List of exoplanets discovered in 2019
Appearance
This list of exoplanets discovered in 2019 is a list of confirmed exoplanets that were first observed during 2019.[1][2]
For exoplanets detected only by radial velocity, the listed value for mass is a lower limit. See Minimum mass for more information.
Name | Mass (MJ) | Radius (RJ) | Period (days) | Semi-major axis (AU) | Temp. (K)[3] | Discovery method | Distance (ly) | Host star mass (M☉) | Host star temp. (K) | Remarks |
---|---|---|---|---|---|---|---|---|---|---|
7 Canis Majoris c | 0.87 | 996.00 | 2.153 | radial vel. | 64.6 | 1.34 | 4826 | [4] | ||
Beta Pictoris c | 9 | 1200 | 2.7 | radial vel. | 64.43 | 1.76 | [5] | |||
DS Tucanae Ab | 0.509±0.015 | 8.138268±0.000011 | 850 | transit | 143.89±0.22 | 1.01±0.06 | 5428±80 | [6] | ||
Epsilon Indi Ab | 3.25 | 16510 | 11.55 | 64.25 | radial vel. | 11.87 | 0.75 | [7] | ||
G 9-40 b | 0.1807 | 5.746007 | 0.0385 | 456 | transit | 91.1 | 0.290 | 3348 | [8][9] | |
Gliese 49 b | 0.0177+0.0021 −0.0021 |
13.8508+0.0053 −0.0051 |
0.0905±0.0011 | radial vel. | 32.145±0.01 | 0.515±0.019 | 3805±51 | [10] | ||
Gliese 357 b | 0.00579 | 0.1086 | 3.93072 | 0.035 | 525 | transit | 30.80 | 0.342 | 3505 | [11] |
Gliese 357 c | 0.0107 | 9.1247 | 0.061 | 401.2 | radial vel. | 30.80 | 0.342 | 3505 | [11] | |
Gliese 357 d | 0.019 | 55.661 | 0.204 | 219.6 | radial vel. | 30.80 | 0.342 | 3505 | Potentially habitable exoplanet[11] | |
Gliese 378 b | 0.04097±0.006 | 3.822±0.001 | 0.082±0.002 | radial vel. | 48.79 | 0.56±0.01 | 3879±67 | [12] | ||
Gliese 411 b | 0.00941±0.00145 | 12.9532±0.0079 | 349.83±0.32 | radial vel. | 8.284 | 0.386±0.039 | 3563±60 | [13]Host star also known as Lalande 21185 | ||
Gliese 685 b | 0.028+0.0053 −0.0057 |
24.160+0.061 −0.047 |
0.1344+0.0052 −0.0051 |
radial vel. | 46.7102 | 0.3816±0.069 | 0.55±0.06 | [14] | ||
Gliese 686 b | 0.022±0.003 | 15.53209+0.00166 −0.00167 |
0.091±0.004 | 379+24 −25 |
radial vel. | 26.612±0.008 | 0.42±0.05 | 3663±68 | [15] | |
Gliese 3512 b | 0.463 | 203.59 | 0.3380 | radial vel. | 30.95 | 0.123 | 3081 | [16] | ||
Gliese 4276 b | 0.05213+0.00296 −0.00299 |
13.352±0.003 | 0.082±0.002 | radial vel. | 69.6±0.1 | 0.41±0.03 | 3387±51 | May be two planwts in 2:1 orbital resonance[17] | ||
HAT-P-69b | 3.58 | 1.676 | 4.7869491 | 0.06555 | 1930 | transit | 1122 | 1.65 | 7394 | [18] |
HAT-P-70b | <6.78 | 1.87 | 2.74432452 | 0.04739 | 4000 | transit | 1073 | 1.89 | 8450 | [18][19] |
HD 8326 b | 0.210±0.062 | 158.991±1.440 | 0.533±0.011 | radial vel. | 100.2 | 0.80±0.05 | 4914+51 −32 |
[20] | ||
HD 13724 b | 26.77+4.40 −2.20 |
14763.405+4901.655 −1599.795 |
12.40+2.60 −0.90 |
radial vel. | 141.9±0.17 | 0.76±0.71 | 5868±27 | [21] | ||
HD 15337 b | 0.0236+0.0034 −0.0032 |
0.146±0.005 | 4.75615±0.00017 | 0.0522±0.0012 | 1001.0±11.5 | transit | 146.36±0.23 | 0.90±0.03 | 5125±50 | Host star also known as TOI-402[22] |
HD 15337 c | 0.0255+0.0057 −0.0053 |
0.213±0.011 | 17.1784±0.0016 | 0.1268±0.0038 | 642±10 | transit | 146.36±0.23 | 0.90±0.03 | 5125±50 | Host star also known as TOI-402[22] |
HD 21411 b | 0.207±0.081 | 84.288±0.127 | 0.362±0.007 | radial vel. | ±95.11 | 0.89±0.05 | 5605+247 −132 |
[20] | ||
HD 21749 b | 0.073+0.007 −0.006 |
0.254+0.023 −0.020 |
35.61253+0.00060 −0.00062 |
0.1915+0.0058 −0.0063 |
422+15 −14 |
transit | 53.261±0.023 | 0.73±0.07 | 4640±100 | [23] |
HD 21749 c | <0.0116 | 0.0796+0.0057 −0.0052 |
7.78993+0.00051 −0.00044 |
0.0695+0.0021 −0.0023 |
701+25 −23 |
transit | 53.261±0.023 | 0.73±0.07 | 4640±100 | [23] |
HD 24085 b | 0.0371±0.0098 | 2.0455±0.0002 | 0.034±0.001 | radial vel. | 179.4 | 1.22±0.07 | 6034+32 −53 |
[20] | ||
HD 25015 b | 4.48+0.30 −0.28 |
6019.320+679.365 −262.980 |
6.19+0.45 −0.23 |
radial vel. | 122.2±0.22 | 0.86±0.05 | 5160±63 | [21] | ||
HD 39855 b | 0.027±0.005 | 3.2498±0.0004 | 0.041±0.001 | radial vel. | 75.93 | 0.87±0.05 | 5576+50 −46 |
[20] | ||
HD 64114 b | 0.0560±0.0110 | 45.791±0.070 | 0.246±0.005 | radial vel. | 102.9 | 0.95±0.05 | 5676+32 −87 |
[20] | ||
HD 65216c | 1.295±0.062 | 577.6±1.328 | 1.301±0.020 | radial vel. | 114.7±0.1 | 0.95±0.01 | 5718±8 | Rediscovered in 2019 after false positive in 2013[24] | ||
HD 85628 A b | 1.675±0.241 | 1.515±0.044 | 2.8240932±0.0000046 | 0.0474±0.0013 | 1865±25 | transit | 560±3 | 1.75±0.05 | 7800±200 | Host star also known as MASCARA-4[25][26][27] |
HD 92788 c | 3.67+0.30 −0.25 |
11611.2975+5055.06 −905.820 |
10.50+2.90 −0.55 |
radial vel. | 113.1385 | 1.15±0.07 | 5744±24 | [28] | ||
HD 92987 b | 16.88+0.69 −0.65 |
10354.8375+551.5275 −270.2850 |
9.62+0.36 −0.26 |
radial vel. | 142.2±0.22 | 1.08±0.06 | 5770±36 | [21][29] | ||
HD 97048 b | 2.5 | 130 | imaging | 603 | 2.4 | 10000 | Discovered using study of disk kinematics.[30] Unconfirmed. | |||
HD 102843 b | 0.3584±0.0456 | 3090.942±295.049 | 4.074±0.270 | radial vel. | 205.05 | 0.95±0.05 | 5436+144 −69 |
[20] | ||
HD 103949 b | 0.0352±0.0072 | 120.878±0.446 | 0.439±0.009 | radial vel. | 86.50 | 0.77±0.04 | 4792+66 −54 |
[20] | ||
HD 181234 b | 8.37+0.34 −0.36 |
7462.0575+80.3550 −76.7025 |
12.40+2.60 −0.90 |
radial vel. | 155.9±0.42 | 1.01±0.06 | 5386±60 | [21] | ||
HD 202696 b | 1.996+0.220 −0.100 |
517.8+8.9 −3.9 |
1.566+0.016 −0.007 |
radial vel. | 618.3±5.2 | 1.91+0.09 −0.14 |
5040+71 −85 |
[31] | ||
HD 202696 c | 1.864+0.177 −0.227 |
946.6+20.7 −20.9 |
2.342+0.034 −0.035 |
radial vel. | 618.3±5.2 | 1.91+0.09 −0.14 |
5040+71 −85 |
[31] | ||
HD 206255 b | 0.108±0.022 | 96.045±0.317 | 0.461±0.009 | radial vel. | 245.9 | 1.42±0.08 | 5635+82 −99 |
[20] | ||
HD 210193 b | 0.4817±0.0733 | 649.918±8.599 | 1.487±0.031 | radial vel. | 137.8 | 1.04±0.06 | 5790+38 −50 |
[20] | ||
HD 211970 b | 0.0409±0.0079 | 25.201±0.025 | 0.143±0.003 | radial vel. | 42.4 | 0.61±0.04 | 4127+149 −94 |
[20] | ||
HD 213885 b | 0.0278+0.0021 −0.0020 |
0.1557+0.0045 −0.0046 |
1.008035+0.000021 −0.000020 |
0.02012+0.00015 −0.00012 |
transit | 156.45721±0.4566189 | 1.068+0.020 −0.018 |
5978±50 | A transiting 1-day-period super-Earth with an Earth-like composition around a bright (V=7.9) star unveiled by TESS[32] | |
