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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[sửa | sửa mã nguồn]

TênKhối lượng (MJ)Bán kính (RJ)Chu kỳ quỹ đạo (ngày)Bán trục nhỏ (AU)Nhiệt độ (K)Kĩ thuật quan sátKhoảng cách (ly)Khối lượng ngôi sao chủ (M)Nhiệt độ ngôi sao chủ (K)Chú thích
HD 108236 f0.17406+0.00482
−0.00437
29.54255± 0.000690.1759± 0.0037quá cảnh2110.853± 0.0475,720.0± 50.0[1][2]
NGTS-14Ab0.092± 0.0120.444± 0.0303.5357173± 0.00000690.0403± 0.00711,143± 139quá cảnh1,0600.898± 0.0355,187± 11[3]
TOI-1259Ab0.441+0.049
−0.047
1.022+0.030
−0.037
3.4779780+0.0000019
−0.0000017
0.04070+0.00114
−0.00110
936quá cảnh385± 10.68+0.1
−0.01
4,775± 100Also white dwarf on a wide orbit[4]
NGTS-13b4.84± 0.441.142± 0.0464.120.0549+0.0015
−0.0025
1,605± 30quá cảnh21501.30+0.11
−0.18
5,819± 73[5]
TOI-628 b6.33+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 cảnh5821.311+0.066
−0.075
6,250+220
−190
Host star also known as HD 288842[6]
TOI-640 b0.88± 0.161.771+0.060
−0.056
5.0037775± 0.00000480.06608+0.00098
−0.0011
1,749+26
−30
quá cảnh1,1151.536+0.069
−0.076
6,460+130
−150
[6]
TOI-1333 A b2.37± 0.241.396+0.056
−0.054
4.720219± 0.0000110.0626+0.0011
−0.0012
1,679+35
−34
quá cảnh6531.464+0.076
−0.079
6,274± 97Host star also known as BD+47 3521A.[6]
TOI-1478 b0.847+0.052
−0.048
1.061+0.040
−0.038
10.180249± 0.0000150.0903+0.0018
−0.0013
918± 11quá cảnh4980.946+0.059
−0.041
5,595+83
−81
[6]
TOI-1601 b0.99± 0.111.239+0.046
−0.039
5.331751± 0.0000110.06864+0.00079
−0.00075
1,619+24
−23
quá cảnh1,0961.517+0.053
−0.049
5,948+87
−89
[6]
OGLE-2019-BLG-0960Lb0.0071± 0.00271.75± 0.55thấu kính hấp dẫn2,900± 10000.45± 0.15Smallest planet discovered by thấu kính hấp dẫn[7]
HD 110113 b0.0143± 0.00200.183± 0.0112.541+0.0005
−0.001
0.035± 0.0011,371± 14quá cảnh346.5± 2.30.99± 0.085,730Radius gap planet, host star also known as TOI-755[8]
HD 110113 c0.0330± 0.00386.744+0.008
−0.009
0.068+0.001
−0.002
990± 10vận tốc xuyên tâm346.5± 2.30.99± 0.085,730Host star also known as TOI-755.[8]
KOI-5Ab0.1790.635quá cảnh1,870± 701.135861Also called TOI-1241b.[9][10]
TOI-178b0.0047+0.0012
−0.0013
0.102± 0.0061.914558± 0.0000180.02607± 0.000781,040+22
−21
quá cảnh205.16± 0.030.650+0.027
−0.029
4,316± 70[11]
TOI-178c0.015+0.0017
−0.0021
0.149+0.01
−0.008
3.238450+0.000020
−0.000019
0.0370± 0.0011873± 18quá cảnh205.16± 0.030.650+0.027
−0.029
4,316± 70[11]
TOI-178d0.0094+0.0025
−0.0032
0.229± 0.0066.557700± 0.0000160.0592± 0.0018690± 14quá cảnh205.16± 0.030.650+0.027
−0.029
4,316± 70[11]
TOI-178e0.0121+0.0039
−0.0029
0.197+0.007
−0.008
9.961881± 0.0000420.0783+0.0023
−0.0024
600± 12quá cảnh205.16± 0.030.650+0.027
−0.029
4,316± 70[11]
TOI-178f0.0242+0.0052
−0.0047
0.204± 0.00915.231915+0.000115
−0.000095
0.1039± 0.0031521± 11quá cảnh205.16± 0.030.650+0.027
−0.029
4,316± 70[11]
TOI-178g0.0123+0.0041
−0.0050
0.256+0.012
−0.011
20.70950+0.00014
−0.00011
0.1275+0.0038
−0.0039
470± 10quá cảnh205.16± 0.030.650+0.027
−0.029
4,316± 70[11]
HD 183579 b0.0620+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 cảnh186.1± 0.81.031+0.025
−0.026
5,788± 44Host star also known as TOI-1055[12][13]
KMT-2019-BLG-0371b7.70+11.34
−3.90
0.79+0.14
−0.16
thấu kính hấp dẫn2,3000+3,000
−4,000
0.09+0.14
−0.05
Multiple solutions for orbital separation[14]
HD 5278 b0.0245+0.0047
−0.0044
0.219± 0.00414.339156+0.000049
−0.000047
0.1202± 0.0013943± 13quá cảnh183.1± 2.71.126+0.036
−0.035
6,203± 64Host star also known as TOI-130.[15]
HD 5278 c0.0579+0.0057
−0.0060
0.2416± 0.00270.1202± 0.0013943± 13vận tốc xuyên tâm183.1± 2.71.126+0.036
−0.035
6,203± 64Host star also known as TOI-130.[15]
KMT-2018-BLG-1025Lb0.0191+0.0258
−0.0104
1.305+0.194
−0.227
thấu kính hấp dẫn22,000± 3,0000.219+0.297
−0.120
Multiple solutions for orbital parameters[16]
TOI-558b3.61± 0.151.086+0.041
−0.038
14.574071± 0.0000260.1291+0.0020
−0.0021
1,061+13
−12
quá cảnh1,312± 171.349+0.064
−0.065
6,466+95
−93
[17]
TOI-559b6.01+0.24
−0.23
1.091+0.028
−0.025
6.9839095± 0.00000510.0723± 0.00131,180+18
−16
quá cảnh761± 71.026± 0.0575,925+85
−76
[17]
Candidate 10.062-0.1570.3011-0.6386hình ảnh trực tiếp4.37Imaged near Alpha Centauri A
HD 13808 b0.034614.20.11vận tốc xuyên tâm92.20.771± 0.0225,035± 50Candidate since 2011,[18] confirmed in 2021[19]
HD 13808 c0.031553.80.26vận tốc xuyên tâm92.20.771± 0.0225,035± 50Candidate since 2011,[18] confirmed in 2021[19]
TOI 451 b0.1732+0.0134
−0.0116
1.858701+0.000027
−0.000033
0.0271+0.0023
−0.0038
1,524+100
−60
quá cảnh405.1± 1.30.94± 0.0255,550± 56Planets orbiting primary of wide binary system.[20][21] Host star also known as CD-38 1467.
