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 180 b | 0.0261 | 17.380 | 0.103 | radial vel. | 38.95 | 0.43 | 3371 | [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 687 b | 0.058 | 38.14 | 0.16353 | radial vel. | 14.8 | 0.41 | 3413 | [10] | ||
Gliese 3293 b | 0.07406 | 30.5987 | 0.14339 | radial vel. | 51.4 | 0.42 | 3466 | [11] | ||
Gliese 3293 c | 0.06636 | 122.6196 | 0.36175 | radial vel. | 51.4 | 0.42 | 3466 | [11] | ||
Gliese 3341 b | 0.0208 | 14.207 | 0.089 | radial vel. | 77.1 | 0.47 | 3526 | [11] | ||
GU Piscium b | 11.3 | 1.265 | 2000 | imaging | 160 | 0.33 | 3250±32 | [12] | ||
HAT-P-49b | 1.73 | 1.413 | 2.691548 | 0.0438 | 2131 | transit | 1050 | 1.54 | 6820 | [13] |
HAT-P-54b | 0.76 | 0.944 | 3.799847 | 0.04117 | transit | 443 | 0.65 | 4390 | [14] Disputed in 2016,[15] reconfirmed in 2021.[16] | |
HATS-4b | 1.323 | 1.02 | 2.516729 | 0.0362 | 1315 | transit | 1400 | 1 | 5403 | [17] |
HATS-5b | 0.237 | 0.912 | 4.763387 | 0.0542 | 1025 | transit | 840 | 0.94 | 5304 | [18] |
HATS-6b | 0.319 | 0.998 | 3.3252725 | 0.03623 | transit | 484 | 0.57 | 3724 | [19] | |
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 | [20] | ||
HD 5319 c | 1.15 | 886 | 2.071 | radial vel. | 370 | 1.51 | 4958 | [21] | ||
HD 10442 b | 2.1 | 1043 | 2.335 | radial vel. | 443±4 | 1.56 | 5034 | [21] | ||
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 | [21] | ||
HD 14067 b | 7.8 | 1455 | 3.4 | radial vel. | 533 | 2.4 | 4815 | [22] | ||
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 | [21] | ||
HD 100546 b | 3.4 | 53 | imaging | 320 | 2.4 | 10500 | [23] | |||
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 | [24] | ||
HD 141399 b | 0.451 | 94.44 | 0.415 | radial vel. | 118 | 1.07 | 5600 | [25] | ||
HD 141399 c | 1.33 | 201.99 | 0.689 | radial vel. | 118 | 1.07 | 5600 | [25] | ||
HD 141399 d | 1.18 | 1069.8 | 2.09 | radial vel. | 118 | 1.07 | 5600 | [25] | ||
HD 141399 e | 0.66 | 5000 | 5 | radial vel. | 118 | 1.07 | 5600 | [25] | ||
HD 154857 c | 2.58 | 3452 | 5.36 | radial vel. | 223.5 | 1.72 | 5605 | [24] | ||
HIP 67851 b | 1.38 | 88.9 | 0.46 | radial vel. | 208.3±0.6 | 1.63 | 4890 | [26] | ||
HIP 67851 c | 4.34±0.59 | 1741±39 | 3.09±0.18 | radial vel. | 208.3±0.6 | 1.63 | 4890 | [27] | ||
HIP 97233 b | 20 | 1058.8 | 2.55 | radial vel. | 347 | 1.93 | 5020 | [26] | ||
HIP 105854 b | 8.2 | 184.2 | 0.81 | radial vel. | 276 | 2.1 | 4780 | [28] | ||
HIP 116454 b | 0.037 | 0.226 | 9.1205 | 0.0906 | radial vel. | 180 | 0.78 | 5089 | [29] | |
Kapteyn b | 0.015 | 48.616+0.036 −0.032 |
0.168 | radial vel. | 12.8 | 0.28 | 3550 | Existence of planet been disputed.[30][31] | ||
Kapteyn c | 0.022 | 121.54 | 0.311 | radial vel. | 12.8 | 0.28 | 3550 | Existence of planet been disputed.[30][31] | ||
Kepler-23d | 0.196 | 15.274299 | 0.124 | transit | 2600 | 1.11 | 5828 | [32] | ||
Kepler-24d | 0.149 | 4.244384 | 0.051 | transit | 3900 | 1.03 | 5897 | [32] | ||
Kepler-24e | 0.248 | 18.998355 | 0.138 | transit | 3900 | 1.03 | 5897 | [32] | ||
Kepler-25d | 0.283 | 123 | radial vel. | 798±4 | 1.19 | 6270 | [33][32] | |||
Kepler-26d | 0.095 | 3.543919 | 0.039 | transit | 1104±10 | 0.54 | 3914 | [32] | ||
Kepler-26e | 0.215 | 46.827915 | 0.22 | transit | 1104±10 | 0.54 | 3914 | [32] | ||
Kepler-31d | 6.8 | 0.348 | 87.6451 | 0.4 | transit | 6800 | 1.21 | 6340 | [32] | |
Kepler-37e | 51.196 | timing | 220 | 0.8 | 5417 | [32] | ||||
Kepler-48d | 0.025 | 0.182 | 42.8961 | transit | 1009±5 | 0.88 | 5194 | [33][32] | ||
Kepler-48e | 2.067 | 982 | radial vel. | 1009±5 | 0.88 | 5194 | [33] | |||
Kepler-49d | 0.143 | 2.576549 | 0.031 | transit | 1024±8 | 0.55 | 4252 | [32] | ||
Kepler-49e | 0.139 | 18.596108 | 0.116 | transit | 1024±8 | 0.55 | 4252 | [32] | ||
Kepler-51d | 0.024 | 0.865 | 130.194 | 0.509 | transit | 2610±50 | 1.04 | 6018 | [32] | |
Kepler-52d | 0.174 | 36.445171 | 0.182 | transit | 1058±7 | 0.54 | 4263 | [32] | ||
Kepler-53d | 0.189 | 9.751962 | 0.091 | transit | 4600±200 | 0.98 | 5858 | [32] | ||
Kepler-54d | 0.136 | 20.995694 | 0.126 | transit | 893±9 | 0.51 | 4252 | [32] | ||
Kepler-55d | 0.142 | 2.211099 | 0.029 | transit | 1920±30 | 0.62 | 4503 | [32] | ||
Kepler-55e | 0.138 | 4.617534 | 0.048 | transit | 1920±30 | 0.62 | 4503 | [32] | ||
Kepler-55f | 0.142 | 10.198545 | 0.081 | transit | 1920±30 | 0.62 | 4503 | [32] | ||
Kepler-58d | 0.262 | 40.101371 | 0.236 | transit | 3250±80 | 0.95 | 6099 | [32] | ||
Kepler-79d | 0.019 | 0.639 | 52.0902 | 0.287 | 553 | transit | 3230±60 | 1.17 | 6174 | [32] |
Kepler-79e | 0.013 | 0.311 | 81.0659 | 0.386 | 477 | transit | 3230±60 | 1.17 | 6174 | [32] |
Kepler-80d | 0.02124 | 0.136 | 3.07222 | 0.0372 | transit | 1160 | 0.73 | 4540 | [32] | |
Kepler-80e | 0.01299 | 0.143 | 4.64489 | 0.0491 | transit | 1160 | 0.73 | 4540 | [32] | |
Kepler-81d | 0.108 | 20.837846 | 0.128 | transit | 1147±10 | 0.64 | 4500 | [32] | ||
Kepler-82d | 0.158 | 2.382961 | 0.034 | transit | 3030±80 | 0.85 | 5428 | [32] | ||
Kepler-82e | 0.22 | 5.902206 | 0.063 | transit | 3030±80 | 0.85 | 5428 | [32] | ||
Kepler-83d | 0.173 | 5.169796 | 0.051 | transit | 1320±17 | 0.66 | 4648 | [32] | ||
Kepler-84d | 0.123 | 4.224537 | 0.052 | transit | 4700±500 | 1 | 6031 | [32] | ||
Kepler-84e | 0.232 | 27.434389 | 0.181 | transit | 4700±500 | 1 | 6031 | [32] | ||
Kepler-84f | 0.196 | 44.552169 | 0.25 | transit | 4700±500 | 1 | 6031 | [32] | ||
Kepler-85d | 0.107 | 17.91323 | 0.13 | transit | 2550±50 | 0.92 | 5436 | [32] | ||
Kepler-85e | 0.113 | 25.216751 | 0.163 | transit | 2550±50 | 0.92 | 5436 | [32] | ||
Kepler-93b | 0.01265 | 0.132 | 4.72673978 | 0.053 | 1037 | transit | 313.7±0.7 | 0.91 | 5669 | [33] |
Kepler-93c | 3 | 1460 | radial vel. | 313.7±0.7 | 0.91 | 5669 | [33] | |||
Kepler-94b | 0.034 | 0.313 | 2.50806 | transit | 629±2 | 0.81 | 4781 | [33] | ||
Kepler-94c | 9.836 | 820.3 | radial vel. | 629±2 | 0.81 | 4781 | [33] | |||
Kepler-95b | 0.041 | 0.305 | 11.5231 | transit | 1472±18 | 1.08 | 5699 | [33] | ||
Kepler-96b | 0.027 | 0.238 | 16.2385 | transit | 402.2±1.3 | 1 | 5690 | [33] | ||
Kepler-97b | 0.011 | 0.132 | 2.58664 | transit | 1322±11 | 0.94 | 5779 | [33] | ||
Kepler-97c | 1.08 | 789 | radial vel. | 1322±11 | 0.94 | 5779 | [33] | |||
Kepler-98b | 0.011 | 0.178 | 1.54168 | transit | 1154±9 | 0.99 | 5539 | [33] | ||
Kepler-99b | 0.019 | 0.132 | 4.60358 | transit | 683±3 | 0.79 | 4782 | [33] | ||
Kepler-100b | 0.023 | 0.118 | 6.88705 | transit | 1002±5 | 1.08 | 5825 | [33][32] | ||
Kepler-100c | 0.196 | 12.8159 | transit | 1002±5 | 1.08 | 5825 | [33][32] | |||
Kepler-100d | 0.144 | 35.3331 | transit | 1002±5 | 1.08 | 5825 | [33][32] | |||
Kepler-101b | 0.16 | 0.51 | 3.4876812 | 0.0474 | transit | 3110±50 | 1.17 | 5667 | [32] | |
Kepler-101c | 0.01 | 0.112 | 6.02976 | 0.0684 | transit | 3110±50 | 1.17 | 5667 | [32] | |
Kepler-102b | 0.042 | 5.28696 | 792 | transit | 352.7±0.7 | 0.81 | 4909 | [33][32] | ||
Kepler-102c | 0.052 | 7.07142 | 718 | transit | 352.7±0.7 | 0.81 | 4909 | [33][32] | ||
Kepler-102d | 0.012 | 0.105 | 10.3117 | transit | 352.7±0.7 | 0.81 | 4909 | [33][32] | ||
Kepler-102f | 0.079 | 27.4536 | 457 | transit | 352.7±0.7 | 0.81 | 4909 | [33][32] | ||
Kepler-103b | 0.031 | 0.301 | 15.9654 | transit | 1637±19 | 1.09 | 5845 | [33][32] | ||
Kepler-103c | 0.114 | 0.459 | 179.612 | transit | 1637±19 | 1.09 | 5845 | [33][32] | ||
Kepler-104b | 0.277 | 11.427548 | 0.094 | transit | 1322±14 | 0.81 | 5711 | [32] | ||
Kepler-104c | 0.279 | 23.668205 | 0.153 | transit | 1322±14 | 0.81 | 5711 | [32] | ||
Kepler-104d | 0.319 | 51.755394 | 0.257 | transit | 1322±14 | 0.81 | 5711 | [32] | ||
Kepler-105c | 0.01447 | 0.117 | 7.1262 | transit | 1517±18 | 0.96 | 5827 | [32] | ||
Kepler-106b | 0.073 | 6.16486 | transit | 1470±20 | 1 | 5858 | [33] | |||
Kepler-106c | 0.033 | 0.223 | 13.5708 | transit | 1470±20 | 1 | 5858 | [33][32] | ||
Kepler-106d | 0.085 | 23.9802 | transit | 1470±20 | 1 | 5858 | [33][32] | |||
Kepler-106e | 0.035 | 0.228 | 43.8445 | transit | 1470±20 | 1 | 5858 | [33][32] | ||
Kepler-107b | 0.139 | 3.179997 | 0.044 | transit | 1741±18 | 5851 | [32] | |||
Kepler-107c | 0.161 | 4.901425 | 0.059 | transit | 1741±18 | 5851 | [32] | |||
Kepler-107d | 0.095 | 7.958203 | 0.082 | transit | 1741±18 | 5851 | [32] | |||
Kepler-107e | 0.308 | 14.749049 | 0.123 | transit | 1741±18 | 5851 | [32] | |||
Kepler-108b | 0.772 | 49.183921 | 0.292 | transit | 4200±500 | 0.87 | 5854 | [32] | ||
Kepler-108c | 0.73 | 190.323494 | 0.721 | transit | 4200±500 | 0.87 | 5854 | [32] | ||
Kepler-109b | 0.211 | 6.48163 | transit | 1570±17 | 1.04 | 5952 | [33][32] | |||
Kepler-109c | 0.225 | 21.2227 | transit | 1570±17 | 1.04 | 5952 | [33][32] | |||
Kepler-110b | 0.163 | 12.691112 | 0.107 | transit | 1950±30 | 5960 | [32] | |||
Kepler-110c | 0.197 | 31.719775 | 0.198 | transit | 1950±30 | 5960 | [32] | |||
Kepler-111b | 0.141 | 3.341815 | 0.046 | transit | 2190±20 | 5952 | [32] | |||
Kepler-111c | 0.651 | 224.784608 | 0.761 | transit | 2190±20 | 5952 | [32] | |||
Kepler-112b | 0.211 | 8.408878 | 0.076 | transit | 1698±14 | 5544 | [32] | |||
Kepler-112c | 0.214 | 28.574263 | 0.172 | transit | 1698±14 | 5544 | [32] | |||
Kepler-113b | 0.037 | 0.162 | 4.754 | transit | 862±3 | 0.75 | 4725 | [33][32] | ||
Kepler-113c | 0.194 | 8.92507 | transit | 862±3 | 0.75 | 4725 | [33][32] | |||
Kepler-114b | 0.112 | 5.188549 | 0.053 | 722 | transit | 852±4 | 0.56 | 4605 | [32] | |
Kepler-115b | 0.097 | 2.403679 | 0.036 | transit | 2070±20 | 1 | 5979 | [32] | ||
Kepler-115c | 0.232 | 8.990889 | 0.087 | transit | 2070±20 | 1 | 5979 | [32] | ||
