List of exoplanets discovered in 2022

Last updated

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.

Contents


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
astrometry + imaging130.9±0.92.14±0.158790+1513
1292
Host star also known as HIP 99770 [3]
CoRoT-35b 1.10±0.371.68±0.113.22748±0.000080.04290±0.000921747±62transit3700±2001.01+0.07
0.06
6390±130 [4]
CoRoT-36b 0.68+0.47
0.43
1.41±0.145.616531±0.0000230.066±0.0071567±35transit3110±601.32±0.096730±140 [4]
EPIC 206317286 c 0.0168±0.0980.186+0.015
0.014
17.51547+0.00228
0.00296
570transit0.832+0.253
0.367
4752±138 [5]
EPIC 210768568 b 0.088±0.0043.2141±0.00020.0511+0.0021
0.0028
transit9651.018±0.1315711±105 [6]
EPIC 246078343 b 0.068±0.0070.8094±0.000030.0117+0.0009
0.0012
transit9540.808+0.364
0.256
4116±138 [6]
EPIC 246078343 c 0.110±0.0065.3301±0.00030.0426+0.0016
0.0019
transit9540.808+0.364
0.256
4116±138 [6]
EPIC 246220667 b 0.172±0.0066.6690±0.00020.0552+0.0017
0.0023
transit8350.814+0.363
0.251
4343±138 [6]
EPIC 246220667 c 0.109±0.0064.3696±0.00010.0487+0.0027
0.0031
transit8350.814+0.363
0.251
4343±138 [6]
EPIC 247422570 b 0.189±0.0095.9382+0.0006
0.0004
0.0586+0.0032
0.0033
transit21810.893+0.406
0.275
5590±138 [6]
Gaia-1b1.68±0.111.229±0.0213.052524±0.0000170.04047±0.00094transit1201±70.949±0.0665470±110First confirmed exoplanet discovered by Gaia, along with Gaia-2b [7]
Gaia-2b0.817±0.0471.322±0.0133.6915224±0.00000390.0467±0.0015transit676±31.000±0.0955720±84First confirmed exoplanet discovered by Gaia, along with Gaia-1b [7]
Gliese 514b 0.0164±0.0028140.43±0.410.422+0.014
0.015
202±11radial vel.24.850±0.0100.510±0.0513714±51Planetary orbit partially in habitable zone [8]
Gliese 1002 b 0.0034±0.000410.3465±0.0270.0457±0.0013230.9±6.7radial vel.15.808±0.0030.120±0.0103024±52Planet in habitable zone [9]
Gliese 1002 c 0.0043±0.000521.202±0.0130.0738±0.0021181.7±5.2radial vel.15.808±0.0030.120±0.0103024±52Planet in habitable zone [9]
Gliese 3929 b 0.0055±0.00140.097±0.0042.6162745±0.0000030.0252±0.0005568±6transit51.64±0.020.309±0.0143369±51Another planet in system is suspected [10] [11]
Gliese 3929 c 0.0180±0.002915.04±0.030.081±0.002317±3radial vel.51.64±0.020.309±0.0143369±51 [11]
GJ 463 b 3.6±0.43448+110
88
3.53±0.07radial vel.59.91±0.030.49±0.023540±41Host star also known as Ross 690 [12] [13]
GJ 3090 b 0.01050.192.8531042±0.00000320.03165696transit73.21±0.040.519±0.0133556±70Host star also known as TOI-177 [14]
GJ 3090 c 0.053812.734+0.033
0.026
0.08575421radial vel.73.21±0.040.519±0.0133556±70Host star also known as TOI-177 [14]
HD 3167 e 0.0306±0.0037102.09+0.52
0.50
0.4048+0.0077
0.0074
375±7radial vel.154.59±0.130.852+0.026
0.015
5300±73 [15]
HD 18599 b 0.0758+0.0223
0.0242
0.232±0.0124.1374354+0.0000036
0.0000037
0.0480±0.0004935±11transit126.02±0.060.863±0.0205145±50Host star also known as TOI-179, also red dwarf star in the system [16] [17] [18]
HD 20329b 0.0233±0.00340.154±0.0060.926118+0.000050
0.000043
0.0180±0.00032141±27transit207.7±0.90.90±0.055596±50 [19]
HD 22532 b 2.12±0.09872.6±2.81.900±0.004radial vel.526±21.20±0.055067+59
22
Giant host star [20]
HD 22946 b 0.154±0.0094.040301+0.000023
0.000042
0.0528±0.00301378±36transit205.08±0.161.158±0.0586210+173
158
Host star also known as TOI-411, third transiting planet in system is suspected [21]
HD 22946 c 0.245±0.0139.573096+0.000026
0.000023
0.0939±0.00541033±27transit205.08±0.161.158±0.0586210+173
158
Host star also known as TOI-411, third transiting planet in system is suspected [21]
HD 23472 d 0.0017±0.00060.067±0.0053.97664+0.000030
0.000044
0.04298+0.00063
0.00065
909+35
32
transit127.48±0.060.67±0.034684±99 [22]
HD 23472 e 0.0023±0.00090.073±0.0067.90754±0.000110.0680±0.0010723+28
25
transit127.48±0.060.67±0.034684±99 [22]
HD 23472 f 0.0024±0.00130.102±0.00712.1621839+0.00012
0.000099
0.0906±0.0014630+27
23
transit127.48±0.060.67±0.034684±99 [22]
HD 28109 b 0.058+0.029
0.024
0.196±0.00922.89104+0.00035
0.00036
0.1357±0.0034881.2±7.5transit457.0±0.61.26±0.086120±50 [23]
HD 28109 c 0.025+0.013
0.010
0.378±0.01056.00819+0.00194
0.00202
0.308±0.011585.2+8.7
8.3
transit457.0±0.61.26±0.086120±50 [23]
HD 28109 d 0.018+0.009
0.007
0.290±0.01084.25999+0.00744
0.00662
0.411±0.016506.5+8.7
8.0
transit457.0±0.61.26±0.086120±50 [23]
HD 29399 b 1.57±0.11892.7±5.91.913±0.008radial vel.144.2±0.31.15±0.044845±52Giant host star [24]
HD 33142 d 0.89+0.06
0.05
810.2+3.8
4.2
1.955+0.016
0.012
radial vel.394.3±0.91.52±0.035025.4+23.6
15.5
Giant host star [25]
HD 56414 b 0.0944±0.00530.331±0.01829.04992±0.000210.229±0.0041133±30transit873±31.89±0.118500±150Host star also known as TOI-1228 [26]
HD 64121 b 2.56±0.19623.0±3.41.510±0.006radial vel.424.1±1.71.18±0.055066+58
60
Giant host star [20]
HD 69123 b 3.04±0.161193.3±7.02.482±0.010radial vel.245.0±1.31.43±0.074787+280
51
Giant host star [20]
HD 83443 c 1.5+0.5
0.2
8241+1019
530
8.0±0.8radial vel.133.6±0.21.00±0.035442±17Eccentric orbit due to hot Jupiter in system [27]
