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2020年发现的系外行星列表

维基百科,自由的百科全书

这是2020年发现的系外行星列表[1][2]

仅由径向速度发现的太阳系外行星,下列表格记载的质量为其下限

名称 质量(MJ 半径(RJ 轨道周期(天) 半长轴(AU) 温度K[3] 发现方式 距离(ly) 主星质量(M 主星温度(K) 注释
2MASS J1155-7919 b英语2MASS J1155-7919 b 10 582 影像 330 [4]年轻的超级木星,轨道宽广[5]
HD 38677 b 18.57+0.01
0.1462+0.0012
877 径向速度 202.2169+3.261564
1.21+0.03
6196+29
由DMPP(Dispersed Matter Planet Project)发现[6]
HD 38677 c 6.584+0.003
−0.002
0.0733+0.0006
−0.0007
1239 径向速度 202.2169+3.261564
1.21+0.03
6196+29
由DMPP发现[6],与另一颗未确认行有2:1的轨道共振[7]
HD 38677 d 2.882+0.001
0.0422+0.0004
−0.0003
1632 径向速度 202.2169+3.261564
1.21+0.03
6196+29
由DMPP发现[6]
HD 38677 e 5.516+0.002
−0.004
0.0651+0.0005
1314 径向速度 202.2169+3.261564
1.21+0.03
6196+29
由DMPP发现[6]
HD 11231 b 0.426+0.038
−0.052
5.2072+0.0002
−0.0055
0.0664+0.0005
1000 径向速度 437.0495+13.04625
1.44+0.03
6500+100
由DMPP发现[6]
HD 42936 Ab英语HD 42936 2.58+0.35
−0.58
6.6732+0.0011
−0.0003
0.0662+0.0013
854 径向速度 159.4905+1.956938
0.87+0.05
5138+99
由DMPP发现[6]
EPIC 249893012 b日语EPIC 249893012 b 0.02753+0.00343
0.174+0.008
3.5951+0.0003
0.047+0.005
−0.007
1616+150
−80
凌日 1059.03+13.69857
1.05+0.05
5430+85
[8]
EPIC 249893012 c日语EPIC 249893012 c 0.04616+0.00595
0.3274+0.0152
−0.0125
15.624+0.001
0.13+0.01
−0.02
990+68
−29
凌日 1059.03+13.69857
1.05+0.05
5430+85
[8]
EPIC 249893012 d日语EPIC 249893012 d 0.03203+0.00774
−0.00761
0.3515+0.0116
35.747+0.005
0.22+0.02
−0.04
752+69
−37
凌日 1059.03+13.69857
1.05+0.05
5430+85
[8][9]
G 9-40 b英语G 9-40 b 0.1807 5.746007 0.0385 456 凌日 91.1 0.290 3348 [10]
Gliese 180 d 7.56+1.07
106.341+0.261
−0.34
0.31+0.024
−0.029
径向速度 39.96+0.01
0.43 3371 [11]
Gliese 229 Ac 0.025 122.005+0.364
−0.382
0.339+0.024
−0.029
径向速度 18.78+0.004
0.58 3564 [12][13]
Gliese 251 b >0.013 14.238 0.0818 351 径向速度 18.205+0.006
0.360+0.015
3451+51
2019年被否认,2020年被重新确认[14][15]
Gliese 433 d 0.019 36.052+0.045
−0.031
0.178+0.013
−0.015
径向速度 29.57+0.01
0.48 3600 [16][17]
Gliese 1061 b 0.00431+0.00050
−0.00047
3.204+0.001
0.021+0.001
径向速度 11.98+0.003
0.12+0.01
2953+98
[18]
Gliese 1061 c 0.00547+0.00072
6.689+0.005
0.035+0.001
径向速度 11.98+0.003
0.12+0.01
2953+98
[19]
Gliese 1061 d 0.00516+0.00076
−0.00072
13.031+0.025
−0.032
0.054+0.001
径向速度 11.98+0.003
0.12+0.01
2953+98
[20]
Gliese 1252 b 0.00658+0.00176
0.1064+0.0066
0.5182349+0.0000063
−0.0000050
0.00916+0.00076
1089+69
凌日 66.49+0.06
0.381+0.019
3458+140
−133
[21]
GJ 3082 b日语GJ 3082 b 0.02759+0.011
−0.01334
11.949+0.022
0.079+0.006
−0.007
径向速度 54.2 0.47 [22]
HATS-47b 0.369 1.117 3.9228 852.9 凌日 984.01+6.20
0.674 [23]
HATS-48Ab 0.243 0.800 3.1317 0.03769+0.00011
954.6 凌日 865 0.7279 4546.0+23
−18
[23][24]
HATS-49b 0.353 0.765 4.1480 834.8 凌日 1058.70+7.18
0.7133 [23]
HATS-72b 0.1254 0.7224 7.3279 739.3 凌日 416.37+1.70
0.7311 [23]
HD 80653 b 0.0176+0.0014
0.1439+0.0063
0.719573+0.000021
0.0166+0.0003
凌日 358.1197+2.641867
1.18+0.04
[25]
HIP 65 Ab日语HIP 65 Ab 3.213+0.078
2.03+0.61
−0.49
0.9809761+0.000037
−0.000034
0.01782+0.00021
1411+15
凌日 201.85818+0.2609251
0.781+0.027
4590+49
周期很短,围绕明亮的K4型星(V=11.1 mag)运动[26][27][28]
KELT-2019-BLG-1953 b 0.59+0.71
−0.32
0.8+0.9
−0.6
微重力透镜 23000+3600
−4300
0.31+0.37
−0.17
[29][30]
KELT-2019-BLG-1953 c 0.28+0.35
−0.15
0.8+0.9
−0.7
微重力透镜 23000+3600
−4300
0.31+0.37
−0.17
[31][30]
开普勒-1661(AB) b 0.053+0.038
0.345+0.005
175.06+0.06
0.633+0.005
243 凌日 1355.26+9.56
0.841+0.022
5100+100
[32][33]
L 168-9b日语ルイテン168-9 b 0.0145+0.00176
0.124+0.008
1.4015+0.00018
0.02091+0.00024
816+160
凌日 82.02833+0.07827753
0.62+0.03
3800+70
[34]
OGLE-2018-BLG-0677Lb日语OGLE-2018-BLG-0677Lb 0.0125+0.0185
−0.0084
0.68+0.27
−0.22
微重力透镜 27000+3500
0.12+0.14
−0.08
在银河系核球[35]
TOI-132 b 0.07048+0.00598
−0.00604
0.305+0.012
2.1097019+0.000012
−0.000011
0.026+0.002
−0.003
1395+52
−72
凌日 536.43+89.11
0.970+0.06
5397+46
[36]
TOI-257 b日语TOI-257 b 0.134+0.023
0.626+0.013
18.38827+0.00072
0.1523+0.0017
1033+19
凌日 251.37+0.065
1.38+0.056
−0.009
6075+90
主星又名HD 19916[37][38][39]
TOI-700 b英语TOI-700 0.00406+0.003
−0.00116
0.0901+0.00839
−0.00776
9.97701+0.00024
−0.00028
0.0637+0.0064
−0.006
凌日 101.5 0.416+0.01
3480+135
[40]
TOI-700 c英语TOI-700 0.0249+0.0085
−0.0057
0.2346+0.0214
−0.0205
16.051998+0.000089
−0.000092
0.0925+0.0088
−0.0083
凌日 101.5 0.416+0.01
3480+135
[40]
TOI-700 d英语TOI-700 d 0.00711+0.0022
−0.00164
0.1062+0.0098
37.426+0.0007
−0.001
0.163+0.015
295+55
凌日 101.5 0.416+0.01
3480+135
TESS发现的第一个地球大小的系外行星[40][41]
TOI-732 b英语TOI 732 0.098 0.119 0.7683881 0.012 892 凌日 72 0.379 3360 围绕双星系统LDS 3977的主星运动[42][43]
TOI-732 c 0.027 0.205 12.25 0.07673 323 凌日 72 0.379 3360 围绕双星系统LDS 3977的主星运动[42][43]
TOI-813 b 0.599+0.034
83.8911+0.0027
−0.0031
0.423+0.031
−0.037
610+28
−21
凌日 864.8192+5.156379
1.32+0.06
5907+150
[44]
TOI-1338 b英语TOI 1338 0.1038 0.611 95.2 0.4607 724 凌日 1301 TESS发现的第一个环联星运转行星[45][46]
HD 191939 b英语HD 191939 0.301 8.880411 0.089 778+58
−41
凌日 175 0.92 5400 主星又名TOI-1339[47]
HD 191939 c英语HD 191939 0.287 28.58060 0.178 550+45
凌日 175 0.92 5400 主星又名TOI-1339[47]
HD 191939 d英语HD 191939 0.282 38.3561 0.216 499+12
−11
凌日 175 0.92 5400 主星又名TOI-1339[47]
USco1621 b 16 2880 2270 影像 450 0.36 3460 [48]
USco1556 b 15 3500 2240 影像 459 0.33 3410 [48]
XO-7b 0.709 1.373 2.8641424 0.04421 1743 凌日 763 1.405 6250 [49]
LHS 1815 b日语LHS 1815 b 0.0132+0.0047
0.0971+0.005
3.81433+0.00003
0.0404+0.0094
617+84
凌日 97 0.502 3643+142
[50][51]
TOI-157 b日语TOI-157 b 1.18+0.13
1.29+0.02
2.0845435+0.0000023
0.03138+0.00025
−0.00020
1588+21
−20
凌日 1171 0.948+0.023
−0.018
5404+70
−67
[26]
TOI-169 b日语TOI-169 b 0.791+0.064
−0.06
1.086+0.081
−0.048
2.2554477+0.0000063
0.03524+0.00069
−0.00079
1715+22
−20
凌日 1345 1.147+0.069
−0.075
5880+54
−49
[26]
TOI-849 b 0.128+0.008
0.308+0.014
−0.011
0.7655240+0.0000027
0.01598+0.00013
1800 凌日 735 0.929+0.023
5329+48
海王星沙漠行星[52]
HD 95338 b 0.124+0.019
−0.013
0.355+0.008
−0.007
55.086+0.018
−0.019
0.231+0.005
−0.009
402+6
−9
凌日 120 0.76+0.16
−0.1
5212+16
−11
[53]
HD 332231 b 0.244+0.021
0.867+0.027
−0.025
18.71204+0.00043
0.1436+0.0032
−0.0033
876+17
凌日 262 1.127+0.077
6089+97
−96
TOI 1456[54]
TOI-1130 b 0.3256+0.009
4.066499+0.000046
0.04394+0.00035
−0.00038
876+17
凌日 190 0.684+0.16
−0.17
4250+67
[55][56]
TOI-1130 c 0.974+0.043
−0.044
1.5+0.27
−0.22
8.350381+0.000033
0.07098+0.00056
−0.0006
637+12
凌日 190 0.684+0.16
−0.17
4250+67
[55][57]
HD 79211 b 0.032+0.005
24.45+0.02
0.141+0.005
345 径向速度 20.658+0.005
0.64+0.07
4005+51
围绕双星系统 ADS 7251的主星运动[58]
WASP-150 b 8.46+0.28
−0.2
1.07+0.024
−0.025
5.644207+0.00003
−0.000004
0.0694+0.0011
−0.0008
1460+11
凌日 2422 1.394+0.07
−0.049
6218+49
−45
[59]
WASP-176 b 0.855+0.072
−0.069
1.505+0.05
−0.045
3.899052+0.00005
0.0535+0.001
−0.0019
1721+28
−21
凌日 1883 1.345+0.08
−0.13
5941+77
−79
[59]
TOI-1235 b 0.0217+0.00025
0.155+0.007
3.444729+0.000031
−0.000028
0.03845+0.00037
−0.0004
754+18
凌日 129 0.640+0.016
3872+70
该系统中可能还有多于一个的行星[60]
OGLE-2017-BLG-0406 b 0.41+0.05
3.5+0.3
微重力透镜 17000+1600
0.56+0.07
4848 有高精度微重力透镜事件[61]
TOI-421 b 0.051+0.004
−0.003
0.461+0.012
16.06815+0.00034
−0.00035
0.1182+0.0026
−0.0027
696.6+12.2
凌日 244.3+1.9
0.852+0.029
