List of exoplanets discovered in 2021
Appearance
This list of exoplanets discovered in 2021 is a list of confirmed exoplanets that were first observed in 2021. 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 |
---|---|---|---|---|---|---|---|---|---|---|
HD 108236 f | 0.17406+0.00482 −0.00437 |
29.54255±0.00069 | 0.1759±0.0037 | transit | 211 | 0.853±0.047 | 5720.0±50.0 | [1][2] | ||
NGTS-14Ab | 0.092±0.012 | 0.444±0.030 | 3.5357173±0.0000069 | 0.0403±0.0071 | 1143±139 | transit | 1060 | 0.898±0.035 | 5187±11 | [3] |
TOI-1259Ab | 0.441+0.049 −0.047 |
1.022+0.030 −0.037 |
3.4779780+0.0000019 −0.0000017 |
0.04070+0.00114 −0.00110 |
936 | transit | 385±1 | 0.68+0.1 −0.01 |
4775±100 | Also white dwarf on a wide orbit[4] |
NGTS-13b | 4.84±0.44 | 1.142±0.046 | 4.12 | 0.0549+0.0015 −0.0025 |
1605±30 | transit | 2150 | 1.30+0.11 −0.18 |
5819±73 | [5] |
TOI-628 b | 6.33+0.29 −0.31 |
1.060+0.041 −0.034 |
3.4095675+0.0000070 −0.0000069 |
0.04860+0.00080 −0.00094 |
1586+52 −40 |
transit | 582 | 1.311+0.066 −0.075 |
6250+220 −190 |
Host star also known as HD 288842[6] |
TOI-640 b | 0.88±0.16 | 1.771+0.060 −0.056 |
5.0037775±0.0000048 | 0.06608+0.00098 −0.0011 |
1749+26 −30 |
transit | 1115 | 1.536+0.069 −0.076 |
6460+130 −150 |
[6] |
TOI-1333 A b | 2.37±0.24 | 1.396+0.056 −0.054 |
4.720219±0.000011 | 0.0626+0.0011 −0.0012 |
1679+35 −34 |
transit | 653 | 1.464+0.076 −0.079 |
6274±97 | Host star also known as BD+47 3521A[6] |
TOI-1478 b | 0.847+0.052 −0.048 |
1.061+0.040 −0.038 |
10.180249±0.000015 | 0.0903+0.0018 −0.0013 |
918±11 | transit | 498 | 0.946+0.059 −0.041 |
5595+83 −81 |
[6] |
TOI-1601 b | 0.99±0.11 | 1.239+0.046 −0.039 |
5.331751±0.000011 | 0.06864+0.00079 −0.00075 |
1619+24 −23 |
transit | 1096 | 1.517+0.053 −0.049 |
5948+87 −89 |
[6] |
OGLE-2019-BLG-0960Lb | 0.0071±0.0027 | 1.75±0.55 | microlensing | 2900±1000 | 0.45±0.15 | Smallest planet discovered by microlensing[7] | ||||
HD 110113 b | 0.0143±0.0020 | 0.183±0.011 | 2.541+0.0005 −0.001 |
0.035±0.001 | 1371±14 | transit | 346.5±2.3 | 0.99±0.08 | 5730 | Radius gap planet, host star also known as TOI-755[8] |
HD 110113 c | 0.0330±0.0038 | 6.744+0.008 −0.009 |
0.068+0.001 −0.002 |
990±10 | radial vel. | 346.5±2.3 | 0.99±0.08 | 5730 | Host star also known as TOI-755[8] | |
KOI-5Ab | 0.179 | 0.63 | 5 | transit | 1870±70 | 1.13 | 5861 | Also called TOI-1241b[9][10] | ||
TOI-178b | 0.0047+0.0012 −0.0013 |
0.102±0.006 | 1.914558±0.000018 | 0.02607±0.00078 | 1040+22 −21 |
transit | 205.16±0.03 | 0.650+0.027 −0.029 |
4316±70 | [11] |
TOI-178c | 0.015+0.0017 −0.0021 |
0.149+0.01 −0.008 |
3.238450+0.000020 −0.000019 |
0.0370±0.0011 | 873±18 | transit | 205.16±0.03 | 0.650+0.027 −0.029 |
4316±70 | [11] |
TOI-178d | 0.0094+0.0025 −0.0032 |
0.229±0.006 | 6.557700±0.000016 | 0.0592±0.0018 | 690±14 | transit | 205.16±0.03 | 0.650+0.027 −0.029 |
