This is a List of exoplanets discovered in 2014.
For exoplanets detected only by radial velocity, the mass value is actually a lower limit. (See Minimum mass for more information)
Name | Mass (MJ) | Radius (RJ) | Period (days) | Semi-major axis (AU) | Temp. (K)[1] | Discovery method | Distance (ly) | Host star mass (M☉) | Host star temp. (K) | Remarks |
---|---|---|---|---|---|---|---|---|---|---|
BD-11 4672 b | 0.53 | 1667 | 2.28 | radial vel. | 89 | 0.57 | 4475 | [2] | ||
Beta Cancri b | 7.8 | 605.2 | 1.7 | radial vel. | 290.4 | 1.7 | 4092.1 | [3] | ||
Beta Ursae Minoris b | 6.1 | 522.3 | 1.4 | radial vel. | 126.5 | 1.4 | 4126 | [3] | ||
COROT-22b | 0.038 | 0.435 | 9.75598 | 0.092 | 885 | transit | 1930 | 1.1 | 5939 | [4] |
COROT-24b | 0.018 | 0.33 | 5.1134 | 0.056 | 1070 | transit | 2000 | 0.91 | 4950 | [5] |
COROT-24c | 0.088 | 0.44 | 11.759 | 0.098 | 850 | transit | 2000 | 0.91 | 4950 | [5] |
COROT-27b | 10.39 | 1.007 | 3.57532 | 0.0476 | 1500 | transit | 3400±200 | 1.05 | 5900 | [6] Planet lost[7] |
Gliese 15 Ab | 0.017 | 11.4433 | 0.0717 | radial vel. | 11.6 | 0.38 | 3567 | [8] | ||
Gliese 27.1 b | 0.0409 | 15.819 | 0.101 | radial vel. | 77.05 | 0.53 | 3542 | Alternately known as Gliese 9018,[9] not related to Gliese 27. | ||
Gliese 160.2 b | 0.0321 | 5.2354 | 0.053 | radial vel. | 84.39 | 0.69 | 4347 | Alternately known as Gliese 9144, not related to Gliese 160. Disproven exoplanet[9][10] | ||
Gliese 180 b | 0.0261 | 17.380 | 0.103 | radial vel. | 38.95 | 0.43 | 3371 | [9] | ||
Gliese 180 c | 0.0201 | 24.329 | 0.129 | radial vel. | 38.95 | 0.43 | 3371 | Unconfirmed as of 2020[11][9] | ||
Gliese 229 Ab | 0.10 | 471 | 0.970 | radial vel. | 18.77 | 0.58 | 3564 | [9] | ||
Gliese 433 c | 0.14 | 4900+1800 −1000 |
4.7+1.2 −0.8 |
radial vel. | 29.57 | 0.48 | 3472 | [9] | ||
Gliese 422 b | 0.0311 | 26.161 | 0.119 | radial vel. | 41.32 | 0.35 | 3323 | [9] | ||
Gliese 682 b | 0.014 | 17.478 | 0.080 | radial vel. | 16.33 | 0.27 | 3028 | Disproven exoplanet[9][10] | ||
Gliese 682 c | 0.0274 | 57.32 | 0.176 | radial vel. | 16.33 | 0.27 | 3028 | Disproven exoplanet[9][10] | ||
Gliese 687 b | 0.058 | 38.14 | 0.16353 | radial vel. | 14.8 | 0.41 | 3413 | [12] | ||
Gliese 832 c | 0.017 | 35.68 | 0.163 | radial vel. | 16.1 | 0.45 | 3472 | Habitable zone planet,[13] likely do not exist.[14] | ||
Gliese 3293 b | 0.07406 | 30.5987 | 0.14339 | radial vel. | 51.4 | 0.42 | 3466 | [15] | ||
Gliese 3293 c | 0.06636 | 122.6196 | 0.36175 | radial vel. | 51.4 | 0.42 | 3466 | [15] | ||
Gliese 3341 b | 0.0208 | 14.207 | 0.089 | radial vel. | 77.1 | 0.47 | 3526 | [15] | ||
GU Piscium b | 11.3 | 1.265 | 2000 | imaging | 160 | 0.33 | 3250±32 | [16] | ||
HAT-P-49b | 1.73 | 1.413 | 2.691548 | 0.0438 | 2131 | transit | 1050 | 1.54 | 6820 | [17] |
HAT-P-54b | 0.76 | 0.944 | 3.799847 | 0.04117 | transit | 443 | 0.65 | 4390 | [18] Disputed in 2016,[19] reconfirmed in 2021.[20] | |
HATS-4b | 1.323 | 1.02 | 2.516729 | 0.0362 | 1315 | transit | 1400 | 1 | 5403 | [21] |
HATS-5b | 0.237 | 0.912 | 4.763387 | 0.0542 | 1025 | transit | 840 | 0.94 | 5304 | [22] |
HATS-6b | 0.319 | 0.998 | 3.3252725 | 0.03623 | transit | 484 | 0.57 | 3724 | [23] | |
HD 564 b | 0.33 | 492.3 | 1.2 | radial vel. | 175 | 0.96 | 5902 | [2] | ||
HD 4203 c | 2.17 | 6700 | 6.95 | radial vel. | 253.8 | 1.13 | 5702 | [24] | ||
HD 5319 c | 1.15 | 886 | 2.071 | radial vel. | 370 | 1.51 | 4958 | [25] | ||
HD 10442 b | 2.1 | 1043 | 2.335 | radial vel. | 443±4 | 1.56 | 5034 | [25] | ||
HD 11506 c | 0.408±0.057 | 223.41±0.32 | 0.774±0.038 | radial vel. | 167.4±0.4 | 1.12±0.02 | 5833±28 | [25] | ||
HD 14067 b | 7.8 | 1455 | 3.4 | radial vel. | 533 | 2.4 | 4815 | [26] | ||
HD 30669 b | 0.47 | 1684 | 2.69 | radial vel. | 186 | 0.92 | 5400 | [2] | ||
HD 75784 b | 1.15 | 341.7 | 1.073 | radial vel. | 224 | 1.41 | 4917 | [25] | ||
HD 100546 b | 6.9 | 53 | imaging | 320 | 2.4 | 10500 | Largest exoplanet discovered[27] | |||
HD 103720 b | 0.62 | 4.5557 | 0.0498 | radial vel. | 136 | 0.79 | 5017 | [2] | ||
HD 108341 b | 3.5 | 1129 | 2 | radial vel. | 161 | 0.84 | 5122 | [2] | ||
HD 114613 b | 0.48 | 3827 | 5.16 | radial vel. | 66.8 | 1.36 | 5729 | [28] | ||
HD 141399 b | 0.451 | 94.44 | 0.415 | radial vel. | 118 | 1.07 | 5600 | [29] | ||
HD 141399 c | 1.33 | 201.99 | 0.689 | radial vel. | 118 | 1.07 | 5600 | [29] | ||
HD 141399 d | 1.18 | 1069.8 | 2.09 | radial vel. | 118 | 1.07 | 5600 | [29] | ||
HD 141399 e | 0.66 | 5000 | 5 | radial vel. | 118 | 1.07 | 5600 | [29] | ||
HD 154857 c | 2.58 | 3452 | 5.36 | radial vel. | 223.5 | 1.72 | 5605 | [28] | ||
HIP 67851 b | 1.38 | 88.9 | 0.46 | radial vel. | 208.3±0.6 | 1.63 | 4890 | [30] | ||
HIP 67851 c | 4.34±0.59 | 1741±39 | 3.09±0.18 | radial vel. | 208.3±0.6 | 1.63 | 4890 | [31] | ||
HIP 97233 b | 20 | 1058.8 | 2.55 | radial vel. | 347 | 1.93 | 5020 | [30] | ||
HIP 105854 b | 8.2 | 184.2 | 0.81 | radial vel. | 276 | 2.1 | 4780 | [32] | ||
HIP 116454 b | 0.037 | 0.226 | 9.1205 | 0.0906 | radial vel. | 180 | 0.78 | 5089 | [33] | |
Kapteyn b | 0.015 | 48.616+0.036 −0.032 |
0.168 | radial vel. | 12.8 | 0.28 | 3550 | Existence of planet been disputed.[34][35] | ||
Kapteyn c | 0.022 | 121.54 | 0.311 | radial vel. | 12.8 | 0.28 | 3550 | Existence of planet been disputed.[34][35] | ||
KIC 10001893 b | 0.2197 | orbital brightness modulation | 5700±500 | 27500 | Disproven exoplanet[36][37] | |||||
KIC 10001893 c | 0.32528 | orbital brightness modulation | 5700±500 | 27500 | Disproven exoplanet[36][37] | |||||
KIC 10001893 d | 0.81161 | orbital brightness modulation | 5700±500 | 27500 | Disproven exoplanet[36][37] | |||||
Kepler-23d | 0.196 | 15.274299 | 0.124 | transit | 2600 | 1.11 | 5828 | [38] | ||
Kepler-24d | 0.149 | 4.244384 | 0.051 | transit | 3900 | 1.03 | 5897 | [38] | ||
Kepler-24e | 0.248 | 18.998355 | 0.138 | transit | 3900 | 1.03 | 5897 | [38] | ||
Kepler-25d | 0.283 | 123 | radial vel. | 798±4 | 1.19 | 6270 | [39][38] | |||
Kepler-26d | 0.095 | 3.543919 | 0.039 | transit | 1104±10 | 0.54 | 3914 | [38] | ||
Kepler-26e | 0.215 | 46.827915 | 0.22 | transit | 1104±10 | 0.54 | 3914 | [38] | ||
Kepler-31d | 6.8 | 0.348 | 87.6451 | 0.4 | transit | 6800 | 1.21 | 6340 | [38] | |
Kepler-37e | 51.196 | timing | 220 | 0.8 | 5417 | [38] | ||||
Kepler-48d | 0.025 | 0.182 | 42.8961 | transit | 1009±5 | 0.88 | 5194 | [39][38] | ||
Kepler-48e | 2.067 | 982 | radial vel. | 1009±5 | 0.88 | 5194 | [39] | |||
Kepler-49d | 0.143 | 2.576549 | 0.031 | transit | 1024±8 | 0.55 | 4252 | [38] | ||
Kepler-49e | 0.139 | 18.596108 | 0.116 | transit | 1024±8 | 0.55 | 4252 | [38] | ||
Kepler-51d | 0.024 | 0.865 | 130.194 | 0.509 | transit | 2610±50 | 1.04 | 6018 | [38] | |
Kepler-52d | 0.174 | 36.445171 | 0.182 | transit | 1058±7 | 0.54 | 4263 | [38] | ||
Kepler-53d | 0.189 | 9.751962 | 0.091 | transit | 4600±200 | 0.98 | 5858 | [38] | ||
Kepler-54d | 0.136 | 20.995694 | 0.126 | transit | 893±9 | 0.51 | 4252 | [38] | ||
Kepler-55d | 0.142 | 2.211099 | 0.029 | transit | 1920±30 | 0.62 | 4503 | [38] | ||
Kepler-55e | 0.138 | 4.617534 | 0.048 | transit | 1920±30 | 0.62 | 4503 | [38] | ||
Kepler-55f | 0.142 | 10.198545 | 0.081 | transit | 1920±30 | 0.62 | 4503 | [38] | ||
Kepler-58d | 0.262 | 40.101371 | 0.236 | transit | 3250±80 | 0.95 | 6099 | [38] | ||
Kepler-79d | 0.019 | 0.639 | 52.0902 | 0.287 | 553 | transit | 3230±60 | 1.17 | 6174 | [38] |
Kepler-79e | 0.013 | 0.311 | 81.0659 | 0.386 | 477 | transit | 3230±60 | 1.17 | 6174 | [38] |
Kepler-80d | 0.02124 | 0.136 | 3.07222 | 0.0372 | transit | 1160 | 0.73 | 4540 | [38] | |
Kepler-80e | 0.01299 | 0.143 | 4.64489 | 0.0491 | transit | 1160 | 0.73 | 4540 | [38] | |
Kepler-81d | 0.108 | 20.837846 | 0.128 | transit | 1147±10 | 0.64 | 4500 | [38] | ||
Kepler-82d | 0.158 | 2.382961 | 0.034 | transit | 3030±80 | 0.85 | 5428 | [38] | ||
Kepler-82e | 0.22 | 5.902206 | 0.063 | transit | 3030±80 | 0.85 | 5428 | [38] | ||
Kepler-83d | 0.173 | 5.169796 | 0.051 | transit | 1320±17 | 0.66 | 4648 | [38] | ||
Kepler-84d | 0.123 | 4.224537 | 0.052 | transit | 4700±500 | 1 | 6031 | [38] | ||
Kepler-84e | 0.232 | 27.434389 | 0.181 | transit | 4700±500 | 1 | 6031 | [38] | ||
Kepler-84f | 0.196 | 44.552169 | 0.25 | transit | 4700±500 | 1 | 6031 | [38] | ||
Kepler-85d | 0.107 | 17.91323 | 0.13 | transit | 2550±50 | 0.92 | 5436 | [38] | ||
Kepler-85e | 0.113 | 25.216751 | 0.163 | transit | 2550±50 | 0.92 | 5436 | [38] | ||
Kepler-93b | 0.01265 | 0.132 | 4.72673978 | 0.053 | 1037 | transit | 313.7±0.7 | 0.91 | 5669 | [39] |
Kepler-93c | 3 | 1460 | radial vel. | 313.7±0.7 | 0.91 | 5669 | [39] | |||
Kepler-94b | 0.034 | 0.313 | 2.50806 | transit | 629±2 | 0.81 | 4781 | [39] | ||
Kepler-94c | 9.836 | 820.3 | radial vel. | 629±2 | 0.81 | 4781 | [39] | |||
Kepler-95b | 0.041 | 0.305 | 11.5231 | transit | 1472±18 | 1.08 | 5699 | [39] | ||
Kepler-96b | 0.027 | 0.238 | 16.2385 | transit | 402.2±1.3 | 1 | 5690 | [39] | ||
Kepler-97b | 0.011 | 0.132 | 2.58664 | transit | 1322±11 | 0.94 | 5779 | [39] | ||
Kepler-97c | 1.08 | 789 | radial vel. | 1322±11 | 0.94 | 5779 | [39] | |||
Kepler-98b | 0.011 | 0.178 | 1.54168 | transit | 1154±9 | 0.99 | 5539 | [39] | ||
Kepler-99b | 0.019 | 0.132 | 4.60358 | transit | 683±3 | 0.79 | 4782 | [39] | ||
Kepler-100b | 0.023 | 0.118 | 6.88705 | transit | 1002±5 | 1.08 | 5825 | [39][38] | ||
Kepler-100c | 0.196 | 12.8159 | transit | 1002±5 | 1.08 | 5825 | [39][38] | |||
Kepler-100d | 0.144 | 35.3331 | transit | 1002±5 | 1.08 | 5825 | [39][38] | |||
Kepler-101b | 0.16 | 0.51 | 3.4876812 | 0.0474 | transit | 3110±50 | 1.17 | 5667 | [38] | |
Kepler-101c | 0.01 | 0.112 | 6.02976 | 0.0684 | transit | 3110±50 | 1.17 | 5667 | [38] | |
Kepler-102b | 0.042 | 5.28696 | 792 | transit | 352.7±0.7 | 0.81 | 4909 | [39][38] | ||
Kepler-102c | 0.052 | 7.07142 | 718 | transit | 352.7±0.7 | 0.81 | 4909 | [39][38] | ||
Kepler-102d | 0.012 | 0.105 | 10.3117 | transit | 352.7±0.7 | 0.81 | 4909 | [39][38] | ||
Kepler-102f | 0.079 | 27.4536 | 457 | transit | 352.7±0.7 | 0.81 | 4909 | [39][38] | ||
Kepler-103b | 0.031 | 0.301 | 15.9654 | transit | 1637±19 | 1.09 | 5845 | [39][38] | ||
Kepler-103c | 0.114 | 0.459 | 179.612 | transit | 1637±19 | 1.09 | 5845 | [39][38] | ||
Kepler-104b | 0.277 | 11.427548 | 0.094 | transit | 1322±14 | 0.81 | 5711 | [38] | ||
Kepler-104c | 0.279 | 23.668205 | 0.153 | transit | 1322±14 | 0.81 | 5711 | [38] | ||
Kepler-104d | 0.319 | 51.755394 | 0.257 | transit | 1322±14 | 0.81 | 5711 | [38] | ||
Kepler-105c | 0.01447 | 0.117 | 7.1262 | transit | 1517±18 | 0.96 | 5827 | [38] | ||
Kepler-106b | 0.073 | 6.16486 | transit | 1470±20 | 1 | 5858 | [39] | |||
Kepler-106c | 0.033 | 0.223 | 13.5708 | transit | 1470±20 | 1 | 5858 | [39][38] | ||
Kepler-106d | 0.085 | 23.9802 | transit | 1470±20 | 1 | 5858 | [39][38] | |||
Kepler-106e | 0.035 | 0.228 | 43.8445 | transit | 1470±20 | 1 | 5858 | [39][38] | ||
Kepler-107b | 0.139 | 3.179997 | 0.044 | transit | 1741±18 | 5851 | [38] | |||
Kepler-107c | 0.161 | 4.901425 | 0.059 | transit | 1741±18 | 5851 | [38] | |||
Kepler-107d | 0.095 | 7.958203 | 0.082 | transit | 1741±18 | 5851 | [38] | |||
Kepler-107e | 0.308 | 14.749049 | 0.123 | transit | 1741±18 | 5851 | [38] | |||
Kepler-108b | 0.772 | 49.183921 | 0.292 | transit | 4200±500 | 0.87 | 5854 | [38] | ||
Kepler-108c | 0.73 | 190.323494 | 0.721 | transit | 4200±500 | 0.87 | 5854 | [38] | ||
Kepler-109b | 0.211 | 6.48163 | transit | 1570±17 | 1.04 | 5952 | [39][38] | |||
Kepler-109c | 0.225 | 21.2227 | transit | 1570±17 | 1.04 | 5952 | [39][38] | |||
Kepler-110b | 0.163 | 12.691112 | 0.107 | transit | 1950±30 | 5960 | [38] | |||
Kepler-110c | 0.197 | 31.719775 | 0.198 | transit | 1950±30 | 5960 | [38] | |||
Kepler-111b | 0.141 | 3.341815 | 0.046 | transit | 2190±20 | 5952 | [38] | |||
Kepler-111c | 0.651 | 224.784608 | 0.761 | transit | 2190±20 | 5952 | [38] | |||
Kepler-112b | 0.211 | 8.408878 | 0.076 | transit | 1698±14 | 5544 | [38] | |||
Kepler-112c | 0.214 | 28.574263 | 0.172 | transit | 1698±14 | 5544 | [38] | |||
Kepler-113b | 0.037 | 0.162 | 4.754 | transit | 862±3 | 0.75 | 4725 | [39][38] | ||
Kepler-113c | 0.194 | 8.92507 | transit | 862±3 | 0.75 | 4725 | [39][38] | |||
Kepler-114b | 0.112 | 5.188549 | 0.053 | 722 | transit | 852±4 | 0.56 | 4605 | [38] | |
Kepler-115b | 0.097 | 2.403679 | 0.036 | transit | 2070±20 | 1 | 5979 | [38] | ||
Kepler-115c | 0.232 | 8.990889 | 0.087 | transit | 2070±20 | 1 | 5979 | [38] | ||
Kepler-116b | 0.305 | 5.968734 | 0.069 | transit | 3200±50 | 1.16 | 6142 | [38] | ||
Kepler-116c | 0.205 | 13.07163 | 0.116 | transit | 3200±50 | 1.16 | 6142 | [38] | ||
Kepler-117b | 0.094 | 0.719 | 18.7959228 | 0.1445 | transit | 4700 | 1.13 | 6150 | [38] | |
Kepler-117c | 1.84 | 1.101 | 50.790391 | 0.2804 | transit | 4700 | 1.13 | 6150 | [38] | |
Kepler-118b | 0.175 | 7.518496 | 0.073 | transit | 1900±20 | 0.86 | 5274 | [38] | ||
Kepler-118c | 0.685 | 20.17202 | 0.141 | transit | 1900±20 | 0.86 | 5274 | [38] | ||
