We report the confirmation of a transiting planet around the bright weakly active M0.5 V star TOI-1235 (TYC 4384-1735-1, V ≈ 11.5 mag), whose transit signal was detected in the photometric time series of sectors 14, 20, and 21 of the TESS space mission. We confirm the planetary nature of the transit signal, which has a period of 3.44 d, by using precise RV measurements with the CARMENES, HARPS-N, and iSHELL spectrographs, supplemented by high-resolution imaging and ground-based photometry. A comparison of the properties derived for TOI-1235 b with theoretical models reveals that the planet has a rocky composition, with a bulk density slightly higher than that of Earth. In particular, we measure a mass of Mp = 5.9 \ub1 0.6 M⊕ and a radius of...
Dynamical histories of planetary systems, as well as the atmospheric evolution of highly irradiated ...
Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero ...
Context. Exoplanets with orbital periods of less than one day are known as ultra-short period (USP) ...
We report the confirmation of a transiting planet around the bright weakly active M0.5 V star TOI-12...
We report the confirmation of a transiting planet around the bright weakly active M0.5 V star TOI-12...
Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero ...
Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero ...
Populating the exoplanet mass-radius diagram in order to identify the underlying relationship that g...
We report the discovery of TO1-2285b, a sub-Neptune-sized planet transiting a nearby (42 pc) M dwarf...
We report the discovery and characterization of two small transiting planets orbiting the bright M3....
Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero ...
Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero ...
Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero ...
We report the discovery of a super-Earth and a sub-Neptune transiting the star HD 15337 (TOI-402, TI...
Studies of close-in planets orbiting M dwarfs have suggested that the M-dwarf radius valley may be w...
Dynamical histories of planetary systems, as well as the atmospheric evolution of highly irradiated ...
Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero ...
Context. Exoplanets with orbital periods of less than one day are known as ultra-short period (USP) ...
We report the confirmation of a transiting planet around the bright weakly active M0.5 V star TOI-12...
We report the confirmation of a transiting planet around the bright weakly active M0.5 V star TOI-12...
Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero ...
Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero ...
Populating the exoplanet mass-radius diagram in order to identify the underlying relationship that g...
We report the discovery of TO1-2285b, a sub-Neptune-sized planet transiting a nearby (42 pc) M dwarf...
We report the discovery and characterization of two small transiting planets orbiting the bright M3....
Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero ...
Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero ...
Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero ...
We report the discovery of a super-Earth and a sub-Neptune transiting the star HD 15337 (TOI-402, TI...
Studies of close-in planets orbiting M dwarfs have suggested that the M-dwarf radius valley may be w...
Dynamical histories of planetary systems, as well as the atmospheric evolution of highly irradiated ...
Small planets on close-in orbits tend to exhibit envelope mass fractions of either effectively zero ...
Context. Exoplanets with orbital periods of less than one day are known as ultra-short period (USP) ...