TOI-3288 b and TOI-4666 b (red encircled) compared to known transiting exoplanets from the PlanetS catalogue (Otegi et al. 2020; Parc et al. 2024, updated August 2025). Marker colours show stellar metallicity, with grey for stars of unknown metallicity. Stellar markers indicate planetary companions in binary systems. Circles are single stars. The vertical grey line marks 4600 K. The relative occurrence of the gas giants with masses between 0.1 and 13 M_Jup is shown as a histogram at the top. Our two mass characterisations contribute to a rare population of exoplanets.