Danh sách ngoại hành tinh được phát hiện năm 2021

Danh sách ngoại hành tinh được phát hiện năm 2021 là danh sách các ngoại hành tinh đã được xác nhận lần đầu là được quan sát vào năm 2021.

Danh sách

Tên	Khối lượng (`M`_J)	Bán kính (`R`_J)	Chu kỳ quỹ đạo (ngày)	Bán trục nhỏ (AU)	Nhiệt độ (K)	Kĩ thuật quan sát	Khoảng cách (ly)	Khối lượng ngôi sao chủ (M_☉)	Nhiệt độ ngôi sao chủ (K)	Chú thích
HD 108236 f		0.17406^+0.00482 _−0.00437	29.54255± 0.00069	0.1759± 0.0037		quá cảnh	211	0.853± 0.047	5,720.0± 50.0	^[1]^[2]
NGTS-14Ab	0.092± 0.012	0.444± 0.030	3.5357173± 0.0000069	0.0403± 0.0071	1,143± 139	quá cảnh	1,060	0.898± 0.035	5,187± 11	^[3]
TOI-1259Ab	0.441^+0.049 _−0.047	1.022^+0.030 _−0.037	3.4779780^+0.0000019 _−0.0000017	0.04070^+0.00114 _−0.00110	936	quá cảnh	385± 1	0.68^+0.1 _−0.01	4,775± 100	Also white dwarf on a wide orbit^[4]
NGTS-13b	4.84± 0.44	1.142± 0.046	4.12	0.0549^+0.0015 _−0.0025	1,605± 30	quá cảnh	2150	1.30^+0.11 _−0.18	5,819± 73	^[5]
TOI-628 b	6.33^+0.29 _−0.31	1.060^+0.041 _−0.034	3.4095675^+0.0000070 _−0.0000069	0.04860^+0.00080 _−0.00094	1,586⁺⁵² ₋₄₀	quá cảnh	582	1.311^+0.066 _−0.075	6,250⁺²²⁰ ₋₁₉₀	Host star also known as HD 288842^[6]
TOI-640 b	0.88± 0.16	1.771^+0.060 _−0.056	5.0037775± 0.0000048	0.06608^+0.00098 _−0.0011	1,749⁺²⁶ ₋₃₀	quá cảnh	1,115	1.536^+0.069 _−0.076	6,460⁺¹³⁰ ₋₁₅₀	^[6]
TOI-1333 A b	2.37± 0.24	1.396^+0.056 _−0.054	4.720219± 0.000011	0.0626^+0.0011 _−0.0012	1,679⁺³⁵ ₋₃₄	quá cảnh	653	1.464^+0.076 _−0.079	6,274± 97	Host star also known as BD+47 3521A.^[6]
TOI-1478 b	0.847^+0.052 _−0.048	1.061^+0.040 _−0.038	10.180249± 0.000015	0.0903^+0.0018 _−0.0013	918± 11	quá cảnh	498	0.946^+0.059 _−0.041	5,595⁺⁸³ ₋₈₁	^[6]
TOI-1601 b	0.99± 0.11	1.239^+0.046 _−0.039	5.331751± 0.000011	0.06864^+0.00079 _−0.00075	1,619⁺²⁴ ₋₂₃	quá cảnh	1,096	1.517^+0.053 _−0.049	5,948⁺⁸⁷ ₋₈₉	^[6]
OGLE-2019-BLG-0960Lb	0.0071± 0.0027			1.75± 0.55		thấu kính hấp dẫn	2,900± 1000	0.45± 0.15		Smallest planet discovered by thấu kính hấp dẫn^[7]
HD 110113 b	0.0143± 0.0020	0.183± 0.011	2.541^+0.0005 _−0.001	0.035± 0.001	1,371± 14	quá cảnh	346.5± 2.3	0.99± 0.08	5,730	Radius gap planet, host star also known as TOI-755^[8]
HD 110113 c	0.0330± 0.0038		6.744^+0.008 _−0.009	0.068^+0.001 _−0.002	990± 10	vận tốc xuyên tâm	346.5± 2.3	0.99± 0.08	5,730	Host star also known as TOI-755.^[8]
KOI-5Ab	0.179	0.63	5			quá cảnh	1,870± 70	1.13	5861	Also called TOI-1241b.^[9]^[10]
TOI-178b	0.0047^+0.0012 _−0.0013	0.102± 0.006	1.914558± 0.000018	0.02607± 0.00078	1,040⁺²² ₋₂₁	quá cảnh	205.16± 0.03	0.650^+0.027 _−0.029	4,316± 70	^[11]
TOI-178c	0.015^+0.0017 _−0.0021	0.149^+0.01 _−0.008	3.238450^+0.000020 _−0.000019	0.0370± 0.0011	873± 18	quá cảnh	205.16± 0.03	0.650^+0.027 _−0.029	4,316± 70	^[11]
TOI-178d	0.0094^+0.0025 _−0.0032	0.229± 0.006	6.557700± 0.000016	0.0592± 0.0018	690± 14	quá cảnh	205.16± 0.03	0.650^+0.027 _−0.029	4,316± 70	^[11]
TOI-178e	0.0121^+0.0039 _−0.0029	0.197^+0.007 _−0.008	9.961881± 0.000042	0.0783^+0.0023 _−0.0024	600± 12	quá cảnh	205.16± 0.03	0.650^+0.027 _−0.029	4,316± 70	^[11]
TOI-178f	0.0242^+0.0052 _−0.0047	0.204± 0.009	15.231915^+0.000115 _−0.000095	0.1039± 0.0031	521± 11	quá cảnh	205.16± 0.03	0.650^+0.027 _−0.029	4,316± 70	^[11]
TOI-178g	0.0123^+0.0041 _−0.0050	0.256^+0.012 _−0.011	20.70950^+0.00014 _−0.00011	0.1275^+0.0038 _−0.0039	470± 10	quá cảnh	205.16± 0.03	0.650^+0.027 _−0.029	4,316± 70	^[11]
HD 183579 b	0.0620^+0.0126 _−0.0123	0.317^+0.013 _−0.011	17.471278^+0.000058 _−0.000060	0.1334^+0.0062 _−0.0061	769⁺¹⁷ ₋₁₃	quá cảnh	186.1± 0.8	1.031^+0.025 _−0.026	5,788± 44	Host star also known as TOI-1055^[12]^[13]
KMT-2019-BLG-0371b	7.70^+11.34 _−3.90			0.79^+0.14 _−0.16		thấu kính hấp dẫn	2,3000^+3,000 _−4,000	0.09^+0.14 _−0.05		Multiple solutions for orbital separation^[14]
HD 5278 b	0.0245^+0.0047 _−0.0044	0.219± 0.004	14.339156^+0.000049 _−0.000047	0.1202± 0.0013	943± 13	quá cảnh	183.1± 2.7	1.126^+0.036 _−0.035	6,203± 64	Host star also known as TOI-130.^[15]
HD 5278 c	0.0579^+0.0057 _−0.0060		0.2416± 0.0027	0.1202± 0.0013	943± 13	vận tốc xuyên tâm	183.1± 2.7	1.126^+0.036 _−0.035	6,203± 64	Host star also known as TOI-130.^[15]
KMT-2018-BLG-1025Lb	0.0191^+0.0258 _−0.0104			1.305^+0.194 _−0.227		thấu kính hấp dẫn	22,000± 3,000	0.219^+0.297 _−0.120		Multiple solutions for orbital parameters^[16]
TOI-558b	3.61± 0.15	1.086^+0.041 _−0.038	14.574071± 0.000026	0.1291^+0.0020 _−0.0021	1,061⁺¹³ ₋₁₂	quá cảnh	1,312± 17	1.349^+0.064 _−0.065	6,466⁺⁹⁵ ₋₉₃	^[17]
TOI-559b	6.01^+0.24 _−0.23	1.091^+0.028 _−0.025	6.9839095± 0.0000051	0.0723± 0.0013	1,180⁺¹⁸ ₋₁₆	quá cảnh	761± 7	1.026± 0.057	5,925⁺⁸⁵ ₋₇₆	^[17]
Candidate 1	0.062-0.157	0.3011-0.6386				hình ảnh trực tiếp	4.37		Imaged near Alpha Centauri A
HD 13808 b	0.0346		14.2	0.11		vận tốc xuyên tâm	92.2	0.771± 0.022	5,035± 50	Candidate since 2011,^[18] confirmed in 2021^[19]
HD 13808 c	0.0315		53.8	0.26		vận tốc xuyên tâm	92.2	0.771± 0.022	5,035± 50	Candidate since 2011,^[18] confirmed in 2021^[19]
TOI 451 b		0.1732^+0.0134 _−0.0116	1.858701^+0.000027 _−0.000033	0.0271^+0.0023 _−0.0038	1,524⁺¹⁰⁰ ₋₆₀	quá cảnh	405.1± 1.3	0.94± 0.025	5,550± 56	Planets orbiting primary of wide binary system.^[20]^[21] Host star also known as CD-38 1467.
TOI 451 c		0.2741± 0.0125	9.192523^+0.000064 _−0.000084	0.0771^+0.0066 _−0.0093	903⁺⁵³ ₋₃₆	quá cảnh	405.1± 1.3	0.94± 0.025	5,550± 56	Planets orbiting primary of wide binary system.^[20]^[21] Host star also known as CD-38 1467.
TOI 451 d		0.3598± 0.0134	16.364981^+0.000047 _−0.000049	0.1255^+0.0057 _−0.0065	708⁺¹⁵ ₋₁₂	quá cảnh	405.1± 1.3	0.94± 0.025	5,550± 56	Planets orbiting primary of wide binary system^[20]^[21] Host star also known as CD-38 1467.
HD 110082 b		0.2857± 0.0089	10.18271± 0.00004	0.113^+0.009 _−0.013		quá cảnh	342.8± 0.9	1.21± 0.06	6,200± 100	Orbiting a primary of wide binary system^[22] Host star also known as TOI-1098.
OGLE-2018-BLG-0567Lb	0.32^+0.34 _−0.16			2.72^+0.49 _−0.55		thấu kính hấp dẫn	23,000± 3,000	0.24^+0.16 _−0.13		^[23]
OGLE-2018-BLG-0962Lb	1.37^+0.80 _−0.72			3.57^+0.68 _−1.02		thấu kính hấp dẫn	21,000^+3,000 _−5,000	0.55^+0.32 _−0.29		^[23]
Gliese 740 b	0.0093± 0.0016		2.37756^+0.00013 _−0.00011	0.029± 0.001	829⁺⁴⁰ ₋₅₀	vận tốc xuyên tâm	36.21± 0.02	0.58± 0.06	3,913± 21	^[24]
OGLE-2018-BLG-1428Lb	0.77^+0.77 _−0.53			3.30^+0.59 _−0.83		thấu kính hấp dẫn	20,000^+3,000 _−5,000	0.43^+0.33 _−0.22		^[25]
LHS 1478 b	0.0073± 0.0006	0.111± 0.004	1.9495378^+0.0000040 _−0.0000041	0.01848^+0.00061 _−0.0006	595⁺¹⁰ ₋₉	quá cảnh	59.40± 0.03	0.236± 0.012	3,381± 54	^[26] Host star also known as TOI-1640 or G 245-61.
TOI-1685 b	0.0121± 0.030	0.131± 0.006	0.6691425± 0.0000037	0.01156± 0.00009	1,052± 21	quá cảnh	122.68± 0.09	0.495± 0.019	3,434± 51	^[27]^[28] Host star also known as UCAC4 666-026266
TOI-1685 c	0.0290± 0.0065		9.025^+0.104 _−0.119		449.1± 6.9	vận tốc xuyên tâm	122.68± 0.09	0.495± 0.019	3,434± 51	Unconfirmed^[27]
KMT-2020-BLG-0414Lb	0.0032			0.15		thấu kính hấp dẫn	3,300± 300	0.3		Also a brown dwarf with mass 17 `M`_J in the system at 15 AU separation^[29]
HD 39474 b	0.42^+0.05 _−0.03	1.008^+0.012 _−0.015	52.97818^+0.00004 _−0.00004	0.30^+0.02 _−0.03	759⁺³⁷ ₋₂₆	quá cảnh	372.5± 1.1	1.316± 0.027	6,394± 75	Host star also known as TOI-201^[30]
Gliese 486 b	0.0089± 0.0004	0.117± 0.006	1.467119^+0.000031 _−0.000030	0.01734^+0.00026 _−0.00027	701± 13	quá cảnh	26.344± 0.013	0.323± 0.015	3,340± 54	Planet may have a measurable atmosphere^[31]
NGTS-15b	0.751^+0.102 _−0.088	1.10± 0.10	3.27623± 0.00001	0.0441± 0.0046	1,146± 47	quá cảnh	2,580± 60	0.995± 0.015	5,600± 150	^[32]
NGTS-16b	0.667^+0.157 _−0.129	1.30^+0.13 _−0.12	4.84532± 0.00002	0.0523± 0.0064	1,177± 59	quá cảnh	2,910⁺⁹⁵ ₋₇₅	1.002± 0.011	5,550± 150	^[32]
NGTS-17b	0.764^+0.195 _−0.164	1.24± 0.11	3.24253± 0.00001	0.0391± 0.0043	1,457± 50	quá cảnh	3,420± 90	1.025^+0.015 _−0.014	5,650± 100	^[32]
NGTS-18b	0.409^+0.081 _−0.063	1.21± 0.18	3.05125± 0.00001	0.0448± 0.0068	1,381⁺⁵⁵ ₋₅₃	quá cảnh	3,610± 140	1.003^+0.020 _−0.012	5,610± 150	^[32]
OGLE-2019-BLG-1053Lb	0.0078^+0.0037 _−0.0031			3.4± 0.5		thấu kính hấp dẫn	22,000^+3,000 _−2,000	0.61^+0.29 _−0.24		^[33]
TOI-1634 b	0.0313± 0.0030	0.158± 0.007	0.9893457± 0.0000034	0.01491± 0.00015	921± 21	quá cảnh	114.40± 0.08	0.452± 0.014	3,472± 48	^[28]^[34]
KMT-2019-BLG-1715	2.56^+1.13 _−1.16			3.32^+0.82 _−0.92		thấu kính hấp dẫn	13,000± 3,000	0.61^+0.27 _−0.28		Multiple solutions for orbital separation, also 0.15M_☉ red dwarf in the system.^[35]
OGLE-2018-BLG-1185b	0.026^+0.025 _−0.015			1.54^+0.18 _−0.22		thấu kính hấp dẫn	24,000^+2,000 _−3,000	0.37^+0.35 _−0.21		Multiple solutions for planet and star masses.^[36]
TOI-1260 b	0.0271^+0.0043 _−0.0037	0.208^+0.009 _−0.008	3.12748^+0.000047 _−0.000038	0.0366^+0.0022 _−0.0036	860⁺⁴⁷ ₋₃₁	quá cảnh	239.5± 0.3	0.66± 0.01	4,227± 85	^[37]
TOI-1260 c	0.0373^+0.0106 _−0.0102	0.252± 0.013	7.49325^+0.00015 _−0.00013	0.0656^+0.0039 _−0.0065	643⁺³⁵ ₋₂₃	quá cảnh	239.5± 0.3	0.66± 0.01	4,227± 85	^[37]
KMT-2018-BLG-1976Lb	1.96^+1.23 _−1.12			2.04^+0.72 _−0.83		thấu kính hấp dẫn	19,000± 2,000	0.65^+0.41 _−0.37		^[38]
KMT-2018-BLG-1996Lb	1.22^+0.72 _−0.63			1.97^+0.51 _−0.25		thấu kính hấp dẫn	19,000± 2,000	0.69^+0.40 _−0.38		^[38]
OGLE-2019-BLG-0954Lb	14.2^+9.9 _−7.5			2.65^+0.89 _−1.20		thấu kính hấp dẫn	12,000^+1,000 _−2,000	0.80^+0.55 _−0.42		^[38]
YSES 2 b	6.3^+1.6 _−0.9			115		hình ảnh trực tiếp	356.4± 0.5	1.10± 0.03	4,749± 40	^[39]
KMT-2016-BLG-2605b	0.8^+1.2 _−0.4			0.68± 0.11		thấu kính hấp dẫn	21,000± 3,000	0.065^+0.10 _−0.035		^[40]
TOI-1431 b	3.14^+0.19 _−0.18	1.51± 0.06	2.65022± 0.00001	0.047± 0.002	2,370± 100	quá cảnh	488± 3	1.90^+0.10 _−0.08	7,690⁺⁴⁰⁰ ₋₂₅₀	Also known as MASCARA-5b^[41]^[42]
TOI-269 b	0.0277± 0.0044	0.247± 0.011	3.697723^+0.000018 _−0.000017	0.0345± 0.0015	531± 25	quá cảnh	186.01± 0.25	0.3917± 0.0095	3,514± 70	^[43]
TOI-220 b	0.0434± 0.0031	0.271± 0.013	10.695264	0.08911± 0.0010	805± 21	quá cảnh	290± 13	0.825± 0.028	5,298± 65	Additional long-period planet suspected^[44]
TOI 1062 b	0.0320± 0.0026	0.202± 0.008	4.11412^+0.0014 _−0.0015	0.052	1,077⁺¹⁰ ₋₉	quá cảnh	268.7± 0.2	0.94± 0.02	5,328± 56	^[45]
TOI 1062 c	0.0294± 0.0039		7.978^+0.021 _−0.023	0.080^+0.013 _−0.012	859⁺⁹ ₋₈	vận tốc xuyên tâm	268.7± 0.2	0.94± 0.02	5,328± 56	^[45]
Kepler-129d	8.3^+1.1 _−0.7		2646⁺¹⁴⁰ ₋₉₄	4.0± 0.1		vận tốc xuyên tâm	1,349± 14	1.18	5,770	^[46]
Gliese 9689 b	0.0304± 0.0046		18.27± 0.01	0.1139± 0.0039	453± 39	vận tốc xuyên tâm	100.10± 0.04	0.59± 0.06	3,836± 69	^[47]
TOI-1231 b	0.0485± 0.0104	0.326± 0.014	24.245586^+0.000064 _−0.000066	0.1288^+0.0021 _−0.0022	330	quá cảnh	89.68± 0.04	0.485± 0.024	3,553± 31	^[48]
TIC 172900988 b	2.84± 0.25	1.009± 0.043	196.5± 7.7			quá cảnh	799± 9	1.24 and 1.20	6050 and 5983	Circumbinary planet^[49]
TOI-1444 b	0.0122± 0.0022	0.125± 0.006	0.4702694± 0.0000044	0.1288^+0.0021 _−0.0022	330	quá cảnh	408.9± 0.5	0.934± 0.038	5,430± 90	^[50]
BD+45 0564 b	1.36± 0.12		307.88± 1.47	0.83± 0.04		vận tốc xuyên tâm	174± 2	0.81± 0.07	5,004± 50	^[51]
BD+55 0362 b	0.72± 0.08		265.59± 1.04	0.78± 0.05		vận tốc xuyên tâm	168± 2	0.909± 0.099	5,012± 78	Additional giant planet is suspected^[51]
BD+63 1405 b	3.96± 0.31		1,198.48± 60.79	2.06± 0.14		vận tốc xuyên tâm	124.4± 1.2	0.82± 0.08	5,000± 53	Extremely eccentric orbit^[51]
HD 124330 b	0.75± 0.06		270.66± 1.21	0.86± 0.04		vận tốc xuyên tâm	198± 3	1.15± 0.079	5,873± 19	Additional giant planet is suspected^[51]
HD 155193 b	0.75± 0.06		352.65± 2.58	1.04± 0.04		vận tốc xuyên tâm	186± 6	1.221± 0.083	6,239± 20	^[51]
HD 331093 b	1.50± 0.11		621.62± 16.11	1.44± 0.07		vận tốc xuyên tâm	164.07± 0.14	1.030± 0.079	5,544± 33	^[51]
HD 107148 c	0.0626^+0.0097 _−0.0098		18.3267^+0.0022 _−0.0024	0.1406± 0.0018		vận tốc xuyên tâm	161.4± 0.4	1.1± 0.1	5,789± 36	^[52]
