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Contents

   



(Top)
  


1 Specific exoplanet lists  


1.1  Lists of exoplanets by year of discovery  






2 References  













List of exoplanets discovered in 2022






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From Wikipedia, the free encyclopedia
  

This is a dynamic list and may never be able to satisfy particular standards for completeness. You can help by adding missing items with reliable sources.

This list of exoplanets discovered in 2022 is a list of confirmed exoplanets that were first reported in 2022. For exoplanets detected only by radial velocity, the listed value for mass is a lower limit. See Minimum mass for more information.


On 31 March 2022, K2-2016-BLG-0005Lb was reported to be the most distant exoplanet found by Kepler to date.[1][2]

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
29 Cygni b 13.9+6.1
−5.1 		16.9+3.4
−1.9 		imaging 130.9±0.9 2.14±0.15 8790+1513
−1292 		Host star also known as HIP 99770[3]
CoRoT-35b 1.10±0.37 1.68±0.11 3.22748±0.00008 0.04290±0.00092 1747±62 transit 3700±200 1.01+0.07
−0.06 		6390±130 [4]
CoRoT-36b 0.68+0.47
−0.43 		1.41±0.14 5.616531±0.000023 0.066±0.007 1567±35 transit 3110±60 1.32±0.09 6730±140 [4]
EPIC 206317286 c 0.0168±0.098 0.186+0.015
−0.014 		17.51547+0.00228
−0.00296 		570 transit 0.832+0.253
−0.367 		4752±138 [5]
EPIC 210768568 b 0.088±0.004 3.2141±0.0002 0.0511+0.0021
−0.0028 		transit 965 1.018±0.131 5711±105 [6]
EPIC 246078343 b 0.068±0.007 0.8094±0.00003 0.0117+0.0009
−0.0012 		transit 954 0.808+0.364
−0.256 		4116±138 [6]
EPIC 246078343 c 0.110±0.006 5.3301±0.0003 0.0426+0.0016
−0.0019 		transit 954 0.808+0.364
−0.256 		4116±138 [6]
EPIC 246220667 b 0.172±0.006 6.6690±0.0002 0.0552+0.0017
−0.0023 		transit 835 0.814+0.363
−0.251 		4343±138 [6]
EPIC 246220667 c 0.109±0.006 4.3696±0.0001 0.0487+0.0027
−0.0031 		transit 835 0.814+0.363
−0.251 		4343±138 [6]
EPIC 247422570 b 0.189±0.009 5.9382+0.0006
−0.0004 		0.0586+0.0032
−0.0033 		transit 2181 0.893+0.406
−0.275 		5590±138 [6]
Gaia-1b 1.68±0.11 1.229±0.021 3.052524±0.000017 0.04047±0.00094 transit 1201±7 0.949±0.066 5470±110 First confirmed exoplanet discovered by Gaia, along with Gaia-2b[7]
Gaia-2b 0.817±0.047 1.322±0.013 3.6915224±0.0000039 0.0467±0.0015 transit 676±3 1.000±0.095 5720±84 First confirmed exoplanet discovered by Gaia, along with Gaia-1b[7]
Gliese 514b 0.0164±0.0028 140.43±0.41 0.422+0.014
−0.015 		202±11 radial vel. 24.850±0.010 0.510±0.051 3714±51 Planetary orbit partially in habitable zone[8]
Gliese 1002 b 0.0034±0.0004 10.3465±0.027 0.0457±0.0013 230.9±6.7 radial vel. 15.808±0.003 0.120±0.010 3024±52 Planet in habitable zone[9]
Gliese 1002 c 0.0043±0.0005 21.202±0.013 0.0738±0.0021 181.7±5.2 radial vel. 15.808±0.003 0.120±0.010 3024±52 Planet in habitable zone[9]
Gliese 3929 b 0.0055±0.0014 0.097±0.004 2.6162745±0.000003 0.0252±0.0005 568±6 transit 51.64±0.02 0.309±0.014 3369±51 Another planet in system is suspected[10][11]
Gliese 3929 c 0.0180±0.0029 15.04±0.03 0.081±0.002 317±3 radial vel. 51.64±0.02 0.309±0.014 3369±51 [11]
GJ 463 b 3.6±0.4 3448+110
−88 		3.53±0.07 radial vel. 59.91±0.03 0.49±0.02 3540±41 Host star also known as Ross 690[12][13]
GJ 3090 b 0.0105 0.19 2.8531042±0.0000032 0.03165 696 transit 73.21±0.04 0.519±0.013 3556±70 Host star also known as TOI-177[14]
GJ 3090 c 0.0538 12.734+0.033
−0.026 		0.08575 421 radial vel. 73.21±0.04 0.519±0.013 3556±70 Host star also known as TOI-177[14]
HD 3167 e 0.0306±0.0037 102.09+0.52
−0.50 		0.4048+0.0077
−0.0074 		375±7 radial vel. 154.59±0.13 0.852+0.026
−0.015 		5300±73 [15]
HD 18599 b 0.0758+0.0223
−0.0242 		0.232±0.012 4.1374354+0.0000036
−0.0000037 		0.0480±0.0004 935±11 transit 126.02±0.06 0.863±0.020 5145±50 Host star also known as TOI-179, also red dwarf star in the system[16][17][18]
HD 20329b 0.0233±0.0034 0.154±0.006 0.926118+0.000050
−0.000043 		0.0180±0.0003 2141±27 transit 207.7±0.9 0.90±0.05 5596±50 [19]
HD 22532 b 2.12±0.09 872.6±2.8 1.900±0.004 radial vel. 526±2 1.20±0.05 5067+59
−22 		Giant host star[20]
HD 22946 b 0.154±0.009 4.040301+0.000023
−0.000042 		0.0528±0.0030 1378±36 transit 205.08±0.16 1.158±0.058 6210+173
−158 		Host star also known as TOI-411, third transiting planet in system is suspected[21]
HD 22946 c 0.245±0.013 9.573096+0.000026
−0.000023 		0.0939±0.0054 1033±27 transit 205.08±0.16 1.158±0.058 6210+173
−158 		Host star also known as TOI-411, third transiting planet in system is suspected[21]
HD 23472 d 0.0017±0.0006 0.067±0.005 3.97664+0.000030
−0.000044 		0.04298+0.00063
−0.00065 		909+35
−32 		transit 127.48±0.06 0.67±0.03 4684±99 [22]
HD 23472 e 0.0023±0.0009 0.073±0.006 7.90754±0.00011 0.0680±0.0010 723+28
−25 		transit 127.48±0.06 0.67±0.03 4684±99 [22]
HD 23472 f 0.0024±0.0013 0.102±0.007 12.1621839+0.00012
−0.000099 		0.0906±0.0014 630+27
−23 		transit 127.48±0.06 0.67±0.03 4684±99 [22]
HD 28109 b 0.058+0.029
−0.024 		0.196±0.009 22.89104+0.00035
−0.00036 		0.1357±0.0034 881.2±7.5 transit 457.0±0.6 1.26±0.08 6120±50 [23]
HD 28109 c 0.025+0.013
−0.010 		0.378±0.010 56.00819+0.00194
−0.00202 		0.308±0.011 585.2+8.7
−8.3 		transit 457.0±0.6 1.26±0.08 6120±50 [23]
HD 28109 d 0.018+0.009
−0.007 		0.290±0.010 84.25999+0.00744
−0.00662 		0.411±0.016 506.5+8.7
−8.0 		transit 457.0±0.6 1.26±0.08 6120±50 [23]
HD 29399 b 1.57±0.11 892.7±5.9 1.913±0.008 radial vel. 144.2±0.3 1.15±0.04 4845±52 Giant host star[24]
HD 33142 d [ja] 0.89+0.06
−0.05 		810.2+3.8
−4.2 		1.955+0.016
−0.012 		radial vel. 394.3±0.9 1.52±0.03 5025.4+23.6
−15.5 		Giant host star[25]
HD 56414 b 0.0944±0.0053 0.331±0.018 29.04992±0.00021 0.229±0.004 1133±30 transit 873±3 1.89±0.11 8500±150 Host star also known as TOI-1228[26]
HD 64121 b 2.56±0.19 623.0±3.4 1.510±0.006 radial vel. 424.1±1.7 1.18±0.05 5066+58
−60 		Giant host star[20]
HD 69123 b 3.04±0.16 1193.3±7.0 2.482±0.010 radial vel. 245.0±1.3 1.43±0.07 4787+280
−51 		Giant host star[20]
HD 83443 c 1.5+0.5
−0.2 		8241+1019
−530 		8.0±0.8 radial vel. 133.6±0.2 1.00±0.03 5442±17 Eccentric orbit due to hot Jupiter in system[27]
HD 93963A b 0.121±0.004 1.0391353+0.0000049
−0.0000045 		0.02085±0.00037 2042±27 transit 268.6±1.3 1.109±0.043 5987±64 Host star also known as TOI-1797[28]
HD 93963A c 0.288±0.005 3.6451398+0.0000106
−0.0000142 		0.04813±0.00085 1344±18 transit 268.6±1.3 1.109±0.043 5987±64 Host star also known as TOI-1797[28]
HD 109833 b 0.258+0.014
−0.012 		9.188526±0.000026 transit 259.5±0.2 1.08±0.05 5881±50 Young host star also known as TOI-1097[29]
HD 109833 c 0.231+0.018
−0.016 		13.900148±0.000057 transit 259.5±0.2 1.08±0.05 5881±50 Young host star also known as TOI-1097[29]
HD 114082 b 8.0±1.0 1.00±0.03 109.75+0.40
−0.37 		0.5109+0.0081
−0.0083 		transit 310.1±0.7 1.47±0.07 6651±35 Young star, eccentric planetary orbit[30][31]
HD 167768 b [zh] 0.85+0.12
−0.11 		20.6532+0.0032
−0.0032 		0.1512+0.0058
−0.0063 		1874 radial vel. 353.5 1.08+0.14
−0.12 		4830 Host red giant star also known as HR 8640, other planets in system are suspected[32]
HD 191939 g 0.0425±0.0063 284+10
−8 		0.812±0.028 278±6 radial vel. 174.4±0.1 0.81±0.04 5348±100 Habitable zone planet[33]
HD 191939 f >2.1 >2200 >3.2 <125 174.4±0.1 0.81±0.04 5348±100 [33]
HD 199981 b 10.070±2.483 21000±8000 13.048±3.073 radial vel. 66.7±2.4 Host star also known as GJ 9714[34]
HD 105618 b 0.079±0.008 9.9 0.091±0.004 radial vel. 227.8±0.4 Also brown dwarf in the system[34]
HD 206893 c [fr] 12.3+1.1
−1.2 		1.46+0.18
−0.06 		2082 3.53+0.08
−0.07 		1181.9+20.6
−53.9 		radial vel. 125.1±2.6 1.24 6486 Some deuterium burning despite its low mass, also another brown dwarf is present in the system[35]
HD 21019 b [zh] 0.014±0.002 2.56 0.034±0.002 radial vel. 120 Host star also known as GJ 2030[34]
HD 21019 c [zh] 12.934±2.361 25600±2500 16.752±1.312 radial vel. 120 Host star also known as GJ 2030[34]
HD 21175 b 0.038±0.010 10.6 0.091±0.004 radial vel. 57.7 Host star also known as GJ 3222, planet on extremely eccentric orbit, also brown dwarf in the system[34]
HD 260655 b 0.0067±0.0011 0.111±0.002 2.76953±0.00003 0.02933±0.00024 709±4 transit 32.63±0.07 0.439±0.011 3803±10 Host star also known as TOI-4599[36]
HD 260655 c 0.0097±0.0015 0.137±0.004 5.70588±0.00007 0.04749±0.00039 557±3 transit 32.63±0.07 0.439±0.011 3803±10 Host star also known as TOI-4599[36]
HIP 34269 b [ja] 0.0052±0.0007 0.103±0.005 0.548177±0.000019 0.01188±0.00040 1617±41 transit 154.81±0.15 0.740±0.017 4440±100 Host star also known as TOI-500[37]
HIP 34269 c [ja] 0.0146±0.0016 6.6356±0.0040 radial vel. 154.81±0.15 0.740±0.017 4440±100 Host star also known as TOI-500[37]
HIP 34269 d [ja] 0.1055±0.0033 26.233±0.020 radial vel. 154.81±0.15 0.740±0.017 4440±100 Host star also known as TOI-500[37]
HIP 34269 e [ja] 0.0376±0.0042 61.30±0.28 radial vel. 154.81±0.15 0.740±0.017 4440±100 Host star also known as TOI-500[37]
HIP 94235 b 0.268±0.027 7.713057±0.000021 0.07870+0.00056
−0.00017 		1060±50 transit 191.2±0.4 1.094+0.024
−0.007 		5991±50 Host star also known as TOI-4399, shares system with a red dwarf[38]
HR 7321 b 0.30±0.07 285.1+1.2
−1.5 		0.937±0.003 radial vel. 200.2 1.35+0.19
−0.21 		4971 Red giant host star also known as HD 184010[39]
HR 7321 c 0.28+0.08
−0.10 		483.3+3.2
−4.0 		1.332+0.006
−0.007 		radial vel. 200.2 1.35+0.19
−0.21 		4971 Red giant host star also known as HD 184010[39]
HR 7321 d 0.46±0.08 837.7+6.4
−5.5 		1.922+0.010
−0.008 		radial vel. 200.2 1.35+0.19
−0.21 		4971 Red giant host star also known as HD 184010[39]
K2-365 b 0.0272±0.0172 0.259+0.017
−0.015 		23.448172+0.00076
−0.00099 		710 transit 0.823+0.369
−0.25 		5561±138 [5]
K2-366 b 0.0199±0.0115 0.210+0.016
−0.014 		15.93703+0.00079
−0.00114 		770 transit 0.825+0.366
−0.255 		5601±138 [5]
K2-367 b 0.0203±0.0126 0.215+0.020
−0.017 		20.64509+0.00099
−0.00137 		450 transit 0.756+0.231
−0.347 		4348±128 [5]
K2-368 b 0.0073±0.0042 0.118+0.009
−0.008 		5.02559+0.00028
−0.00034 		800 transit 0.746+0.334
−0.232 		4663±138 [5]
K2-368 c 0.0078±0.0041 0.121+0.010
−0.009 		9.66018±0.00116 650 transit 0.746+0.334
−0.232 		4663±138 [5]
K2-368 d 0.0146±0.0085 0.173+0.013
−0.012 		20.20108+0.00235
−0.00273 		500 transit 0.746+0.334
−0.232 		4663±138 [5]
K2-369 b 0.0069±0.0040 0.117+0.009
−0.008 		5.76161+0.00084
−0.00071 		1080 transit 0.735+0.334
