
203728604 2 10.56 36.11 0.15 0.018 0.321 0.12 0.024 T Prot = 2.3 d (pulsations?)
204407880 2 12.14 34.37 0.10 0.010 0.718 0.03 0.021 T Prot = 13.3 d
204576757 2 13.67 23.28 0.19 0.010 N
204748201 2 14.63 7.36 0.18 0.028 0.500 0.008 0.028 T
204760247 2 5.95 9.20 0.38 0.040 0.500 0.15 0.040 T HD 142883. Pulsations. FEROS spectra
204822807 2 11.80 67.53 0.30 0.020 0.448 0.13 0.018 T
204870619 2 13.22 34.07 0.08 0.014 0.430 0.04 0.020 T
205020466 2 13.44 8.76 0.52 0.022 0.325 0.40 0.024 P Prot = 6.7, 5.7 d, HRS spectra
205170307 2 12.28 67.50 0.14 0.008 0.304 0.03 0.009 T Prot = 17 d
205546169 2 11.66 24.44 0.24 0.009 0.265 0.01 0.014 P
205703649 2 12.49 8.12 0.08 0.040 0.500 0.07 0.040 P
205919993 3 10.14 11.00 0.06 0.012 0.552 0.06 0.013 P LP 819–72, Prot = 13.4 d
205982900 3 10.23 6.72 0.43 0.051 0.475 0.39 0.071 P BW Aqr, pulsations
206066862 3 10.28 11.09 0.13 0.015 0.384 0.03 0.016 P BD − 13° 6219. Prot = 12.2 d.
206066909 3 12.37 12.94 0.22 0.016 0.686 0.04 0.027 T
206075677 3 12.30 31.02 0.30 0.010 0.569 0.02 0.013 P Prot = 9.3, 4.3, 7.7 d. Triple?
206084435 3 14.65 48.22 0.19 0.008 0.443 0.04 0.009 P
206109641 3 12.38 62.59 0.46 0.008 0.123 0.40 0.008 T Period from K2+WASP data
206212261 3 12.70 30.99 0.10 0.016 0.525 0.02 0.014 T
206241558 3 13.38 56.59 0.28 0.005 0.218 0.05 0.008 P Period from K2+WASP data
206253908 3 11.18 65.45 0.10 0.005 N Period from K2+WASP data
206288770 3 12.45 24.76 0.19 0.011 0.679 0.01 0.015 T
206433263 3 12.01 21.19 0.26 0.020 0.482 0.16 0.017 T

Notes. The campaign number is given in the column headed “C”. The characteristics of the light curve are noted as follows: P – orbital period; D1, D2 – eclipse depths as a fraction of the mean flux between eclipses; W1, W2 – eclipse widths (from first to last contact) in phase units; ϕ2 phase of secondary eclipse in phase units. “Type” is used to note light curves with partial eclipses (P), total eclipses (T), or with no visible secondary eclipse (N). The estimated apparent magnitudes in the Kepler band, Kp, are taken from the K2 Ecliptic Plane Input Catalog (EPIC; Huber et al. 2016).

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