List of exoplanets discovered in 2024
This list of exoplanets discovered in 2024 is a list of confirmed exoplanets that were first reported in 2024. For exoplanets detected only by radial velocity, the listed value for mass is a lower limit. See Minimum mass for more information.
Name | Mass (MJ) | Radius (RJ) | Period (days) | Semi-major axis (AU) | Temp. (K) | Discovery method | Distance (ly) | Host star mass (M☉) | Host star temp. (K) | Remarks |
---|---|---|---|---|---|---|---|---|---|---|
2MASS J05581644-4501559 b | 6–12 | 1043 | imaging | 94.5 | 0.259±0.02[1] | 3218±158[1] | [2] | |||
BD-14 3065 b | 12.11+0.95 −0.91 |
1.926±0.094 | 4.3 | 0.0646±0.0026 | 1957±28 | transit | 1847.4[3][a] | 1.4±0.06 | 6985±90 | Located in a triple star system. It orbits the primary component of the system (BD-14 3065 A), a subgiant star.[4] Also known as TOI-4987 b |
CI Tauri c | 3.6±0.3 | 25.2±1.8 | 0.17 | radial vel. | 522.6±1.3 | 0.9±0.02 | 4250±50 | [5]Highly eccentric orbit (e = 0.58). Cited as confirmed by NASA Exoplanet Archive and exoplanet.eu.[6][5] | ||
Gaia20eae b | 6 | 0.062 | disc thermal instability | 9226+3130 −2021[7] |
1.15 | 4330±300[7] | [8] | |||
Gliese 12 b | 0.002769+0.00123 −0.0008 |
0.0892±0.0089[b] | 12.7 | 0.066±0.002 | 315±5 | transit | 39.65 | 0.241±0.006 | 3253±55 | [9] |
Gliese 238 b | 0.05049±0.0012 | 1.74 | 0.02123+0.00016 −0.00017 |
758+16 −15 |
transit | 49.6 | 0.419±0.01 | 3485±140 | Mars-sized exoplanet, one of the smallest exoplanets currently known[10] | |
Gliese 341 b | 0.00227±0.00044 | 0.0821±0.045 | 7.577 | 540 | transit | 33.9 | 0.506 | 3745 | [11]Also known as TOI-741 b | |
HD 63433 d | 0.09573±0.0141 | 4.21 | 0.0503±0.0027 | 1040±40 | transit | 71.7 | 0.99±0.03 | 5688±28 | [12]Hot Earth-sized exoplanet | |
HD 77344 b | 0.00939+0.00787 −0.00599 |
0.2573+0.0073 −0.0064 |
15.6 | 0.131 | 911±7 | transit | 114.7 | 1.2±0.02 | 6220±64 | The temperature can be as high as 1,066 K if the planet is tidally locked. Another planet in the system (HD 77344 c) is suspected. It has a minimum mass of 116.3 ME and an orbital period of 66 days[13] |
HD 77946 b | 0.02637±0.00415 | 0.24133+0.00767 −0.0071 |
6.527 | 0.072±0.0012 | 1248+40 −38 |
transit | 322.7±1 | 1.17±0.06 | 6046.0±50.0 | [14]Also known as TOI-1778 b |
HD 104067 c | 0.0415 | 13.8992+0.0047 −0.0037 |
0.1058±0.0013 | radial vel. | 66.34±0.03 | 0.82±0.03 | 4952±100 | [15] | ||
HD 134606 e | 0.00726+0.00113 −0.0011 |
4.32 | 0.0527±0.0012 | radial vel. | 87.4±0.068 | 1.046+0.07 −0.059 |
5576+86 −85 |
[16] | ||
HD 134606 f | 0.01737+0.00232 −0.00229 |
26.915 | 0.1784±0.004 | radial vel. | 87.4±0.068 | 1.046+0.07 −0.059 |
5576+86 −85 |
[16] | ||
HIP 39017 b | 23.6+9.1 −7.4 |
0.87 | 30681+18627.8 −9496.5 |
22.1+8.0 −4.9 |
imaging | 214.9±0.3 | 1.52+0.28 −0.26 |
7201+142 −112[17] |
[18] May be a brown dwarf. Estimated of the mass vary from 13.8 MJ to 30+31 −12 MJ. | |
HS Piscium b | 1.44+0.56 −0.44 |
3.986 | 0.0435±0.0017 | radial vel. | 122.79+0.12 −0.14 |
0.69±0.07 | 4203±116 | [19] | ||
KMT-2016-BLG-2321Lb | 3.58±1.22 | 3.58±0.81 | microlensing | 11,670±3980 | 0.73±0.28 | [20] | ||||
KMT-2023-BLG-0416Lb | 6.15+3.03 −3.2 |
3.73+0.56 −0.8 |
microlensing | 20,640+3100 −4400 |
0.61+0.3 −0.32 |
[21]The mass of the planet can be as low as 0.042+0.021 −0.022 MJ | ||||
KMT-2023-BLG-0469Lb | 0.124+0.092 −0.067 |
2.37±0.9 | microlensing | 23,050+3260 −3910 |
0.47±0.36 | [22] | ||||
KMT-2023-BLG-0735Lb | 0.12±0.07 | 2.75±1 | microlensing | 20,830+3910 −3260 |
0.61±0.34 | [22] | ||||
KMT-2023-BLG-1454Lb | 0.63+0.71 −0.34 |
1.18+0.17 −0.18 |
microlensing | 23,540+3460 −3590 |
0.17+0.19 −0.09 |
[21]Estimates of the planet's mass varies between 0.3+0.34 −0.16 MJ and 0.77+0.87 −0.42 MJ | ||||
KMT-2023-BLG-1642Lb | 1.08+1.53 −0.58 |
1.41+0.22 −0.27 |
microlensing | 22,750+3550 −4370 |
0.17+0.24 −0.09 |
[21] | ||||
KMT-2023-BLG-1866Lb | 0.00828+0.00132 −0.00214 |
2.63+0.37 −0.34 |
microlensing | 20,240+2840 −1100 |
0.51+0.08 −0.13 |
Super-Earth planet detected by microlensing[23] | ||||
LHS 1678 d | 0.00289+0.00208 −0.00107 |
0.08752±0.0062 | 4.965 | 0.04+0.0018 −0.0017 |
transit | 65 | 0.345±0.014 | 3490±50 | [24] | |
M62H b | 2.83 | <0.683 [c][d] | 0.133 | 0.004908 | timing | 21,500[25] | 1.4 | Pulsar planet located in the globular cluster Messier 62.[26] | ||
MOA-2016-BLG-526Lb | 6.93±0.75 | 2.07±0.35 | microlensing | 22,490 | 0.4 | [20] | ||||
MOA-2022-BLG-563Lb | 0.4+0.31 −0.25 |