4316±70 | [11] |
TOI-178e | 0.0121+0.0039 −0.0029 |
0.197+0.007 −0.008 |
9.961881±0.000042 | 0.0783+0.0023 −0.0024 |
600±12 | transit | 205.16±0.03 | 0.650+0.027 −0.029 |
4316±70 | [11] |
TOI-178f | 0.0242+0.0052 −0.0047 |
0.204±0.009 | 15.231915+0.000115 −0.000095 |
0.1039±0.0031 | 521±11 | transit | 205.16±0.03 | 0.650+0.027 −0.029 |
4316±70 | [11] |
TOI-178g | 0.0123+0.0041 −0.0050 |
0.256+0.012 −0.011 |
20.70950+0.00014 −0.00011 |
0.1275+0.0038 −0.0039 |
470±10 | transit | 205.16±0.03 | 0.650+0.027 −0.029 |
4316±70 | [11] |
HD 183579 b | 0.0620+0.0126 −0.0123 |
0.317+0.013 −0.011 |
17.471278+0.000058 −0.000060 |
0.1334+0.0062 −0.0061 |
769+17 −13 |
transit | 186.1±0.8 | 1.031+0.025 −0.026 |
5788±44 | Host star also known as TOI-1055[12] |
KMT-2019-BLG-0371b | 7.70+11.34 −3.90 |
0.79+0.14 −0.16 |
microlensing | 23000+3000 −4000 |
0.09+0.14 −0.05 |
Multiple solutions for orbital separation[13] | ||||
HD 5278 b | 0.0245+0.0047 −0.0044 |
0.219±0.004 | 14.339156+0.000049 −0.000047 |
0.1202±0.0013 | 943±13 | transit | 183.1±2.7 | 1.126+0.036 −0.035 |
6203±64 | Host star also known as TOI-130[14] |
HD 5278 c | 0.0579+0.0057 −0.0060 |
0.2416±0.0027 | 0.1202±0.0013 | 943±13 | radial vel. | 183.1±2.7 | 1.126+0.036 −0.035 |
6203±64 | Host star also known as TOI-130[14] | |
KMT-2018-BLG-1025Lb | 0.0191+0.0258 −0.0104 |
1.305+0.194 −0.227 |
microlensing | 22000±3000 | 0.219+0.297 −0.120 |
Multiple solutions for orbital parameters[15] | ||||
Gliese 1151b | 0.0079±0.0016 | 2.02 | 0.01735+0.00065 −0.00070 |
radial vel. | 26.23±0.01 | 0.154 | 3143±26 | [16] Refuted a month after confirmation.[17] | ||
TOI-558b | 3.61±0.15 | 1.086+0.041 −0.038 |
14.574071±0.000026 | 0.1291+0.0020 −0.0021 |
1061+13 −12 |
transit | 1312±17 | 1.349+0.064 −0.065 |
6466+95 −93 |
[18] |
TOI-559b | 6.01+0.24 −0.23 |
1.091+0.028 −0.025 |
6.9839095±0.0000051 | 0.0723±0.0013 | 1180+18 −16 |
transit | 761±7 | 1.026±0.057 | 5925+85 −76 |
[18] |
HD 13808 b | 0.0346 | 14.2 | 0.11 | radial vel. | 92.2 | 0.771±0.022 | 5035±50 | Candidate since 2011, confirmed in 2021[19] | ||
HD 13808 c | 0.0315 | 53.8 | 0.26 | radial vel. | 92.2 | 0.771±0.022 | 5035±50 | Candidate since 2011, confirmed in 2021[19] | ||
TOI 451 b | 0.1732+0.0134 −0.0116 |
1.858701+0.000027 −0.000033 |
0.0271+0.0023 −0.0038 |
1524+100 −60 |
transit | 405.1±1.3 | 0.94±0.025 | 5550±56 | Planets orbiting primary of wide binary system.[20][21] Host star also known as CD-38 1467. | |
TOI 451 c | 0.2741±0.0125 | 9.192523+0.000064 −0.000084 |
0.0771+0.0066 −0.0093 |
903+53 −36 |
transit | 405.1±1.3 | 0.94±0.025 | 5550±56 | Planets orbiting primary of wide binary system.[20][21] Host star also known as CD-38 1467. | |
TOI 451 d | 0.3598±0.0134 | 16.364981+0.000047 −0.000049 |
0.1255+0.0057 −0.0065 |
708+15 −12 |
