// Workers AI · dad joke modeWhy was 2013's exoplanet list a star? It was out of this world.

This is a List of exoplanets discovered in 2013.

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

Name	Mass (`M`_J)	Radius (`R`_J)	Period (days)	Semi-major axis (AU)	Temp. (K)^[1]	Discovery method	Distance (ly)	Host star mass (`M`_☉)	Host star temp. (K)	Remarks
2MASS J01225093-2439505 b	24.5			52		imaging	120	0.4	3530	^[2]
BD+15 2940 b	1.11		137.48	0.539		radial vel.	572.2	1.1	4796	^[3]
CoRoT-25b	0.27	1.08	4.86069	0.0578		transit	3300	1.09	6040	^[4]
CoRoT-26b	0.52	1.26	4.20474	0.0526		transit	5400	1.09	5590	^[4]
DENIS-P J082303.1-491201 b	28.5		246.36	0.36		astrometry	67.7	0.07	2150	^[5]
Gliese 163 b	0.03335		8.63182	0.0607		radial vel.	48.8	0.4	3500	^[6]
Gliese 163 c	0.0214		25.63058	0.1254		radial vel.	48.8	0.4	3500	^[6]
Gliese 163 d	0.0925		603.95116	1.0304		radial vel.	48.8	0.4	3500	^[6]
Gliese 221b	0.027		3.8728	0.0428		radial vel.	66	0.7	4324	^[7]^[8] Disputed^[9]
Gliese 221 c	0.17		125.94	0.435		radial vel.	66	0.7	4324	^[7]^[8]
Gliese 328b	2.3		4100	4.5		radial vel.	65.3	0.69	3900	^[10]
Gliese 504 b	4			43.5		imaging	58.5	1.22	6234	^[11]
HAT-P-44b	0.352	1.242	4.301219	0.0507		transit	1180	0.94	5295	^[12]
HAT-P-44c	4		872.2	1.752		radial vel.	1180	0.94	5295	Period is ambiguous^[12]
HAT-P-45b	0.892	1.426	3.128992	0.0452		transit	990	1.26	6330	^[12]
HAT-P-46b	0.493	1.284	4.463129	0.0577		transit	970	1.28	6120	^[12]
HATS-2b	1.345	1.168	1.354133	0.023		transit	1200	0.88	5227	^[13]
HATS-3b	1.071	1.381	3.547851	0.0485	1648	transit	1480	1.21	6351	^[14]
HD 2952 b [ru]	1.6		311.6	1.2		radial vel.	375.8	2.54	4844	^[15]
HD 13908 b [fr]	0.865		19.382	0.154		radial vel.	218.2	1.29	6255	^[16]
HD 13908 c [fr]	5.13		931	2.03		radial vel.	218.2	1.29	6255	^[16]
HD 65216c	0.17		152.6	0.54		radial vel.	116.1	0.92	5666	^[17] False positive, another planet with same assigned name discovered in 2019.^[18]
HD 95086 b	5			55.7		imaging	298.7	1.6		^[19]
HD 103774 b	0.367		5.8881	0.07		radial vel.	173.1	1.33	6489	^[7]
HD 106906 b	11			650		imaging	299.5	1.5	6516	^[20]
HD 109271 b	0.054		7.8543	0.079		radial vel.	185.6	1.05	5783	^[7]
HD 109271 c	0.076		30.93	0.196		radial vel.	185.6	1.05	5783	^[7]
HD 113337 b	2.83		324	0.92		radial vel.	122.0	1.4	6576.6	^[21]
HD 120084 b	4.5		2082	4.3		radial vel.	318.5	2.39	4892	^[15]
HD 159243 b	1.13		12.62	0.11		radial vel.	223.7	1.12	6123	^[16]
HD 159243 c [fr]	1.9		248.4	0.8		radial vel.	223.7	1.12	6123	^[16]
HD 233604 b	6.575		192	0.747		radial vel.	2830±90	1.5	4791	^[3]
HD 285507 b	0.92±0.03		6.0962±0.0002			radial vel.	153	0.73±0.03	4503⁺⁸⁵ ₋₆₁	member of Hyades (star cluster)^[22]^[23]
HD 112410 b	9.18		124.6	0.565		radial vel.	486.8	1.54	4830	^[24]
HIP 91258 b [fr]	1.068		5.0505	0.057		radial vel.	145.0	0.95	5519	^[16]
