List of exoplanets discovered in 2023
Appearance
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 Cet 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] | |||
HD 6860 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 Beta Andromedae[22] | ||
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 | [23] | |
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 | [23] | |
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 | [24] | ||
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 | [25] |
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 | [26] | ||
HD 73256 c | 16±1 | 2690+60 −102 |
3.8±0.1 | radial vel. | 119.7253+0.1833 −0.1823 |
1.00±0.05 | [27] | |||
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 | [27] | |||
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 | [28] | ||
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[29] | |||
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 | [27] | |||
HD 112300 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 | [30] | ||
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 | [27] | |||
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 | [27] | |||
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 | [27] | |||
HD 169142 b | 3±2 | 37.2±1.5 | imaging | 435.744+2.717 −2.674 |
1.85 | [31] | ||||
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 | [27] | |||
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 | [32] |
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[33] | |
HIP 9618 b | 0.0315±0.0098 | 3.900±0.044 | 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 | [34] |
HIP 9618 c | <0.0576±0.0053 | 3.343±0.039 | 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 | [34] |
HIP 29442 b | 0.032±0.0025 | 3.48+0.07 −0.08 |
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[35] |
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 | [35] |
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 | [35] |
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 | [27] | |||
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 |
[36] | ||
HIP 99770 b | 16.1+5.4 −5.0 |
1.09 | 18600+6200 −2800 |
16.9+3.4 −1.9 |
imaging | 131 | 0.291±0.013 | 8000 | Gas giant.[37][38] | |
HIP 113103 b | 1.829+0.096 −0.067 |
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 | [39] | |
HIP 113103 c | 2.40+0.10 −0.08 |
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 | [39] | |
HN Lib 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[40] | |
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 | [41] | ||
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 | [42] |
K2-416 b | <5.2 | 2.66+0.19 −0.14 |
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 | [43] |
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 | [43] |
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.[44][45] | ||
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 | [41] | ||
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 | [46] | |||
Kepler-58 d | 0.1509503920 | 4.458169937 | transit | 1.017 +0.167 −0.125 |
6100+193 −214 |
[47] | ||||
Kepler-164 e | 0.3570351276 | 94.8864975 | transit | 0.966 +0.075 −0.068 |
5888 +106 −117 |
[47] | ||||
Kepler-290 d | 0.0794273806 | 0.764007986 | transit | 0.84 +0.065 −0.09 |
5142±153 | [47] | ||||
Kepler-297 d | 0.6351157298 | 150.0209961 | transit | 0.846 +0.059 −0.049 |
5618±112 | [47] | ||||
Kepler-311 d | 0.1849409870 | 232.0469971 | transit | 0.974 +0.082 −0.062 |
5903 +106 −117 |
[47] | ||||
Kepler-347 d | 0.2346332985 | 85.51660156 | transit | 1±0.072 | 5592±75 | [47] | ||||
Kepler-416 d | 0.1543405297 | 3.076410055 | transit | 0.949 +0.067 −0.055 |
5670±114 | [47] | ||||
Kepler-549 d | 0.4055676538 | 24.6147995 | transit | 0.859 +0.06 −0.033 |
5312±79 | [47] | ||||
Kepler-618 d | 0.3911149410 | 11.67889977 | transit | 1.041±0.139 | 6122 +169 −190 |
[47] | ||||
Kepler-656 c | 0.1360516194 | 5.254559994 | transit | 1.05+0.075 −0.113 |
5550 +166 −183 |
[47] | ||||
Kepler-763 c | 0.1464004690 | 4.096680164 | transit | 0.8 +0.048 −0.028 |
