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List of exoplanets discovered in 2012

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This is a List of exoplanets discovered in 2012.[1] 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)[2] Discovery method Distance (ly) Host star mass (M☉) Host star temp. (K) Remarks
75 Ceti b 3 691.9 2.1 radial vel. 266 2.49 4846 [3]
BD+20 274 b 4.2 578.2 1.3 radial vel. 4500±300 0.8 4296 [4]
BD+48 740 b 1.7±0.7 733+5
−8 		1.7±0.1 radial vel. 2214±72 1.09±0.16 4534±8 [5] Confirmed in 2018.[6]
CoRoT-21b 2.26 1.3 2.72 0.0417 1867 transit 4600±900 1.29 6200 [7]
Epsilon Coronae Borealis b 6.7 417.9 1.3 radial vel. 229.7 1.7 4406 [8]
Gliese 676 Ad 0.014 3.6005 0.0413±0.0014 radial vel. 52.29±0.03 0.71±0.04 3734 [9]
Gliese 676 Ae 0.025 35.39 0.187±0.007 radial vel. 52.29±0.03 0.71±0.04 3734 [9]
Gliese 3470 b 0.043 0.346 3.3366487 0.031 radial vel. 82 0.51 3652 [10]
HAT-P-34b 7.01 1.35 5.45265 0.06774 1520 transit 818.94 4.26 6442 [11] Proper name Ġgantija
HAT-P-35b 7.52 3.55 3.64671 0.0498 1581 transit 1677 23.56 6096 [11]
HAT-P-36b 1.8482 1.277 1.32734683 0.0241 1781 transit 968.49 1.03 5620 [11] Proper name Bran
HAT-P-37b 1.169 1.178 2.797436 0.0379 1271 transit 1341 0.93 5500 [11]Additional planets in system are suspected[12]
HAT-P-38b 0.267 0.825 4.640382 0.0523 transit 810 0.89 5330 [13] Proper name Hiisi
HAT-P-39b 0.599 1.571 3.54387 0.0509 transit 2090 1.4 6430 [14]
HAT-P-40b 0.615 1.73 4.457243 0.0608 transit 1630 1.51 6080 [14] Proper name Vytis
HAT-P-41b 0.8 1.685 2.694047 0.0426 transit 1120 1.42 6390 [15][14][16]
HAT-P-42b 1.044 1.28 4.641878 0.0575 1427 transit 1460 1.18 5743 [17] Proper name Iolaus
HAT-P-43b 0.662 1.281 3.332687 0.0443 1361 transit 1770 1.05 5645 [17]
HATS-1b 1.855 1.302 3.446459 0.0444 transit 990 0.99 5870 [18]
HD 142 c 5.3 6005 6.8 radial vel. 83.6 1.23 6245 [19]
HD 4732 b 2.37 360.2 1.19 radial vel. 184 1.74 4959 [20]
HD 4732 c 2.37 2732 4.6 radial vel. 184 1.74 4959 [20]
HD 5608 b 1.4 792.6 1.9 radial vel. 189.7 1.55 4854 [3]
HD 24040 b 4.10±0.12 3490±25 4.637±0.067 radial vel. 152.3±0.4 1.14±0.02 5917±52 [21] Suspected since 2006
HD 27631 b 1.45 2208 3.25 radial vel. 145.3 0.94 5737 [22]
HD 37605 c 3.366 2720 3.814 radial vel. 139.9 1 5448 [23]
HD 40307 e 0.0110±0.0044 34.62+0.21
−0.20 		0.1886+0.083
−0.0104 		radial vel. 41.8 0.77 4956 [24]
HD 40307 f 0.0164 51.76 0.247 radial vel. 41.8 0.77 4956 [24]
HD 40307 g 0.0223 197.8 0.6 radial vel. 41.8 0.77 4956 [24]
HD 66141 b 6 480.5 1.2 radial vel. 261.1 1.1 4323 [25]
HD 77338b 0.05 5.7361 0.0614 radial vel. 134.6 0.93 5370 [26]
HD 79498 b 1.34 1807 2.98 radial vel. 159.89 1.08 5748 [27]
HD 98649 b 6.8 4951 5.6 radial vel. 139.5 1 5759 [22]
HD 106515 Ab 9.61 3630 4.59 radial vel. 118.6 0.97 5362 [22]
HD 150706 b 2.71 5894 6.7 radial vel. 88.8 1.17 5961 [21]
HD 159868 c 0.73 352.3 1 radial vel. 171.9 1.09 5558 [19]
HD 166724 b 3.53 5144 5.42 radial vel. 140.2 0.81 5127 [22]
HD 197037 b 0.79 1035.7 2.07 radial vel. 107.1 1.063±0.022 6137±20 [27]
HD 207832 b 0.56 161.97 0.57 radial vel. 180.4 0.94 5710 [28] Suspected false positive[29]