Kepler-116b | 0.305 | 5.968734 | 0.069 | transit | 3200±50 | 1.16 | 6142 | [32] | ||
Kepler-116c | 0.205 | 13.07163 | 0.116 | transit | 3200±50 | 1.16 | 6142 | [32] | ||
Kepler-117b | 0.094 | 0.719 | 18.7959228 | 0.1445 | transit | 4700 | 1.13 | 6150 | [32] | |
Kepler-117c | 1.84 | 1.101 | 50.790391 | 0.2804 | transit | 4700 | 1.13 | 6150 | [32] | |
Kepler-118b | 0.175 | 7.518496 | 0.073 | transit | 1900±20 | 0.86 | 5274 | [32] | ||
Kepler-118c | 0.685 | 20.17202 | 0.141 | transit | 1900±20 | 0.86 | 5274 | [32] | ||
Kepler-119b | 0.321 | 2.422082 | 0.035 | transit | 2340±40 | 5595 | [32] | |||
Kepler-119c | 0.082 | 4.125103 | 0.049 | transit | 2340±40 | 5595 | [32] | |||
Kepler-120b | 0.192 | 6.312501 | 0.055 | transit | 1281±10 | 4096 | [32] | |||
Kepler-120c | 0.136 | 12.794585 | 0.088 | transit | 1281±10 | 4096 | [32] | |||
Kepler-121b | 0.209 | 3.177422 | 0.039 | transit | 1690±20 | 5311 | [32] | |||
Kepler-121c | 0.203 | 41.008011 | 0.216 | transit | 1690±20 | 5311 | [32] | |||
Kepler-122b | 0.209 | 5.766193 | 0.064 | transit | 3450±70 | 0.99 | 6050 | [32] | ||
Kepler-122c | 0.524 | 12.465988 | 0.108 | transit | 3450±70 | 0.99 | 6050 | [32] | ||
Kepler-122d | 0.196 | 21.587475 | 0.155 | transit | 3450±70 | 0.99 | 6050 | [32] | ||
Kepler-122e | 0.232 | 37.993273 | 0.227 | transit | 3450±70 | 0.99 | 6050 | [32] | ||
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 | [32] | ||
Kepler-123c | 0.132 | 26.695074 | 0.181 | transit | 3430±80 | 1.03 | 6089 | [32] | ||
Kepler-124b | 0.065 | 3.410493 | 0.039 | transit | 1386±10 | 4984 | [32] | |||
Kepler-124c | 0.156 | 13.821375 | 0.1 | transit | 1386±10 | 4984 | [32] | |||
Kepler-124d | 0.099 | 30.950851 | 0.17 | transit | 1386±10 | 4984 | [32] | |||
Kepler-125b | 0.211 | 4.164389 | 0.041 | transit | 601±3 | 0.55 | 3810 | [32] | ||
Kepler-125c | 0.066 | 5.774464 | 0.051 | transit | 601±3 | 0.55 | 3810 | [32] | ||
Kepler-126b | 0.136 | 10.495711 | 0.099 | transit | 779±5 | 6239 | [32] | |||
Kepler-126c | 0.141 | 21.869741 | 0.162 | transit | 779±5 | 6239 | [32] | |||
Kepler-126d | 0.223 | 100.283134 | 0.448 | transit | 779±5 | 6239 | [32] | |||
Kepler-127b | 0.125 | 14.435889 | 0.125 | transit | 1162±8 | 6106 | [32] | |||
Kepler-127c | 0.237 | 29.393195 | 0.2 | transit | 1162±8 | 6106 | [32] | |||
Kepler-127d | 0.236 | 48.630408 | 0.28 | transit | 1162±8 | 6106 | [32] | |||
Kepler-129b | 0.211 | 15.79186 | 0.131 | transit | 1349±14 | 1.18 | 5770 | [32] | ||
Kepler-129c | 0.227 | 82.20017 | 0.393 | transit | 1349±14 | 1.18 | 5770 | [32] | ||
Kepler-130c | 0.259 | 27.50868 | 0.178 | transit | 1042±7 | 1 | 5884 | [32] | ||
Kepler-130d | 0.146 | 87.517905 | 0.377 | transit | 1042±7 | 1 | 5884 | [32] | ||
Kepler-131b | 0.051 | 0.215 | 16.092 | transit | 750±4 | 1.02 | 5685 | [33][32] | ||
Kepler-131c | 0.026 | 0.075 | 25.5169 | transit | 750±4 | 1.02 | 5685 | [33][32] | ||
Kepler-132b | 0.108 | 6.178196 | 0.067 | transit | 900±70 | 6003 | [32] | |||
Kepler-132c | 0.114 | 6.414914 | 0.068 | transit | 900±70 | 6003 | [32] | |||
Kepler-132d | 0.138 | 18.010199 | 0.136 | transit | 900±70 | 6003 | [32] | |||
Kepler-133b | 0.157 | 8.129976 | 0.083 | transit | 2170±60 | 5736 | [32] | |||
Kepler-133c | 0.253 | 31.517586 | 0.204 | transit | 2170±60 | 5736 | [32] | |||
Kepler-134b | 0.178 | 5.317429 | 0.06 | transit | 1102±7 | 5983 | [32] | |||
Kepler-134c | 0.112 | 10.105785 | 0.092 | transit | 1102±7 | 5983 | [32] | |||
Kepler-135b | 0.161 | 6.00253 | 0.067 | transit | 2060±40 | 6090 | [32] | |||
Kepler-135c | 0.103 | 11.448708 | 0.103 | transit | 2060±40 | 6090 | [32] | |||
Kepler-136b | 0.183 | 11.5789 | 0.106 | transit | 1389±14 | 1.2 | 6165 | [32] | ||
Kepler-136c | 0.178 | 16.399235 | 0.133 | transit | 1389±14 | 1.2 | 6165 | [32] | ||
Kepler-137b | 0.131 | 8.436387 | 0.077 | transit | 996±6 | 5187 | [32] | |||
Kepler-137c | 0.168 | 18.735753 | 0.13 | transit | 996±6 | 5187 | [32] | |||
Kepler-138b | 0.00021 | 0.047 | 10.3126 | transit | 218.5±0.3 | 0.52 | 3841 | [32] | ||
Kepler-138c | 0.0062 | 0.107 | 13.7813 | transit | 218.5±0.3 | 0.52 | 3841 | [32] | ||
Kepler-138d | 0.00201 | 0.108 | 23.0881 | 431 | transit | 218.5±0.3 | 0.52 | 3841 | [32] | |
Kepler-139b | 0.262 | 15.771044 | 0.127 | transit | 1289±13 | 1.08 | 5594 | [32] | ||
Kepler-139c | 0.302 | 157.072878 | 0.586 | transit | 1289±13 | 1.08 | 5594 | [32] | ||
Kepler-140b | 0.144 | 3.25427 | 0.045 | transit | 1940±20 | 6077 | [32] | |||
Kepler-140c | 0.161 | 91.353282 | 0.414 | transit | 1940±20 | 6077 | [32] | |||
Kepler-141b | 0.062 | 3.107675 | 0.039 | transit | 990±4 | 1 | 4910 | [32] | ||
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 | [32] | ||
Kepler-142c | 0.255 | 4.761702 | 0.057 | transit | 1818±13 | 0.99 | 5790 | [32] | ||
Kepler-142d | 0.193 | 41.809118 | 0.242 | transit | 1818±13 | 0.99 | 5790 | [32] | ||
Kepler-143b | 0.215 | 16.007583 | 0.127 | transit | 2700±40 | 5848 | [32] | |||
Kepler-143c | 0.301 | 27.082511 | 0.181 | transit | 2700±40 | 5848 | [32] | |||
Kepler-144b | 0.119 | 5.885273 | 0.066 | transit | 1269±10 | 1.03 | 6075 | [32] | ||
Kepler-144c | 0.12 | 10.104665 | 0.094 | transit | 1269±10 | 1.03 | 6075 | [32] | ||
Kepler-146b | 0.331 | 31.158799 | 0.2 | transit | 2390±30 | 5948 | [32] | |||
Kepler-146c | 0.279 | 76.732171 | 0.364 | transit | 2390±30 | 5948 | [32] | |||
Kepler-147b | 0.136 | 12.610584 | 0.113 | transit | 3500±90 | 1.01 | 6012 | [32] | ||
Kepler-147c | 0.217 | 33.416423 | 0.216 | transit | 3500±90 | 1.01 | 6012 | [32] | ||
Kepler-148b | 0.161 | 1.729366 | 0.028 | transit | 2640±50 | 5272 | [32] | |||
Kepler-148c | 0.321 | 4.180043 | 0.05 | transit | 2640±50 | 5272 | [32] | |||
Kepler-149b | 0.376 | 29.198943 | 0.184 | transit | 1893±19 | 5381 | [32] | |||
Kepler-149c | 0.144 | 55.328328 | 0.281 | transit | 1893±19 | 5381 | [32] | |||
Kepler-149d | 0.353 | 160.018032 | 0.571 | transit | 1893±19 | 5381 | [32] | |||
Kepler-150b | 0.112 | 3.428054 | 0.044 | transit | 2980±60 | 5560 | [32] | |||
Kepler-150c | 0.329 | 7.381998 | 0.073 | transit | 2980±60 | 5560 | [32] | |||
Kepler-150d | 0.249 | 12.56093 | 0.104 | transit | 2980±60 | 5560 | [32] | |||
Kepler-150e | 0.278 | 30.826557 | 0.189 | transit | 2980±60 | 5560 | [32] | |||
Kepler-151b | 0.273 | 15.228958 | 0.116 | transit | 2160±30 | 0.83 | 5460 | [32] | ||
Kepler-151c | 0.186 | 24.674612 | 0.16 | transit | 2160±30 | 0.83 | 5460 | [32] | ||
Kepler-152b | 0.249 | 18.207973 | 0.124 | transit | 1457±10 | 5088 | [32] | |||
Kepler-152c | 0.213 | 88.255055 | 0.356 | transit | 1457±10 | 5088 | [32] | |||
Kepler-153b | 0.261 | 18.870227 | 0.129 | transit | 1518±11 | 5404 | [32] | |||
Kepler-153c | 0.226 | 46.90232 | 0.237 | transit | 1518±11 | 5404 | [32] | |||
Kepler-154b | 0.202 | 33.040532 | 0.198 | transit | 3070±60 | 0.89 | 5690 | [32] | ||
Kepler-154c | 0.263 | 62.303276 | 0.303 | transit | 3070±60 | 0.89 | 5690 | [32] | ||
Kepler-155b | 0.186 | 5.931194 | 0.056 | transit | 965±7 | 0.58 | 4508 | [32] | ||
Kepler-155c | 0.2 | 52.661793 | 0.242 | transit | 965±7 | 0.58 | 4508 | [32] | ||
Kepler-156b | 0.205 | 4.973456 | 0.054 | transit | 1465±11 | 5094 | [32] | |||
Kepler-156c | 0.227 | 15.906801 | 0.117 | transit | 1465±11 | 5094 | [32] | |||
Kepler-157b | 0.118 | 1.732342 | 0.028 | transit | 2580±40 | 5774 | [32] | |||
Kepler-157c | 0.2 | 13.5405 | 0.11 | transit | 2580±40 | 5774 | [32] | |||
Kepler-158b | 0.189 | 16.709184 | 0.111 | transit | 1037±6 | 4623 | [32] | |||
Kepler-158c | 0.17 | 28.551383 | 0.158 | transit | 1037±6 | 4623 | [32] | |||
Kepler-159b | 0.212 | 10.139623 | 0.082 | transit | 1232±10 | 4625 | [32] | |||
Kepler-159c | 0.304 | 43.595792 | 0.218 | transit | 1232±10 | 4625 | [32] | |||
Kepler-160b | 0.137 | 4.309427 | 0.05 | transit | 3140±60 | 0.88 | 5471+115 −37 |
[32][34] | ||
Kepler-160c | 0.322 | 13.699087 | 0.109 | transit | 3140±60 | 0.88 | 5471+115 −37 |
[32][34] | ||
Kepler-161b | 0.189 | 4.921355 | 0.054 | transit | 1435±10 | 0.77 | 5078 | [32] | ||
Kepler-161c | 0.183 | 7.06424 | 0.068 | transit | 1435±10 | 0.77 | 5078 | [32] | ||
Kepler-162b | 0.112 | 6.919798 | 0.069 | transit | 2860±50 | 5816 | [32] | |||
Kepler-162c | 0.27 | 19.446355 | 0.137 | transit | 2860±50 | 5816 | [32] | |||
Kepler-163b | 0.094 | 7.810937 | 0.078 | transit | 2300±40 | 0.96 | 5776 | [32] | ||
Kepler-163c | 0.202 | 21.347262 | 0.152 | transit | 2300±40 | 0.96 | 5776 | [32] | ||
Kepler-164b | 0.126 | 5.03503 | 0.058 | transit | 2980±50 | 1.11 | 5888 | [32] | ||
Kepler-164c | 0.244 | 10.945723 | 0.097 | transit | 2980±50 | 1.11 | 5888 | [32] | ||
Kepler-164d | 0.219 | 28.986769 | 0.187 | transit | 2980±50 | 1.11 | 5888 | [32] | ||
Kepler-165b | 0.207 | 8.180848 | 0.072 | transit | 1860±20 | 5211 | [32] | |||
Kepler-165c | 0.199 | 15.31299 | 0.11 | transit | 1860±20 | 5211 | [32] | |||
Kepler-166b | 0.203 | 7.650254 | 0.072 | transit | 2000±20 | 5413 | [32] | |||
Kepler-166c | 0.212 | 34.260281 | 0.195 | transit | 2000±20 | 5413 | [32] | |||
Kepler-167b | 0.144 | 4.3931632 | 0.0483 | transit | 1100 | 0.77 | 4890 | [32] | ||
Kepler-167c | 0.138 | 7.406114 | 0.0684 | transit | 1100 | 0.77 | 4890 | [32] | ||
Kepler-168b | 0.13 | 4.425391 | 0.056 | transit | 4550±160 | 6282 | [32] | |||
Kepler-168c | 0.24 | 13.193242 | 0.116 | transit | 4550±160 | 6282 | [32] | |||
Kepler-169b | 0.101 | 3.250619 | 0.04 | transit | 1341±9 | 0.86 | 4997 | [32] | ||
Kepler-169c | 0.108 | 6.195469 | 0.062 | transit | 1341±9 | 0.86 | 4997 | [32] | ||
Kepler-169d | 0.112 | 8.348125 | 0.075 | transit | 1341±9 | 0.86 | 4997 | [32] | ||
