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List of exoplanets discovered in 2017

From Wikipedia, the free encyclopedia

This is alist of exoplanets discovered in 2017.

For exoplanets detected only by radial velocity, the mass value is actually a lower limit. (SeeMinimum 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
BD+03 2562 b	6.4		481.9	1.3		radial vel.	8540	1.14	4095	^[2]
CoRoT-30 b	2.90±0.22	1.009±0.076	9.06005±0.00024	0.0844±0.0012		transit	3100±200	0.98^+0.03 _−0.05	5650±100	^[3]
CoRoT-31 b	0.84±0.34	1.46±0.30	4.62941±0.00075	0.0586±0.0034		transit	7000±2000	1.25^+0.22 _−0.21	5700±120	^[3]
CoRoT-32 b	0.15	0.57	6.71837	0.071	938	transit		1.08	5970	Host star also known as CoRoT 223977153^[4]
Luyten b	0.00909		18.6498	0.091101	259	radial vel.	12	0.29	3382	Potentially habitable exoplanet.^[5]
Luyten c	0.00371		4.7234	0.036467		radial vel.	12	0.29	3382	^[5]
Gliese 625 b	0.00887		14.628	0.078361		radial vel.	21	0.30	3499	^[6]
Gliese 1148 c	0.2141		532.58	0.912		radial vel.	35.98	0.357±0.013		Host star also known as Ross 1003^[7]
Gliese 3138 b	0.0056		1.22003	0.0197		radial vel.	92.9	0.68	3717	^[5]
Gliese 3138 c	0.01315		5.974	0.057		radial vel.	92.9	0.68	3717	^[5]
Gliese 3138 d	0.03304		257.8	0.698		radial vel.	92.9	0.68	3717	^[5]
Gliese 3293 d	0.02391		48.1345	0.19394		radial vel.	51.4	0.42	3466	^[5]
Gliese 3293 e	0.01032		13.2543	0.08208		radial vel.	51.4	0.42	3466	^[5]
Gliese 3323 b	0.00636		5.3636	0.03282		radial vel.	17.4	0.16	3159	^[5]
Gliese 3323 c	0.00727		40.54	0.1264		radial vel.	17.4	0.16	3159	^[5]
Gliese 3942 b	0.0225		6.905	0.0608	590	radial vel.	55.3	0.63	3867	^[8]
HAT-P-67b	0.34	2.085	4.81010250	0.06505		transit	1000	1.642	6406	^[9]
HATS-36b	2.79±0.40	1.263±0.045	4.1752379±0.0000021	0.0529±0.0011	1363±40	transit	2860±70	1.135±0.067	5970±160	Host star also known as K2-145^[10] Host star also known as K2-145
HATS-43b	0.261±0.054	1.180±0.050	4.3888497	0.04944±0.00046	1003±27	transit	1194.1±7.4	0.837±0.023	5099±61	^[11]
HATS-44b	0.56±0.11	1.067^+0.125 _−0.071	2.7439004	0.03649±0.00030	1161±34	transit	1474±11	0.860±0.021	5080±100	^[11]
HATS-45b	0.70±0.15	1.286±0.093	4.1876244	0.05511±0.00069	1518±45	transit	2575±38	1.272±0.048	6450±110	^[11]
HATS-46b	0.173±0.062	0.903^+0.058 _−0.045	4.7423729	0.05367±0.00053	1054±29	transit	1500±13	0.917±0.027	5495±69	^[11]
HATS-50b	0.39	1.130	3.8297015	0.05046		transit	2340	1.17	5990	^[12]
HATS-51b	0.768	1.41	3.3488702	0.04639	1553	transit	1560	1.17	5758	^[12]
HATS-52b	2.24	1.382	1.36665436	0.02498	1834	transit	2060	1.11	6010	^[12]
HATS-53b	0.595	1.340	3.8537768	0.04753	1312	transit	2000	0.96	5644	^[12]
HD 3167 d	0.0217		8.509	0.07757		radial vel.	149	0.86	5261	^[13]
HD 17674 b	0.87		623.8	1.42		radial vel.	145	0.98	5904	^[14]
HD 20781 d	0.0061^+0.0012 _−0.0011	0.2052	5.3135±0.001	0.0529^+0.0024 _−0.0027		radial vel.	115.36±4.4	0.7	5256±29	^[15]
HD 20781 e	0.0168^+0.0022 _−0.0021	0.2183	13.8905^+0.0033 _−0.0034	0.1004^+0.0046 _−0.0051		radial vel.	115.36±4.4	0.7	5256±29	^[15]
HD 20794 e	0.0150		147.02	0.509		radial vel.	19.8	0.7	5401	^[16]
HD 27894 c	0.162		36.07	0.198		radial vel.	138.2	0.8	4875	^[17]
HD 27894 d	5.415		5174	5.448		radial vel.	138.2	0.8	4875	^[17]
HD 29021 b	2.4		1362.3	2.28		radial vel.	100	0.85	5560	^[14]
HD 40956 b	2.7		578.6	1.4		radial vel.	385	2.00	4869	^[18]
HD 42012 b	1.6		857.5	1.67		radial vel.	121	0.83	5405	^[14]
HD 45184 c	0.0277^+0.0034 _−0.0032		13.1354^+0.0026 _−0.0025	0.11^+0.0034 _−0.0036		radial vel.	71.36±0.62	1.03	5869±14	^[19]
HD 76920 b	3.93		415.891^+0.043 _−0.039	1.149		radial vel.	602.7	1.17	4698	Extremely eccentric orbit around an evolvedred giant^[20]^[21]^[22]
HD 93385 Ab	0.0125±0.0015		7.3422±0.0014	0.0749±0.0017	1129±19	radial vel.	141.6±0.2	1.04±0.01	5823±35	^[19] Confirmed in 2021, renamed from HD 93385 d^[23]
HD 106315 b	0.0255	0.207	9.55804	0.0905	1046	transit	358	1.08	6277	Host star also known as K2-109^[24]
HD 106315 c	0.0560	0.385	21.05788	0.1533	804	transit	358	1.08	6277	Host star also known as K2-109^[24]
HD 111591 b	4.4		1056.4	2.5		radial vel.	352	1.94	4884	^[18]
HD 113996 b	6.3		610.2	1.6		radial vel.	331.4	1.49	4181	^[18]
HD 147379 b	0.0777		86.54	0.3193		radial vel.	35.01	0.58	4090	^[25]
HD 176986 b	0.0181		6.48980	0.06296		radial vel.	86.1	0.79	4931	^[26]
HD 176986 c	0.02888		16.8191	0.11878		radial vel.	86.1	0.79	4931	^[26]
HD 177565 b	0.04751		44.505	0.246		radial vel.	56	1.0		^[27]
