List of exoplanets discovered by the TESS mission

The list of exoplanets detected by the Transiting Exoplanet Survey Satellite (TESS) contains bodies with a wide variety of properties, with significant ranges in orbital distances, masses, radii, composition, habitability, and host star type. As of 17 September 2025, the TESS Mission has detected 8,361 planets and confirmed 693 planets, including hot Jupiters, super-Earths, circumbinary planets, and planets located in the circumstellar habitable zones of their host stars.[1] TESS has detected over 7,668 unconfirmed planet candidates.

Table

Name Mass (MJ) Radius (RJ) Period (days) Semi-major axis (AU) Temp. (K) Discovery method Distance (ly) Host star Host star mass (M) Host star temp. (K) Year of Discovery Remarks
Earth (for reference) Sun [2]
TESS Object of Interest (TOI)
TOI 122 b 0.028+0.029
−0.010
0.243±0.016 5.078030±0.000015 0.0392±0.0007 471 transit 202.9±0.7 TOI-122 0.312±0.007 3403±100 2020 [3]
TOI-125 b 0.0299±0.00277 0.2432±0.00669 4.65382±0.00033 0.05186+0.00086
−0.00077
1037±11 transit 363.3382±1.435088 TOI-125 0.859+0.044
−0.038
5320±39 2019 [4]
TOI-125 c 0.02086±0.00311 0.24614±0.009 9.15059+0.0007
−0.00082
0.814±0.0013 827.8±8.6 transit 363.3382±1.435088 0.859+0.044
−0.038
5320±39 [4]
TOI-125 d 0.0428±0.0038 0.2614±0.0152 19.98+0.005
−0.0056
0.05186+0.00086
−0.00077
638.1±6.6 transit 363.3382±1.435088 0.859+0.044
−0.038
5320±39 [5][4]
TOI-132 b 0.07048+0.00598
−0.00604
0.305±0.012 2.1097019+0.000012
−0.000011
0.026+0.002
−0.003
1395+52
−72
transit 536.43±89.11 TOI-132 0.970±0.06 5397±46 2020 [6]
TOI-150 b 1.75+0.14
−0.17
1.38±0.04 5.857342+0.000065
−0.000066
0.0583+0.0013
−0.0018
1493+29
−32
transit 1095.89±6.52 TO-150 1.25+0.07
−0.12
6003+104
−98
2019 [7]
TOI-157 b 1.18±0.13 1.29±0.02 2.0845435±0.0000023 0.03138+0.00025
−0.00020
1588+21
−20
transit 1171 TOI-157 0.948+0.023
−0.018
5404+70
−67
2020 [4]
TOI-163b 1.22 1.489 4.231306 0.0580 1669 transit 1359 TOI-163 1.44 6495 2019 [7]
TOI-172b 5.42+0.22
−0.20
0.965+0.032
−0.029
9.47725+0.00064
−0.00079
0.0914±0.0017 transit 1097.418 TOI-172 1.128+0.065
−0.061
5645±50 2019 [8]
TOI-175b 0.00126+0.00050
−0.00048
0.0642+0.0046
−0.0035
2.2531136+0.0000012
−0.0000015
0.02191+0.00080
−0.00084
627+33
−36
transit 34.636±0.010 L 98-59 0.273±0.030 3415±135 2019 [9]To date, it is the lowest mass planet confirmed, or measured, using the radial velocity technique.[10] Host star also known as L 98-59.[11]
GJ 3090 b (TOI-177 b) 0.0105 0.19 2.8531042±0.0000032 0.03165 696 transit 73.21±0.04 TOI-177 0.519±0.013 3556±70 2022 [12]
HD 21749 b (TOI-186 b) 0.073+0.007
−0.006
0.254+0.023
−0.020
35.61253+0.00060
−0.00062
0.1915+0.0058
−0.0063
422+15
−14
transit 53.261±0.023 HD 21749 0.73±0.07 4640±100 2019 [13]
HD 21749 c (TOI-186 c) <0.0116 0.0796+0.0057
−0.0052
7.78993+0.00051
−0.00044
0.0695+0.0021
−0.0023
701+25
−23
transit 53.261±0.023 0.73±0.07 4640±100 [13]
DS Tucanae Ab (TOI-200 b) 0.509±0.015 8.138268±0.000011 850 transit 143.89±0.22 DS Tucanae 1.01±0.06 5428±80 2019 [14]