TOI 451 c0.2741± 0.01259.192523+0.000064
−0.000084
0.0771+0.0066
−0.0093
903+53
−36
quá cảnh405.1± 1.30.94± 0.0255,550± 56Planets orbiting primary of wide binary system.[20][21] Host star also known as CD-38 1467.
TOI 451 d0.3598± 0.013416.364981+0.000047
−0.000049
0.1255+0.0057
−0.0065
708+15
−12
quá cảnh405.1± 1.30.94± 0.0255,550± 56Planets orbiting primary of wide binary system[20][21] Host star also known as CD-38 1467.
HD 110082 b0.2857± 0.008910.18271± 0.000040.113+0.009
−0.013
quá cảnh342.8± 0.91.21± 0.066,200± 100Orbiting a primary of wide binary system[22] Host star also known as TOI-1098.
OGLE-2018-BLG-0567Lb0.32+0.34
−0.16
2.72+0.49
−0.55
thấu kính hấp dẫn23,000± 3,0000.24+0.16
−0.13
[23]
OGLE-2018-BLG-0962Lb1.37+0.80
−0.72
3.57+0.68
−1.02
thấu kính hấp dẫn21,000+3,000
−5,000
0.55+0.32
−0.29
[23]
Gliese 740 b0.0093± 0.00162.37756+0.00013
−0.00011
0.029± 0.001829+40
−50
vận tốc xuyên tâm36.21± 0.020.58± 0.063,913± 21[24]
OGLE-2018-BLG-1428Lb0.77+0.77
−0.53
3.30+0.59
−0.83
thấu kính hấp dẫn20,000+3,000
−5,000
0.43+0.33
−0.22
[25]
LHS 1478 b0.0073± 0.00060.111± 0.0041.9495378+0.0000040
−0.0000041
0.01848+0.00061
−0.0006
595+10
−9
quá cảnh59.40± 0.030.236± 0.0123,381± 54[26] Host star also known as TOI-1640 or G 245-61.
TOI-1685 b0.0121± 0.0300.131± 0.0060.6691425± 0.00000370.01156± 0.000091,052± 21quá cảnh122.68± 0.090.495± 0.0193,434± 51[27][28] Host star also known as UCAC4 666-026266
TOI-1685 c0.0290± 0.00659.025+0.104
−0.119
449.1± 6.9vận tốc xuyên tâm122.68± 0.090.495± 0.0193,434± 51Unconfirmed[27]
KMT-2020-BLG-0414Lb0.00320.15thấu kính hấp dẫn3,300± 3000.3Also a brown dwarf with mass 17 MJ in the system at 15 AU separation[29]
HD 39474 b0.42+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 cảnh372.5± 1.11.316± 0.0276,394± 75Host star also known as TOI-201[30]
Gliese 486 b0.0089± 0.00040.117± 0.0061.467119+0.000031
−0.000030
0.01734+0.00026
−0.00027
701± 13quá cảnh26.344± 0.0130.323± 0.0153,340± 54Planet may have a measurable atmosphere[31]
NGTS-15b0.751+0.102
−0.088
1.10± 0.103.27623± 0.000010.0441± 0.00461,146± 47quá cảnh2,580± 600.995± 0.0155,600± 150[32]
NGTS-16b0.667+0.157
−0.129
1.30+0.13
−0.12
4.84532± 0.000020.0523± 0.00641,177± 59quá cảnh2,910+95
−75
1.002± 0.0115,550± 150[32]
NGTS-17b0.764+0.195
−0.164
1.24± 0.113.24253± 0.000010.0391± 0.00431,457± 50quá cảnh3,420± 901.025+0.015
−0.014
5,650± 100[32]
NGTS-18b0.409+0.081
−0.063
1.21± 0.183.05125± 0.000010.0448± 0.00681,381+55
−53
quá cảnh3,610± 1401.003+0.020
−0.012
5,610± 150[32]
OGLE-2019-BLG-1053Lb0.0078+0.0037
−0.0031
3.4± 0.5thấu kính hấp dẫn22,000+3,000
−2,000
0.61+0.29
−0.24
[33]
TOI-1634 b0.0313± 0.00300.158± 0.0070.9893457± 0.00000340.01491± 0.00015921± 21quá cảnh114.40± 0.080.452± 0.0143,472± 48[28][34]
KMT-2019-BLG-17152.56+1.13
−1.16
3.32+0.82
−0.92
thấu kính hấp dẫn13,000± 3,0000.61+0.27
−0.28
Multiple solutions for orbital separation, also 0.15M red dwarf in the system.[35]
OGLE-2018-BLG-1185b0.026+0.025
−0.015
1.54+0.18
−0.22
thấu kính hấp dẫn24,000+2,000
−3,000
0.37+0.35
−0.21
Multiple solutions for planet and star masses.[36]
TOI-1260 b0.0271+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 cảnh239.5± 0.30.66± 0.014,227± 85[37]
TOI-1260 c0.0373+0.0106
−0.0102
0.252± 0.0137.49325+0.00015
−0.00013
0.0656+0.0039
−0.0065
643+35
−23
quá cảnh239.5± 0.30.66± 0.014,227± 85[37]
KMT-2018-BLG-1976Lb1.96+1.23
−1.12
2.04+0.72
−0.83
thấu kính hấp dẫn19,000± 2,0000.65+0.41
−0.37
[38]
KMT-2018-BLG-1996Lb1.22+0.72
−0.63
1.97+0.51
−0.25
thấu kính hấp dẫn19,000± 2,0000.69+0.40
−0.38
[38]
OGLE-2019-BLG-0954Lb14.2+9.9
−7.5
2.65+0.89
−1.20
thấu kính hấp dẫn12,000+1,000
−2,000
0.80+0.55
−0.42
[38]
YSES 2 b6.3+1.6
−0.9
115hình ảnh trực tiếp356.4± 0.51.10± 0.034,749± 40[39]
KMT-2016-BLG-2605b0.8+1.2
−0.4
0.68± 0.11thấu kính hấp dẫn21,000± 3,0000.065+0.10
−0.035
[40]
TOI-1431 b3.14+0.19
−0.18
1.51± 0.062.65022± 0.000010.047± 0.0022,370± 100quá cảnh488± 31.90+0.10
−0.08
7,690+400
−250
Also known as MASCARA-5b[41][42]
TOI-269 b0.0277± 0.00440.247± 0.0113.697723+0.000018
−0.000017
0.0345± 0.0015531± 25quá cảnh186.01± 0.250.3917± 0.00953,514± 70[43]
TOI-220 b0.0434± 0.00310.271± 0.01310.6952640.08911± 0.0010805± 21quá cảnh290± 130.825± 0.0285,298± 65Additional long-period planet suspected[44]