HD 207832 c 0.73 1155.7 2.112 radial vel. 180.4 0.94 5710 [28] Suspected false positive[29]
HD 208527 b 9.9 875.5 2.1 radial vel. 1148.4 1.6 4035 [30]
HD 219077 b 10.39 5501 6.22 radial vel. 95 1.05 5362 [22]
HD 219415 b 1 2093.3 3.2 radial vel. 553.7 1 4820 [4]
HD 220074 b 11.1 672.1 1.6 radial vel. 942.7 1.2 3935 [30]
HD 220689 b 1.06 2209 3.36 radial vel. 147.5 1.04 5921 [22]
HD 220773 b 1.45 3724.7 4.94 radial vel. 159.82 1.16 5940 [27]
HD 222155 b 2.12 3999 5.14 radial vel. 165.3 1.21 5701 [21]
HW Virginis b 14.3 4640 4.69 timing 590 0.485 [31]Likely false positive[32]
Kappa Andromedae b 13.616 55 1850 imaging 169.7 2.6 10900 Has a reddish color, and may be a brown dwarf[33]
KELT-1b 27.23 1.11 1.217514 0.02466 2423 transit 850 1.32 6518 [34]
KELT-2Ab 1.522 1.286 4.1137912 0.05496 transit 405.2 1.31 6151 [35]
Kepler-30b 0.036 0.348 29.33434 0.18 transit 4600 0.99 5498 [36]
Kepler-30c 2.01 1.097 60.323105 0.3 transit 4600 0.99 5498 [36]
Kepler-30d 0.073 0.785 143.34394 0.5 transit 4600 0.99 5498 [36]
Kepler-32d 0.241 22.7802 0.13 transit 990 0.58 3900 [36]
Kepler-32e 0.134 2.896 0.033 transit 990 0.58 3900 Weak evidence[36]
Kepler-32f 0.073 0.74296 0.013 transit 990 0.58 3900 Weak evidence[36]
Kepler-33f 0.03036 0.398 41.02902 0.2535 transit 4086 1.29 5904 [37]
Kepler-34b 0.22 0.764 288.822 1.0896 transit 4889 1.05 5913 [38]
Kepler-35b 0.127 0.728 131.458 0.60347 transit 5365 0.89 5606 [38]
Kepler-36b 0.014 0.133 13.83989 0.1153 transit 1500 1.07 5911 [39]
Kepler-36c 0.025 0.328 16.23855 0.1283 transit 1500 1.07 5911 [39]
Kepler-38b 0.384 0.384 105.599 0.4632 transit 2000 0.94 5623 [40]
Kepler-46b 6 0.808 33.60134 0.1968 transit 2790 0.9 5309 [41]
Kepler-46c 0.376 57.011 0.2799 timing 2790 0.9 5309 [41]
Kepler-47b 2 0.27 49.532 0.2962 transit 4900 1.05 5636 [42]
Kepler-47c 28 0.411 303.137 0.991 transit 4900 1.05 5636 [42]
Kepler-48b [ru] 0.0124 0.168 4.778 transit 1009±5 0.88 5194 [43][44]
Kepler-48c [ru] 0.04597 0.242 9.67395 transit 1009±5 0.88 5194 [43][44]
Kepler-49b [ru] 0.98 0.243 7.2037945 transit 1024±8 0.55 4252 [43][44]
Kepler-49c [ru] 0.72 0.227 10.9129343 transit 1024±8 0.55 4252 [43][44]
Kepler-50b [ru] 0.153 7.81254 0.077 transit 821±6 1.24 6225 [44]
Kepler-50c [ru] 0.194 9.37647 0.087 transit 821±6 1.24 6225 [44]
Kepler-51b 0.007 0.633 45.154 0.2514 543 transit 2610±50 1.04 6018 [44]
Kepler-51c 0.013 0.803 85.312 0.384 439 transit 2610±50 1.04 6018 [44]
Kepler-52b [ru] 8.7 0.187 7.8773565 transit 1058±7 0.54 4263 [44]
Kepler-52c [ru] 10.41 0.164 16.3850021 transit 1058±7 0.54 4263 [44]
Kepler-53b [ru] 18.41 0.258 18.6489525 transit 4600±200 0.98 5858 [43][44]
Kepler-53c [ru] 15.74 0.283 38.5583038 transit 4600±200 0.98 5858 [43][44]
Kepler-54b [ru] 0.92 0.187 8.0109434 transit 893±9 0.51 4252 [44]
Kepler-54c [ru] 0.37 0.11 12.0717249 transit 893±9 0.51 4252 [44]
Kepler-55b [ru] 1.49 0.217 27.9481449 transit 1920±30 0.62 4503 [44]
Kepler-55c [ru] 1.11 0.197 42.1516418 transit 1920±30 0.62 4503 [44]
Kepler-56b 0.07 0.581 10.5016 0.1028 transit 3060±80 1.32 4840 [44]
Kepler-56c 0.57 0.874 21.40239 0.1652 transit 3060±80 1.32 4840 [44]
Kepler-57b [ru] 18.86 0.195 5.7293196 0.057 transit 3140±30 0.83 5145 [43][44]
