List of exoplanets discovered in 2023

From Wikipedia - Reading time: 37 min

This list of exoplanets discovered in 2023 is a list of confirmed exoplanets that were first reported in 2023. 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) Discovery method Distance (ly) Host star mass (M) Host star temp. (K) Remarks
75 Ceti c 0.9120+0.0880
−0.1430
2051.62+45.98
−40.47
3.929+0.058
−0.052
radial vel. 270.58326 ±2.36023 1.92+0.07
−0.08
4809 [1]
AF Leporis b 3.2+0.7
−0.6
8030 ±1800 8.4+1.1
−1.3
1400 ±300 imaging 87.562 ±0.046 1.20 ±0.06 6130 ±60 Host star also known as HD 35850[2][3][4]
AU Microscopii d 0.00331 ±0.00161 12.73596 ±0.00793 0.1108 ±0.0020 459+13
−12
transit 32 0.510+0.028
−0.027
3678+90
−88
Potentially rocky super-Earth.[5][6]
BD-21 397 b 0.7 ±0.1 1891+56
−48
2.63+0.06
−0.05
radial vel. 77.4046+0.0744
−0.0740
0.679 ±0.017 4051 ±239 [7]
BD-21 397 c 2.4+1.5
−0.7
6360+6260
−711
5.9+3.4
−0.5
radial vel. 77.4046+0.0744
−0.0740
0.679 ±0.017 4051 ±239 [7]
DMPP-4 b 0.0384+0.0057
−0.0060
3.4982+0.0022
−0.2327
radial vel. 82.6101+0.1246
−0.1239
1.25 ±0.02 6400 ±50 [8]
EPIC 229004835 b 0.0327+0.0050
−0.0047
0.2080+0.0071
−0.0084
16.141132 ±0.000019 0.1237 ±0.0017 804 ±10 transit 398.255+2.867
−2.825
0.970 ±0.040 5868 ±60 [9]
Gliese 328 c 0.0673+0.0107
−0.0101
241.8+1.3
−1.7
0.657+0.026
−0.028
radial vel. 66.96874 ±0.54957 0.65 ±0.08 3897 ±71 [10]
Gliese 367 c 0.0130 ±0.0011 11.5301 ±0.0078 radial vel. 30.69986 ±0.00925 0.455 ±0.011 3522 ±70 [11]
Gliese 367 d 0.0190 ±0.0015 34.369 ±0.073 radial vel. 30.69986 ±0.00925 0.455 ±0.011 3522 ±70 [11]
Gliese 806 b 0.006 ±0.00053 0.11874 ±0.00205 0.9263237 ±0.0000009 0.1406 ±0.0003 940.0 ±10.0 transit 39.348 0.413 ±0.011 3600 ±16 [12] Host star also known as TOI-4481[13]
Gliese 806 c 0.0182 ±0.0009 6.65064 ±0.00025 0.0523 ±0.001 480.0 ±5.0 radial vel. 39.348 0.413 ±0.011 3600 ±16 [12] Host star also known as TOI-4481[14]
GJ 1151 c 0.03341+0.00412
−0.00463
0.29[15] 389.7+5.4
−6.5
0.5714+0.0053
−0.0064
radial vel. 26.23 ±0.01 0.1639 ±0.0093 3143 ±26 [16] Planet on 2-day orbit was suspected but refuted in 2021[17][18]
GJ 3988 b 0.0116 ±0.0013 6.9442 ±0.0010 0.0405+0.0011
−0.0012
radial vel. 32.32369 ±0.01357 0.1842 ±0.0153 3273 ±101 [19]
GJ 9404 b 0.0374 ±0.0060 13.4586+0.0044
−0.0067
0.0943 ±0.0036 radial vel. 77.8988+0.0828
−0.0825
0.62 ±0.07 [20]
HAT-P-2 c 10.7+5.2
−2.2
8500+2600
−1500
radial vel. 416.744+1.386
−1.380
1.33 ±0.03 6412.830+102.682
−110.120
Also known as HD 147506 c[21]
Beta Andromedae b 28.26+2.05
−2.17
663.87+4.61
−4.31
2.03 ±0.01 radial vel. 199.36184 ±9.26130 2.49 3802 Host star also known as Mirach[22]
HD 6061 b 0.0340±0.0085 0.219±0.008 5.254467±0.000009 0.059±0.001 1194±28 transit 220.548+0.670
−0.665
1.00±0.06 5920±110 Also known as TOI-1473 b[23]
HD 15906 b 0.200 ±0.007 10.924709 ±0.000032 0.200 ±0.007 668 ±13 transit 148.6035+0.2880
−0.2870
0.790+0.020
−0.036
4757 ±89 [24]
HD 15906 c 0.261+0.006
−0.005
21.583298+0.000052
−0.000055
0.141+0.002
−0.001
532 ±10 transit 148.6035+0.2880
−0.2870
0.790+0.020
−0.036
4757 ±89 [24]
HD 18438 b 21 ±1 803 ±5 2.1 ±0.1 radial vel. 731.066+29.409
−27.254
1.84 ±0.09 3860 ±100 [25]
HD 22946 d <0.08360 0.2326 ±0.0054 47.42489+0.00010
−0.00011
0.2958+0.0044
−0.0042
546 ±6 transit 204.7581+0.3787
−0.3370
1.098+0.040
−0.039
6169 ±64 [26]
HD 25463 b 0.0267±0.0098 0.234±0.014 7.049144±0.000009 0.076±0.002 1290±41 transit 148.786+0.409
−0.407
1.19±0.07 6220±110 Also known as TOI-554 b.[23]
HD 25463 c <0.013 0.134±0.011 3.044050±0.000008 0.0435±0.0009 1707±54 transit 148.786+0.409
−0.407
1.19±0.07 6220±110 Also known as TOI-554 c.[23]
HD 36384 b 6.6 ±0.5 490 ±3 1.3 ±0.1 radial vel. 682.674+11.588
−11.210
1.14 ±0.15 3940 ±40 [27]
HD 73256 c 16 ±1 2690+60
−102
3.8 ±0.1 radial vel. 119.7253+0.1833
−0.1823
1.00 ±0.05 [28]
HD 74698 b 0.07 ±0.01 15.017 ±0.002 0.121 ±0.001 radial vel. 169.8125+0.2479
−0.2472
1.039 ±0.025 5873 ±19 [7]
HD 74698 c 0.40 ±0.06 3449+189
−210
4.5 ±0.2 radial vel. 169.8125+0.2479
−0.2472
1.039 ±0.025 5873 ±19 [7]
HD 75302 b 5.4+0.5
−0.4
4356+173
−112
5.3+0.2
−0.1
radial vel. 98.9192+0.1973
−0.1970
1.06 ±0.05 [28]
HD 89839 b 5.01+0.79
−0.76
3441+18
−17
4.761 ±0.042 radial vel. 186.9079+0.3584
−0.3568
1.21 ±0.03 6314 ±65 [29]
HD 94771 b 0.53 ±0.03 2164+21
−20
3.48 ±0.03 radial vel. 188.4552+0.3930
−0.3911
1.200 ±0.024 5631 ±21 [7]
HD 99492 c 17.9 ±1.3 95.233+0.098
−0.096
radial vel. 59.3728+0.1895
−0.1882
0.85 ±0.02 4929 ±44 Host star also known as 83 Leonis[30]
HD 108202 b 3.0+0.7
−0.5
2990+54
−51
3.7 ±0.1 radial vel. 126.1689+0.2202
−0.2195
0.74 ±0.04 [28]
Delta Virginis b 15.83+2.33
−2.74
466.63+2.33
−2.74
1.33+0.08
−0.11
radial vel. 202.45560 ±11.05904 1.4 ±0.3 3657 [31]Host star also known as Minelauva or Auva
HD 135625 b 2.3+0.8
−0.3
4055+45
−44
5.4 ±0.1 radial vel. 184.3368+0.3803
−0.3734
1.28 ±0.06 [28]
HD 135694 b 0.018±0.007 0.224±0.012 15.92346±0.00002 0.120±0.003 815±27 transit 240.936+0.469
−0.468
0.90±0.06 5710±110 Also known as TOI-1247 b.[23]
HD 163296 b 0.267 46 disk kinematics 330.15±3.85[32] 2.041±0.395[32] 8291±510[32] [33]
HD 163296 c 0.189 54 disk kinematics [33]
HD 163296 d 0.40 84.5 disk kinematics [33]
HD 163296 e 1 137 disk kinematics [33]
HD 165131 b 19+2
−1
2343 ±2 3.59+0.06
−0.07
radial vel. 187.2993+0.0689
−0.0684
1.10 ±0.06 [28]
HD 167677 b 3.7+1.6
−1.1
1804 ±73 2.9 ±0.1 radial vel. 177.1869+0.9031
−0.8940
1.00 ±0.05 [28]
HD 169142 b 3 ±2 37.2 ±1.5 imaging 435.744+2.717
−2.674
1.85 [34]
HD 185283 b 1.3+0.3
−0.1
4060+148
−112
4.6+0.2
−0.1
radial vel. 102.3967+0.1778
−0.1768
0.80 ±0.04 [28]
HD 207496 b 0.0192 ±0.0050 0.201 ±0.010 6.441008 ±0.000011 0.0629 ±0.0011 743 ±26 transit 77.11 ±0.04 0.80 ±0.04 4819 ±94 [35]
HD 235088 b 0.1824 ±0.0067 7.4341393 ±0.0000062 0.0720 ±0.0026 805+13
−12
transit 134.2804 ±0.4612 0.789+0.022
−0.021
5037 ±14 Host star also known as TOI-1430[36]
HIP 8152 b 0.025±0.006 0.228±0.017 10.75101±0.00006 0.092±0.002 855±28 transit 331.681+1.373
−1.360
0.91±0.06 5530±110 Also known as TOI-266 b.[23]
HIP 8152 c 0.0296±0.0069 0.221±0.017 19.6053±0.0003 0.138±0.003 699±23 transit 331.681+1.373
−1.360
0.91±0.06 5530±110 Also known as TOI-266 c.[23]
HIP 9618 b 0.0315 ±0.0098 0.348 20.772907 ±0.000023 0.1438+0.0025
−0.0037
663.4+9.1
−6.3
transit 220.3112+0.5108
−0.5085
1.022+0.043
−0.076
5609.0 ±33.0 [37]
HIP 9618 c <0.0576 ±0.0053 0.298 52.563491 ±0.000072 0.2669+0.0046
−0.0069
486.9+6.6
−4.6
transit 220.3112+0.5108
−0.5085
1.022+0.043
−0.076
5609.0 ±33.0 [37]
HIP 29442 b 0.032 ±0.0025 0.31 13.63083 ±0.00003 0.1070 ±0.0016 777 ±18 transit 222.4123+0.5779
−0.5750
0.89 ±0.04 5289 ±69 Host star also known as TOI-469[38]
HIP 29442 c 0.014 ±0.001 1.58+0.10
−0.11
3.53796 ±0.00003 0.0436+0.0006
−0.0007
1217 ±29 radial vel. 222.4123+0.5779
−0.5750
0.89 ±0.04 5289 ±69 [38]
HIP 29442 d 0.016 ±0.001 1.37 ±0.11 6.42975+0.00009
−0.00010
0.0649+0.0009
−0.0010
998.0 ±24.0 radial vel. 222.4123+0.5779
−0.5750
0.89 ±0.04 5289 ±69 [38]
HIP 54597 b 2.4+0.4
−0.2
3274+47
−46
4.0 ±0.1 radial vel. 129.6239+0.2166
−0.2162
0.80 ±0.04 [28]
HIP 81208 C b 14.8 ±0.4 104100+107260
−40934
23.04+13.88
−6.55
2050+35
−20
imaging 481.188+4.837
−4.472
0.135+0.010
−0.013
[39]
HIP 113103 b 0.163 7.610303 ±0.000018 0.06899+0.00029
−0.00023
721 ±10 transit 150.7239+0.2818
−0.2805
0.761 ±0.038 4930 ±100 [40]
HIP 113103 c 0.2141 14.245648 ±0.000019 0.10479+0.00045
−0.00035
585 ±10 transit 150.7239+0.2818
−0.2805
0.761 ±0.038 4930 ±100 [40]
HN Librae b 0.0172 ±0.0024 36.116+0.027
−0.029
0.1417 ±0.0023 234.4+5.5
−5.3
radial vel. 20.36655 ±0.01453 0.291 ±0.013 3347 ±50 Habitable zone planet. Host star also known as Gliese 555[41]
K2-312 c 5.41++0.52
−0.44
921.2 ±10.8 1.961 ±0.027 radial vel. 358.315+2.645
−2.609
1.18 ±0.04 5959 ±61 [42]
K2-415b 0.0094 ±0.0085 0.091 ±0.005 4.0179694 ±0.0000027 0.0270 ±0.0002 412 ±9 transit 71.126 ±0.030 0.1635 ±0.0041 3173 ±53 [43]
K2-416 b <5.2 0.241+0.027
−0.0152
13.1020+0.0026
−0.0024
0.0880+0.0100
−0.0210
447 ±49 transit 392.402+1.973
−1.954
0.548 ±0.012 3746 ±72 [44]
K2-417 b <2.2 0.295+0.012
−0.011
6.5350 ±0.0014 0.063+0.006
−0.014
558 ±55 transit 306.7249+0.9860
−0.9794
0.569 ±0.012 3861 ±77 [44]
K2-2016-BLG-0005L b 1.16 ±0.09 1.23 4700 +3000
−700
4.11 ±0.32 microlensing 16960 0.574 ±0.037 Gas giant.[45][46]
Kepler-10 d 0.03990 ±0.00705 151.04 ±0.45 0.5379 ±0.0044 radial vel. 605.039+2.645
−2.626
0.910 ±0.021 5708 ±28 [42]
Kepler-68 e 0.272 ±0.032 3455 +348
−169
4.60 +0.32
−0.16
radial vel. 1.057 +0.022
−0.020
5847 ±75 [47]
Kepler-58 d 0.1509503920 4.458169937 transit 1.017 +0.167
−0.125
6100+193
−214
[48]
Kepler-164 e 0.3570351276 94.8864975 transit 0.966 +0.075
−0.068
5888 +106
−117
[48]
Kepler-290 d 0.0794273806 0.764007986 transit 0.84 +0.065
−0.09
5142 ±153 [48]
Kepler-297 d 0.6351157298 150.0209961 transit 0.846 +0.059
−0.049
5618 ±112 [48]
Kepler-311 d 0.1849409870 232.0469971 transit 0.974 +0.082
−0.062
5903 +106
−117
[48]
Kepler-347 d 0.2346332985 85.51660156 transit 1 ±0.072 5592 ±75 [48]
Kepler-416 d 0.1543405297 3.076410055 transit 0.949 +0.067
−0.055
5670 ±114 [48]
Kepler-549 d 0.4055676538 24.6147995 transit 0.859 +0.06
−0.033
5312 ±79 [48]
Kepler-618 d 0.3911149410 11.67889977 transit 1.041 ±0.139 6122 +169
−190
[48]
Kepler-656 c 0.1360516194 5.254559994 transit 1.05+0.075
−0.113
5550 +166
−183
[48]
Kepler-763 c 0.1464004690 4.096680164 transit 0.8 +0.048
−0.028
4999 ±79 [48]
Kepler-763 d 0.1754842890 6.503270149 transit 0.8 +0.048
−0.028
4999 ±79 [48]
Kepler-784 c 0.1583551639 17.15699959 transit 1.016 +0.093
−0.084
5676 +115
−104
[48]
Kepler-864 c 0.157641449 2.421489954 transit 1.27 +0.142
−0.156
6213 +173
−259
[48]
Kepler-865 c 0.09474546031 6.209179878 transit 0.782 +0.116
−0.062
5440 ±162 [48]
Kepler-880 c 0.2816491659 11.80609989 transit 1.714 +0.17
−0.316
6900 +184
−204
[48]
Kepler-896 c 0.2770100246 29.54210091 transit 0.877 +0.083
−0.092
5510 +166
−149
[48]
Kepler-949 c 0.4607912263 20.99720001 transit 0.813 +0.104
−0.064
5211 +181
−163
[48]
Kepler-975 c 0.5035248257 5.05821991 transit 0.951 +0.198
−0.144
4883 +146
−132
[48]
Kepler-1052 c 0.2112591764 180.9259949 transit 0.937 +0.09
−0.121
5818 +139
−157
[48]
Kepler-1126 c 0.1500582511 199.6679993 transit 0.794 +0.071
−0.03
5678 +113
−102
[48]
Kepler-1162 c 0.1675442283 59.28409958 transit 0.861 +0.05
−0.041
5225 +83
−73
[48]
Kepler-1181 c 0.1555895228 8.934909821 transit 1.336 ±0.2 6688 +187
−281
[48]
Kepler-1471 c 0.2001966118 11.60449982 transit 0.934 +0.063
−0.045
5533 +83
−74
[48]
Kepler-1487 c 0.7992697886 35.79949951 transit 1.801 +0.193
−0.359
5745 +86
−77
[48]
Kepler-1491 c 0.2788835142 61.5685997 transit 0.991 +0.079
−0.065
5626 ±77 [48]
Kepler-1513 c 0.266 +0.098
−0.063
841.4+8.1
−5.3
transit 0.943 ±0.037 5491 ±100 [49]
Kepler-1518 c 0.212775814 9.630929947 transit 1.06 +0.177
−0.133
6432+155
−214
[48]
Kepler-1610 c 0.196806485 44.98529816 transit 0.825 +0.096
−0.078
5295 ±185 [48]
Kepler-1669 d 0.1427426870 4.729469776 transit 0.609 ±0.033 4224 ±84 [48]
Kepler-1801 c 0.3621203501 116.5849991 transit 0.936 +0.114
−0.093
5738 +156
−173
[48]
Kepler-1814 c 0.1476494621 0.626281977 transit 0.79 +0.073
−0.064
4922 ±169 [48]
Kepler-1834 c 0.129895841 0.766691983 transit 0.765 +0.051
−0.028
4821 ±76 [48]
Kepler-1859 c 0.1531807444 3.596430063 transit 1.09 +0.07
