2021年发现的系外行星列表
这是2021年发现的系外行星列表。仅由径向速度发现的太陽系外行星，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） | 发现方式 | 距离（ly） | 主星质量（M☉） | 主星温度（K） | 注释 |
|---|---|---|---|---|---|---|---|---|---|---|
| HD 108236 f | 0.17406+0.00482 −0.00437 |
29.54255+0.00069 − |
0.1759+0.0037 − |
凌日 | 211 | 0.853+0.047 − |
5,720.0+50.0 − |
[1][2] | ||
| NGTS-14Ab | 0.092+0.012 − |
0.444+0.030 − |
3.5357173+0.0000069 − |
0.0403+0.0071 − |
1,143+139 − |
凌日 | 1,060 | 0.898+0.035 − |
5,187+11 − |
[3] |
| TOI-1259Ab | 0.441+0.049 −0.047 |
1.022+0.030 −0.037 |
3.4779780+0.0000019 −0.0000017 |
0.04070+0.00114 −0.00110 |
936 | 凌日 | 385+1 − |
0.68+0.1 −0.01 |
4,775+100 − |
[4] |
| NGTS-13b | 4.84+0.44 − |
1.142+0.046 − |
4.12 | 0.0549+0.0015 −0.0025 |
1,605+30 − |
凌日 | 2150 | 1.30+0.11 −0.18 |
5,819+73 − |
[5] |
| TOI-628 b | 6.33+0.29 −0.31 |
1.060+0.041 −0.034 |
3.4095675+0.0000070 −0.0000069 |
0.04860+0.00080 −0.00094 |
1,586+52 −40 |
凌日 | 582 | 1.311+0.066 −0.075 |
6,250+220 −190 |
主星又名HD 288842[6] |
| TOI-640 b | 0.88+0.16 − |
1.771+0.060 −0.056 |
5.0037775+0.0000048 − |
0.06608+0.00098 −0.0011 |
1,749+26 −30 |
凌日 | 1,115 | 1.536+0.069 −0.076 |
6,460+130 −150 |
[6] |
| TOI-1333 A b | 2.37+0.24 − |
1.396+0.056 −0.054 |
4.720219+0.000011 − |
0.0626+0.0011 −0.0012 |
1,679+35 −34 |
凌日 | 653 | 1.464+0.076 −0.079 |
6,274+97 − |
主星又名BD+47 3521A[6] |
| TOI-1478 b | 0.847+0.052 −0.048 |
1.061+0.040 −0.038 |
10.180249+0.000015 − |
0.0903+0.0018 −0.0013 |
918+11 − |
凌日 | 498 | 0.946+0.059 −0.041 |
5,595+83 −81 |
[6] |
| TOI-1601 b | 0.99+0.11 − |
1.239+0.046 −0.039 |
5.331751+0.000011 − |
0.06864+0.00079 −0.00075 |
1,619+24 −23 |
凌日 | 1,096 | 1.517+0.053 −0.049 |
5,948+87 −89 |
[6] |
| OGLE-2019-BLG-0960Lb | 0.0071+0.0027 − |
1.75+0.55 − |
微重力透镜 | 2,900+1000 − |
0.45+0.15 − |
用微重力透镜法发现的最小行星[7] | ||||
| HD 110113 b | 0.0143+0.0020 − |
0.183+0.011 − |
2.541+0.0005 −0.001 |
0.035+0.001 − |
1,371+14 − |
凌日 | 346.5+2.3 − |
0.99+0.08 − |
5,730 | 主星又名TOI-755[8] |
| HD 110113 c | 0.0330+0.0038 − |
6.744+0.008 −0.009 |
0.068+0.001 −0.002 |
990+10 − |
径向速度 | 346.5+2.3 − |
0.99+0.08 − |
5,730 | 主星又名TOI-755[8] | |
| KOI-5Ab | 0.179 | 0.63 | 5 | 凌日 | 1,870+70 − |
1.13 | 5861 | 又名 TOI-1241b[9][10] | ||
| TOI-178b | 0.0047+0.0012 −0.0013 |
0.102+0.006 − |
1.914558+0.000018 − |
0.02607+0.00078 − |
1,040+22 −21 |
凌日 | 205.16+0.03 − |
0.650+0.027 −0.029 |
4,316+70 − |
[11] |
| TOI-178c | 0.015+0.0017 −0.0021 |
0.149+0.01 −0.008 |
3.238450+0.000020 −0.000019 |
0.0370+0.0011 − |
873+18 − |
凌日 | 205.16+0.03 − |
0.650+0.027 −0.029 |
4,316+70 − |
[11] |
| TOI-178d | 0.0094+0.0025 −0.0032 |
0.229+0.006 − |
6.557700+0.000016 − |
0.0592+0.0018 − |
690+14 − |
凌日 | 205.16+0.03 − |
0.650+0.027 −0.029 |
4,316+70 − |
[11] |
| TOI-178e | 0.0121+0.0039 −0.0029 |
0.197+0.007 −0.008 |
9.961881+0.000042 − |
0.0783+0.0023 −0.0024 |
600+12 − |
凌日 | 205.16+0.03 − |
0.650+0.027 −0.029 |
4,316+70 − |
[11] |
| TOI-178f | 0.0242+0.0052 −0.0047 |
0.204+0.009 − |
15.231915+0.000115 −0.000095 |
0.1039+0.0031 − |
521+11 − |
凌日 | 205.16+0.03 − |
0.650+0.027 −0.029 |
4,316+70 − |
[11] |
| TOI-178g | 0.0123+0.0041 −0.0050 |
0.256+0.012 −0.011 |
20.70950+0.00014 −0.00011 |
0.1275+0.0038 −0.0039 |
470+10 − |
凌日 | 205.16+0.03 − |
0.650+0.027 −0.029 |
4,316+70 − |
[11] |
| HD 183579 b | 0.0620+0.0126 −0.0123 |
0.317+0.013 −0.011 |
17.471278+0.000058 −0.000060 |
0.1334+0.0062 −0.0061 |
769+17 −13 |
凌日 | 186.1+0.8 − |
1.031+0.025 −0.026 |
5,788+44 − |
主星又名TOI-1055[12][13] |
| KMT-2019-BLG-0371b | 7.70+11.34 −3.90 |
0.79+0.14 −0.16 |
微重力透镜 | 2,3000+3,000 −4,000 |
0.09+0.14 −0.05 |
[14] | ||||
| HD 5278 b | 0.0245+0.0047 −0.0044 |
0.219+0.004 − |
14.339156+0.000049 −0.000047 |
0.1202+0.0013 − |
943+13 − |
凌日 | 183.1+2.7 − |
1.126+0.036 −0.035 |
6,203+64 − |
主星又名TOI-130[15] |
| HD 5278 c | 0.0579+0.0057 −0.0060 |
0.2416+0.0027 − |
0.1202+0.0013 − |
943+13 − |
径向速度 | 183.1+2.7 − |
1.126+0.036 −0.035 |
6,203+64 − |
主星又名TOI-130[15] | |
| KMT-2018-BLG-1025Lb | 0.0191+0.0258 −0.0104 |
1.305+0.194 −0.227 |
微重力透镜 | 22,000+3,000 − |
0.219+0.297 −0.120 |
[16] | ||||
| 格利泽1151b | 0.0079+0.0016 − |
2.02 | 0.01735+0.00065 −0.00070 |
径向速度 | 26.23+0.01 − |
0.154 | 3,143+26 − |
[17][18] | ||
| TOI-558b | 3.61+0.15 − |
1.086+0.041 −0.038 |
14.574071+0.000026 − |
0.1291+0.0020 −0.0021 |
1,061+13 −12 |
凌日 | 1,312+17 − |
1.349+0.064 −0.065 |
6,466+95 −93 |
[19] |
| TOI-559b | 6.01+0.24 −0.23 |
1.091+0.028 −0.025 |
6.9839095+0.0000051 − |
0.0723+0.0013 − |
1,180+18 −16 |
凌日 | 761+7 − |
1.026+0.057 − |
5,925+85 −76 |
[19] |
| Candidate 1 | 0.062-0.157 | 0.3011-0.6386 | 影像 | 4.37 | 图像在南门二附近 | |||||
| HD 13808 b | 0.0346 | 14.2 | 0.11 | 径向速度 | 92.2 | 0.771+0.022 − |
5,035+50 − |
2011年成为候选系外行星，2021年正式确认[20][21] | ||
| HD 13808 c | 0.0315 | 53.8 | 0.26 | 径向速度 | 92.2 | 0.771+0.022 − |
5,035+50 − |
2011年成为候选系外行星，2021年正式确认[20][21] | ||
| TOI 451 b | 0.1732+0.0134 −0.0116 |
1.858701+0.000027 −0.000033 |
0.0271+0.0023 −0.0038 |
1,524+100 −60 |
凌日 | 405.1+1.3 − |
0.94+0.025 − |
5,550+56 − |
[22][23] 主星又名CD-38 1467 | |
| TOI 451 c | 0.2741+0.0125 − |
9.192523+0.000064 −0.000084 |
0.0771+0.0066 −0.0093 |
903+53 −36 |
凌日 | 405.1+1.3 − |
0.94+0.025 − |
5,550+56 − |
[22][23] 主星又名CD-38 1467 | |
| TOI 451 d | 0.3598+0.0134 − |
16.364981+0.000047 −0.000049 |
0.1255+0.0057 −0.0065 |
708+15 −12 |
凌日 | 405.1+1.3 − |
0.94+0.025 − |
5,550+56 − |
[22][23] 主星又名CD-38 1467. | |
| HD 110082 b | 0.2857+0.0089 − |
10.18271+0.00004 − |
0.113+0.009 −0.013 |
凌日 | 342.8+0.9 − |
1.21+0.06 − |
6,200+100 − |
[24]主星又名TOI-1098. | ||
| OGLE-2018-BLG-0567Lb | 0.32+0.34 −0.16 |
2.72+0.49 −0.55 |
微重力透镜 | 23,000+3,000 − |
0.24+0.16 −0.13 |
[25] | ||||
| OGLE-2018-BLG-0962Lb | 1.37+0.80 −0.72 |
3.57+0.68 −1.02 |
微重力透镜 | 21,000+3,000 −5,000 |
0.55+0.32 −0.29 |
[25] | ||||
| Gliese 740 b | 0.0093+0.0016 − |
2.37756+0.00013 −0.00011 |
0.029+0.001 − |
829+40 −50 |
径向速度 | 36.21+0.02 − |
0.58+0.06 − |
3,913+21 − |
[26] | |
| OGLE-2018-BLG-1428Lb | 0.77+0.77 −0.53 |
3.30+0.59 −0.83 |
微重力透镜 | 20,000+3,000 −5,000 |
0.43+0.33 −0.22 |
[27] | ||||
| LHS 1478 b | 0.0073+0.0006 − |
0.111+0.004 − |
1.9495378+0.0000040 −0.0000041 |
0.01848+0.00061 −0.0006 |
595+10 −9 |
凌日 | 59.40+0.03 − |
0.236+0.012 − |
3,381+54 − |
[28] 主星又名TOI-1640或G 245-61. |
| TOI-1685 b | 0.0121+0.030 − |
0.131+0.006 − |
0.6691425+0.0000037 − |
0.01156+0.00009 − |
1,052+21 − |
凌日 | 122.68+0.09 − |
0.495+0.019 − |
3,434+51 − |
[29][30] 主星又名UCAC4 666-026266 |
| TOI-1685 c | 0.0290+0.0065 − |
9.025+0.104 −0.119 |
449.1+6.9 − |
径向速度 | 122.68+0.09 − |
0.495+0.019 − |
3,434+51 − |
未证实[29] | ||
| KMT-2020-BLG-0414Lb | 0.0032 | 0.15 | 微重力透镜 | 3,300+300 − |
0.3 | 距离主星15AU处有一质量17 MJ 的棕矮星[31] | ||||
| HD 39474 b | 0.42+0.05 −0.03 |
1.008+0.012 −0.015 |
52.97818+0.00004 −0.00004 |
0.30+0.02 −0.03 |
759+37 −26 |
凌日 | 372.5+1.1 − |
1.316+0.027 − |
6,394+75 − |
主星又名TOI-201[32] |
| 格利泽486b | 0.0089+0.0004 − |
0.117+0.006 − |
1.467119+0.000031 −0.000030 |
0.01734+0.00026 −0.00027 |
701+13 − |
凌日 | 26.344+0.013 − |
0.323+0.015 − |
3,340+54 − |
可能有可测量的大气层[33] |
| NGTS-15b | 0.751+0.102 −0.088 |
1.10+0.10 − |
3.27623+0.00001 − |
0.0441+0.0046 − |
1,146+47 − |
凌日 | 2,580+60 − |
0.995+0.015 − |
5,600+150 − |
[34] |
| NGTS-16b | 0.667+0.157 −0.129 |
1.30+0.13 −0.12 |
4.84532+0.00002 − |
0.0523+0.0064 − |
1,177+59 − |
凌日 | 2,910+95 −75 |
1.002+0.011 − |
5,550+150 − |
[34] |
| NGTS-17b | 0.764+0.195 −0.164 |
1.24+0.11 − |
3.24253+0.00001 − |
0.0391+0.0043 − |
1,457+50 − |
凌日 | 3,420+90 − |
1.025+0.015 −0.014 |
5,650+100 − |
[34] |
| NGTS-18b | 0.409+0.081 −0.063 |
1.21+0.18 − |
3.05125+0.00001 − |
0.0448+0.0068 − |
1,381+55 −53 |
凌日 | 3,610+140 − |
1.003+0.020 −0.012 |
5,610+150 − |
[34] |
| OGLE-2019-BLG-1053Lb | 0.0078+0.0037 −0.0031 |
3.4+0.5 − |
微重力透镜 | 22,000+3,000 −2,000 |
0.61+0.29 −0.24 |
[35] | ||||
| TOI-1634 b | 0.0313+0.0030 − |
0.158+0.007 − |
0.9893457+0.0000034 − |
0.01491+0.00015 − |
921+21 − |
凌日 | 114.40+0.08 − |
0.452+0.014 − |
3,472+48 − |
[30][36] |
| KMT-2019-BLG-1715 | 2.56+1.13 −1.16 |
3.32+0.82 −0.92 |
微重力透镜 | 13,000+3,000 − |
0.61+0.27 −0.28 |
星系内有一质量为0.15M☉ 的红矮星[37] | ||||
| OGLE-2018-BLG-1185b | 0.026+0.025 −0.015 |
1.54+0.18 −0.22 |
微重力透镜 | 24,000+2,000 −3,000 |
0.37+0.35 −0.21 |
行星质量可能有多种情况[38] | ||||
| TOI-1260 b | 0.0271+0.0043 −0.0037 |
0.208+0.009 −0.008 |