Kepler-57c [ru] 6.95 0.138 11.6092567 0.092 631 transit 3140±30 0.83 5145 [43][44]
Kepler-58b [ru] 1.39 0.248 10.2184954 transit 3250±80 0.95 6099 [43][44]
Kepler-58c [ru] 2.19 0.255 15.5741568 transit 3250±80 0.95 6099 [43][44]
Kepler-59b 2.05 0.098 11.8681707 transit 3925±75 1.04 6074 [44]
Kepler-59c 1.37 0.177 17.9801235 transit 3925±75 1.04 6074 [44]
Kepler-60b [ru] 0.01318 0.153 7.1334 transit 3440±70 1.04 5905 [44]
Kepler-60c [ru] 0.01211 0.17 8.9187 transit 3440±70 1.04 5905 [44]
Kepler-60d 0.01309 0.178 11.8981 transit 3440±70 1.04 5905 [44]
Kepler-64b 0.531 0.551 138.317 0.652 transit 6200±1000 1.53 6407 [45] Quadruple star system
Kepler-79b 0.0343 0.31 13.4845 0.117 868 transit 3430±60 1.17 6174 [43]
Kepler-79c 0.019 0.332 27.4029 0.187 685 transit 3430±60 1.17 6174 [43]
Kepler-80b 0.0218 0.238 7.05246 0.0648 transit 1160 0.73 4540 [43]
Kepler-80c 0.02121 0.244 9.52355 0.0792 transit 1160 0.73 4540 [43]
Kepler-81b 0.216 5.955 646 transit 1147±10 0.64 4500 [43]
Kepler-81c 0.211 12.04 513 transit 1147±10 0.64 4500 [43]
Kepler-82b 0.357 26.444 581 transit 3030±80 0.85 5428 [43]
Kepler-82c 0.477 51.538 464 transit 3030±80 0.85 5428 [43]
Kepler-83b 0.252 9.77 transit 1320±17 0.66 4648 [43][46]
Kepler-83c 0.211 20.09 transit 1320±17 0.66 4648 [43][46]
Kepler-84b 0.199 8.726 937 transit 4700±500 1 6031 [43][46]
Kepler-84c 0.211 12.883 821 transit 4700±500 1 6031 [43][46]
Kepler-85b 0.176 8.306 transit 2550±50 0.92 5436 [43] KOI-2038[47]
Kepler-85c 0.194 12.513 transit 2550±50 0.92 5436 [43] KOI-2038[47]
MOA-2011-BLG-293Lb [ja] 2.4+1.4
−0.9 		1.0±0.1 microlensing 23000±2000 0.675±0.525 [48]
MOA-2010-BLG-073Lb 11 1.21 microlensing 9100 0.16 Possibly brown dwarf[49]
MOA-2010-BLG-477Lb 1.4±0.3 2.8±0.5 microlensing 7500±2000 0.53±0.11 5950±150 [50]White dwarf host star[51]
MOA-bin-1Lb 3.7±2.1 8.3+4.5
−2.7 		microlensing 17000 0.75+0.33
−0.41 		[52]
Mu2 Octantis b 6.9 3638 5.02 radial vel. 142.1 1.29 6017 [22]
Nu Ophiuchi b 24 530.32 1.9 radial vel. 152.8 3.04 4928 Brown dwarf or small star[3]
Nu Ophiuchi c 27 3186 6.1 radial vel. 152.8 3.04 4928 Brown dwarf or small star[3]
OGLE-2012-BLG-0026Lb 0.145 4 microlensing 13110 1.06 [53]
OGLE-2012-BLG-0026Lc 0.86 4.8 microlensing 13110 1.06 [53]
Omicron Coronae Borealis b 1.5 187.83 0.83 radial vel. 274.1 2.13 4749 [3]
Omicron Ursae Majoris b 4.1 1630 3.9 radial vel. 183.7 3.09 5242 [3]
Pr0201 b 0.54 4.4264 radial vel. 610 1.23 6174 [54] In Beehive Cluster
Pr0211 b 1.88 2.1461 0.03176 radial vel. 610 0.94 5300 [54] Multi-planet system In Beehive Cluster
RR Caeli b 3.0±0.3 1900±40 5.2±0.1 timing 69.10±0.03 0.18+0.44 3100+7540 Circumbinary planet around red and white dwarfs.[55][56]
Tau Ceti e 0.0124 162.87 0.538 radial vel. 12 0.78 [57] Potentially habitable exoplanet
Tau Ceti f 0.0124 636.13 1.334 radial vel. 12 0.78 [57]
WASP-42b 0.527 1.122 4.9816819 0.0561 1021±19 transit 520 0.95 5315 [58]
WASP-47b 1.21 1.15 4.16071 0.052 1275 transit 650 1.11 5576 [59]
WASP-49b 0.378 1.115 2.7817387 0.0379 1369±39 transit 550 0.94 5600 [58]
WASP-52b 0.46 1.27 1.7497798 0.0272 1315±35 transit 460 0.87 5000 [60] Proper name Göktürk
