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List of exoplanets discovered in 2013

Topic: Astronomy

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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[40]
Kepler-87c 0.02 0.548 191.2318 0.676 403 transit 4170±90 1.1 5600 Two more unconfirmed planets in the system[40]
Kepler-88b 0.027 0.337 10.95416 transit 1110 0.96 5471 [41]
Kepler-88c 0.626 22.3395 0.15525 timing 1110 0.96 5471 [41][42]
Kepler-89b 0.033 0.153 3.743208 0.05119 transit 1577±16 1.28 6182 [43]
Kepler-89c 0.049 0.385 10.423648 0.1013 transit 1577±16 1.28 6182 [43]
Kepler-89d 0.334 1.005 22.342989 0.1684 transit 1577±16 1.28 6182 [43]
Kepler-89e 0.11 0.585 54.32031 0.3046 transit 1577±16 1.28 6182 [43]
Kepler-90b 0.117 7.008151 0.074 1056 transit 2500 1.2 6080 [44]
Kepler-90c 0.106 8.719375 0.089 981 transit 2500 1.2 6080 [44]
Kepler-90d 0.256 59.73667 0.32 518 transit 2500 1.2 6080 [44]
Kepler-90e 0.237 91.93913 0.42 448 transit 2500 1.2 6080 [44]
Kepler-90f 0.257 124.9144 0.48 592 transit 2500 1.2 6080 [44]
Kepler-90g 0.723 210.60697 0.71 340 transit 2500 1.2 6080 [44]
Kepler-90h 1.008 331.60059 1.01 292 transit 2500 1.2 6080 [44]
Kepler-91b 0.81 1.367 6.24658 0.0731 transit 3400 1.31 4550 [45]
Kepler-92b 0.202 0.313 13.749 transit 1580±17 1.21 5883 [46]
Kepler-92c 0.019 0.232 26.723 transit 1580±17 1.21 5883 [46]
Kepler-102e 0.028 0.198 16.1457 579 transit 352.7±0.7 0.81 4909 [47]
Kepler-105b 0.429 5.4122 0.066 transit 1517±18 0.96 5827 [47]
Kepler-114c 0.009 0.143 8.041 623 transit 852±4 0.56 4605 [46]
Kepler-114d 0.012 0.226 11.776 549 transit 852±4 0.56 4605 [46]
Kepler-128b 0.097 0.101 15.09 transit 1307±12 1.18 6090 [46]
Kepler-128c 0.105 0.101 22.804 transit 1307±12 1.18 6090 [46]
Kepler-130b 0.091 8.457458 0.079 transit 1042±7 1 5884 [47]
Kepler-145b 0.117 0.236 22.951 transit 1880±30 1.32 6022 [46]
Kepler-145c 0.25 0.385 42.882 transit 1880±30 1.32 6022 [46]
Kepler-177b 0.006 0.259 36.855 transit 4880±140 1.07 5942 [46]
Kepler-177c 0.024 0.633 49.412 transit 4880±140 1.07 5942 [46]
Kepler-238e 0.534 0.5 23.654 transit 6200±300 1.06 5751 [46]
Kepler-238f 0.042 0.178 50.447 transit 6200±300 1.06 5751 [46]
Kepler-276c 0.052 0.259 31.884 transit 3850±150 1.1 6105 [46]
Kepler-276d 0.051 0.25 48.648 transit 3850±150 1.1 6105 [46]
Kepler-277b 0.275 0.261 17.324 transit 3280±50 1.12 5946 [46]
Kepler-277c 0.202 0.3 33.006 transit 3280±50 1.12 5946 [46]
Kepler-279b 0.323 12.309681 0.112 transit 3480±70 1.1 6363 KOI-1236.01[48]
Kepler-279c 0.155 0.384 35.736 transit 3490±70 1.1 6363 KOI-1236.02[48][46]
Kepler-279d 0.118 0.277 54.414 transit 3490±70 1.1 6363 [46]
Kepler-282d 0.192 0.219 24.806 transit 4540±150 0.97 5602 [46]
Kepler-282e 0.177 0.277 44.347 transit 4540±150 0.97 5602 [46]
Kepler-305b 0.033 0.321 5.487 transit 2900±90 0.76 5100 [46]KOI-1563.01[48]
Kepler-305c 0.019 0.294 8.291 transit 2900±90 0.76 5100 [46]KOI-1563.02[48]
Kepler-307b 0.02341 0.217 10.4208 transit 1908±17 0.91 5367 [46]
Kepler-307c 0.01145 0.196 13.0729 transit 1908±17 0.91 5367 [46]
Kepler-328b 0.09 0.205 34.921 transit 7700±500 1.15 5914 [46]