TOI-201 c 14.2±2.0 0.99±0.017 2,800+360
−210
4.28+0.36
−0.2
timing + transit 372.5 TOI-201 1.316±0.027 6,394±75 2025 [15]
TOI-216 b 0.059±0.002 0.714+0.268
−0.179
17.1607 0.1293+0.0067
−0.0051
628+13
−11
transit 583±3 TOI-216 0.77 5026±125 2019 Semi-major axes are strongly variable due to planet-planet interaction on a timescale of few years[16][17][18]
TOI-216 c 0.56±0.02 0.902±0.018 34.525528 0.2069+0.0107
−0.0082
497+10
−8
transit 583±3 0.77 5026±125
TOI-237 c 0.1076±0.0031 1.74486147 0.0160+0.0005
−0.0006
515+11
−8
transit 124.86 TOI-237 0.1698+0.0385
−0.0350
3226+47
−48
2026 [19]
TOI-333 b 0.0632±0.0076 0.3801±0.0098 3.785250±0.000006 0.049±0.001 1445 transit 1132 TOI-333 1.2±0.1 6,241±73 2025 [20]
Gliese 238 b (TOI-486 b) 0.05049±0.0012 1.74 0.02123+0.00016
−0.00017
758+16
−15
transit 49.6 Gliese 238 0.419±0.01 3485±140 2024 Mars-sized exoplanet, one of the smallest exoplanets currently known[21]
TOI-270b 0.0050 0.1112 3.360080 0.0306 528 transit 73.23 TOI-270 0.40 3386 2019 [22][23]
TOI-270c 0.0193 0.216 5.660172 0.0472 424 transit 73.23 0.40 3386 [22][23]
TOI-270d 0.0150 0.190 11.38014 0.0733 340 transit 73.23 0.40 3386 [22][23]Hydrogen and steam atmosphere[24]
NGTS-6b (TOI-448 b) 1.339 1.326 0.8820590 0.01677 transit 1010 NGTS-6 0.77 4730 2019 [25]
GJ 3473 b (TOI-488 b) 0.0059±0.0009 0.113+0.0045
−0.0044
1.1980035+0.0000018
−0.0000019
0.01589±0.00062 773+16
−15
transit 89.29±0.13 GJ 3473 0.360±0.016 3347±54 2020 Potentially rocky world, larger than Earth, also called TOI-488 b[26]
GJ 3473 c (TOI-488 c) 0.0233+0.0029
−0.0027
0.235 15.509±0.033 0.0876+0.0035
−0.0034
329.1+6.6
−6.4
radial vel. 89.29±0.13 0.360±0.016 3347±54 Neptune-like ice giant also called TOI-488 c[26][27][28]
TOI-512 b 0.01123+0.00167
−0.00173
0.1374±0.0089 7.18886+0.000069
−0.000077
1,009±29 transit 219.16±0.14 TOi-512 0.74±0.03 5,277±67 2025 [29]
TOI-561 b 0.0050±0.0011 0.127±0.006 0.446578±0.000017 0.01055±0.00008 transit 279.2±1.6 TOI-561 0.785±0.018 5455+65
−47
2020 [30][31]
TOI-561 c 0.017±0.003 0.257±0.009 10.779±0.004 0.08809±0.0007 transit 279.2±1.6 0.785±0.018 5455+65
−47
[30][31]
TOI-561 d 0.038±0.004 0.226±0.011 25.62±0.04 0.1569±0.0012 transit 279.2±1.6 0.785±0.018 5455+65
−47
[30][31]
TOI-561 e 0.050±0.007 0.238±0.010 77.23±0.39 0.3274+0.0028
−0.0027
transit 279.2±1.6 0.785±0.018 5455+65
−47
[30]
TOI-564b 1.463+0.10
−0.096
1.02+0.71
−0.29
1.651144±0.000018 0.02734+0.00061
−0.00053
1714+20
−21
transit 643.8±5.9 TOI-564 0.998+0.068
−0.057
5640+34
−37
2019 [32]
TOI-700 b 0.00406+0.003
−0.00116
0.0901+0.00839
−0.00776
9.97701+0.00024
−0.00028
0.0637+0.0064
−0.006
transit 101.5 TOI-700 0.416±0.01 3480±135 2020 [33]
TOI-700 c 0.0249+0.0085
−0.0057
0.2346+0.0214
−0.0205
16.051998+0.000089
−0.000092
0.0925+0.0088
−0.0083
transit 101.5 0.416±0.01 3480±135 [33]
TOI-700 d 0.00711+0.0022
−0.00164
0.1062±0.0098 37.426+0.0007
−0.001
0.163±0.015 295±55 transit 101.5 0.416±0.01 3480±135 First "Earth sized" discovered by TESS[33][34]
