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Lista de exoplanetas descobertos em 2013

Esta é uma Lista de exoplanetas descobertos em 2013.

Para exoplanetas detectados apenas pela velocidade radial, o valor da massa é na verdade um limite inferior. (Consulte a massa mínima para obter mais informações)

Nome Massa (MJ) Raio (RJ) Período (dais) Semieixo maior (AU) Temp. (K)[1] Método de descoberta Distância (ly) Massa da estrela-mãe (M☉) Temperatura da estrela-mãe (K) Observações
2MASS J01225093-2439505 b 24.5 52 Imagem direta 120 0.4 3530 [2]
BD+15 2940 b 1.11 137.48 0.539 Vel. radial 572.2 1.1 4796 [3]
COROT-25b 0.27 1.08 4.86069 0.0578 Trânsito 3300 1.09 6040 [4]
COROT-26b 0.52 1.26 4.20474 0.0526 Trânsito 5400 1.09 5590 [4]
DENIS-P J082303.1-491201 b 28.5 246.36 0.36 Astrometria 67.7 0.07 2150 [5]
Gliese 163 b 0.03335 8.63182 0.0607 Vel. radial 48.8 0.4 3500 [6]
Gliese 163 c 0.0214 25.63058 0.1254 Vel. radial 48.8 0.4 3500 [6]
Gliese 163 d 0.0925 603.95116 1.0304 Vel. radial 48.8 0.4 3500 [6]
Gliese 221b 0.027 3.8728 0.0428 Vel. radial 66 0.7 4324 [7][8] Disputado[9]
Gliese 221 c 0.17 125.94 0.435 Vel. radial 66 0.7 4324 [7][8]
Gliese 328 b 2.3 4100 4.5 Vel. radial 65.3 0.69 3900 [10]
Gliese 504 b 4 43.5 Imagem direta 58.5 1.22 6234 [11]
HAT-P-44b 0.352 1.242 4.301219 0.0507 Trânsito 1180 0.94 5295 [12]
HAT-P-44c 4 872.2 1.752 Vel. radial 1180 0.94 5295 O período é ambíguo[12]
HAT-P-45b 0.892 1.426 3.128992 0.0452 Trânsito 990 1.26 6330 [12]
HAT-P-46b 0.493 1.284 4.463129 0.0577 Trânsito 970 1.28 6120 [12]
HATS-2b 1.345 1.168 1.354133 0.023 Trânsito 1200 0.88 5227 [13]
HATS-3b 1.071 1.381 3.547851 0.0485 1648 Trânsito 1480 1.21 6351 [14]
HD 2952 b 1.6 311.6 1.2 Vel. radial 375.8 2.54 4844 [15]
HD 13908 b 0.865 19.382 0.154 Vel. radial 218.2 1.29 6255 [16]
HD 13908 c 5.13 931 2.03 Vel. radial 218.2 1.29 6255 [16]
HD 65216c 0.17 152.6 0.54 Vel. radial 116.1 0.92 5666 [17] Falso positivo, outro planeta com o mesmo nome atribuído foi descoberto em 2019[18]
HD 95086 b 5 55.7 Imagem direta 298.7 1.6 [19]
HD 103774 b 0.367 5.8881 0.07 Vel. radial 173.1 1.33 6489 [7]
HD 106906 b 11 650 Imagem direta 299.5 1.5 6516 [20]
HD 109271 b 0.054 7.8543 0.079 Vel. radial 185.6 1.05 5783 [7]
HD 109271 c 0.076 30.93 0.196 Vel. radial 185.6 1.05 5783 [7]
HD 113337 b 2.83 324 0.92 Vel. radial 122.0 1.4 6576.6 [21]
HD 120084 b 4.5 2082 4.3 Vel. radial 318.5 2.39 4892 [15]
HD 159243 b 1.13 12.62 0.11 Vel. radial 223.7 1.12 6123 [16]
HD 159243 c 1.9 248.4 0.8 Vel. radial 223.7 1.12 6123 [16]
HD 233604 b 6.575 192 0.747 Vel. radial 2830±90 1.5 4791 [3]
HD 285507 b 0.92±0.03 6.0962±0.0002 Vel. radial 153 0.73±0.03 4503+85
−61 		Pertence ao aglomerado aberto de Híades[22][23]
HD 112410 b 9.18 124.6 0.565 Vel. radial 486.8 1.54 4830 [24]
HIP 91258 b 1.068 5.0505 0.057 Vel. radial 145.0 0.95 5519 [16]
KELT-3b 1.477 1.345 2.7033904 0.04122 Trânsito 580 1.28 6306 [25]
KELT-6b 0.442 1.18 7.8455821 0.08 Trânsito 720 1.13 6272 [26]
Kepler-37b 0.03146 0.029 13.3675 Trânsito 220 0.8 5417 [27]
Kepler-37c 0.03776 0.067 21.302 Trânsito 220 0.8 5417 [27]
Kepler-37d 0.03839 0.173 39.7922 Trânsito 220 0.8 5417 [27]
Kepler-61b 0.192 59.87756 Trânsito 1103±16 0.64 4017 [28]
Kepler-62b 0.03 0.117 5.714932 0.0553 Trânsito 1200 0.69 4925 [29]
Kepler-62c 0.013 0.048 12.4417 0.0929 Trânsito 1200 0.69 4925 [29]
Kepler-62d 0.044 0.174 18.16406 0.12 Trânsito 1200 0.69 4925 [29]
Kepler-62e 0.113 0.144 122.3874 0.427 Trânsito 1200 0.69 4925 Exoplaneta potencialmente habitável[29]
Kepler-62f 0.11 0.126 267.291 0.718 Trânsito 1200 0.69 4925 Exoplaneta potencialmente habitável[29]
Kepler-63b 0.378 0.545 9.4341505 0.08 Trânsito 650 0.98 5576 [30]
Kepler-65b 0.127 2.15491 0.035 Trânsito 999±8 1.25 6211 [31]
Kepler-65c 0.23 5.859944 0.068 Trânsito 999±8 1.25 6211 [31]
Kepler-65d 0.136 8.13123 0.084 Trânsito 999±8 1.25 6211 [31]
Kepler-66b 0.25 17.815815 0.1352 Trânsito 3610 1.04 5962 Pertence ao aglomerado aberto NGC 6811[32]
Kepler-67b 0.262 15.7259 0.1171 Trânsito 3610 0.86 5331 Pertence ao aglomerado aberto NGC 6811[32]
Kepler-68b 0.01878 0.208 5.39875 1280 Trânsito 440 1.08 5793 [33]
Kepler-68c 0.02265 0.089 9.60504 Trânsito 440 1.08 5793 [33]
Kepler-68d 0.84007 625 Vel. radial 440 1.08 5793 [33]
Kepler-69b 0.2 13.722341 0.094 Trânsito 2430±30 0.81 5638 [34]
Kepler-69c 0.153 242.4613 0.64 Trânsito 2430±30 0.81 5638 [34][35]
Kepler-74b 0.63 0.96 7.340711 0.0781 Trânsito 4300 1.18 6000 [36]