−0.224 		5682±138 [5]
K2-370 b 0.0327±0.0207 0.286+0.020
−0.048 		2.14084+0.00003
−0.00004 		1420 transit 0.984+0.428
−0.303 		5377±138 [5]
K2-371 b 4.7±2.2 1.162+0.082
−0.077 		3.11490±0.00001 1000 transit 0.958+0.44
−0.298 		4925±138 [5]
K2-372 b 0.0289±0.0168 0.262±0.006 9.84407+0.00056
−0.00057 		870 transit 0.847+0.101
−0.088 		5479±27 [5]
K2-373 b 0.0162±0.0089 0.184+0.013
−0.012 		11.02066+0.00143
−0.00136 		1130 transit 1.158+0.499
−0.349 		6138±138 [5]
K2-374 b 0.0113±0.0058 0.142±0.005 4.52195+0.00032
−0.00040 		1210 transit 0.731+0.067
−0.061 		5789±21 [5]
K2-374 c 0.0179±0.0109 0.197+0.008
−0.007 		16.43445+0.00237
−0.00270 		790 transit 0.731+0.067
−0.061 		5789±21 [5]
K2-375 b 0.0183±0.0106 0.200+0.016
−0.015 		14.45389+0.00477
−0.00417 		1000 transit 1.119+0.492
−0.344 		5822±138 [5]
K2-376 b 0.0129±0.0074 0.155+0.011
−0.010 		5.77647+0.00026
−0.00023 		1240 transit 0.908+0.394
−0.281 		5937±138 [5]
K2-377 b 0.0123±0.0073 0.151+0.013
−0.011 		12.83223+0.00155
−0.00161 		530 transit 0.821+0.371
−0.258 		4200±138 [5]
K2-378 b 0.0283±0.0173 0.257+0.024
−0.020 		2.06043+0.00011
−0.00007 		1130 transit 0.923+0.425
−0.291 		4823±138 [5]
K2-379 b 0.0175±0.0104 0.194+0.032
−0.017 		8.77724+0.00062
−0.00061 		680 transit 0.856+0.375
−0.265 		4603±138 [5]
K2-380 b 0.0250±0.0144 0.243+0.016
−0.015 		9.40131+0.00046
−0.00050 		1110 transit 0.993+0.416
−0.302 		5911±138 [5]
K2-381 b 0.0040±0.0026 0.095+0.012
−0.009 		7.93893±0.00059 670 transit 0.754+0.337
−0.239 		4473±138 [5]
K2-381 c 0.0158±0.0094 0.178+0.016
−0.013 		16.03465+0.00184
−0.00157 		530 transit 0.754+0.337
−0.239 		4473±138 [5]
K2-381 d 0.0121±0.0070 0.150+0.016
−0.012 		26.80302+0.00277
−0.00304 		440 transit 0.754+0.337
−0.239 		4473±138 [5]
K2-382 b 0.0162±0.0101 0.185+0.013
−0.011 		21.70015+0.00202
−0.00191 		610 transit 0.922+0.401
−0.284 		5452±138 [5]
K2-383 b 0.0102±0.0052 0.139+0.010
−0.009 		1.86596±0.00001 1270 transit 1.061+0.459
−0.327 		5129±138 [5]
K2-384b [ja] 0.0040±0.0026 0.096+0.020
−0.005 		2.23152+0.0019
−0.00032 		600 transit 0.330±0.009 3623±138 [5]
K2-384c [ja] 0.0054±0.0027 0.106+0.004
−0.006 		4.19476+0.00030
−0.00018 		480 transit 0.330±0.009 3623±138 [5]
K2-384d [ja] 0.0085±0.0044 0.124+0.010
−0.006 		6.67958+0.00071
−0.00049 		410 transit 0.330±0.009 3623±138 [5]
K2-384e [ja] 0.0075±0.0042 0.120+0.012
−0.007 		9.71504+0.00100
−0.00073 		370 transit 0.330±0.009 3623±138 [5]
K2-384f [ja] 0.0179±0.0104 0.198+0.008
−0.007 		13.62749+0.00034
−0.00057 		330 transit 0.330±0.009 3623±138 [5]
K2-385 b 0.0100±0.0056 0.137+0.012
−0.011 		2.38086+0.00016
−0.00021 		1100 transit 1370±20 0.9270+0.4120
−0.2860 		4844±138 [5]
K2-386 b 0.0195±0.0115 0.207+0.006
−0.005 		7.47322+0.00037
−0.00031 		1010 transit 1400±30 0.911+0.088
−0.083 		5749±22 [5]
K2-387 b 0.1430±0.0996 0.653±0.023 28.73532±0.00099 340 transit 870±12 0.570+0.051
−0.048 		3572±138 [5]
K2-388 b 0.0412±0.0263 0.326+0.029
−0.020 		6.33906+0.00022
−0.00018 		970 transit 948±13 0.8420+0.3760
−0.2590 		5367±138 [5]
K2-389 b 0.0177±0.0103 0.195±0.010 8.58404+0.00088
−0.00202 		1050 transit 846±9 0.8020+0.3570
−0.2460 		5782±138 [5]
K2-389 c 0.0165±0.0085 0.182+0.013
−0.012 		20.85133+0.00280
−0.00298 		780 transit 846±9 0.8020+0.3570
−0.2460 		5782±138 [5]
K2-390 b 0.0636±0.0390 0.416+0.027
−0.030 		3.31279±0.00010 1310 transit 1490±18 0.7890+0.3510
−0.2390 		5558±138 [5]
K2-391 b 0.0078±0.0053 0.122+0.025
−0.016 		4.62265+0.00022
−0.00025 		900 transit 1660±50 0.7570+0.3410
−0.2400 		5543±138 [5]
K2-392 b 0.0140±0.0079 0.165+0.014
−0.013 		15.39872+0.00242
−0.00193 		840 transit 1330±30 0.8410+0.3700
−0.2580 		5726±138 [5]
K2-393 b 0.0199±0.0127 0.210+0.015
−0.014 		10.41318+0.00093
−0.00069 		950 transit 867±9 0.8810+0.3810
−0.2690 		5678±138 [5]
K2-394 b 0.0123±0.0063 0.151+0.012
−0.011 		5.09571±0.00011 890 transit 319.7±1.5 0.478+0.214
−0.147 		4938±138 [5]
K2-395 b 0.0240±0.0141 0.231+0.017
−0.015 		4.80335+0.00035
−0.00046 		910 transit 935±10 0.9520+0.4210
−0.2930 		5007±138 [5]
K2-395 c 0.0371±0.0220 0.303+0.025
−0.022 		8.49128+0.00033
−0.00030 		750 transit 935±10 0.9520+0.4210
−0.2930 		5007±138 [5]
K2-396 b 0.0106±0.0061 0.140+0.010
−0.009 		0.6736±0.00001 1990 transit 897±9 0.9540+0.4290
−0.2930 		5236±138 [5]
K2-396 c 0.0314±0.0189 0.278+0.015
−0.010 		25.76051+0.00199
−0.00188 		590 transit 897±9 0.9540+0.4290
−0.2930 		5236±138 [5]
K2-397 b 0.0212±0.0127 0.216±0.016 3.57232+0.00018
−0.00015 		1210 transit 650±5 0.9370+0.4060
−0.2850 		5387±138 [5]
K2-398 b 0.0191±0.0112 0.203+0.010
−0.009 		6.39302+0.00113
−0.00075 		1240 transit 1980±40 0.9450+0.0900
−0.0830 		5946±20 [5]
K2-398 c 0.0736±0.0412 0.455±0.013 18.78783+0.00087
−0.00099 		870 transit 1980±40 0.9450+0.0900
−0.0830 		5946±20 [5]
K2-399 b 0.1015±0.0697 0.540+0.093
−0.042 		0.75997±0.00001 2780 transit 1680±40 0.783+0.131
−0.114 		5690±38 [5]
K2-400 b 0.0051±0.0025 0.103±0.004 3.86505±0.00018 570 transit 203.5±0.8 0.374±0.009 3578±138 [5]
K2-401 b 0.0183±0.0117 0.201+0.018
−0.017 		6.29309+0.00057
−0.00070 		660 transit 655±5 0.8700+0.3950
−0.2690 		4213±138 [5]
K2-402 b 0.0245±0.0149 0.239+0.019
−0.017 		17.27474+0.00259
−0.00317 		870 transit 1710±60 0.9440+0.4190
−0.2900 		5716±138 [5]
K2-403 b 0.0783±0.0515 0.476+0.031
−0.034 		33.58977±0.00076 580 transit 804±8 0.7840+0.3400
−0.2410 		5511±138 [5]
K2-404 b 0.0230±0.0127 0.225±0.007 13.11536+0.00044
−0.00060 		450 transit 397±2 0.552±0.015 3748±138 [5]
K2-405 b 0.0586±0.0342 0.407+0.007
−0.010 		3.43547±0.00003 980 transit 643±7 1.034+0.459
−0.314 		4927±138 [5]
K2-406 b 0.063±0.039 0.410+0.027
−0.026 		22.5494+0.00137
−0.00143 		720 transit 278±2 0.7980+0.3390
−0.2450 		5784±138 [5]
K2-407 b 0.0066±0.0035 0.114+0.008
−0.007 		4.9419+0.00066
−0.00069 		1110 transit [5]
K2-407 c 0.0078±0.0044 0.121+0.008
−0.007 		9.22453+0.00132
−0.00091 		900 transit [5]
K2-408 b 0.0122±0.0062 0.149+0.010
−0.009 		20.97895+0.00130
−0.00124 		610 transit [5]
K2-409 b 0.0212±0.0127 0.221+0.015
−0.014 		1.90808+0.00004
−0.00005 		1800 transit [5]
K2-2016-BLG-0005Lb 1.1±0.1 4.4+1.9
−0.4 		4700+3300
−700 		microlensing 17000±700 0.58±0.03 [1]
Kepler-451 c 1.61±0.14 1460±90 2.1±0.2 timing 1340±20 0.48+0.12 [40]
Kepler-451 d 1.76±0.18 43.0±0.1 0.20±0.03 timing 1340±20 0.48+0.12 [40]
Kepler-1656 c 0.40±0.09 1919+27
−24 		3.053±0.049 radial vel. 1.03±0.04 [41]
Kepler-1708b <4.6 0.8886+0.0535
−0.0526 		737.11310+0.00146
−0.00770 		1.64±0.10 transit 5436+334
−298 		1.088±0.072 6157+231
−202 		Possible exomoon host[42][43]
Kepler-1972b [ja] 0.0064±0.0019 0.072±0.004 7.54425±0.00054 transit 923±3 1.12±0.03 5818±27 Very dense planets, additional planet in system suspected[44]
Kepler-1972c [ja] 0.0066±0.0020 0.078±0.005 11.3295±0.0011 transit 923±3 1.12±0.03 5818±27 Very dense planets, additional planet in system suspected[44]
KMT-2016-BLG-1105b 0.007+0.023
−0.005 		2.44+0.88
−0.75 		microlensing 17000±7000 0.41+0.25
−0.21 		[45]
KMT-2017-BLG-0428b 0.018+0.011
−0.009 		1.81+0.55
−0.59 		microlensing 18000+6000
−8000 		0.34+0.22
−0.17 		[45]
KMT-2017-BLG-0673Lb 3.67+2.17
−2.07 		2.34+0.56
−0.74 		microlensing 17000+4000
−5000 		0.63+0.37
−0.35 		[46]
KMT-2017-BLG-1003b 0.016+0.017
−0.009 		1.38+0.39
−0.32 		microlensing 23000±2000 0.32+0.31
−0.17 		[45]
KMT-2017-BLG-1194b 0.011±0.006 1.78+0.45
−0.46 		microlensing 14000±6000 0.41+0.23
−0.19 		[45]
KMT-2018-BLG-0030b 1.45+1.23
−0.88 		4.39+2.18
−2.40 		microlensing 21000+4000
−6000 		0.51+0.43
−0.31 		[47]
KMT-2018-BLG-0087b 0.23+0.32
−0.12 		0.87+0.24
−0.25 		microlensing 23000+3000
−4000 		0.10+0.14
−0.05 		[47]
KMT-2018-BLG-0247b 2.11+2.09
−1.04 		2.46+0.51
−0.58 		microlensing 22000+3000
−4000 		0.29+0.28
−0.14 		[47]
KMT-2018-BLG-2004b 0.27±\0.12 4.62+0.80
−1.10 		microlensing 23000+3000
−4000 		0.69+0.32
−0.31 		[48]
KMT-2018-BLG-2602b 1.15+0.73
−0.63 		3.81+2.96
−2.32 		microlensing 14000±6000 0.66+0.42
−0.36 		[47]
KMT-2018-BLG-2718b 16.0+11.7
−8.0 		4.86+2.97
−2.55 		microlensing 15000+10000
−7000 		0.82+0.57
−0.39 		[48]
KMT-2019-BLG-0414Lb 4.57+3.74
−2.06 		1.16+0.47
−0.51 		microlensing 14000+5000
−6000 		0.74+0.43
−0.38 		[46]
KMT-2019-BLG-1042Lb 0.19+0.21
−0.11 		1.7±0.5 microlensing 22000+3000
−5000 		0.30+0.34
−0.18 		[49]
KMT-2019-BLG-1367b 0.013+0.008
−0.007 		1.70+0.50
−0.56 		microlensing 15000+8000
−7000 		0.25+0.16
−0.13 		[45]
KMT-2019-BLG-1552Lb 4.05+1.73
−1.85 		2.6+0.6
−0.8 		microlensing 15000+6000
−5000 		0.79+0.33
−0.36 		[49]
KMT-2019-BLG-1806b 0.015±0.005 3.02+0.70
−0.73 		microlensing 22000+2000
−7000 		0.74±0.25 [45]
KMT-2019-BLG-2974Lb 0.28+0.29
−0.18 		2.0+0.8
−0.7 		microlensing 20000+5000
−7000 		0.47+0.41
−0.28 		[49]
KMT-2021-BLG-0171Lb 0.0352+0.0173
−0.0142 		3.5+1.3
−1.0 		microlensing 15000+5000
−4000 		0.78+0.29
−0.26 		[50]
KMT-2021-BLG-0240 b 0.40+0.07
−0.08 		2.5+2.8
−1.9 		microlensing 23000+3000
−5000 		0.47+0.33
−0.24 		Multiple solutions for orbital separation[51]
KMT-2021-BLG-0240 c 0.64+0.25
−0.24 		1.0+1.1
−0.8 		microlensing 23000+3000
−5000 		0.47+0.33
−0.24 		Multiple solutions for orbital separation[51]
KMT-2021-BLG-0320Lb 0.10+0.13
−0.07 		1.54+0.24
−0.30 		microlensing 23000+3000
−4000 		0.32+0.39
−0.21 		[52]
KMT-2021-BLG-0748b 0.45+0.40
−0.25 		2.43±0.67 microlensing 20000+3000
−4000 		0.36+0.32
−0.20 		[53]
KMT-2021-BLG-0119Lb 5.97+2.94
−2.60 		3.23+0.76
−0.80 		microlensing 11000+6000
−4000 		0.69+0.34
−0.30 		Multiple orbital solutions[54]
KMT-2021-BLG-0192Lb 0.19+0.09
−0.10 		2.07+0.35
−0.47 		microlensing 22000+3000
−5000 		0.55+0.26
−0.28 		Multiple orbital solutions[54]
KMT-2021-BLG-0712b 0.12+0.06
−0.04 		2.22+0.66
−0.48 		microlensing 10000+3000
−2000 		0.22+0.12
−0.07 		[55]
KMT-2021-BLG-0909b 1.26+1.01
−0.66 		1.75±0.42 microlensing 21000+3000
−5000 		0.38+0.30
−0.20 		[55]
KMT-2021-BLG-1077Lb 0.22+0.31
−0.12 		1.26+1.41
−1.08 		microlensing 27000±3000 0.14+0.19
−0.07 		[56]
KMT-2021-BLG-1077Lc 0.25+0.35
−0.13 		0.93+1.05
−0.80 		microlensing 27000±3000 0.14+0.19
−0.07 		[56]
KMT-2021-BLG-1105b 1.30±0.68 3.54±1.06 microlensing 15000±5000 0.63±0.33 [55]
KMT-2021-BLG-1253b 0.0599+0.0643
−0.0319 		1.52+0.57
−0.41 		microlensing 22000+3000
−4000 		0.24+0.26
−0.13 		[53]
KMT-2021-BLG-1303Lb 0.38+0.22
−0.20 		2.89+0.44
−0.66 		microlensing 20000+3000
−5000 		0.57+0.32
