Astronomy:List of exoplanets discovered in 2017

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This is a list of exoplanets discovered in 2017.

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

Name Mass (MJ) Radius (RJ) 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 34445 c 0.168 214.67 0.7181 radial vel. 146.8 1.07 5836 [18] Likely a false positive[19]
HD 34445 d 0.0970 117.87 0.4817 radial vel. 146.8 1.07 5836 [18] Likely a false positive[19]
HD 34445 e 0.0529 49.175 0.2687 radial vel. 146.8 1.07 5836 [18] Likely a false positive[19]
HD 34445 f 0.119 676.8 1.543 radial vel. 146.8 1.07 5836 [18] Likely a false positive[19]
HD 34445 g 0.38 5700 6.36 radial vel. 146.8 1.07 5836 [18] Likely a false positive[19]
HD 40956 b 2.7 578.6 1.4 radial vel. 385 2.00 4869 [20]
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 [21]
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 evolved red giant[22][23][24]
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 [21] Confirmed in 2021, renamed from HD 93385 d[25]
HD 106315 b 0.0255 0.207 9.55804 0.0905 1046 transit 358 1.08 6277 Host star also known as K2-109[26]
HD 106315 c 0.0560 0.385 21.05788 0.1533 804 transit 358 1.08 6277 Host star also known as K2-109[26]
HD 111591 b 4.4 1056.4 2.5 radial vel. 352 1.94 4884 [20]
HD 113996 b 6.3 610.2 1.6 radial vel. 331.4 1.49 4181 [20]
HD 147379 b 0.0777 86.54 0.3193 radial vel. 35.01 0.58 4090 [27]
HD 176986 b 0.0181 6.48980 0.06296 radial vel. 86.1 0.79 4931 [28]
HD 176986 c 0.02888 16.8191 0.11878 radial vel. 86.1 0.79 4931 [28]
HD 177565 b 0.04751 44.505 0.246 radial vel. 56 1.0 [29]
HD 208897 b 1.40 352.7 1.05 radial vel. 211 1.25 4860 [30]
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[31][32]
K2-18c 0.0236 8.962 0.060 363 radial vel. 110 0.36 3547 [33]
K2-105b 0.09439 0.369 8.266902 0.081 transit 760 1.01 5434 [34]
K2-106b 0.0263 0.136 0.571292 0.0116 2333 transit 798 0.95 5470 [35] Host star also known as EPIC 220674823
K2-106c 0.226 13.341245 transit 830 0.93 5590 [35] Host star also known as EPIC 220674823
K2-108b 0.18689 0.471 4.73401 0.0573 1446 transit 1530 1.12 5474 [36]
K2-111b 0.0271 0.17 5.35117 0.0621 1309 transit 680 0.88 5730 [37]
K2-114b 1.85 0.942 11.39109 0.09309 719 transit 1570 0.83 5027 [38]
K2-115b 0.84 1.115 20.273034 0.1367 682 transit 1360 0.83 5560 [38]
K2-116b 0.062 4.655411 0.048 transit 183.1 0.69 4348 [39] Host star also known as BD-12 6259
K2-117b 0.175 1.291505 0.019 transit 333.5 0.58 3842 [40]
K2-117c 0.181 5.444820 0.051 transit 333.5 0.58 3842 [40]
K2-118b 0.227 50.92092 0.245 transit 1057 0.76 4726 [39]
K2-119b 0.204 7.728578 0.070 transit 1180 0.76 4753 [39]
K2-120b 0.179 9.562742 0.078 transit 950 0.69 4350 [39]
K2-121b 0.814 5.185754 0.052 transit 552 0.71 4471 [39]
K2-122b 0.114 2.219405 0.029 transit 236 0.63 3993 [39][40]
K2-123b 0.236 30.956763 0.167 transit 529 0.65 4076 [39][40]
K2-124b 0.236 6.413539 0.051 transit 448 0.44 3561 [39]
K2-125b 0.194 21.750264 0.121 transit 415 0.49 3654 [39]
K2-126b 0.164 7.387073 0.066 transit 332 0.70 4368 [39]
K2-127b 0.773 3.588165 0.041 transit 2370 0.70 4388 [39]
K2-128b 0.127 5.675819 0.056 transit 373 0.71 4470 [39]
K2-129b 0.0928 8.239493 0.057 transit 90.19±0.07 0.36 3459 [39] Host star also known as LP 868-19
K2-130b 0.112 2.494120 0.032 transit 384.4±0.6 0.70 4356 [39]
K2-131b 0.017 0.152 0.36931 0.009500 2062 transit 501 0.84 5245 [41]
K2-132b 1.30 9.1751 transit 568 1.08±0.08 4840±90 [42]
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[43]