HD 136925 b	0.84^+0.078 _−0.074		4,540⁺¹⁶⁰ ₋₁₄₀	5.13^+0.12 _−0.11		vận tốc xuyên tâm	156.2		5715	Additional planet suspected^[52]
Lambda Serpentis b	0.0428^+0.0047 _−0.0045		15.5083^+0.0016 _−0.0018	0.1238± 0.002		vận tốc xuyên tâm	38.87± 0.07	1.14	5,884± 4	^[52]
HD 156668 c	0.0991^+0.0079 _−0.0077		811.3^+5.2 _−5.3	1.570± 0.017		vận tốc xuyên tâm	79.34± 0.03	0.772± 0.020	4,850± 88	Additional body in system is suspected^[52]
HD 164922 e	0.0331± 0.0031		41.763± 0.012	0.2293^+0.0026 _−0.0027		vận tốc xuyên tâm	71.69± 0.03	0.874± 0.012	5,293± 32	^[52]
HD 168009 b	0.0300^+0.0038 _−0.0037		15.1479^+0.0035 _−0.0037	0.1192^+0.0017 _−0.0018		vận tốc xuyên tâm	75.97± 0.03	0.99	5,792± 80	^[52]
HD 213472 b	3.48^+1.10 _−0.59		16,700^+12,000 _−4,800	13.0^+5.7 _−2.6		vận tốc xuyên tâm	210.6			^[52]
HD 24040 c	0.201± 0.027		515.4^+2.2 _−2.5	1.3± 0.021		vận tốc xuyên tâm	152.3± 0.4	1.14± 0.02	5,917± 52	^[52]
HD 26161 b	13.5^+8.5 _−3.7		32,000^+21,000 _−10,000	20.4^+7.9 _−4.9		vận tốc xuyên tâm	133.6± 0.3			Very eccentric orbit, and also red dwarf in the system^[52]
HD 3765 b	0.173^+0.014 _−0.013		1,211⁺¹⁵ ₋₁₆	2.108^+0.032 _−0.033		vận tốc xuyên tâm	78.5± 0.1			^[52]
HD 66428 c	27⁺²² ₋₁₇		39,000^+56,000 _−18,000	23.0^+19.0 _−7.6		vận tốc xuyên tâm	174.1± 0.7	1.09± 0.02	5,773± 55	^[52]
HD 68988 c	15.0^+2.8 _−1.5		16,100^+11,000 _−3,500	13.2^+5.3 _−2.0		vận tốc xuyên tâm	198.8± 0.6	1.16± 0.01	5,919± 11	Suspected since 2006^[52]
Lalande 21185 c	0.0568^+0.0091 _−0.0083		3190⁺²⁰⁰ ₋₁₇₀	3.1^+0.13 _−0.11		vận tốc xuyên tâm	8.31± 0.01	0.390± 0.011	3,601± 51	^[52]
G 264-12 b	0.0079± 0.0009		2.30538± 0.00031	0.02279± 0.00061	587± 16	vận tốc xuyên tâm	52.14± 0.03	0.297± 0.024	3,326± 54	^[53]
G 264-12 c	0.0118± 0.0015		8.0518± 0.0034	0.0525± 0.0014	387± 11	vận tốc xuyên tâm	52.14± 0.03	0.297± 0.024	3,326± 54	^[53]
Gliese 393 b	0.0054± 0.0008		7.02679^+0.00082 _−0.00085	0.05402± 0.00072	485± 11	vận tốc xuyên tâm	22.956± 0.008	0.426± 0.017	3,579± 51	^[53]
TOI-674b	0.0739± 0.0104	0.470± 0.016	1.977143± 0.000003	0.0231± 0.0007	661± 14	quá cảnh	150.86± 0.11	0.442± 0.007	3,505⁺²⁸ ₋₃₂	^[54] Possibly steam atmosphere^[55]
HD 152843 b [ja]	0.0364^+0.0207 _−0.0193	0.304± 0.012	11.6264^+0.0022 _−0.0025	0.1053^+0.003 _−0.0031		quá cảnh	352.0± 1.0	1.15± 0.04	6,310± 100	^[56]
HD 152843 c [ja]	0.0865	0.521± 0.013	24.38^+6.23 _−3.4			quá cảnh	352.0± 1.0	1.15± 0.04	6,310± 100	^[56]
KMT-2019-BLG-0253b	0.029^+0.016 _−0.013			3.1^+0.8 _−0.9		thấu kính hấp dẫn	16,000^+6,000 _−5,000	0.70^+0.34 _−0.31		^[57]
OGLE-2018-BLG-0506	0.051^+0.038 _−0.027			3.0^+0.7 _−0.8		thấu kính hấp dẫn	18,000± 5,000	0.63^+0.37 _−0.32		^[57]
OGLE-2018-BLG-0516	0.063^+0.052 _−0.034			2.2^+0.8 _−0.7		thấu kính hấp dẫn	7,000^+3,000 _−2,000	0.47^+0.38 _−0.25		^[57]
OGLE-2019-BLG-1492	0.117^+0.079 _−0.061			2.7± 0.9		thấu kính hấp dẫn	18,000^+6,000 _−7,000	0.68± 0.34		^[57]
OGLE-2018-BLG-0977	0.020^+0.016 _−0.012			2.0^+0.6 _−0.5		thấu kính hấp dẫn	7,000± 2,000	0.47^+0.38 _−0.27		^[57]
TOI-1789 b	0.70± 0.16	1.40^+0.22 _−0.13	3.208666± 0.000016	0.04873^+0.00065 _−0.0016	1,929⁺²⁸ ₋₁₈	quá cảnh	729± 3	1.499^+0.061 _−0.15	5,984⁺⁵⁵ ₋₅₇	^[58]
TOI-942 b		0.347^+0.022 _−0.020	4.32421± 0.000019	0.04866^+0.00016 _−0.00013		quá cảnh	493.9± 1.0	0.8220^+0.0079 _−0.0064		^[59]
TOI-942 c		0.417^+0.030 _−0.027	10.156272^+0.000037 _−0.000034	0.08598^+0.00027 _−0.00022		quá cảnh	493.9± 1.0	0.8220^+0.0079 _−0.0064		^[59]
KMT-2018-BLG-1743	0.245^+0.339 _−0.135			1.449^+0.209 _−0.229		thấu kính hấp dẫn	21,000± 3,000	0.193^+0.268 _−0.107		Multiple orbital solutions, binary host star^[60]
TOI-1749 b	0.060^+0.07 _−0.04	0.124± 0.018	2.388821^+0.000057 _−0.000073	0.0291± 0.0005	831± 18	quá cảnh	324.8± 0.4	0.58± 0.03	3,985± 55	^[61]
TOI-1749 c	0.007^+0.018 _−0.005	0.189± 0.011	4.489010^+0.000040 _−0.000061	0.0443± 0.0008	673± 15	quá cảnh	324.8± 0.4	0.58± 0.03	3,985± 55	^[61]
TOI-1749 d	0.014^+0.020 _−0.011	0.225± 0.013	9.04455± 0.00012	0.0707± 0.0012	533± 12	quá cảnh	324.8± 0.4	0.58± 0.03	3,985± 55	^[61]
HD 27969 b	4.80^+0.24 _−0.23		654.5^+5.7 _−5.8	1.552^+0.032 _−0.033	261± 11	vận tốc xuyên tâm		1.16± 0.07	5,966± 21	^[62]
HD 80869 b	4.86^+0.65 _−0.29		1711.7^+9.3 _−9.6	2.878^+0.045 _−0.046	203.2^+6.8 _−5.5	vận tốc xuyên tâm		1.08± 0.05	5,837± 15	Very eccentric orbit^[62]
HD 95544 b	6.84± 0.31		2172⁺²³ ₋₂₁	3.386^+0.075 _−0.077	156.5^+5.4 _−5.5	vận tốc xuyên tâm		1.09± 0.07	5,722± 15	^[62]
HD 109286 b	2.99± 0.15		520.1± 2.3	1.259± 0.021	259.4± 5.5	vận tốc xuyên tâm		0.98± 0.05	5,694± 23	^[62]
HD 115954 b	8.29^+0.75 _−0.58		3700⁺¹⁵⁰⁰ ₋₃₉₀	5.00^+1.3 _−0.36	144.9^+8.1 ₋₁₃	vận tốc xuyên tâm		1.18± 0.06	5957± 26	^[62]
HD 211403 b	5.54^+0.39 _−0.38		223.8± 0.41	0.768± 0.013	380± 13	vận tốc xuyên tâm		1.20± 0.06	6,273± 44	^[62]
Kepler-1704b	4.15± 0.29	1.065^+0.043 _−0.041	988.88113^+0.00091 _−0.00092	2.026^+0.024 _−0.031	253.8^+3.7 _−4.1	quá cảnh	2,690± 40	1.131^+0.040 _−0.051	5,745⁺⁸⁸ ₋₈₉	Very eccentric orbit (e=0.921),^[63]
TOI-532b	0.1935^+0.0305 _−0.0293	0.520± 0.017	2.3266508± 0.0000030	0.0296± 0.00035	867± 18	quá cảnh	439.1± 1.2	0.639± 0.023	3927± 37	Neptunian desert planet^[64]
TOI-2406b	0.0286^+0.0223 _−0.0126	0.263^+0.015 _−0.014	3.0766896± 0.0000065	0.0228± 0.0016	447± 15	quá cảnh	181.4± 0.4	0.162± 0.008	3,100± 75	^[65]
KIC 8121913 b	2.1± 0.4		3.294601^+0.000013 _−0.00022			orbital brightness modulation	2350	1.456^+0.069 _−0.15	5075.3^+110.2 _−109.4	^[66]
KIC 10068024 b	2.0± 0.4		2.073549^+0.000008 _−0.000177			orbital brightness modulation	3,600	1.22^+0.175 _−0.139	6,118.4^+127.2 _−121.2	^[66]
KIC 5479689 b	0.5^+0.4 _−0.1		1.701531^+0.000008 _−0.000419			orbital brightness modulation	1,504	0.966^+0.03 _−0.04	5459.1^+90.0 _−85.2	^[66]
LTT 1445 Ac	0.0048± 0.0006	0.103	3.12390	0.02661^+0.00047 _−0.00049		quá cảnh	22.41± 0.01	0.256± 0.014	3337± 150	^[67]
Luyten 98-59 e	0.0094		12.8	0.071	342⁺²⁰ ₋₁₈	vận tốc xuyên tâm	34.6	0.32± 0.03	3500± 150	^[68]
Luyten 98-59 f	0.0078		23.2	0.103	285⁺¹⁸ ₋₁₇	vận tốc xuyên tâm	34.6	0.32± 0.03	3500± 150	Unconfirmed, potentially habitable exoplanet^[68]
HD 191939 e	0.34± 0.01		101.4± 0.4	0.397± 0.005	397± 16	vận tốc xuyên tâm	175.1± 0.2	0.92	5400	Also suspected brown dwarf on wider orbit^[69]
OGLE-2019-BLG-1058	6.836± 6.027					thấu kính hấp dẫn	8,000± 5,000			Multiple solutions, rogue planet^[70]
TOI-2184 b	0.65± 0.16	1.017± 0.051	6.90683± 0.00009			quá cảnh	2,515± 22	1.53± 0.12	5,966± 136	^[71]
TOI-431 b	0.0097± 0.0011	0.0014± 0.004	0.490047^+0.000010 _−0.000007	0.0113^+0.0002 _−0.0003	1,862± 42	quá cảnh	106.37± 0.03	0.78± 0.07	4,850± 75	Host star lso known as CD-26 2288 or HIP 26013.^[72]
TOI-431 c	0.0089^+0.0013 _−0.0011		4.8494^+0.0003 _−0.0002	0.0052± 0.001	867± 20	vận tốc xuyên tâm	106.37± 0.03	0.78± 0.07	4,850± 75	Host star also known as CD-26 2288 or HIP 26013.^[72]
TOI-431 d	0.0312± 0.0047	0.294± 0.008	12.46103± 0.00002	0.098± 0.002	633± 14	quá cảnh	106.37± 0.03	0.78± 0.07	4,850± 75	Host star lso known as CD-26 2288 or HIP 26013.^[72]
TOI-2202 b	0.927^+0.047 _−0.048	1.01^+0.522 _−0.080	11.9108^+0.0009 _−0.0009	0.0956^+0.0015 _−0.0016		quá cảnh	770± 3	0.823^+0.027 _−0.023	5,144± 50	^[73]
TOI-2202 c	0.191^+0.033 _−0.030		24.7545^+0.0073 _−0.0078	0.1558^+0.0025 _−0.0026		timing	770± 3	0.823^+0.027 _−0.023	5,144± 50	^[73]
EPIC 211314705.01		0.139± 0.007	3.793306^+0.000324 _−0.000343		543⁺⁸ ₋₉	quá cảnh	300.0± 1.7	0.43± 0.01	3,669⁺⁸⁸ ₋₈₂	^[74] Two more planets in system are suspected.^[75]
EPIC 211401787.01		0.247^+0.013 _−0.008	13.774798^+0.000028 _−0.000028		969± 9	quá cảnh	525± 5	1.23± 0.02	6,232⁺³³ ₋₃₉	^[74] Host star also known as BD+12 1842.
K2-268f		0.199^+0.013 _−0.008	26.270570^+0.000105 _−0.000109		492⁺⁸ ₋₁₀	quá cảnh	1,079± 10	0.84± 0.02	5,106⁺⁷⁰ ₋₆₁	Two more planets were previously known; host star also known as EPIC 211413752.^[74]
K2-268d		0.133^+0.013 _−0.006	4.528598^+0.000016 _−0.000015		888⁺¹⁶ ₋₁₅	quá cảnh	1,079± 10	0.84± 0.02	5,106⁺⁷⁰ ₋₆₁	Two more planets were previously known; host star also known as EPIC 211413752.^[74]
K2-268e		0.119^+0.010 _−0.007	6.131243^+0.000032 _−0.000033		801± 13	quá cảnh	1,079± 10	0.84± 0.02	5,106⁺⁷⁰ ₋₆₁	Two more planets were previously known; host star also known as EPIC 211413752.^[74]
EPIC 211502222.01		0.243^+0.013 _−0.009	22.996591^+0.001848 _−0.001859		673⁺¹² ₋₁₁	quá cảnh	694± 6	1.10^+0.03 _−0.04	5,994⁺⁹³ ₋₉₁	^[74]
EPIC 211502222.02		0.160^+0.013 _−0.009	9.398977^+0.001506 _−0.001348		909± 14	quá cảnh	694± 6	1.10^+0.03 _−0.04	5,994⁺⁹³ ₋₉₁	^[74]
EPIC 211579112.01		0.196^+0.017 _−0.014	17.706320± 0.000063		266⁺⁵ ₋₈	quá cảnh	403± 5	0.27^+0.01 _−0.02	3,315⁺¹³⁷ ₋₁₅₂	^[74]
K2-185c		0.213± 0.008	52.713494^+0.000155 _−0.000164		477⁺¹⁴ ₋₁₇	quá cảnh	882± 11	0.96^+0.05 _−0.07	5,788⁺¹⁹⁰ ₋₁₅₇	Host star also known as EPIC 211611158.^[74]
EPIC 211647930.01		0.552^+0.025 _−0.022	14.759287^+0.000243 _−0.000240		826⁺¹⁴ ₋₁₇	quá cảnh	1,133± 17	1.06± 0.04	5,880⁺⁸⁵ ₋₈₂	^[74]
EPIC 211730024.01		0.504^+0.032 _−0.025	5.113981^+0.000061 _−0.000062		1,380⁺³⁴ ₋₃₀	quá cảnh	1,226± 21	1.36± 0.05	6,502⁺¹³² ₋₁₃₀	^[74]
EPIC 211743874.01		0.197^+0.016 _−0.013	12.283211± 0.000051		949⁺²¹ ₋₂₆	quá cảnh	1,850± 60	1.23± 0.04	6,222⁺⁹⁶ ₋₉₁	^[74]
EPIC 211763214.01		0.109^+0.008 _−0.005	21.194733^+0.000108 _−0.000107		569⁺¹⁵ ₋₂₂	quá cảnh	786± 9	0.86^+0.03 _−0.05	5,424⁺¹⁹² ₋₁₄₄	^[74]
EPIC 211770696.01		0.234^+0.017 _−0.013	16.273563^+0.000054 _−0.000053		850⁺¹⁹ ₋₁₈	quá cảnh	1,390± 30	0.94^+0.04 _−0.03	5,869⁺⁸⁸ ₋₈₁	^[74]
EPIC 211779390.01		0.092^+0.010 _−0.005	3.850614± 0.000012		783⁺¹² ₋₁₄	quá cảnh	514± 2	0.66± 0.02	4,558⁺⁹¹ ₋₈₁	^[74]
EPIC 211897691.02		0.171^+0.017 _−0.011	19.507428^+0.000116 _−0.000113		508± 12	quá cảnh	1,187± 17	0.74^+0.04 _−0.03	4,857⁺⁸⁶ ₋₈₄	^[74]
EPIC 211923431.01		0.300^+0.039 _−0.029	29.740451^+0.000169 _−0.000161		606⁺³¹ ₋₃₆	quá cảnh	2,460± 70	0.93± 0.04	5,532± 90	^[74]
EPIC 211978988.01		0.287^+0.022 _−0.017	36.552551^+0.000127 _−0.000122		598⁺¹⁶ ₋₁₅	quá cảnh	1,390± 20	0.98± 0.07	5,817⁺⁴⁵ ₋₄₈	^[74]
TOI-1518 b	2.3	1.875± 0.053	1.902603± 0.000011	0.0389± 0.0011	3,237± 59	quá cảnh	742± 6	1.79± 0.26	7,300± 100	^[74]
EPIC 212058012.01		0.181^+0.012 _−0.008	11.561052^+0.000690 _−0.000668		861⁺¹⁴ ₋₁₅	quá cảnh	684± 6	1.01± 0.05	5,920± 104	^[74]
EPIC 212072539.01		0.180^+0.009 _−0.006	7.676972^+0.000012 _−0.000012		465± 7	quá cảnh	545± 3	0.49± 0.01	3,804⁺⁹³ ₋₇₄	^[74]
EPIC 212072539.02		0.147^+0.015 _−0.007	2.787174± 0.000004		653⁺¹⁰ ₋₁₂	quá cảnh	545± 3	0.49± 0.01	3,804⁺⁹³ ₋₇₄	^[74]
EPIC 212081533.01		0.142^+0.009 _−0.004	3.355850^+0.000091 _−0.000093		722⁺⁷ ₋₁₀	quá cảnh	245.8	0.51± 0.01	4,374⁺³⁸ ₋₃₄	^[74]
EPIC 212088059.01		0.188^+0.018 _−0.008	10.367437^+0.000020 _−0.000019		437⁺⁴ ₋₅	quá cảnh	532± 3	0.56± 0.01	3,779⁺³⁰ ₋₂₆	^[74]
EPIC 212132195.01		0.202^+0.017 _−0.009	26.201446^+0.003331 _−0.003124		450± 5	quá cảnh	345.5± 1.6	0.71± 0.02	4,801± 49	^[74]
EPIC 212161956.01		0.215^+0.010 _−0.009	7.187257^+0.000020 _−0.000021		640⁺²⁰ ₋₂₁	quá cảnh	1055± 13	0.66± 0.03	4,599⁺¹⁷⁸ ₋₁₅₂	^[74]
EPIC 212204403.01		0.291^+0.020 _−0.010	4.688418^+0.000119 _−0.000117		908⁺¹² ₋₁₁	quá cảnh	662± 5	0.83^+0.02 _−0.01	5,077⁺⁴⁰ ₋₃₉	^[74]
EPIC 212204403.02		0.238^+0.021 _−0.010	12.550171^+0.001018 _−0.001057		655⁺⁷ ₋₉	quá cảnh	662± 5	0.83^+0.02 _−0.01	5,077⁺⁴⁰ ₋₃₉	^[74]
K2-304c		0.203^+0.017 _−0.011	5.213965± 0.000442		866⁺²⁷ ₋₃₇	quá cảnh	1,380± 20	0.83^+0.05 _−0.04	5,171⁺¹⁷² ₋₁₃₀	Host star also known as EPIC 212297394.^[74]
EPIC 212420823.01		0.123^+0.009 _−0.006	9.032178± 0.000874		518⁺⁵ ₋₄	quá cảnh	1,450± 20	0.54± 0.01	4,385⁺²⁹ ₋₃₁	^[74]
EPIC 212440430.02		0.138^+0.013 _−0.010	4.163873^+0.000022 _−0.000023		1,158⁺²⁹ ₋₃₄	quá cảnh	1,620± 20	0.98± 0.02	5,789⁺⁴⁶ ₋₅₀	^[74]