Kepler-328c 0.124 0.482 71.312 transit 7700±500 1.15 5914 [46]
Kepler-350c 0.019 0.277 17.849 transit 3210±70 1 6186 [46]
Kepler-350d 0.047 0.25 26.136 transit 3210±70 1 6186 [46]
Kepler-396b 0.238 0.312 42.994 transit 734±5 0.85 5384 [46]KOI-2672.01[48]
Kepler-396c 0.056 0.473 88.505 transit 734±5 0.85 5384 [46]KOI-2672.02[48]
Kepler-410Ab 0.253 17.833648 0.1226 transit 430 1.21 6273 [49]
Kepler-411b 0.168 3.00516 0.038 1040 transit 503.5±1.5 0.83 4974 [47]
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 [44]Also called KIC 6436029 c, discovery retracted in 2015 after 3rd transit was proven to be false.[50]
MOA-2008-BLG-379Lb 4.1 3.3 microlensing 11000 0.56 [51]
MOA-2010-BLG-328Lb 0.02895 0.92 microlensing 2600 0.11 [52]
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[53]
MOA-2011-BLG-262L 4 N/A microlensing 22830 3300 Host star may be a rogue planet, planet may be an exomoon[53]
MOA-2011-BLG-293Lb 4.8 1.1 microlensing 25200 0.86 [54]
MOA-2011-BLG-322Lb 11.6 4.3 microlensing 24700 0.39 [55]
OGLE-2011-BLG-0251Lb 0.53 2.72 microlensing 8400 0.26 [56]
OGLE-2012-BLG-358Lb 1.85 0.87 microlensing 5700 0.02 Orbiting a brown dwarf[57]
OGLE-2012-BLG-406Lb 2.73 3.45 microlensing 16200 0.44 [58]
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 [59]Also called Kepler-86b
POTS-1b 2.31 0.941 3.1606296 0.03734 transit 3900 0.69 4400 [60]
PSO J318.5−22 6.5 1.53 N/A N/A 1160 imaging 80 N/A N/A Rogue planet[61]
ROXs 12b 16 210 imaging 390 0.87 3850 [62]
ROXs 42Bb 9 157 imaging 440 1 [62]
WASP-8c 9.45 4323 5.28 radial vel. 280 1.03 5600 [63]
WASP-65b 1.55 1.112 2.3114243 0.0334 transit 1000 0.93 5600 [64]
WASP-68b 0.95 1.24 5.084298 0.06206 transit 962±8 1.24 5911 [65]
WASP-69b 0.26 1.057 3.8681382 0.04525 963 transit 160 0.83 4715 [66]
WASP-70Ab 0.59 1.164 3.7130203 0.04853 1387 transit 800 1.11 5763 [66]
WASP-73b 1.88 1.16 4.08722 0.05512 1790 transit 1042±9 1.34 6036 [65]
WASP-75b 1.07 1.27 2.484193 0.0375 transit 850 1.14 6100 [64][67]
WASP-76b 0.92 1.83 1.809886 0.033 2190 transit 390 1.46 6250 [68]
WASP-80b 0.538 0.999 3.06785234 0.0344 transit 200 0.58 4143 [69]Proper name Wadirum
WASP-82#Planetary system (fr) 1.24 1.67 2.705782 0.0447 2190 transit 650 1.63 6490 [68]
WASP-84b 0.694 0.942 8.5234865 0.0771 797 transit 410 0.84 5314 [66]
WASP-88b 0.56 1.7 4.954 0.06431 1775 transit 1730±30 1.45 6431 [65]
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 [68]
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 [70]
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 [70]
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 [70]
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 [70]
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 [70]
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 [70]
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 [70]
WTS-2b 1.12 1.363 1.0187068 0.01855 2000 transit 3300 0.82 5000 [71][72]

Specific exoplanet lists

References

  1. ↑ "The Extrasolar Planets Encyclopaedia". Extrasolar Planets Encyclopaedia. https://exoplanet.eu/catalog/. 