KELT-3b	1.477	1.345	2.7033904	0.04122		transit	580	1.28	6306	^[25]
KELT-6b	0.442	1.18	7.8455821	0.08		transit	720	1.13	6272	^[26]
Kepler-37b	0.03146	0.029	13.3675			transit	220	0.8	5417	^[27]
Kepler-37c	0.03776	0.067	21.302			transit	220	0.8	5417	^[27]
Kepler-37d	0.03839	0.173	39.7922			transit	220	0.8	5417	^[27]
Kepler-61b		0.192	59.87756			transit	1103±16	0.64	4017	^[28]
Kepler-62b	0.03	0.117	5.714932	0.0553		transit	1200	0.69	4925	^[29]
Kepler-62c	0.013	0.048	12.4417	0.0929		transit	1200	0.69	4925	^[29]
Kepler-62d	0.044	0.174	18.16406	0.12		transit	1200	0.69	4925	^[29]
Kepler-62e	0.113	0.144	122.3874	0.427		transit	1200	0.69	4925	Potentially habitable exoplanet^[29]
Kepler-62f	0.11	0.126	267.291	0.718		transit	1200	0.69	4925	Potentially habitable exoplanet^[29]
Kepler-63b	0.378	0.545	9.4341505	0.08		transit	650	0.98	5576	^[30]
Kepler-65b		0.127	2.15491	0.035		transit	999±8	1.25	6211	^[31]
Kepler-65c		0.23	5.859944	0.068		transit	999±8	1.25	6211	^[31]
Kepler-65d		0.136	8.13123	0.084		transit	999±8	1.25	6211	^[31]
Kepler-66b		0.25	17.815815	0.1352		transit	3610	1.04	5962	Belongs to open cluster NGC 6811^[32]
Kepler-67b		0.262	15.7259	0.1171		transit	3610	0.86	5331	Belongs to open cluster NGC 6811^[32]
Kepler-68b	0.01878	0.208	5.39875		1280	transit	440	1.08	5793	^[33]
Kepler-68c	0.02265	0.089	9.60504			transit	440	1.08	5793	^[33]
Kepler-68d	0.84007		625			radial vel.	440	1.08	5793	^[33]
Kepler-69b		0.2	13.722341	0.094		transit	2430±30	0.81	5638	^[34]
Kepler-69c		0.153	242.4613	0.64		transit	2430±30	0.81	5638	^[34]^[35]
Kepler-74b [es]	0.63	0.96	7.340711	0.0781		transit	4300	1.18	6000	^[36]
Kepler-75b [es]	10.1	1.05	8.8849116	0.0818		transit	3700	0.91	5200	^[36]
Kepler-76b	2.01	1.36	1.5449298	0.0274		orbital brightness modulation	2750±30	1.2	6409	^[37]
Kepler-77b [es]	0.43	0.96	3.57878087	0.04501		transit	1900	0.95	5520	^[38]
Kepler-78b	0.006	0.105	0.355		2330	transit	407.1±1.1	0.76	5058	^[39]
Kepler-87b	1.02	1.204	114.73635	0.481	478	transit	4170±90	1.1	5600	Two more unconfirmed planets in the system^[39]
Kepler-87c	0.02	0.548	191.2318	0.676	403	transit	4170±90	1.1	5600	Two more unconfirmed planets in the system^[39]
Kepler-88b	0.027	0.337	10.95416			transit	1110	0.96	5471	^[40]
Kepler-88c	0.626		22.3395	0.15525		timing	1110	0.96	5471	^[40]^[41]
Kepler-89b	0.033	0.153	3.743208	0.05119		transit	1577±16	1.28	6182	^[42]
Kepler-89c	0.049	0.385	10.423648	0.1013		transit	1577±16	1.28	6182	^[42]
Kepler-89d	0.334	1.005	22.342989	0.1684		transit	1577±16	1.28	6182	^[42]
Kepler-89e	0.11	0.585	54.32031	0.3046		transit	1577±16	1.28	6182	^[42]
Kepler-90b		0.117	7.008151	0.074	1056	transit	2500	1.2	6080	^[43]
Kepler-90c		0.106	8.719375	0.089	981	transit	2500	1.2	6080	^[43]
Kepler-90d		0.256	59.73667	0.32	518	transit	2500	1.2	6080	^[43]
Kepler-90e		0.237	91.93913	0.42	448	transit	2500	1.2	6080	^[43]
