Astronomy: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 0.0124 0.168 4.778 transit 1009±5 0.88 5194 [43][44]
Kepler-48c 0.04597 0.242 9.67395 transit 1009±5 0.88 5194 [43][44]
Kepler-49b 0.98 0.243 7.2037945 transit 1024±8 0.55 4252 [43][44]
Kepler-49c 0.72 0.227 10.9129343 transit 1024±8 0.55 4252 [43][44]
Kepler-50b 0.153 7.81254 0.077 transit 821±6 1.24 6225 [44]
Kepler-50c 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 8.7 0.187 7.8773565 transit 1058±7 0.54 4263 [44]
Kepler-52c 10.41 0.164 16.3850021 transit 1058±7 0.54 4263 [44]
Kepler-53b 18.41 0.258 18.6489525 transit 4600±200 0.98 5858 [43][44]
Kepler-53c 15.74 0.283 38.5583038 transit 4600±200 0.98 5858 [43][44]
Kepler-54b 0.92 0.187 8.0109434 transit 893±9 0.51 4252 [44]
Kepler-54c 0.37 0.11 12.0717249 transit 893±9 0.51 4252 [44]
Kepler-55b 1.49 0.217 27.9481449 transit 1920±30 0.62 4503 [44]
Kepler-55c 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 18.86 0.195 5.7293196 transit 3140±30 0.83 5145 [43][44]
Kepler-57c 6.95 0.138 11.6092567 transit 3140±30 0.83 5145 [43][44]
Kepler-58b 1.39 0.248 10.2184954 transit 3250±80 0.95 6099 [43][44]
Kepler-58c 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 0.01318 0.153 7.1334 transit 3440±70 1.04 5905 [44]
Kepler-60c 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

References

  1. ↑ "NASA Exoplanet Archive". https://exoplanetarchive.ipac.caltech.edu/cgi-bin/TblView/nph-tblView?app=ExoTbls&config=compositepars. 
  2. ↑ "The Extrasolar Planets Encyclopaedia". Extrasolar Planets Encyclopaedia. https://exoplanet.eu/catalog/. 
  3. ↑ 3.0 3.1 3.2 3.3 3.4 3.5 Sato, Bun'ei et al. (2012). "Substellar Companions to Seven Evolved Intermediate-Mass Stars". Publications of the Astronomical Society of Japan 64 (6): 135. doi:10.1093/pasj/64.6.135. Bibcode: 2012PASJ...64..135S. 
  4. ↑ 4.0 4.1 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, doi:10.1088/0004-637X/756/1/53, Bibcode: 2012ApJ...756...53G 
  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. doi:10.1088/2041-8205/754/1/L15. Bibcode: 2012ApJ...754L..15A. 
  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, doi:10.1051/0004-6361/201732161 
  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. doi:10.1051/0004-6361/201219347. A5. Bibcode: 2012A&A...546A...5L. 
  9. ↑ 9.0 9.1 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". Astronomy 548: A58. doi:10.1051/0004-6361/201219910. Bibcode: 2012A&A...548A..58A. http://goedoc.uni-goettingen.de/goescholar/bitstream/handle/1/9595/aa19910-12.pdf?sequence=2. 
  10. ↑ Bonfils, Xavier; Gillon, Michaël; Udry, Stéphane; Armstrong, David; Bouchy, François; Delfosse, Xavier; Forveille, Thierry; Fumel, Aurélie et al. (2012). "A hot Uranus transiting the nearby M dwarf GJ3470. Detected with HARPS velocimetry. Captured in transit with TRAPPIST photometry". Astronomy & Astrophysics 546: A27. doi:10.1051/0004-6361/201219623. Bibcode: 2012A&A...546A..27B. http://orbi.ulg.ac.be/jspui/handle/2268/135085. 