Kepler-75b 10.1 1.05 8.8849116 0.0818 Trânsito 3700 0.91 5200 [36]
Kepler-76b 2.01 1.36 1.5449298 0.0274 Modulação de brilho orbital 2750±30 1.2 6409 [37]
Kepler-77b 0.43 0.96 3.57878087 0.04501 Trânsito 1900 0.95 5520 [38]
Kepler-78b 0.006 0.105 0.355 2330 Trânsito 407.1±1.1 0.76 5058 [39]
Kepler-87b 1.02 1.204 114.73635 0.481 478 Trânsito 4170±90 1.1 5600 Mais dois planetas não confirmados no sistema[40]
Kepler-87c 0.02 0.548 191.2318 0.676 403 Trânsito 4170±90 1.1 5600 Mais dois planetas não confirmados no sistema[40]
Kepler-88b 0.027 0.337 10.95416 Trânsito 1110 0.96 5471 [41]
Kepler-88c 0.626 22.3395 0.15525 Tempo 1110 0.96 5471 [41][42]
Kepler-89b 0.033 0.153 3.743208 0.05119 Trânsito 1577±16 1.28 6182 [43]
Kepler-89c 0.049 0.385 10.423648 0.1013 Trânsito 1577±16 1.28 6182 [43]
Kepler-89d 0.334 1.005 22.342989 0.1684 Trânsito 1577±16 1.28 6182 [43]
Kepler-89e 0.11 0.585 54.32031 0.3046 Trânsito 1577±16 1.28 6182 [43]
Kepler-90b 0.117 7.008151 0.074 1056 Trânsito 2500 1.2 6080 [44]
Kepler-90c 0.106 8.719375 0.089 981 Trânsito 2500 1.2 6080 [44]
Kepler-90d 0.256 59.73667 0.32 518 Trânsito 2500 1.2 6080 [44]
Kepler-90e 0.237 91.93913 0.42 448 Trânsito 2500 1.2 6080 [44]
Kepler-90f 0.257 124.9144 0.48 592 Trânsito 2500 1.2 6080 [44]
Kepler-90g 0.723 210.60697 0.71 340 Trânsito 2500 1.2 6080 [44]
Kepler-90h 1.008 331.60059 1.01 292 Trânsito 2500 1.2 6080 [44]
Kepler-91b 0.81 1.367 6.24658 0.0731 Trânsito 3400 1.31 4550 [45]
Kepler-92b 0.202 0.313 13.749 Trânsito 1580±17 1.21 5883 [46]
Kepler-92c 0.019 0.232 26.723 Trânsito 1580±17 1.21 5883 [46]
Kepler-102e 0.028 0.198 16.1457 579 Trânsito 352.7±0.7 0.81 4909 [47]
Kepler-105b 0.429 5.4122 0.066 Trânsito 1517±18 0.96 5827 [47]
Kepler-114c 0.009 0.143 8.041 623 Trânsito 852±4 0.56 4605 [46]
Kepler-114d 0.012 0.226 11.776 549 Trânsito 852±4 0.56 4605 [46]
Kepler-128b 0.097 0.101 15.09 Trânsito 1307±12 1.18 6090 [46]
Kepler-128c 0.105 0.101 22.804 Trânsito 1307±12 1.18 6090 [46]
Kepler-130b 0.091 8.457458 0.079 Trânsito 1042±7 1 5884 [47]
Kepler-145b 0.117 0.236 22.951 Trânsito 1880±30 1.32 6022 [46]
Kepler-145c 0.25 0.385 42.882 Trânsito 1880±30 1.32 6022 [46]
Kepler-177b 0.006 0.259 36.855 Trânsito 4880±140 1.07 5942 [46]
Kepler-177c 0.024 0.633 49.412 Trânsito 4880±140 1.07 5942 [46]
Kepler-238e 0.534 0.5 23.654 Trânsito 6200±300 1.06 5751 [46]
Kepler-238f 0.042 0.178 50.447 Trânsito 6200±300 1.06 5751 [46]
Kepler-276c 0.052 0.259 31.884 Trânsito 3850±150 1.1 6105 [46]
Kepler-276d 0.051 0.25 48.648 Trânsito 3850±150 1.1 6105 [46]
Kepler-277b 0.275 0.261 17.324 Trânsito 3280±50 1.12 5946 [46]
Kepler-277c 0.202 0.3 33.006 Trânsito 3280±50 1.12 5946 [46]
Kepler-279b 0.323 12.309681 0.112 Trânsito 3480±70 1.1 6363 KOI-1236.01[48]
Kepler-279c 0.155 0.384 35.736 Trânsito 3490±70 1.1 6363 KOI-1236.02[48][46]
Kepler-279d 0.118 0.277 54.414 Trânsito 3490±70 1.1 6363 [46]
Kepler-282d 0.192 0.219 24.806 Trânsito 4540±150 0.97 5602 [46]
Kepler-282e 0.177 0.277 44.347 Trânsito 4540±150 0.97 5602 [46]
Kepler-305b 0.033 0.321 5.487 Trânsito 2900±90 0.76 5100 [46]KOI-1563.01[48]
Kepler-305c 0.019 0.294 8.291 Trânsito 2900±90 0.76 5100 [46]KOI-1563.02[48]
Kepler-307b 0.02341 0.217 10.4208 Trânsito 1908±17 0.91 5367 [46]
Kepler-307c 0.01145 0.196 13.0729 Trânsito 1908±17 0.91 5367 [46]
Kepler-328b 0.09 0.205 34.921 Trânsito 7700±500 1.15 5914 [46]
Kepler-328c 0.124 0.482 71.312 Trânsito 7700±500 1.15 5914 [46]
Kepler-350c 0.019 0.277 17.849 Trânsito 3210±70 1 6186 [46]
Kepler-350d 0.047 0.25 26.136 Trânsito 3210±70 1 6186 [46]
Kepler-396b 0.238 0.312 42.994 Trânsito 734±5 0.85 5384 [46]KOI-2672.01[48]
Kepler-396c 0.056 0.473 88.505 Trânsito 734±5 0.85 5384 [46]KOI-2672.02[48]
Kepler-410Ab 0.253 17.833648 0.1226 Trânsito 430 1.21 6273 [49]
Kepler-411b 0.168 3.00516 0.038 1040 Trânsito 503.5±1.5 0.83 4974 [47]
Kepler-1359c 0.3711+0.12
−0.06 		505.46+0.05
−0.04 		1.143±0.018 Trânsito 2182+81
−82 		0.78+0.03
−0.04 		4709+46
−56 		[44] Also called KIC 6436029 c, discovery retracted in 2015 after 3rd transit was proven to be false.[50]
MOA-2008-BLG-379Lb 4.1 3.3 Microlente 11000 0.56 [51]
MOA-2010-BLG-328Lb 0.02895 0.92 Microlente 2600 0.11 [52]
MOA-2011-BLG-262Lb 0.056634 0.383 1 Microlente 22830 0.1 3300 A estrela-mãe pode ser um planeta interestelar, o planeta pode ser uma exolua[53]
MOA-2011-BLG-262L 4 N/A Microlente 22830 3300 A estrela-mãe pode ser um planeta interestelar, o planeta pode ser uma exolua[53]
MOA-2011-BLG-293Lb 4.8 1.1 Microlente 25200 0.86 [54]
