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Lista de exoplanetas descobertos em 2012

Esta é uma Lista de exoplanetas descobertos em 2012.[1]

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) Método de descoberta Distância (ly) Massa da estrela-mãe (M☉) Temperatura da estrela-mãe (K) Observações
75 Ceti b 3 691.9 2.1 Vel. radial 266 2.49 4846 [2]
BD+20 274 b 4.2 578.2 1.3 Vel. radial 4500±300 0.8 4296 [3]
BD+48 740 b 1.7±0.7 733+5
−8 		1.7±0.1 Vel. radial 2214±72 1.09±0.16 4534±8 [4] Confirmed in 2018.[5]
CoRoT-21b 2.26 1.3 2.72 0.0417 1867 Trânsito 4600±900 1.29 6200 [6]
Epsilon Coronae Borealis b 6.7 417.9 1.3 Vel. radial 229.7 1.7 4406 [7]
Gliese 676 Ad 0.014 3.6005 0.0413±0.0014 Vel. radial 52.29±0.03 0.71±0.04 3734 [8]
Gliese 676 Ae 0.025 35.39 0.187±0.007 Vel. radial 52.29±0.03 0.71±0.04 3734 [8]
Gliese 3470 b 0.043 0.346 3.3366487 0.031 Vel. radial 82 0.51 3652 [9]
HAT-P-34b 7.01 1.35 5.45265 0.06774 1520 Trânsito 818.94 4.26 6442 [10] Nome próprio Ġgantija
HAT-P-35b 7.52 3.55 3.64671 0.0498 1581 Trânsito 1677 23.56 6096 [10]
HAT-P-36b 1.8482 1.277 1.32734683 0.0241 1781 Trânsito 968.49 1.03 5620 [10] Nome próprio Bran
HAT-P-37b 1.169 1.178 2.797436 0.0379 1271 Trânsito 1341 0.93 5500 [10] Additional planets in system are suspected[11]
HAT-P-38b 0.267 0.825 4.640382 0.0523 Trânsito 810 0.89 5330 [12] Nome próprio Hiisi
HAT-P-39b 0.599 1.571 3.54387 0.0509 Trânsito 2090 1.4 6430 [13]
HAT-P-40b 0.615 1.73 4.457243 0.0608 Trânsito 1630 1.51 6080 [13] Nome próprio Vytis
HAT-P-41b 0.8 1.685 2.694047 0.0426 Trânsito 1120 1.42 6390 [14][13][15]
HAT-P-42b 1.044 1.28 4.641878 0.0575 1427 Trânsito 1460 1.18 5743 [16] Nome próprio Iolaus
HAT-P-43b 0.662 1.281 3.332687 0.0443 1361 Trânsito 1770 1.05 5645 [16]
HATS-1b 1.855 1.302 3.446459 0.0444 Trânsito 990 0.99 5870 [17]
HD 142 c 5.3 6005 6.8 Vel. radial 83.6 1.23 6245 [18]
HD 4732 b 2.37 360.2 1.19 Vel. radial 184 1.74 4959 [19]
HD 4732 c 2.37 2732 4.6 Vel. radial 184 1.74 4959 [19]
HD 5608 b 1.4 792.6 1.9 Vel. radial 189.7 1.55 4854 [2]
HD 24040 b 4.10±0.12 3490±25 4.637±0.067 Vel. radial 152.3±0.4 1.14±0.02 5917±52 [20] Suspeito desde 2006
HD 27631 b 1.45 2208 3.25 Vel. radial 145.3 0.94 5737 [21]
HD 37605 c 3.366 2720 3.814 Vel. radial 139.9 1 5448 [22]
HD 40307 e 0.0110±0.0044 34.62+0.21
−0.20 		0.1886+0.083
−0.0104 		Vel. radial 41.8 0.77 4956 [23]
HD 40307 f 0.0164 51.76 0.247 Vel. radial 41.8 0.77 4956 [23]
HD 40307 g 0.0223 197.8 0.6 Vel. radial 41.8 0.77 4956 [23]
HD 66141 b 6 480.5 1.2 Vel. radial 261.1 1.1 4323 [24]
HD 77338b 0.05 5.7361 0.0614 Vel. radial 134.6 0.93 5370 [25]
HD 79498 b 1.34 1807 2.98 Vel. radial 159.89 1.08 5748 [26]
HD 98649 b 6.8 4951 5.6 Vel. radial 139.5 1 5759 [21]
HD 106515 Ab 9.61 3630 4.59 Vel. radial 118.6 0.97 5362 [21]
HD 150706 b 2.71 5894 6.7 Vel. radial 88.8 1.17 5961 [20]
HD 159868 c 0.73 352.3 1 Vel. radial 171.9 1.09 5558 [18]
HD 166724 b 3.53 5144 5.42 Vel. radial 140.2 0.81 5127 [21]
HD 197037 b 0.79 1035.7 2.07 Vel. radial 107.1 1.063±0.022 6137±20 [26]