Kepler-119b | 0.321 | 2.422082 | 0.035 | transit | 2340±40 | 5595 | [38] | |||
Kepler-119c | 0.082 | 4.125103 | 0.049 | transit | 2340±40 | 5595 | [38] | |||
Kepler-120b | 0.192 | 6.312501 | 0.055 | transit | 1281±10 | 4096 | [38] | |||
Kepler-120c | 0.136 | 12.794585 | 0.088 | transit | 1281±10 | 4096 | [38] | |||
Kepler-121b | 0.209 | 3.177422 | 0.039 | transit | 1690±20 | 5311 | [38] | |||
Kepler-121c | 0.203 | 41.008011 | 0.216 | transit | 1690±20 | 5311 | [38] | |||
Kepler-122b | 0.209 | 5.766193 | 0.064 | transit | 3450±70 | 0.99 | 6050 | [38] | ||
Kepler-122c | 0.524 | 12.465988 | 0.108 | transit | 3450±70 | 0.99 | 6050 | [38] | ||
Kepler-122d | 0.196 | 21.587475 | 0.155 | transit | 3450±70 | 0.99 | 6050 | [38] | ||
Kepler-122e | 0.232 | 37.993273 | 0.227 | transit | 3450±70 | 0.99 | 6050 | [38] | ||
Kepler-122f | 0.113 | 0.156 | 56.268 | timing | 3450±70 | 0.99 | 6050 | ? | ||
Kepler-123b | 0.262 | 17.232366 | 0.135 | transit | 3430±80 | 1.03 | 6089 | [38] | ||
Kepler-123c | 0.132 | 26.695074 | 0.181 | transit | 3430±80 | 1.03 | 6089 | [38] | ||
Kepler-124b | 0.065 | 3.410493 | 0.039 | transit | 1386±10 | 4984 | [38] | |||
Kepler-124c | 0.156 | 13.821375 | 0.1 | transit | 1386±10 | 4984 | [38] | |||
Kepler-124d | 0.099 | 30.950851 | 0.17 | transit | 1386±10 | 4984 | [38] | |||
Kepler-125b | 0.211 | 4.164389 | 0.041 | transit | 601±3 | 0.55 | 3810 | [38] | ||
Kepler-125c | 0.066 | 5.774464 | 0.051 | transit | 601±3 | 0.55 | 3810 | [38] | ||
Kepler-126b | 0.136 | 10.495711 | 0.099 | transit | 779±5 | 6239 | [38] | |||
Kepler-126c | 0.141 | 21.869741 | 0.162 | transit | 779±5 | 6239 | [38] | |||
Kepler-126d | 0.223 | 100.283134 | 0.448 | transit | 779±5 | 6239 | [38] | |||
Kepler-127b | 0.125 | 14.435889 | 0.125 | transit | 1162±8 | 6106 | [38] | |||
Kepler-127c | 0.237 | 29.393195 | 0.2 | transit | 1162±8 | 6106 | [38] | |||
Kepler-127d | 0.236 | 48.630408 | 0.28 | transit | 1162±8 | 6106 | [38] | |||
Kepler-129b | 0.211 | 15.79186 | 0.131 | transit | 1349±14 | 1.18 | 5770 | [38] | ||
Kepler-129c | 0.227 | 82.20017 | 0.393 | transit | 1349±14 | 1.18 | 5770 | [38] | ||
Kepler-130c | 0.259 | 27.50868 | 0.178 | transit | 1042±7 | 1 | 5884 | [38] | ||
Kepler-130d | 0.146 | 87.517905 | 0.377 | transit | 1042±7 | 1 | 5884 | [38] | ||
Kepler-131b | 0.051 | 0.215 | 16.092 | transit | 750±4 | 1.02 | 5685 | [39][38] | ||
Kepler-131c | 0.026 | 0.075 | 25.5169 | transit | 750±4 | 1.02 | 5685 | [39][38] | ||
Kepler-132b | 0.108 | 6.178196 | 0.067 | transit | 900±70 | 6003 | [38] | |||
Kepler-132c | 0.114 | 6.414914 | 0.068 | transit | 900±70 | 6003 | [38] | |||
Kepler-132d | 0.138 | 18.010199 | 0.136 | transit | 900±70 | 6003 | [38] | |||
Kepler-133b | 0.157 | 8.129976 | 0.083 | transit | 2170±60 | 5736 | [38] | |||
Kepler-133c | 0.253 | 31.517586 | 0.204 | transit | 2170±60 | 5736 | [38] | |||
Kepler-134b | 0.178 | 5.317429 | 0.06 | transit | 1102±7 | 5983 | [38] | |||
Kepler-134c | 0.112 | 10.105785 | 0.092 | transit | 1102±7 | 5983 | [38] | |||
Kepler-135b | 0.161 | 6.00253 | 0.067 | transit | 2060±40 | 6090 | [38] | |||
Kepler-135c | 0.103 | 11.448708 | 0.103 | transit | 2060±40 | 6090 | [38] | |||
Kepler-136b | 0.183 | 11.5789 | 0.106 | transit | 1389±14 | 1.2 | 6165 | [38] | ||
Kepler-136c | 0.178 | 16.399235 | 0.133 | transit | 1389±14 | 1.2 | 6165 | [38] | ||
Kepler-137b | 0.131 | 8.436387 | 0.077 | transit | 996±6 | 5187 | [38] | |||
Kepler-137c | 0.168 | 18.735753 | 0.13 | transit | 996±6 | 5187 | [38] | |||
Kepler-138b | 0.00021 | 0.047 | 10.3126 | transit | 218.5±0.3 | 0.52 | 3841 | [38] | ||
Kepler-138c | 0.0062 | 0.107 | 13.7813 | transit | 218.5±0.3 | 0.52 | 3841 | [38] | ||
Kepler-138d | 0.00201 | 0.108 | 23.0881 | 431 | transit | 218.5±0.3 | 0.52 | 3841 | [38] | |
Kepler-139b | 0.262 | 15.771044 | 0.127 | transit | 1289±13 | 1.08 | 5594 | [38] | ||
Kepler-139c | 0.302 | 157.072878 | 0.586 | transit | 1289±13 | 1.08 | 5594 | [38] | ||
Kepler-140b | 0.144 | 3.25427 | 0.045 | transit | 1940±20 | 6077 | [38] | |||
Kepler-140c | 0.161 | 91.353282 | 0.414 | transit | 1940±20 | 6077 | [38] | |||
Kepler-141b | 0.062 | 3.107675 | 0.039 | transit | 990±4 | 1 | 4910 | [38] | ||
Kepler-141c | 0.126 | 7.010606 | 0.067 | transit | 990±4 | 1 | 4910 | ? | ||
Kepler-142b | 0.178 | 2.024152 | 0.032 | transit | 1818±13 | 0.99 | 5790 | [38] | ||
Kepler-142c | 0.255 | 4.761702 | 0.057 | transit | 1818±13 | 0.99 | 5790 | [38] | ||
Kepler-142d | 0.193 | 41.809118 | 0.242 | transit | 1818±13 | 0.99 | 5790 | [38] | ||
Kepler-143b | 0.215 | 16.007583 | 0.127 | transit | 2700±40 | 5848 | [38] | |||
Kepler-143c | 0.301 | 27.082511 | 0.181 | transit | 2700±40 | 5848 | [38] | |||
Kepler-144b | 0.119 | 5.885273 | 0.066 | transit | 1269±10 | 1.03 | 6075 | [38] | ||
Kepler-144c | 0.12 | 10.104665 | 0.094 | transit | 1269±10 | 1.03 | 6075 | [38] | ||
Kepler-146b | 0.331 | 31.158799 | 0.2 | transit | 2390±30 | 5948 | [38] | |||
Kepler-146c | 0.279 | 76.732171 | 0.364 | transit | 2390±30 | 5948 | [38] | |||
Kepler-147b | 0.136 | 12.610584 | 0.113 | transit | 3500±90 | 1.01 | 6012 | [38] | ||
Kepler-147c | 0.217 | 33.416423 | 0.216 | transit | 3500±90 | 1.01 | 6012 | [38] | ||
Kepler-148b | 0.161 | 1.729366 | 0.028 | transit | 2640±50 | 5272 | [38] | |||
Kepler-148c | 0.321 | 4.180043 | 0.05 | transit | 2640±50 | 5272 | [38] | |||
Kepler-149b | 0.376 | 29.198943 | 0.184 | transit | 1893±19 | 5381 | [38] | |||
Kepler-149c | 0.144 | 55.328328 | 0.281 | transit | 1893±19 | 5381 | [38] | |||
Kepler-149d | 0.353 | 160.018032 | 0.571 | transit | 1893±19 | 5381 | [38] | |||
Kepler-150b | 0.112 | 3.428054 | 0.044 | transit | 2980±60 | 5560 | [38] | |||
Kepler-150c | 0.329 | 7.381998 | 0.073 | transit | 2980±60 | 5560 | [38] | |||
Kepler-150d | 0.249 | 12.56093 | 0.104 | transit | 2980±60 | 5560 | [38] | |||
Kepler-150e | 0.278 | 30.826557 | 0.189 | transit | 2980±60 | 5560 | [38] | |||
Kepler-151b | 0.273 | 15.228958 | 0.116 | transit | 2160±30 | 0.83 | 5460 | [38] | ||
Kepler-151c | 0.186 | 24.674612 | 0.16 | transit | 2160±30 | 0.83 | 5460 | [38] | ||
Kepler-152b | 0.249 | 18.207973 | 0.124 | transit | 1457±10 | 5088 | [38] | |||
Kepler-152c | 0.213 | 88.255055 | 0.356 | transit | 1457±10 | 5088 | [38] | |||
Kepler-153b | 0.261 | 18.870227 | 0.129 | transit | 1518±11 | 5404 | [38] | |||
Kepler-153c | 0.226 | 46.90232 | 0.237 | transit | 1518±11 | 5404 | [38] | |||
Kepler-154b | 0.202 | 33.040532 | 0.198 | transit | 3070±60 | 0.89 | 5690 | [38] | ||
Kepler-154c | 0.263 | 62.303276 | 0.303 | transit | 3070±60 | 0.89 | 5690 | [38] | ||
Kepler-155b | 0.186 | 5.931194 | 0.056 | transit | 965±7 | 0.58 | 4508 | [38] | ||
Kepler-155c | 0.2 | 52.661793 | 0.242 | transit | 965±7 | 0.58 | 4508 | [38] | ||
Kepler-156b | 0.205 | 4.973456 | 0.054 | transit | 1465±11 | 5094 | [38] | |||
Kepler-156c | 0.227 | 15.906801 | 0.117 | transit | 1465±11 | 5094 | [38] | |||
Kepler-157b | 0.118 | 1.732342 | 0.028 | transit | 2580±40 | 5774 | [38] | |||
Kepler-157c | 0.2 | 13.5405 | 0.11 | transit | 2580±40 | 5774 | [38] | |||
Kepler-158b | 0.189 | 16.709184 | 0.111 | transit | 1037±6 | 4623 | [38] | |||
Kepler-158c | 0.17 | 28.551383 | 0.158 | transit | 1037±6 | 4623 | [38] | |||
Kepler-159b | 0.212 | 10.139623 | 0.082 | transit | 1232±10 | 4625 | [38] | |||
Kepler-159c | 0.304 | 43.595792 | 0.218 | transit | 1232±10 | 4625 | [38] | |||
Kepler-160b | 0.137 | 4.309427 | 0.05 | transit | 3140±60 | 0.88 | 5471+115 −37 |
[38][40] | ||
Kepler-160c | 0.322 | 13.699087 | 0.109 | transit | 3140±60 | 0.88 | 5471+115 −37 |
[38][40] | ||
Kepler-161b | 0.189 | 4.921355 | 0.054 | transit | 1435±10 | 0.77 | 5078 | [38] | ||
Kepler-161c | 0.183 | 7.06424 | 0.068 | transit | 1435±10 | 0.77 | 5078 | [38] | ||
Kepler-162b | 0.112 | 6.919798 | 0.069 | transit | 2860±50 | 5816 | [38] | |||
Kepler-162c | 0.27 | 19.446355 | 0.137 | transit | 2860±50 | 5816 | [38] | |||
Kepler-163b | 0.094 | 7.810937 | 0.078 | transit | 2300±40 | 0.96 | 5776 | [38] | ||
Kepler-163c | 0.202 | 21.347262 | 0.152 | transit | 2300±40 | 0.96 | 5776 | [38] | ||
Kepler-164b | 0.126 | 5.03503 | 0.058 | transit | 2980±50 | 1.11 | 5888 | [38] | ||
Kepler-164c | 0.244 | 10.945723 | 0.097 | transit | 2980±50 | 1.11 | 5888 | [38] | ||
Kepler-164d | 0.219 | 28.986769 | 0.187 | transit | 2980±50 | 1.11 | 5888 | [38] | ||
Kepler-165b | 0.207 | 8.180848 | 0.072 | transit | 1860±20 | 5211 | [38] | |||
Kepler-165c | 0.199 | 15.31299 | 0.11 | transit | 1860±20 | 5211 | [38] | |||
Kepler-166b | 0.203 | 7.650254 | 0.072 | transit | 2000±20 | 5413 | [38] | |||
Kepler-166c | 0.212 | 34.260281 | 0.195 | transit | 2000±20 | 5413 | [38] | |||
Kepler-167b | 0.144 | 4.3931632 | 0.0483 | transit | 1100 | 0.77 | 4890 | [38] | ||
Kepler-167c | 0.138 | 7.406114 | 0.0684 | transit | 1100 | 0.77 | 4890 | [38] | ||
Kepler-168b | 0.13 | 4.425391 | 0.056 | transit | 4550±160 | 6282 | [38] | |||
Kepler-168c | 0.24 | 13.193242 | 0.116 | transit | 4550±160 | 6282 | [38] | |||
Kepler-169b | 0.101 | 3.250619 | 0.04 | transit | 1341±9 | 0.86 | 4997 | [38] | ||
Kepler-169c | 0.108 | 6.195469 | 0.062 | transit | 1341±9 | 0.86 | 4997 | [38] | ||
Kepler-169d | 0.112 | 8.348125 | 0.075 | transit | 1341±9 | 0.86 | 4997 | [38] | ||
Kepler-169e | 0.196 | 13.767102 | 0.105 | transit | 1341±9 | 0.86 | 4997 | [38] | ||
Kepler-169f | 0.23 | 87.090195 | 0.359 | transit | 1341±9 | 0.86 | 4997 | [38] | ||
Kepler-170b | 0.285 | 7.930592 | 0.08 | transit | 2460±40 | 5679 | [38] | |||
Kepler-170c | 0.255 | 16.665863 | 0.131 | transit | 2460±40 | 5679 | [38] | |||
Kepler-171b | 0.209 | 4.166972 | 0.05 | transit | 2890±60 | 5642 | [38] | |||
Kepler-171c | 0.228 | 11.463462 | 0.098 | transit | 2890±60 | 5642 | [38] | |||
Kepler-171d | 0.169 | 39.595519 | 0.223 | transit | 2890±60 | 5642 | [38] | |||
Kepler-172b | 0.21 | 2.940309 | 0.04 | transit | 2770±60 | 0.86 | 5526 | [38] | ||
Kepler-172c | 0.255 | 6.388996 | 0.068 | transit | 2770±60 | 0.86 | 5526 | [38] | ||
Kepler-172d | 0.201 | 14.627119 | 0.118 | transit | 2770±60 | 0.86 | 5526 | [38] | ||
Kepler-172e | 0.246 | 35.118736 | 0.211 | transit | 2770±60 | 0.86 | 5526 | [38] | ||
Kepler-173b | 0.115 | 4.263742 | 0.048 | transit | 2780±50 | 0.78 | 6031 | [38] | ||
Kepler-173c | 0.217 | 8.005777 | 0.074 | transit | 2780±50 | 0.78 | 6031 | [38] | ||
Kepler-174b | 0.175 | 13.98179 | 0.1 | transit | 1268±8 | 4880 | [38] | |||
Kepler-174c | 0.133 | 44.000529 | 0.214 | transit | 1268±8 | 4880 | [38] | |||
Kepler-174d | 0.195 | 247.35373 | 0.677 | transit | 1268±8 | 4880 | [38] | |||
Kepler-175b | 0.228 | 11.903515 | 0.105 | transit | 4450±150 | 1.04 | 6064 | [38] | ||
Kepler-175c | 0.277 | 34.035257 | 0.213 | transit | 4450±150 | 1.04 | 6064 | [38] | ||
Kepler-176b | 0.128 | 5.433074 | 0.058 | transit | 1750±20 | 5232 | [38] | |||
Kepler-176c | 0.232 | 12.759712 | 0.102 | transit | 1750±20 | 5232 | [38] | |||
Kepler-176d | 0.224 | 25.751974 | 0.163 | transit | 1750±20 | 5232 | [38] | |||
Kepler-178b | 0.259 | 9.576694 | 0.085 | transit | 2380±30 | 5676 | [38] | |||
Kepler-178c | 0.257 | 20.552802 | 0.142 | transit | 2380±30 | 5676 | [38] | |||
Kepler-178d | 0.352 | 96.678988 | 0.397 | transit | 2380±30 | 5676 | [38] | |||
Kepler-179b | 0.146 | 2.735926 | 0.036 | transit | 2010±20 | 5302 | [38] | |||
Kepler-179c | 0.178 | 6.40013 | 0.064 | transit | 2010±20 | 5302 | [38] | |||
Kepler-180b | 0.134 | 13.817124 | 0.109 | transit | 2320±30 | 0.84 | 5731 | [38] | ||
Kepler-180c | 0.269 | 41.885775 | 0.229 | transit | 2320±30 | 0.84 | 5731 | [38] | ||
Kepler-181b | 0.113 | 3.137873 | 0.04 | transit | 2020±30 | 5333 | [38] | |||
Kepler-181c | 0.178 | 4.302149 | 0.049 | transit | 2020±30 | 5333 | [38] | |||
Kepler-182b | 0.23 | 9.825792 | 0.096 | transit | 5290±180 | 1.14 | 6250 | [38] | ||
Kepler-182c | 0.306 | 20.684342 | 0.157 | transit | 5290±180 | 1.14 | 6250 | [38] | ||
Kepler-183b | 0.184 | 5.687945 | 0.064 | transit | 3530±100 | 5888 | [38] | |||
Kepler-183c | 0.203 | 11.637071 | 0.103 | transit | 3530±100 | 5888 | [38] | |||
Kepler-184b | 0.211 | 10.687576 | 0.092 | transit | 2030±20 | 5788 | [38] | |||
Kepler-184c | 0.176 | 20.303005 | 0.141 | transit | 2030±20 | 5788 | [38] | |||
Kepler-184d | 0.222 | 29.022358 | 0.179 | transit | 2030±20 | 5788 | [38] | |||
Kepler-185b | 0.104 | 1.6329 | 0.026 | transit | 1542±15 | 0.79 | 5208 | [38] | ||
Kepler-185c | 0.18 | 20.729042 | 0.139 | transit | 1542±15 | 0.79 | 5208 | [38] | ||
Kepler-186b | 0.095 | 3.8867907 | 0.0343 | transit | 560 | 0.54 | 3755 | [38] | ||
Kepler-186c | 0.112 | 7.267302 | 0.0451 | transit | 560 | 0.54 | 3755 | [38] | ||
Kepler-186d | 0.125 | 13.342996 | 0.0781 | transit | 560 | 0.54 | 3755 | [38] | ||
Kepler-186e | 0.113 | 22.407704 | 0.11 | transit | 560 | 0.54 | 3755 | [38] | ||
Kepler-186f | 0.104 | 129.9441 | 0.432 | transit | 560 | 0.54 | 3755 | ? Potentially habitable exoplanet | ||
Kepler-187b | 0.126 | 4.938864 | 0.059 | transit | 3850±110 | 0.85 | 6105 | [38] | ||