HD 213885 c | 0.06277+0.00434 −0.00428 |
4.78503+0.00056 −0.000051 |
0.056798+0.00044 −0.00032 |
1265.4+7.3 −8.4 |
radial vel. | 156.45721±0.4566189 | 1.068+0.020 −0.018 |
5978±50 | [32] | |
HD 221416 b | 0.190±0.018 | 0.836+0.031 −0.028 |
14.2767±0.0037 | 0.1228+0.00025 −0.00026 |
transit | 310.0931 | 1.212±0.074 | 5080±90 | Host star also known as TOI-197 or HIP 116158[33] | |
HD 221420 b | 9.70+1.10 −1.00 |
22482+4200 −4100 |
18.5±2.3 | radial vel. | 101.7±0.12 | 1.67±0.11 | 5830±44 | [29] | ||
HIP 35173 b | 0.0400±0.0085 | 41.516±0.077 | 0.217±0.004 | radial vel. | 108.25 | 0.79±0.05 | 4881+55 −81 |
[20] | ||
HIP 54373 b | 0.02712±0.00579 | 7.760±0.003 | 0.063±0.001 | radial vel. | 61.09 | 0.57±0.03 | 4021+226 −146 |
[20] | ||
HIP 54373 c | 0.03914±0.00664 | 15.144±0.008 | 0.0990±0.0020 | radial vel. | 61.09 | 0.57±0.03 | 4021+226 −146 |
[20] | ||
HIP 71135 b | 0.0592±0.0129 | 87.190±0.381 | 0.335±0.007 | radial vel. | 105.5 | 0.66±0.04 | 4146+107 −110 |
[20] | ||
HIP 79098 (AB)b | 20.5±4.5 | 345±6 | 2450±150 | imaging | 477.2±8.2 | 3.75±1.25 | Brown dwarf[34] | |||
HR 858 b | 0.1860+0.0061 −0.0057 |
3.58599±0.00015 | 0.0480+0.0010 −0.0011 |
1572+22 −19 |
transit | 104.35 | 1.145+0.074 −0.080 |
6201±50 | [35] | |
HR 858 c | 0.1730±0.0062 | 5.97293+0.00060 −0.00053 |
0.0674+0.0014 −0.0016 |
1326+18 −16 |
transit | 104.35 | 1.145+0.074 −0.080 |
6201±50 | [35] | |
HR 858 d | 0.1931+0.0077 −0.0074 |
11.2300+0.0011 −0.0010 |
0.1027+0.0022 −0.0025 |
1075+15 −13 |
transit | 104.35 | 1.145+0.074 −0.080 |
6201±50 | [35] | |
HR 5183 b | 3.23 | 27000 | 18 | 171 | radial vel. | 102.7 | 1.07 | 5794 | Exoplanet found with one of the most elliptical orbits as of 2019[36] | |
K2-32e | 0.0901+0.0089 −0.008 |
4.34882+0.00069 −0.00075 |
0.04951±0.00055 | transit | 516.6±4.2 | 0.856±0.028 | With a radius almost identical to that of the Earth it is almost certainly a terrestrial planet[37] | |||
K2-43c | 0.216 | 2.198884 | 1093.7 | transit | 598 | 0.57 | 3841 | [38] | ||
K2-50c | 0.089+0.011 −0.01 |
3.96151+0.00046 −0.00051 |
transit | 845.82±10.63 | 0.61±0.06 | [39] | ||||
K2-63c | 0.35±0.11 | 25.4556±0.0047 | 0.189±0.011 | transit | 524.414±21 | 1.40±0.25 | 6771±303 | |||
K2-133e | 0.154+0.012 −0.012 |
26.5841+0.0018 −0.0017 |
0.1346±0.0011 | 296±10 | transit | 245.3±0.7 | 0.46±0.01 | 3655±80 | [40]Host star also known as LP 358-499 | |
K2-146c | 0.02358 | 0.195 | 4.00498 | 1093.7 | transit | 259 | 0.33 | 3385 | [41] | |
K2-166c | 0.109+0.019 −0.015 |
3.80464+0.00091 −0.00105 |
transit | 1568.81+31.64 −29.03 |
1.07±0.03 | [39] | ||||
K2-168c | 0.105+0.012 −0.009 |
8.0468+0.0024 −0.0025 |
transit | 800.91±13.67 | 0.91±0.03 | [38][39] | ||||
K2-198c | 0.1270 | 3.3596055 | 1229.9 | transit | 362 | 0.80 | 5213 | [38] | ||
K2-198d | 0.2175 | 7.4500177 | 943.2 | transit | 362 | 0.80 | 5213 | [38] | ||
K2-282c | 0.132+0.012 −0.009 |
0.70531±0.00005 | transit | 1638.22±25.34 | 0.94±0.04 | 5499±109 | [39]3rd planet discovered in 2020[42] | |||
K2-286b | 0.0214±0.0135 | 0.1873±0.0178 | 27.359±0.005 | 0.1768+0.0175 −0.0205 |
347+21 −11 |
transit | 248.9±0.8 | 0.64±0.02 | 3926±100 | [43] |
K2-288Bb | 0.17±0.03 | 31.393463+0.000067 −0.000069 |
0.164±0.030 | 226.36±22.30 | transit | 214.3±2.8 | 0.33±0.02 | 3341±276 | [44] | |
K2-290b | 0.0664 | 0.273±0.014 | 9.21165+0.00033 −0.00034 |
0.0923±0.0066 | 1230±38 | transit | 897±12 | 1.19+0.07 −0.08 |
6302±120 | [45] Two planets on a retrograde orbit[46] |
K2-290c | 0.774±0.047 | 1.006±0.050 | 48.36685+0.00041 −0.00040 |
0.0923±0.0066 | 676±16 | transit | 897±12 | 1.19+0.07 −0.08 |
6302±120 | [45] Two planets on a retrograde orbit[46] |
K2-291b | 0.0204±0.0036 | 0.1418+0.0085 −0.0064 |
2.225177+0.000066 −0.000068 |
0.03261±0.00044 | transit | 295±2 | 0.93±0.04 | 5520±60 | [47] | |
K2-293b | 0.219+0.031 −0.022 |
13.1225+0.0011 −0.0012 |
750+170 −50 |
transit | 1290±22 | 0.96+0.04 −0.03 |
5532±78 | [48] | ||
K2-294b | 0.148+0.019 −0.017 |
2.50387+0.00022 −0.00023 |
1425+79 −54 |
transit | 1230±20 | 0.99+0.03 −0.03 |
5612±50 | [48] | ||
K2-296b | 0.167+0.018 −0.04 |
28.1656+0.0027 −0.0028 |
transit | 521.78±4.57 | 0.41+0.11 −0.05 |
|||||
K2-297b | 0.062+0.005 −0.004 |
2.13174±0.00022 | transit | 831.31±5.48 | 0.78+0.09 −0.17 |
|||||
K2-298b | 0.098+0.012 −0.011 |
4.16959+0.00051 −0.00053 |
transit | 1441.42±26.65 | 0.8+0.08 −0.16 |
|||||
K2-299b | 0.152+0.053 −0.028 |
4.50756+0.00062 −0.0006 |
transit | 1219.21±16.28 | 0.93+0.08 −0.1 |
5724±72 | Two more planets in star system discovered in 2020[42] | |||
K2-300b | 0.09+0.021 −0.012 |
2.87814+0.00023 −0.00026 |
transit | 528.67±5.87 | 0.22+0.04 −0.06 |
|||||
K2-301b | 0.145+0.015 −0.017 |
5.29711+0.00074 −0.0007 |
transit | 1491.42±44.98 | 0.56±0.05 | 4114±99 | ||||
K2-302b | 0.08+0.017 −0.018 |
2.25372±0.00047 | transit | 359.49±3.52 | 0.41+0.1 −0.08 |
Two more planets in system discovered in 2020[42] | ||||
K2-303b | 0.086+0.01 −0.013 |
1.58252+0.00017 −0.00018 |
transit | 1034.57±9.59 | 0.71+0.09 −0.03 |
|||||
K2-304b | 0.118+0.007 −0.008 |
2.28943±0.00019 | transit | 1380.78±23.94 | 0.83+0.09 −0.12 |
|||||
K2-305b | 0.194+0.06 −0.037 |
18.0983+0.006 −0.0058 |
transit | 2030.88±33.92 | 1.11+0.14 −0.12 |
|||||
K2-306b | 0.143+0.012 −0.014 |
34.885+0.011 −0.01 |
transit | 931.54±6.69 | 0.91+0.04 −0.16 |
|||||
K2-307b | 0.1+0.011 −0.008 |
15.2841+0.0037 −0.0029 |
transit | 1053.09±20.65 | 0.98+0.04 −0.03 |
6004+77 −78 |
Two more planets in system are suspected,[49] second planet in system confirmed in 2021[50] | |||
K2-308b | 0.884±0.087 | 3.38628±0.00002 | transit | 1.09±0.09 | 6100±263 | |||||
K2-310b | 0.2307±0.0112 | 13.6030±0.0013 | 0.0980±0.0040 | 536±18 | transit | 1133.22 | 0.690±0.038 | 4684±79 | ||
K2-310c | 0.2400±0.0130 | 65.5500±0.0089 | 0.280±0.006 | 316±10 | transit | 1133.22 | 0.690±0.038 | 4684±79 | ||
K2-311b | <13 | 1.11±0.07 | 3650+1280 −1130 |
4.5±1.0 | 183+25 −18 |
transit | 1826.48 | 0.90±0.09 | 4898±68 | |
KELT-23Ab | 0.938+0.048 −0.044 |
1.323±0.025 | 2.255251+0.000011 −0.000012 |
0.03302+0.00068 −0.00064 |
