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List of exoplanets discovered in 2017

From Wikipedia, the free encyclopedia

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]
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[43]
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[43]
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[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]
K2-136b [ru] 0.0883 7.975292 553 transit 0.74 4499 [45]
K2-136c [ru] 0.057±0.006 0.260 17.307137 0.11728 425 transit 0.74 4499 [45][46]
K2-136d [ru] 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]
Kepler-1653b [it] 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]

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  • THE CLOSEST EXOPLANETS LIKELY TO HARBOUR LIFE
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Transcription

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanet by year of discovery


References

  1. ^ "The Extrasolar Planets Encyclopaedia". Extrasolar Planets Encyclopaedia. 1995. Retrieved 2015-11-09.
  2. ^ 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.
  3. ^ a b "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. hdl:1887/3133644. Archived from the original on 2021-12-06. 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, arXiv:1709.00351, doi:10.1093/mnras/stx2187
  5. ^ a b c d e f g h i 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. arXiv:1703.05386. Bibcode:2017A&A...602A..88A. doi:10.1051/0004-6361/201630153. S2CID 119418595.
  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. arXiv:1705.06537. Bibcode:2017A&A...605A..92S. doi:10.1051/0004-6361/201730957. S2CID 119003137.
  7. ^ Trifonov, T.; et al. (2018), "The CARMENES search for exoplanets around M dwarfs", Astronomy & Astrophysics, 609: A117, arXiv:1710.01595, doi:10.1051/0004-6361/201731442
  8. ^ 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
  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, arXiv:1702.00106, doi:10.3847/1538-3881/aa674a, S2CID 119491990
  10. ^ 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
  11. ^ a b c d Brahm, 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
  12. ^ a b c d Henning, 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, doi:10.3847/1538-3881/aaa254, S2CID 119516821
  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, arXiv:1706.01892, Bibcode:2017AJ....154..122C, doi:10.3847/1538-3881/aa832d, S2CID 54196245, 122.
  14. ^ a b c Rey, 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
  15. ^ a b Udry, 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
  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. arXiv:1705.05124. Bibcode:2017A&A...605A.103F. doi:10.1051/0004-6361/201730406. S2CID 119084078.
  17. ^ a b Trifonov, 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.
  18. ^ a b c d e Vogt, Steven S.; et al. (2017). "A Six-planet System around the Star HD 34445". The Astronomical Journal. 154 (5): 181. arXiv:1710.07337. Bibcode:2017AJ....154..181V. doi:10.3847/1538-3881/aa8b61. S2CID 119182115.
  19. ^ a b c d e Rosenthal, Lee J.; Fulton, Benjamin J.; Hirsch, Lea A.; Isaacson, Howard T.; Howard, Andrew W.; Dedrick, Cayla M.; Sherstyuk, Ilya A.; Blunt, Sarah C.; Petigura, Erik A.; Knutson, Heather A.; Behmard, Aida; Chontos, Ashley; Crepp, Justin R.; Crossfield, Ian J. M.; Dalba, Paul A.; Fischer, Debra A.; Henry, Gregory W.; Kane, Stephen R.; Kosiarek, Molly; Marcy, Geoffrey W.; Rubenzahl, Ryan A.; Weiss, Lauren M.; Wright, Jason T. (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. arXiv:2105.11583. doi:10.3847/1538-4365/abe23c. S2CID 235186973.
  20. ^ a b c Jeong, 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
  21. ^ a b Gillon, 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), "The Spitzersearch for the transits of HARPS low-mass planets", Astronomy & Astrophysics, 601: A117, arXiv:1701.01303, doi:10.1051/0004-6361/201629270, S2CID 86862862
  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; 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, doi:10.3847/1538-3881/aa9894, S2CID 55417878
  23. ^ 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, doi:10.1017/pasa.2021.8, S2CID 231942350
  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, arXiv:2302.01102, doi:10.3847/1538-4357/acb8ac
  25. ^ Unger, N.; et al. (2021), "The HARPS search for southern extra-solar planets", Astronomy & Astrophysics, 654: A104, arXiv:2108.10198, doi:10.1051/0004-6361/202141351, S2CID 239033129
  26. ^ a b Ferraz, Alvaro; Kochetov, Evgenii (2017), A Multi-Planet System Transiting the V = 9 Rapidly Rotating F-Star HD 106315, arXiv:1701.03808
  27. ^ 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
  28. ^ a b Suárez 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
  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, arXiv:1705.03089, doi:10.1093/mnras/stx1126
  30. ^ 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, doi:10.1051/0004-6361/201731184, S2CID 118863243
  31. ^ Chauvin, G.; et al. (2017), "Discovery of a warm, dusty giant planet around HIP 65426", Astronomy & Astrophysics, 605: L9, arXiv:1707.01413, doi:10.1051/0004-6361/201731152, S2CID 102344893
  32. ^ "HIP 65426 b - Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 2023-12-03.
  33. ^ 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, doi:10.1051/0004-6361/201731558, S2CID 118955175
  34. ^ 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
  35. ^ a b 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, arXiv:1705.04163, Bibcode:2017A&A...608A..93G, doi:10.1051/0004-6361/201730885, S2CID 55692535
  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.; 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, doi:10.3847/1538-3881/aa5ea5, S2CID 599957
  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, arXiv:1704.08284, doi:10.1051/0004-6361/201730822, S2CID 39412906
  38. ^ a b Shporer, 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, doi:10.3847/1538-3881/aa8bb9, S2CID 468318
