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List of exoplanets discovered in 2023

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Thislist of exoplanets discovered in 2023 is a list of confirmedexoplanets that were first reported in 2023.For exoplanets detected only byradial velocity, the listed value for mass is a lower limit. SeeMinimum mass for more information.

Name	Mass (`M`_J)	Radius (`R`_J)	Period (days)	Semi-major axis (AU)	Temp. (K)	Discovery method	Distance (ly)	Host star mass (`M`_☉)	Host star temp. (K)	Remarks
75 Ceti c	0.9120^+0.0880 _−0.1430		2051.62^+45.98 _−40.47	3.929^+0.058 _−0.052		radial vel.	270.58326 ±2.36023	1.92^+0.07 _−0.08	4809	^[1]
AF Leporis b	3.2^+0.7 _−0.6		8030 ±1800	8.4^+1.1 _−1.3	1400 ±300	imaging	87.562 ±0.046	1.20 ±0.06	6130 ±60	Host star also known as HD 35850^[2]^[3]^[4]
AU Microscopii d	0.00331 ±0.00161		12.73596 ±0.00793	0.1108 ±0.0020		timing	32	0.510^+0.028 _−0.027	3678⁺⁹⁰ ₋₈₈	Potentially rocky super-Earth.^[5]^[6] The orbital solution is yet uncertain.^[5]
BD-21 397 b	0.7 ±0.1		1891⁺⁵⁶ ₋₄₈	2.63^+0.06 _−0.05		radial vel.	77.4046^+0.0744 _−0.0740	0.679 ±0.017	4051 ±239	^[7]
BD-21 397 c	2.4^+1.5 _−0.7		6360⁺⁶²⁶⁰ ₋₇₁₁	5.9^+3.4 _−0.5		radial vel.	77.4046^+0.0744 _−0.0740	0.679 ±0.017	4051 ±239	^[7]
DMPP-4 b	0.0384^+0.0057 _−0.0060		3.4982^+0.0022 _−0.2327			radial vel.	82.6101^+0.1246 _−0.1239	1.25 ±0.02	6400 ±50	^[8]
EPIC 229004835 b	0.0327^+0.0050 _−0.0047	0.2080^+0.0071 _−0.0084	16.141132 ±0.000019	0.1237 ±0.0017	804 ±10	transit	398.255^+2.867 _−2.825	0.970 ±0.040	5868 ±60	^[9]
Gliese 328 c	0.0673^+0.0107 _−0.0101		241.8^+1.3 _−1.7	0.657^+0.026 _−0.028		radial vel.	66.96874 ±0.54957	0.65 ±0.08	3897 ±71	^[10]
Gliese 367 c	0.0130 ±0.0011		11.5301 ±0.0078			radial vel.	30.69986 ±0.00925	0.455 ±0.011	3522 ±70	^[11]
Gliese 367 d	0.0190 ±0.0015		34.369 ±0.073			radial vel.	30.69986 ±0.00925	0.455 ±0.011	3522 ±70	^[11]
Gliese 806 b	0.006 ±0.00053	0.11874 ±0.00205	0.9263237 ±0.0000009	0.1406 ±0.0003	940.0 ±10.0	transit	39.348	0.413 ±0.011	3600 ±16	^[12] Host star also known as TOI-4481^[13]
Gliese 806 c	0.0182 ±0.0009		6.65064 ±0.00025	0.0523 ±0.001	480.0 ±5.0	radial vel.	39.348	0.413 ±0.011	3600 ±16	^[12] Host star also known as TOI-4481^[14]
GJ 1151 c	0.03341^+0.00412 _−0.00463	0.29^[15]	389.7^+5.4 _−6.5	0.5714^+0.0053 _−0.0064		radial vel.	26.23 ±0.01	0.1639 ±0.0093	3143 ±26	^[16] Planet on 2-day orbit was suspected but refuted in 2021^[17]^[18]
GJ 3988 b	0.0116 ±0.0013		6.9442 ±0.0010	0.0405^+0.0011 _−0.0012		radial vel.	32.32369 ±0.01357	0.1842 ±0.0153	3273 ±101	^[19]
GJ 9404 b	0.0374 ±0.0060		13.4586^+0.0044 _−0.0067	0.0943 ±0.0036		radial vel.	77.8988^+0.0828 _−0.0825	0.62 ±0.07		^[20]
HAT-P-2 c	10.7^+5.2 _−2.2		8500⁺²⁶⁰⁰ ₋₁₅₀₀			radial vel.	416.744^+1.386 _−1.380	1.33 ±0.03	6412.830^+102.682 _−110.120	Also known as HD 147506 c^[21]
Beta Andromedae b	28.26^+2.05 _−2.17		663.87^+4.61 _−4.31	2.03 ±0.01		radial vel.	199.36184 ±9.26130	2.49	3802	Host star also known asMirach^[22]
HD 6061 b	0.0340±0.0085	0.219±0.008	5.254467±0.000009	0.059±0.001	1194±28	transit	220.548^+0.670 _−0.665	1.00±0.06	5920±110	Also known as TOI-1473 b^[23]
HD 15906 b		0.200 ±0.007	10.924709 ±0.000032	0.200 ±0.007	668 ±13	transit	148.6035^+0.2880 _−0.2870	0.790^+0.020 _−0.036	4757 ±89	^[24]
HD 15906 c		0.261^+0.006 _−0.005	21.583298^+0.000052 _−0.000055	0.141^+0.002 _−0.001	532 ±10	transit	148.6035^+0.2880 _−0.2870	0.790^+0.020 _−0.036	4757 ±89	^[24]
HD 18438 b	21 ±1		803 ±5	2.1 ±0.1		radial vel.	731.066^+29.409 _−27.254	1.84 ±0.09	3860 ±100	^[25]
HD 22946 d	<0.08360	0.2326 ±0.0054	47.42489^+0.00010 _−0.00011	0.2958^+0.0044 _−0.0042	546 ±6	transit	204.7581^+0.3787 _−0.3370	1.098^+0.040 _−0.039	6169 ±64	^[26]
HD 25463 b	0.0267±0.0098	0.234±0.014	7.049144±0.000009	0.076±0.002	1290±41	transit	148.786^+0.409 _−0.407	1.19±0.07	6220±110	Also known as TOI-554 b.^[23]
HD 25463 c	<0.013	0.134±0.011	3.044050±0.000008	0.0435±0.0009	1707±54	transit	148.786^+0.409 _−0.407	1.19±0.07	6220±110	Also known as TOI-554 c.^[23]
HD 36384 b	6.6 ±0.5		490 ±3	1.3 ±0.1		radial vel.	682.674^+11.588 _−11.210	1.14 ±0.15	3940 ±40	^[27]
HD 73256 c	16 ±1		2690⁺⁶⁰ ₋₁₀₂	3.8 ±0.1		radial vel.	119.7253^+0.1833 _−0.1823	1.00 ±0.05		^[28]
HD 74698 b	0.07 ±0.01		15.017 ±0.002	0.121 ±0.001		radial vel.	169.8125^+0.2479 _−0.2472	1.039 ±0.025	5873 ±19	^[7]