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[43]
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[43]
K2-135b 0.156 1.208957 0.020 1043.5 transit 98.8 0.66 4255 [44]
K2-135c 0.121 3.64802 0.042 721.9 transit 98.8 0.66 4255 [44]
K2-135d 0.187 6.20141 0.060 604.9 transit 98.8 0.66 4255 [44]
0.0883 7.975292 553 transit 0.74 4499 [45]
0.057±0.006 0.260 17.307137 0.11728 425 transit 0.74 4499 [45][46]
0.129 25.575065 373 transit 0.74 4499 [45]
K2-137b 0.5 0.079 0.179715 0.0058 1471 transit 0.46 3492 [47]
K2-139b 0.387 0.808 28.38236 0.179 565 transit 496 1.8 5340 [48]
K2-140b 0.211 1.093 6.56918 0.0687 957 transit 1110 1.00 5705 [49]
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 [50][51]
K2-146b 0.196±0.021 2.644646 0.0266±0.0010 transit 259.2±1.5 0.358±0.042 3385±70 [40]
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 [40] Also called EPIC 213715787[52]
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 [40]
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 [40]
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 [40]
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 [40]
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 [40]
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 [40]
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 [40]
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 [40]
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 [40]
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 [40]
KELT-9b 2.88 1.891 1.4811235 0.03462 4050 transit 615.5 2.52 10170 Hottest confirmed exoplanet[53]
KELT-18b 1.18 1.570 2.8717518 0.04550 2085 transit 1.52 6670 [54]
KELT-19Ab <4.07 1.91 4.6117093 0.0637 1935 transit 950 1.62 7500 [55]
KELT-20b 1.741 3.4741085 0.0542 2262 transit 455.6 1.76 8720 [56] Also known as MASCARA-2b[57]
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 [58]
Kepler-19d 0.0708 62.95 radial vel. 6910 0.94 5541 [59]
Kepler-80g 0.101 14.64558 418 transit 1160 0.73 4540 [60]
Kepler-90i 0.118 14.44912 709 transit 2540 1.2 6080 [60]
Kepler-150 f 0.325 637.2093 1.24 transit 2980±50 5560 [61]
Kepler-1649b 0.0964 8.689090 0.0514 transit 0.22 3240 [62]
Kepler-1650b 0.0856 1.53818001 transit 393 0.33 3410 [63]
Kepler-1651b 0.164 9.87863917 transit 226 0.52 3713 [63]
Kepler-1652b 0.143 38.09722 0.1654 268 transit 822 0.40 3638 [64]
0.194 140.2524 0.4706 284 transit 2460 0.72 4807 [64]
LHS 1140 b 0.0209 0.128 24.73712 0.0875 254 transit 40.7 0.18 3216 Potentially habitable exoplanet[65]
MASCARA-1b 3.7 1.5 2.148780 0.043 2570 transit 615.5 1.72 7554 [66]
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 [67]
MOA-2012-BLG-006Lb 8.40 10.2 microlensing 17000 0.49 [68]
MOA-2012-BLG-505Lb 0.02108 0.900 microlensing 23500 0.10 [69]
MOA-2016-BLG-227Lb 2.8 1.67 microlensing 21000 0.29 [70]
MXB 1658-298 b 23.7 760 1.613 timing 1.98 Circumbinary planet[71]
NGTS-1b 0.812 1.33 2.647298 0.0326 790 transit 731 0.617 3916 Largest exoplanet in relation to its star[72]
OGLE-2013-BLG-0132Lb 0.29 3.6 microlensing 13000 0.54 [73]
OGLE-2013-BLG-1721Lb 0.64 2.6 microlensing 21000 0.46 [73]
OGLE-2013-BLG-1761Lb 2.7+2.5−1.5 1.8±0.5 microlensing 23000+3300−3900 0.33+0.32−0.19 [74]
OGLE-2016-BLG-0263Lb 4.10 5.4 microlensing 21000 0.13 [75]
OGLE-2016-BLG-0613(AB)b 4.18 6.40 microlensing 11100 0.72 [76]
OGLE-2016-BLG-1190Lb 13.38 1224 2.17 microlensing 22100 0.88 Extremely massive; possible brown dwarf[77]
OGLE-2016-BLG-1195Lb 0.031 2.62±0.28 microlensing 22000±2000 0.57±0.06 [78][79]
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[80] Not an OGLE-2011-BLG-0173Lb!