HD 207832 b 0.56 161.97 0.57 Vel. radial 180.4 0.94 5710 [27] Suspeita de falso positivo[28]
HD 207832 c 0.73 1155.7 2.112 Vel. radial 180.4 0.94 5710 [27] Suspeita de falso positivo[28]
HD 208527 b 9.9 875.5 2.1 Vel. radial 1148.4 1.6 4035 [29]
HD 219077 b 10.39 5501 6.22 Vel. radial 95 1.05 5362 [21]
HD 219415 b 1 2093.3 3.2 Vel. radial 553.7 1 4820 [3]
HD 220074 b 11.1 672.1 1.6 Vel. radial 942.7 1.2 3935 [29]
HD 220689 b 1.06 2209 3.36 Vel. radial 147.5 1.04 5921 [21]
HD 220773 b 1.45 3724.7 4.94 Vel. radial 159.82 1.16 5940 [26]
HD 222155 b 2.12 3999 5.14 Vel. radial 165.3 1.21 5701 [20]
HW Virginis b 14.3 4640 4.69 Tempo 590 0.485 [30] Provavelmente falso positivo[31]
Kappa Andromedae b 13.616 55 1850 Imagem direta 169.7 2.6 10900 Tem uma cor avermelhada e pode ser uma anã marrom[32]
KELT-1b 27.23 1.11 1.217514 0.02466 2423 Trânsito 850 1.32 6518 [33]
KELT-2Ab 1.522 1.286 4.1137912 0.05496 Trânsito 405.2 1.31 6151 [34]
Kepler-30b 0.036 0.348 29.33434 0.18 Trânsito 4600 0.99 5498 [35]
Kepler-30c 2.01 1.097 60.323105 0.3 Trânsito 4600 0.99 5498 [35]
Kepler-30d 0.073 0.785 143.34394 0.5 Trânsito 4600 0.99 5498 [35]
Kepler-32d 0.241 22.7802 0.13 Trânsito 990 0.58 3900 [35]
Kepler-32e 0.134 2.896 0.033 Trânsito 990 0.58 3900 Evidência fraca[35]
Kepler-32f 0.073 0.74296 0.013 Trânsito 990 0.58 3900 Evidência fraca[35]
Kepler-33f 0.03036 0.398 41.02902 0.2535 Trânsito 4086 1.29 5904 [36]
Kepler-34b 0.22 0.764 288.822 1.0896 Trânsito 4889 1.05 5913 [37]
Kepler-35b 0.127 0.728 131.458 0.60347 Trânsito 5365 0.89 5606 [37]
Kepler-36b 0.014 0.133 13.83989 0.1153 Trânsito 1500 1.07 5911 [38]
Kepler-36c 0.025 0.328 16.23855 0.1283 Trânsito 1500 1.07 5911 [38]
Kepler-38b 0.384 0.384 105.599 0.4632 Trânsito 2000 0.94 5623 [39]
Kepler-46b 6 0.808 33.60134 0.1968 Trânsito 2790 0.9 5309 [40]
Kepler-46c 0.376 57.011 0.2799 Tempo 2790 0.9 5309 [40]
Kepler-47b 2 0.27 49.532 0.2962 Trânsito 4900 1.05 5636 [41]
Kepler-47c 28 0.411 303.137 0.991 Trânsito 4900 1.05 5636 [41]
Kepler-48b 0.0124 0.168 4.778 Trânsito 1009±5 0.88 5194 [42][43]
Kepler-48c 0.04597 0.242 9.67395 Trânsito 1009±5 0.88 5194 [42][43]
Kepler-49b 0.98 0.243 7.2037945 Trânsito 1024±8 0.55 4252 [42][43]
Kepler-49c 0.72 0.227 10.9129343 Trânsito 1024±8 0.55 4252 [42][43]
Kepler-50b 0.153 7.81254 0.077 Trânsito 821±6 1.24 6225 [43]
Kepler-50c 0.194 9.37647 0.087 Trânsito 821±6 1.24 6225 [43]
Kepler-51b 0.007 0.633 45.154 0.2514 543 Trânsito 2610±50 1.04 6018 [43]
Kepler-51c 0.013 0.803 85.312 0.384 439 Trânsito 2610±50 1.04 6018 [43]
Kepler-52b 8.7 0.187 7.8773565 Trânsito 1058±7 0.54 4263 [43]
Kepler-52c 10.41 0.164 16.3850021 Trânsito 1058±7 0.54 4263 [43]
Kepler-53b 18.41 0.258 18.6489525 Trânsito 4600±200 0.98 5858 [42][43]
Kepler-53c 15.74 0.283 38.5583038 Trânsito 4600±200 0.98 5858 [42][43]
Kepler-54b 0.92 0.187 8.0109434 Trânsito 893±9 0.51 4252 [43]
Kepler-54c 0.37 0.11 12.0717249 Trânsito 893±9 0.51 4252 [43]
Kepler-55b 1.49 0.217 27.9481449 Trânsito 1920±30 0.62 4503 [43]