MOA-2011-BLG-322Lb 11.6 4.3 Microlente 24700 0.39 [55]
OGLE-2011-BLG-0251Lb 0.53 2.72 Microlente 8400 0.26 [56]
OGLE-2012-BLG-358Lb 1.85 0.87 Microlente 5700 0.02 Orbitando uma anã marrom[57]
OGLE-2012-BLG-406Lb 2.73 3.45 Microlente 16200 0.44 [58]
Omega Serpentis b 1.7 277.02 1.1 Vel. radial 263.0 2.17 4770 [15]
PH2b 0.903 282.5255 0.828 281 Trânsito 1130±10 0.94 5629 [59] Também chamado Kepler-86b
POTS-1b 2.31 0.941 3.1606296 0.03734 Trânsito 3900 0.69 4400 [60]
PSO J318.5−22 6.5 1.53 N/A N/A 1160 Imagem direta 80 N/A N/A Planeta interestelar[61]
ROXs 12b 16 210 Imagem direta 390 0.87 3850 [62]
ROXs 42Bb 9 157 Imagem direta 440 1 [62]
WASP-8c 9.45 4323 5.28 Vel. radial 280 1.03 5600 [63]
WASP-65b 1.55 1.112 2.3114243 0.0334 Trânsito 1000 0.93 5600 [64]
WASP-68b 0.95 1.24 5.084298 0.06206 Trânsito 962±8 1.24 5911 [65]
WASP-69b 0.26 1.057 3.8681382 0.04525 963 Trânsito 160 0.83 4715 [66]
WASP-70Ab 0.59 1.164 3.7130203 0.04853 1387 Trânsito 800 1.11 5763 [66]
WASP-73b 1.88 1.16 4.08722 0.05512 1790 Trânsito 1042±9 1.34 6036 [65]
WASP-75b 1.07 1.27 2.484193 0.0375 Trânsito 850 1.14 6100 [64][67]
WASP-76b 0.92 1.83 1.809886 0.033 2190 Trânsito 390 1.46 6250 [68]
WASP-80b 0.538 0.999 3.06785234 0.0344 Trânsito 200 0.58 4143 [69] Nome próprio Wadirum
WASP-82b 1.24 1.67 2.705782 0.0447 2190 Trânsito 650 1.63 6490 [68]
WASP-84b 0.694 0.942 8.5234865 0.0771 797 Trânsito 410 0.84 5314 [66]
WASP-88b 0.56 1.7 4.954 0.06431 1775 Trânsito 1730±30 1.45 6431 [65]
WASP-90b 0.63±0.07 1.63±0.09 3.916243±0.000003 0.0562±0.0012 1840±50 Trânsito 1100±200 1.55±0.10 6440±130 [68]
WASP-95b 1.13 1.21 2.184673 0.03416 1570 Trânsito 450±2 1.11 5630 [70]
WASP-96b 0.48 1.2 3.4252602 0.0453 1285 Trânsito 1161±15 1.06 5540 [70]
WASP-97b 1.32 1.13 2.07276 0.03303 1555 Trânsito 494.9±1.7 1.12 5640 [70]
WASP-98b 0.922 1.144 2.96264036 0.03762 1180 Trânsito 926±5 0.81 5473 [70]
WASP-99b 2.78 1.1 5.75251 0.0717 1480 Trânsito 519±2 1.48 6180 [70]
WASP-100b 2.03 1.69 2.849375 0.0457 2190 Trânsito 1201±9 1.57 6900 [70]
WASP-101b 0.5 1.41 3.585722 0.0506 1560 Trânsito 660±3 1.34 6400 [70]
WTS-2b 1.12 1.363 1.0187068 0.01855 2000 Trânsito 3300 0.82 5000 [71][72]

Listas específicas de exoplanetas

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Referências

  1. ↑ «The Extrasolar Planets Encyclopaedia». Consultado em 9 de novembro de 2015 
  2. ↑ PLANETS AROUND LOW-MASS STARS. III. A YOUNG DUSTY L DWARF COMPANION AT THE DEUTERIUM-BURNING LIMIT
  3. ↑ a b BD+15 2940 AND HD 233604: TWO GIANTS WITH PLANETS CLOSE TO THE ENGULFMENT ZONE
  4. ↑ a b Transiting exoplanets from the CoRoT space mission XXIV. CoRoT-25b and CoRoT-26b: two low-density giant planets
  5. ↑ Sahlmann, J.; Lazorenko, P. F.; Ségransan, D.; Martín, Eduardo L.; Queloz, D.; Mayor, M.; Udry, S. (2013), «Astrometric orbit of a low-mass companion to an ultracool dwarf», Astronomy & Astrophysics, 556: A133, Bibcode:2013A&A...556A.133S, arXiv:1306.3225 , doi:10.1051/0004-6361/201321871 
  6. ↑ a b c Tuomi, M.; Anglada-Escudé, G. (2013). «Up to four planets around the M dwarf GJ 163». Astronomy & Astrophysics. 556: A111. arXiv:1306.1717 . doi:10.1051/0004-6361/201321174 
  7. ↑ a b c d e Lo Curto, G.; Mayor, M.; Benz, W.; Bouchy, F.; Hébrard, G.; Lovis, C.; Moutou, C.; Naef, D.; Pepe, F.; Queloz, D.; Santos, N. C.; Segransan, D.; Udry, S. (2013). «The HARPS search for southern extrasolar planets: XXXVI. New multi-planet systems in the HARPS volume limited sample: a super-Earth and a Neptune in the habitable zone». Astronomy & Astrophysics. 551. 7 páginas. Bibcode:2013A&A...551A..59L. arXiv:1301.2741 . doi:10.1051/0004-6361/201220415. A59 
  8. ↑ a b Arriagada, Pamela; Anglada-Escudé, Guillem; Butler, R. Paul; Crane, Jeffrey D.; Shectman, Stephen A.; Thompson, Ian; Wende, Sebastian; Minniti, Dante (2013), «Two planetary companions around the K7 dwarf GJ 221 : a hot super-Earth and a candidate in the sub-Saturn desert range», The Astrophysical Journal, 771 (1): 42, Bibcode:2013ApJ...771...42A, arXiv:1305.2203 , doi:10.1088/0004-637X/771/1/42 
  9. ↑ Simpson, Emilie R.; Fetherolf, Tara; Kane, Stephen R.; Li, Zhexing; Pepper, Joshua; Močnik, Teo (2022), «Revisiting BD-06 1339b: A Likely False Positive Caused by Stellar Activity», The Astronomical Journal, 163 (5): 215, arXiv:2203.06191 , doi:10.3847/1538-3881/ac5d41 