2.25±0.25 | microlensing | 21,290+3650 −5220 |
0.48+0.36 −0.3 |
[22] | ||||
OGLE-2016-BLG-1598Lb | 5.91±1.74 | 2.5±0.88 | microlensing | 19,270±5670 | 0.55±0.32 | [20] | ||||
NGTS-26 b | 0.29+0.07 −0.06 |
1.33+0.06 −0.05 |
4.52 | 0.0490+0.0038 −0.0032 |
1331+85 −72 |
transit | 3610±100 | 0.96+0.04 −0.03 |
5550±100 | Highly inflated planet (density = 0.153 g/cm3)[27] |
NGTS-27 b | 0.593+0.095 −0.072 |
1.396+0.038 −0.035 |
3.37 | 0.0446+0.0026 −0.0036 |
1783+104 −88 |
transit | 3185±55 | 1.07±0.06 | 5700±80 | [27] |
NGTS-29 b | 0.393 | 0.857 | 69.33 | 0.347 | 414 | transit | 487±1 | 1.034±0.032 | 5730±80 | [28] |
NGTS-30 b | 0.96 | 0.93 | 98.3 | 0.408 | 390 | transit | 762.5 | 0.94 | 5455 | [29] Also known as TOI-4862 b |
OGLE-2016-BLG-1800Lb | 2.59±1.46 | 1.88±0.51 | microlensing | 21,100±3360 | 0.41±0.22 | [20] | ||||
OGLE-2017-BLG-0640Lb | 1.62+1.64 −0.94 |
1.14±0.38 | microlensing | 21,600+3550 −4730 |
0.32+0.32 −0.18 |
[30] | ||||
OGLE-2017-BLG-1237Lb | 3.8+2.49 −1.99 |
2.53+0.5 −0.64 |
microlensing | 19,660+3060 −4990 |
0.46+0.3 −0.24 |
[30] | ||||
OGLE-2017-BLG-1275Lb | 5.9±2.2 | 1.19±0.36 | microlensing | 25,070±2930 | 0.63±0.23 | [30]Another solution suggests a larger semi-major axis, of 2.09±0.63 AU | ||||
OGLE-2023-BLG-0836Lb | 4.36+2.35 −2.2 |
3.7+1 −1.2 |
microlensing | 16,690+4430 −5250 |
[e] | [31]The planet is located in a binary star system, and is likely to be orbiting both stars in the system. | ||||
S1429 b | 1.8±0.2 | 77.51±0.2 | 0.384±0.4 | 683±9 | radial vel. | 2836±26 | 1.26±0.04 | 6000±40 | [32]Located in the open cluster Messier 67 | |
SPECULOOS-3 b | 0.08716 | 0.719 | 0.00733 | 553 | transit | 57.9 | 0.1 | 2800 | Ultra-short period planet[33] | |
Teegarden's Star d | 0.00258±0.00053 | 26.13 | 0.0791 ±0.0027 | 159±3 | radial vel. | 12.5 | 0.097±0.01 | 3034±45 | Orbits beyond the habitable zone of its star. Another planet in the system is suspected.[34] | |
TIC 4672985 b | 12.74±1.01 | 1.026+0.065 −0.067 |
69.05 | 0.33±0.019 | 517.2+11.3 −11.2 |
transit | 823.4[35][a] | 1.01±0.03 | 5757+72 −65 |
[36] |
TIC 139270665 b | 0.463 | 0.645 | 23.624 | 0.163 | 700 | transit | 618 | 1.035+0.052 −0.062 |
5844+84 −82 |
[37][38] |
TIC 139270665 c | 4.89+0.66 −0.37 |
1010+780 −220 |
2+0.93 −0.31 |
200+18 −35 |
radial vel. | 618 | 1.035+0.052 −0.062 |
5844+84 −82 |
[38] | |
TIC 365102760 b | 0.060 | 0.55 | 4.21285367±0.00000074 | 0.0622±0.0049 | radial vel. | 1811.8±24.79 | 1.17±0.12 | 4900±90 | [39] | |
TIC 393818343 b | 4.34±0.15 | 1.087+0.023 −0.021 |
16.25 | 0.129±0.002 | 805.5+9.6 −9.4 |
transit | 306.3±1.1 | 1.082+0.055 −0.056 |
5756+57 −66 |
Highly eccentricit orbit (e=0.6058)[40] Also known as TOI-6883 b[41] |
TOI-238 c | 0.0211±0.0035 | 0.1945±0.0161 | 8.466 | 0.0749±0.0013 | 696±15 | transit | 261.328±0.312 | 0.79±0.022 | 5059±89 | [42] |
TOI-260 b | 0.0104 | 0.1311 | 13.47 | 0.09 | transit | 66 | Host star also known as HIP 1532[43] | |||
TOI-329 b | 0.1271 | 5.71 | 0.064 | transit | 927.1 | 0.98 | 5560 | Radius of the host star is significantly larger compared to mass (1.61 R☉)[44] | ||
TOI-480 b | 0.0654 | 6.866 | transit | 177.8 | 1.2 | 6,212 | [45] | |||
TOI-782 b | <0.06 | 0.244±0.008 | 8.024 | 0.0578±0.0018 | 398±6–435±6[f] | transit | 170.2±0.2 | 0.397±0.01 | 3370+29 −32 |
[46] |
TOI-815 b | 0.0239±0.0047 | 0.2622±0.0044 | 11.197 | 0.0903+0.0018 −0.0019 |
686+13 −14 |
transit | 193.76±0.15 | 0.776±0.036 | 4869±77 | [47] The host star is part of a binary star system with a red dwarf companion |
TOI-815 c | 0.0739±0.00755 | 0.2337+0.0089 −0.008 |
34.976 | 0.193±0.004 | 469±9 | transit | 193.76±0.15 | 0.776±0.036 | 4869±77 | [47] The host star is part of a binary star system with a red dwarf companion |
TOI-1135 b | 0.062+0.033 −0.031 |
0.805±0.02 | 5.13±0.27 | 0.082±0.003 | 1198.9±21.3 | transit | 371.4±0.5 | 1.125±0.032 | 6122±25 | [48] |
TOI-1173 Ab | 0.08213±0.00598 | 0.723±0.015 | 7.064 | 0.0702±0.0012 | 863.9±9.8 | transit | 430.85[49][a] | 0.911+0.028 −0.03 |
5350±340 | [50]Low-density planet located in a wide binary system |
TOI-1199 b | 0.239±0.02 | 0.938±0.025 | 3.671 | 0.04988±0.0009 | 1486±20 | transit | 805±2.6 | 1.23±0.07 | 5710±40 | [51] |
TOI-1273 b | 0.222±0.015 | 0.99±0.2 | 4.631 | 0.0549±0.001 | 1211±15 | transit | 574±1.3 | 1.06±0.06 | 5690±40 | [51] |
TOI-1347 b | 0.0349±0.0038 | 0.161±0.009 | 0.847 | 1400±40 | transit | 480.8±2 | 0.913±0.033 | 5464±100 | [52] Ultra-short period planet | |
