List of exoplanets discovered in 2013

!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

|24.5

|

|

|52

|

|style="background:#FF6CDA"|imaging

|120

|0.4

|3530

|[https://iopscience.iop.org/article/10.1088/0004-637X/774/1/55/pdf PLANETS AROUND LOW-MASS STARS. III. A YOUNG DUSTY L DWARF COMPANION AT THE DEUTERIUM-BURNING LIMIT]

|1.11

|

|137.48

|0.539

|

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

|572.2

|1.1

|4796

|[https://iopscience.iop.org/article/10.1088/0004-637X/770/1/53/pdf BD+15 2940 AND HD 233604: TWO GIANTS WITH PLANETS CLOSE TO THE ENGULFMENT ZONE]

|0.27

|1.08

|4.86069

|0.0578

|

|style="background:#FFFF00"|transit

|3300

|1.09

|6040

|[https://www.aanda.org/articles/aa/pdf/2013/07/aa21462-13.pdf Transiting exoplanets from the CoRoT space mission XXIV. CoRoT-25b and CoRoT-26b: two low-density giant planets]

|0.52

|1.26

|4.20474

|0.0526

|

|style="background:#FFFF00"|transit

|5400

|1.09

|5590

|

|28.5

|

|246.36

|0.36

|

|style="background:#909090"|astrometry

|67.7

|0.07

|2150

|{{citation |arxiv=1306.3225 |year=2013 |title=Astrometric orbit of a low-mass companion to an ultracool dwarf |doi=10.1051/0004-6361/201321871 |last1=Sahlmann |first1=J. |last2=Lazorenko |first2=P. F. |last3=Ségransan|first3=D. |last4=Martín |first4=Eduardo L. |last5=Queloz |first5=D. |last6=Mayor |first6=M. |last7=Udry |first7=S. |journal=Astronomy & Astrophysics |volume=556 |pages=A133 |bibcode=2013A&A...556A.133S |s2cid=119193690 }}

|0.03335

|

|8.63182

|0.0607

|

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

|48.8

|0.4

|3500

|{{Cite journal |arxiv = 1306.1717|doi = 10.1051/0004-6361/201321174|title = Up to four planets around the M dwarf GJ 163|journal = Astronomy & Astrophysics|volume = 556|pages = A111|year = 2013|last1 = Tuomi|first1 = M.|last2 = Anglada-Escudé|first2 = G.|s2cid = 16214668}}

|0.0214

|

|25.63058

|0.1254

|

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

|48.8

|0.4

|3500

|

|0.0925

|

|603.95116

|1.0304

|

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

|48.8

|0.4

|3500

|

|0.027

|

|3.8728

|0.0428

|

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

|66

|0.7

|4324

|{{citation|arxiv=1305.2203|year=2013|title=Two planetary companions around the K7 dwarf GJ 221 : a hot super-Earth and a candidate in the sub-Saturn desert range|doi=10.1088/0004-637X/771/1/42|last1=Arriagada|first1=Pamela|last2=Anglada-Escudé|first2=Guillem|last3=Butler|first3=R. Paul|last4=Crane|first4=Jeffrey D.|last5=Shectman|first5=Stephen A.|last6=Thompson|first6=Ian|last7=Wende|first7=Sebastian|last8=Minniti|first8=Dante|journal=The Astrophysical Journal|volume=771|issue=1|page=42|bibcode=2013ApJ...771...42A|s2cid=119212312}} Disputed{{citation|arxiv=2203.06191|year=2022|title=Revisiting BD-06 1339b: A Likely False Positive Caused by Stellar Activity|doi=10.3847/1538-3881/ac5d41 |last1=Simpson |first1=Emilie R. |last2=Fetherolf |first2=Tara |last3=Kane |first3=Stephen R. |last4=Li |first4=Zhexing |last5=Pepper |first5=Joshua |last6=Močnik |first6=Teo |journal=The Astronomical Journal |volume=163 |issue=5 |page=215 |bibcode=2022AJ....163..215S |s2cid=247446960 |doi-access=free }}

|0.17

|

|125.94

|0.435

|

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

|66

|0.7

|4324

|

|2.3

|

|4100

|4.5

|

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

|65.3

|0.69

|3900

|{{citation|arxiv=1307.7640|year=2013|title=Secretly Eccentric: The Giant Planet and Activity Cycle of GJ 328|doi=10.1088/0004-637X/774/2/147|last1=Robertson|first1=Paul|last2=Endl|first2=Michael|last3=Cochran|first3=William D.|last4=MacQueen|first4=Phillip J.|last5=Boss|first5=Alan P.|journal=The Astrophysical Journal|volume=774|issue=2|page=147|bibcode=2013ApJ...774..147R|s2cid=118514735}}

|4

|

|

|43.5

|

|style="background:#FF6CDA"|imaging

|58.5

|1.22

|6234

|{{Cite journal|arxiv=1307.2886|title=Direct Imaging of a Cold Jovian Exoplanet in Orbit around the Sun-like Star GJ 504|journal=The Astrophysical Journal|volume=774|issue=11|pages=11|date=2013|last1= Kuzuhara|first1=M.|last2= Tamura|first2=M.|last3= Kudo|first3=T.|last4= Janson|first4=M.|last5= Kandori|first5=R.|last6= Brandt|first6=T. D.|last7= Thalmann|first7=C.|last8= Spiegel|first8=D.|last9= Biller|first9=B.|last10= Carson|first10=J.|last11= Hori|first11=Y.|last12= Suzuki|first12=R.|last13= Burrows|first13=A.|last14= Henning|first14=T.|last15= Turner|first15=E. L.|last16= McElwain|first16=M. W.|last17= Moro-Martin|first17=A.|last18= Suenaga|first18=T.|last19= Takahashi|first19=Y. H.|last20= Kwon|first20=J.|last21= Lucas|first21=P.|last22= Abe|first22=L.|last23= Brandner|first23=W.|last24= Egner|first24=S.|last25= Feldt|first25=M.|last26= Fujiwara|first26=H.|last27= Goto|first27=M.|last28= Grady|first28=C. A.|last29= Guyon|first29=O.|last30= Hashimoto|first30=J.|display-authors=9|doi=10.1088/0004-637X/774/1/11|bibcode = 2013ApJ...774...11K |s2cid=53343537}}

|0.352

|1.242

|4.301219

|0.0507

|

|style="background:#FFFF00"|transit

|1180

|0.94

|5295

|{{citation|arxiv=1308.2937|year=2013|title=HAT-P-44b, HAT-P-45b, AND HAT-P-46b: THREE TRANSITING HOT JUPITERS IN POSSIBLE MULTI-PLANET SYSTEMS|doi=10.1088/0004-6256/147/6/128|last1=Hartman|first1=J. D.|last2=Bakos|first2=G. Á.|last3=Torres|first3=G.|last4=Kovács|first4=G.|last5=Johnson|first5=J. A.|last6=Howard|first6=A. W.|last7=Marcy|first7=G. W.|last8=Latham|first8=D. W.|last9=Bieryla|first9=A.|last10=Buchhave|first10=L. A.|last11=Bhatti|first11=W.|last12=Béky|first12=B.|last13=Csubry|first13=Z.|last14=Penev|first14=K.|last15=De Val-Borro|first15=M.|last16=Noyes|first16=R. W.|last17=Fischer|first17=D. A.|last18=Esquerdo|first18=G. A.|last19=Everett|first19=M.|last20=Szklenár|first20=T.|last21=Zhou|first21=G.|last22=Bayliss|first22=D.|last23=Shporer|first23=A.|last24=Fulton|first24=B. J.|last25=Sanchis-Ojeda|first25=R.|last26=Falco|first26=E.|last27=Lázár|first27=J.|last28=Papp|first28=I.|last29=Sári|first29=P.|journal=The Astronomical Journal|volume=147|issue=6|page=128|s2cid=119293498}}

|4

|

|872.2

|1.752

|

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

|1180

|0.94

|5295

|Period is ambiguous

|0.892

|1.426

|3.128992

|0.0452

|

|style="background:#FFFF00"|transit

|990

|1.26

|6330

|

|0.493

|1.284

|4.463129

|0.0577

|

|style="background:#FFFF00"|transit

|970

|1.28

|6120

|

|1.345

|1.168

|1.354133

|0.023

|

|style="background:#FFFF00"|transit

|1200

|0.88

|5227

|{{citation|arxiv=1304.2140|year=2013|title=HATS-2b: A transiting extrasolar planet orbiting a K-type star showing starspot activity|doi=10.1051/0004-6361/201321663|last1=Mohler-Fischer|first1=M.|last2=Mancini|first2=L.|last3=Hartman|first3=J. D.|last4=Bakos|first4=G. Á.|last5=Penev|first5=K.|last6=Bayliss|first6=D.|last7=Jordán|first7=A.|last8=Csubry|first8=Z.|last9=Zhou|first9=G.|last10=Rabus|first10=M.|last11=Nikolov|first11=N.|last12=Brahm|first12=R.|last13=Espinoza|first13=N.|last14=Buchhave|first14=L. A.|last15=Béky|first15=B.|last16=Suc|first16=V.|last17=Csák|first17=B.|last18=Henning|first18=T.|last19=Wright|first19=D. J.|last20=Tinney|first20=C. G.|last21=Addison|first21=B. C.|last22=Schmidt|first22=B.|last23=Noyes|first23=R. W.|last24=Papp|first24=I.|last25=Lázár|first25=J.|last26=Sári|first26=P.|last27=Conroy|first27=P.|journal=Astronomy & Astrophysics|volume=558|pages=A55|bibcode=2013A&A...558A..55M|s2cid=59134384}}

|1.071

|1.381

|3.547851

|0.0485

|1648

|style="background:#FFFF00"|transit

|1480

|1.21

|6351

|{{citation|arxiv=1306.0624|title=HATS-3b: An inflated hot Jupiter transiting an F-type star|year=2013|doi=10.1088/0004-6256/146/5/113|last1=Bayliss|first1=D.|last2=Zhou|first2=G.|last3=Penev|first3=K.|last4=Bakos|first4=G. Á.|last5=Hartman|first5=J. D.|last6=Jordán|first6=A.|last7=Mancini|first7=L.|last8=Mohler-Fischer|first8=M.|last9=Suc|first9=V.|last10=Rabus|first10=M.|last11=Béky|first11=B.|last12=Csubry|first12=Z.|last13=Buchhave|first13=L.|last14=Henning|first14=T.|last15=Nikolov|first15=N.|last16=Csák|first16=B.|last17=Brahm|first17=R.|last18=Espinoza|first18=N.|last19=Noyes|first19=R. W.|last20=Schmidt|first20=B.|last21=Conroy|first21=P.|last22=Wright|first22=D. J.|last23=Tinney|first23=C. G.|last24=Addison|first24=B. C.|last25=Sackett|first25=P. D.|last26=Sasselov|first26=D. D.|last27=Lázár|first27=J.|last28=Papp|first28=I.|last29=Sári|first29=P.|journal=The Astronomical Journal|volume=146|issue=5|page=113|bibcode=2013AJ....146..113B|s2cid=119194040}}