HD 74698 c	0.40 ±0.06		3449⁺¹⁸⁹ ₋₂₁₀	4.5 ±0.2		radial vel.	169.8125^+0.2479 _−0.2472	1.039 ±0.025	5873 ±19	^[7]
HD 75302 b	5.4^+0.5 _−0.4		4356⁺¹⁷³ ₋₁₁₂	5.3^+0.2 _−0.1		radial vel.	98.9192^+0.1973 _−0.1970	1.06 ±0.05		^[28]
HD 89839 b	5.01^+0.79 _−0.76		3441⁺¹⁸ ₋₁₇	4.761 ±0.042		radial vel.	186.9079^+0.3584 _−0.3568	1.21 ±0.03	6314 ±65	^[29]
HD 94771 b	0.53 ±0.03		2164⁺²¹ ₋₂₀	3.48 ±0.03		radial vel.	188.4552^+0.3930 _−0.3911	1.200 ±0.024	5631 ±21	^[7]
HD 99492 c	17.9 ±1.3		95.233^+0.098 _−0.096			radial vel.	59.3728^+0.1895 _−0.1882	0.85 ±0.02	4929 ±44	Host star also known as 83 Leonis^[30]
HD 108202 b	3.0^+0.7 _−0.5		2990⁺⁵⁴ ₋₅₁	3.7 ±0.1		radial vel.	126.1689^+0.2202 _−0.2195	0.74 ±0.04		^[28]
Delta Virginis b	15.83^+2.33 _−2.74		466.63^+2.33 _−2.74	1.33^+0.08 _−0.11		radial vel.	202.45560 ±11.05904	1.4 ±0.3	3657	^[31] Host star also known as Minelauva or Auva
HD 135625 b	2.3^+0.8 _−0.3		4055⁺⁴⁵ ₋₄₄	5.4 ±0.1		radial vel.	184.3368^+0.3803 _−0.3734	1.28 ±0.06		^[28]
HD 135694 b	0.018±0.007	0.224±0.012	15.92346±0.00002	0.120±0.003	815±27	transit	240.936^+0.469 _−0.468	0.90±0.06	5710±110	Also known as TOI-1247 b.^[23]
HD 163296 b	0.267			46		disk kinematics	330.15±3.85^[32]	2.041±0.395^[32]	8291±510^[32]	^[33]
HD 163296 c	0.189			54		disk kinematics				^[33]
HD 163296 d	0.40			84.5		disk kinematics				^[33]
HD 163296 e	1			137		disk kinematics				^[33]
HD 165131 b	19⁺² ₋₁		2343 ±2	3.59^+0.06 _−0.07		radial vel.	187.2993^+0.0689 _−0.0684	1.10 ±0.06		^[28]
HD 167677 b	3.7^+1.6 _−1.1		1804 ±73	2.9 ±0.1		radial vel.	177.1869^+0.9031 _−0.8940	1.00 ±0.05		^[28]
HD 169142 b	3 ±2			37.2 ±1.5		imaging	435.744^+2.717 _−2.674	1.85		^[34]
HD 185283 b	1.3^+0.3 _−0.1		4060⁺¹⁴⁸ ₋₁₁₂	4.6^+0.2 _−0.1		radial vel.	102.3967^+0.1778 _−0.1768	0.80 ±0.04		^[28]
HD 207496 b	0.0192 ±0.0050	0.201 ±0.010	6.441008 ±0.000011	0.0629 ±0.0011	743 ±26	transit	77.11 ±0.04	0.80 ±0.04	4819 ±94	^[35]
HD 235088 b		0.1824 ±0.0067	7.4341393 ±0.0000062	0.0720 ±0.0026	805⁺¹³ ₋₁₂	transit	134.2804 ±0.4612	0.789^+0.022 _−0.021	5037 ±14	Host star also known as TOI-1430^[36]
HIP 8152 b	0.025±0.006	0.228±0.017	10.75101±0.00006	0.092±0.002	855±28	transit	331.681^+1.373 _−1.360	0.91±0.06	5530±110	Also known as TOI-266 b.^[23]
HIP 8152 c	0.0296±0.0069	0.221±0.017	19.6053±0.0003	0.138±0.003	699±23	transit	331.681^+1.373 _−1.360	0.91±0.06	5530±110	Also known as TOI-266 c.^[23]
HIP 9618 b	0.0315 ±0.0098	0.348	20.772907 ±0.000023	0.1438^+0.0025 _−0.0037	663.4^+9.1 _−6.3	transit	220.3112^+0.5108 _−0.5085	1.022^+0.043 _−0.076	5609.0 ±33.0	^[37]
HIP 9618 c	<0.0576 ±0.0053	0.298	52.563491 ±0.000072	0.2669^+0.0046 _−0.0069	486.9^+6.6 _−4.6	transit	220.3112^+0.5108 _−0.5085	1.022^+0.043 _−0.076	5609.0 ±33.0	^[37]
HIP 29442 b	0.032 ±0.0025	0.31	13.63083 ±0.00003	0.1070 ±0.0016	777 ±18	transit	222.4123^+0.5779 _−0.5750	0.89 ±0.04	5289 ±69	Host star also known as TOI-469^[38]
HIP 29442 c	0.014 ±0.001	1.58^+0.10 _−0.11	3.53796 ±0.00003	0.0436^+0.0006 _−0.0007	1217 ±29	radial vel.	222.4123^+0.5779 _−0.5750	0.89 ±0.04	5289 ±69	^[38]
HIP 29442 d	0.016 ±0.001	1.37 ±0.11	6.42975^+0.00009 _−0.00010	0.0649^+0.0009 _−0.0010	998.0 ±24.0	radial vel.	222.4123^+0.5779 _−0.5750	0.89 ±0.04	5289 ±69	^[38]
HIP 54597 b	2.4^+0.4 _−0.2		3274⁺⁴⁷ ₋₄₆	4.0 ±0.1		radial vel.	129.6239^+0.2166 _−0.2162	0.80 ±0.04		^[28]
HIP 81208 C b	14.8 ±0.4		104100^+107260 ₋₄₀₉₃₄	23.04^+13.88 _−6.55	2050⁺³⁵ ₋₂₀	imaging	481.188^+4.837 _−4.472	0.135^+0.010 _−0.013		^[39]
HIP 113103 b		0.163	7.610303 ±0.000018	0.06899^+0.00029 _−0.00023	721 ±10	transit	150.7239^+0.2818 _−0.2805	0.761 ±0.038	4930 ±100	^[40]
HIP 113103 c		0.2141	14.245648 ±0.000019	0.10479^+0.00045 _−0.00035	585 ±10	transit	150.7239^+0.2818 _−0.2805	0.761 ±0.038	4930 ±100	^[40]
HN Librae b	0.0172 ±0.0024		36.116^+0.027 _−0.029	0.1417 ±0.0023	234.4^+5.5 _−5.3	radial vel.	20.36655 ±0.01453	0.291 ±0.013	3347 ±50	Habitable zone planet. Host star also known as Gliese 555^[41]
K2-312 c	5.41+^+0.52 _−0.44		921.2 ±10.8	1.961 ±0.027		radial vel.	358.315^+2.645 _−2.609	1.18 ±0.04	5959 ±61	^[42]
K2-415b	0.0094 ±0.0085	0.091 ±0.005	4.0179694 ±0.0000027	0.0270 ±0.0002	412 ±9	transit	71.126 ±0.030	0.1635 ±0.0041	3173 ±53	^[43]
K2-416 b	<5.2	0.241^+0.027 _−0.0152	13.1020^+0.0026 _−0.0024	0.0880^+0.0100 _−0.0210	447 ±49	transit	392.402^+1.973 _−1.954	0.548 ±0.012	3746 ±72	^[44]
K2-417 b	<2.2	0.295^+0.012 _−0.011	6.5350 ±0.0014	0.063^+0.006 _−0.014	558 ±55	transit	306.7249^+0.9860 _−0.9794	0.569 ±0.012	3861 ±77	^[44]
