Radius-period diagram of close-in exoplanets with mass and radius measured to an accuracy of at least 5 σ. The data were obtained from the NASA Exoplanet Archive on February 13, 2025. Error bars have been suppressed for clarity. The position of TOI-5795 b is highlighted, together with the population-based boundaries of the Neptunian desert, ridge, and savanna, as derived by Castro-González et al. (2024a). This plot was generated with nep-des (https://github.com/castro-gzlz/nep-des).