List of exoplanets discovered in 2014

Short description: None

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

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BD-11 4672 b | 0.53  |  | 1667  | 2.28  |  | radial vel.  | 89  | 0.57  | 4475  | [2]
Beta Cancri b | 7.8  |  | 605.2  | 1.7  |  | radial vel.  | 290.4  | 1.7  | 4092.1  | [3]
Beta Ursae Minoris b | 6.1  |  | 522.3  | 1.4  |  | radial vel.  | 126.5  | 1.4  | 4126  | [3]
COROT-22b | 0.038  | 0.435  | 9.75598  | 0.092  | 885  | transit  | 1930  | 1.1  | 5939  | [4]
COROT-24b  | 0.018  | 0.33  | 5.1134  | 0.056  | 1070  | transit  | 2000  | 0.91  | 4950  | [5]
COROT-24c  | 0.088  | 0.44  | 11.759  | 0.098  | 850  | transit  | 2000  | 0.91  | 4950  | [5]
COROT-27b  | 10.39  | 1.007  | 3.57532  | 0.0476  | 1500  | transit  | 3400±200  | 1.05  | 5900  | [6] Planet lost[7]
Gliese 15 Ab | 0.017  |  | 11.4433  | 0.0717  |  | radial vel.  | 11.6  | 0.38  | 3567  | [8]
Gliese 27.1 b | 0.0409  |  | 15.819  | 0.101  |  | radial vel.  | 77.05  | 0.53  | 3542  | Alternately known as Gliese 9018,[9] not related to Gliese 27.
Gliese 160.2 b  | 0.0321  |  | 5.2354  | 0.053  |  | radial vel.  | 84.39  | 0.69  | 4347  | Alternately known as Gliese 9144, not related to Gliese 160. Disproven exoplanet[9][10]
Gliese 180 b | 0.0261  |  | 17.380  | 0.103  |  | radial vel.  | 38.95  | 0.43  | 3371  | [9]
Gliese 180 c | 0.0201  |  | 24.329  | 0.129  |  | radial vel.  | 38.95  | 0.43  | 3371  | Unconfirmed as of 2020[11][9]
Gliese 229 Ab  | 0.10  |  | 471  | 0.970  |  | radial vel.  | 18.77  | 0.58  | 3564  | [9]
Gliese 433 c | 0.14  |  | 4900+1800−1000 | 4.7+1.2−0.8 |  | radial vel.  | 29.57  | 0.48  | 3472  | [9]
Gliese 422 b | 0.0311  |  | 26.161  | 0.119  |  | radial vel.  | 41.32  | 0.35  | 3323  | [9]
Gliese 682 b | 0.014  |  | 17.478  | 0.080  |  | radial vel.  | 16.33  | 0.27  | 3028  | Disproven exoplanet[9][10]
Gliese 682 c | 0.0274  |  | 57.32  | 0.176  |  | radial vel.  | 16.33  | 0.27  | 3028  | Disproven exoplanet[9][10]
Gliese 687 b | 0.058  |  | 38.14  | 0.16353  |  | radial vel.  | 14.8  | 0.41  | 3413  | [12]
Gliese 832 c | 0.017  |  | 35.68  | 0.163  |  | radial vel.  | 16.1  | 0.45  | 3472  | Habitable zone planet,[13] likely do not exist.[14]
Gliese 3293 b | 0.07406  |  | 30.5987  | 0.14339  |  | radial vel.  | 51.4  | 0.42  | 3466  | [15]
Gliese 3293 c | 0.06636  |  | 122.6196  | 0.36175  |  | radial vel.  | 51.4  | 0.42  | 3466  | [15]
Gliese 3341 b  | 0.0208  |  | 14.207  | 0.089  |  | radial vel.  | 77.1  | 0.47  | 3526  | [15]
GU Piscium b | 11.3  | 1.265  |  | 2000  |  | imaging  | 160  | 0.33  | 3250±32  | [16]
HAT-P-49b  | 1.73  | 1.413  | 2.691548  | 0.0438  | 2131  | transit  | 1050  | 1.54  | 6820  | [17]
HAT-P-54b  | 0.76  | 0.944  | 3.799847  | 0.04117  |  | transit  | 443  | 0.65  | 4390  | [18] Disputed in 2016,[19] reconfirmed in 2021.[20]
HATS-4b  | 1.323  | 1.02  | 2.516729  | 0.0362  | 1315  | transit  | 1400  | 1  | 5403  | [21]
HATS-5b  | 0.237  | 0.912  | 4.763387  | 0.0542  | 1025  | transit  | 840  | 0.94  | 5304  | [22]
HATS-6b  | 0.319  | 0.998  | 3.3252725  | 0.03623  |  | transit  | 484  | 0.57  | 3724  | [23]
HD 564 b  | 0.33  |  | 492.3  | 1.2  |  | radial vel.  | 175  | 0.96  | 5902  | [2]
HD 4203 c | 2.17  |  | 6700  | 6.95  |  | radial vel.  | 253.8  | 1.13  | 5702  | [24]
HD 5319 c | 1.15  |  | 886  | 2.071  |  | radial vel.  | 370  | 1.51  | 4958  | [25]
HD 10442 b  | 2.1  |  | 1043  | 2.335  |  | radial vel.  | 443±4  | 1.56  | 5034  | [25]
HD 11506 c | 0.408±0.057  |  | 223.41±0.32  | 0.774±0.038  |  | radial vel.  | 167.4±0.4  | 1.12±0.02  | 5833±28  | [25]
HD 14067 b  | 7.8  |  | 1455  | 3.4  |  | radial vel.  | 533  | 2.4  | 4815  | [26]
HD 30669 b | 0.47  |  | 1684  | 2.69  |  | radial vel.  | 186  | 0.92  | 5400  | [2]
HD 75784 b  | 1.15  |  | 341.7  | 1.073  |  | radial vel.  | 224  | 1.41  | 4917  | [25]
HD 100546 b |  | 6.9  |  | 53  |  | imaging  | 320  | 2.4  | 10500  | Largest exoplanet discovered[27]
HD 103720 b  | 0.62  |  | 4.5557  | 0.0498  |  | radial vel.  | 136  | 0.79  | 5017  | [2]
HD 108341 b  | 3.5  |  | 1129  | 2  |  | radial vel.  | 161  | 0.84  | 5122  | [2]
HD 114613 b  | 0.48  |  | 3827  | 5.16  |  | radial vel.  | 66.8  | 1.36  | 5729  | [28]
HD 141399 b | 0.451  |  | 94.44  | 0.415  |  | radial vel.  | 118  | 1.07  | 5600  | [29]
HD 141399 c | 1.33  |  | 201.99  | 0.689  |  | radial vel.  | 118  | 1.07  | 5600  | [29]
HD 141399 d | 1.18  |  | 1069.8  | 2.09  |  | radial vel.  | 118  | 1.07  | 5600  | [29]
HD 141399 e | 0.66  |  | 5000  | 5  |  | radial vel.  | 118  | 1.07  | 5600  | [29]
HD 154857 c | 2.58  |  | 3452  | 5.36  |  | radial vel.  | 223.5  | 1.72  | 5605  | [28]
HIP 67851 b | 1.38  |  | 88.9  | 0.46  |  | radial vel.  | 208.3±0.6  | 1.63  | 4890  | [30]
HIP 67851 c | 4.34±0.59  |  | 1741±39  | 3.09±0.18  |  | radial vel.  | 208.3±0.6  | 1.63  | 4890  | [31]
HIP 97233 b  | 20  |  | 1058.8  | 2.55  |  | radial vel.  | 347  | 1.93  | 5020  | [30]
HIP 105854 b | 8.2  |  | 184.2  | 0.81  |  | radial vel.  | 276  | 2.1  | 4780  | [32]
HIP 116454 b | 0.037  | 0.226  | 9.1205  | 0.0906  |  | radial vel.  | 180  | 0.78  | 5089  | [33]
Kapteyn b | 0.015  |  | 48.616+0.036−0.032 | 0.168  |  | radial vel.  | 12.8  | 0.28  | 3550  | Existence of planet been disputed.[34][35]
Kapteyn c | 0.022  |  | 121.54  | 0.311  |  | radial vel.  | 12.8  | 0.28  | 3550
KIC 10001893 b |  |  | 0.2197  |  |  | orbital brightness modulation  | 5700±500  |  | 27500  | Disproven exoplanet[36][37]
KIC 10001893 c |  |  | 0.32528  |  |  | orbital brightness modulation  | 5700±500  |  | 27500  | Disproven exoplanet[36][37]
KIC 10001893 d |  |  | 0.81161  |  |  | orbital brightness modulation  | 5700±500  |  | 27500  | Disproven exoplanet[36][37]
Kepler-23d |  | 0.196  | 15.274299  | 0.124  |  | transit  | 2600  | 1.11  | 5828  | [38]
Kepler-24d |  | 0.149  | 4.244384  | 0.051  |  | transit  | 3900  | 1.03  | 5897  | [38]
Kepler-24e |  | 0.248  | 18.998355  | 0.138  |  | transit  | 3900  | 1.03  | 5897  | [38]
Kepler-25d | 0.283  |  | 123  |  |  | radial vel.  | 798±4  | 1.19  | 6270  | [39][38]
Kepler-26d |  | 0.095  | 3.543919  | 0.039  |  | transit  | 1104±10  | 0.54  | 3914  | [38]
Kepler-26e |  | 0.215  | 46.827915  | 0.22  |  | transit  | 1104±10  | 0.54  | 3914  | [38]
Kepler-31d | 6.8  | 0.348  | 87.6451  | 0.4  |  | transit  | 6800  | 1.21  | 6340  | [38]
Kepler-37e |  |  | 51.196  |  |  | timing  | 220  | 0.8  | 5417  | [38]
Kepler-48d  | 0.025  | 0.182  | 42.8961  |  |  | transit  | 1009±5  | 0.88  | 5194  | [39][38]
Kepler-48e  | 2.067  |  | 982  |  |  | radial vel.  | 1009±5  | 0.88  | 5194  | [39]
Kepler-49d  |  | 0.143  | 2.576549  | 0.031  |  | transit  | 1024±8  | 0.55  | 4252  | [38]
Kepler-49e  |  | 0.139  | 18.596108  | 0.116  |  | transit  | 1024±8  | 0.55  | 4252  | [38]
Kepler-51d | 0.024  | 0.865  | 130.194  | 0.509  |  | transit  | 2610±50  | 1.04  | 6018  | [38]
Kepler-52d  |  | 0.174  | 36.445171  | 0.182  |  | transit  | 1058±7  | 0.54  | 4263  | [38]
Kepler-53d  |  | 0.189  | 9.751962  | 0.091  |  | transit  | 4600±200  | 0.98  | 5858  | [38]
Kepler-54d  |  | 0.136  | 20.995694  | 0.126  |  | transit  | 893±9  | 0.51  | 4252  | [38]
Kepler-55d  |  | 0.142  | 2.211099  | 0.029  |  | transit  | 1920±30  | 0.62  | 4503  | [38]
Kepler-55e  |  | 0.138  | 4.617534  | 0.048  |  | transit  | 1920±30  | 0.62  | 4503  | [38]
Kepler-55f  |  | 0.142  | 10.198545  | 0.081  |  | transit  | 1920±30  | 0.62  | 4503  | [38]
Kepler-58d  |  | 0.262  | 40.101371  | 0.236  |  | transit  | 3250±80  | 0.95  | 6099  | [38]
Kepler-79d  | 0.019  | 0.639  | 52.0902  | 0.287  | 553  | transit  | 3230±60  | 1.17  | 6174  | [38]
Kepler-79e  | 0.013  | 0.311  | 81.0659  | 0.386  | 477  | transit  | 3230±60  | 1.17  | 6174  | [38]
Kepler-80d | 0.02124  | 0.136  | 3.07222  | 0.0372  |  | transit  | 1160  | 0.73  | 4540  | [38]
Kepler-80e | 0.01299  | 0.143  | 4.64489  | 0.0491  |  | transit  | 1160  | 0.73  | 4540  | [38]
Kepler-81d  |  | 0.108  | 20.837846  | 0.128  |  | transit  | 1147±10  | 0.64  | 4500  | [38]
Kepler-82d  |  | 0.158  | 2.382961  | 0.034  |  | transit  | 3030±80  | 0.85  | 5428  | [38]
Kepler-82e  |  | 0.22  | 5.902206  | 0.063  |  | transit  | 3030±80  | 0.85  | 5428  | [38]
Kepler-83d  |  | 0.173  | 5.169796  | 0.051  |  | transit  | 1320±17  | 0.66  | 4648  | [38]
Kepler-84d  |  | 0.123  | 4.224537  | 0.052  |  | transit  | 4700±500  | 1  | 6031  | [38]
Kepler-84e  |  | 0.232  | 27.434389  | 0.181  |  | transit  | 4700±500  | 1  | 6031  | [38]
Kepler-84f  |  | 0.196  | 44.552169  | 0.25  |  | transit  | 4700±500  | 1  | 6031  | [38]
Kepler-85d  |  | 0.107  | 17.91323  | 0.13  |  | transit  | 2550±50  | 0.92  | 5436  | [38]
Kepler-85e  |  | 0.113  | 25.216751  | 0.163  |  | transit  | 2550±50  | 0.92  | 5436  | [38]
Kepler-93b | 0.01265  | 0.132  | 4.72673978  | 0.053  | 1037  | transit  | 313.7±0.7  | 0.91  | 5669  | [39]
Kepler-93c  | 3  |  | 1460  |  |  | radial vel.  | 313.7±0.7  | 0.91  | 5669  | [39]
Kepler-94b  | 0.034  | 0.313  | 2.50806  |  |  | transit  | 629±2  | 0.81  | 4781  | [39]
Kepler-94c  | 9.836  |  | 820.3  |  |  | radial vel.  | 629±2  | 0.81  | 4781  | [39]
Kepler-95b  | 0.041  | 0.305  | 11.5231  |  |  | transit  | 1472±18  | 1.08  | 5699  | [39]
Kepler-96b  | 0.027  | 0.238  | 16.2385  |  |  | transit  | 402.2±1.3  | 1  | 5690  | [39]
Kepler-97b  | 0.011  | 0.132  | 2.58664  |  |  | transit  | 1322±11  | 0.94  | 5779  | [39]
Kepler-97c  | 1.08  |  | 789  |  |  | radial vel.  | 1322±11  | 0.94  | 5779  | [39]
Kepler-98b  | 0.011  | 0.178  | 1.54168  |  |  | transit  | 1154±9  | 0.99  | 5539  | [39]
Kepler-99b  | 0.019  | 0.132  | 4.60358  |  |  | transit  | 683±3  | 0.79  | 4782  | [39]
Kepler-100b  | 0.023  | 0.118  | 6.88705  |  |  | transit  | 1002±5  | 1.08  | 5825  | [39][38]
Kepler-100c  |  | 0.196  | 12.8159  |  |  | transit  | 1002±5  | 1.08  | 5825  | [39][38]
Kepler-100d  |  | 0.144  | 35.3331  |  |  | transit  | 1002±5  | 1.08  | 5825  | [39][38]
Kepler-101b  | 0.16  | 0.51  | 3.4876812  | 0.0474  |  | transit  | 3110±50  | 1.17  | 5667  | [38]
Kepler-101c  | 0.01  | 0.112  | 6.02976  | 0.0684  |  | transit  | 3110±50  | 1.17  | 5667  | [38]
Kepler-102b |  | 0.042  | 5.28696  |  | 792  | transit  | 352.7±0.7  | 0.81  | 4909  | [39][38]
Kepler-102c |  | 0.052  | 7.07142  |  | 718  | transit  | 352.7±0.7  | 0.81  | 4909  | [39][38]
Kepler-102d | 0.012  | 0.105  | 10.3117  |  |  | transit  | 352.7±0.7  | 0.81  | 4909  | [39][38]
Kepler-102f |  | 0.079  | 27.4536  |  | 457  | transit  | 352.7±0.7  | 0.81  | 4909  | [39][38]
Kepler-103b  | 0.031  | 0.301  | 15.9654  |  |  | transit  | 1637±19  | 1.09  | 5845  | [39][38]
Kepler-103c  | 0.114  | 0.459  | 179.612  |  |  | transit  | 1637±19  | 1.09  | 5845  | [39][38]
Kepler-104b  |  | 0.277  | 11.427548  | 0.094  |  | transit  | 1322±14  | 0.81  | 5711  | [38]
Kepler-104c  |  | 0.279  | 23.668205  | 0.153  |  | transit  | 1322±14  | 0.81  | 5711  | [38]
Kepler-104d  |  | 0.319  | 51.755394  | 0.257  |  | transit  | 1322±14  | 0.81  | 5711  | [38]
Kepler-105c  | 0.01447  | 0.117  | 7.1262  |  |  | transit  | 1517±18  | 0.96  | 5827  | [38]
Kepler-106b  |  | 0.073  | 6.16486  |  |  | transit  | 1470±20  | 1  | 5858  | [39]
Kepler-106c  | 0.033  | 0.223  | 13.5708  |  |  | transit  | 1470±20  | 1  | 5858  | [39][38]
Kepler-106d  |  | 0.085  | 23.9802  |  |  | transit  | 1470±20  | 1  | 5858  | [39][38]
Kepler-106e  | 0.035  | 0.228  | 43.8445  |  |  | transit  | 1470±20  | 1  | 5858  | [39][38]
Kepler-107b |  | 0.139  | 3.179997  | 0.044  |  | transit  | 1741±18  |  | 5851  | [38]
Kepler-107c |  | 0.161  | 4.901425  | 0.059  |  | transit  | 1741±18  |  | 5851  | [38]
Kepler-107d |  | 0.095  | 7.958203  | 0.082  |  | transit  | 1741±18  |  | 5851  | [38]
Kepler-107e |  | 0.308  | 14.749049  | 0.123  |  | transit  | 1741±18  |  | 5851  | [38]
Kepler-108b  |  | 0.772  | 49.183921  | 0.292  |  | transit  | 4200±500  | 0.87  | 5854  | [38]
Kepler-108c  |  | 0.73  | 190.323494  | 0.721  |  | transit  | 4200±500  | 0.87  | 5854  | [38]
Kepler-109b  |  | 0.211  | 6.48163  |  |  | transit  | 1570±17  | 1.04  | 5952  | [39][38]
Kepler-109c  |  | 0.225  | 21.2227  |  |  | transit  | 1570±17  | 1.04  | 5952  | [39][38]
Kepler-110b  |  | 0.163  | 12.691112  | 0.107  |  | transit  | 1950±30  |  | 5960  | [38]
Kepler-110c  |  | 0.197  | 31.719775  | 0.198  |  | transit  | 1950±30  |  | 5960  | [38]
Kepler-111b  |  | 0.141  | 3.341815  | 0.046  |  | transit  | 2190±20  |  | 5952  | [38]
Kepler-111c  |  | 0.651  | 224.784608  | 0.761  |  | transit  | 2190±20  |  | 5952  | [38]
Kepler-112b  |  | 0.211  | 8.408878  | 0.076  |  | transit  | 1698±14  |  | 5544  | [38]
Kepler-112c  |  | 0.214  | 28.574263  | 0.172  |  | transit  | 1698±14  |  | 5544  | [38]
Kepler-113b  | 0.037  | 0.162  | 4.754  |  |  | transit  | 862±3  | 0.75  | 4725  | [39][38]
Kepler-113c  |  | 0.194  | 8.92507  |  |  | transit  | 862±3  | 0.75  | 4725  | [39][38]
Kepler-114b  |  | 0.112  | 5.188549  | 0.053  | 722  | transit  | 852±4  | 0.56  | 4605  | [38]
Kepler-115b  |  | 0.097  | 2.403679  | 0.036  |  | transit  | 2070±20  | 1  | 5979  | [38]
Kepler-115c  |  | 0.232  | 8.990889  | 0.087  |  | transit  | 2070±20  | 1  | 5979  | [38]
Kepler-116b  |  | 0.305  | 5.968734  | 0.069  |  | transit  | 3200±50  | 1.16  | 6142  | [38]
Kepler-116c  |  | 0.205  | 13.07163  | 0.116  |  | transit  | 3200±50  | 1.16  | 6142  | [38]
Kepler-117b  | 0.094  | 0.719  | 18.7959228  | 0.1445  |  | transit  | 4700  | 1.13  | 6150  | [38]
Kepler-117c  | 1.84  | 1.101  | 50.790391  | 0.2804  |  | transit  | 4700  | 1.13  | 6150  | [38]
Kepler-118b  |  | 0.175  | 7.518496  | 0.073  |  | transit  | 1900±20  | 0.86  | 5274  | [38]
Kepler-118c  |  | 0.685  | 20.17202  | 0.141  |  | transit  | 1900±20  | 0.86  | 5274  | [38]
Kepler-119b  |  | 0.321  | 2.422082  | 0.035  |  | transit  | 2340±40  |  | 5595  | [38]
Kepler-119c  |  | 0.082  | 4.125103  | 0.049  |  | transit  | 2340±40  |  | 5595  | [38]
Kepler-120b  |  | 0.192  | 6.312501  | 0.055  |  | transit  | 1281±10  |  | 4096  | [38]
Kepler-120c  |  | 0.136  | 12.794585  | 0.088  |  | transit  | 1281±10  |  | 4096  | [38]
Kepler-121b  |  | 0.209  | 3.177422  | 0.039  |  | transit  | 1690±20  |  | 5311  | [38]
Kepler-121c  |  | 0.203  | 41.008011  | 0.216  |  | transit  | 1690±20  |  | 5311  | [38]
Kepler-122b  |  | 0.209  | 5.766193  | 0.064  |  | transit  | 3450±70  | 0.99  | 6050  | [38]
Kepler-122c  |  | 0.524  | 12.465988  | 0.108  |  | transit  | 3450±70  | 0.99  | 6050  | [38]
Kepler-122d  |  | 0.196  | 21.587475  | 0.155  |  | transit  | 3450±70  | 0.99  | 6050  | [38]
Kepler-122e  |  | 0.232  | 37.993273  | 0.227  |  | transit  | 3450±70  | 0.99  | 6050  | [38]
Kepler-122f  | 0.113  | 0.156  | 56.268  |  |  | timing  | 3450±70  | 0.99  | 6050  | ?