HD 93963A b 0.121±0.0041.0391353+0.0000049
0.0000045
0.02085±0.000372042±27transit268.6±1.31.109±0.0435987±64Host star also known as TOI-1797 [28]
HD 93963A c 0.288±0.0053.6451398+0.0000106
0.0000142
0.04813±0.000851344±18transit268.6±1.31.109±0.0435987±64Host star also known as TOI-1797 [28]
HD 109833 b 0.258+0.014
0.012
9.188526±0.000026transit259.5±0.21.08±0.055881±50Young host star also known as TOI-1097 [29]
HD 109833 c 0.231+0.018
0.016
13.900148±0.000057transit259.5±0.21.08±0.055881±50Young host star also known as TOI-1097 [29]
HD 114082 b 8.0±1.01.00±0.03109.75+0.40
0.37
0.5109+0.0081
0.0083
transit310.1±0.71.47±0.076651±35Young 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
1874radial vel.353.51.08+0.14
0.12
4830Host red giant star also known as HR 6840, other planets in system are suspected [32]
HD 191939 g 0.0425±0.0063284+10
8
0.812±0.028278±6radial vel.174.4±0.10.81±0.045348±100Habitable zone planet [33]
HD 191939 f >2.1>2200>3.2<125174.4±0.10.81±0.045348±100 [33]
HD 199981 b 10.070±2.48321000±800013.048±3.073radial vel.66.7±2.4Host star also known as GJ 9714 [34]
HD 105618 b 0.079±0.0089.90.091±0.004radial vel.227.8±0.4Also brown dwarf in the system [34]
HD 206893 c  [ fr ]12.3+1.1
1.2
1.46+0.18
0.06
20823.53+0.08
0.07
1181.9+20.6
53.9
radial vel.125.1±2.61.246486Some deuterium burning despite its low mass, also another brown dwarf is present in the system [35]
HD 21019 b  [ zh ]0.014±0.0022.560.034±0.002radial vel.120Host star also known as GJ 2030 [34]
HD 21019 c  [ zh ]12.934±2.36125600±250016.752±1.312radial vel.120Host star also known as GJ 2030 [34]
HD 21175 b 0.038±0.01010.60.091±0.004radial vel.57.7Host star also known as GJ 3222, planet on extremely eccentric orbit, also brown dwarf in the system [34]
HD 260655 b 0.0067±0.00110.111±0.0022.76953±0.000030.02933±0.00024709±4transit32.63±0.070.439±0.0113803±10Host star also known as TOI-4599 [36]
HD 260655 c 0.0097±0.00150.137±0.0045.70588±0.000070.04749±0.00039557±3transit32.63±0.070.439±0.0113803±10Host star also known as TOI-4599 [36]
HIP 34269 b  [ ja ]0.0052±0.00070.103±0.0050.548177±0.0000190.01188±0.000401617±41transit154.81±0.150.740±0.0174440±100Host star also known as TOI-500 [37]
HIP 34269 c  [ ja ]0.0146±0.00166.6356±0.0040radial vel.154.81±0.150.740±0.0174440±100Host star also known as TOI-500 [37]
HIP 34269 d  [ ja ]0.1055±0.003326.233±0.020radial vel.154.81±0.150.740±0.0174440±100Host star also known as TOI-500 [37]
HIP 34269 e  [ ja ]0.0376±0.004261.30±0.28radial vel.154.81±0.150.740±0.0174440±100Host star also known as TOI-500 [37]
HIP 94235 b 0.268±0.0277.713057±0.0000210.07870+0.00056
0.00017
1060±50transit191.2±0.41.094+0.024
0.007
5991±50Host star also known as TOI-4399, shares system with a red dwarf [38]
HR 7321 b 0.30±0.07285.1+1.2
1.5
0.937±0.003radial vel.200.21.35+0.19
0.21
4971Red 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.200.21.35+0.19
0.21
4971Red giant host star also known as HD 184010 [39]
HR 7321 d 0.46±0.08837.7+6.4
5.5
1.922+0.010
0.008
radial vel.200.21.35+0.19
0.21
4971Red giant host star also known as HD 184010 [39]
K2-365 b 0.0272±0.01720.259+0.017
0.015
23.448172+0.00076
0.00099
710transit0.823+0.369
0.25
5561±138 [5]
K2-366 b 0.0199±0.01150.210+0.016
0.014
15.93703+0.00079
0.00114
770transit0.825+0.366
0.255
5601±138 [5]
K2-367 b 0.0203±0.01260.215+0.020
0.017
20.64509+0.00099
0.00137
450transit0.756+0.231
0.347
4348±128 [5]
K2-368 b 0.0073±0.00420.118+0.009
0.008
5.02559+0.00028
0.00034
800transit0.746+0.334
0.232
4663±138 [5]
K2-368 c 0.0078±0.00410.121+0.010
0.009
9.66018±0.00116650transit0.746+0.334
0.232
4663±138 [5]
K2-368 d 0.0146±0.00850.173+0.013
0.012
20.20108+0.00235
0.00273
500transit0.746+0.334
0.232
4663±138 [5]
K2-369 b 0.0069±0.00400.117+0.009
0.008
5.76161+0.00084
0.00071
1080transit0.735+0.334
0.224
5682±138 [5]
K2-370 b 0.0327±0.02070.286+0.020
0.048
2.14084+0.00003
0.00004
1420transit0.984+0.428
0.303
5377±138 [5]
K2-371 b 4.7±2.21.162+0.082
0.077
3.11490±0.000011000transit0.958+0.44
0.298
4925±138 [5]
K2-372 b 0.0289±0.01680.262±0.0069.84407+0.00056
0.00057
870transit0.847+0.101
0.088
5479±27 [5]
K2-373 b 0.0162±0.00890.184+0.013
0.012
11.02066+0.00143
0.00136
1130transit1.158+0.499
0.349
6138±138 [5]
K2-374 b 0.0113±0.00580.142±0.0054.52195+0.00032
0.00040
1210transit0.731+0.067
0.061
5789±21 [5]
K2-374 c 0.0179±0.01090.197+0.008
0.007
16.43445+0.00237
0.00270
790transit0.731+0.067
0.061
5789±21 [5]
K2-375 b 0.0183±0.01060.200+0.016
0.015
14.45389+0.00477
0.00417
1000transit1.119+0.492
0.344
5822±138 [5]
K2-376 b 0.0129±0.00740.155+0.011
0.010
5.77647+0.00026
0.00023
1240transit0.908+0.394
0.281
5937±138 [5]
K2-377 b 0.0123±0.00730.151+0.013
0.011
12.83223+0.00155
0.00161
530transit0.821+0.371
0.258
4200±138 [5]
K2-378 b 0.0283±0.01730.257+0.024
0.020
2.06043+0.00011
0.00007
1130transit0.923+0.425
0.291
4823±138 [5]
K2-379 b 0.0175±0.01040.194+0.032
0.017
