List of exoplanets discovered in 2014

{{Short description|None}}

This is a List of exoplanets discovered in 2014.

For exoplanets detected only by radial velocity, the mass value is actually a lower limit. (See Minimum mass for more information)

class="wikitable plainrowheaders sortable" style="width: 100%; font-size: 83%; text-align: center;"

!Name

!data-sort-type="number"|Mass ({{Jupiter mass}})

!data-sort-type="number"|Radius ({{Jupiter radius}})

!data-sort-type="number"|Period (days)

!data-sort-type="number"|Semi-major axis (AU)

!data-sort-type="number"|Temp. (K){{Cite web

|url = https://exoplanet.eu/catalog/

|title = The Extrasolar Planets Encyclopaedia

|date = 1995

|access-date = 2015-11-09}}

!Discovery method

!data-sort-type="number"|Distance (ly)

!data-sort-type="number"|Host star mass ({{solar mass|link=yes}})

!data-sort-type="number"|Host star temp. (K)

!Remarks

BD-11 4672 b

|0.53

|

|1667

|2.28

|

|style="background:#00FF00"|radial vel.

|89

|0.57

|4475

|{{citation|arxiv=1412.6591|year=2014|title=The HARPS search for southern extra-solar planets XXXVI: Five new long-period giant planets and a system update|doi=10.1051/0004-6361/201424965|last1=Moutou|first1=C.|last2=Lo Curto|first2=G.|last3=Mayor|first3=M.|last4=Bouchy|first4=F.|last5=Benz|first5=W.|last6=Lovis|first6=C.|last7=Naef|first7=D.|last8=Pepe|first8=F.|last9=Queloz|first9=D.|last10=Santos|first10=N. C.|last11=Ségransan|first11=D.|last12=Sousa|first12=S. G.|last13=Udry|first13=S.|journal=Astronomy & Astrophysics|volume=576|pages=A48|s2cid=118512899}}

Beta Cancri b

|7.8

|

|605.2

|1.7

|

|style="background:#00FF00"|radial vel.

|290.4

|1.7

|4092.1

|

Beta Ursae Minoris b

|6.1

|

|522.3

|1.4

|

|style="background:#00FF00"|radial vel.

|126.5

|1.4

|4126

|

COROT-22b

|0.038

|0.435

|9.75598

|0.092

|885

|style="background:#FFFF00"|transit

|1930

|1.1

|5939

|{{citation|arxiv=1408.2576|year=2014|title=CoRoT-22 b: A validated 4.9 R⊕ exoplanet in 10-d orbit★†|doi=10.1093/mnras/stu1645|last1=Moutou|first1=C.|last2=Almenara|first2=J. M.|last3=Díaz|first3=R. F.|last4=Alonso|first4=R.|last5=Deleuil|first5=M.|last6=Guenther|first6=E.|last7=Pasternacki|first7=T.|last8=Aigrain|first8=S.|last9=Baglin|first9=A.|last10=Barge|first10=P.|last11=Bonomo|first11=A. S.|last12=Bordé|first12=P.|last13=Bouchy|first13=F.|last14=Cabrera|first14=J.|last15=Carpano|first15=S.|last16=Cochran|first16=W. D.|last17=Csizmadia|first17=Sz.|last18=Deeg|first18=H. J.|last19=Dvorak|first19=R.|last20=Endl|first20=M.|last21=Erikson|first21=A.|last22=Ferraz-Mello|first22=S.|last23=Fridlund|first23=M.|last24=Gandolfi|first24=D.|last25=Guillot|first25=T.|last26=Hatzes|first26=A.|last27=Hébrard|first27=G.|last28=Lovis|first28=C.|last29=Lammer|first29=H.|last30=MacQueen|first30=P. J.|journal=Monthly Notices of the Royal Astronomical Society|volume=444|issue=3|pages=2783–2792|doi-access=free |display-authors=1}}

COROT-24b

|0.018

|0.33

|5.1134

|0.056

|1070

|style="background:#FFFF00"|transit

|2000

|0.91

|4950

|{{citation|arxiv=1406.1270|title=Transiting exoplanets from the CoRoT space mission|year=2014|doi=10.1051/0004-6361/201118662|last1=Alonso|first1=R.|last2=Moutou|first2=C.|last3=Endl|first3=M.|last4=Almenara|first4=J.-M.|last5=Guenther|first5=E. W.|last6=Deleuil|first6=M.|last7=Hatzes|first7=A.|last8=Aigrain|first8=S.|last9=Auvergne|first9=M.|last10=Baglin|first10=A.|last11=Barge|first11=P.|last12=Bonomo|first12=A. S.|last13=Bordé|first13=P.|last14=Bouchy|first14=F.|last15=Cavarroc|first15=C.|last16=Cabrera|first16=J.|last17=Carpano|first17=S.|last18=Csizmadia|first18=Sz.|last19=Cochran|first19=W. D.|last20=Deeg|first20=H. J.|last21=Díaz|first21=R. F.|last22=Dvorak|first22=R.|last23=Erikson|first23=A.|last24=Ferraz-Mello|first24=S.|last25=Fridlund|first25=M.|last26=Fruth|first26=T.|last27=Gandolfi|first27=D.|last28=Gillon|first28=M.|last29=Grziwa|first29=S.|last30=Guillot|first30=T.|journal=Astronomy & Astrophysics|volume=567|pages=A112|s2cid=96458405|display-authors=1}}

COROT-24c

|0.088

|0.44

|11.759

|0.098

|850

|style="background:#FFFF00"|transit

|2000

|0.91

|4950

|

COROT-27b

|10.39

|1.007

|3.57532

|0.0476

|1500

|style="background:#FFFF00"|transit

|3400{{±|200}}

|1.05

|5900

|{{citation|arxiv=1401.1122|year=2014|title=Transiting exoplanets from the CoRoT space mission|doi=10.1051/0004-6361/201323049|last1=Parviainen|first1=H.|last2=Gandolfi|first2=D.|last3=Deleuil|first3=M.|last4=Moutou|first4=C.|last5=Deeg|first5=H. J.|last6=Ferraz-Mello|first6=S.|last7=Samuel|first7=B.|last8=Csizmadia|first8=Sz.|last9=Pasternacki|first9=T.|last10=Wuchterl|first10=G.|last11=Havel|first11=M.|last12=Fridlund|first12=M.|last13=Angus|first13=R.|last14=Tingley|first14=B.|last15=Grziwa|first15=S.|last16=Korth|first16=J.|last17=Aigrain|first17=S.|last18=Almenara|first18=J. M.|last19=Alonso|first19=R.|last20=Baglin|first20=A.|last21=Barros|first21=S. C. C.|last22=Bordé|first22=P.|last23=Bouchy|first23=F.|last24=Cabrera|first24=J.|last25=Díaz|first25=R. F.|last26=Dvorak|first26=R.|last27=Erikson|first27=A.|last28=Guillot|first28=T.|last29=Hatzes|first29=A.|last30=Hébrard|first30=G.|journal=Astronomy & Astrophysics|volume=562|pages=A140|s2cid=46747735|display-authors=1}} Planet lost{{citation|arxiv=1812.01536|year=2018|title=Transit analysis of the CoRoT-5, CoRoT-8, CoRoT-12, CoRoT-18, CoRoT-20, and CoRoT-27 systems with combined ground- and space-based photometry|doi=10.1093/mnras/sty3085 |last1=Raetz |first1=St |last2=Heras |first2=A. M. |last3=Fernández |first3=M. |last4=Casanova |first4=V. |last5=Marka |first5=C. |journal=Monthly Notices of the Royal Astronomical Society |volume=483 |pages=824–839 |doi-access=free }}

Gliese 15 Ab

|0.017

|

|11.4433

|0.0717

|

|style="background:#00FF00"|radial vel.

|11.6

|0.38

|3567

|{{citation|arxiv=1408.5645|year=2014|title=The Nasa-Uc-Uh Eta-Earth Program. Iv. A Low-Mass Planet Orbiting an M Dwarf 3.6 Pc from Earth|doi=10.1088/0004-637X/794/1/51|last1=Howard|first1=Andrew W.|last2=Marcy|first2=Geoffrey W.|last3=Fischer|first3=Debra A.|last4=Isaacson|first4=Howard|last5=Muirhead|first5=Philip S.|last6=Henry|first6=Gregory W.|last7=Boyajian|first7=Tabetha S.|last8=von Braun|first8=Kaspar|last9=Becker|first9=Juliette C.|last10=Wright|first10=Jason T.|last11=Johnson|first11=John Asher|journal=The Astrophysical Journal|volume=794|issue=1 |page=51|bibcode=2014ApJ...794...51H |s2cid=17361592}}

Gliese 27.1 b

|0.0409

|

|15.819

|0.101

|

|style="background:#00FF00"|radial vel.

|77.05

|0.53

|3542

|Alternately known as Gliese 9018,{{citation|arxiv=1403.0430|year=2014|title=Bayesian search for low-mass planets around nearby M dwarfs – estimates for occurrence rate based on global detectability statistics|doi=10.1093/mnras/stu358|last1=Tuomi|first1=Mikko|last2=Jones|first2=Hugh R. A.|last3=Barnes|first3=John R.|last4=Anglada-Escudé|first4=Guillem|last5=Jenkins|first5=James S.|journal=Monthly Notices of the Royal Astronomical Society|volume=441|issue=2|pages=1545–1569|doi-access=free }} not related to Gliese 27.

Gliese 180 b

|0.0261

|

|17.380

|0.103

|

|style="background:#00FF00"|radial vel.

|38.95

|0.43

|3371

|

Gliese 433 c

|0.14

|

|4900{{±|1800|1000}}

|4.7{{±|1.2|0.8}}

|

|style="background:#00FF00"|radial vel.

|29.57

|0.48

|3472

|

Gliese 422 b

|0.0311

|

|26.161

|0.119

|

|style="background:#00FF00"|radial vel.

|41.32

|0.35

|3323

|

Gliese 687 b

|0.058

|

|38.14

|0.16353

|

|style="background:#00FF00"|radial vel.

|14.8

|0.41

|3413

|{{cite journal |arxiv=1405.2929 |title=The Lick–Carnegie exoplanet survey: Gliese 687 b: A Neptune-mass planet orbiting a nearby red dwarf|year=2014|doi=10.1088/0004-637X/789/2/114|last1=Burt|first1=Jennifer|last2=Vogt|first2=Steven S.|last3=Butler|first3=R. Paul|last4=Hanson|first4=Russell|last5=Meschiari|first5=Stefano|last6=Rivera|first6=Eugenio J.|last7=Henry|first7=Gregory W.|last8=Laughlin|first8=Gregory|journal=The Astrophysical Journal|volume=789|issue=2|page=114|bibcode=2014ApJ...789..114B|s2cid=17668957}}

Gliese 3293 b

|0.07406

|

|30.5987

|0.14339

|

|style="background:#00FF00"|radial vel.

|51.4

|0.42

|3466

|

Gliese 3293 c

|0.06636

|

|122.6196

|0.36175

|

|style="background:#00FF00"|radial vel.

|51.4

|0.42

|3466

|

Gliese 3341 b

|0.0208

|

|14.207

|0.089

|

|style="background:#00FF00"|radial vel.

|77.1

|0.47

|3526

|{{cite journal

| doi=10.1051/0004-6361/201424253

| bibcode=2015A&A...575A.119A

| title=Planetary systems and stellar activity of the M dwarfs GJ 3293, GJ 3341, and GJ 3543

| journal=Astronomy & Astrophysics

| volume=575

| pages=A119

| arxiv=1411.7048v1

| last1=Astudillo-Defru | first1=Nicola

| last2=Bonfils | first2=Xavier

| last3=Delfosse | first3=Xavier

| last4=Ségransan | first4=Damien

| last5=Forveille | first5=Thierry

| last6=Bouchy | first6=François

| last7=Gillon | first7=Michaël

| last8=Lovis | first8=Christophe

| last9=Mayor | first9=Michel

| last10=Neves | first10=Vasco

| last11=Pepe | first11=Francesco

| last12=Perrier | first12=Christian

| last13=Queloz | first13=Didier

| last14=Rojo | first14=Patricio

| last15=Santos | first15=Nuno C.

| last16=Udry | first16=Stéphane

| year=2015

| s2cid=67754095

}}

GU Piscium b

|11.3

|1.265

|

|2000

|

|style="background:#FF6CDA"|imaging

|160

|0.33

|3250{{±|32}}

|{{cite journal |title= Discovery of a Wide Planetary-mass Companion to the Young M3 Star GU Psc |author1=Marie-Eve Naud |author2=Étienne Artigau |author3=Lison Malo |author4=Loïc Albert |author5=René Doyon |author6=David Lafrenière |author7=Jonathan Gagné |author8=Didier Saumon |author9=Caroline V. Morley |author10=France Allard |author11=Derek Homeier |author12=Charles A. Beichman |author13=Christopher R. Gelino |author14=Anne Boucher |date= 12 May 2014 |doi= 10.1088/0004-637X/787/1/5|arxiv= 1405.2932|bibcode= 2014ApJ...787....5N |journal= The Astrophysical Journal |volume= 787 |issue= 1 |id= 5 |page= 16 |s2cid=35264096 |publication-date= May 2014}}

HAT-P-49b

|1.73

|1.413

|2.691548

|0.0438

|2131

|style="background:#FFFF00"|transit

|1050

|1.54

|6820

|{{citation|arxiv=1401.5460|year=2014|title=HAT-P-49b: A 1.7MJPLANET TRANSITING a BRIGHT 1.5M☉F-STAR|doi=10.1088/0004-6256/147/4/84|last1=Bieryla|first1=A.|last2=Hartman|first2=J. D.|last3=Bakos|first3=G. Á.|last4=Bhatti|first4=W.|last5=Kovács|first5=G.|last6=Boisse|first6=I.|last7=Latham|first7=D. W.|last8=Buchhave|first8=L. A.|last9=Csubry|first9=Z.|last10=Penev|first10=K.|last11=De Val-Borro|first11=M.|last12=Béky|first12=B.|last13=Falco|first13=E.|last14=Torres|first14=G.|last15=Noyes|first15=R. W.|last16=Berlind|first16=P.|last17=Calkins|first17=M. C.|last18=Esquerdo|first18=G. A.|last19=Lázár|first19=J.|last20=Papp|first20=I.|last21=Sári|first21=P.|journal=The Astronomical Journal|volume=147|issue=4|page=84|bibcode=2014AJ....147...84B |s2cid=119265999}}

HAT-P-54b

|0.76

|0.944

|3.799847

|0.04117

|

|style="background:#FFFF00"|transit

|443

|0.65

|4390

|{{citation|arxiv=1404.4417|year=2014|title=HAT-P-54b: A HOT JUPITER TRANSITING a 0.64M⊙STAR IN FIELD 0 OF THE K2 MISSION|doi=10.1088/0004-6256/149/4/149 |last1=Bakos |first1=G. Á. |last2=Hartman |first2=J. D. |last3=Bhatti |first3=W. |last4=Bieryla |first4=A. |last5=Val-Borro |first5=M. de |last6=Latham |first6=D. W. |last7=Buchhave |first7=L. A. |last8=Csubry |first8=Z. |last9=Penev |first9=K. |last10=Kovács |first10=G. |last11=Béky |first11=B. |last12=Falco |first12=E. |last13=Kovács |first13=T. |last14=Howard |first14=A. W. |last15=Johnson |first15=J. A. |last16=Isaacson |first16=H. |last17=Marcy |first17=G. W. |last18=Torres |first18=G. |last19=Noyes |first19=R. W. |last20=Berlind |first20=P. |last21=Calkins |first21=M. L. |last22=Esquerdo |first22=G. A. |last23=Lázár |first23=J. |last24=Papp |first24=I. |last25=Sári |first25=P. |journal=The Astronomical Journal |volume=149 |issue=4 |page=149 |s2cid=119239193 }} Disputed in 2016,{{citation|arxiv=1607.05263|year=2021|title=197 CANDIDATES AND 104 VALIDATED PLANETS IN K2 's FIRST FIVE FIELDS|doi=10.3847/0067-0049/226/1/7 |last1=Crossfield |first1=Ian J. M. |last2=Ciardi |first2=David R. |last3=Petigura |first3=Erik A. |last4=Sinukoff |first4=Evan |last5=Schlieder |first5=Joshua E. |last6=Howard |first6=Andrew W. |last7=Beichman |first7=Charles A. |last8=Isaacson |first8=Howard |last9=Dressing |first9=Courtney D. |last10=Christiansen |first10=Jessie L. |last11=Fulton |first11=Benjamin J. |last12=Lépine |first12=Sébastien |last13=Weiss |first13=Lauren |last14=Hirsch |first14=Lea |last15=Livingston |first15=John |last16=Baranec |first16=Christoph |last17=Law |first17=Nicholas M. |last18=Riddle |first18=Reed |last19=Ziegler |first19=Carl |last20=Howell |first20=Steve B. |last21=Horch |first21=Elliott |last22=Everett |first22=Mark |last23=Teske |first23=Johanna |last24=Martinez |first24=Arturo O. |last25=Obermeier |first25=Christian |last26=Benneke |first26=Björn |last27=Scott |first27=Nic |last28=Deacon |first28=Niall |last29=Aller |first29=Kimberly M. |last30=Hansen |first30=Brad M. S. |journal=The Astrophysical Journal Supplement Series |volume=226 |page=7 |s2cid=56125109 |display-authors=1 |doi-access=free }} reconfirmed in 2021.{{citation|arxiv=2105.09668|year=2021|title=Multiband Transit Follow-up Observations of Five Hot Jupiters with Critical Noise Treatments: Improved Physical Properties|doi=10.3847/1538-3881/ac01dd |last1=Saha |first1=Suman |last2=Chakrabarty |first2=Aritra |last3=Sengupta |first3=Sujan |journal=The Astronomical Journal |volume=162 |issue=1 |page=18 |bibcode=2021AJ....162...18S |s2cid=234790451 |doi-access=free }}

HATS-4b

|1.323

|1.02

|2.516729

|0.0362

|1315

|style="background:#FFFF00"|transit

|1400

|1

|5403

|{{citation|arxiv=1402.6546|year=2014|title=HATS-4b: A DENSE HOT JUPITER TRANSITING a SUPER METAL-RICH G STAR|doi=10.1088/0004-6256/148/2/29|last1=Jordán|first1=Andrés|last2=Brahm|first2=Rafael|last3=Bakos|first3=G. Á.|last4=Bayliss|first4=D.|last5=Penev|first5=K.|last6=Hartman|first6=J. D.|last7=Zhou|first7=G.|last8=Mancini|first8=L.|last9=Mohler-Fischer|first9=M.|last10=Ciceri|first10=S.|last11=Sato|first11=B.|last12=Csubry|first12=Z.|last13=Rabus|first13=M.|last14=Suc|first14=V.|last15=Espinoza|first15=N.|last16=Bhatti|first16=W.|last17=De Val Borro|first17=M.|last18=Buchhave|first18=L.|last19=Csák|first19=B.|last20=Henning|first20=T.|last21=Schmidt|first21=B.|last22=Tan|first22=T. G.|last23=Noyes|first23=R. W.|last24=Béky|first24=B.|last25=Butler|first25=R. P.|last26=Shectman|first26=S.|last27=Crane|first27=J.|last28=Thompson|first28=I.|last29=Williams|first29=A.|last30=Martin|first30=R.|journal=The Astronomical Journal|volume=148|issue=2|page=29|bibcode=2014AJ....148...29J |s2cid=119189535|display-authors=1}}

HATS-5b

|0.237

|0.912

|4.763387

|0.0542

|1025

|style="background:#FFFF00"|transit

|840

|0.94

|5304

|{{citation|arxiv=1401.1582|year=2014|title=HATS-5b: A TRANSITING HOT SATURN FROM THE HATSouth SURVEY|doi=10.1088/0004-6256/147/6/144|last1=Zhou|first1=G.|last2=Bayliss|first2=D.|last3=Penev|first3=K.|last4=Bakos|first4=G. Á.|last5=Hartman|first5=J. D.|last6=Jordán|first6=A.|last7=Mancini|first7=L.|last8=Mohler|first8=M.|last9=Csubry|first9=Z.|last10=Ciceri|first10=S.|last11=Brahm|first11=R.|last12=Rabus|first12=M.|last13=Buchhave|first13=L.|last14=Henning|first14=T.|last15=Suc|first15=V.|last16=Espinoza|first16=N.|last17=Béky|first17=B.|last18=Noyes|first18=R. W.|last19=Schmidt|first19=B.|last20=Butler|first20=R. P.|last21=Shectman|first21=S.|last22=Thompson|first22=I.|last23=Crane|first23=J.|last24=Sato|first24=B.|last25=Csák|first25=B.|last26=Lázár|first26=J.|last27=Papp|first27=I.|last28=Sári|first28=P.|last29=Nikolov|first29=N.|journal=The Astronomical Journal|volume=147|issue=6|page=144|bibcode=2014AJ....147..144Z |s2cid=118654298}}

HATS-6b

|0.319

|0.998

|3.3252725

|0.03623

|

|style="background:#FFFF00"|transit

|484

|0.57

|3724

|{{citation|arxiv=1408.1758|year=2014|title=HATS-6b: A WARM SATURN TRANSITING AN EARLY M DWARF STAR, AND a SET OF EMPIRICAL RELATIONS FOR CHARACTERIZING K AND M DWARF PLANET HOSTS|doi=10.1088/0004-6256/149/5/166 |last1=Hartman |first1=J. D. |last2=Bayliss |first2=D. |last3=Brahm |first3=R. |last4=Bakos |first4=G. Á. |last5=Mancini |first5=L. |last6=Jordán |first6=A. |last7=Penev |first7=K. |last8=Rabus |first8=M. |last9=Zhou |first9=G. |last10=Butler |first10=R. P. |last11=Espinoza |first11=N. |last12=De Val-Borro |first12=M. |last13=Bhatti |first13=W. |last14=Csubry |first14=Z. |last15=Ciceri |first15=S. |last16=Henning |first16=T. |last17=Schmidt |first17=B. |last18=Arriagada |first18=P. |last19=Shectman |first19=S. |last20=Crane |first20=J. |last21=Thompson |first21=I. |last22=Suc |first22=V. |last23=Csák |first23=B. |last24=Tan |first24=T. G. |last25=Noyes |first25=R. W. |last26=Lázár |first26=J. |last27=Papp |first27=I. |last28=Sári |first28=P. |journal=The Astronomical Journal |volume=149 |issue=5 |page=166 |s2cid=119286461 }}

HD 564 b

|0.33

|

|492.3

|1.2

|

|style="background:#00FF00"|radial vel.

|175

|0.96

|5902

|

HD 4203 c

|2.17

|

|6700

|6.95

|

|style="background:#00FF00"|radial vel.

|253.8

|1.13

|5702

|{{cite journal | title=Limits on Stellar Companions to Exoplanet Host Stars with Eccentric Planets | display-authors=1 | last1=Kane | first1=Stephen R. | last2=Howell | first2=Steve B. | last3=Horch | first3=Elliott P. | last4=Feng | first4=Ying | last5=Hinkel | first5=Natalie R. | last6=Ciardi | first6=David R. | last7=Everett | first7=Mark E. | last8=Howard | first8=Andrew W. | last9=Wright | first9=Jason T. | journal=The Astrophysical Journal | volume=785 | issue=2 | id=93 | pages=10 | date=April 2014 | doi=10.1088/0004-637X/785/2/93 | arxiv=1401.1544 | bibcode=2014ApJ...785...93K | s2cid=2053475 }}

HD 5319 c

|1.15

|

|886

|2.071

|

|style="background:#00FF00"|radial vel.

|370

|1.51

|4958

|{{cite journal | title=Newly Discovered Planets Orbiting HD 5319, HD 11506, HD 75784 and HD 10442 from the N2K Consortium | last1=Giguere | first1=Matthew J. | last2=Fischer | first2=Debra A. | last3=Payne | first3=Matthew J. | last4=Brewer | first4=John M. | last5=Johnson | first5=John Asher | last6=Howard | first6=Andrew W. | last7=Isaacson | first7=Howard T. | display-authors=1 | journal=The Astrophysical Journal | volume=799 | issue=1 | at=89 | year=2015 | arxiv=1411.5374 | bibcode=2015ApJ...799...89G | doi=10.1088/0004-637X/799/1/89 | s2cid=56121568 }}

HD 10442 b

|2.1

|

|1043

|2.335

|

|style="background:#00FF00"|radial vel.

|443{{±|4}}

|1.56

|5034

|

HD 11506 c

|0.408±0.057

|

|223.41{{±|0.32}}

|0.774{{±|0.038}}

|

|style="background:#00FF00"|radial vel.

|167.4{{±|0.4}}

|1.12{{±|0.02}}

|5833{{±|28}}

|

HD 14067 b

|7.8

|

|1455

|3.4

|

|style="background:#00FF00"|radial vel.

|533

|2.4

|4815

|{{citation|arxiv=1409.6081|year=2014|title=A long-period eccentric substellar companion to the evolved intermediate-mass star HD 14067|doi=10.1093/pasj/psu113|last1=Wang|first1=Liang|last2=Sato|first2=Bun'ei|last3=Omiya|first3=Masashi|last4=Harakawa|first4=Hiroki|last5=Liu|first5=Yujuan|last6=Song|first6=Nan|last7=He|first7=Wei|last8=Wu|first8=Xiaoshu|last9=Izumiura|first9=Hideyuki|last10=Kambe|first10=Eiji|last11=Takeda|first11=Yoichi|last12=Yoshida|first12=Michitoshi|last13=Itoh|first13=Yoichi|last14=Ando|first14=Hiroyasu|last15=Kokubo|first15=Eiichiro|last16=Ida|first16=Shigeru|last17=Zhao|first17=Gang|journal=Publications of the Astronomical Society of Japan|volume=66|issue=6|page=118}}