WASP-54b 0.636 1.653 3.6936411 0.04987 1742+49
−69 		transit 650 1.21 6100 [61]
WASP-55b 0.627 1.335 4.4656291 0.0558 1290 transit 1100 1.16 6070 [59]
WASP-56b 0.571 1.092 4.617101 0.05458 1200 transit 830 1.03 5600 [61]
WASP-57b 0.644 1.05 2.83891856 0.03769 1338±29 transit 1480 0.89 5600 [61]
WASP-58b 0.89 1.37 5.01718 0.0561 1270±80 transit 980 0.94 5800 [60]
WASP-59b 0.863 0.775 7.919585 0.0697 670±35 transit 410 0.72 4650 [60]
WASP-60b 0.514 0.86 4.3050011 0.0531 1479±35 transit 1300 1.08 5900 [60] Proper name Vlasina
WASP-61b 2.06 1.24 3.8559 0.0514 1565±35 transit 1600 1.22 6320 [59]
WASP-62b 0.57 1.39 4.411953 0.0567 1329.6±44.8 transit 520 1.25 6280 [59] Proper name Krotoa
WASP-63b 0.38 1.43 4.37809 0.0574 1536±37 transit 1100 1.32 5570 [59]
WASP-64b 1.271 1.271 1.5732918 0.02648 1989+87
−88 		transit 1100 1 5400 [62] Proper name Agouto
WASP-66b 2.32 1.39 4.086052 0.0546 1790±60 transit 1200 1.3 6580 [59]
WASP-67b 0.42 1.4 4.61442 0.0517 1050 transit 730 0.87 5240 [59]
WASP-71b 2.242 1.46 2.9036747 0.04619 2016.1+67.0
−52.5 		transit 1130 1.56 6059 [63] Proper name Tanzanite
WASP-72b 1.5461 1.27 2.2167421 0.03708 2210+120
−130 		transit 1100 1.39 6250 [62] Proper name Cuptor
WASP-77Ab 1.76 1.21 1.3600309 0.024 1715 transit 300 1 5500 Orbiting primary star of binary star system[64]
WASP-78b 0.89 1.7 2.17517632 0.0362 2350 transit 1800 1.17 6100 [65]
WASP-79b 0.9 2.09 3.6623866 0.0535 1900±50 transit 780 1.38 6600 [65] Proper name Pollera
WISE 1217+1626 B 22 0.934 8 450 imaging 29±3 0.03 575 Brown dwarf[66]
WTS-1b 4.01 1.49 3.352057 0.047 1500±100 transit 8100±1000 1.2 6250 [67]

Specific exoplanet lists

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Lists of exoplanets

Lists of exoplanets by year of discovery

[edit]


References

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  1. ^ "NASA Exoplanet Archive". Retrieved 20 December 2019.
  2. ^ "The Extrasolar Planets Encyclopaedia". 1995. Retrieved 2015-11-09.
  3. ^ 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. arXiv:1207.3141. Bibcode:2012PASJ...64..135S. doi:10.1093/pasj/64.6.135. S2CID 119197073.
  4. ^ 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, arXiv:1207.0488, Bibcode:2012ApJ...756...53G, doi:10.1088/0004-637X/756/1/53, S2CID 119234699
  5. ^ 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. arXiv:1206.4938. Bibcode:2012ApJ...754L..15A. doi:10.1088/2041-8205/754/1/L15. S2CID 53550985.
  6. ^ 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, S2CID 56091464
  7. ^ Transiting exoplanets from the CoRoT space mission XXIII. CoRoT-21b: a doomed large Jupiter around a faint subgiant star
  8. ^ 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. arXiv:1209.1187. Bibcode:2012A&A...546A...5L. doi:10.1051/0004-6361/201219347. S2CID 55260442. A5.
  9. ^ 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. arXiv:1206.7118. Bibcode:2012A&A...548A..58A. doi:10.1051/0004-6361/201219910. S2CID 17115882.
  10. ^ 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. arXiv:1206.5307. Bibcode:2012A&A...546A..27B. doi:10.1051/0004-6361/201219623. S2CID 12963626.
