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Список екзопланет, відкритих в 2021 році. Різні методи відмічені різними кольорами. Для екзопланет, відкритих методом зміни радіальних швидкостей, наведені мінімальні маси<ref>{{cite web|url=https://exoplanetarchive.ipac.caltech.edu/cgi-bin/TblView/nph-tblView?app=ExoTbls&config=compositepars|title=NASA Exoplanet Archive|author=<!--Not stated-->|date=|website=|publisher=|access-date=20 грудня 2019|quote=}}</ref>.

Умовні позначення в таблиці:

* МП&nbsp;— маса планети у [[Маса Юпітера|масах Юпітера]] ({{Jupiter mass}})
* РП&nbsp;— радіус планети у [[Юпітер (планета)|радіусах Юпітера]] ({{Jupiter radius}})
* МЗ&nbsp;— маса материнської зорі у [[Маса Сонця|масах Сонця]] ({{solar mass|link=yes}})
* P&nbsp;— орбітальний період в добах
* a&nbsp;— [[велика піввісь]] орбіти планети в [[а.о.]]
* ТП&nbsp;— температура поверхні планети або умовної поверхні для газових гігантів в [[кельвін]]ах
* d&nbsp;— вістань від Землі до екзопланети у [[Світловий рік|світлових роках]].

У першій колонці в дужках наведена офіційна назва екзопланети за каталогом та власна назва в дужках. Також, якщо замість власної офіційної є власна неофіційна назва планети, то наводиться неофіційна назва.

== Таблиця ==
{| class="wikitable plainrowheaders sortable" id="table" style="width: 100%; font-size: 83%; text-align: center;"
!Назва (власна назва)
! data-sort-type="number" |МП
! data-sort-type="number" |РП
! data-sort-type="number" |P
! data-sort-type="number" |a
! data-sort-type="number" |ТП
!Метод відкриття
! data-sort-type="number" |d
! data-sort-type="number" |МЗ
! data-sort-type="number" |ТЗ
!Примітки
|-
|[[HD 108236 f]]
|
|0.17406{{±|0.00482|0.00437}}
|29.54255{{±|0.00069}}
|0.1759{{±|0.0037}}
|
| style="background:#FFFF00" |Транзит
|211
|0.853{{±|0.047}}
|5,720.0{{±|50.0}}
|<ref>{{citation|title=HD 108236 f|url=http://exoplanet.eu/catalog/hd_108236_f/|website=exoplanet.eu|access-date=4 січня 2021}}</ref><ref>{{citation|display-authors=1|doi=10.1051/0004-6361/202039608|title=CHEOPS observations of the HD 108236 planetary system: A fifth planet, improved ephemerides, and planetary radii|year=2021|last1=Bonfanti|first1=A.|last2=Delrez|first2=L.|last3=Hooton|first3=M. J.|last4=Wilson|first4=T. G.|last5=Fossati|first5=L.|last6=Alibert|first6=Y.|last7=Hoyer|first7=S.|last8=Mustill|first8=A. J.|last9=Osborn|first9=H. P.|last10=Adibekyan|first10=V.|last11=Gandolfi|first11=D.|last12=Salmon|first12=S.|last13=Sousa|first13=S. G.|last14=Tuson|first14=A.|last15=Van Grootel|first15=V.|last16=Cabrera|first16=J.|last17=Nascimbeni|first17=V.|last18=Maxted|first18=P. F. L.|last19=Barros|first19=S. C. C.|last20=Billot|first20=N.|last21=Bonfils|first21=X.|last22=Borsato|first22=L.|last23=Broeg|first23=C.|last24=Davies|first24=M. B.|last25=Deleuil|first25=M.|last26=Demangeon|first26=O. D. S.|last27=Fridlund|first27=M.|last28=Lacedelli|first28=G.|last29=Lendl|first29=M.|last30=Persson|first30=C.|journal=Astronomy & Astrophysics|volume=646|pages=A157|arxiv=2101.00663|bibcode=2021A&A...646A.157B|s2cid=230437723}}</ref>
|-
|[[NGTS-14Ab]]
|0.092{{±|0.012}}
|0.444{{±|0.030}}
|3.5357173{{±|0.0000069}}
|0.0403{{±|0.0071}}
|1,143{{±|139}}
| style="background:#FFFF00" |Транзит
|1,060
|0.898{{±|0.035}}
|5,187{{±|11}}
|<ref>{{citation|display-authors=1|arxiv=2101.01470|year=2021|title=NGTS-14Ab: A Neptune-sized Транзитing planet in the desert|last1=Smith|first1=A. M. S.|last2=Acton|first2=J. S.|last3=Anderson|first3=D. R.|last4=Armstrong|first4=D. J.|last5=Bayliss|first5=D.|last6=Belardi|first6=C.|last7=Bouchy|first7=F.|last8=Brahm|first8=R.|last9=Briegal|first9=J. T.|last10=Bryant|first10=E. M.|last11=Burleigh|first11=M. R.|last12=Cabrera|first12=J.|last13=Chaushev|first13=A.|last14=Cooke|first14=B. F.|last15=Costes|first15=J. C.|last16=Csizmadia|first16=Sz.|last17=Eigmüller|first17=Ph.|last18=Erikson|first18=A.|last19=Gill|first19=S.|last20=Gillen|first20=E.|last21=Goad|first21=M. R.|last22=Günther|first22=M. N.|last23=Henderson|first23=B. A.|last24=Hogan|first24=A.|last25=Jordán|first25=A.|last26=Lendl|first26=M.|last27=McCormac|first27=J.|last28=Moyano|first28=M.|last29=Nielsen|first29=L. D.|last30=Rauer|first30=H.|journal=Astronomy & Astrophysics|volume=646|pages=A183|doi=10.1051/0004-6361/202039712|bibcode=2021A&A...646A.183S|s2cid=230524042}}</ref>
|-
|[[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
| style="background:#FFFF00" |Транзит
|385{{±|1}}
|0.68{{±|0.1|0.01}}
|4,775{{±|100}}
|В системі також є білий карлик<ref>{{citation|display-authors=1|arxiv=2101.02707|year=2021|title=TOI-1259Ab – a gas giant planet with 2.7 per cent deep Транзитs and a bound white dwarf companion|last1=Martin|first1=David V.|last2=El-Badry|first2=Kareem|author3=Vedad Kunovac Hodžić|last4=Triaud|first4=Amaury H. M. J.|last5=Angus|first5=Ruth|last6=Birky|first6=Jessica|last7=Foreman-Mackey|first7=Daniel|last8=Hedges|first8=Christina|last9=Montet|first9=Benjamin T.|last10=Murphy|first10=Simon J.|last11=Santerne|first11=Alexandre|last12=Stassun|first12=Keivan G.|last13=Stephan|first13=Alexander P.|last14=Wang|first14=Ji|last15=Benni|first15=Paul|last16=Krushinsky|first16=Vadim|last17=Chazov|first17=Nikita|last18=Mishevskiy|first18=Nikolay|last19=Ziegler|first19=Carl|last20=Soubkiou|first20=Abderahmane|last21=Benkhaldoun|first21=Zouhair|last22=Caldwell|first22=Douglas A.|last23=Collins|first23=Karen|last24=Henze|first24=Christopher E.|last25=Guerrero|first25=Natalia M.|last26=Jenkins|first26=Jon M.|last27=Latham|first27=David W.|last28=Levine|first28=Adam|last29=McDermott|first29=Scott|last30=Mullally|first30=Susan E.|journal=Monthly Notices of the Royal Astronomical Society|volume=507|issue=3|pages=4132–4148|doi=10.1093/mnras/stab2129}}</ref>
|-
|[[NGTS-13b]]
|4.84{{±|0.44}}
|1.142{{±|0.046}}
|4.12
|0.0549{{±|0.0015|0.0025}}
|1,605{{±|30}}
| style="background:#FFFF00" |Транзит
|2150
|1.30{{±|0.11|0.18}}
|5,819{{±|73}}
|<ref>{{citation|display-authors=1|arxiv=2101.04245|year=2021|title=NGTS-13b: A hot 4.8 Jupiter-mass planet Транзитing a subgiant star|last1=Grieves|first1=Nolan|last2=Nielsen|first2=Louise D.|last3=Vines|first3=Jose I.|last4=Bryant|first4=Edward M.|last5=Gill|first5=Samuel|last6=Bouchy|first6=François|last7=Lendl|first7=Monika|last8=Bayliss|first8=Daniel|last9=Eigmueller|first9=Philipp|last10=Segransan|first10=Damien|last11=Acton|first11=Jack S.|last12=Anderson|first12=David R.|last13=Burleigh|first13=Matthew R.|last14=Casewell|first14=Sarah L.|last15=Chaushev|first15=Alexander|last16=Cooke|first16=Benjamin F.|last17=Gillen|first17=Edward|last18=Goad|first18=Michael R.|last19=Günther|first19=Maximilian N.|last20=Henderson|first20=Beth A.|last21=Hogan|first21=Aleisha|last22=Jenkins|first22=James S.|last23=Alves|first23=Douglas R.|last24=Jordán|first24=Andrés|last25=McCormac|first25=James|last26=Moyano|first26=Maximiliano|last27=Queloz|first27=Didier|last28=Raynard|first28=Liam|last29=Seidel|first29=Julia V.|last30=Smith|first30=Alexis M. S.|journal=Astronomy & Astrophysics|volume=647|pages=A180|doi=10.1051/0004-6361/202039586|bibcode=2021A&A...647A.180G|s2cid=231582818}}</ref>
|-
|[[TOI-628 b]] ('''HD 288842''')
|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}}
| style="background:#FFFF00" |Транзит
|582
|1.311{{±|0.066|0.075}}
|6,250{{±|220|190}}
|<ref name="Rodriguez2021">{{citation|display-authors=1|arxiv=2101.01726|year=2021|title=TESS Delivers Five New Hot Giant Planets Orbiting Bright Stars from the Full-frame Images|last1=Rodriguez|first1=Joseph E.|last2=Quinn|first2=Samuel N.|last3=Zhou|first3=George|last4=Vanderburg|first4=Andrew|last5=Nielsen|first5=Louise D.|last6=Wittenmyer|first6=Robert A.|last7=Brahm|first7=Rafael|last8=Reed|first8=Phillip A.|last9=Huang|first9=Chelsea X.|last10=Vach|first10=Sydney|last11=Ciardi|first11=David R.|last12=Oelkers|first12=Ryan J.|last13=Stassun|first13=Keivan G.|last14=Hellier|first14=Coel|last15=Scott Gaudi|first15=B.|last16=Eastman|first16=Jason D.|last17=Collins|first17=Karen A.|last18=Bieryla|first18=Allyson|last19=Christian|first19=Sam|last20=Latham|first20=David W.|last21=Carleo|first21=Ilaria|last22=Wright|first22=Duncan J.|last23=Matthews|first23=Elisabeth|last24=Gonzales|first24=Erica J.|last25=Ziegler|first25=Carl|last26=Dressing|first26=Courtney D.|last27=Howell|first27=Steve B.|last28=Tan|first28=Thiam-Guan|last29=Wittrock|first29=Justin|last30=Plavchan|first30=Peter|journal=The Astronomical Journal|volume=161|issue=4|page=194|doi=10.3847/1538-3881/abe38a|bibcode=2021AJ....161..194R|s2cid=230770138}}</ref>
|-
|[[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}}
| style="background:#FFFF00" |Транзит
|1,115
|1.536{{±|0.069|0.076}}
|6,460{{±|130|150}}
|<ref name="Rodriguez2021" />
|-
|[[TOI-1333 b|TOI-1333 A b]] ('''BD+47 3521A''')
|2.37{{±|0.24}}
|1.396{{±|0.056|0.054}}
|4.720219{{±|0.000011}}
|0.0626{{±|0.0011|0.0012}}
|1,679{{±|35|34}}
| style="background:#FFFF00" |Транзит
|653
|1.464{{±|0.076|0.079}}
|6,274{{±|97}}
|<ref name="Rodriguez2021" />
|-
|[[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}}
| style="background:#FFFF00" |Транзит
|498
|0.946{{±|0.059|0.041}}
|5,595{{±|83|81}}
|<ref name="Rodriguez2021" />
|-
|[[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}}
| style="background:#FFFF00" |Транзит
|1,096
|1.517{{±|0.053|0.049}}
|5,948{{±|87|89}}
|<ref name="Rodriguez2021" />
|-
|[[OGLE-2019-BLG-0960Lb]]
|0.0071{{±|0.0027}}
|
|
|1.75{{±|0.55}}
|
| style="background:#0099FF" |Мікролінзування
|2,900{{±|1000}}
|0.45{{±|0.15}}
|
|Найменша планета, знайдена методом мікролінзування<ref>{{cite journal|last1=Yee|first1=Jennifer C.|last2=Zang|first2=Weicheng|last3=Udalski|first3=Andrzej|last4=Ryu|first4=Yoon-Hyun|last5=Green|first5=Jonathan|last6=Hennerley|first6=Steve|last7=Marmont|first7=Andrew|last8=Sumi|first8=Takahiro|last9=Mao|first9=Shude|display-authors=1|year=2021|title=OGLE-2019-BLG-0960 Lb: The Smallest Мікролінзування Planet|journal=The Astronomical Journal|volume=162|issue=5|page=180|arxiv=2101.04696|bibcode=2021AJ....162..180Y|doi=10.3847/1538-3881/ac1582|mode=cs2|last10=Gromadzki|first10=Mariusz|last11=Mróz|first11=Przemek|last12=Skowron|first12=Jan|last13=Poleski|first13=Radoslaw|last14=Szymański|first14=Michał K.|last15=Soszyński|first15=Igor|last16=Pietrukowicz|first16=Paweł|last17=Kozłowski|first17=Szymon|last18=Ulaczyk|first18=Krzysztof|last19=Rybicki|first19=Krzysztof A.|last20=Iwanek|first20=Patryk|last21=Wrona|first21=Marcin|last22=Albrow|first22=Michael D.|last23=Chung|first23=Sun-Ju|last24=Gould|first24=Andrew|last25=Han|first25=Cheongho|last26=Hwang|first26=Kyu-Ha|author27=Youn Kil Jung|last28=Kim|first28=Hyoun-Woo|last29=Shin|first29=In-Gu|last30=Shvartzvald|first30=Yossi|s2cid=231592669}}</ref>
|-
|[[TOI-755|HD 110113 b]] ('''TOI-755''')
|0.0143{{±|0.0020}}
|0.183{{±|0.011}}
|2.541{{±|0.0005|0.001}}
|0.035{{±|0.001}}
|1,371{{±|14}}
| style="background:#FFFF00" |Транзит
|346.5{{±|2.3}}
|0.99{{±|0.08}}
|5,730
|<ref name="Osborn2021">{{citation|display-authors=1|arxiv=2101.04745|title=A hot mini-Neptune in the radius valley orbiting solar analogue HD 110113|year=2021|doi=10.1093/mnras/stab182|last1=Osborn|first1=H. P.|last2=Armstrong|first2=D. J.|last3=Adibekyan|first3=V.|last4=Collins|first4=K. A.|last5=Delgado-Mena|first5=E.|last6=Howell|first6=S. B.|last7=Hellier|first7=C.|last8=King|first8=G. W.|last9=Lillo-Box|first9=J.|last10=Nielsen|first10=L. D.|last11=Otegi|first11=J. F.|last12=Santos|first12=N. C.|last13=Ziegler|first13=C.|last14=Anderson|first14=D. R.|last15=Briceño|first15=C.|last16=Burke|first16=C.|last17=Bayliss|first17=D.|last18=Barrado|first18=D.|last19=Bryant|first19=E. M.|last20=Brown|first20=D J A.|last21=Barros|first21=S C C.|last22=Bouchy|first22=F.|last23=Caldwell|first23=D. A.|last24=Conti|first24=D. M.|last25=Díaz|first25=R. F.|last26=Dragomir|first26=D.|last27=Deleuil|first27=M.|last28=Demangeon|first28=O D S.|last29=Dorn|first29=C.|last30=Daylan|first30=T.|journal=Monthly Notices of the Royal Astronomical Society|volume=502|issue=4|pages=4842–4857|bibcode=2021MNRAS.502.4842O}}</ref>
|-
|[[TOI-755|HD 110113 c]] ('''TOI-755''')
|0.0330{{±|0.0038}}
|
|6.744{{±|0.008|0.009}}
|0.068{{±|0.001|0.002}}
|990{{±|10}}
| style="background:#00FF00" |Радіальна швидкість
|346.5{{±|2.3}}
|0.99{{±|0.08}}
|5,730
|<ref name="Osborn2021" />
|-
|[[KOI-5Ab]] ('''TOI-1241 b''')
|0.179
|0.63
|5
|
|
| style="background:#FFFF00" |Транзит
|1,870{{±|70}}
|1.13
|5861
|<ref name="Kirsch2017">{{citation|display-authors=1|arxiv=1701.06577|year=2017|title=ASSESSING THE EFFECT OF STELLAR COMPANIONS FROM HIGH-RESOLUTION Пряме спостереження OF Kepler OBJECTS OF INTEREST|doi=10.3847/1538-3881/153/3/117|last1=Hirsch|first1=Lea A.|last2=Ciardi|first2=David R.|last3=Howard|first3=Andrew W.|last4=Everett|first4=Mark E.|last5=Furlan|first5=Elise|last6=Saylors|first6=Mindy|last7=Horch|first7=Elliott P.|last8=Howell|first8=Steve B.|last9=Teske|first9=Johanna|last10=Marcy|first10=Geoffrey W.|journal=The Astronomical Journal|volume=153|issue=3|page=117|bibcode=2017AJ....153..117H|s2cid=39321033}}</ref><ref name="Ciardi2021">{{Cite web|url=https://aas.org/sites/default/files/2021-01/AAS237_Mon2_Ciardi.pdf|title=AT LAST! CONFIRMATION OF KEPLER'S SECOND PLANETARY CANDIDATE|access-date=18 січня 2021|archive-date=15 січня 2021|archive-url=https://web.archive.org/web/20210115192529/https://aas.org/sites/default/files/2021-01/AAS237_Mon2_Ciardi.pdf|url-status=live}}</ref>
|-
|[[TOI-178b]]
|0.0047{{±|0.0012|0.0013}}
|0.102{{±|0.006}}
|1.914558{{±|0.000018}}
|0.02607{{±|0.00078}}
|1,040{{±|22|21}}
| style="background:#FFFF00" |Транзит
|205.16{{±|0.03}}
|0.650{{±|0.027|0.029}}
|4,316{{±|70}}
|<ref name="Leleu2021">{{citation|display-authors=1|arxiv=2101.09260|title=Six Транзитing planets and a chain of Laplace resonances in TOI-178|year=2021|doi=10.1051/0004-6361/202039767|last1=Leleu|first1=A.|last2=Alibert|first2=Y.|last3=Hara|first3=N. C.|last4=Hooton|first4=M. J.|last5=Wilson|first5=T. G.|last6=Robutel|first6=P.|last7=Delisle|first7=J.-B.|last8=Laskar|first8=J.|last9=Hoyer|first9=S.|last10=Lovis|first10=C.|last11=Bryant|first11=E. M.|last12=Ducrot|first12=E.|last13=Cabrera|first13=J.|last14=Acton|first14=J.|last15=Adibekyan|first15=V.|last16=Allart|first16=R.|last17=Allende Prieto|first17=C.|last18=Alonso|first18=R.|last19=Alves|first19=D.|last20=Anderson|first20=D. R.|last21=Al|first21=D. R.|last22=Angerhausen|first22=D.|last23=Anglada Escudé|first23=G.|last24=Asquier|first24=J.|last25=Barrado|first25=D.|last26=Barros|first26=S. C. C.|last27=Baumjohann|first27=W.|last28=Bayliss|first28=D.|last29=Beck|first29=M.|last30=Beck|first30=T.|journal=Astronomy & Astrophysics|volume=649|pages=A26|bibcode=2021A&A...649A..26L|s2cid=231693292}}</ref>
|-
|[[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}}
| style="background:#FFFF00" |Транзит
|205.16{{±|0.03}}
|0.650{{±|0.027|0.029}}
|4,316{{±|70}}
|<ref name="Leleu2021" />
|-
|[[TOI-178d]]
|0.0094{{±|0.0025|0.0032}}
|0.229{{±|0.006}}
|6.557700{{±|0.000016}}
|0.0592{{±|0.0018}}
|690{{±|14}}
| style="background:#FFFF00" |Транзит
|205.16{{±|0.03}}
|0.650{{±|0.027|0.029}}
|4,316{{±|70}}
|<ref name="Leleu2021" />
|-
|[[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}}
| style="background:#FFFF00" |Транзит
|205.16{{±|0.03}}
|0.650{{±|0.027|0.029}}
|4,316{{±|70}}
|<ref name="Leleu2021" />
|-
|[[TOI-178f]]
|0.0242{{±|0.0052|0.0047}}
|0.204{{±|0.009}}
|15.231915{{±|0.000115|0.000095}}
|0.1039{{±|0.0031}}
|521{{±|11}}
| style="background:#FFFF00" |Транзит
|205.16{{±|0.03}}
|0.650{{±|0.027|0.029}}
|4,316{{±|70}}
|<ref name="Leleu2021" />
|-
|[[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}}
| style="background:#FFFF00" |Транзит
|205.16{{±|0.03}}
|0.650{{±|0.027|0.029}}
|4,316{{±|70}}
|<ref name="Leleu2021" />
|-
|[[HD 183579 b]] ('''TOI-1055''')
|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}}
| style="background:#FFFF00" |Транзит
|186.1{{±|0.8}}
|1.031{{±|0.025|0.026}}
|5,788{{±|44}}
|<ref>{{citation|display-authors=1|arxiv=2101.12137|year=2021|title=Validation of HD 183579b Using Archival Radial Velocities: A Warm Neptune Orbiting a Bright Solar Analog|last1=Palatnick|first1=Skyler|last2=Kipping|first2=David|last3=Yahalomi|first3=Daniel|journal=The Astrophysical Journal Letters|volume=909|issue=1|pages=L6|doi=10.3847/2041-8213/abe0bb|bibcode=2021ApJ...909L...6P|s2cid=231719821}}</ref><ref>{{citation|display-authors=1|arxiv=2107.14015|year=2021|title=HD 183579b: A Warm Sub-Neptune Транзитing a Solar Twin Detected by TESS|doi=10.1093/mnras/stab2224|last1=Gan|first1=Tianjun|last2=Bedell|first2=Megan|last3=Wang|first3=Sharon Xuesong|last4=Foreman-Mackey|first4=Daniel|last5=Meléndez|first5=Jorge|last6=Mao|first6=Shude|last7=Stassun|first7=Keivan G.|last8=Howell|first8=Steve B.|last9=Ziegler|first9=Carl|last10=Wittenmyer|first10=Robert A.|last11=Hellier|first11=Coel|last12=Collins|first12=Karen A.|last13=Shporer|first13=Avi|last14=Ricker|first14=George R.|last15=Vanderspek|first15=Roland|last16=Latham|first16=David W.|last17=Seager|first17=Sara|last18=Winn|first18=Joshua N.|last19=Jenkins|first19=Jon M.|last20=Addison|first20=Brett C.|last21=Ballard|first21=Sarah|last22=Barclay|first22=Thomas|last23=Bean|first23=Jacob L.|last24=Bowler|first24=Brendan P.|last25=Briceño|first25=César|last26=Crossfield|first26=Ian J M.|last27=Dittman|first27=Jason|last28=Horner|first28=Jonathan|last29=Jensen|first29=Eric L N.|last30=Kane|first30=Stephen R.|journal=Monthly Notices of the Royal Astronomical Society|volume=507|issue=2|pages=2220–2240}}</ref><ref>{{citation|arxiv=2302.10664|year=2023|title=TOI-1055 b: a neptunian planet characterised with HARPS, TESS, and CHEOPS}}</ref>
|-
|[[KMT-2019-BLG-0371b]]
|7.70{{±|11.34|3.90}}
|
|
|0.79{{±|0.14|0.16}}
|
| style="background:#0099FF" |Мікролінзування
|2,3000{{±|3,000|4,000}}
|0.09{{±|0.14|0.05}}
|
|Багато розв'язків для параметрів орбіти<ref>{{citation|display-authors=1|arxiv=2101.12206|year=2021|title=KMT-2019-BLG-0371 and the Limits of Bayesian Analysis|author1=Yun Hak Kim|last2=Chung|first2=Sun-Ju|last3=Yee|first3=Jennifer C.|last4=Udalski|first4=A.|last5=Bond|first5=Ian A.|author6=Youn Kil Jung|last7=Gould|first7=Andrew|last8=Albrow|first8=Michael D.|last9=Han|first9=Cheongho|last10=Hwang|first10=Kyu-Ha|last11=Ryu|first11=Yoon-Hyun|last12=Shin|first12=In-gu|last13=Shvartzvald|first13=Yossi|last14=Zang|first14=Weicheng|last15=Cha|first15=Sang-Mok|last16=Kim|first16=Dong-Jin|last17=Kim|first17=Hyoun-Woo|last18=Kim|first18=Seung-Lee|last19=Lee|first19=Chung-Uk|last20=Lee|first20=Dong-Joo|last21=Lee|first21=Yongseok|last22=Park|first22=Byeong-Gon|last23=Pogge|first23=Richard W.|last24=Poleski|first24=Radek|last25=Mróz|first25=Przemek|last26=Skowron|first26=Jan|last27=Szymański|first27=Michal K.|last28=Pietrukowicz|first28=Pawel|last29=Kozłowski|first29=Szymon|last30=Ulaczyk|first30=Krzysztof|journal=The Astronomical Journal|volume=162|issue=1|page=17|doi=10.3847/1538-3881/abf930|bibcode=2021AJ....162...17K|s2cid=231728667}}</ref>
|-
|[[HD 5278|HD 5278 b]] ('''TOI-130''')
|0.0245{{±|0.0047|0.0044}}
|0.219{{±|0.004}}
|14.339156{{±|0.000049|0.000047}}
|0.1202{{±|0.0013}}
|943{{±|13}}
| style="background:#FFFF00" |Транзит
|183.1{{±|2.7}}
|1.126{{±|0.036|0.035}}
|6,203{{±|64}}
|<ref name="Sozzetti2021">{{citation|display-authors=1|arxiv=2101.12300|year=2021|title=A sub-Neptune and a non-Транзитing Neptune-mass companion unveiled by ESPRESSO around the bright late-F dwarf HD 5278 (TOI-130)|last1=Sozzetti|first1=A.|last2=Damasso|first2=M.|last3=Bonomo|first3=A. S.|last4=Alibert|first4=Y.|last5=Sousa|first5=S. G.|last6=Adibekyan|first6=V.|last7=Zapatero Osorio|first7=M. R.|last8=González Hernández|first8=J. I.|last9=Barros|first9=S. C. C.|last10=Lillo-Box|first10=J.|last11=Stassun|first11=K. G.|last12=Winn|first12=J.|last13=Cristiani|first13=S.|last14=Pepe|first14=F.|last15=Rebolo|first15=R.|last16=Santos|first16=N. C.|last17=Allart|first17=R.|last18=Barclay|first18=T.|last19=Bouchy|first19=F.|last20=Cabral|first20=A.|last21=Ciardi|first21=D.|last22=Di Marcantonio|first22=P.|last23=D'Odorico|first23=V.|last24=Ehrenreich|first24=D.|last25=Fasnaugh|first25=M.|last26=Figueira|first26=P.|last27=Haldemann|first27=J.|last28=Jenkins|first28=J. M.|last29=Latham|first29=D. W.|last30=Lavie|first30=B.|journal=Astronomy & Astrophysics|volume=648|pages=A75|doi=10.1051/0004-6361/202040034|bibcode=2021A&A...648A..75S|s2cid=231728514}}</ref>
|-
|[[HD 5278|HD 5278 c]] ('''TOI-130''')
|0.0579{{±|0.0057|0.0060}}
|
|0.2416{{±|0.0027}}
|0.1202{{±|0.0013}}
|943{{±|13}}
| style="background:#00FF00" |Радіальна швидкість
|183.1{{±|2.7}}
|1.126{{±|0.036|0.035}}
|6,203{{±|64}}
|<ref name="Sozzetti2021" />
|-
|[[KMT-2018-BLG-1025Lb]]
|0.0191{{±|0.0258|0.0104}}
|
|
|1.305{{±|0.194|0.227}}
|
| style="background:#0099FF" |Мікролінзування
|22,000{{±|3,000}}
|0.219{{±|0.297|0.120}}
|
|Багато розв'язків для параметрів орбіти<ref>{{citation|display-authors=1|arxiv=2102.01890|year=2021|title=KMT-2018-BLG-1025Lb: Мікролінзування super-Earth planet orbiting a low-mass star|last1=Han|first1=Cheongho|last2=Udalski|first2=Andrzej|last3=Lee|first3=Chung-Uk|last4=Albrow|first4=Michael D.|last5=Chung|first5=Sun-Ju|last6=Gould|first6=Andrew|last7=Hwang|first7=Kyu-Ha|author8=Youn Kil Jung|last9=Kim|first9=Doeon|last10=Kim|first10=Hyoun-Woo|last11=Ryu|first11=Yoon-Hyun|last12=Shin|first12=In-Gu|last13=Shvartzvald|first13=Yossi|last14=Yee|first14=Jennifer C.|last15=Zang|first15=Weicheng|last16=Cha|first16=Sang-Mok|last17=Kim|first17=Dong-Jin|last18=Kim|first18=Seung-Lee|last19=Lee|first19=Dong-Joo|last20=Lee|first20=Yongseok|last21=Park|first21=Byeong-Gon|last22=Pogge|first22=Richard W.|last23=Kim|first23=Chun-Hwey|last24=Kim|first24=Woong-Tae|last25=Mróz|first25=Przemek|last26=Szymański|first26=Michał K.|last27=Skowron|first27=Jan|last28=Poleski|first28=Radosław|last29=Soszyński|first29=Igor|last30=Pietrukowicz|first30=Paweł|journal=Astronomy & Astrophysics|volume=649|pages=A90|doi=10.1051/0004-6361/202039817|bibcode=2021A&A...649A..90H|s2cid=231786450}}</ref>
|-
|[[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}}
| style="background:#FFFF00" |Транзит
|1,312{{±|17}}
|1.349{{±|0.064|0.065}}
|6,466{{±|95|93}}
