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] | |||
1.11 | 137.48 | 0.539 | radial vel. | 572.2 | 1.1 | 4796 | [3] | |||
0.27 | 1.08 | 4.86069 | 0.0578 | transit | 3300 | 1.09 | 6040 | [4] | ||
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] | ||
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 | [9] | ||
Gliese 504 b | 4 | 43.5 | imaging | 58.5 | 1.22 | 6234 | [10] | |||
0.352 | 1.242 | 4.301219 | 0.0507 | transit | 1180 | 0.94 | 5295 | [11] | ||
4 | 872.2 | 1.752 | radial vel. | 1180 | 0.94 | 5295 | Period is ambiguous[11] | |||
0.892 | 1.426 | 3.128992 | 0.0452 | transit | 990 | 1.26 | 6330 | [11] | ||
0.493 | 1.284 | 4.463129 | 0.0577 | transit | 970 | 1.28 | 6120 | [11] | ||
1.345 | 1.168 | 1.354133 | 0.023 | transit | 1200 | 0.88 | 5227 | [12] | ||
HATS-3b | 1.071 | 1.381 | 3.547851 | 0.0485 | 1648 | transit | 1480 | 1.21 | 6351 | [13] |
1.6 | 311.6 | 1.2 | radial vel. | 375.8 | 2.54 | 4844 | [14] | |||
0.865 | 19.382 | 0.154 | radial vel. | 218.2 | 1.29 | 6255 | [15] | |||
5.13 | 931 | 2.03 | radial vel. | 218.2 | 1.29 | 6255 | [15] | |||
HD 65216c | 0.17 | 152.6 | 0.54 | radial vel. | 116.1 | 0.92 | 5666 | [16]False positive, another planet with same assigned name discovered in 2019.[17] | ||
HD 95086 b | 5 | 55.7 | imaging | 298.7 | 1.6 | [18] | ||||
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 | [19] | |||
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 | [20] | ||
HD 120084 b | 4.5 | 2082 | 4.3 | radial vel. | 318.5 | 2.39 | 4892 | [14] | ||
HD 159243 b | 1.13 | 12.62 | 0.11 | radial vel. | 223.7 | 1.12 | 6123 | [15] | ||
1.9 | 248.4 | 0.8 | radial vel. | 223.7 | 1.12 | 6123 | [15] | |||
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)[21][22] | |||
HD 112410 b | 9.18 | 124.6 | 0.565 | radial vel. | 486.8 | 1.54 | 4830 | [23] | ||
1.068 | 5.0505 | 0.057 | radial vel. | 145.0 | 0.95 | 5519 | [15] | |||
KELT-3b | 1.477 | 1.345 | 2.7033904 | 0.04122 | transit | 580 | 1.28 | 6306 | [24] | |
KELT-6b | 0.442 | 1.18 | 7.8455821 | 0.08 | transit | 720 | 1.13 | 6272 | [25] | |
Kepler-37b | 0.03146 | 0.029 | 13.3675 | transit | 220 | 0.8 | 5417 | [26] | ||
Kepler-37c | 0.03776 | 0.067 | 21.302 | transit | 220 | 0.8 | 5417 | [26] | ||
Kepler-37d | 0.03839 | 0.173 | 39.7922 | transit | 220 | 0.8 | 5417 | [26] | ||
Kepler-61b | 0.192 | 59.87756 | transit | 1103±16 | 0.64 | 4017 | [27] | |||
Kepler-62b | 0.03 | 0.117 | 5.714932 | 0.0553 | transit | 1200 | 0.69 | 4925 | [28] | |
Kepler-62c | 0.013 | 0.048 | 12.4417 | 0.0929 | transit | 1200 | 0.69 | 4925 | [28] | |
Kepler-62d | 0.044 | 0.174 | 18.16406 | 0.12 | transit | 1200 | 0.69 | 4925 | [28] | |
Kepler-62e | 0.113 | 0.144 | 122.3874 | 0.427 | transit | 1200 | 0.69 | 4925 | Potentially habitable exoplanet[28] | |
Kepler-62f | 0.11 | 0.126 | 267.291 | 0.718 | transit | 1200 | 0.69 | 4925 | Potentially habitable exoplanet[28] | |
Kepler-63b | 0.378 | 0.545 | 9.4341505 | 0.08 | transit | 650 | 0.98 | 5576 | [29] | |
Kepler-65b | 0.127 | 2.15491 | 0.035 | transit | 999±8 | 1.25 | 6211 | [30] | ||
Kepler-65c | 0.23 | 5.859944 | 0.068 | transit | 999±8 | 1.25 | 6211 | [30] | ||
Kepler-65d | 0.136 | 8.13123 | 0.084 | transit | 999±8 | 1.25 | 6211 | [30] | ||
Kepler-66b | 0.25 | 17.815815 | 0.1352 | transit | 3610 | 1.04 | 5962 | Belongs to open cluster NGC 6811[31] | ||