−0.29 		Host star also known as MOA-2021-BLG-182[52]
KMT-2021-BLG-1372b 0.1928±0.1129 2.37±0.77 microlensing 19000+5000
−8000 		0.42±0.25 [53]
KMT-2021-BLG-1391b 0.0143±0.0073 2.29+0.56
−0.71 		microlensing 19000+3000
−5000 		0.37±0.19 [53]
KMT-2021-BLG-1554Lb 0.12+0.20
−0.07 		0.72+0.13
−0.14 		microlensing 25000+3000
−4000 		0.08+0.13
−0.04 		[52]
KMT-2021-BLG-1689Lb 0.145+0.094
−0.072 		2.5+0.8
−06 		microlensing 23000+2000
−4000 		0.58+0.33
−0.27 		[50]
KMT-2021-BLG-1898 b 0.73+0.50
−0.40 		1.9+0.3
−0.5 		microlensing 23000+3000
−4000 		0.48+0.33
−0.26 		Possibly a binary star system[57]
KMT-2021-BLG-2294Lb 0.07+0.10
−0.03 		0.94±0.16 microlensing 22000±3000 0.11+0.17
−0.06 		Multiple orbital solutions[54]
KMT-2021-BLG-2478b 0.80+0.56
−0.35 		1.38±0.26 microlensing 8000+4000
−3000 		0.12+0.09
−0.06 		[55]
L 363-38 b 0.0147±0.0014 8.781±0.007 0.048±0.006 330 radial vel. 33.31 0.21 3129 Host star also known as Gliese 3049[58]
MOA-2019-BLG-008L b 30 microlensing 8000±2000 0.8 [59]
MOA-2020-BLG-135Lb 0.036+0.060
−0.021 		1.11+0.23
−0.20 		microlensing 26000±3000 0.23+0.39
−0.14 		[60]
MOA-2020-BLG-208Lb 0.217+0.116
−0.106 		2.88+0.40
−0.41 		microlensing 25000±3000 0.656+0.346
−0.322 		[61]
Mu2 Scorpii b 14.4 290 imaging 474 9.1 21900 [62]
Mu2 Scorpii c 18.5 21 imaging 474 9.1 21900 [62]
NGTS-20 b 2.98+0.16
−0.15 		1.07±0.04 54.18915±0.00015 0.313±0.013 688+14
−13 		transit 1195±8 1.47±0.09 5980±80 Planet on eccentric orbit, host star also known as TOI-5152[63]
NGTS-21b 2.36±0.21 1.33±0.03 1.5433897±0.0000016 0.0236±0.0005 1357±15 transit 2090+90
−80 		0.72±0.04 4660±41 [64]
NGTS-23b 0.613±0.097 1.267±0.030 4.0764326±0.0000041 0.0504±0.012 1327+17
−16 		transit 3230±70 1.01+0.06
−0.07 		6057±64 [65]
NGTS-24b 0.52+0.12
−0.11 		1.214+0.058
−0.062 		3.4678796±0.0000070 0.0479+0.0028
−0.0030 		1499+41
−36 		transit 2360±80 1.26+0.05
−0.21 		5820+93
−8 		[65]
NGTS-25b 0.639+0.058
−0.052 		1.023+0.035
−0.052 		2.8230930±0.0000033 0.0388+0.0014
−0.002 		1101+15
−14 		transit 2350±30 0.91+0.03
−0.04 		5321±58 [65]
OGLE-2016-BLG-1093Lb 0.71±0.12 2.13±0.33 microlensing 26000±2000 0.46±0.08 [66]
OGLE-2017-BLG-1691Lb 0.046+0.037
−0.025 		2.41+0.34
−0.44 		microlensing 24000+3000
−4000 		0.45+0.36
−0.25 		Host star also known as KMT-2017-BLG-0752[52]
OGLE-2017-BLG-1806b 0.017+0.015
−0.009 		1.75+0.46
−0.47 		microlensing 21000+3000
−5000 		0.38+0.34
−0.20 		[45]
OGLE-2018-BLG-0298Lb 0.14+0.07
−0.06 		2.86+0.73
−0.80 		microlensing 21000+3000
−4000 		0.69+0.34
−0.30 		[47]
OGLE-2018-BLG-0932b 0.89+0.36
−0.31 		1.75+0.24
−0.23 		microlensing 22000±3000 0.72+0.29
−0.25 		[48]
OGLE-2018-BLG-1119Lb 0.91+0.66
−0.52 		4.06+2.14
−2.58 		microlensing 19000+5000
−8000 		0.48+0.35
−0.28 		[47]
OGLE-2018-BLG-1126b 0.056+0.033
−0.031 		3.23+1.29
−1.71 		microlensing 19000+6000
−8000 		0.69+0.41
−0.38 		[48]
OGLE-2018-BLG-1212b 0.20+0.16
−0.13 		1.68+1.47
−0.63 		microlensing 5100+4100
−1800 		0.16+0.12
−0.10 		[48]
OGLE-2018-BLG-1367b 0.95+0.75
−0.44 		3.63+1.02
−0.96 		microlensing 0.28+0.22
−0.13 		Multiple solutions for frojected separation[48]
OGLE-2018-BLG-1544b 11.2+6.3
−5.9 		6.21+1.32
−2.10 		microlensing 21000+4000
−7000 		0.62+0.38
−0.36 		Multiple solutions for frojected separation[48]
OGLE-2018-BLG-1647b 0.97+1.78
−0.56 		1.36+0.20
−0.17 		microlensing 26000+4000
−3000 		0.092+0.170
−0.053 		[48]
OGLE-2019-BLG-0362Lb 3.26+0.83
−0.58 		2.18+0.58
−0.72 		microlensing 19000±2000 0.42+0.34
−0.23 		Multiple solutions for planetary parameters[67]
OGLE-2019-BLG-1470LABc 2.2+1.8
−1.3 		3.1+1.2
−1.1 		microlensing 20000±4000 0.55+0.17 Circumbinary planet[68]
Pi Mensae d 0.0421±0.0042 124.64+0.48
−0.52 		radial vel. 59.62±0.07 1.11±0.01 6013±18 [69]
Proxima Centauri d 0.0008±0.0002 5.122+0.002
−0.0036 		0.02885+0.00019
−0.00022 		360 radial vel. 4.2465±0.0003 0.1221±0.0022 2900±100 [70]
PSR J2007+3120 b 0.0072±0.0009 723±8 timing 22000 Pulsar planet, another planet in the system is suspected.[71]
Ross 508 b 0.0126±0.0019 10.76+0.01
−0.02 		0.05353+0.00047
−0.00051 		radial vel. 36.594±0.011 0.1774±0.0045 3071+34
−22 		Host star also known as Gliese 585, planet close to habitable zone.[72]
TOI-181b 0.127891+0.013510
−0.025081 		0.631521+0.007554
−0.009811 		4.532058+0.000002
−0.000002 		0.055780+0.005563
−0.003893 		878+32
−41 		transit 314±2 0.781±0.042 4994±50 [73]
TOI-206 b 0.116±0.004 0.7363104±0.0000003 0.0112±0.0001 910±36 transit 155.9 0.35±0.01 3383±157 [74]
TOI-277 b 0.0239+0.0179
−0.0098 		0.237±0.016 3.9940±0.0004 0.0269±0.0011 transit 212.6+0.6
−0.3 		0.16±0.01 4031+21
−23 		[75]
TOI-500 b 0.104±0.010 0.5481579±0.0000006 0.0128±0.0011 1693±105 transit 154.8 0.88±0.25 4621±50 [74]
TOI-544 b 0.181±0.009 1.5483510±0.0000015 0.0251 ± 0.0019 1082±47 transit 132.7 0.85±0.20 4369±100 [74]
TOI-620 b 5.0988179+0.0000045
−0.0000046 		0.04825+0.00065
−0.00066 		603.6+5.5
−5.3 		transit 107.81±0.19 0.577+0.024
−0.023 		3708+57
−56 		[76]
TOI-778 b 2.76±0.24 1.375±0.045 4.633611±0.000001 0.060±0.003 1561+33
−32 		transit 530±4 1.428±0.094 6715±128 [77]
TOI-833 b 0.113±0.006 1.0418777±0.0000324 0.0171±0.0003 1118±49 transit 136.3 0.61±0.03 3920±160 [74]
TOI-969 b 0.0286±0.0031 0.247±0.033 1.8237305+0.0000020
−0.0000021 		0.02636±0.00017 941±31 transit 253.8±0.5 0.730±0.037 4550±75 [78]
TOI-969 c 11.3+1.1
−0.9 		1700+290
−280 		2.52+0.27
−0.29 		96.4+6.8
−5.8 		radial vel. 253.8±0.5 0.730±0.037 4550±75 Eccentric orbit[78]
TOI-1064b 0.0425±0.0055 0.231±0.004 6.443868±0.000025 0.06152+0.00086
−0.00089 		784±13 transit 224.5±0.2 0.748±0.032 4734±67 [79]
TOI-1064c 0.0079+0.0057
−0.0063 		0.237±0.004 12.226574+0.000046
−0.000043 		0.09429+0.00132
−0.00136 		634±10 transit 224.5±0.2 0.748±0.032 4734±67 [79]
TOI-1075 b 0.154±0.007 0.6047328±0.0000032 0.0118±0.0001 1336±56 transit 200.9 0.60±0.02 3921±157 [74]
TOI-1075 b 0.0313±0.0042 0.160+0.010
−0.007 		0.6047328±0.0000032 0.01159+0.00023
−0.00020 		1323±44 transit 200.4+0.6
−2.2 		0.604±0.030 3875±75 [80]
TOI-1107b 3.35±0.18 1.30±0.05 4.0782387+0.0000024
−0.0000025 		0.0561+0.0024
−0.0025 		1728±27 transit 925±7 1.35±0.08 6311±98 [81]
TOI-1136 b 0.0095+0.0022
−0.0028 		0.170+0.019
−0.013 		4.1728±0.0002 transit 275.8±0.5 1.022±0.027 5770±50 [82]
TOI-1136 c 0.0189+0.0041
−0.0053 		0.257±0.005 6.2573±0.0002 transit 275.8±0.5 1.022±0.027 5770±50 [82]
TOI-1136 d 0.0252+0.0076
−0.0060 		0.413±0.007 12.5194±0.0004 transit 275.8±0.5 1.022±0.027 5770±50 [82]
TOI-1136 e 0.0170±0.0031 0.236+0.006
−0.008 		18.7992+0.0017
−0.0015 		transit 275.8±0.5 1.022±0.027 5770±50 [82]
TOI-1136 f 0.0261+0.0088
−0.0113 		0.346±0.010 26.3162+0.0017
−0.0013 		transit 275.8±0.5 1.022±0.027 5770±50 [82]
TOI-1136 g 0.0151+0.0148
−0.0104 		0.226±0.010 39.5387+0.0036
−0.0030 		transit 275.8±0.5 1.022±0.027 5770±50 [82]
TOI-1181 b 1.18±0.14 1.30±0.08 2.103195+0.000012
−0.000011 		2162 transit 1013±3 1.38+0.086
−0.082 		6260±100 Subgiant host star[83]
TOI-1221 b 0.259±0.011 91.68278+0.00032
−0.00041 		0.404+0.026
−0.023 		400 transit 447.1±0.7 1.03±0.06 5592±50 [84]
TOI-1246 b [ja] 0.0255±0.0035 0.269±0.005 4.30744±0.00002 0.049±0.002 955 transit 557.9±1.0 1.12±0.16 5217±50 [85]
TOI-1246 c [ja] 0.0277±0.0038 0.224±0.007 5.904144±0.000083 0.061±0.002 860 transit 557.9±1.0 1.12±0.16 5217±50 [85]
TOI-1246 d [ja] 0.0167±0.0053 0.313±0.008 18.65590±0.00048 0.131±0.004 586 transit 557.9±1.0 1.12±0.16 5217±50 [85]
TOI-1246 e [ja] 0.0466±0.0072 0.338±0.014 37.9216±0.0010 0.211±0.007 462 transit 557.9±1.0 1.12±0.16 5217±50 [85]
TOI-1260 d 0.0373±0.0245 0.276±0.008 16.608164±0.000083 0.1116±0.0033 499±4 transit 239.5±0.3 0.66±0.01 4227±85 [86]
TOI-1268 b 0.303±0.026 0.81±0.05 8.1577080±0.0000044 0.072+0.009
−0.010 		919 transit 359.1±0.4 0.92±0.03 5290±117 [87]
TOI-1272 b 0.0774±0.0072 0.370±0.019 3.31599±0.00002 0.0412±0.0008 961±32 transit 450.6±1.3 0.851±0.049 4985±121 [88]
TOI-1272 c 0.0840±0.0098 8.689±0.008 0.0783±0.0014 697±23 radial vel. 450.6±1.3 0.851±0.049 4985±121 [88]
TOI-1288 b 0.0712+0.0574
−0.0304 		0.454±0.010 2.69998±0.00015 0.0429±0.0006 transit 375.3+1.3
−0.5 		1.46±0.06 5307+18
−16 		[75]
TOI-1288 c 0.2643±0.0220 443+11
−13 		radial vel. 375.3+1.3
−0.5 		1.46±0.06 5307+18
−16 		[89]
TOI-1411 b 0.121±0.013 1.4520358±0.0000098 0.0230±0.0026 1136±59 transit 106.0 0.59±0.23 4266±100 [74]
TOI-1422 b 0.0283+0.0072
−0.0063 		0.354+0.012
−0.010 		12.9972±0.0006 0.108±0.003 867±17 transit 504.17+0.12
−0.09 		0.981+0.062
−0.065 		5840±62 Another planet in the system is suspected.[90]
TOI-1442 b 0.104±0.005 0.4090677±0.0000003 0.0071±0.0002 1072±54 transit 134.5 0.29±0.02 3330±160 [74]
TOI-1452 b 0.0152±0.0041 0.149±0.006 11.06201±0.00002 0.061±0.003 326±7 transit 99.51±0.04 0.249±0.008 3185±50 Also a red dwarf on a 97AU separation in the system[91]
TOI-1468 b 0.0101±0.0008 0.114±0.003 1.8805136+0.0000024
−0.0000026 		682.2+7.4
−6.9 		transit 80.64±0.07 0.339±0.011 3496±25 [92]
TOI-1468 c 0.0209±0.0021 0.184±0.004 15.532482+0.000034
−0.000033 		337.5+3.7
−3.4 		transit 80.64±0.07 0.339±0.011 3496±25 [92]
TOI-1516 b 3.16±0.12 1.36±0.03 2.056014±0.000002 1820 transit 804.6±1.9 1.085+0.061
−0.066 		6420±100 [83]
TOI-1669 b 0.0132±0.0085 0.214±0.016 2.7 transit 364.6 1.00±0.05 5542.3±100.0 [93] Host star also known as BD+82 71, planet suspected since 2020[94]
TOI-1669 c 0.602±0.078 501±16 radial vel. 364.6 1.00±0.05 5542.3±100.0 [93] Host star also known as BD+82 71, additional long-period companion is suspected.
TOI-1694 b 0.0979±0.0066 0.461±0.016 3.8 transit 405.7 0.84±0.03 5066±100 [93] Host star also known as TYC 4108-1434-1, planet suspected since 2020[94]
TOI-1694 c 0.929±0.037 393.2±4.3 radial vel. 405.7 0.84±0.03 5066±100 [93] Host star also known as TYC 4108-1434-1
TOI-1670 b 0.04±0.03 0.184+0.017
−0.013 		10.98462+0.00046
−0.00051 		0.103±0.002 1062+14
−13 		transit 540.6+1.0
−1.2 		1.21±0.02 6170±61 [95]
TOI-1670 c 0.63+0.09
−0.08 		0.987±0.025 40.74976+0.000022
−0.00021 		0.249±0.005 684±9 transit 540.6+1.0
−1.2 		1.21±0.02 6170±61 [95]
TOI-1693 b 0.126±0.009 1.7666957±0.0000054 0.0226±0.0004 764±19 transit 100.6 0.49±0.03 3499±70 [74]
TOI-1695 b 0.0173±0.0031 0.181±0.016 3.1342790±0.0000072 0.033548+0.000260
−0.000268 		590±90 transit 147.2±0.2 0.51±0.02 3627±31 [96][97]
TOI-1696 b 0.1781 0.276±0.010 2.500311±0.000004 0.0229±0.0002 489±13 transit 210.8±0.5 0.255±0.0066 3185±76 [98][99]