TOI-771 c 0.00903 7.61 0.046±0.002 365 radial vel. 82.45 TOI-771 0.22±0.024 3,201±100 2025 [35]
TOI-905b 0.667+0.042
−0.041
1.171+0.052
−0.051
3.739494±0.000038 0.04666+0.00096
−0.0011
1192+39
−36
transit 489.9+23.5
−22.5
TOI-905 0.968+0.061
−0.068
5570+150
−140
2019 [32]
TOI-1117 b 0.028±0.003 0.219+0.012
−0.011
2.22816±0.00001 0.0330±0.0002 1,538±21 transit 546.64±2.94 TOI-1117 0.97±0.02 5,635±62 2025 [36]
TOI-1117 c 0.0276+0.0037
−0.0038
4.579±0.004 0.0534±0.0003 1,210±16 radial vel.
TOI-1117 d 0.0337±0.0050 8.665±0.011 0.0817±0.0006 978±13 radial vel.
TOI-1243 b 0.0242±0.0047 0.2079±0.0107 4.65948 0.0437±0.0001 450 transit 140.6 TOI-1243 0.515±0.027 3,515±79 2026 [37]
TOI-3862 b 0.1688+0.0087
−0.0090
0.493±0.016 1.55745774 0.02539+0.00064
−0.00068
1539 transit 801.2 TOI-3861 0.90±0.07 5300±50 2026 [38]
TOI-4336 Ac 0.1039+0.0054
−0.0052
7.587270 0.0481±0.0027 378±12 transit 73.23 TOI-4336 0.2853+0.0438
−0.0356
3369+51
−57
2026 [19]
TOI-4495 b 0.024+0.004
−0.05
0.221+0.012
−0.008
2.56699 0.03957±0.00047 1735 transit 801.2 TOI-4495 1.247±0.045 6210±70 2026 [39]
TOI-4529 b 0.0154 0.1579±0.008 5.87958 0.04997±0.0008 511 transit 92.6 TOI-4529 0.482±0.023 3,697±71 2026 [37]
BD-14 3065 b (TOI-4987 b) 12.11+0.95
−0.91
1.926±0.094 4.3 0.0646±0.0026 3520±130 transit 1847.4[40][a] BD-14 3065 1.4±0.06 6985±90 2024 Located in a triple star system. It orbits the primary component of the system (BD-14 3065 A), a subgiant star. Also known as TOI-4987 b[41]
TOI-5788 b 0.0117±0.0030 0.1365±0.0067 6.340758 0.0640±0.0011 transit 318.2 TOI-5788 0.87±0.04 5615±25 2026 [42]
TOI-5788 c 0.0201±0.0038 0.2025±0.0036 16.213358 0.1197±0.0020 transit
Gliese 12 b (TOI-6251 b) 0.002769+0.00123
−0.0008
0.0892±0.0089[b] 12.7 0.066±0.002 315±5 transit 39.65 Gliese 12 0.241±0.006 3253±55 2024 [43]
HD 101581 b (TOI-6276 b) 0.0877 4.47 transit 41.7 HD 101581 0.740±0.087 4675±53 2024 Host star is the brightest star with multiple known transiting Earth-size exoplanets. Another transiting planet in the system is suspected.[44]
HD 101581 c (TOI-6276 c) 0.0925 6.21 transit 41.7 0.740±0.087 4675±53
TOI-6716 b 0.0874±0.0062 4.71859 0.032±0.003 369 transit 61.6 TOI-6716 0.223±0.011 3,110±80 2026 [45]
TOI-7384 b 0.3176±0.0187 6.23403 0.0439±0.004 378 transit 218 TOI-7384 0.318±0.016 3,185±75 2026 [45]
TESS Input Catalog (TIC)
TIC 237913194b 1.942+0.092
−0.091
1.117+0.054
−0.047
15.168865±0.000018 0.1207±0.0037 974 transit 1009±6 TIC 237913194 1.026+0.057
−0.055
5788±80 2020 Very eccentric orbit[46]
BD+05 4868 Ab (TIC 466376085 b) 0.000063 0.028 1.27187 0.0208±0.0003 1,820±45 transit 142.4±0.1 BD+05 4868 0.70±0.02 4,596+65
−64
2025 A disintegrating planet with a comet-like tail.[47]
TIC 88785435 b 0.449±0.019 10.508843 0.08432±0.00068 635±16 transit 398.2±0.8 TIC 88785435 0.724±0.017 3,998±95 2025 [48]

See also

Notes

  1. ^ Cite error: The named reference distp was invoked but never defined (see the help page).