Kepler-123b  |  | 0.262  | 17.232366  | 0.135  |  | transit  | 3430±80  | 1.03  | 6089  | [38]
Kepler-123c  |  | 0.132  | 26.695074  | 0.181  |  | transit  | 3430±80  | 1.03  | 6089  | [38]
Kepler-124b |  | 0.065  | 3.410493  | 0.039  |  | transit  | 1386±10  |  | 4984  | [38]
Kepler-124c  |  | 0.156  | 13.821375  | 0.1  |  | transit  | 1386±10  |  | 4984  | [38]
Kepler-124d  |  | 0.099  | 30.950851  | 0.17  |  | transit  | 1386±10  |  | 4984  | [38]
Kepler-125b  |  | 0.211  | 4.164389  | 0.041  |  | transit  | 601±3  | 0.55  | 3810  | [38]
Kepler-125c  |  | 0.066  | 5.774464  | 0.051  |  | transit  | 601±3  | 0.55  | 3810  | [38]
Kepler-126b  |  | 0.136  | 10.495711  | 0.099  |  | transit  | 779±5  |  | 6239  | [38]
Kepler-126c  |  | 0.141  | 21.869741  | 0.162  |  | transit  | 779±5  |  | 6239  | [38]
Kepler-126d  |  | 0.223  | 100.283134  | 0.448  |  | transit  | 779±5  |  | 6239  | [38]
Kepler-127b  |  | 0.125  | 14.435889  | 0.125  |  | transit  | 1162±8  |  | 6106  | [38]
Kepler-127c  |  | 0.237  | 29.393195  | 0.2  |  | transit  | 1162±8  |  | 6106  | [38]
Kepler-127d  |  | 0.236  | 48.630408  | 0.28  |  | transit  | 1162±8  |  | 6106  | [38]
Kepler-129b  |  | 0.211  | 15.79186  | 0.131  |  | transit  | 1349±14  | 1.18  | 5770  | [38]
Kepler-129c  |  | 0.227  | 82.20017  | 0.393  |  | transit  | 1349±14  | 1.18  | 5770  | [38]
Kepler-130c  |  | 0.259  | 27.50868  | 0.178  |  | transit  | 1042±7  | 1  | 5884  | [38]
Kepler-130d  |  | 0.146  | 87.517905  | 0.377  |  | transit  | 1042±7  | 1  | 5884  | [38]
Kepler-131b  | 0.051  | 0.215  | 16.092  |  |  | transit  | 750±4  | 1.02  | 5685  | [39][38]
Kepler-131c  | 0.026  | 0.075  | 25.5169  |  |  | transit  | 750±4  | 1.02  | 5685  | [39][38]
Kepler-132b  |  | 0.108  | 6.178196  | 0.067  |  | transit  | 900±70  |  | 6003  | [38]
Kepler-132c  |  | 0.114  | 6.414914  | 0.068  |  | transit  | 900±70  |  | 6003  | [38]
Kepler-132d  |  | 0.138  | 18.010199  | 0.136  |  | transit  | 900±70  |  | 6003  | [38]
Kepler-133b  |  | 0.157  | 8.129976  | 0.083  |  | transit  | 2170±60  |  | 5736  | [38]
Kepler-133c  |  | 0.253  | 31.517586  | 0.204  |  | transit  | 2170±60  |  | 5736  | [38]
Kepler-134b  |  | 0.178  | 5.317429  | 0.06  |  | transit  | 1102±7  |  | 5983  | [38]
Kepler-134c  |  | 0.112  | 10.105785  | 0.092  |  | transit  | 1102±7  |  | 5983  | [38]
Kepler-135b  |  | 0.161  | 6.00253  | 0.067  |  | transit  | 2060±40  |  | 6090  | [38]
Kepler-135c  |  | 0.103  | 11.448708  | 0.103  |  | transit  | 2060±40  |  | 6090  | [38]
Kepler-136b  |  | 0.183  | 11.5789  | 0.106  |  | transit  | 1389±14  | 1.2  | 6165  | [38]
Kepler-136c  |  | 0.178  | 16.399235  | 0.133  |  | transit  | 1389±14  | 1.2  | 6165  | [38]
Kepler-137b  |  | 0.131  | 8.436387  | 0.077  |  | transit  | 996±6  |  | 5187  | [38]
Kepler-137c  |  | 0.168  | 18.735753  | 0.13  |  | transit  | 996±6  |  | 5187  | [38]
Kepler-138b | 0.00021  | 0.047  | 10.3126  |  |  | transit  | 218.5±0.3  | 0.52  | 3841  | [38]
Kepler-138c | 0.0062  | 0.107  | 13.7813  |  |  | transit  | 218.5±0.3  | 0.52  | 3841  | [38]
Kepler-138d | 0.00201  | 0.108  | 23.0881  |  | 431  | transit  | 218.5±0.3  | 0.52  | 3841  | [38]
Kepler-139b  |  | 0.262  | 15.771044  | 0.127  |  | transit  | 1289±13  | 1.08  | 5594  | [38]
Kepler-139c  |  | 0.302  | 157.072878  | 0.586  |  | transit  | 1289±13  | 1.08  | 5594  | [38]
Kepler-140b  |  | 0.144  | 3.25427  | 0.045  |  | transit  | 1940±20  |  | 6077  | [38]
Kepler-140c  |  | 0.161  | 91.353282  | 0.414  |  | transit  | 1940±20  |  | 6077  | [38]
Kepler-141b  |  | 0.062  | 3.107675  | 0.039  |  | transit  | 990±4  | 1  | 4910  | [38]
Kepler-141c  |  | 0.126  | 7.010606  | 0.067  |  | transit  | 990±4  | 1  | 4910  | ?
Kepler-142b  |  | 0.178  | 2.024152  | 0.032  |  | transit  | 1818±13  | 0.99  | 5790  | [38]
Kepler-142c  |  | 0.255  | 4.761702  | 0.057  |  | transit  | 1818±13  | 0.99  | 5790  | [38]
Kepler-142d  |  | 0.193  | 41.809118  | 0.242  |  | transit  | 1818±13  | 0.99  | 5790  | [38]
Kepler-143b  |  | 0.215  | 16.007583  | 0.127  |  | transit  | 2700±40  |  | 5848  | [38]
Kepler-143c  |  | 0.301  | 27.082511  | 0.181  |  | transit  | 2700±40  |  | 5848  | [38]
Kepler-144b  |  | 0.119  | 5.885273  | 0.066  |  | transit  | 1269±10  | 1.03  | 6075  | [38]
Kepler-144c  |  | 0.12  | 10.104665  | 0.094  |  | transit  | 1269±10  | 1.03  | 6075  | [38]
Kepler-146b  |  | 0.331  | 31.158799  | 0.2  |  | transit  | 2390±30  |  | 5948  | [38]
Kepler-146c  |  | 0.279  | 76.732171  | 0.364  |  | transit  | 2390±30  |  | 5948  | [38]
Kepler-147b  |  | 0.136  | 12.610584  | 0.113  |  | transit  | 3500±90  | 1.01  | 6012  | [38]
Kepler-147c  |  | 0.217  | 33.416423  | 0.216  |  | transit  | 3500±90  | 1.01  | 6012  | [38]
Kepler-148b  |  | 0.161  | 1.729366  | 0.028  |  | transit  | 2640±50  |  | 5272  | [38]
Kepler-148c  |  | 0.321  | 4.180043  | 0.05  |  | transit  | 2640±50  |  | 5272  | [38]
Kepler-149b  |  | 0.376  | 29.198943  | 0.184  |  | transit  | 1893±19  |  | 5381  | [38]
Kepler-149c  |  | 0.144  | 55.328328  | 0.281  |  | transit  | 1893±19  |  | 5381  | [38]
Kepler-149d  |  | 0.353  | 160.018032  | 0.571  |  | transit  | 1893±19  |  | 5381  | [38]
Kepler-150b  |  | 0.112  | 3.428054  | 0.044  |  | transit  | 2980±60  |  | 5560  | [38]
Kepler-150c  |  | 0.329  | 7.381998  | 0.073  |  | transit  | 2980±60  |  | 5560  | [38]
Kepler-150d  |  | 0.249  | 12.56093  | 0.104  |  | transit  | 2980±60  |  | 5560  | [38]
Kepler-150e  |  | 0.278  | 30.826557  | 0.189  |  | transit  | 2980±60  |  | 5560  | [38]
Kepler-151b  |  | 0.273  | 15.228958  | 0.116  |  | transit  | 2160±30  | 0.83  | 5460  | [38]
Kepler-151c  |  | 0.186  | 24.674612  | 0.16  |  | transit  | 2160±30  | 0.83  | 5460  | [38]
Kepler-152b  |  | 0.249  | 18.207973  | 0.124  |  | transit  | 1457±10  |  | 5088  | [38]
Kepler-152c  |  | 0.213  | 88.255055  | 0.356  |  | transit  | 1457±10  |  | 5088  | [38]
Kepler-153b  |  | 0.261  | 18.870227  | 0.129  |  | transit  | 1518±11  |  | 5404  | [38]
Kepler-153c  |  | 0.226  | 46.90232  | 0.237  |  | transit  | 1518±11  |  | 5404  | [38]
Kepler-154b  |  | 0.202  | 33.040532  | 0.198  |  | transit  | 3070±60  | 0.89  | 5690  | [38]
Kepler-154c  |  | 0.263  | 62.303276  | 0.303  |  | transit  | 3070±60  | 0.89  | 5690  | [38]
Kepler-155b  |  | 0.186  | 5.931194  | 0.056  |  | transit  | 965±7  | 0.58  | 4508  | [38]
Kepler-155c  |  | 0.2  | 52.661793  | 0.242  |  | transit  | 965±7  | 0.58  | 4508  | [38]
Kepler-156b  |  | 0.205  | 4.973456  | 0.054  |  | transit  | 1465±11  |  | 5094  | [38]
Kepler-156c  |  | 0.227  | 15.906801  | 0.117  |  | transit  | 1465±11  |  | 5094  | [38]
Kepler-157b  |  | 0.118  | 1.732342  | 0.028  |  | transit  | 2580±40  |  | 5774  | [38]
Kepler-157c  |  | 0.2  | 13.5405  | 0.11  |  | transit  | 2580±40  |  | 5774  | [38]
Kepler-158b  |  | 0.189  | 16.709184  | 0.111  |  | transit  | 1037±6  |  | 4623  | [38]
Kepler-158c  |  | 0.17  | 28.551383  | 0.158  |  | transit  | 1037±6  |  | 4623  | [38]
Kepler-159b  |  | 0.212  | 10.139623  | 0.082  |  | transit  | 1232±10  |  | 4625  | [38]
Kepler-159c  |  | 0.304  | 43.595792  | 0.218  |  | transit  | 1232±10  |  | 4625  | [38]
Kepler-160b |  | 0.137  | 4.309427  | 0.05  |  | transit  | 3140±60  | 0.88  | 5471+115−37 | [38][40]
Kepler-160c |  | 0.322  | 13.699087  | 0.109  |  | transit  | 3140±60  | 0.88  | 5471+115−37 | [38][40]
Kepler-161b  |  | 0.189  | 4.921355  | 0.054  |  | transit  | 1435±10  | 0.77  | 5078  | [38]
Kepler-161c  |  | 0.183  | 7.06424  | 0.068  |  | transit  | 1435±10  | 0.77  | 5078  | [38]
Kepler-162b  |  | 0.112  | 6.919798  | 0.069  |  | transit  | 2860±50  |  | 5816  | [38]
Kepler-162c  |  | 0.27  | 19.446355  | 0.137  |  | transit  | 2860±50  |  | 5816  | [38]
Kepler-163b  |  | 0.094  | 7.810937  | 0.078  |  | transit  | 2300±40  | 0.96  | 5776  | [38]
Kepler-163c  |  | 0.202  | 21.347262  | 0.152  |  | transit  | 2300±40  | 0.96  | 5776  | [38]
Kepler-164b  |  | 0.126  | 5.03503  | 0.058  |  | transit  | 2980±50  | 1.11  | 5888  | [38]
Kepler-164c  |  | 0.244  | 10.945723  | 0.097  |  | transit  | 2980±50  | 1.11  | 5888  | [38]
Kepler-164d  |  | 0.219  | 28.986769  | 0.187  |  | transit  | 2980±50  | 1.11  | 5888  | [38]
Kepler-165b  |  | 0.207  | 8.180848  | 0.072  |  | transit  | 1860±20  |  | 5211  | [38]
Kepler-165c  |  | 0.199  | 15.31299  | 0.11  |  | transit  | 1860±20  |  | 5211  | [38]
Kepler-166b  |  | 0.203  | 7.650254  | 0.072  |  | transit  | 2000±20  |  | 5413  | [38]
Kepler-166c  |  | 0.212  | 34.260281  | 0.195  |  | transit  | 2000±20  |  | 5413  | [38]
Kepler-167b  |  | 0.144  | 4.3931632  | 0.0483  |  | transit  | 1100  | 0.77  | 4890  | [38]
Kepler-167c  |  | 0.138  | 7.406114  | 0.0684  |  | transit  | 1100  | 0.77  | 4890  | [38]
Kepler-168b  |  | 0.13  | 4.425391  | 0.056  |  | transit  | 4550±160  |  | 6282  | [38]
Kepler-168c  |  | 0.24  | 13.193242  | 0.116  |  | transit  | 4550±160  |  | 6282  | [38]
Kepler-169b  |  | 0.101  | 3.250619  | 0.04  |  | transit  | 1341±9  | 0.86  | 4997  | [38]
Kepler-169c  |  | 0.108  | 6.195469  | 0.062  |  | transit  | 1341±9  | 0.86  | 4997  | [38]
Kepler-169d  |  | 0.112  | 8.348125  | 0.075  |  | transit  | 1341±9  | 0.86  | 4997  | [38]
Kepler-169e  |  | 0.196  | 13.767102  | 0.105  |  | transit  | 1341±9  | 0.86  | 4997  | [38]
Kepler-169f  |  | 0.23  | 87.090195  | 0.359  |  | transit  | 1341±9  | 0.86  | 4997  | [38]
Kepler-170b  |  | 0.285  | 7.930592  | 0.08  |  | transit  | 2460±40  |  | 5679  | [38]
Kepler-170c  |  | 0.255  | 16.665863  | 0.131  |  | transit  | 2460±40  |  | 5679  | [38]
Kepler-171b  |  | 0.209  | 4.166972  | 0.05  |  | transit  | 2890±60  |  | 5642  | [38]
Kepler-171c  |  | 0.228  | 11.463462  | 0.098  |  | transit  | 2890±60  |  | 5642  | [38]
Kepler-171d  |  | 0.169  | 39.595519  | 0.223  |  | transit  | 2890±60  |  | 5642  | [38]
Kepler-172b  |  | 0.21  | 2.940309  | 0.04  |  | transit  | 2770±60  | 0.86  | 5526  | [38]
Kepler-172c  |  | 0.255  | 6.388996  | 0.068  |  | transit  | 2770±60  | 0.86  | 5526  | [38]
Kepler-172d  |  | 0.201  | 14.627119  | 0.118  |  | transit  | 2770±60  | 0.86  | 5526  | [38]
Kepler-172e  |  | 0.246  | 35.118736  | 0.211  |  | transit  | 2770±60  | 0.86  | 5526  | [38]
Kepler-173b  |  | 0.115  | 4.263742  | 0.048  |  | transit  | 2780±50  | 0.78  | 6031  | [38]
Kepler-173c  |  | 0.217  | 8.005777  | 0.074  |  | transit  | 2780±50  | 0.78  | 6031  | [38]
Kepler-174b |  | 0.175  | 13.98179  | 0.1  |  | transit  | 1268±8  |  | 4880  | [38]
Kepler-174c |  | 0.133  | 44.000529  | 0.214  |  | transit  | 1268±8  |  | 4880  | [38]
Kepler-174d |  | 0.195  | 247.35373  | 0.677  |  | transit  | 1268±8  |  | 4880  | [38]
Kepler-175b  |  | 0.228  | 11.903515  | 0.105  |  | transit  | 4450±150  | 1.04  | 6064  | [38]
Kepler-175c  |  | 0.277  | 34.035257  | 0.213  |  | transit  | 4450±150  | 1.04  | 6064  | [38]
Kepler-176b  |  | 0.128  | 5.433074  | 0.058  |  | transit  | 1750±20  |  | 5232  | [38]
Kepler-176c  |  | 0.232  | 12.759712  | 0.102  |  | transit  | 1750±20  |  | 5232  | [38]
Kepler-176d  |  | 0.224  | 25.751974  | 0.163  |  | transit  | 1750±20  |  | 5232  | [38]
Kepler-178b  |  | 0.259  | 9.576694  | 0.085  |  | transit  | 2380±30  |  | 5676  | [38]
Kepler-178c  |  | 0.257  | 20.552802  | 0.142  |  | transit  | 2380±30  |  | 5676  | [38]
Kepler-178d  |  | 0.352  | 96.678988  | 0.397  |  | transit  | 2380±30  |  | 5676  | [38]
Kepler-179b  |  | 0.146  | 2.735926  | 0.036  |  | transit  | 2010±20  |  | 5302  | [38]
Kepler-179c  |  | 0.178  | 6.40013  | 0.064  |  | transit  | 2010±20  |  | 5302  | [38]
Kepler-180b  |  | 0.134  | 13.817124  | 0.109  |  | transit  | 2320±30  | 0.84  | 5731  | [38]
Kepler-180c  |  | 0.269  | 41.885775  | 0.229  |  | transit  | 2320±30  | 0.84  | 5731  | [38]
Kepler-181b  |  | 0.113  | 3.137873  | 0.04  |  | transit  | 2020±30  |  | 5333  | [38]
Kepler-181c  |  | 0.178  | 4.302149  | 0.049  |  | transit  | 2020±30  |  | 5333  | [38]