8.77724+0.00062
0.00061
680transit0.856+0.375
0.265
4603±138 [5]
K2-380 b 0.0250±0.01440.243+0.016
0.015
9.40131+0.00046
0.00050
1110transit0.993+0.416
0.302
5911±138 [5]
K2-381 b 0.0040±0.00260.095+0.012
0.009
7.93893±0.00059670transit0.754+0.337
0.239
4473±138 [5]
K2-381 c 0.0158±0.00940.178+0.016
0.013
16.03465+0.00184
0.00157
530transit0.754+0.337
0.239
4473±138 [5]
K2-381 d 0.0121±0.00700.150+0.016
0.012
26.80302+0.00277
0.00304
440transit0.754+0.337
0.239
4473±138 [5]
K2-382 b 0.0162±0.01010.185+0.013
0.011
21.70015+0.00202
0.00191
610transit0.922+0.401
0.284
5452±138 [5]
K2-383 b 0.0102±0.00520.139+0.010
0.009
1.86596±0.000011270transit1.061+0.459
0.327
5129±138 [5]
K2-384b  [ ja ]0.0040±0.00260.096+0.020
0.005
2.23152+0.0019
0.00032
600transit0.330±0.0093623±138 [5]
K2-384c  [ ja ]0.0054±0.00270.106+0.004
0.006
4.19476+0.00030
0.00018
480transit0.330±0.0093623±138 [5]
K2-384d  [ ja ]0.0085±0.00440.124+0.010
0.006
6.67958+0.00071
0.00049
410transit0.330±0.0093623±138 [5]
K2-384e  [ ja ]0.0075±0.00420.120+0.012
0.007
9.71504+0.00100
0.00073
370transit0.330±0.0093623±138 [5]
K2-384f  [ ja ]0.0179±0.01040.198+0.008
0.007
13.62749+0.00034
0.00057
330transit0.330±0.0093623±138 [5]
K2-385 b 0.0100±0.00560.137+0.012
0.011
2.38086+0.00016
0.00021
1100transit1370±200.9270+0.4120
0.2860
4844±138 [5]
K2-386 b 0.0195±0.01150.207+0.006
0.005
7.47322+0.00037
0.00031
1010transit1400±300.911+0.088
0.083
5749±22 [5]
K2-387 b 0.1430±0.09960.653±0.02328.73532±0.00099340transit870±120.570+0.051
0.048
3572±138 [5]
K2-388 b 0.0412±0.02630.326+0.029
0.020
6.33906+0.00022
0.00018
970transit948±130.8420+0.3760
0.2590
5367±138 [5]
K2-389 b 0.0177±0.01030.195±0.0108.58404+0.00088
0.00202
1050transit846±90.8020+0.3570
0.2460
5782±138 [5]
K2-389 c 0.0165±0.00850.182+0.013
0.012
20.85133+0.00280
0.00298
780transit846±90.8020+0.3570
0.2460
5782±138 [5]
K2-390 b 0.0636±0.03900.416+0.027
0.030
3.31279±0.000101310transit1490±180.7890+0.3510
0.2390
5558±138 [5]
K2-391 b 0.0078±0.00530.122+0.025
0.016
4.62265+0.00022
0.00025
900transit1660±500.7570+0.3410
0.2400
5543±138 [5]
K2-392 b 0.0140±0.00790.165+0.014
0.013
15.39872+0.00242
0.00193
840transit1330±300.8410+0.3700
0.2580
5726±138 [5]
K2-393 b 0.0199±0.01270.210+0.015
0.014
10.41318+0.00093
0.00069
950transit867±90.8810+0.3810
0.2690
5678±138 [5]
K2-394 b 0.0123±0.00630.151+0.012
0.011
5.09571±0.00011890transit319.7±1.50.478+0.214
0.147
4938±138 [5]
K2-395 b 0.0240±0.01410.231+0.017
0.015
4.80335+0.00035
0.00046
910transit935±100.9520+0.4210
0.2930
5007±138 [5]
K2-395 c 0.0371±0.02200.303+0.025
0.022
8.49128+0.00033
0.00030
750transit935±100.9520+0.4210
0.2930
5007±138 [5]
K2-396 b 0.0106±0.00610.140+0.010
0.009
0.6736±0.000011990transit897±90.9540+0.4290
0.2930
5236±138 [5]
K2-396 c 0.0314±0.01890.278+0.015
0.010
25.76051+0.00199
0.00188
590transit897±90.9540+0.4290
0.2930
5236±138 [5]
K2-397 b 0.0212±0.01270.216±0.0163.57232+0.00018
0.00015
1210transit650±50.9370+0.4060
0.2850
5387±138 [5]
K2-398 b 0.0191±0.01120.203+0.010
0.009
6.39302+0.00113
0.00075
1240transit1980±400.9450+0.0900
0.0830
5946±20 [5]
K2-398 c 0.0736±0.04120.455±0.01318.78783+0.00087
0.00099
870transit1980±400.9450+0.0900
0.0830
5946±20 [5]
K2-400 b 0.0051±0.00250.103±0.0043.86505±0.00018570transit203.5±0.80.374±0.0093578±138 [5]
K2-401 b 0.0183±0.01170.201+0.018
0.017
6.29309+0.00057
0.00070
660transit655±50.8700+0.3950
0.2690
4213±138 [5]
K2-402 b 0.0245±0.01490.239+0.019
0.017
17.27474+0.00259
0.00317
870transit1710±600.9440+0.4190
0.2900
5716±138 [5]
K2-403 b 0.0783±0.05150.476+0.031
0.034
33.58977±0.00076580transit804±80.7840+0.3400
0.2410
5511±138 [5]
K2-404 b 0.0230±0.01270.225±0.00713.11536+0.00044
0.00060
450transit397±20.552±0.0153748±138 [5]
K2-405 b 0.0586±0.03420.407+0.007
0.010
3.43547±0.00003980transit643±71.034+0.459
0.314
4927±138 [5]
K2-406 b 0.063±0.0390.410+0.027
0.026
22.5494+0.00137
0.00143
720transit278±20.7980+0.3390
0.2450
5784±138 [5]
K2-407 b 0.0066±0.00350.114+0.008
0.007
4.9419+0.00066
0.00069
1110transit [5]
K2-407 c 0.0078±0.00440.121+0.008
0.007
9.22453+0.00132
0.00091
900transit [5]
K2-408 b 0.0122±0.00620.149+0.010
0.009
20.97895+0.00130
0.00124
610transit [5]
K2-409 b 0.0212±0.01270.221+0.015
0.014
1.90808+0.00004
0.00005
1800transit [5]
K2-2016-BLG-0005Lb 1.1±0.14.4+1.9
0.4
4700+3300
700
microlensing17000±7000.58±0.03 [1]
Kepler-451 c 1.61±0.141460±902.1±0.2timing1340±200.48+0.12 [40]
Kepler-451 d 1.76±0.1843.0±0.10.20±0.03timing1340±200.48+0.12 [40]
Kepler-1656 c 0.40±0.091919+27
24
3.053±0.049radial vel.1.03±0.04 [41]
Kepler-1708b <4.60.8886+0.0535
0.0526
737.11310+0.00146
0.00770
1.64±0.10transit5436+334
298
1.088±0.0726157+231
202
Possible exomoon host [42] [43]
Kepler-1972b  [ ja ]0.0064±0.00190.072±0.0047.54425±0.00054transit923±31.12±0.035818±27Very dense planets, additional planet in system suspected [44]
Kepler-1972c  [ ja ]0.0066±0.00200.078±0.00511.3295±0.0011transit923±31.12±0.035818±27Very dense planets, additional planet in system suspected [44]