−0.021
5325+78
−58
星系中有一颗红矮星,距离主星2200天文单位[62]
TOI-421 c 0.0222+0.0022
0.243+0.017
5.19676+0.00049
−0.00048
0.0557+0.0012
−0.0013
1014.9+17.9
−17.6
凌日 244.3+1.9
0.852+0.029
−0.021
5325+78
−58
星系中有一颗红矮星,距离主星2200天文单位[62]
HD108236 b英语HD 108236 0.1415+0.0087
3.79523+0.00047
−0.00044
0.0469+0.0017
1099+19
−18
凌日 211 0.97 5730+50
[63]
HD108236 c英语HD 108236 0.1845+0.0089
−0.0081
6.2037+0.00064
−0.00052
0.0651+0.0024
932+17
−16
凌日 211 0.97 5730+50
[63]
HD108236 d英语HD 108236 0.2423+0.0097
14.1756+0.001
−0.0011
0.1131+0.004
708+13
−12
凌日 211 0.97 5730+50
[63]
HD108236 e英语HD 108236 0.279+0.012
−0.011
19.592+0.002
0.14+0.0052
636+12
−11
凌日 211 0.97 5730+50
[63]
WASP-148 b 0.291+0.025
0.722+0.055
8.80381+0.000043
0.22+0.063
940+80
凌日 809+5
1.00+0.08
5460+130
[64][65]
WASP-148 c 0.397+0.203
−0.044
34.515+0.029
0.359+0.086
590+50
径向速度 809+5
1.00+0.08
5460+130
[64][65]
NGTS-11 b 0.37+0.14
0.823+0.035
35.4553+0.0002
0.201+0.002
440+40
凌日 624+6
0.862+0.028
5050+80
[66]
HIP 67522 b日语HIP 67522 b 0.25 0.894+0.048
−0.047
6.9596+0.000016
−0.000015
1174+21
凌日 416+4
1.22+0.05
5675+75
可能是行星。非常年轻,形成不超过2000万年[67]
HD 63433 b俄语ru 0.017 +0.009
7.10801+0.00046
−0.00034
0.0710+0.0033
−0.0041
凌日 73.08+0.07
0.99+0.03
5640+74
[68]
HD 63433 c俄语V377 Близнецов#Планетная система 0.023 0.238+0.01
20.5455+0.001
0.1531+0.0074
−0.0092
凌日 73.08+0.07
0.99+0.03
5640+74
[68][69]
HD 164922 d 0.013+0.003
12.458+0.003
0.103+0.003
径向速度 72.1+0.9
0.874+0.012
5293+32
[70]
OGLE-2006-BLG-284 b 0.45+0.14
−0.40
2.2+0.8
微重力透镜 13000+4900
0.35+0.3
−0.2
轨道不确定[71]
Wendelstein-1b 0.59+0.17
−0.13
1.0314+0.00204
−0.021
2.663416+0.000001
0.0282+0.0009
1727+78
−90
凌日 1004+10
0.65+0.1
3984+152
−46
[72]
Wendelstein-2b 0.731+0.541
−0.311
1.1592+0.0061
1.7522239+0.0000008
0.0234+0.0015
1852+120
−140
凌日 1875+20
0.73+0.11
4288+133
−111
有气体包层[72]
开普勒-160d英语Kepler-160d 0.170+0.015
−0.012
378.417+0.028
−0.025
1.089+0.037
−0.073
244.8+2.1
−2.9
凌日 3140+60
0.88 5471+115
−37
[73]
K2-315b英语K2-315b 0.085+0.005
3.1443189+0.0000049
0.0234 460+5
凌日 185+1
0.174+0.004
3300+30
因其轨道周期长度,又名Pi Eeath或EPIC 249631677b[74]
TOI-1266 b 0.2193+0.074
−0.066
10.894879+0.00007
−0.00007
0.0745+0.0046
−0.0069
410+21
−15
凌日 117.4+1.0
0.437+0.021
3563+77
[75]
TOI-1266 c 0.1492+0.077
−0.095
18.80152+0.00054
−0.00067
0.1037+0.0026
−0.0025
347.1+7.9
−8
凌日 117.4+1.0
0.437+0.021
3563+77
[75]
AU Microscopii b 0.18 0.375 8.46321+0.00004
0.066 凌日 32.3+0.3
0.31 3500+100
[76][77][78]
TOI-1728 b日语TOI-1728 b 0.084+0.017
−0.016
0.450+0.014
3.491510+0.000062
−0.000057
0.0391+0.0009
767+8
凌日 198.2+0.5
0.646+0.023
−0.022
3980+31
−32
[79]
BD-11 4672 c英语BD-11 4672 0.048+0.009
74.2+0.06
−0.08
0.30+0.01
径向速度 88.63+0.11
0.651+0.031
−0.029
4550+110
处在宜居带内,轨道高度偏心[80]
OGLE-2018-BLG-1269Lb 0.69+0.44
−0.22
4383 4.61+1.70
−1.17
微重力透镜 8300+3000
−2000
0.35+0.3
−0.2
[81]
Lacaille 9352 b 0.0132+0.0019
9.262+0.001
0.068+0.002
468 径向速度 10.721+0.002
0.468+0.012
3688+86
[82]
Lacaille 9352 c英语Lacaille 9352 c 0.0234+0.0038
21.789+0.004
−0.005
0.120+0.004
352 径向速度 10.721+0.002
0.468+0.012
3688+86
[82]
HAT-P-58b 0.372+0.03
1.332+0.043
4.0138379+0.0000024
0.04994+0.00044
1622+18
凌日 1690+40
1.031+0.028
6078+48
[83]
HAT-P-59b 1.540+0.067
1.123+0.013
4.1419771+0.0000012
0.05064+0.00037
1278+7
凌日 871+4
1.008+0.022
5678+16
[83]
HAT-P-60b 0.574+0.038
1.631+0.024
4.7947813+0.0000024
0.06277+0.00017
1772+12
凌日 767+7
1.435+0.012
6212+26
[83]
HAT-P-61b 1.057+0.07
0.899+0.027
1.90231289+0.00000077
0.03010+0.00034
1505+16
凌日 1120+20
1.004+0.012
5587+45
[83]
HAT-P-62b 0.761+0.088
1.073+0.029
2.6453235+0.0000039
0.03772+0.00024
1512+13
凌日 1150+20
1.023+0.020
5629+48
[83]
HAT-P-63b 0.614+0.024
1.119+0.033
3.377728+0.000013
0.04294+0.00035
1237+11
凌日 1330+20
0.925+0.023
5400+55
−39
[83]
HAT-P-64b 0.58+0.18
−0.13
1.703+0.07
4.0072320+0.0000017
0.05387+0.00030
1766+22
−16
凌日 2135+20
1.298+0.021
6457+55
−36
[83]
TOI-1899 b 0.66+0.07
1.37+0.05
−0.06
29.02+0.36
−0.23
0.1587+0.067
−0.075
362+7
凌日 419+1
0.627+0.026
−0.028
3841+54
−45
[84]
HATS-37A b 0.099+0.042
0.606+0.016
4.3315 0.1587+0.067
−0.075
1085+16
−12
凌日 695 0.843+0.017
−0.012
5247+50
星系中还有一个红矮星[85]
HATS-38 b 0.074+0.011
0.614+0.0176
4.3750 0.1587+0.067
−0.075
1294+10
凌日 1131 0.890+0.016
−0.012
5740+50
[85]
TYC 8998-760-1 c 6+1
1.1+0.6
−0.3
320 1240+160
−170
影像 309.4+0.9
4783 [86]
HD 86226 c 0.023+0.004
0.193+0.007
3.98442+0.00018
0.049+0.001
1311+28
凌日 149 1.019+0.061
−0.066
5863+88
[87]
Gliese 2056 b 0.444+0.053
69.971+0.061
0.283+0.0013
径向速度 92.8 0.62+0.08
处于宜居带内[88]
Gliese 480 b 0.042+0.005
9.567+0.005
0.068+0.001
径向速度 46.4 0.45+0.02
[88]
Gliese 687 c 0.050+0.013
728+12
1.165+0.023
径向速度 14.83 0.40+0.02
该系统中发现的第二个海王星大小行星[88]
HIP 107772 b日语HIP 107772 b 0.049+0.014
−0.030
55.259+0.111
−0.311
0.243+0.022
−0.027
径向速度 77.1 0.63+0.08
处于宜居带内[88]
HIP 38594 b日语HIP 38594 b 0.026+0.012
−0.014
60.711+0.426
−0.192
0.256+0.006
−0.007
径向速度 58.0 0.61+0.02
处于宜居带内[88]
HIP 38594 c 0.135+0.077
−0.035
3525+541
−572
3.842+0.399
−0.441
径向速度 58.0 0.61+0.02
[88]
HIP 4845 b 0.053+0.016
−0.028
34.151+0.17
−0.09
0.177+0.016
−0.020
径向速度 68.8 0.62+0.04
[88]
HIP 48714 b 0.071+0.023
−0.020
17.819+0.004
−0.009
0.112+0.003
径向速度 34.3 0.58+0.02
[88]
TOI 824 b 0.058+0.006
0.261+0.018
−0.017
1.392978+0.000018
−0.000017
0.02177+0.00032
1253+38
−37
凌日 208 0.69+0.009
−0.007
4569+50
海王星沙漠行星[89]
Proxima Centauri c 0.0179+0.006
1928+20
1.489+0.049
39+16
−18
径向速度 4.244+0.001
0.1221+0.0022
3042+117
已知轨道第二近的行星[90][91]
TOI-763 b 0.031+0.002
0.203+0.010
5.6057+0.0013
0.0600+0.0006
1038+16
凌日 311 0.917+0.028
5444+110
[92]
TOI-763 c 0.029+0.003
0.235+0.011
12.2737+0.0053
−0.0077
0.1011+0.0010
800+12
凌日 311 0.917+0.028
5444+110
[92]
TOI-763 d 0.030+0.005
47.7991+2.7399
0.2504+0.0093
−0.0105
509+12
径向速度 311 0.917+0.028
5444+110
[92]
TOI-561 b 0.0050+0.0011
0.127+0.006
0.446578+0.000017
0.01055+0.00008
凌日 279.2+1.6
0.785+0.018
5455+65
−47
[93][94]
TOI-561 c 0.017+0.003
0.257+0.009
10.779+0.004
0.08809+0.0007
凌日 279.2+1.6
0.785+0.018
5455+65
−47
[93][94]
TOI-561 d 0.038+0.004
0.226+0.011
25.62+0.04
0.1569+0.0012
凌日 279.2+1.6
0.785+0.018
5455+65
−47
[93][94]
TOI-561 e 0.050+0.007
0.238+0.010
77.23+0.39
0.3274+0.0028
−0.0027
凌日 279.2+1.6
0.785+0.018
5455+65
−47
[93]
TOI-1266 b 0.042+0.035
−0.028
0.212+0.014
−0.011
10.894843+0.000067
−0.000066
0.0736+0.0016
−0.0017
413+20
凌日 117.5+0.1
0.48+0.1
3570+100
[95]
TOI-1266 c 0.007+0.006
−0.005
0.139+0.013
−0.012
18.80151+0.00067
−0.00069
0.1058+0.0023
−0.0024
344+16
凌日 117.5+0.1
0.48+0.1
3570+100
[95]
Gl 414 A b 0.029+0.010
−0.008
0.263+0.099
−0.081
50.817+0.031
−0.03
0.24+0.01
303.7+32.5
径向速度 38.8 0.650+0.08
4120+109
行星围绕双星系统的主星运动[96]
Gl 414 A c 0.177+0.033
−0.031
0.784+0.360
−0.238
748.3+1.3
−1.2
1.43+0.06
123.3+13.2
径向速度 38.8 0.650+0.08
4120+109
行星围绕双星系统的主星运动[96]
TOI 837 b <1.2 0.768+0.091
−0.072
8.3248762+0.0000157
凌日 466.5+1.2
1.118+0.059
6047+162
位于疏散星团 IC 2602[97]
TOI-776 b 0.0147+0.0031
0.163+0.010
8.24664+0.00009
−0.00006
0.0652+0.0011
513+12
凌日 88.6+0.1
0.544+0.028
3709+70
[98]
TOI-776 c 0.0192+0.0047
0.184+0.012
15.6653+0.0008