TOI-1710 b 0.0890±0.0148 0.477±0.010 24.283429±0.00043 0.16±0.04 687±50 transit 264.7±0.2 0.984+0.050
−0.059 		5665±55 [100]
TOI-1759 b 0.021±0.06 0.279±0.02 18.849975±0.000006 0.1176±0.0013 433±14 transit 130.85±0.05 0.606±0.020 4065±51 [101][102]
TOI-1811 b 0.974+0.075
−0.076 		1.002+0.026
−0.024 		3.7130818±0.0000028 0.04393+0.00058
−0.00054 		961.5±8 transit 418±3 0.819+0.033
−0.030 		4753+54
−55 		[103]
TOI-1820 b 2.3±0.2 1.12±0.02 4.860700±0.000010 0.069±0.005 1295±11 transit 807±13 1.04±0.13 5734±50 [104]
TOI-1860 b 0.117±0.005 1.0662107±0.0000014 0.0204±0.0002 1885±28 transit 149.8 0.99±0.03 5752±100 [74]
TOI-1937 b 2.01+0.17
−0.16 		1.247+0.059
−0.062 		0.94667944±0.00000047 0.01932+0.00035
−0.00039 		2097+35
−36 		transit 1366±6 1.072+0.059
−0.064 		5814+91
−93 		[105]
TOI-2000 b 0.0324±0.0070 0.236±0.010 3.098331+0.000021
−0.000019 		0.04260+0.00076
−0.00067 		1475+120
−158 		transit 566.3±1.0 1.074+0.059
−0.050 		5607+86
−82 		[106]
TOI-2000 c 0.238±0.012 0.711±0.011 9.1270553±0.0000073 0.0875+0.0016
−0.0014 		1029+84
−111 		transit 566.3±1.0 1.074+0.059
−0.050 		5607+86
−82 		[106]
TOI-2025 b 4.4±0.4 1.120±0.009 8.872086±0.000009 0.089±0.004 1186±11 transit 1106±7 1.32±0.14 5880±53 [104]
TOI-2025 b 3.51+0.36
−0.35 		1.118+0.031
−0.030 		8.8720942+0.0000080
−0.0000079 		0.0886+0.0019
−0.0024 		1172+18
−17 		transit 1095±11 1.176+0.079
−0.091 		5928+76
−75 		[103]
TOI-2046 b 2.30±0.08 1.44±0.11 1.4971842+0.0000031
−0.0000033 		1998 transit 940±3 1.153+0.100
−0.093 		6160±100 Young host star[83]
TOI-2048 b 0.184±0.018 13.79019+0.00065
−0.00084 		640±20 transit 379.7±0.5 0.83±0.03 5185±60 Young host star belongs to NGC 3532[107]
TOI-2081 b 0.0157+0.0151
−0.0076 		0.182±0.046 10.50534+0.00007
−0.00008 		0.0752+0.0047
−0.0119 		488+28
−52 		transit 203.26±0.16 0.540±0.080 3800±100 [108]
TOI-2136 b 0.0200+0.0077
−0.0072 		0.196±0.015 7.851928+0.000018
−0.000016 		0.057±0.006 395+24
−22 		transit 108.82±0.07 0.34±0.02 3342±100 [109][110]
TOI-2145 b 5.35+0.32
−0.35 		1.103+0.031
−0.029 		10.261081+0.000026
−0.000027 		0.1108+0.0012
−0.0015 		1484+16
−14 		transit 733±5 1.720+0.057
−0.068 		6189±67 Host star also known as HIP 86040[103]
TOI-2152A b 2.83+0.38
−0.37 		1.281+0.050
−0.046 		3.3773512+0.0000060
−0.0000061 		0.05064+0.00093
−0.0011 		1802+60
−54 		transit 988±13 1.516+0.085
−0.10 		6630+300
−290 		Planet orbiting primary of binary star[103]
TOI-2154 b 0.92+0.19
−0.18 		1.453+0.053
−0.048 		3.8240801±0.0000025 0.0513+0.0011
−0.0013 		1580±27 transit 967±10 1.233+0.077
−0.090 		6280±160 [103]
TOI-2180 b 2.755+0.087
−0.081 		1.010+0.022
−0.019 		260.79+0.59
−0.58 		0.828±0.012 348.0+3.3
−3.6 		transit 379.4±0.8 1.111+0.047
−0.046 		5695+58
−60 		[111]
TOI-2158 b 0.82±0.08 0.960±0.012 8.60077±0.00003 0.075±0.004 1188±10 transit 652±3 1.12±0.12 5673±50 [104]
TOI-2193 b 0.94±0.18 1.77 2.1225735±0.0000016 0.03319+0.00052
−0.00051 		1763+21
−22 		transit 1126±3 1.082+0.052
−0.049 		5974±110 Also 0.54M☉ star in the system[112]
TOI-2196 b 0.0818±0.0041 0.313±0.013 1.1947268+0.0000079
−0.0000093 		0.02234±0.00060 1860±20 transit 861±3 1.032±0.038 5634±31 Neptunian desert planet[113]
TOI-2207 b 0.64+0.10
−0.12 		0.995+0.028
−0.027 		8.001968+0.000024
−0.000025 		0.0854+0.0015
−0.0016 		1259+16
−15 		transit 1242±9 1.296+0.069
−0.072 		6075±110 [112]
TOI-2260 b 0.145±0.012 0.3524728±0.0000047 0.0097±0.0001 2609±86 transit 331.2 0.99±0.04 5534±100 [74]
TOI-2236 b 1.58+0.40
−0.39 		1.282+0.032
−0.031 		3.5315902±0.0000026 0.05009+0.00080
−0.00082 		1688+19
−21 		transit 1149±5 1.343+0.066
−0.065 		6164±50 [112]
TOI-2337b 1.60±0.15 0.9±0.1 2.99432±0.00008 0.04467 transit 1780±20 1.325±0.118 4780±100 [114]
TOI-2364 b 0.225+0.043
−0.049 		0.768+0.023
−0.018 		4.0197517±0.0000043 0.04871+0.00069
−0.00079 		1091+17
−14 		transit 713±6 0.954+0.041
−0.046 		5306+76
−68 		[105]
TOI-2411 b 0.150±0.010 0.7826942±0.0000037 0.0144±0.0001 1355±45 transit 194.5 0.65±0.02 4099±123 [74]
TOI-2421 b 0.333±0.079 0.925+0.035
−0.034 		4.3474032+0.0000079
−0.0000078 		0.0543+0.0021
−0.0010 		1534+20
−28 		transit 1067±7 1.131+0.130
−0.064 		5577±50 [112]
TOI-2427 b 0.161±0.011 1.3060011±0.0000102 0.0202±0.0002 1117±46 transit 93.1 0.64±0.02 4072±121 [74]
TOI-2445 b 0.112±0.007 0.3711281±0.0000005 0.0064±0.0001 1060±54 transit 158.7 0.25±0.01 3333±157 [74]
TOI-2497 b 5.21±0.52 1.000+0.040
−0.038 		10.655661±0.000026 0.1167+0.0018
−0.0017 		1596+44
−41 		transit 930±14 1.861+0.086
−0.081 		7360+290
−270 		[103]
TOI-2567 b 0.201+0.034
−0.031 		0.975+0.031
−0.029 		5.983944±0.000013 0.0672+0.0024
−0.0012 		1352+18
−19 		transit 1691±8 1.130+0.130
−0.059 		5650±50 [112]
TOI-2570 b 0.820+0.063
−0.065 		1.217+0.035
−0.034 		2.9887615±0.0000022 0.04145+0.00081
−0.00086 		1431+24
−23 		transit 1179±6 1.063+0.063
−0.065 		5765±50 [112]
TOI-2583 b 0.250+0.058
−0.056 		1.290+0.040
−0.033 		4.5207265±0.0000049 0.0571+0.0010
−0.0013 		1456+19
−16 		transit 1831±9 1.215+0.063
−0.082 		5936+65
−68 		[105]
TOI-2587 b 0.218+0.054
−0.046 		1.077+0.042
−0.040 		5.456640±0.000011 0.0635+0.0025
−0.0013 		1445+23
−26 		transit 1242±10 1.15+0.14
−0.07 		5760+80
−79 		[105]
TOI-2669b 0.61±0.19 1.76±0.16 6.2034±0.0001 transit 1294±9 1.19±0.16 4800±100 [114]
TOI-2796 b 0.44+0.10
−0.11 		1.59 4.8084983+0.0000057
−0.0000056 		0.0569+0.0010
−0.0011 		1205+18
−17 		transit 1150±6 1.063+0.057
−0.062 		5764+81
−78 		[105]
TOI-2803 b 0.975+0.083
−0.070 		1.616+0.034
−0.032 		1.96229325±0.00000082 0.03185±0.00052 1893+29
−28 		transit 1635±9 1.118+0.056
−0.054 		6280+99
−96 		[105]
TOI-2818 b 0.71±0.26 1.363+0.046
−0.045 		4.0397090+0.0000024
−0.0000023 		0.0493+0.0010
−0.0008 		1376+26
−24 		transit 1028±3 0.977+0.063
−0.049 		5721+88
−83 		[105]
TOI-2842 b 0.370+0.052
−0.047 		1.146+0.051
−0.048 		3.5514058+0.0000077
−0.0000078 		0.0475+0.0010
−0.0011 		1471+29
−27 		transit 1501±8 1.135+0.077
−0.079 		5910±100 [105]
TOI-2977 b 1.68+0.26
−0.25 		1.174+0.031
−0.027 		2.3505614±0.0000025 0.03386+0.00067
−0.00050 		1544±26 transit 1160±30 0.936+0.057
−0.041 		5691+94
−93 		[105]
TOI-3023 b 0.62+0.10
−0.09 		1.466+0.043
−0.032 		3.9014971±0.0000031 0.0505+0.0015
−0.0009 		1596+24
−25 		transit 1281±5 1.12+0.11
−0.06 		5760+85
−88 		[105]
TOI-3331 b 2.27±0.16 1.158±0.043 2.0180231+0.0000043
−0.0000044 		0.03144+0.00048
−0.00055 		1488+31
−29 		transit 733±4 1.016+0.047
−0.052 		5521±110 Also 0.6M☉ star in the system[112]
TOI-3364 b 1.67+0.12
−0.13 		1.091+0.038
−0.032 		5.8768918±0.0000069 0.0675+0.0011
−0.0016 		1264+22
−21 		transit 899±3 1.186+0.059
−0.083 		5706+95
−91 		[105]
TOI-3540 b 1.18±0.14 2.10 3.1199990±0.0000079 0.04289+0.00092
−0.00093 		1498±22 transit 921±10 1.081+0.071
−0.069 		5969±50 Also 0.8M☉ star in the system[112]
TOI-3629 b 0.26±0.02 0.74±0.02 3.936551+0.000005
−0.000006 		0.043±0.002 690±20 transit 423.1±1.0 0.63±0.02 3870±90 [115]
TOI-3688 b 0.98+0.10
−0.11 		1.167+0.048
−0.044 		3.246075±0.000012 0.04560+0.00089
−0.00098 		1534+29
−28 		transit 1308±6 1.199+0.072
−0.076 		5950±100 [105]
TOI-3693 b 1.02+0.24
−0.22 		1.124+0.029
−0.023 		9.088516+0.000026
−0.000027 		0.0813+0.0011
−0.0012 		801+13
−12 		transit 576±2 0.867+0.036
−0.037 		5274±50 [112]
TOI-3714 b 0.70±0.003 1.01±0.03 2.154849±0.000001 0.027±0.001 750±20 transit 367.0+0.6
−1.3 		0.53±0.02 3660±90 [115]
TOI-3757 b 0.2684±0.0276 1.07+0.04
−0.05 		3.4387530+0.0000039
−0.0000040 		0.03845±0.00043 759±13 transit 579±2 0.64±0.02 3913±56 [116]
TOI-3807 b 1.04+0.15
−0.14 		2.00 2.8989727+0.0000038
−0.0000039 		0.0421+0.0007
−0.0011 		1646+25
−24 		transit 1399±7 1.181+0.064
−0.092 		5772+84
−80 		[105]
TOI-3819 b 1.11+0.18
−0.20 		1.172+0.036
−0.035 		3.2443141±0.0000055 0.04611+0.00069
−0.00096 		1633+21
−19 		transit 1834±17 1.242+0.057
−0.076 		5859+72
−71 		[105]
TOI-3884 b 0.0519+0.0110
−0.0057 		0.563±0.025 4.5445697±0.0000094 0.0354±0.0014 463±12 transit 141.37±0.16 0.2813±0.0067 3269±70 [117][118]
TOI-3912 b 0.406+0.071
−0.068 		1.274+0.041
−0.040 		3.4936264±0.0000038 0.0463+0.0012
−0.0010 		1512±20 transit 1533±9 1.088+0.086
−0.070 		5725+69
−68 		[105]
TOI-3976 b 0.175+0.037
−0.036 		1.095+0.036
−0.035 		6.607662+0.000016
−0.000015 		0.0743+0.0013
−0.0014 		1295+16
−14 		transit 1703±8 1.254+0.067
−0.072 		5975+70
−69 		[105]
TOI-4087 b 0.73±0.14 1.164+0.025
−0.024 		3.17748350±0.00000094 0.04469+0.00048
−0.00054 		1458+20
−17 		transit 1013±4 1.178+0.039
−0.042 		6060+74
−67 		[105]
TOI-4137 b 1.44+0.17
−0.15 		1.211+0.040
−0.039 		3.8016122±0.0000065 0.05222+0.00089
−0.00096 		1570+25
−24 		transit 1128±7 1.313+0.068
−0.071 		6134±50 [112]
TOI-4145 b 0.43±0.13 1.187+0.032
−0.031 		4.0664428±0.0000058 0.04823+0.00075
−0.00079 		1074+19
−16 		transit 668.7±1.3 0.905+0.043
−0.044 		5281+86
−76 		[105]
TOI-4329b 0.45±0.09 1.50±0.19 2.9223±0.00015 transit 2258±16 1.538±0.049 6000±100 [114]
TOI-4463 b 0.794+0.039
−0.040 		1.183+0.064
−0.045 		2.8807198+0.0000028
−0.0000027 		0.04036+0.00074
−0.00082 		1395+25
−22 		transit 579.5±1.8 1.056+0.059
−0.063 		5640+89
−82 		[105]
TOI-4479 b 0.0261+0.0252
−0.0126 		0.252±0.057 1.15890+0.00001
−0.00002 		0.0164+0.0015
−0.0029 		861+64
−103 		transit 262.9±0.3 0.452±0.090 3400±100 [108]
TOI-4562 b 3.29+1.88
−0.82 		1.072+0.044
−0.043 		225.11757+0.00027
−0.00025 		0.771±0.013 349±10 transit 1131±12 1.218+0.054
−0.048 		6096±32 Highly eccentric orbit[119]
TOI-4582 b 0.53±0.05 0.94+0.09
−0.12 		31.034±0.001 transit 1242 1.34±0.06 5190±100 Evolved star, eccentric planetary orbit[120]
TOI-4791 b 2.31+0.32
−0.33 		1.110±0.050 4.280880+0.000022
−0.000023 		0.0555+0.0011
−0.0012 		1472+26
−24 		transit 1051±6 1.242+0.072
−0.077 		6058+99
−94 		[105]
TOI-5153 b 3.26+0.18
−0.17 		1.06±0.04 20.33003±0.00007 0.158±0.006 906±13 transit 1272.336±11 1.24±0.07 6300±80 [63]
TOI-5174 b 0.07801 0.47667 12.214 transit 1.0±0.125 [121][122]
TOI-5205b 1.08±0.06 1.03±0.03 1.630757±0.000001 0.0199±0.0002 737±15 transit 283.35±0.16 0.392±0.015 3430±54 [123]
TOI-5542 b 1.32±0.10 1.009+0.036
−0.035 		75.12375+0.00019
−0.00018 		0.332±0.016 441+48
−74 		transit 1154±12 0.890+0.056
−0.031 		5700±80 [124]
TYC 2187-512-1 b 0.33±0.02 691.90+8.77
−8.61 		1.22±0.02 radial vel. 50.512±0.016 0.498±0.019 3734±54 [125]
WASP-132c 0.165±0.009 1.011534±0.000005 0.0182±0.0003 transit 390 0.782±0.034 4714+87
−88 		[126]