Kepler-90f		0.257	124.9144	0.48	592	transit	2500	1.2	6080	^[43]
Kepler-90g		0.723	210.60697	0.71	340	transit	2500	1.2	6080	^[43]
Kepler-90h		1.008	331.60059	1.01	292	transit	2500	1.2	6080	^[43]
Kepler-91b	0.81	1.367	6.24658	0.0731		transit	3400	1.31	4550	^[44]
Kepler-92b	0.202	0.313	13.749			transit	1580±17	1.21	5883	^[45]
Kepler-92c	0.019	0.232	26.723			transit	1580±17	1.21	5883	^[45]
Kepler-102e	0.028	0.198	16.1457		579	transit	352.7±0.7	0.81	4909	^[46]
Kepler-105b		0.429	5.4122	0.066		transit	1517±18	0.96	5827	^[46]
Kepler-114c	0.009	0.143	8.041		623	transit	852±4	0.56	4605	^[45]
Kepler-114d	0.012	0.226	11.776		549	transit	852±4	0.56	4605	^[45]
Kepler-128b	0.097	0.101	15.09			transit	1307±12	1.18	6090	^[45]
Kepler-128c	0.105	0.101	22.804			transit	1307±12	1.18	6090	^[45]
Kepler-130b		0.091	8.457458	0.079		transit	1042±7	1	5884	^[46]
Kepler-145b	0.117	0.236	22.951			transit	1880±30	1.32	6022	^[45]
Kepler-145c	0.25	0.385	42.882			transit	1880±30	1.32	6022	^[45]
Kepler-177b	0.006	0.259	36.855			transit	4880±140	1.07	5942	^[45]
Kepler-177c	0.024	0.633	49.412			transit	4880±140	1.07	5942	^[45]
Kepler-238e	0.534	0.5	23.654			transit	6200±300	1.06	5751	^[45]
Kepler-238f	0.042	0.178	50.447			transit	6200±300	1.06	5751	^[45]
Kepler-276c	0.052	0.259	31.884			transit	3850±150	1.1	6105	^[45]
Kepler-276d	0.051	0.25	48.648			transit	3850±150	1.1	6105	^[45]
Kepler-277b	0.275	0.261	17.324			transit	3280±50	1.12	5946	^[45]
Kepler-277c	0.202	0.3	33.006			transit	3280±50	1.12	5946	^[45]
Kepler-279b		0.323	12.309681	0.112		transit	3480±70	1.1	6363	KOI-1236.01^[47]
Kepler-279c	0.155	0.384	35.736			transit	3490±70	1.1	6363	KOI-1236.02^[47]^[45]
Kepler-279d	0.118	0.277	54.414			transit	3490±70	1.1	6363	^[45]
Kepler-282d	0.192	0.219	24.806			transit	4540±150	0.97	5602	^[45]
Kepler-282e	0.177	0.277	44.347			transit	4540±150	0.97	5602	^[45]
Kepler-305b	0.033	0.321	5.487			transit	2900±90	0.76	5100	^[45] KOI-1563.01^[47]
Kepler-305c	0.019	0.294	8.291			transit	2900±90	0.76	5100	^[45] KOI-1563.02^[47]
Kepler-307b	0.02341	0.217	10.4208			transit	1908±17	0.91	5367	^[45]
Kepler-307c	0.01145	0.196	13.0729			transit	1908±17	0.91	5367	^[45]
Kepler-328b	0.09	0.205	34.921			transit	7700±500	1.15	5914	^[45]
Kepler-328c	0.124	0.482	71.312			transit	7700±500	1.15	5914	^[45]
Kepler-350c	0.019	0.277	17.849			transit	3210±70	1	6186	^[45]
Kepler-350d	0.047	0.25	26.136			transit	3210±70	1	6186	^[45]
Kepler-396b	0.238	0.312	42.994			transit	734±5	0.85	5384	^[45] KOI-2672.01^[47]
Kepler-396c	0.056	0.473	88.505			transit	734±5	0.85	5384	^[45] KOI-2672.02^[47]
Kepler-410Ab		0.253	17.833648	0.1226		transit	430	1.21	6273	^[48]
Kepler-411b		0.168	3.00516	0.038	1040	transit	503.5±1.5	0.83	4974	^[46]
