This list of exoplanets discovered in 2021 is a list of confirmed exoplanets that were first observed in 2021. For exoplanets detected only by radial velocity, the listed value for mass is a lower limit. See Minimum mass for more information.

Name Mass (MJ) Radius (RJ) Period (days) Semi-major axis (AU) Temp. (K) Discovery method Distance (ly) Host star mass (M☉) Host star temp. (K) Remarks
2M0437 b 4±1 1.16 1,136,000 115 1,450±50 imaging 417.9±1.5 0.165±0.015 3,100 Gas giant also known as 2MASSJ04372171 b[1][2][3]
b Centauri b 10.9±1.6 200000±100000 556±17 imaging 325±10 8±2 Circumbinary planet in unusually massive host star system[4]
BD+45 0564 b 1.36±0.12 307.88±1.47 0.83±0.04 radial vel. 174±2 0.81±0.07 5,004±50 [5]
BD+55 0362 b 0.72±0.08 265.59±1.04 0.78±0.05 radial vel. 168±2 0.909±0.099 5,012±78 Additional giant planet is suspected[5]
BD+60 1417b 15±5 1.31±0.06 1662 1303±74 imaging 146.65±0.09 1.0 4993±124 Young (≈100 million years) host star[6]
BD+63 1405 b 3.96±0.31 1,198.48±60.79 2.06±0.14 radial vel. 124.4±1.2 0.82±0.08 5,000±53 Extremely eccentric orbit[5]
Candidate 1 0.062-0.157 0.3011-0.6386 imaging 4.37 Imaged near Alpha Centauri A
EPIC 201427007 b 0.0090 0.134±0.018 0.72091±0.000067 transit 2304±55 0.930 5633±111 [7][8]
EPIC 201595106 b 0.00705 0.116±0.009 0.877214±0.000087 transit 762±9 5820±20 Candidate since 2018[7][9]
EPIC 211314705.01 0.139±0.007 3.793306+0.000324
−0.000343		 543+8
−9		 transit 300.0±1.7 0.43±0.01 3,669+88
−82		 [10] Two more planets in system are suspected.[11]
EPIC 211401787.01 0.247+0.013
−0.008		 13.774798+0.000028
−0.000028		 969±9 transit 525±5 1.23±0.02 6,232+33
−39		 [10] Host star also known as BD+12 1842.
EPIC 211502222.01 0.243+0.013
−0.009		 22.996591+0.001848
−0.001859		 673+12
−11		 transit 694±6 1.10+0.03
−0.04		 5,994+93
−91		 [10]
EPIC 211502222.02 0.160+0.013
−0.009		 9.398977+0.001506
−0.001348		 909±14 transit 694±6 1.10+0.03
−0.04		 5,994+93
−91		 [10]
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		 transit 0.96+0.05
−0.06		 5,790+177
−147		 [12]
EPIC 211537087.01 0.204+0.013
−0.011		 21.0267366+0.0036912
−0.0038993		 0.1599+0.0178
−0.0306		 624+0
−37		 transit 0.90+0.05
−0.06		 5,568+178
−150		 [12]
EPIC 211579112.01 0.196+0.017
−0.014		 17.706320±0.000063 266+5
−8		 transit 403±5 0.27+0.01
−0.02		 3,315+137
−152		 [10]
EPIC 211647930.01 0.552+0.025
−0.022		 14.759287+0.000243
−0.000240		 826+14
−17		 transit 1,133±17 1.06±0.04 5,880+85
−82		 [10]
EPIC 211730024.01 0.504+0.032
−0.025		 5.113981+0.000061
−0.000062		 1,380+34
−30		 transit 1,226±21 1.36±0.05 6,502+132
−130		 [10]
EPIC 211730267.01 0.332+0.021
−0.019		 16.3488637+0.0013811
−0.0014022		 0.1450+0.0136
−0.0235		 735+8
−39		 transit 0.98±0.07 5,794+210
−169		 [12]
EPIC 211743874.01 0.197+0.016
−0.013		 12.283211±0.000051 949+21
−26		 transit 1,850±60 1.23±0.04 6,222+96
−91		 [10]
EPIC 211763214.01 0.109+0.008
−0.005		 21.194733+0.000108
−0.000107		 569+15
−22		 transit 786±9 0.86+0.03
−0.05		 5,424+192
−144		 [10]
EPIC 211770696.01 0.234+0.017
−0.013		 16.273563+0.000054
−0.000053		 850+19
−18		 transit 1,390±30 0.94+0.04
−0.03		 5,869+88
−81		 [10]
EPIC 211779390.01 0.092+0.010
−0.005		 3.850614±0.000012 783+12
−14		 transit 514±2 0.66±0.02 4,558+91
−81		 [10]
EPIC 211897691.02 0.171+0.017
−0.011		 19.507428+0.000116
−0.000113		 508±12 transit 1,187±17 0.74+0.04
−0.03		 4,857+86
−84		 [10]
EPIC 211914998.01 0.239+0.015
−0.013		 11.2510285+0.0018188
−0.0017892		 0.0863+0.0079
−0.0159		 888+0
−47		 transit 0.93±0.06 5,650+193
−152		 [12]
EPIC 211923431.01 0.300+0.039
−0.029		 29.740451+0.000169
−0.000161		 606+31
−36		 transit 2,460±70 0.93±0.04 5,532±90 [10]
EPIC 211978988.01 0.287+0.022
−0.017		 36.552551+0.000127
−0.000122		 598+16
−15		 transit 1,390±20 0.98±0.07 5,817+45
−48		 [10]
EPIC 212058012.01 0.181+0.012
−0.008		 11.561052+0.000690
−0.000668		 861+14
−15		 transit 684±6 1.01±0.05 5,920±104 [10]
EPIC 212072539.01 0.180+0.009
−0.006		 7.676972+0.000012
−0.000012		 465±7 transit 545±3 0.49±0.01 3,804+93
−74		 [10]
EPIC 212072539.02 0.147+0.015
−0.007		 2.787174±0.000004 653+10
−12		 transit 545±3 0.49±0.01 3,804+93
−74		 [10]
EPIC 212081533.01 0.142+0.009
−0.004		 3.355850+0.000091
−0.000093		 722+7
−10		 transit 245.8 0.51±0.01 4,374+38
−34		 [10]
EPIC 212088059.01 0.188+0.018
−0.008		 10.367437+0.000020
−0.000019		 437+4
−5		 transit 532±3 0.56±0.01 3,779+30
−26		 [10]
EPIC 212132195.01 0.202+0.017
−0.009		 26.201446+0.003331
−0.003124		 450±5 transit 345.5±1.6 0.71±0.02 4,801±49 [10]
EPIC 212161956.01 0.215+0.010
−0.009		 7.187257+0.000020
−0.000021		 640+20
−21		 transit 1055±13 0.66±0.03 4,599+178
−152		 [10]
EPIC 212204403.01 0.291+0.020
−0.010		 4.688418+0.000119
−0.000117		 908+12
−11		 transit 662±5 0.83+0.02
−0.01		 5,077+40
−39		 [10]
EPIC 212204403.02 0.238+0.021
−0.010		 12.550171+0.001018
−0.001057		 655+7
−9		 transit 662±5 0.83+0.02
−0.01		 5,077+40
−39		 [10]
EPIC 212420823.01 0.123+0.009
−0.006		 9.032178±0.000874 518+5
−4		 transit 1,450±20 0.54±0.01 4,385+29