HD 30669 b

|0.47

|

|1684

|2.69

|

|style="background:#00FF00"|radial vel.

|186

|0.92

|5400

|

HD 75784 b

|1.15

|

|341.7

|1.073

|

|style="background:#00FF00"|radial vel.

|224

|1.41

|4917

|

HD 100546 b

|

|3.4

|

|53

|

|style="background:#FF6CDA"|imaging

|320

|2.4

|10500

|{{cite journal|bibcode=2017PhDT.......406S |date=2017 |title=Observation of extrasolar planets at various ages |last1=Sissa |journal=PhD Thesis, University of Padua, 2017}}

HD 103720 b

|0.62

|

|4.5557

|0.0498

|

|style="background:#00FF00"|radial vel.

|136

|0.79

|5017

|

HD 108341 b

|3.5

|

|1129

|2

|

|style="background:#00FF00"|radial vel.

|161

|0.84

|5122

|

HD 114613 b

|0.48

|

|3827

|5.16

|

|style="background:#00FF00"|radial vel.

|66.8

|1.36

|5729

|{{cite journal | title=The Anglo-Australian Planet Search. XXIII. Two New Jupiter Analogs | last1=Wittenmyer | first1=Robert A. | last2=Horner | first2=Jonathan | last3=Tinney | first3=C.G. | last4=Butler | first4=R. P. | last5=Jones | first5=H.R.A. | last6=Tuomi | first6=Mikko | last7=Salter | first7=G.S. | last8=Carter | first8=B.D. | last9=Koch | first9=F. Elliot | last10=O'Toole | first10=S.J. | last11=Bailey | first11=J. | last12=Wright | first12= D. | display-authors=1 | journal=The Astrophysical Journal | date=2014 | arxiv=1401.5525 |bibcode = 2014ApJ...783..103W |doi = 10.1088/0004-637X/783/2/103 | volume=783 | issue=2 | pages=103| s2cid=14082923 }}

HD 141399 b

|0.451

|

|94.44

|0.415

|

|style="background:#00FF00"|radial vel.

|118

|1.07

|5600

|{{citation|arxiv=1404.7462|title=A Four-Planet System Orbiting the K0V Star Hd 141399|year=2014|doi=10.1088/0004-637X/787/2/97|last1=Vogt|first1=Steven S.|last2=Butler|first2=R. Paul|last3=Rivera|first3=Eugenio J.|last4=Kibrick|first4=Robert|last5=Burt|first5=Jennifer|last6=Hanson|first6=Russell|last7=Meschiari|first7=Stefano|last8=Henry|first8=Gregory W.|last9=Laughlin|first9=Gregory|journal=The Astrophysical Journal|volume=787|issue=2|page=97|bibcode=2014ApJ...787...97V |s2cid=10477331}}

HD 141399 c

|1.33

|

|201.99

|0.689

|

|style="background:#00FF00"|radial vel.

|118

|1.07

|5600

|

HD 141399 d

|1.18

|

|1069.8

|2.09

|

|style="background:#00FF00"|radial vel.

|118

|1.07

|5600

|

HD 141399 e

|0.66

|

|5000

|5

|

|style="background:#00FF00"|radial vel.

|118

|1.07

|5600

|

HD 154857 c

|2.58

|

|3452

|5.36

|

|style="background:#00FF00"|radial vel.

|223.5

|1.72

|5605

|

HIP 67851 b

|1.38

|

|88.9

|0.46

|

|style="background:#00FF00"|radial vel.

|208.3{{±|0.6}}

|1.63

|4890

|{{citation|arxiv=1409.7429|year=2015|title=A planetary system and a highly eccentric brown dwarf around the giant stars HIP 67851 and HIP 97233|doi=10.1051/0004-6361/201424771|last1=Jones|first1=M. I.|last2=Jenkins|first2=J. S.|last3=Rojo|first3=P.|last4=Melo|first4=C. H. F.|last5=Bluhm|first5=P.|journal=Astronomy & Astrophysics|volume=573|pages=A3|bibcode=2015A&A...573A...3J |s2cid=53638707}}

HIP 67851 c

|4.34{{±|0.59}}

|

|1741{{±|39}}

|3.09{{±|0.18}}

|

|style="background:#00FF00"|radial vel.

|208.3{{±|0.6}}

|1.63

|4890

|{{citation|arxiv=1412.6889|year=2014|title=The Pan-Pacific Planet Search. Ii. Confirmation of a Two-Planet System Around Hd 121056|doi=10.1088/0004-637X/800/1/74|last1=Wittenmyer|first1=Robert A.|last2=Wang|first2=Liang|last3=Liu|first3=Fan|last4=Horner|first4=Jonathan|last5=Endl|first5=Michael|last6=Johnson|first6=John Asher|last7=Tinney|first7=C. G.|last8=Carter|first8=B. D.|journal=The Astrophysical Journal|volume=800|page=74|s2cid=53684180}}

HIP 97233 b

|20

|

|1058.8

|2.55

|

|style="background:#00FF00"|radial vel.

|347

|1.93

|5020

|

HIP 105854 b

|8.2

|

|184.2

|0.81

|

|style="background:#00FF00"|radial vel.

|276

|2.1

|4780

|{{citation|arxiv=1406.0884|year=2014|title=The properties of planets around giant stars|doi=10.1051/0004-6361/201323345|last1=Jones|first1=M. I.|last2=Jenkins|first2=J. S.|last3=Bluhm|first3=P.|last4=Rojo|first4=P.|last5=Melo|first5=C. H. F.|journal=Astronomy & Astrophysics|volume=566|pages=A113|bibcode=2014A&A...566A.113J |s2cid=118396750}}

HIP 116454 b

|0.037

|0.226

|9.1205

|0.0906

|

|style="background:#00FF00"|radial vel.

|180

|0.78

|5089

|{{cite journal | title=Characterizing K2 Planet Discoveries: A super-Earth transiting the bright K-dwarf HIP 116454 | first1=Andrew | last1=Vanderburg | first2=Benjamin T. | last2=Montet | first3=John Asher | last3=Johnson | first4=Lars A. | last4=Buchhave | first5=Li | last5=Zeng | first6=Francesco | last6=Pepe | first7=Andrew Collier | last7=Cameron | first8=David W. | last8=Latham | first9=Emilio | last9=Molinari | first10=Stephane | last10=Udry | first11=Christophe | last11=Lovis | first12=Jaymie M. | last12=Matthews | first13=Chris | last13=Cameron | first14=Nicholas | last14=Law | first15=Brendan P. | last15=Bowler | first16=Ruth | last16=Angus | first17=Christoph | last17=Baranec | first18=Allyson | last18=Bieryla | first19=Walter | last19=Boschin | first20=David | last20=Charbonneau | first21=Rosario | last21=Cosentino | first22=Xavier | last22=Dumusque | first23=Pedro | last23=Figueira | first24=David B. | last24=Guenther | first25=Avet | last25=Harutyunyan | first26=Coel | last26=Hellier | first27=Rainer | last27=Kuschnig | first28=Mercedes | last28=Lopez-Morales | first29=Michel | last29=Mayor | first30=Giusi | last30=Micela | first31=Anthony F. J. | last31=Moffat | first32=Marco | last32=Pedani | first33=David F. | last33=Phillips | first34=Giampaolo | last34=Piotto | first35=Don | last35=Pollacco | first36=Didier | last36=Queloz | first37=Ken | last37=Rice | first38=Reed | last38=Riddle | first39=Jason F. | last39=Rowe | first40=Slavek M. | last40=Rucinski | first41=Dimitar | last41=Sasselov | first42=Damien | last42=Segransan | first43=Alessandro | last43=Sozzetti | first44=Andrew | last44=Szentgyorgyi | first45=Chris | last45=Watson | first46=Werner W. | last46=Weiss | display-authors=1 | journal=The Astrophysical Journal | volume=800 | issue=1 | at=59 | date=February 2015 | arxiv=1412.5674 | bibcode=2015ApJ...800...59V | doi=10.1088/0004-637X/800/1/59 | doi-access=free }}

Kapteyn b

|0.015

|

|48.616{{±|0.036|0.032}}

|0.168

|

|style="background:#00FF00"|radial vel.

|12.8

|0.28

|3550

|Existence of planet been disputed.

Kapteyn c

|0.022

|

|121.54

|0.311

|

|style="background:#00FF00"|radial vel.

|12.8

|0.28

|3550

|Existence of planet been disputed.{{citation|arxiv=1406.0818|title=Two planets around Kapteyn's star : a cold and a temperate super-Earth orbiting the nearest halo red-dwarf |journal=Monthly Notices of the Royal Astronomical Society: Letters |volume=443 |pages=L89–L93 | display-authors=1|first1=Guillem|last1=Anglada-Escudé|first2= Pamela|last2=Arriagada|first3= Mikko|last3=Tuomi|first4= Mathias|last4=Zechmeister|year=2014|bibcode = 2014MNRAS.443L..89A |doi = 10.1093/mnrasl/slu076 |doi-access=free |s2cid=67807856 }}{{citation|arxiv=2103.02709|title=A Gaussian Process Regression Reveals No Evidence for Planets Orbiting Kapteyn's Star|year=2021|doi=10.3847/1538-3881/abec89|last1=Bortle|first1=Anna|last2=Fausey|first2=Hallie|last3=Ji|first3=Jinbiao|last4=Dodson-Robinson|first4=Sarah|last5=Ramirez Delgado|first5=Victor|last6=Gizis|first6=John|journal=The Astronomical Journal|volume=161|issue=5|page=230|bibcode=2021AJ....161..230B |s2cid=232110395 |doi-access=free }}

Kepler-23d

|

|0.196

|15.274299

|0.124

|

|style="background:#FFFF00"|transit

|2600

|1.11

|5828

|

Kepler-24d

|

|0.149

|4.244384

|0.051

|

|style="background:#FFFF00"|transit

|3900

|1.03

|5897

|

Kepler-24e

|

|0.248

|18.998355

|0.138

|

|style="background:#FFFF00"|transit

|3900

|1.03

|5897

|

Kepler-25d

|0.283

|

|123

|

|

|style="background:#00FF00"|radial vel.

|798{{±|4}}

|1.19

|6270

|

Kepler-26d

|

|0.095

|3.543919

|0.039

|

|style="background:#FFFF00"|transit

|1104{{±|10}}

|0.54

|3914

|

Kepler-26e

|

|0.215

|46.827915

|0.22

|

|style="background:#FFFF00"|transit

|1104{{±|10}}

|0.54

|3914

|

Kepler-31d

|6.8

|0.348

|87.6451

|0.4

|

|style="background:#FFFF00"|transit

|6800

|1.21

|6340

|

Kepler-37e

|

|

|51.196

|

|

|style="background:#FF7519"|timing

|220

|0.8

|5417

|

Kepler-48d

|0.025

|0.182

|42.8961

|

|

|style="background:#FFFF00"|transit

|1009{{±|5}}

|0.88

|5194

|

Kepler-48e

|2.067

|

|982

|

|

|style="background:#00FF00"|radial vel.

|1009{{±|5}}

|0.88

|5194

|

Kepler-49d

|

|0.143

|2.576549

|0.031

|

|style="background:#FFFF00"|transit

|1024{{±|8}}

|0.55

|4252

|

Kepler-49e

|

|0.139

|18.596108

|0.116

|

|style="background:#FFFF00"|transit

|1024{{±|8}}

|0.55

|4252

|

Kepler-51d

|0.024

|0.865

|130.194

|0.509

|

|style="background:#FFFF00"|transit

|2610{{±|50}}

|1.04

|6018

|

Kepler-52d

|

|0.174

|36.445171

|0.182

|

|style="background:#FFFF00"|transit

|1058{{±|7}}

|0.54

|4263

|

Kepler-53d

|

|0.189

|9.751962

|0.091

|

|style="background:#FFFF00"|transit

|4600{{±|200}}

|0.98

|5858

|

Kepler-54d

|

|0.136

|20.995694

|0.126

|

|style="background:#FFFF00"|transit

|893{{±|9}}

|0.51

|4252

|

Kepler-55d

|

|0.142

|2.211099

|0.029

|

|style="background:#FFFF00"|transit

|1920{{±|30}}

|0.62

|4503

|

Kepler-55e

|

|0.138

|4.617534

|0.048

|

|style="background:#FFFF00"|transit

|1920{{±|30}}

|0.62

|4503

|

Kepler-55f

|

|0.142

|10.198545

|0.081

|

|style="background:#FFFF00"|transit

|1920{{±|30}}

|0.62

|4503

|

Kepler-58d

|

|0.262

|40.101371

|0.236

|

|style="background:#FFFF00"|transit

|3250{{±|80}}

|0.95

|6099

|

Kepler-79d

|0.019

|0.639

|52.0902

|0.287

|553

|style="background:#FFFF00"|transit

|3230{{±|60}}

|1.17

|6174

|

Kepler-79e

|0.013

|0.311

|81.0659

|0.386

|477

|style="background:#FFFF00"|transit

|3230{{±|60}}

|1.17

|6174

|

Kepler-80d

|0.02124

|0.136

|3.07222

|0.0372

|

|style="background:#FFFF00"|transit

|1160

|0.73

|4540

|

Kepler-80e

|0.01299

|0.143

|4.64489

|0.0491

|

|style="background:#FFFF00"|transit

|1160

|0.73

|4540

|

Kepler-81d

|

|0.108

|20.837846

|0.128

|

|style="background:#FFFF00"|transit

|1147{{±|10}}

|0.64

|4500

|

Kepler-82d

|

|0.158

|2.382961

|0.034

|

|style="background:#FFFF00"|transit

|3030{{±|80}}

|0.85

|5428

|

Kepler-82e

|

|0.22

|5.902206

|0.063

|

|style="background:#FFFF00"|transit

|3030{{±|80}}

|0.85

|5428

|

Kepler-83d

|

|0.173

|5.169796

|0.051

|

|style="background:#FFFF00"|transit

|1320{{±|17}}

|0.66

|4648

|

Kepler-84d

|

|0.123

|4.224537

|0.052

|

|style="background:#FFFF00"|transit

|4700{{±|500}}

|1

|6031

|

Kepler-84e

|

|0.232

|27.434389

|0.181

|

|style="background:#FFFF00"|transit

|4700{{±|500}}

|1

|6031

|

Kepler-84f

|

|0.196

|44.552169

|0.25

|

|style="background:#FFFF00"|transit

|4700{{±|500}}

|1

|6031

|{{citation|arxiv=1402.6534|year=2014|title=Validation Ofkepler's Multiple Planet Candidates. III. Light Curve Analysis and Announcement of Hundreds of New Multi-Planet Systems|doi=10.1088/0004-637X/784/1/45|last1=Rowe|first1=Jason F.|last2=Bryson|first2=Stephen T.|last3=Marcy|first3=Geoffrey W.|last4=Lissauer|first4=Jack J.|last5=Jontof-Hutter|first5=Daniel|last6=Mullally|first6=Fergal|last7=Gilliland|first7=Ronald L.|last8=Issacson|first8=Howard|last9=Ford|first9=Eric|last10=Howell|first10=Steve B.|last11=Borucki|first11=William J.|last12=Haas|first12=Michael|last13=Huber|first13=Daniel|last14=Steffen|first14=Jason H.|last15=Thompson|first15=Susan E.|last16=Quintana|first16=Elisa|last17=Barclay|first17=Thomas|last18=Still|first18=Martin|last19=Fortney|first19=Jonathan|last20=Gautier|first20=T. N.|last21=Hunter|first21=Roger|last22=Caldwell|first22=Douglas A.|last23=Ciardi|first23=David R.|last24=Devore|first24=Edna|last25=Cochran|first25=William|last26=Jenkins|first26=Jon|last27=Agol|first27=Eric|last28=Carter|first28=Joshua A.|last29=Geary|first29=John|journal=The Astrophysical Journal|volume=784|issue=1 |page=45|bibcode=2014ApJ...784...45R |s2cid=119118620}}

Kepler-85d

|

|0.107

|17.91323

|0.13

|

|style="background:#FFFF00"|transit

|2550{{±|50}}

|0.92

|5436

|

Kepler-85e

|

|0.113

|25.216751

|0.163

|

|style="background:#FFFF00"|transit

|2550{{±|50}}

|0.92

|5436

|

Kepler-93b

|0.01265

|0.132

|4.72673978

|0.053

|1037

|style="background:#FFFF00"|transit

|313.7{{±|0.7}}

|0.91

|5669

|

Kepler-93c

|3

|

|1460

|

|

|style="background:#00FF00"|radial vel.

|313.7{{±|0.7}}

|0.91

|5669

|

Kepler-94b

|0.034

|0.313

|2.50806

|

|

|style="background:#FFFF00"|transit

|629{{±|2}}

|0.81

|4781

|

Kepler-94c

|9.836

|

|820.3

|

|

|style="background:#00FF00"|radial vel.

|629{{±|2}}

|0.81

|4781

|

Kepler-95b

|0.041

|0.305

|11.5231

|

|

|style="background:#FFFF00"|transit

|1472{{±|18}}

|1.08

|5699

|

Kepler-96b

|0.027

|0.238

|16.2385

|

|

|style="background:#FFFF00"|transit

|402.2{{±|1.3}}

|1

|5690

|

Kepler-97b

|0.011

|0.132

|2.58664

|

|

|style="background:#FFFF00"|transit

|1322{{±|11}}

|0.94

|5779

|

Kepler-97c

|1.08

|

|789

|

|

|style="background:#00FF00"|radial vel.

|1322{{±|11}}

|0.94

|5779

|

Kepler-98b

|0.011

|0.178

|1.54168

|

|

|style="background:#FFFF00"|transit

|1154{{±|9}}

|0.99

|5539

|

Kepler-99b

|0.019

|0.132

|4.60358

|

|

|style="background:#FFFF00"|transit

|683{{±|3}}

|0.79

|4782

|

Kepler-100b

|0.023

|0.118

|6.88705

|

|

|style="background:#FFFF00"|transit

|1002{{±|5}}

|1.08

|5825

|{{citation|arxiv=1401.4195|title=Masses, Radii, and Orbits of Small Kepler Planets: The Transition from Gaseous to Rocky Planets|year=2014|doi=10.1088/0067-0049/210/2/20|last1=Marcy|first1=Geoffrey W.|last2=Isaacson|first2=Howard|last3=Howard|first3=Andrew W.|last4=Rowe|first4=Jason F.|last5=Jenkins|first5=Jon M.|last6=Bryson|first6=Stephen T.|last7=Latham|first7=David W.|last8=Howell|first8=Steve B.|last9=Gautier|first9=Thomas N.|last10=Batalha|first10=Natalie M.|last11=Rogers|first11=Leslie|last12=Ciardi|first12=David|last13=Fischer|first13=Debra A.|last14=Gilliland|first14=Ronald L.|last15=Kjeldsen|first15=Hans|last16=Christensen-Dalsgaard|first16=Jørgen|last17=Huber|first17=Daniel|last18=Chaplin|first18=William J.|last19=Basu|first19=Sarbani|last20=Buchhave|first20=Lars A.|last21=Quinn|first21=Samuel N.|last22=Borucki|first22=William J.|last23=Koch|first23=David G.|last24=Hunter|first24=Roger|last25=Caldwell|first25=Douglas A.|last26=Van Cleve|first26=Jeffrey|last27=Kolbl|first27=Rea|last28=Weiss|first28=Lauren M.|last29=Petigura|first29=Erik|last30=Seager|first30=Sara|journal=The Astrophysical Journal Supplement Series|volume=210|issue=2|page=20|bibcode=2014ApJS..210...20M |s2cid=10760418|display-authors=1}}

Kepler-100c

|

|0.196

|12.8159

|

|

|style="background:#FFFF00"|transit

|1002{{±|5}}

|1.08

|5825

|

Kepler-100d

|

|0.144

|35.3331

|

|

|style="background:#FFFF00"|transit

|1002{{±|5}}

|1.08

|5825

|

Kepler-101b

|0.16

|0.51

|3.4876812

|0.0474

|

|style="background:#FFFF00"|transit

|3110{{±|50}}

|1.17

|5667

|

Kepler-101c

|0.01

|0.112

|6.02976

|0.0684

|

|style="background:#FFFF00"|transit

|3110{{±|50}}

|1.17

|5667

|

Kepler-102b

|

|0.042

|5.28696

|

|792

|style="background:#FFFF00"|transit

|352.7{{±|0.7}}

|0.81

|4909

|

Kepler-102c

|

|0.052

|7.07142

|

|718

|style="background:#FFFF00"|transit

|352.7{{±|0.7}}

|0.81

|4909

|

Kepler-102d

|0.012

|0.105

|10.3117

|

|

|style="background:#FFFF00"|transit

|352.7{{±|0.7}}

|0.81

|4909

|

Kepler-102f

|

|0.079

|27.4536

|

|457

|style="background:#FFFF00"|transit

|352.7{{±|0.7}}

|0.81

|4909

|

Kepler-103b

|0.031

|0.301

|15.9654

|

|

|style="background:#FFFF00"|transit

|1637{{±|19}}

|1.09

|5845

|

Kepler-103c

|0.114

|0.459

|179.612

|

|

|style="background:#FFFF00"|transit

|1637{{±|19}}

|1.09

|5845

|

Kepler-104b

|

|0.277

|11.427548

|0.094

|

|style="background:#FFFF00"|transit

|1322{{±|14}}

|0.81

|5711

|

Kepler-104c

|

|0.279

|23.668205

|0.153

|

|style="background:#FFFF00"|transit

|1322{{±|14}}

|0.81

|5711

|

Kepler-104d

|

|0.319

|51.755394

|0.257

|

|style="background:#FFFF00"|transit

|1322{{±|14}}

|0.81

|5711

|

Kepler-105c

|0.01447

|0.117

|7.1262

|

|

|style="background:#FFFF00"|transit

|1517{{±|18}}

|0.96

|5827

|

Kepler-106b

|

|0.073

|6.16486

|

|

|style="background:#FFFF00"|transit

|1470{{±|20}}

|1

|5858

|

Kepler-106c

|0.033

|0.223

|13.5708

|

|

|style="background:#FFFF00"|transit

|1470{{±|20}}

|1

|5858

|

Kepler-106d

|

|0.085

|23.9802

|

|

|style="background:#FFFF00"|transit

|1470{{±|20}}

|1

|5858

|

Kepler-106e

|0.035

|0.228

|43.8445

|

|

|style="background:#FFFF00"|transit

|1470{{±|20}}

|1

|5858

|

Kepler-107b

|

|0.139

|3.179997

|0.044

|

|style="background:#FFFF00"|transit

|1741{{±|18}}

|

|5851

|

Kepler-107c

|

|0.161

|4.901425

|0.059

|

|style="background:#FFFF00"|transit

|1741{{±|18}}

|

|5851

|

Kepler-107d

|

|0.095

|7.958203

|0.082

|

|style="background:#FFFF00"|transit

|1741{{±|18}}

|

|5851

|

Kepler-107e

|

|0.308

|14.749049

|0.123

|

|style="background:#FFFF00"|transit

|1741{{±|18}}

|

|5851

|

Kepler-108b

|

|0.772

|49.183921

|0.292

|

|style="background:#FFFF00"|transit

|4200{{±|500}}

|0.87

|5854

|

Kepler-108c

|

|0.73

|190.323494

|0.721

|

|style="background:#FFFF00"|transit

|4200{{±|500}}

|0.87

|5854

|

Kepler-109b

|

|0.211

|6.48163

|

|

|style="background:#FFFF00"|transit

|1570{{±|17}}

|1.04

|5952

|

Kepler-109c

|

|0.225

|21.2227

|

|

|style="background:#FFFF00"|transit

|1570{{±|17}}

|1.04

|5952

|

Kepler-110b

|

|0.163

|12.691112

|0.107

|

|style="background:#FFFF00"|transit

|1950{{±|30}}

|

|5960

|

Kepler-110c

|

|0.197

|31.719775

|0.198

|

|style="background:#FFFF00"|transit

|1950{{±|30}}

|

|5960

|

Kepler-111b

|

|0.141

|3.341815

|0.046

|

|style="background:#FFFF00"|transit

|2190{{±|20}}

|

|5952

|

Kepler-111c

|

|0.651

|224.784608

|0.761

|

|style="background:#FFFF00"|transit

|2190{{±|20}}

|

|5952

|

Kepler-112b

|

|0.211

|8.408878

|0.076

|

|style="background:#FFFF00"|transit

|1698{{±|14}}

|

|5544

|

Kepler-112c

|

|0.214

|28.574263

|0.172

|

|style="background:#FFFF00"|transit

|1698{{±|14}}

|

|5544

|

Kepler-113b

|0.037

|0.162

|4.754

|

|

|style="background:#FFFF00"|transit

|862{{±|3}}

|0.75

|4725

|

Kepler-113c

|

|0.194

|8.92507

|

|

|style="background:#FFFF00"|transit

|862{{±|3}}

|0.75

|4725

|

Kepler-114b

|

|0.112

|5.188549

|0.053

|722

|style="background:#FFFF00"|transit

|852{{±|4}}

|0.56

|4605

|

Kepler-115b

|

|0.097

|2.403679

|0.036

|

|style="background:#FFFF00"|transit

|2070{{±|20}}

|1

|5979

|

Kepler-115c

|

|0.232

|8.990889

|0.087

|

|style="background:#FFFF00"|transit

|2070{{±|20}}

|1

|5979

|

Kepler-116b

|

|0.305

|5.968734

|0.069

|

|style="background:#FFFF00"|transit

|3200{{±|50}}

|1.16

|6142

|

Kepler-116c

|

|0.205

|13.07163

|0.116

|

|style="background:#FFFF00"|transit

|3200{{±|50}}

|1.16

|6142

|

Kepler-117b

|0.094

|0.719

|18.7959228

|0.1445

|

|style="background:#FFFF00"|transit

|4700

|1.13

|6150

|

Kepler-117c

|1.84

|1.101

|50.790391

|0.2804

|

|style="background:#FFFF00"|transit

|4700

|1.13

|6150

|

Kepler-118b

|

|0.175

|7.518496

|0.073

|

|style="background:#FFFF00"|transit

|1900{{±|20}}

|0.86

|5274

|

Kepler-118c

|

|0.685

|20.17202

|0.141

|

|style="background:#FFFF00"|transit

|1900{{±|20}}

|0.86

|5274

|

Kepler-119b

|

|0.321

|2.422082

|0.035

|

|style="background:#FFFF00"|transit

|2340{{±|40}}

|

|5595

|

Kepler-119c

|

|0.082

|4.125103

|0.049

|

|style="background:#FFFF00"|transit

|2340{{±|40}}

|

|5595

|

Kepler-120b

|

|0.192

|6.312501

|0.055

|

|style="background:#FFFF00"|transit

|1281{{±|10}}

|

|4096

|

Kepler-120c

|

|0.136

|12.794585

|0.088

|

|style="background:#FFFF00"|transit

|1281{{±|10}}

|

|4096

|

Kepler-121b

|

|0.209

|3.177422

|0.039

|

|style="background:#FFFF00"|transit

|1690{{±|20}}

|

|5311

|

Kepler-121c

|

|0.203

|41.008011

|0.216

|

|style="background:#FFFF00"|transit

|1690{{±|20}}

|

|5311

|

Kepler-122b

|

|0.209

|5.766193

|0.064

|

|style="background:#FFFF00"|transit

|3450{{±|70}}

|0.99

|6050

|

Kepler-122c

|

|0.524

|12.465988

|0.108

|

|style="background:#FFFF00"|transit

|3450{{±|70}}

|0.99

|6050

|

Kepler-122d

|

|0.196

|21.587475

|0.155

|

|style="background:#FFFF00"|transit

|3450{{±|70}}

|0.99

|6050

|

Kepler-122e

|

|0.232

|37.993273

|0.227

|

|style="background:#FFFF00"|transit

|3450{{±|70}}

|0.99

|6050

|

Kepler-122f

|0.113

|0.156

|56.268

|

|

|style="background:#FF7519"|timing

|3450{{±|70}}

|0.99

|6050

|?