transit | 405.1±1.3 | 0.94±0.025 | 5550±56 | Planets orbiting primary of wide binary system.[20][21] Host star also known as CD-38 1467. | |
HD 110082 b | 0.2857±0.0089 | 10.18271±0.00004 | 0.113+0.009 −0.013 |
transit | 342.8±0.9 | 1.21±0.06 | 6200±100 | Orbiting a primary of wide binary system.[22] Host star also known as TOI-1098. | ||
OGLE-2018-BLG-0567Lb | 0.32+0.34 −0.16 |
2.72+0.49 −0.55 |
microlensing | 23000±3000 | 0.24+0.16 −0.13 |
[23] | ||||
OGLE-2018-BLG-0962Lb | 1.37+0.80 −0.72 |
3.57+0.68 −1.02 |
microlensing | 21000+3000 −5000 |
0.55+0.32 −0.29 |
[23] | ||||
Gliese 740 b | 0.0093±0.0016 | 2.37756+0.00013 −0.00011 |
0.029±0.001 | 829+40 −50 |
radial vel. | 36.21±0.02 | 0.58±0.06 | 3913±21 | [24] | |
OGLE-2018-BLG-1428Lb | 0.77+0.77 −0.53 |
3.30+0.59 −0.83 |
microlensing | 20000+3000 −5000 |
0.43+0.33 −0.22 |
[25] | ||||
LHS 1478 b | 0.0073±0.0006 | 0.111±0.004 | 1.9495378+0.0000040 −0.0000041 |
0.01848+0.00061 −0.0006 |
595+10 −9 |
transit | 59.40±0.03 | 0.236±0.012 | 3381±54 | [26]Host star also known as TOI-1640 or G 245-61 |
TOI-1685 b | 0.0121±0.030 | 0.131±0.006 | 0.6691425±0.0000037 | 0.01156±0.00009 | 1052±21 | transit | 122.68±0.09 | 0.495±0.019 | 3434±51 | [27][28]Host star also known as UCAC4 666-026266 |
TOI-1685 c | 0.0290±0.0065 | 9.025+0.104 −0.119 |
449.1±6.9 | radial vel. | 122.68±0.09 | 0.495±0.019 | 3434±51 | Unconfirmed[27] | ||
KMT-2020-BLG-0414Lb | 0.0032 | 0.15 | microlensing | 3300±300 | 0.3 | Also a brown dwarf with mass 17MJ in the system at 15 AU separation[29] | ||||
HD 39474 b | 0.42+0.05 −0.03 |
1.008+0.012 −0.015 |
52.97818+0.00004 −0.00004 |
0.30+0.02 −0.03 |
759+37 −26 |
transit | 372.5±1.1 | 1.316±0.027 | 6394±75 | Host star also known as TOI-201[30] |
Gliese 486 b | 0.0089±0.0004 | 0.117±0.006 | 1.467119+0.000031 −0.000030 |
0.01734+0.00026 −0.00027 |
701±13 | transit | 26.344±0.013 | 0.323±0.015 | 3340±54 | Planet may have a measurable atmosphere[31] |
NGTS-15b | 0.751+0.102 −0.088 |
1.10±0.10 | 3.27623±0.00001 | 0.0441±0.0046 | 1146±47 | transit | 2580±60 | 0.995±0.015 | 5600±150 | [32] |
NGTS-16b | 0.667+0.157 −0.129 |
1.30+0.13 −0.12 |
4.84532±0.00002 | 0.0523±0.0064 | 1177±59 | transit | 2910+95 −75 |
1.002±0.011 | 5550±150 | [32] |
NGTS-17b | 0.764+0.195 −0.164 |
1.24±0.11 | 3.24253±0.00001 | 0.0391±0.0043 | 1457±50 | transit | 3420±90 | 1.025+0.015 −0.014 |
5650±100 | [32] |
NGTS-18b | 0.409+0.081 −0.063 |
1.21±0.18 | 3.05125±0.00001 | 0.0448±0.0068 | 1381+55 −53 |
transit | 3610±140 | 1.003+0.020 −0.012 |
5610±150 | [32] |
OGLE-2019-BLG-1053Lb | 0.0078+0.0037 −0.0031 |
3.4±0.5 | microlensing | 22000+3000 −2000 |
0.61+0.29 −0.24 |
[33] | ||||
TOI-1634 b | 0.0313±0.0030 | 0.158±0.007 | 0.9893457±0.0000034 | 0.01491±0.00015 | 921±21 | transit | 114.40±0.08 | 0.452±0.014 | 3472±48 | [28][34] |