3.12748+0.000047 −0.000038 |
0.0366+0.0022 −0.0036 |
860+47 −31 |
凌日 | 239.5+0.3 − |
0.66+0.01 − |
4,227+85 − |
[39] |
| TOI-1260 c | 0.0373+0.0106 −0.0102 |
0.252+0.013 − |
7.49325+0.00015 −0.00013 |
0.0656+0.0039 −0.0065 |
643+35 −23 |
凌日 | 239.5+0.3 − |
0.66+0.01 − |
4,227+85 − |
[39] |
| KMT-2018-BLG-1976Lb | 1.96+1.23 −1.12 |
2.04+0.72 −0.83 |
微重力透镜 | 19,000+2,000 − |
0.65+0.41 −0.37 |
[40] | ||||
| KMT-2018-BLG-1996Lb | 1.22+0.72 −0.63 |
1.97+0.51 −0.25 |
微重力透镜 | 19,000+2,000 − |
0.69+0.40 −0.38 |
[40] | ||||
| OGLE-2019-BLG-0954Lb | 14.2+9.9 −7.5 |
2.65+0.89 −1.20 |
微重力透镜 | 12,000+1,000 −2,000 |
0.80+0.55 −0.42 |
[40] | ||||
| YSES 2 b | 6.3+1.6 −0.9 |
115 | 影像 | 356.4+0.5 − |
1.10+0.03 − |
4,749+40 − |
[41] | |||
| KMT-2016-BLG-2605b | 0.8+1.2 −0.4 |
0.68+0.11 − |
微重力透镜 | 21,000+3,000 − |
0.065+0.10 −0.035 |
[42] | ||||
| TOI-1431 b | 3.14+0.19 −0.18 |
1.51+0.06 − |
2.65022+0.00001 − |
0.047+0.002 − |
2,370+100 − |
凌日 | 488+3 − |
1.90+0.10 −0.08 |
7,690+400 −250 |
又名MASCARA-5b[43][44] |
| TOI-269 b | 0.0277+0.0044 − |
0.247+0.011 − |
3.697723+0.000018 −0.000017 |
0.0345+0.0015 − |
531+25 − |
凌日 | 186.01+0.25 − |
0.3917+0.0095 − |
3,514+70 − |
[45] |
| TOI-220 b | 0.0434+0.0031 − |
0.271+0.013 − |
10.695264 | 0.08911+0.0010 − |
805+21 − |
凌日 | 290+13 − |
0.825+0.028 − |
5,298+65 − |
[46] |
| TOI 1062 b | 0.0320+0.0026 − |
0.202+0.008 − |
4.11412+0.0014 −0.0015 |
0.052 | 1,077+10 −9 |
凌日 | 268.7+0.2 − |
0.94+0.02 − |
5,328+56 − |
[47] |
| TOI 1062 c | 0.0294+0.0039 − |
7.978+0.021 −0.023 |
0.080+0.013 −0.012 |
859+9 −8 |
径向速度 | 268.7+0.2 − |
0.94+0.02 − |
5,328+56 − |
[47] | |
| Kepler-129d | 8.3+1.1 −0.7 |
2646+140 −94 |
4.0+0.1 − |
径向速度 | 1,349+14 − |
1.18 | 5,770 | [48] | ||
| Gliese 9689 b | 0.0304+0.0046 − |
18.27+0.01 − |
0.1139+0.0039 − |
453+39 − |
径向速度 | 100.10+0.04 − |
0.59+0.06 − |
3,836+69 − |
[49] | |
| TOI-1231 b | 0.0485+0.0104 − |
0.326+0.014 − |
24.245586+0.000064 −0.000066 |
0.1288+0.0021 −0.0022 |
330 | 凌日 | 89.68+0.04 − |
0.485+0.024 − |
3,553+31 − |
[50] |
| TIC 172900988 b | 2.84+0.25 − |
1.009+0.043 − |
196.5+7.7 − |
凌日 | 799+9 − |
1.24 and 1.20 | 6050 and 5983 | [51] | ||
| TOI-1444 b | 0.0122+0.0022 − |
0.125+0.006 − |
0.4702694+0.0000044 − |
0.1288+0.0021 −0.0022 |
330 | 凌日 | 408.9+0.5 − |
0.934+0.038 − |
5,430+90 − |
[52] |
| BD+45 0564 b | 1.36+0.12 − |
307.88+1.47 − |
0.83+0.04 − |
径向速度 | 174+2 − |
0.81+0.07 − |
5,004+50 − |
[53] | ||
| BD+55 0362 b | 0.72+0.08 − |
265.59+1.04 − |
0.78+0.05 − |
径向速度 | 168+2 − |
0.909+0.099 − |
5,012+78 − |
[53] | ||
| BD+63 1405 b | 3.96+0.31 − |
1,198.48+60.79 − |
2.06+0.14 − |
径向速度 | 124.4+1.2 − |
0.82+0.08 − |
5,000+53 − |
[53] | ||
| HD 124330 b | 0.75+0.06 − |
270.66+1.21 − |
0.86+0.04 − |
径向速度 | 198+3 − |
1.15+0.079 − |
5,873+19 − |
[53] | ||
| HD 155193 b | 0.75+0.06 − |
352.65+2.58 − |
1.04+0.04 − |
径向速度 | 186+6 − |
1.221+0.083 − |
6,239+20 − |
[53] | ||
| HD 331093 b | 1.50+0.11 − |
621.62+16.11 − |
1.44+0.07 − |
径向速度 | 164.07+0.14 − |
1.030+0.079 − |
5,544+33 − |
[53] | ||
| HD 107148 c | 0.0626+0.0097 −0.0098 |
18.3267+0.0022 −0.0024 |
0.1406+0.0018 − |
径向速度 | 161.4+0.4 − |
1.1+0.1 − |
5,789+36 − |
[54] | ||
| HD 136925 b | 0.84+0.078 −0.074 |
4,540+160 −140 |
5.13+0.12 −0.11 |
径向速度 | 156.2 | 5715 | [54] | |||
| 蜀增一b | 0.0428+0.0047 −0.0045 |
15.5083+0.0016 −0.0018 |
0.1238+0.002 − |
径向速度 | 38.87+0.07 − |
1.14 | 5,884+4 − |
[54] | ||
| HD 156668 c | 0.0991+0.0079 −0.0077 |
811.3+5.2 −5.3 |
1.570+0.017 − |
径向速度 | 79.34+0.03 − |
0.772+0.020 − |
4,850+88 − |
[54] | ||
| HD 164922 e | 0.0331+0.0031 − |
41.763+0.012 − |
0.2293+0.0026 −0.0027 |
径向速度 | 71.69+0.03 − |
0.874+0.012 − |
5,293+32 − |
[54] | ||
| HD 168009 b | 0.0300+0.0038 −0.0037 |
15.1479+0.0035 −0.0037 |
0.1192+0.0017 −0.0018 |
径向速度 | 75.97+0.03 − |
0.99 | 5,792+80 − |
[54] | ||
| HD 213472 b | 3.48+1.10 −0.59 |
16,700+12,000 −4,800 |
13.0+5.7 −2.6 |
径向速度 | 210.6 | [54] | ||||
| HD 24040 c | 0.201+0.027 − |
515.4+2.2 −2.5 |
1.3+0.021 − |
径向速度 | 152.3+0.4 − |
1.14+0.02 − |
5,917+52 − |
[54] | ||
| HD 26161 b | 13.5+8.5 −3.7 |
32,000+21,000 −10,000 |
20.4+7.9 −4.9 |
径向速度 | 133.6+0.3 − |
[54] | ||||
| HD 3765 b | 0.173+0.014 −0.013 |
1,211+15 −16 |
2.108+0.032 −0.033 |
径向速度 | 78.5+0.1 − |
[54] | ||||
| HD 66428 c | 27+22 −17 |
39,000+56,000 −18,000 |
23.0+19.0 −7.6 |
径向速度 | 174.1+0.7 − |
1.09+0.02 − |
5,773+55 − |
[54] | ||
| HD 68988 c | 15.0+2.8 −1.5 |
16,100+11,000 −3,500 |
13.2+5.3 −2.0 |
径向速度 | 198.8+0.6 − |
1.16+0.01 − |
5,919+11 − |
2006年成为候选系外行星[54] | ||
| 拉蘭德21185c | 0.0568+0.0091 −0.0083 |
3190+200 −170 |
3.1+0.13 −0.11 |
径向速度 | 8.31+0.01 − |
0.390+0.011 − |
3,601+51 − |
[54] | ||
| G 264-12 b | 0.0079+0.0009 − |
2.30538+0.00031 − |
0.02279+0.00061 − |
587+16 − |
径向速度 | 52.14+0.03 − |
0.297+0.024 − |
3,326+54 − |
[55] | |
| G 264-12 c | 0.0118+0.0015 − |
8.0518+0.0034 − |
0.0525+0.0014 − |
387+11 − |
径向速度 | 52.14+0.03 − |
0.297+0.024 − |
3,326+54 − |
[55] | |
| Gliese 393 b | 0.0054+0.0008 − |
7.02679+0.00082 −0.00085 |
0.05402+0.00072 − |
485+11 − |
径向速度 | 22.956+0.008 − |
0.426+0.017 − |
3,579+51 − |
[55] | |
| TOI-674b | 0.0739+0.0104 − |
0.470+0.016 − |
1.977143+0.000003 − |
0.0231+0.0007 − |
661+14 − |
凌日 | 150.86+0.11 − |
0.442+0.007 − |
3,505+28 −32 |
[56]可能有大气层[57] |
| HD 152843 b | 0.0364+0.0207 −0.0193 |
0.304+0.012 − |
11.6264+0.0022 −0.0025 |
0.1053+0.003 −0.0031 |
凌日 | 352.0+1.0 − |
1.15+0.04 − |
6,310+100 − |
[58] | |
| HD 152843 c | 0.0865 | 0.521+0.013 − |
24.38+6.23 −3.4 |
凌日 | 352.0+1.0 − |
1.15+0.04 − |
6,310+100 − |
[58] | ||
| KMT-2019-BLG-0253b | 0.029+0.016 −0.013 |
3.1+0.8 −0.9 |
微重力透镜 | 16,000+6,000 −5,000 |
0.70+0.34 −0.31 |
[59] | ||||
| OGLE-2018-BLG-0506 | 0.051+0.038 −0.027 |
3.0+0.7 −0.8 |
微重力透镜 | 18,000+5,000 − |
0.63+0.37 −0.32 |
[59] | ||||
| OGLE-2018-BLG-0516 | 0.063+0.052 −0.034 |
2.2+0.8 −0.7 |
微重力透镜 | 7,000+3,000 −2,000 |
0.47+0.38 −0.25 |
[59] | ||||
| OGLE-2019-BLG-1492 | 0.117+0.079 −0.061 |
2.7+0.9 − |
微重力透镜 | 18,000+6,000 −7,000 |
0.68+0.34 − |
[59] | ||||
| OGLE-2018-BLG-0977 | 0.020+0.016 −0.012 |
2.0+0.6 −0.5 |
微重力透镜 | 7,000+2,000 − |
0.47+0.38 −0.27 |
[59] | ||||
| TOI-1789 b | 0.70+0.16 − |
1.40+0.22 −0.13 |
3.208666+0.000016 − |
0.04873+0.00065 −0.0016 |
1,929+28 −18 |
凌日 | 729+3 − |
1.499+0.061 −0.15 |
5,984+55 −57 |
[60] |
| TOI-942 b | 0.347+0.022 −0.020 |
4.32421+0.000019 − |
0.04866+0.00016 −0.00013 |
凌日 | 493.9+1.0 − |
0.8220+0.0079 −0.0064 |
[61] | |||
| TOI-942 c | 0.417+0.030 −0.027 |
10.156272+0.000037 −0.000034 |
0.08598+0.00027 −0.00022 |
凌日 | 493.9+1.0 − |
0.8220+0.0079 −0.0064 |
[61] | |||
| KMT-2018-BLG-1743 | 0.245+0.339 −0.135 |
1.449+0.209 −0.229 |
微重力透镜 | 21,000+3,000 − |
0.193+0.268 −0.107 |
轨道有多种可能，主星为双星系统[62] | ||||
| TOI-1749 b | 0.060+0.07 −0.04 |
0.124+0.018 − |
2.388821+0.000057 −0.000073 |
0.0291+0.0005 − |
831+18 − |
凌日 | 324.8+0.4 − |
0.58+0.03 − |
3,985+55 − |
[63] |
| TOI-1749 c | 0.007+0.018 −0.005 |
0.189+0.011 − |
4.489010+0.000040 −0.000061 |
0.0443+0.0008 − |
673+15 − |
凌日 | 324.8+0.4 − |
0.58+0.03 − |
3,985+55 − |
[63] |
| TOI-1749 d | 0.014+0.020 −0.011 |
0.225+0.013 − |
9.04455+0.00012 − |
0.0707+0.0012 − |
533+12 − |
凌日 | 324.8+0.4 − |
0.58+0.03 − |
3,985+55 − |
[63] |
| HD 27969 b | 4.80+0.24 −0.23 |
654.5+5.7 −5.8 |
1.552+0.032 −0.033 |
261+11 − |
径向速度 | 1.16+0.07 − |
5,966+21 − |
[64] | ||
| HD 80869 b | 4.86+0.65 −0.29 |
1711.7+9.3 −9.6 |
2.878+0.045 −0.046 |
203.2+6.8 −5.5 |
径向速度 | 1.08+0.05 − |
5,837+15 − |
轨道偏心率极高[64] | ||
| HD 95544 b | 6.84+0.31 − |
2172+23 −21 |
3.386+0.075 −0.077 |
156.5+5.4 −5.5 |
径向速度 | 1.09+0.07 − |
5,722+15 − |
[64] | ||
| HD 109286 b | 2.99+0.15 − |
520.1+2.3 − |
1.259+0.021 − |
259.4+5.5 − |
径向速度 | 0.98+0.05 − |
5,694+23 − |
[64] | ||
| HD 115954 b | 8.29+0.75 −0.58 |
3700+1500 −390 |
5.00+1.3 −0.36 |
144.9+8.1 −13 |
径向速度 | 1.18+0.06 − |
5,957+26 − |
[64] | ||
| HD 211403 b | 5.54+0.39 −0.38 |
223.8+0.41 − |
0.768+0.013 − |
380+13 − |
径向速度 | 1.20+0.06 − |
6,273+44 − |
[64] | ||
| 开普勒-1704b | 4.15+0.29 − |
1.065+0.043 −0.041 |
988.88113+0.00091 −0.00092 |
2.026+0.024 −0.031 |
253.8+3.7 −4.1 |
凌日 | 2,690+40 − |
1.131+0.040 −0.051 |
5,745+88 −89 |
高轨道偏心率（e=0.921）[65] |
| TOI-532b | 0.1935+0.0305 −0.0293 |
0.520+0.017 − |
2.3266508+0.0000030 − |
0.0296+0.00035 − |
867+18 − |
凌日 | 439.1+1.2 − |
0.639+0.023 − |
3,927+37 − |