EPIC 212543933.01		0.227^+0.023 _−0.017	7.806164^+0.000673 _−0.000623		934⁺²⁸ ₋₃₂	quá cảnh	1,310± 50	1.02± 0.02	5,769⁺³⁹ ₋₃₇	^[74]
K2-307c		0.207^+0.017 _−0.011	23.228555^+0.000068 _−0.000071		658⁺¹³ ₋₁₄	quá cảnh	1,050± 20	0.99^+0.03 _−0.04	6,004⁺⁷⁷ ₋₇₈	Host star also known as EPIC 212587672.^[74]
EPIC 251319382.01		0.171^+0.012 _−0.006	8.234885^+0.000508 _−0.000475		885⁺¹² ₋₁₄	quá cảnh	577± 6	0.95± 0.02	5,791± 81	^[74]
EPIC 251319382.02		0.199^+0.012 _−0.008	14.871387^+0.000916 _−0.000936		727± 10	quá cảnh	577± 6	0.95± 0.02	5,791± 81	^[74]
EPIC 251319382.03		0.122^+0.009 _−0.006	3.665912^+0.000273 _−0.000295		1,160⁺¹⁶ ₋₁₅	quá cảnh	577± 6	0.95± 0.02	5,791± 81	^[74]
EPIC 251554286.01		0.496^+0.020 _−0.018	15.466805^+0.000572 _−0.000565		735⁺¹³ ₋₁₄	quá cảnh	883± 12	0.87± 0.02	5,698± 55	^[74]
Gliese 146 b	0.0175^+0.0023 _−0.0021		5.09071 ± 0.00026	0.0510^+0.0024 _−0.0026	573⁺⁶³ ₋₆₉	vận tốc xuyên tâm	44.37± 0.01	0.684± 0.013	4,385± 21	Host star also known as HD 22496.^[76]
EPIC 211525753.01		0.201^+0.020 _−0.014	5.7385647^+0.0013939 _−0.0011048	0.0632^+0.0096 _−0.0176	1,066⁺¹⁹⁰ ₋₇₇	quá cảnh		0.96^+0.05 _−0.06	5,790⁺¹⁷⁷ ₋₁₄₇	^[77]
EPIC 211537087.01		0.204^+0.013 _−0.011	21.0267366^+0.0036912 _−0.0038993	0.1599^+0.0178 _−0.0306	624⁺⁰ ₋₃₇	quá cảnh		0.90^+0.05 _−0.06	5,568⁺¹⁷⁸ ₋₁₅₀	^[77]
EPIC 211730267.01		0.332^+0.021 _−0.019	16.3488637^+0.0013811 _−0.0014022	0.1450^+0.0136 _−0.0235	735⁺⁸ ₋₃₉	quá cảnh		0.98± 0.07	5,794⁺²¹⁰ ₋₁₆₉	^[77]
EPIC 211914998.01		0.239^+0.015 _−0.013	11.2510285^+0.0018188 _−0.0017892	0.0863^+0.0079 _−0.0159	888⁺⁰ ₋₄₇	quá cảnh		0.93± 0.06	5,650⁺¹⁹³ ₋₁₅₂	^[77]
TOI-3362b	5.029^+0.668 _−0.646	1.142^+0.043 _−0.041	18.09547± 0.00003	0.153^+0.002 _−0.003		quá cảnh	1,198± 18	1.445^+0.069 _−0.073	6,532⁺⁸⁸ ₋₈₆	High eccentricity orbit^[78]
KMT-2017-BLG-2509b	2.09^+1.68 _−1.26			2.14^+0.27 _−0.39		thấu kính hấp dẫn	23,000± 3,000	0.46^+0.37 _−0.27		^[79]
OGLE-2017-BLG-1099b	3.02^+2.43 _−1.81			2.73^+0.40 _−0.53		thấu kính hấp dẫn	24,000± 3,000	0.45^+0.36 _−0.27		^[79]
OGLE-2019-BLG-0299b	6.22^+3.80 _−3.67			2.80^+0.58 _−0.89		thấu kính hấp dẫn	19,000± 4,000	0.59^+0.36 _−0.35		^[79]
TOI-1296b	0.298± 0.039	1.231± 0.031	3.9443715± 0.0000058	0.0497^+0.0023 _−0.0028	1,562⁺⁴³ ₋₃₁	quá cảnh	1,023± 4	1.17± 0.14	5,603± 47	^[80]
TOI-1298b	0.356± 0.032	0.841± 0.021	4.537164± 0.000012	0.0590± 0.0023	1,388± 24	quá cảnh	1,041± 7	1.44± 0.10	5,889± 43	^[80]
TOI-1201 b	0.0198± 0.0027	0.216± 0.008	2.4919863^+0.0000030 _−0.0000031	0.0287± 0.0012	703⁺¹⁵ ₋₁₄	quá cảnh	122.77± 0.10	0.512± 0.020	3,476± 51	Belongs to the Hyades, also red dwarf in the system.^[81]
RR Caeli c	2.7± 0.7		14,200± 300	9.7± 0.9		timing	69.10± 0.03	0.18+0.44	3,100+7,540	Circumbinary planet around red and white dwarfs^[82]
TIC 257060897b	0.67± 0.03	1.49± 0.04	3.660028± 0.000006	0.051± 0.002	1,762± 21	quá cảnh	1,655± 8	1.32± 0.04	6,128± 57	^[83]
TOI-530b	0.40^+0.09 _−0.10	0.83± 0.06	6.387597^+0.000019 _−0.000018	0.052^+0.005 _−0.004	565⁺²⁸ ₋₃₁	quá cảnh	482± 2	0.53± 0.02	3,659± 120	^[84]
HIP 97166b	0.0629± 0.047	0.245± 0.012	10.28891± 0.00004	0.089± 0.001	757± 25	quá cảnh	215.54± 0.33	0.898± 0.054	5,198± 100	^[85]
HIP 97166c	9.9± 1.8		16.84± 0.22	0.124± 0.002	642± 22	vận tốc xuyên tâm	215.54± 0.33	0.898± 0.054	5,198± 100	^[85]
HD 63935 b	0.0340± 0.0057	0.267± 0.013	9.058811^+0.000017 _−0.000016		911± 27	quá cảnh	159.36± 0.15	0.933± 0.054	5,534± 100	^[86]
HD 63935 c	0.0349± 0.0076	0.259± 0.012	21.4023^+0.00189 _−0.00194		684± 21	quá cảnh	159.36± 0.15	0.933± 0.054	5,534± 100	^[86]
HD 207897 b	0.0453± 0.0050	0.223± 0.007	16.202159^+0.000085 _−0.000083	0.1163^+0.0017 _−0.001	632.2^+8.1 _−7.0	quá cảnh	92.15± 0.10	0.80^+0.036 _−0.030	5,070⁺⁶⁰ ₋₅₇	^[87]
2MASS J04372171+2651014 b	4± 1			115	1,450± 50	hình ảnh trực tiếp	417.9± 1.5	0.165± 0.015	3,100	^[88]^[89]
TOI 1227 b		0.854^+0.067 _−0.052	27.36397± 0.00011	0.0886^+0.0054 _−0.0057		quá cảnh	329.3± 0.8	0.170± 0.015	3,072± 74	^[90]
TOI-2285b		0.155± 0.007	27.26955^+0.00013 _−0.00010	0.1363± 0.0010	284± 6	quá cảnh	138.34± 0.14	0.454± 0.010	3,491± 58	^[91]
LHS 1678 b	0.0002± 0.0003	0.062± 0.004	0.8602322^+0.0000068 _−0.0000048	0.01251^+0.00059 _−0.00056		quá cảnh	64.88± 0.03	0.345± 0.014	3490± 50	^[92]
LHS 1678 c	0.0012^+0.0013 _−0.0008	0.088± 0.006	3.694247^+0.0000024 _−0.0000021	0.0331^+0.0016 _−0.0015		quá cảnh	64.88± 0.03	0.345± 0.014	3490± 50	^[92]
HD 73583 b	0.0315± 0.0098	0.253± 0.009	6.3980418^+0.0000065 _−0.0000063	0.0601± 0.0026	721± 21	quá cảnh	103.08± 0.10	0.71± 0.02	4511± 110	Host star also known as TOI-560,^[93] planetary helium emission detected.^[94]
HD 73583 c	0.0302± 0.0055	0.212± 0.009	18.8797^+0.00088 _−0.00073	0.1236^+0.0053 _−0.0053	503± 15	quá cảnh	103.08± 0.10	0.71± 0.02	4511± 110	Host star also known as TOI-560^[93]
TOI-1807 b [it]	0.0071^+0.0015 _−0.0018	0.165± 0.004	0.549372± 0.000007	0.0135^+0.0013 _−0.0022	1499⁺⁸² ₋₁₂₉	quá cảnh	133.88± 0.25	0.750^+0.025 _−0.024	4757⁺⁵¹ ₋₅₀	Star is co-moving with TOI-2076^[95]^[96]
TOI-2076 b		0.293± 0.038	10.35566± 0.00006	0.0631± 0.0027	870± 13	quá cảnh	136.70± 0.23	0.850^+0.025 _−0.026	5187⁺⁵⁴ ₋₅₃	Star is co-moving with TOI-1807^[95]
TOI-2076 c		0.396± 0.004	21.01538^+0.00084 _−0.00074	0.0885± 0.0038	734± 11	quá cảnh	136.70± 0.23	0.850^+0.025 _−0.026	5187⁺⁵⁴ ₋₅₃	^[97] Star is co-moving with TOI-1807^[95]
TOI-2076 d		0.370± 0.006	25.0893± 0.01	0.1138^+0.0048 _−0.0049	648± 10	quá cảnh	136.70± 0.23	0.850^+0.025 _−0.026	5187⁺⁵⁴ ₋₅₃	Star is co-moving with TOI-1807^[95]
TOI-2257 b		0.196± 0.010	35.189346	0.145± 0.003	256⁺⁶¹ ₋₁₇	quá cảnh	188.5± 0.3	0.33± 0.02	3430± 130	Habitable zone planet^[98]
TOI-712 b	0.0176	0.183^+0.011 _−0.007	9.531361^+0.000018 _−0.000017	0.07928^+0.00096 _−0.00091	650.0^+6.0 _−5.9	quá cảnh	191.2± 0.4	0.732^+0.027 _−0.025	4622⁺⁶¹ ₋₅₉	^[99]
TOI-712 c	0.0274	0.241^+0.008 _−0.007	51.69906± 0.00017	0.2447^+0.0030 _−0.0028	369.9^+3.4 _−3.3	quá cảnh	191.2± 0.4	0.732^+0.027 _−0.025	4622⁺⁶¹ ₋₅₉	^[99]
TOI-712 d	0.0236	0.221^+0.008 _−0.007	84.83960^+0.00043 _−0.00040	0.3405^+0.0041 _−0.0039	313.6^+2.9 _−2.8	quá cảnh	191.2± 0.4	0.732^+0.027 _−0.025	4622⁺⁶¹ ₋₅₉	^[99]
OGLE-2019-BLG-0468Lb	3.43^+1.83 _−1.17			3.29^+4.15 _−2.52		thấu kính hấp dẫn	14000± 3000	0.92^+0.49 _−0.32		Multiple solutions for orbital parameters^[100]
OGLE-2019-BLG-0468Lc	10.22^+5.46 _−3.50			2.77^+3.49 _−2.12		thấu kính hấp dẫn	14000± 3000	0.92^+0.49 _−0.32		Multiple solutions for orbital parameters^[100]
KMT-2021-BLG-0912Lb	0.022^+0.007 _−0.008			3.03^+3.46 _−2.46		thấu kính hấp dẫn	22000± 3000	0.75^+0.23 _−0.28		Multiple solutions for orbital parameters^[101]
HD 137496 b	0.0127± 0.0017	0.117± 0.005	1.62116± 0.00008	0.02732± 0.00019	2130⁺³⁰ ₋₂₉	quá cảnh	509± 6	1.035± 0.022	5799± 61	^[102]
HD 137496 c	7.66± 0.11		479.9^+1.1 _−1.0	1.2163^+0.0087 _−0.0088	370± 5	vận tốc xuyên tâm	509± 6	1.035± 0.022	5799± 61	^[102]
HD 19615 b	8.5± 0.7		402± 2	1.1± 0.1		vận tốc xuyên tâm	872± 7	1.1± 0.1	3987± 125	Red giant host star^[103]
HD 150010 b	2.4± 0.4		562± 8	1.1± 0.1		vận tốc xuyên tâm	473.4± 2.1	1.3± 0.1	4256± 125	Red giant host star^[103]
HD 174205 b	4.2± 0.5		582± 17	1.7± 0.1		vận tốc xuyên tâm	769± 5	1.8± 0.1	4393± 125	Red giant host star^[103]
KMT-2018-BLG-1988Lb	0.021^+0.015 _−0.011			2.83^+1.23 _−0.97		thấu kính hấp dẫn	14000⁺⁶⁰⁰⁰ ₋₅₀₀₀	0.48^+0.33 _−0.25		Multiple solutions for orbital parameters^[104]
KOI-984b	0.0544± 0.0094	0.384± 0.004	4.2881785± 0.0000035	0.0504± 0.0006	1022⁺³¹ ₋₃₀	quá cảnh	749± 4	0.928± 0.031	5295± 150	Another planet in system on poorly constrained orbit^[105]
TOI-2109b	5.02± 0.75	1.347± 0.047	0.67247414± 0.00000028	0.01791± 0.00065	3631± 69	quá cảnh	846± 9	1.447^+0.075 _−0.078	6530⁺¹⁶⁰ ₋₁₅₀	^[106]
TOI-1238b	0.0183± 0.0035	0.108± 0.010	0.764596^+0.000016 _−0.000013	0.0139± 0.0008	1133± 167	quá cảnh	2030.44± 0.20	0.59± 0.02	4089± 54	^[107]
TOI-1238c	0.0262± 0.0059	0.188± 0.013	3.294733^+0.000040 _−0.000047	0.037± 0.002	695± 105	quá cảnh	2030.44± 0.20	0.59± 0.02	4089± 54	^[107]
K2-99c	8.4± 0.2		522.2± 1.4	1.43± 0.01	390± 6	vận tốc xuyên tâm	1980	1.6	5990	^[108]
HIP 5763b	0.51		30.014^+0.1528 _−0.2842	0.170		vận tốc xuyên tâm	104.17± 0.14	0.72		^[109]
HIP 34222b	0.83		160.0^+2.7 _−2.9	0.492		vận tốc xuyên tâm	74.55± 0.09	0.62		^[109]
HIP 86221b	0.71		2.224^+0.0004 _−0.0005	0.031		vận tốc xuyên tâm	96± 11	0.79		^[109]
TOI-1842b	0.214^+0.040 _−0.038	1.04^+0.06 _−0.05	9.5739^+0.0002 _−0.0001	0.01001± 0.0007		quá cảnh	729± 7	1.46± 0.03	6230± 50	^[110]
Gliese 367b [ja]	0.0017± 0.0002	0.064± 0.005	0.321962^+0.000010 _−0.000012	0.0071± 0.0002	1745± 43	quá cảnh	30.695± 0.016	0.45± 0.011	3522± 70	^[111]
HATS-74Ab	1.46± 0.14	1.032± 0.021	1.73185606± 0.00000055	0.02384± 0.00011	895.1± 5.7	quá cảnh	952± 12	0.601± 0.008	3775± 54	Host star also known as TOI-737^[112]
HATS-75b	0.491± 0.039	0.884± 0.013	2.7886556± 0.0000011	0.032742^+0.000134 _−0.000099	772.3± 2.3	quá cảnh	640± 4	0.6017^+0.0074 _−0.0055	3812± 79	Host star also known as TOI-552^[112]
HATS-76b	2.629± 0.089	1.079± 0.031	1.9416423± 0.0000014	0.02658^+0.00021 _−0.00029	939.8± 6.7	quá cảnh	1272± 19	0.662^+0.016 _−0.021	3990± 120	Host star also known as TOI-555^[112]
HATS-77b	1.374^+0.100 _−0.074	1.165± 0.021	3.0876262± 0.0000016	0.03607± 0.00025	828.3± 5.9	quá cảnh	1440± 40	0.655± 0.014	4082± 69	Host star also known as TOI-730^[112]
KOI-4777b		0.046± 0.003	0.412000± 0.000001	0.0080± 0.0003	1180± 20	quá cảnh	565± 4	0.41± 0.02	3515± 69	^[113]
BD+60 1417b	15± 5	1.31± 0.06		1662	1303± 74	hình ảnh trực tiếp	146.65± 0.09	1.0	4993± 124	Young (≈100 million years) host star^[114]
b Centauri b	10.9± 1.6		200000± 100000	556± 17		hình ảnh trực tiếp	325± 10	8± 2		Circumbinary planet in unusually massive host star system^[115]
HD 360 b	0.75^+0.12 _−0.15		273.1^+1.6 _−0.8	0.98^+0.11 _−0.03		vận tốc xuyên tâm	362	1.69^+0.15 _−0.53	4770	^[116]
Epsilon Piscium b	0.77^+0.16 _−0.10		255.3^+2.1 _−1.4	0.88^+0.11 _−0.10		vận tốc xuyên tâm	183.2	1.41^+1.45 _−0.50	4824	Planetary candidate, unconfirmed^[116]
HD 10975 b	0.45^+0.06 _−0.15		283.8^+12.7 _−0.1	0.95^+0.06 _−0.08		vận tốc xuyên tâm	379	1.41^+0.34 _−0.35	4840	^[116]
HD 79181 b	0.64^+0.06 _−0.16		273.1^+1.3 _−0.4	0.90^+0.07 _−0.08		vận tốc xuyên tâm	337	1.28^+0.32 _−0.28	4862	^[116]
HD 99183 b	0.97^+0.06 _−0.25		310.4^+5.2 _−1.7	1.08^+0.05 _−0.07		vận tốc xuyên tâm	355	1.76^+0.31 _−0.30	4886	^[116]
Upsilon Leonis b	0.51^+0.06 _−0.26		385.2^+2.8 _−1.3	1.18^+0.11 _−0.32		vận tốc xuyên tâm	177.8	1.48^+0.90 _−0.38	4836	^[116]
HD 161178 b	0.57^+0.02 _−0.16		279.3^+1.0 _−0.8	0.85^+0.05 _−0.07		vận tốc xuyên tâm	351	1.06^+0.25 _−0.17	4786	^[116]
HD 219139 b	0.78^+0.05 _−0.20		275.5^+2.3 _−1.0	0.94^+0.06 _−0.07		vận tốc xuyên tâm	345	1.46^+0.31 _−0.29	4831	^[116]
Gamma Piscium b	1.34^+0.02 _−0.31		555.1^+6.0 _−2.5	1.32^+0.05 _−0.08		vận tốc xuyên tâm	138	0.99^+0.17 _−0.13	4742	^[116]
OGLE-2014-BLG-0676Lb	3.68^+0.69 _−1.44			4.53^+1.49 _−2.50		thấu kính hấp dẫn	8700⁺²⁵⁰⁰ ₋₄₆₀₀	0.73^+0.14 _−0.29		^[117]
HD 103891 b	1.44^+0.06 _−0.05		1919⁺¹⁴ ₋₁₅	3.27^+0.02 _−0.01		vận tốc xuyên tâm	179.0± 0.4	1.28± 0.01	6072± 20	^[118]
HD 105779 b	0.64± 0.06		2412⁺⁵⁵ ₋₅₂	3.38± 0.05		vận tốc xuyên tâm	179.7± 0.3	0.89± 0.01	5792± 16	^[118]
HD 73583b		0.253^+0.014 _−0.011	6.3980661^+0.0000095 _−0.0000097	0.05995^+0.00074 _−0.00072	742.7^+7.2 _−7.0	quá cảnh	102.97± 0.10	0.701^+0.026 _−0.025	4574⁺⁶² ₋₆₁	Host star also known as TOI 560^[119]
HD 73583c		0.2433^+0.011 _−0.0096	18.8805^+0.0024 _−0.0011	0.1233± 0.0015	517.8⁺⁵ _−4.9	quá cảnh	102.97± 0.10	0.701^+0.026 _−0.025	4574⁺⁶² ₋₆₁	Host star also known as TOI 560^[119]
OGLE-2014-BLG-0319Lb	0.57^+0.36 _−0.31			3.49^+1.17 _−1.12		thấu kính hấp dẫn	25000⁺⁴⁰⁰⁰ ₋₉₀₀₀	0.52^+0.33 _−0.29		^[120]
OGLE-2018-BLG-0383L b	0.0201^+0.0173 _−0.0088			1.8± 0.2		thấu kính hấp dẫn	25000± 2000	0.10^+0.13 _−0.05		^[121]