|<ref name="Ikwut2021">{{cite journal|last1=Ikwut-Ukwa|first1=Mma|last2=Rodriguez|first2=Joseph E.|last3=Quinn|first3=Samuel N.|last4=Zhou|first4=George|last5=Vanderburg|first5=Andrew|last6=Ali|first6=Asma|last7=Bunten|first7=Katya|last8=Scott Gaudi|first8=B.|last9=Latham|first9=David W.|display-authors=1|year=2022|title=Two Massive Jupiters in Eccentric Orbits from the TESS Full-frame Images|journal=The Astronomical Journal|volume=163|issue=1|page=9|arxiv=2102.02222|bibcode=2022AJ....163....9I|doi=10.3847/1538-3881/ac2ee1|mode=cs2|last10=Howell|first10=Steve B.|last11=Huang|first11=Chelsea X.|last12=Bieryla|first12=Allyson|last13=Collins|first13=Karen A.|last14=Carmichael|first14=Theron W.|last15=Rabus|first15=Markus|last16=Eastman|first16=Jason D.|last17=Collins|first17=Kevin I.|last18=Tan|first18=Thiam-Guan|last19=Schwarz|first19=Richard P.|last20=Myers|first20=Gordon|last21=Stockdale|first21=Chris|last22=Kielkopf|first22=John F.|last23=Radford|first23=Don J.|last24=Oelkers|first24=Ryan J.|last25=Jenkins|first25=Jon M.|last26=Ricker|first26=George R.|last27=Seager|first27=Sara|last28=Vanderspek|first28=Roland K.|last29=Winn|first29=Joshua N.|last30=Burt|first30=Jennifer|s2cid=231802379}}</ref>
|-
|[[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}}
| style="background:#FFFF00" |Транзит
|761{{±|7}}
|1.026{{±|0.057}}
|5,925{{±|85|76}}
|<ref name="Ikwut2021" />
|-
|[[Альфа Центавра Ab]]
|0.062-0.157
|0.3011-0.6386
|
|
|
| style="background:#FF6CDA" |Пряме спостереження
|4.37
|
|
|
|-
|[[HD 13808|HD 13808 b]]
|0.0346
|
|14.2
|0.11
|
| style="background:#00FF00" |Радіальна швидкість
|92.2
|0.771{{±|0.022}}
|5,035{{±|50}}
|Кандидат з 2011 року, підтверджена в 2021<ref name="Major2011">{{cite arXiv|mode=cs2|display-authors=1|eprint=1109.2497|year=2011|title=The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets|last1=Mayor|first1=M.|last2=Marmier|first2=M.|last3=Lovis|first3=C.|last4=Udry|first4=S.|last5=Ségransan|first5=D.|last6=Pepe|first6=F.|last7=Benz|first7=W.|last8=Bertaux|first8=J. -L.|last9=Bouchy|first9=F.|last10=Dumusque|first10=X.|last11=Lo Curto|first11=G.|last12=Mordasini|first12=C.|last13=Queloz|first13=D.|last14=Santos|first14=N. C.|class=astro-ph.EP}}</ref><ref name="Ahrer2021">{{citation|display-authors=1|arxiv=2102.03387|year=2021|title=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|last1=Ahrer|first1=E.|last2=Queloz|first2=D.|last3=Rajpaul|first3=V. M.|last4=Ségransan|first4=D.|last5=Bouchy|first5=F.|last6=Hall|first6=R.|last7=Handley|first7=W.|last8=Lovis|first8=C.|last9=Mayor|first9=M.|last10=Mortier|first10=A.|last11=Pepe|first11=F.|last12=Thompson|first12=S.|last13=Udry|first13=S.|last14=Unger|first14=N.|journal=Monthly Notices of the Royal Astronomical Society|volume=503|issue=1|pages=1248–1263|doi=10.1093/mnras/stab373|bibcode=2021MNRAS.503.1248A}}</ref>
|-
|[[HD 13808|HD 13808 c]]
|0.0315
|
|53.8
|0.26
|
| style="background:#00FF00" |Радіальна швидкість
|92.2
|0.771{{±|0.022}}
|5,035{{±|50}}
|Кандидат з 2011 року, підтверджена в 2021<ref name="Major2011" /><ref name="Ahrer2021" />
|-
|[[CD-38 1467|TOI 451 b]] ('''CD-38 1467''')
|
|0.1732{{±|0.0134|0.0116}}
|1.858701{{±|0.000027|0.000033}}
|0.0271{{±|0.0023|0.0038}}
|1,524{{±|100|60}}
| style="background:#FFFF00" |Транзит
|405.1{{±|1.3}}
|0.94{{±|0.025}}
|5,550{{±|56}}
|Планети обертаються навколо головно
зорі у подвійній системі<ref name="Newton2021">{{citation|display-authors=1|arxiv=2102.06049|year=2021|title=TESS Hunt for Young and Maturing Exoplanets (THYME) IV: Three small planets orbiting a 120 Myr-old star in the Pisces–Eridanus stream|doi=10.3847/1538-3881/abccc6|last1=Newton|first1=Elisabeth R.|last2=Mann|first2=Andrew W.|last3=Kraus|first3=Adam L.|last4=Livingston|first4=John H.|last5=Vanderburg|first5=Andrew|last6=Curtis|first6=Jason L.|author7=Pa Chia Thao|last8=Hawkins|first8=Keith|last9=Wood|first9=Mackenna L.|last10=Rizzuto|first10=Aaron C.|last11=Soubkiou|first11=Abderahmane|last12=Tofflemire|first12=Benjamin M.|last13=Zhou|first13=George|last14=Crossfield|first14=Ian J. M.|last15=Pearce|first15=Logan A.|last16=Collins|first16=Karen A.|last17=Conti|first17=Dennis M.|last18=Tan|first18=Thiam-Guan|last19=Villeneuva|first19=Steven|last20=Spencer|first20=Alton|last21=Dragomir|first21=Diana|last22=Quinn|first22=Samuel N.|last23=Jensen|first23=Eric L. N.|last24=Collins|first24=Kevin I.|last25=Stockdale|first25=Chris|last26=Cloutier|first26=Ryan|last27=Hellier|first27=Coel|last28=Benkhaldoun|first28=Zouhair|last29=Ziegler|first29=Carl|last30=Briceño|first30=César|journal=The Astronomical Journal|volume=161|issue=2|page=65|bibcode=2021AJ....161...65N|s2cid=231879927}}</ref><ref name="Barragan2021">{{citation|display-authors=1|arxiv=2103.09746|year=2021|title=TESS re-observes the young multi-planet system TOI-451:refined ephemeris and activity evolution|last1=Barragán|first1=Oscar|last2=Aigrain|first2=Suzanne|last3=Gillen|first3=Edward|last4=Gutiérrez-Canales|first4=Fernando|journal=Research Notes of the American Astronomical Society|volume=5|issue=3|page=51|doi=10.3847/2515-5172/abef70|bibcode=2021RNAAS...5...51B|s2cid=232258104}}</ref>
|-
|[[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}}
| style="background:#FFFF00" |Транзит
|405.1{{±|1.3}}
|0.94{{±|0.025}}
|5,550{{±|56}}
|Планети обертаються навколо головно
зорі у подвійній системі<ref name="Newton2021" /><ref name="Barragan2021" />
|-
|[[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}}
| style="background:#FFFF00" |Транзит
|405.1{{±|1.3}}
|0.94{{±|0.025}}
|5,550{{±|56}}
|Планети обертаються навколо головно
зорі у подвійній системі<ref name="Newton2021" /><ref name="Barragan2021" />
|-
|[[HD 110082 b]] ('''TOI-1098''')
|
|0.2857{{±|0.0089}}
|10.18271{{±|0.00004}}
|0.113{{±|0.009|0.013}}
|
| style="background:#FFFF00" |Транзит
|342.8{{±|0.9}}
|1.21{{±|0.06}}
|6,200{{±|100}}
|Планети обертаються навколо головно
зорі у подвійній системі<ref>{{citation|display-authors=1|arxiv=2102.06066|year=2021|title=TESS Hunt for Young and Maturing Exoplanets (THYME). V. A Sub-Neptune Транзитing a Young Star in a Newly Discovered 250 Myr Association|last1=Tofflemire|first1=Benjamin M.|last2=Rizzuto|first2=Aaron C.|last3=Newton|first3=Elisabeth R.|last4=Kraus|first4=Adam L.|last5=Mann|first5=Andrew W.|last6=Vanderburg|first6=Andrew|last7=Nelson|first7=Tyler|last8=Hawkins|first8=Keith|last9=Wood|first9=Mackenna L.|last10=Zhou|first10=George|last11=Quinn|first11=Samuel N.|last12=Howell|first12=Steve B.|last13=Collins|first13=Karen A.|last14=Schwarz|first14=Richard P.|last15=Stassun|first15=Keivan G.|last16=Bouma|first16=Luke G.|last17=Essack|first17=Zahra|last18=Osborn|first18=Hugh|last19=Boyd|first19=Patricia T.|last20=Furesz|first20=Gabor|last21=Glidden|first21=Ana|last22=Twicken|first22=Joseph D.|last23=Wohler|first23=Bill|last24=McLean|first24=Brian|last25=Ricker|first25=George R.|last26=Vanderspek|first26=Roland|last27=Latham|first27=David W.|last28=Seager|first28=S.|last29=Winn|first29=Joshua N.|last30=Jenkins|first30=Jon M.|journal=The Astronomical Journal|volume=161|issue=4|page=171|doi=10.3847/1538-3881/abdf53|bibcode=2021AJ....161..171T|s2cid=231879915}}</ref>
|-
|[[OGLE-2018-BLG-0567Lb]]
|0.32{{±|0.34|0.16}}
|
|
|2.72{{±|0.49|0.55}}
|
| style="background:#0099FF" |Мікролінзування
|23,000{{±|3,000}}
|0.24{{±|0.16|0.13}}
|
|<ref name="Jung2021">{{citation|display-authors=1|arxiv=2102.07338|year=2021|title=OGLE-2018-BLG-0567Lb and OGLE-2018-BLG-0962Lb: Two Мікролінзування Planets through the Planetary-caustic Channel|doi=10.3847/1538-3881/abf8bd|last1=Kil Jung|first1=Youn|last2=Han|first2=Cheongho|last3=Udalski|first3=Andrzej|last4=Gould|first4=Andrew|last5=Yee|first5=Jennifer C.|last6=Albrow|first6=Michael D.|last7=Chung|first7=Sun-Ju|last8=Hwang|first8=Kyu-Ha|last9=Ryu|first9=Yoon-Hyun|last10=Shin|first10=In-Gu|last11=Shvartzvald|first11=Yossi|last12=Zhu|first12=Wei|last13=Zang|first13=Weicheng|last14=Cha|first14=Sang-Mok|last15=Kim|first15=Dong-Jin|last16=Kim|first16=Hyoun-Woo|last17=Kim|first17=Seung-Lee|last18=Lee|first18=Chung-Uk|last19=Lee|first19=Dong-Joo|last20=Lee|first20=Yongseok|last21=Park|first21=Byeong-Gon|last22=Pogge|first22=Richard W.|last23=Mróz|first23=Przemek|last24=Szymański|first24=Michał K.|last25=Skowron|first25=Jan|last26=Poleski|first26=Radek|last27=Soszyński|first27=Igor|last28=Pietrukowicz|first28=Paweł|last29=Kozłowski|first29=Szymon|last30=Ulaczyk|first30=Krzystof|journal=The Astronomical Journal|volume=161|issue=6|page=293|bibcode=2021AJ....161..293J|s2cid=231924992}}</ref>
|-
|[[OGLE-2018-BLG-0962Lb]]
|1.37{{±|0.80|0.72}}
|
|
|3.57{{±|0.68|1.02}}
|
| style="background:#0099FF" |Мікролінзування
|21,000{{±|3,000|5,000}}
|0.55{{±|0.32|0.29}}
|
|<ref name="Jung2021" />
|-
|[[Gliese 740 b]]
|0.0093{{±|0.0016}}
|
|2.37756{{±|0.00013|0.00011}}
|0.029{{±|0.001}}
|829{{±|40|50}}
| style="background:#00FF00" |Радіальна швидкість
|36.21{{±|0.02}}
|0.58{{±|0.06}}
|3,913{{±|21}}
|<ref>{{citation|display-authors=1|arxiv=2102.09441|year=2021|title=A super-Earth on a close-in orbit around the M1V star GJ 740|doi=10.1051/0004-6361/202040099|last1=Toledo-Padrón|first1=B.|last2=Suárez Mascareño|first2=A.|last3=González Hernández|first3=J. I.|last4=Rebolo|first4=R.|last5=Pinamonti|first5=M.|last6=Perger|first6=M.|last7=Scandariato|first7=G.|last8=Damasso|first8=M.|last9=Sozzetti|first9=A.|last10=Maldonado|first10=J.|last11=Desidera|first11=S.|last12=Ribas|first12=I.|last13=Micela|first13=G.|last14=Affer|first14=L.|last15=González-Alvarez|first15=E.|last16=Leto|first16=G.|last17=Pagano|first17=I.|last18=Zanmar Sánchez|first18=R.|last19=Giacobbe|first19=P.|last20=Herrero|first20=E.|last21=Morales|first21=J. C.|last22=Amado|first22=P. J.|last23=Caballero|first23=J. A.|last24=Quirrenbach|first24=A.|last25=Reiners|first25=A.|last26=Zechmeister|first26=M.|journal=Astronomy & Astrophysics|volume=648|pages=A20|s2cid=231951695}}</ref>
|-
|[[OGLE-2018-BLG-1428Lb]]
|0.77{{±|0.77|0.53}}
|
|
|3.30{{±|0.59|0.83}}
|
| style="background:#0099FF" |Мікролінзування
|20,000{{±|3,000|5,000}}
|0.43{{±|0.33|0.22}}
|
|<ref>{{citation|display-authors=1|arxiv=1303.1184|year=2021|title=A giant planet beyond the snow line in Мікролінзування event OGLE-2011-BLG-0251|doi=10.1051/0004-6361/201220626|last1=Kains|first1=N.|last2=Street|first2=R. A.|last3=Choi|first3=J.-Y.|last4=Han|first4=C.|last5=Udalski|first5=A.|last6=Almeida|first6=L. A.|last7=Jablonski|first7=F.|last8=Tristram|first8=P. J.|last9=Jørgensen|first9=U. G.|last10=Szymański|first10=M. K.|last11=Kubiak|first11=M.|last12=Pietrzyński|first12=G.|last13=Soszyński|first13=I.|last14=Poleski|first14=R.|last15=Kozłowski|first15=S.|last16=Pietrukowicz|first16=P.|last17=Ulaczyk|first17=K.|last18=Wyrzykowski|first18=Ł.|last19=Skowron|first19=J.|last20=Alsubai|first20=K. A.|last21=Bozza|first21=V.|last22=Browne|first22=P.|last23=Burgdorf|first23=M. J.|last24=Calchi Novati|first24=S.|last25=Dodds|first25=P.|last26=Dominik|first26=M.|last27=Dreizler|first27=S.|last28=Fang|first28=X.-S.|last29=Grundahl|first29=F.|last30=Gu|first30=C.-H.|journal=Astronomy & Astrophysics|volume=552|pages=A70|bibcode=2013A&A...552A..70K|s2cid=43146154}}</ref>
|-
|[[LHS 1478 b]] ('''TOI-1640''', '''G 245-61''')
|0.0073{{±|0.0006}}
|0.111{{±|0.004}}
|1.9495378{{±|0.0000040|0.0000041}}
|0.01848{{±|0.00061|0.0006}}
|595{{±|10|9}}
| style="background:#FFFF00" |Транзит
|59.40{{±|0.03}}
|0.236{{±|0.012}}
|3,381{{±|54}}
|<ref>{{citation|display-authors=1|arxiv=2102.11640|year=2021|title=Mass and density of the Транзитing hot and rocky super-Earth LHS 1478 b (TOI-1640 b)|doi=10.1051/0004-6361/202140618|last1=Soto|first1=M. G.|last2=Anglada-Escudé|first2=G.|last3=Dreizler|first3=S.|last4=Molaverdikhani|first4=K.|last5=Kemmer|first5=J.|last6=Rodríguez-López|first6=C.|last7=Lillo-Box|first7=J.|last8=Pallé|first8=E.|last9=Espinoza|first9=N.|last10=Caballero|first10=J. A.|last11=Quirrenbach|first11=A.|last12=Ribas|first12=I.|last13=Reiners|first13=A.|last14=Narita|first14=N.|last15=Hirano|first15=T.|last16=Amado|first16=P. J.|last17=Béjar|first17=V. J. S.|last18=Bluhm|first18=P.|last19=Burke|first19=C. J.|last20=Caldwell|first20=D. A.|last21=Charbonneau|first21=D.|last22=Cloutier|first22=R.|last23=Collins|first23=K. A.|last24=Cortés-Contreras|first24=M.|last25=Girardin|first25=E.|last26=Guerra|first26=P.|last27=Harakawa|first27=H.|last28=Hatzes|first28=A. P.|last29=Irwin|first29=J.|last30=Jenkins|first30=J. M.|journal=Astronomy & Astrophysics|volume=649|pages=A144|bibcode=2021A&A...649A.144S|s2cid=232013854}}</ref>
|-
|[[TOI-1685 b]] ('''UCAC4 666-026266''')
|0.0121{{±|0.030}}
|0.131{{±|0.006}}
|0.6691425{{±|0.0000037}}
|0.01156{{±|0.00009}}
|1,052{{±|21}}
| style="background:#FFFF00" |Транзит
|122.68{{±|0.09}}
|0.495{{±|0.019}}
|3,434{{±|51}}
|<ref name="Bluhm2021">{{citation|display-authors=1|arxiv=2103.01016|year=2021|title=An ultra-short-period Транзитing super-Earth orbiting the M3 dwarf TOI-1685|doi=10.1051/0004-6361/202140688|last1=Bluhm|first1=P.|last2=Pallé|first2=E.|last3=Molaverdikhani|first3=K.|last4=Kemmer|first4=J.|last5=Hatzes|first5=A. P.|last6=Kossakowski|first6=D.|last7=Stock|first7=S.|last8=Caballero|first8=J. A.|last9=Lillo-Box|first9=J.|last10=Béjar|first10=V. J. S.|last11=Soto|first11=M. G.|last12=Amado|first12=P. J.|last13=Brown|first13=P.|last14=Cadieux|first14=C.|last15=Cloutier|first15=R.|last16=Collins|first16=K. A.|last17=Collins|first17=K. I.|last18=Cortés-Contreras|first18=M.|last19=Doyon|first19=R.|last20=Dreizler|first20=S.|last21=Espinoza|first21=N.|last22=Fukui|first22=A.|last23=González-Álvarez|first23=E.|last24=Henning|first24=Th.|last25=Horne|first25=K.|last26=Jeffers|first26=S. V.|last27=Jenkins|first27=J. M.|last28=Jensen|first28=E. L. N.|last29=Kaminski|first29=A.|last30=Kielkopf|first30=J. F.|journal=Astronomy & Astrophysics|volume=650|pages=A78|bibcode=2021A&A...650A..78B|s2cid=232092636}}</ref><ref name="Hirano2021">{{cite journal|last1=Hirano|first1=Teruyuki|last2=Livingston|first2=John H.|last3=Fukui|first3=Akihiko|last4=Narita|first4=Norio|last5=Harakawa|first5=Hiroki|author6=Hiroyuki Tako Ishikawa|last7=Miyakawa|first7=Kohei|last8=Kimura|first8=Tadahiro|last9=Nakayama|first9=Akifumi|display-authors=1|year=2021|title=Two Bright M Dwarfs Hosting Ultra-Short-Period Super-Earths with Earth-like Compositions|journal=The Astronomical Journal|volume=162|issue=4|page=161|arxiv=2103.12760|bibcode=2021AJ....162..161H|doi=10.3847/1538-3881/ac0fdc|mode=cs2|last10=Fujita|first10=Naho|last11=Hori|first11=Yasunori|last12=Stassun|first12=Keivan G.|last13=Bieryla|first13=Allyson|last14=Cadieux|first14=Charles|last15=Ciardi|first15=David R.|last16=Collins|first16=Karen A.|last17=Ikoma|first17=Masahiro|last18=Vanderburg|first18=Andrew|last19=Barclay|first19=Thomas|last20=Brasseur|first20=C. E.|last21=de Leon|first21=Jerome P.|last22=Doty|first22=John P.|last23=Doyon|first23=René|last24=Esparza-Borges|first24=Emma|last25=Esquerdo|first25=Gilbert A.|last26=Furlan|first26=Elise|last27=Gaidos|first27=Eric|last28=Gonzales|first28=Erica J.|last29=Hodapp|first29=Klaus|last30=Kusakabe|first30=Nobuhiko|s2cid=232335413}}</ref>
|-
|[[TOI-1685 c]]
|0.0290{{±|0.0065}}
|
|9.025{{±|0.104|0.119}}
|
|449.1{{±|6.9}}
| style="background:#00FF00" |Радіальна швидкість
|122.68{{±|0.09}}
|0.495{{±|0.019}}
|3,434{{±|51}}
|Непідтверджено<ref name="Bluhm2021" />
|-
|[[KMT-2020-BLG-0414Lb]]
|0.0032
|
|
|0.15
|
| style="background:#0099FF" |Мікролінзування
|3,300{{±|300}}
|0.3
|
|В системі також є коричневий карлик масою 17 мас Юпітера на відстані 15 а.о.<ref>{{cite journal|last1=Zang|first1=Weicheng|last2=Han|first2=Cheongho|last3=Kondo|first3=Iona|last4=Yee|first4=Jennifer C.|last5=Lee|first5=Chung-Uk|last6=Gould|first6=Andrew|last7=Mao|first7=Shude|author8=Leandro de Almeida|last9=Shvartzvald|first9=Yossi|display-authors=1|year=2021|title=An Earth-mass planet in a time of COVID-19: KMT-2020-BLG-0414Lb|journal=Research in Astronomy and Astrophysics|volume=21|issue=9|page=239|arxiv=2103.01896|bibcode=2021RAA....21..239Z|doi=10.1088/1674-4527/21/9/239|mode=cs2|last10=Zhang|first10=Xiangyu|last11=Albrow|first11=Michael D.|last12=Chung|first12=Sun-Ju|last13=Hwang|first13=Kyu-Ha|author14=Youn Kil Jung|last15=Ryu|first15=Yoon-Hyun|last16=Shin|first16=In-Gu|last17=Cha|first17=Sang-Mok|last18=Kim|first18=Dong-Jin|last19=Kim|first19=Hyoun-Woo|last20=Kim|first20=Seung-Lee|last21=Lee|first21=Dong-Joo|last22=Lee|first22=Yongseok|last23=Park|first23=Byeong-Gon|last24=Pogge|first24=Richard W.|last25=Drummond|first25=John|last26=Tan|first26=Thiam-Guan|author27=José Dias do Nascimento Júnior|last28=Maoz|first28=Dan|last29=Penny|first29=Matthew T.|last30=Zhu|first30=Wei|s2cid=232092272}}</ref>
|-
|[[HD 39474 b]] ('''TOI-201''')
|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}}
| style="background:#FFFF00" |Транзит
|372.5{{±|1.1}}
|1.316{{±|0.027}}
|6,394{{±|75}}
|<ref name="Hobson2021">{{citation|display-authors=1|arxiv=2103.02685|year=2021|title=A Транзитing Warm Giant Planet around the Young Active Star TOI-201|doi=10.3847/1538-3881/abeaa1|last1=Hobson|first1=Melissa J.|last2=Brahm|first2=Rafael|last3=Jordán|first3=Andrés|last4=Espinoza|first4=Nestor|last5=Kossakowski|first5=Diana|last6=Henning|first6=Thomas|last7=Rojas|first7=Felipe|last8=Schlecker|first8=Martin|last9=Sarkis|first9=Paula|last10=Trifonov|first10=Trifon|last11=Thorngren|first11=Daniel|last12=Binnenfeld|first12=Avraham|last13=Shahaf|first13=Sahar|last14=Zucker|first14=Shay|last15=Ricker|first15=George R.|last16=Latham|first16=David W.|last17=Seager|first17=S.|last18=Winn|first18=Joshua N.|last19=Jenkins|first19=Jon M.|last20=Addison|first20=Brett|last21=Bouchy|first21=François|last22=Bowler|first22=Brendan P.|last23=Briegal|first23=Joshua T.|last24=Bryant|first24=Edward M.|last25=Collins|first25=Karen A.|last26=Daylan|first26=Tansu|last27=Grieves|first27=Nolan|last28=Horner|first28=Jonathan|last29=Huang|first29=Chelsea|last30=Kane|first30=Stephen R.|journal=The Astronomical Journal|volume=161|issue=5|page=235|bibcode=2021AJ....161..235H|s2cid=232110390}}</ref>
|-
|[[Gliese 486|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}}
| style="background:#FFFF00" |Транзит
|26.344{{±|0.013}}
|0.323{{±|0.015}}
|3,340{{±|54}}
|Планета потенційно має достатньо щільну атмосферу<ref>{{citation|display-authors=1|arxiv=2103.04950|year=2021|title=A nearby Транзитing rocky exoplanet that is suitable for atmospheric investigation|doi=10.1126/science.abd7645|last1=Trifonov|first1=T.|last2=Caballero|first2=J. A.|last3=Morales|first3=J. C.|last4=Seifahrt|first4=A.|last5=Ribas|first5=I.|last6=Reiners|first6=A.|last7=Bean|first7=J. L.|last8=Luque|first8=R.|last9=Parviainen|first9=H.|last10=Pallé|first10=E.|last11=Stock|first11=S.|last12=Zechmeister|first12=M.|last13=Amado|first13=P. J.|last14=Anglada-Escudé|first14=G.|last15=Azzaro|first15=M.|last16=Barclay|first16=T.|last17=Béjar|first17=V. J. S.|last18=Bluhm|first18=P.|last19=Casasayas-Barris|first19=N.|last20=Cifuentes|first20=C.|last21=Collins|first21=K. A.|last22=Collins|first22=K. I.|last23=Cortés-Contreras|first23=M.|last24=De Leon|first24=J.|last25=Dreizler|first25=S.|last26=Dressing|first26=C. D.|last27=Esparza-Borges|first27=E.|last28=Espinoza|first28=N.|last29=Fausnaugh|first29=M.|last30=Fukui|first30=A.|journal=Science|volume=371|issue=6533|pages=1038–1041|pmid=33674491|bibcode=2021Sci...371.1038T|s2cid=232124642}}</ref>
|-
|[[NGTS-15b]]
|0.751{{±|0.102|0.088}}
|1.10{{±|0.10}}
|3.27623{{±|0.00001}}
|0.0441{{±|0.0046}}
|1,146{{±|47}}
| style="background:#FFFF00" |Транзит
|2,580{{±|60}}
|0.995{{±|0.015}}
|5,600{{±|150}}
|<ref name="Tilbrook2021">{{citation|display-authors=1|arxiv=2103.10302|year=2021|title=NGTS 15b, 16b, 17b, and 18b: Four hot Jupiters from the Next-Generation Транзит Survey|doi=10.1093/mnras/stab815|last1=Tilbrook|first1=Rosanna H.|last2=Burleigh|first2=Matthew R.|last3=Costes|first3=Jean C.|last4=Gill|first4=Samuel|last5=Nielsen|first5=Louise D.|last6=Vines|first6=José I.|last7=Queloz|first7=Didier|last8=Hodgkin|first8=Simon T.|last9=Worters|first9=Hannah L.|last10=Goad|first10=Michael R.|last11=Acton|first11=Jack S.|last12=Henderson|first12=Beth A.|last13=Armstrong|first13=David J.|last14=Anderson|first14=David R.|last15=Bayliss|first15=Daniel|last16=Bouchy|first16=François|last17=Briegal|first17=Joshua T.|last18=Bryant|first18=Edward M.|last19=Casewell|first19=Sarah L.|last20=Chaushev|first20=Alexander|last21=Cooke|first21=Benjamin F.|last22=Eigmüller|first22=Philipp|last23=Gillen|first23=Edward|last24=Günther|first24=Maximilian N.|last25=Hogan|first25=Aleisha|last26=Jenkins|first26=James S.|last27=Lendl|first27=Monika|last28=McCormac|first28=James|last29=Moyano|first29=Maximiliano|last30=Raynard|first30=Liam|journal=Monthly Notices of the Royal Astronomical Society|volume=504|issue=4|pages=6018–6032}}</ref>
|-
|[[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}}
| style="background:#FFFF00" |Транзит
|2,910{{±|95|75}}
|1.002{{±|0.011}}
|5,550{{±|150}}
|<ref name="Tilbrook2021" />
|-
|[[NGTS-17b]]
|0.764{{±|0.195|0.164}}
|1.24{{±|0.11}}
|3.24253{{±|0.00001}}
|0.0391{{±|0.0043}}
|1,457{{±|50}}
| style="background:#FFFF00" |Транзит
|3,420{{±|90}}
|1.025{{±|0.015|0.014}}
|5,650{{±|100}}
|<ref name="Tilbrook2021" />
|-
|[[NGTS-18b]]
|0.409{{±|0.081|0.063}}
|1.21{{±|0.18}}
|3.05125{{±|0.00001}}
|0.0448{{±|0.0068}}
|1,381{{±|55|53}}
| style="background:#FFFF00" |Транзит
|3,610{{±|140}}
|1.003{{±|0.020|0.012}}
|5,610{{±|150}}
|<ref name="Tilbrook2021" />
|-
|[[OGLE-2019-BLG-1053Lb]]
|0.0078{{±|0.0037|0.0031}}
|
|
|3.4{{±|0.5}}
|
| style="background:#0099FF" |Мікролінзування
|22,000{{±|3,000|2,000}}
|0.61{{±|0.29|0.24}}
|
|<ref>{{cite journal|last1=Zang|first1=Weicheng|last2=Hwang|first2=Kyu-Ha|last3=Udalski|first3=Andrzej|last4=Wang|first4=Tianshu|last5=Zhu|first5=Wei|last6=Sumi|first6=Takahiro|last7=Gould|first7=Andrew|last8=Mao|first8=Shude|last9=Zhang|first9=Xiangyu|display-authors=1|year=2021|title=Systematic KMTNet Planetary Anomaly Search. I. OGLE-2019-BLG-1053Lb, a Buried Terrestrial Planet|journal=The Astronomical Journal|volume=162|issue=4|page=163|arxiv=2103.11880|bibcode=2021AJ....162..163Z|doi=10.3847/1538-3881/ac12d4|mode=cs2|last10=Albrow|first10=Michael D.|last11=Chung|first11=Sun-Ju|last12=Han|first12=Cheongho|author13=Youn Kil Jung|last14=Ryu|first14=Yoon-Hyun|last15=Shin|first15=In-Gu|last16=Shvartzvald|first16=Yossi|last17=Yee|first17=Jennifer C.|last18=Cha|first18=Sang-Mok|last19=Kim|first19=Dong-Jin|last20=Kim|first20=Hyoun-Woo|last21=Kim|first21=Seung-Lee|last22=Lee|first22=Chung-Uk|last23=Lee|first23=Dong-Joo|last24=Lee|first24=Yongseok|last25=Park|first25=Byeong-Gon|last26=Pogge|first26=Richard W.|last27=Mróz|first27=Przemek|last28=Skowron|first28=Jan|last29=Szymański|first29=Michał~K.|last30=Soszyński|first30=Igor|s2cid=232307459}}</ref>