1561±20 | transit | 409.07±1.14 | 0.94+0.06 −0.05 |
5899±49 | [51] |
KELT-24b | 5.18 | 1.272 | 5.5514926 | 0.06969 | 1459 | transit | 313.2 | 1.46 | 6509 | |
Kepler-47d | 0.05984+0.07501 −0.03672 |
0.628+0.059 −0.044 |
187.366+0.069 −0.051 |
0.6992+0.0031 −0.0033 |
transit | 4900 | 0.957+0.013 −0.015 |
|||
Kepler-65e | 0.653+0.056 −0.055 |
258.8+1.5 −1.3 |
0.362±0.007 | radial vel. | 999.3±8.8 | 1.25±0.06 | 6211±66 | |||
Kepler-82f | 0.0658±0.0031 | 75.732±0.012 | 0.3395±0.0041 | timing | 3026.64 | 0.91±0.03 | 5401±108 | |||
Kepler-88d | 3.15±0.15 | 1409+14 −13 |
2.45±0.02 | radial vel. | 1243±7 | 1.022+0.023 −0.026 |
5513±67 | [52] | ||
Kepler-411d | 0.0478±0.0160 | 0.2961±0.0093 | 58.02035±0.00056 | 0.279±0.004 | 410±10 | transit | 500.94±1.57 | 0.87±0.04 | [53] | |
Kepler-411e | 0.0340±0.0035 | 31.509728±0.000085 | 0.186±0.003 | 503±9 | timing | 500.94±1.57 | 0.87±0.04 | [53] | ||
Kepler-448c | 22 | 2500 | 4.2 | timing | 1318 | 1.5 | ||||
Kepler-1659b | 0.028±0.001 | 0.17±0.02 | 13.608±0.00006 | 0.11229 | transit | 3812.7570 | 1.02 | |||
Kepler-1659c | 0.0014±0.001 | 0.17±0.03 | 20.4415±0.0013 | 0.1472 | transit | 3812.7570 | 1.02 | |||
Kepler-1660b | 7.693±0.054 | 237.68977±0.08237 | timing | 4013.68±73.27 | 1.21 | This detection arose from a search for eclipse timing variations among the more than 2,000 eclipsing binaries observed by Kepler. | ||||
KMT-2016-BLG-0212Lb | 18 | 2.2 | microlensing | 21000 | 0.48 | |||||
KMT-2016-BLG-1107Lb | 3.283+3.468 −1.835 |
0.342+0.070 −0.085 |
microlensing | 21700+3090 −4400 |
0.087+0.092 −0.049 |
|||||
KMT-2017-BLG-0165Lb | 0.11+0.05 −0.04 |
3.45+0.98 −0.95 |
microlensing | 14774.88 | 0.760+0.340 −0.270 |
[54][55] | ||||
KMT-2017-BLG-1038Lb | 2.0+2.0 −1.1 |
1.8+0.6 −0.5 |
microlensing | 19569.3826 | 0.37+0.36 −0.20 |
|||||
KMT-2017-BLG-1146Lb | 0.710+0.800 −0.420 |
1.6±0.6 | microlensing | 21200.16 | 0.33+0.36 −0.20 |
|||||
KMT-2018-BLG-1990Lb | 0.348 | 0.763 | microlensing | 3150 | 0.09 | |||||
LHS 3844 b | 0.1162±0.0020 | 0.46292913±0.00000190 | 0.00622±0.00017 | 805±20 | transit | 48.60±0.03 | 0.15±0.01 | 3036±77 | ||
LP 791-18 b | 0.0999 | 0.9480050 | 0.009690 | 650 | transit | 86.41 | 0.14 | 2960 | [56] | |
LP 791-18 c | 0.206 | 4.989963 | 0.029392 | 370 | transit | 86.41 | 0.14 | 2960 | [56] | |
L 98-59 b | 0.00157+0.00094 −0.00063 |
0.071±0.004 | 2.25314±0.00002 | 0.0233±0.0017 | transit | 34.64 | 0.31±0.01 | 3367±150 | [57] | |
L 98-59 c | 0.00755+0.00566 −0.00252 |
0.12+0.007 −0.006 |
3.690621+0.000013 −0.000014 |
0.0324±0.0023-0.0024 | transit | 34.64 | 0.31±0.01 | 3367±150 | [57] | |
L 98-59 d | 0.0107+0.0085 −0.0044 |
0.14±0.012 | 7.45086+0.00004 −0.00005 |
0.052±0.004 | transit | 34.64 | 0.31±0.01 | 3367±150 | [57] | |
LSPM J2116+0234 b | 0.04185+0.00315 −0.00346 |
14.4399+0.0078 −0.0087 |
0.0876+0.0022 −0.0021 |
radial vel. | 57.53±0.07 | 0.43±0.03 | 3475±51 | [58] | ||
LTT 1445 Ab | 0.0069 | 0.123 | 5.35882 | 0.03807 | 433 | transit | 22.4 | 0.26 | 3337 | [59] |
MOA-bin-29b | 0.600 | 0.48 | microlensing | 23200 | 0.03 | [60] | ||||
NGTS-5b | 0.229±0.037 | 1.136±0.023 | 3.3569866±0.0000026 | 0.0382±0.0013 | 952±24 | transit | 309.5±8.5 | 0.66+0.07 −0.06 |
4987±41 | [61] |
NGTS-6b | 1.339 | 1.326 | 0.8820590 | 0.01677 | transit | 1010 | 0.77 | 4730 | [62] | |
NGTS-8b | 0.93 | 1.09 | 2.49970 | 0.035 | 1345 | transit | 1420 | 0.89 | 5241 | [63] |
NGTS-9b | 2.90 | 1.07 | 4.43527 | 0.058 | 1448 | transit | 1420 | 1.34 | 6330 | [63] |
NSVS 14256825 b | 14.15±0.16 | 3225±22 | 3.12±0.07 | timing | 2734.2±137.31 | 0.42±0.07 | 40000 | Disputed[64] | ||
NY Virginis c | 5.54 | 8799 | timing | 1800 | Disputed[65] | |||||
OGLE-2015-BLG-1649L | 2.54 | 2.07 | microlensing | 1380 | 0.34 | [66] | ||||
OGLE-2018-BLG-0532Lb | 0.02062+0.00285 −0.00254 |
1.103+0.118 −0.107 |
microlensing | [67] | ||||||
OGLE-2018-BLG-0596Lb | 0.04383±0.00491 | 0.97±0.13 | microlensing | 18400±2400 | 0.23±0.03 | [68] | ||||
OGLE-2018-BLG-0740Lb | 4.8 | 5480 | 6.1 | microlensing | 10400 | 1.0 | 5912 | [69] | ||
OGLE-2018-BLG-1011Lb | 1.8 | 6.1 | microlensing | 23000 | 0.18 | [70] | ||||
OGLE-2018-BLG-1011Lc | 2.8 | 0.80 | microlensing | 23000 | 0.18 | [70] | ||||
PDS 70c | 8.0±4.0 | 34.5±2 | imaging | 369.96±1.7 | 0.76±0.02 | 3972±36 | [71] | |||
Qatar-8b | 0.371±0.062 | 1.285±0.022 | 3.71495±0.00100 | 0.0474±0.0008 | 1457±14 | transit | 902.5±11 | 1.03±0.05 | 5738±51 | [72] |
Qatar-9b | 1.19±0.16 | 1.009±0.014 | 1.540731±0.000038 | 0.0234±0.0003 | 1134±9 | transit | 689.5±5.2 | 0.72±0.02 | 4309±31 | [72] |
Qatar-10b | 0.736±0.090 | 1.543±0.040 | 1.645321±0.000010 | 0.0286±0.0006 | 1955±25 | transit | 1760±33 | 1.16±0.07 | 6124±46 | [72] |
SDSS J1228+1040 b | 0.0009+0.0045 −0.000758 |
0.0857±0.00021 | 0.0034±0.000009 | 1800 | timing | 413.337977±0.4892346 | 0.705±0.05 | The smallest known exoplanet discovered.[73] | ||
Teegarden b | 0.00330+0.00041 −0.00038 |
4.9100±0.0014 | 0.0252+0.0008 −0.0009 |
radial vel. | 12.50±0.013 | 0.09±0.01 | 2904±51 | [74] | ||
Teegarden c | 0.00349+0.00050 −0.00047 |
11.409±0.009 | 0.0443+0.0014 −0.0015 |
226 | radial vel. | 12.50±0.013 | 0.09±0.01 | 2904±51 | Potentially habitable exoplanet[74] | |
TOI-125 b | 0.0299±0.00277 | 0.2432±0.00669 | 4.65382±0.00033 | 0.05186+0.00086 −0.00077 |
1037±11 | transit | 363.3382±1.435088 | 0.859+0.044 −0.038 |
5320±39 | [75][76] |
TOI-125 c | 0.02086±0.00311 | 0.24614±0.009 | 9.15059+0.0007 −0.00082 |
0.814±0.0013 | 827.8±8.6 | transit | 363.3382±1.435088 | 0.859+0.044 −0.038 |
5320±39 | [77][76] |
TOI-125 d | 0.0428±0.0038 | 0.2614±0.0152 | 19.98+0.005 −0.0056 |
0.05186+0.00086 −0.00077 |
638.1±6.6 | transit | 363.3382±1.435088 | 0.859+0.044 −0.038 |
5320±39 | [78][76] |
TOI-150b | 1.75+0.14 −0.17 |
1.38±0.04 | 5.857342+0.000065 −0.000066 |
0.0583+0.0013 −0.0018 |
1493+29 −32 |
transit | 1095.89±6.52 | 1.25+0.07 −0.12 |
6003+104 −98 |
[79] |
TOI-163b | 1.22 | 1.489 | 4.231306 | 0.0580 | 1669 | transit | 1359 | 1.44 | 6495 | [79] |
TOI-172b | 5.42+0.22 −0.20 |
0.965+0.032 −0.029 |
9.47725+0.00064 −0.00079 |
0.0914±0.0017 | transit | 1097.418 | 1.128+0.065 −0.061 |
