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List of exoplanets discovered in 2013

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This is a List of exoplanets discovered in 2013.

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)[1] Discovery method Distance (ly) Host star mass (M☉) Host star temp. (K) Remarks
2MASS J01225093-2439505 b 24.5 52 imaging 120 0.4 3530 [2]
BD+15 2940 b 1.11 137.48 0.539 radial vel. 572.2 1.1 4796 [3]
CoRoT-25b 0.27 1.08 4.86069 0.0578 transit 3300 1.09 6040 [4]
CoRoT-26b 0.52 1.26 4.20474 0.0526 transit 5400 1.09 5590 [4]
DENIS-P J082303.1-491201 b 28.5 246.36 0.36 astrometry 67.7 0.07 2150 [5]
Gliese 163 b 0.03335 8.63182 0.0607 radial vel. 48.8 0.4 3500 [6]
Gliese 163 c 0.0214 25.63058 0.1254 radial vel. 48.8 0.4 3500 [6]
Gliese 163 d 0.0925 603.95116 1.0304 radial vel. 48.8 0.4 3500 [6]
Gliese 221b 0.027 3.8728 0.0428 radial vel. 66 0.7 4324 [7][8] Disputed[9]
Gliese 221 c 0.17 125.94 0.435 radial vel. 66 0.7 4324 [7][8]
Gliese 328b 2.3 4100 4.5 radial vel. 65.3 0.69 3900 [10]
Gliese 504 b 4 43.5 imaging 58.5 1.22 6234 [11]
HAT-P-44b 0.352 1.242 4.301219 0.0507 transit 1180 0.94 5295 [12]
HAT-P-44c 4 872.2 1.752 radial vel. 1180 0.94 5295 Period is ambiguous[12]
HAT-P-45b 0.892 1.426 3.128992 0.0452 transit 990 1.26 6330 [12]
HAT-P-46b 0.493 1.284 4.463129 0.0577 transit 970 1.28 6120 [12]
HATS-2b 1.345 1.168 1.354133 0.023 transit 1200 0.88 5227 [13]
HATS-3b 1.071 1.381 3.547851 0.0485 1648 transit 1480 1.21 6351 [14]
HD 2952 b [ru] 1.6 311.6 1.2 radial vel. 375.8 2.54 4844 [15]
HD 13908 b [fr] 0.865 19.382 0.154 radial vel. 218.2 1.29 6255 [16]
HD 13908 c [fr] 5.13 931 2.03 radial vel. 218.2 1.29 6255 [16]
HD 65216c 0.17 152.6 0.54 radial vel. 116.1 0.92 5666 [17] False positive, another planet with same assigned name discovered in 2019.[18]
HD 95086 b 5 55.7 imaging 298.7 1.6 [19]
HD 103774 b 0.367 5.8881 0.07 radial vel. 173.1 1.33 6489 [7]
HD 106906 b 11 650 imaging 299.5 1.5 6516 [20]
HD 109271 b 0.054 7.8543 0.079 radial vel. 185.6 1.05 5783 [7]
HD 109271 c 0.076 30.93 0.196 radial vel. 185.6 1.05 5783 [7]
HD 113337 b 2.83 324 0.92 radial vel. 122.0 1.4 6576.6 [21]
HD 120084 b 4.5 2082 4.3 radial vel. 318.5 2.39 4892 [15]
HD 159243 b 1.13 12.62 0.11 radial vel. 223.7 1.12 6123 [16]
HD 159243 c [fr] 1.9 248.4 0.8 radial vel. 223.7 1.12 6123 [16]
HD 233604 b 6.575 192 0.747 radial vel. 2830±90 1.5 4791 [3]
HD 285507 b 0.92±0.03 6.0962±0.0002 radial vel. 153 0.73±0.03 4503+85
−61 		member of Hyades (star cluster)[22][23]
HD 112410 b 9.18 124.6 0.565 radial vel. 486.8 1.54 4830 [24]
HIP 91258 b [fr] 1.068 5.0505 0.057 radial vel. 145.0 0.95 5519 [16]
KELT-3b 1.477 1.345 2.7033904 0.04122 transit 580 1.28 6306 [25]
KELT-6b 0.442 1.18 7.8455821 0.08 transit 720 1.13 6272 [26]
Kepler-37b 0.03146 0.029 13.3675 transit 220 0.8 5417 [27]
Kepler-37c 0.03776 0.067 21.302 transit 220 0.8 5417 [27]
Kepler-37d 0.03839 0.173 39.7922 transit 220 0.8 5417 [27]
Kepler-61b 0.192 59.87756 transit 1103±16 0.64 4017 [28]
Kepler-62b 0.03 0.117 5.714932 0.0553 transit 1200 0.69 4925 [29]
Kepler-62c 0.013 0.048 12.4417 0.0929 transit 1200 0.69 4925 [29]
Kepler-62d 0.044 0.174 18.16406 0.12 transit 1200 0.69 4925 [29]
Kepler-62e 0.113 0.144 122.3874 0.427 transit 1200 0.69 4925 Potentially habitable exoplanet[29]
Kepler-62f 0.11 0.126 267.291 0.718 transit 1200 0.69 4925 Potentially habitable exoplanet[29]
Kepler-63b 0.378 0.545 9.4341505 0.08 transit 650 0.98 5576 [30]
Kepler-65b 0.127 2.15491 0.035 transit 999±8 1.25 6211 [31]
Kepler-65c 0.23 5.859944 0.068 transit 999±8 1.25 6211 [31]
Kepler-65d 0.136 8.13123 0.084 transit 999±8 1.25 6211 [31]