Kepler-187c | 0.238 | 10.640263 | 0.099 | transit | 3850±110 | 0.85 | 6105 | [38] | ||
Kepler-188b | 0.15 | 2.061897 | 0.032 | transit | 3250±80 | 6021 | [38] | |||
Kepler-188c | 0.285 | 5.996553 | 0.066 | transit | 3250±80 | 6021 | [38] | |||
Kepler-189b | 0.108 | 10.399931 | 0.088 | transit | 1960±20 | 0.79 | 5235 | [38] | ||
Kepler-189c | 0.212 | 20.134866 | 0.137 | transit | 1960±20 | 0.79 | 5235 | [38] | ||
Kepler-190b | 0.139 | 2.019999 | 0.03 | transit | 1431±9 | 0.84 | 5106 | [38] | ||
Kepler-190c | 0.13 | 3.763024 | 0.045 | transit | 1431±9 | 0.84 | 5106 | [38] | ||
Kepler-191b | 0.12 | 9.939632 | 0.087 | transit | 1970±30 | 0.85 | 5282 | [38] | ||
Kepler-191c | 0.166 | 17.738506 | 0.128 | transit | 1970±30 | 0.85 | 5282 | [38] | ||
Kepler-192b | 0.244 | 9.926746 | 0.09 | transit | 2170±20 | 5479 | [38] | |||
Kepler-192c | 0.249 | 21.2234 | 0.15 | transit | 2170±20 | 5479 | [38] | |||
Kepler-193b | 0.213 | 11.38848 | 0.106 | transit | 3390±80 | 6335 | [38] | |||
Kepler-193c | 0.245 | 50.697494 | 0.286 | transit | 3390±80 | 6335 | [38] | |||
Kepler-194b | 0.135 | 2.092281 | 0.032 | transit | 3700±100 | 6089 | [38] | |||
Kepler-194c | 0.231 | 17.308032 | 0.131 | transit | 3700±100 | 6089 | [38] | |||
Kepler-194d | 0.214 | 52.814973 | 0.275 | transit | 3700±100 | 6089 | [38] | |||
Kepler-195b | 0.181 | 8.307872 | 0.077 | transit | 2170±30 | 5329 | [38] | |||
Kepler-195c | 0.138 | 34.096863 | 0.197 | transit | 2170±30 | 5329 | [38] | |||
Kepler-196b | 0.17 | 20.739886 | 0.138 | transit | 1491±10 | 5128 | [38] | |||
Kepler-196c | 0.2 | 47.427737 | 0.24 | transit | 1491±10 | 5128 | [38] | |||
Kepler-197b | 0.091 | 5.599308 | 0.06 | transit | 1088±7 | 6004 | [38] | |||
Kepler-197c | 0.11 | 10.349695 | 0.09 | transit | 1088±7 | 6004 | [38] | |||
Kepler-197d | 0.109 | 15.677563 | 0.119 | transit | 1088±7 | 6004 | [38] | |||
Kepler-197e | 0.081 | 25.209715 | 0.164 | transit | 1088±7 | 6004 | [38] | |||
Kepler-198b | 0.252 | 17.790037 | 0.131 | transit | 1638±14 | 0.93 | 5574 | [38] | ||
Kepler-198c | 0.22 | 49.567416 | 0.259 | transit | 1638±14 | 0.93 | 5574 | [38] | ||
Kepler-199b | 0.277 | 23.637604 | 0.158 | transit | 1725±14 | 5644 | [38] | |||
Kepler-199c | 0.29 | 67.093408 | 0.316 | transit | 1725±14 | 5644 | [38] | |||
Kepler-200b | 0.19 | 8.594805 | 0.08 | transit | 2210±20 | 5678 | [38] | |||
Kepler-200c | 0.142 | 10.222157 | 0.09 | transit | 2210±20 | 5678 | [38] | |||
Kepler-201b | 0.219 | 25.672083 | 0.175 | transit | 2240±30 | 1.17 | 6065 | [38] | ||
Kepler-201c | 0.254 | 151.884058 | 0.573 | transit | 2240±30 | 1.17 | 6065 | [38] | ||
Kepler-202b | 0.145 | 4.069427 | 0.045 | transit | 937±3 | 4668 | [38] | |||
Kepler-202c | 0.165 | 16.282493 | 0.113 | transit | 937±3 | 4668 | [38] | |||
Kepler-203b | 0.229 | 3.162697 | 0.043 | transit | 2340±30 | 0.98 | 5821 | [38] | ||
Kepler-203c | 0.22 | 5.370647 | 0.061 | transit | 2340±30 | 0.98 | 5821 | [38] | ||
Kepler-203d | 0.128 | 11.32972 | 0.1 | transit | 2340±30 | 0.98 | 5821 | [38] | ||
Kepler-204b | 0.226 | 14.400974 | 0.117 | transit | 2280±20 | 0.96 | 5812 | [38] | ||
Kepler-204c | 0.16 | 25.660593 | 0.173 | transit | 2280±20 | 0.96 | 5812 | [38] | ||
Kepler-205b | 0.135 | 2.75564 | 0.032 | transit | 523.4±1.1 | 4321 | [38] | |||
Kepler-205c | 0.146 | 20.306546 | 0.122 | transit | 523.4±1.1 | 4321 | [38] | |||
Kepler-206b | 0.107 | 7.781987 | 0.078 | transit | 1972±16 | 0.94 | 5764 | [38] | ||
Kepler-206c | 0.158 | 13.137471 | 0.111 | transit | 1972±16 | 0.94 | 5764 | [38] | ||
Kepler-206d | 0.106 | 23.44281 | 0.163 | transit | 1972±16 | 0.94 | 5764 | [38] | ||
Kepler-207b | 0.14 | 1.611865 | 0.029 | transit | 2920±30 | 5920 | [38] | |||
Kepler-207c | 0.134 | 3.071571 | 0.044 | transit | 2920±30 | 5920 | [38] | |||
Kepler-207d | 0.295 | 5.868075 | 0.068 | transit | 2920±30 | 5920 | [38] | |||
Kepler-208b | 0.145 | 4.22864 | 0.054 | transit | 2580±20 | 1.03 | 6092 | [38] | ||
Kepler-208c | 0.124 | 7.466623 | 0.079 | transit | 2580±20 | 1.03 | 6092 | [38] | ||
Kepler-208d | 0.107 | 11.131786 | 0.103 | transit | 2580±20 | 1.03 | 6092 | [38] | ||
Kepler-208e | 0.132 | 16.259458 | 0.132 | transit | 2580±20 | 1.03 | 6092 | [38] | ||
Kepler-209b | 0.202 | 16.087845 | 0.122 | transit | 1913±18 | 5513 | [38] | |||
Kepler-209c | 0.277 | 41.749882 | 0.231 | transit | 1913±18 | 5513 | [38] | |||
Kepler-210b | 0.262 | 2.453234 | 0.032 | transit | 764±2 | 4559 | [38] | |||
Kepler-210c | 0.323 | 7.972513 | 0.07 | transit | 764±2 | 4559 | [38] | |||
Kepler-211b | 0.112 | 4.138575 | 0.048 | transit | 1018±5 | 0.97 | 5123 | [38] | ||
Kepler-211c | 0.115 | 6.04045 | 0.062 | transit | 1018±5 | 0.97 | 5123 | [38] | ||
Kepler-212b | 0.097 | 16.257582 | 0.133 | transit | 2280±20 | 1.16 | 5852 | [38] | ||
Kepler-212c | 0.244 | 31.805174 | 0.207 | transit | 2280±20 | 1.16 | 5852 | [38] | ||
Kepler-213b | 0.145 | 2.46236 | 0.036 | transit | 2100±20 | 0.94 | 5696 | [38] | ||
Kepler-213c | 0.209 | 4.822962 | 0.057 | transit | 2100±20 | 0.94 | 5696 | [38] | ||
Kepler-214b | 0.233 | 15.660544 | 0.13 | transit | 4080±70 | 6169 | [38] | |||
Kepler-214c | 0.19 | 28.7798 | 0.194 | transit | 4080±70 | 6169 | [38] | |||
Kepler-215b | 0.145 | 9.360672 | 0.084 | transit | 1607±12 | 0.77 | 5739 | [38] | ||
Kepler-215c | 0.158 | 14.667108 | 0.113 | transit | 1607±12 | 0.77 | 5739 | [38] | ||
Kepler-215d | 0.213 | 30.864423 | 0.185 | transit | 1607±12 | 0.77 | 5739 | [38] | ||
Kepler-215e | 0.156 | 68.16101 | 0.314 | transit | 1607±12 | 0.77 | 5739 | [38] | ||
Kepler-216b | 0.21 | 7.693641 | 0.079 | transit | 4000±70 | 6091 | [38] | |||
Kepler-216c | 0.271 | 17.406669 | 0.136 | transit | 4000±70 | 6091 | [38] | |||
Kepler-217b | 0.199 | 5.374943 | 0.065 | transit | 3720±50 | 6171 | [38] | |||
Kepler-217c | 0.165 | 8.586004 | 0.089 | transit | 3720±50 | 6171 | [38] | |||
Kepler-218b | 0.132 | 3.619337 | 0.046 | transit | 2180±20 | 5502 | [38] | |||
Kepler-218c | 0.28 | 44.699576 | 0.248 | transit | 2180±20 | 5502 | [38] | |||
Kepler-219b | 0.263 | 4.585512 | 0.057 | transit | 2620±30 | 5786 | [38] | |||
Kepler-219c | 0.319 | 22.714613 | 0.165 | transit | 2620±30 | 5786 | [38] | |||
Kepler-219d | 0.251 | 47.903645 | 0.272 | transit | 2620±30 | 5786 | [38] | |||
Kepler-220b | 0.072 | 4.159807 | 0.046 | transit | 560±2 | 4632 | [38] | |||
Kepler-220c | 0.14 | 9.034199 | 0.076 | transit | 560±2 | 4632 | [38] | |||
Kepler-220d | 0.087 | 28.122397 | 0.163 | transit | 560±2 | 4632 | [38] | |||
Kepler-220e | 0.119 | 45.902733 | 0.226 | transit | 560±2 | 4632 | [38] | |||
Kepler-221b | 0.153 | 2.795906 | 0.037 | transit | 1270±9 | 0.72 | 5243 | [38] | ||
Kepler-221c | 0.261 | 5.690586 | 0.059 | transit | 1270±9 | 0.72 | 5243 | [38] | ||
Kepler-221d | 0.244 | 10.04156 | 0.087 | transit | 1270±9 | 0.72 | 5243 | [38] | ||
Kepler-221e | 0.235 | 18.369917 | 0.13 | transit | 1270±9 | 0.72 | 5243 | [38] | ||
Kepler-222b | 0.282 | 3.936981 | 0.048 | transit | 2520±40 | 5433 | [38] | |||
Kepler-222c | 0.414 | 10.08881 | 0.091 | transit | 2520±40 | 5433 | [38] | |||
Kepler-222d | 0.329 | 28.081912 | 0.18 | transit | 2520±40 | 5433 | [38] | |||
Kepler-223b | 0.02328 | 0.267 | 7.38449 | transit | 6400±400 | 1.12 | [38] | |||
Kepler-223c | 0.01605 | 0.307 | 9.84564 | transit | 6400±400 | 1.12 | [38] | |||
Kepler-223d | 0.02517 | 0.467 | 14.78869 | transit | 6400±400 | 1.12 | [38] | |||
Kepler-223e | 0.0151 | 0.41 | 19.72567 | transit | 6400±400 | 1.12 | [38] | |||
Kepler-224b | 0.124 | 3.132924 | 0.038 | transit | 2600±60 | 0.74 | 5018 | [38] | ||
Kepler-224c | 0.278 | 5.925003 | 0.058 | transit | 2600±60 | 0.74 | 5018 | [38] | ||
Kepler-224d | 0.205 | 11.349393 | 0.089 | transit | 2600±60 | 0.74 | 5018 | [38] | ||
Kepler-224e | 0.176 | 18.643577 | 0.124 | transit | 2600±60 | 0.74 | 5018 | [38] | ||
Kepler-225b | 0.107 | 6.738975 | 0.056 | transit | 1850±40 | 3682 | [38] | |||
Kepler-225c | 0.164 | 18.794234 | 0.111 | transit | 1850±40 | 3682 | [38] | |||
Kepler-226b | 0.138 | 3.940997 | 0.047 | transit | 3280±80 | 0.86 | 5571 | [38] | ||
Kepler-226c | 0.203 | 5.349555 | 0.058 | transit | 3280±80 | 0.86 | 5571 | [38] | ||
Kepler-226d | 0.109 | 8.109044 | 0.076 | transit | 3280±80 | 0.86 | 5571 | [38] | ||
Kepler-227b | 0.277 | 9.488015 | 0.09 | transit | 3640±100 | 5854 | [38] | |||
Kepler-227c | 0.271 | 54.418694 | 0.29 | transit | 3640±100 | 5854 | [38] | |||
Kepler-228b | 0.136 | 2.566546 | 0.038 | transit | 5600±300 | 6043 | [38] | |||
Kepler-228c | 0.241 | 4.134444 | 0.052 | transit | 5600±300 | 6043 | [38] | |||
Kepler-228d | 0.36 | 11.094286 | 0.101 | transit | 5600±300 | 6043 | [38] | |||
Kepler-229b | 0.196 | 6.252972 | 0.062 | transit | 2750±70 | 5120 | [38] | |||
Kepler-229c | 0.439 | 16.068638 | 0.117 | transit | 2750±70 | 5120 | [38] | |||
Kepler-229d | 0.343 | 41.194912 | 0.22 | transit | 2750±70 | 5120 | [38] | |||
Kepler-230b | 0.38 | 32.625555 | 0.191 | transit | 2460±40 | 5588 | [38] | |||
Kepler-230c | 0.182 | 91.773242 | 0.38 | transit | 2460±40 | 5588 | [38] | |||
Kepler-231b | 0.154 | 10.065275 | 0.074 | transit | 988±9 | 0.58 | 3767 | [38] | ||
Kepler-231c | 0.172 | 19.271566 | 0.114 | transit | 988±9 | 0.58 | 3767 | [38] | ||
Kepler-232b | 0.275 | 4.431222 | 0.054 | transit | 4570±160 | 5847 | [38] | |||
Kepler-232c | 0.342 | 11.379349 | 0.101 | transit | 4570±160 | 5847 | [38] | |||
Kepler-233b | 0.217 | 8.472382 | 0.077 | transit | 2860±60 | 5360 | [38] | |||
Kepler-233c | 0.242 | 60.418955 | 0.287 | transit | 2860±60 | 5360 | [38] | |||
Kepler-234b | 0.33 | 2.711506 | 0.04 | transit | 5900±300 | 6224 | [38] | |||
Kepler-234c | 0.313 | 7.21205 | 0.077 | transit | 5900±300 | 6224 | [38] | |||
Kepler-235b | 0.199 | 3.340222 | 0.037 | transit | 1410±20 | 0.59 | 4255 | [38] | ||
Kepler-235c | 0.114 | 7.824904 | 0.065 | transit | 1410±20 | 0.59 | 4255 | [38] | ||
Kepler-235d | 0.183 | 20.060548 | 0.122 | transit | 1410±20 | 0.59 | 4255 | [38] | ||
Kepler-235e | 0.198 | 46.183669 | 0.213 | transit | 1410±20 | 0.59 | 4255 | [38] | ||
Kepler-236b | 0.14 | 8.295611 | 0.065 | transit | 949±7 | 0.56 | 3750 | [38] | ||
Kepler-236c | 0.178 | 23.968127 | 0.132 | transit | 949±7 | 0.56 | 3750 | [38] | ||
Kepler-237b | 0.126 | 4.715106 | 0.05 | transit | 2180±30 | 0.7 | 4861 | [38] | ||
Kepler-237c | 0.186 | 8.103636 | 0.071 | transit | 2180±30 | 0.7 | 4861 | [38] | ||
Kepler-238b | 0.154 | 2.090876 | 0.034 | transit | 6200±300 | 1.06 | 5751 | [38] | ||
Kepler-238c | 0.213 | 6.155557 | 0.069 | transit | 6200±300 | 1.06 | 5751 | [38] | ||
Kepler-238d | 0.274 | 13.233549 | 0.115 | transit | 6200±300 | 1.06 | 5751 | [38] | ||
Kepler-239b | 0.208 | 11.763051 | 0.095 | transit | 2150±40 | 0.74 | 4914 | [38] | ||
Kepler-239c | 0.224 | 56.228098 | 0.268 | transit | 2150±40 | 0.74 | 4914 | [38] | ||
Kepler-240b | 0.122 | 4.144495 | 0.048 | transit | 2480±60 | 4985 | [38] | |||
Kepler-240c | 0.196 | 7.953528 | 0.074 | transit | 2480±60 | 4985 | [38] | |||
Kepler-241b | 0.208 | 12.718092 | 0.094 | transit | 1980±130 | 4699 | [38] | |||
Kepler-241c | 0.229 | 36.065978 | 0.189 | transit | 1980±130 | 4699 | [38] | |||
Kepler-242b | 0.233 | 8.20395 | 0.075 | transit | 1990±30 | 5020 | [38] | |||
Kepler-242c | 0.178 | 14.496481 | 0.109 | transit | 1990±30 | 5020 | [38] | |||
Kepler-243b | 0.219 | 5.715442 | 0.062 | transit | 2300±30 | 0.89 | 5228 | [38] | ||
Kepler-243c | 0.178 | 20.026218 | 0.142 | transit | 2300±30 | 0.89 | 5228 | [38] | ||
Kepler-244b | 0.246 | 4.311792 | 0.05 | transit | 3480±120 | 5554 | [38] | |||
Kepler-244c | 0.183 | 9.767292 | 0.087 | transit | 3480±120 | 5554 | [38] | |||
Kepler-244d | 0.206 | 20.050401 | 0.14 | transit | 3480±120 | 5554 | [38] | |||
Kepler-245b | 0.229 | 7.49019 | 0.071 | transit | 2870±80 | 0.8 | 5100 | [38] | ||
Kepler-245c | 0.194 | 17.460812 | 0.124 | transit | 2870±80 | 0.8 | 5100 | [38] | ||
Kepler-245d | 0.27 | 36.277108 | 0.202 | transit | 2870±80 | 0.8 | 5100 | [38] | ||
Kepler-246b | 0.209 | 4.60182 | 0.052 | transit | 2070±20 | 0.86 | 5206 | [38] | ||
Kepler-246c | 0.134 | 11.187161 | 0.095 | transit | 2070±20 | 0.86 | 5206 | [38] | ||
Kepler-247b | 0.146 | 3.33616 | 0.042 | transit | 2200±40 | 5100 | [38] | |||
Kepler-247c | 0.365 | 9.439452 | 0.084 | transit | 2200±40 | 5100 | [38] | |||
Kepler-247d | 0.352 | 20.477912 | 0.14 | transit | 2200±40 | 5100 | [38] | |||
Kepler-248b | 0.269 | 6.308205 | 0.066 | transit | 2460±40 | 5190 | [38] | |||
Kepler-248c | 0.363 | 16.239494 | 0.123 | transit | 2460±40 | 5190 | [38] | |||
Kepler-249b | 0.097 | 3.306539 | 0.035 | transit | 624±3 | 3568 | [38] | |||
Kepler-249c | 0.135 | 7.113702 | 0.058 | transit | 624±3 | 3568 | [38] | |||
Kepler-249d | 0.14 | 15.368459 | 0.097 | transit | 624±3 | 3568 | [38] | |||
Kepler-250b | 0.101 | 4.148141 | 0.048 | transit | 2530±50 | 0.8 | 5160 | [38] | ||
Kepler-250c | 0.203 | 7.156804 | 0.069 | transit | 2530±50 | 0.8 | 5160 | [38] | ||