5645±50 | [80] | |
TOI-216 b | 0.059±0.002 | 0.714+0.268 −0.179 |
17.1607 | 0.1293+0.0067 −0.0051 |
628+13 −11 |
transit | 583±3 | 0.77 | 5026±125 | Semi-major axes are strongly variable due to planet-planet interaction on a timescale of few years[81][82][83] |
TOI-216 c | 0.56±0.02 | 0.902±0.018 | 34.525528 | 0.2069+0.0107 −0.0082 |
497+10 −8 |
transit | 583±3 | 0.77 | 5026±125 | Semi-major axes are strongly variable due to planet-planet interaction on a timescale of few years[81][82][83] |
TOI-270b | 0.0050 | 0.1112 | 3.360080 | 0.0306 | 528 | transit | 73.23 | 0.40 | 3386 | [84][85] |
TOI-270c | 0.0193 | 0.216 | 5.660172 | 0.0472 | 424 | transit | 73.23 | 0.40 | 3386 | [84][85] |
TOI-270d | 0.0150 | 0.190 | 11.38014 | 0.0733 | 340 | transit | 73.23 | 0.40 | 3386 | [84][85]Hydrogen and steam atmosphere[86] |
TOI-564b | 1.463+0.10 −0.096 |
1.02+0.71 −0.29 |
1.651144±0.000018 | 0.02734+0.00061 −0.00053 |
1714+20 −21 |
transit | 643.8±5.9 | 0.998+0.068 −0.057 |
5640+34 −37 |
[87] |
TOI-905b | 0.667+0.042 −0.041 |
1.171+0.052 −0.051 |
3.739494±0.000038 | 0.04666+0.00096 −0.0011 |
1192+39 −36 |
transit | 489.9+23.5 −22.5 |
0.968+0.061 −0.068 |
5570+150 −140 |
[87] |
V1298 Tauri b | 0.911+0.049 −0.053 |
24.13861+0.00102 −0.00090 |
0.1687+0.0025 −0.0026 |
668±22 | transit | 353.9±2.3 | 1.10±0.05 | 4970±120 | [88] | |
V1298 Tauri c | 0.499 | 8.24958 | 0.0825 | 845±27 | transit | 353.9 | 1.10 | 4970 | [89] | |
V1298 Tauri d | 0.572 | 12.4032 | 0.1083 | 677±22 | transit | 353.9 | 1.10 | 4970 | [89] | |
V1298 Tauri e | 0.780 | 60 | 0.308 | 492+66 −104 |
transit | 353.9 | 1.10 | 4970 | [89] | |
WASP-18Ac | 0.174±0.039 | 2.1558 | 0.035 | timing | 404 | 1.22 | 6400 | [90] | ||
WASP-126c | 0.202±0.077 | 7.63±0.17 | timing | 763.206±48.9235 | 1.12 | 5800 | [90]False positive[91] | |||
WASP-169b | 0.561 | 1.304 | 5.6114118 | 0.0681 | 1604 | transit | 2080 | 1.34 | 6110 | [92] |
WASP-171b | 1.084 | 0.980 | 3.8186244 | 0.05040 | 1642 | transit | 2530 | 1.17 | 5965 | [92] |
WASP-175b | 0.990 | 1.208 | 3.0652907 | 0.04403 | 1571 | transit | 2080 | 1.21 | 6229 | [92] |
WASP-177b | 0.508±0.038 | 1.58+0.66 −0.83 |
3.071722±0.000001 | 0.03957±0.00058 | 1142±32 | transit | 580.5583 | 0.876±0.038 | 5017±70 | [93] |
WASP-178b | 1.66 | 1.81 | 3.3448285 | 0.0558 | 2470 | transit | 1360 | 2.07 | 9360 | [94] |
WASP-180Ab | 0.9 | 1.24 | 3.409264 | 0.048 | transit | 830 | 1.3 | 6600 | [95] | |
WASP-181b | 0.299±0.034 | 1.184+0.071 −0.059 |
4.159±0.0000034 | 0.00542±0.00069 | 1186+32 −26 |
transit | 1444.872 | 1.04±0.04 | 5839±70 | [93] |
WASP-182b | 0.148 | 0.850 | 3.3769848 | 0.0451 | 1479 | transit | 1080 | 1.08 | 5638 | [92] |
WASP-183b | 0.502±0.047 | 1.47+0.94 −0.33 |
4.11177±0.0000051 | 0.0463±0.00075 | 1111±30 | transit | 1069.79292 | 1.00±0.03 | 0.784±0.038 | [93] |
WASP-184b | 0.57 | 1.33 | 5.18170 | 0.0627 | 1480 | transit | 2090 | 1.23 | 6000 | [94] |
WASP-185b | 0.980 | 1.25 | 9.38755 | 0.0904 | 1160 | transit | 897 | 1.12 | 5900 | [94] |
WASP-192b | 2.30 | 1.23 | 2.8786765 | 0.0408 | 1620 | transit | 1610 | 1.09 | 5910 | [94] |
KMT-2016-BLG-1836L b | 2.2+1.9 −1.1 |
3.5+1.1 −0.9 |
microlensing | 23157.1+2609.25 −7827.753 |
0.49+0.38 −0.25 |
[96] | ||||
HD 85628 A b | 3.1±0.9 | 1.53+0.07 −0.04 |
2.82406±0.00003 | 0.047±0.004 | 2100±100 | transit | 559.47±3.05 | 1.75±0.05 | 7800±200 | Mascara-4b: A3V giant star and a planet on retrograde orbit.[97] |
OGLE-2016-BLG-1227 b | 0.79+1.3 −0.39 |
3.4+2.1 −1 |
microlensing | 0.1+0.17 −0.05 |
[98] | |||||
OGLE-2013-BLG-0911L b | 9.51+2.72 −1.69 |
microlensing | 10500+1500 −1100 |
0.29+0.07 −0.05 |
[99] | |||||
L 1159-16 b | 0.088+0.060 −0.035 |
241.59+4.6 −4.0 |
0.403+0.039 −0.047 |
radial vel. | 14.584±0.007 | 0.15 | 3158 | [100][101] Refuted in 2022[102] | ||
L 1159-16 c | 0.23±0.02 | 772.05+2.41 −1.84 |
0.88±0.02 | radial vel. | 14.578±0.005 | 0.15±0.01 | 3154±54 | [100][101]Confirmed in 2022 as L 1159-16 b[102] | ||
TOI-175b | 0.00126+0.00050 −0.00048 |
0.0642+0.0046 −0.0035 |
2.2531136+0.0000012 −0.0000015 |
0.02191+0.00080 −0.00084 |
627+33 −36 |
transit | 34.636±0.010 | 0.273±0.030 | 3415±135 | [103] To date, it is the lowest mass planet confirmed, or measured, using the radial velocity technique.[104] Host star also known as L 98-59.[105] |
Specific exoplanet lists
- List of directly imaged exoplanets
- List of exoplanet extremes
- List of exoplanet firsts
- List of exoplanets discovered by the Kepler space telescope
- List of exoplanets observed during Kepler's K2 mission
- List of extrasolar candidates for liquid water
- List of hottest exoplanets
- List of coolest exoplanets
- List of multiplanetary systems
- List of nearest exoplanets
- List of nearest terrestrial exoplanet candidates
- List of potentially habitable exoplanets
- List of proper names of exoplanets
- List of largest exoplanets
- List of smallest exoplanets
- List of transiting exoplanets
Lists of exoplanets by year of discovery
- List of exoplanets discovered before 2000 (31)
- List of exoplanets discovered between 2000–2009 (377)
- List of exoplanets discovered in 2010 (109)
- List of exoplanets discovered in 2011 (179)
- List of exoplanets discovered in 2012 (149)
- List of exoplanets discovered in 2013 (151)
- List of exoplanets discovered in 2014 (870)
- List of exoplanets discovered in 2015 (150)
- List of exoplanets discovered in 2016 (1497)
- List of exoplanets discovered in 2017 (158)
- List of exoplanets discovered in 2018 (304)
- List of exoplanets discovered in 2019 (173)
- List of exoplanets discovered in 2020 (249)
- List of exoplanets discovered in 2021 (257)
- List of exoplanets discovered in 2022 (312)
- List of exoplanets discovered in 2023 (304)
- List of exoplanets discovered in 2024 (176)
References
- ^ "NASA Exoplanet Archive". exoplanetarchive.ipac.caltech.edu. California Institute of Technology. Retrieved 27 March 2018.
- ^ "Extrasolar Planet's Catalogue (sic)". Kyoto University. Retrieved 20 December 2019.
- ^ "The Extrasolar Planets Encyclopaedia". Retrieved 20 January 2018.
