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List of exoplanets discovered in 2013

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(Redirected fromHD 285507 b)

This is aList of exoplanets discovered in 2013.

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)[1]Discovery methodDistance (ly)Host star mass (M)Host star temp. (K)Remarks
2MASS J01225093-2439505 b24.552imaging1200.43530[2]
BD+15 2940 b1.11137.480.539radial vel.572.21.14796[3]
CoRoT-25b0.271.084.860690.0578transit33001.096040[4]
CoRoT-26b0.521.264.204740.0526transit54001.095590[4]
DENIS-P J082303.1-491201 b28.5246.360.36astrometry67.70.072150[5]
Gliese 163 b0.033358.631820.0607radial vel.48.80.43500[6]
Gliese 163 c0.021425.630580.1254radial vel.48.80.43500[6]
Gliese 163 d0.0925603.951161.0304radial vel.48.80.43500[6]
Gliese 221b0.0273.87280.0428radial vel.660.74324[7][8] Disputed[9]
Gliese 221 c0.17125.940.435radial vel.660.74324[7][8]
Gliese 328b2.341004.5radial vel.65.30.693900[10]
Gliese 504 b443.5imaging58.51.226234[11]
HAT-P-44b0.3521.2424.3012190.0507transit11800.945295[12]
HAT-P-44c4872.21.752radial vel.11800.945295Period is ambiguous[12]
HAT-P-45b0.8921.4263.1289920.0452transit9901.266330[12]
HAT-P-46b0.4931.2844.4631290.0577transit9701.286120[12]
HATS-2b1.3451.1681.3541330.023transit12000.885227[13]
HATS-3b1.0711.3813.5478510.04851648transit14801.216351[14]
HD 2952 b [ru]1.6311.61.2radial vel.375.82.544844[15]
HD 13908 b [fr]0.86519.3820.154radial vel.218.21.296255[16]
HD 13908 c [fr]5.139312.03radial vel.218.21.296255[16]
HD 65216c0.17152.60.54radial vel.116.10.925666[17] False positive, another planet with same assigned name discovered in 2019.[18]
HD 95086 b555.7imaging298.71.6[19]
HD 103774 b0.3675.88810.07radial vel.173.11.336489[7]
HD 106906 b11650imaging299.51.56516[20]
HD 109271 b0.0547.85430.079radial vel.185.61.055783[7]
HD 109271 c0.07630.930.196radial vel.185.61.055783[7]
HD 113337 b2.833240.92radial vel.122.01.46576.6[21]
HD 120084 b4.520824.3radial vel.318.52.394892[15]
HD 159243 b1.1312.620.11radial vel.223.71.126123[16]
HD 159243 c [fr]1.9248.40.8radial vel.223.71.126123[16]
HD 233604 b6.5751920.747radial vel.2830±901.54791[3]
HD 285507 b0.92±0.036.0962±0.0002radial vel.1530.73±0.034503+85
−61
member ofHyades (star cluster)[22][23]
HD 112410 b9.18124.60.565radial vel.486.81.544830[24]
HIP 91258 b [fr]1.0685.05050.057radial vel.145.00.955519[16]
KELT-3b1.4771.3452.70339040.04122transit5801.286306[25]
KELT-6b0.4421.187.84558210.08transit7201.136272[26]
Kepler-37b0.031460.02913.3675transit2200.85417[27]
Kepler-37c0.037760.06721.302transit2200.85417[27]
Kepler-37d0.038390.17339.7922transit2200.85417[27]
Kepler-61b0.19259.87756transit1103±160.644017[28]
Kepler-62b0.030.1175.7149320.0553transit12000.694925[29]
Kepler-62c0.0130.04812.44170.0929transit12000.694925[29]
Kepler-62d0.0440.17418.164060.12transit12000.694925[29]
Kepler-62e0.1130.144122.38740.427transit12000.694925Potentially habitable exoplanet[29]
Kepler-62f0.110.126267.2910.718transit12000.694925Potentially habitable exoplanet[29]
Kepler-63b0.3780.5459.43415050.08transit6500.985576[30]
Kepler-65b0.1272.154910.035transit999±81.256211[31]
Kepler-65c0.235.8599440.068transit999±81.256211[31]
Kepler-65d0.1368.131230.084transit999±81.256211[31]
Kepler-66b0.2517.8158150.1352transit36101.045962Belongs to open clusterNGC 6811[32]
Kepler-67b0.26215.72590.1171transit36100.865331Belongs to open clusterNGC 6811[32]
Kepler-68b0.018780.2085.398751280transit4401.085793[33]
Kepler-68c0.022650.0899.60504transit4401.085793[33]
Kepler-68d0.84007625radial vel.4401.085793[33]
Kepler-69b0.213.7223410.094transit2430±300.815638[34]
Kepler-69c0.153242.46130.64transit2430±300.815638[34][35]
Kepler-74b [es]0.630.967.3407110.0781transit43001.186000[36]