Xem thêm

Tham khảo

^ “HD 108236 f”, exoplanet.eu, truy cập ngày 4 tháng 1 năm 2021
^ Bonfanti, A.; và đồng nghiệp (2021), “CHEOPS observations of the HD 108236 planetary system: A fifth planet, improved ephemerides, and planetary radii”, Astronomy & Astrophysics, 646: A157, arXiv:2101.00663, Bibcode:2021A&A...646A.157B, doi:10.1051/0004-6361/202039608, S2CID 230437723
^ Smith, A. M. S.; và đồng nghiệp (2021), “NGTS-14Ab: A Neptune-sized transiting planet in the desert”, Astronomy & Astrophysics, 646: A183, arXiv:2101.01470, Bibcode:2021A&A...646A.183S, doi:10.1051/0004-6361/202039712, S2CID 230524042
^ Martin, David V.; và đồng nghiệp (2021), “TOI-1259Ab – a gas giant planet with 2.7 per cent deep transits and a bound white dwarf companion”, Monthly Notices of the Royal Astronomical Society, 507 (3): 4132–4148, arXiv:2101.02707, doi:10.1093/mnras/stab2129
^ Grieves, Nolan; và đồng nghiệp (2021), “NGTS-13b: A hot 4.8 Jupiter-mass planet transiting a subgiant star”, Astronomy & Astrophysics, 647: A180, arXiv:2101.04245, Bibcode:2021A&A...647A.180G, doi:10.1051/0004-6361/202039586, S2CID 231582818
^ ^a ^b ^c ^d ^e Rodriguez, Joseph E.; và đồng nghiệp (2021), “TESS Delivers Five New Hot Giant Planets Orbiting Bright Stars from the Full-frame Images”, The Astronomical Journal, 161 (4): 194, arXiv:2101.01726, Bibcode:2021AJ....161..194R, doi:10.3847/1538-3881/abe38a, S2CID 230770138
^ Yee, Jennifer C.; và đồng nghiệp (2021), “OGLE-2019-BLG-0960 Lb: The Smallest Microlensing Planet”, The Astronomical Journal, 162 (5): 180, arXiv:2101.04696, Bibcode:2021AJ....162..180Y, doi:10.3847/1538-3881/ac1582, S2CID 231592669
^ ^a ^b Osborn, H. P.; và đồng nghiệp (2021), “A hot mini-Neptune in the radius valley orbiting solar analogue HD 110113”, Monthly Notices of the Royal Astronomical Society, 502 (4): 4842–4857, arXiv:2101.04745, Bibcode:2021MNRAS.502.4842O, doi:10.1093/mnras/stab182
^ Hirsch, Lea A.; và đồng nghiệp (2017), “ASSESSING THE EFFECT OF STELLAR COMPANIONS FROM HIGH-RESOLUTION IMAGING OF Kepler OBJECTS OF INTEREST”, The Astronomical Journal, 153 (3): 117, arXiv:1701.06577, Bibcode:2017AJ....153..117H, doi:10.3847/1538-3881/153/3/117, S2CID 39321033
^ “AT LAST! CONFIRMATION OF KEPLER'S SECOND PLANETARY CANDIDATE” (PDF). Lưu trữ (PDF) bản gốc ngày 15 tháng 1 năm 2021. Truy cập ngày 18 tháng 1 năm 2021.
^ ^a ^b ^c ^d ^e ^f Leleu, A.; và đồng nghiệp (2021), “Six transiting planets and a chain of Laplace resonances in TOI-178”, Astronomy & Astrophysics, 649: A26, arXiv:2101.09260, Bibcode:2021A&A...649A..26L, doi:10.1051/0004-6361/202039767, S2CID 231693292
^ Palatnick, Skyler; và đồng nghiệp (2021), “Validation of HD 183579b Using Archival Radial Velocities: A Warm Neptune Orbiting a Bright Solar Analog”, The Astrophysical Journal Letters, 909 (1): L6, arXiv:2101.12137, Bibcode:2021ApJ...909L...6P, doi:10.3847/2041-8213/abe0bb, S2CID 231719821
^ Gan, Tianjun; và đồng nghiệp (2021), “HD 183579b: A Warm Sub-Neptune Transiting a Solar Twin Detected by TESS”, Monthly Notices of the Royal Astronomical Society, 507 (2): 2220–2240, arXiv:2107.14015, doi:10.1093/mnras/stab2224
^ Yun Hak Kim; và đồng nghiệp (2021), “KMT-2019-BLG-0371 and the Limits of Bayesian Analysis”, The Astronomical Journal, 162 (1): 17, arXiv:2101.12206, Bibcode:2021AJ....162...17K, doi:10.3847/1538-3881/abf930, S2CID 231728667
^ ^a ^b Sozzetti, A.; và đồng nghiệp (2021), “A sub-Neptune and a non-transiting Neptune-mass companion unveiled by ESPRESSO around the bright late-F dwarf HD 5278 (TOI-130)”, Astronomy & Astrophysics, 648: A75, arXiv:2101.12300, Bibcode:2021A&A...648A..75S, doi:10.1051/0004-6361/202040034, S2CID 231728514
^ Han, Cheongho; và đồng nghiệp (2021), “KMT-2018-BLG-1025Lb: Microlensing super-Earth planet orbiting a low-mass star”, Astronomy & Astrophysics, 649: A90, arXiv:2102.01890, Bibcode:2021A&A...649A..90H, doi:10.1051/0004-6361/202039817, S2CID 231786450
^ ^a ^b Ikwut-Ukwa, Mma; và đồng nghiệp (2022), “Two Massive Jupiters in Eccentric Orbits from the TESS Full-frame Images”, The Astronomical Journal, 163 (1): 9, arXiv:2102.02222, Bibcode:2022AJ....163....9I, doi:10.3847/1538-3881/ac2ee1, S2CID 231802379
^ ^a ^b Mayor, M.; Marmier, M.; Lovis, C.; Udry, S.; Ségransan, D.; Pepe, F.; Benz, W.; Bertaux, J. -L.; Bouchy, F. (2011). "The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets". arΧiv:1109.2497 [astro-ph.EP].
^ ^a ^b Ahrer, E.; và đồng nghiệp (2021), “The HARPS search for southern extra-solar planets XLV. Two Neptune mass planets orbiting HD 13808: a study of stellar activity modelling's impact on planet detection”, Monthly Notices of the Royal Astronomical Society, 503 (1): 1248–1263, arXiv:2102.03387, Bibcode:2021MNRAS.503.1248A, doi:10.1093/mnras/stab373
^ ^a ^b ^c Newton, Elisabeth R.; và đồng nghiệp (2021), “TESS Hunt for Young and Maturing Exoplanets (THYME) IV: Three small planets orbiting a 120 Myr-old star in the Pisces–Eridanus stream”, The Astronomical Journal, 161 (2): 65, arXiv:2102.06049, Bibcode:2021AJ....161...65N, doi:10.3847/1538-3881/abccc6, S2CID 231879927
^ ^a ^b ^c Barragán, Oscar; và đồng nghiệp (2021), “TESS re-observes the young multi-planet system TOI-451:refined ephemeris and activity evolution”, Research Notes of the American Astronomical Society, 5 (3): 51, arXiv:2103.09746, Bibcode:2021RNAAS...5...51B, doi:10.3847/2515-5172/abef70, S2CID 232258104
^ Tofflemire, Benjamin M.; và đồng nghiệp (2021), “TESS Hunt for Young and Maturing Exoplanets (THYME). V. A Sub-Neptune Transiting a Young Star in a Newly Discovered 250 Myr Association”, The Astronomical Journal, 161 (4): 171, arXiv:2102.06066, Bibcode:2021AJ....161..171T, doi:10.3847/1538-3881/abdf53, S2CID 231879915
^ ^a ^b Kil Jung, Youn; và đồng nghiệp (2021), “OGLE-2018-BLG-0567Lb and OGLE-2018-BLG-0962Lb: Two Microlensing Planets through the Planetary-caustic Channel”, The Astronomical Journal, 161 (6): 293, arXiv:2102.07338, Bibcode:2021AJ....161..293J, doi:10.3847/1538-3881/abf8bd, S2CID 231924992
^ Toledo-Padrón, B.; và đồng nghiệp (2021), “A super-Earth on a close-in orbit around the M1V star GJ 740”, Astronomy & Astrophysics, 648: A20, arXiv:2102.09441, doi:10.1051/0004-6361/202040099, S2CID 231951695
^ Kains, N.; và đồng nghiệp (2021), “A giant planet beyond the snow line in microlensing event OGLE-2011-BLG-0251”, Astronomy & Astrophysics, 552: A70, arXiv:1303.1184, Bibcode:2013A&A...552A..70K, doi:10.1051/0004-6361/201220626, S2CID 43146154
^ Soto, M. G.; và đồng nghiệp (2021), “Mass and density of the transiting hot and rocky super-Earth LHS 1478 b (TOI-1640 b)”, Astronomy & Astrophysics, 649: A144, arXiv:2102.11640, Bibcode:2021A&A...649A.144S, doi:10.1051/0004-6361/202140618, S2CID 232013854
^ ^a ^b Bluhm, P.; và đồng nghiệp (2021), “An ultra-short-period transiting super-Earth orbiting the M3 dwarf TOI-1685”, Astronomy & Astrophysics, 650: A78, arXiv:2103.01016, Bibcode:2021A&A...650A..78B, doi:10.1051/0004-6361/202140688, S2CID 232092636
^ ^a ^b Hirano, Teruyuki; và đồng nghiệp (2021), “Two Bright M Dwarfs Hosting Ultra-Short-Period Super-Earths with Earth-like Compositions”, The Astronomical Journal, 162 (4): 161, arXiv:2103.12760, Bibcode:2021AJ....162..161H, doi:10.3847/1538-3881/ac0fdc, S2CID 232335413
^ Zang, Weicheng; và đồng nghiệp (2021), “An Earth-mass planet in a time of COVID-19: KMT-2020-BLG-0414Lb”, Research in Astronomy and Astrophysics, 21 (9): 239, arXiv:2103.01896, Bibcode:2021RAA....21..239Z, doi:10.1088/1674-4527/21/9/239, S2CID 232092272
^ Hobson, Melissa J.; và đồng nghiệp (2021), “A Transiting Warm Giant Planet around the Young Active Star TOI-201”, The Astronomical Journal, 161 (5): 235, arXiv:2103.02685, Bibcode:2021AJ....161..235H, doi:10.3847/1538-3881/abeaa1, S2CID 232110390
^ Trifonov, T.; và đồng nghiệp (2021), “A nearby transiting rocky exoplanet that is suitable for atmospheric investigation”, Science, 371 (6533): 1038–1041, arXiv:2103.04950, Bibcode:2021Sci...371.1038T, doi:10.1126/science.abd7645, PMID 33674491, S2CID 232124642
^ ^a ^b ^c ^d Tilbrook, Rosanna H.; và đồng nghiệp (2021), “NGTS 15b, 16b, 17b, and 18b: Four hot Jupiters from the Next-Generation Transit Survey”, Monthly Notices of the Royal Astronomical Society, 504 (4): 6018–6032, arXiv:2103.10302, doi:10.1093/mnras/stab815
^ Zang, Weicheng; và đồng nghiệp (2021), “Systematic KMTNet Planetary Anomaly Search. I. OGLE-2019-BLG-1053Lb, a Buried Terrestrial Planet”, The Astronomical Journal, 162 (4): 163, arXiv:2103.11880, Bibcode:2021AJ....162..163Z, doi:10.3847/1538-3881/ac12d4, S2CID 232307459
^ Cloutier, R.; và đồng nghiệp (2021), “TOI-1634 b: An Ultra-short-period Keystone Planet Sitting inside the M-dwarf Radius Valley”, The Astronomical Journal, 162 (2): 79, arXiv:2103.12790, Bibcode:2021AJ....162...79C, doi:10.3847/1538-3881/ac0157, S2CID 232335385
^ Han, Cheongho; và đồng nghiệp (2021), “KMT-2019-BLG-1715: Planetary Microlensing Event with Three Lens Masses and Two Source Stars”, The Astronomical Journal, 161 (6): 270, arXiv:2104.00293, Bibcode:2021AJ....161..270H, doi:10.3847/1538-3881/abf4d0, S2CID 232478488
^ Kondo, Iona; và đồng nghiệp (2021), “OGLE-2018-BLG-1185b: A Low-mass Microlensing Planet Orbiting a Low-mass Dwarf”, The Astronomical Journal, 162 (2): 77, arXiv:2104.02157, Bibcode:2021AJ....162...77K, doi:10.3847/1538-3881/ac00ba, S2CID 233033627
^ ^a ^b Georgieva, I. Y.; và đồng nghiệp (2021), “Hot planets around cool stars – two short-period mini-Neptunes transiting the late K-dwarf TOI-1260”, Monthly Notices of the Royal Astronomical Society, 505 (4): 4684–4701, arXiv:2104.05653, doi:10.1093/mnras/stab1464
^ ^a ^b ^c Han, Cheongho; và đồng nghiệp (2021), “Three microlensing planets with no caustic-crossing features”, Astronomy & Astrophysics, 650: A89, arXiv:2104.06544, Bibcode:2021A&A...650A..89H, doi:10.1051/0004-6361/202140758, S2CID 233231384
^ Bohn, Alexander J.; và đồng nghiệp (2021), “Discovery of a directly imaged planet to the young solar analog YSES 2”, Astronomy & Astrophysics, 648: A73, arXiv:2104.08285, Bibcode:2021A&A...648A..73B, doi:10.1051/0004-6361/202140508, S2CID 233296087
^ Ryu, Yoon-Hyun; và đồng nghiệp (2021), “Shortest Microlensing Event with a Bound Planet: KMT-2016-BLG-2605”, The Astronomical Journal, 162 (3): 96, arXiv:2104.07906, Bibcode:2021AJ....162...96R, doi:10.3847/1538-3881/ac062a, S2CID 233289612
^ Brett Christopher Addison; và đồng nghiệp (2021), “TOI-1431b/MASCARA-5b: An Ultra-hot Jupiter Orbiting One of the Hottest & Brightest Known Exoplanet Host Stars”, Posters from the Tess Science Conference Ii (Tsc2: 64, arXiv:2104.12078, Bibcode:2021tsc2.confE..64A, doi:10.5281/zenodo.5126266, S2CID 240578462
^ Stangret, M.; và đồng nghiệp (2021), “The obliquity and atmosphere of the ultra-hot Jupiter TOI-1431b (MASCARA-5b): A misaligned orbit and no signs of atomic or molecular absorptions”, Astronomy & Astrophysics, 654: A73, arXiv:2104.12414, Bibcode:2021A&A...654A..73S, doi:10.1051/0004-6361/202040100, S2CID 233393996
^ Cointepas, M.; và đồng nghiệp (2021), “TOI-269 b: An eccentric sub-Neptune transiting a M2 dwarf revisited with ExTrA”, Astronomy & Astrophysics, 650: A145, arXiv:2104.14782, Bibcode:2021A&A...650A.145C, doi:10.1051/0004-6361/202140328, S2CID 233476660
^ Hoyer, S.; và đồng nghiệp (2021), “TOI-220 b: A warm sub-Neptune discovered by TESS”, Monthly Notices of the Royal Astronomical Society, 505 (3): 3361–3379, arXiv:2105.01944, doi:10.1093/mnras/stab1427
^ ^a ^b Otegi, J. F.; và đồng nghiệp (2021), “TESS and HARPS reveal two sub-Neptunes around TOI 1062”, Astronomy & Astrophysics, 653: A105, arXiv:2105.01945, Bibcode:2021A&A...653A.105O, doi:10.1051/0004-6361/202040247, S2CID 233739805
^ Zhang, Jingwen; và đồng nghiệp (2021), “Long-period Jovian Tilts the Orbits of Two sub-Neptunes Relative to Stellar Spin Axis in Kepler-129”, The Astronomical Journal, 162 (3): 89, arXiv:2105.03446, Bibcode:2021AJ....162...89Z, doi:10.3847/1538-3881/ac0634, S2CID 234338914
^ Maldonado, J.; và đồng nghiệp (2021), “HADES RV programme with HARPS-N at TNG”, Astronomy & Astrophysics, 651: A93, arXiv:2105.06155, doi:10.1051/0004-6361/202141141, S2CID 234482717
^ Burt, Jennifer A.; và đồng nghiệp (2021), “TOI-1231 b: A Temperate, Neptune-sized Planet Transiting the Nearby M3 Dwarf NLTT 24399”, The Astronomical Journal, 162 (3): 87, arXiv:2105.08077, Bibcode:2021AJ....162...87B, doi:10.3847/1538-3881/ac0432, S2CID 234763319
^ Kostov, Veselin B.; và đồng nghiệp (2021), “TIC 172900988: A Transiting Circumbinary Planet Detected in One Sector of TESS Data”, The Astronomical Journal, 162 (6): 234, arXiv:2105.08614, Bibcode:2021AJ....162..234K, doi:10.3847/1538-3881/ac223a, S2CID 234762777
^ Dai, Fei; Howard, Andrew W.; Batalha, Natalie M.; Beard, Corey; Behmard, Aida; Blunt, Sarah; Brinkman, Casey L.; Chontos, Ashley; Crossfield, Ian J. M. (2021). "TKS X: Confirmation of TOI-1444b and a Comparative Analysis of the Ultra-short-period Planets with Hot Neptunes". arΧiv:2105.08844 [astro-ph.EP].
^ ^a ^b ^c ^d ^e ^f Dalal, S.; và đồng nghiệp (2021), “The SOPHIE search for northern extrasolar planets”, Astronomy & Astrophysics, 651: A11, arXiv:2105.09741, doi:10.1051/0004-6361/202140712, S2CID 234790136
^ ^a ^b ^c ^d ^e ^f ^g ^h ⁱ ^j ^k ^l ^m Rosenthal, Lee J.; và đồng nghiệp (2021), “The California Legacy Survey. I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades”, The Astrophysical Journal Supplement Series, 255 (1): 8, arXiv:2105.11583, Bibcode:2021ApJS..255....8R, doi:10.3847/1538-4365/abe23c, S2CID 235186973
^ ^a ^b ^c Amado, Pedro J.; Bauer, Florian F.; Rodríguez López, Cristina; Rodríguez, Eloy; Cardona Guillén, C.; Perger, M.; Caballero, José A.; López-González, Maria J.; Muñoz Rodríguez, I.; Pozuelos, F. J.; Sánchez-Rivero, A.; Schlecker, M.; Quirrenbach, Andreas; Ribas, Ignasi; Reiners, Ansgar; Almenara, J.; Astudillo-Defru, N.; Azzaro, M.; Béjar, Victor J. S.; Bohemann, R.; Bonfils, X.; Bouchy, F.; Cifuentes, C.; Cortés-Contreras, M.; Delfosse, Xavier; Dreizler, Stefan; Forveille, Thierry; Hatzes, Artie P.; Henning, Thomas K.; Jeffers, Sandra V.; Kaminski, Adrian; Kürster, Martin; Lafarga, M.; Lodieu, Nicolas; Lovis, C.; Mayor, M.; Montes, David; Morales, Juan Carlos; Morales, Nicolás; Murgas, F.; Ortiz, José L.; Pepe, F.; Perdelwitz, V.; Pollaco, D.; Santos, N. C.; Schöfer, P.; Schweitzer, A.; Ségransan, N. C.; Shan, Y.; Stock, S.; Tal-Or, Lev; Udry, S.; Zapatero-Osorio, María Rosa; Zechmeister, Mathias (28 tháng 5 năm 2021). “The CARMENES search for exoplanets around M dwarfs”. Astronomy & Astrophysics. 650: A188. arXiv:2105.13785. doi:10.1051/0004-6361/202140633. S2CID 235248027.
^ Murgas, F.; và đồng nghiệp (2021), “TOI-674b: An oasis in the desert of exo-Neptunes transiting a nearby M dwarf”, Astronomy & Astrophysics, 653: A60, arXiv:2106.01246, Bibcode:2021A&A...653A..60M, doi:10.1051/0004-6361/202140718, S2CID 235294286
^ Brande, Jonathan; Crossfield, Ian J. M.; Kreidberg, Laura; Oklopčić, Antonija; Polanski, Alex S.; Barman, Travis; Benneke, Björn; Christiansen, Jessie L.; Dragomir, Diana; Foreman-Mackey, Daniel; Fortney, Jonathan J.; Greene, Thomas P.; Howard, Andrew W.; Knutson, Heather A.; Lothringer, Joshua D.; Mikal-Evans, Thomas; Morley, Caroline V. (2022), “A Mirage or an Oasis? Water Vapor in the Atmosphere of the Warm Neptune TOI-674 B”, The Astronomical Journal, 164 (5): 197, arXiv:2201.04197, doi:10.3847/1538-3881/ac8b7e, S2CID 245877576
^ ^a ^b Eisner, N. L.; và đồng nghiệp (2021), “Planet Hunters TESS III: Two transiting planets around the bright G dwarf HD 152843”, Monthly Notices of the Royal Astronomical Society, 505 (2): 1827–1840, arXiv:2106.04603, doi:10.1093/mnras/stab1253
^ ^a ^b ^c ^d ^e Hwang, Kyu-Ha; và đồng nghiệp (2021), “Systematic KMTNet Planetary Anomaly Search, Paper II: Five New q<2×10−4 Mass-ratio Planets”, arXiv:2106.06686, doi:10.3847/1538-3881/ac38ad, S2CID 245740102 Chú thích journal cần |journal= (trợ giúp)
^ Khandelwal, Akanksha; và đồng nghiệp (2021), “Discovery of an inflated hot Jupiter around a slightly evolved star TOI-1789”, Monthly Notices of the Royal Astronomical Society, arXiv:2106.08660, doi:10.1093/mnras/stab2970
^ ^a ^b Wirth, Christopher P.; và đồng nghiệp (2021), “TOI-942b: A Prograde Neptune in a ∼ 60 Myr Old Multi-transiting System”, The Astrophysical Journal Letters, 917 (2): L34, arXiv:2106.14968, Bibcode:2021ApJ...917L..34W, doi:10.3847/2041-8213/ac13a9, S2CID 235670113
^ Han, Cheongho; và đồng nghiệp (2021), “KMT-2018-BLG-1743: Planetary microlensing event occurring on two source stars”, Astronomy & Astrophysics, 652: A145, arXiv:2107.00155, Bibcode:2021A&A...652A.145H, doi:10.1051/0004-6361/202140923, S2CID 235694685
^ ^a ^b ^c Fukui, A.; và đồng nghiệp (2021), “TOI-1749: An M dwarf with a Trio of Planets including a Near-resonant Pair”, The Astronomical Journal, 162 (4): 167, arXiv:2107.05430, Bibcode:2021AJ....162..167F, doi:10.3847/1538-3881/ac13a5, S2CID 235795469
^ ^a ^b ^c ^d ^e ^f Demangeon, O. D. S.; và đồng nghiệp (2021), “The SOPHIE search for northern extrasolar planets”, Astronomy & Astrophysics, 653: A78, arXiv:2107.05089, doi:10.1051/0004-6361/202141079, S2CID 235795175
^ Dalba, Paul A.; và đồng nghiệp (2021), “Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. II. Discovery of a Failed Hot Jupiter on a 2.7 Yr, Highly Eccentric Orbit”, The Astronomical Journal, 162 (4): 154, arXiv:2107.06901, Bibcode:2021AJ....162..154D, doi:10.3847/1538-3881/ac134b, S2CID 235898945
^ Kanodia, Shubham; và đồng nghiệp (2021), “TOI-532b: The Habitable-zone Planet Finder confirms a Large Super Neptune in the Neptune Desert orbiting a metal-rich M-dwarf host”, The Astronomical Journal, 162 (4): 135, arXiv:2107.13670, Bibcode:2021AJ....162..135K, doi:10.3847/1538-3881/ac1940, S2CID 236493328
^ Wells, R. D.; và đồng nghiệp (2021), “A large sub-Neptune transiting the thick-disk M4 V TOI-2406”, Astronomy & Astrophysics, 653: A97, arXiv:2107.14125, Bibcode:2021A&A...653A..97W, doi:10.1051/0004-6361/202141277, S2CID 236493492
^ ^a ^b ^c Lillo-Box, J.; và đồng nghiệp (2021), “Follow-up of non-transiting planets detected by Kepler”, Astronomy & Astrophysics, 654: A9, arXiv:2107.14621, doi:10.1051/0004-6361/202140746, S2CID 236635201