海王星沙漠行星[66] |
| TOI-2406b | 0.0286+0.0223 −0.0126 |
0.263+0.015 −0.014 |
3.0766896+0.0000065 − |
0.0228+0.0016 − |
447+15 − |
凌日 | 181.4+0.4 − |
0.162+0.008 − |
3,100+75 − |
[67] |
| KIC 8121913 b | 2.1+0.4 − |
3.294601+0.000013 −0.00022 |
轨道反射 | 2350 | 1.456+0.069 −0.15 |
5,975.3+110.2 −109.4 |
[68] | |||
| KIC 10068024 b | 2.0+0.4 − |
2.073549+0.000008 −0.000177 |
轨道反射 | 3,600 | 1.22+0.175 −0.139 |
6,118.4+127.2 −121.2 |
[68] | |||
| KIC 5479689 b | 0.5+0.4 −0.1 |
1.701531+0.000008 −0.000419 |
轨道反射 | 1,504 | 0.966+0.03 −0.04 |
5,459.1+90.0 −85.2 |
[68] | |||
| LTT 1445 Ac | 0.0048+0.0006 − |
0.103 | 3.12390 | 0.02661+0.00047 −0.00049 |
凌日 | 22.41+0.01 − |
0.256+0.014 − |
3,337+150 − |
[69] | |
| Luyten 98-59 e | 0.0094 | 12.8 | 0.071 | ±350 | 径向速度 | 34.6 | 0.32+0.03 − |
3,500+150 − |
[70] | |
| Luyten 98-59 f | 0.0078 | 23.2 | 0.103 | 径向速度 | 34.6 | 0.32+0.03 − |
3,500+150 − |
未确认，可能处于宜居带[70] | ||
| HD 191939 e | 0.34+0.01 − |
101.4+0.4 − |
0.397+0.005 − |
397+16 − |
径向速度 | 175.1+0.2 − |
0.92 | 5,400 | [71] | |
| OGLE-2019-BLG-1058 | 6.836+6.027 − |
微重力透镜 | 8,000+5,000 − |
星际行星[72] | ||||||
| TOI-2184 b | 0.65+0.16 − |
1.017+0.051 − |
6.90683+0.00009 − |
凌日 | 2,515+22 − |
1.53+0.12 − |
5,966+136 − |
[73] | ||
| TOI-431 b | 0.0097+0.0011 − |
0.0014+0.004 − |
0.490047+0.000010 −0.000007 |
0.0113+0.0002 −0.0003 |
1,862+42 − |
凌日 | 106.37+0.03 − |
0.78+0.07 − |
4,850+75 − |
主星又名CD-26 2288或HIP 26013[74] |
| TOI-431 c | 0.0089+0.0013 −0.0011 |
4.8494+0.0003 −0.0002 |
0.0052+0.001 − |
867+20 − |
径向速度 | 106.37+0.03 − |
0.78+0.07 − |
4,850+75 − |
主星又名CD-26 2288或HIP 26013.[74] | |
| TOI-431 d | 0.0312+0.0047 − |
0.294+0.008 − |
12.46103+0.00002 − |
0.098+0.002 − |
633+14 − |
凌日 | 106.37+0.03 − |
0.78+0.07 − |
4,850+75 − |
主星又名CD-26 2288或HIP 26013.[74] |
| TOI-2202 b | 0.927+0.047 −0.048 |
1.01+0.522 −0.080 |
11.9108+0.0009 −0.0009 |
0.0956+0.0015 −0.0016 |
凌日 | 770+3 − |
0.823+0.027 −0.023 |
5,144+50 − |
[75] | |
| TOI-2202 c | 0.191+0.033 −0.030 |
24.7545+0.0073 −0.0078 |
0.1558+0.0025 −0.0026 |
计时 | 770+3 − |
0.823+0.027 −0.023 |
5,144+50 − |
[75] | ||
| EPIC 211314705.01 | 0.139+0.007 − |
3.793306+0.000324 −0.000343 |
543+8 −9 |
凌日 | 300.0+1.7 − |
0.43+0.01 − |
3,669+88 −82 |
[76] 星系内可能还存在两个行星[77] | ||
| EPIC 211401787.01 | 0.247+0.013 −0.008 |
13.774798+0.000028 −0.000028 |
969+9 − |
凌日 | 525+5 − |
1.23+0.02 − |
6,232+33 −39 |
[76] 主星又名BD+12 1842 | ||
| K2-268f | 0.199+0.013 −0.008 |
26.270570+0.000105 −0.000109 |
492+8 −10 |
凌日 | 1,079+10 − |
0.84+0.02 − |
5,106+70 −61 |
主星又名EPIC 211413752.[76] | ||
| K2-268d | 0.133+0.013 −0.006 |
4.528598+0.000016 −0.000015 |
888+16 −15 |
凌日 | 1,079+10 − |
0.84+0.02 − |
5,106+70 −61 |
主星又名EPIC 211413752[76] | ||
| K2-268e | 0.119+0.010 −0.007 |
6.131243+0.000032 −0.000033 |
801+13 − |
凌日 | 1,079+10 − |
0.84+0.02 − |
5,106+70 −61 |
主星又名EPIC 211413752[76] | ||
| EPIC 211502222.01 | 0.243+0.013 −0.009 |
22.996591+0.001848 −0.001859 |
673+12 −11 |
凌日 | 694+6 − |
1.10+0.03 −0.04 |
5,994+93 −91 |
[76] | ||
| EPIC 211502222.02 | 0.160+0.013 −0.009 |
9.398977+0.001506 −0.001348 |
909+14 − |
凌日 | 694+6 − |
1.10+0.03 −0.04 |
5,994+93 −91 |
[76] | ||
| EPIC 211579112.01 | 0.196+0.017 −0.014 |
17.706320+0.000063 − |
266+5 −8 |
凌日 | 403+5 − |
0.27+0.01 −0.02 |
3,315+137 −152 |
[76] | ||
| K2-185c | 0.213+0.008 − |
52.713494+0.000155 −0.000164 |
477+14 −17 |
凌日 | 882+11 − |
0.96+0.05 −0.07 |
5,788+190 −157 |
主星又名EPIC 211611158[76] | ||
| EPIC 211647930.01 | 0.552+0.025 −0.022 |
14.759287+0.000243 −0.000240 |
826+14 −17 |
凌日 | 1,133+17 − |
1.06+0.04 − |
5,880+85 −82 |
[76] | ||
| EPIC 211730024.01 | 0.504+0.032 −0.025 |
5.113981+0.000061 −0.000062 |
1,380+34 −30 |
凌日 | 1,226+21 − |
1.36+0.05 − |
6,502+132 −130 |
[76] | ||
| EPIC 211743874.01 | 0.197+0.016 −0.013 |
12.283211+0.000051 − |
949+21 −26 |
凌日 | 1,850+60 − |
1.23+0.04 − |
6,222+96 −91 |
[76] | ||
| EPIC 211763214.01 | 0.109+0.008 −0.005 |
21.194733+0.000108 −0.000107 |
569+15 −22 |
凌日 | 786+9 − |
0.86+0.03 −0.05 |
5,424+192 −144 |
[76] | ||
| EPIC 211770696.01 | 0.234+0.017 −0.013 |
16.273563+0.000054 −0.000053 |
850+19 −18 |
凌日 | 1,390+30 − |
0.94+0.04 −0.03 |
5,869+88 −81 |
[76] | ||
| EPIC 211779390.01 | 0.092+0.010 −0.005 |
3.850614+0.000012 − |
783+12 −14 |
凌日 | 514+2 − |
0.66+0.02 − |
4,558+91 −81 |
[76] | ||
| EPIC 211897691.02 | 0.171+0.017 −0.011 |
19.507428+0.000116 −0.000113 |
508+12 − |
凌日 | 1,187+17 − |
0.74+0.04 −0.03 |
4,857+86 −84 |
[76] | ||
| EPIC 211923431.01 | 0.300+0.039 −0.029 |
29.740451+0.000169 −0.000161 |
606+31 −36 |
凌日 | 2,460+70 − |
0.93+0.04 − |
5,532+90 − |
[76] | ||
| EPIC 211978988.01 | 0.287+0.022 −0.017 |
36.552551+0.000127 −0.000122 |
598+16 −15 |
凌日 | 1,390+20 − |
0.98+0.07 − |
5,817+45 −48 |
[76] | ||
| TOI-1518 b | 2.3 | 1.875+0.053 − |
1.902603+0.000011 − |
0.0389+0.0011 − |
3,237+59 − |
凌日 | 742+6 − |
1.79+0.26 − |
7,300+100 − |
[76] |
| EPIC 212058012.01 | 0.181+0.012 −0.008 |
11.561052+0.000690 −0.000668 |
861+14 −15 |
凌日 | 684+6 − |
1.01+0.05 − |
5,920+104 − |
[76] | ||
| EPIC 212072539.01 | 0.180+0.009 −0.006 |
7.676972+0.000012 −0.000012 |
465+7 − |
凌日 | 545+3 − |
0.49+0.01 − |
3,804+93 −74 |
[76] | ||
| EPIC 212072539.02 | 0.147+0.015 −0.007 |
2.787174+0.000004 − |
653+10 −12 |
凌日 | 545+3 − |
0.49+0.01 − |
3,804+93 −74 |
[76] | ||
| EPIC 212081533.01 | 0.142+0.009 −0.004 |
3.355850+0.000091 −0.000093 |
722+7 −10 |
凌日 | 245.8 | 0.51+0.01 − |
4,374+38 −34 |
[76] | ||
| EPIC 212088059.01 | 0.188+0.018 −0.008 |
10.367437+0.000020 −0.000019 |
437+4 −5 |
凌日 | 532+3 − |
0.56+0.01 − |
3,779+30 −26 |
[76] | ||
| EPIC 212132195.01 | 0.202+0.017 −0.009 |
26.201446+0.003331 −0.003124 |
450+5 − |
凌日 | 345.5+1.6 − |
0.71+0.02 − |
4,801+49 − |
[76] | ||
| EPIC 212161956.01 | 0.215+0.010 −0.009 |
7.187257+0.000020 −0.000021 |
640+20 −21 |
凌日 | 1055+13 − |
0.66+0.03 − |
4,599+178 −152 |
[76] | ||
| EPIC 212204403.01 | 0.291+0.020 −0.010 |
4.688418+0.000119 −0.000117 |
908+12 −11 |
凌日 | 662+5 − |
0.83+0.02 −0.01 |
5,077+40 −39 |
[76] | ||
| EPIC 212204403.02 | 0.238+0.021 −0.010 |
12.550171+0.001018 −0.001057 |
655+7 −9 |
凌日 | 662+5 − |
0.83+0.02 −0.01 |
5,077+40 −39 |
[76] | ||
| K2-304c | 0.203+0.017 −0.011 |
5.213965+0.000442 − |
866+27 −37 |
凌日 | 1,380+20 − |
0.83+0.05 −0.04 |
5,171+172 −130 |
主星又名EPIC 212297394[76] | ||
| EPIC 212420823.01 | 0.123+0.009 −0.006 |
9.032178+0.000874 − |
518+5 −4 |
凌日 | 1,450+20 − |
0.54+0.01 − |
4,385+29 −31 |
[76] | ||
| EPIC 212440430.02 | 0.138+0.013 −0.010 |
4.163873+0.000022 −0.000023 |
1,158+29 −34 |
凌日 | 1,620+20 − |
0.98+0.02 − |
5,789+46 −50 |
[76] | ||
| EPIC 212543933.01 | 0.227+0.023 −0.017 |
7.806164+0.000673 −0.000623 |
934+28 −32 |
凌日 | 1,310+50 − |
1.02+0.02 − |
5,769+39 −37 |
[76] | ||
| K2-307c | 0.207+0.017 −0.011 |
23.228555+0.000068 −0.000071 |
658+13 −14 |
凌日 | 1,050+20 − |
0.99+0.03 −0.04 |
6,004+77 −78 |
主星又名EPIC 212587672[76] | ||
| EPIC 251319382.01 | 0.171+0.012 −0.006 |
8.234885+0.000508 −0.000475 |
885+12 −14 |
凌日 | 577+6 − |
0.95+0.02 − |
5,791+81 − |
[76] | ||
| EPIC 251319382.02 | 0.199+0.012 −0.008 |
14.871387+0.000916 −0.000936 |
727+10 − |
凌日 | 577+6 − |
0.95+0.02 − |
5,791+81 − |
[76] | ||
| EPIC 251319382.03 | 0.122+0.009 −0.006 |
3.665912+0.000273 −0.000295 |
1,160+16 −15 |
凌日 | 577+6 − |
0.95+0.02 − |
5,791+81 − |
[76] | ||
| EPIC 251554286.01 | 0.496+0.020 −0.018 |
15.466805+0.000572 −0.000565 |
735+13 −14 |
凌日 | 883+12 − |
0.87+0.02 − |
5,698+55 − |
[76] | ||
| 格利泽146b | 0.0175+0.0023 −0.0021 |
5.09071 ± 0.00026 | 0.0510+0.0024 −0.0026 |
573+63 −69 |
径向速度 | 44.37+0.01 − |
0.684+0.013 − |
4,385+21 − |
主星又名HD 22496[78] | |
| EPIC 211525753.01 | 0.201+0.020 −0.014 |
5.7385647+0.0013939 −0.0011048 |
0.0632+0.0096 −0.0176 |
1,066+190 −77 |
凌日 | 0.96+0.05 −0.06 |
5,790+177 −147 |
[79] | ||
| EPIC 211537087.01 | 0.204+0.013 −0.011 |
21.0267366+0.0036912 −0.0038993 |
0.1599+0.0178 −0.0306 |
624+0 −37 |
凌日 | 0.90+0.05 −0.06 |
5,568+178 −150 |
[79] | ||
| EPIC 211730267.01 | 0.332+0.021 −0.019 |
16.3488637+0.0013811 −0.0014022 |
0.1450+0.0136 −0.0235 |
735+8 −39 |
凌日 | 0.98+0.07 − |
5,794+210 −169 |
[79] | ||
| EPIC 211914998.01 | 0.239+0.015 −0.013 |
11.2510285+0.0018188 −0.0017892 |
0.0863+0.0079 −0.0159 |
888+0 −47 |
凌日 | 0.93+0.06 − |
5,650+193 −152 |
[79] | ||
| TOI-3362b | 5.029+0.668 −0.646 |