  11. ^ 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, arXiv:1201.0659, Bibcode:2012AJ....144...19B, doi:10.1088/0004-6256/144/1/19, S2CID 119291677
  12. ^ 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, Bibcode:2022AJ....163...77A, doi:10.3847/1538-3881/ac416d, S2CID 245006237
  13. ^ 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
  14. ^ 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. arXiv:1207.3344. Bibcode:2012AJ....144..139H. doi:10.1088/0004-6256/144/5/139. S2CID 118457589.
  15. ^ 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. arXiv:2010.08551. Bibcode:2020ApJ...902L..19L. doi:10.3847/2041-8213/abb77f. S2CID 224706001.
  16. ^ 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. arXiv:2010.09659. Bibcode:2021AJ....161...51S. doi:10.3847/1538-3881/abc8f4. S2CID 224710738.
  17. ^ 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, S2CID 119209692
  18. ^ 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, S2CID 118556930
  19. ^ 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, arXiv:1205.2765, Bibcode:2012ApJ...753..169W, doi:10.1088/0004-637X/753/2/169, S2CID 2941264
  20. ^ 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. arXiv:1210.6798. Bibcode:2013ApJ...762....9S. doi:10.1088/0004-637X/762/1/9. S2CID 67838183.
  21. ^ 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, arXiv:1205.5835, Bibcode:2012A&A...545A..55B, doi:10.1051/0004-6361/201118419, S2CID 119109836
  22. ^ a b c d e f g Marmier, M.; et al. (2013). "The CORALIE survey for southern extrasolar planets XVII. New and updated long period and massive planets". Astronomy and Astrophysics. 551. A90. arXiv:1211.6444. Bibcode:2013A&A...551A..90M. doi:10.1051/0004-6361/201219639. S2CID 59467665.
  23. ^ 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. arXiv:1210.6985. Bibcode:2012ApJ...761...46W. doi:10.1088/0004-637X/761/1/46. S2CID 118679173.
  24. ^ a b c Tuomi, M.; Anglada-Escudé, G.; Gerlach, E.; Jones, H. R. A.; Reiners, A.; Rivera, E. J.; Vogt, S. S.; Butler, R. P. (2012), "Habitable-zone super-Earth candidate in a six-planet system around the K2.5V star HD 40307", Astronomy & Astrophysics, 549: A48, arXiv:1211.1617, doi:10.1051/0004-6361/201220268, S2CID 7424216
  25. ^ 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, arXiv:1211.2054, Bibcode:2012A&A...548A.118L, doi:10.1051/0004-6361/201118014, S2CID 54984721
  26. ^ Jenkins, J. S.; Jones, H. R. A.; Tuomi, M.; Murgas, F.; Hoyer, S.; Jones, M. I.; Barnes, J. R.; Pavlenko, Y. V.; Ivanyuk, O.; Rojo, P.; Jordán, A.; Day-Jones, A. C.; Ruiz, M. T.; Pinfield, D. J. (2012), "A Hot Uranus Orbiting the Super Metal-Rich Star Hd 77338 and the Metallicity-Mass Connection", The Astrophysical Journal, 766 (2): 67, arXiv:1207.1012, doi:10.1088/0004-637X/766/2/67, S2CID 16971803
  27. ^ a b c Robertson, Paul; Endl, Michael; Cochran, William D.; MacQueen, Phillip J.; Wittenmyer, Robert A.; Horner, J.; Brugamyer, Erik J.; Simon, Attila E.; Barnes, Stuart I.; Caldwell, Caroline (2012). "The McDonald Observatory Planet Search: New Long-period Giant Planets and Two Interacting Jupiters in the HD 155358 System". The Astrophysical Journal. 749 (1): 17 pp. arXiv:1202.0265. Bibcode:2012ApJ...749...39R. doi:10.1088/0004-637X/749/1/39. S2CID 59273311.
  28. ^ a b Haghighipour, Nader; Butler, R. Paul; Rivera, Eugenio J.; Henry, Gregory W.; Vogt, Steven S. (2012), "The Lick-Carnegie Survey: A New Two-Planet System Around the Star Hd 207832", The Astrophysical Journal, 756 (1): 91, arXiv:1207.2806, Bibcode:2012ApJ...756...91H, doi:10.1088/0004-637X/756/1/91, S2CID 1137984
  29. ^ a b Luhn, Jacob K.; Wright, Jason T.; Howard, Andrew W.; Isaacson, Howard (2020), "Astrophysical Insights into Radial Velocity Jitter from an Analysis of 600 Planet-search Stars", The Astronomical Journal, 159 (5): 235, arXiv:2004.13734, Bibcode:2020AJ....159..235L, doi:10.3847/1538-3881/ab855a, S2CID 216642215
  30. ^ a b Lee, B.-C.; Han, I.; Park, M.-G. (2012), "Planetary companions orbiting M giants HD 208527 and HD 220074", Astronomy & Astrophysics, 549: A2, arXiv:1211.2051, doi:10.1051/0004-6361/201220301, S2CID 73522393
  31. ^ Beuermann, K.; Dreizler, S.; Hessman, F. V.; Deller, J. (2012). "The quest for companions to post-common envelope binaries. III. A reexamination of HW Virginis". Astronomy & Astrophysics. 543: id.A138. arXiv:1206.3080. Bibcode:2012A&A...543A.138B. doi:10.1051/0004-6361/201219391. S2CID 53680945.