  39. ^ a b c d e f g h i j k l m n Dressing, 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, doi:10.3847/1538-3881/aa89f2, S2CID 13419148
  40. ^ a b c d e f g h i j k l m n o p Hirano, 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
  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, arXiv:1710.00076, doi:10.3847/1538-3881/aa9065, S2CID 55262711
  42. ^ 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, doi:10.3847/1538-3881/aa932d, S2CID 55959801
  43. ^ a b c 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, arXiv:1709.01025, doi:10.1093/mnrasl/slx171
  44. ^ a b c 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. arXiv:1709.01957. Bibcode:2018AJ....155...72R. doi:10.3847/1538-3881/aaa292. S2CID 55459523.
  45. ^ a b c Mann, 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
  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, arXiv:2304.02779, 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, arXiv:1707.04549, 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.; 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
  49. ^ 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
  50. ^ Okoli, Chiamaka (2017), K2-141 b: A 5-M⊕ super-Earth transiting a K7 V star every 6.7 hours, arXiv:1711.05277
  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. arXiv:1801.03502. Bibcode:2018AJ....155..107M. doi:10.3847/1538-3881/aaa5b5. S2CID 54869937.
  52. ^ 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.
  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, arXiv:1706.06723, doi:10.1038/nature22392, PMID 28582774, S2CID 205256410
  54. ^ 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.
  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, arXiv:1709.07010, doi:10.3847/1538-3881/aa9e4d, S2CID 54002227
  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. arXiv:1707.01500. Bibcode:2018A&A...612A..57T. doi:10.1051/0004-6361/201731512. S2CID 119422884.
  57. ^ 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
  58. ^ 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.
  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, arXiv:1703.06885, doi:10.3847/1538-3881/aa6897, S2CID 29845787
  60. ^ a b 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" (PDF). The Astrophysical Journal. 155 (2): 94. arXiv:1712.05044. Bibcode:2018AJ....155...94S. doi:10.3847/1538-3881/aa9e09. S2CID 4535051. 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, arXiv:1703.09229, doi:10.3847/1538-3881/aa62ad, PMC 5783551, PMID 29375142, S2CID 4520222
  62. ^ 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, doi:10.3847/1538-3881/aa615f, S2CID 29545487
  63. ^ a b Mann, 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, doi:10.3847/1538-3881/aa7140, S2CID 119325474
  64. ^ a b Torres, 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 SmallKepler Transiting Planet Candidates in or near the Habitable Zone", The Astronomical Journal, 154 (6): 264, arXiv:1711.01267, doi:10.3847/1538-3881/aa984b, S2CID 73678176
  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. arXiv:2005.10318. Bibcode:2020MNRAS.494.5082G. doi:10.1093/mnras/staa1110.
  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. arXiv:1707.04262. Bibcode:2017A&A...606A..73T. doi:10.1051/0004-6361/201731282. S2CID 119259578.
  67. ^ 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
  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, arXiv:1704.01121, doi:10.1051/0004-6361/201730928, S2CID 56306676
  69. ^ 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: 35, arXiv:1703.10769, doi:10.3847/1538-3881/aa74b2, S2CID 119077625
  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, arXiv:1704.01724, doi:10.3847/1538-3881/aa72e0, S2CID 39514486
  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, arXiv:1703.04433, doi:10.1093/mnrasl/slx039
  72. ^ 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.
  73. ^ a b 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, arXiv:1705.01058, doi:10.3847/1538-3881/aa8f98, S2CID 119093055
  74. ^ Hirao, Y.; et al. (2017), "OGLE-2013-BLG-1761Lb: A Massive Planet around an M/K Dwarf", The Astronomical Journal, 154: 1, arXiv:1703.07623, 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, arXiv:1708.02727, doi:10.3847/1538-3881/aa859a, S2CID 56010958
  76. ^ 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, doi:10.3847/1538-3881/aa9179, S2CID 119012722
  77. ^ 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.
  78. ^ 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.
  79. ^ 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
  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, arXiv:1709.08476, 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, arXiv:1710.01153, Bibcode:2017ARep...61..948S, doi:10.1134/S1063772917110063, S2CID 119460916
  82. ^ 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
  83. ^ 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
  84. ^ 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.
  85. ^ 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
  86. ^ 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
  87. ^ a b Feng, 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.
  88. ^ a b c d 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" (PDF). Nature. 542 (7642): 456–460. arXiv:1703.01424. Bibcode:2017Natur.542..456G. doi:10.1038/nature21360. PMC 5330437. PMID 28230125.
  89. ^ 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
  90. ^ a b c Anderson, 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, doi:10.1051/0004-6361/201730439, S2CID 58910823
  91. ^ a b c 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, arXiv:1710.06321, doi:10.1051/0004-6361/201731735, S2CID 215776387
  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, arXiv:1704.07771, doi:10.1093/mnras/stx1729
  93. ^ a b c Astudillo-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
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