Kepler-123b

|

|0.262

|17.232366

|0.135

|

|style="background:#FFFF00"|transit

|3430{{±|80}}

|1.03

|6089

|

Kepler-123c

|

|0.132

|26.695074

|0.181

|

|style="background:#FFFF00"|transit

|3430{{±|80}}

|1.03

|6089

|

Kepler-124b

|

|0.065

|3.410493

|0.039

|

|style="background:#FFFF00"|transit

|1386{{±|10}}

|

|4984

|

Kepler-124c

|

|0.156

|13.821375

|0.1

|

|style="background:#FFFF00"|transit

|1386{{±|10}}

|

|4984

|

Kepler-124d

|

|0.099

|30.950851

|0.17

|

|style="background:#FFFF00"|transit

|1386{{±|10}}

|

|4984

|

Kepler-125b

|

|0.211

|4.164389

|0.041

|

|style="background:#FFFF00"|transit

|601{{±|3}}

|0.55

|3810

|

Kepler-125c

|

|0.066

|5.774464

|0.051

|

|style="background:#FFFF00"|transit

|601{{±|3}}

|0.55

|3810

|

Kepler-126b

|

|0.136

|10.495711

|0.099

|

|style="background:#FFFF00"|transit

|779{{±|5}}

|

|6239

|

Kepler-126c

|

|0.141

|21.869741

|0.162

|

|style="background:#FFFF00"|transit

|779{{±|5}}

|

|6239

|

Kepler-126d

|

|0.223

|100.283134

|0.448

|

|style="background:#FFFF00"|transit

|779{{±|5}}

|

|6239

|

Kepler-127b

|

|0.125

|14.435889

|0.125

|

|style="background:#FFFF00"|transit

|1162{{±|8}}

|

|6106

|

Kepler-127c

|

|0.237

|29.393195

|0.2

|

|style="background:#FFFF00"|transit

|1162{{±|8}}

|

|6106

|

Kepler-127d

|

|0.236

|48.630408

|0.28

|

|style="background:#FFFF00"|transit

|1162{{±|8}}

|

|6106

|

Kepler-129b

|

|0.211

|15.79186

|0.131

|

|style="background:#FFFF00"|transit

|1349{{±|14}}

|1.18

|5770

|

Kepler-129c

|

|0.227

|82.20017

|0.393

|

|style="background:#FFFF00"|transit

|1349{{±|14}}

|1.18

|5770

|

Kepler-130c

|

|0.259

|27.50868

|0.178

|

|style="background:#FFFF00"|transit

|1042{{±|7}}

|1

|5884

|

Kepler-130d

|

|0.146

|87.517905

|0.377

|

|style="background:#FFFF00"|transit

|1042{{±|7}}

|1

|5884

|

Kepler-131b

|0.051

|0.215

|16.092

|

|

|style="background:#FFFF00"|transit

|750{{±|4}}

|1.02

|5685

|

Kepler-131c

|0.026

|0.075

|25.5169

|

|

|style="background:#FFFF00"|transit

|750{{±|4}}

|1.02

|5685

|

Kepler-132b

|

|0.108

|6.178196

|0.067

|

|style="background:#FFFF00"|transit

|900{{±|70}}

|

|6003

|

Kepler-132c

|

|0.114

|6.414914

|0.068

|

|style="background:#FFFF00"|transit

|900{{±|70}}

|

|6003

|

Kepler-132d

|

|0.138

|18.010199

|0.136

|

|style="background:#FFFF00"|transit

|900{{±|70}}

|

|6003

|

Kepler-133b

|

|0.157

|8.129976

|0.083

|

|style="background:#FFFF00"|transit

|2170{{±|60}}

|

|5736

|

Kepler-133c

|

|0.253

|31.517586

|0.204

|

|style="background:#FFFF00"|transit

|2170{{±|60}}

|

|5736

|

Kepler-134b

|

|0.178

|5.317429

|0.06

|

|style="background:#FFFF00"|transit

|1102{{±|7}}

|

|5983

|

Kepler-134c

|

|0.112

|10.105785

|0.092

|

|style="background:#FFFF00"|transit

|1102{{±|7}}

|

|5983

|

Kepler-135b

|

|0.161

|6.00253

|0.067

|

|style="background:#FFFF00"|transit

|2060{{±|40}}

|

|6090

|

Kepler-135c

|

|0.103

|11.448708

|0.103

|

|style="background:#FFFF00"|transit

|2060{{±|40}}

|

|6090

|

Kepler-136b

|

|0.183

|11.5789

|0.106

|

|style="background:#FFFF00"|transit

|1389{{±|14}}

|1.2

|6165

|

Kepler-136c

|

|0.178

|16.399235

|0.133

|

|style="background:#FFFF00"|transit

|1389{{±|14}}

|1.2

|6165

|

Kepler-137b

|

|0.131

|8.436387

|0.077

|

|style="background:#FFFF00"|transit

|996{{±|6}}

|

|5187

|

Kepler-137c

|

|0.168

|18.735753

|0.13

|

|style="background:#FFFF00"|transit

|996{{±|6}}

|

|5187

|

Kepler-138b

|0.00021

|0.047

|10.3126

|

|

|style="background:#FFFF00"|transit

|218.5{{±|0.3}}

|0.52

|3841

|

Kepler-138c

|0.0062

|0.107

|13.7813

|

|

|style="background:#FFFF00"|transit

|218.5{{±|0.3}}

|0.52

|3841

|

Kepler-138d

|0.00201

|0.108

|23.0881

|

|431

|style="background:#FFFF00"|transit

|218.5{{±|0.3}}

|0.52

|3841

|

Kepler-139b

|

|0.262

|15.771044

|0.127

|

|style="background:#FFFF00"|transit

|1289{{±|13}}

|1.08

|5594

|

Kepler-139c

|

|0.302

|157.072878

|0.586

|

|style="background:#FFFF00"|transit

|1289{{±|13}}

|1.08

|5594

|

Kepler-140b

|

|0.144

|3.25427

|0.045

|

|style="background:#FFFF00"|transit

|1940{{±|20}}

|

|6077

|

Kepler-140c

|

|0.161

|91.353282

|0.414

|

|style="background:#FFFF00"|transit

|1940{{±|20}}

|

|6077

|

Kepler-141b

|

|0.062

|3.107675

|0.039

|

|style="background:#FFFF00"|transit

|990{{±|4}}

|1

|4910

|

Kepler-141c

|

|0.126

|7.010606

|0.067

|

|style="background:#FFFF00"|transit

|990{{±|4}}

|1

|4910

|?

Kepler-142b

|

|0.178

|2.024152

|0.032

|

|style="background:#FFFF00"|transit

|1818{{±|13}}

|0.99

|5790

|

Kepler-142c

|

|0.255

|4.761702

|0.057

|

|style="background:#FFFF00"|transit

|1818{{±|13}}

|0.99

|5790

|

Kepler-142d

|

|0.193

|41.809118

|0.242

|

|style="background:#FFFF00"|transit

|1818{{±|13}}

|0.99

|5790

|

Kepler-143b

|

|0.215

|16.007583

|0.127

|

|style="background:#FFFF00"|transit

|2700{{±|40}}

|

|5848

|

Kepler-143c

|

|0.301

|27.082511

|0.181

|

|style="background:#FFFF00"|transit

|2700{{±|40}}

|

|5848

|

Kepler-144b

|

|0.119

|5.885273

|0.066

|

|style="background:#FFFF00"|transit

|1269{{±|10}}

|1.03

|6075

|

Kepler-144c

|

|0.12

|10.104665

|0.094

|

|style="background:#FFFF00"|transit

|1269{{±|10}}

|1.03

|6075

|

Kepler-146b

|

|0.331

|31.158799

|0.2

|

|style="background:#FFFF00"|transit

|2390{{±|30}}

|

|5948

|

Kepler-146c

|

|0.279

|76.732171

|0.364

|

|style="background:#FFFF00"|transit

|2390{{±|30}}

|

|5948

|

Kepler-147b

|

|0.136

|12.610584

|0.113

|

|style="background:#FFFF00"|transit

|3500{{±|90}}

|1.01

|6012

|

Kepler-147c

|

|0.217

|33.416423

|0.216

|

|style="background:#FFFF00"|transit

|3500{{±|90}}

|1.01

|6012

|

Kepler-148b

|

|0.161

|1.729366

|0.028

|

|style="background:#FFFF00"|transit

|2640{{±|50}}

|

|5272

|

Kepler-148c

|

|0.321

|4.180043

|0.05

|

|style="background:#FFFF00"|transit

|2640{{±|50}}

|

|5272

|

Kepler-149b

|

|0.376

|29.198943

|0.184

|

|style="background:#FFFF00"|transit

|1893{{±|19}}

|

|5381

|

Kepler-149c

|

|0.144

|55.328328

|0.281

|

|style="background:#FFFF00"|transit

|1893{{±|19}}

|

|5381

|

Kepler-149d

|

|0.353

|160.018032

|0.571

|

|style="background:#FFFF00"|transit

|1893{{±|19}}

|

|5381

|

Kepler-150b

|

|0.112

|3.428054

|0.044

|

|style="background:#FFFF00"|transit

|2980{{±|60}}

|

|5560

|

Kepler-150c

|

|0.329

|7.381998

|0.073

|

|style="background:#FFFF00"|transit

|2980{{±|60}}

|

|5560

|

Kepler-150d

|

|0.249

|12.56093

|0.104

|

|style="background:#FFFF00"|transit

|2980{{±|60}}

|

|5560

|

Kepler-150e

|

|0.278

|30.826557

|0.189

|

|style="background:#FFFF00"|transit

|2980{{±|60}}

|

|5560

|

Kepler-151b

|

|0.273

|15.228958

|0.116

|

|style="background:#FFFF00"|transit

|2160{{±|30}}

|0.83

|5460

|

Kepler-151c

|

|0.186

|24.674612

|0.16

|

|style="background:#FFFF00"|transit

|2160{{±|30}}

|0.83

|5460

|

Kepler-152b

|

|0.249

|18.207973

|0.124

|

|style="background:#FFFF00"|transit

|1457{{±|10}}

|

|5088

|

Kepler-152c

|

|0.213

|88.255055

|0.356

|

|style="background:#FFFF00"|transit

|1457{{±|10}}

|

|5088

|

Kepler-153b

|

|0.261

|18.870227

|0.129

|

|style="background:#FFFF00"|transit

|1518{{±|11}}

|

|5404

|

Kepler-153c

|

|0.226

|46.90232

|0.237

|

|style="background:#FFFF00"|transit

|1518{{±|11}}

|

|5404

|

Kepler-154b

|

|0.202

|33.040532

|0.198

|

|style="background:#FFFF00"|transit

|3070{{±|60}}

|0.89

|5690

|

Kepler-154c

|

|0.263

|62.303276

|0.303

|

|style="background:#FFFF00"|transit

|3070{{±|60}}

|0.89

|5690

|

Kepler-155b

|

|0.186

|5.931194

|0.056

|

|style="background:#FFFF00"|transit

|965{{±|7}}

|0.58

|4508

|

Kepler-155c

|

|0.2

|52.661793

|0.242

|

|style="background:#FFFF00"|transit

|965{{±|7}}

|0.58

|4508

|

Kepler-156b

|

|0.205

|4.973456

|0.054

|

|style="background:#FFFF00"|transit

|1465{{±|11}}

|

|5094

|

Kepler-156c

|

|0.227

|15.906801

|0.117

|

|style="background:#FFFF00"|transit

|1465{{±|11}}

|

|5094

|

Kepler-157b

|

|0.118

|1.732342

|0.028

|

|style="background:#FFFF00"|transit

|2580{{±|40}}

|

|5774

|

Kepler-157c

|

|0.2

|13.5405

|0.11

|

|style="background:#FFFF00"|transit

|2580{{±|40}}

|

|5774

|

Kepler-158b

|

|0.189

|16.709184

|0.111

|

|style="background:#FFFF00"|transit

|1037{{±|6}}

|

|4623

|

Kepler-158c

|

|0.17

|28.551383

|0.158

|

|style="background:#FFFF00"|transit

|1037{{±|6}}

|

|4623

|

Kepler-159b

|

|0.212

|10.139623

|0.082

|

|style="background:#FFFF00"|transit

|1232{{±|10}}

|

|4625

|

Kepler-159c

|

|0.304

|43.595792

|0.218

|

|style="background:#FFFF00"|transit

|1232{{±|10}}

|

|4625

|

Kepler-160b

|

|0.137

|4.309427

|0.05

|

|style="background:#FFFF00"|transit

|3140{{±|60}}

|0.88

|5471{{±|115|37}}

|{{cite journal|arxiv=2006.02123|doi=10.1051/0004-6361/201936929|title=Transit least-squares survey|year=2020|last1=Heller|first1=René|last2=Hippke|first2=Michael|last3=Freudenthal|first3=Jantje|last4=Rodenbeck|first4=Kai|last5=Batalha|first5=Natalie M.|last6=Bryson|first6=Steve|s2cid=219260293|journal=Astronomy & Astrophysics|volume=638|pages=A10|bibcode=2020A&A...638A..10H }}