Kepler-169e | 0.196 | 13.767102 | 0.105 | transit | 1341±9 | 0.86 | 4997 | [32] | ||
Kepler-169f | 0.23 | 87.090195 | 0.359 | transit | 1341±9 | 0.86 | 4997 | [32] | ||
Kepler-170b | 0.285 | 7.930592 | 0.08 | transit | 2460±40 | 5679 | [32] | |||
Kepler-170c | 0.255 | 16.665863 | 0.131 | transit | 2460±40 | 5679 | [32] | |||
Kepler-171b | 0.209 | 4.166972 | 0.05 | transit | 2890±60 | 5642 | [32] | |||
Kepler-171c | 0.228 | 11.463462 | 0.098 | transit | 2890±60 | 5642 | [32] | |||
Kepler-171d | 0.169 | 39.595519 | 0.223 | transit | 2890±60 | 5642 | [32] | |||
Kepler-172b | 0.21 | 2.940309 | 0.04 | transit | 2770±60 | 0.86 | 5526 | [32] | ||
Kepler-172c | 0.255 | 6.388996 | 0.068 | transit | 2770±60 | 0.86 | 5526 | [32] | ||
Kepler-172d | 0.201 | 14.627119 | 0.118 | transit | 2770±60 | 0.86 | 5526 | [32] | ||
Kepler-172e | 0.246 | 35.118736 | 0.211 | transit | 2770±60 | 0.86 | 5526 | [32] | ||
Kepler-173b | 0.115 | 4.263742 | 0.048 | transit | 2780±50 | 0.78 | 6031 | [32] | ||
Kepler-173c | 0.217 | 8.005777 | 0.074 | transit | 2780±50 | 0.78 | 6031 | [32] | ||
Kepler-174b | 0.175 | 13.98179 | 0.1 | transit | 1268±8 | 4880 | [32] | |||
Kepler-174c | 0.133 | 44.000529 | 0.214 | transit | 1268±8 | 4880 | [32] | |||
Kepler-174d | 0.195 | 247.35373 | 0.677 | transit | 1268±8 | 4880 | [32] | |||
Kepler-175b | 0.228 | 11.903515 | 0.105 | transit | 4450±150 | 1.04 | 6064 | [32] | ||
Kepler-175c | 0.277 | 34.035257 | 0.213 | transit | 4450±150 | 1.04 | 6064 | [32] | ||
Kepler-176b | 0.128 | 5.433074 | 0.058 | transit | 1750±20 | 5232 | [32] | |||
Kepler-176c | 0.232 | 12.759712 | 0.102 | transit | 1750±20 | 5232 | [32] | |||
Kepler-176d | 0.224 | 25.751974 | 0.163 | transit | 1750±20 | 5232 | [32] | |||
Kepler-178b | 0.259 | 9.576694 | 0.085 | transit | 2380±30 | 5676 | [32] | |||
Kepler-178c | 0.257 | 20.552802 | 0.142 | transit | 2380±30 | 5676 | [32] | |||
Kepler-178d | 0.352 | 96.678988 | 0.397 | transit | 2380±30 | 5676 | [32] | |||
Kepler-179b | 0.146 | 2.735926 | 0.036 | transit | 2010±20 | 5302 | [32] | |||
Kepler-179c | 0.178 | 6.40013 | 0.064 | transit | 2010±20 | 5302 | [32] | |||
Kepler-180b | 0.134 | 13.817124 | 0.109 | transit | 2320±30 | 0.84 | 5731 | [32] | ||
Kepler-180c | 0.269 | 41.885775 | 0.229 | transit | 2320±30 | 0.84 | 5731 | [32] | ||
Kepler-181b | 0.113 | 3.137873 | 0.04 | transit | 2020±30 | 5333 | [32] | |||
Kepler-181c | 0.178 | 4.302149 | 0.049 | transit | 2020±30 | 5333 | [32] | |||
Kepler-182b | 0.23 | 9.825792 | 0.096 | transit | 5290±180 | 1.14 | 6250 | [32] | ||
Kepler-182c | 0.306 | 20.684342 | 0.157 | transit | 5290±180 | 1.14 | 6250 | [32] | ||
Kepler-183b | 0.184 | 5.687945 | 0.064 | transit | 3530±100 | 5888 | [32] | |||
Kepler-183c | 0.203 | 11.637071 | 0.103 | transit | 3530±100 | 5888 | [32] | |||
Kepler-184b | 0.211 | 10.687576 | 0.092 | transit | 2030±20 | 5788 | [32] | |||
Kepler-184c | 0.176 | 20.303005 | 0.141 | transit | 2030±20 | 5788 | [32] | |||
Kepler-184d | 0.222 | 29.022358 | 0.179 | transit | 2030±20 | 5788 | [32] | |||
Kepler-185b | 0.104 | 1.6329 | 0.026 | transit | 1542±15 | 0.79 | 5208 | [32] | ||
Kepler-185c | 0.18 | 20.729042 | 0.139 | transit | 1542±15 | 0.79 | 5208 | [32] | ||
Kepler-186b | 0.095 | 3.8867907 | 0.0343 | transit | 560 | 0.54 | 3755 | [32] | ||
Kepler-186c | 0.112 | 7.267302 | 0.0451 | transit | 560 | 0.54 | 3755 | [32] | ||
Kepler-186d | 0.125 | 13.342996 | 0.0781 | transit | 560 | 0.54 | 3755 | [32] | ||
Kepler-186e | 0.113 | 22.407704 | 0.11 | transit | 560 | 0.54 | 3755 | [32] | ||
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 | [32] | ||
Kepler-187c | 0.238 | 10.640263 | 0.099 | transit | 3850±110 | 0.85 | 6105 | [32] | ||
Kepler-188b | 0.15 | 2.061897 | 0.032 | transit | 3250±80 | 6021 | [32] | |||
Kepler-188c | 0.285 | 5.996553 | 0.066 | transit | 3250±80 | 6021 | [32] | |||
Kepler-189b | 0.108 | 10.399931 | 0.088 | transit | 1960±20 | 0.79 | 5235 | [32] | ||
Kepler-189c | 0.212 | 20.134866 | 0.137 | transit | 1960±20 | 0.79 | 5235 | [32] | ||
Kepler-190b | 0.139 | 2.019999 | 0.03 | transit | 1431±9 | 0.84 | 5106 | [32] | ||
Kepler-190c | 0.13 | 3.763024 | 0.045 | transit | 1431±9 | 0.84 | 5106 | [32] | ||
Kepler-191b | 0.12 | 9.939632 | 0.087 | transit | 1970±30 | 0.85 | 5282 | [32] | ||
Kepler-191c | 0.166 | 17.738506 | 0.128 | transit | 1970±30 | 0.85 | 5282 | [32] | ||
Kepler-192b | 0.244 | 9.926746 | 0.09 | transit | 2170±20 | 5479 | [32] | |||
Kepler-192c | 0.249 | 21.2234 | 0.15 | transit | 2170±20 | 5479 | [32] | |||
Kepler-193b | 0.213 | 11.38848 | 0.106 | transit | 3390±80 | 6335 | [32] | |||
Kepler-193c | 0.245 | 50.697494 | 0.286 | transit | 3390±80 | 6335 | [32] | |||
Kepler-194b | 0.135 | 2.092281 | 0.032 | transit | 3700±100 | 6089 | [32] | |||
Kepler-194c | 0.231 | 17.308032 | 0.131 | transit | 3700±100 | 6089 | [32] | |||
Kepler-194d | 0.214 | 52.814973 | 0.275 | transit | 3700±100 | 6089 | [32] | |||
Kepler-195b | 0.181 | 8.307872 | 0.077 | transit | 2170±30 | 5329 | [32] | |||
Kepler-195c | 0.138 | 34.096863 | 0.197 | transit | 2170±30 | 5329 | [32] | |||
Kepler-196b | 0.17 | 20.739886 | 0.138 | transit | 1491±10 | 5128 | [32] | |||
Kepler-196c | 0.2 | 47.427737 | 0.24 | transit | 1491±10 | 5128 | [32] | |||
Kepler-197b | 0.091 | 5.599308 | 0.06 | transit | 1088±7 | 6004 | [32] | |||
Kepler-197c | 0.11 | 10.349695 | 0.09 | transit | 1088±7 | 6004 | [32] | |||
Kepler-197d | 0.109 | 15.677563 | 0.119 | transit | 1088±7 | 6004 | [32] | |||
Kepler-197e | 0.081 | 25.209715 | 0.164 | transit | 1088±7 | 6004 | [32] | |||
Kepler-198b | 0.252 | 17.790037 | 0.131 | transit | 1638±14 | 0.93 | 5574 | [32] | ||
Kepler-198c | 0.22 | 49.567416 | 0.259 | transit | 1638±14 | 0.93 | 5574 | [32] | ||
Kepler-199b | 0.277 | 23.637604 | 0.158 | transit | 1725±14 | 5644 | [32] | |||
Kepler-199c | 0.29 | 67.093408 | 0.316 | transit | 1725±14 | 5644 | [32] | |||
Kepler-200b | 0.19 | 8.594805 | 0.08 | transit | 2210±20 | 5678 | [32] | |||
Kepler-200c | 0.142 | 10.222157 | 0.09 | transit | 2210±20 | 5678 | [32] | |||
Kepler-201b | 0.219 | 25.672083 | 0.175 | transit | 2240±30 | 1.17 | 6065 | [32] | ||
Kepler-201c | 0.254 | 151.884058 | 0.573 | transit | 2240±30 | 1.17 | 6065 | [32] | ||
Kepler-202b | 0.145 | 4.069427 | 0.045 | transit | 937±3 | 4668 | [32] | |||
Kepler-202c | 0.165 | 16.282493 | 0.113 | transit | 937±3 | 4668 | [32] | |||
Kepler-203b | 0.229 | 3.162697 | 0.043 | transit | 2340±30 | 0.98 | 5821 | [32] | ||
Kepler-203c | 0.22 | 5.370647 | 0.061 | transit | 2340±30 | 0.98 | 5821 | [32] | ||
Kepler-203d | 0.128 | 11.32972 | 0.1 | transit | 2340±30 | 0.98 | 5821 | [32] | ||
Kepler-204b | 0.226 | 14.400974 | 0.117 | transit | 2280±20 | 0.96 | 5812 | [32] | ||
Kepler-204c | 0.16 | 25.660593 | 0.173 | transit | 2280±20 | 0.96 | 5812 | [32] | ||
Kepler-205b | 0.135 | 2.75564 | 0.032 | transit | 523.4±1.1 | 4321 | [32] | |||
Kepler-205c | 0.146 | 20.306546 | 0.122 | transit | 523.4±1.1 | 4321 | [32] | |||
Kepler-206b | 0.107 | 7.781987 | 0.078 | transit | 1972±16 | 0.94 | 5764 | [32] | ||
Kepler-206c | 0.158 | 13.137471 | 0.111 | transit | 1972±16 | 0.94 | 5764 | [32] | ||
Kepler-206d | 0.106 | 23.44281 | 0.163 | transit | 1972±16 | 0.94 | 5764 | [32] | ||
Kepler-207b | 0.14 | 1.611865 | 0.029 | transit | 2920±30 | 5920 | [32] | |||
Kepler-207c | 0.134 | 3.071571 | 0.044 | transit | 2920±30 | 5920 | [32] | |||
Kepler-207d | 0.295 | 5.868075 | 0.068 | transit | 2920±30 | 5920 | [32] | |||
Kepler-208b | 0.145 | 4.22864 | 0.054 | transit | 2580±20 | 1.03 | 6092 | [32] | ||
Kepler-208c | 0.124 | 7.466623 | 0.079 | transit | 2580±20 | 1.03 | 6092 | [32] | ||
Kepler-208d | 0.107 | 11.131786 | 0.103 | transit | 2580±20 | 1.03 | 6092 | [32] | ||
Kepler-208e | 0.132 | 16.259458 | 0.132 | transit | 2580±20 | 1.03 | 6092 | [32] | ||
Kepler-209b | 0.202 | 16.087845 | 0.122 | transit | 1913±18 | 5513 | [32] | |||
Kepler-209c | 0.277 | 41.749882 | 0.231 | transit | 1913±18 | 5513 | [32] | |||
Kepler-210b | 0.262 | 2.453234 | 0.032 | transit | 764±2 | 4559 | [32] | |||
Kepler-210c | 0.323 | 7.972513 | 0.07 | transit | 764±2 | 4559 | [32] | |||
Kepler-211b | 0.112 | 4.138575 | 0.048 | transit | 1018±5 | 0.97 | 5123 | [32] | ||
Kepler-211c | 0.115 | 6.04045 | 0.062 | transit | 1018±5 | 0.97 | 5123 | [32] | ||
Kepler-212b | 0.097 | 16.257582 | 0.133 | transit | 2280±20 | 1.16 | 5852 | [32] | ||
Kepler-212c | 0.244 | 31.805174 | 0.207 | transit | 2280±20 | 1.16 | 5852 | [32] | ||
Kepler-213b | 0.145 | 2.46236 | 0.036 | transit | 2100±20 | 0.94 | 5696 | [32] | ||
Kepler-213c | 0.209 | 4.822962 | 0.057 | transit | 2100±20 | 0.94 | 5696 | [32] | ||
Kepler-214b | 0.233 | 15.660544 | 0.13 | transit | 4080±70 | 6169 | [32] | |||
Kepler-214c | 0.19 | 28.7798 | 0.194 | transit | 4080±70 | 6169 | [32] | |||
Kepler-215b | 0.145 | 9.360672 | 0.084 | transit | 1607±12 | 0.77 | 5739 | [32] | ||
Kepler-215c | 0.158 | 14.667108 | 0.113 | transit | 1607±12 | 0.77 | 5739 | [32] | ||
Kepler-215d | 0.213 | 30.864423 | 0.185 | transit | 1607±12 | 0.77 | 5739 | [32] | ||
Kepler-215e | 0.156 | 68.16101 | 0.314 | transit | 1607±12 | 0.77 | 5739 | [32] | ||
Kepler-216b | 0.21 | 7.693641 | 0.079 | transit | 4000±70 | 6091 | [32] | |||
Kepler-216c | 0.271 | 17.406669 | 0.136 | transit | 4000±70 | 6091 | [32] | |||
Kepler-217b | 0.199 | 5.374943 | 0.065 | transit | 3720±50 | 6171 | [32] | |||
Kepler-217c | 0.165 | 8.586004 | 0.089 | transit | 3720±50 | 6171 | [32] | |||
Kepler-218b | 0.132 | 3.619337 | 0.046 | transit | 2180±20 | 5502 | [32] | |||