Kepler-75b [es]10.11.058.88491160.0818transit37000.915200[36]
Kepler-76b2.011.361.54492980.0274orbital brightness modulation2750±301.26409[37]
Kepler-77b [es]0.430.963.578780870.04501transit19000.955520[38]
Kepler-78b0.0060.1050.3552330transit407.1±1.10.765058[39]
Kepler-87b1.021.204114.736350.481478transit4170±901.15600Two more unconfirmed planets in the system[39]
Kepler-87c0.020.548191.23180.676403transit4170±901.15600Two more unconfirmed planets in the system[39]
Kepler-88b0.0270.33710.95416transit11100.965471[40]
Kepler-88c0.62622.33950.15525timing11100.965471[40][41]
Kepler-89b0.0330.1533.7432080.05119transit1577±161.286182[42]
Kepler-89c0.0490.38510.4236480.1013transit1577±161.286182[42]
Kepler-89d0.3341.00522.3429890.1684transit1577±161.286182[42]
Kepler-89e0.110.58554.320310.3046transit1577±161.286182[42]
Kepler-90b0.1177.0081510.0741056transit25001.26080[43]
Kepler-90c0.1068.7193750.089981transit25001.26080[43]
Kepler-90d0.25659.736670.32518transit25001.26080[43]
Kepler-90e0.23791.939130.42448transit25001.26080[43]
Kepler-90f0.257124.91440.48592transit25001.26080[43]
Kepler-90g0.723210.606970.71340transit25001.26080[43]
Kepler-90h1.008331.600591.01292transit25001.26080[43]
Kepler-91b0.811.3676.246580.0731transit34001.314550[44]
Kepler-92b0.2020.31313.749transit1580±171.215883[45]
Kepler-92c0.0190.23226.723transit1580±171.215883[45]
Kepler-102e0.0280.19816.1457579transit352.7±0.70.814909[46]
Kepler-105b0.4295.41220.066transit1517±180.965827[46]
Kepler-114c0.0090.1438.041623transit852±40.564605[45]
Kepler-114d0.0120.22611.776549transit852±40.564605[45]
Kepler-128b0.0970.10115.09transit1307±121.186090[45]
Kepler-128c0.1050.10122.804transit1307±121.186090[45]
Kepler-130b0.0918.4574580.079transit1042±715884[46]
Kepler-145b0.1170.23622.951transit1880±301.326022[45]
Kepler-145c0.250.38542.882transit1880±301.326022[45]
Kepler-177b0.0060.25936.855transit4880±1401.075942[45]
Kepler-177c0.0240.63349.412transit4880±1401.075942[45]
Kepler-238e0.5340.523.654transit6200±3001.065751[45]
Kepler-238f0.0420.17850.447transit6200±3001.065751[45]
Kepler-276c0.0520.25931.884transit3850±1501.16105[45]
Kepler-276d0.0510.2548.648transit3850±1501.16105[45]
Kepler-277b0.2750.26117.324transit3280±501.125946[45]
Kepler-277c0.2020.333.006transit3280±501.125946[45]
Kepler-279b0.32312.3096810.112transit3480±701.16363KOI-1236.01[47]
Kepler-279c0.1550.38435.736transit3490±701.16363KOI-1236.02[47][45]
Kepler-279d0.1180.27754.414transit3490±701.16363[45]
Kepler-282d0.1920.21924.806transit4540±1500.975602[45]
Kepler-282e0.1770.27744.347transit4540±1500.975602[45]
Kepler-305b0.0330.3215.487transit2900±900.765100[45] KOI-1563.01[47]
Kepler-305c0.0190.2948.291transit2900±900.765100[45] KOI-1563.02[47]
Kepler-307b0.023410.21710.4208transit1908±170.915367[45]
Kepler-307c0.011450.19613.0729transit1908±170.915367[45]
Kepler-328b0.090.20534.921transit7700±5001.155914[45]
Kepler-328c0.1240.48271.312transit7700±5001.155914[45]
Kepler-350c0.0190.27717.849transit3210±7016186[45]
Kepler-350d0.0470.2526.136transit3210±7016186[45]
Kepler-396b0.2380.31242.994transit734±50.855384[45] KOI-2672.01[47]
Kepler-396c0.0560.47388.505transit734±50.855384[45] KOI-2672.02[47]
Kepler-410Ab0.25317.8336480.1226transit4301.216273[48]
Kepler-411b0.1683.005160.0381040transit503.5±1.50.834974[46]
Kepler-1359c0.3711+0.12
−0.06
505.46+0.05
−0.04
1.143±0.018transit2182+81
−82
0.78+0.03
−0.04
4709+46
−56
[43] Also called KIC 6436029 c, discovery retracted in 2015 after 3rd transit was proven to be false.[49]
MOA-2008-BLG-379Lb4.13.3microlensing110000.56[50]
MOA-2010-BLG-328Lb0.028950.92microlensing26000.11[51]
MOA-2011-BLG-262Lb0.0566340.3831microlensing228300.13300Host star may be arogue planet, planet may be anexomoon[52]