Kepler-160c

|

|0.322

|13.699087

|0.109

|

|style="background:#FFFF00"|transit

|3140{{±|60}}

|0.88

|5471{{±|115|37}}

|

Kepler-161b

|

|0.189

|4.921355

|0.054

|

|style="background:#FFFF00"|transit

|1435{{±|10}}

|0.77

|5078

|

Kepler-161c

|

|0.183

|7.06424

|0.068

|

|style="background:#FFFF00"|transit

|1435{{±|10}}

|0.77

|5078

|

Kepler-162b

|

|0.112

|6.919798

|0.069

|

|style="background:#FFFF00"|transit

|2860{{±|50}}

|

|5816

|

Kepler-162c

|

|0.27

|19.446355

|0.137

|

|style="background:#FFFF00"|transit

|2860{{±|50}}

|

|5816

|

Kepler-163b

|

|0.094

|7.810937

|0.078

|

|style="background:#FFFF00"|transit

|2300{{±|40}}

|0.96

|5776

|

Kepler-163c

|

|0.202

|21.347262

|0.152

|

|style="background:#FFFF00"|transit

|2300{{±|40}}

|0.96

|5776

|

Kepler-164b

|

|0.126

|5.03503

|0.058

|

|style="background:#FFFF00"|transit

|2980{{±|50}}

|1.11

|5888

|

Kepler-164c

|

|0.244

|10.945723

|0.097

|

|style="background:#FFFF00"|transit

|2980{{±|50}}

|1.11

|5888

|

Kepler-164d

|

|0.219

|28.986769

|0.187

|

|style="background:#FFFF00"|transit

|2980{{±|50}}

|1.11

|5888

|

Kepler-165b

|

|0.207

|8.180848

|0.072

|

|style="background:#FFFF00"|transit

|1860{{±|20}}

|

|5211

|

Kepler-165c

|

|0.199

|15.31299

|0.11

|

|style="background:#FFFF00"|transit

|1860{{±|20}}

|

|5211

|

Kepler-166b

|

|0.203

|7.650254

|0.072

|

|style="background:#FFFF00"|transit

|2000{{±|20}}

|

|5413

|

Kepler-166c

|

|0.212

|34.260281

|0.195

|

|style="background:#FFFF00"|transit

|2000{{±|20}}

|

|5413

|

Kepler-167b

|

|0.144

|4.3931632

|0.0483

|

|style="background:#FFFF00"|transit

|1100

|0.77

|4890

|

Kepler-167c

|

|0.138

|7.406114

|0.0684

|

|style="background:#FFFF00"|transit

|1100

|0.77

|4890

|

Kepler-168b

|

|0.13

|4.425391

|0.056

|

|style="background:#FFFF00"|transit

|4550{{±|160}}

|

|6282

|

Kepler-168c

|

|0.24

|13.193242

|0.116

|

|style="background:#FFFF00"|transit

|4550{{±|160}}

|

|6282

|

Kepler-169b

|

|0.101

|3.250619

|0.04

|

|style="background:#FFFF00"|transit

|1341{{±|9}}

|0.86

|4997

|

Kepler-169c

|

|0.108

|6.195469

|0.062

|

|style="background:#FFFF00"|transit

|1341{{±|9}}

|0.86

|4997

|

Kepler-169d

|

|0.112

|8.348125

|0.075

|

|style="background:#FFFF00"|transit

|1341{{±|9}}

|0.86

|4997

|

Kepler-169e

|

|0.196

|13.767102

|0.105

|

|style="background:#FFFF00"|transit

|1341{{±|9}}

|0.86

|4997

|

Kepler-169f

|

|0.23

|87.090195

|0.359

|

|style="background:#FFFF00"|transit

|1341{{±|9}}

|0.86

|4997

|

Kepler-170b

|

|0.285

|7.930592

|0.08

|

|style="background:#FFFF00"|transit

|2460{{±|40}}

|

|5679

|

Kepler-170c

|

|0.255

|16.665863

|0.131

|

|style="background:#FFFF00"|transit

|2460{{±|40}}

|

|5679

|

Kepler-171b

|

|0.209

|4.166972

|0.05

|

|style="background:#FFFF00"|transit

|2890{{±|60}}

|

|5642

|

Kepler-171c

|

|0.228

|11.463462

|0.098

|

|style="background:#FFFF00"|transit

|2890{{±|60}}

|

|5642

|

Kepler-171d

|

|0.169

|39.595519

|0.223

|

|style="background:#FFFF00"|transit

|2890{{±|60}}

|

|5642

|

Kepler-172b

|

|0.21

|2.940309

|0.04

|

|style="background:#FFFF00"|transit

|2770{{±|60}}

|0.86

|5526

|

Kepler-172c

|

|0.255

|6.388996

|0.068

|

|style="background:#FFFF00"|transit

|2770{{±|60}}

|0.86

|5526

|

Kepler-172d

|

|0.201

|14.627119

|0.118

|

|style="background:#FFFF00"|transit

|2770{{±|60}}

|0.86

|5526

|

Kepler-172e

|

|0.246

|35.118736

|0.211

|

|style="background:#FFFF00"|transit

|2770{{±|60}}

|0.86

|5526

|

Kepler-173b

|

|0.115

|4.263742

|0.048

|

|style="background:#FFFF00"|transit

|2780{{±|50}}

|0.78

|6031

|

Kepler-173c

|

|0.217

|8.005777

|0.074

|

|style="background:#FFFF00"|transit

|2780{{±|50}}

|0.78

|6031

|

Kepler-174b

|

|0.175

|13.98179

|0.1

|

|style="background:#FFFF00"|transit

|1268{{±|8}}

|

|4880

|

Kepler-174c

|

|0.133

|44.000529

|0.214

|

|style="background:#FFFF00"|transit

|1268{{±|8}}

|

|4880

|

Kepler-174d

|

|0.195

|247.35373

|0.677

|

|style="background:#FFFF00"|transit

|1268{{±|8}}

|

|4880

|

Kepler-175b

|

|0.228

|11.903515

|0.105

|

|style="background:#FFFF00"|transit

|4450{{±|150}}

|1.04

|6064

|

Kepler-175c

|

|0.277

|34.035257

|0.213

|

|style="background:#FFFF00"|transit

|4450{{±|150}}

|1.04

|6064

|

Kepler-176b

|

|0.128

|5.433074

|0.058

|

|style="background:#FFFF00"|transit

|1750{{±|20}}

|

|5232

|

Kepler-176c

|

|0.232

|12.759712

|0.102

|

|style="background:#FFFF00"|transit

|1750{{±|20}}

|

|5232

|

Kepler-176d

|

|0.224

|25.751974

|0.163

|

|style="background:#FFFF00"|transit

|1750{{±|20}}

|

|5232

|

Kepler-178b

|

|0.259

|9.576694

|0.085

|

|style="background:#FFFF00"|transit

|2380{{±|30}}

|

|5676

|

Kepler-178c

|

|0.257

|20.552802

|0.142

|

|style="background:#FFFF00"|transit

|2380{{±|30}}

|

|5676

|

Kepler-178d

|

|0.352

|96.678988

|0.397

|

|style="background:#FFFF00"|transit

|2380{{±|30}}

|

|5676

|

Kepler-179b

|

|0.146

|2.735926

|0.036

|

|style="background:#FFFF00"|transit

|2010{{±|20}}

|

|5302

|

Kepler-179c

|

|0.178

|6.40013

|0.064

|

|style="background:#FFFF00"|transit

|2010{{±|20}}

|

|5302

|

Kepler-180b

|

|0.134

|13.817124

|0.109

|

|style="background:#FFFF00"|transit

|2320{{±|30}}

|0.84

|5731

|

Kepler-180c

|

|0.269

|41.885775

|0.229

|

|style="background:#FFFF00"|transit

|2320{{±|30}}

|0.84

|5731

|

Kepler-181b

|

|0.113

|3.137873

|0.04

|

|style="background:#FFFF00"|transit

|2020{{±|30}}

|

|5333

|

Kepler-181c

|

|0.178

|4.302149

|0.049

|

|style="background:#FFFF00"|transit

|2020{{±|30}}

|

|5333

|

Kepler-182b

|

|0.23

|9.825792

|0.096

|

|style="background:#FFFF00"|transit

|5290{{±|180}}

|1.14

|6250

|

Kepler-182c

|

|0.306

|20.684342

|0.157

|

|style="background:#FFFF00"|transit

|5290{{±|180}}

|1.14

|6250

|

Kepler-183b

|

|0.184

|5.687945

|0.064

|

|style="background:#FFFF00"|transit

|3530{{±|100}}

|

|5888

|

Kepler-183c

|

|0.203

|11.637071

|0.103

|

|style="background:#FFFF00"|transit

|3530{{±|100}}

|

|5888

|

Kepler-184b

|

|0.211

|10.687576

|0.092

|

|style="background:#FFFF00"|transit

|2030{{±|20}}

|

|5788

|

Kepler-184c

|

|0.176

|20.303005

|0.141

|

|style="background:#FFFF00"|transit

|2030{{±|20}}

|

|5788

|

Kepler-184d

|

|0.222

|29.022358

|0.179

|

|style="background:#FFFF00"|transit

|2030{{±|20}}

|

|5788

|

Kepler-185b

|

|0.104

|1.6329

|0.026

|

|style="background:#FFFF00"|transit

|1542{{±|15}}

|0.79

|5208

|

Kepler-185c

|

|0.18

|20.729042

|0.139

|

|style="background:#FFFF00"|transit

|1542{{±|15}}

|0.79

|5208

|

Kepler-186b

|

|0.095

|3.8867907

|0.0343

|

|style="background:#FFFF00"|transit

|560

|0.54

|3755

|

Kepler-186c

|

|0.112

|7.267302

|0.0451

|

|style="background:#FFFF00"|transit

|560

|0.54

|3755

|

Kepler-186d

|

|0.125

|13.342996

|0.0781

|

|style="background:#FFFF00"|transit

|560

|0.54

|3755

|

Kepler-186e

|

|0.113

|22.407704

|0.11

|

|style="background:#FFFF00"|transit

|560

|0.54

|3755

|

Kepler-186f

|

|0.104

|129.9441

|0.432

|

|style="background:#FFFF00"|transit

|560

|0.54

|3755

|? Potentially habitable exoplanet

Kepler-187b

|

|0.126

|4.938864

|0.059

|

|style="background:#FFFF00"|transit

|3850{{±|110}}

|0.85

|6105

|

Kepler-187c

|

|0.238

|10.640263

|0.099

|

|style="background:#FFFF00"|transit

|3850{{±|110}}

|0.85

|6105

|

Kepler-188b

|

|0.15

|2.061897

|0.032

|

|style="background:#FFFF00"|transit

|3250{{±|80}}

|

|6021

|

Kepler-188c

|

|0.285

|5.996553

|0.066

|

|style="background:#FFFF00"|transit

|3250{{±|80}}

|

|6021

|

Kepler-189b

|

|0.108

|10.399931

|0.088

|

|style="background:#FFFF00"|transit

|1960{{±|20}}

|0.79

|5235

|

Kepler-189c

|

|0.212

|20.134866

|0.137

|

|style="background:#FFFF00"|transit

|1960{{±|20}}

|0.79

|5235

|

Kepler-190b

|

|0.139

|2.019999

|0.03

|

|style="background:#FFFF00"|transit

|1431{{±|9}}

|0.84

|5106

|

Kepler-190c

|

|0.13

|3.763024

|0.045

|

|style="background:#FFFF00"|transit

|1431{{±|9}}

|0.84

|5106

|

Kepler-191b

|

|0.12

|9.939632

|0.087

|

|style="background:#FFFF00"|transit

|1970{{±|30}}

|0.85

|5282

|

Kepler-191c

|

|0.166

|17.738506

|0.128

|

|style="background:#FFFF00"|transit

|1970{{±|30}}

|0.85

|5282

|

Kepler-192b

|

|0.244

|9.926746

|0.09

|

|style="background:#FFFF00"|transit

|2170{{±|20}}

|

|5479

|

Kepler-192c

|

|0.249

|21.2234

|0.15

|

|style="background:#FFFF00"|transit

|2170{{±|20}}

|

|5479

|

Kepler-193b

|

|0.213

|11.38848

|0.106

|

|style="background:#FFFF00"|transit

|3390{{±|80}}

|

|6335

|

Kepler-193c

|

|0.245

|50.697494

|0.286

|

|style="background:#FFFF00"|transit

|3390{{±|80}}

|

|6335

|

Kepler-194b

|

|0.135

|2.092281

|0.032

|

|style="background:#FFFF00"|transit

|3700{{±|100}}

|

|6089

|

Kepler-194c

|

|0.231

|17.308032

|0.131

|

|style="background:#FFFF00"|transit

|3700{{±|100}}

|

|6089

|

Kepler-194d

|

|0.214

|52.814973

|0.275

|

|style="background:#FFFF00"|transit

|3700{{±|100}}

|

|6089

|

Kepler-195b

|

|0.181

|8.307872

|0.077

|

|style="background:#FFFF00"|transit

|2170{{±|30}}

|

|5329

|

Kepler-195c

|

|0.138

|34.096863

|0.197

|

|style="background:#FFFF00"|transit

|2170{{±|30}}

|

|5329

|

Kepler-196b

|

|0.17

|20.739886

|0.138

|

|style="background:#FFFF00"|transit

|1491{{±|10}}

|

|5128

|

Kepler-196c

|

|0.2

|47.427737

|0.24

|

|style="background:#FFFF00"|transit

|1491{{±|10}}

|

|5128

|

Kepler-197b

|

|0.091

|5.599308

|0.06

|

|style="background:#FFFF00"|transit

|1088{{±|7}}

|

|6004

|

Kepler-197c

|

|0.11

|10.349695

|0.09

|

|style="background:#FFFF00"|transit

|1088{{±|7}}

|

|6004

|

Kepler-197d

|

|0.109

|15.677563

|0.119

|

|style="background:#FFFF00"|transit

|1088{{±|7}}

|

|6004

|

Kepler-197e

|

|0.081

|25.209715

|0.164

|

|style="background:#FFFF00"|transit

|1088{{±|7}}

|

|6004

|

Kepler-198b

|

|0.252

|17.790037

|0.131

|

|style="background:#FFFF00"|transit

|1638{{±|14}}

|0.93

|5574

|

Kepler-198c

|

|0.22

|49.567416

|0.259

|

|style="background:#FFFF00"|transit

|1638{{±|14}}

|0.93

|5574

|

Kepler-199b

|

|0.277

|23.637604

|0.158

|

|style="background:#FFFF00"|transit

|1725{{±|14}}

|

|5644

|

Kepler-199c

|

|0.29

|67.093408

|0.316

|

|style="background:#FFFF00"|transit

|1725{{±|14}}

|

|5644

|

Kepler-200b

|

|0.19

|8.594805

|0.08

|

|style="background:#FFFF00"|transit

|2210{{±|20}}

|

|5678

|

Kepler-200c

|

|0.142

|10.222157

|0.09

|

|style="background:#FFFF00"|transit

|2210{{±|20}}

|

|5678

|

Kepler-201b

|

|0.219

|25.672083

|0.175

|

|style="background:#FFFF00"|transit

|2240{{±|30}}

|1.17

|6065

|

Kepler-201c

|

|0.254

|151.884058

|0.573

|

|style="background:#FFFF00"|transit

|2240{{±|30}}

|1.17

|6065

|

Kepler-202b

|

|0.145

|4.069427

|0.045

|

|style="background:#FFFF00"|transit

|937{{±|3}}

|

|4668

|

Kepler-202c

|

|0.165

|16.282493

|0.113

|

|style="background:#FFFF00"|transit

|937{{±|3}}

|

|4668

|

Kepler-203b

|

|0.229

|3.162697

|0.043

|

|style="background:#FFFF00"|transit

|2340{{±|30}}

|0.98

|5821

|

Kepler-203c

|

|0.22

|5.370647

|0.061

|

|style="background:#FFFF00"|transit

|2340{{±|30}}

|0.98

|5821

|

Kepler-203d

|

|0.128

|11.32972

|0.1

|

|style="background:#FFFF00"|transit

|2340{{±|30}}

|0.98

|5821

|

Kepler-204b

|

|0.226

|14.400974

|0.117

|

|style="background:#FFFF00"|transit

|2280{{±|20}}

|0.96

|5812

|

Kepler-204c

|

|0.16

|25.660593

|0.173

|

|style="background:#FFFF00"|transit

|2280{{±|20}}

|0.96

|5812

|

Kepler-205b

|

|0.135

|2.75564

|0.032

|

|style="background:#FFFF00"|transit

|523.4{{±|1.1}}

|

|4321

|

Kepler-205c

|

|0.146

|20.306546

|0.122

|

|style="background:#FFFF00"|transit

|523.4{{±|1.1}}

|

|4321

|

Kepler-206b

|

|0.107

|7.781987

|0.078

|

|style="background:#FFFF00"|transit

|1972{{±|16}}

|0.94

|5764

|

Kepler-206c

|

|0.158

|13.137471

|0.111

|

|style="background:#FFFF00"|transit

|1972{{±|16}}

|0.94

|5764

|

Kepler-206d

|

|0.106

|23.44281

|0.163

|

|style="background:#FFFF00"|transit

|1972{{±|16}}

|0.94

|5764

|

Kepler-207b

|

|0.14

|1.611865

|0.029

|

|style="background:#FFFF00"|transit

|2920{{±|30}}

|

|5920

|

Kepler-207c

|

|0.134

|3.071571

|0.044

|

|style="background:#FFFF00"|transit

|2920{{±|30}}

|

|5920

|

Kepler-207d

|

|0.295

|5.868075

|0.068

|

|style="background:#FFFF00"|transit

|2920{{±|30}}

|

|5920

|

Kepler-208b

|

|0.145

|4.22864

|0.054

|

|style="background:#FFFF00"|transit

|2580{{±|20}}

|1.03

|6092

|

Kepler-208c

|

|0.124

|7.466623

|0.079

|

|style="background:#FFFF00"|transit

|2580{{±|20}}

|1.03

|6092

|

Kepler-208d

|

|0.107

|11.131786

|0.103

|

|style="background:#FFFF00"|transit

|2580{{±|20}}

|1.03

|6092

|

Kepler-208e

|

|0.132

|16.259458

|0.132

|

|style="background:#FFFF00"|transit

|2580{{±|20}}

|1.03

|6092

|

Kepler-209b

|

|0.202

|16.087845

|0.122

|

|style="background:#FFFF00"|transit

|1913{{±|18}}

|

|5513

|

Kepler-209c

|

|0.277

|41.749882

|0.231

|

|style="background:#FFFF00"|transit

|1913{{±|18}}

|

|5513

|

Kepler-210b

|

|0.262

|2.453234

|0.032

|

|style="background:#FFFF00"|transit

|764{{±|2}}

|

|4559

|

Kepler-210c

|

|0.323

|7.972513

|0.07

|

|style="background:#FFFF00"|transit

|764{{±|2}}

|

|4559

|

Kepler-211b

|

|0.112

|4.138575

|0.048

|

|style="background:#FFFF00"|transit

|1018{{±|5}}

|0.97

|5123

|

Kepler-211c

|

|0.115

|6.04045

|0.062

|

|style="background:#FFFF00"|transit

|1018{{±|5}}

|0.97

|5123

|

Kepler-212b

|

|0.097

|16.257582

|0.133

|

|style="background:#FFFF00"|transit

|2280{{±|20}}

|1.16

|5852

|

Kepler-212c

|

|0.244

|31.805174

|0.207

|

|style="background:#FFFF00"|transit

|2280{{±|20}}

|1.16

|5852

|

Kepler-213b

|

|0.145

|2.46236

|0.036

|

|style="background:#FFFF00"|transit

|2100{{±|20}}

|0.94

|5696

|

Kepler-213c

|

|0.209

|4.822962

|0.057

|

|style="background:#FFFF00"|transit

|2100{{±|20}}

|0.94

|5696

|

Kepler-214b

|

|0.233

|15.660544

|0.13

|

|style="background:#FFFF00"|transit

|4080{{±|70}}

|

|6169

|

Kepler-214c

|

|0.19

|28.7798

|0.194

|

|style="background:#FFFF00"|transit

|4080{{±|70}}

|

|6169

|

Kepler-215b

|

|0.145

|9.360672

|0.084

|

|style="background:#FFFF00"|transit

|1607{{±|12}}

|0.77

|5739

|

Kepler-215c

|

|0.158

|14.667108

|0.113

|

|style="background:#FFFF00"|transit

|1607{{±|12}}

|0.77

|5739

|

Kepler-215d

|

|0.213

|30.864423

|0.185

|

|style="background:#FFFF00"|transit

|1607{{±|12}}

|0.77

|5739

|

Kepler-215e

|

|0.156

|68.16101

|0.314

|

|style="background:#FFFF00"|transit

|1607{{±|12}}

|0.77

|5739

|

Kepler-216b

|

|0.21

|7.693641

|0.079

|

|style="background:#FFFF00"|transit

|4000{{±|70}}

|

|6091

|

Kepler-216c

|

|0.271

|17.406669

|0.136

|

|style="background:#FFFF00"|transit

|4000{{±|70}}

|

|6091

|

Kepler-217b

|

|0.199

|5.374943

|0.065

|

|style="background:#FFFF00"|transit

|3720{{±|50}}

|

|6171

|

Kepler-217c

|

|0.165

|8.586004

|0.089

|

|style="background:#FFFF00"|transit

|3720{{±|50}}

|

|6171

|

Kepler-218b

|

|0.132

|3.619337

|0.046

|

|style="background:#FFFF00"|transit

|2180{{±|20}}

|

|5502

|

Kepler-218c

|

|0.28

|44.699576

|0.248

|

|style="background:#FFFF00"|transit

|2180{{±|20}}

|

|5502

|

Kepler-219b

|

|0.263

|4.585512

|0.057

|

|style="background:#FFFF00"|transit

|2620{{±|30}}

|

|5786

|

Kepler-219c

|

|0.319

|22.714613

|0.165

|

|style="background:#FFFF00"|transit

|2620{{±|30}}

|

|5786

|

Kepler-219d

|

|0.251

|47.903645

|0.272

|

|style="background:#FFFF00"|transit

|2620{{±|30}}

|

|5786

|

Kepler-220b

|

|0.072

|4.159807

|0.046

|

|style="background:#FFFF00"|transit

|560{{±|2}}

|

|4632

|

Kepler-220c

|

|0.14

|9.034199

|0.076

|

|style="background:#FFFF00"|transit

|560{{±|2}}

|

|4632

|

Kepler-220d

|

|0.087

|28.122397

|0.163

|

|style="background:#FFFF00"|transit

|560{{±|2}}

|

|4632

|

Kepler-220e

|

|0.119

|45.902733

|0.226

|

|style="background:#FFFF00"|transit

|560{{±|2}}

|

|4632

|

Kepler-221b

|

|0.153

|2.795906

|0.037

|

|style="background:#FFFF00"|transit

|1270{{±|9}}

|0.72

|5243

|

Kepler-221c

|

|0.261

|5.690586

|0.059

|

|style="background:#FFFF00"|transit

|1270{{±|9}}

|0.72

|5243

|

Kepler-221d

|

|0.244

|10.04156

|0.087

|

|style="background:#FFFF00"|transit

|1270{{±|9}}

|0.72

|5243

|

Kepler-221e

|

|0.235

|18.369917

|0.13

|

|style="background:#FFFF00"|transit

|1270{{±|9}}

|0.72

|5243

|

Kepler-222b

|

|0.282

|3.936981

|0.048

|

|style="background:#FFFF00"|transit

|2520{{±|40}}

|

|5433

|

Kepler-222c

|

|0.414

|10.08881

|0.091

|

|style="background:#FFFF00"|transit

|2520{{±|40}}

|

|5433

|

Kepler-222d

|

|0.329

|28.081912

|0.18

|

|style="background:#FFFF00"|transit

|2520{{±|40}}

|

|5433

|

Kepler-223b

|0.02328

|0.267

|7.38449

|

|

|style="background:#FFFF00"|transit

|6400{{±|400}}

|1.12

|

|

Kepler-223c

|0.01605

|0.307

|9.84564

|

|

|style="background:#FFFF00"|transit

|6400{{±|400}}

|1.12

|

|

Kepler-223d

|0.02517

|0.467

|14.78869

|

|

|style="background:#FFFF00"|transit

|6400{{±|400}}

|1.12

|

|

Kepler-223e

|0.0151

|0.41

|19.72567

|

|

|style="background:#FFFF00"|transit

|6400{{±|400}}

|1.12

|

|

Kepler-224b