  2. ↑ PLANETS AROUND LOW-MASS STARS. III. A YOUNG DUSTY L DWARF COMPANION AT THE DEUTERIUM-BURNING LIMIT
  3. ↑ 3.0 3.1 BD+15 2940 AND HD 233604: TWO GIANTS WITH PLANETS CLOSE TO THE ENGULFMENT ZONE
  4. ↑ 4.0 4.1 Transiting 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, doi:10.1051/0004-6361/201321871, Bibcode: 2013A&A...556A.133S 
  6. ↑ 6.0 6.1 6.2 Tuomi, M.; Anglada-Escudé, G. (2013). "Up to four planets around the M dwarf GJ 163". Astronomy & Astrophysics 556: A111. doi:10.1051/0004-6361/201321174. 
  7. ↑ 7.0 7.1 7.2 7.3 7.4 Lo Curto, G.; Mayor, M.; Benz, W.; Bouchy, F.; Hébrard, G.; Lovis, C.; Moutou, C.; Naef, D. et al. (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. doi:10.1051/0004-6361/201220415. A59. Bibcode: 2013A&A...551A..59L. 
  8. ↑ 8.0 8.1 Arriagada, 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, doi:10.1088/0004-637X/771/1/42, Bibcode: 2013ApJ...771...42A 
  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, doi:10.3847/1538-3881/ac5d41, Bibcode: 2022AJ....163..215S 
  10. ↑ Robertson, Paul; Endl, Michael; Cochran, William D.; MacQueen, Phillip J.; Boss, Alan P. (2013), "Secretly Eccentric: The Giant Planet and Activity Cycle of GJ 328", The Astrophysical Journal 774 (2): 147, doi:10.1088/0004-637X/774/2/147, Bibcode: 2013ApJ...774..147R 
  11. ↑ Kuzuhara, M.; Tamura, M.; Kudo, T.; Janson, M.; Kandori, R.; Brandt, T. D.; Thalmann, C.; Spiegel, D. et al. (2013). "Direct Imaging of a Cold Jovian Exoplanet in Orbit around the Sun-like Star GJ 504". The Astrophysical Journal 774 (11): 11. doi:10.1088/0004-637X/774/1/11. Bibcode: 2013ApJ...774...11K. 
  12. ↑ 12.0 12.1 12.2 12.3 Hartman, J. D.; Bakos, G. Á.; Torres, G.; Kovács, G.; Johnson, J. A.; Howard, A. W.; Marcy, G. W.; Latham, D. W. et al. (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, doi:10.1088/0004-6256/147/6/128 
  13. ↑ Mohler-Fischer, M.; Mancini, L.; Hartman, J. D.; Bakos, G. Á.; Penev, K.; Bayliss, D.; Jordán, A.; Csubry, Z. et al. (2013), "HATS-2b: A transiting extrasolar planet orbiting a K-type star showing starspot activity", Astronomy & Astrophysics 558: A55, doi:10.1051/0004-6361/201321663, Bibcode: 2013A&A...558A..55M 
  14. ↑ Bayliss, D.; Zhou, G.; Penev, K.; Bakos, G. Á.; Hartman, J. D.; Jordán, A.; Mancini, L.; Mohler-Fischer, M. et al. (2013), "HATS-3b: An inflated hot Jupiter transiting an F-type star", The Astronomical Journal 146 (5): 113, doi:10.1088/0004-6256/146/5/113, Bibcode: 2013AJ....146..113B 
  15. ↑ 15.0 15.1 15.2 Sato, Bun'ei; Omiya, Masashi; Harakawa, Hiroki; Liu, Yu-Juan; Izumiura, Hideyuki; Kambe, Eiji; Takeda, Yoichi; Yoshida, Michitoshi et al. (2013), "Planetary Companions to Three Evolved Intermediate-Mass Stars: HD 2952, HD 120084, andωSerpentis", Publications of the Astronomical Society of Japan 65 (4): 85, doi:10.1093/pasj/65.4.85 
  16. ↑ 16.0 16.1 16.2 16.3 16.4 Moutou, Claire; Hébrard, Guillaume; Bouchy, François; Arnold, Luc; Santos, Nuno C.; Astudillo-Defru, Nicola; Boisse, Isabelle; Bonfils, Xavier et al. (2013), The SOPHIE search for northern extrasolar planets VI. Three new hot Jupiters in multi-planet extrasolar systems, doi:10.1051/0004-6361/201322067 
  17. ↑ Wittenmyer, Robert A.; Wang, Songhu; Horner, Jonathan; Tinney, C. G.; Butler, R. P.; Jones, H. R. A.; O'Toole, S. J.; Bailey, J. et al. (2013), "Forever Alone? Testing Single Eccentric Planetary Systems for Multiple Companions", The Astrophysical Journal Supplement Series 208 (1): 2, doi:10.1088/0067-0049/208/1/2, Bibcode: 2013ApJS..208....2W 
  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. doi:10.1093/mnras/stz290. Bibcode: 2019MNRAS.484.5859W. 