PSR B0329+54 b 0.00620 10140 10.26 timing 1600 1.44 Dubious[81]
PSR J2322-2650 b 0.7949 0.322963997 0.0102 timing 750 1.4 [82]
Qatar-6b 0.668 1.062 3.506195 0.0423 transit 330 0.822 5052 [83]
Ross 128 b 0.00440 9.8658 0.0496 301 radial vel. 11.03 0.17 3192 [84]
SAND978 b 2.18 511.21 radial vel. 2051.3 1.37 4200 [85] Red giant host star, belonging to M67, 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[86]
Tau Ceti g 0.00551 20.00 0.133 radial vel. 12 0.78 [87]
Tau Ceti h 0.00576 49.41 0.243 radial vel. 12 0.78 [87]
TRAPPIST-1e 0.00195 0.082 6.099615 0.02817 251 transit 39 0.08 2559 Potentially habitable exoplanet[88]
TRAPPIST-1f 0.00214 0.093 9.20669 0.0371 219 transit 39 0.08 2559 Potentially habitable exoplanet[88]
TRAPPIST-1g 0.00422 0.101 12.35294 0.0451 199 transit 39 0.08 2559 Potentially habitable exoplanet[88]
TRAPPIST-1h 0.067 20 0.063 168 transit 39 0.08 2559 [88]
TYC 4282-605-1 b 10.78 101.54 0.422 radial vel. 2300 0.97 4300 [89]
WASP-91b 1.34 1.03 2.798581 0.037 1160 transit 490 0.84 4920 [90]
WASP-105b 1.8 0.96 7.87288 0.075 900 transit 0.89 5070 [90]
WASP-107b 0.12 0.94 5.721490 0.055 770 transit 0.69 4430 [90]
WASP-151b 0.31 1.13 4.533471 0.055 1290 transit 1570 1.01 5871 [91] Host star also known as K2-134
WASP-153b 0.39 1.55 3.332609 0.048 1700 transit 1400 1.34 5914 [91]
WASP-156b 0.128 0.51 3.836169 0.0453 970 transit 460 0.84 4910 [91] 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[92]
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 [93]
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 [93]
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 [93]

Specific exoplanet lists

References

  1. ↑ "The Extrasolar Planets Encyclopaedia". Extrasolar Planets Encyclopaedia. 1995. https://exoplanet.eu/catalog/. 
  2. ↑ Villaver, E; Niedzielski, A; Wolszczan, A; Nowak, G; Kowalik, K; Adamów, M; MacIejewski, G; Deka-Szymankiewicz, B et al. (2017). "Tracking Advanced Planetary Systems (TAPAS) with HARPS-N". Astronomy & Astrophysics 606: A38. doi:10.1051/0004-6361/201730471. Bibcode: 2017A&A...606A..38V. 
  3. ↑ 3.0 3.1 "Transiting exoplanets from the CoRoT space mission XXIX. The hot Jupiters CoRoT-30 b and CoRoT-31 b". Astronomy & Astrophysics 635: A122. March 2020. doi:10.1051/0004-6361/201732393. https://www.aanda.org/articles/aa/full_html/2020/03/aa32393-17/aa32393-17.html. Retrieved 2021-09-01. 
  4. ↑ 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, doi:10.1093/mnras/stx2187 
  5. ↑ 5.0 5.1 5.2 5.3 5.4 5.5 5.6 5.7 5.8 Astudillo-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. doi:10.1051/0004-6361/201630153. Bibcode: 2017A&A...602A..88A. https://www.aanda.org/articles/aa/full_html/2017/06/aa30153-16/aa30153-16.html. 
  6. ↑ 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. doi:10.1051/0004-6361/201730957. Bibcode: 2017A&A...605A..92S. https://www.aanda.org/articles/aa/full_html/2017/09/aa30957-17/aa30957-17.html. 
  7. ↑ Trifonov, T. et al. (2018), "The CARMENES search for exoplanets around M dwarfs", Astronomy & Astrophysics 609: A117, doi:10.1051/0004-6361/201731442 
  8. ↑ Perger, M. et al. (2017), "HADES RV Programme with HARPS-N at TNG", Astronomy & Astrophysics 608: A63, doi:10.1051/0004-6361/201731307 
  9. ↑ 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, doi:10.3847/1538-3881/aa674a 
  10. ↑ Bayliss, D.; Hartman, J. D.; Zhou, G.; Bakos, G. Á.; Vanderburg, A.; Bento, J.; Mancini, L.; Ciceri, S. et al. (2017), "HATS-36b and 24 Other Transiting/Eclipsing Systems from the HATSouth-K2 Campaign 7 Program", The Astronomical Journal 155 (3): 119, doi:10.3847/1538-3881/aaa8e6 
  11. ↑ 11.0 11.1 11.2 11.3 Brahm, R.; Hartman, J. D.; Jordán, A.; Bakos, G. Á.; Espinoza, N.; Rabus, M.; Bhatti, W.; Penev, K. et al. (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, doi:10.3847/1538-3881/aaa898 
  12. ↑ 12.0 12.1 12.2 12.3 Henning, Th.; Mancini, L.; Sarkis, P.; Bakos, G. Á.; Hartman, J. D.; Bayliss, D.; Bento, J.; Bhatti, W. et al. (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, doi:10.3847/1538-3881/aaa254 
  13. ↑ 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, doi:10.3847/1538-3881/aa832d, 122, Bibcode: 2017AJ....154..122C. 