- ^ Luque, R.; Trifonov, T.; Reffert, S.; Quirrenbach, A.; Lee, M. H.; Albrecht, S.; Andersen, M. Fredslund; Antoci, V.; Grundahl, F.; Schwab, C.; Wolthoff, V. (13 October 2019). "Precise radial velocities of giant stars XIII. A second Jupiter orbiting in 4:3 resonance in the 7 CMa system". Astronomy & Astrophysics. A136: 631. arXiv:1910.05853. Bibcode:2019A&A...631A.136L. doi:10.1051/0004-6361/201936464. S2CID 204512658.
- ^ "A second planet in the Beta Pictoris system". Nanowerk. 19 August 2019. Retrieved 20 August 2019.
- ^ Benatti, S.; Nardiello, D.; Malavolta, L.; Desidera, S.; Borsato, L.; Nascimbeni, V.; Damasso, M.; D'Orazi, V.; Mesa, D.; Messina, S.; Esposito, M.; Bignamini, A.; Claudi, R.; Covino, E.; Lovis, C.; Sabotta, S. (October 2019). "A possibly inflated planet around the bright young star DS Tucanae A". Astronomy & Astrophysics. 630: A81. arXiv:1904.01591. Bibcode:2019A&A...630A..81B. doi:10.1051/0004-6361/201935598. ISSN 0004-6361. S2CID 102486551.
- ^ Feng, Fabo; Anglada-Escudé, Guillem; Tuomi, Mikko; Jones, Hugh R. A.; Chanamé, Julio; Butler, Paul R.; Janson, Markus (14 October 2019), "Detection of the nearest Jupiter analog in radial velocity and astrometry data", Monthly Notices of the Royal Astronomical Society, 490 (4): 5002–5016, arXiv:1910.06804, Bibcode:2019MNRAS.490.5002F, doi:10.1093/mnras/stz2912, S2CID 204575783
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ Stefansson, Gudmundur; et al. (2020), "A Sub-Neptune-sized Planet Transiting the M2.5 Dwarf G 9-40: Validation with the Habitable-zone Planet Finder", The Astronomical Journal, 159 (3): 100, arXiv:1912.00291, Bibcode:2020AJ....159..100S, doi:10.3847/1538-3881/ab5f15, S2CID 208526899
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ G 9-40 b
- ^ Perger, M.; et al. (April 2019). "Gliese 49: Activity evolution and detection of a super-Earth". Astronomy & Astrophysics. 624: 19. arXiv:1903.04808. Bibcode:2019A&A...624A.123P. doi:10.1051/0004-6361/201935192. ISSN 0004-6361. S2CID 85497416. A123.
- ^ a b c Jenkins, J. S.; Pozuelos, F. J.; Tuomi, M.; Berdiñas, Z. M.; Díaz, M. R.; Vines, J. I.; Suárez, Juan C.; Peña Rojas, P. A. (2019), "GJ 357: A low-mass planetary system uncovered by precision radial velocities and dynamical simulations", Monthly Notices of the Royal Astronomical Society, 490 (4): 5585–5595, arXiv:1909.00831, doi:10.1093/mnras/stz2937
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ Hobson, M. J.; et al. (2019), "The SOPHIE search for northern extrasolar planets", Astronomy & Astrophysics, 625: A18, arXiv:1902.05998, doi:10.1051/0004-6361/201834890
- ^ Díaz, R. F.; et al. (2019), "The SOPHIE search for northern extrasolar planets", Astronomy & Astrophysics, 625: A17, arXiv:1902.06004, doi:10.1051/0004-6361/201935019
- ^ Pinamonti, M.; Sozzetti, A.; Giacobbe, P.; Damasso, M.; Scandariato, G.; Perger, M.; González Hernández, J. I.; Lanza, A. F.; Maldonado, J.; Micela, G.; Suárez Mascareño, A.; Toledo-Padrón, B.; Affer, L.; Benatti, S.; Bignamini, A.; Bonomo, A. S.; Claudi, R.; Cosentino, R.; Desidera, S.; Maggio, A.; Martinez Fiorenzano, A.; Pagano, I.; Piotto, G.; Rainer, M.; Rebolo, R.; Ribas, I. (2019), "The HADES RV programme with HARPS-N at TNG", Astronomy & Astrophysics, 625: A126, arXiv:1903.11853, doi:10.1051/0004-6361/201834969
- ^ Affer, L.; Damasso, M.; Micela, G.; Poretti, E.; Scandariato, G.; Maldonado, J.; Lanza, A. F.; Covino, E.; Rubio, A. Garrido (31 January 2019). "HADES RV program with HARPS-N at TNG. IX. A super-Earth around the M dwarf Gl686". Astronomy & Astrophysics. 622: A193. arXiv:1901.05338. Bibcode:2019A&A...622A.193A. doi:10.1051/0004-6361/201834868. ISSN 0004-6361. S2CID 118863481.
- ^ Morales, J. C.; et al. (2019). "A giant exoplanet orbiting a very-low-mass star challenges planet formation models". Science. 365 (6460): 1441–1445. arXiv:1909.12174. Bibcode:2019Sci...365.1441M. doi:10.1126/science.aax3198. ISSN 0036-8075. PMID 31604272. S2CID 202888425.
- ^ The CARMENES search for exoplanets around M dwarfs - The enigmatic planetary system GJ 4276: One eccentric planet or two planets in a 2:1 resonance?, 2019, arXiv:1901.02367
- ^ a b Zhou, G.; et al. (2019), "Two New HATNet Hot Jupiters around a Stars and the First Glimpse at the Occurrence Rate of Hot Jupiters from TESS", The Astronomical Journal, 158 (4): 141, arXiv:1906.00462, Bibcode:2019AJ....158..141Z, doi:10.3847/1538-3881/ab36b5, S2CID 173990300
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ Bello-Arufe, Aaron; Cabot, Samuel H. C.; Mendonça, João M.; Buchhave, Lars A.; Rathcke, Alexander D. (2022), "Mining the Ultrahot Skies of HAT-P-70b: Detection of a Profusion of Neutral and Ionized Species", The Astronomical Journal, 163 (2): 96, arXiv:2112.03292, Bibcode:2022AJ....163...96B, doi:10.3847/1538-3881/ac402e, S2CID 244920901
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ a b c d e f g h i j k l m n Search for nearby Earth analogs I. 15 planet candidates found in PFS data, 2019, arXiv:1904.08567
- ^ a b c d The CORALIE survey for southern extrasolar planets XVIII Three new massive planets and two low mass brown dwarfs at separation larger than 5 AU, 2019, arXiv:1904.01573
- ^ a b Hot, rocky and warm, puffy super-Earths orbiting TOI-402 (HD 15337), 2019, arXiv:1903.05419
- ^ a b Dragomir, Diana; et al. (2019), "TESS Delivers Its First Earth-sized Planet and a Warm Sub-Neptune", The Astrophysical Journal, 875 (2): L7, arXiv:1901.00051, Bibcode:2019ApJ...875L...7D, doi:10.3847/2041-8213/ab12ed, S2CID 129945503
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ Wittenmyer, Robert A.; et al. (2019). "Truly eccentric – I. Revisiting eight single-eccentric planetary systems". Monthly Notices of the Royal Astronomical Society. 484 (4): 5859–5867. arXiv:1901.08471. Bibcode:2019MNRAS.484.5859W. doi:10.1093/mnras/stz290.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ Dorval, P.; Talens, G. J. J.; Otten, G. P. P. L.; Brahm, R.; Jordán, A.; Torres, P.; Vanzi, L.; Zapata, A.; Henry, T.; Paredes, L.; Jao, W. C.; James, H.; Hinojosa, R.; Bakos, G. A.; Csubry, Z.; Bhatti, W.; Suc, V.; Osip, D.; Mamajek, E. E.; Mellon, S. N.; Wyttenbach, A.; Stuik, R.; Kenworthy, M.; Bailey, J.; Ireland, M.; Crawford, S.; Lomberg, B.; Kuhn, R.; Snellen, I. (2020), "MASCARA-4 b/B Ring-1 b: A retrograde hot Jupiter around a bright A-type star", Astronomy & Astrophysics, 635: A60, arXiv:1904.02733, Bibcode:2020A&A...635A..60D, doi:10.1051/0004-6361/201935611, S2CID 102351446
- ^ Ahlers, John P.; Kruse, Ethan; Colón, Knicole D.; Dorval, Patrick; Talens, Geert Jan; Snellen, Ignas; Albrecht, Simon; Otten, Gilles; Ricker, George; Vanderspek, Roland; Latham, David; Seager, Sara; Winn, Joshua; Jenkins, Jon M.; Haworth, Kari; Cartwright, Scott; Morris, Robert; Rowden, Pam; Tenenbaum, Peter; Ting, Eric B. (2020), "Gravity-darkening Analysis of the Misaligned Hot Jupiter MASCARA-4 B", The Astrophysical Journal, 888 (2): 63, arXiv:1911.05025, Bibcode:2020ApJ...888...63A, doi:10.3847/1538-4357/ab59d0, S2CID 207863659
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ Zhang, Yapeng; Snellen, Ignas A. G.; Wyttenbach, Aurèlien; Nielsen, Louise D.; Lendl, Monika; Casasayas-Barris, Núria; Chaverot, Guillaume; Kesseli, Aurora Y.; Lovis, Christophe; Pepe, Francesco A.; Psaridi, Angelica; Seidel, Julia V.; Udry, Stéphane; Ulmer-Moll, Solène (2022), "Transmission spectroscopy of the ultra-hot Jupiter MASCARA-4 B", Astronomy & Astrophysics, 666: A47, arXiv:2208.11427, doi:10.1051/0004-6361/202244203, S2CID 251678624
- ^ Rickman, E. L.; et al. (May 2019). "The CORALIE survey for southern extrasolar planets. XVIII. Three new massive planets and two low-mass brown dwarfs at greater than 5 AU separation". Astronomy & Astrophysics. 625: 16. arXiv:1904.01573. Bibcode:2019A&A...625A..71R. doi:10.1051/0004-6361/201935356. S2CID 91184450. A71.