|-
|[[TOI-1634 b]]
|0.0313{{±|0.0030}}
|0.158{{±|0.007}}
|0.9893457{{±|0.0000034}}
|0.01491{{±|0.00015}}
|921{{±|21}}
| style="background:#FFFF00" |Транзит
|114.40{{±|0.08}}
|0.452{{±|0.014}}
|3,472{{±|48}}
|<ref name="Hirano2021" /><ref>{{citation|display-authors=1|arxiv=2103.12790|year=2021|title=TOI-1634 b: An Ultra-short-period Keystone Planet Sitting inside the M-dwarf Radius Valley|last1=Cloutier|first1=R.|last2=Charbonneau|first2=D.|last3=Stassun|first3=K. G.|last4=Murgas|first4=F.|last5=Mortier|first5=A.|last6=Massey|first6=R.|last7=Lissauer|first7=J. J.|last8=Latham|first8=D. W.|last9=Irwin|first9=J.|last10=Haywood|first10=R. D.|last11=Guerra|first11=P.|last12=Girardin|first12=E.|last13=Giacalone|first13=S. A.|last14=Bosch-Cabot|first14=P.|last15=Bieryla|first15=A.|last16=Winn|first16=J.|last17=Watson|first17=C. A.|last18=Vanderspek|first18=R.|last19=Udry|first19=S.|last20=Tamura|first20=M.|last21=Sozzetti|first21=A.|last22=Shporer|first22=A.|last23=Ségransan|first23=D.|last24=Seager|first24=S.|last25=Savel|first25=A. B.|last26=Sasselov|first26=D.|last27=Rose|first27=M.|last28=Ricker|first28=G.|last29=Rice|first29=K.|last30=Quintana|first30=E. V.|journal=The Astronomical Journal|volume=162|issue=2|page=79|doi=10.3847/1538-3881/ac0157|bibcode=2021AJ....162...79C|s2cid=232335385}}</ref>
|-
|[[KMT-2019-BLG-1715]]
|2.56{{±|1.13|1.16}}
|
|
|3.32{{±|0.82|0.92}}
|
| style="background:#0099FF" |Мікролінзування
|13,000{{±|3,000}}
|0.61{{±|0.27|0.28}}
|
|Багато можливих розв'язків для орбіти, в системі також є червоний карлик масою 0.15{{Solar_mass}}<ref>{{citation|display-authors=1|arxiv=2104.00293|year=2021|title=KMT-2019-BLG-1715: Planetary Мікролінзування Event with Three Lens Masses and Two Source Stars|doi=10.3847/1538-3881/abf4d0|last1=Han|first1=Cheongho|last2=Udalski|first2=Andrzej|last3=Kim|first3=Doeon|last4=Kil Jung|first4=Youn|last5=Lee|first5=Chung-Uk|last6=Bond|first6=Ian A.|last7=Albrow|first7=Michael D.|last8=Chung|first8=Sun-Ju|last9=Gould|first9=Andrew|last10=Hwang|first10=Kyu-Ha|last11=Kim|first11=Hyoun-Woo|last12=Ryu|first12=Yoon-Hyun|last13=Shin|first13=In-Gu|last14=Shvartzvald|first14=Yossi|last15=Zang|first15=Weicheng|last16=Yee|first16=Jennifer C.|last17=Cha|first17=Sang-Mok|last18=Kim|first18=Dong-Jin|last19=Kim|first19=Seung-Lee|last20=Lee|first20=Dong-Joo|last21=Lee|first21=Yongseok|last22=Park|first22=Byeong-Gon|last23=Pogge|first23=Richard W.|last24=Kim|first24=Chun-Hwey|last25=Kim|first25=Woong-Tae|last26=Mróz|first26=Przemek|last27=Szymański|first27=Michał K.|last28=Skowron|first28=Jan|last29=Poleski|first29=Radek|last30=Soszyński|first30=Igor|journal=The Astronomical Journal|volume=161|issue=6|page=270|bibcode=2021AJ....161..270H|s2cid=232478488}}</ref>
|-
|[[OGLE-2018-BLG-1185b]]
|0.026{{±|0.025|0.015}}
|
|
|1.54{{±|0.18|0.22}}
|
| style="background:#0099FF" |Мікролінзування
|24,000{{±|2,000|3,000}}
|0.37{{±|0.35|0.21}}
|
|Багато можливих розв'язків для мас планети і зорі<ref>{{citation|display-authors=1|arxiv=2104.02157|year=2021|title=OGLE-2018-BLG-1185b: A Low-mass Мікролінзування Planet Orbiting a Low-mass Dwarf|last1=Kondo|first1=Iona|last2=Yee|first2=Jennifer C.|last3=Bennett|first3=David P.|last4=Sumi|first4=Takahiro|last5=Koshimoto|first5=Naoki|last6=Bond|first6=Ian A.|last7=Gould|first7=Andrew|last8=Udalski|first8=Andrzej|last9=Shvartzvald|first9=Yossi|author10=Youn Kil Jung|last11=Zang|first11=Weicheng|last12=Bozza|first12=Valerio|last13=Bachelet|first13=Etienne|last14=Hundertmark|first14=Markus P. G.|last15=Rattenbury|first15=Nicholas J.|last16=Abe|first16=F.|last17=Barry|first17=R.|last18=Bhattacharya|first18=A.|last19=Donachie|first19=M.|last20=Fukui|first20=A.|last21=Fujii|first21=H.|last22=Hirao|first22=Y.|last23=Ishitani Silva|first23=S.|last24=Itow|first24=Y.|last25=Kirikawa|first25=R.|last26=Li|first26=M. C. A.|last27=Matsubara|first27=Y.|last28=Miyazaki|first28=S.|last29=Muraki|first29=Y.|last30=Olmschenk|first30=G.|journal=The Astronomical Journal|volume=162|issue=2|page=77|doi=10.3847/1538-3881/ac00ba|bibcode=2021AJ....162...77K|s2cid=233033627}}</ref>
|-
|[[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}}
| style="background:#FFFF00" |Транзит
|239.5{{±|0.3}}
|0.66{{±|0.01}}
|4,227{{±|85}}
|<ref name="Georgieva2021">{{citation|display-authors=1|arxiv=2104.05653|year=2021|title=Hot planets around cool stars – two short-period mini-Neptunes Транзитing the late K-dwarf TOI-1260|doi=10.1093/mnras/stab1464|last1=Georgieva|first1=I. Y.|last2=Persson|first2=C. M.|last3=Barragán|first3=O.|last4=Nowak|first4=G.|last5=Fridlund|first5=M.|last6=Locci|first6=D.|last7=Palle|first7=E.|last8=Luque|first8=R.|last9=Carleo|first9=I.|last10=Gandolfi|first10=D.|last11=Kane|first11=S. R.|last12=Korth|first12=J.|last13=Stassun|first13=K. G.|last14=Livingston|first14=J.|last15=Matthews|first15=E. C.|last16=Collins|first16=K. A.|last17=Howell|first17=S. B.|last18=Serrano|first18=L. M.|last19=Albrecht|first19=S.|last20=Bieryla|first20=A.|last21=Brasseur|first21=C. E.|last22=Ciardi|first22=D.|last23=Cochran|first23=W. D.|last24=Colon|first24=K. D.|last25=Crossfield|first25=I J M.|last26=Csizmadia|first26=Sz|last27=Deeg|first27=H. J.|last28=Esposito|first28=M.|last29=Furlan|first29=E.|last30=Gan|first30=T.|journal=Monthly Notices of the Royal Astronomical Society|volume=505|issue=4|pages=4684–4701}}</ref>
|-
|[[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}}
| style="background:#FFFF00" |Транзит
|239.5{{±|0.3}}
|0.66{{±|0.01}}
|4,227{{±|85}}
|<ref name="Georgieva2021" />
|-
|[[KMT-2018-BLG-1976Lb]]
|1.96{{±|1.23|1.12}}
|
|
|2.04{{±|0.72|0.83}}
|
| style="background:#0099FF" |Мікролінзування
|19,000{{±|2,000}}
|0.65{{±|0.41|0.37}}
|
|<ref name="Han2021">{{citation|display-authors=1|arxiv=2104.06544|year=2021|title=Three Мікролінзування planets with no caustic-crossing features|doi=10.1051/0004-6361/202140758|last1=Han|first1=Cheongho|last2=Udalski|first2=Andrzej|last3=Kim|first3=Doeon|last4=Lee|first4=Chung-Uk|last5=Albrow|first5=Michael D.|last6=Chung|first6=Sun-Ju|last7=Gould|first7=Andrew|last8=Hwang|first8=Kyu-Ha|last9=Jung|first9=Youn Kil|last10=Ryu|first10=Yoon-Hyun|last11=Shin|first11=In-Gu|last12=Shvartzvald|first12=Yossi|last13=Yee|first13=Jennifer C.|last14=Zang|first14=Weicheng|last15=Cha|first15=Sang-Mok|last16=Kim|first16=Dong-Jin|last17=Kim|first17=Hyoun-Woo|last18=Kim|first18=Seung-Lee|last19=Lee|first19=Dong-Joo|last20=Lee|first20=Yongseok|last21=Park|first21=Byeong-Gon|last22=Pogge|first22=Richard W.|last23=Mróz|first23=Przemek|last24=Szymański|first24=Michał K.|last25=Skowron|first25=Jan|last26=Poleski|first26=Radosław|last27=Soszyński|first27=Igor|last28=Pietrukowicz|first28=Paweł|last29=Kozłowski|first29=Szymon|last30=Ulaczyk|first30=Krzysztof|journal=Astronomy & Astrophysics|volume=650|pages=A89|bibcode=2021A&A...650A..89H|s2cid=233231384}}</ref>
|-
|[[KMT-2018-BLG-1996Lb]]
|1.22{{±|0.72|0.63}}
|
|
|1.97{{±|0.51|0.25}}
|
| style="background:#0099FF" |Мікролінзування
|19,000{{±|2,000}}
|0.69{{±|0.40|0.38}}
|
|<ref name="Han2021" />
|-
|[[OGLE-2019-BLG-0954Lb]]
|14.2{{±|9.9|7.5}}
|
|
|2.65{{±|0.89|1.20}}
|
| style="background:#0099FF" |Мікролінзування
|12,000{{±|1,000|2,000}}
|0.80{{±|0.55|0.42}}
|
|<ref name="Han2021" />
|-
|[[YSES 2 b]]
|6.3{{±|1.6|0.9}}
|
|
|115
|
| style="background:#FF6CDA" |Пряме спостереження
|356.4{{±|0.5}}
|1.10{{±|0.03}}
|4,749{{±|40}}
|<ref>{{citation|display-authors=1|arxiv=2104.08285|year=2021|title=Discovery of a directly imaged planet to the young solar analog YSES 2|doi=10.1051/0004-6361/202140508|last1=Bohn|first1=Alexander J.|last2=Ginski|first2=Christian|last3=Kenworthy|first3=Matthew A.|last4=Mamajek|first4=Eric E.|last5=Pecaut|first5=Mark J.|last6=Mugrauer|first6=Markus|last7=Vogt|first7=Nikolaus|last8=Adam|first8=Christian|last9=Meshkat|first9=Tiffany|last10=Reggiani|first10=Maddalena|last11=Snik|first11=Frans|journal=Astronomy & Astrophysics|volume=648|pages=A73|bibcode=2021A&A...648A..73B|s2cid=233296087}}</ref>
|-
|[[KMT-2016-BLG-2605b]]
|0.8{{±|1.2|0.4}}
|
|
|0.68{{±|0.11}}
|
| style="background:#0099FF" |Мікролінзування
|21,000{{±|3,000}}
|0.065{{±|0.10|0.035}}
|
|<ref>{{citation|display-authors=1|arxiv=2104.07906|year=2021|title=Shortest Мікролінзування Event with a Bound Planet: KMT-2016-BLG-2605|last1=Ryu|first1=Yoon-Hyun|last2=Hwang|first2=Kyu-Ha|last3=Gould|first3=Andrew|last4=Yee|first4=Jennifer C.|last5=Albrow|first5=Michael D.|last6=Chung|first6=Sun-Ju|last7=Han|first7=Cheongho|author8=Youn Kil Jung|last9=Kim|first9=Hyoun-Woo|last10=Shin|first10=In-Gu|last11=Shvartzvald|first11=Yossi|last12=Zang|first12=Weicheng|last13=Cha|first13=Sang-Mok|last14=Kim|first14=Dong-Jin|last15=Kim|first15=Seung-Lee|last16=Lee|first16=Chung-Uk|last17=Lee|first17=Dong-Joo|last18=Lee|first18=Yongseok|last19=Park|first19=Byeong-Gon|last20=Pogge|first20=Richard W.|journal=The Astronomical Journal|volume=162|issue=3|page=96|doi=10.3847/1538-3881/ac062a|bibcode=2021AJ....162...96R|s2cid=233289612}}</ref>
|-
|[[TOI-1431 b]] ('''MASCARA-5b''')
|3.14{{±|0.19|0.18}}
|1.51{{±|0.06}}
|2.65022{{±|0.00001}}
|0.047{{±|0.002}}
|2,370{{±|100}}
| style="background:#FFFF00" |Транзит
|488{{±|3}}
|1.90{{±|0.10|0.08}}
|7,690{{±|400|250}}
|<ref>{{citation|display-authors=1|arxiv=2104.12078|year=2021|title=TOI-1431b/MASCARA-5b: An Ultra-hot Jupiter Orbiting One of the Hottest & Brightest Known Exoplanet Host Stars|author1=Brett Christopher Addison|last2=Knudstrup|first2=Emil|last3=Wong|first3=Ian|last4=Hebrard|first4=Guillaume|last5=Dorval|first5=Patrick|last6=Snellen|first6=Ignas|last7=Albrecht|first7=Simon|last8=Bello-Arufe|first8=Aaron|last9=Almenara|first9=Jose-Manuel|last10=Boisse|first10=Isabelle|last11=Bonfils|first11=Xavier|last12=Dalal|first12=Shweta|last13=Demangeon|first13=Olivier|last14=Hoyer|first14=Sergio|last15=Kiefer|first15=Flavien|last16=Santos|first16=N. C.|last17=Nowak|first17=Grzegorz|last18=Luque|first18=Rafael|last19=Stangret|first19=Monika|last20=Palle|first20=Enric|last21=Tronsgaard|first21=Rene|last22=Antoci|first22=Victoria|last23=Buchhave|first23=Lars A.|last24=Gunther|first24=Maximilian N.|last25=Daylan|first25=Tansu|last26=Murgas|first26=Felipe|last27=Parviainen|first27=Hannu|last28=Esparza-Borges|first28=Emma|last29=Crouzet|first29=Nicolas|last30=Narita|first30=Norio|journal=Posters from the Tess Science Conference Ii (Tsc2|page=64|doi=10.5281/zenodo.5126266|bibcode=2021tsc2.confE..64A|s2cid=240578462}}</ref><ref>{{cite journal|last1=Stangret|first1=M.|last2=Pallé|first2=E.|last3=Casasayas-Barris|first3=N.|last4=Oshagh|first4=M.|last5=Bello-Arufe|first5=A.|last6=Luque|first6=R.|last7=Nascimbeni|first7=V.|last8=Yan|first8=F.|last9=Orell-Miquel|first9=J.|display-authors=1|year=2021|title=The obliquity and atmosphere of the ultra-hot Jupiter TOI-1431b (MASCARA-5b): A misaligned orbit and no signs of atomic or molecular absorptions|journal=Astronomy & Astrophysics|volume=654|pages=A73|arxiv=2104.12414|bibcode=2021A&A...654A..73S|doi=10.1051/0004-6361/202040100|mode=cs2|last10=Sicilia|first10=D.|last11=Malavolta|first11=L.|last12=Addison|first12=B. C.|last13=Buchhave|first13=L. A.|last14=Bonomo|first14=A. S.|last15=Borsa|first15=F.|last16=Cabot|first16=S. H. C.|last17=Cecconi|first17=M.|last18=Fischer|first18=D. A.|last19=Harutyunyan|first19=A.|last20=Mendonça|first20=J. M.|last21=Nowak|first21=G.|last22=Parviainen|first22=H.|last23=Sozzetti|first23=A.|last24=Tronsgaard|first24=R.|s2cid=233393996}}</ref>
|-
|[[TOI-269 b]]
|0.0277{{±|0.0044}}
|0.247{{±|0.011}}
|3.697723{{±|0.000018|0.000017}}
|0.0345{{±|0.0015}}
|531{{±|25}}
| style="background:#FFFF00" |Транзит
|186.01{{±|0.25}}
|0.3917{{±|0.0095}}
|3,514{{±|70}}
|<ref>{{citation|display-authors=1|arxiv=2104.14782|year=2021|title=TOI-269 b: An eccentric sub-Neptune Транзитing a M2 dwarf revisited with ExTrA|doi=10.1051/0004-6361/202140328|last1=Cointepas|first1=M.|last2=Almenara|first2=J. M.|last3=Bonfils|first3=X.|last4=Bouchy|first4=F.|last5=Astudillo-Defru|first5=N.|last6=Murgas|first6=F.|last7=Otegi|first7=J. F.|last8=Wyttenbach|first8=A.|last9=Anderson|first9=D. R.|last10=Artigau|first10=É.|last11=Canto Martins|first11=B. L.|last12=Charbonneau|first12=D.|last13=Collins|first13=K. A.|last14=Collins|first14=K. I.|last15=Correia|first15=J.-J.|last16=Curaba|first16=S.|last17=Delboulbé|first17=A.|last18=Delfosse|first18=X.|last19=Díaz|first19=R. F.|last20=Dorn|first20=C.|last21=Doyon|first21=R.|last22=Feautrier|first22=P.|last23=Figueira|first23=P.|last24=Forveille|first24=T.|last25=Gaisne|first25=G.|last26=Gan|first26=T.|last27=Gluck|first27=L.|last28=Helled|first28=R.|last29=Hellier|first29=C.|last30=Jocou|first30=L.|journal=Astronomy & Astrophysics|volume=650|pages=A145|bibcode=2021A&A...650A.145C|s2cid=233476660}}</ref>
|-
|[[TOI-220 b]]
|0.0434{{±|0.0031}}
|0.271{{±|0.013}}
|10.695264
|0.08911{{±|0.0010}}
|805{{±|21}}
| style="background:#FFFF00" |Транзит
|290{{±|13}}
|0.825{{±|0.028}}
|5,298{{±|65}}
|Припускається наявність додаткової планети з великим періодом<ref>{{citation|display-authors=1|arxiv=2105.01944|year=2021|title=TOI-220 b: A warm sub-Neptune discovered by TESS|doi=10.1093/mnras/stab1427|last1=Hoyer|first1=S.|last2=Gandolfi|first2=D.|last3=Armstrong|first3=D. J.|last4=Deleuil|first4=M.|last5=Acuña|first5=L.|last6=De Medeiros|first6=J. R.|last7=Goffo|first7=E.|last8=Lillo-Box|first8=J.|last9=Delgado Mena|first9=E.|last10=Lopez|first10=T. A.|last11=Santerne|first11=A.|last12=Sousa|first12=S.|last13=Fridlund|first13=M.|last14=Adibekyan|first14=V.|last15=Collins|first15=K. A.|last16=Serrano|first16=L. M.|last17=Cortés-Zuleta|first17=P.|last18=Howell|first18=S. B.|last19=Deeg|first19=H.|last20=Aguichine|first20=A.|last21=Barragán|first21=O.|last22=Bryant|first22=E. M.|last23=Canto Martins|first23=B. L.|last24=Collins|first24=K. I.|last25=Cooke|first25=B. F.|last26=Díaz|first26=R. F.|last27=Esposito|first27=M.|last28=Furlan|first28=E.|last29=Hojjatpanah|first29=S.|last30=Jackman|first30=J.|journal=Monthly Notices of the Royal Astronomical Society|volume=505|issue=3|pages=3361–3379}}</ref>
|-
|[[TOI 1062 b]]
|0.0320{{±|0.0026}}
|0.202{{±|0.008}}
|4.11412{{±|0.0014|0.0015}}
|0.052
|1,077{{±|10|9}}
| style="background:#FFFF00" |Транзит
|268.7{{±|0.2}}
|0.94{{±|0.02}}
|5,328{{±|56}}
|<ref name="Otegi2021">{{cite journal|last1=Otegi|first1=J. F.|last2=Bouchy|first2=F.|last3=Helled|first3=R.|last4=Armstrong|first4=D. J.|last5=Stalport|first5=M.|last6=Stassun|first6=K. G.|last7=Delgado-Mena|first7=E.|last8=Santos|first8=N. C.|last9=Collins|first9=K.|display-authors=1|year=2021|title=TESS and HARPS reveal two sub-Neptunes around TOI 1062|journal=Astronomy & Astrophysics|volume=653|pages=A105|arxiv=2105.01945|bibcode=2021A&A...653A.105O|doi=10.1051/0004-6361/202040247|mode=cs2|last10=Gandhi|first10=S.|last11=Dorn|first11=C.|last12=Brogi|first12=M.|last13=Fridlund|first13=M.|last14=Osborn|first14=H. P.|last15=Hoyer|first15=S.|last16=Udry|first16=S.|last17=Hojjatpanah|first17=S.|last18=Nielsen|first18=L. D.|last19=Dumusque|first19=X.|last20=Adibekyan|first20=V.|last21=Conti|first21=D.|last22=Schwarz|first22=R.|last23=Wang|first23=G.|last24=Figueira|first24=P.|last25=Lillo-Box|first25=J.|last26=Díaz|first26=R. F.|last27=Hadjigeorghiou|first27=A.|last28=Bayliss|first28=D.|last29=Strøm|first29=P. A.|last30=Sousa|first30=S. G.|s2cid=233739805}}</ref>
|-
|[[TOI 1062 c]]
|0.0294{{±|0.0039}}
|
|7.978{{±|0.021|0.023}}
|0.080{{±|0.013|0.012}}
|859{{±|9|8}}
| style="background:#00FF00" |Радіальна швидкість
|268.7{{±|0.2}}
|0.94{{±|0.02}}
|5,328{{±|56}}
|<ref name="Otegi2021" />
|-
|[[Kepler-129d]]
|8.3{{±|1.1|0.7}}
|
|2646{{±|140|94}}
|4.0{{±|0.1}}
|
| style="background:#00FF00" |Радіальна швидкість
|1,349{{±|14}}
|1.18
|5,770
|<ref>{{citation|display-authors=1|arxiv=2105.03446|year=2021|title=Long-period Jovian Tilts the Orbits of Two sub-Neptunes Relative to Stellar Spin Axis in Kepler-129|last1=Zhang|first1=Jingwen|last2=Weiss|first2=Lauren M.|last3=Huber|first3=Daniel|last4=Blunt|first4=Sarah|last5=Chontos|first5=Ashley|last6=Fulton|first6=Benjamin J.|last7=Grunblatt|first7=Samuel|last8=Howard|first8=Andrew W.|last9=Isaacson|first9=Howard|last10=Kosiarek|first10=Molly R.|last11=Petigura|first11=Erik A.|last12=Rosenthal|first12=Lee J.|last13=Rubenzahl|first13=Ryan A.|journal=The Astronomical Journal|volume=162|issue=3|page=89|doi=10.3847/1538-3881/ac0634|bibcode=2021AJ....162...89Z|s2cid=234338914}}</ref>
|-
|[[Gliese 9689 b]]
|0.0304{{±|0.0046}}
|
|18.27{{±|0.01}}
|0.1139{{±|0.0039}}
|453{{±|39}}
| style="background:#00FF00" |Радіальна швидкість
|100.10{{±|0.04}}
|0.59{{±|0.06}}
|3,836{{±|69}}
|<ref>{{citation|display-authors=1|arxiv=2105.06155|year=2021|title=HADES RV programme with HARPS-N at TNG|last1=Maldonado|first1=J.|last2=Petralia|first2=A.|last3=Damasso|first3=M.|last4=Pinamonti|first4=M.|last5=Scandariato|first5=G.|last6=González-Álvarez|first6=E.|last7=Affer|first7=L.|last8=Micela|first8=G.|last9=Lanza|first9=A. F.|last10=Leto|first10=G.|last11=Poretti|first11=E.|last12=Sozzetti|first12=A.|last13=Perger|first13=M.|last14=Giacobbe|first14=P.|last15=Zanmar Sánchez|first15=R.|last16=Maggio|first16=A.|last17=González Hernández|first17=J. I.|last18=Rebolo|first18=R.|last19=Ribas|first19=I.|last20=Suárez-Mascareño|first20=A.|last21=Toledo-Padrón|first21=B.|last22=Bignamini|first22=A.|last23=Molinari|first23=E.|last24=Covino|first24=E.|last25=Claudi|first25=R.|last26=Desidera|first26=S.|last27=Herrero|first27=E.|last28=Morales|first28=J. C.|last29=Pagano|first29=I.|last30=Piotto|first30=G.|journal=Astronomy & Astrophysics|volume=651|pages=A93|doi=10.1051/0004-6361/202141141|s2cid=234482717}}</ref>
|-
|[[TOI-1231 b]]
|0.0485{{±|0.0104}}
|0.326{{±|0.014}}
|24.245586{{±|0.000064|0.000066}}
|0.1288{{±|0.0021|0.0022}}
|330
| style="background:#FFFF00" |Транзит
|89.68{{±|0.04}}
|0.485{{±|0.024}}
|3,553{{±|31}}
|<ref>{{citation|display-authors=1|arxiv=2105.08077|year=2021|title=TOI-1231 b: A Temperate, Neptune-sized Planet Транзитing the Nearby M3 Dwarf NLTT 24399|last1=Burt|first1=Jennifer A.|last2=Dragomir|first2=Diana|last3=Mollière|first3=Paul|last4=Youngblood|first4=Allison|author5=Antonio García Muñoz|last6=McCann|first6=John|last7=Kreidberg|first7=Laura|last8=Huang|first8=Chelsea X.|last9=Collins|first9=Karen A.|last10=Eastman|first10=Jason D.|last11=Abe|first11=Lyu|last12=Almenara|first12=Jose M.|last13=Crossfield|first13=Ian J. M.|last14=Ziegler|first14=Carl|last15=Rodriguez|first15=Joseph E.|last16=Mamajek|first16=Eric E.|last17=Stassun|first17=Keivan G.|last18=Halverson|first18=Samuel P.|last19=Villanueva|first19=Steven Jr.|last20=Paul Butler|first20=R.|author21=Sharon Xuesong Wang|last22=Schwarz|first22=Richard P.|last23=Ricker|first23=George R.|last24=Vanderspek|first24=Roland|last25=Latham|first25=David W.|last26=Seager|first26=S.|last27=Winn|first27=Joshua N.|last28=Jenkins|first28=Jon M.|last29=Agabi|first29=Abdelkrim|last30=Bonfils|first30=Xavier|journal=The Astronomical Journal|volume=162|issue=3|page=87|doi=10.3847/1538-3881/ac0432|doi-access=free|bibcode=2021AJ....162...87B|s2cid=234763319|s2cid-access=free}}</ref>
|-
|[[TIC 172900988 b]]
|2.84{{±|0.25}}
|1.009{{±|0.043}}
|196.5{{±|7.7}}
|
|
| style="background:#FFFF00" |Транзит
|799{{±|9}}
|1.24 and 1.20
|6050 and 5983
|Планета в подвійній системі<ref>{{cite journal|last1=Kostov|first1=Veselin B.|last2=Powell|first2=Brian P.|last3=Orosz|first3=Jerome A.|last4=Welsh|first4=William F.|last5=Cochran|first5=William|last6=Collins|first6=Karen A.|last7=Endl|first7=Michael|last8=Hellier|first8=Coel|last9=Latham|first9=David W.|display-authors=1|year=2021|title=TIC 172900988: A Транзитing Circumbinary Planet Detected in One Sector of TESS Data|journal=The Astronomical Journal|volume=162|issue=6|page=234|arxiv=2105.08614|bibcode=2021AJ....162..234K|doi=10.3847/1538-3881/ac223a|mode=cs2|last10=MacQueen|first10=Phillip|last11=Pepper|first11=Joshua|last12=Quarles|first12=Billy|last13=Sairam|first13=Lalitha|last14=Torres|first14=Guillermo|last15=Wilson|first15=Robert F.|last16=Bergeron|first16=Serge|last17=Boyce|first17=Pat|last18=Buchheim|first18=Robert|author19=Caleb Ben Christiansen|last20=Ciardi|first20=David R.|last21=Collins|first21=Kevin I.|last22=Conti|first22=Dennis M.|last23=Dixon|first23=Scott|last24=Guerra|first24=Pere|last25=Haghighipour|first25=Nader|last26=Herman|first26=Jeffrey|last27=Hintz|first27=Eric G.|last28=Howard|first28=Ward S.|last29=Jensen|first29=Eric L. N.|last30=Kruse|first30=Ethan|s2cid=234762777}}</ref>
|-
|[[TOI-1444 b]]
|0.0122{{±|0.0022}}
|0.125{{±|0.006}}
|0.4702694{{±|0.0000044}}
|0.1288{{±|0.0021|0.0022}}
|330
| style="background:#FFFF00" |Транзит
|408.9{{±|0.5}}
|0.934{{±|0.038}}
|5,430{{±|90}}
|<ref>{{cite arXiv|mode=cs2|display-authors=1|eprint=2105.08844|year=2021|title=TKS X: Confirmation of TOI-1444b and a Comparative Analysis of the Ultra-short-period Planets with Hot Neptunes|last1=Dai|first1=Fei|last2=Howard|first2=Andrew W.|last3=Batalha|first3=Natalie M.|last4=Beard|first4=Corey|last5=Behmard|first5=Aida|last6=Blunt|first6=Sarah|last7=Brinkman|first7=Casey L.|last8=Chontos|first8=Ashley|last9=Crossfield|first9=Ian J. M.|last10=Dalba|first10=Paul A.|last11=Dressing|first11=Courtney|last12=Fulton|first12=Benjamin|last13=Giacalone|first13=Steven|last14=Hill|first14=Michelle L.|last15=Huber|first15=Daniel|last16=Isaacson|first16=Howard|last17=Kane|first17=Stephen R.|last18=Lubin|first18=Jack|last19=Mayo|first19=Andrew|last20=Mocnik|first20=Teo|last21=Akana Murphy|first21=Joseph M.|last22=Petigura|first22=Erik A.|last23=Rice|first23=Malena|last24=Robertson|first24=Paul|last25=Rosenthal|first25=Lee|last26=Roy|first26=Arpita|last27=Rubenzahl|first27=Ryan A.|last28=Weiss|first28=Lauren M.|author29=Judah Van Zandt|last30=Beichman|first30=Charles|class=astro-ph.EP}}</ref>
