Add to ORKGHigh-resolution spectroscopy (HRS) has been used to detect a number of species in the atmospheres of hot Jupiters. Key to such detections is accurately and precisely modelled spectra for cross-correlation against the R 20 000 observations. There is a need for the latest generation of opacities which form the basis for high signal-to-noise detections using such spectra. In this study we present and make publicly available cross-sections for six molecular species, H2O, CO, HCN, CH4, NH3, and CO2 using the latest line lists most suitable for lowand high-resolution spectroscopy. We focus on the infrared (0.95–5 μm) and between 500 and 1500 K where these species have strong spectral signatures. We generate these cross-sections on a grid ...
Of the many recently discovered worlds orbiting distant stars, very little is yet known of their che...
The desire to characterize and model the atmospheres of the many extrasolar planets that have been d...
The atmospheres of gaseous giant exoplanets orbiting close to their parent stars (hot Jupiters) have...
High-resolution spectroscopy (HRS) has been used to detect a number of species in the atmospheres of...
High-resolution spectroscopy (HRS) has been used to detect a number of species in the atmospheres of...
Context. Recently, there have been a series of detections of molecules in the atmospheres of extraso...
Context. After many attempts over more than a decade, high-resolution spectroscopy has recently de...
Observations to characterize planets larger than Earth but smaller than Neptune have led to largely ...
Infrared line positions and pressure-broadening data of atmospheric key absorbers \chem{H_2O} and \c...
Ultra-hot jupiters (UHJs) are giant planets on short orbital periods with high equilibrium temperatu...
Observations to characterize planets larger than Earth but smaller than Neptune have led to largely ...
Of the many recently discovered worlds orbiting distant stars, very lit-tle is yet known of their ch...
AbstractOf the many recently discovered worlds orbiting distant stars, very little is yet known of t...
The elemental ratios of carbon, nitrogen, and oxygen in the atmospheres of hot Jupiters may hold clu...
High-resolution spectroscopy (R ≥ 25,000) has recently emerged as one of the leading methods for det...
Of the many recently discovered worlds orbiting distant stars, very little is yet known of their che...
The desire to characterize and model the atmospheres of the many extrasolar planets that have been d...
The atmospheres of gaseous giant exoplanets orbiting close to their parent stars (hot Jupiters) have...
High-resolution spectroscopy (HRS) has been used to detect a number of species in the atmospheres of...
High-resolution spectroscopy (HRS) has been used to detect a number of species in the atmospheres of...
Context. Recently, there have been a series of detections of molecules in the atmospheres of extraso...
Context. After many attempts over more than a decade, high-resolution spectroscopy has recently de...
Observations to characterize planets larger than Earth but smaller than Neptune have led to largely ...
Infrared line positions and pressure-broadening data of atmospheric key absorbers \chem{H_2O} and \c...
Ultra-hot jupiters (UHJs) are giant planets on short orbital periods with high equilibrium temperatu...
Observations to characterize planets larger than Earth but smaller than Neptune have led to largely ...
Of the many recently discovered worlds orbiting distant stars, very lit-tle is yet known of their ch...
AbstractOf the many recently discovered worlds orbiting distant stars, very little is yet known of t...
The elemental ratios of carbon, nitrogen, and oxygen in the atmospheres of hot Jupiters may hold clu...
High-resolution spectroscopy (R ≥ 25,000) has recently emerged as one of the leading methods for det...
Of the many recently discovered worlds orbiting distant stars, very little is yet known of their che...
The desire to characterize and model the atmospheres of the many extrasolar planets that have been d...
The atmospheres of gaseous giant exoplanets orbiting close to their parent stars (hot Jupiters) have...