Kepler-66b 0.25 17.815815 0.1352 transit 3610 1.04 5962 Belongs to open cluster NGC 6811[32]
Kepler-67b 0.262 15.7259 0.1171 transit 3610 0.86 5331 Belongs to open cluster NGC 6811[32]
Kepler-68b 0.01878 0.208 5.39875 1280 transit 440 1.08 5793 [33]
Kepler-68c 0.02265 0.089 9.60504 transit 440 1.08 5793 [33]
Kepler-68d 0.84007 625 radial vel. 440 1.08 5793 [33]
Kepler-69b 0.2 13.722341 0.094 transit 2430±30 0.81 5638 [34]
Kepler-69c 0.153 242.4613 0.64 transit 2430±30 0.81 5638 [34][35]
Kepler-74b [es] 0.63 0.96 7.340711 0.0781 transit 4300 1.18 6000 [36]
Kepler-75b [es] 10.1 1.05 8.8849116 0.0818 transit 3700 0.91 5200 [36]
Kepler-76b 2.01 1.36 1.5449298 0.0274 orbital brightness modulation 2750±30 1.2 6409 [37]
Kepler-77b [es] 0.43 0.96 3.57878087 0.04501 transit 1900 0.95 5520 [38]
Kepler-78b 0.006 0.105 0.355 2330 transit 407.1±1.1 0.76 5058 [39]
Kepler-87b 1.02 1.204 114.73635 0.481 478 transit 4170±90 1.1 5600 Two more unconfirmed planets in the system[39]
Kepler-87c 0.02 0.548 191.2318 0.676 403 transit 4170±90 1.1 5600 Two more unconfirmed planets in the system[39]
Kepler-88b 0.027 0.337 10.95416 transit 1110 0.96 5471 [40]
Kepler-88c 0.626 22.3395 0.15525 timing 1110 0.96 5471 [40][41]
Kepler-89b 0.033 0.153 3.743208 0.05119 transit 1577±16 1.28 6182 [42]
Kepler-89c 0.049 0.385 10.423648 0.1013 transit 1577±16 1.28 6182 [42]
Kepler-89d 0.334 1.005 22.342989 0.1684 transit 1577±16 1.28 6182 [42]
Kepler-89e 0.11 0.585 54.32031 0.3046 transit 1577±16 1.28 6182 [42]
Kepler-90b 0.117 7.008151 0.074 1056 transit 2500 1.2 6080 [43]
Kepler-90c 0.106 8.719375 0.089 981 transit 2500 1.2 6080 [43]
Kepler-90d 0.256 59.73667 0.32 518 transit 2500 1.2 6080 [43]
Kepler-90e 0.237 91.93913 0.42 448 transit 2500 1.2 6080 [43]
Kepler-90f 0.257 124.9144 0.48 592 transit 2500 1.2 6080 [43]
Kepler-90g 0.723 210.60697 0.71 340 transit 2500 1.2 6080 [43]
Kepler-90h 1.008 331.60059 1.01 292 transit 2500 1.2 6080 [43]
Kepler-91b 0.81 1.367 6.24658 0.0731 transit 3400 1.31 4550 [44]
Kepler-92b 0.202 0.313 13.749 transit 1580±17 1.21 5883 [45]
Kepler-92c 0.019 0.232 26.723 transit 1580±17 1.21 5883 [45]
Kepler-102e 0.028 0.198 16.1457 579 transit 352.7±0.7 0.81 4909 [46]
Kepler-105b 0.429 5.4122 0.066 transit 1517±18 0.96 5827 [46]
Kepler-114c 0.009 0.143 8.041 623 transit 852±4 0.56 4605 [45]
Kepler-114d 0.012 0.226 11.776 549 transit 852±4 0.56 4605 [45]
Kepler-128b 0.097 0.101 15.09 transit 1307±12 1.18 6090 [45]
Kepler-128c 0.105 0.101 22.804 transit 1307±12 1.18 6090 [45]
Kepler-130b 0.091 8.457458 0.079 transit 1042±7 1 5884 [46]
Kepler-145b 0.117 0.236 22.951 transit 1880±30 1.32 6022 [45]
Kepler-145c 0.25 0.385 42.882 transit 1880±30 1.32 6022 [45]
Kepler-177b 0.006 0.259 36.855 transit 4880±140 1.07 5942 [45]
Kepler-177c 0.024 0.633 49.412 transit 4880±140 1.07 5942 [45]
Kepler-238e 0.534 0.5 23.654 transit 6200±300 1.06 5751 [45]
Kepler-238f 0.042 0.178 50.447 transit 6200±300 1.06 5751 [45]
Kepler-276c 0.052 0.259 31.884 transit 3850±150 1.1 6105 [45]
Kepler-276d 0.051 0.25 48.648 transit 3850±150 1.1 6105 [45]
Kepler-277b 0.275 0.261 17.324 transit 3280±50 1.12 5946 [45]
Kepler-277c 0.202 0.3 33.006 transit 3280±50 1.12 5946 [45]
Kepler-279b 0.323 12.309681 0.112 transit 3480±70 1.1 6363 KOI-1236.01[47]
Kepler-279c 0.155 0.384 35.736 transit 3490±70 1.1 6363 KOI-1236.02[47][45]
Kepler-279d 0.118 0.277 54.414 transit 3490±70 1.1 6363 [45]
Kepler-282d 0.192 0.219 24.806 transit 4540±150 0.97 5602 [45]
Kepler-282e 0.177 0.277 44.347 transit 4540±150 0.97 5602 [45]
Kepler-305b 0.033 0.321 5.487 transit 2900±90 0.76 5100 [45] KOI-1563.01[47]