KMT-2019-BLG-1715 | 2.56+1.13 −1.16 |
3.32+0.82 −0.92 |
microlensing | 13000±3000 | 0.61+0.27 −0.28 |
Multiple solutions for orbital separation, also 0.15M☉ red dwarf in the system.[35] | ||||
OGLE-2018-BLG-1185b | 0.026+0.025 −0.015 |
1.54+0.18 −0.22 |
microlensing | 24000+2000 −3000 |
0.37+0.35 −0.21 |
Multiple solutions for planet and star masses.[36] | ||||
TOI-1260 b | 0.0271+0.0043 −0.0037 |
0.208+0.009 −0.008 |
3.12748+0.000047 −0.000038 |
0.0366+0.0022 −0.0036 |
860+47 −31 |
transit | 239.5±0.3 | 0.66±0.01 | 4227±85 | [37] |
TOI-1260 c | 0.0373+0.0106 −0.0102 |
0.252±0.013 | 7.49325+0.00015 −0.00013 |
0.0656+0.0039 −0.0065 |
643+35 −23 |
transit | 239.5±0.3 | 0.66±0.01 | 4227±85 | [37] |
KMT-2018-BLG-1976Lb | 1.96+1.23 −1.12 |
2.04+0.72 −0.83 |
microlensing | 19000±2000 | 0.65+0.41 −0.37 |
[38] | ||||
KMT-2018-BLG-1996Lb | 1.22+0.72 −0.63 |
1.97+0.51 −0.25 |
microlensing | 19000±2000 | 0.69+0.40 −0.38 |
[38] | ||||
OGLE-2019-BLG-0954Lb | 14.2+9.9 −7.5 |
2.65+0.89 −1.20 |
microlensing | 12000+1000 −2000 |
0.80+0.55 −0.42 |
[38] | ||||
YSES 2b | 6.3+1.6 −0.9 |
115 | imaging | 356.4±0.5 | 1.10±0.03 | 4749±40 | [39] | |||
KMT-2016-BLG-2605b | 0.8+1.2 −0.4 |
0.68±0.11 | microlensing | 21000±3000 | 0.065+0.10 −0.035 |
[40] | ||||
TOI-1431 b | 3.14+0.19 −0.18 |
1.51±0.06 | 2.65022±0.00001 | 0.047±0.002 | 2370±100 | transit | 488±3 | 1.90+0.10 −0.08 |
7690+400 −250 |
Also known as MASCARA-5b[41][42] |
Specific exoplanet lists
- List of directly imaged exoplanets
- List of exoplanet extremes
- List of exoplanet firsts
- List of exoplanets discovered by the Kepler space telescope
- List of exoplanets observed during Kepler's K2 mission
- List of extrasolar candidates for liquid water
- List of 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 largest exoplanets
- List of smallest exoplanets
- List of transiting exoplanets
- List of exoplanets and planetary debris around white dwarfs
Lists of exoplanets by year of discovery
- List of exoplanets discovered before 2000 (31)
- List of exoplanets discovered between 2000–2009 (377)
- List of exoplanets discovered in 2010 (109)
- List of exoplanets discovered in 2011 (179)
- List of exoplanets discovered in 2012 (149)
- List of exoplanets discovered in 2013 (151)
- List of exoplanets discovered in 2014 (870)
- List of exoplanets discovered in 2015 (149)
- List of exoplanets discovered in 2016 (1497)
- List of exoplanets discovered in 2017 (158)
- List of exoplanets discovered in 2018 (303)
- List of exoplanets discovered in 2019 (172)
- List of exoplanets discovered in 2020 (249)
- List of exoplanets discovered in 2021 (59)
- List of exoplanets discovered in 2022 (313)
- List of exoplanets discovered in 2023 (307)
- List of exoplanets discovered in 2024 (238)
References
- ^ "HD 108236 f". exoplanet.eu. Retrieved 4 January 2021.