−0.078
5887 +70
−79
[48]
Kepler-1894 c 0.1417613278 5.053750038 transit 0.999 +0.114
−0.125
5772 +156
−173
[48]
Kepler-1921 c 0.1505043216 3.157219887 transit 1.251 +0.19
−0.233
6120 +195
−217
[48]
Kepler-1976 b 1.043 4.96 transit 1.097 +0.21
−0.135
6117 +156
−210
[50]
Kepler-1977 b 0.1625482348 4.537000179 transit 0.769 +0.053
−0.079
4805 ±144 [48]
Kepler-1978 b 0.2683562384 10.849699997 transit 0.869 +0.06
−0.095
5251 ±158 [48]
Kepler-1980 b 0.2538143392 33.0257988 transit 1.049 +0.059
−0.073
5819 +69
−87
[48]
Kepler-1981 b 0.8396838173 453.5429993 transit 1.519 +0.15
−0.376
5874 +87
−79
[48]
Kepler-1982 b 0.773130047 3.823159933 transit 1.213 +0.076
−0.093
6202 +99
−149
[48]
Kepler-1983 b 0.1465788952 7.328519821 transit 0.812 +0.058
−0.029
5135 +84
−75
[48]
Kepler-1984 b 0.718709408 1.99285996 transit 0.42 +0.046
−0.056
3638 +72
−87
[48]
Kepler-1985 b 0.1981446855 3.420650005 transit 0.877 +0.064
−0.037
3638 +72
−87
[48]
Kepler-1986 b 0.2631818295 19.54929924 transit 0.776 +0.089
−0.065
5549 ±163 [48]
Kepler-1987 b 0.134713408 2.345860004 transit 0.799 +0.041
−0.081
4769 ±172 [48]
Kepler-1987 c 0.151307244 3.648269892 transit 0.799 +0.041
−0.081
4769 ±172 [48]
Kepler-1987 d 0.2912843007 5.644889832 transit 0.799 +0.041
−0.081
4769 ±172 [48]
Kepler-1987 e 0.2188423849 8.742970467 transit 0.799 +0.041
−0.081
4769 ±172 [48]
Kepler-1988 b 0.1382819717 1.549999952 transit 1.127 +0.189
−0.172
6033 ±183 [48]
Kepler-1989 b 0.4247487156 10.16100025 transit 0.999 +0.153
−0.126
6032 +189
−232
[48]
Kepler-1990 b 0.3491842959 1.735129952 transit 1.028 +0.074
−0.067
5751 +103
−114
[48]
Kepler-1990 c 0.1058972326 1.187000036 transit 1.028 +0.074
−0.067
5751 +103
−114
[48]
Kepler-1991 b 0.1646893688 13.26080036 transit 0.914 +0.061
−0.042
5478 +82
−74
[48]
Kepler-1991 c 0.2594348291 22.79019928 transit 0.914 +0.061
−0.042
5478 +82
−74
[48]
Kepler-1992 b 0.0916229564 15.61120033 transit 0.874 +0.048
−0.054
5383 ±107 [48]
Kepler-1993 b 0.3949511704 26.65660095 transit 1.373 +0.205
−0.512
5159 +171
−155
[48]
Kepler-1994 b 0.0555001398 4.612319946 transit 0.932 +0.052
−0.047
5495 +74
−82
[48]
Kepler-1995 b 0.4119018693 73.75779724 transit 0.847 +0.068
−0.049
5029 +192
−174
[48]
Kepler-1996 b 0.204657316 32.37609863 transit 0.748 +0.027
−0.043
4580 ±92 [48]
Kepler-1996 c 0.2509594797 92.72949982 transit 0.748 +0.027
−0.043
4580 ±92 [48]
Kepler-1997 b 0.2179502440 26.75749969 transit 1.111 ±0.153 6215 +194
−259
[48]
Kepler-1998 b 0.0619324805 3.03263998 transit 0.962 +0.054
−0.068
5640 +101
−113
[48]
Kepler-1999 b 0.3169779722 8.739450455 transit 0.632 +0.063
−0.057
4406 +154
−170
[48]
Kepler-2000 b 0.2961910652 6.383150101 transit 0.581 ±0.029 3757 +74
−82
[48]
Kepler-2000 c 0.1963604037 20.6182003 transit 0.581 ±0.029 3757 +74
−82
[48]
Kepler-2001 b 0.1062540847 1.190999985 transit 0.864 +0.049
−0.085
5081 +166
−136
[48]
Kepler-2001 c 0.3639938397 14.09449959 transit 0.864 +0.049
−0.085
5081 +166
−136
[48]
KMT-2016-BLG-0625L b 0.05 ±0.04 1.40 ±0.17 microlensing 21000 ±2000 0.25 ±0.14 [51]
KMT-2016-BLG-1105L b 0.00415 ±0.00176 2.26+0.51
−0.69
microlensing 10665+4175
−3751
0.43 ±0.18 [52]
KMT-2016-BLG-1751L b 1.20 ±1.21 1.39 ±0.50 microlensing 23000 ±4000 0.18 ±0.18 [51]
KMT-2017-BLG-0428L b 0.0175+0.0111
−0.0088
1.85+0.55
−0.60
microlensing 17612+5936
−8480
0.34+0.22
−0.17
[52]
KMT-2017-BLG-1003L b 0.0117+0.0117
−0.0057
1.25+0.27
−0.25
microlensing 23353+1990
−2120
0.27+0.26
−0.13
[52]
KMT-2017-BLG-1194L b 0.0111+0.0061
−0.0051
1.78+0.45
−0.46
microlensing 13829+7045
−5577
0.41+0.23
−0.19
[52]
KMT-2019-BLG-0298L b 1.81 ±0.96 5.67 ±2.70 microlensing 22000 ±5000 0.70 ±0.37 [53]
KMT-2019-BLG-1216L b 0.094 ±0.050 2.44 ±1.12 microlensing 9000 ±3000 0.39 ±0.21 [53]
KMT-2019-BLG-1367L b 0.0128+0.0081
−0.0065
1.70+0.50
−0.56
microlensing 15231+7990
−6849
0.25+0.16
−0.13
[52]
KMT-2019-BLG-1806L b 0.0147 ±0.0048 2.87+0.64
−0.66
microlensing 21592+2348
−6295
0.75+0.24
−0.25
[52]
KMT-2019-BLG-2783L b 1.16 ±0.77 1.85 ±0.93 microlensing 19000 ±5000 0.34 ±0.25 [53]
KMT-2021-BLG-0712L b 0.1255+0.0648
−0.0374
2.29+0.64
−0.42
microlensing 10437+2968
−2188
0.23+0.12
−0.07
[54]
KMT-2021-BLG-0909L b 1.26+1.01
−0.66
1.75 ±0.42 microlensing 21134+3262
−4501
0.38+0.30
−0.20
[54]
KMT-2021-BLG-1105L b 1.30 ±0.68 3.54 ±1.06 microlensing 14807 ±5447 0.63 ±0.33 [54]
KMT-2021-BLG-2010 b 1.07+1.15
−0.68
1.79+0.30
−0.38
microlensing 23000+4000
−5000
0.37+0.4
−0.23
Multiple orbital solutions[55]
KMT-2021-BLG-2478L b 0.900+0.420
−0.240
1.85 ±0.31 microlensing 9687 ±2348 0.20+0.10
−0.05
[54]
KMT-2022-BLG-0371 b 0.26+0.13
−0.11
3.02+0.45
−0.56
microlensing 23000+3000
−4000
0.63+0.32
−0.28
Multiple orbital solutions[55]
KMT-2022-BLG-0440L b 0.0485+0.0302
−0.0233
1.9 ±0.7 microlensing 11000 ±5000 0.53+0.31
−0.26
[56][57]
KMT-2022-BLG-1013 b 0.31+0.46
−0.16
1.38+0.18
−0.20
microlensing 25000 ±3000 0.18+0.28
−0.10
[55]
L 363-38 b 0.0147 ±0.0014 8.781 ±0.006 0.048 ±0.006 330 radial vel. 33.372 ±0.014 0.210 ±77 3129 ±6 [58]
LHS 3154 b 0.0414 ±0.0026 3.71778+0.00080
−0.00081
0.02262 ±0.00018 radial vel. 51.43 ±0.03 0.1118 ±0.0027 2861 ±77 [59]
LHS 475 b 0.002876 ±0.000588 0.0883 ±0.0045 2.029088 ±0.000006 0.0206 586.0 transit 40.704 0.262 3312.0 [60][61] Host star also known as TOI-910[62] Also the first exoplanet confirmed by the James Webb Space Telescope.[63]
LP 791-18 d 0.0028 +0.0016
−0.0013
0.09207+0.00393
−0.00384
2.753436 ±0.000013 0.01992 ±0.00024 395.5+2.6
−2.3
transit 86.4077+0.20874
−0.20809
0.139 ±0.005 2960 ±55 [64]
MOA-2016-BLG-0532L b 0.39 ±0.31 1.09 ±0.17 microlensing 24000 ±2000 0.09 ±0.07 [51]
MOA-2020-BLG-208L b 0.14+0.13
−0.08
2.74+0.43
−0.47
microlensing 24400 +3200
−3700
0.43 +0.39
−0.23
[65]
MOA-2022-BLG-249Lb 0.015 ±0.005 1.63 ±0.35 microlensing 6500 ±1400 0.18 ±0.05 [66]
MWC 758 c 100 500 ±100 imaging 159.537 +1.742
−1.706
1.5 [67]
OGLE-2016-BLG-1635L b 11.49 ±7.96 1.34 ±0.47 microlensing 22000 ±5000 0.43 ±0.29 [51]
OGLE-2016-BLG-1850L b 0.03 ±0.01 1.46 ±0.16 microlensing 7000 ±2000 0.26 ±0.11 [51]
OGLE-2017-BLG-1806L b 0.0166 +0.0148
−0.0086
1.75+0.46
−0.47
microlensing 20870+2510
−4920
0.38+0.34
−0.20
[52]
OGLE-2019-BLG-0249L b 7.12 ±1.47 1.84 ±0.44 microlensing 21000 ±3000 0.91 ±0.19 [53]
OGLE-2019-BLG-0679L b 3.34 ±1.90 6.99 ±3.21 microlensing 18000 ±6000 0.66 ±0.38 [53]
Rho Coronae Borealis d 0.0680 ±0.0079 282.2+2.2
−3.7
0.827 ±0.011 radial vel. 56.7901+0.0786
−0.0783
0.95 ±0.01 5817 ±24 [68]
Rho Coronae Borealis e 0.0119+0.0017
−0.0017
12.949 ±0.014 0.1061 ±0.0011 radial vel. 56.7901+0.0786
−0.0783
0.95 ±0.01 5817 ±24 [68]
TIC 279401253 b 6.14+0.39
−0.42
1.00 ±0.04 76.80 ±0.06 0.369 ±0.003 transit 937 ±6 1.13+0.02
−0.03
5951 ±80 [69]
TIC 279401253 c 8.02 ±0.18 155.3 ±0.7 0.591+0.005
−0.006
radial vel. 937 ±6 1.13+0.02
−0.03
5951 ±80 [69]
TIC 365102760 b 0.06 0.55 4.21285 0.0622 ±0.0049 transit 1810 ±20 1.21+0.06
−0.05
4694+27
−20
Still have an atmosphere despite high temperatures and low mass[70]
TOI-139 b 0.0208 0.219+0.019
−0.011
11.070850+0.000024
−0.000030
561.17 transit 138.4 0.6900 ±0.0852 4570 ±50 [71]
TOI-181 b 0.1452+0.0085
−0.0240
0.6339+0.0079
−0.0092
4.532000 ±0.000002 0.0539+0.0043
−0.0036
895.10+32.14
−33.86
transit 313.873+1.886
−1.864
0.822 ±0.040 4994 ±50 [72]
TOI-198 b 0.128 ±0.007 10.21520 ±0.00006 0.100 ±0.006 368 ±26 transit 77.38461 ±0.08659 0.467 ±0.023 3650 ±75 [73]
TOI-199 b 0.17 ±0.02 0.810 ±0.005 104.854+0.001
−0.002
0.4254 ±0.0020 transit 333.561+0.623
−0.620
0.936+0.003
−0.005
5255+12
−10
[74]
TOI-199 c 0.28+0.02
−0.01
273.69+0.26
−0.22
0.807 ±0.003 transit 333.561+0.623
−0.620
0.936+0.003
−0.005
5255+12
−10
[74]
TOI-238 b 0.0107+0.00145
−0.00142
0.1278+0.00765
−0.00784
1.2730988 ±0.0000029 0.02118 ±0.00038 1311 ±28 transit 261.328 ±0.312 0.79 ±0.022 5059 ±89 [75]
TOI-244 b 0.00843 ±0.00094 0.136 ±0.011 7.397225+0.000026
−0.000023
0.0559 ±0.0013 458 ±20 transit 71.8644+0.0334
−0.0333
0.428 ±0.029 3433 ±100 [76]
TOI-262 b 0.185 ±0.013 11.14529 ±0.00003 0.163 ±0.002 584 ±45 transit 143.287+0.383
−0.381
0.913 ±0.029 5310 ±124 [73]
TOI-277 b 0.0308 0.276+0.026
−0.013
3.994086+0.000008
−0.000009
739.9 transit 211.7 0.5204 ±0.0203 3748 ±64 [71]
TOI-332 b 0.180 ±0.005 0.285+0.014
−0.010
0.777038 ±0.000001 0.0159 ±0.0001 1871+30
−25
transit 726.847+12.231
−11.836
0.88 ±0.02 5251 ±71 [77]
TOI-444 b 0.247 ±0.018 17.96360 ±0.00004 0.133 ±0.006 609 ±61 transit 187.205+0.270
−0.269
0.960 ±0.130 5225 ±70 [73]
TOI-470 b 0.387 ±0.026 12.19148 ±0.00003 0.119 ±0.008 660 ±70 transit 425.50+1.31
−1.30
0.87 ±0.09 5190 ±90 [73]
TOI-615 b 0.435+0.086
−0.082
1.693+0.052
−0.057
4.6615983+0.0000025
−0.0000016
0.0678+0.0031
−0.0026
1666 ±24 transit 1155 ±6 1.449 ±0.087 6850 ±100 [78]
TOI-622 b 0.303+0.069
−0.072
0.824+0.028
−0.029
6.402513+0.000031
−0.000054
0.0708+0.0052
−0.0059
1388 ±22 transit 400.2 ±0.6 1.313 ±0.079 6400 ±100 [78]
TOI-669 b 0.0308±0.0047 0.232±0.015 3.94515±0.00002 0.047±0.001 1235±37 transit 465.970+2.789
−2.759
0.90±0.06 5600±110 [23]
TOI-672 b 0.0760 0.470+0.008
−0.009
3.633575 ±0.000001 676.15 transit 0.5399 ±0.0204 3765 ±65 [71]
TOI-700 e 0.0025730809[79] 0.08502+0.00794
−0.00669
27.80978+0.00046
−0.0004
0.134 ±0.0022 350[80] transit 101.52 0.416 ±0.01 3480 ±135 Habitable zone planet[81][82]
TOI-715 b 0.1383 ±0.0057 19.288004+0.000027
−0.000024
0.0830 ±0.0027 234 ±12 transit 138.306+0.280
−0.279
0.240 ±0.012 3075 ±75 [83]
TOI-733 b 0.0180 ±0.0022 0.178 ±0.008 4.884765+0.000019
−0.000024
0.0618+0.0036
−0.0039
1055.8+36.2
−31.3
transit 245.5 ±0.2 0.956+0.050
−0.026
5585 ±60 [84]
TOI-771 b 0.00881+0.00629
−0.00283
0.127+0.00964
−0.00767
2.326021 ±0.000001 0.0207 ±0.0008 527.19 ±22.08 transit 82.452 ±0.130 0.220+0.024
−0.023
3201+100
−95
[75]
TOI-778 b 2.8 ±0.2 1.37 ±0.04 4.633611 ±0.000001 0.060 ±0.003 1561+33
−32
transit 527.536+3.663
−3.614
1.40 ±0.05 6643 ±150 [85]
TOI-784 b 0.03043+0.00261
−0.00258
0.172+0.010
−0.008
2.7970365+0.0000031
−0.0000030
0.038 ±0.001 transit 210.696+0.360
−0.359
0.910 ±0.100 5558 ±100 Also known as HD 307842.[86]
TOI-836 b 0.0143+0.0029
−0.0027
0.1520 ±0.0060 3.81673 ±0.00001 0.04220 ±0.00093 871 ±36 transit 89.7009+0.0959
−0.0956
0.665 ±0.010 4552 ±154 [87]
TOI-836 c 0.0302+0.0085
−0.0027
0.2308 ±0.0079 8.59545 ±0.00001 0.0750 ±0.0016 665 ±27 transit 89.7009+0.0959
−0.0956
0.665 ±0.010 4552 ±154 [87]
TOI-858B b 1.10+0.08
−0.07
1.255 ±0.039 3.2797178 ±0.0000014 0.04435+0.00100
−0.00098
1529+23
−22
transit 816.987+4.951
−4.892
1.081+0.076
−0.070
5842+84
−79
[88]
TOI-871 b 0.0120+0.00849
−0.00440
0.148+0.0102
−0.0101
14.362565 ±0.00009 0.1054 ±0.0021 621 ±16.05 transit 221.917 ±0.489 0.758+0.046
−0.044
4929+80
−75
[75]
TOI-908 b 0.050773+0.012938
−0.012708
0.2842 ±0.0138 3.183792 ±0.000007 0.041657 ±0.000002 1317 ±38 transit 573.214+0.638
−0.634
0.950 ±0.010 5626 ±61 [89]
TOI-913 b 0.0208 0.219+0.011
−0.009
11.098644+0.000587
−0.000581
712.01 transit 212.1 0.8200 ±0.0973 4969 ±129 [71]
TOI-1052 b 0.0532 ±0.0053 0.256+0.026
−0.021
9.139703+0.00062
−0.00063
0.09103+0.00062
−0.00063
1135 transit 423.365+1.826
−1.810
1.204 ±0.025 6146 ±62 [90]
TOI-1052 c 0.108+0.013
−0.012
35.806+0.453
−0.381
0.2263+0.0024
−0.0023
719 radial vel. 423.365+1.826
−1.810
1.204 ±0.025 6146 ±62 [90]
TOI-1194 b 0.456+0.055
−0.051
0.767+0.045
−0.041