HD 208897 b	1.40		352.7	1.05		radial vel.	211	1.25	4860	^[28]
HIP 65426 b	9.0±3.0	1.5±0.1	230,400	92	1500⁺¹⁰⁰ ₋₂₀₀	imaging	363.3±12.3	1.96±0.05	8840±200	Gas giant orbiting the host star also known as HD 116434^[29]^[30]
K2-18c	0.0236		8.962	0.060	363	radial vel.	110	0.36	3547	^[31]
K2-105b	0.09439	0.369	8.266902	0.081		transit	760	1.01	5434	^[32]
K2-106b	0.0263	0.136	0.571292	0.0116	2333	transit	798	0.95	5470	^[33] Host star also known as EPIC 220674823
K2-106c		0.226	13.341245			transit	830	0.93	5590	^[33] Host star also known as EPIC 220674823
K2-108b	0.18689	0.471	4.73401	0.0573	1446	transit	1530	1.12	5474	^[34]
K2-111b	0.0271	0.17	5.35117	0.0621	1309	transit	680	0.88	5730	^[35]
K2-114b	1.85	0.942	11.39109	0.09309	719	transit	1570	0.83	5027	^[36]
K2-115b	0.84	1.115	20.273034	0.1367	682	transit	1360	0.83	5560	^[36]
K2-116b [ru]		0.062	4.655411	0.048		transit	183.1	0.69	4348	^[37] Host star also known as BD-12 6259
K2-117b		0.175	1.291505	0.019		transit	333.5	0.58	3842	^[38]
K2-117c		0.181	5.444820	0.051		transit	333.5	0.58	3842	^[38]
K2-118b		0.227	50.92092	0.245		transit	1057	0.76	4726	^[37]
K2-119b		0.204	7.728578	0.070		transit	1180	0.76	4753	^[37]
K2-120b		0.179	9.562742	0.078		transit	950	0.69	4350	^[37]
K2-121b		0.814	5.185754	0.052		transit	552	0.71	4471	^[37]
K2-122b		0.114	2.219405	0.029		transit	236	0.63	3993	^[37]^[38]
K2-123b		0.236	30.956763	0.167		transit	529	0.65	4076	^[37]^[38]
K2-124b		0.236	6.413539	0.051		transit	448	0.44	3561	^[37]
K2-125b		0.194	21.750264	0.121		transit	415	0.49	3654	^[37]
K2-126b		0.164	7.387073	0.066		transit	332	0.70	4368	^[37]
K2-127b		0.773	3.588165	0.041		transit	2370	0.70	4388	^[37]
K2-128b		0.127	5.675819	0.056		transit	373	0.71	4470	^[37]
K2-129b		0.0928	8.239493	0.057		transit	90.19±0.07	0.36	3459	^[37] Host star also known as LP 868-19
K2-130b		0.112	2.494120	0.032		transit	384.4±0.6	0.70	4356	^[37]
K2-131b	0.017	0.152	0.36931	0.009500	2062	transit	501	0.84	5245	^[39]
K2-132b		1.30	9.1751			transit	568	1.08±0.08	4840±90	^[40]
K2-133b [ru]		0.117	3.0712	0.033		transit	245.3±0.7	0.46±0.01	3655±80	Host star also known as LP 358–499, 4 planets in system^[41]
K2-133c [ru]		0.132	4.8682	0.045		transit	245.3±0.7	0.46±0.01	3655±80	Host star also known as LP 358–499, 4 planets in system^[41]
K2-133d [ru]		0.180	11.0234	0.077		transit	245.3±0.7	0.46±0.01	3655±80	Host star also known as LP 358–499, 4 planets in system^[41]
K2-135b		0.156	1.208957	0.020	1043.5	transit	98.8	0.66	4255	^[42]
K2-135c		0.121	3.64802	0.042	721.9	transit	98.8	0.66	4255	^[42]
K2-135d		0.187	6.20141	0.060	604.9	transit	98.8	0.66	4255	^[42]
K2-136b		0.0883	7.975292		553	transit		0.74	4499	^[43]
K2-136c	0.057±0.006	0.260	17.307137	0.11728	425	transit		0.74	4499	^[43]^[44]
K2-136d		0.129	25.575065		373	transit		0.74	4499	^[43]
K2-137b	0.5	0.079	0.179715	0.0058	1471	transit		0.46	3492	^[45]
K2-139b	0.387	0.808	28.38236	0.179	565	transit	496	1.8	5340	^[46]
K2-140b	0.211	1.093	6.56918	0.0687	957	transit	1110	1.00	5705	^[47]
K2-141b	0.0160±0.0013	0.135±0.004	0.2803226	0.00716^+0.00055 _−0.00065	2039⁺⁸⁷ ₋₄₈	transit	202.16±0.54	0.708±0.028	4599±79	^[48]^[49]
K2-146b		0.196±0.021	2.644646	0.0266±0.0010		transit	259.2±1.5	0.358±0.042	3385±70	^[38]
K2-147b		0.123^+0.015 _−0.013	0.961917	0.0159±0.0005		transit	296.10±0.90	0.583±0.059	3672±70	^[38] Also called EPIC 213715787^[50]
K2-148b		0.119^+0.017 _−0.016	4.38395±0.00080	0.0454±0.0014		transit	407.4±2.0	0.650±0.061	4079±70	^[38]
K2-148c		0.154^+0.021 _−0.019	6.92260±0.00070	0.0616±0.0019		transit	407.4±2.0	0.650±0.061	4079±70	^[38]
K2-148d		0.146^+0.021 _−0.019	9.7579±0.0010	0.0774±0.0024		transit	407.4±2.0	0.650±0.061	4079±70	^[38]
K2-149b		0.146^+0.018 _−0.016	11.3320±0.0013	0.0830±0.0027		transit	404.8±1.8	0.595±0.059	3745±70	^[38]
K2-150b		0.178^+0.024 _−0.019	10.59357±0.00084	0.0727±0.0027		transit	335.2±2.6	0.457±0.051	3499±70	^[38]
K2-151b		0.120^+0.014 _−0.012	3.835592	0.0365±0.0014		transit	227.07±0.49	0.440±0.050	3585±70	^[38]
K2-152b		0.204^+0.022 _−0.021	32.6527±0.0035	0.1716±0.0012	337±3	transit	354.8±1.3	0.63±0.01	4044⁺³⁴ ₋₃₅	^[38]
K2-153b		0.178^+0.019 _−0.016	7.51554	0.0614±0.0004	497±6	transit	468.7±3.0	0.55±0.01	3845±37	^[38]
K2-154b		0.178^+0.019 _−0.010	3.67635	0.0405±0.0003	715⁺⁹ ₋₈	transit	423.5±1.5	0.65^+0.02 _−0.01	4097⁺⁴⁰ ₋₄₅	^[38]
K2-154c		0.185^+0.016 _−0.012	7.95478	0.0677±0.0005	552±7	transit	423.5±1.5	0.65^+0.02 _−0.01	4097⁺⁴⁰ ₋₄₅	^[38]