Kepler-218c | 0.28 | 44.699576 | 0.248 | transit | 2180±20 | 5502 | [32] | |||
Kepler-219b | 0.263 | 4.585512 | 0.057 | transit | 2620±30 | 5786 | [32] | |||
Kepler-219c | 0.319 | 22.714613 | 0.165 | transit | 2620±30 | 5786 | [32] | |||
Kepler-219d | 0.251 | 47.903645 | 0.272 | transit | 2620±30 | 5786 | [32] | |||
Kepler-220b | 0.072 | 4.159807 | 0.046 | transit | 560±2 | 4632 | [32] | |||
Kepler-220c | 0.14 | 9.034199 | 0.076 | transit | 560±2 | 4632 | [32] | |||
Kepler-220d | 0.087 | 28.122397 | 0.163 | transit | 560±2 | 4632 | [32] | |||
Kepler-220e | 0.119 | 45.902733 | 0.226 | transit | 560±2 | 4632 | [32] | |||
Kepler-221b | 0.153 | 2.795906 | 0.037 | transit | 1270±9 | 0.72 | 5243 | [32] | ||
Kepler-221c | 0.261 | 5.690586 | 0.059 | transit | 1270±9 | 0.72 | 5243 | [32] | ||
Kepler-221d | 0.244 | 10.04156 | 0.087 | transit | 1270±9 | 0.72 | 5243 | [32] | ||
Kepler-221e | 0.235 | 18.369917 | 0.13 | transit | 1270±9 | 0.72 | 5243 | [32] | ||
Kepler-222b | 0.282 | 3.936981 | 0.048 | transit | 2520±40 | 5433 | [32] | |||
Kepler-222c | 0.414 | 10.08881 | 0.091 | transit | 2520±40 | 5433 | [32] | |||
Kepler-222d | 0.329 | 28.081912 | 0.18 | transit | 2520±40 | 5433 | [32] | |||
Kepler-223b | 0.02328 | 0.267 | 7.38449 | transit | 6400±400 | 1.12 | [32] | |||
Kepler-223c | 0.01605 | 0.307 | 9.84564 | transit | 6400±400 | 1.12 | [32] | |||
Kepler-223d | 0.02517 | 0.467 | 14.78869 | transit | 6400±400 | 1.12 | [32] | |||
Kepler-223e | 0.0151 | 0.41 | 19.72567 | transit | 6400±400 | 1.12 | [32] | |||
Kepler-224b | 0.124 | 3.132924 | 0.038 | transit | 2600±60 | 0.74 | 5018 | [32] | ||
Kepler-224c | 0.278 | 5.925003 | 0.058 | transit | 2600±60 | 0.74 | 5018 | [32] | ||
Kepler-224d | 0.205 | 11.349393 | 0.089 | transit | 2600±60 | 0.74 | 5018 | [32] | ||
Kepler-224e | 0.176 | 18.643577 | 0.124 | transit | 2600±60 | 0.74 | 5018 | [32] | ||
Kepler-225b | 0.107 | 6.738975 | 0.056 | transit | 1850±40 | 3682 | [32] | |||
Kepler-225c | 0.164 | 18.794234 | 0.111 | transit | 1850±40 | 3682 | [32] | |||
Kepler-226b | 0.138 | 3.940997 | 0.047 | transit | 3280±80 | 0.86 | 5571 | [32] | ||
Kepler-226c | 0.203 | 5.349555 | 0.058 | transit | 3280±80 | 0.86 | 5571 | [32] | ||
Kepler-226d | 0.109 | 8.109044 | 0.076 | transit | 3280±80 | 0.86 | 5571 | [32] | ||
Kepler-227b | 0.277 | 9.488015 | 0.09 | transit | 3640±100 | 5854 | [32] | |||
Kepler-227c | 0.271 | 54.418694 | 0.29 | transit | 3640±100 | 5854 | [32] | |||
Kepler-228b | 0.136 | 2.566546 | 0.038 | transit | 5600±300 | 6043 | [32] | |||
Kepler-228c | 0.241 | 4.134444 | 0.052 | transit | 5600±300 | 6043 | [32] | |||
Kepler-228d | 0.36 | 11.094286 | 0.101 | transit | 5600±300 | 6043 | [32] | |||
Kepler-229b | 0.196 | 6.252972 | 0.062 | transit | 2750±70 | 5120 | [32] | |||
Kepler-229c | 0.439 | 16.068638 | 0.117 | transit | 2750±70 | 5120 | [32] | |||
Kepler-229d | 0.343 | 41.194912 | 0.22 | transit | 2750±70 | 5120 | [32] | |||
Kepler-230b | 0.38 | 32.625555 | 0.191 | transit | 2460±40 | 5588 | [32] | |||
Kepler-230c | 0.182 | 91.773242 | 0.38 | transit | 2460±40 | 5588 | [32] | |||
Kepler-231b | 0.154 | 10.065275 | 0.074 | transit | 988±9 | 0.58 | 3767 | [32] | ||
Kepler-231c | 0.172 | 19.271566 | 0.114 | transit | 988±9 | 0.58 | 3767 | [32] | ||
Kepler-232b | 0.275 | 4.431222 | 0.054 | transit | 4570±160 | 5847 | [32] | |||
Kepler-232c | 0.342 | 11.379349 | 0.101 | transit | 4570±160 | 5847 | [32] | |||
Kepler-233b | 0.217 | 8.472382 | 0.077 | transit | 2860±60 | 5360 | [32] | |||
Kepler-233c | 0.242 | 60.418955 | 0.287 | transit | 2860±60 | 5360 | [32] | |||
Kepler-234b | 0.33 | 2.711506 | 0.04 | transit | 5900±300 | 6224 | [32] | |||
Kepler-234c | 0.313 | 7.21205 | 0.077 | transit | 5900±300 | 6224 | [32] | |||
Kepler-235b | 0.199 | 3.340222 | 0.037 | transit | 1410±20 | 0.59 | 4255 | [32] | ||
Kepler-235c | 0.114 | 7.824904 | 0.065 | transit | 1410±20 | 0.59 | 4255 | [32] | ||
Kepler-235d | 0.183 | 20.060548 | 0.122 | transit | 1410±20 | 0.59 | 4255 | [32] | ||
Kepler-235e | 0.198 | 46.183669 | 0.213 | transit | 1410±20 | 0.59 | 4255 | [32] | ||
Kepler-236b | 0.14 | 8.295611 | 0.065 | transit | 949±7 | 0.56 | 3750 | [32] | ||
Kepler-236c | 0.178 | 23.968127 | 0.132 | transit | 949±7 | 0.56 | 3750 | [32] | ||
Kepler-237b | 0.126 | 4.715106 | 0.05 | transit | 2180±30 | 0.7 | 4861 | [32] | ||
Kepler-237c | 0.186 | 8.103636 | 0.071 | transit | 2180±30 | 0.7 | 4861 | [32] | ||
Kepler-238b | 0.154 | 2.090876 | 0.034 | transit | 6200±300 | 1.06 | 5751 | [32] | ||
Kepler-238c | 0.213 | 6.155557 | 0.069 | transit | 6200±300 | 1.06 | 5751 | [32] | ||
Kepler-238d | 0.274 | 13.233549 | 0.115 | transit | 6200±300 | 1.06 | 5751 | [32] | ||
Kepler-239b | 0.208 | 11.763051 | 0.095 | transit | 2150±40 | 0.74 | 4914 | [32] | ||
Kepler-239c | 0.224 | 56.228098 | 0.268 | transit | 2150±40 | 0.74 | 4914 | [32] | ||
Kepler-240b | 0.122 | 4.144495 | 0.048 | transit | 2480±60 | 4985 | [32] | |||
Kepler-240c | 0.196 | 7.953528 | 0.074 | transit | 2480±60 | 4985 | [32] | |||
Kepler-241b | 0.208 | 12.718092 | 0.094 | transit | 1980±130 | 4699 | [32] | |||
Kepler-241c | 0.229 | 36.065978 | 0.189 | transit | 1980±130 | 4699 | [32] | |||
Kepler-242b | 0.233 | 8.20395 | 0.075 | transit | 1990±30 | 5020 | [32] | |||
Kepler-242c | 0.178 | 14.496481 | 0.109 | transit | 1990±30 | 5020 | [32] | |||
Kepler-243b | 0.219 | 5.715442 | 0.062 | transit | 2300±30 | 0.89 | 5228 | [32] | ||
Kepler-243c | 0.178 | 20.026218 | 0.142 | transit | 2300±30 | 0.89 | 5228 | [32] | ||
Kepler-244b | 0.246 | 4.311792 | 0.05 | transit | 3480±120 | 5554 | [32] | |||
Kepler-244c | 0.183 | 9.767292 | 0.087 | transit | 3480±120 | 5554 | [32] | |||
Kepler-244d | 0.206 | 20.050401 | 0.14 | transit | 3480±120 | 5554 | [32] | |||
Kepler-245b | 0.229 | 7.49019 | 0.071 | transit | 2870±80 | 0.8 | 5100 | [32] | ||
Kepler-245c | 0.194 | 17.460812 | 0.124 | transit | 2870±80 | 0.8 | 5100 | [32] | ||
Kepler-245d | 0.27 | 36.277108 | 0.202 | transit | 2870±80 | 0.8 | 5100 | [32] | ||
Kepler-246b | 0.209 | 4.60182 | 0.052 | transit | 2070±20 | 0.86 | 5206 | [32] | ||
Kepler-246c | 0.134 | 11.187161 | 0.095 | transit | 2070±20 | 0.86 | 5206 | [32] | ||
Kepler-247b | 0.146 | 3.33616 | 0.042 | transit | 2200±40 | 5100 | [32] | |||
Kepler-247c | 0.365 | 9.439452 | 0.084 | transit | 2200±40 | 5100 | [32] | |||
Kepler-247d | 0.352 | 20.477912 | 0.14 | transit | 2200±40 | 5100 | [32] | |||
Kepler-248b | 0.269 | 6.308205 | 0.066 | transit | 2460±40 | 5190 | [32] | |||
Kepler-248c | 0.363 | 16.239494 | 0.123 | transit | 2460±40 | 5190 | [32] | |||
Kepler-249b | 0.097 | 3.306539 | 0.035 | transit | 624±3 | 3568 | [32] | |||
Kepler-249c | 0.135 | 7.113702 | 0.058 | transit | 624±3 | 3568 | [32] | |||
Kepler-249d | 0.14 | 15.368459 | 0.097 | transit | 624±3 | 3568 | [32] | |||
Kepler-250b | 0.101 | 4.148141 | 0.048 | transit | 2530±50 | 0.8 | 5160 | [32] | ||
Kepler-250c | 0.203 | 7.156804 | 0.069 | transit | 2530±50 | 0.8 | 5160 | [32] | ||
Kepler-250d | 0.194 | 17.648312 | 0.127 | transit | 2530±50 | 0.8 | 5160 | [32] | ||
Kepler-251b | 0.119 | 4.790936 | 0.053 | transit | 3090±90 | 0.91 | 5526 | [32] | ||
Kepler-251c | 0.247 | 16.514043 | 0.122 | transit | 3090±90 | 0.91 | 5526 | [32] | ||
Kepler-251d | 0.247 | 30.133001 | 0.182 | transit | 3090±90 | 0.91 | 5526 | [32] | ||
Kepler-251e | 0.247 | 99.640161 | 0.404 | transit | 3090±90 | 0.91 | 5526 | [32] | ||
Kepler-252b | 0.11 | 6.668391 | 0.058 | transit | 1251±11 | 0.52 | 4208 | [32] | ||
Kepler-252c | 0.192 | 10.848463 | 0.08 | transit | 1251±11 | 0.52 | 4208 | [32] | ||
Kepler-253b | 0.145 | 3.783986 | 0.046 | transit | 2800±60 | 5208 | [32] | |||
Kepler-253c | 0.236 | 10.281951 | 0.089 | transit | 2800±60 | 5208 | [32] | |||
Kepler-253d | 0.283 | 18.119869 | 0.13 | transit | 2800±60 | 5208 | [32] | |||
Kepler-254b | 0.345 | 5.826662 | 0.064 | transit | 4700±200 | 5957 | [32] | |||
Kepler-254c | 0.192 | 12.412183 | 0.105 | transit | 4700±200 | 5957 | [32] | |||
Kepler-254d | 0.223 | 18.746477 | 0.139 | transit | 4700±200 | 5957 | [32] | |||
Kepler-255b | 0.138 | 5.714606 | 0.063 | transit | 3530±100 | 0.97 | 5573 | [32] | ||
Kepler-255c | 0.267 | 9.946047 | 0.092 | transit | 3530±100 | 0.97 | 5573 | [32] | ||
Kepler-256b | 0.142 | 1.620493 | 0.027 | transit | 3440±80 | 1.02 | 5551 | [32] | ||
Kepler-256c | 0.192 | 3.38802 | 0.045 | transit | 3440±80 | 1.02 | 5551 | [32] | ||
Kepler-256d | 0.221 | 5.839172 | 0.064 | transit | 3440±80 | 1.02 | 5551 | [32] | ||
Kepler-256e | 0.21 | 10.681572 | 0.096 | transit | 3440±80 | 1.02 | 5551 | [32] | ||
Kepler-257b | 0.233 | 2.382667 | 0.034 | transit | 2600±50 | 5180 | [32] | |||
Kepler-257c | 0.483 | 6.581484 | 0.066 | transit | 2600±50 | 5180 | [32] | |||
Kepler-257d | 0.442 | 24.664551 | 0.16 | transit | 2600±50 | 5180 | [32] | |||
Kepler-258b | 0.362 | 13.19722 | 0.103 | transit | 1900±20 | 0.8 | 4942 | [32] | ||
Kepler-258c | 0.322 | 33.653079 | 0.193 | transit | 1900±20 | 0.8 | 4942 | [32] | ||
Kepler-259b | 0.25 | 8.115317 | 0.079 | transit | 3360±80 | 5938 | [32] | |||
Kepler-259c | 0.241 | 36.924931 | 0.217 | transit | 3360±80 | 5938 | [32] | |||
Kepler-260b | 0.179 | 8.187399 | 0.075 | transit | 2080±20 | 0.88 | 5250 | [32] | ||
Kepler-260c | 0.155 | 76.050178 | 0.332 | transit | 2080±20 | 0.88 | 5250 | [32] | ||
Kepler-261b | 0.194 | 10.381227 | 0.088 | transit | 1044±5 | 0.87 | 5098 | [32] | ||
Kepler-261c | 0.178 | 24.570858 | 0.156 | transit | 1044±5 | 0.87 | 5098 | [32] | ||
Kepler-262b | 0.121 | 13.060855 | 0.108 | transit | 2030±20 | 5841 | [32] | |||