1.142+0.043 −0.041 |
18.09547+0.00003 − |
0.153+0.002 −0.003 |
凌日 | 1,198+18 − |
1.445+0.069 −0.073 |
6,532+88 −86 |
高轨道偏心率[80] | |
| KMT-2017-BLG-2509b | 2.09+1.68 −1.26 |
2.14+0.27 −0.39 |
微重力透镜 | 23,000+3,000 − |
0.46+0.37 −0.27 |
[81] | ||||
| OGLE-2017-BLG-1099b | 3.02+2.43 −1.81 |
2.73+0.40 −0.53 |
微重力透镜 | 24,000+3,000 − |
0.45+0.36 −0.27 |
[81] | ||||
| OGLE-2019-BLG-0299b | 6.22+3.80 −3.67 |
2.80+0.58 −0.89 |
微重力透镜 | 19,000+4,000 − |
0.59+0.36 −0.35 |
[81] | ||||
| TOI-1296b | 0.298+0.039 − |
1.231+0.031 − |
3.9443715+0.0000058 − |
0.0497+0.0023 −0.0028 |
1,562+43 −31 |
凌日 | 1,023+4 − |
1.17+0.14 − |
5,603+47 − |
[82] |
| TOI-1298b | 0.356+0.032 − |
0.841+0.021 − |
4.537164+0.000012 − |
0.0590+0.0023 − |
1,388+24 − |
凌日 | 1,041+7 − |
1.44+0.10 − |
5,889+43 − |
[82] |
| TOI-1201 b | 0.0198+0.0027 − |
0.216+0.008 − |
2.4919863+0.0000030 −0.0000031 |
0.0287+0.0012 − |
703+15 −14 |
凌日 | 122.77+0.10 − |
0.512+0.020 − |
3,476+51 − |
属于毕宿星团, [83] |
| 雕具座RRc | 2.7+0.7 − |
14,200+300 − |
9.7+0.9 − |
计时 | 69.10+0.03 − |
0.18+0.44 | 3,100+7,540 | [84] | ||
| TIC 257060897b | 0.67+0.03 − |
1.49+0.04 − |
3.660028+0.000006 − |
0.051+0.002 − |
1,762+21 − |
凌日 | 1,655+8 − |
1.32+0.04 − |
6,128+57 − |
[85] |
| TOI-530b | 0.40+0.09 −0.10 |
0.83+0.06 − |
6.387597+0.000019 −0.000018 |
0.052+0.005 −0.004 |
565+28 −31 |
凌日 | 482+2 − |
0.53+0.02 − |
3,659+120 − |
[86] |
| HIP 97166b | 0.0629+0.047 − |
0.245+0.012 − |
10.28891+0.00004 − |
0.089+0.001 − |
757+25 − |
凌日 | 215.54+0.33 − |
0.898+0.054 − |
5,198+100 − |
[87] |
| HIP 97166c | 9.9+1.8 − |
16.84+0.22 − |
0.124+0.002 − |
642+22 − |
径向速度 | 215.54+0.33 − |
0.898+0.054 − |
5,198+100 − |
[87] | |
| HD 63935 b | 0.0340+0.0057 − |
0.267+0.013 − |
9.058811+0.000017 −0.000016 |
911+27 − |
凌日 | 159.36+0.15 − |
0.933+0.054 − |
5,534+100 − |
[88] | |
| HD 63935 c | 0.0349+0.0076 − |
0.259+0.012 − |
21.4023+0.00189 −0.00194 |
684+21 − |
凌日 | 159.36+0.15 − |
0.933+0.054 − |
5,534+100 − |
[88] | |
| HD 207897 b | 0.0453+0.0050 − |
0.223+0.007 − |
16.202159+0.000085 −0.000083 |
0.1163+0.0017 −0.001 |
632.2+8.1 −7.0 |
凌日 | 92.15+0.10 − |
0.80+0.036 −0.030 |
5,070+60 −57 |
[89] |
| 2MASS J04372171+2651014 b | 4+1 − |
115 | 1,450+50 − |
影像 | 417.9+1.5 − |
0.165+0.015 − |
3,100 | [90][91] | ||
| TOI 1227 b | 0.854+0.067 −0.052 |
27.36397+0.00011 − |
0.0886+0.0054 −0.0057 |
凌日 | 329.3+0.8 − |
0.170+0.015 − |
3,072+74 − |
[92] | ||
| TOI-2285b | 0.155+0.007 − |
27.26955+0.00013 −0.00010 |
0.1363+0.0010 − |
284+6 − |
凌日 | 138.34+0.14 − |
0.454+0.010 − |
3,491+58 − |
[93] | |
| LHS 1678 b | 0.0002+0.0003 − |
0.062+0.004 − |
0.8602322+0.0000068 −0.0000048 |
0.01251+0.00059 −0.00056 |
凌日 | 64.88+0.03 − |
0.345+0.014 − |
3490+50 − |
[94] | |
| LHS 1678 c | 0.0012+0.0013 −0.0008 |
0.088+0.006 − |
3.694247+0.0000024 −0.0000021 |
0.0331+0.0016 −0.0015 |
凌日 | 64.88+0.03 − |
0.345+0.014 − |
3490+50 − |
[94] | |
| HD 73583 b | 0.0315+0.0098 − |
0.253+0.009 − |
6.3980418+0.0000065 −0.0000063 |
0.0601+0.0026 − |
721+21 − |
凌日 | 103.08+0.10 − |
0.71+0.02 − |
4511+110 − |
主星又名TOI-560[95][96] |
| HD 73583 c | 0.0302+0.0055 − |
0.212+0.009 − |
18.8797+0.00088 −0.00073 |
0.1236+0.0053 −0.0053 |
503+15 − |
凌日 | 103.08+0.10 − |
0.71+0.02 − |
4511+110 − |
主星又名TOI-560[95] |
| TOI-1807 b | 0.165+0.004 − |
0.549372+0.000007 − |
0.00812+0.00037 −0.00038 |
2100+39 −40 |
凌日 | 133.88+0.25 − |
0.750+0.025 −0.024 |
4757+51 −50 |
恒星与TOI-2076一起运动[97] | |
| TOI-2076 b | 0.293+0.038 − |
10.35566+0.00006 − |
0.0631+0.0027 − |
870+13 − |
凌日 | 136.70+0.23 − |
0.850+0.025 −0.026 |
5187+54 −53 |
恒星与TOI-1807一起运动[97] | |
| TOI-2076 c | 0.396+0.004 − |
21.01538+0.00084 −0.00074 |
0.0885+0.0038 − |
734+11 − |
凌日 | 136.70+0.23 − |
0.850+0.025 −0.026 |
5187+54 −53 |
[98][97] | |
| TOI-2076 d | 0.370+0.006 − |
25.0893+0.01 − |
0.1138+0.0048 −0.0049 |
648+10 − |
凌日 | 136.70+0.23 − |
0.850+0.025 −0.026 |
5187+54 −53 |
恒星与TOI-1807一起运动[97] | |
| TOI-2257 b | 0.196+0.010 − |
35.189346 | 0.145+0.003 − |
256+61 −17 |
凌日 | 188.5+0.3 − |
0.33+0.02 − |
3430+130 − |
处于宜居带[99] | |
| TOI-712 b | 0.0176 | 0.183+0.011 −0.007 |
9.531361+0.000018 −0.000017 |
0.07928+0.00096 −0.00091 |
650.0+6.0 −5.9 |
凌日 | 191.2+0.4 − |
0.732+0.027 −0.025 |
4622+61 −59 |
[100] |
| TOI-712 c | 0.0274 | 0.241+0.008 −0.007 |
51.69906+0.00017 − |
0.2447+0.0030 −0.0028 |
369.9+3.4 −3.3 |
凌日 | 191.2+0.4 − |
0.732+0.027 −0.025 |
4622+61 −59 |
[100] |
| TOI-712 d | 0.0236 | 0.221+0.008 −0.007 |
84.83960+0.00043 −0.00040 |
0.3405+0.0041 −0.0039 |
313.6+2.9 −2.8 |
凌日 | 191.2+0.4 − |
0.732+0.027 −0.025 |
4622+61 −59 |
[100] |
| OGLE-2019-BLG-0468Lb | 3.43+1.83 −1.17 |
3.29+4.15 −2.52 |
微重力透镜 | 14000+3000 − |
0.92+0.49 −0.32 |
轨道参数多变[101] | ||||
| OGLE-2019-BLG-0468Lc | 10.22+5.46 −3.50 |
2.77+3.49 −2.12 |
微重力透镜 | 14000+3000 − |
0.92+0.49 −0.32 |
轨道参数多变[101] | ||||
| KMT-2021-BLG-0912Lb | 0.022+0.007 −0.008 |
3.03+3.46 −2.46 |
微重力透镜 | 22000+3000 − |
0.75+0.23 −0.28 |
轨道参数多变[102] | ||||
| HD 137496 b | 0.0127+0.0017 − |
0.117+0.005 − |
1.62116+0.00008 − |
0.02732+0.00019 − |
2130+30 −29 |
凌日 | 509+6 − |
1.035+0.022 − |
5799+61 − |
[103] |
| HD 137496 c | 7.66+0.11 − |
479.9+1.1 −1.0 |
1.2163+0.0087 −0.0088 |
370+5 − |
径向速度 | 509+6 − |
1.035+0.022 − |
5799+61 − |
[103] | |
| HD 19615 b | 8.5+0.7 − |
402+2 − |
1.1+0.1 − |
径向速度 | 872+7 − |
1.1+0.1 − |
3987+125 − |
主星为红巨星[104] | ||
| HD 150010 b | 2.4+0.4 − |
562+8 − |
1.1+0.1 − |
径向速度 | 473.4+2.1 − |
1.3+0.1 − |
4256+125 − |
主星为红巨星[104] | ||
| HD 174205 b | 4.2+0.5 − |
582+17 − |
1.7+0.1 − |
径向速度 | 769+5 − |
1.8+0.1 − |
4393+125 − |
主星为红巨星[104] | ||
| KMT-2018-BLG-1988Lb | 0.021+0.015 −0.011 |
2.83+1.23 −0.97 |
微重力透镜 | 14000+6000 −5000 |
0.48+0.33 −0.25 |
轨道参数多变[105] | ||||
| KOI-984b | 0.0544+0.0094 − |
0.384+0.004 − |
4.2881785+0.0000035 − |
0.0504+0.0006 − |
1022+31 −30 |
凌日 | 749+4 − |
0.928+0.031 − |
5295+150 − |
[106] |
| TOI-2109b | 5.02+0.75 − |
1.347+0.047 − |
0.67247414+0.00000028 − |
0.01791+0.00065 − |
3631+69 − |
凌日 | 846+9 − |
1.447+0.075 −0.078 |
6530+160 −150 |
[107] |
| TOI-1238b | 0.0183+0.0035 − |
0.108+0.010 − |
0.764596+0.000016 −0.000013 |
0.0139+0.0008 − |
1133+167 − |
凌日 | 2030.44+0.20 − |
0.59+0.02 − |
4089+54 − |
[108] |
| TOI-1238c | 0.0262+0.0059 − |
0.188+0.013 − |
3.294733+0.000040 −0.000047 |
0.037+0.002 − |
695+105 − |
凌日 | 2030.44+0.20 − |
0.59+0.02 − |
4089+54 − |
[108] |
| K2-99c | 8.4+0.2 − |
522.2+1.4 − |
1.43+0.01 − |
390+6 − |
径向速度 | 1980 | 1.6 | 5990 | [109] | |
| HIP 5763b | 0.51 | 30.014+0.1528 −0.2842 |
0.170 | 径向速度 | 104.17+0.14 − |
0.72 | [110] | |||
| HIP 34222b | 0.83 | 160.0+2.7 −2.9 |
0.492 | 径向速度 | 74.55+0.09 − |
0.62 | [110] | |||
| HIP 86221b | 0.71 | 2.224+0.0004 −0.0005 |
0.031 | 径向速度 | 96+11 − |
0.79 | [110] | |||
| TOI-1842b | 0.214+0.040 −0.038 |
1.04+0.06 −0.05 |
9.5739+0.0002 −0.0001 |
0.01001+0.0007 − |
凌日 | 729+7 − |
1.46+0.03 − |
6230+50 − |
[111] | |
| 格利泽367b | 0.0017+0.0002 − |
0.064+0.005 − |
0.321962+0.000010 −0.000012 |
0.0071+0.0002 − |
1745+43 − |
凌日 | 30.695+0.016 − |
0.45+0.011 − |
3522+70 − |
[112] |
| HATS-74Ab | 1.46+0.14 − |
1.032+0.021 − |
1.73185606+0.00000055 − |
0.02384+0.00011 − |
895.1+5.7 − |
凌日 | 952+12 − |
0.601+0.008 − |
3775+54 − |
主星又名TOI-737[113] |
| HATS-75b | 0.491+0.039 − |
0.884+0.013 − |
2.7886556+0.0000011 − |
0.032742+0.000134 −0.000099 |
772.3+2.3 − |
凌日 | 640+4 − |
0.6017+0.0074 −0.0055 |
3812+79 − |
主星又名TOI-552[113] |
| HATS-76b | 2.629+0.089 − |
1.079+0.031 − |
1.9416423+0.0000014 − |
0.02658+0.00021 −0.00029 |
939.8+6.7 − |
凌日 | 1272+19 − |
0.662+0.016 −0.021 |
3990+120 − |
主星又名TOI-555[113] |
| HATS-77b | 1.374+0.100 −0.074 |
1.165+0.021 − |
3.0876262+0.0000016 − |
0.03607+0.00025 − |
828.3+5.9 − |
凌日 | 1440+40 − |
0.655+0.014 − |
4082+69 − |
主星又名TOI-730[113] |
| KOI-4777b | 0.046+0.003 − |
0.412000+0.000001 − |
0.0080+0.0003 − |
1180+20 − |
凌日 | 565+4 − |
0.41+0.02 − |
3515+69 − |
[114] | |
| BD+60 1417b | 15+5 − |
1.31+0.06 − |
1662 | 1303+74 − |
影像 | 146.65+0.09 − |
1.0 | 4993+124 − |
主星很年轻，年龄约为1亿年[115] | |
| HD 129116 b | 10.9+1.6 − |
200000+100000 − |
556+17 − |
影像 | 325+10 − |
8+2 − |
[116] | |||
| HD 360 b | 0.75+0.12 −0.15 |
273.1+1.6 −0.8 |
0.98+0.11 −0.03 |
径向速度 | 362 | 1.69+0.15 −0.53 |
4770 | [117] | ||
| 外屏二b | 0.77+0.16 −0.10 |
255.3+2.1 −1.4 |
0.88+0.11 −0.10 |
径向速度 | 183.2 | 1.41+1.45 −0.50 |
