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List of exoplanets discovered in 2012

From Wikipedia, the free encyclopedia

This is aList of exoplanets discovered in 2012.[1]For exoplanets detected only by radial velocity, the mass value is actually a lower limit. (SeeMinimum mass for more information)

NameMass (MJ)Radius (RJ)Period (days)Semi-major axis (AU)Temp. (K)[2]Discovery methodDistance (ly)Host star mass (M)Host star temp. (K)Remarks
75 Ceti b3691.92.1radial vel.2662.494846[3]
BD+20 274 b4.2578.21.3radial vel.4500±3000.84296[4]
BD+48 740 b1.7±0.7733+5
−8
1.7±0.1radial vel.2214±721.09±0.164534±8[5] Confirmed in 2018.[6]
CoRoT-21b2.261.32.720.04171867transit4600±9001.296200[7]
Epsilon Coronae Borealis b6.7417.91.3radial vel.229.71.74406[8]
Gliese 676 Ad0.0143.60050.0413±0.0014radial vel.52.29±0.030.71±0.043734[9]
Gliese 676 Ae0.02535.390.187±0.007radial vel.52.29±0.030.71±0.043734[9]
Gliese 3470 b0.0430.3463.33664870.031radial vel.820.513652[10]
HAT-P-34b7.011.355.452650.067741520transit818.944.266442[11] Proper nameĠgantija
HAT-P-35b7.523.553.646710.04981581transit167723.566096[11]
HAT-P-36b1.84821.2771.327346830.02411781transit968.491.035620[11] Proper nameBran
HAT-P-37b1.1691.1782.7974360.03791271transit13410.935500[11] Additional planets in system are suspected[12]
HAT-P-38b0.2670.8254.6403820.0523transit8100.895330[13] Proper nameHiisi
HAT-P-39b0.5991.5713.543870.0509transit20901.46430[14]
HAT-P-40b0.6151.734.4572430.0608transit16301.516080[14] Proper nameVytis
HAT-P-41b0.81.6852.6940470.0426transit11201.426390[15][14][16]
HAT-P-42b1.0441.284.6418780.05751427transit14601.185743[17] Proper nameIolaus
HAT-P-43b0.6621.2813.3326870.04431361transit17701.055645[17]
HATS-1b1.8551.3023.4464590.0444transit9900.995870[18]
HD 142 c5.360056.8radial vel.83.61.236245[19]
HD 4732 b2.37360.21.19radial vel.1841.744959[20]
HD 4732 c2.3727324.6radial vel.1841.744959[20]
HD 5608 b1.4792.61.9radial vel.189.71.554854[3]
HD 24040 b4.10±0.123490±254.637±0.067radial vel.152.3±0.41.14±0.025917±52[21] Suspected since 2006
HD 27631 b1.4522083.25radial vel.145.30.945737[22]
HD 37605 c3.36627203.814radial vel.139.915448[23]
HD 40307 e0.0110±0.004434.62+0.21
−0.20
0.1886+0.083
−0.0104
radial vel.41.80.774956[24] Disputed planet.[25]
HD 40307 f0.016451.760.247radial vel.41.80.774956[24]
HD 40307 g0.0223197.80.6radial vel.41.80.774956[24] Disputed planet.[25]
HD 66141 b6480.51.2radial vel.261.11.14323[26]
HD 77338b0.055.73610.0614radial vel.134.60.935370[27]
HD 79498 b1.3418072.98radial vel.159.891.085748[28]
HD 98649 b6.849515.6radial vel.139.515759[22]
HD 106515 Ab9.6136304.59radial vel.118.60.975362[22]
HD 150706 b2.7158946.7radial vel.88.81.175961[21]
HD 159868 c0.73352.31radial vel.171.91.095558[19]
HD 166724 b3.5351445.42radial vel.140.20.815127[22]
HD 197037 b0.791035.72.07radial vel.107.11.063±0.0226137±20[28]
HD 207832 b0.56161.970.57radial vel.180.40.945710[29] Suspected false positive[30]
HD 207832 c0.731155.72.112radial vel.180.40.945710[29] Suspected false positive[30]
HD 208527 b9.9875.52.1radial vel.1148.41.64035[31]
HD 219077 b10.3955016.22radial vel.951.055362[22]
HD 219415 b12093.33.2radial vel.553.714820[4]
HD 220074 b11.1672.11.6radial vel.942.71.23935[31]
HD 220689 b1.0622093.36radial vel.147.51.045921[22]
HD 220773 b1.453724.74.94radial vel.159.821.165940[28]
HD 222155 b2.1239995.14radial vel.165.31.215701[21]
HW Virginis b14.346404.69timing5900.485[32] Likely false positive[33]
Kappa Andromedae b13.616551850imaging169.72.610900Has a reddish color, and may be abrown dwarf[34]
KELT-1b27.231.111.2175140.024662423transit8501.326518[35]
KELT-2Ab1.5221.2864.11379120.05496transit405.21.316151[36]
Kepler-30b0.0360.34829.334340.18transit46000.995498[37]
Kepler-30c2.011.09760.3231050.3transit46000.995498[37]
Kepler-30d0.0730.785143.343940.5transit46000.995498[37]
Kepler-32d0.24122.78020.13transit9900.583900[37]
Kepler-32e0.1342.8960.033transit9900.583900Weak evidence[37]