−31		 [10]
EPIC 212440430.02 0.138+0.013
−0.010		 4.163873+0.000022
−0.000023		 1,158+29
−34		 transit 1,620±20 0.98±0.02 5,789+46
−50		 [10]
EPIC 212543933.01 0.227+0.023
−0.017		 7.806164+0.000673
−0.000623		 934+28
−32		 transit 1,310±50 1.02±0.02 5,769+39
−37		 [10]
EPIC 212624936 b 0.00589 0.517+0.098
−0.027		 0.578657±0.000066 transit 5765±170 [7] Host star TYC 5557-667-1[13]
EPIC 212624936 c 0.019 0.214+0.098
−0.057		 11.811437±0.00016 transit 5765±170 [7] Host star TYC 5557-667-1[14]
EPIC 220492298 b 0.00295 0.085±0.018 0.762406±0.00014 transit 5620±31 [7][15]
EPIC 228836835 b 0.00431 0.089±0.027 0.728113±0.00004 transit 491±6 3782±152 [7][16]
EPIC 251319382.01 0.171+0.012
−0.006		 8.234885+0.000508
−0.000475		 885+12
−14		 transit 577±6 0.95±0.02 5,791±81 [10]
EPIC 251319382.02 0.199+0.012
−0.008		 14.871387+0.000916
−0.000936		 727±10 transit 577±6 0.95±0.02 5,791±81 [10]
EPIC 251319382.03 0.122+0.009
−0.006		 3.665912+0.000273
−0.000295		 1,160+16
−15		 transit 577±6 0.95±0.02 5,791±81 [10]
EPIC 251554286.01 0.496+0.020
−0.018		 15.466805+0.000572
−0.000565		 735+13
−14		 transit 883±12 0.87±0.02 5,698±55 [10]
Epsilon Piscium b 0.77+0.16
−0.10		 255.3+2.1
−1.4		 0.88+0.11
−0.10		 radial vel. 183.2 1.41+1.45
−0.50		 4824 Planetary candidate, unconfirmed[17]
G 264-12 b 0.0079±0.0009 2.30538±0.00031 0.02279±0.00061 587±16 radial vel. 52.14±0.03 0.297±0.024 3,326±54 [18]
G 264-12 c 0.0118±0.0015 8.0518±0.0034 0.0525±0.0014 387±11 radial vel. 52.14±0.03 0.297±0.024 3,326±54 [18]
Gamma Piscium b 1.34+0.02
−0.31		 555.1+6.0
−2.5		 1.32+0.05
−0.08		 radial vel. 138 0.99+0.17
−0.13		 4742 [17]
Gliese 146 b 0.0175+0.0023
−0.0021		 5.09071 ± 0.00026 0.0510+0.0024
−0.0026		 573+63
−69		 radial vel. 44.37±0.01 0.684±0.013 4,385±21 Host star also known as HD 22496.[19]
Gliese 367b 0.0017±0.0002 0.064±0.005 0.321962+0.000010
−0.000012		 0.0071±0.0002 1745±43 transit 30.695±0.016 0.45±0.011 3522±70 [20]
Gliese 393 b 0.0054±0.0008 7.02679+0.00082
−0.00085		 0.05402±0.00072 485±11 radial vel. 22.956±0.008 0.426±0.017 3,579±51 [18]
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 transit 26.344±0.013 0.323±0.015 3,340±54 Planet may have a measurable atmosphere[21]
Gliese 740 b 0.0093±0.0016 2.37756+0.00013
−0.00011		 0.029±0.001 829+40
−50		 radial vel. 36.21±0.02 0.58±0.06 3,913±21 [22]
Gliese 9689 b 0.0304±0.0046 18.27±0.01 0.1139±0.0039 453±39 radial vel. 100.10±0.04 0.59±0.06 3,836±69 [23]
HAT-P-58b 0.372±0.03 1.332±0.043 4.0138379±0.0000024 0.04994±0.00044 1622±18 transit 1690±40 1.031±0.028 6078±48 [24]
HAT-P-59b 1.540±0.067 1.123±0.013 4.1419771±0.0000012 0.05064±0.00037 1278±7 transit 871±4 1.008±0.022 5678±16 [24]
HAT-P-60b 0.574±0.038 1.631±0.024 4.7947813±0.0000024 0.06277±0.00017 1772±12 transit 767±7 1.435±0.012 6212±26 [24]
HAT-P-61b 1.057±0.07 0.899±0.027 1.90231289±0.00000077 0.03010±0.00034 1505±16 transit 1120±20 1.004±0.012 5587±45 [24]
HAT-P-62b 0.761±0.088 1.073±0.029 2.6453235±0.0000039 0.03772±0.00024 1512±13 transit 1150±20 1.023±0.020 5629±48 [24]
HAT-P-63b 0.614±0.024 1.119±0.033 3.377728±0.000013 0.04294±0.00035 1237±11 transit 1330±20 0.925±0.023 5400+55
−39		 [24]
HAT-P-64b 0.58+0.18
−0.13		 1.703±0.07 4.0072320±0.0000017 0.05387±0.00030 1766+22
−16		 transit 2135±20 1.298±0.021 6457+55
−36		 [24]
HATS-74Ab 1.46±0.14 1.032±0.021 1.73185606±0.00000055 0.02384±0.00011 895.1±5.7 transit 952±12 0.601±0.008 3775±54 Host star also known as TOI-737[25]
HATS-75b 0.491±0.039 0.884±0.013 2.7886556±0.0000011 0.032742+0.000134
−0.000099		 772.3±2.3 transit 640±4 0.6017+0.0074
−0.0055		 3812±79 Host star also known as TOI-552[25]
HATS-76b 2.629±0.089 1.079±0.031 1.9416423±0.0000014 0.02658+0.00021
−0.00029		 939.8±6.7 transit 1272±19 0.662+0.016
−0.021		 3990±120 Host star also known as TOI-555[25]
HATS-77b 1.374+0.100
−0.074		 1.165±0.021 3.0876262±0.0000016 0.03607±0.00025 828.3±5.9 transit 1440±40 0.655±0.014 4082±69 Host star also known as TOI-730[25]
HD 360 b 0.75+0.12
−0.15		 273.1+1.6
−0.8		 0.98+0.11
−0.03		 radial vel. 362 1.69+0.15
−0.53		 4770 [17]
HD 3765 b 0.173+0.014
−0.013		 1,211+15
−16		 2.108+0.032
−0.033		 radial vel. 78.5±0.1 [26]
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 transit 183.1±2.7 1.126+0.036
−0.035		 6,203±64 Host star also known as TOI-130.[27]
HD 5278 c 0.0579+0.0057
−0.0060		 0.2416±0.0027 0.1202±0.0013 943±13 radial vel. 183.1±2.7 1.126+0.036
−0.035		 6,203±64 Host star also known as TOI-130.[27]
HD 10975 b 0.45+0.06
−0.15		 283.8+12.7
−0.1		 0.95+0.06
−0.08		 radial vel. 379 1.41+0.34
−0.35		 4840 [17]
HD 13808 b 0.0346 14.2 0.11 radial vel. 92.2 0.771±0.022 5,035±50 Candidate since 2011,[28] confirmed in 2021[29]
HD 13808 c 0.0315 53.8 0.26 radial vel. 92.2 0.771±0.022 5,035±50 Candidate since 2011,[28] confirmed in 2021[29]
HD 19615 b 8.5±0.7 402±2 1.1±0.1 radial vel. 872±7 1.1±0.1 3987±125 Red giant host star[30]
HD 24040 c 0.201±0.027 515.4+2.2
−2.5		 1.3±0.021 radial vel. 152.3±0.4 1.14±0.02 5,917±52 [26]
HD 26161 b 13.5+8.5
−3.7		 32,000+21,000