|-
|[[BD+45 0564|BD+45 0564 b]]
|1.36{{±|0.12}}
|
|307.88{{±|1.47}}
|0.83{{±|0.04}}
|
| style="background:#00FF00" |Радіальна швидкість
|174{{±|2}}
|0.81{{±|0.07}}
|5,004{{±|50}}
|<ref name="Dalal2021">{{citation|display-authors=1|arxiv=2105.09741|year=2021|title=The SOPHIE search for northern extrasolar planets|doi=10.1051/0004-6361/202140712|last1=Dalal|first1=S.|last2=Kiefer|first2=F.|last3=Hébrard|first3=G.|last4=Sahlmann|first4=J.|last5=Sousa|first5=S. G.|last6=Forveille|first6=T.|last7=Delfosse|first7=X.|last8=Arnold|first8=L.|last9=Astudillo-Defru|first9=N.|last10=Bonfils|first10=X.|last11=Boisse|first11=I.|last12=Bouchy|first12=F.|last13=Bourrier|first13=V.|last14=Brugger|first14=B.|last15=Cortés-Zuleta|first15=P.|last16=Deleuil|first16=M.|last17=Demangeon|first17=O. D. S.|last18=Díaz|first18=R. F.|last19=Hara|first19=N. C.|last20=Heidari|first20=N.|last21=Hobson|first21=M. J.|last22=Lopez|first22=T.|last23=Lovis|first23=C.|last24=Martioli|first24=E.|last25=Mignon|first25=L.|last26=Mousis|first26=O.|last27=Moutou|first27=C.|last28=Rey|first28=J.|last29=Santerne|first29=A.|last30=Santos|first30=N. C.|journal=Astronomy & Astrophysics|volume=651|pages=A11|s2cid=234790136}}</ref>
|-
|[[BD+55 0362|BD+55 0362 b]]
|0.72{{±|0.08}}
|
|265.59{{±|1.04}}
|0.78{{±|0.05}}
|
| style="background:#00FF00" |Радіальна швидкість
|168{{±|2}}
|0.909{{±|0.099}}
|5,012{{±|78}}
|Припускається наявність додаткової планети<ref name="Dalal2021" />
|-
|[[BD+63 1405|BD+63 1405 b]]
|3.96{{±|0.31}}
|
|1,198.48{{±|60.79}}
|2.06{{±|0.14}}
|
| style="background:#00FF00" |Радіальна швидкість
|124.4{{±|1.2}}
|0.82{{±|0.08}}
|5,000{{±|53}}
|Дуже витягнута орбіта<ref name="Dalal2021" />
|-
|[[HD 124330|HD 124330 b]]
|0.75{{±|0.06}}
|
|270.66{{±|1.21}}
|0.86{{±|0.04}}
|
| style="background:#00FF00" |Радіальна швидкість
|198{{±|3}}
|1.15{{±|0.079}}
|5,873{{±|19}}
|Припускається наявність додаткової планети<ref name="Dalal2021" />
|-
|[[HD 155193|HD 155193 b]]
|0.75{{±|0.06}}
|
|352.65{{±|2.58}}
|1.04{{±|0.04}}
|
| style="background:#00FF00" |Радіальна швидкість
|186{{±|6}}
|1.221{{±|0.083}}
|6,239{{±|20}}
|<ref name="Dalal2021" />
|-
|[[HD 331093|HD 331093 b]]
|1.50{{±|0.11}}
|
|621.62{{±|16.11}}
|1.44{{±|0.07}}
|
| style="background:#00FF00" |Радіальна швидкість
|164.07{{±|0.14}}
|1.030{{±|0.079}}
|5,544{{±|33}}
|<ref name="Dalal2021" />
|-
|[[HD 107148|HD 107148 c]]
|0.0626{{±|0.0097|0.0098}}
|
|18.3267{{±|0.0022|0.0024}}
|0.1406{{±|0.0018}}
|
| style="background:#00FF00" |Радіальна швидкість
|161.4{{±|0.4}}
|1.1{{±|0.1}}
|5,789{{±|36}}
|<ref name="Rosenthal2021">{{citation|display-authors=1|arxiv=2105.11583|year=2021|title=The California Legacy Survey. I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades|doi=10.3847/1538-4365/abe23c|last1=Rosenthal|first1=Lee J.|last2=Fulton|first2=Benjamin J.|last3=Hirsch|first3=Lea A.|last4=Isaacson|first4=Howard T.|last5=Howard|first5=Andrew W.|last6=Dedrick|first6=Cayla M.|last7=Sherstyuk|first7=Ilya A.|last8=Blunt|first8=Sarah C.|last9=Petigura|first9=Erik A.|last10=Knutson|first10=Heather A.|last11=Behmard|first11=Aida|last12=Chontos|first12=Ashley|last13=Crepp|first13=Justin R.|last14=Crossfield|first14=Ian J. M.|last15=Dalba|first15=Paul A.|last16=Fischer|first16=Debra A.|last17=Henry|first17=Gregory W.|last18=Kane|first18=Stephen R.|last19=Kosiarek|first19=Molly|last20=Marcy|first20=Geoffrey W.|last21=Rubenzahl|first21=Ryan A.|last22=Weiss|first22=Lauren M.|last23=Wright|first23=Jason T.|journal=The Astrophysical Journal Supplement Series|volume=255|issue=1|page=8|bibcode=2021ApJS..255....8R|s2cid=235186973}}</ref>
|-
|[[HD 136925|HD 136925 b]]
|0.84{{±|0.078|0.074}}
|
|4,540{{±|160|140}}
|5.13{{±|0.12|0.11}}
|
| style="background:#00FF00" |Радіальна швидкість
|156.2
|
|5715
|Припускається наявність додаткової планети<ref name="Rosenthal2021" />
|-
|[[Лямбда Змії b]]
|0.0428{{±|0.0047|0.0045}}
|
|15.5083{{±|0.0016|0.0018}}
|0.1238{{±|0.002}}
|
| style="background:#00FF00" |Радіальна швидкість
|38.87{{±|0.07}}
|1.14
|5,884{{±|4}}
|<ref name="Rosenthal2021" />
|-
|[[HD 156668|HD 156668 c]]
|0.0991{{±|0.0079|0.0077}}
|
|811.3{{±|5.2|5.3}}
|1.570{{±|0.017}}
|
| style="background:#00FF00" |Радіальна швидкість
|79.34{{±|0.03}}
|0.772{{±|0.020}}
|4,850{{±|88}}
|Припускається наявність додаткової планети<ref name="Rosenthal2021" />
|-
|[[HD 164922|HD 164922 e]]
|0.0331{{±|0.0031}}
|
|41.763{{±|0.012}}
|0.2293{{±|0.0026|0.0027}}
|
| style="background:#00FF00" |Радіальна швидкість
|71.69{{±|0.03}}
|0.874{{±|0.012}}
|5,293{{±|32}}
|<ref name="Rosenthal2021" />
|-
|[[HD 168009|HD 168009 b]]
|0.0300{{±|0.0038|0.0037}}
|
|15.1479{{±|0.0035|0.0037}}
|0.1192{{±|0.0017|0.0018}}
|
| style="background:#00FF00" |Радіальна швидкість
|75.97{{±|0.03}}
|0.99
|5,792{{±|80}}
|<ref name="Rosenthal2021" />
|-
|[[HD 213472|HD 213472 b]]
|3.48{{±|1.10|0.59}}
|
|16,700{{±|12,000|4,800}}
|13.0{{±|5.7|2.6}}
|
| style="background:#00FF00" |Радіальна швидкість
|210.6
|
|
|<ref name="Rosenthal2021" />
|-
|[[HD 24040|HD 24040 c]]
|0.201{{±|0.027}}
|
|515.4{{±|2.2|2.5}}
|1.3{{±|0.021}}
|
| style="background:#00FF00" |Радіальна швидкість
|152.3{{±|0.4}}
|1.14{{±|0.02}}
|5,917{{±|52}}
|<ref name="Rosenthal2021" />
|-
|[[HD 26161|HD 26161 b]]
|13.5{{±|8.5|3.7}}
|
|32,000{{±|21,000|10,000}}
|20.4{{±|7.9|4.9}}
|
| style="background:#00FF00" |Радіальна швидкість
|133.6{{±|0.3}}
|
|
|Дуже витягнута орбіта; в системі також є червоний карлик<ref name="Rosenthal2021" />
|-
|[[HD 3765|HD 3765 b]]
|0.173{{±|0.014|0.013}}
|
|1,211{{±|15|16}}
|2.108{{±|0.032|0.033}}
|
| style="background:#00FF00" |Радіальна швидкість
|78.5{{±|0.1}}
|
|
|<ref name="Rosenthal2021" />
|-
|[[HD 66428|HD 66428 c]]
|27{{±|22|17}}
|
|39,000{{±|56,000|18,000}}
|23.0{{±|19.0|7.6}}
|
| style="background:#00FF00" |Радіальна швидкість
|174.1{{±|0.7}}
|1.09{{±|0.02}}
|5,773{{±|55}}
|<ref name="Rosenthal2021" />
|-
|[[HD 68988 c]]
|15.0{{±|2.8|1.5}}
|
|16,100{{±|11,000|3,500}}
|13.2{{±|5.3|2.0}}
|
| style="background:#00FF00" |Радіальна швидкість
|198.8{{±|0.6}}
|1.16{{±|0.01}}
|5,919{{±|11}}
|Кандидат з 2006<ref name="Rosenthal2021" />
|-
|[[Lalande 21185|Lalande 21185 c]]
|0.0568{{±|0.0091|0.0083}}
|
|3190{{±|200|170}}
|3.1{{±|0.13|0.11}}
|
| style="background:#00FF00" |Радіальна швидкість
|8.31{{±|0.01}}
|0.390{{±|0.011}}
|3,601{{±|51}}
|<ref name="Rosenthal2021" />
|-
|[[G 264-12|G 264-12 b]]
|0.0079{{±|0.0009}}
|
|2.30538{{±|0.00031}}
|0.02279{{±|0.00061}}
|587{{±|16}}
| style="background:#00FF00" |Радіальна швидкість
|52.14{{±|0.03}}
|0.297{{±|0.024}}
|3,326{{±|54}}
|<ref name="Amado2021">{{cite journal|last1=Amado|first1=Pedro J.|last2=Bauer|first2=Florian F.|last3=Rodríguez López|first3=Cristina|last4=Rodríguez|first4=Eloy|last5=Cardona Guillén|first5=C.|last6=Perger|first6=M.|last7=Caballero|first7=José A.|last8=López-González|first8=Maria J.|last9=Muñoz Rodríguez|first9=I.|date=2021-05-28|title=The CARMENES search for exoplanets around M dwarfs|journal=Astronomy & Astrophysics|volume=650|pages=A188|arxiv=2105.13785|doi=10.1051/0004-6361/202140633|last10=Pozuelos|first10=F. J.|last11=Sánchez-Rivero|first11=A.|last12=Schlecker|first12=M.|last13=Quirrenbach|first13=Andreas|last14=Ribas|first14=Ignasi|last15=Reiners|first15=Ansgar|last16=Almenara|first16=J.|last17=Astudillo-Defru|first17=N.|last18=Azzaro|first18=M.|last19=Béjar|first19=Victor J. S.|last20=Bohemann|first20=R.|last21=Bonfils|first21=X.|last22=Bouchy|first22=F.|last23=Cifuentes|first23=C.|last24=Cortés-Contreras|first24=M.|last25=Delfosse|first25=Xavier|last26=Dreizler|first26=Stefan|last27=Forveille|first27=Thierry|last28=Hatzes|first28=Artie P.|last29=Henning|first29=Thomas K.|last30=Jeffers|first30=Sandra V.|last31=Kaminski|first31=Adrian|last32=Kürster|first32=Martin|last33=Lafarga|first33=M.|last34=Lodieu|first34=Nicolas|last35=Lovis|first35=C.|last36=Mayor|first36=M.|last37=Montes|first37=David|last38=Morales|first38=Juan Carlos|last39=Morales|first39=Nicolás|last40=Murgas|first40=F.|last41=Ortiz|first41=José L.|last42=Pepe|first42=F.|last43=Perdelwitz|first43=V.|last44=Pollaco|first44=D.|last45=Santos|first45=N. C.|last46=Schöfer|first46=P.|last47=Schweitzer|first47=A.|last48=Ségransan|first48=N. C.|last49=Shan|first49=Y.|last50=Stock|first50=S.|last51=Tal-Or|first51=Lev|last52=Udry|first52=S.|last53=Zapatero-Osorio|first53=María Rosa|last54=Zechmeister|first54=Mathias|s2cid=235248027}}</ref>
|-
|[[G 264-12|G 264-12 c]]
|0.0118{{±|0.0015}}
|
|8.0518{{±|0.0034}}
|0.0525{{±|0.0014}}
|387{{±|11}}
| style="background:#00FF00" |Радіальна швидкість
|52.14{{±|0.03}}
|0.297{{±|0.024}}
|3,326{{±|54}}
|<ref name="Amado2021" />
|-
|[[Gliese 393|Gliese 393 b]]
|0.0054{{±|0.0008}}
|
|7.02679{{±|0.00082|0.00085}}
|0.05402{{±|0.00072}}
|485{{±|11}}
| style="background:#00FF00" |Радіальна швидкість
|22.956{{±|0.008}}
|0.426{{±|0.017}}
|3,579{{±|51}}
|<ref name="Amado2021" />
|-
|[[TOI-674b]]
|0.0739{{±|0.0104}}
|0.470{{±|0.016}}
|1.977143{{±|0.000003}}
|0.0231{{±|0.0007}}
|661{{±|14}}
| style="background:#FFFF00" |Транзит
|150.86{{±|0.11}}
|0.442{{±|0.007}}
|3,505{{±|28|32}}
|Можлива атмосфера з пару<ref>{{citation|display-authors=1|arxiv=2106.01246|year=2021|title=TOI-674b: An oasis in the desert of exo-Neptunes Транзитing a nearby M dwarf|last1=Murgas|first1=F.|last2=Astudillo-Defru|first2=N.|last3=Bonfils|first3=X.|last4=Crossfield|first4=Ian|last5=Almenara|first5=J. M.|last6=Livingston|first6=John|last7=Stassun|first7=Keivan G.|last8=Korth|first8=Judith|last9=Orell-Miquel|first9=Jaume|last10=Morello|first10=G.|last11=Eastman|first11=Jason D.|last12=Lissauer|first12=Jack J.|last13=Kane|first13=Stephen R.|last14=Morales|first14=Farisa Y.|last15=Werner|first15=Michael W.|last16=Gorjian|first16=Varoujan|last17=Benneke|first17=Björn|last18=Dragomir|first18=Diana|last19=Matthews|first19=Elisabeth C.|last20=Howell|first20=Steve B.|last21=Ciardi|first21=David|last22=Gonzales|first22=Erica|last23=Matson|first23=Rachel|last24=Beichman|first24=Charles|last25=Schlieder|first25=Joshua|last26=Collins|first26=Karen A.|last27=Collins|first27=Kevin I.|last28=Jensen|first28=Eric L. N.|last29=Evans|first29=Phil|last30=Pozuelos|first30=Francisco J.|journal=Astronomy & Astrophysics|volume=653|pages=A60|doi=10.1051/0004-6361/202140718|bibcode=2021A&A...653A..60M|s2cid=235294286}}</ref><ref>{{citation|arxiv=2201.04197|year=2022|title=A Mirage or an Oasis? Water Vapor in the Atmosphere of the Warm Neptune TOI-674 B|last1=Brande|first1=Jonathan|last2=Crossfield|first2=Ian J. M.|last3=Kreidberg|first3=Laura|last4=Oklopčić|first4=Antonija|last5=Polanski|first5=Alex S.|last6=Barman|first6=Travis|last7=Benneke|first7=Björn|last8=Christiansen|first8=Jessie L.|last9=Dragomir|first9=Diana|last10=Foreman-Mackey|first10=Daniel|last11=Fortney|first11=Jonathan J.|last12=Greene|first12=Thomas P.|last13=Howard|first13=Andrew W.|last14=Knutson|first14=Heather A.|last15=Lothringer|first15=Joshua D.|last16=Mikal-Evans|first16=Thomas|last17=Morley|first17=Caroline V.|journal=The Astronomical Journal|volume=164|issue=5|page=197|doi=10.3847/1538-3881/ac8b7e|s2cid=245877576}}</ref>
|-
|[[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}}
|
| style="background:#FFFF00" |Транзит
|352.0{{±|1.0}}
|1.15{{±|0.04}}
|6,310{{±|100}}
|<ref name="Eisner2021">{{citation|display-authors=1|arxiv=2106.04603|year=2021|title=Planet Hunters TESS III: Two Транзитing planets around the bright G dwarf HD 152843|doi=10.1093/mnras/stab1253|last1=Eisner|first1=N. L.|last2=Nicholson|first2=B. A.|last3=Barragán|first3=O.|last4=Aigrain|first4=S.|last5=Lintott|first5=C.|last6=Kaye|first6=L.|last7=Klein|first7=B.|last8=Miller|first8=G.|last9=Taylor|first9=J.|last10=Zicher|first10=N.|last11=Buchhave|first11=L. A.|last12=Caldwell|first12=D. A.|last13=Horner|first13=J.|last14=Llama|first14=J.|last15=Mortier|first15=A.|last16=Rajpaul|first16=V. M.|last17=Stassun|first17=K.|last18=Sporer|first18=A.|last19=Tkachenko|first19=A.|last20=Jenkins|first20=J. M.|last21=Latham|first21=D.|last22=Ricker|first22=G.|last23=Seager|first23=S.|last24=Winn|first24=J.|last25=Alhassan|first25=S.|last26=Baeten|first26=E M L.|last27=Bean|first27=S. J.|last28=Bundy|first28=D. M.|last29=Efremov|first29=V.|last30=Ferstenou|first30=R.|journal=Monthly Notices of the Royal Astronomical Society|volume=505|issue=2|pages=1827–1840}}</ref>
|-
|[[HD 152843 c]]
|0.0865
|0.521{{±|0.013}}
|24.38{{±|6.23|3.4}}
|
|
| style="background:#FFFF00" |Транзит
|352.0{{±|1.0}}
|1.15{{±|0.04}}
|6,310{{±|100}}
|<ref name="Eisner2021" />
|-
|[[KMT-2019-BLG-0253b]]
|0.029{{±|0.016|0.013}}
|
|
|3.1{{±|0.8|0.9}}
|
| style="background:#0099FF" |Мікролінзування
|16,000{{±|6,000|5,000}}
|0.70{{±|0.34|0.31}}
|
|<ref name="Hwang2021">{{cite journal|last1=Hwang|first1=Kyu-Ha|last2=Zang|first2=Weicheng|last3=Gould|first3=Andrew|last4=Udalski|first4=Andrzej|last5=Bond|first5=Ian A.|last6=Yang|first6=Hongjing|last7=Mao|first7=Shude|last8=Albrow|first8=Michael D.|last9=Chung|first9=Sun-Ju|display-authors=1|year=2021|title=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|mode=cs2|last10=Han|first10=Cheongho|author11=Youn Kil Jung|last12=Ryu|first12=Yoon-Hyun|last13=Shin|first13=In-Gu|last14=Shvartzvald|first14=Yossi|last15=Yee|first15=Jennifer C.|last16=Cha|first16=Sang-Mok|last17=Kim|first17=Dong-Jin|last18=Kim|first18=Hyoun-Woo|last19=Kim|first19=Seung-Lee|last20=Lee|first20=Chung-Uk|last21=Lee|first21=Dong-Joo|last22=Lee|first22=Yongseok|last23=Park|first23=Byeong-Gon|last24=Pogge|first24=Richard W.|last25=Mróz|first25=Przemek|last26=Poleski|first26=Radek|last27=Skowron|first27=Jan|last28=Szymański|first28=Michal K.|last29=Soszyński|first29=Igor|last30=Pietrukowicz|first30=Pawel|s2cid=245740102}}</ref>
|-
|[[OGLE-2018-BLG-0506]]
|0.051{{±|0.038|0.027}}
|
|
|3.0{{±|0.7|0.8}}
|
| style="background:#0099FF" |Мікролінзування
|18,000{{±|5,000}}
|0.63{{±|0.37|0.32}}
|
|<ref name="Hwang2021" />
|-
|[[OGLE-2018-BLG-0516]]
|0.063{{±|0.052|0.034}}
|
|
|2.2{{±|0.8|0.7}}
|
| style="background:#0099FF" |Мікролінзування
|7,000{{±|3,000|2,000}}
|0.47{{±|0.38|0.25}}
|
|<ref name="Hwang2021" />
|-
|[[OGLE-2019-BLG-1492]]
|0.117{{±|0.079|0.061}}
|
|
|2.7{{±|0.9}}
|
| style="background:#0099FF" |Мікролінзування
|18,000{{±|6,000|7,000}}
|0.68{{±|0.34}}
|
|<ref name="Hwang2021" />
|-
|[[OGLE-2018-BLG-0977]]
|0.020{{±|0.016|0.012}}
|
|
|2.0{{±|0.6|0.5}}
|
| style="background:#0099FF" |Мікролінзування
|7,000{{±|2,000}}
|0.47{{±|0.38|0.27}}
|
|<ref name="Hwang2021" />
|-
|[[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}}
| style="background:#FFFF00" |Транзит
|729{{±|3}}
|1.499{{±|0.061|0.15}}
|5,984{{±|55|57}}
|<ref>{{cite journal|last1=Khandelwal|first1=Akanksha|last2=Chaturvedi|first2=Priyanka|last3=Chakraborty|first3=Abhijit|last4=Sharma|first4=Rishikesh|last5=Guenther|first5=Eike. W.|last6=Persson|first6=Carina M.|last7=Fridlund|first7=Malcolm|last8=Hatzes|first8=Artie P.|last9=Prasad|first9=Neelam J. S. S. V.|display-authors=1|year=2021|title=Discovery of an inflated hot Jupiter around a slightly evolved star TOI-1789|journal=Monthly Notices of the Royal Astronomical Society|arxiv=2106.08660|doi=10.1093/mnras/stab2970|mode=cs2|last10=Esposito|first10=Massimiliano|last11=Chamarthi|first11=Sireesha|last12=Nayak|first12=Ashirbad|author13=Dishendra}}</ref>
|-
|[[TOI-942 b]]
|
|0.347{{±|0.022|0.020}}
|4.32421{{±|0.000019}}
|0.04866{{±|0.00016|0.00013}}
|
| style="background:#FFFF00" |Транзит
|493.9{{±|1.0}}
|0.8220{{±|0.0079|0.0064}}
|
|<ref name="Wirth2021">{{citation|display-authors=1|arxiv=2106.14968|year=2021|title=TOI-942b: A Prograde Neptune in a ∼ 60 Myr Old Multi-Транзитing System|last1=Wirth|first1=Christopher P.|last2=Zhou|first2=George|last3=Quinn|first3=Samuel N.|last4=Mann|first4=Andrew W.|last5=Bouma|first5=Luke G.|last6=Latham|first6=David W.|last7=Teske|first7=Johanna K.|last8=Wang|first8=Sharon X.|last9=Shectman|first9=Stephen A.|last10=Butler|first10=R. P.|last11=Crane|first11=Jeffrey D.|journal=The Astrophysical Journal Letters|volume=917|issue=2|pages=L34|doi=10.3847/2041-8213/ac13a9|bibcode=2021ApJ...917L..34W|s2cid=235670113}}</ref>
|-
|[[TOI-942 c]]
|
|0.417{{±|0.030|0.027}}
|10.156272{{±|0.000037|0.000034}}
|0.08598{{±|0.00027|0.00022}}
|
| style="background:#FFFF00" |Транзит
|493.9{{±|1.0}}
|0.8220{{±|0.0079|0.0064}}
|
|<ref name="Wirth2021" />
|-
|[[KMT-2018-BLG-1743]]
|0.245{{±|0.339|0.135}}
|
|
|1.449{{±|0.209|0.229}}
|
| style="background:#0099FF" |Мікролінзування
|21,000{{±|3,000}}
|0.193{{±|0.268|0.107}}
|
|Подвійна материнська зоря<ref>{{citation|display-authors=1|arxiv=2107.00155|year=2021|title=KMT-2018-BLG-1743: Planetary Мікролінзування event occurring on two source stars|last1=Han|first1=Cheongho|last2=Albrow|first2=Michael D.|last3=Chung|first3=Sun-Ju|last4=Gould|first4=Andrew|last5=Hwang|first5=Kyu-Ha|author6=Youn Kil Jung|last7=Kim|first7=Doeon|last8=Kim|first8=Hyoun-Woo|last9=Lee|first9=Chung-Uk|last10=Ryu|first10=Yoon-Hyun|last11=Shin|first11=In-Gu|last12=Shvartzvald|first12=Yossi|last13=Yee|first13=Jennifer C.|last14=Zang|first14=Weicheng|last15=Cha|first15=Sang-Mok|last16=Kim|first16=Dong-Jin|last17=Kim|first17=Seung-Lee|last18=Lee|first18=Dong-Joo|last19=Lee|first19=Yongseok|last20=Park|first20=Byeong-Gon|last21=Pogge|first21=Richard W.|journal=Astronomy & Astrophysics|volume=652|pages=A145|doi=10.1051/0004-6361/202140923|bibcode=2021A&A...652A.145H|s2cid=235694685}}</ref>
|-
|[[TOI-1749|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}}
| style="background:#FFFF00" |Транзит
|324.8{{±|0.4}}
|0.58{{±|0.03}}
|3,985{{±|55}}
|<ref name="Fukui2021">{{cite journal|last1=Fukui|first1=A.|last2=Korth|first2=J.|last3=Livingston|first3=J. H.|last4=Twicken|first4=J. D.|last5=Zapatero Osorio|first5=M. R.|last6=Jenkins|first6=J. M.|last7=Mori|first7=M.|last8=Murgas|first8=F.|last9=Ogihara|first9=M.|display-authors=1|year=2021|title=TOI-1749: An M dwarf with a Trio of Planets including a Near-resonant Pair|journal=The Astronomical Journal|volume=162|issue=4|page=167|arxiv=2107.05430|bibcode=2021AJ....162..167F|doi=10.3847/1538-3881/ac13a5|mode=cs2|last10=Narita|first10=N.|last11=Pallé|first11=E.|last12=Stassun|first12=K. G.|last13=Nowak|first13=G.|last14=Ciardi|first14=D. R.|last15=Alvarez-Hernandez|first15=L.|last16=Béjar|first16=V. J. S.|last17=Casasayas-Barris|first17=N.|last18=Crouzet|first18=N.|last19=de Leon|first19=J. P.|last20=Esparza-Borges|first20=E.|last21=Hidalgo Soto|first21=D.|last22=Isogai|first22=K.|last23=Kawauchi|first23=K.|last24=Klagyivik|first24=P.|last25=Kodama|first25=T.|last26=Kurita|first26=S.|last27=Kusakabe|first27=N.|last28=Luque|first28=R.|last29=Madrigal-Aguado|first29=A.|last30=Montanes Rodriguez|first30=P.|s2cid=235795469}}</ref>
|-
|[[TOI-1749|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}}
| style="background:#FFFF00" |Транзит
|324.8{{±|0.4}}
|0.58{{±|0.03}}
|3,985{{±|55}}
|<ref name="Fukui2021" />
|-
|[[TOI-1749|TOI-1749 d]]
|0.014{{±|0.020|0.011}}
|0.225{{±|0.013}}
|9.04455{{±|0.00012}}
|0.0707{{±|0.0012}}
|533{{±|12}}
| style="background:#FFFF00" |Транзит
|324.8{{±|0.4}}
|0.58{{±|0.03}}
|3,985{{±|55}}
|<ref name="Fukui2021" />
|-
|[[HD 27969|HD 27969 b]]
|4.80{{±|0.24|0.23}}
|
|654.5{{±|5.7|5.8}}
|1.552{{±|0.032|0.033}}
|261{{±|11}}
| style="background:#00FF00" |Радіальна швидкість
|
|1.16{{±|0.07}}
|5,966{{±|21}}
|<ref name="Demangeon2021">{{cite journal|last1=Demangeon|first1=O. D. S.|last2=Dalal|first2=S.|last3=Hébrard|first3=G.|last4=Nsamba|first4=B.|last5=Kiefer|first5=F.|last6=Camacho|first6=J. D.|last7=Sahlmann|first7=J.|last8=Arnold|first8=L.|last9=Astudillo-Defru|first9=N.|display-authors=1|year=2021|title=The SOPHIE search for northern extrasolar planets|journal=Astronomy & Astrophysics|volume=653|pages=A78|arxiv=2107.05089|doi=10.1051/0004-6361/202141079|mode=cs2|last10=Bonfils|first10=X.|last11=Boisse|first11=I.|last12=Bouchy|first12=F.|last13=Bourrier|first13=V.|last14=Campante|first14=T.|last15=Delfosse|first15=X.|last16=Deleuil|first16=M.|last17=Díaz|first17=R. F.|last18=Faria|first18=J.|last19=Forveille|first19=T.|last20=Hara|first20=N.|last21=Heidari|first21=N.|last22=Hobson|first22=M. J.|last23=Lopez|first23=T.|last24=Moutou|first24=C.|last25=Rey|first25=J.|last26=Santerne|first26=A.|last27=Sousa|first27=S.|last28=Santos|first28=N. C.|last29=Strøm|first29=P. A.|last30=Tsantaki|first30=M.|s2cid=235795175}}</ref>
|-
|[[HD 80869|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}}
| style="background:#00FF00" |Радіальна швидкість
|
|1.08{{±|0.05}}
|5,837{{±|15}}
|Дуже витягнута орбіта<ref name="Demangeon2021" />
|-
|[[HD 95544|HD 95544 b]]
|6.84{{±|0.31}}
|
|2172{{±|23|21}}
|3.386{{±|0.075|0.077}}
|156.5{{±|5.4|5.5}}
| style="background:#00FF00" |Радіальна швидкість
|
|1.09{{±|0.07}}
|5,722{{±|15}}
|<ref name="Demangeon2021" />
|-
|[[HD 109286|HD 109286 b]]
|2.99{{±|0.15}}
|
|520.1{{±|2.3}}
|1.259{{±|0.021}}
|259.4{{±|5.5}}
| style="background:#00FF00" |Радіальна швидкість
|
|0.98{{±|0.05}}
|5,694{{±|23}}
|<ref name="Demangeon2021" />
|-
|[[HD 115954|HD 115954 b]]
|8.29{{±|0.75|0.58}}
|
|3700{{±|1500|390}}
|5.00{{±|1.3|0.36}}
|144.9{{±|8.1|13}}
| style="background:#00FF00" |Радіальна швидкість
|
|1.18{{±|0.06}}
|5957{{±|26}}
|<ref name="Demangeon2021" />
|-
|[[HD 211403|HD 211403 b]]
|5.54{{±|0.39|0.38}}
|
|223.8{{±|0.41}}
|0.768{{±|0.013}}
|380{{±|13}}
| style="background:#00FF00" |Радіальна швидкість
|
|1.20{{±|0.06}}
|6,273{{±|44}}
|<ref name="Demangeon2021" />
|-
|[[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}}
| style="background:#FFFF00" |Транзит
|2,690{{±|40}}
|1.131{{±|0.040|0.051}}
|5,745{{±|88|89}}
|Дуже витягнута орбіта (e=0.921)<ref>{{cite journal|last1=Dalba|first1=Paul A.|last2=Kane|first2=Stephen R.|last3=Li|first3=Zhexing|last4=Macdougall|first4=Mason G.|last5=Rosenthal|first5=Lee J.|last6=Cherubim|first6=Collin|last7=Isaacson|first7=Howard|last8=Thorngren|first8=Daniel P.|last9=Fulton|first9=Benjamin|display-authors=1|year=2021|title=Giant Outer Транзитing Exoplanet Mass (GOT 'EM) Survey. II. Discovery of a Failed Hot Jupiter on a 2.7 Yr, Highly Eccentric Orbit|journal=The Astronomical Journal|volume=162|issue=4|page=154|arxiv=2107.06901|bibcode=2021AJ....162..154D|doi=10.3847/1538-3881/ac134b|mode=cs2|last10=Howard|first10=Andrew W.|last11=Petigura|first11=Erik A.|last12=Schwieterman|first12=Edward W.|last13=Peluso|first13=Dan O.|last14=Esposito|first14=Thomas M.|last15=Marchis|first15=Franck|last16=Payne|first16=Matthew J.|s2cid=235898945}}</ref>