Kepler-32f0.0730.742960.013transit9900.583900Weak evidence[37]
Kepler-33f0.030360.39841.029020.2535transit40861.295904[38]
Kepler-34b0.220.764288.8221.0896transit48891.055913[39]
Kepler-35b0.1270.728131.4580.60347transit53650.895606[39]
Kepler-36b0.0140.13313.839890.1153transit15001.075911[40]
Kepler-36c0.0250.32816.238550.1283transit15001.075911[40]
Kepler-38b0.3840.384105.5990.4632transit20000.945623[41]
Kepler-46b60.80833.601340.1968transit27900.95309[42]
Kepler-46c0.37657.0110.2799timing27900.95309[42]
Kepler-47b20.2749.5320.2962transit49001.055636[43]
Kepler-47c280.411303.1370.991transit49001.055636[43]
Kepler-48b0.01240.1684.778transit1009±50.885194[44][45]
Kepler-48c0.045970.2429.67395transit1009±50.885194[44][45]
Kepler-49b [ru]0.980.2437.2037945transit1024±80.554252[44][45]
Kepler-49c [ru]0.720.22710.9129343transit1024±80.554252[44][45]
Kepler-50b [ru]0.1537.812540.077transit821±61.246225[45]
Kepler-50c [ru]0.1949.376470.087transit821±61.246225[45]
Kepler-51b0.0070.63345.1540.2514543transit2610±501.046018[45]
Kepler-51c0.0130.80385.3120.384439transit2610±501.046018[45]
Kepler-52b [ru]8.70.1877.8773565transit1058±70.544263[45]
Kepler-52c [ru]10.410.16416.3850021transit1058±70.544263[45]
Kepler-53b [ru]18.410.25818.6489525transit4600±2000.985858[44][45]
Kepler-53c [ru]15.740.28338.5583038transit4600±2000.985858[44][45]
Kepler-54b [ru]0.920.1878.0109434transit893±90.514252[45]
Kepler-54c [ru]0.370.1112.0717249transit893±90.514252[45]
Kepler-55b [ru]1.490.21727.9481449transit1920±300.624503[45]
Kepler-55c [ru]1.110.19742.1516418transit1920±300.624503[45]
Kepler-56b0.070.58110.50160.1028transit3060±801.324840[45]
Kepler-56c0.570.87421.402390.1652transit3060±801.324840[45]
Kepler-57b [ru]18.860.1955.72931960.057transit3140±300.835145[44][45]
Kepler-57c [ru]6.950.13811.60925670.092631transit3140±300.835145[44][45]
Kepler-58b [ru]1.390.24810.2184954transit3250±800.956099[44][45]
Kepler-58c [ru]2.190.25515.5741568transit3250±800.956099[44][45]
Kepler-59b2.050.09811.8681707transit3925±751.046074[45]
Kepler-59c1.370.17717.9801235transit3925±751.046074[45]
Kepler-60b [ru]0.013180.1537.1334transit3440±701.045905[45]
Kepler-60c [ru]0.012110.178.9187transit3440±701.045905[45]
Kepler-60d0.013090.17811.8981transit3440±701.045905[45]
Kepler-64b0.5310.551138.3170.652transit6200±10001.536407[46] Quadruple star system
Kepler-79b0.03430.3113.48450.117868transit3430±601.176174[44]
Kepler-79c0.0190.33227.40290.187685transit3430±601.176174[44]
Kepler-80b0.02180.2387.052460.0648transit11600.734540[44]
Kepler-80c0.021210.2449.523550.0792transit11600.734540[44]
Kepler-81b0.2165.955646transit1147±100.644500[44]
Kepler-81c0.21112.04513transit1147±100.644500[44]
Kepler-82b0.35726.444581transit3030±800.855428[44]
Kepler-82c0.47751.538464transit3030±800.855428[44]
Kepler-83b0.2529.77transit1320±170.664648[44][47]
Kepler-83c0.21120.09transit1320±170.664648[44][47]
Kepler-84b0.1998.726937transit4700±50016031[44][47]
Kepler-84c0.21112.883821transit4700±50016031[44][47]
Kepler-85b0.1768.306transit2550±500.925436[44] KOI-2038[48]
Kepler-85c0.19412.513transit2550±500.925436[44] KOI-2038[48]
MOA-2011-BLG-293Lb [ja]2.4+1.4
−0.9
1.0±0.1microlensing23000±20000.675±0.525[49]
MOA-2010-BLG-073Lb111.21microlensing91000.16Possibly brown dwarf[50]
MOA-2010-BLG-477Lb1.4±0.32.8±0.5microlensing7500±20000.53±0.115950±150[51] White dwarf host star[52]
MOA-bin-1Lb3.7±2.18.3+4.5
−2.7
microlensing170000.75+0.33
−0.41
[53]
Mu2 Octantis b6.936385.02radial vel.142.11.296017[22]
Nu Ophiuchi b24530.321.9radial vel.152.83.044928Brown dwarf or small star[3]
Nu Ophiuchi c2731866.1radial vel.152.83.044928Brown dwarf or small star[3]
OGLE-2012-BLG-0026Lb0.1454microlensing131101.06[54]
OGLE-2012-BLG-0026Lc0.864.8microlensing131101.06[54]
Omicron Coronae Borealis b1.5187.830.83radial vel.274.12.134749[3]
Omicron Ursae Majoris b4.116303.9radial vel.183.73.095242[3]
Pr0201 b0.544.4264radial vel.6101.236174[55] InBeehive Cluster