- ^ CHEOPS observations of the HD 108236 planetary system: A fifth planet, improved ephemerides, and planetary radii
- ^ Smith, A. M. S.; Acton, J. S.; Anderson, D. R.; Armstrong, D. J.; Bayliss, D.; Belardi, C.; Bouchy, F.; Brahm, R.; Briegal, J. T.; Bryant, E. M.; Burleigh, M. R.; Cabrera, J.; Chaushev, A.; Cooke, B. F.; Costes, J. C.; Csizmadia, Sz.; Eigmüller, Ph.; Erikson, A.; Gill, S.; Gillen, E.; Goad, M. R.; Günther, M. N.; Henderson, B. A.; Hogan, A.; Jordán, A.; Lendl, M.; McCormac, J.; Moyano, M.; Nielsen, L. D.; et al. (2021), NGTS-14Ab: a Neptune-sized transiting planet in the desert, arXiv:2101.01470
- ^ Martin, David V.; El-Badry, Kareem; Vedad Kunovac Hodžić; Triaud, Amaury H. M. J.; Angus, Ruth; Birky, Jessica; Foreman-Mackey, Daniel; Hedges, Christina; Montet, Benjamin T.; Murphy, Simon J.; Santerne, Alexandre; Stassun, Keivan G.; Stephan, Alexander P.; Wang, Ji; Benni, Paul; Krushinsky, Vadim; Chazov, Nikita; Mishevskiy, Nikolay; Ziegler, Carl; Soubkiou, Abderahmane; Benkhaldoun, Zouhair; Caldwell, Douglas A.; Collins, Karen; Henze, Christopher E.; Guerrero, Natalia M.; Jenkins, Jon M.; Latham, David W.; Levine, Adam; McDermott, Scott; et al. (2021), TOI-1259Ab – a gas giant planet with 2.7% deep transits and a bound white dwarf companion, arXiv:2101.02707
- ^ Grieves, Nolan; Nielsen, Louise D.; Vines, Jose I.; Bryant, Edward M.; Gill, Samuel; Bouchy, François; Lendl, Monika; Bayliss, Daniel; Eigmueller, Philipp; Segransan, Damien; Acton, Jack S.; Anderson, David R.; Burleigh, Matthew R.; Casewell, Sarah L.; Chaushev, Alexander; Cooke, Benjamin F.; Gillen, Edward; Goad, Michael R.; Günther, Maximilian N.; Henderson, Beth A.; Hogan, Aleisha; Jenkins, James S.; Alves, Douglas R.; Jordán, Andrés; McCormac, James; Moyano, Maximiliano; Queloz, Didier; Raynard, Liam; Seidel, Julia V.; et al. (2021), NGTS-13b: A hot 4.8 Jupiter-mass planet transiting a subgiant star, arXiv:2101.04245
- ^ a b c d e Rodriguez, Joseph E.; Quinn, Samuel N.; Zhou, George; Vanderburg, Andrew; Nielsen, Louise D.; Wittenmyer, Robert A.; Brahm, Rafael; Reed, Phillip A.; Huang, Chelsea X.; Vach, Sydney; Ciardi, David R.; Oelkers, Ryan J.; Stassun, Keivan G.; Hellier, Coel; Scott Gaudi, B.; Eastman, Jason D.; Collins, Karen A.; Bieryla, Allyson; Christian, Sam; Latham, David W.; Carleo, Ilaria; Wright, Duncan J.; Matthews, Elisabeth; Gonzales, Erica J.; Ziegler, Carl; Dressing, Courtney D.; Howell, Steve B.; Tan, Thiam-Guan; Wittrock, Justin; et al. (2021), TESS Delivers Five New Hot Giant Planets Orbiting Bright Stars from the Full Frame Images, arXiv:2101.01726
- ^ Yee, Jennifer C.; Zang, Weicheng; Udalski, Andrzej; Ryu, Yoon-Hyun; Green, Jonathan; Hennerley, Steve; Marmont, Andrew; Sumi, Takahiro; Mao, Shude; Gromadzki, Mariusz; Mróz, Przemek; Skowron, Jan; Poleski, Radoslaw; Szymański, Michał K.; Soszyński, Igor; Pietrukowicz, Paweł; Kozłowski, Szymon; Ulaczyk, Krzysztof; Rybicki, Krzysztof A.; Iwanek, Patryk; Wrona, Marcin; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Han, Cheongho; Hwang, Kyu-Ha; Youn Kil Jung; Kim, Hyoun-Woo; Shin, In-Gu; et al. (2021), OGLE-2019-BLG-0960Lb: The Smallest Microlensing Planet, arXiv:2101.04696