KELT-9b	2.88	1.891	1.4811235	0.03462	4050	transit	615.5	2.52	10170	Hottest confirmed exoplanet^[51]
KELT-18b	1.18	1.570	2.8717518	0.04550	2085	transit		1.52	6670	^[52]
KELT-19Ab	<4.07	1.91	4.6117093	0.0637	1935	transit	950	1.62	7500	^[53]
KELT-20b		1.741	3.4741085	0.0542	2262	transit	455.6	1.76	8720	^[54] Also known as MASCARA-2b^[55]
KELT-21b	3.91⁺⁰ _−3.91	1.586^+0.039 _−0.040	3.6127647	0.05224^+0.00035 _−0.00034	2051⁺²⁹ ₋₃₀	transit	1557±21	1.458^+0.029 _−0.028	7598⁺⁸¹ ₋₈₄	^[56]
Kepler-19d	0.0708		62.95			radial vel.	6910	0.94	5541	^[57]
Kepler-80g		0.101	14.64558		418	transit	1160	0.73	4540	^[58]
Kepler-90i		0.118	14.44912		709	transit	2540	1.2	6080	^[58]
Kepler-150 f		0.325	637.2093	1.24		transit	2980±50		5560	^[59]
Kepler-1649b		0.0964	8.689090	0.0514		transit		0.22	3240	^[60]
Kepler-1650b		0.0856	1.53818001			transit	393	0.33	3410	^[61]
Kepler-1651b		0.164	9.87863917			transit	226	0.52	3713	^[61]
Kepler-1652b		0.143	38.09722	0.1654	268	transit	822	0.40	3638	^[62]
Kepler-1653b [it]		0.194	140.2524	0.4706	284	transit	2460	0.72	4807	^[62]
LHS 1140 b	0.0209	0.128	24.73712	0.0875	254	transit	40.7	0.18	3216	Potentially habitable exoplanet^[63]
MASCARA-1b	3.7	1.5	2.148780	0.043	2570	transit	615.5	1.72	7554	^[64]
MOA-2010-BLG-117Lb	0.54±0.10		2369⁺⁸³⁵ ₋₂₇₁₇	2.9^+1.6 _−0.6		microlensing	11400±1300	0.58±0.11	4000⁺⁴⁵⁰ ₋₃₅₀	^[65]
MOA-2012-BLG-006Lb	8.40			10.2		microlensing	17000	0.49		^[66]
MOA-2012-BLG-505Lb	0.02108			0.900		microlensing	23500	0.10		^[67]
MOA-2016-BLG-227Lb	2.8			1.67		microlensing	21000	0.29		^[68]
MXB 1658-298 b	23.7		760	1.613		timing		1.98		Circumbinary planet^[69]
NGTS-1b	0.812	1.33	2.647298	0.0326	790	transit	731	0.617	3916	Largest exoplanet in relation to its star^[70]
OGLE-2013-BLG-0132Lb	0.29			3.6		microlensing	13000	0.54		^[71]
OGLE-2013-BLG-1721Lb	0.64			2.6		microlensing	21000	0.46		^[71]
OGLE-2013-BLG-1761Lb	2.7^+2.5 _−1.5			1.8±0.5		microlensing	23000⁺³³⁰⁰ ₋₃₉₀₀	0.33^+0.32 _−0.19		^[72]
OGLE-2016-BLG-0263Lb	4.10			5.4		microlensing	21000	0.13		^[73]
OGLE-2016-BLG-0613(AB)b	4.18			6.40		microlensing	11100	0.72		^[74]
OGLE-2016-BLG-1190Lb	13.38		1224	2.17		microlensing	22100	0.88		Extremely massive; possiblebrown dwarf^[75]
OGLE-2016-BLG-1195Lb	0.031			2.62±0.28		microlensing	22000±2000	0.57±0.06		^[76]^[77]
OGLE-2017-BLG-0173Lb	0.0103^+0.0121 _−0.0063		4493⁺³⁰⁹⁰ ₋₇₀₅₅	3.9±1.6		microlensing	15700⁺⁴⁹⁰⁰ ₋₅₉₀₀	0.40^+0.39 _−0.23	3500⁺¹⁵⁰⁰ ₋₅₀₀	Atypical lensing event^[78] Not an OGLE-2011-BLG-0173Lb!
PSR J2322-2650 b	0.7949		0.322963997	0.0102		timing	750	1.4		^[79]
Qatar-6b	0.668	1.062	3.506195	0.0423		transit	330	0.822	5052	^[80]
Ross 128 b	0.00440		9.8658	0.0496	301	radial vel.	11.03	0.17	3192	^[81]
SAND978 b	2.18		511.21			radial vel.	2051.3	1.37	4200	^[82] Red giant host star, belonging toM67, is also known as NGC 2682 108
TAP 26 b	1.66		10.79	0.0968		radial vel.	480	1.04	4620	Host star also known as V1069 Tauri^[83]
Tau Ceti g	0.00551		20.00	0.133		radial vel.	12	0.78		^[84]
Tau Ceti h	0.00576		49.41	0.243		radial vel.	12	0.78		^[84]
TRAPPIST-1e	0.00195	0.082	6.099615	0.02817	251	transit	39	0.08	2559	Potentially habitable exoplanet^[85]
TRAPPIST-1f	0.00214	0.093	9.20669	0.0371	219	transit	39	0.08	2559	Potentially habitable exoplanet^[85]
TRAPPIST-1g	0.00422	0.101	12.35294	0.0451	199	transit	39	0.08	2559	Potentially habitable exoplanet^[85]
TRAPPIST-1h		0.067	20	0.063	168	transit	39	0.08	2559	^[85]
TYC 4282-605-1 b	10.78		101.54	0.422		radial vel.	2300	0.97	4300	^[86]
WASP-91b	1.34	1.03	2.798581	0.037	1160	transit	490	0.84	4920	^[87]
WASP-105b	1.8	0.96	7.87288	0.075	900	transit		0.89	5070	^[87]
WASP-107b	0.12	0.94	5.721490	0.055	770	transit		0.69	4430	^[87]
WASP-151b	0.31	1.13	4.533471	0.055	1290	transit	1570	1.01	5871	^[88] Host star also known as K2-134
WASP-153b	0.39	1.55	3.332609	0.048	1700	transit	1400	1.34	5914	^[88]
WASP-156b	0.128	0.51	3.836169	0.0453	970	transit	460	0.84	4910	^[88] Host star also known as TOI-465
WASP-167b		1.58	2.0219596	0.0365	2329	transit	1240	1.59	7000	Host star also known as KELT-13^[89]
YZ Ceti b	0.0024		1.96876	0.01634^+0.00035 _−0.00041		radial vel.	12.122±0.002	0.130±0.013	3056±60	^[90]
YZ Ceti c	0.00308		3.06008	0.02156^+0.00046 _−0.00054		radial vel.	12.122±0.002	0.130±0.013	3056±60	^[90]
YZ Ceti d	0.00359		4.65627	0.02851^+0.00061 _−0.00071		radial vel.	12.122±0.002	0.130±0.013	3056±60	^[90]

