Hot Jupiters were the first exoplanets to be discovered around main sequence stars and
astonished us with their close-in orbits. They are a prime example of how exoplanets have …

Planet-forming disc evolution is not independent of the star formation and feedback process
in giant molecular clouds. In particular, OB stars emit UV radiation that heats and disperses …

Transmission spectroscopy of exoplanets has the potential to provide precise
measurements of atmospheric chemical abundances, in particular of hot Jupiters whose …

Abstract The Apache Point Observatory Galactic Evolution Experiment 2 (APOGEE-2) is a
dual-hemisphere, near-infrared (NIR), spectroscopic survey with the goal of producing a …

We report the discovery of TOI 837b and its validation as a transiting planet. We characterize
the system using data from the NASA Transiting Exoplanet Survey Satellite mission, the ESA …

We investigate how the occurrence rate of giant planets (minimum mass> 0.3 M Jup) around
Sun-like stars depends on the age, mass, and metallicity of their host stars. We develop a …

The discovery of only a handful of exoplanets required establishing a correlation between
giant planet occurrence and metallicity of their host stars. More than 20 years have already …

The TESS mission will survey∼ 85 per cent of the sky, giving us the opportunity of extracting
high-precision light curves of millions of stars, including stellar cluster members. In this work …

K2-136: A Binary System in the Hyades Cluster Hosting a Neptune-sized Planet - IOPscience
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The scope of the project 'A PSF-based Approach to TESS High Quality data Of Stellar
clusters'(PATHOS) is the extraction and analysis of high-precision light curves of stars in …