The characterisation of giant exoplanets is crucial to constrain giant planet formation and
evolution theory and for putting the solar-system's giant planets in perspective. Typically …

Ground-based high-resolution spectroscopy (HRS) has detected numerous chemical
species and atmospheric dynamics in exoplanets, most notably ultrahot Jupiters (UHJs) …

Relating planet formation to atmospheric composition has been a long-standing goal of the
planetary science community. So far, most modeling studies have focused on predicting the …

We present the discovery of TOI-5205b, a transiting Jovian planet orbiting a solar metallicity
M4V star, which was discovered using Transiting Exoplanet Survey Satellite photometry and …

Giant exoplanets seem to have on average a much higher heavy-element content than the
Solar System giants. Past attempts to explain this heavy-element content include collisions …

One of the main objectives of the European Space Agency's Ariel telescope (launch 2029) is
to understand the formation and evolution processes of a large sample of planets in our …

One of the current challenges of planet formation theory is to explain the enrichment of
observed exoplanetary atmospheres. While past studies have focused on scenarios where …

Among the hundreds of known hot Jupiters (HJs), only five have been found to have
companions on short-period orbits. Within this rare class of multiple planetary systems, the …

The two prevailing planet formation scenarios, core accretion and disk instability, predict
distinct planetary mass–metallicity relations. Yet, the detection of this trend remains …

We report on the confirmation and follow-up characterization of two long-period transiting
substellar companions on low-eccentricity orbits around TIC 4672985 and TOI-2529, whose …