MOA-2011-BLG-262L4N/Amicrolensing228303300Host star may be arogue planet, planet may be anexomoon[52]
MOA-2011-BLG-293Lb4.81.1microlensing252000.86[53]
MOA-2011-BLG-322Lb11.64.3microlensing247000.39[54]
OGLE-2011-BLG-0251Lb0.532.72microlensing84000.26[55]
OGLE-2012-BLG-358Lb1.850.87microlensing57000.02Orbiting a brown dwarf[56]
OGLE-2012-BLG-406Lb2.733.45microlensing162000.44[57]
Omega Serpentis b1.7277.021.1radial vel.263.02.174770[15]
PH2b0.903282.52550.828281transit1130±100.945629[58] Also called Kepler-86b
POTS-1b2.310.9413.16062960.03734transit39000.694400[59]
PSO J318.5−226.51.53N/AN/A1160imaging80N/AN/ARogue planet[60]
ROXs 12b16210imaging3900.873850[61]
ROXs 42Bb9157imaging4401[61]
WASP-8c9.4543235.28radial vel.2801.035600[62]
WASP-65b1.551.1122.31142430.0334transit10000.935600[63]
WASP-68b0.951.245.0842980.06206transit962±81.245911[64]
WASP-69b0.261.0573.86813820.04525963transit1600.834715[65]
WASP-70Ab0.591.1643.71302030.048531387transit8001.115763[65]
WASP-73b1.881.164.087220.055121790transit1042±91.346036[64]
WASP-75b1.071.272.4841930.0375transit8501.146100[63][66]
WASP-76b0.921.831.8098860.0332190transit3901.466250[67]
WASP-80b0.5380.9993.067852340.0344transit2000.584143[68] Proper nameWadirum
WASP-82b [fr]1.241.672.7057820.04472190transit6501.636490[67]
WASP-84b0.6940.9428.52348650.0771797transit4100.845314[65]
WASP-88b0.561.74.9540.064311775transit1730±301.456431[64]
WASP-90b0.63±0.071.63±0.093.916243±0.0000030.0562±0.00121840±50transit1100±2001.55±0.106440±130[67]
WASP-95b1.13+0.1
−0.04
1.21±0.062.184673±0.00000140.03416±0.000831570±50transit450±21.11±0.095630±130[69]
WASP-96b0.48±0.031.2±0.063.4252602±0.00000270.0453±0.00131285±40transit1161±151.06±0.095540±140[69]
WASP-97b1.32±0.051.13±0.062.07276±0.0000010.03303±0.000561555±40transit494.9±1.71.12±0.065640±100[69]
WASP-98b0.83±0.071.10±0.042.96264036±0.00000130.03762±0.0011180±30transit926±50.69±0.065525±130[69]
WASP-99b2.78±0.131.10+0.08
−0.05
5.75251±0.000040.0717±0.00161480±40transit519±21.48±0.106180±100[69]
WASP-100b2.03±0.121.69±0.292.849375±0.0000080.0457±0.00102190±140transit1201±91.57±0.106900±120[69]
WASP-101b0.50±0.041.41±0.053.585722±0.0000040.0506±0.00091560±35transit660±31.34±0.076400±110[69]
WTS-2b1.121.3631.01870680.018552000transit33000.825000[70][71]

Specific exoplanet lists

[edit]

Lists of exoplanets

Lists of exoplanets by year of discovery

[edit]


References

[edit]
  1. ^"The Extrasolar Planets Encyclopaedia". 1995. Retrieved2015-11-09.
  2. ^PLANETS AROUND LOW-MASS STARS. III. A YOUNG DUSTY L DWARF COMPANION AT THE DEUTERIUM-BURNING LIMIT
  3. ^abBD+15 2940 AND HD 233604: TWO GIANTS WITH PLANETS CLOSE TO THE ENGULFMENT ZONE
  4. ^abTransiting exoplanets from the CoRoT space mission XXIV. CoRoT-25b and CoRoT-26b: two low-density giant planets
  5. ^Sahlmann, J.; Lazorenko, P. F.; Ségransan, D.; Martín, Eduardo L.; Queloz, D.; Mayor, M.; Udry, S. (2013), "Astrometric orbit of a low-mass companion to an ultracool dwarf",Astronomy & Astrophysics,556: A133,arXiv:1306.3225,Bibcode:2013A&A...556A.133S,doi:10.1051/0004-6361/201321871,S2CID 119193690
  6. ^abcTuomi, M.; Anglada-Escudé, G. (2013). "Up to four planets around the M dwarf GJ 163".Astronomy & Astrophysics.556: A111.arXiv:1306.1717.doi:10.1051/0004-6361/201321174.S2CID 16214668.
  7. ^abcdeLo Curto, G.; Mayor, M.; Benz, W.; Bouchy, F.; Hébrard, G.; Lovis, C.; Moutou, C.; Naef, D.; Pepe, F.; Queloz, D.; Santos, N. C.; Segransan, D.; Udry, S. (2013). "The HARPS search for southern extrasolar planets: XXXVI. New multi-planet systems in the HARPS volume limited sample: a super-Earth and a Neptune in the habitable zone".Astronomy & Astrophysics.551: 7.arXiv:1301.2741.Bibcode:2013A&A...551A..59L.doi:10.1051/0004-6361/201220415.S2CID 116916728. A59.
