In a variety of astronomical objects including gas giant (exo-)planets, brown dwarfs and cool stars, molecular hydrogen and helium are the major line broadeners. However, there is currently no systematic source for these parameters, particularly at the elevated temperatures encountered in many of these objects. The ExoMol project provides comprehensive molecular line lists for exoplanet and other hot atmospheres. The ExoMol database has recently been extended to provide additional data including temperature-dependent, pressure-broadening parameters. Here we assemble H2 and He pressure-broadening datasets for the molecules H2O, NH3, SO2, CH4, PH3, HCN and H2CO using available experimental and theoretical studies
Stellar, substellar, and planetary atmosphere models are all highly sensitive to the input absorptio...
High-resolution spectroscopy (HRS) has been used to detect a number of species in the atmospheres of...
Author Institution: Department of Physics and Astronomy, University College London, London, WC1E 6BT...
Many atmospheres (cool stars, brown dwarfs, giant planets, extrasolar planets) are predominately com...
Infrared line positions and pressure-broadening data of atmospheric key absorbers \chem{H_2O} and \c...
In this study, the pressure-broadened H2O absorption cross-sections (ACS) data are computed for two ...
To increase the potential for use of the HITRAN database in astronomy, experimental and theoretical ...
For accurate modelling of observations of exoplanet atmospheres, quantification of the pressure broa...
We describe the recent updates to the ExoMol database regarding the molecular spectral line shapes. ...
Citing the Data If you use this data be sure to cite the paper that describes the work, as well as...
Methane (CH$_{4}$) is the dominant carbon-bearing molecule in terrestrial and exoplanetary atmospher...
This research is a composite of projects which have individually contributed new results to their re...
The discovery of super-Earth and mini-Neptune exoplanets means that atmospheric signals from low-mas...
To increase the potential of the HITRAN database in astronomy, experimental and theoretical line bro...
ISMB2015, 28 junio al 3 de julio de 2015, Segovia (España); http://www.ucm.es/ismbWater is a fundame...
Stellar, substellar, and planetary atmosphere models are all highly sensitive to the input absorptio...
High-resolution spectroscopy (HRS) has been used to detect a number of species in the atmospheres of...
Author Institution: Department of Physics and Astronomy, University College London, London, WC1E 6BT...
Many atmospheres (cool stars, brown dwarfs, giant planets, extrasolar planets) are predominately com...
Infrared line positions and pressure-broadening data of atmospheric key absorbers \chem{H_2O} and \c...
In this study, the pressure-broadened H2O absorption cross-sections (ACS) data are computed for two ...
To increase the potential for use of the HITRAN database in astronomy, experimental and theoretical ...
For accurate modelling of observations of exoplanet atmospheres, quantification of the pressure broa...
We describe the recent updates to the ExoMol database regarding the molecular spectral line shapes. ...
Citing the Data If you use this data be sure to cite the paper that describes the work, as well as...
Methane (CH$_{4}$) is the dominant carbon-bearing molecule in terrestrial and exoplanetary atmospher...
This research is a composite of projects which have individually contributed new results to their re...
The discovery of super-Earth and mini-Neptune exoplanets means that atmospheric signals from low-mas...
To increase the potential of the HITRAN database in astronomy, experimental and theoretical line bro...
ISMB2015, 28 junio al 3 de julio de 2015, Segovia (España); http://www.ucm.es/ismbWater is a fundame...
Stellar, substellar, and planetary atmosphere models are all highly sensitive to the input absorptio...
High-resolution spectroscopy (HRS) has been used to detect a number of species in the atmospheres of...
Author Institution: Department of Physics and Astronomy, University College London, London, WC1E 6BT...