Kepler-305c 0.019 0.294 8.291 transit 2900±90 0.76 5100 [45] KOI-1563.02[47]
Kepler-307b 0.02341 0.217 10.4208 transit 1908±17 0.91 5367 [45]
Kepler-307c 0.01145 0.196 13.0729 transit 1908±17 0.91 5367 [45]
Kepler-328b 0.09 0.205 34.921 transit 7700±500 1.15 5914 [45]
Kepler-328c 0.124 0.482 71.312 transit 7700±500 1.15 5914 [45]
Kepler-350c 0.019 0.277 17.849 transit 3210±70 1 6186 [45]
Kepler-350d 0.047 0.25 26.136 transit 3210±70 1 6186 [45]
Kepler-396b 0.238 0.312 42.994 transit 734±5 0.85 5384 [45] KOI-2672.01[47]
Kepler-396c 0.056 0.473 88.505 transit 734±5 0.85 5384 [45] KOI-2672.02[47]
Kepler-410Ab 0.253 17.833648 0.1226 transit 430 1.21 6273 [48]
Kepler-411b 0.168 3.00516 0.038 1040 transit 503.5±1.5 0.83 4974 [46]
Kepler-1359c 0.3711+0.12
−0.06 		505.46+0.05
−0.04 		1.143±0.018 transit 2182+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-379Lb 4.1 3.3 microlensing 11000 0.56 [50]
MOA-2010-BLG-328Lb 0.02895 0.92 microlensing 2600 0.11 [51]
MOA-2011-BLG-262Lb 0.056634 0.383 1 microlensing 22830 0.1 3300 Host star may be a rogue planet, planet may be an exomoon[52]
MOA-2011-BLG-262L 4 N/A microlensing 22830 3300 Host star may be a rogue planet, planet may be an exomoon[52]
MOA-2011-BLG-293Lb 4.8 1.1 microlensing 25200 0.86 [53]
MOA-2011-BLG-322Lb 11.6 4.3 microlensing 24700 0.39 [54]
OGLE-2011-BLG-0251Lb 0.53 2.72 microlensing 8400 0.26 [55]
OGLE-2012-BLG-358Lb 1.85 0.87 microlensing 5700 0.02 Orbiting a brown dwarf[56]
OGLE-2012-BLG-406Lb 2.73 3.45 microlensing 16200 0.44 [57]
Omega Serpentis b 1.7 277.02 1.1 radial vel. 263.0 2.17 4770 [15]
PH2b 0.903 282.5255 0.828 281 transit 1130±10 0.94 5629 [58] Also called Kepler-86b
POTS-1b 2.31 0.941 3.1606296 0.03734 transit 3900 0.69 4400 [59]
PSO J318.5−22 6.5 1.53 N/A N/A 1160 imaging 80 N/A N/A Rogue planet[60]
ROXs 12b 16 210 imaging 390 0.87 3850 [61]
ROXs 42Bb 9 157 imaging 440 1 [61]
WASP-8c 9.45 4323 5.28 radial vel. 280 1.03 5600 [62]
WASP-65b 1.55 1.112 2.3114243 0.0334 transit 1000 0.93 5600 [63]
WASP-68b 0.95 1.24 5.084298 0.06206 transit 962±8 1.24 5911 [64]
WASP-69b 0.26 1.057 3.8681382 0.04525 963 transit 160 0.83 4715 [65]
WASP-70Ab 0.59 1.164 3.7130203 0.04853 1387 transit 800 1.11 5763 [65]
WASP-73b 1.88 1.16 4.08722 0.05512 1790 transit 1042±9 1.34 6036 [64]
WASP-75b 1.07 1.27 2.484193 0.0375 transit 850 1.14 6100 [63][66]
WASP-76b 0.92 1.83 1.809886 0.033 2190 transit 390 1.46 6250 [67]
WASP-80b 0.538 0.999 3.06785234 0.0344 transit 200 0.58 4143 [68] Proper name Wadirum
WASP-82b [fr] 1.24 1.67 2.705782 0.0447 2190 transit 650 1.63 6490 [67]
WASP-84b 0.694 0.942 8.5234865 0.0771 797 transit 410 0.84 5314 [65]
WASP-88b 0.56 1.7 4.954 0.06431 1775 transit 1730±30 1.45 6431 [64]
WASP-90b 0.63±0.07 1.63±0.09 3.916243±0.000003 0.0562±0.0012 1840±50 transit 1100±200 1.55±0.10 6440±130 [67]
WASP-95b 1.13+0.1
−0.04 		1.21±0.06 2.184673±0.0000014 0.03416±0.00083 1570±50 transit 450±2 1.11±0.09 5630±130 [69]
WASP-96b 0.48±0.03 1.2±0.06 3.4252602±0.0000027 0.0453±0.0013 1285±40 transit 1161±15 1.06±0.09 5540±140 [69]
WASP-97b 1.32±0.05 1.13±0.06 2.07276±0.000001 0.03303±0.00056 1555±40 transit 494.9±1.7 1.12±0.06 5640±100 [69]
WASP-98b 0.83±0.07 1.10±0.04 2.96264036±0.0000013 0.03762±0.001 1180±30 transit 926±5 0.69±0.06 5525±130 [69]
WASP-99b 2.78±0.13 1.10+0.08
−0.05 		5.75251±0.00004 0.0717±0.0016 1480±40 transit 519±2 1.48±0.10 6180±100 [69]
WASP-100b 2.03±0.12 1.69±0.29 2.849375±0.000008 0.0457±0.0010 2190±140 transit 1201±9 1.57±0.10 6900±120 [69]
WASP-101b 0.50±0.04 1.41±0.05 3.585722±0.000004 0.0506±0.0009 1560±35 transit 660±3 1.34±0.07 6400±110 [69]
WTS-2b 1.12 1.363 1.0187068 0.01855 2000 transit 3300 0.82 5000 [70][71]