Kepler-67b | 0.262 | 15.7259 | 0.1171 | transit | 3610 | 0.86 | 5331 | Belongs to open cluster NGC 6811[31] | ||
Kepler-68b | 0.01878 | 0.208 | 5.39875 | 1280 | transit | 440 | 1.08 | 5793 | [32] | |
Kepler-68c | 0.02265 | 0.089 | 9.60504 | transit | 440 | 1.08 | 5793 | [32] | ||
Kepler-68d | 0.84007 | 625 | radial vel. | 440 | 1.08 | 5793 | [32] | |||
Kepler-69b | 0.2 | 13.722341 | 0.094 | transit | 2430±30 | 0.81 | 5638 | [33] | ||
Kepler-69c | 0.153 | 242.4613 | 0.64 | transit | 2430±30 | 0.81 | 5638 | [33][34] | ||
0.63 | 0.96 | 7.340711 | 0.0781 | transit | 4300 | 1.18 | 6000 | [35] | ||
10.1 | 1.05 | 8.8849116 | 0.0818 | transit | 3700 | 0.91 | 5200 | [35] | ||
Kepler-76b | 2.01 | 1.36 | 1.5449298 | 0.0274 | orbital brightness modulation | 2750±30 | 1.2 | 6409 | [36] | |
0.43 | 0.96 | 3.57878087 | 0.04501 | transit | 1900 | 0.95 | 5520 | [37] | ||
Kepler-78b | 0.006 | 0.105 | 0.355 | 2330 | transit | 407.1±1.1 | 0.76 | 5058 | [38] | |
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] | |
0.202 | 0.313 | 13.749 | transit | 1580±17 | 1.21 | 5883 | [45] | |||
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] | ||
0.009 | 0.143 | 8.041 | 623 | transit | 852±4 | 0.56 | 4605 | [45] | ||
0.012 | 0.226 | 11.776 | 549 | transit | 852±4 | 0.56 | 4605 | [45] | ||
0.097 | 0.101 | 15.09 | transit | 1307±12 | 1.18 | 6090 | [45] | |||
0.105 | 0.101 | 22.804 | transit | 1307±12 | 1.18 | 6090 | [45] | |||
0.091 | 8.457458 | 0.079 | transit | 1042±7 | 1 | 5884 | [46] | |||
0.117 | 0.236 | 22.951 | transit | 1880±30 | 1.32 | 6022 | [45] | |||
0.25 | 0.385 | 42.882 | transit | 1880±30 | 1.32 | 6022 | [45] | |||
0.006 | 0.259 | 36.855 | transit | 4880±140 | 1.07 | 5942 | [45] | |||
0.024 | 0.633 | 49.412 | transit | 4880±140 | 1.07 | 5942 | [45] | |||
0.534 | 0.5 | 23.654 | transit | 6200±300 | 1.06 | 5751 | [45] | |||
0.042 | 0.178 | 50.447 | transit | 6200±300 | 1.06 | 5751 | [45] | |||
0.052 | 0.259 | 31.884 | transit | 3850±150 | 1.1 | 6105 | [45] | |||
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] | ||
0.323 | 12.309681 | 0.112 | transit | 3480±70 | 1.1 | 6363 | KOI-1236.01[47] | |||
0.155 | 0.384 | 35.736 | transit | 3490±70 | 1.1 | 6363 | KOI-1236.02[47][45] | |||
0.118 | 0.277 | 54.414 | transit | 3490±70 | 1.1 | 6363 | [45] | |||
0.192 | 0.219 | 24.806 | transit | 4540±150 | 0.97 | 5602 | [45] | |||
0.177 | 0.277 | 44.347 | transit | 4540±150 | 0.97 | 5602 | [45] | |||
0.033 | 0.321 | 5.487 | transit | 2900±90 | 0.76 | 5100 | [45]KOI-1563.01[47] | |||
0.019 | 0.294 | 8.291 | transit | 2900±90 | 0.76 | 5100 | [45]KOI-1563.02[47] | |||
0.02341 | 0.217 | 10.4208 | transit | 1908±17 | 0.91 | 5367 | [45] | |||
0.01145 | 0.196 | 13.0729 | transit | 1908±17 | 0.91 | 5367 | [45] | |||
0.09 | 0.205 | 34.921 | transit | 7700±500 | 1.15 | 5914 | [45] | |||
0.124 | 0.482 | 71.312 | transit | 7700±500 | 1.15 | 5914 | [45] | |||
0.019 | 0.277 | 17.849 | transit | 3210±70 | 1 | 6186 | [45] | |||
0.047 | 0.25 | 26.136 | transit | 3210±70 | 1 | 6186 | [45] | |||
0.238 | 0.312 | 42.994 | transit | 734±5 | 0.85 | 5384 | [45]KOI-2672.01[47] | |||
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] | ||
4.1 | 3.3 | microlensing | 11000 | 0.56 | [50] | |||||