−10,000		 20.4+7.9
−4.9		 radial vel. 133.6±0.3 Very eccentric orbit, and also red dwarf in the system[26]
HD 27969 b 4.80+0.24
−0.23		 654.5+5.7
−5.8		 1.552+0.032
−0.033		 261±11 radial vel. 1.16±0.07 5,966±21 [31]
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		 transit 372.5±1.1 1.316±0.027 6,394±75 Host star also known as TOI-201[32]
HD 63935 b 0.0340±0.0057 0.267±0.013 9.058811+0.000017
−0.000016		 911±27 transit 159.36±0.15 0.933±0.054 5,534±100 [33]
HD 63935 c 0.0349±0.0076 0.259±0.012 21.4023+0.00189
−0.00194		 684±21 transit 159.36±0.15 0.933±0.054 5,534±100 [33]
HD 66428 c 27+22
−17		 39,000+56,000
−18,000		 23.0+19.0
−7.6		 radial vel. 174.1±0.7 1.09±0.02 5,773±55 [26]
HD 68988 c 15.0+2.8
−1.5		 16,100+11,000
−3,500		 13.2+5.3
−2.0		 radial vel. 198.8±0.6 1.16±0.01 5,919±11 Suspected since 2006[26]
HD 73583 b 0.0315±0.0098 0.253±0.009 6.3980418+0.0000065
−0.0000063		 0.0601±0.0026 721±21 transit 103.08±0.10 0.71±0.02 4511±110 Host star also known as TOI-560,[34] planetary helium emission detected.[35]
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		 transit 102.97±0.10 0.701+0.026
−0.025		 4574+62
−61		 Host star also known as TOI 560[36]
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 transit 103.08±0.10 0.71±0.02 4511±110 Host star also known as TOI-560[34]
HD 73583c 0.2433+0.011
−0.0096		 18.8805+0.0024
−0.0011		 0.1233±0.0015 517.8+5
−4.9		 transit 102.97±0.10 0.701+0.026
−0.025		 4574+62
−61		 Host star also known as TOI 560[36]
HD 79181 b 0.64+0.06
−0.16		 273.1+1.3
−0.4		 0.90+0.07
−0.08		 radial vel. 337 1.28+0.32
−0.28		 4862 [17]
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		 radial vel. 1.08±0.05 5,837±15 Very eccentric orbit[31]
HD 95544 b 6.84±0.31 2172+23
−21		 3.386+0.075
−0.077		 156.5+5.4
−5.5		 radial vel. 1.09±0.07 5,722±15 [31]
HD 99183 b 0.97+0.06
−0.25		 310.4+5.2
−1.7		 1.08+0.05
−0.07		 radial vel. 355 1.76+0.31
−0.30		 4886 [17]
HD 107148 c 0.0626+0.0097
−0.0098		 18.3267+0.0022
−0.0024		 0.1406±0.0018 radial vel. 161.4±0.4 1.1±0.1 5,789±36 [26]
HD 108236 f 0.17406+0.00482
−0.00437		 29.54255±0.00069 0.1759±0.0037 transit 211 0.853±0.047 5,720.0±50.0 [37][38]
HD 109286 b 2.99±0.15 520.1±2.3 1.259±0.021 259.4±5.5 radial vel. 0.98±0.05 5,694±23 [31]
HD 103891 b 1.44+0.06
−0.05		 1919+14
−15		 3.27+0.02
−0.01		 radial vel. 179.0±0.4 1.28±0.01 6072±20 [39]
HD 105779 b 0.64±0.06 2412+55
−52		 3.38±0.05 radial vel. 179.7±0.3 0.89±0.01 5792±16 [39]
HD 110082 b 0.2857±0.0089 10.18271±0.00004 0.113+0.009
−0.013		 transit 342.8±0.9 1.21±0.06 6,200±100 Orbiting a primary of wide binary system[40] Host star also known as TOI-1098.
HD 110113 b 0.0143±0.0020 0.183±0.011 2.541+0.0005
−0.001		 0.035±0.001 1,371±14 transit 346.5±2.3 0.99±0.08 5,730 Radius gap planet, host star also known as TOI-755[41]
HD 110113 c 0.0330±0.0038 6.744+0.008
−0.009		 0.068+0.001
−0.002		 990±10 radial vel. 346.5±2.3 0.99±0.08 5,730 Host star also known as TOI-755.[41]
HD 115954 b 8.29+0.75
−0.58		 3700+1500
−390		 5.00+1.3
−0.36		 144.9+8.1
−13		 radial vel. 1.18±0.06 5957±26 [31]
HD 124330 b 0.75±0.06 270.66±1.21 0.86±0.04 radial vel. 198±3 1.15±0.079 5,873±19 Additional giant planet is suspected[5]
HD 136925 b 0.84+0.078
−0.074		 4,540+160
−140		 5.13+0.12
−0.11		 radial vel. 156.2 5715 Additional planet suspected[26]
HD 137496 b 0.0127±0.0017 0.117±0.005 1.62116±0.00008 0.02732±0.00019 2130+30
−29		 transit 509±6 1.035±0.022 5799±61 [42]
HD 137496 c 7.66±0.11 479.9+1.1
−1.0		 1.2163+0.0087
−0.0088		 370±5 radial vel. 509±6 1.035±0.022 5799±61 [42]
HD 150010 b 2.4±0.4 562±8 1.1±0.1 radial vel. 473.4±2.1 1.3±0.1 4256±125 Red giant host star[30]
HD 152843 b 0.0364+0.0207
−0.0193		 0.304±0.012 11.6264+0.0022
−0.0025		 0.1053+0.003
−0.0031		 transit 352.0±1.0 1.15±0.04 6,310±100 [43]
HD 152843 c 0.0865 0.521±0.013 24.38+6.23
−3.4		 transit 352.0±1.0 1.15±0.04 6,310±100 [43]
HD 155193 b 0.75±0.06 352.65±2.58 1.04±0.04 radial vel. 186±6 1.221±0.083 6,239±20 [5]
HD 156668 c 0.0991+0.0079
−0.0077		 811.3+5.2
−5.3		 1.570±0.017 radial vel. 79.34±0.03 0.772±0.020 4,850±88 Additional body in system is suspected[26]
HD 161178 b 0.57+0.02
−0.16		 279.3+1.0
−0.8		 0.85+0.05
−0.07		 radial vel. 351 1.06+0.25
−0.17		 4786 [17]
HD 164922 e 0.0331±0.0031 41.763±0.012 0.2293+0.0026
−0.0027		 radial vel. 71.69±0.03 0.874±0.012 5,293±32 [26]
HD 168009 b 0.0300+0.0038
−0.0037		 15.1479+0.0035
−0.0037		 0.1192+0.0017
−0.0018		 radial vel. 75.97±0.03 0.99 5,792±80 [26]
HD 174205 b 4.2±0.5 582±17 1.7±0.1 radial vel. 769±5 1.8±0.1 4393±125 Red giant host star[30]
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		 transit 186.1±0.8 1.031+0.025
−0.026		 5,788±44 Host star also known as TOI-1055[44][45][46]
HD 191939 e >0.3531±0.0126 101.12±0.13 0.4007±0.012 390±8 radial vel. 175.1±0.2 0.92 5400 Also suspected brown dwarf on wider orbit[47][48]
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		 transit 92.15±0.10 0.80+0.036
−0.030		 5,070+60
−57		 [49]
HD 211403 b 5.54+0.39
−0.38		 223.8±0.41 0.768±0.013 380±13 radial vel. 1.20±0.06 6,273±44 [31]