Kepler-182b |  | 0.23  | 9.825792  | 0.096  |  | transit  | 5290±180  | 1.14  | 6250  | [38]
Kepler-182c |  | 0.306  | 20.684342  | 0.157  |  | transit  | 5290±180  | 1.14  | 6250  | [38]
Kepler-183b  |  | 0.184  | 5.687945  | 0.064  |  | transit  | 3530±100  |  | 5888  | [38]
Kepler-183c  |  | 0.203  | 11.637071  | 0.103  |  | transit  | 3530±100  |  | 5888  | [38]
Kepler-184b  |  | 0.211  | 10.687576  | 0.092  |  | transit  | 2030±20  |  | 5788  | [38]
Kepler-184c  |  | 0.176  | 20.303005  | 0.141  |  | transit  | 2030±20  |  | 5788  | [38]
Kepler-184d  |  | 0.222  | 29.022358  | 0.179  |  | transit  | 2030±20  |  | 5788  | [38]
Kepler-185b  |  | 0.104  | 1.6329  | 0.026  |  | transit  | 1542±15  | 0.79  | 5208  | [38]
Kepler-185c  |  | 0.18  | 20.729042  | 0.139  |  | transit  | 1542±15  | 0.79  | 5208  | [38]
Kepler-186b |  | 0.095  | 3.8867907  | 0.0343  |  | transit  | 560  | 0.54  | 3755  | [38]
Kepler-186c |  | 0.112  | 7.267302  | 0.0451  |  | transit  | 560  | 0.54  | 3755  | [38]
Kepler-186d |  | 0.125  | 13.342996  | 0.0781  |  | transit  | 560  | 0.54  | 3755  | [38]
Kepler-186e |  | 0.113  | 22.407704  | 0.11  |  | transit  | 560  | 0.54  | 3755  | [38]
Kepler-186f |  | 0.104  | 129.9441  | 0.432  |  | transit  | 560  | 0.54  | 3755  | ? Potentially habitable exoplanet
Kepler-187b  |  | 0.126  | 4.938864  | 0.059  |  | transit  | 3850±110  | 0.85  | 6105  | [38]
Kepler-187c  |  | 0.238  | 10.640263  | 0.099  |  | transit  | 3850±110  | 0.85  | 6105  | [38]
Kepler-188b  |  | 0.15  | 2.061897  | 0.032  |  | transit  | 3250±80  |  | 6021  | [38]
Kepler-188c  |  | 0.285  | 5.996553  | 0.066  |  | transit  | 3250±80  |  | 6021  | [38]
Kepler-189b  |  | 0.108  | 10.399931  | 0.088  |  | transit  | 1960±20  | 0.79  | 5235  | [38]
Kepler-189c  |  | 0.212  | 20.134866  | 0.137  |  | transit  | 1960±20  | 0.79  | 5235  | [38]
Kepler-190b  |  | 0.139  | 2.019999  | 0.03  |  | transit  | 1431±9  | 0.84  | 5106  | [38]
Kepler-190c  |  | 0.13  | 3.763024  | 0.045  |  | transit  | 1431±9  | 0.84  | 5106  | [38]
Kepler-191b  |  | 0.12  | 9.939632  | 0.087  |  | transit  | 1970±30  | 0.85  | 5282  | [38]
Kepler-191c  |  | 0.166  | 17.738506  | 0.128  |  | transit  | 1970±30  | 0.85  | 5282  | [38]
Kepler-192b  |  | 0.244  | 9.926746  | 0.09  |  | transit  | 2170±20  |  | 5479  | [38]
Kepler-192c  |  | 0.249  | 21.2234  | 0.15  |  | transit  | 2170±20  |  | 5479  | [38]
Kepler-193b  |  | 0.213  | 11.38848  | 0.106  |  | transit  | 3390±80  |  | 6335  | [38]
Kepler-193c  |  | 0.245  | 50.697494  | 0.286  |  | transit  | 3390±80  |  | 6335  | [38]
Kepler-194b  |  | 0.135  | 2.092281  | 0.032  |  | transit  | 3700±100  |  | 6089  | [38]
Kepler-194c  |  | 0.231  | 17.308032  | 0.131  |  | transit  | 3700±100  |  | 6089  | [38]
Kepler-194d  |  | 0.214  | 52.814973  | 0.275  |  | transit  | 3700±100  |  | 6089  | [38]
Kepler-195b  |  | 0.181  | 8.307872  | 0.077  |  | transit  | 2170±30  |  | 5329  | [38]
Kepler-195c  |  | 0.138  | 34.096863  | 0.197  |  | transit  | 2170±30  |  | 5329  | [38]
Kepler-196b  |  | 0.17  | 20.739886  | 0.138  |  | transit  | 1491±10  |  | 5128  | [38]
Kepler-196c  |  | 0.2  | 47.427737  | 0.24  |  | transit  | 1491±10  |  | 5128  | [38]
Kepler-197b  |  | 0.091  | 5.599308  | 0.06  |  | transit  | 1088±7  |  | 6004  | [38]
Kepler-197c  |  | 0.11  | 10.349695  | 0.09  |  | transit  | 1088±7  |  | 6004  | [38]
Kepler-197d  |  | 0.109  | 15.677563  | 0.119  |  | transit  | 1088±7  |  | 6004  | [38]
Kepler-197e  |  | 0.081  | 25.209715  | 0.164  |  | transit  | 1088±7  |  | 6004  | [38]
Kepler-198b  |  | 0.252  | 17.790037  | 0.131  |  | transit  | 1638±14  | 0.93  | 5574  | [38]
Kepler-198c  |  | 0.22  | 49.567416  | 0.259  |  | transit  | 1638±14  | 0.93  | 5574  | [38]
Kepler-199b  |  | 0.277  | 23.637604  | 0.158  |  | transit  | 1725±14  |  | 5644  | [38]
Kepler-199c  |  | 0.29  | 67.093408  | 0.316  |  | transit  | 1725±14  |  | 5644  | [38]
Kepler-200b  |  | 0.19  | 8.594805  | 0.08  |  | transit  | 2210±20  |  | 5678  | [38]
Kepler-200c  |  | 0.142  | 10.222157  | 0.09  |  | transit  | 2210±20  |  | 5678  | [38]
Kepler-201b  |  | 0.219  | 25.672083  | 0.175  |  | transit  | 2240±30  | 1.17  | 6065  | [38]
Kepler-201c  |  | 0.254  | 151.884058  | 0.573  |  | transit  | 2240±30  | 1.17  | 6065  | [38]
Kepler-202b  |  | 0.145  | 4.069427  | 0.045  |  | transit  | 937±3  |  | 4668  | [38]
Kepler-202c  |  | 0.165  | 16.282493  | 0.113  |  | transit  | 937±3  |  | 4668  | [38]
Kepler-203b  |  | 0.229  | 3.162697  | 0.043  |  | transit  | 2340±30  | 0.98  | 5821  | [38]
Kepler-203c  |  | 0.22  | 5.370647  | 0.061  |  | transit  | 2340±30  | 0.98  | 5821  | [38]
Kepler-203d  |  | 0.128  | 11.32972  | 0.1  |  | transit  | 2340±30  | 0.98  | 5821  | [38]
Kepler-204b  |  | 0.226  | 14.400974  | 0.117  |  | transit  | 2280±20  | 0.96  | 5812  | [38]
Kepler-204c  |  | 0.16  | 25.660593  | 0.173  |  | transit  | 2280±20  | 0.96  | 5812  | [38]
Kepler-205b  |  | 0.135  | 2.75564  | 0.032  |  | transit  | 523.4±1.1  |  | 4321  | [38]
Kepler-205c  |  | 0.146  | 20.306546  | 0.122  |  | transit  | 523.4±1.1  |  | 4321  | [38]
Kepler-206b  |  | 0.107  | 7.781987  | 0.078  |  | transit  | 1972±16  | 0.94  | 5764  | [38]
Kepler-206c  |  | 0.158  | 13.137471  | 0.111  |  | transit  | 1972±16  | 0.94  | 5764  | [38]
Kepler-206d  |  | 0.106  | 23.44281  | 0.163  |  | transit  | 1972±16  | 0.94  | 5764  | [38]
Kepler-207b  |  | 0.14  | 1.611865  | 0.029  |  | transit  | 2920±30  |  | 5920  | [38]
Kepler-207c  |  | 0.134  | 3.071571  | 0.044  |  | transit  | 2920±30  |  | 5920  | [38]
Kepler-207d  |  | 0.295  | 5.868075  | 0.068  |  | transit  | 2920±30  |  | 5920  | [38]
Kepler-208b  |  | 0.145  | 4.22864  | 0.054  |  | transit  | 2580±20  | 1.03  | 6092  | [38]
Kepler-208c  |  | 0.124  | 7.466623  | 0.079  |  | transit  | 2580±20  | 1.03  | 6092  | [38]
Kepler-208d  |  | 0.107  | 11.131786  | 0.103  |  | transit  | 2580±20  | 1.03  | 6092  | [38]
Kepler-208e  |  | 0.132  | 16.259458  | 0.132  |  | transit  | 2580±20  | 1.03  | 6092  | [38]
Kepler-209b  |  | 0.202  | 16.087845  | 0.122  |  | transit  | 1913±18  |  | 5513  | [38]
Kepler-209c  |  | 0.277  | 41.749882  | 0.231  |  | transit  | 1913±18  |  | 5513  | [38]
Kepler-210b  |  | 0.262  | 2.453234  | 0.032  |  | transit  | 764±2  |  | 4559  | [38]
Kepler-210c  |  | 0.323  | 7.972513  | 0.07  |  | transit  | 764±2  |  | 4559  | [38]
Kepler-211b  |  | 0.112  | 4.138575  | 0.048  |  | transit  | 1018±5  | 0.97  | 5123  | [38]
Kepler-211c  |  | 0.115  | 6.04045  | 0.062  |  | transit  | 1018±5  | 0.97  | 5123  | [38]
Kepler-212b  |  | 0.097  | 16.257582  | 0.133  |  | transit  | 2280±20  | 1.16  | 5852  | [38]
Kepler-212c  |  | 0.244  | 31.805174  | 0.207  |  | transit  | 2280±20  | 1.16  | 5852  | [38]
Kepler-213b  |  | 0.145  | 2.46236  | 0.036  |  | transit  | 2100±20  | 0.94  | 5696  | [38]
Kepler-213c  |  | 0.209  | 4.822962  | 0.057  |  | transit  | 2100±20  | 0.94  | 5696  | [38]
Kepler-214b  |  | 0.233  | 15.660544  | 0.13  |  | transit  | 4080±70  |  | 6169  | [38]
Kepler-214c  |  | 0.19  | 28.7798  | 0.194  |  | transit  | 4080±70  |  | 6169  | [38]
Kepler-215b  |  | 0.145  | 9.360672  | 0.084  |  | transit  | 1607±12  | 0.77  | 5739  | [38]
Kepler-215c  |  | 0.158  | 14.667108  | 0.113  |  | transit  | 1607±12  | 0.77  | 5739  | [38]
Kepler-215d  |  | 0.213  | 30.864423  | 0.185  |  | transit  | 1607±12  | 0.77  | 5739  | [38]
Kepler-215e  |  | 0.156  | 68.16101  | 0.314  |  | transit  | 1607±12  | 0.77  | 5739  | [38]
Kepler-216b  |  | 0.21  | 7.693641  | 0.079  |  | transit  | 4000±70  |  | 6091  | [38]
Kepler-216c  |  | 0.271  | 17.406669  | 0.136  |  | transit  | 4000±70  |  | 6091  | [38]
Kepler-217b  |  | 0.199  | 5.374943  | 0.065  |  | transit  | 3720±50  |  | 6171  | [38]
Kepler-217c  |  | 0.165  | 8.586004  | 0.089  |  | transit  | 3720±50  |  | 6171  | [38]
Kepler-218b  |  | 0.132  | 3.619337  | 0.046  |  | transit  | 2180±20  |  | 5502  | [38]
Kepler-218c  |  | 0.28  | 44.699576  | 0.248  |  | transit  | 2180±20  |  | 5502  | [38]
Kepler-219b  |  | 0.263  | 4.585512  | 0.057  |  | transit  | 2620±30  |  | 5786  | [38]
Kepler-219c  |  | 0.319  | 22.714613  | 0.165  |  | transit  | 2620±30  |  | 5786  | [38]
Kepler-219d  |  | 0.251  | 47.903645  | 0.272  |  | transit  | 2620±30  |  | 5786  | [38]
Kepler-220b  |  | 0.072  | 4.159807  | 0.046  |  | transit  | 560±2  |  | 4632  | [38]
Kepler-220c  |  | 0.14  | 9.034199  | 0.076  |  | transit  | 560±2  |  | 4632  | [38]
Kepler-220d  |  | 0.087  | 28.122397  | 0.163  |  | transit  | 560±2  |  | 4632  | [38]
Kepler-220e  |  | 0.119  | 45.902733  | 0.226  |  | transit  | 560±2  |  | 4632  | [38]
Kepler-221b  |  | 0.153  | 2.795906  | 0.037  |  | transit  | 1270±9  | 0.72  | 5243  | [38]
Kepler-221c  |  | 0.261  | 5.690586  | 0.059  |  | transit  | 1270±9  | 0.72  | 5243  | [38]
Kepler-221d  |  | 0.244  | 10.04156  | 0.087  |  | transit  | 1270±9  | 0.72  | 5243  | [38]
Kepler-221e  |  | 0.235  | 18.369917  | 0.13  |  | transit  | 1270±9  | 0.72  | 5243  | [38]
Kepler-222b  |  | 0.282  | 3.936981  | 0.048  |  | transit  | 2520±40  |  | 5433  | [38]
Kepler-222c  |  | 0.414  | 10.08881  | 0.091  |  | transit  | 2520±40  |  | 5433  | [38]
Kepler-222d  |  | 0.329  | 28.081912  | 0.18  |  | transit  | 2520±40  |  | 5433  | [38]
Kepler-223b | 0.02328  | 0.267  | 7.38449  |  |  | transit  | 6400±400  | 1.12  |  | [38]
Kepler-223c | 0.01605  | 0.307  | 9.84564  |  |  | transit  | 6400±400  | 1.12  |  | [38]
Kepler-223d | 0.02517  | 0.467  | 14.78869  |  |  | transit  | 6400±400  | 1.12  |  | [38]
Kepler-223e | 0.0151  | 0.41  | 19.72567  |  |  | transit  | 6400±400  | 1.12  |  | [38]
Kepler-224b  |  | 0.124  | 3.132924  | 0.038  |  | transit  | 2600±60  | 0.74  | 5018  | [38]
Kepler-224c  |  | 0.278  | 5.925003  | 0.058  |  | transit  | 2600±60  | 0.74  | 5018  | [38]
Kepler-224d  |  | 0.205  | 11.349393  | 0.089  |  | transit  | 2600±60  | 0.74  | 5018  | [38]
Kepler-224e  |  | 0.176  | 18.643577  | 0.124  |  | transit  | 2600±60  | 0.74  | 5018  | [38]
Kepler-225b  |  | 0.107  | 6.738975  | 0.056  |  | transit  | 1850±40  |  | 3682  | [38]
Kepler-225c  |  | 0.164  | 18.794234  | 0.111  |  | transit  | 1850±40  |  | 3682  | [38]
Kepler-226b  |  | 0.138  | 3.940997  | 0.047  |  | transit  | 3280±80  | 0.86  | 5571  | [38]
Kepler-226c  |  | 0.203  | 5.349555  | 0.058  |  | transit  | 3280±80  | 0.86  | 5571  | [38]
Kepler-226d  |  | 0.109  | 8.109044  | 0.076  |  | transit  | 3280±80  | 0.86  | 5571  | [38]
Kepler-227b  |  | 0.277  | 9.488015  | 0.09  |  | transit  | 3640±100  |  | 5854  | [38]
Kepler-227c  |  | 0.271  | 54.418694  | 0.29  |  | transit  | 3640±100  |  | 5854  | [38]
Kepler-228b  |  | 0.136  | 2.566546  | 0.038  |  | transit  | 5600±300  |  | 6043  | [38]
Kepler-228c  |  | 0.241  | 4.134444  | 0.052  |  | transit  | 5600±300  |  | 6043  | [38]
Kepler-228d  |  | 0.36  | 11.094286  | 0.101  |  | transit  | 5600±300  |  | 6043  | [38]
Kepler-229b  |  | 0.196  | 6.252972  | 0.062  |  | transit  | 2750±70  |  | 5120  | [38]
Kepler-229c  |  | 0.439  | 16.068638  | 0.117  |  | transit  | 2750±70  |  | 5120  | [38]
Kepler-229d  |  | 0.343  | 41.194912  | 0.22  |  | transit  | 2750±70  |  | 5120  | [38]
Kepler-230b  |  | 0.38  | 32.625555  | 0.191  |  | transit  | 2460±40  |  | 5588  | [38]
Kepler-230c  |  | 0.182  | 91.773242  | 0.38  |  | transit  | 2460±40  |  | 5588  | [38]
Kepler-231b  |  | 0.154  | 10.065275  | 0.074  |  | transit  | 988±9  | 0.58  | 3767  | [38]
Kepler-231c  |  | 0.172  | 19.271566  | 0.114  |  | transit  | 988±9  | 0.58  | 3767  | [38]
Kepler-232b  |  | 0.275  | 4.431222  | 0.054  |  | transit  | 4570±160  |  | 5847  | [38]
Kepler-232c  |  | 0.342  | 11.379349  | 0.101  |  | transit  | 4570±160  |  | 5847  | [38]
Kepler-233b  |  | 0.217  | 8.472382  | 0.077  |  | transit  | 2860±60  |  | 5360  | [38]
Kepler-233c  |  | 0.242  | 60.418955  | 0.287  |  | transit  | 2860±60  |  | 5360  | [38]
Kepler-234b  |  | 0.33  | 2.711506  | 0.04  |  | transit  | 5900±300  |  | 6224  | [38]