TOI-1347 c | 0.0088±0.0072 | 0.143±0.009 | 4.842 | 1000±25 | transit | 480.8±2 | 0.913±0.033 | 5464±100 | [52] | |
TOI-1386 b | 0.148+0.019 −0.018 |
0.54+0.018 −0.016 |
25.838 | 0.1732+0.0027 −0.0033 |
676.4+10 −8.3 |
transit | 478.8±2.2 | 1.038+0.05 −0.058 |
5793+76 −73 |
[53] |
TOI-1386 c | 0.309±0.038 | 227.6+4.6 −4 |
0.739+0.015 −0.016 |
327.4+5.3 −4.6 |
radial vel. | 478.8±2.2 | 1.038+0.05 −0.058 |
5793+76 −73 |
[53] | |
TOI-1448 b | <0.0613 | 0.245±0.006 | 8.112 | 0.0567±0.0015 | 389±5–426±6[f] | transit | 240±0.3 | 0.372±0.009 | 3412+28 −32 |
[46] |
TOI-1450 Ab | 0.00396±0.0004 | 0.1±0.004 | 2.04 | 722±35 | transit | 73.2±0.1 | 0.48±0.24 | 3437±86 | Located in a binary star system. It is the second-lowest mass transiting planet with a high-precision mass measurement.[54] | |
TOI-1450 Ac | 0.0048±0.0006 | 5.07 | 533±26 | radial vel. | 73.2±0.1 | 0.48±0.24 | 3437±86 | Located in a binary system, its true mass could be similar to the minimum mass assuming coplanarity with TOI-1450 Ab [54] | ||
TOI-1751 b | 0.0538±0.0101 | 0.2489±0.0259 | 37.468 | 0.2115±0.0024 | 820 | transit | 370.3±0.3 | 1.15±0.17 | 6116±22 | [55]The host star is metal-poor ([Fe/H] = –0.40 dex) |
TOI-1824 b | 0.0582±0.01 | 0.2346±0.0133 | 22.8 | 0.149±0.003 | 577±19 | transit | 192.3 | 0.85±0.05 | 5180±110 | High-density planet, situated in the small group of "superdense sub-Neptunes". TOI-1824 has also a red dwarf companion star named TIC 142387022.[56] |
TOI-1855 b | 1.133±0.096 | 1.65+0.37 −0.62 |
1.364 | 0.02398+0.00037 −0.00036 |
1700±20 | transit + radial vel. | 576.3±4.6 | 0.987+0.058 −0.045 |
5359+89 −83 |
[57] |
TOI-2107 b | 0.83±0.11 | 1.211±0.035 | 2.454 | 0.0315+0.0006 −0.00067 |
1397±20 | transit + radial vel. | 767.4+6.2 −5.9 |
0.961+0.049 −0.054 |
5627+94 −93 |
[57] |
TOI-2120 b | <0.02139 | 0.1893±0.0056 | 5.8 | 0.0377±0.0013 | 351±6–384±6[f] | transit | 104.9 | 0.211±0.005 | 3131±30 | [46] |
TOI-2266 b | 0.1374±0.008 | 2.326 | 0.02±0.002 | 550±47 | transit | 168.6±0.2 | 0.23±0.02 | 3240±160 | [58] | |
TOI-2368 b | 0.65±0.18 | 0.967+0.06 −0.03 |
5.175 | 0.05649±0.001 | 1000+44 −30 |
transit | 685±3.9 | 0.897+0.048 −0.049 |
5360+230 −170 |
[57] |
TOI-2373 b | 9.3±0.2 | 0.93±0.02 | 13.337 | 0.112±0.001 | 860±10 | transit | 1617±33 | 1.041+0.032 −0.028 |
5651±180 | [59] |
TOI-2416 b | 3+0.1 −0.09 |
0.88±0.02 | 8.275 | 0.0831±0.0007 | 1080±10 | transit | 1767±261 | 1.118+0.029 −0.027 |
5808±80 | [59] |
TOI-2524 b | 0.64±0.04 | 1+0.02 −0.03 |
7.186 | 0.073±0.0007 | 1100±20 | transit | 1399±36 | 1.007+0.032 −0.029 |
5831±80 | [59] |
TOI-2529 b | 2.34±0.2 | 1.03±0.05 | 64.5949±0.0003 | 0.327±0.02 | 636±15.7 | transit | 965.8+14 −13.7 |
1.11+0.02 −0.02 |
5802+60 −52 |
[36] |
TOI-3321 b | 0.554±0.076 | 1.39+0.07 −0.06 |
3.652 | 0.047±0.001 | 1616±30 | transit | 928+10.8 −10.4 |
1.041+0.084 −0.068 |
5850±140 | [57] |
TOI-3894 b | 0.85±0.15 | 1.36±0.05 | 4.335 | 0.0543±0.0014 | 1519±22 | transit | 1343+12.7 −12.4 |
1.138+0.089 −0.075 |
6000±110 | [57] |
TOI-3919 b | 3.88±0.023 | 1.1±0.05 | 7.433 | 0.0795±0.0016 | 1200±15 | transit | 1973+28.7 −28.4 |
1.208+0.067 −0.07 |
6100±110 | [57] |
TOI-4153 b | 1.15±0.38 | 1.438±0.045 | 4.617 | 0.06311+0.00084 −0.00096 |
1670+30 −40 |
transit | 1366±11.4 | 1.572+0.064 −0.071 |
6860+150 −180 |
[57] |
TOI-4336 Ab | 0.017+0.013 −0.007 |
0.1891 | 16.337 | 0.0872+0.0013 −0.0014 |
308±9 | transit | 73.15 | 0.331±0.015 | 3298+75 −73 |
[60]Located in a triple hierarchical stellar system |
TOI-4438 b | 0.017±0.0035 | 0.2248±0.0116 | 7.44 | 0.0534±0.009 | 400±50 | transit | 98 | 0.368±0.021 | 3422±81 | [61] |
TOI-4633 c | 0.15+0.087 −0.075 |
0.285+0.018 −0.017 |
271.94 | 0.847±0.061 | 290 | transit | 310.4±0.78 | 1.05±0.06 or 1.1±0.06[g] | 5600±50 or 5800±50 [g] | Habitable-zone planet located in a binary star system. The temperature reaches 420 K when the stars are at periastron.[62] |
TOI-5232 b | 2.34±0.16 | 1.14+0.05 −0.045 |
4.097 | 0.0599±0.001 | 1772+40 −45 |
transit | 1985+28 −27 |
1.389+0.068 −0.075 |
6500+180 −190 |
[57] |
TOI-5301 b | 3.65±0.4 | 1.18+0.08 −0.07 |
5.859 | 0.0726+0.0013 −0.0024 |
1655±40 | transit | 1914+59 −55 |
1.483+0.081 −0.14 |
6240±160 | [57] |
TOI-5720 b | 0.0041+0.0029 −0.0015 |
0.0972±0.0062 | 1.434 | 0.0183±0.0003 | 708±19 | transit | 116.9±0.1 | 0.383±0.019 | 3325±75 | [63] |
TOI-6008 b | 0.00346+0.0023 −0.0011 |
