List of exoplanets discovered in 2016#Kepler-705b

{{Short description|None}}

This is a list of exoplanets discovered in 2016. As of 2024, 2016 was the year with the most discoveries of exoplanets.

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

List

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

2MASS J22362452+4751425 b

|12.5

|

|

|230

|

|style="background:#FF6CDA"|imaging

|240

|0.6

|4045

|member of AB Doradus moving group{{citation|arxiv=1611.00364|year=2016|title=Planets Around Low-Mass Stars (Palms). Vi. Discovery of a Remarkably Red Planetary-Mass Companion to the Ab Dor Moving Group Candidate 2Mass J22362452+4751425|doi=10.3847/1538-3881/153/1/18|last1=Bowler|first1=Brendan P.|last2=Liu|first2=Michael C.|last3=Mawet|first3=Dimitri|last4=Ngo|first4=Henry|last5=Malo|first5=Lison|last6=Mace|first6=Gregory N.|last7=McLane|first7=Jacob N.|last8=Lu|first8=Jessica R.|last9=Tristan|first9=Isaiah I.|last10=Hinkley|first10=Sasha|last11=Hillenbrand|first11=Lynne A.|last12=Shkolnik|first12=Evgenya L.|last13=Benneke|first13=Björn|last14=Best|first14=William M. J.|journal=The Astronomical Journal|volume=153|page=18|s2cid=3165698 |doi-access=free |bibcode=2017AJ....153...18B }}

BD+15 2375 b

|1.061

|

|153.22

|0.576

|

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

|2520

|1.08

|4649

|{{citation|arxiv=1601.06832|year=2016|title=Tracking Advanced Planetary Systems (TAPAS) with HARPS-N. III. HD 5583 and BD+15 2375 - two cool giants with warm companions|bibcode=2016A&A...588A..62N|last1=Niedzielski|first1=A.|last2=Villaver|first2=E.|last3=Nowak|first3=G.|last4=Adamów|first4=M.|last5=Kowalik|first5=K.|last6=Wolszczan|first6=A.|last7=Deka-Szymankiewicz|first7=B.|last8=Adamczyk|first8=M.|last9=MacIejewski|first9=G.|journal=Astronomy and Astrophysics|volume=588|pages=A62|doi=10.1051/0004-6361/201527869|s2cid=118724053}}

BD+20 594 b

|0.05129

|0.199

|41.6855

|0.241

|386

|style="background:#FFFF00"|transit

|496

|0.96

|5766

|Unusually high density planet{{Cite journal |arxiv = 1601.07608|bibcode = 2016ApJ...830...43E|title = Discovery and Validation of a High-Density sub-Neptune from the K2 Mission|journal = The Astrophysical Journal|volume = 830|issue = 1|pages = 43|last1 = Espinoza|first1 = Néstor|last2 = Brahm|first2 = Rafael|last3 = Jordán|first3 = Andrés|last4 = Jenkins|first4 = James S|last5 = Rojas|first5 = Felipe|last6 = Jofré|first6 = Paula|last7 = Mädler|first7 = Thomas|last8 = Rabus|first8 = Markus|last9 = Chanamé|first9 = Julio|last10 = Pantoja|first10 = Blake|last11 = Soto|first11 = Maritza G|last12 = Morzinski|first12 = Katie M|last13 = Males|first13 = Jared R|last14 = Ward-Duong|first14 = Kimberly|last15 = Close|first15 = Laird M|year = 2016|doi = 10.3847/0004-637X/830/1/43|s2cid = 119118301 | doi-access=free }}

EPIC 211901114 b

|<5

|0.9±0.5

|1.6489±0.0001

|0.0211±0.0003

|

|style="background:#FFFF00"|transit

|592±20

|0.46±0.02

|3440±65

|2% false positive probability,{{citation|arxiv=1609.00726|year=2016|bibcode=2017AJ....153...64M|last1=Mann|first1=Andrew W.|last2=Gaidos|first2=Eric|last3=Vanderburg|first3=Andrew|last4=Rizzuto|first4=Aaron C.|last5=Ansdell|first5=Megan|last6=Medina|first6=Jennifer Vanessa|last7=Mace|first7=Gregory N.|last8=Kraus|first8=Adam L.|last9=Sokal|first9=Kimberly R.|title=Zodiacal Exoplanets in Time (Zeit). Iv. Seven Transiting Planets in the Praesepe Cluster|journal=The Astronomical Journal|volume=153|issue=2|page=64|doi=10.1088/1361-6528/aa5276|s2cid=119260879}} host star also known as CK Cancri

Gliese 536 b

|0.01686

|

|8.7076

|0.06661

|

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

|32.7

|0.52

|3685

|{{cite journal | title=A super-Earth orbiting the nearby M dwarf GJ 536 | url=https://www.aanda.org/articles/aa/full_html/2017/01/aa29291-16/aa29291-16.html | last1=Suárez Mascareño | first1=A. | last2=González Hernández | first2=J. I. | last3=Rebolo | first3=R. | last4=Astudillo-Defru | first4=N. | last5=Bonfils | first5=X. | last6=Bouchy | first6=F. | last7=Delfosse | first7=X. | last8=Forveille | first8=T. | last9=Lovis | first9=C. | last10=Mayor | first10=M. | last11=Murgas | first11=F. | last12=Pepe | first12=F. | last13=Santos | first13=N. C. | last14=Udry | first14=S. | last15=Wünsche | first15=A. | last16=Velasco | first16=S. | display-authors=1 | journal=Astronomy and Astrophysics | volume=597 | at=A108 | year=2017 | arxiv=1611.02122 | bibcode=2017A&A...597A.108S | doi=10.1051/0004-6361/201629291 | s2cid=15249240 }}

Gliese 676 Ac

|6.8

|

|7337

|6.6

|

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

|55

|0.71

|

|{{citation|arxiv=1608.00918|year=2016|title=The mass of planet GJ 676A b from ground-based astrometry A planetary system with two mature gas giants suitable for direct imaging|bibcode=2016A&A...595A..77S|last1=Sahlmann|first1=J.|last2=Lazorenko|first2=P. F.|last3=Ségransan|first3=D.|last4=Astudillo-Defru|first4=N.|last5=Bonfils|first5=X.|last6=Delfosse|first6=X.|last7=Forveille|first7=T.|last8=Hagelberg|first8=J.|last9=Lo Curto|first9=G.|last10=Pepe|first10=F.|last11=Queloz|first11=D.|last12=Udry|first12=S.|last13=Zimmerman|first13=N. T.|journal=Astronomy and Astrophysics|volume=595|page=595|doi=10.1051/0004-6361/201628854|s2cid=118480445}}

Gliese 3998 b

|0.00777

|

|2.64977

|0.029

|740

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

|58.0

|0.5

|3722

|{{citation|arxiv=1607.03632|year=2016|title=HADES RV program with HARPS-N at the TNG GJ 3998: An early M-dwarf hosting a system of super-Earths|doi=10.1051/0004-6361/201628690|last1=Affer|first1=L.|last2=Micela|first2=G.|last3=Damasso|first3=M.|last4=Perger|first4=M.|last5=Ribas|first5=I.|last6=Suárez Mascareño|first6=A.|last7=González Hernández|first7=J. I.|last8=Rebolo|first8=R.|last9=Poretti|first9=E.|last10=Maldonado|first10=J.|last11=Leto|first11=G.|last12=Pagano|first12=I.|last13=Scandariato|first13=G.|last14=Zanmar Sanchez|first14=R.|last15=Sozzetti|first15=A.|last16=Bonomo|first16=A. S.|last17=Malavolta|first17=L.|last18=Morales|first18=J. C.|last19=Rosich|first19=A.|last20=Bignamini|first20=A.|last21=Gratton|first21=R.|last22=Velasco|first22=S.|last23=Cenadelli|first23=D.|last24=Claudi|first24=R.|last25=Cosentino|first25=R.|last26=Desidera|first26=S.|last27=Giacobbe|first27=P.|last28=Herrero|first28=E.|last29=Lafarga|first29=M.|last30=Lanza|first30=A. F.|journal=Astronomy & Astrophysics|volume=593|pages=A117|bibcode=2016A&A...593A.117A|s2cid=119294882|display-authors=1}}

Gliese 3998 c

|0.0197

|

|13.74

|0.089

|420

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

|58.0

|0.5

|3722

|

HAT-P-65b

|0.527

|1.89

|2.6054552

|0.03951

|1930

|style="background:#FFFF00"|transit

|2740

|1.21

|5835

|{{cite journal |last1=Hartman |first1=J. D. |last2=Bakos |first2=G. Á. |last3=Bhatti |first3=W. |last4=Penev |first4=K. |last5=Bieryla |first5=A. |last6=Latham |first6=D. W. |last7=Kovács |first7=G. |last8=Torres |first8=G. |last9=Csubry |first9=Z. |last10=de Val-Borro |first10=M. |last11=Buchhave |first11=L. |last12=Kovács |first12=T. |last13=Quinn |first13=S. |last14=Howard |first14=A. W. |last15=Isaacson |first15=H. |last16=Fulton |first16=B. J. |last17=Everett |first17=M. E. |last18=Esquerdo |first18=G. |last19=Béky |first19=B. |last20=Szklenar |first20=T. |last21=Falco |first21=E. |last22=Santerne |first22=A. |last23=Boisse |first23=I. |last24=Hébrard |first24=G. |last25=Burrows |first25=A. |last26=Lázár |first26=J. |last27=Papp |first27=I. |last28=Sári |first28=P. |title=HAT-P-65b and HAT-P-66b: Two Transiting Inflated Hot Jupiters and Observational Evidence for the Reinflation of Close-in Giant Planets |journal=The Astronomical Journal |date=1 December 2016 |volume=152 |issue=6 |pages=182 |doi=10.3847/0004-6256/152/6/182 |arxiv=1609.02767 |bibcode=2016AJ....152..182H |s2cid=118546031 |issn=0004-6256 |doi-access=free }}

HAT-P-66b

|0.783

|1.59

|2.972086

|0.04363

|{{val|1896|66|42}}

|style="background:#FFFF00"|transit

|3020

|1.25

|6002

|

HATS-11b

|0.85

|1.51

|3.6191613

|0.04614

|1637

|style="background:#FFFF00"|transit

|2950

|1

|6060

|{{citation|arxiv=1603.02894|year=2016|title=HATS-11b and HATS-12b: Two transiting Hot Jupiters orbiting sub-solar metallicity stars selected for the K2 Campaign 7|bibcode=2016AJ....152...88R|last1=Rabus|first1=M.|last2=Jordán|first2=A.|last3=Hartman|first3=J. D.|last4=Bakos|first4=G. Á.|last5=Espinoza|first5=N.|last6=Brahm|first6=R.|last7=Penev|first7=K.|last8=Ciceri|first8=S.|last9=Zhou|first9=G.|last10=Bayliss|first10=D.|last11=Mancini|first11=L.|last12=Bhatti|first12=W.|last13=De Val-Borro|first13=M.|last14=Csbury|first14=Z.|last15=Sato|first15=B.|last16=Tan|first16=T. -G.|last17=Henning|first17=T.|last18=Schmidt|first18=B.|last19=Bento|first19=J.|last20=Suc|first20=V.|last21=Noyes|first21=R.|last22=Lázár|first22=J.|last23=Papp|first23=I.|last24=Sári|first24=P.|journal=The Astronomical Journal|volume=152|issue=4|page=88|doi=10.3847/0004-6256/152/4/88|s2cid=44027206 |doi-access=free }}

HATS-12b

|2.38

|1.35

|3.142833

|0.04795

|2097

|style="background:#FFFF00"|transit

|3200

|1.49

|6408

|

HATS-18b

|1.98

|1.337

|0.8378434

|0.01761

|2060

|style="background:#FFFF00"|transit

|2100

|1.04

|5600

|{{citation|arxiv=1606.00848|year=2016|title=HATS-18 b: An Extreme Short--Period Massive Transiting Planet Spinning Up Its Star|bibcode=2016AJ....152..127P|last1=Penev|first1=K.|last2=Hartman|first2=J. D.|last3=Bakos|first3=G. Á.|last4=Ciceri|first4=S.|last5=Brahm|first5=R.|last6=Bayliss|first6=D.|last7=Bento|first7=J.|last8=Jordán|first8=A.|last9=Csubry|first9=Z.|last10=Bhatti|first10=W.|last11=De Val-Borro|first11=M.|last12=Espinoza|first12=N.|last13=Zhou|first13=G.|last14=Mancini|first14=L.|last15=Rabus|first15=M.|last16=Suc|first16=V.|last17=Henning|first17=T.|last18=Schmidt|first18=B.|last19=Noyes|first19=R. W.|last20=Lázár|first20=J.|last21=Papp|first21=I.|last22=Sári|first22=P.|journal=The Astronomical Journal|volume=152|issue=5|page=127|doi=10.3847/0004-6256/152/5/127|s2cid=119286902 |doi-access=free }}

HATS-19b

|0.427{{±|0.071}}

|1.66{{±|0.27|0.21}}

|4.569673{{±|0.000010}}

|0.0589{{±|0.0013}}

|1570{{±|110}}

|style="background:#FFFF00"|transit

|1860{{±|30}}

|1.303{{±|0.083}}

|5896{{±|77}}

|{{citation|arxiv=1607.00322|year=2016|title=HATS-19b, HATS-20b, HATS-21b: Three Transiting Hot-Saturns Discovered by the HATSouth Survey|last1=Bhatti|first1=W.|last2=Bakos|first2=G. Á.|last3=Hartman|first3=J. D.|last4=Zhou|first4=G.|last5=Penev|first5=K.|last6=Bayliss|first6=D.|last7=Jordán|first7=A.|last8=Brahm|first8=R.|last9=Espinoza|first9=N.|last10=Rabus|first10=M.|last11=Mancini|first11=L.|last12=De Val-Borro|first12=M.|last13=Bento|first13=J.|last14=Ciceri|first14=S.|last15=Csubry|first15=Z.|last16=Henning|first16=T.|last17=Schmidt|first17=B.|last18=Arriagada|first18=P.|last19=Butler|first19=R. P.|last20=Crane|first20=J.|last21=Shectman|first21=S.|last22=Thompson|first22=I.|last23=Tan|first23=T. G.|last24=Suc|first24=V.|last25=Lázár|first25=J.|last26=Papp|first26=I.|last27=Sári|first27=P.}}

HATS-20b

|0.273{{±|0.035}}

|0.776{{±|0.055}}

|3.7992969{{±|0.0000079}}

|0.04619{{±|0.00044}}

|1147{{±|36}}

|style="background:#FFFF00"|transit

|1610{{±|40}}

|0.910{{±|0.026}}

|5406{{±|49}}

|

HATS-21b

|0.332{{±|0.040|0.030}}

|1.123{{±|0.147|0.054}}

|3.5543973{{±|0.0000058}}

|0.04676{{±|0.00038}}

|1284{{±|55|31}}

|style="background:#FFFF00"|transit

|954{{±|10}}

|1.080{{±|0.026}}

|5695{{±|67}}

|

HATS-22b

|2.74

|0.953

|4.7228124

|0.05025

|858

|style="background:#FFFF00"|transit

|678

|0.76

|4803

|{{citation|arxiv=1607.00688|year=2016|title=HATS-22b, HATS-23b AND HATS-24b: THREE NEW TRANSITING SUPER-JUPITERS FROM THE HATSOUTH PROJECT|bibcode=2017MNRAS.468..835B|last1=Bento|first1=J.|last2=Schmidt|first2=B.|last3=Hartman|first3=J. D.|last4=Bakos|first4=G. Á.|last5=Ciceri|first5=S.|last6=Brahm|first6=R.|last7=Bayliss|first7=D.|last8=Espinoza|first8=N.|last9=Zhou|first9=G.|last10=Rabus|first10=M.|last11=Bhatti|first11=W.|last12=Penev|first12=K.|last13=Csubry|first13=Z.|last14=Jordán|first14=A.|last15=Mancini|first15=L.|last16=Henning|first16=T.|last17=De Val-Borro|first17=M.|last18=Tinney|first18=C. G.|last19=Wright|first19=D. J.|last20=Durkan|first20=S.|last21=Suc|first21=V.|last22=Noyes|first22=R.|last23=Lázár|first23=J.|last24=Papp|first24=I.|last25=Sári|first25=P.|journal=Monthly Notices of the Royal Astronomical Society|volume=468|issue=1|page=835|doi=10.1093/mnras/stx500|doi-access=free }}

HATS-23b

|1.47

|1.86

|2.1605156

|0.03397

|1654

|style="background:#FFFF00"|transit

|2440

|1.12

|5780

|

HATS-24b

|2.44

|1.487

|1.3484954

|0.02547

|2067

|style="background:#FFFF00"|transit

|1700

|1.21

|6346

|

HATS-25b

|0.613

|1.26

|4.2986432

|0.05163

|

|style="background:#FFFF00"|transit

|1520

|0.99

|5715

|{{citation|arxiv=1606.00023|year=2016|title=HATS-25b through HATS-30b: A Half-dozen New Inflated Transiting Hot Jupiters from the HATSouth Survey|bibcode=2016AJ....152..108E|last1=Espinoza|first1=N.|last2=Bayliss|first2=D.|last3=Hartman|first3=J. D.|last4=Bakos|first4=G. Á.|last5=Jordán|first5=A.|last6=Zhou|first6=G.|last7=Mancini|first7=L.|last8=Brahm|first8=R.|last9=Ciceri|first9=S.|last10=Bhatti|first10=W.|last11=Csubry|first11=Z.|last12=Rabus|first12=M.|last13=Penev|first13=K.|last14=Bento|first14=J.|last15=De Val-Borro|first15=M.|last16=Henning|first16=T.|last17=Schmidt|first17=B.|last18=Suc|first18=V.|last19=Wright|first19=D. J.|last20=Tinney|first20=C. G.|last21=Tan|first21=T. G.|last22=Noyes|first22=R.|journal=The Astronomical Journal|volume=152|issue=4|page=108|doi=10.3847/0004-6256/152/4/108|s2cid=119104881 |doi-access=free }}

HATS-26b

|0.65

|1.75

|3.3023881

|0.04735

|

|style="background:#FFFF00"|transit

|2960

|1.3

|6071

|

HATS-27b

|0.53

|1.5

|4.637038

|0.0611

|

|style="background:#FFFF00"|transit

|2700

|1.42

|6438

|

HATS-28b

|0.672

|1.194

|3.1810781

|0.04131

|

|style="background:#FFFF00"|transit

|1700

|0.93

|5498

|

HATS-29b

|0.653

|1.251

|4.6058749

|0.05475

|

|style="background:#FFFF00"|transit

|1140

|1.03

|5670

|

HATS-30b

|0.706

|1.175

|3.1743516

|0.04354

|

|style="background:#FFFF00"|transit

|1110

|1.09

|5943

|

HATS-31b

|0.88

|1.64

|3.37796

|0.0478

|1823

|style="background:#FFFF00"|transit

|2840

|1.27

|6050

|{{citation|arxiv=1607.00006|year=2016|title=HATS-31b Through HATS-35b: Five Transiting Hot Jupiters Discovered by the HATSouth Survey|bibcode=2016AJ....152..161D|last1=De Val-Borro|first1=M.|last2=Bakos|first2=G. Á.|last3=Brahm|first3=R.|last4=Hartman|first4=J. D.|last5=Espinoza|first5=N.|last6=Penev|first6=K.|last7=Ciceri|first7=S.|last8=Jordán|first8=A.|last9=Bhatti|first9=W.|last10=Csubry|first10=Z.|last11=Bayliss|first11=D.|last12=Bento|first12=J.|last13=Zhou|first13=G.|last14=Rabus|first14=M.|last15=Mancini|first15=L.|last16=Henning|first16=T.|last17=Schmidt|first17=B.|last18=Tan|first18=T. G.|last19=Tinney|first19=C. G.|last20=Wright|first20=D. J.|last21=Kedziora-Chudczer|first21=L.|last22=Bailey|first22=J.|last23=Suc|first23=V.|last24=Durkan|first24=S.|last25=Lázár|first25=J.|last26=Papp|first26=I.|last27=Sári|first27=P.|journal=The Astronomical Journal|volume=152|issue=6|page=161|doi=10.3847/0004-6256/152/6/161|s2cid=119283473 |doi-access=free }}

HATS-32b

|0.92

|1.249

|2.8126548

|0.04024

|1437

|style="background:#FFFF00"|transit

|2740

|1.1

|5700

|

HATS-33b

|1.192

|1.23

|2.5495551

|0.03727

|1429

|style="background:#FFFF00"|transit

|830

|1.06

|5659

|

HATS-34b

|0.941

|1.43

|2.1061607

|0.03166

|1445

|style="background:#FFFF00"|transit

|1740

|0.95

|5380

|

HATS-35b

|1.222

|1.464

|1.8209993

|0.03199

|2037

|style="background:#FFFF00"|transit

|1820

|1.32

|6300

|

HD 3167 b

|

|0.139

|0.959628

|

|

|style="background:#FFFF00"|transit

|149

|0.86

|5261

|{{citation | title=Two Small Planets Transiting HD 3167 | display-authors=1 | last1=Vanderburg | first1=Andrew | last2=Bieryla | first2=Allyson | last3=Duev | first3=Dmitry A. | last4=Jensen-Clem |first4=Rebecca | last5=Latham | first5=David W. | last6=Mayo | first6=Andrew W. | last7=Baranec | first7=Christoph| last8=Berlind | first8=Perry | last9=Kulkarni | first9=Shrinivas| last10=Law | first10=Nicholas M. | last11=Nieberding | first11=Megan N.| last12=Riddle | first12=Reed | last13=Salama | first13=Maïssa | journal=The Astrophysical Journal Letters| volume=829 | issue=1 | id=L9 | pages=6 | date=September 2016| doi=10.3847/2041-8205/829/1/L9|bibcode=2016ApJ...829L...9V | arxiv=1607.05248 | s2cid=41001644 | postscript=. | doi-access=free }}

HD 3167 c

|

|0.254

|29.8454

|

|

|style="background:#FFFF00"|transit

|149

|0.86

|5261

|

HD 5583 b

|5.78

|

|139.35

|0.53

|

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

|720

|1.01

|4830

|

{{ill|HD 9174 b|id|HD 9174 b}}

|1.11

|

|1179

|2.2

|

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

|257.4

|1.03

|5577

|{{citation|arxiv=1603.09391|year=2016|title=New planetary systems from the Calan–Hertfordshire Extrasolar Planet Search|doi=10.1093/mnras/stw2811|last1=Jenkins|first1=J. S.|last2=Jones|first2=H. R. A.|last3=Tuomi|first3=M.|last4=Díaz|first4=M.|last5=Cordero|first5=J. P.|last6=Aguayo|first6=A.|last7=Pantoja|first7=B.|last8=Arriagada|first8=P.|last9=Mahu|first9=R.|last10=Brahm|first10=R.|last11=Rojo|first11=P.|last12=Soto|first12=M. G.|last13=Ivanyuk|first13=O.|last14=Becerra Yoma|first14=N.|last15=Day-Jones|first15=A. C.|last16=Ruiz|first16=M. T.|last17=Pavlenko|first17=Y. V.|last18=Barnes|first18=J. R.|last19=Murgas|first19=F.|last20=Pinfield|first20=D. J.|last21=Jones|first21=M. I.|last22=López-Morales|first22=M.|last23=Shectman|first23=S.|last24=Butler|first24=R. P.|last25=Minniti|first25=D.|journal=Monthly Notices of the Royal Astronomical Society|volume=466|pages=443–473|doi-access=free }}

HD 12484 b

|2.98

|

|58.83

|0.297

|

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

|167

|1.01

|5920

|

HD 30177 c

|7.6

|

|11613

|9.89

|

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

|178.4

|0.99

|5580

|{{cite journal | title=The Anglo-Australian Planet Search. XXV. A Candidate Massive Saturn Analog Orbiting HD 30177 | last1=Wittenmyer | first1=Robert A. | last2=Horner | first2=Jonathan | last3=Mengel | first3=M. W. |last4=Butler | first4=R. P. | last5=Wright | first5=D. J. | last6=Tinney | first6=C. G. | last7=Carter | first7=B. D. | last8=Jones | first8=H. R. A. | last9=Anglada-Escudé | first9=G. | last10=Bailey | first10=J. | last11=o'Toole | first11=Simon J. | display-authors=1 | journal=The Astronomical Journal | volume=153 | issue=4 | at=167 | year=2017 | arxiv=1612.02072 | bibcode=2017AJ....153..167W | bibcode-access=free | doi=10.3847/1538-3881/aa5f17 | doi-access=free }}

HD 35759 b

|3.76

|

|82.467

|0.389

|

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

|236

|1.15

|6060

|

{{ill|HD 42618 b|id|HD 42618 b}}

|0.04531

|

|149.61

|0.554

|337

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

|77

|1.01

|5727

|

HD 47366 b

|1.75

|

|363.3

|1.214

|

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

|260

|1.81

|4866

|{{citation|arxiv=1601.04417|year=2016|title=A Pair of Giant Planets Around the Evolved Intermediate-Mass Star Hd 47366: Multiple Circular Orbits or a Mutually Retrograde Configuration|doi=10.3847/0004-637X/819/1/59 |last1=Sato |first1=Bun'ei |last2=Wang |first2=Liang |last3=Liu |first3=Yu-Juan |last4=Zhao |first4=Gang |last5=Omiya |first5=Masashi |last6=Harakawa |first6=Hiroki |last7=Nagasawa |first7=Makiko |last8=Wittenmyer |first8=Robert A. |last9=Butler |first9=Paul |last10=Song |first10=Nan |last11=He |first11=Wei |last12=Zhao |first12=Fei |last13=Kambe |first13=Eiji |last14=Noguchi |first14=Kunio |last15=Ando |first15=Hiroyasu |last16=Izumiura |first16=Hideyuki |last17=Okada |first17=Norio |last18=Yoshida |first18=Michitoshi |last19=Takeda |first19=Yoichi |last20=Itoh |first20=Yoichi |last21=Kokubo |first21=Eiichiro |last22=Ida |first22=Shigeru |journal=The Astrophysical Journal |volume=819 |issue=1 |page=59 |bibcode=2016ApJ...819...59S |s2cid=118535422 |doi-access=free }}

HD 47366 c

|1.86

|

|684.7

|1.853

|

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

|260

|1.81

|4866

|

HD 68402 b

|3.07

|

|1103

|2.18

|

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

|250

|1.12

|5950

|

{{ill|HD 72892 b|id|HD 72892 b}}

|5.45

|

|39.475

|0.228

|

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

|237.4

|1.02

|5688

|

HD 86950 b

|3.6

|

|1270

|2.72

|

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

|550

|1.66

|4805

|{{citation|arxiv=1611.07648|year=2016|title=The Pan-Pacific Planet Search VI: Giant planets orbiting HD 86950 and HD 222076|bibcode=2017AJ....153...51W|last1=Wittenmyer|first1=Robert A.|last2=Jones|first2=M. I.|last3=Zhao|first3=Jinglin|last4=Marshall|first4=J. P.|last5=Butler|first5=R. P.|last6=Tinney|first6=C. G.|last7=Wang|first7=Liang|last8=Johnson|first8=John Asher|journal=The Astronomical Journal|volume=153|issue=2|page=51|doi=10.3847/1538-3881/153/2/51|s2cid=119446216 |doi-access=free }}

{{ill|HD 87646#Planetary system|lt=HD 87646 b|fr|HD 87646#HD 87646 Ab ou MARVELS-7 b : planète ou naine brune ?}}

|12.4

|

|13.481

|0.117

|

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

|240.0

|1.12

|5770

|Also brown dwarf in the system{{citation|arxiv=1608.03597|year=2016|title=Very Low-Mass Stellar and Substellar Companions to Solar-like Stars From MARVELS VI: A Giant Planet and a Brown Dwarf Candidate in a Close Binary System HD 87646|bibcode=2016AJ....152..112M|last1=Ma|first1=Bo|last2=Ge|first2=Jian|last3=Wolszczan|first3=Alex|last4=Muterspaugh|first4=Matthew W.|last5=Lee|first5=Brian|last6=Henry|first6=Gregory W.|last7=Schneider|first7=Donald P.|last8=Martín|first8=Eduardo L.|last9=Niedzielski|first9=Andrzej|last10=Xie|first10=Jiwei|last11=Fleming|first11=Scott W.|last12=Thomas|first12=Neil|last13=Williamson|first13=Michael|last14=Zhu|first14=Zhaohuan|last15=Agol|first15=Eric|last16=Bizyaev|first16=Dmitry|last17=Nicolaci Da Costa|first17=Luiz|last18=Jiang|first18=Peng|last19=Martinez Fiorenzano|first19=A. F.|last20=González Hernández|first20=Jonay I.|last21=Guo|first21=Pengcheng|last22=Grieves|first22=Nolan|last23=Li|first23=Rui|last24=Liu|first24=Jane|last25=Mahadevan|first25=Suvrath|last26=Mazeh|first26=Tsevi|last27=Nguyen|first27=Duy Cuong|last28=Paegert|first28=Martin|last29=Sithajan|first29=Sirinrat|last30=Stassun|first30=Keivan|journal=The Astronomical Journal|volume=152|issue=5|page=112|doi=10.3847/0004-6256/152/5/112|s2cid=118506921|display-authors=1 |doi-access=free }}

HD 95089 c

|3.97{{±|0.33|0.59}}

|

|1860{{±|370|570}}

|

|

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

|42.1{{±|0.59}}

|1.58{{±|0.11}}

|5002{{±|44}}

|

HD 99706 c

|5.69{{±|1.43|0.96}}

|

|1278{{±|151|198}}

|

|

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

|480{{±|4}}

|1.70{{±|0.35}}

|4891{{±|35}}

|{{citation|arxiv=1601.07595|year=2016|doi=10.3847/0004-637X/821/2/89|last1=Bryan|first1=Marta L.|last2=Knutson|first2=Heather A.|last3=Howard|first3=Andrew W.|last4=Ngo|first4=Henry|last5=Batygin|first5=Konstantin|last6=Crepp|first6=Justin R.|last7=Fulton|first7=B. J.|last8=Hinkley|first8=Sasha|last9=Isaacson|first9=Howard|last10=Johnson|first10=John A.|last11=Marcy|first11=Geoffry W.|last12=Wright|first12=Jason T.|title=Statistics of Long Period Gas Giant Planets in Known Planetary Systems|journal=The Astrophysical Journal|volume=821|issue=2|page=89|bibcode=2016ApJ...821...89B|s2cid=19709252 |doi-access=free }}

HD 102329 c

|1.52{{±|0.30|0.25}}

|

|1123{{±|79|53}}

|

|

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

|66.97{{±|0.96}}

|3.21{{±|1.28}}

|4745{{±|71}}

|

HD 116029 c

|1.27{{±|0.15}}

|

|907{{±|30|29}}

|

|

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

|37.92{{±|0.18}}

|0.83{{±|0.24}}

|4819{{±|54}}

|

{{ill|HD 128356 b|id|HD 128356 b}}

|0.89

|

|298.2

|0.87

|

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

|84.9

|0.65

|4875

|

HD 133131 Ab

|1.42

|

|649

|1.44

|

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

|150

|0.95

|5799

|{{cite journal|bibcode=2016AJ....152..167T|doi=10.3847/0004-6256/152/6/167|arxiv=1608.06216|title=The Magellan PFS Planet Search Program: Radial Velocity and Stellar Abundance Analyses of the 360 AU, Metal-Poor Binary "Twins" HD 133131A & B|journal=The Astronomical Journal|volume=152|issue=6|pages=167|year=2016|last1=Teske|first1=Johanna K|last2=Shectman|first2=Stephen A|last3=Vogt|first3=Steve S|last4=Díaz|first4=Matías|last5=Butler|first5=R. Paul|last6=Crane|first6=Jeffrey D|last7=Thompson|first7=Ian B|last8=Arriagada|first8=Pamela|s2cid=118852162 |doi-access=free }}

HD 133131 Ac

|0.42

|

|3568

|4.49

|

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

|150

|0.95

|5799

|

HD 133131 Bb

|2.5

|

|5769

|6.15

|

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

|150

|0.93

|5805

|

HD 143105 b

|1.21

|

|2.1974

|0.0379

|

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

|159

|1.51

|6380

|

{{ill|HD 147873 b|id|HD 147873 b}}

|5.14

|

|116.596

|0.522

|

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

|342.2

|1.38

|5972

|

{{ill|HD 147873 c|id|HD 147873 c}}

|2.3

|

|491.54

|1.36

|

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

|342.2

|1.38

|5972

|

HD 156279 c

|8.60{{±|0.50|0.55}}

|

|4191{{±|270|310}}

|

|

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

|119.109{{±|0.011}}

|0.95{{±|0.08}}

|5453{{±|40}}

|

HD 164922 c

|0.04059

|

|75.765

|0.3351

|400

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

|72.2

|0.87

|5293

|

HD 165155 b

|2.89

|

|434.5

|1.13

|

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

|211.9

|1.02

|5426

|

HD 191806 b

|8.52

|

|1606.3

|2.8

|

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

|239.6

|1.14

|6010

|{{cite journal |doi=10.1051/0004-6361/201628331 |arxiv=1604.07610 |bibcode=2016A&A...591A.146D |title=The SOPHIE search for northern extrasolar planets XI. Three new companions and an orbit update: Giant planets in the habitable zone |journal=Astronomy & Astrophysics |volume=591 |pages=A146 |year=2016 |last1=Díaz |first1=Rodrigo F. |last2=Rey |first2=Javiera |last3=Demangeon |first3=Olivier D. S. |last4=Hébrard |first4=Guillaume |last5=Boisse |first5=Isabelle |last6=Arnold |first6=Luc |last7=Astudillo-Defru |first7=Nicola |last8=Beuzit |first8=Jean-Luc |last9=Bonfils |first9=Xavier |last10=Borgniet |first10=Simon |last11=Bouchy |first11=François |last12=Bourrier |first12=Vincent |last13=Courcol |first13=Bastien |last14=Deleuil |first14=Magali |last15=Delfosse |first15=Xavier |last16=Ehrenreich |first16=David |last17=Forveille |first17=Thierry |last18=Lagrange |first18=Anne-Marie |last19=Mayor |first19=Michel |last20=Moutou |first20=Claire |last21=Pepe |first21=Francesco |last22=Queloz |first22=Didier |last23=Santerne |first23=Alexandre |last24=Santos |first24=Nuno C. |last25=Sahlmann |first25=Johannes |last26=Ségransan |first26=Damien |last27=Udry |first27=Stéphane |last28=Wilson |first28=Paul A. |s2cid=3282336 |url=http://www.aanda.org/10.1051/0004-6361/201628331 }}

{{ill|HD 214823 b|id|HD 214823 b}}

|19.2

|

|1877

|3.18

|

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

|317.9

|1.22

|6215

|

HD 219828 c

|15.1

|

|4791

|5.96

|

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

|254

|1.23

|5891

|{{cite journal | title=An extreme planetary system around HD219828. One long-period super Jupiter to a hot-neptune host star | first1=N. C. | last1=Santos | first2=A. | last2=Santerne | first3=J. P. | last3=Faria | first4=J. | last4=Rey | first5=A. C. M. | last5=Correia | first6=J. | last6=Laskar | first7=S. | last7=Udry | first8=V. | last8=Adibekyan | first9=F. | last9=Bouchy | first10=E. | last10=Delgado-Mena | first11=C. | last11=Melo | first12=X. | last12=Dumusque | first13=G. | last13=Hébrard | first14=C. | last14=Lovis | first15=M. | last15=Mayor | first16=M. | last16=Montalto | first17=A. | last17=Mortier | first18=F. | last18=Pepe | first19=P. | last19=Figueira | first20=J. | last20=Sahlmann | first21=D. | last21=Ségransan | first22=S. G. | last22=Sousa | display-authors=1 | journal=Astronomy & Astrophysics | date=2016 | volume=592 | page=A13 | arxiv=1605.06942 | doi=10.1051/0004-6361/201628374 | bibcode=2016A&A...592A..13S | s2cid=96428891}}

HD 220842 b

|3.18

|

|218.47

|0.74

|

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

|204

|1.13

|5960

|

{{ill|HD 221585 b|id|HD 221585 b}}

|1.61

|

|1173

|2.306

|

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

|174.8

|1.19

|5620

|

{{ill|HD 222076 b|id|HD 222076 b}}

|1.56

|

|871

|1.83

|

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

|272

|1.07

|4806

|

{{ill|HD 224538 b|id|HD 224538 b}}

|5.97

|

|1189.1

|2.28

|

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

|253.6

|1.34

|6097

|

HD 11343 b

|5.5

|

|1560.2

|2.8

|

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

|550.0

|1.17

|4670

|Host star also known as HIP 8541

HIP 41378 b

|

|0.259

|15.5712

|

|

|style="background:#FFFF00"|transit

|378.8

|1.15

|6199

|{{citation|arxiv=1606.08441|year=2016|title=Five Planets Transiting a Ninth Magnitude Star|bibcode=2016ApJ...827L..10V|last1=Vanderburg|first1=Andrew|last2=Becker|first2=Juliette C.|last3=Kristiansen|first3=Martti H.|last4=Bieryla|first4=Allyson|last5=Duev|first5=Dmitry A.|last6=Jensen-Clem|first6=Rebecca|last7=Morton|first7=Timothy D.|last8=Latham|first8=David W.|last9=Adams|first9=Fred C.|last10=Baranec|first10=Christoph|last11=Berlind|first11=Perry|last12=Calkins|first12=Michael L.|last13=Esquerdo|first13=Gilbert A.|last14=Kulkarni|first14=Shrinivas|last15=Law|first15=Nicholas M.|last16=Riddle|first16=Reed|last17=Salama|first17=Maïssa|last18=Schmitt|first18=Allan R.|journal=The Astrophysical Journal|volume=827|issue=1|pages=L10|doi=10.3847/2041-8205/827/1/L10|s2cid=8794583 |doi-access=free }}

HIP 41378 c

|

|0.228

|31.6978

|

|

|style="background:#FFFF00"|transit

|378.8

|1.15

|6199

|

HIP 41378 d

|

|0.353

|156

|

|

|style="background:#FFFF00"|transit

|378.8

|1.15

|6199

|

HIP 41378 e

|

|0.492

|131

|

|

|style="background:#FFFF00"|transit

|378.8

|1.15

|6199

|

HIP 41378 f

|

|0.91

|324

|

|

|style="background:#FFFF00"|transit

|378.8

|1.15

|6199

|Possible ring system

HIP 65407 b

|0.428

|

|28.125

|0.177

|

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

|181

|0.93

|5460

|{{citation|arxiv=1602.04622|year=2016|title=The SOPHIE search for northern extrasolar planets. X. Detection and characterization of giant planets by the dozen|bibcode=2016A&A...588A.145H|last1=Hébrard|first1=G.|last2=Arnold|first2=L.|last3=Forveille|first3=T.|last4=Correia|first4=A. C. M.|last5=Laskar|first5=J.|last6=Bonfils|first6=X.|last7=Boisse|first7=I.|last8=Díaz|first8=R. F.|last9=Hagelberg|first9=J.|last10=Sahlmann|first10=J.|last11=Santos|first11=N. C.|last12=Astudillo-Defru|first12=N.|last13=Borgniet|first13=S.|last14=Bouchy|first14=F.|last15=Bourrier|first15=V.|last16=Courcol|first16=B.|last17=Delfosse|first17=X.|last18=Deleuil|first18=M.|last19=Demangeon|first19=O.|last20=Ehrenreich|first20=D.|last21=Gregorio|first21=J.|last22=Jovanovic|first22=N.|last23=Labrevoir|first23=O.|last24=Lagrange|first24=A. -M.|last25=Lovis|first25=C.|last26=Lozi|first26=J.|last27=Moutou|first27=C.|last28=Montagnier|first28=G.|last29=Pepe|first29=F.|last30=Rey|first30=J.|journal=Astronomy and Astrophysics|volume=588|pages=A145|doi=10.1051/0004-6361/201527585|s2cid=55138055|display-authors=1}}