2.310644 ±0.000001 0.03428 ±0.00055 1391+38
−37
transit 488.149+2.136
−2.117
1.007+0.050
−0.048
5446+51
−48
[91]
TOI-1221 b <3.5 0.260+0.012
−0.011
91.68278+0.00032
−0.00041
0.387+0.026
−0.023
440 ±60 transit 451.437+1.262
−1.259
0.930 ±0.220 5592 ±50 [92]
TOI-1338 c 0.205 ±0.037 215.5 ±3.3 0.794 ±0.016 radial vel. 1318 ±5 1.13+0.31 6160 Circumbinary planet[93]
TOI-1408 b 1.69 ±0.20 1.5 4.4247110 ±0.0000016 0.05804 ±0.00020 transit 454.937+1.363
−1.360
1.331 ±0.014 6306 ±32 [94]
TOI-1410 b 0.0334 0.290+0.014
−0.010
1.216901 ±0.000038 1181.44 transit 236.8 0.7960 ±0.0370 4668 ±50 [71]
TOI-1416 b 0.0109 ±0.0015 0.145 ±0.007 1.0697568 ±0.0000028 0.0190 ±0.0003 1517 ±39 transit 179.430+0.253
−0.252
0.798+0.035
−0.044
4884 ±70 [95]
TOI-1420 b 0.0790 ±0.0120 1.061 ±0.029 6.9561063 ±0.0000017 0.0710 ±0.0012 957 ±17 transit 658.569+0.918
−0.911
0.9870 ±0.0480 5510 ±110 [96]
TOI-1467 b 0.0138+0.0101
−0.00535
0.164+0.0142
−0.0139
5.971143 ±0.000006 0.0510 ±0.0009 558.89 ±16.37 transit 122.113 ±0.196 0.498+0.026
−0.025
3810+73
−78
[75]
TOI-1470 b 0.0230+0.0038
−0.0039
0.194 ±0.004 2.527093+0.000004
−0.000003
0.0285 ±0.0004 734 transit 169.439 ±0.243 0.471 ±0.011 3709 ±11 [97]
TOI-1470 c 0.02278+0.00903
−0.00872
0.220 ±0.002 18.08816+0.00006
−0.00008
0.106 ±0.001 373 transit 169.439 ±0.243 0.471 ±0.011 3709 ±11 [97]
TOI-1669 b 0.573 ±0.074 502 ±16 radial vel. 362.934+1.210
−1.200
1.00 ±0.05 5542.3 ±100.0 [98]
TOI-1680 b 0.0100 +0.0035
−0.0022
0.131 +0.00562
−0.00437
4.8026345+0.0000040
−0.0000039
0.03144+0.00025
−0.00026
404 ±14 transit 121.1 1.1798 ±0.0044 3225+99
−100
super-Earth planet[99]
TOI-1694 b 0.0809 0.487+0.042
−0.071
3.770179+0.000058
−0.000060
1136.57 transit 405.7 0.8450 ±0.1089 5135 ±50 [71]
TOI-1694 c 1.05 ±0.05 389.2 ±3.9 radial vel. 405.7 0.8450 ±0.1089 5135 ±50 [100]
TOI-1736 b 0.040 ±0.016 0.223 ±0.016 7.073088 ±0.000007 0.0740 ±0.0009 1076 ±39 transit 290.111+1.050
−1.043
1.08 ±0.04 5807 ±46 [101]
TOI-1736 c 8.70+1.50
−0.60
570.1 ±0.7 1.381 ±0.017 249 ±9 radial vel. 290.111+1.050
−1.043
1.08 ±0.04 5807 ±46 [101]
TOI-1739 b 0.0126+0.00849
−0.00472
0.151+0.00874
−0.00758
8.303342+0.000011
−0.000013
0.0742 ±0.0014 755.55 ±20.19 transit 231.506 ±0.522 0.790+0.046
−0.045
4922+94
−91
[75]
TOI-1801 b 0.0158 0.187+0.005
−0.006
10.643976+0.000014
−0.000014
490.47 transit 100.8 0.5413 ±0.0204 3815 ±157 [71]
TOI-1811 b 0.9720+0.0760
−0.0780
0.9940+0.0250
−0.0230
3.7130765 ±0.0000017 0.04389+0.00058
−0.00055
962.2+8.0
−7.9
transit 418.231+2.319
−2.296
0.817+0.033
−0.030
4766+52
−54
[102]
TOI-1853 b 0.0406 0.325+0.020
−0.016
1.243702+0.000121
−0.000114
1510.96 transit 539 ±3 0.8200 ±0.0992 5175 ±50 [71]
TOI-1859 b 0.87 ±0.07 63.48347 ±0.00010 0.337+0.044
−0.036
transit 731.847+3.826
−3.787
1.287 ±0.061 6341+68
−70
[103]
TOI-1937A b 2.01+0.17
−0.16
1.247+0.059
−0.062
0.946679944 ±0.00000047 0.01932+0.00035
−0.00039
2097+35
−36
transit 1353.99+9.55
−9.42
1.072+0.059
−0.064
5814+91
−93
[104]
TOI-2000 b 0.0347+0.0077
−0.0075
0.241 ±0.014 3.098330+0.000021
−0.000019
0.04271+0.00076
−0.00067
1488+122
−160
transit 30.3424 ±0.0685 1.082+0.059
−0.050
5611+85
−82
[105]
TOI-2000 c 0.0257+0.015
−0.014
0.727+0.028
−0.027
9.1270550+0.0000073
−0.0000072
0.0878+0.0016
−0.0014
1038+84
−111
transit 30.3424 ±0.0685 1.082+0.059
−0.050
5611+85
−82
[105]
TOI-2010 b 1.286+0.055
−0.057
1.054 ±0.027 141.834025+0.000065
−0.000066
0.5516+0.0078
−0.0093
400.2+5.6
−5.7
transit 356.131+1.050
−1.044
1.112+0.048
−0.055
5929 ±74 [106]
TOI-2015 b 0.0516±0.0129 0.302±0.012 3.348968±0.000004 0.0301+0.0013
−0.0012
512±11 transit 154.34+0.13
−0.10
0.342+0.021
−0.025
3194±56 [107]
TOI-2018 b 0.0185 0.204+0.009
−0.007
7.435588 ±0.000009 652.44 transit 0.6600 ±0.0868 4348 ±100 [71]
TOI-2068 b 0.0138+0.0101
−0.00503
0.162+0.0145
−0.0133
7.768915+0.000025
−0.000037
0.0632 ±0.0011 520.62 ±14.18 transit 172.635+0.294
−0.261
0.559+0.027
−0.029
3710+57
−58
[75]
TOI-2084 b 0.220 ±0.012 6.0784247 ±0.0000096 0.05006 ±0.00103 527 ±8 transit 373.609+1.115
−1.106
0.453+0.029
−0.027
3551+49
−52
[108]
TOI-2095 b 0.116 ±0.009 17.664872+0.000045
−0.000051
0.1010+0.0088
−0.0084
347 ±9 transit 136.73 ±0.08 0.465 ±0.012 3662 ±130 [109][110]
TOI-2095 c 0.124+0.010
−0.009
28.17221+0.00011
−0.00014
0.138+0.012
−0.011
297 ±8 transit 136.73 ±0.08 0.465 ±0.012 3662 ±130 [109][110]
TOI-2096 b 0.0060+0.0044
−0.0019
0.110 ±0.006 3.1190633+0.000010
−0.0000093
0.025 ±0.001 445 ±13 transit 158.08 ±0.13 0.231 ±0.012 3300 ±50 [111]
TOI-2096 c 0.0145+0.0110
−0.0057
0.171 ±0.008 6.387840 ±0.000012 0.040 ±0.002 349+10
−9
transit 158.08 ±0.13 0.231 ±0.012 3300 ±50 [111]
TOI-2134 b 0.0287+0.0025
−0.0024
0.240 ±0.014 9.2292005 ±0.0000063 0.0780 ±0.0009 666 ±8 transit 73.7773+0.0522
−0.0519
0.744 ±0.027 4580 ±50 [71][112]
TOI-2134 c 0.1318+0.0242
−0.0246
0.649 ±0.037 95.50+0.36
−0.25
0.371 ±0.004 306 ±4 transit 73.7773+0.0522
−0.0519
0.744 ±0.027 4580 ±50 [112]
TOI-2141 b 0.075 ±0.012 0.278 ±0.021 18.26157 ±0.00006 0.1330 ±0.0009 722 ±23 transit 253.365+0.736
−0.732
0.94 ±0.02 5659 ±48 [101]
TOI-2152A b 2.83+0.38
−0.37
1.281+0.050
−0.046
3.3773512+0.0000060
−0.0000061
0.05064+0.00093
−0.00110
1802+60
−54
transit 988.275+10.143
−9.945
1.516+0.085
−0.100
6630+300
−200
[102]
TOI-2154 b 0.920+0.190
−0.180
1.453+0.053
−0.048
3.8240801 ±0.0000025 0.0513+0.0011
−0.0013
1580 ±27 transit 966.924+2.174
−2.143
1.233+0.077
−0.090
6280 ±160 [102]
TOI-2194 b 0.0145 0.178+0.012
−0.006
15.337597+0.001585
−0.001616
590.88 transit 63.84 ±0.12 0.7400 ±0.0854 4756 ±50 [71]
TOI-2338 b 5.98+0.21
−0.20
1.00 ±0.02 22.65398 ±0.00002 0.158 ±0.03 799+10
−11
transit 1032 ±7 0.99+0.03
−0.02
5581 ±60 [113]
TOI-2364 b 0.225+0.043
−0.049
0.768+0.023
−0.018
4.0197517 ±0.0000043 0.04871+0.00069
−0.00079
1091+17
−14
transit 716.286+5.594
−5.509
0.954+0.041
−0.046
5306+76
−68
[104]
TOI-2443 b 0.0256 0.248 ±0.004 15.669494+0.000926
−0.001004
600.83 transit 0.6600 ±0.0789 4357 ±100 [71]
TOI-2459 b 0.0285 0.264+0.008
−0.006
19.104718+0.000023
−0.000024
445.01 transit 0.6600 ±0.0763 4195 ±124 [71]
TOI-2497 b 4.82 ±0.41 0.9940+0.0550
−0.0490
10.655669 ±0.000038 0.1166 ±0.0018 1595+45
−42
transit 930.489+11.624
−11.347
1.859+0.087
−0.083
7360+320
−300
[102]
TOI-2498 b 0.1089+0.0129
−0.0129
0.541+0.026
−0.024
3.738252 ±0.000004 0.0491 ±0.0030 1443+15
−28
transit 897.796+13.712
−13.314
1.12 ±0.02 5905 ±12 [114]
TOI-2525 b 0.088+0.005
−0.004
0.774 ±0.010 23.288+0.001
−0.002
0.1511 ±0.0025 500 transit 1305 ±8 0.849+0.024
−0.033
5096 ±80 [115]
TOI-2525 c 0.709 ±0.034 0.904 ±0.010 49.260 ±0.001 0.2491+0.0041
−0.0042
390 transit 1305 ±8 0.849+0.024
−0.033
5096 ±80 [115]
TOI-2583A b 0.250+0.058
−0.056
1.290+0.040
−0.033
4.5207265 ±0.0000049 0.0571+0.0010
−0.0013
1456+19
−16
transit 1846.66+21.10
−20.64
1.215+0.063
−0.082
5936+65
−68
[104]
TOI-2587A b 0.218+0.054
−0.046
1.077+0.042
−0.040
5.456640 ±0.000011 0.0635+0.0025
−0.0013
1445+23
−26
transit 1218.77+5.953
−5.772
1.15+0.14
−0.07
5760+80
−79
[104]
TOI-2589 b 3.5 ±0.1 1.08 ±0.03 61.6277 ±0.0002 0.300+0.006
−0.005
592+7
−8
transit 658 ±3 0.93+0.03
−0.02
5579 ±70 [113]
TOI-2641 b 0.367+0.049
−0.040
1.615+0.462
−0.640
4.880974+0.000023
−0.000037
0.0607+0.0042
−0.0043
1387+22
−23
transit 1131 ±7 1.16 ±0.07 6100 ±100 Extremely grazing transit[78]
TOI-2796 b 0.44+0.10
−0.11
>1.54 4.8084983+0.0000057
−0.0000056
0.0569+0.0010
−0.0011
1205+18
−17
transit 1142.67+19.63
−18.99
1.063+0.057
−0.062
5764+81
−78
[104]
TOI-2803A b 0.9750+0.0830
−0.0700
1.616+0.034
−0.032
1.96229325 ±0.00000082 0.03185 ±0.00052 1893+29
−28
transit 1613.88+21.68
−21.13
1.118+0.056
−0.054
6280+99
−96
[104]
TOI-2818 b 0.71 ±0.26 1.363+0.046
−0.045
4.0397090+0.0000024
−0.0000023
0.0493+0.0010
−0.0008
1376+26
−24
transit 1019.81+7.39
−7.28
0.9770+0.0630
−0.0490
5721+88
−83
[104]
TOI-2842 b 0.370+0.052
−0.047
1.146+0.051
−0.048
3.5514058+0.0000077
−0.0000078
0.0475+0.0010
−0.0011
1471+29
−27
transit 1503.57+25.18
−24.37
1.135+0.077
−0.079
5910 ±100 [104]
TOI-2977 b 1.68+0.26
−0.25
1.174+0.031
−0.027
2.3505614 ±0.0000025 0.03386+0.00067
−0.00050
1544 ±26 transit 0.936+0.057
−0.041
5691+94
−93
[104]
TOI-3023 b 0.62+0.10
−0.09
1.466+0.043
−0.032
3.9014971 ±0.0000031 0.0505+0.0015
−0.0009
1596+24
−25
transit 1271.74+10.42
−10.26
1.12+0.11
−0.06
5760+85
−88
[104]
TOI-3082 b 0.0411 0.327 ±0.013 1.926907+0.000128
−0.000134
1032.78 transit 368.8 ±1.5 0.6640 ±0.0798 4263 ±100 [71]
TOI-3235 b 0.665 ±0.025 1.017 ±0.044 2.59261842 ±0.00000041 0.02709 ±0.00046 604 ±19 transit 236.7 ±0.5 0.394 ±0.003 3389 ±6 [116]
TOI-3364 b 1.67+0.12
−0.13
1.091+0.038
−0.032
5.8768918 ±0.0000069 0.0675+0.0011
−0.0016
1264+22
−21
transit 906.386+8.170
−8.027
1.186+0.059
−0.083
5706+95
−91
[104]
TOI-3688A b 0.980+0.100
−0.110
1.167+0.048
−0.044
3.246075 ±0.000012 0.04560+0.00089
−0.00098
1534+29
−28
transit 1292.81+19.67
−19.10
1.199+0.072
−0.076
5950 ±100 [104]
TOI-3785 b 0.0470 ±0.0126 0.459 ±0.014 4.6747373 ±0.0000038 0.043 ±0.001 582 ±16 transit 259.0 ±0.3 0.52 ±0.02 3576 ±88 [117]
TOI-3807 b 1.04+0.15
−0.14
>1.65 2.8989727+0.0000038
−0.0000039
0.0421+0.0007
−0.0011
1646+25
−24
transit 1375.55+15.20
−14.88
1.181+0.0064
−0.0092
5772+84
−80
[104]
TOI-3819 b 1.11+0.18
−0.20
1.172+0.036
−0.035
3.2443141 ±0.0000055 0.04611+0.00069
−0.00096
1633+21
−19
transit 1820.41+42.55
−40.68
1.242+0.057
−0.076
5859+72
−71
[104]
TOI-3912 b 0.406+0.071
−0.068
1.274+0.041
−0.040
3.4936264 ±0.0000038 0.0463+0.0012
−0.0010
1512 ±20 transit 1519.86+21.48
−20.90
1.088+0.086
−0.070
5725+69
−68
[104]
TOI-3976A b 0.175+0.037
−0.036
1.095+0.036
−0.035
6.607662+0.000016
−0.000015
0.0743+0.0013
−0.0014
1295+16
−14
transit 1683.25+19.30
−18.88
1.254+0.067
−0.072
5975+70
−69
[104]
TOI-3984A b 0.14 ±0.03 0.71 ±0.02 4.35326 ±0.000005 0.041+0.002
−0.001
563 ±15 transit 353.6+1.0
−0.7
0.49 ±0.02 3476 ±88 [118]
TOI-4010 b 0.03461+0.00406
−0.00400
0.269 ±0.007 1.348335+0.000003
−0.000002
0.0229 ±0.0002 1441+14
−13
transit 578.941+3.242
−3.203
0.88 ±0.03 4960 ±36 [119]
TOI-4010 c 0.06390+0.00670
−0.00664
0.529+0.010
−0.011
5.414654 ±0.000007 0.058 ±0.001 907+9
−8
transit 578.941+3.242
−3.203
0.88 ±0.03 4960 ±36 [119]
TOI-4010 d 0.1200+0.0103
−0.0101
0.551+0.012
−0.013
14.70886 ±0.00003 0.113 ±0.001 650 ±6 transit 578.941+3.242
−3.203
0.88 ±0.03 4960 ±36 [119]
TOI-4010 e 2.18+0.21
−0.20
>762 ±90 1.57+0.12
−0.13
174+8
−6
radial vel. 578.941+3.242
−3.203
0.88 ±0.03 4960 ±36 [119]
TOI-4087 b 0.73 ±0.14 1.164+0.025
−0.024
3.17748350 ±0.00000094 0.04469+0.00048
−0.00054
1458+20
−17
transit 983.937+7.257
−7.153
1.178+0.039
−0.042
6060+74
−67
[104]
TOI-4127 b 2.30 ±0.11 1.096+0.039
−0.032
56.39879 ±0.00010 0.3081+0.0055
−0.0058
605.1+9.6
−8.2
transit 1060 ±20 1.23 ±0.07 6096 ±115 Highly eccentric orbit[120]
TOI-4145A b 0.43 ±0.13 1.187+0.032
−0.031
4.0664428 ±0.0000058 0.04823+0.00075
−0.00079
1074+19
−16
transit 669.884+3.904
−3.862
0.905+0.043
−0.044
5281+86
−76
[104]
TOI-4184 b 0.217 ±0.019 4.9019804 ±0.0000052 0.0336 ±0.0015 412 ±8 transit 226.238+1.058
−1.049
0.2109+0.0290
−0.0260
3238+48
−49
[108]
TOI-4201 b 2.589 ±0.066 1.133 ±0.024 3.5819111 ±1.7e-06 0.03939 ±0.0004 745 ±14 transit 611.54+1.96
−2.28
0.63 ±0.02 3920 ±50 [121][122]
TOI-4308 b 0.0203 0.216 ±0.023 9.151201+0.000036
−0.000037
763.05 transit 0.9000 ±0.1133 5243 ±126 [71]