  11. ↑ 11.0 11.1 11.2 11.3 Bakos, G. Á.; Hartman, J. D.; Torres, G.; Béky, B.; Latham, D. W.; Buchhave, L. A.; Csubry, Z.; Kovács, G. et al. (2012), "HAT-P-34b-HAT-P-37b: FOUR TRANSITING PLANETS MORE MASSIVE THAN JUPITER ORBITING MODERATELY BRIGHT STARS", The Astronomical Journal 144 (1): 19, doi:10.1088/0004-6256/144/1/19, Bibcode: 2012AJ....144...19B 
  12. ↑ A-thano, Napaporn; Jiang, Ing-Guey; Awiphan, Supachai; Rattanamala, Ronnakrit; Su, Li-Hsin; Hengpiya, Torik; Sariya, Devesh P.; Yeh, Li-Chin et al. (2022), "The Transit Timing and Atmosphere of Hot Jupiter HAT-P-37b", The Astronomical Journal 163 (2): 77, doi:10.3847/1538-3881/ac416d 
  13. ↑ Sato, Bun'ei; Hartman, Joel D.; Bakos, Gáspár Á.; Béky, Bence; Torres, Guillermo; Latham, David W.; Kovács, Géza; Csubry, Zoltán et al. (2012), "HAT-P-38b: A Saturn-Mass Planet Transiting a Late G Star", Publications of the Astronomical Society of Japan 64 (5): 97, doi:10.1093/pasj/64.5.97 
  14. ↑ 14.0 14.1 14.2 Hartman, J. D. (2012). "HAT-P-39b–HAT-P-41b: Three Highly Inflated Transiting Hot Jupiters". The Astronomical Journal 144 (5): 139. doi:10.1088/0004-6256/144/5/139. Bibcode: 2012AJ....144..139H. 
  15. ↑ Lewis, N. K. (2020). "Into the UV: The Atmosphere of the Hot Jupiter HAT-P-41b Revealed". The Astrophysical Journal 902 (1): L19. doi:10.3847/2041-8213/abb77f. Bibcode: 2020ApJ...902L..19L. 
  16. ↑ Sheppard, Kyle B. (2021). "The Hubble PanCET Program: A Metal-rich Atmosphere for the Inflated Hot Jupiter HAT-P-41b". The Astronomical Journal 161 (2): 51. doi:10.3847/1538-3881/abc8f4. Bibcode: 2021AJ....161...51S. 
  17. ↑ 17.0 17.1 Boisse, I.; Hartman, J. D.; Bakos, G. Á.; Penev, K.; Csubry, Z.; Béky, B.; Latham, D. W.; Bieryla, A. et al. (2012), "HAT-P-42b and HAT-P-43b", Astronomy & Astrophysics 558: A86, doi:10.1051/0004-6361/201220993 
  18. ↑ Penev, K.; Bakos, G. Á.; Bayliss, D.; Jordán, A.; Mohler, M.; Zhou, G.; Suc, V.; Rabus, M. et al. (2012), "HATS-1b: THE FIRST TRANSITING PLANET DISCOVERED BY THE HATSouth SURVEY", The Astronomical Journal 145: 5, doi:10.1088/0004-6256/145/1/5 
  19. ↑ 19.0 19.1 Wittenmyer, Robert A.; Horner, J.; Tuomi, Mikko; Salter, G. S.; Tinney, C. G.; Butler, R. P.; Jones, H. R. A.; o'Toole, S. J. et al. (2012), "The Anglo-Australian Planet Search. Xxii. Two New Multi-Planet Systems", The Astrophysical Journal 753 (2): 169, doi:10.1088/0004-637X/753/2/169, Bibcode: 2012ApJ...753..169W 
  20. ↑ 20.0 20.1 Sato, Bun'ei et al. (2013). "A Double Planetary System around the Evolved Intermediate-mass Star HD 4732". The Astrophysical Journal 762 (1): 9. doi:10.1088/0004-637X/762/1/9. Bibcode: 2013ApJ...762....9S. 