  2. ^ The radius is the same as that of the Earth, with an uncertainty of 10%

Reference

  1. ^ "Exoplanet and Candidate Statistics". exoplanetarchive.ipac.caltech.edu. Retrieved 2025-09-24.
  2. ^ NASA. "Jupiter Fact Sheet". NASA. Archived from the original on 2011-09-26. Retrieved 2013-03-31.
  3. ^ Waalkes, William C.; et al. (2021), "TOI 122b and TOI 237b: Two Small Warm Planets Orbiting Inactive M Dwarfs Found by TESS", The Astronomical Journal, 161 (1): 13, arXiv:2010.15905, Bibcode:2021AJ....161...13W, doi:10.3847/1538-3881/abc3b9, S2CID 226221997
  4. ^ a b c d Nielsen, L. D.; Gandolfi, D.; Armstrong, D. J.; Jenkins, J. S.; Fridlund, M.; Santos, N. C.; Dai, F.; Adibekyan, V.; Luque, R.; Steffen, J. H.; Esposito, M.; Meru, F.; Sabotta, S.; Bolmont, E.; Kossakowski, D.; Otegi, J. F.; Murgas, F.; Stalport, M.; Rodler, F.; Díaz, M. R.; Kurtovic, N. T.; Ricker, G.; Vanderspek, R.; Latham, D. W.; Seager, S.; Winn, J. N.; Jenkins, J. M.; Allart, R.; Almenara, J. M.; et al. (2020). "Mass determinations of the three mini-Neptunes transiting TOI-125". Monthly Notices of the Royal Astronomical Society. 492 (4): 5399. arXiv:2001.08834. Bibcode:2020MNRAS.492.5399N. doi:10.1093/mnras/staa197.
  5. ^ "exoplanet.eu toi-125_d". Extrasolar Planets Encyclopaedia.
  6. ^ TOI-132 b
  7. ^ a b Kossakowski, Diana; et al. (2019), "TOI-150b and TOI-163b: Two transiting hot Jupiters, one eccentric and one inflated, revealed by TESS near and at the edge of the JWST CVZ", Monthly Notices of the Royal Astronomical Society, 490: 1094–1110, arXiv:1906.09866, doi:10.1093/mnras/stz2433
  8. ^ Rodriguez, Joseph E.; et al. (2019), "An Eccentric Massive Jupiter Orbiting a Subgiant on a 9.5-day Period Discovered in the Transiting Exoplanet Survey Satellite Full Frame Images", The Astronomical Journal, 157 (5): 191, arXiv:1901.09950, Bibcode:2019AJ....157..191R, doi:10.3847/1538-3881/ab11d9, S2CID 119314505
  9. ^ Kostov, Veselin B.; Schlieder, Joshua E.; Barclay, Thomas; Quintana, Elisa V.; Colón, Knicole D.; Brande, Jonathan; Collins, Karen A.; Feinstein, Adina D.; Hadden, Samuel; Kane, Stephen R.; Kreidberg, Laura; Kruse, Ethan; Lam, Christopher; Matthews, Elisabeth; Montet, Benjamin T. (2019-06-27). "The L 98-59 System: Three Transiting, Terrestrial-size Planets Orbiting a Nearby M Dwarf". The Astronomical Journal. 158 (1): 32. arXiv:1903.08017. Bibcode:2019AJ....158...32K. doi:10.3847/1538-3881/ab2459. ISSN 1538-3881.
