List of exoplanets discovered in 2013
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 | 1.21 | 2.184673 | 0.03416 | 1570 | transit | 450±2 | 1.11 | 5630 | [70] |
WASP-96b | 0.48 | 1.2 | 3.4252602 | 0.0453 | 1285 | transit | 1161±15 | 1.06 | 5540 | [70] |
WASP-97b | 1.32 | 1.13 | 2.07276 | 0.03303 | 1555 | transit | 494.9±1.7 | 1.12 | 5640 | [70] |
WASP-98b | 0.922 | 1.144 | 2.96264036 | 0.03762 | 1180 | transit | 926±5 | 0.81 | 5473 | [70] |
WASP-99b | 2.78 | 1.1 | 5.75251 | 0.0717 | 1480 | transit | 519±2 | 1.48 | 6180 | [70] |
WASP-100b | 2.03 | 1.69 | 2.849375 | 0.0457 | 2190 | transit | 1201±9 | 1.57 | 6900 | [70] |
WASP-101b | 0.5 | 1.41 | 3.585722 | 0.0506 | 1560 | transit | 660±3 | 1.34 | 6400 | [70] |
WTS-2b | 1.12 | 1.363 | 1.0187068 | 0.01855 | 2000 | transit | 3300 | 0.82 | 5000 | [71][72] |
Specific exoplanet lists
- List of directly imaged exoplanets
- List of exoplanet extremes
- List of exoplanet firsts
- List of exoplanets discovered by the Kepler space telescope
- List of exoplanets observed during Kepler's K2 mission
- List of extrasolar candidates for liquid water
- List of multiplanetary systems
- List of nearest exoplanets
- List of nearest terrestrial exoplanet candidates
- List of Neptunian exoplanets
- List of potentially habitable exoplanets
- List of proper names of exoplanets
- List of transiting exoplanets
Lists of exoplanet by year of discovery
- List of exoplanets discovered before 2000 (32)
- List of exoplanets discovered between 2000–2009 (379)
- List of exoplanets discovered in 2010 (109)
- List of exoplanets discovered in 2011 (179)
- List of exoplanets discovered in 2012 (149)
- List of exoplanets discovered in 2013 (151)
- List of exoplanets discovered in 2014 (878)
- List of exoplanets discovered in 2015 (151)
- List of exoplanets discovered in 2016 (1513)
- List of exoplanets discovered in 2017 (158)
- List of exoplanets discovered in 2018 (306)
- List of exoplanets discovered in 2019 (171)
- List of exoplanets discovered in 2020 (264)
- List of exoplanets discovered in 2021 (242)
- List of exoplanets discovered in 2022 (314)
- List of exoplanets discovered in 2023 (125)
References
- "The Extrasolar Planets Encyclopaedia". Retrieved 2015-11-09.
- PLANETS AROUND LOW-MASS STARS. III. A YOUNG DUSTY L DWARF COMPANION AT THE DEUTERIUM-BURNING LIMIT
- BD+15 2940 AND HD 233604: TWO GIANTS WITH PLANETS CLOSE TO THE ENGULFMENT ZONE
- Transiting exoplanets from the CoRoT space mission XXIV. CoRoT-25b and CoRoT-26b: two low-density giant planets
- 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
- 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.
- 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.
- 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
- 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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