Kepler-234c  |  | 0.313  | 7.21205  | 0.077  |  | transit  | 5900±300  |  | 6224  | [38]
Kepler-235b  |  | 0.199  | 3.340222  | 0.037  |  | transit  | 1410±20  | 0.59  | 4255  | [38]
Kepler-235c  |  | 0.114  | 7.824904  | 0.065  |  | transit  | 1410±20  | 0.59  | 4255  | [38]
Kepler-235d  |  | 0.183  | 20.060548  | 0.122  |  | transit  | 1410±20  | 0.59  | 4255  | [38]
Kepler-235e |  | 0.198  | 46.183669  | 0.213  |  | transit  | 1410±20  | 0.59  | 4255  | [38]
Kepler-236b  |  | 0.14  | 8.295611  | 0.065  |  | transit  | 949±7  | 0.56  | 3750  | [38]
Kepler-236c  |  | 0.178  | 23.968127  | 0.132  |  | transit  | 949±7  | 0.56  | 3750  | [38]
Kepler-237b  |  | 0.126  | 4.715106  | 0.05  |  | transit  | 2180±30  | 0.7  | 4861  | [38]
Kepler-237c  |  | 0.186  | 8.103636  | 0.071  |  | transit  | 2180±30  | 0.7  | 4861  | [38]
Kepler-238b  |  | 0.154  | 2.090876  | 0.034  |  | transit  | 6200±300  | 1.06  | 5751  | [38]
Kepler-238c  |  | 0.213  | 6.155557  | 0.069  |  | transit  | 6200±300  | 1.06  | 5751  | [38]
Kepler-238d  |  | 0.274  | 13.233549  | 0.115  |  | transit  | 6200±300  | 1.06  | 5751  | [38]
Kepler-239b  |  | 0.208  | 11.763051  | 0.095  |  | transit  | 2150±40  | 0.74  | 4914  | [38]
Kepler-239c  |  | 0.224  | 56.228098  | 0.268  |  | transit  | 2150±40  | 0.74  | 4914  | [38]
Kepler-240b  |  | 0.122  | 4.144495  | 0.048  |  | transit  | 2480±60  |  | 4985  | [38]
Kepler-240c  |  | 0.196  | 7.953528  | 0.074  |  | transit  | 2480±60  |  | 4985  | [38]
Kepler-241b  |  | 0.208  | 12.718092  | 0.094  |  | transit  | 1980±130  |  | 4699  | [38]
Kepler-241c  |  | 0.229  | 36.065978  | 0.189  |  | transit  | 1980±130  |  | 4699  | [38]
Kepler-242b  |  | 0.233  | 8.20395  | 0.075  |  | transit  | 1990±30  |  | 5020  | [38]
Kepler-242c  |  | 0.178  | 14.496481  | 0.109  |  | transit  | 1990±30  |  | 5020  | [38]
Kepler-243b  |  | 0.219  | 5.715442  | 0.062  |  | transit  | 2300±30  | 0.89  | 5228  | [38]
Kepler-243c  |  | 0.178  | 20.026218  | 0.142  |  | transit  | 2300±30  | 0.89  | 5228  | [38]
Kepler-244b  |  | 0.246  | 4.311792  | 0.05  |  | transit  | 3480±120  |  | 5554  | [38]
Kepler-244c  |  | 0.183  | 9.767292  | 0.087  |  | transit  | 3480±120  |  | 5554  | [38]
Kepler-244d  |  | 0.206  | 20.050401  | 0.14  |  | transit  | 3480±120  |  | 5554  | [38]
Kepler-245b  |  | 0.229  | 7.49019  | 0.071  |  | transit  | 2870±80  | 0.8  | 5100  | [38]
Kepler-245c  |  | 0.194  | 17.460812  | 0.124  |  | transit  | 2870±80  | 0.8  | 5100  | [38]
Kepler-245d  |  | 0.27  | 36.277108  | 0.202  |  | transit  | 2870±80  | 0.8  | 5100  | [38]
Kepler-246b  |  | 0.209  | 4.60182  | 0.052  |  | transit  | 2070±20  | 0.86  | 5206  | [38]
Kepler-246c  |  | 0.134  | 11.187161  | 0.095  |  | transit  | 2070±20  | 0.86  | 5206  | [38]
Kepler-247b  |  | 0.146  | 3.33616  | 0.042  |  | transit  | 2200±40  |  | 5100  | [38]
Kepler-247c  |  | 0.365  | 9.439452  | 0.084  |  | transit  | 2200±40  |  | 5100  | [38]
Kepler-247d  |  | 0.352  | 20.477912  | 0.14  |  | transit  | 2200±40  |  | 5100  | [38]
Kepler-248b  |  | 0.269  | 6.308205  | 0.066  |  | transit  | 2460±40  |  | 5190  | [38]
Kepler-248c  |  | 0.363  | 16.239494  | 0.123  |  | transit  | 2460±40  |  | 5190  | [38]
Kepler-249b  |  | 0.097  | 3.306539  | 0.035  |  | transit  | 624±3  |  | 3568  | [38]
Kepler-249c  |  | 0.135  | 7.113702  | 0.058  |  | transit  | 624±3  |  | 3568  | [38]
Kepler-249d  |  | 0.14  | 15.368459  | 0.097  |  | transit  | 624±3  |  | 3568  | [38]
Kepler-250b  |  | 0.101  | 4.148141  | 0.048  |  | transit  | 2530±50  | 0.8  | 5160  | [38]
Kepler-250c  |  | 0.203  | 7.156804  | 0.069  |  | transit  | 2530±50  | 0.8  | 5160  | [38]
Kepler-250d  |  | 0.194  | 17.648312  | 0.127  |  | transit  | 2530±50  | 0.8  | 5160  | [38]
Kepler-251b  |  | 0.119  | 4.790936  | 0.053  |  | transit  | 3090±90  | 0.91  | 5526  | [38]
Kepler-251c  |  | 0.247  | 16.514043  | 0.122  |  | transit  | 3090±90  | 0.91  | 5526  | [38]
Kepler-251d  |  | 0.247  | 30.133001  | 0.182  |  | transit  | 3090±90  | 0.91  | 5526  | [38]
Kepler-251e  |  | 0.247  | 99.640161  | 0.404  |  | transit  | 3090±90  | 0.91  | 5526  | [38]
Kepler-252b  |  | 0.11  | 6.668391  | 0.058  |  | transit  | 1251±11  | 0.52  | 4208  | [38]
Kepler-252c  |  | 0.192  | 10.848463  | 0.08  |  | transit  | 1251±11  | 0.52  | 4208  | [38]
Kepler-253b  |  | 0.145  | 3.783986  | 0.046  |  | transit  | 2800±60  |  | 5208  | [38]
Kepler-253c  |  | 0.236  | 10.281951  | 0.089  |  | transit  | 2800±60  |  | 5208  | [38]
Kepler-253d  |  | 0.283  | 18.119869  | 0.13  |  | transit  | 2800±60  |  | 5208  | [38]
Kepler-254b  |  | 0.345  | 5.826662  | 0.064  |  | transit  | 4700±200  |  | 5957  | [38]
Kepler-254c  |  | 0.192  | 12.412183  | 0.105  |  | transit  | 4700±200  |  | 5957  | [38]
Kepler-254d  |  | 0.223  | 18.746477  | 0.139  |  | transit  | 4700±200  |  | 5957  | [38]
Kepler-255b  |  | 0.138  | 5.714606  | 0.063  |  | transit  | 3530±100  | 0.97  | 5573  | [38]
Kepler-255c  |  | 0.267  | 9.946047  | 0.092  |  | transit  | 3530±100  | 0.97  | 5573  | [38]
Kepler-256b  |  | 0.142  | 1.620493  | 0.027  |  | transit  | 3440±80  | 1.02  | 5551  | [38]
Kepler-256c  |  | 0.192  | 3.38802  | 0.045  |  | transit  | 3440±80  | 1.02  | 5551  | [38]
Kepler-256d  |  | 0.221  | 5.839172  | 0.064  |  | transit  | 3440±80  | 1.02  | 5551  | [38]
Kepler-256e  |  | 0.21  | 10.681572  | 0.096  |  | transit  | 3440±80  | 1.02  | 5551  | [38]
Kepler-257b  |  | 0.233  | 2.382667  | 0.034  |  | transit  | 2600±50  |  | 5180  | [38]
Kepler-257c  |  | 0.483  | 6.581484  | 0.066  |  | transit  | 2600±50  |  | 5180  | [38]
Kepler-257d  |  | 0.442  | 24.664551  | 0.16  |  | transit  | 2600±50  |  | 5180  | [38]
Kepler-258b  |  | 0.362  | 13.19722  | 0.103  |  | transit  | 1900±20  | 0.8  | 4942  | [38]
Kepler-258c  |  | 0.322  | 33.653079  | 0.193  |  | transit  | 1900±20  | 0.8  | 4942  | [38]
Kepler-259b  |  | 0.25  | 8.115317  | 0.079  |  | transit  | 3360±80  |  | 5938  | [38]
Kepler-259c  |  | 0.241  | 36.924931  | 0.217  |  | transit  | 3360±80  |  | 5938  | [38]
Kepler-260b  |  | 0.179  | 8.187399  | 0.075  |  | transit  | 2080±20  | 0.88  | 5250  | [38]
Kepler-260c  |  | 0.155  | 76.050178  | 0.332  |  | transit  | 2080±20  | 0.88  | 5250  | [38]
Kepler-261b  |  | 0.194  | 10.381227  | 0.088  |  | transit  | 1044±5  | 0.87  | 5098  | [38]
Kepler-261c  |  | 0.178  | 24.570858  | 0.156  |  | transit  | 1044±5  | 0.87  | 5098  | [38]
Kepler-262b  |  | 0.121  | 13.060855  | 0.108  |  | transit  | 2030±20  |  | 5841  | [38]
Kepler-262c  |  | 0.146  | 21.853722  | 0.152  |  | transit  | 2030±20  |  | 5841  | [38]
Kepler-263b  |  | 0.238  | 16.568087  | 0.12  |  | transit  | 2510±50  |  | 5265  | [38]
Kepler-263c  |  | 0.22  | 47.332773  | 0.242  |  | transit  | 2510±50  |  | 5265  | [38]
Kepler-264b  |  | 0.297  | 40.806231  | 0.249  |  | transit  | 3150±60  | 1.32  | 6158  | [38]
Kepler-264c  |  | 0.252  | 140.101261  | 0.566  |  | transit  | 3150±60  | 1.32  | 6158  | [38]
Kepler-265b  |  | 0.166  | 6.846262  | 0.069  |  | transit  | 4330±160  | 1.03  | 5835  | [38]
Kepler-265c  |  | 0.235  | 17.028937  | 0.127  |  | transit  | 4330±160  | 1.03  | 5835  | [38]
Kepler-265d  |  | 0.222  | 43.130617  | 0.236  |  | transit  | 4330±160  | 1.03  | 5835  | [38]
Kepler-265e  |  | 0.231  | 67.831024  | 0.319  |  | transit  | 4330±160  | 1.03  | 5835  | [38]
Kepler-266b  |  | 0.221  | 6.61833  | 0.071  |  | transit  | 4640±190  | 0.99  | 5885  | [38]
Kepler-266c  |  | 0.347  | 107.723601  | 0.457  |  | transit  | 4640±190  | 0.99  | 5885  | [38]
Kepler-267b  |  | 0.177  | 3.353728  | 0.037  |  | transit  | 870±8  | 0.56  | 4258  | [38]
Kepler-267c  |  | 0.19  | 6.87745  | 0.06  |  | transit  | 870±8  | 0.56  | 4258  | [38]
Kepler-267d  |  | 0.203  | 28.464515  | 0.154  |  | transit  | 870±8  | 0.56  | 4258  | [38]
Kepler-268b  |  | 0.227  | 25.934138  | 0.18  |  | transit  | 2840±30  |  | 6081  | [38]
Kepler-268c  |  | 0.302  | 83.446393  | 0.391  |  | transit  | 2840±30  |  | 6081  | [38]
Kepler-269b  |  | 0.22  | 5.326718  | 0.061  |  | transit  | 7900±600  | 0.98  | 5847  | [38]
Kepler-269c  |  | 0.151  | 8.127899  | 0.081  |  | transit  | 7900±600  | 0.98  | 5847  | [38]
Kepler-270b  |  | 0.179  | 11.476094  | 0.107  |  | transit  | 3180±40  |  | 6067  | [38]
Kepler-270c  |  | 0.158  | 25.262887  | 0.18  |  | transit  | 3180±40  |  | 6067  | [38]
Kepler-271b  |  | 0.079  | 5.217738  | 0.056  |  | transit  | 1334±12  |  | 5524  | [38]
Kepler-271c  |  | 0.089  | 7.410935  | 0.071  |  | transit  | 1334±12  |  | 5524  | [38]
Kepler-272b  |  | 0.128  | 2.971353  | 0.038  |  | transit  | 2970±40  | 0.79  | 5297  | [38]
Kepler-272c  |  | 0.16  | 6.057342  | 0.061  |  | transit  | 2970±40  | 0.79  | 5297  | [38]
Kepler-272d  |  | 0.201  | 10.937304  | 0.091  |  | transit  | 2970±40  | 0.79  | 5297  | [38]
Kepler-273b  |  | 0.134  | 2.936532  | 0.037  |  | transit  | 2370±30  |  | 5626  | [38]
Kepler-273c  |  | 0.177  | 8.014927  | 0.073  |  | transit  | 2370±30  |  | 5626  | [38]
Kepler-274b  |  | 0.137  | 11.634788  | 0.101  |  | transit  | 4510±140  |  | 6023  | [38]
Kepler-274c  |  | 0.164  | 33.197861  | 0.204  |  | transit  | 4510±140  |  | 6023  | [38]
Kepler-275b  |  | 0.209  | 10.300682  | 0.098  |  | transit  | 7000±500  | 1.24  | 6165  | [38]
Kepler-275c  |  | 0.302  | 16.088134  | 0.132  |  | transit  | 7000±500  | 1.24  | 6165  | [38]
Kepler-275d  |  | 0.297  | 35.676062  | 0.224  |  | transit  | 7000±500  | 1.24  | 6165  | [38]
Kepler-276b  |  | 0.256  | 14.12841  | 0.119  |  | transit  | 3850±150  | 1.1  | 6105  | [38]
Kepler-278b  |  | 0.363  | 30.160546  | 0.207  |  | transit  | 1460±20  |  | 4991  | [38]
Kepler-278c  |  | 0.32  | 51.078775  | 0.294  |  | transit  | 1460±20  |  | 4991  | [38]
Kepler-280b  |  | 0.129  | 2.139542  | 0.032  |  | transit  | 2600±30  | 0.91  | 5744  | [38]
Kepler-280c  |  | 0.179  | 4.807091  | 0.056  |  | transit  | 2600±30  | 0.91  | 5744  | [38]
Kepler-281b  |  | 0.252  | 14.646008  | 0.117  |  | transit  | 6000±300  | 0.98  | 5723  | [38]
Kepler-281c  |  | 0.474  | 36.337373  | 0.215  |  | transit  | 6000±300  | 0.98  | 5723  | [38]
Kepler-282b  |  | 0.09  | 9.220524  | 0.082  |  | transit  | 4530±150  | 0.97  | 5602  | [38]
Kepler-282c  |  | 0.107  | 13.638723  | 0.106  |  | transit  | 4530±150  | 0.97  | 5602  | [38]
Kepler-283b  |  | 0.19  | 11.008151  | 0.082  |  | transit  | 1540±20  |  | 4351  | [38]
Kepler-283c |  | 0.162  | 92.743711  | 0.341  |  | transit  | 1540±20  |  | 4351  | [38]
Kepler-284b  |  | 0.2  | 12.699149  | 0.104  |  | transit  | 3460±110  |  | 5615  | [38]
Kepler-284c  |  | 0.233  | 37.514456  | 0.213  |  | transit  | 3460±110  |  | 5615  | [38]
Kepler-285b  |  | 0.12  | 2.633867  | 0.036  |  | transit  | 2750±50  | 0.85  | 5411  | [38]
Kepler-285c  |  | 0.1  | 6.186676  | 0.064  |  | transit  | 2750±50  | 0.85  | 5411  | [38]
Kepler-286b  |  | 0.111  | 1.796302  | 0.027  |  | transit  | 4100±400  |  | 5580  | [38]
Kepler-286c  |  | 0.122  | 3.468095  | 0.042  |  | transit  | 4100±400  |  | 5580  | [38]
Kepler-286d  |  | 0.119  | 5.914323  | 0.061  |  | transit  | 4100±400  |  | 5580  | [38]
Kepler-286e  |  | 0.158  | 29.221289  | 0.176  |  | transit  | 4100±400  |  | 5580  | [38]
Kepler-287b  |  | 0.208  | 20.342199  | 0.145  |  | transit  | 2790±50  |  | 5806  | [38]
Kepler-287c  |  | 0.291  | 44.851896  | 0.246  |  | transit  | 2790±50  |  | 5806  | [38]
Kepler-288b  |  | 0.149  | 6.097326  | 0.065  |  | transit  | 4030±110  | 0.89  | 5918  | [38]
Kepler-288c  |  | 0.254  | 19.305772  | 0.14  |  | transit  | 4030±110  | 0.89  | 5918  | [38]
Kepler-288d  |  | 0.238  | 56.633742  | 0.287  |  | transit  | 4030±110  | 0.89  | 5918  | [38]
Kepler-289b | 0.023  | 0.192  | 34.545  | 0.21  |  | transit  | 2340±20  | 1.08  | 5990  | [38]
Kepler-289c | 0.42  | 1.034  | 125.8518  | 0.51  |  | transit  | 2340±20  | 1.08  | 5990  | [38]
Kepler-289d | 0.013  | 0.239  | 66.0634  | 0.33  |  | transit  | 2340±20  | 1.08  | 5990  | ?