Kepler-262c | 0.146 | 21.853722 | 0.152 | transit | 2030±20 | 5841 | [32] | |||
Kepler-263b | 0.238 | 16.568087 | 0.12 | transit | 2510±50 | 5265 | [32] | |||
Kepler-263c | 0.22 | 47.332773 | 0.242 | transit | 2510±50 | 5265 | [32] | |||
Kepler-264b | 0.297 | 40.806231 | 0.249 | transit | 3150±60 | 1.32 | 6158 | [32] | ||
Kepler-264c | 0.252 | 140.101261 | 0.566 | transit | 3150±60 | 1.32 | 6158 | [32] | ||
Kepler-265b | 0.166 | 6.846262 | 0.069 | transit | 4330±160 | 1.03 | 5835 | [32] | ||
Kepler-265c | 0.235 | 17.028937 | 0.127 | transit | 4330±160 | 1.03 | 5835 | [32] | ||
Kepler-265d | 0.222 | 43.130617 | 0.236 | transit | 4330±160 | 1.03 | 5835 | [32] | ||
Kepler-265e | 0.231 | 67.831024 | 0.319 | transit | 4330±160 | 1.03 | 5835 | [32] | ||
Kepler-266b | 0.221 | 6.61833 | 0.071 | transit | 4640±190 | 0.99 | 5885 | [32] | ||
Kepler-266c | 0.347 | 107.723601 | 0.457 | transit | 4640±190 | 0.99 | 5885 | [32] | ||
Kepler-267b | 0.177 | 3.353728 | 0.037 | transit | 870±8 | 0.56 | 4258 | [32] | ||
Kepler-267c | 0.19 | 6.87745 | 0.06 | transit | 870±8 | 0.56 | 4258 | [32] | ||
Kepler-267d | 0.203 | 28.464515 | 0.154 | transit | 870±8 | 0.56 | 4258 | [32] | ||
Kepler-268b | 0.227 | 25.934138 | 0.18 | transit | 2840±30 | 6081 | [32] | |||
Kepler-268c | 0.302 | 83.446393 | 0.391 | transit | 2840±30 | 6081 | [32] | |||
Kepler-269b | 0.22 | 5.326718 | 0.061 | transit | 7900±600 | 0.98 | 5847 | [32] | ||
Kepler-269c | 0.151 | 8.127899 | 0.081 | transit | 7900±600 | 0.98 | 5847 | [32] | ||
Kepler-270b | 0.179 | 11.476094 | 0.107 | transit | 3180±40 | 6067 | [32] | |||
Kepler-270c | 0.158 | 25.262887 | 0.18 | transit | 3180±40 | 6067 | [32] | |||
Kepler-271b | 0.079 | 5.217738 | 0.056 | transit | 1334±12 | 5524 | [32] | |||
Kepler-271c | 0.089 | 7.410935 | 0.071 | transit | 1334±12 | 5524 | [32] | |||
Kepler-272b | 0.128 | 2.971353 | 0.038 | transit | 2970±40 | 0.79 | 5297 | [32] | ||
Kepler-272c | 0.16 | 6.057342 | 0.061 | transit | 2970±40 | 0.79 | 5297 | [32] | ||
Kepler-272d | 0.201 | 10.937304 | 0.091 | transit | 2970±40 | 0.79 | 5297 | [32] | ||
Kepler-273b | 0.134 | 2.936532 | 0.037 | transit | 2370±30 | 5626 | [32] | |||
Kepler-273c | 0.177 | 8.014927 | 0.073 | transit | 2370±30 | 5626 | [32] | |||
Kepler-274b | 0.137 | 11.634788 | 0.101 | transit | 4510±140 | 6023 | [32] | |||
Kepler-274c | 0.164 | 33.197861 | 0.204 | transit | 4510±140 | 6023 | [32] | |||
Kepler-275b | 0.209 | 10.300682 | 0.098 | transit | 7000±500 | 1.24 | 6165 | [32] | ||
Kepler-275c | 0.302 | 16.088134 | 0.132 | transit | 7000±500 | 1.24 | 6165 | [32] | ||
Kepler-275d | 0.297 | 35.676062 | 0.224 | transit | 7000±500 | 1.24 | 6165 | [32] | ||
Kepler-276b | 0.256 | 14.12841 | 0.119 | transit | 3850±150 | 1.1 | 6105 | [32] | ||
Kepler-278b | 0.363 | 30.160546 | 0.207 | transit | 1460±20 | 4991 | [32] | |||
Kepler-278c | 0.32 | 51.078775 | 0.294 | transit | 1460±20 | 4991 | [32] | |||
Kepler-280b | 0.129 | 2.139542 | 0.032 | transit | 2600±30 | 0.91 | 5744 | [32] | ||
Kepler-280c | 0.179 | 4.807091 | 0.056 | transit | 2600±30 | 0.91 | 5744 | [32] | ||
Kepler-281b | 0.252 | 14.646008 | 0.117 | transit | 6000±300 | 0.98 | 5723 | [32] | ||
Kepler-281c | 0.474 | 36.337373 | 0.215 | transit | 6000±300 | 0.98 | 5723 | [32] | ||
Kepler-282b | 0.09 | 9.220524 | 0.082 | transit | 4530±150 | 0.97 | 5602 | [32] | ||
Kepler-282c | 0.107 | 13.638723 | 0.106 | transit | 4530±150 | 0.97 | 5602 | [32] | ||
Kepler-283b | 0.19 | 11.008151 | 0.082 | transit | 1540±20 | 4351 | [32] | |||
Kepler-283c | 0.162 | 92.743711 | 0.341 | transit | 1540±20 | 4351 | [32] | |||
Kepler-284b | 0.2 | 12.699149 | 0.104 | transit | 3460±110 | 5615 | [32] | |||
Kepler-284c | 0.233 | 37.514456 | 0.213 | transit | 3460±110 | 5615 | [32] | |||
Kepler-285b | 0.12 | 2.633867 | 0.036 | transit | 2750±50 | 0.85 | 5411 | [32] | ||
Kepler-285c | 0.1 | 6.186676 | 0.064 | transit | 2750±50 | 0.85 | 5411 | [32] | ||
Kepler-286b | 0.111 | 1.796302 | 0.027 | transit | 4100±400 | 5580 | [32] | |||
Kepler-286c | 0.122 | 3.468095 | 0.042 | transit | 4100±400 | 5580 | [32] | |||
Kepler-286d | 0.119 | 5.914323 | 0.061 | transit | 4100±400 | 5580 | [32] | |||
Kepler-286e | 0.158 | 29.221289 | 0.176 | transit | 4100±400 | 5580 | [32] | |||
Kepler-287b | 0.208 | 20.342199 | 0.145 | transit | 2790±50 | 5806 | [32] | |||
Kepler-287c | 0.291 | 44.851896 | 0.246 | transit | 2790±50 | 5806 | [32] | |||
Kepler-288b | 0.149 | 6.097326 | 0.065 | transit | 4030±110 | 0.89 | 5918 | [32] | ||
Kepler-288c | 0.254 | 19.305772 | 0.14 | transit | 4030±110 | 0.89 | 5918 | [32] | ||
Kepler-288d | 0.238 | 56.633742 | 0.287 | transit | 4030±110 | 0.89 | 5918 | [32] | ||
Kepler-289b | 0.023 | 0.192 | 34.545 | 0.21 | transit | 2340±20 | 1.08 | 5990 | [32] | |
Kepler-289c | 0.42 | 1.034 | 125.8518 | 0.51 | transit | 2340±20 | 1.08 | 5990 | [32] | |
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 | [32] | |||
Kepler-290c | 0.241 | 36.77031 | 0.205 | transit | 2310±40 | 5147 | [32] | |||
Kepler-291b | 0.193 | 3.546511 | 0.047 | transit | 6100±400 | 1.03 | 6002 | [32] | ||
Kepler-291c | 0.168 | 5.700786 | 0.065 | transit | 6100±400 | 1.03 | 6002 | [32] | ||
Kepler-292b | 0.118 | 2.580827 | 0.035 | transit | 3540±150 | 0.88 | 5299 | [32] | ||
Kepler-292c | 0.131 | 3.715335 | 0.045 | transit | 3540±150 | 0.88 | 5299 | [32] | ||
Kepler-292d | 0.199 | 7.055679 | 0.068 | transit | 3540±150 | 0.88 | 5299 | [32] | ||
Kepler-292e | 0.238 | 11.97901 | 0.097 | transit | 3540±150 | 0.88 | 5299 | [32] | ||
Kepler-292f | 0.21 | 20.834237 | 0.141 | transit | 3540±150 | 0.88 | 5299 | [32] | ||
Kepler-293b | 0.274 | 19.254196 | 0.144 | transit | 3260±70 | 1.01 | 5804 | [32] | ||
Kepler-293c | 0.342 | 54.155743 | 0.286 | transit | 3260±70 | 1.01 | 5804 | [32] | ||
Kepler-294b | 0.158 | 3.701212 | 0.048 | transit | 4600±200 | 5913 | [32] | |||
Kepler-294c | 0.242 | 6.6264 | 0.071 | transit | 4600±200 | 5913 | [32] | |||
Kepler-295b | 0.109 | 12.645164 | 0.099 | transit | 5800±300 | 5603 | [32] | |||
Kepler-295c | 0.104 | 21.526258 | 0.142 | transit | 5800±300 | 5603 | [32] | |||
Kepler-295d | 0.121 | 33.884054 | 0.192 | transit | 5800±300 | 5603 | [32] | |||
Kepler-296b | 0.144 | 10.864384 | 0.079 | transit | 740 | 0.5 | 3740 | [32] | ||
Kepler-296c | 0.178 | 5.8416366 | 0.0521 | transit | 740 | 0.5 | 3740 | [32] | ||
Kepler-296d | 0.186 | 19.850291 | 0.118 | transit | 740 | 0.5 | 3740 | [32] | ||
Kepler-296e | 0.136 | 34.14211 | 0.169 | transit | 740 | 0.5 | 3740 | [32] | ||
Kepler-296f | 0.161 | 63.33627 | 0.255 | transit | 740 | 0.5 | 3740 | [32] | ||
Kepler-297b | 0.256 | 38.871826 | 0.217 | transit | 2300±20 | 5619 | [32] | |||
Kepler-297c | 0.583 | 74.920137 | 0.336 | transit | 2300±20 | 5619 | [32] | |||
Kepler-298b | 0.175 | 10.475464 | 0.08 | transit | 1710±20 | 0.65 | 4465 | [32] | ||
Kepler-298c | 0.172 | 22.92881 | 0.136 | transit | 1710±20 | 0.65 | 4465 | [32] | ||
Kepler-298d | 0.223 | 77.473633 | 0.305 | transit | 1710±20 | 0.65 | 4465 | [32] | ||
Kepler-299b | 0.118 | 2.927128 | 0.04 | transit | 3530±80 | 0.97 | 5617 | [32] | ||
Kepler-299c | 0.236 | 6.885875 | 0.07 | transit | 3530±80 | 0.97 | 5617 | [32] | ||
Kepler-299d | 0.166 | 15.054786 | 0.118 | transit | 3530±80 | 0.97 | 5617 | [32] | ||
Kepler-299e | 0.167 | 38.285489 | 0.22 | transit | 3530±80 | 0.97 | 5617 | [32] | ||
Kepler-300b | 0.149 | 10.446347 | 0.094 | transit | 3690±60 | 0.94 | 5986 | [32] | ||
Kepler-300c | 0.201 | 40.714955 | 0.232 | transit | 3690±60 | 0.94 | 5986 | [32] | ||
Kepler-301b | 0.12 | 2.508553 | 0.036 | transit | 2390±30 | 0.91 | 5815 | [32] | ||
Kepler-301c | 0.12 | 5.419026 | 0.06 | transit | 2390±30 | 0.91 | 5815 | [32] | ||
Kepler-301d | 0.156 | 13.751243 | 0.112 | transit | 2390±30 | 0.91 | 5815 | [32] | ||
Kepler-302b | 0.362 | 30.184104 | 0.193 | transit | 4760±190 | 5740 | [32] | |||
Kepler-302c | 1.111 | 127.282184 | 0.503 | transit | 4760±190 | 5740 | [32] | |||
Kepler-303b | 0.079 | 1.937055 | 0.024 | transit | 688±3 | 0.59 | 3944 | [32] | ||
Kepler-303c | 0.102 | 7.061149 | 0.057 | transit | 688±3 | 0.59 | 3944 | [32] | ||
Kepler-304b | 0.255 | 3.295709 | 0.039 | transit | 1435±17 | 0.8 | 4731 | [32] | ||
Kepler-304c | 0.194 | 5.315946 | 0.054 | transit | 1435±17 | 0.8 | 4731 | [32] | ||
Kepler-304d | 0.245 | 9.653471 | 0.08 | transit | 1435±17 | 0.8 | 4731 | [32] | ||
Kepler-305d | 0.242 | 16.738661 | 0.121 | transit | 2900±80 | 0.76 | 5100 | [32] | ||
Kepler-306b | 0.136 | 4.646186 | 0.05 | transit | 2580±60 | 0.82 | 4954 | [32] | ||
Kepler-306c | 0.21 | 7.240193 | 0.067 | transit | 2580±60 | 0.82 | 4954 | [32] | ||
Kepler-306d | 0.22 | 17.326644 | 0.12 | transit | 2580±60 | 0.82 | 4954 | [32] | ||
Kepler-306e | 0.203 | 44.840975 | 0.227 | transit | 2580±60 | 0.82 | 4954 | [32] | ||
Kepler-308b | 0.189 | 9.694928 | 0.09 | transit | 4500±200 | 5895 | [32] | |||
Kepler-308c | 0.193 | 15.38231 | 0.123 | transit | 4500±200 | 5895 | [32] | |||
Kepler-309b | 0.139 | 5.923653 | 0.059 | transit | 1804±19 | 4713 | [32] | |||
Kepler-309c | 0.224 | 105.356383 | 0.401 | transit | 1804±19 | 4713 | [32] | |||
Kepler-310b | 0.106 | 13.930698 | 0.111 | transit | 1990±20 | 0.85 | 5797 | [32] | ||
Kepler-310c | 0.302 | 56.47542 | 0.281 | transit | 1990±20 | 0.85 | 5797 | [32] | ||
Kepler-310d | 0.22 | 92.876125 | 0.392 | transit | 1990±20 | 0.85 | 5797 | [32] | ||
Kepler-311b | 0.152 | 9.176092 | 0.087 | transit | 2590±30 | 1.06 | 5905 | [32] | ||
Kepler-311c | 0.128 | 19.738286 | 0.145 | transit | 2590±30 | 1.06 | 5905 | [32] | ||
Kepler-312b | 0.115 | 1.772419 | 0.031 | transit | 2660±40 | 1.23 | 6115 | [32] | ||
