List of exoplanets discovered in 2022

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.

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.


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
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[3]
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[3]
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[3]
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[4]
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[5][6]
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 [7]
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 [7]
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 [8]
TOI-4329b 0.45±0.09 1.50±0.19 2.9223±0.00015 transit 2258±16 1.538±0.049 6000±100 [8]
TOI-2669b 0.61±0.19 1.76±0.16 6.2034±0.0001 transit 1294±9 1.19±0.16 4800±100 [8]
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		 [9]
OGLE-2016-BLG-1093Lb 0.71±0.12 2.13±0.33 microlensing 26000±2000 0.46±0.08 [10]
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 [11]
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 [11]
Kepler-1972 b 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[12]
Kepler-1972 c 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[12]
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 [13]
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 [13]
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 [13]
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 [13]
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 [13]
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 [13]
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 [13]
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 [13]
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 [13]
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 [13]
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 [13]
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 [13]
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 [13]
Gliese 3929 b 0.0038±0.0013 0.103±0.004 2.6162745±0.000003 0.02569±0.00088 568.8+9.4
−9.3		 transit 51.64±0.02 0.309±0.014 3369±51 Another planet in system is suspected[14]
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 [15][16]
Kepler-451 c 1.61±0.14 1460±90 2.1±0.2 timing 1340±20 0.48+0.12 [17]
Kepler-451 d 1.76±0.18 43.0±0.1 0.20±0.03 timing 1340±20 0.48+0.12 [17]
KMT-2021-BLG-1391b 0.0143±0.0073 2.29+0.56
−0.71		 microlensing 19000+3000
−5000		 0.37±0.19 [18]
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		 [18]
KMT-2021-BLG-1372b 0.1928±0.1129 2.37±0.77 microlensing 19000+5000
−8000		 0.42±0.25 [18]
KMT-2021-BLG-0748b 0.45+0.40
−0.25		 2.43±0.67 microlensing 20000+3000
−4000		 0.36+0.32
−0.20		 [18]
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 [19]
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 [20]
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 [21][22]
PSR J2007+3120 b 0.0072±0.0009 723±8 timing 22000 Pulsar planet, another planet in the system is suspected.[23]
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 [24]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
K2-384 b 0.0040±0.0026 0.096+0.020
−0.005		 2.23152+0.0019
−0.00032		 600 transit 0.330±0.009 3623±138 [25]
K2-384 c 0.0054±0.0027 0.106+0.004
−0.006		 4.19476+0.00030
−0.00018		 480 transit 0.330±0.009 3623±138 [25]
K2-384 d 0.0085±0.0044 0.124+0.010
−0.006		 6.67958+0.00071
−0.00049		 410 transit 0.330±0.009 3623±138 [25]
K2-384 e 0.0075±0.0042 0.120+0.012
−0.007		 9.71504+0.00100
−0.00073		 370 transit 0.330±0.009 3623±138 [25]
K2-384 f 0.0179±0.0104 0.198+0.008
−0.007		 13.62749+0.00034
−0.00057		 330 transit 0.330±0.009 3623±138 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
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 [25]
K2-407 b 0.0066±0.0035 0.114+0.008
−0.007		 4.9419+0.00066
−0.00069		 1110 transit [25]
K2-407 c 0.0078±0.0044 0.121+0.008
−0.007		 9.22453+0.00132
−0.00091		 900 transit [25]
K2-408 b 0.0122±0.0062 0.149+0.010
−0.009		 20.97895+0.00130
−0.00124		 610 transit [25]
K2-409 b 0.0212±0.0127 0.221+0.015
−0.014		 1.90808+0.00004
−0.00005		 1800 transit [25]
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 [25]
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 [26][27]
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 [28]
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 [28]
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 [29]
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 [30]
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		 [31]
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		 [31]
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]
KMT-20109-BLG-1042Lb 0.19+0.21
−0.11		 1.7±0.5 microlensing 22000+3000
−5000		 0.30+0.34
−0.18		 [32]
KMT-20109-BLG-1552Lb 4.05+1.73
−1.85		 2.6+0.6
−0.8		 microlensing 15000+6000
−5000		 0.79+0.33
−0.36		 [32]
KMT-20109-BLG-2974Lb 0.28+0.29
−0.18		 2.0+0.8
−0.7		 microlensing 20000+5000
−7000		 0.47+0.41
−0.28		 [32]
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		 [33]
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		 [34]
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		 [35]
KMT-2018-BLG-2004b 0.27±\0.12 4.62+0.80
−1.10		 microlensing 23000+3000
−4000		 0.69+0.32
−0.31		 [35]
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		 [35]
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[35]
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[35]
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		 [35]
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		 [35]
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		 [35]
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[36]
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[37]
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[38]
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 [39]
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[40]
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[40]