Specific exoplanet lists

[edit]

Lists of exoplanets

Lists of exoplanets by year of discovery

[edit]

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 (170)
List of exoplanets discovered in 2020 (247)
List of exoplanets discovered in 2021 (254)
List of exoplanets discovered in 2022 (313)
List of exoplanets discovered in 2023 (307)
List of exoplanets discovered in 2024 (285)
List of exoplanets discovered in 2025 (107)

References

[edit]

^"The Extrasolar Planets Encyclopaedia". 1995. Retrieved2015-11-09.
^Villaver, E; Niedzielski, A; Wolszczan, A; Nowak, G; Kowalik, K; Adamów, M; MacIejewski, G; Deka-Szymankiewicz, B; Maldonado, J (2017). "Tracking Advanced Planetary Systems (TAPAS) with HARPS-N".Astronomy & Astrophysics.606: A38.arXiv:1706.01278.Bibcode:2017A&A...606A..38V.doi:10.1051/0004-6361/201730471.S2CID 119228758.
^^a ^bBordé, P.; et al. (March 2020)."Transiting exoplanets from the CoRoT space mission XXIX. The hot Jupiters CoRoT-30 b and CoRoT-31 b".Astronomy & Astrophysics.635: A122.Bibcode:2020A&A...635A.122B.doi:10.1051/0004-6361/201732393.hdl:1887/3133644.Archived from the original on 2021-12-06. Retrieved2021-09-01.
^Boufleur, Rodrigo C.; Emilio, Marcelo; Janot-Pacheco, Eduardo; Andrade, Laerte; Ferraz-Mello, Sylvio; Do Nascimento Jr, José-Dias; de la Reza, Ramiro (2017), "A modified CoRoT detrend algorithm and the discovery of a new planetary companion",Monthly Notices of the Royal Astronomical Society,473:710–720,arXiv:1709.00351,doi:10.1093/mnras/stx2187
^^a ^b ^c ^d ^e ^f ^g ^h ⁱAstudillo-Defru, Nicola; Forveille, Thierry; Bonfils, Xavier; Ségransan, Damien; Bouchy, François; Delfosse, Xavier; et al. (2017)."The HARPS search for southern extra-solar planets. XLI. A dozen planets around the M dwarfs GJ 3138, GJ 3323, GJ 273, GJ 628, and GJ 3293".Astronomy and Astrophysics.602. A88.arXiv:1703.05386.Bibcode:2017A&A...602A..88A.doi:10.1051/0004-6361/201630153.S2CID 119418595.
^Suárez Mascareño, A.; et al. (2017)."HADES RV Programme with HARPS-N at TNG. V. A super-Earth on the inner edge of the habitable zone of the nearby M dwarf GJ 625".Astronomy and Astrophysics.605. A92.arXiv:1705.06537.Bibcode:2017A&A...605A..92S.doi:10.1051/0004-6361/201730957.S2CID 119003137.
^Trifonov, T.; et al. (2018), "The CARMENES search for exoplanets around M dwarfs",Astronomy & Astrophysics,609: A117,arXiv:1710.01595,Bibcode:2018A&A...609A.117T,doi:10.1051/0004-6361/201731442
^Perger, M.; et al. (2017), "HADES RV Programme with HARPS-N at TNG",Astronomy & Astrophysics,608: A63,arXiv:1709.06851,doi:10.1051/0004-6361/201731307,S2CID 260555995
^Zhou, G.; et al. (2017), "HAT-P-67b: An Extremely Low Density Saturn Transiting an F-subgiant Confirmed via Doppler Tomography",The Astronomical Journal,153 (5): 211,arXiv:1702.00106,Bibcode:2017AJ....153..211Z,doi:10.3847/1538-3881/aa674a,S2CID 119491990
^Bayliss, D.; Hartman, J. D.; Zhou, G.; Bakos, G. Á.; Vanderburg, A.; Bento, J.; Mancini, L.; Ciceri, S.; Brahm, R.; Jordán, A.; Espinoza, N.; Rabus, M.; Tan, T. G.; Penev, K.; Bhatti, W.; De Val-Borro, M.; Suc, V.; Csubry, Z.; Henning, Th.; Sarkis, P.; Lázár, J.; Papp, I.; Sári, P. (2017), "HATS-36b and 24 Other Transiting/Eclipsing Systems from the HATSouth-K2 Campaign 7 Program",The Astronomical Journal,155 (3): 119,arXiv:1706.03858,doi:10.3847/1538-3881/aaa8e6,S2CID 119383417
^^a ^b ^c ^dBrahm, R.; Hartman, J. D.; Jordán, A.; Bakos, G. Á.; Espinoza, N.; Rabus, M.; Bhatti, W.; Penev, K.; Sarkis, P.; Suc, V.; Csubry, Z.; Bayliss, D.; Bento, J.; Zhou, G.; Mancini, L.; Henning, T.; Ciceri, S.; Val-Borro, M. de; Shectman, S.; Crane, J. D.; Arriagada, P.; Butler, P.; Teske, J.; Thompson, I.; Osip, D.; Díaz, M.; Schmidt, B.; Lázár, J.; Papp, I.; Sári, P. (2017), "HATS-43b, HATS-44b, HATS-45b, and HATS-46b: Four Short-period Transiting Giant Planets in the Neptune–Jupiter Mass Range",The Astronomical Journal,155 (3): 112,arXiv:1707.07093,doi:10.3847/1538-3881/aaa898,S2CID 119070247
^^a ^b ^c ^dHenning, Th.; Mancini, L.; Sarkis, P.; Bakos, G. Á.; Hartman, J. D.; Bayliss, D.; Bento, J.; Bhatti, W.; Brahm, R.; Ciceri, S.; Csubry, Z.; Val-Borro, M. de; Espinoza, N.; Fulton, B. J.; Howard, A. W.; Isaacson, H. T.; Jordán, A.; Marcy, G. W.; Penev, K.; Rabus, M.; Suc, V.; Tan, T. G.; Tinney, C. G.; Wright, D. J.; Zhou, G.; Durkan, S.; Lazar, J.; Papp, I.; Sari, P. (2018), "HATS-50b through HATS-53b: Four Transiting Hot Jupiters Orbiting G-type Stars Discovered by the HATSouth Survey",The Astronomical Journal,155 (2): 79,arXiv:1712.04324,Bibcode:2018AJ....155...79H,doi:10.3847/1538-3881/aaa254,S2CID 119516821
^Christiansen, Jessie L.; Vanderburg, Andrew; et al. (September 2017), "Three's Company: An Additional Non-transiting Super-Earth in the Bright HD 3167 System, and Masses for All Three Planets",The Astronomical Journal,154 (3): 17,arXiv:1706.01892,Bibcode:2017AJ....154..122C,doi:10.3847/1538-3881/aa832d,S2CID 54196245, 122.
^^a ^b ^cRey, J.; Hébrard, G.; Bouchy, F.; Bourrier, V.; Boisse, I.; Santos, N. C.; Arnold, L.; Astudillo-Defru, N.; Bonfils, X.; Borgniet, S.; Courcol, B.; Deleuil, M.; Delfosse, X.; Demangeon, O.; Díaz, R. F.; Ehrenreich, D.; Forveille, T.; Marmier, M.; Moutou, C.; Pepe, F.; Santerne, A.; Sahlmann, J.; Ségransan, D.; Udry, S.; Wilson, P. A. (2017), "The SOPHIE search for northern extrasolar planets",Astronomy & Astrophysics,601: A9,arXiv:1702.06393,doi:10.1051/0004-6361/201630089,S2CID 119080874
^^a ^bUdry, S.; Dumusque, X.; Lovis, C.; Segransan, D.; Diaz, R. F.; Benz, W.; Bouchy, F.; Coffinet, A.; Lo Curto, G.; Mayor, M.; Mordasini, C.; Motalebi, F.; Pepe, F.; Queloz, D.; Santos, N. C.; Wyttenbach, A.; Alonso, R.; Collier Cameron, A.; Deleuil, M.; Figueira, P.; Gillon, M.; Moutou, C.; Pollacco, D.; Pompei, E. (2019), "The HARPS search for southern extra-solar planets. XLII. Eight HARPS multi-planet systems hosting 20 super-Earth and Neptune-mass companions",Astronomy & Astrophysics,A37: 622,arXiv:1705.05153,Bibcode:2019A&A...622A..37U,doi:10.1051/0004-6361/201731173,S2CID 119095511
^Feng, F.; Tuomi, M.; Jones, H.R.A. (September 2017). "Evidence for at least three planet candidates orbiting HD 20794".Astronomy and Astrophysics.605 (103): 11.arXiv:1705.05124.Bibcode:2017A&A...605A.103F.doi:10.1051/0004-6361/201730406.S2CID 119084078.