Kepler-55c 1.11 0.197 42.1516418 Trânsito 1920±30 0.62 4503 [43]
Kepler-56b 0.07 0.581 10.5016 0.1028 Trânsito 3060±80 1.32 4840 [43]
Kepler-56c 0.57 0.874 21.40239 0.1652 Trânsito 3060±80 1.32 4840 [43]
Kepler-57b 18.86 0.195 5.7293196 Trânsito 3140±30 0.83 5145 [42][43]
Kepler-57c 6.95 0.138 11.6092567 Trânsito 3140±30 0.83 5145 [42][43]
Kepler-58b 1.39 0.248 10.2184954 Trânsito 3250±80 0.95 6099 [42][43]
Kepler-58c 2.19 0.255 15.5741568 Trânsito 3250±80 0.95 6099 [42][43]
Kepler-59b 2.05 0.098 11.8681707 Trânsito 3925±75 1.04 6074 [43]
Kepler-59c 1.37 0.177 17.9801235 Trânsito 3925±75 1.04 6074 [43]
Kepler-60b 0.01318 0.153 7.1334 Trânsito 3440±70 1.04 5905 [43]
Kepler-60c 0.01211 0.17 8.9187 Trânsito 3440±70 1.04 5905 [43]
Kepler-60d 0.01309 0.178 11.8981 Trânsito 3440±70 1.04 5905 [43]
Kepler-64b 0.531 0.551 138.317 0.652 Trânsito 6200±1000 1.53 6407 [44] Sistema estelar quádruplo
Kepler-79b 0.0343 0.31 13.4845 0.117 868 Trânsito 3430±60 1.17 6174 [42]
Kepler-79c 0.019 0.332 27.4029 0.187 685 Trânsito 3430±60 1.17 6174 [42]
Kepler-80b 0.0218 0.238 7.05246 0.0648 Trânsito 1160 0.73 4540 [42]
Kepler-80c 0.02121 0.244 9.52355 0.0792 Trânsito 1160 0.73 4540 [42]
Kepler-81b 0.216 5.955 646 Trânsito 1147±10 0.64 4500 [42]
Kepler-81c 0.211 12.04 513 Trânsito 1147±10 0.64 4500 [42]
Kepler-82b 0.357 26.444 581 Trânsito 3030±80 0.85 5428 [42]
Kepler-82c 0.477 51.538 464 Trânsito 3030±80 0.85 5428 [42]
Kepler-83b 0.252 9.77 Trânsito 1320±17 0.66 4648 [42][45]
Kepler-83c 0.211 20.09 Trânsito 1320±17 0.66 4648 [42][45]
Kepler-84b 0.199 8.726 937 Trânsito 4700±500 1 6031 [42][45]
Kepler-84c 0.211 12.883 821 Trânsito 4700±500 1 6031 [42][45]
Kepler-85b 0.176 8.306 Trânsito 2550±50 0.92 5436 [42] KOI-2038[46]
Kepler-85c 0.194 12.513 Trânsito 2550±50 0.92 5436 [42] KOI-2038[46]
MOA-2011-BLG-293Lb 2.4+1.4
−0.9 		1.0±0.1 Microlente 23000±2000 0.675±0.525 [47]
MOA-2010-BLG-073Lb 11 1.21 Microlente 9100 0.16 Possivelmente anã marrom[48]
MOA-2010-BLG-477Lb 1.4±0.3 2.8±0.5 Microlente 7500±2000 0.53±0.11 5950±150 [49] Estrela-mãe anã branca[50]
MOA-bin-1Lb 3.7±2.1 8.3+4.5
−2.7 		Microlente 17000 0.75+0.33
−0.41 		[51]
Mu2 Octantis b 6.9 3638 5.02 Vel. radial 142.1 1.29 6017 [21]
Nu Ophiuchi b 24 530.32 1.9 Vel. radial 152.8 3.04 4928 Anã marrom ou pequena estrela[2]
Nu Ophiuchi c 27 3186 6.1 Vel. radial 152.8 3.04 4928 Anã marrom ou pequena estrela[2]
OGLE-2012-BLG-0026Lb 0.145 4 Microlente 13110 1.06 [52]
OGLE-2012-BLG-0026Lc 0.86 4.8 Microlente 13110 1.06 [52]
Omicron Coronae Borealis b 1.5 187.83 0.83 Vel. radial 274.1 2.13 4749 [2]
Omicron Ursae Majoris b 4.1 1630 3.9 Vel. radial 183.7 3.09 5242 [2]
Pr0201 b 0.54 4.4264 Vel. radial 610 1.23 6174 [53] Em Messier 44
Pr0211 b 1.88 2.1461 0.03176 Vel. radial 610 0.94 5300 [53] Sistema multiplanetário em Messier 44
RR Caeli b 3.0±0.3 1900±40 5.2±0.1 Tempo 69.10±0.03 0.18+0.44 3100+7540 Planeta circumbinário em torno de anãs vermelhas e brancas.[54][55]
Tau Ceti e 0.0124 162.87 0.538 Vel. radial 12 0.78 [56] Exoplaneta potencialmente habitável