Kepler-290b  |  | 0.201  | 14.589347  | 0.11  |  | transit  | 2310±40  |  | 5147  | [38]
Kepler-290c  |  | 0.241  | 36.77031  | 0.205  |  | transit  | 2310±40  |  | 5147  | [38]
Kepler-291b  |  | 0.193  | 3.546511  | 0.047  |  | transit  | 6100±400  | 1.03  | 6002  | [38]
Kepler-291c  |  | 0.168  | 5.700786  | 0.065  |  | transit  | 6100±400  | 1.03  | 6002  | [38]
Kepler-292b  |  | 0.118  | 2.580827  | 0.035  |  | transit  | 3540±150  | 0.88  | 5299  | [38]
Kepler-292c  |  | 0.131  | 3.715335  | 0.045  |  | transit  | 3540±150  | 0.88  | 5299  | [38]
Kepler-292d  |  | 0.199  | 7.055679  | 0.068  |  | transit  | 3540±150  | 0.88  | 5299  | [38]
Kepler-292e  |  | 0.238  | 11.97901  | 0.097  |  | transit  | 3540±150  | 0.88  | 5299  | [38]
Kepler-292f  |  | 0.21  | 20.834237  | 0.141  |  | transit  | 3540±150  | 0.88  | 5299  | [38]
Kepler-293b  |  | 0.274  | 19.254196  | 0.144  |  | transit  | 3260±70  | 1.01  | 5804  | [38]
Kepler-293c  |  | 0.342  | 54.155743  | 0.286  |  | transit  | 3260±70  | 1.01  | 5804  | [38]
Kepler-294b  |  | 0.158  | 3.701212  | 0.048  |  | transit  | 4600±200  |  | 5913  | [38]
Kepler-294c  |  | 0.242  | 6.6264  | 0.071  |  | transit  | 4600±200  |  | 5913  | [38]
Kepler-295b  |  | 0.109  | 12.645164  | 0.099  |  | transit  | 5800±300  |  | 5603  | [38]
Kepler-295c  |  | 0.104  | 21.526258  | 0.142  |  | transit  | 5800±300  |  | 5603  | [38]
Kepler-295d  |  | 0.121  | 33.884054  | 0.192  |  | transit  | 5800±300  |  | 5603  | [38]
Kepler-296b |  | 0.144  | 10.864384  | 0.079  |  | transit  | 740  | 0.5  | 3740  | [38]
Kepler-296c  |  | 0.178  | 5.8416366  | 0.0521  |  | transit  | 740  | 0.5  | 3740  | [38]
Kepler-296d |  | 0.186  | 19.850291  | 0.118  |  | transit  | 740  | 0.5  | 3740  | [38]
Kepler-296e |  | 0.136  | 34.14211  | 0.169  |  | transit  | 740  | 0.5  | 3740  | [38]
Kepler-296f |  | 0.161  | 63.33627  | 0.255  |  | transit  | 740  | 0.5  | 3740  | [38]
Kepler-297b  |  | 0.256  | 38.871826  | 0.217  |  | transit  | 2300±20  |  | 5619  | [38]
Kepler-297c  |  | 0.583  | 74.920137  | 0.336  |  | transit  | 2300±20  |  | 5619  | [38]
Kepler-298b  |  | 0.175  | 10.475464  | 0.08  |  | transit  | 1710±20  | 0.65  | 4465  | [38]
Kepler-298c  |  | 0.172  | 22.92881  | 0.136  |  | transit  | 1710±20  | 0.65  | 4465  | [38]
Kepler-298d |  | 0.223  | 77.473633  | 0.305  |  | transit  | 1710±20  | 0.65  | 4465  | [38]
Kepler-299b  |  | 0.118  | 2.927128  | 0.04  |  | transit  | 3530±80  | 0.97  | 5617  | [38]
Kepler-299c  |  | 0.236  | 6.885875  | 0.07  |  | transit  | 3530±80  | 0.97  | 5617  | [38]
Kepler-299d  |  | 0.166  | 15.054786  | 0.118  |  | transit  | 3530±80  | 0.97  | 5617  | [38]
Kepler-299e  |  | 0.167  | 38.285489  | 0.22  |  | transit  | 3530±80  | 0.97  | 5617  | [38]
Kepler-300b  |  | 0.149  | 10.446347  | 0.094  |  | transit  | 3690±60  | 0.94  | 5986  | [38]
Kepler-300c  |  | 0.201  | 40.714955  | 0.232  |  | transit  | 3690±60  | 0.94  | 5986  | [38]
Kepler-301b  |  | 0.12  | 2.508553  | 0.036  |  | transit  | 2390±30  | 0.91  | 5815  | [38]
Kepler-301c  |  | 0.12  | 5.419026  | 0.06  |  | transit  | 2390±30  | 0.91  | 5815  | [38]
Kepler-301d  |  | 0.156  | 13.751243  | 0.112  |  | transit  | 2390±30  | 0.91  | 5815  | [38]
Kepler-302b  |  | 0.362  | 30.184104  | 0.193  |  | transit  | 4760±190  |  | 5740  | [38]
Kepler-302c  |  | 1.111  | 127.282184  | 0.503  |  | transit  | 4760±190  |  | 5740  | [38]
Kepler-303b  |  | 0.079  | 1.937055  | 0.024  |  | transit  | 688±3  | 0.59  | 3944  | [38]
Kepler-303c  |  | 0.102  | 7.061149  | 0.057  |  | transit  | 688±3  | 0.59  | 3944  | [38]
Kepler-304b  |  | 0.255  | 3.295709  | 0.039  |  | transit  | 1435±17  | 0.8  | 4731  | [38]
Kepler-304c  |  | 0.194  | 5.315946  | 0.054  |  | transit  | 1435±17  | 0.8  | 4731  | [38]
Kepler-304d  |  | 0.245  | 9.653471  | 0.08  |  | transit  | 1435±17  | 0.8  | 4731  | [38]
Kepler-305d  |  | 0.242  | 16.738661  | 0.121  |  | transit  | 2900±80  | 0.76  | 5100  | [38]
Kepler-306b  |  | 0.136  | 4.646186  | 0.05  |  | transit  | 2580±60  | 0.82  | 4954  | [38]
Kepler-306c  |  | 0.21  | 7.240193  | 0.067  |  | transit  | 2580±60  | 0.82  | 4954  | [38]
Kepler-306d  |  | 0.22  | 17.326644  | 0.12  |  | transit  | 2580±60  | 0.82  | 4954  | [38]
Kepler-306e  |  | 0.203  | 44.840975  | 0.227  |  | transit  | 2580±60  | 0.82  | 4954  | [38]
Kepler-308b  |  | 0.189  | 9.694928  | 0.09  |  | transit  | 4500±200  |  | 5895  | [38]
Kepler-308c  |  | 0.193  | 15.38231  | 0.123  |  | transit  | 4500±200  |  | 5895  | [38]
Kepler-309b  |  | 0.139  | 5.923653  | 0.059  |  | transit  | 1804±19  |  | 4713  | [38]
Kepler-309c  |  | 0.224  | 105.356383  | 0.401  |  | transit  | 1804±19  |  | 4713  | [38]
Kepler-310b  |  | 0.106  | 13.930698  | 0.111  |  | transit  | 1990±20  | 0.85  | 5797  | [38]
Kepler-310c  |  | 0.302  | 56.47542  | 0.281  |  | transit  | 1990±20  | 0.85  | 5797  | [38]
Kepler-310d  |  | 0.22  | 92.876125  | 0.392  |  | transit  | 1990±20  | 0.85  | 5797  | [38]
Kepler-311b  |  | 0.152  | 9.176092  | 0.087  |  | transit  | 2590±30  | 1.06  | 5905  | [38]
Kepler-311c  |  | 0.128  | 19.738286  | 0.145  |  | transit  | 2590±30  | 1.06  | 5905  | [38]
Kepler-312b  |  | 0.115  | 1.772419  | 0.031  |  | transit  | 2660±40  | 1.23  | 6115  | [38]
Kepler-312c  |  | 0.281  | 19.747412  | 0.153  |  | transit  | 2660±40  | 1.23  | 6115  | [38]
Kepler-313b  |  | 0.226  | 14.970418  | 0.125  |  | transit  | 3500±300  | 0.9  | 5727  | [38]
Kepler-313c  |  | 0.229  | 32.273273  | 0.208  |  | transit  | 3500±300  | 0.9  | 5727  | [38]
Kepler-314b  |  | 0.074  | 2.461069  | 0.035  |  | transit  | 883±5  | 1.02  | 5378  | [38]
Kepler-314c  |  | 0.259  | 5.960392  | 0.064  |  | transit  | 883±5  | 1.02  | 5378  | [38]
Kepler-315b  |  | 0.336  | 96.101141  | 0.402  |  | transit  | 3910±120  | 0.78  | 5796  | [38]
Kepler-315c  |  | 0.37  | 265.469335  | 0.791  |  | transit  | 3910±120  | 0.78  | 5796  | [38]
Kepler-316b  |  | 0.095  | 2.240508  | 0.027  |  | transit  | 1269±12  | 0.53  | 4204  | [38]
Kepler-316c  |  | 0.103  | 6.827766  | 0.058  |  | transit  | 1269±12  | 0.53  | 4204  | [38]
Kepler-317b  |  | 0.186  | 5.524242  | 0.061  |  | transit  | 3150±80  | 0.95  | 5497  | [38]
Kepler-317c  |  | 0.153  | 8.77501  | 0.083  |  | transit  | 3150±80  | 0.95  | 5497  | [38]
Kepler-318b  |  | 0.42  | 4.662715  | 0.056  |  | transit  | 1618±10  | 1.05  | 5746  | [38]
Kepler-318c  |  | 0.328  | 11.815007  | 0.105  |  | transit  | 1618±10  | 1.05  | 5746  | [38]
Kepler-319b  |  | 0.145  | 4.362705  | 0.051  |  | transit  | 1666±15  | 1.29  | 5526  | [38]
Kepler-319c  |  | 0.235  | 6.941357  | 0.069  |  | transit  | 1666±15  | 1.29  | 5526  | [38]
Kepler-319d  |  | 0.204  | 31.781925  | 0.191  |  | transit  | 1666±15  | 1.29  | 5526  | [38]
Kepler-320b  |  | 0.102  | 8.371554  | 0.085  |  | transit  | 2760±30  |  | 6435  | [38]
Kepler-320c  |  | 0.122  | 17.934937  | 0.142  |  | transit  | 2760±30  |  | 6435  | [38]
Kepler-321b  |  | 0.158  | 4.915379  | 0.057  |  | transit  | 1268±11  | 1.01  | 5740  | [38]
Kepler-321c  |  | 0.207  | 13.093921  | 0.11  |  | transit  | 1268±11  | 1.01  | 5740  | [38]
Kepler-322b  |  | 0.09  | 1.653888  | 0.027  |  | transit  | 1321±8  | 0.91  | 5388  | [38]
Kepler-322c  |  | 0.149  | 4.337234  | 0.051  |  | transit  | 1321±8  | 0.91  | 5388  | [38]
Kepler-323b  |  | 0.128  | 1.678327  | 0.028  |  | transit  | 1500±20  | 1.09  | 5987  | [38]
Kepler-323c  |  | 0.145  | 3.553822  | 0.046  |  | transit  | 1500±20  | 1.09  | 5987  | [38]
Kepler-324b  |  | 0.102  | 4.385315  | 0.05  |  | transit  | 1659±12  | 0.86  | 5194  | [38]
Kepler-324c  |  | 0.281  | 51.805612  | 0.26  |  | transit  | 1659±12  | 0.86  | 5194  | [38]
Kepler-325b  |  | 0.26  | 4.544439  | 0.053  |  | transit  | 2740±40  | 0.87  | 5752  | [38]
Kepler-325c  |  | 0.227  | 12.762172  | 0.105  |  | transit  | 2740±40  | 0.87  | 5752  | [38]
Kepler-325d  |  | 0.249  | 38.715185  | 0.22  |  | transit  | 2740±40  | 0.87  | 5752  | [38]
Kepler-326b  |  | 0.136  | 2.248329  | 0.032  |  | transit  | 1610±30  | 0.98  | 5105  | [38]
Kepler-326c  |  | 0.125  | 4.580358  | 0.051  |  | transit  | 1610±30  | 0.98  | 5105  | [38]
Kepler-326d  |  | 0.108  | 6.766888  | 0.066  |  | transit  | 1610±30  | 0.98  | 5105  | [38]
Kepler-327b  |  | 0.099  | 2.549575  | 0.029  |  | transit  | 794±4  | 0.55  | 3799  | [38]
Kepler-327c  |  | 0.092  | 5.212333  | 0.047  |  | transit  | 794±4  | 0.55  | 3799  | [38]
Kepler-327d  |  | 0.154  | 13.969457  | 0.09  |  | transit  | 794±4  | 0.55  | 3799  | [38]
Kepler-329b  |  | 0.125  | 7.416397  | 0.061  |  | transit  | 1450±20  | 0.53  | 4257  | [38]
Kepler-329c  |  | 0.172  | 18.684737  | 0.113  |  | transit  | 1450±20  | 0.53  | 4257  | [38]
Kepler-330b  |  | 0.12  | 8.25978  | 0.075  |  | transit  | 2380±40  | 0.78  | 5117  | [38]
Kepler-330c  |  | 0.174  | 15.955387  | 0.116  |  | transit  | 2380±40  | 0.78  | 5117  | [38]
Kepler-331b  |  | 0.162  | 8.457496  | 0.065  |  | transit  | 1920±40  | 0.51  | 4347  | [38]
Kepler-331c  |  | 0.164  | 17.28111  | 0.105  |  | transit  | 1920±40  | 0.51  | 4347  | [38]
Kepler-331d  |  | 0.146  | 32.134328  | 0.159  |  | transit  | 1920±40  | 0.51  | 4347  | [38]
Kepler-332b  |  | 0.104  | 7.626324  | 0.07  |  | transit  | 1133±5  | 0.8  | 4955  | [38]
Kepler-332c  |  | 0.097  | 15.995622  | 0.114  |  | transit  | 1133±5  | 0.8  | 4955  | [38]
Kepler-332d  |  | 0.105  | 34.21154  | 0.189  |  | transit  | 1133±5  | 0.8  | 4955  | [38]
Kepler-333b  |  | 0.118  | 12.551158  | 0.087  |  | transit  | 1068±7  | 0.54  | 4259  | [38]
Kepler-333c  |  | 0.099  | 24.08821  | 0.135  |  | transit  | 1068±7  | 0.54  | 4259  | [38]
Kepler-334b  |  | 0.1  | 5.470319  | 0.061  |  | transit  | 1408±14  | 1  | 5828  | [38]
Kepler-334c  |  | 0.128  | 12.758005  | 0.107  |  | transit  | 1408±14  | 1  | 5828  | [38]
Kepler-334d  |  | 0.126  | 25.09849  | 0.168  |  | transit  | 1408±14  | 1  | 5828  | [38]
Kepler-335b  |  | 0.302  | 6.562331  | 0.075  |  | transit  | 4320±100  | 0.99  | 5877  | [38]
Kepler-335c  |  | 0.274  | 67.844469  | 0.356  |  | transit  | 4320±100  | 0.99  | 5877  | [38]
Kepler-336b  |  | 0.091  | 2.024823  | 0.033  |  | transit  | 8000±7000  | 0.89  | 5867  | [38]
Kepler-336c  |  | 0.187  | 9.600001  | 0.092  |  | transit  | 8000±7000  | 0.89  | 5867  | [38]
Kepler-336d  |  | 0.211  | 20.678772  | 0.154  |  | transit  | 8000±7000  | 0.89  | 5867  | [38]
Kepler-337b  |  | 0.137  | 3.292781  | 0.045  |  | transit  | 2250±30  | 0.96  | 5684  | [38]
Kepler-337c  |  | 0.183  | 9.693201  | 0.093  |  | transit  | 2250±30  | 0.96  | 5684  | [38]
Kepler-338b  |  | 0.218  | 13.726976  | 0.117  |  | transit  | 1830±20  | 1.1  | 5923  | [38]
Kepler-338c  |  | 0.209  | 24.310856  | 0.172  |  | transit  | 1830±20  | 1.1  | 5923  | [38]
Kepler-338d  |  | 0.268  | 44.431014  | 0.257  |  | transit  | 1830±20  | 1.1  | 5923  | [38]
Kepler-338e  | 0.027  | 0.139  | 9.341  |  |  | timing  | 1830±20  | 1.1  | 5923  | ?