4999±79 | [47] | ||||
Kepler-763 d | 0.1754842890 | 6.503270149 | transit | 0.8 +0.048 −0.028 |
4999±79 | [47] | ||||
Kepler-784 c | 0.1583551639 | 17.15699959 | transit | 1.016 +0.093 −0.084 |
5676 +115 −104 |
[47] | ||||
Kepler-864 c | 0.157641449 | 2.421489954 | transit | 1.27 +0.142 −0.156 |
6213 +173 −259 |
[47] | ||||
Kepler-865 c | 0.09474546031 | 6.209179878 | transit | 0.782 +0.116 −0.062 |
5440±162 | [47] | ||||
Kepler-880 c | 0.2816491659 | 11.80609989 | transit | 1.714 +0.17 −0.316 |
6900 +184 −204 |
[47] | ||||
Kepler-896 c | 0.2770100246 | 29.54210091 | transit | 0.877 +0.083 −0.092 |
5510 +166 −149 |
[47] | ||||
Kepler-949 c | 0.4607912263 | 20.99720001 | transit | 0.813 +0.104 −0.064 |
5211 +181 −163 |
[47] | ||||
Kepler-975 c | 0.5035248257 | 5.05821991 | transit | 0.951 +0.198 −0.144 |
4883 +146 −132 |
[47] | ||||
Kepler-1052 c | 0.2112591764 | 180.9259949 | transit | 0.937 +0.09 −0.121 |
5818 +139 −157 |
[47] | ||||
Kepler-1126 c | 0.1500582511 | 199.6679993 | transit | 0.794 +0.071 −0.03 |
5678 +113 −102 |
[47] | ||||
Kepler-1162 c | 0.1675442283 | 59.28409958 | transit | 0.861 +0.05 −0.041 |
5225 +83 −73 |
[47] | ||||
Kepler-1181 c | 0.1555895228 | 8.934909821 | transit | 1.336 ±0.2 | 6688 +187 −281 |
[47] | ||||
Kepler-1471 c | 0.2001966118 | 11.60449982 | transit | 0.934 +0.063 −0.045 |
5533 +83 −74 |
[47] | ||||
Kepler-1487 c | 0.7992697886 | 35.79949951 | transit | 1.801 +0.193 −0.359 |
5745 +86 −77 |
[47] | ||||
Kepler-1491 c | 0.2788835142 | 61.5685997 | transit | 0.991 +0.079 −0.065 |
5626±77 | [47] | ||||
Kepler-1513 c | 0.266 +0.098 −0.063 |
841.4+8.1 −5.3 |
transit | 0.943±0.037 | 5491±100 | [48] | ||||
Kepler-1518 c | 0.212775814 | 9.630929947 | transit | 1.06 +0.177 −0.133 |
6432+155 −214 |
[47] | ||||
Kepler-1610 c | 0.196806485 | 44.98529816 | transit | 0.825 +0.096 −0.078 |
5295±185 | [47] | ||||
Kepler-1669 d | 0.1427426870 | 4.729469776 | transit | 0.609 ±0.033 | 4224±84 | [47] | ||||
Kepler-1801 c | 0.3621203501 | 116.5849991 | transit | 0.936 +0.114 −0.093 |
5738 +156 −173 |
[47] | ||||
Kepler-1814 c | 0.1476494621 | 0.626281977 | transit | 0.79 +0.073 −0.064 |
4922±169 | [47] | ||||
Kepler-1834 c | 0.129895841 | 0.766691983 | transit | 0.765 +0.051 −0.028 |
4821±76 | [47] | ||||
Kepler-1859 c | 0.1531807444 | 3.596430063 | transit | 1.09 +0.07 −0.078 |
5887 +70 −79 |
[47] | ||||
Kepler-1894 c | 0.1417613278 | 5.053750038 | transit | 0.999 +0.114 −0.125 |
5772 +156 −173 |
[47] | ||||
Kepler-1921 c | 0.1505043216 | 3.157219887 | transit | 1.251 +0.19 −0.233 |
6120 +195 −217 |
[47] | ||||
Kepler-1976 b | 1.043 | 4.96 | transit | 1.097 +0.21 −0.135 |
6117 +156 −210 |
[49] | ||||
Kepler-1977 b | 0.1625482348 | 4.537000179 | transit | 0.769 +0.053 −0.079 |
4805 ±144 | [47] | ||||
Kepler-1978 b | 0.2683562384 | 10.849699997 | transit | 0.869 +0.06 −0.095 |
5251±158 | [47] | ||||
Kepler-1980 b | 0.2538143392 | 33.0257988 | transit | 1.049 +0.059 −0.073 |
5819 +69 −87 |
[47] | ||||
Kepler-1981 b | 0.8396838173 | 453.5429993 | transit | 1.519 +0.15 −0.376 |
5874 +87 −79 |
[47] | ||||
Kepler-1982 b | 0.773130047 | 3.823159933 | transit | 1.213 +0.076 −0.093 |
6202 +99 −149 |
[47] | ||||
Kepler-1983 b | 0.1465788952 | 7.328519821 | transit | 0.812 +0.058 −0.029 |
5135 +84 −75 |
[47] | ||||
Kepler-1984 b | 0.718709408 | 1.99285996 | transit | 0.42 +0.046 −0.056 |
3638 +72 −87 |
[47] | ||||
Kepler-1985 b | 0.1981446855 | 3.420650005 | transit | 0.877 +0.064 −0.037 |
3638 +72 −87 |
[47] | ||||
Kepler-1986 b | 0.2631818295 | 19.54929924 | transit | 0.776 +0.089 −0.065 |
5549±163 | [47] | ||||
Kepler-1987 b | 0.134713408 | 2.345860004 | transit | 0.799 +0.041 −0.081 |
4769±172 | [47] | ||||
Kepler-1987 c | 0.151307244 | 3.648269892 | transit | 0.799 +0.041 −0.081 |
4769±172 | [47] | ||||
Kepler-1987 d | 0.2912843007 | 5.644889832 | transit | 0.799 +0.041 −0.081 |
4769±172 | [47] | ||||
Kepler-1987 e | 0.2188423849 | 8.742970467 | transit | 0.799 +0.041 −0.081 |
4769±172 | [47] | ||||