Kepler-1359c		0.3711^+0.12 _−0.06	505.46^+0.05 _−0.04	1.143±0.018		transit	2182⁺⁸¹ ₋₈₂	0.78^+0.03 _−0.04	4709⁺⁴⁶ ₋₅₆	^[43] Also called KIC 6436029 c, discovery retracted in 2015 after 3rd transit was proven to be false.^[49]
MOA-2008-BLG-379Lb	4.1			3.3		microlensing	11000	0.56		^[50]
MOA-2010-BLG-328Lb	0.02895			0.92		microlensing	2600	0.11		^[51]
MOA-2011-BLG-293Lb	4.8			1.1		microlensing	25200	0.86		^[52]
MOA-2011-BLG-322Lb	11.6			4.3		microlensing	24700	0.39		^[53]
OGLE-2011-BLG-0251Lb	0.53			2.72		microlensing	8400	0.26		^[54]
OGLE-2012-BLG-358Lb	1.85			0.87		microlensing	5700	0.02		Orbiting a brown dwarf^[55]
OGLE-2012-BLG-406Lb	2.73			3.45		microlensing	16200	0.44		^[56]
Omega Serpentis b	1.7		277.02	1.1		radial vel.	263.0	2.17	4770	^[15]
PH2b		0.903	282.5255	0.828	281	transit	1130±10	0.94	5629	^[57] Also called Kepler-86b
POTS-1b	2.31	0.941	3.1606296	0.03734		transit	3900	0.69	4400	^[58]
PSO J318.5−22	6.5	1.53	N/A	N/A	1160	imaging	80	N/A	N/A	Rogue planet^[59]
ROXs 12b	16			210		imaging	390	0.87	3850	^[60]
ROXs 42Bb	9			157		imaging	440	1		^[60]
WASP-8c	9.45		4323	5.28		radial vel.	280	1.03	5600	^[61]
WASP-65b	1.55	1.112	2.3114243	0.0334		transit	1000	0.93	5600	^[62]
WASP-68b	0.95	1.24	5.084298	0.06206		transit	962±8	1.24	5911	^[63]
WASP-69b	0.26	1.057	3.8681382	0.04525	963	transit	160	0.83	4715	^[64]
WASP-70Ab	0.59	1.164	3.7130203	0.04853	1387	transit	800	1.11	5763	^[64]
WASP-73b	1.88	1.16	4.08722	0.05512	1790	transit	1042±9	1.34	6036	^[63]
WASP-75b	1.07	1.27	2.484193	0.0375		transit	850	1.14	6100	^[62]^[65]
WASP-76b	0.92	1.83	1.809886	0.033	2190	transit	390	1.46	6250	^[66]
WASP-80b	0.538	0.999	3.06785234	0.0344		transit	200	0.58	4143	^[67] Proper name Wadirum
WASP-82b [fr]	1.24	1.67	2.705782	0.0447	2190	transit	650	1.63	6490	^[66]
WASP-84b	0.694	0.942	8.5234865	0.0771	797	transit	410	0.84	5314	^[64]
WASP-88b	0.56	1.7	4.954	0.06431	1775	transit	1730±30	1.45	6431	^[63]
WASP-90b	0.63±0.07	1.63±0.09	3.916243±0.000003	0.0562±0.0012	1840±50	transit	1100±200	1.55±0.10	6440±130	^[66]
WASP-95b	1.13^+0.1 _−0.04	1.21±0.06	2.184673±0.0000014	0.03416±0.00083	1570±50	transit	450±2	1.11±0.09	5630±130	^[68]
WASP-96b	0.48±0.03	1.2±0.06	3.4252602±0.0000027	0.0453±0.0013	1285±40	transit	1161±15	1.06±0.09	5540±140	^[68]
WASP-97b	1.32±0.05	1.13±0.06	2.07276±0.000001	0.03303±0.00056	1555±40	transit	494.9±1.7	1.12±0.06	5640±100	^[68]
WASP-98b	0.83±0.07	1.10±0.04	2.96264036±0.0000013	0.03762±0.001	1180±30	transit	926±5	0.69±0.06	5525±130	^[68]
WASP-99b	2.78±0.13	1.10^+0.08 _−0.05	5.75251±0.00004	0.0717±0.0016	1480±40	transit	519±2	1.48±0.10	6180±100	^[68]
WASP-100b	2.03±0.12	1.69±0.29	2.849375±0.000008	0.0457±0.0010	2190±140	transit	1201±9	1.57±0.10	6900±120	^[68]
WASP-101b	0.50±0.04	1.41±0.05	3.585722±0.000004	0.0506±0.0009	1560±35	transit	660±3	1.34±0.07	6400±110	^[68]
WTS-2b	1.12	1.363	1.0187068	0.01855	2000	transit	3300	0.82	5000	^[69]^[70]