K2-2016-BLG-0005L b	1.16 ±0.09	1.23	4700⁺³⁰⁰⁰ ₋₇₀₀	4.11 ±0.32		microlensing	16960	0.574 ±0.037		Gas giant.^[45]^[46]
Kepler-10 d	0.03990 ±0.00705		151.04 ±0.45	0.5379 ±0.0044		radial vel.	605.039^+2.645 _−2.626	0.910 ±0.021	5708 ±28	^[42]
Kepler-68 e	0.272 ±0.032		3455⁺³⁴⁸ ₋₁₆₉	4.60^+0.32 _−0.16		radial vel.	470.2^[47]	1.057^+0.022 _−0.020	5847 ±75	^[48]
Kepler-58 d		0.1509503920	4.458169937			transit		1.017^+0.167 _−0.125	6100⁺¹⁹³ ₋₂₁₄	^[49]
Kepler-164 e		0.3570351276	94.8864975			transit		0.966^+0.075 _−0.068	5888⁺¹⁰⁶ ₋₁₁₇	^[49]
Kepler-290 d		0.0794273806	0.764007986			transit		0.84^+0.065 _−0.09	5142 ±153	^[49]
Kepler-297 d		0.6351157298	150.0209961			transit		0.846^+0.059 _−0.049	5618 ±112	^[49]
Kepler-311 d		0.1849409870	232.0469971			transit		0.974^+0.082 _−0.062	5903⁺¹⁰⁶ ₋₁₁₇	^[49]
Kepler-347 d		0.2346332985	85.51660156			transit		1 ±0.072	5592 ±75	^[49]
Kepler-416 d		0.1543405297	3.076410055			transit		0.949^+0.067 _−0.055	5670 ±114	^[49]
Kepler-549 d		0.4055676538	24.6147995			transit		0.859^+0.06 _−0.033	5312 ±79	^[49]
Kepler-618 d		0.3911149410	11.67889977			transit		1.041 ±0.139	6122⁺¹⁶⁹ ₋₁₉₀	^[49]
Kepler-656 c		0.1360516194	5.254559994			transit		1.05^+0.075 _−0.113	5550⁺¹⁶⁶ ₋₁₈₃	^[49]
Kepler-763 c		0.1464004690	4.096680164			transit		0.8^+0.048 _−0.028	4999 ±79	^[49]
Kepler-763 d		0.1754842890	6.503270149			transit		0.8^+0.048 _−0.028	4999 ±79	^[49]
Kepler-784 c		0.1583551639	17.15699959			transit		1.016^+0.093 _−0.084	5676⁺¹¹⁵ ₋₁₀₄	^[49]
Kepler-864 c		0.157641449	2.421489954			transit		1.27^+0.142 _−0.156	6213⁺¹⁷³ ₋₂₅₉	^[49]
Kepler-865 c		0.09474546031	6.209179878			transit		0.782^+0.116 _−0.062	5440 ±162	^[49]
Kepler-880 c		0.2816491659	11.80609989			transit		1.714^+0.17 _−0.316	6900⁺¹⁸⁴ ₋₂₀₄	^[49]
Kepler-896 c		0.2770100246	29.54210091			transit		0.877^+0.083 _−0.092	5510⁺¹⁶⁶ ₋₁₄₉	^[49]
Kepler-949 c		0.4607912263	20.99720001			transit		0.813^+0.104 _−0.064	5211⁺¹⁸¹ ₋₁₆₃	^[49]
Kepler-975 c		0.5035248257	5.05821991			transit		0.951^+0.198 _−0.144	4883⁺¹⁴⁶ ₋₁₃₂	^[49]
Kepler-1052 c		0.2112591764	180.9259949			transit		0.937^+0.09 _−0.121	5818⁺¹³⁹ ₋₁₅₇	^[49]
Kepler-1126 c		0.1500582511	199.6679993			transit		0.794^+0.071 _−0.03	5678⁺¹¹³ ₋₁₀₂	^[49]
Kepler-1162 c		0.1675442283	59.28409958			transit		0.861^+0.05 _−0.041	5225⁺⁸³ ₋₇₃	^[49]
Kepler-1181 c		0.1555895228	8.934909821			transit		1.336 ±0.2	6688⁺¹⁸⁷ ₋₂₈₁	^[49]
Kepler-1471 c		0.2001966118	11.60449982			transit		0.934^+0.063 _−0.045	5533⁺⁸³ ₋₇₄	^[49]
Kepler-1487 c		0.7992697886	35.79949951			transit		1.801^+0.193 _−0.359	5745⁺⁸⁶ ₋₇₇	^[49]
Kepler-1491 c		0.2788835142	61.5685997			transit		0.991^+0.079 _−0.065	5626 ±77	^[49]
Kepler-1513 c	0.266^+0.098 _−0.063		841.4^+8.1 _−5.3			transit		0.943 ±0.037	5491 ±100	^[50]
Kepler-1518 c		0.212775814	9.630929947			transit		1.06^+0.177 _−0.133	6432⁺¹⁵⁵ ₋₂₁₄	^[49]
Kepler-1610 c		0.196806485	44.98529816			transit		0.825^+0.096 _−0.078	5295 ±185	^[49]
Kepler-1669 d		0.1427426870	4.729469776			transit		0.609 ±0.033	4224 ±84	^[49]
Kepler-1801 c		0.3621203501	116.5849991			transit		0.936^+0.114 _−0.093	5738⁺¹⁵⁶ ₋₁₇₃	^[49]
Kepler-1814 c		0.1476494621	0.626281977			transit		0.79^+0.073 _−0.064	4922 ±169	^[49]
Kepler-1834 c		0.129895841	0.766691983			transit		0.765^+0.051 _−0.028	4821 ±76	^[49]
Kepler-1859 c		0.1531807444	3.596430063			transit		1.09^+0.07 _−0.078	5887⁺⁷⁰ ₋₇₉	^[49]
Kepler-1894 c		0.1417613278	5.053750038			transit		0.999^+0.114 _−0.125	5772⁺¹⁵⁶ ₋₁₇₃	^[49]
Kepler-1921 c		0.1505043216	3.157219887			transit		1.251^+0.19 _−0.233	6120⁺¹⁹⁵ ₋₂₁₇	^[49]
Kepler-1976 b		1.043	4.96			transit		1.097^+0.21 _−0.135	6117⁺¹⁵⁶ ₋₂₁₀	^[51]
Kepler-1977 b		0.1625482348	4.537000179			transit		0.769^+0.053 _−0.079	4805 ±144	^[49]
Kepler-1978 b		0.2683562384	10.849699997			transit		0.869^+0.06 _−0.095	5251 ±158	^[49]
Kepler-1980 b		0.2538143392	33.0257988			transit		1.049^+0.059 _−0.073	5819⁺⁶⁹ ₋₈₇	^[49]
Kepler-1981 b		0.8396838173	453.5429993			transit		1.519^+0.15 _−0.376	5874⁺⁸⁷ ₋₇₉	^[49]
Kepler-1982 b		0.773130047	3.823159933			transit		1.213^+0.076 _−0.093	6202⁺⁹⁹ ₋₁₄₉	^[49]
Kepler-1983 b		0.1465788952	7.328519821			transit		0.812^+0.058 _−0.029	5135⁺⁸⁴ ₋₇₅	^[49]
Kepler-1984 b		0.718709408	1.99285996			transit		0.42^+0.046 _−0.056	3638⁺⁷² ₋₈₇	^[49]
Kepler-1985 b		0.1981446855	3.420650005			transit		0.877^+0.064 _−0.037	3638⁺⁷² ₋₈₇	^[49]