0.0919±0.0045 | 0.858 | 0.0108±0.0002 | 707±19 | transit | 75.05±0.03 | 0.23±0.011 | 3075±75 | Ultra-short period planet[63] |
TOI-6086 b | 0.00346+0.00362 −0.00176 |
0.1053±0.0062 | 1.389 | 0.0154±0.0002 | 634±16 | transit | 102.6 | 0.254±0.013 | 3200±75 | [63] |
V808 Aurigae b | 6.8±0.7 | 4109±362 | timing | 698±13 | 0.9±0.1 | [64]The planet's host star is a polar. The mass value for the planet is only a minimum mass. | ||||
VHS J183135.58-551355.9 | 6.5±1.5 | 1.42+0.04 −0.03 |
1085±60 | imaging | 180.6±17.9 | Free-floating planet[65] | ||||
Wolf 327 b | 0.00796±0.00145 | 0.1106±0.0054 | 0.573 | 0.01 | 996±22 | transit | 92.9 | 0.405±0.019 | 3542±70 | [66] Ultra-short period planet |
Specific exoplanet lists[edit]
- 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 hottest exoplanets
- List of coolest exoplanets
- List of multiplanetary systems
- List of nearest exoplanets
- List of nearest terrestrial exoplanet candidates
- List of potentially habitable exoplanets
- List of proper names of exoplanets
- List of smallest exoplanets
- List of transiting exoplanets
Lists of exoplanets by year of discovery[edit]
- List of exoplanets discovered before 2000 (31)
- List of exoplanets discovered between 2000–2009 (378)
- List of exoplanets discovered in 2010 (109)
- List of exoplanets discovered in 2011 (178)
- List of exoplanets discovered in 2012 (149)
- List of exoplanets discovered in 2013 (151)
- List of exoplanets discovered in 2014 (870)
- List of exoplanets discovered in 2015 (150)
- 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 (172)
- List of exoplanets discovered in 2020 (253)
- List of exoplanets discovered in 2021 (257)
- List of exoplanets discovered in 2022 (313)
- List of exoplanets discovered in 2023 (297)
- List of exoplanets discovered in 2024 (88)
Notes[edit]
- ^ a b c Distance calculated from parallax
- ^ The radius is the same as that of the Earth, with an uncertainty of 10%
- ^ Radius calculated with mass and lower limit in density in the equation d=(1.89813*10^(30)*m)/((4/3)*π*r3), where d is density (in g/cm3), m is the mass (in MJ and r is the radius (in centimeters). Should be divided by 7.1492×109 to convert from centimeters to RJ
- ^ Since the density is only a lower limit, the radius is an upper limit.
- ^ The planet is located in a two-star system, with masses of 0.78+0.38
−0.36 M☉ and 0.56+0.3
−0.28 M☉. There is a large chance that it is orbiting both stars in the system, so the "host star mass" would be 0.78+0.38
−0.36 M☉ + 0.56+0.3
−0.28 M☉. However, there is a small chance that is orbiting only one of the stars in the system. - ^ a b c Assuming albedos of 0.3 and 0 respectively.
- ^ a b It is not known which of the stars the planet orbits.
References[edit]
- ^ a b "VizieR".
- ^ Marocco, Federico; Kirkpatrick, J. Davy; Schneider, Adam C.; Meisner, Aaron M.; Popinchalk, Mark; Gelino, Christopher R.; Faherty, Jacqueline K.; Burgasser, Adam J.; Caselden, Dan (22 April 2024), Thirteen New M Dwarf + T Dwarf Pairs Identified with WISE/NEOWISE, arXiv:2404.14324
- ^ "BD-14 3065". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ Šubjak, Ján; Latham, David W.; Quinn, Samuel N.; Berlind, Perry; Calkins, Michael L.; Esquerdo, Gilbert A.; Brahm, Rafael; Guenther, Eike; Janík, Jan (18 March 2024). "BD-14 3065b (TOI-4987b): from giant planet to brown dwarf: evidence for deuterium burning in old age?". arXiv:2403.12311 [astro-ph.EP].
- ^ a b "CI Tau | NASA Exoplanet Archive". exoplanetarchive.ipac.caltech.edu. Retrieved 29 March 2024.
- ^ Martin, Pierre-Yves (2024). "Planet Cl Tau c". exoplanet.eu. Retrieved 29 March 2024.
- ^ a b Cruz-Sáenz de Miera, Fernando; Kóspál, Ágnes; Ábrahám, Péter; Park, Sunkyung; Nagy, Zsófia; Siwak, Michał; Kun, Mária; Fiorellino, Eleonora; Szabó, Zsófia Marianna; Antoniucci, Simone; Giannini, Teresa; Nisini, Brunella; Szabados, László; Kriskovics, Levente; Ordasi, András (1 March 2022). "Recurrent Strong Outbursts of an EXor-like Young Eruptive Star Gaia20eae". The Astrophysical Journal. 927 (1): 125. arXiv:2112.04140. Bibcode:2022ApJ...927..125C. doi:10.3847/1538-4357/ac477f. ISSN 0004-637X.
- ^ Nayakshin, Sergei; de Miera, Fernando Cruz Sáenz; Kóspál, Ágnes (27 April 2024). "The youngest of hot jupiters in action: episodic accretion outbursts in Gaia20eae". Monthly Notices of the Royal Astronomical Society: Letters. 532: L27–L32. arXiv:2405.09904. doi:10.1093/mnrasl/slae034. ISSN 1745-3925.