HIP 65407 c

|0.784

|

|67.3

|0.316

|

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

|181

|0.93

|5460

|

{{ill|HD 120457|lt=HIP 67537 b|zh|HD 120457}}

|11.1

|

|2556.5

|4.91

|

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

|

|2.41

|4985

|Eccentric orbit, host star also known as HD 120457{{citation|arxiv=1612.06252|year=2017|title=An eccentric companion at the edge of the brown dwarf desert orbiting the 2.4M⊙giant star HIP 67537|doi=10.1051/0004-6361/201630278 |last1=Jones |first1=M. I. |last2=Brahm |first2=R. |last3=Wittenmyer |first3=R. A. |last4=Drass |first4=H. |last5=Jenkins |first5=J. S. |last6=Melo |first6=C. H. F. |last7=Vos |first7=J. |last8=Rojo |first8=P. |journal=Astronomy & Astrophysics |volume=602 |pages=A58 |bibcode=2017A&A...602A..58J |s2cid=55755173 }}

{{ill|HD 135760#Planetary system|lt=HD 135760 b|ru|HD 135760}}

|2.4

|

|822.3

|2.1

|

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

|298.4

|1.74

|4850

|Host star also known as HIP 74890{{citation|arxiv=1603.03738|year=2016|title=Four new planets around giant stars and the mass-metallicity correlation of planet-hosting stars|bibcode=2016A&A...590A..38J|last1=Jones|first1=M. I.|last2=Jenkins|first2=J. S.|last3=Brahm|first3=R.|last4=Wittenmyer|first4=R. A.|last5=Olivares e.|first5=F.|last6=Melo|first6=C. H. F.|last7=Rojo|first7=P.|last8=Jordán|first8=A.|last9=Drass|first9=H.|last10=Butler|first10=R. P.|last11=Wang|first11=L.|journal=Astronomy and Astrophysics|volume=590|pages=A38|doi=10.1051/0004-6361/201628067|s2cid=45730401}}

HIP 109384 b

|1.56

|

|499.48

|1.134

|

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

|183

|0.78

|5180

|

HIP 109600 b

|2.68

|

|232.08

|0.706

|

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

|191

|0.87

|5530

|

HR 2562 b

|30

|1.11

|

|20.3

|

|style="background:#FF6CDA"|imaging

|109.7

|1.3

|

|{{cite journal|last1=Konopacky|first1=Quinn M.|last2=Rameau|first2=Julien|last3=Duchêne|first3=Gaspard|last4=Filippazzo|first4=Joseph C.|last5=Godfrey|first5=Paige A. Giorla|last6=Marois|first6=Christian|last7=Nielsen|first7=Eric L.|last8=Pueyo|first8=Laurent|last9=Rafikov|first9=Roman R.|date=2016|title=Discovery of a Substellar Companion to the Nearby Debris Disk Host HR 2562|bibcode=2016ApJ...829L...4K|arxiv=1608.06660|journal=The Astrophysical Journal Letters|language=en|volume=829|issue=1|pages=L4|doi=10.3847/2041-8205/829/1/L4|s2cid=44216698|issn=2041-8205 |doi-access=free }}

K2-8c

|

|0.215

|5.06416

|0.0532

|631

|style="background:#FFFF00"|transit

|

|0.78

|4870

|{{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 }}

K2-19d

|0.044

|0.102

|2.50856

|0.0344

|1252

|style="background:#FFFF00"|transit

|950

|0.93

|5430

|{{citation|arxiv=1604.01413|year=2016|title=Doppler Monitoring of five K2 Transiting Planetary Systems|bibcode=2016ApJ...823..115D|last1=Dai|first1=Fei|last2=Winn|first2=Joshua N.|last3=Albrecht|first3=Simon|last4=Arriagada|first4=Pamela|last5=Bieryla|first5=Allyson|last6=Butler|first6=R. Paul|last7=Crane|first7=Jeffrey D.|last8=Hirano|first8=Teriyaki|last9=Johnson|first9=John Asher|last10=Kiilerich|first10=Amanda|last11=Latham|first11=David W.|last12=Narita|first12=Norio|last13=Nowak|first13=Grzegorz|last14=Palle|first14=Enric|last15=Ribas|first15=Ignasi|last16=Rogers|first16=Leslie A.|last17=Sanchis-Ojeda|first17=Roberto|last18=Shectman|first18=Stephen A.|last19=Teske|first19=Johanna K.|last20=Thompson|first20=Ian B.|last21=Van Eylen|first21=Vincent|last22=Vanderburg|first22=Andrew|last23=Wittenmyer|first23=Robert A.|last24=Yu|first24=Liang|journal=The Astrophysical Journal|volume=823|issue=2|page=115|doi=10.3847/0004-637X/823/2/115|s2cid=59047478 |doi-access=free }}

K2-24b

|0.062

|0.52

|20.88508

|0.1542

|709

|style="background:#FFFF00"|transit

|590

|1.12

|5743

|

K2-24c

|0.082

|0.723

|42.36342

|0.2471

|560

|style="background:#FFFF00"|transit

|590

|1.12

|5743

|

|{{interlanguage link|K2-26|lt=K2-26b|ru|K2-26}}

|

|0.238

|14.5665

|0.0962

|

|style="background:#FFFF00"|transit

|300

|0.56

|3785

|

K2-27b

|0.09722

|0.4

|6.771315

|0.06702

|

|style="background:#FFFF00"|transit

|

|0.87

|5248

|

K2-29b

|0.73

|1.19

|3.2588321

|0.04217

|1171

|style="background:#FFFF00"|transit

|600

|0.94

|5358

|{{citation|arxiv=1601.07844|year=2016|title=Two Hot Jupiters from K2 Campaign 4|bibcode=2016AJ....151..171J|last1=Johnson|first1=Marshall C.|last2=Gandolfi|first2=Davide|last3=Fridlund|first3=Malcolm|last4=Csizmadia|first4=Szilard|last5=Endl|first5=Michael|last6=Cabrera|first6=Juan|last7=Cochran|first7=William D.|last8=Deeg|first8=Hans J.|last9=Grziwa|first9=Sascha|last10=Ramírez|first10=Ivan|last11=Hatzes|first11=Artie P.|last12=Eigmüller|first12=Philipp|last13=Barragán|first13=Oscar|last14=Erikson|first14=Anders|last15=Guenther|first15=Eike W.|last16=Korth|first16=Judith|last17=Kuutma|first17=Teet|last18=Nespral|first18=David|last19=Pätzold|first19=Martin|last20=Palle|first20=Enric|last21=Prieto-Arranz|first21=Jorge|last22=Rauer|first22=Heike|last23=Saario|first23=Joonas|journal=The Astronomical Journal|volume=151|issue=6|page=171|doi=10.3847/0004-6256/151/6/171|s2cid=54856428 |doi-access=free }}

K2-30b

|0.579

|1.039

|4.098503

|0.04839

|1185

|style="background:#FFFF00"|transit

|910

|0.9

|5425

|{{citation|arxiv=1601.07635|year=2016|title=K2-30 b and K2-34 b: two inflated hot-Jupiters around Solar-type stars|bibcode=2016A&A...594A..50L|last1=Lillo-Box|first1=J.|last2=Demangeon|first2=O.|last3=Santerne|first3=A.|last4=Barros|first4=S. C. C.|last5=Barrado|first5=D.|last6=Hébrard|first6=G.|last7=Osborn|first7=H. P.|last8=Armstrong|first8=D. J.|last9=Almenara|first9=J. -M.|last10=Boisse|first10=I.|last11=Bouchy|first11=F.|last12=Brown|first12=D. J. A.|last13=Courcol|first13=B.|last14=Deleuil|first14=M.|last15=Delgado Mena|first15=E.|last16=Díaz|first16=R. F.|last17=Kirk|first17=J.|last18=Lam|first18=K. W. F.|last19=McCormac|first19=J.|last20=Pollacco|first20=D.|last21=Rajpurohit|first21=A.|last22=Rey|first22=J.|last23=Santos|first23=N. C.|last24=Sousa|first24=S. G.|last25=Tsantaki|first25=M.|last26=Wilson|first26=P. A.|journal=Astronomy and Astrophysics|volume=594|page=594|doi=10.1051/0004-6361/201628204|s2cid=119263051}}{{citation|arxiv=1603.01721|year=2016|title=An independent discovery of two hot Jupiters from the K2 mission|bibcode=2016PASP..128l4402B|last1=Brahm|first1=Rafael|last2=Jones|first2=Matías|last3=Espinoza|first3=Néstor|last4=Jordán|first4=Andrés|last5=Rabus|first5=Markus|last6=Rojas|first6=Felipe|last7=Jenkins|first7=James S.|last8=Cortés|first8=Cristián|last9=Drass|first9=Holger|last10=Pantoja|first10=Blake|last11=Soto|first11=Maritza G.|last12=Vučković|first12=Maja|journal=Publications of the Astronomical Society of the Pacific|volume=128|issue=970|page=124402|doi=10.1088/1538-3873/128/970/124402|s2cid=118824050}}

K2-31b

|1.774

|1.06

|1.25785

|0.022

|

|style="background:#FFFF00"|transit

|

|0.91

|5280

|

K2-32b

|0.05191

|0.458

|8.99213

|0.08036

|

|style="background:#FFFF00"|transit

|

|0.86

|5275

|

K2-32c

|0.03807

|0.269

|20.6602

|0.1399

|

|style="background:#FFFF00"|transit

|

|0.86

|5275

|

K2-32d

|0.03241

|0.306

|31.7154

|0.1862

|

|style="background:#FFFF00"|transit

|

|0.86

|5275

|

K2-33b

|3.7

|0.45

|5.424865

|

|

|style="background:#FFFF00"|transit

|470

|0.56

|3540

|{{cite journal | title=Zodiacal Exoplanets in Time (ZEIT). III. A Short-Period Planet Orbiting a Pre-Main-Sequence Star in the Upper Scorpius OB Association | last1=Mann | first1=Andrew W. | last2=Newton | first2=Elisabeth R. | last3=Rizzuto | first3=Aaron C. | last4=Irwin | first4=Jonathan | last5=Feiden | first5=Gregory A. | last6=Gaidos | first6=Eric | last7=Mace | first7=Gregory N. | last8=Kraus | first8=Adam L. | last9=James | first9=David J. | last10=Ansdell | first10=Megan | last11=Charbonneau | first11=David | last12=Covey | first12=Kevin R. | last13=Ireland | first13=Michael J. | last14=Jaffe | first14=Daniel T. | last15=Johnson | first15=Marshall C. | last16=Kidder | first16=Benjamin | last17=Vanderburg | first17=Andrew | display-authors=1 | journal=The Astronomical Journal | volume=152 | issue=3 | at=61 | year=2016 | arxiv=1604.06165 | bibcode=2016AJ....152...61M | doi=10.3847/0004-6256/152/3/61 | doi-access=free }}

K2-34b

|1.76

|1.35

|2.995607

|0.04419

|1742

|style="background:#FFFF00"|transit

|1230

|1.28

|6132

|{{citation|arxiv=1602.00638|year=2016|title=The K2-ESPRINT Project IV: A Hot Jupiter in a Prograde Orbit with a Possible Stellar Companion|bibcode=2016ApJ...825...53H|last1=Hirano|first1=Teruyuki|last2=Nowak|first2=Grzegorz|last3=Kuzuhara|first3=Masayuki|last4=Palle|first4=Enric|last5=Dai|first5=Fei|last6=Yu|first6=Liang|last7=Van Eylen|first7=Vincent|last8=Takeda|first8=Yoichi|last9=Brandt|first9=Timothy D.|last10=Narita|first10=Norio|last11=Velasco|first11=Sergio|last12=Prieto Arranz|first12=Jorge|last13=Sanchis-Ojeda|first13=Roberto|last14=Winn|first14=Joshua N.|last15=Kudo|first15=Tomoyuki|last16=Kusakabe|first16=Nobuhiko|last17=Fukui|first17=Akihiko|last18=Sato|first18=Bun'ei|last19=Albrecht|first19=Simon|last20=Ribas|first20=Ignasi|last21=Ryu|first21=Tsuguru|last22=Tamura|first22=Motohide|journal=The Astrophysical Journal|volume=825|issue=1|page=53|doi=10.3847/0004-637X/825/1/53|s2cid=118390501 |doi-access=free }}

K2-35b

|

|0.125

|2.39984

|0.032

|

|style="background:#FFFF00"|transit

|

|0.76

|4680

|{{citation|arxiv=1511.09213|year=2015|bibcode=2016ApJ...827...78S|last1=Sinukoff|first1=Evan|last2=Howard|first2=Andrew W.|last3=Petigura|first3=Erik A.|last4=Schlieder|first4=Joshua E.|last5=Crossfield|first5=Ian J. M.|last6=Ciardi|first6=David R.|last7=Fulton|first7=Benjamin J.|last8=Isaacson|first8=Howard|last9=Aller|first9=Kimberly M.|last10=Baranec|first10=Christoph|last11=Beichman|first11=Charles A.|last12=Hansen|first12=Brad M. S.|last13=Knutson|first13=Heather A.|last14=Law|first14=Nicholas M.|last15=Liu|first15=Michael C.|last16=Riddle|first16=Reed|last17=Dressing|first17=Courtney D.|title=Eleven Multiplanet Systems Fromk2Campaigns 1 and 2 and the Masses of Two Hot Super-Earths|journal=The Astrophysical Journal|volume=827|issue=1|page=78|doi=10.3847/0004-637X/827/1/78|s2cid=31029473 |doi-access=free }}

K2-35c

|

|0.186

|5.60912

|0.0564

|

|style="background:#FFFF00"|transit

|

|0.76

|4680

|

K2-36b

|

|0.118

|1.42266

|0.023

|

|style="background:#FFFF00"|transit

|

|0.8

|4924

|

K2-36c

|

|0.25

|5.34059

|0.0555

|

|style="background:#FFFF00"|transit

|

|0.8

|4924

|

K2-37b

|

|0.144

|4.44117

|0.0511

|

|style="background:#FFFF00"|transit

|

|0.9

|5413

|

K2-37c

|

|0.245

|6.42904

|0.0654

|

|style="background:#FFFF00"|transit

|

|0.9

|5413

|

K2-37d

|

|0.244

|14.09189

|0.1103

|

|style="background:#FFFF00"|transit

|

|0.9

|5413

|

K2-38b

|0.03776

|0.138

|4.01593

|0.0506

|

|style="background:#FFFF00"|transit

|631{{±|9}}

|1.03{{±|0.04|0.02}}

|5731{{±|66}}

| Also candidate planet K2-38d in system not coplanar with two transiting planets{{citation|arxiv=2007.01081|title=Characterization of the K2-38 planetary system|year=2020|doi=10.1051/0004-6361/202038187|last1=Toledo-Padrón|first1=B.|last2=Lovis|first2=C.|last3=Suárez Mascareño|first3=A.|last4=Barros|first4=S. C. C.|last5=González Hernández|first5=J. I.|last6=Sozzetti|first6=A.|last7=Bouchy|first7=F.|last8=Zapatero Osorio|first8=M. R.|last9=Rebolo|first9=R.|last10=Cristiani|first10=S.|last11=Pepe|first11=F. A.|last12=Santos|first12=N. C.|last13=Sousa|first13=S. G.|last14=Tabernero|first14=H. M.|last15=Lillo-Box|first15=J.|last16=Bossini|first16=D.|last17=Adibekyan|first17=V.|last18=Allart|first18=R.|last19=Damasso|first19=M.|last20=d'Odorico|first20=V.|last21=Figueira|first21=P.|last22=Lavie|first22=B.|last23=Lo Curto|first23=G.|last24=Mehner|first24=A.|last25=Micela|first25=G.|last26=Modigliani|first26=A.|last27=Nunes|first27=N. J.|last28=Pallé|first28=E.|last29=Abreu|first29=M.|last30=Affolter|first30=M.|journal=Astronomy & Astrophysics|volume=641|pages=A92|s2cid=220302044|display-authors=1}}

K2-38c

|0.03115

|0.216

|10.56103

|0.0964

|

|style="background:#FFFF00"|transit

|631{{±|9}}

|1.03{{±|0.04|0.02}}

|5731{{±|66}}

| Also candidate planet K2-38d in system not coplanar with two transiting planets

|{{interlanguage link|K2-39|lt=K2-39b|ru|K2-39}}

|0.12522

|0.509

|4.60497

|0.0574

|

|style="background:#FFFF00"|transit

|972.5

|1.19

|4912

|

K2-42b

|

|0.192

|6.68796

|0.0617

|

|style="background:#FFFF00"|transit

|

|0.7

|4613

|

K2-43b

|

|0.368

|3.47114

|0.03784

|

|style="background:#FFFF00"|transit

|

|0.6

|3939

|

K2-44b

|

|0.243

|5.65688

|0.0651

|

|style="background:#FFFF00"|transit

|

|1.15

|5912

|

K2-45b

|

|0.599

|1.7292684

|0.0224

|

|style="background:#FFFF00"|transit

|

|0.5

|4103

|

K2-46b

|

|0.183

|19.1541

|0.13821

|

|style="background:#FFFF00"|transit

|

|0.96

|6256

|

K2-47b

|

|0.169

|31.6372

|0.1779

|

|style="background:#FFFF00"|transit

|

|0.75

|5054

|

K2-48b

|

|0.2

|20.5065

|0.1344

|

|style="background:#FFFF00"|transit

|

|0.77

|4899

|

K2-49b

|

|0.172

|2.77065

|0.0309

|

|style="background:#FFFF00"|transit

|

|0.51

|4175

|

K2-50b

|

|0.142

|8.7529

|0.0705

|

|style="background:#FFFF00"|transit

|

|0.61

|4326

|

K2-52b

|

|0.99

|3.53482

|0.0485

|

|style="background:#FFFF00"|transit

|

|1.21

|6113

|

K2-53b

|

|0.223

|12.2054

|0.0975

|

|style="background:#FFFF00"|transit

|

|0.83

|5269

|

|{{interlanguage link|K2-54|lt=K2-54b|ru|K2-54}}

|

|0.103

|9.7843

|0.0671

|

|style="background:#FFFF00"|transit

|

|0.42

|3798

|

|{{interlanguage link|K2-55|lt=K2-55b|ru|K2-55}}

|

|0.341

|2.849258

|0.03486

|

|style="background:#FFFF00"|transit

|

|0.7

|4456

|

|{{interlanguage link|K2-57|lt=K2-57b|ru|K2-57}}

|

|0.187

|9.0063

|0.0746

|

|style="background:#FFFF00"|transit

|

|0.68

|4434

|

K2-58b

|

|0.239

|7.05254

|0.0692

|

|style="background:#FFFF00"|transit

|

|0.89

|5413

|

K2-58c

|

|0.145

|2.53726

|0.035

|

|style="background:#FFFF00"|transit

|

|0.89

|5413

|

K2-58d

|

|0.153

|22.8827

|0.1517

|

|style="background:#FFFF00"|transit

|

|0.89

|5413

|

|{{interlanguage link|K2-59|lt=K2-59b|ru|K2-59}}

|

|0.215

|20.6921

|0.1354

|

|style="background:#FFFF00"|transit

|

|0.77

|5055

|

|{{interlanguage link|K2-59|lt=K2-59c|ru|K2-59}}

|

|0.205

|11.2954

|0.0905

|

|style="background:#FFFF00"|transit

|

|0.77

|5055

|

|{{interlanguage link|K2-60|lt=K2-60b|ru|K2-60}}

|0.426

|0.683

|3.00265

|0.045

|1400

|style="background:#FFFF00"|transit

|

|0.97

|5500

|

|{{interlanguage link|K2-61|lt=K2-61b|ru|K2-61}}

|

|0.221

|2.57302

|0.0392

|

|style="background:#FFFF00"|transit

|

|1.21

|6293

|

|{{interlanguage link|K2-62|lt=K2-62b|ru|K2-62}}

|

|0.191

|6.67202

|0.0636

|

|style="background:#FFFF00"|transit

|

|0.77

|4880

|

|{{interlanguage link|K2-62|lt=K2-62c|ru|K2-62}}

|

|0.191

|16.1966

|0.1148

|

|style="background:#FFFF00"|transit

|

|0.77

|4880

|

|{{interlanguage link|K2-63|lt=K2-63b|ru|K2-63}}

|

|0.287

|20.257

|0.1627

|

|style="background:#FFFF00"|transit

|1710

|1.4

|6771

|

|{{interlanguage link|K2-64|lt=K2-64b|ru|K2-64}}

|

|0.185

|6.53044

|0.0619

|

|style="background:#FFFF00"|transit

|

|0.74

|5312

|

|{{interlanguage link|K2-65|lt=K2-65b|ru|K2-65}}

|

|0.141

|12.6475

|0.1014

|

|style="background:#FFFF00"|transit

|254.6

|0.87

|5213

|

K2-66b

|

|0.222

|5.06965

|0.06069

|

|style="background:#FFFF00"|transit

|

|1.16

|5958

|

|{{interlanguage link|K2-68|lt=K2-68b|ru|K2-68}}

|

|0.141

|8.05428

|0.0708

|

|style="background:#FFFF00"|transit

|

|0.73

|4746

|

|{{interlanguage link|K2-69|lt=K2-69b|ru|K2-69}}

|

|0.207

|7.06599

|0.0591

|

|style="background:#FFFF00"|transit

|

|0.55

|4127

|

|{{interlanguage link|K2-70|lt=K2-70b|ru|K2-70}}

|

|0.258

|13.97896

|0.1112

|

|style="background:#FFFF00"|transit

|

|0.94

|5622

|

|{{interlanguage link|K2-71|lt=K2-71b|ru|K2-71}}

|

|0.192

|6.98541

|0.0559

|

|style="background:#FFFF00"|transit

|

|0.48

|4006

|

K2-72b

|

|0.067

|5.57739

|0.037

|

|style="background:#FFFF00"|transit

|217

|0.22

|3497

|

K2-72c

|

|0.077

|15.1871

|0.0722

|

|style="background:#FFFF00"|transit

|217

|0.22

|3497

| Potentially habitable exoplanet

K2-72d

|

|0.065

|7.7599

|0.0461

|

|style="background:#FFFF00"|transit

|217

|0.22

|3497

|

K2-72e

|

|0.073

|24.1669

|0.098

|

|style="background:#FFFF00"|transit

|217

|0.22

|3497

| Potentially habitable exoplanet

|{{interlanguage link|K2-73|lt=K2-73b|ru|K2-73}}

|

|0.219

|7.49543

|0.07619

|

|style="background:#FFFF00"|transit

|

|1.05

|5922

|

|{{interlanguage link|K2-74|lt=K2-74b|ru|K2-74}}

|

|0.206

|19.5666

|0.1402

|

|style="background:#FFFF00"|transit

|

|0.96

|6060

|

|{{interlanguage link|K2-75|lt=K2-75b|ru|K2-75}}

|

|0.238

|7.8142

|0.081

|

|style="background:#FFFF00"|transit

|

|1.16

|5995

|

|{{interlanguage link|K2-75|lt=K2-75c|ru|K2-75}}

|

|0.247

|18.311

|0.1429

|

|style="background:#FFFF00"|transit

|

|1.16

|5995

|

K2-77b

|1.9

|0.205

|8.199796

|

|

|style="background:#FFFF00"|transit

|460

|0.8

|4970

|

K2-79b

|0.0371{{±|0.0113}}

|0.365{{±|0.015}}

|10.99573

|0.0987

|

|style="background:#FFFF00"|transit

|

|1.06

|5926

|{{citation|arxiv=2111.02608|year=2021|title=K2-79b and K2-222b: Mass measurements of two small exoplanets with periods beyond 10 days that overlap with periodic magnetic activity signals|last1=Nava|first1=Chantanelle|last2=López-Morales|first2=Mercedes|last3=Mortier|first3=Annelies|last4=Zeng|first4=Li|last5=Giles|first5=Helen A. C.|last6=Bieryla|first6=Allyson|last7=Vanderburg|first7=Andrew|last8=Buchhave|first8=Lars A.|last9=Poretti|first9=Ennio|last10=Saar|first10=Steven H.|last11=Dumusque|first11=Xavier|last12=Latham|first12=David W.|last13=Charbonneau|first13=David|last14=Damasso|first14=Mario|last15=Bonomo|first15=Aldo S.|last16=Lovis|first16=Christophe|last17=Collier Cameron|first17=Andrew|last18=Eastman|first18=Jason D.|last19=Sozzetti|first19=Alessandro|last20=Cosentino|first20=Rosario|last21=Pedani|first21=Marco|last22=Pepe|first22=Francesco|last23=Molinari|first23=Emilio|last24=Sasselov|first24=Dimitar|last25=Mayor|first25=Michel|last26=Stalport|first26=Manu|last27=Malavolta|first27=Luca|last28=Rice|first28=Ken|last29=Watson|first29=Christopher A.|last30=Martinez Fiorenzano|first30=A. F.|journal=The Astronomical Journal|volume=163|issue=2|page=41|doi=10.3847/1538-3881/ac3141|bibcode=2022AJ....163...41N|s2cid=242757805|display-authors=1 |doi-access=free }}

K2-80b

|

|0.179

|19.0918

|0.135

|

|style="background:#FFFF00"|transit

|

|0.9

|5441

|

K2-80c

|

|0.131

|5.605

|0.0596

|

|style="background:#FFFF00"|transit

|

|0.9

|5441

|

K2-81b

|

|0.162

|6.10224

|0.0579

|

|style="background:#FFFF00"|transit

|

|0.7

|4530

|

K2-83b

|

|0.111

|2.74697

|0.03014

|

|style="background:#FFFF00"|transit

|

|0.48

|3910

|

K2-83c

|

|0.132

|9.99767

|0.07131

|

|style="background:#FFFF00"|transit

|

|0.48

|3910

|

K2-84b

|

|0.215

|6.4215

|0.0665

|

|style="background:#FFFF00"|transit

|

|0.95

|5652

|

K2-84c

|

|0.181

|27.86

|0.1768

|

|style="background:#FFFF00"|transit

|

|0.95

|5652

|

K2-85b

|

|0.09

|0.684533

|0.01263

|

|style="background:#FFFF00"|transit

|

|0.57

|4268

|

K2-86b

|

|0.175

|8.77683

|0.077

|

|style="background:#FFFF00"|transit

|

|0.79

|5482

|

K2-87b

|

|0.41

|9.72739

|0.0876

|

|style="background:#FFFF00"|transit

|

|0.95

|5406

|

K2-88b

|

|0.11

|4.6122

|0.0345

|

|style="background:#FFFF00"|transit

|

|0.26

|3537

|

K2-89b

|

|0.055

|1.096026

|0.01462

|

|style="background:#FFFF00"|transit

|

|0.35

|3691

|

K2-90b

|

|0.182

|13.7311

|0.0926

|

|style="background:#FFFF00"|transit

|

|0.56

|4136

|

K2-90c

|

|0.091

|2.90032

|0.0328

|

|style="background:#FFFF00"|transit

|

|0.56

|4136

|

K2-91b

|

|0.098

|1.419549

|0.0164

|

|style="background:#FFFF00"|transit

|

|0.29

|3622

|

K2-93b

|

|0.228

|

|0.138

|

|style="background:#FFFF00"|transit

|360

|1.2

|6200

|{{cite journal|arxiv=1911.07519|last1=Lund|first1=Mikkel N.|title=Asteroseismology of the Multiplanet System K2-93|last2=Knudstrup|first2=Emil|author3=Victor Silva Aguirre|last4=Basu|first4=Sarbani|last5=Chontos|first5=Ashley|author6=Carolina Von Essen|last7=Chaplin|first7=William J.|last8=Bieryla|first8=Allyson|last9=Casagrande|first9=Luca|last10=Vanderburg|first10=Andrew|last11=Huber|first11=Daniel|last12=Kane|first12=Stephen R.|last13=Albrecht|first13=Simon|last14=Latham|first14=David W.|last15=Davies|first15=Guy R.|last16=Becker|first16=Juliette C.|last17=Rodriguez|first17=Joseph E.|journal=The Astronomical Journal|year=2019|volume=158|issue=6|page=248|doi=10.3847/1538-3881/ab5280|bibcode=2019AJ....158..248L|s2cid=208138056 |doi-access=free }}

K2-93c

|

|0.259

|

|0.22

|

|style="background:#FFFF00"|transit

|360

|1.2

|6200

|

{{ill|K2-95b|id|K2-95b}}

|0.03458

|0.31

|10.13389

|0.0653

|

|style="background:#FFFF00"|transit

|560

|0.36

|3471

|{{citation|arxiv=1608.04760|year=2016|title=K2 Discovers a Busy Bee: An Unusual Transiting Neptune Found in the Beehive Cluster|bibcode=2016AJ....152..223O|last1=Obermeier|first1=Christian|last2=Henning|first2=Thomas|last3=Schlieder|first3=Joshua E.|last4=Crossfield|first4=Ian J. M.|last5=Petigura|first5=Erik A.|last6=Howard|first6=Andrew W.|last7=Sinukoff|first7=Evan|last8=Isaacson|first8=Howard|last9=Ciardi|first9=David R.|last10=David|first10=Trevor J.|last11=Hillenbrand|first11=Lynne A.|last12=Beichman|first12=Charles A.|last13=Howell|first13=Steve B.|last14=Horch|first14=Elliott|last15=Everett|first15=Mark|last16=Hirsch|first16=Lea|last17=Teske|first17=Johanna|last18=Christiansen|first18=Jessie L.|last19=Lépine|first19=Sébastien|last20=Aller|first20=Kimberly M.|last21=Liu|first21=Michael C.|last22=Saglia|first22=Roberto P.|last23=Livingston|first23=John|last24=Kluge|first24=Matthias|journal=The Astronomical Journal|volume=152|issue=6|page=223|doi=10.3847/1538-3881/152/6/223|s2cid=20884671 |doi-access=free }}

{{ill|K2-97b|id|K2-97b}}

|0.48{{±|0.07}}

|1.31{{±|0.11}}

|8.4061

|

|

|style="background:#FFFF00"|transit

|2490

|1.16

|4790

|{{citation|arxiv=1606.05818|year=2016|title=K2-97b: A (Re-?)Inflated Planet Orbiting a Red Giant Star|bibcode=2016AJ....152..185G|last1=Grunblatt|first1=Samuel K.|last2=Huber|first2=Daniel|last3=Gaidos|first3=Eric J.|last4=Lopez|first4=Eric D.|last5=Fulton|first5=Benjamin J.|last6=Vanderburg|first6=Andrew|last7=Barclay|first7=Thomas|last8=Fortney|first8=Jonathan J.|last9=Howard|first9=Andrew W.|last10=Isaacson|first10=Howard T.|last11=Mann|first11=Andrew W.|last12=Petigura|first12=Erik|last13=Silva Aguirre|first13=Victor|last14=Sinukoff|first14=Evan J.|journal=The Astronomical Journal|volume=152|issue=6|page=185|doi=10.3847/0004-6256/152/6/185|s2cid=33895160 |doi-access=free }}{{citation|arxiv=1706.05865|year=2017|title=Seeing Double withK2: Testing Re-inflation with Two Remarkably Similar Planets around Red Giant Branch Stars|doi=10.3847/1538-3881/aa932d |last1=Grunblatt |first1=Samuel K. |last2=Huber |first2=Daniel |last3=Gaidos |first3=Eric |last4=Lopez |first4=Eric D. |last5=Howard |first5=Andrew W. |last6=Isaacson |first6=Howard T. |last7=Sinukoff |first7=Evan |last8=Vanderburg |first8=Andrew |last9=Nofi |first9=Larissa |last10=Yu |first10=Jie |last11=North |first11=Thomas S. H. |last12=Chaplin |first12=William |last13=Foreman-Mackey |first13=Daniel |last14=Petigura |first14=Erik |last15=Ansdell |first15=Megan |last16=Weiss |first16=Lauren |last17=Fulton |first17=Benjamin |last18=Lin |first18=Douglas N. C. |journal=The Astronomical Journal |volume=154 |issue=6 |page=254 |bibcode=2017AJ....154..254G |s2cid=55959801 |doi-access=free }}

{{ill|K2-98b|id|K2-98b}}

|0.10131

|0.384

|10.13675

|0.0943

|

|style="background:#FFFF00"|transit

|1420

|1.07

|6120

|{{citation|arxiv=1608.01165|year=2016|title=K2-98b: A 32M⊕NEPTUNE-SIZE PLANET IN a 10 DAY ORBIT TRANSITING AN F8 STAR|doi=10.3847/0004-6256/152/6/193|last1=Barragán|first1=Oscar|last2=Grziwa|first2=Sascha|last3=Gandolfi|first3=Davide|last4=Fridlund|first4=Malcolm|last5=Endl|first5=Michael|last6=Deeg|first6=Hans J.|last7=Cagigal|first7=Manuel P.|last8=Lanza|first8=Antonino F.|last9=Moroni|first9=Pier G. Prada|last10=Smith|first10=Alexis M. S.|last11=Korth|first11=Judith|last12=Bedell|first12=Megan|last13=Cabrera|first13=Juan|last14=Cochran|first14=William D.|last15=Cusano|first15=Felice|last16=Csizmadia|first16=Szilard|last17=Eigmüller|first17=Philipp|last18=Erikson|first18=Anders|last19=Guenther|first19=Eike W.|last20=Hatzes|first20=Artie P.|last21=Nespral|first21=David|last22=Pätzold|first22=Martin|last23=Prieto-Arranz|first23=Jorge|last24=Rauer|first24=Heike|journal=The Astronomical Journal|volume=152|issue=6|page=193|s2cid=59424381 |doi-access=free }}

K2-99b

|0.97

|1.06{{±|0.01}}

|18.249

|0.159

|

|style="background:#FFFF00"|transit

|1980

|1.6

|5990

|{{citation|arxiv=1609.00239|year=2017|title=K2-99: a subgiant hosting a transiting warm Jupiter in an eccentric orbit and a long-period companion|bibcode=2017MNRAS.464.2708S|last1=Smith|first1=A. M. S.|last2=Gandolfi|first2=D.|last3=Barragán|first3=O.|last4=Bowler|first4=B.|last5=Csizmadia|first5=Sz.|last6=Endl|first6=M.|last7=Fridlund|first7=M. C. V.|last8=Grziwa|first8=S.|last9=Guenther|first9=E.|last10=Hatzes|first10=A. P.|last11=Nowak|first11=G.|last12=Albrecht|first12=S.|last13=Alonso|first13=R.|last14=Cabrera|first14=J.|last15=Cochran|first15=W. D.|last16=Deeg|first16=H. J.|last17=Cusano|first17=F.|last18=Eigmüller|first18=Ph.|last19=Erikson|first19=A.|last20=Hidalgo|first20=D.|last21=Hirano|first21=T.|last22=Johnson|first22=M. C.|last23=Korth|first23=J.|last24=Mann|first24=A.|last25=Narita|first25=N.|last26=Nespral|first26=D.|last27=Palle|first27=E.|last28=Pätzold|first28=M.|last29=Prieto-Arranz|first29=J.|last30=Rauer|first30=H.|journal=Monthly Notices of the Royal Astronomical Society|volume=464|issue=3|page=2708|doi=10.1093/mnras/stw2487|doi-access=free |display-authors=1}}{{citation|arxiv=2111.14660|year=2021|title=K2-99 revisited: a non-inflated warm Jupiter, and a temperate giant planet on a 522-d orbit around a subgiant|bibcode=2022MNRAS.510.5035S|last1=Smith|first1=A. M. S.|last2=Breton|first2=S. N.|last3=Csizmadia|first3=Sz|last4=Dai|first4=F.|last5=Gandolfi|first5=D.|last6=García|first6=R. A.|last7=Howard|first7=A. W.|last8=Isaacson|first8=H.|last9=Korth|first9=J.|last10=Lam|first10=K. W. F.|last11=Mathur|first11=S.|last12=Nowak|first12=G.|last13=Pérez Hernández|first13=F.|last14=Persson|first14=C. M.|last15=Albrecht|first15=S. H.|last16=Barragán|first16=O.|last17=Cabrera|first17=J.|last18=Cochran|first18=W. D.|last19=Deeg|first19=H. J.|last20=Fridlund|first20=M.|last21=Georgieva|first21=I. Y.|last22=Goffo|first22=E.|last23=Guenther|first23=E. W.|last24=Hatzes|first24=A. P.|last25=Kabath|first25=P.|last26=Livingston|first26=J. H.|last27=Luque|first27=R.|last28=Palle|first28=E.|last29=Redfield|first29=S.|last30=Rodler|first30=F.|journal=Monthly Notices of the Royal Astronomical Society|volume=510|issue=4|pages=5035–5049|doi=10.1093/mnras/stab3497|doi-access=free |display-authors=1}}

K2-100b

|

|0.312

|1.673916

|

|

|style="background:#FFFF00"|transit

|592

|1.18

|6120

|

K2-101b

|

|0.178

|14.677286

|

|

|style="background:#FFFF00"|transit

|592

|0.8

|4819

|

K2-102b

|

|0.116

|9.915615

|

|

|style="background:#FFFF00"|transit

|592

|0.77

|4695

|

K2-103b

|

|0.196

|21.169619

|

|

|style="background:#FFFF00"|transit

|592

|0.61

|3880

|Host star (also known as EPIC 211822797), belongs to Beehive Cluster{{citation|arxiv=1607.02339|year=2016|title=New planetary and eclipsing binary candidates from campaigns 1-6 of the K2 mission|bibcode=2016A&A...594A.100B|last1=Barros|first1=S. C. C.|last2=Demangeon|first2=O.|last3=Deleuil|first3=M.|journal=Astronomy and Astrophysics|volume=594|page=594|doi=10.1051/0004-6361/201628902|s2cid=119282186}}

K2-104b

|

|0.17

|1.97419

|

|

|style="background:#FFFF00"|transit

|592

|0.51

|3660

|

K2-107b

|0.84

|1.44

|3.31392

|0.048

|

|style="background:#FFFF00"|transit

|

|1.3

|6030

|{{citation|arxiv=1611.03704|year=2016|title=K2-60b and K2-107b. A Sub-Jovian and a Jovian Planet from the K2 Mission|doi=10.3847/1538-3881/aa5d0b |last1=Eigmüller |first1=Philipp |last2=Gandolfi |first2=Davide |last3=Persson |first3=Carina M. |last4=Donati |first4=Paolo |last5=Fridlund |first5=Malcolm |last6=Csizmadia |first6=Szilard |last7=Barragán |first7=Oscar |last8=Smith |first8=Alexis M. S. |last9=Cabrera |first9=Juan |last10=Korth |first10=Judith |last11=Grziwa |first11=Sascha |last12=Prieto-Arranz |first12=Jorge |last13=Nespral |first13=David |last14=Saario |first14=Joonas |last15=Cochran |first15=William D. |last16=Cusano |first16=Felice |last17=Deeg |first17=Hans J. |last18=Endl |first18=Michael |last19=Erikson |first19=Anders |last20=Guenther |first20=Eike W. |last21=Hatzes |first21=Artie P. |last22=Pätzold |first22=Martin |last23=Rauer |first23=Heike |journal=The Astronomical Journal |volume=153 |issue=3 |page=130 |s2cid=119001914 |doi-access=free }}