|

|0.124

|3.132924

|0.038

|

|style="background:#FFFF00"|transit

|2600{{±|60}}

|0.74

|5018

|

Kepler-224c

|

|0.278

|5.925003

|0.058

|

|style="background:#FFFF00"|transit

|2600{{±|60}}

|0.74

|5018

|

Kepler-224d

|

|0.205

|11.349393

|0.089

|

|style="background:#FFFF00"|transit

|2600{{±|60}}

|0.74

|5018

|

Kepler-224e

|

|0.176

|18.643577

|0.124

|

|style="background:#FFFF00"|transit

|2600{{±|60}}

|0.74

|5018

|

Kepler-225b

|

|0.107

|6.738975

|0.056

|

|style="background:#FFFF00"|transit

|1850{{±|40}}

|

|3682

|

Kepler-225c

|

|0.164

|18.794234

|0.111

|

|style="background:#FFFF00"|transit

|1850{{±|40}}

|

|3682

|

Kepler-226b

|

|0.138

|3.940997

|0.047

|

|style="background:#FFFF00"|transit

|3280{{±|80}}

|0.86

|5571

|

Kepler-226c

|

|0.203

|5.349555

|0.058

|

|style="background:#FFFF00"|transit

|3280{{±|80}}

|0.86

|5571

|

Kepler-226d

|

|0.109

|8.109044

|0.076

|

|style="background:#FFFF00"|transit

|3280{{±|80}}

|0.86

|5571

|

Kepler-227b

|

|0.277

|9.488015

|0.09

|

|style="background:#FFFF00"|transit

|3640{{±|100}}

|

|5854

|

Kepler-227c

|

|0.271

|54.418694

|0.29

|

|style="background:#FFFF00"|transit

|3640{{±|100}}

|

|5854

|

Kepler-228b

|

|0.136

|2.566546

|0.038

|

|style="background:#FFFF00"|transit

|5600{{±|300}}

|

|6043

|

Kepler-228c

|

|0.241

|4.134444

|0.052

|

|style="background:#FFFF00"|transit

|5600{{±|300}}

|

|6043

|

Kepler-228d

|

|0.36

|11.094286

|0.101

|

|style="background:#FFFF00"|transit

|5600{{±|300}}

|

|6043

|

Kepler-229b

|

|0.196

|6.252972

|0.062

|

|style="background:#FFFF00"|transit

|2750{{±|70}}

|

|5120

|

Kepler-229c

|

|0.439

|16.068638

|0.117

|

|style="background:#FFFF00"|transit

|2750{{±|70}}

|

|5120

|

Kepler-229d

|

|0.343

|41.194912

|0.22

|

|style="background:#FFFF00"|transit

|2750{{±|70}}

|

|5120

|

Kepler-230b

|

|0.38

|32.625555

|0.191

|

|style="background:#FFFF00"|transit

|2460{{±|40}}

|

|5588

|

Kepler-230c

|

|0.182

|91.773242

|0.38

|

|style="background:#FFFF00"|transit

|2460{{±|40}}

|

|5588

|

Kepler-231b

|

|0.154

|10.065275

|0.074

|

|style="background:#FFFF00"|transit

|988{{±|9}}

|0.58

|3767

|

Kepler-231c

|

|0.172

|19.271566

|0.114

|

|style="background:#FFFF00"|transit

|988{{±|9}}

|0.58

|3767

|

Kepler-232b

|

|0.275

|4.431222

|0.054

|

|style="background:#FFFF00"|transit

|4570{{±|160}}

|

|5847

|

Kepler-232c

|

|0.342

|11.379349

|0.101

|

|style="background:#FFFF00"|transit

|4570{{±|160}}

|

|5847

|

Kepler-233b

|

|0.217

|8.472382

|0.077

|

|style="background:#FFFF00"|transit

|2860{{±|60}}

|

|5360

|

Kepler-233c

|

|0.242

|60.418955

|0.287

|

|style="background:#FFFF00"|transit

|2860{{±|60}}

|

|5360

|

Kepler-234b

|

|0.33

|2.711506

|0.04

|

|style="background:#FFFF00"|transit

|5900{{±|300}}

|

|6224

|

Kepler-234c

|

|0.313

|7.21205

|0.077

|

|style="background:#FFFF00"|transit

|5900{{±|300}}

|

|6224

|

Kepler-235b

|

|0.199

|3.340222

|0.037

|

|style="background:#FFFF00"|transit

|1410{{±|20}}

|0.59

|4255

|

Kepler-235c

|

|0.114

|7.824904

|0.065

|

|style="background:#FFFF00"|transit

|1410{{±|20}}

|0.59

|4255

|

Kepler-235d

|

|0.183

|20.060548

|0.122

|

|style="background:#FFFF00"|transit

|1410{{±|20}}

|0.59

|4255

|

{{vanchor|Kepler-235e}}

|

|0.198

|46.183669

|0.213

|

|style="background:#FFFF00"|transit

|1410{{±|20}}

|0.59

|4255

|

Kepler-236b

|

|0.14

|8.295611

|0.065

|

|style="background:#FFFF00"|transit

|949{{±|7}}

|0.56

|3750

|

Kepler-236c

|

|0.178

|23.968127

|0.132

|

|style="background:#FFFF00"|transit

|949{{±|7}}

|0.56

|3750

|

Kepler-237b

|

|0.126

|4.715106

|0.05

|

|style="background:#FFFF00"|transit

|2180{{±|30}}

|0.7

|4861

|

Kepler-237c

|

|0.186

|8.103636

|0.071

|

|style="background:#FFFF00"|transit

|2180{{±|30}}

|0.7

|4861

|

Kepler-238b

|

|0.154

|2.090876

|0.034

|

|style="background:#FFFF00"|transit

|6200{{±|300}}

|1.06

|5751

|

Kepler-238c

|

|0.213

|6.155557

|0.069

|

|style="background:#FFFF00"|transit

|6200{{±|300}}

|1.06

|5751

|

Kepler-238d

|

|0.274

|13.233549

|0.115

|

|style="background:#FFFF00"|transit

|6200{{±|300}}

|1.06

|5751

|

Kepler-239b

|

|0.208

|11.763051

|0.095

|

|style="background:#FFFF00"|transit

|2150{{±|40}}

|0.74

|4914

|

Kepler-239c

|

|0.224

|56.228098

|0.268

|

|style="background:#FFFF00"|transit

|2150{{±|40}}

|0.74

|4914

|

Kepler-240b

|

|0.122

|4.144495

|0.048

|

|style="background:#FFFF00"|transit

|2480{{±|60}}

|

|4985

|

Kepler-240c

|

|0.196

|7.953528

|0.074

|

|style="background:#FFFF00"|transit

|2480{{±|60}}

|

|4985

|

Kepler-241b

|

|0.208

|12.718092

|0.094

|

|style="background:#FFFF00"|transit

|1980{{±|130}}

|

|4699

|

Kepler-241c

|

|0.229

|36.065978

|0.189

|

|style="background:#FFFF00"|transit

|1980{{±|130}}

|

|4699

|

Kepler-242b

|

|0.233

|8.20395

|0.075

|

|style="background:#FFFF00"|transit

|1990{{±|30}}

|

|5020

|

Kepler-242c

|

|0.178

|14.496481

|0.109

|

|style="background:#FFFF00"|transit

|1990{{±|30}}

|

|5020

|

Kepler-243b

|

|0.219

|5.715442

|0.062

|

|style="background:#FFFF00"|transit

|2300{{±|30}}

|0.89

|5228

|

Kepler-243c

|

|0.178

|20.026218

|0.142

|

|style="background:#FFFF00"|transit

|2300{{±|30}}

|0.89

|5228

|

Kepler-244b

|

|0.246

|4.311792

|0.05

|

|style="background:#FFFF00"|transit

|3480{{±|120}}

|

|5554

|

Kepler-244c

|

|0.183

|9.767292

|0.087

|

|style="background:#FFFF00"|transit

|3480{{±|120}}

|

|5554

|

Kepler-244d

|

|0.206

|20.050401

|0.14

|

|style="background:#FFFF00"|transit

|3480{{±|120}}

|

|5554

|

Kepler-245b

|

|0.229

|7.49019

|0.071

|

|style="background:#FFFF00"|transit

|2870{{±|80}}

|0.8

|5100

|

Kepler-245c

|

|0.194

|17.460812

|0.124

|

|style="background:#FFFF00"|transit

|2870{{±|80}}

|0.8

|5100

|

Kepler-245d

|

|0.27

|36.277108

|0.202

|

|style="background:#FFFF00"|transit

|2870{{±|80}}

|0.8

|5100

|

Kepler-246b

|

|0.209

|4.60182

|0.052

|

|style="background:#FFFF00"|transit

|2070{{±|20}}

|0.86

|5206

|

Kepler-246c

|

|0.134

|11.187161

|0.095

|

|style="background:#FFFF00"|transit

|2070{{±|20}}

|0.86

|5206

|

Kepler-247b

|

|0.146

|3.33616

|0.042

|

|style="background:#FFFF00"|transit

|2200{{±|40}}

|

|5100

|

Kepler-247c

|

|0.365

|9.439452

|0.084

|

|style="background:#FFFF00"|transit

|2200{{±|40}}

|

|5100

|

Kepler-247d

|

|0.352

|20.477912

|0.14

|

|style="background:#FFFF00"|transit

|2200{{±|40}}

|

|5100

|

Kepler-248b

|

|0.269

|6.308205

|0.066

|

|style="background:#FFFF00"|transit

|2460{{±|40}}

|

|5190

|

Kepler-248c

|

|0.363

|16.239494

|0.123

|

|style="background:#FFFF00"|transit

|2460{{±|40}}

|

|5190

|

Kepler-249b

|

|0.097

|3.306539

|0.035

|

|style="background:#FFFF00"|transit

|624{{±|3}}

|

|3568

|

Kepler-249c

|

|0.135

|7.113702

|0.058

|

|style="background:#FFFF00"|transit

|624{{±|3}}

|

|3568

|

Kepler-249d

|

|0.14

|15.368459

|0.097

|

|style="background:#FFFF00"|transit

|624{{±|3}}

|

|3568

|

Kepler-250b

|

|0.101

|4.148141

|0.048

|

|style="background:#FFFF00"|transit

|2530{{±|50}}

|0.8

|5160

|

Kepler-250c

|

|0.203

|7.156804

|0.069

|

|style="background:#FFFF00"|transit

|2530{{±|50}}

|0.8

|5160

|

Kepler-250d

|

|0.194

|17.648312

|0.127

|

|style="background:#FFFF00"|transit

|2530{{±|50}}

|0.8

|5160

|

Kepler-251b

|

|0.119

|4.790936

|0.053

|

|style="background:#FFFF00"|transit

|3090{{±|90}}

|0.91

|5526

|

Kepler-251c

|

|0.247

|16.514043

|0.122

|

|style="background:#FFFF00"|transit

|3090{{±|90}}

|0.91

|5526

|

Kepler-251d

|

|0.247

|30.133001

|0.182

|

|style="background:#FFFF00"|transit

|3090{{±|90}}

|0.91

|5526

|

Kepler-251e

|

|0.247

|99.640161

|0.404

|

|style="background:#FFFF00"|transit

|3090{{±|90}}

|0.91

|5526

|

Kepler-252b

|

|0.11

|6.668391

|0.058

|

|style="background:#FFFF00"|transit

|1251{{±|11}}

|0.52

|4208

|

Kepler-252c

|

|0.192

|10.848463

|0.08

|

|style="background:#FFFF00"|transit

|1251{{±|11}}

|0.52

|4208

|

Kepler-253b

|

|0.145

|3.783986

|0.046

|

|style="background:#FFFF00"|transit

|2800{{±|60}}

|

|5208

|

Kepler-253c

|

|0.236

|10.281951

|0.089

|

|style="background:#FFFF00"|transit

|2800{{±|60}}

|

|5208

|

Kepler-253d

|

|0.283

|18.119869

|0.13

|

|style="background:#FFFF00"|transit

|2800{{±|60}}

|

|5208

|

Kepler-254b

|

|0.345

|5.826662

|0.064

|

|style="background:#FFFF00"|transit

|4700{{±|200}}

|

|5957

|

Kepler-254c

|

|0.192

|12.412183

|0.105

|

|style="background:#FFFF00"|transit

|4700{{±|200}}

|

|5957

|

Kepler-254d

|

|0.223

|18.746477

|0.139

|

|style="background:#FFFF00"|transit

|4700{{±|200}}

|

|5957

|

Kepler-255b

|

|0.138

|5.714606

|0.063

|

|style="background:#FFFF00"|transit

|3530{{±|100}}

|0.97

|5573

|

Kepler-255c

|

|0.267

|9.946047

|0.092

|

|style="background:#FFFF00"|transit

|3530{{±|100}}

|0.97

|5573

|

Kepler-256b

|

|0.142

|1.620493

|0.027

|

|style="background:#FFFF00"|transit

|3440{{±|80}}

|1.02

|5551

|

Kepler-256c

|

|0.192

|3.38802

|0.045

|

|style="background:#FFFF00"|transit

|3440{{±|80}}

|1.02

|5551

|

Kepler-256d

|

|0.221

|5.839172

|0.064

|

|style="background:#FFFF00"|transit

|3440{{±|80}}

|1.02

|5551

|

Kepler-256e

|

|0.21

|10.681572

|0.096

|

|style="background:#FFFF00"|transit

|3440{{±|80}}

|1.02

|5551

|

Kepler-257b

|

|0.233

|2.382667

|0.034

|

|style="background:#FFFF00"|transit

|2600{{±|50}}

|

|5180

|

Kepler-257c

|

|0.483

|6.581484

|0.066

|

|style="background:#FFFF00"|transit

|2600{{±|50}}

|

|5180

|

Kepler-257d

|

|0.442

|24.664551

|0.16

|

|style="background:#FFFF00"|transit

|2600{{±|50}}

|

|5180

|

Kepler-258b

|

|0.362

|13.19722

|0.103

|

|style="background:#FFFF00"|transit

|1900{{±|20}}

|0.8

|4942

|

Kepler-258c

|

|0.322

|33.653079

|0.193

|

|style="background:#FFFF00"|transit

|1900{{±|20}}

|0.8

|4942

|

Kepler-259b

|

|0.25

|8.115317

|0.079

|

|style="background:#FFFF00"|transit

|3360{{±|80}}

|

|5938

|

Kepler-259c

|

|0.241

|36.924931

|0.217

|

|style="background:#FFFF00"|transit

|3360{{±|80}}

|

|5938

|

Kepler-260b

|

|0.179

|8.187399

|0.075

|

|style="background:#FFFF00"|transit

|2080{{±|20}}

|0.88

|5250

|

Kepler-260c

|

|0.155

|76.050178

|0.332

|

|style="background:#FFFF00"|transit

|2080{{±|20}}

|0.88

|5250

|

Kepler-261b

|

|0.194

|10.381227

|0.088

|

|style="background:#FFFF00"|transit

|1044{{±|5}}

|0.87

|5098

|

Kepler-261c

|

|0.178

|24.570858

|0.156

|

|style="background:#FFFF00"|transit

|1044{{±|5}}

|0.87

|5098

|

Kepler-262b

|

|0.121

|13.060855

|0.108

|

|style="background:#FFFF00"|transit

|2030{{±|20}}

|

|5841

|

Kepler-262c

|

|0.146

|21.853722

|0.152

|

|style="background:#FFFF00"|transit

|2030{{±|20}}

|

|5841

|

Kepler-263b

|

|0.238

|16.568087

|0.12

|

|style="background:#FFFF00"|transit

|2510{{±|50}}

|

|5265

|

Kepler-263c

|

|0.22

|47.332773

|0.242

|

|style="background:#FFFF00"|transit

|2510{{±|50}}

|

|5265

|

Kepler-264b

|

|0.297

|40.806231

|0.249

|

|style="background:#FFFF00"|transit

|3150{{±|60}}

|1.32

|6158

|

Kepler-264c

|

|0.252

|140.101261

|0.566

|

|style="background:#FFFF00"|transit

|3150{{±|60}}

|1.32

|6158

|

Kepler-265b

|

|0.166

|6.846262

|0.069

|

|style="background:#FFFF00"|transit

|4330{{±|160}}

|1.03

|5835

|

Kepler-265c

|

|0.235

|17.028937

|0.127

|

|style="background:#FFFF00"|transit

|4330{{±|160}}

|1.03

|5835

|

Kepler-265d

|

|0.222

|43.130617

|0.236

|

|style="background:#FFFF00"|transit

|4330{{±|160}}

|1.03

|5835

|

Kepler-265e

|

|0.231

|67.831024

|0.319

|

|style="background:#FFFF00"|transit

|4330{{±|160}}

|1.03

|5835

|

Kepler-266b

|

|0.221

|6.61833

|0.071

|

|style="background:#FFFF00"|transit

|4640{{±|190}}

|0.99

|5885

|

Kepler-266c

|

|0.347

|107.723601

|0.457

|

|style="background:#FFFF00"|transit

|4640{{±|190}}

|0.99

|5885

|

Kepler-267b

|

|0.177

|3.353728

|0.037

|

|style="background:#FFFF00"|transit

|870{{±|8}}

|0.56

|4258

|

Kepler-267c

|

|0.19

|6.87745

|0.06

|

|style="background:#FFFF00"|transit

|870{{±|8}}

|0.56

|4258

|

Kepler-267d

|

|0.203

|28.464515

|0.154

|

|style="background:#FFFF00"|transit

|870{{±|8}}

|0.56

|4258

|

Kepler-268b

|

|0.227

|25.934138

|0.18

|

|style="background:#FFFF00"|transit

|2840{{±|30}}

|

|6081

|

Kepler-268c

|

|0.302

|83.446393

|0.391

|

|style="background:#FFFF00"|transit

|2840{{±|30}}

|

|6081

|

Kepler-269b

|

|0.22

|5.326718

|0.061

|

|style="background:#FFFF00"|transit

|7900{{±|600}}

|0.98

|5847

|

Kepler-269c

|

|0.151

|8.127899

|0.081

|

|style="background:#FFFF00"|transit

|7900{{±|600}}

|0.98

|5847

|

Kepler-270b

|

|0.179

|11.476094

|0.107

|

|style="background:#FFFF00"|transit

|3180{{±|40}}

|

|6067

|

Kepler-270c

|

|0.158

|25.262887

|0.18

|

|style="background:#FFFF00"|transit

|3180{{±|40}}

|

|6067

|

Kepler-271b

|

|0.079

|5.217738

|0.056

|

|style="background:#FFFF00"|transit

|1334{{±|12}}

|

|5524

|

Kepler-271c

|

|0.089

|7.410935

|0.071

|

|style="background:#FFFF00"|transit

|1334{{±|12}}

|

|5524

|

Kepler-272b

|

|0.128

|2.971353

|0.038

|

|style="background:#FFFF00"|transit

|2970{{±|40}}

|0.79

|5297

|

Kepler-272c

|

|0.16

|6.057342

|0.061

|

|style="background:#FFFF00"|transit

|2970{{±|40}}

|0.79

|5297

|

Kepler-272d

|

|0.201

|10.937304

|0.091

|

|style="background:#FFFF00"|transit

|2970{{±|40}}

|0.79

|5297

|

Kepler-273b

|

|0.134

|2.936532

|0.037

|

|style="background:#FFFF00"|transit

|2370{{±|30}}

|

|5626

|

Kepler-273c

|

|0.177

|8.014927

|0.073

|

|style="background:#FFFF00"|transit

|2370{{±|30}}

|

|5626

|

Kepler-274b

|

|0.137

|11.634788

|0.101

|

|style="background:#FFFF00"|transit

|4510{{±|140}}

|

|6023

|

Kepler-274c

|

|0.164

|33.197861

|0.204

|

|style="background:#FFFF00"|transit

|4510{{±|140}}

|

|6023

|

Kepler-275b

|

|0.209

|10.300682

|0.098

|

|style="background:#FFFF00"|transit

|7000{{±|500}}

|1.24

|6165

|

Kepler-275c

|

|0.302

|16.088134

|0.132

|

|style="background:#FFFF00"|transit

|7000{{±|500}}

|1.24

|6165

|

Kepler-275d

|

|0.297

|35.676062

|0.224

|

|style="background:#FFFF00"|transit

|7000{{±|500}}

|1.24

|6165

|

Kepler-276b

|

|0.256

|14.12841

|0.119

|

|style="background:#FFFF00"|transit

|3850{{±|150}}

|1.1

|6105

|

Kepler-278b

|

|0.363

|30.160546

|0.207

|

|style="background:#FFFF00"|transit

|1460{{±|20}}

|

|4991

|

Kepler-278c

|

|0.32

|51.078775

|0.294

|

|style="background:#FFFF00"|transit

|1460{{±|20}}

|

|4991

|

Kepler-280b

|

|0.129

|2.139542

|0.032

|

|style="background:#FFFF00"|transit

|2600{{±|30}}

|0.91

|5744

|

Kepler-280c

|

|0.179

|4.807091

|0.056

|

|style="background:#FFFF00"|transit

|2600{{±|30}}

|0.91

|5744

|

Kepler-281b

|

|0.252

|14.646008

|0.117

|

|style="background:#FFFF00"|transit

|6000{{±|300}}

|0.98

|5723

|

Kepler-281c

|

|0.474

|36.337373

|0.215

|

|style="background:#FFFF00"|transit

|6000{{±|300}}

|0.98

|5723

|

Kepler-282b

|

|0.09

|9.220524

|0.082

|

|style="background:#FFFF00"|transit

|4530{{±|150}}

|0.97

|5602

|

Kepler-282c

|

|0.107

|13.638723

|0.106

|

|style="background:#FFFF00"|transit

|4530{{±|150}}

|0.97

|5602

|

Kepler-283b

|

|0.19

|11.008151

|0.082

|

|style="background:#FFFF00"|transit

|1540{{±|20}}

|

|4351

|

Kepler-283c

|

|0.162

|92.743711

|0.341

|

|style="background:#FFFF00"|transit

|1540{{±|20}}

|

|4351

|

Kepler-284b

|

|0.2

|12.699149

|0.104

|

|style="background:#FFFF00"|transit

|3460{{±|110}}

|

|5615

|

Kepler-284c

|

|0.233

|37.514456

|0.213

|

|style="background:#FFFF00"|transit

|3460{{±|110}}

|

|5615

|

Kepler-285b

|

|0.12

|2.633867

|0.036

|

|style="background:#FFFF00"|transit

|2750{{±|50}}

|0.85

|5411

|

Kepler-285c

|

|0.1

|6.186676

|0.064

|

|style="background:#FFFF00"|transit

|2750{{±|50}}

|0.85

|5411

|

Kepler-286b

|

|0.111

|1.796302

|0.027

|

|style="background:#FFFF00"|transit

|4100{{±|400}}

|

|5580

|

Kepler-286c

|

|0.122

|3.468095

|0.042

|

|style="background:#FFFF00"|transit

|4100{{±|400}}

|

|5580

|

Kepler-286d

|

|0.119

|5.914323

|0.061

|

|style="background:#FFFF00"|transit

|4100{{±|400}}

|

|5580

|

Kepler-286e

|

|0.158

|29.221289

|0.176

|

|style="background:#FFFF00"|transit

|4100{{±|400}}

|

|5580

|

Kepler-287b

|

|0.208

|20.342199

|0.145

|

|style="background:#FFFF00"|transit

|2790{{±|50}}

|

|5806

|

Kepler-287c

|

|0.291

|44.851896

|0.246

|

|style="background:#FFFF00"|transit

|2790{{±|50}}

|

|5806

|

Kepler-288b

|

|0.149

|6.097326

|0.065

|

|style="background:#FFFF00"|transit

|4030{{±|110}}

|0.89

|5918

|

Kepler-288c

|

|0.254

|19.305772

|0.14

|

|style="background:#FFFF00"|transit

|4030{{±|110}}

|0.89

|5918

|

Kepler-288d

|

|0.238

|56.633742

|0.287

|

|style="background:#FFFF00"|transit

|4030{{±|110}}

|0.89

|5918

|

Kepler-289b

|0.023

|0.192

|34.545

|0.21

|

|style="background:#FFFF00"|transit

|2340{{±|20}}

|1.08

|5990

|

Kepler-289c

|0.42

|1.034

|125.8518

|0.51

|

|style="background:#FFFF00"|transit

|2340{{±|20}}

|1.08

|5990

|

Kepler-289d

|0.013

|0.239

|66.0634

|0.33

|

|style="background:#FFFF00"|transit

|2340{{±|20}}

|1.08

|5990

|?