Kepler-250d | 0.194 | 17.648312 | 0.127 | transit | 2530±50 | 0.8 | 5160 | [38] | ||
Kepler-251b | 0.119 | 4.790936 | 0.053 | transit | 3090±90 | 0.91 | 5526 | [38] | ||
Kepler-251c | 0.247 | 16.514043 | 0.122 | transit | 3090±90 | 0.91 | 5526 | [38] | ||
Kepler-251d | 0.247 | 30.133001 | 0.182 | transit | 3090±90 | 0.91 | 5526 | [38] | ||
Kepler-251e | 0.247 | 99.640161 | 0.404 | transit | 3090±90 | 0.91 | 5526 | [38] | ||
Kepler-252b | 0.11 | 6.668391 | 0.058 | transit | 1251±11 | 0.52 | 4208 | [38] | ||
Kepler-252c | 0.192 | 10.848463 | 0.08 | transit | 1251±11 | 0.52 | 4208 | [38] | ||
Kepler-253b | 0.145 | 3.783986 | 0.046 | transit | 2800±60 | 5208 | [38] | |||
Kepler-253c | 0.236 | 10.281951 | 0.089 | transit | 2800±60 | 5208 | [38] | |||
Kepler-253d | 0.283 | 18.119869 | 0.13 | transit | 2800±60 | 5208 | [38] | |||
Kepler-254b | 0.345 | 5.826662 | 0.064 | transit | 4700±200 | 5957 | [38] | |||
Kepler-254c | 0.192 | 12.412183 | 0.105 | transit | 4700±200 | 5957 | [38] | |||
Kepler-254d | 0.223 | 18.746477 | 0.139 | transit | 4700±200 | 5957 | [38] | |||
Kepler-255b | 0.138 | 5.714606 | 0.063 | transit | 3530±100 | 0.97 | 5573 | [38] | ||
Kepler-255c | 0.267 | 9.946047 | 0.092 | transit | 3530±100 | 0.97 | 5573 | [38] | ||
Kepler-256b | 0.142 | 1.620493 | 0.027 | transit | 3440±80 | 1.02 | 5551 | [38] | ||
Kepler-256c | 0.192 | 3.38802 | 0.045 | transit | 3440±80 | 1.02 | 5551 | [38] | ||
Kepler-256d | 0.221 | 5.839172 | 0.064 | transit | 3440±80 | 1.02 | 5551 | [38] | ||
Kepler-256e | 0.21 | 10.681572 | 0.096 | transit | 3440±80 | 1.02 | 5551 | [38] | ||
Kepler-257b | 0.233 | 2.382667 | 0.034 | transit | 2600±50 | 5180 | [38] | |||
Kepler-257c | 0.483 | 6.581484 | 0.066 | transit | 2600±50 | 5180 | [38] | |||
Kepler-257d | 0.442 | 24.664551 | 0.16 | transit | 2600±50 | 5180 | [38] | |||
Kepler-258b | 0.362 | 13.19722 | 0.103 | transit | 1900±20 | 0.8 | 4942 | [38] | ||
Kepler-258c | 0.322 | 33.653079 | 0.193 | transit | 1900±20 | 0.8 | 4942 | [38] | ||
Kepler-259b | 0.25 | 8.115317 | 0.079 | transit | 3360±80 | 5938 | [38] | |||
Kepler-259c | 0.241 | 36.924931 | 0.217 | transit | 3360±80 | 5938 | [38] | |||
Kepler-260b | 0.179 | 8.187399 | 0.075 | transit | 2080±20 | 0.88 | 5250 | [38] | ||
Kepler-260c | 0.155 | 76.050178 | 0.332 | transit | 2080±20 | 0.88 | 5250 | [38] | ||
Kepler-261b | 0.194 | 10.381227 | 0.088 | transit | 1044±5 | 0.87 | 5098 | [38] | ||
Kepler-261c | 0.178 | 24.570858 | 0.156 | transit | 1044±5 | 0.87 | 5098 | [38] | ||
Kepler-262b | 0.121 | 13.060855 | 0.108 | transit | 2030±20 | 5841 | [38] | |||
Kepler-262c | 0.146 | 21.853722 | 0.152 | transit | 2030±20 | 5841 | [38] | |||
Kepler-263b | 0.238 | 16.568087 | 0.12 | transit | 2510±50 | 5265 | [38] | |||
Kepler-263c | 0.22 | 47.332773 | 0.242 | transit | 2510±50 | 5265 | [38] | |||
Kepler-264b | 0.297 | 40.806231 | 0.249 | transit | 3150±60 | 1.32 | 6158 | [38] | ||
Kepler-264c | 0.252 | 140.101261 | 0.566 | transit | 3150±60 | 1.32 | 6158 | [38] | ||
Kepler-265b | 0.166 | 6.846262 | 0.069 | transit | 4330±160 | 1.03 | 5835 | [38] | ||
Kepler-265c | 0.235 | 17.028937 | 0.127 | transit | 4330±160 | 1.03 | 5835 | [38] | ||
Kepler-265d | 0.222 | 43.130617 | 0.236 | transit | 4330±160 | 1.03 | 5835 | [38] | ||
Kepler-265e | 0.231 | 67.831024 | 0.319 | transit | 4330±160 | 1.03 | 5835 | [38] | ||
Kepler-266b | 0.221 | 6.61833 | 0.071 | transit | 4640±190 | 0.99 | 5885 | [38] | ||
Kepler-266c | 0.347 | 107.723601 | 0.457 | transit | 4640±190 | 0.99 | 5885 | [38] | ||
Kepler-267b | 0.177 | 3.353728 | 0.037 | transit | 870±8 | 0.56 | 4258 | [38] | ||
Kepler-267c | 0.19 | 6.87745 | 0.06 | transit | 870±8 | 0.56 | 4258 | [38] | ||
Kepler-267d | 0.203 | 28.464515 | 0.154 | transit | 870±8 | 0.56 | 4258 | [38] | ||
Kepler-268b | 0.227 | 25.934138 | 0.18 | transit | 2840±30 | 6081 | [38] | |||
Kepler-268c | 0.302 | 83.446393 | 0.391 | transit | 2840±30 | 6081 | [38] | |||
Kepler-269b | 0.22 | 5.326718 | 0.061 | transit | 7900±600 | 0.98 | 5847 | [38] | ||
Kepler-269c | 0.151 | 8.127899 | 0.081 | transit | 7900±600 | 0.98 | 5847 | [38] | ||
Kepler-270b | 0.179 | 11.476094 | 0.107 | transit | 3180±40 | 6067 | [38] | |||
Kepler-270c | 0.158 | 25.262887 | 0.18 | transit | 3180±40 | 6067 | [38] | |||
Kepler-271b | 0.079 | 5.217738 | 0.056 | transit | 1334±12 | 5524 | [38] | |||
Kepler-271c | 0.089 | 7.410935 | 0.071 | transit | 1334±12 | 5524 | [38] | |||
Kepler-272b | 0.128 | 2.971353 | 0.038 | transit | 2970±40 | 0.79 | 5297 | [38] | ||
Kepler-272c | 0.16 | 6.057342 | 0.061 | transit | 2970±40 | 0.79 | 5297 | [38] | ||
Kepler-272d | 0.201 | 10.937304 | 0.091 | transit | 2970±40 | 0.79 | 5297 | [38] | ||
Kepler-273b | 0.134 | 2.936532 | 0.037 | transit | 2370±30 | 5626 | [38] | |||
Kepler-273c | 0.177 | 8.014927 | 0.073 | transit | 2370±30 | 5626 | [38] | |||
Kepler-274b | 0.137 | 11.634788 | 0.101 | transit | 4510±140 | 6023 | [38] | |||
Kepler-274c | 0.164 | 33.197861 | 0.204 | transit | 4510±140 | 6023 | [38] | |||
Kepler-275b | 0.209 | 10.300682 | 0.098 | transit | 7000±500 | 1.24 | 6165 | [38] | ||
Kepler-275c | 0.302 | 16.088134 | 0.132 | transit | 7000±500 | 1.24 | 6165 | [38] | ||
Kepler-275d | 0.297 | 35.676062 | 0.224 | transit | 7000±500 | 1.24 | 6165 | [38] | ||
Kepler-276b | 0.256 | 14.12841 | 0.119 | transit | 3850±150 | 1.1 | 6105 | [38] | ||
Kepler-278b | 0.363 | 30.160546 | 0.207 | transit | 1460±20 | 4991 | [38] | |||
Kepler-278c | 0.32 | 51.078775 | 0.294 | transit | 1460±20 | 4991 | [38] | |||
Kepler-280b | 0.129 | 2.139542 | 0.032 | transit | 2600±30 | 0.91 | 5744 | [38] | ||
Kepler-280c | 0.179 | 4.807091 | 0.056 | transit | 2600±30 | 0.91 | 5744 | [38] | ||
Kepler-281b | 0.252 | 14.646008 | 0.117 | transit | 6000±300 | 0.98 | 5723 | [38] | ||
Kepler-281c | 0.474 | 36.337373 | 0.215 | transit | 6000±300 | 0.98 | 5723 | [38] | ||
Kepler-282b | 0.09 | 9.220524 | 0.082 | transit | 4530±150 | 0.97 | 5602 | [38] | ||
Kepler-282c | 0.107 | 13.638723 | 0.106 | transit | 4530±150 | 0.97 | 5602 | [38] | ||
Kepler-283b | 0.19 | 11.008151 | 0.082 | transit | 1540±20 | 4351 | [38] | |||
Kepler-283c | 0.162 | 92.743711 | 0.341 | transit | 1540±20 | 4351 | [38] | |||
Kepler-284b | 0.2 | 12.699149 | 0.104 | transit | 3460±110 | 5615 | [38] | |||
Kepler-284c | 0.233 | 37.514456 | 0.213 | transit | 3460±110 | 5615 | [38] | |||
Kepler-285b | 0.12 | 2.633867 | 0.036 | transit | 2750±50 | 0.85 | 5411 | [38] | ||
Kepler-285c | 0.1 | 6.186676 | 0.064 | transit | 2750±50 | 0.85 | 5411 | [38] | ||
Kepler-286b | 0.111 | 1.796302 | 0.027 | transit | 4100±400 | 5580 | [38] | |||
Kepler-286c | 0.122 | 3.468095 | 0.042 | transit | 4100±400 | 5580 | [38] | |||
Kepler-286d | 0.119 | 5.914323 | 0.061 | transit | 4100±400 | 5580 | [38] | |||
Kepler-286e | 0.158 | 29.221289 | 0.176 | transit | 4100±400 | 5580 | [38] | |||
Kepler-287b | 0.208 | 20.342199 | 0.145 | transit | 2790±50 | 5806 | [38] | |||
Kepler-287c | 0.291 | 44.851896 | 0.246 | transit | 2790±50 | 5806 | [38] | |||
Kepler-288b | 0.149 | 6.097326 | 0.065 | transit | 4030±110 | 0.89 | 5918 | [38] | ||
Kepler-288c | 0.254 | 19.305772 | 0.14 | transit | 4030±110 | 0.89 | 5918 | [38] | ||
Kepler-288d | 0.238 | 56.633742 | 0.287 | transit | 4030±110 | 0.89 | 5918 | [38] | ||
Kepler-289b | 0.023 | 0.192 | 34.545 | 0.21 | transit | 2340±20 | 1.08 | 5990 | [38] | |
Kepler-289c | 0.42 | 1.034 | 125.8518 | 0.51 | transit | 2340±20 | 1.08 | 5990 | [38] | |
Kepler-289d | 0.013 | 0.239 | 66.0634 | 0.33 | transit | 2340±20 | 1.08 | 5990 | ? | |
Kepler-290b | 0.201 | 14.589347 | 0.11 | transit | 2310±40 | 5147 | [38] | |||
Kepler-290c | 0.241 | 36.77031 | 0.205 | transit | 2310±40 | 5147 | [38] | |||
Kepler-291b | 0.193 | 3.546511 | 0.047 | transit | 6100±400 | 1.03 | 6002 | [38] | ||
Kepler-291c | 0.168 | 5.700786 | 0.065 | transit | 6100±400 | 1.03 | 6002 | [38] | ||
Kepler-292b | 0.118 | 2.580827 | 0.035 | transit | 3540±150 | 0.88 | 5299 | [38] | ||
Kepler-292c | 0.131 | 3.715335 | 0.045 | transit | 3540±150 | 0.88 | 5299 | [38] | ||
Kepler-292d | 0.199 | 7.055679 | 0.068 | transit | 3540±150 | 0.88 | 5299 | [38] | ||
Kepler-292e | 0.238 | 11.97901 | 0.097 | transit | 3540±150 | 0.88 | 5299 | [38] | ||
Kepler-292f | 0.21 | 20.834237 | 0.141 | transit | 3540±150 | 0.88 | 5299 | [38] | ||
Kepler-293b | 0.274 | 19.254196 | 0.144 | transit | 3260±70 | 1.01 | 5804 | [38] | ||
Kepler-293c | 0.342 | 54.155743 | 0.286 | transit | 3260±70 | 1.01 | 5804 | [38] | ||
Kepler-294b | 0.158 | 3.701212 | 0.048 | transit | 4600±200 | 5913 | [38] | |||
Kepler-294c | 0.242 | 6.6264 | 0.071 | transit | 4600±200 | 5913 | [38] | |||
Kepler-295b | 0.109 | 12.645164 | 0.099 | transit | 5800±300 | 5603 | [38] | |||
Kepler-295c | 0.104 | 21.526258 | 0.142 | transit | 5800±300 | 5603 | [38] | |||
Kepler-295d | 0.121 | 33.884054 | 0.192 | transit | 5800±300 | 5603 | [38] | |||
Kepler-296b | 0.144 | 10.864384 | 0.079 | transit | 740 | 0.5 | 3740 | [38] | ||
Kepler-296c | 0.178 | 5.8416366 | 0.0521 | transit | 740 | 0.5 | 3740 | [38] | ||
Kepler-296d | 0.186 | 19.850291 | 0.118 | transit | 740 | 0.5 | 3740 | [38] | ||
Kepler-296e | 0.136 | 34.14211 | 0.169 | transit | 740 | 0.5 | 3740 | [38] | ||
Kepler-296f | 0.161 | 63.33627 | 0.255 | transit | 740 | 0.5 | 3740 | [38] | ||
Kepler-297b | 0.256 | 38.871826 | 0.217 | transit | 2300±20 | 5619 | [38] | |||
Kepler-297c | 0.583 | 74.920137 | 0.336 | transit | 2300±20 | 5619 | [38] | |||
Kepler-298b | 0.175 | 10.475464 | 0.08 | transit | 1710±20 | 0.65 | 4465 | [38] | ||
Kepler-298c | 0.172 | 22.92881 | 0.136 | transit | 1710±20 | 0.65 | 4465 | [38] | ||
Kepler-298d | 0.223 | 77.473633 | 0.305 | transit | 1710±20 | 0.65 | 4465 | [38] | ||
Kepler-299b | 0.118 | 2.927128 | 0.04 | transit | 3530±80 | 0.97 | 5617 | [38] | ||
Kepler-299c | 0.236 | 6.885875 | 0.07 | transit | 3530±80 | 0.97 | 5617 | [38] | ||
Kepler-299d | 0.166 | 15.054786 | 0.118 | transit | 3530±80 | 0.97 | 5617 | [38] | ||
Kepler-299e | 0.167 | 38.285489 | 0.22 | transit | 3530±80 | 0.97 | 5617 | [38] | ||
Kepler-300b | 0.149 | 10.446347 | 0.094 | transit | 3690±60 | 0.94 | 5986 | [38] | ||
Kepler-300c | 0.201 | 40.714955 | 0.232 | transit | 3690±60 | 0.94 | 5986 | [38] | ||
Kepler-301b | 0.12 | 2.508553 | 0.036 | transit | 2390±30 | 0.91 | 5815 | [38] | ||
Kepler-301c | 0.12 | 5.419026 | 0.06 | transit | 2390±30 | 0.91 | 5815 | [38] | ||
Kepler-301d | 0.156 | 13.751243 | 0.112 | transit | 2390±30 | 0.91 | 5815 | [38] | ||
Kepler-302b | 0.362 | 30.184104 | 0.193 | transit | 4760±190 | 5740 | [38] | |||
Kepler-302c | 1.111 | 127.282184 | 0.503 | transit | 4760±190 | 5740 | [38] | |||
Kepler-303b | 0.079 | 1.937055 | 0.024 | transit | 688±3 | 0.59 | 3944 | [38] | ||
Kepler-303c | 0.102 | 7.061149 | 0.057 | transit | 688±3 | 0.59 | 3944 | [38] | ||
Kepler-304b | 0.255 | 3.295709 | 0.039 | transit | 1435±17 | 0.8 | 4731 | [38] | ||
Kepler-304c | 0.194 | 5.315946 | 0.054 | transit | 1435±17 | 0.8 | 4731 | [38] | ||
Kepler-304d | 0.245 | 9.653471 | 0.08 | transit | 1435±17 | 0.8 | 4731 | [38] | ||
Kepler-305d | 0.242 | 16.738661 | 0.121 | transit | 2900±80 | 0.76 | 5100 | [38] | ||
Kepler-306b | 0.136 | 4.646186 | 0.05 | transit | 2580±60 | 0.82 | 4954 | [38] | ||
Kepler-306c | 0.21 | 7.240193 | 0.067 | transit | 2580±60 | 0.82 | 4954 | [38] | ||
Kepler-306d | 0.22 | 17.326644 | 0.12 | transit | 2580±60 | 0.82 | 4954 | [38] | ||
Kepler-306e | 0.203 | 44.840975 | 0.227 | transit | 2580±60 | 0.82 | 4954 | [38] | ||
Kepler-308b | 0.189 | 9.694928 | 0.09 | transit | 4500±200 | 5895 | [38] | |||
Kepler-308c | 0.193 | 15.38231 | 0.123 | transit | 4500±200 | 5895 | [38] | |||
Kepler-309b | 0.139 | 5.923653 | 0.059 | transit | 1804±19 | 4713 | [38] | |||
Kepler-309c | 0.224 | 105.356383 | 0.401 | transit | 1804±19 | 4713 | [38] | |||
Kepler-310b | 0.106 | 13.930698 | 0.111 | transit | 1990±20 | 0.85 | 5797 | [38] | ||
Kepler-310c | 0.302 | 56.47542 | 0.281 | transit | 1990±20 | 0.85 | 5797 | [38] | ||
Kepler-310d | 0.22 | 92.876125 | 0.392 | transit | 1990±20 | 0.85 | 5797 | [38] | ||
Kepler-311b | 0.152 | 9.176092 | 0.087 | transit | 2590±30 | 1.06 | 5905 | [38] | ||
Kepler-311c | 0.128 | 19.738286 | 0.145 | transit | 2590±30 | 1.06 | 5905 | [38] | ||
Kepler-312b | 0.115 | 1.772419 | 0.031 | transit | 2660±40 | 1.23 | 6115 | [38] | ||
Kepler-312c | 0.281 | 19.747412 | 0.153 | transit | 2660±40 | 1.23 | 6115 | [38] | ||
Kepler-313b | 0.226 | 14.970418 | 0.125 | transit | 3500±300 | 0.9 | 5727 | [38] | ||
Kepler-313c | 0.229 | 32.273273 | 0.208 | transit | 3500±300 | 0.9 | 5727 | [38] | ||
Kepler-314b | 0.074 | 2.461069 | 0.035 | transit | 883±5 | 1.02 | 5378 | [38] | ||
Kepler-314c | 0.259 | 5.960392 | 0.064 | transit | 883±5 | 1.02 | 5378 | [38] | ||
Kepler-315b | 0.336 | 96.101141 | 0.402 | transit | 3910±120 | 0.78 | 5796 | [38] | ||
Kepler-315c | 0.37 | 265.469335 | 0.791 | transit | 3910±120 | 0.78 | 5796 | [38] | ||
Kepler-316b | 0.095 | 2.240508 | 0.027 | transit | 1269±12 | 0.53 | 4204 | [38] | ||