  10. ^ Demangeon, O. D. S.; Zapatero Osorio, M. R.; Alibert, Y.; Barros, S. C. C.; Adibekyan, V.; Tabernero, H. M.; Antoniadis-Karnavas, A.; Camacho, J. D.; al, et (2021). "Warm terrestrial planet with half the mass of Venus transiting a nearby star" (PDF). Astronomy & Astrophysics. 653: A41. arXiv:2108.03323. Bibcode:2021A&A...653A..41D. doi:10.1051/0004-6361/202140728. S2CID 236957385.
  11. ^ "Planet L 98-59 b". Extrasolar Planets Encyclopaedia. 1995. Retrieved 6 August 2021.
  12. ^ Almenara, J. M.; et al. (2022), "GJ 3090 b: One of the most favourable mini-Neptune for atmospheric characterisation", Astronomy & Astrophysics, 665: A91, arXiv:2207.14121, Bibcode:2022A&A...665A..91A, doi:10.1051/0004-6361/202243975, S2CID 252367299
  13. ^ a b Dragomir, Diana; et al. (2019), "TESS Delivers Its First Earth-sized Planet and a Warm Sub-Neptune", The Astrophysical Journal, 875 (2): L7, arXiv:1901.00051, Bibcode:2019ApJ...875L...7D, doi:10.3847/2041-8213/ab12ed, S2CID 129945503
  14. ^ Benatti, S.; Nardiello, D.; Malavolta, L.; Desidera, S.; Borsato, L.; Nascimbeni, V.; Damasso, M.; D'Orazi, V.; Mesa, D.; Messina, S.; Esposito, M.; Bignamini, A.; Claudi, R.; Covino, E.; Lovis, C.; Sabotta, S. (October 2019). "A possibly inflated planet around the bright young star DS Tucanae A". Astronomy & Astrophysics. 630: A81. arXiv:1904.01591. Bibcode:2019A&A...630A..81B. doi:10.1051/0004-6361/201935598. ISSN 0004-6361. S2CID 102486551.
  15. ^ Maciejewski, Gracjan; Łoboda, Weronika (2025). "A Transiting Giant on a 7.7 yr Orbit Revealed by Transit Timing Variations in the TOI-201 System". The Astrophysical Journal Letters. 988 (2): L63. arXiv:2507.11504. Bibcode:2025ApJ...988L..63M. doi:10.3847/2041-8213/adefe5.
  16. ^ Teachey, Alex; Jansen, Tiffany; Bakos, Gaspar; Torres, Guillermo; Hartman, Joel; Nesvorný, David; Kipping, David (2019). "A resonant pair of warm giant planets revealed by TESS". Monthly Notices of the Royal Astronomical Society. 486 (4): 4980–4986. arXiv:1902.03900. doi:10.1093/mnras/stz1141.
  17. ^ Dawson, Rebekah I.; et al. (2019). "TOI-216b and TOI-216 c: Two Warm, Large Exoplanets in or Slightly Wide of the 2:1 Orbital Resonance". The Astronomical Journal. 158 (2): 65. arXiv:1904.11852. Bibcode:2019AJ....158...65D. doi:10.3847/1538-3881/ab24ba. S2CID 135466349.
  18. ^ Dawson, Rebekah I.; Huang, Chelsea X.; Brahm, Rafael; Collins, Karen A.; Hobson, Melissa J.; Jordán, Andrés; Dong, Jiayin; Korth, Judith; Trifonov, Trifon; Abe, Lyu; Agabi, Abdelkrim; Bruni, Ivan; Butler, R. Paul; Barbieri, Mauro; Collins, Kevin I.; Conti, Dennis M.; Crane, Jeffrey D.; Crouzet, Nicolas; Dransfield, Georgina; Evans, Phil; Espinoza, Néstor; Gan, Tianjun; Guillot, Tristan; Henning, Thomas; Lissauer, Jack J.; Jensen, Eric L. N.; Sainte, Wenceslas Marie; Mékarnia, Djamel; Myers, Gordon; et al. (2021), "Precise transit and radial-velocity characterization of a resonant pair: a warm Jupiter TOI-216c and eccentric warm Neptune TOI-216b", The Astronomical Journal, 161 (4): 161, arXiv:2102.06754, Bibcode:2021AJ....161..161D, doi:10.3847/1538-3881/abd8d0, S2CID 231924886
  19. ^ a b Timmermans, M.; et al. (2026-01-29). "Hidden Gems in TESS: sherlock finds two new rocky planets around nearby M dwarfs". arXiv:2601.21774 [astro-ph.EP].