Kepler-1986 b		0.2631818295	19.54929924			transit		0.776^+0.089 _−0.065	5549 ±163	^[49]
Kepler-1987 b		0.134713408	2.345860004			transit		0.799^+0.041 _−0.081	4769 ±172	^[49]
Kepler-1987 c		0.151307244	3.648269892			transit		0.799^+0.041 _−0.081	4769 ±172	^[49]
Kepler-1987 d		0.2912843007	5.644889832			transit		0.799^+0.041 _−0.081	4769 ±172	^[49]
Kepler-1987 e		0.2188423849	8.742970467			transit		0.799^+0.041 _−0.081	4769 ±172	^[49]
Kepler-1988 b		0.1382819717	1.549999952			transit		1.127^+0.189 _−0.172	6033 ±183	^[49]
Kepler-1989 b		0.4247487156	10.16100025			transit		0.999^+0.153 _−0.126	6032⁺¹⁸⁹ ₋₂₃₂	^[49]
Kepler-1990 b		0.3491842959	1.735129952			transit		1.028^+0.074 _−0.067	5751⁺¹⁰³ ₋₁₁₄	^[49]
Kepler-1990 c		0.1058972326	1.187000036			transit		1.028^+0.074 _−0.067	5751⁺¹⁰³ ₋₁₁₄	^[49]
Kepler-1991 b		0.1646893688	13.26080036			transit		0.914^+0.061 _−0.042	5478⁺⁸² ₋₇₄	^[49]
Kepler-1991 c		0.2594348291	22.79019928			transit		0.914^+0.061 _−0.042	5478⁺⁸² ₋₇₄	^[49]
Kepler-1992 b		0.0916229564	15.61120033			transit		0.874^+0.048 _−0.054	5383 ±107	^[49]
Kepler-1993 b		0.3949511704	26.65660095			transit		1.373^+0.205 _−0.512	5159⁺¹⁷¹ ₋₁₅₅	^[49]
Kepler-1994 b		0.0555001398	4.612319946			transit		0.932^+0.052 _−0.047	5495⁺⁷⁴ ₋₈₂	^[49]
Kepler-1995 b		0.4119018693	73.75779724			transit		0.847^+0.068 _−0.049	5029⁺¹⁹² ₋₁₇₄	^[49]
Kepler-1996 b		0.204657316	32.37609863			transit		0.748^+0.027 _−0.043	4580 ±92	^[49]
Kepler-1996 c		0.2509594797	92.72949982			transit		0.748^+0.027 _−0.043	4580 ±92	^[49]
Kepler-1997 b		0.2179502440	26.75749969			transit		1.111 ±0.153	6215⁺¹⁹⁴ ₋₂₅₉	^[49]
Kepler-1998 b		0.0619324805	3.03263998			transit		0.962^+0.054 _−0.068	5640⁺¹⁰¹ ₋₁₁₃	^[49]
Kepler-1999 b		0.3169779722	8.739450455			transit		0.632^+0.063 _−0.057	4406⁺¹⁵⁴ ₋₁₇₀	^[49]
Kepler-2000 b		0.2961910652	6.383150101			transit		0.581 ±0.029	3757⁺⁷⁴ ₋₈₂	^[49]
Kepler-2000 c		0.1963604037	20.6182003			transit		0.581 ±0.029	3757⁺⁷⁴ ₋₈₂	^[49]
Kepler-2001 b		0.1062540847	1.190999985			transit		0.864^+0.049 _−0.085	5081⁺¹⁶⁶ ₋₁₃₆	^[49]
Kepler-2001 c		0.3639938397	14.09449959			transit		0.864^+0.049 _−0.085	5081⁺¹⁶⁶ ₋₁₃₆	^[49]
KMT-2016-BLG-0625L b	0.05 ±0.04			1.40 ±0.17		microlensing	21000 ±2000	0.25 ±0.14		^[52]
KMT-2016-BLG-1105L b	0.00415 ±0.00176			2.26^+0.51 _−0.69		microlensing	10665⁺⁴¹⁷⁵ ₋₃₇₅₁	0.43 ±0.18		^[53]
KMT-2016-BLG-1751L b	1.20 ±1.21			1.39 ±0.50		microlensing	23000 ±4000	0.18 ±0.18		^[52]
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		^[53]
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		^[53]
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		^[53]
KMT-2019-BLG-0298L b	1.81 ±0.96			5.67 ±2.70		microlensing	22000 ±5000	0.70 ±0.37		^[54]
KMT-2019-BLG-1216L b	0.094 ±0.050			2.44 ±1.12		microlensing	9000 ±3000	0.39 ±0.21		^[54]
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		^[53]
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		^[53]
KMT-2019-BLG-2783L b	1.16 ±0.77			1.85 ±0.93		microlensing	19000 ±5000	0.34 ±0.25		^[54]
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		^[55]
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		^[55]
KMT-2021-BLG-1105L b	1.30 ±0.68			3.54 ±1.06		microlensing	14807 ±5447	0.63 ±0.33		^[55]
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^[56]
KMT-2021-BLG-2478L b	0.900^+0.420 _−0.240			1.85 ±0.31		microlensing	9687 ±2348	0.20^+0.10 _−0.05		^[55]
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^[56]
KMT-2022-BLG-0440L b	0.0485^+0.0302 _−0.0233			1.9 ±0.7		microlensing	11000 ±5000	0.53^+0.31 _−0.26		^[57]^[58]
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		^[56]
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	^[59]
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	^[60]
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	^[61]^[62] Host star also known as TOI-910^[63] Also the first exoplanet confirmed by theJames Webb Space Telescope.^[64]
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	^[65]
MOA-2016-BLG-0532L b	0.39 ±0.31			1.09 ±0.17		microlensing	24000 ±2000	0.09 ±0.07		^[52]
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		^[66]
MOA-2022-BLG-249Lb	0.015 ±0.005			1.63 ±0.35		microlensing	6500 ±1400	0.18 ±0.05		^[67]
MWC 758 c				100	500 ±100	imaging	159.537^+1.742 _−1.706	1.5		^[68]
OGLE-2016-BLG-1635L b	11.49 ±7.96			1.34 ±0.47		microlensing	22000 ±5000	0.43 ±0.29		^[52]