  10. ↑ Robertson, Paul; Endl, Michael; Cochran, William D.; MacQueen, Phillip J.; Boss, Alan P. (2013), «Secretly Eccentric: The Giant Planet and Activity Cycle of GJ 328», The Astrophysical Journal, 774 (2): 147, Bibcode:2013ApJ...774..147R, arXiv:1307.7640 , doi:10.1088/0004-637X/774/2/147 
  11. ↑ Kuzuhara, M.; Tamura, M.; Kudo, T.; Janson, M.; Kandori, R.; Brandt, T. D.; Thalmann, C.; Spiegel, D.; Biller, B.; et al. (2013). «Direct Imaging of a Cold Jovian Exoplanet in Orbit around the Sun-like Star GJ 504». The Astrophysical Journal. 774 (11). 11 páginas. Bibcode:2013ApJ...774...11K. arXiv:1307.2886 . doi:10.1088/0004-637X/774/1/11 
  12. ↑ a b c d Hartman, J. D.; Bakos, G. Á.; Torres, G.; Kovács, G.; Johnson, J. A.; Howard, A. W.; Marcy, G. W.; Latham, D. W.; Bieryla, A.; Buchhave, L. A.; Bhatti, W.; Béky, B.; Csubry, Z.; Penev, K.; De Val-Borro, M.; Noyes, R. W.; Fischer, D. A.; Esquerdo, G. A.; Everett, M.; Szklenár, T.; Zhou, G.; Bayliss, D.; Shporer, A.; Fulton, B. J.; Sanchis-Ojeda, R.; Falco, E.; Lázár, J.; Papp, I.; Sári, P. (2013), «HAT-P-44b, HAT-P-45b, AND HAT-P-46b: THREE TRANSITING HOT JUPITERS IN POSSIBLE MULTI-PLANET SYSTEMS», The Astronomical Journal, 147 (6): 128, arXiv:1308.2937 , doi:10.1088/0004-6256/147/6/128 
  13. ↑ Mohler-Fischer, M.; Mancini, L.; Hartman, J. D.; Bakos, G. Á.; Penev, K.; Bayliss, D.; Jordán, A.; Csubry, Z.; Zhou, G.; Rabus, M.; Nikolov, N.; Brahm, R.; Espinoza, N.; Buchhave, L. A.; Béky, B.; Suc, V.; Csák, B.; Henning, T.; Wright, D. J.; Tinney, C. G.; Addison, B. C.; Schmidt, B.; Noyes, R. W.; Papp, I.; Lázár, J.; Sári, P.; Conroy, P. (2013), «HATS-2b: A transiting extrasolar planet orbiting a K-type star showing starspot activity», Astronomy & Astrophysics, 558: A55, Bibcode:2013A&A...558A..55M, arXiv:1304.2140 , doi:10.1051/0004-6361/201321663 
  14. ↑ Bayliss, D.; Zhou, G.; Penev, K.; Bakos, G. Á.; Hartman, J. D.; Jordán, A.; Mancini, L.; Mohler-Fischer, M.; Suc, V.; Rabus, M.; Béky, B.; Csubry, Z.; Buchhave, L.; Henning, T.; Nikolov, N.; Csák, B.; Brahm, R.; Espinoza, N.; Noyes, R. W.; Schmidt, B.; Conroy, P.; Wright, D. J.; Tinney, C. G.; Addison, B. C.; Sackett, P. D.; Sasselov, D. D.; Lázár, J.; Papp, I.; Sári, P. (2013), «HATS-3b: An inflated hot Jupiter transiting an F-type star», The Astronomical Journal, 146 (5): 113, Bibcode:2013AJ....146..113B, arXiv:1306.0624 , doi:10.1088/0004-6256/146/5/113 
  15. ↑ a b c Sato, Bun'ei; Omiya, Masashi; Harakawa, Hiroki; Liu, Yu-Juan; Izumiura, Hideyuki; Kambe, Eiji; Takeda, Yoichi; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro; Ida, Shigeru (2013), «Planetary Companions to Three Evolved Intermediate-Mass Stars: HD 2952, HD 120084, andωSerpentis», Publications of the Astronomical Society of Japan, 65 (4): 85, arXiv:1304.4328 , doi:10.1093/pasj/65.4.85 
  16. ↑ a b c d e Moutou, Claire; Hébrard, Guillaume; Bouchy, François; Arnold, Luc; Santos, Nuno C.; Astudillo-Defru, Nicola; Boisse, Isabelle; Bonfils, Xavier; Borgniet, Simon; Delfosse, Xavier; Díaz, Rodrigo F.; Ehrenreich, David; Forveille, Thierry; Gregório, João; Labrevoir, Olivier; Lagrange, Anne-Marie; Montagnier, Guillaume; Montalto, Marco; Pepe, Francesco; Sahlmann, Johannes; Santerne, Alexandre; Ségransan, Damien; Udry, Stéphane; Vanhuysse, Michael (2013), The SOPHIE search for northern extrasolar planets VI. Three new hot Jupiters in multi-planet extrasolar systems, arXiv:1311.5271 , doi:10.1051/0004-6361/201322067 
  17. ↑ Wittenmyer, Robert A.; Wang, Songhu; Horner, Jonathan; Tinney, C. G.; Butler, R. P.; Jones, H. R. A.; O'Toole, S. J.; Bailey, J.; Carter, B. D.; Salter, G. S.; Wright, D.; Zhou, Ji-Lin (2013), «Forever Alone? Testing Single Eccentric Planetary Systems for Multiple Companions», The Astrophysical Journal Supplement Series, 208 (1): 2, Bibcode:2013ApJS..208....2W, arXiv:1307.0894 , doi:10.1088/0067-0049/208/1/2 
  18. ↑ Wittenmyer, Robert A.; et al. (2019). «Truly eccentric – I. Revisiting eight single-eccentric planetary systems». Monthly Notices of the Royal Astronomical Society. 484 (4): 5859–5867. Bibcode:2019MNRAS.484.5859W. arXiv:1901.08471 . doi:10.1093/mnras/stz290 
  19. ↑ Rameau, J., Chauvin, G., Lagrange, A.-M., Boccaletti, A., Quanz, S. P., Currie, T., Mawet, D., Girard, J. H., Bonnefoy, M., Kenworthy, M. (2013). «Confirmation of the planet around HD 95086 by direct imaging». The Astrophysical Journal. 779 (2): L26. Bibcode:2013ApJ...779L..26R. arXiv:1310.7483 . doi:10.1088/2041-8205/779/2/L26 
