The collision-induced fundamental vibration–rotation band at 6.4 μm is the strongest
absorption feature from O2 in the infrared,–, yet it has not been previously incorporated into …

We present the Polarization of Hot Exoplanets (PolHEx) code for modelling the total flux (F)
and degree of linear Polarization (P) of light spectra reflected by close-in, tidally locked …

The goal of this white paper is to provide a snapshot of the data availability and data needs
primarily for the Ariel space mission, but also for related atmospheric studies of exoplanets …

LOUPE, the Lunar Observatory for Unresolved Polarimetry of the Earth, is a small, robust
spectro-polarimeter for observing the Earth as an exoplanet. Detecting Earth-like planets in …

Context. The circular polarization of light that planets reflect is often neglected because it is
very small compared to the linear polarization. It could, however, provide information on a …

PYMIEDAP (the Python Mie Doubling-Adding Programme) is a Python-based tool for
computing the total linearly and circularly polarized fluxes of incident unpolarized sunlight or …

Abstract In the JWST, Extremely Large Telescopes, and LUVOIR era, we expect to
characterize a number of potentially habitable Earth-like exoplanets. However, the …

Context. Understanding the total flux and polarization signals of Earth-like planets and their
spectral and temporal variability is essential for the future characterization of such …

Context. Clouds have already been detected in exoplanetary atmospheres. They play
crucial roles in a planet's atmosphere and climate and can also create ambiguities in the …

Context. Earthshine, ie, sunlight scattered by Earth and back-reflected from the lunar surface
to Earth, allows observations of the total flux and polarization of Earth with ground-based …