^ Winters, Jennifer G.; Cloutier, Ryan; Medina, Amber A.; Irwin, Jonathan M.; Charbonneau, David; Astudillo-Defru, Nicola; Bonfils, Xavier; Howard, Andrew W.; Isaacson, Howard; Bean, J. L.; Seifahrt, A.; Teske, J. K.; Eastman, Jason D.; Twicken, Joseph D.; Collins, K. A.; Jensen, E. L. N.; Quinn, S. N.; Payne, M. J.; Kristiansen, M. H.; Spencer, A.; Vanderburg, Andrew; Zechmeister, Mathias; Weiss, L. M.; Wang, S. X.; Wang, G.; Udry, Stéphane; Terentev, I. A.; Sturmer, J.; Stefansson, G.; Shectman, Stephen A.; Sefako, R.; Schwengeler, H. M.; Schwarz, R. P.; Scarsdale, N.; Rubenzahl, R. A.; Roy, A.; Rosenthal, L. J.; Robertson, P.; Petigura, Erik A.; Pepe, Francesco; Omohundro, M.; Murphy, J. M. A.; Murgas, Felipe; Movcnik, T.; Montet, B. T.; Mennickent, R.; Mayo, A. W.; Massey, B.; Lubin, J.; Lovis, Christophe; Lewin, P.; Kasper, D.; Kane, S. R.; Jenkins, J. M.; Huber, D.; Horne, K.; Hill, M. L.; Gorrini, P.; Giacalone, S.; Fulton, Benjamin J.; Forveille, Thierry; Figueira, Pedro; Fetherolf, T.; Dressing, Courtney D.; Díaz, Rodrigo F.; Delfosse, Xavier; Dalba, P. A.; Dai, F.; Cortes, C. C.; Crossfield, Ian J. M.; Crane, Jeffrey D.; Conti, D. M.; Collins, K. I.; Chontos, A.; Butler, R. Paul; Brown, P.; Brady, M.; Bouchy, François; Behmard, A.; Beard, C.; Batalha, Natalie M.; Almenara, José M. (2022). “A Second Planet Transiting LTT 1445A and a Determination of the Masses of Both Worlds”. The Astronomical Journal. 163 (4): 168. arXiv:2107.14737. Bibcode:2022AJ....163..168W. doi:10.3847/1538-3881/ac50a9. S2CID 236635391.
^ ^a ^b “A warm terrestrial planet with half the mass of Venus transiting a nearby star” (PDF). Lưu trữ (PDF) bản gốc ngày 13 tháng 11 năm 2021. Truy cập ngày 8 tháng 8 năm 2021.
^ Lubin, Jack; và đồng nghiệp (2022), “TESS-Keck Survey. IX. Masses of Three Sub-Neptunes Orbiting HD 191939 and the Discovery of a Warm Jovian plus a Distant Substellar Companion”, The Astronomical Journal, 163 (2): 101, arXiv:2108.02208, Bibcode:2022AJ....163..101L, doi:10.3847/1538-3881/ac3d38, S2CID 236924440
^ Shin, In-Gu; và đồng nghiệp (2021), “Using Source Proper Motion to Validate Terrestrial Parallax: OGLE-2019-BLG-1058”, The Astronomical Journal, 162 (6): 267, arXiv:2108.02499, Bibcode:2021AJ....162..267S, doi:10.3847/1538-3881/ac2ba5, S2CID 236924486
^ Saunders, Nicholas; và đồng nghiệp (2022), “TESS Giants Transiting Giants. I.: A Noninflated Hot Jupiter Orbiting a Massive Subgiant”, The Astronomical Journal, 163 (2): 53, arXiv:2108.02294, Bibcode:2022AJ....163...53S, doi:10.3847/1538-3881/ac38a1, S2CID 236924647
^ ^a ^b ^c Osborn, Ares; và đồng nghiệp (2021), “TOI-431/HIP 26013: a super-Earth and a sub-Neptune transiting a bright, early K dwarf, with a third RV planet”, Monthly Notices of the Royal Astronomical Society, 507 (2): 2782–2803, arXiv:2108.02310, doi:10.1093/mnras/stab2313
^ ^a ^b Trifonov, Trifon; và đồng nghiệp (2021), “A Pair of Warm Giant Planets near the 2:1 Mean Motion Resonance around the K-dwarf Star TOI-2202”, The Astronomical Journal, 162 (6): 283, arXiv:2108.05323, Bibcode:2021AJ....162..283T, doi:10.3847/1538-3881/ac1bbe, S2CID 236976243
^ ^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 De Leon, J. P.; và đồng nghiệp (2021), “37 New Validated Planets in Overlapping K2 Campaigns”, Monthly Notices of the Royal Astronomical Society, 508: 195–218, arXiv:2108.05621, doi:10.1093/mnras/stab2305
^ Kovacs, Geza (2020), “More planetary candidates from K2 Campaign 5 using TRAN_K2”, Astronomy & Astrophysics, 643: A169, arXiv:2008.10075, Bibcode:2020A&A...643A.169K, doi:10.1051/0004-6361/202038726, S2CID 221266076
^ Lillo-Box, J.; và đồng nghiệp (2021), “HD 22496 b: The first ESPRESSO stand-alone planet discovery”, Astronomy & Astrophysics, 654: A60, arXiv:2109.00226, Bibcode:2021A&A...654A..60L, doi:10.1051/0004-6361/202141714, S2CID 237371680
^ ^a ^b ^c ^d Castro-González, A.; và đồng nghiệp (2022), “The K2-OjOS Project: New and revisited planets and candidates in K2 campaigns 5, 16, & 18”, Monthly Notices of the Royal Astronomical Society, 509: 1075–1095, arXiv:2109.03346, doi:10.1093/mnras/stab2669
^ Dong, Jiayin; và đồng nghiệp (2021), “TOI-3362b: A Proto Hot Jupiter Undergoing High-eccentricity Tidal Migration”, The Astrophysical Journal Letters, 920 (1): L16, arXiv:2109.03771, Bibcode:2021ApJ...920L..16D, doi:10.3847/2041-8213/ac2600, S2CID 237442300
^ ^a ^b ^c Han, Cheongho; và đồng nghiệp (2021), “Three faint-source microlensing planets detected via the resonant-caustic channel”, Astronomy & Astrophysics, 655: A21, arXiv:2109.07068, Bibcode:2021A&A...655A..21H, doi:10.1051/0004-6361/202141517, S2CID 237513708
^ ^a ^b Moutou, C.; và đồng nghiệp (2021), “TOI-1296b and TOI-1298b observed with TESS and SOPHIE: Two hot Saturn-mass exoplanets with different densities around metal-rich stars”, Astronomy & Astrophysics, 653: A147, arXiv:2109.09252, Bibcode:2021A&A...653A.147M, doi:10.1051/0004-6361/202141151, S2CID 237571683
^ Kossakowski, D.; và đồng nghiệp (2021), “TOI-1201 b: A mini-Neptune transiting a bright and moderately young M dwarf”, Astronomy & Astrophysics, 656: A124, arXiv:2109.09346, Bibcode:2021A&A...656A.124K, doi:10.1051/0004-6361/202141587, S2CID 237571914
^ Rattanamala, R.; Awiphan, S.; Komonjinda, S.; Phriksee, A.; Sappankum, P.; A-thano, N.; Chitchak, S.; Rittipruk, P.; Sawangwit, U.; Poshyachinda, S.; Reichart, D. E.; Haislip, J. B. (2021), Two circumbinary planets in RR Cae eclipsing binary system, arXiv:2109.09397
^ Montalto, M.; Malavolta, L.; Gregorio, J.; Mantovan, G.; Desidera, S.; Piotto, G.; Nascimbeni, V.; Granata, V.; Manthopoulou, E. E.; Claudi, R. (2022), “TIC 257060897b: An inflated, low-density, hot-Jupiter transiting a rapidly evolving subgiant star”, Monthly Notices of the Royal Astronomical Society, 509 (2): 2908–2919, arXiv:2110.00489, doi:10.1093/mnras/stab2923
^ Gan, Tianjun; và đồng nghiệp (2021), “TOI-530b: A giant planet transiting an M dwarf detected by TESS”, Monthly Notices of the Royal Astronomical Society, 511: 83–99, arXiv:2110.04220, doi:10.1093/mnras/stab3708
^ ^a ^b MacDougall, Mason G.; và đồng nghiệp (2021), “The TESS–Keck Survey. VI. Two Eccentric Sub-Neptunes Orbiting HIP-97166”, The Astronomical Journal, 162 (6): 265, arXiv:2110.05628, Bibcode:2021AJ....162..265M, doi:10.3847/1538-3881/ac295e, S2CID 238634523
^ ^a ^b Scarsdale, Nicholas; và đồng nghiệp (2021), “TESS-Keck Survey. V. Twin Sub-Neptunes Transiting the Nearby G Star HD 63935”, The Astronomical Journal, 162 (5): 215, arXiv:2110.06885, Bibcode:2021AJ....162..215S, doi:10.3847/1538-3881/ac18cb, S2CID 238743956
^ Heidari, N.; và đồng nghiệp (2022), “HD 207897 b: A dense sub-Neptune transiting a nearby and bright K-type star”, Astronomy & Astrophysics, 658: A176, arXiv:2110.08597, Bibcode:2022A&A...658A.176H, doi:10.1051/0004-6361/202141429, S2CID 239016573
^ Gaidos, E.; Hirano, T.; Kraus, A. L.; Kuzuhara, M.; Zhang, Z.; Lee, R. A.; Salama, M.; Berger, T. A.; Grunblatt, S. K.; Ansdell, M.; Liu, M. C.; Harakawa, H.; Hodapp, K. W.; Jacobson, S.; Konishi, M.; Kotani, T.; Kudo, T.; Kurokawa, T.; Nishikawa, J.; Omiya, M.; Serizawa, T.; Tamura, M.; Ueda, A.; Vievard, S. (2021), “Zodiacal Exoplanets in Time (ZEIT) XII: A Directly-Imaged Planetary-Mass Companion to a Young Taurus M Dwarf Star”, Monthly Notices of the Royal Astronomical Society, 512: 583–601, arXiv:2110.08655, doi:10.1093/mnras/stab3069
^ “Astronomers Discover Infant Planet – One of the Youngest Exoplanets Ever Observed”. 23 tháng 10 năm 2021. Lưu trữ bản gốc ngày 25 tháng 10 năm 2021. Truy cập ngày 25 tháng 10 năm 2021.
^ Mann, Andrew W.; và đồng nghiệp (2022), “TESS Hunt for Young and Maturing Exoplanets (THYME). VI. An 11 Myr Giant Planet Transiting a Very-low-mass Star in Lower Centaurus Crux”, The Astronomical Journal, 163 (4): 156, arXiv:2110.09531, Bibcode:2022AJ....163..156M, doi:10.3847/1538-3881/ac511d, S2CID 239024522
^ Fukui, Akihiko; và đồng nghiệp (2021), “TOI-2285b: A 1.7 Earth-radius planet near the habitable zone around a nearby M dwarf”, Publications of the Astronomical Society of Japan, 74: L1–L8, arXiv:2110.10215, doi:10.1093/pasj/psab106
^ ^a ^b Silverstein, Michele L.; và đồng nghiệp (2022), “The LHS 1678 System: Two Earth-sized Transiting Planets and an Astrometric Companion Orbiting an M Dwarf Near the Convective Boundary at 20 pc”, The Astronomical Journal, 163 (4): 151, arXiv:2110.12079, Bibcode:2022AJ....163..151S, doi:10.3847/1538-3881/ac32e3, S2CID 239768873
^ ^a ^b Barragán, O.; và đồng nghiệp (2022), “The young HD 73583 (TOI-560) planetary system: Two 10-M⊕ mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarf”, Monthly Notices of the Royal Astronomical Society, 514 (2): 1606–1627, arXiv:2110.13069, doi:10.1093/mnras/stac638
^ Zhang, Michael; Knutson, Heather A.; Wang, Lile; Dai, Fei; Barragán, Oscar (2022), “Escaping Helium from TOI 560.01, a Young Mini-Neptune”, The Astronomical Journal, 163 (2): 67, arXiv:2110.13150, Bibcode:2022AJ....163...67Z, doi:10.3847/1538-3881/ac3fa7, S2CID 239885237
^ ^a ^b ^c ^d Hedges, Christina; và đồng nghiệp (2021), “TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow up”, The Astronomical Journal, 162 (2): 54, arXiv:2111.01311, Bibcode:2021AJ....162...54H, doi:10.3847/1538-3881/ac06cd, S2CID 235805026
^ Peng, Peifeng; Xiong, Hongyi; Li, He; Li, Felix; Wang, Tianqi (2022), New Parameter Measurements for the Ultra-Short-Period Planet TOI-1807b, arXiv:2210.04162
^ Osborn, H.; và đồng nghiệp (2022), “Uncovering the true periods of the young sub-Neptunes orbiting TOI-2076”, Astronomy & Astrophysics, 664: A156, arXiv:2203.03194, doi:10.1051/0004-6361/202243065, S2CID 247292643
^ Schanche, N.; và đồng nghiệp (2022), “TOI-2257 b: A highly eccentric long-period sub-Neptune transiting a nearby M dwarf”, Astronomy & Astrophysics, 657: A45, arXiv:2111.01749, Bibcode:2022A&A...657A..45S, doi:10.1051/0004-6361/202142280, S2CID 240419956
^ ^a ^b ^c Vach, Sydney; và đồng nghiệp (2022), “TOI-712: A System of Adolescent Mini-Neptunes Extending to the Habitable Zone”, The Astronomical Journal, 164 (2): 71, arXiv:2111.02416, doi:10.3847/1538-3881/ac7954, S2CID 242757638
^ ^a ^b Han, Cheongho; và đồng nghiệp (2022), “OGLE-2019-BLG-0468Lb,c: Two microlensing giant planets around a G-type star”, Astronomy & Astrophysics, 658: A93, arXiv:2111.03755, Bibcode:2022A&A...658A..93H, doi:10.1051/0004-6361/202142327, S2CID 243847948
^ Han, Cheongho; và đồng nghiệp (2022), “KMT-2021-BLG-0912Lb: A microlensing super Earth around a K-type star”, Astronomy & Astrophysics, 658: A94, arXiv:2111.04861, Bibcode:2022A&A...658A..94H, doi:10.1051/0004-6361/202142495, S2CID 243860989
^ ^a ^b Azevedo Silva, T.; và đồng nghiệp (2022), “The HD 137496 system: A dense, hot super-Mercury and a cold Jupiter”, Astronomy & Astrophysics, 657: A68, arXiv:2111.08764, Bibcode:2022A&A...657A..68A, doi:10.1051/0004-6361/202141520, S2CID 243809625
^ ^a ^b ^c Jeong, G.; Lee, B. C.; Park, M. G.; Bang, T. Y.; Han, I. (2022), “Search for exoplanets around northern circumpolar stars”, Astronomy & Astrophysics, 662: A12, arXiv:2111.08899, doi:10.1051/0004-6361/202142379, S2CID 244270271
^ Han, Cheongho; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Youn Kil Jung; Kim, Doeon; Lee, Chung-Uk; Mao, Shude; Ryu, Yoon-Hyun; Shin, In-Gu; Shvartzvald, Yossi; Yee, Jennifer C.; Zang, Weicheng; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Hyoun-Woo; Kim, Seung-Lee; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W.; Kim, Chun-Hwey (2022), “KMT-2018-BLG-1988Lb: Microlensing super-Earth orbiting a low-mass disk dwarf”, Astronomy & Astrophysics, 658: A62, arXiv:2111.08955, Bibcode:2022A&A...658A..62H, doi:10.1051/0004-6361/202142077, S2CID 244270928
^ Sun, Leilei; Ioannidis, Panagiotis; Gu, Shenghong; Schmitt, Jürgen H. M. M.; Wang, Xiaobin; Kouwenhoven, M. B. N.; Perdelwitz, Volker; Francesco Flammini Dotti; Czesla, Stefan (2022), “A highly mutually inclined compact warm-Jupiter system KOI-984?”, Monthly Notices of the Royal Astronomical Society, 512 (3): 4604–4617, arXiv:2111.09668, doi:10.1093/mnras/stab3367
^ Wong, Ian; và đồng nghiệp (2021), “TOI-2109: An Ultrahot Gas Giant on a 16 hr Orbit”, The Astronomical Journal, 162 (6): 256, arXiv:2111.12074, Bibcode:2021AJ....162..256W, doi:10.3847/1538-3881/ac26bd, S2CID 244488632
^ ^a ^b González-Álvarez, E.; và đồng nghiệp (2022), “A multi-planetary system orbiting the early-M dwarf TOI-1238”, Astronomy & Astrophysics, 658: A138, arXiv:2111.14602, Bibcode:2022A&A...658A.138G, doi:10.1051/0004-6361/202142128, S2CID 244715047
^ Smith, A M S.; và đồng nghiệp (2021), “K2-99 revisited: A non-inflated warm Jupiter, and a temperate giant planet on a 522-d orbit around a subgiant”, Monthly Notices of the Royal Astronomical Society, 510 (4): 5035–5049, arXiv:2111.14660, doi:10.1093/mnras/stab3497
^ ^a ^b ^c Paredes, Leonardo A.; Henry, Todd J.; Quinn, Samuel N.; Gies, Douglas R.; Hinojosa-Goñi, Rodrigo; James, Hodari-Sadiki; Jao, Wei-Chun; White, Russel J. (2021), “The Solar Neighborhood XLVIII: Nine Giant Planets Orbiting Nearby K Dwarfs, and the CHIRON Spectrograph's Radial Velocity Performance”, The Astronomical Journal, 162 (5): 176, arXiv:2111.15028, Bibcode:2021AJ....162..176P, doi:10.3847/1538-3881/ac082a, S2CID 237285778
^ Wittenmyer, Robert A.; và đồng nghiệp (2021), “TOI-1842b: A Transiting Warm Saturn Undergoing Re-Inflation around an Evolving Subgiant”, The Astronomical Journal, 163 (2): 82, arXiv:2112.00198, Bibcode:2022AJ....163...82W, doi:10.3847/1538-3881/ac3f39, S2CID 244773259
^ Lam, Kristine W. F.; và đồng nghiệp (2021), “GJ 367b: A dense, ultrashort-period sub-Earth planet transiting a nearby red dwarf star”, Science, 374 (6572): 1271–1275, arXiv:2112.01309, Bibcode:2021Sci...374.1271L, doi:10.1126/science.aay3253, PMID 34855492, S2CID 244799656
^ ^a ^b ^c ^d Jordán, A.; và đồng nghiệp (2022), “HATS-74Ab, HATS-75b, HATS-76b, and HATS-77b: Four Transiting Giant Planets Around K and M Dwarfs”, The Astronomical Journal, 163 (3): 125, arXiv:2112.01928, Bibcode:2022AJ....163..125J, doi:10.3847/1538-3881/ac4a77, S2CID 244896205
^ Cañas, Caleb I.; Mahadevan, Suvrath; Cochran, William D.; Bender, Chad F.; Feigelson, Eric D.; Harman, C. E.; Kopparapu, Ravi Kumar; Caceres, Gabriel A.; Diddams, Scott A.; Endl, Michael; Ford, Eric B.; Halverson, Samuel; Hearty, Fred; Jones, Sinclaire; Kanodia, Shubham; Lin, Andrea S. J.; Metcalf, Andrew J.; Monson, Andrew; Ninan, Joe P.; Ramsey, Lawrence W.; Robertson, Paul; Roy, Arpita; Schwab, Christian; Stefánsson, Guđmundur (2022), “A Hot Mars-sized Exoplanet Transiting an M Dwarf”, The Astronomical Journal, 163 (1): 3, arXiv:2112.03958, Bibcode:2022AJ....163....3C, doi:10.3847/1538-3881/ac3088, S2CID 244954104
^ Faherty, Jacqueline K.; Gagné, Jonathan; Popinchalk, Mark; Vos, Johanna M.; Burgasser, Adam J.; Schümann, Jörg; Schneider, Adam C.; Kirkpatrick, J. Davy; Meisner, Aaron M.; Kuchner, Marc J.; Bardalez Gagliuffi, Daniella C.; Marocco, Federico; Caselden, Dan; Gonzales, Eileen C.; Rothermich, Austin; Casewell, Sarah L.; Debes, John H.; Aganze, Christian; Ayala, Andrew; Hsu, Chih-Chun; Cooper, William J.; Smart, R. L.; Gerasimov, Roman; Theissen, Christopher A.; The Backyard Worlds; Planet 9 Collaboration (2021), “A Wide Planetary Mass Companion Discovered through the Citizen Science Project Backyard Worlds: Planet 9”, The Astrophysical Journal, 923 (1): 48, arXiv:2112.04678, Bibcode:2021ApJ...923...48F, doi:10.3847/1538-4357/ac2499, S2CID 245005964
^ Janson, Markus; Gratton, Raffaele; Rodet, Laetitia; Vigan, Arthur; Bonnefoy, Mickaël; Delorme, Philippe; Mamajek, Eric E.; Reffert, Sabine; Stock, Lukas; Marleau, Gabriel-Dominique; Langlois, Maud; Chauvin, Gaël; Desidera, Silvano; Ringqvist, Simon; Mayer, Lucio; Viswanath, Gayathri; Squicciarini, Vito; Meyer, Michael R.; Samland, Matthias; Petrus, Simon; Helled, Ravit; Kenworthy, Matthew A.; Quanz, Sascha P.; Biller, Beth; Henning, Thomas; Mesa, Dino; Engler, Natalia; Carson, Joseph C. (2021), “A wide-orbit giant planet in the high-mass b Centauri binary system”, Nature, 600 (7888): 231–234, arXiv:2112.04833, Bibcode:2021Natur.600..231J, doi:10.1038/s41586-021-04124-8, PMID 34880428, S2CID 245005994
^ ^a ^b ^c ^d ^e ^f ^g ^h ⁱ Teng, Huan-Yu; Sato, Bun'ei; Takarada, Takuya; Omiya, Masashi; Harakawa, Hiroki; Izumiura, Hideyuki; Kambe, Eiji; Takeda, Yoichi; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro (2021), “Regular radial velocity variations in nine G- and K-type giant stars: Eight planets and one planet candidate”, Publications of the Astronomical Society of Japan, 74: 92–127, arXiv:2112.07169, doi:10.1093/pasj/psab112
^ Xie, Xiao-Jia; Dong, Subo; Shvartzvald, Yossi; Gould, Andrew; Udalski, Andrzej; Beaulieu, Jean-Philippe; Beichman, Charles; Close, Laird Miller; b. Henderson, Calen; r. Males, Jared; Marquette, Jean-Baptiste; m. Morzinski, Katie; r. Gelino, Christopher (2022), “Characterizing microlensing planetary system OGLE-2014-BLG-0676Lb with adaptive optics imaging”, Research in Astronomy and Astrophysics, 21 (12): 303, arXiv:2112.08030, doi:10.1088/1674-4527/ac2a09, S2CID 244211319
^ ^a ^b Sreenivas, K. R.; Perdelwitz, V.; Tal-Or, L.; Trifonov, T.; Zucker, S.; Mazeh, T. (2022), “Analysis of the public HARPS/ESO spectroscopic archive”, Astronomy & Astrophysics, 660: A124, arXiv:2112.09029, doi:10.1051/0004-6361/202142612, S2CID 245219286
^ ^a ^b Mohammed El Mufti; và đồng nghiệp (2021), TOI 560 : Two Transiting Planets Orbiting a K Dwarf Validated with iSHELL, PFS and HIRES RVs, arXiv:2112.13448
^ Miyazaki, Shota; và đồng nghiệp (2022), “OGLE-2014-BLG-0319: A Sub-Jupiter-mass Planetary Event Encountered Degeneracy with Different Mass Ratios and Lens-source Relative Proper Motions”, The Astronomical Journal, 163 (3): 123, arXiv:2112.14997, Bibcode:2022AJ....163..123M, doi:10.3847/1538-3881/ac4960, S2CID 245634898
^ Wang(王涵悦), Hanyue; và đồng nghiệp (2022), “Systematic Korea Microlensing Telescope Network planetary anomaly search – III. One wide-orbit planet and two stellar binaries”, Monthly Notices of the Royal Astronomical Society, 510 (2): 1778–1790, arXiv:2112.02414, doi:10.1093/mnras/stab3581