|-
|[[TOI-532b]]
|0.1935{{±|0.0305|0.0293}}
|0.520{{±|0.017}}
|2.3266508{{±|0.0000030}}
|0.0296{{±|0.00035}}
|867{{±|18}}
| style="background:#FFFF00" |Транзит
|439.1{{±|1.2}}
|0.639{{±|0.023}}
|3927{{±|37}}
|<ref>{{citation|display-authors=1|arxiv=2107.13670|year=2021|title=TOI-532b: The Habitable-zone Planet Finder confirms a Large Super Neptune in the Neptune Desert orbiting a metal-rich M-dwarf host|last1=Kanodia|first1=Shubham|last2=Stefansson|first2=Gudmundur|last3=Canas|first3=Caleb I.|last4=Maney|first4=Marissa|last5=Lin|first5=Andrea S.|last6=Ninan|first6=Joe P.|last7=Jones|first7=Sinclaire|last8=Monson|first8=Andrew J.|last9=Parker|first9=Brock A.|last10=Kobulnicky|first10=Henry A.|last11=Rothenberg|first11=Jason|last12=Beard|first12=Corey|last13=Lubin|first13=Jack|last14=Robertson|first14=Paul|last15=Gupta|first15=Arvind F.|last16=Mahadevan|first16=Suvrath|last17=Cochran|first17=William D.|last18=Bender|first18=Chad F.|last19=Diddams|first19=Scott A.|last20=Fredrick|first20=Connor|last21=Halverson|first21=Samuel P.|last22=Hawley|first22=Suzanne L.|last23=Hearty|first23=Fred R.|last24=Hebb|first24=Leslie|last25=Kopparapu|first25=Ravi K.|last26=Metcalf|first26=Andrew J.|last27=Ramsey|first27=Lawrence W.|last28=Roy|first28=Arpita|last29=Schwab|first29=Christian|last30=Schutte|first30=Maria|journal=The Astronomical Journal|volume=162|issue=4|page=135|doi=10.3847/1538-3881/ac1940|bibcode=2021AJ....162..135K|s2cid=236493328}}</ref>
|-
|[[TOI-2406b]]
|0.0286{{±|0.0223|0.0126}}
|0.263{{±|0.015|0.014}}
|3.0766896{{±|0.0000065}}
|0.0228{{±|0.0016}}
|447{{±|15}}
| style="background:#FFFF00" |Транзит
|181.4{{±|0.4}}
|0.162{{±|0.008}}
|3,100{{±|75}}
|<ref>{{cite journal|last1=Wells|first1=R. D.|last2=Rackham|first2=B. V.|last3=Schanche|first3=N.|last4=Petrucci|first4=R.|last5=Gomez Maqueo Chew|first5=Y.|last6=Demory|first6=B. -O.|last7=Burgasser|first7=A. J.|last8=Burn|first8=R.|last9=Pozuelos|first9=F. J.|display-authors=1|year=2021|title=A large sub-Neptune Транзитing the thick-disk M4 V TOI-2406|journal=Astronomy & Astrophysics|volume=653|pages=A97|arxiv=2107.14125|bibcode=2021A&A...653A..97W|doi=10.1051/0004-6361/202141277|mode=cs2|last10=Gunther|first10=M. N.|last11=Sabin|first11=L.|last12=Schroffenegger|first12=U.|last13=Gomez-Munoz|first13=M. A.|last14=Stassun|first14=K. G.|last15=Van Grootel|first15=V.|last16=Howell|first16=S. B.|last17=Sebastian|first17=D.|last18=Triaud|first18=A. H. M. J.|last19=Apai|first19=D.|last20=Plauchu-Frayn|first20=I.|last21=Guerrero|first21=C. A.|last22=Guillen|first22=P. F.|last23=Landa|first23=A.|last24=Melgoza|first24=G.|last25=Montalvo|first25=F.|last26=Serrano|first26=H.|last27=Riesgo|first27=H.|last28=Barkaoui|first28=K.|last29=Bixel|first29=A.|last30=Burdanov|first30=A.|s2cid=236493492}}</ref>
|-
|[[KIC 8121913 b]]
|2.1{{±|0.4}}
|
|3.294601{{±|0.000013|0.00022}}
|
|
| style="background:#00c9c2" |Модуляція яскравості
|2350
|1.456{{±|0.069|0.15}}
|5075.3{{±|110.2|109.4}}
|<ref name="Lillo-Box2021">{{cite journal|last1=Lillo-Box|first1=J.|last2=Millholland|first2=S.|last3=Laughlin|first3=G.|display-authors=1|year=2021|title=Follow-up of non-Транзитing planets detected by Kepler|journal=Astronomy & Astrophysics|volume=654|pages=A9|arxiv=2107.14621|doi=10.1051/0004-6361/202140746|mode=cs2|s2cid=236635201}}</ref>
|-
|[[KIC 10068024 b]]
|2.0{{±|0.4}}
|
|2.073549{{±|0.000008|0.000177}}
|
|
| style="background:#00c9c2" |Модуляція яскравості
|3,600
|1.22{{±|0.175|0.139}}
|6,118.4{{±|127.2|121.2}}
|<ref name="Lillo-Box2021" />
|-
|[[KIC 5479689 b]]
|0.5{{±|0.4|0.1}}
|
|1.701531{{±|0.000008|0.000419}}
|
|
| style="background:#00c9c2" |Модуляція яскравості
|1,504
|0.966{{±|0.03|0.04}}
|5459.1{{±|90.0|85.2}}
|<ref name="Lillo-Box2021" />
|-
|[[LTT 1445|LTT 1445 Ac]]
|0.0048{{±|0.0006}}
|0.103
|3.12390
|0.02661{{±|0.00047|0.00049}}
|
| style="background:#FFFF00" |Транзит
|22.41{{±|0.01}}
|0.256{{±|0.014}}
|3337{{±|150}}
|<ref name="Winters2021">{{cite journal|last1=Winters|first1=Jennifer G.|last2=Cloutier|first2=Ryan|last3=Medina|first3=Amber A.|last4=Irwin|first4=Jonathan M.|last5=Charbonneau|first5=David|last6=Astudillo-Defru|first6=Nicola|last7=Bonfils|first7=Xavier|last8=Howard|first8=Andrew W.|last9=Isaacson|first9=Howard|year=2022|title=A Second Planet Транзитing LTT 1445A and a Determination of the Masses of Both Worlds|journal=The Astronomical Journal|volume=163|issue=4|page=168|arxiv=2107.14737|bibcode=2022AJ....163..168W|doi=10.3847/1538-3881/ac50a9|last10=Bean|first10=J. L.|last11=Seifahrt|first11=A.|last12=Teske|first12=J. K.|last13=Eastman|first13=Jason D.|last14=Twicken|first14=Joseph D.|last15=Collins|first15=K. A.|last16=Jensen|first16=E. L. N.|last17=Quinn|first17=S. N.|last18=Payne|first18=M. J.|last19=Kristiansen|first19=M. H.|last20=Spencer|first20=A.|last21=Vanderburg|first21=Andrew|last22=Zechmeister|first22=Mathias|last23=Weiss|first23=L. M. <!-- Lauren ? -->|last24=Wang|first24=S. X.|last25=Wang|first25=G.|last26=Udry|first26=Stéphane|last27=Terentev|first27=I. A.|last28=Sturmer|first28=J.|last29=Stefansson|first29=G.|last30=Shectman|first30=Stephen A.|last31=Sefako|first31=R.|last32=Schwengeler|first32=H. M.|last33=Schwarz|first33=R. P.|last34=Scarsdale|first34=N.|last35=Rubenzahl|first35=R. A.|last36=Roy|first36=A.|last37=Rosenthal|first37=L. J.|last38=Robertson|first38=P.|last39=Petigura|first39=Erik A.|last40=Pepe|first40=Francesco|last41=Omohundro|first41=M.|last42=Murphy|first42=J. M. A.|last43=Murgas|first43=Felipe|last44=Movcnik|first44=T.|last45=Montet|first45=B. T.|last46=Mennickent|first46=R.|last47=Mayo|first47=A. W.|last48=Massey|first48=B.|last49=Lubin|first49=J.|last50=Lovis|first50=Christophe|last51=Lewin|first51=P.|last52=Kasper|first52=D.|last53=Kane|first53=S. R.|last54=Jenkins|first54=J. M.|last55=Huber|first55=D.|last56=Horne|first56=K.|last57=Hill|first57=M. L.|last58=Gorrini|first58=P.|last59=Giacalone|first59=S.|last60=Fulton|first60=Benjamin J.|last61=Forveille|first61=Thierry|last62=Figueira|first62=Pedro|last63=Fetherolf|first63=T.|last64=Dressing|first64=Courtney D.|last65=Díaz|first65=Rodrigo F.|last66=Delfosse|first66=Xavier|last67=Dalba|first67=P. A.|last68=Dai|first68=F.|last69=Cortes|first69=C. C.|last70=Crossfield|first70=Ian J. M.|last71=Crane|first71=Jeffrey D.|last72=Conti|first72=D. M.|last73=Collins|first73=K. I.|last74=Chontos|first74=A.|last75=Butler|first75=R. Paul|last76=Brown|first76=P.|last77=Brady|first77=M.|last78=Bouchy|first78=François|last79=Behmard|first79=A.|last80=Beard|first80=C.|last81=Batalha|first81=Natalie M.|last82=Almenara|first82=José M.|s2cid=236635391}}</ref>
|-
|[[L 98-59|Luyten 98-59 e]]
|0.0094
|
|12.8
|0.071
|342{{±|20|18}}
| style="background:#00FF00" |Радіальна швидкість
|34.6
|0.32{{±|0.03}}
|3500{{±|150}}
|<ref name="Demangeon2021-7">{{Cite web|url=https://www.eso.org/public/archives/releases/sciencepapers/eso2112/eso2112a.pdf|title=A warm terrestrial planet with half the mass of Venus Транзитing a nearby star|access-date=8 серпня 2021|archive-date=13 листопада 2021|archive-url=https://web.archive.org/web/20211113184620/https://www.eso.org/public/archives/releases/sciencepapers/eso2112/eso2112a.pdf|url-status=live}}</ref>
|-
|[[L 98-59|Luyten 98-59 f]]
|0.0078
|
|23.2
|0.103
|285{{±|18|17}}
| style="background:#00FF00" |Радіальна швидкість
|34.6
|0.32{{±|0.03}}
|3500{{±|150}}
|Непідтверджена, потенційно придатна для життя<ref name="Demangeon2021-7" />
|-
|[[HD 191939|HD 191939 e]]
|0.34{{±|0.01}}
|
|101.4{{±|0.4}}
|0.397{{±|0.005}}
|397{{±|16}}
| style="background:#00FF00" |Радіальна швидкість
|175.1{{±|0.2}}
|0.92
|5400
|Також припускається наявність коричневого карлика<ref name="Lubin2021">{{cite journal|last1=Lubin|first1=Jack|author2=Judah Van Zandt|last3=Holcomb|first3=Rae|last4=Weiss|first4=Lauren M.|author5=Erik A Petigura|last6=Robertson|first6=Paul|last7=Akana Murphy|first7=Joseph M.|last8=Scarsdale|first8=Nicholas|last9=Batygin|first9=Konstantin|display-authors=1|year=2022|title=TESS-Keck Survey. IX. Masses of Three Sub-Neptunes Orbiting HD 191939 and the Discovery of a Warm Jovian plus a Distant Substellar Companion|journal=The Astronomical Journal|volume=163|issue=2|page=101|arxiv=2108.02208|bibcode=2022AJ....163..101L|doi=10.3847/1538-3881/ac3d38|mode=cs2|last10=Polanski|first10=Alex S.|last11=Batalha|first11=Natalie M.|last12=Crossfield|first12=Ian J. M.|last13=Dressing|first13=Courtney|last14=Fulton|first14=Benjamin|last15=Howard|first15=Andrew W.|last16=Huber|first16=Daniel|last17=Isaacson|first17=Howard|last18=Kane|first18=Stephen R.|last19=Roy|first19=Arpita|last20=Beard|first20=Corey|last21=Blunt|first21=Sarah|last22=Chontos|first22=Ashley|last23=Dai|first23=Fei|last24=Dalba|first24=Paul A.|last25=Giacalone|first25=Steven|last26=Hill|first26=Michelle L.|last27=Mayo|first27=Andrew|last28=Mocnik|first28=Teo|last29=Kosiarek|first29=Molly R.|last30=Rice|first30=Malena|s2cid=236924440}}</ref>
|-
|[[OGLE-2019-BLG-1058]]
|6.836{{±|6.027}}
|
|
|
|
| style="background:#0099FF" |Мікролінзування
|8,000{{±|5,000}}
|
|
|Планета-сирота<ref>{{cite journal|last1=Shin|first1=In-Gu|last2=Yee|first2=Jennifer C.|last3=Hwang|first3=Kyu-Ha|last4=Udalski|first4=Andrzej|last5=Gould|first5=Andrew|last6=Albrow|first6=Michael D.|last7=Chung|first7=Sun-Ju|last8=Han|first8=Cheongho|author9=Youn Kil Jung|display-authors=1|year=2021|title=Using Source Proper Motion to Validate Terrestrial Parallax: OGLE-2019-BLG-1058|journal=The Astronomical Journal|volume=162|issue=6|page=267|arxiv=2108.02499|bibcode=2021AJ....162..267S|doi=10.3847/1538-3881/ac2ba5|mode=cs2|last10=Kim|first10=Hyoun-Woo|last11=Ryu|first11=Yoon-Hyun|last12=Shvartzvald|first12=Yossi|last13=Zang|first13=Weicheng|last14=Cha|first14=Sang-Mok|last15=Kim|first15=Dong-Jin|last16=Kim|first16=Seung-Lee|last17=Lee|first17=Chung-Uk|last18=Lee|first18=Dong-Joo|last19=Lee|first19=Yongseok|last20=Park|first20=Byeong-Gon|last21=Pogge|first21=Richard W.|last22=Mróz|first22=Przemek|last23=Szymański|first23=Michał K.|last24=Skowron|first24=Jan|last25=Poleski|first25=Radek|last26=Soszyński|first26=Igor|last27=Pietrukowicz|first27=Paweł|last28=Kozłowski|first28=Szymon|last29=Ulaczyk|first29=Krzysztof|last30=Rybicki|first30=Krzysztof A.|s2cid=236924486}}</ref>
|-
|[[TOI-2184 b]]
|0.65{{±|0.16}}
|1.017{{±|0.051}}
|6.90683{{±|0.00009}}
|
|
| style="background:#FFFF00" |Транзит
|2,515{{±|22}}
|1.53{{±|0.12}}
|5,966{{±|136}}
|<ref>{{cite journal|last1=Saunders|first1=Nicholas|last2=Grunblatt|first2=Samuel K.|last3=Huber|first3=Daniel|last4=Collins|first4=Karen A.|last5=Jensen|first5=Eric L. N.|last6=Vanderburg|first6=Andrew|last7=Brahm|first7=Rafael|last8=Jordán|first8=Andrés|last9=Espinoza|first9=Néstor|display-authors=1|year=2022|title=TESS Giants Транзитing Giants. I.: A Noninflated Hot Jupiter Orbiting a Massive Subgiant|journal=The Astronomical Journal|volume=163|issue=2|page=53|arxiv=2108.02294|bibcode=2022AJ....163...53S|doi=10.3847/1538-3881/ac38a1|mode=cs2|last10=Henning|first10=Thomas|last11=Hobson|first11=Melissa J.|last12=Quinn|first12=Samuel N.|last13=Zhou|first13=George|last14=Paul Butler|first14=R.|last15=Crause|first15=Lisa|last16=Kuhn|first16=Rudi B.|last17=Moses Mogotsi|first17=K.|last18=Hellier|first18=Coel|last19=Angus|first19=Ruth|last20=Hattori|first20=Soichiro|last21=Chontos|first21=Ashley|last22=Ricker|first22=George R.|last23=Jenkins|first23=Jon M.|last24=Tenenbaum|first24=Peter|last25=Latham|first25=David W.|last26=Seager|first26=Sara|last27=Vanderspek|first27=Roland K.|last28=Winn|first28=Joshua N.|last29=Stockdale|first29=Chris|last30=Cloutier|first30=Ryan|s2cid=236924647}}</ref>
|-
|[[TOI-431|TOI-431 b]] ('''CD-26 2288''', '''HIP 26013''')
|0.0097{{±|0.0011}}
|0.0014{{±|0.004}}
|0.490047{{±|0.000010|0.000007}}
|0.0113{{±|0.0002|0.0003}}
|1,862{{±|42}}
| style="background:#FFFF00" |Транзит
|106.37{{±|0.03}}
|0.78{{±|0.07}}
|4,850{{±|75}}
|<ref name="Osborn2021-8">{{citation|display-authors=1|arxiv=2108.02310|year=2021|title=TOI-431/HIP 26013: a super-Earth and a sub-Neptune Транзитing a bright, early K dwarf, with a third RV planet|doi=10.1093/mnras/stab2313|last1=Osborn|first1=Ares|last2=Armstrong|first2=David J.|last3=Cale|first3=Bryson|last4=Brahm|first4=Rafael|last5=Wittenmyer|first5=Robert A.|last6=Dai|first6=Fei|last7=Crossfield|first7=Ian J. M.|last8=Bryant|first8=Edward M.|last9=Adibekyan|first9=Vardan|last10=Cloutier|first10=Ryan|last11=Collins|first11=Karen A.|last12=Delgado Mena|first12=E.|last13=Fridlund|first13=Malcolm|last14=Hellier|first14=Coel|last15=Howell|first15=Steve B.|last16=King|first16=George W.|last17=Lillo-Box|first17=Jorge|last18=Otegi|first18=Jon|last19=Sousa|first19=S.|last20=Stassun|first20=Keivan G.|last21=Matthews|first21=Elisabeth C.|last22=Ziegler|first22=Carl|last23=Ricker|first23=George|last24=Vanderspek|first24=Roland|last25=Latham|first25=David W.|last26=Seager|first26=S.|last27=Winn|first27=Joshua N.|last28=Jenkins|first28=Jon M.|last29=Acton|first29=Jack S.|last30=Addison|first30=Brett C.|journal=Monthly Notices of the Royal Astronomical Society|volume=507|issue=2|pages=2782–2803}}</ref>
|-
|[[TOI-431|TOI-431 c]] ('''CD-26 2288''', '''HIP 26013''')
|0.0089{{±|0.0013|0.0011}}
|
|4.8494{{±|0.0003|0.0002}}
|0.0052{{±|0.001}}
|867{{±|20}}
| style="background:#00FF00" |Радіальна швидкість
|106.37{{±|0.03}}
|0.78{{±|0.07}}
|4,850{{±|75}}
|<ref name="Osborn2021-8" />
|-
|[[TOI-431|TOI-431 d]] ('''CD-26 2288''', '''HIP 26013''')
|0.0312{{±|0.0047}}
|0.294{{±|0.008}}
|12.46103{{±|0.00002}}
|0.098{{±|0.002}}
|633{{±|14}}
| style="background:#FFFF00" |Транзит
|106.37{{±|0.03}}
|0.78{{±|0.07}}
|4,850{{±|75}}
|<ref name="Osborn2021-8" />
|-
|[[TOI-2202|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}}
|
| style="background:#FFFF00" |Транзит
|770{{±|3}}
|0.823{{±|0.027|0.023}}
|5,144{{±|50}}
|<ref name="Trifonov2021">{{cite journal|last1=Trifonov|first1=Trifon|last2=Brahm|first2=Rafael|last3=Espinoza|first3=Nestor|last4=Henning|first4=Thomas|last5=Jordán|first5=Andrés|last6=Nesvorny|first6=David|last7=Dawson|first7=Rebekah I.|last8=Lissauer|first8=Jack J.|author9=Man Hoi Lee|display-authors=1|year=2021|title=A Pair of Warm Giant Planets near the 2:1 Mean Motion Resonance around the K-dwarf Star TOI-2202|journal=The Astronomical Journal|volume=162|issue=6|page=283|arxiv=2108.05323|bibcode=2021AJ....162..283T|doi=10.3847/1538-3881/ac1bbe|mode=cs2|last10=Kossakowski|first10=Diana|last11=Rojas|first11=Felipe I.|last12=Hobson|first12=Melissa J.|last13=Sarkis|first13=Paula|last14=Schlecker|first14=Martin|last15=Bitsch|first15=Bertram|last16=Bakos|first16=Gaspar Á.|last17=Barbieri|first17=Mauro|last18=Bhatti|first18=Waqas|last19=Paul Butler|first19=R.|last20=Crane|first20=Jeffrey D.|last21=Nandakumar|first21=Sangeetha|last22=Díaz|first22=Matías R.|last23=Shectman|first23=Stephen|last24=Teske|first24=Johanna|last25=Torres|first25=Pascal|last26=Suc|first26=Vincent|last27=Vines|first27=Jose I.|last28=Wang|first28=Sharon X.|last29=Ricker|first29=George R.|last30=Shporer|first30=Avi|s2cid=236976243}}</ref>
|-
|[[TOI-2202|TOI-2202 c]]
|0.191{{±|0.033|0.030}}
|
|24.7545{{±|0.0073|0.0078}}
|0.1558{{±|0.0025|0.0026}}
|
| style="background:#FF7519" |Таймінг
|770{{±|3}}
|0.823{{±|0.027|0.023}}
|5,144{{±|50}}
|<ref name="Trifonov2021" />
|-
|[[EPIC 211314705.01]]
|
|0.139{{±|0.007}}
|3.793306{{±|0.000324|0.000343}}
|
|543{{±|8|9}}
| style="background:#FFFF00" |Транзит
|300.0{{±|1.7}}
|0.43{{±|0.01}}
|3,669{{±|88|82}}
|Припускається наявність ще 2 планет<ref name="Leon2021">{{citation|display-authors=1|arxiv=2108.05621|year=2021|title=37 New Validated Planets in Overlapping K2 Campaigns|doi=10.1093/mnras/stab2305|last1=De Leon|first1=J. P.|last2=Livingston|first2=J.|last3=Endl|first3=M.|last4=Cochran|first4=W. D.|last5=Hirano|first5=T.|last6=A|first6=R A Garcí|last7=Mathur|first7=S.|last8=Lam|first8=K W F.|last9=Korth|first9=J.|last10=Trani|first10=A. A.|last11=Dai|first11=F.|last12=Alonso|first12=E Díez|last13=Castro-González|first13=A.|last14=Fridlund|first14=M.|last15=Fukui|first15=A.|last16=Gandolfi|first16=D.|last17=Kabath|first17=P.|last18=Kuzuhara|first18=M.|last19=Luque|first19=R.|last20=Savel|first20=A. B.|last21=Gill|first21=H.|last22=Dressing|first22=C.|last23=Giacalone|first23=S.|last24=Narita|first24=N.|last25=Palle|first25=E.|last26=Van Eylen|first26=V.|last27=Tamura|first27=M.|journal=Monthly Notices of the Royal Astronomical Society|volume=508|pages=195–218}}</ref><ref name="Kovaks2020">{{citation|arxiv=2008.10075|year=2020|title=More planetary candidates from K2 Campaign 5 using TRAN_K2|doi=10.1051/0004-6361/202038726|last1=Kovacs|first1=Geza|journal=Astronomy & Astrophysics|volume=643|pages=A169|bibcode=2020A&A...643A.169K|s2cid=221266076}}</ref>
|-
|[[EPIC 211401787.01]] ('''BD+12 1842''')
|
|0.247{{±|0.013|0.008}}
|13.774798{{±|0.000028|0.000028}}
|
|969{{±|9}}
| style="background:#FFFF00" |Транзит
|525{{±|5}}
|1.23{{±|0.02}}
|6,232{{±|33|39}}
|<ref name="Leon2021" />
|-
|[[K2-268]]f ('''EPIC 211413752''')
|
|0.199{{±|0.013|0.008}}
|26.270570{{±|0.000105|0.000109}}
|
|492{{±|8|10}}
| style="background:#FFFF00" |Транзит
|1,079{{±|10}}
|0.84{{±|0.02}}
|5,106{{±|70|61}}
|<ref name="Leon2021" />
|-
|[[K2-268]]d ('''EPIC 211413752''')
|
|0.133{{±|0.013|0.006}}
|4.528598{{±|0.000016|0.000015}}
|
|888{{±|16|15}}
| style="background:#FFFF00" |Транзит
|1,079{{±|10}}
|0.84{{±|0.02}}
|5,106{{±|70|61}}
|<ref name="Leon2021" />
|-
|[[K2-268]]e ('''EPIC 211413752''')
|
|0.119{{±|0.010|0.007}}
|6.131243{{±|0.000032|0.000033}}
|
|801{{±|13}}
| style="background:#FFFF00" |Транзит
|1,079{{±|10}}
|0.84{{±|0.02}}
|5,106{{±|70|61}}
|<ref name="Leon2021" />
|-
|[[EPIC 211502222.01]]
|
|0.243{{±|0.013|0.009}}
|22.996591{{±|0.001848|0.001859}}
|
|673{{±|12|11}}
| style="background:#FFFF00" |Транзит
|694{{±|6}}
|1.10{{±|0.03|0.04}}
|5,994{{±|93|91}}
|<ref name="Leon2021" />
|-
|[[EPIC 211502222.02]]
|
|0.160{{±|0.013|0.009}}
|9.398977{{±|0.001506|0.001348}}
|
|909{{±|14}}
| style="background:#FFFF00" |Транзит
|694{{±|6}}
|1.10{{±|0.03|0.04}}
|5,994{{±|93|91}}
|<ref name="Leon2021" />
|-
|[[EPIC 211579112.01]]
|
|0.196{{±|0.017|0.014}}
|17.706320{{±|0.000063}}
|
|266{{±|5|8}}
| style="background:#FFFF00" |Транзит
|403{{±|5}}
|0.27{{±|0.01|0.02}}
|3,315{{±|137|152}}
|<ref name="Leon2021" />
|-
|[[K2-185c]] ('''EPIC 211611158''')
|
|0.213{{±|0.008}}
|52.713494{{±|0.000155|0.000164}}
|
|477{{±|14|17}}
| style="background:#FFFF00" |Транзит
|882{{±|11}}
|0.96{{±|0.05|0.07}}
|5,788{{±|190|157}}
|<ref name="Leon2021" />
|-
|[[EPIC 211647930.01]]
|
|0.552{{±|0.025|0.022}}
|14.759287{{±|0.000243|0.000240}}
|
|826{{±|14|17}}
| style="background:#FFFF00" |Транзит
|1,133{{±|17}}
|1.06{{±|0.04}}
|5,880{{±|85|82}}
|<ref name="Leon2021" />
|-
|[[EPIC 211730024.01]]
|
|0.504{{±|0.032|0.025}}
|5.113981{{±|0.000061|0.000062}}
|
|1,380{{±|34|30}}
| style="background:#FFFF00" |Транзит
|1,226{{±|21}}
|1.36{{±|0.05}}
|6,502{{±|132|130}}
|<ref name="Leon2021" />
|-
|[[EPIC 211743874.01]]
|
|0.197{{±|0.016|0.013}}
|12.283211{{±|0.000051}}
|
|949{{±|21|26}}
| style="background:#FFFF00" |Транзит
|1,850{{±|60}}
|1.23{{±|0.04}}
|6,222{{±|96|91}}
|<ref name="Leon2021" />
|-
|[[EPIC 211763214.01]]
|
|0.109{{±|0.008|0.005}}
|21.194733{{±|0.000108|0.000107}}
|
|569{{±|15|22}}
| style="background:#FFFF00" |Транзит
|786{{±|9}}
|0.86{{±|0.03|0.05}}
|5,424{{±|192|144}}
|<ref name="Leon2021" />
|-
|[[EPIC 211770696.01]]
|
|0.234{{±|0.017|0.013}}
|16.273563{{±|0.000054|0.000053}}
|
|850{{±|19|18}}
| style="background:#FFFF00" |Транзит
|1,390{{±|30}}
|0.94{{±|0.04|0.03}}
|5,869{{±|88|81}}
|<ref name="Leon2021" />
|-
|[[EPIC 211779390.01]]
|
|0.092{{±|0.010|0.005}}
|3.850614{{±|0.000012}}
|
|783{{±|12|14}}
| style="background:#FFFF00" |Транзит
|514{{±|2}}
|0.66{{±|0.02}}
|4,558{{±|91|81}}
|<ref name="Leon2021" />
|-
|[[EPIC 211897691.02]]
|
|0.171{{±|0.017|0.011}}
|19.507428{{±|0.000116|0.000113}}
|
|508{{±|12}}
| style="background:#FFFF00" |Транзит
|1,187{{±|17}}
|0.74{{±|0.04|0.03}}
|4,857{{±|86|84}}
|<ref name="Leon2021" />
|-
|[[EPIC 211923431.01]]
|
|0.300{{±|0.039|0.029}}
|29.740451{{±|0.000169|0.000161}}
|
|606{{±|31|36}}
| style="background:#FFFF00" |Транзит
|2,460{{±|70}}
|0.93{{±|0.04}}
|5,532{{±|90}}
|<ref name="Leon2021" />
|-
|[[EPIC 211978988.01]]
|
|0.287{{±|0.022|0.017}}
|36.552551{{±|0.000127|0.000122}}
|
|598{{±|16|15}}
| style="background:#FFFF00" |Транзит
|1,390{{±|20}}
|0.98{{±|0.07}}
|5,817{{±|45|48}}
|<ref name="Leon2021" />
|-
|[[TOI-1518 b]]
|2.3
|1.875{{±|0.053}}
|1.902603{{±|0.000011}}
|0.0389{{±|0.0011}}
|3,237{{±|59}}
| style="background:#FFFF00" |Транзит
|742{{±|6}}
|1.79{{±|0.26}}
|7,300{{±|100}}
|<ref name="Leon2021" />
|-
|[[EPIC 212058012.01]]
|
|0.181{{±|0.012|0.008}}
|11.561052{{±|0.000690|0.000668}}
|
|861{{±|14|15}}
| style="background:#FFFF00" |Транзит
|684{{±|6}}
|1.01{{±|0.05}}
|5,920{{±|104}}
|<ref name="Leon2021" />
|-
|[[EPIC 212072539.01]]
|
|0.180{{±|0.009|0.006}}
|7.676972{{±|0.000012|0.000012}}
|
|465{{±|7}}
| style="background:#FFFF00" |Транзит
|545{{±|3}}
|0.49{{±|0.01}}
|3,804{{±|93|74}}
|<ref name="Leon2021" />
|-
|[[EPIC 212072539.02]]
|
|0.147{{±|0.015|0.007}}
|2.787174{{±|0.000004}}
|
|653{{±|10|12}}
| style="background:#FFFF00" |Транзит
|545{{±|3}}
|0.49{{±|0.01}}
|3,804{{±|93|74}}
|<ref name="Leon2021" />
|-
|[[EPIC 212081533.01]]
|
|0.142{{±|0.009|0.004}}
|3.355850{{±|0.000091|0.000093}}
|
|722{{±|7|10}}
| style="background:#FFFF00" |Транзит
|245.8
|0.51{{±|0.01}}
|4,374{{±|38|34}}
|<ref name="Leon2021" />
|-
|[[EPIC 212088059.01]]
|
|0.188{{±|0.018|0.008}}
|10.367437{{±|0.000020|0.000019}}
|
|437{{±|4|5}}
| style="background:#FFFF00" |Транзит
|532{{±|3}}
|0.56{{±|0.01}}
|3,779{{±|30|26}}
|<ref name="Leon2021" />
|-
|[[EPIC 212132195.01]]
|
|0.202{{±|0.017|0.009}}
|26.201446{{±|0.003331|0.003124}}
|
|450{{±|5}}
| style="background:#FFFF00" |Транзит
|345.5{{±|1.6}}
|0.71{{±|0.02}}
|4,801{{±|49}}
|<ref name="Leon2021" />
|-
|[[EPIC 212161956.01]]
|