  14. ↑ 14.0 14.1 14.2 Rey, J.; Hébrard, G.; Bouchy, F.; Bourrier, V.; Boisse, I.; Santos, N. C.; Arnold, L.; Astudillo-Defru, N. et al. (2017), "The SOPHIE search for northern extrasolar planets", Astronomy & Astrophysics 601: A9, doi:10.1051/0004-6361/201630089 
  15. ↑ 15.0 15.1 Udry, S.; Dumusque, X.; Lovis, C.; Segransan, D.; Diaz, R. F.; Benz, W.; Bouchy, F.; Coffinet, A. et al. (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, doi:10.1051/0004-6361/201731173, Bibcode: 2019A&A...622A..37U 
  16. ↑ 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. doi:10.1051/0004-6361/201730406. Bibcode: 2017A&A...605A.103F. 
  17. ↑ 17.0 17.1 Trifonov, T.; Kürster, M.; Zechmeister, M.; Zakhozhay, O. V.; Reffert, S.; Lee, M. H.; Rodler, F.; Vogt, S. S. et al. (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. doi:10.1051/0004-6361/201731044. Bibcode: 2017A&A...602L...8T. 
  18. ↑ 18.0 18.1 18.2 18.3 18.4 Vogt, Steven S. et al. (2017). "A Six-planet System around the Star HD 34445". The Astronomical Journal 154 (5): 181. doi:10.3847/1538-3881/aa8b61. Bibcode: 2017AJ....154..181V. 
  19. ↑ 19.0 19.1 19.2 19.3 19.4 Rosenthal, Lee J.; Fulton, Benjamin J.; Hirsch, Lea A.; Isaacson, Howard T.; Howard, Andrew W.; Dedrick, Cayla M.; Sherstyuk, Ilya A.; Blunt, Sarah C. et al. (2021). "The California Legacy Survey. I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades". The Astrophysical Journal Supplement Series 255: 8. doi:10.3847/1538-4365/abe23c. 
  20. ↑ 20.0 20.1 20.2 Jeong, G.; Lee, B.-C.; Han, I.; Omiya, M.; Izumiura, H.; Sato, B.; Harakawa, H.; Kambe, E. et al. (2017), "Detection of planet candidates around K giants. HD 40956, HD 111591, and HD 113996", Astronomy & Astrophysics 610: A3, doi:10.1051/0004-6361/201629185 
  21. ↑ 21.0 21.1 Gillon, M.; Demory, B.-O.; Lovis, C.; Deming, D.; Ehrenreich, D.; Lo Curto, G.; Mayor, M.; Pepe, F. et al. (2017), "The Spitzersearch for the transits of HARPS low-mass planets", Astronomy & Astrophysics 601: A117, doi:10.1051/0004-6361/201629270 
  22. ↑ Wittenmyer, Robert A.; Jones, M. I.; Horner, Jonathan; Kane, Stephen R.; Marshall, J. P.; Mustill, A. J.; Jenkins, J. S.; Rojas, P. A. Pena et al. (2017), "The Pan-Pacific Planet Search. VII. The Most Eccentric Planet Orbiting a Giant Star", The Astronomical Journal 154 (6): 274, doi:10.3847/1538-3881/aa9894 
  23. ↑ Bergmann, C.; Jones, M. I.; Zhao, J.; Mustill, A. J.; Brahm, R.; Torres, P.; Wittenmyer, R. A.; Gunn, F. et al. (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, doi:10.1017/pasa.2021.8 
  24. ↑ Jiang, Chen et al. (2023), "TESS Asteroseismic Analysis of HD 76920: The Giant Star Hosting an Extremely Eccentric Exoplanet", The Astrophysical Journal 945: 20, doi:10.3847/1538-4357/acb8ac 
  25. ↑ Unger, N. et al. (2021), "The HARPS search for southern extra-solar planets", Astronomy & Astrophysics 654: A104, doi:10.1051/0004-6361/202141351 
  26. ↑ 26.0 26.1 Ferraz, Alvaro; Kochetov, Evgenii (2017), A Multi-Planet System Transiting the V = 9 Rapidly Rotating F-Star HD 106315 
  27. ↑ Reiners, A. et al. (2017), "The CARMENES search for exoplanets around M dwarfs", Astronomy & Astrophysics 609: L5, doi:10.1051/0004-6361/201732165 
  28. ↑ 28.0 28.1 Suárez Mascareño, A.; González Hernández, J. I.; Rebolo, R.; Velasco, S.; Toledo-Padrón, B.; Udry, S.; Motalebi, F.; Ségrasan, D. et al. (2018), "The RoPES project with HARPS and HARPS-N", Astronomy & Astrophysics 612: A41, doi:10.1051/0004-6361/201732042 
  29. ↑ 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, doi:10.1093/mnras/stx1126 