|1.6

|

|311.6

|1.2

|

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

|375.8

|2.54

|4844

|{{citation|arxiv=1304.4328|year=2013|title=Planetary Companions to Three Evolved Intermediate-Mass Stars: HD 2952, HD 120084, andωSerpentis|doi=10.1093/pasj/65.4.85|last1=Sato|first1=Bun'ei|last2=Omiya|first2=Masashi|last3=Harakawa|first3=Hiroki|last4=Liu|first4=Yu-Juan|last5=Izumiura|first5=Hideyuki|last6=Kambe|first6=Eiji|last7=Takeda|first7=Yoichi|last8=Yoshida|first8=Michitoshi|last9=Itoh|first9=Yoichi|last10=Ando|first10=Hiroyasu|last11=Kokubo|first11=Eiichiro|last12=Ida|first12=Shigeru|journal=Publications of the Astronomical Society of Japan|volume=65|issue=4|page=85}}

|0.865

|

|19.382

|0.154

|

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

|218.2

|1.29

|6255

|{{citation |doi=10.1051/0004-6361/201322067 |arxiv=1311.5271 |year=2013 |title=The SOPHIE search for northern extrasolar planets VI. Three new hot Jupiters in multi-planet extrasolar systems |last1=Moutou |first1=Claire |last2=Hébrard |first2=Guillaume |last3=Bouchy |first3=François |last4=Arnold |first4=Luc |last5=Santos |first5=Nuno C. |last6=Astudillo-Defru |first6=Nicola |last7=Boisse |first7=Isabelle |last8=Bonfils |first8=Xavier |last9=Borgniet |first9=Simon |last10=Delfosse |first10=Xavier |last11=Díaz |first11=Rodrigo F. |last12=Ehrenreich |first12=David |last13=Forveille |first13=Thierry |last14=Gregório |first14=João |last15=Labrevoir |first15=Olivier |last16=Lagrange |first16=Anne-Marie |last17=Montagnier |first17=Guillaume |last18=Montalto |first18=Marco |last19=Pepe |first19=Francesco |last20=Sahlmann |first20=Johannes |last21=Santerne |first21=Alexandre |last22=Ségransan |first22=Damien |last23=Udry |first23=Stéphane |last24=Vanhuysse |first24=Michael |s2cid=118676953 }}

|5.13

|

|931

|2.03

|

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

|218.2

|1.29

|6255

|

|0.17

|

|152.6

|0.54

|

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

|116.1

|0.92

|5666

|{{citation|arxiv=1307.0894|title=Forever Alone? Testing Single Eccentric Planetary Systems for Multiple Companions|year=2013|doi=10.1088/0067-0049/208/1/2|last1=Wittenmyer|first1=Robert A.|last2=Wang|first2=Songhu|last3=Horner|first3=Jonathan|last4=Tinney|first4=C. G.|last5=Butler|first5=R. P.|last6=Jones|first6=H. R. A.|last7=O'Toole|first7=S. J.|last8=Bailey|first8=J.|last9=Carter|first9=B. D.|last10=Salter|first10=G. S.|last11=Wright|first11=D.|last12=Zhou|first12=Ji-Lin|journal=The Astrophysical Journal Supplement Series|volume=208|issue=1|page=2|bibcode=2013ApJS..208....2W|s2cid=14109907}} False positive, another planet with same assigned name discovered in 2019.{{cite journal | last1=Wittenmyer | first1=Robert A. | last2=Clark | first2=Jake T. | last3=Zhao | first3=Jinglin | last4=Horner | first4=Jonathan | last5=Wang | first5=Songhu | last6=Johns | first6=Daniel | display-authors=1 | title=Truly eccentric – I. Revisiting eight single-eccentric planetary systems | journal=Monthly Notices of the Royal Astronomical Society | volume=484 | issue=4 | pages=5859–5867 | year=2019 | arxiv=1901.08471 | bibcode=2019MNRAS.484.5859W | doi=10.1093/mnras/stz290 | doi-access=free }}

|5

|

|

|55.7

|

|style="background:#FF6CDA"|imaging

|298.7

|1.6

|

|{{cite journal | arxiv=1310.7483 | title = Confirmation of the planet around HD 95086 by direct imaging | author=Rameau, J., Chauvin, G., Lagrange, A.-M., Boccaletti, A., Quanz, S. P., Currie, T., Mawet, D., Girard, J. H., Bonnefoy, M., Kenworthy, M. | doi=10.1088/2041-8205/779/2/L26 | volume=779 | issue = 2 | journal=The Astrophysical Journal | page=L26|bibcode = 2013ApJ...779L..26R | year = 2013 | s2cid = 28985252 }}

|0.367

|

|5.8881

|0.07

|

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

|173.1

|1.33

|6489

|{{cite journal |journal = Astronomy & Astrophysics |volume = 551| id=A59|pages= 7 |title=The HARPS search for southern extrasolar planets: XXXVI. New multi-planet systems in the HARPS volume limited sample: a super-Earth and a Neptune in the habitable zone |arxiv=1301.2741|author1=Lo Curto, G. |author2=Mayor, M. |author3=Benz, W. |author4=Bouchy, F. |author5=Hébrard, G. |author6=Lovis, C. |author7=Moutou, C. |author8=Naef, D. |author9=Pepe, F. |author10=Queloz, D. |author11=Santos, N. C. |author12=Segransan, D. |author13=Udry, S. |year=2013|bibcode = 2013A&A...551A..59L |doi=10.1051/0004-6361/201220415|s2cid = 116916728}}

|11

|

|

|650

|

|style="background:#FF6CDA"|imaging

|299.5

|1.5

|6516

|{{cite journal |title=HD 106906 b: A planetary-mass companion outside a massive debris disk |journal=The Astrophysical Journal Letters |first1=Vanessa |last1=Bailey |first2=Tiffany |last2=Meshkat |first3=Megan |last3=Reiter |first4=Katie |last4=Morzinski |first5=Jared |last5=Males |first6=Kate Y. L. |last6=Su |first7=Philip M. |last7=Hinz |first8=Matthew |last8=Kenworthy |first9=Daniel |last9=Stark |first10=Eric |last10=Mamajek |first11=Runa |last11=Briguglio |first12=Laird M. |last12=Close |first13=Katherine B. |last13=Follette |first14=Alfio |last14=Puglisi |first15=Timothy |last15=Rodigas |first16=Alycia J. |last16=Weinberger |first17=Marco |last17=Xompero |display-authors=1 |volume=780 |issue=1 |page=L4 |date=January 2014 |arxiv=1312.1265 |doi=10.1088/2041-8205/780/1/L4 |bibcode=2014ApJ...780L...4B|s2cid=119113709 }}

|0.054

|

|7.8543

|0.079

|

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

|185.6

|1.05

|5783

|

|0.076

|

|30.93

|0.196

|

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

|185.6

|1.05

|5783

|

|2.83

|

|324

|0.92

|

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

|122.0

|1.4

|6576.6

|{{citation |doi=10.1051/0004-6361/201321783 |arxiv=1310.1994 |title=Extrasolar planets and brown dwarfs around A--F type stars. VIII. A giant planet orbiting the young star HD113337 |year=2013 |last1=Borgniet |first1=Simon |last2=Boisse |first2=Isabelle |last3=Lagrange |first3=Anne-Marie |last4=Bouchy |first4=François |last5=Arnold |first5=Luc |last6=Díaz |first6=Rodrigo F. |last7=Galland |first7=Franck |last8=Delorme |first8=Philippe |last9=Hébrard |first9=Guillaume |last10=Santerne |first10=Alexandre |last11=Ehrenreich |first11=David |last12=Ségransan |first12=Damien |last13=Bonfils |first13=Xavier |last14=Delfosse |first14=Xavier |last15=Santos |first15=Nuno C. |last16=Forveille |first16=Thierry |last17=Moutou |first17=Claire |last18=Udry |first18=Stéphane |last19=Eggenberger |first19=Anne |last20=Pepe |first20=Francesco |last21=Astudillo-Defru |first21=Nicola |last22=Montagnier |first22=Guillaume |journal=Astronomy & Astrophysics |volume=561 |pages=A65 |s2cid=118538542 }}

|4.5

|

|2082

|4.3

|

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

|318.5

|2.39

|4892

|

|1.13

|

|12.62

|0.11

|

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

|223.7

|1.12

|6123

|

|1.9

|

|248.4

|0.8

|

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

|223.7

|1.12

|6123

|

|6.575

|

|192

|0.747

|

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

|2830{{±|90}}

|1.5

|4791

|

|0.92{{±|0.03}}

|

|6.0962{{±|0.0002}}

|

|

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

|153

|0.73{{±|0.03}}

|4503{{±|85|61}}

|member of Hyades (star cluster){{cite journal|arxiv=2002.10562|last1=Carleo|first1=I.|s2cid=211296466|display-authors=etal|title=The GAPS Programme at TNG XXI -- A GIARPS case-study of known young planetary candidates: Confirmation of HD 285507 b and refutation of AD Leo B|journal=Astronomy & Astrophysics|year=2020|volume=A5|page=638|doi=10.1051/0004-6361/201937369|bibcode=2020A&A...638A...5C}}[http://www.openexoplanetcatalogue.com/planet/HD%20285507%20b/ Open exoplanet catalogue HD 285507]

|9.18

|

|124.6

|0.565

|

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

|486.8

|1.54

|4830

|{{cite journal | last1=Jones | first1=M. I. | last2=Jenkins | first2=J. S. | last3=Rojo | first3=P. | last4=Melo | first4=C. H. F. | last5=Bluhm | first5=Paz | display-authors=1 | title=Study of the Impact of the Post-MS evolution of the Host Star on the Orbits of Close-in Planets. II. A Giant Planet in a Close-in Orbit around the RGB Star HIP 63242 | journal=Astronomy & Astrophysics | volume=556 | issue=A78 | pages=5 | year=2013 | arxiv=1306.3939 | bibcode=2013A&A...556A..78J| doi=10.1051/0004-6361/201321660 | s2cid=118618692 }}