Kepler-290b

|

|0.201

|14.589347

|0.11

|

|style="background:#FFFF00"|transit

|2310{{±|40}}

|

|5147

|

Kepler-290c

|

|0.241

|36.77031

|0.205

|

|style="background:#FFFF00"|transit

|2310{{±|40}}

|

|5147

|

Kepler-291b

|

|0.193

|3.546511

|0.047

|

|style="background:#FFFF00"|transit

|6100{{±|400}}

|1.03

|6002

|

Kepler-291c

|

|0.168

|5.700786

|0.065

|

|style="background:#FFFF00"|transit

|6100{{±|400}}

|1.03

|6002

|

Kepler-292b

|

|0.118

|2.580827

|0.035

|

|style="background:#FFFF00"|transit

|3540{{±|150}}

|0.88

|5299

|

Kepler-292c

|

|0.131

|3.715335

|0.045

|

|style="background:#FFFF00"|transit

|3540{{±|150}}

|0.88

|5299

|

Kepler-292d

|

|0.199

|7.055679

|0.068

|

|style="background:#FFFF00"|transit

|3540{{±|150}}

|0.88

|5299

|

Kepler-292e

|

|0.238

|11.97901

|0.097

|

|style="background:#FFFF00"|transit

|3540{{±|150}}

|0.88

|5299

|

Kepler-292f

|

|0.21

|20.834237

|0.141

|

|style="background:#FFFF00"|transit

|3540{{±|150}}

|0.88

|5299

|

Kepler-293b

|

|0.274

|19.254196

|0.144

|

|style="background:#FFFF00"|transit

|3260{{±|70}}

|1.01

|5804

|

Kepler-293c

|

|0.342

|54.155743

|0.286

|

|style="background:#FFFF00"|transit

|3260{{±|70}}

|1.01

|5804

|

Kepler-294b

|

|0.158

|3.701212

|0.048

|

|style="background:#FFFF00"|transit

|4600{{±|200}}

|

|5913

|

Kepler-294c

|

|0.242

|6.6264

|0.071

|

|style="background:#FFFF00"|transit

|4600{{±|200}}

|

|5913

|

Kepler-295b

|

|0.109

|12.645164

|0.099

|

|style="background:#FFFF00"|transit

|5800{{±|300}}

|

|5603

|

Kepler-295c

|

|0.104

|21.526258

|0.142

|

|style="background:#FFFF00"|transit

|5800{{±|300}}

|

|5603

|

Kepler-295d

|

|0.121

|33.884054

|0.192

|

|style="background:#FFFF00"|transit

|5800{{±|300}}

|

|5603

|

Kepler-296b

|

|0.144

|10.864384

|0.079

|

|style="background:#FFFF00"|transit

|740

|0.5

|3740

|

Kepler-296c

|

|0.178

|5.8416366

|0.0521

|

|style="background:#FFFF00"|transit

|740

|0.5

|3740

|

Kepler-296d

|

|0.186

|19.850291

|0.118

|

|style="background:#FFFF00"|transit

|740

|0.5

|3740

|

Kepler-296e

|

|0.136

|34.14211

|0.169

|

|style="background:#FFFF00"|transit

|740

|0.5

|3740

|

Kepler-296f

|

|0.161

|63.33627

|0.255

|

|style="background:#FFFF00"|transit

|740

|0.5

|3740

|

Kepler-297b

|

|0.256

|38.871826

|0.217

|

|style="background:#FFFF00"|transit

|2300{{±|20}}

|

|5619

|

Kepler-297c

|

|0.583

|74.920137

|0.336

|

|style="background:#FFFF00"|transit

|2300{{±|20}}

|

|5619

|

Kepler-298b

|

|0.175

|10.475464

|0.08

|

|style="background:#FFFF00"|transit

|1710{{±|20}}

|0.65

|4465

|

Kepler-298c

|

|0.172

|22.92881

|0.136

|

|style="background:#FFFF00"|transit

|1710{{±|20}}

|0.65

|4465

|

Kepler-298d

|

|0.223

|77.473633

|0.305

|

|style="background:#FFFF00"|transit

|1710{{±|20}}

|0.65

|4465

|

Kepler-299b

|

|0.118

|2.927128

|0.04

|

|style="background:#FFFF00"|transit

|3530{{±|80}}

|0.97

|5617

|

Kepler-299c

|

|0.236

|6.885875

|0.07

|

|style="background:#FFFF00"|transit

|3530{{±|80}}

|0.97

|5617

|

Kepler-299d

|

|0.166

|15.054786

|0.118

|

|style="background:#FFFF00"|transit

|3530{{±|80}}

|0.97

|5617

|

Kepler-299e

|

|0.167

|38.285489

|0.22

|

|style="background:#FFFF00"|transit

|3530{{±|80}}

|0.97

|5617

|

Kepler-300b

|

|0.149

|10.446347

|0.094

|

|style="background:#FFFF00"|transit

|3690{{±|60}}

|0.94

|5986

|

Kepler-300c

|

|0.201

|40.714955

|0.232

|

|style="background:#FFFF00"|transit

|3690{{±|60}}

|0.94

|5986

|

Kepler-301b

|

|0.12

|2.508553

|0.036

|

|style="background:#FFFF00"|transit

|2390{{±|30}}

|0.91

|5815

|

Kepler-301c

|

|0.12

|5.419026

|0.06

|

|style="background:#FFFF00"|transit

|2390{{±|30}}

|0.91

|5815

|

Kepler-301d

|

|0.156

|13.751243

|0.112

|

|style="background:#FFFF00"|transit

|2390{{±|30}}

|0.91

|5815

|

Kepler-302b

|

|0.362

|30.184104

|0.193

|

|style="background:#FFFF00"|transit

|4760{{±|190}}

|

|5740

|

Kepler-302c

|

|1.111

|127.282184

|0.503

|

|style="background:#FFFF00"|transit

|4760{{±|190}}

|

|5740

|

Kepler-303b

|

|0.079

|1.937055

|0.024

|

|style="background:#FFFF00"|transit

|688{{±|3}}

|0.59

|3944

|

Kepler-303c

|

|0.102

|7.061149

|0.057

|

|style="background:#FFFF00"|transit

|688{{±|3}}

|0.59

|3944

|

Kepler-304b

|

|0.255

|3.295709

|0.039

|

|style="background:#FFFF00"|transit

|1435{{±|17}}

|0.8

|4731

|

Kepler-304c

|

|0.194

|5.315946

|0.054

|

|style="background:#FFFF00"|transit

|1435{{±|17}}

|0.8

|4731

|

Kepler-304d

|

|0.245

|9.653471

|0.08

|

|style="background:#FFFF00"|transit

|1435{{±|17}}

|0.8

|4731

|

Kepler-305d

|

|0.242

|16.738661

|0.121

|

|style="background:#FFFF00"|transit

|2900{{±|80}}

|0.76

|5100

|

Kepler-306b

|

|0.136

|4.646186

|0.05

|

|style="background:#FFFF00"|transit

|2580{{±|60}}

|0.82

|4954

|

Kepler-306c

|

|0.21

|7.240193

|0.067

|

|style="background:#FFFF00"|transit

|2580{{±|60}}

|0.82

|4954

|

Kepler-306d

|

|0.22

|17.326644

|0.12

|

|style="background:#FFFF00"|transit

|2580{{±|60}}

|0.82

|4954

|

Kepler-306e

|

|0.203

|44.840975

|0.227

|

|style="background:#FFFF00"|transit

|2580{{±|60}}

|0.82

|4954

|

Kepler-308b

|

|0.189

|9.694928

|0.09

|

|style="background:#FFFF00"|transit

|4500{{±|200}}

|

|5895

|

Kepler-308c

|

|0.193

|15.38231

|0.123

|

|style="background:#FFFF00"|transit

|4500{{±|200}}

|

|5895

|

Kepler-309b

|

|0.139

|5.923653

|0.059

|

|style="background:#FFFF00"|transit

|1804{{±|19}}

|

|4713

|

Kepler-309c

|

|0.224

|105.356383

|0.401

|

|style="background:#FFFF00"|transit

|1804{{±|19}}

|

|4713

|

Kepler-310b

|

|0.106

|13.930698

|0.111

|

|style="background:#FFFF00"|transit

|1990{{±|20}}

|0.85

|5797

|

Kepler-310c

|

|0.302

|56.47542

|0.281

|

|style="background:#FFFF00"|transit

|1990{{±|20}}

|0.85

|5797

|

Kepler-310d

|

|0.22

|92.876125

|0.392

|

|style="background:#FFFF00"|transit

|1990{{±|20}}

|0.85

|5797

|

Kepler-311b

|

|0.152

|9.176092

|0.087

|

|style="background:#FFFF00"|transit

|2590{{±|30}}

|1.06

|5905

|

Kepler-311c

|

|0.128

|19.738286

|0.145

|

|style="background:#FFFF00"|transit

|2590{{±|30}}

|1.06

|5905

|

Kepler-312b

|

|0.115

|1.772419

|0.031

|

|style="background:#FFFF00"|transit

|2660{{±|40}}

|1.23

|6115

|

Kepler-312c

|

|0.281

|19.747412

|0.153

|

|style="background:#FFFF00"|transit

|2660{{±|40}}

|1.23

|6115

|

Kepler-313b

|

|0.226

|14.970418

|0.125

|

|style="background:#FFFF00"|transit

|3500{{±|300}}

|0.9

|5727

|

Kepler-313c

|

|0.229

|32.273273

|0.208

|

|style="background:#FFFF00"|transit

|3500{{±|300}}

|0.9

|5727

|

Kepler-314b

|

|0.074

|2.461069

|0.035

|

|style="background:#FFFF00"|transit

|883{{±|5}}

|1.02

|5378

|

Kepler-314c

|

|0.259

|5.960392

|0.064

|

|style="background:#FFFF00"|transit

|883{{±|5}}

|1.02

|5378

|

Kepler-315b

|

|0.336

|96.101141

|0.402

|

|style="background:#FFFF00"|transit

|3910{{±|120}}

|0.78

|5796

|

Kepler-315c

|

|0.37

|265.469335

|0.791

|

|style="background:#FFFF00"|transit

|3910{{±|120}}

|0.78

|5796

|

Kepler-316b

|

|0.095

|2.240508

|0.027

|

|style="background:#FFFF00"|transit

|1269{{±|12}}

|0.53

|4204

|

Kepler-316c

|

|0.103

|6.827766

|0.058

|

|style="background:#FFFF00"|transit

|1269{{±|12}}

|0.53

|4204

|

Kepler-317b

|

|0.186

|5.524242

|0.061

|

|style="background:#FFFF00"|transit

|3150{{±|80}}

|0.95

|5497

|

Kepler-317c

|

|0.153

|8.77501

|0.083

|

|style="background:#FFFF00"|transit

|3150{{±|80}}

|0.95

|5497

|

Kepler-318b

|

|0.42

|4.662715

|0.056

|

|style="background:#FFFF00"|transit

|1618{{±|10}}

|1.05

|5746

|

Kepler-318c

|

|0.328

|11.815007

|0.105

|

|style="background:#FFFF00"|transit

|1618{{±|10}}

|1.05

|5746

|

Kepler-319b

|

|0.145

|4.362705

|0.051

|

|style="background:#FFFF00"|transit

|1666{{±|15}}

|1.29

|5526

|

Kepler-319c

|

|0.235

|6.941357

|0.069

|

|style="background:#FFFF00"|transit

|1666{{±|15}}

|1.29

|5526

|

Kepler-319d

|

|0.204

|31.781925

|0.191

|

|style="background:#FFFF00"|transit

|1666{{±|15}}

|1.29

|5526

|

Kepler-320b

|

|0.102

|8.371554

|0.085

|

|style="background:#FFFF00"|transit

|2760{{±|30}}

|

|6435

|

Kepler-320c

|

|0.122

|17.934937

|0.142

|

|style="background:#FFFF00"|transit

|2760{{±|30}}

|

|6435

|

Kepler-321b

|

|0.158

|4.915379

|0.057

|

|style="background:#FFFF00"|transit

|1268{{±|11}}

|1.01

|5740

|

Kepler-321c

|

|0.207

|13.093921

|0.11

|

|style="background:#FFFF00"|transit

|1268{{±|11}}

|1.01

|5740

|

Kepler-322b

|

|0.09

|1.653888

|0.027

|

|style="background:#FFFF00"|transit

|1321{{±|8}}

|0.91

|5388

|

Kepler-322c

|

|0.149

|4.337234

|0.051

|

|style="background:#FFFF00"|transit

|1321{{±|8}}

|0.91

|5388

|

Kepler-323b

|

|0.128

|1.678327

|0.028

|

|style="background:#FFFF00"|transit

|1500{{±|20}}

|1.09

|5987

|

Kepler-323c

|

|0.145

|3.553822

|0.046

|

|style="background:#FFFF00"|transit

|1500{{±|20}}

|1.09

|5987

|

Kepler-324b

|

|0.102

|4.385315

|0.05

|

|style="background:#FFFF00"|transit

|1659{{±|12}}

|0.86

|5194

|

Kepler-324c

|

|0.281

|51.805612

|0.26

|

|style="background:#FFFF00"|transit

|1659{{±|12}}

|0.86

|5194

|

Kepler-325b

|

|0.26

|4.544439

|0.053

|

|style="background:#FFFF00"|transit

|2740{{±|40}}

|0.87

|5752

|

Kepler-325c

|

|0.227

|12.762172

|0.105

|

|style="background:#FFFF00"|transit

|2740{{±|40}}

|0.87

|5752

|

Kepler-325d

|

|0.249

|38.715185

|0.22

|

|style="background:#FFFF00"|transit

|2740{{±|40}}

|0.87

|5752

|

Kepler-326b

|

|0.136

|2.248329

|0.032

|

|style="background:#FFFF00"|transit

|1610{{±|30}}

|0.98

|5105

|

Kepler-326c

|

|0.125

|4.580358

|0.051

|

|style="background:#FFFF00"|transit

|1610{{±|30}}

|0.98

|5105

|

Kepler-326d

|

|0.108

|6.766888

|0.066

|

|style="background:#FFFF00"|transit

|1610{{±|30}}

|0.98

|5105

|

Kepler-327b

|

|0.099

|2.549575

|0.029

|

|style="background:#FFFF00"|transit

|794{{±|4}}

|0.55

|3799

|

Kepler-327c

|

|0.092

|5.212333

|0.047

|

|style="background:#FFFF00"|transit

|794{{±|4}}

|0.55

|3799

|

Kepler-327d

|

|0.154

|13.969457

|0.09

|

|style="background:#FFFF00"|transit

|794{{±|4}}

|0.55

|3799

|

Kepler-329b

|

|0.125

|7.416397

|0.061

|

|style="background:#FFFF00"|transit

|1450{{±|20}}

|0.53

|4257

|

Kepler-329c

|

|0.172

|18.684737

|0.113

|

|style="background:#FFFF00"|transit

|1450{{±|20}}

|0.53

|4257

|

Kepler-330b

|

|0.12

|8.25978

|0.075

|

|style="background:#FFFF00"|transit

|2380{{±|40}}

|0.78

|5117

|

Kepler-330c

|

|0.174

|15.955387

|0.116

|

|style="background:#FFFF00"|transit

|2380{{±|40}}

|0.78

|5117

|

Kepler-331b

|

|0.162

|8.457496

|0.065

|

|style="background:#FFFF00"|transit

|1920{{±|40}}

|0.51

|4347

|

Kepler-331c

|

|0.164

|17.28111

|0.105

|

|style="background:#FFFF00"|transit

|1920{{±|40}}

|0.51

|4347

|

Kepler-331d

|

|0.146

|32.134328

|0.159

|

|style="background:#FFFF00"|transit

|1920{{±|40}}

|0.51

|4347

|

Kepler-332b

|

|0.104

|7.626324

|0.07

|

|style="background:#FFFF00"|transit

|1133{{±|5}}

|0.8

|4955

|

Kepler-332c

|

|0.097

|15.995622

|0.114

|

|style="background:#FFFF00"|transit

|1133{{±|5}}

|0.8

|4955

|

Kepler-332d

|

|0.105

|34.21154

|0.189

|

|style="background:#FFFF00"|transit

|1133{{±|5}}

|0.8

|4955

|

Kepler-333b

|

|0.118

|12.551158

|0.087

|

|style="background:#FFFF00"|transit

|1068{{±|7}}

|0.54

|4259

|

Kepler-333c

|

|0.099

|24.08821

|0.135

|

|style="background:#FFFF00"|transit

|1068{{±|7}}

|0.54

|4259

|

Kepler-334b

|

|0.1

|5.470319

|0.061

|

|style="background:#FFFF00"|transit

|1408{{±|14}}

|1

|5828

|

Kepler-334c

|

|0.128

|12.758005

|0.107

|

|style="background:#FFFF00"|transit

|1408{{±|14}}

|1

|5828

|

Kepler-334d

|

|0.126

|25.09849

|0.168

|

|style="background:#FFFF00"|transit

|1408{{±|14}}

|1

|5828

|

Kepler-335b

|

|0.302

|6.562331

|0.075

|

|style="background:#FFFF00"|transit

|4320{{±|100}}

|0.99

|5877

|

Kepler-335c

|

|0.274

|67.844469

|0.356

|

|style="background:#FFFF00"|transit

|4320{{±|100}}

|0.99

|5877

|

Kepler-336b

|

|0.091

|2.024823

|0.033

|

|style="background:#FFFF00"|transit

|8000{{±|7000}}

|0.89

|5867

|

Kepler-336c

|

|0.187

|9.600001

|0.092

|

|style="background:#FFFF00"|transit

|8000{{±|7000}}

|0.89

|5867

|

Kepler-336d

|

|0.211

|20.678772

|0.154

|

|style="background:#FFFF00"|transit

|8000{{±|7000}}

|0.89

|5867

|

Kepler-337b

|

|0.137

|3.292781

|0.045

|

|style="background:#FFFF00"|transit

|2250{{±|30}}

|0.96

|5684

|

Kepler-337c

|

|0.183

|9.693201

|0.093

|

|style="background:#FFFF00"|transit

|2250{{±|30}}

|0.96

|5684

|

Kepler-338b

|

|0.218

|13.726976

|0.117

|

|style="background:#FFFF00"|transit

|1830{{±|20}}

|1.1

|5923

|

Kepler-338c

|

|0.209

|24.310856

|0.172

|

|style="background:#FFFF00"|transit

|1830{{±|20}}

|1.1

|5923

|

Kepler-338d

|

|0.268

|44.431014

|0.257

|

|style="background:#FFFF00"|transit

|1830{{±|20}}

|1.1

|5923

|

Kepler-338e

|0.027

|0.139

|9.341

|

|

|style="background:#FF7519"|timing

|1830{{±|20}}

|1.1

|5923

|?