K2-110b

|0.0525

|0.2312

|13.86375

|0.1021

|640

|style="background:#FFFF00"|transit

|385

|0.74

|5010

|{{citation|arxiv=1605.04291|year=2017|title=K2-110 b: A massive mini-Neptune exoplanet|doi=10.1051/0004-6361/201628932 |last1=Osborn |first1=H. P. |last2=Santerne |first2=A. |last3=Barros |first3=S. C. C. |last4=Santos |first4=N. C. |last5=Dumusque |first5=X. |last6=Malavolta |first6=L. |last7=Armstrong |first7=D. J. |last8=Hojjatpanah |first8=S. |last9=Demangeon |first9=O. |last10=Adibekyan |first10=V. |last11=Almenara |first11=J.-M. |last12=Barrado |first12=D. |last13=Bayliss |first13=D. |last14=Boisse |first14=I. |last15=Bouchy |first15=F. |last16=Brown |first16=D. J. A. |last17=Cameron |first17=A. C. |last18=Charbonneau |first18=D. |last19=Deleuil |first19=M. |last20=Delgado Mena |first20=E. |last21=Díaz |first21=R. F. |last22=Hébrard |first22=G. |last23=Kirk |first23=J. |last24=King |first24=G. W. |last25=Lam |first25=K. W. F. |last26=Latham |first26=D. |last27=Lillo-Box |first27=J. |last28=Louden |first28=T. M. |last29=Lovis |first29=C. |last30=Marmier |first30=M. |journal=Astronomy & Astrophysics |volume=604 |pages=A19 |bibcode=2017A&A...604A..19O |s2cid=118559798 |display-authors=1 }}

K2-113b

|1.29

|0.930

|5.817608

|0.0558

|1178

|style="background:#FFFF00"|transit

|1800

|1.01

|5627

|{{citation|arxiv=1611.07614|year=2016|title=K2-113: A dense hot-Jupiter transiting a solar analogue|doi=10.1093/mnras/stx1862 |last1=Espinoza |first1=Néstor |last2=Rabus |first2=Markus |last3=Brahm |first3=Rafael |last4=Jones |first4=Matías |last5=Jordán |first5=Andrés |last6=Rojas |first6=Felipe |last7=Drass |first7=Holger |last8=Vučković |first8=Maja |last9=Hartman |first9=Joel D. |last10=Jenkins |first10=James S. |last11=Cortés |first11=Cristián |journal=Monthly Notices of the Royal Astronomical Society |volume=471 |issue=4 |pages=4374–4380 |doi-access=free }}

KELT-11b

|0.195{{±|0.019}}

|1.3{{±|0.18|0.12}}

|4.736529{{±|0.000068|0.000059}}

|0.06229{{±|0.00088|0.00076}}

|1712

|style="background:#FFFF00"|transit

|320{{±|16}}

|1.438{{±|0.061|0.052}}

|5370{{±|51}}

|{{Cite journal |arxiv = 1607.01755v1|doi = 10.3847/1538-3881/aa6572|title = KELT-11b: A Highly Inflated Sub-Saturn Exoplanet Transiting the V = 8 Subgiant HD 93396|year = 2017|last1 = Pepper|first1 = Joshua|last2 = Rodriguez|first2 = Joseph E.|last3 = Collins|first3 = Karen A.|last4 = Johnson|first4 = John Asher|last5 = Fulton|first5 = Benjamin J.|last6 = Howard|first6 = Andrew W.|last7 = Beatty|first7 = Thomas G.|last8 = Stassun|first8 = Keivan G.|last9 = Isaacson|first9 = Howard|last10 = Colón|first10 = Knicole D.|last11 = Lund|first11 = Michael B.|last12 = Kuhn|first12 = Rudolf B.|last13 = Siverd|first13 = Robert J.|last14 = Gaudi|first14 = B. Scott|last15 = Tan|first15 = T. G.|last16 = Curtis|first16 = Ivan|last17 = Stockdale|first17 = Christopher|last18 = Mawet|first18 = Dimitri|last19 = Bottom|first19 = Michael|last20 = James|first20 = David|last21 = Zhou|first21 = George|last22 = Bayliss|first22 = Daniel|last23 = Cargile|first23 = Phillip|last24 = Bieryla|first24 = Allyson|last25 = Penev|first25 = Kaloyan|last26 = Latham|first26 = David W.|last27 = Labadie-Bartz|first27 = Jonathan|last28 = Kielkopf|first28 = John|last29 = Eastman|first29 = Jason D.|last30 = Oberst|first30 = Thomas E.|journal = The Astronomical Journal|volume = 153|issue = 5|page = 215|bibcode = 2017AJ....153..215P|s2cid = 30219578|display-authors = 29 | doi-access=free }}

KELT-12b

|0.950

|1.78

|5.031623

|0.06708

|1800

|style="background:#FFFF00"|transit

|

|1.59

|6279

|{{citation|arxiv=1608.04714|year=2016|title=KELT-12b: AP~ 5 day, Highly Inflated Hot Jupiter Transiting a Mildly Evolved Hot Star|doi=10.3847/1538-3881/aa5ffb|last1=Stevens|first1=Daniel J.|last2=Collins|first2=Karen A.|last3=Gaudi|first3=B. Scott|last4=Beatty|first4=Thomas G.|last5=Siverd|first5=Robert J.|last6=Bieryla|first6=Allyson|last7=Fulton|first7=Benjamin J.|last8=Crepp|first8=Justin R.|last9=Gonzales|first9=Erica J.|last10=Coker|first10=Carl T.|last11=Penev|first11=Kaloyan|last12=Stassun|first12=Keivan G.|last13=Jensen|first13=Eric L. N.|last14=Howard|first14=Andrew W.|last15=Latham|first15=David W.|last16=Rodriguez|first16=Joseph E.|last17=Zambelli|first17=Roberto|last18=Bozza|first18=Valerio|last19=Reed|first19=Phillip A.|last20=Gregorio|first20=Joao|last21=Buchhave|first21=Lars A.|last22=Penny|first22=Matthew T.|last23=Pepper|first23=Joshua|last24=Berlind|first24=Perry|last25=Novati|first25=Sebastiano Calchi|last26=Calkins|first26=Michael L.|last27=d'Ago|first27=Giuseppe|last28=Eastman|first28=Jason D.|last29=Bayliss|first29=D.|last30=Colón|first30=Knicole D.|journal=The Astronomical Journal|volume=153|issue=4|page=178|bibcode=2017AJ....153..178S |s2cid=27321568|display-authors=1 |doi-access=free }}

KELT-16b

|2.75

|1.415

|0.9689951

|0.02044

|

|style="background:#FFFF00"|transit

|1289.2

|1.21

|6236

|{{citation|arxiv=1608.00618|year=2016|title=KELT-16b: A Highly Irradiated, Ultra-short Period Hot Jupiter Nearing Tidal Disruption|doi=10.3847/1538-3881/153/3/97 |last1=Oberst |first1=Thomas E. |last2=Rodriguez |first2=Joseph E. |last3=Colón |first3=Knicole D. |last4=Angerhausen |first4=Daniel |last5=Bieryla |first5=Allyson |last6=Ngo |first6=Henry |last7=Stevens |first7=Daniel J. |last8=Stassun |first8=Keivan G. |last9=Gaudi |first9=B. Scott |last10=Pepper |first10=Joshua |last11=Penev |first11=Kaloyan |last12=Mawet |first12=Dimitri |last13=Latham |first13=David W. |last14=Heintz |first14=Tyler M. |last15=Osei |first15=Baffour W. |last16=Collins |first16=Karen A. |last17=Kielkopf |first17=John F. |last18=Visgaitis |first18=Tiffany |last19=Reed |first19=Phillip A. |last20=Escamilla |first20=Alejandra |last21=Yazdi |first21=Sormeh |last22=McLeod |first22=Kim K. |last23=Lunsford |first23=Leanne T. |last24=Spencer |first24=Michelle |last25=Joner |first25=Michael D. |last26=Gregorio |first26=Joao |last27=Gaillard |first27=Clement |last28=Matt |first28=Kyle |last29=Dumont |first29=Mary Thea |last30=Stephens |first30=Denise C. |journal=The Astronomical Journal |volume=153 |issue=3 |page=97 |s2cid=42949556 |display-authors=1 |doi-access=free }}

KELT-17b

|1.31

|1.525

|3.0801716

|0.04881

|2087

|style="background:#FFFF00"|transit

|680

|1.64

|7454

|{{citation|arxiv=1607.03512|year=2016|title=Kelt-17B: A Hot-Jupiter Transiting an A-Star in a Misaligned Orbit Detected with Doppler Tomography|doi=10.3847/0004-6256/152/5/136|last1=Zhou|first1=George|last2=Rodriguez|first2=Joseph E.|last3=Collins|first3=Karen A.|last4=Beatty|first4=Thomas|last5=Oberst|first5=Thomas|last6=Heintz|first6=Tyler M.|last7=Stassun|first7=Keivan G.|last8=Latham|first8=David W.|last9=Kuhn|first9=Rudolf B.|last10=Bieryla|first10=Allyson|last11=Lund|first11=Michael B.|last12=Labadie-Bartz|first12=Jonathan|last13=Siverd|first13=Robert J.|last14=Stevens|first14=Daniel J.|last15=Gaudi|first15=B. Scott|last16=Pepper|first16=Joshua|last17=Buchhave|first17=Lars A.|last18=Eastman|first18=Jason|last19=Colón|first19=Knicole|last20=Cargile|first20=Phillip|last21=James|first21=David|last22=Gregorio|first22=Joao|last23=Reed|first23=Phillip A.|last24=Jensen|first24=Eric L. N.|last25=Cohen|first25=David H.|last26=McLeod|first26=Kim K.|last27=Tan|first27=T. G.|last28=Zambelli|first28=Roberto|last29=Bayliss|first29=Daniel|last30=Bento|first30=Joao|journal=The Astronomical Journal|volume=152|issue=5|page=136|bibcode=2016AJ....152..136Z|s2cid=55618030|display-authors=1 |doi-access=free }}

KIC 7917485 b

|11.8

|

|840

|2.03

|

|style="background:#FF7519"|timing

|

|1.63

|7067

|{{citation|arxiv=1608.02945|year=2016|title=A Planet in an 840 Day Orbit Around a Kepler Main-Sequence a Star Found from Phase Modulation of ITS Pulsations|doi=10.3847/2041-8205/827/1/L17|last1=Murphy|first1=Simon J.|last2=Bedding|first2=Timothy R.|last3=Shibahashi|first3=Hiromoto|journal=The Astrophysical Journal|volume=827|issue=1|pages=L17|bibcode=2016ApJ...827L..17M|s2cid=119203444 |doi-access=free }}

Kepler-20g

|0.0628

|

|34.94

|0.2055

|

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

|950

|0.95

|5495

|{{cite journal |arxiv=1608.06836 |doi=10.3847/0004-6256/152/6/160 |title=A 1.9 Earth Radius Rocky Planet and the Discovery of a Non-Transiting Planet in the Kepler-20 System |year=2016 |last1=Buchhave |first1=Lars A. |last2=Dressing |first2=Courtney D. |last3=Dumusque |first3=Xavier |last4=Rice |first4=Ken |last5=Vanderburg |first5=Andrew |last6=Mortier |first6=Annelies |last7=Lopez-Morales |first7=Mercedes |last8=Lopez |first8=Eric |last9=Lundkvist |first9=Mia S. |last10=Kjeldsen |first10=Hans |last11=Affer |first11=Laura |last12=Bonomo |first12=Aldo S. |last13=Charbonneau |first13=David |last14=Cameron |first14=Andrew Collier |last15=Cosentino |first15=Rosario |last16=Figueira |first16=Pedro |last17=Fiorenzano |first17=Aldo F. M. |last18=Harutyunyan |first18=Avet |last19=Haywood |first19=Raphaëlle D. |last20=Johnson |first20=John Asher |last21=Latham |first21=David W. |last22=Lovis |first22=Christophe |last23=Malavolta |first23=Luca |last24=Mayor |first24=Michel |last25=Micela |first25=Giusi |last26=Molinari |first26=Emilio |last27=Motalebi |first27=Fatemeh |last28=Nascimbeni |first28=Valerio |last29=Pepe |first29=Francesco |last30=Phillips |first30=David F. |s2cid=216077870 |journal=The Astronomical Journal |volume=152 |issue=6 |page=160 |bibcode=2016AJ....152..160B |display-authors=29 |doi-access=free }}

Kepler-46d

|

|0.146

|6.766589

|0.067

|

|style="background:#FFFF00"|transit

|2790

|0.9

|5309

|{{citation|arxiv=1601.05095|year=2016|title=Warm Jupiters Are Less Lonely Than Hot Jupiters: Close Neighbors|doi=10.3847/0004-637X/825/2/98|last1=Huang|first1=Chelsea|last2=Wu|first2=Yanqin|author2-link= Yanqin Wu |last3=Triaud|first3=Amaury H. M. J.|journal=The Astrophysical Journal|volume=825|issue=2|page=98|bibcode=2016ApJ...825...98H|s2cid=119290761 |doi-access=free }}

Kepler-56d

|5.61{{±|0.38}}

|

|1002{{±|5}}

|2.16{{±|0.08}}

|

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

|3060{{±|80}}

|1.32

|4840

|{{citation|arxiv=1608.03627|year=2016|title=The Orbit and Mass of the Third Planet in the Kepler-56 System|doi=10.3847/0004-6256/152/6/165|last1=Otor|first1=Oderah Justin|last2=Montet|first2=Benjamin T.|last3=Johnson|first3=John Asher|last4=Charbonneau|first4=David|last5=Collier-Cameron|first5=Andrew|last6=Howard|first6=Andrew W.|last7=Isaacson|first7=Howard|last8=Latham|first8=David W.|last9=Lopez-Morales|first9=Mercedes|last10=Lovis|first10=Christophe|last11=Mayor|first11=Michel|last12=Micela|first12=Giusi|last13=Molinari|first13=Emilio|last14=Pepe|first14=Francesco|last15=Piotto|first15=Giampaolo|last16=Phillips|first16=David F.|last17=Queloz|first17=Didier|last18=Rice|first18=Ken|last19=Sasselov|first19=Dimitar|last20=Ségransan|first20=Damien|last21=Sozzetti|first21=Alessandro|last22=Udry|first22=Stéphane|last23=Watson|first23=Chris|journal=The Astronomical Journal|volume=152|issue=6|page=165|bibcode=2016AJ....152..165O|s2cid=53354667 |doi-access=free }}

Kepler-80f

|

|0.108

|0.9867873

|0.0175

|

|style="background:#FFFF00"|transit

|1160

|0.73

|4540

|

Kepler-132e

|

|0.105

|110.2869374

|

|

|style="background:#FFFF00"|transit

|900{{±|70}}

|

|6003

|

Kepler-148d

|

|0.774

|51.84688575

|

|

|style="background:#FFFF00"|transit

|2630{{±|50}}

|

|5272

|

Kepler-154d

|

|0.343

|20.54981883

|

|

|style="background:#FFFF00"|transit

|3060{{±|50}}

|0.89

|5690

|

Kepler-154e

|

|0.134

|3.93276465

|

|

|style="background:#FFFF00"|transit

|3060{{±|50}}

|0.89

|5690

|

Kepler-154f

|

|0.134

|9.91935684

|

|

|style="background:#FFFF00"|transit

|3060{{±|50}}

|0.89

|5690

|

Kepler-157d

|

|0.13

|7.02573474

|

|

|style="background:#FFFF00"|transit

|2580{{±|30}}

|

|5774

|

Kepler-166d

|

|0.154

|1.55400393

|

|

|style="background:#FFFF00"|transit

|2000{{±|20}}

|

|5413

|

Kepler-167d

|

|0.107

|21.803855

|0.1405

|536

|style="background:#FFFF00"|transit

|1100

|0.77

|4890

|

Kepler-167e

|

|0.906

|1071.23228

|1.89

|131

|style="background:#FFFF00"|transit

|1100

|0.77

|4890

|

Kepler-176e

|

|0.129

|51.16579

|

|

|style="background:#FFFF00"|transit

|1740{{±|19}}

|

|5232

|

Kepler-191d

|

|0.203

|5.94504102

|

|

|style="background:#FFFF00"|transit

|1970{{±|20}}

|0.85

|5282

|

Kepler-192d

|

|0.091

|6.47027579

|

|

|style="background:#FFFF00"|transit

|2160{{±|20}}

|

|5479

|

Kepler-198d

|

|0.136

|1.31184443

|

|

|style="background:#FFFF00"|transit

|1638{{±|14}}

|0.93

|5574

|

Kepler-217d

|

|0.118

|3.88689525

|

|

|style="background:#FFFF00"|transit

|3720{{±|50}}

|

|6171

|

Kepler-218d

|

|0.237

|124.5244647

|

|

|style="background:#FFFF00"|transit

|2180{{±|20}}

|

|5502

|

Kepler-245e

|

|0.156

|3.21982106

|

|

|style="background:#FFFF00"|transit

|2870{{±|80}}

|0.8

|5100

|

Kepler-255d

|

|0.118

|1.04562266

|

|

|style="background:#FFFF00"|transit

|3530{{±|100}}

|0.97

|5573

|

Kepler-271d

|

|0.059

|5.24972541

|

|

|style="background:#FFFF00"|transit

|1334{{±|12}}

|

|5524

|

Kepler-304e

|

|0.107

|1.49914695

|

|

|style="background:#FFFF00"|transit

|1435{{±|17}}

|0.8

|4731

|

Kepler-342e

|

|0.079

|1.64422461

|

|

|style="background:#FFFF00"|transit

|2600{{±|30}}

|1.13

|6175

|

Kepler-351d

|

|0.243

|142.544247

|

|

|style="background:#FFFF00"|transit

|3640{{±|140}}

|0.89

|5643

|

Kepler-398d

|

|0.079

|6.83437001

|

|

|style="background:#FFFF00"|transit

|581.4{{±|1.8}}

|

|4493

|

Kepler-401d

|

|0.203

|184.256405

|

|

|style="background:#FFFF00"|transit

|3230{{±|50}}

|

|6117

|

Kepler-403d

|

|0.127

|13.61159129

|

|

|style="background:#FFFF00"|transit

|2800{{±|50}}

|

|6090

|

Kepler-411c

|

|0.292

|7.83442788

|

|

|style="background:#FFFF00"|transit

|503.5{{±|1.5}}

|0.83

|4974

|

Kepler-436c

|

|0.208

|16.79713874

|

|

|style="background:#FFFF00"|transit

|2020

|0.73

|4651

|

Kepler-461b

|

|0.23

|8.31378306

|

|

|style="background:#FFFF00"|transit

|1530

|0.98

|5634

|{{citation|arxiv=1605.02825|year=2016|title=False Positive Probabilities for Allkeplerobjects of Interest: 1284 Newly Validated Planets and 428 Likely False Positives|doi=10.3847/0004-637X/822/2/86|last1=Morton|first1=Timothy D.|last2=Bryson|first2=Stephen T.|last3=Coughlin|first3=Jeffrey L.|last4=Rowe|first4=Jason F.|last5=Ravichandran|first5=Ganesh|last6=Petigura|first6=Erik A.|last7=Haas|first7=Michael R.|last8=Batalha|first8=Natalie M.|journal=The Astrophysical Journal|volume=822|issue=2|page=86|bibcode=2016ApJ...822...86M|s2cid=20832201 |doi-access=free }}

Kepler-462b

|

|0.336

|84.6879808

|

|

|style="background:#FFFF00"|transit

|2390

|1.59

|7070

|

Kepler-463b

|

|0.272

|8.98101683

|

|

|style="background:#FFFF00"|transit

|1100

|0.87

|5661

|

Kepler-464b

|

|0.294

|7.25696522

|

|

|style="background:#FFFF00"|transit

|2130

|1.21

|5933

|

Kepler-465b

|

|0.263

|9.94067247

|

|

|style="background:#FFFF00"|transit

|1910

|1.23

|6310

|

Kepler-466b

|

|0.254

|51.07926307

|

|

|style="background:#FFFF00"|transit

|1420

|1.04

|5927

|

Kepler-466c

|

|0.112

|3.70921385

|

|

|style="background:#FFFF00"|transit

|1420

|1.04

|5927

|

Kepler-467b

|

|0.201

|24.99324193

|

|

|style="background:#FFFF00"|transit

|1490

|1.05

|5809

|

Kepler-468b

|

|1.19

|38.47875707

|

|

|style="background:#FFFF00"|transit

|1550

|0.96

|5498

|

Kepler-471b

|

|1.335

|5.01423457

|

|

|style="background:#FFFF00"|transit

|4480

|1.49

|6733

|

Kepler-472b

|

|0.287

|4.17625551

|

|

|style="background:#FFFF00"|transit

|980

|0.85

|4996

|

Kepler-473b

|

|0.364

|14.55731705

|

|

|style="background:#FFFF00"|transit

|2090

|1.06

|5816

|

Kepler-474b

|

|0.273

|5.66067294

|

|

|style="background:#FFFF00"|transit

|1850

|0.99

|5785

|

Kepler-475b

|

|0.222

|3.10550819

|

|

|style="background:#FFFF00"|transit

|910

|0.86

|5009

|

Kepler-476b

|

|0.275

|14.00640607

|

|

|style="background:#FFFF00"|transit

|2240

|1.03

|5837

|

Kepler-477b

|

|0.185

|11.11990653

|

|

|style="background:#FFFF00"|transit

|1200

|0.87

|5240

|

Kepler-478b

|

|0.242

|13.2217576

|

|

|style="background:#FFFF00"|transit

|1400

|0.85

|5210

|

Kepler-479b

|

|0.189

|12.49341307

|

|

|style="background:#FFFF00"|transit

|1210

|0.86

|5247

|

Kepler-480b

|

|0.248

|4.9195838

|

|

|style="background:#FFFF00"|transit

|2630

|1.25

|6322

|

Kepler-481b

|

|0.223

|10.06082567

|

|

|style="background:#FFFF00"|transit

|2330

|1.01

|5802

|

Kepler-482b

|

|0.211

|56.35418576

|

|

|style="background:#FFFF00"|transit

|950

|0.75

|4871

|

Kepler-483b

|

|0.286

|30.229104

|

|

|style="background:#FFFF00"|transit

|3110

|1.28

|6346

|

Kepler-484b

|

|0.203

|10.04556931

|

|

|style="background:#FFFF00"|transit

|1230

|0.96

|5668

|

Kepler-485b

|

|1.286

|3.2432598

|

|

|style="background:#FFFF00"|transit

|3830

|1.07

|5958

|

Kepler-487b

|

|1.019

|15.3587684

|

|

|style="background:#FFFF00"|transit

|2720

|0.91

|5444

|

Kepler-487c

|

|0.239

|38.6519976

|

|

|style="background:#FFFF00"|transit

|2720

|0.91

|5444

|

Kepler-489b

|

|0.689

|17.27629612

|

|

|style="background:#FFFF00"|transit

|1240

|0.82

|5014

|

Kepler-490b

|

|1.039

|3.26869515

|

|

|style="background:#FFFF00"|transit

|4070

|1.08

|6045

|

Kepler-491b

|

|0.796

|4.22538451

|

|

|style="background:#FFFF00"|transit

|2140

|1.04

|5582

|

Kepler-493b

|

|1.35

|3.00387658

|

|

|style="background:#FFFF00"|transit

|6330

|1.36

|6457

|

Kepler-495b

|

|0.467

|3.41303622

|

|

|style="background:#FFFF00"|transit

|2100

|0.86

|5346

|

Kepler-496b

|

|0.207

|8.30864937

|

|

|style="background:#FFFF00"|transit

|2140

|0.86

|5293

|

Kepler-497b

|

|0.539

|3.57320367

|

|

|style="background:#FFFF00"|transit

|3500

|1.09

|5834

|

Kepler-498b

|

|0.27

|9.61375356

|

|

|style="background:#FFFF00"|transit

|2430

|0.98

|5744

|

Kepler-499b

|

|0.194

|5.63252845

|

|

|style="background:#FFFF00"|transit

|1710

|0.87

|5312

|

Kepler-500b

|

|0.23

|8.5083244

|

|

|style="background:#FFFF00"|transit

|2440

|1.02

|5813

|

Kepler-501b

|

|0.384

|5.64067757

|

|

|style="background:#FFFF00"|transit

|3410

|1.03

|5904

|

Kepler-502b

|

|0.426

|4.28686431

|

|

|style="background:#FFFF00"|transit

|4670

|1.15

|6125

|

Kepler-504b

|

|0.142

|9.54927542

|

|

|style="background:#FFFF00"|transit

|240

|0.33

|3519

|

Kepler-505b

|

|0.232

|27.52197994

|

|

|style="background:#FFFF00"|transit

|720

|0.55

|3931

|

Kepler-506b

|

|0.244

|6.8834055

|

|

|style="background:#FFFF00"|transit

|750

|1.19

|6236

|

Kepler-507b

|

|0.116

|3.56809693

|

|

|style="background:#FFFF00"|transit

|1300

|1.16

|6113

|

Kepler-508b

|

|0.146

|25.30889748

|

|

|style="background:#FFFF00"|transit

|1060

|1.16

|6025

|

Kepler-509b

|

|0.222

|41.74600392

|

|

|style="background:#FFFF00"|transit

|1110

|1.1

|6060

|

Kepler-510b

|

|0.22

|19.55659418

|

|

|style="background:#FFFF00"|transit

|1230

|0.91

|5746

|

Kepler-511b

|

|0.567

|296.637865

|

|

|style="background:#FFFF00"|transit

|1460

|1

|5770

|

Kepler-512b

|

|0.24

|34.43587975

|

|

|style="background:#FFFF00"|transit

|1730

|1.17

|5997

|

Kepler-513b

|

|0.196

|28.86235584

|

|

|style="background:#FFFF00"|transit

|1520

|1.02

|5849

|

Kepler-514b

|

|0.153

|5.65179605

|

|

|style="background:#FFFF00"|transit

|1590

|1.28

|6106

|

Kepler-515b

|

|0.13

|19.96371318

|

|

|style="background:#FFFF00"|transit

|830

|0.9

|5293

|

Kepler-516b

|

|0.512

|24.85462415

|

|

|style="background:#FFFF00"|transit

|2530

|1.62

|7099

|

Kepler-517b

|

|0.238

|60.92832271

|

|

|style="background:#FFFF00"|transit

|930

|0.95

|5690

|

Kepler-518b

|

|0.188

|8.51203588

|

|

|style="background:#FFFF00"|transit

|1060

|0.96

|5842

|

Kepler-519b

|

|0.187

|24.3078946

|

|

|style="background:#FFFF00"|transit

|760

|0.89

|5260

|

Kepler-520b

|

|0.148

|19.67416124

|

|

|style="background:#FFFF00"|transit

|1600

|1.1

|6112

|

Kepler-520c

|

|0.095

|5.21104261

|

|

|style="background:#FFFF00"|transit

|1600

|1.1

|6112

|

Kepler-521b

|

|0.284

|22.20813214

|

|

|style="background:#FFFF00"|transit

|2400

|1.34

|6406

|

Kepler-522b

|

|0.616

|38.58422849

|

|

|style="background:#FFFF00"|transit

|2440

|1.54

|6392

|

Kepler-523b

|

|0.175

|5.83598311

|

|

|style="background:#FFFF00"|transit

|880

|0.93

|5515

|

Kepler-524b

|

|0.17

|7.97419807

|

|

|style="background:#FFFF00"|transit

|2400

|1.09

|6014

|

Kepler-524c

|

|0.086

|1.88897906

|

|

|style="background:#FFFF00"|transit

|2400

|1.09

|6014

|

Kepler-525b

|

|0.235

|18.68404933

|

|

|style="background:#FFFF00"|transit

|1850

|0.95

|5573

|

Kepler-526b

|

|0.178

|5.45849832

|

|

|style="background:#FFFF00"|transit

|1640

|1.15

|5894

|

Kepler-527b

|

|0.253

|13.28535633

|

|

|style="background:#FFFF00"|transit

|2940

|1.28

|6388

|

Kepler-528b

|

|0.186

|19.78297415

|

|

|style="background:#FFFF00"|transit

|2320

|1.01

|5807

|

Kepler-529b

|

|0.166

|1.98035766

|

|

|style="background:#FFFF00"|transit

|2570

|1.07

|6087

|

Kepler-529c

|

|0.178

|12.8345022

|

|

|style="background:#FFFF00"|transit

|2570

|1.07

|6087

|

Kepler-530b

|

|0.269

|39.30941904

|

|

|style="background:#FFFF00"|transit

|1510

|0.97

|5697

|

Kepler-531b

|

|0.248

|29.88485741

|

|

|style="background:#FFFF00"|transit

|830

|0.78

|4893

|

Kepler-532b

|

|0.229

|12.92491623

|

|

|style="background:#FFFF00"|transit

|1060

|0.87

|5192

|

Kepler-533b

|

|0.302

|28.51120525

|

|

|style="background:#FFFF00"|transit

|990

|0.78

|4758

|

Kepler-534b

|

|0.2

|15.95994513

|

|

|style="background:#FFFF00"|transit

|1540

|1.05

|5884

|

Kepler-535b

|

|0.211

|4.90332155

|

|

|style="background:#FFFF00"|transit

|2210

|1.18

|6123

|

Kepler-536b

|

|0.277

|1.8270823

|

|

|style="background:#FFFF00"|transit

|1450

|0.92

|5524

|

Kepler-537b

|

|0.126

|3.24755522

|

|

|style="background:#FFFF00"|transit

|1520

|1.07

|5763

|

Kepler-538b

|

|0.202

|81.73780699

|

|

|style="background:#FFFF00"|transit

|540

|0.96

|5650

|

Kepler-539b

|0.97

|0.747

|125.63243

|0.4988

|

|style="background:#FFFF00"|transit

|1020

|1.05

|5820

|

Kepler-539c

|2.4

|

|1000

|2.42

|

|style="background:#FFFF00"|transit

|1020

|1.05

|5820

|

Kepler-540b

|

|0.242

|172.7049784

|

|

|style="background:#FFFF00"|transit

|1100

|1.02

|5946

|

Kepler-541b

|

|0.3

|5.08005848

|

|

|style="background:#FFFF00"|transit

|3300

|1.41

|6166

|

Kepler-542b

|

|0.14

|13.14497566

|

|

|style="background:#FFFF00"|transit

|1430

|0.93

|5526

|

Kepler-543b

|

|0.223

|13.89961966

|

|

|style="background:#FFFF00"|transit

|690

|0.7

|4671

|

Kepler-544b

|

|0.189

|21.41616926

|

|

|style="background:#FFFF00"|transit

|2600

|1.16

|6206

|

Kepler-545b

|

|0.24

|13.24934059

|

|

|style="background:#FFFF00"|transit

|2710

|1.04

|5882

|

Kepler-546b

|

|0.624

|4.14702026

|

|

|style="background:#FFFF00"|transit

|2920

|1.11

|5967

|

Kepler-547b

|

|0.357

|6.01038429

|

|

|style="background:#FFFF00"|transit

|1180

|0.78

|4828

|

Kepler-548b

|

|1.07

|4.45419434

|

|

|style="background:#FFFF00"|transit

|2530

|0.93

|5535

|

Kepler-549b

|

|0.229

|42.9495649

|

|

|style="background:#FFFF00"|transit

|2110

|0.88

|5360

|

Kepler-549c

|

|0.261

|117.040498

|

|

|style="background:#FFFF00"|transit

|2110

|0.88

|5360

|

Kepler-550b

|

|0.394

|8.60010411

|

|

|style="background:#FFFF00"|transit

|1840

|0.87

|5322

|

Kepler-551b

|

|0.244

|12.3764661

|

|

|style="background:#FFFF00"|transit

|1020

|0.65

|4286

|

Kepler-552b

|

|0.352

|5.26341577

|

|

|style="background:#FFFF00"|transit

|2720

|1.03

|5863

|

Kepler-553b

|

|0.413

|4.03046804

|

|

|style="background:#FFFF00"|transit

|2360

|0.92

|5266

|

Kepler-553c

|

|0.999

|328.2399546

|

|

|style="background:#FFFF00"|transit

|2360

|0.92

|5266

|

Kepler-554b

|

|0.383

|1.90220856

|

|

|style="background:#FFFF00"|transit

|2090

|0.93

|5447

|

Kepler-555b

|

|0.252

|16.21775407

|

|

|style="background:#FFFF00"|transit

|2520

|1.03

|5894

|

Kepler-556b

|

|0.2

|11.72292176

|

|

|style="background:#FFFF00"|transit

|2380

|1

|5740

|

Kepler-557b

|

|0.238

|3.70598955

|

|

|style="background:#FFFF00"|transit

|3670

|1.11

|6068

|

Kepler-558b

|

|0.211

|29.00790538

|

|

|style="background:#FFFF00"|transit

|2130

|0.85

|5242

|

Kepler-559b

|

|0.322

|17.58752333

|

|

|style="background:#FFFF00"|transit

|2590

|0.96

|5630

|

Kepler-560b

|

|0.153

|18.47764449

|

|

|style="background:#FFFF00"|transit

|290

|0.34

|3556

| Potentially habitable exoplanet{{cite journal |last1=Torres |first1=Guillermo |display-authors=etal |title=Validation of Small Kepler Transiting Planet Candidates in or near the Habitable Zone |journal=The Astronomical Journal |date=December 2017 |volume=154 |issue=6 |pages=264 |doi=10.3847/1538-3881/aa984b |arxiv=1711.01267 |bibcode=2017AJ....154..264T|s2cid=73678176 |doi-access=free }}