Specific exoplanet lists[edit]

Lists of exoplanets

Lists of exoplanets by year of discovery[edit]


References[edit]

  1. ^ a b Specht, D.; et al. (2023). "Kepler K2Campaign 9 – II. First space-based discovery of an exoplanet using microlensing". Monthly Notices of the Royal Astronomical Society. 520 (4): 6350–6366. arXiv:2203.16959. doi:10.1093/mnras/stad212.
  • ^ Starr, Michelle (4 April 2022). "The Most Distant Exoplanet Ever Found by Kepler Is... Surprisingly Familiar". ScienceAlert. Retrieved 4 April 2022.
  • ^ Currie, Thayne; et al. (2023), "Direct imaging and astrometric detection of a gas giant planet orbiting an accelerating star", Science, 380 (6641): 198–203, arXiv:2212.00034, Bibcode:2023Sci...380..198C, doi:10.1126/science.abo6192, PMID 37053312, S2CID 258108042
  • ^ a b Sebastian, D.; Guenther, E. W.; Deleuil, M.; Dorsch, M.; Heber, U.; Heuser, C.; Gandolfi, D.; Grziwa, S.; Deeg, H. J.; Alonso, R.; Bouchy, F.; Csizmadia, Sz; Cusano, F.; Fridlund, M.; Geier, S.; Irrgang, A.; Korth, J.; Nespral, D.; Rauer, H.; Tal-Or, L. (2022), "Sub-stellar companions of intermediate-mass stars with CoRoT: CoRoT–34b, CoRoT–35b, and CoRoT–36b", Monthly Notices of the Royal Astronomical Society, 516: 636–655, arXiv:2207.08742, doi:10.1093/mnras/stac2131
  • ^ 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 ae af ag ah ai aj ak al am an ao ap aq ar as at au av aw ax ay az ba bb bc bd be bf bg bh Christiansen, Jessie L.; et al. (2022), "Scaling K2. V. Statistical Validation of 60 New Exoplanets from K2 Campaigns 2–18", The Astronomical Journal, 163 (6): 244, arXiv:2203.02087, Bibcode:2022AJ....163..244C, doi:10.3847/1538-3881/ac5c4c, S2CID 247244871
  • ^ a b c d e f Del Ser, D.; Fors, O.; Del Alcázar, M.; Dyachenko, V.; Horch, E. P.; Tokovinin, A.; Ziegler, C.; Van Belle, G. T.; Clark, C. A.; Hartman, Z. D. (2023), "TFAW survey II: Six newly validated planets and 13 planet candidates from K2", Monthly Notices of the Royal Astronomical Society, 518: 669–690, arXiv:2210.10805, doi:10.1093/mnras/stac3087
  • ^ a b Panahi, Aviad; Zucker, Shay; Clementini, Gisella; Audard, Marc; Binnenfeld, Avraham; Cusano, Felice; Evans, Dafydd Wyn; Gomel, Roy; Holl, Berry; Ilyin, Ilya; De Fombelle, Grégory Jevardat; Mazeh, Tsevi; Mowlavi, Nami; Nienartowicz, Krzysztof; Rimoldini, Lorenzo; Shahaf, Sahar; Eyer, Laurent (2022). "The detection of transiting exoplanets by Gaia". Astronomy & Astrophysics. 663: A101. arXiv:2205.10197. Bibcode:2022A&A...663A.101P. doi:10.1051/0004-6361/202243497. S2CID 248965147.
  • ^ Damasso, M.; et al. (2022), "A quarter century of spectroscopic monitoring of the nearby M dwarf Gl 514", Astronomy & Astrophysics, 666: A187, arXiv:2204.06376, doi:10.1051/0004-6361/202243522, S2CID 248157318
  • ^ a b Suárez Mascareño, A.; et al. (2022), "Two temperate Earth-mass planets orbiting the nearby star GJ 1002", Astronomy & Astrophysics, 670: A5, arXiv:2212.07332, doi:10.1051/0004-6361/202244991, S2CID 254353639
  • ^ Kemmer, J.; et al. (2022), "Discovery and mass measurement of the hot, transiting, Earth-sized planet, GJ 3929 B", Astronomy & Astrophysics, 659: A17, arXiv:2202.00970, Bibcode:2022A&A...659A..17K, doi:10.1051/0004-6361/202142653, S2CID 246473345
  • ^ a b Beard, Corey; et al. (2022), "GJ 3929: High-precision Photometric and Doppler Characterization of an Exo-Venus and Its Hot, Mini-Neptune-mass Companion", The Astrophysical Journal, 936 (1): 55, arXiv:2207.10672, Bibcode:2022ApJ...936...55B, doi:10.3847/1538-4357/ac8480, S2CID 251018402
  • ^ A Jupiter Analog Orbiting The Nearby M Dwarf GJ 463
  • ^ Sozzetti, A. (2023), "A dynamical mass for GJ 463 b: A massive super-Jupiter companion beyond the snow line of a nearby M dwarf", Astronomy & Astrophysics, 670: L17, arXiv:2302.00413, Bibcode:2023A&A...670L..17S, doi:10.1051/0004-6361/202245454, S2CID 256253670
  • ^ a b 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
  • ^ Bourrier, V.; et al. (2022), "A CHEOPS-enhanced view of the HD 3167 system", Astronomy & Astrophysics, 668: A31, arXiv:2209.06937, doi:10.1051/0004-6361/202243778, S2CID 251861892
  • ^ Desidera, S.; et al. (2023), "TOI-179: A young system with a transiting compact Neptune-mass planet and a low-mass companion in outer orbit", Astronomy & Astrophysics, 675: A158, arXiv:2210.07933, doi:10.1051/0004-6361/202244611, S2CID 252907692
  • ^ de Leon, Jerome P.; et al. (2023), "A sub-Neptune transiting the young field star HD 18599 at 40 pc", Monthly Notices of the Royal Astronomical Society, 522: 750–766, arXiv:2210.08179, doi:10.1093/mnras/stad894
  • ^ Vines, Jose I.; Jenkins, James S.; Berdiñas, Zaira; Soto, Maritza G.; Díaz, Matías R.; Alves, Douglas R.; Tuomi, Mikko; Wittenmyer, Robert A.; De Leon, Jerome Pitogo; Peña, Pablo; Lissauer, Jack J.; Ballard, Sarah; Bedding, Timothy; Bowler, Brendan P.; Horner, Jonathan; Jones, Hugh R A.; Kane, Stephen R.; Kielkopf, John; Plavchan, Peter; Shporer, Avi; Tinney, C. G.; Wright, Hui Zhang Duncan J.; Addison, Brett; Mengel, Matthew W.; Okumura, Jack; Samadi-Ghadim, Anya (2022), "A dense mini-Neptune orbiting the bright young star HD 18599", Monthly Notices of the Royal Astronomical Society, 518 (2): 2627–2639, arXiv:2210.07945, doi:10.1093/mnras/stac2845
  • ^ Murgas, F.; et al. (2022), "HD 20329b: An ultra-short-period planet around a solar-type star found by TESS", Astronomy & Astrophysics, 668: A158, arXiv:2211.02547, Bibcode:2022A&A...668A.158M, doi:10.1051/0004-6361/202244459, S2CID 253370507
  • ^ a b c Ottoni, G.; Udry, S.; Ségransan, D.; et al. (2022). "CORALIE radial-velocity search for companions around evolved stars (CASCADES). I. Sample definition and first results: Three new planets orbiting giant stars". Astronomy & Astrophysics. 657: A87. arXiv:2201.01528. Bibcode:2022A&A...657A..87O. doi:10.1051/0004-6361/202040078. ISSN 0004-6361. S2CID 245440163.
  • ^ a b Cacciapuoti, Luca; et al. (2022), "TESS discovery of a super-Earth and two sub-Neptunes orbiting the bright, nearby, Sun-like star HD 22946", Astronomy & Astrophysics, 668: A85, arXiv:2209.09597, Bibcode:2022A&A...668A..85C, doi:10.1051/0004-6361/202243565, S2CID 252383725
  • ^ a b c Barros, S. C. C.; et al. (2022), "HD 23472: A multi-planetary system with three super-Earths and two potential super-Mercuries", Astronomy & Astrophysics, 665: A154, arXiv:2209.13345, Bibcode:2022A&A...665A.154B, doi:10.1051/0004-6361/202244293, S2CID 251463803
  • ^ a b c Dransfield, Georgina; et al. (2022), "HD 28109 hosts a trio of transiting Neptunian planets including a near-resonant pair, confirmed by ASTEP from Antarctica", Monthly Notices of the Royal Astronomical Society, 515: 1328–1345, arXiv:2205.09046, doi:10.1093/mnras/stac1383
  • ^ Pezzotti, C.; Ottoni, G.; Buldgen, G.; et al. (22 April 2021). "Coralie radial-velocity search for companions around evolved stars (CASCADES). III. A new Jupiter host-star: in-depth analysis of HD29399 using TESS data". Astronomy & Astrophysics. 657. EDP Sciences: A89. arXiv:2201.01553. doi:10.1051/0004-6361/202040080. ISSN 0004-6361. S2CID 242974999.
  • ^ Trifonov, Trifon; Wollbold, Anna; Kürster, Martin; Eberhardt, Jan; Stock, Stephan; Henning, Thomas; Reffert, Sabine; Butler, R. Paul; Vogt, Steven S.; Reiners, Ansgar; Lee, Man Hoi; Bitsch, Bertram; Zechmeister, Mathias; Rodler, Florian; Perdelwitz, Volker; Tal-Or, Lev; Rybizki, Jan; Heeren, Paul; Gandolfi, Davide; Barragán, Oscar; Zakhozhay, Olga; Sarkis, Paula; Pinto, Marcelo Tala; Kossakowski, Diana; Wolthoff, Vera; Brems, Stefan S.; Passegger, Vera Maria (2022), "A New Third Planet and the Dynamical Architecture of the HD 33142 Planetary System", The Astronomical Journal, 164 (4): 156, arXiv:2206.03899, Bibcode:2022AJ....164..156T, doi:10.3847/1538-3881/ac7ce0, S2CID 249461702
  • ^ Giacalone, Steven; Dressing, Courtney D.; Muñoz, A. García; Hooton, Matthew J.; Stassun, Keivan G.; Quinn, Samuel N.; Zhou, George; Ziegler, Carl; Vanderspek, Roland; Latham, David W.; Seager, S.; Winn, Joshua N.; Jenkins, Jon M.; Briceño, César; Huang, Chelsea X.; Rodriguez, David R.; Shporer, Avi; Mann, Andrew W.; Watanabe, David; Wohler, Bill (2022), "HD 56414 b: A Warm Neptune Transiting an A-type Star", The Astrophysical Journal Letters, 935 (1): L10, arXiv:2208.06396, Bibcode:2022ApJ...935L..10G, doi:10.3847/2041-8213/ac80f4, S2CID 251538927
  • ^ Errico, Adriana; Wittenmyer, Robert A.; Horner, Jonathan; Li, Zhexing; Brandt, G. Mirek; Kane, Stephen R.; Fetherolf, Tara; Holt, Timothy R.; Carter, Brad; Clark, Jake T.; Butler, R. P.; Tinney, C. G.; Ballard, Sarah; Bowler, Brendan P.; Kielkopf, John; Liu, Huigen; Plavchan, Peter P.; Shporer, Avi; Zhang, Hui; Wright, Duncan J.; Addison, Brett C.; Mengel, Matthew W.; Okumura, Jack (2022), "HD 83443c: A Highly Eccentric Giant Planet on a 22 yr Orbit", The Astronomical Journal, 163 (6): 273, arXiv:2204.05711, Bibcode:2022AJ....163..273E, doi:10.3847/1538-3881/ac6589, S2CID 248118529
  • ^ a b Serrano, L. M.; et al. (2022), "The HD 93963 a transiting system: A 1.04 d super-Earth and a 3.65 d sub-Neptune discovered by TESS and CHEOPS", Astronomy & Astrophysics, 667: A1, arXiv:2207.13920, Bibcode:2022A&A...667A...1S, doi:10.1051/0004-6361/202243093, S2CID 250709574
  • ^ a b Choi, Gong jun; Yanagida, Tsutomu T.; Yokozaki, Norimi (2022), "The upper bound of the second Higgs boson mass in minimal gauge mediation with the gravitino warm dark matter", Journal of High Energy Physics, 2021 (4), arXiv:2012.03266, doi:10.1007/JHEP04(2021)024, S2CID 227340010
  • ^ Zakhozhay, O.; Launhardt, R.; Trifonov, T.; Kürster, M.; Reffert, S.; Henning, Th.; Brahm, R.; Vinés, J.; Marleau, G. -D.; Patel, J. (2022), "Radial velocity survey for planets around young stars (RVSPY)", Astronomy & Astrophysics, 667: L14, arXiv:2211.08294, doi:10.1051/0004-6361/202244747, S2CID 235028524
  • ^ Engler, N.; et al. (2023), "The high-albedo, low polarization disk around HD 114082 that harbors a Jupiter-sized transiting planet", Astronomy & Astrophysics, 672: A1, arXiv:2211.11767, doi:10.1051/0004-6361/202244380, S2CID 256215468