TOI-4342 b 0.16 ±0.16 0.202 ±0.003 5.5382498+0.0000057
−0.0000058
0.05251 ±0.00011 633.6+6.2
−6.3
transit 200.73 0.6296 ±0.0086 3901 ±69 [123]
TOI-4342 c 0.145 ±0.145 0.215 ±0.004 10.688716 ±0.000015 0.08140 ±0.00017 508.9 ±5.0 transit 200.73 0.6296 ±0.0086 3901 ±69 [123]
TOI-4377 b 0.9570+0.0890
−0.0870
1.348 ±0.081 4.378081 ±0.000019 0.0579+0.0010
−0.0011
1395+25
−22
transit 1486.69+16.01
−15.68
1.36+0.08
−0.07
4974 ±57 [124]
TOI-4406 b 0.30 ±0.03 1.00 ±0.02 30.08364 ±0.00005 0.201 ±0.005 904+16
−17
transit 861 ±7 1.19 ±0.03 6219 ±70 [113]
TOI-4463A b 0.794+0.039
−0.040
1.183+0.064
−0.045
2.8807198+0.0000028
−0.0000027
0.04036+0.00074
−0.00082
1395+25
−22
transit 564.633+4.250
−4.191
1.062+0.059
−0.063
5640+89
−82
[104]
TOI-4515 b 2.005 ±0.052 1.086 ±0.039 15.266 0.118 ±0.001 705 ±10 transit 0.949 ±0.020 5433 ±70 [125]Highly eccentric orbit (e = 0.46)
TOI-4551 b 1.49 ±0.13 1.058+0.110
−0.062
9.955810+0.000076
−0.000078
0.09940+0.00300
−0.00320
transit 704.453+8.033
−7.857
1.31+0.07
−0.18
4896 ±110 [124]
TOI-4559 b 0.00849+0.00629
−0.00315
0.126+0.0112
−0.00999
3.965991+0.000314
−0.000332
0.0359 ±0.0008 554.16 ±19.14 transit 90.704 ±0.0978 0.392+0.027
−0.026
3558+73
−83
[75]
TOI-4562 b 2.30+0.48
−0.47
1.118+0.014
−0.013
225.11781+0.00025
−0.00022
0.768 ±0.005 318 ±4 transit 1107.64+8.25
−8.12
1.192 ±0.057 6096 ±32 [126]
TOI-4582 b 0.53 ±0.05 0.940+0.090
−0.120
31.034 ±0.001 transit 1251.94+11.83
−11.62
1.34 ±0.06 5190 ±100 [127]
TOI-4600 b ~0.0976 0.607+0.026
−0.028
82.6869 ±0.0003 0.349 ±0.021 347+12
−11
transit 705.97 ±1.68 0.89 ±0.05 5170 ±120 [128]
TOI-4600 c ~0.1510 0.841 ±0.037 482.8191+0.0018
−0.0017
1.152 ±0.068 191 ±6 transit 705.97 ±1.68 0.89 ±0.05 5170 ±120 As of August 2023, longest-period confirmed planet discovered by TESS[128]
TOI-4603 b 12.89+0.58
−0.57
1.042+0.038
−0.035
7.24599+0.00022
−0.00021
0.0888 ±0.0010 1677 ±24 transit 731 ±3 1.765 ±0.061 6264+95
−94
Metal enriched gas giant[129]
TOI-4791 b 2.31+0.32
−0.33
1.110 ±0.050 4.280880+0.000022
−0.000023
0.0555+0.0011
−0.0012
1472+26
−24
transit 1072.41+12.05
−11.79
1.242+0.072
−0.077
6058+99
−94
[104]
TOI-4860 b 0.67 ±0.14 0.756 ±0.024 1.52275959+0.00000032
−0.00000035
0.01845 ±0.00059 624 ±30 transit 261.390+2.114
−2.081
0.3357 ±0.0081 3390 ±120 [130]
TOI-5126 b 0.423+0.014
−0.012
5.4588385+0.0000070
−0.0000072
0.06519+0.00087
−0.00082
1442+46
−40
transit 523.201+5.264
−5.160
1.240+0.050
−0.046
6150+110
−130
[131]
TOI-5126 c 0.344+0.015
−0.014
17.8999+0.0018
−0.0013
0.1439+0.0019
−0.0018
971.0+31.0
−27.0
transit 523.201+5.264
−5.160
1.240+0.050
−0.046
6150+110
−130
[131]
TOI-5205 b 1.08 ±0.06 1.03 ±0.03 1.630757 ±0.000001 0.0199 ±0.0002 transit 281.960+1.363
−1.350
0.394 ±0.011 3430 ±54 [132]
TOI-5293A b 0.54 ±0.07 1.06 ±0.04 2.930289 ±0.000004 0.034+0.004
−0.003
675+42
−30
transit 525 ±2 0.54 ±0.02 3586 ±88 [118]
TOI-5344 b 0.412 ±0.040 0.946 ±0.021 3.7926220 ±0.0000062 0.04041 ±0.00075 689 ±12 transit 451.293+4.357
−4.276
0.612 ±0.034 3747 ±64 [133]
TOI-5398 c 0.0371+0.0151
−0.0148
0.314 ±0.017 4.77271+0.00016
−0.00014
0.057 ±0.003 1242 ±37 transit 426.792+2.237
−2.211
1.146 ±0.013 6000 ±75 [134]
TOI-5678 b 0.063 ±0.013 0.438 ±0.007 47.73022+0.00014
−0.00013
0.249 ±0.005 513+8
−7
transit 539.441+2.293
−2.277
0.905+0.039
−0.041
5485 ±63 [135]
TOI-5704 b 0.288 3.7711160+0.0000115
−0.0000107
949.07 transit 292.357+0.881
−0.876
0.7575 ±0.0593 4590 ±126 [71]
TOI-5799 b 0.0116+0.00849
−0.00440
0.145+0.0171
−0.0114
4.164753+0.00038
−0.000427
0.0352 ±0.0011 518.01 ±20.15 transit 90.704 ±0.0978 0.337+0.027
−0.032
3514+95
−94
[75]
TOI-5803 b 0.0339 0.292 ±0.011 5.383050+0.000207
−0.000200
678.87 transit 0.8700 ±0.1032 5134 ±121 [71]
WASP-84 c 0.048+0.014
−0.013
0.174 ±0.011 1.4468849+0.0000022
−0.0000016
0.02359 ±0.00100 1329+31
−30
transit 328.075+1.595
−1.579
0.853 ±0.038 [136]
WASP-193 b 0.139 ±0.029 1.464+0.059
−0.057
6.2463345 ±0.0000003 0.0676 ±0.0015 1254 ±31 transit 1180.97+17.56
−17.06
1.059+0.067
−0.068
6078 ±120 [137]
WISE J033605.05-014350.4 b 8.25 ±4.25 2560 ±730 0.970 ±0.050 325+15
−10
imaging 0.01310 ±0.00597 415 ±20 [138]
Wolf 1069 b 0.003963425 ±0.0006605 15.564 ±0.015 0.0672 ±0.0014 250.0 ±6.6 radial vel. 31.228 0.167 ±0.011 3158 ±54 Habitable zone planet[139][140]

Specific exoplanet lists

[edit]

Lists of exoplanets

Lists of exoplanets by year of discovery

[edit]


References

[edit]
  1. ^ Teng, Huan-Yu; Sato, Bun'ei; Kuzuhara, Masayuki; Takarada, Takuya; Omiya, Masashi; Harakawa, Hiroki; Izumiura, Hideyuki; Kambe, Eiji; Yilmaz, Mesut; Bikmaev, Ilfan; Selam, Selim O.; Brandt, Timothy D.; Xiao, Guang-Yao; Yoshida, Michitoshi; Itoh, Yoichi (2023). "Revisiting Planetary Systems in Okayama Planet Search Program: A new long-period planet, RV astrometry joint analysis, and multiplicity-metallicity trend around evolved stars". arXiv:2308.05343 [astro-ph.EP].
  2. ^ Franson, Kyle; Bowler, Brendan P.; Zhou, Yifan; Pearce, Tim D.; Bardalez Gagliuffi, Daniella C.; Biddle, Lauren; Brandt, Timothy D.; Crepp, Justin R.; Dupuy, Trent J.; Faherty, Jacqueline; Jensen-Clem, Rebecca; Morgan, Marvin; Sanghi, Aniket; Theissen, Christopher A.; Tran, Quang H.; Wolf, Trevor A. (February 2023). "Astrometric Accelerations as Dynamical Beacons: A Giant Planet Imaged Inside the Debris Disk of the Young Star AF Lep". The Astrophysical Journal Letters. 950 (2): L19. arXiv:2302.05420. Bibcode:2023ApJ...950L..19F. doi:10.3847/2041-8213/acd6f6. S2CID 256808203.
  3. ^ De Rosa, Robert J.; Nielsen, Eric L.; Wahhaj, Zahed; Ruffio, Jean-Baptise; Kalas, Paul G.; Peck, Anne E.; Hirsch, Lea A.; Roberson, William (February 2023). "Direct imaging discovery of a super-Jovian around the young Sun-like star AF Leporis". Astronomy & Astrophysics. 672: A94. arXiv:2302.06332. Bibcode:2023A&A...672A..94D. doi:10.1051/0004-6361/202345877. S2CID 256827414.
  4. ^ Mesa, D.; Gratton, R.; et al. (February 2023). "AF Lep b: the lowest mass planet detected coupling astrometric and direct imaging data". Astronomy & Astrophysics. 672: A93. arXiv:2302.06213. Bibcode:2023A&A...672A..93M. doi:10.1051/0004-6361/202345865. S2CID 256827302.
  5. ^ Wittrock, Justin M.; Plavchan, Peter P.; Cale, Bryson L.; Barclay, Thomas; Ludwig, Mathis R.; Schwarz, Richard P.; Mékarnia, Djamel; J. Triaud, Amaury H. M.; Abe, Lyu; Suarez, Olga; Guillot, Tristan; Conti, Dennis M.; Collins, Karen A.; Waite, Ian A.; Kielkopf, John F. (1 December 2023). "Validating AU Microscopii d with Transit Timing Variations". The Astronomical Journal. 166 (6): 232. arXiv:2302.04922. Bibcode:2023AJ....166..232W. doi:10.3847/1538-3881/acfda8. ISSN 0004-6256.
  6. ^ "AU Microscopii d - Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Archived from the original on 3 December 2023. Retrieved 3 December 2023.
  7. ^ a b c d e Frensch, Y. G. C.; Curto, G. Lo; Bouchy, F.; Mayor, M.; Hébrard, G.; Lovis, C.; Moutou, C.; Pepe, F. A.; Queloz, D.; Santos, N.; Segransan, D.; Udry, S.; Unger, N. (1 July 2023). "The HARPS search for southern extra-solar planets - XLVII. Five Jupiter-mass planets in long-period orbits, one highly irradiated Neptune, one brown dwarf, and five stellar binaries". Astronomy & Astrophysics. 675: A173. arXiv:2306.04420. Bibcode:2023A&A...675A.173F. doi:10.1051/0004-6361/202346203. ISSN 0004-6361. S2CID 265829649. Archived from the original on 16 December 2023. Retrieved 26 July 2023.
  8. ^ Barnes, J R; Standing, M R; Haswell, C A; Staab, D; Doherty, J P J; Waller-Bridge, M; Fossati, L; Soto, M; Anglada-Escudé, G; Llama, J; McCune, C; Lewis, F W (29 July 2023). "DMPP-4: candidate sub-Neptune mass planets orbiting a naked-eye star". Monthly Notices of the Royal Astronomical Society. 524 (4): 5196–5212. arXiv:2307.07530. doi:10.1093/mnras/stad2109. ISSN 0035-8711. Archived from the original on 26 August 2023. Retrieved 26 August 2023.
  9. ^ Bonomo, A. S.; Dumusque, X.; Massa, A.; Mortier, A.; Bongiolatti, R.; Malavolta, L.; Sozzetti, A.; Buchhave, L. A.; Damasso, M.; Haywood, R. D.; Morbidelli, A.; Latham, D. W.; Molinari, E.; Pepe, F.; Poretti, E. (2023). "Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities". Astronomy & Astrophysics. 677: A33. arXiv:2304.05773. Bibcode:2023A&A...677A..33B. doi:10.1051/0004-6361/202346211. S2CID 258078829.
  10. ^ Pinamonti, M.; Barbato, D.; Sozzetti, A.; Affer, L.; Benatti, S.; Biazzo, K.; Bignamini, A.; Borsa, F.; Damasso, M.; Desidera, S.; Lanza, A. F.; Maldonado, J.; Mancini, L.; Naponiello, L.; Nardiello, D. (2023). "The GAPS programme at TNG". Astronomy & Astrophysics. 677: A122. arXiv:2306.04419. doi:10.1051/0004-6361/202346476. S2CID 259095781.
  11. ^ a b Goffo, Elisa; Gandolfi, Davide; Egger, Jo Ann; Mustill, Alexander J.; Albrecht, Simon H.; Hirano, Teruyuki; Kochukhov, Oleg; Astudillo-Defru, Nicola; Barragan, Oscar; Serrano, Luisa M.; Hatzes, Artie P.; Alibert, Yann; Guenther, Eike; Dai, Fei; Lam, Kristine W. F. (2023). "Company for the ultra-high density, ultra-short period sub-Earth GJ 367 b: discovery of two additional low-mass planets at 11.5 and 34 days". The Astrophysical Journal. 955 (1): L3. arXiv:2307.09181. Bibcode:2023ApJ...955L...3G. doi:10.3847/2041-8213/ace0c7.
  12. ^ a b Palle, E.; Orell-Miquel, J.; et al. (January 2023). "GJ 806 (TOI-4481): A bright nearby multi-planetary system with a transiting hot low-density super-Earth". Astronomy & Astrophysics. 678: A80. arXiv:2301.06873. Bibcode:2023A&A...678A..80P. doi:10.1051/0004-6361/202244261. S2CID 255941564.
  13. ^ "The Extrasolar Planet Encyclopaedia — TOI-4481 b". Extrasolar Planets Encyclopaedia. 23 October 1995. Retrieved 19 January 2023.
  14. ^ "The Extrasolar Planet Encyclopaedia — TOI-4481 c". Extrasolar Planets Encyclopaedia. 23 October 1995. Retrieved 19 January 2023.
  15. ^ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Archived from the original on 9 November 2023. Retrieved 9 November 2023.
  16. ^ Blanco-Pozo, J.; Perger, M.; et al. (March 2023). "The CARMENES search for exoplanets around M dwarfs. A long-period planet around GJ 1151 measured with CARMENES and HARPS-N data". Astronomy & Astrophysics. 671: A50. arXiv:2301.04442. Bibcode:2023A&A...671A..50B. doi:10.1051/0004-6361/202245053. S2CID 265978783.
  17. ^ Mahadevan, Suvrath; et al. (2021). "The Habitable-zone Planet Finder Detects a Terrestrial-mass Planet Candidate Closely Orbiting Gliese 1151: The Likely Source of Coherent Low-frequency Radio Emission from an Inactive Star". The Astrophysical Journal Letters. 919 (1): L9. arXiv:2102.02233. Bibcode:2021ApJ...919L...9M. doi:10.3847/2041-8213/abe2b2. S2CID 231802021.
  18. ^ Perger, M.; et al. (2021). "The CARMENES search for exoplanets around M dwarfs". Astronomy & Astrophysics. 649: L12. arXiv:2103.10216. Bibcode:2021A&A...649L..12P. doi:10.1051/0004-6361/202140786. S2CID 232269942.
  19. ^ Gorrini, P.; Kemmer, J.; Dreizler, S.; Burn, R.; Hirano, T.; Pozuelos, F. J.; Kuzuhara, M.; Caballero, J. A.; Amado, P. J.; Harakawa, H.; Kudo, T.; Quirrenbach, A.; Reiners, A.; Ribas, I.; Béjar, V. J. S. (December 2023). "Planetary companions orbiting the M dwarfs GJ 724 and GJ 3988: A CARMENES and IRD collaboration" (PDF). Astronomy & Astrophysics. 680: A28. arXiv:2310.05599. Bibcode:2023A&A...680A..28G. doi:10.1051/0004-6361/202347108. ISSN 0004-6361.