  32. ^ Jonathan Horner; Robert Wittenmyer; Tobias Hinse; Jonathan Marshall; Alex Mustill (2014). "Wobbling Ancient Binaries - Here Be Planets?". arXiv:1401.6742 [astro-ph.EP].
  33. ^ Carson; Thalmann; Janson; Kozakis; Bonnefoy; Biller; Schlieder; Currie; McElwain (November 15, 2012). "Direct Imaging Discovery of a 'Super-Jupiter' Around the late B-Type Star Kappa And". The Astrophysical Journal. 763 (2): L32. arXiv:1211.3744. Bibcode:2013ApJ...763L..32C. doi:10.1088/2041-8205/763/2/L32. S2CID 119253577.
  34. ^ Fabrycky, Daniel C.; et al. (2012), "Transit Timing Observations Fromkepler. Iv. Confirmation of Four Multiple-Planet Systems by Simple Physical Models", The Astrophysical Journal, 750 (2): 114, arXiv:1201.5415, Bibcode:2012ApJ...750..114F, doi:10.1088/0004-637X/750/2/114, S2CID 9075167
  35. ^ Beatty, Thomas G.; et al. (2012). "KELT-2Ab: A Hot Jupiter Transiting the Bright (V = 8.77) Primary Star of a Binary System". The Astrophysical Journal Letters. 756 (2). L39. arXiv:1206.1592. Bibcode:2012ApJ...756L..39B. doi:10.1088/2041-8205/756/2/L39. hdl:1969.1/178896. S2CID 14271501.
  36. ^ a b c d e f Fabrycky, Daniel C.; et al. (2012), "Transit Timing Observations Fromkepler. Iv. Confirmation of Four Multiple-Planet Systems by Simple Physical Models", The Astrophysical Journal, 750 (2): 114, arXiv:1201.5415, Bibcode:2012ApJ...750..114F, doi:10.1088/0004-637X/750/2/114, S2CID 9075167
  37. ^ 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 May 2012). "Almost All of Kepler's Multiple Planet Candidates are Planets". The Astrophysical Journal. 750 (2): 112. arXiv:1201.5424. Bibcode:2012ApJ...750..112L. doi:10.1088/0004-637X/750/2/112. S2CID 30549908.
  38. ^ a b Welsh, William F.; et al. (2012). "Transiting circumbinary planets Kepler-34 b and Kepler-35 b". Nature. 481 (7382): 475–479. arXiv:1204.3955. Bibcode:2012Natur.481..475W. doi:10.1038/nature10768. PMID 22237021. S2CID 4426222.
  39. ^ a b Carter, J. A.; et al. (2012). "Kepler-36: A Pair of Planets with Neighboring Orbits and Dissimilar Densities". Science. 337 (6094): 556–559. arXiv:1206.4718. Bibcode:2012Sci...337..556C. doi:10.1126/science.1223269. PMID 22722249. S2CID 40245894.
  40. ^ Orosz, Jerome A.; et al. (2012), "THE NEPTUNE-SIZED CIRCUMBINARY PLANET KEPLER-38b", The Astrophysical Journal, 758 (2): 87, arXiv:1208.3712, Bibcode:2012ApJ...758...87O, doi:10.1088/0004-637X/758/2/87, S2CID 119226095
  41. ^ a b Nesvorny, D.; et al. (2012). "The Detection and Characterization of a Nontransiting Planet by Transit Timing Variations". Science. 336 (6085): 1133–6. arXiv:1208.0942. Bibcode:2012Sci...336.1133N. doi:10.1126/science.1221141. PMID 22582018. S2CID 41455466.
  42. ^ a b Orosz, Jerome A.; Welsh, William F.; Carter, Joshua A.; Fabrycky, Daniel C.; Cochran, William D.; Endl, Michael; Ford, Eric B.; Haghighipour, Nader; MacQueen, Phillip J.; Mazeh, Tsevi; Sanchis-Ojeda, Roberto; Short, Donald R.; Torres, Guillermo; Agol, Eric; Buchhave, Lars A.; Doyle, Laurance R.; Isaacson, Howard; Lissauer, Jack J.; Marcy, Geoffrey W.; Shporer, Avi; Windmiller, Gur; Barclay, Thomas; Boss, Alan P.; Clarke, Bruce D.; Fortney, Jonathan; Geary, John C.; Holman, Matthew J.; Huber, Daniel; Jenkins, Jon M.; et al. (2012). "Kepler-47: A Transiting Circumbinary Multi-Planet System". Science. 337 (6101): 1511–4. arXiv:1208.5489v1. Bibcode:2012Sci...337.1511O. doi:10.1126/science.1228380. PMID 22933522. S2CID 44970411.