  20. ↑ Bailey, Vanessa; et al. (janeiro de 2014). «HD 106906 b: A planetary-mass companion outside a massive debris disk». The Astrophysical Journal Letters. 780 (1): L4. Bibcode:2014ApJ...780L...4B. arXiv:1312.1265 . doi:10.1088/2041-8205/780/1/L4 
  21. ↑ Borgniet, Simon; Boisse, Isabelle; Lagrange, Anne-Marie; Bouchy, François; Arnold, Luc; Díaz, Rodrigo F.; Galland, Franck; Delorme, Philippe; Hébrard, Guillaume; Santerne, Alexandre; Ehrenreich, David; Ségransan, Damien; Bonfils, Xavier; Delfosse, Xavier; Santos, Nuno C.; Forveille, Thierry; Moutou, Claire; Udry, Stéphane; Eggenberger, Anne; Pepe, Francesco; Astudillo-Defru, Nicola; Montagnier, Guillaume (2013), «Extrasolar planets and brown dwarfs around A--F type stars. VIII. A giant planet orbiting the young star HD113337», Astronomy & Astrophysics, 561: A65, arXiv:1310.1994 , doi:10.1051/0004-6361/201321783 
  22. ↑ Carleo, I.; et al. (2020). «The GAPS Programme at TNG XXI -- A GIARPS case-study of known young planetary candidates: Confirmation of HD 285507 b and refutation of AD Leo B». Astronomy & Astrophysics. A5: 638. Bibcode:2020A&A...638A...5C. arXiv:2002.10562 . doi:10.1051/0004-6361/201937369 
  23. ↑ Open exoplanet catalogue HD 285507
  24. ↑ Jones, M. I.; et al. (2013). «Study of the Impact of the Post-MS evolution of the Host Star on the Orbits of Close-in Planets. II. A Giant Planet in a Close-in Orbit around the RGB Star HIP 63242». Astronomy & Astrophysics. 556 (A78). 5 páginas. Bibcode:2013A&A...556A..78J. arXiv:1306.3939 . doi:10.1051/0004-6361/201321660 
  25. ↑ Pepper, Joshua; Siverd, Robert J.; Beatty, Thomas G.; Gaudi, B. Scott; Stassun, Keivan G.; Eastman, Jason; Collins, Karen; Latham, David W.; Bieryla, Allyson; Buchhave, Lars A.; Jensen, Eric L. N. (1 de agosto de 2013). «KELT-3b: A Hot Jupiter Transiting a V = 9.8 Late-F Star». The Astrophysical Journal. 773 (1). 64 páginas. Bibcode:2013ApJ...773...64P. ISSN 0004-637X. arXiv:1211.1031 . doi:10.1088/0004-637X/773/1/64 
  26. ↑ Collins, Karen A.; et al. (2013), «KELT-6b: AP∼ 7.9 DAY HOT SATURN TRANSITING a METAL-POOR STAR WITH a LONG-PERIOD COMPANION», The Astronomical Journal, 147 (2): 39, arXiv:1308.2296 , doi:10.1088/0004-6256/147/2/39 
  27. ↑ a b c Barclay, Thomas; et al. (2013), «A sub-Mercury-sized exoplanet», Nature, 494 (7438): 452–454, Bibcode:2013Natur.494..452B, PMID 23426260, arXiv:1305.5587 , doi:10.1038/nature11914 
  28. ↑ Exoplanet Characterization by Proxy: a Transiting 2.15 R_Earth Planet Near the Habitable Zone of the Late K dwarf Kepler-61 Sarah Ballard, David Charbonneau, Francois Fressin, Guillermo Torres, Jonathan Irwin, Jean-Michel Desert, Elisabeth Newton, Andrew W. Mann, David R. Ciardi, Justin R. Crepp, Christopher E. Henze, Stephen T. Bryson, Steven B. Howell, Elliott P. Horch, Mark E. Everett, Avi Shporer et al. April 26, 2013
  29. ↑ a b c d e Borucki, William J.; et al. (2013), «Kepler-62: A Five-Planet System with Planets of 1.4 and 1.6 Earth Radii in the Habitable Zone», Science, 340 (6132): 587–590, Bibcode:2013Sci...340..587B, PMID 23599262, arXiv:1304.7387 , doi:10.1126/science.1234702 
  30. ↑ Sanchis-Ojeda, Roberto; Winn, Joshua N.; Marcy, Geoffrey W.; Howard, Andrew W.; Isaacson, Howard; Johnson, John Asher; Torres, Guillermo; Albrecht, Simon; Campante, Tiago L.; Chaplin, William J.; Davies, Guy R.; Lund, Mikkel N.; Carter, Joshua A.; Dawson, Rebekah I.; Buchhave, Lars A.; Everett, Mark E.; Fischer, Debra A.; Geary, John C.; Gilliland, Ronald L.; Horch, Elliott P.; Howell, Steve B.; Latham, David W. (2013), «KEPLER-63b: A GIANT PLANET IN a POLAR ORBIT AROUND a YOUNG SUN-LIKE STAR», The Astrophysical Journal, 775 (1): 54, Bibcode:2013ApJ...775...54S, arXiv:1307.8128 , doi:10.1088/0004-637X/775/1/54 
  31. ↑ a b c Chaplin, W. J.; Sanchis-Ojeda, R.; Campante, T. L.; Handberg, R.; Stello, D.; Winn, J. N.; Basu, S.; Christensen-Dalsgaard, J.; Davies, G. R.; Metcalfe, T. S.; Buchhave, L. A.; Fischer, D. A.; Bedding, T. R.; Cochran, W. D.; Elsworth, Y.; Gilliland, R. L.; Hekker, S.; Huber, D.; Isaacson, H.; Karoff, C.; Kawaler, S. D.; Kjeldsen, H.; Latham, D. W.; Lund, M. N.; Lundkvist, M.; Marcy, G. W.; Miglio, A.; Barclay, T.; Lissauer, J. J. (2013), «Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65», The Astrophysical Journal, 766 (2): 101, Bibcode:2013ApJ...766..101C, arXiv:1302.3728 , doi:10.1088/0004-637X/766/2/101 
  32. ↑ a b The same frequency of planets inside and outside open clusters of stars