Tau Ceti f 0.0124 636.13 1.334 Vel. radial 12 0.78 [56]
WASP-42b 0.527 1.122 4.9816819 0.0561 1021±19 Trânsito 520 0.95 5315 [57]
WASP-47b 1.21 1.15 4.16071 0.052 1275 Trânsito 650 1.11 5576 [58]
WASP-49b 0.378 1.115 2.7817387 0.0379 1369±39 Trânsito 550 0.94 5600 [57]
WASP-52b 0.46 1.27 1.7497798 0.0272 1315±35 Trânsito 460 0.87 5000 [59] Nome próprio Göktürk
WASP-54b 0.636 1.653 3.6936411 0.04987 1742+49
−69 		Trânsito 650 1.21 6100 [60]
WASP-55b 0.627 1.335 4.4656291 0.0558 1290 Trânsito 1100 1.16 6070 [58]
WASP-56b 0.571 1.092 4.617101 0.05458 1200 Trânsito 830 1.03 5600 [60]
WASP-57b 0.644 1.05 2.83891856 0.03769 1338±29 Trânsito 1480 0.89 5600 [60]
WASP-58b 0.89 1.37 5.01718 0.0561 1270±80 Trânsito 980 0.94 5800 [59]
WASP-59b 0.863 0.775 7.919585 0.0697 670±35 Trânsito 410 0.72 4650 [59]
WASP-60b 0.514 0.86 4.3050011 0.0531 1479±35 Trânsito 1300 1.08 5900 [59] Nome próprio Vlasina
WASP-61b 2.06 1.24 3.8559 0.0514 1565±35 Trânsito 1600 1.22 6320 [58]
WASP-62b 0.57 1.39 4.411953 0.0567 1329.6±44.8 Trânsito 520 1.25 6280 [58] Nome próprio Krotoa
WASP-63b 0.38 1.43 4.37809 0.0574 1536±37 Trânsito 1100 1.32 5570 [58]
WASP-64b 1.271 1.271 1.5732918 0.02648 1989+87
−88 		Trânsito 1100 1 5400 [61] Nome próprio Agouto
WASP-66b 2.32 1.39 4.086052 0.0546 1790±60 Trânsito 1200 1.3 6580 [58]
WASP-67b 0.42 1.4 4.61442 0.0517 1050 Trânsito 730 0.87 5240 [58]
WASP-71b 2.242 1.46 2.9036747 0.04619 2016.1+67.0
−52.5 		Trânsito 1130 1.56 6059 [62] Nome próprio Tanzanite
WASP-72b 1.5461 1.27 2.2167421 0.03708 2210+120
−130 		Trânsito 1100 1.39 6250 [61] Nome próprio Cuptor
WASP-77Ab 1.76 1.21 1.3600309 0.024 1715 Trânsito 300 1 5500 Orbitando estrela primária do sistema estelar binário[63]
WASP-78b 0.89 1.7 2.17517632 0.0362 2350 Trânsito 1800 1.17 6100 [64]
WASP-79b 0.9 2.09 3.6623866 0.0535 1900±50 Trânsito 780 1.38 6600 [64] Nome próprio Pollera
WISE 1217+1626 B 22 0.934 8 450 Imagem direta 29±3 0.03 575 Anã marrom[65]
WTS-1b 4.01 1.49 3.352057 0.047 1500±100 Trânsito 8100±1000 1.2 6250 [66]

Listas específicas de exoplanetas

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Referências

  1. ↑ «NASA Exoplanet Archive». Consultado em 20 de dezembro de 2019 
  2. ↑ a b c d e f Sato, Bun'ei; et al. (2012). «Substellar Companions to Seven Evolved Intermediate-Mass Stars». Publications of the Astronomical Society of Japan. 64 (6). 135. Bibcode:2012PASJ...64..135S. arXiv:1207.3141 . doi:10.1093/pasj/64.6.135 
  3. ↑ a b Gettel, S.; Wolszczan, A.; Niedzielski, A.; Nowak, G.; Adamów, M.; Zieliński, P.; MacIejewski, G. (2012), «Planets Around the K-Giants Bd+20 274 and Hd 219415», The Astrophysical Journal, 756 (1): 53, Bibcode:2012ApJ...756...53G, arXiv:1207.0488 , doi:10.1088/0004-637X/756/1/53 
  4. ↑ Adamów, M.; Niedzielski, A.; Villaver, E.; Nowak, G.; Wolszczan, A. (2012). «BD+48 740—Li Overabundant Giant Star with a Planet: A Case of Recent Engulfment?». The Astrophysical Journal. 754 (1): L15. Bibcode:2012ApJ...754L..15A. arXiv:1206.4938 . doi:10.1088/2041-8205/754/1/L15 