- ^ Dholakia, Shishir; Palethorpe, Larissa; Venner, Alexander; Mortier, Annelies; Wilson, Thomas G.; Huang, Chelsea X.; Rice, Ken; Van Eylen, Vincent; Nabbie, Emma (21 May 2024), "Gliese 12 b, A Temperate Earth-sized Planet at 12 Parsecs Discovered with TESS and CHEOPS", Monthly Notices of the Royal Astronomical Society, 531 (1): 1276, arXiv:2405.13118, Bibcode:2024MNRAS.531.1276D, doi:10.1093/mnras/stae1152
- ^ Tey, Evan; Shporer, Avi; Lin, Zifan; Stassun, Keivan G.; Lissauer, Jack J.; Hellier, Coel; Collins, Karen A.; Collins, Kevin I.; Wingham, Geof; Relles, Howard M.; Mallia, Franco; Isopi, Giovanni; Kielkopf, John F.; Conti, Dennis M.; Schwarz, Richard P. (24 May 2024). "GJ 238 b: A 0.57 Earth Radius Planet Orbiting an M2.5 Dwarf Star at 15.2 pc". The Astronomical Journal. 167 (6): 283. Bibcode:2024AJ....167..283T. doi:10.3847/1538-3881/ad3df1. ISSN 0004-6256.
- ^ Kirk, James; Stevenson, Kevin B.; Fu, Guangwei; Lustig-Yaeger, Jacob; Moran, Sarah E.; Peacock, Sarah; Alam, Munazza K.; Batalha, Natasha E.; Bennett, Katherine A. (11 January 2024), "JWST/NIRCam Transmission Spectroscopy of the Nearby Sub-Earth GJ 341b", The Astronomical Journal, 167 (3): 90, arXiv:2401.06043, Bibcode:2024AJ....167...90K, doi:10.3847/1538-3881/ad19df
- ^ Capistrant, Benjamin K.; Soares-Furtado, Melinda; Vanderburg, Andrew; Jankowski, Alyssa; Mann, Andrew W.; Ross, Gabrielle; Srdoc, Gregor; Hinkel, Natalie R.; Becker, Juliette (9 January 2024), "TESS Hunt for Young and Maturing Exoplanets (THYME) XI: An Earth-sized Planet Orbiting a Nearby, Solar-like Host in the 400Myr Ursa Major Moving Group", The Astronomical Journal, 167 (2): 54, arXiv:2401.04785, Bibcode:2024AJ....167...54C, doi:10.3847/1538-3881/ad1039
- ^ Sulis, S.; Crossfield, I. J. M.; Santerne, A.; Saillenfest, M.; Sousa, S.; Mary, D.; Aguichine, A.; Deleuil, M.; Mena, E. Delgado (27 May 2024), "A low-mass sub-Neptune planet transiting the bright active star HD 73344", Astronomy & Astrophysics, arXiv:2405.17155, doi:10.1051/0004-6361/202449559
- ^ Palethorpe, L.; John, A. Anna; Mortier, A.; Davoult, J.; Wilson, T. G.; Rice, K.; Cameron, A. C.; Alibert, Y.; Buchhave, L. A. (7 March 2024). "Confronting compositional confusion through the characterisation of the sub-Neptune orbiting HD 77946". Monthly Notices of the Royal Astronomical Society. 529 (4): 3323. arXiv:2403.04464. Bibcode:2024MNRAS.529.3323P. doi:10.1093/mnras/stae707.
- ^ Kane, Stephen R.; Fetherolf, Tara; Li, Zhexing; Polanski, Alex S.; Howard, Andrew W.; Isaacson, Howard; Močnik, Teo; Welter, Sadie G. (25 March 2024). "A Perfect Tidal Storm: HD 104067 Planetary Architecture Creating an Incandescent World". The Astronomical Journal. 167 (5): 239. arXiv:2403.17062. Bibcode:2024AJ....167..239K. doi:10.3847/1538-3881/ad3820.
- ^ a b Li, Zhexing; Kane, Stephen R.; Brandt, Timothy D.; Fetherolf, Tara; Robertson, Paul; Zhao, Jinglin; Dalba, Paul A.; Wittenmyer, Robert A.; Butler, R. Paul (30 January 2024), "Revised Architecture and Two New Super-Earths in the HD 134606 Planetary System", The Astronomical Journal, 167 (4): 155, arXiv:2401.17415, Bibcode:2024AJ....167..155L, doi:10.3847/1538-3881/ad2461
- ^ "HIP 39017 | NASA Exoplanet Archive". exoplanetarchive.ipac.caltech.edu. Retrieved 26 April 2024.
- ^ Tobin, Taylor L.; Currie, Thayne; Li, Yiting; Chilcote, Jeffrey; Brandt, Timothy D.; Lacy, Brianna; Kuzuhara, Masayuki; Vincent, Maria; El Morsy, Mona; Deo, Vincent; Williams, Jonathan P.; Guyon, Olivier; Lozi, Julien; Vievard, Sebastien; Skaf, Nour; Ahn, Kyohoon; Groff, Tyler; Kasdin, N. Jeremy; Uyama, Taichi; Tamura, Motohide; Gibbs, Aidan; Lewis, Briley L.; Bowens-Rubin, Rachel; Salama, Maïssa; An, Qier; Chen, Minghan (9 April 2024). "Direct-imaging Discovery of a Substellar Companion Orbiting the Accelerating Variable Star HIP 39017". The Astronomical Journal. 167 (5): 205. arXiv:2403.04000. Bibcode:2024AJ....167..205T. doi:10.3847/1538-3881/ad3077.
- ^ Tran, Quang H.; Bowler, Brendan P.; Cochran, William D.; Halverson, Samuel; Mahadevan, Suvrath; Ninan, Joe P.; Robertson, Paul; Stefánsson, Guðmundur; Terrien, Ryan C. (4 March 2024). "The Epoch of Giant Planet Migration Planet Search Program. II. A Young Hot Jupiter Candidate around the AB Dor Member HS Psc". The Astronomical Journal. 167 (5): 193. arXiv:2403.02378. Bibcode:2024AJ....167..193T. doi:10.3847/1538-3881/ad2eaf.
