The field of exoplanet atmospheric characterization has recently made considerable
advances with the advent of high-resolution spectroscopy from large ground-based …

The JWST has ushered in a new era in atmospheric characterisations of temperate low-
mass exoplanets with recent detections of carbon-bearing molecules in the candidate …

OVERVIEW Nearly 30 years after the discovery of the first exoplanet around a main
sequence star, thousands of planets have now been confirmed. These discoveries have …

We present the results for the detectability of the O 2 and O 3 molecular species in the
atmosphere of an Earth-like planet using reflected light at visible wavelengths. By …

In this study, we treat Earth as an exoplanet and investigate our home planet by means of a
potential future mid-infrared space mission called the Large Interferometer For Exoplanets …

Located at the bottom of the main sequence, ultracool dwarf stars are widespread in the
solar neighbourhood. Nevertheless, their extremely low luminosity has left their planetary …

Stars appear darker at their limbs than at their disk centres because at the limb we are
viewing the higher and cooler layers of stellar photospheres. Yet, limb darkening derived …

In the past decade the study of exoplanet atmospheres at high-spectral resolution, via
transmission/emission spectroscopy and cross-correlation techniques for atomic/molecular …

The JWST has ushered in a new era of exoplanet transit spectroscopy. Among the JWST
instruments, the Near-Infrared Spectrograph (NIRSpec) has the most extensive set of …

Ultra-cool dwarf stars are abundant, long-lived, and uniquely suited to enable the
atmospheric study of transiting terrestrial companions with JWST. Amongst them, the most …