  20. ^ Baycroft, Thomas A.; Badnell, Harry; Blacker, Samuel; Triaud, Amaury H. M. J. (1 August 2023). "GJ 9404 b: A Confirmed Eccentric Planet, and not a Candidate". Research Notes of the American Astronomical Society. 7 (8): 175. arXiv:2308.12309. Bibcode:2023RNAAS...7..175B. doi:10.3847/2515-5172/acefc5. ISSN 2515-5172.
  21. ^ de Beurs, Zoë L.; de Wit, Julien; Venner, Alexander; Berardo, David; Bryan, Jared; Winn, Joshua N.; Fulton, Benjamin J.; Howard, Andrew W. (1 October 2023). "Revisiting Orbital Evolution in HAT-P-2 b and Confirmation of HAT-P-2 c". The Astronomical Journal. 166 (4): 136. arXiv:2309.03256. Bibcode:2023AJ....166..136D. doi:10.3847/1538-3881/acedf1. ISSN 0004-6256.
  22. ^ Lee, Byeong-Cheol; Do, Hee-Jin; Park, Myeong-Gu; Lim, Beomdu; Choi, Yeon-Ho; Koo, Jae-Rim; Bang, Tae-Yang; Oh, Hyeong-Ill; Han, Inwoo; Chang, Heon-Young (2023). "Long-period radial velocity variations of nine M red giants: The detection of sub-stellar companions around HD 6860 and HD 112300". Astronomy and Astrophysics. 678. arXiv:2307.15897. Bibcode:2023A&A...678A.106L. doi:10.1051/0004-6361/202243725. S2CID 260334453.
  23. ^ a b c d e f g Akana Murphy, Joseph M.; et al. (48) (8 September 2023). "The TESS-Keck Survey. XVI. Mass Measurements for 12 Planets in Eight Systems". The Astronomical Journal. 166 (4): 153. arXiv:2306.16587. Bibcode:2023AJ....166..153A. doi:10.3847/1538-3881/ace2ca.
  24. ^ a b Tuson, Amy; Queloz, Didier; Osborn, Hugh P.; Wilson, Thomas G.; Hooton, Matthew J.; Beck, Mathias; Lendl, Monika; Olofsson, Göran; Fortier, Andrea; Bonfanti, Andrea; Brandeker, Alexis; Buchhave, Lars A.; Cameron, Andrew Collier; Ciardi, David R.; Collins, Karen A. (2023). "TESS and CHEOPS discover two warm sub-Neptunes transiting the bright K-dwarf HD 15906". Monthly Notices of the Royal Astronomical Society. 523 (2): 3090–3118. arXiv:2306.04511. doi:10.1093/mnras/stad1369.
  25. ^ Lee, Byeong-Cheol; Koo, Jae-Rim; Jeong, Gwanghui; Park, Myeong-Gu; Han, Inwoo; Choi, Yeon-Ho (1 March 2023). "A Search for Exoplanets around Northern Circumpolar Stars VII. Detection of Planetary Companion Orbiting the Largest Host Star HD 18438". Journal of Korean Astronomical Society. 56 (1): 35–40. arXiv:2303.08357. Bibcode:2023JKAS...56...35L. doi:10.5303/JKAS.2023.56.1.35. ISSN 1225-4614. S2CID 257532879. Archived from the original on 6 October 2023. Retrieved 10 September 2023.
  26. ^ Garai, Z.; Osborn, H. P.; Gandolfi, D.; Brandeker, A.; Sousa, S. G.; Lendl, M.; Bekkelien, A.; Broeg, C.; Cameron, A. Collier; Egger, J. A.; Hooton, M. J.; Alibert, Y.; Delrez, L.; Fossati, L.; Salmon, S. (1 June 2023). "Refined parameters of the HD 22946 planetary system and the true orbital period of planet d★". Astronomy and Astrophysics. 674: A44. arXiv:2306.04468. Bibcode:2023A&A...674A..44G. doi:10.1051/0004-6361/202345943. ISSN 0004-6361. S2CID 259095617. Archived from the original on 16 December 2023. Retrieved 1 January 2024.
  27. ^ Lee, Byeong-Cheol; Han, Inwoo; Jeong, Gwanghui; Koo, Jae-Rim; Lim, Beomdu; Park, Myeong-Gu; Bang, Tae-Yang; Choi, Yeon-Ho; Choi, Yeon-Ho; Oh, Hyeong-Ill (22 August 2023). "A Search for Exoplanets around Northern Circumpolar Stars. VIII. Filtering Out a Planet Cycle from the Multi-Period Radial Velocity Variations in M Giant HD 36384". Journal of the Korean Astronomical Society. 56 (2): 195–199. arXiv:2308.05994. Bibcode:2023JKAS...56..195L. doi:10.5303/JKAS.2023.56.2.195.
  28. ^ a b c d e f g h Philipot, F.; Lagrange, A. -M.; Kiefer, F.; Rubini, P.; Delorme, P.; Chomez, A. (2023). "A multi-technique approach to identifying and/Or constraining radial-velocity substellar companions". Astronomy & Astrophysics. 678: A107. arXiv:2308.05417. Bibcode:2023A&A...678A.107P. doi:10.1051/0004-6361/202346612. S2CID 260775968.
  29. ^ Xiao, Guang-Yao; Liu, Yu-Juan; Teng, Huan-Yu; Wang, Wei; Brandt, Timothy D.; Zhao, Gang; Zhao, Fei; Zhai, Meng; Gao, Qi (1 May 2023). "The Masses of a Sample of Radial-velocity Exoplanets with Astrometric Measurements". Research in Astronomy and Astrophysics. 23 (5): 055022. arXiv:2303.12409. Bibcode:2023RAA....23e5022X. doi:10.1088/1674-4527/accb7e. ISSN 1674-4527. S2CID 257663647.
  30. ^ Stalport, M.; Cretignier, M.; Udry, S.; John, A. Anna; Wilson, T. G.; Delisle, J. -B.; Bonomo, A. S.; Buchhave, L. A.; Charbonneau, D.; Dalal, S.; Damasso, M.; Di Fabrizio, L.; Dumusque, X.; Fiorenzano, A.; Harutyunyan, A. (2023). "A review of planetary systems around HD 99492, HD 147379, and HD 190007 with HARPS-N". Astronomy & Astrophysics. 678: A90. arXiv:2308.05669. Bibcode:2023A&A...678A..90S. doi:10.1051/0004-6361/202346887. S2CID 260775534.
  31. ^ Lee, Byeong-Cheol; Do, Hee-Jin; Park, Myeong-Gu; Lim, Beomdu; Choi, Yeon-Ho; Koo, Jae-Rim; Bang, Tae-Yang; Oh, Hyeong-Ill; Han, Inwoo; Chang, Heon-Young (2023). "Long-period radial velocity variations of nine M red giants: The detection of sub-stellar companions around HD 6860 and HD 112300". Astronomy and Astrophysics. 678. arXiv:2307.15897. Bibcode:2023A&A...678A.106L. doi:10.1051/0004-6361/202243725. S2CID 260334453.
  32. ^ a b c Paegert, M.; Stassun, K. G.; Collins, K. A.; Pepper, J.; Torres, G.; Jenkins, J.; Twicken, J. D.; Latham, D. W. (1 February 2022). "VizieR Online Data Catalog: TESS Input Catalog version 8.2 (TIC v8.2) (Paegert+, 2021)". VizieR Online Data Catalog. 4039: IV/39. Bibcode:2022yCat.4039....0P.
  33. ^ a b c d Garrido-Deutelmoser, Juan; Petrovich, Cristobal; Charalambous, Carolina; Guzmán, Viviana V.; Zhang, Ke (1 March 2023). "A gap-sharing planet pair shaping the crescent in HD 163296: a disk sculpted by a resonant chain". The Astrophysical Journal Letters. 945 (2): L37. arXiv:2301.13260. doi:10.3847/2041-8213/acbea8. ISSN 2041-8205.
  34. ^ Hammond, Iain; Christiaens, Valentin; Price, Daniel J.; Toci, Claudia; Pinte, Christophe; Juillard, Sandrine; Garg, Himanshi (1 June 2023). "Confirmation and Keplerian motion of the gap-carving protoplanet HD 169142 b". Monthly Notices of the Royal Astronomical Society. 522 (1): L51–L55. arXiv:2302.11302. Bibcode:2023MNRAS.522L..51H. doi:10.1093/mnrasl/slad027. ISSN 0035-8711.
  35. ^ Barros, S. C. C.; et al. (2023). "The young mini-Neptune HD 207496b that is either a naked core or on the verge of becoming one". Astronomy & Astrophysics. 673: A4. arXiv:2303.03775. Bibcode:2023A&A...673A...4B. doi:10.1051/0004-6361/202245741. S2CID 257378182.
  36. ^ Orell-Miquel, J.; Lampón, M.; López-Puertas, M.; Mallorquín, M.; Murgas, F.; Peláez-Torres, A.; Pallé, E.; Esparza-Borges, E.; Sanz-Forcada, J.; Tabernero, H. M.; Nortmann, L.; Nagel, E.; Parviainen, H.; Osorio, M. R. Zapatero; Caballero, J. A. (2023). "Confirmation of an He I evaporating atmosphere around the 650-Myr-old sub-Neptune HD 235088 b (TOI-1430 b) with CARMENES". Astronomy & Astrophysics. 677: A56. arXiv:2307.05191. Bibcode:2023A&A...677A..56O. doi:10.1051/0004-6361/202346445. S2CID 259766771.
  37. ^ a b Osborn, Hugh P.; Nowak, Grzegorz; Hébrard, Guillaume; Masseron, Thomas; Lillo-Box, J.; Pallé, Enric; Bekkelien, Anja; Florén, Hans-Gustav; Guterman, Pascal; Simon, Attila E.; Adibekyan, V.; Bieryla, Allyson; Borsato, Luca; Brandeker, Alexis; Ciardi, David R. (2023). "Two warm Neptunes transiting HIP 9618 revealed by TESS and Cheops". Monthly Notices of the Royal Astronomical Society. 523 (2): 3069–3089. arXiv:2306.04450. doi:10.1093/mnras/stad1319.
  38. ^ a b c Damasso, M.; Rodrigues, J.; Castro-González, A.; Lavie, B.; Davoult, J.; Osorio, M. R. Zapatero; Dou, J.; Sousa, S. G.; Owen, J. E.; Sossi, P.; Adibekyan, V.; Osborn, H.; Leinhardt, Z.; Alibert, Y.; Lovis, C. (2023). "A compact multi-planet system transiting HIP 29442 (TOI-469) discovered by TESS and ESPRESSO. Radial velocities lead to the detection of transits with low signal-to-noise ratio". Astronomy and Astrophysics. 679. arXiv:2308.13310. Bibcode:2023A&A...679A..33D. doi:10.1051/0004-6361/202347240. S2CID 261214427.
  39. ^ Chomez, A.; Squicciarini, V.; Lagrange, A. -M.; Delorme, P.; Viswanath, G.; Janson, M.; Flasseur, O.; Chauvin, G.; Langlois, M.; Rubini, P.; Bergeon, S.; Albert, D.; Bonnefoy, M.; Desidera, S.; Engler, N. (2023). "An imaged 15 M Jup companion within a hierarchical quadruple system". Astronomy & Astrophysics. 676: L10. arXiv:2307.01195. Bibcode:2023A&A...676L..10C. doi:10.1051/0004-6361/202347044. S2CID 259316431.
  40. ^ a b Lowson, N; Zhou, G; Huang, C X; Wright, D J; Edwards, B; Nabbie, E; Venner, A; Quinn, S N; Collins, K A; Gillen, E; Battley, M; Triaud, A; Hellier, C; Seager, S; Winn, J N (12 September 2023). "Two mini-Neptunes Transiting the Adolescent K-star HIP 113103 Confirmed with TESS and CHEOPS". Monthly Notices of the Royal Astronomical Society. 527: 1146–1162. doi:10.1093/mnras/stad2756. ISSN 0035-8711.
  41. ^ González-Álvarez, E.; Kemmer, J.; Chaturvedi, P.; Caballero, J. A.; Quirrenbach, A.; Amado, P. J.; Béjar, V. J. S.; Cifuentes, C.; Herrero, E.; Kossakowski, D.; Reiners, A.; Ribas, I.; Rodríguez, E.; Rodríguez-López, C.; Sanz-Forcada, J. (2023). "The CARMENES search for exoplanets around M dwarfs". Astronomy & Astrophysics. 675: A141. arXiv:2305.19677. doi:10.1051/0004-6361/202346276. S2CID 265978782.
  42. ^ a b Bonomo, A. S.; Dumusque, X.; Massa, A.; Mortier, A.; Bongiolatti, R.; Malavolta, L.; Sozzetti, A.; Buchhave, L. A.; Damasso, M.; Haywood, R. D.; Morbidelli, A.; Latham, D. W.; Molinari, E.; Pepe, F.; Poretti, E. (2023). "Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities. No excess of cold Jupiters in small planet systems". Astronomy & Astrophysics. 677. arXiv:2304.05773. Bibcode:2023A&A...677A..33B. doi:10.1051/0004-6361/202346211. S2CID 258078829.
  43. ^ Hirano, Teruyuki; et al. (2023). "An Earth-sized Planet around an M5 Dwarf Star at 22 pc". The Astronomical Journal. 165 (3): 131. arXiv:2302.00699. Bibcode:2023AJ....165..131H. doi:10.3847/1538-3881/acb7e1. S2CID 256503980.
  44. ^ a b Incha, Elyse; Vanderburg, Andrew; Jacobs, Tom; LaCourse, Daryll; Bieryla, Allyson; Pass, Emily; Howell, Steve B; Berlind, Perry; Calkins, Michael; Esquerdo, Gilbert; Latham, David W; Mann, Andrew W (23 May 2023). "Kepler 's last planet discoveries: two new planets and one single-transit candidate from K2 campaign 19". Monthly Notices of the Royal Astronomical Society. 523 (1): 474–487. arXiv:2305.18516. doi:10.1093/mnras/stad1049. ISSN 0035-8711. Archived from the original on 1 December 2023. Retrieved 6 October 2023.
  45. ^ Specht, D; Poleski, R; Penny, M T; Kerins, E; McDonald, I; Lee, Chung-Uk; Udalski, A; Bond, I A; Shvartzvald, Y; Zang, Weicheng; Street, R A; Hogg, D W; Gaudi, B S; Barclay, T; Barentsen, G (22 February 2023). "Kepler K2 Campaign 9 – II. First space-based discovery of an exoplanet using microlensing". Monthly Notices of the Royal Astronomical Society. 520 (4): 6350–6366. arXiv:2203.16959. doi:10.1093/mnras/stad212. ISSN 0035-8711.
  46. ^ "K2-2016-BLG-005L b - Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Archived from the original on 3 December 2023. Retrieved 3 December 2023.
  47. ^ Bonomo, A. S.; Dumusque, X.; Massa, A.; Mortier, A.; Bongiolatti, R.; Malavolta, L.; Sozzetti, A.; Buchhave, L. A.; Damasso, M.; Haywood, R. D.; Morbidelli, A.; Latham, D. W.; Molinari, E.; Pepe, F.; Poretti, E. (September 2023). "Cold Jupiters and improved masses in 38 Kepler and K2 small planet systems from 3661 HARPS-N radial velocities: No excess of cold Jupiters in small planet systems" (PDF). Astronomy & Astrophysics. 677 (A33): 18. arXiv:2304.05773. Bibcode:2023A&A...677A..33B. doi:10.1051/0004-6361/202346211. ISSN 0004-6361. S2CID 261556620. Archived (PDF) from the original on 3 December 2023. Retrieved 7 December 2023.
  48. ^ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh bi bj bk bl bm bn bo Valizadegan, Hamed; Martinho, Miguel J. S.; Jenkins, Jon M.; Caldwell, Douglas A.; Twicken, Joseph D.; Bryson, Stephen T. (1 July 2023). "Multiplicity Boost of Transit Signal Classifiers: Validation of 69 New Exoplanets using the Multiplicity Boost of ExoMiner". The Astronomical Journal. 166 (1): 28. arXiv:2305.02470. Bibcode:2023AJ....166...28V. doi:10.3847/1538-3881/acd344. ISSN 0004-6256.
  49. ^ Yahalomi, Daniel A; Kipping, David; Nesvorný, David; Dalba, Paul A; Benni, Paul; Cacho-Negrete, Ceiligh; Collins, Karen; Earwicker, Joel T; Lewis, John Arban; McLeod, Kim K; Schwarz, Richard P; Wang, Gavin (28 October 2023). "Not-so-fast Kepler-1513: a perturbing planetary interloper in the exomoon corridor". Monthly Notices of the Royal Astronomical Society. 527 (1): 620–639. arXiv:2310.03802. Bibcode:2024MNRAS.527..620Y. doi:10.1093/mnras/stad3070. ISSN 0035-8711. Archived from the original on 9 December 2023. Retrieved 6 December 2023.
  50. ^ Wu, Dong-Hong; Rice, Malena; Wang, Songhu (1 April 2023). "Evidence for Hidden Nearby Companions to Hot Jupiters". The Astronomical Journal. 165 (4): 171. arXiv:2302.12778. Bibcode:2023AJ....165..171W. doi:10.3847/1538-3881/acbf3f. ISSN 0004-6256.
  51. ^ a b c d e Shin, In-Gu; et al. (2023). "Systematic KMTNet Planetary Anomaly Search. IX. Complete Sample of 2016 Prime-Field Planets". The Astronomical Journal. 166 (3): 104. arXiv:2303.16881. Bibcode:2023AJ....166..104S. doi:10.3847/1538-3881/ace96d.