Bodies previously considered as candidates

MOA-2011-BLG-262L was once considered as a candidate exoplanet. It was once believed to be either an exoplanet with 3.2 times the mass of Jupiter and a exomoon with 0.47 times Earth's mass or a red dwarf with a mass of 0.11 solar masses orbited by a ~17 M_🜨 planet,^[71]^[72] but the latter scenario was confirmed in 2024 based on observations of the host star by the Keck telescope, 10 years after the ending of the microlensing event.^[73]

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanets by year of discovery

List of exoplanets discovered before 2000 (31)
List of exoplanets discovered between 2000–2009 (375)
List of exoplanets discovered in 2010 (109)
List of exoplanets discovered in 2011 (179)
List of exoplanets discovered in 2012 (149)
List of exoplanets discovered in 2013 (149)
List of exoplanets discovered in 2014 (869)
List of exoplanets discovered in 2015 (144)
List of exoplanets discovered in 2016 (1498)
List of exoplanets discovered in 2017 (152)
List of exoplanets discovered in 2018 (300)
List of exoplanets discovered in 2019 (169)
List of exoplanets discovered in 2020 (256)
List of exoplanets discovered in 2021 (253)
List of exoplanets discovered in 2022 (312)
List of exoplanets discovered in 2023 (304)
List of exoplanets discovered in 2024 (284)
List of exoplanets discovered in 2025 (238)
List of exoplanets discovered in 2026 (283)

References

↑ "The Extrasolar Planets Encyclopaedia". 1995. Retrieved 2015-11-09.
↑ PLANETS AROUND LOW-MASS STARS. III. A YOUNG DUSTY L DWARF COMPANION AT THE DEUTERIUM-BURNING LIMIT
1 2 BD+15 2940 AND HD 233604: TWO GIANTS WITH PLANETS CLOSE TO THE ENGULFMENT ZONE
1 2 Transiting exoplanets from the CoRoT space mission XXIV. CoRoT-25b and CoRoT-26b: two low-density giant planets
↑ Sahlmann, J.; Lazorenko, P. F.; Ségransan, D.; Martín, Eduardo L.; Queloz, D.; Mayor, M.; Udry, S. (2013), "Astrometric orbit of a low-mass companion to an ultracool dwarf", Astronomy & Astrophysics, 556: A133, arXiv:1306.3225, Bibcode:2013A&A...556A.133S, doi:10.1051/0004-6361/201321871, S2CID 119193690
1 2 3 Tuomi, M.; Anglada-Escudé, G. (2013). "Up to four planets around the M dwarf GJ 163". Astronomy & Astrophysics. 556: A111. arXiv:1306.1717. doi:10.1051/0004-6361/201321174. S2CID 16214668.
1 2 3 4 5 Lo Curto, G.; Mayor, M.; Benz, W.; Bouchy, F.; Hébrard, G.; Lovis, C.; Moutou, C.; Naef, D.; Pepe, F.; Queloz, D.; Santos, N. C.; Segransan, D.; Udry, S. (2013). "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". Astronomy & Astrophysics. 551: 7. arXiv:1301.2741. Bibcode:2013A&A...551A..59L. doi:10.1051/0004-6361/201220415. S2CID 116916728. A59.
1 2 Arriagada, Pamela; Anglada-Escudé, Guillem; Butler, R. Paul; Crane, Jeffrey D.; Shectman, Stephen A.; Thompson, Ian; Wende, Sebastian; Minniti, Dante (2013), "Two planetary companions around the K7 dwarf GJ 221 : a hot super-Earth and a candidate in the sub-Saturn desert range", The Astrophysical Journal, 771 (1): 42, arXiv:1305.2203, Bibcode:2013ApJ...771...42A, doi:10.1088/0004-637X/771/1/42, S2CID 119212312
↑ Simpson, Emilie R.; Fetherolf, Tara; Kane, Stephen R.; Li, Zhexing; Pepper, Joshua; Močnik, Teo (2022), "Revisiting BD-06 1339b: A Likely False Positive Caused by Stellar Activity", The Astronomical Journal, 163 (5): 215, arXiv:2203.06191, Bibcode:2022AJ....163..215S, doi:10.3847/1538-3881/ac5d41, S2CID 247446960
↑ Robertson, Paul; Endl, Michael; Cochran, William D.; MacQueen, Phillip J.; Boss, Alan P. (2013), "Secretly Eccentric: The Giant Planet and Activity Cycle of GJ 328", The Astrophysical Journal, 774 (2): 147, arXiv:1307.7640, Bibcode:2013ApJ...774..147R, doi:10.1088/0004-637X/774/2/147, S2CID 118514735
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1 2 The same frequency of planets inside and outside open clusters of stars
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[Xie2013-45] 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 Xie, Ji-Wei (2013), "Transit Timing Variation of Near-Resonance Planetary Pairs. Ii. Confirmation of 30 Planets in 15 Multiple-Planet Systems", The Astrophysical Journal Supplement Series, 210 (2): 25, arXiv:1309.2329, doi:10.1088/0067-0049/210/2/25, S2CID 119105092