HD 213472 b 3.48+1.10
−0.59		 16,700+12,000
−4,800		 13.0+5.7
−2.6		 radial vel. 210.6 [26]
HD 219139 b 0.78+0.05
−0.20		 275.5+2.3
−1.0		 0.94+0.06
−0.07		 radial vel. 345 1.46+0.31
−0.29		 4831 [17]
HD 331093 b 1.50±0.11 621.62±16.11 1.44±0.07 radial vel. 164.07±0.14 1.030±0.079 5,544±33 [5]
HIP 5763b 0.51 30.014+0.1528
−0.2842		 0.170 radial vel. 104.17±0.14 0.72 [50]
HIP 34222b 0.83 160.0+2.7
−2.9		 0.492 radial vel. 74.55±0.09 0.62 [50]
HIP 56640 b 7.1±1.6 2574.9±86.1 3.73±0.08 radial vel. 400.4±1.9 1.04+0.07
−0.06		 4769±55 Red giant host star also known as HD100939b[51][52]
HIP 86221b 0.71 2.224+0.0004
−0.0005		 0.031 radial vel. 96±11 0.79 [50]
HIP 90988 b 2.102+0.079
−0.085		 455.73816+2.11413
−1.88939		 1.26±0.01 radial vel. 307.6±1.2 1.30±0.08 4884±58 Gas giant orbiting a red giant host star also known as HD 170707[53][52][54]
HIP 97166b 0.0629±0.047 0.245±0.012 10.28891±0.00004 0.089±0.001 757±25 transit 215.54±0.33 0.898±0.054 5,198±100 [55]
HIP 97166c 9.9±1.8 16.84±0.22 0.124±0.002 642±22 radial vel. 215.54±0.33 0.898±0.054 5,198±100 [55]
K2-99c 8.4±0.2 522.2±1.4 1.43±0.01 390±6 radial vel. 1980 1.6 5990 [56]
K2-268d 0.133+0.013
−0.006		 4.528598+0.000016
−0.000015		 888+16
−15		 transit 1,079±10 0.84±0.02 5,106+70
−61		 Two more planets were previously known; host star also known as EPIC 211413752.[10]
K2-268e 0.119+0.010
−0.007		 6.131243+0.000032
−0.000033		 801±13 transit 1,079±10 0.84±0.02 5,106+70
−61		 Two more planets were previously known; host star also known as EPIC 211413752.[10]
K2-268f 0.199+0.013
−0.008		 26.270570+0.000105
−0.000109		 492+8
−10		 transit 1,079±10 0.84±0.02 5,106+70
−61		 Two more planets were previously known; host star also known as EPIC 211413752.[10]
K2-185c 0.213±0.008 52.713494+0.000155
−0.000164		 477+14
−17		 transit 882±11 0.96+0.05
−0.07		 5,788+190
−157		 Host star also known as EPIC 211611158.[10]
K2-304c 0.203+0.017
−0.011		 5.213965±0.000442 866+27
−37		 transit 1,380±20 0.83+0.05
−0.04		 5,171+172
−130		 Host star also known as EPIC 212297394.[10]
K2-307c 0.207+0.017
−0.011		 23.228555+0.000068
−0.000071		 658+13
−14		 transit 1,050±20 0.99+0.03
−0.04		 6,004+77
−78		 Host star also known as EPIC 212587672.[10]
Kepler-129d 8.3+1.1
−0.7		 2646+140
−94		 4.0±0.1 radial vel. 1,349±14 1.18 5,770 [57]
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		 transit 2,690±40 1.131+0.040
−0.051		 5,745+88
−89		 Very eccentric orbit (e=0.921),[58]
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		 [59]
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		 [59]
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		 [59]
KMT-2016-BLG-2605b 0.8+1.2
−0.4		 0.68±0.11 microlensing 21,000±3,000 0.065+0.10
−0.035		 [60]
KMT-2017-BLG-2509b 2.09+1.68
−1.26		 2.14+0.27
−0.39		 microlensing 23,000±3,000 0.46+0.37
−0.27		 [61]
KMT-2018-BLG-1025Lb 0.0191+0.0258
−0.0104		 1.305+0.194
−0.227		 microlensing 22,000±3,000 0.219+0.297
−0.120		 Multiple solutions for orbital parameters[62]
KMT-2018-BLG-1743 0.245+0.339
−0.135		 1.449+0.209
−0.229		 microlensing 21,000±3,000 0.193+0.268
−0.107		 Multiple orbital solutions, binary host star[63]
KMT-2018-BLG-1976Lb 1.96+1.23
−1.12		 2.04+0.72
−0.83		 microlensing 19,000±2,000 0.65+0.41
−0.37		 [64]
KMT-2018-BLG-1996Lb 1.22+0.72
−0.63		 1.97+0.51
−0.25		 microlensing 19,000±2,000 0.69+0.40
−0.38		 [64]
KMT-2018-BLG-1988Lb 0.021+0.015
−0.011		 2.83+1.23
−0.97		 microlensing 14000+6000
−5000		 0.48+0.33
−0.25		 Multiple solutions for orbital parameters[65]
KMT-2019-BLG-0371b 7.70+11.34
−3.90		 0.79+0.14
−0.16		 microlensing 2,3000+3,000
−4,000		 0.09+0.14
−0.05		 Multiple solutions for orbital separation[66]
KMT-2019-BLG-0253b 0.029+0.016
−0.013		 3.1+0.8
−0.9		 microlensing 16,000+6,000
−5,000		 0.70+0.34
−0.31		 [67]
KMT-2019-BLG-1715 2.56+1.13
−1.16		 3.32+0.82
−0.92		 microlensing 13,000±3,000 0.61+0.27
−0.28		 Multiple solutions for orbital separation, also 0.15M☉ red dwarf in the system.[68]
KMT-2020-BLG-0414Lb 0.0032 0.15 microlensing 3,300±300 0.3 Also a brown dwarf with mass 17 MJ in the system at 15 AU separation[69]
KMT-2021-BLG-0912Lb 0.022+0.007
−0.008		 3.03+3.46
−2.46		 microlensing 22000±3000 0.75+0.23
−0.28		 Multiple solutions for orbital parameters[70]
KOI-5Ab 0.179 0.63 5 transit 1,870±70 1.13 5861 Also called TOI-1241b.[71][72]
KOI-984b 0.0544±0.0094 0.384±0.004 4.2881785±0.0000035 0.0504±0.0006 1022+31
−30		 transit 749±4 0.928±0.031 5295±150 Another planet in system on poorly constrained orbit[73]
KOI-4777b 0.046±0.003 0.412000±0.000001 0.0080±0.0003 1180±20 transit 565±4 0.41±0.02 3515±69 [74]
Lalande 21185 c 0.0568+0.0091
−0.0083		 3190+200
−170		 3.1+0.13
−0.11		 radial vel. 8.31±0.01 0.390±0.011 3,601±51 [26]
Lambda Serpentis b 0.0428+0.0047
−0.0045		 15.5083+0.0016
−0.0018		 0.1238±0.002 radial vel. 38.87±0.07 1.14 5,884±4 [26]
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		 transit 59.40±0.03 0.236±0.012 3,381±54 [75] Host star also known as TOI-1640 or G 245-61.