TOI 1062 b0.0320± 0.00260.202± 0.0084.11412+0.0014
−0.0015
0.0521,077+10
−9
quá cảnh268.7± 0.20.94± 0.025,328± 56[45]
TOI 1062 c0.0294± 0.00397.978+0.021
−0.023
0.080+0.013
−0.012
859+9
−8
vận tốc xuyên tâm268.7± 0.20.94± 0.025,328± 56[45]
Kepler-129d8.3+1.1
−0.7
2646+140
−94
4.0± 0.1vận tốc xuyên tâm1,349± 141.185,770[46]
Gliese 9689 b0.0304± 0.004618.27± 0.010.1139± 0.0039453± 39vận tốc xuyên tâm100.10± 0.040.59± 0.063,836± 69[47]
TOI-1231 b0.0485± 0.01040.326± 0.01424.245586+0.000064
−0.000066
0.1288+0.0021
−0.0022
330quá cảnh89.68± 0.040.485± 0.0243,553± 31[48]
TIC 172900988 b2.84± 0.251.009± 0.043196.5± 7.7quá cảnh799± 91.24 and 1.206050 and 5983Circumbinary planet[49]
TOI-1444 b0.0122± 0.00220.125± 0.0060.4702694± 0.00000440.1288+0.0021
−0.0022
330quá cảnh408.9± 0.50.934± 0.0385,430± 90[50]
BD+45 0564 b1.36± 0.12307.88± 1.470.83± 0.04vận tốc xuyên tâm174± 20.81± 0.075,004± 50[51]
BD+55 0362 b0.72± 0.08265.59± 1.040.78± 0.05vận tốc xuyên tâm168± 20.909± 0.0995,012± 78Additional giant planet is suspected[51]
BD+63 1405 b3.96± 0.311,198.48± 60.792.06± 0.14vận tốc xuyên tâm124.4± 1.20.82± 0.085,000± 53Extremely eccentric orbit[51]
HD 124330 b0.75± 0.06270.66± 1.210.86± 0.04vận tốc xuyên tâm198± 31.15± 0.0795,873± 19Additional giant planet is suspected[51]
HD 155193 b0.75± 0.06352.65± 2.581.04± 0.04vận tốc xuyên tâm186± 61.221± 0.0836,239± 20[51]
HD 331093 b1.50± 0.11621.62± 16.111.44± 0.07vận tốc xuyên tâm164.07± 0.141.030± 0.0795,544± 33[51]
HD 107148 c0.0626+0.0097
−0.0098
18.3267+0.0022
−0.0024
0.1406± 0.0018vận tốc xuyên tâm161.4± 0.41.1± 0.15,789± 36[52]
HD 136925 b0.84+0.078
−0.074
4,540+160
−140
5.13+0.12
−0.11
vận tốc xuyên tâm156.25715Additional planet suspected[52]
Lambda Serpentis b0.0428+0.0047
−0.0045
15.5083+0.0016
−0.0018
0.1238± 0.002vận tốc xuyên tâm38.87± 0.071.145,884± 4[52]
HD 156668 c0.0991+0.0079
−0.0077
811.3+5.2
−5.3
1.570± 0.017vận tốc xuyên tâm79.34± 0.030.772± 0.0204,850± 88Additional body in system is suspected[52]
HD 164922 e0.0331± 0.003141.763± 0.0120.2293+0.0026
−0.0027
vận tốc xuyên tâm71.69± 0.030.874± 0.0125,293± 32[52]
HD 168009 b0.0300+0.0038
−0.0037
15.1479+0.0035
−0.0037
0.1192+0.0017
−0.0018
vận tốc xuyên tâm75.97± 0.030.995,792± 80[52]
HD 213472 b3.48+1.10
−0.59
16,700+12,000
−4,800
13.0+5.7
−2.6
vận tốc xuyên tâm210.6[52]
HD 24040 c0.201± 0.027515.4+2.2
−2.5
1.3± 0.021vận tốc xuyên tâm152.3± 0.41.14± 0.025,917± 52[52]
HD 26161 b13.5+8.5
−3.7
32,000+21,000
−10,000
20.4+7.9
−4.9
vận tốc xuyên tâm133.6± 0.3Very eccentric orbit, and also red dwarf in the system[52]
HD 3765 b0.173+0.014
−0.013
1,211+15
−16
2.108+0.032
−0.033
vận tốc xuyên tâm78.5± 0.1[52]
HD 66428 c27+22
−17
39,000+56,000
−18,000
23.0+19.0
−7.6
vận tốc xuyên tâm174.1± 0.71.09± 0.025,773± 55[52]
HD 68988 c15.0+2.8
−1.5
16,100+11,000
−3,500
13.2+5.3
−2.0
vận tốc xuyên tâm198.8± 0.61.16± 0.015,919± 11Suspected since 2006[52]
Lalande 21185 c0.0568+0.0091
−0.0083
3190+200
−170
3.1+0.13
−0.11
vận tốc xuyên tâm8.31± 0.010.390± 0.0113,601± 51[52]
G 264-12 b0.0079± 0.00092.30538± 0.000310.02279± 0.00061587± 16vận tốc xuyên tâm52.14± 0.030.297± 0.0243,326± 54[53]
G 264-12 c0.0118± 0.00158.0518± 0.00340.0525± 0.0014387± 11vận tốc xuyên tâm52.14± 0.030.297± 0.0243,326± 54[53]
Gliese 393 b0.0054± 0.00087.02679+0.00082
−0.00085
0.05402± 0.00072485± 11vận tốc xuyên tâm22.956± 0.0080.426± 0.0173,579± 51[53]
TOI-674b0.0739± 0.01040.470± 0.0161.977143± 0.0000030.0231± 0.0007661± 14quá cảnh150.86± 0.110.442± 0.0073,505+28
−32
[54] Possibly steam atmosphere[55]
HD 152843 b (ja)0.0364+0.0207
−0.0193
0.304± 0.01211.6264+0.0022
−0.0025
0.1053+0.003
−0.0031
quá cảnh352.0± 1.01.15± 0.046,310± 100[56]
HD 152843 c (ja)0.08650.521± 0.01324.38+6.23
−3.4
quá cảnh352.0± 1.01.15± 0.046,310± 100[56]
KMT-2019-BLG-0253b0.029+0.016
−0.013
3.1+0.8
−0.9
thấu kính hấp dẫn16,000+6,000
−5,000
0.70+0.34
−0.31
[57]
OGLE-2018-BLG-05060.051+0.038
−0.027
3.0+0.7
−0.8
thấu kính hấp dẫn18,000± 5,0000.63+0.37
−0.32
[57]
OGLE-2018-BLG-05160.063+0.052
−0.034
2.2+0.8
−0.7
thấu kính hấp dẫn7,000+3,000
−2,000
0.47+0.38
−0.25
[57]
OGLE-2019-BLG-14920.117+0.079
−0.061
2.7± 0.9thấu kính hấp dẫn18,000+6,000
−7,000
0.68± 0.34[57]
OGLE-2018-BLG-09770.020+0.016