  21. ↑ 21.0 21.1 21.2 Boisse, Isabelle; Pepe, Francesco; Perrier, Christian; Queloz, Didier; Bonfils, Xavier; Bouchy, François; Santos, Nuno C.; Arnold, Luc et al. (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, doi:10.1051/0004-6361/201118419, Bibcode: 2012A&A...545A..55B, http://www.aanda.org/articles/aa/full_html/2012/09/aa18419-11/aa18419-11.html 
  22. ↑ 22.0 22.1 22.2 22.3 22.4 22.5 22.6 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. doi:10.1051/0004-6361/201219639. Bibcode: 2013A&A...551A..90M. 
  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. doi:10.1088/0004-637X/761/1/46. Bibcode: 2012ApJ...761...46W. 
  24. ↑ 24.0 24.1 24.2 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, doi:10.1051/0004-6361/201220268 
  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, doi:10.1051/0004-6361/201118014, Bibcode: 2012A&A...548A.118L 
  26. ↑ Jenkins, J. S.; Jones, H. R. A.; Tuomi, M.; Murgas, F.; Hoyer, S.; Jones, M. I.; Barnes, J. R.; Pavlenko, Y. V. et al. (2012), "A Hot Uranus Orbiting the Super Metal-Rich Star Hd 77338 and the Metallicity-Mass Connection", The Astrophysical Journal 766 (2): 67, doi:10.1088/0004-637X/766/2/67 
  27. ↑ 27.0 27.1 27.2 Robertson, Paul; Endl, Michael; Cochran, William D.; MacQueen, Phillip J.; Wittenmyer, Robert A.; Horner, J.; Brugamyer, Erik J.; Simon, Attila E. et al. (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. doi:10.1088/0004-637X/749/1/39. Bibcode: 2012ApJ...749...39R. 
  28. ↑ 28.0 28.1 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, doi:10.1088/0004-637X/756/1/91, Bibcode: 2012ApJ...756...91H 
  29. ↑ 29.0 29.1 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, doi:10.3847/1538-3881/ab855a, Bibcode: 2020AJ....159..235L 
  30. ↑ 30.0 30.1 Lee, B.-C.; Han, I.; Park, M.-G. (2012), "Planetary companions orbiting M giants HD 208527 and HD 220074", Astronomy & Astrophysics 549: A2, doi:10.1051/0004-6361/201220301 
  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. doi:10.1051/0004-6361/201219391. Bibcode: 2012A&A...543A.138B. 
  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 et al. (November 15, 2012). "Direct Imaging Discovery of a 'Super-Jupiter' Around the late B-Type Star Kappa And". The Astrophysical Journal 763 (2): L32. doi:10.1088/2041-8205/763/2/L32. Bibcode: 2013ApJ...763L..32C. 
  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, doi:10.1088/0004-637X/750/2/114, Bibcode: 2012ApJ...750..114F 
  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. doi:10.1088/2041-8205/756/2/L39. Bibcode: 2012ApJ...756L..39B. 
  36. ↑ 36.0 36.1 36.2 36.3 36.4 36.5 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, doi:10.1088/0004-637X/750/2/114, Bibcode: 2012ApJ...750..114F 
  37. ↑ Lissauer, Jack J.; Marcy, Geoffrey W.; Rowe, Jason F.; Bryson, Stephen T.; Adams, Elisabeth; Buchhave, Lars A.; Ciardi, David R.; Cochran, William D. et al. (10 May 2012). "Almost All of Kepler's Multiple Planet Candidates are Planets". The Astrophysical Journal 750 (2): 112. doi:10.1088/0004-637X/750/2/112. Bibcode: 2012ApJ...750..112L. 
  38. ↑ 38.0 38.1 Welsh, William F. et al. (2012). "Transiting circumbinary planets Kepler-34 b and Kepler-35 b". Nature 481 (7382): 475–479. doi:10.1038/nature10768. PMID 22237021. Bibcode: 2012Natur.481..475W. 
  39. ↑ 39.0 39.1 Carter, J. A. et al. (2012). "Kepler-36: A Pair of Planets with Neighboring Orbits and Dissimilar Densities". Science 337 (6094): 556–559. doi:10.1126/science.1223269. PMID 22722249. Bibcode: 2012Sci...337..556C. 
