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 1.6 311.6 1.2 radial vel. 375.8 2.54 4844 [15]
HD 13908 b 0.865 19.382 0.154 radial vel. 218.2 1.29 6255 [16]
HD 13908 c 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 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 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 0.63 0.96 7.340711 0.0781 transit 4300 1.18 6000 [36]
Kepler-75b 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 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-82b 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

Lists of exoplanets

Lists of exoplanet by year of discovery

References

  1. ↑ "The Extrasolar Planets Encyclopaedia". Extrasolar Planets Encyclopaedia. Retrieved 2015-11-09.
  2. ↑ PLANETS AROUND LOW-MASS STARS. III. A YOUNG DUSTY L DWARF COMPANION AT THE DEUTERIUM-BURNING LIMIT
  3. 1 2 BD+15 2940 AND HD 233604: TWO GIANTS WITH PLANETS CLOSE TO THE ENGULFMENT ZONE
  4. 1 2 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, arXiv:1306.3225, Bibcode:2013A&A...556A.133S, doi:10.1051/0004-6361/201321871, S2CID 119193690
  6. 1 2 3 Tuomi, 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. 1 2 3 4 5 Lo 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. 1 2 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, 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
  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, arXiv:1307.7640, Bibcode:2013ApJ...774..147R, doi:10.1088/0004-637X/774/2/147, S2CID 118514735
  11. ↑ Kuzuhara, M.; Tamura, M.; Kudo, T.; Janson, M.; Kandori, R.; Brandt, T. D.; Thalmann, C.; Spiegel, D.; Biller, B.; 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. arXiv:1307.2886. Bibcode:2013ApJ...774...11K. doi:10.1088/0004-637X/774/1/11. S2CID 53343537.
  12. 1 2 3 4 Hartman, 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
  14. ↑ Bayliss, D.; Zhou, G.; Penev, K.; Bakos, G. Á.; Hartman, J. D.; Jordán, A.; Mancini, L.; Mohler-Fischer, M.; Suc, V.; Rabus, M.; Béky, B.; Csubry, Z.; Buchhave, L.; Henning, T.; Nikolov, N.; Csák, B.; Brahm, R.; Espinoza, N.; Noyes, R. W.; Schmidt, B.; Conroy, P.; Wright, D. J.; Tinney, C. G.; Addison, B. C.; Sackett, P. D.; Sasselov, D. D.; Lázár, J.; Papp, I.; Sári, P. (2013), "HATS-3b: An inflated hot Jupiter transiting an F-type star", The Astronomical Journal, 146 (5): 113, arXiv:1306.0624, Bibcode:2013AJ....146..113B, doi:10.1088/0004-6256/146/5/113, S2CID 119194040
  15. 1 2 3 Sato, Bun'ei; Omiya, Masashi; Harakawa, Hiroki; Liu, Yu-Juan; Izumiura, Hideyuki; Kambe, Eiji; Takeda, Yoichi; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro; Ida, Shigeru (2013), "Planetary Companions to Three Evolved Intermediate-Mass Stars: HD 2952, HD 120084, andωSerpentis", Publications of the Astronomical Society of Japan, 65 (4): 85, arXiv:1304.4328, doi:10.1093/pasj/65.4.85
  16. 1 2 3 4 5 Moutou, 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
  17. ↑ Wittenmyer, Robert A.; Wang, Songhu; Horner, Jonathan; Tinney, C. G.; Butler, R. P.; Jones, H. R. A.; O'Toole, S. J.; Bailey, J.; Carter, B. D.; Salter, G. S.; Wright, D.; Zhou, Ji-Lin (2013), "Forever Alone? Testing Single Eccentric Planetary Systems for Multiple Companions", The Astrophysical Journal Supplement Series, 208 (1): 2, arXiv:1307.0894, Bibcode:2013ApJS..208....2W, doi:10.1088/0067-0049/208/1/2, S2CID 14109907
  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.
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  32. 1 2 The same frequency of planets inside and outside open clusters of stars
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