Kepler-561b

|

|0.621

|58.3620495

|

|

|style="background:#FFFF00"|transit

|2180

|0.96

|5646

|

Kepler-561c

|

|0.239

|5.35016198

|

|

|style="background:#FFFF00"|transit

|2180

|0.96

|5646

|

Kepler-562b

|

|0.465

|18.00931444

|

|

|style="background:#FFFF00"|transit

|2680

|0.93

|5575

|

Kepler-563b

|

|0.276

|22.18432708

|

|

|style="background:#FFFF00"|transit

|1820

|0.8

|5066

|

Kepler-564b

|

|0.413

|3.75083228

|

|

|style="background:#FFFF00"|transit

|2700

|0.95

|5626

|

Kepler-565b

|

|0.325

|4.24374723

|

|

|style="background:#FFFF00"|transit

|3400

|0.98

|5735

|

Kepler-566b

|

|0.192

|18.42794624

|

|

|style="background:#FFFF00"|transit

|2050

|0.83

|5132

|

Kepler-567b

|

|0.201

|16.54297375

|

|

|style="background:#FFFF00"|transit

|1850

|0.84

|5148

|

Kepler-568b

|

|0.202

|11.02347475

|

|

|style="background:#FFFF00"|transit

|410

|0.55

|3768

|

Kepler-569b

|

|0.282

|34.18890521

|

|

|style="background:#FFFF00"|transit

|2100

|0.95

|5616

|

Kepler-570b

|

|0.219

|4.301662

|

|

|style="background:#FFFF00"|transit

|2090

|0.93

|5496

|

Kepler-571b

|

|0.236

|4.79859939

|

|

|style="background:#FFFF00"|transit

|2470

|0.93

|5527

|

Kepler-572b

|

|0.23

|17.20523483

|

|

|style="background:#FFFF00"|transit

|1740

|0.83

|5212

|

Kepler-573b

|

|0.249

|22.18329658

|

|

|style="background:#FFFF00"|transit

|2470

|0.99

|5746

|

Kepler-574b

|

|0.213

|7.65880414

|

|

|style="background:#FFFF00"|transit

|2440

|0.95

|5612

|

Kepler-575b

|

|0.213

|9.37891944

|

|

|style="background:#FFFF00"|transit

|2780

|0.97

|5710

|

Kepler-576b

|

|0.292

|29.91136794

|

|

|style="background:#FFFF00"|transit

|2280

|0.99

|5672

|

Kepler-577b

|

|0.227

|25.69578251

|

|

|style="background:#FFFF00"|transit

|1790

|0.78

|4984

|

Kepler-578b

|

|0.178

|1.6168837

|

|

|style="background:#FFFF00"|transit

|1850

|0.87

|5334

|

Kepler-579b

|

|0.178

|9.66857723

|

|

|style="background:#FFFF00"|transit

|2160

|0.99

|5636

|

Kepler-580b

|

|0.229

|8.22241966

|

|

|style="background:#FFFF00"|transit

|1090

|0.67

|4298

|

Kepler-581b

|

|0.235

|40.6069821

|

|

|style="background:#FFFF00"|transit

|2720

|1

|5772

|

Kepler-582b

|

|0.328

|18.49235668

|

|

|style="background:#FFFF00"|transit

|2450

|0.93

|5564

|

Kepler-583b

|

|0.203

|6.5100253

|

|

|style="background:#FFFF00"|transit

|2630

|0.94

|5523

|

Kepler-584b

|

|0.376

|35.1810304

|

|

|style="background:#FFFF00"|transit

|4710

|1.17

|6195

|

Kepler-585b

|

|0.252

|2.75235975

|

|

|style="background:#FFFF00"|transit

|1970

|0.96

|5593

|

Kepler-586b

|

|0.249

|2.10472218

|

|

|style="background:#FFFF00"|transit

|2310

|0.94

|5575

|

Kepler-587b

|

|0.199

|10.94027841

|

|

|style="background:#FFFF00"|transit

|2780

|0.92

|5549

|

Kepler-588b

|

|0.235

|4.22162536

|

|

|style="background:#FFFF00"|transit

|3170

|1.01

|5835

|

Kepler-589b

|

|0.203

|16.54964934

|

|

|style="background:#FFFF00"|transit

|2100

|0.88

|5296

|

Kepler-590b

|

|0.359

|5.85296257

|

|

|style="background:#FFFF00"|transit

|3220

|1.1

|6000

|

Kepler-591b

|

|0.302

|81.1694299

|

|

|style="background:#FFFF00"|transit

|2590

|0.97

|5677

|

Kepler-592b

|

|0.213

|2.82019241

|

|

|style="background:#FFFF00"|transit

|3370

|1.04

|5913

|

Kepler-593b

|

|0.256

|21.21708973

|

|

|style="background:#FFFF00"|transit

|3310

|1.08

|5967

|

Kepler-594b

|

|0.194

|13.64618192

|

|

|style="background:#FFFF00"|transit

|2420

|0.91

|5485

|

Kepler-595b

|

|0.34

|25.30292332

|

|

|style="background:#FFFF00"|transit

|2080

|0.87

|5247

|

Kepler-596b

|

|0.309

|21.30022655

|

|

|style="background:#FFFF00"|transit

|3530

|1.21

|6267

|

Kepler-597b

|

|0.211

|13.02365861

|

|

|style="background:#FFFF00"|transit

|2200

|0.97

|5683

|

Kepler-598b

|

|0.134

|3.70175428

|

|

|style="background:#FFFF00"|transit

|2240

|0.87

|5307

|

Kepler-599b

|

|0.253

|15.65562652

|

|

|style="background:#FFFF00"|transit

|2050

|0.83

|5127

|

Kepler-600b

|

|0.259

|23.67517607

|

|

|style="background:#FFFF00"|transit

|2040

|0.84

|5279

|

Kepler-601b

|

|0.17

|5.37886844

|

|

|style="background:#FFFF00"|transit

|1400

|0.85

|5160

|

Kepler-602b

|

|0.186

|15.28469497

|

|

|style="background:#FFFF00"|transit

|3170

|1.08

|6062

|

Kepler-603b

|

|0.236

|21.05358596

|

|

|style="background:#FFFF00"|transit

|3150

|1.01

|5808

|

Kepler-603c

|

|0.58

|127.9075774

|

|

|style="background:#FFFF00"|transit

|3150

|1.01

|5808

|

Kepler-603d

|

|0.118

|6.2171292

|

|

|style="background:#FFFF00"|transit

|3150

|1.01

|5808

|

Kepler-604b

|

|0.231

|25.85501786

|

|

|style="background:#FFFF00"|transit

|3200

|1.02

|5890

|

Kepler-605b

|

|0.128

|3.38353807

|

|

|style="background:#FFFF00"|transit

|1900

|0.91

|5462

|

Kepler-605c

|

|0.077

|2.35895152

|

|

|style="background:#FFFF00"|transit

|1900

|0.91

|5462

|

Kepler-606b

|

|0.295

|24.31575992

|

|

|style="background:#FFFF00"|transit

|3940

|1.13

|6161

|

Kepler-607b

|

|0.078

|0.6381632

|

|

|style="background:#FFFF00"|transit

|1600

|0.84

|5196

|

Kepler-608b

|

|0.325

|6.41251504

|

|

|style="background:#FFFF00"|transit

|3020

|1

|5820

|

Kepler-609b

|

|0.299

|6.52121067

|

|

|style="background:#FFFF00"|transit

|3730

|1.09

|5971

|

Kepler-610b

|

|0.374

|6.99692655

|

|

|style="background:#FFFF00"|transit

|3630

|1.1

|5943

|

Kepler-610c

|

|0.294

|151.86392

|

|

|style="background:#FFFF00"|transit

|3630

|1.1

|5943

|

Kepler-611b

|

|0.147

|2.4370333

|

|

|style="background:#FFFF00"|transit

|2950

|1.01

|5761

|

Kepler-612b

|

|0.253

|3.72215641

|

|

|style="background:#FFFF00"|transit

|3040

|0.98

|5693

|

Kepler-613b

|

|0.204

|15.77979614

|

|

|style="background:#FFFF00"|transit

|2820

|0.98

|5723

|

Kepler-614b

|

|0.213

|14.03491514

|

|

|style="background:#FFFF00"|transit

|1860

|0.85

|5268

|

Kepler-615b

|

|0.155

|10.35584657

|

|

|style="background:#FFFF00"|transit

|1100

|0.73

|4655

|

Kepler-616b

|

|0.217

|9.99761851

|

|

|style="background:#FFFF00"|transit

|3320

|0.98

|5753

|

Kepler-616c

|

|0.304

|90.4113556

|

|

|style="background:#FFFF00"|transit

|3320

|0.98

|5753

|

Kepler-617b

|

|0.118

|1.68269615

|

|

|style="background:#FFFF00"|transit

|490

|0.51

|3712

|

Kepler-618b

|

|0.232

|3.59576964

|

|

|style="background:#FFFF00"|transit

|3640

|1.05

|5860

|

Kepler-619b

|

|0.282

|5.4042722

|

|

|style="background:#FFFF00"|transit

|3620

|1.09

|5980

|

Kepler-619c

|

|0.151

|1.20846503

|

|

|style="background:#FFFF00"|transit

|3620

|1.09

|5980

|

Kepler-620b

|

|0.296

|12.91375431

|

|

|style="background:#FFFF00"|transit

|4050

|1.15

|6155

|

Kepler-621b

|

|0.205

|2.62811375

|

|

|style="background:#FFFF00"|transit

|1270

|0.72

|4521

|

Kepler-622b

|

|0.19

|14.28226676

|

|

|style="background:#FFFF00"|transit

|840

|0.64

|4201

|

Kepler-623b

|

|0.269

|9.07097734

|

|

|style="background:#FFFF00"|transit

|2650

|0.9

|5443

|

Kepler-624b

|

|0.206

|14.58649607

|

|

|style="background:#FFFF00"|transit

|2380

|1.1

|6117

|

Kepler-625b

|

|0.178

|7.75192492

|

|

|style="background:#FFFF00"|transit

|1640

|1.04

|5789

|

Kepler-625c

|

|0.094

|4.1653651

|

|

|style="background:#FFFF00"|transit

|1640

|1.04

|5789

|

Kepler-626b

|

|0.204

|14.48585199

|

|

|style="background:#FFFF00"|transit

|2300

|1.01

|5813

|

Kepler-627b

|

|0.333

|40.6994443

|

|

|style="background:#FFFF00"|transit

|3730

|1.3

|6424

|

Kepler-629b

|

|0.123

|7.2385854

|

|

|style="background:#FFFF00"|transit

|1250

|0.93

|5444

|

Kepler-630b

|

|0.284

|161.4743937

|

|

|style="background:#FFFF00"|transit

|2140

|1.02

|5829

|

Kepler-631b

|

|0.259

|17.97979059

|

|

|style="background:#FFFF00"|transit

|2750

|1.24

|6185

|

Kepler-632b

|

|0.197

|30.99660733

|

|

|style="background:#FFFF00"|transit

|1140

|0.91

|5322

|

Kepler-633b

|

|0.145

|8.50340718

|

|

|style="background:#FFFF00"|transit

|2070

|1.02

|5899

|

Kepler-634b

|

|0.169

|5.16950177

|

|

|style="background:#FFFF00"|transit

|2470

|1.03

|6075

|

Kepler-635b

|

|0.236

|23.44971004

|

|

|style="background:#FFFF00"|transit

|2690

|1.33

|6174

|

Kepler-636b

|

|0.397

|16.08066115

|

|

|style="background:#FFFF00"|transit

|1110

|0.85

|5203

|

Kepler-637b

|

|0.424

|23.20584623

|

|

|style="background:#FFFF00"|transit

|5140

|1.64

|6096

|

Kepler-638b

|

|0.163

|6.07972888

|

|

|style="background:#FFFF00"|transit

|1390

|0.88

|5382

|

Kepler-639b

|

|0.212

|10.21420496

|

|

|style="background:#FFFF00"|transit

|2200

|1.14

|5896

|

Kepler-640b

|

|0.228

|22.24813967

|

|

|style="background:#FFFF00"|transit

|1750

|1.01

|5653

|

Kepler-641b

|

|0.165

|9.48961571

|

|

|style="background:#FFFF00"|transit

|2200

|1.02

|5713

|

Kepler-642b

|

|0.259

|4.41745855

|

|

|style="background:#FFFF00"|transit

|3330

|1.4

|6570

|

Kepler-643b

|

|0.906

|16.33889626

|

|

|style="background:#FFFF00"|transit

|3360

|1

|4908

|

Kepler-644b

|

|0.281

|3.1739171

|

|

|style="background:#FFFF00"|transit

|4610

|1.49

|6747

|

Kepler-645b

|

|0.187

|3.27582262

|

|

|style="background:#FFFF00"|transit

|2940

|1.13

|6170

|

Kepler-646b

|

|0.178

|15.87364565

|

|

|style="background:#FFFF00"|transit

|1670

|0.93

|5634

|

Kepler-647b

|

|0.104

|16.2254649

|

|

|style="background:#FFFF00"|transit

|2570

|1.03

|6020

|

Kepler-648b

|

|0.287

|17.4211749

|

|

|style="background:#FFFF00"|transit

|2170

|1.05

|5741

|

Kepler-649b

|

|0.202

|29.90722674

|

|

|style="background:#FFFF00"|transit

|1710

|0.97

|5871

|

Kepler-650b

|

|0.264

|3.03214559

|

|

|style="background:#FFFF00"|transit

|2630

|1.08

|5849

|

Kepler-651b

|

|0.211

|21.38521506

|

|

|style="background:#FFFF00"|transit

|1750

|0.92

|5522

|

Kepler-652b

|

|0.222

|4.18200253

|

|

|style="background:#FFFF00"|transit

|1380

|0.97

|5490

|

Kepler-653b

|

|0.174

|14.70748976

|

|

|style="background:#FFFF00"|transit

|1930

|1.02

|5665

|

Kepler-653c

|

|0.07

|0.90037648

|

|

|style="background:#FFFF00"|transit

|1930

|1.02

|5665

|

Kepler-654b

|

|0.185

|13.72465129

|

|

|style="background:#FFFF00"|transit

|2160

|1.04

|5865

|

Kepler-655b

|

|0.242

|46.4063358

|

|

|style="background:#FFFF00"|transit

|2550

|1.15

|6170

|

Kepler-656b

|

|0.278

|1.26025909

|

|

|style="background:#FFFF00"|transit

|2830

|0.86

|5281

|

Kepler-657b

|

|0.314

|24.54350418

|

|

|style="background:#FFFF00"|transit

|4060

|1.01

|5808

|

Kepler-658b

|

|0.145

|1.28707676

|

|

|style="background:#FFFF00"|transit

|1110

|0.63

|4103

|

Kepler-659b

|

|0.223

|17.671796

|

|

|style="background:#FFFF00"|transit

|2240

|0.79

|4870

|

Kepler-660b

|

|0.229

|9.27358194

|

|

|style="background:#FFFF00"|transit

|1840

|0.75

|4779

|

Kepler-661b

|

|0.274

|6.02930132

|

|

|style="background:#FFFF00"|transit

|1820

|0.7

|4483

|

Kepler-662b

|

|0.194

|21.67697486

|

|

|style="background:#FFFF00"|transit

|2090

|0.79

|4897

|

Kepler-663b

|

|0.232

|4.99678284

|

|

|style="background:#FFFF00"|transit

|3400

|0.86

|5264

|

Kepler-664b

|

|0.237

|2.52559332

|

|

|style="background:#FFFF00"|transit

|4520

|1.01

|5754

|

Kepler-665b

|

|0.232

|16.01310205

|

|

|style="background:#FFFF00"|transit

|2120

|0.79

|4913

|

Kepler-666b

|

|0.214

|4.49876092

|

|

|style="background:#FFFF00"|transit

|4300

|1.03

|5887

|

Kepler-667b

|

|0.422

|41.43962808

|

|

|style="background:#FFFF00"|transit

|2960

|0.91

|5327

|

Kepler-668b

|

|0.241

|8.35390639

|

|

|style="background:#FFFF00"|transit

|2860

|0.87

|5352

|

Kepler-669b

|

|0.431

|4.12554687

|

|

|style="background:#FFFF00"|transit

|5800

|1.15

|6038

|

Kepler-670b

|

|1.176

|2.81650485

|

|

|style="background:#FFFF00"|transit

|3200

|0.99

|5709

|

Kepler-671b

|

|0.24

|4.28095859

|

|

|style="background:#FFFF00"|transit

|3710

|0.97

|5624

|

Kepler-672b

|

|0.223

|38.3774623

|

|

|style="background:#FFFF00"|transit

|3300

|0.95

|5627

|

Kepler-673b

|

|0.583

|3.72873109

|

|

|style="background:#FFFF00"|transit

|3190

|0.88

|5355

|

Kepler-674b

|

|0.151

|2.24338185

|

|

|style="background:#FFFF00"|transit

|980

|0.6

|4192

|

Kepler-675b

|

|0.218

|2.33743801

|

|

|style="background:#FFFF00"|transit

|2120

|0.79

|4945

|

Kepler-676b

|

|0.271

|11.59822172

|

|

|style="background:#FFFF00"|transit

|790

|0.51

|3701

|

Kepler-677b

|

|0.48

|6.57531678

|

|

|style="background:#FFFF00"|transit

|3800

|1

|5723

|

Kepler-678b

|

|0.459

|7.27503724

|

|

|style="background:#FFFF00"|transit

|2850

|0.94

|5520

|

Kepler-679b

|

|0.269

|12.39358604

|

|

|style="background:#FFFF00"|transit

|3160

|0.87

|5403

|

Kepler-680b

|

|0.216

|3.68992629

|

|

|style="background:#FFFF00"|transit

|4380

|1.08

|5890

|

Kepler-681b

|

|0.275

|26.39435646

|

|

|style="background:#FFFF00"|transit

|2170

|0.8

|5021

|

Kepler-682b

|

|0.658

|12.61190667

|

|

|style="background:#FFFF00"|transit

|3100

|0.92

|5559

|

Kepler-683b

|

|0.176

|2.53918318

|

|

|style="background:#FFFF00"|transit

|3180

|0.96

|5703

|

Kepler-684b

|

|0.3

|6.77030201

|

|

|style="background:#FFFF00"|transit

|3480

|0.89

|5493

|

Kepler-685b

|

|0.944

|1.6255222

|

|

|style="background:#FFFF00"|transit

|3730

|1.11

|5963

|

Kepler-686b

|

|1.084

|1.59474546

|

|

|style="background:#FFFF00"|transit

|3920

|0.94

|5649

|

Kepler-687b

|

|0.314

|20.50586978

|

|

|style="background:#FFFF00"|transit

|2050

|0.77

|4841

|

Kepler-688b

|

|0.871

|3.89593684

|

|

|style="background:#FFFF00"|transit

|4070

|0.98

|5715

|

Kepler-689b

|

|0.258

|22.36656079

|

|

|style="background:#FFFF00"|transit

|3410

|0.91

|5518

|

Kepler-690b

|

|0.531

|7.74809437

|

|

|style="background:#FFFF00"|transit

|5390

|1.11

|5913

|

Kepler-691b

|

|0.186

|8.114379

|

|

|style="background:#FFFF00"|transit

|780

|0.53

|3715

|

Kepler-692b

|

|0.277

|21.81293494

|

|

|style="background:#FFFF00"|transit

|3300

|0.9

|5440

|

Kepler-693b

|

|0.908

|15.37563332

|

|

|style="background:#FFFF00"|transit

|3270

|0.76

|4881

|

Kepler-694b

|

|0.25

|6.36584161

|

|

|style="background:#FFFF00"|transit

|3340

|0.97

|5700

|

Kepler-695b

|

|0.822

|3.04033042

|

|

|style="background:#FFFF00"|transit

|2000

|0.84

|5181

|

Kepler-696b

|

|0.548

|4.19042557

|

|

|style="background:#FFFF00"|transit

|4190

|1.06

|5903

|

Kepler-697b

|

|0.368

|3.70987065

|

|

|style="background:#FFFF00"|transit

|3560

|0.92

|5513

|

Kepler-698b

|

|0.328

|16.32976218

|

|

|style="background:#FFFF00"|transit

|3700

|0.94

|5612

|

Kepler-700b

|

|0.534

|80.8720639

|

|

|style="background:#FFFF00"|transit

|3460

|0.98

|5692

|

Kepler-701b

|

|0.253

|10.35533177

|

|

|style="background:#FFFF00"|transit

|2460

|0.88

|5343

|

Kepler-702b

|

|0.818

|10.52629406

|

|

|style="background:#FFFF00"|transit

|2910

|0.9

|5419

|

Kepler-703b

|

|0.732

|4.58352176

|

|

|style="background:#FFFF00"|transit

|4830

|1.18

|6185

|

Kepler-704b

|

|0.233

|3.76182115

|

|

|style="background:#FFFF00"|transit

|3440

|0.97

|5616

|

{{vanchor|Kepler-705b}}

|

|0.188

|56.0560538

|

|

|style="background:#FFFF00"|transit

|820

|0.53

|3722

| Potentially habitable exoplanet

Kepler-707b

|

|0.119

|2.23749275

|

|

|style="background:#FFFF00"|transit

|2040

|0.8

|5099

|

Kepler-708b

|

|0.261

|3.16789194

|

|

|style="background:#FFFF00"|transit

|4050

|0.97

|5692

|

Kepler-709b

|

|0.261

|16.08524954

|

|

|style="background:#FFFF00"|transit

|2180

|0.8

|5071

|

Kepler-710b

|

|0.168

|4.34728553

|

|

|style="background:#FFFF00"|transit

|3000

|0.94

|5611

|

Kepler-711b

|

|0.304

|23.58914398

|

|

|style="background:#FFFF00"|transit

|2170

|0.84

|5222

|

Kepler-712b

|

|0.304

|21.02247699

|

|

|style="background:#FFFF00"|transit

|3080

|0.84

|5148

|

Kepler-712c

|

|0.433

|226.89047

|

|

|style="background:#FFFF00"|transit

|3080

|0.84

|5148

|

Kepler-713b

|

|0.221

|7.411141

|

|

|style="background:#FFFF00"|transit

|3270

|0.98

|5785

|

Kepler-714b

|

|0.863

|8.09888799

|

|

|style="background:#FFFF00"|transit

|4800

|1.09

|5995

|

Kepler-715b

|

|0.335

|10.00652995

|

|

|style="background:#FFFF00"|transit

|3960

|1.04

|5871

|

Kepler-716b

|

|0.259

|10.37168453

|

|

|style="background:#FFFF00"|transit

|2200

|0.83

|5099

|

Kepler-717b

|

|0.216

|4.40840023

|

|

|style="background:#FFFF00"|transit

|3670

|0.88

|5485

|

Kepler-718b

|

|1.477

|2.0523499

|

|

|style="background:#FFFF00"|transit

|5000

|1.18

|6191

|

Kepler-719b

|

|0.76

|5.00731778

|

|

|style="background:#FFFF00"|transit

|4650

|0.99

|5777

|

Kepler-720b

|

|0.75

|4.70832654

|

|

|style="background:#FFFF00"|transit

|2900

|0.95

|5618

|

Kepler-721b

|

|0.236

|5.39202539

|

|

|style="background:#FFFF00"|transit

|2770

|0.82

|5075

|

Kepler-722b

|

|0.235

|4.09357325

|

|

|style="background:#FFFF00"|transit

|4480

|1.03

|5863

|

Kepler-722c

|

|0.252

|105.144749

|

|

|style="background:#FFFF00"|transit

|4480

|1.03

|5863

|

Kepler-723b

|

|1.088

|4.08227507

|

|

|style="background:#FFFF00"|transit

|3150

|0.92

|5539

|

Kepler-724b

|

|0.294

|3.31494634

|

|

|style="background:#FFFF00"|transit

|2810

|0.9

|5437

|

Kepler-725b

|

|0.948

|39.64317811

|

|

|style="background:#FFFF00"|transit

|2540

|0.88

|5363

|

Kepler-726b

|

|0.291

|21.80451088

|

|

|style="background:#FFFF00"|transit

|2730

|0.88

|5452

|

Kepler-727b

|

|0.226

|5.15448442

|

|

|style="background:#FFFF00"|transit

|2910

|0.89

|5441

|

Kepler-728b

|

|0.298

|5.74347727

|

|

|style="background:#FFFF00"|transit

|4030

|0.95

|5660

|

Kepler-729b

|

|0.319

|3.16635371

|

|

|style="background:#FFFF00"|transit

|4150

|0.94

|5633

|

Kepler-730b

|

|0.822

|6.49168426

|

|

|style="background:#FFFF00"|transit

|4750

|1

|5726

|

Kepler-731b

|

|1.238

|3.85560355

|

|

|style="background:#FFFF00"|transit

|4280

|1.03

|5849

|

Kepler-732b

|

|0.194

|9.46781405

|

|

|style="background:#FFFF00"|transit

|490

|0.49

|3631

|

Kepler-732c

|

|0.113

|0.89304124

|

|

|style="background:#FFFF00"|transit

|490

|0.49

|3631

|

Kepler-733b

|

|0.252

|20.83424726

|

|

|style="background:#FFFF00"|transit

|3200

|0.9

|5418

|

Kepler-734b

|

|0.318

|6.10485286

|

|

|style="background:#FFFF00"|transit

|1800

|0.85

|5326

|

Kepler-735b

|

|0.263

|11.51516988

|

|

|style="background:#FFFF00"|transit

|2600

|0.85

|5107

|

Kepler-736b

|

|0.261

|3.60147201

|

|

|style="background:#FFFF00"|transit

|3280

|0.86

|5217

|

Kepler-737b

|

|0.175

|28.59915399

|

|

|style="background:#FFFF00"|transit

|640

|0.51

|3813

|

Kepler-738b

|

|0.223

|24.58721573

|

|

|style="background:#FFFF00"|transit

|3240

|0.86

|5327

|

Kepler-739b

|

|0.296

|12.53248465

|

|

|style="background:#FFFF00"|transit

|3680

|0.93

|5601

|

Kepler-740b

|

|0.408

|3.58410122

|

|

|style="background:#FFFF00"|transit

|4120

|0.91

|5438

|

Kepler-741b

|

|0.265

|7.03902374

|

|

|style="background:#FFFF00"|transit

|5000

|1.16

|6129

|

Kepler-742b

|

|0.289

|8.36086824

|

|

|style="background:#FFFF00"|transit

|1630

|0.76

|4642

|

Kepler-743b

|

|0.108

|3.17926292

|

|

|style="background:#FFFF00"|transit

|840

|0.94

|5486

|

Kepler-744b

|

|0.145

|12.06222443

|

|

|style="background:#FFFF00"|transit

|1590

|0.94

|5594

|

Kepler-745b

|

|0.193

|9.93143556

|

|

|style="background:#FFFF00"|transit

|3910

|1.04

|5849

|

Kepler-746b

|

|0.099

|3.48159251

|

|

|style="background:#FFFF00"|transit

|1500

|0.91

|5418

|

Kepler-747b

|

|0.47

|35.61760587

|

|

|style="background:#FFFF00"|transit

|2790

|0.82

|5096

| May not be a planet

Kepler-748b

|

|0.225

|7.40742793

|

|

|style="background:#FFFF00"|transit

|4150

|1.07

|5934

|

Kepler-749b

|

|0.277

|17.31716585

|

|

|style="background:#FFFF00"|transit

|2460

|0.79

|5009

|

Kepler-750b

|

|0.274

|9.42887179

|

|

|style="background:#FFFF00"|transit

|3850

|1.15

|6160

|

Kepler-750c

|

|0.145

|4.08899022

|

|

|style="background:#FFFF00"|transit

|3850

|1.15

|6160

|

Kepler-751b

|

|0.219

|17.44490636

|

|

|style="background:#FFFF00"|transit

|2440

|0.87

|5387

|

Kepler-752b

|

|0.251

|18.82747265

|

|

|style="background:#FFFF00"|transit

|3510

|0.87

|5373

|

Kepler-753b

|

|0.17

|5.74772501

|

|

|style="background:#FFFF00"|transit

|910

|0.68

|4346

|

Kepler-754b

|

|0.179

|14.5596237

|

|

|style="background:#FFFF00"|transit

|3890

|1.06

|5935

|

Kepler-755b

|

|0.157

|1.26909037

|

|

|style="background:#FFFF00"|transit

|1200

|0.82

|5043

|

Kepler-755c

|

|0.112

|2.85313364

|

|

|style="background:#FFFF00"|transit

|1200

|0.82

|5043

|

Kepler-756b

|

|0.1

|1.22486632

|

|

|style="background:#FFFF00"|transit

|2780

|0.82

|5282

|

Kepler-757b

|

|0.121

|1.02267882

|

|

|style="background:#FFFF00"|transit

|3310

|1.08

|6014

|

Kepler-758b

|

|0.221

|12.1097104

|

|

|style="background:#FFFF00"|transit

|4410

|1.16

|6228

|

Kepler-758c

|

|0.151

|4.75793986

|

|

|style="background:#FFFF00"|transit

|4410

|1.16

|6228

|

Kepler-758d

|

|0.189

|20.4966197

|

|

|style="background:#FFFF00"|transit

|4410

|1.16

|6228

|

Kepler-758e

|

|0.136

|8.1934719

|

|

|style="background:#FFFF00"|transit

|4410

|1.16

|6228

|

Kepler-759b

|

|0.203

|41.805985

|

|

|style="background:#FFFF00"|transit

|2910

|1.04

|5860

|

Kepler-760b

|

|0.273

|8.70419416

|

|

|style="background:#FFFF00"|transit

|2550

|0.89

|5322

|

Kepler-760c

|

|0.132

|2.46697439

|

|

|style="background:#FFFF00"|transit

|2550

|0.89

|5322

|

Kepler-761b

|

|0.181

|10.12804789

|

|

|style="background:#FFFF00"|transit

|2830

|0.95

|5706

|

Kepler-762b

|

|1.131

|3.7705521

|

|

|style="background:#FFFF00"|transit

|4780

|1.06

|5944

|

Kepler-763b

|

|0.109

|1.19655156

|

|

|style="background:#FFFF00"|transit

|2940

|0.84

|5166

|

Kepler-764b

|

|0.146

|7.33683936

|

|

|style="background:#FFFF00"|transit

|3300

|0.92

|5557

|

Kepler-765b

|

|0.217

|27.6655226

|

|

|style="background:#FFFF00"|transit

|3300

|1.05

|5901

|

Kepler-766b

|

|0.302

|6.10027804

|

|

|style="background:#FFFF00"|transit

|5260

|1.1

|5992

|

Kepler-767b

|

|0.592

|161.5280101

|

|

|style="background:#FFFF00"|transit

|3860

|0.96

|5694

|

Kepler-768b

|

|0.16

|11.3910025

|

|

|style="background:#FFFF00"|transit

|2590

|0.82

|5108

|

Kepler-769b

|

|0.261

|7.42608998

|

|

|style="background:#FFFF00"|transit

|4440

|1.19

|6186

|

Kepler-769c

|

|0.16

|15.9870174

|

|

|style="background:#FFFF00"|transit

|4440

|1.19

|6186

|

Kepler-770b

|

|0.205

|18.92540274

|

|

|style="background:#FFFF00"|transit

|2480

|0.94

|5598

|

Kepler-770c

|

|0.107

|1.47532231

|

|

|style="background:#FFFF00"|transit

|2480

|0.94

|5598

|

Kepler-770d

|

|0.125

|4.15244722

|

|

|style="background:#FFFF00"|transit

|2480

|0.94

|5598

|

Kepler-771b

|

|0.162

|8.73485836

|

|

|style="background:#FFFF00"|transit

|3300

|1.03

|5906

|

Kepler-772b

|

|0.162

|12.99207337

|

|

|style="background:#FFFF00"|transit

|2250

|0.98

|5714

|

Kepler-773b

|

|0.128

|3.74910006

|

|

|style="background:#FFFF00"|transit

|1720

|1.04

|5850

|

Kepler-774b

|

|0.283

|11.0895723

|

|

|style="background:#FFFF00"|transit

|3900

|1.57

|6403

|

Kepler-775b

|

|0.106

|0.97486893

|

|

|style="background:#FFFF00"|transit

|1300

|0.92

|5468

|

Kepler-776b

|

|0.114

|4.89718784

|

|

|style="background:#FFFF00"|transit

|2370

|0.83

|5071

|

Kepler-777b

|

|0.131

|5.72812599

|

|

|style="background:#FFFF00"|transit

|1250

|0.58

|4043

|

Kepler-778b

|

|0.15

|3.75574426

|

|

|style="background:#FFFF00"|transit

|2930

|0.81

|5102

|

Kepler-779b

|

|0.082

|7.09714223

|

|

|style="background:#FFFF00"|transit

|730

|0.46

|3804

|

Kepler-780b

|

|0.079

|0.67737516

|

|

|style="background:#FFFF00"|transit

|1700

|1.01

|5769

|

Kepler-781b

|

|0.258

|13.2140732

|

|

|style="background:#FFFF00"|transit

|3380

|0.81

|5162

|

Kepler-782b

|

|0.286

|158.6853308

|

|

|style="background:#FFFF00"|transit

|1340

|0.98

|5867

|

Kepler-783b

|

|0.07

|4.29264638

|

|

|style="background:#FFFF00"|transit

|1770

|0.93

|5521

|

Kepler-784b

|

|0.141

|31.5922646

|

|

|style="background:#FFFF00"|transit

|1970

|1

|5674

|

Kepler-785b

|

|1.162

|1.97376093

|

|

|style="background:#FFFF00"|transit

|2170

|0.77

|4739

|

Kepler-786b

|

|0.217

|53.5293487

|

|

|style="background:#FFFF00"|transit

|1670

|0.81

|4838

|

Kepler-787b

|

|0.114

|0.9283105

|

|

|style="background:#FFFF00"|transit

|1530

|0.65

|4248

|

Kepler-788b

|

|0.227

|8.39846269

|

|

|style="background:#FFFF00"|transit

|5380

|1.16

|6159

|

Kepler-789b

|

|0.189

|8.63847725

|

|

|style="background:#FFFF00"|transit

|2980

|1.01

|5870

|

Kepler-790b

|

|0.194

|13.73469807

|

|

|style="background:#FFFF00"|transit

|2370

|0.84

|5208

|

Kepler-791b

|

|0.272

|14.5539759

|

|

|style="background:#FFFF00"|transit

|4720

|1.3

|6383

|

Kepler-792b

|

|0.175

|11.30119217

|

|

|style="background:#FFFF00"|transit

|3930

|1.09

|5971

|

Kepler-793b

|

|0.122

|4.24153639

|

|

|style="background:#FFFF00"|transit

|2590

|0.98

|5745

|

Kepler-794b

|

|0.188

|11.13125132

|

|

|style="background:#FFFF00"|transit

|2490

|1.19

|5839

|

Kepler-795b

|

|0.15

|29.6193421

|

|

|style="background:#FFFF00"|transit

|1490

|0.94

|5631

|

Kepler-796b

|

|0.116

|6.40087618

|

|

|style="background:#FFFF00"|transit

|1230

|0.93

|5475

|

Kepler-797b

|

|0.194

|27.07237711

|

|

|style="background:#FFFF00"|transit

|2450

|0.96

|5680

|

Kepler-798b

|

|0.213

|13.71933369

|

|

|style="background:#FFFF00"|transit

|3540

|1.19

|6224

|

Kepler-799b

|

|0.614

|133.4605235

|

|

|style="background:#FFFF00"|transit

|3360

|0.95

|5681

|

Kepler-800b

|

|0.254

|14.13176026

|

|

|style="background:#FFFF00"|transit

|3420

|0.85

|5315

|

Kepler-801b

|

|0.178

|11.41928253

|

|

|style="background:#FFFF00"|transit

|1370

|0.67

|4435

|

Kepler-802b

|

|0.316

|40.0587473

|

|

|style="background:#FFFF00"|transit

|2700

|0.93

|5507

|

Kepler-803b

|

|0.338

|50.28638192

|

|

|style="background:#FFFF00"|transit

|2010

|1.05

|5919

|

Kepler-804b

|

|0.173

|14.37457351

|

|

|style="background:#FFFF00"|transit

|2110

|1.01

|5817

|

Kepler-804c

|

|0.102

|9.65185017

|

|

|style="background:#FFFF00"|transit

|2110

|1.01

|5817

|

Kepler-805b

|

|0.258

|30.8638931

|

|

|style="background:#FFFF00"|transit

|2140

|1.19

|6112

|

Kepler-806b

|

|0.102

|8.09219642

|

|

|style="background:#FFFF00"|transit

|850

|0.99

|5770

|

Kepler-808b

|

|0.13

|0.63133235

|

|

|style="background:#FFFF00"|transit

|1050

|0.76

|4653

|

Kepler-809b

|

|0.269

|55.63934

|

|

|style="background:#FFFF00"|transit

|3040

|0.99

|5734

|

Kepler-810b

|

|0.172

|4.59725385

|

|

|style="background:#FFFF00"|transit

|5070

|1.03

|5803

|

Kepler-811b

|

|0.241

|23.58447697

|

|

|style="background:#FFFF00"|transit

|2760

|1.01

|5747

|

Kepler-812b

|

|0.317

|10.11716531

|

|

|style="background:#FFFF00"|transit

|4830

|1.45

|6761

|

Kepler-813b

|

|0.191

|19.12947337

|

|

|style="background:#FFFF00"|transit

|2700

|0.95

|5743

|

Kepler-814b

|

|0.189

|6.1469851

|

|

|style="background:#FFFF00"|transit

|4330

|1.15

|6162

|

Kepler-815b

|

|0.367

|8.57503552

|

|

|style="background:#FFFF00"|transit

|3910

|1.25

|5028

|

Kepler-816b

|

|0.914

|10.50682565

|

|

|style="background:#FFFF00"|transit

|3450

|0.9

|5286

|

Kepler-817b

|

|0.806

|3.99010623

|

|

|style="background:#FFFF00"|transit

|4570

|1.03

|5861

|

Kepler-818b

|

|0.456

|10.03538581

|

|

|style="background:#FFFF00"|transit

|3150

|0.94

|5638

|

Kepler-819b

|

|0.246

|33.1995648

|

|

|style="background:#FFFF00"|transit

|2350

|0.86

|5279

|

Kepler-820b

|

|0.543

|127.8338098

|

|

|style="background:#FFFF00"|transit

|3230

|1.23

|6260

|

Kepler-821b

|

|0.117

|1.92279873

|

|

|style="background:#FFFF00"|transit

|2020

|0.84

|5191

|

Kepler-822b

|

|0.158

|3.22296927

|

|

|style="background:#FFFF00"|transit

|3120

|1.06

|5928

|

Kepler-823b

|

|0.14

|4.16809082

|

|

|style="background:#FFFF00"|transit

|2920

|0.98

|5643

|

Kepler-824b

|

|0.167

|4.51436633

|

|

|style="background:#FFFF00"|transit

|4410

|1.15

|6035

|

Kepler-825b

|

|0.136

|3.77360059

|

|

|style="background:#FFFF00"|transit

|2700

|1.03

|5976

|

Kepler-825c

|

|0.164

|8.1818246

|

|

|style="background:#FFFF00"|transit

|2700

|1.03

|5976

|

Kepler-826b

|

|0.112

|4.48758907

|

|

|style="background:#FFFF00"|transit

|2120

|1.05

|6079

|

Kepler-827b

|

|0.502

|51.92927591

|

|

|style="background:#FFFF00"|transit

|4410

|0.93

|5602

|

Kepler-828b

|

|0.135

|0.56785714

|

|

|style="background:#FFFF00"|transit

|2040

|0.81

|5039

|

Kepler-829b

|

|0.188

|6.88337562

|

|

|style="background:#FFFF00"|transit

|3110

|0.98

|5698

|

Kepler-830b

|

|0.152

|11.29695137

|

|

|style="background:#FFFF00"|transit

|3660

|1.07

|6037

|

Kepler-831b

|

|0.113

|5.62153941

|

|

|style="background:#FFFF00"|transit

|1880

|0.99

|5732

|

Kepler-832b

|

|0.184

|7.1396941

|

|

|style="background:#FFFF00"|transit

|4390

|0.92

|5596

|

Kepler-833b

|

|0.18

|18.7546998

|

|

|style="background:#FFFF00"|transit

|1370

|0.64

|4339

|

Kepler-834b

|

|0.18

|13.32388301

|

|

|style="background:#FFFF00"|transit

|2000

|0.7

|4554

|

Kepler-835b

|

|0.249

|11.41909375

|

|

|style="background:#FFFF00"|transit

|6560

|1.08

|5954

|

Kepler-836b

|

|0.244

|11.36112327

|

|

|style="background:#FFFF00"|transit

|3270

|1.03

|5895

|

Kepler-837b

|

|0.228

|16.56059504

|

|

|style="background:#FFFF00"|transit

|2760

|0.85

|5403

|

Kepler-838b

|

|0.244

|15.74957994

|

|

|style="background:#FFFF00"|transit

|3900

|0.98

|5770

|

Kepler-839b

|

|0.229

|37.8144514

|

|

|style="background:#FFFF00"|transit

|2720

|1.22

|6058

|

Kepler-841b

|

|0.467

|124.4198398

|

|

|style="background:#FFFF00"|transit

|3430

|0.85

|5324

|

Kepler-842b

|

|0.143

|1.21956827

|

|

|style="background:#FFFF00"|transit

|1800

|0.78

|4848

|

Kepler-843b

|

|0.231

|2.05387982

|

|

|style="background:#FFFF00"|transit

|4070

|1.02

|5830

|

Kepler-844b

|

|0.15

|2.61302086

|

|

|style="background:#FFFF00"|transit

|1290

|0.59

|4128

|

Kepler-845b

|

|0.182

|0.92785982

|

|