  • ^ Teng, Huan-Yu; Sato, Bun'ei; Kunitomo, Masanobu; Takarada, Takuya; Omiya, Masashi; Harakawa, Hiroki; Xiao, Guang-Yao; Liu, Yu-Juan; Izumiura, Hideyuki; Kambe, Eiji; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro; Shigeru, Ida (2022), "A close-in planet orbiting giant star HD 167768", Publications of the Astronomical Society of Japan, 75: 169–176, arXiv:2211.06576, doi:10.1093/pasj/psac097
  • ^ a b Orell-Miquel, J.; Nowak, G.; Murgas, F.; Palle, E.; Morello, G.; Luque, R.; Badenas-Agusti, M.; Ribas, I.; Lafarga, M.; Espinoza, N.; Morales, J. C.; Zechmeister, M.; Alqasim, A.; Cochran, W. D.; Gandolfi, D.; Goffo, E.; Kabáth, P.; Korth, J.; Livingston, J.; Lam, K. W. F.; Muresan, A.; Persson, C. M.; Van Eylen, V. (2023). "HD 191939 revisited: New and refined planet mass determinations, and a new planet in the habitable zone". Astronomy & Astrophysics. 669: A40. arXiv:2211.00667. Bibcode:2023A&A...669A..40O. doi:10.1051/0004-6361/202244120. S2CID 253197272.
  • ^ a b c d e Feng, Fabo; Butler, R. Paul; Vogt, Steven S.; Clement, Matthew S.; Tinney, C. G.; Cui, Kaiming; Aizawa, Masataka; Jones, Hugh R. A.; Bailey, J.; Burt, Jennifer; Carter, B. D.; Crane, Jeffrey D.; Dotti, Francesco Flammini; Holden, Bradford; Ma, Bo; Ogihara, Masahiro; Oppenheimer, Rebecca; o'Toole, S. J.; Shectman, Stephen A.; Wittenmyer, Robert A.; Wang, Sharon X.; Wright, D. J.; Xuan, Yifan (2022), "3D Selection of 167 Substellar Companions to Nearby Stars", The Astrophysical Journal Supplement Series, 262 (1): 21, arXiv:2208.12720, Bibcode:2022ApJS..262...21F, doi:10.3847/1538-4365/ac7e57, S2CID 251864022
  • ^ Hinkley, S.; et al. (2023), "Direct discovery of the inner exoplanet in the HD 206893 system", Astronomy & Astrophysics, 671: L5, arXiv:2208.04867, doi:10.1051/0004-6361/202244727, S2CID 251442869
  • ^ a b Luque, R.; et al. (2022), "The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc", Astronomy & Astrophysics, 664: A199, arXiv:2204.10261, Bibcode:2022A&A...664A.199L, doi:10.1051/0004-6361/202243834, S2CID 248300168
  • ^ a b c d Serrano, Luisa Maria; et al. (2022), "A low-eccentricity migration pathway for a 13-h-period Earth analogue in a four-planet system", Nature Astronomy, 6 (6): 736–750, arXiv:2204.13573, Bibcode:2022NatAs...6..736S, doi:10.1038/s41550-022-01641-y, S2CID 248426734
  • ^ Zhou, George; et al. (2022), "A Mini-Neptune from TESS and CHEOPS Around the 120 Myr Old AB Dor Member HIP 94235", The Astronomical Journal, 163 (6): 289, arXiv:2204.11975, Bibcode:2022AJ....163..289Z, doi:10.3847/1538-3881/ac69e3, S2CID 248392044
  • ^ a b c Teng, Huan-Yu; Sato, Bun'ei; Takarada, Takuya; Omiya, Masashi; Harakawa, Hiroki; Nagasawa, Makiko; Hasegawa, Ryo; Izumiura, Hideyuki; Kambe, Eiji; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro; Ida, Shigeru (2022), "A trio of giant planets orbiting evolved star HD 184010", Publications of the Astronomical Society of Japan, 74 (6): 1309–1328, arXiv:2209.09426, doi:10.1093/pasj/psac070
  • ^ a b Ekrem Murat Esmer; Baştürk, Özgür; Selim Osman Selam; Aliş, Sinan (2022), "Detection of two additional circumbinary planets around Kepler-451", Monthly Notices of the Royal Astronomical Society, 511 (4): 5207–5216, arXiv:2202.02118, doi:10.1093/mnras/stac357
  • ^ Angelo, Isabel; Naoz, Smadar; Petigura, Erik; MacDougall, Mason; Stephan, Alexander P.; Isaacson, Howard; Howard, Andrew W. (2022), "Kepler-1656b's Extreme Eccentricity: Signature of a Gentle Giant", The Astronomical Journal, 163 (5): 227, arXiv:2204.00019, Bibcode:2022AJ....163..227A, doi:10.3847/1538-3881/ac6094, S2CID 247922620
  • ^ Kipping, David; Bryson, Steve; et al. (13 January 2022). "An exomoon survey of 70 cool giant exoplanets and the new candidate Kepler-1708 b-i". Nature. 6 (3): 367–380. arXiv:2201.04643. Bibcode:2022NatAs...6..367K. doi:10.1038/s41550-021-01539-1. PMC 8938273. PMID 35399159.
  • ^ "Kepler-1708". NASA Exoplanet Archive. Retrieved 13 January 2022.
  • ^ a b Leleu, A.; Delisle, J. -B.; Mardling, R.; Udry, S.; Chatel, G.; Alibert, Y.; Eggenberger, P. (2022), "Alleviating the transit timing variation bias in transit surveys", Astronomy & Astrophysics, 661: A141, arXiv:2201.11459, doi:10.1051/0004-6361/202142822, S2CID 246294682
  • ^ a b c d e f g Zang, Weicheng; et al. (2023), "Systematic KMTNet Planetary Anomaly Search. VII. Complete Sample of q < 10−4 Planets from the First 4 yr Survey", The Astronomical Journal, 165 (3): 103, arXiv:2210.12344, Bibcode:2023AJ....165..103Z, doi:10.3847/1538-3881/acb34b, S2CID 253098604
  • ^ a b Han, Cheongho; Lee, Chung-Uk; Gould, Andrew; Youn Kil Jung; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Kim, Doeon; Ryu, Yoon-Hyun; Shin, In-Gu; Shvartzvald, Yossi; Yang, Hongjing; 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. (2022), "KMT-2017-BLG-0673Lb and KMT-2019-BLG-0414Lb: Two microlensing planets detected in peripheral fields of KMTNet survey", Astronomy & Astrophysics, 666: A132, arXiv:2209.00112, Bibcode:2022A&A...666A.132H, doi:10.1051/0004-6361/202244438, S2CID 251979813
  • ^ a b c d e f Youn Kil Jung; et al. (2022), "Systematic KMTNet Planetary Anomaly Search. VI. Complete Sample of 2018 Sub-prime-field Planets", The Astronomical Journal, 164 (6): 262, arXiv:2206.11409, Bibcode:2022AJ....164..262J, doi:10.3847/1538-3881/ac9c5c, S2CID 249953591
  • ^ a b c d e f g h Gould, Andrew; et al. (2022), "Systematic KMTNet planetary anomaly search", Astronomy & Astrophysics, 664: A13, arXiv:2204.04354, doi:10.1051/0004-6361/202243744, S2CID 248085003
  • ^ a b c Zang, Weicheng; et al. (2022), "Systematic KMTNet planetary anomaly search. IV. Complete sample of 2019 prime-field", Monthly Notices of the Royal Astronomical Society, 515: 928–939, arXiv:2204.02017, doi:10.1093/mnras/stac1883
  • ^ a b Yang, Hongjing; et al. (2022), "KMT-2021-BLG-0171Lb and KMT-2021-BLG-1689Lb: Two microlensing planets in the KMTNet high-cadence fields with followup observations", Monthly Notices of the Royal Astronomical Society, 516 (2): 1894–1909, arXiv:2205.12584, doi:10.1093/mnras/stac2023
  • ^ a b Han, Cheongho; Kim, Doeon; Yang, Hongjing; Gould, Andrew; Youn Kil Jung; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Lee, Chung-Uk; 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. (2022), "KMT-2021-BLG-0240: Microlensing event with a deformed planetary signal", Astronomy & Astrophysics, 664: A114, arXiv:2204.11383, Bibcode:2022A&A...664A.114H, doi:10.1051/0004-6361/202243161, S2CID 248377479
  • ^ a b c d Han, Cheongho; et al. (2022), "Four sub-Jovian-mass planets detected by high-cadence microlensing surveys", Astronomy & Astrophysics, 664: A33, arXiv:2205.10510, Bibcode:2022A&A...664A..33H, doi:10.1051/0004-6361/202243484, S2CID 248986310
  • ^ a b c d Ryu, Yoon-Hyun; Youn Kil Jung; Yang, Hongjing; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Han, Cheongho; Hwang, Kyu-Ha; Shin, In-Gu; Shvartzvald, Yossi; Yee, Jennifer C.; 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 (2022), "Mass Production of 2021 KMTNet Microlensing Planets I", The Astronomical Journal, 164 (5): 180, arXiv:2202.03022, Bibcode:2022AJ....164..180R, doi:10.3847/1538-3881/ac8d6c, S2CID 246634000
  • ^ a b c Shin, In-Gu; et al. (2023), "Mass Production of 2021 KMTNet Microlensing Planets. III. Analysis of Three Giant Planets", The Astronomical Journal, 165 (1): 8, arXiv:2209.03886, Bibcode:2023AJ....165....8S, doi:10.3847/1538-3881/ac9d93, S2CID 254407196
  • ^ a b c d Ryu, Yoon-Hyun; Shin, In-Gu; Yang, Hongjing; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Han, Cheongho; Hwang, Kyu-Ha; Youn Kil Jung; Shvartzvald, Yossi; Yee, Jennifer C.; 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. (2023), "Mass Production of 2021 KMTNet Microlensing Planets II", The Astronomical Journal, 165 (3): 83, arXiv:2207.07295, Bibcode:2023AJ....165...83R, doi:10.3847/1538-3881/acab6b, S2CID 256544515
  • ^ a b Han, Cheongho; et al. (2022), "KMT-2021-BLG-1077L: The fifth confirmed multiplanetary system detected by microlensing", Astronomy & Astrophysics, 662: A70, arXiv:2203.16734, Bibcode:2022A&A...662A..70H, doi:10.1051/0004-6361/202243550, S2CID 247839227
  • ^ Han, Cheongho; Gould, Andrew; Kim, Doeon; Youn Kil Jung; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Lee, Chung-Uk; 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. (2022), "KMT-2021-BLG-1898: Planetary microlensing event involved with binary source stars", Astronomy & Astrophysics, 663: A145, arXiv:2204.11378, Bibcode:2022A&A...663A.145H, doi:10.1051/0004-6361/202243102, S2CID 248377122
  • ^ Sartori, Lia F.; Lovis, Christophe; Delisle, Jean-Baptiste; Lendl, Monika; Cugno, Gabriele; Boehle, Anna; Dannert, Felix; Krenn, Andrea; Gubler, Jonas L.; Quanz, Sascha P. (2023), "L 363-38 b: A planet newly discovered with ESPRESSO orbiting a nearby M dwarf star", Astronomy & Astrophysics, 670: A42, arXiv:2210.12710, Bibcode:2023A&A...670A..42S, doi:10.1051/0004-6361/202244347, S2CID 253098575
  • ^ Bachelet, E.; et al. (2022), "MOA-2019-BLG-008Lb: A New Microlensing Detection of an Object at the Planet/Brown Dwarf Boundary", The Astronomical Journal, 164 (3): 75, arXiv:2205.07522, Bibcode:2022AJ....164...75B, doi:10.3847/1538-3881/ac78ed, S2CID 248810881
  • ^ Stela Ishitani Silva; et al. (2022), "MOA-2020-BLG-135Lb: A New Neptune-class Planet for the Extended MOA-II Exoplanet Microlens Statistical Analysis", The Astronomical Journal, 164 (3): 118, arXiv:2204.03672, Bibcode:2022AJ....164..118I, doi:10.3847/1538-3881/ac82b8, S2CID 248069150
  • ^ Olmschenk, Greg; et al. (2023), "MOA-2020-BLG-208Lb: Cool Sub-Saturn-mass Planet within Predicted Desert", The Astronomical Journal, 165 (4): 175, arXiv:2210.02436, Bibcode:2023AJ....165..175O, doi:10.3847/1538-3881/acbcc8, S2CID 252715812
  • ^ a b Squicciarini, V.; Gratton, R.; Janson, M.; Mamajek, E. E.; Chauvin, G.; Delorme, P.; Langlois, M.; Vigan, A.; Ringqvist, S. C.; Meeus, G.; Reffert, S.; Kenworthy, M.; Meyer, M. R.; Bonnefoy, M.; Bonavita, M.; Mesa, D.; Samland, M.; Desidera, S.; D'Orazi, V.; Engler, N.; Alecian, E.; Miglio, A.; Henning, T.; Quanz, S. P.; Mayer, L.; Flasseur, O.; Marleau, G. D. (2022), "A scaled-up planetary system around a supernova progenitor", Astronomy & Astrophysics, 664: A9, arXiv:2205.02279, Bibcode:2022A&A...664A...9S, doi:10.1051/0004-6361/202243675, S2CID 248524983