  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. doi:10.1088/2041-8205/779/2/L26. Bibcode: 2013ApJ...779L..26R. 
  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. doi:10.1088/2041-8205/780/1/L4. Bibcode: 2014ApJ...780L...4B. 
  21. ↑ Borgniet, Simon; Boisse, Isabelle; Lagrange, Anne-Marie; Bouchy, François; Arnold, Luc; Díaz, Rodrigo F.; Galland, Franck; Delorme, Philippe et al. (2013), "Extrasolar planets and brown dwarfs around A--F type stars. VIII. A giant planet orbiting the young star HD113337", Astronomy & Astrophysics 561: A65, doi:10.1051/0004-6361/201321783 
  22. ↑ Carleo, I. (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. doi:10.1051/0004-6361/201937369. Bibcode: 2020A&A...638A...5C. 
  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. doi:10.1051/0004-6361/201321660. Bibcode: 2013A&A...556A..78J. 
  25. ↑ Pepper, Joshua; Siverd, Robert J.; Beatty, Thomas G.; Gaudi, B. Scott; Stassun, Keivan G.; Eastman, Jason; Collins, Karen; Latham, David W. et al. (2013-08-01). "KELT-3b: A Hot Jupiter Transiting a V = 9.8 Late-F Star". The Astrophysical Journal 773 (1): 64. doi:10.1088/0004-637X/773/1/64. ISSN 0004-637X. Bibcode: 2013ApJ...773...64P. http://adsabs.harvard.edu/abs/2013ApJ...773...64P. 
  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, doi:10.1088/0004-6256/147/2/39 
  27. ↑ 27.0 27.1 27.2 Barclay, Thomas et al. (2013), "A sub-Mercury-sized exoplanet", Nature 494 (7438): 452–454, doi:10.1038/nature11914, PMID 23426260, Bibcode: 2013Natur.494..452B 
  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
  29. ↑ 29.0 29.1 29.2 29.3 29.4 Borucki, 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, doi:10.1126/science.1234702, PMID 23599262, Bibcode: 2013Sci...340..587B 
  30. ↑ Sanchis-Ojeda, Roberto; Winn, Joshua N.; Marcy, Geoffrey W.; Howard, Andrew W.; Isaacson, Howard; Johnson, John Asher; Torres, Guillermo; Albrecht, Simon et al. (2013), "KEPLER-63b: A GIANT PLANET IN a POLAR ORBIT AROUND a YOUNG SUN-LIKE STAR", The Astrophysical Journal 775 (1): 54, doi:10.1088/0004-637X/775/1/54, Bibcode: 2013ApJ...775...54S 
  31. ↑ 31.0 31.1 31.2 Chaplin, W. J.; Sanchis-Ojeda, R.; Campante, T. L.; Handberg, R.; Stello, D.; Winn, J. N.; Basu, S.; Christensen-Dalsgaard, J. et al. (2013), "Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65", The Astrophysical Journal 766 (2): 101, doi:10.1088/0004-637X/766/2/101, Bibcode: 2013ApJ...766..101C 
  32. ↑ 32.0 32.1 The same frequency of planets inside and outside open clusters of stars
  33. ↑ 33.0 33.1 33.2 Gilliland, 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. doi:10.1088/0004-637X/766/1/40. Bibcode: 2013ApJ...766...40G. 
  34. ↑ 34.0 34.1 Barclay, 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, doi:10.1088/0004-637X/768/2/101, Bibcode: 2013ApJ...768..101B 
  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, doi:10.1088/2041-8205/770/2/L20, Bibcode: 2013ApJ...770L..20K 
  36. ↑ 36.0 36.1 Hébrard, G.; Almenara, J.-M.; Santerne, A.; Deleuil, M.; Damiani, C.; Bonomo, A. S.; Bouchy, F.; Bruno, G. et al. (2013), "KOI-200 b and KOI-889 b: Two transiting exoplanets detected and characterized with Kepler, SOPHIE, and HARPS-N", Astronomy & Astrophysics 554: A114, doi:10.1051/0004-6361/201321394, Bibcode: 2013A&A...554A.114H 
  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. doi:10.1088/0004-637X/771/1/26. Bibcode: 2013ApJ...771...26F. 
