| Exoplaneta | Estrela | Descoberta | Método de detecção | Massa |
| SRGeJ0411 b | GALEX J041130.0+685350 | 2024 | — | 40,00 MJ |
| TOI-1135 b | BD+85 211 | 2024 | — | 0,16 MJ |
| TOI-1180 b | TYC 4565-656-1 | 2024 | — | 0,03 MJ |
| TOI-1723 b | BD+68 495 | 2024 | — | 0,03 MJ |
| HD 36384 b | HD 36384 | 2023 | espectroscopia Dopple | 6,60 MJ |
| SRGeJ0453 b | GALEX J045400.1+622444 | 2023 | — | 44,00 MJ |
| TOI-1694 b | TYC 4108-1434-1 | 2023 | — | 0,08 MJ |
| TOI-4127 b | TYC 4367-1160-1 | 2023 | — | 2,30 MJ |
| HD 46588 b | HD 46588 | 2022 | espectroscopia Dopple | 0,25 MJ |
| HD 46588 c | HD 46588 | 2022 | — | 52,00 MJ |
| TOI-1694 c | TYC 4108-1434-1 | 2022 | espectroscopia Dopple | 0,93 MJ |
| TOI-1710 Ab | BD+76 227 | 2022 | — | 0,09 MJ |
| TOI-2257b | UCAC4 839-012174 | 2022 | — | 0,02 MJ |
| TOI-4137 b | TYC 4346-736-1 | 2022 | — | 1,44 MJ |
| Gaia-2 b | TYC 4123-515-1 | 2021 | — | 0,82 MJ |
| HD 95544 Ab | HD 95544 | 2021 | espectroscopia Dopple | 7,74 MJ |
| HAT-P-58 b | HAT-P-58 | 2020 | — | 0,37 MJ |
| HD 60292 b | HD 60292 | 2020 | espectroscopia Dopple | 6,50 MJ |
| TOI-1728b | UCAC4 774-029023 | 2020 | — | 0,08 MJ |
| V470 Cam (AB) c | V* V470 Cam | 2020 | — | 11,80 MJ |
| WISE J0458+6434 A | — | 2019 | Astrometria | 57,00 MJ |
| WISE J0458+6434 B | — | 2019 | Astrometria | 14,00 MJ |
| HD 40956 b | HD 40956 | 2018 | espectroscopia Dopple | 2,70 MJ |
| HD 44385 b | HD 44385 | 2018 | espectroscopia Dopple | 5,90 MJ |
| HD 29021 b | HD 29021 | 2017 | espectroscopia Dopple | 4,47 MJ |
| PSR B0329+54 b | PSR B0329+54 | 2017 | — | 0,01 MJ |
| XO-6b | XO-6 | 2017 | — | 4,40 MJ |
| HD 35759 b | HD 35759 | 2016 | espectroscopia Dopple | 3,76 MJ |
| HD 24064 b | HD 24064 | 2015 | espectroscopia Dopple | 9,40 MJ |
| V470 Cam (AB) b | V* V470 Cam | 2013 | — | 27,00 MJ |
| HD 32518 b | HD 32518 | 2009 | espectroscopia Dopple | 3,04 MJ |
| XO-3b | XO-3 | 2007 | — | 11,70 MJ |
| HD 33564 b | HD 33564 | 2005 | espectroscopia Dopple | 9,10 MJ |
| HD 104985 b | HD 104985 | 2003 | espectroscopia Dopple | 8,30 MJ |