|style="background:#FFFF00"|transit

|1540

|0.79

|4913

|

Kepler-846b

|

|0.221

|19.80792185

|

|

|style="background:#FFFF00"|transit

|4020

|0.94

|5579

|

Kepler-847b

|

|0.105

|2.3432319

|

|

|style="background:#FFFF00"|transit

|1730

|0.83

|4940

|

Kepler-848b

|

|0.152

|6.91134416

|

|

|style="background:#FFFF00"|transit

|2600

|1.01

|5695

|

Kepler-849b

|

|0.637

|394.6244904

|

|

|style="background:#FFFF00"|transit

|2440

|1.23

|6059

|

Kepler-850b

|

|0.159

|7.19303878

|

|

|style="background:#FFFF00"|transit

|5010

|1.06

|5932

|

Kepler-851b

|

|0.15

|8.50699658

|

|

|style="background:#FFFF00"|transit

|2830

|0.89

|5455

|

Kepler-852b

|

|0.227

|44.9309804

|

|

|style="background:#FFFF00"|transit

|2790

|1.19

|6100

|

Kepler-853b

|

|0.151

|7.16892463

|

|

|style="background:#FFFF00"|transit

|2000

|1.3

|6350

|

Kepler-855b

|

|0.745

|7.8866311

|

|

|style="background:#FFFF00"|transit

|3400

|1.03

|5835

|

Kepler-856b

|

|0.83

|8.02768059

|

|

|style="background:#FFFF00"|transit

|3830

|0.96

|5535

|

Kepler-857b

|

|0.607

|85.35129427

|

|

|style="background:#FFFF00"|transit

|3390

|0.99

|5773

|

Kepler-858b

|

|0.434

|76.13602028

|

|

|style="background:#FFFF00"|transit

|970

|0.96

|5653

|

Kepler-859b

|

|0.276

|20.38177573

|

|

|style="background:#FFFF00"|transit

|2980

|0.81

|5020

|

Kepler-860b

|

|0.289

|5.10137945

|

|

|style="background:#FFFF00"|transit

|4220

|1.04

|5836

|

Kepler-861b

|

|0.203

|3.94963138

|

|

|style="background:#FFFF00"|transit

|2630

|0.82

|5047

|

Kepler-862b

|

|0.197

|3.14866453

|

|

|style="background:#FFFF00"|transit

|2630

|0.88

|5333

|

Kepler-863b

|

|0.259

|15.59461874

|

|

|style="background:#FFFF00"|transit

|3730

|0.96

|5678

|

Kepler-864b

|

|0.214

|5.83376092

|

|

|style="background:#FFFF00"|transit

|5130

|1

|5754

|

Kepler-865b

|

|0.222

|14.16399294

|

|

|style="background:#FFFF00"|transit

|2170

|0.93

|5570

|

Kepler-866b

|

|0.145

|2.61703254

|

|

|style="background:#FFFF00"|transit

|2300

|0.75

|4751

|

Kepler-867b

|

|0.414

|150.242127

|

|

|style="background:#FFFF00"|transit

|2690

|0.92

|5541

|

Kepler-868b

|

|0.183

|5.03251791

|

|

|style="background:#FFFF00"|transit

|4140

|0.93

|5614

|

Kepler-869b

|

|0.322

|40.4287755

|

|

|style="background:#FFFF00"|transit

|3120

|0.97

|5664

|

Kepler-870b

|

|0.248

|21.3587621

|

|

|style="background:#FFFF00"|transit

|4010

|1.01

|5857

|

Kepler-871b

|

|0.334

|22.0459018

|

|

|style="background:#FFFF00"|transit

|5530

|1.11

|5993

|

Kepler-872b

|

|0.178

|2.57885507

|

|

|style="background:#FFFF00"|transit

|3630

|1.05

|5902

|

Kepler-873b

|

|0.335

|20.5533844

|

|

|style="background:#FFFF00"|transit

|4560

|1.18

|6163

|

Kepler-874b

|

|0.352

|40.0686727

|

|

|style="background:#FFFF00"|transit

|3500

|1.09

|6020

|

Kepler-875b

|

|0.259

|27.5073799

|

|

|style="background:#FFFF00"|transit

|4060

|1.06

|5958

|

Kepler-876b

|

|0.128

|5.14438011

|

|

|style="background:#FFFF00"|transit

|2400

|0.81

|5060

|

Kepler-877b

|

|0.189

|18.45847097

|

|

|style="background:#FFFF00"|transit

|1870

|0.85

|5261

|

Kepler-878b

|

|0.172

|25.9422033

|

|

|style="background:#FFFF00"|transit

|1850

|0.81

|5044

|

Kepler-879b

|

|0.229

|33.3855938

|

|

|style="background:#FFFF00"|transit

|2520

|1.02

|5792

|

Kepler-880b

|

|0.237

|7.71468975

|

|

|style="background:#FFFF00"|transit

|2200

|1.46

|6761

|

Kepler-881b

|

|0.159

|4.44448017

|

|

|style="background:#FFFF00"|transit

|4450

|1.06

|5961

|

Kepler-882b

|

|0.11

|3.98953967

|

|

|style="background:#FFFF00"|transit

|1710

|0.9

|5476

|

Kepler-883b

|

|0.159

|12.98495573

|

|

|style="background:#FFFF00"|transit

|1790

|1.06

|6116

|

Kepler-884b

|

|0.11

|5.69919514

|

|

|style="background:#FFFF00"|transit

|1400

|1

|5715

|

Kepler-885b

|

|0.223

|18.11472949

|

|

|style="background:#FFFF00"|transit

|2060

|1.21

|6187

|

Kepler-886b

|

|0.136

|6.24146367

|

|

|style="background:#FFFF00"|transit

|2800

|1.1

|6098

|

Kepler-887b

|

|0.164

|20.42228798

|

|

|style="background:#FFFF00"|transit

|2710

|1.19

|6194

|

Kepler-887c

|

|0.101

|7.63846023

|

|

|style="background:#FFFF00"|transit

|2710

|1.19

|6194

|

Kepler-888b

|

|0.157

|70.6979061

|

|

|style="background:#FFFF00"|transit

|1350

|0.97

|5875

|

Kepler-889b

|

|0.097

|3.744439

|

|

|style="background:#FFFF00"|transit

|1670

|1.14

|5961

|

Kepler-890b

|

|0.793

|52.75875577

|

|

|style="background:#FFFF00"|transit

|4520

|1.09

|5954

|

Kepler-891b

|

|0.572

|53.44945593

|

|

|style="background:#FFFF00"|transit

|4470

|1.06

|5887

|

Kepler-892b

|

|0.251

|13.7521072

|

|

|style="background:#FFFF00"|transit

|2100

|0.75

|4747

|

Kepler-893b

|

|0.27

|6.33855761

|

|

|style="background:#FFFF00"|transit

|3970

|1

|5820

|

Kepler-894b

|

|0.248

|9.803224

|

|

|style="background:#FFFF00"|transit

|3600

|0.87

|5603

|

Kepler-895b

|

|0.137

|2.80624233

|

|

|style="background:#FFFF00"|transit

|1680

|0.65

|4315

|

Kepler-896b

|

|0.226

|144.547396

|

|

|style="background:#FFFF00"|transit

|2920

|0.84

|5262

|

Kepler-897b

|

|0.213

|8.0472642

|

|

|style="background:#FFFF00"|transit

|3740

|1.03

|5839

|

Kepler-898b

|

|0.133

|5.8706191

|

|

|style="background:#FFFF00"|transit

|1560

|0.65

|4223

|

Kepler-899b

|

|0.239

|19.17891293

|

|

|style="background:#FFFF00"|transit

|3390

|0.93

|5595

|

Kepler-900b

|

|0.186

|6.9913086

|

|

|style="background:#FFFF00"|transit

|1650

|0.78

|4836

|

Kepler-901b

|

|0.122

|3.51749439

|

|

|style="background:#FFFF00"|transit

|790

|0.59

|4184

|

Kepler-902b

|

|0.227

|40.1099547

|

|

|style="background:#FFFF00"|transit

|2950

|0.95

|5647

|

Kepler-903b

|

|0.179

|10.3507721

|

|

|style="background:#FFFF00"|transit

|2700

|0.98

|5682

|

Kepler-903c

|

|0.226

|62.9228557

|

|

|style="background:#FFFF00"|transit

|2700

|0.98

|5682

|

Kepler-904b

|

|0.158

|3.02166863

|

|

|style="background:#FFFF00"|transit

|3750

|1.16

|6160

|

Kepler-905b

|

|0.126

|5.08274652

|

|

|style="background:#FFFF00"|transit

|1700

|0.95

|5461

|

Kepler-906b

|

|0.188

|41.6979976

|

|

|style="background:#FFFF00"|transit

|2470

|1.06

|6035

|

Kepler-907b

|

|0.107

|15.86621821

|

|

|style="background:#FFFF00"|transit

|1150

|1.08

|6106

|

Kepler-908b

|

|0.109

|1.34059747

|

|

|style="background:#FFFF00"|transit

|820

|1.11

|5973

|

Kepler-909b

|

|0.131

|13.93290318

|

|

|style="background:#FFFF00"|transit

|1040

|1.17

|6154

|

Kepler-910b

|

|0.073

|2.36436901

|

|

|style="background:#FFFF00"|transit

|1310

|1.26

|6230

|

Kepler-911b

|

|0.232

|20.310501

|

|

|style="background:#FFFF00"|transit

|1850

|1.34

|6112

|

Kepler-912b

|

|0.25

|2.53475627

|

|

|style="background:#FFFF00"|transit

|4130

|1.07

|5998

|

Kepler-913b

|

|0.184

|10.29672521

|

|

|style="background:#FFFF00"|transit

|1950

|0.63

|4687

|

Kepler-914b

|

|0.123

|4.40966548

|

|

|style="background:#FFFF00"|transit

|2210

|1.1

|5877

|

Kepler-915b

|

|0.134

|4.59489604

|

|

|style="background:#FFFF00"|transit

|2630

|1.21

|6173

|

Kepler-916b

|

|0.157

|32.2968798

|

|

|style="background:#FFFF00"|transit

|2510

|0.85

|5248

|

Kepler-917b

|

|0.17

|2.97041437

|

|

|style="background:#FFFF00"|transit

|3350

|0.8

|5418

|

Kepler-918b

|

|0.155

|4.85386933

|

|

|style="background:#FFFF00"|transit

|4060

|1.11

|6028

|

Kepler-919b

|

|0.201

|11.04603384

|

|

|style="background:#FFFF00"|transit

|3980

|1.15

|6113

|

Kepler-920b

|

|0.216

|6.53192704

|

|

|style="background:#FFFF00"|transit

|3020

|0.89

|5403

|

Kepler-920c

|

|0.339

|100.8274113

|

|

|style="background:#FFFF00"|transit

|3020

|0.89

|5403

|

Kepler-921b

|

|0.256

|51.300634

|

|

|style="background:#FFFF00"|transit

|2760

|0.93

|5663

|

Kepler-922b

|

|0.127

|0.93846683

|

|

|style="background:#FFFF00"|transit

|1820

|0.95

|5671

|

Kepler-923b

|

|0.123

|6.93366476

|

|

|style="background:#FFFF00"|transit

|3150

|1.11

|5988

|

Kepler-924b

|

|0.274

|61.0370117

|

|

|style="background:#FFFF00"|transit

|3250

|1.14

|6167

|

Kepler-925b

|

|0.209

|33.8678531

|

|

|style="background:#FFFF00"|transit

|2030

|0.77

|4673

|

Kepler-926b

|

|0.206

|52.0688601

|

|

|style="background:#FFFF00"|transit

|2510

|1.01

|5806

|

Kepler-927b

|

|0.153

|9.1149903

|

|

|style="background:#FFFF00"|transit

|2870

|0.99

|5743

|

Kepler-928b

|

|0.142

|3.9324613

|

|

|style="background:#FFFF00"|transit

|1740

|0.73

|4700

|

Kepler-929b

|

|0.099

|0.92103214

|

|

|style="background:#FFFF00"|transit

|2700

|1.01

|5869

|

Kepler-930b

|

|0.19

|71.4517775

|

|

|style="background:#FFFF00"|transit

|2950

|1.25

|6335

|

Kepler-931b

|

|0.119

|8.03755877

|

|

|style="background:#FFFF00"|transit

|1600

|0.86

|5241

|

Kepler-932b

|

|0.122

|1.9214374

|

|

|style="background:#FFFF00"|transit

|1560

|0.87

|5331

|

Kepler-933b

|

|0.219

|14.20443009

|

|

|style="background:#FFFF00"|transit

|3010

|0.87

|5346

|

Kepler-934b

|

|0.186

|55.6738309

|

|

|style="background:#FFFF00"|transit

|1970

|0.81

|5001

|

Kepler-935b

|

|0.12

|4.88083852

|

|

|style="background:#FFFF00"|transit

|1570

|0.78

|4830

|

Kepler-936b

|

|0.129

|10.56134221

|

|

|style="background:#FFFF00"|transit

|2240

|0.92

|5482

|

Kepler-937b

|

|0.332

|67.668827

|

|

|style="background:#FFFF00"|transit

|4830

|1.15

|6095

|

Kepler-937c

|

|0.238

|153.343364

|

|

|style="background:#FFFF00"|transit

|4830

|1.15

|6095

|

Kepler-938b

|

|0.198

|52.6298417

|

|

|style="background:#FFFF00"|transit

|2810

|0.92

|5533

|

Kepler-939b

|

|0.156

|14.878296

|

|

|style="background:#FFFF00"|transit

|3360

|0.88

|5471

|

Kepler-940b

|

|0.298

|59.6225257

|

|

|style="background:#FFFF00"|transit

|4300

|0.97

|5769

|

Kepler-941b

|

|0.275

|17.42395198

|

|

|style="background:#FFFF00"|transit

|3600

|0.89

|5539

|

Kepler-942b

|

|0.19

|44.96417488

|

|

|style="background:#FFFF00"|transit

|710

|0.81

|4861

|

Kepler-943b

|

|0.529

|49.7701438

|

|

|style="background:#FFFF00"|transit

|4040

|0.93

|5612

|

Kepler-944b

|

|0.235

|43.3167737

|

|

|style="background:#FFFF00"|transit

|3380

|0.86

|5409

|

Kepler-945b

|

|0.235

|31.0033814

|

|

|style="background:#FFFF00"|transit

|5030

|0.97

|5718

|

Kepler-946b

|

|0.172

|11.79162572

|

|

|style="background:#FFFF00"|transit

|2990

|0.94

|5665

|

Kepler-947b

|

|0.203

|26.9644317

|

|

|style="background:#FFFF00"|transit

|3870

|0.9

|5508

|

Kepler-948b

|

|0.165

|7.76846622

|

|

|style="background:#FFFF00"|transit

|2880

|0.96

|5679

|

Kepler-949b

|

|0.26

|8.6893073

|

|

|style="background:#FFFF00"|transit

|1870

|0.89

|5403

|

Kepler-950b

|

|0.801

|98.7180406

|

|

|style="background:#FFFF00"|transit

|4860

|1.02

|5857

|

Kepler-951b

|

|0.499

|71.52530845

|

|

|style="background:#FFFF00"|transit

|1330

|0.77

|4834

|

Kepler-952b

|

|0.682

|130.3546919

|

|

|style="background:#FFFF00"|transit

|3810

|1

|5730

|

Kepler-953b

|

|0.376

|88.40655258

|

|

|style="background:#FFFF00"|transit

|780

|0.95

|5416

|

Kepler-953c

|

|0.106

|9.10967112

|

|

|style="background:#FFFF00"|transit

|780

|0.95

|5416

|

Kepler-954b

|

|0.207

|16.78176602

|

|

|style="background:#FFFF00"|transit

|730

|0.82

|4990

|

Kepler-955b

|

|0.279

|14.53244172

|

|

|style="background:#FFFF00"|transit

|2080

|0.89

|5350

|

Kepler-956b

|

|0.268

|5.24867263

|

|

|style="background:#FFFF00"|transit

|2060

|1.1

|6040

|

Kepler-957b

|

|0.491

|5.90741354

|

|

|style="background:#FFFF00"|transit

|2440

|0.81

|4963

|

Kepler-958b

|

|0.184

|9.7678805

|

|

|style="background:#FFFF00"|transit

|1520

|0.91

|5421

|

Kepler-959b

|

|0.391

|14.80074836

|

|

|style="background:#FFFF00"|transit

|3270

|1.6

|7005

|

Kepler-960b

|

|0.204

|3.12686223

|

|

|style="background:#FFFF00"|transit

|970

|0.77

|4755

|

Kepler-961b

|

|0.227

|16.87727414

|

|

|style="background:#FFFF00"|transit

|1980

|0.96

|5582

|

Kepler-962b

|

|0.176

|12.05707239

|

|

|style="background:#FFFF00"|transit

|1430

|0.93

|5478

|

Kepler-963b

|

|0.237

|9.97683705

|

|

|style="background:#FFFF00"|transit

|2560

|0.91

|5461

|

Kepler-964b

|

|0.189

|13.5225106

|

|

|style="background:#FFFF00"|transit

|1560

|0.93

|5427

|

Kepler-965b

|

|0.302

|134.2527298

|

|

|style="background:#FFFF00"|transit

|2020

|1.05

|5886

|

Kepler-966b

|

|0.368

|99.747622

|

|

|style="background:#FFFF00"|transit

|2520

|1.02

|5840

|

Kepler-967b

|

|0.21

|13.22713379

|

|

|style="background:#FFFF00"|transit

|1630

|0.84

|5178

|

Kepler-967c

|

|0.326

|198.7112502

|

|

|style="background:#FFFF00"|transit

|1630

|0.84

|5178

|

Kepler-968b

|

|0.178

|3.69298373

|

|

|style="background:#FFFF00"|transit

|1020

|0.76

|4598

|

Kepler-968c

|

|0.151

|5.70940492

|

|

|style="background:#FFFF00"|transit

|1020

|0.76

|4598

|

Kepler-969b

|

|0.185

|34.1731714

|

|

|style="background:#FFFF00"|transit

|1340

|0.92

|5214

|

Kepler-969c

|

|0.088

|1.6829346

|

|

|style="background:#FFFF00"|transit

|1340

|0.92

|5214

|

Kepler-970b

|

|0.247

|16.73652231

|

|

|style="background:#FFFF00"|transit

|1100

|0.7

|4511

|

Kepler-971b

|

|0.19

|9.59070716

|

|

|style="background:#FFFF00"|transit

|1130

|0.88

|5431

|

Kepler-972b

|

|0.415

|7.03932553

|

|

|style="background:#FFFF00"|transit

|4250

|1.15

|6146

|

Kepler-973b

|

|0.175

|49.6077331

|

|

|style="background:#FFFF00"|transit

|970

|0.86

|5213

|

Kepler-974b

|

|0.14

|4.19449651

|

|

|style="background:#FFFF00"|transit

|390

|0.52

|3687

|

Kepler-975b

|

|0.132

|1.97034246

|

|

|style="background:#FFFF00"|transit

|1320

|0.8

|4897

|

Kepler-976b

|

|0.353

|105.9564148

|

|

|style="background:#FFFF00"|transit

|3300

|0.87

|5232

|

Kepler-977b

|

|0.234

|26.85328322

|

|

|style="background:#FFFF00"|transit

|2170

|0.87

|5315

|

Kepler-978b

|

|0.267

|49.6221509

|

|

|style="background:#FFFF00"|transit

|2040

|1.07

|6002

|

Kepler-979b

|

|0.243

|8.0880135

|

|

|style="background:#FFFF00"|transit

|1980

|0.87

|5310

|

Kepler-980b

|

|0.238

|11.55102504

|

|

|style="background:#FFFF00"|transit

|2620

|1.05

|5935

|

Kepler-981b

|

|0.206

|4.46975774

|

|

|style="background:#FFFF00"|transit

|2980

|0.98

|5718

|

Kepler-982b

|

|0.201

|15.7738221

|

|

|style="background:#FFFF00"|transit

|2290

|1.16

|6139

|

Kepler-983b

|

|0.211

|60.0855082

|

|

|style="background:#FFFF00"|transit

|2140

|1.13

|6052

|

Kepler-984b

|

|0.189

|43.0342272

|

|

|style="background:#FFFF00"|transit

|1500

|0.96

|5610

|

Kepler-985b

|

|0.266

|116.331901

|

|

|style="background:#FFFF00"|transit

|2420

|0.91

|5434

|

Kepler-986b

|

|0.211

|56.4349938

|

|

|style="background:#FFFF00"|transit

|1840

|0.96

|5642

|

Kepler-987b

|

|0.291

|105.3033148

|

|

|style="background:#FFFF00"|transit

|3050

|0.97

|5637

|

Kepler-988b

|

|0.185

|17.76080053

|

|

|style="background:#FFFF00"|transit

|810

|0.55

|4005

|

Kepler-989b

|

|0.197

|7.96431535

|

|

|style="background:#FFFF00"|transit

|1580

|0.82

|5074

|

Kepler-990b

|

|0.232

|9.91723428

|

|

|style="background:#FFFF00"|transit

|3040

|1.05

|5948

|

Kepler-990c

|

|0.136

|0.53835431

|

|

|style="background:#FFFF00"|transit

|3040

|1.05

|5948

|

Kepler-991b

|

|0.227

|82.5342519

|

|

|style="background:#FFFF00"|transit

|1200

|0.64

|4392

|

Kepler-992b

|

|0.145

|20.16034462

|

|

|style="background:#FFFF00"|transit

|870

|0.8

|4944

|

Kepler-993b

|

|0.265

|22.08557563

|

|

|style="background:#FFFF00"|transit

|970

|0.57

|3843

|

Kepler-994b

|

|0.143

|1.15116651

|

|

|style="background:#FFFF00"|transit

|550

|0.56

|3934

|

Kepler-995b

|

|0.241

|28.26731672

|

|

|style="background:#FFFF00"|transit

|2150

|0.83

|5206

|

Kepler-996b

|

|0.177

|3.77059058

|

|

|style="background:#FFFF00"|transit

|3580

|1.09

|6014

|

Kepler-997b

|

|0.121

|2.70730672

|

|

|style="background:#FFFF00"|transit

|1500

|1.22

|6150

|

Kepler-998b

|

|0.207

|5.65377733

|

|

|style="background:#FFFF00"|transit

|3250

|1.12

|6058

|

Kepler-999b

|

|0.209

|5.99185702

|

|

|style="background:#FFFF00"|transit

|1850

|1.29

|6237

|

Kepler-1000b

|

|0.425

|120.0181272

|

|

|style="background:#FFFF00"|transit

|3020

|1.4

|6453

|

Kepler-1001b

|

|0.281

|14.30511983

|

|

|style="background:#FFFF00"|transit

|3290

|0.9

|5491

|

Kepler-1002b

|

|0.153

|4.33642933

|

|

|style="background:#FFFF00"|transit

|1390

|1.22

|6144

|

Kepler-1003b

|

|0.159

|3.55485691

|

|

|style="background:#FFFF00"|transit

|2850

|1.11

|6109

|

Kepler-1004b

|

|0.56

|5.28789787

|

|

|style="background:#FFFF00"|transit

|3500

|1.11

|4972

|

Kepler-1005b

|

|0.134

|6.49801525

|

|

|style="background:#FFFF00"|transit

|1680

|1

|5782

|

Kepler-1006b

|

|0.137

|19.76172042

|

|

|style="background:#FFFF00"|transit

|1620

|0.78

|5328

|

Kepler-1007b

|

|0.128

|5.18500207

|

|

|style="background:#FFFF00"|transit

|1190

|0.73

|4587

|

Kepler-1008b

|

|0.114

|12.43931193

|

|

|style="background:#FFFF00"|transit

|980

|0.81

|5066

|

Kepler-1009b

|

|0.194

|11.35011917

|

|

|style="background:#FFFF00"|transit

|920

|0.59

|4027

|

Kepler-1010b

|

|0.207

|34.2685705

|

|

|style="background:#FFFF00"|transit

|2000

|0.86

|5253

|

Kepler-1011b

|

|0.256

|5.75322197

|

|

|style="background:#FFFF00"|transit

|2800

|0.91

|5416

|

Kepler-1012b

|

|0.115

|5.50860439

|

|

|style="background:#FFFF00"|transit

|1400

|0.95

|5556

|

Kepler-1013b

|

|0.192

|18.93054959

|

|

|style="background:#FFFF00"|transit

|1410

|0.81

|4954

|

Kepler-1014b

|

|0.213

|16.57110363

|

|

|style="background:#FFFF00"|transit

|2190

|0.88

|5388

|

Kepler-1015b

|

|0.317

|16.00494214

|

|

|style="background:#FFFF00"|transit

|3040

|1.49

|6769

|

Kepler-1016b

|

|0.194

|1.95452434

|

|

|style="background:#FFFF00"|transit

|4040

|0.99

|5821

|

Kepler-1016c

|

|0.328

|105.6551369

|

|

|style="background:#FFFF00"|transit

|4040

|0.99

|5821

|

Kepler-1017b

|

|0.178

|7.23400469

|

|

|style="background:#FFFF00"|transit

|1810

|0.93

|5473

|

Kepler-1018b

|

|0.23

|49.1013514

|

|

|style="background:#FFFF00"|transit

|2920

|0.91

|5518

|

Kepler-1019b

|

|0.13

|1.41122985

|

|

|style="background:#FFFF00"|transit

|650

|0.7

|4433

|

Kepler-1020b

|

|0.203

|96.9151496

|

|

|style="background:#FFFF00"|transit

|1450

|0.87

|5227

|

Kepler-1021b

|

|0.208

|13.47469571

|

|

|style="background:#FFFF00"|transit

|2730

|0.89

|5431

|

Kepler-1022b

|

|0.211

|10.99469878

|

|

|style="background:#FFFF00"|transit

|1480

|0.71

|4445

|

Kepler-1023b

|

|0.235

|62.1387714

|

|

|style="background:#FFFF00"|transit

|2240

|0.93

|5494

|

Kepler-1024b

|

|0.349

|66.4162133

|

|

|style="background:#FFFF00"|transit

|3320

|0.81

|5143

|

Kepler-1025b

|

|0.177

|37.3229493

|

|

|style="background:#FFFF00"|transit

|2340

|1.09

|6089

|

Kepler-1026b

|

|0.197

|36.5156053

|

|

|style="background:#FFFF00"|transit

|1270

|0.79

|4948

|

Kepler-1027b

|

|0.079

|1.9078052

|

|

|style="background:#FFFF00"|transit

|950

|0.91

|5436

|

Kepler-1028b

|

|0.119

|2.51462432

|

|

|style="background:#FFFF00"|transit

|2060

|0.9

|5522

|

Kepler-1029b

|

|0.112

|4.41769648

|

|

|style="background:#FFFF00"|transit

|1380

|0.82

|5030

|

Kepler-1030b

|

|0.221

|19.32952416

|

|

|style="background:#FFFF00"|transit

|2590

|0.8

|4983

|

Kepler-1031b

|

|0.078

|1.22621732

|

|

|style="background:#FFFF00"|transit

|2420

|1.09

|6011

|

Kepler-1032b

|

|0.167

|3.29011795

|

|

|style="background:#FFFF00"|transit

|1980

|0.77

|4647

|

Kepler-1033b

|

|0.224

|7.56052806

|

|

|style="background:#FFFF00"|transit

|4650

|0.94

|5547

|

Kepler-1034b

|

|0.202

|12.12400943

|

|

|style="background:#FFFF00"|transit

|2300

|0.83

|5198

|

Kepler-1035b

|

|0.104

|2.71407755

|

|

|style="background:#FFFF00"|transit

|1330

|0.98

|5763

|

Kepler-1036b

|

|0.269

|122.8808058

|

|

|style="background:#FFFF00"|transit

|1650

|0.95

|5533

|

Kepler-1037b

|

|0.114

|1.06378867

|

|

|style="background:#FFFF00"|transit

|1470

|0.82

|5105

|

Kepler-1038b

|

|0.315

|148.4603382

|

|

|style="background:#FFFF00"|transit

|2030

|0.87

|5335

|

Kepler-1039b

|

|0.13

|0.93488424

|

|

|style="background:#FFFF00"|transit

|1060

|0.79

|4870

|

Kepler-1040b

|

|0.186

|201.1214

|

|

|style="background:#FFFF00"|transit

|1540

|0.98

|5694

|

Kepler-1041b

|

|0.262

|24.7576421

|

|

|style="background:#FFFF00"|transit

|3190

|1.06

|5957

|

Kepler-1042b

|

|0.195

|10.13202575

|

|

|style="background:#FFFF00"|transit

|2150

|0.75

|4815

|

Kepler-1043b

|

|0.227

|38.5053398

|

|

|style="background:#FFFF00"|transit

|2730

|0.92

|5629

|

Kepler-1044b

|

|0.238

|6.77408868

|

|

|style="background:#FFFF00"|transit

|4920

|1.08

|5985

|

Kepler-1045b

|

|0.24

|26.41045478

|

|

|style="background:#FFFF00"|transit

|3170

|0.86

|5301

|

Kepler-1046b

|

|0.153

|14.37508035

|

|

|style="background:#FFFF00"|transit

|1690

|1.04

|5913

|

Kepler-1047b

|

|0.186

|56.1886887

|

|

|style="background:#FFFF00"|transit

|1850

|1.08

|5754

|

Kepler-1047c

|

|0.088

|3.18897601

|

|

|style="background:#FFFF00"|transit

|1850

|1.08

|5754

|

Kepler-1048b

|

|0.144

|6.92101021

|

|

|style="background:#FFFF00"|transit

|1350

|0.75

|4651

|

Kepler-1049b

|

|0.085

|3.27346074

|

|

|style="background:#FFFF00"|transit

|420

|0.51

|3864

|

Kepler-1050b

|

|0.143

|15.3787546

|

|

|style="background:#FFFF00"|transit

|1810

|1.09

|6010

|

Kepler-1050c

|

|0.132

|21.1284569

|

|

|style="background:#FFFF00"|transit

|1810

|1.09

|6010

|

Kepler-1051b

|

|0.303

|25.96200249

|

|

|style="background:#FFFF00"|transit

|3330

|1.43

|6675

|

Kepler-1052b

|

|0.261

|34.8538276

|

|

|style="background:#FFFF00"|transit

|3430

|1.03

|5888

|

Kepler-1053b

|

|0.087

|2.41435165

|

|

|style="background:#FFFF00"|transit

|560

|0.74

|4529

|

Kepler-1054b

|

|0.235

|4.30655689

|

|

|style="background:#FFFF00"|transit

|3400

|1.22

|6209

|

Kepler-1055b

|

|0.11

|2.29503623

|

|

|style="background:#FFFF00"|transit

|1380

|0.98

|5723

|

Kepler-1056b

|

|0.269

|27.495606

|

|

|style="background:#FFFF00"|transit

|3170

|1.12

|6127

|

Kepler-1057b

|

|0.3

|14.08827448

|

|

|style="background:#FFFF00"|transit

|4770

|1.07

|5987

|

Kepler-1058b

|

|0.243

|110.96546

|

|

|style="background:#FFFF00"|transit

|1710

|0.73

|4644

|

Kepler-1059b

|

|0.154

|3.76419105

|

|

|style="background:#FFFF00"|transit

|2200

|0.75

|4906

|

Kepler-1060b

|

|0.212

|46.8779367

|

|

|style="background:#FFFF00"|transit

|2810

|0.99

|5797

|

Kepler-1061b

|

|0.177

|2.75798267

|

|

|style="background:#FFFF00"|transit

|1910

|1.09

|6067

|

Kepler-1062b

|

|0.157

|9.30412078

|

|

|style="background:#FFFF00"|transit

|1270

|0.75

|4597

|

Kepler-1063b

|

|0.133

|14.07971466

|

|

|style="background:#FFFF00"|transit

|1190

|1.09

|5945

|

Kepler-1064b

|

|0.138

|16.54080322

|

|

|style="background:#FFFF00"|transit

|1220

|0.85

|5153

|

Kepler-1065b

|

|0.333

|3.60930891

|

|

|style="background:#FFFF00"|transit

|3520

|0.94

|5635

|

Kepler-1065c

|

|0.143

|2.37030743

|

|

|style="background:#FFFF00"|transit

|3520

|0.94

|5635

|

Kepler-1066b

|

|0.211

|1.93155984

|

|

|style="background:#FFFF00"|transit

|1300

|0.98

|5762

|

Kepler-1067b

|

|0.071

|0.76212926

|

|

|style="background:#FFFF00"|transit

|2250

|0.95

|5592

|

Kepler-1068b

|

|0.324

|16.92344113

|

|

|style="background:#FFFF00"|transit

|5000

|1.01

|5806

|

Kepler-1069b

|

|0.143

|23.8990296

|

|

|style="background:#FFFF00"|transit

|1420

|0.99

|5722

|

Kepler-1070b

|

|0.154

|6.2216147

|

|

|style="background:#FFFF00"|transit

|3400

|1.21

|6261

|

Kepler-1071b

|

|0.212

|6.1799844

|

|

|style="background:#FFFF00"|transit

|3140

|0.86

|5215

|

Kepler-1072b

|

|0.141

|1.5690665

|

|

|style="background:#FFFF00"|transit

|3180

|1.2

|6199

|

Kepler-1073b

|

|0.205

|8.67888593

|

|

|style="background:#FFFF00"|transit

|2730

|1

|5792

|

Kepler-1073c

|

|0.146

|4.02582254

|

|

|style="background:#FFFF00"|transit

|2730

|1

|5792

|

Kepler-1074b

|

|0.112

|5.94566534

|

|

|style="background:#FFFF00"|transit

|800

|0.6

|4002

|

Kepler-1075b

|

|0.127

|1.52372816

|

|

|style="background:#FFFF00"|transit

|860

|0.56

|3959

|

Kepler-1076b

|

|0.071

|6.14727918

|

|

|style="background:#FFFF00"|transit

|650

|0.79

|4868

|

Kepler-1077b

|

|0.247

|34.3511874

|

|

|style="background:#FFFF00"|transit

|3580

|1.02

|5816

|

Kepler-1078b

|

|0.17

|3.00725242

|

|

|style="background:#FFFF00"|transit

|3960

|0.94

|5612

|

Kepler-1079b

|

|0.145

|13.24503188

|

|

|style="background:#FFFF00"|transit

|1570

|1.08

|5758

|

Kepler-1080b

|

|0.293

|77.2548396

|

|

|style="background:#FFFF00"|transit

|2240

|1.1

|5956

|

Kepler-1081b

|

|0.09

|3.85691855

|

|

|style="background:#FFFF00"|transit

|1390

|0.88

|5345

|

Kepler-1082b

|

|0.1

|1.5432066

|

|

|style="background:#FFFF00"|transit

|2050

|1.03

|5923

|

Kepler-1083b

|

|0.3

|33.4177993

|

|

|style="background:#FFFF00"|transit

|2970

|0.81

|5049

|

Kepler-1084b

|

|0.099

|2.05333679

|

|

|style="background:#FFFF00"|transit

|1390

|1.12

|6113

|

Kepler-1085b

|

|0.644

|219.3217528

|

|

|style="background:#FFFF00"|transit

|4950

|1.11

|6000

|

Kepler-1086b

|

|0.218

|18.78425728

|

|

|style="background:#FFFF00"|transit

|1510

|0.7

|4350

|

Kepler-1086c

|

|0.262

|161.5163345

|

|

|style="background:#FFFF00"|transit

|1510

|0.7

|4350

|

Kepler-1087b

|

|0.054

|0.69384285

|

|

|style="background:#FFFF00"|transit

|1150

|0.96

|5589

|

Kepler-1088b

|

|0.127

|23.12748644

|

|

|style="background:#FFFF00"|transit

|980

|1.08

|5975

|

Kepler-1089b

|

|0.163

|5.13248562

|

|

|style="background:#FFFF00"|transit

|740

|0.52

|3753

|

Kepler-1090b

|

|0.201

|198.680179

|

|

|style="background:#FFFF00"|transit

|2290

|0.86

|5321

|

Kepler-1091b

|

|0.13

|1.43474156

|

|

|style="background:#FFFF00"|transit

|2980

|1.01

|5851

|

Kepler-1092b

|

|0.185

|58.6017925

|

|

|style="background:#FFFF00"|transit

|2980

|0.99

|5862

|

Kepler-1093b

|

|0.174

|25.0824626

|

|

|style="background:#FFFF00"|transit

|2770

|1.13

|6166

|

Kepler-1093c

|

|0.175

|89.722292

|

|

|style="background:#FFFF00"|transit

|2770

|1.13

|6166

|

Kepler-1094b

|

|0.284

|78.1000231

|

|

|style="background:#FFFF00"|transit

|4470

|1.14

|6112

|

Kepler-1095b

|

|0.108

|4.27103091

|

|

|style="background:#FFFF00"|transit

|2470

|0.94

|5658

|

Kepler-1096b

|

|0.111

|2.89221751

|

|

|style="background:#FFFF00"|transit

|1120

|0.66

|4306

|

Kepler-1097b

|

|0.291

|187.747029

|

|

|style="background:#FFFF00"|transit

|2410

|0.82

|5211

|

Kepler-1098b

|

|0.116

|2.54307286

|

|

|style="background:#FFFF00"|transit

|2860

|0.99

|5794

|

Kepler-1099b

|

|0.252

|2.16845259

|

|

|style="background:#FFFF00"|transit

|3940

|1.01

|5837

|

Kepler-1100b

|

|0.156

|6.42200058

|

|

|style="background:#FFFF00"|transit

|3100

|1.21

|6247

|

Kepler-1101b

|

|0.22

|81.3151059

|

|

|style="background:#FFFF00"|transit

|2930

|0.94

|5614

|

Kepler-1102b

|

|0.237

|51.3285623

|

|

|style="background:#FFFF00"|transit

|3220

|0.96

|5724

|

Kepler-1103b

|

|0.203

|19.79191978

|

|

|style="background:#FFFF00"|transit

|3000

|1.11

|6092

|

Kepler-1104b

|

|0.11

|5.03728015

|

|

|style="background:#FFFF00"|transit

|1680

|1.3

|6417

|

Kepler-1105b

|

|0.179

|4.42157218

|

|

|style="background:#FFFF00"|transit

|1200

|0.71

|4299

|

Kepler-1106b

|

|0.147

|1.25275217

|

|

|style="background:#FFFF00"|transit

|3810

|1.11

|6104

|

Kepler-1107b

|

|0.12

|0.57103852

|

|

|style="background:#FFFF00"|transit

|1490

|0.86

|5268

|

Kepler-1108b

|

|0.13

|4.51005748

|

|

|style="background:#FFFF00"|transit

|2490

|0.88

|5406

|

Kepler-1109b

|

|0.195

|37.6467384

|

|

|style="background:#FFFF00"|transit

|2600

|1.05

|5893

|

Kepler-1110b

|

|0.237

|9.69312032

|

|

|style="background:#FFFF00"|transit

|2370

|0.73

|4781

|

Kepler-1111b

|

|0.178

|8.79617863

|

|

|style="background:#FFFF00"|transit

|3720

|1.1

|6077

|

Kepler-1112b

|

|0.269

|14.36267939

|

|

|style="background:#FFFF00"|transit

|5660

|1.34

|6496

|

Kepler-1113b

|

|0.251

|42.3004954

|

|

|style="background:#FFFF00"|transit

|3680

|1.12

|5931

|

Kepler-1114b

|

|0.12

|14.97435694

|

|

|style="background:#FFFF00"|transit

|1390

|0.87

|5374

|

Kepler-1115b

|

|0.152

|23.5540725

|

|

|style="background:#FFFF00"|transit

|3050

|1.6

|8480

|

Kepler-1116b

|

|0.227

|41.6977827

|

|

|style="background:#FFFF00"|transit

|3320

|0.95

|5641

|

Kepler-1117b

|

|0.099

|4.79028459

|

|

|style="background:#FFFF00"|transit

|2020

|0.95

|5612

|

Kepler-1118b

|

|0.244

|38.6715075

|

|

|style="background:#FFFF00"|transit

|2670

|0.96

|5688

|

Kepler-1119b

|

|0.171

|8.3265153

|

|

|style="background:#FFFF00"|transit

|4200

|1.11

|6083

|

Kepler-1120b

|

|0.123

|2.94902905

|

|

|style="background:#FFFF00"|transit

|2070

|0.78

|4904

|

Kepler-1121b

|

|0.17

|13.15141081

|

|

|style="background:#FFFF00"|transit

|1730

|1.29

|6231

|

Kepler-1122b

|

|0.182

|42.1917357

|

|

|style="background:#FFFF00"|transit

|3010

|0.92

|5544

|

Kepler-1123b

|

|0.149

|4.33946454

|

|

|style="background:#FFFF00"|transit

|2600

|0.93

|5500

|

Kepler-1124b

|

|0.114

|2.85234897

|

|

|style="background:#FFFF00"|transit

|580

|0.35

|3658

|

Kepler-1125b

|

|0.164

|17.6700642

|

|

|style="background:#FFFF00"|transit

|3000

|0.95

|5683

|

Kepler-1126b

|

|0.154

|108.593329

|

|

|style="background:#FFFF00"|transit

|2180

|0.92

|5798

|

Kepler-1127b

|

|0.175

|5.12330347

|

|

|style="background:#FFFF00"|transit

|3250

|0.97

|5664

|

Kepler-1128b

|

|0.326

|61.6178167

|

|

|style="background:#FFFF00"|transit

|3790

|0.94

|5543

|

Kepler-1129b

|

|0.264

|24.3397804

|

|

|style="background:#FFFF00"|transit

|4100

|1

|5831

|

Kepler-1129c

|

|0.244

|76.5369586

|

|

|style="background:#FFFF00"|transit

|4100

|1

|5831

|

Kepler-1130b

|

|0.071

|5.45298175

|

|

|style="background:#FFFF00"|transit

|760

|0.9

|5403

|

Kepler-1131b

|

|0.142

|3.53232449

|

|

|style="background:#FFFF00"|transit

|3620