Kepler-312c | 0.281 | 19.747412 | 0.153 | transit | 2660±40 | 1.23 | 6115 | [32] | ||
Kepler-313b | 0.226 | 14.970418 | 0.125 | transit | 3500±300 | 0.9 | 5727 | [32] | ||
Kepler-313c | 0.229 | 32.273273 | 0.208 | transit | 3500±300 | 0.9 | 5727 | [32] | ||
Kepler-314b | 0.074 | 2.461069 | 0.035 | transit | 883±5 | 1.02 | 5378 | [32] | ||
Kepler-314c | 0.259 | 5.960392 | 0.064 | transit | 883±5 | 1.02 | 5378 | [32] | ||
Kepler-315b | 0.336 | 96.101141 | 0.402 | transit | 3910±120 | 0.78 | 5796 | [32] | ||
Kepler-315c | 0.37 | 265.469335 | 0.791 | transit | 3910±120 | 0.78 | 5796 | [32] | ||
Kepler-316b | 0.095 | 2.240508 | 0.027 | transit | 1269±12 | 0.53 | 4204 | [32] | ||
Kepler-316c | 0.103 | 6.827766 | 0.058 | transit | 1269±12 | 0.53 | 4204 | [32] | ||
Kepler-317b | 0.186 | 5.524242 | 0.061 | transit | 3150±80 | 0.95 | 5497 | [32] | ||
Kepler-317c | 0.153 | 8.77501 | 0.083 | transit | 3150±80 | 0.95 | 5497 | [32] | ||
Kepler-318b | 0.42 | 4.662715 | 0.056 | transit | 1618±10 | 1.05 | 5746 | [32] | ||
Kepler-318c | 0.328 | 11.815007 | 0.105 | transit | 1618±10 | 1.05 | 5746 | [32] | ||
Kepler-319b | 0.145 | 4.362705 | 0.051 | transit | 1666±15 | 1.29 | 5526 | [32] | ||
Kepler-319c | 0.235 | 6.941357 | 0.069 | transit | 1666±15 | 1.29 | 5526 | [32] | ||
Kepler-319d | 0.204 | 31.781925 | 0.191 | transit | 1666±15 | 1.29 | 5526 | [32] | ||
Kepler-320b | 0.102 | 8.371554 | 0.085 | transit | 2760±30 | 6435 | [32] | |||
Kepler-320c | 0.122 | 17.934937 | 0.142 | transit | 2760±30 | 6435 | [32] | |||
Kepler-321b | 0.158 | 4.915379 | 0.057 | transit | 1268±11 | 1.01 | 5740 | [32] | ||
Kepler-321c | 0.207 | 13.093921 | 0.11 | transit | 1268±11 | 1.01 | 5740 | [32] | ||
Kepler-322b | 0.09 | 1.653888 | 0.027 | transit | 1321±8 | 0.91 | 5388 | [32] | ||
Kepler-322c | 0.149 | 4.337234 | 0.051 | transit | 1321±8 | 0.91 | 5388 | [32] | ||
Kepler-323b | 0.128 | 1.678327 | 0.028 | transit | 1500±20 | 1.09 | 5987 | [32] | ||
Kepler-323c | 0.145 | 3.553822 | 0.046 | transit | 1500±20 | 1.09 | 5987 | [32] | ||
Kepler-324b | 0.102 | 4.385315 | 0.05 | transit | 1659±12 | 0.86 | 5194 | [32] | ||
Kepler-324c | 0.281 | 51.805612 | 0.26 | transit | 1659±12 | 0.86 | 5194 | [32] | ||
Kepler-325b | 0.26 | 4.544439 | 0.053 | transit | 2740±40 | 0.87 | 5752 | [32] | ||
Kepler-325c | 0.227 | 12.762172 | 0.105 | transit | 2740±40 | 0.87 | 5752 | [32] | ||
Kepler-325d | 0.249 | 38.715185 | 0.22 | transit | 2740±40 | 0.87 | 5752 | [32] | ||
Kepler-326b | 0.136 | 2.248329 | 0.032 | transit | 1610±30 | 0.98 | 5105 | [32] | ||
Kepler-326c | 0.125 | 4.580358 | 0.051 | transit | 1610±30 | 0.98 | 5105 | [32] | ||
Kepler-326d | 0.108 | 6.766888 | 0.066 | transit | 1610±30 | 0.98 | 5105 | [32] | ||
Kepler-327b | 0.099 | 2.549575 | 0.029 | transit | 794±4 | 0.55 | 3799 | [32] | ||
Kepler-327c | 0.092 | 5.212333 | 0.047 | transit | 794±4 | 0.55 | 3799 | [32] | ||
Kepler-327d | 0.154 | 13.969457 | 0.09 | transit | 794±4 | 0.55 | 3799 | [32] | ||
Kepler-329b | 0.125 | 7.416397 | 0.061 | transit | 1450±20 | 0.53 | 4257 | [32] | ||
Kepler-329c | 0.172 | 18.684737 | 0.113 | transit | 1450±20 | 0.53 | 4257 | [32] | ||
Kepler-330b | 0.12 | 8.25978 | 0.075 | transit | 2380±40 | 0.78 | 5117 | [32] | ||
Kepler-330c | 0.174 | 15.955387 | 0.116 | transit | 2380±40 | 0.78 | 5117 | [32] | ||
Kepler-331b | 0.162 | 8.457496 | 0.065 | transit | 1920±40 | 0.51 | 4347 | [32] | ||
Kepler-331c | 0.164 | 17.28111 | 0.105 | transit | 1920±40 | 0.51 | 4347 | [32] | ||
Kepler-331d | 0.146 | 32.134328 | 0.159 | transit | 1920±40 | 0.51 | 4347 | [32] | ||
Kepler-332b | 0.104 | 7.626324 | 0.07 | transit | 1133±5 | 0.8 | 4955 | [32] | ||
Kepler-332c | 0.097 | 15.995622 | 0.114 | transit | 1133±5 | 0.8 | 4955 | [32] | ||
Kepler-332d | 0.105 | 34.21154 | 0.189 | transit | 1133±5 | 0.8 | 4955 | [32] | ||
Kepler-333b | 0.118 | 12.551158 | 0.087 | transit | 1068±7 | 0.54 | 4259 | [32] | ||
Kepler-333c | 0.099 | 24.08821 | 0.135 | transit | 1068±7 | 0.54 | 4259 | [32] | ||
Kepler-334b | 0.1 | 5.470319 | 0.061 | transit | 1408±14 | 1 | 5828 | [32] | ||
Kepler-334c | 0.128 | 12.758005 | 0.107 | transit | 1408±14 | 1 | 5828 | [32] | ||
Kepler-334d | 0.126 | 25.09849 | 0.168 | transit | 1408±14 | 1 | 5828 | [32] | ||
Kepler-335b | 0.302 | 6.562331 | 0.075 | transit | 4320±100 | 0.99 | 5877 | [32] | ||
Kepler-335c | 0.274 | 67.844469 | 0.356 | transit | 4320±100 | 0.99 | 5877 | [32] | ||
Kepler-336b | 0.091 | 2.024823 | 0.033 | transit | 8000±7000 | 0.89 | 5867 | [32] | ||
Kepler-336c | 0.187 | 9.600001 | 0.092 | transit | 8000±7000 | 0.89 | 5867 | [32] | ||
Kepler-336d | 0.211 | 20.678772 | 0.154 | transit | 8000±7000 | 0.89 | 5867 | [32] | ||
Kepler-337b | 0.137 | 3.292781 | 0.045 | transit | 2250±30 | 0.96 | 5684 | [32] | ||
Kepler-337c | 0.183 | 9.693201 | 0.093 | transit | 2250±30 | 0.96 | 5684 | [32] | ||
Kepler-338b | 0.218 | 13.726976 | 0.117 | transit | 1830±20 | 1.1 | 5923 | [32] | ||
Kepler-338c | 0.209 | 24.310856 | 0.172 | transit | 1830±20 | 1.1 | 5923 | [32] | ||
Kepler-338d | 0.268 | 44.431014 | 0.257 | transit | 1830±20 | 1.1 | 5923 | [32] | ||
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 | [32] | ||
Kepler-339c | 0.103 | 6.988055 | 0.069 | transit | 2040±30 | 0.84 | 5631 | [32] | ||
Kepler-339d | 0.104 | 10.558345 | 0.091 | transit | 2040±30 | 0.84 | 5631 | [32] | ||
Kepler-340b | 0.226 | 14.844387 | 0.134 | transit | 2690±60 | 2.11 | 6620 | [32] | ||
Kepler-340c | 0.301 | 22.824669 | 0.178 | transit | 2690±60 | 2.11 | 6620 | [32] | ||
Kepler-341b | 0.105 | 5.195528 | 0.06 | transit | 3520±60 | 0.94 | 6012 | [32] | ||
Kepler-341c | 0.152 | 8.01041 | 0.08 | transit | 3520±60 | 0.94 | 6012 | [32] | ||
Kepler-341d | 0.165 | 27.666313 | 0.182 | transit | 3520±60 | 0.94 | 6012 | [32] | ||
Kepler-341e | 0.178 | 42.473269 | 0.242 | transit | 3520±60 | 0.94 | 6012 | [32] | ||
Kepler-342b | 0.201 | 15.170318 | 0.128 | transit | 2600±30 | 1.13 | 6175 | [32] | ||
Kepler-342c | 0.175 | 26.234138 | 0.185 | transit | 2600±30 | 1.13 | 6175 | [32] | ||
Kepler-342d | 0.222 | 39.459357 | 0.242 | transit | 2600±30 | 1.13 | 6175 | [32] | ||
Kepler-343b | 0.215 | 8.96855 | 0.088 | transit | 3100±60 | 1.04 | 5807 | [32] | ||
Kepler-343c | 0.18 | 23.22182 | 0.167 | transit | 3100±60 | 1.04 | 5807 | [32] | ||
Kepler-344b | 0.233 | 21.963945 | 0.153 | transit | 3360±100 | 0.9 | 5774 | [32] | ||
Kepler-344c | 0.263 | 125.596809 | 0.488 | transit | 3360±100 | 0.9 | 5774 | [32] | ||
Kepler-345b | 0.066 | 7.415563 | 0.066 | transit | 1180±50 | 0.59 | 4504 | [32] | ||
Kepler-345c | 0.107 | 9.387427 | 0.077 | transit | 1180±50 | 0.59 | 4504 | [32] | ||
Kepler-346b | 0.237 | 6.511127 | 0.071 | transit | 3300±80 | 0.97 | 6033 | [32] | ||
Kepler-346c | 0.274 | 23.851549 | 0.168 | transit | 3300±80 | 0.97 | 6033 | [32] | ||
Kepler-347b | 0.176 | 12.79836 | 0.11 | transit | 4400±90 | 1.04 | 6088 | [32] | ||
Kepler-347c | 0.156 | 27.320871 | 0.183 | transit | 4400±90 | 1.04 | 6088 | [32] | ||
Kepler-348b | 0.136 | 7.05677 | 0.076 | transit | 1890±20 | 1.15 | 6177 | [32] | ||
Kepler-348c | 0.119 | 17.265427 | 0.138 | transit | 1890±20 | 1.15 | 6177 | [32] | ||
Kepler-349b | 0.17 | 5.929778 | 0.065 | transit | 3150±60 | 0.97 | 5956 | [32] | ||
Kepler-349c | 0.175 | 12.247629 | 0.105 | transit | 3150±60 | 0.97 | 5956 | [32] | ||
Kepler-350b | 0.165 | 11.189562 | 0.104 | transit | 3200±60 | 1 | 6186 | [32] | ||
Kepler-351b | 0.273 | 37.054919 | 0.214 | transit | 3640±40 | 0.89 | 5643 | [32] | ||
Kepler-351c | 0.285 | 57.24809 | 0.287 | transit | 3640±40 | 0.89 | 5643 | [32] | ||
Kepler-352b | 0.077 | 10.05537 | 0.085 | transit | 830±4 | 0.79 | 5212 | [32] | ||
Kepler-352c | 0.111 | 16.332995 | 0.118 | transit | 830±4 | 0.79 | 5212 | [32] | ||
Kepler-353b | 0.079 | 5.795278 | 0.051 | transit | 1268±16 | 0.54 | 3903 | [32] | ||
Kepler-353c | 0.123 | 8.410894 | 0.065 | transit | 1268±16 | 0.54 | 3903 | [32] | ||
Kepler-354b | 0.164 | 5.47666 | 0.054 | transit | 1830±20 | 0.65 | 4648 | [32] | ||
Kepler-354c | 0.117 | 16.934402 | 0.115 | transit | 1830±20 | 0.65 | 4648 | [32] | ||
Kepler-354d | 0.111 | 24.209842 | 0.146 | transit | 1830±20 | 0.65 | 4648 | [32] | ||
Kepler-355b | 0.13 | 11.03189 | 0.102 | transit | 4870±160 | 1.05 | 6184 | [32] | ||
Kepler-355c | 0.242 | 25.762294 | 0.179 | transit | 4870±160 | 1.05 | 6184 | [32] | ||
Kepler-356b | 0.14 | 4.612696 | 0.057 | transit | 2350±30 | 0.97 | 6133 | [32] | ||
Kepler-356c | 0.161 | 13.121632 | 0.115 | transit | 2350±30 | 0.97 | 6133 | [32] | ||
Kepler-357b | 0.164 | 6.475434 | 0.063 | transit | 2290±40 | 0.78 | 5036 | [32] | ||
Kepler-357c | 0.238 | 16.85837 | 0.12 | transit | 2290±40 | 0.78 | 5036 | [32] | ||
Kepler-357d | 0.306 | 49.499875 | 0.246 | transit | 2290±40 | 0.78 | 5036 | [32] | ||
Kepler-358b | 0.243 | 34.060467 | 0.21 | transit | 3700±130 | 0.95 | 5908 | [32] | ||
Kepler-358c | 0.254 | 83.488369 | 0.381 | transit | 3700±130 | 0.95 | 5908 | [32] | ||
Kepler-359b | 0.315 | 25.563222 | 0.178 | transit | 4900±300 | 1.07 | 6248 | [32] | ||
Kepler-359c | 0.384 | 57.68802 | 0.307 | transit | 4900±300 | 1.07 | 6248 | [32] | ||
Kepler-359d | 0.358 | 77.095691 | 0.372 | transit | 4900±300 | 1.07 | 6248 | [32] | ||
Kepler-360b | 0.147 | 3.289672 | 0.044 | transit | 2930±50 | 0.95 | 6053 | [32] | ||
Kepler-360c | 0.187 | 7.186434 | 0.075 | transit | 2930±50 | 0.95 | 6053 | [32] | ||
Kepler-361b | 0.129 | 8.486616 | 0.086 | transit | 3110±50 | 1.07 | 6169 | [32] | ||
Kepler-361c | 0.225 | 55.188023 | 0.3 | transit | 3110±50 | 1.07 | 6169 | [32] | ||
