Fig. 14

Density-equilibrium temperature diagram of warm-hot exoplanets with a radius of less than 3 R⊕ around M dwarfs. All planets have mass determination by either RVs or TTVs. TOI-1685 b is labeled and marked with a thicker black borderline. Some densities are marked as reference by horizontal lines, including Earth (dashed orange), H2O (blue), and 50% H2O, 50% silicate (green). The observed ρ-Teq space before the discovery of TOI-1685 b is shaded in red to illustrate the dissimilarity of TOI-1685 b with previous discoveries.
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.