Kepler-339b

|

|0.127

|4.977656

|0.055

|

|style="background:#FFFF00"|transit

|2040{{±|30}}

|0.84

|5631

|

Kepler-339c

|

|0.103

|6.988055

|0.069

|

|style="background:#FFFF00"|transit

|2040{{±|30}}

|0.84

|5631

|

Kepler-339d

|

|0.104

|10.558345

|0.091

|

|style="background:#FFFF00"|transit

|2040{{±|30}}

|0.84

|5631

|

Kepler-340b

|

|0.226

|14.844387

|0.134

|

|style="background:#FFFF00"|transit

|2690{{±|60}}

|2.11

|6620

|

Kepler-340c

|

|0.301

|22.824669

|0.178

|

|style="background:#FFFF00"|transit

|2690{{±|60}}

|2.11

|6620

|

Kepler-341b

|

|0.105

|5.195528

|0.06

|

|style="background:#FFFF00"|transit

|3520{{±|60}}

|0.94

|6012

|

Kepler-341c

|

|0.152

|8.01041

|0.08

|

|style="background:#FFFF00"|transit

|3520{{±|60}}

|0.94

|6012

|

Kepler-341d

|

|0.165

|27.666313

|0.182

|

|style="background:#FFFF00"|transit

|3520{{±|60}}

|0.94

|6012

|

Kepler-341e

|

|0.178

|42.473269

|0.242

|

|style="background:#FFFF00"|transit

|3520{{±|60}}

|0.94

|6012

|

Kepler-342b

|

|0.201

|15.170318

|0.128

|

|style="background:#FFFF00"|transit

|2600{{±|30}}

|1.13

|6175

|

Kepler-342c

|

|0.175

|26.234138

|0.185

|

|style="background:#FFFF00"|transit

|2600{{±|30}}

|1.13

|6175

|

Kepler-342d

|

|0.222

|39.459357

|0.242

|

|style="background:#FFFF00"|transit

|2600{{±|30}}

|1.13

|6175

|

Kepler-343b

|

|0.215

|8.96855

|0.088

|

|style="background:#FFFF00"|transit

|3100{{±|60}}

|1.04

|5807

|

Kepler-343c

|

|0.18

|23.22182

|0.167

|

|style="background:#FFFF00"|transit

|3100{{±|60}}

|1.04

|5807

|

Kepler-344b

|

|0.233

|21.963945

|0.153

|

|style="background:#FFFF00"|transit

|3360{{±|100}}

|0.9

|5774

|

Kepler-344c

|

|0.263

|125.596809

|0.488

|

|style="background:#FFFF00"|transit

|3360{{±|100}}

|0.9

|5774

|

Kepler-345b

|

|0.066

|7.415563

|0.066

|

|style="background:#FFFF00"|transit

|1180{{±|50}}

|0.59

|4504

|

Kepler-345c

|

|0.107

|9.387427

|0.077

|

|style="background:#FFFF00"|transit

|1180{{±|50}}

|0.59

|4504

|

Kepler-346b

|

|0.237

|6.511127

|0.071

|

|style="background:#FFFF00"|transit

|3300{{±|80}}

|0.97

|6033

|

Kepler-346c

|

|0.274

|23.851549

|0.168

|

|style="background:#FFFF00"|transit

|3300{{±|80}}

|0.97

|6033

|

Kepler-347b

|

|0.176

|12.79836

|0.11

|

|style="background:#FFFF00"|transit

|4400{{±|90}}

|1.04

|6088

|

Kepler-347c

|

|0.156

|27.320871

|0.183

|

|style="background:#FFFF00"|transit

|4400{{±|90}}

|1.04

|6088

|

Kepler-348b

|

|0.136

|7.05677

|0.076

|

|style="background:#FFFF00"|transit

|1890{{±|20}}

|1.15

|6177

|

Kepler-348c

|

|0.119

|17.265427

|0.138

|

|style="background:#FFFF00"|transit

|1890{{±|20}}

|1.15

|6177

|

Kepler-349b

|

|0.17

|5.929778

|0.065

|

|style="background:#FFFF00"|transit

|3150{{±|60}}

|0.97

|5956

|

Kepler-349c

|

|0.175

|12.247629

|0.105

|

|style="background:#FFFF00"|transit

|3150{{±|60}}

|0.97

|5956

|

Kepler-350b

|

|0.165

|11.189562

|0.104

|

|style="background:#FFFF00"|transit

|3200{{±|60}}

|1

|6186

|

Kepler-351b

|

|0.273

|37.054919

|0.214

|

|style="background:#FFFF00"|transit

|3640{{±|40}}

|0.89

|5643

|

Kepler-351c

|

|0.285

|57.24809

|0.287

|

|style="background:#FFFF00"|transit

|3640{{±|40}}

|0.89

|5643

|

Kepler-352b

|

|0.077

|10.05537

|0.085

|

|style="background:#FFFF00"|transit

|830{{±|4}}

|0.79

|5212

|

Kepler-352c

|

|0.111

|16.332995

|0.118

|

|style="background:#FFFF00"|transit

|830{{±|4}}

|0.79

|5212

|

Kepler-353b

|

|0.079

|5.795278

|0.051

|

|style="background:#FFFF00"|transit

|1268{{±|16}}

|0.54

|3903

|

Kepler-353c

|

|0.123

|8.410894

|0.065

|

|style="background:#FFFF00"|transit

|1268{{±|16}}

|0.54

|3903

|

Kepler-354b

|

|0.164

|5.47666

|0.054

|

|style="background:#FFFF00"|transit

|1830{{±|20}}

|0.65

|4648

|

Kepler-354c

|

|0.117

|16.934402

|0.115

|

|style="background:#FFFF00"|transit

|1830{{±|20}}

|0.65

|4648

|

Kepler-354d

|

|0.111

|24.209842

|0.146

|

|style="background:#FFFF00"|transit

|1830{{±|20}}

|0.65

|4648

|

Kepler-355b

|

|0.13

|11.03189

|0.102

|

|style="background:#FFFF00"|transit

|4870{{±|160}}

|1.05

|6184

|

Kepler-355c

|

|0.242

|25.762294

|0.179

|

|style="background:#FFFF00"|transit

|4870{{±|160}}

|1.05

|6184

|

Kepler-356b

|

|0.14

|4.612696

|0.057

|

|style="background:#FFFF00"|transit

|2350{{±|30}}

|0.97

|6133

|

Kepler-356c

|

|0.161

|13.121632

|0.115

|

|style="background:#FFFF00"|transit

|2350{{±|30}}

|0.97

|6133

|

Kepler-357b

|

|0.164

|6.475434

|0.063

|

|style="background:#FFFF00"|transit

|2290{{±|40}}

|0.78

|5036

|

Kepler-357c

|

|0.238

|16.85837

|0.12

|

|style="background:#FFFF00"|transit

|2290{{±|40}}

|0.78

|5036

|

Kepler-357d

|

|0.306

|49.499875

|0.246

|

|style="background:#FFFF00"|transit

|2290{{±|40}}

|0.78

|5036

|

Kepler-358b

|

|0.243

|34.060467

|0.21

|

|style="background:#FFFF00"|transit

|3700{{±|130}}

|0.95

|5908

|

Kepler-358c

|

|0.254

|83.488369

|0.381

|

|style="background:#FFFF00"|transit

|3700{{±|130}}

|0.95

|5908

|

Kepler-359b

|

|0.315

|25.563222

|0.178

|

|style="background:#FFFF00"|transit

|4900{{±|300}}

|1.07

|6248

|

Kepler-359c

|

|0.384

|57.68802

|0.307

|

|style="background:#FFFF00"|transit

|4900{{±|300}}

|1.07

|6248

|

Kepler-359d

|

|0.358

|77.095691

|0.372

|

|style="background:#FFFF00"|transit

|4900{{±|300}}

|1.07

|6248

|

Kepler-360b

|

|0.147

|3.289672

|0.044

|

|style="background:#FFFF00"|transit

|2930{{±|50}}

|0.95

|6053

|

Kepler-360c

|

|0.187

|7.186434

|0.075

|

|style="background:#FFFF00"|transit

|2930{{±|50}}

|0.95

|6053

|

Kepler-361b

|

|0.129

|8.486616

|0.086

|

|style="background:#FFFF00"|transit

|3110{{±|50}}

|1.07

|6169

|

Kepler-361c

|

|0.225

|55.188023

|0.3

|

|style="background:#FFFF00"|transit

|3110{{±|50}}

|1.07

|6169

|

Kepler-362b

|

|0.079

|10.327186

|0.087

|

|style="background:#FFFF00"|transit

|3660{{±|180}}

|0.77

|5788

|

Kepler-362c

|

|0.129

|37.866281

|0.207

|

|style="background:#FFFF00"|transit

|3660{{±|180}}

|0.77

|5788

|

Kepler-363b

|

|0.103

|3.614568

|0.048

|

|style="background:#FFFF00"|transit

|2540{{±|20}}

|1.23

|5593

|

Kepler-363c

|

|0.151

|7.542427

|0.079

|

|style="background:#FFFF00"|transit

|2540{{±|20}}

|1.23

|5593

|

Kepler-363d

|

|0.183

|11.932125

|0.107

|

|style="background:#FFFF00"|transit

|2540{{±|20}}

|1.23

|5593

|

Kepler-364b

|

|0.138

|25.745718

|0.178

|

|style="background:#FFFF00"|transit

|2980{{±|30}}

|1.2

|6108

|

Kepler-364c

|

|0.192

|59.980627

|0.312

|

|style="background:#FFFF00"|transit

|2980{{±|30}}

|1.2

|6108

|

Kepler-365b

|

|0.182

|10.664903

|0.098

|

|style="background:#FFFF00"|transit

|2800{{±|200}}

|0.99

|6012

|

Kepler-365c

|

|0.146

|17.784129

|0.137

|

|style="background:#FFFF00"|transit

|2800{{±|200}}

|0.99

|6012

|

Kepler-366b

|

|0.13

|3.281959

|0.045

|

|style="background:#FFFF00"|transit

|6400{{±|400}}

|1.05

|6209

|

Kepler-366c

|

|0.16

|12.51616

|0.11

|

|style="background:#FFFF00"|transit

|6400{{±|400}}

|1.05

|6209

|

Kepler-367b

|

|0.116

|37.815724

|0.201

|

|style="background:#FFFF00"|transit

|616{{±|2}}

|0.75

|4710

|

Kepler-367c

|

|0.107

|53.578637

|0.253

|

|style="background:#FFFF00"|transit

|616{{±|2}}

|0.75

|4710

|

Kepler-368b

|

|0.291

|26.84768

|0.186

|

|style="background:#FFFF00"|transit

|2570{{±|40}}

|0.71

|5502

|

Kepler-368c

|

|0.346

|72.379334

|0.36

|

|style="background:#FFFF00"|transit

|2570{{±|40}}

|0.71

|5502

|

Kepler-369b

|

|0.101

|2.732756

|0.03

|

|style="background:#FFFF00"|transit

|840{{±|120}}

|0.54

|3591

|

Kepler-369c

|

|0.126

|14.871572

|0.094

|

|style="background:#FFFF00"|transit

|840{{±|120}}

|0.54

|3591

|

Kepler-370b

|

|0.142

|4.57953

|0.054

|

|style="background:#FFFF00"|transit

|3930{{±|120}}

|0.94

|5852

|

Kepler-370c

|

|0.17

|19.02293

|0.14

|

|style="background:#FFFF00"|transit

|3930{{±|120}}

|0.94

|5852

|

Kepler-371b

|

|0.169

|34.763278

|0.2

|

|style="background:#FFFF00"|transit

|2710{{±|40}}

|0.94

|5666

|

Kepler-371c

|

|0.159

|67.968015

|0.313

|

|style="background:#FFFF00"|transit

|2710{{±|40}}

|0.94

|5666

|

Kepler-372b

|

|0.121

|6.849692

|0.075

|

|style="background:#FFFF00"|transit

|5090{{±|170}}

|1.15

|6509

|

Kepler-372c

|

|0.186

|20.053763

|0.154

|

|style="background:#FFFF00"|transit

|5090{{±|170}}

|1.15

|6509

|

Kepler-372d

|

|0.151

|30.092568

|0.201

|

|style="background:#FFFF00"|transit

|5090{{±|170}}

|1.15

|6509

|

Kepler-373b

|

|0.121

|5.535309

|0.06

|

|style="background:#FFFF00"|transit

|3670{{±|70}}

|0.87

|5787

|

Kepler-373c

|

|0.111

|16.725948

|0.126

|

|style="background:#FFFF00"|transit

|3670{{±|70}}

|0.87

|5787

|

Kepler-374b

|

|0.092

|1.897806

|0.029

|

|style="background:#FFFF00"|transit

|4280{{±|120}}

|0.84

|5977

|

Kepler-374c

|

|0.098

|3.282807

|0.042

|

|style="background:#FFFF00"|transit

|4280{{±|120}}

|0.84

|5977

|

Kepler-374d

|

|0.117

|5.028219

|0.056

|

|style="background:#FFFF00"|transit

|4280{{±|120}}

|0.84

|5977

|

Kepler-375b

|

|0.129

|12.125934

|0.101

|

|style="background:#FFFF00"|transit

|4180{{±|180}}

|0.89

|5826

|

Kepler-375c

|

|0.236

|19.986326

|0.141

|

|style="background:#FFFF00"|transit

|4180{{±|180}}

|0.89

|5826

|

Kepler-376b

|

|0.095

|4.920199

|0.057

|

|style="background:#FFFF00"|transit

|3090{{±|50}}

|1.05

|5900

|

Kepler-376c

|

|0.16

|14.172327

|0.115

|

|style="background:#FFFF00"|transit

|3090{{±|50}}

|1.05

|5900

|

Kepler-377b

|

|0.124

|12.509529

|0.109

|

|style="background:#FFFF00"|transit

|2750{{±|40}}

|0.88

|5949

|

Kepler-377c

|

|0.184

|27.014976

|0.182

|

|style="background:#FFFF00"|transit

|2750{{±|40}}

|0.88

|5949

|

Kepler-378b

|

|0.067

|16.092361

|0.112

|

|style="background:#FFFF00"|transit

|498.3{{±|1.4}}

|0.96

|4661

|

Kepler-378c

|

|0.062

|28.906009

|0.166

|

|style="background:#FFFF00"|transit

|498.3{{±|1.4}}

|0.96

|4661

|

Kepler-379b

|

|0.148

|20.09838

|0.152

|

|style="background:#FFFF00"|transit

|2430{{±|20}}

|1.08

|6054

|

Kepler-379c

|

|0.204

|62.784697

|0.326

|

|style="background:#FFFF00"|transit

|2430{{±|20}}

|1.08

|6054

|

Kepler-380b

|

|0.106

|3.930821

|0.05

|

|style="background:#FFFF00"|transit

|2710{{±|40}}

|1.05

|6045

|

Kepler-380c

|

|0.113

|7.630004

|0.078

|

|style="background:#FFFF00"|transit

|2710{{±|40}}

|1.05

|6045

|

Kepler-381b

|

|0.088

|5.629021

|0.066

|

|style="background:#FFFF00"|transit

|878{{±|5}}

|1.34

|6152

|

Kepler-381c

|

|0.1

|13.391635

|0.117

|

|style="background:#FFFF00"|transit

|878{{±|5}}

|1.34

|6152

|

Kepler-382b

|

|0.118

|5.262155

|0.055

|

|style="background:#FFFF00"|transit

|3130{{±|60}}

|0.8

|5600

|

Kepler-382c

|

|0.142

|12.162701

|0.097

|

|style="background:#FFFF00"|transit

|3130{{±|60}}

|0.8

|5600

|

Kepler-383b

|

|0.118

|12.904532

|0.095

|

|style="background:#FFFF00"|transit

|1695

|0.67

|4710

|

Kepler-383c

|

|0.111

|31.200751

|0.172

|

|style="background:#FFFF00"|transit

|1695

|0.67

|4710

|

Kepler-384b

|

|0.1

|22.597053

|0.148

|

|style="background:#FFFF00"|transit

|2990{{±|30}}

|0.76

|5577

|

Kepler-384c

|

|0.101

|45.348269

|0.236

|

|style="background:#FFFF00"|transit

|2990{{±|30}}

|0.76

|5577

|

Kepler-385b

|

|0.244

|10.043686

|0.097

|

|style="background:#FFFF00"|transit

|4870{{±|160}}

|1.09

|6326

|

Kepler-385c

|

|0.271

|15.163161

|0.127

|

|style="background:#FFFF00"|transit

|4870{{±|160}}

|1.09

|6326

|

Kepler-386b

|

|0.124

|12.31043

|0.096

|

|style="background:#FFFF00"|transit

|2950{{±|90}}

|0.74

|5178

|

Kepler-386c

|

|0.141

|25.193458

|0.155

|

|style="background:#FFFF00"|transit

|2950{{±|90}}

|0.74

|5178

|

Kepler-387b

|

|0.092

|6.791636

|0.068

|

|style="background:#FFFF00"|transit

|2670{{±|30}}

|1.03

|5774

|

Kepler-387c

|

|0.079

|11.837549

|0.098

|

|style="background:#FFFF00"|transit

|2670{{±|30}}

|1.03

|5774

|

Kepler-388b

|

|0.072

|3.173315

|0.036

|

|style="background:#FFFF00"|transit

|2000{{±|200}}

|0.59

|4498

|

Kepler-388c

|

|0.077

|13.297004

|0.093

|

|style="background:#FFFF00"|transit

|2000{{±|200}}

|0.59

|4498

|

Kepler-389b

|

|0.135

|3.244107

|0.041

|

|style="background:#FFFF00"|transit

|2720{{±|70}}

|0.78

|5376

|

Kepler-389c

|

|0.13

|14.51143

|0.11

|

|style="background:#FFFF00"|transit

|2720{{±|70}}

|0.78

|5376

|

Kepler-390b

|

|0.073

|6.738088

|0.065

|

|style="background:#FFFF00"|transit

|1437{{±|12}}

|0.67

|5166

|

Kepler-390c

|

|0.07

|13.060022

|0.101

|

|style="background:#FFFF00"|transit

|1437{{±|12}}

|0.67

|5166

|

Kepler-391b

|

|0.285

|7.416755

|0.082

|

|style="background:#FFFF00"|transit

|2900{{±|40}}

|1.22

|4940

|

Kepler-391c

|

|0.316

|20.485435

|0.161

|

|style="background:#FFFF00"|transit

|2900{{±|40}}

|1.22

|4940

|

Kepler-392b

|

|0.089

|5.341853

|0.059

|

|style="background:#FFFF00"|transit

|2260{{±|20}}

|1.13

|5938

|

Kepler-392c

|

|0.098

|10.423118

|0.093

|

|style="background:#FFFF00"|transit

|2260{{±|20}}

|1.13

|5938

|

Kepler-393b

|

|0.115

|9.182417

|0.091

|

|style="background:#FFFF00"|transit

|2940{{±|40}}

|1.32

|6189

|

Kepler-393c

|

|0.119

|14.613612

|0.124

|

|style="background:#FFFF00"|transit

|2940{{±|40}}

|1.32

|6189

|

Kepler-394b

|

|0.143

|8.005013

|0.083

|

|style="background:#FFFF00"|transit

|3560{{±|80}}

|1.11

|6402

|

Kepler-394c

|

|0.148

|12.130686

|0.11

|

|style="background:#FFFF00"|transit

|3560{{±|80}}

|1.11

|6402

|

Kepler-395b

|

|0.092

|7.054346

|0.061

|

|style="background:#FFFF00"|transit

|1390{{±|20}}

|0.53

|4262

|

Kepler-395c

|

|0.118

|34.989262

|0.177

|

|style="background:#FFFF00"|transit

|1390{{±|20}}

|0.53

|4262

|Potentially habitable exoplanet

Kepler-397b

|

|0.219

|22.250949

|0.144

|

|style="background:#FFFF00"|transit

|3760

|

|5307

|

Kepler-397c

|

|0.551

|135.498527

|0.48

|

|style="background:#FFFF00"|transit

|3760

|

|5307

|

Kepler-398b

|

|0.083

|4.081423

|0.044

|

|style="background:#FFFF00"|transit

|581.4{{±|1.8}}

|

|4493

|

Kepler-398c

|

|0.09

|11.419412

|0.087

|

|style="background:#FFFF00"|transit

|581.4{{±|1.8}}

|

|4493

|

Kepler-399b

|

|0.086

|14.425281

|0.103

|

|style="background:#FFFF00"|transit

|4400{{±|700}}

|

|5502

|

Kepler-399c

|

|0.128

|26.67569

|0.155

|

|style="background:#FFFF00"|transit

|4400{{±|700}}

|

|5502

|

Kepler-399d

|

|0.169

|58.034616

|0.261

|

|style="background:#FFFF00"|transit

|4400{{±|700}}

|

|5502

|

Kepler-400b

|

|0.147

|9.024389

|0.087

|

|style="background:#FFFF00"|transit

|2340

|

|5886

|

Kepler-400c

|

|0.133

|17.340824

|0.134

|

|style="background:#FFFF00"|transit

|2340

|

|5886

|

Kepler-401b

|

|0.153

|14.383035

|0.122

|

|style="background:#FFFF00"|transit

|3230{{±|50}}

|

|6117

|

Kepler-401c

|

|0.192

|47.318218

|0.269

|

|style="background:#FFFF00"|transit

|3230{{±|50}}

|

|6117

|

Kepler-402b

|

|0.109

|4.028751

|0.051

|

|style="background:#FFFF00"|transit

|2070{{±|20}}

|

|6090

|

Kepler-402c

|

|0.139

|6.124821

|0.068

|

|style="background:#FFFF00"|transit

|2070{{±|20}}

|

|6090

|

Kepler-402d

|

|0.123

|8.921099

|0.087

|

|style="background:#FFFF00"|transit

|2070{{±|20}}

|

|6090

|

Kepler-402e

|

|0.13

|11.242861

|0.102

|

|style="background:#FFFF00"|transit

|2070{{±|20}}

|

|6090

|

Kepler-403b

|

|0.112

|7.031462

|0.076

|

|style="background:#FFFF00"|transit

|2800{{±|50}}

|

|6090

|

Kepler-403c

|

|0.156

|54.280749

|0.297

|

|style="background:#FFFF00"|transit

|2800{{±|50}}

|

|6090

|

Kepler-404b

|

|0.113

|11.829851

|0.102

|

|style="background:#FFFF00"|transit

|2710{{±|40}}

|

|5654

|

Kepler-404c

|

|0.153

|14.751166

|0.118

|

|style="background:#FFFF00"|transit

|2710{{±|40}}

|

|5654

|

Kepler-405b

|

|0.186

|10.613839

|0.095

|

|style="background:#FFFF00"|transit

|3570{{±|140}}

|

|5818

|

Kepler-405c

|

|0.416

|29.726682

|0.188

|

|style="background:#FFFF00"|transit

|3570{{±|140}}

|

|5818

|

Kepler-406b

|0.02

|0.128

|2.42629

|

|

|style="background:#FFFF00"|transit

|1199{{±|11}}

|1.07

|5538

|

Kepler-406c

|0.009

|0.076

|4.62332

|

|

|style="background:#FFFF00"|transit

|1199{{±|11}}

|1.07

|5538

|

Kepler-407b

|

|0.095

|0.66931

|

|

|style="background:#FFFF00"|transit

|1114{{±|8}}

|1

|5476

|

Kepler-407c

|12.6

|

|3000

|

|

|style="background:#00FF00"|radial vel.

|1114{{±|8}}

|1

|5476

|

Kepler-408b

|

|0.073

|2.46502

|

|

|style="background:#FFFF00"|transit

|290.3{{±|0.9}}

|1.08

|6104

|Host star known as HD 176693 or KOI-1612. Reported as 2.1% false positive probable in 2014, but confirmed by 2016.{{citation|arxiv=1601.06052|title=Spin–Orbit Alignment of Exoplanet Systems: Ensemble Analysis Using Asteroseismology|year=2016|doi=10.3847/0004-637X/819/1/85|last1=Campante|first1=T. L.|last2=Lund|first2=M. N.|last3=Kuszlewicz|first3=J. S.|last4=Davies|first4=G. R.|last5=Chaplin|first5=W. J.|last6=Albrecht|first6=S.|last7=Winn|first7=J. N.|last8=Bedding|first8=T. R.|last9=Benomar|first9=O.|last10=Bossini|first10=D.|last11=Handberg|first11=R.|last12=Santos|first12=A. R. G.|last13=Van Eylen|first13=V.|last14=Basu|first14=S.|last15=Christensen-Dalsgaard|first15=J.|last16=Elsworth|first16=Y. P.|last17=Hekker|first17=S.|last18=Hirano|first18=T.|last19=Huber|first19=D.|last20=Karoff|first20=C.|last21=Kjeldsen|first21=H.|last22=Lundkvist|first22=M. S.|last23=North|first23=T. S. H.|last24=Silva Aguirre|first24=V.|last25=Stello|first25=D.|last26=White|first26=T. R.|journal=The Astrophysical Journal|volume=819|issue=1 |page=85|bibcode=2016ApJ...819...85C |s2cid=56307453 |doi-access=free }}

Kepler-409b

|

|0.106

|68.9584

|

|

|style="background:#FFFF00"|transit

|222.8{{±|0.3}}

|0.92

|5460

|Host star known as Gliese 409

Kepler-412b

|0.941

|1.341

|1.7208604

|0.02897

|

|style="background:#FFFF00"|transit

|3650{{±|60}}

|1.17

|5750

|{{Cite web|url=https://www.aanda.org/articles/aa/pdf/2014/04/aa23017-13.pdf |title=SOPHIE velocimetry of Kepler transit candidates XI. Kepler-412 system: probing the properties of a new inflated hot Jupiter|website=www.aanda.org}}

Kepler-413b

|0.211

|0.388

|66.262

|0.3553

|

|style="background:#FFFF00"|transit

|2830{{±|70}}

|0.82

|4700

|{{citation|arxiv=1401.7275|title=Kepler-413B: A Slightly Misaligned, Neptune-Size Transiting Circumbinary Planet|year=2014|doi=10.1088/0004-637X/784/1/14|last1=Kostov|first1=V. B.|last2=McCullough|first2=P. R.|last3=Carter|first3=J. A.|last4=Deleuil|first4=M.|last5=Díaz|first5=R. F.|last6=Fabrycky|first6=D. C.|last7=Hébrard|first7=G.|last8=Hinse|first8=T. C.|last9=Mazeh|first9=T.|last10=Orosz|first10=J. A.|last11=Tsvetanov|first11=Z. I.|last12=Welsh|first12=W. F.|journal=The Astrophysical Journal|volume=784|issue=1 |page=14|bibcode=2014ApJ...784...14K |s2cid=118418065}}

Kepler-414b

|0.011

|0.153

|4.7

|

|

|style="background:#FF7519"|timing

|1364{{±|9}}

|0.89

|

|See [https://iopscience.iop.org/article/10.1088/0004-637X/787/1/80#apj494697t2 Table 2. Planet Nominal Masses] in {{cite journal |doi=10.1088/0004-637X/787/1/80|title=Densities and Eccentricities of 139Keplerplanets from Transit Time Variations |year=2014 |last1=Hadden |first1=Sam |last2=Lithwick |first2=Yoram |journal=The Astrophysical Journal |volume=787 |issue=1 |page=80 |arxiv=1310.7942 |bibcode=2014ApJ...787...80H |s2cid=119097836 }}

Kepler-414c

|0.094

|0.269

|7.171

|

|

|style="background:#FF7519"|timing

|1364{{±|9}}

|0.89

|

|

Kepler-415b

|0.377

|0.108

|4.176

|

|

|style="background:#FF7519"|timing

|1750{{±|30}}

|0.67

|

|

Kepler-415c

|

|

|8.708

|

|

|style="background:#FFFF00"|transit

|1750{{±|30}}

|0.67

|

|?

Kepler-416b

|0.183

|0.221

|6.319

|

|

|style="background:#FF7519"|timing

|2290{{±|30}}

|1

|

|

Kepler-416c

|

|

|12.209

|

|

|style="background:#FFFF00"|transit

|2290{{±|30}}

|1

|

|?

Kepler-417b

|0.035

|0.206

|12.331

|

|

|style="background:#FFFF00"|transit

|3250{{±|150}}

|0.9

|

|

Kepler-417c

|

|

|15.943

|

|

|style="background:#FFFF00"|transit

|3250{{±|150}}

|0.9

|

|?

Kepler-418b

|1.1

|1.2

|86.67856

|

|

|style="background:#FFFF00"|transit

|3360{{±|60}}

|0.98

|5820

|{{citation|arxiv=1405.5354|year=2014|title=Confirmation of an exoplanet using the transit color signature: Kepler-418b, a blended giant planet in a multiplanet system|doi=10.1051/0004-6361/201323175|last1=Tingley|first1=B.|last2=Parviainen|first2=H.|last3=Gandolfi|first3=D.|last4=Deeg|first4=H. J.|last5=Palle|first5=E.|last6=Montañés Rodriguez|first6=P.|last7=Murgas|first7=F.|last8=Alonso|first8=R.|last9=Bruntt|first9=H.|last10=Fridlund|first10=M.|journal=Astronomy & Astrophysics|volume=567|pages=A14|bibcode=2014A&A...567A..14T |s2cid=118668437}}

Kepler-419b

|2.5

|0.96

|69.7546

|0.37

|

|style="background:#FFFF00"|transit

|3390{{±|80}}

|1.39

|6430

|{{citation|arxiv=1405.5229|year=2014|title=Large Eccentricity, Low Mutual Inclination: The Three-Dimensional Architecture of a Hierarchical System of Giant Planets|doi=10.1088/0004-637X/791/2/89|last1=Dawson|first1=Rebekah I.|last2=Johnson|first2=John Asher|last3=Fabrycky|first3=Daniel C.|last4=Foreman-Mackey|first4=Daniel|last5=Murray-Clay|first5=Ruth A.|last6=Buchhave|first6=Lars A.|last7=Cargile|first7=Phillip A.|last8=Clubb|first8=Kelsey I.|last9=Fulton|first9=Benjamin J.|last10=Hebb|first10=Leslie|last11=Howard|first11=Andrew W.|last12=Huber|first12=Daniel|last13=Shporer|first13=Avi|last14=Valenti|first14=Jeff A.|journal=The Astrophysical Journal|volume=791|issue=2|page=89|bibcode=2014ApJ...791...89D |s2cid=29630098}}

Kepler-419c

|7.3

|

|675.47

|1.68

|

|style="background:#FF7519"|timing

|3390{{±|80}}

|1.39

|6430

|

Kepler-420Ab

|1.45

|0.94

|86.647661

|0.382

|511

|style="background:#FFFF00"|transit

|2900

|0.99

|5520

|{{citation|arxiv=1406.6172|year=2014|title=SOPHIE velocimetry of Keplertransit candidates|doi=10.1051/0004-6361/201424158|last1=Santerne|first1=A.|last2=Hébrard|first2=G.|last3=Deleuil|first3=M.|last4=Havel|first4=M.|last5=Correia|first5=A. C. M.|last6=Almenara|first6=J.-M.|last7=Alonso|first7=R.|last8=Arnold|first8=L.|last9=Barros|first9=S. C. C.|last10=Behrend|first10=R.|last11=Bernasconi|first11=L.|last12=Boisse|first12=I.|last13=Bonomo|first13=A. S.|last14=Bouchy|first14=F.|last15=Bruno|first15=G.|last16=Damiani|first16=C.|last17=Díaz|first17=R. F.|last18=Gravallon|first18=D.|last19=Guillot|first19=T.|last20=Labrevoir|first20=O.|last21=Montagnier|first21=G.|last22=Moutou|first22=C.|last23=Rinner|first23=C.|last24=Santos|first24=N. C.|last25=Abe|first25=L.|last26=Audejean|first26=M.|last27=Bendjoya|first27=P.|last28=Gillier|first28=C.|last29=Gregorio|first29=J.|last30=Martinez|first30=P.|journal=Astronomy & Astrophysics|volume=571|pages=A37|s2cid=118582477|display-authors=1}}

Kepler-421b

|

|0.371

|704.1984

|1.219

|

|style="background:#FFFF00"|transit

|1148{{±|6}}

|0.79

|5308

|{{citation|arxiv=1407.4807|year=2014|title=Discovery of a Transiting Planet Near the Snow-Line|doi=10.1088/0004-637X/795/1/25|last1=Kipping|first1=D. M.|last2=Torres|first2=G.|last3=Buchhave|first3=L. A.|last4=Kenyon|first4=S. J.|last5=Henze|first5=C.|last6=Isaacson|first6=H.|last7=Kolbl|first7=R.|last8=Marcy|first8=G. W.|last9=Bryson|first9=S. T.|last10=Stassun|first10=K.|last11=Bastien|first11=F.|journal=The Astrophysical Journal|volume=795|issue=1 |page=25|bibcode=2014ApJ...795...25K |s2cid=119240746}}

Kepler-422b

|0.43

|1.15

|7.8914483

|0.082

|

|style="background:#FFFF00"|transit

|2400{{±|20}}

|1.15

|5972

|

Kepler-423b

|0.595

|1.192

|2.6843285

|0.03585

|1605

|style="background:#FFFF00"|transit

|2520{{±|40}}

|0.85

|5560

|

Kepler-424b

|1.03

|0.89

|3.3118644

|0.044

|

|style="background:#FFFF00"|transit

|2320{{±|30}}

|1.01

|5460

|{{citation|arxiv=1409.8156|year=2014|title=KEPLER-424 b: A "LONELY" HOT JUPITER THAT FOUND a COMPANION|doi=10.1088/0004-637X/795/2/151|last1=Endl|first1=Michael|last2=Caldwell|first2=Douglas A.|last3=Barclay|first3=Thomas|last4=Huber|first4=Daniel|last5=Isaacson|first5=Howard|last6=Buchhave|first6=Lars A.|last7=Brugamyer|first7=Erik|last8=Robertson|first8=Paul|last9=Cochran|first9=William D.|last10=MacQueen|first10=Phillip J.|last11=Havel|first11=Mathieu|last12=Lucas|first12=Phillip|last13=Howell|first13=Steve B.|last14=Fischer|first14=Debra|last15=Quintana|first15=Elisa|last16=Ciardi|first16=David R.|journal=The Astrophysical Journal|volume=795|issue=2|page=151|bibcode=2014ApJ...795..151E |s2cid=1274827}}

Kepler-424c

|6.97

|

|223.3

|0.73

|

|style="background:#00FF00"|radial vel.

|2320{{±|30}}

|1.01

|5460

|

Kepler-425b

|0.25

|0.978

|3.79701816

|0.0464

|1070

|style="background:#FFFF00"|transit

|2140{{±|30}}

|0.93

|5170

|{{citation|arxiv=1409.8554|year=2014|title=Characterization of the four new transiting planets KOI-188b, KOI-195b, KOI-192b, and KOI-830b|doi=10.1051/0004-6361/201424268|last1=Hébrard|first1=G.|last2=Santerne|first2=A.|last3=Montagnier|first3=G.|last4=Bruno|first4=G.|last5=Deleuil|first5=M.|last6=Havel|first6=M.|last7=Almenara|first7=J.-M.|last8=Damiani|first8=C.|last9=Barros|first9=S. C. C.|last10=Bonomo|first10=A. S.|last11=Bouchy|first11=F.|last12=Díaz|first12=R. F.|last13=Moutou|first13=C.|journal=Astronomy & Astrophysics|volume=572|pages=A93|bibcode=2014A&A...572A..93H |s2cid=119187433}}

Kepler-426b

|0.34

|1.09

|3.21751883

|0.0414

|1300

|style="background:#FFFF00"|transit

|2810{{±|40}}

|0.91

|5725

|

Kepler-427b

|0.29

|1.23

|10.290994

|0.091

|1100

|style="background:#FFFF00"|transit

|3410{{±|50}}

|0.96

|5800

|

Kepler-428b

|1.27

|1.08

|3.52563254

|0.0433

|1070

|style="background:#FFFF00"|transit

|2280{{±|50}}

|0.87

|5150

|

Kepler-430b

|

|0.29

|35.968

|0.2244

|667

|style="background:#FFFF00"|transit

|3070{{±|50}}

|1.17

|5884

|{{citation|arxiv=1411.3621|title=High-Resolution Multi-Band Imaging for Validation and Characterization of Smallkeplerplanets|year=2014|doi=10.1088/0004-6256/149/2/55 |last1=Everett |first1=Mark E. |last2=Barclay |first2=Thomas |last3=Ciardi |first3=David R. |last4=Horch |first4=Elliott P. |last5=Howell |first5=Steve B. |last6=Crepp |first6=Justin R. |last7=Silva |first7=David R. |journal=The Astronomical Journal |volume=149 |issue=2 |page=55 |s2cid=32515106 }}

Kepler-430c

|

|0.16

|110.979

|0.4757

|458

|style="background:#FFFF00"|transit

|3070{{±|50}}

|1.17

|5884

|

Kepler-431b

|

|0.068

|6.803

|0.0719

|1032

|style="background:#FFFF00"|transit

|1609{{±|15}}

|1.07

|6004

|

Kepler-431c

|

|0.06

|8.703

|0.0847

|951

|style="background:#FFFF00"|transit

|1609{{±|15}}

|1.07

|6004

|

Kepler-431d

|

|0.1

|11.922

|0.1045

|856

|style="background:#FFFF00"|transit

|1609{{±|15}}

|1.07

|6004

|

Kepler-432b

|5.41

|1.145

|52.501129

|0.301

|

|style="background:#FFFF00"|transit

|2830{{±|60}}

|1.32

|4995

|Eccentric orbit{{Cite journal|arxiv=1411.4666|last1= Quinn|first1= Samuel N.|title= Kepler-432: A red giant interacting with one of its two long period giant planets|journal= The Astrophysical Journal|volume= 803|issue= 2|pages= 49|last2= White|first2= Timothy R.|last3= Latham|first3= David W.|last4= Chaplin|first4= William J.|last5= Handberg|first5= Rasmus|last6= Huber|first6= Daniel|last7= Kipping|first7= David M.|last8= Payne|first8= Matthew J.|last9= Jiang|first9= Chen|author10= Victor Silva Aguirre|last11= Stello|first11= Dennis|last12= Sliski|first12= David H.|last13= Ciardi|first13= David R.|last14= Buchhave|first14= Lars A.|last15= Bedding|first15= Timothy R.|last16= Davies|first16= Guy R.|last17= Hekker|first17= Saskia|last18= Kjeldsen|first18= Hans|last19= Everett|first19= Mark E.|last20= Howell|first20= Steve B.|last21= Basu|first21= Sarbani|last22= Campante|first22= Tiago L.|last23= Christensen-Dalsgaard|first23= Jørgen|last24= Elsworth|first24= Yvonne P.|last25= Karoff|first25= Christoffer|last26= Kawaler|first26= Steven D.|last27= Lund|first27= Mikkel N.|last28= Lundkvist|first28= Mia|last29= Esquerdo|first29= Gilbert A.|last30= Calkins|first30= Michael L.|display-authors= 29|year= 2014|doi= 10.1088/0004-637X/803/2/49|bibcode = 2015ApJ...803...49Q |s2cid= 28994316}}

Kepler-432c

|2.43{{±|0.22|0.24}}

|

|406.2{{±|3.9|2.5}}

|

|

|style="background:#00FF00"|radial vel.

|2830{{±|60}}

|1.32

|4995

|

Kepler-453b

|0.00063

|0.553

|240.503

|0.7903

|

|style="background:#FFFF00"|transit

|1463{{±|9}}

|0.94

|5527

|{{cite journal | title=KIC 9632895 - The 10th Kepler Transiting Circumbinary Planet | last1=Welsh | first1=William F. | last2=Orosz | first2=Jerome A. | last3=Short | first3=Donald R. | last4=Cochran | first4=William D. | last5=Endl | first5=Michael | last6=Brugamyer | first6=Erik | last7=Haghighipour | first7=Nader | last8=Buchhave | first8=Lars A. | last9=Doyle | first9=Laurance R. | last10=Fabrycky | first10=Daniel C. | last11=Hinse | first11=Tobias Cornelius | last12=Kane | first12=Stephen R. | last13=Kostov | first13=Veselin | last14=Mazeh | first14=Tsevi | last15=Mills | first15=Sean M. | last16=Müller | first16=Tobias W. A. | last17=Quarles | first17=Billy | last18=Quinn | first18=Samuel N. | last19=Ragozzine | first19=Darin | last20=Shporer | first20=Avi | last21=Steffen | first21=Jason H. | last22=Tal-Or | first22=Lev | last23=Torres | first23=Guillermo | last24=Windmiller | first24=Gur | last25=Borucki | first25=William J. | display-authors=1 | journal=The Astrophysical Journal | volume=809 | issue=1 | at=26 | date=2015 | arxiv=1409.1605 | bibcode=2015ApJ...809...26W | doi=10.1088/0004-637X/809/1/26 | s2cid=55158342 }}

Mu Leonis b

|2.4

|

|357.8

|1.1

|

|style="background:#00FF00"|radial vel.

|133.0

|1.5

|4538.2

|{{cite journal | title=Planetary Companions in K giants β Cancri, μ Leonis, and β Ursae Minoris | display-authors=1 | last1=Lee | first1=B.-C. | last2=Han | first2=I. | last3=Park | first3=M.-G. | last4=Mkrtichian | first4=D.E. | last5=Hatzes | first5=A.P. | last6=Kim | first6=K.-M. | journal=Astronomy & Astrophysics | volume=566 | id=A67 | pages=7 | year=2014 | doi=10.1051/0004-6361/201322608 | bibcode=2014A&A...566A..67L | arxiv=1405.2127 | s2cid=118631934 }}

OGLE-2008-BLG-355Lb

|4.6

|

|

|1.7

|

|style="background:#0099FF"|microlensing

|22000

|0.37

|

|{{citation|arxiv=1403.7005|year=2014|title=OGLE-2008-BLG-355Lb: A MASSIVE PLANET AROUND a LATE-TYPE STAR|doi=10.1088/0004-637X/788/2/128|last1=Koshimoto|first1=N.|last2=Udalski|first2=A.|last3=Sumi|first3=T.|last4=Bennett|first4=D. P.|last5=Bond|first5=I. A.|last6=Rattenbury|first6=N.|last7=Abe|first7=Andf.|last8=Botzler|first8=C. S.|last9=Freeman|first9=M.|last10=Fukagawa|first10=M.|last11=Fukui|first11=A.|last12=Furusawa|first12=K.|last13=Itow|first13=Y.|last14=Ling|first14=C. H.|last15=Masuda|first15=K.|last16=Matsubara|first16=Y.|last17=Muraki|first17=Y.|last18=Ohnishi|first18=K.|last19=Saito|first19=To.|last20=Shibai|first20=H.|last21=Sullivan|first21=D. J.|last22=Suzuki|first22=K.|last23=Suzuki|first23=D.|last24=Sweatman|first24=W. L.|last25=Takino|first25=S.|last26=Tristram|first26=P. J.|last27=Wada|first27=K.|last28=Yock|first28=P. C. M.|last29=Szymański|first29=M. K.|last30=Kubiak|first30=M.|journal=The Astrophysical Journal|volume=788|issue=2|page=128|bibcode=2014ApJ...788..128K |s2cid=119194503|display-authors=1}}

OGLE-2008-BLG-92Lb

|0.18

|

|

|18

|

|style="background:#0099FF"|microlensing

|26000

|0.71

|

|{{citation|arxiv=1408.6223|year=2014|title=Triple Microlens Ogle-2008-BLG-092L: Binary Stellar System with a Circumprimary Uranus-Type Planet|doi=10.1088/0004-637X/795/1/42|last1=Poleski|first1=Radosław|last2=Skowron|first2=Jan|last3=Udalski|first3=Andrzej|last4=Han|first4=Cheongho|last5=Kozłowski|first5=Szymon|last6=Wyrzykowski|first6=Łukasz|last7=Dong|first7=Subo|last8=Szymański|first8=Michał K.|last9=Kubiak|first9=Marcin|last10=Pietrzyński|first10=Grzegorz|last11=Soszyński|first11=Igor|last12=Ulaczyk|first12=Krzysztof|last13=Pietrukowicz|first13=Paweł|last14=Gould|first14=Andrew|journal=The Astrophysical Journal|volume=795|issue=1 |page=42|bibcode=2014ApJ...795...42P |s2cid=118678130}}