Kepler-362b | 0.079 | 10.327186 | 0.087 | transit | 3660±180 | 0.77 | 5788 | [32] | ||
Kepler-362c | 0.129 | 37.866281 | 0.207 | transit | 3660±180 | 0.77 | 5788 | [32] | ||
Kepler-363b | 0.103 | 3.614568 | 0.048 | transit | 2540±20 | 1.23 | 5593 | [32] | ||
Kepler-363c | 0.151 | 7.542427 | 0.079 | transit | 2540±20 | 1.23 | 5593 | [32] | ||
Kepler-363d | 0.183 | 11.932125 | 0.107 | transit | 2540±20 | 1.23 | 5593 | [32] | ||
Kepler-364b | 0.138 | 25.745718 | 0.178 | transit | 2980±30 | 1.2 | 6108 | [32] | ||
Kepler-364c | 0.192 | 59.980627 | 0.312 | transit | 2980±30 | 1.2 | 6108 | [32] | ||
Kepler-365b | 0.182 | 10.664903 | 0.098 | transit | 2800±200 | 0.99 | 6012 | [32] | ||
Kepler-365c | 0.146 | 17.784129 | 0.137 | transit | 2800±200 | 0.99 | 6012 | [32] | ||
Kepler-366b | 0.13 | 3.281959 | 0.045 | transit | 6400±400 | 1.05 | 6209 | [32] | ||
Kepler-366c | 0.16 | 12.51616 | 0.11 | transit | 6400±400 | 1.05 | 6209 | [32] | ||
Kepler-367b | 0.116 | 37.815724 | 0.201 | transit | 616±2 | 0.75 | 4710 | [32] | ||
Kepler-367c | 0.107 | 53.578637 | 0.253 | transit | 616±2 | 0.75 | 4710 | [32] | ||
Kepler-368b | 0.291 | 26.84768 | 0.186 | transit | 2570±40 | 0.71 | 5502 | [32] | ||
Kepler-368c | 0.346 | 72.379334 | 0.36 | transit | 2570±40 | 0.71 | 5502 | [32] | ||
Kepler-369b | 0.101 | 2.732756 | 0.03 | transit | 840±120 | 0.54 | 3591 | [32] | ||
Kepler-369c | 0.126 | 14.871572 | 0.094 | transit | 840±120 | 0.54 | 3591 | [32] | ||
Kepler-370b | 0.142 | 4.57953 | 0.054 | transit | 3930±120 | 0.94 | 5852 | [32] | ||
Kepler-370c | 0.17 | 19.02293 | 0.14 | transit | 3930±120 | 0.94 | 5852 | [32] | ||
Kepler-371b | 0.169 | 34.763278 | 0.2 | transit | 2710±40 | 0.94 | 5666 | [32] | ||
Kepler-371c | 0.159 | 67.968015 | 0.313 | transit | 2710±40 | 0.94 | 5666 | [32] | ||
Kepler-372b | 0.121 | 6.849692 | 0.075 | transit | 5090±170 | 1.15 | 6509 | [32] | ||
Kepler-372c | 0.186 | 20.053763 | 0.154 | transit | 5090±170 | 1.15 | 6509 | [32] | ||
Kepler-372d | 0.151 | 30.092568 | 0.201 | transit | 5090±170 | 1.15 | 6509 | [32] | ||
Kepler-373b | 0.121 | 5.535309 | 0.06 | transit | 3670±70 | 0.87 | 5787 | [32] | ||
Kepler-373c | 0.111 | 16.725948 | 0.126 | transit | 3670±70 | 0.87 | 5787 | [32] | ||
Kepler-374b | 0.092 | 1.897806 | 0.029 | transit | 4280±120 | 0.84 | 5977 | [32] | ||
Kepler-374c | 0.098 | 3.282807 | 0.042 | transit | 4280±120 | 0.84 | 5977 | [32] | ||
Kepler-374d | 0.117 | 5.028219 | 0.056 | transit | 4280±120 | 0.84 | 5977 | [32] | ||
Kepler-375b | 0.129 | 12.125934 | 0.101 | transit | 4180±180 | 0.89 | 5826 | [32] | ||
Kepler-375c | 0.236 | 19.986326 | 0.141 | transit | 4180±180 | 0.89 | 5826 | [32] | ||
Kepler-376b | 0.095 | 4.920199 | 0.057 | transit | 3090±50 | 1.05 | 5900 | [32] | ||
Kepler-376c | 0.16 | 14.172327 | 0.115 | transit | 3090±50 | 1.05 | 5900 | [32] | ||
Kepler-377b | 0.124 | 12.509529 | 0.109 | transit | 2750±40 | 0.88 | 5949 | [32] | ||
Kepler-377c | 0.184 | 27.014976 | 0.182 | transit | 2750±40 | 0.88 | 5949 | [32] | ||
Kepler-378b | 0.067 | 16.092361 | 0.112 | transit | 498.3±1.4 | 0.96 | 4661 | [32] | ||
Kepler-378c | 0.062 | 28.906009 | 0.166 | transit | 498.3±1.4 | 0.96 | 4661 | [32] | ||
Kepler-379b | 0.148 | 20.09838 | 0.152 | transit | 2430±20 | 1.08 | 6054 | [32] | ||
Kepler-379c | 0.204 | 62.784697 | 0.326 | transit | 2430±20 | 1.08 | 6054 | [32] | ||
Kepler-380b | 0.106 | 3.930821 | 0.05 | transit | 2710±40 | 1.05 | 6045 | [32] | ||
Kepler-380c | 0.113 | 7.630004 | 0.078 | transit | 2710±40 | 1.05 | 6045 | [32] | ||
Kepler-381b | 0.088 | 5.629021 | 0.066 | transit | 878±5 | 1.34 | 6152 | [32] | ||
Kepler-381c | 0.1 | 13.391635 | 0.117 | transit | 878±5 | 1.34 | 6152 | [32] | ||
Kepler-382b | 0.118 | 5.262155 | 0.055 | transit | 3130±60 | 0.8 | 5600 | [32] | ||
Kepler-382c | 0.142 | 12.162701 | 0.097 | transit | 3130±60 | 0.8 | 5600 | [32] | ||
Kepler-383b | 0.118 | 12.904532 | 0.095 | transit | 1695 | 0.67 | 4710 | [32] | ||
Kepler-383c | 0.111 | 31.200751 | 0.172 | transit | 1695 | 0.67 | 4710 | [32] | ||
Kepler-384b | 0.1 | 22.597053 | 0.148 | transit | 2990±30 | 0.76 | 5577 | [32] | ||
Kepler-384c | 0.101 | 45.348269 | 0.236 | transit | 2990±30 | 0.76 | 5577 | [32] | ||
Kepler-385b | 0.244 | 10.043686 | 0.097 | transit | 4870±160 | 1.09 | 6326 | [32] | ||
Kepler-385c | 0.271 | 15.163161 | 0.127 | transit | 4870±160 | 1.09 | 6326 | [32] | ||
Kepler-386b | 0.124 | 12.31043 | 0.096 | transit | 2950±90 | 0.74 | 5178 | [32] | ||
Kepler-386c | 0.141 | 25.193458 | 0.155 | transit | 2950±90 | 0.74 | 5178 | [32] | ||
Kepler-387b | 0.092 | 6.791636 | 0.068 | transit | 2670±30 | 1.03 | 5774 | [32] | ||
Kepler-387c | 0.079 | 11.837549 | 0.098 | transit | 2670±30 | 1.03 | 5774 | [32] | ||
Kepler-388b | 0.072 | 3.173315 | 0.036 | transit | 2000±200 | 0.59 | 4498 | [32] | ||
Kepler-388c | 0.077 | 13.297004 | 0.093 | transit | 2000±200 | 0.59 | 4498 | [32] | ||
Kepler-389b | 0.135 | 3.244107 | 0.041 | transit | 2720±70 | 0.78 | 5376 | [32] | ||
Kepler-389c | 0.13 | 14.51143 | 0.11 | transit | 2720±70 | 0.78 | 5376 | [32] | ||
Kepler-390b | 0.073 | 6.738088 | 0.065 | transit | 1437±12 | 0.67 | 5166 | [32] | ||
Kepler-390c | 0.07 | 13.060022 | 0.101 | transit | 1437±12 | 0.67 | 5166 | [32] | ||
Kepler-391b | 0.285 | 7.416755 | 0.082 | transit | 2900±40 | 1.22 | 4940 | [32] | ||
Kepler-391c | 0.316 | 20.485435 | 0.161 | transit | 2900±40 | 1.22 | 4940 | [32] | ||
Kepler-392b | 0.089 | 5.341853 | 0.059 | transit | 2260±20 | 1.13 | 5938 | [32] | ||
Kepler-392c | 0.098 | 10.423118 | 0.093 | transit | 2260±20 | 1.13 | 5938 | [32] | ||
Kepler-393b | 0.115 | 9.182417 | 0.091 | transit | 2940±40 | 1.32 | 6189 | [32] | ||
Kepler-393c | 0.119 | 14.613612 | 0.124 | transit | 2940±40 | 1.32 | 6189 | [32] | ||
Kepler-394b | 0.143 | 8.005013 | 0.083 | transit | 3560±80 | 1.11 | 6402 | [32] | ||
Kepler-394c | 0.148 | 12.130686 | 0.11 | transit | 3560±80 | 1.11 | 6402 | [32] | ||
Kepler-395b | 0.092 | 7.054346 | 0.061 | transit | 1390±20 | 0.53 | 4262 | [32] | ||
Kepler-395c | 0.118 | 34.989262 | 0.177 | transit | 1390±20 | 0.53 | 4262 | Potentially habitable exoplanet[32] | ||
Kepler-397b | 0.219 | 22.250949 | 0.144 | transit | 3760 | 5307 | [32] | |||
Kepler-397c | 0.551 | 135.498527 | 0.48 | transit | 3760 | 5307 | [32] | |||
Kepler-398b | 0.083 | 4.081423 | 0.044 | transit | 581.4±1.8 | 4493 | [32] | |||
Kepler-398c | 0.09 | 11.419412 | 0.087 | transit | 581.4±1.8 | 4493 | [32] | |||
Kepler-399b | 0.086 | 14.425281 | 0.103 | transit | 4400±700 | 5502 | [32] | |||
Kepler-399c | 0.128 | 26.67569 | 0.155 | transit | 4400±700 | 5502 | [32] | |||
Kepler-399d | 0.169 | 58.034616 | 0.261 | transit | 4400±700 | 5502 | [32] | |||
Kepler-400b | 0.147 | 9.024389 | 0.087 | transit | 2340 | 5886 | [32] | |||
Kepler-400c | 0.133 | 17.340824 | 0.134 | transit | 2340 | 5886 | [32] | |||
Kepler-401b | 0.153 | 14.383035 | 0.122 | transit | 3230±50 | 6117 | [32] | |||
Kepler-401c | 0.192 | 47.318218 | 0.269 | transit | 3230±50 | 6117 | [32] | |||
Kepler-402b | 0.109 | 4.028751 | 0.051 | transit | 2070±20 | 6090 | [32] | |||
Kepler-402c | 0.139 | 6.124821 | 0.068 | transit | 2070±20 | 6090 | [32] | |||
Kepler-402d | 0.123 | 8.921099 | 0.087 | transit | 2070±20 | 6090 | [32] | |||
Kepler-402e | 0.13 | 11.242861 | 0.102 | transit | 2070±20 | 6090 | [32] | |||
Kepler-403b | 0.112 | 7.031462 | 0.076 | transit | 2800±50 | 6090 | [32] | |||
Kepler-403c | 0.156 | 54.280749 | 0.297 | transit | 2800±50 | 6090 | [32] | |||
Kepler-404b | 0.113 | 11.829851 | 0.102 | transit | 2710±40 | 5654 | [32] | |||
Kepler-404c | 0.153 | 14.751166 | 0.118 | transit | 2710±40 | 5654 | [32] | |||
Kepler-405b | 0.186 | 10.613839 | 0.095 | transit | 3570±140 | 5818 | [32] | |||
Kepler-405c | 0.416 | 29.726682 | 0.188 | transit | 3570±140 | 5818 | [32] | |||
Kepler-406b | 0.02 | 0.128 | 2.42629 | transit | 1199±11 | 1.07 | 5538 | [33] | ||
Kepler-406c | 0.009 | 0.076 | 4.62332 | transit | 1199±11 | 1.07 | 5538 | [33] | ||
Kepler-407b | 0.095 | 0.66931 | transit | 1114±8 | 1 | 5476 | [33] | |||
Kepler-407c | 12.6 | 3000 | radial vel. | 1114±8 | 1 | 5476 | [33] | |||
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,[33] but confirmed by 2016.[35] | |||
Kepler-409b | 0.106 | 68.9584 | transit | 222.8±0.3 | 0.92 | 5460 | Host star known as Gliese 409[33] | |||
Kepler-412b | 0.941 | 1.341 | 1.7208604 | 0.02897 | transit | 3650±60 | 1.17 | 5750 | [36] | |
Kepler-413b | 0.211 | 0.388 | 66.262 | 0.3553 | transit | 2830±70 | 0.82 | 4700 | [37] | |
Kepler-414b | 0.011 | 0.153 | 4.7 | timing | 1364±9 | 0.89 | [38] | |||
Kepler-414c | 0.094 | 0.269 | 7.171 | timing | 1364±9 | 0.89 | [38] | |||
Kepler-415b | 0.377 | 0.108 | 4.176 | timing | 1750±30 | 0.67 | [38] | |||
Kepler-415c | 8.708 | transit | 1750±30 | 0.67 | ? | |||||
Kepler-416b | 0.183 | 0.221 | 6.319 | timing | 2290±30 | 1 | [38] | |||
Kepler-416c | 12.209 | transit | 2290±30 | 1 | ? | |||||
Kepler-417b | 0.035 | 0.206 | 12.331 | transit | 3250±150 | 0.9 | [38] | |||
Kepler-417c | 15.943 | transit | 3250±150 | 0.9 | ? | |||||
Kepler-418b | 1.1 | 1.2 | 86.67856 | transit | 3360±60 | 0.98 | 5820 | [39] | ||
Kepler-419b | 2.5 | 0.96 | 69.7546 | 0.37 | transit | 3390±80 | 1.39 | 6430 | [40] | |
Kepler-419c | 7.3 | 675.47 | 1.68 | timing | 3390±80 | 1.39 | 6430 | [40] | ||
Kepler-420Ab | 1.45 | 0.94 | 86.647661 | 0.382 | 511 | transit | 2900 | 0.99 | 5520 | [41] |
Kepler-421b | 0.371 | 704.1984 | 1.219 | transit | 1148±6 | 0.79 | 5308 | [42] | ||