  40. ↑ Orosz, Jerome A. et al. (2012), "THE NEPTUNE-SIZED CIRCUMBINARY PLANET KEPLER-38b", The Astrophysical Journal 758 (2): 87, doi:10.1088/0004-637X/758/2/87, Bibcode: 2012ApJ...758...87O 
  41. ↑ 41.0 41.1 Nesvorny, D. et al. (2012). "The Detection and Characterization of a Nontransiting Planet by Transit Timing Variations". Science 336 (6085): 1133–6. doi:10.1126/science.1221141. PMID 22582018. Bibcode: 2012Sci...336.1133N. 
  42. ↑ 42.0 42.1 Orosz, Jerome A.; Welsh, William F.; Carter, Joshua A.; Fabrycky, Daniel C.; Cochran, William D.; Endl, Michael; Ford, Eric B.; Haghighipour, Nader et al. (2012). "Kepler-47: A Transiting Circumbinary Multi-Planet System". Science 337 (6101): 1511–4. doi:10.1126/science.1228380. PMID 22933522. Bibcode: 2012Sci...337.1511O. 
  43. ↑ 43.00 43.01 43.02 43.03 43.04 43.05 43.06 43.07 43.08 43.09 43.10 43.11 43.12 43.13 43.14 43.15 43.16 43.17 43.18 43.19 43.20 43.21 43.22 43.23 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, doi:10.1088/0067-0049/208/2/22 
  44. ↑ 44.00 44.01 44.02 44.03 44.04 44.05 44.06 44.07 44.08 44.09 44.10 44.11 44.12 44.13 44.14 44.15 44.16 44.17 44.18 44.19 44.20 44.21 44.22 44.23 44.24 44.25 44.26 Steffen, Jason H.; Fabrycky, Daniel C.; Agol, Eric; Ford, Eric B.; Morehead, Robert C.; Cochran, William D.; Lissauer, Jack J.; Adams, Elisabeth R. et al. (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, 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" (in en). The Astrophysical Journal 770 (1): 52. doi:10.1088/0004-637X/770/1/52. ISSN 0004-637X. Bibcode: 2013ApJ...770...52K. 
  46. ↑ 46.0 46.1 46.2 46.3 Rowe, Jason F.; Bryson, Stephen T.; Marcy, Geoffrey W.; Lissauer, Jack J.; Jontof-Hutter, Daniel; Mullally, Fergal; Gilliland, Ronald L.; Issacson, Howard et al. (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, doi:10.1088/0004-637X/784/1/45, Bibcode: 2014ApJ...784...45R 
  47. ↑ 47.0 47.1 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, doi:10.1088/0004-637X/778/2/110, Bibcode: 2013ApJ...778..110Y 
  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, 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, doi:10.1088/0004-637X/763/1/67 
  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. doi:10.1088/0004-637X/754/1/73. Bibcode: 2012ApJ...754...73B. 
  51. ↑ Blackman, J. W.; Beaulieu, J. P.; Bennett, D. P.; Danielski, C.; Alard, C.; Cole, A. A.; Vandorou, A.; Ranc, C. et al. (2021), "A Jovian analogue orbiting a white dwarf star", Nature 598 (7880): 272–275, doi:10.1038/s41586-021-03869-6, PMID 34646001, Bibcode: 2021Natur.598..272B 
  52. ↑ Bennett, D. P.; Sumi, T.; Bond, I. A.; Kamiya, K.; Abe, F.; Botzler, C. S.; Fukui, A.; Furusawa, K. et al. (2012), "Planetary and Other Short Binary Microlensing Events from the Moa Short-Event Analysis", The Astrophysical Journal 757 (2): 119, doi:10.1088/0004-637X/757/2/119, Bibcode: 2012ApJ...757..119B 
  53. ↑ 53.0 53.1 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, doi:10.1088/2041-8205/762/2/L28 
  54. ↑ 54.0 54.1 Quinn, Samuel N.; White, Russel J.; Latham, David W.; Buchhave, Lars A.; Cantrell, Justin R.; Dahm, Scott E.; Fűrész, Gabor; Szentgyorgyi, Andrew H. et al. (2012). "TWO "b"s IN THE BEEHIVE: THE DISCOVERY OF THE FIRST HOT JUPITERS IN AN OPEN CLUSTER". The Astrophysical Journal 756 (2): L33. doi:10.1088/2041-8205/756/2/L33. Bibcode: 2012ApJ...756L..33Q. 