[Wang2013-46] 1 2 3 4 Wang, Ji; Xie, Ji-Wei; Barclay, Thomas; Fischer, Debra A. (2013), "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", The Astrophysical Journal, 783 (1): 4, arXiv:1309.7097, Bibcode:2014ApJ...783....4W, doi:10.1088/0004-637X/783/1/4, S2CID 119214390

[Ming2013-47] 1 2 3 4 5 6 Yang, Ming; Liu, Hui-Gen; Zhang, Hui; Zhou, Ji-Lin (2013), "8 Planets in 4 Multi-planet Systems via TTVs in 1350 Days", The Astrophysical Journal, 778 (2): 110, arXiv:1308.0996, Bibcode:2013ApJ...778..110Y, doi:10.1088/0004-637X/778/2/110, S2CID 117080296

[48] Van Eylen, V.; Lund, M. N.; Aguirre, V. Silva; Arentoft, T.; Kjeldsen, H.; Albrecht, S.; Chaplin, W. J.; Isaacson, H.; Pedersen, M. G.; Jessen-Hansen, J.; Tingley, B.; Christensen-Dalsgaard, J.; Aerts, C.; Campante, T. L.; Bryson, S. T. (2013), "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", The Astrophysical Journal, 782 (1): 14, arXiv:1312.4938, Bibcode:2014ApJ...782...14V, doi:10.1088/0004-637X/782/1/14, S2CID 15893540

[49] Wang, Ji; et al. (2015), "Planet Hunters. Viii. Characterization of 41 Long-Period Exoplanet Candidates from Kepler Archival Data", The Astrophysical Journal, 815 (2): 127, arXiv:1512.02559, Bibcode:2015ApJ...815..127W, doi:10.1088/0004-637X/815/2/127, S2CID 6327352

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[51] Furusawa, K.; et al. (2013), "MOA-2010-BLG-328Lb: A SUB-NEPTUNE ORBITING VERY LATE M DWARF?", The Astrophysical Journal, 779 (2): 91, arXiv:1309.7714, Bibcode:2013ApJ...779...91F, doi:10.1088/0004-637X/779/2/91, S2CID 59519570

[52] Batista, V.; Beaulieu, J. -P.; Gould, A.; Bennett, D. P.; Yee, J. C.; Fukui, A.; Gaudi, B. S.; Sumi, T.; Udalski, A. (2013), "MOA-2011-BLG-293Lb: First Microlensing Planet possibly in the Habitable Zone", The Astrophysical Journal, 780: 54, arXiv:1310.3706, doi:10.1088/0004-637X/780/1/54, S2CID 118442165