  • ^ a b Ulmer-Moll, S.; et al. (2022), "Two long-period transiting exoplanets on eccentric orbits: NGTS-20 b (TOI-5152 b) and TOI-5153 B", Astronomy & Astrophysics, 666: A46, arXiv:2207.03911, Bibcode:2022A&A...666A..46U, doi:10.1051/0004-6361/202243583, S2CID 250408027
  • ^ Alves, Douglas R.; et al. (2022), "NGTS-21b: An Inflated Super-Jupiter Orbiting a Metal-poor K dwarf", Monthly Notices of the Royal Astronomical Society, 517 (3): 4447–4457, arXiv:2210.01027, doi:10.1093/mnras/stac2884
  • ^ a b c Jackson, David G.; et al. (2022), "The discovery of three hot Jupiters, NGTS-23b, 24b and 25b, and updated parameters for HATS-54b from the Next Generation Transit Survey", Monthly Notices of the Royal Astronomical Society, 518 (4): 4845–4860, arXiv:2211.01044, doi:10.1093/mnras/stac3192
  • ^ Shin, In-Gu; et al. (2022), "OGLE-2016-BLG-1093Lb: A Sub-Jupiter-mass Spitzer Planet Located in the Galactic Bulge", The Astronomical Journal, 163 (6): 254, arXiv:2201.04312, Bibcode:2022AJ....163..254S, doi:10.3847/1538-3881/ac6513, S2CID 245877628
  • ^ Chung, Sun-Ju; et al. (2022), "OGLE-2019-BLG-0362Lb: A SUPER-JOVIAN-MASS PLANET AROUND a LOW-MASS STAR", Journal of the Korean Astronomical Society, 55 (4): 123, arXiv:2208.04230, Bibcode:2022JKAS...55..123C, doi:10.5303/JKAS.2022.55.4.123, S2CID 251402706
  • ^ Kuang, Renkun; et al. (2022), "OGLE-2019-BLG-1470LABc: Another microlensing giant planet in a binary system?", Monthly Notices of the Royal Astronomical Society, 516 (2): 1704–1720, arXiv:2204.05606, doi:10.1093/mnras/stac2315
  • ^ Hatzes, Artie P.; et al. (2022), "A Radial Velocity Study of the Planetary System of π Mensae: Improved Planet Parameters for π Mensae c and a Third Planet on a 125 Day Orbit", The Astronomical Journal, 163 (5): 223, arXiv:2203.01018, Bibcode:2022AJ....163..223H, doi:10.3847/1538-3881/ac5dcb, S2CID 247218413
  • ^ Faria, J. P.; et al. (2022), "A candidate short-period sub-Earth orbiting Proxima Centauri", Astronomy & Astrophysics, 658: A115, arXiv:2202.05188, Bibcode:2022A&A...658A.115F, doi:10.1051/0004-6361/202142337, S2CID 246706321
  • ^ Niţu, Iuliana C.; Keith, Michael J.; Stappers, Ben W.; Lyne, Andrew G.; Mickaliger, Mitchell B. (2022), "A search for planetary companions around 800 pulsars from the Jodrell Bank pulsar timing programme", Monthly Notices of the Royal Astronomical Society, 512 (2): 2446–2459, arXiv:2203.01136, doi:10.1093/mnras/stac593
  • ^ Harakawa, Hiroki; et al. (2022), "A super-Earth orbiting near the inner edge of the habitable zone around the M4.5 dwarf Ross 508", Publications of the Astronomical Society of Japan, 74 (4): 904–922, arXiv:2205.11986, doi:10.1093/pasj/psac044
  • ^ Mistry, Priyashkumar; Pathak, Kamlesh; Lekkas, Georgios; Prasad, Aniket; Bhattarai, Surendra; Maity, Mousam; Beichman, Charles A.; Ciardi, David R.; Evans, Phil; Lucero, Jennifer P. (2023), "VaTEST I: Validation of sub-Saturn exoplanet TOI-181b in narrow orbit from its host star", Monthly Notices of the Royal Astronomical Society, 521: 1066–1078, arXiv:2211.07957, doi:10.1093/mnras/stad543
  • ^ a b c d e f g h i j k l m Giacalone, Steven; et al. (2022), "Validation of 13 Hot and Potentially Terrestrial TESS Planets", The Astronomical Journal, 163 (2): 99, arXiv:2201.12661, Bibcode:2022AJ....163...99G, doi:10.3847/1538-3881/ac4334, S2CID 246386453
  • ^ a b Magliano, Christian; Covone, Giovanni; Dobal, Richa; Cacciapuoti, Luca; Tonietti, Luca; Giacalone, Steven; Vines, Jose I.; Inno, Laura; Jenkins, James S.; Lissauer, Jack J.; Bieryla, Allyson; Oliva, Fabrizio; Pagano, Isabella; Kostov, Veselin; Ziegler, Carl; Ciardi, David R.; Gonzales, Erica J.; Dressing, Courtney D.; Buchhave, Lars A.; Howell, Steve B.; Matson, Rachel A.; Matthews, Elisabeth; Rotundi, Alessandra; Alves, Douglas; Fiscale, Stefano; Ienco, Riccardo M.; Pena, Pablo; Gallo, Francesco; Muscari Tomajoli, Maria T. (2022), "A systematic validation of hot Neptunes in TESS data", Monthly Notices of the Royal Astronomical Society, 519: 1562–1577, arXiv:2211.08490, doi:10.1093/mnras/stac3404
  • ^ Reefe, Michael A.; et al. (2022), "A Close-in Puffy Neptune with Hidden Friends: The Enigma of TOI 620", The Astronomical Journal, 163 (6): 269, arXiv:2204.03108, Bibcode:2022AJ....163..269R, doi:10.3847/1538-3881/ac658b, S2CID 248006000
  • ^ Clark, Jake; et al. (2023), "Spinning up a Daze: TESS Uncovers a Hot Jupiter Orbiting the Rapid Rotator TOI-778", The Astronomical Journal, 165 (5): 207, arXiv:2212.08242, Bibcode:2023AJ....165..207C, doi:10.3847/1538-3881/acc3a0, S2CID 254823145
  • ^ a b Lillo-Box, J.; et al. (2023), "TOI-969: A late-K dwarf with a hot mini-Neptune in the desert and an eccentric cold Jupiter", Astronomy & Astrophysics, 669: A109, arXiv:2210.08996, Bibcode:2023A&A...669A.109L, doi:10.1051/0004-6361/202243879, S2CID 252917906
  • ^ a b Wilson, Thomas G.; et al. (2022), "A pair of sub-Neptunes transiting the bright K-dwarf TOI-1064 characterized with CHEOPS", Monthly Notices of the Royal Astronomical Society, 511: 1043–1071, arXiv:2201.03570, doi:10.1093/mnras/stab3799
  • ^ Essack, Zahra; et al. (2023), "TOI-1075 b: A Dense, Massive, Ultra-short-period Hot Super-Earth Straddling the Radius Gap", The Astronomical Journal, 165 (2): 47, arXiv:2210.14901, Bibcode:2023AJ....165...47E, doi:10.3847/1538-3881/ac9c5b, S2CID 253117166
  • ^ Psaridi, A.; et al. (2022), "Three new brown dwarfs and a massive hot Jupiter revealed by TESS around early-type stars", Astronomy & Astrophysics, 664: A94, arXiv:2205.10854, Bibcode:2022A&A...664A..94P, doi:10.1051/0004-6361/202243454, S2CID 248872705
  • ^ a b c d e f Dai, Fei; et al. (2023), "TOI-1136 is a Young, Coplanar, Aligned Planetary System in a Pristine Resonant Chain", The Astronomical Journal, 165 (2): 33, arXiv:2210.09283, Bibcode:2023AJ....165...33D, doi:10.3847/1538-3881/aca327, S2CID 252918416
  • ^ a b c Kabáth, Petr; et al. (2022), "TOI-2046b, TOI-1181b and TOI-1516b, three new hot Jupiters from TESS: Planets orbiting a young star, a subgiant and a normal star", Monthly Notices of the Royal Astronomical Society, 513 (4): 5955–5972, arXiv:2205.01860, doi:10.1093/mnras/stac1254
  • ^ Mann, Christopher R.; Lafrenière, David; Dragomir, Diana; Quinn, Samuel N.; Tan, Thiam-Guan; Collins, Karen A.; Howell, Steve B.; Ziegler, Carl; Mann, Andrew W.; Stassun, Keivan G.; Kristiansen, Martti H.; Osborn, Hugh; Boyajian, Tabetha; Eisner, Nora; Hellier, Coel; Ricker, George R.; Vanderspek, Roland; Latham, David W.; Seager, S.; Winn, Joshua N.; Jenkins, Jon M.; McLean, Brian; Rowden, Pamela; Torres, Guillermo; Caldwell, Douglas A.; Collins, Kevin I.; Schwarz, Richard P. (2023), "Validation of TOI-1221 b: A Warm Sub-Neptune Exhibiting Transit Timing Variations around a Sun-like Star", The Astronomical Journal, 165 (5): 217, arXiv:2209.13651, Bibcode:2023AJ....165..217M, doi:10.3847/1538-3881/acc8d4, S2CID 252568279
  • ^ a b c d Turtelboom, Emma V.; et al. (2022), "The TESS-Keck Survey. XI. Mass Measurements for Four Transiting Sub-Neptunes Orbiting K Dwarf TOI–1246", The Astronomical Journal, 163 (6): 293, arXiv:2204.11895, Bibcode:2022AJ....163..293T, doi:10.3847/1538-3881/ac69e5, S2CID 248392257
  • ^ Lam, Kristine W F.; et al. (2022), "Discovery of TOI-1260d and the characterisation of the multi-planet system", Monthly Notices of the Royal Astronomical Society, 519: 1437–1451, arXiv:2212.04307, doi:10.1093/mnras/stac3639
  • ^ Šubjak, J.; et al. (2022), "TOI-1268b: The youngest hot Saturn-mass transiting exoplanet", Astronomy & Astrophysics, 662: A107, arXiv:2201.13341, Bibcode:2022A&A...662A.107S, doi:10.1051/0004-6361/202142883, S2CID 246430777
  • ^ a b MacDougall, Mason G.; et al. (2022), "The TESS–Keck Survey. XIII. An Eccentric Hot Neptune with a Similar-mass Outer Companion around TOI-1272", The Astronomical Journal, 164 (3): 97, arXiv:2206.14327, Bibcode:2022AJ....164...97M, doi:10.3847/1538-3881/ac7ce1, S2CID 250113765
  • ^ Knudstrup, E.; et al. (2022), "Radial velocity confirmation of a hot super-Neptune discovered by TESS with a warm Saturn-mass companion", Monthly Notices of the Royal Astronomical Society, 519 (4): 5637–5655, arXiv:2211.17035, doi:10.1093/mnras/stac3684
  • ^ Naponiello, L.; et al. (2022), "The GAPS programme at TNG. XL. A puffy and warm Neptune-sized planet and an outer Neptune-mass candidate orbiting the solar-type star TOI-1422", Astronomy & Astrophysics, A8: 667, arXiv:2207.03293, Bibcode:2022A&A...667A...8N, doi:10.1051/0004-6361/202244079, S2CID 250334523
  • ^ Cadieux, Charles; Doyon, René; et al. (27 June 2022). "TOI-1452 b: SPIRou and TESS Reveal a Super-Earth in a Temperate Orbit Transiting an M4 Dwarf". The Astronomical Journal. 164:96 (3) (published 12 August 2022): 28pp. arXiv:2208.06333. Bibcode:2022AJ....164...96C. doi:10.3847/1538-3881/ac7cea.
  • ^ a b Chaturvedi, P.; et al. (2022), "TOI-1468: A system of two transiting planets, a super-Earth and a mini-Neptune, on opposite sides of the radius valley", Astronomy & Astrophysics, 666: A155, arXiv:2208.10351, Bibcode:2022A&A...666A.155C, doi:10.1051/0004-6361/202244056, S2CID 251718760
  • ^ a b c d Van Zandt, Judah E.; et al. (2023), "TESS-Keck Survey. XIV. Two Giant Exoplanets from the Distant Giants Survey", The Astronomical Journal, 165 (2): 60, arXiv:2209.06958, Bibcode:2023AJ....165...60V, doi:10.3847/1538-3881/aca6ef, S2CID 252280288
  • ^ a b Giacalone, Steven; et al. (2020), "Vetting of 384 TESS Objects of Interest with TRICERATOPS and Statistical Validation of 12 Planet Candidates", The Astronomical Journal, 161: 24, arXiv:2002.00691, doi:10.3847/1538-3881/abc6af, S2CID 227141512
  • ^ a b Tran, Quang H.; et al. (2022), "TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to Have Originated from High-eccentricity Migration", The Astronomical Journal, 163 (5): 225, arXiv:2203.04334, Bibcode:2022AJ....163..225T, doi:10.3847/1538-3881/ac5c4f, S2CID 247318919
  • ^ Kiefer, F.; et al. (2023), "A sub-Neptune planet around TOI-1695 discovered and characterized with SPIRou and TESS", Astronomy & Astrophysics, 670: A136, arXiv:2211.06205, Bibcode:2023A&A...670A.136K, doi:10.1051/0004-6361/202245129, S2CID 253498974
