Journal: Monthly Notices of the Royal Astronomical Society
Publication
TOI-220 b: a warm sub-Neptune discovered by TESS
In this paper, we report the discovery of TOI-220 b, a new sub-Neptune detected by the Transiting Exoplanet Survey Satellite (TESS) and confirmed by radial...
TOI-2379 b and TOI-2384 b: two super-Jupiter mass planets transiting low-mass host stars
Short-period gas giant planets have been shown to be significantly rarer for host stars less massive than the Sun. We report the discovery of two transiting...
We present the validation of TOI-2407 b, a warm Neptune-sized planet with a radius of $4.26\pm 0.26$ R $_{\oplus }$, orbiting an early M-type star with a period...
TOI-257b (HD 19916b): a warm sub-saturn orbiting an evolved F-type star
We report the discovery of a warm sub-Saturn, TOI-257b (HD 19916b), based on data from NASA's Transiting Exoplanet Survey Satellite (TESS). The transit signal...
TOI-5126: a hot super-Neptune and warm Neptune pair discovered by TESS and CHEOPS
We present the confirmation of a hot super-Neptune with an exterior Neptune companion orbiting a bright (V = 10.1 mag) F-dwarf identified by the Transiting...
TOI-530b: a giant planet transiting an M-dwarf detected by TESS
We report the discovery of TOI-530b, a transiting Saturn-like planet around an M0.5V dwarf, delivered by the Transiting Exoplanet Survey Satellite (TESS). The...
TOI-544 b: a potential water-world inside the radius valley in a two-planet system
We report on the precise radial velocity follow-up of TOI-544 (HD 290498), a bright K star (V = 10.8), which hosts a small transiting planet recently discovered...
TOI-544 b: a potential water-world inside the radius valley in a two-planet system
We report on the precise radial velocity follow-up of TOI-544 (HD 290498), a bright K star (V = 10.8), which hosts a small transiting planet recently discovered...
TOI-6478 b: a cold underdense Neptune transiting a fully convective M dwarf from the thick disc
Growing numbers of exoplanet detections continue to reveal the diverse nature of planetary systems. Planet formation around late-type M dwarfs is of particular...