  38. ↑ Gandolfi, D.; Parviainen, H.; Fridlund, M.; Hatzes, A. P.; Deeg, H. J.; Frasca, A.; Lanza, A. F.; Prada Moroni, P. G. et al. (2013), "Kepler-77b: A very low albedo, Saturn-mass transiting planet around a metal-rich solar-like star", Astronomy & Astrophysics 557: A74, doi:10.1051/0004-6361/201321901, Bibcode: 2013A&A...557A..74G 
  39. ↑ Ofir, Aviv; Dreizler, Stefan; Zechmeister, Mathias; Husser, Tim-Oliver (2013), "An independent planet search in the Keplerdataset", Astronomy & Astrophysics 561: A103, doi:10.1051/0004-6361/201220935 
  40. ↑ 40.0 40.1 Ofir, Aviv; Dreizler, Stefan; Zechmeister, Mathias; Husser, Tim-Oliver (2013), "An independent planet search in the Keplerdataset", Astronomy & Astrophysics 561: A103, doi:10.1051/0004-6361/201220935 
  41. ↑ 41.0 41.1 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, doi:10.1088/0004-637X/777/1/3, Bibcode: 2013ApJ...777....3N 
  42. ↑ Barros, S. C. C.; Díaz, R. F.; Santerne, A.; Bruno, G.; Deleuil, M.; Almenara, J.-M.; Bonomo, A. S.; Bouchy, F. et al. (2013), "SOPHIE velocimetry of Keplertransit candidates", Astronomy & Astrophysics 561: L1, doi:10.1051/0004-6361/201323067 
  43. ↑ 43.0 43.1 43.2 43.3 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. doi:10.1088/0004-637X/778/2/185. Bibcode: 2013ApJ...778..185M. 
  44. ↑ 44.0 44.1 44.2 44.3 44.4 44.5 44.6 44.7 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, doi:10.1088/0004-6256/148/2/28 
  45. ↑ Lillo-Box, J.; Barrado, D.; Moya, A.; Montesinos, B.; Montalbán, J.; Bayo, A.; Barbieri, M.; Régulo, C. et al. (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. doi:10.1051/0004-6361/201322001. Bibcode: 2014A&A...562A.109L. 
  46. ↑ 46.00 46.01 46.02 46.03 46.04 46.05 46.06 46.07 46.08 46.09 46.10 46.11 46.12 46.13 46.14 46.15 46.16 46.17 46.18 46.19 46.20 46.21 46.22 46.23 46.24 46.25 46.26 46.27 46.28 46.29 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, doi:10.1088/0067-0049/210/2/25 
  47. ↑ 47.0 47.1 47.2 47.3 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: 4, doi:10.1088/0004-637X/783/1/4, Bibcode: 2014ApJ...783....4W 
  48. ↑ 48.0 48.1 48.2 48.3 48.4 48.5 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, doi:10.1088/0004-637X/778/2/110, Bibcode: 2013ApJ...778..110Y 
  49. ↑ Van Eylen, V.; Lund, M. N.; Aguirre, V. Silva; Arentoft, T.; Kjeldsen, H.; Albrecht, S.; Chaplin, W. J.; Isaacson, H. et al. (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: 14, doi:10.1088/0004-637X/782/1/14, Bibcode: 2014ApJ...782...14V 
  50. ↑ 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, doi:10.1088/0004-637X/815/2/127, Bibcode: 2015ApJ...815..127W 
  51. ↑ 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, doi:10.1088/0004-637X/780/2/123 
  52. ↑ Furusawa, K. et al. (2013), "MOA-2010-BLG-328Lb: A SUB-NEPTUNE ORBITING VERY LATE M DWARF?", The Astrophysical Journal 779 (2): 91, doi:10.1088/0004-637X/779/2/91, Bibcode: 2013ApJ...779...91F 
  53. ↑ 53.0 53.1 MOA-2011-BLG-262Lb: A SUB-EARTH-MASS MOON ORBITING A GAS GIANT PRIMARY OR A HIGH VELOCITY PLANETARY SYSTEM IN THE GALACTIC BULGE
  54. ↑ Batista, V.; Beaulieu, J. -P.; Gould, A.; Bennett, D. P.; Yee, J. C.; Fukui, A.; Gaudi, B. S.; Sumi, T. et al. (2013), "MOA-2011-BLG-293Lb: First Microlensing Planet possibly in the Habitable Zone", The Astrophysical Journal 780: 54, doi:10.1088/0004-637X/780/1/54 
  55. ↑ 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, doi:10.1093/mnras/stt2477 
  56. ↑ Kains, N.; Street, R. A.; Choi, J.-Y.; Han, C.; Udalski, A.; Almeida, L. A.; Jablonski, F.; Tristram, P. J. et al. (2013), "A Giant Planet beyond the Snow Line in Microlensing Event OGLE-2011-BLG-0251", Astronomy & Astrophysics 552: A70, doi:10.1051/0004-6361/201220626, Bibcode: 2013A&A...552A..70K 
  57. ↑ 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, doi:10.1088/0004-637X/778/1/38, Bibcode: 2013ApJ...778...38H 
  58. ↑ Poleski, Radosław; Udalski, Andrzej; Dong, Subo; Szymański, Michał K.; Soszyński, Igor; Kubiak, Marcin; Pietrzyński, Grzegorz; Kozłowski, Szymon et al. (2014), "SUPER-MASSIVE PLANETS AROUND LATE-TYPE STARS—THE CASE OF OGLE-2012-BLG-0406Lb", The Astrophysical Journal 782 (1): 47, doi:10.1088/0004-637X/782/1/47, Bibcode: 2014ApJ...782...47P 
  59. ↑ 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].