−0.012
2.0+0.6
−0.5
thấu kính hấp dẫn7,000± 2,0000.47+0.38
−0.27
[57]
TOI-1789 b0.70± 0.161.40+0.22
−0.13
3.208666± 0.0000160.04873+0.00065
−0.0016
1,929+28
−18
quá cảnh729± 31.499+0.061
−0.15
5,984+55
−57
[58]
TOI-942 b0.347+0.022
−0.020
4.32421± 0.0000190.04866+0.00016
−0.00013
quá cảnh493.9± 1.00.8220+0.0079
−0.0064
[59]
TOI-942 c0.417+0.030
−0.027
10.156272+0.000037
−0.000034
0.08598+0.00027
−0.00022
quá cảnh493.9± 1.00.8220+0.0079
−0.0064
[59]
KMT-2018-BLG-17430.245+0.339
−0.135
1.449+0.209
−0.229
thấu kính hấp dẫn21,000± 3,0000.193+0.268
−0.107
Multiple orbital solutions, binary host star[60]
TOI-1749 b0.060+0.07
−0.04
0.124± 0.0182.388821+0.000057
−0.000073
0.0291± 0.0005831± 18quá cảnh324.8± 0.40.58± 0.033,985± 55[61]
TOI-1749 c0.007+0.018
−0.005
0.189± 0.0114.489010+0.000040
−0.000061
0.0443± 0.0008673± 15quá cảnh324.8± 0.40.58± 0.033,985± 55[61]
TOI-1749 d0.014+0.020
−0.011
0.225± 0.0139.04455± 0.000120.0707± 0.0012533± 12quá cảnh324.8± 0.40.58± 0.033,985± 55[61]
HD 27969 b4.80+0.24
−0.23
654.5+5.7
−5.8
1.552+0.032
−0.033
261± 11vận tốc xuyên tâm1.16± 0.075,966± 21[62]
HD 80869 b4.86+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 tâm1.08± 0.055,837± 15Very eccentric orbit[62]
HD 95544 b6.84± 0.312172+23
−21
3.386+0.075
−0.077
156.5+5.4
−5.5
vận tốc xuyên tâm1.09± 0.075,722± 15[62]
HD 109286 b2.99± 0.15520.1± 2.31.259± 0.021259.4± 5.5vận tốc xuyên tâm0.98± 0.055,694± 23[62]
HD 115954 b8.29+0.75
−0.58
3700+1500
−390
5.00+1.3
−0.36
144.9+8.1
−13
vận tốc xuyên tâm1.18± 0.065957± 26[62]
HD 211403 b5.54+0.39
−0.38
223.8± 0.410.768± 0.013380± 13vận tốc xuyên tâm1.20± 0.066,273± 44[62]
Kepler-1704b4.15± 0.291.065+0.043
−0.041
988.88113+0.00091
−0.00092
2.026+0.024
−0.031
253.8+3.7
−4.1
quá cảnh2,690± 401.131+0.040
−0.051
5,745+88
−89
Very eccentric orbit (e=0.921),[63]
TOI-532b0.1935+0.0305
−0.0293
0.520± 0.0172.3266508± 0.00000300.0296± 0.00035867± 18quá cảnh439.1± 1.20.639± 0.0233927± 37Neptunian desert planet[64]
TOI-2406b0.0286+0.0223
−0.0126
0.263+0.015
−0.014
3.0766896± 0.00000650.0228± 0.0016447± 15quá cảnh181.4± 0.40.162± 0.0083,100± 75[65]
KIC 8121913 b2.1± 0.43.294601+0.000013
−0.00022
orbital brightness modulation23501.456+0.069
−0.15
5075.3+110.2
−109.4
[66]
KIC 10068024 b2.0± 0.42.073549+0.000008
−0.000177
orbital brightness modulation3,6001.22+0.175
−0.139
6,118.4+127.2
−121.2
[66]
KIC 5479689 b0.5+0.4
−0.1
1.701531+0.000008
−0.000419
orbital brightness modulation1,5040.966+0.03
−0.04
5459.1+90.0
−85.2
[66]
LTT 1445 Ac0.0048± 0.00060.1033.123900.02661+0.00047
−0.00049
quá cảnh22.41± 0.010.256± 0.0143337± 150[67]
Luyten 98-59 e0.009412.80.071342+20
−18
vận tốc xuyên tâm34.60.32± 0.033500± 150[68]
Luyten 98-59 f0.007823.20.103285+18
−17
vận tốc xuyên tâm34.60.32± 0.033500± 150Unconfirmed, potentially habitable exoplanet[68]
HD 191939 e0.34± 0.01101.4± 0.40.397± 0.005397± 16vận tốc xuyên tâm175.1± 0.20.925400Also suspected brown dwarf on wider orbit[69]
OGLE-2019-BLG-10586.836± 6.027thấu kính hấp dẫn8,000± 5,000Multiple solutions, rogue planet[70]
TOI-2184 b0.65± 0.161.017± 0.0516.90683± 0.00009quá cảnh2,515± 221.53± 0.125,966± 136[71]
TOI-431 b0.0097± 0.00110.0014± 0.0040.490047+0.000010
−0.000007
0.0113+0.0002
−0.0003
1,862± 42quá cảnh106.37± 0.030.78± 0.074,850± 75Host star lso known as CD-26 2288 or HIP 26013.[72]
TOI-431 c0.0089+0.0013
−0.0011
4.8494+0.0003
−0.0002
0.0052± 0.001867± 20vận tốc xuyên tâm106.37± 0.030.78± 0.074,850± 75Host star also known as CD-26 2288 or HIP 26013.[72]
TOI-431 d0.0312± 0.00470.294± 0.00812.46103± 0.000020.098± 0.002633± 14quá cảnh106.37± 0.030.78± 0.074,850± 75Host star lso known as CD-26 2288 or HIP 26013.[72]
TOI-2202 b0.927+0.047
−0.048
1.01+0.522
−0.080
11.9108+0.0009
−0.0009
0.0956+0.0015
−0.0016
quá cảnh770± 30.823+0.027
−0.023
5,144± 50[73]
TOI-2202 c0.191+0.033
−0.030
24.7545+0.0073
−0.0078
0.1558+0.0025
−0.0026
timing770± 30.823+0.027
−0.023
5,144± 50[73]
EPIC 211314705.010.139± 0.0073.793306+0.000324
−0.000343
543+8
−9
quá cảnh300.0± 1.70.43± 0.013,669+88
−82
[74] Two more planets in system are suspected.[75]
EPIC 211401787.010.247+0.013
−0.008
13.774798+0.000028
−0.000028
969± 9quá cảnh525± 51.23± 0.026,232+33
−39
[74] Host star also known as BD+12 1842.