|1.068

|

|5.0505

|0.057

|

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

|145.0

|0.95

|5519

|

|1.477

|1.345

|2.7033904

|0.04122

|

|style="background:#FFFF00"|transit

|580

|1.28

|6306

|{{Cite journal|last1=Pepper|first1=Joshua|last2=Siverd|first2=Robert J.|last3=Beatty|first3=Thomas G.|last4=Gaudi|first4=B. Scott|last5=Stassun|first5=Keivan G.|last6=Eastman|first6=Jason|last7=Collins|first7=Karen|last8=Latham|first8=David W.|last9=Bieryla|first9=Allyson|last10=Buchhave|first10=Lars A.|last11=Jensen|first11=Eric L. N.|date=2013-08-01|title=KELT-3b: A Hot Jupiter Transiting a V = 9.8 Late-F Star|url=http://adsabs.harvard.edu/abs/2013ApJ...773...64P|journal=The Astrophysical Journal|volume=773|issue=1|pages=64|doi=10.1088/0004-637X/773/1/64|issn=0004-637X|arxiv=1211.1031|bibcode=2013ApJ...773...64P|s2cid=14691090}}

|0.442

|1.18

|7.8455821

|0.08

|

|style="background:#FFFF00"|transit

|720

|1.13

|6272

|{{citation|arxiv=1308.2296|year=2013|title=KELT-6b: AP~ 7.9 DAY HOT SATURN TRANSITING a METAL-POOR STAR WITH a LONG-PERIOD COMPANION|doi=10.1088/0004-6256/147/2/39|last1=Collins|first1=Karen A.|last2=Eastman|first2=Jason D.|last3=Beatty|first3=Thomas G.|last4=Siverd|first4=Robert J.|last5=Gaudi|first5=B. Scott|last6=Pepper|first6=Joshua|last7=Kielkopf|first7=John F.|last8=Johnson|first8=John Asher|last9=Howard|first9=Andrew W.|last10=Fischer|first10=Debra A.|last11=Manner|first11=Mark|last12=Bieryla|first12=Allyson|last13=Latham|first13=David W.|last14=Fulton|first14=Benjamin J.|last15=Gregorio|first15=Joao|last16=Buchhave|first16=Lars A.|last17=Jensen|first17=Eric L. N.|last18=Stassun|first18=Keivan G.|last19=Penev|first19=Kaloyan|last20=Crepp|first20=Justin R.|last21=Hinkley|first21=Sasha|last22=Street|first22=Rachel A.|last23=Cargile|first23=Phillip|last24=Mack|first24=Claude E.|last25=Oberst|first25=Thomas E.|last26=Avril|first26=Ryan L.|last27=Mellon|first27=Samuel N.|last28=McLeod|first28=Kim K.|last29=Penny|first29=Matthew T.|last30=Stefanik|first30=Robert P.|journal=The Astronomical Journal|volume=147|issue=2|page=39|s2cid=15020416|display-authors=1}}

|0.03146

|0.029

|13.3675

|

|

|style="background:#FFFF00"|transit

|220

|0.8

|5417

|{{citation|arxiv=1305.5587|year=2013|title=A sub-Mercury-sized exoplanet|doi=10.1038/nature11914|last1=Barclay|first1=Thomas|last2=Rowe|first2=Jason F.|last3=Lissauer|first3=Jack J.|last4=Huber|first4=Daniel|last5=Fressin|first5=François|last6=Howell|first6=Steve B.|last7=Bryson|first7=Stephen T.|last8=Chaplin|first8=William J.|last9=Désert|first9=Jean-Michel|last10=Lopez|first10=Eric D.|last11=Marcy|first11=Geoffrey W.|last12=Mullally|first12=Fergal|last13=Ragozzine|first13=Darin|last14=Torres|first14=Guillermo|last15=Adams|first15=Elisabeth R.|last16=Agol|first16=Eric|last17=Barrado|first17=David|last18=Basu|first18=Sarbani|last19=Bedding|first19=Timothy R.|last20=Buchhave|first20=Lars A.|last21=Charbonneau|first21=David|last22=Christiansen|first22=Jessie L.|last23=Christensen-Dalsgaard|first23=Jørgen|last24=Ciardi|first24=David|last25=Cochran|first25=William D.|last26=Dupree|first26=Andrea K.|last27=Elsworth|first27=Yvonne|last28=Everett|first28=Mark|last29=Fischer|first29=Debra A.|last30=Ford|first30=Eric B.|journal=Nature|volume=494|issue=7438|pages=452–454|pmid=23426260|bibcode=2013Natur.494..452B|s2cid=205232792|display-authors=1}}

|0.03776

|0.067

|21.302

|

|

|style="background:#FFFF00"|transit

|220

|0.8

|5417

|

|0.03839

|0.173

|39.7922

|

|

|style="background:#FFFF00"|transit

|220

|0.8

|5417

|

|

|0.192

|59.87756

|

|

|style="background:#FFFF00"|transit

|1103{{±|16}}

|0.64

|4017

|Exoplanet Characterization by Proxy: a Transiting 2.15 R_Earth Planet Near the Habitable Zone of the Late K dwarf Kepler-61 Sarah Ballard, David Charbonneau, Francois Fressin, Guillermo Torres, Jonathan Irwin, Jean-Michel Desert, Elisabeth Newton, Andrew W. Mann, David R. Ciardi, Justin R. Crepp, Christopher E. Henze, Stephen T. Bryson, Steven B. Howell, Elliott P. Horch, Mark E. Everett, Avi Shporer et al. April 26, 2013

|0.03

|0.117

|5.714932

|0.0553

|

|style="background:#FFFF00"|transit

|1200

|0.69

|4925

|{{citation|arxiv=1304.7387|year=2013|title=Kepler-62: A Five-Planet System with Planets of 1.4 and 1.6 Earth Radii in the Habitable Zone|doi=10.1126/science.1234702|last1=Borucki|first1=William J.|last2=Agol|first2=Eric|last3=Fressin|first3=Francois|last4=Kaltenegger|first4=Lisa|last5=Rowe|first5=Jason|last6=Isaacson|first6=Howard|last7=Fischer|first7=Debra|last8=Batalha|first8=Natalie|last9=Lissauer|first9=Jack J.|last10=Marcy|first10=Geoffrey W.|last11=Fabrycky|first11=Daniel|last12=Désert|first12=Jean-Michel|last13=Bryson|first13=Stephen T.|last14=Barclay|first14=Thomas|last15=Bastien|first15=Fabienne|last16=Boss|first16=Alan|last17=Brugamyer|first17=Erik|last18=Buchhave|first18=Lars A.|last19=Burke|first19=Chris|last20=Caldwell|first20=Douglas A.|last21=Carter|first21=Josh|last22=Charbonneau|first22=David|last23=Crepp|first23=Justin R.|last24=Christensen-Dalsgaard|first24=Jørgen|last25=Christiansen|first25=Jessie L.|last26=Ciardi|first26=David|last27=Cochran|first27=William D.|last28=Devore|first28=Edna|last29=Doyle|first29=Laurance|last30=Dupree|first30=Andrea K.|journal=Science|volume=340|issue=6132|pages=587–590|pmid=23599262|bibcode=2013Sci...340..587B|s2cid=21029755|display-authors=1}}

|0.013

|0.048

|12.4417

|0.0929

|

|style="background:#FFFF00"|transit

|1200

|0.69

|4925

|

|0.044

|0.174

|18.16406

|0.12

|

|style="background:#FFFF00"|transit

|1200

|0.69

|4925

|

|0.113

|0.144

|122.3874

|0.427

|

|style="background:#FFFF00"|transit

|1200

|0.69

|4925

|Potentially habitable exoplanet

|0.11

|0.126

|267.291

|0.718

|

|style="background:#FFFF00"|transit

|1200

|0.69

|4925

|Potentially habitable exoplanet

|0.378

|0.545

|9.4341505

|0.08

|

|style="background:#FFFF00"|transit

|650

|0.98

|5576

|{{citation|arxiv=1307.8128|title=KEPLER-63b: A GIANT PLANET IN a POLAR ORBIT AROUND a YOUNG SUN-LIKE STAR|year=2013|doi=10.1088/0004-637X/775/1/54|last1=Sanchis-Ojeda|first1=Roberto|last2=Winn|first2=Joshua N.|last3=Marcy|first3=Geoffrey W.|last4=Howard|first4=Andrew W.|last5=Isaacson|first5=Howard|last6=Johnson|first6=John Asher|last7=Torres|first7=Guillermo|last8=Albrecht|first8=Simon|last9=Campante|first9=Tiago L.|last10=Chaplin|first10=William J.|last11=Davies|first11=Guy R.|last12=Lund|first12=Mikkel N.|last13=Carter|first13=Joshua A.|last14=Dawson|first14=Rebekah I.|last15=Buchhave|first15=Lars A.|last16=Everett|first16=Mark E.|last17=Fischer|first17=Debra A.|last18=Geary|first18=John C.|last19=Gilliland|first19=Ronald L.|last20=Horch|first20=Elliott P.|last21=Howell|first21=Steve B.|last22=Latham|first22=David W.|journal=The Astrophysical Journal|volume=775|issue=1|page=54|bibcode=2013ApJ...775...54S|s2cid=36615256}}

|

|0.127

|2.15491

|0.035

|

|style="background:#FFFF00"|transit

|999{{±|8}}

|1.25

|6211

|

|

|0.23

|5.859944

|0.068

|

|style="background:#FFFF00"|transit

|999{{±|8}}

|1.25

|6211

|

|

|0.136

|8.13123

|0.084

|

|style="background:#FFFF00"|transit

|999{{±|8}}

|1.25

|6211

|{{citation|arxiv=1302.3728|year=2013|title=Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65|doi=10.1088/0004-637X/766/2/101|last1=Chaplin|first1=W. J.|last2=Sanchis-Ojeda|first2=R.|last3=Campante|first3=T. L.|last4=Handberg|first4=R.|last5=Stello|first5=D.|last6=Winn|first6=J. N.|last7=Basu|first7=S.|last8=Christensen-Dalsgaard|first8=J.|last9=Davies|first9=G. R.|last10=Metcalfe|first10=T. S.|last11=Buchhave|first11=L. A.|last12=Fischer|first12=D. A.|last13=Bedding|first13=T. R.|last14=Cochran|first14=W. D.|last15=Elsworth|first15=Y.|last16=Gilliland|first16=R. L.|last17=Hekker|first17=S.|last18=Huber|first18=D.|last19=Isaacson|first19=H.|last20=Karoff|first20=C.|last21=Kawaler|first21=S. D.|last22=Kjeldsen|first22=H.|last23=Latham|first23=D. W.|last24=Lund|first24=M. N.|last25=Lundkvist|first25=M.|last26=Marcy|first26=G. W.|last27=Miglio|first27=A.|last28=Barclay|first28=T.|last29=Lissauer|first29=J. J.|journal=The Astrophysical Journal|volume=766|issue=2|page=101|bibcode=2013ApJ...766..101C|s2cid=17748525}}