- ^ a b Osborn, H. P.; Armstrong, D. J.; Adibekyan, V.; Collins, K. A.; Delgado-Mena, E.; Howell, S. B.; Hellier, C.; King, G. W.; Lillo-Box, J.; Nielsen, L. D.; Otegi, J. F.; Santos, N. C.; Ziegler, C.; Anderson, D. R.; Briceño, C.; Burke, C.; Bayliss, D.; Barrado, D.; Bryant, E. M.; Brown, D J A.; Barros, S C C.; Bouchy, F.; Caldwell, D. A.; Conti, D. M.; Díaz, R. F.; Dragomir, D.; Deleuil, M.; Demangeon, O D S.; Dorn, C.; et al. (2021), "A hot mini-Neptune in the radius valley orbiting solar analogue HD 110113", Monthly Notices of the Royal Astronomical Society, arXiv:2101.04745, Bibcode:2021MNRAS.tmp..240O, doi:10.1093/mnras/stab182
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: CS1 maint: bibcode (link) CS1 maint: unflagged free DOI (link) - ^ Hirsch, Lea A.; Ciardi, David R.; Howard, Andrew W.; Everett, Mark E.; Furlan, Elise; Saylors, Mindy; Horch, Elliott P.; Howell, Steve B.; Teske, Johanna; Marcy, Geoffrey W. (2017), "ASSESSING THE EFFECT OF STELLAR COMPANIONS FROM HIGH-RESOLUTION IMAGING OF Kepler OBJECTS OF INTEREST", The Astronomical Journal, 153 (3): 117, arXiv:1701.06577, Bibcode:2017AJ....153..117H, doi:10.3847/1538-3881/153/3/117, S2CID 39321033
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: CS1 maint: unflagged free DOI (link) - ^ AT LAST! CONFIRMATION OF KEPLER'S SECOND PLANETARY CANDIDATE
- ^ a b c d e f Leleu, A.; Alibert, Y.; Hara, N. C.; Hooton, M. J.; Wilson, T. G.; Robutel, P.; Delisle, J.-B.; Laskar, J.; Hoyer, S.; Lovis, C.; Bryant, E. M.; Ducrot, E.; Cabrera, J.; Acton, J.; Adibekyan, V.; Allart, R.; Allende Prieto, C.; Alonso, R.; Alves, D.; Anderson, D. R.; Al, D. R.; Angerhausen, D.; Anglada Escudé, G.; Asquier, J.; Barrado, D.; Barros, S. C. C.; Baumjohann, W.; Bayliss, D.; Beck, M.; et al. (2021), "Six transiting planets and a chain of Laplace resonances in TOI-178", Astronomy & Astrophysics, arXiv:2101.09260, doi:10.1051/0004-6361/202039767, S2CID 231693292
- ^ Palatnick, Skyler; Kipping, David; Yahalomi, Daniel (2021), VALIDATION OF HD 183579b USING ARCHIVAL RADIAL VELOCITIES: A WARM-NEPTUNE ORBITING A BRIGHT SOLAR ANALOG, arXiv:2101.12137
- ^ Yun Hak Kim; Chung, Sun-Ju; Yee, Jennifer C.; Udalski, A.; Bond, Ian A.; Youn Kil Jung; Gould, Andrew; Albrow, Michael D.; Han, Cheongho; Hwang, Kyu-Ha; Ryu, Yoon-Hyun; Shin, In-gu; Shvartzvald, Yossi; Zang, Weicheng; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Hyoun-Woo; Kim, Seung-Lee; Lee, Chung-Uk; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W.; Poleski, Radek; Mróz, Przemek; Skowron, Jan; Szymański, Michal K.; Pietrukowicz, Pawel; Kozłowski, Szymon; et al. (2021), KMT-2019-BLG-0371 and the Limits of Bayesian Analysis, arXiv:2101.12206
- ^ a b Sozzetti, A.; Damasso, M.; Bonomo, A. S.; Alibert, Y.; Sousa, S. G.; Adibekyan, V.; Zapatero Osorio, M. R.; González Hernández, J. I.; Barros, S. C. C.; Lillo-Box, J.; Stassun, K. G.; Winn, J.; Cristiani, S.; Pepe, F.; Rebolo, R.; Santos, N. C.; Allart, R.; Barclay, T.; Bouchy, F.; Cabral, A.; Ciardi, D.; Di Marcantonio, P.; D'Odorico, V.; Ehrenreich, D.; Fasnaugh, M.; Figueira, P.; Haldemann, J.; Jenkins, J. M.; Latham, D. W.; et al. (2021), A sub-Neptune and a non-transiting Neptune-mass companion unveiled by ESPRESSO around the bright late-F dwarf HD 5278 (TOI-130), arXiv:2101.12300