LHS 1678 b 0.0002±0.0003 0.062±0.004 0.8602322+0.0000068
−0.0000048		 0.01251+0.00059
−0.00056		 transit 64.88±0.03 0.345±0.014 3490±50 [76]
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		 transit 64.88±0.03 0.345±0.014 3490±50 [76]
LTT 1445 Ac 0.0048±0.0006 0.103 3.12390 0.02661+0.00047
−0.00049		 transit 22.41±0.01 0.256±0.014 3337±150 [77]
Luyten 98-59 e 0.0094 12.8 0.071 342+20
−18		 radial vel. 34.6 0.32±0.03 3500±150 [78]
Luyten 98-59 f 0.0078 23.2 0.103 285+18
−17		 radial vel. 34.6 0.32±0.03 3500±150 Unconfirmed, potentially habitable exoplanet[78]
NGTS-13b 4.84±0.44 1.142±0.046 4.12 0.0549+0.0015
−0.0025		 1,605±30 transit 2150 1.30+0.11
−0.18		 5,819±73 [79]
NGTS-14Ab 0.092±0.012 0.444±0.030 3.5357173±0.0000069 0.0403±0.0071 1,143±139 transit 1,060 0.898±0.035 5,187±11 [80]
NGTS-15b 0.751+0.102
−0.088		 1.10±0.10 3.27623±0.00001 0.0441±0.0046 1,146±47 transit 2,580±60 0.995±0.015 5,600±150 [81]
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 transit 2,910+95
−75		 1.002±0.011 5,550±150 [81]
NGTS-17b 0.764+0.195
−0.164		 1.24±0.11 3.24253±0.00001 0.0391±0.0043 1,457±50 transit 3,420±90 1.025+0.015
−0.014		 5,650±100 [81]
NGTS-18b 0.409+0.081
−0.063		 1.21±0.18 3.05125±0.00001 0.0448±0.0068 1,381+55
−53		 transit 3,610±140 1.003+0.020
−0.012		 5,610±150 [81]
OGLE-2014-BLG-0319Lb 0.57+0.36
−0.31		 3.49+1.17
−1.12		 microlensing 25000+4000
−9000		 0.52+0.33
−0.29		 [82]
OGLE-2014-BLG-0676Lb 3.68+0.69
−1.44		 4.53+1.49
−2.50		 microlensing 8700+2500
−4600		 0.73+0.14
−0.29		 [83]
OGLE-2017-BLG-1099b 3.02+2.43
−1.81		 2.73+0.40
−0.53		 microlensing 24,000±3,000 0.45+0.36
−0.27		 [61]
OGLE-2018-BLG-0383L b 0.0201+0.0173
−0.0088		 1.8±0.2 microlensing 25000±2000 0.10+0.13
−0.05		 [84]
OGLE-2018-BLG-0506 0.051+0.038
−0.027		 3.0+0.7
−0.8		 microlensing 18,000±5,000 0.63+0.37
−0.32		 [67]
OGLE-2018-BLG-0516 0.063+0.052
−0.034		 2.2+0.8
−0.7		 microlensing 7,000+3,000
−2,000		 0.47+0.38
−0.25		 [67]
OGLE-2018-BLG-0567Lb 0.32+0.34
−0.16		 2.72+0.49
−0.55		 microlensing 23,000±3,000 0.24+0.16
−0.13		 [85]
OGLE-2018-BLG-0962Lb 1.37+0.80
−0.72		 3.57+0.68
−1.02		 microlensing 21,000+3,000
−5,000		 0.55+0.32
−0.29		 [85]
OGLE-2018-BLG-0977 0.020+0.016
−0.012		 2.0+0.6
−0.5		 microlensing 7,000±2,000 0.47+0.38
−0.27		 [67]
OGLE-2018-BLG-1428Lb 0.77+0.77
−0.53		 3.30+0.59
−0.83		 microlensing 20,000+3,000
−5,000		 0.43+0.33
−0.22		 [86]
OGLE-2019-BLG-0299b 6.22+3.80
−3.67		 2.80+0.58
−0.89		 microlensing 19,000±4,000 0.59+0.36
−0.35		 [61]
OGLE-2019-BLG-0468Lb 3.43+1.83
−1.17		 3.29+4.15
−2.52		 microlensing 14000±3000 0.92+0.49
−0.32		 Multiple solutions for orbital parameters[87]
OGLE-2019-BLG-0468Lc 10.22+5.46
−3.50		 2.77+3.49
−2.12		 microlensing 14000±3000 0.92+0.49
−0.32		 Multiple solutions for orbital parameters[87]
OGLE-2019-BLG-0954Lb 14.2+9.9
−7.5		 2.65+0.89
−1.20		 microlensing 12,000+1,000
−2,000		 0.80+0.55
−0.42		 [64]
OGLE-2019-BLG-0960Lb 0.0071±0.0027 1.75±0.55 microlensing 2,900±1000 0.45±0.15 Smallest planet discovered by microlensing[88]
OGLE-2019-BLG-1053Lb 0.0078+0.0037
−0.0031		 3.4±0.5 microlensing 22,000+3,000
−2,000		 0.61+0.29
−0.24		 [89]
OGLE-2019-BLG-1058 6.836±6.027 microlensing 8,000±5,000 Multiple solutions, rogue planet[90]
OGLE-2018-BLG-1185b 0.026+0.025
−0.015		 1.54+0.18
−0.22		 microlensing 24,000+2,000
−3,000		 0.37+0.35
−0.21		 Multiple solutions for planet and star masses.[91]
OGLE-2019-BLG-1492 0.117+0.079
−0.061		 2.7±0.9 microlensing 18,000+6,000
−7,000		 0.68±0.34 [67]
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[92]
TIC 172900988 b 2.84±0.25 1.009±0.043 196.5±7.7 transit 799±9 1.24 and 1.20 6050 and 5983 Circumbinary planet[93]
TIC 257060897b 0.67±0.03 1.49±0.04 3.660028±0.000006 0.051±0.002 1,762±21 transit 1,655±8 1.32±0.04 6,128±57 [94]
TOI-178b 0.0047+0.0012
−0.0013		 0.102±0.006 1.914558±0.000018 0.02607±0.00078 1,040+22
−21		 transit 205.16±0.03 0.650+0.027
−0.029		 4,316±70 [95]
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 transit 205.16±0.03 0.650+0.027
−0.029		 4,316±70 [95]
TOI-178d 0.0094+0.0025
−0.0032		 0.229±0.006 6.557700±0.000016 0.0592±0.0018 690±14 transit 205.16±0.03 0.650+0.027
−0.029		 4,316±70 [95]
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 transit 205.16±0.03 0.650+0.027
−0.029		 4,316±70 [95]
TOI-178f 0.0242+0.0052
−0.0047		 0.204±0.009 15.231915+0.000115
−0.000095		 0.1039±0.0031 521±11 transit 205.16±0.03 0.650+0.027
−0.029		 4,316±70 [95]
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 transit 205.16±0.03 0.650+0.027
−0.029		 4,316±70 [95]
TOI-220 b 0.0434±0.0031 0.271±0.013 10.695264 0.08911±0.0010 805±21 transit 290±13 0.825±0.028 5,298±65 Additional long-period planet suspected[96]
TOI-269 b 0.0277±0.0044 0.247±0.011 3.697723+0.000018
−0.000017		 0.0345±0.0015 531±25 transit 186.01±0.25 0.3917±0.0095 3,514±70 [97]
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 transit 106.37±0.03 0.78±0.07 4,850±75 Host star lso known as CD-26 2288 or HIP 26013.[98]
TOI-431 c 0.0089+0.0013
−0.0011		 4.8494+0.0003
−0.0002		 0.0052±0.001 867±20 radial vel. 106.37±0.03 0.78±0.07 4,850±75 Host star also known as CD-26 2288 or HIP 26013.[98]
TOI-431 d 0.0312±0.0047 0.294±0.008 12.46103±0.00002 0.098±0.002 633±14 transit 106.37±0.03 0.78±0.07 4,850±75 Host star lso known as CD-26 2288 or HIP 26013.[98]
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		 transit 405.1±1.3 0.94±0.025 5,550±56 Planets orbiting primary of wide binary system.[99][100] 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		 transit 405.1±1.3 0.94±0.025 5,550±56 Planets orbiting primary of wide binary system.[99][100] 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		 transit 405.1±1.3 0.94±0.025 5,550±56 Planets orbiting primary of wide binary system[99][100] Host star also known as CD-38 1467.