Kepler-1988 b | 0.1382819717 | 1.549999952 | transit | 1.127 +0.189 −0.172 |
6033±183 | [47] | ||||
Kepler-1989 b | 0.4247487156 | 10.16100025 | transit | 0.999 +0.153 −0.126 |
6032 +189 −232 |
[47] | ||||
Kepler-1990 b | 0.3491842959 | 1.735129952 | transit | 1.028 +0.074 −0.067 |
5751 +103 −114 |
[47] | ||||
Kepler-1990 c | 0.1058972326 | 1.187000036 | transit | 1.028 +0.074 −0.067 |
5751 +103 −114 |
[47] | ||||
Kepler-1991 b | 0.1646893688 | 13.26080036 | transit | 0.914 +0.061 −0.042 |
5478 +82 −74 |
[47] | ||||
Kepler-1991 c | 0.2594348291 | 22.79019928 | transit | 0.914 +0.061 −0.042 |
5478 +82 −74 |
[47] | ||||
Kepler-1992 b | 0.0916229564 | 15.61120033 | transit | 0.874 +0.048 −0.054 |
5383±107 | [47] | ||||
Kepler-1993 b | 0.3949511704 | 26.65660095 | transit | 1.373 +0.205 −0.512 |
5159 +171 −155 |
[47] | ||||
Kepler-1994 b | 0.0555001398 | 4.612319946 | transit | 0.932 +0.052 −0.047 |
5495 +74 −82 |
[47] | ||||
Kepler-1995 b | 0.4119018693 | 73.75779724 | transit | 0.847 +0.068 −0.049 |
5029 +192 −174 |
[47] | ||||
Kepler-1996 b | 0.204657316 | 32.37609863 | transit | 0.748 +0.027 −0.043 |
4580±92 | [47] | ||||
Kepler-1996 c | 0.2509594797 | 92.72949982 | transit | 0.748 +0.027 −0.043 |
4580±92 | [47] | ||||
Kepler-1997 b | 0.2179502440 | 26.75749969 | transit | 1.111±0.153 | 6215 +194 −259 |
[47] | ||||
Kepler-1998 b | 0.0619324805 | 3.03263998 | transit | 0.962 +0.054 −0.068 |
5640 +101 −113 |
[47] | ||||
Kepler-1999 b | 0.3169779722 | 8.739450455 | transit | 0.632 +0.063 −0.057 |
4406 +154 −170 |
[47] | ||||
Kepler-2000 b | 0.2961910652 | 6.383150101 | transit | 0.581±0.029 | 3757 +74 −82 |
[47] | ||||
Kepler-2000 c | 0.1963604037 | 20.6182003 | transit | 0.581±0.029 | 3757 +74 −82 |
[47] | ||||
Kepler-2001 b | 0.1062540847 | 1.190999985 | transit | 0.864 +0.049 −0.085 |
5081 +166 −136 |
[47] | ||||
Kepler-2001 c | 0.3639938397 | 14.09449959 | transit | 0.864 +0.049 −0.085 |
5081 +166 −136 |
[47] | ||||
KMT-2016-BLG-0625L b | 0.05±0.04 | 1.40±0.17 | microlensing | 21000±2000 | 0.25±0.14 | [50] | ||||
KMT-2016-BLG-1105L b | 0.00415±0.00176 | 2.26+0.51 −0.69 |
microlensing | 10665+4175 −3751 |
0.43±0.18 | [51] | ||||
KMT-2016-BLG-1751L b | 1.20±1.21 | 1.39±0.50 | microlensing | 23000±4000 | 0.18±0.18 | [50] | ||||
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 |
[51] | ||||
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 |
[51] | ||||
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 |
[51] | ||||
KMT-2019-BLG-0298L b | 1.81±0.96 | 5.67±2.70 | microlensing | 22000±5000 | 0.70±0.37 | [52] | ||||
KMT-2019-BLG-1216L b | 0.094±0.050 | 2.44±1.12 | microlensing | 9000±3000 | 0.39±0.21 | [52] | ||||
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 |
[51] | ||||
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 |
[51] | ||||
KMT-2019-BLG-2783L b | 1.16±0.77 | 1.85±0.93 | microlensing | 19000±5000 | 0.34±0.25 | [52] | ||||
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 |
[53] | ||||
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 |
[53] | ||||
KMT-2021-BLG-1105L b | 1.30±0.68 | 3.54±1.06 | microlensing | 14807±5447 | 0.63±0.33 | [53] | ||||
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[54] | ||||
KMT-2021-BLG-2478L b | 0.900+0.420 −0.240 |
1.85±0.31 | microlensing | 9687±2348 | 0.20+0.10 −0.05 |
[53] | ||||
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[54] | ||||
KMT-2022-BLG-0440L b | 0.0485+0.0302 −0.0233 |
1.9±0.7 | microlensing | 11000±5000 | 0.53+0.31 −0.26 |
[55][56] | ||||
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 |
[54] | ||||
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 | [57] | |
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 | [58] | ||
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 | [59][60] Host star also known as TOI-910[61] Also the first exoplanet confirmed by the James Webb Space Telescope.[62] |
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 | [63] |
MOA-2016-BLG-0532L b | 0.39±0.31 | 1.09±0.17 | microlensing | 24000±2000 | 0.09±0.07 | [50] | ||||