OGLE-2016-BLG-1850L b	0.03 ±0.01			1.46 ±0.16		microlensing	7000 ±2000	0.26 ±0.11		^[52]
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		^[53]
OGLE-2019-BLG-0249L b	7.12 ±1.47			1.84 ±0.44		microlensing	21000 ±3000	0.91 ±0.19		^[54]
OGLE-2019-BLG-0679L b	3.34 ±1.90			6.99 ±3.21		microlensing	18000 ±6000	0.66 ±0.38		^[54]
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 high temperatures 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-238 b	0.0107^+0.00145 _−0.00142	0.1278^+0.00765 _−0.00784	1.2730988 ±0.0000029	0.02118 ±0.00038	1311 ±28	transit	261.328 ±0.312	0.79 ±0.022	5059 ±89	^[76]
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	^[77]
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	^[74]
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	^[74]
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	^[74]
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	^[79]
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	^[79]
TOI-669 b	0.0308±0.0047	0.232±0.015	3.94515±0.00002	0.047±0.001	1235±37	transit	465.970^+2.789 _−2.759	0.90±0.06	5600±110	^[23]
TOI-672 b	0.0760	0.470^+0.008 _−0.009	3.633575 ±0.000001		676.15	transit		0.5399 ±0.0204	3765 ±65	^[72]
TOI-700 e	0.0025730809^[80]	0.08502^+0.00794 _−0.00669	27.80978^+0.00046 _−0.0004	0.134 ±0.0022	350^[81]	transit	101.52	0.416 ±0.01	3480 ±135	Habitable zone planet^[82]^[83]
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	^[84]
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	^[85]
TOI-771 b	0.00881^+0.00629 _−0.00283	0.127^+0.00964 _−0.00767	2.326021 ±0.000001	0.0207 ±0.0008	527.19 ±22.08	transit	82.452 ±0.130	0.220^+0.024 _−0.023	3201⁺¹⁰⁰ ₋₉₅	^[76]
TOI-778 b	2.8 ±0.2	1.37 ±0.04	4.633611 ±0.000001	0.060 ±0.003	1561⁺³³ ₋₃₂	transit	527.536^+3.663 _−3.614	1.40 ±0.05	6643 ±150	^[86]
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.^[87]
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	^[88]
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	^[88]
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	^[89]
TOI-871 b	0.0120^+0.00849 _−0.00440	0.148^+0.0102 _−0.0101	14.362565 ±0.00009	0.1054 ±0.0021	621 ±16.05	transit	221.917 ±0.489	0.758^+0.046 _−0.044	4929⁺⁸⁰ ₋₇₅	^[76]
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	^[90]
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	^[91]
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	^[91]
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	^[92]
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	^[93]
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^[94]
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	^[95]
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	^[96]
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	^[97]
TOI-1467 b	0.0138^+0.0101 _−0.00535	0.164^+0.0142 _−0.0139	5.971143 ±0.000006	0.0510 ±0.0009	558.89 ±16.37	transit	122.113 ±0.196	0.498^+0.026 _−0.025	3810⁺⁷³ ₋₇₈	^[76]
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	^[98]
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	^[98]
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	^[99]
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^[100]
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	^[101]
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	^[102]
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	^[102]
TOI-1739 b	0.0126^+0.00849 _−0.00472	0.151^+0.00874 _−0.00758	8.303342^+0.000011 _−0.000013	0.0742 ±0.0014	755.55 ±20.19	transit	231.506 ±0.522	0.790^+0.046 _−0.045	4922⁺⁹⁴ ₋₉₁	^[76]
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	^[103]
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	^[104]
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	^[105]
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	^[106]
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	^[106]
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	^[107]
TOI-2015 b	0.0516±0.0129	0.302±0.012	3.348968±0.000004	0.0301^+0.0013 _−0.0012	512±11	transit	154.34^+0.13 _−0.10	0.342^+0.021 _−0.025	3194±56	^[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-2068 b	0.0138^+0.0101 _−0.00503	0.162^+0.0145 _−0.0133	7.768915^+0.000025 _−0.000037	0.0632 ±0.0011	520.62 ±14.18	transit	172.635^+0.294 _−0.261	0.559^+0.027 _−0.029	3710⁺⁵⁷ ₋₅₈	^[76]
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	^[102]