|0.215{{±|0.010|0.009}}
|7.187257{{±|0.000020|0.000021}}
|
|640{{±|20|21}}
| style="background:#FFFF00" |Транзит
|1055{{±|13}}
|0.66{{±|0.03}}
|4,599{{±|178|152}}
|<ref name="Leon2021" />
|-
|[[EPIC 212204403.01]]
|
|0.291{{±|0.020|0.010}}
|4.688418{{±|0.000119|0.000117}}
|
|908{{±|12|11}}
| style="background:#FFFF00" |Транзит
|662{{±|5}}
|0.83{{±|0.02|0.01}}
|5,077{{±|40|39}}
|<ref name="Leon2021" />
|-
|[[EPIC 212204403.02]]
|
|0.238{{±|0.021|0.010}}
|12.550171{{±|0.001018|0.001057}}
|
|655{{±|7|9}}
| style="background:#FFFF00" |Транзит
|662{{±|5}}
|0.83{{±|0.02|0.01}}
|5,077{{±|40|39}}
|<ref name="Leon2021" />
|-
|[[K2-304c]] ('''EPIC 212297394''')
|
|0.203{{±|0.017|0.011}}
|5.213965{{±|0.000442}}
|
|866{{±|27|37}}
| style="background:#FFFF00" |Транзит
|1,380{{±|20}}
|0.83{{±|0.05|0.04}}
|5,171{{±|172|130}}
|<ref name="Leon2021" />
|-
|[[EPIC 212420823.01]]
|
|0.123{{±|0.009|0.006}}
|9.032178{{±|0.000874}}
|
|518{{±|5|4}}
| style="background:#FFFF00" |Транзит
|1,450{{±|20}}
|0.54{{±|0.01}}
|4,385{{±|29|31}}
|<ref name="Leon2021" />
|-
|[[EPIC 212440430.02]]
|
|0.138{{±|0.013|0.010}}
|4.163873{{±|0.000022|0.000023}}
|
|1,158{{±|29|34}}
| style="background:#FFFF00" |Транзит
|1,620{{±|20}}
|0.98{{±|0.02}}
|5,789{{±|46|50}}
|<ref name="Leon2021" />
|-
|[[EPIC 212543933.01]]
|
|0.227{{±|0.023|0.017}}
|7.806164{{±|0.000673|0.000623}}
|
|934{{±|28|32}}
| style="background:#FFFF00" |Транзит
|1,310{{±|50}}
|1.02{{±|0.02}}
|5,769{{±|39|37}}
|<ref name="Leon2021" />
|-
|[[K2-307]]c ('''EPIC 212587672''')
|
|0.207{{±|0.017|0.011}}
|23.228555{{±|0.000068|0.000071}}
|
|658{{±|13|14}}
| style="background:#FFFF00" |Транзит
|1,050{{±|20}}
|0.99{{±|0.03|0.04}}
|6,004{{±|77|78}}
|<ref name="Leon2021" />
|-
|[[EPIC 251319382.01]]
|
|0.171{{±|0.012|0.006}}
|8.234885{{±|0.000508|0.000475}}
|
|885{{±|12|14}}
| style="background:#FFFF00" |Транзит
|577{{±|6}}
|0.95{{±|0.02}}
|5,791{{±|81}}
|<ref name="Leon2021" />
|-
|[[EPIC 251319382.02]]
|
|0.199{{±|0.012|0.008}}
|14.871387{{±|0.000916|0.000936}}
|
|727{{±|10}}
| style="background:#FFFF00" |Транзит
|577{{±|6}}
|0.95{{±|0.02}}
|5,791{{±|81}}
|<ref name="Leon2021" />
|-
|[[EPIC 251319382.03]]
|
|0.122{{±|0.009|0.006}}
|3.665912{{±|0.000273|0.000295}}
|
|1,160{{±|16|15}}
| style="background:#FFFF00" |Транзит
|577{{±|6}}
|0.95{{±|0.02}}
|5,791{{±|81}}
|<ref name="Leon2021" />
|-
|[[EPIC 251554286.01]]
|
|0.496{{±|0.020|0.018}}
|15.466805{{±|0.000572|0.000565}}
|
|735{{±|13|14}}
| style="background:#FFFF00" |Транзит
|883{{±|12}}
|0.87{{±|0.02}}
|5,698{{±|55}}
|<ref name="Leon2021" />
|-
|[[Gliese 146|Gliese 146 b]] ('''HD 22496''')
|0.0175{{±|0.0023|0.0021}}
|
|5.09071 ± 0.00026
|0.0510{{±|0.0024|0.0026}}
|573{{±|63|69}}
| style="background:#00FF00" |Радіальна швидкість
|44.37{{±|0.01}}
|0.684{{±|0.013}}
|4,385{{±|21}}
|<ref>{{cite journal|last1=Lillo-Box|first1=J.|last2=Faria|first2=J. P.|last3=Suárez Mascareño|first3=A.|last4=Figueira|first4=P.|last5=Sousa|first5=S. G.|last6=Tabernero|first6=H.|last7=Lovis|first7=C.|last8=Silva|first8=A. M.|last9=Demangeon|first9=O. D. S.|display-authors=1|year=2021|title=HD 22496 b: The first ESPRESSO stand-alone planet discovery|journal=Astronomy & Astrophysics|volume=654|pages=A60|arxiv=2109.00226|bibcode=2021A&A...654A..60L|doi=10.1051/0004-6361/202141714|mode=cs2|last10=Benatti|first10=S.|last11=Santos|first11=N. C.|last12=Mehner|first12=A.|last13=Pepe|first13=F. A.|last14=Sozzetti|first14=A.|last15=Zapatero Osorio|first15=M. R.|last16=González Hernández|first16=J. I.|last17=Micela|first17=G.|last18=Hojjatpanah|first18=S.|last19=Rebolo|first19=R.|last20=Cristiani|first20=S.|last21=Adibekyan|first21=V.|last22=Allart|first22=R.|last23=Allende Prieto|first23=C.|last24=Cabral|first24=A.|last25=Damasso|first25=M.|last26=Di Marcantonio|first26=P.|last27=Lo Curto|first27=G.|last28=Martins|first28=C. J. A. P.|last29=Megevand|first29=D.|last30=Molaro|first30=P.|s2cid=237371680}}</ref>
|-
|[[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}}
| style="background:#FFFF00" |Транзит
|
|0.96{{±|0.05|0.06}}
|5,790{{±|177|147}}
|<ref name="Castro2021">{{cite journal|last1=Castro-González|first1=A.|last2=Díez Alonso|first2=E.|last3=Menéndez Blanco|first3=J.|last4=Livingston|first4=J.|last5=de Leon|first5=J. P.|last6=Lillo-Box|first6=J.|last7=Korth|first7=J.|last8=Fernández Menéndez|first8=S.|last9=Recio|first9=J. M.|display-authors=1|year=2022|title=The K2-OjOS Project: New and revisited planets and candidates in K2 campaigns 5, 16, & 18|journal=Monthly Notices of the Royal Astronomical Society|volume=509|pages=1075–1095|arxiv=2109.03346|doi=10.1093/mnras/stab2669|mode=cs2|last10=Izquierdo-Ruiz|first10=F.|last11=Coya Lozano|first11=A.|last12=García de la Cuesta|first12=F.|last13=Gómez Hernández|first13=N.|last14=Vidal Blanco|first14=J. R.|last15=Hevia Díaz|first15=R.|last16=Pardo Silva|first16=R.|last17=Pérez Acevedo|first17=S.|last18=Polancos Ruiz|first18=J.|last19=Padilla Tijerín|first19=P.|last20=Vázquez García|first20=D.|last21=Suárez Gómez|first21=S. L.|last22=García Riesgo|first22=F.|last23=González Gutiérrez|first23=C.|last24=Bonavera|first24=L.|last25=González-Nuevo|first25=J.|last26=Rodríguez Pereira|first26=C.|last27=Sánchez Lasheras|first27=F.|last28=Sánchez Rodríguez|first28=M. L.|last29=Muñiz|first29=R.|last30=Santos Rodríguez|first30=J. D.}}</ref>
|-
|[[EPIC 211537087.01]]
|
|0.204{{±|0.013|0.011}}
|21.0267366{{±|0.0036912|0.0038993}}
|0.1599{{±|0.0178|0.0306}}
|624{{±|0|37}}
| style="background:#FFFF00" |Транзит
|
|0.90{{±|0.05|0.06}}
|5,568{{±|178|150}}
|<ref name="Castro2021" />
|-
|[[EPIC 211730267.01]]
|
|0.332{{±|0.021|0.019}}
|16.3488637{{±|0.0013811|0.0014022}}
|0.1450{{±|0.0136|0.0235}}
|735{{±|8|39}}
| style="background:#FFFF00" |Транзит
|
|0.98{{±|0.07}}
|5,794{{±|210|169}}
|<ref name="Castro2021" />
|-
|[[EPIC 211914998.01]]
|
|0.239{{±|0.015|0.013}}
|11.2510285{{±|0.0018188|0.0017892}}
|0.0863{{±|0.0079|0.0159}}
|888{{±|0|47}}
| style="background:#FFFF00" |Транзит
|
|0.93{{±|0.06}}
|5,650{{±|193|152}}
|<ref name="Castro2021" />
|-
|[[TOI-3362b]]
|5.029{{±|0.668|0.646}}
|1.142{{±|0.043|0.041}}
|18.09547{{±|0.00003}}
|0.153{{±|0.002|0.003}}
|
| style="background:#FFFF00" |Транзит
|1,198{{±|18}}
|1.445{{±|0.069|0.073}}
|6,532{{±|88|86}}
|Висока витягнутість орбіти<ref>{{cite journal|last1=Dong|first1=Jiayin|last2=Huang|first2=Chelsea X.|last3=Zhou|first3=George|last4=Dawson|first4=Rebekah I.|last5=Rodriguez|first5=Joseph E.|last6=Eastman|first6=Jason D.|last7=Collins|first7=Karen A.|last8=Quinn|first8=Samuel N.|last9=Shporer|first9=Avi|display-authors=1|year=2021|title=TOI-3362b: A Proto Hot Jupiter Undergoing High-eccentricity Tidal Migration|journal=The Astrophysical Journal Letters|volume=920|issue=1|pages=L16|arxiv=2109.03771|bibcode=2021ApJ...920L..16D|doi=10.3847/2041-8213/ac2600|mode=cs2|last10=Triaud|first10=Amaury H. M. J.|last11=Wang|first11=Songhu|last12=Beatty|first12=Thomas|last13=Jackson|first13=Jonathon|last14=Collins|first14=Kevin I.|last15=Abe|first15=Lyu|last16=Suarez|first16=Olga|last17=Crouzet|first17=Nicolas|last18=MeKarnia|first18=Djamel|last19=Dransfield|first19=Georgina|last20=Jensen|first20=Eric L. N.|last21=Stockdale|first21=Chris|last22=Barkaoui|first22=Khalid|last23=Heitzmann|first23=Alexis|last24=Wright|first24=Duncan J.|last25=Addison|first25=Brett C.|last26=Wittenmyer|first26=Robert A.|last27=Okumura|first27=Jack|last28=Bowler|first28=Brendan P.|last29=Horner|first29=Jonathan|last30=Kane|first30=Stephen R.|s2cid=237442300}}</ref>
|-
|[[KMT-2017-BLG-2509b]]
|2.09{{±|1.68|1.26}}
|
|
|2.14{{±|0.27|0.39}}
|
| style="background:#0099FF" |Мікролінзування
|23,000{{±|3,000}}
|0.46{{±|0.37|0.27}}
|
|<ref name="Han2021-09">{{citation|arxiv=2109.07068|year=2021|title=Three faint-source Мікролінзування planets detected via the resonant-caustic channel|doi=10.1051/0004-6361/202141517|last1=Han|first1=Cheongho|last2=Udalski|first2=Andrzej|last3=Kim|first3=Doeon|last4=Ryu|first4=Yoon-Hyun|last5=Bozza|first5=Valerio|last6=Albrow|first6=Michael D.|last7=Chung|first7=Sun-Ju|last8=Gould|first8=Andrew|last9=Hwang|first9=Kyu-Ha|last10=Jung|first10=Youn Kil|last11=Lee|first11=Chung-Uk|last12=Shin|first12=In-Gu|last13=Shvartzvald|first13=Yossi|last14=Yee|first14=Jennifer C.|last15=Zang|first15=Weicheng|last16=Cha|first16=Sang-Mok|last17=Kim|first17=Dong-Jin|last18=Kim|first18=Hyoun-Woo|last19=Kim|first19=Seung-Lee|last20=Lee|first20=Dong-Joo|last21=Lee|first21=Yongseok|last22=Park|first22=Byeong-Gon|last23=Pogge|first23=Richard W.|last24=Mróz|first24=Przemek|last25=Szymański|first25=Michał K.|last26=Skowron|first26=Jan|last27=Poleski|first27=Radosław|last28=Soszyński|first28=Igor|last29=Pietrukowicz|first29=Paweł|last30=Kozłowski|first30=Szymon|journal=Astronomy & Astrophysics|volume=655|pages=A21|bibcode=2021A&A...655A..21H|s2cid=237513708|display-authors=1}}</ref>
|-
|[[OGLE-2017-BLG-1099b]]
|3.02{{±|2.43|1.81}}
|
|
|2.73{{±|0.40|0.53}}
|
| style="background:#0099FF" |Мікролінзування
|24,000{{±|3,000}}
|0.45{{±|0.36|0.27}}
|
|<ref name="Han2021-09" />
|-
|[[OGLE-2019-BLG-0299b]]
|6.22{{±|3.80|3.67}}
|
|
|2.80{{±|0.58|0.89}}
|
| style="background:#0099FF" |Мікролінзування
|19,000{{±|4,000}}
|0.59{{±|0.36|0.35}}
|
|<ref name="Han2021-09" />
|-
|[[TOI-1296b]]
|0.298{{±|0.039}}
|1.231{{±|0.031}}
|3.9443715{{±|0.0000058}}
|0.0497{{±|0.0023|0.0028}}
|1,562{{±|43|31}}
| style="background:#FFFF00" |Транзит
|1,023{{±|4}}
|1.17{{±|0.14}}
|5,603{{±|47}}
|<ref name="Moutou2021">{{citation|arxiv=2109.09252|year=2021|title=TOI-1296b and TOI-1298b observed with TESS and SOPHIE: Two hot Saturn-mass exoplanets with different densities around metal-rich stars|doi=10.1051/0004-6361/202141151|last1=Moutou|first1=C.|last2=Almenara|first2=J. M.|last3=Hébrard|first3=G.|last4=Santos|first4=N. C.|last5=Stassun|first5=K. G.|last6=Deheuvels|first6=S.|last7=Barros|first7=S.|last8=Benni|first8=P.|last9=Bieryla|first9=A.|last10=Boisse|first10=I.|last11=Bonfils|first11=X.|last12=Boyd|first12=P. T.|last13=Collins|first13=K. A.|last14=Baker|first14=D.|last15=Cortés-Zuleta|first15=P.|last16=Dalal|first16=S.|last17=Debras|first17=F.|last18=Deleuil|first18=M.|last19=Delfosse|first19=X.|last20=Demangeon|first20=O.|last21=Essack|first21=Z.|last22=Forveille|first22=T.|last23=Girardin|first23=E.|last24=Guerra|first24=P.|last25=Heidari|first25=N.|last26=Hesse|first26=K.|last27=Hoyer|first27=S.|last28=Jenkins|first28=J. M.|last29=Kiefer|first29=F.|last30=König|first30=P. C.|journal=Astronomy & Astrophysics|volume=653|pages=A147|bibcode=2021A&A...653A.147M|s2cid=237571683|display-authors=1}}</ref>
|-
|[[TOI-1298b]]
|0.356{{±|0.032}}
|0.841{{±|0.021}}
|4.537164{{±|0.000012}}
|0.0590{{±|0.0023}}
|1,388{{±|24}}
| style="background:#FFFF00" |Транзит
|1,041{{±|7}}
|1.44{{±|0.10}}
|5,889{{±|43}}
|<ref name="Moutou2021" />
|-
|[[TOI-1201 b]]
|0.0198{{±|0.0027}}
|0.216{{±|0.008}}
|2.4919863{{±|0.0000030|0.0000031}}
|0.0287{{±|0.0012}}
|703{{±|15|14}}
| style="background:#FFFF00" |Транзит
|122.77{{±|0.10}}
|0.512{{±|0.020}}
|3,476{{±|51}}
|В системі також є коричневий карлик<ref>{{citation|arxiv=2109.09346|year=2021|title=TOI-1201 b: A mini-Neptune Транзитing a bright and moderately young M dwarf|doi=10.1051/0004-6361/202141587|last1=Kossakowski|first1=D.|last2=Kemmer|first2=J.|last3=Bluhm|first3=P.|last4=Stock|first4=S.|last5=Caballero|first5=J. A.|last6=Béjar|first6=V. J. S.|last7=Guillén|first7=C. Cardona|last8=Lodieu|first8=N.|last9=Collins|first9=K. A.|last10=Oshagh|first10=M.|last11=Schlecker|first11=M.|last12=Espinoza|first12=N.|last13=Pallé|first13=E.|last14=Henning|first14=Th.|last15=Kreidberg|first15=L.|last16=Kürster|first16=M.|last17=Amado|first17=P. J.|last18=Anderson|first18=D. R.|last19=Morales|first19=J. C.|last20=Cartwright|first20=S.|last21=Charbonneau|first21=D.|last22=Chaturvedi|first22=P.|last23=Cifuentes|first23=C.|last24=Conti|first24=D. M.|last25=Cortés-Contreras|first25=M.|last26=Dreizler|first26=S.|last27=Galadí-Enríquez|first27=D.|last28=Guerra|first28=P.|last29=Hart|first29=R.|last30=Hellier|first30=C.|journal=Astronomy & Astrophysics|volume=656|pages=A124|bibcode=2021A&A...656A.124K|s2cid=237571914|display-authors=1}}</ref>
|-
|[[RR Різця c]]
|2.7{{±|0.7}}
|
|14,200{{±|300}}
|9.7{{±|0.9}}
|
| style="background:#FF7519" |Таймінг
|69.10{{±|0.03}}
|0.18+0.44
|3,100+7,540
|Планета в подвійній системі з білого та червоного карлика<ref>{{citation|arxiv=2109.09397|year=2021|title=Two circumbinary planets in RR Cae eclipsing binary system|last1=Rattanamala|first1=R.|last2=Awiphan|first2=S.|last3=Komonjinda|first3=S.|last4=Phriksee|first4=A.|last5=Sappankum|first5=P.|last6=A-thano|first6=N.|last7=Chitchak|first7=S.|last8=Rittipruk|first8=P.|last9=Sawangwit|first9=U.|last10=Poshyachinda|first10=S.|last11=Reichart|first11=D. E.|last12=Haislip|first12=J. B.}}</ref>
|-
|[[TIC 257060897b]]
|0.67{{±|0.03}}
|1.49{{±|0.04}}
|3.660028{{±|0.000006}}
|0.051{{±|0.002}}
|1,762{{±|21}}
| style="background:#FFFF00" |Транзит
|1,655{{±|8}}
|1.32{{±|0.04}}
|6,128{{±|57}}
|<ref>{{citation|arxiv=2110.00489|year=2022|title=TIC 257060897b: An inflated, low-density, hot-Jupiter Транзитing a rapidly evolving subgiant star|doi=10.1093/mnras/stab2923|last1=Montalto|first1=M.|last2=Malavolta|first2=L.|last3=Gregorio|first3=J.|last4=Mantovan|first4=G.|last5=Desidera|first5=S.|last6=Piotto|first6=G.|last7=Nascimbeni|first7=V.|last8=Granata|first8=V.|last9=Manthopoulou|first9=E. E.|last10=Claudi|first10=R.|journal=Monthly Notices of the Royal Astronomical Society|volume=509|issue=2|pages=2908–2919}}</ref>
|-
|[[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}}
| style="background:#FFFF00" |Транзит
|482{{±|2}}
|0.53{{±|0.02}}
|3,659{{±|120}}
|<ref>{{citation|arxiv=2110.04220|year=2021|title=TOI-530b: A giant planet Транзитing an M dwarf detected by TESS|doi=10.1093/mnras/stab3708|last1=Gan|first1=Tianjun|last2=Lin|first2=Zitao|last3=Wang|first3=Sharon Xuesong|last4=Mao|first4=Shude|last5=Fouqué|first5=Pascal|last6=Fan|first6=Jiahao|last7=Bedell|first7=Megan|last8=Stassun|first8=Keivan G.|last9=Giacalone|first9=Steven|last10=Fukui|first10=Akihiko|last11=Murgas|first11=Felipe|last12=Ciardi|first12=David R.|last13=Howell|first13=Steve B.|last14=c̃Ollins|first14=Karen A.|last15=Shporer|first15=Avi|last16=Arnold|first16=Luc|last17=Barclay|first17=Thomas|last18=Charbonneau|first18=David|last19=Christiansen|first19=Jessie|last20=Crossfield|first20=Ian J M.|last21=Dressing|first21=Courtney D.|last22=Elliott|first22=Ashley|last23=Esparza-Borges|first23=Emma|last24=Evans|first24=Phil|last25=Gnilka|first25=Crystal L.|last26=Gonzales|first26=Erica J.|last27=Howard|first27=Andrew W.|last28=Isogai|first28=Keisuke|last29=Kawauchi|first29=Kiyoe|last30=Kurita|first30=Seiya|journal=Monthly Notices of the Royal Astronomical Society|volume=511|pages=83–99|display-authors=1}}</ref>
|-
|[[HIP 97166]]b
|0.0629{{±|0.047}}
|0.245{{±|0.012}}
|10.28891{{±|0.00004}}
|0.089{{±|0.001}}
|757{{±|25}}
| style="background:#FFFF00" |Транзит
|215.54{{±|0.33}}
|0.898{{±|0.054}}
|5,198{{±|100}}
|<ref name="MacDougall2021">{{citation|arxiv=2110.05628|year=2021|title=The TESS–Keck Survey. VI. Two Eccentric Sub-Neptunes Orbiting HIP-97166|doi=10.3847/1538-3881/ac295e|last1=MacDougall|first1=Mason G.|last2=Petigura|first2=Erik A.|last3=Angelo|first3=Isabel|last4=Lubin|first4=Jack|last5=Batalha|first5=Natalie M.|last6=Beard|first6=Corey|last7=Behmard|first7=Aida|last8=Blunt|first8=Sarah|last9=Brinkman|first9=Casey|last10=Chontos|first10=Ashley|last11=Crossfield|first11=Ian J. M.|last12=Dai|first12=Fei|last13=Dalba|first13=Paul A.|last14=Dressing|first14=Courtney|last15=Fulton|first15=Benjamin|last16=Giacalone|first16=Steven|last17=Hill|first17=Michelle L.|last18=Howard|first18=Andrew W.|last19=Huber|first19=Daniel|last20=Isaacson|first20=Howard|last21=Kane|first21=Stephen R.|last22=Mayo|first22=Andrew|last23=Močnik|first23=Teo|last24=Akana Murphy|first24=Joseph M.|last25=Polanski|first25=Alex|last26=Rice|first26=Malena|last27=Robertson|first27=Paul|last28=Rosenthal|first28=Lee J.|last29=Roy|first29=Arpita|last30=Rubenzahl|first30=Ryan A.|journal=The Astronomical Journal|volume=162|issue=6|page=265|bibcode=2021AJ....162..265M|s2cid=238634523|display-authors=1}}</ref>
|-
|[[HIP 97166]]c
|9.9{{±|1.8}}
|
|16.84{{±|0.22}}
|0.124{{±|0.002}}
|642{{±|22}}
| style="background:#00FF00" |Радіальна швидкість
|215.54{{±|0.33}}
|0.898{{±|0.054}}
|5,198{{±|100}}
|<ref name="MacDougall2021" />
|-
|[[HD 63935|HD 63935 b]]
|0.0340{{±|0.0057}}
|0.267{{±|0.013}}
|9.058811{{±|0.000017|0.000016}}
|
|911{{±|27}}
| style="background:#FFFF00" |Транзит
|159.36{{±|0.15}}
|0.933{{±|0.054}}
|5,534{{±|100}}
|<ref name="Scarsdale2021">{{citation|arxiv=2110.06885|year=2021|title=TESS-Keck Survey. V. Twin Sub-Neptunes Транзитing the Nearby G Star HD 63935|doi=10.3847/1538-3881/ac18cb|last1=Scarsdale|first1=Nicholas|last2=Murphy|first2=Joseph M. Akana|last3=Batalha|first3=Natalie M.|last4=Crossfield|first4=Ian J. M.|last5=Dressing|first5=Courtney D.|last6=Fulton|first6=Benjamin|last7=Howard|first7=Andrew W.|last8=Huber|first8=Daniel|last9=Isaacson|first9=Howard|last10=Kane|first10=Stephen R.|last11=Petigura|first11=Erik A.|last12=Robertson|first12=Paul|last13=Roy|first13=Arpita|last14=Weiss|first14=Lauren M.|last15=Beard|first15=Corey|last16=Behmard|first16=Aida|last17=Chontos|first17=Ashley|last18=Christiansen|first18=Jessie L.|last19=Ciardi|first19=David R.|last20=Claytor|first20=Zachary R.|last21=Collins|first21=Karen A.|last22=Collins|first22=Kevin I.|last23=Dai|first23=Fei|last24=Dalba|first24=Paul A.|last25=Dragomir|first25=Diana|last26=Fetherolf|first26=Tara|last27=Fukui|first27=Akihiko|last28=Giacalone|first28=Steven|last29=Gonzales|first29=Erica J.|last30=Hill|first30=Michelle L.|journal=The Astronomical Journal|volume=162|issue=5|page=215|bibcode=2021AJ....162..215S|s2cid=238743956|display-authors=1}}</ref>
|-
|[[HD 63935|HD 63935 c]]
|0.0349{{±|0.0076}}
|0.259{{±|0.012}}
|21.4023{{±|0.00189|0.00194}}
|
|684{{±|21}}
| style="background:#FFFF00" |Транзит
|159.36{{±|0.15}}
|0.933{{±|0.054}}
|5,534{{±|100}}
|<ref name="Scarsdale2021" />
|-
|[[HD 207897|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}}
| style="background:#FFFF00" |Транзит
|92.15{{±|0.10}}
|0.80{{±|0.036|0.030}}
|5,070{{±|60|57}}
|<ref>{{citation|arxiv=2110.08597|year=2022|title=HD 207897 b: A dense sub-Neptune Транзитing a nearby and bright K-type star|last1=Heidari|first1=N.|last2=Boisse|first2=I.|last3=Orell-Mique|first3=J.|last4=Hebrard|first4=G.|last5=Acuna|first5=L.|last6=Hara|first6=N. C.|last7=Lillo-Box|first7=J.|last8=Eastman|first8=J. D.|last9=Arnold|first9=L.|last10=Astudillo-Defru|first10=N.|last11=Adibekyan|first11=V.|last12=Bieryla|first12=A.|last13=Bonfils|first13=X.|last14=Bouchy|first14=F.|last15=Barclay|first15=T.|last16=Brasseur|first16=C. E.|last17=Borgniet|first17=S.|last18=Bourrier|first18=V.|last19=Buchhave|first19=L.|last20=Behmard|first20=A.|last21=Beard|first21=C.|last22=Batalha|first22=N. M.|last23=Courcol|first23=B.|last24=Cortes-Zuleta|first24=P.|last25=Collins|first25=K.|last26=Carmona|first26=A.|last27=Crossfield|first27=I. J. M.|last28=Chontos|first28=A.|last29=Delfosse|first29=X.|last30=Dalal|first30=S.|journal=Astronomy & Astrophysics|volume=658|pages=A176|doi=10.1051/0004-6361/202141429|bibcode=2022A&A...658A.176H|s2cid=239016573|display-authors=1}}</ref>
|-
|[[2MASS J04372171+2651014 b]]
|4{{±|1}}
|
|
|115
|1,450{{±|50}}
| style="background:#FF6CDA" |Пряме спостереження
|417.9{{±|1.5}}
|0.165{{±|0.015}}
|3,100
|<ref>{{citation|arxiv=2110.08655|year=2021|title=Zodiacal Exoplanets in Time (ZEIT) XII: A Directly-Imaged Planetary-Mass Companion to a Young Taurus M Dwarf Star|doi=10.1093/mnras/stab3069|last1=Gaidos|first1=E.|last2=Hirano|first2=T.|last3=Kraus|first3=A. L.|last4=Kuzuhara|first4=M.|last5=Zhang|first5=Z.|last6=Lee|first6=R. A.|last7=Salama|first7=M.|last8=Berger|first8=T. A.|last9=Grunblatt|first9=S. K.|last10=Ansdell|first10=M.|last11=Liu|first11=M. C.|last12=Harakawa|first12=H.|last13=Hodapp|first13=K. W.|last14=Jacobson|first14=S.|last15=Konishi|first15=M.|last16=Kotani|first16=T.|last17=Kudo|first17=T.|last18=Kurokawa|first18=T.|last19=Nishikawa|first19=J.|last20=Omiya|first20=M.|last21=Serizawa|first21=T.|last22=Tamura|first22=M.|last23=Ueda|first23=A.|last24=Vievard|first24=S.|journal=Monthly Notices of the Royal Astronomical Society|volume=512|pages=583–601}}</ref><ref>{{Cite web|url=https://scitechdaily.com/astronomers-discover-infant-planet-one-of-the-youngest-exoplanets-ever-observed/|title=Astronomers Discover Infant Planet – One of the Youngest Exoplanets Ever Observed|date=23 жовтня 2021|access-date=25 жовтня 2021|archive-date=25 жовтня 2021|archive-url=https://web.archive.org/web/20211025013248/https://scitechdaily.com/astronomers-discover-infant-planet-one-of-the-youngest-exoplanets-ever-observed/|url-status=live}}</ref>
|-
|[[TOI 1227 b]]
|
|0.854{{±|0.067|0.052}}
|27.36397{{±|0.00011}}
|0.0886{{±|0.0054|0.0057}}
|
| style="background:#FFFF00" |Транзит
|329.3{{±|0.8}}
|0.170{{±|0.015}}
|3,072{{±|74}}
|<ref>{{citation|arxiv=2110.09531|year=2022|title=TESS Hunt for Young and Maturing Exoplanets (THYME). VI. An 11 Myr Giant Planet Транзитing a Very-low-mass Star in Lower Centaurus Crux|last1=Mann|first1=Andrew W.|last2=Wood|first2=Mackenna L.|last3=Schmidt|first3=Stephen P.|last4=Barber|first4=Madyson G.|last5=Owen|first5=James E.|last6=Tofflemire|first6=Benjamin M.|last7=Newton|first7=Elisabeth R.|last8=Mamajek|first8=Eric E.|last9=Bush|first9=Jonathan L.|last10=Mace|first10=Gregory N.|last11=Kraus|first11=Adam L.|author12=Pa Chia Thao|last13=Vanderburg|first13=Andrew|last14=Llama|first14=Joe|last15=Johns-Krull|first15=Christopher M.|last16=Prato|first16=L.|last17=Stahl|first17=Asa G.|last18=Tang|first18=Shih-Yun|last19=Fields|first19=Matthew J.|last20=Collins|first20=Karen A.|last21=Collins|first21=Kevin I.|last22=Gan|first22=Tianjun|last23=Jensen|first23=Eric L. N.|last24=Kamler|first24=Jacob|last25=Schwarz|first25=Richard P.|last26=Furlan|first26=Elise|last27=Gnilka|first27=Crystal L.|last28=Howell|first28=Steve B.|last29=Lester|first29=Kathryn V.|last30=Owens|first30=Dylan A.|journal=The Astronomical Journal|volume=163|issue=4|page=156|doi=10.3847/1538-3881/ac511d|bibcode=2022AJ....163..156M|s2cid=239024522|display-authors=1}}</ref>