Kepler-339b  |  | 0.127  | 4.977656  | 0.055  |  | transit  | 2040±30  | 0.84  | 5631  | [38]
Kepler-339c  |  | 0.103  | 6.988055  | 0.069  |  | transit  | 2040±30  | 0.84  | 5631  | [38]
Kepler-339d  |  | 0.104  | 10.558345  | 0.091  |  | transit  | 2040±30  | 0.84  | 5631  | [38]
Kepler-340b  |  | 0.226  | 14.844387  | 0.134  |  | transit  | 2690±60  | 2.11  | 6620  | [38]
Kepler-340c  |  | 0.301  | 22.824669  | 0.178  |  | transit  | 2690±60  | 2.11  | 6620  | [38]
Kepler-341b  |  | 0.105  | 5.195528  | 0.06  |  | transit  | 3520±60  | 0.94  | 6012  | [38]
Kepler-341c  |  | 0.152  | 8.01041  | 0.08  |  | transit  | 3520±60  | 0.94  | 6012  | [38]
Kepler-341d  |  | 0.165  | 27.666313  | 0.182  |  | transit  | 3520±60  | 0.94  | 6012  | [38]
Kepler-341e  |  | 0.178  | 42.473269  | 0.242  |  | transit  | 3520±60  | 0.94  | 6012  | [38]
Kepler-342b  |  | 0.201  | 15.170318  | 0.128  |  | transit  | 2600±30  | 1.13  | 6175  | [38]
Kepler-342c  |  | 0.175  | 26.234138  | 0.185  |  | transit  | 2600±30  | 1.13  | 6175  | [38]
Kepler-342d  |  | 0.222  | 39.459357  | 0.242  |  | transit  | 2600±30  | 1.13  | 6175  | [38]
Kepler-343b  |  | 0.215  | 8.96855  | 0.088  |  | transit  | 3100±60  | 1.04  | 5807  | [38]
Kepler-343c  |  | 0.18  | 23.22182  | 0.167  |  | transit  | 3100±60  | 1.04  | 5807  | [38]
Kepler-344b  |  | 0.233  | 21.963945  | 0.153  |  | transit  | 3360±100  | 0.9  | 5774  | [38]
Kepler-344c  |  | 0.263  | 125.596809  | 0.488  |  | transit  | 3360±100  | 0.9  | 5774  | [38]
Kepler-345b |  | 0.066  | 7.415563  | 0.066  |  | transit  | 1180±50  | 0.59  | 4504  | [38]
Kepler-345c  |  | 0.107  | 9.387427  | 0.077  |  | transit  | 1180±50  | 0.59  | 4504  | [38]
Kepler-346b  |  | 0.237  | 6.511127  | 0.071  |  | transit  | 3300±80  | 0.97  | 6033  | [38]
Kepler-346c  |  | 0.274  | 23.851549  | 0.168  |  | transit  | 3300±80  | 0.97  | 6033  | [38]
Kepler-347b  |  | 0.176  | 12.79836  | 0.11  |  | transit  | 4400±90  | 1.04  | 6088  | [38]
Kepler-347c  |  | 0.156  | 27.320871  | 0.183  |  | transit  | 4400±90  | 1.04  | 6088  | [38]
Kepler-348b  |  | 0.136  | 7.05677  | 0.076  |  | transit  | 1890±20  | 1.15  | 6177  | [38]
Kepler-348c  |  | 0.119  | 17.265427  | 0.138  |  | transit  | 1890±20  | 1.15  | 6177  | [38]
Kepler-349b  |  | 0.17  | 5.929778  | 0.065  |  | transit  | 3150±60  | 0.97  | 5956  | [38]
Kepler-349c  |  | 0.175  | 12.247629  | 0.105  |  | transit  | 3150±60  | 0.97  | 5956  | [38]
Kepler-350b  |  | 0.165  | 11.189562  | 0.104  |  | transit  | 3200±60  | 1  | 6186  | [38]
Kepler-351b  |  | 0.273  | 37.054919  | 0.214  |  | transit  | 3640±40  | 0.89  | 5643  | [38]
Kepler-351c  |  | 0.285  | 57.24809  | 0.287  |  | transit  | 3640±40  | 0.89  | 5643  | [38]
Kepler-352b  |  | 0.077  | 10.05537  | 0.085  |  | transit  | 830±4  | 0.79  | 5212  | [38]
Kepler-352c  |  | 0.111  | 16.332995  | 0.118  |  | transit  | 830±4  | 0.79  | 5212  | [38]
Kepler-353b  |  | 0.079  | 5.795278  | 0.051  |  | transit  | 1268±16  | 0.54  | 3903  | [38]
Kepler-353c  |  | 0.123  | 8.410894  | 0.065  |  | transit  | 1268±16  | 0.54  | 3903  | [38]
Kepler-354b  |  | 0.164  | 5.47666  | 0.054  |  | transit  | 1830±20  | 0.65  | 4648  | [38]
Kepler-354c  |  | 0.117  | 16.934402  | 0.115  |  | transit  | 1830±20  | 0.65  | 4648  | [38]
Kepler-354d  |  | 0.111  | 24.209842  | 0.146  |  | transit  | 1830±20  | 0.65  | 4648  | [38]
Kepler-355b  |  | 0.13  | 11.03189  | 0.102  |  | transit  | 4870±160  | 1.05  | 6184  | [38]
Kepler-355c  |  | 0.242  | 25.762294  | 0.179  |  | transit  | 4870±160  | 1.05  | 6184  | [38]
Kepler-356b  |  | 0.14  | 4.612696  | 0.057  |  | transit  | 2350±30  | 0.97  | 6133  | [38]
Kepler-356c  |  | 0.161  | 13.121632  | 0.115  |  | transit  | 2350±30  | 0.97  | 6133  | [38]
Kepler-357b  |  | 0.164  | 6.475434  | 0.063  |  | transit  | 2290±40  | 0.78  | 5036  | [38]
Kepler-357c  |  | 0.238  | 16.85837  | 0.12  |  | transit  | 2290±40  | 0.78  | 5036  | [38]
Kepler-357d  |  | 0.306  | 49.499875  | 0.246  |  | transit  | 2290±40  | 0.78  | 5036  | [38]
Kepler-358b  |  | 0.243  | 34.060467  | 0.21  |  | transit  | 3700±130  | 0.95  | 5908  | [38]
Kepler-358c  |  | 0.254  | 83.488369  | 0.381  |  | transit  | 3700±130  | 0.95  | 5908  | [38]
Kepler-359b  |  | 0.315  | 25.563222  | 0.178  |  | transit  | 4900±300  | 1.07  | 6248  | [38]
Kepler-359c  |  | 0.384  | 57.68802  | 0.307  |  | transit  | 4900±300  | 1.07  | 6248  | [38]
Kepler-359d  |  | 0.358  | 77.095691  | 0.372  |  | transit  | 4900±300  | 1.07  | 6248  | [38]
Kepler-360b  |  | 0.147  | 3.289672  | 0.044  |  | transit  | 2930±50  | 0.95  | 6053  | [38]
Kepler-360c  |  | 0.187  | 7.186434  | 0.075  |  | transit  | 2930±50  | 0.95  | 6053  | [38]
Kepler-361b  |  | 0.129  | 8.486616  | 0.086  |  | transit  | 3110±50  | 1.07  | 6169  | [38]
Kepler-361c  |  | 0.225  | 55.188023  | 0.3  |  | transit  | 3110±50  | 1.07  | 6169  | [38]
Kepler-362b  |  | 0.079  | 10.327186  | 0.087  |  | transit  | 3660±180  | 0.77  | 5788  | [38]
Kepler-362c  |  | 0.129  | 37.866281  | 0.207  |  | transit  | 3660±180  | 0.77  | 5788  | [38]
Kepler-363b  |  | 0.103  | 3.614568  | 0.048  |  | transit  | 2540±20  | 1.23  | 5593  | [38]
Kepler-363c  |  | 0.151  | 7.542427  | 0.079  |  | transit  | 2540±20  | 1.23  | 5593  | [38]
Kepler-363d  |  | 0.183  | 11.932125  | 0.107  |  | transit  | 2540±20  | 1.23  | 5593  | [38]
Kepler-364b  |  | 0.138  | 25.745718  | 0.178  |  | transit  | 2980±30  | 1.2  | 6108  | [38]
Kepler-364c  |  | 0.192  | 59.980627  | 0.312  |  | transit  | 2980±30  | 1.2  | 6108  | [38]
Kepler-365b  |  | 0.182  | 10.664903  | 0.098  |  | transit  | 2800±200  | 0.99  | 6012  | [38]
Kepler-365c  |  | 0.146  | 17.784129  | 0.137  |  | transit  | 2800±200  | 0.99  | 6012  | [38]
Kepler-366b  |  | 0.13  | 3.281959  | 0.045  |  | transit  | 6400±400  | 1.05  | 6209  | [38]
Kepler-366c  |  | 0.16  | 12.51616  | 0.11  |  | transit  | 6400±400  | 1.05  | 6209  | [38]
Kepler-367b  |  | 0.116  | 37.815724  | 0.201  |  | transit  | 616±2  | 0.75  | 4710  | [38]
Kepler-367c  |  | 0.107  | 53.578637  | 0.253  |  | transit  | 616±2  | 0.75  | 4710  | [38]
Kepler-368b  |  | 0.291  | 26.84768  | 0.186  |  | transit  | 2570±40  | 0.71  | 5502  | [38]
Kepler-368c  |  | 0.346  | 72.379334  | 0.36  |  | transit  | 2570±40  | 0.71  | 5502  | [38]
Kepler-369b  |  | 0.101  | 2.732756  | 0.03  |  | transit  | 840±120  | 0.54  | 3591  | [38]
Kepler-369c  |  | 0.126  | 14.871572  | 0.094  |  | transit  | 840±120  | 0.54  | 3591  | [38]
Kepler-370b  |  | 0.142  | 4.57953  | 0.054  |  | transit  | 3930±120  | 0.94  | 5852  | [38]
Kepler-370c  |  | 0.17  | 19.02293  | 0.14  |  | transit  | 3930±120  | 0.94  | 5852  | [38]
Kepler-371b |  | 0.169  | 34.763278  | 0.2  |  | transit  | 2710±40  | 0.94  | 5666  | [38]
Kepler-371c |  | 0.159  | 67.968015  | 0.313  |  | transit  | 2710±40  | 0.94  | 5666  | [38]
Kepler-372b  |  | 0.121  | 6.849692  | 0.075  |  | transit  | 5090±170  | 1.15  | 6509  | [38]
Kepler-372c  |  | 0.186  | 20.053763  | 0.154  |  | transit  | 5090±170  | 1.15  | 6509  | [38]
Kepler-372d  |  | 0.151  | 30.092568  | 0.201  |  | transit  | 5090±170  | 1.15  | 6509  | [38]
Kepler-373b  |  | 0.121  | 5.535309  | 0.06  |  | transit  | 3670±70  | 0.87  | 5787  | [38]
Kepler-373c  |  | 0.111  | 16.725948  | 0.126  |  | transit  | 3670±70  | 0.87  | 5787  | [38]
Kepler-374b  |  | 0.092  | 1.897806  | 0.029  |  | transit  | 4280±120  | 0.84  | 5977  | [38]
Kepler-374c  |  | 0.098  | 3.282807  | 0.042  |  | transit  | 4280±120  | 0.84  | 5977  | [38]
Kepler-374d  |  | 0.117  | 5.028219  | 0.056  |  | transit  | 4280±120  | 0.84  | 5977  | [38]
Kepler-375b  |  | 0.129  | 12.125934  | 0.101  |  | transit  | 4180±180  | 0.89  | 5826  | [38]
Kepler-375c  |  | 0.236  | 19.986326  | 0.141  |  | transit  | 4180±180  | 0.89  | 5826  | [38]
Kepler-376b  |  | 0.095  | 4.920199  | 0.057  |  | transit  | 3090±50  | 1.05  | 5900  | [38]
Kepler-376c  |  | 0.16  | 14.172327  | 0.115  |  | transit  | 3090±50  | 1.05  | 5900  | [38]
Kepler-377b  |  | 0.124  | 12.509529  | 0.109  |  | transit  | 2750±40  | 0.88  | 5949  | [38]
Kepler-377c  |  | 0.184  | 27.014976  | 0.182  |  | transit  | 2750±40  | 0.88  | 5949  | [38]
Kepler-378b  |  | 0.067  | 16.092361  | 0.112  |  | transit  | 498.3±1.4  | 0.96  | 4661  | [38]
Kepler-378c  |  | 0.062  | 28.906009  | 0.166  |  | transit  | 498.3±1.4  | 0.96  | 4661  | [38]
Kepler-379b  |  | 0.148  | 20.09838  | 0.152  |  | transit  | 2430±20  | 1.08  | 6054  | [38]
Kepler-379c  |  | 0.204  | 62.784697  | 0.326  |  | transit  | 2430±20  | 1.08  | 6054  | [38]
Kepler-380b  |  | 0.106  | 3.930821  | 0.05  |  | transit  | 2710±40  | 1.05  | 6045  | [38]
Kepler-380c  |  | 0.113  | 7.630004  | 0.078  |  | transit  | 2710±40  | 1.05  | 6045  | [38]
Kepler-381b  |  | 0.088  | 5.629021  | 0.066  |  | transit  | 878±5  | 1.34  | 6152  | [38]
Kepler-381c  |  | 0.1  | 13.391635  | 0.117  |  | transit  | 878±5  | 1.34  | 6152  | [38]
Kepler-382b  |  | 0.118  | 5.262155  | 0.055  |  | transit  | 3130±60  | 0.8  | 5600  | [38]
Kepler-382c  |  | 0.142  | 12.162701  | 0.097  |  | transit  | 3130±60  | 0.8  | 5600  | [38]
Kepler-383b  |  | 0.118  | 12.904532  | 0.095  |  | transit  | 1695  | 0.67  | 4710  | [38]
Kepler-383c  |  | 0.111  | 31.200751  | 0.172  |  | transit  | 1695  | 0.67  | 4710  | [38]
Kepler-384b  |  | 0.1  | 22.597053  | 0.148  |  | transit  | 2990±30  | 0.76  | 5577  | [38]
Kepler-384c  |  | 0.101  | 45.348269  | 0.236  |  | transit  | 2990±30  | 0.76  | 5577  | [38]
Kepler-385b |  | 0.244  | 10.043686  | 0.097  |  | transit  | 4870±160  | 1.09  | 6326  | [38]
Kepler-385c |  | 0.271  | 15.163161  | 0.127  |  | transit  | 4870±160  | 1.09  | 6326  | [38]
Kepler-386b  |  | 0.124  | 12.31043  | 0.096  |  | transit  | 2950±90  | 0.74  | 5178  | [38]
Kepler-386c  |  | 0.141  | 25.193458  | 0.155  |  | transit  | 2950±90  | 0.74  | 5178  | [38]
Kepler-387b  |  | 0.092  | 6.791636  | 0.068  |  | transit  | 2670±30  | 1.03  | 5774  | [38]
Kepler-387c  |  | 0.079  | 11.837549  | 0.098  |  | transit  | 2670±30  | 1.03  | 5774  | [38]
Kepler-388b  |  | 0.072  | 3.173315  | 0.036  |  | transit  | 2000±200  | 0.59  | 4498  | [38]
Kepler-388c  |  | 0.077  | 13.297004  | 0.093  |  | transit  | 2000±200  | 0.59  | 4498  | [38]
Kepler-389b  |  | 0.135  | 3.244107  | 0.041  |  | transit  | 2720±70  | 0.78  | 5376  | [38]
Kepler-389c  |  | 0.13  | 14.51143  | 0.11  |  | transit  | 2720±70  | 0.78  | 5376  | [38]
Kepler-390b  |  | 0.073  | 6.738088  | 0.065  |  | transit  | 1437±12  | 0.67  | 5166  | [38]
Kepler-390c  |  | 0.07  | 13.060022  | 0.101  |  | transit  | 1437±12  | 0.67  | 5166  | [38]
Kepler-391b  |  | 0.285  | 7.416755  | 0.082  |  | transit  | 2900±40  | 1.22  | 4940  | [38]
Kepler-391c  |  | 0.316  | 20.485435  | 0.161  |  | transit  | 2900±40  | 1.22  | 4940  | [38]
Kepler-392b  |  | 0.089  | 5.341853  | 0.059  |  | transit  | 2260±20  | 1.13  | 5938  | [38]
Kepler-392c  |  | 0.098  | 10.423118  | 0.093  |  | transit  | 2260±20  | 1.13  | 5938  | [38]
Kepler-393b  |  | 0.115  | 9.182417  | 0.091  |  | transit  | 2940±40  | 1.32  | 6189  | [38]
Kepler-393c  |  | 0.119  | 14.613612  | 0.124  |  | transit  | 2940±40  | 1.32  | 6189  | [38]
Kepler-394b  |  | 0.143  | 8.005013  | 0.083  |  | transit  | 3560±80  | 1.11  | 6402  | [38]
Kepler-394c  |  | 0.148  | 12.130686  | 0.11  |  | transit  | 3560±80  | 1.11  | 6402  | [38]
Kepler-395b  |  | 0.092  | 7.054346  | 0.061  |  | transit  | 1390±20  | 0.53  | 4262  | [38]
Kepler-395c |  | 0.118  | 34.989262  | 0.177  |  | transit  | 1390±20  | 0.53  | 4262  | Potentially habitable exoplanet[38]
Kepler-397b  |  | 0.219  | 22.250949  | 0.144  |  | transit  | 3760  |  | 5307  | [38]
Kepler-397c  |  | 0.551  | 135.498527  | 0.48  |  | transit  | 3760  |  | 5307  | [38]
Kepler-398b  |  | 0.083  | 4.081423  | 0.044  |  | transit  | 581.4±1.8  |  | 4493  | [38]
Kepler-398c  |  | 0.09  | 11.419412  | 0.087  |  | transit  | 581.4±1.8  |  | 4493  | [38]
Kepler-399b  |  | 0.086  | 14.425281  | 0.103  |  | transit  | 4400±700  |  | 5502  | [38]
Kepler-399c  |  | 0.128  | 26.67569  | 0.155  |  | transit  | 4400±700  |  | 5502  | [38]
Kepler-399d  |  | 0.169  | 58.034616  | 0.261  |  | transit  | 4400±700  |  | 5502  | [38]
Kepler-400b  |  | 0.147  | 9.024389  | 0.087  |  | transit  | 2340  |  | 5886  | [38]
Kepler-400c  |  | 0.133  | 17.340824  | 0.134  |  | transit  | 2340  |  | 5886  | [38]
Kepler-401b  |  | 0.153  | 14.383035  | 0.122  |  | transit  | 3230±50  |  | 6117  | [38]
Kepler-401c  |  | 0.192  | 47.318218  | 0.269  |  | transit  | 3230±50  |  | 6117  | [38]
Kepler-402b  |  | 0.109  | 4.028751  | 0.051  |  | transit  | 2070±20  |  | 6090  | [38]
Kepler-402c  |  | 0.139  | 6.124821  | 0.068  |  | transit  | 2070±20  |  | 6090  | [38]
Kepler-402d  |  | 0.123  | 8.921099  | 0.087  |  | transit  | 2070±20  |  | 6090  | [38]
Kepler-402e  |  | 0.13  | 11.242861  | 0.102  |  | transit  | 2070±20  |  | 6090  | [38]
Kepler-403b  |  | 0.112  | 7.031462  | 0.076  |  | transit  | 2800±50  |  | 6090  | [38]
Kepler-403c  |  | 0.156  | 54.280749  | 0.297  |  | transit  | 2800±50  |  | 6090  | [38]
Kepler-404b  |  | 0.113  | 11.829851  | 0.102  |  | transit  | 2710±40  |  | 5654  | [38]
Kepler-404c  |  | 0.153  | 14.751166  | 0.118  |  | transit  | 2710±40  |  | 5654  | [38]
Kepler-405b  |  | 0.186  | 10.613839  | 0.095  |  | transit  | 3570±140  |  | 5818  | [38]
Kepler-405c  |  | 0.416  | 29.726682  | 0.188  |  | transit  | 3570±140  |  | 5818  | [38]
Kepler-406b  | 0.02  | 0.128  | 2.42629  |  |  | transit  | 1199±11  | 1.07  | 5538  | [39]
Kepler-406c  | 0.009  | 0.076  | 4.62332  |  |  | transit  | 1199±11  | 1.07  | 5538  | [39]
Kepler-407b  |  | 0.095  | 0.66931  |  |  | transit  | 1114±8  | 1  | 5476  | [39]
Kepler-407c  | 12.6  |  | 3000  |  |  | radial vel.  | 1114±8  | 1  | 5476  | [39]
Kepler-408b |  | 0.073  | 2.46502  |  |  | transit  | 290.3±0.9  | 1.08  | 6104  | Host star known as HD 176693 or KOI-1612. Reported as 2.1% false positive probable in 2014,[39] but confirmed by 2016.[41]
Kepler-409b |  | 0.106  | 68.9584  |  |  | transit  | 222.8±0.3  | 0.92  | 5460  | Host star known as Gliese 409[39]
Kepler-412b  | 0.941  | 1.341  | 1.7208604  | 0.02897  |  | transit  | 3650±60  | 1.17  | 5750  | [42]
Kepler-413b | 0.211  | 0.388  | 66.262  | 0.3553  |  | transit  | 2830±70  | 0.82  | 4700  | [43]
Kepler-414b  | 0.011  | 0.153  | 4.7  |  |  | timing  | 1364±9  | 0.89  |  | [44]
Kepler-414c  | 0.094  | 0.269  | 7.171  |  |  | timing  | 1364±9  | 0.89  |  | [44]
Kepler-415b  | 0.377  | 0.108  | 4.176  |  |  | timing  | 1750±30  | 0.67  |  | [44]
Kepler-415c  |  |  | 8.708  |  |  | transit  | 1750±30  | 0.67  |  | ?
Kepler-416b  | 0.183  | 0.221  | 6.319  |  |  | timing  | 2290±30  | 1  |  | [44]
Kepler-416c  |  |  | 12.209  |  |  | transit  | 2290±30  | 1  |  | ?
Kepler-417b  | 0.035  | 0.206  | 12.331  |  |  | transit  | 3250±150  | 0.9  |  | [44]
Kepler-417c  |  |  | 15.943  |  |  | transit  | 3250±150  | 0.9  |  | ?