KMT-2016-BLG-1105b 0.007+0.023
0.005
2.44+0.88
0.75
microlensing17000±70000.41+0.25
0.21
[45]
KMT-2017-BLG-0428b 0.018+0.011
0.009
1.81+0.55
0.59
microlensing18000+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
microlensing17000+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
microlensing23000±20000.32+0.31
0.17
[45]
KMT-2017-BLG-1194b 0.011±0.0061.78+0.45
0.46
microlensing14000±60000.41+0.23
0.19
[45]
KMT-2018-BLG-0030b 1.45+1.23
0.88
4.39+2.18
2.40
microlensing21000+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
microlensing23000+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
microlensing22000+3000
4000
0.29+0.28
0.14
[47]
KMT-2018-BLG-2004b 0.27±\0.124.62+0.80
1.10
microlensing23000+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
microlensing14000±60000.66+0.42
0.36
[47]
KMT-2018-BLG-2718b 16.0+11.7
8.0
4.86+2.97
2.55
microlensing15000+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
microlensing14000+5000
6000
0.74+0.43
0.38
[46]
KMT-2019-BLG-1042Lb 0.19+0.21
0.11
1.7±0.5microlensing22000+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
microlensing15000+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
microlensing15000+6000
5000
0.79+0.33
0.36
[49]
KMT-2019-BLG-1806b 0.015±0.0053.02+0.70
0.73
microlensing22000+2000
7000
0.74±0.25 [45]
KMT-2019-BLG-2974Lb 0.28+0.29
0.18
2.0+0.8
0.7
microlensing20000+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
microlensing15000+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
microlensing23000+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
microlensing23000+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
microlensing23000+3000
4000
0.32+0.39
0.21
[52]
KMT-2021-BLG-0748b 0.45+0.40
0.25
2.43±0.67microlensing20000+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
microlensing11000+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
microlensing22000+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
microlensing10000+3000
2000
0.22+0.12
0.07
[55]
KMT-2021-BLG-0909b 1.26+1.01
0.66
1.75±0.42microlensing21000+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
microlensing27000±30000.14+0.19
0.07
[56]
KMT-2021-BLG-1077Lc 0.25+0.35
0.13
0.93+1.05
0.80
microlensing27000±30000.14+0.19
0.07
[56]
KMT-2021-BLG-1105b 1.30±0.683.54±1.06microlensing15000±50000.63±0.33 [55]
KMT-2021-BLG-1253b 0.0599+0.0643
0.0319
1.52+0.57
0.41
microlensing22000+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
microlensing20000+3000
5000
0.57+0.32
0.29
Host star also known as MOA-2021-BLG-182 [52]
KMT-2021-BLG-1372b 0.1928±0.11292.37±0.77microlensing19000+5000
8000
0.42±0.25 [53]
KMT-2021-BLG-1391b 0.0143±0.00732.29+0.56
0.71
microlensing19000+3000
5000
0.37±0.19 [53]
KMT-2021-BLG-1554Lb 0.12+0.20
0.07
0.72+0.13
0.14
microlensing25000+3000
4000
0.08+0.13
0.04
[52]
KMT-2021-BLG-1689Lb 0.145+0.094
0.072
2.5+0.8
06
microlensing23000+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
microlensing23000+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±0.16microlensing22000±30000.11+0.17
0.06
Multiple orbital solutions [54]
KMT-2021-BLG-2478b 0.80+0.56
0.35
1.38±0.26microlensing8000+4000
3000
0.12+0.09
0.06
[55]
L 363-38 b 0.0147±0.00148.781±0.0070.048±0.006330radial vel.33.310.213129Host star also known as Gliese 3049 [58]
MOA-2019-BLG-008L b 30microlensing8000±20000.8 [59]
MOA-2020-BLG-135Lb 0.036+0.060
0.021
1.11+0.23
0.20
microlensing26000±30000.23+0.39
0.14
[60]
MOA-2020-BLG-208Lb 0.217+0.116
0.106
2.88+0.40
0.41
microlensing25000±30000.656+0.346
0.322
[61]
Mu2 Scorpii b 14.4290imaging4749.121900 [62]
Mu2 Scorpii c 18.521imaging4749.121900 [62]
NGTS-20 b 2.98+0.16
0.15
1.07±0.0454.18915±0.000150.313±0.013688+14
13
transit1195±81.47±0.095980±80Planet on eccentric orbit, host star also known as TOI-5152 [63]
NGTS-21b 2.36±0.211.33±0.031.5433897±0.00000160.0236±0.00051357±15transit2090+90
80
0.72±0.044660±41 [64]
NGTS-23b 0.613±0.0971.267±0.0304.0764326±0.00000410.0504±0.0121327+17
16
transit3230±701.01+0.06
0.07
6057±64 [65]
NGTS-24b 0.52+0.12
0.11
1.214+0.058
0.062
3.4678796±0.00000700.0479+0.0028
0.0030
1499+41
36
transit2360±801.26+0.05
0.21
5820+93
8
[65]
NGTS-25b 0.639+0.058
0.052
1.023+0.035
0.052
2.8230930±0.00000330.0388+0.0014
0.002
1101+15
14
transit2350±300.91+0.03
0.04
5321±58 [65]
OGLE-2016-BLG-1093Lb 0.71±0.122.13±0.33microlensing26000±20000.46±0.08 [66]
OGLE-2017-BLG-1691Lb 0.046+0.037
0.025
2.41+0.34
0.44
microlensing24000+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
microlensing21000+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
microlensing21000+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
microlensing22000±30000.72+0.29
0.25
[48]
OGLE-2018-BLG-1119Lb 0.91+0.66
0.52
4.06+2.14
2.58
microlensing19000+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
microlensing19000+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