- ^ a b c d Shin, In-Gu; Yee, Jennifer C.; Zang, Weicheng; Han, Cheongho; Yang, Hongjing; Gould, Andrew; Lee, Chung-Uk; Udalski, Andrzej; Sumi, Takahiro (8 January 2024), "Systematic KMTNet Planetary Anomaly Search. XI. Complete Sample of 2016 Sub-Prime Field Planets", The Astronomical Journal, 167 (6): 269, arXiv:2401.04256, Bibcode:2024AJ....167..269S, doi:10.3847/1538-3881/ad3ba3
- ^ a b c Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk; Zang, Weicheng; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Hwang, Kyu-Ha; Jung, Youn Kil (16 January 2024). "KMT-2023-BLG-0416, KMT-2023-BLG-1454, KMT-2023-BLG-1642: Microlensing planets identified from partially covered signals". Astronomy and Astrophysics. 683: A187. arXiv:2401.08904. Bibcode:2024A&A...683A.187H. doi:10.1051/0004-6361/202348245.
- ^ a b c Han, Cheongho; Jung, Youn Kil; Bond, Ian A.; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Lee, Chung-Uk; Ryu, Yoon-Hyun (20 January 2024). "MOA-2022-BLG-563Lb, KMT-2023-BLG-0469Lb, and KMT-2023-BLG-0735Lb: Three sub-Jovian-mass microlensing planets". arXiv:2401.11329 [astro-ph.EP].
- ^ Han, Cheongho; et al. (2024). "KMT-2023-BLG-1866Lb: Microlensing super-Earth around an M dwarf host". arXiv:2405.07514v1 [astro-ph.EP].
- ^ Silverstein, Michele L.; Barclay, Thomas; Schlieder, Joshua E.; Collins, Karen A.; Schwarz, Richard P.; Hord, Benjamin J.; Rowe, Jason F.; Kruse, Ethan; Astudillo-Defru, Nicola (29 February 2024). "Validation of a Third Planet in the LHS 1678 System". The Astronomical Journal. 167 (6): 255. arXiv:2403.00110. Bibcode:2024AJ....167..255S. doi:10.3847/1538-3881/ad3040.
- ^ Oliveira, R. A. P.; Ortolani, S.; Barbuy, B.; Kerber, L. O.; Maia, F. F. S.; Bica, E.; Cassisi, S.; Souza, S. O.; Pérez-Villegas, A. (January 2022). "Precise distances from OGLE-IV member RR Lyrae stars in six bulge globular clusters". Astronomy & Astrophysics. 657: A123. arXiv:2110.13943. Bibcode:2022A&A...657A.123O. doi:10.1051/0004-6361/202141596. ISSN 0004-6361.
- ^ Vleeschower, L.; Corongiu, A.; Stappers, B. W.; Freire, P. C. C.; Ridolfi, A.; Abbate, F.; Ransom, S. M.; Possenti, A.; Padmanabh, P. V.; Balakrishnan, V.; Kramer, M.; Krishnan, V. Venkatraman; Zhang, L.; Bailes, M.; Barr, E. D. (1 March 2024). "Discoveries and timing of pulsars in M62". Monthly Notices of the Royal Astronomical Society. 530 (2): 1436–1456. arXiv:2403.12137. Bibcode:2024MNRAS.530.1436V. doi:10.1093/mnras/stae816. ISSN 0035-8711.
- ^ a b https://www.aanda.org/articles/aa/pdf/forth/aa47162-23.pdf
- ^ Gill, Samuel; et al. (2024). "TOI-2447 b / NGTS-29 b: A 69-day Saturn around a Solar analogue". arXiv:2405.07367v1 [astro-ph.EP].
- ^ Battley, M. P.; Collins, K. A.; Ulmer-Moll, S.; Quinn, S. N.; Lendl, M.; Gill, S.; Brahm, R.; Hobson, M. J.; Osborn, H. P. (3 April 2024), NGTS-30 b/TOI-4862 b: An 1 Gyr old 98-day transiting warm Jupiter, arXiv:2404.02974
- ^ a b c Ryu, Yoon-Hyun; Udalski, Andrzej; Yee, Jennifer C.; Zang, Weicheng; Shvartzvald, Yossi; Han, Cheongho; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Jung, Youn Kil; Shin, In-Gu; Yang, Hongjing; Cha, Sang-Mok; Kim, Dong-Jin (1 March 2024). "Systematic KMTNet Planetary Anomaly Search. X. Complete Sample of 2017 Prime-field Planets". The Astronomical Journal. 167 (3): 88. arXiv:2307.13359. Bibcode:2024AJ....167...88R. doi:10.3847/1538-3881/ad1888. ISSN 0004-6256.
- ^ Han, Cheongho; Udalski, Andrzej; Jung, Youn Kil; Gould, Andrew; Kim, Doeon; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Lee, Chung-Uk (12 February 2024). "OGLE-2023-BLG-0836L: The sixth microlensing planet in a binary stellar system". Astronomy and Astrophysics. 685: A16. arXiv:2402.08116. Bibcode:2024A&A...685A..16H. doi:10.1051/0004-6361/202348791.
- ^ Thomas, Luis; Saglia, Roberto; Pasquini, Luca; Brucalassi, Anna; Bonifacio, Piercarlo; de Medeiros, José Renan; Leão, Izan de Castro; Martins, Bruno Leonardo Canto; Ruh, Henrik Lukas (5 March 2024). "Search for giant planets in M 67 V: A warm Jupiter orbiting the turn-off star S1429". Astronomy & Astrophysics. 686: A19. arXiv:2403.02911. Bibcode:2024A&A...686A..19T. doi:10.1051/0004-6361/202449233.
- ^ "The Extrasolar Planet Encyclopaedia — SPECULOOS-3 b". Extrasolar Planets Encyclopaedia. Paris Observatory. Retrieved 15 May 2024.
- ^ Dreizler, S.; Luque, R.; Ribas, I.; Koseleva, V.; Ruh, H. L.; Nagel, E.; Pozuelos, F. J.; Zechmeister, M.; Reiners, A. (1 February 2024). "Teegarden's Star revisited: A nearby planetary system with at least three planets". Astronomy and Astrophysics. 684. arXiv:2402.00923. Bibcode:2024A&A...684A.117D. doi:10.1051/0004-6361/202348033.
- ^ "TIC 4672985". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b Jones, Matias I.; Reinarz, Yared; Brahm, Rafael; Pinto, Marcelo Tala; Eberhardt, Jan; Rojas, Felipe; Triaud, Amaury H. M. J.; Gupta, Arvind F.; Ziegler, Carl (17 January 2024). "A long-period transiting substellar companion in the super-Jupiters to brown dwarfs mass regime and a prototypical warm-Jupiter detected by TESS". Astronomy and Astrophysics. 683: A192. arXiv:2401.09657. Bibcode:2024A&A...683A.192J. doi:10.1051/0004-6361/202348147.