K2-268f0.199+0.013
−0.008
26.270570+0.000105
−0.000109
492+8
−10
quá cảnh1,079± 100.84± 0.025,106+70
−61
Two more planets were previously known; host star also known as EPIC 211413752.[74]
K2-268d0.133+0.013
−0.006
4.528598+0.000016
−0.000015
888+16
−15
quá cảnh1,079± 100.84± 0.025,106+70
−61
Two more planets were previously known; host star also known as EPIC 211413752.[74]
K2-268e0.119+0.010
−0.007
6.131243+0.000032
−0.000033
801± 13quá cảnh1,079± 100.84± 0.025,106+70
−61
Two more planets were previously known; host star also known as EPIC 211413752.[74]
EPIC 211502222.010.243+0.013
−0.009
22.996591+0.001848
−0.001859
673+12
−11
quá cảnh694± 61.10+0.03
−0.04
5,994+93
−91
[74]
EPIC 211502222.020.160+0.013
−0.009
9.398977+0.001506
−0.001348
909± 14quá cảnh694± 61.10+0.03
−0.04
5,994+93
−91
[74]
EPIC 211579112.010.196+0.017
−0.014
17.706320± 0.000063266+5
−8
quá cảnh403± 50.27+0.01
−0.02
3,315+137
−152
[74]
K2-185c0.213± 0.00852.713494+0.000155
−0.000164
477+14
−17
quá cảnh882± 110.96+0.05
−0.07
5,788+190
−157
Host star also known as EPIC 211611158.[74]
EPIC 211647930.010.552+0.025
−0.022
14.759287+0.000243
−0.000240
826+14
−17
quá cảnh1,133± 171.06± 0.045,880+85
−82
[74]
EPIC 211730024.010.504+0.032
−0.025
5.113981+0.000061
−0.000062
1,380+34
−30
quá cảnh1,226± 211.36± 0.056,502+132
−130
[74]
EPIC 211743874.010.197+0.016
−0.013
12.283211± 0.000051949+21
−26
quá cảnh1,850± 601.23± 0.046,222+96
−91
[74]
EPIC 211763214.010.109+0.008
−0.005
21.194733+0.000108
−0.000107
569+15
−22
quá cảnh786± 90.86+0.03
−0.05
5,424+192
−144
[74]
EPIC 211770696.010.234+0.017
−0.013
16.273563+0.000054
−0.000053
850+19
−18
quá cảnh1,390± 300.94+0.04
−0.03
5,869+88
−81
[74]
EPIC 211779390.010.092+0.010
−0.005
3.850614± 0.000012783+12
−14
quá cảnh514± 20.66± 0.024,558+91
−81
[74]
EPIC 211897691.020.171+0.017
−0.011
19.507428+0.000116
−0.000113
508± 12quá cảnh1,187± 170.74+0.04
−0.03
4,857+86
−84
[74]
EPIC 211923431.010.300+0.039
−0.029
29.740451+0.000169
−0.000161
606+31
−36
quá cảnh2,460± 700.93± 0.045,532± 90[74]
EPIC 211978988.010.287+0.022
−0.017
36.552551+0.000127
−0.000122
598+16
−15
quá cảnh1,390± 200.98± 0.075,817+45
−48
[74]
TOI-1518 b2.31.875± 0.0531.902603± 0.0000110.0389± 0.00113,237± 59quá cảnh742± 61.79± 0.267,300± 100[74]
EPIC 212058012.010.181+0.012
−0.008
11.561052+0.000690
−0.000668
861+14
−15
quá cảnh684± 61.01± 0.055,920± 104[74]
EPIC 212072539.010.180+0.009
−0.006
7.676972+0.000012
−0.000012
465± 7quá cảnh545± 30.49± 0.013,804+93
−74
[74]
EPIC 212072539.020.147+0.015
−0.007
2.787174± 0.000004653+10
−12
quá cảnh545± 30.49± 0.013,804+93
−74
[74]
EPIC 212081533.010.142+0.009
−0.004
3.355850+0.000091
−0.000093
722+7
−10
quá cảnh245.80.51± 0.014,374+38
−34
[74]
EPIC 212088059.010.188+0.018
−0.008
10.367437+0.000020
−0.000019
437+4
−5
quá cảnh532± 30.56± 0.013,779+30
−26
[74]
EPIC 212132195.010.202+0.017
−0.009
26.201446+0.003331
−0.003124
450± 5quá cảnh345.5± 1.60.71± 0.024,801± 49[74]
EPIC 212161956.010.215+0.010
−0.009
7.187257+0.000020
−0.000021
640+20
−21
quá cảnh1055± 130.66± 0.034,599+178
−152
[74]
EPIC 212204403.010.291+0.020
−0.010
4.688418+0.000119
−0.000117
908+12
−11
quá cảnh662± 50.83+0.02
−0.01
5,077+40
−39
[74]
EPIC 212204403.020.238+0.021
−0.010
12.550171+0.001018
−0.001057
655+7
−9
quá cảnh662± 50.83+0.02
−0.01
5,077+40
−39
[74]
K2-304c0.203+0.017
−0.011
5.213965± 0.000442866+27
−37
quá cảnh1,380± 200.83+0.05
−0.04
5,171+172
−130
Host star also known as EPIC 212297394.[74]
EPIC 212420823.010.123+0.009
−0.006
9.032178± 0.000874518+5
−4
quá cảnh1,450± 200.54± 0.014,385+29
−31
[74]
EPIC 212440430.020.138+0.013
−0.010
4.163873+0.000022
−0.000023
1,158+29
−34
quá cảnh1,620± 200.98± 0.025,789+46
−50
[74]
EPIC 212543933.010.227+0.023
−0.017
7.806164+0.000673
−0.000623
934+28
−32
quá cảnh1,310± 501.02± 0.025,769+39
−37
[74]
K2-307c0.207+0.017
−0.011
23.228555+0.000068
−0.000071
658+13
−14
quá cảnh1,050± 200.99+0.03
−0.04
6,004+77
−78
Host star also known as EPIC 212587672.[74]
EPIC 251319382.010.171+0.012
−0.006
8.234885+0.000508
−0.000475
885+12
−14
quá cảnh577± 60.95± 0.025,791± 81[74]
EPIC 251319382.020.199+0.012
−0.008
14.871387+0.000916
−0.000936
727± 10quá cảnh577± 60.95± 0.025,791± 81[74]
EPIC 251319382.030.122+0.009
−0.006
3.665912+0.000273
−0.000295
1,160+16
−15
quá cảnh577± 60.95± 0.025,791± 81[74]
EPIC 251554286.010.496+0.020
−0.018
15.466805+0.000572
−0.000565
735+13
−14
quá cảnh883± 120.87± 0.025,698± 55[74]
Gliese 146 b0.0175+0.0023
−0.0021
5.09071 ± 0.000260.0510+0.0024
−0.0026
573+63
−69
vận tốc xuyên tâm44.37± 0.010.684± 0.0134,385± 21Host star also known as HD 22496.[76]
EPIC 211525753.010.201+0.020
−0.014
5.7385647+0.0013939
−0.0011048
0.0632+0.0096
−0.0176
1,066+190
−77
quá cảnh0.96+0.05
−0.06
5,790+177
−147
[77]
