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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