|

|0.25

|17.815815

|0.1352

|

|style="background:#FFFF00"|transit

|3610

|1.04

|5962

|Belongs to open cluster NGC 6811[https://www.nature.com/articles/nature12279 The same frequency of planets inside and outside open clusters of stars]

|

|0.262

|15.7259

|0.1171

|

|style="background:#FFFF00"|transit

|3610

|0.86

|5331

|Belongs to open cluster NGC 6811

|0.01878

|0.208

|5.39875

|

|1280

|style="background:#FFFF00"|transit

|440

|1.08

|5793

|{{cite journal | title=Kepler-68: Three Planets, One with a Density Between That of Earth and Ice Giants | last1=Gilliland | first1=Ronald L. | last2=Marcy | first2=Geoffrey W. | last3=Rowe | first3=Jason F. | last4=Rogers | first4=Leslie | last5=Torres | first5=Guillermo | last6=Fressin | first6=Francois | last7=Lopez | first7=Eric D. | last8=Buchhave | first8=Lars A. | last9=Christensen-Dalsgaard | first9=Jørgen | last10=Désert | first10=Jean-Michel | last11=Henze | first11=Christopher E. | last12=Isaacson | first12=Howard | last13=Jenkins | first13=Jon M. | last14=Lissauer | first14=Jack J. | last15=Chaplin | first15=William J. | last16=Basu | first16=Sarbani | last17=Metcalfe | first17=Travis S. | last18=Elsworth | first18=Yvonne | last19=Handberg | first19=Rasmus | last20=Hekker | first20=Saskia | last21=Huber | first21=Daniel | last22=Karoff | first22=Christoffer | last23=Kjeldsen | first23=Hans | last24=Lund | first24=Mikkel N. | last25=Lundkvist | first25=Mia | last26=Miglio | first26=Andrea | last27=Charbonneau | first27=David | last28=Ford | first28=Eric B. | last29=Fortney | first29=Jonathan J. | last30=Haas | first30=Michael R. | display-authors=1 | journal=The Astrophysical Journal | volume=766 | issue=1 | at=40 | year=2013 | arxiv=1302.2596 | bibcode=2013ApJ...766...40G | bibcode-access=free | doi=10.1088/0004-637X/766/1/40 | doi-access=free }}

|0.02265

|0.089

|9.60504

|

|

|style="background:#FFFF00"|transit

|440

|1.08

|5793

|

|0.84007

|

|625

|

|

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

|440

|1.08

|5793

|

|

|0.2

|13.722341

|0.094

|

|style="background:#FFFF00"|transit

|2430{{±|30}}

|0.81

|5638

|{{citation|arxiv=1304.4941|year=2013|title=A Super-Earth-Sized Planet Orbiting in or Near the Habitable Zone Around a Sun-Like Star|doi=10.1088/0004-637X/768/2/101|last1=Barclay|first1=Thomas|last2=Burke|first2=Christopher J.|last3=Howell|first3=Steve B.|last4=Rowe|first4=Jason F.|last5=Huber|first5=Daniel|last6=Isaacson|first6=Howard|last7=Jenkins|first7=Jon M.|last8=Kolbl|first8=Rea|last9=Marcy|first9=Geoffrey W.|last10=Quintana|first10=Elisa V.|last11=Still|first11=Martin|last12=Twicken|first12=Joseph D.|last13=Bryson|first13=Stephen T.|last14=Borucki|first14=William J.|last15=Caldwell|first15=Douglas A.|last16=Ciardi|first16=David|last17=Clarke|first17=Bruce D.|last18=Christiansen|first18=Jessie L.|last19=Coughlin|first19=Jeffrey L.|last20=Fischer|first20=Debra A.|last21=Li|first21=Jie|last22=Haas|first22=Michael R.|last23=Hunter|first23=Roger|last24=Lissauer|first24=Jack J.|last25=Mullally|first25=Fergal|last26=Sabale|first26=Anima|last27=Seader|first27=Shawn E.|last28=Smith|first28=Jeffrey C.|last29=Tenenbaum|first29=Peter|last30=Kamal Uddin|first30=A. K. M.|journal=The Astrophysical Journal|volume=768|issue=2|page=101|bibcode=2013ApJ...768..101B|s2cid=51490784|display-authors=1}}

|

|0.153

|242.4613

|0.64

|

|style="background:#FFFF00"|transit

|2430{{±|30}}

|0.81

|5638

|{{citation|arxiv=1305.2933|year=2013|title=A Potential Super-Venus in the Kepler-69 System|doi=10.1088/2041-8205/770/2/L20|last1=Kane|first1=Stephen R.|last2=Barclay|first2=Thomas|last3=Gelino|first3=Dawn M.|journal=The Astrophysical Journal|volume=770|issue=2|pages=L20|bibcode=2013ApJ...770L..20K|s2cid=9808447}}

|0.63

|0.96

|7.340711

|0.0781

|

|style="background:#FFFF00"|transit

|4300

|1.18

|6000

|

|10.1

|1.05

|8.8849116

|0.0818

|

|style="background:#FFFF00"|transit

|3700

|0.91

|5200

|{{citation|arxiv=1304.6002|year=2013|title=KOI-200 b and KOI-889 b: Two transiting exoplanets detected and characterized with Kepler, SOPHIE, and HARPS-N|doi=10.1051/0004-6361/201321394|last1=Hébrard|first1=G.|last2=Almenara|first2=J.-M.|last3=Santerne|first3=A.|last4=Deleuil|first4=M.|last5=Damiani|first5=C.|last6=Bonomo|first6=A. S.|last7=Bouchy|first7=F.|last8=Bruno|first8=G.|last9=Díaz|first9=R. F.|last10=Montagnier|first10=G.|last11=Moutou|first11=C.|journal=Astronomy & Astrophysics|volume=554|pages=A114|bibcode=2013A&A...554A.114H|s2cid=55185674}}

|2.01

|1.36

|1.5449298

|0.0274

|

|style="background:#00c9c2"|orbital brightness modulation

|2750{{±|30}}

|1.2

|6409

|{{cite journal | title=BEER Analysis of Kepler and CoRoT Light Curves. I. Discovery of Kepler-76b: A Hot Jupiter with Evidence for Superrotation | last1=Faigler | first1=S. | last2=Tal-Or | first2=L. | last3=Mazeh | first3=T. | last4=Latham | first4=D. W. | last5=Buchhave | first5=L. A. | display-authors=1 | journal=The Astrophysical Journal | volume=771 | issue=1 | at=26 | year=2013 | arxiv=1304.6841 | bibcode=2013ApJ...771...26F | doi=10.1088/0004-637X/771/1/26 | s2cid=119247392 }}

|0.43

|0.96

|3.57878087

|0.04501

|

|style="background:#FFFF00"|transit

|1900

|0.95

|5520

|{{citation|arxiv=1305.3891|year=2013|title=Kepler-77b: A very low albedo, Saturn-mass transiting planet around a metal-rich solar-like star|doi=10.1051/0004-6361/201321901|last1=Gandolfi|first1=D.|last2=Parviainen|first2=H.|last3=Fridlund|first3=M.|last4=Hatzes|first4=A. P.|last5=Deeg|first5=H. J.|last6=Frasca|first6=A.|last7=Lanza|first7=A. F.|last8=Prada Moroni|first8=P. G.|last9=Tognelli|first9=E.|last10=McQuillan|first10=A.|last11=Aigrain|first11=S.|last12=Alonso|first12=R.|last13=Antoci|first13=V.|last14=Cabrera|first14=J.|last15=Carone|first15=L.|last16=Csizmadia|first16=Sz.|last17=Djupvik|first17=A. A.|last18=Guenther|first18=E. W.|last19=Jessen-Hansen|first19=J.|last20=Ofir|first20=A.|last21=Telting|first21=J.|journal=Astronomy & Astrophysics|volume=557|pages=A74|bibcode=2013A&A...557A..74G|s2cid=30232940}}

|0.006

|0.105

|0.355

|

|2330

|style="background:#FFFF00"|transit

|407.1{{±|1.1}}

|0.76

|5058

|

|1.02

|1.204

|114.73635

|0.481

|478

|style="background:#FFFF00"|transit

|4170{{±|90}}

|1.1

|5600

|Two more unconfirmed planets in the system{{citation|arxiv=1310.2064|year=2013|title=An independent planet search in the Keplerdataset|doi=10.1051/0004-6361/201220935|last1=Ofir|first1=Aviv|last2=Dreizler|first2=Stefan|last3=Zechmeister|first3=Mathias|last4=Husser|first4=Tim-Oliver|journal=Astronomy & Astrophysics|volume=561|pages=A103|s2cid=118691606}}

|0.02

|0.548

|191.2318

|0.676

|403

|style="background:#FFFF00"|transit

|4170{{±|90}}

|1.1

|5600

|Two more unconfirmed planets in the system

|0.027

|0.337

|10.95416

|

|

|style="background:#FFFF00"|transit

|1110

|0.96

|5471

|

|0.626

|

|22.3395

|0.15525

|

|style="background:#FF7519"|timing

|1110

|0.96

|5471

|{{citation|arxiv=1304.4283|title=Koi-142, the King of Transit Variations, is a Pair of Planets Near the 2:1 Resonance|year=2013|doi=10.1088/0004-637X/777/1/3|last1=Nesvorný|first1=David|last2=Kipping|first2=David|last3=Terrell|first3=Dirk|last4=Hartman|first4=Joel|last5=Bakos|first5=Gáspár Á.|last6=Buchhave|first6=Lars A.|journal=The Astrophysical Journal|volume=777|issue=1|page=3|bibcode=2013ApJ...777....3N|s2cid=59933168}}{{citation|arxiv=1311.4335|year=2013|title=SOPHIE velocimetry of Keplertransit candidates|doi=10.1051/0004-6361/201323067|last1=Barros|first1=S. C. C.|last2=Díaz|first2=R. F.|last3=Santerne|first3=A.|last4=Bruno|first4=G.|last5=Deleuil|first5=M.|last6=Almenara|first6=J.-M.|last7=Bonomo|first7=A. S.|last8=Bouchy|first8=F.|last9=Damiani|first9=C.|last10=Hébrard|first10=G.|last11=Montagnier|first11=G.|last12=Moutou|first12=C.|journal=Astronomy & Astrophysics|volume=561|pages=L1|s2cid=118446884}}