  20. ^ Alves, Douglas R.; et al. (2026). "TOI-333b: A Neptune-desert planet around an F7V star". Astronomy & Astrophysics. 705: A210. arXiv:2511.13832. Bibcode:2026A&A...705A.210A. doi:10.1051/0004-6361/202557014.
  21. ^ 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. (2024-05-24). "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. arXiv:2407.18199. Bibcode:2024AJ....167..283T. doi:10.3847/1538-3881/ad3df1. ISSN 0004-6256.
  22. ^ a b c "太陽系外惑星「TOI 270 b、c、d」を発見。地球外生命体の存在は?". sorae. 2019-07-30. Retrieved 2021-01-08.
  23. ^ a b c Van Eylen, Vincent; Astudillo-Defru, Nicola; Bonfils, Xavier; Livingston, J.; Hirano, T.; Luque, Rafael; Lam, K. W. F.; Justesen, A. B.; Winn, J. N.; Gandolfi, D.; Nowak, G.; Palle, E.; Albrecht, S.; Dai, F.; Campos Estrada, B.; Owen, J. E.; Foreman-Mackey, D.; Fridlund, M.; Korth, J.; Mathur, S.; Forveille, Thierry; Mikal-Evans, T.; Osborne, H. L. M.; Ho, C. S. K.; Almenara, José M.; Artigau, Étienne; Barragán, O.; Bouchy, François; Cabrera, J.; et al. (2021), "Masses and compositions of three small planets orbiting the nearby M dwarf L231-32 (TOI-270) and the M dwarf radius valley", Monthly Notices of the Royal Astronomical Society stab2143, arXiv:2101.01593, doi:10.1093/mnras/stab2143
  24. ^ Mikal-Evans, Thomas; Madhusudhan, Nikku; Dittmann, Jason; Guenther, Maximilian N.; Welbanks, Luis; Vincent Van Eylen; Crossfield, Ian J. M.; Daylan, Tansu; Kreidberg, Laura (2023), "Hubble Space Telescope Transmission Spectroscopy for the Temperate Sub-Neptune TOI-270 d: A Possible Hydrogen-rich Atmosphere Containing Water Vapor", The Astronomical Journal, 165 (3): 84, arXiv:2211.15576, Bibcode:2023AJ....165...84M, doi:10.3847/1538-3881/aca90b, S2CID 254044155
  25. ^ Vines, Jose I.; et al. (2019), "NGTS-6b: An ultrashort period hot-Jupiter orbiting an old K dwarf", Monthly Notices of the Royal Astronomical Society, 489 (3): 4125–4134, arXiv:1904.07997, doi:10.1093/mnras/stz2349
  26. ^ a b Kemmer, J.; et al. (2020), "Discovery of a hot, transiting, Earth-sized planet and a second temperate, non-transiting planet around the M4 dwarf GJ 3473 (TOI-488)", Astronomy & Astrophysics, 642: A236, arXiv:2009.10432, Bibcode:2020A&A...642A.236K, doi:10.1051/0004-6361/202038967, S2CID 221836679
  27. ^ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. 22 October 2020. Retrieved 2023-11-25.
  28. ^ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. 14 February 2020. Retrieved 2023-11-25.
  29. ^ Rodrigues, J.; et al. (2025-02-20). "TOI-512: Super-Earth transiting a K-type star discovered by TESS and ESPRESSO". Astronomy and Astrophysics. 695: A237. arXiv:2502.14472. Bibcode:2025A&A...695A.237R. doi:10.1051/0004-6361/202452887.
  30. ^ a b c d Lacedelli, G.; et al. (2021), "An unusually low density ultra-short period super-Earth and three mini-Neptunes around the old star TOI-561", Monthly Notices of the Royal Astronomical Society, 501 (3): 4148–4166, arXiv:2009.02332, doi:10.1093/mnras/staa3728
  31. ^ a b c Weiss, Lauren M.; et al. (2021), "The TESS-Keck Survey. II. An Ultra-short-period Rocky Planet and Its Siblings Transiting the Galactic Thick-disk Star TOI-561", The Astronomical Journal, 161 (2): 56, arXiv:2009.03071, Bibcode:2021AJ....161...56W, doi:10.3847/1538-3881/abd409, S2CID 229279232
  32. ^ a b Davis, Allen B.; Wang, Songhu; et al. (2020). "TOI 564 b and TOI 905 b: Grazing and Fully Transiting Hot Jupiters Discovered by TESS". Astronomical Journal. 160 (5): 229. arXiv:1912.10186. Bibcode:2020AJ....160..229D. doi:10.3847/1538-3881/aba49d. hdl:1721.1/134083. S2CID 209444463.