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		 transit 482±2 0.53±0.02 3,659±120 [101]
TOI-532b 0.1935+0.0305
−0.0293		 0.520±0.017 2.3266508±0.0000030 0.0296±0.00035 867±18 transit 439.1±1.2 0.639±0.023 3927±37 Neptunian desert planet[102]
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		 transit 1,312±17 1.349+0.064
−0.065		 6,466+95
−93		 [103]
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		 transit 761±7 1.026±0.057 5,925+85
−76		 [103]
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		 transit 582 1.311+0.066
−0.075		 6,250+220
−190		 Host star also known as HD 288842[104]
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		 transit 1,115 1.536+0.069
−0.076		 6,460+130
−150		 [104]
TOI-674b 0.0739±0.0104 0.470±0.016 1.977143±0.000003 0.0231±0.0007 661±14 transit 150.86±0.11 0.442±0.007 3,505+28
−32		 [105] Possibly steam atmosphere[106]
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		 transit 191.2±0.4 0.732+0.027
−0.025		 4622+61
−59		 [107]
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		 transit 191.2±0.4 0.732+0.027
−0.025		 4622+61
−59		 [107]
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		 transit 191.2±0.4 0.732+0.027
−0.025		 4622+61
−59		 [107]
TOI-942 b 0.347+0.022
−0.020		 4.32421±0.000019 0.04866+0.00016
−0.00013		 transit 493.9±1.0 0.8220+0.0079
−0.0064		 [108]
TOI-942 c 0.417+0.030
−0.027		 10.156272+0.000037
−0.000034		 0.08598+0.00027
−0.00022		 transit 493.9±1.0 0.8220+0.0079
−0.0064		 [108]
TOI 1062 b 0.0320±0.0026 0.202±0.008 4.11412+0.0014
−0.0015		 0.052 1,077+10
−9		 transit 268.7±0.2 0.94±0.02 5,328±56 [109]
TOI 1062 c 0.0294±0.0039 7.978+0.021
−0.023		 0.080+0.013
−0.012		 859+9
−8		 radial vel. 268.7±0.2 0.94±0.02 5,328±56 [109]
TOI-1201 b 0.0198±0.0027 0.216±0.008 2.4919863+0.0000030
−0.0000031		 0.0287±0.0012 703+15
−14		 transit 122.77±0.10 0.512±0.020 3,476±51 Belongs to the Hyades, also red dwarf in the system.[110]
TOI 1227 b 0.854+0.067
−0.052		 27.36397±0.00011 0.0886+0.0054
−0.0057		 transit 329.3±0.8 0.170±0.015 3,072±74 [111]
TOI-1231 b 0.0485±0.0104 0.326±0.014 24.245586+0.000064
−0.000066		 0.1288+0.0021
−0.0022		 330 transit 89.68±0.04 0.485±0.024 3,553±31 [112]
TOI-1238b 0.0183±0.0035 0.108±0.010 0.764596+0.000016
−0.000013		 0.0139±0.0008 1133±167 transit 2030.44±0.20 0.59±0.02 4089±54 [113]
TOI-1238c 0.0262±0.0059 0.188±0.013 3.294733+0.000040
−0.000047		 0.037±0.002 695±105 transit 2030.44±0.20 0.59±0.02 4089±54 [113]
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 transit 385±1 0.68+0.1
−0.01		 4,775±100 Also white dwarf on a wide orbit[114]
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		 transit 239.5±0.3 0.66±0.01 4,227±85 [115]
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		 transit 239.5±0.3 0.66±0.01 4,227±85 [115]
TOI-1296b 0.298±0.039 1.231±0.031 3.9443715±0.0000058 0.0497+0.0023
−0.0028		 1,562+43
−31		 transit 1,023±4 1.17±0.14 5,603±47 [116]
TOI-1298b 0.356±0.032 0.841±0.021 4.537164±0.000012 0.0590±0.0023 1,388±24 transit 1,041±7 1.44±0.10 5,889±43 [116]
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		 transit 653 1.464+0.076
−0.079		 6,274±97 Host star also known as BD+47 3521A.[104]
TOI-1431 b 3.14+0.19
−0.18		 1.51±0.06 2.65022±0.00001 0.047±0.002 2,370±100 transit 488±3 1.90+0.10
−0.08		 7,690+400
−250		 Also known as MASCARA-5b[117][118]
TOI-1444 b 0.0122±0.0022 0.125±0.006 0.4702694±0.0000044 0.1288+0.0021
−0.0022		 330 transit 408.9±0.5 0.934±0.038 5,430±90 [119]
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 transit 498 0.946+0.059
−0.041		 5,595+83
−81		 [104]
TOI-1518 b 2.3 1.875±0.053 1.902603±0.000011 0.0389±0.0011 3,237±59 transit 742±6 1.79±0.26 7,300±100 [10]
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		 transit 1,096 1.517+0.053
−0.049		 5,948+87
−89		 [104]
TOI-1634 b 0.0313±0.0030 0.158±0.007 0.9893457±0.0000034 0.01491±0.00015 921±21 transit 114.40±0.08 0.452±0.014 3,472±48 [120][121]
TOI-1685 b 0.0121±0.030 0.131±0.006 0.6691425±0.0000037 0.01156±0.00009 1,052±21 transit 122.68±0.09 0.495±0.019 3,434±51 [122][120] 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 radial vel. 122.68±0.09 0.495±0.019 3,434±51 Unconfirmed[122]
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 transit 324.8±0.4 0.58±0.03 3,985±55 [123]
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 transit 324.8±0.4 0.58±0.03 3,985±55 [123]
TOI-1749 d 0.014+0.020
−0.011		 0.225±0.013 9.04455±0.00012 0.0707±0.0012 533±12 transit 324.8±0.4 0.58±0.03 3,985±55 [123]
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		 transit 729±3 1.499+0.061
−0.15		 5,984+55
−57		 [124]
TOI-1807 b 0.0071+0.0015
−0.0018		 0.165±0.004 0.549372±0.000007 0.0135+0.0013
−0.0022		 1499+82
−129		 transit 133.88±0.25 0.750+0.025
−0.024		 4757+51
−50		 Star is co-moving with TOI-2076[125][126]
TOI-1842b 0.214+0.040
−0.038		 1.04+0.06
−0.05		 9.5739+0.0002
−0.0001		 0.01001±0.0007 transit 729±7 1.46±0.03 6230±50 [127]
TOI-2076 b 0.293±0.038 10.35566±0.00006 0.0631±0.0027 870±13 transit 136.70±0.23 0.850+0.025
−0.026		 5187+54
−53		 Star is co-moving with TOI-1807[125]
TOI-2076 c 0.396±0.004 21.01538+0.00084
−0.00074		 0.0885±0.0038 734±11 transit 136.70±0.23 0.850+0.025
−0.026		 5187+54
−53		 [128] Star is co-moving with TOI-1807[125]
TOI-2076 d 0.370±0.006 25.0893±0.01 0.1138+0.0048
−0.0049		 648±10 transit 136.70±0.23 0.850+0.025
−0.026		 5187+54
−53		 Star is co-moving with TOI-1807[125]
TOI-2109b 5.02±0.75 1.347±0.047 0.67247414±0.00000028 0.01791±0.00065 3631±69 transit 846±9 1.447+0.075
−0.078		 6530+160
−150		 [129]
TOI-2184 b 0.65±0.16 1.017±0.051 6.90683±0.00009 transit 2,515±22 1.53±0.12 5,966±136 [130]
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		 transit 770±3 0.823+0.027
−0.023		 5,144±50 [131]
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 [131]
TOI-2257 b 0.196±0.010 35.189346 0.145±0.003 256+61
−17		 transit 188.5±0.3 0.33±0.02 3430±130 Habitable zone planet[132]
TOI-2285b 0.155±0.007 27.26955+0.00013
−0.00010		 0.1363±0.0010 284±6 transit 138.34±0.14 0.454±0.010 3,491±58 [133]
TOI-2406b 0.0286+0.0223
−0.0126		 0.263+0.015
−0.014		 3.0766896±0.0000065 0.0228±0.0016 447±15 transit 181.4±0.4 0.162±0.008 3,100±75 [134]
TOI-3362b 5.029+0.668
−0.646		 1.142+0.043
−0.041		 18.09547±0.00003 0.153+0.002
−0.003		 transit 1,198±18 1.445+0.069
−0.073		 6,532+88
−86		 High eccentricity orbit[135]
Upsilon Leonis b 0.51+0.06
−0.26		 385.2+2.8
−1.3		 1.18+0.11
−0.32		 radial vel. 177.8 1.48+0.90
−0.38		 4836 [17]
YSES 2 b 6.3+1.6
−0.9		 115 imaging 356.4±0.5 1.10±0.03 4,749±40 [136]

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanet by year of discovery

References

  1. ↑ 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.