  30. ↑ Yılmaz, M.; Sato, B.; Bikmaev, I.; Selam, S. O.; Izumiura, H.; Keskin, V.; Kambe, E.; Melnikov, S. S. et al. (2017), "A Jupiter-mass planet around the K0 giant HD 208897", Astronomy & Astrophysics 608: A14, doi:10.1051/0004-6361/201731184 
  31. ↑ Chauvin, G. et al. (2017), "Discovery of a warm, dusty giant planet around HIP 65426", Astronomy & Astrophysics 605: L9, doi:10.1051/0004-6361/201731152 
  32. ↑ "HIP 65426 b - Exoplanet-catalog" (in en). https://exoplanets.nasa.gov/exoplanet-catalog/7220/hip-65426-b/. 
  33. ↑ Cloutier, R.; Astudillo-Defru, N.; Doyon, R.; Bonfils, X.; Almenara, J.-M.; Benneke, B.; Bouchy, F.; Delfosse, X. et al. (2017), "Characterization of the K2-18 multi-planetary system with HARPS", Astronomy & Astrophysics 608: A35, doi:10.1051/0004-6361/201731558 
  34. ↑ Narita, Norio; Hirano, Teruyuki; Fukui, Akihiko; Hori, Yasunori; Dai, Fei; Yu, Liang; Livingston, John; Ryu, Tsuguru et al. (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), doi:10.1093/pasj/psx002 
  35. ↑ 35.0 35.1 Guenther, E. W. et al. (2017), "K2-106, a system containing a metal-rich planet and a planet of lower density", Astronomy & Astrophysics 608: A93, doi:10.1051/0004-6361/201730885, Bibcode: 2017A&A...608A..93G 
  36. ↑ Petigura, Erik A.; Sinukoff, Evan; Lopez, Eric D.; Crossfield, Ian J. M.; Howard, Andrew W.; Brewer, John M.; Fulton, Benjamin J.; Isaacson, Howard T. et al. (2017), "Four Sub-Saturns with Dissimilar Densities: Windows into Planetary Cores and Envelopes", The Astronomical Journal 153 (4): 142, doi:10.3847/1538-3881/aa5ea5 
  37. ↑ Fridlund, Malcolm et al. (2017), "K2-111 b − a short period super-Earth transiting a metal poor, evolved old star", Astronomy & Astrophysics 604: A16, doi:10.1051/0004-6361/201730822 
  38. ↑ 38.0 38.1 Shporer, Avi; Zhou, George; Fulton, Benjamin J.; Vanderburg, Andrew; Espinoza, Nestor; Collins, Karen; Ciardi, David; Bayliss, Daniel et al. (2017), "K2-114b and K2-115b: Two Transiting Warm Jupiters", The Astronomical Journal 154 (5): 188, doi:10.3847/1538-3881/aa8bb9 
  39. ↑ 39.00 39.01 39.02 39.03 39.04 39.05 39.06 39.07 39.08 39.09 39.10 39.11 39.12 39.13 Dressing, Courtney D.; Vanderburg, Andrew; Schlieder, Joshua E.; Crossfield, Ian J. M.; Knutson, Heather A.; Newton, Elisabeth R.; Ciardi, David R.; Fulton, Benjamin J. et al. (2017), "Characterizing K2 Candidate Planetary Systems Orbiting Low-mass Stars. II. Planetary Systems Observed During Campaigns 1–7", The Astronomical Journal 154 (5): 207, doi:10.3847/1538-3881/aa89f2 
  40. ↑ 40.00 40.01 40.02 40.03 40.04 40.05 40.06 40.07 40.08 40.09 40.10 40.11 40.12 40.13 40.14 40.15 Hirano, Teruyuki et al. (2017), "Exoplanets around Low-mass Stars Unveiled byK2", The Astronomical Journal 155 (3): 127, doi:10.3847/1538-3881/aaa9c1 
  41. ↑ 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, doi:10.3847/1538-3881/aa9065 
  42. ↑ Grunblatt, Samuel K.; Huber, Daniel; Gaidos, Eric; Lopez, Eric D.; Howard, Andrew W.; Isaacson, Howard T.; Sinukoff, Evan; Vanderburg, Andrew et al. (2017), "Seeing Double withK2: Testing Re-inflation with Two Remarkably Similar Planets around Red Giant Branch Stars", The Astronomical Journal 154 (6): 254, doi:10.3847/1538-3881/aa932d 
  43. ↑ 43.0 43.1 43.2 Wells, 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, doi:10.1093/mnrasl/slx171 
  44. ↑ 44.0 44.1 44.2 Rodriguez, 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. doi:10.3847/1538-3881/aaa292. Bibcode: 2018AJ....155...72R. 