Specific exoplanet lists

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Lists of exoplanets

Lists of exoplanets by year of discovery

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References

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  1. ^ "The Extrasolar Planets Encyclopaedia". 1995. Retrieved 2015-11-09.
  2. ^ PLANETS AROUND LOW-MASS STARS. III. A YOUNG DUSTY L DWARF COMPANION AT THE DEUTERIUM-BURNING LIMIT
  3. ^ a b BD+15 2940 AND HD 233604: TWO GIANTS WITH PLANETS CLOSE TO THE ENGULFMENT ZONE
  4. ^ a b Transiting exoplanets from the CoRoT space mission XXIV. CoRoT-25b and CoRoT-26b: two low-density giant planets
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  23. ^ Open exoplanet catalogue HD 285507
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  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.
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  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 Shporer et al. April 26, 2013
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  32. ^ a b The same frequency of planets inside and outside open clusters of stars
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  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. ^ a b Hébrard, 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 with Kepler, 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. ^ a b c Ofir, Aviv; Dreizler, Stefan; Zechmeister, Mathias; Husser, Tim-Oliver (2013), "An independent planet search in the Keplerdataset", Astronomy & Astrophysics, 561: A103, arXiv:1310.2064, doi:10.1051/0004-6361/201220935, S2CID 118691606
  40. ^ a b Nesvorný, 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 of Keplertransit candidates", Astronomy & Astrophysics, 561: L1, arXiv:1311.4335, doi:10.1051/0004-6361/201323067, S2CID 118446884
  42. ^ a b c d Masuda, 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. ^ a b c d e f g h Schmitt, 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. ^ 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 ab ac ad Xie, 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. ^ a b c d Wang, 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. ^ a b c d e f Yang, 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. ^ a b MOA-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-Omega Cam 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. ^ a b Kraus, 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. ^ a b Gómez 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. ^ a b c Delrez, 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. ^ a b c Anderson, 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. ^ a b c West, 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. ^ a b c d e f g Hellier, 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?
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