  2. ↑ "Astronomers Discover Infant Planet – One of the Youngest Exoplanets Ever Observed". 23 October 2021. Archived from the original on 25 October 2021. Retrieved 25 October 2021.
  3. ↑ "2M0437 b - Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 3 December 2023.
  4. ↑ 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.
  5. 1 2 3 4 5 6 Dalal, S.; et al. (2021). "The SOPHIE search for northern extrasolar planets". Astronomy & Astrophysics. 651: A11. arXiv:2105.09741. doi:10.1051/0004-6361/202140712. S2CID 234790136.
  6. ↑ Faherty, Jacqueline K.; et al. (1 December 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. ISSN 0004-637X. S2CID 245005964.
  7. 1 2 3 4 5 6 Adams, Elisabeth R.; et al. (1 August 2021). "Ultra-short-period Planets in K2. III. Neighbors are Common with 13 New Multiplanet Systems and 10 Newly Validated Planets in Campaigns 0–8 and 10". The Planetary Science Journal. 2 (4): 152. arXiv:2011.11698. doi:10.3847/PSJ/ac0ea0. ISSN 2632-3338.
  8. ↑ "Open Exoplanet Catalogue - EPIC 201427007 b". openexoplanetcatalogue.com. Retrieved 24 November 2023.
  9. ↑ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 24 November 2023.
  10. 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 De Leon, J. P.; et al. (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.
  11. ↑ 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.
  12. 1 2 3 4 Castro-González, A.; et al. (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
  13. ↑ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 24 November 2023.
  14. ↑ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 24 November 2023.
  15. ↑ "Exoplanet-catalog – Exoplanet Exploration: Planets Beyond our Solar System". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 24 November 2023.
  16. ↑ "Exoplanet-catalog – Exoplanet Exploration: Planets Beyond our Solar System". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 24 November 2023.
  17. 1 2 3 4 5 6 7 8 9 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.
  18. 1 2 3 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 May 2021). "The CARMENES search for exoplanets around M dwarfs". Astronomy & Astrophysics. 650: A188. arXiv:2105.13785. doi:10.1051/0004-6361/202140633. S2CID 235248027.
  19. ↑ Lillo-Box, J.; et al. (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
  20. ↑ Lam, Kristine W. F.; et al. (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.
  21. ↑ Trifonov, T.; et al. (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.
  22. ↑ Toledo-Padrón, B.; et al. (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.
  23. ↑ Maldonado, J.; et al. (2021). "HADES RV programme with HARPS-N at TNG". Astronomy & Astrophysics. 651: A93. arXiv:2105.06155. doi:10.1051/0004-6361/202141141. S2CID 234482717.
  24. 1 2 3 4 5 6 7 Bakos, G. á.; Hartman, J. D.; Bhatti, W.; Csubry, Z.; Penev, K.; Bieryla, A.; Latham, D. W.; Quinn, S.; Buchhave, L. A.; Kovács, G.; Torres, Guillermo; Noyes, R. W.; Falco, E.; Béky, Bence; Szklenár, T. (1 July 2021). "HAT-P-58b–HAT-P-64b: Seven Planets Transiting Bright Stars*". The Astronomical Journal. 162 (1): 31. arXiv:2007.05528. doi:10.3847/1538-3881/abf637. ISSN 0004-6256.
  25. 1 2 3 4 Jordán, A.; et al. (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.
  26. 1 2 3 4 5 6 7 8 9 10 11 12 13 Rosenthal, Lee J.; et al. (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.
  27. 1 2 Sozzetti, A.; et al. (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.
  28. 1 2 Mayor, M.; et al. (2011), "The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets", arXiv:1109.2497 [astro-ph.EP]
  29. 1 2 Ahrer, E.; et al. (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.
  30. 1 2 3 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.
  31. 1 2 3 4 5 6 Demangeon, O. D. S.; et al. (2021), "The SOPHIE search for northern extrasolar planets", Astronomy & Astrophysics, 653: A78, arXiv:2107.05089, doi:10.1051/0004-6361/202141079, S2CID 235795175
  32. ↑ Hobson, Melissa J.; et al. (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.
  33. 1 2 Scarsdale, Nicholas; et al. (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.
  34. 1 2 Barragán, O.; et al. (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.
  35. ↑ 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.
  36. 1 2 El Mufti, Mohammed; et al. (1 January 2023). "TOI 560: Two Transiting Planets Orbiting a K Dwarf Validated with iSHELL, PFS, and HIRES RVs". The Astronomical Journal. 165 (1): 10. arXiv:2112.13448. doi:10.3847/1538-3881/ac9834. ISSN 0004-6256.
  37. ↑ "HD 108236 f". Extrasolar Planets Encyclopaedia. 3 December 1995. Retrieved 4 January 2021.
  38. ↑ Bonfanti, A.; et al. (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
  39. 1 2 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.
  40. ↑ Tofflemire, Benjamin M.; et al. (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.
  41. 1 2 Osborn, H. P.; et al. (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.
  42. 1 2 Azevedo Silva, T.; et al. (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.
  43. 1 2 Eisner, N. L.; et al. (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.
  44. ↑ Palatnick, Skyler; et al. (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.
  45. ↑ Gan, Tianjun; et al. (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.
  46. ↑ Bonfanti, A.; et al. (2023). "TOI-1055 b: Neptunian planet characterised with HARPS, TESS, and CHEOPS". Astronomy & Astrophysics. 671: L8. arXiv:2302.10664. Bibcode:2023A&A...671L...8B. doi:10.1051/0004-6361/202245607. S2CID 257050671.
  47. ↑ Lubin, Jack; et al. (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
  48. ↑ Orell-Miquel, J. (2023). "HD 191939 revisited: New and refined planet mass determinations, and a new planet in the habitable zone". Astronomy & Astrophysics. 669: A40. arXiv:2211.00667. doi:10.1051/0004-6361/202244120. S2CID 253197272.
  49. ↑ Heidari, N.; et al. (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.
  50. 1 2 3 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.
  51. ↑ Jones, M. I.; Wittenmyer, R.; Aguilera-Gómez, C.; Soto, M. G.; Torres, P.; Trifonov, T.; Jenkins, J. S.; Zapata, A.; Sarkis, P.; Zakhozhay, O.; Brahm, R.; Ramírez, R.; Santana, F.; Vines, J. I.; Díaz, M. R.; Vučković, M.; Pantoja, B. (2021), "Four Jovian planets around low-luminosity giant stars observed by the EXPRESS and PPPS", Astronomy & Astrophysics, 646: A131, arXiv:2006.01277, Bibcode:2021A&A...646A.131J, doi:10.1051/0004-6361/202038555, S2CID 219179316
  52. 1 2 Feng, Fabo; Butler, R. Paul; Vogt, Steven S.; Clement, Matthew S.; Tinney, C. G.; Cui, Kaiming; Aizawa, Masataka; Jones, Hugh R. A.; Bailey, J.; Burt, Jennifer; Carter, B. D.; Crane, Jeffrey D.; Dotti, Francesco Flammini; Holden, Bradford; Ma, Bo; Ogihara, Masahiro; Oppenheimer, Rebecca; O’Toole, S. J.; Shectman, Stephen A.; Wittenmyer, Robert A.; Wang, Sharon X.; Wright, D. J.; Xuan, Yifan (1 September 2022). "3D Selection of 167 Substellar Companions to Nearby Stars". The Astrophysical Journal Supplement Series. 262 (1): 21. arXiv:2208.12720. Bibcode:2022ApJS..262...21F. doi:10.3847/1538-4365/ac7e57. ISSN 0067-0049.