  5. ↑ Adamów, M.; Niedzielski, A.; Kowalik, K.; Villaver, E.; Wolszczan, A.; MacIejewski, G.; Gromadzki, M. (2018), «Tracking Advanced Planetary Systems (TAPAS) with HARPS-N», Astronomy & Astrophysics, 613: A47, arXiv:1801.04379 , doi:10.1051/0004-6361/201732161 
  6. ↑ Transiting exoplanets from the CoRoT space mission XXIII. CoRoT-21b: a doomed large Jupiter around a faint subgiant star
  7. ↑ Lee, B.-C.; Han, I.; Park, M.-G.; Mkrtichian, D. E.; Kim, K.-M. (2012). «A planetary companion around the K giant ɛ Corona Borealis». Astronomy & Astrophysics. 546. 5 páginas. Bibcode:2012A&A...546A...5L. arXiv:1209.1187 . doi:10.1051/0004-6361/201219347. A5 
  8. ↑ a b Anglada-Escudé, Guillem; Tuomi, Mikko (2012). «A planetary system with gas giants and super-Earths around the nearby M dwarf GJ 676A. Optimizing data analysis techniques for the detection of multi-planetary systems» (PDF). Astronomy. 548: A58. Bibcode:2012A&A...548A..58A. arXiv:1206.7118 . doi:10.1051/0004-6361/201219910 
  9. ↑ Bonfils, Xavier; Gillon, Michaël; Udry, Stéphane; Armstrong, David; Bouchy, François; Delfosse, Xavier; Forveille, Thierry; Fumel, Aurélie; Jehin, Emmanuël; Lendl, Monika; Lovis, Christophe; Mayor, Michel; McCormac, James; Neves, Vasco; Pepe, Francesco; Perrier, Christian; Pollacco, Don L.; Queloz, Didier; Santos, Nuno C. (2012). «A hot Uranus transiting the nearby M dwarf GJ3470. Detected with HARPS velocimetry. Captured in transit with TRAPPIST photometry». Astronomy & Astrophysics. 546: A27. Bibcode:2012A&A...546A..27B. arXiv:1206.5307 . doi:10.1051/0004-6361/201219623 
  10. ↑ a b c d Bakos, G. Á.; Hartman, J. D.; Torres, G.; Béky, B.; Latham, D. W.; Buchhave, L. A.; Csubry, Z.; Kovács, G.; Bieryla, A.; Quinn, S.; Szklenár, T.; Esquerdo, G. A.; Shporer, A.; Noyes, R. W.; Fischer, D. A.; Johnson, J. A.; Howard, A. W.; Marcy, G. W.; Sato, B.; Penev, K.; Everett, M.; Sasselov, D. D.; Fűrész, G.; Stefanik, R. P.; Lázár, J.; Papp, I.; Sári, P. (2012), «HAT-P-34b-HAT-P-37b: FOUR TRANSITING PLANETS MORE MASSIVE THAN JUPITER ORBITING MODERATELY BRIGHT STARS», The Astronomical Journal, 144 (1): 19, Bibcode:2012AJ....144...19B, arXiv:1201.0659 , doi:10.1088/0004-6256/144/1/19 
  11. ↑ A-thano, Napaporn; Jiang, Ing-Guey; Awiphan, Supachai; Rattanamala, Ronnakrit; Su, Li-Hsin; Hengpiya, Torik; Sariya, Devesh P.; Yeh, Li-Chin; Shlyapnikov, A. A.; Gorbachev, Mark A.; Rublevski, Alexey N.; Vineet Kumar Mannaday; Thakur, Parijat; Sahu, D. K.; Mkrtichian, David; Griv, Evgeny (2022), «The Transit Timing and Atmosphere of Hot Jupiter HAT-P-37b», The Astronomical Journal, 163 (2): 77, arXiv:2112.04724 , doi:10.3847/1538-3881/ac416d 
  12. ↑ Sato, Bun'ei; Hartman, Joel D.; Bakos, Gáspár Á.; Béky, Bence; Torres, Guillermo; Latham, David W.; Kovács, Géza; Csubry, Zoltán; Penev, Kaloyan; Noyes, Robert W.; Buchhave, Lars A.; Quinn, Samuel N.; Everett, Mark; Esquerdo, Gilbert A.; Fischer, Debra A.; Howard, Andrew W.; Johnson, John A.; Marcy, Geoff W.; Sasselov, Dimitar D.; Szklenár, Tamás; Lázár, József; Papp, István; Sári, Pál (2012), «HAT-P-38b: A Saturn-Mass Planet Transiting a Late G Star», Publications of the Astronomical Society of Japan, 64 (5): 97, arXiv:1201.5075 , doi:10.1093/pasj/64.5.97 