4824 | 系外行星候选，未确认[117] | ||
| HD 10975 b | 0.45+0.06 −0.15 |
283.8+12.7 −0.1 |
0.95+0.06 −0.08 |
径向速度 | 379 | 1.41+0.34 −0.35 |
4840 | [117] | ||
| HD 79181 b | 0.64+0.06 −0.16 |
273.1+1.3 −0.4 |
0.90+0.07 −0.08 |
径向速度 | 337 | 1.28+0.32 −0.28 |
4862 | [117] | ||
| HD 99183 b | 0.97+0.06 −0.25 |
310.4+5.2 −1.7 |
1.08+0.05 −0.07 |
径向速度 | 355 | 1.76+0.31 −0.30 |
4886 | [117] | ||
| 獅子座υb | 0.51+0.06 −0.26 |
385.2+2.8 −1.3 |
1.18+0.11 −0.32 |
径向速度 | 177.8 | 1.48+0.90 −0.38 |
4836 | [117] | ||
| HD 161178 b | 0.57+0.02 −0.16 |
279.3+1.0 −0.8 |
0.85+0.05 −0.07 |
径向速度 | 351 | 1.06+0.25 −0.17 |
4786 | [117] | ||
| HD 219139 b | 0.78+0.05 −0.20 |
275.5+2.3 −1.0 |
0.94+0.06 −0.07 |
径向速度 | 345 | 1.46+0.31 −0.29 |
4831 | [117] | ||
| 霹雳二b | 1.34+0.02 −0.31 |
555.1+6.0 −2.5 |
1.32+0.05 −0.08 |
径向速度 | 138 | 0.99+0.17 −0.13 |
4742 | [117] | ||
| OGLE-2014-BLG-0676Lb | 3.68+0.69 −1.44 |
4.53+1.49 −2.50 |
微重力透镜 | 8700+2500 −4600 |
0.73+0.14 −0.29 |
[118] | ||||
| HD 103891 b | 1.44+0.06 −0.05 |
1919+14 −15 |
3.27+0.02 −0.01 |
径向速度 | 179.0+0.4 − |
1.28+0.01 − |
6072+20 − |
[119] | ||
| HD 105779 b | 0.64+0.06 − |
2412+55 −52 |
3.38+0.05 − |
径向速度 | 179.7+0.3 − |
0.89+0.01 − |
5792+16 − |
[119] | ||
| HD 73583b | 0.253+0.014 −0.011 |
6.3980661+0.0000095 −0.0000097 |
0.05995+0.00074 −0.00072 |
742.7+7.2 −7.0 |
凌日 | 102.97+0.10 − |
0.701+0.026 −0.025 |
4574+62 −61 |
主星又名TOI 560[120] | |
| HD 73583c | 0.2433+0.011 −0.0096 |
18.8805+0.0024 −0.0011 |
0.1233+0.0015 − |
517.8+5 −4.9 |
凌日 | 102.97+0.10 − |
0.701+0.026 −0.025 |
4574+62 −61 |
主星又名TOI 560[120] | |
| OGLE-2014-BLG-0319Lb | 0.57+0.36 −0.31 |
3.49+1.17 −1.12 |
微重力透镜 | 25000+4000 −9000 |
0.52+0.33 −0.29 |
[121] | ||||
| OGLE-2018-BLG-0383L b | 0.0201+0.0173 −0.0088 |
1.8+0.2 − |
微重力透镜 | 25000+2000 − |
0.10+0.13 −0.05 |
[122] |
参考[编辑]
- ^ HD 108236 f, exoplanet.eu, [4 January 2021], （原始内容存档于2022-08-29）
- ^ Bonfanti, A.; et al, CHEOPS observations of the HD 108236 planetary system: A fifth planet, improved ephemerides, and planetary radii, Astronomy & Astrophysics, 2021, 646: A157, Bibcode:2021A&A...646A.157B, S2CID 230437723, arXiv:2101.00663
, doi:10.1051/0004-6361/202039608
- ^ Smith, A. M. S.; et al, NGTS-14Ab: A Neptune-sized transiting planet in the desert, Astronomy & Astrophysics, 2021, 646: A183, Bibcode:2021A&A...646A.183S, S2CID 230524042, arXiv:2101.01470 , doi:10.1051/0004-6361/202039712
- ^ Martin, David V.; et al, TOI-1259Ab – a gas giant planet with 2.7 per cent deep transits and a bound white dwarf companion, Monthly Notices of the Royal Astronomical Society, 2021, 507 (3): 4132–4148, arXiv:2101.02707 , doi:10.1093/mnras/stab2129
- ^ Grieves, Nolan; et al, NGTS-13b: A hot 4.8 Jupiter-mass planet transiting a subgiant star, Astronomy & Astrophysics, 2021, 647: A180, Bibcode:2021A&A...647A.180G, S2CID 231582818, arXiv:2101.04245 , doi:10.1051/0004-6361/202039586
- ^ 6.0 6.1 6.2 6.3 6.4 Rodriguez, Joseph E.; et al, TESS Delivers Five New Hot Giant Planets Orbiting Bright Stars from the Full-frame Images, The Astronomical Journal, 2021, 161 (4): 194, Bibcode:2021AJ....161..194R, S2CID 230770138, arXiv:2101.01726 , doi:10.3847/1538-3881/abe38a
- ^ Yee, Jennifer C.; et al, OGLE-2019-BLG-0960 Lb: The Smallest Microlensing Planet, The Astronomical Journal, 2021, 162 (5): 180, Bibcode:2021AJ....162..180Y, S2CID 231592669, arXiv:2101.04696 , doi:10.3847/1538-3881/ac1582
- ^ 8.0 8.1 Osborn, H. P.; et al, A hot mini-Neptune in the radius valley orbiting solar analogue HD 110113, Monthly Notices of the Royal Astronomical Society, 2021, 502 (4): 4842–4857, Bibcode:2021MNRAS.tmp..240O, arXiv:2101.04745 , doi:10.1093/mnras/stab182
- ^ Hirsch, Lea A.; et al, ASSESSING THE EFFECT OF STELLAR COMPANIONS FROM HIGH-RESOLUTION IMAGING OF Kepler OBJECTS OF INTEREST, The Astronomical Journal, 2017, 153 (3): 117, Bibcode:2017AJ....153..117H, S2CID 39321033, arXiv:1701.06577 , doi:10.3847/1538-3881/153/3/117
- ^ AT LAST! CONFIRMATION OF KEPLER'S SECOND PLANETARY CANDIDATE (PDF). [2022-08-29]. （原始内容存档 (PDF)于2021-01-15）.
- ^ 11.0 11.1 11.2 11.3 11.4 11.5 Leleu, A.; et al, Six transiting planets and a chain of Laplace resonances in TOI-178, Astronomy & Astrophysics, 2021, 649: A26, Bibcode:2021A&A...649A..26L, S2CID 231693292, arXiv:2101.09260 , doi:10.1051/0004-6361/202039767
- ^ Palatnick, Skyler; et al, Validation of HD 183579b Using Archival Radial Velocities: A Warm Neptune Orbiting a Bright Solar Analog, The Astrophysical Journal Letters, 2021, 909 (1): L6, Bibcode:2021ApJ...909L...6P, S2CID 231719821, arXiv:2101.12137 , doi:10.3847/2041-8213/abe0bb
- ^ Gan, Tianjun; et al, HD 183579b: A Warm Sub-Neptune Transiting a Solar Twin Detected by TESS, Monthly Notices of the Royal Astronomical Society, 2021, 507 (2): 2220–2240, arXiv:2107.14015 , doi:10.1093/mnras/stab2224
- ^ Yun Hak Kim; et al, KMT-2019-BLG-0371 and the Limits of Bayesian Analysis, The Astronomical Journal, 2021, 162 (1): 17, Bibcode:2021AJ....162...17K, S2CID 231728667, arXiv:2101.12206 , doi:10.3847/1538-3881/abf930
- ^ 15.0 15.1 Sozzetti, A.; et al, A sub-Neptune and a non-transiting Neptune-mass companion unveiled by ESPRESSO around the bright late-F dwarf HD 5278 (TOI-130), Astronomy & Astrophysics, 2021, 648: A75, Bibcode:2021A&A...648A..75S, S2CID 231728514, arXiv:2101.12300 , doi:10.1051/0004-6361/202040034
- ^ Han, Cheongho; et al, KMT-2018-BLG-1025Lb: Microlensing super-Earth planet orbiting a low-mass star, Astronomy & Astrophysics, 2021, 649: A90, Bibcode:2021A&A...649A..90H, S2CID 231786450, arXiv:2102.01890 , doi:10.1051/0004-6361/202039817
- ^ Mahadevan, Suvrath; et al, The Habitable-zone Planet Finder Detects a Terrestrial-mass Planet Candidate Closely Orbiting Gliese 1151: The Likely Source of Coherent Low-frequency Radio Emission from an Inactive Star, The Astrophysical Journal Letters, 2021, 919 (1): L9, Bibcode:2021ApJ...919L...9M, S2CID 231802021, arXiv:2102.02233 , doi:10.3847/2041-8213/abe2b2
- ^ Perger, M.; et al, The CARMENES search for exoplanets around M dwarfs, Astronomy & Astrophysics, 2021, 649: L12, S2CID 232269942, arXiv:2103.10216 , doi:10.1051/0004-6361/202140786
- ^ 19.0 19.1 Ikwut-Ukwa, Mma; et al, Two Massive Jupiters in Eccentric Orbits from the TESS Full-frame Images, The Astronomical Journal, 2022, 163 (1): 9, Bibcode:2022AJ....163....9I, S2CID 231802379, arXiv:2102.02222 , doi:10.3847/1538-3881/ac2ee1
- ^ 20.0 20.1 Mayor, M.; et al, The HARPS search for southern extra-solar planets XXXIV. Occurrence, mass distribution and orbital properties of super-Earths and Neptune-mass planets, 2011, arXiv:1109.2497 [astro-ph.EP]
- ^ 21.0 21.1 Ahrer, E.; et al, The HARPS search for southern extra-solar planets XLV. Two Neptune mass planets orbiting HD 13808: a study of stellar activity modelling's impact on planet detection, Monthly Notices of the Royal Astronomical Society, 2021, 503 (1): 1248–1263, Bibcode:2021MNRAS.503.1248A, arXiv:2102.03387 , doi:10.1093/mnras/stab373
- ^ 22.0 22.1 22.2 Newton, Elisabeth R.; et al, TESS Hunt for Young and Maturing Exoplanets (THYME) IV: Three small planets orbiting a 120 Myr-old star in the Pisces–Eridanus stream, The Astronomical Journal, 2021, 161 (2): 65, Bibcode:2021AJ....161...65N, S2CID 231879927, arXiv:2102.06049 , doi:10.3847/1538-3881/abccc6
- ^ 23.0 23.1 23.2 Barragán, Oscar; et al, TESS re-observes the young multi-planet system TOI-451:refined ephemeris and activity evolution, Research Notes of the American Astronomical Society, 2021, 5 (3): 51, Bibcode:2021RNAAS...5...51B, S2CID 232258104, arXiv:2103.09746 , doi:10.3847/2515-5172/abef70
- ^ Tofflemire, Benjamin M.; et al, TESS Hunt for Young and Maturing Exoplanets (THYME). V. A Sub-Neptune Transiting a Young Star in a Newly Discovered 250 Myr Association, The Astronomical Journal, 2021, 161 (4): 171, Bibcode:2021AJ....161..171T, S2CID 231879915, arXiv:2102.06066 , doi:10.3847/1538-3881/abdf53
- ^ 25.0 25.1 Kil Jung, Youn; et al, OGLE-2018-BLG-0567Lb and OGLE-2018-BLG-0962Lb: Two Microlensing Planets through the Planetary-caustic Channel, The Astronomical Journal, 2021, 161 (6): 293, Bibcode:2021AJ....161..293J, S2CID 231924992, arXiv:2102.07338 , doi:10.3847/1538-3881/abf8bd
