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Santos, N. Law, N. Schanche, R. Hounsell, S. C. C. Barros, S. Gandhi, S. G. Sousa, S. Seager, T.-G. Tan, V. Adibekyan, V. Bourrier, Z. Benkhaldoun, Z. Essack","submitted_at":"2024-09-26T17:59:55Z","abstract_excerpt":"The Neptunian desert and savanna have recently been found to be separated by a ridge, an overdensity of planets in the period range of $\\simeq$3-5 days. These features are thought to be shaped by dynamical and atmospheric processes, but their roles are not yet well understood. Our aim was to confirm and characterize the super-Neptune TESS candidate TOI-5005.01, which orbits a moderately bright (V = 11.8) solar-type star (G2 V) with an orbital period of 6.3 days. 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