- ^ Peluso, Daniel O’Conner; Dalba, Paul A.; Wright, Duncan; Esposito, Thomas M.; Sgro, Lauren A.; Weaver, Ian C.; Marchis, Franck; Dragomir, Diana; Villanueva, Steven; Fulton, Benjamin; Isaacson, Howard; Gupta, Arvind F.; Jacobs, Thomas Lee; LaCourse, Daryll M.; Gagliano, Robert (March 2024). "Confirming the Warm and Dense Sub-Saturn TIC 139270665 b with the Automated Planet Finder and Unistellar Citizen Science Network". The Astronomical Journal. 167 (4): 170. Bibcode:2024AJ....167..170P. doi:10.3847/1538-3881/ad2772. ISSN 1538-3881.
- ^ a b "TIC 139270665 Overview". NASA Exoplanet Archive. Retrieved 10 May 2024.
- ^ Grunblatt, Samuel K.; Saunders, Nicholas; Huber, Daniel; Thorngren, Daniel; Vissapragada, Shreyas; Yoshida, Stephanie; Schlaufman, Kevin C.; Giacalone, Steven; Macdougall, Mason; Chontos, Ashley; Turtelboom, Emma; Beard, Corey; Murphy, Joseph M. Akana; Rice, Malena; Isaacson, Howard; Angus, Ruth; Howard, Andrew W. (5 June 2024). "TESS Giants Transiting Giants. IV. A Low-density Hot Neptune Orbiting a Red Giant Star". The Astronomical Journal. 168 (1): 1. doi:10.3847/1538-3881/ad4149.
- ^ Sgro, Lauren A.; Dalba, Paul A.; Esposito, Thomas M.; Marchis, Franck; Dragomir, Diana; Villanueva Jr., Steven; Fulton, Benjamin; Billiani, Mario; Loose, Margaret (23 May 2024), Confirmation and Characterization of the Eccentric, Warm Jupiter TIC 393818343 b with a Network of Citizen Scientists, arXiv:2405.15021
- ^ Conzo, G.; Moriconi, M. (26 February 2024). "TOI-6883.01: A Single-transit Planet Candidate Detected from TESS". Research Notes of the AAS. 8 (2): 53. Bibcode:2024RNAAS...8...53C. doi:10.3847/2515-5172/ad2c85. ISSN 2515-5172.
- ^ Mascareño, A. Suárez; Passegger, V. M.; Hernández, J. I. González; Armstrong, D. J.; Nielsen, L. D.; Lovis, C.; Lavie, B.; Sousa, S. G.; Silva, A. M. (6 February 2024). "TESS and ESPRESSO discover a super-Earth and a mini-Neptune orbiting the K-dwarf TOI-238". Astronomy and Astrophysics. 685: A56. arXiv:2402.04113. Bibcode:2024A&A...685A..56S. doi:10.1051/0004-6361/202348958.
- ^ "The Extrasolar Planet Encyclopaedia — TOI-260 b". Extrasolar Planets Encyclopaedia. Paris Observatory.
- ^ "The Extrasolar Planet Encyclopaedia — TOI-329 b". Extrasolar Planets Encyclopaedia. Paris Observatory.
- ^ "The Extrasolar Planet Encyclopaedia — TOI-480 b". Extrasolar Planets Encyclopaedia. Paris Observatory.
- ^ a b c Hori, Y.; Fukui, A.; Hirano, T.; Narita, N.; de Leon, J. P.; Ishikawa, H. T.; Hartman, J. D.; Morello, G.; García, N. Abreu (21 May 2024), The Discovery and Follow-up of Four Transiting Short-period Sub-Neptunes Orbiting M dwarfs, arXiv:2405.12637
- ^ a b Psaridi, Angelica; Osborn, Hugh; Bouchy, François; Lendl, Monika; Parc, Léna; Billot, Nicolas; Broeg, Christopher; Sousa, Sérgio G.; Adibekyan, Vardan (30 January 2024). "Discovery of two warm mini-Neptunes with contrasting densities orbiting the young K3V star TOI-815". Astronomy and Astrophysics. 685: A5. arXiv:2401.15709. Bibcode:2024A&A...685A...5P. doi:10.1051/0004-6361/202348678.
- ^ Mallorquín, M.; Lodieu, N.; Béjar, V. J. S.; Osorio, M. R. Zapatero; Sanz-Forcada, J.; Alarcon, M. R.; Tabernero, H. M.; Nagel, E.; Collins, K. A. (27 February 2024). "TOI-1135 b: A young hot Saturn-size planet orbiting a solar-type star". Astronomy and Astrophysics. 685: A90. arXiv:2402.17448. Bibcode:2024A&A...685A..90M. doi:10.1051/0004-6361/202349016.
- ^ "TYC 4404-396-1". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ Jhon Yana Galarza; Ferreira, Thiago; Lorenzo-Oliveira, Diego; Simon, Joshua D.; Reggiani, Henrique; Piro, Anthony L.; McWilliam, Andrew; Netto, Yuri; Valio, Adriana; Ciardi, David R. (2024). "TOI-1173 A $b$: The First Inflated Super-Neptune in a Wide Binary System". arXiv:2403.06240v1 [astro-ph.EP].
- ^ a b Bell, J. Serrano; Díaz, R. F.; Hébrard, G.; Martioli, E.; Heidari, N.; Sousa, S.; Boisse, I.; Almenara, J. M.; Alonso-Santiago, J. (12 February 2024). "TOI-1199 b and TOI-1273 b: Two new transiting hot Saturns detected and characterized with SOPHIE and TESS". Astronomy & Astrophysics. 684: A6. arXiv:2402.07861. Bibcode:2024A&A...684A...6S. doi:10.1051/0004-6361/202348288.
- ^ a b Rubenzahl, Ryan A.; Dai, Fei; Howard, Andrew W.; Lissauer, Jack J.; Van Zandt, Judah; Beard, Corey; Giacalone, Steven; Murphy, Joseph M. Akana; Chontos, Ashley (12 February 2024). "The TESS-Keck Survey. XII. A Dense 1.8 R🜨 Ultra-Short-Period Planet Possibly Clinging to a High-Mean-Molecular-Weight Atmosphere After the First Gyr". arXiv:2402.07451 [astro-ph.EP].