Pr0211 b1.882.14610.03176radial vel.6100.945300[55] Multi-planet system InBeehive Cluster
RR Caeli b3.0±0.31900±405.2±0.1timing69.10±0.030.18+0.443100+7540Circumbinary planet around red and white dwarfs.[56][57]
Tau Ceti e0.0124162.870.538radial vel.120.78[58] Potentially habitable exoplanet
Tau Ceti f0.0124636.131.334radial vel.120.78[58]
WASP-42b0.5271.1224.98168190.05611021±19transit5200.955315[59]
WASP-47b1.211.154.160710.0521275transit6501.115576[60]
WASP-49b0.3781.1152.78173870.03791369±39transit5500.945600[59]
WASP-52b0.461.271.74977980.02721315±35transit4600.875000[61] Proper nameGöktürk
WASP-54b0.6361.6533.69364110.049871742+49
−69
transit6501.216100[62]
WASP-55b0.6271.3354.46562910.05581290transit11001.166070[60]
WASP-56b0.5711.0924.6171010.054581200transit8301.035600[62]
WASP-57b0.6441.052.838918560.037691338±29transit14800.895600[62]
WASP-58b0.891.375.017180.05611270±80transit9800.945800[61]
WASP-59b0.8630.7757.9195850.0697670±35transit4100.724650[61]
WASP-60b0.5140.864.30500110.05311479±35transit13001.085900[61] Proper nameVlasina
WASP-61b2.061.243.85590.05141565±35transit16001.226320[60]
WASP-62b0.571.394.4119530.05671329.6±44.8transit5201.256280[60] Proper nameKrotoa
WASP-63b0.381.434.378090.05741536±37transit11001.325570[60]
WASP-64b1.2711.2711.57329180.026481989+87
−88
transit110015400[63] Proper nameAgouto
WASP-66b2.321.394.0860520.05461790±60transit12001.36580[60]
WASP-67b0.421.44.614420.05171050transit7300.875240[60]
WASP-71b2.2421.462.90367470.046192016.1+67.0
−52.5
transit11301.566059[64] Proper nameTanzanite
WASP-72b1.54611.272.21674210.037082210+120
−130
transit11001.396250[63] Proper nameCuptor
WASP-77Ab1.761.211.36003090.0241715transit30015500Orbiting primary star of binary star system[65]
WASP-78b0.891.72.175176320.03622350transit18001.176100[66]
WASP-79b0.92.093.66238660.05351900±50transit7801.386600[66] Proper namePollera
WISE 1217+1626 B220.9348450imaging29±30.03575Brown dwarf[67]
WTS-1b4.011.493.3520570.0471500±100transit8100±10001.26250[68]

Specific exoplanet lists

[edit]

Lists of exoplanets

Lists of exoplanets by year of discovery

[edit]


References

[edit]
  1. ^"NASA Exoplanet Archive". Retrieved20 December 2019.
  2. ^"The Extrasolar Planets Encyclopaedia". 1995. Retrieved2015-11-09.
  3. ^abcdefSato, 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. ^abGettel, 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. ^abAnglada-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.
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  11. ^abcdBakos, 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. ^abcHartman, 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.
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  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. ^abBoisse, 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
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  52. ^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
  53. ^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
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  55. ^abQuinn, 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.
  56. ^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
  57. ^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.
  58. ^abTuomi, 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.
  59. ^abLendl, 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
  60. ^abcdefgHellier, 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
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  63. ^abGillon, 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
  64. ^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
  65. ^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
  66. ^abSmalley, 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
  67. ^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.
  68. ^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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