^^a ^bTrifonov, T.; Kürster, M.; Zechmeister, M.; Zakhozhay, O. V.; Reffert, S.; Lee, M. H.; Rodler, F.; Vogt, S. S.; Brems, S. S. (2017). "Three planets around HD 27894. A close-in pair with a 2:1 period ratio and an eccentric Jovian planet at 5.4 AU".Astronomy & Astrophysics.602: L8.arXiv:1706.00509.Bibcode:2017A&A...602L...8T.doi:10.1051/0004-6361/201731044.S2CID 119105619.
^^a ^b ^cJeong, G.; Lee, B.-C.; Han, I.; Omiya, M.; Izumiura, H.; Sato, B.; Harakawa, H.; Kambe, E.; Mkrtichian, D. (2017), "Detection of planet candidates around K giants. HD 40956, HD 111591, and HD 113996",Astronomy & Astrophysics,610: A3,arXiv:1711.07173,doi:10.1051/0004-6361/201629185,S2CID 119209663
^^a ^bGillon, M.; Demory, B.-O.; Lovis, C.; Deming, D.; Ehrenreich, D.; Lo Curto, G.; Mayor, M.; Pepe, F.; Queloz, D.; Seager, S.; Ségransan, D.; Udry, S. (2017), "TheSpitzersearch for the transits of HARPS low-mass planets",Astronomy & Astrophysics,601: A117,arXiv:1701.01303,Bibcode:2017A&A...601A.117G,doi:10.1051/0004-6361/201629270,S2CID 86862862
^Wittenmyer, Robert A.; Jones, M. I.; Horner, Jonathan; Kane, Stephen R.; Marshall, J. P.; Mustill, A. J.; Jenkins, J. S.; Rojas, P. A. Pena; Zhao, Jinglin; Villaver, Eva; Butler, R. P.; Clark, Jake (2017), "The Pan-Pacific Planet Search. VII. The Most Eccentric Planet Orbiting a Giant Star",The Astronomical Journal,154 (6): 274,arXiv:1711.05378,Bibcode:2017AJ....154..274W,doi:10.3847/1538-3881/aa9894,S2CID 55417878
^Bergmann, C.; Jones, M. I.; Zhao, J.; Mustill, A. J.; Brahm, R.; Torres, P.; Wittenmyer, R. A.; Gunn, F.; Pollard, K. R.; Zapata, A.; Vanzi, L.; Wang, Songhu (2021), "HD 76920 b pinned down: A detailed analysis of the most eccentric planetary system around an evolved star",Publications of the Astronomical Society of Australia,38,arXiv:2102.08902,Bibcode:2021PASA...38...19B,doi:10.1017/pasa.2021.8,S2CID 231942350
^Jiang, Chen; et al. (2023), "TESS Asteroseismic Analysis of HD 76920: The Giant Star Hosting an Extremely Eccentric Exoplanet",The Astrophysical Journal,945 (1): 20,arXiv:2302.01102,Bibcode:2023ApJ...945...20J,doi:10.3847/1538-4357/acb8ac
^Unger, N.; et al. (2021), "The HARPS search for southern extra-solar planets",Astronomy & Astrophysics,654: A104,arXiv:2108.10198,Bibcode:2021A&A...654A.104U,doi:10.1051/0004-6361/202141351,S2CID 239033129
^^a ^bFerraz, Alvaro; Kochetov, Evgenii (2017),A Multi-Planet System Transiting the V = 9 Rapidly Rotating F-Star HD 106315,arXiv:1701.03808
^Reiners, A.; et al. (2017), "The CARMENES search for exoplanets around M dwarfs",Astronomy & Astrophysics,609: L5,arXiv:1712.05797,doi:10.1051/0004-6361/201732165,S2CID 55661984
^^a ^bSuárez Mascareño, A.; González Hernández, J. I.; Rebolo, R.; Velasco, S.; Toledo-Padrón, B.; Udry, S.; Motalebi, F.; Ségrasan, D.; Wyttenbach, A.; Mayor, M.; Pepe, F.; Lovis, C.; Santos, N. C.; Figueira, P.; Esposito, M. (2018), "The RoPES project with HARPS and HARPS-N",Astronomy & Astrophysics,612: A41,arXiv:1712.01046,doi:10.1051/0004-6361/201732042,S2CID 118989904
^Feng, F.; Tuomi, M.; Jones, H. R. A. (2017), "Agatha: Disentangling periodic signals from correlated noise in a periodogram framework",Monthly Notices of the Royal Astronomical Society,470 (4):4794–4814,arXiv:1705.03089,doi:10.1093/mnras/stx1126
^Yılmaz, M.; Sato, B.; Bikmaev, I.; Selam, S. O.; Izumiura, H.; Keskin, V.; Kambe, E.; Melnikov, S. S.; Galeev, A.; Özavcı, İ.; Irtuganov, E. N.; Zhuchkov, R. Ya. (2017), "A Jupiter-mass planet around the K0 giant HD 208897",Astronomy & Astrophysics,608: A14,arXiv:1708.01895,Bibcode:2017A&A...608A..14Y,doi:10.1051/0004-6361/201731184,S2CID 118863243
^Chauvin, G.; et al. (2017), "Discovery of a warm, dusty giant planet around HIP 65426",Astronomy & Astrophysics,605: L9,arXiv:1707.01413,Bibcode:2017A&A...605L...9C,doi:10.1051/0004-6361/201731152,S2CID 102344893
^"HIP 65426 b - Exoplanet-catalog".Exoplanet Exploration: Planets Beyond our Solar System. Retrieved2023-12-03.
^Cloutier, R.; Astudillo-Defru, N.; Doyon, R.; Bonfils, X.; Almenara, J.-M.; Benneke, B.; Bouchy, F.; Delfosse, X.; Ehrenreich, D.; Forveille, T.; Lovis, C.; Mayor, M.; Menou, K.; Murgas, F.; Pepe, F.; Rowe, J.; Santos, N. C.; Udry, S.; Wünsche, A. (2017), "Characterization of the K2-18 multi-planetary system with HARPS",Astronomy & Astrophysics,608: A35,arXiv:1707.04292,Bibcode:2017A&A...608A..35C,doi:10.1051/0004-6361/201731558,S2CID 118955175
^Narita, Norio; Hirano, Teruyuki; Fukui, Akihiko; Hori, Yasunori; Dai, Fei; Yu, Liang; Livingston, John; Ryu, Tsuguru; Nowak, Grzegorz; Kuzuhara, Masayuki; Sato, Bun'ei; Takeda, Yoichi; Albrecht, Simon; Kudo, Tomoyuki; Kusakabe, Nobuhiko; Palle, Enric; Ribas, Ignasi; Tamura, Motohide; Van Eylen, Vincent; Winn, Joshua N. (2017), "The K2-ESPRINT project. VI. K2-105 b, a hot Neptune around a metal-rich G-dwarf",Publications of the Astronomical Society of Japan,69 (2),arXiv:1701.01294,doi:10.1093/pasj/psx002
^^a ^bGuenther, E. W.; et al. (2017), "K2-106, a system containing a metal-rich planet and a planet of lower density",Astronomy & Astrophysics,608: A93,arXiv:1705.04163,Bibcode:2017A&A...608A..93G,doi:10.1051/0004-6361/201730885,S2CID 55692535
^Petigura, Erik A.; Sinukoff, Evan; Lopez, Eric D.; Crossfield, Ian J. M.; Howard, Andrew W.; Brewer, John M.; Fulton, Benjamin J.; Isaacson, Howard T.; Ciardi, David R.; Howell, Steve B.; Everett, Mark E.; Horch, Elliott P.; Hirsch, Lea A.; Weiss, Lauren M.; Schlieder, Joshua E. (2017), "Four Sub-Saturns with Dissimilar Densities: Windows into Planetary Cores and Envelopes",The Astronomical Journal,153 (4): 142,arXiv:1702.00013,Bibcode:2017AJ....153..142P,doi:10.3847/1538-3881/aa5ea5,S2CID 599957
^Fridlund, Malcolm; et al. (2017), "K2-111 b − a short period super-Earth transiting a metal poor, evolved old star",Astronomy & Astrophysics,604: A16,arXiv:1704.08284,Bibcode:2017A&A...604A..16F,doi:10.1051/0004-6361/201730822,S2CID 39412906
^^a ^bShporer, Avi; Zhou, George; Fulton, Benjamin J.; Vanderburg, Andrew; Espinoza, Nestor; Collins, Karen; Ciardi, David; Bayliss, Daniel; Armstrong, James D.; Bento, Joao; Bouchy, Francois; Cochran, William D.; Cameron, Andrew Collier; Colón, Knicole; Crossfield, Ian; Dragomir, Diana; Howard, Andrew W.; Howell, Steve B.; Isaacson, Howard; Kielkopf, John F.; Murgas, Felipe; Sefako, Ramotholo; Sinukoff, Evan; Siverd, Robert; Udry, Stephane (2017), "K2-114b and K2-115b: Two Transiting Warm Jupiters",The Astronomical Journal,154 (5): 188,arXiv:1708.07128,Bibcode:2017AJ....154..188S,doi:10.3847/1538-3881/aa8bb9,S2CID 468318