[1] “HD 108236 f”, exoplanet.eu, truy cập ngày 4 tháng 1 năm 2021

[2] Bonfanti, A.; và đồng nghiệp (2021), “CHEOPS observations of the HD 108236 planetary system: A fifth planet, improved ephemerides, and planetary radii”, Astronomy & Astrophysics, 646: A157, arXiv:2101.00663, Bibcode:2021A&A...646A.157B, doi:10.1051/0004-6361/202039608, S2CID 230437723

[3] Smith, A. M. S.; và đồng nghiệp (2021), “NGTS-14Ab: A Neptune-sized transiting planet in the desert”, Astronomy & Astrophysics, 646: A183, arXiv:2101.01470, Bibcode:2021A&A...646A.183S, doi:10.1051/0004-6361/202039712, S2CID 230524042

[4] Martin, David V.; và đồng nghiệp (2021), “TOI-1259Ab – a gas giant planet with 2.7 per cent deep transits and a bound white dwarf companion”, Monthly Notices of the Royal Astronomical Society, 507 (3): 4132–4148, arXiv:2101.02707, doi:10.1093/mnras/stab2129

[5] Grieves, Nolan; và đồng nghiệp (2021), “NGTS-13b: A hot 4.8 Jupiter-mass planet transiting a subgiant star”, Astronomy & Astrophysics, 647: A180, arXiv:2101.04245, Bibcode:2021A&A...647A.180G, doi:10.1051/0004-6361/202039586, S2CID 231582818

[Rodriguez2021-6] Rodriguez, Joseph E.; và đồng nghiệp (2021), “TESS Delivers Five New Hot Giant Planets Orbiting Bright Stars from the Full-frame Images”, The Astronomical Journal, 161 (4): 194, arXiv:2101.01726, Bibcode:2021AJ....161..194R, doi:10.3847/1538-3881/abe38a, S2CID 230770138

[7] Yee, Jennifer C.; và đồng nghiệp (2021), “OGLE-2019-BLG-0960 Lb: The Smallest Microlensing Planet”, The Astronomical Journal, 162 (5): 180, arXiv:2101.04696, Bibcode:2021AJ....162..180Y, doi:10.3847/1538-3881/ac1582, S2CID 231592669

[Osborn2021-8] Osborn, H. P.; và đồng nghiệp (2021), “A hot mini-Neptune in the radius valley orbiting solar analogue HD 110113”, Monthly Notices of the Royal Astronomical Society, 502 (4): 4842–4857, arXiv:2101.04745, Bibcode:2021MNRAS.502.4842O, doi:10.1093/mnras/stab182

[Kirsch2017-9] Hirsch, Lea A.; và đồng nghiệp (2017), “ASSESSING THE EFFECT OF STELLAR COMPANIONS FROM HIGH-RESOLUTION IMAGING OF Kepler OBJECTS OF INTEREST”, The Astronomical Journal, 153 (3): 117, arXiv:1701.06577, Bibcode:2017AJ....153..117H, doi:10.3847/1538-3881/153/3/117, S2CID 39321033

[Ciardi2021-10] “AT LAST! CONFIRMATION OF KEPLER'S SECOND PLANETARY CANDIDATE” (PDF). Lưu trữ (PDF) bản gốc ngày 15 tháng 1 năm 2021. Truy cập ngày 18 tháng 1 năm 2021.

[Leleu2021-11] ^ ^a ^b ^c ^d ^e ^f Leleu, A.; và đồng nghiệp (2021), “Six transiting planets and a chain of Laplace resonances in TOI-178”, Astronomy & Astrophysics, 649: A26, arXiv:2101.09260, Bibcode:2021A&A...649A..26L, doi:10.1051/0004-6361/202039767, S2CID 231693292

[12] Palatnick, Skyler; và đồng nghiệp (2021), “Validation of HD 183579b Using Archival Radial Velocities: A Warm Neptune Orbiting a Bright Solar Analog”, The Astrophysical Journal Letters, 909 (1): L6, arXiv:2101.12137, Bibcode:2021ApJ...909L...6P, doi:10.3847/2041-8213/abe0bb, S2CID 231719821

[13] Gan, Tianjun; và đồng nghiệp (2021), “HD 183579b: A Warm Sub-Neptune Transiting a Solar Twin Detected by TESS”, Monthly Notices of the Royal Astronomical Society, 507 (2): 2220–2240, arXiv:2107.14015, doi:10.1093/mnras/stab2224

[14] Yun Hak Kim; và đồng nghiệp (2021), “KMT-2019-BLG-0371 and the Limits of Bayesian Analysis”, The Astronomical Journal, 162 (1): 17, arXiv:2101.12206, Bibcode:2021AJ....162...17K, doi:10.3847/1538-3881/abf930, S2CID 231728667

[Sozzetti2021-15] Sozzetti, A.; và đồng nghiệp (2021), “A sub-Neptune and a non-transiting Neptune-mass companion unveiled by ESPRESSO around the bright late-F dwarf HD 5278 (TOI-130)”, Astronomy & Astrophysics, 648: A75, arXiv:2101.12300, Bibcode:2021A&A...648A..75S, doi:10.1051/0004-6361/202040034, S2CID 231728514

[16] Han, Cheongho; và đồng nghiệp (2021), “KMT-2018-BLG-1025Lb: Microlensing super-Earth planet orbiting a low-mass star”, Astronomy & Astrophysics, 649: A90, arXiv:2102.01890, Bibcode:2021A&A...649A..90H, doi:10.1051/0004-6361/202039817, S2CID 231786450

[Ikwut2021-17] Ikwut-Ukwa, Mma; và đồng nghiệp (2022), “Two Massive Jupiters in Eccentric Orbits from the TESS Full-frame Images”, The Astronomical Journal, 163 (1): 9, arXiv:2102.02222, Bibcode:2022AJ....163....9I, doi:10.3847/1538-3881/ac2ee1, S2CID 231802379

[Major2011-18] Mayor, M.; Marmier, M.; Lovis, C.; Udry, S.; Ségransan, D.; Pepe, F.; Benz, W.; Bertaux, J. -L.; Bouchy, F. (2011). "The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets". arΧiv:1109.2497 [astro-ph.EP].

[Ahrer2021-19] Ahrer, E.; và đồng nghiệp (2021), “The HARPS search for southern extra-solar planets XLV. Two Neptune mass planets orbiting HD 13808: a study of stellar activity modelling's impact on planet detection”, Monthly Notices of the Royal Astronomical Society, 503 (1): 1248–1263, arXiv:2102.03387, Bibcode:2021MNRAS.503.1248A, doi:10.1093/mnras/stab373

[Newton2021-20] Newton, Elisabeth R.; và đồng nghiệp (2021), “TESS Hunt for Young and Maturing Exoplanets (THYME) IV: Three small planets orbiting a 120 Myr-old star in the Pisces–Eridanus stream”, The Astronomical Journal, 161 (2): 65, arXiv:2102.06049, Bibcode:2021AJ....161...65N, doi:10.3847/1538-3881/abccc6, S2CID 231879927

[Barragan2021-21] Barragán, Oscar; và đồng nghiệp (2021), “TESS re-observes the young multi-planet system TOI-451:refined ephemeris and activity evolution”, Research Notes of the American Astronomical Society, 5 (3): 51, arXiv:2103.09746, Bibcode:2021RNAAS...5...51B, doi:10.3847/2515-5172/abef70, S2CID 232258104

[22] Tofflemire, Benjamin M.; và đồng nghiệp (2021), “TESS Hunt for Young and Maturing Exoplanets (THYME). V. A Sub-Neptune Transiting a Young Star in a Newly Discovered 250 Myr Association”, The Astronomical Journal, 161 (4): 171, arXiv:2102.06066, Bibcode:2021AJ....161..171T, doi:10.3847/1538-3881/abdf53, S2CID 231879915

[Jung2021-23] Kil Jung, Youn; và đồng nghiệp (2021), “OGLE-2018-BLG-0567Lb and OGLE-2018-BLG-0962Lb: Two Microlensing Planets through the Planetary-caustic Channel”, The Astronomical Journal, 161 (6): 293, arXiv:2102.07338, Bibcode:2021AJ....161..293J, doi:10.3847/1538-3881/abf8bd, S2CID 231924992

[24] Toledo-Padrón, B.; và đồng nghiệp (2021), “A super-Earth on a close-in orbit around the M1V star GJ 740”, Astronomy & Astrophysics, 648: A20, arXiv:2102.09441, doi:10.1051/0004-6361/202040099, S2CID 231951695

[25] Kains, N.; và đồng nghiệp (2021), “A giant planet beyond the snow line in microlensing event OGLE-2011-BLG-0251”, Astronomy & Astrophysics, 552: A70, arXiv:1303.1184, Bibcode:2013A&A...552A..70K, doi:10.1051/0004-6361/201220626, S2CID 43146154

[26] Soto, M. G.; và đồng nghiệp (2021), “Mass and density of the transiting hot and rocky super-Earth LHS 1478 b (TOI-1640 b)”, Astronomy & Astrophysics, 649: A144, arXiv:2102.11640, Bibcode:2021A&A...649A.144S, doi:10.1051/0004-6361/202140618, S2CID 232013854

[Bluhm2021-27] Bluhm, P.; và đồng nghiệp (2021), “An ultra-short-period transiting super-Earth orbiting the M3 dwarf TOI-1685”, Astronomy & Astrophysics, 650: A78, arXiv:2103.01016, Bibcode:2021A&A...650A..78B, doi:10.1051/0004-6361/202140688, S2CID 232092636

[Hirano2021-28] Hirano, Teruyuki; và đồng nghiệp (2021), “Two Bright M Dwarfs Hosting Ultra-Short-Period Super-Earths with Earth-like Compositions”, The Astronomical Journal, 162 (4): 161, arXiv:2103.12760, Bibcode:2021AJ....162..161H, doi:10.3847/1538-3881/ac0fdc, S2CID 232335413

[29] Zang, Weicheng; và đồng nghiệp (2021), “An Earth-mass planet in a time of COVID-19: KMT-2020-BLG-0414Lb”, Research in Astronomy and Astrophysics, 21 (9): 239, arXiv:2103.01896, Bibcode:2021RAA....21..239Z, doi:10.1088/1674-4527/21/9/239, S2CID 232092272