  45. ↑ 45.0 45.1 45.2 Mann, Andrew W.; Vanderburg, Andrew; Rizzuto, Aaron C.; Kraus, Adam L.; Berlind, Perry; Bieryla, Allyson; Calkins, Michael L.; Esquerdo, Gilbert A. et al. (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, doi:10.3847/1538-3881/aa9791 
  46. ↑ 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, doi:10.3847/1538-3881/acca1c 
  47. ↑ 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, doi:10.1093/mnras/stx2891 
  48. ↑ Barragán, O.; Gandolfi, D.; Smith, A M S.; Deeg, H. J.; Fridlund, M C V.; Persson, C. M.; Donati, P.; Endl, M. et al. (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, doi:10.1093/mnras/stx3207 
  49. ↑ Giles, H A C.; Bayliss, D.; Espinoza, N.; Brahm, R.; Blanco-Cuaresma, S.; Shporer, A.; Armstrong, D.; Lovis, C. et al. (2017), "K2-140b – an eccentric 6.57 d transiting hot Jupiter in Virgo", Monthly Notices of the Royal Astronomical Society 475 (2): 1809–1818, doi:10.1093/mnras/stx3300 
  50. ↑ Okoli, Chiamaka (2017), K2-141 b: A 5-M⊕ super-Earth transiting a K7 V star every 6.7 hours 
  51. ↑ 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. doi:10.3847/1538-3881/aaa5b5. Bibcode: 2018AJ....155..107M. 
  52. ↑ Adams, Elisabeth R. (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. doi:10.3847/PSJ/ac0ea0. Bibcode: 2021PSJ.....2..152A. 
  53. ↑ Gaudi, B. Scott et al. (2017), "A giant planet undergoing extreme-ultraviolet irradiation by its hot massive-star host", Nature 546 (7659): 514–518, doi:10.1038/nature22392, PMID 28582774 
  54. ↑ McLeod, Kim K.; Rodriguez, Joseph E.; Oelkers, Ryan J.; Collins, Karen A.; Bieryla, Allyson; Fulton, Benjamin J.; Stassun, Keivan G.; Gaudi, B. Scott et al. (1 June 2017). "KELT-18b: Puffy Planet, Hot Host, Probably Perturbed". The Astronomical Journal 153 (6): 263. doi:10.3847/1538-3881/aa6d5d. ISSN 0004-6256. Bibcode: 2017AJ....153..263M. 
  55. ↑ 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, doi:10.3847/1538-3881/aa9e4d 
  56. ↑ Talens, G. J. J et al. (2018). "MASCARA-2 b: A hot Jupiter transiting a mV = 7.6 A-star". Astronomy & Astrophysics A57: 612. doi:10.1051/0004-6361/201731512. Bibcode: 2018A&A...612A..57T. 
  57. ↑ Rainer, M. et al. (2021), "The GAPS programme at TNG", Astronomy & Astrophysics 649: A29, doi:10.1051/0004-6361/202039247 
  58. ↑ Johnson, Marshall C; Rodriguez, Joseph E; Zhou, George; Gonzales, Erica J; Cargile, Phillip A; Crepp, Justin R; Penev, Kaloyan; Stassun, Keivan G 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. doi:10.3847/1538-3881/aaa5af. Bibcode: 2018AJ....155..100J. 
  59. ↑ 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, doi:10.3847/1538-3881/aa6897 
  60. ↑ 60.0 60.1 Shallue, 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". The Astrophysical Journal 155 (2): 94. doi:10.3847/1538-3881/aa9e09. Bibcode: 2018AJ....155...94S. https://www.cfa.harvard.edu/~avanderb/kepler90i.pdf. Retrieved 2017-12-15. 