  8. ^abArriagada, Pamela; Anglada-Escudé, Guillem; Butler, R. Paul; Crane, Jeffrey D.; Shectman, Stephen A.; Thompson, Ian; Wende, Sebastian; Minniti, Dante (2013), "Two planetary companions around the K7 dwarf GJ 221 : a hot super-Earth and a candidate in the sub-Saturn desert range",The Astrophysical Journal,771 (1): 42,arXiv:1305.2203,Bibcode:2013ApJ...771...42A,doi:10.1088/0004-637X/771/1/42,S2CID 119212312
  9. ^Simpson, Emilie R.; Fetherolf, Tara; Kane, Stephen R.; Li, Zhexing; Pepper, Joshua; Močnik, Teo (2022), "Revisiting BD-06 1339b: A Likely False Positive Caused by Stellar Activity",The Astronomical Journal,163 (5): 215,arXiv:2203.06191,Bibcode:2022AJ....163..215S,doi:10.3847/1538-3881/ac5d41,S2CID 247446960
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  12. ^abcdHartman, J. D.; Bakos, G. Á.; Torres, G.; Kovács, G.; Johnson, J. A.; Howard, A. W.; Marcy, G. W.; Latham, D. W.; Bieryla, A.; Buchhave, L. A.; Bhatti, W.; Béky, B.; Csubry, Z.; Penev, K.; De Val-Borro, M.; Noyes, R. W.; Fischer, D. A.; Esquerdo, G. A.; Everett, M.; Szklenár, T.; Zhou, G.; Bayliss, D.; Shporer, A.; Fulton, B. J.; Sanchis-Ojeda, R.; Falco, E.; Lázár, J.; Papp, I.; Sári, P. (2013), "HAT-P-44b, HAT-P-45b, AND HAT-P-46b: THREE TRANSITING HOT JUPITERS IN POSSIBLE MULTI-PLANET SYSTEMS",The Astronomical Journal,147 (6): 128,arXiv:1308.2937,doi:10.1088/0004-6256/147/6/128,S2CID 119293498
  13. ^Mohler-Fischer, M.; Mancini, L.; Hartman, J. D.; Bakos, G. Á.; Penev, K.; Bayliss, D.; Jordán, A.; Csubry, Z.; Zhou, G.; Rabus, M.; Nikolov, N.; Brahm, R.; Espinoza, N.; Buchhave, L. A.; Béky, B.; Suc, V.; Csák, B.; Henning, T.; Wright, D. J.; Tinney, C. G.; Addison, B. C.; Schmidt, B.; Noyes, R. W.; Papp, I.; Lázár, J.; Sári, P.; Conroy, P. (2013), "HATS-2b: A transiting extrasolar planet orbiting a K-type star showing starspot activity",Astronomy & Astrophysics,558: A55,arXiv:1304.2140,Bibcode:2013A&A...558A..55M,doi:10.1051/0004-6361/201321663,S2CID 59134384
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  16. ^abcdeMoutou, Claire; Hébrard, Guillaume; Bouchy, François; Arnold, Luc; Santos, Nuno C.; Astudillo-Defru, Nicola; Boisse, Isabelle; Bonfils, Xavier; Borgniet, Simon; Delfosse, Xavier; Díaz, Rodrigo F.; Ehrenreich, David; Forveille, Thierry; Gregório, João; Labrevoir, Olivier; Lagrange, Anne-Marie; Montagnier, Guillaume; Montalto, Marco; Pepe, Francesco; Sahlmann, Johannes; Santerne, Alexandre; Ségransan, Damien; Udry, Stéphane; Vanhuysse, Michael (2013),The SOPHIE search for northern extrasolar planets VI. Three new hot Jupiters in multi-planet extrasolar systems,arXiv:1311.5271,doi:10.1051/0004-6361/201322067,S2CID 118676953
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  18. ^Wittenmyer, Robert A.; et al. (2019)."Truly eccentric – I. Revisiting eight single-eccentric planetary systems".Monthly Notices of the Royal Astronomical Society.484 (4):5859–5867.arXiv:1901.08471.Bibcode:2019MNRAS.484.5859W.doi:10.1093/mnras/stz290.
  19. ^Rameau, J., Chauvin, G., Lagrange, A.-M., Boccaletti, A., Quanz, S. P., Currie, T., Mawet, D., Girard, J. H., Bonnefoy, M., Kenworthy, M. (2013). "Confirmation of the planet around HD 95086 by direct imaging".The Astrophysical Journal.779 (2): L26.arXiv:1310.7483.Bibcode:2013ApJ...779L..26R.doi:10.1088/2041-8205/779/2/L26.S2CID 28985252.{{cite journal}}: CS1 maint: multiple names: authors list (link)
  20. ^Bailey, Vanessa; et al. (January 2014). "HD 106906 b: A planetary-mass companion outside a massive debris disk".The Astrophysical Journal Letters.780 (1): L4.arXiv:1312.1265.Bibcode:2014ApJ...780L...4B.doi:10.1088/2041-8205/780/1/L4.S2CID 119113709.
  21. ^Borgniet, Simon; Boisse, Isabelle; Lagrange, Anne-Marie; Bouchy, François; Arnold, Luc; Díaz, Rodrigo F.; Galland, Franck; Delorme, Philippe; Hébrard, Guillaume; Santerne, Alexandre; Ehrenreich, David; Ségransan, Damien; Bonfils, Xavier; Delfosse, Xavier; Santos, Nuno C.; Forveille, Thierry; Moutou, Claire; Udry, Stéphane; Eggenberger, Anne; Pepe, Francesco; Astudillo-Defru, Nicola; Montagnier, Guillaume (2013), "Extrasolar planets and brown dwarfs around A--F type stars. VIII. A giant planet orbiting the young star HD113337",Astronomy & Astrophysics,561: A65,arXiv:1310.1994,doi:10.1051/0004-6361/201321783,S2CID 118538542
  22. ^Carleo, I.; et al. (2020). "The GAPS Programme at TNG XXI -- A GIARPS case-study of known young planetary candidates: Confirmation of HD 285507 b and refutation of AD Leo B".Astronomy & Astrophysics.A5: 638.arXiv:2002.10562.Bibcode:2020A&A...638A...5C.doi:10.1051/0004-6361/201937369.S2CID 211296466.
  23. ^Open exoplanet catalogue HD 285507
  24. ^Jones, M. I.; et al. (2013). "Study of the Impact of the Post-MS evolution of the Host Star on the Orbits of Close-in Planets. II. A Giant Planet in a Close-in Orbit around the RGB Star HIP 63242".Astronomy & Astrophysics.556 (A78): 5.arXiv:1306.3939.Bibcode:2013A&A...556A..78J.doi:10.1051/0004-6361/201321660.S2CID 118618692.
  25. ^Pepper, Joshua; Siverd, Robert J.; Beatty, Thomas G.; Gaudi, B. Scott; Stassun, Keivan G.; Eastman, Jason; Collins, Karen; Latham, David W.; Bieryla, Allyson; Buchhave, Lars A.; Jensen, Eric L. N. (2013-08-01)."KELT-3b: A Hot Jupiter Transiting a V = 9.8 Late-F Star".The Astrophysical Journal.773 (1): 64.arXiv:1211.1031.Bibcode:2013ApJ...773...64P.doi:10.1088/0004-637X/773/1/64.ISSN 0004-637X.S2CID 14691090.