[53] Shvartzvald, Y.; et al. (2013), "MOA-2011-BLG-322Lb: A 'second generation survey' microlensing planet", Monthly Notices of the Royal Astronomical Society, 439: 604–610, arXiv:1310.0008, doi:10.1093/mnras/stt2477

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[55] Han, C.; et al. (2013), "Microlensing Discovery of a Tight, Low-Mass-Ratio Planetary-Mass Object Around an Old Field Brown Dwarf", The Astrophysical Journal, 778 (1): 38, arXiv:1307.6335, Bibcode:2013ApJ...778...38H, doi:10.1088/0004-637X/778/1/38, S2CID 118663575

[56] Poleski, Radosław; Udalski, Andrzej; Dong, Subo; Szymański, Michał K.; Soszyński, Igor; Kubiak, Marcin; Pietrzyński, Grzegorz; Kozłowski, Szymon; Pietrukowicz, Paweł; Ulaczyk, Krzysztof; Skowron, Jan; Wyrzykowski, Łukasz; Gould, Andrew (2014), "SUPER-MASSIVE PLANETS AROUND LATE-TYPE STARS—THE CASE OF OGLE-2012-BLG-0406Lb", The Astrophysical Journal, 782 (1): 47, arXiv:1307.4084, Bibcode:2014ApJ...782...47P, doi:10.1088/0004-637X/782/1/47, S2CID 118695225

[57] Wang, Ji (January 3, 2013). "Planet Hunters. V. A Confirmed Jupiter-Size Planet in the Habitable Zone and 42 Planet Candidates from the Kepler Archive Data". arXiv:1301.0644v1 [astro-ph].

[58] Koppenhoefer, J.; Saglia, R. P.; Fossati, L.; Lyubchik, Y.; Mugrauer, M.; Bender, R.; Lee, C.- H.; Riffeser, A.; Afonso, P.; Greiner, J.; Henning, T.; Neuhauser, R.; Snellen, I. A. G.; Pavlenko, Y.; Verdugo, M.; Vogt, N. (2013), "A hot Jupiter transiting a mid-K dwarf found in the pre-Omega Cam Transit Survey", Monthly Notices of the Royal Astronomical Society, 435 (4): 3133–3147, arXiv:1308.6574, doi:10.1093/mnras/stt1512

[59] Michael C. Liu; Eugene A. Magnier; Niall R. Deacon; Katelyn N. Allers; et al. (1 October 2013). "The Extremely Red, Young L Dwarf PSO J318-22: A Free-Floating Planetary-Mass Analog to Directly Imaged Young Gas-Giant Planets". Astrophysical Journal Letters. 777 (2). arXiv:1310.0457. Bibcode:2013ApJ...777L..20L. doi:10.1088/2041-8205/777/2/L20. S2CID 54007072.

[Kraus2013-60] 1 2 Kraus, Adam L.; Ireland, Michael J.; Cieza, Lucas A.; Hinkley, Sasha; Dupuy, Trent J.; Bowler, Brendan P.; Liu, Michael C. (2013), "THREE WIDE PLANETARY-MASS COMPANIONS TO FW TAU, ROXs 12, AND ROXs 42B", The Astrophysical Journal, 781 (1): 20, arXiv:1311.7664, Bibcode:2014ApJ...781...20K, doi:10.1088/0004-637X/781/1/20, S2CID 41086512

[61] Knutson, Heather A.; Fulton, Benjamin J.; Montet, Benjamin T.; Kao, Melodie; Ngo, Henry; Howard, Andrew W.; Crepp, Justin R.; Hinkley, Sasha; Bakos, Gaspar A.; Batygin, Konstantin; John Asher Johnson; Morton, Timothy D.; Muirhead, Philip S. (2013), "Friends of Hot Jupiters. I. A Radial Velocity Search for Massive, Long-Period Companions to Close-In Gas Giant Planets", The Astrophysical Journal, 785 (2): 126, arXiv:1312.2954, doi:10.1088/0004-637X/785/2/126, S2CID 42687848