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] | ||||
4.8 | 1.1 | microlensing | 25200 | 0.86 | [53] | |||||
11.6 | 4.3 | microlensing | 24700 | 0.39 | [54] | |||||
0.53 | 2.72 | microlensing | 8400 | 0.26 | [55] | |||||
1.85 | 0.87 | microlensing | 5700 | 0.02 | Orbiting a brown dwarf[56] | |||||
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 | [14] | ||
PH2b | 0.903 | 282.5255 | 0.828 | 281 | transit | 1130±10 | 0.94 | 5629 | [58]Also called Kepler-86b | |
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] | ||
1.55 | 1.112 | 2.3114243 | 0.0334 | transit | 1000 | 0.93 | 5600 | [63] | ||
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] |
0.59 | 1.164 | 3.7130203 | 0.04853 | 1387 | transit | 800 | 1.11 | 5763 | [65] | |
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 | 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 | 1.21 | 2.184673 | 0.03416 | 1570 | transit | 450±2 | 1.11 | 5630 | [69] |
0.48 | 1.2 | 3.4252602 | 0.0453 | 1285 | transit | 1161±15 | 1.06 | 5540 | [69] | |
1.32 | 1.13 | 2.07276 | 0.03303 | 1555 | transit | 494.9±1.7 | 1.12 | 5640 | [69] | |
0.922 | 1.144 | 2.96264036 | 0.03762 | 1180 | transit | 926±5 | 0.81 | 5473 | [69] | |
2.78 | 1.1 | 5.75251 | 0.0717 | 1480 | transit | 519±2 | 1.48 | 6180 | [69] | |
2.03 | 1.69 | 2.849375 | 0.0457 | 2190 | transit | 1201±9 | 1.57 | 6900 | [69] | |
0.5 | 1.41 | 3.585722 | 0.0506 | 1560 | transit | 660±3 | 1.34 | 6400 | [69] | |
1.12 | 1.363 | 1.0187068 | 0.01855 | 2000 | transit | 3300 | 0.82 | 5000 | [70][71] |
Specific exoplanet lists[]
- Lists of exoplanets
- List of exoplanets discovered before 2000 (32)
- List of exoplanets discovered between 2000–2009 (378)
- List of exoplanets discovered in 2010 (108)
- List of exoplanets discovered in 2011 (169)
- List of exoplanets discovered in 2012 (148)
- List of exoplanets discovered in 2013 (151)
- List of exoplanets discovered in 2014 (868)
- List of exoplanets discovered in 2015 (152)
- List of exoplanets discovered in 2016 (1505)
- List of exoplanets discovered in 2017 (154)
- List of exoplanets discovered in 2018 (314)
- List of exoplanets discovered in 2019 (192)
- List of exoplanets discovered in 2020 (260)
- List of exoplanets discovered in 2021 (177)
- List of potentially habitable exoplanets
- List of proper names of exoplanets
- List of multiplanetary systems
- List of exoplanet firsts
- List of exoplanet extremes
- List of exoplanets discovered using the Kepler space telescope
- List of exoplanets observed during Kepler's K2 mission
- List of extrasolar candidates for liquid water
- List of nearest exoplanets
- List of nearest terrestrial exoplanet candidates
- List of transiting exoplanets
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
- ^ Jump up to: a b BD+15 2940 AND HD 233604: TWO GIANTS WITH PLANETS CLOSE TO THE ENGULFMENT ZONE
- ^ Jump up to: a b 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
- ^ Jump up to: a b c 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.
- ^ Jump up to: a b c d e 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.
- ^ Jump up to: a b 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
- ^ 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
- ^ 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.