Kepler-418b  | 1.1  | 1.2  | 86.67856  |  |  | transit  | 3360±60  | 0.98  | 5820  | [45]
Kepler-419b | 2.5  | 0.96  | 69.7546  | 0.37  |  | transit  | 3390±80  | 1.39  | 6430  | [46]
Kepler-419c | 7.3  |  | 675.47  | 1.68  |  | timing  | 3390±80  | 1.39  | 6430  | [46]
Kepler-420Ab  | 1.45  | 0.94  | 86.647661  | 0.382  | 511  | transit  | 2900  | 0.99  | 5520  | [47]
Kepler-421b |  | 0.371  | 704.1984  | 1.219  |  | transit  | 1148±6  | 0.79  | 5308  | [48]
Kepler-422b  | 0.43  | 1.15  | 7.8914483  | 0.082  |  | transit  | 2400±20  | 1.15  | 5972  | [49]
Kepler-423b  | 0.595  | 1.192  | 2.6843285  | 0.03585  | 1605  | transit  | 2520±40  | 0.85  | 5560  | [49]
Kepler-424b  | 1.03  | 0.89  | 3.3118644  | 0.044  |  | transit  | 2320±30  | 1.01  | 5460  | [49]
Kepler-424c  | 6.97  |  | 223.3  | 0.73  |  | radial vel.  | 2320±30  | 1.01  | 5460  | [49]
Kepler-425b  | 0.25  | 0.978  | 3.79701816  | 0.0464  | 1070  | transit  | 2140±30  | 0.93  | 5170  | [50]
Kepler-426b  | 0.34  | 1.09  | 3.21751883  | 0.0414  | 1300  | transit  | 2810±40  | 0.91  | 5725  | [50]
Kepler-427b  | 0.29  | 1.23  | 10.290994  | 0.091  | 1100  | transit  | 3410±50  | 0.96  | 5800  | [50]
Kepler-428b  | 1.27  | 1.08  | 3.52563254  | 0.0433  | 1070  | transit  | 2280±50  | 0.87  | 5150  | [50]
Kepler-430b  |  | 0.29  | 35.968  | 0.2244  | 667  | transit  | 3070±50  | 1.17  | 5884  | [51]
Kepler-430c  |  | 0.16  | 110.979  | 0.4757  | 458  | transit  | 3070±50  | 1.17  | 5884  | [51]
Kepler-431b  |  | 0.068  | 6.803  | 0.0719  | 1032  | transit  | 1609±15  | 1.07  | 6004  | [51]
Kepler-431c  |  | 0.06  | 8.703  | 0.0847  | 951  | transit  | 1609±15  | 1.07  | 6004  | [51]
Kepler-431d  |  | 0.1  | 11.922  | 0.1045  | 856  | transit  | 1609±15  | 1.07  | 6004  | [51]
Kepler-432b | 5.41  | 1.145  | 52.501129  | 0.301  |  | transit  | 2830±60  | 1.32  | 4995  | Eccentric orbit[52]
Kepler-432c | 2.43+0.22−0.24 |  | 406.2+3.9−2.5 |  |  | radial vel.  | 2830±60  | 1.32  | 4995  | [52]
Kepler-453b | 0.00063  | 0.553  | 240.503  | 0.7903  |  | transit  | 1463±9  | 0.94  | 5527  | [53]
Mu Leonis b | 2.4  |  | 357.8  | 1.1  |  | radial vel.  | 133.0  | 1.5  | 4538.2  | [3]
OGLE-2008-BLG-355Lb  | 4.6  |  |  | 1.7  |  | microlensing  | 22000  | 0.37  |  | [54]
OGLE-2008-BLG-92Lb  | 0.18  |  |  | 18  |  | microlensing  | 26000  | 0.71  |  | [55]
OGLE-2011-BLG-265Lb  | 0.88  |  |  | 1.89  |  | microlensing  | 14300  | 0.21  |  | [56]
OGLE-2013-BLG-102Lb  | 12.569  |  |  | 0.8  |  | microlensing  | 9900  | 0.1  |  | Additional planet or brown dwarf in the system.[57]
OGLE-2013-BLG-341LBb  | 0.0073  |  |  | 0.883  |  | microlensing  | 3790  | 0.15  |  | One more red dwarf in the system.[58]
OGLE-2014-BLG-0124Lb | 0.51  |  |  | 3.11  |  | microlensing  | 13000  | 0.71  |  | [59]
SAND364 b  | 1.54  |  | 121.71  |  |  | radial vel.  | 2730±130  | 1.35  | 4284  | Belongs to Messier 67, also known as BD+12 1917b[60]
TYC 1422-614-1 b  | 2.5  |  | 198.4  | 0.69  |  | radial vel.  | 2480  | 1.15  | 4806  | [61]
TYC 1422-614-1 c  | 10  |  | 559.3  | 1.37  |  | radial vel.  | 2480  | 1.15  | 4806  | [61]
WASP-20#Planetary system (ru)  | 0.72±0,06  | 1.32±0.03  | 3.16158  | 0.04317  |  | transit  | 663.39  | 1.05  | 5990  | Binary with planet orbiting primary star[62][63]
WASP-74b  | 0.95  | 1.56  | 2.13775  | 0.037  | 1910  | transit  | 390  | 1.48  | 5970  | [64]
WASP-83b  | 0.3  | 1.04  | 4.971252  | 0.059  | 1120  | transit  | 980  | 1.11  | 5510  | [64]
WASP-85Ab | 1.265  | 1.24  | 2.6556777  | 0.039  | 1452  | transit  | 243  | 1.09  | 6112  | [65]
WASP-87 b  | 2.18±0.15  | 1.39±0.06  | 1.6828  | 0.0295±0.0008  |  | transit  | 982±12  | 1.20±0.09  | 6450±120  | [66] Host star also known as CD-52 4998.
WASP-89b  | 5.9  | 1.04  | 3.3564227  | 0.0427  | 1120  | transit  | 957  | 0.92  | 5130  | [64]
WASP-94Ab  | 0.452  | 1.72  | 3.9501907  | 0.055  | 1604  | transit  | 590  | 1.45  | 6153  | [67]
WASP-94Bb  | 0.618  |  | 2.00839  | 0.0335  |  | radial vel.  | 590  | 1.24  | 6040  | [67]
WASP-103b | 1.49  | 1.528  | 0.925542  | 0.01985  | 2508  | transit  | 1500  | 1.22  | 6110  | Planet close to tidal disruption[68][69]
WASP-104b | 1.272  | 1.137  | 1.7554137  | 0.02918  | 1516  | transit  | 470  | 1.08  | 5475  | [70]
WASP-106b  | 1.925  | 1.085  | 9.289715  | 0.0917  | 1140  | transit  | 920  | 1.19  | 6055  | [70]
WASP-108 b  | 1.167+0.092−0.091 | 1.215±0.040  | 2.6755463±0.0000021  | 0.0397±0.001  | 1590  | transit  | 717.6±0.3  | 1.167±0.092  | 6000±140  | [66] Host star also known as TYC 8254-1624-1
WASP-109 b  | 0.91±0.13  | 1.443±0.053  | 3.3190233±0.0000042  | 0.0463±0.0011  | 1695  | transit  | 1173±16  | 1.203±0.090  | 6520±140  | [66] Host star also known as TYC 6184-1397-1
WASP-110 b  | 0.515±0.064  | 1.238±0.056  | 3.7783977±0.0000031  | 0.0457±0.0012  | 1134  | transit  | 904±10  | 0.892±0.072  | 5400±140  | [66]
WASP-111 b  | 1.85±0.16  | 1.442±0.094  | 2.310965±0.0000034  | 0.03914±0.00098  | 2140  | transit  | 980±20  | 1.50±0.11  | 6400±150  | [66] Host star also known as HD 208180
WASP-112 b  | 0.88±0.12  | 1.191±0.049  | 3.0353992±0.0000038  | 0.0382±0.0011  | 1395  | transit  | 1900±40  | 0.807±0.073  | 5610±130  | [66]
WASP-116b  | 0.59±0.05  | 1.43±0.07  | 6.61321±0.00002  | 0.0730±0.0011  | 1400±4  | transit  | 1770±60  | 1.25±0.18  | 5950±100  | [65]
WASP-117b  | 0.2755  | 1.021  | 10.02165  | 0.09459  | 1024  | transit  | 518±2  | 1.13  | 6038  | [71][72]
WASP-149b  | 1.02±0.04  | 1.32±0.04  | 1.332811±0.000001  | 0.0247±0.0004  | 1870±1  | transit  | 1770±60  | 1.12±0.17  | 5750±100  | [65]
XO-2Sb | 0.259  |  | 18.157  | 0.1344  |  | radial vel.  | 480  | 0.98  | 5399  | [73]
XO-2Sc | 1.37  |  | 120.8  | 0.4756  |  | radial vel.  | 480  | 0.98  | 5399  | [73]
YBP 1194 b | 0.32  |  | 6.959  |  |  | radial vel.  | 2920±100  | 1.01  | 5780  | Belongs to Messier 67[60]
YBP 1514 b  | 0.4  |  | 5.118  |  |  | radial vel.  | 3060±100  | 0.96  | 5725  | Belongs to Messier 67[60]

## Specific exoplanet lists

## References

1. ↑ "The Extrasolar Planets Encyclopaedia". Extrasolar Planets Encyclopaedia. 1995. https://exoplanet.eu/catalog/.
2. ↑ 2.0 2.1 2.2 2.3 2.4 Moutou, C.; Lo Curto, G.; Mayor, M.; Bouchy, F.; Benz, W.; Lovis, C.; Naef, D.; Pepe, F. et al. (2014), "The HARPS search for southern extra-solar planets XXXVI: Five new long-period giant planets and a system update", Astronomy & Astrophysics 576: A48, doi:10.1051/0004-6361/201424965
3. ↑ 3.0 3.1 3.2 Lee, B.-C. et al. (2014). "Planetary Companions in K giants β Cancri, μ Leonis, and β Ursae Minoris". Astronomy & Astrophysics 566: 7. doi:10.1051/0004-6361/201322608. A67. Bibcode: 2014A&A...566A..67L.
4. ↑ 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, doi:10.1093/mnras/stu1645
5. ↑ 5.0 5.1 Alonso, R. et al. (2014), "Transiting exoplanets from the CoRoT space mission", Astronomy & Astrophysics 567: A112, doi:10.1051/0004-6361/201118662
6. ↑ Parviainen, H. et al. (2014), "Transiting exoplanets from the CoRoT space mission", Astronomy & Astrophysics 562: A140, doi:10.1051/0004-6361/201323049
7. ↑ 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, doi:10.1093/mnras/sty3085
8. ↑ Howard, Andrew W.; Marcy, Geoffrey W.; Fischer, Debra A.; Isaacson, Howard; Muirhead, Philip S.; Henry, Gregory W.; Boyajian, Tabetha S.; von Braun, Kaspar et al. (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, doi:10.1088/0004-637X/794/1/51, Bibcode: 2014ApJ...794...51H
9. ↑ 9.0 9.1 9.2 9.3 9.4 9.5 9.6 9.7 9.8 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, doi:10.1093/mnras/stu358
10. ↑ 10.0 10.1 10.2 Feng, Fabo; Butler, R. Paul; Shectman, Stephen A.; Crane, Jeffrey D.; Vogt, Steve; Chambers, John; Jones, Hugh R. A.; Wang, Sharon Xuesong et al. (8 January 2020). "Search for Nearby Earth Analogs. II. Detection of Five New Planets, Eight Planet Candidates, and Confirmation of Three Planets around Nine Nearby M Dwarfs". The Astrophysical Journal Supplement Series 246 (1): 11. doi:10.3847/1538-4365/ab5e7c. Bibcode: 2020ApJS..246...11F.
11. ↑ Feng, Fabo; Butler, R. Paul; Shectman, Stephen A.; Crane, Jeffrey D.; Vogt, Steve; Chambers, John; Jones, Hugh R. A.; Wang, Sharon Xuesong et al. (2020-01-08). "Search for Nearby Earth Analogs. II. Detection of Five New Planets, Eight Planet Candidates, and Confirmation of Three Planets around Nine Nearby M Dwarfs". The Astrophysical Journal Supplement Series 246 (1): 11. doi:10.3847/1538-4365/ab5e7c. ISSN 1538-4365. Bibcode: 2020ApJS..246...11F.
12. ↑ 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. doi:10.1088/0004-637X/789/2/114. Bibcode: 2014ApJ...789..114B.
13. ↑ Wittenmyer, R. A. (August 2014). "GJ 832c: A super-earth in the habitable zone". The Astrophysical Journal 791 (2): 114. doi:10.1088/0004-637X/791/2/114. 114. Bibcode: 2014ApJ...791..114W.
14. ↑ Gorrini, P.; Astudillo-Defru, N.; Dreizler, S.; Damasso, M.; Díaz, R. F.; Bonfils, X.; Jeffers, S. V.; Barnes, J. R. et al. (2022), "Detailed stellar activity analysis and modelling of GJ 832", Astronomy & Astrophysics 664: A64, doi:10.1051/0004-6361/202243063
15. ↑ 15.0 15.1 15.2 Astudillo-Defru, Nicola; Bonfils, Xavier; Delfosse, Xavier; Ségransan, Damien; Forveille, Thierry; Bouchy, François; Gillon, Michaël; Lovis, Christophe et al. (2015). "Planetary systems and stellar activity of the M dwarfs GJ 3293, GJ 3341, and GJ 3543". Astronomy & Astrophysics 575: A119. doi:10.1051/0004-6361/201424253. Bibcode: 2015A&A...575A.119A.
16. ↑ Marie-Eve Naud; Étienne Artigau; Lison Malo; Loïc Albert; René Doyon; David Lafrenière; Jonathan Gagné; Didier Saumon et al. (12 May 2014). "Discovery of a Wide Planetary-mass Companion to the Young M3 Star GU Psc". The Astrophysical Journal 787 (1): 16. May 2014. doi:10.1088/0004-637X/787/1/5. 5. Bibcode: 2014ApJ...787....5N.
17. ↑ Bieryla, A.; Hartman, J. D.; Bakos, G. Á.; Bhatti, W.; Kovács, G.; Boisse, I.; Latham, D. W.; Buchhave, L. A. et al. (2014), "HAT-P-49b: A 1.7MJPLANET TRANSITING a BRIGHT 1.5M☉F-STAR", The Astronomical Journal 147 (4): 84, doi:10.1088/0004-6256/147/4/84, Bibcode: 2014AJ....147...84B
18. ↑ Bakos, G. Á.; Hartman, J. D.; Bhatti, W.; Bieryla, A.; Val-Borro, M. de; Latham, D. W.; Buchhave, L. A.; Csubry, Z. et al. (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, doi:10.1088/0004-6256/149/4/149
19. ↑ 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, doi:10.3847/0067-0049/226/1/7
20. ↑ 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, doi:10.3847/1538-3881/ac01dd, Bibcode: 2021AJ....162...18S
21. ↑ Jordán, Andrés et al. (2014), "HATS-4b: A DENSE HOT JUPITER TRANSITING a SUPER METAL-RICH G STAR", The Astronomical Journal 148 (2): 29, doi:10.1088/0004-6256/148/2/29, Bibcode: 2014AJ....148...29J
22. ↑ Zhou, G.; Bayliss, D.; Penev, K.; Bakos, G. Á.; Hartman, J. D.; Jordán, A.; Mancini, L.; Mohler, M. et al. (2014), "HATS-5b: A TRANSITING HOT SATURN FROM THE HATSouth SURVEY", The Astronomical Journal 147 (6): 144, doi:10.1088/0004-6256/147/6/144, Bibcode: 2014AJ....147..144Z
23. ↑ Hartman, J. D.; Bayliss, D.; Brahm, R.; Bakos, G. Á.; Mancini, L.; Jordán, A.; Penev, K.; Rabus, M. et al. (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, doi:10.1088/0004-6256/149/5/166
24. ↑ Kane, Stephen R. et al. (April 2014). "Limits on Stellar Companions to Exoplanet Host Stars with Eccentric Planets". The Astrophysical Journal 785 (2): 10. doi:10.1088/0004-637X/785/2/93. 93. Bibcode: 2014ApJ...785...93K.
25. ↑ 25.0 25.1 25.2 25.3 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. doi:10.1088/0004-637X/799/1/89. Bibcode: 2015ApJ...799...89G.
26. ↑ Wang, Liang; Sato, Bun'ei; Omiya, Masashi; Harakawa, Hiroki; Liu, Yujuan; Song, Nan; He, Wei; Wu, Xiaoshu et al. (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, doi:10.1093/pasj/psu113
27. ↑ Acke, B.; van den Ancker, M. E. (16 March 2006). "Resolving the disk rotation of HD 97048 and HD 100546 in the [O I] 6300 Å line: evidence for a giant planet orbiting HD 100546". Astronomy & Astrophysics 449 (1): 267–279. doi:10.1051/0004-6361:20054330. Bibcode: 2006A&A...449..267A.
28. ↑ 28.0 28.1 Wittenmyer, Robert A. et al. (2014). "The Anglo-Australian Planet Search. XXIII. Two New Jupiter Analogs". The Astrophysical Journal 783 (2): 103. doi:10.1088/0004-637X/783/2/103. Bibcode: 2014ApJ...783..103W.
29. ↑ 29.0 29.1 29.2 29.3 Vogt, Steven S.; Butler, R. Paul; Rivera, Eugenio J.; Kibrick, Robert; Burt, Jennifer; Hanson, Russell; Meschiari, Stefano; Henry, Gregory W. et al. (2014), "A Four-Planet System Orbiting the K0V Star Hd 141399", The Astrophysical Journal 787 (2): 97, doi:10.1088/0004-637X/787/2/97, Bibcode: 2014ApJ...787...97V
30. ↑ 30.0 30.1 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, doi:10.1051/0004-6361/201424771, Bibcode: 2015A&A...573A...3J
31. ↑ 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, doi:10.1088/0004-637X/800/1/74
32. ↑ 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, doi:10.1051/0004-6361/201323345, Bibcode: 2014A&A...566A.113J
33. ↑ 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. doi:10.1088/0004-637X/800/1/59. Bibcode: 2015ApJ...800...59V.
34. ↑ Cite error: Invalid `<ref>` tag; no text was provided for refs named `Guillem2014`
35. ↑ Cite error: Invalid `<ref>` tag; no text was provided for refs named `Bortle2021`
36. ↑ 36.0 36.1 36.2 Silvotti, R.; Charpinet, S.; Green, E.; Fontaine, G.; Telting, J. H.; Østensen, R. H.; Van Grootel, V.; Baran, A. S. et al. (2014), "Keplerdetection of a new extreme planetary system orbiting the subdwarf-B pulsator KIC 10001893", Astronomy & Astrophysics 570: A130, doi:10.1051/0004-6361/201424509, Bibcode: 2014A&A...570A.130S
37. ↑ 37.0 37.1 37.2 Blokesz, A. (July 2019). "Analysis of putative exoplanetary signatures found in light curves of two sdBV stars observed by Kepler". Astronomy & Astrophysics 627: A86. doi:10.1051/0004-6361/201835003. Bibcode: 2019A&A...627A..86B.