[Chew2013-62] 1 2 Gómez Maqueo Chew, Y.; Faedi, F.; Pollacco, D.; Brown, D. J. A.; Doyle, A. P.; Collier Cameron, A.; Gillon, M.; Lendl, M.; Smalley, B.; Triaud, A. H. M. J.; West, R. G.; Wheatley, P. J.; Busuttil, R.; Liebig, C.; Anderson, D. R.; Armstrong, D. J.; Barros, S. C. C.; Bento, J.; Bochinski, J.; Burwitz, V.; Delrez, L.; Enoch, B.; Fumel, A.; Haswell, C. A.; Hébrard, G.; Hellier, C.; Holmes, S.; Jehin, E.; Kolb, U.; et al. (2013), "Discovery of WASP-65b and WASP-75b: Two Hot Jupiters Without Highly Inflated Radii", Astronomy & Astrophysics, 559: A36, arXiv:1307.6532, Bibcode:2013A&A...559A..36G, doi:10.1051/0004-6361/201322314, S2CID 1008674

[Delrez2013-63] 1 2 3 Delrez, L.; Van Grootel, V.; Anderson, D. R.; Collier-Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M.; Neveu-VanMalle, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Udry, S.; West, R. G. (2013), "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", Astronomy and Astrophysics, 563, arXiv:1312.1827, Bibcode:2014A&A...563A.143D, doi:10.1051/0004-6361/201323204, S2CID 54846964

[Anderson2013-64] 1 2 3 Anderson, D. R.; Collier Cameron, A.; Delrez, L.; Doyle, A. P.; Faedi, F.; Fumel, A.; Gillon, M.; Gómez Maqueo Chew, Y.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Skillen, I.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Turner, O. D.; Udry, S.; West, R. G. (2013), 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, arXiv:1310.5654, doi:10.1093/mnras/stu1737

[Clark2013-65] Clark, B. J. M.; Anderson, D. R.; Hellier, C.; Turner, O. D.; Močnik, T. (2013), "An Analysis of Transiting Hot Jupiters Observed with K2: WASP-55b and WASP-75b", Publications of the Astronomical Society of the Pacific, 130 (985): 034401, arXiv:1802.02132, doi:10.1088/1538-3873/aaa33e, S2CID 119077382

[West2013-66] 1 2 3 West, R. G.; Hellier, C.; Almenara, J.-M.; Anderson, D. R.; Barros, S. C. C.; Bouchy, F.; Brown, D. J. A.; Collier Cameron, A.; Deleuil, M.; Delrez, L.; Doyle, A. P.; Faedi, F.; Fumel, A.; Gillon, M.; Gómez Maqueo Chew, Y.; Hébrard, G.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Udry, S. (2016), "Three irradiated and bloated hot Jupiters", Astronomy & Astrophysics, 585: A126, arXiv:1310.5607, Bibcode:2016A&A...585A.126W, doi:10.1051/0004-6361/201527276, S2CID 54746373

[67] Triaud, A. H. M. J.; Anderson, D. R.; Collier Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M.; Lovis, C.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Udry, S.; West, R. G.; Wheatley, P. J. (2013), "WASP-80b: a gas giant transiting a cool dwarf", Astronomy & Astrophysics, 551: A80, arXiv:1303.0254, Bibcode:2013A&A...551A..80T, doi:10.1051/0004-6361/201220900, S2CID 67805044

[Hellier2013-68] 1 2 3 4 5 6 7 Hellier, Coel; Anderson, D. R.; Cameron, A. Collier; Delrez, L.; Gillon, M.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Udry, S.; West, R. G. (2013), "Transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-95b to WASP-101b", Monthly Notices of the Royal Astronomical Society, 440 (3): 1982–1992, arXiv:1310.5630, doi:10.1093/mnras/stu410

[69] WTS-2 b: Too close for comfort?

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[Bennett2014-71] Bennett, D.P.; Batista, V.; et al. (13 December 2013). "A Sub-Earth-Mass Moon Orbiting a Gas Giant Primary or a High Velocity Planetary System in the Galactic Bulge". The Astrophysical Journal. 785 (2): 155. arXiv:1312.3951. Bibcode:2014ApJ...785..155B. doi:10.1088/0004-637X/785/2/155. S2CID 118327512.

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Bodies previously considered as candidates

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References