|1.03

|5851

|

Kepler-1132b

|

|0.21

|62.8916228

|

|

|style="background:#FFFF00"|transit

|3100

|0.87

|5298

|

Kepler-1133b

|

|0.176

|11.55562343

|

|

|style="background:#FFFF00"|transit

|2680

|0.93

|5569

|

Kepler-1134b

|

|0.236

|17.13263989

|

|

|style="background:#FFFF00"|transit

|3250

|0.84

|5281

|

Kepler-1135b

|

|0.165

|76.957857

|

|

|style="background:#FFFF00"|transit

|2370

|0.96

|5656

|

Kepler-1136b

|

|0.146

|2.36172433

|

|

|style="background:#FFFF00"|transit

|1780

|0.72

|4512

|

Kepler-1137b

|

|0.196

|23.9210791

|

|

|style="background:#FFFF00"|transit

|3170

|1.5

|6807

|

Kepler-1138b

|

|0.152

|3.17060005

|

|

|style="background:#FFFF00"|transit

|3590

|0.95

|5582

|

Kepler-1139b

|

|0.106

|0.81316672

|

|

|style="background:#FFFF00"|transit

|1810

|0.94

|5550

|

Kepler-1140b

|

|0.247

|24.0862707

|

|

|style="background:#FFFF00"|transit

|2140

|0.76

|4850

|

Kepler-1141b

|

|0.073

|2.34451194

|

|

|style="background:#FFFF00"|transit

|1190

|1.01

|5791

|

Kepler-1142b

|

|0.131

|18.3027248

|

|

|style="background:#FFFF00"|transit

|2270

|0.97

|5685

|

Kepler-1143b

|

|0.149

|2.88890485

|

|

|style="background:#FFFF00"|transit

|2060

|0.81

|5053

|

Kepler-1143c

|

|0.321

|210.630591

|

|

|style="background:#FFFF00"|transit

|2060

|0.81

|5053

|

Kepler-1144b

|

|0.178

|17.14647302

|

|

|style="background:#FFFF00"|transit

|3300

|0.98

|5753

|

Kepler-1145b

|

|0.125

|3.97076766

|

|

|style="background:#FFFF00"|transit

|2330

|0.79

|5064

|

Kepler-1146b

|

|0.11

|2.3522658

|

|

|style="background:#FFFF00"|transit

|2260

|0.74

|4692

|

Kepler-1147b

|

|0.233

|10.62784997

|

|

|style="background:#FFFF00"|transit

|4810

|1.09

|5941

|

Kepler-1148b

|

|0.151

|1.10446351

|

|

|style="background:#FFFF00"|transit

|2220

|0.81

|5054

|

Kepler-1149b

|

|0.128

|3.73089898

|

|

|style="background:#FFFF00"|transit

|3340

|1.02

|5833

|

Kepler-1150b

|

|0.091

|2.78786839

|

|

|style="background:#FFFF00"|transit

|1220

|0.76

|4754

|

Kepler-1151b

|

|0.198

|65.6478424

|

|

|style="background:#FFFF00"|transit

|2490

|0.88

|5470

|

Kepler-1152b

|

|0.078

|1.64680191

|

|

|style="background:#FFFF00"|transit

|600

|0.55

|3964

|

Kepler-1153b

|

|0.154

|1.75583533

|

|

|style="background:#FFFF00"|transit

|3860

|0.91

|5470

|

Kepler-1154b

|

|0.209

|5.1856142

|

|

|style="background:#FFFF00"|transit

|4990

|1.26

|6327

|

Kepler-1154c

|

|0.211

|8.45808312

|

|

|style="background:#FFFF00"|transit

|4990

|1.26

|6327

|

Kepler-1155b

|

|0.181

|33.469743

|

|

|style="background:#FFFF00"|transit

|3220

|1.03

|5842

|

Kepler-1156b

|

|0.118

|11.89520511

|

|

|style="background:#FFFF00"|transit

|2480

|1

|5778

|

Kepler-1157b

|

|0.097

|4.45743164

|

|

|style="background:#FFFF00"|transit

|1130

|0.76

|4679

|

Kepler-1158b

|

|0.209

|13.5396293

|

|

|style="background:#FFFF00"|transit

|4100

|1.41

|6203

|

Kepler-1159b

|

|0.211

|22.70816791

|

|

|style="background:#FFFF00"|transit

|4040

|1.19

|6217

|

Kepler-1160b

|

|0.191

|7.97034958

|

|

|style="background:#FFFF00"|transit

|4220

|0.92

|5519

|

Kepler-1161b

|

|0.19

|10.71252541

|

|

|style="background:#FFFF00"|transit

|1400

|0.59

|4253

|

Kepler-1162b

|

|0.197

|32.5637069

|

|

|style="background:#FFFF00"|transit

|3230

|0.89

|5390

|

Kepler-1163b

|

|0.092

|6.11786898

|

|

|style="background:#FFFF00"|transit

|1590

|1.22

|6302

|

Kepler-1164b

|

|0.1

|3.97599768

|

|

|style="background:#FFFF00"|transit

|1460

|0.85

|5183

|

Kepler-1165b

|

|0.138

|9.478522

|

|

|style="background:#FFFF00"|transit

|3530

|1.13

|6080

|

Kepler-1166b

|

|0.151

|33.2406882

|

|

|style="background:#FFFF00"|transit

|2110

|0.9

|5446

|

Kepler-1167b

|

|0.153

|1.00393374

|

|

|style="background:#FFFF00"|transit

|2650

|0.79

|4971

|

Kepler-1168b

|

|0.223

|55.8226539

|

|

|style="background:#FFFF00"|transit

|2970

|0.87

|5157

|

Kepler-1169b

|

|0.084

|6.11009134

|

|

|style="background:#FFFF00"|transit

|1750

|1.24

|6191

|

Kepler-1170b

|

|0.215

|9.98969327

|

|

|style="background:#FFFF00"|transit

|2970

|0.8

|5069

|

Kepler-1171b

|

|0.228

|1.44259224

|

|

|style="background:#FFFF00"|transit

|2010

|1.58

|7044

|

Kepler-1172b

|

|0.285

|26.0204423

|

|

|style="background:#FFFF00"|transit

|4210

|0.92

|5558

|

Kepler-1173b

|

|0.079

|0.7698536

|

|

|style="background:#FFFF00"|transit

|1310

|0.86

|5252

|

Kepler-1174b

|

|0.142

|6.89225223

|

|

|style="background:#FFFF00"|transit

|2700

|1.04

|5936

|

Kepler-1175b

|

|0.267

|37.94563

|

|

|style="background:#FFFF00"|transit

|4060

|0.9

|5453

|

Kepler-1176b

|

|0.219

|24.1738579

|

|

|style="background:#FFFF00"|transit

|3340

|1.01

|5844

|

Kepler-1177b

|

|0.17

|106.247547

|

|

|style="background:#FFFF00"|transit

|2700

|0.98

|5712

|

Kepler-1178b

|

|0.095

|31.80634

|

|

|style="background:#FFFF00"|transit

|1100

|0.8

|4990

|

Kepler-1179b

|

|0.118

|2.68505749

|

|

|style="background:#FFFF00"|transit

|1480

|0.84

|5212

|

Kepler-1180b

|

|0.178

|16.8601286

|

|

|style="background:#FFFF00"|transit

|4190

|1.09

|6077

|

Kepler-1181b

|

|0.14

|4.89337519

|

|

|style="background:#FFFF00"|transit

|2830

|1.17

|6176

|

Kepler-1182b

|

|0.215

|11.17394617

|

|

|style="background:#FFFF00"|transit

|4100

|1.04

|5924

|

Kepler-1183b

|

|0.252

|28.5057189

|

|

|style="background:#FFFF00"|transit

|4490

|1

|5765

|

Kepler-1184b

|

|0.239

|53.5991044

|

|

|style="background:#FFFF00"|transit

|3890

|1.05

|5983

|

Kepler-1185b

|

|0.119

|104.3518976

|

|

|style="background:#FFFF00"|transit

|970

|0.96

|5622

|

Kepler-1186b

|

|0.199

|16.07677615

|

|

|style="background:#FFFF00"|transit

|3630

|0.95

|5635

|

Kepler-1187b

|

|0.233

|18.87064068

|

|

|style="background:#FFFF00"|transit

|3360

|1.06

|5975

|

Kepler-1188b

|

|0.186

|17.1369543

|

|

|style="background:#FFFF00"|transit

|3920

|1.04

|5913

|

Kepler-1189b

|

|0.158

|3.78858982

|

|

|style="background:#FFFF00"|transit

|2880

|1.11

|6012

|

Kepler-1190b

|

|0.119

|10.45843441

|

|

|style="background:#FFFF00"|transit

|1250

|0.76

|4730

|

Kepler-1191b

|

|0.135

|5.60014851

|

|

|style="background:#FFFF00"|transit

|2860

|0.85

|5308

|

Kepler-1192b

|

|0.211

|25.2034787

|

|

|style="background:#FFFF00"|transit

|3610

|0.86

|5438

|

Kepler-1193b

|

|0.118

|2.83265213

|

|

|style="background:#FFFF00"|transit

|2270

|1.08

|5908

|

Kepler-1194b

|

|0.135

|16.22371307

|

|

|style="background:#FFFF00"|transit

|2010

|0.94

|5590

|

Kepler-1195b

|

|0.186

|8.49642241

|

|

|style="background:#FFFF00"|transit

|2650

|0.74

|4965

|

Kepler-1196b

|

|0.199

|66.1849031

|

|

|style="background:#FFFF00"|transit

|3090

|0.98

|5756

|

Kepler-1197b

|

|0.112

|2.03231845

|

|

|style="background:#FFFF00"|transit

|1650

|0.78

|4708

|

Kepler-1198b

|

|0.131

|7.6847716

|

|

|style="background:#FFFF00"|transit

|2530

|0.93

|5517

|

Kepler-1199b

|

|0.103

|15.0447198

|

|

|style="background:#FFFF00"|transit

|1800

|0.94

|5889

|

Kepler-1200b

|

|0.095

|1.11854972

|

|

|style="background:#FFFF00"|transit

|1890

|0.74

|4612

|

Kepler-1201b

|

|0.204

|15.18725932

|

|

|style="background:#FFFF00"|transit

|3920

|1.15

|6177

|

Kepler-1202b

|

|0.262

|28.6851324

|

|

|style="background:#FFFF00"|transit

|4540

|1.03

|5834

|

Kepler-1203b

|

|0.095

|0.58800076

|

|

|style="background:#FFFF00"|transit

|880

|0.64

|4105

|

Kepler-1204b

|

|0.272

|85.7350285

|

|

|style="background:#FFFF00"|transit

|4180

|1.03

|5825

|

Kepler-1205b

|

|0.126

|1.07839035

|

|

|style="background:#FFFF00"|transit

|2500

|0.84

|5226

|

Kepler-1206b

|

|0.146

|1.21699766

|

|

|style="background:#FFFF00"|transit

|2630

|0.8

|4877

|

Kepler-1207b

|

|0.145

|13.68237119

|

|

|style="background:#FFFF00"|transit

|3090

|1.06

|5909

|

Kepler-1208b

|

|0.207

|11.08507637

|

|

|style="background:#FFFF00"|transit

|2860

|0.8

|5001

|

Kepler-1209b

|

|0.135

|25.369116

|

|

|style="background:#FFFF00"|transit

|1820

|1.23

|6210

|

Kepler-1210b

|

|0.152

|8.07124073

|

|

|style="background:#FFFF00"|transit

|3770

|0.94

|5568

|

Kepler-1211b

|

|0.227

|11.01816836

|

|

|style="background:#FFFF00"|transit

|4850

|0.96

|5705

|

Kepler-1212b

|

|0.191

|12.94130146

|

|

|style="background:#FFFF00"|transit

|4250

|1.1

|6051

|

Kepler-1213b

|

|0.106

|5.34982412

|

|

|style="background:#FFFF00"|transit

|2230

|1.14

|6050

|

Kepler-1214b

|

|0.211

|18.82634264

|

|

|style="background:#FFFF00"|transit

|2470

|0.85

|5130

|

Kepler-1215b

|

|0.109

|4.76703963

|

|

|style="background:#FFFF00"|transit

|2290

|0.95

|5616

|

Kepler-1216b

|

|0.124

|4.37034536

|

|

|style="background:#FFFF00"|transit

|3670

|0.99

|5743

|

Kepler-1217b

|

|0.178

|2.03232507

|

|

|style="background:#FFFF00"|transit

|4450

|1.06

|5905

|

Kepler-1218b

|

|0.128

|22.9221266

|

|

|style="background:#FFFF00"|transit

|2180

|1.06

|5986

|

Kepler-1219b

|

|0.189

|16.10467749

|

|

|style="background:#FFFF00"|transit

|2030

|1.25

|5944

|

Kepler-1220b

|

|0.136

|7.42693741

|

|

|style="background:#FFFF00"|transit

|3120

|1

|5842

|

Kepler-1221b

|

|0.168

|12.00096042

|

|

|style="background:#FFFF00"|transit

|2960

|0.87

|5194

|

Kepler-1222b

|

|0.07

|1.91694425

|

|

|style="background:#FFFF00"|transit

|1480

|0.84

|5239

|

Kepler-1223b

|

|0.109

|16.301259

|

|

|style="background:#FFFF00"|transit

|1480

|0.8

|4870

|

Kepler-1224b

|

|0.119

|13.32351601

|

|

|style="background:#FFFF00"|transit

|1890

|1.18

|6155

|

Kepler-1225b

|

|0.162

|7.01075434

|

|

|style="background:#FFFF00"|transit

|4050

|1.13

|6140

|

Kepler-1226b

|

|0.129

|17.2923453

|

|

|style="background:#FFFF00"|transit

|2540

|1.02

|5923

|

Kepler-1227b

|

|0.204

|94.2887577

|

|

|style="background:#FFFF00"|transit

|2180

|0.97

|5747

|

Kepler-1228b

|

|0.137

|0.57736958

|

|

|style="background:#FFFF00"|transit

|1780

|0.78

|5063

|

Kepler-1229b

|

|0.125

|86.828989

|

|

|style="background:#FFFF00"|transit

|770

|0.54

|3784

| Potentially habitable exoplanet{{citation|arxiv=1801.00748|year=2018|title=Habitability of Exoplanet Waterworlds|doi=10.3847/1538-4357/aad6e0|last1=Kite|first1=Edwin S.|last2=Ford|first2=Eric B.|journal=The Astrophysical Journal|volume=864|issue=1|page=75|bibcode=2018ApJ...864...75K|s2cid=46991835 |doi-access=free }}

Kepler-1230b

|

|0.242

|9.95661537

|

|

|style="background:#FFFF00"|transit

|4670

|1.06

|5961

|

Kepler-1231b

|

|0.127

|10.41725184

|

|

|style="background:#FFFF00"|transit

|3090

|1.01

|5778

|

Kepler-1232b

|

|0.172

|26.7839183

|

|

|style="background:#FFFF00"|transit

|2400

|0.92

|5471

|

Kepler-1233b

|

|0.232

|45.1263042

|

|

|style="background:#FFFF00"|transit

|4180

|1.16

|6198

|

Kepler-1234b

|

|0.251

|11.94014029

|

|

|style="background:#FFFF00"|transit

|2820

|0.8

|4967

|

Kepler-1235b

|

|0.07

|4.16055856

|

|

|style="background:#FFFF00"|transit

|1740

|0.93

|5541

|

Kepler-1236b

|

|0.191

|31.0571618

|

|

|style="background:#FFFF00"|transit

|3520

|0.86

|5337

|

Kepler-1237b

|

|0.255

|84.5733226

|

|

|style="background:#FFFF00"|transit

|3660

|0.94

|5472

|

Kepler-1238b

|

|0.172

|4.14787559

|

|

|style="background:#FFFF00"|transit

|5000

|1.3

|6386

|

Kepler-1239b

|

|0.259

|5.19104016

|

|

|style="background:#FFFF00"|transit

|8190

|1.4

|6564

|

Kepler-1240b

|

|0.103

|4.8663815

|

|

|style="background:#FFFF00"|transit

|2000

|0.98

|5682

|

Kepler-1241b

|

|0.235

|18.5525701

|

|

|style="background:#FFFF00"|transit

|3050

|0.84

|5261

|

Kepler-1242b

|

|0.202

|13.62798432

|

|

|style="background:#FFFF00"|transit

|2220

|0.77

|4895

|

Kepler-1243b

|

|0.156

|16.8320729

|

|

|style="background:#FFFF00"|transit

|2860

|0.96

|5667

|

Kepler-1244b

|

|0.12

|3.70428172

|

|

|style="background:#FFFF00"|transit

|2490

|1.46

|6680

|

Kepler-1245b

|

|0.128

|4.35409304

|

|

|style="background:#FFFF00"|transit

|2810

|0.86

|5306

|

Kepler-1245c

|

|0.128

|2.93658468

|

|

|style="background:#FFFF00"|transit

|2810

|0.86

|5306

|

Kepler-1246b

|

|0.121

|11.32271513

|

|

|style="background:#FFFF00"|transit

|1420

|0.73

|4611

|

Kepler-1247b

|

|0.208

|13.71220213

|

|

|style="background:#FFFF00"|transit

|3570

|0.86

|5303

|

Kepler-1248b

|

|0.105

|7.46725407

|

|

|style="background:#FFFF00"|transit

|1800

|1.21

|6149

|

Kepler-1249b

|

|0.212

|24.3347127

|

|

|style="background:#FFFF00"|transit

|5460

|1.19

|6202

|

Kepler-1250b

|

|0.171

|2.60754383

|

|

|style="background:#FFFF00"|transit

|4470

|0.99

|5717

|

Kepler-1251b

|

|0.164

|45.0904643

|

|

|style="background:#FFFF00"|transit

|2810

|0.92

|5545

|

Kepler-1252b

|

|0.149

|15.0540329

|

|

|style="background:#FFFF00"|transit

|2700

|1.06

|5949

|

Kepler-1253b

|

|0.119

|68.8861915

|

|

|style="background:#FFFF00"|transit

|1300

|0.97

|5850

|

Kepler-1254b

|

|0.138

|9.99113313

|

|

|style="background:#FFFF00"|transit

|2200

|0.78

|4985

|

Kepler-1254c

|

|0.116

|3.60084276

|

|

|style="background:#FFFF00"|transit

|2200

|0.78

|4985

|

Kepler-1254d

|

|0.117

|5.72717226

|

|

|style="background:#FFFF00"|transit

|2200

|0.78

|4985

|

Kepler-1255b

|

|0.207

|36.2919336

|

|

|style="background:#FFFF00"|transit

|4380

|1.08

|6018

|

Kepler-1256b

|

|0.133

|12.4127754

|

|

|style="background:#FFFF00"|transit

|2810

|1.17

|6129

|

Kepler-1257b

|

|0.136

|2.66831376

|

|

|style="background:#FFFF00"|transit

|3530

|0.9

|5502

|

Kepler-1258b

|

|0.077

|0.98494017

|

|

|style="background:#FFFF00"|transit

|2120

|0.99

|5839

|

Kepler-1259b

|

|0.128

|0.66308526

|

|

|style="background:#FFFF00"|transit

|2300

|0.8

|5053

|

Kepler-1260b

|

|0.158

|19.1187753

|

|

|style="background:#FFFF00"|transit

|3400

|1.06

|5961

|

Kepler-1261b

|

|0.202

|48.4308991

|

|

|style="background:#FFFF00"|transit

|2590

|0.82

|5006

|

Kepler-1262b

|

|0.162

|8.67900242

|

|

|style="background:#FFFF00"|transit

|3760

|0.99

|5771

|

Kepler-1263b

|

|0.102

|4.55139967

|

|

|style="background:#FFFF00"|transit

|2270

|0.84

|5213

|

Kepler-1264b

|

|0.105

|0.96852602

|

|

|style="background:#FFFF00"|transit

|2650

|0.99

|5791

|

Kepler-1265b

|

|0.12

|6.49441289

|

|

|style="background:#FFFF00"|transit

|1890

|0.71

|4630

|

Kepler-1266b

|

|0.23

|28.474748

|

|

|style="background:#FFFF00"|transit

|2940

|0.8

|5044

|

Kepler-1267b

|

|0.269

|13.0313945

|

|

|style="background:#FFFF00"|transit

|5310

|1.15

|6096

|

Kepler-1268b

|

|0.181

|40.9903986

|

|

|style="background:#FFFF00"|transit

|4590

|1.06

|5904

|

Kepler-1269b

|

|0.145

|37.3331536

|

|

|style="background:#FFFF00"|transit

|2300

|1.1

|5998

|

Kepler-1270b

|

|0.296

|6.03356196

|

|

|style="background:#FFFF00"|transit

|3930

|1.28

|5047

|

Kepler-1271b

|

|0.132

|3.0255955

|

|

|style="background:#FFFF00"|transit

|2890

|1.13

|6143

|

Kepler-1272b

|

|0.211

|51.1309704

|

|

|style="background:#FFFF00"|transit

|2920

|1.06

|5926

|

Kepler-1273b

|

|0.222

|28.625653

|

|

|style="background:#FFFF00"|transit

|4420

|0.94

|5566

|

Kepler-1274b

|

|0.127

|6.98152703

|

|

|style="background:#FFFF00"|transit

|1990

|1.45

|6179

|

Kepler-1275b

|

|0.132

|3.65691115

|

|

|style="background:#FFFF00"|transit

|4200

|1.23

|6296

|

Kepler-1276b

|

|0.106

|12.5720095

|

|

|style="background:#FFFF00"|transit

|1910

|1.14

|6188

|

Kepler-1277b

|

|0.143

|40.8365012

|

|

|style="background:#FFFF00"|transit

|1980

|0.94

|5578

|

Kepler-1278b

|

|0.09

|3.23941344

|

|

|style="background:#FFFF00"|transit

|2420

|1.11

|6074

|

Kepler-1279b

|

|0.156

|23.4774101

|

|

|style="background:#FFFF00"|transit

|3320

|1.21

|6221

|

Kepler-1280b

|

|0.167

|66.5579057

|

|

|style="background:#FFFF00"|transit

|3280

|1.2

|6227

|

Kepler-1281b

|

|0.146

|3.11602791

|

|

|style="background:#FFFF00"|transit

|3600

|0.87

|5353

|

Kepler-1282b

|

|0.138

|2.13194651

|

|

|style="background:#FFFF00"|transit

|3670

|0.92

|5504

|

Kepler-1283b

|

|0.17

|12.9460978

|

|

|style="background:#FFFF00"|transit

|4740

|1.16

|6175

|

Kepler-1284b

|

|0.108

|0.66407381

|

|

|style="background:#FFFF00"|transit

|2780

|0.84

|5123

|

Kepler-1285b

|

|0.087

|14.7967458

|

|

|style="background:#FFFF00"|transit

|1190

|1.2

|6170

|

Kepler-1286b

|

|0.192

|11.25402929

|

|

|style="background:#FFFF00"|transit

|3800

|1

|5753

|

Kepler-1287b

|

|0.137

|11.47685909

|

|

|style="background:#FFFF00"|transit

|3350

|0.96

|5715

|

Kepler-1288b

|

|0.1

|2.76122421

|

|

|style="background:#FFFF00"|transit

|2330

|1.2

|6132

|

Kepler-1289b

|

|0.136

|7.99019627

|

|

|style="background:#FFFF00"|transit

|3450

|1.1

|6080

|

Kepler-1290b

|

|0.127

|4.69500134

|

|

|style="background:#FFFF00"|transit

|4310

|0.95

|5660

|

Kepler-1291b

|

|0.148

|8.63043276

|

|

|style="background:#FFFF00"|transit

|3200

|0.84

|5216

|

Kepler-1292b

|

|0.162

|3.27646405

|

|

|style="background:#FFFF00"|transit

|4590

|0.95

|5556

|

Kepler-1293b

|

|0.087

|5.57654784

|

|

|style="background:#FFFF00"|transit

|2500

|1.18

|6241

|

Kepler-1294b

|

|0.285

|115.6862258

|

|

|style="background:#FFFF00"|transit

|3700

|0.99

|5776

|

Kepler-1295b

|

|0.138

|3.81371974

|

|

|style="background:#FFFF00"|transit

|4100

|0.92

|5486

|

Kepler-1296b

|

|0.081

|8.3839865

|

|

|style="background:#FFFF00"|transit

|2060

|0.87

|5359

|

Kepler-1297b

|

|0.087

|1.68189002

|

|

|style="background:#FFFF00"|transit

|3250

|0.99

|5818

|

Kepler-1298b

|

|0.117

|7.12811928

|

|

|style="background:#FFFF00"|transit

|1620

|1.45

|6339

|

Kepler-1299b

|

|0.266

|19.9400874

|

|

|style="background:#FFFF00"|transit

|4410

|0.94

|5609

|

Kepler-1300b

|

|0.122

|22.2419092

|

|

|style="background:#FFFF00"|transit

|2470

|1.29

|6130

|

Kepler-1301b

|

|0.125

|9.08237046

|

|

|style="background:#FFFF00"|transit

|2660

|0.85

|5188

|

Kepler-1302b

|

|0.128

|8.83922659

|

|

|style="background:#FFFF00"|transit

|2370

|0.86

|5236

|

Kepler-1303b

|

|0.127

|7.56127224

|

|

|style="background:#FFFF00"|transit

|2950

|1.01

|5771

|

Kepler-1304b

|

|0.204

|16.1288853

|

|

|style="background:#FFFF00"|transit

|2220

|0.85

|5259

|

Kepler-1305b

|

|0.168

|13.5630972

|

|

|style="background:#FFFF00"|transit

|4380

|0.97

|5701

|

Kepler-1306b

|

|0.17

|16.29595382

|

|

|style="background:#FFFF00"|transit

|3700

|0.98

|5727

|

Kepler-1307b

|

|0.22

|18.01621096

|

|

|style="background:#FFFF00"|transit

|4550

|1.06

|5884

|

Kepler-1308b

|

|0.046

|2.10433812

|

|

|style="background:#FFFF00"|transit

|240

|0.35

|3468

|

Kepler-1309b

|

|0.211

|28.8432647

|

|

|style="background:#FFFF00"|transit

|2760

|0.85

|5235

|

Kepler-1310b

|

|0.128

|0.67933627

|

|

|style="background:#FFFF00"|transit

|1900

|0.91

|5549

|

Kepler-1311b

|

|0.111

|11.1726994

|

|

|style="background:#FFFF00"|transit

|2300

|1.05

|5748

|

Kepler-1311c

|

|0.109

|2.53573424

|

|

|style="background:#FFFF00"|transit

|2300

|1.05

|5748

|

Kepler-1312b

|

|0.187

|5.44832529

|

|

|style="background:#FFFF00"|transit

|990

|0.99

|5719

|

Kepler-1313b

|

|0.157

|3.83309118

|

|

|style="background:#FFFF00"|transit

|610

|0.92

|5453

|

Kepler-1314b

|

|0.456

|5.42474928

|

|

|style="background:#FFFF00"|transit

|1510

|0.6

|4188

|

Kepler-1315b

|

|0.123

|0.84338011

|

|

|style="background:#FFFF00"|transit

|1650

|0.8

|4861

|

Kepler-1316b

|

|0.316

|87.9732136

|

|

|style="background:#FFFF00"|transit

|2460

|1.04

|5884

|

Kepler-1317b

|

|0.139

|0.56887443

|

|

|style="background:#FFFF00"|transit

|2390

|0.83

|5144

|

Kepler-1318b

|

|0.277

|213.257663

|

|

|style="background:#FFFF00"|transit

|1550

|0.73

|4598

|

Kepler-1319b

|

|0.12

|2.88676265

|

|

|style="background:#FFFF00"|transit

|370

|0.56

|3655

|

Kepler-1320b

|

|0.152

|0.86838653

|

|

|style="background:#FFFF00"|transit

|2510

|0.8

|4817

|

Kepler-1321b

|

|0.439

|11.12830484

|

|

|style="background:#FFFF00"|transit

|1780

|0.54

|4094

|

Kepler-1321c

|

|0.214

|2.22649109

|

|

|style="background:#FFFF00"|transit

|1780

|0.54

|4094

|

Kepler-1322b

|

|0.144

|0.96286738

|

|

|style="background:#FFFF00"|transit

|3970

|0.9

|5488

|

Kepler-1323b

|

|0.136

|0.92990668

|

|

|style="background:#FFFF00"|transit

|1700

|1.18

|6169

|

Kepler-1324b

|

|0.135

|4.11584468

|

|

|style="background:#FFFF00"|transit

|1700

|0.78

|4776

|

Kepler-1325b

|

|0.255

|33.8786838

|

|

|style="background:#FFFF00"|transit

|3110

|0.93

|5550

|

Kepler-1326b

|

|0.373

|42.3514267

|

|

|style="background:#FFFF00"|transit

|3000

|1.45

|6725

|

Kepler-1327b

|

|0.161

|14.88801098

|

|

|style="background:#FFFF00"|transit

|2240

|1.02

|5885

|

Kepler-1328b

|

|0.087

|4.52158888

|

|

|style="background:#FFFF00"|transit

|2100

|1

|5780

|

Kepler-1329b

|

|0.194

|9.33646594

|

|

|style="background:#FFFF00"|transit

|2040

|0.72

|4500

|

Kepler-1330b

|

|0.147

|10.10769068

|

|

|style="background:#FFFF00"|transit

|3060

|0.97

|5608

|

Kepler-1331b

|

|0.094

|0.78916165

|

|

|style="background:#FFFF00"|transit

|1190

|0.72

|4508

|

Kepler-1332b

|

|0.122

|11.87456832

|

|

|style="background:#FFFF00"|transit

|1680

|0.95

|5581

|

Kepler-1333b

|

|0.251

|109.6471842

|

|

|style="background:#FFFF00"|transit

|3120

|0.94

|5628

|

Kepler-1334b

|

|0.204

|15.64591713

|

|

|style="background:#FFFF00"|transit

|3410

|0.94

|5614

|

Kepler-1335b

|

|0.129

|6.26406846

|

|

|style="background:#FFFF00"|transit

|2050

|0.77

|4903

|

Kepler-1336b

|

|0.177

|23.198681

|

|

|style="background:#FFFF00"|transit

|2680

|0.94

|5512

|

Kepler-1336c

|

|0.153

|5.77721211

|

|

|style="background:#FFFF00"|transit

|2680

|0.94

|5512

|

Kepler-1337b

|

|0.215

|24.4002549

|

|

|style="background:#FFFF00"|transit

|1920

|0.7

|4523

|

Kepler-1338b

|

|0.082

|0.93511806

|

|

|style="background:#FFFF00"|transit

|2020

|1.04

|5909

|

Kepler-1339b

|

|0.063

|1.34155513

|

|

|style="background:#FFFF00"|transit

|870

|0.94

|5586

|

Kepler-1340b

|

|0.138

|0.66502692

|

|

|style="background:#FFFF00"|transit

|4630

|1.27

|6331

|

Kepler-1341b

|

|0.267

|132.9968322

|

|

|style="background:#FFFF00"|transit

|1520

|0.79

|4662

|

Kepler-1342b

|

|0.148

|2.21571036

|

|

|style="background:#FFFF00"|transit

|3070

|0.93

|5527

|

Kepler-1343b

|

|0.172

|3.35183158

|

|

|style="background:#FFFF00"|transit

|4260

|0.95

|5759

|

Kepler-1344b

|

|0.164

|4.7683049

|

|

|style="background:#FFFF00"|transit

|2780

|1.09

|5981

|

Kepler-1345b

|

|0.211

|44.6169557

|

|

|style="background:#FFFF00"|transit

|3800

|1.32

|6449

|

Kepler-1346b

|

|0.141

|3.40165668

|

|

|style="background:#FFFF00"|transit

|3660

|1.14

|6133

|

Kepler-1347b

|

|0.092

|14.00947528

|

|

|style="background:#FFFF00"|transit

|1050

|0.82

|5193

|

Kepler-1348b

|

|0.173

|27.5722742

|

|

|style="background:#FFFF00"|transit

|3370

|1.04

|5911

|

Kepler-1349b

|

|0.062

|2.12823928

|

|

|style="background:#FFFF00"|transit

|850

|1.16

|6086

|

Kepler-1350b

|

|0.225

|4.4968604

|

|

|style="background:#FFFF00"|transit

|1100

|0.55

|3827

|

Kepler-1350c

|

|0.154

|1.76678906

|

|

|style="background:#FFFF00"|transit

|1100

|0.55

|3827

|

Kepler-1351b

|

|0.058

|0.91614077

|

|

|style="background:#FFFF00"|transit

|790

|0.7

|4439

|

Kepler-1352b

|

|0.079

|1.87788275

|

|

|style="background:#FFFF00"|transit

|2080

|1.11

|6118

|

Kepler-1353b

|

|0.161

|24.7543966

|

|

|style="background:#FFFF00"|transit

|1940

|0.76

|4776

|

Kepler-1354b

|

|0.265

|76.613377

|

|

|style="background:#FFFF00"|transit

|3450

|1.16

|6168

|

Kepler-1355b

|

|0.13

|1.28958811

|

|

|style="background:#FFFF00"|transit

|3140

|0.88

|5352

|

Kepler-1356b

|

|0.136

|0.63400294

|

|

|style="background:#FFFF00"|transit

|2870

|0.82

|5106

|

Kepler-1357b

|

|0.114

|3.0091324

|

|

|style="background:#FFFF00"|transit

|3350

|0.93

|5597

|

Kepler-1358b

|

|0.1

|7.06317341

|

|

|style="background:#FFFF00"|transit

|1820

|0.82

|5181

|

Kepler-1359b

|

|0.252

|59.4970952

|

|

|style="background:#FFFF00"|transit

|2180

|0.78

|4709

|

Kepler-1360b

|

|0.303

|40.5286413

|

|

|style="background:#FFFF00"|transit

|4580

|1.51

|6778

|

Kepler-1361b

|

|0.077

|3.57554956

|

|

|style="background:#FFFF00"|transit

|1320

|0.83

|5131

|

Kepler-1362b

|

|0.232

|136.205626

|

|

|style="background:#FFFF00"|transit

|2500

|0.8

|4857

|

Kepler-1363b

|

|0.112

|2.94194094

|

|

|style="background:#FFFF00"|transit

|1820

|0.76

|4839

|

Kepler-1364b

|

|0.192

|13.32196237

|

|

|style="background:#FFFF00"|transit

|3750

|1.49

|6805

|

Kepler-1365b

|

|0.082

|7.69993485

|

|

|style="background:#FFFF00"|transit

|1760

|1

|5770

|

Kepler-1365c

|

|0.071

|4.77468005

|

|

|style="background:#FFFF00"|transit

|1760

|1

|5770

|

Kepler-1366b

|

|0.128

|2.16457097

|

|

|style="background:#FFFF00"|transit

|1290

|0.62

|4070

|

Kepler-1367b

|

|0.082

|1.57409027

|

|

|style="background:#FFFF00"|transit

|1160

|0.62

|4106

|

Kepler-1368b

|

|0.147

|0.67564949

|

|

|style="background:#FFFF00"|transit

|5700

|1.07

|5906

|

Kepler-1369b

|

|0.24

|25.873148

|

|

|style="background:#FFFF00"|transit

|4030

|0.99

|5761

|

Kepler-1370b

|

|0.164

|20.2641684

|

|

|style="background:#FFFF00"|transit

|2860

|1.19

|6202

|

Kepler-1370c

|

|0.113

|7.44142113

|

|

|style="background:#FFFF00"|transit

|2860

|1.19

|6202

|

Kepler-1371b

|

|0.065

|3.4462039

|

|

|style="background:#FFFF00"|transit

|1500

|0.87

|5361

|

Kepler-1371c

|

|0.057

|2.00541269

|

|

|style="background:#FFFF00"|transit

|1500

|0.87

|5361

|

Kepler-1372b

|

|0.113

|1.31155557

|

|

|style="background:#FFFF00"|transit

|3790

|0.98

|5677

|

Kepler-1373b

|

|0.103

|1.29123275

|

|

|style="background:#FFFF00"|transit

|3630

|1.22

|6299

|

Kepler-1374b

|

|0.204

|10.65276707

|

|

|style="background:#FFFF00"|transit

|3700

|0.85

|5323

|

Kepler-1375b

|

|0.155

|3.3004192

|

|

|style="background:#FFFF00"|transit

|4040

|1.47

|6704

|

Kepler-1376b

|

|0.094

|5.30880656

|

|

|style="background:#FFFF00"|transit

|2820

|0.98

|5659

|

Kepler-1377b

|

|0.112

|0.74092842

|

|

|style="background:#FFFF00"|transit

|3320

|0.86

|5218

|

Kepler-1378b

|

|0.196

|11.95398936

|

|

|style="background:#FFFF00"|transit

|1830

|0.7

|4407

|

Kepler-1379b

|

|0.116

|0.88184115

|

|

|style="background:#FFFF00"|transit

|3100

|0.83

|5188

|

Kepler-1380b

|

|0.128

|10.3108245

|

|

|style="background:#FFFF00"|transit

|3940

|0.96

|5570

|

Kepler-1381b

|

|0.201

|25.3842686

|

|

|style="background:#FFFF00"|transit

|4260

|0.96

|5747

|

Kepler-1382b

|

|0.168

|16.3583055

|

|

|style="background:#FFFF00"|transit

|2400

|1.36

|6161

|

Kepler-1383b

|

|0.126

|13.9093583

|

|

|style="background:#FFFF00"|transit

|3130

|1.26

|6370

|

Kepler-1384b

|

|0.173

|15.36262753

|

|

|style="background:#FFFF00"|transit

|2020

|0.78

|4919

|

Kepler-1385b

|

|0.076

|2.88879862

|

|

|style="background:#FFFF00"|transit

|1720

|1.15

|5732

|

Kepler-1386b

|

|0.111

|6.73972381

|

|

|style="background:#FFFF00"|transit

|2730

|1.02

|5733

|

Kepler-1387b

|

|0.083

|2.27952666

|

|

|style="background:#FFFF00"|transit

|1600

|0.82

|5046

|

Kepler-1388b

|

|0.231

|12.2854603

|

|

|style="background:#FFFF00"|transit

|1600

|0.63

|4098

|

Kepler-1388c

|

|0.202

|5.53608151

|

|

|style="background:#FFFF00"|transit

|1600

|0.63

|4098

|

Kepler-1388d

|

|0.255

|20.9568158

|

|

|style="background:#FFFF00"|transit

|1600

|0.63

|4098

|

Kepler-1388e

|

|0.219

|37.6327084

|

|

|style="background:#FFFF00"|transit

|1600

|0.63

|4098

|

Kepler-1389b

|

|0.158

|99.2530951

|

|

|style="background:#FFFF00"|transit

|1700

|0.81

|5078

|

Kepler-1390b

|

|0.105

|6.48021673

|

|

|style="background:#FFFF00"|transit

|2500

|0.98

|5753

|

Kepler-1391b

|

|0.15

|54.4092333

|

|

|style="background:#FFFF00"|transit

|2350

|1.03

|5840

|

Kepler-1392b

|

|0.175

|15.1410397

|

|

|style="background:#FFFF00"|transit

|3640

|0.88

|5479

|

Kepler-1393b

|

|0.071

|2.44357812

|

|

|style="background:#FFFF00"|transit

|1510

|0.95

|5697

|

Kepler-1394b

|

|0.124

|3.93766373

|

|

|style="background:#FFFF00"|transit

|2700

|1.64

|6481

|

Kepler-1395b

|

|0.071

|3.78470649

|

|

|style="background:#FFFF00"|transit

|1650

|1.17

|6138

|

Kepler-1396b

|

|0.185

|18.2206421

|

|

|style="background:#FFFF00"|transit

|4030

|1.18

|6195

|

Kepler-1397b

|

|0.153

|47.449955

|

|

|style="background:#FFFF00"|transit

|2500

|1.09

|6026

|

Kepler-1398b

|

|0.08

|2.78815679

|

|

|style="background:#FFFF00"|transit

|2590

|1.13

|6126

|

Kepler-1398c

|

|0.092

|4.13827595

|

|

|style="background:#FFFF00"|transit

|2590

|1.13

|6126

|

Kepler-1399b

|

|0.112

|1.63865306

|

|

|style="background:#FFFF00"|transit

|4100

|0.97

|5735

|

Kepler-1400b

|

|0.145

|9.06689421

|

|

|style="background:#FFFF00"|transit

|2870

|0.83

|5044

|

Kepler-1401b

|

|0.15

|11.20066445

|

|

|style="background:#FFFF00"|transit

|4050

|1.07

|5964

|

Kepler-1402b

|

|0.068

|2.03387914

|

|

|style="background:#FFFF00"|transit

|2220

|0.9

|5416

|

Kepler-1403b

|

|0.191

|5.19492202

|

|

|style="background:#FFFF00"|transit

|5870

|1.11

|6060

|

Kepler-1404b

|

|0.179

|15.9314739

|

|

|style="background:#FFFF00"|transit

|3090

|0.84

|5261

|

Kepler-1405b

|

|0.353

|28.2274184

|

|

|style="background:#FFFF00"|transit

|5230

|1.05

|5925

|

Kepler-1406b

|

|0.098

|11.62905828

|

|

|style="background:#FFFF00"|transit

|1910

|1.05

|5892

|

Kepler-1407b

|

|0.201

|20.0711504

|

|

|style="background:#FFFF00"|transit

|4160

|1.1

|6010

|

Kepler-1408b

|

|0.079

|2.99793191

|

|

|style="background:#FFFF00"|transit

|1390

|1.21

|6170

|

Kepler-1409b

|

|0.093

|0.76486493

|

|

|style="background:#FFFF00"|transit

|2350

|0.83

|5160

|

Kepler-1410b

|

|0.159

|60.866168

|

|

|style="background:#FFFF00"|transit

|1200

|0.63

|4092

| Potentially habitable exoplanet{{citation|arxiv=1911.04441|year=2019|chapter=|doi=10.2458/azu_uapress_9780816540068|title=Planetary Astrobiology|isbn=978-0-8165-4006-8|author1=Ravi kumar Kopparapu|last2=Wolf|first2=Eric T.|last3=Meadows|first3=Victoria S.|s2cid=209140478 }}