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 |
[64] | ||||
MOA-2022-BLG-249Lb | 0.015±0.005 | 1.63±0.35 | microlensing | 6500±1400 | 0.18±0.05 | [65] | ||||
MWC 758 c | 100 | 500±100 | imaging | 159.537 +1.742 −1.706 |
1.5 | [66] | ||||
OGLE-2016-BLG-1635L b | 11.49±7.96 | 1.34±0.47 | microlensing | 22000±5000 | 0.43±0.29 | [50] | ||||
OGLE-2016-BLG-1850L b | 0.03±0.01 | 1.46±0.16 | microlensing | 7000±2000 | 0.26±0.11 | [50] | ||||
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 |
[67] | ||||
OGLE-2019-BLG-0249L b | 7.12±1.47 | 1.84±0.44 | microlensing | 21000±3000 | 0.91±0.19 | [52] | ||||
OGLE-2019-BLG-0679L b | 3.34±1.90 | 6.99±3.21 | microlensing | 18000±6000 | 0.66±0.38 | [52] | ||||
PZ Telescopii b | 27+25 −9 |
44000+40000 −10000 |
27+14 −4 |
imaging | 153.505+0.439 −0.436 |
1.36+0.15 −0.13 |
[68] | |||
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 | [69] | ||
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 | [69] | ||
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 | [70] | |
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 | [70] | ||
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 of high temperature and low mass[71] | |
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 | [72] | |
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 | [73] |
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 | [74] | |
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 |
[75] | |
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 |
[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 | [77] | |
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 | [72] | |
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 | [78] |
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 | [79] | |
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 | [79] | |
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 | [80] |
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 | [80] |
TOI-672 b | 0.0760 | 0.470+0.008 −0.009 |
3.633575±0.000001 | 676.15 | transit | 0.5399±0.0204 | 3765±65 | [72] | ||
TOI-700 e | 0.0025730809[81] | 0.08502+0.00794 −0.00669 |
27.80978+0.00046 −0.0004 |
0.134±0.0022 | 3500[82] | transit | 101.52 | 0.416±0.01 | 3480±135 | Habitable zone planet[83][84] |
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 | [85] | |
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 | [86] |
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 |
140±0.05 | 6643±150 | [87] |
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.[88] | |
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 | [89] |
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 | [89] |
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 |
[90] |
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 | [91] |
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 | [72] | |
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 | [92] |
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 | [92] | |
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 |
[93] |
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 | [94] |
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[95] | ||
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 | [96] | |
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 | [72] | |
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 | [97] |
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 | [98] |
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 | [99] |
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 | [99] |
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 | [100] | |||
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[101] |
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 | [72] | |
TOI-1694 c | 1.05±0.05 | 389.2±3.9 | radial vel. | 405.7 | 0.8450±0.1089 | 5135±50 | [102] | |||
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 | [103] |
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 | [103] | |
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 | [72] | |