- ^ a b Hill, Michelle L.; Kane, Stephen R.; Dalba, Paul A.; MacDougall, Mason; Fetherolf, Tara; Li, Zhexing; Pidhorodetska, Daria; Batalha, Natalie M.; Crossfield, Ian J. M. (5 February 2024), "The TESS–Keck Survey. XIX. A Warm Transiting Sub-Saturn-mass Planet and a Nontransiting Saturn-mass Planet Orbiting a Solar Analog", The Astronomical Journal, 167 (4): 151, arXiv:2402.03498, Bibcode:2024AJ....167..151H, doi:10.3847/1538-3881/ad2765
- ^ a b Brady, M.; Bean, J.; Seifahrt, A.; Kasper, D.; Luque, R.; Stefánsson, G.; Stürmer, J.; Charbonneau, D.; Collins, K. (16 May 2024), Early Results from the HUMDRUM Survey: A Small, Earth-mass Planet Orbits TOI-1450A, arXiv:2405.10400
- ^ Desai, Anmol; Turtelboom, Emma V.; Harada, Caleb K.; Dressing, Courtney D.; Rice, David R.; Murphy, Joseph M. Akana; Brinkman, Casey L.; Chontos, Ashley; Crossfield, Ian J. M. (11 February 2024). "The TESS-Keck Survey. XVIII. A sub-Neptune and spurious long-period signal in the TOI-1751 system". The Astronomical Journal. 167 (5): 194. arXiv:2402.07110. Bibcode:2024AJ....167..194D. doi:10.3847/1538-3881/ad29ee.
- ^ Lange, Sarah; Murphy, Joseph M. Akana; Batalha, Natalie M.; Crossfield, Ian J. M.; Dressing, Courtney D.; Fulton, Benjamin; Howard, Andrew W.; Huber, Daniel; Isaacson, Howard; Kane, Stephen R.; Petigura, Erik A.; Robertson, Paul; Weiss, Lauren M.; Behmard, Aida; Beard, Corey (23 May 2024). "The TESS-Keck Survey. VII. A Superdense Sub-Neptune Orbiting TOI-1824*". The Astronomical Journal. 167 (6): 282. Bibcode:2024AJ....167..282L. doi:10.3847/1538-3881/ad34d9. ISSN 1538-3881.
- ^ a b c d e f g h i Schulte, Jack; Rodriguez, Joseph E.; Bieryla, Allyson; Quinn, Samuel N.; Collins, Karen A.; Yee, Samuel W.; Nine, Andrew C.; Soares-Furtado, Melinda; Latham, David W. (11 January 2024), "Migration and Evolution of giant ExoPlanets (MEEP) I: Nine Newly Confirmed Hot Jupiters from the TESS Mission", arXiv:2401.05923 [astro-ph.EP]
- ^ Parviainen, Hannu; Murgas, Felipe; Esparza-Borges, Emma; Peláez-Torres, A.; Palle, Enric; Luque, Rafael; Zapatero-Osorio, M. R.; Korth, Judith; Fukui, Akihiko (22 January 2024). "TOI-2266 b: a keystone super-Earth at the edge of the M dwarf radius valley". Astronomy and Astrophysics. 683: A170. arXiv:2401.11879. Bibcode:2024A&A...683A.170P. doi:10.1051/0004-6361/202347431.
- ^ a b c Eberhardt, Jan; Hobson, Melissa J.; Henning, Thomas; Trifonov, Trifon; Brahm, Rafael; Espinoza, Nestor; Jordán, Andrés; Thorngren, Daniel; Burn, Remo; Rojas, Felipe I.; Sarkis, Paula; Schlecker, Martin; Pinto, Marcelo Tala; Barkaoui, Khalid; Schwarz, Richard P. (27 February 2024). "Three Warm Jupiters around Solar-analog stars detected with TESS". The Astronomical Journal. 166 (6): 271. arXiv:2402.17592. doi:10.3847/1538-3881/ad06bc. ISSN 0004-6256.
- ^ Timmermans, M.; Dransfield, G.; Gillon, M.; Triaud, A. H. M. J.; Rackham, B. V.; Aganze, C.; Barkaoui, K.; Briceño, C.; Burgasser, A. J. (19 April 2024), TOI-4336 A b: A temperate sub-Neptune ripe for atmospheric characterization in a nearby triple M-dwarf system, arXiv:2404.12722
- ^ Martin, Pierre-Yves (2024). "Planet TOI-4438 b". exoplanet.eu. Retrieved 6 March 2024.
- ^ Eisner, Nora L.; Grunblatt, Samuel K.; Barragán, Oscar; Faridani, Thea H.; Lintott, Chris; Aigrain, Suzanne; Johnston, Cole; Mason, Ian R.; Stassun, Keivan G.; Bedell, Megan; Boyle, Andrew W.; Ciardi, David R.; Clark, Catherine A.; Hebrard, Guillaume; Hogg, David W. (1 May 2024). "Planet Hunters TESS V: a planetary system around a binary star, including a mini-Neptune in the habitable zone". The Astronomical Journal. 167 (5): 241. arXiv:2404.18997. Bibcode:2024AJ....167..241E. doi:10.3847/1538-3881/ad1d5c. ISSN 0004-6256.
- ^ a b c Barkaoui, K.; Schwarz, R. P.; Narita, N.; Mistry, P.; Magliano, C.; Hirano, T.; Maity, M.; Burgasser, A. J.; Rackham, B. V. (10 May 2024), Three short-period Earth-sized planets around M dwarfs discovered by TESS: TOI-5720b, TOI-6008b and TOI-6086b, arXiv:2405.06350
- ^ Leichty, McKenna; Garnavich, Peter; Littlefield, Colin; Schwope, Axel D.; Kurpas, Jan; Mason, Paul A.; Beuermann, Klaus (26 February 2024). "An Eccentric Planet Orbiting the Polar V808 Aurigae". The Astrophysical Journal. 967 (2): 81. arXiv:2402.16959. Bibcode:2024ApJ...967...81L. doi:10.3847/1538-4357/ad3bac.
- ^ Bickle, Thomas P.; Schneider, Adam C.; Gagné, Jonathan; Faherty, Jacqueline K.; Rothermich, Austin; Vos, Johanna M.; Suárez, Genaro; Kirkpatrick, J. Davy; Meisner, Aaron M. (6 May 2024), Discovery of the Remarkably Red L/T Transition Object VHS J183135.58-551355.9, arXiv:2405.03849
- ^ Murgas, F.; Pallé, E.; Orell-Miquel, J.; Carleo, I.; Peña-Moñino, L.; Pérez-Torres, M.; Watkins, C. N.; Jeffers, S. V.; Azzaro, M. (22 January 2024). "Wolf 327b: A new member of the pack of ultra-short-period super-Earths around M dwarfs". Astronomy and Astrophysics. 684: A83. arXiv:2401.12150. Bibcode:2024A&A...684A..83M. doi:10.1051/0004-6361/202348813.