|0.033

|0.153

|3.743208

|0.05119

|

|style="background:#FFFF00"|transit

|1577{{±|16}}

|1.28

|6182

|{{cite journal | title=Characterization of the KOI-94 System with Transit Timing Variation Analysis: Implication for the Planet-Planet Eclipse | last1=Masuda | first1=Kento | last2=Hirano | first2=Teruyuki | last3=Taruya | first3=Atsushi | last4=Nagasawa | first4=Makiko | last5=Suto | first5=Yasushi | display-authors=1 | journal=The Astrophysical Journal | volume=778 | issue=2 | at=185 | year=2013 | arxiv=1310.5771 | bibcode = 2013ApJ...778..185M | bibcode-access=free | doi=10.1088/0004-637X/778/2/185 | doi-access=free }}

|0.049

|0.385

|10.423648

|0.1013

|

|style="background:#FFFF00"|transit

|1577{{±|16}}

|1.28

|6182

|

|0.334

|1.005

|22.342989

|0.1684

|

|style="background:#FFFF00"|transit

|1577{{±|16}}

|1.28

|6182

|

|0.11

|0.585

|54.32031

|0.3046

|

|style="background:#FFFF00"|transit

|1577{{±|16}}

|1.28

|6182

|

|

|0.117

|7.008151

|0.074

|1056

|style="background:#FFFF00"|transit

|2500

|1.2

|6080

|

|

|0.106

|8.719375

|0.089

|981

|style="background:#FFFF00"|transit

|2500

|1.2

|6080

|

|

|0.256

|59.73667

|0.32

|518

|style="background:#FFFF00"|transit

|2500

|1.2

|6080

|

|

|0.237

|91.93913

|0.42

|448

|style="background:#FFFF00"|transit

|2500

|1.2

|6080

|

|

|0.257

|124.9144

|0.48

|592

|style="background:#FFFF00"|transit

|2500

|1.2

|6080

|

|

|0.723

|210.60697

|0.71

|340

|style="background:#FFFF00"|transit

|2500

|1.2

|6080

|

|

|1.008

|331.60059

|1.01

|292

|style="background:#FFFF00"|transit

|2500

|1.2

|6080

|

|0.81

|1.367

|6.24658

|0.0731

|

|style="background:#FFFF00"|transit

|3400

|1.31

|4550

|{{Cite journal|arxiv=1312.3943|last1= Lillo-Box|first1= J.|title= Kepler-91b: A planet at the end of its life. Planet and giant host star properties via light-curve variations|journal= Astronomy & Astrophysics|volume= 562|pages= A109|last2= Barrado|first2= D.|last3= Moya|first3= A.|last4= Montesinos|first4= B.|last5= Montalbán|first5= J.|last6= Bayo|first6= A.|last7= Barbieri|first7= M.|last8= Régulo|first8= C.|last9= Mancini|first9= L.|last10= Bouy|first10= H.|last11= Henning|first11= T.|year= 2013|doi= 10.1051/0004-6361/201322001|bibcode= 2014A&A...562A.109L|s2cid= 118486056}}

|0.202

|0.313

|13.749

|

|

|style="background:#FFFF00"|transit

|1580{{±|17}}

|1.21

|5883

|

|0.019

|0.232

|26.723

|

|

|style="background:#FFFF00"|transit

|1580{{±|17}}

|1.21

|5883

|

|0.028

|0.198

|16.1457

|

|579

|style="background:#FFFF00"|transit

|352.7{{±|0.7}}

|0.81

|4909

|

|

|0.429

|5.4122

|0.066

|

|style="background:#FFFF00"|transit

|1517{{±|18}}

|0.96

|5827

|

|0.009

|0.143

|8.041

|

|623

|style="background:#FFFF00"|transit

|852{{±|4}}

|0.56

|4605

|{{citation|arxiv=1309.2329|year=2013|title=Transit Timing Variation of Near-Resonance Planetary Pairs. Ii. Confirmation of 30 Planets in 15 Multiple-Planet Systems|doi=10.1088/0067-0049/210/2/25|last1=Xie|first1=Ji-Wei|journal=The Astrophysical Journal Supplement Series|volume=210|issue=2|page=25|s2cid=119105092}}

|0.012

|0.226

|11.776

|

|549

|style="background:#FFFF00"|transit

|852{{±|4}}

|0.56

|4605

|

|0.097

|0.101

|15.09

|

|

|style="background:#FFFF00"|transit

|1307{{±|12}}

|1.18

|6090

|

|0.105

|0.101

|22.804

|

|

|style="background:#FFFF00"|transit

|1307{{±|12}}

|1.18

|6090

|

|

|0.091

|8.457458

|0.079

|

|style="background:#FFFF00"|transit

|1042{{±|7}}

|1

|5884

|

|0.117

|0.236

|22.951

|

|

|style="background:#FFFF00"|transit

|1880{{±|30}}

|1.32

|6022

|

|0.25

|0.385

|42.882

|

|

|style="background:#FFFF00"|transit

|1880{{±|30}}

|1.32

|6022

|

|0.006

|0.259

|36.855

|

|

|style="background:#FFFF00"|transit

|4880{{±|140}}

|1.07

|5942

|

|0.024

|0.633

|49.412

|

|

|style="background:#FFFF00"|transit

|4880{{±|140}}

|1.07

|5942

|

|0.534

|0.5

|23.654

|

|

|style="background:#FFFF00"|transit

|6200{{±|300}}

|1.06

|5751

|

|0.042

|0.178

|50.447

|

|

|style="background:#FFFF00"|transit

|6200{{±|300}}

|1.06

|5751

|

|0.052

|0.259

|31.884

|

|

|style="background:#FFFF00"|transit

|3850{{±|150}}

|1.1

|6105

|

|0.051

|0.25

|48.648

|

|

|style="background:#FFFF00"|transit

|3850{{±|150}}

|1.1

|6105

|

|0.275

|0.261

|17.324

|

|

|style="background:#FFFF00"|transit

|3280{{±|50}}

|1.12

|5946

|

|0.202

|0.3

|33.006

|

|

|style="background:#FFFF00"|transit

|3280{{±|50}}

|1.12

|5946

|

|

|0.323

|12.309681

|0.112

|

|style="background:#FFFF00"|transit

|3480{{±|70}}

|1.1

|6363

|KOI-1236.01{{citation|arxiv=1308.0996|title=8 Planets in 4 Multi-planet Systems via TTVs in 1350 Days|year=2013|doi=10.1088/0004-637X/778/2/110|last1=Yang|first1=Ming|last2=Liu|first2=Hui-Gen|last3=Zhang|first3=Hui|last4=Zhou|first4=Ji-Lin|journal=The Astrophysical Journal |volume=778 |issue=2 |page=110 |bibcode=2013ApJ...778..110Y |s2cid=117080296}}

|0.155

|0.384

|35.736

|

|

|style="background:#FFFF00"|transit

|3490{{±|70}}

|1.1

|6363

|KOI-1236.02

|0.118

|0.277

|54.414

|

|

|style="background:#FFFF00"|transit

|3490{{±|70}}

|1.1

|6363

|

|0.192

|0.219

|24.806

|

|

|style="background:#FFFF00"|transit

|4540{{±|150}}

|0.97

|5602

|

|0.177

|0.277

|44.347

|

|

|style="background:#FFFF00"|transit

|4540{{±|150}}

|0.97

|5602

|

|0.033

|0.321

|5.487

|

|

|style="background:#FFFF00"|transit

|2900{{±|90}}

|0.76

|5100

| KOI-1563.01

|0.019

|0.294

|8.291

|

|

|style="background:#FFFF00"|transit

|2900{{±|90}}

|0.76

|5100

| KOI-1563.02

|0.02341

|0.217

|10.4208

|

|

|style="background:#FFFF00"|transit

|1908{{±|17}}

|0.91

|5367

|

|0.01145

|0.196

|13.0729

|

|

|style="background:#FFFF00"|transit

|1908{{±|17}}

|0.91

|5367

|

|0.09

|0.205

|34.921

|

|

|style="background:#FFFF00"|transit

|7700{{±|500}}

|1.15

|5914

|

|0.124

|0.482

|71.312

|

|

|style="background:#FFFF00"|transit

|7700{{±|500}}

|1.15

|5914

|

|0.019

|0.277

|17.849

|

|

|style="background:#FFFF00"|transit

|3210{{±|70}}

|1

|6186

|

|0.047

|0.25

|26.136

|

|

|style="background:#FFFF00"|transit

|3210{{±|70}}

|1

|6186

|

|0.238

|0.312

|42.994

|

|

|style="background:#FFFF00"|transit

|734{{±|5}}

|0.85

|5384

| KOI-2672.01

|0.056

|0.473

|88.505

|

|

|style="background:#FFFF00"|transit

|734{{±|5}}

|0.85

|5384

| KOI-2672.02

|

|0.253

|17.833648

|0.1226

|

|style="background:#FFFF00"|transit

|430

|1.21

|6273

|{{citation|arxiv=1312.4938|title=WHAT ASTEROSEISMOLOGY CAN DO FOR EXOPLANETS: KEPLER-410A b IS a SMALL NEPTUNE AROUND a BRIGHT STAR, IN AN ECCENTRIC ORBIT CONSISTENT WITH LOW OBLIQUITY|year=2013|doi=10.1088/0004-637X/782/1/14|last1=Van Eylen|first1=V.|last2=Lund|first2=M. N.|last3=Aguirre|first3=V. Silva|last4=Arentoft|first4=T.|last5=Kjeldsen|first5=H.|last6=Albrecht|first6=S.|last7=Chaplin|first7=W. J.|last8=Isaacson|first8=H.|last9=Pedersen|first9=M. G.|last10=Jessen-Hansen|first10=J.|last11=Tingley|first11=B.|last12=Christensen-Dalsgaard|first12=J.|last13=Aerts|first13=C.|last14=Campante|first14=T. L.|last15=Bryson|first15=S. T.|journal=The Astrophysical Journal|volume=782|issue=1 |page=14|bibcode=2014ApJ...782...14V |s2cid=15893540}}

