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ExoAtmospheres: a community database for exoplanet atmospheres research
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<p>The stud of exoplanet atmospheres is an exciting and vibrant field of research, where new discoveries and publications occur at a very fast pace and it is easy to miss many interesting results. The main purpose of the <strong>Exoplanet Atmospheres Database</strong> is to become a quick and useful repository of all available exoplanet atmospheres publications, and also to help in the gathering of useful references for a given planet or plane types.</p>
Title: ExoAtmospheres: a community database for exoplanet atmospheres research
Description:
<p>The stud of exoplanet atmospheres is an exciting and vibrant field of research, where new discoveries and publications occur at a very fast pace and it is easy to miss many interesting results.
The main purpose of the <strong>Exoplanet Atmospheres Database</strong> is to become a quick and useful repository of all available exoplanet atmospheres publications, and also to help in the gathering of useful references for a given planet or plane types.
</p>.
Related Results
High-temperature measurements of VUV absorption cross sections with application to warm exoplanet atmospheres
High-temperature measurements of VUV absorption cross sections with application to warm exoplanet atmospheres
) IntroductionWith current observational constraints, a large fraction of observed exoplanets whose atmospheres can be studied with spectroscopy orbits closely from their host star...
Atmospheric characterization by combining HARPS and NIRPS
Atmospheric characterization by combining HARPS and NIRPS
Over the last decade, the use of ground-based high-resolution spectrographs has tremendously increased. Such instruments can resolve individual atomic and molecular lines. Therefor...
A Homogeneous Study of Exoplanetary Atmospheres Using High-Resolution Transit Spectroscopy
A Homogeneous Study of Exoplanetary Atmospheres Using High-Resolution Transit Spectroscopy
Thousands of exoplanets have been confirmed in the last two decades, and yet observational constraints on their compositions have only been obtained for a few hundred of them so fa...
Accelerating Radiative Transfer in 3D Simulations of the Venusian Atmosphere
Accelerating Radiative Transfer in 3D Simulations of the Venusian Atmosphere
This work introduces an approach to enhance the computational efficiency of 3D Global Circulation Model (GCM) simulations by integrating a machine-learned surrogate model into the ...
Analysis of the public HARPS/ESO spectroscopic archive
Analysis of the public HARPS/ESO spectroscopic archive
Context. Magnetic activity is currently the primary limiting factor in radial velocity (RV) exoplanet searches. Even inactive stars, such as the Sun, exhibit RV jitter of the order...
Evolution of Antimicrobial Resistance in Community vs. Hospital-Acquired Infections
Evolution of Antimicrobial Resistance in Community vs. Hospital-Acquired Infections
Abstract
Introduction
Hospitals are high-risk environments for infections. Despite the global recognition of these pathogens, few studies compare microorganisms from community-acqu...
The Pursuit of A Meticulous Chemical Survey of Exoplanets
The Pursuit of A Meticulous Chemical Survey of Exoplanets
<p>Thousands of exoplanets have now been discovered with a huge range of bulk parameters. However, the essential nature of these planets remains largely mysterious. W...
Exoplanet Atmospheres with HST: An open science framework for the characterisation of exoplanets
Exoplanet Atmospheres with HST: An open science framework for the characterisation of exoplanets
The field of exoplanets is one of the most rapidly growing, with more than 4000 new planets discovered over the past 25 years. In the last decade, we have entered in a new era, the...