EPIC 211537087.010.204+0.013
−0.011
21.0267366+0.0036912
−0.0038993
0.1599+0.0178
−0.0306
624+0
−37
quá cảnh0.90+0.05
−0.06
5,568+178
−150
[77]
EPIC 211730267.010.332+0.021
−0.019
16.3488637+0.0013811
−0.0014022
0.1450+0.0136
−0.0235
735+8
−39
quá cảnh0.98± 0.075,794+210
−169
[77]
EPIC 211914998.010.239+0.015
−0.013
11.2510285+0.0018188
−0.0017892
0.0863+0.0079
−0.0159
888+0
−47
quá cảnh0.93± 0.065,650+193
−152
[77]
TOI-3362b5.029+0.668
−0.646
1.142+0.043
−0.041
18.09547± 0.000030.153+0.002
−0.003
quá cảnh1,198± 181.445+0.069
−0.073
6,532+88
−86
High eccentricity orbit[78]
KMT-2017-BLG-2509b2.09+1.68
−1.26
2.14+0.27
−0.39
thấu kính hấp dẫn23,000± 3,0000.46+0.37
−0.27
[79]
OGLE-2017-BLG-1099b3.02+2.43
−1.81
2.73+0.40
−0.53
thấu kính hấp dẫn24,000± 3,0000.45+0.36
−0.27
[79]
OGLE-2019-BLG-0299b6.22+3.80
−3.67
2.80+0.58
−0.89
thấu kính hấp dẫn19,000± 4,0000.59+0.36
−0.35
[79]
TOI-1296b0.298± 0.0391.231± 0.0313.9443715± 0.00000580.0497+0.0023
−0.0028
1,562+43
−31
quá cảnh1,023± 41.17± 0.145,603± 47[80]
TOI-1298b0.356± 0.0320.841± 0.0214.537164± 0.0000120.0590± 0.00231,388± 24quá cảnh1,041± 71.44± 0.105,889± 43[80]
TOI-1201 b0.0198± 0.00270.216± 0.0082.4919863+0.0000030
−0.0000031
0.0287± 0.0012703+15
−14
quá cảnh122.77± 0.100.512± 0.0203,476± 51Belongs to the Hyades, also red dwarf in the system.[81]
RR Caeli c2.7± 0.714,200± 3009.7± 0.9timing69.10± 0.030.18+0.443,100+7,540Circumbinary planet around red and white dwarfs[82]
TIC 257060897b0.67± 0.031.49± 0.043.660028± 0.0000060.051± 0.0021,762± 21quá cảnh1,655± 81.32± 0.046,128± 57[83]
TOI-530b0.40+0.09
−0.10
0.83± 0.066.387597+0.000019
−0.000018
0.052+0.005
−0.004
565+28
−31
quá cảnh482± 20.53± 0.023,659± 120[84]
HIP 97166b0.0629± 0.0470.245± 0.01210.28891± 0.000040.089± 0.001757± 25quá cảnh215.54± 0.330.898± 0.0545,198± 100[85]
HIP 97166c9.9± 1.816.84± 0.220.124± 0.002642± 22vận tốc xuyên tâm215.54± 0.330.898± 0.0545,198± 100[85]
HD 63935 b0.0340± 0.00570.267± 0.0139.058811+0.000017
−0.000016
911± 27quá cảnh159.36± 0.150.933± 0.0545,534± 100[86]
HD 63935 c0.0349± 0.00760.259± 0.01221.4023+0.00189
−0.00194
684± 21quá cảnh159.36± 0.150.933± 0.0545,534± 100[86]
HD 207897 b0.0453± 0.00500.223± 0.00716.202159+0.000085
−0.000083
0.1163+0.0017
−0.001
632.2+8.1
−7.0
quá cảnh92.15± 0.100.80+0.036
−0.030
5,070+60
−57
[87]
2MASS J04372171+2651014 b4± 11151,450± 50hình ảnh trực tiếp417.9± 1.50.165± 0.0153,100[88][89]
TOI 1227 b0.854+0.067
−0.052
27.36397± 0.000110.0886+0.0054
−0.0057
quá cảnh329.3± 0.80.170± 0.0153,072± 74[90]
TOI-2285b0.155± 0.00727.26955+0.00013
−0.00010
0.1363± 0.0010284± 6quá cảnh138.34± 0.140.454± 0.0103,491± 58[91]
LHS 1678 b0.0002± 0.00030.062± 0.0040.8602322+0.0000068
−0.0000048
0.01251+0.00059
−0.00056
quá cảnh64.88± 0.030.345± 0.0143490± 50[92]
LHS 1678 c0.0012+0.0013
−0.0008
0.088± 0.0063.694247+0.0000024
−0.0000021
0.0331+0.0016
−0.0015
quá cảnh64.88± 0.030.345± 0.0143490± 50[92]
HD 73583 b0.0315± 0.00980.253± 0.0096.3980418+0.0000065
−0.0000063
0.0601± 0.0026721± 21quá cảnh103.08± 0.100.71± 0.024511± 110Host star also known as TOI-560,[93] planetary helium emission detected.[94]
HD 73583 c0.0302± 0.00550.212± 0.00918.8797+0.00088
−0.00073
0.1236+0.0053
−0.0053
503± 15quá cảnh103.08± 0.100.71± 0.024511± 110Host star also known as TOI-560[93]
TOI-1807 b (it)0.0071+0.0015
−0.0018
0.165± 0.0040.549372± 0.0000070.0135+0.0013
−0.0022
1499+82
−129
quá cảnh133.88± 0.250.750+0.025
−0.024
4757+51
−50
Star is co-moving with TOI-2076[95][96]
TOI-2076 b0.293± 0.03810.35566± 0.000060.0631± 0.0027870± 13quá cảnh136.70± 0.230.850+0.025
−0.026
5187+54
−53
Star is co-moving with TOI-1807[95]
TOI-2076 c0.396± 0.00421.01538+0.00084
−0.00074
0.0885± 0.0038734± 11quá cảnh136.70± 0.230.850+0.025
−0.026
5187+54
−53
[97] Star is co-moving with TOI-1807[95]
TOI-2076 d0.370± 0.00625.0893± 0.010.1138+0.0048
−0.0049
648± 10quá cảnh136.70± 0.230.850+0.025
−0.026
5187+54
−53
Star is co-moving with TOI-1807[95]
TOI-2257 b0.196± 0.01035.1893460.145± 0.003256+61
−17
quá cảnh188.5± 0.30.33± 0.023430± 130Habitable zone planet[98]
TOI-712 b0.01760.183+0.011
−0.007
9.531361+0.000018
−0.000017
0.07928+0.00096
−0.00091
650.0+6.0
−5.9
quá cảnh191.2± 0.40.732+0.027
−0.025
4622+61
−59
[99]
TOI-712 c0.02740.241+0.008
−0.007
51.69906± 0.000170.2447+0.0030
−0.0028
369.9+3.4
−3.3
quá cảnh191.2± 0.40.732+0.027
−0.025
4622+61
−59
[99]
TOI-712 d0.02360.221+0.008
−0.007
84.83960+0.00043
−0.00040
0.3405+0.0041
−0.0039
313.6+2.9
−2.8
quá cảnh191.2± 0.40.732+0.027
−0.025
4622+61
−59
[99]
OGLE-2019-BLG-0468Lb3.43+1.83
−1.17
3.29+4.15
−2.52
thấu kính hấp dẫn14000± 30000.92+0.49
−0.32
Multiple solutions for orbital parameters[100]
OGLE-2019-BLG-0468Lc10.22+5.46
−3.50
2.77+3.49
−2.12
thấu kính hấp dẫn14000± 30000.92+0.49
−0.32