|

|0.168

|3.00516

|0.038

|1040

|style="background:#FFFF00"|transit

|503.5{{±|1.5}}

|0.83

|4974

|{{citation|arxiv=1309.7097|year=2013|title=Influence of Stellar Multiplicity on Planet Formation. I. Evidence of Suppressed Planet Formation Due to Stellar Companions within 20 Au and Validation of Four Planets from Thekeplermultiple Planet Candidates|doi=10.1088/0004-637X/783/1/4|last1=Wang|first1=Ji|last2=Xie|first2=Ji-Wei|last3=Barclay|first3=Thomas|last4=Fischer|first4=Debra A.|journal=The Astrophysical Journal|volume=783|issue=1 |page=4|bibcode=2014ApJ...783....4W |s2cid=119214390}}

|

|0.3711{{±|0.12|0.06}}

|505.46{{±|0.05|0.04}}

|1.143±0.018

|

|style="background:#FFFF00"|transit

|2182{{±|81|82}}

|0.78{{±|0.03|0.04}}

|4709{{±|46|56}}

|{{citation|arxiv=1310.5912|year=2013|title=Planet Hunters. Vi. An Independent Characterization of Koi-351 and Several Long Period Planet Candidates from Thekeplerarchival Data|doi=10.1088/0004-6256/148/2/28|last1=Schmitt|first1=Joseph R.|last2=Wang|first2=Ji|last3=Fischer|first3=Debra A.|last4=Jek|first4=Kian J.|last5=Moriarty|first5=John C.|last6=Boyajian|first6=Tabetha S.|last7=Schwamb|first7=Megan E.|last8=Lintott|first8=Chris|last9=Lynn|first9=Stuart|last10=Smith|first10=Arfon M.|last11=Parrish|first11=Michael|last12=Schawinski|first12=Kevin|last13=Simpson|first13=Robert|last14=Lacourse|first14=Daryll|last15=Omohundro|first15=Mark R.|last16=Winarski|first16=Troy|last17=Goodman|first17=Samuel Jon|last18=Jebson|first18=Tony|last19=Schwengeler|first19=Hans Martin|last20=Paterson|first20=David A.|last21=Sejpka|first21=Johann|last22=Terentev|first22=Ivan|last23=Jacobs|first23=Tom|last24=Alsaadi|first24=Nawar|last25=Bailey|first25=Robert C.|last26=Ginman|first26=Tony|last27=Granado|first27=Pete|last28=Guttormsen|first28=Kristoffer Vonstad|last29=Mallia|first29=Franco|last30=Papillon|first30=Alfred L.|journal=The Astronomical Journal|volume=148|issue=2|page=28|s2cid=119238163|display-authors=1}} Also called KIC 6436029 c, discovery retracted in 2015 after 3rd transit was proven to be false.{{citation|arxiv=1512.02559|year=2015|title=Planet Hunters. Viii. Characterization of 41 Long-Period Exoplanet Candidates from Kepler Archival Data|doi=10.1088/0004-637X/815/2/127|last1=Wang|first1=Ji|last2=Fischer|first2=Debra A.|last3=Barclay|first3=Thomas|last4=Picard|first4=Alyssa|last5=Ma|first5=Bo|last6=Bowler|first6=Brendan P.|last7=Schmitt|first7=Joseph R.|last8=Boyajian|first8=Tabetha S.|last9=Jek|first9=Kian J.|last10=Lacourse|first10=Daryll|last11=Baranec|first11=Christoph|last12=Riddle|first12=Reed|last13=Law|first13=Nicholas M.|last14=Lintott|first14=Chris|last15=Schawinski|first15=Kevin|last16=Simister|first16=Dean Joseph|last17=Grégoire|first17=Boscher|last18=Babin|first18=Sean P.|last19=Poile|first19=Trevor|last20=Jacobs|first20=Thomas Lee|last21=Jebson|first21=Tony|last22=Omohundro|first22=Mark R.|last23=Schwengeler|first23=Hans Martin|last24=Sejpka|first24=Johann|last25=Terentev|first25=Ivan A.|last26=Gagliano|first26=Robert|last27=Paakkonen|first27=Jari-Pekka|last28=Berge|first28=Hans Kristian Otnes|last29=Winarski|first29=Troy|last30=Green|first30=Gerald R.|journal=The Astrophysical Journal|volume=815|issue=2|page=127|bibcode=2015ApJ...815..127W|s2cid=6327352|display-authors=1}}

|4.1

|

|

|3.3

|

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

|11000

|0.56

|

|{{citation|arxiv=1311.3424|year=2013|title=MOA-2008-BLG-379Lb: A MASSIVE PLANET FROM a HIGH MAGNIFICATION EVENT WITH a FAINT SOURCE|doi=10.1088/0004-637X/780/2/123|last1=Suzuki|first1=D.|last2=Udalski|first2=A.|last3=Sumi|first3=T.|last4=Bennett|first4=D. P.|last5=Bond|first5=I. A.|last6=Abe|first6=F.|last7=Botzler|first7=C. S.|last8=Freeman|first8=M.|last9=Fukagawa|first9=M.|last10=Fukui|first10=A.|last11=Furusawa|first11=K.|last12=Itow|first12=Y.|last13=Ling|first13=C. H.|last14=Masuda|first14=K.|last15=Matsubara|first15=Y.|last16=Muraki|first16=Y.|last17=Ohnishi|first17=K.|last18=Rattenbury|first18=N.|last19=Saito|first19=To.|last20=Shibai|first20=H.|last21=Sullivan|first21=D. J.|last22=Suzuki|first22=K.|last23=Sweatman|first23=W. L.|last24=Takino|first24=S.|last25=Tristram|first25=P. J.|last26=Wada|first26=K.|last27=Yock|first27=and P. C. M.|last28=Szymański|first28=M. K.|last29=Kubiak|first29=M.|last30=Soszyński|first30=I.|journal=The Astrophysical Journal|volume=780|issue=2|page=123|s2cid=119257768|display-authors=1}}

|0.02895

|

|

|0.92

|

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

|2600

|0.11

|

|{{citation|arxiv=1309.7714|year=2013|title=MOA-2010-BLG-328Lb: A SUB-NEPTUNE ORBITING VERY LATE M DWARF?|doi=10.1088/0004-637X/779/2/91|last1=Furusawa|first1=K.|last2=Udalski|first2=A.|last3=Sumi|first3=T.|last4=Bennett|first4=D. P.|last5=Bond|first5=I. A.|last6=Gould|first6=A.|last7=Jørgensen|first7=U. G.|last8=Snodgrass|first8=C.|last9=Prester|first9=D. Dominis|last10=Albrow|first10=M. D.|last11=Abe|first11=F.|last12=Botzler|first12=C. S.|last13=Chote|first13=P.|last14=Freeman|first14=M.|last15=Fukui|first15=A.|last16=Harris|first16=P.|last17=Itow|first17=Y.|last18=Ling|first18=C. H.|last19=Masuda|first19=K.|last20=Matsubara|first20=Y.|last21=Miyake|first21=N.|last22=Muraki|first22=Y.|last23=Ohnishi|first23=K.|last24=Rattenbury|first24=N. J.|last25=Saito|first25=To.|last26=Sullivan|first26=D. J.|last27=Suzuki|first27=D.|last28=Sweatman|first28=W. L.|last29=Tristram|first29=P. J.|last30=Wada|first30=K.|journal=The Astrophysical Journal|volume=779|issue=2|page=91|bibcode=2013ApJ...779...91F|s2cid=59519570|display-authors=1}}

|4.8

|

|

|1.1

|

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

|25200

|0.86

|

|{{citation|arxiv=1310.3706|title=MOA-2011-BLG-293Lb: First Microlensing Planet possibly in the Habitable Zone|year=2013|doi=10.1088/0004-637X/780/1/54|last1=Batista|first1=V.|last2=Beaulieu|first2=J. -P.|last3=Gould|first3=A.|last4=Bennett|first4=D. P.|last5=Yee|first5=J. C.|last6=Fukui|first6=A.|last7=Gaudi|first7=B. S.|last8=Sumi|first8=T.|last9=Udalski|first9=A.|journal=The Astrophysical Journal|volume=780|page=54|s2cid=118442165}}

|11.6

|

|

|4.3

|

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

|24700

|0.39

|

|{{citation|arxiv=1310.0008|year=2013|title=MOA-2011-BLG-322Lb: A 'second generation survey' microlensing planet|doi=10.1093/mnras/stt2477|last1=Shvartzvald|first1=Y.|last2=Maoz|first2=D.|last3=Kaspi|first3=S.|last4=Sumi|first4=T.|last5=Udalski|first5=A.|last6=Gould|first6=A.|last7=Bennett|first7=D. P.|last8=Han|first8=C.|last9=Abe|first9=F.|last10=Bond|first10=I. A.|last11=Botzler|first11=C. S.|last12=Freeman|first12=M.|last13=Fukui|first13=A.|last14=Fukunaga|first14=D.|last15=Itow|first15=Y.|last16=Koshimoto|first16=N.|last17=Ling|first17=C. H.|last18=Masuda|first18=K.|last19=Matsubara|first19=Y.|last20=Muraki|first20=Y.|last21=Namba|first21=S.|last22=Ohnishi|first22=K.|last23=Rattenbury|first23=N. J.|last24=Saito|first24=To.|last25=Sullivan|first25=D. J.|last26=Sweatman|first26=W. L.|last27=Suzuki|first27=D.|last28=Tristram|first28=P. J.|last29=Wada|first29=K.|last30=Yock|first30=P. C. M.|journal=Monthly Notices of the Royal Astronomical Society|volume=439|pages=604–610|doi-access=free |display-authors=1}}

|0.53

|

|

|2.72

|

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

|8400

|0.26

|

|{{citation|arxiv=1303.1184|title=A Giant Planet beyond the Snow Line in Microlensing Event OGLE-2011-BLG-0251|year=2013|doi=10.1051/0004-6361/201220626|last1=Kains|first1=N.|last2=Street|first2=R. A.|last3=Choi|first3=J.-Y.|last4=Han|first4=C.|last5=Udalski|first5=A.|last6=Almeida|first6=L. A.|last7=Jablonski|first7=F.|last8=Tristram|first8=P. J.|last9=Jørgensen|first9=U. G.|last10=Szymański|first10=M. K.|last11=Kubiak|first11=M.|last12=Pietrzyński|first12=G.|last13=Soszyński|first13=I.|last14=Poleski|first14=R.|last15=Kozłowski|first15=S.|last16=Pietrukowicz|first16=P.|last17=Ulaczyk|first17=K.|last18=Wyrzykowski|first18=Ł.|last19=Skowron|first19=J.|last20=Alsubai|first20=K. A.|last21=Bozza|first21=V.|last22=Browne|first22=P.|last23=Burgdorf|first23=M. J.|last24=Calchi Novati|first24=S.|last25=Dodds|first25=P.|last26=Dominik|first26=M.|last27=Dreizler|first27=S.|last28=Fang|first28=X.-S.|last29=Grundahl|first29=F.|last30=Gu|first30=C.-H.|journal=Astronomy & Astrophysics|volume=552|pages=A70|bibcode=2013A&A...552A..70K|s2cid=43146154|display-authors=29}}