- ^ Han, Cheongho; Udalski, Andrzej; Lee, Chung-Uk; Albrow, Michael D.; Chung, Sun-Ju; Gould, Andrew; Hwang, Kyu-Ha; Youn Kil Jung; Kim, Doeon; Kim, Hyoun-Woo; Ryu, Yoon-Hyun; Shin, In-Gu; Shvartzvald, Yossi; Yee, Jennifer C.; Zang, Weicheng; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Seung-Lee; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W.; Kim, Chun-Hwey; Kim, Woong-Tae; Mróz, Przemek; Szymański, Michał K.; Skowron, Jan; Poleski, Radosław; Soszyński, Igor; et al. (2021), KMT-2018-BLG-1025Lb: microlensing super-Earth planet orbiting a low-mass star, arXiv:2102.01890
- ^ Mahadevan, Suvrath; Stefánsson, Guðmundur; Robertson, Paul; Terrien, Ryan C.; Ninan, Joe P.; Holcomb, Rae J.; Halverson, Samuel; Cochran, William D.; Kanodia, Shubham; Ramsey, Lawrence W.; Wolszczan, Alexander; Endl, Michael; Bender, Chad F.; Diddams, Scott A.; Fredrick, Connor; Hearty, Fred; Monson, Andrew; Metcalf, Andrew J.; Roy, Arpita; Schwab, Christian (2021), The Habitable-zone Planet Finder Detects a Terrestrial-mass Planet Candidate Closely Orbiting Gliese 1151: The Likely Source of Coherent Low-frequency Radio Emission from an Inactive Star, arXiv:2102.02233
- ^ The CARMENES search for exoplanets around M dwarfs No evidence for a super-Earth in a 2-day orbit around GJ 1151, 2021, arXiv:2103.10216
- ^ a b Ikwut-Ukwa, Mma; Rodriguez, Joseph E.; Quinn, Samuel N.; Zhou, George; Vanderburg, Andrew; Ali, Asma; Bunten, Katya; Scott Gaudi, B.; Latham, David W.; Howell, Steve B.; Huang, Chelsea X.; Bieryla, Allyson; Collins, Karen A.; Carmichael, Theron W.; Rabus, Markus; Eastman, Jason D.; Collins, Kevin I.; Tan, Thiam-Guan; Schwarz, Richard P.; Myers, Gordon; Stockdale, Chris; Kielkopf, John F.; Radford, Don J.; Oelkers, Ryan J.; Jenkins, Jon M.; Ricker, George R.; Seager, Sara; Vanderspek, Roland K.; Winn, Joshua N.; et al. (2021), Two Massive Jupiters in Eccentric Orbits from the TESS Full Frame Images, arXiv:2102.02222
- ^ a b Ahrer, E.; Queloz, D.; Rajpaul, V. M.; Ségransan, D.; Bouchy, F.; Hall, R.; Handley, W.; Lovis, C.; Mayor, M.; Mortier, A.; Pepe, F.; Thompson, S.; Udry, S.; Unger, N. (2021), "The HARPS search for southern extra-solar planets XLV. Two Neptune mass planets orbiting HD 13808: a study of stellar activity modelling's impact on planet detection", Monthly Notices of the Royal Astronomical Society, arXiv:2102.03387, Bibcode:2021MNRAS.tmp..407A, doi:10.1093/mnras/stab373
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: CS1 maint: bibcode (link) CS1 maint: unflagged free DOI (link) - ^ a b c Newton, Elisabeth R.; Mann, Andrew W.; Kraus, Adam L.; Livingston, John H.; Vanderburg, Andrew; Curtis, Jason L.; Pa Chia Thao; Hawkins, Keith; Wood, Mackenna L.; Rizzuto, Aaron C.; Soubkiou, Abderahmane; Tofflemire, Benjamin M.; Zhou, George; Crossfield, Ian J. M.; Pearce, Logan A.; Collins, Karen A.; Conti, Dennis M.; Tan, Thiam-Guan; Villeneuva, Steven; Spencer, Alton; Dragomir, Diana; Quinn, Samuel N.; Jensen, Eric L. N.; Collins, Kevin I.; Stockdale, Chris; Cloutier, Ryan; Hellier, Coel; Benkhaldoun, Zouhair; Ziegler, Carl; et al. (2021), "TESS Hunt for Young and Maturing Exoplanets (THYME) IV: Three small planets orbiting a 120 Myr-old star in the Pisces–Eridanus stream", The Astronomical Journal, 161 (2): 65, arXiv:2102.06049, Bibcode:2021AJ....161...65N, doi:10.3847/1538-3881/abccc6, S2CID 231879927