microlensing5100+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
microlensing0.28+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
microlensing21000+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
microlensing26000+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
microlensing19000±20000.42+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
microlensing20000±40000.55+0.17Circumbinary planet [68]
Pi Mensae d 0.0421±0.0042124.64+0.48
0.52
radial vel.59.62±0.071.11±0.016013±18 [69]
Proxima Centauri d 0.0008±0.00025.122+0.002
0.0036
0.02885+0.00019
0.00022
360radial vel.4.2465±0.00030.1221±0.00222900±100 [70]
PSR J2007+3120 b 0.0072±0.0009723±8timing22000Pulsar planet, another planet in the system is suspected. [71]
Ross 508 b 0.0126±0.001910.76+0.01
0.02
0.05353+0.00047
0.00051
radial vel.36.594±0.0110.1774±0.00453071+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
transit314±20.781±0.0424994±50 [73]
TOI-206 b 0.116±0.0040.7363104±0.00000030.0112±0.0001910±36transit155.90.35±0.013383±157 [74]
TOI-277 b 0.0239+0.0179
0.0098
0.237±0.0163.9940±0.00040.0269±0.0011transit212.6+0.6
0.3
0.16±0.014031+21
23
[75]
TOI-500 b 0.104±0.0100.5481579±0.00000060.0128±0.00111693±105transit154.80.88±0.254621±50 [74]
TOI-544 b 0.181±0.0091.5483510±0.00000150.0251 ± 0.00191082±47transit132.70.85±0.204369±100 [74]
TOI-620 b 5.0988179+0.0000045
0.0000046
0.04825+0.00065
0.00066
603.6+5.5
5.3
transit107.81±0.190.577+0.024
0.023
3708+57
56
[76]
TOI-778 b 2.76±0.241.375±0.0454.633611±0.0000010.060±0.0031561+33
32
transit530±41.428±0.0946715±128 [77]
TOI-833 b 0.113±0.0061.0418777±0.00003240.0171±0.00031118±49transit136.30.61±0.033920±160 [74]
TOI-969 b 0.0286±0.00310.247±0.0331.8237305+0.0000020
0.0000021
0.02636±0.00017941±31transit253.8±0.50.730±0.0374550±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±0.50.730±0.0374550±75Eccentric orbit [78]
TOI-1064b 0.0425±0.00550.231±0.0046.443868±0.0000250.06152+0.00086
0.00089
784±13transit224.5±0.20.748±0.0324734±67 [79]
TOI-1064c 0.0079+0.0057
0.0063
0.237±0.00412.226574+0.000046
0.000043
0.09429+0.00132
0.00136
634±10transit224.5±0.20.748±0.0324734±67 [79]
TOI-1075 b 0.154±0.0070.6047328±0.00000320.0118±0.00011336±56transit200.90.60±0.023921±157 [74]
TOI-1075 b 0.0313±0.00420.160+0.010
0.007
0.6047328±0.00000320.01159+0.00023
0.00020
1323±44transit200.4+0.6
2.2
0.604±0.0303875±75 [80]
TOI-1107b 3.35±0.181.30±0.054.0782387+0.0000024
0.0000025
0.0561+0.0024
0.0025
1728±27transit925±71.35±0.086311±98 [81]
TOI-1136 b 0.0095+0.0022
0.0028
0.170+0.019
0.013
4.1728±0.0002transit275.8±0.51.022±0.0275770±50 [82]
TOI-1136 c 0.0189+0.0041
0.0053
0.257±0.0056.2573±0.0002transit275.8±0.51.022±0.0275770±50 [82]
TOI-1136 d 0.0252+0.0076
0.0060
0.413±0.00712.5194±0.0004transit275.8±0.51.022±0.0275770±50 [82]
TOI-1136 e 0.0170±0.00310.236+0.006
0.008
18.7992+0.0017
0.0015
transit275.8±0.51.022±0.0275770±50 [82]
TOI-1136 f 0.0261+0.0088
0.0113
0.346±0.01026.3162+0.0017
0.0013
transit275.8±0.51.022±0.0275770±50 [82]
TOI-1136 g 0.0151+0.0148
0.0104
0.226±0.01039.5387+0.0036
0.0030
transit275.8±0.51.022±0.0275770±50 [82]
TOI-1181 b 1.18±0.141.30±0.082.103195+0.000012
0.000011
2162transit1013±31.38+0.086
0.082
6260±100Subgiant host star [83]
TOI-1221 b 0.259±0.01191.68278+0.00032
0.00041
0.404+0.026
0.023
400transit447.1±0.71.03±0.065592±50 [84]
TOI-1246 b  [ ja ]0.0255±0.00350.269±0.0054.30744±0.000020.049±0.002955transit557.9±1.01.12±0.165217±50 [85]
TOI-1246 c  [ ja ]0.0277±0.00380.224±0.0075.904144±0.0000830.061±0.002860transit557.9±1.01.12±0.165217±50 [85]
TOI-1246 d  [ ja ]0.0167±0.00530.313±0.00818.65590±0.000480.131±0.004586transit557.9±1.01.12±0.165217±50 [85]
TOI-1246 e  [ ja ]0.0466±0.00720.338±0.01437.9216±0.00100.211±0.007462transit557.9±1.01.12±0.165217±50 [85]
TOI-1260 d 0.0373±0.02450.276±0.00816.608164±0.0000830.1116±0.0033499±4transit239.5±0.30.66±0.014227±85 [86]
TOI-1268 b 0.303±0.0260.81±0.058.1577080±0.00000440.072+0.009
0.010
919transit359.1±0.40.92±0.035290±117 [87]
TOI-1272 b 0.0774±0.00720.370±0.0193.31599±0.000020.0412±0.0008961±32transit450.6±1.30.851±0.0494985±121 [88]
TOI-1272 c 0.0840±0.00988.689±0.0080.0783±0.0014697±23radial vel.450.6±1.30.851±0.0494985±121 [88]
TOI-1288 b 0.0712+0.0574
0.0304
0.454±0.0102.69998±0.000150.0429±0.0006transit375.3+1.3
0.5
1.46±0.065307+18
16
[75]
TOI-1288 c 0.2643±0.0220443+11
13
radial vel.375.3+1.3
0.5
1.46±0.065307+18
16
[89]
TOI-1411 b 0.121±0.0131.4520358±0.00000980.0230±0.00261136±59transit106.00.59±0.234266±100 [74]
TOI-1422 b 0.0283+0.0072
0.0063
0.354+0.012
0.010
12.9972±0.00060.108±0.003867±17transit504.17+0.12
0.09
0.981+0.062
0.065
5840±62Another planet in the system is suspected. [90]
TOI-1442 b 0.104±0.0050.4090677±0.00000030.0071±0.00021072±54transit134.50.29±0.023330±160 [74]
TOI-1452 b 0.0152±0.00410.149±0.00611.06201±0.000020.061±0.003326±7transit99.51±0.040.249±0.0083185±50Also a red dwarf on a 97AU separation in the system [91]