  52. ^ a b c d e f g Zang, Weicheng; Jung, Youn Kil; Yang, Hongjing; Zhang, Xiangyu; Udalski, Andrzej; Yee, Jennifer C.; Gould, Andrew; Mao, Shude; Albrow, Michael D.; Chung, Sun-Ju; Han, Cheongho; Hwang, Kyu-Ha; Ryu, Yoon-Hyun; Shin, In-Gu; Shvartzvald, Yossi (1 March 2023). "Systematic KMTNet Planetary Anomaly Search. VII. Complete Sample of q < 10 −4 Planets from the First 4 yr Survey". The Astronomical Journal. 165 (3): 103. arXiv:2210.12344. Bibcode:2023AJ....165..103Z. doi:10.3847/1538-3881/acb34b. ISSN 0004-6256.
  53. ^ a b c d e Youn Kil Jung; et al. (2023). "Systematic KMTNet Planetary Anomaly Search. VIII. Complete Sample of 2019 Subprime Field Planets". The Astronomical Journal. 165 (6): 226. arXiv:2302.13544. Bibcode:2023AJ....165..226J. doi:10.3847/1538-3881/accb8f. S2CID 258505742.
  54. ^ a b c d Ryu, Yoon-Hyun; Shin, In-Gu; Yang, Hongjing; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Han, Cheongho; Hwang, Kyu-Ha; Kil Jung, Youn; Shvartzvald, Yossi; Yee, Jennifer C.; Zang, Weicheng; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Seung-Lee (1 March 2023). "Mass Production of 2021 KMTNet Microlensing Planets II". The Astronomical Journal. 165 (3): 83. arXiv:2207.07295. Bibcode:2023AJ....165...83R. doi:10.3847/1538-3881/acab6b. ISSN 0004-6256.
  55. ^ a b c Han, Cheongho; Lee, Chung-Uk; Zang, Weicheng; Youn Kil Jung; Christie, Grant W.; Zhang, Jiyuan; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Hwang, Kyu-Ha; Kim, Doeon; Ryu, Yoon-Hyun; Shin, In-Gu; Shvartzvald, Yossi; Yang, Hongjing; Yee, Jennifer C.; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Seung-Lee; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W.; Natusch, Tim; Mao, Shude; Maoz, Dan; Penny, Matthew T.; Zhu, Wei (2023). "KMT-2021-BLG-2010Lb, KMT-2022-BLG-0371Lb, and KMT-2022-BLG-1013Lb: Three microlensing planets detected via partially covered signals". Astronomy & Astrophysics. 674: A90. arXiv:2304.03871. Bibcode:2023A&A...674A..90H. doi:10.1051/0004-6361/202346298. S2CID 258048865.
  56. ^ "The Extrasolar Planet Encyclopaedia — KMT-2022-BLG-0440L b". Extrasolar Planets Encyclopaedia. 23 October 1995. Retrieved 19 January 2023.
  57. ^ Zhang, Jiyuan; et al. (2023). "KMT-2022-BLG-0440Lb: A new q < 10−4 microlensing planet with the central-resonant caustic degeneracy broken". Monthly Notices of the Royal Astronomical Society. 522 (4): 6055–6069. arXiv:2301.06779. doi:10.1093/mnras/stad1398.
  58. ^ Sartori, Lia F.; Lovis, Christophe; Delisle, Jean-Baptiste; Lendl, Monika; Cugno, Gabriele; Boehle, Anna; Dannert, Felix; Krenn, Andreas; Gubler, Jonas L.; Quanz, Sascha P. (February 2023). "L 363-38 b: A planet newly discovered with ESPRESSO orbiting a nearby M dwarf star". Astronomy & Astrophysics. 670 (A42): 12. arXiv:2210.12710. Bibcode:2023A&A...670A..42S. doi:10.1051/0004-6361/202244347. ISSN 0004-6361. S2CID 253098575.
  59. ^ Stefansson, Gudmundur; Mahadevan, Suvrath; Miguel, Yamila; Robertson, Paul; Delamer, Megan; Kanodia, Shubham; Cañas, Caleb; Winn, Joshua; Ninan, Joe; Terrien, Ryan; Holcomb, Rae; Ford, Eric; Zawadzki, Brianna; Bowler, Brendan P.; Bender, Chad; Cochran, William; Diddams, Scott; Endl, Michael; Fredrick, Connor; Halverson, Samuel; Hearty, Fred; Hill, Gary J.; Lin, Andrea; Metcalf, Andrew; Monson, Andrew; Ramsey, Lawrence; Roy, Arpita; Schwab, Christian; Wright, Jason; Zeimann, Gregory (2023). "An extreme test case for planet formation: a close-in Neptune orbiting an ultracool star". arXiv:2303.13321 [astro-ph.EP].
  60. ^ Lustig-Yaeger, J.; Fu, G.; et al. (January 2023). "A JWST transmission spectrum of the nearby Earth-sized exoplanet LHS 475 B". Nature Astronomy. 7 (11): 1317–1328. arXiv:2301.04191. Bibcode:2023NatAs...7.1317L. doi:10.1038/s41550-023-02064-z. S2CID 261439142.
  61. ^ "The Extrasolar Planet Encyclopaedia — LHS 475 b". Extrasolar Planets Encyclopaedia. 23 October 1995. Archived from the original on 20 December 2023. Retrieved 12 January 2023.
  62. ^ Ment, Kristo; Charbonneau, David; Irwin, Jonathan; Winters, Jennifer G.; Pass, Emily; Shporer, Avi; Essack, Zahra; Kostov, Veselin B.; Kunimoto, Michelle; Levine, Alan; Seager, Sara; Vanderspek, Roland; Winn, Joshua N. (2023). "LHS 475 b: A Venus-sized Planet Orbiting a Nearby M Dwarf". arXiv:2304.01920 [astro-ph.EP].
  63. ^ "Webb Discovers LHS 475 b, an Earth-Sized, Rocky Planet". 12 January 2023.
  64. ^ Peterson, Merrin S.; Benneke, Björn; Collins, Karen; Piaulet, Caroline; Crossfield, Ian J. M.; Ali-Dib, Mohamad; Christiansen, Jessie L.; Gagné, Jonathan; Faherty, Jackie; Kite, Edwin; Dressing, Courtney; Charbonneau, David; Murgas, Felipe; Cointepas, Marion; Almenara, Jose Manuel (25 May 2023). "A temperate Earth-sized planet with tidal heating transiting an M6 star". Nature. 617 (7962): 701–705. Bibcode:2023Natur.617..701P. doi:10.1038/s41586-023-05934-8. hdl:11603/28165. ISSN 0028-0836. PMID 37198481. S2CID 258764768. Archived from the original on 29 December 2023. Retrieved 7 December 2023.
  65. ^ Olmschenk, Greg; Bennett, David P.; Bond, Ian A.; Zang, Weicheng; Jung, Youn Kil; Yee, Jennifer C.; Bachelet, Etienne; Abe, Fumio; Barry, Richard K.; Bhattacharya, Aparna; Fujii, Hirosane; Fukui, Akihiko; Hirao, Yuki; Silva, Stela Ishitani; Itow, Yoshitaka (1 April 2023). "MOA-2020-BLG-208Lb: Cool Sub-Saturn-mass Planet within Predicted Desert". The Astronomical Journal. 165 (4): 175. arXiv:2210.02436. Bibcode:2023AJ....165..175O. doi:10.3847/1538-3881/acbcc8. ISSN 0004-6256.
  66. ^ Han, Cheongho; et al. (2023). "MOA-2022-BLG-249Lb: Nearby microlensing super-Earth planet detected from high-cadence surveys". Astronomy & Astrophysics. 674: A89. arXiv:2304.02815. Bibcode:2023A&A...674A..89H. doi:10.1051/0004-6361/202346166. S2CID 257985492.
  67. ^ Wagner, Kevin; Stone, Jordan; Skemer, Andrew; Ertel, Steve; Dong, Ruobing; Apai, Dániel; Spalding, Eckhart; Leisenring, Jarron; Sitko, Michael; Kratter, Kaitlin; Barman, Travis; Marley, Mark; Miles, Brittany; Boccaletti, Anthony; Assani, Korash (6 July 2023). "Direct images and spectroscopy of a giant protoplanet driving spiral arms in MWC 758". Nature Astronomy. 7 (10): 1208–1217. arXiv:2307.04021. Bibcode:2023NatAs...7.1208W. doi:10.1038/s41550-023-02028-3. ISSN 2397-3366. S2CID 259501395. Archived from the original on 7 September 2023. Retrieved 7 December 2023.
  68. ^ a b Brewer, John M.; Zhao, Lily L.; Fischer, Debra A.; Roettenbacher, Rachael M.; Henry, Gregory W.; Llama, Joe; Szymkowiak, Andrew E.; Cabot, Samuel H. C.; Weiss, Sam A.; McCarthy, Chris (1 August 2023). "EXPRES. IV. Two Additional Planets Orbiting ρ Coronae Borealis Reveal Uncommon System Architecture". The Astronomical Journal. 166 (2): 46. arXiv:2306.06888. Bibcode:2023AJ....166...46B. doi:10.3847/1538-3881/acdd6f. ISSN 0004-6256.
  69. ^ a b Bozhilov, Vladimir; Antonova, Desislava; Hobson, Melissa J.; Brahm, Rafael; Jordan, Andres; Henning, Thomas; Eberhardt, Jan; Rojas, Felipe I.; Batygin, Konstantin; Torres-Miranda, Pascal; Stassun, Keivan G.; Millholland, Sarah C.; Stoeva, Denitza; Minev, Milen; Espinoza, Nestor; Ricker, George R.; Latham, David W.; Dragomir, Diana; Kunimoto, Michelle; Jenkins, Jon M.; Ting, Eric B.; Seager, Sara; Winn, Joshua N.; Jesus Noel Villasenor; Bouma, Luke G.; Medina, Jennifer; Trifonov, Trifon (2023). "A 2:1 Mean-motion Resonance Super-Jovian Pair Revealed by TESS, FEROS, and HARPS". The Astrophysical Journal Letters. 946 (2): L36. arXiv:2302.10838. Bibcode:2023ApJ...946L..36B. doi:10.3847/2041-8213/acbd4f. S2CID 257050718.
  70. ^ Grunblatt, Samuel; Saunders, Nicholas; Huber, Daniel; Thorngren, Daniel; Vissapragada, Shreyas; Yoshida, Stephanie; Schlaufman, Kevin; Giacalone, Steven; MacDougall, Mason; Chontos, Ashley; Turtelboom, Emma; Beard, Corey; Akana Murphy, Joseph M.; Rice, Malena; Isaacson, Howard; Angus, Ruth; Howard, Andrew W. (2023). "An unlikely survivor: a low-density hot Neptune orbiting a red giant star". arXiv:2303.06728 [astro-ph.EP].
  71. ^ a b c d e f g h i j k l m n o p q Mistry, Priyashkumar; et al. (2023). "VaTEST. II. Statistical Validation of 11 TESS-detected Exoplanets Orbiting K-type Stars". The Astronomical Journal. 166 (1): 9. arXiv:2301.09865. Bibcode:2023AJ....166....9M. doi:10.3847/1538-3881/acd548. S2CID 258685555.
  72. ^ Mistry, Priyashkumar; Pathak, Kamlesh; Lekkas, Georgios; Prasad, Aniket; Bhattarai, Surendra; Maity, Mousam; Beichman, Charles A; Ciardi, David R; Evans, Phil; Bieryla, Allyson; Eastman, Jason D; Esquerdo, Gilbert A; Lucero, Jennifer P (2 March 2023). "VaTEST I: validation of sub-Saturn exoplanet TOI-181b in narrow orbit from its host star". Monthly Notices of the Royal Astronomical Society. 521 (1): 1066–1078. arXiv:2211.07957. doi:10.1093/mnras/stad543. ISSN 0035-8711.
  73. ^ a b c d Oddo, Dominic; Dragomir, Diana; Brandeker, Alexis; Osborn, Hugh P.; Collins, Karen; Stassun, Keivan G.; Astudillo-Defru, Nicola; Bieryla, Allyson; Howell, Steve B.; Ciardi, David R.; Quinn, Samuel; Almenara, Jose M.; Briceño, César; Collins, Kevin I.; Colón, Knicole D. (1 March 2023). "Characterization of a Set of Small Planets with TESS and CHEOPS and an Analysis of Photometric Performance". The Astronomical Journal. 165 (3): 134. arXiv:2301.08162. Bibcode:2023AJ....165..134O. doi:10.3847/1538-3881/acb4e3. ISSN 0004-6256.
  74. ^ a b Hobson, Melissa J.; Trifonov, Trifon; Henning, Thomas; Jordán, Andrés; Rojas, Felipe; Espinoza, Nestor; Brahm, Rafael; Eberhardt, Jan; Jones, Matías I.; Mekarnia, Djamel; Kossakowski, Diana; Schlecker, Martin; Tala Pinto, Marcelo; Torres Miranda, Pascal José; Abe, Lyu (1 November 2023). "TOI-199 b: A Well-characterized 100 day Transiting Warm Giant Planet with TTVs Seen from Antarctica". The Astronomical Journal. 166 (5): 201. arXiv:2309.14915. Bibcode:2023AJ....166..201H. doi:10.3847/1538-3881/acfc1d. ISSN 0004-6256.
  75. ^ a b c d e f g h Priyashkumar, Mistry; Prasad, Aniket; Maity, Mousam; Pathak, Kamlesh; Gharat, Sarvesh; Lekkas, Georgios; Bhattarai, Surendra; Kumar, Dhruv; Lissauer, Jack J.; Twicken, Joseph D.; Soubkiou, Abderahmane; Pozuelos, Francisco J.; Jenkins, Jon; Horne, Keith; Giacalone, Steven; Barkaoui, Khalid; Timmermans, Mathilde; Watkins, Cristilyn N.; Sefako, Ramotholo; Collins, Karen A.; Shporer, Avi; Benkhaldoun, Zouhair; Stockdale, Chris; Jehin, Emmanuël; Murgas, Felipe; Paegert, Martin; Lund, Michael B.; Narita, Norio; Schwarz, Richard P.; Goeke, Robert F.; Tan, Thiam-Guan; Kawai, Yugo (1 November 2023). "VaTEST III: Validation of 8 Potential Super-Earths from TESS Data". arXiv:2311.00688 [astro-ph.EP].
  76. ^ Castro-González, A.; Demangeon, O. D. S.; Lillo-Box, J.; Lovis, C.; Lavie, B.; Adibekyan, V.; Acuña, L.; Deleuil, M.; Aguichine, A.; Zapatero Osorio, M. R.; Tabernero, H. M.; Davoult, J.; Alibert, Y.; Santos, N.; Sousa, S. G. (July 2023). "An unusually low-density super-Earth transiting the bright early-type M-dwarf GJ 1018 (TOI-244)". Astronomy & Astrophysics. 675: A52. arXiv:2305.04922. Bibcode:2023A&A...675A..52C. doi:10.1051/0004-6361/202346550. ISSN 0004-6361. S2CID 258556864.
  77. ^ Osborn, Ares; Armstrong, David J; Fernández Fernández, Jorge; Knierim, Henrik; Adibekyan, Vardan; Collins, Karen A; Delgado Mena, Elisa; Fridlund, Malcolm; Gomes da Silva, João; Hellier, Coel; Jackson, David G; King, George W; Lillo-Box, Jorge; Matson, Rachel A; Matthews, Elisabeth C (21 September 2023). "TOI-332 b: a super dense Neptune found deep within the Neptunian desert". Monthly Notices of the Royal Astronomical Society. 526 (1): 548–566. arXiv:2308.12137. doi:10.1093/mnras/stad2575. ISSN 0035-8711. Archived from the original on 9 December 2023. Retrieved 9 December 2023.
  78. ^ a b c Psaridi, Angelica; et al. (2023). "Three Saturn-mass planets transiting F-type stars revealed with TESS and HARPS". Astronomy & Astrophysics. 675: A39. arXiv:2303.15080. doi:10.1051/0004-6361/202346406. S2CID 257766828.
  79. ^ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Archived from the original on 1 October 2023. Retrieved 9 November 2023.
  80. ^ "TOI-700 e: NASA Discovers New Earth-Like World Around Distant Star". AZoQuantum.com. 15 February 2023. Archived from the original on 9 November 2023. Retrieved 9 November 2023.
  81. ^ Gilbert, Emily A.; et al. (2023). "A Second Earth-sized Planet in the Habitable Zone of the M Dwarf, TOI-700". The Astrophysical Journal Letters. 944 (2): L35. arXiv:2301.03617. Bibcode:2023ApJ...944L..35G. doi:10.3847/2041-8213/acb599. S2CID 255570018.
  82. ^ "The Extrasolar Planet Encyclopaedia — TOI-700 e". Extrasolar Planets Encyclopaedia. 23 October 1995. Retrieved 12 January 2023.
  83. ^ Dransfield, Georgina; Timmermans, Mathilde; Triaud, Amaury H M J; Dévora-Pajares, Martín; Aganze, Christian; Barkaoui, Khalid; Burgasser, Adam J; Collins, Karen A; Cointepas, Marion; Ducrot, Elsa; Günther, Maximilian N; Howell, Steve B; Murray, Catriona A; Niraula, Prajwal; Rackham, Benjamin V (28 October 2023). "A 1.55 R⊕ habitable-zone planet hosted by TOI-715, an M4 star near the ecliptic South Pole". Monthly Notices of the Royal Astronomical Society. 527 (1): 35–52. arXiv:2305.06206. doi:10.1093/mnras/stad1439. ISSN 0035-8711. Archived from the original on 9 December 2023. Retrieved 9 December 2023.