  60. ↑ Koppenhoefer, J.; Saglia, R. P.; Fossati, L.; Lyubchik, Y.; Mugrauer, M.; Bender, R.; Lee, C.- H.; Riffeser, A. et al. (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, doi:10.1093/mnras/stt1512 
  61. ↑ 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). doi:10.1088/2041-8205/777/2/L20. Bibcode: 2013ApJ...777L..20L. 
  62. ↑ 62.0 62.1 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, doi:10.1088/0004-637X/781/1/20 
  63. ↑ Knutson, Heather A.; Fulton, Benjamin J.; Montet, Benjamin T.; Kao, Melodie; Ngo, Henry; Howard, Andrew W.; Crepp, Justin R.; Hinkley, Sasha et al. (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, doi:10.1088/0004-637X/785/2/126 
  64. ↑ 64.0 64.1 Gómez Maqueo Chew, Y.; Faedi, F.; Pollacco, D.; Brown, D. J. A.; Doyle, A. P.; Collier Cameron, A.; Gillon, M.; Lendl, M. et al. (2013), "Discovery of WASP-65b and WASP-75b: Two Hot Jupiters Without Highly Inflated Radii", Astronomy & Astrophysics 559: A36, doi:10.1051/0004-6361/201322314, Bibcode: 2013A&A...559A..36G 
  65. ↑ 65.0 65.1 65.2 Delrez, L.; Van Grootel, V.; Anderson, D. R.; Collier-Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hellier, C. et al. (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, doi:10.1051/0004-6361/201323204, Bibcode: 2014A&A...563A.143D 
  66. ↑ 66.0 66.1 66.2 Anderson, D. R.; Collier Cameron, A.; Delrez, L.; Doyle, A. P.; Faedi, F.; Fumel, A.; Gillon, M.; Gómez Maqueo Chew, Y. et al. (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, doi:10.1093/mnras/stu1737 
  67. ↑ 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, doi:10.1088/1538-3873/aaa33e 
  68. ↑ 68.0 68.1 68.2 West, R. G.; Hellier, C.; Almenara, J.-M.; Anderson, D. R.; Barros, S. C. C.; Bouchy, F.; Brown, D. J. A.; Collier Cameron, A. et al. (2016), "Three irradiated and bloated hot Jupiters", Astronomy & Astrophysics 585: A126, doi:10.1051/0004-6361/201527276, Bibcode: 2016A&A...585A.126W 
  69. ↑ Triaud, A. H. M. J.; Anderson, D. R.; Collier Cameron, A.; Doyle, A. P.; Fumel, A.; Gillon, M.; Hellier, C.; Jehin, E. et al. (2013), "WASP-80b: a gas giant transiting a cool dwarf", Astronomy & Astrophysics 551: A80, doi:10.1051/0004-6361/201220900, Bibcode: 2013A&A...551A..80T 
  70. ↑ 70.0 70.1 70.2 70.3 70.4 70.5 70.6 Hellier, Coel; Anderson, D. R.; Cameron, A. Collier; Delrez, L.; Gillon, M.; Jehin, E.; Lendl, M.; Maxted, P. F. L. et al. (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, doi:10.1093/mnras/stu410 
  71. ↑ WTS-2 b: Too close for comfort?
  72. ↑ 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, doi:10.1093/mnras/stu343 



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