TOI-1468 b 0.0101±0.00080.114±0.0031.8805136+0.0000024
0.0000026
682.2+7.4
6.9
transit80.64±0.070.339±0.0113496±25 [92]
TOI-1468 c 0.0209±0.00210.184±0.00415.532482+0.000034
0.000033
337.5+3.7
3.4
transit80.64±0.070.339±0.0113496±25 [92]
TOI-1516 b 3.16±0.121.36±0.032.056014±0.0000021820transit804.6±1.91.085+0.061
0.066
6420±100 [83]
TOI-1669 b 0.0132±0.00850.214±0.0162.7transit364.61.00±0.055542.3±100.0 [93] Host star also known as BD+82 71, planet suspected since 2020 [94]
TOI-1669 c 0.602±0.078501±16radial vel.364.61.00±0.055542.3±100.0 [93] Host star also known as BD+82 71, additional long-period companion is suspected.
TOI-1694 b 0.0979±0.00660.461±0.0163.8transit405.70.84±0.035066±100 [93] Host star also known as TYC 4108-1434-1, planet suspected since 2020 [94]
TOI-1694 c 0.929±0.037393.2±4.3radial vel.405.70.84±0.035066±100 [93] Host star also known as TYC 4108-1434-1
TOI-1670 b 0.04±0.030.184+0.017
0.013
10.98462+0.00046
0.00051
0.103±0.0021062+14
13
transit540.6+1.0
1.2
1.21±0.026170±61 [95]
TOI-1670 c 0.63+0.09
0.08
0.987±0.02540.74976+0.000022
0.00021
0.249±0.005684±9transit540.6+1.0
1.2
1.21±0.026170±61 [95]
TOI-1693 b 0.126±0.0091.7666957±0.00000540.0226±0.0004764±19transit100.60.49±0.033499±70 [74]
TOI-1695 b 0.0173±0.00310.181±0.0163.1342790±0.00000720.033548+0.000260
0.000268
590±90transit147.2±0.20.51±0.023627±31 [96] [97]
TOI-1696 b 0.17810.276±0.0102.500311±0.0000040.0229±0.0002489±13transit210.8±0.50.255±0.00663185±76 [98] [99]
TOI-1710 b 0.0890±0.01480.477±0.01024.283429±0.000430.16±0.04687±50transit264.7±0.20.984+0.050
0.059
5665±55 [100]
TOI-1759 b 0.021±0.060.279±0.0218.849975±0.0000060.1176±0.0013433±14transit130.85±0.050.606±0.0204065±51 [101] [102]
TOI-1811 b 0.974+0.075
0.076
1.002+0.026
0.024
3.7130818±0.00000280.04393+0.00058
0.00054
961.5±8transit418±30.819+0.033
0.030
4753+54
55
[103]
TOI-1820 b 2.3±0.21.12±0.024.860700±0.0000100.069±0.0051295±11transit807±131.04±0.135734±50 [104]
TOI-1860 b 0.117±0.0051.0662107±0.00000140.0204±0.00021885±28transit149.80.99±0.035752±100 [74]
TOI-1937 b 2.01+0.17
0.16
1.247+0.059
0.062
0.94667944±0.000000470.01932+0.00035
0.00039
2097+35
36
transit1366±61.072+0.059
0.064
5814+91
93
[105]
TOI-2000 b 0.0324±0.00700.236±0.0103.098331+0.000021
0.000019
0.04260+0.00076
0.00067
1475+120
158
transit566.3±1.01.074+0.059
0.050
5607+86
82
[106]
TOI-2000 c 0.238±0.0120.711±0.0119.1270553±0.00000730.0875+0.0016
0.0014
1029+84
111
transit566.3±1.01.074+0.059
0.050
5607+86
82
[106]
TOI-2025 b 4.4±0.41.120±0.0098.872086±0.0000090.089±0.0041186±11transit1106±71.32±0.145880±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
transit1095±111.176+0.079
0.091
5928+76
75
[103]
TOI-2046 b 2.30±0.081.44±0.111.4971842+0.0000031
0.0000033
1998transit940±31.153+0.100
0.093
6160±100Young host star [83]
TOI-2048 b 0.184±0.01813.79019+0.00065
0.00084
640±20transit379.7±0.50.83±0.035185±60Young host star belongs to NGC 3532 [107]
TOI-2081 b 0.0157+0.0151
0.0076
0.182±0.04610.50534+0.00007
0.00008
0.0752+0.0047
0.0119
488+28
52
transit203.26±0.160.540±0.0803800±100 [108]
TOI-2136 b 0.0200+0.0077
0.0072
0.196±0.0157.851928+0.000018
0.000016
0.057±0.006395+24
22
transit108.82±0.070.34±0.023342±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
transit733±51.720+0.057
0.068
6189±67Host 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
transit988±131.516+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±0.00000250.0513+0.0011
0.0013
1580±27transit967±101.233+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±0.012348.0+3.3
3.6
transit379.4±0.81.111+0.047
0.046
5695+58
60
[111]
TOI-2158 b 0.82±0.080.960±0.0128.60077±0.000030.075±0.0041188±10transit652±31.12±0.125673±50 [104]
TOI-2193 b 0.94±0.181.772.1225735±0.00000160.03319+0.00052
0.00051
1763+21
22
transit1126±31.082+0.052
0.049
5974±110Also 0.54M star in the system [112]
TOI-2196 b 0.0818±0.00410.313±0.0131.1947268+0.0000079
0.0000093
0.02234±0.000601860±20transit861±31.032±0.0385634±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
transit1242±91.296+0.069
0.072
6075±110 [112]
TOI-2260 b 0.145±0.0120.3524728±0.00000470.0097±0.00012609±86transit331.20.99±0.045534±100 [74]
TOI-2236 b 1.58+0.40
0.39
1.282+0.032
0.031
3.5315902±0.00000260.05009+0.00080
0.00082
1688+19
21
transit1149±51.343+0.066
0.065
6164±50 [112]
TOI-2337b 1.60±0.150.9±0.12.99432±0.000080.04467transit1780±201.325±0.1184780±100 [114]
TOI-2364 b 0.225+0.043
0.049
0.768+0.023
0.018
4.0197517±0.00000430.04871+0.00069
0.00079
1091+17
14
transit713±60.954+0.041
0.046
5306+76
68
[105]
TOI-2411 b 0.150±0.0100.7826942±0.00000370.0144±0.00011355±45transit194.50.65±0.024099±123 [74]
TOI-2421 b 0.333±0.0790.925+0.035
0.034
4.3474032+0.0000079
0.0000078
0.0543+0.0021
0.0010
1534+20
28
transit1067±71.131+0.130
0.064
5577±50 [112]
TOI-2427 b 0.161±0.0111.3060011±0.00001020.0202±0.00021117±46transit93.10.64±0.024072±121 [74]
TOI-2445 b 0.112±0.0070.3711281±0.00000050.0064±0.00011060±54transit158.70.25±0.013333±157 [74]