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 |
[104] |
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 | [72] | |
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 |
[105] | ||
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 |
[106] |
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 |
[107] |
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 |
[107] |
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 | [108] |
TOI-2018 b | 0.0185 | 0.204+0.009 −0.007 |
7.435588±0.000009 | 652.44 | transit | 0.6600±0.0868 | 4348±100 | [72] | ||
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 |
[109] | |
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 | [110][111] | |
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 | [110][111] | |
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 | [112] |
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 | [112] |
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 | [72][113] |
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 | [113] |
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 | [103] |
TOI-2145 b | 1.069+0.029 −0.028 |
10.26075+0.00083 −0.00082 |
0.1108+0.0012 −0.0016 |
1484+16 −14 |
transit | 732.975+3.594 −3.562 |
1.720+0.057 −0.075 |
6177±67 | [114] | |
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 |
[115] |
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 | [115] |
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 | [72] | |
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 | [116] |
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 |
[106] |
TOI-2443 b | 0.0256 | 0.248±0.004 | 15.669494+0.000926 −0.001004 |
600.83 | transit | 0.6600±0.0789 | 4357±100 | [72] | ||
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 | [72] | ||
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 |
[115] |
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 | [117] |
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 | [118] |
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 | [118] |
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 |
[106] |
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 |
[106] |
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 | [116] |
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[80] |
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 |
[106] |
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 |
[106] |
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 |
[106] |
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 | [106] |
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 |
[106] | |
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 |
[106] |
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 | [72] | |
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 | [119] |
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 |
[106] |
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 | [106] |
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 | [120] |
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 |
[106] |
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 |
[106] |
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 |
[106] |
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 |
[106] |
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 | [121] |
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 | [122] |
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 | [122] |
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 | [122] |
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 | [122] | |
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 |
[106] |
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[123] |
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 |
[106] |
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 |
[109] | |
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 | [124][125] |
TOI-4308 b | 0.0203 | 0.216±0.023 | 9.151201+0.000036 −0.000037 |
763.05 | transit | 0.9000±0.1133 | 5243±126 | [72] | ||