  13. ↑ a b c Hartman, J. D.; et al. (2012). «HAT-P-39b–HAT-P-41b: Three Highly Inflated Transiting Hot Jupiters». The Astronomical Journal. 144 (5): 139. Bibcode:2012AJ....144..139H. arXiv:1207.3344 . doi:10.1088/0004-6256/144/5/139 
  14. ↑ Lewis, N. K.; et al. (2020). «Into the UV: The Atmosphere of the Hot Jupiter HAT-P-41b Revealed». The Astrophysical Journal. 902 (1): L19. Bibcode:2020ApJ...902L..19L. arXiv:2010.08551 . doi:10.3847/2041-8213/abb77f 
  15. ↑ Sheppard, Kyle B.; et al. (2021). «The Hubble PanCET Program: A Metal-rich Atmosphere for the Inflated Hot Jupiter HAT-P-41b». The Astronomical Journal. 161 (2): 51. Bibcode:2021AJ....161...51S. arXiv:2010.09659 . doi:10.3847/1538-3881/abc8f4 
  16. ↑ a b Boisse, I.; Hartman, J. D.; Bakos, G. Á.; Penev, K.; Csubry, Z.; Béky, B.; Latham, D. W.; Bieryla, A.; Torres, G.; Kovács, G.; Buchhave, L. A.; Hansen, T.; Everett, M.; Esquerdo, G. A.; Szklenár, T.; Falco, E.; Shporer, A.; Fulton, B. J.; Noyes, R. W.; Stefanik, R. P.; Lázár, J.; Papp, I.; Sári, P. (2012), «HAT-P-42b and HAT-P-43b», Astronomy & Astrophysics, 558: A86, arXiv:1212.6448 , doi:10.1051/0004-6361/201220993 
  17. ↑ Penev, K.; Bakos, G. Á.; Bayliss, D.; Jordán, A.; Mohler, M.; Zhou, G.; Suc, V.; Rabus, M.; Hartman, J. D.; Mancini, L.; Béky, B.; Csubry, Z.; Buchhave, L.; Henning, T.; Nikolov, N.; Csák, B.; Brahm, R.; Espinoza, N.; Conroy, P.; Noyes, R. W.; Sasselov, D. D.; Schmidt, B.; Wright, D. J.; Tinney, C. G.; Addison, B. C.; Lázár, J.; Papp, I.; Sári, P. (2012), «HATS-1b: THE FIRST TRANSITING PLANET DISCOVERED BY THE HATSouth SURVEY», The Astronomical Journal, 145: 5, arXiv:1206.1524 , doi:10.1088/0004-6256/145/1/5 
  18. ↑ a b Wittenmyer, Robert A.; Horner, J.; Tuomi, Mikko; Salter, G. S.; Tinney, C. G.; Butler, R. P.; Jones, H. R. A.; o'Toole, S. J.; Bailey, J.; Carter, B. D.; Jenkins, J. S.; Zhang, Z.; Vogt, S. S.; Rivera, Eugenio J. (2012), «The Anglo-Australian Planet Search. Xxii. Two New Multi-Planet Systems», The Astrophysical Journal, 753 (2): 169, Bibcode:2012ApJ...753..169W, arXiv:1205.2765 , doi:10.1088/0004-637X/753/2/169 
  19. ↑ a b Sato, Bun'ei; et al. (2013). «A Double Planetary System around the Evolved Intermediate-mass Star HD 4732». The Astrophysical Journal. 762 (1). 9. Bibcode:2013ApJ...762....9S. arXiv:1210.6798 . doi:10.1088/0004-637X/762/1/9 
  20. ↑ a b c Boisse, Isabelle; Pepe, Francesco; Perrier, Christian; Queloz, Didier; Bonfils, Xavier; Bouchy, François; Santos, Nuno C.; Arnold, Luc; Beuzit, Jean-Luc; Dìaz, Rodrigo F.; Delfosse, Xavier; Eggenberger, Anne; Ehrenreich, David; Forveille, Thierry; Hébrard, Guillaume; Lagrange, Anne-Marie; Lovis, Christophe; Mayor, Michel; Moutou, Claire; Naef, Dominique; Santerne, Alexandre; Ségransan, Damien; Sivan, Jean-Pierre; Udry, Stéphane (2012), «The SOPHIE search for northern extrasolar planets V. Follow-up of ELODIE candidates: Jupiter-analogs around Sun-like stars», Astronomy and Astrophysics, 545: A55, Bibcode:2012A&A...545A..55B, arXiv:1205.5835 , doi:10.1051/0004-6361/201118419 