TOI-2497 b 5.21±0.521.000+0.040
0.038
10.655661±0.0000260.1167+0.0018
0.0017
1596+44
41
transit930±141.861+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±0.0000130.0672+0.0024
0.0012
1352+18
19
transit1691±81.130+0.130
0.059
5650±50 [112]
TOI-2570 b 0.820+0.063
0.065
1.217+0.035
0.034
2.9887615±0.00000220.04145+0.00081
0.00086
1431+24
23
transit1179±61.063+0.063
0.065
5765±50 [112]
TOI-2583 b 0.250+0.058
0.056
1.290+0.040
0.033
4.5207265±0.00000490.0571+0.0010
0.0013
1456+19
16
transit1831±91.215+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±0.0000110.0635+0.0025
0.0013
1445+23
26
transit1242±101.15+0.14
0.07
5760+80
79
[105]
TOI-2669b 0.61±0.191.76±0.166.2034±0.0001transit1294±91.19±0.164800±100 [114]
TOI-2796 b 0.44+0.10
0.11
1.594.8084983+0.0000057
0.0000056
0.0569+0.0010
0.0011
1205+18
17
transit1150±61.063+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±0.000000820.03185±0.000521893+29
28
transit1635±91.118+0.056
0.054
6280+99
96
[105]
TOI-2818 b 0.71±0.261.363+0.046
0.045
4.0397090+0.0000024
0.0000023
0.0493+0.0010
0.0008
1376+26
24
transit1028±30.977+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
transit1501±81.135+0.077
0.079
5910±100 [105]
TOI-2977 b 1.68+0.26
0.25
1.174+0.031
0.027
2.3505614±0.00000250.03386+0.00067
0.00050
1544±26transit1160±300.936+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±0.00000310.0505+0.0015
0.0009
1596+24
25
transit1281±51.12+0.11
0.06
5760+85
88
[105]
TOI-3331 b 2.27±0.161.158±0.0432.0180231+0.0000043
0.0000044
0.03144+0.00048
0.00055
1488+31
29
transit733±41.016+0.047
0.052
5521±110Also 0.6M star in the system [112]
TOI-3364 b 1.67+0.12
0.13
1.091+0.038
0.032
5.8768918±0.00000690.0675+0.0011
0.0016
1264+22
21
transit899±31.186+0.059
0.083
5706+95
91
[105]
TOI-3540 b 1.18±0.142.103.1199990±0.00000790.04289+0.00092
0.00093
1498±22transit921±101.081+0.071
0.069
5969±50Also 0.8M star in the system [112]
TOI-3629 b 0.26±0.020.74±0.023.936551+0.000005
0.000006
0.043±0.002690±20transit423.1±1.00.63±0.023870±90 [115]
TOI-3688 b 0.98+0.10
0.11
1.167+0.048
0.044
3.246075±0.0000120.04560+0.00089
0.00098
1534+29
28
transit1308±61.199+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
transit576±20.867+0.036
0.037
5274±50 [112]
TOI-3714 b 0.70±0.0031.01±0.032.154849±0.0000010.027±0.001750±20transit367.0+0.6
1.3
0.53±0.023660±90 [115]
TOI-3757 b 0.2684±0.02761.07+0.04
0.05
3.4387530+0.0000039
0.0000040
0.03845±0.00043759±13transit579±20.64±0.023913±56 [116]
TOI-3807 b 1.04+0.15
0.14
2.002.8989727+0.0000038
0.0000039
0.0421+0.0007
0.0011
1646+25
24
transit1399±71.181+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±0.00000550.04611+0.00069
0.00096
1633+21
19
transit1834±171.242+0.057
0.076
5859+72
71
[105]
TOI-3884 b 0.0519+0.0110
0.0057
0.563±0.0254.5445697±0.00000940.0354±0.0014463±12transit141.37±0.160.2813±0.00673269±70 [117] [118]
TOI-3912 b 0.406+0.071
0.068
1.274+0.041
0.040
3.4936264±0.00000380.0463+0.0012
0.0010
1512±20transit1533±91.088+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
transit1703±81.254+0.067
0.072
5975+70
69
[105]
TOI-4087 b 0.73±0.141.164+0.025
0.024
3.17748350±0.000000940.04469+0.00048
0.00054
1458+20
17
transit1013±41.178+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±0.00000650.05222+0.00089
0.00096
1570+25
24
transit1128±71.313+0.068
0.071
6134±50 [112]
TOI-4145 b 0.43±0.131.187+0.032
0.031
4.0664428±0.00000580.04823+0.00075
0.00079
1074+19
16
transit668.7±1.30.905+0.043
0.044
5281+86
76
[105]
TOI-4329b 0.45±0.091.50±0.192.9223±0.00015transit2258±161.538±0.0496000±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
transit579.5±1.81.056+0.059
0.063
5640+89
82
[105]
TOI-4479 b 0.0261+0.0252
0.0126
0.252±0.0571.15890+0.00001
0.00002
0.0164+0.0015
0.0029
861+64
103
transit262.9±0.30.452±0.0903400±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±0.013349±10transit1131±121.218+0.054
0.048
6096±32Highly eccentric orbit [119]
TOI-4582 b 0.53±0.050.94+0.09
0.12
31.034±0.001transit12421.34±0.065190±100Evolved star, eccentric planetary orbit [120]
TOI-4791 b 2.31+0.32
0.33
1.110±0.0504.280880+0.000022
0.000023
0.0555+0.0011
0.0012
1472+26
24
transit1051±61.242+0.072
0.077
6058+99
94
[105]
TOI-5153 b 3.26+0.18
0.17
1.06±0.0420.33003±0.000070.158±0.006906±13transit1272.336±111.24±0.076300±80 [63]
TOI-5174 b 0.078010.4766712.214transit1.0±0.125 [121] [122]
TOI-5205b 1.08±0.061.03±0.031.630757±0.0000010.0199±0.0002737±15transit283.35±0.160.392±0.0153430±54 [123]
TOI-5542 b 1.32±0.101.009+0.036
0.035
75.12375+0.00019
0.00018
0.332±0.016441+48
74
transit1154±120.890+0.056
0.031
5700±80 [124]
Berry 37a 0.69+0.47
0.43
1.41±0.145.616531±0.0000230.066±0.007961.5±8transit20±601.32±0.094200±140 [125]
TYC 2187-512-1 b 0.33±0.02691.90+8.77
8.61
1.22±0.02radial vel.50.512±0.0160.498±0.0193734±54 [125]
WASP-132c 0.165±0.0091.011534±0.0000050.0182±0.0003transit3900.782±0.0344714+87
88
[126]