  26. ^Collins, Karen A.; et al. (2013), "KELT-6b: AP~ 7.9 DAY HOT SATURN TRANSITING a METAL-POOR STAR WITH a LONG-PERIOD COMPANION",The Astronomical Journal,147 (2): 39,arXiv:1308.2296,doi:10.1088/0004-6256/147/2/39,S2CID 15020416
  27. ^abcBarclay, Thomas; et al. (2013), "A sub-Mercury-sized exoplanet",Nature,494 (7438):452–454,arXiv:1305.5587,Bibcode:2013Natur.494..452B,doi:10.1038/nature11914,PMID 23426260,S2CID 205232792
  28. ^Exoplanet Characterization by Proxy: a Transiting 2.15 R_Earth Planet Near the Habitable Zone of the Late K dwarf Kepler-61 Sarah Ballard, David Charbonneau, Francois Fressin, Guillermo Torres, Jonathan Irwin, Jean-Michel Desert, Elisabeth Newton, Andrew W. Mann, David R. Ciardi, Justin R. Crepp, Christopher E. Henze, Stephen T. Bryson, Steven B. Howell, Elliott P. Horch, Mark E. Everett, Avi Shporeret al. April 26, 2013
  29. ^abcdeBorucki, William J.; et al. (2013), "Kepler-62: A Five-Planet System with Planets of 1.4 and 1.6 Earth Radii in the Habitable Zone",Science,340 (6132):587–590,arXiv:1304.7387,Bibcode:2013Sci...340..587B,doi:10.1126/science.1234702,PMID 23599262,S2CID 21029755
  30. ^Sanchis-Ojeda, Roberto; Winn, Joshua N.; Marcy, Geoffrey W.; Howard, Andrew W.; Isaacson, Howard; Johnson, John Asher; Torres, Guillermo; Albrecht, Simon; Campante, Tiago L.; Chaplin, William J.; Davies, Guy R.; Lund, Mikkel N.; Carter, Joshua A.; Dawson, Rebekah I.; Buchhave, Lars A.; Everett, Mark E.; Fischer, Debra A.; Geary, John C.; Gilliland, Ronald L.; Horch, Elliott P.; Howell, Steve B.; Latham, David W. (2013), "KEPLER-63b: A GIANT PLANET IN a POLAR ORBIT AROUND a YOUNG SUN-LIKE STAR",The Astrophysical Journal,775 (1): 54,arXiv:1307.8128,Bibcode:2013ApJ...775...54S,doi:10.1088/0004-637X/775/1/54,S2CID 36615256
  31. ^abcChaplin, W. J.; Sanchis-Ojeda, R.; Campante, T. L.; Handberg, R.; Stello, D.; Winn, J. N.; Basu, S.; Christensen-Dalsgaard, J.; Davies, G. R.; Metcalfe, T. S.; Buchhave, L. A.; Fischer, D. A.; Bedding, T. R.; Cochran, W. D.; Elsworth, Y.; Gilliland, R. L.; Hekker, S.; Huber, D.; Isaacson, H.; Karoff, C.; Kawaler, S. D.; Kjeldsen, H.; Latham, D. W.; Lund, M. N.; Lundkvist, M.; Marcy, G. W.; Miglio, A.; Barclay, T.; Lissauer, J. J. (2013), "Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65",The Astrophysical Journal,766 (2): 101,arXiv:1302.3728,Bibcode:2013ApJ...766..101C,doi:10.1088/0004-637X/766/2/101,S2CID 17748525
  32. ^abThe same frequency of planets inside and outside open clusters of stars
  33. ^abcGilliland, Ronald L.; et al. (2013)."Kepler-68: Three Planets, One with a Density Between That of Earth and Ice Giants".The Astrophysical Journal.766 (1). 40.arXiv:1302.2596.Bibcode:2013ApJ...766...40G.doi:10.1088/0004-637X/766/1/40.
  34. ^abBarclay, Thomas; et al. (2013), "A Super-Earth-Sized Planet Orbiting in or Near the Habitable Zone Around a Sun-Like Star",The Astrophysical Journal,768 (2): 101,arXiv:1304.4941,Bibcode:2013ApJ...768..101B,doi:10.1088/0004-637X/768/2/101,S2CID 51490784
  35. ^Kane, Stephen R.; Barclay, Thomas; Gelino, Dawn M. (2013), "A Potential Super-Venus in the Kepler-69 System",The Astrophysical Journal,770 (2): L20,arXiv:1305.2933,Bibcode:2013ApJ...770L..20K,doi:10.1088/2041-8205/770/2/L20,S2CID 9808447
  36. ^abHébrard, G.; Almenara, J.-M.; Santerne, A.; Deleuil, M.; Damiani, C.; Bonomo, A. S.; Bouchy, F.; Bruno, G.; Díaz, R. F.; Montagnier, G.; Moutou, C. (2013), "KOI-200 b and KOI-889 b: Two transiting exoplanets detected and characterized withKepler, SOPHIE, and HARPS-N",Astronomy & Astrophysics,554: A114,arXiv:1304.6002,Bibcode:2013A&A...554A.114H,doi:10.1051/0004-6361/201321394,S2CID 55185674
  37. ^Faigler, S.; et al. (2013). "BEER Analysis of Kepler and CoRoT Light Curves. I. Discovery of Kepler-76b: A Hot Jupiter with Evidence for Superrotation".The Astrophysical Journal.771 (1). 26.arXiv:1304.6841.Bibcode:2013ApJ...771...26F.doi:10.1088/0004-637X/771/1/26.S2CID 119247392.