−0.0007
0.1000+0.0017
415+10
凌日 88.6+0.1
0.544+0.028
3709+70
[98]
MOA-2009-BLG-319Lb 0.2077+0.0255
2.03+0.21
微重力透镜 22800+2300
0.514+0.063
[99]
TOI-481 b 1.53+0.03
0.99+0.01
10.33111+0.00002
0.097+0.001
1370+10
凌日 587 1.14+0.02
−0.01
5735+72
[100]
TOI-892 b 0.95+0.07
1.07+0.02
10.62656+0.00007
0.092+0.005
1397+40
凌日 1120 1.28+0.03
−0.02
6261+80
[100]
GJ 3473 b 0.0059+0.0009
0.113+0.004
1.1980035+0.0000018
−0.0000019
0.01589+0.00062
773+16
−15
凌日 89.29+0.13
0.360+0.016
3347+54
又称TOI-488 b[101]
GJ 3473 c 0.0233+0.0029
−0.0027
15.509+0.033
0.0876+0.0035
−0.0034
329.1+6.6
−6.4
径向速度 89.29+0.13
0.360+0.016
3347+54
又称TOI-488 c[101]
NGTS-12b 0.208+0.022
1.048+0.032
7.532806+0.000048
0.0757+0.0014
1257+34
凌日 1474+25
1.021+0.056
−0.049
5690+130
[102]
OGLE-2016-BLG-1928 0.001 n/a 微重力透镜 30000 n/a n/a 星际行星[103]
LTT 9779 0.092+0.003
0.421+0.021
0.792054+0.000014
0.01679+0.0014
2000 凌日 262.8+1.0
1.02+0.02
−0.03
5499+50
海王星沙漠 行星[104]
TOI-540 b日语TOI-540 b 0.081+0.005
1.2391491+0.0000017
0.01223+0.00036
611+23
凌日 45.67+0.29
0.159+0.014
3216+83
[105]
HD 238090 b 0.0217+0.0029
−0.0030
13.671+0.011
−0.010
0.0932+0.0011
469.6+2.3
−2.6
径向速度 49.68+0.03
0.578+0.021
3933+51
在格利泽458双星系统中绕主星转动[15]
TIC 237913194b 1.942+0.092
−0.091
1.117+0.054
−0.047
15.168865+0.000018
0.1207+0.0037
974 凌日 1009+6
1.026+0.057
−0.055
5788+80
轨道十分偏心[106]
EPIC 201170410 b 0.09341 6.7987 0.0349 凌日 437+149
−130
0.287+0.101
−0.084
3648+172
−143
[107]
EPIC 201757695 b 0.08101 2.0478 0.0296 凌日 1880+110
0.727+0.044
−0.053
4520+108
−54
[107]
OGLE-2018-BLG-0799Lb英语OGLE-2018-BLG-0799Lb 0.22+0.19
−0.06
1.27+0.45
−0.29
微重力透镜 16000 0.08+0.08
−0.02
[108]
TOI-954 b 0.174+0.018
−0.017
0.852+0.053
−0.062
3.6849729+0.0000027
−0.0000028
0.04963+0.00089
−0.00090
1526+123
−164
凌日 768.5+8.3
1.201+0.066
−0.064
5710+53
−49
[109]
EPIC 246193072 b 0.260+0.020
−0.022
0.774+0.026
−0.024
12.4551225+0.0000031
0.1016+0.0018
−0.0019
650+53
−70
凌日 760+9
0.912+0.048
−0.049
5282+40
−39
[109]
WASP-186 b 4.22+0.18
1.11+0.03
5.026799+0.000012
−0.000014
0.0600+0.0012
−0.0013
1348+23
−22
凌日 913+11
1.22+0.07
−0.08
6361+105
−82
又称TOI-1494[110]
WASP-187 b 0.80+0.09
1.64+0.05
5.147878+0.000005
−0.000009
0.0653+0.0013
1726+31
−2
凌日 1224+21
1.54+0.09
6150+92
−85
又称TOI-1493[110]
TOI 122b 0.028+0.029
−0.010
0.243+0.016
5.078030+0.000015
0.0392+0.0007
471 凌日 202.9+0.7
0.312+0.007
3403+100
[111]
TOI 237b 0.009+0.006
−0.003
0.128+0.011
5.436098+0.000039
0.0341+0.0010
388 凌日 124.2+0.7
0.179+0.004
3212+100
[111]
HAT-P-68b 0.724+0.043
1.072+0.012
2.29840551+0.00000052
0.02996+0.00043
−0.00012
1027.8+8.2
凌日 662+3
0.6785+0.0299
−0.0079
4514+50
[112]
LP 714-47 b 0.097+0.005
0.420+0.027
4.052037+0.000004
0.0417+0.0005
700+19
−24
凌日 171.8+0.4
0.59+0.02
3950+51
主星又名G 160-62或TOI 442。海王星沙漠行星[113]
CFHTWIR-Oph 98 B 7.8+0.7
−0.8
1.86+0.04
200 1800+40
影像 447+13
0.015 2320+40
年轻的超级木星,围绕棕矮星运动。又名2MASS J16274422-2358521[114]
HD 190007 b英语HD 190007 0.052+0.005
11.72 径向速度 41.47+0.03
0.77+0.02
4610+20
[115]
HD 216520 b 0.032+0.003
35.45 径向速度 63.77+0.03
0.82+0.04
5103+20
[115]
HD 216520 c 0.030+0.005
154.43 径向速度 63.77+0.03
0.82+0.04
5103+20
[115]
TOI-519 b <14 0.75+0.21
1.2652328+0.0000005
0.012+0.004
760+54
凌日 378+3
0.369+0.026
−0.097
3350+100
−200
主星很暗,绝对星等为17[116]
TOI-260 b 0.009+0.013
−0.009
0.157+0.027
13.478048+0.005188
凌日 65.84+0.07
主星又称HIP 1532或BD-10 47[117]
TOI-784 b 0.031+0.004
0.171+0.015
2.797179+0.000158
凌日 211+0.4
主星又称HD 307842[117]
TOI-836 b 0.047+0.011
0.224+0.029
8.592004+0.002328
凌日 89.73+0.10
主星又称HIP 73427或CD-23 12010[117]
TOI-836 c 0.018+0.004
0.162+0.024
3.816514+0.000757
凌日 89.73+0.10
主星又称HIP 73427或CD-23 12010[117]
EPIC 201085153 b 0.214+0.089
0.25722+0.000039
凌日 3945+386
轨道短[118]
EPIC 201085153 c 0.125+0.179
−0.125
2.259797+0.0008
凌日 3945+386
[118]
EPIC 201427007 b 0.134+0.018
0.72091+0.000067
凌日 5633+111
[118]
EPIC 201595106 b 0.116+0.009
0.877214+0.000087
凌日 762+9
5820+20
2018年成为行星候选[118]
EPIC 201650711 c 0.036+0.007
5.544059+0.00016
凌日 298.8+1.7
4310+92
位于三元恒星系,行星b为确认[118]
EPIC 205152172 b 0.107+0.018
0.980088+0.000026
凌日 517+2
0.669+0.016
4202+242
2016年成为行星候选[118]
K2-299c 0.223+0.080
14.648966+0.000031
凌日 1219+16
5724+72
又名EPIC 206024342 p2[118]
K2-299d 0.152+0.054
4.507464+0.0000077
凌日 1219+16
5724+72
又名EPIC 206024342 p3[118]
K2-301c英语K2-301 0.152+0.018
5.2986+0.00035
凌日 1491+45
4114+99
又名EPIC 206042996 p2[118]
TOI-251b 0.245+0.016
4.937770+0.000028
−0.000029
0.05741+0.00023
−0.00017
凌日 324.4+1.4
1.036+0.013
−0.009
5875+100
−190
[119]
TOI-942b 0.429+0.018
4.324190+0.00003
0.04796+0.00073
−0.00065
凌日 498+2
0.788+0.037
−0.031
4928+125
−85
[119][120]主星为 TYC 5909-319-1
TOI-942c 0.517+0.017
−0.016
10.156430+0.000069
−0.000079
0.0847+0.0012
−0.0011
凌日 498+2
0.788+0.037
−0.031
4928+125
−85
[119][120]主星为 TYC 5909-319-1
K2-302c 0.089+0.009
2.255438+0.000037
凌日 359.3+3.5
3297+73
又名EPIC 206215704 p2[118]
K2-302d 0.098+0.009
2.909216+0.000032
凌日 359.3+3.5
3297+73
又名EPIC 206215704 p3[118]
EPIC 206298289 b 0.078+0.009
0.434847+0.000022
凌日 492+6
3875+157
2016年成为行星候选[118]
K2-85 b 0.107+0.009
0.684559+0.000026
凌日 317.8+1.2
4427+48
又名EPIC 210707130 p1[118]
EPIC 210801536 b 0.088+0.027
0.892592+0.00012
凌日 5304+259
2019年成为行星候选。该星系里可能还有一个行星[118]
EPIC 212624936 b 0.517+0.098
−0.027
0.578657+0.000066
凌日 5765+170
[118]主星为 TYC 5557-667-1
EPIC 212624936 c 0.214+0.098
−0.057
11.811437+0.00016
凌日 5765+170
[118]主星为 TYC 5557-667-1
K2-211c 0.116+0.018
2.601404+0.000072
凌日 895+14
0.882+0.019
−0.027
5360+51
[118]
EPIC 220440058 b 0.125+0.036
0.626683+0.00005
凌日 3682+217
该星系里可能还有一个行星[118]
EPIC 220492298 b 0.085+0.018
0.762406+0.00014
凌日 5620+31
[118]
K2-282d 0.232+0.027
27.248322+0.00047
凌日 1638.22+25.34
0.94+0.04
5499+109
[118]
EPIC 228836835 b 0.089+0.027
0.728113+0.00004
凌日 491+6
3782+152
[118]
K2-106c 0.188+0.018
13.334621+0.000068
凌日 803+10
5613+39
2017年成为行星候选[118]
开普勒-1514c 0.1049+0.0051
−0.0039
10.514181+0.000039
0.0997+0.0018
1066+16
−14
凌日 1240 1.196+0.065
−0.063
6145+99
−80
[121]
OGLE-2017-BLG-1049Lb 5.53+3.62
−2.87
3.92+1.10
−1.32
微重力透镜 18500+3600
−4500
0.55+0.36
−0.29
[122]
AU Microscopii c <0.087 0.320+0.014
18.858991+0.000010
0.1101+0.0022
454+16
凌日 31.7 0.50+0.03
3700+100
[123]
HD 25723 b 2.51 456.78 1.49 径向速度 375 2.1+0.3
主星为巨星[124]
HD 25723 c 1.33 2369.84 4.35 径向速度 375 2.1+0.3
主星为巨星[124]
Chi Scorpii b英语17 Sco b 4.32+0.15
−0.12
573.4+2.0
1.45+0.02
径向速度 408 1.09+0.15
4157+11
主星为巨星[124]
HD 60292 b 6.5+1.0
495.4+3.0
1.5+0.1
径向速度 1036+10
1.7+0.2
4348+28
主星为巨星[125]
HD 112640 b 5.0+1.0
613.2+5.8
1.7+0.1
径向速度 1065+6
1.8+0.2
4155+15
主星为巨星[125]
K2-111 c 0.0356+0.0035
15.6785+0.0064
−0.0063
0.1166+0.0025
径向速度 680+60
0.89+0.02
5730+50
[126]
K2-316b 0.119 1.133 0.0147 841 凌日 368 EPIC 249384674b[127]
K2-316c 0.163 5.260 0.0582 423 凌日 368 EPIC 249384674c[127]
K2-317b 0.261 6.220 0.0542 432 凌日 577 EPIC 249557502b[127]
K2-318b 0.148 7.010 0.0911 456 凌日 483 EPIC 249826231b[127]
K2-319b 0.249 26.680 0.1516 641 凌日 686 EPIC 201663879b[127]
K2-320b 0.234 1.995 0.0142 698 凌日 356 EPIC 201796690b[127]
K2-321b 0.174 2.298 0.0410 701 凌日 254 EPIC 248480671b[127]
