Danh sách ngoại hành tinh được phát hiện năm 2021

Bách khoa toàn thư mở Wikipedia

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]

Tên Khối lượng (MJ) Bán kính (RJ) 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 MJ 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]

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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