  33. ↑ a b c Gilliland, Ronald L.; et al. (2013). «Kepler-68: Three Planets, One with a Density Between That of Earth and Ice Giants». The Astrophysical Journal. 766 (1). 40. Bibcode:2013ApJ...766...40G . arXiv:1302.2596 . doi:10.1088/0004-637X/766/1/40 
  34. ↑ a b Barclay, Thomas; et al. (2013), «A Super-Earth-Sized Planet Orbiting in or Near the Habitable Zone Around a Sun-Like Star», The Astrophysical Journal, 768 (2): 101, Bibcode:2013ApJ...768..101B, arXiv:1304.4941 , doi:10.1088/0004-637X/768/2/101 
  35. ↑ Kane, Stephen R.; Barclay, Thomas; Gelino, Dawn M. (2013), «A Potential Super-Venus in the Kepler-69 System», The Astrophysical Journal, 770 (2): L20, Bibcode:2013ApJ...770L..20K, arXiv:1305.2933 , doi:10.1088/2041-8205/770/2/L20 
  36. ↑ a b Hébrard, G.; Almenara, J.-M.; Santerne, A.; Deleuil, M.; Damiani, C.; Bonomo, A. S.; Bouchy, F.; Bruno, G.; Díaz, R. F.; Montagnier, G.; Moutou, C. (2013), «KOI-200 b and KOI-889 b: Two transiting exoplanets detected and characterized with Kepler, SOPHIE, and HARPS-N», Astronomy & Astrophysics, 554: A114, Bibcode:2013A&A...554A.114H, arXiv:1304.6002 , doi:10.1051/0004-6361/201321394 
  37. ↑ Faigler, S.; et al. (2013). «BEER Analysis of Kepler and CoRoT Light Curves. I. Discovery of Kepler-76b: A Hot Jupiter with Evidence for Superrotation». The Astrophysical Journal. 771 (1). 26. Bibcode:2013ApJ...771...26F. arXiv:1304.6841 . doi:10.1088/0004-637X/771/1/26 
  38. ↑ Gandolfi, D.; Parviainen, H.; Fridlund, M.; Hatzes, A. P.; Deeg, H. J.; Frasca, A.; Lanza, A. F.; Prada Moroni, P. G.; Tognelli, E.; McQuillan, A.; Aigrain, S.; Alonso, R.; Antoci, V.; Cabrera, J.; Carone, L.; Csizmadia, Sz.; Djupvik, A. A.; Guenther, E. W.; Jessen-Hansen, J.; Ofir, A.; Telting, J. (2013), «Kepler-77b: A very low albedo, Saturn-mass transiting planet around a metal-rich solar-like star», Astronomy & Astrophysics, 557: A74, Bibcode:2013A&A...557A..74G, arXiv:1305.3891 , doi:10.1051/0004-6361/201321901 
  39. ↑ Ofir, Aviv; Dreizler, Stefan; Zechmeister, Mathias; Husser, Tim-Oliver (2013), «An independent planet search in the Keplerdataset», Astronomy & Astrophysics, 561: A103, arXiv:1310.2064 , doi:10.1051/0004-6361/201220935 
  40. ↑ a b Ofir, Aviv; Dreizler, Stefan; Zechmeister, Mathias; Husser, Tim-Oliver (2013), «An independent planet search in the Keplerdataset», Astronomy & Astrophysics, 561: A103, arXiv:1310.2064 , doi:10.1051/0004-6361/201220935 
  41. ↑ a b Nesvorný, David; Kipping, David; Terrell, Dirk; Hartman, Joel; Bakos, Gáspár Á.; Buchhave, Lars A. (2013), «Koi-142, the King of Transit Variations, is a Pair of Planets Near the 2:1 Resonance», The Astrophysical Journal, 777 (1): 3, Bibcode:2013ApJ...777....3N, arXiv:1304.4283 , doi:10.1088/0004-637X/777/1/3 
  42. ↑ Barros, S. C. C.; Díaz, R. F.; Santerne, A.; Bruno, G.; Deleuil, M.; Almenara, J.-M.; Bonomo, A. S.; Bouchy, F.; Damiani, C.; Hébrard, G.; Montagnier, G.; Moutou, C. (2013), «SOPHIE velocimetry of Keplertransit candidates», Astronomy & Astrophysics, 561: L1, arXiv:1311.4335 , doi:10.1051/0004-6361/201323067 
  43. ↑ a b c d Masuda, Kento; et al. (2013). «Characterization of the KOI-94 System with Transit Timing Variation Analysis: Implication for the Planet-Planet Eclipse». The Astrophysical Journal. 778 (2). 185. Bibcode:2013ApJ...778..185M . arXiv:1310.5771 . doi:10.1088/0004-637X/778/2/185 
  44. ↑ a b c d e f g h Schmitt, Joseph R.; et al. (2013), «Planet Hunters. Vi. An Independent Characterization of Koi-351 and Several Long Period Planet Candidates from Thekeplerarchival Data», The Astronomical Journal, 148 (2): 28, arXiv:1310.5912 , doi:10.1088/0004-6256/148/2/28 
  45. ↑ Lillo-Box, J.; Barrado, D.; Moya, A.; Montesinos, B.; Montalbán, J.; Bayo, A.; Barbieri, M.; Régulo, C.; Mancini, L.; Bouy, H.; Henning, T. (2013). «Kepler-91b: A planet at the end of its life. Planet and giant host star properties via light-curve variations». Astronomy & Astrophysics. 562: A109. Bibcode:2014A&A...562A.109L. arXiv:1312.3943 . doi:10.1051/0004-6361/201322001 
  46. ↑ a b c d e f g h i j k l m n o p q r s t u v w x y z aa ab ac ad Xie, Ji-Wei (2013), «Transit Timing Variation of Near-Resonance Planetary Pairs. Ii. Confirmation of 30 Planets in 15 Multiple-Planet Systems», The Astrophysical Journal Supplement Series, 210 (2): 25, arXiv:1309.2329 , doi:10.1088/0067-0049/210/2/25 
  47. ↑ a b c d Wang, Ji; Xie, Ji-Wei; Barclay, Thomas; Fischer, Debra A. (2013), «Influence of Stellar Multiplicity on Planet Formation. I. Evidence of Suppressed Planet Formation Due to Stellar Companions within 20 Au and Validation of Four Planets from Thekeplermultiple Planet Candidates», The Astrophysical Journal, 783: 4, arXiv:1309.7097 , doi:10.1088/0004-637X/783/1/4 