- ^ Toledo-Padrón, B.; et al, A super-Earth on a close-in orbit around the M1V star GJ 740, Astronomy & Astrophysics, 2021, 648: A20, S2CID 231951695, arXiv:2102.09441 , doi:10.1051/0004-6361/202040099
- ^ Kains, N.; et al, A giant planet beyond the snow line in microlensing event OGLE-2011-BLG-0251, Astronomy & Astrophysics, 2021, 552: A70, S2CID 43146154, arXiv:1303.1184 , doi:10.1051/0004-6361/201220626
- ^ Soto, M. G.; et al, Mass and density of the transiting hot and rocky super-Earth LHS 1478 b (TOI-1640 b), Astronomy & Astrophysics, 2021, 649: A144, Bibcode:2021A&A...649A.144S, S2CID 232013854, arXiv:2102.11640 , doi:10.1051/0004-6361/202140618
- ^ 29.0 29.1 Bluhm, P.; et al, An ultra-short-period transiting super-Earth orbiting the M3 dwarf TOI-1685, Astronomy & Astrophysics, 2021, 650: A78, Bibcode:2021A&A...650A..78B, S2CID 232092636, arXiv:2103.01016 , doi:10.1051/0004-6361/202140688
- ^ 30.0 30.1 Hirano, Teruyuki; et al, Two Bright M Dwarfs Hosting Ultra-Short-Period Super-Earths with Earth-like Compositions, The Astronomical Journal, 2021, 162 (4): 161, Bibcode:2021AJ....162..161H, S2CID 232335413, arXiv:2103.12760 , doi:10.3847/1538-3881/ac0fdc
- ^ Zang, Weicheng; et al, An Earth-mass planet in a time of COVID-19: KMT-2020-BLG-0414Lb, Research in Astronomy and Astrophysics, 2021, 21 (9): 239, Bibcode:2021RAA....21..239Z, S2CID 232092272, arXiv:2103.01896 , doi:10.1088/1674-4527/21/9/239
- ^ Hobson, Melissa J.; et al, A Transiting Warm Giant Planet around the Young Active Star TOI-201, The Astronomical Journal, 2021, 161 (5): 235, Bibcode:2021AJ....161..235H, S2CID 232110390, arXiv:2103.02685 , doi:10.3847/1538-3881/abeaa1
- ^ Trifonov, T.; et al, A nearby transiting rocky exoplanet that is suitable for atmospheric investigation, Science, 2021, 371 (6533): 1038–1041, Bibcode:2021Sci...371.1038T, PMID 33674491, S2CID 232124642, arXiv:2103.04950 , doi:10.1126/science.abd7645
- ^ 34.0 34.1 34.2 34.3 Tilbrook, Rosanna H.; et al, NGTS 15b, 16b, 17b, and 18b: Four hot Jupiters from the Next-Generation Transit Survey, Monthly Notices of the Royal Astronomical Society, 2021, 504 (4): 6018–6032, arXiv:2103.10302 , doi:10.1093/mnras/stab815
- ^ Zang, Weicheng; et al, Systematic KMTNet Planetary Anomaly Search. I. OGLE-2019-BLG-1053Lb, a Buried Terrestrial Planet, The Astronomical Journal, 2021, 162 (4): 163, Bibcode:2021AJ....162..163Z, S2CID 232307459, arXiv:2103.11880 , doi:10.3847/1538-3881/ac12d4
- ^ Cloutier, R.; et al, TOI-1634 b: An Ultra-short-period Keystone Planet Sitting inside the M-dwarf Radius Valley, The Astronomical Journal, 2021, 162 (2): 79, Bibcode:2021AJ....162...79C, S2CID 232335385, arXiv:2103.12790 , doi:10.3847/1538-3881/ac0157
- ^ Han, Cheongho; et al, KMT-2019-BLG-1715: Planetary Microlensing Event with Three Lens Masses and Two Source Stars, The Astronomical Journal, 2021, 161 (6): 270, Bibcode:2021AJ....161..270H, S2CID 232478488, arXiv:2104.00293 , doi:10.3847/1538-3881/abf4d0
- ^ Kondo, Iona; et al, OGLE-2018-BLG-1185b: A Low-mass Microlensing Planet Orbiting a Low-mass Dwarf, The Astronomical Journal, 2021, 162 (2): 77, Bibcode:2021AJ....162...77K, S2CID 233033627, arXiv:2104.02157 , doi:10.3847/1538-3881/ac00ba
- ^ 39.0 39.1 Georgieva, I. Y.; et al, Hot planets around cool stars – two short-period mini-Neptunes transiting the late K-dwarf TOI-1260, Monthly Notices of the Royal Astronomical Society, 2021, 505 (4): 4684–4701, arXiv:2104.05653 , doi:10.1093/mnras/stab1464
- ^ 40.0 40.1 40.2 Han, Cheongho; et al, Three microlensing planets with no caustic-crossing features, Astronomy & Astrophysics, 2021, 650: A89, Bibcode:2021A&A...650A..89H, S2CID 233231384, arXiv:2104.06544 , doi:10.1051/0004-6361/202140758
- ^ Bohn, Alexander J.; et al, Discovery of a directly imaged planet to the young solar analog YSES 2, Astronomy & Astrophysics, 2021, 648: A73, Bibcode:2021A&A...648A..73B, S2CID 233296087, arXiv:2104.08285 , doi:10.1051/0004-6361/202140508
- ^ Ryu, Yoon-Hyun; et al, Shortest Microlensing Event with a Bound Planet: KMT-2016-BLG-2605, The Astronomical Journal, 2021, 162 (3): 96, Bibcode:2021AJ....162...96R, S2CID 233289612, arXiv:2104.07906 , doi:10.3847/1538-3881/ac062a
- ^ Brett Christopher Addison; et al, TOI-1431b/MASCARA-5b: An Ultra-hot Jupiter Orbiting One of the Hottest & Brightest Known Exoplanet Host Stars, Posters from the Tess Science Conference Ii (Tsc2, 2021: 64, Bibcode:2021tsc2.confE..64A, arXiv:2104.12078 , doi:10.5281/zenodo.5126266
- ^ Stangret, M.; et al, The obliquity and atmosphere of the ultra-hot Jupiter TOI-1431b (MASCARA-5b): A misaligned orbit and no signs of atomic or molecular absorptions, Astronomy & Astrophysics, 2021, 654: A73, Bibcode:2021A&A...654A..73S, S2CID 233393996, arXiv:2104.12414 , doi:10.1051/0004-6361/202040100
- ^ Cointepas, M.; et al, TOI-269 b: An eccentric sub-Neptune transiting a M2 dwarf revisited with ExTrA, Astronomy & Astrophysics, 2021, 650: A145, Bibcode:2021A&A...650A.145C, S2CID 233476660, arXiv:2104.14782 , doi:10.1051/0004-6361/202140328
- ^ Hoyer, S.; et al, TOI-220 b: A warm sub-Neptune discovered by TESS, Monthly Notices of the Royal Astronomical Society, 2021, 505 (3): 3361–3379, arXiv:2105.01944 , doi:10.1093/mnras/stab1427
- ^ 47.0 47.1 Otegi, J. F.; et al, TESS and HARPS reveal two sub-Neptunes around TOI 1062, Astronomy & Astrophysics, 2021, 653: A105, Bibcode:2021A&A...653A.105O, S2CID 233739805, arXiv:2105.01945 , doi:10.1051/0004-6361/202040247
- ^ Zhang, Jingwen; et al, Long-period Jovian Tilts the Orbits of Two sub-Neptunes Relative to Stellar Spin Axis in Kepler-129, The Astronomical Journal, 2021, 162 (3): 89, Bibcode:2021AJ....162...89Z, S2CID 234338914, arXiv:2105.03446 , doi:10.3847/1538-3881/ac0634
- ^ Maldonado, J.; et al, HADES RV programme with HARPS-N at TNG, Astronomy & Astrophysics, 2021, 651: A93, S2CID 234482717, arXiv:2105.06155 , doi:10.1051/0004-6361/202141141
- ^ Burt, Jennifer A.; et al, TOI-1231 b: A Temperate, Neptune-sized Planet Transiting the Nearby M3 Dwarf NLTT 24399, The Astronomical Journal, 2021, 162 (3): 87, Bibcode:2021AJ....162...87B, S2CID 234763319 , arXiv:2105.08077 , doi:10.3847/1538-3881/ac0432
- ^ Kostov, Veselin B.; et al, TIC 172900988: A Transiting Circumbinary Planet Detected in One Sector of TESS Data, The Astronomical Journal, 2021, 162 (6): 234, Bibcode:2021AJ....162..234K, S2CID 234762777, arXiv:2105.08614 , doi:10.3847/1538-3881/ac223a
- ^ Dai, Fei; et al, TKS X: Confirmation of TOI-1444b and a Comparative Analysis of the Ultra-short-period Planets with Hot Neptunes, 2021, arXiv:2105.08844 [astro-ph.EP]
- ^ 53.0 53.1 53.2 53.3 53.4 53.5 Dalal, S.; et al, The SOPHIE search for northern extrasolar planets, Astronomy & Astrophysics, 2021, 651: A11, S2CID 234790136, arXiv:2105.09741 , doi:10.1051/0004-6361/202140712
- ^ 54.00 54.01 54.02 54.03 54.04 54.05 54.06 54.07 54.08 54.09 54.10 54.11 54.12 Rosenthal, Lee J.; et al, The California Legacy Survey. I. A Catalog of 178 Planets from Precision Radial Velocity Monitoring of 719 Nearby Stars over Three Decades, The Astrophysical Journal Supplement Series, 2021, 255 (1): 8, Bibcode:2021ApJS..255....8R, S2CID 235186973, arXiv:2105.11583 , doi:10.3847/1538-4365/abe23c
- ^ 55.0 55.1 55.2 Amado, Pedro J.; Bauer, Florian F.; Rodríguez López, Cristina; Rodríguez, Eloy; Cardona Guillén, C.; Perger, M.; Caballero, José A.; López-González, Maria J.; Muñoz Rodríguez, I.; Pozuelos, F. J.; Sánchez-Rivero, A.; Schlecker, M.; Quirrenbach, Andreas; Ribas, Ignasi; Reiners, Ansgar; Almenara, J.; Astudillo-Defru, N.; Azzaro, M.; Béjar, Victor J. S.; Bohemann, R.; Bonfils, X.; Bouchy, F.; Cifuentes, C.; Cortés-Contreras, M.; Delfosse, Xavier; Dreizler, Stefan; Forveille, Thierry; Hatzes, Artie P.; Henning, Thomas K.; Jeffers, Sandra V.; Kaminski, Adrian; Kürster, Martin; Lafarga, M.; Lodieu, Nicolas; Lovis, C.; Mayor, M.; Montes, David; Morales, Juan Carlos; Morales, Nicolás; Murgas, F.; Ortiz, José L.; Pepe, F.; Perdelwitz, V.; Pollaco, D.; Santos, N. C.; Schöfer, P.; Schweitzer, A.; Ségransan, N. C.; Shan, Y.; Stock, S.; Tal-Or, Lev; Udry, S.; Zapatero-Osorio, María Rosa; Zechmeister, Mathias. The CARMENES search for exoplanets around M dwarfs. Astronomy & Astrophysics. 2021-05-28, 650: A188. S2CID 235248027. arXiv:2105.13785 . doi:10.1051/0004-6361/202140633.