38. ↑ 38.000 38.001 38.002 38.003 38.004 38.005 38.006 38.007 38.008 38.009 38.010 38.011 38.012 38.013 38.014 38.015 38.016 38.017 38.018 38.019 38.020 38.021 38.022 38.023 38.024 38.025 38.026 38.027 38.028 38.029 38.030 38.031 38.032 38.033 38.034 38.035 38.036 38.037 38.038 38.039 38.040 38.041 38.042 38.043 38.044 38.045 38.046 38.047 38.048 38.049 38.050 38.051 38.052 38.053 38.054 38.055 38.056 38.057 38.058 38.059 38.060 38.061 38.062 38.063 38.064 38.065 38.066 38.067 38.068 38.069 38.070 38.071 38.072 38.073 38.074 38.075 38.076 38.077 38.078 38.079 38.080 38.081 38.082 38.083 38.084 38.085 38.086 38.087 38.088 38.089 38.090 38.091 38.092 38.093 38.094 38.095 38.096 38.097 38.098 38.099 38.100 38.101 38.102 38.103 38.104 38.105 38.106 38.107 38.108 38.109 38.110 38.111 38.112 38.113 38.114 38.115 38.116 38.117 38.118 38.119 38.120 38.121 38.122 38.123 38.124 38.125 38.126 38.127 38.128 38.129 38.130 38.131 38.132 38.133 38.134 38.135 38.136 38.137 38.138 38.139 38.140 38.141 38.142 38.143 38.144 38.145 38.146 38.147 38.148 38.149 38.150 38.151 38.152 38.153 38.154 38.155 38.156 38.157 38.158 38.159 38.160 38.161 38.162 38.163 38.164 38.165 38.166 38.167 38.168 38.169 38.170 38.171 38.172 38.173 38.174 38.175 38.176 38.177 38.178 38.179 38.180 38.181 38.182 38.183 38.184 38.185 38.186 38.187 38.188 38.189 38.190 38.191 38.192 38.193 38.194 38.195 38.196 38.197 38.198 38.199 38.200 38.201 38.202 38.203 38.204 38.205 38.206 38.207 38.208 38.209 38.210 38.211 38.212 38.213 38.214 38.215 38.216 38.217 38.218 38.219 38.220 38.221 38.222 38.223 38.224 38.225 38.226 38.227 38.228 38.229 38.230 38.231 38.232 38.233 38.234 38.235 38.236 38.237 38.238 38.239 38.240 38.241 38.242 38.243 38.244 38.245 38.246 38.247 38.248 38.249 38.250 38.251 38.252 38.253 38.254 38.255 38.256 38.257 38.258 38.259 38.260 38.261 38.262 38.263 38.264 38.265 38.266 38.267 38.268 38.269 38.270 38.271 38.272 38.273 38.274 38.275 38.276 38.277 38.278 38.279 38.280 38.281 38.282 38.283 38.284 38.285 38.286 38.287 38.288 38.289 38.290 38.291 38.292 38.293 38.294 38.295 38.296 38.297 38.298 38.299 38.300 38.301 38.302 38.303 38.304 38.305 38.306 38.307 38.308 38.309 38.310 38.311 38.312 38.313 38.314 38.315 38.316 38.317 38.318 38.319 38.320 38.321 38.322 38.323 38.324 38.325 38.326 38.327 38.328 38.329 38.330 38.331 38.332 38.333 38.334 38.335 38.336 38.337 38.338 38.339 38.340 38.341 38.342 38.343 38.344 38.345 38.346 38.347 38.348 38.349 38.350 38.351 38.352 38.353 38.354 38.355 38.356 38.357 38.358 38.359 38.360 38.361 38.362 38.363 38.364 38.365 38.366 38.367 38.368 38.369 38.370 38.371 38.372 38.373 38.374 38.375 38.376 38.377 38.378 38.379 38.380 38.381 38.382 38.383 38.384 38.385 38.386 38.387 38.388 38.389 38.390 38.391 38.392 38.393 38.394 38.395 38.396 38.397 38.398 38.399 38.400 38.401 38.402 38.403 38.404 38.405 38.406 38.407 38.408 38.409 38.410 38.411 38.412 38.413 38.414 38.415 38.416 38.417 38.418 38.419 38.420 38.421 38.422 38.423 38.424 38.425 38.426 38.427 38.428 38.429 38.430 38.431 38.432 38.433 38.434 38.435 38.436 38.437 38.438 38.439 38.440 38.441 38.442 38.443 38.444 38.445 38.446 38.447 38.448 38.449 38.450 38.451 38.452 38.453 38.454 38.455 38.456 38.457 38.458 38.459 38.460 38.461 38.462 38.463 38.464 38.465 38.466 38.467 38.468 38.469 38.470 38.471 38.472 38.473 38.474 38.475 38.476 38.477 38.478 38.479 38.480 38.481 38.482 38.483 38.484 38.485 38.486 38.487 38.488 38.489 38.490 38.491 38.492 38.493 38.494 38.495 38.496 38.497 38.498 38.499 38.500 38.501 38.502 38.503 38.504 38.505 38.506 38.507 38.508 38.509 38.510 38.511 38.512 38.513 38.514 38.515 38.516 38.517 38.518 38.519 38.520 38.521 38.522 38.523 38.524 38.525 38.526 38.527 38.528 38.529 38.530 38.531 38.532 38.533 38.534 38.535 38.536 38.537 38.538 38.539 38.540 38.541 38.542 38.543 38.544 38.545 38.546 38.547 38.548 38.549 38.550 38.551 38.552 38.553 38.554 38.555 38.556 38.557 38.558 38.559 38.560 38.561 38.562 38.563 38.564 38.565 38.566 38.567 38.568 38.569 38.570 38.571 38.572 38.573 38.574 38.575 38.576 38.577 38.578 38.579 38.580 38.581 38.582 38.583 38.584 38.585 38.586 38.587 38.588 38.589 38.590 38.591 38.592 38.593 38.594 38.595 38.596 38.597 38.598 38.599 38.600 38.601 38.602 38.603 38.604 38.605 38.606 38.607 38.608 38.609 38.610 38.611 38.612 38.613 38.614 38.615 38.616 38.617 38.618 38.619 38.620 38.621 38.622 38.623 38.624 38.625 38.626 38.627 38.628 38.629 38.630 38.631 38.632 38.633 38.634 38.635 38.636 38.637 38.638 38.639 38.640 38.641 38.642 38.643 38.644 38.645 38.646 38.647 38.648 38.649 38.650 38.651 38.652 38.653 38.654 38.655 38.656 38.657 38.658 38.659 38.660 38.661 38.662 38.663 38.664 38.665 38.666 38.667 38.668 38.669 38.670 38.671 38.672 38.673 38.674 38.675 38.676 38.677 38.678 38.679 38.680 38.681 38.682 38.683 38.684 38.685 38.686 38.687 38.688 38.689 38.690 38.691 38.692 38.693 38.694 38.695 38.696 38.697 38.698 38.699 38.700 38.701 38.702 38.703 38.704 38.705 38.706 38.707 38.708 38.709 38.710 38.711 38.712 38.713 38.714 38.715 38.716 38.717 38.718 38.719 38.720 38.721 38.722 38.723 38.724 38.725 38.726 38.727 38.728 38.729 38.730 38.731 38.732 38.733 38.734 38.735 Rowe, Jason F.; Bryson, Stephen T.; Marcy, Geoffrey W.; Lissauer, Jack J.; Jontof-Hutter, Daniel; Mullally, Fergal; Gilliland, Ronald L.; Issacson, Howard et al. (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, doi:10.1088/0004-637X/784/1/45, Bibcode: 2014ApJ...784...45R
39. ↑ 39.00 39.01 39.02 39.03 39.04 39.05 39.06 39.07 39.08 39.09 39.10 39.11 39.12 39.13 39.14 39.15 39.16 39.17 39.18 39.19 39.20 39.21 39.22 39.23 39.24 39.25 39.26 39.27 39.28 39.29 39.30 39.31 39.32 39.33 39.34 39.35 39.36 39.37 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, doi:10.1088/0067-0049/210/2/20, Bibcode: 2014ApJS..210...20M
40. ↑ 40.0 40.1 Heller, René; Hippke, Michael; Freudenthal, Jantje; Rodenbeck, Kai; Batalha, Natalie M.; Bryson, Steve (2020). "Transit least-squares survey". Astronomy & Astrophysics 638: A10. doi:10.1051/0004-6361/201936929.
41. ↑ Campante, T. L.; Lund, M. N.; Kuszlewicz, J. S.; Davies, G. R.; Chaplin, W. J.; Albrecht, S.; Winn, J. N.; Bedding, T. R. et al. (2016), "Spin–Orbit Alignment of Exoplanet Systems: Ensemble Analysis Using Asteroseismology", The Astrophysical Journal 819 (1): 85, doi:10.3847/0004-637X/819/1/85, Bibcode: 2016ApJ...819...85C
42. ↑ "SOPHIE velocimetry of Kepler transit candidates XI. Kepler-412 system: probing the properties of a new inflated hot Jupiter". https://www.aanda.org/articles/aa/pdf/2014/04/aa23017-13.pdf.
43. ↑ Kostov, V. B.; McCullough, P. R.; Carter, J. A.; Deleuil, M.; Díaz, R. F.; Fabrycky, D. C.; Hébrard, G.; Hinse, T. C. et al. (2014), "Kepler-413B: A Slightly Misaligned, Neptune-Size Transiting Circumbinary Planet", The Astrophysical Journal 784 (1): 14, doi:10.1088/0004-637X/784/1/14, Bibcode: 2014ApJ...784...14K
44. ↑ 44.0 44.1 44.2 44.3 44.4 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. doi:10.1088/0004-637X/787/1/80. Bibcode: 2014ApJ...787...80H.
45. ↑ Tingley, B.; Parviainen, H.; Gandolfi, D.; Deeg, H. J.; Palle, E.; Montañés Rodriguez, P.; Murgas, F.; Alonso, R. et al. (2014), "Confirmation of an exoplanet using the transit color signature: Kepler-418b, a blended giant planet in a multiplanet system", Astronomy & Astrophysics 567: A14, doi:10.1051/0004-6361/201323175, Bibcode: 2014A&A...567A..14T
46. ↑ 46.0 46.1 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. et al. (2014), "Large Eccentricity, Low Mutual Inclination: The Three-Dimensional Architecture of a Hierarchical System of Giant Planets", The Astrophysical Journal 791 (2): 89, doi:10.1088/0004-637X/791/2/89, Bibcode: 2014ApJ...791...89D
47. ↑ Santerne, A. et al. (2014), "SOPHIE velocimetry of Keplertransit candidates", Astronomy & Astrophysics 571: A37, doi:10.1051/0004-6361/201424158
48. ↑ Kipping, D. M.; Torres, G.; Buchhave, L. A.; Kenyon, S. J.; Henze, C.; Isaacson, H.; Kolbl, R.; Marcy, G. W. et al. (2014), "Discovery of a Transiting Planet Near the Snow-Line", The Astrophysical Journal 795 (1): 25, doi:10.1088/0004-637X/795/1/25, Bibcode: 2014ApJ...795...25K
49. ↑ 49.0 49.1 49.2 49.3 Endl, Michael; Caldwell, Douglas A.; Barclay, Thomas; Huber, Daniel; Isaacson, Howard; Buchhave, Lars A.; Brugamyer, Erik; Robertson, Paul et al. (2014), "KEPLER-424 b: A "LONELY" HOT JUPITER THAT FOUND a COMPANION", The Astrophysical Journal 795 (2): 151, doi:10.1088/0004-637X/795/2/151, Bibcode: 2014ApJ...795..151E
50. ↑ 50.0 50.1 50.2 50.3 Hébrard, G.; Santerne, A.; Montagnier, G.; Bruno, G.; Deleuil, M.; Havel, M.; Almenara, J.-M.; Damiani, C. et al. (2014), "Characterization of the four new transiting planets KOI-188b, KOI-195b, KOI-192b, and KOI-830b", Astronomy & Astrophysics 572: A93, doi:10.1051/0004-6361/201424268, Bibcode: 2014A&A...572A..93H
51. ↑ 51.0 51.1 51.2 51.3 51.4 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, doi:10.1088/0004-6256/149/2/55
52. ↑ 52.0 52.1 Quinn, Samuel N.; White, Timothy R.; Latham, David W.; Chaplin, William J.; Handberg, Rasmus; Huber, Daniel; Kipping, David M.; Payne, Matthew J. et al. (2014). "Kepler-432: A red giant interacting with one of its two long period giant planets". The Astrophysical Journal 803 (2): 49. doi:10.1088/0004-637X/803/2/49. Bibcode: 2015ApJ...803...49Q.
53. ↑ Welsh, William F. et al. (2015). "KIC 9632895 - The 10th Kepler Transiting Circumbinary Planet". The Astrophysical Journal 809 (1): 26. doi:10.1088/0004-637X/809/1/26. Bibcode: 2015ApJ...809...26W.
54. ↑ Koshimoto, N. et al. (2014), "OGLE-2008-BLG-355Lb: A MASSIVE PLANET AROUND a LATE-TYPE STAR", The Astrophysical Journal 788 (2): 128, doi:10.1088/0004-637X/788/2/128, Bibcode: 2014ApJ...788..128K
55. ↑ Poleski, Radosław; Skowron, Jan; Udalski, Andrzej; Han, Cheongho; Kozłowski, Szymon; Wyrzykowski, Łukasz; Dong, Subo; Szymański, Michał K. et al. (2014), "Triple Microlens Ogle-2008-BLG-092L: Binary Stellar System with a Circumprimary Uranus-Type Planet", The Astrophysical Journal 795 (1): 42, doi:10.1088/0004-637X/795/1/42, Bibcode: 2014ApJ...795...42P
56. ↑ Skowron, J. et al. (2014), "OGLE-2011-BLG-0265Lb: A JOVIAN MICROLENSING PLANET ORBITING AN M DWARF", The Astrophysical Journal 804: 33, doi:10.1088/0004-637X/804/1/33
57. ↑ 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, doi:10.1088/0004-637X/798/2/123
58. ↑ 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, doi:10.1126/science.1251527, PMID 24994642, Bibcode: 2014Sci...345...46G
59. ↑ Udalski, A.; Yee, J. C.; Gould, A.; Carey, S.; Zhu, W.; Skowron, J.; Kozłowski, S.; Poleski, R. et al. (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, doi:10.1088/0004-637X/799/2/237
60. ↑ 60.0 60.1 60.2 Brucalassi, A.; Pasquini, L.; Saglia, R.; Ruiz, M. T.; Bonifacio, P.; Bedin, L. R.; Biazzo, K.; Melo, C. et al. (2014), "Three planetary companions around M 67 stars", Astronomy & Astrophysics 561: L9, doi:10.1051/0004-6361/201322584, Bibcode: 2014A&A...561L...9B
61. ↑ 61.0 61.1 Niedzielski, A.; Villaver, E.; Wolszczan, A.; Adamów, M.; Kowalik, K.; MacIejewski, G.; Nowak, G.; García-Hernández, D. A. et al. (2014), "Tracking Advanced Planetary Systems (TAPAS) with HARPS-N", Astronomy & Astrophysics 573: A36, doi:10.1051/0004-6361/201424399
62. ↑ Anderson, D. R.; Collier Cameron, A.; Hellier, C.; Lendl, M.; Lister, T. A.; Maxted, P. F. L.; Queloz, D.; Smalley, B. et al. (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. doi:10.1051/0004-6361/201423591. Bibcode: 2015A&A...575A..61A.
63. ↑ 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. doi:10.3847/2041-8213/833/2/L19. Bibcode: 2016ApJ...833L..19E.
64. ↑ 64.0 64.1 64.2 Hellier, Coel; Anderson, D. R.; Collier Cameron, A.; Delrez, L.; Gillon, M.; Jehin, E.; Lendl, M.; Maxted, P. F. L. et al. (2014), "Three WASP-South transiting exoplanets: WASP-74b, WASP-83b & WASP-89b", The Astronomical Journal 150 (1): 18, doi:10.1088/0004-6256/150/1/18, Bibcode: 2015AJ....150...18H
65. ↑ 65.0 65.1 65.2 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
66. ↑ 66.0 66.1 66.2 66.3 66.4 66.5 Anderson, D. R.; Brown, D. J. A.; Collier Cameron, A.; Delrez, L.; Fumel, A.; Gillon, M.; Hellier, C.; Jehin, E. et al. (2014), Six newly-discovered hot Jupiters transiting F/G stars: WASP-87b, WASP-108b, WASP-109b, WASP-110b, WASP-111b & WASP-112b
67. ↑ 67.0 67.1 Neveu-Vanmalle, M.; Queloz, D.; Anderson, D. R.; Charbonnel, C.; Collier Cameron, A.; Delrez, L.; Gillon, M.; Hellier, C. et al. (2014), "WASP-94 a and B planets: Hot-Jupiter cousins in a twin-star system", Astronomy & Astrophysics 572: A49, doi:10.1051/0004-6361/201424744, Bibcode: 2014A&A...572A..49N
68. ↑ Gillon, M.; Anderson, D. R.; Collier-Cameron, A.; Delrez, L.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L. et al. (2014), "WASP-103 b: A new planet at the edge of tidal disruption", Astronomy & Astrophysics 562: L3, doi:10.1051/0004-6361/201323014, Bibcode: 2014A&A...562L...3G
69. ↑ Southworth, John; Mancini, L.; Ciceri, S.; Budaj, J.; Dominik, M.; Figuera Jaimes, R.; Haugbølle, T.; Jørgensen, U. G. et al. (2014), "High-precision photometry by telescope defocusing – VII. The ultrashort period planet WASP-103★", Monthly Notices of the Royal Astronomical Society 447: 711–721, doi:10.1093/mnras/stu2394
70. ↑ 70.0 70.1 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. doi:10.1051/0004-6361/201424752. Bibcode: 2014A&A...570A..64S. https://www.aanda.org/articles/aa/full_html/2014/10/aa24752-14/aa24752-14.html.
71. ↑ Lendl, M.; Triaud, A. H. M. J.; Anderson, D. R.; Collier Cameron, A.; Delrez, L.; Doyle, A. P.; Gillon, M.; Hellier, C. et al. (2014). "WASP-117b: A 10-day-period Saturn in an eccentric and misaligned orbit". Astronomy & Astrophysics 568: A81. doi:10.1051/0004-6361/201424481. Bibcode: 2014A&A...568A..81L.
72. ↑ Carone, Ludmila; Mollière, Paul; Zhou, Yifan; Bouwman, Jeroen; Yan, Fei; Baeyens, Robin; Apai, Dániel; Espinoza, Nestor et al. (2021). "Indications for very high metallicity and absence of methane in the eccentric exo-Saturn WASP-117b". Astronomy & Astrophysics 646: A168. doi:10.1051/0004-6361/202038620. Bibcode: 2021A&A...646A.168C.
73. ↑ 73.0 73.1 Desidera, S. et al. (2014), "The GAPS programme with HARPS-N at TNG", Astronomy & Astrophysics 567: L6, doi:10.1051/0004-6361/201424339

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