  33. ^ a b c Gilbert, Emily A.; Barclay, Thomas; Schlieder, Joshua E.; Quintana, Elisa V.; Hord, Benjamin J.; Kostov, Veselin B.; Lopez, Eric D.; Rowe, Jason F.; Hoffman, Kelsey; Walkowicz, Lucianne M.; Silverstein, Michele L.; Rodriguez, Joseph E.; Vanderburg, Andrew; Suissa, Gabrielle; Airapetian, Vladimir S.; Clement, Matthew S.; Raymond, Sean N.; Mann, Andrew W.; Kruse, Ethan; Lissauer, Jack J.; Colón, Knicole D.; Ravi kumar Kopparapu; Kreidberg, Laura; Zieba, Sebastian; Collins, Karen A.; Quinn, Samuel N.; Howell, Steve B.; Ziegler, Carl; Eliot Halley Vrijmoet; et al. (2020). "The First Habitable-zone Earth-sized Planet from TESS. I. Validation of the TOI-700 System". The Astronomical Journal. 160 (3): 116. arXiv:2001.00952. Bibcode:2020AJ....160..116G. doi:10.3847/1538-3881/aba4b2. S2CID 209862554.
  34. ^ Suissa, Gabrielle; Wolf, Eric T.; Ravi kumar Kopparapu; Villanueva, Geronimo L.; Fauchez, Thomas; Mandell, Avi M.; Arney, Giada; Gilbert, Emily A.; Schlieder, Joshua E.; Barclay, Thomas; Quintana, Elisa V.; Lopez, Eric; Rodriguez, Joseph E.; Vanderburg, Andrew (2020). "The First Habitable-zone Earth-sized Planet from TESS. III. Climate States and Characterization Prospects for TOI-700 D". The Astronomical Journal. 160 (3): 118. arXiv:2001.00955. Bibcode:2020AJ....160..118S. doi:10.3847/1538-3881/aba4b4. S2CID 209862275.
  35. ^ Lacedelli, G.; Pallé, E.; Davis, Y. T.; Luque, R.; Morello, G.; Tabernero, H. M.; Zapatero Osorio, M. R.; Pozuelos, F. J.; Jankowski, D.; Nowak, G.; Murgas, F.; Orell-Miquel, J.; Akana Murphy, J. M.; Barkaoui, K.; Charbonneau, D.; Dransfield, G.; Ducrot, E.; Geraldía-González, S.; Irwin, J.; Jehin, E.; Osborne, H. L. M.; Pedersen, P. P.; Rackham, B. V.; Scott, M. G.; Timmermans, M.; Triaud, A.; Van Eylen, V. (2025). "A transiting rocky super-Earth and a non-transiting sub-Neptune orbiting the M dwarf TOI-771". Astronomy & Astrophysics. 698: A223. arXiv:2504.18223. Bibcode:2025A&A...698A.223L. doi:10.1051/0004-6361/202554161.
  36. ^ Lockley, Isobel S.; Armstrong, David J.; Fernández, Jorge Fernández; Millholland, Sarah; Knierim, Henrik; Mena, Elisa Delgado; Sousa, Sergio; Collins, Karen A.; Watkins, Cristilyn N.; Howell, Steve B.; Adibekyan, Vardan; Helled, Ravit; Ziegler, Carl; Bayliss, Daniel; Briceño, César (June 2025). "The TOI-1117 Multi-planetary System: 3 sub-Neptunes, 1 in both the Neptunian Desert and Radius Valley". Monthly Notices of the Royal Astronomical Society. 541 (2): 919–938. arXiv:2506.05521. Bibcode:2025MNRAS.541..919L. doi:10.1093/mnras/staf939. ISSN 0035-8711.
  37. ^ a b Poultourtzidis, E.; et al. (2026). "Characterization of two new transiting sub-Neptunes and a terrestrial planet around M-dwarf hosts". arXiv:2601.07414 [astro-ph.EP].