  • ^ Cherubim, Collin; et al. (2023), "TOI-1695 b: A Water World Orbiting an Early-M Dwarf in the Planet Radius Valley", The Astronomical Journal, 165 (4): 167, arXiv:2211.06445, Bibcode:2023AJ....165..167C, doi:10.3847/1538-3881/acbdfd, S2CID 256627151
  • ^ Mori, Mayuko; et al. (2022), "TOI-1696: A Nearby M4 Dwarf with a 3 R ⊕ Planet in the Neptunian Desert", The Astronomical Journal, 163 (6): 298, arXiv:2203.02694, Bibcode:2022AJ....163..298M, doi:10.3847/1538-3881/ac6bf8, S2CID 247291913
  • ^ Beard, Corey; et al. (2022), "TOI-1696 and TOI-2136: Constraining the Masses of Two Mini-Neptunes with the Habitable-Zone Planet Finder", The Astronomical Journal, 163 (6): 286, arXiv:2204.09063, Bibcode:2022AJ....163..286B, doi:10.3847/1538-3881/ac69ec, S2CID 248266475
  • ^ König, P. -C.; et al. (2022), "A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE, and HARPS-N", Astronomy & Astrophysics, 666: A183, arXiv:2204.08984, Bibcode:2022A&A...666A.183K, doi:10.1051/0004-6361/202143002, S2CID 248239823
  • ^ Espinoza, Néstor; et al. (2022), "A Transiting, Temperate Mini-Neptune Orbiting the M Dwarf TOI-1759 Unveiled by TESS", The Astronomical Journal, 163 (3): 133, arXiv:2202.01240, Bibcode:2022AJ....163..133E, doi:10.3847/1538-3881/ac4af0, S2CID 246485680
  • ^ Martioli, E.; et al. (2022), "TOI-1759 b: A transiting sub-Neptune around a low mass star characterized with SPIRou and TESS", Astronomy & Astrophysics, 660: A86, arXiv:2202.01259, Bibcode:2022A&A...660A..86M, doi:10.1051/0004-6361/202142540, S2CID 246485686
  • ^ a b c d e f Rodriguez, Joseph E.; et al. (2023), "Another shipment of six short-period giant planets from TESS", Monthly Notices of the Royal Astronomical Society, 521 (2): 2765–2785, arXiv:2205.05709, doi:10.1093/mnras/stad595
  • ^ a b c Knudstrup, E.; et al. (2022), "Confirmation and characterisation of three giant planets detected by TESS from the FIES/NOT and Tull/Mc Donald spectrographs", Astronomy & Astrophysics, 667: A22, arXiv:2204.13956, Bibcode:2022A&A...667A..22K, doi:10.1051/0004-6361/202243656, S2CID 251083570
  • ^ a b c d e f g h i j k l m n o p q r s t Yee, Samuel W.; et al. (2023), "The TESS Grand Unified Hot Jupiter Survey. II. Twenty New Giant Planets", The Astrophysical Journal Supplement Series, 265 (1): 1, arXiv:2210.15473, Bibcode:2023ApJS..265....1Y, doi:10.3847/1538-4365/aca286, S2CID 253157404
  • ^ a b Sha, Lizhou; et al. (2023), "TESS spots a mini-neptune interior to a hot saturn in the TOI-2000 system", Monthly Notices of the Royal Astronomical Society, 524: 1113–1138, arXiv:2209.14396, doi:10.1093/mnras/stad1666
  • ^ Newton, Elisabeth R.; et al. (2022), "TESS Hunt for Young and Maturing Exoplanets (THYME). VII. Membership, Rotation, and Lithium in the Young Cluster Group-X and a New Young Exoplanet", The Astronomical Journal, 164 (3): 115, arXiv:2206.06254, Bibcode:2022AJ....164..115N, doi:10.3847/1538-3881/ac8154, S2CID 249626353
  • ^ a b Esparza-Borges, E.; et al. (2022), "A hot sub-Neptune in the desert and a temperate super-Earth around faint M dwarfs", Astronomy & Astrophysics, 666: A10, arXiv:2206.10643, doi:10.1051/0004-6361/202243731, S2CID 249926978
  • ^ Gan, Tianjun; et al. (2022), "TESS discovery of a sub-Neptune orbiting a mid-M dwarf TOI-2136", Monthly Notices of the Royal Astronomical Society, 514 (3): 4120–4139, arXiv:2202.10024, doi:10.1093/mnras/stac1448
  • ^ Kawauchi, K.; et al. (2022), "Validation and atmospheric exploration of the sub-Neptune TOI-2136b around a nearby M3 dwarf", Astronomy & Astrophysics, 666: A4, arXiv:2202.10182, Bibcode:2022A&A...666A...4K, doi:10.1051/0004-6361/202243381, S2CID 247011479
  • ^ Dalba, Paul A.; et al. (2022), "The TESS-Keck Survey. VIII. Confirmation of a Transiting Giant Planet on an Eccentric 261 Day Orbit with the Automated Planet Finder Telescope", The Astronomical Journal, 163 (2): 61, arXiv:2201.04146, Bibcode:2022AJ....163...61D, doi:10.3847/1538-3881/ac415b, S2CID 245877799
  • ^ a b c d e f g h i j Yee, Samuel W.; et al. (2022), "The TESS Grand Unified Hot Jupiter Survey. I. Ten TESS Planets", The Astronomical Journal, 164 (2): 70, arXiv:2205.09728, Bibcode:2022AJ....164...70Y, doi:10.3847/1538-3881/ac73ff, S2CID 248887656
  • ^ Persson, Carina M.; et al. (2022), "TOI-2196 b: Rare planet in the hot Neptune desert transiting a G-type star", Astronomy & Astrophysics, 666: A184, arXiv:2208.05797, Bibcode:2022A&A...666A.184P, doi:10.1051/0004-6361/202244118, S2CID 251478602
  • ^ a b c Grunblatt, Samuel K.; et al. (2022), "TESS Giants Transiting Giants. II. The Hottest Jupiters Orbiting Evolved Stars", The Astronomical Journal, 163 (3): 120, arXiv:2201.04140, Bibcode:2022AJ....163..120G, doi:10.3847/1538-3881/ac4972, S2CID 245877793
  • ^ a b Cañas, Caleb I.; et al. (2022), "TOI-3714 b and TOI-3629 b: Two Gas Giants Transiting M Dwarfs Confirmed with the Habitable-zone Planet Finder and NEID", The Astronomical Journal, 164 (2): 50, arXiv:2201.09963, Bibcode:2022AJ....164...50C, doi:10.3847/1538-3881/ac7804, S2CID 246275821
  • ^ Kanodia, Shubham; et al. (2022), "TOI-3757 b: A Low-density Gas Giant Orbiting a Solar-metallicity M Dwarf", The Astronomical Journal, 164 (3): 81, arXiv:2203.07178, Bibcode:2022AJ....164...81K, doi:10.3847/1538-3881/ac7c20, S2CID 247446993
  • ^ Almenara, J. M.; Bonfils, X.; Forveille, T.; Astudillo-Defru, N.; Ciardi, D. R.; Schwarz, R. P.; Collins, K. A.; Cointepas, M.; Lund, M. B.; Bouchy, F.; Charbonneau, D.; Díaz, R. F.; Delfosse, X.; Kidwell, R. C.; Kunimoto, M.; Latham, D. W.; Lissauer, J. J.; Murgas, F.; Ricker, G.; Seager, S.; Vezie, M.; Watanabe, D. (2022), "TOI-3884 b: A rare 6-RE planet that transits a low-mass star with a giant and likely polar spot", Astronomy & Astrophysics, 667: L11, arXiv:2210.10909, Bibcode:2022A&A...667L..11A, doi:10.1051/0004-6361/202244791, S2CID 253018639
  • ^ Libby-Roberts, Jessica E.; Schutte, Maria; Hebb, Leslie; Kanodia, Shubham; Canas, Caleb; Stefansson, Gudmundur; Lin, Andrea S. J.; Mahadevan, Suvrath; Parts, Winter; Powers, Luke; Wisniewski, John; Bender, Chad F.; Cochran, William D.; Diddams, Scott A.; Everett, Mark E.; Gupta, Arvind F.; Halverson, Samuel; Kobulnicky, Henry A.; Kowalski, Adam F.; Larsen, Alexander; Monson, Andrew; Ninan, Joe P.; Parker, Brock A.; Ramsey, Lawrence W.; Robertson, Paul; Schwab, Christian; Swaby, Tera N.; Terrien, Ryan C. (2023), An In-Depth Look at TOI-3884b: a Super-Neptune Transiting a M4 Dwarf with Persistent Star Spot Crossings, arXiv:2302.04757
  • ^ Heitzmann, Alexis; et al. (2023), "TOI-4562b: A Highly Eccentric Temperate Jupiter Analog Orbiting a Young Field Star", The Astronomical Journal, 165 (3): 121, arXiv:2208.10854, Bibcode:2023AJ....165..121H, doi:10.3847/1538-3881/acb5a2, S2CID 251741424
  • ^ Grunblatt, Samuel K.; Saunders, Nicholas; Chontos, Ashley; Hattori, Soichiro; Veras, Dimitri; Huber, Daniel; Angus, Ruth; Rice, Malena; Breivik, Katelyn; Blunt, Sarah; Giacalone, Steven; Lubin, Jack; Isaacson, Howard; Howard, Andrew W.; Ciardi, David R.; Safonov, Boris S.; Strakhov, Ivan A.; Latham, David W.; Bieryla, Allyson; Ricker, George R.; Jenkins, Jon M.; Tenenbaum, Peter; Shporer, Avi; Morgan, Edward H.; Kostov, Veselin; Osborn, Hugh P.; Dragomir, Diana; Seager, Sara; Vanderspek, Roland K.; Winn, Joshua N. (2023), "TESS Giants Transiting Giants. III. An Eccentric Warm Jupiter Supports a Period−Eccentricity Relation for Giant Planets Transiting Evolved Stars", The Astronomical Journal, 165 (2): 44, arXiv:2210.17062, Bibcode:2023AJ....165...44G, doi:10.3847/1538-3881/aca670, S2CID 253237700
  • ^ "The Extrasolar Planet Encyclopaedia — TOI-5174 b". Extrasolar Planets Encyclopaedia. 3 December 1995. Retrieved 16 January 2023.
  • ^ "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 16 January 2023.
  • ^ Kanodia, Shubham; Mahadevan, Suvrath; Libby-Roberts, Jessica; Stefansson, Gudmundur; Canas, Caleb I.; Piette, Anjali A. A.; Boss, Alan; Teske, Johanna; Chambers, John; Zeimann, Greg; Monson, Andrew; Robertson, Paul; Ninan, Joe P.; Lin, Andrea S. J.; Bender, Chad F.; Cochran, William D.; Diddams, Scott A.; Gupta, Arvind F.; Halverson, Samuel; Hawley, Suzanne; Kobulnicky, Henry A.; Metcalf, Andrew J.; Parker, Brock A.; Powers, Luke; Ramsey, Lawrence W.; Roy, Arpita; Schwab, Christian; Swaby, Tera N.; Terrien, Ryan C.; Wisniewski, John (2023), "TOI-5205b: A Short-period Jovian Planet Transiting a Mid-M Dwarf", The Astronomical Journal, 165 (3): 120, arXiv:2209.11160, Bibcode:2023AJ....165..120K, doi:10.3847/1538-3881/acabce, S2CID 257050897
  • ^ Grieves, Nolan; et al. (2022), "An old warm Jupiter orbiting the metal-poor G-dwarf TOI-5542", Astronomy & Astrophysics, 668: A29, arXiv:2209.14830, Bibcode:2022A&A...668A..29G, doi:10.1051/0004-6361/202244077, S2CID 252595745
  • ^ Quirrenbach, A.; Passegger, V. M.; Trifonov, T.; Amado, P. J.; Caballero, J. A.; Reiners, A.; Ribas, I.; Aceituno, J.; Bejar, V. J. S.; Chaturvedi, P.; Gonzalez-Cuesta, L.; Henning, T.; Herrero, E.; Kaminski, A.; Kuerster, M.; Lalitha, S.; Lodieu, N.; Lopez-Gonzalez, M. J.; Montes, D.; Palle, E.; Perger, M.; Pollacco, D.; Reffert, S.; Rodriguez, E.; Rodriguez Lopez, C.; Shan, Y.; Tal-Or, L.; Zapatero Osorio, M. R.; Zechmeister, M. (2022), "The CARMENES search for exoplanets around M dwarfs", Astronomy & Astrophysics, 663: A48, arXiv:2203.16504, doi:10.1051/0004-6361/202142915, S2CID 247835988
  • ^ Hord, Benjamin J.; Colón, Knicole D.; Berger, Travis A.; Kostov, Veselin; Silverstein, Michele L.; Stassun, Keivan G.; Lissauer, Jack J.; Collins, Karen A.; Schwarz, Richard P.; Sefako, Ramotholo; Ziegler, Carl; Briceño, César; Law, Nicholas; Mann, Andrew W.; Ricker, George R.; Latham, David W.; Seager, Sara; Winn, Joshua N.; Jenkins, Jon M.; Bouma, Luke G.; Falk, Ben; Torres, Guillermo; Twicken, Joseph D.; Vanderburg, Andrew (2022), "The Discovery of a Planetary Companion Interior to Hot Jupiter WASP-132 B", The Astronomical Journal, 164 (1): 13, arXiv:2205.02501, Bibcode:2022AJ....164...13H, doi:10.3847/1538-3881/ac6f57, S2CID 248524687
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