  61. ↑ Schmitt, Joseph R.; Jenkins, Jon M.; Fischer, Debra A. (2017), "A Search for Lost Planets in theKepler Multi-planet Systems and the Discovery of the Long-period, Neptune-sized Exoplanet Kepler-150 F", The Astronomical Journal 153 (4): 180, doi:10.3847/1538-3881/aa62ad, PMID 29375142 
  62. ↑ Angelo, Isabel; Rowe, Jason F.; Howell, Steve B.; Quintana, Elisa V.; Still, Martin; Mann, Andrew W.; Burningham, Ben; Barclay, Thomas et al. (2017), "Kepler-1649b: An Exo-Venus in the Solar Neighborhood", The Astronomical Journal 153 (4): 162, doi:10.3847/1538-3881/aa615f 
  63. ↑ 63.0 63.1 Mann, Andrew W.; Dupuy, Trent; Muirhead, Philip S.; Johnson, Marshall C.; Liu, Michael C.; Ansdell, Megan; Dalba, Paul A.; Swift, Jonathan J. et al. (2017), "The Gold Standard: Accurate Stellar and Planetary Parameters for EightKeplerM Dwarf Systems Enabled by Parallaxes", The Astronomical Journal 153 (6): 267, doi:10.3847/1538-3881/aa7140 
  64. ↑ 64.0 64.1 Torres, Guillermo; Kane, Stephen R.; Rowe, Jason F.; Batalha, Natalie M.; Henze, Christopher E.; Ciardi, David R.; Barclay, Thomas; Borucki, William J. et al. (2017), "Validation of SmallKepler Transiting Planet Candidates in or near the Habitable Zone", The Astronomical Journal 154 (6): 264, doi:10.3847/1538-3881/aa984b 
  65. ↑ 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. doi:10.1093/mnras/staa1110. Bibcode: 2020MNRAS.494.5082G. 
  66. ↑ Talens, G. J. J et al. (2017). "MASCARA-1 b. A hot Jupiter transiting a bright mV = 8.3 A-star in a misaligned orbit". Astronomy & Astrophysics 606: A73. doi:10.1051/0004-6361/201731282. Bibcode: 2017A&A...606A..73T. 
  67. ↑ Bennett, D. P. et al. (2017), "The First Planetary Microlensing Event with Two Microlensed Source Stars", The Astronomical Journal 155 (3): 141, doi:10.3847/1538-3881/aaadfa 
  68. ↑ 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, doi:10.1051/0004-6361/201730928 
  69. ↑ Nagakane, M.; Sumi, T.; Koshimoto, N.; Bennett, D. P.; Bond, I. A.; Rattenbury, N.; Suzuki, D.; Abe, F. et al. (2017), "MOA-2012-BLG-505Lb: A Super-Earth-mass Planet That Probably Resides in the Galactic Bulge", The Astronomical Journal 154: 35, doi:10.3847/1538-3881/aa74b2 
  70. ↑ 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: 3, doi:10.3847/1538-3881/aa72e0 
  71. ↑ 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, doi:10.1093/mnrasl/slx039 
  72. ↑ Bayliss, Danile (31 October 2017). "NGTS-1b: A hot Jupiter transiting an M-dwarf". Monthly Notices of the Royal Astronomical Society 475 (4): 4467–4475. doi:10.1093/mnras/stx2778. Bibcode: 2018MNRAS.475.4467B. 
  73. ↑ 73.0 73.1 Mróz, 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, doi:10.3847/1538-3881/aa8f98 
  74. ↑ Hirao, Y. et al. (2017), "OGLE-2013-BLG-1761Lb: A Massive Planet around an M/K Dwarf", The Astronomical Journal 154: 1, doi:10.3847/1538-3881/aa73da 
  75. ↑ 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, doi:10.3847/1538-3881/aa859a 
  76. ↑ Han, C. et al. (2017), "OGLE-2016-BLG-0613LABb: A Microlensing Planet in a Binary System", The Astronomical Journal 154 (6): 223, doi:10.3847/1538-3881/aa9179 
  77. ↑ Ryu, Y.-H. (27 October 2017). "OGLE-2016-BLG-1190Lb: First Spitzer Bulge Planet Lies Near the Planet/Brown-Dwarf Boundary". The Astronomical Journal 155: 40. doi:10.3847/1538-3881/aa9be4. 
  78. ↑ Shvartzvald, Y (1 May 2017). "An Earth-mass Planet in a 1 au Orbit around an Ultracool Dwarf". The Astrophysical Journal Letters 840 (L3): L3. doi:10.3847/2041-8213/aa6d09. Bibcode: 2017ApJ...840L...3S. 