|-
|[[TOI-2285b]]
|
|0.155{{±|0.007}}
|27.26955{{±|0.00013|0.00010}}
|0.1363{{±|0.0010}}
|284{{±|6}}
| style="background:#FFFF00" |Транзит
|138.34{{±|0.14}}
|0.454{{±|0.010}}
|3,491{{±|58}}
|<ref>{{citation|arxiv=2110.10215|year=2021|title=TOI-2285b: A 1.7 Earth-radius planet near the habitable zone around a nearby M dwarf|doi=10.1093/pasj/psab106|last1=Fukui|first1=Akihiko|last2=Kimura|first2=Tadahiro|last3=Hirano|first3=Teruyuki|last4=Narita|first4=Norio|last5=Kodama|first5=Takanori|last6=Hori|first6=Yasunori|last7=Ikoma|first7=Masahiro|last8=Pallé|first8=Enric|last9=Murgas|first9=Felipe|last10=Parviainen|first10=Hannu|last11=Kawauchi|first11=Kiyoe|last12=Mori|first12=Mayuko|last13=Esparza-Borges|first13=Emma|last14=Bieryla|first14=Allyson|last15=Irwin|first15=Jonathan|last16=Safonov|first16=Boris S.|last17=Stassun|first17=Keivan G.|last18=Alvarez-Hernandez|first18=Leticia|last19=Béjar|first19=Víctor J S.|last20=Casasayas-Barris|first20=Núria|last21=Chen|first21=Guo|last22=Crouzet|first22=Nicolas|last23=De Leon|first23=Jerome P.|last24=Isogai|first24=Keisuke|last25=Kagetani|first25=Taiki|last26=Klagyivik|first26=Peter|last27=Korth|first27=Judith|last28=Kurita|first28=Seiya|last29=Kusakabe|first29=Nobuhiko|last30=Livingston|first30=John|journal=Publications of the Astronomical Society of Japan|volume=74|pages=L1–L8|display-authors=1}}</ref>
|-
|[[LHS 1678|LHS 1678 b]]
|0.0002{{±|0.0003}}
|0.062{{±|0.004}}
|0.8602322{{±|0.0000068|0.0000048}}
|0.01251{{±|0.00059|0.00056}}
|
| style="background:#FFFF00" |Транзит
|64.88{{±|0.03}}
|0.345{{±|0.014}}
|3490{{±|50}}
|<ref name="Sirverstein2021">{{citation|arxiv=2110.12079|year=2022|title=The LHS 1678 System: Two Earth-sized Транзитing Planets and an Astrometric Companion Orbiting an M Dwarf Near the Convective Boundary at 20 pc|last1=Silverstein|first1=Michele L.|last2=Schlieder|first2=Joshua E.|last3=Barclay|first3=Thomas|last4=Hord|first4=Benjamin J.|last5=Jao|first5=Wei-Chun|author6=Eliot Halley Vrijmoet|last7=Henry|first7=Todd J.|last8=Cloutier|first8=Ryan|last9=Kostov|first9=Veselin B.|last10=Kruse|first10=Ethan|last11=Winters|first11=Jennifer G.|last12=Irwin|first12=Jonathan M.|last13=Kane|first13=Stephen R.|last14=Stassun|first14=Keivan G.|last15=Huang|first15=Chelsea|last16=Kunimoto|first16=Michelle|last17=Tey|first17=Evan|last18=Vanderburg|first18=Andrew|last19=Astudillo-Defru|first19=Nicola|last20=Bonfils|first20=Xavier|last21=Brasseur|first21=C. E.|last22=Charbonneau|first22=David|last23=Ciardi|first23=David R.|last24=Collins|first24=Karen A.|last25=Collins|first25=Kevin I.|last26=Conti|first26=Dennis M.|last27=Crossfield|first27=Ian J. M.|last28=Daylan|first28=Tansu|last29=Doty|first29=John P.|last30=Dressing|first30=Courtney D.|journal=The Astronomical Journal|volume=163|issue=4|page=151|doi=10.3847/1538-3881/ac32e3|bibcode=2022AJ....163..151S|s2cid=239768873|display-authors=1}}</ref>
|-
|[[LHS 1678|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}}
|
| style="background:#FFFF00" |Транзит
|64.88{{±|0.03}}
|0.345{{±|0.014}}
|3490{{±|50}}
|<ref name="Sirverstein2021" />
|-
|[[HD 73583|HD 73583 b]] ('''TOI-560''')
|0.0315{{±|0.0098}}
|0.253{{±|0.009}}
|6.3980418{{±|0.0000065|0.0000063}}
|0.0601{{±|0.0026}}
|721{{±|21}}
| style="background:#FFFF00" |Транзит
|103.08{{±|0.10}}
|0.71{{±|0.02}}
|4511{{±|110}}
|<ref name="Barragan2021-10">{{citation|arxiv=2110.13069|year=2022|title=The young HD 73583 (TOI-560) planetary system: Two 10-M⊕ mini-Neptunes Транзитing a 500-Myr-old, bright, and active K dwarf|last1=Barragán|first1=O.|last2=Armstrong|first2=D. J.|last3=Gandolfi|first3=D.|last4=Carleo|first4=I.|last5=Vidotto|first5=A. A.|last6=Villarreal D'Angelo|first6=C.|last7=Oklopčić|first7=A.|last8=Isaacson|first8=H.|last9=Oddo|first9=D.|last10=Collins|first10=K.|last11=Fridlund|first11=M.|last12=Sousa|first12=S. G.|last13=Persson|first13=C. M.|last14=Hellier|first14=C.|last15=Howell|first15=S.|last16=Howard|first16=A.|last17=Redfield|first17=S.|last18=Eisner|first18=N.|last19=Georgieva|first19=I. Y.|last20=Dragomir|first20=D.|last21=Bayliss|first21=D.|last22=Nielsen|first22=L. D.|last23=Klein|first23=B.|last24=Aigrain|first24=S.|last25=Zhang|first25=M.|last26=Teske|first26=J.|last27=Twicken|first27=J D.|last28=Jenkins|first28=J.|last29=Esposito|first29=M.|last30=Van Eylen|first30=V.|journal=Monthly Notices of the Royal Astronomical Society|volume=514|issue=2|pages=1606–1627|doi=10.1093/mnras/stac638|display-authors=1}}</ref><ref>{{citation|arxiv=2110.13150|year=2022|title=Escaping Helium from TOI 560.01, a Young Mini-Neptune|last1=Zhang|first1=Michael|last2=Knutson|first2=Heather A.|last3=Wang|first3=Lile|last4=Dai|first4=Fei|last5=Barragán|first5=Oscar|journal=The Astronomical Journal|volume=163|issue=2|page=67|doi=10.3847/1538-3881/ac3fa7|bibcode=2022AJ....163...67Z|s2cid=239885237}}</ref>
|-
|[[HD 73583|HD 73583 c]] ('''TOI-560''')
|0.0302{{±|0.0055}}
|0.212{{±|0.009}}
|18.8797{{±|0.00088|0.00073}}
|0.1236{{±|0.0053|0.0053}}
|503{{±|15}}
| style="background:#FFFF00" |Транзит
|103.08{{±|0.10}}
|0.71{{±|0.02}}
|4511{{±|110}}
|<ref name="Barragan2021-10" />
|-
|{{ill|TOI-1807#Planetary system|it|TOI-1807 b|lt=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}}
| style="background:#FFFF00" |Транзит
|133.88{{±|0.25}}
|0.750{{±|0.025|0.024}}
|4757{{±|51|50}}
|<ref name="Hedges2021">{{citation|arxiv=2111.01311|year=2021|title=TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow up|doi=10.3847/1538-3881/ac06cd|last1=Hedges|first1=Christina|last2=Hughes|first2=Alex|last3=Zhou|first3=George|last4=David|first4=Trevor J.|last5=Becker|first5=Juliette|last6=Giacalone|first6=Steven|last7=Vanderburg|first7=Andrew|last8=Rodriguez|first8=Joseph E.|last9=Bieryla|first9=Allyson|last10=Wirth|first10=Christopher|last11=Atherton|first11=Shaun|last12=Fetherolf|first12=Tara|last13=Collins|first13=Karen A.|last14=Price-Whelan|first14=Adrian M.|last15=Bedell|first15=Megan|last16=Quinn|first16=Samuel N.|last17=Gan|first17=Tianjun|last18=Ricker|first18=George R.|last19=Latham|first19=David W.|last20=Vanderspek|first20=Roland K.|last21=Seager|first21=Sara|last22=Winn|first22=Joshua N.|last23=Jenkins|first23=Jon M.|last24=Kielkopf|first24=John F.|last25=Schwarz|first25=Richard P.|last26=Dressing|first26=Courtney D.|last27=Gonzales|first27=Erica J.|last28=Crossfield|first28=Ian J. M.|last29=Matthews|first29=Elisabeth C.|last30=Jensen|first30=Eric L. N.|journal=The Astronomical Journal|volume=162|issue=2|page=54|bibcode=2021AJ....162...54H|s2cid=235805026|display-authors=1}}</ref><ref>{{citation|arxiv=2210.04162|year=2022|title=New Parameter Measurements for the Ultra-Short-Period Planet TOI-1807b|last1=Peng|first1=Peifeng|last2=Xiong|first2=Hongyi|last3=Li|first3=He|last4=Li|first4=Felix|last5=Wang|first5=Tianqi}}</ref>
|-
|[[TOI-2076|TOI-2076 b]]
|
|0.293{{±|0.038}}
|10.35566{{±|0.00006}}
|0.0631{{±|0.0027}}
|870{{±|13}}
| style="background:#FFFF00" |Транзит
|136.70{{±|0.23}}
|0.850{{±|0.025|0.026}}
|5187{{±|54|53}}
|<ref name="Hedges2021" />
|-
|[[TOI-2076|TOI-2076 c]]
|
|0.396{{±|0.004}}
|21.01538{{±|0.00084|0.00074}}
|0.0885{{±|0.0038}}
|734{{±|11}}
| style="background:#FFFF00" |Транзит
|136.70{{±|0.23}}
|0.850{{±|0.025|0.026}}
|5187{{±|54|53}}
|<ref name="Hedges2021" /><ref>{{citation|arxiv=2203.03194|year=2022|title=Uncovering the true periods of the young sub-Neptunes orbiting TOI-2076|doi=10.1051/0004-6361/202243065|last1=Osborn|first1=H.|last2=Bonfanti|first2=A.|last3=Gandolfi|first3=D.|last4=Hedges|first4=C.|last5=Leleu|first5=A.|last6=Fortier|first6=A.|last7=Futyan|first7=D.|last8=Gutermann|first8=P.|last9=Maxted|first9=P.|last10=Borsato|first10=L.|last11=Collins|first11=K.|last12=Gómezmaqueochew|first12=Y.|last13=Hooton|first13=M.J.|last14=Lendl|first14=M.|last15=Parviainen|first15=H.|last16=Salmon|first16=S.|last17=Schanche|first17=N.|last18=Serrano|first18=L.|last19=Sousa|first19=S.|last20=Tuson|first20=A.|last21=Ulmer-Moll|first21=S.|last22=Ulmer-Moll|first22=Solène|author23=Valerie Van Grootel|last24=Wells|first24=R. D.|last25=Wilson|first25=Thomas G.|last26=Alibert|first26=Yann|last27=Alonso|first27=Roi|last28=Anglada|first28=Guillem|last29=Asquier|first29=Joel|author30=David Barrado y Navascues|display-authors=1|journal=Astronomy & Astrophysics|volume=664|pages=A156|s2cid=247292643}}</ref>
|-
|[[TOI-2076|TOI-2076 d]]
|
|0.370{{±|0.006}}
|25.0893{{±|0.01}}
|0.1138{{±|0.0048|0.0049}}
|648{{±|10}}
| style="background:#FFFF00" |Транзит
|136.70{{±|0.23}}
|0.850{{±|0.025|0.026}}
|5187{{±|54|53}}
|<ref name="Hedges2021" />
|-
|[[TOI-2257 b]]
|
|0.196{{±|0.010}}
|35.189346
|0.145{{±|0.003}}
|256{{±|61|17}}
| style="background:#FFFF00" |Транзит
|188.5{{±|0.3}}
|0.33{{±|0.02}}
|3430{{±|130}}
|Планета в зоні, придатній для життя<ref>{{citation|arxiv=2111.01749|year=2022|title=TOI-2257 b: A highly eccentric long-period sub-Neptune Транзитing a nearby M dwarf|last1=Schanche|first1=N.|last2=Pozuelos|first2=F. J.|last3=Günther|first3=M. N.|last4=Wells|first4=R. D.|last5=Burgasser|first5=A. J.|last6=Chinchilla|first6=P.|last7=Delrez|first7=L.|last8=Ducrot|first8=E.|last9=Garcia|first9=L. J.|last10=Gómez Maqueo Chew|first10=Y.|last11=Jofré|first11=E.|last12=Rackham|first12=B. V.|last13=Sebastian|first13=D.|last14=Stassun|first14=K. G.|last15=Stern|first15=D.|last16=Timmermans|first16=M.|last17=Barkaoui|first17=K.|last18=Belinski|first18=A.|last19=Benkhaldoun|first19=Z.|last20=Benz|first20=W.|last21=Charbonneau|first21=D.|last22=Christiansen|first22=Jessie L.|last23=Collins|first23=Karen A.|last24=Demory|first24=B. -O.|last25=Dévora-Pajares|first25=M.|last26=de Wit|first26=J.|last27=Dragomir|first27=D.|last28=Dransfield|first28=G.|last29=Furlan|first29=E.|last30=Ghachou|first30=M.|journal=Astronomy & Astrophysics|volume=657|pages=A45|doi=10.1051/0004-6361/202142280|bibcode=2022A&A...657A..45S|s2cid=240419956|display-authors=1}}</ref>
|-
|[[TOI-712|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}}
| style="background:#FFFF00" |Транзит
|191.2{{±|0.4}}
|0.732{{±|0.027|0.025}}
|4622{{±|61|59}}
|<ref name="Vach2021">{{citation|arxiv=2111.02416|year=2022|title=TOI-712: A System of Adolescent Mini-Neptunes Extending to the Habitable Zone|last1=Vach|first1=Sydney|last2=Quinn|first2=Samuel N.|last3=Vanderburg|first3=Andrew|last4=Kane|first4=Stephen R.|last5=Collins|first5=Karen A.|last6=Kraus|first6=Adam L.|last7=Zhou|first7=George|last8=Medina|first8=Amber A.|last9=Schwarz|first9=Richard P.|last10=Collins|first10=Kevin I.|last11=Conti|first11=Dennis M.|last12=Stockdale|first12=Chris|last13=Massey|first13=Bob|last14=Suarez|first14=Olga|last15=Guillot|first15=Tristan|last16=Mekarnia|first16=Djamel|last17=Abe|first17=Lyu|last18=Dransfield|first18=Georgina|last19=Crouzet|first19=Nicolas|last20=Triaud|first20=Amaury H. M. J.|last21=Schmider|first21=François-Xavier|last22=Agabi|first22=Abelkrim|last23=Buttu|first23=Marco|last24=Furlan|first24=Elise|last25=Gnilka|first25=Crystal L.|last26=Howell|first26=Steve B.|last27=Ziegler|first27=Carl|last28=Briceño|first28=César|last29=Law|first29=Nicholas|last30=Mann|first30=Andrew W.|journal=The Astronomical Journal|volume=164|issue=2|page=71|doi=10.3847/1538-3881/ac7954|s2cid=242757638|display-authors=1}}</ref>
|-
|[[TOI-712|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}}
| style="background:#FFFF00" |Транзит
|191.2{{±|0.4}}
|0.732{{±|0.027|0.025}}
|4622{{±|61|59}}
|<ref name="Vach2021" />
|-
|[[TOI-712|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}}
| style="background:#FFFF00" |Транзит
|191.2{{±|0.4}}
|0.732{{±|0.027|0.025}}
|4622{{±|61|59}}
|<ref name="Vach2021" />
|-
|[[OGLE-2019-BLG-0468Lb]]
|3.43{{±|1.83|1.17}}
|
|
|3.29{{±|4.15|2.52}}
|
| style="background:#0099FF" |Мікролінзування
|14000{{±|3000}}
|0.92{{±|0.49|0.32}}
|
|Багато можливих розв'язків параметрів орбіти<ref name="Han2021-11">{{citation|arxiv=2111.03755|year=2022|title=OGLE-2019-BLG-0468Lb,c: Two Мікролінзування giant planets around a G-type star|last1=Han|first1=Cheongho|last2=Udalski|first2=Andrzej|last3=Lee|first3=Chung-Uk|last4=Kim|first4=Doeon|last5=Zhu|first5=Wei|last6=Albrow|first6=Michael D.|last7=Chung|first7=Sun-Ju|last8=Gould|first8=Andrew|last9=Hwang|first9=Kyu-Ha|author10=Youn Kil Jung|last11=Kim|first11=Hyoun-Woo|last12=Ryu|first12=Yoon-Hyun|last13=Shin|first13=In-Gu|last14=Shvartzvald|first14=Yossi|last15=Yee|first15=Jennifer C.|last16=Zang|first16=Weicheng|last17=Cha|first17=Sang-Mok|last18=Kim|first18=Dong-Jin|last19=Kim|first19=Seung-Lee|last20=Lee|first20=Dong-Joo|last21=Lee|first21=Yongseok|last22=Park|first22=Byeong-Gon|last23=Pogge|first23=Richard W.|last24=Kim|first24=Chun-Hwey|last25=Kim|first25=Woong-Tae|last26=Mróz|first26=Przemek|last27=Szymański|first27=Michał K.|last28=Skowron|first28=Jan|last29=Poleski|first29=Radosław|last30=Soszyński|first30=Igor|journal=Astronomy & Astrophysics|volume=658|pages=A93|doi=10.1051/0004-6361/202142327|bibcode=2022A&A...658A..93H|s2cid=243847948|display-authors=1}}</ref>
|-
|[[OGLE-2019-BLG-0468Lc]]
|10.22{{±|5.46|3.50}}
|
|
|2.77{{±|3.49|2.12}}
|
| style="background:#0099FF" |Мікролінзування
|14000{{±|3000}}
|0.92{{±|0.49|0.32}}
|
|Багато можливих розв'язків параметрів орбіти<ref name="Han2021-11" />
|-
|[[KMT-2021-BLG-0912Lb]]
|0.022{{±|0.007|0.008}}
|
|
|3.03{{±|3.46|2.46}}
|
| style="background:#0099FF" |Мікролінзування
|22000{{±|3000}}
|0.75{{±|0.23|0.28}}
|
|Багато можливих розв'язків параметрів орбіти<ref>{{citation|arxiv=2111.04861|year=2022|title=KMT-2021-BLG-0912Lb: A Мікролінзування super Earth around a K-type star|last1=Han|first1=Cheongho|last2=Bond|first2=Ian A.|last3=Yee|first3=Jennifer C.|last4=Zang|first4=Weicheng|last5=Albrow|first5=Michael D.|last6=Chung|first6=Sun-Ju|last7=Gould|first7=Andrew P.|last8=Hwang|first8=Kyu-Ha|author9=Youn Kil Jung|last10=Kim|first10=Doeon|last11=Lee|first11=Chung-Uk|last12=Ryu|first12=Yoon-Hyun|last13=Shin|first13=In-Gu|last14=Shvartzvald|first14=Yossi|last15=Cha|first15=Sang-Mok|last16=Kim|first16=Dong-Jin|last17=Kim|first17=Seung-Lee|last18=Lee|first18=Dong-Joo|last19=Lee|first19=Yongseok|last20=Park|first20=Byeong-Gon|last21=Pogge|first21=Richard W.|last22=Abe|first22=Fumio|last23=Barry|first23=Richard|last24=Bennett|first24=David P.|last25=Bhattacharya|first25=Aparna|last26=Hirao|first26=Yuki|last27=Fujii|first27=Hirosane|last28=Fukui|first28=Akihiko|last29=Itow|first29=Yoshitaka|last30=Kirikawa|first30=Rintaro|journal=Astronomy & Astrophysics|volume=658|pages=A94|doi=10.1051/0004-6361/202142495|bibcode=2022A&A...658A..94H|s2cid=243860989|display-authors=1}}</ref>
|-
|[[HD 137496|HD 137496 b]]
|0.0127{{±|0.0017}}
|0.117{{±|0.005}}
|1.62116{{±|0.00008}}
|0.02732{{±|0.00019}}
|2130{{±|30|29}}
| style="background:#FFFF00" |Транзит
|509{{±|6}}
|1.035{{±|0.022}}
|5799{{±|61}}
|<ref name="Silva2021">{{citation|arxiv=2111.08764|year=2022|title=The HD 137496 system: A dense, hot super-Mercury and a cold Jupiter|last1=Azevedo Silva|first1=T.|last2=Demangeon|first2=O. D. S.|last3=Barros|first3=S. C. C.|last4=Armstrong|first4=D. J.|last5=Otegi|first5=J. F.|last6=Bossini|first6=D.|last7=Delgado Mena|first7=E.|last8=Sousa|first8=S. G.|last9=Adibekyan|first9=V.|last10=Nielsen|first10=L. D.|last11=Dorn|first11=C.|last12=Lillo-Box|first12=J.|last13=Santos|first13=N. C.|last14=Hoyer|first14=S.|last15=Stassun|first15=K. G.|last16=Almenara|first16=J. M.|last17=Bayliss|first17=D.|last18=Barrado|first18=D.|last19=Boisse|first19=I.|last20=Brown|first20=D. J. A.|last21=Díaz|first21=R. F.|last22=Dumusque|first22=X.|last23=Figueira|first23=P.|last24=Hadjigeorghiou|first24=A.|last25=Hojjatpanah|first25=S.|last26=Mousis|first26=O.|last27=Osborn|first27=A.|last28=Santerne|first28=A.|last29=Strøm|first29=P. A.|last30=Udry|first30=S.|journal=Astronomy & Astrophysics|volume=657|pages=A68|doi=10.1051/0004-6361/202141520|bibcode=2022A&A...657A..68A|s2cid=243809625|display-authors=1}}</ref>
|-
|[[HD 137496|HD 137496 c]]
|7.66{{±|0.11}}
|
|479.9{{±|1.1|1.0}}
|1.2163{{±|0.0087|0.0088}}
|370{{±|5}}
| style="background:#00FF00" |Радіальна швидкість
|509{{±|6}}
|1.035{{±|0.022}}
|5799{{±|61}}
|<ref name="Silva2021" />
|-
|[[HD 19615|HD 19615 b]]
|8.5{{±|0.7}}
|
|402{{±|2}}
|1.1{{±|0.1}}
|
| style="background:#00FF00" |Радіальна швидкість
|872{{±|7}}
|1.1{{±|0.1}}
|3987{{±|125}}
|Материнська зоря&nbsp;— червоний гігант<ref name="Jeong2021">{{citation|arxiv=2111.08899|year=2022|title=Search for exoplanets around northern circumpolar stars|last1=Jeong|first1=G.|last2=Lee|first2=B. C.|last3=Park|first3=M. G.|last4=Bang|first4=T. Y.|last5=Han|first5=I.|journal=Astronomy & Astrophysics|volume=662|pages=A12|doi=10.1051/0004-6361/202142379|s2cid=244270271}}</ref>
|-
|[[HD 150010|HD 150010 b]]
|2.4{{±|0.4}}
|
|562{{±|8}}
|1.1{{±|0.1}}
|
| style="background:#00FF00" |Радіальна швидкість
|473.4{{±|2.1}}
|1.3{{±|0.1}}
|4256{{±|125}}
|Материнська зоря&nbsp;— червоний гігант<ref name="Jeong2021" />
|-
|[[HD 174205|HD 174205 b]]
|4.2{{±|0.5}}
|
|582{{±|17}}
|1.7{{±|0.1}}
|
| style="background:#00FF00" |Радіальна швидкість
|769{{±|5}}
|1.8{{±|0.1}}
|4393{{±|125}}
|Материнська зоря&nbsp;— червоний гігант<ref name="Jeong2021" />
|-
|[[KMT-2018-BLG-1988Lb]]
|0.021{{±|0.015|0.011}}
|
|
|2.83{{±|1.23|0.97}}
|
| style="background:#0099FF" |Мікролінзування
|14000{{±|6000|5000}}
|0.48{{±|0.33|0.25}}
|
|Багато можливих розв'язків параметрів орбіти<ref>{{citation|arxiv=2111.08955|year=2022|title=KMT-2018-BLG-1988Lb: Мікролінзування super-Earth orbiting a low-mass disk dwarf|last1=Han|first1=Cheongho|last2=Gould|first2=Andrew|last3=Albrow|first3=Michael D.|last4=Chung|first4=Sun-Ju|last5=Hwang|first5=Kyu-Ha|author6=Youn Kil Jung|last7=Kim|first7=Doeon|last8=Lee|first8=Chung-Uk|last9=Mao|first9=Shude|last10=Ryu|first10=Yoon-Hyun|last11=Shin|first11=In-Gu|last12=Shvartzvald|first12=Yossi|last13=Yee|first13=Jennifer C.|last14=Zang|first14=Weicheng|last15=Cha|first15=Sang-Mok|last16=Kim|first16=Dong-Jin|last17=Kim|first17=Hyoun-Woo|last18=Kim|first18=Seung-Lee|last19=Lee|first19=Dong-Joo|last20=Lee|first20=Yongseok|last21=Park|first21=Byeong-Gon|last22=Pogge|first22=Richard W.|last23=Kim|first23=Chun-Hwey|journal=Astronomy & Astrophysics|volume=658|pages=A62|doi=10.1051/0004-6361/202142077|bibcode=2022A&A...658A..62H|s2cid=244270928}}</ref>
|-
|[[KOI-984b]]
|0.0544{{±|0.0094}}
|0.384{{±|0.004}}
|4.2881785{{±|0.0000035}}
|0.0504{{±|0.0006}}
|1022{{±|31|30}}
| style="background:#FFFF00" |Транзит
|749{{±|4}}
|0.928{{±|0.031}}
|5295{{±|150}}
|В системі є додаткова планета з неточно відомими параметрами орбіти<ref>{{citation|arxiv=2111.09668|year=2022|title=A highly mutually inclined compact warm-Jupiter system KOI-984?|last1=Sun|first1=Leilei|last2=Ioannidis|first2=Panagiotis|last3=Gu|first3=Shenghong|last4=Schmitt|first4=Jürgen H. M. M.|last5=Wang|first5=Xiaobin|last6=Kouwenhoven|first6=M. B. N.|last7=Perdelwitz|first7=Volker|author8=Francesco Flammini Dotti|last9=Czesla|first9=Stefan|journal=Monthly Notices of the Royal Astronomical Society|volume=512|issue=3|pages=4604–4617|doi=10.1093/mnras/stab3367}}</ref>
|-
|[[TOI-2109b]]
|5.02{{±|0.75}}
|1.347{{±|0.047}}
|0.67247414{{±|0.00000028}}
|0.01791{{±|0.00065}}
|3631{{±|69}}
| style="background:#FFFF00" |Транзит
|846{{±|9}}
|1.447{{±|0.075|0.078}}
|6530{{±|160|150}}
|<ref>{{citation|arxiv=2111.12074|year=2021|title=TOI-2109: An Ultrahot Gas Giant on a 16 hr Orbit|doi=10.3847/1538-3881/ac26bd|last1=Wong|first1=Ian|last2=Shporer|first2=Avi|last3=Zhou|first3=George|last4=Kitzmann|first4=Daniel|last5=Komacek|first5=Thaddeus D.|last6=Tan|first6=Xianyu|last7=Tronsgaard|first7=René|last8=Buchhave|first8=Lars A.|last9=Vissapragada|first9=Shreyas|last10=Greklek-Mckeon|first10=Michael|last11=Rodriguez|first11=Joseph E.|last12=Ahlers|first12=John P.|last13=Quinn|first13=Samuel N.|last14=Furlan|first14=Elise|last15=Howell|first15=Steve B.|last16=Bieryla|first16=Allyson|last17=Heng|first17=Kevin|last18=Knutson|first18=Heather A.|last19=Collins|first19=Karen A.|last20=McLeod|first20=Kim K.|last21=Berlind|first21=Perry|last22=Brown|first22=Peyton|last23=Calkins|first23=Michael L.|last24=De Leon|first24=Jerome P.|last25=Esparza-Borges|first25=Emma|last26=Esquerdo|first26=Gilbert A.|last27=Fukui|first27=Akihiko|last28=Gan|first28=Tianjun|last29=Girardin|first29=Eric|last30=Gnilka|first30=Crystal L.|journal=The Astronomical Journal|volume=162|issue=6|page=256|bibcode=2021AJ....162..256W|s2cid=244488632|display-authors=1}}</ref>
|-
|[[TOI-1238]]b
|0.0183{{±|0.0035}}
|0.108{{±|0.010}}
|0.764596{{±|0.000016|0.000013}}
|0.0139{{±|0.0008}}
|1133{{±|167}}
| style="background:#FFFF00" |Транзит
|2030.44{{±|0.20}}
|0.59{{±|0.02}}
|4089{{±|54}}
|<ref name="Alvarez2021">{{citation|arxiv=2111.14602|year=2022|title=A multi-planetary system orbiting the early-M dwarf TOI-1238|last1=González-Álvarez|first1=E.|last2=Zapatero Osorio|first2=M. R.|last3=Sanz-Forcada|first3=J.|last4=Caballero|first4=J. A.|last5=Reffert|first5=S.|last6=Béjar|first6=V. J. S.|last7=Hatzes|first7=A. P.|last8=Herrero|first8=E.|last9=Jeffers|first9=S. V.|last10=Kemmer|first10=J.|last11=López-González|first11=M. J.|last12=Luque|first12=R.|last13=Molaverdikhani|first13=K.|last14=Morello|first14=G.|last15=Nagel|first15=E.|last16=Quirrenbach|first16=A.|last17=Rodríguez|first17=E.|last18=Rodríguez-López|first18=C.|last19=Schlecker|first19=M.|last20=Schweitzer|first20=A.|last21=Stock|first21=S.|last22=Passegger|first22=V. M.|last23=Trifonov|first23=T.|last24=Amado|first24=P. J.|last25=Baker|first25=D.|last26=Boyd|first26=P. T.|last27=Cadieux|first27=C.|last28=Charbonneau|first28=D.|last29=Collins|first29=K. A.|last30=Doyon|first30=R.|journal=Astronomy & Astrophysics|volume=658|pages=A138|doi=10.1051/0004-6361/202142128|bibcode=2022A&A...658A.138G|s2cid=244715047|display-authors=1}}</ref>
|-
|[[TOI-1238]]c
|0.0262{{±|0.0059}}
|0.188{{±|0.013}}
|3.294733{{±|0.000040|0.000047}}
|0.037{{±|0.002}}
|695{{±|105}}
| style="background:#FFFF00" |Транзит
|2030.44{{±|0.20}}
|0.59{{±|0.02}}
|4089{{±|54}}
|<ref name="Alvarez2021" />
|-
|[[K2-99c]]
|8.4{{±|0.2}}
|
|522.2{{±|1.4}}
|1.43{{±|0.01}}
|390{{±|6}}
| style="background:#00FF00" |Радіальна швидкість
|1980
|1.6
|5990