Specific exoplanet lists

References
  1. Specht, D.; et al. (31 March 2022). "Kepler K2 Campaign 9: II. First space-based discovery of an exoplanet using microlensing". arxiv. Retrieved 4 April 2022.
  2. Starr, Michelle (4 April 2022). "The Most Distant Exoplanet Ever Found by Kepler Is... Surprisingly Familiar". ScienceAlert. Retrieved 4 April 2022.
  3. Ottoni, G.; Udry, S.; Ségransan, D.; et al. (22 December 2021). "CORALIE radial-velocity search for companions around evolved stars (CASCADES). I. Sample definition and first results: Three new planets orbiting giant stars". Astronomy & Astrophysics. EDP Sciences. arXiv:2201.01528. doi:10.1051/0004-6361/202040078. ISSN 0004-6361. S2CID 245440163.
  4. 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. EDP Sciences. arXiv:2201.01553. doi:10.1051/0004-6361/202040080. ISSN 0004-6361. S2CID 242974999.
  5. 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. Retrieved 13 January 2022.
  6. "Kepler-1708". NASA Exoplanet Archive. Retrieved 13 January 2022.
  7. A pair of Sub-Neptunes transiting the bright K-dwarf TOI-1064 characterised with CHEOPS, 2022, arXiv:2201.03570
  8. TESS Giants Transiting Giants II: The hottest Jupiters orbiting evolved stars, 2022, arXiv:2201.04140
  9. The TESS-Keck Survey. VIII. Confirmation of a Transiting Giant Planet on an Eccentric 261 day Orbit with the Automated Planet Finder Telescope, 2022, arXiv:2201.04146
  10. OGLE-2016-BLG-1093Lb: A Sub-Jupiter-mass Spitzer Planet Located in Galactic Bulge, 2022, arXiv:2201.04312
  11. Two gas giants transiting M dwarfs confirmed with HPF and NEID, 2022, arXiv:2201.09963
  12. Alleviating the Transit Timing Variations bias in transit surveys. II. RIVERS: Twin resonant Earth-sized planets around Kepler-1972 recovered from Kepler's false positive, 2022, arXiv:2201.11459
  13. Validation of 13 Hot and Potentially Terrestrial TESS Planets, 2022, arXiv:2201.12661
  14. Discovery and mass measurement of the hot, transiting, Earth-sized planet GJ 3929 b, 2022, arXiv:2202.00970
  15. A transiting, temperate mini-Neptune orbiting the M dwarf TOI-1759 unveiled by TESS, 2022, arXiv:2202.01240
  16. TOI-1759 b: a transiting sub-Neptune around a low mass star characterized with SPIRou and TESS, 2022, arXiv:2202.01259
  17. Detection of two additional circumbinary planets around Kepler-451, 2022, arXiv:2202.02118
  18. Mass Production of 2021 KMTNet Microlensing Planets I, 2022, arXiv:2202.03022
  19. A candidate short-period sub-Earth orbiting Proxima Centauri, 2022, arXiv:2202.05188
  20. TOI-1268b: the youngest hot Saturn-mass transiting exoplanet, 2022, arXiv:2201.13341
  21. TESS discovery of a sub-Neptune orbiting a mid-M dwarf TOI-2136, 2022, arXiv:2202.10024
  22. Validation and atmospheric exploration of the sub-Neptune TOI-2136b around a nearby M3 dwarf, 2022, arXiv:2202.10182
  23. A search for planetary companions around 800 pulsars from the Jodrell Bank pulsar timing programme, 2022, arXiv:2203.01136
  24. 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-d Orbit, 2022, arXiv:2203.01018
  25. Scaling K2. V. Statistical Validation of 60 New Exoplanets From K2 Campaigns 2-18, 2022, arXiv:2203.02087
  26. TOI-1696: a nearby M4 dwarf with a 3R⊕ planet in the Neptunian desert, 2022, arXiv:2203.02694
  27. TOI-1696 and TOI-2136: Constraining the Masses of Two Mini-Neptunes with HPF, 2022, arXiv:2204.09063
  28. TOI-1670 b and c: An Inner Sub-Neptune with an Outer Warm Jupiter Unlikely to have Originated from High-Eccentricity Migration, 2022, arXiv:2203.04334
  29. TOI-3757 b: A low density gas giant orbiting a solar-metallicity M dwarf, 2022, arXiv:2203.07178
  30. The CARMENES search for exoplanets around M dwarfs Two Saturn-mass planets orbiting active stars, 2022, arXiv:2203.16504
  31. KMT-2021-BLG-1077L: The fifth confirmed multiplanetary system detected by microlensing, 2022, arXiv:2203.16734
  32. Systematic KMTNet Planetary Anomaly Search. IV. Complete Statistical Sample of 2019 Prime-Field Microlensing Planets, 2022, arXiv:2204.02017
  33. A close-in puffy Neptune with hidden friends: The enigma of TOI 620, 2022, arXiv:2204.03108
  34. MOA-2020-BLG-135Lb: A New Neptune-class Planet for the Extended MOA-II Exoplanet Microlens Statistical Analysis, 2022, arXiv:2204.03672
  35. Systematic KMTNet Planetary Anomaly Search. V. Complete Sample of 2018 Prime-Field, 2022, arXiv:2204.04354
  36. HD 83443c: A highly eccentric giant planet on a 22-year orbit, 2022, arXiv:2204.05711
  37. OGLE-2019-BLG-1470LABc: Another Microlensing Giant Planet in a Binary System, 2022, arXiv:2204.05606
  38. A quarter century of spectroscopic monitoring of the nearby M dwarf Gl 514 A super-Earth on an eccentric orbit moving in and out of the habitable zone, 2022, arXiv:2204.06376
  39. A warm super-Neptune around the G-dwarf star TOI-1710 revealed with TESS, SOPHIE and HARPS-N, 2022, arXiv:2204.08984
  40. The HD 260655 system: Two rocky worlds transiting a bright M dwarf at 10 pc, 2022, arXiv:2204.10261
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