  43. ^ a b c d e f g h i j k l m n o p q r s t u v w x Xie, Ji-Wei (2012), "Transit Timing Variation of Near-Resonance Planetary Pairs: Confirmation of 12 Multiple-Planet Systems", The Astrophysical Journal Supplement Series, 208 (2): 22, arXiv:1208.3312, Bibcode:2013ApJS..208...22X, doi:10.1088/0067-0049/208/2/22, S2CID 17160267
  44. ^ 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 Steffen, Jason H.; Fabrycky, Daniel C.; Agol, Eric; Ford, Eric B.; Morehead, Robert C.; Cochran, William D.; Lissauer, Jack J.; Adams, Elisabeth R.; Borucki, William J.; Bryson, Steve; Caldwell, Douglas A.; Dupree, Andrea; Jenkins, Jon M.; Robertson, Paul; Rowe, Jason F.; Seader, Shawn; Thompson, Susan; Twicken, Joseph D. (2012), "Transit timing observations from Kepler – VII. Confirmation of 27 planets in 13 multiplanet systems via transit timing variations and orbital stability", Monthly Notices of the Royal Astronomical Society, 428 (2): 1077–1087, arXiv:1208.3499, doi:10.1093/mnras/sts090
  45. ^ Kostov, V. B.; McCullough, P. R.; Hinse, T. C.; Tsvetanov, Z. I.; Hébrard, G.; Díaz, R. F.; Deleuil, M.; Valenti, J. A. (2013-01-01). "A Gas Giant Circumbinary Planet Transiting the F Star Primary of the Eclipsing Binary Star KIC 4862625 and the Independent Discovery and Characterization of the Two Transiting Planets in the Kepler-47 System". The Astrophysical Journal. 770 (1): 52. arXiv:1210.3850. Bibcode:2013ApJ...770...52K. doi:10.1088/0004-637X/770/1/52. ISSN 0004-637X. S2CID 119279690.
  46. ^ a b c d Rowe, Jason F.; Bryson, Stephen T.; Marcy, Geoffrey W.; Lissauer, Jack J.; Jontof-Hutter, Daniel; Mullally, Fergal; Gilliland, Ronald L.; Issacson, Howard; Ford, Eric; Howell, Steve B.; Borucki, William J.; Haas, Michael; Huber, Daniel; Steffen, Jason H.; Thompson, Susan E.; Quintana, Elisa; Barclay, Thomas; Still, Martin; Fortney, Jonathan; Gautier, T. N.; Hunter, Roger; Caldwell, Douglas A.; Ciardi, David R.; Devore, Edna; Cochran, William; Jenkins, Jon; Agol, Eric; Carter, Joshua A.; Geary, John (2014), "Validation Ofkepler's Multiple Planet Candidates. III. Light Curve Analysis and Announcement of Hundreds of New Multi-Planet Systems", The Astrophysical Journal, 784 (1): 45, arXiv:1402.6534, Bibcode:2014ApJ...784...45R, doi:10.1088/0004-637X/784/1/45, S2CID 119118620
  47. ^ a b Yang, Ming; Liu, Hui-Gen; Zhang, Hui; Yang, Jia-Yi; Zhou, Ji-Lin (2013), "Eight Planets in Four Multi-Planet Systems Via Transit Timing Variations in 1350 Days", The Astrophysical Journal, 778 (2): 110, arXiv:1308.0996, Bibcode:2013ApJ...778..110Y, doi:10.1088/0004-637X/778/2/110, S2CID 117080296
  48. ^ Yee, J. C.; et al. (2012), "MOA-2011-BLG-293Lb: A TEST OF PURE SURVEY MICROLENSING PLANET DETECTIONS", The Astrophysical Journal, 755 (2): 102, arXiv:1201.1002, Bibcode:2012ApJ...755..102Y, doi:10.1088/0004-637X/755/2/102
  49. ^ Street, R. A.; et al. (2012), "Moa-2010-BLG-073L: An M-Dwarf with a Substellar Companion at the Planet/Brown Dwarf Boundary", The Astrophysical Journal, 763: 67, arXiv:1211.3782, doi:10.1088/0004-637X/763/1/67, S2CID 53710373
  50. ^ Bachelet, E.; Shin, I.-G.; Han, C.; Fouqué, P.; Gould, A.; Menzies, J. W.; Beaulieu, J.-P.; Bennett, D. P.; et al. (2012). "MOA-2010-BLG-477Lb: Constraining the mass of a microlensing planet from microlensing parallax, orbital motion and detection of blended light". The Astrophysical Journal. 754 (1): 73. arXiv:1205.6323. Bibcode:2012ApJ...754...73B. doi:10.1088/0004-637X/754/1/73. S2CID 119223374.