|1.85

|

|

|0.87

|

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

|5700

|0.02

|

|Orbiting a brown dwarf{{citation|arxiv=1307.6335|year=2013|title=Microlensing Discovery of a Tight, Low-Mass-Ratio Planetary-Mass Object Around an Old Field Brown Dwarf|doi=10.1088/0004-637X/778/1/38|last1=Han|first1=C.|last2=Jung|first2=Y. K.|last3=Udalski|first3=A.|last4=Sumi|first4=T.|last5=Gaudi|first5=B. S.|last6=Gould|first6=A.|last7=Bennett|first7=D. P.|last8=Tsapras|first8=Y.|last9=Szymański|first9=M. K.|last10=Kubiak|first10=M.|last11=Pietrzyński|first11=G.|last12=Soszyński|first12=I.|last13=Skowron|first13=J.|last14=Kozłowski|first14=S.|last15=Poleski|first15=R.|last16=Ulaczyk|first16=K.|last17=Wyrzykowski|first17=Ł.|last18=Pietrukowicz|first18=P.|last19=Abe|first19=F.|last20=Bond|first20=I. A.|last21=Botzler|first21=C. S.|last22=Chote|first22=P.|last23=Freeman|first23=M.|last24=Fukui|first24=A.|last25=Furusawa|first25=K.|last26=Harris|first26=P.|last27=Itow|first27=Y.|last28=Ling|first28=C. H.|last29=Masuda|first29=K.|last30=Matsubara|first30=Y.|journal=The Astrophysical Journal|volume=778|issue=1|page=38|bibcode=2013ApJ...778...38H|s2cid=118663575|display-authors=1}}

|2.73

|

|

|3.45

|

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

|16200

|0.44

|

|{{citation|arxiv=1307.4084|year=2014|title=SUPER-MASSIVE PLANETS AROUND LATE-TYPE STARS—THE CASE OF OGLE-2012-BLG-0406Lb|doi=10.1088/0004-637X/782/1/47|last1=Poleski|first1=Radosław|last2=Udalski|first2=Andrzej|last3=Dong|first3=Subo|last4=Szymański|first4=Michał K.|last5=Soszyński|first5=Igor|last6=Kubiak|first6=Marcin|last7=Pietrzyński|first7=Grzegorz|last8=Kozłowski|first8=Szymon|last9=Pietrukowicz|first9=Paweł|last10=Ulaczyk|first10=Krzysztof|last11=Skowron|first11=Jan|last12=Wyrzykowski|first12=Łukasz|last13=Gould|first13=Andrew|journal=The Astrophysical Journal|volume=782|issue=1|page=47|bibcode=2014ApJ...782...47P|s2cid=118695225}}

|1.7

|

|277.02

|1.1

|

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

|263.0

|2.17

|4770

|

|

|0.903

|282.5255

|0.828

|281

|style="background:#FFFF00"|transit

|1130{{±|10}}

|0.94

|5629

|{{cite arXiv |last1=Wang |first1=Ji |eprint=1301.0644v1 |title=Planet Hunters. V. A Confirmed Jupiter-Size Planet in the Habitable Zone and 42 Planet Candidates from the Kepler Archive Data |class=astro-ph |date=January 3, 2013 }} Also called Kepler-86b

|2.31

|0.941

|3.1606296

|0.03734

|

|style="background:#FFFF00"|transit

|3900

|0.69

|4400

|{{citation|arxiv=1308.6574|year=2013|title=A hot Jupiter transiting a mid-K dwarf found in the pre-Omega Cam Transit Survey|doi=10.1093/mnras/stt1512|last1=Koppenhoefer|first1=J.|last2=Saglia|first2=R. P.|last3=Fossati|first3=L.|last4=Lyubchik|first4=Y.|last5=Mugrauer|first5=M.|last6=Bender|first6=R.|last7=Lee|first7=C.- H.|last8=Riffeser|first8=A.|last9=Afonso|first9=P.|last10=Greiner|first10=J.|last11=Henning|first11=T.|last12=Neuhauser|first12=R.|last13=Snellen|first13=I. A. G.|last14=Pavlenko|first14=Y.|last15=Verdugo|first15=M.|last16=Vogt|first16=N.|journal=Monthly Notices of the Royal Astronomical Society|volume=435|issue=4|pages=3133–3147|doi-access=free }}

|6.5

|1.53

|N/A

|N/A

|1160

|style="background:#FF6CDA"|imaging

|80

|N/A

|N/A

|Rogue planet{{cite journal | title = The Extremely Red, Young L Dwarf PSO J318-22: A Free-Floating Planetary-Mass Analog to Directly Imaged Young Gas-Giant Planets | journal = Astrophysical Journal Letters | date = 1 October 2013 | author = Michael C. Liu | display-authors = 4 | author2 = Eugene A. Magnier | author3 = Niall R. Deacon | author4 = Katelyn N. Allers | author5 = Trent J. Dupuy | author6 = Michael C. Kotson | author7 = Kimberly M. Aller | author8 = W. S. Burgett | author9 = K. C. Chambers | author10 = P. W. Draper | author11 = K. W. Hodapp | author12 = R. Jedicke | author13 = R.-P. Kudritzki | author14 = N. Metcalfe | author15 = J. S. Morgan | author16 = N. Kaiser | author17 = P. A. Price | author18 = J. L. Tonry | author19 = R. J. Wainscoat | volume = 777| issue = 2 | doi = 10.1088/2041-8205/777/2/L20 | arxiv=1310.0457|bibcode = 2013ApJ...777L..20L | s2cid = 54007072 }}

|16

|

|

|210

|

|style="background:#FF6CDA"|imaging

|390

|0.87

|3850

|{{citation|arxiv=1311.7664|year=2013|title=THREE WIDE PLANETARY-MASS COMPANIONS TO FW TAU, ROXs 12, AND ROXs 42B|doi=10.1088/0004-637X/781/1/20|last1=Kraus|first1=Adam L.|last2=Ireland|first2=Michael J.|last3=Cieza|first3=Lucas A.|last4=Hinkley|first4=Sasha|last5=Dupuy|first5=Trent J.|last6=Bowler|first6=Brendan P.|last7=Liu|first7=Michael C.|journal=The Astrophysical Journal|volume=781|page=20|bibcode=2014ApJ...781...20K |s2cid=41086512}}

|9

|

|

|157

|

|style="background:#FF6CDA"|imaging

|440

|1

|

|

|9.45

|

|4323

|5.28

|

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

|280

|1.03

|5600

|{{citation|arxiv=1312.2954|year=2013|doi=10.1088/0004-637X/785/2/126|last1=Knutson|first1=Heather A.|last2=Fulton|first2=Benjamin J.|last3=Montet|first3=Benjamin T.|last4=Kao|first4=Melodie|last5=Ngo|first5=Henry|last6=Howard|first6=Andrew W.|last7=Crepp|first7=Justin R.|last8=Hinkley|first8=Sasha|last9=Bakos|first9=Gaspar A.|last10=Batygin|first10=Konstantin|author11=John Asher Johnson|last12=Morton|first12=Timothy D.|last13=Muirhead|first13=Philip S.|title=Friends of Hot Jupiters. I. A Radial Velocity Search for Massive, Long-Period Companions to Close-In Gas Giant Planets|journal=The Astrophysical Journal|volume=785|issue=2|page=126|s2cid=42687848}}

|1.55

|1.112

|2.3114243

|0.0334

|

|style="background:#FFFF00"|transit

|1000

|0.93

|5600

|

|0.95

|1.24

|5.084298

|0.06206

|

|style="background:#FFFF00"|transit

|962{{±|8}}

|1.24

|5911

|

|0.26

|1.057

|3.8681382

|0.04525

|963

|style="background:#FFFF00"|transit

|160

|0.83

|4715

|{{citation|arxiv=1310.5654|title=Three sub-Jupiter-mass planets: WASP-69b & WASP-84b transit active K dwarfs and WASP-70Ab transits the evolved primary of a G4+K3 binary|year=2013|doi=10.1093/mnras/stu1737|last1=Anderson|first1=D. R.|last2=Collier Cameron|first2=A.|last3=Delrez|first3=L.|last4=Doyle|first4=A. P.|last5=Faedi|first5=F.|last6=Fumel|first6=A.|last7=Gillon|first7=M.|last8=Gómez Maqueo Chew|first8=Y.|last9=Hellier|first9=C.|last10=Jehin|first10=E.|last11=Lendl|first11=M.|last12=Maxted|first12=P. F. L.|last13=Pepe|first13=F.|last14=Pollacco|first14=D.|last15=Queloz|first15=D.|last16=Ségransan|first16=D.|last17=Skillen|first17=I.|last18=Smalley|first18=B.|last19=Smith|first19=A. M. S.|last20=Southworth|first20=J.|last21=Triaud|first21=A. H. M. J.|last22=Turner|first22=O. D.|last23=Udry|first23=S.|last24=West|first24=R. G.|doi-access=free }}