[Hobson2021-30] Hobson, Melissa J.; và đồng nghiệp (2021), “A Transiting Warm Giant Planet around the Young Active Star TOI-201”, The Astronomical Journal, 161 (5): 235, arXiv:2103.02685, Bibcode:2021AJ....161..235H, doi:10.3847/1538-3881/abeaa1, S2CID 232110390

[31] Trifonov, T.; và đồng nghiệp (2021), “A nearby transiting rocky exoplanet that is suitable for atmospheric investigation”, Science, 371 (6533): 1038–1041, arXiv:2103.04950, Bibcode:2021Sci...371.1038T, doi:10.1126/science.abd7645, PMID 33674491, S2CID 232124642

[Tilbrook2021-32] Tilbrook, Rosanna H.; và đồng nghiệp (2021), “NGTS 15b, 16b, 17b, and 18b: Four hot Jupiters from the Next-Generation Transit Survey”, Monthly Notices of the Royal Astronomical Society, 504 (4): 6018–6032, arXiv:2103.10302, doi:10.1093/mnras/stab815

[33] Zang, Weicheng; và đồng nghiệp (2021), “Systematic KMTNet Planetary Anomaly Search. I. OGLE-2019-BLG-1053Lb, a Buried Terrestrial Planet”, The Astronomical Journal, 162 (4): 163, arXiv:2103.11880, Bibcode:2021AJ....162..163Z, doi:10.3847/1538-3881/ac12d4, S2CID 232307459

[34] Cloutier, R.; và đồng nghiệp (2021), “TOI-1634 b: An Ultra-short-period Keystone Planet Sitting inside the M-dwarf Radius Valley”, The Astronomical Journal, 162 (2): 79, arXiv:2103.12790, Bibcode:2021AJ....162...79C, doi:10.3847/1538-3881/ac0157, S2CID 232335385

[35] Han, Cheongho; và đồng nghiệp (2021), “KMT-2019-BLG-1715: Planetary Microlensing Event with Three Lens Masses and Two Source Stars”, The Astronomical Journal, 161 (6): 270, arXiv:2104.00293, Bibcode:2021AJ....161..270H, doi:10.3847/1538-3881/abf4d0, S2CID 232478488

[36] Kondo, Iona; và đồng nghiệp (2021), “OGLE-2018-BLG-1185b: A Low-mass Microlensing Planet Orbiting a Low-mass Dwarf”, The Astronomical Journal, 162 (2): 77, arXiv:2104.02157, Bibcode:2021AJ....162...77K, doi:10.3847/1538-3881/ac00ba, S2CID 233033627

[Georgieva2021-37] Georgieva, I. Y.; và đồng nghiệp (2021), “Hot planets around cool stars – two short-period mini-Neptunes transiting the late K-dwarf TOI-1260”, Monthly Notices of the Royal Astronomical Society, 505 (4): 4684–4701, arXiv:2104.05653, doi:10.1093/mnras/stab1464

[Han2021-38] Han, Cheongho; và đồng nghiệp (2021), “Three microlensing planets with no caustic-crossing features”, Astronomy & Astrophysics, 650: A89, arXiv:2104.06544, Bibcode:2021A&A...650A..89H, doi:10.1051/0004-6361/202140758, S2CID 233231384

[39] Bohn, Alexander J.; và đồng nghiệp (2021), “Discovery of a directly imaged planet to the young solar analog YSES 2”, Astronomy & Astrophysics, 648: A73, arXiv:2104.08285, Bibcode:2021A&A...648A..73B, doi:10.1051/0004-6361/202140508, S2CID 233296087

[40] Ryu, Yoon-Hyun; và đồng nghiệp (2021), “Shortest Microlensing Event with a Bound Planet: KMT-2016-BLG-2605”, The Astronomical Journal, 162 (3): 96, arXiv:2104.07906, Bibcode:2021AJ....162...96R, doi:10.3847/1538-3881/ac062a, S2CID 233289612

[41] Brett Christopher Addison; và đồng nghiệp (2021), “TOI-1431b/MASCARA-5b: An Ultra-hot Jupiter Orbiting One of the Hottest & Brightest Known Exoplanet Host Stars”, Posters from the Tess Science Conference Ii (Tsc2: 64, arXiv:2104.12078, Bibcode:2021tsc2.confE..64A, doi:10.5281/zenodo.5126266, S2CID 240578462

[42] Stangret, M.; và đồng nghiệp (2021), “The obliquity and atmosphere of the ultra-hot Jupiter TOI-1431b (MASCARA-5b): A misaligned orbit and no signs of atomic or molecular absorptions”, Astronomy & Astrophysics, 654: A73, arXiv:2104.12414, Bibcode:2021A&A...654A..73S, doi:10.1051/0004-6361/202040100, S2CID 233393996

[43] Cointepas, M.; và đồng nghiệp (2021), “TOI-269 b: An eccentric sub-Neptune transiting a M2 dwarf revisited with ExTrA”, Astronomy & Astrophysics, 650: A145, arXiv:2104.14782, Bibcode:2021A&A...650A.145C, doi:10.1051/0004-6361/202140328, S2CID 233476660

[44] Hoyer, S.; và đồng nghiệp (2021), “TOI-220 b: A warm sub-Neptune discovered by TESS”, Monthly Notices of the Royal Astronomical Society, 505 (3): 3361–3379, arXiv:2105.01944, doi:10.1093/mnras/stab1427

[Otegi2021-45] Otegi, J. F.; và đồng nghiệp (2021), “TESS and HARPS reveal two sub-Neptunes around TOI 1062”, Astronomy & Astrophysics, 653: A105, arXiv:2105.01945, Bibcode:2021A&A...653A.105O, doi:10.1051/0004-6361/202040247, S2CID 233739805

[46] Zhang, Jingwen; và đồng nghiệp (2021), “Long-period Jovian Tilts the Orbits of Two sub-Neptunes Relative to Stellar Spin Axis in Kepler-129”, The Astronomical Journal, 162 (3): 89, arXiv:2105.03446, Bibcode:2021AJ....162...89Z, doi:10.3847/1538-3881/ac0634, S2CID 234338914

[47] Maldonado, J.; và đồng nghiệp (2021), “HADES RV programme with HARPS-N at TNG”, Astronomy & Astrophysics, 651: A93, arXiv:2105.06155, doi:10.1051/0004-6361/202141141, S2CID 234482717

[48] Burt, Jennifer A.; và đồng nghiệp (2021), “TOI-1231 b: A Temperate, Neptune-sized Planet Transiting the Nearby M3 Dwarf NLTT 24399”, The Astronomical Journal, 162 (3): 87, arXiv:2105.08077, Bibcode:2021AJ....162...87B, doi:10.3847/1538-3881/ac0432, S2CID 234763319

[49] Kostov, Veselin B.; và đồng nghiệp (2021), “TIC 172900988: A Transiting Circumbinary Planet Detected in One Sector of TESS Data”, The Astronomical Journal, 162 (6): 234, arXiv:2105.08614, Bibcode:2021AJ....162..234K, doi:10.3847/1538-3881/ac223a, S2CID 234762777

[50] Dai, Fei; Howard, Andrew W.; Batalha, Natalie M.; Beard, Corey; Behmard, Aida; Blunt, Sarah; Brinkman, Casey L.; Chontos, Ashley; Crossfield, Ian J. M. (2021). "TKS X: Confirmation of TOI-1444b and a Comparative Analysis of the Ultra-short-period Planets with Hot Neptunes". arΧiv:2105.08844 [astro-ph.EP].

[Dalal2021-51] ^ ^a ^b ^c ^d ^e ^f Dalal, S.; và đồng nghiệp (2021), “The SOPHIE search for northern extrasolar planets”, Astronomy & Astrophysics, 651: A11, arXiv:2105.09741, doi:10.1051/0004-6361/202140712, S2CID 234790136

[Rosenthal2021-52] ^ ^a ^b ^c ^d ^e ^f ^g ^h ⁱ ^j ^k ^l ^m Rosenthal, Lee J.; và đồng nghiệp (2021), “The California Legacy Survey. I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades”, The Astrophysical Journal Supplement Series, 255 (1): 8, arXiv:2105.11583, Bibcode:2021ApJS..255....8R, doi:10.3847/1538-4365/abe23c, S2CID 235186973

[Amado2021-53] Amado, Pedro J.; Bauer, Florian F.; Rodríguez López, Cristina; Rodríguez, Eloy; Cardona Guillén, C.; Perger, M.; Caballero, José A.; López-González, Maria J.; Muñoz Rodríguez, I.; Pozuelos, F. J.; Sánchez-Rivero, A.; Schlecker, M.; Quirrenbach, Andreas; Ribas, Ignasi; Reiners, Ansgar; Almenara, J.; Astudillo-Defru, N.; Azzaro, M.; Béjar, Victor J. S.; Bohemann, R.; Bonfils, X.; Bouchy, F.; Cifuentes, C.; Cortés-Contreras, M.; Delfosse, Xavier; Dreizler, Stefan; Forveille, Thierry; Hatzes, Artie P.; Henning, Thomas K.; Jeffers, Sandra V.; Kaminski, Adrian; Kürster, Martin; Lafarga, M.; Lodieu, Nicolas; Lovis, C.; Mayor, M.; Montes, David; Morales, Juan Carlos; Morales, Nicolás; Murgas, F.; Ortiz, José L.; Pepe, F.; Perdelwitz, V.; Pollaco, D.; Santos, N. C.; Schöfer, P.; Schweitzer, A.; Ségransan, N. C.; Shan, Y.; Stock, S.; Tal-Or, Lev; Udry, S.; Zapatero-Osorio, María Rosa; Zechmeister, Mathias (28 tháng 5 năm 2021). “The CARMENES search for exoplanets around M dwarfs”. Astronomy & Astrophysics. 650: A188. arXiv:2105.13785. doi:10.1051/0004-6361/202140633. S2CID 235248027.

[54] Murgas, F.; và đồng nghiệp (2021), “TOI-674b: An oasis in the desert of exo-Neptunes transiting a nearby M dwarf”, Astronomy & Astrophysics, 653: A60, arXiv:2106.01246, Bibcode:2021A&A...653A..60M, doi:10.1051/0004-6361/202140718, S2CID 235294286

[55] Brande, Jonathan; Crossfield, Ian J. M.; Kreidberg, Laura; Oklopčić, Antonija; Polanski, Alex S.; Barman, Travis; Benneke, Björn; Christiansen, Jessie L.; Dragomir, Diana; Foreman-Mackey, Daniel; Fortney, Jonathan J.; Greene, Thomas P.; Howard, Andrew W.; Knutson, Heather A.; Lothringer, Joshua D.; Mikal-Evans, Thomas; Morley, Caroline V. (2022), “A Mirage or an Oasis? Water Vapor in the Atmosphere of the Warm Neptune TOI-674 B”, The Astronomical Journal, 164 (5): 197, arXiv:2201.04197, doi:10.3847/1538-3881/ac8b7e, S2CID 245877576

[Eisner2021-56] Eisner, N. L.; và đồng nghiệp (2021), “Planet Hunters TESS III: Two transiting planets around the bright G dwarf HD 152843”, Monthly Notices of the Royal Astronomical Society, 505 (2): 1827–1840, arXiv:2106.04603, doi:10.1093/mnras/stab1253

[Hwang2021-57] Hwang, Kyu-Ha; và đồng nghiệp (2021), “Systematic KMTNet Planetary Anomaly Search, Paper II: Five New q<2×10−4 Mass-ratio Planets”, arXiv:2106.06686, doi:10.3847/1538-3881/ac38ad, S2CID 245740102 Chú thích journal cần |journal= (trợ giúp)

[58] Khandelwal, Akanksha; và đồng nghiệp (2021), “Discovery of an inflated hot Jupiter around a slightly evolved star TOI-1789”, Monthly Notices of the Royal Astronomical Society, arXiv:2106.08660, doi:10.1093/mnras/stab2970

[Wirth2021-59] Wirth, Christopher P.; và đồng nghiệp (2021), “TOI-942b: A Prograde Neptune in a ∼ 60 Myr Old Multi-transiting System”, The Astrophysical Journal Letters, 917 (2): L34, arXiv:2106.14968, Bibcode:2021ApJ...917L..34W, doi:10.3847/2041-8213/ac13a9, S2CID 235670113

[60] Han, Cheongho; và đồng nghiệp (2021), “KMT-2018-BLG-1743: Planetary microlensing event occurring on two source stars”, Astronomy & Astrophysics, 652: A145, arXiv:2107.00155, Bibcode:2021A&A...652A.145H, doi:10.1051/0004-6361/202140923, S2CID 235694685

[Fukui2021-61] Fukui, A.; và đồng nghiệp (2021), “TOI-1749: An M dwarf with a Trio of Planets including a Near-resonant Pair”, The Astronomical Journal, 162 (4): 167, arXiv:2107.05430, Bibcode:2021AJ....162..167F, doi:10.3847/1538-3881/ac13a5, S2CID 235795469

[Demangeon2021-62] ^ ^a ^b ^c ^d ^e ^f Demangeon, O. D. S.; và đồng nghiệp (2021), “The SOPHIE search for northern extrasolar planets”, Astronomy & Astrophysics, 653: A78, arXiv:2107.05089, doi:10.1051/0004-6361/202141079, S2CID 235795175

[63] Dalba, Paul A.; và đồng nghiệp (2021), “Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. II. Discovery of a Failed Hot Jupiter on a 2.7 Yr, Highly Eccentric Orbit”, The Astronomical Journal, 162 (4): 154, arXiv:2107.06901, Bibcode:2021AJ....162..154D, doi:10.3847/1538-3881/ac134b, S2CID 235898945

[64] Kanodia, Shubham; và đồng nghiệp (2021), “TOI-532b: The Habitable-zone Planet Finder confirms a Large Super Neptune in the Neptune Desert orbiting a metal-rich M-dwarf host”, The Astronomical Journal, 162 (4): 135, arXiv:2107.13670, Bibcode:2021AJ....162..135K, doi:10.3847/1538-3881/ac1940, S2CID 236493328

[65] Wells, R. D.; và đồng nghiệp (2021), “A large sub-Neptune transiting the thick-disk M4 V TOI-2406”, Astronomy & Astrophysics, 653: A97, arXiv:2107.14125, Bibcode:2021A&A...653A..97W, doi:10.1051/0004-6361/202141277, S2CID 236493492

[Lillo-Box2021-66] Lillo-Box, J.; và đồng nghiệp (2021), “Follow-up of non-transiting planets detected by Kepler”, Astronomy & Astrophysics, 654: A9, arXiv:2107.14621, doi:10.1051/0004-6361/202140746, S2CID 236635201

[Winters2021-67] Winters, Jennifer G.; Cloutier, Ryan; Medina, Amber A.; Irwin, Jonathan M.; Charbonneau, David; Astudillo-Defru, Nicola; Bonfils, Xavier; Howard, Andrew W.; Isaacson, Howard; Bean, J. L.; Seifahrt, A.; Teske, J. K.; Eastman, Jason D.; Twicken, Joseph D.; Collins, K. A.; Jensen, E. L. N.; Quinn, S. N.; Payne, M. J.; Kristiansen, M. H.; Spencer, A.; Vanderburg, Andrew; Zechmeister, Mathias; Weiss, L. M.; Wang, S. X.; Wang, G.; Udry, Stéphane; Terentev, I. A.; Sturmer, J.; Stefansson, G.; Shectman, Stephen A.; Sefako, R.; Schwengeler, H. M.; Schwarz, R. P.; Scarsdale, N.; Rubenzahl, R. A.; Roy, A.; Rosenthal, L. J.; Robertson, P.; Petigura, Erik A.; Pepe, Francesco; Omohundro, M.; Murphy, J. M. A.; Murgas, Felipe; Movcnik, T.; Montet, B. T.; Mennickent, R.; Mayo, A. W.; Massey, B.; Lubin, J.; Lovis, Christophe; Lewin, P.; Kasper, D.; Kane, S. R.; Jenkins, J. M.; Huber, D.; Horne, K.; Hill, M. L.; Gorrini, P.; Giacalone, S.; Fulton, Benjamin J.; Forveille, Thierry; Figueira, Pedro; Fetherolf, T.; Dressing, Courtney D.; Díaz, Rodrigo F.; Delfosse, Xavier; Dalba, P. A.; Dai, F.; Cortes, C. C.; Crossfield, Ian J. M.; Crane, Jeffrey D.; Conti, D. M.; Collins, K. I.; Chontos, A.; Butler, R. Paul; Brown, P.; Brady, M.; Bouchy, François; Behmard, A.; Beard, C.; Batalha, Natalie M.; Almenara, José M. (2022). “A Second Planet Transiting LTT 1445A and a Determination of the Masses of Both Worlds”. The Astronomical Journal. 163 (4): 168. arXiv:2107.14737. Bibcode:2022AJ....163..168W. doi:10.3847/1538-3881/ac50a9. S2CID 236635391.

[Demangeon2021-7-68] “A warm terrestrial planet with half the mass of Venus transiting a nearby star” (PDF). Lưu trữ (PDF) bản gốc ngày 13 tháng 11 năm 2021. Truy cập ngày 8 tháng 8 năm 2021.

[Lubin2021-69] Lubin, Jack; và đồng nghiệp (2022), “TESS-Keck Survey. IX. Masses of Three Sub-Neptunes Orbiting HD 191939 and the Discovery of a Warm Jovian plus a Distant Substellar Companion”, The Astronomical Journal, 163 (2): 101, arXiv:2108.02208, Bibcode:2022AJ....163..101L, doi:10.3847/1538-3881/ac3d38, S2CID 236924440

[70] Shin, In-Gu; và đồng nghiệp (2021), “Using Source Proper Motion to Validate Terrestrial Parallax: OGLE-2019-BLG-1058”, The Astronomical Journal, 162 (6): 267, arXiv:2108.02499, Bibcode:2021AJ....162..267S, doi:10.3847/1538-3881/ac2ba5, S2CID 236924486

[71] Saunders, Nicholas; và đồng nghiệp (2022), “TESS Giants Transiting Giants. I.: A Noninflated Hot Jupiter Orbiting a Massive Subgiant”, The Astronomical Journal, 163 (2): 53, arXiv:2108.02294, Bibcode:2022AJ....163...53S, doi:10.3847/1538-3881/ac38a1, S2CID 236924647

[Osborn2021-8-72] Osborn, Ares; và đồng nghiệp (2021), “TOI-431/HIP 26013: a super-Earth and a sub-Neptune transiting a bright, early K dwarf, with a third RV planet”, Monthly Notices of the Royal Astronomical Society, 507 (2): 2782–2803, arXiv:2108.02310, doi:10.1093/mnras/stab2313

[Trifonov2021-73] Trifonov, Trifon; và đồng nghiệp (2021), “A Pair of Warm Giant Planets near the 2:1 Mean Motion Resonance around the K-dwarf Star TOI-2202”, The Astronomical Journal, 162 (6): 283, arXiv:2108.05323, Bibcode:2021AJ....162..283T, doi:10.3847/1538-3881/ac1bbe, S2CID 236976243

[Leon2021-74] ^ ^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 De Leon, J. P.; và đồng nghiệp (2021), “37 New Validated Planets in Overlapping K2 Campaigns”, Monthly Notices of the Royal Astronomical Society, 508: 195–218, arXiv:2108.05621, doi:10.1093/mnras/stab2305

[Kovaks2020-75] Kovacs, Geza (2020), “More planetary candidates from K2 Campaign 5 using TRAN_K2”, Astronomy & Astrophysics, 643: A169, arXiv:2008.10075, Bibcode:2020A&A...643A.169K, doi:10.1051/0004-6361/202038726, S2CID 221266076

[76] Lillo-Box, J.; và đồng nghiệp (2021), “HD 22496 b: The first ESPRESSO stand-alone planet discovery”, Astronomy & Astrophysics, 654: A60, arXiv:2109.00226, Bibcode:2021A&A...654A..60L, doi:10.1051/0004-6361/202141714, S2CID 237371680

[Castro2021-77] Castro-González, A.; và đồng nghiệp (2022), “The K2-OjOS Project: New and revisited planets and candidates in K2 campaigns 5, 16, & 18”, Monthly Notices of the Royal Astronomical Society, 509: 1075–1095, arXiv:2109.03346, doi:10.1093/mnras/stab2669

