TOI-544 b: a potential water-world inside the radius valley in a two-planet system

Author(s):
Osborne, H.L.M.; Eylen, V. van; Goffo, E.; Gandolfi, D.; Nowak, G.; Persson, C.M.; Livingston, J.; Weeks, A.; Pallé, E.; Luque, R.; Hellier, C.; Carleo, I.; Redfield, S.; Hirano, T.; Gili, M.G.; Alarcon, J.; Barragán, O.; Casasayas-Barris, N.; Díaz, M.R.; Esposito, M.; Jenkins, J.S.; Knudstrup, E.; Murgas, F.; Orell-Miquel, J.; Rodler, F.; Serrano, L.; Stangret, M.; Albrecht, S.H.; Alqasim, A.; Cochran, W.D.; Deeg, H.J.; Fridlund, M.; Hatzes, A.; Korth, J.; Lam, K.W.F.
Published
2024
Publication type
Article / Letter to editor
ExoplanetsTechniques: radial velocitiesPlanets and satellites: compositionPlanets and satellites: detectionAstrophysics - Earth and Planetary Astrophysics
Date issued
2024
Language
English
Is part of
Monthly Notices of the Royal Astronomical Society (2024), Vol. 527, no. 4, p. 11138–11157
hdl
1887/3718998
doi
10.1093/mnras/stad3837
URL
https://ui.adsabs.harvard.edu/abs/2023MNRAS.tmp.3690O