  48. ↑ a b c d e f Yang, Ming; Liu, Hui-Gen; Zhang, Hui; Zhou, Ji-Lin (2013), «8 Planets in 4 Multi-planet Systems via TTVs in 1350 Days», The Astrophysical Journal, 778 (2): 110, Bibcode:2013ApJ...778..110Y, arXiv:1308.0996 , doi:10.1088/0004-637X/778/2/110 
  49. ↑ Van Eylen, V.; Lund, M. N.; Aguirre, V. Silva; Arentoft, T.; Kjeldsen, H.; Albrecht, S.; Chaplin, W. J.; Isaacson, H.; Pedersen, M. G.; Jessen-Hansen, J.; Tingley, B.; Christensen-Dalsgaard, J.; Aerts, C.; Campante, T. L.; Bryson, S. T. (2013), «WHAT ASTEROSEISMOLOGY CAN DO FOR EXOPLANETS: KEPLER-410A b IS a SMALL NEPTUNE AROUND a BRIGHT STAR, IN AN ECCENTRIC ORBIT CONSISTENT WITH LOW OBLIQUITY», The Astrophysical Journal, 782: 14, arXiv:1312.4938 , doi:10.1088/0004-637X/782/1/14 
  50. ↑ Wang, Ji; et al. (2015), «Planet Hunters. Viii. Characterization of 41 Long-Period Exoplanet Candidates from Kepler Archival Data», The Astrophysical Journal, 815 (2): 127, Bibcode:2015ApJ...815..127W, arXiv:1512.02559 , doi:10.1088/0004-637X/815/2/127 
  51. ↑ Suzuki, D.; et al. (2013), «MOA-2008-BLG-379Lb: A MASSIVE PLANET FROM a HIGH MAGNIFICATION EVENT WITH a FAINT SOURCE», The Astrophysical Journal, 780 (2): 123, arXiv:1311.3424 , doi:10.1088/0004-637X/780/2/123 
  52. ↑ Furusawa, K.; et al. (2013), «MOA-2010-BLG-328Lb: A SUB-NEPTUNE ORBITING VERY LATE M DWARF?», The Astrophysical Journal, 779 (2): 91, Bibcode:2013ApJ...779...91F, arXiv:1309.7714 , doi:10.1088/0004-637X/779/2/91 
  53. ↑ a b MOA-2011-BLG-262Lb: A SUB-EARTH-MASS MOON ORBITING A GAS GIANT PRIMARY OR A HIGH VELOCITY PLANETARY SYSTEM IN THE GALACTIC BULGE
  54. ↑ Batista, V.; Beaulieu, J. -P.; Gould, A.; Bennett, D. P.; Yee, J. C.; Fukui, A.; Gaudi, B. S.; Sumi, T.; Udalski, A. (2013), «MOA-2011-BLG-293Lb: First Microlensing Planet possibly in the Habitable Zone», The Astrophysical Journal, 780: 54, arXiv:1310.3706 , doi:10.1088/0004-637X/780/1/54 
  55. ↑ Shvartzvald, Y.; et al. (2013), «MOA-2011-BLG-322Lb: A 'second generation survey' microlensing planet», Monthly Notices of the Royal Astronomical Society, 439: 604–610, arXiv:1310.0008 , doi:10.1093/mnras/stt2477 
  56. ↑ Kains, N.; Street, R. A.; Choi, J.-Y.; Han, C.; Udalski, A.; Almeida, L. A.; Jablonski, F.; Tristram, P. J.; Jørgensen, U. G.; Szymański, M. K.; Kubiak, M.; Pietrzyński, G.; Soszyński, I.; Poleski, R.; Kozłowski, S.; Pietrukowicz, P.; Ulaczyk, K.; Wyrzykowski, Ł.; Skowron, J.; Alsubai, K. A.; Bozza, V.; Browne, P.; Burgdorf, M. J.; Calchi Novati, S.; Dodds, P.; Dominik, M.; Dreizler, S.; Fang, X.-S.; Grundahl, F.; et al. (2013), «A Giant Planet beyond the Snow Line in Microlensing Event OGLE-2011-BLG-0251», Astronomy & Astrophysics, 552: A70, Bibcode:2013A&A...552A..70K, arXiv:1303.1184 , doi:10.1051/0004-6361/201220626 
  57. ↑ Han, C.; et al. (2013), «Microlensing Discovery of a Tight, Low-Mass-Ratio Planetary-Mass Object Around an Old Field Brown Dwarf», The Astrophysical Journal, 778 (1): 38, Bibcode:2013ApJ...778...38H, arXiv:1307.6335 , doi:10.1088/0004-637X/778/1/38 
  58. ↑ Poleski, Radosław; Udalski, Andrzej; Dong, Subo; Szymański, Michał K.; Soszyński, Igor; Kubiak, Marcin; Pietrzyński, Grzegorz; Kozłowski, Szymon; Pietrukowicz, Paweł; Ulaczyk, Krzysztof; Skowron, Jan; Wyrzykowski, Łukasz; Gould, Andrew (2014), «SUPER-MASSIVE PLANETS AROUND LATE-TYPE STARS—THE CASE OF OGLE-2012-BLG-0406Lb», The Astrophysical Journal, 782 (1): 47, Bibcode:2014ApJ...782...47P, arXiv:1307.4084 , doi:10.1088/0004-637X/782/1/47 
  59. ↑ Wang, Ji (3 de janeiro de 2013). «Planet Hunters. V. A Confirmed Jupiter-Size Planet in the Habitable Zone and 42 Planet Candidates from the Kepler Archive Data». arXiv:1301.0644v1  [astro-ph] 
  60. ↑ Koppenhoefer, J.; Saglia, R. P.; Fossati, L.; Lyubchik, Y.; Mugrauer, M.; Bender, R.; Lee, C.- H.; Riffeser, A.; Afonso, P.; Greiner, J.; Henning, T.; Neuhauser, R.; Snellen, I. A. G.; Pavlenko, Y.; Verdugo, M.; Vogt, N. (2013), «A hot Jupiter transiting a mid-K dwarf found in the pre-Omega Cam Transit Survey», Monthly Notices of the Royal Astronomical Society, 435 (4): 3133–3147, arXiv:1308.6574 , doi:10.1093/mnras/stt1512 