- ^ Jump up to: a b c d HAT-P-44b, HAT-P-45b, AND HAT-P-46b: THREE TRANSITING HOT JUPITERS IN POSSIBLE MULTI-PLANET SYSTEMS, 2013, arXiv:1308.2937
- ^ 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
- ^ 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
- ^ Jump up to: a b c Planetary Companions to Three Evolved Intermediate-Mass Stars: HD 2952, HD 120084, and ω Serpentis, 2013, arXiv:1304.4328
- ^ Jump up to: a b c d e Moutou, C.; Hebrard, G.; Bouchy, F.; Arnold, L.; Santos, N. C.; Astudillo-Defru, N.; Boisse, I.; Bonfils, X.; Borgniet, S.; Delfosse, X.; Diaz, R. F.; Ehrenreich, D.; Forveille, Thierry; Gregorio, J.; Labrevoir, O.; Lagrange, A. M.; Montagnier, G.; Montalto, M.; Pepe, F.; Sahlmann, J.; Santerne, A.; Segransan, D.; Udry, S.; Vanhuysse, M. (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
- ^ Forever alone? Testing single eccentric planetary systems for multiple companions, 2013, arXiv:1307.0894
- ^ 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.
- ^ 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.CS1 maint: multiple names: authors list (link)
- ^ 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.
- ^ Borgniet, S.; Boisse, I.; Lagrange, A.-M.; Bouchy, F.; Arnold, L.; Díaz, R. F.; Galland, F.; Delorme, P.; Hébrard, G.; Santerne, A.; Ehrenreich, D.; Ségransan, D.; Bonfils, X.; Delfosse, X.; Santos, N. C.; Forveille, Thierry; Moutou, C.; Udry, S.; Eggenberger, A.; Pepe, F.; Astudillo, N.; Montagnier, G. (2013), "Extrasolar planets and brown dwarfs around A--F type stars. VIII. A giant planet orbiting the young star HD113337", Astronomy & Astrophysics, 561: A65, arXiv:1310.1994, doi:10.1051/0004-6361/201321783, S2CID 118538542
- ^ Carleo, I.; et al. (2020). "The GAPS Programme at TNG XXI -- A GIARPS case-study of known young planetary candidates: Confirmation of HD 285507 b and refutation of AD Leo B". Astronomy & Astrophysics. A5: 638. arXiv:2002.10562. Bibcode:2020A&A...638A...5C. doi:10.1051/0004-6361/201937369. S2CID 211296466.
- ^ Open exoplanet catalogue HD 285507
- ^ Jones, M. I.; et al. (2013). "Study of the Impact of the Post-MS evolution of the Host Star on the Orbits of Close-in Planets. II. A Giant Planet in a Close-in Orbit around the RGB Star HIP 63242". Astronomy & Astrophysics. 556 (A78): 5. arXiv:1306.3939. Bibcode:2013A&A...556A..78J. doi:10.1051/0004-6361/201321660. S2CID 118618692.
- ^ 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: 64. arXiv:1211.1031. doi:10.1088/0004-637X/773/1/64. ISSN 0004-637X.
- ^ KELT-6b: A P~7.9 d HOT SATURN TRANSITING A METAL-POOR STAR WITH A LONG-PERIOD COMPANION, 2013, arXiv:1308.2296
- ^ Jump up to: a b c A sub-Mercury-sized exoplanet, 2013, arXiv:1305.5587
- ^ 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
- ^ Jump up to: a b c d e Kepler-62: A five-planet system with planets of 1.4 and 1.6 Earth radii in the habitable zone, 2013, arXiv:1304.7387
- ^ Kepler-63b: A Giant Planet in a Polar Orbit around a Young Sun-like Star, 2013, arXiv:1307.8128
- ^ Jump up to: a b c Chaplin, W. J.; Sanchis-Ojeda, R.; Campante, T. L.; Handberg, R.; Stello, D.; Winn, J. N.; Basu, S.; Christensen-Dalsgaard, J.; Davies, G. R.; Metcalfe, T. S.; Buchhave, L. A.; Fischer, D. A.; Bedding, T. R.; Cochran, W. D.; Elsworth, Y.; Gilliland, R. L.; Hekker, S.; Huber, D.; Isaacson, H.; Karoff, C.; Kawaler, S. D.; Kjeldsen, H.; Latham, D. W.; Lund, M. N.; Lundkvist, M.; Marcy, G. W.; Miglio, A.; Barclay, T.; Lissauer, J. J. (2013), "Asteroseismic determination of obliquities of the exoplanet systems Kepler-50 and Kepler-65", The Astrophysical Journal, 766 (2): 101, arXiv:1302.3728, Bibcode:2013ApJ...766..101C, doi:10.1088/0004-637X/766/2/101, S2CID 17748525
- ^ Jump up to: a b The same frequency of planets inside and outside open clusters of stars
- ^ Jump up to: a b c 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. arXiv:1302.2596. Bibcode:2013ApJ...766...40G. doi:10.1088/0004-637X/766/1/40.