Kepler-316c | 0.103 | 6.827766 | 0.058 | transit | 1269±12 | 0.53 | 4204 | [38] | ||
Kepler-317b | 0.186 | 5.524242 | 0.061 | transit | 3150±80 | 0.95 | 5497 | [38] | ||
Kepler-317c | 0.153 | 8.77501 | 0.083 | transit | 3150±80 | 0.95 | 5497 | [38] | ||
Kepler-318b | 0.42 | 4.662715 | 0.056 | transit | 1618±10 | 1.05 | 5746 | [38] | ||
Kepler-318c | 0.328 | 11.815007 | 0.105 | transit | 1618±10 | 1.05 | 5746 | [38] | ||
Kepler-319b | 0.145 | 4.362705 | 0.051 | transit | 1666±15 | 1.29 | 5526 | [38] | ||
Kepler-319c | 0.235 | 6.941357 | 0.069 | transit | 1666±15 | 1.29 | 5526 | [38] | ||
Kepler-319d | 0.204 | 31.781925 | 0.191 | transit | 1666±15 | 1.29 | 5526 | [38] | ||
Kepler-320b | 0.102 | 8.371554 | 0.085 | transit | 2760±30 | 6435 | [38] | |||
Kepler-320c | 0.122 | 17.934937 | 0.142 | transit | 2760±30 | 6435 | [38] | |||
Kepler-321b | 0.158 | 4.915379 | 0.057 | transit | 1268±11 | 1.01 | 5740 | [38] | ||
Kepler-321c | 0.207 | 13.093921 | 0.11 | transit | 1268±11 | 1.01 | 5740 | [38] | ||
Kepler-322b | 0.09 | 1.653888 | 0.027 | transit | 1321±8 | 0.91 | 5388 | [38] | ||
Kepler-322c | 0.149 | 4.337234 | 0.051 | transit | 1321±8 | 0.91 | 5388 | [38] | ||
Kepler-323b | 0.128 | 1.678327 | 0.028 | transit | 1500±20 | 1.09 | 5987 | [38] | ||
Kepler-323c | 0.145 | 3.553822 | 0.046 | transit | 1500±20 | 1.09 | 5987 | [38] | ||
Kepler-324b | 0.102 | 4.385315 | 0.05 | transit | 1659±12 | 0.86 | 5194 | [38] | ||
Kepler-324c | 0.281 | 51.805612 | 0.26 | transit | 1659±12 | 0.86 | 5194 | [38] | ||
Kepler-325b | 0.26 | 4.544439 | 0.053 | transit | 2740±40 | 0.87 | 5752 | [38] | ||
Kepler-325c | 0.227 | 12.762172 | 0.105 | transit | 2740±40 | 0.87 | 5752 | [38] | ||
Kepler-325d | 0.249 | 38.715185 | 0.22 | transit | 2740±40 | 0.87 | 5752 | [38] | ||
Kepler-326b | 0.136 | 2.248329 | 0.032 | transit | 1610±30 | 0.98 | 5105 | [38] | ||
Kepler-326c | 0.125 | 4.580358 | 0.051 | transit | 1610±30 | 0.98 | 5105 | [38] | ||
Kepler-326d | 0.108 | 6.766888 | 0.066 | transit | 1610±30 | 0.98 | 5105 | [38] | ||
Kepler-327b | 0.099 | 2.549575 | 0.029 | transit | 794±4 | 0.55 | 3799 | [38] | ||
Kepler-327c | 0.092 | 5.212333 | 0.047 | transit | 794±4 | 0.55 | 3799 | [38] | ||
Kepler-327d | 0.154 | 13.969457 | 0.09 | transit | 794±4 | 0.55 | 3799 | [38] | ||
Kepler-329b | 0.125 | 7.416397 | 0.061 | transit | 1450±20 | 0.53 | 4257 | [38] | ||
Kepler-329c | 0.172 | 18.684737 | 0.113 | transit | 1450±20 | 0.53 | 4257 | [38] | ||
Kepler-330b | 0.12 | 8.25978 | 0.075 | transit | 2380±40 | 0.78 | 5117 | [38] | ||
Kepler-330c | 0.174 | 15.955387 | 0.116 | transit | 2380±40 | 0.78 | 5117 | [38] | ||
Kepler-331b | 0.162 | 8.457496 | 0.065 | transit | 1920±40 | 0.51 | 4347 | [38] | ||
Kepler-331c | 0.164 | 17.28111 | 0.105 | transit | 1920±40 | 0.51 | 4347 | [38] | ||
Kepler-331d | 0.146 | 32.134328 | 0.159 | transit | 1920±40 | 0.51 | 4347 | [38] | ||
Kepler-332b | 0.104 | 7.626324 | 0.07 | transit | 1133±5 | 0.8 | 4955 | [38] | ||
Kepler-332c | 0.097 | 15.995622 | 0.114 | transit | 1133±5 | 0.8 | 4955 | [38] | ||
Kepler-332d | 0.105 | 34.21154 | 0.189 | transit | 1133±5 | 0.8 | 4955 | [38] | ||
Kepler-333b | 0.118 | 12.551158 | 0.087 | transit | 1068±7 | 0.54 | 4259 | [38] | ||
Kepler-333c | 0.099 | 24.08821 | 0.135 | transit | 1068±7 | 0.54 | 4259 | [38] | ||
Kepler-334b | 0.1 | 5.470319 | 0.061 | transit | 1408±14 | 1 | 5828 | [38] | ||
Kepler-334c | 0.128 | 12.758005 | 0.107 | transit | 1408±14 | 1 | 5828 | [38] | ||
Kepler-334d | 0.126 | 25.09849 | 0.168 | transit | 1408±14 | 1 | 5828 | [38] | ||
Kepler-335b | 0.302 | 6.562331 | 0.075 | transit | 4320±100 | 0.99 | 5877 | [38] | ||
Kepler-335c | 0.274 | 67.844469 | 0.356 | transit | 4320±100 | 0.99 | 5877 | [38] | ||
Kepler-336b | 0.091 | 2.024823 | 0.033 | transit | 8000±7000 | 0.89 | 5867 | [38] | ||
Kepler-336c | 0.187 | 9.600001 | 0.092 | transit | 8000±7000 | 0.89 | 5867 | [38] | ||
Kepler-336d | 0.211 | 20.678772 | 0.154 | transit | 8000±7000 | 0.89 | 5867 | [38] | ||
Kepler-337b | 0.137 | 3.292781 | 0.045 | transit | 2250±30 | 0.96 | 5684 | [38] | ||
Kepler-337c | 0.183 | 9.693201 | 0.093 | transit | 2250±30 | 0.96 | 5684 | [38] | ||
Kepler-338b | 0.218 | 13.726976 | 0.117 | transit | 1830±20 | 1.1 | 5923 | [38] | ||
Kepler-338c | 0.209 | 24.310856 | 0.172 | transit | 1830±20 | 1.1 | 5923 | [38] | ||
Kepler-338d | 0.268 | 44.431014 | 0.257 | transit | 1830±20 | 1.1 | 5923 | [38] | ||
Kepler-338e | 0.027 | 0.139 | 9.341 | timing | 1830±20 | 1.1 | 5923 | ? | ||
Kepler-339b | 0.127 | 4.977656 | 0.055 | transit | 2040±30 | 0.84 | 5631 | [38] | ||
Kepler-339c | 0.103 | 6.988055 | 0.069 | transit | 2040±30 | 0.84 | 5631 | [38] | ||
Kepler-339d | 0.104 | 10.558345 | 0.091 | transit | 2040±30 | 0.84 | 5631 | [38] | ||
Kepler-340b | 0.226 | 14.844387 | 0.134 | transit | 2690±60 | 2.11 | 6620 | [38] | ||
Kepler-340c | 0.301 | 22.824669 | 0.178 | transit | 2690±60 | 2.11 | 6620 | [38] | ||
Kepler-341b | 0.105 | 5.195528 | 0.06 | transit | 3520±60 | 0.94 | 6012 | [38] | ||
Kepler-341c | 0.152 | 8.01041 | 0.08 | transit | 3520±60 | 0.94 | 6012 | [38] | ||
Kepler-341d | 0.165 | 27.666313 | 0.182 | transit | 3520±60 | 0.94 | 6012 | [38] | ||
Kepler-341e | 0.178 | 42.473269 | 0.242 | transit | 3520±60 | 0.94 | 6012 | [38] | ||
Kepler-342b | 0.201 | 15.170318 | 0.128 | transit | 2600±30 | 1.13 | 6175 | [38] | ||
Kepler-342c | 0.175 | 26.234138 | 0.185 | transit | 2600±30 | 1.13 | 6175 | [38] | ||
Kepler-342d | 0.222 | 39.459357 | 0.242 | transit | 2600±30 | 1.13 | 6175 | [38] | ||
Kepler-343b | 0.215 | 8.96855 | 0.088 | transit | 3100±60 | 1.04 | 5807 | [38] | ||
Kepler-343c | 0.18 | 23.22182 | 0.167 | transit | 3100±60 | 1.04 | 5807 | [38] | ||
Kepler-344b | 0.233 | 21.963945 | 0.153 | transit | 3360±100 | 0.9 | 5774 | [38] | ||
Kepler-344c | 0.263 | 125.596809 | 0.488 | transit | 3360±100 | 0.9 | 5774 | [38] | ||
Kepler-345b | 0.066 | 7.415563 | 0.066 | transit | 1180±50 | 0.59 | 4504 | [38] | ||
Kepler-345c | 0.107 | 9.387427 | 0.077 | transit | 1180±50 | 0.59 | 4504 | [38] | ||
Kepler-346b | 0.237 | 6.511127 | 0.071 | transit | 3300±80 | 0.97 | 6033 | [38] | ||
Kepler-346c | 0.274 | 23.851549 | 0.168 | transit | 3300±80 | 0.97 | 6033 | [38] | ||
Kepler-347b | 0.176 | 12.79836 | 0.11 | transit | 4400±90 | 1.04 | 6088 | [38] | ||
Kepler-347c | 0.156 | 27.320871 | 0.183 | transit | 4400±90 | 1.04 | 6088 | [38] | ||
Kepler-348b | 0.136 | 7.05677 | 0.076 | transit | 1890±20 | 1.15 | 6177 | [38] | ||
Kepler-348c | 0.119 | 17.265427 | 0.138 | transit | 1890±20 | 1.15 | 6177 | [38] | ||
Kepler-349b | 0.17 | 5.929778 | 0.065 | transit | 3150±60 | 0.97 | 5956 | [38] | ||
Kepler-349c | 0.175 | 12.247629 | 0.105 | transit | 3150±60 | 0.97 | 5956 | [38] | ||
Kepler-350b | 0.165 | 11.189562 | 0.104 | transit | 3200±60 | 1 | 6186 | [38] | ||
Kepler-351b | 0.273 | 37.054919 | 0.214 | transit | 3640±40 | 0.89 | 5643 | [38] | ||
Kepler-351c | 0.285 | 57.24809 | 0.287 | transit | 3640±40 | 0.89 | 5643 | [38] | ||
Kepler-352b | 0.077 | 10.05537 | 0.085 | transit | 830±4 | 0.79 | 5212 | [38] | ||
Kepler-352c | 0.111 | 16.332995 | 0.118 | transit | 830±4 | 0.79 | 5212 | [38] | ||
Kepler-353b | 0.079 | 5.795278 | 0.051 | transit | 1268±16 | 0.54 | 3903 | [38] | ||
Kepler-353c | 0.123 | 8.410894 | 0.065 | transit | 1268±16 | 0.54 | 3903 | [38] | ||
Kepler-354b | 0.164 | 5.47666 | 0.054 | transit | 1830±20 | 0.65 | 4648 | [38] | ||
Kepler-354c | 0.117 | 16.934402 | 0.115 | transit | 1830±20 | 0.65 | 4648 | [38] | ||
Kepler-354d | 0.111 | 24.209842 | 0.146 | transit | 1830±20 | 0.65 | 4648 | [38] | ||
Kepler-355b | 0.13 | 11.03189 | 0.102 | transit | 4870±160 | 1.05 | 6184 | [38] | ||
Kepler-355c | 0.242 | 25.762294 | 0.179 | transit | 4870±160 | 1.05 | 6184 | [38] | ||
Kepler-356b | 0.14 | 4.612696 | 0.057 | transit | 2350±30 | 0.97 | 6133 | [38] | ||
Kepler-356c | 0.161 | 13.121632 | 0.115 | transit | 2350±30 | 0.97 | 6133 | [38] | ||
Kepler-357b | 0.164 | 6.475434 | 0.063 | transit | 2290±40 | 0.78 | 5036 | [38] | ||
Kepler-357c | 0.238 | 16.85837 | 0.12 | transit | 2290±40 | 0.78 | 5036 | [38] | ||
Kepler-357d | 0.306 | 49.499875 | 0.246 | transit | 2290±40 | 0.78 | 5036 | [38] | ||
Kepler-358b | 0.243 | 34.060467 | 0.21 | transit | 3700±130 | 0.95 | 5908 | [38] | ||
Kepler-358c | 0.254 | 83.488369 | 0.381 | transit | 3700±130 | 0.95 | 5908 | [38] | ||
Kepler-359b | 0.315 | 25.563222 | 0.178 | transit | 4900±300 | 1.07 | 6248 | [38] | ||
Kepler-359c | 0.384 | 57.68802 | 0.307 | transit | 4900±300 | 1.07 | 6248 | [38] | ||
Kepler-359d | 0.358 | 77.095691 | 0.372 | transit | 4900±300 | 1.07 | 6248 | [38] | ||
Kepler-360b | 0.147 | 3.289672 | 0.044 | transit | 2930±50 | 0.95 | 6053 | [38] | ||
Kepler-360c | 0.187 | 7.186434 | 0.075 | transit | 2930±50 | 0.95 | 6053 | [38] | ||
Kepler-361b | 0.129 | 8.486616 | 0.086 | transit | 3110±50 | 1.07 | 6169 | [38] | ||
Kepler-361c | 0.225 | 55.188023 | 0.3 | transit | 3110±50 | 1.07 | 6169 | [38] | ||
Kepler-362b | 0.079 | 10.327186 | 0.087 | transit | 3660±180 | 0.77 | 5788 | [38] | ||
Kepler-362c | 0.129 | 37.866281 | 0.207 | transit | 3660±180 | 0.77 | 5788 | [38] | ||
Kepler-363b | 0.103 | 3.614568 | 0.048 | transit | 2540±20 | 1.23 | 5593 | [38] | ||
Kepler-363c | 0.151 | 7.542427 | 0.079 | transit | 2540±20 | 1.23 | 5593 | [38] | ||
Kepler-363d | 0.183 | 11.932125 | 0.107 | transit | 2540±20 | 1.23 | 5593 | [38] | ||
Kepler-364b | 0.138 | 25.745718 | 0.178 | transit | 2980±30 | 1.2 | 6108 | [38] | ||
Kepler-364c | 0.192 | 59.980627 | 0.312 | transit | 2980±30 | 1.2 | 6108 | [38] | ||
Kepler-365b | 0.182 | 10.664903 | 0.098 | transit | 2800±200 | 0.99 | 6012 | [38] | ||
Kepler-365c | 0.146 | 17.784129 | 0.137 | transit | 2800±200 | 0.99 | 6012 | [38] | ||
Kepler-366b | 0.13 | 3.281959 | 0.045 | transit | 6400±400 | 1.05 | 6209 | [38] | ||
Kepler-366c | 0.16 | 12.51616 | 0.11 | transit | 6400±400 | 1.05 | 6209 | [38] | ||
Kepler-367b | 0.116 | 37.815724 | 0.201 | transit | 616±2 | 0.75 | 4710 | [38] | ||
Kepler-367c | 0.107 | 53.578637 | 0.253 | transit | 616±2 | 0.75 | 4710 | [38] | ||
Kepler-368b | 0.291 | 26.84768 | 0.186 | transit | 2570±40 | 0.71 | 5502 | [38] | ||
Kepler-368c | 0.346 | 72.379334 | 0.36 | transit | 2570±40 | 0.71 | 5502 | [38] | ||
Kepler-369b | 0.101 | 2.732756 | 0.03 | transit | 840±120 | 0.54 | 3591 | [38] | ||
Kepler-369c | 0.126 | 14.871572 | 0.094 | transit | 840±120 | 0.54 | 3591 | [38] | ||
Kepler-370b | 0.142 | 4.57953 | 0.054 | transit | 3930±120 | 0.94 | 5852 | [38] | ||
Kepler-370c | 0.17 | 19.02293 | 0.14 | transit | 3930±120 | 0.94 | 5852 | [38] | ||
Kepler-371b | 0.169 | 34.763278 | 0.2 | transit | 2710±40 | 0.94 | 5666 | [38] | ||
Kepler-371c | 0.159 | 67.968015 | 0.313 | transit | 2710±40 | 0.94 | 5666 | [38] | ||
Kepler-372b | 0.121 | 6.849692 | 0.075 | transit | 5090±170 | 1.15 | 6509 | [38] | ||
Kepler-372c | 0.186 | 20.053763 | 0.154 | transit | 5090±170 | 1.15 | 6509 | [38] | ||
Kepler-372d | 0.151 | 30.092568 | 0.201 | transit | 5090±170 | 1.15 | 6509 | [38] | ||
Kepler-373b | 0.121 | 5.535309 | 0.06 | transit | 3670±70 | 0.87 | 5787 | [38] | ||
Kepler-373c | 0.111 | 16.725948 | 0.126 | transit | 3670±70 | 0.87 | 5787 | [38] | ||
Kepler-374b | 0.092 | 1.897806 | 0.029 | transit | 4280±120 | 0.84 | 5977 | [38] | ||
Kepler-374c | 0.098 | 3.282807 | 0.042 | transit | 4280±120 | 0.84 | 5977 | [38] | ||
Kepler-374d | 0.117 | 5.028219 | 0.056 | transit | 4280±120 | 0.84 | 5977 | [38] | ||
Kepler-375b | 0.129 | 12.125934 | 0.101 | transit | 4180±180 | 0.89 | 5826 | [38] | ||
Kepler-375c | 0.236 | 19.986326 | 0.141 | transit | 4180±180 | 0.89 | 5826 | [38] | ||
Kepler-376b | 0.095 | 4.920199 | 0.057 | transit | 3090±50 | 1.05 | 5900 | [38] | ||
Kepler-376c | 0.16 | 14.172327 | 0.115 | transit | 3090±50 | 1.05 | 5900 | [38] | ||
Kepler-377b | 0.124 | 12.509529 | 0.109 | transit | 2750±40 | 0.88 | 5949 | [38] | ||
Kepler-377c | 0.184 | 27.014976 | 0.182 | transit | 2750±40 | 0.88 | 5949 | [38] | ||
Kepler-378b | 0.067 | 16.092361 | 0.112 | transit | 498.3±1.4 | 0.96 | 4661 | [38] | ||
Kepler-378c | 0.062 | 28.906009 | 0.166 | transit | 498.3±1.4 | 0.96 | 4661 | [38] | ||
Kepler-379b | 0.148 | 20.09838 | 0.152 | transit | 2430±20 | 1.08 | 6054 | [38] | ||
Kepler-379c | 0.204 | 62.784697 | 0.326 | transit | 2430±20 | 1.08 | 6054 | [38] | ||
Kepler-380b | 0.106 | 3.930821 | 0.05 | transit | 2710±40 | 1.05 | 6045 | [38] | ||
Kepler-380c | 0.113 | 7.630004 | 0.078 | transit | 2710±40 | 1.05 | 6045 | [38] | ||
Kepler-381b | 0.088 | 5.629021 | 0.066 | transit | 878±5 | 1.34 | 6152 | [38] | ||
Kepler-381c | 0.1 | 13.391635 | 0.117 | transit | 878±5 | 1.34 | 6152 | [38] | ||
Kepler-382b | 0.118 | 5.262155 | 0.055 | transit | 3130±60 | 0.8 | 5600 | [38] | ||
Kepler-382c | 0.142 | 12.162701 | 0.097 | transit | 3130±60 | 0.8 | 5600 | [38] | ||
Kepler-383b | 0.118 | 12.904532 | 0.095 | transit | 1695 | 0.67 | 4710 | [38] | ||