^^a ^b ^c ^d ^e ^f ^g ^h ⁱ ^j ^k ^l ^m ⁿDressing, Courtney D.; Vanderburg, Andrew; Schlieder, Joshua E.; Crossfield, Ian J. M.; Knutson, Heather A.; Newton, Elisabeth R.; Ciardi, David R.; Fulton, Benjamin J.; Gonzales, Erica J.; Howard, Andrew W.; Isaacson, Howard; Livingston, John; Petigura, Erik A.; Sinukoff, Evan; Everett, Mark; Horch, Elliott; Howell, Steve B. (2017), "Characterizing K2 Candidate Planetary Systems Orbiting Low-mass Stars. II. Planetary Systems Observed During Campaigns 1–7",The Astronomical Journal,154 (5): 207,arXiv:1703.07416,Bibcode:2017AJ....154..207D,doi:10.3847/1538-3881/aa89f2,S2CID 13419148
^^a ^b ^c ^d ^e ^f ^g ^h ⁱ ^j ^k ^l ^m ⁿ ^o ^pHirano, Teruyuki; et al. (2017), "Exoplanets around Low-mass Stars Unveiled byK2",The Astronomical Journal,155 (3): 127,arXiv:1710.03239,doi:10.3847/1538-3881/aaa9c1,S2CID 54590874
^Dai, Fei; et al. (2017), "The Discovery and Mass Measurement of a New Ultra-short-period Planet: K2-131b",The Astronomical Journal,154 (6): 226,arXiv:1710.00076,Bibcode:2017AJ....154..226D,doi:10.3847/1538-3881/aa9065,S2CID 55262711
^Grunblatt, Samuel K.; Huber, Daniel; Gaidos, Eric; Lopez, Eric D.; Howard, Andrew W.; Isaacson, Howard T.; Sinukoff, Evan; Vanderburg, Andrew; Nofi, Larissa; Yu, Jie; North, Thomas S. H.; Chaplin, William; Foreman-Mackey, Daniel; Petigura, Erik; Ansdell, Megan; Weiss, Lauren; Fulton, Benjamin; Lin, Douglas N. C. (2017), "Seeing Double withK2: Testing Re-inflation with Two Remarkably Similar Planets around Red Giant Branch Stars",The Astronomical Journal,154 (6): 254,arXiv:1706.05865,Bibcode:2017AJ....154..254G,doi:10.3847/1538-3881/aa932d,S2CID 55959801
^^a ^b ^cWells, R.; Poppenhaeger, K.; Watson, C. A. (2017), "Three small transiting planets around the M-dwarf host star LP 358-499",Monthly Notices of the Royal Astronomical Society: Letters,473:L131 –L135,arXiv:1709.01025,doi:10.1093/mnrasl/slx171
^^a ^b ^cRodriguez, Joseph E; Vanderburg, Andrew; Eastman, Jason D; Mann, Andrew W; Crossfield, Ian J. M; Ciardi, David R; Latham, David W; Quinn, Samuel N (2018)."A System of Three Super Earths Transiting the Late K-Dwarf GJ 9827 at 30 pc".The Astronomical Journal.155 (2): 72.arXiv:1709.01957.Bibcode:2018AJ....155...72R.doi:10.3847/1538-3881/aaa292.S2CID 55459523.
^^a ^b ^cMann, Andrew W.; Vanderburg, Andrew; Rizzuto, Aaron C.; Kraus, Adam L.; Berlind, Perry; Bieryla, Allyson; Calkins, Michael L.; Esquerdo, Gilbert A.; Latham, David W.; Mace, Gregory N.; Morris, Nathan R.; Quinn, Samuel N.; Sokal, Kimberly R.; Stefanik, Robert P. (2017), "Zodiacal Exoplanets in Time (ZEIT). VI. A Three-planet System in the Hyades Cluster Including an Earth-sized Planet",The Astronomical Journal,155: 4,arXiv:1709.10328,doi:10.3847/1538-3881/aa9791,S2CID 119216533
^Mayo, Andrew W.; et al. (2023), "Hyades Member K2-136c: The Smallest Planet in an Open Cluster with a Precisely Measured Mass",The Astronomical Journal,165 (6): 235,arXiv:2304.02779,Bibcode:2023AJ....165..235M,doi:10.3847/1538-3881/acca1c
^Smith, A M S.; et al. (2018), "K2-137 b: An Earth-sized planet in a 4.3-h orbit around an M-dwarf",Monthly Notices of the Royal Astronomical Society,474 (4):5523–5533,arXiv:1707.04549,doi:10.1093/mnras/stx2891
^Barragán, O.; Gandolfi, D.; Smith, A M S.; Deeg, H. J.; Fridlund, M C V.; Persson, C. M.; Donati, P.; Endl, M.; Csizmadia, Sz; Grziwa, S.; Nespral, D.; Hatzes, A. P.; Cochran, W. D.; Fossati, L.; Brems, S. S.; Cabrera, J.; Cusano, F.; Eigmüller, Ph; Eiroa, C.; Erikson, A.; Guenther, E.; Korth, J.; Lorenzo-Oliveira, D.; Mancini, L.; Pätzold, M.; Prieto-Arranz, J.; Rauer, H.; Rebollido, I.; Saario, J.; Zakhozhay, O. V. (2017), "K2-139 b: A low-mass warm Jupiter on a 29-d orbit transiting an active K0 V star",Monthly Notices of the Royal Astronomical Society,475 (2):1765–1776,arXiv:1702.00691,doi:10.1093/mnras/stx3207
^Giles, H A C.; Bayliss, D.; Espinoza, N.; Brahm, R.; Blanco-Cuaresma, S.; Shporer, A.; Armstrong, D.; Lovis, C.; Udry, S.; Bouchy, F.; Marmier, M.; Jordán, A.; Bento, J.; Cameron, A Collier; Sefako, R.; Cochran, W. D.; Rojas, F.; Rabus, M.; Jenkins, J. S.; Jones, M.; Pantoja, B.; Soto, M.;Jensen-Clem, R.; Duev, D. A.; Salama, M.; Riddle, R.; Baranec, C.; Law, N. M. (2017), "K2-140b – an eccentric 6.57 d transiting hot Jupiter in Virgo",Monthly Notices of the Royal Astronomical Society,475 (2):1809–1818,arXiv:1706.06865,doi:10.1093/mnras/stx3300
^Okoli, Chiamaka (2017),K2-141 b: A 5-M⊕ super-Earth transiting a K7 V star every 6.7 hours,arXiv:1711.05277
^Malavolta, Luca; et al. (2018)."An Ultra-short Period Rocky Super-Earth with a Secondary Eclipse and a Neptune-like Companion around K2-141".The Astronomical Journal.155 (3). 107.arXiv:1801.03502.Bibcode:2018AJ....155..107M.doi:10.3847/1538-3881/aaa5b5.S2CID 54869937.
^Adams, Elisabeth R.; et al. (2020)."Ultra Short Period Planets in K2 III: Neighbors are Common with 13 New Multi-Planet Systems and 10 Newly Validated Planets in Campaigns 0-8, 10".The Planetary Science Journal.2 (4): 152.arXiv:2011.11698.Bibcode:2021PSJ.....2..152A.doi:10.3847/PSJ/ac0ea0.S2CID 227151802.
^Gaudi, B. Scott; et al. (2017), "A giant planet undergoing extreme-ultraviolet irradiation by its hot massive-star host",Nature,546 (7659):514–518,arXiv:1706.06723,Bibcode:2017Natur.546..514G,doi:10.1038/nature22392,PMID 28582774,S2CID 205256410
^McLeod, Kim K.; Rodriguez, Joseph E.; Oelkers, Ryan J.; Collins, Karen A.; Bieryla, Allyson; Fulton, Benjamin J.; Stassun, Keivan G.; Gaudi, B. Scott; Penev, Kaloyan; Stevens, Daniel J.; et al. (1 June 2017)."KELT-18b: Puffy Planet, Hot Host, Probably Perturbed".The Astronomical Journal.153 (6): 263.arXiv:1702.01657.Bibcode:2017AJ....153..263M.doi:10.3847/1538-3881/aa6d5d.ISSN 0004-6256.S2CID 54667386.
^Siverd, Robert J.; et al. (2017), "KELT-19Ab: AP~ 4.6-day Hot Jupiter Transiting a Likely Am Star with a Distant Stellar Companion",The Astronomical Journal,155: 35,arXiv:1709.07010,doi:10.3847/1538-3881/aa9e4d,S2CID 54002227
^Talens, G. J. J; et al. (2018). "MASCARA-2 b: A hot Jupiter transiting a m_V = 7.6 A-star".Astronomy & Astrophysics.A57: 612.arXiv:1707.01500.Bibcode:2018A&A...612A..57T.doi:10.1051/0004-6361/201731512.S2CID 119422884.
^Rainer, M.; et al. (2021), "The GAPS programme at TNG",Astronomy & Astrophysics,649: A29,arXiv:2103.10395,doi:10.1051/0004-6361/202039247,S2CID 232270019