- ^ Jump up to: a b A SUPER-EARTH-SIZED PLANET ORBITING IN OR NEAR THE HABITABLE ZONE AROUND SUN-LIKE STAR, 2013, arXiv:1304.4941
- ^ A POTENTIAL SUPER-VENUS IN THE KEPLER-69 SYSTEM, 2013, arXiv:1305.2933
- ^ Jump up to: a b KOI-200b and KOI-889b: two transiting exoplanets detected and characterized with Kepler, SOPHIE and HARPS-N, 2013, arXiv:1304.6002
- ^ 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.
- ^ Kepler-77b: a very low albedo, Saturn-mass transiting planet around a metal-rich solar-like star, 2013, arXiv:1305.3891
- ^ A Rocky Composition for an Earth-sized Exoplanet, 2013, arXiv:1310.2064
- ^ Jump up to: a b An Independent Planet Search In The Kepler Dataset. II. An extremely low-density super-Earth mass planet around Kepler-87, 2013, arXiv:1310.2064
- ^ Jump up to: a b KOI-142, THE KING OF TRANSIT VARIATIONS, IS A PAIR OF PLANETS NEAR THE 2:1 RESONANCE, 2013, arXiv:1304.4283
- ^ SOPHIE velocimetry of Kepler transit candidates X KOI-142 c: first radial velocity confirmation of a non-transiting exoplanet discovered by transit timing, 2013, arXiv:1311.4335
- ^ Jump up to: 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.
- ^ Jump up to: a b c d e f g h Planet Hunters VI: An Independent Characterization of KOI-351 and Several Long Period Planet Candidates from the Kepler Archival Data, 2013, arXiv:1310.5912
- ^ 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.
- ^ Jump up to: 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 TRANSIT TIMING VARIATION OF NEAR-RESONANCE PLANETARY PAIRS. II. CONFIRMATION OF 30 PLANETS IN 15 MULTIPLE PLANET SYSTEMS, 2013, arXiv:1309.2329
- ^ Jump up to: a b c d 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 the Kepler Multiple Planet Candidates, 2013, arXiv:1309.7097
- ^ Jump up to: 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, arXiv:1308.0996, doi:10.1088/0004-637X/778/2/110, S2CID 117080296
- ^ 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, 2013, arXiv:1312.4938
- ^ PLANET HUNTERS. VIII. CHARACTERIZATION OF 41 LONG-PERIOD EXOPLANET CANDIDATES FROM KEPLER ARCHIVAL DATA, 2015, arXiv:1512.02559
- ^ MOA-2008-BLG-379Lb: A Massive Planet from a High Magnification Event with a Faint Source, 2013, arXiv:1311.3424
- ^ MOA-2010-BLG-328Lb: a sub-Neptune orbiting very late M dwarf ?, 2013, arXiv:1309.7714
- ^ Jump up to: 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
- ^ 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
- ^ MOA-2011-BLG-322Lb: a "second generation survey" microlensing planet, 2013, arXiv:1310.0008
- ^ 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
- ^ Microlensing Discovery of a Tight, Low Mass-ratio Planetary-mass Object around an Old, Field Brown Dwarf, 2013, arXiv:1307.6335
- ^ Super-massive planets around late-type stars - the case of OGLE-2012-BLG-0406Lb, 2013, arXiv:1307.4084
- ^ 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].
- ^ A hot Jupiter transiting a mid-K dwarf found in the pre-OmegaCam Transit Survey, 2013, arXiv:1308.6574
- ^ 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. arXiv:1310.0457. Bibcode:2013ApJ...777L..20L. doi:10.1088/2041-8205/777/2/L20.
- ^ Jump up to: a b Three Wide Planetary-Mass Companions to FW Tau, ROXs 12, and ROXs 42B, 2013, arXiv:1311.7664
- ^ 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, arXiv:1312.2954, doi:10.1088/0004-637X/785/2/126, S2CID 42687848
- ^ Jump up to: 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
- ^ Jump up to: 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, arXiv:1312.1827, doi:10.1051/0004-6361/201323204, S2CID 54846964
- ^ Jump up to: 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
- ^ 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
- ^ Jump up to: a b c Three irradiated and bloated hot Jupiters: WASP-76b, WASP-82b & WASP-90b, 2013, arXiv:1310.5607
- ^ 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
- ^ Jump up to: a b c d e f g Transiting hot Jupiters from WASP-South, Euler and TRAPPIST: WASP-95b to WASP-101b, 2013, arXiv:1310.5630
- ^ WTS-2 b: Too close for comfort?
- ^ WTS-2 b: a hot Jupiter orbiting near its tidal destruction radius around a K-dwarf, 2014, arXiv:1402.5416
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