|0.59

|1.164

|3.7130203

|0.04853

|1387

|style="background:#FFFF00"|transit

|800

|1.11

|5763

|

|1.88

|1.16

|4.08722

|0.05512

|1790

|style="background:#FFFF00"|transit

|1042{{±|9}}

|1.34

|6036

|

|1.07

|1.27

|2.484193

|0.0375

|

|style="background:#FFFF00"|transit

|850

|1.14

|6100

|{{citation|arxiv=1307.6532|title=Discovery of WASP-65b and WASP-75b: Two Hot Jupiters Without Highly Inflated Radii|year=2013|doi=10.1051/0004-6361/201322314|last1=Gómez Maqueo Chew|first1=Y.|last2=Faedi|first2=F.|last3=Pollacco|first3=D.|last4=Brown|first4=D. J. A.|last5=Doyle|first5=A. P.|last6=Collier Cameron|first6=A.|last7=Gillon|first7=M.|last8=Lendl|first8=M.|last9=Smalley|first9=B.|last10=Triaud|first10=A. H. M. J.|last11=West|first11=R. G.|last12=Wheatley|first12=P. J.|last13=Busuttil|first13=R.|last14=Liebig|first14=C.|last15=Anderson|first15=D. R.|last16=Armstrong|first16=D. J.|last17=Barros|first17=S. C. C.|last18=Bento|first18=J.|last19=Bochinski|first19=J.|last20=Burwitz|first20=V.|last21=Delrez|first21=L.|last22=Enoch|first22=B.|last23=Fumel|first23=A.|last24=Haswell|first24=C. A.|last25=Hébrard|first25=G.|last26=Hellier|first26=C.|last27=Holmes|first27=S.|last28=Jehin|first28=E.|last29=Kolb|first29=U.|last30=Maxted|first30=P. F. L.|journal=Astronomy & Astrophysics|volume=559|pages=A36|bibcode=2013A&A...559A..36G|s2cid=1008674|display-authors=29}}{{citation|arxiv=1802.02132|year=2013|title=An Analysis of Transiting Hot Jupiters Observed with K2: WASP-55b and WASP-75b|doi=10.1088/1538-3873/aaa33e|last1=Clark|first1=B. J. M.|last2=Anderson|first2=D. R.|last3=Hellier|first3=C.|last4=Turner|first4=O. D.|last5=Močnik|first5=T.|journal=Publications of the Astronomical Society of the Pacific|volume=130|issue=985|page=034401|s2cid=119077382}}

|0.92

|1.83

|1.809886

|0.033

|2190

|style="background:#FFFF00"|transit

|390

|1.46

|6250

|{{citation|arxiv=1310.5607|year=2016|title=Three irradiated and bloated hot Jupiters|doi=10.1051/0004-6361/201527276|last1=West|first1=R. G.|last2=Hellier|first2=C.|last3=Almenara|first3=J.-M.|last4=Anderson|first4=D. R.|last5=Barros|first5=S. C. C.|last6=Bouchy|first6=F.|last7=Brown|first7=D. J. A.|last8=Collier Cameron|first8=A.|last9=Deleuil|first9=M.|last10=Delrez|first10=L.|last11=Doyle|first11=A. P.|last12=Faedi|first12=F.|last13=Fumel|first13=A.|last14=Gillon|first14=M.|last15=Gómez Maqueo Chew|first15=Y.|last16=Hébrard|first16=G.|last17=Jehin|first17=E.|last18=Lendl|first18=M.|last19=Maxted|first19=P. F. L.|last20=Pepe|first20=F.|last21=Pollacco|first21=D.|last22=Queloz|first22=D.|last23=Ségransan|first23=D.|last24=Smalley|first24=B.|last25=Smith|first25=A. M. S.|last26=Southworth|first26=J.|last27=Triaud|first27=A. H. M. J.|last28=Udry|first28=S.|journal=Astronomy & Astrophysics|volume=585|pages=A126|bibcode=2016A&A...585A.126W |s2cid=54746373}}

|0.538

|0.999

|3.06785234

|0.0344

|

|style="background:#FFFF00"|transit

|200

|0.58

|4143

|{{citation|arxiv=1303.0254|title=WASP-80b: a gas giant transiting a cool dwarf|year=2013|doi=10.1051/0004-6361/201220900|last1=Triaud|first1=A. H. M. J.|last2=Anderson|first2=D. R.|last3=Collier Cameron|first3=A.|last4=Doyle|first4=A. P.|last5=Fumel|first5=A.|last6=Gillon|first6=M.|last7=Hellier|first7=C.|last8=Jehin|first8=E.|last9=Lendl|first9=M.|last10=Lovis|first10=C.|last11=Maxted|first11=P. F. L.|last12=Pepe|first12=F.|last13=Pollacco|first13=D.|last14=Queloz|first14=D.|last15=Ségransan|first15=D.|last16=Smalley|first16=B.|last17=Smith|first17=A. M. S.|last18=Udry|first18=S.|last19=West|first19=R. G.|last20=Wheatley|first20=P. J.|journal=Astronomy & Astrophysics|volume=551|pages=A80|bibcode=2013A&A...551A..80T|s2cid=67805044}} Proper name Wadirum

|1.24

|1.67

|2.705782

|0.0447

|2190

|style="background:#FFFF00"|transit

|650

|1.63

|6490

|

|0.694

|0.942

|8.5234865

|0.0771

|797

|style="background:#FFFF00"|transit

|410

|0.84

|5314

|

|0.56

|1.7

|4.954

|0.06431

|1775

|style="background:#FFFF00"|transit

|1730{{±|30}}

|1.45

|6431

|{{citation|arxiv=1312.1827|title=Transiting planets from WASP-South, Euler and TRAPPIST:WASP-68 b, WASP-73 b and WASP-88 b, three hot Jupiters transiting evolved solar-type stars|year=2013|doi=10.1051/0004-6361/201323204|last1=Delrez|first1=L.|last2=Van Grootel|first2=V.|last3=Anderson|first3=D. R.|last4=Collier-Cameron|first4=A.|last5=Doyle|first5=A. P.|last6=Fumel|first6=A.|last7=Gillon|first7=M.|last8=Hellier|first8=C.|last9=Jehin|first9=E.|last10=Lendl|first10=M.|last11=Neveu-VanMalle|first11=M.|last12=Maxted|first12=P. F. L.|last13=Pepe|first13=F.|last14=Pollacco|first14=D.|last15=Queloz|first15=D.|last16=Ségransan|first16=D.|last17=Smalley|first17=B.|last18=Smith|first18=A. M. S.|last19=Southworth|first19=J.|last20=Triaud|first20=A. H. M. J.|last21=Udry|first21=S.|last22=West|first22=R. G.|journal=Astronomy and Astrophysics |volume=563 |bibcode=2014A&A...563A.143D |s2cid=54846964}}

|0.63{{±|0.07}}

|1.63{{±|0.09}}

|3.916243{{±|0.000003}}

|0.0562{{±|0.0012}}

|1840{{±|50}}

|style="background:#FFFF00"|transit

|1100{{±|200}}

|1.55{{±|0.10}}

|6440{{±|130}}

|

|1.13{{±|0.1|0.04}}

|1.21{{±|0.06}}

|2.184673{{±|0.0000014}}

|0.03416{{±|0.00083}}

|1570{{±|50}}

|style="background:#FFFF00"|transit

|450{{±|2}}

|1.11{{±|0.09}}

|5630{{±|130}}

|{{citation|arxiv=1310.5630|year=2013|title=Transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-95b to WASP-101b|doi=10.1093/mnras/stu410|last1=Hellier|first1=Coel|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=Pepe|first9=F.|last10=Pollacco|first10=D.|last11=Queloz|first11=D.|last12=Ségransan|first12=D.|last13=Smalley|first13=B.|last14=Smith|first14=A. M. S.|last15=Southworth|first15=J.|last16=Triaud|first16=A. H. M. J.|last17=Udry|first17=S.|last18=West|first18=R. G.|journal=Monthly Notices of the Royal Astronomical Society|volume=440|issue=3|pages=1982–1992|doi-access=free }}

|0.48{{±|0.03}}

|1.2{{±|0.06}}

|3.4252602{{±|0.0000027}}

|0.0453{{±|0.0013}}

|1285{{±|40}}

|style="background:#FFFF00"|transit

|1161{{±|15}}

|1.06{{±|0.09}}

|5540{{±|140}}

|

|1.32{{±|0.05}}

|1.13{{±|0.06}}

|2.07276{{±|0.000001}}

|0.03303{{±|0.00056}}

|1555{{±|40}}

|style="background:#FFFF00"|transit

|494.9{{±|1.7}}

|1.12{{±|0.06}}

|5640{{±|100}}

|

|0.83{{±|0.07}}

|1.10{{±|0.04}}

|2.96264036{{±|0.0000013}}

|0.03762{{±|0.001}}

|1180{{±|30}}

|style="background:#FFFF00"|transit

|926{{±|5}}

|0.69{{±|0.06}}

|5525{{±|130}}

|

|2.78{{±|0.13}}

|1.10{{±|0.08|0.05}}

|5.75251{{±|0.00004}}

|0.0717{{±|0.0016}}

|1480{{±|40}}

|style="background:#FFFF00"|transit

|519{{±|2}}

|1.48{{±|0.10}}

|6180{{±|100}}

|

|2.03{{±|0.12}}

|1.69{{±|0.29}}

|2.849375{{±|0.000008}}

|0.0457{{±|0.0010}}

|2190{{±|140}}

|style="background:#FFFF00"|transit

|1201{{±|9}}

|1.57{{±|0.10}}

|6900{{±|120}}

|

|0.50{{±|0.04}}

|1.41{{±|0.05}}

|3.585722{{±|0.000004}}

|0.0506{{±|0.0009}}

|1560{{±|35}}

|style="background:#FFFF00"|transit

|660{{±|3}}

|1.34{{±|0.07}}

|6400{{±|110}}

|

|1.12

|1.363

|1.0187068

|0.01855

|2000

|style="background:#FFFF00"|transit

|3300

|0.82

|5000

|[https://www.epj-conferences.org/articles/epjconf/abs/2013/08/epjconf_hpcs2012_01004/epjconf_hpcs2012_01004.html WTS-2 b: Too close for comfort?]{{citation|arxiv=1402.5416|year=2014|title=WTS-2 b: A hot Jupiter orbiting near its tidal destruction radius around a K dwarf|doi=10.1093/mnras/stu343|last1=Birkby|first1=J. L.|last2=Cappetta|first2=M.|last3=Cruz|first3=P.|last4=Koppenhoefer|first4=J.|last5=Ivanyuk|first5=O.|last6=Mustill|first6=A. J.|last7=Hodgkin|first7=S. T.|last8=Pinfield|first8=D. J.|last9=Sipőcz|first9=B.|last10=Kovács|first10=G.|last11=Saglia|first11=R.|last12=Pavlenko|first12=Y.|last13=Barrado|first13=D.|last14=Bayo|first14=A.|last15=Campbell|first15=D.|last16=Catalan|first16=S.|last17=Fossati|first17=L.|last18=Gálvez-Ortiz|first18=M.-C.|last19=Kenworthy|first19=M.|last20=Lillo-Box|first20=J.|last21=Martín|first21=E. L.|last22=Mislis|first22=D.|last23=De Mooij|first23=E. J. W.|last24=Nefs|first24=S. V.|last25=Snellen|first25=I. A. G.|last26=Stoev|first26=H.|last27=Zendejas|first27=J.|last28=Burgo|first28=C. del|last29=Barnes|first29=J.|last30=Goulding|first30=N.|journal=Monthly Notices of the Royal Astronomical Society|volume=440|issue=2|pages=1470–1489|doi-access=free |display-authors=1}}