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 | [126] |
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 | [126] |
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 | [127] |
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 | [116] |
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 | [127] | |
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 |
[106] |
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 | [128] |
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 | [129] | ||
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 | [130] |
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[update], longest-period confirmed planet discovered by TESS[130] |
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[131] |
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 |
[106] |
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 | [132] |
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 |
[133] | |
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 |
[133] | |
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 | [134] | |
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 | [121] |
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 | [135] |
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 | [136] |
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 | [137] |
TOI-5704 b | 2.8793+0.01671 −0.01247 |
3.7711160+0.0000115 −0.0000107 |
949.07 | transit | 292.357+0.881 −0.876 |
0.7575±0.0593 | 4590±126 | [72] | ||
TOI-5803 b | 0.0339 | 0.292±0.011 | 5.383050+0.000207 −0.000200 |
678.87 | transit | 0.8700±0.1032 | 5134±121 | [72] | ||
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 | [138] | |
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 | [139] |
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 | [140] | ||
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[141][142] |
Specific exoplanet lists
- List of directly imaged exoplanets
- List of exoplanet extremes
- List of exoplanet firsts
- List of exoplanets discovered by the Kepler space telescope
- List of exoplanets observed during Kepler's K2 mission
- List of extrasolar candidates for liquid water
- List of hottest exoplanets
- List of coolest exoplanets
- List of multiplanetary systems
- List of nearest exoplanets
- List of nearest terrestrial exoplanet candidates
- List of potentially habitable exoplanets
- List of proper names of exoplanets
- List of largest exoplanets
- List of smallest exoplanets
- List of transiting exoplanets
- List of exoplanets and planetary debris around white dwarfs
Lists of exoplanets by year of discovery
- List of exoplanets discovered before 2000 (31)
- List of exoplanets discovered between 2000–2009 (377)
- List of exoplanets discovered in 2010 (109)
- List of exoplanets discovered in 2011 (179)
- List of exoplanets discovered in 2012 (149)
- List of exoplanets discovered in 2013 (151)
- List of exoplanets discovered in 2014 (870)
- List of exoplanets discovered in 2015 (150)
- List of exoplanets discovered in 2016 (1497)
- List of exoplanets discovered in 2017 (158)
- List of exoplanets discovered in 2018 (304)
- List of exoplanets discovered in 2019 (172)
- List of exoplanets discovered in 2020 (249)
- List of exoplanets discovered in 2021 (257)
- List of exoplanets discovered in 2022 (313)
- List of exoplanets discovered in 2023 (289)
- List of exoplanets discovered in 2024 (205)
References
- ^ 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].
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ "AU Microscopii d - Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Archived from the original on 3 December 2023. Retrieved 3 December 2023.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ "The Extrasolar Planet Encyclopaedia — TOI-4481 b". Extrasolar Planets Encyclopaedia. 23 October 1995. Retrieved 19 January 2023.
- ^ "The Extrasolar Planet Encyclopaedia — TOI-4481 c". Extrasolar Planets Encyclopaedia. 23 October 1995. Retrieved 19 January 2023.