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	^[103]
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	^[103]
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	^[114]
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	^[105]
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	^[103]
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	^[115]
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	^[116]
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	^[116]
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	^[105]
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	^[105]
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	^[114]
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^[79]
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	^[105]
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	^[105]
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	^[105]
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	^[105]
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	^[105]
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	^[105]
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	^[117]
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	^[105]
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	^[105]
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	^[118]
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	^[105]
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	^[105]
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	^[105]
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	^[105]
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	^[119]
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	^[120]
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	^[120]
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	^[120]
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	^[120]
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	^[105]
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^[121]
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	^[105]
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	^[122]^[123]
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	^[124]
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	^[124]
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	^[125]
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	^[114]
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	^[105]
TOI-4515 b	2.005 ±0.052	1.086 ±0.039	15.266	0.118 ±0.001	705 ±10	transit		0.949 ±0.020	5433 ±70	^[126] Highly eccentric orbit(e = 0.46)
TOI-4551 b	1.49 ±0.13	1.058^+0.110 _−0.062	9.955810^+0.000076 _−0.000078	0.09940^+0.00300 _−0.00320		transit	704.453^+8.033 _−7.857	1.31^+0.07 _−0.18	4896 ±110	^[125]
TOI-4559 b	0.00849^+0.00629 _−0.00315	0.126^+0.0112 _−0.00999	3.965991^+0.000314 _−0.000332	0.0359 ±0.0008	554.16 ±19.14	transit	90.704 ±0.0978	0.392^+0.027 _−0.026	3558⁺⁷³ ₋₈₃	^[76]
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	^[127]
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	^[128]
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	^[129]
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^[129]
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^[130]
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	^[105]
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	^[131]
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	^[132]
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	^[132]
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	^[133]
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	^[119]
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	^[134]
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	^[135]
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	^[136]
TOI-5704 b		0.288	3.7711160^+0.0000115 _−0.0000107		949.07	transit	292.357^+0.881 _−0.876	0.7575 ±0.0593	4590 ±126	^[72]
TOI-5799 b	0.0116^+0.00849 _−0.00440	0.145^+0.0171 _−0.0114	4.164753^+0.00038 _−0.000427	0.0352 ±0.0011	518.01 ±20.15	transit	90.704 ±0.0978	0.337^+0.027 _−0.032	3514⁺⁹⁵ ₋₉₄	^[76]
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		^[137]
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	^[138]
WISE J033605.05-014350.4 b	8.25 ±4.25		2560 ±730	0.970 ±0.050	325⁺¹⁵ ₋₁₀	imaging	32.7 ± 0.7^[a]	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]