OGLE-2011-BLG-265Lb

|0.88

|

|

|1.89

|

|style="background:#0099FF"|microlensing

|14300

|0.21

|

|{{citation|arxiv=1410.8252|year=2014|title=OGLE-2011-BLG-0265Lb: A JOVIAN MICROLENSING PLANET ORBITING AN M DWARF|doi=10.1088/0004-637X/804/1/33 |last1=Skowron |first1=J. |last2=Shin |first2=I.-G. |last3=Udalski |first3=A. |last4=Han |first4=C. |last5=Sumi |first5=T. |last6=Shvartzvald |first6=Y. |last7=Gould |first7=A. |last8=Dominis Prester |first8=D. |last9=Street |first9=R. A. |last10=Jørgensen |first10=U. G. |last11=Bennett |first11=D. P. |last12=Bozza |first12=V. |last13=Szymański |first13=M. K. |last14=Kubiak |first14=M. |last15=Pietrzyński |first15=G. |last16=Soszyński |first16=I. |last17=Poleski |first17=R. |last18=Kozłowski |first18=S. |last19=Pietrukowicz |first19=P. |last20=Ulaczyk |first20=K. |last21=Wyrzykowski |first21=Ł. |last22=Abe |first22=F. |last23=Bhattacharya |first23=A. |last24=Bond |first24=I. A. |last25=Botzler |first25=C. S. |last26=Freeman |first26=M. |last27=Fukui |first27=A. |last28=Fukunaga |first28=D. |last29=Itow |first29=Y. |last30=Ling |first30=C. H. |journal=The Astrophysical Journal |volume=804 |page=33 |s2cid=45737293 |display-authors=1 }}

OGLE-2013-BLG-102Lb

|12.569

|

|

|0.8

|

|style="background:#0099FF"|microlensing

|9900

|0.1

|

|Additional planet or brown dwarf in the system.{{citation|arxiv=1407.7926|year=2014|title=Ogle-2013-BLG-0102La,B: Microlensing Binary with Components at Star/Brown Dwarf and Brown Dwarf/Planet Boundaries|doi=10.1088/0004-637X/798/2/123|last1=Jung|first1=Y. K.|last2=Udalski|first2=A.|last3=Sumi|first3=T.|last4=Han|first4=C.|last5=Gould|first5=A.|last6=Skowron|first6=J.|last7=Kozłowski|first7=S.|last8=Poleski|first8=R.|last9=Wyrzykowski|first9=Ł.|last10=Szymański|first10=M. K.|last11=Pietrzyński|first11=G.|last12=Soszyński|first12=I.|last13=Ulaczyk|first13=K.|last14=Pietrukowicz|first14=P.|last15=Mróz|first15=P.|last16=Kubiak|first16=M.|last17=Abe|first17=F.|last18=Bennett|first18=D. P.|last19=Bond|first19=I. A.|last20=Botzler|first20=C. S.|last21=Freeman|first21=M.|last22=Fukui|first22=A.|last23=Fukunaga|first23=D.|last24=Itow|first24=Y.|last25=Koshimoto|first25=N.|last26=Larsen|first26=P.|last27=Ling|first27=C. H.|last28=Masuda|first28=K.|last29=Matsubara|first29=Y.|last30=Muraki|first30=Y.|journal=The Astrophysical Journal|volume=798|issue=2|page=123|s2cid=119250588|display-authors=1}}

OGLE-2013-BLG-341LBb

|0.0073

|

|

|0.883

|

|style="background:#0099FF"|microlensing

|3790

|0.15

|

|One more red dwarf in the system.{{citation|arxiv=1407.1115|year=2014|title=A terrestrial planet in a ~1-AU orbit around one member of a ~15-AU binary|doi=10.1126/science.1251527|last1=Gould|first1=A.|last2=Udalski|first2=A.|last3=Shin|first3=I.-G.|last4=Porritt|first4=I.|last5=Skowron|first5=J.|last6=Han|first6=C.|last7=Yee|first7=J. C.|last8=Kozłowski|first8=S.|last9=Choi|first9=J.-Y.|last10=Poleski|first10=R.|last11=Wyrzykowski|first11=Ł.|last12=Ulaczyk|first12=K.|last13=Pietrukowicz|first13=P.|last14=Mróz|first14=P.|last15=Szymański|first15=M. K.|last16=Kubiak|first16=M.|last17=Soszyński|first17=I.|last18=Pietrzyński|first18=G.|last19=Gaudi|first19=B. S.|last20=Christie|first20=G. W.|last21=Drummond|first21=J.|last22=McCormick|first22=J.|last23=Natusch|first23=T.|last24=Ngan|first24=H.|last25=Tan|first25=T.-G.|last26=Albrow|first26=M.|last27=Depoy|first27=D. L.|last28=Hwang|first28=K.-H.|last29=Jung|first29=Y. K.|last30=Lee|first30=C.-U.|journal=Science|volume=345|issue=6192|pages=46–49|pmid=24994642|bibcode=2014Sci...345...46G |s2cid=206555598|display-authors=1}}

OGLE-2014-BLG-0124Lb

|0.51

|

|

|3.11

|

|style="background:#0099FF"|microlensing

|13000

|0.71

|

|{{citation|arxiv=1410.4219|year=2014|title=Spitzeras a Microlens Parallax Satellite: Mass Measurement for the Ogle-2014-BLG-0124L Planet and ITS Host Star|doi=10.1088/0004-637X/799/2/237 |last1=Udalski |first1=A. |last2=Yee |first2=J. C. |last3=Gould |first3=A. |last4=Carey |first4=S. |last5=Zhu |first5=W. |last6=Skowron |first6=J. |last7=Kozłowski |first7=S. |last8=Poleski |first8=R. |last9=Pietrukowicz |first9=P. |last10=Pietrzyński |first10=G. |last11=Szymański |first11=M. K. |last12=Mróz |first12=P. |last13=Soszyński |first13=I. |last14=Ulaczyk |first14=K. |last15=Wyrzykowski |first15=Ł. |last16=Han |first16=C. |last17=Calchi Novati |first17=S. |last18=Pogge |first18=R. W. |journal=The Astrophysical Journal |volume=799 |issue=2 |page=237 |s2cid=30683835 }}

SAND364 b

|1.54

|

|121.71

|

|

|style="background:#00FF00"|radial vel.

|2730{{±|130}}

|1.35

|4284

|Belongs to Messier 67, also known as BD+12 1917b

TYC 1422-614-1 b

|2.5

|

|198.4

|0.69

|

|style="background:#00FF00"|radial vel.

|2480

|1.15

|4806

|{{citation|arxiv=1410.5971|year=2014|title=Tracking Advanced Planetary Systems (TAPAS) with HARPS-N|doi=10.1051/0004-6361/201424399|last1=Niedzielski|first1=A.|last2=Villaver|first2=E.|last3=Wolszczan|first3=A.|last4=Adamów|first4=M.|last5=Kowalik|first5=K.|last6=MacIejewski|first6=G.|last7=Nowak|first7=G.|last8=García-Hernández|first8=D. A.|last9=Deka|first9=B.|last10=Adamczyk|first10=M.|journal=Astronomy & Astrophysics|volume=573|pages=A36|s2cid=53531092}}

TYC 1422-614-1 c

|10

|

|559.3

|1.37

|

|style="background:#00FF00"|radial vel.

|2480

|1.15

|4806

|

WASP-20 A b

|0.72{{±|0,06}}

|1.32{{±|0.03}}

|3.16158

|0.04317

|

|style="background:#FFFF00"|transit

|663.39

|1.05

|5990

|Binary with planet orbiting primary star{{cite journal|arxiv=1402.1482|doi=10.1051/0004-6361/201423591|title=WASP-20b and WASP-28b: A hot Saturn and a hot Jupiter in near-aligned orbits around solar-type stars|year=2015|last1=Anderson|first1=D. R.|last2=Collier Cameron|first2=A.|last3=Hellier|first3=C.|last4=Lendl|first4=M.|last5=Lister|first5=T. A.|last6=Maxted|first6=P. F. L.|last7=Queloz|first7=D.|last8=Smalley|first8=B.|last9=Smith|first9=A. M. S.|last10=Triaud|first10=A. H. M. J.|last11=Brown|first11=D. J. A.|last12=Gillon|first12=M.|last13=Neveu-Vanmalle|first13=M.|last14=Pepe|first14=F.|last15=Pollacco|first15=D.|last16=Ségransan|first16=D.|last17=Udry|first17=S.|last18=West|first18=R. G.|last19=Wheatley|first19=P. J.|s2cid=119211951|journal=Astronomy & Astrophysics|volume=575|pages=A61|bibcode=2015A&A...575A..61A}}{{cite journal|arxiv=1611.08735|doi=10.3847/2041-8213/833/2/L19|title=Wasp-20 is a Close Visual Binary with a Transiting Hot Jupiter|year=2016|last1=Evans|first1=Daniel F.|last2=Southworth|first2=John|last3=Smalley|first3=Barry|s2cid=119488567|journal=The Astrophysical Journal|volume=833|issue=2|pages=L19|bibcode=2016ApJ...833L..19E |doi-access=free }}

WASP-74b

|0.95

|1.56

|2.13775

|0.037

|1910

|style="background:#FFFF00"|transit

|390

|1.48

|5970

|

WASP-83b

|0.3

|1.04

|4.971252

|0.059

|1120

|style="background:#FFFF00"|transit

|980

|1.11

|5510

|

WASP-85Ab

|1.265

|1.24

|2.6556777

|0.039

|1452

|style="background:#FFFF00"|transit

|243

|1.09

|6112

|{{citation|arxiv=1412.7761|title=Three transiting planet discoveries from the Wide Angle Search for Planets: WASP-85 A b; WASP-116 b, and WASP-149 b|year=2014|last1=Brown|first1=D. J. A.|last2=Anderson|first2=D. R.|last3=Doyle|first3=A. P.|last4=Maxted|first4=E. GillenP. F. L.|last5=Smalley|first5=B.|last6=McCormac|first6=J.|last7=Almenera|first7=J. M.|last8=Prieto-Arranz|first8=J.|last9=Deleuil|first9=M.|last10=Diaz|first10=R. F.|last11=Foxell|first11=E.|last12=Hebrard|first12=G.|last13=Lendl|first13=M.|last14=Delrez|first14=L.|last15=Gillon|first15=M.|last16=Jehin|first16=E.|last17=Lam|first17=K. W. F.|last18=Triaud|first18=A. H. M. J.|last19=Turner|first19=O. D.|last20=Armstrong|first20=D. J.|last21=Bouchy|first21=F.|last22=Collier Cameron|first22=A.|last23=Pollacco|first23=D.|last24=Faedi|first24=F.|last25=Gomez Maqueo Chew|first25=Y.|last26=Hebb|first26=L.|last27=Hellier|first27=C.|last28=Neveu-VanMalle|first28=M.|last29=Palle|first29=E.|last30=Queloz|first30=D.|display-authors=1}}

WASP-87 b

|2.18{{±|0.15}}

|1.39{{±|0.06}}

|1.6828

|0.0295{{±|0.0008}}

|

|style="background:#FFFF00"|transit

|982{{±|12}}

|1.20{{±|0.09}}

|6450{{±|120}}

|{{citation|arxiv=1410.3449|year=2014|title=Six newly-discovered hot Jupiters transiting F/G stars: WASP-87b, WASP-108b, WASP-109b, WASP-110b, WASP-111b & WASP-112b|last1=Anderson|first1=D. R.|last2=Brown|first2=D. J. A.|last3=Collier Cameron|first3=A.|last4=Delrez|first4=L.|last5=Fumel|first5=A.|last6=Gillon|first6=M.|last7=Hellier|first7=C.|last8=Jehin|first8=E.|last9=Lendl|first9=M.|last10=Maxted|first10=P. F. L.|last11=Neveu-VanMalle|first11=M.|last12=Pepe|first12=F.|last13=Pollacco|first13=D.|last14=Queloz|first14=D.|last15=Rojo|first15=P.|last16=Segransan|first16=D.|last17=Serenelli|first17=A. M.|last18=Smalley|first18=B.|last19=Smith|first19=A. M. S.|last20=Southworth|first20=J.|last21=Triaud|first21=A. H. M. J.|last22=Turner|first22=O. D.|last23=Udry|first23=S.|last24=West|first24=R. G.}} Host star also known as CD-52 4998.

WASP-89b

|5.9

|1.04

|3.3564227

|0.0427

|1120

|style="background:#FFFF00"|transit

|957

|0.92

|5130

|{{citation|arxiv=1410.6358|year=2014|title=Three WASP-South transiting exoplanets: WASP-74b, WASP-83b & WASP-89b|last1=Hellier|first1=Coel|last2=Anderson|first2=D. R.|last3=Collier Cameron|first3=A.|last4=Delrez|first4=L.|last5=Gillon|first5=M.|last6=Jehin|first6=E.|last7=Lendl|first7=M.|last8=Maxted|first8=P. F. L.|last9=Pepe|first9=F.|last10=Pollacco|first10=D.|last11=Queloz|first11=D.|last12=Segransan|first12=D.|last13=Smalley|first13=B.|last14=Smith|first14=A. M. S.|last15=Southworth|first15=J.|last16=Triaud|first16=A. H. M. J.|last17=Turner|first17=O. D.|last18=Udry|first18=S.|last19=West|first19=R. G.|journal=The Astronomical Journal |volume=150 |issue=1 |page=18 |doi=10.1088/0004-6256/150/1/18 |bibcode=2015AJ....150...18H |s2cid=16878578 }}

WASP-94Ab

|0.452

|1.72

|3.9501907

|0.055

|1604

|style="background:#FFFF00"|transit

|590

|1.45

|6153

|{{citation|arxiv=1409.7566|year=2014|title=WASP-94 a and B planets: Hot-Jupiter cousins in a twin-star system|doi=10.1051/0004-6361/201424744|last1=Neveu-Vanmalle|first1=M.|last2=Queloz|first2=D.|last3=Anderson|first3=D. R.|last4=Charbonnel|first4=C.|last5=Collier Cameron|first5=A.|last6=Delrez|first6=L.|last7=Gillon|first7=M.|last8=Hellier|first8=C.|last9=Jehin|first9=E.|last10=Lendl|first10=M.|last11=Maxted|first11=P. F. L.|last12=Pepe|first12=F.|last13=Pollacco|first13=D.|last14=Ségransan|first14=D.|last15=Smalley|first15=B.|last16=Smith|first16=A. M. S.|last17=Southworth|first17=J.|last18=Triaud|first18=A. H. M. J.|last19=Udry|first19=S.|last20=West|first20=R. G.|journal=Astronomy & Astrophysics|volume=572|pages=A49|bibcode=2014A&A...572A..49N |s2cid=53470970}}

WASP-94Bb

|0.618

|

|2.00839

|0.0335

|

|style="background:#00FF00"|radial vel.

|590

|1.24

|6040

|

WASP-103b

|1.49

|1.528

|0.925542

|0.01985

|2508

|style="background:#FFFF00"|transit

|1500

|1.22

|6110

|Planet close to tidal disruption{{citation|arxiv=1401.2784|year=2014|title=WASP-103 b: A new planet at the edge of tidal disruption|doi=10.1051/0004-6361/201323014|last1=Gillon|first1=M.|last2=Anderson|first2=D. R.|last3=Collier-Cameron|first3=A.|last4=Delrez|first4=L.|last5=Hellier|first5=C.|last6=Jehin|first6=E.|last7=Lendl|first7=M.|last8=Maxted|first8=P. F. L.|last9=Pepe|first9=F.|last10=Pollacco|first10=D.|last11=Queloz|first11=D.|last12=Ségransan|first12=D.|last13=Smith|first13=A. M. S.|last14=Smalley|first14=B.|last15=Southworth|first15=J.|last16=Triaud|first16=A. H. M. J.|last17=Udry|first17=S.|last18=Van Grootel|first18=V.|last19=West|first19=R. G.|journal=Astronomy & Astrophysics|volume=562|pages=L3|bibcode=2014A&A...562L...3G |s2cid=53680974}}{{citation|arxiv=1411.2767|year=2014|title=High-precision photometry by telescope defocusing – VII. The ultrashort period planet WASP-103★|doi=10.1093/mnras/stu2394|last1=Southworth|first1=John|last2=Mancini|first2=L.|last3=Ciceri|first3=S.|last4=Budaj|first4=J.|last5=Dominik|first5=M.|last6=Figuera Jaimes|first6=R.|last7=Haugbølle|first7=T.|last8=Jørgensen|first8=U. G.|last9=Popovas|first9=A.|last10=Rabus|first10=M.|last11=Rahvar|first11=S.|last12=von Essen|first12=C.|last13=Schmidt|first13=R. W.|last14=Wertz|first14=O.|last15=Alsubai|first15=K. A.|last16=Bozza|first16=V.|last17=Bramich|first17=D. M.|last18=Calchi Novati|first18=S.|last19=d'Ago|first19=G.|last20=Hinse|first20=T. C.|last21=Henning|first21=Th.|last22=Hundertmark|first22=M.|last23=Juncher|first23=D.|last24=Korhonen|first24=H.|last25=Skottfelt|first25=J.|last26=Snodgrass|first26=C.|last27=Starkey|first27=D.|last28=Surdej|first28=J.|journal=Monthly Notices of the Royal Astronomical Society|volume=447|pages=711–721|doi-access=free }}

WASP-104b

|1.272

|1.137

|1.7554137

|0.02918

|1516

|style="background:#FFFF00"|transit

|470

|1.08

|5475

|{{cite journal | title=WASP-104b and WASP-106b: Two transiting hot Jupiters in 1.75-day and 9.3-day orbits | url=https://www.aanda.org/articles/aa/full_html/2014/10/aa24752-14/aa24752-14.html | last1=Smith | first1=A. M. S. | last2=Anderson | first2=D. R. | last3=Armstrong | first3=D. J. | last4=Barros | first4=S. C. C. | last5=Bonomo | first5=A. S. | last6=Bouchy | first6=F. | last7=Brown | first7=D. J. A. | last8=Collier Cameron | first8=A. | last9=Delrez | first9=L. | last10=Faedi | first10=F. | last11=Gillon | first11=M. | last12=Gómez Maqueo Chew | first12=Y. | last13=Hébrard | first13=G. | last14=Jehin | first14=E. | last15=Lendl | first15=M. | last16=Louden | first16=T. M. | last17=Maxted | first17=P. F. L. | last18=Montagnier | first18=G. | last19=Neveu-Vanmalle | first19=M. | last20=Osborn | first20=H. P. | last21=Pepe | first21=F. | last22=Pollacco | first22=D. | last23=Queloz | first23=D. | last24=Rostron | first24=J. W. | last25=Segransan | first25=D. | last26=Smalley | first26=B. | last27=Triaud | first27=A. H. M. J. | last28=Turner | first28=O. D. | last29=Udry | first29=S. | last30=Walker | first30=S. R. | display-authors=1 | journal=Astronomy and Astrophysics | volume=570 | at=A64 | year=2014 | arxiv=1408.0887 | bibcode=2014A&A...570A..64S | doi=10.1051/0004-6361/201424752 | s2cid=119245284 }}

WASP-106b

|1.925

|1.085

|9.289715

|0.0917

|1140

|style="background:#FFFF00"|transit

|920

|1.19

|6055

|

WASP-108 b

|1.167{{±|0.092|0.091}}

|1.215{{±|0.040}}

|2.6755463{{±|0.0000021}}

|0.0397{{±|0.001}}

|1590

|style="background:#FFFF00"|transit

|717.6{{±|0.3}}

|1.167{{±|0.092}}

|6000{{±|140}}

| Host star also known as TYC 8254-1624-1

WASP-109 b

|0.91{{±|0.13}}

|1.443{{±|0.053}}

|3.3190233{{±|0.0000042}}

|0.0463{{±|0.0011}}

|1695

|style="background:#FFFF00"|transit

|1173{{±|16}}

|1.203{{±|0.090}}

|6520{{±|140}}

| Host star also known as TYC 6184-1397-1

WASP-110 b

|0.515{{±|0.064}}

|1.238{{±|0.056}}

|3.7783977{{±|0.0000031}}

|0.0457{{±|0.0012}}

|1134

|style="background:#FFFF00"|transit

|904{{±|10}}

|0.892{{±|0.072}}

|5400{{±|140}}

|

WASP-111 b

|1.85{{±|0.16}}

|1.442{{±|0.094}}

|2.310965{{±|0.0000034}}

|0.03914{{±|0.00098}}

|2140

|style="background:#FFFF00"|transit

|980{{±|20}}

|1.50{{±|0.11}}

|6400{{±|150}}

| Host star also known as HD 208180

WASP-112 b

|0.88{{±|0.12}}

|1.191{{±|0.049}}

|3.0353992{{±|0.0000038}}

|0.0382{{±|0.0011}}

|1395

|style="background:#FFFF00"|transit

|1900{{±|40}}

|0.807{{±|0.073}}

|5610{{±|130}}

|

WASP-116b

|0.59{{±|0.05}}

|1.43{{±|0.07}}

|6.61321{{±|0.00002}}

|0.0730{{±|0.0011}}

|1400{{±|4}}

|style="background:#FFFF00"|transit

|1770{{±|60}}

|1.25{{±|0.18}}

|5950{{±|100}}

|

WASP-117b

|0.2755

|1.021

|10.02165

|0.09459

|1024

|style="background:#FFFF00"|transit

|518{{±|2}}

|1.13

|6038

|{{cite journal|arxiv=1406.6942|doi=10.1051/0004-6361/201424481|title=WASP-117b: A 10-day-period Saturn in an eccentric and misaligned orbit|year=2014|last1=Lendl|first1=M.|last2=Triaud|first2=A. H. M. J.|last3=Anderson|first3=D. R.|last4=Collier Cameron|first4=A.|last5=Delrez|first5=L.|last6=Doyle|first6=A. P.|last7=Gillon|first7=M.|last8=Hellier|first8=C.|last9=Jehin|first9=E.|last10=Maxted|first10=P. F. L.|last11=Neveu-Vanmalle|first11=M.|last12=Pepe|first12=F.|last13=Pollacco|first13=D.|last14=Queloz|first14=D.|last15=Ségransan|first15=D.|last16=Smalley|first16=B.|last17=Smith|first17=A. M. S.|last18=Udry|first18=S.|last19=Van Grootel|first19=V.|last20=West|first20=R. G.|s2cid=54605901|journal=Astronomy & Astrophysics|volume=568|pages=A81|bibcode=2014A&A...568A..81L}}{{cite journal|arxiv=2006.05382|last1=Carone|first1=Ludmila|last2=Mollière|first2=Paul|last3=Zhou|first3=Yifan|last4=Bouwman|first4=Jeroen|last5=Yan|first5=Fei|last6=Baeyens|first6=Robin|last7=Apai|first7=Dániel|last8=Espinoza|first8=Nestor|last9=Rackham|first9=Benjamin V.|last10=Jordán|first10=Andrés|last11=Angerhausen|first11=Daniel|last12=Decin|first12=Leen|last13=Lendl|first13=Monika|last14=Venot|first14=Olivia|last15=Henning|first15=Thomas|title=Indications for very high metallicity and absence of methane in the eccentric exo-Saturn WASP-117b|journal=Astronomy & Astrophysics|year=2021|volume=646|pages=A168|doi=10.1051/0004-6361/202038620|bibcode=2021A&A...646A.168C |s2cid=219559116}}

WASP-149b

|1.02{{±|0.04}}

|1.32{{±|0.04}}

|1.332811{{±|0.000001}}

|0.0247{{±|0.0004}}

|1870{{±|1}}

|style="background:#FFFF00"|transit

|1770{{±|60}}

|1.12{{±|0.17}}

|5750{{±|100}}

|

XO-2Sb

|0.259

|

|18.157

|0.1344

|

|style="background:#00FF00"|radial vel.

|480

|0.98

|5399

|{{citation|arxiv=1407.0251|year=2014|title=The GAPS programme with HARPS-N at TNG|doi=10.1051/0004-6361/201424339|last1=Desidera|first1=S.|last2=Bonomo|first2=A. S.|last3=Claudi|first3=R. U.|last4=Damasso|first4=M.|last5=Biazzo|first5=K.|last6=Sozzetti|first6=A.|last7=Marzari|first7=F.|last8=Benatti|first8=S.|last9=Gandolfi|first9=D.|last10=Gratton|first10=R.|last11=Lanza|first11=A. F.|last12=Nascimbeni|first12=V.|last13=Andreuzzi|first13=G.|last14=Affer|first14=L.|last15=Barbieri|first15=M.|last16=Bedin|first16=L. R.|last17=Bignamini|first17=A.|last18=Bonavita|first18=M.|last19=Borsa|first19=F.|last20=Calcidese|first20=P.|last21=Christille|first21=J. M.|last22=Cosentino|first22=R.|last23=Covino|first23=E.|last24=Esposito|first24=M.|last25=Giacobbe|first25=P.|last26=Harutyunyan|first26=A.|last27=Latham|first27=D.|last28=Lattanzi|first28=M.|last29=Leto|first29=G.|last30=Lodato|first30=G.|journal=Astronomy & Astrophysics|volume=567|pages=L6|s2cid=118567085|display-authors=1}}

XO-2Sc

|1.37

|

|120.8

|0.4756

|

|style="background:#00FF00"|radial vel.

|480

|0.98

|5399

|

YBP 1194 b

|0.32

|

|6.959

|

|

|style="background:#00FF00"|radial vel.

|2920{{±|100}}

|1.01

|5780

|Belongs to Messier 67

YBP 1514 b

|0.4

|

|5.118

|

|

|style="background:#00FF00"|radial vel.

|3060{{±|100}}

|0.96

|5725

|Belongs to Messier 67{{citation|arxiv=1401.4905|year=2014|title=Three planetary companions around M 67 stars|doi=10.1051/0004-6361/201322584|last1=Brucalassi|first1=A.|last2=Pasquini|first2=L.|last3=Saglia|first3=R.|last4=Ruiz|first4=M. T.|last5=Bonifacio|first5=P.|last6=Bedin|first6=L. R.|last7=Biazzo|first7=K.|last8=Melo|first8=C.|last9=Lovis|first9=C.|last10=Randich|first10=S.|journal=Astronomy & Astrophysics|volume=561|pages=L9|bibcode=2014A&A...561L...9B |s2cid=36895080}}

Specific exoplanet lists

{{#section:List of exoplanets|fullList}}

References

{{reflist}}

{{Exoplanet}}

2014

*

exoplanets