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: CS1 maint: unflagged free DOI (link) - ^ a b c TESS re-observes the young multi-planet system TOI-451:refined ephemeris and activity evolution, 2021, arXiv:2103.09746
- ^ Tofflemire, Benjamin M.; Rizzuto, Aaron C.; Newton, Elisabeth R.; Kraus, Adam L.; Mann, Andrew W.; Vanderburg, Andrew; Nelson, Tyler; Hawkins, Keith; Wood, Mackenna L.; Zhou, George; Quinn, Samuel N.; Howell, Steve B.; Collins, Karen A.; Schwarz, Richard P.; Stassun, Keivan G.; Bouma, Luke G.; Essack, Zahra; Osborn, Hugh; Boyd, Patricia T.; Furesz, Gabor; Glidden, Ana; Twicken, Joseph D.; Wohler, Bill; McLean, Brian; Ricker, George R.; Vanderspek, Roland; Latham, David W.; Seager, S.; Winn, Joshua N.; Jenkins, Jon M. (2021), TESS Hunt for Young and Maturing Exoplanets (THYME) V: A Sub-Neptune Transiting a Young Star in a Newly Discovered 250 Myr Association, arXiv:2102.06066
- ^ a b OGLE-2018-BLG-0567Lb and OGLE-2018-BLG-0962Lb: Two Microlensing Planets through Planetary-Caustic Channel, 2021, arXiv:2102.07338
- ^ A super-Earth on a close-in orbit around the M1V star GJ 740. A HADES and CARMENES collaboration, 2021, arXiv:2102.09441
- ^ OGLE-2018-BLG-1428Lb: a Jupiter-mass planet beyond the snow line of a dwarf star, 2021, arXiv:1303.1184
- ^ Mass and density of the transiting hot and rocky super-Earth LHS 1478 b (TOI-1640 b), 2021, arXiv:2102.11640
- ^ a b An ultra-short-period transiting super-Earth orbiting the M3 dwarf TOI-1685, 2021, arXiv:2103.01016
- ^ a b Two Bright M Dwarfs Hosting Ultra-Short-Period Super-Earths with Earth-like Compositions, 2021, arXiv:2103.12760
- ^ An Earth-mass Planet in a Time of Covid-19: KMT-2020-BLG-0414Lb, 2021, arXiv:2103.01896
- ^ A transiting warm giant planet around the young active star TOI-201, 2021, arXiv:2103.02685
- ^ A nearby transiting rocky exoplanet that is suitable for atmospheric investigation, 2021, arXiv:2103.04950
- ^ a b c d NGTS 15b, 16b, 17b and 18b: four hot Jupiters from the Next Generation Transit Survey, 2021, arXiv:2103.10302
- ^ Systematic KMTNet Planetary Anomaly Search, Paper I: OGLE-2019-BLG-1053Lb, A Buried Terrestrial Planet, 2021, arXiv:2103.11880
- ^ TOI-1634 b: an Ultra-Short Period Keystone Planet Sitting Inside the M Dwarf Radius Valley, 2021, arXiv:2103.12790
- ^ KMT-2019-BLG-1715: planetary microlensing event with three lens masses and two source stars, 2021, arXiv:2104.00293
- ^ OGLE-2018-BLG-1185b : A Low-Mass Microlensing Planet Orbiting a Low-Mass Dwarf, 2021, arXiv:2104.02157
- ^ a b Hot planets around cool stars – two short-period mini-Neptunes transiting the late K-dwarf TOI-1260, 2021, arXiv:2104.05653
- ^ a b c Three microlensing planets with no caustic-crossing features, 2021, arXiv:2104.06544
- ^ Discovery of a directly imaged planet to the young solar analog YSES 2, 2021, arXiv:2104.08285
- ^ Shortest Microlensing Event with a Bound Planet:KMT-2016-BLG-2605, 2021, arXiv:2104.07906
- ^ TOI-1431 b/MASCARA-5 b: A Highly Irradiated Ultra-Hot Jupiter Orbiting One of the Hottest & Brightest Known Exoplanet Host Stars, 2021, arXiv:2104.12078
- ^ The obliquity and atmosphere of the ultra-hot Jupiter TOI-1431b (MASCARA-5b): A misaligned orbit and no signs of atomic or molecular absorptions, 2021, arXiv:2104.12414