[78] Dong, Jiayin; và đồng nghiệp (2021), “TOI-3362b: A Proto Hot Jupiter Undergoing High-eccentricity Tidal Migration”, The Astrophysical Journal Letters, 920 (1): L16, arXiv:2109.03771, Bibcode:2021ApJ...920L..16D, doi:10.3847/2041-8213/ac2600, S2CID 237442300

[Han2021-09-79] Han, Cheongho; và đồng nghiệp (2021), “Three faint-source microlensing planets detected via the resonant-caustic channel”, Astronomy & Astrophysics, 655: A21, arXiv:2109.07068, Bibcode:2021A&A...655A..21H, doi:10.1051/0004-6361/202141517, S2CID 237513708

[Moutou2021-80] Moutou, C.; và đồng nghiệp (2021), “TOI-1296b and TOI-1298b observed with TESS and SOPHIE: Two hot Saturn-mass exoplanets with different densities around metal-rich stars”, Astronomy & Astrophysics, 653: A147, arXiv:2109.09252, Bibcode:2021A&A...653A.147M, doi:10.1051/0004-6361/202141151, S2CID 237571683

[81] Kossakowski, D.; và đồng nghiệp (2021), “TOI-1201 b: A mini-Neptune transiting a bright and moderately young M dwarf”, Astronomy & Astrophysics, 656: A124, arXiv:2109.09346, Bibcode:2021A&A...656A.124K, doi:10.1051/0004-6361/202141587, S2CID 237571914

[82] Rattanamala, R.; Awiphan, S.; Komonjinda, S.; Phriksee, A.; Sappankum, P.; A-thano, N.; Chitchak, S.; Rittipruk, P.; Sawangwit, U.; Poshyachinda, S.; Reichart, D. E.; Haislip, J. B. (2021), Two circumbinary planets in RR Cae eclipsing binary system, arXiv:2109.09397

[83] Montalto, M.; Malavolta, L.; Gregorio, J.; Mantovan, G.; Desidera, S.; Piotto, G.; Nascimbeni, V.; Granata, V.; Manthopoulou, E. E.; Claudi, R. (2022), “TIC 257060897b: An inflated, low-density, hot-Jupiter transiting a rapidly evolving subgiant star”, Monthly Notices of the Royal Astronomical Society, 509 (2): 2908–2919, arXiv:2110.00489, doi:10.1093/mnras/stab2923

[84] Gan, Tianjun; và đồng nghiệp (2021), “TOI-530b: A giant planet transiting an M dwarf detected by TESS”, Monthly Notices of the Royal Astronomical Society, 511: 83–99, arXiv:2110.04220, doi:10.1093/mnras/stab3708

[MacDougall2021-85] MacDougall, Mason G.; và đồng nghiệp (2021), “The TESS–Keck Survey. VI. Two Eccentric Sub-Neptunes Orbiting HIP-97166”, The Astronomical Journal, 162 (6): 265, arXiv:2110.05628, Bibcode:2021AJ....162..265M, doi:10.3847/1538-3881/ac295e, S2CID 238634523

[Scarsdale2021-86] Scarsdale, Nicholas; và đồng nghiệp (2021), “TESS-Keck Survey. V. Twin Sub-Neptunes Transiting the Nearby G Star HD 63935”, The Astronomical Journal, 162 (5): 215, arXiv:2110.06885, Bibcode:2021AJ....162..215S, doi:10.3847/1538-3881/ac18cb, S2CID 238743956

[87] Heidari, N.; và đồng nghiệp (2022), “HD 207897 b: A dense sub-Neptune transiting a nearby and bright K-type star”, Astronomy & Astrophysics, 658: A176, arXiv:2110.08597, Bibcode:2022A&A...658A.176H, doi:10.1051/0004-6361/202141429, S2CID 239016573

[88] Gaidos, E.; Hirano, T.; Kraus, A. L.; Kuzuhara, M.; Zhang, Z.; Lee, R. A.; Salama, M.; Berger, T. A.; Grunblatt, S. K.; Ansdell, M.; Liu, M. C.; Harakawa, H.; Hodapp, K. W.; Jacobson, S.; Konishi, M.; Kotani, T.; Kudo, T.; Kurokawa, T.; Nishikawa, J.; Omiya, M.; Serizawa, T.; Tamura, M.; Ueda, A.; Vievard, S. (2021), “Zodiacal Exoplanets in Time (ZEIT) XII: A Directly-Imaged Planetary-Mass Companion to a Young Taurus M Dwarf Star”, Monthly Notices of the Royal Astronomical Society, 512: 583–601, arXiv:2110.08655, doi:10.1093/mnras/stab3069

[89] “Astronomers Discover Infant Planet – One of the Youngest Exoplanets Ever Observed”. 23 tháng 10 năm 2021. Lưu trữ bản gốc ngày 25 tháng 10 năm 2021. Truy cập ngày 25 tháng 10 năm 2021.

[90] Mann, Andrew W.; và đồng nghiệp (2022), “TESS Hunt for Young and Maturing Exoplanets (THYME). VI. An 11 Myr Giant Planet Transiting a Very-low-mass Star in Lower Centaurus Crux”, The Astronomical Journal, 163 (4): 156, arXiv:2110.09531, Bibcode:2022AJ....163..156M, doi:10.3847/1538-3881/ac511d, S2CID 239024522

[91] Fukui, Akihiko; và đồng nghiệp (2021), “TOI-2285b: A 1.7 Earth-radius planet near the habitable zone around a nearby M dwarf”, Publications of the Astronomical Society of Japan, 74: L1–L8, arXiv:2110.10215, doi:10.1093/pasj/psab106

[Sirverstein2021-92] Silverstein, Michele L.; và đồng nghiệp (2022), “The LHS 1678 System: Two Earth-sized Transiting Planets and an Astrometric Companion Orbiting an M Dwarf Near the Convective Boundary at 20 pc”, The Astronomical Journal, 163 (4): 151, arXiv:2110.12079, Bibcode:2022AJ....163..151S, doi:10.3847/1538-3881/ac32e3, S2CID 239768873

[Barragan2021-10-93] Barragán, O.; và đồng nghiệp (2022), “The young HD 73583 (TOI-560) planetary system: Two 10-M⊕ mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarf”, Monthly Notices of the Royal Astronomical Society, 514 (2): 1606–1627, arXiv:2110.13069, doi:10.1093/mnras/stac638

[94] Zhang, Michael; Knutson, Heather A.; Wang, Lile; Dai, Fei; Barragán, Oscar (2022), “Escaping Helium from TOI 560.01, a Young Mini-Neptune”, The Astronomical Journal, 163 (2): 67, arXiv:2110.13150, Bibcode:2022AJ....163...67Z, doi:10.3847/1538-3881/ac3fa7, S2CID 239885237

[Hedges2021-95] Hedges, Christina; và đồng nghiệp (2021), “TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow up”, The Astronomical Journal, 162 (2): 54, arXiv:2111.01311, Bibcode:2021AJ....162...54H, doi:10.3847/1538-3881/ac06cd, S2CID 235805026

[96] Peng, Peifeng; Xiong, Hongyi; Li, He; Li, Felix; Wang, Tianqi (2022), New Parameter Measurements for the Ultra-Short-Period Planet TOI-1807b, arXiv:2210.04162

[97] Osborn, H.; và đồng nghiệp (2022), “Uncovering the true periods of the young sub-Neptunes orbiting TOI-2076”, Astronomy & Astrophysics, 664: A156, arXiv:2203.03194, doi:10.1051/0004-6361/202243065, S2CID 247292643

[98] Schanche, N.; và đồng nghiệp (2022), “TOI-2257 b: A highly eccentric long-period sub-Neptune transiting a nearby M dwarf”, Astronomy & Astrophysics, 657: A45, arXiv:2111.01749, Bibcode:2022A&A...657A..45S, doi:10.1051/0004-6361/202142280, S2CID 240419956

[Vach2021-99] Vach, Sydney; và đồng nghiệp (2022), “TOI-712: A System of Adolescent Mini-Neptunes Extending to the Habitable Zone”, The Astronomical Journal, 164 (2): 71, arXiv:2111.02416, doi:10.3847/1538-3881/ac7954, S2CID 242757638

[Han2021-11-100] Han, Cheongho; và đồng nghiệp (2022), “OGLE-2019-BLG-0468Lb,c: Two microlensing giant planets around a G-type star”, Astronomy & Astrophysics, 658: A93, arXiv:2111.03755, Bibcode:2022A&A...658A..93H, doi:10.1051/0004-6361/202142327, S2CID 243847948

[101] Han, Cheongho; và đồng nghiệp (2022), “KMT-2021-BLG-0912Lb: A microlensing super Earth around a K-type star”, Astronomy & Astrophysics, 658: A94, arXiv:2111.04861, Bibcode:2022A&A...658A..94H, doi:10.1051/0004-6361/202142495, S2CID 243860989

[Silva2021-102] Azevedo Silva, T.; và đồng nghiệp (2022), “The HD 137496 system: A dense, hot super-Mercury and a cold Jupiter”, Astronomy & Astrophysics, 657: A68, arXiv:2111.08764, Bibcode:2022A&A...657A..68A, doi:10.1051/0004-6361/202141520, S2CID 243809625

[Jeong2021-103] Jeong, G.; Lee, B. C.; Park, M. G.; Bang, T. Y.; Han, I. (2022), “Search for exoplanets around northern circumpolar stars”, Astronomy & Astrophysics, 662: A12, arXiv:2111.08899, doi:10.1051/0004-6361/202142379, S2CID 244270271

[104] Han, Cheongho; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Youn Kil Jung; Kim, Doeon; Lee, Chung-Uk; Mao, Shude; Ryu, Yoon-Hyun; Shin, In-Gu; Shvartzvald, Yossi; Yee, Jennifer C.; Zang, Weicheng; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Hyoun-Woo; Kim, Seung-Lee; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W.; Kim, Chun-Hwey (2022), “KMT-2018-BLG-1988Lb: Microlensing super-Earth orbiting a low-mass disk dwarf”, Astronomy & Astrophysics, 658: A62, arXiv:2111.08955, Bibcode:2022A&A...658A..62H, doi:10.1051/0004-6361/202142077, S2CID 244270928

[105] Sun, Leilei; Ioannidis, Panagiotis; Gu, Shenghong; Schmitt, Jürgen H. M. M.; Wang, Xiaobin; Kouwenhoven, M. B. N.; Perdelwitz, Volker; Francesco Flammini Dotti; Czesla, Stefan (2022), “A highly mutually inclined compact warm-Jupiter system KOI-984?”, Monthly Notices of the Royal Astronomical Society, 512 (3): 4604–4617, arXiv:2111.09668, doi:10.1093/mnras/stab3367

[106] Wong, Ian; và đồng nghiệp (2021), “TOI-2109: An Ultrahot Gas Giant on a 16 hr Orbit”, The Astronomical Journal, 162 (6): 256, arXiv:2111.12074, Bibcode:2021AJ....162..256W, doi:10.3847/1538-3881/ac26bd, S2CID 244488632

[Alvarez2021-107] González-Álvarez, E.; và đồng nghiệp (2022), “A multi-planetary system orbiting the early-M dwarf TOI-1238”, Astronomy & Astrophysics, 658: A138, arXiv:2111.14602, Bibcode:2022A&A...658A.138G, doi:10.1051/0004-6361/202142128, S2CID 244715047

[108] Smith, A M S.; và đồng nghiệp (2021), “K2-99 revisited: A non-inflated warm Jupiter, and a temperate giant planet on a 522-d orbit around a subgiant”, Monthly Notices of the Royal Astronomical Society, 510 (4): 5035–5049, arXiv:2111.14660, doi:10.1093/mnras/stab3497

[Paredes2021-109] Paredes, Leonardo A.; Henry, Todd J.; Quinn, Samuel N.; Gies, Douglas R.; Hinojosa-Goñi, Rodrigo; James, Hodari-Sadiki; Jao, Wei-Chun; White, Russel J. (2021), “The Solar Neighborhood XLVIII: Nine Giant Planets Orbiting Nearby K Dwarfs, and the CHIRON Spectrograph's Radial Velocity Performance”, The Astronomical Journal, 162 (5): 176, arXiv:2111.15028, Bibcode:2021AJ....162..176P, doi:10.3847/1538-3881/ac082a, S2CID 237285778

[110] Wittenmyer, Robert A.; và đồng nghiệp (2021), “TOI-1842b: A Transiting Warm Saturn Undergoing Re-Inflation around an Evolving Subgiant”, The Astronomical Journal, 163 (2): 82, arXiv:2112.00198, Bibcode:2022AJ....163...82W, doi:10.3847/1538-3881/ac3f39, S2CID 244773259

[111] Lam, Kristine W. F.; và đồng nghiệp (2021), “GJ 367b: A dense, ultrashort-period sub-Earth planet transiting a nearby red dwarf star”, Science, 374 (6572): 1271–1275, arXiv:2112.01309, Bibcode:2021Sci...374.1271L, doi:10.1126/science.aay3253, PMID 34855492, S2CID 244799656

[Jordan2021-112] Jordán, A.; và đồng nghiệp (2022), “HATS-74Ab, HATS-75b, HATS-76b, and HATS-77b: Four Transiting Giant Planets Around K and M Dwarfs”, The Astronomical Journal, 163 (3): 125, arXiv:2112.01928, Bibcode:2022AJ....163..125J, doi:10.3847/1538-3881/ac4a77, S2CID 244896205

[113] Cañas, Caleb I.; Mahadevan, Suvrath; Cochran, William D.; Bender, Chad F.; Feigelson, Eric D.; Harman, C. E.; Kopparapu, Ravi Kumar; Caceres, Gabriel A.; Diddams, Scott A.; Endl, Michael; Ford, Eric B.; Halverson, Samuel; Hearty, Fred; Jones, Sinclaire; Kanodia, Shubham; Lin, Andrea S. J.; Metcalf, Andrew J.; Monson, Andrew; Ninan, Joe P.; Ramsey, Lawrence W.; Robertson, Paul; Roy, Arpita; Schwab, Christian; Stefánsson, Guđmundur (2022), “A Hot Mars-sized Exoplanet Transiting an M Dwarf”, The Astronomical Journal, 163 (1): 3, arXiv:2112.03958, Bibcode:2022AJ....163....3C, doi:10.3847/1538-3881/ac3088, S2CID 244954104

[114] Faherty, Jacqueline K.; Gagné, Jonathan; Popinchalk, Mark; Vos, Johanna M.; Burgasser, Adam J.; Schümann, Jörg; Schneider, Adam C.; Kirkpatrick, J. Davy; Meisner, Aaron M.; Kuchner, Marc J.; Bardalez Gagliuffi, Daniella C.; Marocco, Federico; Caselden, Dan; Gonzales, Eileen C.; Rothermich, Austin; Casewell, Sarah L.; Debes, John H.; Aganze, Christian; Ayala, Andrew; Hsu, Chih-Chun; Cooper, William J.; Smart, R. L.; Gerasimov, Roman; Theissen, Christopher A.; The Backyard Worlds; Planet 9 Collaboration (2021), “A Wide Planetary Mass Companion Discovered through the Citizen Science Project Backyard Worlds: Planet 9”, The Astrophysical Journal, 923 (1): 48, arXiv:2112.04678, Bibcode:2021ApJ...923...48F, doi:10.3847/1538-4357/ac2499, S2CID 245005964

[115] Janson, Markus; Gratton, Raffaele; Rodet, Laetitia; Vigan, Arthur; Bonnefoy, Mickaël; Delorme, Philippe; Mamajek, Eric E.; Reffert, Sabine; Stock, Lukas; Marleau, Gabriel-Dominique; Langlois, Maud; Chauvin, Gaël; Desidera, Silvano; Ringqvist, Simon; Mayer, Lucio; Viswanath, Gayathri; Squicciarini, Vito; Meyer, Michael R.; Samland, Matthias; Petrus, Simon; Helled, Ravit; Kenworthy, Matthew A.; Quanz, Sascha P.; Biller, Beth; Henning, Thomas; Mesa, Dino; Engler, Natalia; Carson, Joseph C. (2021), “A wide-orbit giant planet in the high-mass b Centauri binary system”, Nature, 600 (7888): 231–234, arXiv:2112.04833, Bibcode:2021Natur.600..231J, doi:10.1038/s41586-021-04124-8, PMID 34880428, S2CID 245005994

[Teng2021-116] ^ ^a ^b ^c ^d ^e ^f ^g ^h ⁱ Teng, Huan-Yu; Sato, Bun'ei; Takarada, Takuya; Omiya, Masashi; Harakawa, Hiroki; Izumiura, Hideyuki; Kambe, Eiji; Takeda, Yoichi; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro (2021), “Regular radial velocity variations in nine G- and K-type giant stars: Eight planets and one planet candidate”, Publications of the Astronomical Society of Japan, 74: 92–127, arXiv:2112.07169, doi:10.1093/pasj/psab112

[117] Xie, Xiao-Jia; Dong, Subo; Shvartzvald, Yossi; Gould, Andrew; Udalski, Andrzej; Beaulieu, Jean-Philippe; Beichman, Charles; Close, Laird Miller; b. Henderson, Calen; r. Males, Jared; Marquette, Jean-Baptiste; m. Morzinski, Katie; r. Gelino, Christopher (2022), “Characterizing microlensing planetary system OGLE-2014-BLG-0676Lb with adaptive optics imaging”, Research in Astronomy and Astrophysics, 21 (12): 303, arXiv:2112.08030, doi:10.1088/1674-4527/ac2a09, S2CID 244211319

[Sreenivas2021-118] Sreenivas, K. R.; Perdelwitz, V.; Tal-Or, L.; Trifonov, T.; Zucker, S.; Mazeh, T. (2022), “Analysis of the public HARPS/ESO spectroscopic archive”, Astronomy & Astrophysics, 660: A124, arXiv:2112.09029, doi:10.1051/0004-6361/202142612, S2CID 245219286

[Mufti2021-119] Mohammed El Mufti; và đồng nghiệp (2021), TOI 560 : Two Transiting Planets Orbiting a K Dwarf Validated with iSHELL, PFS and HIRES RVs, arXiv:2112.13448

[120] Miyazaki, Shota; và đồng nghiệp (2022), “OGLE-2014-BLG-0319: A Sub-Jupiter-mass Planetary Event Encountered Degeneracy with Different Mass Ratios and Lens-source Relative Proper Motions”, The Astronomical Journal, 163 (3): 123, arXiv:2112.14997, Bibcode:2022AJ....163..123M, doi:10.3847/1538-3881/ac4960, S2CID 245634898

[121] Wang(王涵悦), Hanyue; và đồng nghiệp (2022), “Systematic Korea Microlensing Telescope Network planetary anomaly search – III. One wide-orbit planet and two stellar binaries”, Monthly Notices of the Royal Astronomical Society, 510 (2): 1778–1790, arXiv:2112.02414, doi:10.1093/mnras/stab3581

[1]

[2]

[3]

[4]

[5]

[6]

[7]

[8]

[9]

[10]

[11]

[12]

[13]

[14]

[15]

[16]

[17]

[18]

[19]

[20]

[21]

[22]

[23]

[24]

[25]

[26]

[27]

[28]

[29]

[30]

[31]

[32]

[33]

[34]

[35]

[36]

[37]

[38]

[39]

[40]

[41]

[42]

[43]

[44]

[45]

[46]

[47]

[48]

[49]

[50]

[51]

[52]

[53]

[54]

[55]

[56]

[57]

[58]

[59]

[60]

[61]

[62]

[63]

[64]

[65]

[66]

[67]

[68]

[69]

[70]

[71]

[72]

[73]

[74]

[75]

[76]

[77]

[78]

[79]

[80]

[81]

[82]

[83]

[84]

[85]

[86]

[87]

[88]

[89]

[90]

[91]

[92]

[93]

[94]

[95]

[96]

[97]

[98]

[99]

[100]

Danh sách ngoại hành tinh được phát hiện năm 2021

Danh sách

Xem thêm

Tham khảo

Information related to Danh sách ngoại hành tinh được phát hiện năm 2021

Portal di Ensiklopedia Dunia