Multiple solutions for orbital parameters[100]
KMT-2021-BLG-0912Lb0.022+0.007
−0.008
3.03+3.46
−2.46
thấu kính hấp dẫn22000± 30000.75+0.23
−0.28
Multiple solutions for orbital parameters[101]
HD 137496 b0.0127± 0.00170.117± 0.0051.62116± 0.000080.02732± 0.000192130+30
−29
quá cảnh509± 61.035± 0.0225799± 61[102]
HD 137496 c7.66± 0.11479.9+1.1
−1.0
1.2163+0.0087
−0.0088
370± 5vận tốc xuyên tâm509± 61.035± 0.0225799± 61[102]
HD 19615 b8.5± 0.7402± 21.1± 0.1vận tốc xuyên tâm872± 71.1± 0.13987± 125Red giant host star[103]
HD 150010 b2.4± 0.4562± 81.1± 0.1vận tốc xuyên tâm473.4± 2.11.3± 0.14256± 125Red giant host star[103]
HD 174205 b4.2± 0.5582± 171.7± 0.1vận tốc xuyên tâm769± 51.8± 0.14393± 125Red giant host star[103]
KMT-2018-BLG-1988Lb0.021+0.015
−0.011
2.83+1.23
−0.97
thấu kính hấp dẫn14000+6000
−5000
0.48+0.33
−0.25
Multiple solutions for orbital parameters[104]
KOI-984b0.0544± 0.00940.384± 0.0044.2881785± 0.00000350.0504± 0.00061022+31
−30
quá cảnh749± 40.928± 0.0315295± 150Another planet in system on poorly constrained orbit[105]
TOI-2109b5.02± 0.751.347± 0.0470.67247414± 0.000000280.01791± 0.000653631± 69quá cảnh846± 91.447+0.075
−0.078
6530+160
−150
[106]
TOI-1238b0.0183± 0.00350.108± 0.0100.764596+0.000016
−0.000013
0.0139± 0.00081133± 167quá cảnh2030.44± 0.200.59± 0.024089± 54[107]
TOI-1238c0.0262± 0.00590.188± 0.0133.294733+0.000040
−0.000047
0.037± 0.002695± 105quá cảnh2030.44± 0.200.59± 0.024089± 54[107]
K2-99c8.4± 0.2522.2± 1.41.43± 0.01390± 6vận tốc xuyên tâm19801.65990[108]
HIP 5763b0.5130.014+0.1528
−0.2842
0.170vận tốc xuyên tâm104.17± 0.140.72[109]
HIP 34222b0.83160.0+2.7
−2.9
0.492vận tốc xuyên tâm74.55± 0.090.62[109]
HIP 86221b0.712.224+0.0004
−0.0005
0.031vận tốc xuyên tâm96± 110.79[109]
TOI-1842b0.214+0.040
−0.038
1.04+0.06
−0.05
9.5739+0.0002
−0.0001
0.01001± 0.0007quá cảnh729± 71.46± 0.036230± 50[110]
Gliese 367b (ja)0.0017± 0.00020.064± 0.0050.321962+0.000010
−0.000012
0.0071± 0.00021745± 43quá cảnh30.695± 0.0160.45± 0.0113522± 70[111]
HATS-74Ab1.46± 0.141.032± 0.0211.73185606± 0.000000550.02384± 0.00011895.1± 5.7quá cảnh952± 120.601± 0.0083775± 54Host star also known as TOI-737[112]
HATS-75b0.491± 0.0390.884± 0.0132.7886556± 0.00000110.032742+0.000134
−0.000099
772.3± 2.3quá cảnh640± 40.6017+0.0074
−0.0055
3812± 79Host star also known as TOI-552[112]
HATS-76b2.629± 0.0891.079± 0.0311.9416423± 0.00000140.02658+0.00021
−0.00029
939.8± 6.7quá cảnh1272± 190.662+0.016
−0.021
3990± 120Host star also known as TOI-555[112]
HATS-77b1.374+0.100
−0.074
1.165± 0.0213.0876262± 0.00000160.03607± 0.00025828.3± 5.9quá cảnh1440± 400.655± 0.0144082± 69Host star also known as TOI-730[112]
KOI-4777b0.046± 0.0030.412000± 0.0000010.0080± 0.00031180± 20quá cảnh565± 40.41± 0.023515± 69[113]
BD+60 1417b15± 51.31± 0.0616621303± 74hình ảnh trực tiếp146.65± 0.091.04993± 124Young (≈100 million years) host star[114]
b Centauri b10.9± 1.6200000± 100000556± 17hình ảnh trực tiếp325± 108± 2Circumbinary planet in unusually massive host star system[115]
HD 360 b0.75+0.12
−0.15
273.1+1.6
−0.8
0.98+0.11
−0.03
vận tốc xuyên tâm3621.69+0.15
−0.53
4770[116]
Epsilon Piscium b0.77+0.16
−0.10
255.3+2.1
−1.4
0.88+0.11
−0.10
vận tốc xuyên tâm183.21.41+1.45
−0.50
4824Planetary candidate, unconfirmed[116]
HD 10975 b0.45+0.06
−0.15
283.8+12.7
−0.1
0.95+0.06
−0.08
vận tốc xuyên tâm3791.41+0.34
−0.35
4840[116]
HD 79181 b0.64+0.06
−0.16
273.1+1.3
−0.4
0.90+0.07
−0.08
vận tốc xuyên tâm3371.28+0.32
−0.28
4862[116]
HD 99183 b0.97+0.06
−0.25
310.4+5.2
−1.7
1.08+0.05
−0.07
vận tốc xuyên tâm3551.76+0.31
−0.30
4886[116]
Upsilon Leonis b0.51+0.06
−0.26
385.2+2.8
−1.3
1.18+0.11
−0.32
vận tốc xuyên tâm177.81.48+0.90
−0.38
4836[116]
HD 161178 b0.57+0.02
−0.16
279.3+1.0
−0.8
0.85+0.05
−0.07
vận tốc xuyên tâm3511.06+0.25
−0.17
4786[116]
HD 219139 b0.78+0.05
−0.20
275.5+2.3
−1.0
0.94+0.06
−0.07
vận tốc xuyên tâm3451.46+0.31
−0.29
4831[116]
Gamma Piscium b1.34+0.02
−0.31
555.1+6.0
−2.5
1.32+0.05
−0.08
vận tốc xuyên tâm1380.99+0.17
−0.13
4742[116]
OGLE-2014-BLG-0676Lb3.68+0.69
−1.44
4.53+1.49
−2.50
thấu kính hấp dẫn8700+2500
−4600
0.73+0.14
−0.29
[117]
HD 103891 b1.44+0.06
−0.05
1919+14
−15
3.27+0.02
−0.01
vận tốc xuyên tâm179.0± 0.41.28± 0.016072± 20[118]
HD 105779 b0.64± 0.062412+55
−52
3.38± 0.05vận tốc xuyên tâm179.7± 0.30.89± 0.015792± 16[118]
HD 73583b0.253+0.014
−0.011
6.3980661+0.0000095
−0.0000097
0.05995+0.00074
−0.00072
742.7+7.2
−7.0
quá cảnh102.97± 0.100.701+0.026
−0.025
4574+62
−61
Host star also known as TOI 560[119]
HD 73583c0.2433+0.011
−0.0096
18.8805+0.0024
−0.0011
0.1233± 0.0015517.8+5
−4.9
quá cảnh102.97± 0.100.701+0.026
−0.025
4574+62
−61
Host star also known as TOI 560[119]
OGLE-2014-BLG-0319Lb0.57+0.36
−0.31
3.49+1.17
−1.12
thấu kính hấp dẫn25000+4000
−9000
0.52+0.33
−0.29
[120]