  53. ↑ Jones, M. I.; Wittenmyer, R.; Aguilera-Gómez, C.; Soto, M. G.; Torres, P.; Trifonov, T.; Jenkins, J. S.; Zapata, A.; Sarkis, P.; Zakhozhay, O.; Brahm, R.; Ramírez, R.; Santana, F.; Vines, J. I.; Díaz, M. R. (February 2021). "Four Jovian planets around low-luminosity giant stars observed by the EXPRESS and PPPS" (PDF). Astronomy & Astrophysics. 646: A131. arXiv:2006.01277. Bibcode:2021A&A...646A.131J. doi:10.1051/0004-6361/202038555. ISSN 0004-6361. S2CID 219179316.
  54. ↑ "HIP 90988 b - Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 4 December 2023.
  55. 1 2 MacDougall, Mason G.; et al. (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.
  56. ↑ Smith, A M S.; et al. (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.
  57. ↑ Zhang, Jingwen; et al. (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.
  58. ↑ Dalba, Paul A.; et al. (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
  59. 1 2 3 Lillo-Box, J.; et al. (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
  60. ↑ Ryu, Yoon-Hyun; et al. (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.
  61. 1 2 3 Han, Cheongho; et al. (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.
  62. ↑ Han, Cheongho; et al. (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.
  63. ↑ Han, Cheongho; et al. (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
  64. 1 2 3 Han, Cheongho; et al. (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.
  65. ↑ 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.
  66. ↑ Yun Hak Kim; et al. (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.
  67. 1 2 3 4 5 Hwang, Kyu-Ha; et al. (2021), "Systematic KMTNet Planetary Anomaly Search, Paper II: Five New q<2×10−4 Mass-ratio Planets", The Astronomical Journal, arXiv:2106.06686, doi:10.3847/1538-3881/ac38ad, S2CID 245740102
  68. ↑ Han, Cheongho; et al. (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.
  69. ↑ Zang, Weicheng; et al. (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
  70. ↑ Han, Cheongho; et al. (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.
  71. ↑ Hirsch, Lea A.; et al. (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.
  72. ↑ "AT LAST! CONFIRMATION OF KEPLER'S SECOND PLANETARY CANDIDATE" (PDF). Archived (PDF) from the original on 15 January 2021. Retrieved 18 January 2021.
  73. ↑ 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.
  74. ↑ 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.
  75. ↑ Soto, M. G.; et al. (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.
  76. 1 2 Silverstein, Michele L.; et al. (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.
  77. ↑ 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.
  78. 1 2 "A warm terrestrial planet with half the mass of Venus transiting a nearby star" (PDF). Archived (PDF) from the original on 13 November 2021. Retrieved 8 August 2021.
  79. ↑ Grieves, Nolan; et al. (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.
  80. ↑ Smith, A. M. S.; et al. (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.
  81. 1 2 3 4 Tilbrook, Rosanna H.; et al. (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.
  82. ↑ Miyazaki, Shota; et al. (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.
  83. ↑ 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.
  84. ↑ Wang(王涵悦), Hanyue; et al. (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.
  85. 1 2 Kil Jung, Youn; et al. (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.
  86. ↑ Kains, N.; et al. (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.
  87. 1 2 Han, Cheongho; et al. (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.
  88. ↑ Yee, Jennifer C.; et al. (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
  89. ↑ Zang, Weicheng; et al. (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
  90. ↑ Shin, In-Gu; et al. (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
  91. ↑ Kondo, Iona; et al. (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.
  92. ↑ 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
  93. ↑ Kostov, Veselin B.; et al. (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
  94. ↑ 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.
  95. 1 2 3 4 5 6 Leleu, A.; et al. (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.
  96. ↑ Hoyer, S.; et al. (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.
  97. ↑ Cointepas, M.; et al. (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.
  98. 1 2 3 Osborn, Ares; et al. (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.
  99. 1 2 3 Newton, Elisabeth R.; et al. (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.
  100. 1 2 3 Barragán, Oscar; et al. (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.
  101. ↑ Gan, Tianjun; et al. (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.
  102. ↑ Kanodia, Shubham; et al. (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
  103. 1 2 Ikwut-Ukwa, Mma; et al. (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
  104. 1 2 3 4 5 Rodriguez, Joseph E.; et al. (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.
  105. ↑ Murgas, F.; et al. (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
  106. ↑ 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. Bibcode:2022AJ....164..197B. doi:10.3847/1538-3881/ac8b7e. S2CID 245877576.
  107. 1 2 3 Vach, Sydney; et al. (2022). "TOI-712: A System of Adolescent Mini-Neptunes Extending to the Habitable Zone". The Astronomical Journal. 164 (2): 71. arXiv:2111.02416. Bibcode:2022AJ....164...71V. doi:10.3847/1538-3881/ac7954. S2CID 242757638.
  108. 1 2 Wirth, Christopher P.; et al. (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
  109. 1 2 Otegi, J. F.; et al. (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
  110. ↑ Kossakowski, D.; et al. (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.
  111. ↑ Mann, Andrew W.; et al. (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.
  112. ↑ Burt, Jennifer A.; et al. (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.
  113. 1 2 González-Álvarez, E.; et al. (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.
  114. ↑ Martin, David V.; et al. (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.
  115. 1 2 Georgieva, I. Y.; et al. (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.
  116. 1 2 Moutou, C.; et al. (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.
  117. ↑ Brett Christopher Addison; et al. (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
  118. ↑ Stangret, M.; et al. (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
  119. ↑ Dai, Fei; et al. (2021), "TKS X: Confirmation of TOI-1444b and a Comparative Analysis of the Ultra-short-period Planets with Hot Neptunes", The Astronomical Journal, 162 (2): 62, arXiv:2105.08844, Bibcode:2021AJ....162...62D, doi:10.3847/1538-3881/ac02bd, S2CID 234778143
  120. 1 2 Hirano, Teruyuki; et al. (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
  121. ↑ Cloutier, R.; et al. (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.
  122. 1 2 Bluhm, P.; et al. (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.
  123. 1 2 3 Fukui, A.; et al. (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
  124. ↑ Khandelwal, Akanksha; et al. (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
  125. 1 2 3 4 Hedges, Christina; et al. (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.
  126. ↑ 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
  127. ↑ Wittenmyer, Robert A.; et al. (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.
  128. ↑ Osborn, H.; et al. (2022). "Uncovering the true periods of the young sub-Neptunes orbiting TOI-2076". Astronomy & Astrophysics. 664: A156. arXiv:2203.03194. Bibcode:2022A&A...664A.156O. doi:10.1051/0004-6361/202243065. S2CID 247292643.
  129. ↑ Wong, Ian; et al. (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.
  130. ↑ Saunders, Nicholas; et al. (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
  131. 1 2 Trifonov, Trifon; et al. (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
  132. ↑ Schanche, N.; et al. (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.
  133. ↑ Fukui, Akihiko; et al. (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.
  134. ↑ Wells, R. D.; et al. (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
  135. ↑ Dong, Jiayin; et al. (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
  136. ↑ Bohn, Alexander J.; et al. (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.
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