Planets observed with CHEOPS. Two super-Earths orbiting the red dwarf star TOI-776
Context. M-dwarf stars are the most common of potential exoplanet host stars in the Galaxy. It is therefore very important to understand planetary systems orbiting such stars and to determine the physical parameters of such planets with high precision. Also with the launch of the James Webb Space Telescope (JWST) the observation of atmospheric
Fridlund, M. et al.
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2024