|<ref>{{citation|arxiv=2111.14660|year=2021|title=K2-99 revisited: A non-inflated warm Jupiter, and a temperate giant planet on a 522-d orbit around a subgiant|doi=10.1093/mnras/stab3497|last1=Smith|first1=A M S.|last2=Breton|first2=S. N.|last3=Csizmadia|first3=Sz|last4=Dai|first4=F.|last5=Gandolfi|first5=D.|last6=García|first6=R. A.|last7=Howard|first7=A. W.|last8=Isaacson|first8=H.|last9=Korth|first9=J.|last10=Lam|first10=K W F.|last11=Mathur|first11=S.|last12=Nowak|first12=G.|last13=Hernández|first13=F Pérez|last14=Persson|first14=C. M.|last15=Albrecht|first15=S. H.|last16=Barragán|first16=O.|last17=Cabrera|first17=J.|last18=Cochran|first18=W. D.|last19=Deeg|first19=H. J.|last20=Fridlund|first20=M.|last21=Georgieva|first21=I. Y.|last22=Goffo|first22=E.|last23=Guenther|first23=E. W.|last24=Hatzes|first24=A. P.|last25=Kabath|first25=P.|last26=Livingston|first26=J. H.|last27=Luque|first27=R.|last28=Palle|first28=E.|last29=Redfield|first29=S.|last30=Rodler|first30=F.|journal=Monthly Notices of the Royal Astronomical Society|volume=510|issue=4|pages=5035–5049|display-authors=1}}</ref>
|-
|[[HIP 5763b]]
|0.51
|
|30.014{{±|0.1528|0.2842}}
|0.170
|
| style="background:#00FF00" |Радіальна швидкість
|104.17{{±|0.14}}
|0.72
|
|<ref name="Paredes2021">{{citation|arxiv=2111.15028|year=2021|title=The Solar Neighborhood XLVIII: Nine Giant Planets Orbiting Nearby K Dwarfs, and the CHIRON Spectrograph's Radial Velocity Performance|doi=10.3847/1538-3881/ac082a|last1=Paredes|first1=Leonardo A.|last2=Henry|first2=Todd J.|last3=Quinn|first3=Samuel N.|last4=Gies|first4=Douglas R.|last5=Hinojosa-Goñi|first5=Rodrigo|last6=James|first6=Hodari-Sadiki|last7=Jao|first7=Wei-Chun|last8=White|first8=Russel J.|journal=The Astronomical Journal|volume=162|issue=5|page=176|bibcode=2021AJ....162..176P|s2cid=237285778}}</ref>
|-
|[[HIP 34222b]]
|0.83
|
|160.0{{±|2.7|2.9}}
|0.492
|
| style="background:#00FF00" |Радіальна швидкість
|74.55{{±|0.09}}
|0.62
|
|<ref name="Paredes2021" />
|-
|[[HIP 86221b]]
|0.71
|
|2.224{{±|0.0004|0.0005}}
|0.031
|
| style="background:#00FF00" |Радіальна швидкість
|96{{±|11}}
|0.79
|
|<ref name="Paredes2021" />
|-
|[[TOI-1842b]]
|0.214{{±|0.040|0.038}}
|1.04{{±|0.06|0.05}}
|9.5739{{±|0.0002|0.0001}}
|0.01001{{±|0.0007}}
|
| style="background:#FFFF00" |Транзит
|729{{±|7}}
|1.46{{±|0.03}}
|6230{{±|50}}
|<ref>{{citation|arxiv=2112.00198|year=2021|title=TOI-1842b: A Транзитing Warm Saturn Undergoing Re-Inflation around an Evolving Subgiant|last1=Wittenmyer|first1=Robert A.|last2=Clark|first2=Jake T.|last3=Trifonov|first3=Trifon|last4=Addison|first4=Brett C.|last5=Wright|first5=Duncan J.|last6=Stassun|first6=Keivan G.|last7=Horner|first7=Jonathan|last8=Lowson|first8=Nataliea|last9=Kielkopf|first9=John|last10=Kane|first10=Stephen R.|last11=Plavchan|first11=Peter|last12=Shporer|first12=Avi|last13=Zhang|first13=Hui|last14=Bowler|first14=Brendan P.|last15=Mengel|first15=Matthew W.|last16=Okumura|first16=Jack|last17=Rabus|first17=Markus|last18=Johnson|first18=Marshall C.|last19=Harbeck|first19=Daniel|last20=Tronsgaard|first20=Rene|last21=Buchhave|first21=Lars A.|last22=Collins|first22=Karen A.|last23=Collins|first23=Kevin I.|last24=Gan|first24=Tianjun|last25=Jensen|first25=Eric L. N.|last26=Howell|first26=Steve B.|last27=Furlan|first27=E.|last28=Gnilka|first28=Crystal L.|last29=Lester|first29=Kathryn V.|last30=Matson|first30=Rachel A.|journal=The Astronomical Journal|volume=163|issue=2|page=82|doi=10.3847/1538-3881/ac3f39|bibcode=2022AJ....163...82W|s2cid=244773259|display-authors=1}}</ref>
|-
|[[Gliese 367 b]]
|0.0017{{±|0.0002}}
|0.064{{±|0.005}}
|0.321962{{±|0.000010|0.000012}}
|0.0071{{±|0.0002}}
|1745{{±|43}}
| style="background:#FFFF00" |Транзит
|30.695{{±|0.016}}
|0.45{{±|0.011}}
|3522{{±|70}}
|<ref>{{citation|arxiv=2112.01309|year=2021|title=GJ 367b: A dense, ultrashort-period sub-Earth planet Транзитing a nearby red dwarf star|doi=10.1126/science.aay3253|last1=Lam|first1=Kristine W. F.|last2=Csizmadia|first2=Szilárd|last3=Astudillo-Defru|first3=Nicola|last4=Bonfils|first4=Xavier|last5=Gandolfi|first5=Davide|last6=Padovan|first6=Sebastiano|last7=Esposito|first7=Massimiliano|last8=Hellier|first8=Coel|last9=Hirano|first9=Teruyuki|last10=Livingston|first10=John|last11=Murgas|first11=Felipe|last12=Smith|first12=Alexis M. S.|last13=Collins|first13=Karen A.|last14=Mathur|first14=Savita|last15=Garcia|first15=Rafael A.|last16=Howell|first16=Steve B.|last17=Santos|first17=Nuno C.|last18=Dai|first18=Fei|last19=Ricker|first19=George R.|last20=Vanderspek|first20=Roland|last21=Latham|first21=David W.|last22=Seager|first22=Sara|last23=Winn|first23=Joshua N.|last24=Jenkins|first24=Jon M.|last25=Albrecht|first25=Simon|last26=Almenara|first26=Jose M.|last27=Artigau|first27=Etienne|last28=Barragán|first28=Oscar|last29=Bouchy|first29=François|last30=Cabrera|first30=Juan|journal=Science|volume=374|issue=6572|pages=1271–1275|pmid=34855492|bibcode=2021Sci...374.1271L|s2cid=244799656|display-authors=1}}</ref>
|-
|[[HATS-74Ab]] ('''TOI-737''')
|1.46{{±|0.14}}
|1.032{{±|0.021}}
|1.73185606{{±|0.00000055}}
|0.02384{{±|0.00011}}
|895.1{{±|5.7}}
| style="background:#FFFF00" |Транзит
|952{{±|12}}
|0.601{{±|0.008}}
|3775{{±|54}}
|<ref name="Jordan2021">{{citation|arxiv=2112.01928|year=2022|title=HATS-74Ab, HATS-75b, HATS-76b, and HATS-77b: Four Транзитing Giant Planets Around K and M Dwarfs|last1=Jordán|first1=A.|last2=Hartman|first2=J. D.|last3=Bayliss|first3=D.|last4=Bakos|first4=G. Á.|last5=Brahm|first5=R.|last6=Bryant|first6=E. M.|last7=Csubry|first7=Z.|last8=Henning|first8=Th.|last9=Hobson|first9=M.|last10=Mancini|first10=L.|last11=Penev|first11=K.|last12=Rabus|first12=M.|last13=Suc|first13=V.|last14=de Val-Borro|first14=M.|last15=Wallace|first15=J.|last16=Barkaoui|first16=K.|last17=Ciardi|first17=D. R.|last18=Collins|first18=K. A.|last19=Esparza-Borges|first19=E.|last20=Furlan|first20=E.|last21=Gan|first21=T.|last22=Ghachoui|first22=M.|last23=Gillon|first23=M.|last24=Howell|first24=S.|last25=Jehin|first25=E.|last26=Fukui|first26=A.|last27=Kawauchi|first27=K.|last28=Livingston|first28=J. H.|last29=Luque|first29=R.|last30=Matson|first30=R.|journal=The Astronomical Journal|volume=163|issue=3|page=125|doi=10.3847/1538-3881/ac4a77|bibcode=2022AJ....163..125J|s2cid=244896205|display-authors=1}}</ref>
|-
|[[HATS-75b]] ('''TOI-552''')
|0.491{{±|0.039}}
|0.884{{±|0.013}}
|2.7886556{{±|0.0000011}}
|0.032742{{±|0.000134|0.000099}}
|772.3{{±|2.3}}
| style="background:#FFFF00" |Транзит
|640{{±|4}}
|0.6017{{±|0.0074|0.0055}}
|3812{{±|79}}
|<ref name="Jordan2021" />
|-
|[[HATS-76b]] ('''TOI-555''')
|2.629{{±|0.089}}
|1.079{{±|0.031}}
|1.9416423{{±|0.0000014}}
|0.02658{{±|0.00021|0.00029}}
|939.8{{±|6.7}}
| style="background:#FFFF00" |Транзит
|1272{{±|19}}
|0.662{{±|0.016|0.021}}
|3990{{±|120}}
|<ref name="Jordan2021" />
|-
|[[HATS-77b]] ('''TOI-730''')
|1.374{{±|0.100|0.074}}
|1.165{{±|0.021}}
|3.0876262{{±|0.0000016}}
|0.03607{{±|0.00025}}
|828.3{{±|5.9}}
| style="background:#FFFF00" |Транзит
|1440{{±|40}}
|0.655{{±|0.014}}
|4082{{±|69}}
|<ref name="Jordan2021" />
|-
|[[KOI-4777b]]
|
|0.046{{±|0.003}}
|0.412000{{±|0.000001}}
|0.0080{{±|0.0003}}
|1180{{±|20}}
| style="background:#FFFF00" |Транзит
|565{{±|4}}
|0.41{{±|0.02}}
|3515{{±|69}}
|<ref>{{citation|arxiv=2112.03958|year=2022|title=A Hot Mars-sized Exoplanet Транзитing an M Dwarf|doi=10.3847/1538-3881/ac3088|last1=Cañas|first1=Caleb I.|last2=Mahadevan|first2=Suvrath|last3=Cochran|first3=William D.|last4=Bender|first4=Chad F.|last5=Feigelson|first5=Eric D.|last6=Harman|first6=C. E.|last7=Kopparapu|first7=Ravi Kumar|last8=Caceres|first8=Gabriel A.|last9=Diddams|first9=Scott A.|last10=Endl|first10=Michael|last11=Ford|first11=Eric B.|last12=Halverson|first12=Samuel|last13=Hearty|first13=Fred|last14=Jones|first14=Sinclaire|last15=Kanodia|first15=Shubham|last16=Lin|first16=Andrea S. J.|last17=Metcalf|first17=Andrew J.|last18=Monson|first18=Andrew|last19=Ninan|first19=Joe P.|last20=Ramsey|first20=Lawrence W.|last21=Robertson|first21=Paul|last22=Roy|first22=Arpita|last23=Schwab|first23=Christian|last24=Stefánsson|first24=Guđmundur|journal=The Astronomical Journal|volume=163|issue=1|page=3|bibcode=2022AJ....163....3C|s2cid=244954104}}</ref>
|-
|[[BD+60 1417b]]
|15{{±|5}}
|1.31{{±|0.06}}
|
|1662
|1303{{±|74}}
| style="background:#FF6CDA" |Пряме спостереження
|146.65{{±|0.09}}
|1.0
|4993{{±|124}}
|Молода материнська зоря<ref>{{citation|arxiv=2112.04678|year=2021|title=A Wide Planetary Mass Companion Discovered through the Citizen Science Project Backyard Worlds: Planet 9|doi=10.3847/1538-4357/ac2499|last1=Faherty|first1=Jacqueline K.|last2=Gagné|first2=Jonathan|last3=Popinchalk|first3=Mark|last4=Vos|first4=Johanna M.|last5=Burgasser|first5=Adam J.|last6=Schümann|first6=Jörg|last7=Schneider|first7=Adam C.|last8=Kirkpatrick|first8=J. Davy|last9=Meisner|first9=Aaron M.|last10=Kuchner|first10=Marc J.|last11=Bardalez Gagliuffi|first11=Daniella C.|last12=Marocco|first12=Federico|last13=Caselden|first13=Dan|last14=Gonzales|first14=Eileen C.|last15=Rothermich|first15=Austin|last16=Casewell|first16=Sarah L.|last17=Debes|first17=John H.|last18=Aganze|first18=Christian|last19=Ayala|first19=Andrew|last20=Hsu|first20=Chih-Chun|last21=Cooper|first21=William J.|last22=Smart|first22=R. L.|last23=Gerasimov|first23=Roman|last24=Theissen|first24=Christopher A.|author25=The Backyard Worlds|author26=Planet 9 Collaboration|journal=The Astrophysical Journal|volume=923|issue=1|page=48|bibcode=2021ApJ...923...48F|s2cid=245005964}}</ref>
|-
|[[b Центавра b]]
|10.9{{±|1.6}}
|
|200000{{±|100000}}
|556{{±|17}}
|
| style="background:#FF6CDA" |Пряме спостереження
|325{{±|10}}
|8{{±|2}}
|
|Планета в подвійній системі з масивною головною зорею<ref>{{citation|arxiv=2112.04833|year=2021|title=A wide-orbit giant planet in the high-mass b Centauri binary system|doi=10.1038/s41586-021-04124-8|last1=Janson|first1=Markus|last2=Gratton|first2=Raffaele|last3=Rodet|first3=Laetitia|last4=Vigan|first4=Arthur|last5=Bonnefoy|first5=Mickaël|last6=Delorme|first6=Philippe|last7=Mamajek|first7=Eric E.|last8=Reffert|first8=Sabine|last9=Stock|first9=Lukas|last10=Marleau|first10=Gabriel-Dominique|last11=Langlois|first11=Maud|last12=Chauvin|first12=Gaël|last13=Desidera|first13=Silvano|last14=Ringqvist|first14=Simon|last15=Mayer|first15=Lucio|last16=Viswanath|first16=Gayathri|last17=Squicciarini|first17=Vito|last18=Meyer|first18=Michael R.|last19=Samland|first19=Matthias|last20=Petrus|first20=Simon|last21=Helled|first21=Ravit|last22=Kenworthy|first22=Matthew A.|last23=Quanz|first23=Sascha P.|last24=Biller|first24=Beth|last25=Henning|first25=Thomas|last26=Mesa|first26=Dino|last27=Engler|first27=Natalia|last28=Carson|first28=Joseph C.|journal=Nature|volume=600|issue=7888|pages=231–234|pmid=34880428|bibcode=2021Natur.600..231J|s2cid=245005994}}</ref>
|-
|[[HD 360|HD 360 b]]
|0.75{{±|0.12|0.15}}
|
|273.1{{±|1.6|0.8}}
|0.98{{±|0.11|0.03}}
|
| style="background:#00FF00" |Радіальна швидкість
|362
|1.69{{±|0.15|0.53}}
|4770
|<ref name="Teng2021">{{citation|arxiv=2112.07169|year=2021|title=Regular radial velocity variations in nine G- and K-type giant stars: Eight planets and one planet candidate|doi=10.1093/pasj/psab112|last1=Teng|first1=Huan-Yu|last2=Sato|first2=Bun'ei|last3=Takarada|first3=Takuya|last4=Omiya|first4=Masashi|last5=Harakawa|first5=Hiroki|last6=Izumiura|first6=Hideyuki|last7=Kambe|first7=Eiji|last8=Takeda|first8=Yoichi|last9=Yoshida|first9=Michitoshi|last10=Itoh|first10=Yoichi|last11=Ando|first11=Hiroyasu|last12=Kokubo|first12=Eiichiro|journal=Publications of the Astronomical Society of Japan|volume=74|pages=92–127}}</ref>
|-
|[[Епсилон Риб b]]
|0.77{{±|0.16|0.10}}
|
|255.3{{±|2.1|1.4}}
|0.88{{±|0.11|0.10}}
|
| style="background:#00FF00" |Радіальна швидкість
|183.2
|1.41{{±|1.45|0.50}}
|4824
|Кандидат, не підтверджена<ref name="Teng2021" />
|-
|[[HD 10975|HD 10975 b]]
|0.45{{±|0.06|0.15}}
|
|283.8{{±|12.7|0.1}}
|0.95{{±|0.06|0.08}}
|
| style="background:#00FF00" |Радіальна швидкість
|379
|1.41{{±|0.34|0.35}}
|4840
|<ref name="Teng2021" />
|-
|[[HD 79181|HD 79181 b]]
|0.64{{±|0.06|0.16}}
|
|273.1{{±|1.3|0.4}}
|0.90{{±|0.07|0.08}}
|
| style="background:#00FF00" |Радіальна швидкість
|337
|1.28{{±|0.32|0.28}}
|4862
|<ref name="Teng2021" />
|-
|[[HD 99183|HD 99183 b]]
|0.97{{±|0.06|0.25}}
|
|310.4{{±|5.2|1.7}}
|1.08{{±|0.05|0.07}}
|
| style="background:#00FF00" |Радіальна швидкість
|355
|1.76{{±|0.31|0.30}}
|4886
|<ref name="Teng2021" />
|-
|[[Upsilon Leonis|Upsilon Leonis b]]
|0.51{{±|0.06|0.26}}
|
|385.2{{±|2.8|1.3}}
|1.18{{±|0.11|0.32}}
|
| style="background:#00FF00" |Радіальна швидкість
|177.8
|1.48{{±|0.90|0.38}}
|4836
|<ref name="Teng2021" />
|-
|[[HD 161178|HD 161178 b]]
|0.57{{±|0.02|0.16}}
|
|279.3{{±|1.0|0.8}}
|0.85{{±|0.05|0.07}}
|
| style="background:#00FF00" |Радіальна швидкість
|351
|1.06{{±|0.25|0.17}}
|4786
|<ref name="Teng2021" />
|-
|[[HD 219139|HD 219139 b]]
|0.78{{±|0.05|0.20}}
|
|275.5{{±|2.3|1.0}}
|0.94{{±|0.06|0.07}}
|
| style="background:#00FF00" |Радіальна швидкість
|345
|1.46{{±|0.31|0.29}}
|4831
|<ref name="Teng2021" />
|-
|[[Гамма Риб b]]
|1.34{{±|0.02|0.31}}
|
|555.1{{±|6.0|2.5}}
|1.32{{±|0.05|0.08}}
|
| style="background:#00FF00" |Радіальна швидкість
|138
|0.99{{±|0.17|0.13}}
|4742
|<ref name="Teng2021" />
|-
|[[OGLE-2014-BLG-0676Lb]]
|3.68{{±|0.69|1.44}}
|
|
|4.53{{±|1.49|2.50}}
|
| style="background:#0099FF" |Мікролінзування
|8700{{±|2500|4600}}
|0.73{{±|0.14|0.29}}
|
|<ref>{{citation|arxiv=2112.08030|year=2022|title=Characterizing Мікролінзування planetary system OGLE-2014-BLG-0676Lb with adaptive optics Пряме спостереження|doi=10.1088/1674-4527/ac2a09|last1=Xie|first1=Xiao-Jia|last2=Dong|first2=Subo|last3=Shvartzvald|first3=Yossi|last4=Gould|first4=Andrew|last5=Udalski|first5=Andrzej|last6=Beaulieu|first6=Jean-Philippe|last7=Beichman|first7=Charles|last8=Close|first8=Laird Miller|last9=b. Henderson|first9=Calen|last10=r. Males|first10=Jared|last11=Marquette|first11=Jean-Baptiste|last12=m. Morzinski|first12=Katie|last13=r. Gelino|first13=Christopher|journal=Research in Astronomy and Astrophysics|volume=21|issue=12|page=303|s2cid=244211319}}</ref>
|-
|[[HD 103891|HD 103891 b]]
|1.44{{±|0.06|0.05}}
|
|1919{{±|14|15}}
|3.27{{±|0.02|0.01}}
|
| style="background:#00FF00" |Радіальна швидкість
|179.0{{±|0.4}}
|1.28{{±|0.01}}
|6072{{±|20}}
|<ref name="Sreenivas2021">{{citation|arxiv=2112.09029|year=2022|title=Analysis of the public HARPS/ESO spectroscopic archive|last1=Sreenivas|first1=K. R.|last2=Perdelwitz|first2=V.|last3=Tal-Or|first3=L.|last4=Trifonov|first4=T.|last5=Zucker|first5=S.|last6=Mazeh|first6=T.|journal=Astronomy & Astrophysics|volume=660|pages=A124|doi=10.1051/0004-6361/202142612|s2cid=245219286}}</ref>
|-
|[[HD 105779|HD 105779 b]]
|0.64{{±|0.06}}
|
|2412{{±|55|52}}
|3.38{{±|0.05}}
|
| style="background:#00FF00" |Радіальна швидкість
|179.7{{±|0.3}}
|0.89{{±|0.01}}
|5792{{±|16}}
|<ref name="Sreenivas2021" />
|-
|[[HD 73583]]b ('''TOI 560''')
|
|0.253{{±|0.014|0.011}}
|6.3980661{{±|0.0000095|0.0000097}}
|0.05995{{±|0.00074|0.00072}}
|742.7{{±|7.2|7.0}}
| style="background:#FFFF00" |Транзит
|102.97{{±|0.10}}
|0.701{{±|0.026|0.025}}
|4574{{±|62|61}}
|<ref name="Mufti2021">{{citation|arxiv=2112.13448|year=2021|title=TOI 560 : Two Транзитing Planets Orbiting a K Dwarf Validated with iSHELL, PFS and HIRES RVs|author1=Mohammed El Mufti|last2=Plavchan|first2=Peter P.|last3=Isaacson|first3=Howard|last4=Cale|first4=Bryson L.|last5=Feliz|first5=Dax L.|last6=Reefe|first6=Michael A.|last7=Hellier|first7=Coel|last8=Stassun|first8=Keivan|last9=Eastman|first9=Jason|last10=Polanski|first10=Alex|last11=Crossfield|first11=Ian J. M.|last12=Gaidos|first12=Eric|last13=Kostov|first13=Veselin|last14=Villasenor|first14=Joel|last15=Schlieder|first15=Joshua E.|last16=Bouma|first16=Luke G.|last17=Collins|first17=Kevin I.|last18=Wittrock|first18=Justin M.|last19=Zohrabi|first19=Farzaneh|last20=Lee|first20=Rena A.|last21=Sohani|first21=Ahmad|last22=Berberian|first22=John|last23=Vermilion|first23=David|last24=Newman|first24=Patrick|last25=Geneser|first25=Claire|last26=Tanner|first26=Angelle|last27=Batalha|first27=Natalie M.|last28=Dressing|first28=Courtney|last29=Fulton|first29=Benjamin|last30=Howard|first30=Andrew W.|display-authors=1}}</ref>
|-
|[[HD 73583]]c ('''TOI 560''')
|
|0.2433{{±|0.011|0.0096}}
|18.8805{{±|0.0024|0.0011}}
|0.1233{{±|0.0015}}
|517.8{{±|5|4.9}}
| style="background:#FFFF00" |Транзит
|102.97{{±|0.10}}
|0.701{{±|0.026|0.025}}
|4574{{±|62|61}}
|<ref name="Mufti2021" />
|-
|[[OGLE-2014-BLG-0319Lb]]
|0.57{{±|0.36|0.31}}
|
|
|3.49{{±|1.17|1.12}}
|
| style="background:#0099FF" |Мікролінзування
|25000{{±|4000|9000}}
|0.52{{±|0.33|0.29}}
|
|<ref>{{citation|arxiv=2112.14997|year=2022|title=OGLE-2014-BLG-0319: A Sub-Jupiter-mass Planetary Event Encountered Degeneracy with Different Mass Ratios and Lens-source Relative Proper Motions|last1=Miyazaki|first1=Shota|last2=Suzuki|first2=Daisuke|last3=Udalski|first3=Andrzej|last4=Koshimoto|first4=Naoki|last5=Bennett|first5=David P.|last6=Rattenbury|first6=Nicholas J.|last7=Sumi|first7=Takahiro|last8=Abe|first8=Fumio|last9=Barry|first9=Richard K.|last10=Bhattacharya|first10=Aparna|last11=Bond|first11=Ian A.|last12=Fukui|first12=Akihiko|last13=Fujii|first13=Hirosane|last14=Hirao|first14=Yuki|last15=Silva|first15=Stela|last16=Itow|first16=Yoshitaka|last17=Kirikawa|first17=Rintaro|last18=Kondo|first18=Iona|last19=Munford|first19=Brandon|last20=Matsubara|first20=Y.|last21=Matsumoto|first21=Sho|last22=Muraki|first22=Yasushi|last23=Okamura|first23=Arisa|last24=Olmschenk|first24=Greg|last25=Ranc|first25=Clément|last26=Satoh|first26=Yuki K.|last27=Toda|first27=Taiga|last28=Tristram|first28=P. J.|last29=Yama|first29=Hibiki|last30=Yonehara|first30=A.|journal=The Astronomical Journal|volume=163|issue=3|page=123|doi=10.3847/1538-3881/ac4960|bibcode=2022AJ....163..123M|s2cid=245634898|display-authors=1}}</ref>
|-
|[[OGLE-2018-BLG-0383L b]]
|0.0201{{±|0.0173|0.0088}}
|
|
|1.8{{±|0.2}}
|
| style="background:#0099FF" |Мікролінзування
|25000{{±|2000}}
|0.10{{±|0.13|0.05}}
|
|<ref>{{citation|arxiv=2112.02414|year=2022|title=Systematic Korea Мікролінзування Telescope Network planetary anomaly search – III. One wide-orbit planet and two stellar binaries|doi=10.1093/mnras/stab3581|last1=Wang(王涵悦)|first1=Hanyue|last2=Zang(臧伟呈)|first2=Weicheng|last3=Zhu(祝伟)|first3=Wei|last4=Hwang|first4=Kyu-Ha|last5=Udalski|first5=Andrzej|last6=Gould|first6=Andrew|last7=Han|first7=Cheongho|last8=Albrow|first8=Michael D.|last9=Chung|first9=Sun-Ju|last10=Jung|first10=Youn Kil|last11=Kim|first11=Doeon|last12=Ryu|first12=Yoon-Hyun|last13=Shin|first13=In-Gu|last14=Shvartzvald|first14=Yossi|last15=Yee|first15=Jennifer C.|last16=Cha|first16=Sang-Mok|last17=Kim|first17=Dong-Jin|last18=Kim|first18=Hyoun-Woo|last19=Kim|first19=Seung-Lee|last20=Lee|first20=Chung-Uk|last21=Lee|first21=Dong-Joo|last22=Lee|first22=Yongseok|last23=Park|first23=Byeong-Gon|last24=Pogge|first24=Richard W.|last25=Poleski|first25=Radoslaw|last26=Mróz|first26=Przemek|last27=Skowron|first27=Jan|last28=Szymański|first28=Michał K.|last29=Soszyński|first29=Igor|last30=Pietrukowicz|first30=Paweł|journal=Monthly Notices of the Royal Astronomical Society|volume=510|issue=2|pages=1778–1790|display-authors=1}}</ref>
|}

== Див. також ==
* [[Списки екзопланет]]
* Списки екзопланет за роком відкриття: [[Список екзопланет, відкритих до 2000 року|до 2000]], [[Список екзопланет, відкритих в 2000-2009 роках|2000–2009]], [[Список екзопланет, відкритих у 2010 році|2010]], [[Список екзопланет, відкритих у 2011 році|2011]], [[Список екзопланет, відкритих у 2012 році|2012]], [[Список екзопланет, відкритих у 2013 році|2013]], [[Список екзопланет, відкритих у 2014 році|2014]], [[Список екзопланет, відкритих у 2015 році|2015]], [[Список екзопланет, відкритих у 2016 році|2016]], [[Список екзопланет, відкритих у 2017 році|2017]], [[Список екзопланет, відкритих у 2018 році|2018]], [[Список екзопланет, відкритих у 2019 році|2019]], [[Список екзопланет, відкритих у 2020 році|2020]], '''2021''', [[Список екзопланет, відкритих у 2022 році|2022]], [[Список екзопланет, відкритих у 2023 році|2023]]

== Література ==
<references group=""></references>{{Екзопланети за роком відкриття}}{{Екзопланети}}
[[Категорія:Списки астрономічних об'єктів]]
[[Категорія:Екзопланети за роком відкриття]]
Шаблони, використані на цій сторінці:
Шаблон:Citation (переглянути вихідний код) (частково захищено)
Шаблон:Cite arXiv (редагувати)
Шаблон:Cite journal (переглянути вихідний код) (захищено)
Шаблон:Cite web (переглянути вихідний код) (захищено)
Шаблон:Hlist/styles.css (переглянути вихідний код) (захищено)
Шаблон:Ill (редагувати)
Шаблон:Interlanguage link multi (редагувати)
Шаблон:Jupiter mass (редагувати)
Шаблон:Jupiter radius (редагувати)
Шаблон:Navbox (переглянути вихідний код) (захищено)
Шаблон:Separated entries (редагувати)
Шаблон:Solar mass (редагувати)
Шаблон:Su (редагувати)
Шаблон:± (редагувати)
Шаблон:Екзопланети (редагувати)
Шаблон:Екзопланети за роком відкриття (редагувати)
Шаблон:Маса Сонця (редагувати)
Шаблон:Окремі пункти (редагувати)
Модуль:Arguments (переглянути вихідний код) (захищено)
Модуль:Citation/CS1 (переглянути вихідний код) (захищено)
Модуль:Citation/CS1/COinS (переглянути вихідний код) (захищено)
Модуль:Citation/CS1/Configuration (переглянути вихідний код) (захищено)
Модуль:Citation/CS1/Identifiers (переглянути вихідний код) (захищено)
Модуль:Citation/CS1/Utilities (переглянути вихідний код) (захищено)
Модуль:Citation/CS1/Whitelist (переглянути вихідний код) (захищено)
Модуль:Citation/CS1/styles.css (переглянути вихідний код) (захищено)
Модуль:Navbar (переглянути вихідний код) (захищено)
Модуль:Navbar/configuration (переглянути вихідний код) (захищено)
Модуль:Navbar/styles.css (переглянути вихідний код) (захищено)
Модуль:Navbox (переглянути вихідний код) (захищено)
Модуль:Navbox/configuration (переглянути вихідний код) (захищено)
Модуль:Navbox/styles.css (переглянути вихідний код) (захищено)
Модуль:Su (редагувати)
Модуль:TableTools (переглянути вихідний код) (захищено)
Модуль:Окремі пункти (переглянути вихідний код) (частково захищено)
Повернення до сторінки «Список екзопланет, відкритих у 2021 році».
Отримано з https://uk.wikipedia.org/wiki/Список_екзопланет,_відкритих_у_2021_році