  84. ^ Georgieva, Iskra Y.; et al. (2023). "TOI-733 b: A planet in the small-planet radius valley orbiting a Sun-like star". Astronomy & Astrophysics. 674: A117. arXiv:2304.06655. Bibcode:2023A&A...674A.117G. doi:10.1051/0004-6361/202345961. S2CID 258108052.
  85. ^ Clark, Jake T.; Addison, Brett C.; Okumura, Jack; Vach, Sydney; Errico, Adriana; Heitzmann, Alexis; Rodriguez, Joseph E.; Wright, Duncan J.; Clerté, Mathieu; Brown, Carolyn J.; Fetherolf, Tara; Wittenmyer, Robert A.; Plavchan, Peter; Kane, Stephen R.; Horner, Jonathan (1 May 2023). "Spinning up a Daze: TESS Uncovers a Hot Jupiter Orbiting the Rapid Rotator TOI-778". The Astronomical Journal. 165 (5): 207. arXiv:2212.08242. Bibcode:2023AJ....165..207C. doi:10.3847/1538-3881/acc3a0. ISSN 0004-6256.
  86. ^ Hua, Xinyan; Wang, Sharon Xuesong; Teske, Johanna K.; Gan, Tianjun; Shporer, Avi; Zhou, George; Stassun, Keivan G.; Rabus, Markus; Howell, Steve B.; Ziegler, Carl; Lissauer, Jack J.; Winn, Joshua N.; Jenkins, Jon M.; Ting, Eric B.; Collins, Karen A. (1 July 2023). "A Transiting Super-Earth in the Radius Valley and an Outer Planet Candidate Around HD 307842". The Astronomical Journal. 166 (1): 32. arXiv:2306.14655. Bibcode:2023AJ....166...32H. doi:10.3847/1538-3881/acd751. ISSN 0004-6256.
  87. ^ a b Hawthorn, Faith; Bayliss, Daniel; Wilson, Thomas G; Bonfanti, Andrea; Adibekyan, Vardan; Alibert, Yann; Sousa, Sérgio G; Collins, Karen A; Bryant, Edward M; Osborn, Ares; Armstrong, David J; Abe, Lyu; Acton, Jack S; Addison, Brett C; Agabi, Karim (15 February 2023). "TOI-836: A super-Earth and mini-Neptune transiting a nearby K-dwarf". Monthly Notices of the Royal Astronomical Society. 520 (3): 3649–3668. arXiv:2208.07328. doi:10.1093/mnras/stad306. ISSN 0035-8711. Archived from the original on 19 May 2023. Retrieved 9 December 2023.
  88. ^ Hagelberg, J.; Nielsen, L. D.; Attia, O.; Bourrier, V.; Pearce, L.; Venturini, J.; Winn, J. N.; Bouchy, F.; Bouma, L. G.; Briceño, C.; Collins, K. A.; Davis, A. B.; Eastman, J. D.; Evans, P.; Falk, B. (November 2023). "TOI-858 B b: A hot Jupiter on a polar orbit in a loose binary". Astronomy & Astrophysics. 679: A70. arXiv:2309.11390. Bibcode:2023A&A...679A..70H. doi:10.1051/0004-6361/202244940. ISSN 0004-6361. S2CID 262064260.
  89. ^ Hawthorn, Faith; Bayliss, Daniel; Armstrong, David J; Fernández Fernández, Jorge; Osborn, Ares; Sousa, Sérgio G; Adibekyan, Vardan; Davoult, Jeanne; Collins, Karen A; Alibert, Yann; Barros, Susana C C; Bouchy, François; Brogi, Matteo; Ciardi, David R; Daylan, Tansu (24 July 2023). "TOI-908: a planet at the edge of the Neptune desert transiting a G-type star". Monthly Notices of the Royal Astronomical Society. 524 (3): 3877–3893. doi:10.1093/mnras/stad1840. hdl:10023/28054. ISSN 0035-8711. Archived from the original on 9 December 2023. Retrieved 9 December 2023.
  90. ^ a b Armstrong, David J; Osborn, Ares; Adibekyan, Vardan; Delgado-Mena, Elisa; Hojjatpanah, Saeed; Howell, Steve B; Hoyer, Sergio; Knierim, Henrik; Sousa, Sérgio G; Stassun, Keivan G; Veras, Dimitri; Anderson, David R; Bayliss, Daniel; Bouchy, François; Burke, Christopher J (29 July 2023). "Discovery and characterization of two Neptune-mass planets orbiting HD 212729 with TESS". Monthly Notices of the Royal Astronomical Society. 524 (4): 5804–5816. arXiv:2307.11566. doi:10.1093/mnras/stad2183. ISSN 0035-8711. Archived from the original on 8 December 2023. Retrieved 8 December 2023.
  91. ^ Wang, Jia-Qi; Jiang, Xiao-Jun; Zheng, Jie; Kellermann, Hanna; Riffeser, Arno; Wang, Liang; Collins, Karen A.; Bieryla, Allyson; Buchhave, Lars A.; Howell, Steve B.; Furlan, Elise; Girardin, Eric; Gregorio, Joao; Jensen, Eric; Murgas, Felipe (2023). "Confirmation of a Sub-Saturn-size transiting exoplanet orbiting a G dwarf: TOI-1194 b and a very low mass companion star: TOI-1251 B from TESS". arXiv:2310.12458 [astro-ph.EP].
  92. ^ Mann, Christopher; Lafreniére, David; Dragomir, Diana; Quinn, Samuel N.; Tan, Thiam-Guan; Collins, Karen A.; Howell, Steve B.; Ziegler, Carl; Mann, Andrew W.; Stassun, Keivan G.; Kristiansen, Martti H.; Osborn, Hugh; Boyajian, Tabetha; Eisner, Nora; Hellier, Coel (1 May 2023). "Validation of TOI-1221 b: A Warm Sub-Neptune Exhibiting Transit Timing Variations around a Sun-like Star". The Astronomical Journal. 165 (5): 217. arXiv:2209.13651. Bibcode:2023AJ....165..217M. doi:10.3847/1538-3881/acc8d4. ISSN 0004-6256.
  93. ^ Standing, Matthew R.; Sairam, Lalitha; Martin, David V.; Triaud, Amaury H. M. J.; Correia, Alexandre C. M.; Coleman, Gavin A. L.; Baycroft, Thomas A.; Kunovac, Vedad; Boisse, Isabelle; Andrew Collier Cameron; Dransfield, Georgina; Faria, João P.; Gillon, Michaël; Hara, Nathan C.; Hellier, Coel; Howard, Jonathan; Lane, Ellie; Mardling, Rosemary; Maxted, Pierre F. L.; Miller, Nicola J.; Nelson, Richard P.; Orosz, Jerome A.; Pepe, Franscesco; Santerne, Alexandre; Sebastian, Daniel; Udry, Stéphane; Welsh, William F. (2023). "Radial-velocity discovery of a second planet in the TOI-1338/BEBOP-1 circumbinary system". Nature Astronomy. 7 (6): 702–714. arXiv:2301.10794. Bibcode:2023NatAs...7..702S. doi:10.1038/s41550-023-01948-4. S2CID 259138442.
  94. ^ Galazutdinov, G A; Baluev, R V; Valyavin, G; Aitov, V; Gadelshin, D; Valeev, A; Sendzikas, E; Sokov, E; Mitiani, G; Burlakova, T; Yakunin, I; Antonyuk, K A; Vlasyuk, V; Romanyuk, I; Rzaev, A (9 August 2023). "Doppler confirmation of TESS planet candidate TOI−1408.01: grazing transit and likely eccentric orbit". Monthly Notices of the Royal Astronomical Society: Letters. 526 (1): L111–L115. arXiv:2309.03009. doi:10.1093/mnrasl/slad127. ISSN 1745-3925. Archived from the original on 8 December 2023. Retrieved 8 December 2023.
  95. ^ Deeg, H. J.; Georgieva, I. Y.; Nowak, G.; Persson, C. M.; Cale, B. L.; Murgas, F.; Pallé, E.; Godoy-Rivera, D.; Dai, F.; Ciardi, D. R.; Murphy, J. M. Akana; Beck, P. G.; Burke, C. J.; Cabrera, J.; Carleo, I. (September 2023). "TOI-1416: A system with a super-Earth planet with a 1.07 d period". Astronomy & Astrophysics. 677: A12. arXiv:2305.18542. Bibcode:2023A&A...677A..12D. doi:10.1051/0004-6361/202346370. ISSN 0004-6361. S2CID 258967404.
  96. ^ Yoshida, Stephanie; Vissapragada, Shreyas; Latham, David W.; Bieryla, Allyson; Thorngren, Daniel P.; Eastman, Jason D.; López-Morales, Mercedes; Barkaoui, Khalid; Beichman, Charles; Berlind, Perry; Buchave, Lars A.; Calkins, Michael L.; Ciardi, David R.; Collins, Karen A.; Cosentino, Rosario (1 November 2023). "TESS Spots a Super-puff: The Remarkably Low Density of TOI-1420b". The Astronomical Journal. 166 (5): 181. arXiv:2309.09945. Bibcode:2023AJ....166..181Y. doi:10.3847/1538-3881/acf858. ISSN 0004-6256.
  97. ^ a b González-Álvarez, E.; Zapatero Osorio, M. R.; Caballero, J. A.; Béjar, V. J. S.; Cifuentes, C.; Fukui, A.; Herrero, E.; Kawauchi, K.; Livingston, J. H.; López-González, M. J.; Morello, G.; Murgas, F.; Narita, N.; Pallé, E.; Passegger, V. M. (July 2023). "Two sub-Neptunes around the M dwarf TOI-1470". Astronomy & Astrophysics. 675: A177. arXiv:2306.08516. Bibcode:2023A&A...675A.177G. doi:10.1051/0004-6361/202346292. ISSN 0004-6361. S2CID 259165370.
  98. ^ Van Zandt, Judah; Petigura, Erik A.; MacDougall, Mason; Gilbert, Gregory J.; Lubin, Jack; Barclay, Thomas; Batalha, Natalie M.; Crossfield, Ian J. M.; Dressing, Courtney; Fulton, Benjamin; Howard, Andrew W.; Huber, Daniel; Isaacson, Howard; Kane, Stephen R.; Robertson, Paul (1 February 2023). "TESS-Keck Survey. XIV. Two Giant Exoplanets from the Distant Giants Survey". The Astronomical Journal. 165 (2): 60. arXiv:2209.06958. Bibcode:2023AJ....165...60V. doi:10.3847/1538-3881/aca6ef. ISSN 0004-6256.
  99. ^ Ghachoui, M.; Soubkiou, A.; Wells, R. D.; Rackham, B. V.; Triaud, A. H. M. J.; Sebastian, D.; Giacalone, S.; Stassun, K. G.; Ciardi, D. R.; Collins, K. A.; Liu, A.; Gómez Maqueo Chew, Y.; Gillon, M.; Benkhaldoun, Z.; Delrez, L. (1 September 2023). "TESS discovery of a super-Earth orbiting the M-dwarf star TOI-1680". Astronomy and Astrophysics. 677: A31. arXiv:2307.05368. Bibcode:2023A&A...677A..31G. doi:10.1051/0004-6361/202347040. ISSN 0004-6361. S2CID 260278487. Archived from the original on 23 November 2023. Retrieved 1 January 2024.
  100. ^ Van Zandt, Judah; Petigura, Erik A.; MacDougall, Mason; Gilbert, Gregory J.; Lubin, Jack; Barclay, Thomas; Batalha, Natalie M.; Crossfield, Ian J. M.; Dressing, Courtney; Fulton, Benjamin; Howard, Andrew W.; Huber, Daniel; Isaacson, Howard; Kane, Stephen R.; Robertson, Paul (1 February 2023). "TESS-Keck Survey. XIV. Two Giant Exoplanets from the Distant Giants Survey". The Astronomical Journal. 165 (2): 60. arXiv:2209.06958. Bibcode:2023AJ....165...60V. doi:10.3847/1538-3881/aca6ef. ISSN 0004-6256.
  101. ^ a b c Martioli, E.; Hébrard, G.; de Almeida, L.; Heidari, N.; Lorenzo-Oliveira, D.; Kiefer, F.; Almenara, J. M.; Bieryla, A.; Boisse, I.; Bonfils, X.; Briceño, C.; Collins, K. A.; Cortés-Zuleta, P.; Dalal, S.; Deleuil, M. (2023). "TOI-1736 and TOI-2141: Two systems including sub-Neptunes around solar analogs revealed by TESS and SOPHIE". Astronomy & Astrophysics. 680: A84. arXiv:2311.07011. Bibcode:2023A&A...680A..84M. doi:10.1051/0004-6361/202347744. S2CID 264471812.
  102. ^ a b c d Rodriguez, Joseph E; Quinn, Samuel N; Vanderburg, Andrew; Zhou, George; Eastman, Jason D; Thygesen, Erica; Cale, Bryson; Ciardi, David R; Reed, Phillip A; Oelkers, Ryan J; Collins, Karen A; Bieryla, Allyson; Latham, David W; Gonzales, Erica J; Scott Gaudi, B (14 March 2023). "Another shipment of six short-period giant planets from TESS". Monthly Notices of the Royal Astronomical Society. 521 (2): 2765–2785. arXiv:2205.05709. doi:10.1093/mnras/stad595. ISSN 0035-8711. Archived from the original on 8 December 2023. Retrieved 8 December 2023.
  103. ^ Dong, Jiayin; Wang, Songhu; Rice, Malena; Zhou, George; Huang, Chelsea X.; Dawson, Rebekah I.; Stefánsson, Gudmundur K.; Halverson, Samuel; Kanodia, Shubham; Mahadevan, Suvrath; McElwain, Michael W.; Alvarado-Montes, Jaime A.; Ninan, Joe P.; Robertson, Paul; Roy, Arpita (1 July 2023). "TOI-1859b: A 64 Day Warm Jupiter on an Eccentric and Misaligned Orbit". The Astrophysical Journal Letters. 951 (2): L29. arXiv:2305.16495. Bibcode:2023ApJ...951L..29D. doi:10.3847/2041-8213/acd93d. ISSN 2041-8205.
  104. ^ a b c d e f g h i j k l m n o p q r s t Yee, Samuel W.; Winn, Joshua N.; Hartman, Joel D.; Bouma, Luke G.; Zhou, George; Quinn, Samuel N.; Latham, David W.; Bieryla, Allyson; Rodriguez, Joseph E.; Collins, Karen A.; Alfaro, Owen; Barkaoui, Khalid; Beard, Corey; Belinski, Alexander A.; Benkhaldoun, Zouhair (1 March 2023). "The TESS Grand Unified Hot Jupiter Survey. II. Twenty New Giant Planets*". The Astrophysical Journal Supplement Series. 265 (1): 1. arXiv:2210.15473. Bibcode:2023ApJS..265....1Y. doi:10.3847/1538-4365/aca286. ISSN 0067-0049.
  105. ^ a b Sha, Lizhou; Vanderburg, Andrew M; Huang, Chelsea X; Armstrong, David J; Brahm, Rafael; Giacalone, Steven; Wood, Mackenna L; Collins, Karen A; Nielsen, Louise D; Hobson, Melissa J; Ziegler, Carl; Howell, Steve B; Torres-Miranda, Pascal; Mann, Andrew W; Zhou, George (4 July 2023). "TESS spots a mini-neptune interior to a hot saturn in the TOI-2000 system". Monthly Notices of the Royal Astronomical Society. 524 (1): 1113–1138. arXiv:2209.14396. doi:10.1093/mnras/stad1666. ISSN 0035-8711.
  106. ^ Mann, Christopher R.; Dalba, Paul A.; Lafrenière, David; Fulton, Benjamin J.; Hébrard, Guillaume; Boisse, Isabelle; Dalal, Shweta; Deleuil, Magali; Delfosse, Xavier; Demangeon, Olivier; Forveille, Thierry; Heidari, Neda; Kiefer, Flavien; Martioli, Eder; Moutou, Claire (1 December 2023). "Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. III. Recovery and Confirmation of a Temperate, Mildly Eccentric, Single-transit Jupiter Orbiting TOI-2010". The Astronomical Journal. 166 (6): 239. arXiv:2311.10232. Bibcode:2023AJ....166..239M. doi:10.3847/1538-3881/ad00bc. ISSN 0004-6256.
  107. ^ Jones, Sinclaire E.; Stefánsson, Guðmundur; Masuda, Kento; Libby-Roberts, Jessica E.; Gardner, Cristilyn N.; Holcomb, Rae; Beard, Corey; Robertson, Paul; Cañas, Caleb I.; Mahadevan, Suvrath; Kanodia, Shubham; Lin, Andrea S. J.; Kobulnicky, Henry A.; Parker, Brock A.; Bender, Chad F.; Cochran, William D.; Diddams, Scott A.; Fernandes, Rachel B.; Gupta, Arvind F.; Halverson, Samuel; Hawley, Suzanne L.; Hearty, Fred R.; Hebb, Leslie; Kowalski, Adam; Lubin, Jack; Monson, Andrew; Ninan, Joe P.; Ramsey, Lawrence; Roy, Arpita; Schwab, Christian; Terrien, Ryan C.; Wisniewski, John (9 May 2024). "TOI-2015b: A Warm Neptune with Transit Timing Variations Orbiting an Active mid M Dwarf". arXiv:2310.11775 [astro-ph.EP].
  108. ^ a b Barkaoui, K.; Timmermans, M.; Soubkiou, A.; Rackham, B. V.; Burgasser, A. J.; Chouqar, J.; Pozuelos, F. J.; Collins, K. A.; Howell, S. B.; Simcoe, R.; Melis, C.; Stassun, K. G.; Tregloan-Reed, J.; Cointepas, M.; Gillon, M. (September 2023). "TOI-2084 b and TOI-4184 b: Two new sub-Neptunes around M dwarf stars". Astronomy & Astrophysics. 677: A38. arXiv:2306.15095. Bibcode:2023A&A...677A..38B. doi:10.1051/0004-6361/202346838. ISSN 0004-6361. S2CID 259262549.