K2-322b 0.171 8.205 0.0594 635 凌日 404 EPIC 248558190b[127]
K2-323b 0.187 24.930 0.1275 318 凌日 387 EPIC 248616368b[127]
K2-324b 0.217 3.262 0.0331 707 凌日 447 EPIC 248639308b[127]
K2-325b 0.196 6.930 0.0419 423 凌日 365 EPIC 246074965b[127]
K2-326b 0.203 1.256 0.0198 1114 凌日 928 EPIC 246472939b[127]
KMT-2016-BLG-2397b 2.42 2.83 微重力透镜 16000 0.62+0.29
−0.30
这个行星有多种可能的情况[128]
KMT-2016-BLG-2364b 3.93 2.63 微重力透镜 21000 0.50+0.40
−0.22
[128]
OGLE-2017-BLG-1375b 10.33 2.97 微重力透镜 12000 0.77+0.27
−0.23
这个行星有多种可能的情况[128]
OGLE-2017-BLG-0604b 0.51 4.06 微重力透镜 13000 0.70+0.28
[128]
KMT-2018-BLG-0748Lb 0.18+0.29
−0.10
0.62+0.09
微重力透镜 24000 0.0870+0.138
−0.047
[129]
KMT-2019-BLG-1339Lb 12.2+16.1
−6.7
0.67+0.77
−0.55
微重力透镜 23000+3000
0.27+0.366
−0.15
这个行星有多种可能的情况[130]
KMT-2019-BLG-2073日语KMT-2019-BLG-2073 0.19 微重力透镜 12000 [131]
OGLE-2019-BLG-0551 0.0242 微重力透镜 [132]
TVLM 513-46546 b 0.38+0.24
221+5
0.3+0.0036
天体测量 34.90+0.07
0.09 2500 [133]
CD Ceti西班牙语CD Ceti 0.0124+0.0013
−0.0014
2.29070+0.00012
0.0185+0.0013
−0.0013
464+18
径向速度 28.07 0.161+0.010
3130+51
[134]
OGLE-2018-BLG-0799Lb英语OGLE-2018-BLG-0799Lb 0.22+0.19
−0.06
1.27+0.45
−0.29
微重力透镜 16000 0.08+0.08
−0.02
[135]
WD 1856+534 b 13.8 0.93+0.09
1.4079405+0.0000011
0.0204+0.0012
凌日 80.737+0.144
0.518+0.055
4710+60
围绕白矮星运动[136]
开普勒-1649c英语Kepler-1649c 0.0038 0.095+0.014
−0.010
19.53527+0.00010
0.0649 234+20
凌日 301.6+1.6
0.1977+0.0051
3240+61
处于宜居带内,行星像地球[137]
Kepler-305e 0.160 3.20538 凌日 2900+90
[138]
Kepler-385d 0.233 56.4159 凌日 4870+160
[138]
Kepler-598c 0.270 86.4945 凌日 2260+40
FPP=1.0%[138]
Kepler-647c 0.357 29.6663 凌日 3660+70
[138]
Kepler-716c 0.124 3.96999 凌日 2110+30
FPP=0.6%[138]
Kepler-783c 0.208 7.05395 凌日 1707+15
[138]
Kepler-1001c 0.140 9.18186 凌日 3110+80
[138]
Kepler-1085c 0.291 56.7771 凌日 4630+150
[138]
开普勒-1662b 0.223 0.790 134.4628 凌日 [139]主星又名KOI-1783[140]
开普勒-1663b 0.294 17.6046 凌日 1112+11
主星又名KOI-252[138]
开普勒-1664b 0.270 14.3868 凌日 主星又名KOI-349[138]
开普勒-1665b 0.253 11.9548 凌日 1104+5
主星又名KOI-650[138]
Kepler-1666b 0.257 25.8476 凌日 4680+190
主星又名KOI-945[138]
Kepler-1666c 0.257 25.8476 凌日 4680+190
主星又名KOI-945[138]
开普勒-1667b 0.266 83.5781 凌日 2080+20
主星又名KOI-1311[138]
开普勒-1668b 0.388 15.434 凌日 4500+200
主星又名KOI-1470[138]
开普勒-1669b 0.248 9.51216 凌日 1800+40
主星又名KOI-1475[138]
开普勒-1670b 0.299 20.4998 凌日 7200+400
主星又名KOI-1705[138]
开普勒-1671b 0.118 4.16787 凌日 1176+7
主星又名KOI-1738[138]
开普勒-1672b 0.265 150.878 凌日 1189+14
主星又名KOI-1822[138]
开普勒-1673b 0.262 33.7888 凌日 2420+20
主星又名KOI-1863[138]
开普勒-1674b 0.286 62.5611 凌日 3400+100
主星又名KOI-1892[138]
开普勒-1675b 0.279 63.0382 凌日 2163+19
主星又名KOI-1928[138]
开普勒-1676b 0.301 29.9221 凌日 主星又名KOI-1943[138]
开普勒-1677b 0.241 22.064 凌日 2250+30
主星又名KOI-1984, FPP=0.6%[138]
开普勒-1678b 0.295 147.974 凌日 2830+70
主星又名KOI-2066, FPP=0.5%[138]
开普勒-1679b 0.184 9.75376 凌日 3040+100
主星又名KOI-2106[138]
开普勒-1680b 0.121 8.77424 凌日 1020+5
主星又名KOI-2120[138]
开普勒-1681b 0.2227 69.8956 凌日 2100+300
主星又名KOI-2132[138]
开普勒-1682b 0.257 14.8334 凌日 3900+160
主星又名KOI-2229[138]
开普勒-1683b 0.167 15.0337 凌日 2440+50
主星又名KOI-2293[138]
开普勒-1684b 0.256 47.7055 凌日 2060+40
主星又名KOI-2417[138]
开普勒-1685b 0.230 20.4905 凌日 3840+150
主星又名KOI-2504[138]
开普勒-1686b 0.127 9.30987 凌日 2430+30
主星又名KOI-2559[138]
开普勒-1687b 0.147 5.77954 凌日 1375+17
主星又名KOI-2588[138]
开普勒-1688b 0.112 5.62012 凌日 1850+380
主星又名KOI-2733[138]
开普勒-1689b 0.084 8.483 凌日 967+5
主星又名KOI-2755[138]
开普勒-1690b 0.250 234.636 凌日 2340+30
主星又名KOI-2757[138]
开普勒-1691b 0.163 3.8482 凌日 4290+110
主星又名KOI-2802[138]
开普勒-1692b 0.099 5.95966 凌日 1960+20
主星又名KOI-2849[138]
开普勒-1693b 0.115 12.0999 凌日 2530+50
主星又名KOI-2871[138]
开普勒-1694b 0.105 3.89526 凌日 1698+16
主星又名KOI-2878, FPP=0.6%[138]
开普勒-1695b 0.099 4.7329 凌日 2640+40
主星又名KOI-3048, FPP=0.5%[138]
开普勒-1696b 0.250 65.9409 凌日 5100+200
主星又名KOI-3361[138]
开普勒-1697b 0.112 33.4969 凌日 813+2
主星又名KOI-3478[138]
开普勒-1698b 0.095 1.2107 凌日 729+3
主星又名KOI-3864[138]
开普勒-1699b 0.139 3.49082 凌日 主星又名KOI-3933[138]
Kepler-1701b 0.198 169.134 凌日 1940+20
主星又名KOI-4054,[138] 可能宜居的系外行星
开普勒-1702b英语Kepler-1702b 0.143 18.5012 凌日 2860+90
主星又名KOI-4386[138]


参考

[编辑]
  1. ^ NASA Exoplanet Archive. [20 December 2019]. (原始内容存档于2021-03-22). 
  2. ^ Extrasolar Planet's Catalogue (sic). Kyoto University. [20 December 2019]. (原始内容存档于2022-04-06). 
  3. ^ The Extrasolar Planets Encyclopaedia. [2015-11-09]. (原始内容存档于2012-07-05). 
  4. ^ exoplanet.eu Planet 2MASS J1155-7919 b. [2021-08-24]. (原始内容存档于2021-11-28). 
  5. ^ www.sci-news.com Astronomers Discover Nearest-Known Newborn Gas Giant. [2021-08-24]. (原始内容存档于2020-03-03). 
  6. ^ 6.0 6.1 6.2 6.3 6.4 6.5 Haswell, Carole A.; et al. Dispersed Matter Planet Project discoveries of ablating planets orbiting nearby bright stars. Nature Astronomy. 2019, 4 (4): 408–418. Bibcode:2020NatAs...4..408H. S2CID 209444484. arXiv:1912.10874可免费查阅. doi:10.1038/s41550-019-0973-y. 
  7. ^ Jones, Mark H.; Haswell, Carole A.; Barnes, John R.; Staab, Daniel; Heller, René. A possible transit of a disintegrating exoplanet in the nearby multiplanet system DMPP-1. The Astrophysical Journal. 2020, 895 (1): L17. Bibcode:2020ApJ...895L..17J. S2CID 218630238. arXiv:2005.07086可免费查阅. doi:10.3847/2041-8213/ab8f2b. 
  8. ^ 8.0 8.1 8.2 Hidalgo, D.; Pallé, E.; Alonso, R.; Gandolfi, D.; Fridlund, M.; Nowak, G.; Luque, R.; Hirano, T.; Justesen, A. B.; Cochran, W. D.; Barragán, O.; Spina, L.; Rodler, F.; Albrecht, S.; Anderson, D.; Amado, P.; Bryant, E.; Caballero, J. A.; Cabrera, J.; Csizmadia, Sz.; Dai, F.; De Leon, J.; Deeg, H. J.; Eigmuller, Ph.; Endl, M.; Erikson, A.; Esposito, M.; Figueira, P.; Georgieva, I.; et al, Three planets transiting the evolved star EPIC 249893012: a hot 8.8-M⊕ super-Earth and two warm 14.7 and 10.2-M⊕ sub-Neptunes, Astronomy & Astrophysics, 2020, 636: A89, Bibcode:2020A&A...636A..89H, S2CID 211032193, arXiv:2002.01755v1可免费查阅, doi:10.1051/0004-6361/201937080 
  9. ^ exoplanet.eu Planet EPIC 249893012 d. [2021-08-24]. (原始内容存档于2021-07-27). 
  10. ^ G 9-40 b. [2021-08-24]. (原始内容存档于2021-07-26). 
  11. ^ GJ 180 d. [2021-08-24]. (原始内容存档于2021-07-26). 
  12. ^ GJ 229 A c. [2021-08-24]. (原始内容存档于2021-07-26). 
  13. ^ Feng, Fabo; Butler, R. Paul; Shectman, Stephen A.; Crane, Jeffrey D.; Vogt, Steve; Chambers, John; Jones, Hugh R. A.; Wang, Sharon Xuesong; Teske, Johanna K.; Burt, Jenn; Díaz, Matías R.; Thompson, Ian B. Search for Nearby Earth Analogs. II. Detection of Five New Planets, Eight Planet Candidates, and Confirmation of Three Planets around Nine Nearby M Dwarfs. The Astrophysical Journal Supplement Series. 2020, 246 (1): 11. Bibcode:2020ApJS..246...11F. S2CID 210064560. arXiv:2001.02577可免费查阅. doi:10.3847/1538-4365/ab5e7c. 
  14. ^ Barnes, J. R.; et al. Frequency of planets orbiting M dwarfs in the Solar neighbourhood. 2019-06-11. arXiv:1906.04644可免费查阅 (英语). 
  15. ^ 15.0 15.1 The CARMENES search for exoplanets around M dwarfs Three temperate-to-warm super-Earths, 2020, arXiv:2010.00474可免费查阅 
  16. ^ www.sci-news.com Astronomers Discover Five New Planets around Nearby Red Dwarfs. [2021-08-24]. (原始内容存档于2021-07-26). 