^Johnson, Marshall C; Rodriguez, Joseph E; Zhou, George; Gonzales, Erica J; Cargile, Phillip A; Crepp, Justin R; Penev, Kaloyan; Stassun, Keivan G; Gaudi, B. Scott; Colón, Knicole D; Stevens, Daniel J; Strassmeier, Klaus G; Ilyin, Ilya; Collins, Karen A; Kielkopf, John F; Oberst, Thomas E; Maritch, Luke; Reed, Phillip A; Gregorio, Joao; Bozza, Valerio; Novati, Sebastiano Calchi; d'Ago, Giuseppe; Scarpetta, Gaetano; Zambelli, Roberto; Latham, David W; Bieryla, Allyson; Cochran, William D; Endl, Michael; Tayar, Jamie; et al. (2018)."KELT-21b: A Hot Jupiter Transiting the Rapidly Rotating Metal-poor Late-A Primary of a Likely Hierarchical Triple System".The Astronomical Journal.155 (2): 100.arXiv:1712.03241.Bibcode:2018AJ....155..100J.doi:10.3847/1538-3881/aaa5af.S2CID 73559090.
^Malavolta, Luca; et al. (2017), "The Kepler-19 System: A Thick-envelope Super-Earth with Two Neptune-mass Companions Characterized Using Radial Velocities and Transit Timing Variations",The Astronomical Journal,153 (5): 224,arXiv:1703.06885,Bibcode:2017AJ....153..224M,doi:10.3847/1538-3881/aa6897,S2CID 29845787
^^a ^bShallue, C. J.; Vanderburg, A. (2017)."Identifying Exoplanets With Deep Learning: A Five Planet Resonant Chain Around Kepler-80 And An Eighth Planet Around Kepler-90"(PDF).The Astrophysical Journal.155 (2): 94.arXiv:1712.05044.Bibcode:2018AJ....155...94S.doi:10.3847/1538-3881/aa9e09.S2CID 4535051. Retrieved2017-12-15.
^Schmitt, Joseph R.; Jenkins, Jon M.; Fischer, Debra A. (2017), "A Search for Lost Planets in theKeplerMulti-planet Systems and the Discovery of the Long-period, Neptune-sized Exoplanet Kepler-150 F",The Astronomical Journal,153 (4): 180,arXiv:1703.09229,Bibcode:2017AJ....153..180S,doi:10.3847/1538-3881/aa62ad,PMC 5783551,PMID 29375142,S2CID 4520222
^Angelo, Isabel; Rowe, Jason F.; Howell, Steve B.; Quintana, Elisa V.; Still, Martin; Mann, Andrew W.; Burningham, Ben; Barclay, Thomas; Ciardi, David R.; Huber, Daniel; Kane, Stephen R. (2017), "Kepler-1649b: An Exo-Venus in the Solar Neighborhood",The Astronomical Journal,153 (4): 162,arXiv:1704.03136,Bibcode:2017AJ....153..162A,doi:10.3847/1538-3881/aa615f,S2CID 29545487
^^a ^bMann, Andrew W.; Dupuy, Trent; Muirhead, Philip S.; Johnson, Marshall C.; Liu, Michael C.; Ansdell, Megan; Dalba, Paul A.; Swift, Jonathan J.; Hadden, Sam (2017), "The Gold Standard: Accurate Stellar and Planetary Parameters for EightKeplerM Dwarf Systems Enabled by Parallaxes",The Astronomical Journal,153 (6): 267,arXiv:1705.01545,Bibcode:2017AJ....153..267M,doi:10.3847/1538-3881/aa7140,S2CID 119325474
^^a ^bTorres, Guillermo; Kane, Stephen R.; Rowe, Jason F.; Batalha, Natalie M.; Henze, Christopher E.; Ciardi, David R.; Barclay, Thomas; Borucki, William J.; Buchhave, Lars A.; Crepp, Justin R.; Everett, Mark E.; Horch, Elliott P.; Howard, Andrew W.; Howell, Steve B.; Isaacson, Howard T.; Jenkins, Jon M.; Latham, David W.; Petigura, Erik A.; Quintana, Elisa V. (2017), "Validation of SmallKeplerTransiting Planet Candidates in or near the Habitable Zone",The Astronomical Journal,154 (6): 264,arXiv:1711.01267,Bibcode:2017AJ....154..264T,doi:10.3847/1538-3881/aa984b,S2CID 73678176
^Ferraz-Mello, S.; Gomes, G. O. (2020)."Tidal evolution of exoplanetary systems hosting potentially habitable exoplanets. The cases of LHS-1140 b-c and K2-18 b-c".Monthly Notices of the Royal Astronomical Society.494 (4):5082–5090.arXiv:2005.10318.Bibcode:2020MNRAS.494.5082G.doi:10.1093/mnras/staa1110.
^Talens, G. J. J; et al. (2017). "MASCARA-1 b. A hot Jupiter transiting a bright m_V = 8.3 A-star in a misaligned orbit".Astronomy & Astrophysics.606: A73.arXiv:1707.04262.Bibcode:2017A&A...606A..73T.doi:10.1051/0004-6361/201731282.S2CID 119259578.
^Bennett, D. P.; et al. (2017), "The First Planetary Microlensing Event with Two Microlensed Source Stars",The Astronomical Journal,155 (3): 141,arXiv:1707.09667,doi:10.3847/1538-3881/aaadfa
^Poleski, R.; et al. (2017), "A companion on the planet/Brown dwarf mass boundary on a wide orbit discovered by gravitational microlensing",Astronomy & Astrophysics,604: A103,arXiv:1704.01121,Bibcode:2017A&A...604A.103P,doi:10.1051/0004-6361/201730928,S2CID 56306676
^Nagakane, M.; Sumi, T.; Koshimoto, N.; Bennett, D. P.; Bond, I. A.; Rattenbury, N.; Suzuki, D.; Abe, F.; Asakura, Y.; Barry, R.; Bhattacharya, A.; Donachie, M.; Fukui, A.; Hirao, Y.; Itow, Y.; Li, M. C. A.; Ling, C. H.; Masuda, K.; Matsubara, Y.; Matsuo, T.; Muraki, Y.; Ohnishi, K.; Ranc, C.; Saito, To.; Sharan, A.; Shibai, H.; Sullivan, D. J.; Tristram, P. J.; Yamada, T.; Yonehara, A. (2017), "MOA-2012-BLG-505Lb: A Super-Earth-mass Planet That Probably Resides in the Galactic Bulge",The Astronomical Journal,154 (1): 35,arXiv:1703.10769,Bibcode:2017AJ....154...35N,doi:10.3847/1538-3881/aa74b2,S2CID 119077625
^Koshimoto, N.; et al. (2017), "MOA-2016-BLG-227Lb: A Massive Planet Characterized by Combining Light-curve Analysis and Keck AO Imaging",The Astronomical Journal,154 (1): 3,arXiv:1704.01724,Bibcode:2017AJ....154....3K,doi:10.3847/1538-3881/aa72e0,S2CID 39514486
^Jain, Chetana; Paul, Biswajit; Sharma, Rahul; Jaleel, Abdul; Dutta, Anjan (2017), "Indication of a massive circumbinary planet orbiting the low-mass X-ray binary MXB 1658−298",Monthly Notices of the Royal Astronomical Society: Letters,468:L118 –L122,arXiv:1703.04433,Bibcode:2017MNRAS.468L.118J,doi:10.1093/mnrasl/slx039
^Bayliss, Danile; et al. (31 October 2017)."NGTS-1b: A hot Jupiter transiting an M-dwarf".Monthly Notices of the Royal Astronomical Society.475 (4):4467–4475.arXiv:1710.11099.Bibcode:2018MNRAS.475.4467B.doi:10.1093/mnras/stx2778.S2CID 39357327.
^^a ^bMróz, Przemek; et al. (2017), "OGLE-2013-BLG-0132Lb and OGLE-2013-BLG-1721Lb: Two Saturn-mass Planets Discovered around M-dwarfs",The Astronomical Journal,154 (5): 205,arXiv:1705.01058,Bibcode:2017AJ....154..205M,doi:10.3847/1538-3881/aa8f98,S2CID 119093055
^Hirao, Y.; et al. (2017), "OGLE-2013-BLG-1761Lb: A Massive Planet around an M/K Dwarf",The Astronomical Journal,154 (1): 1,arXiv:1703.07623,Bibcode:2017AJ....154....1H,doi:10.3847/1538-3881/aa73da
^Han, C.; et al. (2017), "OGLE-2016-BLG-0263Lb: Microlensing Detection of a Very Low-mass Binary Companion through a Repeating Event Channel",The Astronomical Journal,154 (4): 133,arXiv:1708.02727,Bibcode:2017AJ....154..133H,doi:10.3847/1538-3881/aa859a,S2CID 56010958