  38. ^Gandolfi, D.; Parviainen, H.; Fridlund, M.; Hatzes, A. P.; Deeg, H. J.; Frasca, A.; Lanza, A. F.; Prada Moroni, P. G.; Tognelli, E.; McQuillan, A.; Aigrain, S.; Alonso, R.; Antoci, V.; Cabrera, J.; Carone, L.; Csizmadia, Sz.; Djupvik, A. A.; Guenther, E. W.; Jessen-Hansen, J.; Ofir, A.; Telting, J. (2013), "Kepler-77b: A very low albedo, Saturn-mass transiting planet around a metal-rich solar-like star",Astronomy & Astrophysics,557: A74,arXiv:1305.3891,Bibcode:2013A&A...557A..74G,doi:10.1051/0004-6361/201321901,S2CID 30232940
  39. ^abcOfir, Aviv; Dreizler, Stefan; Zechmeister, Mathias; Husser, Tim-Oliver (2013), "An independent planet search in theKeplerdataset",Astronomy & Astrophysics,561: A103,arXiv:1310.2064,doi:10.1051/0004-6361/201220935,S2CID 118691606
  40. ^abNesvorný, David; Kipping, David; Terrell, Dirk; Hartman, Joel; Bakos, Gáspár Á.; Buchhave, Lars A. (2013), "Koi-142, the King of Transit Variations, is a Pair of Planets Near the 2:1 Resonance",The Astrophysical Journal,777 (1): 3,arXiv:1304.4283,Bibcode:2013ApJ...777....3N,doi:10.1088/0004-637X/777/1/3,S2CID 59933168
  41. ^Barros, S. C. C.; Díaz, R. F.; Santerne, A.; Bruno, G.; Deleuil, M.; Almenara, J.-M.; Bonomo, A. S.; Bouchy, F.; Damiani, C.; Hébrard, G.; Montagnier, G.; Moutou, C. (2013), "SOPHIE velocimetry ofKeplertransit candidates",Astronomy & Astrophysics,561: L1,arXiv:1311.4335,doi:10.1051/0004-6361/201323067,S2CID 118446884
  42. ^abcdMasuda, Kento; et al. (2013)."Characterization of the KOI-94 System with Transit Timing Variation Analysis: Implication for the Planet-Planet Eclipse".The Astrophysical Journal.778 (2). 185.arXiv:1310.5771.Bibcode:2013ApJ...778..185M.doi:10.1088/0004-637X/778/2/185.
  43. ^abcdefghSchmitt, Joseph R.; et al. (2013), "Planet Hunters. Vi. An Independent Characterization of Koi-351 and Several Long Period Planet Candidates from Thekeplerarchival Data",The Astronomical Journal,148 (2): 28,arXiv:1310.5912,doi:10.1088/0004-6256/148/2/28,S2CID 119238163
  44. ^Lillo-Box, J.; Barrado, D.; Moya, A.; Montesinos, B.; Montalbán, J.; Bayo, A.; Barbieri, M.; Régulo, C.; Mancini, L.; Bouy, H.; Henning, T. (2013). "Kepler-91b: A planet at the end of its life. Planet and giant host star properties via light-curve variations".Astronomy & Astrophysics.562: A109.arXiv:1312.3943.Bibcode:2014A&A...562A.109L.doi:10.1051/0004-6361/201322001.S2CID 118486056.
  45. ^abcdefghijklmnopqrstuvwxyzaaabacadXie, Ji-Wei (2013), "Transit Timing Variation of Near-Resonance Planetary Pairs. Ii. Confirmation of 30 Planets in 15 Multiple-Planet Systems",The Astrophysical Journal Supplement Series,210 (2): 25,arXiv:1309.2329,doi:10.1088/0067-0049/210/2/25,S2CID 119105092
  46. ^abcdWang, Ji; Xie, Ji-Wei; Barclay, Thomas; Fischer, Debra A. (2013), "Influence of Stellar Multiplicity on Planet Formation. I. Evidence of Suppressed Planet Formation Due to Stellar Companions within 20 Au and Validation of Four Planets from Thekeplermultiple Planet Candidates",The Astrophysical Journal,783 (1): 4,arXiv:1309.7097,Bibcode:2014ApJ...783....4W,doi:10.1088/0004-637X/783/1/4,S2CID 119214390
  47. ^abcdefYang, Ming; Liu, Hui-Gen; Zhang, Hui; Zhou, Ji-Lin (2013), "8 Planets in 4 Multi-planet Systems via TTVs in 1350 Days",The Astrophysical Journal,778 (2): 110,arXiv:1308.0996,Bibcode:2013ApJ...778..110Y,doi:10.1088/0004-637X/778/2/110,S2CID 117080296
  48. ^Van Eylen, V.; Lund, M. N.; Aguirre, V. Silva; Arentoft, T.; Kjeldsen, H.; Albrecht, S.; Chaplin, W. J.; Isaacson, H.; Pedersen, M. G.; Jessen-Hansen, J.; Tingley, B.; Christensen-Dalsgaard, J.; Aerts, C.; Campante, T. L.; Bryson, S. T. (2013), "WHAT ASTEROSEISMOLOGY CAN DO FOR EXOPLANETS: KEPLER-410A b IS a SMALL NEPTUNE AROUND a BRIGHT STAR, IN AN ECCENTRIC ORBIT CONSISTENT WITH LOW OBLIQUITY",The Astrophysical Journal,782 (1): 14,arXiv:1312.4938,Bibcode:2014ApJ...782...14V,doi:10.1088/0004-637X/782/1/14,S2CID 15893540