- ^ a b Detection of Planetary and Stellar Companions to Neighboring Stars via a Combination of Radial Velocity and Direct Imaging Techniques, 2019, arXiv:1904.12931
- ^ Kinematic detection of a planet carving a gap in a protoplanetary disc, 2023, arXiv:1907.02538
- ^ a b Trifonov, Trifon; Stock, Stephan; Henning, Thomas; Reffert, Sabine; Kürster, Martin; Lee, Man Hoi; Bitsch, Bertram; Butler, R. Paul; Vogt, Steven S. (2019), "Two Jovian Planets around the Giant Star HD 202696: A Growing Population of Packed Massive Planetary Pairs around Massive Stars?", The Astronomical Journal, 157 (3): 93, arXiv:1901.01935, Bibcode:2019AJ....157...93T, doi:10.3847/1538-3881/aafa11, S2CID 119047091
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ a b HD 213885b: A transiting 1-day-period super-Earth with an Earth-like composition around a bright (V=7.9) star unveiled by TESS, 2019, arXiv:1903.07694
- ^ A Hot Saturn Orbiting An Oscillating Late Subgiant Discovered by TESS, 2019, arXiv:1901.01643
- ^ The B-Star Exoplanet Abundance Study: a co-moving 16-25 Mjup companion to the young binary system HIP 79098, 2019, arXiv:1906.02787
- ^ a b c Vanderburg, Andrew; et al. (2019). "TESS Spots a Compact System of Super-Earths around the Naked-Eye Star HR 858". The Astrophysical Journal. 881 (1): L19. arXiv:1905.05193. Bibcode:2019ApJ...881L..19V. doi:10.3847/2041-8213/ab322d. S2CID 153311715.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ Blunt, Sarah; Endl, Michael; Weiss, Lauren M.; Cochran, William D.; Howard, Andrew W.; MacQueen, Phillip J.; et al. (August 2019). "Radial Velocity Discovery of an Eccentric Jovian World Orbiting at 18 au". The Astronomical Journal. 158 (5): 181. arXiv:1908.09925. Bibcode:2019AJ....158..181B. doi:10.3847/1538-3881/ab3e63. S2CID 201646255.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ Transit least-squares survey - I. Discovery and validation of an Earth-sized planet in the four-planet system K2-32 near the 1:2:5:7 resonance, 2019, arXiv:1904.00651
- ^ a b c d Four Small Planets Buried in K2 Systems: What Can We Learn For TESS?, 2019, arXiv:1907.08244
- ^ a b c d , 2019, arXiv:1905.09038
{{citation}}
: Missing or empty|title=
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suggested) (help) - ^ Wells, R.; Poppenhaeger, K.; Watson, C. A. (2019), "Validation of a temperate fourth planet in the K2-133 multiplanet system", Monthly Notices of the Royal Astronomical Society, 487 (2): 1865–1873, arXiv:1905.05206, doi:10.1093/mnras/stz1334
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ K2-146: Discovery of Planet c, Precise Masses from Transit Timing, and Observed Precession, 2019, arXiv:1907.10620
- ^ a b c Adams, Elisabeth R.; Jackson, Brian; Johnson, Samantha; Ciardi, David R.; Cochran, William D.; Endl, Michael; Everett, Mark E.; Furlan, Elise; Howell, Steve B.; Jayanthi, Prasanna; MacQueen, Phillip J.; Matson, Rachel A.; Partyka-Worley, Ciera; Schlieder, Joshua; Scott, Nicholas J.; Stanton, Sevio M.; Ziegler, Carl (2020), ULTRA SHORT PERIOD PLANETS IN K2 III: NEIGHBORS ARE COMMON WITH 12 NEW MULTI-PLANET SYSTEMS AND 26 NEWLY VALIDATED PLANETS IN CAMPAIGNS 0-8, 10, arXiv:2011.11698
- ^ Alonso, E Díez; Hernández, J I González; Toledo–Padrón, B.; Gómez, S L Suárez; Mascareño, A Suárez; Aguado, D. S.; Gutiérrez, C González; Cabrera-Lavers, A.; Carballido–Landeira, J.; Bonavera, L.; Juez, F J de Cos; Rebolo, R. (2019), "A transiting super-Earth close to the inner edge of the habitable zone of an M0 dwarf star", Monthly Notices of the Royal Astronomical Society, arXiv:1901.04739, doi:10.1093/mnras/sty3467
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ Feinstein, Adina D.; et al. (7 January 2019). "K2-288Bb: A Small Temperate Planet in a Low-mass Binary System Discovered by Citizen Scientists" (PDF). The Astronomical Journal. 157 (2): 40. arXiv:1902.02789. Bibcode:2019AJ....157...40F. doi:10.3847/1538-3881/aafa70. hdl:1721.1/121222.
- ^ a b Hjorth, M.; Justesen, A. B.; Hirano, T.; Albrecht, S.; Gandolfi, D.; Dai, F.; Alonso, R.; Barragán, O.; Esposito, M.; Kuzuhara, M.; Lam, K. W. F.; Livingston, J. H.; Montanes-Rodriguez, P.; Narita, N.; Nowak, G.; Prieto-Arranz, J.; Redfield, S.; Rodler, F.; Van Eylen, V.; Winn, J. N.; Antoniciello, G.; Cabrera, J.; Cochran, W. D.; Csizmadia, Sz; De Leon, J.; Deeg, H.; Eigmüller, Ph; Endl, M.; Erikson, A.; et al. (2019), "K2-290: a warm Jupiter and a mini-Neptune in a triple-star system", Monthly Notices of the Royal Astronomical Society, 484 (3): 3522, arXiv:1901.03716, Bibcode:2019MNRAS.484.3522H, doi:10.1093/mnras/stz139
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ a b Hjorth, Maria; Albrecht, Simon; Hirano, Teruyuki; Winn, Joshua N.; Dawson, Rebekah I.; Zanazzi, J. J.; Knudstrup, Emil; Sato, Bun'ei (2021), "A backward-spinning star with two coplanar planets", Proceedings of the National Academy of Sciences of the United States of America, 118 (8): e2017418118, arXiv:2102.07677, Bibcode:2021PNAS..11817418H, doi:10.1073/pnas.2017418118, PMC 7923373, PMID 33593909
- ^ K2-291 b: A rocky super-Earth in a 2.2 day orbit, 2019, arXiv:1901.04558
- ^ a b IDENTIFYING EXOPLANETS WITH DEEP LEARNING II: TWO NEW SUPER-EARTHS UNCOVERED BY A NEURAL NETWORK IN K2 DATA, 2019, arXiv:1903.110507
{{citation}}
: Check|arxiv=
value (help) - ^ Kovacs, Geza (2020), "More planetary candidates from K2 Campaign 5 using TRAN_K2", Astronomy & Astrophysics, 643: A169, arXiv:2008.10075, Bibcode:2020A&A...643A.169K, doi:10.1051/0004-6361/202038726, S2CID 221266076
- ^ De Leon, J. P.; Livingston, J.; Endl, M.; Cochran, W. D.; Hirano, T.; García, R. A.; Mathur, S.; Lam, K W F.; Korth, J.; Trani, A. A.; Dai, F.; Díez Alonso, E.; Castro-González, A.; Fridlund, M.; Fukui, A.; Gandolfi, D.; Kabath, P.; Kuzuhara, M.; Luque, R.; Savel, A. B.; Gill, H.; Dressing, C.; Giacalone, S.; Narita, N.; Palle, E.; Van Eylen, V.; Tamura, M. (2021), "37 new validated planets in overlapping K2 campaigns", Monthly Notices of the Royal Astronomical Society, 508: 195–218, arXiv:2108.05621, doi:10.1093/mnras/stab2305
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ Johns, Daniel; et al. (2019), "KELT-23Ab: A Hot Jupiter Transiting a Near-solar Twin Close to the TESS and JWST Continuous Viewing Zones", The Astronomical Journal, 158 (2): 78, arXiv:1903.00031, doi:10.3847/1538-3881/ab24c7, S2CID 119252456
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ Weiss, Lauren M.; Fabrycky, Daniel C.; Agol, Eric; Mills, Sean M.; Howard, Andrew W.; Isaacson, Howard; Petigura, Erik A.; Fulton, Benjamin; Hirsch, Lea; Sinukoff, Evan (2020-04-29). "The Discovery of the Long-Period, Eccentric Planet Kepler-88 d and System Characterization with Radial Velocities and Photodynamical Analysis" (PDF). The Astronomical Journal. 159 (5): 242. arXiv:1909.02427. Bibcode:2020AJ....159..242W. doi:10.3847/1538-3881/ab88ca. ISSN 1538-3881. S2CID 202539420.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ a b Sun, L.; Ioannidis, P.; Gu, S.; Schmitt, J. H. M. M.; Wang, X.; Kouwenhoven, M. B. N. (2019), "Kepler-411: a four-planet system with an active host star", Astronomy & Astrophysics, 624: A15, arXiv:1902.09719, Bibcode:2019A&A...624A..15S, doi:10.1051/0004-6361/201834275, S2CID 102481339
- ^ Jung, Youn Kil; Gould, Andrew; Zang, Weicheng; Hwang, Kyu-Ha; Ryu, Yoon-Hyun; Han, Cheongho; Yee, Jennifer C.; Albrow, Michael D.; Chung, Sun-Ju; Shin, In-Gu; Shvartzvald, Yossi; Zhu, Wei; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Hyoun-Woo; Kim, Seung-Lee; Lee, Chung-Uk; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W.; KMTNet Collaboration; Penny, Matthew T.; Mao, Shude; Fouqué, Pascal; Wang, Tianshu; CFHT Collaboration (2018), "KMT-2017-BLG-0165Lb: A Super-Neptune mass planet Orbiting a Sun-like Host Star", The Astronomical Journal, 157 (2): 72, arXiv:1809.01288, Bibcode:2019AJ....157...72J, doi:10.3847/1538-3881/aaf87f, S2CID 119096973