  17. ^ GJ 433 d. [2021-08-24]. (原始内容存档于2021-07-26). 
  18. ^ GJ 1061 b. [2021-08-24]. (原始内容存档于2021-07-26). 
  19. ^ GJ 1061 c. [2021-08-24]. (原始内容存档于2021-07-26). 
  20. ^ GJ 1061 d. [2021-08-24]. (原始内容存档于2020-10-14). 
  21. ^ GJ 1252 b. [2021-08-24]. (原始内容存档于2021-07-26). 
  22. ^ exoplanet.eu Planet GJ 3082 b. [2021-08-24]. (原始内容存档于2021-07-26). 
  23. ^ 23.0 23.1 23.2 23.3 Hartman, J. D.; et al. HATS-47b, HATS-48Ab, HATS-49b and HATS-72b: Four Warm Giant Planets Transiting K Dwarfs. The Astronomical Journal. 2020, 159 (4): 173. Bibcode:2020AJ....159..173H. S2CID 211126666. arXiv:2002.05776可免费查阅. doi:10.3847/1538-3881/ab7821. 
  24. ^ exoplanet.eu hats-48a b. [2021-08-24]. (原始内容存档于2022-03-18). 
  25. ^ exoplanet.eu HD 80653 b. [2021-08-24]. (原始内容存档于2021-07-26). 
  26. ^ 26.0 26.1 26.2 Nielsen, L.; et al. Three Short Period Jupiters from TESS. Astronomy & Astrophysics. 2020, 639: A76. S2CID 212675311. arXiv:2003.05932可免费查阅. doi:10.1051/0004-6361/202037941. 
  27. ^ exoplanet.eu HIP 65A b. [2021-08-24]. (原始内容存档于2021-07-26). 
  28. ^ Wong, Ian; et al. Systematic Phase Curve Study of Known Transiting Systems from Year 1 of the TESS Mission. 2020. arXiv:2003.06407可免费查阅 [astro-ph.EP]. 
  29. ^ exoplanet.eu Planet KELT-2019-BLG-1953 b. [2021-08-24]. (原始内容存档于2020-02-17). 
  30. ^ 30.0 30.1 Han, Cheongho; et al. One Planet or Two Planets? The Ultra-sensitive Extreme-magnification Microlensing Event KMT-2019-BLG-1953. The Astronomical Journal. 2020, 160 (1): 17. Bibcode:2020AJ....160...17H. S2CID 211096807. arXiv:2002.05310可免费查阅. doi:10.3847/1538-3881/ab91ac. 
  31. ^ exoplanet.eu Planet KELT-2019-BLG-1953 c. [2021-08-24]. (原始内容存档于2020-02-17). 
  32. ^ Kepler-1661 b. [2021-08-24]. (原始内容存档于2021-07-26). 
  33. ^ Socia, Quentin J.; et al. Kepler-1661 b: A Neptune-sized Kepler Transiting Circumbinary Planet around a Grazing Eclipsing Binary. The Astronomical Journal. 2020, 159 (3): 94. Bibcode:2020AJ....159...94S. S2CID 210116655. arXiv:2001.02840可免费查阅. doi:10.3847/1538-3881/ab665b. 
  34. ^ exoplanet.eu L 168-9 b. [2021-08-24]. (原始内容存档于2021-07-27). 
  35. ^ Herrera-Martín, Antonio; et al. Ogle-2018-BLG-0677lb: A super earth near the galactic bulge. The Astronomical Journal. 2020, 159 (6): 256. Bibcode:2020AJ....159..256H. S2CID 212628627. arXiv:2003.02983可免费查阅. doi:10.3847/1538-3881/ab893e. 
  36. ^ TOI-132 b. [2021-08-24]. (原始内容存档于2021-07-26). 
  37. ^ exoplanet.eu toi-257_b. [2021-08-24]. (原始内容存档于2021-07-27). 
  38. ^ TOI-257b (HD 19916b): A Warm sub-Saturn on a Moderately Eccentric Orbit Around an Evolved F-type Star, 2020, arXiv:2001.07345可免费查阅 
  39. ^ TIDAL INFLATION RECONCILES LOW-DENSITY SUB-SATURNS WITH CORE ACCRETION, 2020, arXiv:2005.11209可免费查阅 
  40. ^ 40.0 40.1 40.2 Gilbert, Emily A.; Barclay, Thomas; Schlieder, Joshua E.; Quintana, Elisa V.; Hord, Benjamin J.; Kostov, Veselin B.; Lopez, Eric D.; Rowe, Jason F.; Hoffman, Kelsey; Walkowicz, Lucianne M.; Silverstein, Michele L.; Rodriguez, Joseph E.; Vanderburg, Andrew; Suissa, Gabrielle; Airapetian, Vladimir S.; Clement, Matthew S.; Raymond, Sean N.; Mann, Andrew W.; Kruse, Ethan; Lissauer, Jack J.; Colón, Knicole D.; Ravi kumar Kopparapu; Kreidberg, Laura; Zieba, Sebastian; Collins, Karen A.; Quinn, Samuel N.; Howell, Steve B.; Ziegler, Carl; Eliot Halley Vrijmoet; et al. The First Habitable Zone Earth-sized Planet from TESS. I: Validation of the TOI-700 System. 2020. arXiv:2001.00952可免费查阅 [astro-ph.EP]. 
  41. ^ Suissa, Gabrielle; Wolf, Eric T.; Ravi kumar Kopparapu; Villanueva, Geronimo L.; Fauchez, Thomas; Mandell, Avi M.; Arney, Giada; Gilbert, Emily A.; Schlieder, Joshua E.; Barclay, Thomas; Quintana, Elisa V.; Lopez, Eric; Rodriguez, Joseph E.; Vanderburg, Andrew. The First Habitable Zone Earth-sized Planet from TESS. III: Climate States and Characterization Prospects for TOI-700 D. 2020. arXiv:2001.00955可免费查阅 [astro-ph.EP]. 
  42. ^ 42.0 42.1 Cloutier, Ryan; et al. A pair of TESS planets spanning the radius valley around the nearby mid-M dwarf LTT 3780. The Astronomical Journal. 2020, 160 (1): 3. Bibcode:2020AJ....160....3C. S2CID 211817805. arXiv:2003.01136可免费查阅. doi:10.3847/1538-3881/ab91c2. 
  43. ^ 43.0 43.1 Nowak, G.; et al. The CARMENES search for exoplanets around M dwarfs. Two planets on the opposite sides of the radius gap transiting the nearby M dwarf LP 729-54. 2020. arXiv:2003.01140可免费查阅 [astro-ph.EP]. 
  44. ^ exoplanet.eu toi-813_b. [2021-08-24]. (原始内容存档于2021-07-19). 
  45. ^ Kostov, Veselin B.; Orosz, Jerome A.; Feinstein, Adina D.; Welsh, William F.; Cukier, Wolf; Haghighipour, Nader; Quarles, Billy; Martin, David V.; Montet, Benjamin T.; Torres, Guillermo; Triaud, Amaury H. M. J.; Barclay, Thomas; Boyd, Patricia; Briceno, Cesar; Andrew Collier Cameron; Correia, Alexandre C. M.; Gilbert, Emily A.; Gill, Samuel; Gillon, Michael; Haqq-Misra, Jacob; Hellier, Coel; Dressing, Courtney; Fabrycky, Daniel C.; Furesz, Gabor; Jenkins, Jon; Kane, Stephen R.; Kopparapu, Ravi; Vedad Kunovac Hodzic; Latham, David W.; et al. TOI-1338: TESS' First Transiting Circumbinary Planet. The Astronomical Journal. 2020, 159 (6): 253. Bibcode:2020AJ....159..253K. S2CID 215785933. arXiv:2004.07783可免费查阅. doi:10.3847/1538-3881/ab8a48. 
  46. ^ Exoplanet-catalog - Exoplanet TOI-1338 b. [2021-08-24]. (原始内容存档于2021-08-08). 
  47. ^ 47.0 47.1 47.2 Badenas-Agusti, Mariona; et al. HD 191939: Three Sub-Neptunes Transiting a Sun-like Star Only 54 pc Away. 2020. arXiv:2002.03958可免费查阅 [astro-ph.EP]. 
  48. ^ 48.0 48.1 Chinchilla, Patricia; et al. USco1621 B and USco1556 B: Two wide companions at the deuterium-burning mass limit in Upper Scorpius. Astronomy & Astrophysics. 2020, 633: A152. Bibcode:2020A&A...633A.152C. S2CID 208910589. arXiv:1912.04150可免费查阅. doi:10.1051/0004-6361/201936130. 
  49. ^ Crouzet, Nicolas; et al. XO-7 b: A Transiting Hot Jupiter with a Massive Companion on a Wide Orbit. The Astronomical Journal. 2020, 159 (2): 44. Bibcode:2020AJ....159...44C. S2CID 208857410. arXiv:1912.02821可免费查阅. doi:10.3847/1538-3881/ab5b12. 
  50. ^ Gan, Tianjun; et al. LHS 1815b: The First Thick-Disk Planet Detected by TESS. The Astronomical Journal. 2020, 159 (4): 160. Bibcode:2020AJ....159..160G. S2CID 212644667. arXiv:2003.04525可免费查阅. doi:10.3847/1538-3881/ab775a. 
  51. ^ exoplanet.eu LHS 1815 b. [2021-08-24]. (原始内容存档于2021-07-26). 
  52. ^ Armstrong, David J.; et al. A remnant planetary core in the hot Neptunian desert. Nature. 2020, 583 (7814): 39–42. Bibcode:2020Natur.583...39A. PMID 32612222. S2CID 214612138. arXiv:2003.10314可免费查阅. doi:10.1038/s41586-020-2421-7. 
  53. ^ Díaz, Matías R.; et al. The Magellan/PFS Exoplanet Search: A 55-day period dense Neptune transiting the bright ($V=8.6$) star HD 95338. 2020. S2CID 214611611. arXiv:2003.10319可免费查阅. doi:10.1093/mnras/staa1724. 
  54. ^ Dalba, Paul A.; et al. The TESS-Keck Survey I: A Warm Sub-Saturn-Mass Planet and a Caution about Stray Light in TESS Cameras. The Astronomical Journal. 2020, 159 (5): 241. Bibcode:2020AJ....159..241D. S2CID 214623340. arXiv:2003.10451可免费查阅. doi:10.3847/1538-3881/ab84e3. 
  55. ^ 55.0 55.1 Huang, Chelsea X.; et al. TESS Spots a Hot Jupiter with an Inner Transiting Neptune. The Astrophysical Journal. 2020, 892 (1): L7. Bibcode:2020ApJ...892L...7H. S2CID 214623301. arXiv:2003.10852可免费查阅. doi:10.3847/2041-8213/ab7302. 
  56. ^ exoplanet.eu toi-1130 b. [2021-08-24]. (原始内容存档于2021-07-26). 
  57. ^ exoplanet.eu toi-1130 c. [2021-08-24]. (原始内容存档于2021-07-26). 
  58. ^ González-Álvarez, E.; Zapatero Osorio, M. R.; Caballero, J. A.; Sanz-Forcada, J.; Béjar, V. J. S.; González-Cuesta, L.; Dreizler, S.; Bauer, F. F.; Rodríguez, E.; Tal-Or, L.; Zechmeister, M.; Montes, D.; López-González, M. J.; Ribas, I.; Reiners, A.; Quirrenbach, A.; Amado, P. J.; Anglada-Escudé, G.; Azzaro, M.; Cortés-Contreras, M.; Hatzes, A. P.; Henning, T.; Jeffers, S. V.; Kaminski, A.; Kürster, M.; Lafarga, M.; Morales, J. C.; Pallé, E.; Perger, M.; Schmitt, J. H. M. M. The CARMENES search for exoplanets around M dwarfs. A super-Earth planet orbiting HD 79211 (GJ 338 B). Astronomy & Astrophysics. 2020, A93: 637. Bibcode:2020A&A...637A..93G. S2CID 214714124. arXiv:2003.13052可免费查阅. doi:10.1051/0004-6361/201937050. 