- ^ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Archived from the original on 9 November 2023. Retrieved 9 November 2023.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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. doi:10.1051/0004-6361/202347108. ISSN 0004-6361.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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. Archived from the original on 6 October 2023. Retrieved 10 September 2023.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ 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.
- ^ 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.
- ^ 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.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ 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.
- ^ 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.
- ^ Currie, Thayne; Brandt, G. Mirek; Brandt, Timothy D.; Lacy, Brianna; Burrows, Adam; Guyon, Olivier; Tamura, Motohide; Liu, Ranger Y.; Sagynbayeva, Sabina; Tobin, Taylor; Chilcote, Jeffrey; Groff, Tyler; Marois, Christian; Thompson, William; Murphy, Simon J. (April 2023). "Direct imaging and astrometric detection of a gas giant planet orbiting an accelerating star". Science. 380 (6641): 198–203. arXiv:2212.00034. Bibcode:2023Sci...380..198C. doi:10.1126/science.abo6192. ISSN 0036-8075. PMID 37053312. S2CID 258108042. Archived from the original on 3 December 2023. Retrieved 3 December 2023.
- ^ "HIP 99770 b - Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Archived from the original on 12 December 2023. Retrieved 3 December 2023.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ "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.
- ^ 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.
- ^ 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.
- ^ 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. doi:10.1093/mnras/stad3070. ISSN 0035-8711. Archived from the original on 9 December 2023. Retrieved 6 December 2023.
- ^ 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.
- ^ 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.
- ^ a b c d e f 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ "The Extrasolar Planet Encyclopaedia — KMT-2022-BLG-0440L b". Extrasolar Planets Encyclopaedia. 23 October 1995. Retrieved 19 January 2023.
- ^ 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.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ 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.
- ^ 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].
- ^ 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.
- ^ "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.
- ^ 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].
- ^ https://astrobiology.com/2023/01/webb-discovers-lhs-475-b-an-earth-sized-rocky-planet.html
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ Franson, Kyle; Bowler, Brendan P. (1 June 2023). "Dynamical Mass of the Young Brown Dwarf Companion PZ Tel B". The Astronomical Journal. 165 (6): 246. arXiv:2304.01302. Bibcode:2023AJ....165..246F. doi:10.3847/1538-3881/acca18. ISSN 0004-6256.
- ^ 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.
- ^ 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.
- ^ 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].
- ^ 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.
- ^ 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.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ a b 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.
- ^ 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.
- ^ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Archived from the original on 1 October 2023. Retrieved 9 November 2023.
- ^ "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.
- ^ 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.
- ^ "The Extrasolar Planet Encyclopaedia — TOI-700 e". Extrasolar Planets Encyclopaedia. 23 October 1995. Retrieved 12 January 2023.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ 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.
- ^ 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.
- ^ 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.
- ^ 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". eprint arXiv:2310.12458. arXiv:2310.12458.
- ^ 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.
- ^ 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.
- ^ 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.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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. doi:10.1051/0004-6361/202347744. S2CID 264471812.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ a b c 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ Delamer, Megan; Kanodia, Shubham; Cañas, Caleb I.; et al. (2023). "TOI-4201: An Early M-dwarf Hosting a Massive Transiting Jupiter Stretching Theories of Core-Accretion". arXiv:2307.06880 [astro-ph.EP].
- ^ "The Extrasolar Planet Encyclopaedia — Planet TOI-4201 b". Extrasolar Planets Encyclopaedia. 23 October 1995. Retrieved 19 July 2023.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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.
- ^ 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". arXiv:2310.16888.
{{cite journal}}
: Cite journal requires|journal=
(help) - ^ 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.
- ^ 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.
{{cite journal}}
: CS1 maint: unflagged free DOI (link) - ^ 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". arXiv:2307.08350.
{{cite journal}}
: Cite journal requires|journal=
(help) - ^ 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.
- ^ 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.
- ^ "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.