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ Ryu, Yoon-Hyun; Mróz, Przemek; Gould, Andrew; Hwang, Kyu-Ha; Kim, Hyoun-Woo; Yee, Jennifer C.; Albrow, Michael D.; Chung, Sun-Ju; Jung, Youn Kil; Shin, In-Gu; Shvartzvald, Yossi; Zang, Weicheng; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Seung-Lee; Lee, Chung-Uk; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Han, Cheongho; Pogge, Richard W.; Udalski, Andrzej; Poleski, Radek; Skowron, Jan; Szymański, Michał K.; Soszyński, Igor; Pietrukowicz, Paweł; Kozłowski, Szymon; Ulaczyk, Krzysztof; et al. (2021), "KMT-2017-BLG-2820 and the Nature of the Free-Floating Planet Population", The Astronomical Journal, 161 (3): 126, arXiv:2010.07527, Bibcode:2021AJ....161..126R, doi:10.3847/1538-3881/abd55f, S2CID 222378863
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ a b A super-Earth and sub-Neptune transiting the late-type M dwarf LP 791-18, 2019, arXiv:1906.09267
- ^ a b c The L 98-59 System: Three Transiting, Terrestrial-Sized Planets Orbiting a Nearby M-dwarf, 2019, arXiv:1903.08017
- ^ The CARMENES search for exoplanets around M dwarfs Detection of a mini-Neptune around LSPM J2116+0234 and refinement of orbital parameters of a super-Earth around GJ 686 (BD+18 3421)
- ^ Winters, Jennifer G.; et al. (2019), "Three Red Suns in the Sky: A Transiting, Terrestrial Planet in a Triple M-dwarf System at 6.9 pc", The Astronomical Journal, 158 (4): 152, arXiv:1906.10147, Bibcode:2019AJ....158..152W, doi:10.3847/1538-3881/ab364d, S2CID 195584444
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ Kondo, Iona; et al. (2019), "MOA-bin-29b: A Microlensing Gas-giant Planet Orbiting a Low-mass Host Star", The Astronomical Journal, 158 (6): 224, arXiv:1905.01239, Bibcode:2019AJ....158..224K, doi:10.3847/1538-3881/ab4e9e, S2CID 145052576
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ Eigmüller, Philipp; et al. (2019), "NGTS-5b: A highly inflated planet offering insights into the sub-Jovian desert", Astronomy & Astrophysics, 625: A142, arXiv:1905.02593, Bibcode:2019A&A...625A.142E, doi:10.1051/0004-6361/201935206, S2CID 146809360
- ^ Vines, Jose I.; et al. (2019), "NGTS-6b: An ultrashort period hot-Jupiter orbiting an old K dwarf", Monthly Notices of the Royal Astronomical Society, 489 (3): 4125–4134, arXiv:1904.07997, doi:10.1093/mnras/stz2349
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ a b NGTS-8b and NGTS-9b: two non-inflated hot-Jupiters, 2019, arXiv:1911.02814
- ^ Zhu, Li-Ying; Qian, Sheng-Bang; Fernández Lajús, Eduardo; Wang, Zhi-Hua; Li, Lin-Jia; -J, Li L. (2019). "A close-in substellar object orbiting the sdOB-type eclipsing-binary system NSVS 14256825". Research in Astronomy and Astrophysics. 19 (9): 134. arXiv:1904.11664. Bibcode:2019RAA....19..134Z. doi:10.1088/1674-4527/19/9/134. S2CID 135471537.
- ^ Song, Shuo; Mai, Xinyu; Mutel, Robert L.; Pulley, David; Faillace, George; Watkins, Americo (2019). "An Updated Model for Circumbinary Planets Orbiting the SDB Binary NY Virginis". The Astronomical Journal. 157 (5): 184. Bibcode:2019AJ....157..184S. doi:10.3847/1538-3881/ab1139.
- ^ OGLE-2015-BLG-1649Lb: A gas giant planet around a low-mass dwarf, 2019, arXiv:1907.11536
- ^ Ryu, Yoon-Hyun; et al. (2020), "OGLE-2018-BLG-0532Lb: Cold Neptune with Possible Jovian Sibling", The Astronomical Journal, 160 (4): 183, arXiv:1905.08148, Bibcode:2020AJ....160..183R, doi:10.3847/1538-3881/abaa3f, S2CID 159041062
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ Spitzer Parallax of OGLE-2018-BLG-0596: A Low-mass-ratio Planet around an M-dwarf, 2019, arXiv:1905.05873
- ^ Spectroscopic Mass and Host-star Metallicity Measurements for Newly Discovered Microlensing Planet OGLE-2018-BLG-0740Lb, 2019, arXiv:1905.00155
- ^ a b OGLE-2018-BLG-1011L\lowercase{b,c}: Microlensing Planetary System with Two Giant Planets Orbiting a Low-mass Star, 2019, arXiv:1907.01741
- ^ "A Pair of Fledgling Planets Directly Seen Growing Around a Young Star". hubblesite.org. NASA. 3 June 2019. Retrieved 3 June 2019.
- ^ a b c Qatar Exoplanet Survey: Qatar-8b, 9b and 10b --- A Hot Saturn and Two Hot Jupiters, 2019, arXiv:1903.09258
- ^ Manser, Christopher J.; et al. (April 2019). "A planetesimal orbiting within the debris disc around a white dwarf star". Science. 364 (6435): 66–69. arXiv:1904.02163. Bibcode:2019Sci...364...66M. doi:10.1126/science.aat5330. PMID 30948547. S2CID 96434522.
- ^ a b Caballero, J. A.; Reiners, Ansgar; Ribas, I.; Dreizler, S.; Zechmeister, M.; et al. (12 June 2019). "The CARMENES search for exoplanets around M dwarfs. Two temperate Earth-mass planet candidates around Teegarden's Star" (PDF). Astronomy & Astrophysics. 627: A49. arXiv:1906.07196. Bibcode:2019A&A...627A..49Z. doi:10.1051/0004-6361/201935460. ISSN 0004-6361. S2CID 189999121.
- ^ "The Extrasolar Planet Encyclopaedia — TOI-813 b". exoplanet.eu.
- ^ a b c Nielsen, L. D.; Gandolfi, D.; Armstrong, D. J.; Jenkins, J. S.; Fridlund, M.; Santos, N. C.; Dai, F.; Adibekyan, V.; Luque, R.; Steffen, J. H.; Esposito, M.; Meru, F.; Sabotta, S.; Bolmont, E.; Kossakowski, D.; Otegi, J. F.; Murgas, F.; Stalport, M.; Rodler, F.; Díaz, M. R.; Kurtovic, N. T.; Ricker, G.; Vanderspek, R.; Latham, D. W.; Seager, S.; Winn, J. N.; Jenkins, J. M.; Allart, R.; Almenara, J. M.; et al. (2020), "Mass determinations of the three mini-Neptunes transiting TOI-125", Monthly Notices of the Royal Astronomical Society, 492 (4): 5399, arXiv:2001.08834, Bibcode:2020MNRAS.492.5399N, doi:10.1093/mnras/staa197
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ "exoplanet.eu toi-125_c".[permanent dead link]
- ^ "exoplanet.eu toi-125_d".[permanent dead link]
- ^ a b TOI-150b and TOI-163b: two transiting hot Jupiters, one eccentric and one inflated, revealed by TESS near and at the edge of the JWST CVZ, 2019, arXiv:1906.09866
- ^ An Eccentric Massive Jupiter Orbiting a Sub-Giant on a 9.5 Day Period Discovered in the Transiting Exoplanet Survey Satellite Full Frame Images, 2019, arXiv:1901.09950
- ^ a b Teachey, Alex; Jansen, Tiffany; Bakos, Gaspar; Torres, Guillermo; Hartman, Joel; Nesvorný, David; Kipping, David (2019). "A resonant pair of warm giant planets revealed by TESS". Monthly Notices of the Royal Astronomical Society. 486 (4): 4980–4986. arXiv:1902.03900. doi:10.1093/mnras/stz1141.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ a b Dawson, Rebekah I.; et al. (2019). "TOI-216b and TOI-216 c: Two Warm, Large Exoplanets in or Slightly Wide of the 2:1 Orbital Resonance". The Astronomical Journal. 158 (2): 65. arXiv:1904.11852. Bibcode:2019AJ....158...65D. doi:10.3847/1538-3881/ab24ba. S2CID 135466349.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ a b Dawson, Rebekah I.; Huang, Chelsea X.; Brahm, Rafael; Collins, Karen A.; Hobson, Melissa J.; Jordán, Andrés; Dong, Jiayin; Korth, Judith; Trifonov, Trifon; Abe, Lyu; Agabi, Abdelkrim; Bruni, Ivan; Butler, R. Paul; Barbieri, Mauro; Collins, Kevin I.; Conti, Dennis M.; Crane, Jeffrey D.; Crouzet, Nicolas; Dransfield, Georgina; Evans, Phil; Espinoza, Néstor; Gan, Tianjun; Guillot, Tristan; Henning, Thomas; Lissauer, Jack J.; Jensen, Eric L. N.; Sainte, Wenceslas Marie; Mékarnia, Djamel; Myers, Gordon; et al. (2021), "Precise transit and radial-velocity characterization of a resonant pair: a warm Jupiter TOI-216c and eccentric warm Neptune TOI-216b", The Astronomical Journal, 161 (4): 161, arXiv:2102.06754, Bibcode:2021AJ....161..161D, doi:10.3847/1538-3881/abd8d0, S2CID 231924886
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ a b c "太陽系外惑星「TOI 270 b、c、d」を発見。地球外生命体の存在は?". sorae. 2019-07-30. Retrieved 2021-01-08.