  109. ^ a b Quintana, Elisa V.; et al. (2023). "Two Warm Super-Earths Transiting the Nearby M Dwarf, TOI-2095". The Astronomical Journal. 166 (5): 195. arXiv:2304.09189. Bibcode:2023AJ....166..195Q. doi:10.3847/1538-3881/acfa9f.
  110. ^ a b Murgas, F.; et al. (2023). "Two super-Earths at the edge of the habitable zone of the nearby M dwarf TOI-2095". Astronomy & Astrophysics. 677: A182. arXiv:2304.09220. Bibcode:2023A&A...677A.182M. doi:10.1051/0004-6361/202346692. S2CID 258212464.
  111. ^ a b Pozuelos, F. J.; et al. (2023). "A super-Earth and a mini-Neptune near the 2:1 MMR straddling the radius valley around the nearby mid-M dwarf TOI-2096". Astronomy & Astrophysics. 672: A70. arXiv:2303.08174. Bibcode:2023A&A...672A..70P. doi:10.1051/0004-6361/202245440. S2CID 256927017.
  112. ^ a b Rescigno, F; Hébrard, G; Vanderburg, A; Mann, A W; Mortier, A; Morrell, S; Buchhave, L A; Collins, K A; Mann, C R; Hellier, C; Haywood, R D; West, R; Stalport, M; Heidari, N; Anderson, D (27 November 2023). "A hot mini-Neptune and a temperate, highly eccentric sub-Saturn around the bright K-dwarf TOI-2134". Monthly Notices of the Royal Astronomical Society. 527 (3): 5385–5407. doi:10.1093/mnras/stad3255. hdl:10023/28862. ISSN 0035-8711. Archived from the original on 8 December 2023. Retrieved 8 December 2023.
  113. ^ a b c Brahm, Rafael; et al. (2023). "Three Long-period Transiting Giant Planets from TESS". The Astronomical Journal. 165 (6): 227. arXiv:2304.02139. Bibcode:2023AJ....165..227B. doi:10.3847/1538-3881/accadd. S2CID 257952381.
  114. ^ Frame, Ginger; Armstrong, David J; Cegla, Heather M; Fernández Fernández, Jorge; Osborn, Ares; Adibekyan, Vardan; Collins, Karen A; Delgado Mena, Elisa; Giacalone, Steven; Kielkopf, John F; Santos, Nuno C; Sousa, Sérgio G; Stassun, Keivan G; Ziegler, Carl; Anderson, David R (23 May 2023). "TOI-2498 b: a hot bloated super-Neptune within the Neptune desert". Monthly Notices of the Royal Astronomical Society. 523 (1): 1163–1174. arXiv:2305.06950. doi:10.1093/mnras/stad1452. ISSN 0035-8711. Archived from the original on 9 December 2023. Retrieved 9 December 2023.
  115. ^ a b Trifonov, Trifon; et al. (2023). "TOI-2525 b and c: A Pair of Massive Warm Giant Planets with Strong Transit Timing Variations Revealed by TESS". The Astronomical Journal. 165 (4): 179. arXiv:2302.05694. Bibcode:2023AJ....165..179T. doi:10.3847/1538-3881/acba9b. S2CID 256827169.
  116. ^ Hobson, Melissa J.; et al. (2023). "TOI-3235 b: A Transiting Giant Planet around an M4 Dwarf Star". The Astrophysical Journal Letters. 946 (1): L4. arXiv:2302.10008. Bibcode:2023ApJ...946L...4H. doi:10.3847/2041-8213/acbd9a. S2CID 257038386.
  117. ^ Powers, Luke C.; Libby-Roberts, Jessica; Lin, Andrea S. J.; Cañas, Caleb I.; Kanodia, Shubham; Mahadevan, Suvrath; Ninan, Joe P.; Stefánsson, Guðmundur; Gupta, Arvind F.; Jones, Sinclaire; Kobulnicky, Henry A.; Monson, Andrew; Parker, Brock A.; Swaby, Tera N.; Bender, Chad F.; Cochran, William D.; Hebb, Leslie; Metcalf, Andrew J.; Robertson, Paul; Schwab, Christian; Wisniewski, John; Wright, Jason T. (2023). "TOI-3785 b: A Low-density Neptune Orbiting an M2-dwarf Star". The Astronomical Journal. 166 (2): 44. arXiv:2304.04730. Bibcode:2023AJ....166...44P. doi:10.3847/1538-3881/acd8bf. S2CID 258048476.
  118. ^ a b Cañas, Caleb I.; et al. (2023). "TOI-3984 a b and TOI-5293 a b: Two Temperate Gas Giants Transiting Mid-M Dwarfs in Wide Binary Systems". The Astronomical Journal. 166 (1): 30. arXiv:2302.07714. Bibcode:2023AJ....166...30C. doi:10.3847/1538-3881/acdac7. S2CID 256868404.
  119. ^ a b c d Kunimoto, Michelle; Vanderburg, Andrew; Huang, Chelsea X.; Davis, M. Ryleigh; Affer, Laura; Cameron, Andrew Collier; Charbonneau, David; Cosentino, Rosario; Damasso, Mario; Dumusque, Xavier; Fiorenzano, A. F. Martnez; Ghedina, Adriano; Haywood, R. D.; Lienhard, Florian; López-Morales, Mercedes (1 July 2023). "TOI-4010: A System of Three Large Short-period Planets with a Massive Long-period Companion". The Astronomical Journal. 166 (1): 7. arXiv:2306.05308. Bibcode:2023AJ....166....7K. doi:10.3847/1538-3881/acd537. ISSN 0004-6256.
  120. ^ Gupta, Arvind F.; et al. (2023). "A High-Eccentricity Warm Jupiter Orbiting TOI-4127". The Astronomical Journal. 165 (6): 234. arXiv:2303.14570. Bibcode:2023AJ....165..234G. doi:10.3847/1538-3881/accb9b. S2CID 257766926.
  121. ^ Delamer, Megan; Kanodia, Shubham; Cañas, Caleb I.; et al. (2024). "TOI-4201: An Early M-dwarf Hosting a Massive Transiting Jupiter Stretching Theories of Core-Accretion". The Astrophysical Journal. 962 (2): L22. arXiv:2307.06880. Bibcode:2024ApJ...962L..22D. doi:10.3847/2041-8213/ad1a19.
  122. ^ "The Extrasolar Planet Encyclopaedia — Planet TOI-4201 b". Extrasolar Planets Encyclopaedia. 23 October 1995. Retrieved 19 July 2023.
  123. ^ a b Tey, Evan; Huang, Chelsea X.; et al. (January 2023). "TESS Discovery of Twin Planets near 2:1 Resonance around Early M-Dwarf TOI 4342". The Astronomical Journal. 165 (3): 93. arXiv:2301.01370. Bibcode:2023AJ....165...93T. doi:10.3847/1538-3881/acaf88. S2CID 255416187.
  124. ^ a b Pereira, Filipe; Grunblatt, Samuel K; Psaridi, Angelica; Campante, Tiago L; Cunha, Margarida S; Santos, Nuno C; Bossini, Diego; Thorngren, Daniel; Hellier, Coel; Bouchy, François; Lendl, Monika; Mounzer, Dany; Udry, Stéphane; Beard, Corey; Brinkman, Casey L (27 November 2023). "TESS giants transiting giants V – two hot Jupiters orbiting red giant hosts". Monthly Notices of the Royal Astronomical Society. 527 (3): 6332–6345. arXiv:2311.06678. doi:10.1093/mnras/stad3449. ISSN 0035-8711. Archived from the original on 9 December 2023. Retrieved 9 December 2023.
  125. ^ Carleo, I.; Malavolta, L.; Desidera, S.; Nardiello, D.; Wang, S.; Turrini, D.; Lanza, A. F.; Baratella, M.; Marzari, F.; Benatti, S.; Biazzo, K.; Bieryla, A.; Brahm, R.; Bonavita, M.; Collins, K. A. (1 February 2024). "The GAPS programme at TNG. L. TOI-4515 b: An eccentric warm Jupiter orbiting a 1.2 Gyr-old G-star". Astronomy and Astrophysics. 682: A135. arXiv:2311.11903. Bibcode:2024A&A...682A.135C. doi:10.1051/0004-6361/202348207. ISSN 0004-6361.
  126. ^ Heitzmann, Alexis; Zhou, George; Quinn, Samuel N.; Huang, Chelsea X.; Dong, Jiayin; Bouma, L. G.; Dawson, Rebekah I.; Marsden, Stephen C.; Wright, Duncan; Petit, Pascal; Collins, Karen A.; Barkaoui, Khalid; Wittenmyer, Robert A.; Gillen, Edward; Brahm, Rafael (1 March 2023). "TOI-4562b: A Highly Eccentric Temperate Jupiter Analog Orbiting a Young Field Star". The Astronomical Journal. 165 (3): 121. arXiv:2208.10854. Bibcode:2023AJ....165..121H. doi:10.3847/1538-3881/acb5a2. ISSN 0004-6256.
  127. ^ Grunblatt, Samuel K.; Saunders, Nicholas; Chontos, Ashley; Hattori, Soichiro; Veras, Dimitri; Huber, Daniel; Angus, Ruth; Rice, Malena; Breivik, Katelyn; Blunt, Sarah; Giacalone, Steven; Lubin, Jack; Isaacson, Howard; Howard, Andrew W.; Ciardi, David R. (1 February 2023). "TESS Giants Transiting Giants. III. An Eccentric Warm Jupiter Supports a Period−Eccentricity Relation for Giant Planets Transiting Evolved Stars". The Astronomical Journal. 165 (2): 44. arXiv:2210.17062. Bibcode:2023AJ....165...44G. doi:10.3847/1538-3881/aca670. ISSN 0004-6256.
  128. ^ a b Mireles, Ismael; Dragomir, Diana; Osborn, Hugh P.; et al. (30 August 2023). "TOI-4600 b and c: Two Long-period Giant Planets Orbiting an Early K Dwarf". The Astrophysical Journal Letters. 954 (1). American Astronomical Society: L15. arXiv:2308.15572. Bibcode:2023ApJ...954L..15M. doi:10.3847/2041-8213/aceb69. ISSN 2041-8205.
  129. ^ Khandelwal, Akanksha; Sharma, Rishikesh; Chakraborty, Abhijit; Chaturvedi, Priyanka; Ulmer-Moll, Solène; Ciardi, David R.; Boyle, Andrew W.; Baliwal, Sanjay; Bieryla, Allyson; Latham, David W.; Prasad, Neelam J. S. S. V.; Nayak, Ashirbad; Lendl, Monika; Mordasini, Christoph (2023). "Discovery of a massive giant planet with extreme density around the sub-giant star TOI-4603". Astronomy & Astrophysics. 672: L7. arXiv:2303.11841. Bibcode:2023A&A...672L...7K. doi:10.1051/0004-6361/202245608. S2CID 257637141.
  130. ^ Triaud, Amaury H M J; Dransfield, Georgina; Kagetani, Taiki; Timmermans, Mathilde; Narita, Norio; Barkaoui, Khalid; Hirano, Teruyuki; Rackham, Benjamin V; Mori, Mayuko; Baycroft, Thomas; Benkhaldoun, Zouhair; Burgasser, Adam J; Caldwell, Douglas A; Collins, Karen A; Davis, Yasmin T (4 July 2023). "An M dwarf accompanied by a close-in giant orbiter with SPECULOOS". Monthly Notices of the Royal Astronomical Society: Letters. 525 (1): L98–L104. arXiv:2308.02253. doi:10.1093/mnrasl/slad097. ISSN 1745-3925. Archived from the original on 9 December 2023. Retrieved 9 December 2023.
  131. ^ a b Fairnington, Tyler R; Nabbie, Emma; Huang, Chelsea X; Zhou, George; Foo, Orion; Millholland, Sarah; Wright, Duncan; Belinski, Alexandre A; Bieryla, Allyson; Ciardi, David R; Collins, Karen A; Collins, Kevin I; Everett, Mark; Howell, Steve B; Lissauer, Jack J (9 October 2023). "TOI-5126: A hot super-Neptune and warm Neptune pair discovered by TESS and CHEOPS". Monthly Notices of the Royal Astronomical Society. 527 (3): 8768–8783. doi:10.1093/mnras/stad3036. ISSN 0035-8711.
  132. ^ Kanodia, Shubham; Mahadevan, Suvrath; Libby-Roberts, Jessica; Stefansson, Gudmundur; Cañas, Caleb I.; Piette, Anjali A. A.; Boss, Alan; Teske, Johanna; Chambers, John; Zeimann, Greg; Monson, Andrew; Robertson, Paul; Ninan, Joe P.; Lin, Andrea S. J.; Bender, Chad F. (1 March 2023). "TOI-5205b: A Short-period Jovian Planet Transiting a Mid-M Dwarf". The Astronomical Journal. 165 (3): 120. arXiv:2209.11160. Bibcode:2023AJ....165..120K. doi:10.3847/1538-3881/acabce. ISSN 0004-6256.
  133. ^ Hartman, J. D.; Bakos, G. á.; Csubry, Z.; Howard, A. W.; Isaacson, H.; Giacalone, S.; Chontos, A.; Narita, N.; Fukui, A.; de Leon, J. P.; Watanabe, N.; Mori, M.; Kagetani, T.; Fukuda, I.; Kawai, Y. (1 October 2023). "TOI 4201 b and TOI 5344 b: Discovery of Two Transiting Giant Planets around M-dwarf Stars and Revised Parameters for Three Others". The Astronomical Journal. 166 (4): 163. arXiv:2307.06809. Bibcode:2023AJ....166..163H. doi:10.3847/1538-3881/acf56e. ISSN 0004-6256.
  134. ^ Mantovan, G.; Malavolta, L.; Desidera, S.; Zingales, T.; Borsato, L.; Piotto, G.; Maggio, A.; Locci, D.; Polychroni, D.; Turrini, D.; Baratella, M.; Biazzo, K.; Nardiello, D.; Stassun, K.; Nascimbeni, V. (2023). "The GAPS programme at TNG XLIX. TOI-5398, the youngest compact multi-planet system composed of an inner sub-Neptune and an outer warm Saturn". Astronomy and Astrophysics. 682. arXiv:2310.16888. Bibcode:2024A&A...682A.129M. doi:10.1051/0004-6361/202347472.
  135. ^ Ulmer-Moll, S.; Osborn, H. P.; Tuson, A.; Egger, J. A.; Lendl, M.; Maxted, P.; Bekkelien, A.; Simon, A. E.; Olofsson, G.; Adibekyan, V.; Alibert, Y.; Bonfanti, A.; Bouchy, F.; Brandeker, A.; Fridlund, M. (June 2023). "TOI-5678b: A 48-day transiting Neptune-mass planet characterized with CHEOPS and HARPS". Astronomy & Astrophysics. 674: A43. arXiv:2306.04295. Bibcode:2023A&A...674A..43U. doi:10.1051/0004-6361/202245478. ISSN 0004-6361. S2CID 259095853.
  136. ^ Maciejewski, G; Golonka, J; Łoboda, W; Ohlert, J; Fernández, M; Aceituno, F (4 July 2023). "A hot super-Earth planet in the WASP-84 planetary system". Monthly Notices of the Royal Astronomical Society: Letters. 525 (1): L43–L49. arXiv:2305.09177. doi:10.1093/mnrasl/slad078. ISSN 1745-3925. Archived from the original on 1 January 2024. Retrieved 9 December 2023.
  137. ^ Barkaoui, Khalid; Pozuelos, Francisco J.; Hellier, Coel; Smalley, Barry; Nielsen, Louise D.; Dorn, Caroline; Niraula, Prajwal; Gillon, Michaël; de Wit, Julien; Helled, Ravit; Müller, Simon; Jehin, Emmanuel; Demory, Brice-Olivier; Van Grootel, V.; Soubkiou, Abderahmane (2023). "WASP-193b: An extremely low-density super-Neptune". Astrophysics. arXiv:2307.08350. doi:10.1038/s41550-024-02259-y.
  138. ^ Calissendorff, Per; De Furio, Matthew; Meyer, Michael; Albert, Loïc; Aganze, Christian; Ali-Dib, Mohamad; Bardalez Gagliuffi, Daniella C.; Baron, Frederique; Beichman, Charles A.; Burgasser, Adam J.; Cushing, Michael C.; Faherty, Jacqueline Kelly; Fontanive, Clémence; Gelino, Christopher R.; Gizis, John E. (1 April 2023). "JWST/NIRCam Discovery of the First Y+Y Brown Dwarf Binary: WISE J033605.05–014350.4". The Astrophysical Journal Letters. 947 (2): L30. arXiv:2303.16923. Bibcode:2023ApJ...947L..30C. doi:10.3847/2041-8213/acc86d. ISSN 2041-8205.
  139. ^ Kossakowski, D.; et al. (2023). "The CARMENES search for exoplanets around M dwarfs. Wolf 1069 b: Earth-mass planet in the habitable zone of a nearby, very low-mass starr". Astronomy & Astrophysics. 670. arXiv:2301.02477. Bibcode:2023A&A...670A..84K. doi:10.1051/0004-6361/202245322. S2CID 265978789.
  140. ^ "The Extrasolar Planet Encyclopaedia — Wolf 1069 b". Extrasolar Planets Encyclopaedia. 23 October 1995. Archived from the original on 1 January 2024. Retrieved 9 January 2023.

Licensed under CC BY-SA 3.0 | Source: https://en.wikipedia.org/wiki/List_of_exoplanets_discovered_in_2023
9 views |
Download as ZWI file
Encyclosphere.org EncycloReader is supported by the EncyclosphereKSF