  61. ↑ Michael C. Liu; Eugene A. Magnier; Niall R. Deacon; Katelyn N. Allers; et al. (1 de outubro de 2013). «The Extremely Red, Young L Dwarf PSO J318-22: A Free-Floating Planetary-Mass Analog to Directly Imaged Young Gas-Giant Planets». Astrophysical Journal Letters. 777 (2). Bibcode:2013ApJ...777L..20L. arXiv:1310.0457 . doi:10.1088/2041-8205/777/2/L20 
  62. ↑ a b Kraus, Adam L.; Ireland, Michael J.; Cieza, Lucas A.; Hinkley, Sasha; Dupuy, Trent J.; Bowler, Brendan P.; Liu, Michael C. (2013), «THREE WIDE PLANETARY-MASS COMPANIONS TO FW TAU, ROXs 12, AND ROXs 42B», The Astrophysical Journal, 781: 20, arXiv:1311.7664 , doi:10.1088/0004-637X/781/1/20 
  63. ↑ Knutson, Heather A.; Fulton, Benjamin J.; Montet, Benjamin T.; Kao, Melodie; Ngo, Henry; Howard, Andrew W.; Crepp, Justin R.; Hinkley, Sasha; Bakos, Gaspar A.; Batygin, Konstantin; John Asher Johnson; Morton, Timothy D.; Muirhead, Philip S. (2013), «Friends of Hot Jupiters. I. A Radial Velocity Search for Massive, Long-Period Companions to Close-In Gas Giant Planets», The Astrophysical Journal, 785 (2): 126, arXiv:1312.2954 , doi:10.1088/0004-637X/785/2/126 
  64. ↑ a b Gómez Maqueo Chew, Y.; Faedi, F.; Pollacco, D.; Brown, D. J. A.; Doyle, A. P.; Collier Cameron, A.; Gillon, M.; Lendl, M.; Smalley, B.; Triaud, A. H. M. J.; West, R. G.; Wheatley, P. J.; Busuttil, R.; Liebig, C.; Anderson, D. R.; Armstrong, D. J.; Barros, S. C. C.; Bento, J.; Bochinski, J.; Burwitz, V.; Delrez, L.; Enoch, B.; Fumel, A.; Haswell, C. A.; Hébrard, G.; Hellier, C.; Holmes, S.; Jehin, E.; Kolb, U.; et al. (2013), «Discovery of WASP-65b and WASP-75b: Two Hot Jupiters Without Highly Inflated Radii», Astronomy & Astrophysics, 559: A36, Bibcode:2013A&A...559A..36G, arXiv:1307.6532 , doi:10.1051/0004-6361/201322314 
  65. ↑ a b c Delrez, L.; Van Grootel, V.; Anderson, D. R.; Collier-Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M.; Neveu-VanMalle, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Udry, S.; West, R. G. (2013), «Transiting planets from WASP-South, Euler and TRAPPIST:WASP-68 b, WASP-73 b and WASP-88 b, three hot Jupiters transiting evolved solar-type stars», Astronomy and Astrophysics, 563, Bibcode:2014A&A...563A.143D, arXiv:1312.1827 , doi:10.1051/0004-6361/201323204 
  66. ↑ a b c Anderson, D. R.; Collier Cameron, A.; Delrez, L.; Doyle, A. P.; Faedi, F.; Fumel, A.; Gillon, M.; Gómez Maqueo Chew, Y.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Skillen, I.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Turner, O. D.; Udry, S.; West, R. G. (2013), Three sub-Jupiter-mass planets: WASP-69b & WASP-84b transit active K dwarfs and WASP-70Ab transits the evolved primary of a G4+K3 binary, arXiv:1310.5654 , doi:10.1093/mnras/stu1737 
  67. ↑ Clark, B. J. M.; Anderson, D. R.; Hellier, C.; Turner, O. D.; Močnik, T. (2013), «An Analysis of Transiting Hot Jupiters Observed with K2: WASP-55b and WASP-75b», Publications of the Astronomical Society of the Pacific, 130 (985): 034401, arXiv:1802.02132 , doi:10.1088/1538-3873/aaa33e 
  68. ↑ a b c West, R. G.; Hellier, C.; Almenara, J.-M.; Anderson, D. R.; Barros, S. C. C.; Bouchy, F.; Brown, D. J. A.; Collier Cameron, A.; Deleuil, M.; Delrez, L.; Doyle, A. P.; Faedi, F.; Fumel, A.; Gillon, M.; Gómez Maqueo Chew, Y.; Hébrard, G.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Udry, S. (2016), «Three irradiated and bloated hot Jupiters», Astronomy & Astrophysics, 585: A126, Bibcode:2016A&A...585A.126W, arXiv:1310.5607 , doi:10.1051/0004-6361/201527276 
  69. ↑ Triaud, A. H. M. J.; Anderson, D. R.; Collier Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M.; Lovis, C.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Udry, S.; West, R. G.; Wheatley, P. J. (2013), «WASP-80b: a gas giant transiting a cool dwarf», Astronomy & Astrophysics, 551: A80, Bibcode:2013A&A...551A..80T, arXiv:1303.0254 , doi:10.1051/0004-6361/201220900 
  70. ↑ a b c d e f g Hellier, Coel; Anderson, D. R.; Cameron, A. Collier; Delrez, L.; Gillon, M.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Udry, S.; West, R. G. (2013), «Transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-95b to WASP-101b», Monthly Notices of the Royal Astronomical Society, 440 (3): 1982–1992, arXiv:1310.5630 , doi:10.1093/mnras/stu410 
  71. ↑ WTS-2 b: Too close for comfort?
  72. ↑ Birkby, J. L.; et al. (2014), «WTS-2 b: A hot Jupiter orbiting near its tidal destruction radius around a K dwarf», Monthly Notices of the Royal Astronomical Society, 440 (2): 1470–1489, arXiv:1402.5416 , doi:10.1093/mnras/stu343 
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