- ^ a b c Van Eylen, Vincent; Astudillo-Defru, Nicola; Bonfils, Xavier; Livingston, J.; Hirano, T.; Luque, Rafael; Lam, K. W. F.; Justesen, A. B.; Winn, J. N.; Gandolfi, D.; Nowak, G.; Palle, E.; Albrecht, S.; Dai, F.; Campos Estrada, B.; Owen, J. E.; Foreman-Mackey, D.; Fridlund, M.; Korth, J.; Mathur, S.; Forveille, Thierry; Mikal-Evans, T.; Osborne, H. L. M.; Ho, C. S. K.; Almenara, José M.; Artigau, Étienne; Barragán, O.; Bouchy, François; Cabrera, J.; et al. (2021), "Masses and compositions of three small planets orbiting the nearby M dwarf L231-32 (TOI-270) and the M dwarf radius valley", Monthly Notices of the Royal Astronomical Society, arXiv:2101.01593, doi:10.1093/mnras/stab2143
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ Mikal-Evans, Thomas; Madhusudhan, Nikku; Dittmann, Jason; Guenther, Maximilian N.; Welbanks, Luis; Vincent Van Eylen; Crossfield, Ian J. M.; Daylan, Tansu; Kreidberg, Laura (2022), Hubble Space Telescope transmission spectroscopy for the temperate sub-Neptune TOI-270d: a possible hydrogen-rich atmosphere containing water vapour, arXiv:2211.15576
- ^ a b Davis, Allen B.; Wang, Songhu; et al. (2020). "TOI 564 b and TOI 905 b: Grazing and Fully Transiting Hot Jupiters Discovered by TESS". Astronomical Journal. 160 (5): 229. arXiv:1912.10186. Bibcode:2020AJ....160..229D. doi:10.3847/1538-3881/aba49d. hdl:1721.1/134083. S2CID 209444463.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ David, Trevor J.; Cody, Ann Marie; Hedges, Christina L.; Mamajek, Eric E.; Hillenbrand, Lynne A.; Ciardi, David R.; Beichman, Charles A.; Petigura, Erik A.; Fulton, Benjamin J.; Isaacson, Howard T.; Howard, Andrew W.; Gagné, Jonathan; Saunders, Nicholas K.; Rebull, Luisa M.; Stauffer, John R.; Vasisht, Gautam; Hinkley, Sasha (2019), "A Warm Jupiter-sized Planet Transiting the Pre-main-sequence Star V1298 Tau", The Astronomical Journal, 158 (2): 79, arXiv:1902.09670, Bibcode:2019AJ....158...79D, doi:10.3847/1538-3881/ab290f, S2CID 119003936
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ a b c David, Trevor J.; Petigura, Erik A.; Luger, Rodrigo; Foreman-Mackey, Daniel; Livingston, John H.; Mamajek, Eric E.; Hillenbrand, Lynne A. (2019), "Four newborn planets transiting the young solar analog V1298 Tau", The Astrophysical Journal, 885 (1): L12, arXiv:1910.04563, Bibcode:2019ApJ...885L..12D, doi:10.3847/2041-8213/ab4c99, S2CID 204008446
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ a b A search for multi-planet systems with TESS using a Bayesian N-body retrieval and machine learning, 2019, arXiv:1907.03377
- ^ Search for planets in hot Jupiter systems with multi-sector TESS photometry. I. No companions in planetary systems KELT-18, KELT-23, KELT-24, Qatar-8, WASP-62, WASP-100, WASP-119, and WASP-126, 2020, arXiv:2010.11977
- ^ a b c d WASP-169, WASP-171, WASP-175 and WASP-182: three hot Jupiters and one bloated sub-Saturn mass planet discovered by WASP-south, 2019, arXiv:1904.10388
- ^ a b c Three Hot-Jupiters on the upper edge of the mass-radius distribution: WASP-177, WASP-181 and WASP-183, 2019, arXiv:1903.06622
- ^ a b c d Hellier, Coel; Anderson, D. R.; Barkaoui, K.; Benkhaldoun, Z.; Bouchy, F.; Burdanov, A.; Collier Cameron, A.; Delrez, L.; Gillon, M.; Jehin, E.; Nielsen, L. D.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Pozuelos, F. J.; Queloz, D.; Ségransan, D.; Smalley, B.; Triaud, A. H. M. J.; Turner, O. D.; Udry, S.; West, R. G. (2019), "WASP-South hot Jupiters: WASP-178b, WASP-184b, WASP-185b & WASP-192b", Monthly Notices of the Royal Astronomical Society, 490 (1): 1479, arXiv:1907.11667, Bibcode:2019MNRAS.490.1479H, doi:10.1093/mnras/stz2713
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ WASP-180Ab: Doppler tomography of an hot Jupiter orbiting the primary star in a visual binary, 2019, arXiv:1903.08002
- ^ Yang, Hongjing; et al. (2020). "KMT-2016-BLG-1836Lb: A Super-Jovian Planet from a High-cadence Microlensing Field". The Astronomical Journal. 159 (3): 98. arXiv:1908.10011. Bibcode:2020AJ....159...98Y. doi:10.3847/1538-3881/ab660e. S2CID 201646063.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ "MASCARA-4 b/bRing-1b - A retrograde hot Jupiter around the bright A3V star HD 85628". GroundAI.
- ^ "The Extrasolar Planet Encyclopaedia — OGLE-2016-BLG-1227 b". exoplanet.eu.
- ^ "The Extrasolar Planet Encyclopaedia — OGLE-2013-BLG-0911L b". exoplanet.eu.
- ^ a b Barnes, J. R.; et al. (2019-06-11), Frequency of planets orbiting M dwarfs in the Solar neighbourhood, arXiv:1906.04644v1, Bibcode:2019arXiv190604644T.
- ^ a b Feng, Fabo; Shectman, Stephen A.; Clement, Matthew S.; Vogt, Steven S.; Tuomi, Mikko; Teske, Johanna K.; Burt, Jennifer; Crane, Jeffrey D.; Holden, Bradford; Sharon Xuesong Wang; Thompson, Ian B.; Diaz, Matias R.; Paul Butler, R. (2020), "Search for Nearby Earth Analogs. III. Detection of ten new planets, three planet candidates, and confirmation of three planets around eleven nearby M dwarfs", The Astrophysical Journal Supplement Series, 250 (2): 29, arXiv:2008.07998, Bibcode:2020ApJS..250...29F, doi:10.3847/1538-4365/abb139, S2CID 221150644
{{citation}}
: CS1 maint: unflagged free DOI (link) - ^ a b Quirrenbach, A.; Passegger, V. M.; Trifonov, T.; Amado, P. J.; Caballero, J. A.; Reiners, A.; Ribas, I.; Aceituno, J.; Béjar, V. J. S.; Chaturvedi, P.; González-Cuesta, L.; Henning, T.; Herrero, E.; Kaminski, A.; Kürster, M.; Lalitha, S.; Lodieu, N.; López-González, M. J.; Montes, D.; Pallé, E.; Perger, M.; Pollacco, D.; Reffert, S.; Rodríguez, E.; López, C. Rodríguez; Shan, Y.; Tal-Or, L.; Osorio, M. R. Zapatero; Zechmeister, M. (2022), "The CARMENES search for exoplanets around M dwarfs", Astronomy & Astrophysics, 663: A48, arXiv:2203.16504, doi:10.1051/0004-6361/202142915, S2CID 247835988
- ^ Kostov, Veselin B.; Schlieder, Joshua E.; et al. (2019). "The L 98-59 System: Three Transiting, Terrestrial-size Planets Orbiting a Nearby M Dwarf". The Astronomical Journal. 158 (1): 32. arXiv:1903.08017. Bibcode:2019AJ....158...32K. doi:10.3847/1538-3881/ab2459. hdl:1721.1/124742. ISSN 1538-3881. S2CID 118855908.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ Demangeon, O. D. S.; Zapatero Osorio, M. R.; Alibert, Y.; Barros, S. C. C.; Adibekyan, V.; Tabernero, H. M.; Antoniadis-Karnavas, A.; Camacho, J. D.; al, et (2021). "Warm terrestrial planet with half the mass of Venus transiting a nearby star" (PDF). Astronomy & Astrophysics. 653: A41. arXiv:2108.03323. Bibcode:2021A&A...653A..41D. doi:10.1051/0004-6361/202140728. S2CID 236957385.
- ^ "Planet L 98-59 b". exoplanet.eu. Retrieved 6 August 2021.