^Han, C.; et al. (2017), "OGLE-2016-BLG-0613LABb: A Microlensing Planet in a Binary System",The Astronomical Journal,154 (6): 223,arXiv:1710.00924,Bibcode:2017AJ....154..223H,doi:10.3847/1538-3881/aa9179,S2CID 119012722
^Ryu, Y.-H.; et al. (27 October 2017)."OGLE-2016-BLG-1190Lb: First Spitzer Bulge Planet Lies Near the Planet/Brown-Dwarf Boundary".The Astronomical Journal.155: 40.arXiv:1710.09974.doi:10.3847/1538-3881/aa9be4.S2CID 54706921.
^Shvartzvald, Y; et al. (1 May 2017)."An Earth-mass Planet in a 1 au Orbit around an Ultracool Dwarf".The Astrophysical Journal Letters.840 (L3): L3.arXiv:1703.08548.Bibcode:2017ApJ...840L...3S.doi:10.3847/2041-8213/aa6d09.hdl:10092/13689.S2CID 39292551.
^Vandorou, Aikaterini; Dang, Lisa; Bennett, David P.; Koshimoto, Naoki; Terry, Sean K.; Beaulieu, Jean-Phillipe; Alard, Christophe; Bhattacharya, Aparna; Blackman, Joshua W.; Bouchoutrouch-Ku, Tarik; Cole, Andrew A.; Cowan, Nicolas B.; Marquette, Jean-Baptiste; Ranc, Clément; Rektsini, Natalia (2023),OGLE-2016-BLG-1195Lb: A Sub-Neptune Beyond the Snow Line of an M-Dwarf Confirmed by Keck AO,arXiv:2302.01168
^Hwang, K.-H.; et al. (2017), "OGLE-2017-BLG-0173Lb: Low-mass-ratio Planet in a "Hollywood" Microlensing Event",The Astronomical Journal,155: 20,arXiv:1709.08476,doi:10.3847/1538-3881/aa992f
^Spiewak, R.; Bailes, M.; Barr, E. D.; Bhat, N D R.; Burgay, M.; Cameron, A. D.; Champion, D. J.; Flynn, C M L.; Jameson, A.; Johnston, S.; Keith, M. J.; Kramer, M.; Kulkarni, S. R.; Levin, L.; Lyne, A. G.; Morello, V.; Ng, C.; Possenti, A.; Ravi, V.; Stappers, B. W.; Van Straten, W.; Tiburzi, C. (2017), "PSR J2322−2650 – a low-luminosity millisecond pulsar with a planetary-mass companion",Monthly Notices of the Royal Astronomical Society,475:469–477,arXiv:1712.04445,doi:10.1093/mnras/stx3157
^Alsubai, Khalid; Tsvetanov, Zlatan I.; Latham, David W.; Bieryla, Allyson; Esquerdo, Gilbert A.; Mislis, Dimitris; Pyrzas, Stylianos; Foxell, Emma; McCormac, James; Baranec, Christoph; Vilchez, Nicolas P. E.; West, Richard; Esamdin, Ali; Dang, Zhenwei; Dalee, Hani M.; Al-Rajihi, Amani A.; Al-Harbi, Abeer Kh. (2017), "Qatar Exoplanet Survey: Qatar-6b—A Grazing Transiting Hot Jupiter",The Astronomical Journal,155 (2): 52,arXiv:1712.03216,doi:10.3847/1538-3881/aaa000
^Bonfils, Xavier (2017). "A temperate exo-Earth around a quiet M dwarf at 3.4 parsecs".Astronomy and Astrophysics.613: A25.arXiv:1711.06177.Bibcode:2018A&A...613A..25B.doi:10.1051/0004-6361/201731973.S2CID 37148632.
^Brucalassi, A.; Koppenhoefer, J.; Saglia, R.; Pasquini, L.; Ruiz, M. T.; Bonifacio, P.; Bedin, L. R.; Libralato, M.; Biazzo, K.; Melo, C.; Lovis, C.; Randich, S. (2017), "Search for giant planets in M 67",Astronomy & Astrophysics,603: A85,arXiv:1703.04296,doi:10.1051/0004-6361/201527562,S2CID 119248679
^Yu, L.; Donati, J.-F.; Hébrard, E. M.; Moutou, C.; Malo, L.; Grankin, K.; Hussain, G.; Collier Cameron, A.; Vidotto, A. A.; Baruteau, C.; Alencar, S.H.P.; Bouvier, J.; Petit, P.; Takami, M.; Herczeg, G.; Gregory, S. G.; Jardine, M.; Morin, J.; Ménard, F.; the MaTYSSE collaboration (2017), "A hot Jupiter around the very active weak-line T Tauri star TAP 26",Monthly Notices of the Royal Astronomical Society stx009,arXiv:1701.01512,doi:10.1093/mnras/stx009
^^a ^bFeng, Fabo; et al. (2017)."Color Difference Makes a Difference: Four Planet Candidates around Tau Ceti".The Astronomical Journal.154 (4): 135.arXiv:1708.02051.Bibcode:2017AJ....154..135F.doi:10.3847/1538-3881/aa83b4.S2CID 53500995.
^^a ^b ^c ^dGillon, M.; Triaud, A. H. M. J.; Demory, B.-O.; et al. (February 2017)."Seven temperate terrestrial planets around the nearby ultracool dwarf star TRAPPIST-1"(PDF).Nature.542 (7642):456–460.arXiv:1703.01424.Bibcode:2017Natur.542..456G.doi:10.1038/nature21360.PMC 5330437.PMID 28230125.
^González-Álvarez, E.; et al. (2022), "The GAPS Programme with HARPS-N at TNG",Astronomy & Astrophysics,606: A51,arXiv:1706.06955,doi:10.1051/0004-6361/201731124,S2CID 119098853
^^a ^b ^cAnderson, D. R.; Collier Cameron, A.; Delrez, L.; Doyle, A. P.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Madhusudhan, N.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Triaud, A. H. M. J.; Turner, O. D.; Udry, S.; West, R. G. (2017), "The discoveries of WASP-91b, WASP-105b and WASP-107b: Two warm Jupiters and a planet in the transition region between ice giants and gas giants",Astronomy & Astrophysics,604: A110,arXiv:1701.03776,Bibcode:2017A&A...604A.110A,doi:10.1051/0004-6361/201730439,S2CID 58910823
^^a ^b ^cDemangeon, O. D. S.; et al. (2018), "The discovery of WASP-151b, WASP-153b, WASP-156b: Insights on giant planet migration and the upper boundary of the Neptunian desert",Astronomy & Astrophysics,610: A63,arXiv:1710.06321,Bibcode:2018A&A...610A..63D,doi:10.1051/0004-6361/201731735,S2CID 215776387
^Temple, L. Y.; et al. (2017), "WASP-167b/KELT-13b: Joint discovery of a hot Jupiter transiting a rapidly rotating F1V star",Monthly Notices of the Royal Astronomical Society,471 (3):2743–2752,arXiv:1704.07771,doi:10.1093/mnras/stx1729
^^a ^b ^cAstudillo-Defru, N.; Díaz, R. F.; Bonfils, X.; Almenara, J. M.; Delisle, J.-B.; Bouchy, F.; Delfosse, X.; Forveille, T.; Lovis, C.; Mayor, M.; Murgas, F.; Pepe, F.; Santos, N. C.; Ségransan, D.; Udry, S.; Wünsche, A. (2017), "The HARPS search for southern extra-solar planets",Astronomy & Astrophysics,605: L11,arXiv:1708.03336,doi:10.1051/0004-6361/201731581,S2CID 119393757

Exoplanets

Main topics

Sizes
and
types

Terrestrial	Carbon planet Catastrophically evaporating planet Coreless planet Desert planet Dwarf planet Hycean planet Ice planet Iron planet (Super-Mercury) Lava planet Ocean world Mega-Earth Steam world Sub-Earth Super-Earth
Gaseous	Cold Jupiter Eccentric Jupiter Mini-Neptune (Gas dwarf) Helium planet Hot Jupiter Hot Neptune Gas giant Ice giant Neptunian Jupiter analogue Super-Jupiter Super-Neptune Super-puff Ultra-hot Jupiter Ultra-hot Neptune Warm Jupiter
Other types	Blanet Brown dwarf Chthonian planet Circumbinary planet Circumtriple planet Disrupted planet Double planet Ecumenopolis Eyeball planet Giant planet Mesoplanet Planemo Planet/Brown dwarf boundary Planetesimal Protoplanet Pulsar planet Sub-brown dwarf Sub-Neptune Toroidal planet Ultra-cool dwarf Ultra-short period planet (USP)