  49. ^Wang, Ji; et al. (2015), "Planet Hunters. Viii. Characterization of 41 Long-Period Exoplanet Candidates from Kepler Archival Data",The Astrophysical Journal,815 (2): 127,arXiv:1512.02559,Bibcode:2015ApJ...815..127W,doi:10.1088/0004-637X/815/2/127,S2CID 6327352
  50. ^Suzuki, D.; et al. (2013), "MOA-2008-BLG-379Lb: A MASSIVE PLANET FROM a HIGH MAGNIFICATION EVENT WITH a FAINT SOURCE",The Astrophysical Journal,780 (2): 123,arXiv:1311.3424,doi:10.1088/0004-637X/780/2/123,S2CID 119257768
  51. ^Furusawa, K.; et al. (2013), "MOA-2010-BLG-328Lb: A SUB-NEPTUNE ORBITING VERY LATE M DWARF?",The Astrophysical Journal,779 (2): 91,arXiv:1309.7714,Bibcode:2013ApJ...779...91F,doi:10.1088/0004-637X/779/2/91,S2CID 59519570
  52. ^abMOA-2011-BLG-262Lb: A SUB-EARTH-MASS MOON ORBITING A GAS GIANT PRIMARY OR A HIGH VELOCITY PLANETARY SYSTEM IN THE GALACTIC BULGE
  53. ^Batista, V.; Beaulieu, J. -P.; Gould, A.; Bennett, D. P.; Yee, J. C.; Fukui, A.; Gaudi, B. S.; Sumi, T.; Udalski, A. (2013), "MOA-2011-BLG-293Lb: First Microlensing Planet possibly in the Habitable Zone",The Astrophysical Journal,780: 54,arXiv:1310.3706,doi:10.1088/0004-637X/780/1/54,S2CID 118442165
  54. ^Shvartzvald, Y.; et al. (2013), "MOA-2011-BLG-322Lb: A 'second generation survey' microlensing planet",Monthly Notices of the Royal Astronomical Society,439:604–610,arXiv:1310.0008,doi:10.1093/mnras/stt2477
  55. ^Kains, N.; Street, R. A.; Choi, J.-Y.; Han, C.; Udalski, A.; Almeida, L. A.; Jablonski, F.; Tristram, P. J.; Jørgensen, U. G.; Szymański, M. K.; Kubiak, M.; Pietrzyński, G.; Soszyński, I.; Poleski, R.; Kozłowski, S.; Pietrukowicz, P.; Ulaczyk, K.; Wyrzykowski, Ł.; Skowron, J.; Alsubai, K. A.; Bozza, V.; Browne, P.; Burgdorf, M. J.; Calchi Novati, S.; Dodds, P.; Dominik, M.; Dreizler, S.; Fang, X.-S.; Grundahl, F.; et al. (2013), "A Giant Planet beyond the Snow Line in Microlensing Event OGLE-2011-BLG-0251",Astronomy & Astrophysics,552: A70,arXiv:1303.1184,Bibcode:2013A&A...552A..70K,doi:10.1051/0004-6361/201220626,S2CID 43146154
  56. ^Han, C.; et al. (2013), "Microlensing Discovery of a Tight, Low-Mass-Ratio Planetary-Mass Object Around an Old Field Brown Dwarf",The Astrophysical Journal,778 (1): 38,arXiv:1307.6335,Bibcode:2013ApJ...778...38H,doi:10.1088/0004-637X/778/1/38,S2CID 118663575
  57. ^Poleski, Radosław; Udalski, Andrzej; Dong, Subo; Szymański, Michał K.; Soszyński, Igor; Kubiak, Marcin; Pietrzyński, Grzegorz; Kozłowski, Szymon; Pietrukowicz, Paweł; Ulaczyk, Krzysztof; Skowron, Jan; Wyrzykowski, Łukasz; Gould, Andrew (2014), "SUPER-MASSIVE PLANETS AROUND LATE-TYPE STARS—THE CASE OF OGLE-2012-BLG-0406Lb",The Astrophysical Journal,782 (1): 47,arXiv:1307.4084,Bibcode:2014ApJ...782...47P,doi:10.1088/0004-637X/782/1/47,S2CID 118695225
  58. ^Wang, Ji (January 3, 2013). "Planet Hunters. V. A Confirmed Jupiter-Size Planet in the Habitable Zone and 42 Planet Candidates from the Kepler Archive Data".arXiv:1301.0644v1 [astro-ph].
  59. ^Koppenhoefer, J.; Saglia, R. P.; Fossati, L.; Lyubchik, Y.; Mugrauer, M.; Bender, R.; Lee, C.- H.; Riffeser, A.; Afonso, P.; Greiner, J.; Henning, T.; Neuhauser, R.; Snellen, I. A. G.; Pavlenko, Y.; Verdugo, M.; Vogt, N. (2013), "A hot Jupiter transiting a mid-K dwarf found in the pre-OmegaCam Transit Survey",Monthly Notices of the Royal Astronomical Society,435 (4):3133–3147,arXiv:1308.6574,doi:10.1093/mnras/stt1512
  60. ^Michael C. Liu; Eugene A. Magnier; Niall R. Deacon; Katelyn N. Allers; et al. (1 October 2013). "The Extremely Red, Young L Dwarf PSO J318-22: A Free-Floating Planetary-Mass Analog to Directly Imaged Young Gas-Giant Planets".Astrophysical Journal Letters.777 (2).arXiv:1310.0457.Bibcode:2013ApJ...777L..20L.doi:10.1088/2041-8205/777/2/L20.S2CID 54007072.