Notes

[edit]

^Distance calculated from the given parallax of 99.8 milliarcseconds.^[139]

Specific exoplanet lists

[edit]

Lists of exoplanets

Lists of exoplanets by year of discovery

[edit]

List of exoplanets discovered before 2000 (31)
List of exoplanets discovered between 2000–2009 (375)
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 (149)
List of exoplanets discovered in 2014 (869)
List of exoplanets discovered in 2015 (144)
List of exoplanets discovered in 2016 (1498)
List of exoplanets discovered in 2017 (152)
List of exoplanets discovered in 2018 (300)
List of exoplanets discovered in 2019 (170)
List of exoplanets discovered in 2020 (247)
List of exoplanets discovered in 2021 (254)
List of exoplanets discovered in 2022 (313)
List of exoplanets discovered in 2023 (307)
List of exoplanets discovered in 2024 (285)
List of exoplanets discovered in 2025 (103)

References

[edit]

^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.
^^a ^bWittrock, 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. Retrieved3 December 2023.
^^a ^b ^c ^d ^eFrensch, 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. Retrieved26 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. Retrieved26 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 ^bGoffo, 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 ^bPalle, 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. Retrieved19 January 2023.
^"The Extrasolar Planet Encyclopaedia — TOI-4481 c".Extrasolar Planets Encyclopaedia. 23 October 1995. Retrieved19 January 2023.
^"Exoplanet-catalog".Exoplanet Exploration: Planets Beyond our Solar System.Archived from the original on 9 November 2023. Retrieved9 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.arXiv:2310.05599.Bibcode:2023A&A...680A..28G.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 ^c ^d ^e ^f ^gAkana Murphy, Joseph M.; et al. (48) (8 September 2023)."The TESS-Keck Survey. XVI. Mass Measurements for 12 Planets in Eight Systems".The Astronomical Journal.166 (4): 153.arXiv:2306.16587.Bibcode:2023AJ....166..153A.doi:10.3847/1538-3881/ace2ca.
^^a ^bTuson, 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 andCHEOPS 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.
^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 the 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. Retrieved10 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. Retrieved1 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 ^hPhilipot, 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.
^^a ^b ^cPaegert, M.; Stassun, K. G.; Collins, K. A.; Pepper, J.; Torres, G.; Jenkins, J.; Twicken, J. D.; Latham, D. W. (1 February 2022). "VizieR Online Data Catalog: TESS Input Catalog version 8.2 (TIC v8.2) (Paegert+, 2021)".VizieR Online Data Catalog.4039: IV/39.Bibcode:2022yCat.4039....0P.
^^a ^b ^c ^dGarrido-Deutelmoser, Juan; Petrovich, Cristobal; Charalambous, Carolina; Guzmán, Viviana V.; Zhang, Ke (1 March 2023)."A gap-sharing planet pair shaping the crescent in HD 163296: a disk sculpted by a resonant chain".The Astrophysical Journal Letters.945 (2): L37.arXiv:2301.13260.doi:10.3847/2041-8213/acbea8.ISSN 2041-8205.
^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.
^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 ^bOsborn, 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 byTESS andCheops".Monthly Notices of the Royal Astronomical Society.523 (2):3069–3089.arXiv:2306.04450.doi:10.1093/mnras/stad1319.
^^a ^b ^cDamasso, 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 15M_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.
^^a ^bLowson, 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 ^bBonomo, 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 ^bIncha, 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. Retrieved6 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.
^"K2-2016-BLG-005L b - Exoplanet-catalog".Exoplanet Exploration: Planets Beyond our Solar System.Archived from the original on 3 December 2023. Retrieved3 December 2023.
^"The Extrasolar Planet Encyclopaedia — Kepler-68 e.".Extrasolar Planets Encyclopaedia. 2025.
^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. Retrieved7 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 ^boValizadegan, 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.arXiv:2310.03802.Bibcode:2024MNRAS.527..620Y.doi:10.1093/mnras/stad3070.ISSN 0035-8711.Archived from the original on 9 December 2023. Retrieved6 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 ^eShin, 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 ^gZang, 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 ^eYoun 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 ^dRyu, 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 ^cHan, 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. Retrieved19 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.
^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. Retrieved12 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].
^"Webb Discovers LHS 475 b, an Earth-Sized, Rocky Planet". 12 January 2023.
^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. Retrieved7 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. Retrieved7 December 2023.
^^a ^bBrewer, 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 ^bBozhilov, 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 ^qMistry, 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.
^^a ^b ^c ^dOddo, 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 ^bHobson, 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.
^^a ^b ^c ^d ^e ^f ^g ^hPriyashkumar, Mistry; Prasad, Aniket; Maity, Mousam; Pathak, Kamlesh; Gharat, Sarvesh; Lekkas, Georgios; Bhattarai, Surendra; Kumar, Dhruv; Lissauer, Jack J.; Twicken, Joseph D.; Soubkiou, Abderahmane; Pozuelos, Francisco J.; Jenkins, Jon; Horne, Keith; Giacalone, Steven; Barkaoui, Khalid; Timmermans, Mathilde; Watkins, Cristilyn N.; Sefako, Ramotholo; Collins, Karen A.; Shporer, Avi; Benkhaldoun, Zouhair; Stockdale, Chris; Jehin, Emmanuël; Murgas, Felipe; Paegert, Martin; Lund, Michael B.; Narita, Norio; Schwarz, Richard P.; Goeke, Robert F.; Tan, Thiam-Guan; Kawai, Yugo (1 November 2023). "VaTEST III: Validation of 8 Potential Super-Earths from TESS Data".arXiv:2311.00688 [astro-ph.EP].
^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.
^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. Retrieved9 December 2023.