Kepler-422b | 0.43 | 1.15 | 7.8914483 | 0.082 | transit | 2400±20 | 1.15 | 5972 | [43] | |
Kepler-423b | 0.595 | 1.192 | 2.6843285 | 0.03585 | 1605 | transit | 2520±40 | 0.85 | 5560 | [43] |
Kepler-424b | 1.03 | 0.89 | 3.3118644 | 0.044 | transit | 2320±30 | 1.01 | 5460 | [43] | |
Kepler-424c | 6.97 | 223.3 | 0.73 | radial vel. | 2320±30 | 1.01 | 5460 | [43] | ||
Kepler-425b | 0.25 | 0.978 | 3.79701816 | 0.0464 | 1070 | transit | 2140±30 | 0.93 | 5170 | [44] |
Kepler-426b | 0.34 | 1.09 | 3.21751883 | 0.0414 | 1300 | transit | 2810±40 | 0.91 | 5725 | [44] |
Kepler-427b | 0.29 | 1.23 | 10.290994 | 0.091 | 1100 | transit | 3410±50 | 0.96 | 5800 | [44] |
Kepler-428b | 1.27 | 1.08 | 3.52563254 | 0.0433 | 1070 | transit | 2280±50 | 0.87 | 5150 | [44] |
Kepler-430b | 0.29 | 35.968 | 0.2244 | 667 | transit | 3070±50 | 1.17 | 5884 | [45] | |
Kepler-430c | 0.16 | 110.979 | 0.4757 | 458 | transit | 3070±50 | 1.17 | 5884 | [45] | |
Kepler-431b | 0.068 | 6.803 | 0.0719 | 1032 | transit | 1609±15 | 1.07 | 6004 | [45] | |
Kepler-431c | 0.06 | 8.703 | 0.0847 | 951 | transit | 1609±15 | 1.07 | 6004 | [45] | |
Kepler-431d | 0.1 | 11.922 | 0.1045 | 856 | transit | 1609±15 | 1.07 | 6004 | [45] | |
Kepler-432b | 5.41 | 1.145 | 52.501129 | 0.301 | transit | 2830±60 | 1.32 | 4995 | Eccentric orbit[46] | |
Kepler-432c | 2.43+0.22 −0.24 |
406.2+3.9 −2.5 |
radial vel. | 2830±60 | 1.32 | 4995 | [46] | |||
Kepler-453b | 0.00063 | 0.553 | 240.503 | 0.7903 | transit | 1463±9 | 0.94 | 5527 | [47] | |
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 | [48] | ||||
OGLE-2008-BLG-92Lb | 0.18 | 18 | microlensing | 26000 | 0.71 | [49] | ||||
OGLE-2011-BLG-265Lb | 0.88 | 1.89 | microlensing | 14300 | 0.21 | [50] | ||||
OGLE-2013-BLG-102Lb | 12.569 | 0.8 | microlensing | 9900 | 0.1 | Additional planet or brown dwarf in the system.[51] | ||||
OGLE-2013-BLG-341LBb | 0.0073 | 0.883 | microlensing | 3790 | 0.15 | One more red dwarf in the system.[52] | ||||
OGLE-2014-BLG-0124Lb | 0.51 | 3.11 | microlensing | 13000 | 0.71 | [53] | ||||
SAND364 b | 1.54 | 121.71 | radial vel. | 2730±130 | 1.35 | 4284 | Belongs to Messier 67, also known as BD+12 1917b[54] | |||
TYC 1422-614-1 b | 2.5 | 198.4 | 0.69 | radial vel. | 2480 | 1.15 | 4806 | [55] | ||
TYC 1422-614-1 c | 10 | 559.3 | 1.37 | radial vel. | 2480 | 1.15 | 4806 | [55] | ||
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[56][57] | |
WASP-74b | 0.95 | 1.56 | 2.13775 | 0.037 | 1910 | transit | 390 | 1.48 | 5970 | [58] |
WASP-83b | 0.3 | 1.04 | 4.971252 | 0.059 | 1120 | transit | 980 | 1.11 | 5510 | [58] |
WASP-85Ab | 1.265 | 1.24 | 2.6556777 | 0.039 | 1452 | transit | 243 | 1.09 | 6112 | [59] |
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 | [60] Host star also known as CD-52 4998. | |
WASP-89b | 5.9 | 1.04 | 3.3564227 | 0.0427 | 1120 | transit | 957 | 0.92 | 5130 | [58] |
WASP-94Ab | 0.452 | 1.72 | 3.9501907 | 0.055 | 1604 | transit | 590 | 1.45 | 6153 | [61] |
WASP-94Bb | 0.618 | 2.00839 | 0.0335 | radial vel. | 590 | 1.24 | 6040 | [61] | ||
WASP-103b | 1.49 | 1.528 | 0.925542 | 0.01985 | 2508 | transit | 1500 | 1.22 | 6110 | Planet close to tidal disruption[62][63] |
WASP-104b | 1.272 | 1.137 | 1.7554137 | 0.02918 | 1516 | transit | 470 | 1.08 | 5475 | [64] |
WASP-106b | 1.925 | 1.085 | 9.289715 | 0.0917 | 1140 | transit | 920 | 1.19 | 6055 | [64] |
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 | [60] 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 | [60] 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 | [60] |
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 | [60] 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 | [60] |
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 | [59] |
WASP-117b | 0.2755 | 1.021 | 10.02165 | 0.09459 | 1024 | transit | 518±2 | 1.13 | 6038 | [65][66] |
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 | [59] |
XO-2Sb | 0.259 | 18.157 | 0.1344 | radial vel. | 480 | 0.98 | 5399 | [67] | ||
XO-2Sc | 1.37 | 120.8 | 0.4756 | radial vel. | 480 | 0.98 | 5399 | [67] | ||
YBP 1194 b | 0.32 | 6.959 | radial vel. | 2920±100 | 1.01 | 5780 | Belongs to Messier 67[54] | |||
YBP 1514 b | 0.4 | 5.118 | radial vel. | 3060±100 | 0.96 | 5725 | Belongs to Messier 67[54] |
Specific exoplanet lists
edit- 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 largest exoplanets
- List of smallest exoplanets
- List of transiting exoplanets
- List of exoplanets and planetary debris around white dwarfs
Lists of exoplanets by year of discovery
edit- List of exoplanets discovered before 2000 (31)
- List of exoplanets discovered between 2000–2009 (377)
- 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 (870)
- List of exoplanets discovered in 2015 (149)
- List of exoplanets discovered in 2016 (1497)
- List of exoplanets discovered in 2017 (158)
- List of exoplanets discovered in 2018 (303)
- List of exoplanets discovered in 2019 (172)
- List of exoplanets discovered in 2020 (249)
- List of exoplanets discovered in 2021 (257)
- List of exoplanets discovered in 2022 (313)
- List of exoplanets discovered in 2023 (307)
- List of exoplanets discovered in 2024 (238)
References
edit- ^ "The Extrasolar Planets Encyclopaedia". 1995. Retrieved 2015-11-09.
- ^ a b c d e 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
- ^ a b c 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
- ^ a b 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
- ^ a b c d e 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
- ^ 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.
- ^ a b c 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. 787 (1) (published May 2014): 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.
- ^ a b c d 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
- ^ Sissa (2017). "Observation of extrasolar planets at various ages". PhD Thesis, University of Padua, 2017. Bibcode:2017PhDT.......406S.
- ^ a b 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.
- ^ a b c d 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
- ^ a b 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.
- ^ a b 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
- ^ a b 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
- ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh bi bj bk bl bm bn bo bp bq br bs bt bu bv bw bx by bz ca cb cc cd ce cf cg ch ci cj ck cl cm cn co cp cq cr cs ct cu cv cw cx cy cz da db dc dd de df dg dh di dj dk dl dm dn do dp dq dr ds dt du dv dw dx dy dz ea eb ec ed ee ef eg eh ei ej ek el em en eo ep eq er es et eu ev ew ex ey ez fa fb fc fd fe ff fg fh fi fj fk fl fm fn fo fp fq fr fs ft fu fv fw fx fy fz ga gb gc gd ge gf gg gh gi gj gk gl gm gn go gp gq gr gs gt gu gv gw gx gy gz ha hb hc hd he hf hg hh hi hj hk hl hm hn ho hp hq hr hs ht hu hv hw hx hy hz ia ib ic id ie if ig ih ii ij ik il im in io ip iq ir is it iu iv iw ix iy iz ja jb jc jd je jf jg jh ji jj jk jl jm jn jo jp jq jr js jt ju jv jw jx jy jz ka kb kc kd ke kf kg kh ki kj kk kl km kn ko kp kq kr ks kt ku kv kw kx ky kz la lb lc ld le lf lg lh li lj lk ll lm ln lo lp lq lr ls lt lu lv lw lx ly lz ma mb mc md me mf mg mh mi mj mk ml mm mn mo mp mq mr ms mt mu mv mw mx my mz na nb nc nd ne nf ng nh ni nj nk nl nm nn no np nq nr ns nt nu nv nw nx ny nz oa ob oc od oe of og oh oi oj ok ol om on oo op oq or os ot ou ov ow ox oy oz pa pb pc pd pe pf pg ph pi pj pk pl pm pn po pp pq pr ps pt pu pv pw px py pz qa qb qc qd qe qf qg qh qi qj qk ql qm qn qo qp qq qr qs qt qu qv qw qx qy qz ra rb rc rd re rf rg rh ri rj rk rl rm rn ro rp rq rr rs rt ru rv rw rx ry rz sa sb sc sd se sf sg sh si sj sk sl sm sn so sp sq sr ss st su sv sw sx sy sz ta tb tc td te tf tg th ti tj tk tl tm tn to tp tq tr ts tt tu tv tw tx ty tz ua ub uc ud ue uf ug uh ui uj uk ul um un uo up uq ur us ut uu uv uw ux uy uz va vb vc vd ve vf vg vh vi vj vk vl vm vn vo vp vq vr vs vt vu vv vw vx vy vz wa wb wc wd we wf wg wh wi wj wk wl wm wn wo wp wq wr ws wt wu wv ww wx wy wz xa xb xc xd xe xf xg xh xi xj xk xl xm xn xo xp xq xr xs xt xu xv xw xx xy xz ya yb yc yd ye yf yg yh yi yj yk yl ym yn yo yp yq yr ys yt yu yv yw yx yy yz za zb zc zd ze zf zg zh zi zj zk zl zm zn zo zp zq zr zs zt zu zv zw zx zy zz aaa aab aac aad aae aaf aag aah aai aaj aak aal aam aan aao aap aaq aar aas aat aau aav aaw aax aay aaz aba abb abc abd abe abf abg abh 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
- ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al 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
- ^ a b 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. Bibcode:2020A&A...638A..10H. 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
- ^ a b c d e 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
- ^ a b 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
- ^ a b c d 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
- ^ a b c d 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
- ^ a b c d e 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
- ^ a b 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
- ^ a b c 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
- ^ a b 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.
- ^ a b c 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
- ^ a b c 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
- ^ a b c d e f 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
- ^ a b 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
- ^ a b 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.
- ^ a b 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