  59. ^ 59.0 59.1 Cooke, Benjamin F.; Pollacco, Don; Almleaky, Y.; Barkaoui, K.; Benkhaldoun, Z.; Blake, James A.; Bouchy, François; Boumis, Panos; Brown, D. J. A.; Bruni, Ivan; Burdanov, A.; Andrew Collier Cameron; Chote, Paul; Daassou, A.; D'ago, Giuseppe; Dalal, Shweta; Damasso, Mario; Delrez, L.; Doyle, A. P.; Ducrot, E.; Gillon, M.; Hébrard, G.; Hellier, C.; Henning, Thomas; Jehin, E.; Kiefer, Flavien; King, George W.; Liakos, Alexios; Lopez, Théo; et al. Two transiting hot Jupiters from the WASP survey: WASP-150b and WASP-176b. The Astronomical Journal. 2020, 159 (6): 255. Bibcode:2020AJ....159..255C. S2CID 215754471. arXiv:2004.06622可免费查阅. doi:10.3847/1538-3881/ab88db. 
  60. ^ Cloutier, Ryan; Rodriguez, Joseph E.; Irwin, Jonathan; Charbonneau, David; Stassun, Keivan G.; Mortier, Annelies; Latham, David W.; Isaacson, Howard; Howard, Andrew W.; Udry, Stéphane; Wilson, Thomas G.; Watson, Christopher A.; Pinamonti, Matteo; Lienhard, Florian; Giacobbe, Paolo; Guerra, Pere; Collins, Karen A.; Beiryla, Allyson; Esquerdo, Gilbert A.; Matthews, Elisabeth; Crossfield, Ian J. M.; Winters, Jennifer G.; Nava, Chantanelle; Ment, Kristo; Lopez, Eric D.; Ricker, George; Vanderspek, Roland; Seager, Sara; Jenkins, Jon M.; et al. TOI-1235 b: A keystone super-Earth for testing radius valley emergence models around early M dwarfs. The Astronomical Journal. 2020, 160 (1): 22. Bibcode:2020AJ....160...22C. S2CID 215754432. arXiv:2004.06682可免费查阅. doi:10.3847/1538-3881/ab9534. 
  61. ^ Hirao, Yuki; Bennett, David P.; Ryu, Yoon-Hyun; Koshimoto, Naoki; Udalski, Andrzej; Yee, Jennifer C.; Sumi, Takahiro; Bond, Ian A.; Shvartzvald, Yossi; Abe, Fumio; Barry, Richard K.; Bhattacharya, Aparna; Donachie, Martin; Fukui, Akihiko; Itow, Yoshitaka; Kondo, Iona; Man Cheung Alex Li; Matsubara, Yutaka; Matsuo, Taro; Miyazaki, Shota; Muraki, Yasushi; Nagakane, Masayuki; Onishi, Kohji; Ranc, Clement; Rattenbury, Nicholas J.; Suematsu, Haruno; Shibai, Hiroshi; Sullivan, Denis J.; Suzuki, Daisuke; et al. OGLE-2017-BLG-0406: ${\it Spitzer}$ Microlens Parallax Reveals Saturn-mass Planet orbiting M-dwarf Host in the Inner Galactic Disk. 2020. S2CID 215827466. arXiv:2004.09067可免费查阅. doi:10.3847/1538-3881/ab9ac3. 
  62. ^ 62.0 62.1 Carleo, Ilaria; Gandolfi, Davide; Barragán, Oscar; Livingston, John H.; Persson, Carina M.; Lam, Kristine W. F.; Vidotto, Aline; Lund, Michael B.; Carolina Villarreal D'Angelo; Collins, Karen A.; LucaFossati; Howard, Andrew W.; Kubyshkina, Daria; Brahm, Rafael; Oklopčić, Antonija; Mollière, Paul; Redfield, Seth; Luisa Maria Serrano; Dai, Fei; Fridlund, Malcolm; Borsa, Francesco; Korth, Judith; Esposito, Massimiliano; Díaz, Matías R.; Louise Dyregaard Nielsen; Hellier, Coel; Mathur, Savita; Deeg, Hans J.; Hatzes, Artie P.; et al. The multi-planet system TOI-421 -- A warm Neptune and a super puffy mini-Neptune transiting a G9 V star in a visual binary. 2020. arXiv:2004.10095可免费查阅 [astro-ph.EP]. 
  63. ^ 63.0 63.1 63.2 63.3 Daylan, Tansu; Pingle, Kartik; Wright, Jasmine; Guenther, Maximilian N.; Stassun, Keivan G.; Kane, Stephen R.; Vanderburg, Andrew; Jontof-Hutter, Daniel; Rodriguez, Joseph E.; Shporer, Avi; Huang, Chelsea; Mikal-Evans, Tom; Badenas-Agusti, Mariona; Collins, Karen A.; Rackham, Benjamin; Quinn, Sam; Cloutier, Ryan; Collins, Kevin I.; Guerra, Pere; Jensen, Eric L. N.; Kielkopf, John F.; Massey, Bob; Schwarz, Richard P.; Charbonneau, David; Lissauer, Jack J.; Irwin, Jonathan M.; Basturk, Ozgur; Fulton, Benjamin; Soubkiou, Abderahmane; et al. TESS discovery of a super-Earth and three sub-Neptunes hosted by the bright, Sun-like star HD 108236. 2020. arXiv:2004.11314可免费查阅 [astro-ph.EP]. 
  64. ^ 64.0 64.1 Hebrard, G.; Diaz, R. F.; Correia, A. C. M.; Collier Cameron, A.; Laskar, J.; Pollacco, D.; Almenara, J. -M.; Anderson, D. R.; Barros, S. C. C.; Boisse, I.; Bonomo, A. S.; Bouchy, F.; Boue, G.; Boumis, P.; Brown, D. J. A.; Dalal, S.; Deleuil, M.; Demangeon, O.; Doyle, A. P.; Haswell, C. A.; Hellier, C.; Osborn, H.; Kiefer, F.; Kolb, U. C.; Lam, K.; Lecavelier des Etangs, A.; Lopez, T.; Martin-Lagarde, M.; Maxted, P.; et al. Discovery and characterization of the exoplanets WASP-148b and c. A transiting system with two interacting giant planets. Astronomy & Astrophysics. 2020, A32: 640. Bibcode:2020A&A...640A..32H. S2CID 216867348. arXiv:2004.14645可免费查阅. doi:10.1051/0004-6361/202038296. 
  65. ^ 65.0 65.1 A Newtonian model for the WASP-148 exoplanetary system enhanced with TESS and ground-based photometric observations, 2020, arXiv:2012.02602可免费查阅 
  66. ^ Gill, Samuel; Wheatley, Peter J.; Cooke, Benjamin F.; Jordán, Andrés; Nielsen, Louise D.; Bayliss, Daniel; Anderson, David R.; Vines, Jose I.; Lendl, Monika; Acton, Jack S.; Armstrong, David J.; Bouchy, François; Brahm, Rafael; Bryant, Edward M.; Burleigh, Matthew R.; Casewell, Sarah L.; Eigmüller, Philipp; Espinoza, Néstor; Gillen, Edward; Goad, Michael R.; Grieves, Nolan; Günther, Maximilian N.; Henning, Thomas; Hobson, Melissa J.; Hogan, Aleisha; Jenkins, James S.; McCormac, James; Moyano, Maximiliano; Osborn, Hugh P.; et al. NGTS-11 b / TIC-54002556 b: A transiting warm Saturn recovered from a TESS single-transit event. 2020. S2CID 220845943. arXiv:2005.00006可免费查阅. doi:10.3847/2041-8213/ab9eb9. 
  67. ^ Rizzuto, Aaron C.; Newton, Elisabeth R.; Mann, Andrew W.; Tofflemire, Benjamin M.; Vanderburg, Andrew; Kraus, Adam L.; Wood, Mackenna L.; Quinn, Samuel N.; Zhou, George; Pa Chia Thao; Law, Nicholas M.; Ziegler, Carl; Briceno, Cesar. TESS Hunt for Young and Maturing Exoplanets (THYME) II: A 17 Myr Old Transiting Hot Jupiter in the Sco-Cen Association. The Astronomical Journal. 2020, 160 (1): 33. Bibcode:2020AJ....160...33R. S2CID 218470215. arXiv:2005.00013可免费查阅. doi:10.3847/1538-3881/ab94b7. 
  68. ^ 68.0 68.1 Mann, Andrew W.; Johnson, Marshall C.; Vanderburg, Andrew; Kraus, Adam L.; Rizzuto, Aaron C.; Wood, Mackenna L.; Bush, Jonathan L.; Rockcliffe, Keighley; Newton, Elisabeth R.; Latham, David W.; Mamajek, Eric E.; Zhou, George; Quinn, Samuel N.; Pa Chia Thao; Benatti, Serena; Cosentino, Rosario; Desidera, Silvano; Harutyunyan, Avet; Lovis, Christophe; Mortier, Annelies; Pepe, Francesco A.; Poretti, Ennio; Wilson, Thomas G.; Kristiansen, Martti H.; Gagliano, Robert; Jacobs, Thomas; LaCourse, Daryll M.; Omohundro, Mark; Hans Martin Schwengeler; et al. TESS Hunt for Young and Maturing Exoplanets (THYME) III: A two-planet system in the 400 Myr Ursa Major Group. 2020. arXiv:2005.00047可免费查阅 [astro-ph.EP]. 
  69. ^ The TESS-Keck Survey III: A Stellar Obliquity Measurement of TOI-1726 c, 2020, arXiv:2008.12397可免费查阅 
  70. ^ Benatti, S.; Damasso, M.; Desidera, S.; Marzari, F.; Biazzo, K.; Claudi, R.; Di Mauro, M. P.; Lanza, A. F.; Pinamonti, M.; Barbato, D.; Malavolta, L.; Poretti, E.; Sozzetti, A.; Affer, L.; Bignamini, A.; Bonomo, A. S.; Borsa, F.; Brogi, M.; Bruno, G.; Carleo, I.; Cosentino, R.; Covino, E.; Frustagli, G.; Giacobbe, P.; Gonzalez, M.; Gratton, R.; Harutyunyan, A.; Knapic, C.; Leto, G.; et al. The GAPS Programme at TNG -- XXIII. HD 164922 d: A close-in super-Earth discovered with HARPS-N in a system with a long-period Saturn mass companion. Astronomy & Astrophysics. 2020, A50: 639. Bibcode:2020A&A...639A..50B. S2CID 218538033. arXiv:2005.03368可免费查阅. doi:10.1051/0004-6361/202037939. 
  71. ^ Bennett, David P.; Udalski, Andrzej; Bond, Ian A.; Abe, Fumio; Barry, Richard K.; Bhattacharya, Aparna; Donachie, Martin; Fujii, Hirosane; Fukui, Akihiko; Hirao, Yuki; Itow, Yoshitaka; Kawasaki, Kohei; Kirikawa, Rintaro; Kondo, Iona; Koshimoto, Naoki; Man Cheung Alex Li; Matsubara, Yutaka; Miyazaki, Shota; Muraki, Yasushi; Ranc, Clément; Rattenbury, Nicholas J.; Satoh, Yuki; Shoji, Hikaru; Sumi, Takahiro; Suzuki, Daisuke; Tanaka, Yuzuru; Tristram, Paul J.; Yamawaki, Tsubasa; Yonehara, Atsunori; et al. A Gas Giant Planet in the OGLE-2006-BLG-284L Stellar Binary System. The Astronomical Journal. 2020, 160 (2): 72. Bibcode:2020AJ....160...72B. S2CID 218665248. arXiv:2005.07199可免费查阅. doi:10.3847/1538-3881/ab9cb9. 
  72. ^ 72.0 72.1 Obermeier, C.; Steuer, J.; Kellermann, H.; Saglia, R. P.; Henning, Th.; Riffeser, A.; Hopp, U.; Stefansson, G.; Cañas, C.; Ninan, J.; Mahadevan, S.; Isaacson, H.; Howard, A. W.; Livingston, J.; Koppenhoefer, J.; Bender, R. Following the TraCS of exoplanets with Pan-Planets: Wendelstein-1b and Wendelstein-2b. Astronomy & Astrophysics. 2020, 639: A130. Bibcode:2020A&A...639A.130O. S2CID 218971735. arXiv:2005.13560可免费查阅. doi:10.1051/0004-6361/202037715. 