Kepler-1411b

|

|0.252

|86.1150888

|

|

|style="background:#FFFF00"|transit

|4670

|0.95

|5664

|

Kepler-1412b

|

|0.074

|3.6146051

|

|

|style="background:#FFFF00"|transit

|2080

|1.06

|5880

|

Kepler-1413b

|

|0.162

|13.1829642

|

|

|style="background:#FFFF00"|transit

|3790

|0.84

|5196

|

Kepler-1414b

|

|0.11

|3.51576315

|

|

|style="background:#FFFF00"|transit

|1740

|0.8

|4951

|

Kepler-1415b

|

|0.115

|0.63642408

|

|

|style="background:#FFFF00"|transit

|3480

|0.89

|5267

|

Kepler-1416b

|

|0.079

|1.49514952

|

|

|style="background:#FFFF00"|transit

|2630

|1.09

|6019

|

Kepler-1417b

|

|0.089

|20.3505213

|

|

|style="background:#FFFF00"|transit

|2140

|1.02

|5839

|

Kepler-1418b

|

|0.148

|22.4764425

|

|

|style="background:#FFFF00"|transit

|1630

|0.77

|4770

|

Kepler-1419b

|

|0.255

|42.5215895

|

|

|style="background:#FFFF00"|transit

|4710

|1.01

|5796

|

Kepler-1420b

|

|0.114

|6.69960006

|

|

|style="background:#FFFF00"|transit

|3010

|0.82

|5187

|

Kepler-1421b

|

|0.083

|6.9131112

|

|

|style="background:#FFFF00"|transit

|2200

|1.25

|6335

|

Kepler-1422b

|

|0.18

|18.6051942

|

|

|style="background:#FFFF00"|transit

|6790

|1.15

|6194

|

Kepler-1423b

|

|0.095

|23.955378

|

|

|style="background:#FFFF00"|transit

|1460

|0.79

|4939

|

Kepler-1424b

|

|0.103

|29.6091744

|

|

|style="background:#FFFF00"|transit

|2000

|1.02

|5838

|

Kepler-1425b

|

|0.084

|14.4541302

|

|

|style="background:#FFFF00"|transit

|1630

|0.97

|5718

|

Kepler-1426b

|

|0.139

|14.2563227

|

|

|style="background:#FFFF00"|transit

|3950

|1.02

|5831

|

Kepler-1427b

|

|0.098

|0.96897238

|

|

|style="background:#FFFF00"|transit

|4000

|1.01

|5793

|

Kepler-1428b

|

|0.146

|10.67607169

|

|

|style="background:#FFFF00"|transit

|2620

|1.28

|6184

|

Kepler-1429b

|

|0.115

|4.48487493

|

|

|style="background:#FFFF00"|transit

|3770

|1.05

|5902

|

Kepler-1430b

|

|0.105

|2.46050993

|

|

|style="background:#FFFF00"|transit

|1760

|0.77

|4796

|

Kepler-1431b

|

|0.131

|5.86601526

|

|

|style="background:#FFFF00"|transit

|4100

|1.03

|5806

|

Kepler-1432b

|

|0.198

|23.9109011

|

|

|style="background:#FFFF00"|transit

|5060

|1.09

|6031

|

Kepler-1433b

|

|0.139

|4.13592271

|

|

|style="background:#FFFF00"|transit

|4330

|1.14

|6097

|

Kepler-1434b

|

|0.099

|8.05333618

|

|

|style="background:#FFFF00"|transit

|2200

|1.47

|6291

|

Kepler-1435b

|

|0.077

|4.45343281

|

|

|style="background:#FFFF00"|transit

|2220

|1.21

|6356

|

Kepler-1436b

|

|0.117

|9.705716

|

|

|style="background:#FFFF00"|transit

|3720

|1.06

|5972

|

Kepler-1437b

|

|0.122

|10.9295461

|

|

|style="background:#FFFF00"|transit

|3860

|0.93

|5557

|

Kepler-1438b

|

|0.084

|2.31942009

|

|

|style="background:#FFFF00"|transit

|2820

|0.97

|5530

|

Kepler-1439b

|

|0.13

|8.07392849

|

|

|style="background:#FFFF00"|transit

|700

|0.46

|3578

|

Kepler-1440b

|

|0.112

|39.859484

|

|

|style="background:#FFFF00"|transit

|2230

|0.98

|5698

|

Kepler-1441b

|

|0.117

|39.4419839

|

|

|style="background:#FFFF00"|transit

|2450

|1

|5802

|

Kepler-1442b

|

|0.351

|81.4162941

|

|

|style="background:#FFFF00"|transit

|1710

|1.34

|6394

|

Kepler-1443b

|

|0.087

|2.41811321

|

|

|style="background:#FFFF00"|transit

|1550

|1.19

|6289

|

Kepler-1444b

|

|0.194

|33.42035034

|

|

|style="background:#FFFF00"|transit

|1100

|1.03

|5810

|

Kepler-1445b

|

|0.086

|10.60052251

|

|

|style="background:#FFFF00"|transit

|1570

|1.13

|6150

|

Kepler-1446b

|

|0.073

|0.68996783

|

|

|style="background:#FFFF00"|transit

|530

|0.81

|4865

|

Kepler-1447b

|

|0.259

|56.6747285

|

|

|style="background:#FFFF00"|transit

|2840

|0.97

|5722

|

Kepler-1448b

|

|0.144

|12.27065865

|

|

|style="background:#FFFF00"|transit

|2560

|0.95

|5774

|

Kepler-1449b

|

|0.15

|13.2274528

|

|

|style="background:#FFFF00"|transit

|4310

|1.08

|5979

|

Kepler-1450b

|

|0.153

|54.5094166

|

|

|style="background:#FFFF00"|transit

|1600

|0.71

|4524

|

Kepler-1451b

|

|0.299

|35.622233

|

|

|style="background:#FFFF00"|transit

|3780

|1

|5782

|

Kepler-1452b

|

|0.241

|42.913751

|

|

|style="background:#FFFF00"|transit

|3180

|1.41

|6101

|

Kepler-1453b

|

|0.238

|47.1611696

|

|

|style="background:#FFFF00"|transit

|4190

|0.97

|5665

|

Kepler-1454b

|

|0.168

|47.0319479

|

|

|style="background:#FFFF00"|transit

|2590

|0.9

|5448

|

Kepler-1455b

|

|0.193

|49.276764

|

|

|style="background:#FFFF00"|transit

|1280

|0.62

|4075

| Potentially habitable exoplanet

Kepler-1456b

|

|0.102

|18.1373829

|

|

|style="background:#FFFF00"|transit

|1240

|0.64

|4231

|

Kepler-1457b

|

|0.178

|51.1110243

|

|

|style="background:#FFFF00"|transit

|2370

|1.01

|5866

|

Kepler-1458b

|

|0.246

|47.9872764

|

|

|style="background:#FFFF00"|transit

|2090

|0.96

|5653

|

Kepler-1459b

|

|0.121

|62.8691611

|

|

|style="background:#FFFF00"|transit

|1420

|0.78

|4828

|

Kepler-1460b

|

|0.175

|29.9633247

|

|

|style="background:#FFFF00"|transit

|1870

|0.7

|4422

|

Kepler-1461b

|

|0.181

|29.3494775

|

|

|style="background:#FFFF00"|transit

|2450

|0.79

|4919

|

Kepler-1462b

|

|0.341

|65.6488341

|

|

|style="background:#FFFF00"|transit

|4460

|1

|5756

|

Kepler-1463b

|

|0.166

|25.15864

|

|

|style="background:#FFFF00"|transit

|4370

|0.96

|5679

|

Kepler-1464b

|

|0.148

|31.7785901

|

|

|style="background:#FFFF00"|transit

|2260

|1.02

|5828

|

Kepler-1464c

|

|0.089

|5.32786292

|

|

|style="background:#FFFF00"|transit

|2260

|1.02

|5828

|

Kepler-1465b

|

|0.158

|31.8277111

|

|

|style="background:#FFFF00"|transit

|1100

|0.75

|4726

|

Kepler-1466b

|

|0.138

|31.1750448

|

|

|style="background:#FFFF00"|transit

|2240

|1.01

|5884

|

Kepler-1467b

|

|0.294

|47.0569043

|

|

|style="background:#FFFF00"|transit

|2900

|0.86

|5332

|

Kepler-1468b

|

|0.154

|8.23984869

|

|

|style="background:#FFFF00"|transit

|3700

|1.04

|5893

|

Kepler-1468c

|

|0.103

|3.54553021

|

|

|style="background:#FFFF00"|transit

|3700

|1.04

|5893

|

Kepler-1469b

|

|0.25

|21.8635301

|

|

|style="background:#FFFF00"|transit

|4090

|0.92

|5507

|

Kepler-1470b

|

|0.095

|16.2950903

|

|

|style="background:#FFFF00"|transit

|1860

|0.8

|4961

|

Kepler-1471b

|

|0.126

|3.63899398

|

|

|style="background:#FFFF00"|transit

|3450

|0.95

|5660

|

Kepler-1472b

|

|0.17

|38.1312831

|

|

|style="background:#FFFF00"|transit

|4140

|1.16

|6159

|

Kepler-1473b

|

|0.106

|14.4273551

|

|

|style="background:#FFFF00"|transit

|2040

|1.09

|6046

|

Kepler-1474b

|

|0.193

|36.4333452

|

|

|style="background:#FFFF00"|transit

|3960

|1.04

|5870

|

Kepler-1475b

|

|0.261

|82.177374

|

|

|style="background:#FFFF00"|transit

|5590

|1.18

|6214

|

Kepler-1476b

|

|0.149

|10.35863224

|

|

|style="background:#FFFF00"|transit

|3970

|0.98

|5663

|

Kepler-1477b

|

|0.105

|11.55530021

|

|

|style="background:#FFFF00"|transit

|1710

|0.81

|5100

|

Kepler-1478b

|

|0.154

|26.0840594

|

|

|style="background:#FFFF00"|transit

|4580

|1.04

|5904

|

Kepler-1479b

|

|0.163

|14.53261362

|

|

|style="background:#FFFF00"|transit

|2020

|0.99

|5796

|

Kepler-1480b

|

|0.149

|22.12679948

|

|

|style="background:#FFFF00"|transit

|1800

|0.85

|5156

|

Kepler-1481b

|

|0.11

|5.94220998

|

|

|style="background:#FFFF00"|transit

|1610

|0.8

|4908

|

Kepler-1482b

|

|0.09

|12.25383217

|

|

|style="background:#FFFF00"|transit

|1440

|0.88

|5381

|

Kepler-1483b

|

|0.136

|9.5085156

|

|

|style="background:#FFFF00"|transit

|4330

|1.25

|6337

|

Kepler-1484b

|

|0.188

|30.4549136

|

|

|style="background:#FFFF00"|transit

|3570

|0.94

|5730

|

Kepler-1485b

|

|0.131

|19.9157725

|

|

|style="background:#FFFF00"|transit

|1800

|1.11

|6087

|

Kepler-1486b

|

|0.207

|54.6495759

|

|

|style="background:#FFFF00"|transit

|4780

|1.08

|5965

|

Kepler-1487b

|

|0.19

|7.31946363

|

|

|style="background:#FFFF00"|transit

|3570

|1.38

|6541

|

Kepler-1488b

|

|0.166

|39.8189932

|

|

|style="background:#FFFF00"|transit

|2020

|1.05

|5820

|

Kepler-1489b

|

|0.158

|82.294751

|

|

|style="background:#FFFF00"|transit

|2800

|0.93

|5655

|

Kepler-1490b

|

|0.271

|92.4362973

|

|

|style="background:#FFFF00"|transit

|3160

|0.9

|5515

|

Kepler-1491b

|

|0.135

|16.5861762

|

|

|style="background:#FFFF00"|transit

|4280

|1

|5728

|

Kepler-1492b

|

|0.133

|16.75255007

|

|

|style="background:#FFFF00"|transit

|1210

|0.77

|4712

|

Kepler-1493b

|

|0.126

|15.0217983

|

|

|style="background:#FFFF00"|transit

|1870

|1.06

|5863

|

Kepler-1494b

|

|0.274

|91.080482

|

|

|style="background:#FFFF00"|transit

|3450

|0.96

|5659

|

Kepler-1495b

|

|0.262

|85.273256

|

|

|style="background:#FFFF00"|transit

|4260

|1.03

|5831

|

Kepler-1496b

|

|0.198

|64.6588017

|

|

|style="background:#FFFF00"|transit

|4220

|1.18

|6182

|

Kepler-1497b

|

|0.148

|8.74199772

|

|

|style="background:#FFFF00"|transit

|3660

|0.96

|5675

|

Kepler-1498b

|

|0.119

|48.051405

|

|

|style="background:#FFFF00"|transit

|2400

|0.86

|5256

|

Kepler-1499b

|

|0.106

|44.2008

|

|

|style="background:#FFFF00"|transit

|1000

|0.82

|5097

|

Kepler-1500b

|

|0.107

|15.0330105

|

|

|style="background:#FFFF00"|transit

|2950

|1

|5845

|

Kepler-1501b

|

|0.139

|14.5564533

|

|

|style="background:#FFFF00"|transit

|2900

|1.2

|6229

|

Kepler-1502b

|

|0.284

|41.7083629

|

|

|style="background:#FFFF00"|transit

|5000

|1.44

|6666

|

Kepler-1503b

|

|0.203

|96.16987

|

|

|style="background:#FFFF00"|transit

|2800

|0.77

|5069

|

Kepler-1504b

|

|0.19

|82.304003

|

|

|style="background:#FFFF00"|transit

|3360

|0.85

|5393

|

Kepler-1505b

|

|0.083

|30.8609366

|

|

|style="background:#FFFF00"|transit

|1170

|0.93

|5686

|

Kepler-1506b

|

|0.118

|14.0329154

|

|

|style="background:#FFFF00"|transit

|4300

|0.95

|5676

|

Kepler-1507b

|

|0.075

|16.0506213

|

|

|style="background:#FFFF00"|transit

|1120

|0.89

|5410

|

Kepler-1508b

|

|0.119

|20.7056504

|

|

|style="background:#FFFF00"|transit

|2910

|1.14

|6158

|

Kepler-1509b

|

|0.165

|25.4338197

|

|

|style="background:#FFFF00"|transit

|4170

|1

|5780

|

Kepler-1510b

|

|0.3

|84.703921

|

|

|style="background:#FFFF00"|transit

|5270

|1.19

|6200

|

Kepler-1511b

|

|0.15

|23.2382792

|

|

|style="background:#FFFF00"|transit

|2930

|1.17

|6064

|

Kepler-1512b

|

|0.105

|20.35972599

|

|

|style="background:#FFFF00"|transit

|530

|0.73

|4372

|

Kepler-1513b

|

|0.755

|160.88465087

|

|

|style="background:#FFFF00"|transit

|1250

|0.99

|5617

|

Kepler-1514b

|

|1.055

|217.8317626

|

|

|style="background:#FFFF00"|transit

|1240

|1.21

|6251

|

Kepler-1515b

|

|0.852

|214.3114164

|

|

|style="background:#FFFF00"|transit

|1640

|1.3

|6511

|

Kepler-1516b

|

|0.156

|7.25931979

|

|

|style="background:#FFFF00"|transit

|2840

|1.04

|5904

|

Kepler-1517b

|

|0.871

|5.54608367

|

|

|style="background:#FFFF00"|transit

|2830

|1.58

|7010

|

Kepler-1518b

|

|0.272

|5.11177904

|

|

|style="background:#FFFF00"|transit

|3700

|1.54

|6846

|

Kepler-1519b

|

|0.63

|240.7989397

|

|

|style="background:#FFFF00"|transit

|2800

|0.94

|5644

|

Kepler-1520b

|

|0.515

|0.65355357

|

|

|style="background:#FFFF00"|transit

|2070

|0.76

|4677

|

Kepler-1521b

|

|0.223

|47.14840805

|

|

|style="background:#FFFF00"|transit

|740

|0.81

|5042

|

Kepler-1522b

|

|0.154

|1.84788917

|

|

|style="background:#FFFF00"|transit

|2300

|0.96

|5706

|

Kepler-1523b

|

|0.141

|0.93875077

|

|

|style="background:#FFFF00"|transit

|2990

|0.97

|5708

|

Kepler-1524b

|

|0.316

|70.9674603

|

|

|style="background:#FFFF00"|transit

|1650

|1.17

|6179

|

Kepler-1525b

|

|0.081

|2.41660118

|

|

|style="background:#FFFF00"|transit

|1290

|1.07

|5748

|

Kepler-1526b

|

|0.217

|3.908632

|

|

|style="background:#FFFF00"|transit

|1880

|0.73

|4601

|

Kepler-1527b

|

|0.426

|160.129918

|

|

|style="background:#FFFF00"|transit

|5100

|1.21

|6224

|

Kepler-1528b

|

|0.13

|1.79111021

|

|

|style="background:#FFFF00"|transit

|2990

|1.03

|5857

|

Kepler-1529b

|

|0.187

|5.33905686

|

|

|style="background:#FFFF00"|transit

|2230

|0.81

|5048

|

Kepler-1530b

|

|0.146

|2.5904434

|

|

|style="background:#FFFF00"|transit

|1800

|0.92

|5477

|

Kepler-1530c

|

|0.147

|5.3227406

|

|

|style="background:#FFFF00"|transit

|1800

|0.92

|5477

|

Kepler-1531b

|

|0.099

|1.13854338

|

|

|style="background:#FFFF00"|transit

|2200

|1.16

|6260

|

Kepler-1532b

|

|0.12

|1.09366356

|

|

|style="background:#FFFF00"|transit

|2690

|0.91

|5559

|

Kepler-1533b

|

|0.309

|308.5471

|

|

|style="background:#FFFF00"|transit

|2780

|1.31

|6431

|

Kepler-1534b

|

|0.169

|5.71668872

|

|

|style="background:#FFFF00"|transit

|3610

|0.9

|5442

|

Kepler-1535b

|

|0.227

|138.9442

|

|

|style="background:#FFFF00"|transit

|2870

|1.08

|6021

|

Kepler-1536b

|

|0.28

|364.758031

|

|

|style="background:#FFFF00"|transit

|1310

|0.71

|4434

|

Kepler-1537b

|

|0.105

|1.4444538

|

|

|style="background:#FFFF00"|transit

|1640

|0.81

|5079

|

Kepler-1538b

|

|0.252

|175.138819

|

|

|style="background:#FFFF00"|transit

|4210

|1.03

|5837

|

Kepler-1539b

|

|0.241

|133.3036741

|

|

|style="background:#FFFF00"|transit

|2570

|0.84

|5176

|

Kepler-1540b

|

|0.222

|125.4131177

|

|

|style="background:#FFFF00"|transit

|850

|0.74

|4540

| Potentially habitable exoplanet{{citation|arxiv=1608.00620|year=2016|title=A Catalog Ofkeplerhabitable Zone Exoplanet Candidates|doi=10.3847/0004-637X/830/1/1 |last1=Kane |first1=Stephen R. |last2=Hill |first2=Michelle L. |last3=Kasting |first3=James F. |last4=Kopparapu |first4=Ravi Kumar |last5=Quintana |first5=Elisa V. |last6=Barclay |first6=Thomas |last7=Batalha |first7=Natalie M. |last8=Borucki |first8=William J. |last9=Ciardi |first9=David R. |last10=Haghighipour |first10=Nader |last11=Hinkel |first11=Natalie R. |last12=Kaltenegger |first12=Lisa |last13=Selsis |first13=Franck |last14=Torres |first14=Guillermo |journal=The Astrophysical Journal |volume=830 |issue=1 |page=1 |bibcode=2016ApJ...830....1K |s2cid=40859027 |doi-access=free }}

Kepler-1541b

|

|0.103

|8.40691199

|

|

|style="background:#FFFF00"|transit

|1350

|0.86

|5282

|

Kepler-1542b

|

|0.068

|3.95116882

|

|

|style="background:#FFFF00"|transit

|1100

|0.94

|5564

|

Kepler-1542c

|

|0.058

|2.89223021

|

|

|style="background:#FFFF00"|transit

|1100

|0.94

|5564

|

Kepler-1542d

|

|0.078

|5.99273738

|

|

|style="background:#FFFF00"|transit

|1100

|0.94

|5564

|

Kepler-1542e

|

|0.068

|5.10115756

|

|

|style="background:#FFFF00"|transit

|1100

|0.94

|5564

|

Kepler-1543b

|

|0.242

|6.96710269

|

|

|style="background:#FFFF00"|transit

|3630

|1.39

|6561

|

Kepler-1544b

|

|0.159

|168.811174

|

|

|style="background:#FFFF00"|transit

|1140

|0.81

|4886

| Potentially habitable exoplanet

Kepler-1545b

|

|0.241

|163.692349

|

|

|style="background:#FFFF00"|transit

|2240

|0.84

|5201

|

Kepler-1546b

|

|0.279

|19.5974971

|

|

|style="background:#FFFF00"|transit

|3240

|0.95

|5623

|

Kepler-1547b

|

|0.08

|0.69297968

|

|

|style="background:#FFFF00"|transit

|2170

|1.12

|6078

|

Kepler-1548b

|

|0.236

|124.828679

|

|

|style="background:#FFFF00"|transit

|3800

|0.99

|5706

|

Kepler-1549b

|

|0.229

|214.886545

|

|

|style="background:#FFFF00"|transit

|2580

|0.88

|5324

|

Kepler-1550b

|

|0.269

|225.582809

|

|

|style="background:#FFFF00"|transit

|3920

|1.07

|5991

|

Kepler-1551b

|

|0.237

|24.4973698

|

|

|style="background:#FFFF00"|transit

|5100

|1.14

|6136

|

Kepler-1552b

|

|0.22

|184.771853

|

|

|style="background:#FFFF00"|transit

|2020

|0.85

|5202

|

Kepler-1553b

|

|0.103

|4.24261881

|

|

|style="background:#FFFF00"|transit

|2350

|0.85

|5288

|

Kepler-1554b

|

|0.259

|198.088774

|

|

|style="background:#FFFF00"|transit

|3200

|0.84

|5297

|

Kepler-1555b

|

|0.144

|8.10501635

|

|

|style="background:#FFFF00"|transit

|4510

|1.04

|5866

|

Kepler-1556b

|

|0.175

|8.82713457

|

|

|style="background:#FFFF00"|transit

|3500

|0.97

|5608

|

Kepler-1557b

|

|0.136

|3.74032496

|

|

|style="background:#FFFF00"|transit

|5000

|1.11

|6099

|

Kepler-1558b

|

|0.061

|3.50470358

|

|

|style="background:#FFFF00"|transit

|1120

|0.83

|5101

|

Kepler-1559b

|

|0.064

|0.97191543

|

|

|style="background:#FFFF00"|transit

|1900

|0.86

|5316

|

Kepler-1560b

|

|0.079

|3.03195744

|

|

|style="background:#FFFF00"|transit

|1730

|1.02

|5815

|

Kepler-1561b

|

|0.097

|1.00520701

|

|

|style="background:#FFFF00"|transit

|3240

|1.07

|5957

|

Kepler-1562b

|

|0.317

|64.2737752

|

|

|style="background:#FFFF00"|transit

|4290

|1.02

|5760

|

Kepler-1563b

|

|0.067

|3.43276598

|

|

|style="background:#FFFF00"|transit

|1780

|1

|5765

|

Kepler-1564b

|

|0.131

|18.0540381

|

|

|style="background:#FFFF00"|transit

|2840

|0.93

|5528

|

Kepler-1565b

|

|0.106

|1.53818844

|

|

|style="background:#FFFF00"|transit

|2140

|0.76

|4940

|

Kepler-1566b

|

|0.07

|0.53991524

|

|

|style="background:#FFFF00"|transit

|1670

|0.84

|5254

|

Kepler-1567b

|

|0.244

|153.979578

|

|

|style="background:#FFFF00"|transit

|4000

|0.95

|5655

|

Kepler-1568b

|

|0.116

|20.925392

|

|

|style="background:#FFFF00"|transit

|2880

|1.09

|5956

|

Kepler-1569b

|

|0.15

|5.79180156

|

|

|style="background:#FFFF00"|transit

|3400

|1.25

|6319

|

Kepler-1570b

|

|0.095

|26.548955

|

|

|style="background:#FFFF00"|transit

|1510

|0.92

|5550

|

Kepler-1571b

|

|0.136

|3.38555488

|

|

|style="background:#FFFF00"|transit

|2620

|1.23

|6297

|

Kepler-1572b

|

|0.084

|5.49548621

|

|

|style="background:#FFFF00"|transit

|2000

|0.97

|5618

|

Kepler-1573b

|

|0.107

|2.6157554

|

|

|style="background:#FFFF00"|transit

|3800

|1.01

|5808

|

Kepler-1574b

|

|0.115

|6.9424334

|

|

|style="background:#FFFF00"|transit

|4160

|1.06

|5892

|

Kepler-1575b

|

|0.117

|2.55314213

|

|

|style="background:#FFFF00"|transit

|3800

|0.95

|5667

|

Kepler-1576b

|

|0.093

|6.98471973

|

|

|style="background:#FFFF00"|transit

|1760

|1.05

|5876

|

Kepler-1577b

|

|0.101

|6.30560247

|

|

|style="background:#FFFF00"|transit

|1770

|0.78

|4862

|

Kepler-1578b

|

|0.093

|1.45088691

|

|

|style="background:#FFFF00"|transit

|3310

|0.9

|5545

|

Kepler-1579b

|

|0.075

|0.84990789

|

|

|style="background:#FFFF00"|transit

|1520

|0.75

|4584

|

Kepler-1580b

|

|0.188

|56.6449279

|

|

|style="background:#FFFF00"|transit

|2840

|1.47

|6228

|

Kepler-1581b

|

|0.071

|6.28385491

|

|

|style="background:#FFFF00"|transit

|1440

|1.12

|6022

|

Kepler-1582b

|

|0.133

|4.83817712

|

|

|style="background:#FFFF00"|transit

|370

|0.28

|3208

|

Kepler-1583b

|

|0.054

|9.32807355

|

|

|style="background:#FFFF00"|transit

|1160

|0.94

|5645

|

Kepler-1584b

|

|0.144

|13.3997099

|

|

|style="background:#FFFF00"|transit

|4320

|1.1

|6069

|

Kepler-1585b

|

|0.16

|3.5827463

|

|

|style="background:#FFFF00"|transit

|4140

|0.94

|5538

|

Kepler-1586b

|

|0.136

|15.6049212

|

|

|style="background:#FFFF00"|transit

|2820

|1.45

|6681

|

Kepler-1587b

|

|0.119

|9.4060467

|

|

|style="background:#FFFF00"|transit

|2960

|1.08

|5933

|

Kepler-1588b

|

|0.068

|7.84931739

|

|

|style="background:#FFFF00"|transit

|2150

|0.96

|5817

|

Kepler-1589b

|

|0.097

|0.99166527

|

|

|style="background:#FFFF00"|transit

|4620

|1.18

|6166

|

Kepler-1590b

|

|0.102

|7.61760804

|

|

|style="background:#FFFF00"|transit

|2900

|1.11

|6053

|

Kepler-1591b

|

|0.113

|8.18504949

|

|

|style="background:#FFFF00"|transit

|3600

|1.1

|6082

|

Kepler-1592b

|

|0.137

|3.05710069

|

|

|style="background:#FFFF00"|transit

|4400

|1.18

|6213

|

Kepler-1593b

|

|0.283

|174.509835

|

|

|style="background:#FFFF00"|transit

|2460

|0.81

|4995

| Potentially habitable exoplanet

Kepler-1594b

|

|0.095

|2.71603809

|

|

|style="background:#FFFF00"|transit

|3600

|1.06

|5946

|

Kepler-1595b

|

|0.11

|4.56380468

|

|

|style="background:#FFFF00"|transit

|2740

|0.84

|5203

|

Kepler-1596b

|

|0.17

|66.373379

|

|

|style="background:#FFFF00"|transit

|3800

|0.95

|5706

|

Kepler-1597b

|

|0.095

|2.94654179

|

|

|style="background:#FFFF00"|transit

|4090

|1.25

|6377

|

Kepler-1598b

|

|0.085

|4.34195123

|

|

|style="background:#FFFF00"|transit

|2390

|1.07

|5940

|

Kepler-1599b

|

|0.145

|122.363553

|

|

|style="background:#FFFF00"|transit

|3270

|0.99

|5767

|

Kepler-1600b

|

|0.279

|386.370548

|

|

|style="background:#FFFF00"|transit

|3240

|0.86

|5214

|

Kepler-1601b

|

|0.073

|2.20921951

|

|

|style="background:#FFFF00"|transit

|2200

|1.04

|5869

|

Kepler-1602b

|

|0.12

|11.17931605

|

|

|style="background:#FFFF00"|transit

|2660

|1.22

|6296

|

Kepler-1603b

|

|0.115

|2.27163926

|

|

|style="background:#FFFF00"|transit

|5710

|1.21

|6241

|

Kepler-1604b

|

|0.126

|0.68368426

|

|

|style="background:#FFFF00"|transit

|1830

|0.81

|4976

|

Kepler-1605b

|

|0.096

|85.7565495

|

|

|style="background:#FFFF00"|transit

|730

|0.86

|5280

|

Kepler-1606b

|

|0.185

|196.435224

|

|

|style="background:#FFFF00"|transit

|2900

|0.9

|5422

| Potentially habitable exoplanet

Kepler-1607b

|

|0.082

|13.6473676

|

|

|style="background:#FFFF00"|transit

|2400

|1.14

|6116

|

Kepler-1608b

|

|0.154

|16.4735686

|

|

|style="background:#FFFF00"|transit

|2710

|0.75

|4992

|

Kepler-1609b

|

|0.198

|114.34219

|

|

|style="background:#FFFF00"|transit

|4840

|1.18

|6132

|

Kepler-1610b

|

|0.144

|8.70181574

|

|

|style="background:#FFFF00"|transit

|3470

|0.91

|5383

|

Kepler-1611b

|

|0.072

|5.1762429

|

|

|style="background:#FFFF00"|transit

|2240

|0.94

|5605

|

Kepler-1612b

|

|0.092

|3.91795101

|

|

|style="background:#FFFF00"|transit

|2730

|0.96

|5643

|

Kepler-1613b

|

|0.186

|1.5184299

|

|

|style="background:#FFFF00"|transit

|2790

|1.08

|6005

|

Kepler-1614b

|

|0.133

|3.9466141

|

|

|style="background:#FFFF00"|transit

|3200

|0.79

|5121

|

Kepler-1615b

|

|0.184

|47.3126192

|

|

|style="background:#FFFF00"|transit

|3100

|1.04

|5865

|

Kepler-1616b

|

|0.091

|6.76284377

|

|

|style="background:#FFFF00"|transit

|2810

|1.21

|6266

|

Kepler-1617b

|

|0.107

|27.4785572

|

|

|style="background:#FFFF00"|transit

|2650

|1.15

|6167

|

Kepler-1618b

|

|0.112

|6.10826019

|

|

|style="background:#FFFF00"|transit

|4040

|1.41

|6620

|

Kepler-1619b

|

|0.068

|23.6225913

|

|

|style="background:#FFFF00"|transit

|1700

|1

|5852

|

Kepler-1620b

|

|0.144

|101.951829

|

|

|style="background:#FFFF00"|transit

|2520

|1.15

|6157

|

Kepler-1621b

|

|0.193

|92.263714

|

|

|style="background:#FFFF00"|transit

|4770

|1.15

|6158

|

Kepler-1622b

|

|0.131

|10.8118737

|

|

|style="background:#FFFF00"|transit

|3020

|1.31

|6436

|

Kepler-1623b

|

|0.117

|4.36128348

|

|

|style="background:#FFFF00"|transit

|3220

|1

|5772

|

Kepler-1624b

|

|0.509

|3.29030452

|

|

|style="background:#FFFF00"|transit

|650

|0.5

|3636

|

Kepler-1625b

|

|0.541

|287.378949

|

|

|style="background:#FFFF00"|transit

|3960

|0.96

|5677

|

Kepler-1626b

|

|0.18

|4.13962966

|

|

|style="background:#FFFF00"|transit

|5600

|1.51

|6826

|

Kepler-1627b

|

|0.329

|7.20283653

|

|

|style="background:#FFFF00"|transit

|1010

|0.87

|5445

| Young (38 million years) host star{{citation|arxiv=2112.14776|year=2022|title=A 38 Million Year Old Neptune-sized Planet in the Kepler Field|last1=Bouma|first1=L. G.|last2=Curtis|first2=J. L.|last3=Masuda|first3=K.|last4=Hillenbrand|first4=L. A.|last5=Stefansson|first5=G.|last6=Isaacson|first6=H.|last7=Narita|first7=N.|last8=Fukui|first8=A.|last9=Ikoma|first9=M.|last10=Tamura|first10=M.|last11=Kraus|first11=A. L.|last12=Furlan|first12=E.|last13=Gnilka|first13=C. L.|last14=Lester|first14=K. V.|last15=Howell|first15=S. B.|journal=The Astronomical Journal|volume=163|issue=3|page=121|doi=10.3847/1538-3881/ac4966|bibcode=2022AJ....163..121B|s2cid=245634940 |doi-access=free }}

Kepler-1628b

|

|0.574

|76.378033

|

|

|style="background:#FFFF00"|transit

|1150

|0.55

|3724

|

Kepler-1629b

|

|0.069

|3.87595807

|

|

|style="background:#FFFF00"|transit

|1300

|1.01

|5776

|

Kepler-1630b

|

|0.195

|509.997402

|

|

|style="background:#FFFF00"|transit

|910

|0.66

|4736

|

Kepler-1631b

|

|0.12

|4.09513932

|

|

|style="background:#FFFF00"|transit

|3900

|0.97

|5679

|

Kepler-1632b

|

|0.22

|448.303558

|

|

|style="background:#FFFF00"|transit

|1900

|1.12

|6137

|

Kepler-1633b

|

|0.141

|186.404271

|

|

|style="background:#FFFF00"|transit

|2650

|1.2

|6256

|

Kepler-1634b

|

|0.285

|374.876239

|

|

|style="background:#FFFF00"|transit

|2130

|0.92

|5474

|

Kepler-1635b

|

|0.325

|469.63111

|

|

|style="background:#FFFF00"|transit

|3540

|0.89

|5347

|

Kepler-1636b

|

|0.288

|425.47785

|

|

|style="background:#FFFF00"|transit

|5110

|1.01

|5797

|

Kepler-1637b

|

|0.079

|6.10960324

|

|

|style="background:#FFFF00"|transit

|1650

|1.02

|5789

|

Kepler-1638b

|

|0.167

|259.33683

|

|

|style="background:#FFFF00"|transit

|2870

|0.97

|5710

| Potentially habitable exoplanet{{Cite web|title=The Habitable Exoplanets Catalog - Planetary Habitability Laboratory @ UPR Arecibo|url=http://phl.upr.edu/projects/habitable-exoplanets-catalog|access-date=2021-01-21|website=phl.upr.edu}}

Kepler-1639b

|

|0.23

|9.878482

|

|

|style="background:#FFFF00"|transit

|3810

|1.12

|6150

|

Kepler-1640b

|

|0.43

|7.5844126

|

|

|style="background:#FFFF00"|transit

|4500

|1.27

|6324

|

Kepler-1641b

|

|0.277

|19.672266

|

|

|style="background:#FFFF00"|transit

|3130

|1.12

|6152

|

Kepler-1641c

|

|0.263

|32.657212

|

|

|style="background:#FFFF00"|transit

|3130

|1.12

|6152

|

Kepler-1642b

|

|0.285

|12.2057513

|

|

|style="background:#FFFF00"|transit

|1460

|0.88

|5355

|

Kepler-1642c

|

|0.237

|6.6513802

|

|

|style="background:#FFFF00"|transit

|1460

|0.88

|5355

|

Kepler-1643b

|

|0.205

|5.34264507

|

|

|style="background:#FFFF00"|transit

|1350

|0.92

|5508

| Young host star{{citation|arxiv=2205.01112|year=2022|title=Kepler and the Behemoth: Three Mini-Neptunes in a 40 Million Year Old Association|last1=Bouma |first1=L. G. |last2=Kerr |first2=R. |last3=Curtis |first3=J. L. |last4=Isaacson |first4=H. |last5=Hillenbrand |first5=L. A. |last6=Howard |first6=A. W. |last7=Kraus |first7=A. L. |last8=Bieryla |first8=A. |last9=Latham |first9=D. W. |last10=A Petigura |first10=E. |last11=Huber |first11=D. |journal=The Astronomical Journal |volume=164 |issue=5 |page=215 |doi=10.3847/1538-3881/ac93ff |bibcode=2022AJ....164..215B |doi-access=free }}

Kepler-1644b

|

|0.168

|21.0907758

|

|

|style="background:#FFFF00"|transit

|1930

|0.89

|5499

|

Kepler-1645b

|

|0.159

|16.1779561

|

|

|style="background:#FFFF00"|transit

|2750

|1.02

|5812

|

Kepler-1646b

|

|0.11

|4.48558383

|

|

|style="background:#FFFF00"|transit

|260

|0.24

|3299

|

Kepler-1647b

|1.51968

|1.059

|1107.5923

|2.7205

|

|style="background:#FFFF00"|transit

|

|1.22

|6210

|

OGLE-2007-BLG-349(AB)c

|0.25171

|

|2557

|2.59

|

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

|9000

|0.41

|

|{{Cite journal|last1=Bennett|first1=D. P.|last2=Rhie|first2=S. H.|last3=Udalski|first3=A.|last4=Gould|first4=A.|last5=Tsapras|first5=Y.|last6=Kubas|first6=D.|last7=Bond|first7=I. A.|last8=Greenhill|first8=J.|last9=Cassan|first9=A.|title=The First Circumbinary Planet Found by Microlensing: OGLE-2007-BLG-349L(AB)c|date=September 21, 2016|journal=The Astronomical Journal|volume=152|issue=5|page=125|doi=10.3847/0004-6256/152/5/125|arxiv=1609.06720|bibcode = 2016AJ....152..125B |s2cid=54034608 |doi-access=free }}