- ^ Murgas, F.; et al, TOI-674b: An oasis in the desert of exo-Neptunes transiting a nearby M dwarf, Astronomy & Astrophysics, 2021, 653: A60, Bibcode:2021A&A...653A..60M, S2CID 235294286, arXiv:2106.01246 , doi:10.1051/0004-6361/202140718
- ^ Brande, Jonathan; Crossfield, Ian J. M.; Kreidberg, Laura; Oklopčić, Antonija; Polanski, Alex S.; Barman, Travis; Benneke, Björn; Christiansen, Jessie L.; Dragomir, Diana; Foreman-Mackey, Daniel; Fortney, Jonathan J.; Greene, Thomas P.; Howard, Andrew W.; Knutson, Heather A.; Lothringer, Joshua D.; Mikal-Evans, Thomas; Morley, Caroline V., A Mirage or an Oasis? Water Vapor in the Atmosphere of the Warm Neptune TOI-674 b, 2022, arXiv:2201.04197
- ^ 58.0 58.1 Eisner, N. L.; et al, Planet Hunters TESS III: Two transiting planets around the bright G dwarf HD 152843, Monthly Notices of the Royal Astronomical Society, 2021, 505 (2): 1827–1840, arXiv:2106.04603 , doi:10.1093/mnras/stab1253
- ^ 59.0 59.1 59.2 59.3 59.4 Hwang, Kyu-Ha; et al, Systematic KMTNet Planetary Anomaly Search, Paper II: Five New q<2×10−4 Mass-ratio Planets, 2021, S2CID 245740102, arXiv:2106.06686 , doi:10.3847/1538-3881/ac38ad
- ^ Khandelwal, Akanksha; et al, Discovery of an inflated hot Jupiter around a slightly evolved star TOI-1789, 2021, arXiv:2106.08660 , doi:10.1093/mnras/stab2970
- ^ 61.0 61.1 Wirth, Christopher P.; et al, TOI-942b: A Prograde Neptune in a ∼ 60 Myr Old Multi-transiting System, The Astrophysical Journal Letters, 2021, 917 (2): L34, Bibcode:2021ApJ...917L..34W, S2CID 235670113, arXiv:2106.14968 , doi:10.3847/2041-8213/ac13a9
- ^ Han, Cheongho; et al, KMT-2018-BLG-1743: Planetary microlensing event occurring on two source stars, Astronomy & Astrophysics, 2021, 652: A145, Bibcode:2021A&A...652A.145H, S2CID 235694685, arXiv:2107.00155 , doi:10.1051/0004-6361/202140923
- ^ 63.0 63.1 63.2 Fukui, A.; et al, TOI-1749: An M dwarf with a Trio of Planets including a Near-resonant Pair, The Astronomical Journal, 2021, 162 (4): 167, Bibcode:2021AJ....162..167F, S2CID 235795469, arXiv:2107.05430 , doi:10.3847/1538-3881/ac13a5
- ^ 64.0 64.1 64.2 64.3 64.4 64.5 Demangeon, O. D. S.; et al, The SOPHIE search for northern extrasolar planets, Astronomy & Astrophysics, 2021, 653: A78, S2CID 235795175, arXiv:2107.05089 , doi:10.1051/0004-6361/202141079
- ^ Dalba, Paul A.; et al, Giant Outer Transiting Exoplanet Mass (GOT 'EM) Survey. II. Discovery of a Failed Hot Jupiter on a 2.7 Yr, Highly Eccentric Orbit, The Astronomical Journal, 2021, 162 (4): 154, Bibcode:2021AJ....162..154D, S2CID 235898945, arXiv:2107.06901 , doi:10.3847/1538-3881/ac134b
- ^ Kanodia, Shubham; et al, TOI-532b: The Habitable-zone Planet Finder confirms a Large Super Neptune in the Neptune Desert orbiting a metal-rich M-dwarf host, The Astronomical Journal, 2021, 162 (4): 135, Bibcode:2021AJ....162..135K, S2CID 236493328, arXiv:2107.13670 , doi:10.3847/1538-3881/ac1940
- ^ Wells, R. D.; et al, A large sub-Neptune transiting the thick-disk M4 V TOI-2406, Astronomy & Astrophysics, 2021, 653: A97, Bibcode:2021A&A...653A..97W, S2CID 236493492, arXiv:2107.14125 , doi:10.1051/0004-6361/202141277
- ^ 68.0 68.1 68.2 Lillo-Box, J.; et al, Follow-up of non-transiting planets detected by Kepler, Astronomy & Astrophysics, 2021, 654: A9, S2CID 236635201, arXiv:2107.14621 , doi:10.1051/0004-6361/202140746
- ^ Winters, Jennifer G.; Cloutier, Ryan; Medina, Amber A.; Irwin, Jonathan M.; Charbonneau, David; Astudillo-Defru, Nicola; Bonfils, Xavier; Howard, Andrew W.; Isaacson, Howard; Bean, J. L.; Seifahrt, A.; Teske, J. K.; Eastman, Jason D.; Twicken, Joseph D.; Collins, K. A.; Jensen, E. L. N.; Quinn, S. N.; Payne, M. J.; Kristiansen, M. H.; Spencer, A.; Vanderburg, Andrew; Zechmeister, Mathias; Weiss, L. M.; Wang, S. X.; Wang, G.; Udry, Stéphane; Terentev, I. A.; Sturmer, J.; Stefansson, G.; Shectman, Stephen A.; Sefako, R.; Schwengeler, H. M.; Schwarz, R. P.; Scarsdale, N.; Rubenzahl, R. A.; Roy, A.; Rosenthal, L. J.; Robertson, P.; Petigura, Erik A.; Pepe, Francesco; Omohundro, M.; Murphy, J. M. A.; Murgas, Felipe; Movcnik, T.; Montet, B. T.; Mennickent, R.; Mayo, A. W.; Massey, B.; Lubin, J.; Lovis, Christophe; Lewin, P.; Kasper, D.; Kane, S. R.; Jenkins, J. M.; Huber, D.; Horne, K.; Hill, M. L.; Gorrini, P.; Giacalone, S.; Fulton, Benjamin J.; Forveille, Thierry; Figueira, Pedro; Fetherolf, T.; Dressing, Courtney D.; Díaz, Rodrigo F.; Delfosse, Xavier; Dalba, P. A.; Dai, F.; Cortes, C. C.; Crossfield, Ian J. M.; Crane, Jeffrey D.; Conti, D. M.; Collins, K. I.; Chontos, A.; Butler, R. Paul; Brown, P.; Brady, M.; Bouchy, François; Behmard, A.; Beard, C.; Batalha, Natalie M.; Almenara, José M. A Second Planet Transiting LTT 1445A and a Determination of the Masses of Both Worlds. The Astronomical Journal. 2022, 163 (4): 168. Bibcode:2022AJ....163..168W. S2CID 236635391. arXiv:2107.14737 . doi:10.3847/1538-3881/ac50a9.
- ^ 70.0 70.1 A warm terrestrial planet with half the mass of Venus transiting a nearby star (PDF). [2022-08-29]. （原始内容存档 (PDF)于2021-11-13）.
- ^ Lubin, Jack; et al, TESS-Keck Survey. IX. Masses of Three Sub-Neptunes Orbiting HD 191939 and the Discovery of a Warm Jovian plus a Distant Substellar Companion, The Astronomical Journal, 2022, 163 (2): 101, Bibcode:2022AJ....163..101L, S2CID 236924440, arXiv:2108.02208 , doi:10.3847/1538-3881/ac3d38
- ^ Shin, In-Gu; et al, Using Source Proper Motion to Validate Terrestrial Parallax: OGLE-2019-BLG-1058, The Astronomical Journal, 2021, 162 (6): 267, Bibcode:2021AJ....162..267S, S2CID 236924486, arXiv:2108.02499 , doi:10.3847/1538-3881/ac2ba5
- ^ Saunders, Nicholas; et al, TESS Giants Transiting Giants. I.: A Noninflated Hot Jupiter Orbiting a Massive Subgiant, The Astronomical Journal, 2022, 163 (2): 53, Bibcode:2022AJ....163...53S, S2CID 236924647, arXiv:2108.02294 , doi:10.3847/1538-3881/ac38a1
- ^ 74.0 74.1 74.2 Osborn, Ares; et al, TOI-431/HIP 26013: a super-Earth and a sub-Neptune transiting a bright, early K dwarf, with a third RV planet, Monthly Notices of the Royal Astronomical Society, 2021, 507 (2): 2782–2803, arXiv:2108.02310 , doi:10.1093/mnras/stab2313
- ^ 75.0 75.1 Trifonov, Trifon; et al, A Pair of Warm Giant Planets near the 2:1 Mean Motion Resonance around the K-dwarf Star TOI-2202, The Astronomical Journal, 2021, 162 (6): 283, Bibcode:2021AJ....162..283T, S2CID 236976243, arXiv:2108.05323 , doi:10.3847/1538-3881/ac1bbe
- ^ 76.00 76.01 76.02 76.03 76.04 76.05 76.06 76.07 76.08 76.09 76.10 76.11 76.12 76.13 76.14 76.15 76.16 76.17 76.18 76.19 76.20 76.21 76.22 76.23 76.24 76.25 76.26 76.27 76.28 76.29 76.30 76.31 76.32 76.33 76.34 76.35 76.36 De Leon, J. P.; et al, 37 New Validated Planets in Overlapping K2 Campaigns, Monthly Notices of the Royal Astronomical Society, 2021, 508: 195–218, arXiv:2108.05621 , doi:10.1093/mnras/stab2305
- ^ Kovacs, Geza, More planetary candidates from K2 Campaign 5 using TRAN_K2, Astronomy & Astrophysics, 2020, 643: A169, Bibcode:2020A&A...643A.169K, S2CID 221266076, arXiv:2008.10075 , doi:10.1051/0004-6361/202038726
- ^ Lillo-Box, J.; et al, HD 22496 b: The first ESPRESSO stand-alone planet discovery, Astronomy & Astrophysics, 2021, 654: A60, Bibcode:2021A&A...654A..60L, S2CID 237371680, arXiv:2109.00226 , doi:10.1051/0004-6361/202141714
- ^ 79.0 79.1 79.2 79.3 Castro-González, A.; et al, The K2-OjOS Project: New and revisited planets and candidates in K2 campaigns 5, 16, & 18, Monthly Notices of the Royal Astronomical Society, 2022, 509: 1075–1095, arXiv:2109.03346 , doi:10.1093/mnras/stab2669
- ^ Dong, Jiayin; et al, TOI-3362b: A Proto Hot Jupiter Undergoing High-eccentricity Tidal Migration, The Astrophysical Journal Letters, 2021, 920 (1): L16, Bibcode:2021ApJ...920L..16D, S2CID 237442300, arXiv:2109.03771 , doi:10.3847/2041-8213/ac2600
- ^ 81.0 81.1 81.2 Han, Cheongho; et al, Three faint-source microlensing planets detected via the resonant-caustic channel, Astronomy & Astrophysics, 2021, 655: A21, Bibcode:2021A&A...655A..21H, S2CID 237513708, arXiv:2109.07068 , doi:10.1051/0004-6361/202141517
- ^ 82.0 82.1 Moutou, C.; et al, TOI-1296b and TOI-1298b observed with TESS and SOPHIE: Two hot Saturn-mass exoplanets with different densities around metal-rich stars, Astronomy & Astrophysics, 2021, 653: A147, Bibcode:2021A&A...653A.147M, S2CID 237571683, arXiv:2109.09252 , doi:10.1051/0004-6361/202141151
- ^ Kossakowski, D.; et al, TOI-1201 b: A mini-Neptune transiting a bright and moderately young M dwarf, Astronomy & Astrophysics, 2021, 656: A124, Bibcode:2021A&A...656A.124K, S2CID 237571914, arXiv:2109.09346 , doi:10.1051/0004-6361/202141587
- ^ Rattanamala, R.; Awiphan, S.; Komonjinda, S.; Phriksee, A.; Sappankum, P.; A-thano, N.; Chitchak, S.; Rittipruk, P.; Sawangwit, U.; Poshyachinda, S.; Reichart, D. E.; Haislip, J. B., Two circumbinary planets in RR Cae eclipsing binary system, 2021, arXiv:2109.09397
- ^ Montalto, M.; Malavolta, L.; Gregorio, J.; Mantovan, G.; Desidera, S.; Piotto, G.; Nascimbeni, V.; Granata, V.; Manthopoulou, E. E.; Claudi, R., TIC 257060897b: An inflated, low-density, hot-Jupiter transiting a rapidly evolving subgiant star, Monthly Notices of the Royal Astronomical Society, 2022, 509 (2): 2908–2919, arXiv:2110.00489 , doi:10.1093/mnras/stab2923
- ^ Gan, Tianjun; et al, TOI-530b: A giant planet transiting an M dwarf detected by TESS, Monthly Notices of the Royal Astronomical Society, 2021, 511: 83–99, arXiv:2110.04220 , doi:10.1093/mnras/stab3708
- ^ 87.0 87.1 MacDougall, Mason G.; et al, The TESS–Keck Survey. VI. Two Eccentric Sub-Neptunes Orbiting HIP-97166, The Astronomical Journal, 2021, 162 (6): 265, Bibcode:2021AJ....162..265M, S2CID 238634523, arXiv:2110.05628 , doi:10.3847/1538-3881/ac295e
- ^ 88.0 88.1 Scarsdale, Nicholas; et al, TESS-Keck Survey. V. Twin Sub-Neptunes Transiting the Nearby G Star HD 63935, The Astronomical Journal, 2021, 162 (5): 215, Bibcode:2021AJ....162..215S, S2CID 238743956, arXiv:2110.06885 , doi:10.3847/1538-3881/ac18cb
- ^ Heidari, N.; et al, HD 207897 b: A dense sub-Neptune transiting a nearby and bright K-type star, Astronomy & Astrophysics, 2022, 658: A176, Bibcode:2022A&A...658A.176H, S2CID 239016573, arXiv:2110.08597 , doi:10.1051/0004-6361/202141429
- ^ Gaidos, E.; Hirano, T.; Kraus, A. L.; Kuzuhara, M.; Zhang, Z.; Lee, R. A.; Salama, M.; Berger, T. A.; Grunblatt, S. K.; Ansdell, M.; Liu, M. C.; Harakawa, H.; Hodapp, K. W.; Jacobson, S.; Konishi, M.; Kotani, T.; Kudo, T.; Kurokawa, T.; Nishikawa, J.; Omiya, M.; Serizawa, T.; Tamura, M.; Ueda, A.; Vievard, S., Zodiacal Exoplanets in Time (ZEIT) XII: A Directly-Imaged Planetary-Mass Companion to a Young Taurus M Dwarf Star, Monthly Notices of the Royal Astronomical Society, 2021, 512: 583–601, arXiv:2110.08655 , doi:10.1093/mnras/stab3069
- ^ Astronomers Discover Infant Planet – One of the Youngest Exoplanets Ever Observed. [2022-08-29]. （原始内容存档于2021-10-25）.