  51. ^ Blackman, J. W.; Beaulieu, J. P.; Bennett, D. P.; Danielski, C.; Alard, C.; Cole, A. A.; Vandorou, A.; Ranc, C.; Terry, S. K.; Bhattacharya, A.; Bond, I.; Bachelet, E.; Veras, D.; Koshimoto, N.; Batista, V.; Marquette, J. B. (2021), "A Jovian analogue orbiting a white dwarf star", Nature, 598 (7880): 272–275, arXiv:2110.07934, Bibcode:2021Natur.598..272B, doi:10.1038/s41586-021-03869-6, PMID 34646001, S2CID 238860454
  52. ^ Bennett, D. P.; Sumi, T.; Bond, I. A.; Kamiya, K.; Abe, F.; Botzler, C. S.; Fukui, A.; Furusawa, K.; Itow, Y.; Korpela, A. V.; Kilmartin, P. M.; Ling, C. H.; Masuda, K.; Matsubara, Y.; Miyake, N.; Muraki, Y.; Ohnishi, K.; Rattenbury, N. J.; Saito, To.; Sullivan, D. J.; Suzuki, D.; Sweatman, W. L.; Tristram, P. J.; Wada, K.; Yock, P. C. M.; MOA Collaboration (2012), "Planetary and Other Short Binary Microlensing Events from the Moa Short-Event Analysis", The Astrophysical Journal, 757 (2): 119, arXiv:1203.4560, Bibcode:2012ApJ...757..119B, doi:10.1088/0004-637X/757/2/119, S2CID 118493329
  53. ^ a b Han, C.; et al. (2012), "THE SECOND MULTIPLE-PLANET SYSTEM DISCOVERED BY MICROLENSING: OGLE-2012-BLG-0026Lb, c—A PAIR OF JOVIAN PLANETS BEYOND THE SNOW LINE", The Astrophysical Journal, 762 (2): L28, arXiv:1210.4265, doi:10.1088/2041-8205/762/2/L28, S2CID 118797226
  54. ^ a b Quinn, Samuel N.; White, Russel J.; Latham, David W.; Buchhave, Lars A.; Cantrell, Justin R.; Dahm, Scott E.; Fűrész, Gabor; Szentgyorgyi, Andrew H.; Geary, John C.; Torres, Guillermo; Bieryla, Allyson; Berlind, Perry; Calkins, Michael C.; Esquerdo, Gilbert A.; Stefanik, Robert P. (2012). "TWO "b"s IN THE BEEHIVE: THE DISCOVERY OF THE FIRST HOT JUPITERS IN AN OPEN CLUSTER". The Astrophysical Journal. 756 (2): L33. arXiv:1207.0818. Bibcode:2012ApJ...756L..33Q. doi:10.1088/2041-8205/756/2/L33. S2CID 118825401.
  55. ^ 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
  56. ^ Qian, S. B.; Liu, L.; Zhu, L. Y.; Dai, Z. B.; Fernández Lajús, E.; Baume, G. L. (2012). "A circumbinary planet in orbit around the short-period white dwarf eclipsing binary RR Cae". Monthly Notices of the Royal Astronomical Society: Letters. 422 (1): L24–L27. arXiv:1201.4205. Bibcode:2012MNRAS.422L..24Q. doi:10.1111/j.1745-3933.2012.01228.x. S2CID 119190656.
  57. ^ 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. arXiv:1212.4277. Bibcode:2012yCat..35510079T. doi:10.1051/0004-6361/201220509. S2CID 2390534.
  58. ^ 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, arXiv:1205.2757, Bibcode:2012A&A...544A..72L, doi:10.1051/0004-6361/201219585, S2CID 54186638
  59. ^ 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, arXiv:1204.5095, Bibcode:2012MNRAS.426..739H, doi:10.1111/j.1365-2966.2012.21780.x, S2CID 54713354
  60. ^ 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, S2CID 54502046
  61. ^ 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. arXiv:1210.2329. Bibcode:2013A&A...551A..73F. doi:10.1051/0004-6361/201220520. S2CID 14346225.
  62. ^ 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, S2CID 53687206
  63. ^ 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, arXiv:1211.3045, Bibcode:2013A&A...552A.120S, doi:10.1051/0004-6361/201220727, S2CID 118575479
  64. ^ 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, S2CID 53552999
  65. ^ 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, arXiv:1206.1177, Bibcode:2012A&A...547A..61S, doi:10.1051/0004-6361/201219731, S2CID 119233646
  66. ^ 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. arXiv:1206.4044. Bibcode:2012ApJ...758...57L. doi:10.1088/0004-637X/758/1/57. S2CID 118402490.
  67. ^ 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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