OGLE-2012-BLG-0724Lb

|0.47

|

|

|1.6

|

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

|22000

|0.29

|

|{{citation|arxiv=1604.05463|year=2016|title=OGLE-2012-BLG-0724Lb: A Saturn-mass Planet around an M-dwarf|bibcode=2016ApJ...824..139H|last1=Hirao|first1=Y.|last2=Udalski|first2=A.|last3=Sumi|first3=T.|last4=Bennett|first4=D. P.|last5=Bond|first5=I. A.|last6=Rattenbury|first6=N.|last7=Suzuki|first7=D.|last8=Koshimoto|first8=N.|last9=Abe|first9=F.|last10=Asakura|first10=Y.|last11=Bhattacharya|first11=A.|last12=Freeman|first12=M.|last13=Fukui|first13=A.|last14=Itow|first14=Y.|last15=Li|first15=M. C. A.|last16=Ling|first16=C. H.|last17=Masuda|first17=K.|last18=Matsubara|first18=Y.|last19=Matsuo|first19=T.|last20=Muraki|first20=Y.|last21=Nagakane|first21=M.|last22=Ohnishi|first22=K.|last23=Oyokawa|first23=H.|last24=Saito|first24=To.|last25=Sharan|first25=A.|last26=Shibai|first26=H.|last27=Sullivan|first27=D. J.|last28=Tristram|first28=P. J.|last29=Yonehara|first29=A.|author30=MOA Collaboration|journal=The Astrophysical Journal|volume=824|issue=2|page=139|doi=10.3847/0004-637X/824/2/139|s2cid=118656631|display-authors=1 |doi-access=free }}

OGLE-2014-BLG-0676Lb

|3.09

|

|

|4.4

|

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

|7200

|0.62

|

|{{citation|arxiv=1612.03511|year=2016|title=Faint source star planetary microlensing: the discovery of the cold gas giant planet OGLE-2014-BLG-0676Lb|bibcode=2017MNRAS.466.2710R|last1=Rattenbury|first1=N. J.|last2=Bennett|first2=D. P.|last3=Sumi|first3=T.|last4=Koshimoto|first4=N.|last5=Bond|first5=I. A.|last6=Udalski|first6=A.|last7=Shvartzvald|first7=Y.|last8=Maoz|first8=D.|last9=Jørgensen|first9=U. G.|last10=Dominik|first10=M.|last11=Street|first11=R. A.|last12=Tsapras|first12=Y.|last13=Abe|first13=F.|last14=Asakura|first14=Y.|last15=Barry|first15=R.|last16=Bhattacharya|first16=A.|last17=Donachie|first17=M.|last18=Evans|first18=P.|last19=Freeman|first19=M.|last20=Fukui|first20=A.|last21=Hirao|first21=Y.|last22=Itow|first22=Y.|last23=Li|first23=M. C. A.|last24=Ling|first24=C. H.|last25=Masuda|first25=K.|last26=Matsubara|first26=Y.|last27=Muraki|first27=Y.|last28=Nagakane|first28=M.|last29=Ohnishi|first29=K.|last30=Oyokawa|first30=H.|journal=Monthly Notices of the Royal Astronomical Society|volume=466|issue=3|page=2710|doi=10.1093/mnras/stw3185|doi-access=free |display-authors=1}}

{{ill|OGLE-2015-BLG-0051Lb|id|OGLE-2015-BLG-0051Lb}}

|0.72

|

|

|0.73

|

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

|27000

|0.1

|

|{{citation|arxiv=1606.09352|year=2021|title=Ogle-2015-BLG-0051/KMT-2015-BLG-0048Lb: A Giant Planet Orbiting a Low-Mass Bulge Star Discovered by High-Cadence Microlensing Surveys|doi=10.3847/0004-6256/152/4/95|last1=Han|first1=C.|last2=Udalski|first2=A.|last3=Gould|first3=A.|last4=Bozza|first4=V.|last5=Jung|first5=Y. K.|last6=Albrow|first6=M. D.|last7=Kim|first7=S.-L.|last8=Lee|first8=C.-U.|last9=Cha|first9=S.-M.|last10=Kim|first10=D.-J.|last11=Lee|first11=Y.|last12=Park|first12=B.-G.|last13=Shin|first13=I.-G.|last14=Szymański|first14=M. K.|last15=Soszyński|first15=I.|last16=Skowron|first16=J.|last17=Mróz|first17=P.|last18=Poleski|first18=R.|last19=Pietrukowicz|first19=P.|last20=Kozłowski|first20=S.|last21=Ulaczyk|first21=K.|last22=Wyrzykowski|first22=Ł.|last23=Pawlak|first23=M.|journal=The Astronomical Journal|volume=152|issue=4|page=95|s2cid=119105208 |doi-access=free }}

OGLE-2015-BLG-0954Lb

|3.9

|

|

|1.2

|

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

|2000

|0.33

|

|{{citation|arxiv=1603.00020|year=2016|title=A Super-Jupiter Microlens Planet Characterized by High-Cadence KMTNet Microlensing Survey Observations of OGLE-2015-BLG-0954|bibcode=2016JKAS...49...73S|last1=Shin|first1=I. -G|last2=Ryu|first2=Y. -H.|last3=Udalski|first3=A.|last4=Albrow|first4=M.|last5=Cha|first5=S. -M.|last6=Choi|first6=J. -Y.|last7=Chung|first7=S. -J.|last8=Han|first8=C.|last9=Hwang|first9=K. -H.|last10=Jung|first10=Y. K.|last11=Kim|first11=D. -J.|last12=Kim|first12=S. -L.|last13=Lee|first13=C. -U.|last14=Lee|first14=Y.|last15=Park|first15=B. -G.|last16=Park|first16=H.|last17=Pogge|first17=R. W.|last18=Yee|first18=J. C.|last19=Pietrukowicz|first19=P.|last20=Mroz|first20=P.|last21=Kozlowski|first21=S.|last22=Poleski|first22=R.|last23=Skowron|first23=J.|last24=Soszynski|first24=I.|last25=Szymanski|first25=M. K.|last26=Ulaczyk|first26=K.|last27=Wyrzykowski|first27=L.|last28=Pawlak|first28=M.|last29=Gould|first29=A.|journal=Journal of the Korean Astronomical Society|volume=49|issue=3|page=73|doi=10.5303/JKAS.2016.49.3.73}}

OGLE-2012-BLG-0950Lb

|0.11012

|

|

|2.7

|

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

|9800

|0.56

|

|{{citation|arxiv=1607.03267|year=2016|title=OGLE-2012-BLG-0950Lb: The First Planet Mass Measurement from Only Microlens Parallax and Lens Flux|bibcode=2017AJ....153....1K|last1=Koshimoto|first1=N.|last2=Udalski|first2=A.|last3=Beaulieu|first3=J. P.|last4=Sumi|first4=T.|last5=Bennett|first5=D. P.|last6=Bond|first6=I. A.|last7=Rattenbury|first7=N.|last8=Fukui|first8=A.|last9=Batista|first9=V.|last10=Marquette|first10=J. B.|last11=Brillant|first11=S.|author12=and|last13=Abe|first13=F.|last14=Asakura|first14=Y.|last15=Bhattacharya|first15=A.|last16=Donachie|first16=M.|last17=Freeman|first17=M.|last18=Hirao|first18=Y.|last19=Itow|first19=Y.|last20=Li|first20=M. C. A.|last21=Ling|first21=C. H.|last22=Masuda|first22=K.|last23=Matsubara|first23=Y.|last24=Matsuo|first24=T.|last25=Muraki|first25=Y.|last26=Nagakane|first26=M.|last27=Ohnishi|first27=K.|last28=Oyokawa|first28=H.|last29=Saito|first29=To.|last30=Sharan|first30=A.|journal=The Astronomical Journal|volume=153|issue=1|page=1|doi=10.3847/1538-3881/153/1/1|s2cid=119309343|display-authors=1 |doi-access=free }}

{{ill|OGLE-2014-BLG-1760Lb|id|OGLE-2014-BLG-1760Lb}}

|0.56

|

|

|1.75

|

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

|22400

|0.51

|

|{{citation|arxiv=1603.05677|year=2016|title=Discovery of a Gas giant Planet in Microlensing Event OGLE-2014-BLG-1760|bibcode=2016AJ....152..140B|last1=Bhattacharya|first1=A.|last2=Bennett|first2=D. P.|last3=Bond|first3=I. A.|last4=Sumi|first4=T.|last5=Udalski|first5=A.|last6=Street|first6=R.|last7=Tsapras|first7=Y.|last8=Abe|first8=F.|last9=Freeman|first9=M.|last10=Fukui|first10=A.|last11=Hirao|first11=Y.|last12=Itow|first12=Y.|last13=Koshimoto|first13=N.|last14=Li|first14=M. C. A.|last15=Ling|first15=C. H.|last16=Masuda|first16=K.|last17=Matsubara|first17=Y.|last18=Muraki|first18=Y.|last19=Nagakane|first19=M.|last20=Ohnishi|first20=K.|last21=Rattenbury|first21=N.|last22=Saito|first22=T.|last23=Sharan|first23=A.|last24=Sullivan|first24=D. J.|last25=Suzuki|first25=D.|last26=Tristram|first26=P. J.|author27=MOA Collaboration|last28=Skowron|first28=J.|last29=Szymański|first29=M. K.|last30=Soszyński|first30=I.|journal=The Astronomical Journal|volume=152|issue=5|page=140|doi=10.3847/0004-6256/152/5/140|s2cid=73590811|display-authors=1 |doi-access=free }}

Pr0211 c

|7.79

|

|4850

|5.5

|

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

|

|0.94

|5300

|Host star belongs to Beehive Cluster[http://www.aanda.org/articles/aa/abs/2016/04/aa27933-15/aa27933-15.html The GAPS programme with HARPS-N at TNG XI. Pr 0211 in M 44: the first multi-planet system in an open cluster]

Proxima Centauri b

|0.004

|

|11.186

|0.0485

|

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

|4.2

|0.12

|3050

|Nearest exoplanet to the Solar System, and is potentially habitable{{cite journal|bibcode=2016Natur.536..437A|title = A terrestrial planet candidate in a temperate orbit around Proxima Centauri

| journal = Nature| volume= 536| issue = 7617| pages = 437–440| last1= Anglada-Escudé|first1 = Guillem| last2=Amado|first2 = Pedro J.| last3= Barnes| first3= John| year= 2016| arxiv=1609.03449|doi = 10.1038/nature19106| pmid = 27558064| s2cid = 4451513| url=http://www.eso.org/public/archives/releases/sciencepapers/eso1629/eso1629a.pdf}}

Qatar-3b

|4.31

|1.096

|2.5079204

|0.03783

|1681

|style="background:#FFFF00"|transit

|

|1.15

|6007

|{{Cite journal|last1=Alsubai|first1=Khalid|last2=Mislis|first2=Dimitris|last3=Tsvetanov|first3=Zlatan I.|last4=Latham|first4=David W.|last5=Bieryla|first5=Allyson|last6=Buchhave|first6=Lars A.|last7=Esquerdo|first7=Gilbert A.|last8=Bramich|first8=D. M.|last9=Pyrzas|first9=Stylianos|last10=Vilchez|first10=Nicolas P. E.|last11=Mancini|first11=Luigi|date=2017-04-01|title=Qatar Exoplanet Survey : Qatar-3b, Qatar-4b, and Qatar-5b|journal=The Astronomical Journal|volume=153|issue=4|pages=200|doi=10.3847/1538-3881/aa6340|arxiv=1606.06882|bibcode=2017AJ....153..200A|s2cid=119214858|issn=0004-6256 |doi-access=free }}

Qatar-4b

|6.10

|1.135

|1.8053564

|0.02803

|1385

|style="background:#FFFF00"|transit

|

|0.90

|5215

|

Qatar-5b

|4.32

|1.107

|2.8792319

|0.04127

|1415

|style="background:#FFFF00"|transit

|

|1.13

|5747

|

Rho Coronae Borealis c

|0.07866

|

|102.54

|0.4123

|448

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

|56.2

|0.89

|5627

|{{cite journal |last1=Fulton |first1=Benjamin J. |display-authors=etal |title=Three Temperate Neptunes Orbiting Nearby Stars |journal=The Astrophysical Journal |date=October 2016 |volume=830 |issue=1 |pages=46 |doi=10.3847/0004-637X/830/1/46 |arxiv=1607.00007 |bibcode=2016ApJ...830...46F |s2cid=36666883 |doi-access=free }}

TRAPPIST-1b

|0.00267

|0.097

|1.51087081

|0.01111

|400

|style="background:#FFFF00"|transit

|39

|0.08

|2559

|{{cite journal |title=Temperate Earth-sized planets transiting a nearby ultracool dwarf star |journal=Nature |volume=533 |issue=7602 |pages=221–224 |year=2016 |url=http://www.eso.org/public/archives/releases/sciencepapers/eso1615/eso1615a.pdf |doi=10.1038/nature17448 |last1=Gillon |first1=M. |last2=Jehin |first2=E. |last3=Lederer |first3=S. M. |last4=Delrez |first4=L. |last5=De Wit |first5=J. |last6=Burdanov |first6=A. |last7=Van Grootel |first7=V. |last8=Burgasser |first8=Adam J. |last9=Triaud |first9=A. H. M. J. |last10=Opitom |first10=C. |last11=Demory |first11=B.-O. |last12=Sahu |first12=D. K. |last13=Bardalez Gagliuffi |first13=D. |last14=Magain |first14=P. |last15=Queloz |first15=D. |bibcode=2016Natur.533..221G |pmid=27135924 |pmc=5321506 |arxiv=1605.07211}}

TRAPPIST-1c

|0.00434

|0.094

|2.4218233

|0.01521

|342

|style="background:#FFFF00"|transit

|39

|0.08

|2559

|

TRAPPIST-1d

|0.00129

|0.069

|4.04961

|0.02144

|288

|style="background:#FFFF00"|transit

|39

|0.08

|2559

|Potentially habitable exoplanet

TYC 3667-1280-1 b

|5.4

|

|26.468

|0.21

|1350

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

|1570

|1.87

|5130

|Red giant star host[https://www.aanda.org/articles/aa/abs/2016/05/aa28417-16/aa28417-16.html Tracking Advanced Planetary Systems (TAPAS) with HARPS-N⋆,⋆⋆ IV. TYC 3667-1280-1: The most massive red giant star hosting a warm Jupiter]

V830 Tauri b

|0.7

|

|4.927

|0.057

|

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

|490

|1

|4250

|{{cite journal|title=A hot Jupiter orbiting a 2-million-year-old solar-mass T Tauri star|author=J.-F. Donati|display-authors=etal|journal=Nature|date=20 June 2016|doi=10.1038/nature18305|pmid = 27324847|volume=534|issue=7609|pages=662–666|arxiv = 1606.06236 |bibcode = 2016Natur.534..662D |s2cid=1046761}}

WASP-53b

|2.132

|1.074

|3.3098443

|0.04101

|

|style="background:#FFFF00"|transit

|

|0.84

|4953

|

WASP-53c

|16.35

|

|2840

|3.73

|

|style="background:#FFFF00"|transit

|

|0.84

|4953

|{{citation|arxiv=1612.04166|year=2016|title=Peculiar architectures for the WASP-53 and WASP-81 planet-hosting systems|doi=10.1093/mnras/stx154 |last1=Triaud |first1=Amaury H. M. J. |last2=Neveu-Vanmalle |first2=Marion |last3=Lendl |first3=Monika |last4=Anderson |first4=David R. |last5=Collier Cameron |first5=Andrew |last6=Delrez |first6=Laetitia |last7=Doyle |first7=Amanda |last8=Gillon |first8=Michaël |last9=Hellier |first9=Coel |last10=Jehin |first10=Emmanuël |last11=Maxted |first11=Pierre F. L. |last12=Ségransan |first12=Damien |last13=Smalley |first13=Barry |last14=Queloz |first14=Didier |last15=Pollacco |first15=Don |last16=Southworth |first16=John |last17=Tregloan-Reed |first17=Jeremy |last18=Udry |first18=Stéphane |last19=West |first19=Richard |journal=Monthly Notices of the Royal Astronomical Society |pages=stx154 |doi-access=free }}

WASP-81b

|0.729

|1.429

|2.7164762

|0.03908

|

|style="background:#FFFF00"|transit

|

|1.08

|5870

|

WASP-92b

|0.805

|1.461

|2.1746742

|0.0348

|1871

|style="background:#FFFF00"|transit

|1700

|1.19

|6280

|

WASP-93b

|1.47

|1.597

|2.7325321

|0.04211

|

|style="background:#FFFF00"|transit

|820

|1.33

|6700

|

WASP-113b

|0.475

|1.409

|4.54216875

|0.05885

|1496

|style="background:#FFFF00"|transit

|1200

|1.32

|5890

|{{citation|arxiv=1607.02341|year=2016|title=WASP-113b and WASP-114b, two inflated hot Jupiters with contrasting densities|doi=10.1051/0004-6361/201526517|last1=Barros|first1=S. C. C.|last2=Brown|first2=D. J. A.|last3=Hébrard|first3=G.|last4=Gómez Maqueo Chew|first4=Y.|last5=Anderson|first5=D. R.|last6=Boumis|first6=P.|last7=Delrez|first7=L.|last8=Hay|first8=K. L.|last9=Lam|first9=K. W. F.|last10=Llama|first10=J.|last11=Lendl|first11=M.|last12=McCormac|first12=J.|last13=Skiff|first13=B.|last14=Smalley|first14=B.|last15=Turner|first15=O.|last16=Vanhuysse|first16=M.|last17=Armstrong|first17=D. J.|last18=Boisse|first18=I.|last19=Bouchy|first19=F.|last20=Collier Cameron|first20=A.|last21=Faedi|first21=F.|last22=Gillon|first22=M.|last23=Hellier|first23=C.|last24=Jehin|first24=E.|last25=Liakos|first25=A.|last26=Meaburn|first26=J.|last27=Osborn|first27=H. P.|last28=Pepe|first28=F.|last29=Plauchu-Frayn|first29=I.|last30=Pollacco|first30=D.|journal=Astronomy & Astrophysics|volume=593|pages=A113|bibcode=2016A&A...593A.113B|s2cid=5994445|display-authors=1}}

WASP-114b

|1.769

|1.339

|1.5487743

|0.02851

|2043

|style="background:#FFFF00"|transit

|1500

|1.29

|5940

|

WASP-118b

|0.514

|1.44

|4.0460435

|0.05453

|

|style="background:#FFFF00"|transit

|820

|1.32

|6410

|{{citation|arxiv=1607.00774|year=2016|title=WASP-92b, WASP-93b and WASP-118b: Three new transiting close-in giant planets|doi=10.1093/mnras/stw2090|last1=Hay|first1=K. L.|last2=Collier-Cameron|first2=A.|last3=Doyle|first3=A. P.|last4=Hébrard|first4=G.|last5=Skillen|first5=I.|last6=Anderson|first6=D. R.|last7=Barros|first7=S. C. C.|last8=Brown|first8=D. J. A.|last9=Bouchy|first9=F.|last10=Busuttil|first10=R.|last11=Delorme|first11=P.|last12=Delrez|first12=L.|last13=Demangeon|first13=O.|last14=Díaz|first14=R. F.|last15=Gillon|first15=M.|last16=Gómez Maqueo Chew|first16=Y.|last17=Gonzàlez|first17=E.|last18=Hellier|first18=C.|last19=Holmes|first19=S.|last20=Jarvis|first20=J. F.|last21=Jehin|first21=E.|last22=Joshi|first22=Y. C.|last23=Kolb|first23=U.|last24=Lendl|first24=M.|last25=Maxted|first25=P. F. L.|last26=McCormac|first26=J.|last27=Miller|first27=G. R. M.|last28=Mortier|first28=A.|last29=Pallé|first29=E.|last30=Pollacco|first30=D.|journal=Monthly Notices of the Royal Astronomical Society|volume=463|issue=3|pages=3276–3289|doi-access=free |display-authors=1}}

WASP-119b

|1.23

|1.4

|2.49979

|0.0363

|1600

|style="background:#FFFF00"|transit

|1090

|1.02

|5650

|{{citation|arxiv=1602.01740|year=2016|title=Five transiting hot Jupiters discovered using WASP-South, Euler, and TRAPPIST: WASP-119 b, WASP-124 b, WASP-126 b, WASP-129 b, and WASP-133 b|doi=10.1051/0004-6361/201628250|last1=Maxted|first1=P. F. L.|last2=Anderson|first2=D. R.|last3=Collier Cameron|first3=A.|last4=Delrez|first4=L.|last5=Gillon|first5=M.|last6=Hellier|first6=C.|last7=Jehin|first7=E.|last8=Lendl|first8=M.|last9=Neveu-Vanmalle|first9=M.|last10=Pepe|first10=F.|last11=Pollacco|first11=D.|last12=Queloz|first12=D.|last13=Ségransan|first13=D.|last14=Smalley|first14=B.|last15=Smith|first15=A. M. S.|last16=Southworth|first16=J.|last17=Triaud|first17=A. H. M. J.|last18=Udry|first18=S.|last19=Wagg|first19=T.|last20=West|first20=R. G.|journal=Astronomy & Astrophysics|volume=591|pages=A55|bibcode=2016A&A...591A..55M|s2cid=53612762}}

WASP-124b

|0.6

|1.24

|3.37265

|0.0449

|1400

|style="background:#FFFF00"|transit

|1410

|1.07

|6050

|

WASP-126b

|0.28

|0.96

|3.2888

|0.0449

|1480

|style="background:#FFFF00"|transit

|760

|1.12

|5800

|

WASP-127b

|0.18

|1.37

|4.178062

|0.052

|

|style="background:#FFFF00"|transit

|330

|1.08

|5620

|{{citation|arxiv=2010.15143|title=WASP-127b: A misaligned planet with a partly cloudy atmosphere and tenuous sodium signature seen by ESPRESSO|year=2020|last1=Allart|first1=R.|last2=Pino|first2=L.|last3=Lovis|first3=C.|last4=Sousa|first4=S. G.|last5=Casasayas-Barris|first5=N.|last6=Zapatero Osorio|first6=M. R.|last7=Cretignier|first7=M.|last8=Palle|first8=E.|last9=Pepe|first9=F.|last10=Cristiani|first10=S.|last11=Rebolo|first11=R.|last12=Santos|first12=N. C.|last13=Borsa|first13=F.|last14=Bourrier|first14=V.|last15=Demangeon|first15=O. D. S.|last16=Ehrenreich|first16=D.|last17=Lavie|first17=B.|last18=Lillo-Box|first18=J.|last19=Micela|first19=G.|last20=Oshagh|first20=M.|last21=Sozzetti|first21=A.|last22=Tabernero|first22=H.|last23=Adibekyan|first23=V.|last24=Allende Prieto|first24=C.|last25=Alibert|first25=Y.|last26=Amate|first26=M.|last27=Benz|first27=W.|last28=Bouchy|first28=F.|last29=Cabral|first29=A.|last30=Dekker|first30=H.|journal=Astronomy & Astrophysics|volume=644|pages=A155|doi=10.1051/0004-6361/202039234|bibcode=2020A&A...644A.155A|s2cid=225103317|display-authors=29}}{{cite journal|arxiv=2005.09615|last1=Skaf|first1=Nour|author2=Michelle Fabienne Bieger|last3=Edwards|first3=Billy|last4=Changeat|first4=Quentin|last5=Morvan|first5=Mario|last6=Kiefer|first6=Flavien|last7=Blain|first7=Doriann|last8=Zingales|first8=Tiziano|last9=Poveda|first9=Mathilde|last10=Al-Refaie|first10=Ahmed|last11=Baeyens|first11=Robin|last12=Gressier|first12=Amelie|last13=Guilluy|first13=Gloria|author14=Adam Yassin Jaziri|last15=Modirrousta-Galian|first15=Darius|last16=Mugnai|first16=Lorenzo V.|last17=Pluriel|first17=William|last18=Whiteford|first18=Niall|last19=Wright|first19=Sam|author20=Kai Hou Yip|last21=Charnay|first21=Benjamin|last22=Leconte|first22=Jeremy|last23=Drossart|first23=Pierre|last24=Tsiaras|first24=Angelos|last25=Venot|first25=Olivia|last26=Waldmann|first26=Ingo|last27=Beaulieu|first27=Jean-Philippe|title=ARES II: Characterising the Hot Jupiters WASP-127 b, WASP-79 b and WASP-62 b with HST|year=2020|doi=10.3847/1538-3881/ab94a3|s2cid=218684714|journal=The Astronomical Journal |doi-access=free }}{{Cite journal |arxiv = 1607.07859|bibcode = 2017A&A...599A...3L|title = From dense hot Jupiter to low-density Neptune: The discovery of WASP-127b, WASP-136b, and WASP-138b|journal = Astronomy and Astrophysics|volume = 599|issue = 3|pages = A3|last1 = Lam|first1 = K. W. F|last2 = Faedi|first2 = F|last3 = Brown|first3 = D. J. A|last4 = Anderson|first4 = D. R|last5 = Delrez|first5 = L|last6 = Gillon|first6 = M|last7 = Hébrard|first7 = G|last8 = Lendl|first8 = M|last9 = Mancini|first9 = L|last10 = Southworth|first10 = J|last11 = Smalley|first11 = B|last12 = Triaud|first12 = A. H. M|last13 = Turner|first13 = O. D|last14 = Hay|first14 = K. L|last15 = Armstrong|first15 = D. J|last16 = Barros|first16 = S. C. C|last17 = Bonomo|first17 = A. S|last18 = Bouchy|first18 = F|last19 = Boumis|first19 = P|last20 = Collier Cameron|first20 = A|last21 = Doyle|first21 = A. P|last22 = Hellier|first22 = C|last23 = Henning|first23 = T|last24 = Jehin|first24 = E|last25 = King|first25 = G|last26 = Kirk|first26 = J|last27 = Louden|first27 = T|last28 = Maxted|first28 = P. F. L|last29 = McCormac|first29 = J. J|last30 = Osborn|first30 = H. P|display-authors = 29|year = 2017|doi = 10.1051/0004-6361/201629403|s2cid = 5953163}}

WASP-129b

|1

|0.93

|5.748145

|0.0628

|1100

|style="background:#FFFF00"|transit

|800

|1

|5900

|

WASP-130b

|1.23

|0.89

|11.55098

|0.1012

|833

|style="background:#FFFF00"|transit

|590

|1.04

|5625

|{{citation|arxiv=1604.04195|year=2016|title=WASP-South transiting exoplanets: WASP-130b, WASP-131b, WASP-132b, WASP-139b, WASP-140b, WASP-141b and WASP-142b|doi=10.1093/mnras/stw3005|last1=Hellier|first1=C.|last2=Anderson|first2=D. R.|last3=Cameron|first3=A. Collier|last4=Delrez|first4=L.|last5=Gillon|first5=M.|last6=Jehin|first6=E.|last7=Lendl|first7=M.|last8=Maxted|first8=P. F. L.|last9=Neveu-Vanmalle|first9=M.|last10=Pepe|first10=F.|last11=Pollacco|first11=D.|last12=Queloz|first12=D.|last13=Ségransan|first13=D.|last14=Smalley|first14=B.|last15=Southworth|first15=J.|last16=Triaud|first16=A. H. M. J.|last17=Udry|first17=S.|last18=Wagg|first18=T.|last19=West|first19=R. G.|journal=Monthly Notices of the Royal Astronomical Society|volume=465|issue=3|pages=3693–3707|doi-access=free }}

WASP-131b

|0.27

|1.22

|5.322023

|0.0607

|1400

|style="background:#FFFF00"|transit

|820

|1.06

|6030

|

WASP-132b

|0.41

|0.87

|7.133521

|0.067

|763

|style="background:#FFFF00"|transit

|390

|0.8

|4775

| Second planet discovered in 2022{{citation|arxiv=2205.02501|year=2022|title=The Discovery of a Planetary Companion Interior to Hot Jupiter WASP-132 B|doi=10.3847/1538-3881/ac6f57 |last1=Hord |first1=Benjamin J. |last2=Colón |first2=Knicole D. |last3=Berger |first3=Travis A. |last4=Kostov |first4=Veselin |last5=Silverstein |first5=Michele L. |last6=Stassun |first6=Keivan G. |last7=Lissauer |first7=Jack J. |last8=Collins |first8=Karen A. |last9=Schwarz |first9=Richard P. |last10=Sefako |first10=Ramotholo |last11=Ziegler |first11=Carl |last12=Briceño |first12=César |last13=Law |first13=Nicholas |last14=Mann |first14=Andrew W. |last15=Ricker |first15=George R. |last16=Latham |first16=David W. |last17=Seager |first17=S. |last18=Winn |first18=Joshua N. |last19=Jenkins |first19=Jon M. |last20=Bouma |first20=Luke G. |last21=Falk |first21=Ben |last22=Torres |first22=Guillermo |last23=Twicken |first23=Joseph D. |last24=Vanderburg |first24=Andrew |journal=The Astronomical Journal |volume=164 |issue=1 |page=13 |bibcode=2022AJ....164...13H |s2cid=248524687 |doi-access=free }}

WASP-133b

|1.16

|1.21

|2.176423

|0.0345

|1790

|style="background:#FFFF00"|transit

|1780

|1.16

|5700

|

WASP-136b

|1.51

|1.38

|5.215357

|0.0661

|

|style="background:#FFFF00"|transit

|530

|1.41

|6260

|

WASP-138b

|1.22

|1.09

|3.634433

|0.0494

|

|style="background:#FFFF00"|transit

|1000

|1.22

|6272

|

WASP-139b

|0.117

|0.8

|5.924262

|0.062

|910

|style="background:#FFFF00"|transit

|750

|0.92

|5310

|

WASP-140b

|2.44

|1.44

|2.2359835

|0.0323

|1320

|style="background:#FFFF00"|transit

|590

|0.9

|5260

|{{citation|arxiv=2203.15059|year=2022|title=A New Analysis of Eight Spitzer Phase Curves and Hot Jupiter Population Trends: Qatar-1b, Qatar-2b, WASP-52b, WASP-34b, and WASP-140b|last1=May|first1=Erin|last2=Stevenson|first2=Kevin|last3=Bean|first3=Jacob|last4=Bell|first4=Taylor|last5=Cowan|first5=Nicolas|last6=Dang|first6=Lisa|last7=Desert|first7=Jean-Michel|last8=Fortney|first8=Jonathan|last9=Keating|first9=Dylan|last10=Kempton|first10=Eliza|last11=Komacek|first11=Thaddeus|last12=Lewis|first12=Nikole|last13=Mansfield|first13=Megan|last14=Morley|first14=Caroline|last15=Parmentier|first15=Vivien|last16=Rauscher|first16=Emily|last17=Swain|first17=Mark|last18=Zellem|first18=Robert|last19=Showman|first19=Adam|journal=The Astronomical Journal |volume=163 |issue=6 |page=256 |doi=10.3847/1538-3881/ac6261 |bibcode=2022AJ....163..256M |s2cid=247778438 |doi-access=free }}

WASP-141b

|2.69

|1.21

|3.310651

|0.0469

|1540

|style="background:#FFFF00"|transit

|1900

|1.25

|5900

|

WASP-142b

|0.84

|1.53

|2.052868

|0.0347

|2000

|style="background:#FFFF00"|transit

|2700

|1.33

|6010

|

WASP-157b

|0.574

|1.065

|3.9516205

|0.0529

|1339

|style="background:#FFFF00"|transit

|

|1.26

|5838

|{{citation|arxiv=1603.05638|year=2016|title=WASP-157b, a Transiting Hot Jupiter Observed with K2|bibcode=2016PASP..128l4403M|last1=Močnik|first1=T.|last2=Anderson|first2=D. R.|last3=Brown|first3=D. J. A.|last4=Collier Cameron|first4=A.|last5=Delrez|first5=L.|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=Ségransan|first15=D.|last16=Smalley|first16=B.|last17=Southworth|first17=J.|last18=Triaud|first18=A. H. M. J.|last19=Udry|first19=S.|last20=West|first20=R. G.|journal=Publications of the Astronomical Society of the Pacific|volume=128|issue=970|page=124403|doi=10.1088/1538-3873/128/970/124403|s2cid=55424751}}

XO-6b

|4.4

|2.07

|3.7650007

|0.0815

|1577

|style="background:#FFFF00"|transit

|759.0

|1.47

|6720

|{{Cite journal | last1=Crouzet|first1=N.| last2=McCullough| first2=P. R.| last3=Long| first3=D.| last4=Rodriguez| first4=P. Montanes| last5=Etangs| first5=A. Lecavelier des| last6=Ribas| first6=I.| last7=Bourrier| first7=V.| last8=Hébrard| first8=G.| last9=Vilardell| first9=F.| last10=Deleuil| first10=M.| last11=Herrero| first11=E.| date=2017-02-02| title=Discovery of XO-6b: A Hot Jupiter Transiting a Fast Rotating F5 Star on an Oblique Orbit| journal=The Astronomical Journal|language=en|volume=153|issue=3|pages=94|doi=10.3847/1538-3881/153/3/94|arxiv=1612.02776|bibcode=2017AJ....153...94C|hdl=2117/112256| s2cid=119082666| issn=1538-3881 |doi-access=free }}

YBP 401 b

|0.46

|

|4.087

|

|

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

|

|1.14

|6165

|Belongs to Messier 67{{citation|arxiv=1606.05247|year=2016|title=Search for giant planets in M67 III: excess of hot Jupiters in dense open clusters|bibcode=2016A&A...592L...1B|last1=Brucalassi|first1=A.|last2=Pasquini|first2=L.|last3=Saglia|first3=R.|last4=Ruiz|first4=M. T.|last5=Bonifacio|first5=P.|last6=Leão|first6=I.|last7=Canto Martins|first7=B. L.|last8=De Medeiros|first8=J. R.|last9=Bedin|first9=L. R.|last10=Biazzo|first10=K.|last11=Melo|first11=C.|last12=Lovis|first12=C.|last13=Randich|first13=S.|journal=Astronomy and Astrophysics|volume=592|doi=10.1051/0004-6361/201527561|s2cid=62806509}}

Excluded objects and former candidate

The majority of exoplanet discoveries in 2016 were from a paper by Morton et al. that statistically validated over 1,000 Kepler planets. This statistical validation did not involve mass measurements, and some transiting objects validated as planets were later shown (or even previously known) to be small stars. Such cases include Kepler-469 (KOI-126), Kepler-470 (KOI-129), Kepler-486 (KOI-189), Kepler-488 (KOI-194), Kepler-503 (KOI-242), Kepler-628 (KOI-631), Kepler-699 (KOI-846), Kepler-706 (KOI-855), Kepler-807 (KOI-1288), Kepler-840 (KOI-1416), and Kepler-854 (KOI-1450). In another two cases, Kepler-492 (KOI-205) and Kepler-494 (KOI-219), the companions are brown dwarfs with masses about 40 times that of Jupiter.

HD 131399 Ab had been thought to be a massive directly-imaged planet located in a trinary system. Later analysis showed that it is a background star instead.{{cite web |last1=Oransky |first1=Ivan |title=Triple sunrise, triple sunset: Science paper retracted when it turns out a planet is a star |url=https://retractionwatch.com/2022/04/14/triple-sunrise-triple-sunset-science-paper-retracted-when-it-turns-out-a-planet-is-a-star/#more-124683 |website=Retraction Watch |access-date=25 April 2022 |date=14 April 2022}}

Specific exoplanet lists

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

References

{{reflist|refs=

{{cite journal |last1=Carter |first1=Joshua A. |last2=Fabrycky |first2=Daniel C. |display-authors=etal |date=February 2011 |title=KOI-126: A Triply Eclipsing Hierarchical Triple with Two Low-Mass Stars |journal=Science |volume=331 |issue=6017 |pages=562– |doi=10.1126/science.1201274 |pmid=21224439 |arxiv=1102.0562 |bibcode=2011Sci...331..562C}}

{{cite journal |last1=Díaz |first1=R. F. |last2=Damiani |first2=C. |display-authors=etal |date=March 2013 |title=SOPHIE velocimetry of Kepler transit candidates. VIII. KOI-205 b: a brown-dwarf companion to a K-type dwarf |journal=Astronomy & Astrophysics |volume=551 |issue= |pages=L9 |doi=10.1051/0004-6361/201321124 |arxiv=1302.2628 |bibcode=2013A&A...551L...9D}}

{{cite journal |last1=Díaz |first1=R. F. |last2=Montagnier |first2=G. |display-authors=etal |date=December 2014 |title=SOPHIE velocimetry of Kepler transit candidates. XIII. KOI-189 b and KOI-686 b: two very low-mass stars in long-period orbits |journal=Astronomy & Astrophysics |volume=572 |issue= |pages=A109 |doi=10.1051/0004-6361/201424406 |arxiv=1410.5248 |bibcode=2014A&A...572A.109D}}

{{cite journal |last1=Santerne |first1=A. |last2=Moutou |first2=C. |display-authors=etal |date=March 2016 |title=SOPHIE velocimetry of Kepler transit candidates. XVII. The physical properties of giant exoplanets within 400 days of period |journal=Astronomy & Astrophysics |volume=587 |issue= |pages=A64 |doi=10.1051/0004-6361/201527329 |arxiv=1511.00643 |bibcode=2016A&A...587A..64S}}

{{cite journal |last1=Cañas |first1=Caleb I. |last2=Bender |first2=Chad F. |display-authors=etal |date=July 2018 |title=Kepler-503b: An Object at the Hydrogen Burning Mass Limit Orbiting a Subgiant Star |journal=The Astrophysical Journal Letters |volume=861 |issue=1 |pages=L4 |doi=10.3847/2041-8213/aacbc5 |doi-access=free |arxiv=1805.08820 |bibcode=2018ApJ...861L...4C}}

{{cite journal |last1=Niraula |first1=Prajwal |last2=Shporer |first2=Avi |display-authors=etal |date=April 2022 |title=Revisiting Kepler Transiting Systems: Unvetting Planets and Constraining Relationships among Harmonics in Phase Curves |journal=The Astronomical Journal |volume=163 |issue=4 |pages=172 |doi=10.3847/1538-3881/ac4f64 |doi-access=free |arxiv=2203.07312 |bibcode=2022AJ....163..172N}}

{{cite journal |last1=Cañas |first1=Caleb I. |last2=Bender |first2=Chad F. |display-authors=etal |date=April 2023 |title=Characterization of Low-mass Companions to Kepler Objects of Interest Observed with APOGEE-N |journal=The Astrophysical Journal Supplement Series |volume=265 |issue=2 |pages=50 |doi=10.3847/1538-4365/acbcbe |doi-access=free |arxiv=2302.07713 |bibcode=2023ApJS..265...50C}}

{{cite journal |last1=Li |first1=Canis |last2=Shporer |first2=Avi |date=May 2024 |title=A Search for Temporal Atmospheric Variability of Kepler Hot Jupiters |journal=The Astronomical Journal |volume=167 |issue=5 |pages=245 |doi=10.3847/1538-3881/ad3807 |doi-access=free |arxiv=2403.01295 |bibcode=2024AJ....167..245L}}

}}

{{Exoplanet}}

2016

*

exoplanets