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  22. ↑ Wang Xuesong, Sharon; et al. (2012). «The Discovery of HD 37605c and a Dispositive Null Detection of Transits of HD 37605b». Astrophysical Journal. 761 (1). 46 páginas. Bibcode:2012ApJ...761...46W. arXiv:1210.6985 . doi:10.1088/0004-637X/761/1/46 
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  24. ↑ Lee, B.-C.; Mkrtichian, D. E.; Han, I.; Park, M.-G.; Kim, K.-M. (2012), «Detection of an exoplanet around the evolved K giant HD 66141», Astronomy & Astrophysics, 548: A118, Bibcode:2012A&A...548A.118L, arXiv:1211.2054 , doi:10.1051/0004-6361/201118014 
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  36. ↑ Lissauer, Jack J.; Marcy, Geoffrey W.; Rowe, Jason F.; Bryson, Stephen T.; Adams, Elisabeth; Buchhave, Lars A.; Ciardi, David R.; Cochran, William D.; Fabrycky, Daniel C.; Ford, Eric B.; Fressin, Francois; Geary, John; Gilliland, Ronald L.; Holman, Matthew J.; Howell, Steve B.; Jenkins, Jon M.; Kinemuchi, Karen; Koch, David G.; Morehead, Robert C.; Ragozzine, Darin; Seader, Shawn E.; Tanenbaum, Peter G.; Torres, Guillermo; Twicken, Joseph D. (10 de maio de 2012). «Almost All of Kepler's Multiple Planet Candidates are Planets». The Astrophysical Journal. 750 (2). 112 páginas. Bibcode:2012ApJ...750..112L. arXiv:1201.5424 . doi:10.1088/0004-637X/750/2/112 
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  54. ↑ Rattanamala, R.; Awiphan, S.; Komonjinda, S.; Phriksee, A.; Sappankum, P.; A-thano, N.; Chitchak, S.; Rittipruk, P.; Sawangwit, U.; Poshyachinda, S.; Reichart, D. E.; Haislip, J. B. (2021), Two circumbinary planets in RR Cae eclipsing binary system, arXiv:2109.09397  
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  56. ↑ a b Tuomi, M; Jones, H R A; Jenkins, J S; Tinney, C G; Butler, R P; Vogt, S S; Barnes, J R; Wittenmyer, R A; o'Toole, S; Horner, J; Bailey, J; Carter, B D; Wright, D J; Salter, G S; Pinfield, D (2013). «Signals embedded in the radial velocity noise». Astronomy & Astrophysics. 551: A79. Bibcode:2012yCat..35510079T. arXiv:1212.4277 . doi:10.1051/0004-6361/201220509 
  57. ↑ a b Lendl, M.; Anderson, D. R.; Collier-Cameron, A.; Doyle, A. P.; Gillon, M.; Hellier, C.; Jehin, E.; Lister, T. A.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Smalley, B.; Ségransan, D.; Smith, A. M. S.; Triaud, A. H. M. J.; Udry, S.; West, R. G.; Wheatley, P. J. (2012), «WASP-42 b and WASP-49 b: Two new transiting sub-Jupiters», Astronomy & Astrophysics, 544: A72, Bibcode:2012A&A...544A..72L, arXiv:1205.2757 , doi:10.1051/0004-6361/201219585 