Specific exoplanet lists

Lists of exoplanets

Lists of exoplanets by year of discovery

Related Research Articles

Pi Mensae, also known as HD 39091, is a G-dwarf star in the constellation of Mensa. This star has a high proper motion. The apparent magnitude is 5.67, which can be visible to the naked eye in exceptionally dark, clear skies. It is nearly 60 light-years away. The star is slightly larger than the Sun in terms of mass, size, luminosity, temperature and metallicity, and is about 730 million years younger. It hosts three known planets.

K2-3, also known as EPIC 201367065, is a red dwarf star with three known planets. It is on the borderline of being a late orange dwarf/K-type star, but because of its temperature, it is classified as a red dwarf.

<span class="mw-page-title-main">HD 191939</span> Star in the constellation Draco

HD 191939 is a single yellow (G-type) main-sequence star, located approximately 174 light-years away in the constellation of Draco, taking its primary name from its Henry Draper Catalogue designation.

HD 108236 is a G-type main-sequence star. Its surface temperature is 5660±61 K. HD 108236 is severely depleted in heavy elements compared to the Sun, with a metallicity Fe/H index of −0.28±0.04, and is probably older than the Sun at an age of 6.7+3.3
−3.4
billion years.

TOI-640 b is an exoplanet that was suspected since 2019. Its discovery has been confirmed by the TESS team in January 2021. It is located 1115 light years away from Earth, orbiting a primary F-class star in a binary star system with red dwarf and has an orbital period of 5 days.

<span class="mw-page-title-main">L 98-59 b</span> Terrestrial planet orbiting L 98-59

L 98-59 b is an exoplanet having a size between that of the Earth and Mars and a mass only half that of Venus. It orbits L 98-59, a red dwarf 35 light-years away in the constellation Volans. There are at least 3 other planets in the system: L 98-59 c, d, e, and the unconfirmed L 98-59 f. Its discovery was announced on 27 June 2019 on the NASA website. It was the smallest planet discovered by TESS until the discovery of LHS 1678b, and was the lowest-mass planet whose mass has been measured using radial velocities until Proxima Centauri d was found in 2022.

L 98-59 is a bright M dwarf star, located in the constellation of Volans, at a distance of 10.608 parsecs, as measured by the Gaia spacecraft.

References

  1. 1 2 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 .
  2. Starr, Michelle (4 April 2022). "The Most Distant Exoplanet Ever Found by Kepler Is... Surprisingly Familiar". ScienceAlert . Retrieved 4 April 2022.
  3. 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
  4. 1 2 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
  5. 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35 36 37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53 54 55 56 57 58 59 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
  6. 1 2 3 4 5 6 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
  7. 1 2 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.
  8. 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
  9. 1 2 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
  10. 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
  11. 1 2 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
  12. A Jupiter Analog Orbiting The Nearby M Dwarf GJ 463
  13. 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
  14. 1 2 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
  15. Bourrier, V.; et al. (2022), "A CHEOPS-enhanced view of the HD 3167 system", Astronomy & Astrophysics, 668: A31, arXiv: 2209.06937 , Bibcode:2022A&A...668A..31B, doi:10.1051/0004-6361/202243778, S2CID   251861892
  16. 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 , Bibcode:2023A&A...675A.158D, doi:10.1051/0004-6361/202244611, S2CID   252907692
  17. 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
  18. 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
  19. 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
  20. 1 2 3 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.
  21. 1 2 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
  22. 1 2 3 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
  23. 1 2 3 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
  24. 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.
  25. 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
  26. 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
  27. 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
  28. 1 2 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
  29. 1 2 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
  30. 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
  31. 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
  32. 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
  33. 1 2 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.
  34. 1 2 3 4 5 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
  35. Hinkley, S.; et al. (2023), "Direct discovery of the inner exoplanet in the HD 206893 system", Astronomy & Astrophysics, 671: L5, arXiv: 2208.04867 , Bibcode:2023A&A...671L...5H, doi:10.1051/0004-6361/202244727, S2CID   251442869
  36. 1 2 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
  37. 1 2 3 4 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
  38. 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
  39. 1 2 3 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
  40. 1 2 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 , Bibcode:2022MNRAS.511.5207E, doi: 10.1093/mnras/stac357
  41. 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
  42. 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.
  43. "Kepler-1708". NASA Exoplanet Archive . Retrieved 13 January 2022.
  44. 1 2 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
  45. 1 2 3 4 5 6 7 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
  46. 1 2 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
  47. 1 2 3 4 5 6 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
  48. 1 2 3 4 5 6 7 8 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
  49. 1 2 3 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
  50. 1 2 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
  51. 1 2 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
  52. 1 2 3 4 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
  53. 1 2 3 4 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
  54. 1 2 3 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
  55. 1 2 3 4 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
  56. 1 2 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
  57. 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
  58. 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
  59. 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
  60. 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
  61. 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
  62. 1 2 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
  63. 1 2 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
  64. 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
  65. 1 2 3 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
  66. 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
  67. 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
  68. 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
  69. 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
  70. 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
  71. 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
  72. 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
  73. 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
  74. 1 2 3 4 5 6 7 8 9 10 11 12 13 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
  75. 1 2 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
  76. 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
  77. 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
  78. 1 2 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
  79. 1 2 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
  80. 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
  81. 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
  82. 1 2 3 4 5 6 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
  83. 1 2 3 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
  84. 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
  85. 1 2 3 4 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
  86. 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
  87. 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
  88. 1 2 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
  89. 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
  90. 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
  91. 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 .
  92. 1 2 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
  93. 1 2 3 4 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
  94. 1 2 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
  95. 1 2 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
  96. 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
  97. 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
  98. 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
  99. 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
  100. 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
  101. 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
  102. 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
  103. 1 2 3 4 5 6 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
  104. 1 2 3 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
  105. 1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 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
  106. 1 2 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
  107. 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
  108. 1 2 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
  109. 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
  110. 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
  111. 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
  112. 1 2 3 4 5 6 7 8 9 10 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
  113. 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
  114. 1 2 3 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
  115. 1 2 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
  116. 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
  117. 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
  118. 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
  119. 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
  120. 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
  121. "The Extrasolar Planet Encyclopaedia — TOI-5174 b". Extrasolar Planets Encyclopaedia . 3 December 1995. Retrieved 16 January 2023.
  122. "Exoplanet-catalog". Exoplanet Exploration: Planets Beyond our Solar System. Retrieved 16 January 2023.
  123. 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
  124. 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
  125. 1 2 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
  126. 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