  38. ^ Carleo, Ilaria; Castro-González, Amadeo; Pallé, Enric; et al. (2026-01-15). "TOI-3862 b: A dense super-Neptune deep in the hot Neptune desert". arXiv:2601.10450v1 [astro-ph.EP].
  39. ^ Wang, Mu-Tian; Dai, Fei; Liu, Hui-Gen; et al. (2026-01-06). "TOI-4495: A Pair of Aligned, Near-Resonant Sub-Neptunes that Likely Experienced Overstable Migration". arXiv:2601.02665v1 [astro-ph.EP].
  40. ^ "BD-14 3065". SIMBAD. Centre de données astronomiques de Strasbourg.
  41. ^ Šubjak, Ján; Latham, David W.; Quinn, Samuel N.; Berlind, Perry; Calkins, Michael L.; Esquerdo, Gilbert A.; Brahm, Rafael; Guenther, Eike; Janík, Jan (2024-03-18). "Evolution of BD-14 3065b (TOI-4987b) from giant planet to brown dwarf as possible evidence of deuterium burning at old stellar ages". Astronomy & Astrophysics. 688: A120. arXiv:2403.12311. Bibcode:2024A&A...688A.120S. doi:10.1051/0004-6361/202349028.
  42. ^ Lakeland, Ben S.; Mortier, A.; Haywood, R. D.; et al. (2026-01-20). "Discovery and characterisation of two exoplanets orbiting the metal-poor, solar-type star TOI-5788 with TESS, CHEOPS, and HARPS-N". Monthly Notices of the Royal Astronomical Society stag158. arXiv:2601.14045v1. Bibcode:2026MNRAS.tmp..146L. doi:10.1093/mnras/stag158.{{cite journal}}: CS1 maint: bibcode (link)
  43. ^ Dholakia, Shishir; Palethorpe, Larissa; Venner, Alexander; Mortier, Annelies; Wilson, Thomas G.; Huang, Chelsea X.; Rice, Ken; Van Eylen, Vincent; Nabbie, Emma (2024-05-21). "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.
  44. ^ Kunimoto, Michelle; Lin, Zifan; Millholland, Sarah; Venner, Alexander; Hinkel, Natalie R.; Shporer, Avi; Vanderburg, Andrew; Bailey, Jeremy; Brahm, Rafael (December 2024), "Two Earth-size Planets and an Earth-size Candidate Transiting the Nearby Star HD 101581", The Astronomical Journal, 169 (1): 47, arXiv:2412.08863, Bibcode:2025AJ....169...47K, doi:10.3847/1538-3881/ad9266
  45. ^ a b Scott, Madison G.; et al. (2026). "Two temperate Earth- and Neptune-sized planets orbiting fully convective M dwarfs". Monthly Notices of the Royal Astronomical Society stag070. arXiv:2601.05799. Bibcode:2026MNRAS.tmp...63S. doi:10.1093/mnras/stag070.{{cite journal}}: CS1 maint: bibcode (link)
  46. ^ Schlecker, Martin; et al. (2020), "A Highly Eccentric Warm Jupiter Orbiting TIC 237913194", The Astronomical Journal, 160 (6): 275, arXiv:2010.03570, Bibcode:2020AJ....160..275S, doi:10.3847/1538-3881/abbe03, S2CID 222208966
  47. ^ Hon, Marc; Rappaport, Saul; Shporer, Avi; Vanderburg, Andrew; Collins, Karen A.; Watkins, Cristilyn N.; Schwarz, Richard P.; Barkaoui, Khalid; Yee, Samuel W. (2025-01-09). "A Disintegrating Rocky Planet with Prominent Comet-like Tails Around a Bright Star". The Astrophysical Journal. 984 (1): L3. arXiv:2501.05431. Bibcode:2025ApJ...984L...3H. doi:10.3847/2041-8213/adbf21.
  48. ^ Vach, Sydney; et al. (2025-02-01). "A 16 Myr super-Neptune in Upper-Centaurus Lupus and a preliminary survey of transiting planets in Sco-Cen with TESS". The Astronomical Journal. 170 (2): 131. arXiv:2502.00576. Bibcode:2025AJ....170..131V. doi:10.3847/1538-3881/ade67f.