Kepler-383c | 0.111 | 31.200751 | 0.172 | transit | 1695 | 0.67 | 4710 | [38] | ||
Kepler-384b | 0.1 | 22.597053 | 0.148 | transit | 2990±30 | 0.76 | 5577 | [38] | ||
Kepler-384c | 0.101 | 45.348269 | 0.236 | transit | 2990±30 | 0.76 | 5577 | [38] | ||
Kepler-385b | 0.244 | 10.043686 | 0.097 | transit | 4870±160 | 1.09 | 6326 | [38] | ||
Kepler-385c | 0.271 | 15.163161 | 0.127 | transit | 4870±160 | 1.09 | 6326 | [38] | ||
Kepler-386b | 0.124 | 12.31043 | 0.096 | transit | 2950±90 | 0.74 | 5178 | [38] | ||
Kepler-386c | 0.141 | 25.193458 | 0.155 | transit | 2950±90 | 0.74 | 5178 | [38] | ||
Kepler-387b | 0.092 | 6.791636 | 0.068 | transit | 2670±30 | 1.03 | 5774 | [38] | ||
Kepler-387c | 0.079 | 11.837549 | 0.098 | transit | 2670±30 | 1.03 | 5774 | [38] | ||
Kepler-388b | 0.072 | 3.173315 | 0.036 | transit | 2000±200 | 0.59 | 4498 | [38] | ||
Kepler-388c | 0.077 | 13.297004 | 0.093 | transit | 2000±200 | 0.59 | 4498 | [38] | ||
Kepler-389b | 0.135 | 3.244107 | 0.041 | transit | 2720±70 | 0.78 | 5376 | [38] | ||
Kepler-389c | 0.13 | 14.51143 | 0.11 | transit | 2720±70 | 0.78 | 5376 | [38] | ||
Kepler-390b | 0.073 | 6.738088 | 0.065 | transit | 1437±12 | 0.67 | 5166 | [38] | ||
Kepler-390c | 0.07 | 13.060022 | 0.101 | transit | 1437±12 | 0.67 | 5166 | [38] | ||
Kepler-391b | 0.285 | 7.416755 | 0.082 | transit | 2900±40 | 1.22 | 4940 | [38] | ||
Kepler-391c | 0.316 | 20.485435 | 0.161 | transit | 2900±40 | 1.22 | 4940 | [38] | ||
Kepler-392b | 0.089 | 5.341853 | 0.059 | transit | 2260±20 | 1.13 | 5938 | [38] | ||
Kepler-392c | 0.098 | 10.423118 | 0.093 | transit | 2260±20 | 1.13 | 5938 | [38] | ||
Kepler-393b | 0.115 | 9.182417 | 0.091 | transit | 2940±40 | 1.32 | 6189 | [38] | ||
Kepler-393c | 0.119 | 14.613612 | 0.124 | transit | 2940±40 | 1.32 | 6189 | [38] | ||
Kepler-394b | 0.143 | 8.005013 | 0.083 | transit | 3560±80 | 1.11 | 6402 | [38] | ||
Kepler-394c | 0.148 | 12.130686 | 0.11 | transit | 3560±80 | 1.11 | 6402 | [38] | ||
Kepler-395b | 0.092 | 7.054346 | 0.061 | transit | 1390±20 | 0.53 | 4262 | [38] | ||
Kepler-395c | 0.118 | 34.989262 | 0.177 | transit | 1390±20 | 0.53 | 4262 | Potentially habitable exoplanet[38] | ||
Kepler-397b | 0.219 | 22.250949 | 0.144 | transit | 3760 | 5307 | [38] | |||
Kepler-397c | 0.551 | 135.498527 | 0.48 | transit | 3760 | 5307 | [38] | |||
Kepler-398b | 0.083 | 4.081423 | 0.044 | transit | 581.4±1.8 | 4493 | [38] | |||
Kepler-398c | 0.09 | 11.419412 | 0.087 | transit | 581.4±1.8 | 4493 | [38] | |||
Kepler-399b | 0.086 | 14.425281 | 0.103 | transit | 4400±700 | 5502 | [38] | |||
Kepler-399c | 0.128 | 26.67569 | 0.155 | transit | 4400±700 | 5502 | [38] | |||
Kepler-399d | 0.169 | 58.034616 | 0.261 | transit | 4400±700 | 5502 | [38] | |||
Kepler-400b | 0.147 | 9.024389 | 0.087 | transit | 2340 | 5886 | [38] | |||
Kepler-400c | 0.133 | 17.340824 | 0.134 | transit | 2340 | 5886 | [38] | |||
Kepler-401b | 0.153 | 14.383035 | 0.122 | transit | 3230±50 | 6117 | [38] | |||
Kepler-401c | 0.192 | 47.318218 | 0.269 | transit | 3230±50 | 6117 | [38] | |||
Kepler-402b | 0.109 | 4.028751 | 0.051 | transit | 2070±20 | 6090 | [38] | |||
Kepler-402c | 0.139 | 6.124821 | 0.068 | transit | 2070±20 | 6090 | [38] | |||
Kepler-402d | 0.123 | 8.921099 | 0.087 | transit | 2070±20 | 6090 | [38] | |||
Kepler-402e | 0.13 | 11.242861 | 0.102 | transit | 2070±20 | 6090 | [38] | |||
Kepler-403b | 0.112 | 7.031462 | 0.076 | transit | 2800±50 | 6090 | [38] | |||
Kepler-403c | 0.156 | 54.280749 | 0.297 | transit | 2800±50 | 6090 | [38] | |||
Kepler-404b | 0.113 | 11.829851 | 0.102 | transit | 2710±40 | 5654 | [38] | |||
Kepler-404c | 0.153 | 14.751166 | 0.118 | transit | 2710±40 | 5654 | [38] | |||
Kepler-405b | 0.186 | 10.613839 | 0.095 | transit | 3570±140 | 5818 | [38] | |||
Kepler-405c | 0.416 | 29.726682 | 0.188 | transit | 3570±140 | 5818 | [38] | |||
Kepler-406b | 0.02 | 0.128 | 2.42629 | transit | 1199±11 | 1.07 | 5538 | [39] | ||
Kepler-406c | 0.009 | 0.076 | 4.62332 | transit | 1199±11 | 1.07 | 5538 | [39] | ||
Kepler-407b | 0.095 | 0.66931 | transit | 1114±8 | 1 | 5476 | [39] | |||
Kepler-407c | 12.6 | 3000 | radial vel. | 1114±8 | 1 | 5476 | [39] | |||
Kepler-408b | 0.073 | 2.46502 | transit | 290.3±0.9 | 1.08 | 6104 | Host star known as HD 176693 or KOI-1612. Reported as 2.1% false positive probable in 2014,[39] but confirmed by 2016.[41] | |||
Kepler-409b | 0.106 | 68.9584 | transit | 222.8±0.3 | 0.92 | 5460 | Host star known as Gliese 409[39] | |||
Kepler-412b | 0.941 | 1.341 | 1.7208604 | 0.02897 | transit | 3650±60 | 1.17 | 5750 | [42] | |
Kepler-413b | 0.211 | 0.388 | 66.262 | 0.3553 | transit | 2830±70 | 0.82 | 4700 | [43] | |
Kepler-414b | 0.011 | 0.153 | 4.7 | timing | 1364±9 | 0.89 | [44] | |||
Kepler-414c | 0.094 | 0.269 | 7.171 | timing | 1364±9 | 0.89 | [44] | |||
Kepler-415b | 0.377 | 0.108 | 4.176 | timing | 1750±30 | 0.67 | [44] | |||
Kepler-415c | 8.708 | transit | 1750±30 | 0.67 | ? | |||||
Kepler-416b | 0.183 | 0.221 | 6.319 | timing | 2290±30 | 1 | [44] | |||
Kepler-416c | 12.209 | transit | 2290±30 | 1 | ? | |||||
Kepler-417b | 0.035 | 0.206 | 12.331 | transit | 3250±150 | 0.9 | [44] | |||
Kepler-417c | 15.943 | transit | 3250±150 | 0.9 | ? | |||||
Kepler-418b | 1.1 | 1.2 | 86.67856 | transit | 3360±60 | 0.98 | 5820 | [45] | ||
Kepler-419b | 2.5 | 0.96 | 69.7546 | 0.37 | transit | 3390±80 | 1.39 | 6430 | [46] | |
Kepler-419c | 7.3 | 675.47 | 1.68 | timing | 3390±80 | 1.39 | 6430 | [46] | ||
Kepler-420Ab | 1.45 | 0.94 | 86.647661 | 0.382 | 511 | transit | 2900 | 0.99 | 5520 | [47] |
Kepler-421b | 0.371 | 704.1984 | 1.219 | transit | 1148±6 | 0.79 | 5308 | [48] | ||
Kepler-422b | 0.43 | 1.15 | 7.8914483 | 0.082 | transit | 2400±20 | 1.15 | 5972 | [49] | |
Kepler-423b | 0.595 | 1.192 | 2.6843285 | 0.03585 | 1605 | transit | 2520±40 | 0.85 | 5560 | [49] |
Kepler-424b | 1.03 | 0.89 | 3.3118644 | 0.044 | transit | 2320±30 | 1.01 | 5460 | [49] | |
Kepler-424c | 6.97 | 223.3 | 0.73 | radial vel. | 2320±30 | 1.01 | 5460 | [49] | ||
Kepler-425b | 0.25 | 0.978 | 3.79701816 | 0.0464 | 1070 | transit | 2140±30 | 0.93 | 5170 | [50] |
Kepler-426b | 0.34 | 1.09 | 3.21751883 | 0.0414 | 1300 | transit | 2810±40 | 0.91 | 5725 | [50] |
Kepler-427b | 0.29 | 1.23 | 10.290994 | 0.091 | 1100 | transit | 3410±50 | 0.96 | 5800 | [50] |
Kepler-428b | 1.27 | 1.08 | 3.52563254 | 0.0433 | 1070 | transit | 2280±50 | 0.87 | 5150 | [50] |
Kepler-430b | 0.29 | 35.968 | 0.2244 | 667 | transit | 3070±50 | 1.17 | 5884 | [51] | |
Kepler-430c | 0.16 | 110.979 | 0.4757 | 458 | transit | 3070±50 | 1.17 | 5884 | [51] | |
Kepler-431b | 0.068 | 6.803 | 0.0719 | 1032 | transit | 1609±15 | 1.07 | 6004 | [51] | |
Kepler-431c | 0.06 | 8.703 | 0.0847 | 951 | transit | 1609±15 | 1.07 | 6004 | [51] | |
Kepler-431d | 0.1 | 11.922 | 0.1045 | 856 | transit | 1609±15 | 1.07 | 6004 | [51] | |
Kepler-432b | 5.41 | 1.145 | 52.501129 | 0.301 | transit | 2830±60 | 1.32 | 4995 | Eccentric orbit[52] | |
Kepler-432c | 2.43+0.22 −0.24 |
406.2+3.9 −2.5 |
radial vel. | 2830±60 | 1.32 | 4995 | [52] | |||
Kepler-453b | 0.00063 | 0.553 | 240.503 | 0.7903 | transit | 1463±9 | 0.94 | 5527 | [53] | |
Mu Leonis b | 2.4 | 357.8 | 1.1 | radial vel. | 133.0 | 1.5 | 4538.2 | [3] | ||
OGLE-2008-BLG-355Lb | 4.6 | 1.7 | microlensing | 22000 | 0.37 | [54] | ||||
OGLE-2008-BLG-92Lb | 0.18 | 18 | microlensing | 26000 | 0.71 | [55] | ||||
OGLE-2011-BLG-265Lb | 0.88 | 1.89 | microlensing | 14300 | 0.21 | [56] | ||||
OGLE-2013-BLG-102Lb | 12.569 | 0.8 | microlensing | 9900 | 0.1 | Additional planet or brown dwarf in the system.[57] | ||||
OGLE-2013-BLG-341LBb | 0.0073 | 0.883 | microlensing | 3790 | 0.15 | One more red dwarf in the system.[58] | ||||
OGLE-2014-BLG-0124Lb | 0.51 | 3.11 | microlensing | 13000 | 0.71 | [59] | ||||
SAND364 b | 1.54 | 121.71 | radial vel. | 2730±130 | 1.35 | 4284 | Belongs to Messier 67, also known as BD+12 1917b[60] | |||
TYC 1422-614-1 b | 2.5 | 198.4 | 0.69 | radial vel. | 2480 | 1.15 | 4806 | [61] | ||
TYC 1422-614-1 c | 10 | 559.3 | 1.37 | radial vel. | 2480 | 1.15 | 4806 | [61] | ||
WASP-20 A b | 0.72±0,06 | 1.32±0.03 | 3.16158 | 0.04317 | transit | 663.39 | 1.05 | 5990 | Binary with planet orbiting primary star[62][63] | |
WASP-74b | 0.95 | 1.56 | 2.13775 | 0.037 | 1910 | transit | 390 | 1.48 | 5970 | [64] |
WASP-83b | 0.3 | 1.04 | 4.971252 | 0.059 | 1120 | transit | 980 | 1.11 | 5510 | [64] |
WASP-85Ab | 1.265 | 1.24 | 2.6556777 | 0.039 | 1452 | transit | 243 | 1.09 | 6112 | [65] |
WASP-87 b | 2.18±0.15 | 1.39±0.06 | 1.6828 | 0.0295±0.0008 | transit | 982±12 | 1.20±0.09 | 6450±120 | [66] Host star also known as CD-52 4998. | |
WASP-89b | 5.9 | 1.04 | 3.3564227 | 0.0427 | 1120 | transit | 957 | 0.92 | 5130 | [64] |
WASP-94Ab | 0.452 | 1.72 | 3.9501907 | 0.055 | 1604 | transit | 590 | 1.45 | 6153 | [67] |
WASP-94Bb | 0.618 | 2.00839 | 0.0335 | radial vel. | 590 | 1.24 | 6040 | [67] | ||
WASP-103b | 1.49 | 1.528 | 0.925542 | 0.01985 | 2508 | transit | 1500 | 1.22 | 6110 | Planet close to tidal disruption[68][69] |
WASP-104b | 1.272 | 1.137 | 1.7554137 | 0.02918 | 1516 | transit | 470 | 1.08 | 5475 | [70] |
WASP-106b | 1.925 | 1.085 | 9.289715 | 0.0917 | 1140 | transit | 920 | 1.19 | 6055 | [70] |
WASP-108 b | 1.167+0.092 −0.091 |
1.215±0.040 | 2.6755463±0.0000021 | 0.0397±0.001 | 1590 | transit | 717.6±0.3 | 1.167±0.092 | 6000±140 | [66] Host star also known as TYC 8254-1624-1 |
WASP-109 b | 0.91±0.13 | 1.443±0.053 | 3.3190233±0.0000042 | 0.0463±0.0011 | 1695 | transit | 1173±16 | 1.203±0.090 | 6520±140 | [66] Host star also known as TYC 6184-1397-1 |
WASP-110 b | 0.515±0.064 | 1.238±0.056 | 3.7783977±0.0000031 | 0.0457±0.0012 | 1134 | transit | 904±10 | 0.892±0.072 | 5400±140 | [66] |
WASP-111 b | 1.85±0.16 | 1.442±0.094 | 2.310965±0.0000034 | 0.03914±0.00098 | 2140 | transit | 980±20 | 1.50±0.11 | 6400±150 | [66] Host star also known as HD 208180 |
WASP-112 b | 0.88±0.12 | 1.191±0.049 | 3.0353992±0.0000038 | 0.0382±0.0011 | 1395 | transit | 1900±40 | 0.807±0.073 | 5610±130 | [66] |
WASP-116b | 0.59±0.05 | 1.43±0.07 | 6.61321±0.00002 | 0.0730±0.0011 | 1400±4 | transit | 1770±60 | 1.25±0.18 | 5950±100 | [65] |
WASP-117b | 0.2755 | 1.021 | 10.02165 | 0.09459 | 1024 | transit | 518±2 | 1.13 | 6038 | [71][72] |
WASP-149b | 1.02±0.04 | 1.32±0.04 | 1.332811±0.000001 | 0.0247±0.0004 | 1870±1 | transit | 1770±60 | 1.12±0.17 | 5750±100 | [65] |
XO-2Sb | 0.259 | 18.157 | 0.1344 | radial vel. | 480 | 0.98 | 5399 | [73] | ||
XO-2Sc | 1.37 | 120.8 | 0.4756 | radial vel. | 480 | 0.98 | 5399 | [73] | ||
YBP 1194 b | 0.32 | 6.959 | radial vel. | 2920±100 | 1.01 | 5780 | Belongs to Messier 67[60] | |||
YBP 1514 b | 0.4 | 5.118 | radial vel. | 3060±100 | 0.96 | 5725 | Belongs to Messier 67[60] |
Specific exoplanet lists
- List of directly imaged exoplanets
- List of exoplanet extremes
- List of exoplanet firsts
- List of exoplanets discovered by the Kepler space telescope
- List of exoplanets observed during Kepler's K2 mission
- List of extrasolar candidates for liquid water
- List of hottest exoplanets
- List of coolest exoplanets
- List of multiplanetary systems
- List of nearest exoplanets
- List of nearest terrestrial exoplanet candidates
- List of potentially habitable exoplanets
- List of proper names of exoplanets
- List of smallest exoplanets
- List of transiting exoplanets
Lists of exoplanet by year of discovery
- List of exoplanets discovered before 2000 (31)
- List of exoplanets discovered between 2000–2009 (379)
- List of exoplanets discovered in 2010 (109)
- List of exoplanets discovered in 2011 (179)
- List of exoplanets discovered in 2012 (149)
- List of exoplanets discovered in 2013 (151)
- List of exoplanets discovered in 2014 (878)
- List of exoplanets discovered in 2015 (151)
- List of exoplanets discovered in 2016 (1513)
- List of exoplanets discovered in 2017 (158)
- List of exoplanets discovered in 2018 (306)
- List of exoplanets discovered in 2019 (172)
- List of exoplanets discovered in 2020 (255)
- List of exoplanets discovered in 2021 (257)
- List of exoplanets discovered in 2022 (315)
- List of exoplanets discovered in 2023 (289)
- List of exoplanets discovered in 2024 (11)
References
- ↑ "The Extrasolar Planets Encyclopaedia". Extrasolar Planets Encyclopaedia. 1995. Retrieved 2015-11-09.
- 1 2 3 4 5 Moutou, C.; Lo Curto, G.; Mayor, M.; Bouchy, F.; Benz, W.; Lovis, C.; Naef, D.; Pepe, F.; Queloz, D.; Santos, N. C.; Ségransan, D.; Sousa, S. G.; Udry, S. (2014), "The HARPS search for southern extra-solar planets XXXVI: Five new long-period giant planets and a system update", Astronomy & Astrophysics, 576: A48, arXiv:1412.6591, doi:10.1051/0004-6361/201424965, S2CID 118512899
- 1 2 3 Lee, B.-C.; et al. (2014). "Planetary Companions in K giants β Cancri, μ Leonis, and β Ursae Minoris". Astronomy & Astrophysics. 566: 7. arXiv:1405.2127. Bibcode:2014A&A...566A..67L. doi:10.1051/0004-6361/201322608. S2CID 118631934. A67.