OGLE-2018-BLG-0383L b0.0201+0.0173
−0.0088
1.8± 0.2thấu kính hấp dẫn25000± 20000.10+0.13
−0.05
[121]

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  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
  6. ^ 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
  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
  8. ^ 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
  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
  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.
  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
  15. ^ 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
  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
  17. ^ 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
  18. ^ 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]. 
  19. ^ 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
  20. ^ 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
  21. ^ 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
  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
  23. ^ 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
  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
  27. ^ 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
  28. ^ 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
  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
  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
  32. ^ 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
  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
  37. ^ 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
  38. ^ 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
  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
  45. ^ 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
  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]. 
  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
  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
  53. ^ 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.
  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
  56. ^ 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
  57. ^ 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)
  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
  59. ^ 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
  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
  61. ^ 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
  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
  66. ^ 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
  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.
  68. ^ 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.
  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
  72. ^ 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
  73. ^ 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
  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
  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
  77. ^ 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
  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
  79. ^ 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
  80. ^ 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
  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
  85. ^ 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
  86. ^ 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
  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
  92. ^ 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
  93. ^ 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
  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
  95. ^ 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
  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
  99. ^ 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
  100. ^ 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
  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
  102. ^ 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
  103. ^ 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
  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
  107. ^ 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
  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
  109. ^ 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
  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
  112. ^ 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
  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
  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
  118. ^ 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
  119. ^ 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
  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
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