  58. ↑ a b c d e f g Hellier, Coel; Anderson, D. R.; Collier Cameron, A.; Doyle, A. P.; Fumel, A.; 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. (2012), «Seven transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-47b, WASP-55b, WASP-61b, WASP-62b, WASP-63b, WASP-66b and WASP-67b», Monthly Notices of the Royal Astronomical Society, 426 (1): 739–750, Bibcode:2012MNRAS.426..739H, arXiv:1204.5095 , doi:10.1111/j.1365-2966.2012.21780.x 
  59. ↑ a b c d Hébrard, G.; et al. (2012), «WASP-52b, WASP-58b, WASP-59b, and WASP-60b: Four new transiting close-in giant planets», Astronomy & Astrophysics, 549: A134, arXiv:1211.0810 , doi:10.1051/0004-6361/201220363 
  60. ↑ a b c Faedi, F.; et al. (2013). «WASP-54b, WASP-56b, and WASP-57b: Three new sub-Jupiter mass planets from SuperWASP». Astronomy & Astrophysics. 551: A73. Bibcode:2013A&A...551A..73F. arXiv:1210.2329 . doi:10.1051/0004-6361/201220520 
  61. ↑ a b Gillon, M.; Anderson, D. R.; Collier-Cameron, A.; Doyle, A. P.; Fumel, A.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Montalbán, J.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smith, A. M. S.; Smalley, B.; Southworth, J.; Triaud, A. H. M. J.; Udry, S.; West, R. G. (2012), «WASP-64 b and WASP-72 b: Two new transiting highly irradiated giant planets», Astronomy & Astrophysics, 552: A82, arXiv:1210.4257 , doi:10.1051/0004-6361/201220561 
  62. ↑ Smith, A. M. S.; Anderson, D. R.; Bouchy, F.; Collier Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hébrard, G.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Moutou, C.; Pepe, F.; Pollacco, D.; Queloz, D.; Santerne, A.; Segransan, D.; Smalley, B.; Southworth, J.; Triaud, A. H. M. J.; Udry, S.; West, R. G. (2013), «WASP-71b: A bloated hot Jupiter in a 2.9-day, prograde orbit around an evolved F8 star», Astronomy & Astrophysics, 552: A120, Bibcode:2013A&A...552A.120S, arXiv:1211.3045 , doi:10.1051/0004-6361/201220727 
  63. ↑ Maxted, P. F. L.; Anderson, D. R.; Collier Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M.; Pepe, F.; Pollacco, D. L.; Queloz, D.; Ségransan, D.; Smalley, B.; Southworth, K.; Smith, A. M. S.; Triaud, A. H. M. J.; Udry, S.; West, R. G. (2012), «WASP-77 Ab: A Transiting Hot Jupiter Planet in a Wide Binary System1», Publications of the Astronomical Society of the Pacific, 125 (923): 48–55, arXiv:1211.6033 , doi:10.1086/669231 
  64. ↑ a b Smalley, B.; Anderson, D. R.; Collier-Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Udry, S.; West, R. G. (2012), «WASP-78b and WASP-79b: Two highly-bloated hot Jupiter-mass exoplanets orbiting F-type stars in Eridanus», Astronomy & Astrophysics, 547: A61, Bibcode:2012A&A...547A..61S, arXiv:1206.1177 , doi:10.1051/0004-6361/201219731 
  65. ↑ Liu, Michael C.; Dupuy, Trent J.; Bowler, Brendan P.; Leggett, S. K.; Best, William M. J. (2012). «Two Extraordinary Substellar Binaries at the T/Y Transition and the Y-band Fluxes of the Coolest Brown Dwarfs». The Astrophysical Journal. 758 (1). 57 páginas. Bibcode:2012ApJ...758...57L. arXiv:1206.4044 . doi:10.1088/0004-637X/758/1/57 
  66. ↑ The first planet detected in the WTS: An inflated hot Jupiter in a 3.35d orbit around a late F star
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