  73. ^ Heller, René; Hippke, Michael; Freudenthal, Jantje; Rodenbeck, Kai; Batalha, Natalie M.; Bryson, Steve. Transit least-squares survey. Astronomy & Astrophysics. 2020, 638: A10. S2CID 219260293. arXiv:2006.02123可免费查阅. doi:10.1051/0004-6361/201936929. 
  74. ^ Niraula, Prajwal; Julien de Wit; Rackham, Benjamin V.; Ducrot, Elsa; Burdanov, Artem; Crossfield, Ian J. M.; Valerie Van Grootel; Murray, Catriona; Garcia, Lionel J.; Alonso, Roi; Beard, Corey; Yilen Gomez Maqueo Chew; Delrez, Laetitia; Demory, Brice-Olivier; Fulton, Benjamin J.; Gillon, Michael; Gunther, Maximilian N.; Howard, Andrew W.; Issacson, Howard; Jehin, Emmanuel; Pedersen, Peter P.; Pozuelos, Francisco J.; Queloz, Didier; Rebolo-Lopez, Rafael; Sairam, Lalitha; Sebastian, Daniel; Thompson, Samantha; Triaud, Amaury H. M. J. $π$ Earth: A 3.14-day Earth-sized Planet from $\textit{K2}$'s Kitchen Served Warm by the SPECULOOS Team. 2020. arXiv:2006.07308可免费查阅 [astro-ph.EP]. 
  75. ^ 75.0 75.1 Stefansson, Gudmundur; Kopparapu, Ravi; Lin, Andrea; Mahadevan, Suvrath; Cañas, Caleb; Kanodia, Shubham; Ninan, Joe; Cochran, William; Endl, Michael; Hebb, Leslie; Wisniewski, John; Gupta, Arvind; Everett, Mark; Bender, Chad; Diddams, Scott; Ford, Eric; Fredrick, Connor; Halverson, Samuel; Hearty, Fred; Levi, Eric; Maney, Marissa; Metcalf, Andrew; Monson, Andrew; Ramsey, Lawrence; Robertson, Paul; Roy, Arpita; Schwab, Christian; Terrien, Ryan; Wright, Jason, A Mini-Neptune and a Venus-Zone Planet in the Radius Valley Orbiting the Nearby M2-dwarf TOI-1266: Validation with the Habitable-zone Planet Finder, 2020, arXiv:2006.11180可免费查阅 
  76. ^ Plavchan, Peter; Barclay, Thomas; Gagné, Jonathan; et al. A planet within the debris disk around the pre-main-sequence star AU Microscopii. Nature. 2020, 582 (7813): 497–500. Bibcode:2020Natur.582..497P. PMID 32581383. S2CID 220042005. arXiv:2006.13248可免费查阅. doi:10.1038/s41586-020-2400-z. 
  77. ^ Addison, Brett C.; Horner, Jonathan; Wittenmyer, Robert A.; Plavchan, Peter; Wright, Duncan J.; Nicholson, Belinda A.; Marshall, Jonathan P.; Clark, Jake T.; Kane, Stephen R.; Hirano, Teruyuki; Kielkopf, John; Shporer, Avi; Tinney, C. G.; Zhang, Hui; Ballard, Sarah; Bedding, Timothy; Bowler, Brendan P.; Mengel, Matthew W.; Okumura, Jack; Gaidos, Eric, The Youngest Planet to Have a Spin-Orbit Alignment Measurement AU Mic b, 2020, arXiv:2006.13675可免费查阅 
  78. ^ EXOPLANET CATALOG AU Microscopii b on exoplanets.nasa.gov. [2021-08-24]. (原始内容存档于2021-06-14). 
  79. ^ Kanodia, Shubham; Cañas, Caleb I.; Stefansson, Gudmundur; Ninan, Joe P.; Hebb, Leslie; Lin, Andrea S. J.; Baran, Helen; Maney, Marissa; Terrien, Ryan C.; Mahadevan, Suvrath; Cochran, William D.; Endl, Michael; Dong, Jiayin; Bender, Chad F.; Diddams, Scott A.; Ford, Eric B.; Fredrick, Connor; Halverson, Samuel; Hearty, Fred; Metcalf, Andrew J.; Monson, Andrew; Ramsey, Lawrence W.; Robertson, Paul; Roy, Arpita; Schwab, Christian; Wright, Jason T., TOI-1728b: The Habitable-zone Planet Finder confirms a warm super Neptune orbiting an M dwarf host, The Astrophysical Journal, 2020, 899 (1): 29, Bibcode:2020ApJ...899...29K, S2CID 220056014, arXiv:2006.14546可免费查阅, doi:10.3847/1538-4357/aba0a2 
  80. ^ Barbato, D.; Pinamonti, M.; Sozzetti, A.; Biazzo, K.; Benatti, S.; Damasso, M.; Desidera, S.; Lanza, A. F.; Maldonado, J.; Mancini, L.; Scandariato, G.; Affer, L.; Andreuzzi, G.; Bignamini, A.; Bonomo, A. S.; Borsa, F.; Carleo, I.; Claudi, R.; Cosentino, R.; Covino, E.; Fiorenzano, A. F. M.; Giacobbe, P.; Harutyunyan, A.; Knapic, C.; Leto, G.; Lorenzi, V.; Maggio, A.; Malavolta, L.; Micela, G.; et al, The GAPS Programme at TNG XXIV. An eccentric Neptune-mass planet near the inner edge of the BD-11 4672 habitable zone, 2020, arXiv:2006.14393可免费查阅 
  81. ^ Youn Kil Jung; Gould, Andrew; Udalski, Andrzej; Sumi, Takahiro; Yee, Jennifer C.; Han, Cheongho; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Ryu, Yoon-Hyun; Shin, In-Gu; Shvartzvald, Yossi; Zhu, Wei; 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.; Mróz, Przemek; Szymański, Michał K.; Skowron, Jan; Poleski, Radek; Soszyński, Igor; Pietrukowicz, Paweł; et al, OGLE-2018-BLG-1269Lb: A Jovian Planet With A Bright, I = 16 Host, 2020, arXiv:2006.15774可免费查阅 
  82. ^ 82.0 82.1 Jeffers, S. V.; Dreizler, S.; Barnes, J. R.; Haswell, C. A.; Nelson, R. P.; Rodríguez, E.; López-González, M. J.; Morales, N.; Luque, R.; Zechmeister, M.; Vogt, S. S.; Jenkins, J. S.; Palle, E.; Berdi Ñas, Z. M.; Coleman, G. A. L.; Díaz, M. R.; Ribas, I.; Jones, H. R. A.; Butler, R. P.; Tinney, C. G.; Bailey, J.; Carter, B. D.; o'Toole, S.; Wittenmyer, R. A.; Crane, J. D.; Feng, F.; Shectman, S. A.; Teske, J.; Reiners, A.; et al, A multiple planet system of super-Earths orbiting the brightest red dwarf star GJ887, Science, 2020, 368 (6498): 1477–1481, Bibcode:2020Sci...368.1477J, PMID 32587019, S2CID 220075207, arXiv:2006.16372可免费查阅, doi:10.1126/science.aaz0795 
  83. ^ 83.0 83.1 83.2 83.3 83.4 83.5 83.6 Bakos, G. Á.; Hartman, J. D.; Bhatti, W.; Csubry, Z.; Penev, K.; Bieryla, A.; Latham, D. W.; Quinn, S.; Buchhave, L. A.; Kovács, G.; Torres, G.; Noyes, R. W.; Falco, E.; Béky, B.; Szklenár, T.; Esquerdo, G. A.; Howard, A. W.; Isaacson, H.; Marcy, G.; Sato, B.; Boisse, I.; Santerne, A.; Hébrard, G.; Rabus, M.; Harbeck, D.; McCully, C.; Everett, M. E.; Horch, E. P.; Hirsch, L.; et al, HAT-P-58b–HAT-P-64b: Seven Planets Transiting Bright Stars, 2020, arXiv:2007.05528可免费查阅 
  84. ^ Cañas, Caleb I.; Stefansson, Gudmundur; Kanodia, Shubham; Mahadevan, Suvrath; Cochran, William D.; Endl, Michael; Robertson, Paul; Bender, Chad F.; Ninan, Joe P.; Beard, Corey; Lubin, Jack; Gupta, Arvind F.; Everett, Mark E.; Monson, Andrew; Wilson, Robert F.; Lewis, Hannah M.; Brewer, Mary; Majewski, Steven R.; Hebb, Leslie; Dawson, Rebekah I.; Diddams, Scott A.; Ford, Eric B.; Fredrick, Connor; Halverson, Samuel; Hearty, Fred; Lin, Andrea S. J.; Metcalf, Andrew J.; Rajagopal, Jayadev; Ramsey, Lawrence W.; et al, A warm Jupiter transiting an M dwarf: A TESS single transit event confirmed with the Habitable-zone Planet Finder, 2020, arXiv:2007.07098可免费查阅 
  85. ^ 85.0 85.1 Jordán, A.; Bakos, G. Á.; Bayliss, D.; Bento, J.; Bhatti, W.; Brahm, R.; Csubry, Z.; Espinoza, N.; Hartman, J. D.; Henning, Th.; Mancini, L.; Penev, K.; Rabus, M.; Sarkis, P.; Suc, V.; de Val-Borro, M.; Zhou, G.; Butler, R. P.; Teske, J.; Crane, J.; Shectman, S.; Tan, T. G.; Thompson, I.; Wallace, J. J.; Lázár, J.; Papp, I.; Sári, P., HATS-37Ab AND HATS-38b: TWO TRANSITING HOT NEPTUNES IN THE DESERT, 2020, arXiv:2007.07135可免费查阅 
  86. ^ Bohn, Alexander J.; Kenworthy, Matthew A.; Ginski, Christian; Rieder, Steven; Mamajek, Eric E.; Meshkat, Tiffany; Pecaut, Mark J.; Reggiani, Maddalena; De Boer, Jozua; Keller, Christoph U.; Snik, Frans; Southworth, John, Two Directly Imaged, Wide-orbit Giant Planets around the Young, Solar Analog TYC 8998-760-1, The Astrophysical Journal, 2020, 898 (1): L16, Bibcode:2020ApJ...898L..16B, S2CID 220686536, arXiv:2007.10991可免费查阅, doi:10.3847/2041-8213/aba27e 
  87. ^ Teske, Johanna; Díaz, Matías R.; Luque, Rafael; Močnik, Teo; Seidel, Julia V.; Otegi, Jon Fernández; Feng, Fabo; Jenkins, James S.; Pallè, Enric; Ségransan, Damien; Udry, Stèphane; Collins, Karen A.; Eastman, Jason D.; Ricker, George R.; Vanderspek, Roland; Latham, David W.; Seager, Sara; Winn, Joshua N.; Jenkins, Jon M.; Anderson, David. R.; Barclay, Thomas; Bouchy, François; Burt, Jennifer A.; Butler, R. Paul; Caldwell, Douglas A.; Collins, Kevin I.; Crane, Jeffrey D.; Dorn, Caroline; Flowers, Erin; et al, TESS Reveals a Short-period Sub-Neptune Sibling (HD 86226c) to a Known Long-period Giant Planet, The Astronomical Journal, 2020, 160 (2): 96, Bibcode:2020AJ....160...96T, S2CID 220830943, arXiv:2007.13927可免费查阅, doi:10.3847/1538-3881/ab9f95 
  88. ^ 88.0 88.1 88.2 88.3 88.4 88.5 88.6 88.7 Feng, Fabo; Shectman, Stephen A.; Clement, Matthew S.; Vogt, Steven S.; Tuomi, Mikko; Teske, Johanna K.; Burt, Jennifer; Crane, Jeffrey D.; Holden, Bradford; Sharon Xuesong Wang; Thompson, Ian B.; Diaz, Matias R.; Paul Butler, R., Search for Nearby Earth Analogs. III. Detection of ten new planets, three planet candidates, and confirmation of three planets around eleven nearby M dwarfs, 2020, arXiv:2008.07998可免费查阅 
  89. ^ TOI-824 b: A New Planet on the Lower Edge of the Hot Neptune Desert, 2020, arXiv:2008.11732可免费查阅 
  90. ^ Damasso, Mario; et al. A low-mass planet candidate orbiting Proxima Centauri at a distance of 1.5 AU. Science Advances英语Science Advances. 15 January 2020, 6 (3). eaax7467. Bibcode:2020SciA....6.7467D. PMC 6962037可免费查阅. PMID 31998838. doi:10.1126/sciadv.aax7467. 