- ^ Mann, Andrew W.; et al, TESS Hunt for Young and Maturing Exoplanets (THYME). VI. An 11 Myr Giant Planet Transiting a Very-low-mass Star in Lower Centaurus Crux, The Astronomical Journal, 2022, 163 (4): 156, Bibcode:2022AJ....163..156M, S2CID 239024522, arXiv:2110.09531 , doi:10.3847/1538-3881/ac511d
- ^ Fukui, Akihiko; et al, TOI-2285b: A 1.7 Earth-radius planet near the habitable zone around a nearby M dwarf, Publications of the Astronomical Society of Japan, 2021, 74: L1–L8, arXiv:2110.10215 , doi:10.1093/pasj/psab106
- ^ 94.0 94.1 Silverstein, Michele L.; et al, The LHS 1678 System: Two Earth-sized Transiting Planets and an Astrometric Companion Orbiting an M Dwarf Near the Convective Boundary at 20 pc, The Astronomical Journal, 2022, 163 (4): 151, Bibcode:2022AJ....163..151S, S2CID 239768873, arXiv:2110.12079 , doi:10.3847/1538-3881/ac32e3
- ^ 95.0 95.1 Barragán, O.; et al, The young HD 73583 (TOI-560) planetary system: Two 10-M⊕ mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarf, Monthly Notices of the Royal Astronomical Society, 2022, 514 (2): 1606–1627, arXiv:2110.13069 , doi:10.1093/mnras/stac638
- ^ Zhang, Michael; Knutson, Heather A.; Wang, Lile; Dai, Fei; Barragán, Oscar, Escaping Helium from TOI 560.01, a Young Mini-Neptune, The Astronomical Journal, 2022, 163 (2): 67, Bibcode:2022AJ....163...67Z, S2CID 239885237, arXiv:2110.13150 , doi:10.3847/1538-3881/ac3fa7
- ^ 97.0 97.1 97.2 97.3 Hedges, Christina; et al, TOI-2076 and TOI-1807: Two Young, Comoving Planetary Systems within 50 pc Identified by TESS that are Ideal Candidates for Further Follow up, The Astronomical Journal, 2021, 162 (2): 54, Bibcode:2021AJ....162...54H, S2CID 235805026, arXiv:2111.01311 , doi:10.3847/1538-3881/ac06cd
- ^ Osborn, H.; et al, Uncovering the true periods of the young sub-Neptunes orbiting TOI-2076, Astronomy & Astrophysics, 2022, S2CID 247292643, arXiv:2203.03194 , doi:10.1051/0004-6361/202243065
- ^ Schanche, N.; et al, TOI-2257 b: A highly eccentric long-period sub-Neptune transiting a nearby M dwarf, Astronomy & Astrophysics, 2022, 657: A45, Bibcode:2022A&A...657A..45S, S2CID 240419956, arXiv:2111.01749 , doi:10.1051/0004-6361/202142280
- ^ 100.0 100.1 100.2 Vach, Sydney; et al, TOI-712: a system of adolescent mini-Neptunes extending to the habitable zone, 2021, arXiv:2111.02416
- ^ 101.0 101.1 Han, Cheongho; et al, OGLE-2019-BLG-0468Lb,c: Two microlensing giant planets around a G-type star, Astronomy & Astrophysics, 2022, 658: A93, Bibcode:2022A&A...658A..93H, S2CID 243847948, arXiv:2111.03755 , doi:10.1051/0004-6361/202142327
- ^ Han, Cheongho; et al, KMT-2021-BLG-0912Lb: A microlensing super Earth around a K-type star, Astronomy & Astrophysics, 2022, 658: A94, Bibcode:2022A&A...658A..94H, S2CID 243860989, arXiv:2111.04861 , doi:10.1051/0004-6361/202142495
- ^ 103.0 103.1 Azevedo Silva, T.; et al, The HD 137496 system: A dense, hot super-Mercury and a cold Jupiter, Astronomy & Astrophysics, 2022, 657: A68, Bibcode:2022A&A...657A..68A, S2CID 243809625, arXiv:2111.08764 , doi:10.1051/0004-6361/202141520
- ^ 104.0 104.1 104.2 Jeong, G.; Lee, B. C.; Park, M. G.; Bang, T. Y.; Han, I., Search for exoplanets around northern circumpolar stars, Astronomy & Astrophysics, 2022, 662: A12, S2CID 244270271, arXiv:2111.08899 , doi:10.1051/0004-6361/202142379
- ^ Han, Cheongho; Gould, Andrew; Albrow, Michael D.; Chung, Sun-Ju; Hwang, Kyu-Ha; Youn Kil Jung; Kim, Doeon; Lee, Chung-Uk; Mao, Shude; Ryu, Yoon-Hyun; Shin, In-Gu; Shvartzvald, Yossi; Yee, Jennifer C.; Zang, Weicheng; Cha, Sang-Mok; Kim, Dong-Jin; Kim, Hyoun-Woo; Kim, Seung-Lee; Lee, Dong-Joo; Lee, Yongseok; Park, Byeong-Gon; Pogge, Richard W.; Kim, Chun-Hwey, KMT-2018-BLG-1988Lb: Microlensing super-Earth orbiting a low-mass disk dwarf, Astronomy & Astrophysics, 2022, 658: A62, Bibcode:2022A&A...658A..62H, S2CID 244270928, arXiv:2111.08955 , doi:10.1051/0004-6361/202142077
- ^ Sun, Leilei; Ioannidis, Panagiotis; Gu, Shenghong; Schmitt, Jürgen H. M. M.; Wang, Xiaobin; Kouwenhoven, M. B. N.; Perdelwitz, Volker; Francesco Flammini Dotti; Czesla, Stefan, A highly mutually inclined compact warm-Jupiter system KOI-984?, Monthly Notices of the Royal Astronomical Society, 2022, 512 (3): 4604–4617, arXiv:2111.09668 , doi:10.1093/mnras/stab3367
- ^ Wong, Ian; et al, TOI-2109: An Ultrahot Gas Giant on a 16 hr Orbit, The Astronomical Journal, 2021, 162 (6): 256, Bibcode:2021AJ....162..256W, S2CID 244488632, arXiv:2111.12074 , doi:10.3847/1538-3881/ac26bd
- ^ 108.0 108.1 González-Álvarez, E.; et al, A multi-planetary system orbiting the early-M dwarf TOI-1238, Astronomy & Astrophysics, 2022, 658: A138, Bibcode:2022A&A...658A.138G, S2CID 244715047, arXiv:2111.14602 , doi:10.1051/0004-6361/202142128
- ^ Smith, A M S.; et al, K2-99 revisited: A non-inflated warm Jupiter, and a temperate giant planet on a 522-d orbit around a subgiant, Monthly Notices of the Royal Astronomical Society, 2021, 510 (4): 5035–5049, arXiv:2111.14660 , doi:10.1093/mnras/stab3497
- ^ 110.0 110.1 110.2 Paredes, Leonardo A.; Henry, Todd J.; Quinn, Samuel N.; Gies, Douglas R.; Hinojosa-Goñi, Rodrigo; James, Hodari-Sadiki; Jao, Wei-Chun; White, Russel J., The Solar Neighborhood XLVIII: Nine Giant Planets Orbiting Nearby K Dwarfs, and the CHIRON Spectrograph's Radial Velocity Performance, The Astronomical Journal, 2021, 162 (5): 176, Bibcode:2021AJ....162..176P, S2CID 237285778, arXiv:2111.15028 , doi:10.3847/1538-3881/ac082a
- ^ Wittenmyer, Robert A.; et al, TOI-1842b: A Transiting Warm Saturn Undergoing Re-Inflation around an Evolving Subgiant, The Astronomical Journal, 2021, 163 (2): 82, Bibcode:2022AJ....163...82W, S2CID 244773259, arXiv:2112.00198 , doi:10.3847/1538-3881/ac3f39
- ^ Lam, Kristine W. F.; et al, GJ 367b: A dense, ultrashort-period sub-Earth planet transiting a nearby red dwarf star, Science, 2021, 374 (6572): 1271–1275, Bibcode:2021Sci...374.1271L, PMID 34855492, S2CID 244799656, arXiv:2112.01309 , doi:10.1126/science.aay3253
- ^ 113.0 113.1 113.2 113.3 Jordán, A.; et al, HATS-74Ab, HATS-75b, HATS-76b, and HATS-77b: Four Transiting Giant Planets Around K and M Dwarfs, The Astronomical Journal, 2022, 163 (3): 125, Bibcode:2022AJ....163..125J, S2CID 244896205, arXiv:2112.01928 , doi:10.3847/1538-3881/ac4a77
- ^ Cañas, Caleb I.; Mahadevan, Suvrath; Cochran, William D.; Bender, Chad F.; Feigelson, Eric D.; Harman, C. E.; Kopparapu, Ravi Kumar; Caceres, Gabriel A.; Diddams, Scott A.; Endl, Michael; Ford, Eric B.; Halverson, Samuel; Hearty, Fred; Jones, Sinclaire; Kanodia, Shubham; Lin, Andrea S. J.; Metcalf, Andrew J.; Monson, Andrew; Ninan, Joe P.; Ramsey, Lawrence W.; Robertson, Paul; Roy, Arpita; Schwab, Christian; Stefánsson, Guđmundur, A Hot Mars-sized Exoplanet Transiting an M Dwarf, The Astronomical Journal, 2022, 163 (1): 3, Bibcode:2022AJ....163....3C, S2CID 244954104, arXiv:2112.03958 , doi:10.3847/1538-3881/ac3088
- ^ Faherty, Jacqueline K.; Gagné, Jonathan; Popinchalk, Mark; Vos, Johanna M.; Burgasser, Adam J.; Schümann, Jörg; Schneider, Adam C.; Kirkpatrick, J. Davy; Meisner, Aaron M.; Kuchner, Marc J.; Bardalez Gagliuffi, Daniella C.; Marocco, Federico; Caselden, Dan; Gonzales, Eileen C.; Rothermich, Austin; Casewell, Sarah L.; Debes, John H.; Aganze, Christian; Ayala, Andrew; Hsu, Chih-Chun; Cooper, William J.; Smart, R. L.; Gerasimov, Roman; Theissen, Christopher A.; The Backyard Worlds; Planet 9 Collaboration, A Wide Planetary Mass Companion Discovered through the Citizen Science Project Backyard Worlds: Planet 9, The Astrophysical Journal, 2021, 923 (1): 48, Bibcode:2021ApJ...923...48F, S2CID 245005964, arXiv:2112.04678 , doi:10.3847/1538-4357/ac2499
- ^ Janson, Markus; Gratton, Raffaele; Rodet, Laetitia; Vigan, Arthur; Bonnefoy, Mickaël; Delorme, Philippe; Mamajek, Eric E.; Reffert, Sabine; Stock, Lukas; Marleau, Gabriel-Dominique; Langlois, Maud; Chauvin, Gaël; Desidera, Silvano; Ringqvist, Simon; Mayer, Lucio; Viswanath, Gayathri; Squicciarini, Vito; Meyer, Michael R.; Samland, Matthias; Petrus, Simon; Helled, Ravit; Kenworthy, Matthew A.; Quanz, Sascha P.; Biller, Beth; Henning, Thomas; Mesa, Dino; Engler, Natalia; Carson, Joseph C., A wide-orbit giant planet in the high-mass b Centauri binary system, Nature, 2021, 600 (7888): 231–234, Bibcode:2021Natur.600..231J, PMID 34880428, S2CID 245005994, arXiv:2112.04833 , doi:10.1038/s41586-021-04124-8
- ^ 117.0 117.1 117.2 117.3 117.4 117.5 117.6 117.7 117.8 Teng, Huan-Yu; Sato, Bun'ei; Takarada, Takuya; Omiya, Masashi; Harakawa, Hiroki; Izumiura, Hideyuki; Kambe, Eiji; Takeda, Yoichi; Yoshida, Michitoshi; Itoh, Yoichi; Ando, Hiroyasu; Kokubo, Eiichiro, Regular radial velocity variations in nine G- and K-type giant stars: Eight planets and one planet candidate, Publications of the Astronomical Society of Japan, 2021, 74: 92–127, arXiv:2112.07169 , doi:10.1093/pasj/psab112
- ^ Xie, Xiao-Jia; Dong, Subo; Shvartzvald, Yossi; Gould, Andrew; Udalski, Andrzej; Beaulieu, Jean-Philippe; Beichman, Charles; Close, Laird Miller; b. Henderson, Calen; r. Males, Jared; Marquette, Jean-Baptiste; m. Morzinski, Katie; r. Gelino, Christopher, Characterizing microlensing planetary system OGLE-2014-BLG-0676Lb with adaptive optics imaging, Research in Astronomy and Astrophysics, 2022, 21 (12): 303, S2CID 244211319, arXiv:2112.08030 , doi:10.1088/1674-4527/ac2a09
- ^ 119.0 119.1 Sreenivas, K. R.; Perdelwitz, V.; Tal-Or, L.; Trifonov, T.; Zucker, S.; Mazeh, T., Analysis of the public HARPS/ESO spectroscopic archive, Astronomy & Astrophysics, 2022, 660: A124, S2CID 245219286, arXiv:2112.09029 , doi:10.1051/0004-6361/202142612
- ^ 120.0 120.1 Mohammed El Mufti; et al, TOI 560 : Two Transiting Planets Orbiting a K Dwarf Validated with iSHELL, PFS and HIRES RVs, 2021, arXiv:2112.13448
- ^ Miyazaki, Shota; et al, OGLE-2014-BLG-0319: A Sub-Jupiter-mass Planetary Event Encountered Degeneracy with Different Mass Ratios and Lens-source Relative Proper Motions, The Astronomical Journal, 2022, 163 (3): 123, Bibcode:2022AJ....163..123M, S2CID 245634898, arXiv:2112.14997 , doi:10.3847/1538-3881/ac4960
- ^ Wang(王涵悦), Hanyue; et al, Systematic Korea Microlensing Telescope Network planetary anomaly search – III. One wide-orbit planet and two stellar binaries, Monthly Notices of the Royal Astronomical Society, 2022, 510 (2): 1778–1790, arXiv:2112.02414 , doi:10.1093/mnras/stab3581
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