  61. ^abKraus, Adam L.; Ireland, Michael J.; Cieza, Lucas A.; Hinkley, Sasha; Dupuy, Trent J.; Bowler, Brendan P.; Liu, Michael C. (2013), "THREE WIDE PLANETARY-MASS COMPANIONS TO FW TAU, ROXs 12, AND ROXs 42B",The Astrophysical Journal,781: 20,arXiv:1311.7664,Bibcode:2014ApJ...781...20K,doi:10.1088/0004-637X/781/1/20,S2CID 41086512
  62. ^Knutson, Heather A.; Fulton, Benjamin J.; Montet, Benjamin T.; Kao, Melodie; Ngo, Henry; Howard, Andrew W.; Crepp, Justin R.; Hinkley, Sasha; Bakos, Gaspar A.; Batygin, Konstantin; John Asher Johnson; Morton, Timothy D.; Muirhead, Philip S. (2013), "Friends of Hot Jupiters. I. A Radial Velocity Search for Massive, Long-Period Companions to Close-In Gas Giant Planets",The Astrophysical Journal,785 (2): 126,arXiv:1312.2954,doi:10.1088/0004-637X/785/2/126,S2CID 42687848
  63. ^abGómez Maqueo Chew, Y.; Faedi, F.; Pollacco, D.; Brown, D. J. A.; Doyle, A. P.; Collier Cameron, A.; Gillon, M.; Lendl, M.; Smalley, B.; Triaud, A. H. M. J.; West, R. G.; Wheatley, P. J.; Busuttil, R.; Liebig, C.; Anderson, D. R.; Armstrong, D. J.; Barros, S. C. C.; Bento, J.; Bochinski, J.; Burwitz, V.; Delrez, L.; Enoch, B.; Fumel, A.; Haswell, C. A.; Hébrard, G.; Hellier, C.; Holmes, S.; Jehin, E.; Kolb, U.; et al. (2013), "Discovery of WASP-65b and WASP-75b: Two Hot Jupiters Without Highly Inflated Radii",Astronomy & Astrophysics,559: A36,arXiv:1307.6532,Bibcode:2013A&A...559A..36G,doi:10.1051/0004-6361/201322314,S2CID 1008674
  64. ^abcDelrez, L.; Van Grootel, V.; Anderson, D. R.; Collier-Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M.; Neveu-VanMalle, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Udry, S.; West, R. G. (2013), "Transiting planets from WASP-South, Euler and TRAPPIST:WASP-68 b, WASP-73 b and WASP-88 b, three hot Jupiters transiting evolved solar-type stars",Astronomy and Astrophysics,563,arXiv:1312.1827,Bibcode:2014A&A...563A.143D,doi:10.1051/0004-6361/201323204,S2CID 54846964
  65. ^abcAnderson, D. R.; Collier Cameron, A.; Delrez, L.; Doyle, A. P.; Faedi, F.; Fumel, A.; Gillon, M.; Gómez Maqueo Chew, Y.; Hellier, C.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Skillen, I.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Turner, O. D.; Udry, S.; West, R. G. (2013),Three sub-Jupiter-mass planets: WASP-69b & WASP-84b transit active K dwarfs and WASP-70Ab transits the evolved primary of a G4+K3 binary,arXiv:1310.5654,doi:10.1093/mnras/stu1737
  66. ^Clark, B. J. M.; Anderson, D. R.; Hellier, C.; Turner, O. D.; Močnik, T. (2013), "An Analysis of Transiting Hot Jupiters Observed with K2: WASP-55b and WASP-75b",Publications of the Astronomical Society of the Pacific,130 (985): 034401,arXiv:1802.02132,doi:10.1088/1538-3873/aaa33e,S2CID 119077382
  67. ^abcWest, R. G.; Hellier, C.; Almenara, J.-M.; Anderson, D. R.; Barros, S. C. C.; Bouchy, F.; Brown, D. J. A.; Collier Cameron, A.; Deleuil, M.; Delrez, L.; Doyle, A. P.; Faedi, F.; Fumel, A.; Gillon, M.; Gómez Maqueo Chew, Y.; Hébrard, G.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Udry, S. (2016), "Three irradiated and bloated hot Jupiters",Astronomy & Astrophysics,585: A126,arXiv:1310.5607,Bibcode:2016A&A...585A.126W,doi:10.1051/0004-6361/201527276,S2CID 54746373
  68. ^Triaud, A. H. M. J.; Anderson, D. R.; Collier Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hellier, C.; Jehin, E.; Lendl, M.; Lovis, C.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Udry, S.; West, R. G.; Wheatley, P. J. (2013), "WASP-80b: a gas giant transiting a cool dwarf",Astronomy & Astrophysics,551: A80,arXiv:1303.0254,Bibcode:2013A&A...551A..80T,doi:10.1051/0004-6361/201220900,S2CID 67805044
  69. ^abcdefgHellier, Coel; Anderson, D. R.; Cameron, A. Collier; Delrez, L.; Gillon, M.; Jehin, E.; Lendl, M.; Maxted, P. F. L.; Pepe, F.; Pollacco, D.; Queloz, D.; Ségransan, D.; Smalley, B.; Smith, A. M. S.; Southworth, J.; Triaud, A. H. M. J.; Udry, S.; West, R. G. (2013), "Transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-95b to WASP-101b",Monthly Notices of the Royal Astronomical Society,440 (3):1982–1992,arXiv:1310.5630,doi:10.1093/mnras/stu410
  70. ^WTS-2 b: Too close for comfort?
  71. ^Birkby, J. L.; et al. (2014), "WTS-2 b: A hot Jupiter orbiting near its tidal destruction radius around a K dwarf",Monthly Notices of the Royal Astronomical Society,440 (2):1470–1489,arXiv:1402.5416,doi:10.1093/mnras/stu343
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