^^a ^b ^cPsaridi, 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. Retrieved9 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. Retrieved9 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. Retrieved12 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. Retrieved9 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 ^bHawthorn, 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. Retrieved9 December 2023.
^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.arXiv:2306.09758.doi:10.1093/mnras/stad1840.hdl:10023/28054.ISSN 0035-8711.Archived from the original on 9 December 2023. Retrieved9 December 2023.
^^a ^bArmstrong, 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. Retrieved8 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".arXiv:2310.12458 [astro-ph.EP].
^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. Retrieved8 December 2023.
^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.hdl:1887/3717895.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 ^bGonzález-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. Retrieved1 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 ^cMartioli, E.; Hébrard, G.; de Almeida, L.; Heidari, N.; Lorenzo-Oliveira, D.; Kiefer, F.; Almenara, J. M.; Bieryla, A.; Boisse, I.; Bonfils, X.; Briceño, C.; Collins, K. A.; Cortés-Zuleta, P.; Dalal, S.; Deleuil, M. (2023). "TOI-1736 and TOI-2141: Two systems including sub-Neptunes around solar analogs revealed by TESS and SOPHIE".Astronomy & Astrophysics.680: A84.arXiv:2311.07011.Bibcode:2023A&A...680A..84M.doi:10.1051/0004-6361/202347744.S2CID 264471812.
^^a ^b ^c ^dRodriguez, 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. Retrieved8 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 ^tYee, 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 ^bSha, 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.
^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.
^Jones, Sinclaire E.; Stefánsson, Guðmundur; Masuda, Kento; Libby-Roberts, Jessica E.; Gardner, Cristilyn N.; Holcomb, Rae; Beard, Corey; Robertson, Paul; Cañas, Caleb I.; Mahadevan, Suvrath; Kanodia, Shubham; Lin, Andrea S. J.; Kobulnicky, Henry A.; Parker, Brock A.; Bender, Chad F.; Cochran, William D.; Diddams, Scott A.; Fernandes, Rachel B.; Gupta, Arvind F.; Halverson, Samuel; Hawley, Suzanne L.; Hearty, Fred R.; Hebb, Leslie; Kowalski, Adam; Lubin, Jack; Monson, Andrew; Ninan, Joe P.; Ramsey, Lawrence; Roy, Arpita; Schwab, Christian; Terrien, Ryan C.; Wisniewski, John (9 May 2024). "TOI-2015b: A Warm Neptune with Transit Timing Variations Orbiting an Active mid M Dwarf".arXiv:2310.11775 [astro-ph.EP].
^^a ^bBarkaoui, 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 ^bQuintana, 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 ^bMurgas, 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 ^bPozuelos, 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 ^bRescigno, 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.arXiv:2310.13623.doi:10.1093/mnras/stad3255.hdl:10023/28862.ISSN 0035-8711.Archived from the original on 8 December 2023. Retrieved8 December 2023.
^^a ^b ^cBrahm, 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. Retrieved9 December 2023.
^^a ^bTrifonov, 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 ^bCañas, 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 ^dKunimoto, 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. (2024)."TOI-4201: An Early M-dwarf Hosting a Massive Transiting Jupiter Stretching Theories of Core-Accretion".The Astrophysical Journal.962 (2): L22.arXiv:2307.06880.Bibcode:2024ApJ...962L..22D.doi:10.3847/2041-8213/ad1a19.
^"The Extrasolar Planet Encyclopaedia — Planet TOI-4201 b".Extrasolar Planets Encyclopaedia. 23 October 1995. Retrieved19 July 2023.
^^a ^bTey, 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 ^bPereira, 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. Retrieved9 December 2023.
^Carleo, I.; Malavolta, L.; Desidera, S.; Nardiello, D.; Wang, S.; Turrini, D.; Lanza, A. F.; Baratella, M.; Marzari, F.; Benatti, S.; Biazzo, K.; Bieryla, A.; Brahm, R.; Bonavita, M.; Collins, K. A. (1 February 2024)."The GAPS programme at TNG. L. TOI-4515 b: An eccentric warm Jupiter orbiting a 1.2 Gyr-old G-star".Astronomy and Astrophysics.682: A135.arXiv:2311.11903.Bibcode:2024A&A...682A.135C.doi:10.1051/0004-6361/202348207.ISSN 0004-6361.
^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 ^bMireles, 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. Retrieved9 December 2023.
^^a ^bFairnington, 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".Astronomy and Astrophysics.682.arXiv:2310.16888.Bibcode:2024A&A...682A.129M.doi:10.1051/0004-6361/202347472.
^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. Retrieved9 December 2023.
^Barkaoui, Khalid; Pozuelos, Francisco J.; Hellier, Coel; Smalley, Barry; Nielsen, Louise D.; Dorn, Caroline; Niraula, Prajwal; Gillon, Michaël; de Wit, Julien; Helled, Ravit; Müller, Simon; Jehin, Emmanuel; Demory, Brice-Olivier; Van Grootel, V.; Soubkiou, Abderahmane (2023). "WASP-193b: An extremely low-density super-Neptune".Astrophysics.arXiv:2307.08350.doi:10.1038/s41550-024-02259-y.
^Kirkpatrick, J. Davy; Gelino, Christopher R.; Cushing, Michael C.; Mace, Gregory N.; Griffith, Roger L.; Skrutskie, Michael F.; et al. (July 2012)."Further Defining Spectral Type "Y" and Exploring the Low-mass End of the Field Brown Dwarf Mass Function".The Astrophysical Journal.753 (2): 38.arXiv:1205.2122.Bibcode:2012ApJ...753..156K.doi:10.1088/0004-637X/753/2/156. 156.
^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. Retrieved9 January 2023.

Exoplanets

Main topics

Sizes
and
types

Terrestrial	Carbon planet Catastrophically evaporating planet Coreless planet Desert planet Dwarf planet Hycean planet Ice planet Iron planet (Super-Mercury) Lava planet Ocean world Mega-Earth Steam world Sub-Earth Super-Earth
Gaseous	Cold Jupiter Eccentric Jupiter Mini-Neptune (Gas dwarf) Helium planet Hot Jupiter Hot Neptune Gas giant Ice giant Neptunian Jupiter analogue Super-Jupiter Super-Neptune Super-puff Ultra-hot Jupiter Ultra-hot Neptune Warm Jupiter
Other types	Blanet Brown dwarf Chthonian planet Circumbinary planet Circumtriple planet Disrupted planet Double planet Ecumenopolis Eyeball planet Giant planet Mesoplanet Planemo Planet/Brown dwarf boundary Planetesimal Protoplanet Pulsar planet Sub-brown dwarf Sub-Neptune Toroidal planet Ultra-cool dwarf Ultra-short period planet (USP)