  55. ↑ Rattanamala, R.; Awiphan, S.; Komonjinda, S.; Phriksee, A.; Sappankum, P.; A-thano, N.; Chitchak, S.; Rittipruk, P. et al. (2021), Two circumbinary planets in RR Cae eclipsing binary system 
  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. doi:10.1111/j.1745-3933.2012.01228.x. Bibcode: 2012MNRAS.422L..24Q. 
  57. ↑ 57.0 57.1 Tuomi, M; Jones, H R A; Jenkins, J S; Tinney, C G; Butler, R P; Vogt, S S; Barnes, J R; Wittenmyer, R A et al. (2013). "Signals embedded in the radial velocity noise". Astronomy & Astrophysics 551: A79. doi:10.1051/0004-6361/201220509. Bibcode: 2012yCat..35510079T. 
  58. ↑ 58.0 58.1 Lendl, M.; Anderson, D. R.; Collier-Cameron, A.; Doyle, A. P.; Gillon, M.; Hellier, C.; Jehin, E.; Lister, T. A. et al. (2012), "WASP-42 b and WASP-49 b: Two new transiting sub-Jupiters", Astronomy & Astrophysics 544: A72, doi:10.1051/0004-6361/201219585, Bibcode: 2012A&A...544A..72L 
  59. ↑ 59.0 59.1 59.2 59.3 59.4 59.5 59.6 Hellier, Coel; Anderson, D. R.; Collier Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Jehin, E.; Lendl, M. et al. (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, doi:10.1111/j.1365-2966.2012.21780.x, Bibcode: 2012MNRAS.426..739H 
  60. ↑ 60.0 60.1 60.2 60.3 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, doi:10.1051/0004-6361/201220363 
  61. ↑ 61.0 61.1 61.2 Faedi, F. (2013). "WASP-54b, WASP-56b, and WASP-57b: Three new sub-Jupiter mass planets from SuperWASP". Astronomy & Astrophysics 551: A73. doi:10.1051/0004-6361/201220520. Bibcode: 2013A&A...551A..73F. 
  62. ↑ 62.0 62.1 Gillon, M.; Anderson, D. R.; Collier-Cameron, A.; Doyle, A. P.; Fumel, A.; Hellier, C.; Jehin, E.; Lendl, M. et al. (2012), "WASP-64 b and WASP-72 b: Two new transiting highly irradiated giant planets", Astronomy & Astrophysics 552: A82, doi:10.1051/0004-6361/201220561 
  63. ↑ Smith, A. M. S.; Anderson, D. R.; Bouchy, F.; Collier Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hébrard, G. et al. (2013), "WASP-71b: A bloated hot Jupiter in a 2.9-day, prograde orbit around an evolved F8 star", Astronomy & Astrophysics 552: A120, doi:10.1051/0004-6361/201220727, Bibcode: 2013A&A...552A.120S 
  64. ↑ Maxted, P. F. L.; Anderson, D. R.; Collier Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hellier, C.; Jehin, E. et al. (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, doi:10.1086/669231 
  65. ↑ 65.0 65.1 Smalley, B.; Anderson, D. R.; Collier-Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hellier, C.; Jehin, E. et al. (2012), "WASP-78b and WASP-79b: Two highly-bloated hot Jupiter-mass exoplanets orbiting F-type stars in Eridanus", Astronomy & Astrophysics 547: A61, doi:10.1051/0004-6361/201219731, Bibcode: 2012A&A...547A..61S 
  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. doi:10.1088/0004-637X/758/1/57. Bibcode: 2012ApJ...758...57L. 
  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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