- ↑ Moutou, C.; et al. (2014), "CoRoT-22 b: A validated 4.9 R⊕ exoplanet in 10-d orbit★†", Monthly Notices of the Royal Astronomical Society, 444 (3): 2783–2792, arXiv:1408.2576, doi:10.1093/mnras/stu1645
- 1 2 Alonso, R.; et al. (2014), "Transiting exoplanets from the CoRoT space mission", Astronomy & Astrophysics, 567: A112, arXiv:1406.1270, doi:10.1051/0004-6361/201118662, S2CID 96458405
- ↑ Parviainen, H.; et al. (2014), "Transiting exoplanets from the CoRoT space mission", Astronomy & Astrophysics, 562: A140, arXiv:1401.1122, doi:10.1051/0004-6361/201323049, S2CID 46747735
- ↑ Raetz, St; Heras, A. M.; Fernández, M.; Casanova, V.; Marka, C. (2018), "Transit analysis of the CoRoT-5, CoRoT-8, CoRoT-12, CoRoT-18, CoRoT-20, and CoRoT-27 systems with combined ground- and space-based photometry", Monthly Notices of the Royal Astronomical Society, 483: 824–839, arXiv:1812.01536, doi:10.1093/mnras/sty3085
- ↑ Howard, Andrew W.; Marcy, Geoffrey W.; Fischer, Debra A.; Isaacson, Howard; Muirhead, Philip S.; Henry, Gregory W.; Boyajian, Tabetha S.; von Braun, Kaspar; Becker, Juliette C.; Wright, Jason T.; Johnson, John Asher (2014), "The Nasa-Uc-Uh Eta-Earth Program. Iv. A Low-Mass Planet Orbiting an M Dwarf 3.6 Pc from Earth", The Astrophysical Journal, 794 (1): 51, arXiv:1408.5645, Bibcode:2014ApJ...794...51H, doi:10.1088/0004-637X/794/1/51, S2CID 17361592
- 1 2 3 4 5 6 7 8 9 Tuomi, Mikko; Jones, Hugh R. A.; Barnes, John R.; Anglada-Escudé, Guillem; Jenkins, James S. (2014), "Bayesian search for low-mass planets around nearby M dwarfs – estimates for occurrence rate based on global detectability statistics", Monthly Notices of the Royal Astronomical Society, 441 (2): 1545–1569, arXiv:1403.0430, doi:10.1093/mnras/stu358
- 1 2 3 Feng, Fabo; Butler, R. Paul; Shectman, Stephen A.; Crane, Jeffrey D.; Vogt, Steve; Chambers, John; Jones, Hugh R. A.; Wang, Sharon Xuesong; Teske, Johanna K.; Burt, Jenn; Díaz, Matías R.; Thompson, Ian B. (8 January 2020). "Search for Nearby Earth Analogs. II. Detection of Five New Planets, Eight Planet Candidates, and Confirmation of Three Planets around Nine Nearby M Dwarfs". The Astrophysical Journal Supplement Series. 246 (1): 11. arXiv:2001.02577. Bibcode:2020ApJS..246...11F. doi:10.3847/1538-4365/ab5e7c. S2CID 210064560.
- ↑ Feng, Fabo; Butler, R. Paul; Shectman, Stephen A.; Crane, Jeffrey D.; Vogt, Steve; Chambers, John; Jones, Hugh R. A.; Wang, Sharon Xuesong; Teske, Johanna K.; Burt, Jenn; Díaz, Matías R.; Thompson, Ian B. (2020-01-08). "Search for Nearby Earth Analogs. II. Detection of Five New Planets, Eight Planet Candidates, and Confirmation of Three Planets around Nine Nearby M Dwarfs". The Astrophysical Journal Supplement Series. 246 (1): 11. arXiv:2001.02577. Bibcode:2020ApJS..246...11F. doi:10.3847/1538-4365/ab5e7c. ISSN 1538-4365.
- ↑ Burt, Jennifer; Vogt, Steven S.; Butler, R. Paul; Hanson, Russell; Meschiari, Stefano; Rivera, Eugenio J.; Henry, Gregory W.; Laughlin, Gregory (2014). "The Lick–Carnegie exoplanet survey: Gliese 687 b: A Neptune-mass planet orbiting a nearby red dwarf". The Astrophysical Journal. 789 (2): 114. arXiv:1405.2929. Bibcode:2014ApJ...789..114B. doi:10.1088/0004-637X/789/2/114. S2CID 17668957.
- ↑ Wittenmyer, R. A.; et al. (August 2014). "GJ 832c: A super-earth in the habitable zone". The Astrophysical Journal. 791 (2): 114. arXiv:1406.5587. Bibcode:2014ApJ...791..114W. doi:10.1088/0004-637X/791/2/114. S2CID 12157837. 114.
- ↑ Gorrini, P.; Astudillo-Defru, N.; Dreizler, S.; Damasso, M.; Díaz, R. F.; Bonfils, X.; Jeffers, S. V.; Barnes, J. R.; Del Sordo, F.; Almenara, J.-M.; Artigau, E.; Bouchy, F.; Charbonneau, D.; Delfosse, X.; Doyon, R.; Figueira, P.; Forveille, T.; Haswell, C. A.; López-González, M. J.; Melo, C.; Mennickent, R. E.; Gaisné, G.; Morales, N. Morales; Murgas, F.; Pepe, F.; Rodríguez, E.; Santos, N. C.; Tal-Or, L.; Tsapras, Y.; Udry, S. (2022), "Detailed stellar activity analysis and modelling of GJ 832", Astronomy & Astrophysics, 664: A64, arXiv:2206.07552, doi:10.1051/0004-6361/202243063, S2CID 249674385
- 1 2 3 Astudillo-Defru, Nicola; Bonfils, Xavier; Delfosse, Xavier; Ségransan, Damien; Forveille, Thierry; Bouchy, François; Gillon, Michaël; Lovis, Christophe; Mayor, Michel; Neves, Vasco; Pepe, Francesco; Perrier, Christian; Queloz, Didier; Rojo, Patricio; Santos, Nuno C.; Udry, Stéphane (2015). "Planetary systems and stellar activity of the M dwarfs GJ 3293, GJ 3341, and GJ 3543". Astronomy & Astrophysics. 575: A119. arXiv:1411.7048v1. Bibcode:2015A&A...575A.119A. doi:10.1051/0004-6361/201424253. S2CID 67754095.
- ↑ Marie-Eve Naud; Étienne Artigau; Lison Malo; Loïc Albert; René Doyon; David Lafrenière; Jonathan Gagné; Didier Saumon; Caroline V. Morley; France Allard; Derek Homeier; Charles A. Beichman; Christopher R. Gelino; Anne Boucher (12 May 2014). "Discovery of a Wide Planetary-mass Companion to the Young M3 Star GU Psc". The Astrophysical Journal (published May 2014). 787 (1): 16. arXiv:1405.2932. Bibcode:2014ApJ...787....5N. doi:10.1088/0004-637X/787/1/5. S2CID 35264096. 5.
- ↑ Bieryla, A.; Hartman, J. D.; Bakos, G. Á.; Bhatti, W.; Kovács, G.; Boisse, I.; Latham, D. W.; Buchhave, L. A.; Csubry, Z.; Penev, K.; De Val-Borro, M.; Béky, B.; Falco, E.; Torres, G.; Noyes, R. W.; Berlind, P.; Calkins, M. C.; Esquerdo, G. A.; Lázár, J.; Papp, I.; Sári, P. (2014), "HAT-P-49b: A 1.7MJPLANET TRANSITING a BRIGHT 1.5M☉F-STAR", The Astronomical Journal, 147 (4): 84, arXiv:1401.5460, Bibcode:2014AJ....147...84B, doi:10.1088/0004-6256/147/4/84, S2CID 119265999
- ↑ Bakos, G. Á.; Hartman, J. D.; Bhatti, W.; Bieryla, A.; Val-Borro, M. de; Latham, D. W.; Buchhave, L. A.; Csubry, Z.; Penev, K.; Kovács, G.; Béky, B.; Falco, E.; Kovács, T.; Howard, A. W.; Johnson, J. A.; Isaacson, H.; Marcy, G. W.; Torres, G.; Noyes, R. W.; Berlind, P.; Calkins, M. L.; Esquerdo, G. A.; Lázár, J.; Papp, I.; Sári, P. (2014), "HAT-P-54b: A HOT JUPITER TRANSITING a 0.64M⊙STAR IN FIELD 0 OF THE K2 MISSION", The Astronomical Journal, 149 (4): 149, arXiv:1404.4417, doi:10.1088/0004-6256/149/4/149, S2CID 119239193
- ↑ Crossfield, Ian J. M.; et al. (2021), "197 CANDIDATES AND 104 VALIDATED PLANETS IN K2 's FIRST FIVE FIELDS", The Astrophysical Journal Supplement Series, 226: 7, arXiv:1607.05263, doi:10.3847/0067-0049/226/1/7, S2CID 56125109
- ↑ Saha, Suman; Chakrabarty, Aritra; Sengupta, Sujan (2021), "Multiband Transit Follow-up Observations of Five Hot Jupiters with Critical Noise Treatments: Improved Physical Properties", The Astronomical Journal, 162 (1): 18, arXiv:2105.09668, Bibcode:2021AJ....162...18S, doi:10.3847/1538-3881/ac01dd, S2CID 234790451
- ↑ Jordán, Andrés; et al. (2014), "HATS-4b: A DENSE HOT JUPITER TRANSITING a SUPER METAL-RICH G STAR", The Astronomical Journal, 148 (2): 29, arXiv:1402.6546, Bibcode:2014AJ....148...29J, doi:10.1088/0004-6256/148/2/29, S2CID 119189535
- ↑ Zhou, G.; Bayliss, D.; Penev, K.; Bakos, G. Á.; Hartman, J. D.; Jordán, A.; Mancini, L.; Mohler, M.; Csubry, Z.; Ciceri, S.; Brahm, R.; Rabus, M.; Buchhave, L.; Henning, T.; Suc, V.; Espinoza, N.; Béky, B.; Noyes, R. W.; Schmidt, B.; Butler, R. P.; Shectman, S.; Thompson, I.; Crane, J.; Sato, B.; Csák, B.; Lázár, J.; Papp, I.; Sári, P.; Nikolov, N. (2014), "HATS-5b: A TRANSITING HOT SATURN FROM THE HATSouth SURVEY", The Astronomical Journal, 147 (6): 144, arXiv:1401.1582, Bibcode:2014AJ....147..144Z, doi:10.1088/0004-6256/147/6/144, S2CID 118654298
- ↑ Hartman, J. D.; Bayliss, D.; Brahm, R.; Bakos, G. Á.; Mancini, L.; Jordán, A.; Penev, K.; Rabus, M.; Zhou, G.; Butler, R. P.; Espinoza, N.; De Val-Borro, M.; Bhatti, W.; Csubry, Z.; Ciceri, S.; Henning, T.; Schmidt, B.; Arriagada, P.; Shectman, S.; Crane, J.; Thompson, I.; Suc, V.; Csák, B.; Tan, T. G.; Noyes, R. W.; Lázár, J.; Papp, I.; Sári, P. (2014), "HATS-6b: A WARM SATURN TRANSITING AN EARLY M DWARF STAR, AND a SET OF EMPIRICAL RELATIONS FOR CHARACTERIZING K AND M DWARF PLANET HOSTS", The Astronomical Journal, 149 (5): 166, arXiv:1408.1758, doi:10.1088/0004-6256/149/5/166, S2CID 119286461
- ↑ Kane, Stephen R.; et al. (April 2014). "Limits on Stellar Companions to Exoplanet Host Stars with Eccentric Planets". The Astrophysical Journal. 785 (2): 10. arXiv:1401.1544. Bibcode:2014ApJ...785...93K. doi:10.1088/0004-637X/785/2/93. S2CID 2053475. 93.
- 1 2 3 4 Giguere, Matthew J.; et al. (2015). "Newly Discovered Planets Orbiting HD 5319, HD 11506, HD 75784 and HD 10442 from the N2K Consortium". The Astrophysical Journal. 799 (1). 89. arXiv:1411.5374. Bibcode:2015ApJ...799...89G. doi:10.1088/0004-637X/799/1/89. S2CID 56121568.
- ↑ Wang, Liang; Sato, Bun'ei; Omiya, Masashi; Harakawa, Hiroki; Liu, Yujuan; Song, Nan; He, Wei; Wu, Xiaoshu; Izumiura, Hideyuki; Kambe, Eiji; Takeda, Yoichi; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro; Ida, Shigeru; Zhao, Gang (2014), "A long-period eccentric substellar companion to the evolved intermediate-mass star HD 14067", Publications of the Astronomical Society of Japan, 66 (6): 118, arXiv:1409.6081, doi:10.1093/pasj/psu113
- ↑ Acke, B.; van den Ancker, M. E. (16 March 2006). "Resolving the disk rotation of HD 97048 and HD 100546 in the [O I] 6300 Å line: evidence for a giant planet orbiting HD 100546". Astronomy & Astrophysics. 449 (1): 267–279. arXiv:astro-ph/0512562. Bibcode:2006A&A...449..267A. doi:10.1051/0004-6361:20054330. S2CID 10148216.
- 1 2 Wittenmyer, Robert A.; et al. (2014). "The Anglo-Australian Planet Search. XXIII. Two New Jupiter Analogs". The Astrophysical Journal. 783 (2): 103. arXiv:1401.5525. Bibcode:2014ApJ...783..103W. doi:10.1088/0004-637X/783/2/103. S2CID 14082923.
- 1 2 3 4 Vogt, Steven S.; Butler, R. Paul; Rivera, Eugenio J.; Kibrick, Robert; Burt, Jennifer; Hanson, Russell; Meschiari, Stefano; Henry, Gregory W.; Laughlin, Gregory (2014), "A Four-Planet System Orbiting the K0V Star Hd 141399", The Astrophysical Journal, 787 (2): 97, arXiv:1404.7462, Bibcode:2014ApJ...787...97V, doi:10.1088/0004-637X/787/2/97, S2CID 10477331
- 1 2 Jones, M. I.; Jenkins, J. S.; Rojo, P.; Melo, C. H. F.; Bluhm, P. (2015), "A planetary system and a highly eccentric brown dwarf around the giant stars HIP 67851 and HIP 97233", Astronomy & Astrophysics, 573: A3, arXiv:1409.7429, Bibcode:2015A&A...573A...3J, doi:10.1051/0004-6361/201424771, S2CID 53638707
- ↑ Wittenmyer, Robert A.; Wang, Liang; Liu, Fan; Horner, Jonathan; Endl, Michael; Johnson, John Asher; Tinney, C. G.; Carter, B. D. (2014), "The Pan-Pacific Planet Search. Ii. Confirmation of a Two-Planet System Around Hd 121056", The Astrophysical Journal, 800: 74, arXiv:1412.6889, doi:10.1088/0004-637X/800/1/74, S2CID 53684180
- ↑ Jones, M. I.; Jenkins, J. S.; Bluhm, P.; Rojo, P.; Melo, C. H. F. (2014), "The properties of planets around giant stars", Astronomy & Astrophysics, 566: A113, arXiv:1406.0884, Bibcode:2014A&A...566A.113J, doi:10.1051/0004-6361/201323345, S2CID 118396750
- ↑ Vanderburg, Andrew; et al. (February 2015). "Characterizing K2 Planet Discoveries: A super-Earth transiting the bright K-dwarf HIP 116454". The Astrophysical Journal. 800 (1). 59. arXiv:1412.5674. Bibcode:2015ApJ...800...59V. doi:10.1088/0004-637X/800/1/59.
- 1 2 Anglada-Escudé, Guillem; et al. (2014), "Two planets around Kapteyn's star : a cold and a temperate super-Earth orbiting the nearest halo red-dwarf", Monthly Notices of the Royal Astronomical Society: Letters, 443: L89–L93, arXiv:1406.0818, Bibcode:2014MNRAS.443L..89A, doi:10.1093/mnrasl/slu076, S2CID 67807856
- 1 2 Bortle, Anna; Fausey, Hallie; Ji, Jinbiao; Dodson-Robinson, Sarah; Ramirez Delgado, Victor; Gizis, John (2021), "A Gaussian Process Regression Reveals No Evidence for Planets Orbiting Kapteyn's Star", The Astronomical Journal, 161 (5): 230, arXiv:2103.02709, Bibcode:2021AJ....161..230B, doi:10.3847/1538-3881/abec89, S2CID 232110395
- 1 2 3 Silvotti, R.; Charpinet, S.; Green, E.; Fontaine, G.; Telting, J. H.; Østensen, R. H.; Van Grootel, V.; Baran, A. S.; Schuh, S.; Fox Machado, L. (2014), "Keplerdetection of a new extreme planetary system orbiting the subdwarf-B pulsator KIC 10001893", Astronomy & Astrophysics, 570: A130, arXiv:1409.6975, Bibcode:2014A&A...570A.130S, doi:10.1051/0004-6361/201424509, S2CID 46974308
- 1 2 3 Blokesz, A.; et al. (July 2019). "Analysis of putative exoplanetary signatures found in light curves of two sdBV stars observed by Kepler". Astronomy & Astrophysics. 627: A86. arXiv:1906.03321. Bibcode:2019A&A...627A..86B. doi:10.1051/0004-6361/201835003. S2CID 182952925.