  91. ^ Kervella, Pierre; et al. Orbital inclination and mass of the exoplanet candidate Proxima c. Astronomy & Astrophysics. 29 March 2020, 635: L14. Bibcode:2020A&A...635L..14K. ISSN 0004-6361. S2CID 214713486. arXiv:2003.13106可免费查阅. doi:10.1051/0004-6361/202037551. 
  92. ^ 92.0 92.1 92.2 The TOI-763 system: sub-Neptunes orbiting a Sun-like star, 2020, arXiv:2008.12535可免费查阅 
  93. ^ 93.0 93.1 93.2 93.3 An unusually low density ultra-short period super-Earth and three mini-Neptunes around the old star TOI-561, 2020, arXiv:2009.02332可免费查阅 
  94. ^ 94.0 94.1 94.2 The TESS-Keck Survey II: Masses of Three Sub-Neptunes Transiting the Galactic Thick-Disk Star TOI-561, 2020, arXiv:2009.03071可免费查阅 
  95. ^ 95.0 95.1 A super-Earth and a sub-Neptune orbiting the bright, quiet M3 dwarf TOI-1266, 2020, arXiv:2009.04317可免费查阅 
  96. ^ 96.0 96.1 Two Planets Straddling the Habitable Zone of The Nearby K dwarf Gl 414A, 2020, arXiv:2009.06503可免费查阅 
  97. ^ Cluster Difference Imaging Photometric Survey. II.TOI837: A Young Validated Planet in IC2602, 2020, arXiv:2009.07845可免费查阅 
  98. ^ 98.0 98.1 A planetary system with two transiting mini-Neptunes near the radius valley transition around the bright M dwarf TOI-776, 2020, arXiv:2009.08338可免费查阅 
  99. ^ MOA-2009-BLG-319Lb: A Sub-Saturn Planet Inside the Predicted Mass Desert, 2020, arXiv:2009.08461可免费查阅 
  100. ^ 100.0 100.1 TOI-481 b & TOI-892 b: Two long period hot Jupiters from the Transiting Exoplanet Survey Satellite, 2020, arXiv:2009.08881可免费查阅 
  101. ^ 101.0 101.1 Discovery of a hot, transiting, Earth-sized planet and a second temperate, non-transiting planet around the M4 dwarf GJ 3473 (TOI-488), 2020, arXiv:2009.10432可免费查阅 
  102. ^ NGTS-12b: A sub-Saturn mass transiting exoplanet in a 7.53 day orbit, 2020, arXiv:2009.10620可免费查阅 
  103. ^ A terrestrial-mass rogue planet candidate detected in the shortest-timescale microlensing event, 2020, arXiv:2009.12377可免费查阅 
  104. ^ An Ultra-Hot Neptune in the Neptune desert, 2020, arXiv:2009.12832可免费查阅 
  105. ^ TOI 540 b: A Planet Smaller than Earth Orbiting a Nearby Rapidly Rotating Low-mass Star, 2020, arXiv:2009.13623可免费查阅 
  106. ^ A Highly Eccentric Warm Jupiter Orbiting TIC 237913194, 2020, arXiv:2010.03570可免费查阅 
  107. ^ 107.0 107.1 TFAW survey. I. Wavelet-based denoising of K2 light curves. Discovery and validation of two new Earth-sized planets in K2 campaign 1, arXiv, 2020, arXiv:2009.09285可免费查阅 
  108. ^ OGLE-2018-BLG-0799Lb: a Sub-Saturn-Mass Planet Orbiting a Very Low Mass Dwarf, 2020, arXiv:2010.08732可免费查阅 
  109. ^ 109.0 109.1 TOI-954 b and EPIC 246193072 b: Short-Period Saturn-Mass Planets that Test Whether Irradiation Leads to Inflation, 2020, arXiv:2010.14436可免费查阅 
  110. ^ 110.0 110.1 WASP-186 and WASP-187: two hot Jupiters discovered by SuperWASP and SOPHIE with additional observations by TESS, 2020, arXiv:2010.15205可免费查阅 
  111. ^ 111.0 111.1 TOI 122b and TOI 237b, two small warm planets orbiting inactive M dwarfs, found by TESS, 2020, arXiv:2010.15905可免费查阅 
  112. ^ HAT-P-68b: A TRANSITING HOT JUPITER AROUND A K5 DWARF STAR, 2020, arXiv:2010.16026可免费查阅 
  113. ^ The CARMENES search for exoplanets around M dwarfs LP 714-47 b (TOI 442.01): Populating the Neptune desert, 2020, arXiv:2011.01716可免费查阅 
  114. ^ A wide planetary-mass companion to a young low-mass brown dwarf in Ophiuchus, arXiv:2011.08871可免费查阅 
  115. ^ 115.0 115.1 115.2 A collage of small planets from the Lick Carnegie Exoplanet Survey :Exploring the super-Earth and sub-Neptune mass regime, 2020, arXiv:2011.08867可免费查阅 
  116. ^ TOI-519 b: a short-period substellar object around an M dwarf validated using multicolour photometry and phase curve analysis, 2020, arXiv:2011.11458可免费查阅 
  117. ^ 117.0 117.1 117.2 117.3 The Magellan-TESS Survey I: Survey Description and Mid-Survey Results, 2020, arXiv:2011.11560可免费查阅 
  118. ^ 118.00 118.01 118.02 118.03 118.04 118.05 118.06 118.07 118.08 118.09 118.10 118.11 118.12 118.13 118.14 118.15 118.16 118.17 118.18 118.19 118.20 118.21 ULTRA SHORT PERIOD PLANETS IN K2 III: NEIGHBORS ARE COMMON WITH 12 NEW MULTI-PLANET SYSTEMS AND 26 NEWLY VALIDATED PLANETS IN CAMPAIGNS 0-8, 10, 2020, arXiv:2011.11698可免费查阅 
  119. ^ 119.0 119.1 119.2 Two young planetary systems around field stars with ages between 20 − 320 Myr from TESS, 2020, arXiv:2011.13349可免费查阅 
  120. ^ 120.0 120.1 The GAPS Programme at TNG XXVIII A pair of hot-Neptunes orbiting the young star TOI-942, 2020, arXiv:2011.13795可免费查阅 
  121. ^ Giant Outer Transiting Exoplanet Mass (GOT ‘EM) Survey. I. Confirmation of an Eccentric, Cool Jupiter With an Interior Earth-sized Planet Orbiting Kepler-1514, 2020, arXiv:2012.04676可免费查阅 
  122. ^ OGLE-2017-BLG-1049: Another microlensing event with a giant planet, 2020, arXiv:2012.11080可免费查阅 
  123. ^ New constraints on the planetary system around the young active star AU Mic Two transiting warm Neptunes near mean-motion resonance, 2020, arXiv:2012.13238可免费查阅 
  124. ^ 124.0 124.1 124.2 Precise radial velocities of giant stars XIV. Evidence of planetary companions around HD 25723, 17 Sco, 3 Cnc, and 44 UMa. [2021-08-24]. (原始内容存档于2021-10-09). 
  125. ^ 125.0 125.1 A SEARCH FOR EXOPLANETS AROUND NORTHERN CIRCUMPOLAR STARS VI. DETECTION OF PLANETARY COMPANIONS ORBITING THE GIANTS HD 60292 AND HD 112640 (PDF). [2021-08-24]. (原始内容 (PDF)存档于2022-04-29). 
  126. ^ K2-111: an old system with two planets in near-resonance, 2020, arXiv:2010.01993可免费查阅 
  127. ^ 127.00 127.01 127.02 127.03 127.04 127.05 127.06 127.07 127.08 127.09 127.10 127.11 Castro González, A.; Díez Alonso, E.; Menéndez Blanco, J.; et al. Planetary candidates transiting cool dwarf stars from Campaigns 12 to 15 of K2. 2020. arXiv:2007.12744v2可免费查阅 [astro-ph.EP]. 
  128. ^ 128.0 128.1 128.2 128.3 Four Microlensing Planets with Faint-source Stars Identified in the 2016 and 2017 Season Data, 2020, arXiv:2008.09258可免费查阅 
  129. ^ KMT-2018-BLG-0748Lb: Sub-Saturn Microlensing Planet Orbiting an Ultracool Host, 2020, arXiv:2007.05204可免费查阅 
  130. ^ KMT-2019-BLG-1339L: AN M DWARF WITH A GIANT PLANET OR A COMPANION NEAR THE PLANET/BROWN DWARF BOUNDARY, 2020, arXiv:2003.02375可免费查阅 
  131. ^ KMT-2019-BLG-2073: Fourth Free-Floating-Planet Candidate with θE < 10 µas, 2020, arXiv:2007.06870可免费查阅 
  132. ^ A free-floating or wide-orbit planet in the microlensing event OGLE-2019-BLG-0551, 2020, arXiv:2003.01126可免费查阅 
  133. ^ Curiel, Salvador; Ortiz-León, Gisela N.; Mioduszewski, Amy J.; Torres, Rosa M. An Astrometric Planetary Companion Candidate to the M9 Dwarf TVLM 513–46546. The Astronomical Journal. 2020, 160 (3): 97. Bibcode:2020AJ....160...97C. S2CID 220961489. arXiv:2008.01595可免费查阅. doi:10.3847/1538-3881/ab9e6e. 
  134. ^ The CARMENES search for exoplanets around M dwarfs Measuring precise radial velocities in the near infrared: the example of the super-Earth CD Cet b, 2020, arXiv:2006.01684可免费查阅 
  135. ^ OGLE-2018-BLG-0799Lb: a Sub-Saturn-Mass Planet Orbiting a Very Low Mass Dwarf, 2020, arXiv:2010.08732可免费查阅 
  136. ^ Vanderburg, Andrew; Rappaport, Saul A.; Xu, Siyi; Crossfield, Ian J. M.; Becker, Juliette C.; Gary, Bruce; et al. A giant planet candidate transiting a white dwarf. Nature. September 2020, 585 (7825): 363–367. Bibcode:2020arXiv200907282V. PMID 32939071. S2CID 221738865. arXiv:2009.07282可免费查阅. doi:10.1038/s41586-020-2713-y. 
  137. ^ A Habitable-Zone Earth-Sized Planet Rescued from False Positive Status, 2020, arXiv:2004.06725可免费查阅 
  138. ^ 138.00 138.01 138.02 138.03 138.04 138.05 138.06 138.07 138.08 138.09 138.10 138.11 138.12 138.13 138.14 138.15 138.16 138.17 138.18 138.19 138.20 138.21 138.22 138.23 138.24 138.25 138.26 138.27 138.28 138.29 138.30 138.31 138.32 138.33 138.34 138.35 138.36 138.37 138.38 138.39 138.40 138.41 138.42 138.43 138.44 138.45 138.46 138.47 Exoplanet Validation with Machine Learning: 50 new validated Kepler planets, 2020, arXiv:2008.10516可免费查阅 
  139. ^ Vissapragada, Shreyas; Jontof-Hutter, Daniel; Shporer, Avi; Knutson, Heather A.; Liu, Leo; Thorngren, Daniel; Lee, Eve J.; Chachan, Yayaati; Mawet, Dimitri; Millar-Blanchaer, Maxwell A.; Nilsson, Ricky. Diffuser-Assisted Infrared Transit Photometry for Four Dynamically Interacting \textit{Kepler} Systems. The Astronomical Journal. 2020-02-13, 159 (3): 108. ISSN 1538-3881. doi:10.3847/1538-3881/ab65c8. 
  140. ^ Exoplanet Archive. exoplanetarchive.ipac.caltech.edu. [2021-01-29]. (原始内容存档于2020-10-31).