  79. ↑ Vandorou, Aikaterini; Dang, Lisa; Bennett, David P.; Koshimoto, Naoki; Terry, Sean K.; Beaulieu, Jean-Phillipe; Alard, Christophe; Bhattacharya, Aparna et al. (2023), OGLE-2016-BLG-1195Lb: A Sub-Neptune Beyond the Snow Line of an M-Dwarf Confirmed by Keck AO 
  80. ↑ Hwang, K.-H. et al. (2017), "OGLE-2017-BLG-0173Lb: Low-mass-ratio Planet in a "Hollywood" Microlensing Event", The Astronomical Journal 155: 20, doi:10.3847/1538-3881/aa992f 
  81. ↑ Starovoit, E. D.; Rodin, A. E. (2017). "On the existence of planets around the pulsar PSR B0329+54". Astronomy Reports 61 (11): 948–953. doi:10.1134/S1063772917110063. Bibcode: 2017ARep...61..948S. 
  82. ↑ Spiewak, R.; Bailes, M.; Barr, E. D.; Bhat, N D R.; Burgay, M.; Cameron, A. D.; Champion, D. J.; Flynn, C M L. et al. (2017), "PSR J2322−2650 – a low-luminosity millisecond pulsar with a planetary-mass companion", Monthly Notices of the Royal Astronomical Society 475: 469–477, doi:10.1093/mnras/stx3157 
  83. ↑ Alsubai, Khalid; Tsvetanov, Zlatan I.; Latham, David W.; Bieryla, Allyson; Esquerdo, Gilbert A.; Mislis, Dimitris; Pyrzas, Stylianos; Foxell, Emma et al. (2017), "Qatar Exoplanet Survey: Qatar-6b—A Grazing Transiting Hot Jupiter", The Astronomical Journal 155 (2): 52, doi:10.3847/1538-3881/aaa000 
  84. ↑ Bonfils, Xavier (2017). "A temperate exo-Earth around a quiet M dwarf at 3.4 parsecs". Astronomy and Astrophysics 613: A25. doi:10.1051/0004-6361/201731973. Bibcode: 2018A&A...613A..25B. 
  85. ↑ Brucalassi, A.; Koppenhoefer, J.; Saglia, R.; Pasquini, L.; Ruiz, M. T.; Bonifacio, P.; Bedin, L. R.; Libralato, M. et al. (2017), "Search for giant planets in M 67", Astronomy & Astrophysics 603: A85, doi:10.1051/0004-6361/201527562 
  86. ↑ Yu, L.; Donati, J.-F.; Hébrard, E. M.; Moutou, C.; Malo, L.; Grankin, K.; Hussain, G.; Collier Cameron, A. et al. (2017), "A hot Jupiter around the very active weak-line T Tauri star TAP 26", Monthly Notices of the Royal Astronomical Society: stx009, doi:10.1093/mnras/stx009 
  87. ↑ 87.0 87.1 Feng, Fabo et al. (2017). "Color Difference Makes a Difference: Four Planet Candidates around Tau Ceti". The Astronomical Journal 154 (4): 135. doi:10.3847/1538-3881/aa83b4. Bibcode: 2017AJ....154..135F. 
  88. ↑ 88.0 88.1 88.2 88.3 Gillon, 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". Nature 542 (7642): 456–460. doi:10.1038/nature21360. PMID 28230125. PMC 5330437. Bibcode: 2017Natur.542..456G. http://www.eso.org/public/archives/releases/sciencepapers/eso1706/eso1706a.pdf. 
  89. ↑ González-Álvarez, E. et al. (2022), "The GAPS Programme with HARPS-N at TNG", Astronomy & Astrophysics 606: A51, doi:10.1051/0004-6361/201731124 
  90. ↑ 90.0 90.1 90.2 Anderson, D. R.; Collier Cameron, A.; Delrez, L.; Doyle, A. P.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M. et al. (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, doi:10.1051/0004-6361/201730439 
  91. ↑ 91.0 91.1 91.2 Demangeon, 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, doi:10.1051/0004-6361/201731735 
  92. ↑ 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, doi:10.1093/mnras/stx1729 
  93. ↑ 93.0 93.1 93.2 Astudillo-Defru, N.; Díaz, R. F.; Bonfils, X.; Almenara, J. M.; Delisle, J.-B.; Bouchy, F.; Delfosse, X.; Forveille, T. et al. (2017), "The HARPS search for southern extra-solar planets", Astronomy & Astrophysics 605: L11, doi:10.1051/0004-6361/201731581 



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