- 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 60 61 62 63 64 65 66 67 68 69 70 71 72 73 74 75 76 77 78 79 80 81 82 83 84 85 86 87 88 89 90 91 92 93 94 95 96 97 98 99 100 101 102 103 104 105 106 107 108 109 110 111 112 113 114 115 116 117 118 119 120 121 122 123 124 125 126 127 128 129 130 131 132 133 134 135 136 137 138 139 140 141 142 143 144 145 146 147 148 149 150 151 152 153 154 155 156 157 158 159 160 161 162 163 164 165 166 167 168 169 170 171 172 173 174 175 176 177 178 179 180 181 182 183 184 185 186 187 188 189 190 191 192 193 194 195 196 197 198 199 200 201 202 203 204 205 206 207 208 209 210 211 212 213 214 215 216 217 218 219 220 221 222 223 224 225 226 227 228 229 230 231 232 233 234 235 236 237 238 239 240 241 242 243 244 245 246 247 248 249 250 251 252 253 254 255 256 257 258 259 260 261 262 263 264 265 266 267 268 269 270 271 272 273 274 275 276 277 278 279 280 281 282 283 284 285 286 287 288 289 290 291 292 293 294 295 296 297 298 299 300 301 302 303 304 305 306 307 308 309 310 311 312 313 314 315 316 317 318 319 320 321 322 323 324 325 326 327 328 329 330 331 332 333 334 335 336 337 338 339 340 341 342 343 344 345 346 347 348 349 350 351 352 353 354 355 356 357 358 359 360 361 362 363 364 365 366 367 368 369 370 371 372 373 374 375 376 377 378 379 380 381 382 383 384 385 386 387 388 389 390 391 392 393 394 395 396 397 398 399 400 401 402 403 404 405 406 407 408 409 410 411 412 413 414 415 416 417 418 419 420 421 422 423 424 425 426 427 428 429 430 431 432 433 434 435 436 437 438 439 440 441 442 443 444 445 446 447 448 449 450 451 452 453 454 455 456 457 458 459 460 461 462 463 464 465 466 467 468 469 470 471 472 473 474 475 476 477 478 479 480 481 482 483 484 485 486 487 488 489 490 491 492 493 494 495 496 497 498 499 500 501 502 503 504 505 506 507 508 509 510 511 512 513 514 515 516 517 518 519 520 521 522 523 524 525 526 527 528 529 530 531 532 533 534 535 536 537 538 539 540 541 542 543 544 545 546 547 548 549 550 551 552 553 554 555 556 557 558 559 560 561 562 563 564 565 566 567 568 569 570 571 572 573 574 575 576 577 578 579 580 581 582 583 584 585 586 587 588 589 590 591 592 593 594 595 596 597 598 599 600 601 602 603 604 605 606 607 608 609 610 611 612 613 614 615 616 617 618 619 620 621 622 623 624 625 626 627 628 629 630 631 632 633 634 635 636 637 638 639 640 641 642 643 644 645 646 647 648 649 650 651 652 653 654 655 656 657 658 659 660 661 662 663 664 665 666 667 668 669 670 671 672 673 674 675 676 677 678 679 680 681 682 683 684 685 686 687 688 689 690 691 692 693 694 695 696 697 698 699 700 701 702 703 704 705 706 707 708 709 710 711 712 713 714 715 716 717 718 719 720 721 722 723 724 725 726 727 728 729 730 731 732 733 734 735 736 Rowe, Jason F.; Bryson, Stephen T.; Marcy, Geoffrey W.; Lissauer, Jack J.; Jontof-Hutter, Daniel; Mullally, Fergal; Gilliland, Ronald L.; Issacson, Howard; Ford, Eric; Howell, Steve B.; Borucki, William J.; Haas, Michael; Huber, Daniel; Steffen, Jason H.; Thompson, Susan E.; Quintana, Elisa; Barclay, Thomas; Still, Martin; Fortney, Jonathan; Gautier, T. N.; Hunter, Roger; Caldwell, Douglas A.; Ciardi, David R.; Devore, Edna; Cochran, William; Jenkins, Jon; Agol, Eric; Carter, Joshua A.; Geary, John (2014), "Validation Ofkepler's Multiple Planet Candidates. III. Light Curve Analysis and Announcement of Hundreds of New Multi-Planet Systems", The Astrophysical Journal, 784 (1): 45, arXiv:1402.6534, Bibcode:2014ApJ...784...45R, doi:10.1088/0004-637X/784/1/45, S2CID 119118620
- 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 Marcy, Geoffrey W.; et al. (2014), "Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets", The Astrophysical Journal Supplement Series, 210 (2): 20, arXiv:1401.4195, Bibcode:2014ApJS..210...20M, doi:10.1088/0067-0049/210/2/20, S2CID 10760418
- 1 2 Heller, René; Hippke, Michael; Freudenthal, Jantje; Rodenbeck, Kai; Batalha, Natalie M.; Bryson, Steve (2020). "Transit least-squares survey". Astronomy & Astrophysics. 638: A10. arXiv:2006.02123. doi:10.1051/0004-6361/201936929. S2CID 219260293.
- ↑ Campante, T. L.; Lund, M. N.; Kuszlewicz, J. S.; Davies, G. R.; Chaplin, W. J.; Albrecht, S.; Winn, J. N.; Bedding, T. R.; Benomar, O.; Bossini, D.; Handberg, R.; Santos, A. R. G.; Van Eylen, V.; Basu, S.; Christensen-Dalsgaard, J.; Elsworth, Y. P.; Hekker, S.; Hirano, T.; Huber, D.; Karoff, C.; Kjeldsen, H.; Lundkvist, M. S.; North, T. S. H.; Silva Aguirre, V.; Stello, D.; White, T. R. (2016), "Spin–Orbit Alignment of Exoplanet Systems: Ensemble Analysis Using Asteroseismology", The Astrophysical Journal, 819 (1): 85, arXiv:1601.06052, Bibcode:2016ApJ...819...85C, doi:10.3847/0004-637X/819/1/85, S2CID 56307453
- ↑ "SOPHIE velocimetry of Kepler transit candidates XI. Kepler-412 system: probing the properties of a new inflated hot Jupiter" (PDF). www.aanda.org.
- ↑ Kostov, V. B.; McCullough, P. R.; Carter, J. A.; Deleuil, M.; Díaz, R. F.; Fabrycky, D. C.; Hébrard, G.; Hinse, T. C.; Mazeh, T.; Orosz, J. A.; Tsvetanov, Z. I.; Welsh, W. F. (2014), "Kepler-413B: A Slightly Misaligned, Neptune-Size Transiting Circumbinary Planet", The Astrophysical Journal, 784 (1): 14, arXiv:1401.7275, Bibcode:2014ApJ...784...14K, doi:10.1088/0004-637X/784/1/14, S2CID 118418065
- 1 2 3 4 5 See Table 2. Planet Nominal Masses in Hadden, Sam; Lithwick, Yoram (2014). "Densities and Eccentricities of 139Keplerplanets from Transit Time Variations". The Astrophysical Journal. 787 (1): 80. arXiv:1310.7942. Bibcode:2014ApJ...787...80H. doi:10.1088/0004-637X/787/1/80. S2CID 119097836.
- ↑ Tingley, B.; Parviainen, H.; Gandolfi, D.; Deeg, H. J.; Palle, E.; Montañés Rodriguez, P.; Murgas, F.; Alonso, R.; Bruntt, H.; Fridlund, M. (2014), "Confirmation of an exoplanet using the transit color signature: Kepler-418b, a blended giant planet in a multiplanet system", Astronomy & Astrophysics, 567: A14, arXiv:1405.5354, Bibcode:2014A&A...567A..14T, doi:10.1051/0004-6361/201323175, S2CID 118668437
- 1 2 Dawson, Rebekah I.; Johnson, John Asher; Fabrycky, Daniel C.; Foreman-Mackey, Daniel; Murray-Clay, Ruth A.; Buchhave, Lars A.; Cargile, Phillip A.; Clubb, Kelsey I.; Fulton, Benjamin J.; Hebb, Leslie; Howard, Andrew W.; Huber, Daniel; Shporer, Avi; Valenti, Jeff A. (2014), "Large Eccentricity, Low Mutual Inclination: The Three-Dimensional Architecture of a Hierarchical System of Giant Planets", The Astrophysical Journal, 791 (2): 89, arXiv:1405.5229, Bibcode:2014ApJ...791...89D, doi:10.1088/0004-637X/791/2/89, S2CID 29630098
- ↑ Santerne, A.; et al. (2014), "SOPHIE velocimetry of Keplertransit candidates", Astronomy & Astrophysics, 571: A37, arXiv:1406.6172, doi:10.1051/0004-6361/201424158, S2CID 118582477
- ↑ Kipping, D. M.; Torres, G.; Buchhave, L. A.; Kenyon, S. J.; Henze, C.; Isaacson, H.; Kolbl, R.; Marcy, G. W.; Bryson, S. T.; Stassun, K.; Bastien, F. (2014), "Discovery of a Transiting Planet Near the Snow-Line", The Astrophysical Journal, 795 (1): 25, arXiv:1407.4807, Bibcode:2014ApJ...795...25K, doi:10.1088/0004-637X/795/1/25, S2CID 119240746
- 1 2 3 4 Endl, Michael; Caldwell, Douglas A.; Barclay, Thomas; Huber, Daniel; Isaacson, Howard; Buchhave, Lars A.; Brugamyer, Erik; Robertson, Paul; Cochran, William D.; MacQueen, Phillip J.; Havel, Mathieu; Lucas, Phillip; Howell, Steve B.; Fischer, Debra; Quintana, Elisa; Ciardi, David R. (2014), "KEPLER-424 b: A "LONELY" HOT JUPITER THAT FOUND a COMPANION", The Astrophysical Journal, 795 (2): 151, arXiv:1409.8156, Bibcode:2014ApJ...795..151E, doi:10.1088/0004-637X/795/2/151, S2CID 1274827
- 1 2 3 4 Hébrard, G.; Santerne, A.; Montagnier, G.; Bruno, G.; Deleuil, M.; Havel, M.; Almenara, J.-M.; Damiani, C.; Barros, S. C. C.; Bonomo, A. S.; Bouchy, F.; Díaz, R. F.; Moutou, C. (2014), "Characterization of the four new transiting planets KOI-188b, KOI-195b, KOI-192b, and KOI-830b", Astronomy & Astrophysics, 572: A93, arXiv:1409.8554, Bibcode:2014A&A...572A..93H, doi:10.1051/0004-6361/201424268, S2CID 119187433
- 1 2 3 4 5 Everett, Mark E.; Barclay, Thomas; Ciardi, David R.; Horch, Elliott P.; Howell, Steve B.; Crepp, Justin R.; Silva, David R. (2014), "High-Resolution Multi-Band Imaging for Validation and Characterization of Smallkeplerplanets", The Astronomical Journal, 149 (2): 55, arXiv:1411.3621, doi:10.1088/0004-6256/149/2/55, S2CID 32515106
- 1 2 Quinn, Samuel N.; White, Timothy R.; Latham, David W.; Chaplin, William J.; Handberg, Rasmus; Huber, Daniel; Kipping, David M.; Payne, Matthew J.; Jiang, Chen; Victor Silva Aguirre; Stello, Dennis; Sliski, David H.; Ciardi, David R.; Buchhave, Lars A.; Bedding, Timothy R.; Davies, Guy R.; Hekker, Saskia; Kjeldsen, Hans; Everett, Mark E.; Howell, Steve B.; Basu, Sarbani; Campante, Tiago L.; Christensen-Dalsgaard, Jørgen; Elsworth, Yvonne P.; Karoff, Christoffer; Kawaler, Steven D.; Lund, Mikkel N.; Lundkvist, Mia; Esquerdo, Gilbert A.; et al. (2014). "Kepler-432: A red giant interacting with one of its two long period giant planets". The Astrophysical Journal. 803 (2): 49. arXiv:1411.4666. Bibcode:2015ApJ...803...49Q. doi:10.1088/0004-637X/803/2/49. S2CID 28994316.
- ↑ Welsh, William F.; et al. (2015). "KIC 9632895 - The 10th Kepler Transiting Circumbinary Planet". The Astrophysical Journal. 809 (1). 26. arXiv:1409.1605. Bibcode:2015ApJ...809...26W. doi:10.1088/0004-637X/809/1/26. S2CID 55158342.
- ↑ Koshimoto, N.; et al. (2014), "OGLE-2008-BLG-355Lb: A MASSIVE PLANET AROUND a LATE-TYPE STAR", The Astrophysical Journal, 788 (2): 128, arXiv:1403.7005, Bibcode:2014ApJ...788..128K, doi:10.1088/0004-637X/788/2/128, S2CID 119194503
- ↑ Poleski, Radosław; Skowron, Jan; Udalski, Andrzej; Han, Cheongho; Kozłowski, Szymon; Wyrzykowski, Łukasz; Dong, Subo; Szymański, Michał K.; Kubiak, Marcin; Pietrzyński, Grzegorz; Soszyński, Igor; Ulaczyk, Krzysztof; Pietrukowicz, Paweł; Gould, Andrew (2014), "Triple Microlens Ogle-2008-BLG-092L: Binary Stellar System with a Circumprimary Uranus-Type Planet", The Astrophysical Journal, 795 (1): 42, arXiv:1408.6223, Bibcode:2014ApJ...795...42P, doi:10.1088/0004-637X/795/1/42, S2CID 118678130
- ↑ Skowron, J.; et al. (2014), "OGLE-2011-BLG-0265Lb: A JOVIAN MICROLENSING PLANET ORBITING AN M DWARF", The Astrophysical Journal, 804: 33, arXiv:1410.8252, doi:10.1088/0004-637X/804/1/33, S2CID 45737293
- ↑ Jung, Y. K.; et al. (2014), "Ogle-2013-BLG-0102La,B: Microlensing Binary with Components at Star/Brown Dwarf and Brown Dwarf/Planet Boundaries", The Astrophysical Journal, 798 (2): 123, arXiv:1407.7926, doi:10.1088/0004-637X/798/2/123, S2CID 119250588
- ↑ Gould, A.; et al. (2014), "A terrestrial planet in a ~1-AU orbit around one member of a ~15-AU binary", Science, 345 (6192): 46–49, arXiv:1407.1115, Bibcode:2014Sci...345...46G, doi:10.1126/science.1251527, PMID 24994642, S2CID 206555598
- ↑ Udalski, A.; Yee, J. C.; Gould, A.; Carey, S.; Zhu, W.; Skowron, J.; Kozłowski, S.; Poleski, R.; Pietrukowicz, P.; Pietrzyński, G.; Szymański, M. K.; Mróz, P.; Soszyński, I.; Ulaczyk, K.; Wyrzykowski, Ł.; Han, C.; Calchi Novati, S.; Pogge, R. W. (2014), "Spitzeras a Microlens Parallax Satellite: Mass Measurement for the Ogle-2014-BLG-0124L Planet and ITS Host Star", The Astrophysical Journal, 799 (2): 237, arXiv:1410.4219, doi:10.1088/0004-637X/799/2/237, S2CID 30683835
- 1 2 3 Brucalassi, A.; Pasquini, L.; Saglia, R.; Ruiz, M. T.; Bonifacio, P.; Bedin, L. R.; Biazzo, K.; Melo, C.; Lovis, C.; Randich, S. (2014), "Three planetary companions around M 67 stars", Astronomy & Astrophysics, 561: L9, arXiv:1401.4905, Bibcode:2014A&A...561L...9B, doi:10.1051/0004-6361/201322584, S2CID 36895080
- 1 2 Niedzielski, A.; Villaver, E.; Wolszczan, A.; Adamów, M.; Kowalik, K.; MacIejewski, G.; Nowak, G.; García-Hernández, D. A.; Deka, B.; Adamczyk, M. (2014), "Tracking Advanced Planetary Systems (TAPAS) with HARPS-N", Astronomy & Astrophysics, 573: A36, arXiv:1410.5971, doi:10.1051/0004-6361/201424399, S2CID 53531092
- ↑ Anderson, D. R.; Collier Cameron, A.; Hellier, C.; Lendl, M.; Lister, T. A.; Maxted, P. F. L.; Queloz, D.; Smalley, B.; Smith, A. M. S.; Triaud, A. H. M. J.; Brown, D. J. A.; Gillon, M.; Neveu-Vanmalle, M.; Pepe, F.; Pollacco, D.; Ségransan, D.; Udry, S.; West, R. G.; Wheatley, P. J. (2015). "WASP-20b and WASP-28b: A hot Saturn and a hot Jupiter in near-aligned orbits around solar-type stars". Astronomy & Astrophysics. 575: A61. arXiv:1402.1482. Bibcode:2015A&A...575A..61A. doi:10.1051/0004-6361/201423591. S2CID 119211951.
- ↑ Evans, Daniel F.; Southworth, John; Smalley, Barry (2016). "Wasp-20 is a Close Visual Binary with a Transiting Hot Jupiter". The Astrophysical Journal. 833 (2): L19. arXiv:1611.08735. Bibcode:2016ApJ...833L..19E. doi:10.3847/2041-8213/833/2/L19. S2CID 119488567.
- 1 2 3 Hellier, Coel; Anderson, D. R.; Collier Cameron, A.; Delrez, L.; Gillon, M.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Segransan, D.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Turner, O. D.; Udry, S.; West, R. G. (2014), "Three WASP-South transiting exoplanets: WASP-74b, WASP-83b & WASP-89b", The Astronomical Journal, 150 (1): 18, arXiv:1410.6358, Bibcode:2015AJ....150...18H, doi:10.1088/0004-6256/150/1/18, S2CID 16878578
- 1 2 3 Brown, D. J. A.; et al. (2014), Three transiting planet discoveries from the Wide Angle Search for Planets: WASP-85 A b; WASP-116 b, and WASP-149 b, arXiv:1412.7761
- 1 2 3 4 5 6 Anderson, D. R.; Brown, D. J. A.; Collier Cameron, A.; Delrez, L.; Fumel, A.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Neveu-VanMalle, M.; Pepe, F.; Pollacco, D.; Queloz, D.; Rojo, P.; Segransan, D.; Serenelli, A. M.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Turner, O. D.; Udry, S.; West, R. G. (2014), Six newly-discovered hot Jupiters transiting F/G stars: WASP-87b, WASP-108b, WASP-109b, WASP-110b, WASP-111b & WASP-112b, arXiv:1410.3449
- 1 2 Neveu-Vanmalle, M.; Queloz, D.; Anderson, D. R.; Charbonnel, C.; Collier Cameron, A.; Delrez, L.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Udry, S.; West, R. G. (2014), "WASP-94 a and B planets: Hot-Jupiter cousins in a twin-star system", Astronomy & Astrophysics, 572: A49, arXiv:1409.7566, Bibcode:2014A&A...572A..49N, doi:10.1051/0004-6361/201424744, S2CID 53470970
- ↑ Gillon, M.; Anderson, D. R.; Collier-Cameron, A.; Delrez, L.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smith, A. M. S.; Smalley, B.; Southworth, J.; Triaud, A. H. M. J.; Udry, S.; Van Grootel, V.; West, R. G. (2014), "WASP-103 b: A new planet at the edge of tidal disruption", Astronomy & Astrophysics, 562: L3, arXiv:1401.2784, Bibcode:2014A&A...562L...3G, doi:10.1051/0004-6361/201323014, S2CID 53680974
- ↑ Southworth, John; Mancini, L.; Ciceri, S.; Budaj, J.; Dominik, M.; Figuera Jaimes, R.; Haugbølle, T.; Jørgensen, U. G.; Popovas, A.; Rabus, M.; Rahvar, S.; von Essen, C.; Schmidt, R. W.; Wertz, O.; Alsubai, K. A.; Bozza, V.; Bramich, D. M.; Calchi Novati, S.; d'Ago, G.; Hinse, T. C.; Henning, Th.; Hundertmark, M.; Juncher, D.; Korhonen, H.; Skottfelt, J.; Snodgrass, C.; Starkey, D.; Surdej, J. (2014), "High-precision photometry by telescope defocusing – VII. The ultrashort period planet WASP-103★", Monthly Notices of the Royal Astronomical Society, 447: 711–721, arXiv:1411.2767, doi:10.1093/mnras/stu2394
- 1 2 Smith, A. M. S.; et al. (2014). "WASP-104b and WASP-106b: Two transiting hot Jupiters in 1.75-day and 9.3-day orbits". Astronomy and Astrophysics. 570. A64. arXiv:1408.0887. Bibcode:2014A&A...570A..64S. doi:10.1051/0004-6361/201424752. S2CID 119245284.
- ↑ Lendl, M.; Triaud, A. H. M. J.; Anderson, D. R.; Collier Cameron, A.; Delrez, L.; Doyle, A. P.; Gillon, M.; Hellier, C.; Jehin, E.; Maxted, P. F. L.; Neveu-Vanmalle, M.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Udry, S.; Van Grootel, V.; West, R. G. (2014). "WASP-117b: A 10-day-period Saturn in an eccentric and misaligned orbit". Astronomy & Astrophysics. 568: A81. arXiv:1406.6942. Bibcode:2014A&A...568A..81L. doi:10.1051/0004-6361/201424481. S2CID 54605901.
- ↑ Carone, Ludmila; Mollière, Paul; Zhou, Yifan; Bouwman, Jeroen; Yan, Fei; Baeyens, Robin; Apai, Dániel; Espinoza, Nestor; Rackham, Benjamin V.; Jordán, Andrés; Angerhausen, Daniel; Decin, Leen; Lendl, Monika; Venot, Olivia; Henning, Thomas (2021). "Indications for very high metallicity and absence of methane in the eccentric exo-Saturn WASP-117b". Astronomy & Astrophysics. 646: A168. arXiv:2006.05382. Bibcode:2021A&A...646A.168C. doi:10.1051/0004-6361/202038620. S2CID 219559116.
- 1 2 Desidera, S.; et al. (2014), "The GAPS programme with HARPS-N at TNG", Astronomy & Astrophysics, 567: L6, arXiv:1407.0251, doi:10.1051/0004-6361/201424339, S2CID 118567085
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.